[
{
	"Index" : "18881",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "22 Andromedae, HIP 841, SAO 36123, HD 571, GC 169, HR 27, DM BD+45    17, TYC 3246-880-1",
	"group" : { "backgroundImage" : "images/Alignment/01.png",
		"description" : "Andromeda is one of the 48 constellations listed by the 2nd-century Greco-Roman astronomer Ptolemy and remains one of the 88 modern constellations. Located north of the celestial equator, it is named for Andromeda, daughter of Cassiopeia, in the Greek myth, who was chained to a rock to be eaten by the sea monster Cetus. Andromeda is most prominent during autumn evenings in the Northern Hemisphere, along with several other constellations named for characters in the Perseus myth. Because of its northern declination, Andromeda is only visible north of 40\u00B0 south latitude; for observers farther south it lies below the horizon. It is one of the largest constellations, with an area of 722 square degrees. This is over 1,400 times the size of the full moon, 55% of the size of the largest constellation, Hydra, and over 10 times the size of the smallest constellation, Crux.\r\rIts brightest star, Alpha Andromedae, is a binary star that has also been counted as a part of Pegasus, while Gamma Andromedae is a colorful binary and a popular target for amateur astronomers. Only marginally dimmer than Alpha, Beta Andromedae is a red giant, its color visible to the naked eye. The constellation\u0027s most obvious deep-sky object is the naked-eye Andromeda Galaxy (M31, also called the Great Galaxy of Andromeda), the closest spiral galaxy to the Milky Way and one of the brightest Messier objects. Several fainter galaxies, including M31\u0027s companions M110 and M32, as well as the more distant NGC 891, lie within Andromeda. The Blue Snowball Nebula, a planetary nebula, is visible in a telescope as a blue circular object.\r\rIn Chinese astronomy, the stars that make up Andromeda were members of four different constellations that had astrological and mythological significance; a constellation related to Andromeda also exists in Hindu mythology. Andromeda is the location of the radiant for the Andromedids, a weak meteor shower that occurs in November.\r\rThe uranography of Andromeda has its roots most firmly in the Greek tradition, though a female figure in Andromeda\u0027s location had appeared earlier in Babylonian astronomy. The stars that make up Pisces and the middle portion of modern Andromeda formed a constellation representing a fertility goddess, sometimes named as Anunitum or the Lady of the Heavens.\r\rAndromeda is known as \u0022the Chained Lady\u0022 or \u0022the Chained Woman\u0022 in English. It was known as Mulier Catenata (\u0022chained woman\u0022) in Latin and al-Mar\u0027at al Musalsalah in Arabic. It has also been called Persea (\u0022Perseus\u0027s wife\u0022) or Cepheis (\u0022Cepheus\u0027s daughter\u0022), all names that refer to Andromeda\u0027s role in the Greco-Roman myth of Perseus, in which Cassiopeia, the queen of Ethiopia, bragged that her daughter was more beautiful than the Nereids, sea nymphs blessed with incredible beauty. Offended at her remark, the nymphs petitioned Poseidon to punish Cassiopeia for her insolence, which he did by commanding the sea monster Cetus to attack Ethiopia. Andromeda\u0027s panicked father, Cepheus, was told by the Oracle of Ammon that the only way to save his kingdom was to sacrifice his daughter to Cetus. She was chained to a rock by the sea but was saved by the hero Perseus, who used the head of Medusa to turn the monster into stone; Algol (\u03B2 Persei), the \u0022Demon Star\u0022, marks the head of Medusa. Perseus and Andromeda then married; the myth recounts that the couple had seven children together \u2013 six sons and one daughter \u2013 and founded Mycenae and its Persideae dynasty. After Andromeda\u0027s death Athena placed her in the sky as a constellation, to honor her. Several of the neighboring constellations (Perseus, Cassiopeia, Cetus, and Cepheus) also represent characters in the Perseus myth.\r\rAndromeda was one of the original 48 constellations formulated by Ptolemy in his 2nd-century Almagest, in which it was defined as a specific pattern of stars. She is typically depicted with \u03B1 Andromedae as her head, \u03BF and \u03BB Andromedae as her chains, and \u03B4, \u03C0, \u03BC, \u0392, and \u03B3 Andromedae representing her body and legs. However, there is no universal depiction of Andromeda and the stars used to represent her body, head, and chains. Arab astronomers were aware of Ptolemy\u0027s constellations, but they included a second constellation representing a fish at Andromeda\u0027s feet. Several stars from Andromeda and most of the stars in Lacerta were combined in 1787 by German astronomer Johann Bode to form Frederici Honores (also called Friedrichs Ehre). It was designed to honor King Frederick II of Prussia, but quickly fell into disuse. Since the time of Ptolemy, Andromeda has remained a constellation and is officially recognized by the International Astronomical Union, although like all modern constellations, it is now defined as a specific region of the sky that includes both Ptolemy\u0027s pattern and the surrounding stars. In 1922, the IAU defined its recommended three-letter abbreviation, \u0022And\u0022. The official boundaries of Andromeda were defined in 1930 by Eug\u00E8ne Delporte as a polygon of 36 segments. Its right ascension is between 22h 57.5m and 2h 39.3m and its declination is between 53.19\u00B0 and 21.68\u00B0 in the equatorial coordinate system.",
		"key" : "Andromeda",
		"grouptype" : "Andromeda",
		"Meaning" : "Andromeda (The chained lady or the Princess)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Andromeda",
		"title" : "Andromeda Objects Group" },
	"Common" : "22 Andromedae",
	"OType" : "Star",
	"Distance" : "372.37",
	"RA_S" : 2.58019324,
	"DEC_S" : 46.07227305,
	"Constellation" : "Andromeda ",
	"AMag" : 5.071,
	"key" : 38881,
	"title" : "22 Andromedae"
	},
{
	"Index" : "14824",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "24 Andromedae, Theta Andromedae, HIP 1366, SAO 53777, HD 1280, GC 334, HR 63, DM BD+37    34, TYC 2782-2251-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Theta Andromedae",
	"OType" : "Star",
	"Distance" : "93.77",
	"RA_S" : 4.27289837,
	"DEC_S" : 38.6816459,
	"Constellation" : "Andromeda ",
	"AMag" : 4.607,
	"key" : 34824,
	"title" : "Theta Andromedae"
	},
{
	"Index" : "10558",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "25 Andromedae, Sigma Andromedae, HIP 1473, SAO 53798, HD 1404, GC 362, HR 68, DM BD+35    44, TYC 2273-2081-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Sigma Andromedae",
	"OType" : "Double or multiple star",
	"Distance" : "41.32",
	"RA_S" : 4.58190704,
	"DEC_S" : 36.78522535,
	"Constellation" : "Andromeda ",
	"AMag" : 4.512,
	"key" : 30558,
	"title" : "Sigma Andromedae"
	},
{
	"Index" : "14836",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "27 Andromedae, Rho Andromedae, HIP 1686, SAO 53828, HD 1671, GC 425, HR 82, DM BD+37    45, TYC 2783-2251-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Rho Andromedae",
	"OType" : "Star",
	"Distance" : "48.54",
	"RA_S" : 5.2802847,
	"DEC_S" : 37.96860444,
	"Constellation" : "Andromeda ",
	"AMag" : 5.208,
	"key" : 34836,
	"title" : "Rho Andromedae"
	},
{
	"Index" : "14918",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "HIP 2225, SAO 36390, HD 2421, GC 546, HR 104, DM BD+43   92, TYC 2795-2706-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "HR 104",
	"OType" : "Spectroscopic binary",
	"Distance" : "86.59",
	"RA_S" : 7.05689848,
	"DEC_S" : 44.39445759,
	"Constellation" : "Andromeda ",
	"AMag" : 5.177,
	"key" : 34918,
	"title" : "HR 104"
	},
{
	"Index" : "6192",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "28 Andromedae, HIP 2355, SAO 74041, HD 2628, GC 583, HR 114, DM BD+28    75, TYC 1737-2790-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "28 Andromedae",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "62.72",
	"RA_S" : 7.53068816,
	"DEC_S" : 29.75155887,
	"Constellation" : "Andromeda ",
	"AMag" : 5.246,
	"key" : 26192,
	"title" : "28 Andromedae"
	},
{
	"Index" : "14926",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "HIP 2900, SAO 36509, HD 3346, GC 726, HR 152, DM BD+43  113, TYC 2796-2404-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "V* V428 And",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "188.31",
	"RA_S" : 9.19350563,
	"DEC_S" : 44.48859088,
	"Constellation" : "Andromeda ",
	"AMag" : 5.324,
	"key" : 34926,
	"title" : "V* V428 And"
	},
{
	"Index" : "10595",
	"Description" : "Pi Andromedae (Pi And, \u03C0 Andromedae, \u03C0 And) is the Bayer designation for a binary star system in the northern constellation of Andromeda. With an apparent visual magnitude of 4.4, it is visible to the naked eye. It is located approximately 600 light-years (180 parsecs) from Earth.\r\rThe pair is classified as a blue-white B-type main sequence dwarf with an apparent magnitude of +4.34. It is a spectroscopic binary with an orbital period of 143.6 days and an eccentricity of 0.56. There is a magnitude 8.6 companion 35.9 arcseconds away. At 55 arcseconds separation is an 11th magnitude companion.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of \u03C0 Andromedae, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03C0 Andromedae itself is known as \u594E\u5BBF\u516D (Ku\u00ED S\u00F9 li\u00F9, English: the Sixth Star of Legs.)",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "29 Andromedae, Pi Andromedae, HIP 2912, SAO 54033, HD 3369, GC 729, HR 154, DM BD+32   101, TYC 2279-1665-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Pi Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "182.78",
	"RA_S" : 9.22018753,
	"DEC_S" : 33.71934456,
	"X" : 401,
	"Y" : 424,
	"Constellation" : "Andromeda ",
	"AMag" : 4.319,
	"key" : 30595,
	"title" : "Pi Andromedae"
	},
{
	"Index" : "6262",
	"Description" : "Epsilon Andromedae (Epsilon And, \u03B5 Andromedae, \u03B5 And) is a G-type giant star in the constellation of Andromeda. It has an apparent visual magnitude of approximately 4.37.\r\r\u03B5 Andromedae is believed to be a red clump star which is fusing helium in its core. Its orbit in the Milky Way is highly eccentric, causing it to move rapidly relative to the Sun and its neighboring stars.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of \u03B5 Andromedae, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03B5 Andromedae itself is known as \u594E\u5BBF\u56DB (Ku\u00ED S\u00F9 s\u00EC, English: the Fourth Star of Legs.)",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "30 Andromedae, Epsilon Andromedae, HIP 3031, SAO 74164, HD 3546, GC 759, HR 163, DM BD+28   103, TYC 1744-2936-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Epsilon Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "50.22",
	"RA_S" : 9.63893624,
	"DEC_S" : 29.31175207,
	"X" : 397,
	"Y" : 481,
	"Constellation" : "Andromeda ",
	"AMag" : 4.44,
	"key" : 26262,
	"title" : "Epsilon Andromedae"
	},
{
	"Index" : "10569",
	"Description" : "Delta Andromedae (\u03B4 And, \u03B4 Andromedae) is a multiple star system in the northern constellation of Andromeda. Based upon parallax measurements, is located at a distance of approximately 105.5 light-years (32.3 parsecs) from the Earth. Apart from its Bayer designation, it was also given the title Delta by Elijah H. Burritt in his star atlas.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of \u03B4 Andromedae, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B9 Piscium, \u03B5 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03B4 Andromedae itself is known as \u594E\u5BBF\u4E94 (Ku\u00ED Su w\u01D4, English: the Fifth Star of Legs.)\r\rThis is a long-period spectroscopic binary with an orbital period of approximately 15,000 days (41 years) and an overall apparent visual magnitude of approximately 3.28. The primary of the spectroscopic binary has a stellar classification of K3 III, indicating that it is a giant star. It most likely evolved from a F-type main sequence star after consuming the hydrogen at its core. The secondary is believed to be relatively faint, as it has not been observed interferometrically. The star has two optical companions, the closest of which may be an orbiting red dwarf of class M3 with a separation of at least 900 astronomical units.\r\rAn excess of infrared emission from \u03B4 Andromedae suggested that it may be surrounded by a shell of dust. In 2003 it was determined that this is more likely a circumstellar debris disk.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "31 Andromedae, Delta Andromedae, HIP 3092, SAO 54058, HD 3627, GC 774, HR 165, DM BD+30    91, TYC 2275-1753-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Delta Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "32.35",
	"RA_S" : 9.83199596,
	"DEC_S" : 30.86101828,
	"X" : 451,
	"Y" : 358,
	"Constellation" : "Andromeda ",
	"AMag" : 3.405,
	"key" : 30569,
	"title" : "Delta Andromedae"
	},
{
	"Index" : "14966",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "32 Andromedae, HIP 3231, SAO 54079, HD 3817, GC 812, HR 175, DM BD+38    90, TYC 2801-2091-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "32 Andromedae",
	"OType" : "Star",
	"Distance" : "108.67",
	"RA_S" : 10.27993337,
	"DEC_S" : 39.45866377,
	"Constellation" : "Andromeda ",
	"AMag" : 5.402,
	"key" : 34966,
	"title" : "32 Andromedae"
	},
{
	"Index" : "6216",
	"Description" : "Zeta Andromedae (Zeta And, \u03B6 Andromedae, \u03B6 And) is a star system in the constellation Andromeda. It is approximately 181 light years from Earth.\r\rZeta Andromedae is an eclipsing spectroscopic binary whose primary is classified as an orange K-type bright giant with a mean apparent magnitude of +4.08. In addition to brightness variation due to eclipses, the system is also an RS Canum Venaticorum type or Beta Lyrae type variable star. Its brightness varies from magnitude +3.92 to +4.14 with a period of 17.77 days. The orbital period of the binary is 17.77 days.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "34 Andromedae, Zeta Andromedae, HIP 3693, SAO 74267, HD 4502, GC 940, HR 215, DM BD+23   106, TYC 1739-2317-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Zeta Andromedae",
	"OType" : "Variable of RS CVn type",
	"Distance" : "57.99",
	"RA_S" : 11.83468946,
	"DEC_S" : 24.26717801,
	"X" : 371,
	"Y" : 547,
	"Constellation" : "Andromeda ",
	"AMag" : 4.199,
	"key" : 26216,
	"title" : "Zeta Andromedae"
	},
{
	"Index" : "14965",
	"Description" : "Nu Andromedae (Nu And, \u03BD Andromedae, \u03BD And) is a binary star in the constellation Andromeda. The system has an apparent visual magnitude of 4.5, which is bright enough to be seen with the naked eye. It is approximately 620 light-years (190 parsecs) from Earth. Situated just over a degree to the west of this star is the Andromeda Galaxy.\r\rNu Andromedae is spectroscopic binary system with a nearly circular orbit that has a period of 4.2828 days. The primary component is a B-type main sequence star with a stellar classification of B5 V. The fainter secondary has a classification of F8 V, which makes it an F-type main sequence star. The pair are about 63 million years old.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of \u03BD Andromedae, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03BD Andromedae itself is known as \u594E\u5BBF\u4E03 (Ku\u00ED S\u00F9 q\u012B, English: the Seventh Star of Legs.)",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "35 Andromedae, Nu Andromedae, HIP 3881, SAO 36699, HD 4727, GC 989, HR 226, DM BD+40   171, TYC 2801-2090-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Nu Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "189.21",
	"RA_S" : 12.45352988,
	"DEC_S" : 41.07891001,
	"X" : 368,
	"Y" : 328,
	"Constellation" : "Andromeda ",
	"AMag" : 4.496,
	"key" : 34965,
	"title" : "Nu Andromedae"
	},
{
	"Index" : "14934",
	"Description" : "Mu Andromedae (Mu And, \u03BC Andromedae, \u03BC And) is the Bayer designation for a star in the northern constellation of Andromeda. It has an apparent visual magnitude of 3.87, making it readily visible to the naked eye. Based upon parallax measurements, it is approximately 130 light-years (40 parsecs) from Earth. In the constellation, the star is situated about half way between the bright star Mirach to the southwest and the Andromeda Galaxy (M31) to the northeast.\r\rThe spectrum of this star matches a stellar classification of A5 V, indicating that it is an A-type main sequence star. It has double the mass of the Sun and 2.4 times the Sun\u0027s radius. The star is radiating about 21 times the luminosity of the Sun from its outer envelope at an effective temperature of 7,959 K, giving it the characteristic white glow of an A-type star. It is estimated to be about 600 million years old with a relatively high projected rotational velocity of 75 km/s.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of \u03BC Andromedae, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03BC Andromedae itself is known as \u594E\u5BBF\u516B (Ku\u00ED S\u00F9 b\u0101, English: the Eighth Star of Legs.)",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "37 Andromedae, Mu Andromedae, HIP 4436, SAO 54281, HD 5448, GC 1122, HR 269, DM BD+37   175, TYC 2798-1667-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Mu Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "39.72",
	"RA_S" : 14.1883838,
	"DEC_S" : 38.4993439,
	"X" : 350,
	"Y" : 361,
	"Constellation" : "Andromeda ",
	"AMag" : 3.868,
	"key" : 34934,
	"title" : "Mu Andromedae"
	},
{
	"Index" : "6222",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "38 Andromedae, Eta Andromedae, HIP 4463, SAO 74388, HD 5516, GC 1136, HR 271, DM BD+22   153, TYC 1740-2109-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Eta Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "70.39",
	"RA_S" : 14.3016661,
	"DEC_S" : 23.4176518,
	"Constellation" : "Andromeda ",
	"AMag" : 4.499,
	"key" : 26222,
	"title" : "Eta Andromedae"
	},
{
	"Index" : "15033",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "41 Andromedae, HIP 5317, SAO 36950, HD 6658, GC 1364, HR 324, DM BD+43   234, TYC 2811-2324-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "41 Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "58.94",
	"RA_S" : 17.00353642,
	"DEC_S" : 43.94209444,
	"Constellation" : "Andromeda ",
	"AMag" : 5.046,
	"key" : 35033,
	"title" : "41 Andromedae"
	},
{
	"Index" : "19089",
	"Description" : "Phi Andromedae (\u03C6 Andromedae, \u03C6 And) is the Bayer designation for a binary star system near the border of the northern constellation of Andromeda. This system has a combined apparent visual magnitude of 4.25 and is visible to the naked eye. Based upon parallax measurements made during the Hipparcos mission, this star system is located at a distance of about 720 light-years (220 parsecs) from Earth. With \u03C7 And it forms the Chinese asterism \u8ECD\u5357\u9580 (Keun Nan Mun, Mandarin j\u016Bnn\u00E1nm\u00E9n), \u0022the South Gate of the Camp\u0022.\r\rThe 4.46 magnitude primary component is a Be star with a stellar classification of B7 Ve, indicating that it is a B-type main sequence star that shows prominent emission lines of hydrogen in its spectrum. These emission lines come from a flattened disk of hot, decreated gas that is orbiting the host star. The star is rotating rapidly with a projected rotational velocity of 75 km/s. The pole of the star is inclined around 20\u00B0 to the line of sight from the Earth.\r\rThe 6.06 magnitude companion star is a B-type main sequence star with a classification of B9 V. On average the two stars are separated by about 0.6 arcseconds and have an orbital period of roughly 554 years. Based upon their orbital elements, the system has a combined mass of around 6.5 \u00B1 2.8 times the mass of the Sun.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "42 Andromedae, Phi Andromedae, HIP 5434B, SAO 36972, HD 6811, GC 1394, HR 335, DM BD+46   275, TYC 3268-1358-2",
	"group" : { "key" : "Andromeda" },
	"Common" : "Phi Andromedae",
	"OType" : "Star",
	"Distance" : "215.29",
	"RA_S" : 17.37554333,
	"DEC_S" : 47.24177979,
	"X" : 327,
	"Y" : 245,
	"Constellation" : "Andromeda ",
	"AMag" : 7.772,
	"key" : 39089,
	"title" : "Phi Andromedae"
	},
{
	"Index" : "19088",
	"Description" : "Phi Andromedae (\u03C6 Andromedae, \u03C6 And) is the Bayer designation for a binary star system near the border of the northern constellation of Andromeda. This system has a combined apparent visual magnitude of 4.25 and is visible to the naked eye. Based upon parallax measurements made during the Hipparcos mission, this star system is located at a distance of about 720 light-years (220 parsecs) from Earth. With \u03C7 And it forms the Chinese asterism \u8ECD\u5357\u9580 (Keun Nan Mun, Mandarin j\u016Bnn\u00E1nm\u00E9n), \u0022the South Gate of the Camp\u0022.\r\rThe 4.46 magnitude primary component is a Be star with a stellar classification of B7 Ve, indicating that it is a B-type main sequence star that shows prominent emission lines of hydrogen in its spectrum. These emission lines come from a flattened disk of hot, decreated gas that is orbiting the host star. The star is rotating rapidly with a projected rotational velocity of 75 km/s. The pole of the star is inclined around 20\u00B0 to the line of sight from the Earth.\r\rThe 6.06 magnitude companion star is a B-type main sequence star with a classification of B9 V. On average the two stars are separated by about 0.6 arcseconds and have an orbital period of roughly 554 years. Based upon their orbital elements, the system has a combined mass of around 6.5 \u00B1 2.8 times the mass of the Sun.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "42 Andromedae, Phi Andromedae, HIP 5434A, SAO 36972, HD 6811, GC 1394, HR 335, DM BD+46   275, TYC 3268-1358-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Phi Andromedae",
	"OType" : "Star",
	"Distance" : "215.29",
	"RA_S" : 17.37554333,
	"DEC_S" : 47.24177979,
	"X" : 327,
	"Y" : 245,
	"Constellation" : "Andromeda ",
	"AMag" : 4.284,
	"key" : 39088,
	"title" : "Phi Andromedae"
	},
{
	"Index" : "19054",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "46 Andromedae, Xi Andromedae, HIP 6411, SAO 37155, HD 8207, GC 1647, HR 390, DM BD+44   287, TYC 3265-2400-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Adhil",
	"OType" : "Star",
	"Distance" : "65.72",
	"RA_S" : 20.58508273,
	"DEC_S" : 45.52877917,
	"Constellation" : "Andromeda ",
	"AMag" : 4.988,
	"key" : 39054,
	"title" : "Adhil"
	},
{
	"Index" : "19055",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "48 Andromedae, Omega Andromedae, HIP 6813, SAO 37228, HD 8799, GC 1752, HR 417, DM BD+44   307, TYC 3265-2401-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Omega Andromedae",
	"OType" : "Double or multiple star",
	"Distance" : "28.62",
	"RA_S" : 21.91408519,
	"DEC_S" : 45.40669377,
	"Constellation" : "Andromeda ",
	"AMag" : 4.874,
	"key" : 39055,
	"title" : "Omega Andromedae"
	},
{
	"Index" : "19246",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "49 Andromedae, A Andromedae, HIP 6999, SAO 37275, HD 9057, GC 1806, HR 430, DM BD+46   370, TYC 3282-2272-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "A Andromedae",
	"OType" : "Star",
	"Distance" : "90.1",
	"RA_S" : 22.52542761,
	"DEC_S" : 47.00727721,
	"Constellation" : "Andromeda ",
	"AMag" : 5.372,
	"key" : 39246,
	"title" : "A Andromedae"
	},
{
	"Index" : "15129",
	"Description" : "Upsilon Andromedae (\u03C5 Andromedae, \u03C5 And) is a binary star located approximately 44 light-years away from Earth in the constellation Andromeda. The primary star (Upsilon Andromedae A) is a yellow-white dwarf star that is somewhat younger than the Sun. The second star in the system (Upsilon Andromedae B) is a red dwarf located in a wide orbit.\r\rAs of 2010, four confirmed extrasolar planets are known in orbit around the primary star. All four are likely to be jovian planets that are comparable to Jupiter. Upsilon Andromedae was both the first multiple-planet planetary system to be discovered around a main sequence star, and the first multiple-planet system known in a multiple star system. Upsilon Andromedae A was ranked 21st in the list of top 100 target stars for the NASA Terrestrial Planet Finder mission, which has, however, been reported to have been cancelled as of 2011.\r\rUpsilon Andromedae is located fairly close to the Solar System: the parallax of Upsilon Andromedae A was measured by the Hipparcos astrometry satellite as 74.12 milliarcseconds, corresponding to a distance of 13.49 parsecs (44 light years). Upsilon Andromedae A has an apparent magnitude of +4.09, making it visible to the naked eye even under moderately light-polluted skies, about 10 degrees east of the Andromeda Galaxy. The dimmer star Upsilon Andromedae B is only visible with a telescope.\r\rUpsilon Andromedae A is a yellow-white dwarf of spectral type F8V, similar to the Sun, but younger, more massive, and more luminous. According to its entry in the Geneva\u2013Copenhagen survey, the star is around 3.1 billion years old, and has a similar proportion of iron relative to hydrogen to the Sun. At around 1.3 solar masses, it will have a shorter lifetime than the Sun. The amount of ultraviolet radiation received by any planets in the star\u0027s habitable zone would be similar to the ultraviolet flux the Earth receives from the Sun.\r\rUpsilon Andromedae B is a red dwarf of spectral type M4.5V located at a distance (in the plane of the sky) of 750 AU from the primary star. The true separation between the two stars is unknown because the displacement along the line of sight between us and the Upsilon Andromedae stars is unknown, so this value is a minimum separation. It was discovered in 2002 in data collected as part of the Two Micron All Sky Survey. The star is less massive and far less luminous than the Sun.\r\rThe Washington Double Star Catalog lists two optical components; however, these do not share the system\u0027s proper motion and only appear close to Upsilon Andromedae because they happen to lie near the same line of sight.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "50 Andromedae, Upsilon Andromedae, HIP 7513, SAO 37362, HD 9826, GC 1948, HR 458, DM BD+40   332, TYC 2822-2210-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Upsilon Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "13.49",
	"RA_S" : 24.19934235,
	"DEC_S" : 41.40545674,
	"X" : 254,
	"Y" : 313,
	"Constellation" : "Andromeda ",
	"AMag" : 4.152,
	"key" : 35129,
	"title" : "Upsilon Andromedae"
	},
{
	"Index" : "19245",
	"Description" : "51 Andromedae is a 4th magnitude star, the 5th brighest in the constellation Andromeda. It does not have a Bayer designation. It is occasionally called by the proper name Nembus in Bayer\u0027s Uranometria (1603) and Bode\u0027s star atlas Uranographia (1801).\r\rPtolemy included this star in Andromeda in the Almagest, but it was moved into Perseus by Johann Bayer, who designated it Upsilon Persei (\u03C5 Per). Flamsteed moved it back, and the International Astronomical Union made Flamsteed\u0027s 51 Andromedae its official designation in 1930.\r\rIn Chinese, \u5929\u5927\u5C07\u8ECD (Ti\u0101n D\u00E0 Ji\u0101ng J\u016Bn), meaning Heaven\u0027s Great General, refers to an asterism consisting of 51 Andromedae, \u03B3 Andromedae, \u03C6 Persei, 49 Andromedae, \u03C7 Andromedae, \u03C5 Andromedae, \u03C4 Andromedae, 56 Andromedae, \u03B2 Trianguli, \u03B3 Trianguli and \u03B4 Trianguli. Consequently, 51 Andromedae itself is known as \u5929\u5927\u5C07\u8ECD\u4E09 (Ti\u0101n D\u00E0 Ji\u0101ng J\u016Bn s\u0101n, English: the Third Star of Heaven\u0027s Great General.)\r\r51 Andromedae is an orange K-type giant with an apparent magnitude of +3.59. It is approximately 177 light years from the Earth.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "51 Andromedae, HIP 7607, SAO 37375, HD 9927, GC 1966, HR 464, DM BD+47   467, TYC 3282-2271-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Nembus",
	"OType" : "Star",
	"Distance" : "54.31",
	"RA_S" : 24.49815065,
	"DEC_S" : 48.6282122,
	"X" : 267,
	"Y" : 220,
	"Constellation" : "Andromeda ",
	"AMag" : 3.719,
	"key" : 39245,
	"title" : "Nembus"
	},
{
	"Index" : "15157",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "52 Andromedae, Chi Andromedae, HIP 7719, SAO 37406, HD 10072, GC 1991, HR 469, DM BD+43   343, TYC 2826-2183-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Chi Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "76.58",
	"RA_S" : 24.83749985,
	"DEC_S" : 44.38615816,
	"Constellation" : "Andromeda ",
	"AMag" : 5.106,
	"key" : 35157,
	"title" : "Chi Andromedae"
	},
{
	"Index" : "15102",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "53 Andromedae, Tau Andromedae, HIP 7818, SAO 37418, HD 10205, GC 2025, HR 477, DM BD+39   378, TYC 2819-2290-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Tau Andromedae",
	"OType" : "Variable Star",
	"Distance" : "217.56",
	"RA_S" : 25.14507048,
	"DEC_S" : 40.57704845,
	"Constellation" : "Andromeda ",
	"AMag" : 4.942,
	"key" : 35102,
	"title" : "Tau Andromedae"
	},
{
	"Index" : "15133",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "HIP 7918, SAO 37434, HD 10307, GC 2050, HR 483, DM BD+41  328, TYC 2823-2455-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Gliese 67 (HR 483)",
	"OType" : "Spectroscopic binary",
	"Distance" : "12.74",
	"RA_S" : 25.44648194,
	"DEC_S" : 42.61343591,
	"Constellation" : "Andromeda ",
	"AMag" : 5.027,
	"key" : 35133,
	"title" : "Gliese 67 (HR 483)"
	},
{
	"Index" : "15246",
	"Description" : "Gamma Andromedae (Gamma And, \u03B3 And, \u03B3 Andromedae) is the third brightest star in the constellation of Andromeda. It is also known by the traditional name Almach (also spelt as Almaach, Almaack, Almak, Almaak, or Alamak).\r\rIn 1778, Johann Tobias Mayer discovered that \u03B3 Andromedae was a double star. When examined in a small telescope, it appears to be a bright, golden yellow star (\u03B31 Andromedae) next to a dimmer, indigo blue star (\u03B32 Andromedae), separated by approximately 10 arcseconds. It is considered by stargazers to be a beautiful double star with a striking contrast of color. It was later discovered that \u03B32 Andromedae is itself a triple star system. What appears as a single star to the naked eye is thus a quadruple star system, approximately 350 light-years from the Earth.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "57 Andromedae, Gamma02 Andromedae, HIP 9640B, SAO 37735, HD 12534, GC 2479, HR 604, DM BD+41   395B, TYC 2837-2311-2",
	"group" : { "key" : "Andromeda" },
	"Common" : "Almach",
	"OType" : "Double or multiple star",
	"Distance" : "108",
	"RA_S" : 30.978,
	"DEC_S" : 42.330947,
	"X" : 193,
	"Y" : 289,
	"Constellation" : "Andromeda ",
	"AMag" : 5.021,
	"key" : 35246,
	"title" : "Almach"
	},
{
	"Index" : "15174",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "58 Andromedae, HIP 9977, SAO 55289, HD 13041, GC 2552, HR 620, DM BD+37   486, TYC 2829-2251-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "58 Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "58.67",
	"RA_S" : 32.12191368,
	"DEC_S" : 37.85907972,
	"Constellation" : "Andromeda ",
	"AMag" : 4.804,
	"key" : 35174,
	"title" : "58 Andromedae"
	},
{
	"Index" : "15289",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "60 Andromedae, b Andromedae, HIP 10340, SAO 37867, HD 13520, GC 2645, HR 643, DM BD+43   447, TYC 2842-2371-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "b Andromedae",
	"OType" : "Spectroscopic binary",
	"Distance" : "160.58",
	"RA_S" : 33.30551134,
	"DEC_S" : 44.23165221,
	"Constellation" : "Andromeda ",
	"AMag" : 5.003,
	"key" : 35289,
	"title" : "b Andromedae"
	},
{
	"Index" : "19327",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "6 Persei, HIP 10366, SAO 23047, HD 13530, GC 2653, HR 645, DM BD+50   481, TYC 3293-2271-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "6 Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "64.9",
	"RA_S" : 33.401423,
	"DEC_S" : 51.0658162,
	"Constellation" : "Andromeda ",
	"AMag" : 5.401,
	"key" : 39327,
	"title" : "6 Persei"
	},
{
	"Index" : "19366",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "62 Andromedae, c Andromedae, HIP 10819, SAO 37948, HD 14212, GC 2779, HR 670, DM BD+46   552, TYC 3298-896-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "c Andromedae",
	"OType" : "Star",
	"Distance" : "75.32",
	"RA_S" : 34.81998162,
	"DEC_S" : 47.37997159,
	"Constellation" : "Andromeda ",
	"AMag" : 5.31,
	"key" : 39366,
	"title" : "c Andromedae"
	},
{
	"Index" : "19413",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "64 Andromedae, HIP 11220, SAO 38005, HD 14770, GC 2877, HR 694, DM BD+49   649, TYC 3302-1893-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "64 Andromedae",
	"OType" : "Star",
	"Distance" : "122.21",
	"RA_S" : 36.10381888,
	"DEC_S" : 50.00654637,
	"Constellation" : "Andromeda ",
	"AMag" : 5.291,
	"key" : 39413,
	"title" : "64 Andromedae"
	},
{
	"Index" : "19412",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "65 Andromedae, HIP 11313, SAO 23319, HD 14872, GC 2902, HR 699, DM BD+49   656, TYC 3302-1892-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "65 Andromedae",
	"OType" : "Star",
	"Distance" : "113.13",
	"RA_S" : 36.40593313,
	"DEC_S" : 50.27863162,
	"Constellation" : "Andromeda ",
	"AMag" : 4.895,
	"key" : 39412,
	"title" : "65 Andromedae"
	},
{
	"Index" : "18692",
	"Description" : "Omicron Andromedae (\u03BF And, \u03BF Andromedae) is a star system in the constellation Andromeda. It is approximately 692 light years from Earth.\r\rOmicron Andromedae is a binary star, whose two components are both spectroscopic binaries themselves, making a four-star system. The system as a whole is classified as a blue-white B-type giant with a mean combined apparent magnitude of +3.62.\r\rThe separation of the two brightest components, \u03BF Andromedae A and \u03BF Andromedae B, is 0.34 arcseconds. They have an orbital period of 68.6 years. A is separated from its spectroscopic companion by 0.05 arcseconds. A is a Gamma Cassiopeiae type variable star and the system\u0027s brightness varies from magnitude +3.58 to +3.78. This, in turn, has made determination the orbital period of A\u0027s spectroscopic binary difficult. B\u0027s spectroscopic companion was discovered in 1989, and that binary has a period of 33.01 years.\r\rThis star system has a peculiar velocity of 34.5 \u00B1 5.9 km/s.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "1 Andromedae, Omicron Andromedae, HIP 113726AB, SAO 52609, HD 217675, GC 32095, HR 8762, DM BD+41  4664A, TYC 3224-3434-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Omicron Andromedae",
	"OType" : "Be Star",
	"Distance" : "207.43",
	"RA_S" : 345.48026914,
	"DEC_S" : 42.3259815,
	"X" : 626,
	"Y" : 281,
	"Constellation" : "Andromeda ",
	"AMag" : 3.611,
	"key" : 38692,
	"title" : "Omicron Andromedae"
	},
{
	"Index" : "18691",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "2 Andromedae, HIP 113788AB, SAO 52623, HD 217782A, GC 32110, HR 8766, DM BD+41  4665, TYC 3224-3432-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "2 Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "128.53",
	"RA_S" : 345.65159374,
	"DEC_S" : 42.75780095,
	"Constellation" : "Andromeda ",
	"AMag" : 5.109,
	"key" : 38691,
	"title" : "2 Andromedae"
	},
{
	"Index" : "22287",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "3 Andromedae, HIP 113919, SAO 52649, HD 218031, GC 32144, HR 8780, DM BD+49  4028, TYC 3631-2230-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "3 Andromedae",
	"OType" : "High proper-motion Star",
	"Distance" : "54.16",
	"RA_S" : 346.04576762,
	"DEC_S" : 50.05208912,
	"Constellation" : "Andromeda ",
	"AMag" : 4.759,
	"key" : 42287,
	"title" : "3 Andromedae"
	},
{
	"Index" : "22209",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "4 Andromedae, HIP 114200, SAO 52711, HD 218452, GC 32216, HR 8804, DM BD+45  4149, TYC 3623-2738-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "4 Andromedae",
	"OType" : "Star",
	"Distance" : "106.8",
	"RA_S" : 346.91360554,
	"DEC_S" : 46.38722951,
	"Constellation" : "Andromeda ",
	"AMag" : 5.457,
	"key" : 42209,
	"title" : "4 Andromedae"
	},
{
	"Index" : "22288",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "7 Andromedae, HIP 114570, SAO 52787, HD 219080, GC 32316, HR 8830, DM BD+48  3964, TYC 3631-2231-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "7 Andromedae",
	"OType" : "Star",
	"Distance" : "24.59",
	"RA_S" : 348.13752084,
	"DEC_S" : 49.4062064,
	"Constellation" : "Andromeda ",
	"AMag" : 4.558,
	"key" : 42288,
	"title" : "7 Andromedae"
	},
{
	"Index" : "22410",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "8 Andromedae, HIP 115022, SAO 52871, HD 219734, GC 32432, HR 8860, DM BD+48  3991, TYC 3644-2208-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "8 Andromedae",
	"OType" : "Variable Star",
	"Distance" : "172.23",
	"RA_S" : 349.43602606,
	"DEC_S" : 49.01530047,
	"Constellation" : "Andromeda ",
	"AMag" : 5.012,
	"key" : 42410,
	"title" : "8 Andromedae"
	},
{
	"Index" : "18760",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "14 Andromedae, HIP 116076, SAO 73311, HD 221345, GC 32703, HR 8930, DM BD+38  5023, TYC 3231-323-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "14 Andromedae",
	"OType" : "Variable Star",
	"Distance" : "79.13",
	"RA_S" : 352.82255876,
	"DEC_S" : 39.23619899,
	"Constellation" : "Andromeda ",
	"AMag" : 5.341,
	"key" : 38760,
	"title" : "14 Andromedae"
	},
{
	"Index" : "22367",
	"Description" : "Lambda Andromedae (\u03BB And, \u03BB Andromedae) is the Bayer designation for a binary star in the northern constellation of Andromeda. At an estimated distance of approximately 86.1 light-years (26.4 parsecs) from Earth, it has an apparent visual magnitude of +3.8. This is bright enough to be seen with the naked eye.\r\rLambda Andromedae is a single-lined spectroscopic binary with an orbital period of 20.5212 days. The spectrum of the primary matches a stellar classification of G8 III-IV, suggesting that it is an evolved star that lies part way between the subgiant and giant stages. The mass of this star is similar to the Sun, but it has expanded to around seven times the Sun\u0027s radius. It is radiating over 23 times the luminosity of the Sun from its outer envelope at an effective temperature of 4,800 K, giving it the characteristic yellow hue of a G-type star.\r\rThis is an RS Canum Venaticorum variable and its brightness varies by 0.225 magnitudes, reaching a maximum of 3.70, with a period of 54.2 days. Such variability is theorized to occur because of tidal friction, which results in chromospheric activity. However, the orbit of this system is nearly circular, so the cause of this system\u0027s variability remains uncertain. The X-ray luminosity of this star, as measured by the ROSAT satellite, is 2.95 \u00D7 1030 erg s\u20131.\r\rIn Chinese, \u87A3\u86C7 (T\u00E9ng Sh\u00E9), meaning Flying Serpent, refers to an asterism consisting of \u03BB Andromedae, \u03B1 Lacertae, 4 Lacertae, \u03C02 Cygni, \u03C01 Cygni, HD 206267, \u03B5 Cephei, \u03B2 Lacertae, \u03C3 Cassiopeiae, \u03C1 Cassiopeiae, \u03C4 Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, \u03BA Andromedae, \u03B9 Andromedae, and \u03C8 Andromedae. Consequently, \u03BB Andromedae itself is known as \u87A3\u86C7\u5341\u4E5D (T\u00E9ng Sh\u00E9 sh\u00EDji\u01D4, English: the Nineteenth Star of Flying Serpent)",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "16 Andromedae, Lambda Andromedae, HIP 116584, SAO 53204, HD 222107, GC 32832, HR 8961, DM BD+45  4283, TYC 3638-2515-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Lambda Andromedae",
	"OType" : "Variable of RS CVn type",
	"Distance" : "26.41",
	"RA_S" : 354.39101265,
	"DEC_S" : 46.45815324,
	"X" : 532,
	"Y" : 246,
	"Constellation" : "Andromeda ",
	"AMag" : 3.964,
	"key" : 42367,
	"title" : "Lambda Andromedae"
	},
{
	"Index" : "18852",
	"Description" : "Iota Andromedae (\u03B9 And, \u03B9 Andromedae) is a star in the constellation Andromeda. It has an apparent magnitude of +4.29 and is approximately 500 light years from Earth.\r\rIota Andromedae is a B-type main sequence star with a stellar classification of B8 V. It is among the least variable stars observed during the Hipparcos mission.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "17 Andromedae, Iota Andromedae, HIP 116631, SAO 53216, HD 222173, GC 32850, HR 8965, DM BD+42  4720, TYC 3243-1412-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Iota Andromedae",
	"OType" : "Star",
	"Distance" : "153.03",
	"RA_S" : 354.53417535,
	"DEC_S" : 43.26807471,
	"X" : 539,
	"Y" : 288,
	"Constellation" : "Andromeda ",
	"AMag" : 4.266,
	"key" : 38852,
	"title" : "Iota Andromedae"
	},
{
	"Index" : "22428",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "18 Andromedae, HIP 116709, SAO 35642, HD 222304, GC 32864, HR 8967, DM BD+49  4180, TYC 3646-911-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "18 Andromedae",
	"OType" : "Star",
	"Distance" : "128.93",
	"RA_S" : 354.78471294,
	"DEC_S" : 50.47172762,
	"Constellation" : "Andromeda ",
	"AMag" : 5.33,
	"key" : 42428,
	"title" : "18 Andromedae"
	},
{
	"Index" : "18862",
	"Description" : "Kappa Andromedae (\u03BA And, \u03BA Andromedae) is the Bayer designation for a bright star in the constellation of Andromeda. Its apparent visual magnitude is 4.1. Based on the star\u0027s ranking on the Bortle Dark-Sky Scale, it is luminous enough to be visible from the suburbs and from urban outskirts, but not from brightly lit inner city regions. Parallax measurements made during the Hipparcos mission place it at a distance of approximately 168 light-years (52 parsecs) from Earth.\r\rKappa Andromedae has a stellar classification of B9 IVn, indicating that it is a subgiant star in the process of evolving away from the main sequence. It has 2.3 times the radius of the Sun and is spinning rapidly, with a projected rotational velocity of 176 km/s. The outer envelope of the star is radiating energy into space with an effective temperature of 11,361 K, producing a blue-white hue.",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "19 Andromedae, Kappa Andromedae, HIP 116805, SAO 53264, HD 222439, GC 32886, HR 8976, DM BD+43  4522, TYC 3244-1530-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Kappa Andromedae",
	"OType" : "Star",
	"Distance" : "51.62",
	"RA_S" : 355.10211016,
	"DEC_S" : 44.33393551,
	"X" : 531,
	"Y" : 275,
	"Constellation" : "Andromeda ",
	"AMag" : 4.126,
	"key" : 38862,
	"title" : "Kappa Andromedae"
	},
{
	"Index" : "22368",
	"MapNum" : "01",
	"ImageNum" : "01",
	"Desig" : "20 Andromedae, Psi Andromedae, HIP 117221AE, SAO 53355, HD 223047, GC 32988, HR 9003, DM BD+45  4321, TYC 3638-2516-1",
	"group" : { "key" : "Andromeda" },
	"Common" : "Psi Andromedae",
	"OType" : "Double or multiple star",
	"Distance" : "300.16",
	"RA_S" : 356.50853572,
	"DEC_S" : 46.42026893,
	"Constellation" : "Andromeda ",
	"AMag" : 5.088,
	"key" : 42368,
	"title" : "Psi Andromedae"
	},
{
	"Index" : "50155",
	"Description" : "Epsilon Antliae (\u03B5 Ant, \u03B5 Antliae) is the Bayer designation for a star in the southern constellation of Antlia. The apparent visual magnitude of this star is +4.51, which means it is visible to the naked eye. From parallax measurements, the distance to this star is known to be around 710 light-years (220 parsecs). Photometry measurements during the Hipparcos mission indicate that this star is undergoing periodic variability by 0.0034 magnitudes over an 11.07941 day cycle.\r\rThe stellar classification of this star is K3 IIIa, where the luminosity class of III indicates that this is an evolved giant star. It is around 37 times the radius of the Sun.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Epsilon Antliae, HIP 46515, SAO 200416, HD 82150, GC 13091, HR 3765, DM CD-35  5724, TYC 7166-3038-1",
	"group" : { "backgroundImage" : "images/Alignment/02.png",
		"description" : "Antlia (pron.: /\u02C8\u00E6ntli\u0259/; from Ancient Greek \u1F00\u03BD\u03C4\u03BB\u03AF\u03B1) is a constellation in the southern sky. Its name means \u0022pump\u0022 and it specifically represents an air pump. The constellation was created in the 18th century from an undesignated region of sky, so the stars comprising Antlia are faint. Antlia is bordered by Hydra the sea snake, Pyxis the compass, Vela the sails, and Centaurus the centaur. This group of constellations is prominent in the southern sky in late winter and spring. NGC 2997, a spiral galaxy, and the Antlia Dwarf Galaxy lie within Antlia\u0027s borders.\r\rAntlia was created in 1756 by the French astronomer Abb\u00E9 Nicolas Louis de Lacaille, who created fourteen constellations for the southern sky to fill some faint regions. Though Antlia was technically visible to ancient Greek astronomers, its stars were too faint to have been included in any constellations. Because of this, its main stars have no particular pattern and it is devoid of bright deep-sky objects. It was originally named Antlia pneumatica (\u0022Machine Pneumatique\u0022 in French) to commemorate the air pump invented by the French physicist Denis Papin. Lacaille and Johann Bode each depicted Antlia differently, as either the single-cylinder vacuum pump used in Papin\u0027s initial experiments, or the more advanced double-cylinder version. The International Astronomical Union subsequently adopted it as one of the 88 modern constellations. There is no mythology attached to Antlia as Lacaille discontinued the tradition of giving names from mythology to constellations and instead chose names mostly from scientific instruments.",
		"key" : "Antlia",
		"grouptype" : "Antlia",
		"Meaning" : "air pump",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Antlia",
		"title" : "Antlia Objects Group" },
	"Common" : "Epsilon Antliae",
	"OType" : "Star",
	"Distance" : "217.15",
	"RA_S" : 142.31132975,
	"DEC_S" : -35.95133667,
	"X" : 352,
	"Y" : 264,
	"Constellation" : "Antlia ",
	"AMag" : 4.658,
	"key" : 70155,
	"title" : "Epsilon Antliae"
	},
{
	"Index" : "45929",
	"Description" : "Theta Antliae (\u03B8 Ant, \u03B8 Antliae) is the Bayer designation for a binary star in the southern constellation of Antlia. The pair have a combined apparent visual magnitude of +4.78; the brighter component is magnitude +5.30 while the secondary is +6.18. Based upon parallax measurements, it is located at a distance of around 340 light-years (100 parsecs) from Earth.\r\rThe primary component of this system, \u03B8 Ant A, has a stellar classification of A8 Vm, indicating that it is an A-type main sequence star with enhanced metallic lines in its spectrum. The companion, \u03B8 Ant B, is a giant star with a classification of G7 III. The pair have an orbital period of 18.3 years, a significant eccentricity of 0.445, and they have an angular separation of 0.1 arcseconds.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Theta Antliae, HIP 47758AS, SAO 177908, HD 84367, GC 13425, HR 3871, DM CD-27  6881, TYC 6610-2315-1",
	"group" : { "key" : "Antlia" },
	"Common" : "Theta Antliae",
	"OType" : "Double or multiple star",
	"Distance" : "103.77",
	"RA_S" : 146.05040191,
	"DEC_S" : -27.76947025,
	"X" : 310,
	"Y" : 157,
	"Constellation" : "Antlia ",
	"AMag" : 4.848,
	"key" : 65929,
	"title" : "Theta Antliae"
	},
{
	"Index" : "50266",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Eta Antliae, HIP 48926, SAO 200926, HD 86629, GC 13741, HR 3947, DM CD-35  6050, TYC 7181-1572-1",
	"group" : { "key" : "Antlia" },
	"Common" : "Eta Antliae",
	"OType" : "Star",
	"Distance" : "33.31",
	"RA_S" : 149.71781621,
	"DEC_S" : -35.89097275,
	"Constellation" : "Antlia ",
	"AMag" : 5.258,
	"key" : 70266,
	"title" : "Eta Antliae"
	},
{
	"Index" : "54782",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 50888, SAO 201346, HD 90132, GC 14281, HR 4086, DM CD-37 6509, TYC 7709-2840-1",
	"group" : { "key" : "Antlia" },
	"Common" : "HD  90132",
	"OType" : "High proper-motion Star",
	"Distance" : "41.45",
	"RA_S" : 155.87206249,
	"DEC_S" : -38.00984075,
	"Constellation" : "Antlia ",
	"AMag" : 5.359,
	"key" : 74782,
	"title" : "HD  90132"
	},
{
	"Index" : "50294",
	"Description" : "Alpha Antliae (Alpha Ant, \u03B1 Antliae, \u03B1 Ant) is the brightest star in the constellation of Antlia but it has not been given a proper name. It is approximately 370 light-years from the Solar System. It is a K-type giant star that varies in apparent visual magnitude between 4.22 and 4.29. This star has 2.2 times the mass of the Sun and has expanded to 53 times the solar radius. Compared to the Sun, it has only 41% of the abundance of elements other than hydrogen and helium.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Alpha Antliae, HIP 51172, SAO 201405, HD 90610, GC 14352, HR 4104, DM CD-30  8465, TYC 7184-2065-1",
	"group" : { "key" : "Antlia" },
	"Common" : "Alpha Antliae",
	"OType" : "Variable Star",
	"Distance" : "111.83",
	"RA_S" : 156.78792132,
	"DEC_S" : -31.06777987,
	"X" : 190,
	"Y" : 212,
	"Constellation" : "Antlia ",
	"AMag" : 4.424,
	"key" : 70294,
	"title" : "Alpha Antliae"
	},
{
	"Index" : "50494",
	"Description" : "Iota Antliae (\u03B9 Ant, \u03B9 Antliae) is the Bayer designation for a star in the southern constellation of Antlia. It has an apparent visual magnitude of +4.60, making it a faint naked eye star. From parallax measurements, the distance to this star can be estimated as 190 light-years (58 parsecs). The spectrum of Iota Antliae matches a stellar classification of K1 III, indicating that this is an evolved star that is now in its giant phase. It is a core helium fusing star that is classified as a member of the red clump evolutionary branch.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Iota Antliae, HIP 53502, SAO 201927, HD 94890, GC 15047, HR 4273, DM CD-36  6808, TYC 7211-2295-1",
	"group" : { "key" : "Antlia" },
	"Common" : "Iota Antliae",
	"OType" : "Star",
	"Distance" : "58.27",
	"RA_S" : 164.17938017,
	"DEC_S" : -37.13776866,
	"X" : 127,
	"Y" : 306,
	"Constellation" : "Antlia ",
	"AMag" : 4.707,
	"key" : 70494,
	"title" : "Iota Antliae"
	},
{
	"Index" : "50503",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 54173AB, SAO 202067, HD 96146, GC 15238, HR 4313, DM CD-35 6954, TYC 7212-2221-1",
	"group" : { "key" : "Antlia" },
	"Common" : "HR 4313",
	"OType" : "Star",
	"Distance" : "157.39",
	"RA_S" : 166.22581712,
	"DEC_S" : -35.80467697,
	"Constellation" : "Antlia ",
	"AMag" : 5.416,
	"key" : 70503,
	"title" : "HR 4313"
	},
{
	"Index" : "70719",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Eta Apodis, HIP 69896, SAO 258693, HD 123998, GC 19211, HR 5303, DM CP-80   706, TYC 9439-1501-1",
	"group" : { "backgroundImage" : "images/Alignment/03.png",
		"description" : "Apus is a faint constellation in the southern sky, first defined in the late 16th century. Its name means \u0022no feet\u0022 in Greek, and it represents a bird-of-paradise (which were once believed to lack feet). It is bordered by Triangulum Australe, Circinus, Musca, Chamaeleon, Octans, Pavo and Ara. Its genitive is \u0022Apodis\u0022.\r\rApus was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35 cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. Plancius called the constellation \u0022Paradysvogel Apis Indica\u0022; the first word is Dutch for \u0027bird of paradise[disambiguation needed]\u0027, but the others are Latin for \u0022Indian Bee\u0022; \u0022apis\u0022 (Latin for \u0022bee\u0022) is presumably an error for \u0022avis\u0022 or \u0022bird\u0022. The name \u0022Apus\u0022 is derived from the Greek \u0022apous\u0022, meaning \u0022without feet\u0022, which referred to the Western conception of a bird-of-paradise as one without feet, a misconception perpetuated by the fact that the only specimens available in the West had both feet and wings removed. These specimens began to arrive in Europe in 1522, when the survivors of Ferdinand Magellan\u0027s expedition brought them home.\r\rAfter its introduction on Plancius\u0027s globe, the first known depiction of the constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603, where it was called \u0022Apis Indica\u0022.",
		"key" : "Apus",
		"grouptype" : "Apus",
		"Meaning" : "Bird-of-paradise/Exotic Bird/Extraordinary Bird",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Apus",
		"title" : "Apus Objects Group" },
	"Common" : "Eta Apodis",
	"OType" : "Star",
	"Distance" : "42.33",
	"RA_S" : 214.55788849,
	"DEC_S" : -81.00776096,
	"Constellation" : "Apus ",
	"AMag" : 4.92,
	"key" : 90719,
	"title" : "Eta Apodis"
	},
{
	"Index" : "70699",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Epsilon Apodis, HIP 70248, SAO 257142, HD 124771, GC 19305, HR 5336, DM CP-79   755, TYC 9435-2528-1",
	"group" : { "key" : "Apus" },
	"Common" : "Epsilon Apodis",
	"OType" : "Be Star",
	"Distance" : "197.18",
	"RA_S" : 215.59653693,
	"DEC_S" : -80.1089414,
	"Constellation" : "Apus ",
	"AMag" : 5.033,
	"key" : 90699,
	"title" : "Epsilon Apodis"
	},
{
	"Index" : "70706",
	"Description" : "Alpha Apodis (Alpha Aps, \u03B1 Apodis, \u03B1 Aps) is the brightest star in the southern circumpolar constellation of Apus, with an apparent magnitude of approximately 3.825. It had the Greek alpha designation at part of the constellation Johann Bode called Apis Indica in his 1603 Uranometria star atlas. With a declination of \u201379\u00B0, this is a circumpolar star for much of the southern hemisphere. It can be identified on the night sky by drawing an imaginary line through Alpha Centauri and Alpha Circini then extending it toward the south celestial pole.\r\rThis is a giant star with a stellar classification of K2.5III, indicating that this star has consumed the hydrogen at its core and has evolved away from the main sequence. It has expanded to an estimated radius of about 48 times the radius of the Sun and is emitting 980 times the Sun\u0027s luminosity. The photosphere has an effective temperature of 4,256 K, giving the star the characteristic orange hue of a K-type star. Based upon parallax measurements, this star is roughly 447 light-years from the Earth. It is not known to have a companion.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u7570\u96C0 (Y\u00EC Qu\u00E8), meaning Exotic Bird, refers to an asterism consisting of \u03B1 Apodis, \u03B6 Apodis, \u03B9 Apodis, \u03B2 Apodis, \u03B3 Apodis, \u03B4 Octantis, \u03B41 Apodis, \u03B7 Apodis, and \u03B5 Apodis. Consequently, \u03B1 Apodis itself is known as \u7570\u96C0\u516B (Y\u00EC Qu\u00E8 b\u0101, English: the Eighth Star of Exotic Bird.)",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Alpha Apodis, HIP 72370, SAO 257193, HD 129078, GC 19834, HR 5470, DM CP-78   893, TYC 9436-2393-1",
	"group" : { "key" : "Apus" },
	"Common" : "Alpha Apodis",
	"OType" : "Star",
	"Distance" : "136.93",
	"RA_S" : 221.96545209,
	"DEC_S" : -79.04475077,
	"X" : 412,
	"Y" : 559,
	"Constellation" : "Apus ",
	"AMag" : 3.968,
	"key" : 90706,
	"title" : "Alpha Apodis"
	},
{
	"Index" : "69625",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Kappa01 Apodis, HIP 76013, SAO 257289, HD 137387, GC 20801, HR 5730, DM CP-72  1802, TYC 9271-2376-1",
	"group" : { "key" : "Apus" },
	"Common" : "Kappa01 Apodis",
	"OType" : "Be Star",
	"Distance" : "375.48",
	"RA_S" : 232.878424,
	"DEC_S" : -73.38958753,
	"Constellation" : "Apus ",
	"AMag" : 5.373,
	"key" : 89625,
	"title" : "Kappa01 Apodis"
	},
{
	"Index" : "70774",
	"Description" : "Delta Apodis (\u03B4 Aps, \u03B4 Apodis) is the Bayer designation for a double star in the southern constellation of Apus.\r\rThe brighter star, \u03B4\u00B9 Apodis, is a M-type red giant with a mean apparent magnitude of +4.68. It is classified as an irregular variable star and its brightness varies from magnitude +4.66 to +4.87. At an angular separation of 102.9 arcseconds is \u03B4\u00B2 Apodis, an orange K-type giant with an apparent magnitude of +5.27.\r\rHipparcos data report the distance to \u03B4\u00B9 Apodis to be approximately 760 light years, while \u03B4\u00B2 Apodis is found to be around 610 light years from Earth. They may form a common proper motion pair.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u7570\u96C0 (Y\u00EC Qu\u00E8), meaning Exotic Bird, refers to an asterism consisting of \u03B41 Apodis, \u03B6 Apodis, \u03B9 Apodis, \u03B2 Apodis, \u03B3 Apodis, \u03B4 Octantis, \u03B7 Apodis, \u03B1 Apodis and \u03B5 Apodis. Consequently, \u03B41 Apodis itself is known as \u7570\u96C0\u516D (Y\u00EC Qu\u00E8 li\u00F9, English: the Sixth Star of Exotic Bird.)",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Delta01 Apodis, HIP 80047, SAO 257380, HD 145366, GC 21862, HR 6020, DM CP-78  1092, TYC 9446-3517-1",
	"group" : { "key" : "Apus" },
	"Common" : "Delta Apodis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "233.25",
	"RA_S" : 245.08667778,
	"DEC_S" : -78.69574141,
	"X" : 352,
	"Y" : 558,
	"Constellation" : "Apus ",
	"AMag" : 4.902,
	"key" : 90774,
	"title" : "Delta Apodis"
	},
{
	"Index" : "70773",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Delta02 Apodis, HIP 80057, SAO 257381, HD 145388, GC 21865, HR 6021, DM CP-78  1093, TYC 9446-3516-1",
	"group" : { "key" : "Apus" },
	"Common" : "Delta02 Apodis",
	"OType" : "Star",
	"Distance" : "187.58",
	"RA_S" : 245.11190377,
	"DEC_S" : -78.66749647,
	"Constellation" : "Apus ",
	"AMag" : 5.411,
	"key" : 90773,
	"title" : "Delta02 Apodis"
	},
{
	"Index" : "70798",
	"Description" : "Gamma Apodis (\u03B3 Aps, \u03B3 Apodis) is the Bayer designation for a star in the southern circumpolar constellation of Apus. From parallax measurements, the distance to this star can be estimated as 156 light-years (48 pc). It is visible to the naked eye with an apparent visual magnitude of 3.86. A stellar classification of G9 III identifies it as a giant star in the later stages of its evolution. It is an active X-ray source with a luminosity of 1.607 \u00D7 1030 erg s\u20131, making it one of the 100 strongest stellar X-ray sources within 50 parsecs of the Sun.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u7570\u96C0 (Y\u00EC Qu\u00E8), meaning Exotic Bird, refers to an asterism consisting of \u03B3 Apodis, \u03B6 Apodis, \u03B9 Apodis, \u03B2 Apodis, \u03B4 Octantis, \u03B41 Apodis, \u03B7 Apodis, \u03B1 Apodis and \u03B5 Apodis. Consequently, \u03B3 Apodis itself is known as \u7570\u96C0\u56DB (Y\u00EC Qu\u00E8 s\u00EC, English: the Fourth Star of Exotic Bird.)",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma Apodis, HIP 81065, SAO 257407, HD 147675, GC 22142, HR 6102, DM CP-78  1103, TYC 9450-2282-1",
	"group" : { "key" : "Apus" },
	"Common" : "Gamma Apodis",
	"OType" : "Star",
	"Distance" : "47.91",
	"RA_S" : 248.36284398,
	"DEC_S" : -78.897149,
	"X" : 346,
	"Y" : 563,
	"Constellation" : "Apus ",
	"AMag" : 3.957,
	"key" : 90798,
	"title" : "Gamma Apodis"
	},
{
	"Index" : "70783",
	"Description" : "Beta Apodis (\u03B2 Aps, \u03B2 Apodis) is the Bayer designation for a star in the southern circumpolar constellation of Apus. It is located approximately 158 light-years (48 parsecs) from Earth, as determined by parallax measurements. The apparent visual magnitude of this star is +4.24, which is bright enough to be seen with the naked eye\r\rThe spectrum of this star matches the characteristics of a K0 III, which, according to models of stellar evolution, indicates that it is in the giant star stage, having exhausted the supply of hydrogen at its core. The measured angular diameter of this star is 2.09 \u00B1 0.11 mas. At the estimated distance of this star, this yields a physical size of about 11 times the radius of the Sun. The expanded outer atmosphere of Beta Apodis has an effective temperature of about 4,900 K. This heat is causing it to glow with the characteristic orange hue of a K-type star.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u7570\u96C0 (Y\u00EC Qu\u00E8), meaning Exotic Bird, refers to an asterism consisting of \u03B2 Apodis, \u03B6 Apodis, \u03B9 Apodis, \u03B3 Apodis, \u03B4 Octantis, \u03B41 Apodis, \u03B7 Apodis, \u03B1 Apodis and \u03B5 Apodis. Consequently, \u03B2 Apodis itself is known as \u7570\u96C0\u4E09 (Y\u00EC Qu\u00E8 s\u0101n, English: the Third Star of Exotic Bird.)",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Beta Apodis, HIP 81852, SAO 257424, HD 149324, GC 22370, HR 6163, DM CP-77  1221, TYC 9447-3154-1",
	"group" : { "key" : "Apus" },
	"Common" : "Beta Apodis",
	"OType" : "High proper-motion Star",
	"Distance" : "48.12",
	"RA_S" : 250.76940005,
	"DEC_S" : -77.51743677,
	"X" : 334,
	"Y" : 548,
	"Constellation" : "Apus ",
	"AMag" : 4.346,
	"key" : 90783,
	"title" : "Beta Apodis"
	},
{
	"Index" : "69672",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Zeta Apodis, HIP 84969, SAO 253882, HD 156277, GC 23392, HR 6417, DM CP-67  3310, TYC 9276-1692-1",
	"group" : { "key" : "Apus" },
	"Common" : "Zeta Apodis",
	"OType" : "Star",
	"Distance" : "91.08",
	"RA_S" : 260.49782203,
	"DEC_S" : -67.77066774,
	"Constellation" : "Apus ",
	"AMag" : 4.895,
	"key" : 89672,
	"title" : "Zeta Apodis"
	},
{
	"Index" : "69702",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Iota Apodis, HIP 84979AB, SAO 257491, HD 156190, GC 23388, HR 6411, DM CP-69  2719, TYC 9280-646-1",
	"group" : { "key" : "Apus" },
	"Common" : "Iota Apodis",
	"OType" : "Double or multiple star",
	"Distance" : "404.8583",
	"RA_S" : 260.52448243,
	"DEC_S" : -70.12320647,
	"Constellation" : "Apus ",
	"AMag" : 5.377,
	"key" : 89702,
	"title" : "Iota Apodis"
	},
{
	"Index" : "34321",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "1 Aquarii, HIP 101936, SAO 126062, HD 196758, GC 28761, HR 7897, DM BD-00  4064, TYC 511-1136-1",
	"group" : { "backgroundImage" : "images/Alignment/05.png",
		"description" : "Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for \u0022water-carrier\u0022 or \u0022cup-carrier\u0022, and its symbol is \u2652, a representation of water.\r\rAquarius is one of the oldest of the recognized constellations along the zodiac (the sun\u0027s apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.\r\rAquarius is identified as GU.LA \u0022The Great One\u0022 in the Babylonian star catalogues and represents the god Ea himself, who is commonly depicted holding an overflowing vase. The Babylonian star-figure appears on entitlement stones and cylinder seals from the second millennium. It contained the winter solstice in the Early Bronze Age. In Old Babylonian astronomy, Ea was the ruler of the southernmost quarter of the Sun\u0027s path, the \u0022Way of Ea\u0022, corresponding to the period of 45 days on either side of winter solstice. Aquarius was also associated with the destructive floods that the Babylonians regularly experienced, and thus was negatively connoted. In Ancient Egypt, Aquarius was associated with the annual flood of the Nile; the banks were said to flood when Aquarius put his jar into the river, beginning spring.",
		"key" : "Aquarius",
		"grouptype" : "Aquarius",
		"Meaning" : "water-bearer",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Aquarius",
		"title" : "Aquarius Objects Group" },
	"Common" : "1 Aquarii",
	"OType" : "Star",
	"Distance" : "71.29",
	"RA_S" : 309.85371126,
	"Constellation" : "Aquarius ",
	"AMag" : 5.27,
	"key" : 54321,
	"title" : "1 Aquarii"
	},
{
	"Index" : "39081",
	"Description" : "Epsilon Aquarii (\u03B5 Aqr, \u03B5 Aquarii) is the Bayer designation for a star in the equatorial zodiac constellation of Aquarius. It has an the traditional name Albali and is visible to the naked eye with an apparent visual magnitude of 3.77. The distance to this star can be determined from parallax measurements, yielding an estimated value of around 208 light-years (64 pc) from Earth. Epsilon Aquarii is an A-type main sequence star with a stellar classification of A1 V.\r\rThis star has an obscure traditional name, Albali, from the Arabic \u0627\u0644\u0628\u0627\u0644\u0639 alb\u0101li\u0027 \u0022the swallower\u0022. (See also Albulaan.) In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Nir Saad Bula (\u0646\u064A\u0631 \u0633\u0639\u062F \u0623\u0644\u0628\u0644\u0639 - nayyir sa\u0027d al bula\u02BD), which was translated into Latin as Lucida Fortun\u00E6 Dissipantis, meaning the brightest of luck of the swallower. This star, along with \u03BC Aqr (Albulaan) and \u03BD Aqr (Albulaan), were al Bula\u02BD (\u0627\u0644\u0628\u0644\u0639), the Swallower.\r\rIn Chinese, \u594E\u5BBF (N\u01DA S\u00F9), meaning Girl (asterism) (or Woman), refers to an asterism consisting of \u03B5 Aquarii, \u03BC Aquarii, 4 Aquarii, 5 Aquarii and 3 Aquarii. Consequently, \u03B5 Aquarii itself is known as \u5973\u5BBF\u4E00 (N\u01DA S\u00F9 y\u012B, English: the First Star of Girl / Woman.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "2 Aquarii, Epsilon Aquarii, HIP 102618, SAO 144810, HD 198001, GC 28978, HR 7950, DM BD-10  5506, TYC 5760-1997-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Albali",
	"OType" : "Star suspected of Variability",
	"Distance" : "63.68",
	"RA_S" : 311.91896774,
	"DEC_S" : -9.49577641,
	"X" : 629,
	"Y" : 283,
	"Constellation" : "Aquarius ",
	"AMag" : 3.758,
	"key" : 59081,
	"shortTitle" : "Al Bali; Al'bali",
	"title" : "Albali"
	},
{
	"Index" : "34811",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "3 Aquarii, k Aquarii, HIP 102624, SAO 144814, HD 198026, GC 28979, HR 7951, DM BD-05  5378, TYC 5186-2125-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "k Aquarii",
	"OType" : "Long-period variable star",
	"Distance" : "178.99",
	"RA_S" : 311.93432317,
	"DEC_S" : -5.02769968,
	"Constellation" : "Aquarius ",
	"AMag" : 4.638,
	"key" : 54811,
	"title" : "k Aquarii"
	},
{
	"Index" : "39066",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "6 Aquarii, Mu Aquarii, HIP 103045, SAO 144895, HD 198743, GC 29109, HR 7990, DM BD-09  5598, TYC 5757-1943-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Mu Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "48.2",
	"RA_S" : 313.16347063,
	"DEC_S" : -8.98331511,
	"Constellation" : "Aquarius ",
	"AMag" : 4.756,
	"key" : 59066,
	"title" : "Mu Aquarii"
	},
{
	"Index" : "39190",
	"Description" : "Nu Aquarii (\u03BD Aqr, \u03BD Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It shares the traditional name Albulaan with \u03BC Aquarii. The name derives from an Arabic term al-bulac\u0101n (\u0623\u0644\u0628\u0648\u0644\u0639\u0627\u0646) meaning \u0022the two swallowers\u0022. This star, along with \u03B5 Aqr (Albali) and \u03BC Aqr (Albulaan), were al Bula\u02BD (\u0627\u0644\u0628\u0644\u0639), the Swallower.\r\rIn Chinese, \u5929\u58D8\u57CE (Ti\u0101n L\u011Bi Ch\u00E9ng), meaning Celestial Ramparts, refers to an asterism consisting of \u03BD Aquarii, \u03BE Aquarii, 46 Capricorni, 47 Capricorni, \u03BB Capricorni, 50 Capricorni, 18 Aquarii, 29 Capricorni, 9 Aquarii, 8 Aquarii, 14 Aquarii, 17 Aquarii and 19 Aquarii. Consequently, \u03BD Aquarii itself is known as \u5929\u58D8\u57CE\u5341 (Ti\u0101n L\u011Bi Ch\u00E9ng sh\u00ED, English: the Tenth Star of Celestial Ramparts.)\r\rWith an apparent visual magnitude of 4.52, Nu Aquarii is visible to the naked eye. Its distance from Earth, as determined from parallax measurements, is around 159 light-years (49 parsecs). At an estimated age of 708 million years, it has evolved into a giant star with a spectrum that matches a stellar classification of G8 III. It has than double the mass of the Sun and has expanded to eight times the Sun\u0027s radius. Nu Aquarii is radiating 37-fold the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,920 K. At this heat, the star is glowing with the yellowish hue of a G-type star.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "13 Aquarii, Nu Aquarii, HIP 104459, SAO 164182, HD 201381, GC 29571, HR 8093, DM BD-11  5538, TYC 5779-1803-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Albulaan",
	"OType" : "Star",
	"Distance" : "48.85",
	"RA_S" : 317.39853511,
	"DEC_S" : -11.37169266,
	"X" : 558,
	"Y" : 303,
	"Constellation" : "Aquarius ",
	"AMag" : 4.601,
	"key" : 59190,
	"title" : "Albulaan"
	},
{
	"Index" : "34992",
	"Description" : "Beta Aquarii (\u03B2 Aqr, \u03B2 Aquarii) is a double star in the constellation Aquarius. It has the traditional name Sadalsuud, from an Arabic expression \u0633\u0639\u062F \u0627\u0644\u0633\u0639\u0648\u062F sa\u0027d al-su\u0027\u016Bd, the \u0022luck of lucks\u0022. Other spellings that are sometimes encountered are Sad es Saud, Sadalsund, and Saad el Sund.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Nir Saad al Saaoud, which was translated into Latin as Lucida Fortun\u00E6 Fortunarum (rather identic with R.H. Allen), meaning the brightest of luck of lucks.\r\rSadalsuud is the brightest star in Aquarius with an apparent magnitude of 2.87 and a stellar classification of G0 Ib. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Based upon parallax measurements, it is located at a distance of about 540 light-years (160 parsecs) from the Earth. The mass of this star is about 6.0 to 6.5 times the mass of the Sun, but it is emitting roughly 2,300 times the Sun\u0027s luminosity implying a radius that is 50 times that of the Sun. It has an estimated age of 60 million years; old enough for a star of this mass to evolve into a supergiant. The estimated effective temperature of the star\u0027s outer envelope is about 5,700 K, giving it the characteristic yellow hue of G-type stars.\r\rX-ray emissions from the corona of this star have been detected using the Chandra X-ray Observatory; among the first such detections of X-rays for a G-type supergiant. A secondary X-ray source discovered near Beta Aquarii probably has an extragalactic origin. This star belongs to a group of three intermediate mass stars with a space velocity that is carrying them perpendicular to the plane of the galaxy. The other members of this grouping are Alpha Aquarii and Eta Pegasi.\r\rSadalsuud, when translated, means the \u0022Luckiest of the Lucky\u0022 or the \u0022luck of lucks\u0022. In the context of older worldviews (i.e.Egyptian, Persian and Islamic mythology), Sadalsuud relates to the rising of the Sun when winter has passed (March) and the season of gentle, continuous rain has begun. Hence the myth of \u0022luck\u0022 or \u0022good fortune\u0022 was seen as closely aligned with the essence of spring itself, the burgeoning of new life, and by extension agriculture, which in all societies is the very foundation of prosperity or \u0022good fortune\u0022. This mythological view of \u0022the luck of the lucks\u0022 also belongs to the 22d Manzil (Arabic Lunar Mansion), which included the two stars Bunda (\u03BE Aqr) and c Cap.\r\r\u03B2 and \u03BE Aquarii also constitute the Persian lunar mansion Bunda and the similar Coptic mansion Upuineuti, the meaning of which is \u0022the Foundation\u0022.\r\rIn Chinese mythology, \u03B2 Aqr alone marks the sieu (Chinese Lunar Mansion) Heu, Hiu, or H\u00FC, \u0022the Void\u0022, anciently Ko, the central one of the seven sieu which, taken together, were known as Heung Wu, the Black Warrior, in the northern quarter of the sky. As such, Sadalsuud is an expression of the feminine archetype, the Yin or \u0022Void\u0022 (Cosmic Mother), from which, many cultures have believed, creation itself (birth) emanates.\r\rIn Chinese, \u865A\u5BBF (X\u016B S\u00F9), meaning Emptiness (asterism), refers to an asterism consisting of \u03B2 Aquarii and \u03B1 Equulei. Consequently, \u03B2 Aquarii itself is known as \u865B\u5BBF\u4E00 (X\u016B S\u00F9 y\u012B, English: the First Star of Emptiness.)\r\rSadalsuud is found in Hindu texts as Kalpeny and in the context of the ancient Indian system of astronomy, Jyotisha Veda, is located in the 23rd Nakshatra Shravishth\u0101, a lunar mansion which is ruled by Eight vasus - the \u0022deities of earthly abundance\u0022 . On the Euphrates, Sadalsuud was known as Kakkab Namma\u03C7, the Star of Mighty Destiny; that may have given origin to the title of the manzil, as well as to the astrologers\u0027 name for it \u2014 Fortuna Fortunarum.\r\r\u0022Sadalsuud\u0022 appears to be a single star to the naked eye, but when viewed with a telescope is seen to have two faint optical companions. The first has an apparent magnitude of 11.0. In 1947, the position angle was observed at 321 degrees with a separation from the Beta Aquarii of 35.4 arcseconds. The second star has a magnitude of 11.6. Its position angle is 186 degrees with a separation from Beta Aquarii of 57.2 arcseconds. As of 2008, there is no definitive evidence that the three stars form a ternary star system.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "22 Aquarii, Beta Aquarii, HIP 106278, SAO 145457, HD 204867, GC 30137, HR 8232, DM BD-06  5770, TYC 5216-1725-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sadalsuud",
	"OType" : "Star",
	"Distance" : "164.49",
	"RA_S" : 322.88971548,
	"DEC_S" : -5.57117555,
	"X" : 490,
	"Y" : 224,
	"Constellation" : "Aquarius ",
	"AMag" : 2.958,
	"key" : 54992,
	"shortTitle" : "Sadalsud; Sad es Saud; Sadalsund; Saad el Sund; Sad Ehl'zul",
	"title" : "Sadalsuud"
	},
{
	"Index" : "39241",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "23 Aquarii, Xi Aquarii, HIP 106786, SAO 145537, HD 205767, GC 30268, HR 8264, DM BD-08  5701, TYC 5787-1291-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Xi Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "54.75",
	"RA_S" : 324.43795747,
	"DEC_S" : -7.85420249,
	"Constellation" : "Aquarius ",
	"AMag" : 4.7,
	"key" : 59241,
	"title" : "Xi Aquarii"
	},
{
	"Index" : "37291",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "25 Aquarii, d Aquarii, HIP 106944, SAO 126965, HD 206067, GC 30315, HR 8277, DM BD+01  4517, TYC 547-1047-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "d Aquarii",
	"OType" : "Star",
	"Distance" : "69.41",
	"RA_S" : 324.88861107,
	"DEC_S" : 2.24355816,
	"Constellation" : "Aquarius ",
	"AMag" : 5.215,
	"key" : 57291,
	"title" : "d Aquarii"
	},
{
	"Index" : "35041",
	"Description" : "Omicron Aquarii (\u03BF Aqr, \u03BF Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It has the traditional star name Kae Uh, from the Chinese \u84CB\u5C4B (Mandarin g\u00E0iw\u016B) \u0022the roof\u0022. Visible to the naked eye, it has an apparent visual magnitude of +4.71. Parallax measurements put it at a distance of roughly 440 light-years (130 parsecs) from Earth.\r\rIn Chinese, \u84CB\u5C4B (G\u00E0i W\u016B), meaning Roofing, refers to an asterism consisting of \u03BF Aquarii and 32 Aquarii. Consequently, \u03BF Aquarii itself is known as \u84CB\u5C4B\u4E00 (G\u00E0i W\u016B y\u012B, English: the First Star of Roofing.)\r\rThe spectrum of Omicron Aquarii fits a stellar classification of B7 IVe; the luminosity class of IV suggests that this is a subgiant star that is exhausting the supply of hydrogen at its core and is in the process of evolving into a giant star. The \u0027e\u0027 suffix on the class indicates that the spectrum shows emission lines of hydrogen, thus categorizing this as a Be star. Omicron Aquarii is rotating rapidly with a projected rotational velocity of 205 km/s. The rotation rate along the equator may be as high as 77% of the critical rotation velocity, with the axis of rotation being inclined by around 70\u00B0 \u00B1 20\u00B0. The emission lines are being generated by a decreted circumstellar disk of hot hydrogen gas.\r\rIt is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.68 to +4.89.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "31 Aquarii, Omicron Aquarii, HIP 108874, SAO 145837, HD 209409, GC 30844, HR 8402, DM BD-02  5681, TYC 5224-1808-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Kae Uh",
	"OType" : "Be Star",
	"Distance" : "133.36",
	"RA_S" : 330.82851441,
	"DEC_S" : -2.15536379,
	"X" : 388,
	"Y" : 178,
	"Constellation" : "Aquarius ",
	"AMag" : 4.765,
	"key" : 55041,
	"title" : "Kae Uh"
	},
{
	"Index" : "35040",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "32 Aquarii, HIP 108991, SAO 145853, HD 209625, GC 30872, HR 8410, DM BD-01  4242, TYC 5224-1807-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "32 Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "68.09",
	"RA_S" : 331.197594,
	"DEC_S" : -0.90634365,
	"Constellation" : "Aquarius ",
	"AMag" : 5.303,
	"key" : 55040,
	"title" : "32 Aquarii"
	},
{
	"Index" : "35039",
	"Description" : "Alpha Aquarii (Alpha Aqr, \u03B1 Aquarii, \u03B1 Aqr) is a single star in the Aquarius. It has the traditional name Sadalmelik, which is derived from Arabic for \u0022Luck of the king\u0022. The apparent visual magnitude of 2.94 makes this the second-brightest star in Aquarius. Based upon parallax measurements made during the Hipparcos mission, this star is located at a distance of roughly 520 light-years (160 parsecs) from Earth.\r\rWith an age of 53 million years, this star has evolved into a supergiant with a stellar classification of G2 Ib. It has 6.5 as much mass as the Sun and has expanded to around 77 times the Sun\u0027s radius. It is radiating 3,000 times as much luminosity as the Sun from its outer atmosphere at an effective temperature of 5,210 K. At this heat, the star glows with the yellow hue of a G-type star. Examination of this star with the Chandra X-ray Observatory shows it to be significantly X-ray deficient compared to G-type main sequence stars. This deficit is a common feature of early G-type giant stars.\r\rSadalmelik has a visual companion, designated CCDM J22058-0019B, with an apparent visual magnitude of approximately 12.2. It is at an angular separation of 110.4 arcseconds from Sadalmelik along a position angle of 40\u00B0.\r\rThe name Sadalmelik derives from an Arabic expression \u0633\u0639\u062F \u0627\u0644\u0645\u0644\u0643 sa\u0027d al-malik meaning \u0022Luck of the king\u0022. Ulug Beg was combined the name with \u03BF Aqr. The name Rucbah has also been applied to this star; it shares this name with Delta Cassiopeiae. It is only one of two stars with ancient proper names to lie within a degree of the celestial equator. The origin of the Arabic name is lost to history.\r\rIn Chinese, \u5371\u5BBF (W\u0113i S\u00F9), meaning Rooftop (asterism), refers to an asterism consisting of \u03B1 Aquarii, \u03B8 Pegasi and \u03B5 Pegasi. Consequently, \u03B1 Aquarii itself is known as \u5371\u5BBF\u4E00 (W\u0113i S\u00F9 y\u012B, English: the First Star of Rooftop.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "34 Aquarii, Alpha Aquarii, HIP 109074, SAO 145862, HD 209750, GC 30896, HR 8414, DM BD-01  4246, TYC 5224-1806-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sadalmelik",
	"OType" : "Star",
	"Distance" : "160.33",
	"RA_S" : 331.44598271,
	"X" : 380,
	"Y" : 154,
	"Constellation" : "Aquarius ",
	"AMag" : 3.033,
	"key" : 55039,
	"shortTitle" : "Sadalmelek; Sadlamulk; El Melik; Saad el Melik; Sadal'melik; Sadal'melek",
	"title" : "Sadalmelik"
	},
{
	"Index" : "39374",
	"Description" : "Iota Aquarii (\u03B9 Aqr, \u03B9 Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent magnitude of +4.279. based upon parallax measurements made during the Hipparcos mission, the distance to this star is around 175 light-years (54 parsecs).\r\rThe spectrum of this star fits a stellar classification of B8 V, showing that this is a B-type main sequence star. It has 2.7 times the radius of the Sun and is spinning rapidly with a projected rotational velocity of 135 km/s. A 2010 infrared search for companions around this star was unsuccessful.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "33 Aquarii, Iota Aquarii, HIP 109139, SAO 164861, HD 209819, GC 30914, HR 8418, DM BD-14  6209, TYC 5808-1683-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Iota Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "53.7",
	"RA_S" : 331.60928776,
	"DEC_S" : -13.86968033,
	"X" : 376,
	"Y" : 330,
	"Constellation" : "Aquarius ",
	"AMag" : 4.261,
	"key" : 59374,
	"title" : "Iota Aquarii"
	},
{
	"Index" : "39358",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "38 Aquarii, e Aquarii, HIP 109472, SAO 164910, HD 210424, GC 31021, HR 8452, DM BD-12  6196, TYC 5806-1866-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "e Aquarii",
	"OType" : "Star",
	"Distance" : "137.59",
	"RA_S" : 332.65617755,
	"DEC_S" : -11.56493989,
	"Constellation" : "Aquarius ",
	"AMag" : 5.403,
	"key" : 59358,
	"title" : "e Aquarii"
	},
{
	"Index" : "39385",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "42 Aquarii, HIP 110000, SAO 164974, HD 211361, GC 31150, HR 8496, DM BD-13  6148, TYC 5809-1804-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "42 Aquarii",
	"OType" : "Star",
	"Distance" : "179.19",
	"RA_S" : 334.20018518,
	"DEC_S" : -12.83143396,
	"Constellation" : "Aquarius ",
	"AMag" : 5.459,
	"key" : 59385,
	"title" : "42 Aquarii"
	},
{
	"Index" : "39337",
	"Description" : "Theta Aquarii (\u03B8 Aqr, \u03B8 Aquarii) is the bayer designation for a star in the equatorial constellation of Aquarius. It has the traditional name Ancha; Medieval Latin for \u0022the haunch\u0022. Visible to the naked eye at apparent magnitude 4.175, it is located at a distance of around 187 light-years (57 parsecs) from Earth. Since it is near the ecliptic it can be occulted by the Moon, or very rarely by planets.\r\rIn Chinese, \u6CE3 (Q\u00EC), meaning Weeping, refers to an asterism consisting of \u03B8 Aquarii and \u03C1 Aquarii. Consequently, \u03B8 Aquarii itself is known as \u6CE3\u4E8C (Q\u00EC \u00E8r, English: the Second Star of Weeping.). Possibly, the name Lei meaning tears (weeping) in Chinese, was appear from the Chinese name for this star\r\rAncha belongs to the spectral class G8 with a luminosity class of III\u2013IV suggesting that, at an age of 437 million years, this star is part way between the subgiant and giant stages of its evolution. Estimates of the star\u0027s mass range from 2.39 to 2.78 times the Sun\u0027s mass, with a radius of about 12 times that of the Sun. It is radiating from 72 to 83 times as much luminosity as the Sun from its enlarged outer envelope at an effective temperature of 4,864 K. At this heat, the star glows with the yellow hue of a G-type star.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "43 Aquarii, Theta Aquarii, HIP 110003, SAO 145991, HD 211391, GC 31152, HR 8499, DM BD-08  5845, TYC 5803-1996-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Ancha",
	"OType" : "Star",
	"Distance" : "57.46",
	"RA_S" : 334.20848759,
	"DEC_S" : -7.78328831,
	"X" : 344,
	"Y" : 250,
	"Constellation" : "Aquarius ",
	"AMag" : 4.268,
	"key" : 59337,
	"title" : "Ancha"
	},
{
	"Index" : "39342",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "46 Aquarii, Rho Aquarii, HIP 110273, SAO 146023, HD 211838, GC 31225, HR 8512, DM BD-08  5855, TYC 5804-1742-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Rho Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "266.89",
	"RA_S" : 335.04965428,
	"DEC_S" : -7.821101,
	"Constellation" : "Aquarius ",
	"AMag" : 5.33,
	"key" : 59342,
	"title" : "Rho Aquarii"
	},
{
	"Index" : "43848",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "47 Aquarii, HIP 110391, SAO 191083, HD 212010, GC 31247, HR 8516, DM BD-22  5897, TYC 6384-1571-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "47 Aquarii",
	"OType" : "Red Giant Branch star",
	"Distance" : "52.42",
	"RA_S" : 335.39820168,
	"DEC_S" : -21.59823135,
	"Constellation" : "Aquarius ",
	"AMag" : 5.242,
	"key" : 63848,
	"title" : "47 Aquarii"
	},
{
	"Index" : "35053",
	"Description" : "Gamma Aquarii (\u03B3 Aqr, \u03B3 Aquarii) is the Bayer designation for a star in the constellation Aquarius. It has the traditional name Sadachbia, from an Arabic expression \u0633\u0639\u062F \u0627\u0644\u0623\u062E\u0628\u064A\u0629 sa\u0027d al-\u0027axbiyah \u0022luck of the homes (tents)\u0022 in Hindu system it is also called Sadhabhisk in devnagari, sadhayam in tamil. This star has an apparent visual magnitude of 3.849, making it one of the brighter members of the constellation. Based upon parallax measurements, this star is located at a distance of roughly 164 light-years (50 parsecs) from the Sun, with an error margin of 5%.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Aoul al Achbiya (\u0623\u0648\u0644 \u0623\u0644\u0623\u062C\u0628\u064A\u0629 - awwil al ahbiyah), which was translated into Latin as Prima Tabernaculorum, meaning the first of luck of the homes (tents). This star, along with \u03C0 Aqr (Seat), \u03B6 Aqr (Sadaltager / Achr al Achbiya) and \u03B7 Aqr (Hydria), were al A\u1E23biyah (\u0627\u0644\u0623\u062E\u0628\u064A\u0629), the Tent.<re name=allen1963f/>\r\rIn Chinese, \u58B3\u5893 (F\u00E9n M\u00F9), meaning Tomb, refers to an asterism consisting of \u03B3 Aquarii, \u03B6 Aquarii, \u03B7 Aquarii, \u03C0 Aquarii. Consequently, \u03B3 Aquarii itself is known as \u58B3\u5893\u4E8C (F\u00E9n M\u00F9 \u00E8r, English: the Second Star of Tomb).\r\rGamma Aquarii is an A-type main sequence star with a stellar classification of A0 V, making it both larger and more massive than the Sun. It is a candidate Lambda Bootis star, suggesting it may have accreted low-metallicity circumstellar gas some time in the past. It is spinning relatively rapidly with a projected rotational velocity of 80 km s\u20131. This value gives a lower bound on the actual azimuthal velocity along the star\u0027s equator. The outer atmosphere of Gamma Aquarii is radiating energy at an effective temperature of 10,500 K, which is nearly double the temperature at the surface of the Sun. This heat is what gives Gamma Aquarii the white-hot glow of an A-type star.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "48 Aquarii, Gamma Aquarii, HIP 110395, SAO 146044, HD 212061, GC 31257, HR 8518, DM BD-02  5741, TYC 5226-1606-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sadachbia",
	"OType" : "Star",
	"Distance" : "50.04",
	"RA_S" : 335.41406425,
	"DEC_S" : -1.38733418,
	"X" : 328,
	"Y" : 168,
	"Constellation" : "Aquarius ",
	"AMag" : 3.827,
	"key" : 55053,
	"shortTitle" : "Sadachbia",
	"title" : "Sadachbia"
	},
{
	"Index" : "38202",
	"Description" : "Pi Aquarii (\u03C0 Aqr, \u03C0 Aquarii) is the Bayer designation for a binary star in the equatorial constellation of Aquarius. It shares the traditional name Seat with Delta Aquarii, where it has long been misspelled Skat. It may be from the Arabic word \u0161i\u0027at \u0022a wish\u0022. This system has an apparent visual magnitude of a mean apparent magnitude of +4.57. Based upon parallax measurements, it is located at a distance of roughly 780 light-years (240 parsecs) from Earth.\r\rThis is a binary star system with an orbital period of 84.1 \u00B1 0.004. The primary component is a B-type main sequence star with a stellar classification of B1 Ve. This is a large star with nearly eleven times the mass and over six times the radius of the Sun. Pi Aquarii shines about 7,300 times as brightly as the Sun. This energy is being radiated from its outer atmosphere at an effective temperature of 27,094, giving it the blue-hued glow of a B-type star. It is spinning rapidly with a projected rotational velocity of 215 km/s.\r\rPi Aquarii is notable for having undergone a transition from a Be star (showing hydrogen emission lines) into an ordinary B-type star. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.45 to +4.71; a range of 0.28. The dominant variability period, 83.8 \u00B1 0.8 days, is nearly the same as the orbital period.\r\rIn Chinese, \u58B3\u5893 (F\u00E9n M\u00F9), meaning Tomb, refers to an asterism consisting of \u03C0 Aquarii, \u03B3 Aquarii, \u03B6 Aquarii, \u03B7 Aquarii. Consequently, \u03C0 Aquarii itself is known as \u58B3\u5893\u56DB (F\u00E9n M\u00F9 s\u00EC, English: the Fourth Star of Tomb.)\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Wasat al Achbiya (\u0648\u0633\u0637 \u0623\u0644\u0623\u062C\u0628\u064A\u0629 - wasath al ahbiyah), which was translated into Latin as Media Tabernaculorum, meaning the middle of luck of the homes (tents). This star, along with \u03B3 Aqr (Sadachbia), \u03B6 Aqr (Sadaltager / Achr al Achbiya) and \u03B7 Aqr (Hydria), were al A\u1E23biyah (\u0627\u0644\u0623\u062E\u0628\u064A\u0629), the Tent.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "52 Aquarii, Pi Aquarii, HIP 110672, SAO 127520, HD 212571, GC 31328, HR 8539, DM BD+00  4872, TYC 560-1818-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Seat",
	"OType" : "Be Star",
	"Distance" : "238.52",
	"RA_S" : 336.31926093,
	"DEC_S" : 1.37739729,
	"X" : 316,
	"Y" : 131,
	"Constellation" : "Aquarius ",
	"AMag" : 4.76,
	"key" : 58202,
	"title" : "Seat"
	},
{
	"Index" : "35052",
	"Description" : "Zeta Aquarii (\u03B6 Aqr, \u03B6 Aquarii) is the Bayer designation for a binary, or possibly a triple star system; the central star of the \u0022water jar\u0022 asterism in the equatorial constellation of Aquarius. The combined apparent visual magnitude of this system is 3.65, which is readily visible to the naked eye. Parallax measurements yield a distance estimate of around 92 light-years (28 parsecs) from Earth.\r\rZeta Aquarii has the traditional name Sadaltager (or Altager), from the Arabic \u0633\u0639\u062F \u0627\u0644\u062A\u0627\u062C\u0631 sa\u0027d al-t\u0101jir \u0022luck of the merchant\u0022. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Achr al Achbiya (\u0623\u062C\u0631 \u0623\u0644\u0623\u062C\u0628\u064A\u0629 - akhir al ahbiyah), which was translated into Latin as Postrema Tabernaculorum, meaning the end of luck of the homes (tents). This star, along with \u03B3 Aqr (Sadachbia), \u03C0 Aqr (Seat) and \u03B7 Aqr (Hydria), were al A\u1E23biyah (\u0627\u0644\u0623\u062E\u0628\u064A\u0629), the Tent.\r\rIn Chinese, \u58B3\u5893 (F\u00E9n M\u00F9), meaning Tomb, refers to an asterism consisting of \u03B6 Aquarii, \u03B3 Aquarii, \u03B7 Aquarii and \u03C0 Aquarii. Consequently, \u03B6 Aquarii itself is known as \u58B3\u5893\u4E00 (F\u00E9n M\u00F9 y\u012B, English: the First Star of Tomb.)\r\rChristian Mayer, director of the Mannheim Observatory, is considered the first to have observed Zeta Aquarii to be double, in 1777. A couple of years later, William Herschel also discovered this duality. The two stars have an orbital period of about 587 years. The semimajor axis is 3.8 arcseconds and they have an orbital eccentricity of 0.40. The orbital plane is inclined by 138.2\u00B0 to the line of sight.\r\rThe brighter component, \u03B6 Aquarii A, is a yellow-white-hued F-type main sequence star with an apparent magnitude of +4.42. Its companion, \u03B6 Aquarii B, is a yellow-white-hued F-type subgiant with an apparent magnitude of +4.51. The fact that their brightness is so similar makes the pair easy to measure and resolve.\r\r\u03B6 Aquarii B is a suspected astrometric binary system with a 25.8 year orbital period and a semimajor axis of 10.8 astronomical units. If this is confirmed, then the smaller companion may be a red dwarf with a classification of M0 V and 40% of the Sun\u0027s mass.\r\rZeta Aquarii is currently a northern hemisphere object. In 2004 it was directly above the celestial equator, and before that it was located south of it.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "55 Aquarii, Zeta01 Aquarii, HIP 110960B, SAO 146107, HD 213051, GC 31398, HR 8558, DM BD-00  4365B, TYC 5226-1605-2",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sadaltager",
	"OType" : "Star",
	"Distance" : "28.13",
	"RA_S" : 337.207329,
	"X" : 305,
	"Y" : 150,
	"Constellation" : "Aquarius ",
	"AMag" : 4.492,
	"key" : 55052,
	"title" : "Sadaltager"
	},
{
	"Index" : "35051",
	"Description" : "Zeta Aquarii (\u03B6 Aqr, \u03B6 Aquarii) is the Bayer designation for a binary, or possibly a triple star system; the central star of the \u0022water jar\u0022 asterism in the equatorial constellation of Aquarius. The combined apparent visual magnitude of this system is 3.65, which is readily visible to the naked eye. Parallax measurements yield a distance estimate of around 92 light-years (28 parsecs) from Earth.\r\rZeta Aquarii has the traditional name Sadaltager (or Altager), from the Arabic \u0633\u0639\u062F \u0627\u0644\u062A\u0627\u062C\u0631 sa\u0027d al-t\u0101jir \u0022luck of the merchant\u0022. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Achr al Achbiya (\u0623\u062C\u0631 \u0623\u0644\u0623\u062C\u0628\u064A\u0629 - akhir al ahbiyah), which was translated into Latin as Postrema Tabernaculorum, meaning the end of luck of the homes (tents). This star, along with \u03B3 Aqr (Sadachbia), \u03C0 Aqr (Seat) and \u03B7 Aqr (Hydria), were al A\u1E23biyah (\u0627\u0644\u0623\u062E\u0628\u064A\u0629), the Tent.\r\rIn Chinese, \u58B3\u5893 (F\u00E9n M\u00F9), meaning Tomb, refers to an asterism consisting of \u03B6 Aquarii, \u03B3 Aquarii, \u03B7 Aquarii and \u03C0 Aquarii. Consequently, \u03B6 Aquarii itself is known as \u58B3\u5893\u4E00 (F\u00E9n M\u00F9 y\u012B, English: the First Star of Tomb.)\r\rChristian Mayer, director of the Mannheim Observatory, is considered the first to have observed Zeta Aquarii to be double, in 1777. A couple of years later, William Herschel also discovered this duality. The two stars have an orbital period of about 587 years. The semimajor axis is 3.8 arcseconds and they have an orbital eccentricity of 0.40. The orbital plane is inclined by 138.2\u00B0 to the line of sight.\r\rThe brighter component, \u03B6 Aquarii A, is a yellow-white-hued F-type main sequence star with an apparent magnitude of +4.42. Its companion, \u03B6 Aquarii B, is a yellow-white-hued F-type subgiant with an apparent magnitude of +4.51. The fact that their brightness is so similar makes the pair easy to measure and resolve.\r\r\u03B6 Aquarii B is a suspected astrometric binary system with a 25.8 year orbital period and a semimajor axis of 10.8 astronomical units. If this is confirmed, then the smaller companion may be a red dwarf with a classification of M0 V and 40% of the Sun\u0027s mass.\r\rZeta Aquarii is currently a northern hemisphere object. In 2004 it was directly above the celestial equator, and before that it was located south of it.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "55 Aquarii, Zeta02 Aquarii, HIP 110960A, SAO 146108, HD 213052, GC 31399, HR 8559, DM BD-00  4365A, TYC 5226-1605-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sadaltager",
	"OType" : "Double or multiple star",
	"Distance" : "28.13",
	"RA_S" : 337.207529,
	"X" : 305,
	"Y" : 150,
	"Constellation" : "Aquarius ",
	"AMag" : 4.338,
	"key" : 55051,
	"title" : "Sadaltager"
	},
{
	"Index" : "39432",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "57 Aquarii, Sigma Aquarii, HIP 111123B, SAO 165134, HD 213320, GC 31440, HR 8573, DM BD-11  5850, TYC 5814-1593-2",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sigma Aquarii",
	"OType" : "Star",
	"Distance" : "87.5",
	"RA_S" : 337.6617311,
	"DEC_S" : -10.67795107,
	"Constellation" : "Aquarius ",
	"AMag" : 4.82,
	"key" : 59432,
	"title" : "Sigma Aquarii"
	},
{
	"Index" : "39431",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "57 Aquarii, Sigma Aquarii, HIP 111123A, SAO 165134, HD 213320, GC 31440, HR 8573, DM BD-11  5850, TYC 5814-1593-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Sigma Aquarii",
	"OType" : "Star",
	"Distance" : "87.5",
	"RA_S" : 337.66173198,
	"DEC_S" : -10.67796039,
	"Constellation" : "Aquarius ",
	"AMag" : 4.815,
	"key" : 59431,
	"title" : "Sigma Aquarii"
	},
{
	"Index" : "43901",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "59 Aquarii, Upsilon Aquarii, HIP 111449, SAO 191235, HD 213845, GC 31516, HR 8592, DM BD-21  6251, TYC 6392-1443-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Upsilon Aquarii",
	"OType" : "High proper-motion Star",
	"Distance" : "22.68",
	"RA_S" : 338.67348703,
	"DEC_S" : -20.70821219,
	"Constellation" : "Aquarius ",
	"AMag" : 5.254,
	"key" : 63901,
	"title" : "Upsilon Aquarii"
	},
{
	"Index" : "35110",
	"Description" : "Eta Aquarii (\u03B7 Aqr, \u03B7 Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of 4.04. The distance to this star, as determined by parallax measurements, is about 168 light-years (52 parsecs). Eta Aquarii is near the radiant of a meteor shower named after it.\r\rEta Aquarii has a stellar classification of B9IV-Vn, which may indicate that it is beginning to evolve away from the main sequence into a subgiant as the supply of hydrogen at its core becomes exhausted. It is spinning rapidly with a high projected rotational velocity of 291 km/s. This is causing an equatorial bulge, giving the star an oblate figure with a 24% larger radius at the equator than at the poles. The Doppler effect from the rapid rotation is causing the absorption lines in the star\u0027s spectrum to blur, as indicated by the \u0027n\u0027 suffix in the star\u0027s classification.\r\rThis star sometimes called with the name Hydria, from the Greek word \u0027\u03C5\u03B4\u03C1\u03B9\u03B1 (hudria), meaning \u0022water jar\u0022. Another name of this star is Deli, derived from Hebrew word \u05D3\u05DC\u05D9 (dali) literally meaning \u0022hard\u0022.\r\rThis star, along with \u03B3 Aqr (Sadachbia), \u03C0 Aqr (Seat) and \u03B6 Aqr (Sadaltager / Achr al Achbiya), were al A\u1E23biyah (\u0627\u0644\u0623\u062E\u0628\u064A\u0629), the Tent.\r\rIn Chinese, \u58B3\u5893 (F\u00E9n M\u00F9), meaning Tomb, refers to an asterism consisting of \u03B7 Aquarii, \u03B3 Aquarii, \u03B6 Aquarii, \u03C0 Aquarii. Consequently, \u03B7 Aquarii itself is known as \u58B3\u5893\u4E09 (F\u00E9n M\u00F9 s\u0101n, English: the Third Star of Tomb.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "62 Aquarii, Eta Aquarii, HIP 111497, SAO 146181, HD 213998, GC 31534, HR 8597, DM BD-00  4384, TYC 5233-2298-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Hydria / Deli",
	"OType" : "Star",
	"Distance" : "51.46",
	"RA_S" : 338.838883,
	"X" : 283,
	"Y" : 151,
	"Constellation" : "Aquarius ",
	"AMag" : 4.012,
	"key" : 55110,
	"title" : "Hydria / Deli"
	},
{
	"Index" : "35134",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "63 Aquarii, Kappa Aquarii, HIP 111710, SAO 146210, HD 214376, GC 31581, HR 8610, DM BD-04  5716, TYC 5236-1610-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Situla",
	"OType" : "Star",
	"Distance" : "65.56",
	"RA_S" : 339.43908361,
	"DEC_S" : -4.22805501,
	"Constellation" : "Aquarius ",
	"AMag" : 5.157,
	"key" : 55134,
	"title" : "Situla"
	},
{
	"Index" : "43881",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "66 Aquarii, g Aquarii, HIP 112211, SAO 165252, HD 215167, GC 31708, HR 8649, DM BD-19  6324, TYC 6389-1377-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "g Aquarii",
	"OType" : "Variable Star",
	"Distance" : "132.61",
	"RA_S" : 340.89680448,
	"DEC_S" : -18.83037521,
	"Constellation" : "Aquarius ",
	"AMag" : 4.83,
	"key" : 63881,
	"title" : "g Aquarii"
	},
{
	"Index" : "43885",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "68 Aquarii, HIP 112529, SAO 165293, HD 215721, GC 31794, HR 8670, DM BD-20  6486, TYC 6390-1254-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "68 Aquarii",
	"OType" : "High proper-motion Star",
	"Distance" : "77.8",
	"RA_S" : 341.88801854,
	"DEC_S" : -19.61337688,
	"Constellation" : "Aquarius ",
	"AMag" : 5.345,
	"key" : 63885,
	"title" : "68 Aquarii"
	},
{
	"Index" : "39471",
	"Description" : "Tau2 Aquarii (\u03C42 Aqr, \u03C42 Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of +4.0. This is an orange-hued giant star with a stellar classification of K5 III. The measured angular diameter, after correction for limb darkening, is 5.12 \u00B1 0.05 mas. At an estimated distance of 318 light-years (97 parsecs) based on parallax measurements, this yields a physical size of about 53 times the radius of the Sun.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "71 Aquarii, Tau02 Aquarii, HIP 112716, SAO 165321, HD 216032, GC 31836, HR 8679, DM BD-14  6354, TYC 5819-1247-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Tau2 Aquarii",
	"OType" : "Star",
	"Distance" : "97.28",
	"RA_S" : 342.39792231,
	"DEC_S" : -13.59262957,
	"X" : 240,
	"Y" : 327,
	"Constellation" : "Aquarius ",
	"AMag" : 4.211,
	"key" : 59471,
	"title" : "Tau2 Aquarii"
	},
{
	"Index" : "39424",
	"Description" : "Lambda Aquarii (\u03BB Aqr, \u03BB Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. It has the obscure traditional names Hydor and Ekkhysis, from the ancient Greek \u1F55\u03B4\u03C9\u03C1 \u0022water\u0022 and \u1F14\u03BA\u03C7\u03C5\u03C3\u03B9\u03C2 \u0022outpouring\u0022. The apparent visual magnitude of this star is 3.722, which is bright enough to be visible with the naked eye. It is roughly 390 light-years (120 pc) from Earth.\r\rIn Chinese, \u58D8\u58C1\u9663 (L\u011Bi B\u00EC Zh\u00E8n), meaning Line of Ramparts, refers to an asterism consisting of \u03BB Aquarii, \u03BA Capricorni, \u03B5 Capricorni, \u03B3 Capricorni, \u03B4 Capricorni, \u03B9 Aquarii, \u03C3 Aquarii, \u03C6 Aquarii, 27 Piscium, 29 Piscium, 33 Piscium and 30 Piscium. Consequently, \u03BB Aquarii itself is known as \u58D8\u58C1\u9663\u4E03 (L\u011Bi B\u00EC Zh\u00E8n q\u012B, English: the Seventh Star of Line of Ramparts.)\r\rLambda Aquarii is a red giant star with a stellar classification of M2.5 III. It is a semiregular variable star star with pulsation periods of 24.5, 32.0, and 49.5 days. This star is on the asymptotic giant branch and is generating energy through the nuclear fusion of hydrogen and helium along concentric shells surrounding an inert core of carbon and oxygen.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "73 Aquarii, Lambda Aquarii, HIP 112961, SAO 146362, HD 216386, GC 31903, HR 8698, DM BD-08  5968, TYC 5813-1406-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Hydor / Ekkhysis",
	"OType" : "Long-period variable star",
	"Distance" : "117.21",
	"RA_S" : 343.15364336,
	"DEC_S" : -7.57959838,
	"X" : 228,
	"Y" : 249,
	"Constellation" : "Aquarius ",
	"AMag" : 3.934,
	"key" : 59424,
	"title" : "Hydor / Ekkhysis"
	},
{
	"Index" : "43867",
	"Description" : "Delta Aquarii (\u03B4 Aqr, \u03B4 Aquarii) is the third-brightest star in the constellation Aquarius. It has the traditional name Skat, which has also been used for Beta Pegasi. The apparent visual magnitude is 3.3, which can be seen with the naked eye. The distance to this star is estimated as 160 light-years (49 parsecs) based upon parallax measurements.\r\rThe spectrum of Skat matches a stellar classification of A3 V, indicating this is an A-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. This star has double the Sun\u0027s mass and a radius 2.4 times as large. It is radiating 26 times the luminosity of the Sun from its outer atmosphere at an effective temperature of around 9,000 K. This heat gives it the characteristic white-hued glow of an A-type star. It has a relatively high rate of rotation, with a projected rotational velocity of 81 km s\u22121.\r\rDelta Aquarii has been closely examined for a companion, but none has been discovered. Nor does it display a strong signal of excess infrared emission that might indicate the presence of circumstellar matter. Delta Aquarii is a probable stream star member of the Ursa Major Moving Group, which has an estimated age of 500 million years.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "76 Aquarii, Delta Aquarii, HIP 113136, SAO 165375, HD 216627, GC 31943, HR 8709, DM BD-16  6173, TYC 6387-1382-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Skat",
	"OType" : "Star",
	"Distance" : "48.8",
	"RA_S" : 343.6625563,
	"DEC_S" : -15.82082729,
	"X" : 225,
	"Y" : 356,
	"Constellation" : "Aquarius ",
	"AMag" : 3.258,
	"key" : 63867,
	"shortTitle" : "Scheat; Sheat (see HD217906)",
	"title" : "Skat"
	},
{
	"Index" : "39477",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "83 Aquarii, h Aquarii, HIP 113996AB, SAO 146498, HD 218060, GC 32153, HR 8782, DM BD-08  6018, TYC 5820-1291-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "h Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "64.11",
	"RA_S" : 346.29078873,
	"DEC_S" : -7.69379531,
	"Constellation" : "Aquarius ",
	"AMag" : 5.472,
	"key" : 59477,
	"title" : "h Aquarii"
	},
{
	"Index" : "48248",
	"Description" : "86 Aquarii is the Flamsteed designation for a binary star system in the equatorial constellation of Aquarius. It is faint but visible to the naked eye with an apparent visual magnitude of +4.47. Based upon parallax measurements, the distance to this star is about 220 light-years (67 parsecs).\r\rThe two components of this system have an angular separation of 0.25 arcseconds. The brighter component is a giant star with a spectral classification of G8 III and an apparent magnitude of 4.79. The effective temperature of its outer atmosphere is 4,900 K, giving it the yellowish glow of a G-type star. The fainter component is a star of magnitude 6.77.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "86 Aquarii, c01 Aquarii, HIP 114119AC, SAO 191651, HD 218240, GC 32182, HR 8789, DM CD-24 17497, TYC 6972-1268-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "86 Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "66.13",
	"RA_S" : 346.67018679,
	"DEC_S" : -23.74312068,
	"X" : 193,
	"Y" : 461,
	"Constellation" : "Aquarius ",
	"AMag" : 4.584,
	"key" : 68248,
	"title" : "86 Aquarii"
	},
{
	"Index" : "43961",
	"Description" : "88 Aquarii is the Flamsteed designation for a star in the equatorial constellation of Aquarius. The Bayer designation of this star is c2 Aquarii. In dark conditions it is visible to the naked eye with an apparent visual magnitude of +3.68. Based upon parallax measurements, this star is at a distance of around 271 light-years (83 parsecs) from Earth.\r\rThe spectrum of 88 Aquarii matches an evolved giant star with a classification of K1 III. Its measured angular diameter is 3.24 \u00B1 0.20 mas, which, at the estimated distance of Delta Ophiuchi, yields a physical size of about 29 times the radius of the Sun. The cool, orange hued glow of this star comes from the outer atmosphere\u0027s effective temperature of 4,430 K.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "88 Aquarii, c02 Aquarii, HIP 114341, SAO 191683, HD 218594, GC 32246, HR 8812, DM BD-21  6368, TYC 6401-1355-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "88 Aquarii",
	"OType" : "Star",
	"Distance" : "82.95",
	"RA_S" : 347.36165339,
	"DEC_S" : -21.17241145,
	"X" : 183,
	"Y" : 428,
	"Constellation" : "Aquarius ",
	"AMag" : 3.807,
	"key" : 63961,
	"title" : "88 Aquarii"
	},
{
	"Index" : "43962",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "89 Aquarii, c03 Aquarii, HIP 114375AS, SAO 191687, HD 218640, GC 32262, HR 8817, DM CD-23 17771A, TYC 6401-1356-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "c03 Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "152.54",
	"RA_S" : 347.47873454,
	"DEC_S" : -22.45762372,
	"Constellation" : "Aquarius ",
	"AMag" : 4.802,
	"key" : 63962,
	"title" : "c03 Aquarii"
	},
{
	"Index" : "35232",
	"Description" : "Phi Aquarii (\u03C6 Aqr, \u03C6 Aquarii) is the Bayer designation for a binary star system in the equatorial constellation of Aquarius. It is visible to the naked eye with an apparent visual magnitude of +4.223. Parallax measurements from the Hipparcos mission indicate its estimated distance from Earth is roughly 220 light-years (67 parsecs).\r\rThis is a spectroscopic binary star system with an estimated period of 2,500 days. The primary component is a red giant star with a stellar classification of M1.5 III. The outer envelope of this evolved star has expanded to 39 times the size of the Sun. It is radiating 324 times the luminosity of the Sun at an effective temperature of 3,899 K, giving it the reddish hue of an M-type star.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "90 Aquarii, Phi Aquarii, HIP 114724, SAO 146585, HD 219215, GC 32346, HR 8834, DM BD-06  6170, TYC 5249-1400-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Phi Aquarii",
	"OType" : "Star",
	"Distance" : "61.73",
	"RA_S" : 348.58064419,
	"DEC_S" : -6.04900112,
	"X" : 158,
	"Y" : 231,
	"Constellation" : "Aquarius ",
	"AMag" : 4.406,
	"key" : 55232,
	"title" : "Phi Aquarii"
	},
{
	"Index" : "39490",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "91 Aquarii, Psi01 Aquarii, HIP 114855, SAO 146598, HD 219449, GC 32374, HR 8841, DM BD-09  6156, TYC 5821-1480-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Psi01 Aquarii",
	"OType" : "Star",
	"Distance" : "45.92",
	"RA_S" : 348.97289906,
	"DEC_S" : -9.08773573,
	"Constellation" : "Aquarius ",
	"AMag" : 4.363,
	"key" : 59490,
	"title" : "Psi01 Aquarii"
	},
{
	"Index" : "39488",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "92 Aquarii, Chi Aquarii, HIP 114939, SAO 146612, HD 219576, GC 32401, HR 8850, DM BD-08  6076, TYC 5821-1478-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Chi Aquarii",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "186.89",
	"RA_S" : 349.21224665,
	"DEC_S" : -7.72650053,
	"Constellation" : "Aquarius ",
	"AMag" : 5.169,
	"key" : 59488,
	"title" : "Chi Aquarii"
	},
{
	"Index" : "39491",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "93 Aquarii, Psi02 Aquarii, HIP 115033, SAO 146620, HD 219688, GC 32429, HR 8858, DM BD-09  6160, TYC 5821-1481-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Psi02 Aquarii",
	"OType" : "Be Star",
	"Distance" : "122.83",
	"RA_S" : 349.47589051,
	"DEC_S" : -9.18251876,
	"Constellation" : "Aquarius ",
	"AMag" : 4.373,
	"key" : 59491,
	"title" : "Psi02 Aquarii"
	},
{
	"Index" : "39492",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "95 Aquarii, Psi03 Aquarii, HIP 115115, SAO 146635, HD 219832, GC 32459, HR 8865, DM BD-10  6094, TYC 5821-1482-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Psi03 Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "80.08",
	"RA_S" : 349.74032678,
	"DEC_S" : -9.610743,
	"Constellation" : "Aquarius ",
	"AMag" : 4.999,
	"key" : 59492,
	"title" : "Psi03 Aquarii"
	},
{
	"Index" : "39545",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "94 Aquarii, HIP 115126, SAO 165625, HD 219834A, GC 32462, HR 8866, DM BD-14  6448, TYC 5827-1271-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "94 Aquarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "21.05",
	"RA_S" : 349.77778779,
	"DEC_S" : -13.45855619,
	"Constellation" : "Aquarius ",
	"AMag" : 5.2,
	"key" : 59545,
	"title" : "94 Aquarii"
	},
{
	"Index" : "43926",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "97 Aquarii, HIP 115404AB, SAO 165658, HD 220278, GC 32531, HR 8890, DM BD-15  6406, TYC 6396-1219-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "97 Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "65.15",
	"RA_S" : 350.6631803,
	"DEC_S" : -15.03934818,
	"Constellation" : "Aquarius ",
	"AMag" : 5.22,
	"key" : 63926,
	"title" : "97 Aquarii"
	},
{
	"Index" : "43966",
	"Description" : "98 Aquarii is the Flamsteed designation for a star in the equatorial constellation Aquarius. The Bayer designation for this star is b1 Aquarii. It is visible to the naked eye with an apparent visual magnitude of +3.97. The distance to this star, 163 light-years (50 parsecs), is known from parallax measurements made with the Hipparcos spacecraft.\r\rWith over double the mass of the Sun, this is an evolved giant star that has a stellar classification of K0 III. The measured angular diameter of this star is 2.54 \u00B1 0.13 mas. At the estimated distance of 98 Aquarii, this yields a physical size of about 14 times the radius of the Sun. The expanded outer envelope has an effective temperature of 4,630 K, giving it the orange glow of a K-type star.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "98 Aquarii, b01 Aquarii, HIP 115438, SAO 191858, HD 220321, GC 32540, HR 8892, DM BD-20  6587, TYC 6402-1221-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "98 Aquarii",
	"OType" : "Star",
	"Distance" : "50.09",
	"RA_S" : 350.74260858,
	"DEC_S" : -20.10058231,
	"X" : 140,
	"Y" : 417,
	"Constellation" : "Aquarius ",
	"AMag" : 4.072,
	"key" : 63966,
	"title" : "98 Aquarii"
	},
{
	"Index" : "43968",
	"Description" : "99 Aquarii is the Flamsteed designation for a star in the equatorial constellation of Aquarius. The Bayer designation for this star is b2 Aquarii. It is visible to the naked eye with an apparent visual magnitude of 4.37; according to the Bortle Dark-Sky Scale this is bright enough to be seen even from city skies under ideal viewing conditions. Based upon parallax measurements, the distance to this star is around 283 light-years (87 parsecs).\r\rThis is a giant star with a stellar classification of K4 III. It is a suspected variable star that apparently ranges in magnitude between 4.35 and 4.45. The measured angular diameter of this star is 3.55 \u00B1 0.21 mas. At the estimated distance of Delta Ophiuchi, this yields a physical size of about 33 times the radius of the Sun. The outer atmosphere has an effective temperature of 3980 K, giving it the orange-hued glow of a cool, K-type star.\r\rThis star was a candidate member of the Ursa Major Moving Group based on the work of American astronomer Nancy Roman, but this membership is now in question.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "99 Aquarii, b02 Aquarii, HIP 115669, SAO 191900, HD 220704, GC 32594, HR 8906, DM BD-21  6420, TYC 6402-1223-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "99 Aquarii",
	"OType" : "Variable Star",
	"Distance" : "86.85",
	"RA_S" : 351.5116076,
	"DEC_S" : -20.64201578,
	"X" : 132,
	"Y" : 425,
	"Constellation" : "Aquarius ",
	"AMag" : 4.538,
	"key" : 63968,
	"title" : "99 Aquarii"
	},
{
	"Index" : "44016",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "101 Aquarii, b03 Aquarii, HIP 116247A, SAO 191988, HD 221565, GC 32750, HR 8939, DM BD-21  6437, TYC 6409-1232-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "b03 Aquarii",
	"OType" : "Double or multiple star",
	"Distance" : "89.62",
	"RA_S" : 353.3192625,
	"DEC_S" : -20.9145043,
	"Constellation" : "Aquarius ",
	"AMag" : 4.759,
	"key" : 64016,
	"title" : "b03 Aquarii"
	},
{
	"Index" : "39618",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "102 Aquarii, Omega01 Aquarii, HIP 116758, SAO 165818, HD 222345, GC 32873, HR 8968, DM BD-15  6471, TYC 5836-978-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Omega01 Aquarii",
	"OType" : "Star",
	"Distance" : "43.48",
	"RA_S" : 354.94611541,
	"DEC_S" : -14.22216917,
	"Constellation" : "Aquarius ",
	"AMag" : 5.008,
	"key" : 59618,
	"title" : "Omega01 Aquarii"
	},
{
	"Index" : "43994",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "104 Aquarii, A02 Aquarii, HIP 116901, SAO 165836, HD 222574, GC 32911, HR 8982, DM BD-18  6358, TYC 6407-1131-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "A02 Aquarii",
	"OType" : "Star",
	"Distance" : "255.8",
	"RA_S" : 355.44086029,
	"DEC_S" : -17.81653484,
	"Constellation" : "Aquarius ",
	"AMag" : 4.906,
	"key" : 63994,
	"title" : "A02 Aquarii"
	},
{
	"Index" : "43987",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "HIP 116957, SAO 165841, HD 222643, GC 32925, HR 8987, DM BD-16 6345, TYC 6404-993-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "HR 8987",
	"OType" : "Star",
	"Distance" : "82.68",
	"RA_S" : 355.61592592,
	"DEC_S" : -15.44802909,
	"Constellation" : "Aquarius ",
	"AMag" : 5.412,
	"key" : 63987,
	"title" : "HR 8987"
	},
{
	"Index" : "39619",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "105 Aquarii, Omega02 Aquarii, HIP 116971, SAO 165842, HD 222661, GC 32931, HR 8988, DM BD-15  6476, TYC 5836-979-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "Omega02 Aquarii",
	"OType" : "Star",
	"Distance" : "45.53",
	"RA_S" : 355.68060248,
	"DEC_S" : -14.54490451,
	"Constellation" : "Aquarius ",
	"AMag" : 4.478,
	"key" : 59619,
	"title" : "Omega02 Aquarii"
	},
{
	"Index" : "43996",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "106 Aquarii, i01 Aquarii, HIP 117089, SAO 165854, HD 222847, GC 32958, HR 8998, DM BD-19  6500, TYC 6407-1133-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "i01 Aquarii",
	"OType" : "Star",
	"Distance" : "115.6",
	"RA_S" : 356.05032887,
	"DEC_S" : -18.27693578,
	"Constellation" : "Aquarius ",
	"AMag" : 5.225,
	"key" : 63996,
	"title" : "i01 Aquarii"
	},
{
	"Index" : "44005",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "108 Aquarii, i03 Aquarii, HIP 117629, SAO 165918, HD 223640, GC 33092, HR 9031, DM BD-19  6522, TYC 6408-1356-1",
	"group" : { "key" : "Aquarius" },
	"Common" : "i03 Aquarii",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "97.64",
	"RA_S" : 357.83890967,
	"DEC_S" : -18.90916493,
	"Constellation" : "Aquarius ",
	"AMag" : 5.159,
	"key" : 64005,
	"title" : "i03 Aquarii"
	},
{
	"Index" : "29739",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "4 Aquilae, HIP 91975, SAO 123879, HD 173370, GC 25652, HR 7040, DM BD+01  3766, TYC 451-1386-1",
	"group" : { "backgroundImage" : "images/Alignment/04.png",
		"description" : "Aquila is a constellation in the northern sky. Its name is Latin for \u0027eagle\u0027 and it represents the bird who carried Zeus\u0027s/Jupiter\u0027s thunderbolts in Greco-Roman mythology.\r\rAquila lies just a few degrees North of the celestial equator. The alpha star, Altair, is a vertex of the Summer Triangle asterism. The constellation is best seen in the summer as it is located along the Milky Way. Because of this location along the line of our galaxy, many clusters and nebulae are found within its borders, but they are dim and there are few galaxies.\r\rAquila was one of the 48 constellations described by the 2nd century astronomer Ptolemy. It had been earlier mentioned by Eudoxus in the 4th century BC and Aratus in the 3rd century BC. It is now one of the 88 constellations defined by the International Astronomical Union. The constellation was also known as Vultur volans (the flying vulture) to the Romans, not to be confused with Vultur cadens which was their name for Lyra. It is often held to represent the eagle who held Zeus\u0027s/Jupiter\u0027s thunderbolts in Greco-Roman mythology. Aquila is also associated with the eagle who kidnapped Ganymede (associated with Aquarius) to serve as cup-bearer to the gods.\r\rPtolemy catalogued nineteen stars jointly in this constellation and in the now obsolete constellation of Antinous, which was named in the reign of the emperor Hadrian (AD 117\u2013138), but sometimes erroneously attributed to Tycho Brahe, who catalogued twelve stars in Aquila and seven in Antinous. Hevelius determined twenty-three stars in the first and nineteen in the second.\r\rThe Greek Aquila is probably based on the Babylonian constellation of the Eagle (MUL.A.MUSHEN), which is located in the same area as the Greek constellation.",
		"key" : "Aquila",
		"grouptype" : "Aquila",
		"Meaning" : "eagle",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Aquila",
		"title" : "Aquila Objects Group" },
	"Common" : "4 Aquilae",
	"OType" : "Be Star",
	"Distance" : "142.47",
	"RA_S" : 281.20807377,
	"DEC_S" : 2.06003941,
	"Constellation" : "Aquila ",
	"AMag" : 4.996,
	"key" : 49739,
	"title" : "4 Aquilae"
	},
{
	"Index" : "4869",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "FF Aquilae, HIP 93124, SAO 104296, HD 176155A, GC 26052, HR 7165, DM BD+17  3799, TYC 1589-2551-1",
	"group" : { "key" : "Aquila" },
	"Common" : "FF Aquilae",
	"OType" : "Spectroscopic binary",
	"Distance" : "460.42",
	"RA_S" : 284.56144792,
	"DEC_S" : 17.36091616,
	"Constellation" : "Aquila ",
	"AMag" : 5.435,
	"key" : 24869,
	"title" : "FF Aquilae"
	},
{
	"Index" : "431",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "11 Aquilae, HIP 93203, SAO 104308, HD 176303, GC 26075, HR 7172, DM BD+13  3841, TYC 1051-2478-1",
	"group" : { "key" : "Aquila" },
	"Common" : "11 Aquilae",
	"OType" : "Variable Star",
	"Distance" : "48.42",
	"RA_S" : 284.77391329,
	"DEC_S" : 13.62224432,
	"Constellation" : "Aquila ",
	"AMag" : 5.32,
	"key" : 20431,
	"title" : "11 Aquilae"
	},
{
	"Index" : "4828",
	"Description" : "Epsilon Aquilae (\u03B5 Aql, \u03B5 Aquilae) is the Bayer designation for a binary star in the equatorial constellation of Aquila. It has an apparent visual magnitude of 4.02 and is visible to the naked eye. Based upon an annual parallax of 21.05 mas, Epsilon Aquilae lies at a distance of approximately 155 light-years (48 parsecs) from Earth. This is a spectroscopic binary system. The pair orbit each other over a period of 1,271 days (3.5 years) with an eccentricity of 0.27.\r\rIt has the traditional name Deneb el Okab, from an Arabic term \u0630\u0646\u0628 \u0627\u0644\u0639\u0642\u0627\u0628 \u00F0anab al-cuq\u0101b meaning \u0022the tail of the eagle\u0022, and the Mandarin names Woo and Yu\u00EB, derived from and represent the state Wu (\u5433), an old state was located at the mouth of the Yangtze River, and Yue (\u8D8A), an old state in Zhejiang province (together with 19 Capricorni in Twelve States asterism). According to the R.H. Allen\u0027s works, it shares names with \u03B6 Aquilae. Epsilon Aquilae is more precisely called Deneb el Okab Borealis, because is situated to the north of Zeta Aquilae, which can therefore be called Deneb el Okab Australis.\r\rThe primary component of this system is an evolved giant star with a stellar classification of K1 III. It has more than double the mass of the Sun and has expanded to ten times the Sun\u0027s radius. It shines with 54\u2013fold the Sun\u0027s luminosity, which is being radiated from its outer envelope at an effective temperature of 4,760 K. At this heat, it glows with the orange-hue of a K-type star. This has been designated a barium star, meaning its atmosphere is extremely enriched with barium and other heavy elements. However, this is disputed, with astronomer Andrew McWilliam (1990) finding normal abundances from an s-process.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "13 Aquilae, Epsilon Aquilae, HIP 93244, SAO 104318, HD 176411, GC 26091, HR 7176, DM BD+14  3736, TYC 1585-2531-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Deneb el Okab Borealis",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.44",
	"RA_S" : 284.90565846,
	"DEC_S" : 15.0682972,
	"X" : 537,
	"Y" : 172,
	"Constellation" : "Aquila ",
	"AMag" : 4.129,
	"key" : 24828,
	"shortTitle" : "Deneb (see HD177724)",
	"title" : "Deneb el Okab Borealis"
	},
{
	"Index" : "34514",
	"Description" : "12 Aquilae (12 Aql) is the Flamsteed designation for a star in the equatorial constellation of Aquila. It has the Bayer designation i Aquilae (i Aql). Sometimes, this star is called by the name Bered, derived the Hebrew word \u05D1\u05B8\u05BC\u05E8\u05B8\u05D3 barad, meaning \u0022storm\u0022. In Chinese, \u5929\u5F01 (Ti\u0101n Bi\u00E0n), meaning Market Officer, refers to an asterism consisting of 12 Aquilae, \u03B1 Scuti, \u03B4 Scuti, \u03B5 Scuti, \u03B2 Scuti, \u03B7 Scuti, \u03BB Aquilae, 15 Aquilae and 14 Aquilae. Consequently, 12 Aquilae itself is known as \u5929\u5F01\u516D (Ti\u0101n Bi\u00E0n li\u00F9, English: the Sixth Star of Market Officer.)\r\rThis star has an apparent visual magnitude of 4.02, which is bright enough to be seen with the naked eye, although, according to the Bortle Dark-Sky Scale, it is a challenge to view from the inner city. Based upon an annual parallax shift of 22.66 mas, the distance to this star is 144 light-years (44 parsecs) with a margin of error of one light-year. This is an evolved giant star of stellar class K1 III. It has 12 times the radius of the Sun and shines with 60 times the Sun\u0027s luminosity. This energy is being radiated from its outer atmosphere at an effective temperature of 4,603 K, giving it the cool orange hue of a K-type star.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "12 Aquilae, i Aquilae, HIP 93429, SAO 142931, HD 176678, GC 26141, HR 7193, DM BD-05  4840, TYC 5140-4781-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Bered",
	"OType" : "Variable Star",
	"Distance" : "44.13",
	"RA_S" : 285.42011418,
	"DEC_S" : -5.73911695,
	"X" : 532,
	"Y" : 443,
	"Constellation" : "Aquila ",
	"AMag" : 4.131,
	"key" : 54514,
	"title" : "Bered"
	},
{
	"Index" : "34463",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "14 Aquilae, g Aquilae, HIP 93526, SAO 142959, HD 176984, GC 26190, HR 7209, DM BD-03  4460, TYC 5132-1657-1",
	"group" : { "key" : "Aquila" },
	"Common" : "g Aquilae",
	"OType" : "Star",
	"Distance" : "152.73",
	"RA_S" : 285.72708617,
	"DEC_S" : -3.69898972,
	"Constellation" : "Aquila ",
	"AMag" : 5.396,
	"key" : 54463,
	"title" : "g Aquilae"
	},
{
	"Index" : "444",
	"Description" : "Zeta Aquilae (\u03B6 Aql, \u03B6 Aquilae) is a double star in the equatorial constellation of Aquila. It has the traditional name Deneb el Okab, meaning \u0022the tail of the falcon\u0022. As a third magnitude star, Zeta Aquilae is readily visible with the naked eye. Parallax measurements place it at a distance of approximately 83 light-years (25 parsecs) from Earth.\r\rZeta Aquilae has a stellar classification of A0 Vn, with the luminosity class \u0027V\u0027 indicating is a main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. It has more than double the mass and twice the radius of the Sun, and is radiating more than 39 times the Sun\u0027s luminosity. The effective temperature of the star\u0027s outer envelope is about 9620 K, which gives it the white hue typical of A-type stars. The estimated age of this star is 50\u2013150 million years.\r\rThis star is rotating rapidly, with a projected rotational velocity of 317 km s\u22121 giving a lower bound on the azimuthal velocity along the equator. As a result, it has a pronounced equatorial bulge, causing the star to assume an oblate spheroidal shape. The equatorial radius is about 30.7% greater than the polar radius. Because of the Doppler effect, this rapid rotation makes the absorption lines in the star\u0027s spectrum broaden and smear out, as indicated by the \u0027n\u0027 suffix in the stellar class.\r\rAstronomers use Zeta Aquilae as a telluric standard star. That is, the spectrum of this star is used to correct for telluric contamination from the Earth\u0027s atmosphere when examining the spectra of neighboring stars. Observation of this star in the infrared band during the 2MASS survey appeared to reveal excess emission. However, the distribution of this emission couldn\u0027t be readily explained by a conjectured disk of circumstellar dust. Instead, the detection was later ascribed to errors caused by saturation of the near-infrared detectors.\r\rThis star has two 12th magnitude companions at angular separations of 6.5 and 158.6 arcseconds.\r\rIt has the traditional names Deneb el Okab, from an Arabic term \u0630\u0646\u0628 \u0627\u0644\u0639\u0642\u0627\u0628 \u00F0anab al-cuq\u0101b meaning \u0022the tail of the falcon\u0022, and the Mandarin names Woo and Yu\u00EB, derived from and represent the state Wu (\u5433), an old state was located at the mouth of the Yangtze River, and Yue (\u8D8A), an old state in Zhejiang province (together with 19 Capricorni or \u03C8 Capricorni in R.H.Allen\u0027s version, in Twelve States asterism). According to the R.H. Allen\u0027s works, it shares names with \u03B5 Aquilae.\r\rIn Chinese, \u5929\u5E02\u5DE6\u57A3 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the left borderline of the enclosure, consisting of \u03B6 Aquilae, \u03B4 Herculis, \u03BB Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B81 Serpentis, \u03B7 Serpentis, \u03BD Ophiuchi, \u03BE Serpentis and \u03B7 Ophiuchi. Consequently, \u03B6 Aquilae itself is known as \u5929\u5E02\u5DE6\u57A3\u516D (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n li\u00F9, English: the Sixth Star of Left Wall of Heavenly Market Enclosure), represent the states which have mentioned above.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Dzeneb al Tair (from \u0630\u0646\u0628 \u0627\u0644\u0637\u0627\u0626\u0631 - \u00F0anab a\u1E6D-\u1E6D\u0101\u0027ir), which was translated into Latin as Cauda (Vulturis) Volantis, meaning the eagle\u0027s tail.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "17 Aquilae, Zeta Aquilae, HIP 93747, SAO 104461, HD 177724, GC 26270, HR 7235, DM BD+13  3899, TYC 1052-3027-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Deneb el Okab Australis",
	"OType" : "Double or multiple star",
	"Distance" : "25.46",
	"RA_S" : 286.35253215,
	"DEC_S" : 13.86347684,
	"X" : 519,
	"Y" : 188,
	"Constellation" : "Aquila ",
	"AMag" : 2.958,
	"key" : 20444,
	"shortTitle" : "Deneb (see HD176411)",
	"title" : "Deneb el Okab Australis"
	},
{
	"Index" : "34488",
	"Description" : "Lambda Aquilae (\u03BB Aql, \u03BB Aquilae) is a star in the constellation Aquila. It has the traditional name Al Thalimain, which it shares with \u03B9 Aquilae. The name is derived from the Arabic \u0627\u0644\u062B\u0627\u0644\u0645\u064A\u0646 al-thal\u012Bmain \u0022the two ostriches\u0022. Lambda Aquilae is more precisely Al Thalimain Prior. It has an apparent visual magnitude of 3.43, which is bright enough to be seen with the naked eye. Parallax measurements place it at a distance of about 125 light-years (38 parsecs) from Earth.\r\rIn Chinese, \u5929\u5F01 (Ti\u0101n Bi\u00E0n), meaning Market Officer, refers to an asterism consisting of \u03BB Aquilae, \u03B1 Scuti, \u03B4 Scuti, \u03B5 Scuti, \u03B2 Scuti, \u03B7 Scuti, 12 Aquilae, 15 Aquilae and 14 Aquilae. Consequently, \u03BB Aquilae itself is known as \u5929\u5F01\u4E03 (Ti\u0101n Bi\u00E0n q\u012B, English: the Seventh Star of Market Officer.)\r\rLambda Aquilae is a main sequence star with a stellar classification of B9Vn, which means that, like the Sun, it is generating energy at its core through the nuclear fusion of hydrogen. It is more massive than the Sun, with about three times its mass, and radiates about 55 times the Sun\u0027s luminosity from its outer envelope at a higher effective temperature of 11,780 K. This temperature gives Lambda Aquilae the blue-white hue that is a characteristic of B-type stars. Lambda Aquilae was one of the least variable stars observed by the Hipparcos satellite. It is a suspected Lambda Bootis star and has an age of about 160 million years.\r\rThis star lies about 5\u00B0 from the galactic plane and about 30\u00B0 from the line of sight to the Galactic Center. This region of the sky is crowded with other objects along the line of sight, with at least 55 located within 10 arcseconds of the star. Examination of the star shows no companions with an 85% probability. Despite this, it is suspected of being a spectroscopic binary star. That is, it may have an orbiting companion whose presence is revealed by displacements in the absorption lines in the spectrum caused by the Doppler effect. Based upon the width of these lines, the star is rotating rapidly, with a projected rotational velocity of 103 km s\u20131.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "16 Aquilae, Lambda Aquilae, HIP 93805, SAO 143021, HD 177756, GC 26285, HR 7236, DM BD-05  4876, TYC 5136-2357-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Al Thalimain Prior",
	"OType" : "Star",
	"Distance" : "37.9",
	"RA_S" : 286.56224574,
	"DEC_S" : -4.88255574,
	"X" : 518,
	"Y" : 432,
	"Constellation" : "Aquila ",
	"AMag" : 3.395,
	"key" : 54488,
	"title" : "Al Thalimain Prior"
	},
{
	"Index" : "362",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "18 Aquilae, HIP 93867AB, SAO 104488, HD 178125, GC 26315, HR 7248, DM BD+10  3787, TYC 1044-1453-1",
	"group" : { "key" : "Aquila" },
	"Common" : "18 Aquilae",
	"OType" : "Eclipsing binary",
	"Distance" : "209.56",
	"RA_S" : 286.74416631,
	"DEC_S" : 11.07123635,
	"Constellation" : "Aquila ",
	"AMag" : 5.075,
	"key" : 20362,
	"title" : "18 Aquilae"
	},
{
	"Index" : "31671",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "19 Aquilae, HIP 94068, SAO 124318, HD 178596, GC 26379, HR 7266, DM BD+05  4040, TYC 475-1667-1",
	"group" : { "key" : "Aquila" },
	"Common" : "19 Aquilae",
	"OType" : "Variable Star",
	"Distance" : "45.76",
	"RA_S" : 287.24963457,
	"DEC_S" : 6.0732071,
	"Constellation" : "Aquila ",
	"AMag" : 5.269,
	"key" : 51671,
	"title" : "19 Aquilae"
	},
{
	"Index" : "38756",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "20 Aquilae, HIP 94385, SAO 143134, HD 179406, GC 26461, HR 7279, DM BD-08  4887, TYC 5708-693-1",
	"group" : { "key" : "Aquila" },
	"Common" : "20 Aquilae",
	"OType" : "Variable Star",
	"Distance" : "298.28",
	"RA_S" : 288.16962788,
	"DEC_S" : -7.93951799,
	"Constellation" : "Aquila ",
	"AMag" : 5.359,
	"key" : 58756,
	"title" : "20 Aquilae"
	},
{
	"Index" : "30995",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "21 Aquilae, HIP 94477, SAO 124408, HD 179761, GC 26490, HR 7287, DM BD+02  3824, TYC 467-4986-1",
	"group" : { "key" : "Aquila" },
	"Common" : "21 Aquilae",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "216.83",
	"RA_S" : 288.42793064,
	"DEC_S" : 2.29370724,
	"Constellation" : "Aquila ",
	"AMag" : 5.117,
	"key" : 50995,
	"title" : "21 Aquilae"
	},
{
	"Index" : "420",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "25 Aquilae, Omega01 Aquilae, HIP 94834, SAO 104691, HD 180868, GC 26609, HR 7315, DM BD+11  3790, TYC 1050-593-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Omega01 Aquilae",
	"OType" : "Star",
	"Distance" : "127.02",
	"RA_S" : 289.45415708,
	"DEC_S" : 11.59542347,
	"Constellation" : "Aquila ",
	"AMag" : 5.307,
	"key" : 20420,
	"title" : "Omega01 Aquilae"
	},
{
	"Index" : "30788",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "23 Aquilae, HIP 94885A, SAO 124487, HD 180972, GC 26623, HR 7319, DM BD+00  4168, TYC 464-3404-1",
	"group" : { "key" : "Aquila" },
	"Common" : "23 Aquilae",
	"OType" : "Star",
	"Distance" : "113.31",
	"RA_S" : 289.6354016,
	"DEC_S" : 1.08511912,
	"Constellation" : "Aquila ",
	"AMag" : 5.283,
	"key" : 50788,
	"title" : "23 Aquilae"
	},
{
	"Index" : "34501",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "26 Aquilae, f Aquilae, HIP 95066, SAO 143286, HD 181391, GC 26669, HR 7333, DM BD-05  4936, TYC 5138-2406-1",
	"group" : { "key" : "Aquila" },
	"Common" : "f Aquilae",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.26",
	"RA_S" : 290.13710737,
	"DEC_S" : -5.41576633,
	"Constellation" : "Aquila ",
	"AMag" : 5.094,
	"key" : 54501,
	"title" : "f Aquilae"
	},
{
	"Index" : "34451",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "27 Aquilae, d Aquilae, HIP 95073, SAO 143292, HD 181440, GC 26673, HR 7336, DM BD-01  3716, TYC 5130-2811-1",
	"group" : { "key" : "Aquila" },
	"Common" : "d Aquilae",
	"OType" : "Star",
	"Distance" : "134",
	"RA_S" : 290.14869437,
	"DEC_S" : -0.89216022,
	"Constellation" : "Aquila ",
	"AMag" : 5.444,
	"key" : 54451,
	"title" : "d Aquilae"
	},
{
	"Index" : "561",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "31 Aquilae, b Aquilae, HIP 95447, SAO 104807, HD 182572, GC 26809, HR 7373, DM BD+11  3833, TYC 1063-519-1",
	"group" : { "key" : "Aquila" },
	"Common" : "b Aquilae",
	"OType" : "Variable Star",
	"Distance" : "15.18",
	"RA_S" : 291.24250108,
	"DEC_S" : 11.94441423,
	"Constellation" : "Aquila ",
	"AMag" : 5.243,
	"key" : 20561,
	"title" : "b Aquilae"
	},
{
	"Index" : "31216",
	"Description" : "Delta Aquilae (\u03B4 Aql, \u03B4 Aquilae) is a binary star system in the equatorial constellation of Aquila. The traditional name for this star is Denebokab. It has an apparent visual magnitude of 3.4 and, based upon parallax measurements, is located about 50.6 light-years (15.5 parsecs) from Earth.\r\rDelta Aquilae is an astrometric binary where the two components orbit each other with a period of 3.422 years and an eccentricity of about 0.36. This is a type of binary star system where the presence of the secondary component is revealed by its gravitational perturbation of the primary. The individual components have not been resolved with a telescope.\r\rThe primary component, Delta Aquilae A, is a subgiant star with a stellar classification of F0 IV, where the luminosity class of IV indicates it is in the process of exhausting the supply of hydrogen at its core and evolving into a giant star. The mass of the star is 65% greater than the Sun and it has expanded to more than double the Sun\u0027s radius. It is radiating around 7\u20138 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 7,016 K, giving it the yellow-white hue of an F-type star. Delta Aquilae A is a Delta Scuti variable that exhibits variations in luminosity caused by pulsations in its outer envelope. It is spinning rapidly with a projected rotational velocity of about 87 km s\u20131. This is a lower bound on the azimuthal velocity along the star\u0027s equator.\r\rThe secondary component, Delta Aquilae B, is a smaller star with about 67% of the Sun\u0027s mass and an estimated 61% of the radius of the Sun. It may be a K-type star.\r\rThis star is sometimes called by the name Denebokab, meaning the tail of eagle in Arabic. In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Djenubi Menkib al Nesr (\u0645\u0646\u0643\u0628 \u0623\u0644\u0646\u0633\u0631 \u0623\u0644\u062E\u0646\u0648\u0628\u064A - mankib al-nasr al-jan\u00FAbii), which was translated into Latin as Australior Humerus Vulturis, meaning the southern shoulder of the eagle.\r\rIn Chinese, \u53F3\u65D7 (Y\u00F2u Q\u00ED), meaning Right Flag, refers to an asterism consisting of \u03B4 Aquilae, \u03BC Aquilae, \u03C3 Aquilae, \u03BD Aquilae, \u03B9 Aquilae, 42 Aquilae, HD 184701, \u03BA Aquilae and 56 Aquilae. Consequently, \u03B4 Aquilae itself is known as \u53F3\u65D7\u4E09 (Y\u00F2u Q\u00ED s\u0101n, English: the Third Star of Right Flag.)\r\rThis star, along with \u03B7 Aql and \u03B8 Aql (Tseen Foo) and, were Al Miz\u0101n (\u0623\u0644\u0645\u064A\u0632\u0627\u0646), the Scale-beam. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Miz\u0101n were the title for three stars :\u03B4 Aql as Al Miz\u0101n I, \u03B7 Aql as l Miz\u0101n II and \u03B8 Aql as Al Miz\u0101n III.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "30 Aquilae, Delta Aquilae, HIP 95501, SAO 124603, HD 182640, GC 26816, HR 7377, DM BD+02  3879, TYC 469-6227-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Denebokab",
	"OType" : "Double or multiple star",
	"Distance" : "15.37",
	"RA_S" : 291.37457816,
	"DEC_S" : 3.11478558,
	"X" : 456,
	"Y" : 328,
	"Constellation" : "Aquila ",
	"AMag" : 3.39,
	"key" : 51216,
	"title" : "Denebokab"
	},
{
	"Index" : "30860",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "32 Aquilae, Nu Aquilae, HIP 95585, SAO 124628, HD 182835, GC 26838, HR 7387, DM BD+00  4206, TYC 465-2618-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Nu Aquilae",
	"OType" : "Star",
	"Distance" : "869.5652",
	"RA_S" : 291.62953573,
	"Constellation" : "Aquila ",
	"AMag" : 4.729,
	"key" : 50860,
	"title" : "Nu Aquilae"
	},
{
	"Index" : "34572",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "36 Aquilae, e Aquilae, HIP 95937, SAO 143482, HD 183630, GC 26936, HR 7414, DM BD-03  4612, TYC 5148-3284-1",
	"group" : { "key" : "Aquila" },
	"Common" : "e Aquilae",
	"OType" : "Variable Star",
	"Distance" : "161.62",
	"RA_S" : 292.66598846,
	"DEC_S" : -2.78888641,
	"Constellation" : "Aquila ",
	"AMag" : 5.228,
	"key" : 54572,
	"title" : "e Aquilae"
	},
{
	"Index" : "33185",
	"Description" : "Mu Aquilae (\u03BC Aql, \u03BC Aquilae) is the Bayer designation for a star in the equatorial constellation of Aquila. With an apparent visual magnitude of 4.45, it is visible to the naked eye. The measured annual parallax shift of 30.31 mas, which is equivalent to a distance of 107.6 light-years (33.0 parsecs) from Earth.\r\rThe stellar classification of Mu Aquilae is K3 III, indicating that this is an evolved giant star. It belongs to a sub-category called the red clump, indicating that it is generating energy through the fusion of helium at its core. Compared to the Sun, it has 92% of the mass but has expanded to eight times the size. This inflated outer envelope has an effective temperature of 4,467 K and is radiating 24.5 times the Sun\u0027s luminosity. At this heat, Mu Aquilae glows with the orange hue of a K-type star.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "38 Aquilae, Mu Aquilae, HIP 96229, SAO 124799, HD 184406, GC 27030, HR 7429, DM BD+07  4132, TYC 490-5566-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Mu Aquilae",
	"OType" : "Variable Star",
	"Distance" : "32.99",
	"RA_S" : 293.52230415,
	"DEC_S" : 7.37894182,
	"X" : 428,
	"Y" : 273,
	"Constellation" : "Aquila ",
	"AMag" : 4.576,
	"key" : 53185,
	"title" : "Mu Aquilae"
	},
{
	"Index" : "38875",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "37 Aquilae, HIP 96327, SAO 162792, HD 184492, GC 27046, HR 7430, DM BD-10  5122, TYC 5727-2383-1",
	"group" : { "key" : "Aquila" },
	"Common" : "37 Aquilae",
	"OType" : "Star",
	"Distance" : "139.89",
	"RA_S" : 293.78024054,
	"DEC_S" : -10.56044139,
	"Constellation" : "Aquila ",
	"AMag" : 5.242,
	"key" : 58875,
	"title" : "37 Aquilae"
	},
{
	"Index" : "34545",
	"Description" : "Iota Aquilae (\u03B9 Aql, \u03B9 Aquilae) is the Bayer designation for a star in the equatorial constellation of Aquila. It has the traditional name Al Thalimain, which it shares with \u03BB Aquilae. The name is derived from the Arabic term \u0627\u0644\u062B\u0627\u0644\u0645\u064A\u0646 ath-thal\u012Bmain meaning \u0022The Two Ostriches\u0022. With an apparent visual magnitude of 4.364, this star is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 8.34 \u00B1 0.79 mas, it is located at a distance of around 390 light-years (120 parsecs) from Earth. At that distance, the visual magnitude of the star is diminished by 0.15 from extinction caused by intervening gas and dust.\r\rIn Chinese, \u53F3\u65D7 (Y\u00F2u Q\u00ED), meaning Right Flag, refers to an asterism consisting of \u03B9 Aquilae, \u03BC Aquilae, \u03C3 Aquilae, \u03B4 Aquilae, \u03BD Aquilae, 42 Aquilae, HD 184701, \u03BA Aquilae and 56 Aquilae. Consequently, \u03B9 Aquilae itself is known as \u53F3\u65D7\u4E94 (Y\u00F2u Q\u00ED wu, English: the Fifth Star of Right Flag.)\r\rAlthough Iota Aquilae is listed in star catalogues as a giant star, calculations of its dimension show that in reality it is a main-sequence star. It has nearly five times the mass of the Sun and five to six times the Sun\u0027s radius. It is emitting 851 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 14,552 K, giving it the blue-white hue of a B-type star. The projected rotational velocity of this star is 55 km/s. Even though it is only around 100 million years old, it has already spent 91% of its allotted lifetime on the main sequence.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "41 Aquilae, Iota Aquilae, HIP 96468, SAO 143597, HD 184930, GC 27103, HR 7447, DM BD-01  3782, TYC 5144-3103-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Al Thalimain",
	"OType" : "Star",
	"Distance" : "118.63",
	"RA_S" : 294.18031692,
	"DEC_S" : -1.2866003,
	"X" : 420,
	"Y" : 385,
	"Constellation" : "Aquila ",
	"AMag" : 4.323,
	"key" : 54545,
	"title" : "Al Thalimain"
	},
{
	"Index" : "34617",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "39 Aquilae, Kappa Aquilae, HIP 96483, SAO 143600, HD 184915, GC 27107, HR 7446, DM BD-07  5006, TYC 5156-3185-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Kappa Aquilae",
	"OType" : "Star",
	"Distance" : "508.97",
	"RA_S" : 294.22270594,
	"DEC_S" : -7.02747711,
	"Constellation" : "Aquila ",
	"AMag" : 4.942,
	"key" : 54617,
	"title" : "Kappa Aquilae"
	},
{
	"Index" : "34603",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "42 Aquilae, HIP 96556, SAO 143621, HD 185124, GC 27143, HR 7460, DM BD-04  4861, TYC 5153-2875-1",
	"group" : { "key" : "Aquila" },
	"Common" : "42 Aquilae",
	"OType" : "Star",
	"Distance" : "32.15",
	"RA_S" : 294.44715694,
	"DEC_S" : -4.64764168,
	"Constellation" : "Aquila ",
	"AMag" : 5.485,
	"key" : 54603,
	"title" : "42 Aquilae"
	},
{
	"Index" : "32938",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "44 Aquilae, Sigma Aquilae, HIP 96665, SAO 124903, HD 185507, GC 27185, HR 7474, DM BD+05  4225, TYC 487-3422-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Sigma Aquilae",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "236.63",
	"RA_S" : 294.79850847,
	"DEC_S" : 5.39777571,
	"Constellation" : "Aquila ",
	"AMag" : 5.18,
	"key" : 52938,
	"title" : "Sigma Aquilae"
	},
{
	"Index" : "583",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "47 Aquilae, Chi Aquilae, HIP 96957AB, SAO 105168, HD 186203, GC 27272, HR 7497, DM BD+11  3955A, TYC 1065-3144-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Chi Aquilae",
	"OType" : "Star",
	"Distance" : "256.3",
	"RA_S" : 295.64175091,
	"DEC_S" : 11.8265928,
	"Constellation" : "Aquila ",
	"AMag" : 5.366,
	"key" : 20583,
	"title" : "Chi Aquilae"
	},
{
	"Index" : "539",
	"Description" : "Gamma Aquilae (\u03B3 Aql, \u03B3 Aquilae) is a star in the constellation Aquila. It has the traditional name Tarazed. This star has an apparent visual magnitude of 2.712, so it is readily visible to the naked eye at night. Parallax measurements place it at a distance of 395 light-years (121 parsecs) from Earth.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "50 Aquilae, Gamma Aquilae, HIP 97278, SAO 105223, HD 186791, GC 27354, HR 7525, DM BD+10  4043, TYC 1061-2577-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Tarazed",
	"OType" : "Star",
	"Distance" : "121",
	"RA_S" : 296.56491643,
	"DEC_S" : 10.61326319,
	"X" : 388,
	"Y" : 231,
	"Constellation" : "Aquila ",
	"AMag" : 2.861,
	"key" : 20539,
	"shortTitle" : "Reda",
	"title" : "Tarazed"
	},
{
	"Index" : "38884",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "51 Aquilae, HIP 97650, SAO 163036, HD 187532, GC 27465, HR 7553, DM BD-11  5149, TYC 5729-2871-1",
	"group" : { "key" : "Aquila" },
	"Common" : "51 Aquilae",
	"OType" : "Star",
	"Distance" : "27.87",
	"RA_S" : 297.69493144,
	"DEC_S" : -10.76351378,
	"Constellation" : "Aquila ",
	"AMag" : 5.425,
	"key" : 58884,
	"title" : "51 Aquilae"
	},
{
	"Index" : "548",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "54 Aquilae, Omicron Aquilae, HIP 97675, SAO 105338, HD 187691, GC 27480, HR 7560, DM BD+10  4073, TYC 1062-2701-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Omicron Aquilae",
	"OType" : "High proper-motion Star",
	"Distance" : "19.19",
	"RA_S" : 297.75684735,
	"DEC_S" : 10.41572455,
	"Constellation" : "Aquila ",
	"AMag" : 5.185,
	"key" : 20548,
	"title" : "Omicron Aquilae"
	},
{
	"Index" : "32303",
	"Description" : "Eta Aquilae (\u03B7 Aql, \u03B7 Aquilae) is the Bayer designation for a star in the equatorial constellation of Aquila, the eagle. It was once part of the former constellation Antinous. On average, this star has an apparent visual magnitude of 3.87, making it one of the brighter members of Aquila. Based upon parallax measurements made during the Hipparcos mission, this star is located at a distance of roughly 1,382 light-years (424 parsecs), although the parallax estimate has a 44% margin of error.\r\rThis is a Cepheid variable star, with an apparent magnitude that ranges from 3.5 to 4.4 over a period of 7.176641 days. Along with Delta Cephei, Zeta Geminorum and Beta Doradus, it is one of the most prominent naked eye Cepheids; that is, both the star itself and the variation in its brightness can be distinguished with the naked eye. Some other Cepheids such as Polaris are bright but have only a very small variation in brightness.\r\rAt the relatively young age of 26 million years, this massive star has burned through the hydrogen fuel at its core and evolved into a supergiant, giving it a baseline stellar classification of F6 Ibv. The Ib luminosity class indicates this is a less luminous type of supergiant, while the \u0027v\u0027 suffix shows that the spectrum of the star varies. The periodic pulsations of this star actually cause the stellar class to vary between (F6.5\u2013G2)Ib over the course of each cycle.\r\rCompared to the Sun, Eta Aquilae has around 9 times the mass, roughly 107 times the radius, and is radiating 11,474 times as much luminosity. This energy is being emitted from the outer envelope at an effective temperature of 6,000 K, giving it the yellow-white hued glow of an F-type star. The radius of the star varies by 4.59 \u00D7 106 km (0.007 R\u2609) over the course of a pulsation cycle. Compared to its neighbors, this star has a high peculiar velocity of 16.7 \u00B1 6.9 km s\u20131.\r\rSometimes, this star is called by the name Bezek, derived the Hebrew word \u05D1\u05C7\u05BC\u05D6\u05C7\u05E7 bazak, meaning \u0022lightning\u0022.\r\rIn Chinese, \u5929\u6874 (Ti\u0101n F\u00FA), meaning Celestial Drumstick, refers to an asterism consisting of \u03B7 Aquilae, \u03B8 Aquilae, 62 Aquilae and 58 Aquilae. Consequently, \u03B7 Aquilae itself is known as \u5929\u6874\u56DB (Ti\u0101n F\u00FA s\u00EC, English: the Fourth Star of Celestial Drumstrick.)\r\rThis star, along with \u03B4 Aql (Denebokab) and \u03B8 Aql (Tseen Foo) and, were Al Miz\u0101n (\u0623\u0644\u0645\u064A\u0632\u0627\u0646), the Scale-beam. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Miz\u0101n were the title for three stars :\u03B4 Aql as Al Miz\u0101n I,\u03B7 Aql as Al Miz\u0101n II and \u03B8 Aql as Al Miz\u0101n III.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "55 Aquilae, Eta Aquilae, HIP 97804, SAO 125159, HD 187929, GC 27517, HR 7570, DM BD+00  4337, TYC 480-3027-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Bezek",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "423.7288",
	"RA_S" : 298.11820354,
	"DEC_S" : 1.00565902,
	"X" : 368,
	"Y" : 355,
	"Constellation" : "Aquila ",
	"AMag" : 4.058,
	"key" : 52303,
	"title" : "Bezek"
	},
{
	"Index" : "514",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "59 Aquilae, Xi Aquilae, HIP 97938, SAO 125210, HD 188310, GC 27558, HR 7595, DM BD+08  4261, TYC 1058-3400-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Deneb Okab (see HD176411,177724,182640)",
	"OType" : "Star",
	"Distance" : "56.26",
	"RA_S" : 298.56200897,
	"DEC_S" : 8.46145444,
	"Constellation" : "Aquila ",
	"AMag" : 4.824,
	"key" : 20514,
	"title" : "Deneb Okab (see HD176411,177724,182640)"
	},
{
	"Index" : "33402",
	"Description" : "Beta Aquilae (\u03B2 Aql, \u03B2 Aquilae) is a star in the constellation Aquila. It has the traditional name Alshain from the Perso-Arabic term \u0627\u0644\u0634\u0627\u0647\u064A\u0646 a\u0161-\u0161\u0101h\u012Bn \u0022the (peregrine) falcon\u0022, perhaps by folk etymology from the Persian \u0161\u0101h\u012Bn tar\u0101z\u016B (or possibly \u0161\u0101h\u012Bn tara zed; see \u03B3 Aquilae), the Persian name for the asterism \u03B1, \u03B2 and \u03B3 Aquilae.\r\rIn Chinese, \u6CB3\u9F13 (H\u00E9 G\u016D), meaning River Drum, refers to an asterism consisting of \u03B2 Aquilae, Altair and \u03B3 Aql. Consequently, \u03B2 Aquilae itself is known as \u6CB3\u9F13\u4E00 (H\u00E9 G\u016D y\u012B, English: the First Star of River Drum.)\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Unuk al Ghyrab (\u0639\u0646\u0642 \u0623\u0644\u063A\u0631\u0627\u0628 - \u00FAnuq al-ghuraab), which was translated into Latin as Collum Corvi, meaning the crow\u0027s neck.\r\rBeta Aquilae has magnitude 3.71 and is of spectral class G8IV. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is approximately 44.7 light years from Earth. It has a 12th magnitude optical companion, \u03B2 Aquilae B, which is 13 arcseconds away in the sky.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "60 Aquilae, Beta Aquilae, HIP 98036, SAO 125235, HD 188512, GC 27587, HR 7602, DM BD+06  4357, TYC 493-3355-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Alshain",
	"OType" : "High proper-motion Star",
	"Distance" : "13.7",
	"RA_S" : 298.82830106,
	"DEC_S" : 6.40676319,
	"X" : 359,
	"Y" : 286,
	"Constellation" : "Aquila ",
	"AMag" : 3.807,
	"key" : 53402,
	"shortTitle" : "Alschairn",
	"title" : "Alshain"
	},
{
	"Index" : "709",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "61 Aquilae, Phi Aquilae, HIP 98103, SAO 105438, HD 188728, GC 27604, HR 7610, DM BD+11  4055, TYC 1079-3514-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Phi Aquilae",
	"OType" : "Spectroscopic binary",
	"Distance" : "67.27",
	"RA_S" : 299.0593835,
	"DEC_S" : 11.42372088,
	"Constellation" : "Aquila ",
	"AMag" : 5.278,
	"key" : 20709,
	"title" : "Phi Aquilae"
	},
{
	"Index" : "34650",
	"Description" : "Theta Aquilae (\u03B8 Aql, \u03B8 Aquilae) is a binary star in the constellation Aquila. The combined apparent visual magnitude of the pair is 3.26, making it the fourth brightest member of the constellation. In Chinese, it has the traditional name Tseen Foo, which is derived from the Mandarin \u5929\u6874 ti\u0101nf\u00FA meaning \u0022the heavenly raft(er)\u0022; it may also mean drumsticks, with Altair, Beta Aquilae and Gamma Aquilae being the drum. This distance to this star can be determined through the parallax technique, yielding an estimate of roughly 286 light-years (88 parsecs) from Earth.\r\rTheta Aquilae is a double-lined spectroscopic binary, which indicates that the individual components have not been viewed through a telescope; instead, what can be viewed is their combined spectrum with the individual absorption line features shifting back and forth over the course of an orbit because of the Doppler effect. Their orbit has a period of 17.1 days with a large orbital eccentricity is 0.60. At the estimated distance of this system, the angular separation of 3.2 milliarcseconds corresponds to a physical separation of only about 0.24\u20130.28 Astronomical Units.\r\rBoth stars have a matching stellar classification of B9.5 III, indicating that they are massive, B-type giant stars that have exhausted the supply of hydrogen at their cores and evolved away from the main sequence of stars like the Sun. Hummel et al. (1996) gave the primary component, \u03B8 Aql A, an estimated mass of 3.6 solar, a radius 4.8 the Sun\u0027s, and 278 the luminosity of the Sun. For the secondary component, \u03B8 Aql B, they give the corresponding parameters as 2.9 times the mass, 2.4 times the radius and 68 times the luminosity of the Sun. Based upon their estimated parameters, Kaler (2008) suggests that \u03B8 Aql A is actually a subgiant star, while \u03B8 Aql B is a main sequence star.\r\rIn Chinese, \u5929\u6874 (Ti\u0101n F\u00FA), meaning Celestial Drumstick, refers to an asterism consisting of \u03B8 Aquilae, 62 Aquilae, 58 Aquilae and \u03B7 Aquilae. Consequently, \u03B8 Aquilae itself is known as \u5929\u6874\u4E00 (Ti\u0101n F\u00FA y\u012B, English: the First Star of Celestial Drumstrick.)\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Thanih Ras al Akab (\u062A\u0627\u0646\u064A \u0623\u0644\u0631\u0623\u0633 \u0623\u0644\u0639\u0642\u0627\u0628 - taanii al ra\u0027s al\u0295uq\u0101b), which was translated into Latin as Secunda Capitis Vulturis, meaning the second (star) of eagle\u0027s head.\r\rThis star, along with \u03B4 Aql (Denebokab) and \u03B7 Aql, were Al Miz\u0101n (\u0623\u0644\u0645\u064A\u0632\u0627\u0646), the Scale-beam. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Miz\u0101n were the title for three stars :\u03B4 Aql as Al Miz\u0101n I, \u03B7 Aql as l Miz\u0101n II and \u03B8 Aql as Al Miz\u0101n III.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "65 Aquilae, Theta Aquilae, HIP 99473, SAO 144150, HD 191692, GC 28010, HR 7710, DM BD-01  3911, TYC 5161-2682-1",
	"group" : { "key" : "Aquila" },
	"Common" : "Tseen Foo",
	"OType" : "Spectroscopic binary",
	"Distance" : "87.75",
	"RA_S" : 302.826108,
	"DEC_S" : -0.821475,
	"X" : 307,
	"Y" : 380,
	"Constellation" : "Aquila ",
	"AMag" : 3.208,
	"key" : 54650,
	"title" : "Tseen Foo"
	},
{
	"Index" : "34050",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "HIP 100541, SAO 125747, HD 194013, GC 28351, HR 7794, DM BD+04 4434, TYC 505-2355-1",
	"group" : { "key" : "Aquila" },
	"Common" : "HR 7794",
	"OType" : "Star",
	"Distance" : "75.52",
	"RA_S" : 305.79455903,
	"DEC_S" : 5.34298481,
	"Constellation" : "Aquila ",
	"AMag" : 5.409,
	"key" : 54050,
	"title" : "HR 7794"
	},
{
	"Index" : "34690",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "69 Aquilae, HIP 101101, SAO 144495, HD 195135, GC 28504, HR 7831, DM BD-03  4918, TYC 5167-2593-1",
	"group" : { "key" : "Aquila" },
	"Common" : "69 Aquilae",
	"OType" : "Star",
	"Distance" : "61.25",
	"RA_S" : 307.41249979,
	"DEC_S" : -2.88553365,
	"Constellation" : "Aquila ",
	"AMag" : 5.03,
	"key" : 54690,
	"title" : "69 Aquilae"
	},
{
	"Index" : "34766",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "70 Aquilae, HIP 101692, SAO 144624, HD 196321, GC 28684, HR 7873, DM BD-03  4961, TYC 5180-338-1",
	"group" : { "key" : "Aquila" },
	"Common" : "70 Aquilae",
	"OType" : "Star",
	"Distance" : "390.31",
	"RA_S" : 309.18180097,
	"DEC_S" : -2.54995537,
	"Constellation" : "Aquila ",
	"AMag" : 5.074,
	"key" : 54766,
	"title" : "70 Aquilae"
	},
{
	"Index" : "34751",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "71 Aquilae, l Aquilae, HIP 101847, SAO 144649, HD 196574, GC 28725, HR 7884, DM BD-01  4016, TYC 5177-1878-1",
	"group" : { "key" : "Aquila" },
	"Common" : "l Aquilae",
	"OType" : "Spectroscopic binary",
	"Distance" : "102.67",
	"RA_S" : 309.58451773,
	"DEC_S" : -1.10511663,
	"Constellation" : "Aquila ",
	"AMag" : 4.409,
	"key" : 54751,
	"title" : "l Aquilae"
	},
{
	"Index" : "64436",
	"Description" : "Eta Arae (\u03B7 Ara, \u03B7 Arae) is the Bayer designation for a single  star in the southern constellation of Ara. It is approximately 299 light-years (92 parsecs) from Earth and is visible to the naked eye with an apparent visual magnitude of 3.76. \r\rThe spectrum of this star matches a stellar classification of K5 III, indicating that, at an estimated age of seven billion years, it has reached the giant star stage of its evolution. With a mass nearly the same as the Sun, it has an outer envelope that has expanded to nearly 56 times the Sun\u0027s radius. The star is now spinning so slowly that it takes more than eleven years to complete a single rotation. Eta Arae is radiating energy into space at an effective temperature of 3,886 K, giving it the orange-hued glow of a K-type star.\r\rIt has a 14th magnitude optical companion, located 25.7 arcseconds away.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Eta Arae, HIP 82363, SAO 244168, HD 151249, GC 22606, HR 6229, DM CP-58  6906, TYC 8725-3067-1",
	"group" : { "backgroundImage" : "images/Alignment/06.png",
		"description" : "Ara is a southern constellation situated between Scorpius and Triangulum Australe. Its name is Latin for \u0022altar\u0022. Ara was one of the 48 Greek constellations described by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations defined by the International Astronomical Union.\r\rIn ancient Greek mythology, Ara was identified as the altar where the gods first made offerings and formed an alliance before defeating the Titans. The nearby Milky Way represents the smoke rising from the offerings on the altar.",
		"key" : "Ara",
		"grouptype" : "Ara",
		"Meaning" : "altar",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Ara",
		"title" : "Ara Objects Group" },
	"Common" : "Eta Arae",
	"OType" : "Star",
	"Distance" : "91.71",
	"RA_S" : 252.44648214,
	"DEC_S" : -59.04137698,
	"X" : 504,
	"Y" : 344,
	"Constellation" : "Ara ",
	"AMag" : 3.932,
	"key" : 84436,
	"title" : "Eta Arae"
	},
{
	"Index" : "64492",
	"Description" : "Zeta Arae (\u03B6 Ara, \u03B6 Arae) is a star in the southern constellation Ara. It is sometimes is called by the name Tseen Yin, together with \u03B4 Arae. The apparent visual magnitude of this star is 3.1, which can be seen from suburban skies in the southern hemisphere. From the parallax measurements, it is located at a distance of 490 light-years (150 parsecs) from Earth.\r\rThe spectrum of this star matches a stellar classification of K3 III. The luminosity class of \u0027III\u0027 indicates this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. It is radiating energy from its outer atmosphere at an effective temperature of 4,350 K, which is what gives it the orange hue of a K-type star. This star displays an excess of infrared emission that may indicate circumstellar matter.\r\rIn Chinese, \u6775 (Gu\u012B), meaning Tortoise, refers to an asterism consisting of \u03B6 Arae, \u03B51 Arae, \u03B3 Arae, \u03B4 Arae and \u03B7 Arae. Consequently, \u03B6 Arae itself is known as \u9F9C\u4E94 (Gu\u012B w\u01D4, English: the Fifth Star of Tortoise.)",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Zeta Arae, HIP 83081, SAO 244315, HD 152786, GC 22845, HR 6285, DM CP-55  7766, TYC 8730-1439-1",
	"group" : { "key" : "Ara" },
	"Common" : "Tseen Yin",
	"OType" : "Star",
	"Distance" : "148.89",
	"RA_S" : 254.65505492,
	"DEC_S" : -55.99014141,
	"X" : 507,
	"Y" : 301,
	"Constellation" : "Ara ",
	"AMag" : 3.276,
	"key" : 84492,
	"title" : "Tseen Yin"
	},
{
	"Index" : "64453",
	"Description" : "Epsilon1 Arae (\u03B51 Ara, \u03B51 Arae) is the Bayer designation for a star in the constellation Ara, the Altar. It is visible to the naked eye with an apparent visual magnitude of +4.1 Based upon an annual parallax shift of 9.04 mas, this star is around 360 light-years (110 parsecs) distant from the Earth.\r\r\u03B51 Arae is an evolved giant star with a stellar classification of K3 III. It is around 74% more massive than the Sun. At an age of about 1.7 billion years, the outer envelope of the star has expanded to almost 34 times the Sun\u0027s radius. It is radiating energy into space at an effective temperature of 4,176 K, giving it the orange-hued glow of a K-type star.\r\r\u03B51 Arae was known as \u9F9C\u4E00 (meaning: \u0022the 1st (star) of Gu\u012B\u0022) in traditional Chinese astronomy. Allen erroneously called it as Tso Kang (\u5DE6\u66F4). He probably confused constellation \u0022Ara\u0022 with \u0022Ari\u0022. Tso Kang was lain[clarification needed] in Aries.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Epsilon01 Arae, HIP 83153, SAO 244331, HD 152980, GC 22869, HR 6295, DM CP-52 10372, TYC 8726-2208-1",
	"group" : { "key" : "Ara" },
	"Common" : "Epsilon1 Arae",
	"OType" : "Star",
	"Distance" : "110.5",
	"RA_S" : 254.8960309,
	"DEC_S" : -53.16044073,
	"X" : 521,
	"Y" : 266,
	"Constellation" : "Ara ",
	"AMag" : 4.218,
	"key" : 84453,
	"title" : "Epsilon1 Arae"
	},
{
	"Index" : "64454",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Epsilon02 Arae, HIP 83431AC, SAO 244388, HD 153580, GC 22956, HR 6314, DM CP-53  8316, TYC 8726-2209-1",
	"group" : { "key" : "Ara" },
	"Common" : "Epsilon02 Arae",
	"OType" : "Double or multiple star",
	"Distance" : "27.22",
	"RA_S" : 255.78626437,
	"DEC_S" : -53.23699418,
	"Constellation" : "Ara ",
	"AMag" : 5.333,
	"key" : 84454,
	"title" : "Epsilon02 Arae"
	},
{
	"Index" : "60582",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Iota Arae, HIP 85079, SAO 227886, HD 157042, GC 23470, HR 6451, DM CD-47 11484, TYC 8345-4829-1",
	"group" : { "key" : "Ara" },
	"Common" : "Iota Arae",
	"OType" : "Be Star",
	"Distance" : "284.64",
	"RA_S" : 260.81697907,
	"DEC_S" : -47.46820144,
	"Constellation" : "Ara ",
	"AMag" : 5.229,
	"key" : 80582,
	"title" : "Iota Arae"
	},
{
	"Index" : "64508",
	"Description" : "Beta Arae (\u03B2 Ara, \u03B2 Arae) is the brightest star in the constellation Ara, with an apparent visual magnitude of 2.8. Parallax measurements place it at a distance of roughly 650 light-years (200 parsecs) from Earth.\r\rThe spectrum of this star matches a stellar classification of K3 Ib-IIa, with the luminosity class notation \u0027Ib-IIa\u0027 indicating that the star lies part way between a higher luminosity bright giant (IIa) and a lower luminosity supergiant (Ib). This represents two of the evolutionary stages that a massive star passes through after it has exhausted the hydrogen at its core. Beta Arae is radiating energy from its outer envelope at an effective temperature of 4,582 K, which causes it to take on the orange hue of a K-type star. This enlarged star appears to be rotating slowly with a projected rotational velocity of about 5 km s\u20131. The abundance of elements other than hydrogen and helium, what astronomer term the star\u0027s metallicity, is more than three times the abundance in the Sun.\r\rRarely, this star is called by the name Vasat-\u00FCl-cemre in Turkish spelling, derived from Arabic word \uFEED\uFEB3\uFEC2 (wasath) and \uFE9F\uFEE4\uFEE9\uFEAE (khamra), meaning \u0022middle of fire\u0022. In Chinese, \u6775 (Ch\u01D4), meaning Pestle, refers to an asterism consisting of \u03B2 Arae, \u03C3 Arae and \u03B1 Arae. Consequently, \u03B2 Arae itself is known as \u6775\u4E09 (Ch\u01D4 s\u0101n, English: the Third Star of Pestle.)",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Beta Arae, HIP 85258, SAO 244725, HD 157244, GC 23515, HR 6461, DM CP-55  8100, TYC 8732-2866-1",
	"group" : { "key" : "Ara" },
	"Common" : "Beta Arae",
	"OType" : "Star",
	"Distance" : "194.28",
	"RA_S" : 261.32495658,
	"DEC_S" : -55.52988502,
	"X" : 464,
	"Y" : 276,
	"Constellation" : "Ara ",
	"AMag" : 2.968,
	"key" : 84508,
	"title" : "Beta Arae"
	},
{
	"Index" : "64546",
	"Description" : "Gamma Arae (\u03B3 Ara, \u03B3 Arae) is a star in the southern constellation of Ara. With an apparent visual magnitude of 3.3, it is the fourth brightest star in the constellation and is readily visible to the naked eye. From parallax measurements made during the Hipparcos mission, the distance to this star can be estimated as 1,110 light-years (340 parsecs) from Earth.\r\rThis is an enormous star with 23 times the radius of the Sun. It is radiating 120,000 as much energy as the Sun from its outer envelope at an effective temperature of 21,500 K. This heat gives the star the blue-white glow of a B-type star. The spectrum shows it to match a stellar classification of B1 Ib, with the luminosity class of \u0027Ib\u0027 indicating this is a lower luminosity supergiant star. It is a relatively young body, with an estimated age of around 15.7 million years.\r\rGamma Arae is rotating rapidly with a projected rotational velocity of 269 km s\u22121, causing it to complete a full rotation about every 4.8 days. In the spectrum of this star, this high rate of spin is causing absorption lines to blend together because of the Doppler effect, making them more difficult to analyze. It is a periodically variable star that undergoes non-radial pulsations with a primary period of 1.1811 days and a secondary period of 0.1281 days.\r\rThere is some disagreement about the mass of this star in the literature. Tetzlaff et al. (2011) estimate the mass as 12.5 \u00B1 0.6 solar masses, while Fraser et al. (2010) give a mass of around 19 and Lefever et al. (2007) lists a value of 25. It is shedding mass through its stellar wind at the rate of 3.0 \u00D7 10\u22128 solar masses per year, which is equivalent to losing the mass of the Sun every 33 million years. The wind is being effected by the star\u0027s rapid rotation, resulting in an enhanced outflow along the equator.\r\rGamma Arae has an optical companion located at an angular separation of 17.9 arcseconds, which is an A-type main sequence star with an apparent magnitude of 10.5.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Gamma Arae, HIP 85267, SAO 244726, HD 157246, GC 23517, HR 6462, DM CP-56  8225, TYC 8736-3857-1",
	"group" : { "key" : "Ara" },
	"Common" : "Gamma Arae",
	"OType" : "Be Star",
	"Distance" : "340.08",
	"RA_S" : 261.34858046,
	"DEC_S" : -56.37772633,
	"X" : 461,
	"Y" : 287,
	"Constellation" : "Ara ",
	"AMag" : 3.275,
	"key" : 84546,
	"title" : "Gamma Arae"
	},
{
	"Index" : "60667",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Kappa Arae, HIP 85312, SAO 244734, HD 157457, GC 23552, HR 6468, DM CD-50 11269, TYC 8353-3055-1",
	"group" : { "key" : "Ara" },
	"Common" : "Kappa Arae",
	"OType" : "Star",
	"Distance" : "139.14",
	"RA_S" : 261.50017502,
	"DEC_S" : -50.63350693,
	"Constellation" : "Ara ",
	"AMag" : 5.309,
	"key" : 80667,
	"title" : "Kappa Arae"
	},
{
	"Index" : "67720",
	"Description" : "Delta Arae (\u03B4 Arae, \u03B4 Ara) is the Bayer designation for a double star in the southern constellation Ara. It has an apparent visual magnitude of 3.62 and is visible to the naked eye. Based upon an annual parallax of 16.48 mas, it is about 198 light-years (61 parsecs) distant from the Earth.\r\rDelta Arae is massive B-type main sequence star with a stellar classification of B8 Vn. The \u0027n\u0027 suffix indicates the absorption lines are spread out broadly because the star is spinning rapidly. It has a projected rotational velocity of 255 km/s, resulting in an equatorial bulge with a radius 13% larger than the polar radius. It has a magnitude 9.5 companion G-type main sequence star that may form a binary star system with Delta Arae.\r\rThere is a 12th magnitude optical companion located 47.4 arcseconds away along a position angle of 313\u00B0.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Delta Arae, HIP 85727, SAO 253945, HD 158094, GC 23681, HR 6500, DM CP-60  6842, TYC 9053-4118-1",
	"group" : { "key" : "Ara" },
	"Common" : "Delta Arae",
	"OType" : "Star",
	"Distance" : "60.65",
	"RA_S" : 262.77461993,
	"DEC_S" : -60.68384975,
	"X" : 434,
	"Y" : 337,
	"Constellation" : "Ara ",
	"AMag" : 3.563,
	"key" : 87720,
	"title" : "Delta Arae"
	},
{
	"Index" : "60639",
	"Description" : "Alpha Arae (\u03B1 Arae, \u03B1 Ara) is the second brightest star in the southern constellation of Ara. With an average apparent visual magnitude 2.93, it is readily visible to the naked eye from the southern hemisphere. This star is close enough to the Earth that its distance can be estimated using parallax data collected during the Hipparcos mission. It is around 270 light-years (83 parsecs) away, with a 7% margin of error. The visual magnitude of the star is diminished by 0.10 magnitudes as a result of extinction from intervening gas and dust.\r\rAlpha Arae has a stellar classification of B2 Vne, indicating that it is a massive B-type main sequence star. The \u0027n\u0027 notation in the suffix indicates that the absorption lines in the star\u0027s spectrum appear spread out and nebulous because of the Doppler effect from rapid rotation. The measured projected rotational velocity has been measured as high as 375 km s\u20131. Meilland et al. (2007) estimate the pole of the star is inclined by 55\u00B0 to the line of sight, yielding an equatorial azimuthal velocity of 470 km s\u20131. This is close to the critical velocity where the star would start to breakup. The rapid rotation is causing a pronounced equatorial bulge of about 2.4\u20132.7 times the polar radius.\r\rIt is a Be star, as indicated by the \u0027e\u0027 notation in the star\u0027s classification. This indicates that emission lines are observed in the spectrum, which is coming from a disk of material ejected from the star because of its rapid rotation. In 2003 and 2005, Alpha Arae was observed by infrared interferometry, using the MIDI and AMBER instruments at the VLT Interferometer. The results, published in 2005 and 2007, appear to show that Alpha Arae is surrounded by a dense equatorial disk of material in Keplerian (rather than uniform) rotation, and that it is losing mass by a polar stellar wind with a terminal velocity of approximately 1,000 km/s. There is also some evidence that Alpha Arae is orbited by a companion at 0.7 AU.\r\rThis star has around 9.6 times as much mass as the Sun and an average of 4.5 times the Sun\u0027s radius. It is emitting 5,800 as much luminosity as the Sun from its outer envelope at an effective temperature of 18,044 K. This heat gives Alpha Arae the blue-white hue that is characteristic of B-type stars. It is a variable star with a magnitude that varies between 2.76m and 2.90m.\r\rAlpha Arae has a visual companion star, CCDM J17318-4953B, located approximately 50 arcseconds away along a position angle of 168\u00B0, with an apparent visual magnitude of about 11. The two stars appear close to each other by coincidence and are not physically close in space.\r\rWith \u03B2 and \u03C3 Ara it forms the Chinese asterism Choo \uFF08pinyin: ch\u01D4, \u6775\uFF09, \u0022pestle\u0022 in traditional Chinese astronomy. It was the second star of Choo \uFF08\u6775\u4E8C\uFF09, but R. H. Allen used the name Choo for this star only. Patrick Moore lists Choo as a proper name for this star in his star catalogue of the constellation Ara. This name is also spelt Tchou. There is another Choo in the constellation Pegasus.\r\rIn Chinese, \u6775 (Ch\u01D4), meaning Pestle, refers to an asterism consisting of \u03B1 Arae, \u03C3 Arae and \u03B2 Arae. Consequently, \u03B1 Arae itself is known as \u6775\u4E8C (Ch\u01D4 \u00E8r, English: the Second Star of Pestle.)",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Alpha Arae, HIP 85792, SAO 228069, HD 158427, GC 23708, HR 6510, DM CD-49 11511, TYC 8350-2600-1",
	"group" : { "key" : "Ara" },
	"Common" : "Alpha Arae",
	"OType" : "Be Star",
	"Distance" : "81.49",
	"RA_S" : 262.96037889,
	"DEC_S" : -49.87614279,
	"X" : 473,
	"Y" : 202,
	"Constellation" : "Ara ",
	"AMag" : 2.793,
	"key" : 80639,
	"title" : "Alpha Arae"
	},
{
	"Index" : "60549",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "1 Arae, Sigma Arae, HIP 86092, SAO 228162, HD 159217, GC 23815, HR 6537, DM CD-46 11661, TYC 8342-6346-1",
	"group" : { "key" : "Ara" },
	"Common" : "Sigma Arae",
	"OType" : "Star",
	"Distance" : "115.88",
	"RA_S" : 263.91496645,
	"DEC_S" : -46.50568316,
	"Constellation" : "Ara ",
	"AMag" : 4.561,
	"key" : 80549,
	"title" : "Sigma Arae"
	},
{
	"Index" : "64517",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Pi Arae, HIP 86305, SAO 244896, HD 159492, GC 23862, HR 6549, DM CP-54  8403, TYC 8733-2365-1",
	"group" : { "key" : "Ara" },
	"Common" : "Pi Arae",
	"OType" : "High proper-motion Star",
	"Distance" : "44.56",
	"RA_S" : 264.52298366,
	"DEC_S" : -54.50043304,
	"Constellation" : "Ara ",
	"AMag" : 5.267,
	"key" : 84517,
	"title" : "Pi Arae"
	},
{
	"Index" : "60650",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Lambda Arae, HIP 86486, SAO 228257, HD 160032, GC 23918, HR 6569, DM CD-49 11616, TYC 8351-2577-1",
	"group" : { "key" : "Ara" },
	"Common" : "Lambda Arae",
	"OType" : "Variable Star",
	"Distance" : "21.45",
	"RA_S" : 265.09928159,
	"DEC_S" : -49.41558601,
	"Constellation" : "Ara ",
	"AMag" : 4.799,
	"key" : 80650,
	"title" : "Lambda Arae"
	},
{
	"Index" : "60691",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Mu Arae, HIP 86796, SAO 244981, HD 160691, GC 24024, HR 6585, DM CD-51 11094, TYC 8355-436-1",
	"group" : { "key" : "Ara" },
	"Common" : "Mu Arae",
	"OType" : "High proper-motion Star",
	"Distance" : "15.51",
	"RA_S" : 266.03626987,
	"DEC_S" : -51.83405661,
	"Constellation" : "Ara ",
	"AMag" : 5.197,
	"key" : 80691,
	"title" : "Mu Arae"
	},
{
	"Index" : "60792",
	"Description" : "Theta Arae (\u03B8 Ara, \u03B8 Arae) is the Bayer designation for a star in the constellation Ara. It has an apparent visual magnitude of +3.67, which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 4.01 mas, Theta Arae is 810 light-years (250 parsecs) distant from the Earth.\r\rThis is a supergiant star with a stellar classification of B2 Ib. It has nearly nine times the mass of the Sun and is over 20 times the Sun\u0027s radius. The outer atmosphere of this star has an effective temperature of 17,231 K; much hotter than the surface of the Sun. At this heat, the star shines with the characteristic blue-white hue of a B-type star.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Theta Arae, HIP 88714, SAO 245242, HD 165024, GC 24635, HR 6743, DM CD-50 11720, TYC 8365-1698-1",
	"group" : { "key" : "Ara" },
	"Common" : "Theta Arae",
	"OType" : "Star",
	"Distance" : "248.96",
	"RA_S" : 271.65780026,
	"DEC_S" : -50.09148467,
	"X" : 401,
	"Y" : 187,
	"Constellation" : "Ara ",
	"AMag" : 3.635,
	"key" : 80792,
	"title" : "Theta Arae"
	},
{
	"Index" : "1687",
	"Description" : "Gamma Arietis (\u03B3 Ari, \u03B3 Arietis) is the Bayer designation for a binary star system in the northern constellation of Aries. It has the traditional name Mesarthim, which is of obscure origin. The combined apparent visual magnitude of the two stars is 3.86, which is readily visible to the naked eye and makes this the fourth brightest member of Aries. Based upon an annual parallax shift of 19.88 mas, the distance to Gamma Arietis is approximately 164 light-years (50 parsecs).\r\rThe double star nature of this system was discovered by Robert Hooke in 1664. The two components have an angular separation of 7.606 arcseconds, which can be resolved with a small telescope. The orbital period of the pair is greater than 5000 years. The brighter component, \u03B3\u00B9 Arietis, is a magnitude 4.58 B-type main sequence star with a stellar classification of B9 V. The secondary, \u03B3\u00B2 Arietis, is a Lambda Bootis (chemically peculiar) star with a stellar classification of A1p Si and a magnitude of 4.64. It is classified as an \u03B12 CVn type variable star and its brightness varies by 0.04 magnitudes with a period of 2.61 days.\r\rIt has the traditional name Mesarthim, of obscure origin, and has been called \u0022the First Star in Aries\u0022 as having been at one time the nearest visible star to the equinoctial point. The name Mesarthim may be from the Hebrew word m\u1D4Bsh\u0101r\u1D4Bt\u012Bm, meaning \u0022the minister\u0022, or the Arabic word Al Muthartim (\u0623\u0644\u0645\u062B\u0631\u062A\u0645), meaning \u0022the ram\u0022.The meaning \u0022servants\u0022 has also been suggested.\r\rIn Chinese, \u5A41\u5BBF (L\u00F3us\u00F9), meaning Bond (asterism), refers to an asterism consisting of \u03B3 Arietis, \u03B2 Arietis and \u03B1 Arietis. Consequently, \u03B1 Arietis itself is known as \u5A41\u5BBF\u4E8C (L\u00F3us\u00F9 \u00C8r, English: the Second Star of Bond.)\r\rIn Hindu astrology, Beta Arietis (Sheratan) and Gamma Arieties (Mesartim) are Ashwinis, the twin gods who act as doctors of the divine of the world.(Richard H Allen)",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "5 Arietis, Gamma02 Arietis, HIP 8832A, SAO 92681, HD 11503, GC 2291, HR 545, DM BD+18   243A, TYC 1209-1835-1",
	"group" : { "backgroundImage" : "images/Alignment/07.png",
		"description" : "Aries is one of the constellations of the zodiac, the groups of stars through which the apparent course of the sun passes during the year. It is located in the Northern Hemisphere between Pisces to the west and Taurus to the east. The name Aries is Latin for ram, and its symbol is \u2648, representing a ram\u0027s horns. It is one of the 48 constellations described by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is a mid-sized constellation, ranking 39th overall size, with an area of 441 square degrees (1.1% of the celestial sphere).\r\rAlthough Aries came to represent specifically the ram whose fleece became the Golden Fleece of Ancient Greek mythology, it has represented a ram since late Babylonian times. Before that, the stars of Aries formed a farmhand. Different cultures have incorporated the stars of Aries into different constellations including twin inspectors in China and a porpoise in the Marshall Islands. Aries is a relatively dim constellation, possessing only four bright stars: Hamal (Alpha Arietis, second magnitude), Sheratan (Beta Arietis, third magnitude), Mesartim (Gamma Arietis, fourth magnitude), and 41 Arietis (also fourth magnitude). The few deep-sky objects within the constellation are quite faint and include several pairs of interacting galaxies. Several meteor showers appear to radiate from Aries, including the Daytime Arietids and the Epsilon Arietids.\r\rAries is now recognized as an official constellation, albeit as a specific region of the sky, by the International Astronomical Union. It was originally defined in ancient texts as a specific pattern of stars, and has remained a constellation since ancient times; it now includes the ancient pattern as well as the surrounding stars. In the description of the Babylonian zodiac given in the clay tablets known as the MUL.APIN, the constellation now known as Aries was the final station along the ecliptic. The MUL.APIN was a comprehensive table of the risings and settings of stars, which likely served as an agricultural calendar. Modern-day Aries was known as MULL\u00DA.\u1E2AUN.G\u00C1, \u0022The Agrarian Worker\u0022 or \u0022The Hired Man\u0022. Although likely compiled in the 12th or 11th century BCE, the MUL.APIN reflects a tradition which marks the Pleiades as the vernal equinox, which was the case with some precision at the beginning of the Middle Bronze Age. The earliest identifiable reference to Aries as a distinct constellation comes from the boundary stones that date from 1350 to 1000 BCE. On several boundary stones, a zodiacal ram figure is distinct from the other characters present. The shift in identification from the constellation as the Agrarian Worker to the Ram likely occurred in later Babylonian tradition because of its growing association with Dumuzi the Shepherd. By the time the MUL.APIN was created\u2014by 1000 BCE\u2014modern Aries was identified with both Dumuzi\u0027s ram and a hired laborer. The exact timing of this shift is difficult to determine due to the lack of images of Aries or other ram figures.\r\rIn ancient Egyptian astronomy, Aries was associated with the god Amon-Ra, who was depicted as a man with a ram\u0027s head and represented fertility and creativity. Because it was the location of the vernal equinox, it was called the \u0022Indicator of the Reborn Sun\u0022. During the times of the year when Aries was prominent, priests would process statues of Amon-Ra to temples, a practice that was modified by Persian astronomers centuries later. Aries acquired the title of \u0022Lord of the Head\u0022 in Egypt, referring to its symbolic and mythological importance.\r\rAries was not fully accepted as a constellation until classical times. In Hellenistic astrology, the constellation of Aries is associated with the golden ram of Greek mythology that rescued Phrixos and Helle on orders from Hermes, taking him to the land of Colchis. Phrixos and Helle were the son and daughter of King Athamas and his first wife Nephele. The king\u0027s second wife, Ino, was jealous and wished to kill his children. To accomplish this, she induced a famine in Boeotia, then falsified a message from the Oracle of Delphi that said Phrixos must be sacrificed to end the famine. Athamas was about to sacrifice his son atop Mount Laphystium when Aries, sent by Nephele, arrived. Helle fell off of Aries\u0027s back in flight and drowned in the Dardanelles, also called the Hellespont in her honor. After arriving, Phrixos sacrificed the ram to Zeus and gave the Fleece to Ae\u00EBtes of Colchis, who rewarded him with an engagement to his daughter Chalciope. Ae\u00EBtes hung its skin in a sacred place where it became known as the Golden Fleece and was guarded by a dragon. In a later myth, this Golden Fleece was stolen by Jason and the Argonauts.\r\rHistorically, Aries has been depicted as a crouched, wingless ram with its head turned towards Taurus. Ptolemy asserted in his Almagest that Hipparchus depicted Alpha Arietis as the ram\u0027s muzzle, though Ptolemy did not include it in his constellation figure. Instead, it was listed as an \u0022unformed star\u0022, and denoted as \u0022the star over the head\u0022. John Flamsteed, in his Atlas Coelestis, followed Ptolemy\u0027s description by mapping it above the figure\u0027s head. Flamsteed followed the general convention of maps by depicting Aries laying down. Astrologically, Aries has been associated with the head and its humors. It was strongly associated with Mars, both the planet and the god. It was considered to govern Western Europe and Syria, and to indicate a strong temper in a person.\r\rThe First Point of Aries, the location of the vernal equinox, is named for the constellation. This is because the Sun crossed the celestial equator from south to north in Aries more than two millennia ago. Hipparchus defined it in 130 BCE. as a point south of Gamma Arietis. Because of the precession of the equinoxes, the First Point of Aries has since moved into Pisces and will move into Aquarius by around 2600 CE. The Sun now appears in Aries from late April through mid May, though the constellation is still associated with the beginning of spring.\r\rMedieval Muslim astronomers depicted Aries in various ways. Astronomers like al-Sufi saw the constellation as a ram, modeled on the precedent of Ptolemy. However, some Islamic celestial globes depicted Aries as a nondescript four-legged animal with what may be antlers instead of horns. Some early Bedouin observers saw a ram elsewhere in the sky; this constellation featured the Pleiades as the ram\u0027s tail. The generally accepted Arabic formation of Aries consisted of thirteen stars in a figure along with five \u0022unformed\u0022 stars, four of which were over the animal\u0027s hindquarters and one of which was the disputed star over Aries\u0027s head. Al-Sufi\u0027s depiction differed from both other Arab astronomers\u0027 and Flamsteed\u0027s, in that his Aries was running and looking behind itself.\r\rThe obsolete constellations introduced in Aries (Musca Borealis, Vespa, and Apis) have all been composed of the northern stars. Musca Borealis was created from the stars 33 Arietis, 35 Arietis, 39 Arietis, and 41 Arietis. In 1612, Petrus Plancius introduced Apis, a constellation representing a bee. In 1624, the same stars were used by Jakob Bartsch to create a constellation called Vespa, representing a wasp. Neither constellation became widely accepted. Johann Hevelius renamed the constellation \u0022Musca\u0022 in 1690 in his Firmamentum Sobiescianum. To differentiate it from Musca, the southern fly, it was later renamed Musca Borealis but it did not gain acceptance and its stars were ultimately officially reabsorbed into Aries.\r\rIn 1922, the International Astronomical Union defined its recommended three-letter abbreviation, \u0022Ari\u0022. The official boundaries of Aries were defined in 1930 by Eug\u00E8ne Delporte as a polygon of 12 segments. Its right ascension is between 1h 46.4m and 3h 29.4m and its declination is between 10.36\u00B0 and 31.22\u00B0 in the equatorial coordinate system.",
		"key" : "Aries",
		"grouptype" : "Aries",
		"Meaning" : "ram",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Aries",
		"title" : "Aries Objects Group" },
	"Common" : "Mesarthim",
	"OType" : "Star",
	"Distance" : "62.44",
	"RA_S" : 28.382367,
	"DEC_S" : 19.294078,
	"X" : 561,
	"Y" : 523,
	"Constellation" : "Aries ",
	"AMag" : 4.517,
	"key" : 21687,
	"title" : "Mesarthim"
	},
{
	"Index" : "1686",
	"Description" : "Gamma Arietis (\u03B3 Ari, \u03B3 Arietis) is the Bayer designation for a binary star system in the northern constellation of Aries. It has the traditional name Mesarthim, which is of obscure origin. The combined apparent visual magnitude of the two stars is 3.86, which is readily visible to the naked eye and makes this the fourth brightest member of Aries. Based upon an annual parallax shift of 19.88 mas, the distance to Gamma Arietis is approximately 164 light-years (50 parsecs).\r\rThe double star nature of this system was discovered by Robert Hooke in 1664. The two components have an angular separation of 7.606 arcseconds, which can be resolved with a small telescope. The orbital period of the pair is greater than 5000 years. The brighter component, \u03B3\u00B9 Arietis, is a magnitude 4.58 B-type main sequence star with a stellar classification of B9 V. The secondary, \u03B3\u00B2 Arietis, is a Lambda Bootis (chemically peculiar) star with a stellar classification of A1p Si and a magnitude of 4.64. It is classified as an \u03B12 CVn type variable star and its brightness varies by 0.04 magnitudes with a period of 2.61 days.\r\rIt has the traditional name Mesarthim, of obscure origin, and has been called \u0022the First Star in Aries\u0022 as having been at one time the nearest visible star to the equinoctial point. The name Mesarthim may be from the Hebrew word m\u1D4Bsh\u0101r\u1D4Bt\u012Bm, meaning \u0022the minister\u0022, or the Arabic word Al Muthartim (\u0623\u0644\u0645\u062B\u0631\u062A\u0645), meaning \u0022the ram\u0022.The meaning \u0022servants\u0022 has also been suggested.\r\rIn Chinese, \u5A41\u5BBF (L\u00F3us\u00F9), meaning Bond (asterism), refers to an asterism consisting of \u03B3 Arietis, \u03B2 Arietis and \u03B1 Arietis. Consequently, \u03B1 Arietis itself is known as \u5A41\u5BBF\u4E8C (L\u00F3us\u00F9 \u00C8r, English: the Second Star of Bond.)\r\rIn Hindu astrology, Beta Arietis (Sheratan) and Gamma Arieties (Mesartim) are Ashwinis, the twin gods who act as doctors of the divine of the world.(Richard H Allen)",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "5 Arietis, Gamma01 Arietis, HIP 8832B, SAO 92680, HD 11502, GC 2290, HR 546, DM BD+18   243B, TYC 1209-1833-1",
	"group" : { "key" : "Aries" },
	"Common" : "Mesarthim",
	"OType" : "Star",
	"Distance" : "62.44",
	"RA_S" : 28.382383,
	"DEC_S" : 19.296186,
	"X" : 561,
	"Y" : 523,
	"Constellation" : "Aries ",
	"AMag" : 4.584,
	"key" : 21686,
	"shortTitle" : "Mesartim; \"First Star in Aries\"; Mezartim; Mesartkhim",
	"title" : "Mesarthim"
	},
{
	"Index" : "1715",
	"Description" : "Beta Arietis (\u03B2 Ari, \u03B2 Arietis) is a binary star system in the constellation Aries, marking the Ram\u0027s second horn. It has the traditional name Sheratan (or Sharatan, Sheratim), and the Flamsteed designation 6 Arietis. The traditional name, in full Al Sharatan, is from the Arabic \u0627\u0644\u0634\u0631\u0627\u0637\u0627\u0646 a\u0161-\u0161ar\u0101\u0163\u0101n \u0022the two signs\u0022, a reference to the star having marked the northern vernal equinox together with Gamma Arietis several thousand years ago.\r\rIn Chinese, \u5A41\u5BBF (L\u00F3u Su), meaning Bond (asterism), refers to an asterism consisting of \u03B2 Arietis, \u03B3 Arietis and \u03B1 Arietis. Consequently, \u03B2 Arietis itself is known as \u5A41\u5BBF\u4E00 (L\u00F3u Su y\u012B, English: the First Star of Bond).\r\rBeta Arietis has an apparent visual magnitude of 2.66. Based on parallax measurements, it is located at a distance of 59.6 light-years (18.3 parsecs) from Earth. This is a spectroscopic binary star system consisting of a pair of stars orbiting around each other with a separation that can not currently be resolved with a conventional telescope. However, the pair have been resolved using the Mark III Stellar Interferometer at the Mount Wilson Observatory. This allows the orbital elements to be computed, as well as the individual masses of the two stars. The stars complete their highly elliptical orbit every 107 days.\r\rThe primary star has a stellar classification of A5 V, which means it is an A-type main sequence star that is generating energy through the thermonuclear fusion of hydrogen in its core region. The NStars project gives the star an spectral type of kA4 hA5 mA5 Va under the revised MK spectral classification system. The spectrum of the secondary star has not been determined, but, based on the mass, it may have a stellar classification of F5 III\u2013V or G0 V. It is about four magnitudes fainter than the primary; hence the energy output from the system is dominated by the primary star. In a few million years, as the primary evolves toward a red giant, significant amounts of mass transfer to the secondary component is expected.\r\rThe primary has been classified as a rapid rotator, with a projected rotational velocity of 73 km/s providing a lower bound on the azimuthal rotational velocity along the equator. It may also be a mildly Am star, which is a class of stars that show a peculiar spectrum with strong absorption lines from various elements and deficiencies in others. In \u03B2 Arietis, these absorption lines are broadened because of the Doppler effect from the rotation, making analysis of the abundance patterns difficult.\r\rThis system has been examined with the Spitzer Space Telescope for the presence of an excess emission of infrared, which would indicate a disk of dust. However, no significant excess was detected.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "6 Arietis, Beta Arietis, HIP 8903, SAO 75012, HD 11636, GC 2309, HR 553, DM BD+20   306, TYC 1212-1935-1",
	"group" : { "key" : "Aries" },
	"Common" : "Sheratan",
	"OType" : "Spectroscopic binary",
	"Distance" : "17.98",
	"RA_S" : 28.66004579,
	"DEC_S" : 20.80803147,
	"X" : 554,
	"Y" : 504,
	"Constellation" : "Aries ",
	"AMag" : 2.651,
	"key" : 21715,
	"shortTitle" : "Sharatan; Al Sharatain",
	"title" : "Sheratan"
	},
{
	"Index" : "1697",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "8 Arietis, Iota Arietis, HIP 9110, SAO 92721, HD 11909, GC 2347, HR 563, DM BD+17   289, TYC 1210-1641-1",
	"group" : { "key" : "Aries" },
	"Common" : "Iota Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "158.96",
	"RA_S" : 29.33772753,
	"DEC_S" : 17.81753216,
	"Constellation" : "Aries ",
	"AMag" : 5.206,
	"key" : 21697,
	"title" : "Iota Arietis"
	},
{
	"Index" : "6364",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "9 Arietis, Lambda Arietis, HIP 9153, SAO 75051, HD 11973, GC 2366, HR 569, DM BD+22   288, TYC 1757-1964-1",
	"group" : { "key" : "Aries" },
	"Common" : "Lambda Arietis",
	"OType" : "Star",
	"Distance" : "39.49",
	"RA_S" : 29.48215334,
	"DEC_S" : 23.59606343,
	"Constellation" : "Aries ",
	"AMag" : 4.802,
	"key" : 26364,
	"title" : "Lambda Arietis"
	},
{
	"Index" : "6380",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "12 Arietis, Kappa Arietis, HIP 9836, SAO 75146, HD 12869, GC 2527, HR 613, DM BD+21   279, TYC 1758-2417-1",
	"group" : { "key" : "Aries" },
	"Common" : "Kappa Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "55.65",
	"RA_S" : 31.64135479,
	"DEC_S" : 22.64831392,
	"Constellation" : "Aries ",
	"AMag" : 5.038,
	"key" : 26380,
	"title" : "Kappa Arietis"
	},
{
	"Index" : "6406",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "14 Arietis, HIP 10053, SAO 75171, HD 13174, GC 2573, HR 623, DM BD+25   355, TYC 1761-2536-1",
	"group" : { "key" : "Aries" },
	"Common" : "14 Arietis",
	"OType" : "Star",
	"Distance" : "97.12",
	"RA_S" : 32.35555726,
	"DEC_S" : 25.9398814,
	"Constellation" : "Aries ",
	"AMag" : 5.019,
	"key" : 26406,
	"title" : "14 Arietis"
	},
{
	"Index" : "1764",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "17 Arietis, Eta Arietis, HIP 10306, SAO 75204, HD 13555, GC 2643, HR 646, DM BD+20   348, TYC 1220-1929-1",
	"group" : { "key" : "Aries" },
	"Common" : "Eta Arietis",
	"OType" : "High proper-motion Star",
	"Distance" : "28.87",
	"RA_S" : 33.20035288,
	"DEC_S" : 21.21099295,
	"Constellation" : "Aries ",
	"AMag" : 5.278,
	"key" : 21764,
	"title" : "Eta Arietis"
	},
{
	"Index" : "43686",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "24 Arietis, Xi Arietis, HIP 11249, SAO 92932, HD 14951, GC 2901, HR 702, DM BD+09   316, TYC 635-692-1",
	"group" : { "key" : "Aries" },
	"Common" : "Xi Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "265.46",
	"RA_S" : 36.20440239,
	"DEC_S" : 10.61056223,
	"Constellation" : "Aries ",
	"AMag" : 5.461,
	"key" : 63686,
	"title" : "Xi Arietis"
	},
{
	"Index" : "1777",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "32 Arietis, Nu Arietis, HIP 12332, SAO 75495, HD 16432, GC 3167, HR 773, DM BD+21   362, TYC 1222-2067-1",
	"group" : { "key" : "Aries" },
	"Common" : "Nu Arietis",
	"OType" : "Star",
	"Distance" : "102.55",
	"RA_S" : 39.70414727,
	"DEC_S" : 21.96140783,
	"Constellation" : "Aries ",
	"AMag" : 5.472,
	"key" : 21777,
	"title" : "Nu Arietis"
	},
{
	"Index" : "6503",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "33 Arietis, HIP 12489, SAO 75510, HD 16628, GC 3215, HR 782, DM BD+26   443, TYC 1776-1396-1",
	"group" : { "key" : "Aries" },
	"Common" : "33 Arietis",
	"OType" : "High proper-motion Star",
	"Distance" : "70.93",
	"RA_S" : 40.17114703,
	"DEC_S" : 27.06094247,
	"Constellation" : "Aries ",
	"AMag" : 5.307,
	"key" : 26503,
	"title" : "33 Arietis"
	},
{
	"Index" : "6502",
	"Description" : "35 Arietis is the Flamsteed designation for a binary star in the northern constellation of Aries. It is approximately 340 light-years (100 parsecs) distant from the Earth, based upon an annual parallax shift of 9.51 mas. This star is visible to the naked eye with an apparent visual magnitude of 4.64.\r\rThis is a single-lined spectroscopic binary system, with the presence of a companion being demonstrated by shifts in the spectrum of the primary component. The pair orbit each other with a period of 490.0 days and an eccentricity of 0.14. The primary is a B-type main-sequence star with a stellar classification of B3 V. With a mass around 5.7 times that of the Sun, it is radiating 870 times the Sun\u0027s luminosity. This energy is being emitted from the outer atmosphere at an effective temperature of 17,520 K, causing it to shine with the blue-white hue of a B-type star.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "35 Arietis, HIP 12719, SAO 75532, HD 16908, GC 3273, HR 801, DM BD+27   424, TYC 1776-1395-1",
	"group" : { "key" : "Aries" },
	"Common" : "35 Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.15",
	"RA_S" : 40.86298401,
	"DEC_S" : 27.70715021,
	"X" : 395,
	"Y" : 439,
	"Constellation" : "Aries ",
	"AMag" : 4.624,
	"key" : 26502,
	"title" : "35 Arietis"
	},
{
	"Index" : "44377",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "38 Arietis, HIP 12832, SAO 93083, HD 17093, GC 3308, HR 812, DM BD+11   377, TYC 643-936-1",
	"group" : { "key" : "Aries" },
	"Common" : "38 Arietis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "36.33",
	"RA_S" : 41.23991955,
	"DEC_S" : 12.44576007,
	"Constellation" : "Aries ",
	"AMag" : 5.205,
	"key" : 64377,
	"title" : "38 Arietis"
	},
{
	"Index" : "6610",
	"Description" : "39 Arietis is the Flamsteed designation for a star in the northern constellation of Aries. It is visible to the naked eye with an apparent visual magnitude of +4.5. The distance to this star, as determined from an annual parallax shift of 19.01 mas, is approximately 172 light-years (53 parsecs).\r\rThis is a giant star with a stellar classification of K1.5 III. It is currently at an evolutionary stage known as a red clump, indicating that it is generating energy through the fusion of helium at its core. 39 Arietis has 1.6 times the mass of the Sun, but its outer envelope has expanded to around 11 times the Sun\u0027s radius. It shines with 56 times the luminosity of the Sun. This energy is being radiated into outer space from its outer atmosphere at an effective temperature of 4,603 K, giving it the cool orange-hued glow of a K-type star.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "39 Arietis, HIP 13061, SAO 75578, HD 17361, GC 3356, HR 824, DM BD+28   462, TYC 1793-1611-1",
	"group" : { "key" : "Aries" },
	"Common" : "39 Arietis",
	"OType" : "High proper-motion Star",
	"Distance" : "52.6",
	"RA_S" : 41.97725417,
	"DEC_S" : 29.2471177,
	"X" : 381,
	"Y" : 421,
	"Constellation" : "Aries ",
	"AMag" : 4.639,
	"key" : 26610,
	"title" : "39 Arietis"
	},
{
	"Index" : "1791",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "42 Arietis, Pi Arietis, HIP 13165A, SAO 93127, HD 17543, GC 3378, HR 836, DM BD+16   355, TYC 1223-1987-1",
	"group" : { "key" : "Aries" },
	"Common" : "Pi Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "231.66",
	"RA_S" : 42.32316341,
	"DEC_S" : 17.46431255,
	"Constellation" : "Aries ",
	"AMag" : 5.321,
	"key" : 21791,
	"title" : "Pi Arietis"
	},
{
	"Index" : "1794",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "42 Arietis, Pi Arietis, HIP 13165B, SAO 93127, HD 17543, GC 3378, HR 836, DM BD+16   355, TYC 1223-1990-1",
	"group" : { "key" : "Aries" },
	"Common" : "Pi Arietis",
	"OType" : "Spectroscopic binary",
	"Distance" : "231.66",
	"RA_S" : 42.32316349,
	"DEC_S" : 17.46431022,
	"Constellation" : "Aries ",
	"AMag" : 5.26,
	"key" : 21794,
	"title" : "Pi Arietis"
	},
{
	"Index" : "6582",
	"Description" : "41 Arietis or c Arietis is the Flamsteed designation for a binary star in the northern constellation of Aries. It does not possess a Greek letter Bayer designation, since this star was once part of the now-obsolete constellation Musca Borealis, but is sometimes designated c Arietis. With an apparent visual magnitude of 3.63, this star is readily visible to the naked eye. It has an annual parallax shift of 19.69 mas, which indicates the distance to this star is 166 light-years (51 parsecs). \r\rThe primary component is a B-type main sequence star with a stellar classification of B8 Vn. The suffix \u0027n\u0027 indicates \u0027nebulous\u0027 absorption lines in the star\u0027s spectrum caused by the Doppler effect of rapid rotation. It has a projected rotational velocity of 175 km/s. This is creating an equatorial bulge that is 12% large than the star\u0027s polar radius. It is a candidate member of the AB Doradus moving group and has an orbiting companion at an angular separation of 0.3 arcseconds.\r\r41 Ari is part of the Bharani lunar mansion in Hindu astrology. In Chinese, \u80C3\u5BBF (W\u00E8i Su), meaning Stomach (asterism), refers to an asterism consisting of 41 Arietis, 35 Arietis and 39 Arietis. Consequently, 41 Arietis itself is known as \u80C3\u5BBF\u4E09 (W\u00E8i Su s\u0101n, English: the Third Star of Stomach.)",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "41 Arietis, c Arietis, HIP 13209, SAO 75596, HD 17573, GC 3391, HR 838, DM BD+26   471, TYC 1789-1490-1",
	"group" : { "key" : "Aries" },
	"Common" : "41 Arietis",
	"OType" : "Double or multiple star",
	"Distance" : "50.78",
	"RA_S" : 42.49597556,
	"DEC_S" : 27.26050911,
	"X" : 377,
	"Y" : 447,
	"Constellation" : "Aries ",
	"AMag" : 3.579,
	"key" : 26582,
	"title" : "41 Arietis"
	},
{
	"Index" : "1803",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "43 Arietis, Sigma Arietis, HIP 13327, SAO 93144, HD 17769, GC 3427, HR 847, DM BD+14   480, TYC 1224-1521-1",
	"group" : { "key" : "Aries" },
	"Common" : "Sigma Arietis",
	"OType" : "Star",
	"Distance" : "151.09",
	"RA_S" : 42.87327474,
	"DEC_S" : 15.08206937,
	"Constellation" : "Aries ",
	"AMag" : 5.499,
	"key" : 21803,
	"title" : "Sigma Arietis"
	},
{
	"Index" : "1857",
	"Description" : "Epsilon Arietis (\u03B5 Ari, \u03B5 Arietis) is the Bayer designation for a visual binary star system in the northern constellation of Aries. It has a combined apparent visual magnitude of 4.63 and can be seen with the naked eye, although the two components are too close together to be resolved without a telescope. With an annual parallax shift of 9.81 mas, the distance to this system can be estimated as 330 light-years (100 parsecs), give or take a 30 light-year margin of error.\r\rThe brighter member of this pair has an apparent magnitude of 5.2. At an angular separation of 1.426 \u00B1 0.010 arcseconds from the brighter component, along a position angle of 209.2\u00B0 \u00B1 0.3\u00B0, is the magnitude 5.5 companion. Both are A-type main sequence stars with a stellar classification of A2 Vs. (The \u0027s\u0027 suffix indicates that the absorption lines in the spectrum are distinctly narrow.) In the 2009 Catalogue of Ap, HgMn and Am stars, the two stars have a classification of A3 Ti, indicating they are Ap stars with an anomalous abundance of titanium. Within the measurement margin of error, their projected rotational velocities are deemed identical at 60 km/s.\r\rThis star system, along with \u03B4 Ari, \u03B6 Ari, \u03C0 Ari, and \u03C13 Ari, were Al B\u012Br\u016Bn\u012B\u0027s Al Bu\u1E6Dain (\u0623\u0644\u0628\u0637\u064A\u0646), the dual of Al Ba\u1E6Dn, the Belly. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Bu\u1E6Dain were the title for five stars :\u03B4 Ari as Botein, \u03C0 Ari as Al Bu\u1E6Dain I, \u03C13 Ari as Al Bu\u1E6Dain II, \u03B5 Ari as Al Bu\u1E6Dain III dan \u03B6 Ari as Al Bu\u1E6Dain IV",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "48 Arietis, Epsilon Arietis, HIP 13914B, SAO 75673, HD 18519, GC 3582, HR 887, DM BD+20   484A, TYC 1230-1424-2",
	"group" : { "key" : "Aries" },
	"Common" : "Epsilon Arietis",
	"OType" : "Star",
	"Distance" : "101.15",
	"RA_S" : 44.80296185,
	"DEC_S" : 21.34030518,
	"X" : 354,
	"Y" : 525,
	"Constellation" : "Aries ",
	"AMag" : 5.566,
	"key" : 21857,
	"title" : "Epsilon Arietis"
	},
{
	"Index" : "1856",
	"Description" : "Epsilon Arietis (\u03B5 Ari, \u03B5 Arietis) is the Bayer designation for a visual binary star system in the northern constellation of Aries. It has a combined apparent visual magnitude of 4.63 and can be seen with the naked eye, although the two components are too close together to be resolved without a telescope. With an annual parallax shift of 9.81 mas, the distance to this system can be estimated as 330 light-years (100 parsecs), give or take a 30 light-year margin of error.\r\rThe brighter member of this pair has an apparent magnitude of 5.2. At an angular separation of 1.426 \u00B1 0.010 arcseconds from the brighter component, along a position angle of 209.2\u00B0 \u00B1 0.3\u00B0, is the magnitude 5.5 companion. Both are A-type main sequence stars with a stellar classification of A2 Vs. (The \u0027s\u0027 suffix indicates that the absorption lines in the spectrum are distinctly narrow.) In the 2009 Catalogue of Ap, HgMn and Am stars, the two stars have a classification of A3 Ti, indicating they are Ap stars with an anomalous abundance of titanium. Within the measurement margin of error, their projected rotational velocities are deemed identical at 60 km/s.\r\rThis star system, along with \u03B4 Ari, \u03B6 Ari, \u03C0 Ari, and \u03C13 Ari, were Al B\u012Br\u016Bn\u012B\u0027s Al Bu\u1E6Dain (\u0623\u0644\u0628\u0637\u064A\u0646), the dual of Al Ba\u1E6Dn, the Belly. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Bu\u1E6Dain were the title for five stars :\u03B4 Ari as Botein, \u03C0 Ari as Al Bu\u1E6Dain I, \u03C13 Ari as Al Bu\u1E6Dain II, \u03B5 Ari as Al Bu\u1E6Dain III dan \u03B6 Ari as Al Bu\u1E6Dain IV",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "48 Arietis, Epsilon Arietis, HIP 13914A, SAO 75673, HD 18520, GC 3582, HR 888, DM BD+20   484B, TYC 1230-1424-1",
	"group" : { "key" : "Aries" },
	"Common" : "Epsilon Arietis",
	"OType" : "Star",
	"Distance" : "101.15",
	"RA_S" : 44.80296185,
	"DEC_S" : 21.34030518,
	"X" : 354,
	"Y" : 525,
	"Constellation" : "Aries ",
	"AMag" : 5.169,
	"key" : 21856,
	"title" : "Epsilon Arietis"
	},
{
	"Index" : "6568",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "52 Arietis, HIP 14376AB, SAO 75723, HD 19134, GC 3697, HR 927, DM BD+24   431A, TYC 1787-1187-1",
	"group" : { "key" : "Aries" },
	"Common" : "52 Arietis",
	"OType" : "Double or multiple star",
	"Distance" : "159.42",
	"RA_S" : 46.36120692,
	"DEC_S" : 25.2551679,
	"Constellation" : "Aries ",
	"AMag" : 5.465,
	"key" : 26568,
	"title" : "52 Arietis"
	},
{
	"Index" : "1840",
	"Description" : "Delta Arietis (\u03B4 Ari, \u03B4 Arietis) is the Bayer designation for a star in the northern constellation of Aries. It has the traditional name Botein which is derived from the Arabic word for \u0022belly\u0022. The apparent visual magnitude of this star is 4.35, which is bright enough to be viewed with the naked eye. It has an annual parallax shift of 19.22 mas; corresponding to a physical distance of approximately 170 light-years (52 parsecs) from Earth.\r\rThis is an evolved giant star with a stellar classification of K2 III. It belongs to a population known as red clump giants, which means it is generating energy through the fusion of helium at its core. With close to twice the mass of the Sun, the outer envelope has expanded until it is around ten times the Sun\u0027s radius. It shines with 45 times the Sun\u0027s luminosity at an effective temperature of 4,810 K, giving it the orange-hued glow of a K-type star. It is a suspected variable star that ranges in magnitude from 4.33 to 4.37.\r\rThe term Botein is derived from Al B\u012Br\u016Bn\u012B\u0027s Al Bu\u1E6Dayn (\u0623\u0644\u0628\u0637\u064A\u0646), the dual of Al Ba\u1E6Dn, the Belly. This is the name of star association consisting this star, along with \u03B5 Ari, \u03B6 Ari, \u03C0 Ari, and \u03C13 Ari\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Bu\u1E6Dain were the title for five stars :\u03B4 Ari as Botein, \u03C0 Ari as Al Bu\u1E6Dain I, \u03C13 Ari as Al Bu\u1E6Dain II, \u03B5 Ari as Al Bu\u1E6Dain III dan \u03B6 Ari as Al Bu\u1E6Dain IV\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Nir al Botain, which was translated into Latin as Lucida Ventris, meaning the brightest of the belly.\r\rIn Chinese, \u5929\u9670 (Ti\u0101n Y\u012Bn), meaning Yin Force, refers to an asterism consisting of \u03B4 Arietis, 63 Arietis, \u03B6 Arietis, \u03C4 Arietis and 65 Arietis. Consequently, \u03B4 Arietis itself is known as \u5929\u9670\u56DB (L\u00F3u Su s\u00EC, English: the Fourth Star of Yin Force.)",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "57 Arietis, Delta Arietis, HIP 14838, SAO 93328, HD 19787, GC 3805, HR 951, DM BD+19   477, TYC 1228-2019-1",
	"group" : { "key" : "Aries" },
	"Common" : "Botein",
	"OType" : "Variable Star",
	"Distance" : "52.02",
	"RA_S" : 47.9073618,
	"DEC_S" : 19.7266757,
	"X" : 315,
	"Y" : 548,
	"Constellation" : "Aries ",
	"AMag" : 4.452,
	"key" : 21840,
	"shortTitle" : "Botejn",
	"title" : "Botein"
	},
{
	"Index" : "1957",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "58 Arietis, Zeta Arietis, HIP 15110, SAO 75810, HD 20150, GC 3872, HR 972, DM BD+20   527, TYC 1244-1190-1",
	"group" : { "key" : "Aries" },
	"Common" : "Zeta Arietis",
	"OType" : "Star",
	"Distance" : "80.06",
	"RA_S" : 48.72540591,
	"DEC_S" : 21.04444737,
	"Constellation" : "Aries ",
	"AMag" : 4.867,
	"key" : 21957,
	"title" : "Zeta Arietis"
	},
{
	"Index" : "6623",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 15549, SAO 75871, HD 20644, GC 3981, HR 999, DM BD+28  516, TYC 1796-1306-1",
	"group" : { "key" : "Aries" },
	"Common" : "HR 999",
	"OType" : "Star",
	"Distance" : "166.04",
	"RA_S" : 50.08483464,
	"DEC_S" : 29.0484644,
	"Constellation" : "Aries ",
	"AMag" : 4.639,
	"key" : 26623,
	"title" : "HR 999"
	},
{
	"Index" : "1964",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "61 Arietis, Tau Arietis, HIP 15627A, SAO 75886, HD 20756, GC 4007, HR 1005, DM BD+20   543, TYC 1245-1184-1",
	"group" : { "key" : "Aries" },
	"Common" : "Tau Arietis",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "153.62",
	"RA_S" : 50.30677384,
	"DEC_S" : 21.1470741,
	"Constellation" : "Aries ",
	"AMag" : 5.34,
	"key" : 21964,
	"title" : "Tau Arietis"
	},
{
	"Index" : "1966",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "63 Arietis, Tau-2 Arietis, HIP 15737AB, SAO 75899, HD 20893, GC 4026, HR 1015, DM BD+20   551, TYC 1245-1185-1",
	"group" : { "key" : "Aries" },
	"Common" : "Tau-2 Arietis",
	"OType" : "Double or multiple star",
	"Distance" : "96.97",
	"RA_S" : 50.68850855,
	"DEC_S" : 20.74206658,
	"Constellation" : "Aries ",
	"AMag" : 5.217,
	"key" : 21966,
	"title" : "Tau-2 Arietis"
	},
{
	"Index" : "11390",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "2 Aurigae, HIP 22678, SAO 57475, HD 30834, GC 5934, HR 1551, DM BD+36   952, TYC 2399-1843-1",
	"group" : { "backgroundImage" : "images/Alignment/08.png",
		"description" : "Auriga is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy and remains one of the 88 modern constellations. Located north of the celestial equator, its name is the Latin word for \u0022charioteer\u0022, associating it with various mythological charioteers including Erichthonius and Myrtilus. Auriga is most prominent during winter evenings in the Northern Hemisphere, along with the five other constellations that have stars in the Winter Hexagon asterism. Because of its northern declination, Auriga is only visible as far as 34\u00B0 south; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest constellation, Hydra.\r\rIts brightest star, Capella, is an unusual multiple star system among the brightest stars in the night sky. Beta Aurigae is an interesting variable star in the constellation; Epsilon Aurigae, a nearby eclipsing binary with an unusually long period, has been studied intensively. Because of its position near the winter Milky Way, Auriga has many bright open clusters in its borders, including M36, M37, and M38, popular targets for amateur astronomers. In addition, it has one prominent nebula, the Flaming Star Nebula, associated with the variable star AE Aurigae.\r\rIn Chinese mythology, Auriga\u0027s stars were incorporated into several constellations, including the celestial emperors\u0027 chariots, made up of the modern constellation\u0027s brightest stars. Auriga is home to the radiant for the Aurigids, Zeta Aurigids, Delta Aurigids, and the hypothesized Iota Aurigids.\r\rThe first record of Auriga\u0027s stars was in Mesopotamia as a constellation called GAM, representing a scimitar or crook. However, this may have represented just Capella (Alpha Aurigae) or the modern constellation as a whole; this figure was alternatively called Gamlum or MUL.GAM in the MUL.APIN. The crook of Auriga stood for a goat-herd or shepherd. It was formed from most of the stars of the modern constellation; all of the bright stars were included except for Elnath, traditionally assigned to both Taurus and Auriga. Later, Bedouin astronomers created constellations that were groups of animals, where each star represented one animal. The stars of Auriga comprised a herd of goats, an association also present in Greek mythology. The association with goats carried into the Greek astronomical tradition, though it later became associated with a charioteer along with the shepherd.\r\rIn Greek mythology, Auriga is often identified as the mythological Greek hero Erichthonius of Athens, the chthonic son of Hephaestus who was raised by the goddess Athena. Erichthonius was generally credited to be the inventor of the quadriga, the four-horse chariot, which he used in the battle against the usurper Amphictyon, the event that made Erichthonius the king of Athens. His chariot was created in the image of the Sun\u0027s chariot, the reason Zeus placed him in the heavens. Erichthonius has been credited with inventing the chariot due to his lameness in other myths. The Athenian hero then dedicated himself to Athena and soon after, Zeus raised him into the night sky in honor of his ingenuity and heroic deeds.\r\rAuriga, however, is sometimes named as Myrtilus, who was Hermes\u0027s son and the charioteer of Oenomaus. The association of Auriga and Myrtilus is supported by depictions of the constellation, which rarely show a chariot. Myrtilus\u0027s chariot was destroyed in a race intended for suitors to win the heart of Oenomaus\u0027s daughter Hippodamia. Myrtilus earned his position in the sky when Hippodamia\u0027s successful suitor, Pelops, killed him, despite his complicity in helping Pelops win her hand. After his death, Myrtilus\u0027s father Hermes placed him in the sky. Yet another mythological association of Auriga is Theseus\u0027s son Hippolytus. He was ejected from Athens after he refused the romantic advances of his stepmother Phaedra, who committed suicide as a result. He was killed when his chariot was wrecked, but revived by Asclepius. Regardless of Auriga\u0027s specific representation, it is likely that the constellation was created by the ancient Greeks to commemorate the importance of the chariot in their society.\r\rAn incidental appearance of Auriga in Greek mythology is as the limbs of Medea\u0027s brother. In the myth of Jason and the Argonauts, as they journeyed home, Medea killed her brother and dismembered him, flinging the parts of his body into the sea, represented by the Milky Way. Each individual star represents a different limb.\r\rCapella is associated with the mythological she-goat Amalthea, who breast-fed the infant Zeus. It forms an asterism with the stars Epsilon Aurigae, Zeta Aurigae, and Eta Aurigae, the latter two of which are known as the Haedi (the Kids). Though most often associated with Amalthea, Capella has sometimes been associated with Amalthea\u0027s owner, a nymph. The myth of the nymph says that the goat\u0027s hideous appearance, resembling a Gorgon, was partially responsible for the Titans\u0027 defeat, because Zeus skinned the goat and wore it as his aegis. The asterism containing the three goats had been a separate constellation; however, Ptolemy merged the Charioteer and the Goats in the 2nd century Almagest. Before Ptolemy\u0027s merge, Capella was sometimes seen as its own constellation\u2014by Pliny the Elder and Manilius\u2014called Capra, Caper, or Hircus, all of which relate to its status as the \u0022goat star\u0022. Zeta Aurigae and Eta Aurigae were first called the \u0022Kids\u0022 by Cleostratus, an ancient Greek astronomer.\r\rTraditionally, illustrations of Auriga represent it as a chariot and its driver. The charioteer holds a goat over his left shoulder and has two kids under his left arm; he holds the reins to the chariot in his right hand. However, depictions of Auriga have been inconsistent over the years. The reins in his right hand have also been drawn as a whip, though Capella is almost always over his left shoulder and the Kids under his left arm. The 1488 atlas Hyginus deviated from this typical depiction by showing a four-wheeled cart driven by Auriga, who holds the reins of two oxen, a horse, and a zebra. Jacob Micyllus depicted Auriga in his Hyginus of 1535 as a charioteer with a two-wheeled cart, powered by two horses and two oxen. Arabic and Turkish depictions of Auriga varied wildly from those of the European Renaissance; one Turkish atlas depicted the stars of Auriga as a mule, called Mulus clitellatus by Johann Bayer. One unusual representation of Auriga, from 17th-century France, showed Auriga as Adam kneeling on the Milky Way, with a goat wrapped around his shoulders.\r\rOccasionally, Auriga is seen not as the Charioteer but as Bellerophon, the mortal rider of Pegasus who dared to approach Mount Olympus. In this version of the tale, Jupiter pitied Bellerophon for his foolishness and placed him in the stars.\r\rSome of the stars of Auriga were incorporated into a now-defunct constellation called Telescopium Herschelii. This constellation was introduced by Maximilian Hell to honor William Herschel\u0027s discovery of Uranus. Originally, it included two constellations, Tubus Hershelii Major [sic], in Gemini, Lynx, and Auriga, and Tubus Hershelii Minor [sic] in Orion and Taurus; both represented Herschel\u0027s telescopes. Johann Bode combined Hell\u0027s constellations into Telescopium Herschelii in 1801, located mostly in Auriga.\r\rSince the time of Ptolemy, Auriga has remained a constellation and is officially recognized by the International Astronomical Union, although like all modern constellations, it is now defined as a specific region of the sky that includes both the ancient pattern and the surrounding stars. In 1922, the IAU designated its recommended three-letter abbreviation, \u0022Aur\u0022. The official boundaries of Auriga were created in 1930 by Eug\u00E8ne Delporte as a polygon of 21 segments. Its right ascension is between 4h 37.5m and 7h 30.5m and its declination is between 27.9\u00B0 and 56.2\u00B0 in the equatorial coordinate system.",
		"key" : "Auriga",
		"grouptype" : "Auriga",
		"Meaning" : "charioteer",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Auriga",
		"title" : "Auriga Objects Group" },
	"Common" : "2 Aurigae",
	"OType" : "Star",
	"Distance" : "183.87",
	"RA_S" : 73.15825285,
	"DEC_S" : 36.70318224,
	"Constellation" : "Auriga ",
	"AMag" : 4.939,
	"key" : 31390,
	"title" : "2 Aurigae"
	},
{
	"Index" : "11330",
	"Description" : "Iota Aurigae (\u03B9 Aur, \u03B9 Aurigae) is a star in the northern constellation of Auriga. It has the traditional name Al Kab, short for Kabdhilinan, from the Arabic \u0627\u0644\u0643\u0639\u0628 \u0630\u064A \u0627\u0644\u0639\u0646\u0627\u0646 al-kacb \u00F0\u012Bl-cin\u0101n \u0022the ankle of the rein holder (charioteer)\u0022. Under the name Alkab, this star is a marker on the astrolabe described by Geoffrey Chaucer in his Treatise on the Astrolabe in 1391. In Anton\u00EDn Be\u010Dv\u00E1\u0159\u0027s atlas it has the traditional name Hassaleh. It is known as \u4E94\u8ECA\u4E00 (the First Star of the Five Chariots) in Chinese.\r\rThis star has an apparent visual magnitude of 2.7, which is bright enough to be readily visible to the naked eye. Parallax measurements give a distance estimate of roughly 490 light-years (150 parsecs) from the Earth. At this distance, extinction from interstellar dust is causing a magnitude reduction of about 0.6. Examination of the spectrum yields a stellar classification of K3 II, with the luminosity class of \u0027II\u0027 indicating this is a category of evolved star known as a bright giant. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. The effective temperature of the outer envelope is 4,160 K, which is cooler than the Sun\u0027s effective temperature and gives Iota Aurigae the orange hue of a K-type star.\r\rThis star is a weak X-ray emitter with an X-ray luminosity of about 1.8 \u00D7 1027 ergs s\u20131. This emission is most likely coming from transient loops of plasma in Iota Aurigae\u0027s outer atmosphere, which have a temperature of around 3 million K. This is a suspected variable star, although this variability remains unconfirmed.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "3 Aurigae, Iota Aurigae, HIP 23015, SAO 57522, HD 31398, GC 6029, HR 1577, DM BD+32   855, TYC 2391-1446-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Al Kab / Kabdhilinan",
	"OType" : "Variable Star",
	"Distance" : "150.69",
	"RA_S" : 74.24840612,
	"DEC_S" : 33.16608905,
	"X" : 593,
	"Y" : 305,
	"Constellation" : "Auriga ",
	"AMag" : 2.83,
	"key" : 31330,
	"title" : "Al Kab / Kabdhilinan"
	},
{
	"Index" : "15717",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "4 Aurigae, Omega Aurigae, HIP 23179A, SAO 57548, HD 31647A, GC 6064, HR 1592, DM BD+37  1005, TYC 2894-3065-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Omega Aurigae",
	"OType" : "Star",
	"Distance" : "52.17",
	"RA_S" : 74.81420921,
	"DEC_S" : 37.89024289,
	"Constellation" : "Auriga ",
	"AMag" : 5,
	"key" : 35717,
	"title" : "Omega Aurigae"
	},
{
	"Index" : "15828",
	"Description" : "Epsilon Aurigae (\u03B5 Aur, \u03B5 Aurigae) is the Bayer designation for a star in the northern constellation of Auriga. It is traditionally known as Almaaz, Haldus, or Al Anz. Epsilon Aurigae is an unusual eclipsing binary system comprising an F0 supergiant and a companion which is generally accepted to be a huge dark disk orbiting an unknown object, possibly a binary system of two small B-type stars. About every 27 years, Epsilon Aurigae\u0027s brightness drops from an apparent visual magnitude of +2.92 to +3.83. This dimming lasts 640\u2013730 days. In addition to this eclipse, the system also has a low amplitude pulsation with a non-consistent period of around 66 days. The distance to the system is still a subject of debate, but modern estimates place it approximately 2,000 light years from Earth.\r\rEpsilon Aurigae was first suspected to be a variable star when German astronomer Johann Fritsch observed it in 1821. Later observations by Eduard Heis and Friedrich Wilhelm Argelander reinforced Fritsch\u0027s initial suspicions and attracted attention to the star. Hans Ludendorff, however, was the first to study it in great detail. His work revealed that the system was an eclipsing binary variable, a star that dims when its partner obscures its light.\r\rEpsilon Aurigae\u0027s eclipsing companion has been subject to much debate since the object does not emit as much light as is expected for an object its size. As of 2008, the most popularly accepted model for this companion object is a binary star system surrounded by a massive, opaque disk of dust; theories speculating that the object is a large, semitransparent star or a black hole have since been discarded.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "7 Aurigae, Epsilon Aurigae, HIP 23416, SAO 39955, HD 31964, GC 6123, HR 1605, DM BD+43  1166, TYC 2907-1275-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Almaaz / Haldus / Al Anz",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "653.5948",
	"RA_S" : 75.49221855,
	"DEC_S" : 43.8233072,
	"X" : 557,
	"Y" : 169,
	"Constellation" : "Auriga ",
	"AMag" : 3.069,
	"key" : 35828,
	"shortTitle" : "Almaaz",
	"title" : "Almaaz / Haldus / Al Anz"
	},
{
	"Index" : "15756",
	"Description" : "Zeta Aurigae (\u03B6 Aur, \u03B6 Aurigae) is the Bayer designation for a binary star system in the northern constellation of Auriga. It has the traditional names Haedus and Sadatoni. Based upon parallax measurements made during the Hipparcos mission, this system is approximately 790 light-years (240 parsecs) distant from the Earth. It has a combined apparent visual magnitude of 3.75, which is bright enough to be seen with the naked eye.\r\rThis is an eclipsing binary system with the orbital plane being oriented close to the line of sight from the Earth; the inclination of this system is estimated as 87.0\u00B0. As a result, an eclipse of one star by the other occurs during each orbit, causing the magnitude to decrease to +3.99. The pair have an orbital period of 972 days (2.66 years) and an eccentricity of 0.4. The primary component has been categorized as a K-type bright giant or supergiant star. Its companion is a B-type main sequence star of stellar classification B5 V or B7 V.\r\rIt has the traditional names Haedus (also Hoedus) and Sadatoni (rarely Saclateri). It is one of the two h\u00E6di (kids) of the she-goat Capella, the other being Hoedus II, Eta Aurigae. The name Sadatoni is from the Arabic \u0627\u0644\u0633\u0627\u0639\u062F \u0627\u0644\u062B\u0627\u0646\u064A as-s\u0101cid a\u03B8-\u03B8\u0101n\u012B \u0022the second arm (of the charioteer)\u0022. The rare traditional name Azaleh is shared (in the form Hassaleh) with Iota Aurigae.\r\rIn Chinese, \u67F1 (Zh\u00F9), meaning Pillars, refers to an asterism consisting of \u03B6 Aurigae, \u03B5 Aurigae, \u03B7 Aurigae, \u03C5 Aurigae, \u03BD Aurigae, \u03C4 Aurigae, \u03C7 Aurigae and 26 Aurigae. Consequently, \u03B6 Aurigae itself is known as \u67F1\u4E8C (Zh\u00F9 y\u012B, English: the Second Star of Pillars.)",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "8 Aurigae, Zeta Aurigae, HIP 23453, SAO 39966, HD 32068, GC 6137, HR 1612, DM BD+40  1142A, TYC 2899-2236-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Haedus / Sadatoni",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "239.56",
	"RA_S" : 75.61953354,
	"DEC_S" : 41.07583522,
	"X" : 562,
	"Y" : 205,
	"Constellation" : "Auriga ",
	"AMag" : 3.888,
	"key" : 35756,
	"shortTitle" : "Haedi; Haedus; Sadatoni; Saclateni",
	"title" : "Haedus / Sadatoni"
	},
{
	"Index" : "15757",
	"Description" : "Eta Aurigae (\u03B7 Aur, \u03B7 Aurigae) is a star in the constellation Auriga. It has the traditional name Hoedus II or Haedus II. With an apparent visual magnitude of 3.18, it is visible to the naked eye. Based upon parallax measurements made during the Hipparcos mission, this star is approximately 243 light-years (75 parsecs) distant from the Earth.\r\rEta Aurigae is a larger star than the Sun, with more than five times the Sun\u0027s mass and over three times the Sun\u0027s radius. The spectrum of this star matches a stellar classification of B3 V, which is a B-type main sequence star that is generating its energy through the nuclear fusion of hydrogen at its core. It is radiating 955 times the Sun\u0027s luminosity from its outer atmosphere at an effective temperature of 17,201 K. Based upon its projected rotational velocity of 95, it is spinning with a rotation period of only 1.8 days. Eta Aurigae is around 39 million years old.\r\rAlong with \u03B6 Aurigae it represents one of the Kids of the she-goat Capella, from which it gets its Latin traditional name Hoedus II or Haedus II, from the Latin h\u00E6dus \u0022kid\u0022; Zeta Aurigae is Hoedus I. It has the less common traditional name Mahasim, from the Arabic \u0627\u0644\u0645\u0650\u0639\u0652\u0635\u064E\u0645 al-mic\u015Fam \u0022wrist\u0022 (of the charioteer), which it shares with Theta Aurigae. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It has an apparent visual magnitude of 3.18 and is located at a distance of around 243 light-years (75 parsecs) from Earth.\r\rIn Chinese, \u67F1 (Zh\u00F9), meaning Pillars, refers to an asterism consisting of \u03B7 Aurigae, \u03B5 Aurigae, \u03B6 Aurigae, \u03C5 Aurigae, \u03BD Aurigae, \u03C4 Aurigae, \u03C7 Aurigae and 26 Aurigae. Consequently, \u03B7 Aurigae itself is known as \u67F1\u4E09 (Zh\u01D4 s\u0101n, English: the Third Star of Pillars.)",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "10 Aurigae, Eta Aurigae, HIP 23767, SAO 40026, HD 32630, GC 6226, HR 1641, DM BD+41  1058, TYC 2899-2237-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Hoedus II",
	"OType" : "Variable Star",
	"Distance" : "74.61",
	"RA_S" : 76.62872239,
	"DEC_S" : 41.23447576,
	"X" : 552,
	"Y" : 205,
	"Constellation" : "Auriga ",
	"AMag" : 3.123,
	"key" : 35757,
	"title" : "Hoedus II"
	},
{
	"Index" : "19845",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "9 Aurigae, HIP 23783, SAO 25019, HD 32537A, GC 6219, HR 1637, DM BD+51  1024, TYC 3357-2332-1",
	"group" : { "key" : "Auriga" },
	"Common" : "9 Aurigae",
	"OType" : "Star",
	"Distance" : "26.29",
	"RA_S" : 76.669294,
	"DEC_S" : 51.59771918,
	"Constellation" : "Auriga ",
	"AMag" : 5.014,
	"key" : 39845,
	"title" : "9 Aurigae"
	},
{
	"Index" : "15728",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "11 Aurigae, Mu Aurigae, HIP 24340, SAO 57755, HD 33641, GC 6375, HR 1689, DM BD+38  1063, TYC 2896-2101-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Mu Aurigae",
	"OType" : "Double or multiple star",
	"Distance" : "46.82",
	"RA_S" : 78.35716405,
	"DEC_S" : 38.48449266,
	"Constellation" : "Auriga ",
	"AMag" : 4.847,
	"key" : 35728,
	"title" : "Mu Aurigae"
	},
{
	"Index" : "11351",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "14 Aurigae, HIP 24504A, SAO 57799, HD 33959A, GC 6411, HR 1706, DM BD+32   922, TYC 2394-2028-1",
	"group" : { "key" : "Auriga" },
	"Common" : "14 Aurigae",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "86.9",
	"RA_S" : 78.8516452,
	"DEC_S" : 32.68759618,
	"X" : 536,
	"Y" : 310,
	"Constellation" : "Auriga ",
	"AMag" : 5.028,
	"key" : 31351,
	"title" : "14 Aurigae"
	},
{
	"Index" : "11350",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "16 Aurigae, HIP 24727, SAO 57853, HD 34334, GC 6473, HR 1726, DM BD+33  1000, TYC 2394-2027-1",
	"group" : { "key" : "Auriga" },
	"Common" : "16 Aurigae",
	"OType" : "Spectroscopic binary",
	"Distance" : "71.08",
	"RA_S" : 79.54403863,
	"DEC_S" : 33.3716069,
	"Constellation" : "Auriga ",
	"AMag" : 4.689,
	"key" : 31350,
	"title" : "16 Aurigae"
	},
{
	"Index" : "11349",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "HIP 24799, SAO 57884, HD 34452, GC 6497, HR 1732, DM BD+33 1008, TYC 2394-2026-1",
	"group" : { "key" : "Auriga" },
	"Common" : "V* IQ Aur",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "126.41",
	"RA_S" : 79.75012264,
	"DEC_S" : 33.74839593,
	"Constellation" : "Auriga ",
	"AMag" : 5.343,
	"key" : 31349,
	"title" : "V* IQ Aur"
	},
{
	"Index" : "15767",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "15 Aurigae, Lambda Aurigae, HIP 24813, SAO 40233, HD 34411, GC 6494, HR 1729, DM BD+39  1248, TYC 2900-2157-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Lambda Aurigae",
	"OType" : "High proper-motion Star",
	"Distance" : "12.63",
	"RA_S" : 79.78530918,
	"DEC_S" : 40.09905072,
	"Constellation" : "Auriga ",
	"AMag" : 4.761,
	"key" : 35767,
	"title" : "Lambda Aurigae"
	},
{
	"Index" : "11381",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "19 Aurigae, HIP 24879, SAO 57906, HD 34578, GC 6515, HR 1740, DM BD+33  1013, TYC 2398-1609-1",
	"group" : { "key" : "Auriga" },
	"Common" : "19 Aurigae",
	"OType" : "Variable Star",
	"Distance" : "636.9427",
	"RA_S" : 80.00384454,
	"DEC_S" : 33.95805774,
	"Constellation" : "Auriga ",
	"AMag" : 5.075,
	"key" : 31381,
	"title" : "19 Aurigae"
	},
{
	"Index" : "15898",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "HIP 24902AB, SAO 40248, HD 34557, GC 6516, HR 1738, DM BD+40 1253, TYC 2913-2360-1",
	"group" : { "key" : "Auriga" },
	"Common" : "HR 1738",
	"OType" : "Double or multiple star",
	"Distance" : "84.71",
	"RA_S" : 80.06112185,
	"DEC_S" : 41.0862068,
	"Constellation" : "Auriga ",
	"AMag" : 5.472,
	"key" : 35898,
	"title" : "HR 1738"
	},
{
	"Index" : "15937",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "20 Aurigae, Rho Aurigae, HIP 25048, SAO 40269, HD 34759, GC 6556, HR 1749, DM BD+41  1162, TYC 2917-2528-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Rho Aurigae",
	"OType" : "Spectroscopic binary",
	"Distance" : "161.68",
	"RA_S" : 80.45173447,
	"DEC_S" : 41.80457865,
	"Constellation" : "Auriga ",
	"AMag" : 5.185,
	"key" : 35937,
	"title" : "Rho Aurigae"
	},
{
	"Index" : "11566",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "21 Aurigae, Sigma Aurigae, HIP 25292, SAO 57981, HD 35186, GC 6636, HR 1773, DM BD+37  1175, TYC 2415-1779-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Sigma Aurigae",
	"OType" : "Star",
	"Distance" : "142.88",
	"RA_S" : 81.16308805,
	"DEC_S" : 37.38534706,
	"Constellation" : "Auriga ",
	"AMag" : 5.164,
	"key" : 31566,
	"title" : "Sigma Aurigae"
	},
{
	"Index" : "11523",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "24 Aurigae, Phi Aurigae, HIP 25541, SAO 58051, HD 35620, GC 6715, HR 1805, DM BD+34  1048, TYC 2411-2462-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Phi Aurigae",
	"OType" : "Star",
	"Distance" : "137.74",
	"RA_S" : 81.91202131,
	"DEC_S" : 34.47589104,
	"Constellation" : "Auriga ",
	"AMag" : 5.222,
	"key" : 31523,
	"title" : "Phi Aurigae"
	},
{
	"Index" : "11475",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "25 Aurigae, Chi Aurigae, HIP 25984, SAO 58164, HD 36371, GC 6849, HR 1843, DM BD+32  1024, TYC 2407-2149-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Chi Aurigae",
	"OType" : "Spectroscopic binary",
	"RA_S" : 83.18197424,
	"DEC_S" : 32.19202649,
	"Constellation" : "Auriga ",
	"AMag" : 4.763,
	"key" : 31475,
	"title" : "Chi Aurigae"
	},
{
	"Index" : "11444",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "26 Aurigae, HIP 26536AB, SAO 58280, HD 37269, GC 7002, HR 1914, DM BD+30   963, TYC 2404-1350-1",
	"group" : { "key" : "Auriga" },
	"Common" : "26 Aurigae",
	"OType" : "Double or multiple star",
	"Distance" : "134.38",
	"RA_S" : 84.65869566,
	"DEC_S" : 30.49242391,
	"Constellation" : "Auriga ",
	"AMag" : 5.458,
	"key" : 31444,
	"title" : "26 Aurigae"
	},
{
	"Index" : "19928",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "27 Aurigae, Omicron Aurigae, HIP 27196, SAO 40583, HD 38104, GC 7182, HR 1971, DM BD+49  1398, TYC 3368-1338-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Omicron Aurigae",
	"OType" : "Star",
	"Distance" : "125.04",
	"RA_S" : 86.47516627,
	"DEC_S" : 49.82628127,
	"Constellation" : "Auriga ",
	"AMag" : 5.464,
	"key" : 39928,
	"title" : "Omicron Aurigae"
	},
{
	"Index" : "15871",
	"Description" : "Tau Aurigae (\u03C4 Aur, \u03C4 Aurigae) is the Bayer designation for a star in the constellation Auriga. It is visible to the naked eye with an apparent visual magnitude of 4.505, and is approximately 207 light-years (63 parsecs) distant from Earth. This is an evolved giant star with a stellar classification of G8 III. It has expanded to 11 times the radius of the Sun and shines with 63 times the Sun\u0027s luminosity. This energy is radiated into outer space from the outer atmosphere at an effective temperature of 4,887. This heat gives it the yellow-hued glow of a G-type star.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "29 Aurigae, Tau Aurigae, HIP 27483, SAO 58465, HD 38656, GC 7277, HR 1995, DM BD+39  1418, TYC 2911-1795-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Tau Aurigae",
	"OType" : "High proper-motion Star",
	"Distance" : "63.4",
	"RA_S" : 87.29349494,
	"DEC_S" : 39.18107161,
	"X" : 449,
	"Y" : 241,
	"Constellation" : "Auriga ",
	"AMag" : 4.623,
	"key" : 35871,
	"title" : "Tau Aurigae"
	},
{
	"Index" : "11589",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "31 Aurigae, Upsilon Aurigae, HIP 27639, SAO 58496, HD 38944, GC 7322, HR 2011, DM BD+37  1336, TYC 2418-1571-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Upsilon Aurigae",
	"OType" : "Variable Star",
	"Distance" : "158.2",
	"RA_S" : 87.76016086,
	"DEC_S" : 37.30556814,
	"Constellation" : "Auriga ",
	"AMag" : 4.917,
	"key" : 31589,
	"title" : "Upsilon Aurigae"
	},
{
	"Index" : "15888",
	"Description" : "Nu Aurigae (\u03BD Aur, \u03BD Aurigae) is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.96 and is approximately 220 light-years (67 parsecs) distant from the Earth. This is an evolved giant star with a stellar classification of G9.5 III. It is a red clump star, which indicates that it is generating energy through the fusion of helium at its core. The outer envelope has expanded to 19 times the radius of the Sun and cooled to 4,571 K, giving it the characteristic yellow-hued glow of a G-type star. It shines with 135 times the luminosity of the Sun.\r\rThis is an astrometric binary with a suspected white dwarf companion. A 10th magnitude star 54.6 arcseconds away is an optical companion.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "32 Aurigae, Nu Aurigae, HIP 27673, SAO 58502, HD 39003, GC 7334, HR 2012, DM BD+39  1429, TYC 2912-1835-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Nu Aurigae",
	"OType" : "Star",
	"Distance" : "70.44",
	"RA_S" : 87.87245959,
	"DEC_S" : 39.14849516,
	"X" : 443,
	"Y" : 242,
	"Constellation" : "Auriga ",
	"AMag" : 4.087,
	"key" : 35888,
	"title" : "Nu Aurigae"
	},
{
	"Index" : "23450",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "30 Aurigae, Xi Aurigae, HIP 27949, SAO 25450, HD 39283, GC 7404, HR 2029, DM BD+55  1027, TYC 3754-939-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Xi Aurigae",
	"OType" : "Star",
	"Distance" : "73.01",
	"RA_S" : 88.71158677,
	"DEC_S" : 55.70694678,
	"Constellation" : "Auriga ",
	"AMag" : 4.966,
	"key" : 43450,
	"title" : "Xi Aurigae"
	},
{
	"Index" : "23416",
	"Description" : "Delta Aurigae (\u03B4 Aur, \u03B4 Aurigae) is the Bayer designation for an astrometric binary star in the constellation Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.715. Based upon its annual parallax shift of 25.88 mas, it is some 126 light-years (39 parsecs) distant from the Earth, give or take an eight light-year margin of error. This star is the namesake for the Delta Aurigids, a meteor shower that occurs between October 6\u201315. The radiant point for this shower passes several degrees to the south of the star.\r\rThe visible component of this system is a giant star with a stellar classification of K0 III. It has 11 times the radius of the Sun and shines with 62 times the Sun\u0027s luminosity. This energy is being radiated from the star\u0027s outer envelope at an effective temperature of 4,786 K. This heat gives the star the orange-hued glow of a K-type star.\r\rIn Indian astronomy, it is known by the Sanskrit name Praj\u0101pati (\u092A\u094D\u0930\u091C\u093E\u092A\u0924\u093F), \u0022the Lord of Creation\u0022.\r\rIn Chinese, \u516B\u7A40 (B\u0101 G\u01D4), meaning Eight Kinds of Crops, refers to an asterism consisting of \u03B4 Aurigae, \u03BE Aurigae, 26 Camelopardalis, 14 Camelopardalis, 7 Camelopardalis, 9 Aurigae, 11 Camelopardalis and 31 Camelopardalis. Consequently, \u03B4 Aurigae itself is known as \u516B\u7A40\u4E00 (B\u0101 G\u01D4 y\u012B, English: the First Star of Eight Kinds of Crops.)",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "33 Aurigae, Delta Aurigae, HIP 28358, SAO 25502, HD 40035, GC 7521, HR 2077, DM BD+54   970, TYC 3750-1042-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Delta Aurigae",
	"OType" : "Spectroscopic binary",
	"Distance" : "42.99",
	"RA_S" : 89.88179951,
	"DEC_S" : 54.28467265,
	"X" : 423,
	"Y" : 45,
	"Constellation" : "Auriga ",
	"AMag" : 3.832,
	"key" : 43416,
	"title" : "Delta Aurigae"
	},
{
	"Index" : "19882",
	"Description" : "Pi Aurigae (\u03C0 Aur, \u03C0 Aurigae) is the Bayer designation for a star in the northern constellation of Auriga. Located about one degree north of the 2nd magnitude star Beta Aurigae, Pi Aurigae is visible to the naked eye with an apparent visual magnitude of 4.25 Based upon parallax measurements, it is approximately 800 light-years (250 parsecs) away from Earth. At that distance, the brightness of the star is diminished by 0.54 in magnitude from extinction caused by interstellar gas and dust.\r\rPi Aurigae is a bright giant star with a stellar classification of M3 II. The measured angular diameter of this star, after correction for limb darkening, is 9.56 \u00B1 0.10 mas. At the estimated distance of Pi Aurigae, this yields a physical size of about 265 times the radius of the Sun. It is classified as an slow irregular variable of type LC and its brightness varies from magnitude +4.24 to +4.34.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "35 Aurigae, Pi Aurigae, HIP 28404, SAO 40756, HD 40239, GC 7554, HR 2091, DM BD+45  1217, TYC 3361-1787-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Pi Aurigae",
	"OType" : "Long-period variable star",
	"Distance" : "224.91",
	"RA_S" : 89.98374012,
	"DEC_S" : 45.93673496,
	"X" : 422,
	"Y" : 153,
	"Constellation" : "Auriga ",
	"AMag" : 4.516,
	"key" : 39882,
	"title" : "Pi Aurigae"
	},
{
	"Index" : "16005",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "40 Aurigae, HIP 28946, SAO 58749, HD 41357, GC 7723, HR 2143, DM BD+38  1377, TYC 2925-806-1",
	"group" : { "key" : "Auriga" },
	"Common" : "40 Aurigae",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.34",
	"RA_S" : 91.64623756,
	"DEC_S" : 38.48264248,
	"Constellation" : "Auriga ",
	"AMag" : 5.376,
	"key" : 36005,
	"title" : "40 Aurigae"
	},
{
	"Index" : "7378",
	"Description" : "Kappa Aurigae (\u03BA Aur, \u03BA Aurigae) is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 4.3. Based upon an annual parallax shift of 19.31 mas, it is approximately 169 light-years (52 parsecs) distant from Earth.\r\rThis is an evolved giant star with a stellar classification of G8.5 IIIb. It is a red clump star that is generating energy through the fusion of helium at its core. Kappa Aurigae has expanded to 11 times the radius of the Sun and shines with 54 times the Sun\u0027s luminosity. This energy is radiated into outer space from the outer envelope at an effective temperature of 4,732 K. At this heat, the star glows with the orange-hue of a G-type star.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "44 Aurigae, Kappa Aurigae, HIP 29696, SAO 78143, HD 43039, GC 7981, HR 2219, DM BD+29  1154, TYC 1889-861-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Kappa Aurigae",
	"OType" : "Variable Star",
	"Distance" : "54.25",
	"RA_S" : 93.84453493,
	"DEC_S" : 29.49807515,
	"X" : 378,
	"Y" : 366,
	"Constellation" : "Auriga ",
	"AMag" : 4.434,
	"key" : 27378,
	"title" : "Kappa Aurigae"
	},
{
	"Index" : "23508",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "45 Aurigae, HIP 30247, SAO 25681, HD 43905, GC 8151, HR 2264, DM BD+53  1008, TYC 3764-2617-1",
	"group" : { "key" : "Auriga" },
	"Common" : "45 Aurigae",
	"OType" : "Spectroscopic binary",
	"Distance" : "59.18",
	"RA_S" : 95.44220781,
	"DEC_S" : 53.45217604,
	"Constellation" : "Auriga ",
	"AMag" : 5.385,
	"key" : 43508,
	"title" : "45 Aurigae"
	},
{
	"Index" : "20048",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "46 Aurigae, Psi01 Aurigae, HIP 30520, SAO 41076, HD 44537, GC 8235, HR 2289, DM BD+49  1488, TYC 3384-1194-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi01 Aurigae",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 96.22459422,
	"DEC_S" : 49.28789395,
	"Constellation" : "Auriga ",
	"AMag" : 5.147,
	"key" : 40048,
	"title" : "Psi01 Aurigae"
	},
{
	"Index" : "7365",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "49 Aurigae, HIP 31434, SAO 78524, HD 46553, GC 8557, HR 2398, DM BD+28  1168, TYC 1888-1793-1",
	"group" : { "key" : "Auriga" },
	"Common" : "49 Aurigae",
	"OType" : "Star",
	"Distance" : "113.2",
	"RA_S" : 98.80025756,
	"DEC_S" : 28.02231013,
	"Constellation" : "Auriga ",
	"AMag" : 5.258,
	"key" : 27365,
	"title" : "49 Aurigae"
	},
{
	"Index" : "16058",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "52 Aurigae, Psi03 Aurigae, HIP 31789, SAO 59319, HD 47100, GC 8655, HR 2420, DM BD+40  1665, TYC 2932-2464-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi03 Aurigae",
	"OType" : "Star",
	"Distance" : "407.05",
	"RA_S" : 99.70492173,
	"DEC_S" : 39.90256111,
	"Constellation" : "Auriga ",
	"AMag" : 5.319,
	"key" : 36058,
	"title" : "Psi03 Aurigae"
	},
{
	"Index" : "16091",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "50 Aurigae, Psi02 Aurigae, HIP 31832, SAO 41239, HD 47174, GC 8662, HR 2427, DM BD+42  1585, TYC 2936-2025-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi02 Aurigae",
	"OType" : "Star",
	"Distance" : "127.34",
	"RA_S" : 99.83261633,
	"DEC_S" : 42.48888048,
	"Constellation" : "Auriga ",
	"AMag" : 4.931,
	"key" : 36091,
	"title" : "Psi02 Aurigae"
	},
{
	"Index" : "16215",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "55 Aurigae, Psi04 Aurigae, HIP 32173, SAO 41288, HD 47914, GC 8751, HR 2459, DM BD+44  1518, TYC 2953-1956-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi04 Aurigae",
	"OType" : "Star",
	"Distance" : "99.08",
	"RA_S" : 100.77071334,
	"DEC_S" : 44.52444987,
	"Constellation" : "Auriga ",
	"AMag" : 5.207,
	"key" : 36215,
	"title" : "Psi04 Aurigae"
	},
{
	"Index" : "16217",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "56 Aurigae, Psi05 Aurigae, HIP 32480, SAO 41330, HD 48682, GC 8836, HR 2483, DM BD+43  1595, TYC 2953-1958-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi05 Aurigae",
	"OType" : "Star",
	"Distance" : "16.72",
	"RA_S" : 101.68474118,
	"DEC_S" : 43.57742636,
	"Constellation" : "Auriga ",
	"AMag" : 5.31,
	"key" : 36217,
	"title" : "Psi05 Aurigae"
	},
{
	"Index" : "20160",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "57 Aurigae, Psi06 Aurigae, HIP 32562, SAO 41346, HD 48781, GC 8858, HR 2487, DM BD+48  1436, TYC 3398-2490-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi06 Aurigae",
	"OType" : "Star",
	"Distance" : "110.26",
	"RA_S" : 101.91490771,
	"DEC_S" : 48.78947389,
	"Constellation" : "Auriga ",
	"AMag" : 5.341,
	"key" : 40160,
	"title" : "Psi06 Aurigae"
	},
{
	"Index" : "16200",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "58 Aurigae, Psi07 Aurigae, HIP 32844, SAO 41380, HD 49520, GC 8931, HR 2516, DM BD+41  1536, TYC 2950-1863-1",
	"group" : { "key" : "Auriga" },
	"Common" : "Psi07 Aurigae",
	"OType" : "Star",
	"Distance" : "116.05",
	"RA_S" : 102.69142943,
	"DEC_S" : 41.78123273,
	"Constellation" : "Auriga ",
	"AMag" : 5.118,
	"key" : 36200,
	"title" : "Psi07 Aurigae"
	},
{
	"Index" : "16155",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "63 Aurigae, HIP 34752, SAO 59866, HD 54716, GC 9490, HR 2696, DM BD+39  1882, TYC 2944-1954-1",
	"group" : { "key" : "Auriga" },
	"Common" : "63 Aurigae",
	"OType" : "Star",
	"Distance" : "148.3",
	"RA_S" : 107.91385442,
	"DEC_S" : 39.32054585,
	"Constellation" : "Auriga ",
	"AMag" : 5.059,
	"key" : 36155,
	"title" : "63 Aurigae"
	},
{
	"Index" : "11937",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "65 Aurigae, HIP 35710, SAO 60010, HD 57264, GC 9796, HR 2793, DM BD+37  1707, TYC 2464-2366-1",
	"group" : { "key" : "Auriga" },
	"Common" : "65 Aurigae",
	"OType" : "Star",
	"Distance" : "72.3",
	"RA_S" : 110.51090594,
	"DEC_S" : 36.76058358,
	"Constellation" : "Auriga ",
	"AMag" : 5.241,
	"key" : 31937,
	"title" : "65 Aurigae"
	},
{
	"Index" : "16278",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "66 Aurigae, HIP 35907, SAO 41738, HD 57669, GC 9850, HR 2805, DM BD+40  1852, TYC 2961-2073-1",
	"group" : { "key" : "Auriga" },
	"Common" : "66 Aurigae",
	"OType" : "Star",
	"Distance" : "365.31",
	"RA_S" : 111.0352829,
	"DEC_S" : 40.67238797,
	"Constellation" : "Auriga ",
	"AMag" : 5.328,
	"key" : 36278,
	"title" : "66 Aurigae"
	},
{
	"Index" : "3865",
	"Description" : "Tau Bootis (\u03C4 Boo, \u03C4 Bootis) is a yellow-white dwarf approximately 51 light-years away in the constellation of Bootes. The system is also a binary star system, with the secondary star being a red dwarf. As of 1999, an extrasolar planet has been confirmed to be orbiting the primary star.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "4 Bootis, Tau Bootis, HIP 67275, SAO 100706, HD 120136, GC 18637, HR 5185, DM BD+18  2782, TYC 1460-132-1",
	"group" : { "backgroundImage" : "images/Alignment/09.png",
		"description" : "Bootes (pron.: /bo\u028A\u02C8o\u028Ati\u02D0z/) is a constellation in the northern sky, located between 0\u00B0 and +60\u00B0 declination, and 13 and 16 hours of right ascension on the celestial sphere. The name comes from the Greek \u0392\u03BF\u03CE\u03C4\u03B7\u03C2, Bo\u014Dt\u0113s, meaning herdsman or plowman (literally, ox-driver; from boos, related to the Latin bovis, \u0022cow\u0022). The \u0022o\u0022 in the name is a diaeresis, not an umlaut, meaning that each \u0027o\u0027 is to be pronounced separately.\r\rBootes was one of the 48 constellations described by the 2nd century astronomer Ptolemy and is now one of the 88 modern constellations. It contains the fourth brightest star in the night sky, Arcturus. Bootes is home to many other bright stars, including eight above the fourth magnitude and an additional 21 above the fifth magnitude, making a total of 29 stars easily visible to the naked eye.\r\rIn ancient Babylon the stars of Bootes were known as SHU.PA. They were apparently depicted as the god Enlil, who was the leader of the Babylonian pantheon and special patron of farmers.\r\rExactly whom Bootes is supposed to represent in Greek mythology is not clear. According to one version, he was the son of Demeter, and a ploughman who drove the oxen in the constellation Ursa Major. This is corroborated by the constellation\u0027s name, which itself means \u0022oxen-driver\u0022 or \u0022herdsman.\u0022 ]  The ancient Greeks saw the asterism now called the \u0022Big Dipper\u0022 or \u0022Plough\u0022 as a cart with oxen. This influenced the name\u0027s etymology, derived from the Greek for \u0022noisy\u0022 or \u0022ox-driver\u0022. Another myth associated with Bootes tells that he invented the plow and was memorialized for his ingenuity as a constellation. Bootes was also recognized in Greek literature; in The Odyssey, Homer describes it as \u0022slow to set\u0022 and calls it the \u0022Plowman\u0022.\r\rAnother myth associated with Bootes by Hyginus is that of Icarius, who was schooled as a grape farmer and winemaker by Dionysus. Icarius made wine so strong that those who drank it appeared poisoned, which caused shepherds to avenge their supposedly poisoned friends by killing Icarius. Maera, Icarius\u0027s dog, brought his daughter Erigone to her father\u0027s body, whereupon both she and the dog committed suicide. Zeus then chose to honor all three by placing them in the sky as constellations: Icarius as Bootes, Erigone as Virgo, and Maera as Canis Major or Canis Minor.\r\rFollowing another reading, the constellation is identified with Arcas and also referred to as Arcas and Arcturus, son of Zeus and Callisto. Arcas was brought up by his maternal grandfather Lycaon, to whom one day Zeus went and had a meal. To verify that the guest was really the king of the gods, Lycaon killed his grandson and prepared a meal made from his flesh. Zeus noticed and became very angry, transforming Lycaon into a wolf and gave back life to his son. In the meantime Callisto had been transformed into a she-bear, by Zeus\u0027 wife, Hera, who was angry at Zeus\u0027 infidelity. This is corroborated by the Greek name for Bootes, Arctophylax, which means \u0022Bear Watcher\u0022.. Callisto in form of a bear was almost killed by her son who was out hunting. Zeus rescued her, taking her into the sky where she became Ursa Major, \u0022the Great Bear\u0022. The name Arcturus (the constellation\u0027s brightest star) comes from the Greek word meaning \u0022guardian of the bear\u0022. Sometimes Arcturus is depicted as leading the hunting dogs of nearby Canes Venatici and driving the bears of Ursa Major and Ursa Minor.\r\rSeveral former constellations were formed from stars now included in Bootes. Quadrans Muralis, the Quadrant, was a constellation created near Beta Bootis from faint stars. It was invented in 1795 by J\u00E9r\u00F4me Lalande, an astronomer who used a quadrant to perform detailed astronometric measurements. Lalande worked with Nicole-Reine Lepaute and others to predict the 1758 return of Halley\u0027s Comet. Quadrans Muralis was formed from the stars of eastern Bootes, western Hercules, and Draco. It was originally called Le Mural by Jean Fortin in his 1795 Atlas C\u00E9leste; it was not given the name Quadrans Muralis until Johann Bode\u0027s 1801 Uranographia. The constellation was quite faint, with its brightest stars reaching the 5th magnitude. Mons Maenalus, representing the Maenalus mountains, was created by Johannes Hevelius in 1687 at the foot of the constellation\u0027s figure. The mountain was named for the son of Lycaon, Maenalus. The mountain, one of Diana\u0027s hunting grounds, was also holy to Pan.",
		"key" : "Bootes",
		"grouptype" : "Bootes",
		"Meaning" : "herdsman",
		"Family" : "Ursa Major",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Bootes",
		"title" : "Bootes Objects Group" },
	"Common" : "Tau Bootis",
	"OType" : "Star",
	"Distance" : "15.62",
	"RA_S" : 206.81559567,
	"DEC_S" : 17.45689887,
	"X" : 562,
	"Y" : 530,
	"Constellation" : "Bootes ",
	"AMag" : 4.536,
	"key" : 23865,
	"title" : "Tau Bootis"
	},
{
	"Index" : "3864",
	"Description" : "Upsilon Bootis (\u03C5 Boo, \u03C5 Bootis) is a star in the constellation Bootes.\r\rUpsilon Bootis is an orange K-type giant with an apparent magnitude of +4.05. It is approximately 263 light years from Earth.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "5 Bootis, Upsilon Bootis, HIP 67459, SAO 100725, HD 120477, GC 18674, HR 5200, DM BD+16  2564, TYC 1460-1180-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Upsilon Bootis",
	"OType" : "Variable Star",
	"Distance" : "80.74",
	"RA_S" : 207.36933719,
	"DEC_S" : 15.79791084,
	"X" : 557,
	"Y" : 552,
	"Constellation" : "Bootes ",
	"AMag" : 4.21,
	"key" : 23864,
	"title" : "Upsilon Bootis"
	},
{
	"Index" : "3909",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "6 Bootis, e Bootis, HIP 67480, SAO 83015, HD 120539, GC 18683, HR 5201, DM BD+21  2578, TYC 1466-1082-1",
	"group" : { "key" : "Bootes" },
	"Common" : "e Bootis",
	"OType" : "Spectroscopic binary",
	"Distance" : "120.72",
	"RA_S" : 207.42848094,
	"DEC_S" : 21.26410755,
	"Constellation" : "Bootes ",
	"AMag" : 5.075,
	"key" : 23909,
	"title" : "e Bootis"
	},
{
	"Index" : "3936",
	"Description" : "Eta Bootis (\u03B7 Boo, \u03B7 Bootis) is a star in the constellation Bootes. It has the traditional names Muphrid and Saak, and the Flamsteed designation 8 Bootis. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.\r\rThe name Muphrid is from the Arabic \u0645\u0641\u0631\u062F \u0627\u0644\u0631\u0627\u0645\u062D mufrid ar-r\u0101mi\u0127 \u0022the (single) one of the lancer\u0022. In Chinese, \u53F3\u651D\u63D0 (Y\u00F2u Ni\u00E8 D\u012B), meaning \u0022the Right Conductor\u0022, refers to an asterism consisting of Eta Bootis, Tau Bootis and Upsilon Bootis. Consequently, Eta Bootis itself is known as \u53F3\u651D\u63D0\u4E00 (Y\u00F2u Ni\u00E8 D\u012B y\u012B, English: the First Star of the Right Conductor.) In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Ramih al Ramih (\u0631\u0645\u062D \u0627\u0644\u0631\u0627\u0645\u062D - rum\u1E25 al r\u0101mi\u1E25), which was translated into Latin as Lancea Lanceator, possibly meaning the lance of the lancer.\r\rThis star is a subgiant that has begun the process of evolving from a main sequence star into a red giant. It has about 1.7 times the mass of the Sun and 2.7 times the Sun\u0027s radius. The estimated age of this star is about 2.7 billion years. Based on its spectra, Eta Bootis has a significant excess of elements heavier than helium. In fact the ratio of iron to hydrogen is considered close to the upper limit for dwarf stars in the galactic disk. The star is a suspected spectroscopic binary with a reported period of 494 days, but the companion was not confirmed through speckle interferometry. This measurement does not rule out a low mass stellar companion of spectral class M7.\r\rEta Bootis appears close to the prominent star Arcturus (Alpha Bootis) in Earth\u0027s sky, and Arcturus is in fact its closest stellar neighbor, as both stars are nearly identical in distance from the Sun. The two stars are about 3.24 light years apart , and each would appear bright in the other\u0027s sky. Arcturus would appear as roughly magnitude -5.2 (about 120 times brighter than it appears from Earth, or close to twice the brightness of Venus) in the night sky of a hypothetical planet orbiting Eta Bootis, while Eta Bootis would appear at about magnitude -2.5 in the sky of a hypothetical planet orbiting Arcturus, or over twice the brightness of Sirius in our night sky",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "8 Bootis, Eta Bootis, HIP 67927, SAO 100766, HD 121370, GC 18805, HR 5235, DM BD+19  2725, TYC 1470-1157-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Muphrid / Saak",
	"OType" : "Spectroscopic binary",
	"Distance" : "11.34",
	"RA_S" : 208.67116217,
	"DEC_S" : 18.39772072,
	"X" : 538,
	"Y" : 519,
	"Constellation" : "Bootes ",
	"AMag" : 2.719,
	"key" : 23936,
	"shortTitle" : "Muphrid; Mufride; Muphride; Mifrid",
	"title" : "Muphrid / Saak"
	},
{
	"Index" : "8392",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "9 Bootis, HIP 68103, SAO 83084, HD 121710, GC 18850, HR 5247, DM BD+28  2278, TYC 2002-1056-1",
	"group" : { "key" : "Bootes" },
	"Common" : "9 Bootis",
	"OType" : "Variable Star of irregular type",
	"Distance" : "177.89",
	"RA_S" : 209.14242039,
	"DEC_S" : 27.4920812,
	"Constellation" : "Bootes ",
	"AMag" : 5.167,
	"key" : 28392,
	"title" : "9 Bootis"
	},
{
	"Index" : "16964",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "HIP 69038, SAO 44901, HD 123657, GC 19084, HR 5299, DM BD+44 2325, TYC 3040-969-1",
	"group" : { "key" : "Bootes" },
	"Common" : "HR 5299",
	"OType" : "Long Period Variable candidate",
	"Distance" : "156.92",
	"RA_S" : 211.98231278,
	"DEC_S" : 43.85445186,
	"Constellation" : "Bootes ",
	"AMag" : 5.394,
	"key" : 36964,
	"title" : "HR 5299"
	},
{
	"Index" : "20737",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "13 Bootis, HIP 69068, SAO 44905, HD 123782, GC 19095, HR 5300, DM BD+50  2047, TYC 3468-1122-1",
	"group" : { "key" : "Bootes" },
	"Common" : "13 Bootis",
	"OType" : "Long-period variable star",
	"Distance" : "167.99",
	"RA_S" : 212.07209399,
	"DEC_S" : 49.4581709,
	"Constellation" : "Bootes ",
	"AMag" : 5.452,
	"key" : 40737,
	"title" : "13 Bootis"
	},
{
	"Index" : "8441",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "12 Bootis, d Bootis, HIP 69226, SAO 83203, HD 123999, GC 19127, HR 5304, DM BD+25  2737, TYC 2010-1245-1",
	"group" : { "key" : "Bootes" },
	"Common" : "d Bootis",
	"OType" : "Spectroscopic binary",
	"Distance" : "37.42",
	"RA_S" : 212.59972001,
	"DEC_S" : 25.09167937,
	"Constellation" : "Bootes ",
	"AMag" : 4.868,
	"key" : 28441,
	"title" : "d Bootis"
	},
{
	"Index" : "20754",
	"Description" : "Kappa Bootis (\u03BA Boo, \u03BA Bootis) is a double star in the constellation Bootes. It has the traditional name Asellus Tertius (Latin for \u0022third donkey colt\u0022) and the Flamsteed designation 17 Bootis. The components are separated by an angular distance of 13.4, viewable in a small telescope. Kappa Bootis is approximately 155 light years from Earth.\r\rThis star, along with the other Aselli (\u03B8 Boo and \u03B9 Boo) and \u03BB Boo, were Al Aul\u0101d al Dhi\u02BCbah (\u0623\u0644\u0639\u0648\u0644\u062F \u0623\u0644\u0630\u0639\u0628 - al aul\u0101d al dhi\u02BCb), \u0022the Whelps of the Hyenas\u0022.\r\rIn Chinese, \u6897\u6CB3 (Ti\u0101n Qi\u0101ng), meaning Celestial Spear, refers to an asterism consisting of \u03BA (actually \u03BA2) Bootis, \u03B9 Bootis and \u03B8 Bootis. Consequently, \u03B8 Bootis itself is known as \u5929\u69CD\u4E00 (Ti\u0101n Qi\u0101ng y\u012B, English: the First Star of Celestial Spear.)",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "17 Bootis, Kappa02 Bootis, HIP 69483A, SAO 29046, HD 124675, GC 19207, HR 5329, DM BD+52  1782A, TYC 3471-1250-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Asellus Tertius",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "50.04",
	"RA_S" : 213.37086263,
	"DEC_S" : 51.78996582,
	"X" : 463,
	"Y" : 88,
	"Constellation" : "Bootes ",
	"AMag" : 4.535,
	"key" : 40754,
	"title" : "Asellus Tertius"
	},
{
	"Index" : "67696",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "15 Bootis, HIP 69612A, SAO 100934, HD 124679, GC 19226, HR 5330, DM BD+10  2654, TYC 905-1418-1",
	"group" : { "key" : "Bootes" },
	"Common" : "15 Bootis",
	"OType" : "Star",
	"Distance" : "81.01",
	"RA_S" : 213.71187569,
	"DEC_S" : 10.10060559,
	"Constellation" : "Bootes ",
	"AMag" : 5.439,
	"key" : 87696,
	"title" : "15 Bootis"
	},
{
	"Index" : "3958",
	"Description" : "Arcturus (pron.: /\u0251rk\u02C8tj\u028A\u0259r\u0259s/; \u03B1 Boo, \u03B1 Bootis, Alpha Bootis) is the brightest star in the constellation Bootes and the northern celestial hemisphere. With a visual magnitude of \u22120.04, it is the fourth brightest star in the night sky, after \u22121.46 magnitude Sirius, \u22120.86 magnitude Canopus, and \u22120.27 magnitude Alpha Centauri. It is a relatively close star at only 36.7 light-years from Earth, and, together with Vega and Sirius, one of the most luminous stars in the Sun\u0027s neighborhood.\r\rA type K1.5 IIIpe orange giant star, with an absolute magnitude of -0.30. It has likely exhausted its hydrogen and has begun fusing helium into oxygen and carbon in its core. It will continue to expand before sloughing off its outer shell and ending its life as a white dwarf inside a planetary nebula.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "16 Bootis, Alpha Bootis, HIP 69673B, SAO 100944, HD 124897, GC 19242, HR 5340, DM BD+19  2777, TYC 1472-1436-2",
	"group" : { "key" : "Bootes" },
	"Common" : "Arcturus",
	"OType" : "Red Giant Branch star",
	"Distance" : "11.26",
	"RA_S" : 213.91530029,
	"DEC_S" : 19.18240916,
	"X" : 473,
	"Y" : 512,
	"Constellation" : "Bootes ",
	"key" : 23958,
	"shortTitle" : "Haris-el-sema; Arktur",
	"title" : "Arcturus"
	},
{
	"Index" : "20808",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "21 Bootis, Iota Bootis, HIP 69713, SAO 29071, HD 125161, GC 19269, HR 5350, DM BD+52  1784, TYC 3478-1333-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Asellus Secondus",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "29.07",
	"RA_S" : 214.04137107,
	"DEC_S" : 51.36723206,
	"Constellation" : "Bootes ",
	"AMag" : 4.763,
	"key" : 40808,
	"title" : "Asellus Secondus"
	},
{
	"Index" : "20761",
	"Description" : "Lambda Bootis (\u03BB Boo, \u03BB Bootis) is a star in the constellation Bootes.\r\rLambda Bootis is a white A-type main sequence dwarf with an apparent magnitude of +4.18. It is approximately 97.1 light-years from Earth. Lambda Bootis is the prototype of a group of rare stars known as Lambda Bootis stars, all of which are dwarf stars with unusually low abundances of metals in their spectra. Its diameter has been directly measured to be 1.7 times that of the Sun.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "19 Bootis, Lambda Bootis, HIP 69732, SAO 44965, HD 125162, GC 19273, HR 5351, DM BD+46  1949, TYC 3472-1264-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Lambda Bootis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "30.36",
	"RA_S" : 214.09591297,
	"DEC_S" : 46.08830597,
	"X" : 460,
	"Y" : 162,
	"Constellation" : "Bootes ",
	"AMag" : 4.181,
	"key" : 40761,
	"title" : "Lambda Bootis"
	},
{
	"Index" : "12694",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "A Bootis, HIP 69879, SAO 64053, HD 125351, GC 19296, HR 5361, DM BD+36  2468, TYC 2552-1081-1",
	"group" : { "key" : "Bootes" },
	"Common" : "A Bootis",
	"OType" : "Spectroscopic binary",
	"Distance" : "71.52",
	"RA_S" : 214.49924148,
	"DEC_S" : 35.50950229,
	"Constellation" : "Bootes ",
	"AMag" : 4.913,
	"key" : 32694,
	"title" : "A Bootis"
	},
{
	"Index" : "68519",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "18 Bootis, HIP 69989, SAO 100975, HD 125451, GC 19319, HR 5365, DM BD+13  2782, TYC 915-1442-1",
	"group" : { "key" : "Bootes" },
	"Common" : "18 Bootis",
	"OType" : "Star",
	"Distance" : "26.09",
	"RA_S" : 214.81783774,
	"DEC_S" : 13.00429686,
	"Constellation" : "Bootes ",
	"AMag" : 5.443,
	"key" : 88519,
	"title" : "18 Bootis"
	},
{
	"Index" : "3933",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "20 Bootis, HIP 70027, SAO 100980, HD 125560, GC 19334, HR 5370, DM BD+16  2637, TYC 1469-1455-1",
	"group" : { "key" : "Bootes" },
	"Common" : "20 Bootis",
	"OType" : "Variable Star",
	"Distance" : "57.33",
	"RA_S" : 214.93847695,
	"DEC_S" : 16.30695159,
	"Constellation" : "Bootes ",
	"AMag" : 4.981,
	"key" : 23933,
	"title" : "20 Bootis"
	},
{
	"Index" : "68012",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "HIP 70327A, TYC 909-1493-1",
	"group" : { "key" : "Bootes" },
	"Common" : "HR 5386",
	"OType" : "Double or multiple star",
	"Distance" : "65.82",
	"RA_S" : 215.84455956,
	"DEC_S" : 8.44664538,
	"Constellation" : "Bootes ",
	"AMag" : 5.035,
	"key" : 88012,
	"title" : "HR 5386"
	},
{
	"Index" : "20807",
	"Description" : "Theta Bootis (\u03B8 Boo, \u03B8 Bootis) is a star in the constellation Bootes. It has the traditional name Asellus Primus (Latin for \u0022first donkey colt\u0022) and the Flamsteed designation 23 Bootis.\r\rThis star, along with the other Aselli (\u03B9 Boo and \u03BA Boo) and \u03BB Boo, were Al Aul\u0101d al Dhi\u02BCbah (\u0623\u0644\u0639\u0648\u0644\u062F \u0623\u0644\u0630\u0639\u0628 - al aul\u0101d al dhi\u02BCb), \u0022the Whelps of the Hyenas\u0022.\r\rIn Chinese, \u5929\u67AA (Ti\u0101n Qi\u0101ng), meaning Celestial Spear, refers to an asterism consisting of \u03B8 Bootis, \u03BA2 Bootis and \u03B9 Bootis. Consequently, \u03B8 Bootis itself is known as \u5929\u67AA\u4E09 (Ti\u0101n Qi\u0101ng s\u0101n, English: the Third Star of Celestial Spear.)",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "23 Bootis, Theta Bootis, HIP 70497, SAO 29137, HD 126660, GC 19467, HR 5404, DM BD+52  1804, TYC 3478-1332-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Asellus Primus",
	"OType" : "Variable Star",
	"Distance" : "14.53",
	"RA_S" : 216.29914965,
	"DEC_S" : 51.85074211,
	"X" : 439,
	"Y" : 88,
	"Constellation" : "Bootes ",
	"AMag" : 4.1,
	"key" : 40807,
	"title" : "Asellus Primus"
	},
{
	"Index" : "4006",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "22 Bootis, f Bootis, HIP 70602, SAO 101025, HD 126661, GC 19480, HR 5405, DM BD+19  2810, TYC 1479-1217-1",
	"group" : { "key" : "Bootes" },
	"Common" : "f Bootis",
	"OType" : "Star",
	"Distance" : "89.08",
	"RA_S" : 216.61401943,
	"DEC_S" : 19.22690148,
	"Constellation" : "Bootes ",
	"AMag" : 5.425,
	"key" : 24006,
	"title" : "f Bootis"
	},
{
	"Index" : "12702",
	"Description" : "Rho Bootis (\u03C1 Boo, \u03C1 Bootis) is a star in the northern constellation Bootes. Based upon parallax measurements, it is located at a distance of approximately 149 light-years (46 parsecs) from Earth.\r\rThis is an orange K-type giant with an apparent magnitude of +3.57. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. There is an optical companion, an eleventh magnitude star, located 42 arcseconds away.\r\rIn Chinese, \u6897\u6CB3 (G\u011Bng H\u00E9), meaning Celestial Lance, refers to an asterism consisting of \u03C1 Bootis, \u03B5 Bootis and \u03C3 Bootis. Consequently, \u03C1 Bootis itself is known as \u6897\u6CB3\u4E09 (G\u011Bng H\u00E9 s\u0101n, English: the Third Star of Celestial Lance.)",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "25 Bootis, Rho Bootis, HIP 71053, SAO 64202, HD 127665, GC 19597, HR 5429, DM BD+31  2628, TYC 2553-1140-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Rho Bootis",
	"OType" : "Variable Star",
	"Distance" : "49.09",
	"RA_S" : 217.95745423,
	"DEC_S" : 30.37143819,
	"X" : 424,
	"Y" : 368,
	"Constellation" : "Bootes ",
	"AMag" : 3.71,
	"key" : 32702,
	"title" : "Rho Bootis"
	},
{
	"Index" : "16937",
	"Description" : "Gamma Bootis (\u03B3 Boo, \u03B3 Bootis) is a star in the constellation Bootes. It has the traditional name Seginus (also Segin, Ceginus) of uncertain origin. It was listed as Haris in Be\u010Dv\u00E1\u0159.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "27 Bootis, Gamma Bootis, HIP 71075, SAO 64203, HD 127762, GC 19607, HR 5435, DM BD+38  2565, TYC 3036-1151-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Seginus",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "26.61",
	"RA_S" : 218.01946582,
	"DEC_S" : 38.30825118,
	"X" : 424,
	"Y" : 264,
	"Constellation" : "Bootes ",
	"AMag" : 3.043,
	"key" : 36937,
	"shortTitle" : "Haris; Ceginus (also HD139641); Segin",
	"title" : "Seginus"
	},
{
	"Index" : "8526",
	"Description" : "Sigma Bootis (\u03C3 Boo, \u03C3 Bootis) is a star in the constellation Bootes.\r\rSigma Bootis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.47. It is approximately 50.4 light years from Earth.\r\rIn Chinese, \u6897\u6CB3 (G\u011Bng H\u00E9), meaning Celestial Lance, refers to an asterism consisting of \u03C3 Bootis, \u03B5 Bootis and \u03C1 Bootis. Consequently, \u03C3 Bootis itself is known as \u6897\u6CB3\u4E8C (G\u011Bng H\u00E9 \u00E8r, English: the Second Star of Celestial Lance.)\r\rLocated to the southeast of Rho Bootis, the fusing dwarf Sigma may at first appear as a naked-eye double, but the angular proximity with Rho is merely line-of-sight. Like many of its spectral class, Sigma is apparently a variable of the Delta Scuti variety, which vary subtly with multiple periods of hours.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "28 Bootis, Sigma Bootis, HIP 71284, SAO 83416, HD 128167, GC 19659, HR 5447, DM BD+30  2536, TYC 2021-1323-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Sigma Bootis",
	"OType" : "Variable Star",
	"Distance" : "15.83",
	"RA_S" : 218.67007062,
	"DEC_S" : 29.74512688,
	"X" : 416,
	"Y" : 376,
	"Constellation" : "Bootes ",
	"AMag" : 4.501,
	"key" : 28526,
	"title" : "Sigma Bootis"
	},
{
	"Index" : "16972",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "33 Bootis, HIP 71618, SAO 45153, HD 129002, GC 19747, HR 5468, DM BD+45  2204, TYC 3042-1023-1",
	"group" : { "key" : "Bootes" },
	"Common" : "33 Bootis",
	"OType" : "Star",
	"Distance" : "56.98",
	"RA_S" : 219.70927435,
	"DEC_S" : 44.40450064,
	"Constellation" : "Bootes ",
	"AMag" : 5.39,
	"key" : 36972,
	"title" : "33 Bootis"
	},
{
	"Index" : "3997",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "29 Bootis, Pi-1 Bootis, HIP 71762A, TYC 1477-1336-1",
	"group" : { "key" : "Bootes" },
	"Common" : "29 Pi-1 Bootis (HR 5475)",
	"OType" : "Star in double system",
	"Distance" : "96.37",
	"RA_S" : 220.18153253,
	"DEC_S" : 16.41834243,
	"Constellation" : "Bootes ",
	"AMag" : 4.877,
	"key" : 23997,
	"title" : "29 Pi-1 Bootis (HR 5475)"
	},
{
	"Index" : "3998",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "29 Bootis, Pi01 Bootis, HIP 71762B, SAO 101138, HD 129174, GC 19769, HR 5475, DM BD+17  2768A, TYC 1477-1337-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Pi01 Bootis",
	"OType" : "Star in double system",
	"Distance" : "96.37",
	"RA_S" : 220.1815326,
	"DEC_S" : 16.41832478,
	"Constellation" : "Bootes ",
	"AMag" : 4.49,
	"key" : 23998,
	"title" : "Pi01 Bootis"
	},
{
	"Index" : "68678",
	"Description" : "Zeta Bootis (\u03B6 Boo, \u03B6 Bootis) is a binary star system in the constellation of Bootes that consists of two giant stars with matching stellar classifications of A2III. They have the Flamsteed designation 30 Bootis. This system is approximately 180 light years from Earth and has a combined apparent magnitude of +3.78. The individual magnitudes differ slightly, with component A having a magnitude of 4.43 and component B at the slightly dimmer magnitude 4.83.\r\rThe binary nature of this system has been tracked since 1796. They complete an orbit roughly every 45,460 days, or 124.46 years. The next close approach will occur during August 2023. The orbit of this pair has a very high eccentricity of 0.9977, bringing the stars within 0.3 AU at their closest approach.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "30 Bootis, Zeta Bootis, HIP 71795B, SAO 101145, HD 129246, GC 19777, HR 5477, DM BD+14  2770B, TYC 917-1471-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Zeta Bootis",
	"OType" : "Star",
	"Distance" : "53.77",
	"RA_S" : 220.28722647,
	"DEC_S" : 13.7283469,
	"X" : 393,
	"Y" : 583,
	"Constellation" : "Bootes ",
	"AMag" : 4.464,
	"key" : 88678,
	"title" : "Zeta Bootis"
	},
{
	"Index" : "68679",
	"Description" : "Zeta Bootis (\u03B6 Boo, \u03B6 Bootis) is a binary star system in the constellation of Bootes that consists of two giant stars with matching stellar classifications of A2III. They have the Flamsteed designation 30 Bootis. This system is approximately 180 light years from Earth and has a combined apparent magnitude of +3.78. The individual magnitudes differ slightly, with component A having a magnitude of 4.43 and component B at the slightly dimmer magnitude 4.83.\r\rThe binary nature of this system has been tracked since 1796. They complete an orbit roughly every 45,460 days, or 124.46 years. The next close approach will occur during August 2023. The orbit of this pair has a very high eccentricity of 0.9977, bringing the stars within 0.3 AU at their closest approach.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "30 Bootis, Zeta Bootis, HIP 71795A, SAO 101145, HD 129247, HR 5478, DM BD+14  2770A, TYC 917-1471-2",
	"group" : { "key" : "Bootes" },
	"Common" : "Zeta Bootis",
	"OType" : "Star",
	"Distance" : "53.77",
	"RA_S" : 220.28722647,
	"DEC_S" : 13.7283469,
	"X" : 393,
	"Y" : 583,
	"Constellation" : "Bootes ",
	"AMag" : 4.554,
	"key" : 88679,
	"title" : "Zeta Bootis"
	},
{
	"Index" : "68150",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "31 Bootis, HIP 71832, SAO 120601, HD 129312, GC 19789, HR 5480, DM BD+08  2903, TYC 911-1708-1",
	"group" : { "key" : "Bootes" },
	"Common" : "31 Bootis",
	"OType" : "Variable Star",
	"Distance" : "164.16",
	"RA_S" : 220.41146061,
	"DEC_S" : 8.16176273,
	"Constellation" : "Bootes ",
	"AMag" : 4.973,
	"key" : 88150,
	"title" : "31 Bootis"
	},
{
	"Index" : "8512",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "34 Bootis, W Bootis, HIP 71995, SAO 83488, HD 129712, GC 19831, HR 5490, DM BD+27  2413, TYC 2019-1252-1",
	"group" : { "key" : "Bootes" },
	"Common" : "W Bootis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "215.04",
	"RA_S" : 220.85567784,
	"DEC_S" : 26.52785236,
	"Constellation" : "Bootes ",
	"AMag" : 5.003,
	"key" : 28512,
	"title" : "W Bootis"
	},
{
	"Index" : "8510",
	"Description" : "Epsilon Bootis (\u03B5 Boo, \u03B5 Bootis) is a double star in the northern constellation of Bootes. It has the traditional names Izar and Pulcherrima. The star system can be viewed with the unaided eye at night, but resolving the pair with a small telescope is challenging; an aperture of 76 mm (3.0 in) or greater is required.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "36 Bootis, Epsilon Bootis, HIP 72105B, HD 129988, GC 19856, HR 5505, DM BD+27  2417B, TYC 2019-1250-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Epsilon Bootis",
	"OType" : "Star",
	"Distance" : "61.99",
	"RA_S" : 221.246583,
	"DEC_S" : 27.074928,
	"X" : 385,
	"Y" : 409,
	"Constellation" : "Bootes ",
	"AMag" : 4.808,
	"key" : 28510,
	"shortTitle" : "Mirak (also HD6860,95418); Pulcherrima",
	"title" : "Epsilon Bootis"
	},
{
	"Index" : "8511",
	"Description" : "Epsilon Bootis (\u03B5 Boo, \u03B5 Bootis) is a double star in the northern constellation of Bootes. It has the traditional names Izar and Pulcherrima. The star system can be viewed with the unaided eye at night, but resolving the pair with a small telescope is challenging; an aperture of 76 mm (3.0 in) or greater is required.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "36 Bootis, Epsilon Bootis, HIP 72105A, SAO 83500, HD 129989, GC 19856, HR 5506, DM BD+27  2417A, TYC 2019-1251-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Epsilon Bootis",
	"OType" : "High proper-motion Star",
	"Distance" : "61.99",
	"RA_S" : 221.24676327,
	"DEC_S" : 27.0742078,
	"X" : 385,
	"Y" : 409,
	"Constellation" : "Bootes ",
	"AMag" : 2.578,
	"key" : 28511,
	"shortTitle" : "Mirac (also HD6860); Mirak (also HD6860,95418);; Mirach; Mizar (see HD6860,116656); Pulcherrima",
	"title" : "Epsilon Bootis"
	},
{
	"Index" : "3999",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "35 Bootis, Omicron Bootis, HIP 72125, SAO 101184, HD 129972, GC 19858, HR 5502, DM BD+17  2780, TYC 1477-189-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Omicron Bootis",
	"OType" : "Star",
	"Distance" : "74.49",
	"RA_S" : 221.31025369,
	"DEC_S" : 16.96427649,
	"Constellation" : "Bootes ",
	"AMag" : 4.71,
	"key" : 23999,
	"title" : "Omicron Bootis"
	},
{
	"Index" : "4034",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "37 Bootis, Xi Bootis, HIP 72659A, SAO 101250, HD 131156A, GC 19991, HR 5544, DM BD+19  2870, TYC 1481-722-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Xi Bootis",
	"OType" : "High proper-motion Star",
	"Distance" : "6.71",
	"RA_S" : 222.847025,
	"DEC_S" : 19.100625,
	"Constellation" : "Bootes ",
	"AMag" : 4.757,
	"key" : 24034,
	"title" : "Xi Bootis"
	},
{
	"Index" : "17006",
	"Description" : "Beta Bootis (\u03B2 Boo, \u03B2 Bootis) is the Bayer designation for a star in the northern constellation of Bootes. It has an apparent visual magnitude of 3.5, making it one of the brighter members of the constellation. The traditional name Nakkar or Nekkar for this star is based upon the Arabic name for the constellation. This is a mis-transliteration of the Arabic \u0628\u0642\u0651\u0627\u0631 baqq\u0101r \u0022cattle driver\u0022, the Arabic letters b and n differing only in the placement of the dot. In the modern constellation, it marks the head of Bootis the herdsman. Based upon parallax measurements, this star is approximately 225 light-years (69 parsecs) from Earth. At that distance, the magnitude of the star is reduced by 0.06 from extinction caused by intervening gas and dust.\r\rNakkar has more than three times the mass of the Sun and greater than 21 times the Sun\u0027s radius. (Konig et al. (2006) give it 3.4 solar masses, while Tetzlaff et al. (2011) list a higher estimated mass of 5.0 \u00B1 1.5 solar masses and Takeda et al. (2008) show it as 3.24 solar masses.) At the estimated age of 240\u2013251 million years, it has evolved into a giant star with a stellar classification of G8 IIIa. The star is radiating around 170\u2013194 times as much luminosity as the Sun from its outer envelope at an effective temperature of 4,932 K. This heat gives it the yellow-hued glow of a G-type star. It has an estimated rotation period of about 200 days and the pole is inclined 28\u00B0 \u00B1 6\u00B0 to the line of sight from the Earth.\r\rIn 1993, the ROSAT satellite was used to observe an X-ray flare on Beta Bootis, which released an estimated 1.7 \u00D7 1032 erg. This was the first such observation for a low-activity star of this type. The flare may be explained by an as yet unobserved M-type dwarf companion star.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "42 Bootis, Beta Bootis, HIP 73555, SAO 45337, HD 133208, GC 20226, HR 5602, DM BD+40  2840, TYC 3047-1258-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Nakkar",
	"OType" : "Flare Star",
	"Distance" : "69.05",
	"RA_S" : 225.48650868,
	"DEC_S" : 40.39056814,
	"X" : 349,
	"Y" : 234,
	"Constellation" : "Bootes ",
	"AMag" : 3.577,
	"key" : 37006,
	"shortTitle" : "Merez; Meres; Merets",
	"title" : "Nakkar"
	},
{
	"Index" : "8519",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "41 Bootis, Omega Bootis, HIP 73568, SAO 83624, HD 133124, GC 20224, HR 5600, DM BD+25  2861, TYC 2020-1409-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Omega Bootis",
	"OType" : "Star",
	"Distance" : "113.76",
	"RA_S" : 225.52711771,
	"DEC_S" : 25.00814033,
	"Constellation" : "Bootes ",
	"AMag" : 4.965,
	"key" : 28519,
	"title" : "Omega Bootis"
	},
{
	"Index" : "20861",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "44 Bootis, i Bootis, HIP 73695A, SAO 45357, HD 133640A, GC 20281, HR 5618, DM BD+48  2259, TYC 3484-1580-1",
	"group" : { "key" : "Bootes" },
	"Common" : "i Bootis",
	"OType" : "High proper-motion Star",
	"Distance" : "12.75",
	"RA_S" : 225.94708662,
	"DEC_S" : 47.65404245,
	"Constellation" : "Bootes ",
	"AMag" : 5.203,
	"key" : 40861,
	"title" : "i Bootis"
	},
{
	"Index" : "8564",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "43 Bootis, Psi Bootis, HIP 73745, SAO 83645, HD 133582, GC 20285, HR 5616, DM BD+27  2447, TYC 2027-1405-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Psi Bootis",
	"OType" : "High proper-motion Star",
	"Distance" : "75.38",
	"RA_S" : 226.1114234,
	"DEC_S" : 26.94764897,
	"Constellation" : "Bootes ",
	"AMag" : 4.653,
	"key" : 28564,
	"title" : "Psi Bootis"
	},
{
	"Index" : "24301",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "HIP 73909, SAO 29407, HD 134190, GC 20332, HR 5635, DM BD+55 1730, TYC 3861-1445-1",
	"group" : { "key" : "Bootes" },
	"Common" : "HR 5635",
	"OType" : "Star",
	"Distance" : "78.91",
	"RA_S" : 226.56965356,
	"DEC_S" : 54.55631929,
	"Constellation" : "Bootes ",
	"AMag" : 5.355,
	"key" : 44301,
	"title" : "HR 5635"
	},
{
	"Index" : "8546",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "45 Bootis, c Bootis, HIP 73996, SAO 83671, HD 134083, GC 20342, HR 5634, DM BD+25  2873, TYC 2024-1355-1",
	"group" : { "key" : "Bootes" },
	"Common" : "c Bootis",
	"OType" : "Variable Star",
	"Distance" : "19.55",
	"RA_S" : 226.82527678,
	"DEC_S" : 24.86919657,
	"Constellation" : "Bootes ",
	"AMag" : 4.974,
	"key" : 28546,
	"title" : "c Bootis"
	},
{
	"Index" : "8587",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "48 Bootis, Chi Bootis, HIP 74596, SAO 83729, HD 135502, GC 20495, HR 5676, DM BD+29  2640, TYC 2030-1317-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Chi Bootis",
	"OType" : "Star",
	"Distance" : "77.36",
	"RA_S" : 228.62149401,
	"DEC_S" : 29.16429616,
	"Constellation" : "Bootes ",
	"AMag" : 5.279,
	"key" : 28587,
	"title" : "Chi Bootis"
	},
{
	"Index" : "12792",
	"Description" : "Delta Bootis (\u03B4 Boo, \u03B4 Bootis) is a double star in the northern constellation Bootes. Based upon parallax measurements, it is located at a distance of approximately 121.8 light-years (37.3 parsecs) from the Earth. This star is sometimes called Princeps, meaning prince or prime in Latin. The origin of this name is unclear, although it usually appears in an astrological context. The It has an apparent visual magnitude of this star is 3.5, making it visible to the naked eye even during a Full Moon.\r\rIn Chinese, \u4E03\u516C (Q\u012B G\u014Dng), meaning Seven Excellencies, refers to an asterism consisting of \u03B4 Bootis, 42 Herculis, \u03C4 Herculis, \u03C6 Herculis, \u03C7 Herculis, \u03BD1 Bootis and \u03BC1 Bootis. Consequently, \u03B4 Bootis itself is known as \u4E03\u516C\u4E03 (Q\u012B G\u014Dng q\u012B, English: the Seventh Star of Seven Excellencies.)",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "49 Bootis, Delta Bootis, HIP 74666, SAO 64589, HD 135722, GC 20523, HR 5681, DM BD+33  2561, TYC 2566-1639-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Princeps",
	"OType" : "Star",
	"Distance" : "37.34",
	"RA_S" : 228.87567834,
	"DEC_S" : 33.31483226,
	"X" : 306,
	"Y" : 323,
	"Constellation" : "Bootes ",
	"AMag" : 3.563,
	"key" : 32792,
	"title" : "Princeps"
	},
{
	"Index" : "12793",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "50 Bootis, HIP 75178, SAO 64656, HD 136849, GC 20672, HR 5718, DM BD+33  2581, TYC 2566-1640-1",
	"group" : { "key" : "Bootes" },
	"Common" : "50 Bootis",
	"OType" : "Star",
	"Distance" : "80.29",
	"RA_S" : 230.45239551,
	"DEC_S" : 32.93369512,
	"Constellation" : "Bootes ",
	"AMag" : 5.362,
	"key" : 32793,
	"title" : "50 Bootis"
	},
{
	"Index" : "12816",
	"Description" : "Mu Bootis (\u03BC Boo, \u03BC Bootis) is a triple star system in the constellation Bootes. It has the traditional name Alkalurops (also Inkalunis, Clava, and Venabulum), and the Flamsteed designation 51 Bootis. Mu Bootis is approximately 121 light-years from Earth.\r\rThe name Alkalurops is from Greek \u03BA\u03B1\u03BB\u03B1\u03CD\u03C1\u03BF\u03C8 kalaurops \u0022shepherd\u0027s staff\u0022, through the Arabic.\r\rIt is known as \u4E03\u516C\u516D (the Sixth Star of the Seven Excellencies) in Chinese.\r\rThe primary component, \u03BC\u00B9 Bootis, is a yellow-white F-type subgiant with an apparent magnitude of +4.31.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "51 Bootis, Mu01 Bootis, HIP 75411, SAO 64686, HD 137391, GC 20724, HR 5733, DM BD+37  2636, TYC 2570-1521-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Alkalurops",
	"OType" : "Double or multiple star",
	"Distance" : "37.07",
	"RA_S" : 231.12261791,
	"DEC_S" : 37.3771697,
	"X" : 288,
	"Y" : 267,
	"Constellation" : "Bootes ",
	"AMag" : 4.334,
	"key" : 32816,
	"shortTitle" : "Inkalunis; Icalurus; Clava; Venabulum",
	"title" : "Alkalurops"
	},
{
	"Index" : "17062",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "52 Bootis, Nu01 Bootis, HIP 75973, SAO 45580, HD 138481, GC 20866, HR 5763, DM BD+41  2609, TYC 3055-2341-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Nu01 Bootis",
	"OType" : "Star",
	"Distance" : "255.8",
	"RA_S" : 232.73232707,
	"DEC_S" : 40.83304841,
	"Constellation" : "Bootes ",
	"AMag" : 5.219,
	"key" : 37062,
	"title" : "Nu01 Bootis"
	},
{
	"Index" : "17061",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "53 Bootis, Nu02 Bootis, HIP 76041, SAO 45590, HD 138629, GC 20883, HR 5774, DM BD+41  2611, TYC 3055-2340-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Nu02 Bootis",
	"OType" : "Double or multiple star",
	"Distance" : "130.93",
	"RA_S" : 232.94574314,
	"DEC_S" : 40.89933676,
	"Constellation" : "Bootes ",
	"AMag" : 4.992,
	"key" : 37061,
	"title" : "Nu02 Bootis"
	},
{
	"Index" : "17068",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "54 Bootis, Phi Bootis, HIP 76534, SAO 45643, HD 139641, GC 21032, HR 5823, DM BD+40  2907, TYC 3056-1900-1",
	"group" : { "key" : "Bootes" },
	"Common" : "Ceginus (also HD127762)",
	"OType" : "Star",
	"Distance" : "52.02",
	"RA_S" : 234.45666065,
	"DEC_S" : 40.3534327,
	"Constellation" : "Bootes ",
	"AMag" : 5.353,
	"key" : 37068,
	"title" : "Ceginus (also HD127762)"
	},
{
	"Index" : "20890",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "HIP 76957, SAO 29628, HD 140728, GC 21154, HR 5857, DM BD+52 1898, TYC 3489-1587-1",
	"group" : { "key" : "Bootes" },
	"Common" : "HR 5857",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "91.55",
	"RA_S" : 235.7115011,
	"DEC_S" : 52.36090175,
	"Constellation" : "Bootes ",
	"AMag" : 5.473,
	"key" : 40890,
	"title" : "HR 5857"
	},
{
	"Index" : "53482",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Delta Caeli, HIP 21060, SAO 216850, HD 28873, GC 5527, HR 1443, DM CD-45  1567, TYC 7585-1480-1",
	"group" : { "backgroundImage" : "images/Alignment/10.png",
		"description" : "Caelum (pron.: /\u02C8si\u02D0l\u0259m/) is a faint constellation in the southern sky, introduced in the 1750s by Nicolas Louis de Lacaille. Its name means \u0022the chisel\u0022 in Latin, and it was formerly known as Caelum Scalptorium, \u0022the engraver\u0027s chisel\u0022. It is the eighth smallest constellation, with an area just less than that of Corona Australis.",
		"key" : "Caelum",
		"grouptype" : "Caelum",
		"Meaning" : "chisel",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Caelum",
		"title" : "Caelum Objects Group" },
	"Common" : "Delta Caeli",
	"OType" : "Star",
	"Distance" : "215.55",
	"RA_S" : 67.70875143,
	"DEC_S" : -44.95375186,
	"Constellation" : "Caelum ",
	"AMag" : 5.026,
	"key" : 73482,
	"title" : "Delta Caeli"
	},
{
	"Index" : "53514",
	"Description" : "Alpha Caeli (\u03B1 Cae, \u03B1 Caeli) is a double star system in the constellation Caelum.\r\rAlpha Caeli A is an F-type main sequence star with a stellar classification of F2V and an apparent magnitude of +4.44. It has 1.48 times the mass of the Sun and 1.3 times the solar radius. The projected rotational velocity at the stellar equator is 47.8 km/s. It is suspected of being a Delta Scuti variable star.\r\rThe companion is a spectral class M0.5V red dwarf star with absolute magnitude 9.80. It is a UV Ceti variable star that undergoes random increases in luminosity. This star is currently separated from the primary by an angle of 6.6 arcseconds, which indicates an orbit with a semimajor axis whose expected value is 206 AU.\r\rAlpha Caeli is approximately 65.7 light years from Earth and is an estimated 900 million years old. The space velocity components of this system are U = 10, V = 6 and W = -10 km/s. It is orbiting the Milky Way galaxy at an average distance of 8.006 kpc from the core and with an orbital eccentricity of 0.07. This orbit lies close to the galactic plane, and the system travels no more than 0.05 kpc above or below this plane. Alpha Caeli is probably a member of the Ursa Major moving group of stars that have similar kinematic properties and probably originated from the same star cluster.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Alpha Caeli, HIP 21770, SAO 216926, HD 29875A, GC 5708, HR 1502, DM CD-42  1587, TYC 7589-1693-1",
	"group" : { "key" : "Caelum" },
	"Common" : "Alpha Caeli",
	"OType" : "Star",
	"Distance" : "20.17",
	"RA_S" : 70.14046987,
	"DEC_S" : -41.86375152,
	"X" : 452,
	"Y" : 531,
	"Constellation" : "Caelum ",
	"AMag" : 4.479,
	"key" : 73514,
	"title" : "Alpha Caeli"
	},
{
	"Index" : "48906",
	"Description" : "Beta Caeli (\u03B2 Cae, \u03B2 Caeli) is the bayer designation for a star in the southern constellation of Caelum. It is categorized as an F-type main sequence star with an apparent magnitude of +5.04. Beta Caeli is approximately 90.2 light years from Earth and slightly over six times brighter than the Sun.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Beta Caeli, HIP 21861, SAO 195239, HD 29992, GC 5740, HR 1503, DM CD-37  1867, TYC 7045-130-1",
	"group" : { "key" : "Caelum" },
	"Common" : "Beta Caeli",
	"OType" : "High proper-motion Star",
	"Distance" : "28.66",
	"RA_S" : 70.51450153,
	"DEC_S" : -37.14429188,
	"X" : 460,
	"Y" : 469,
	"Constellation" : "Caelum ",
	"AMag" : 5.081,
	"key" : 68906,
	"title" : "Beta Caeli"
	},
{
	"Index" : "48990",
	"Description" : "Gamma1 Caeli (\u03B31 Cae, \u03B31 Caeli) is a double star in the constellation Caelum. It is approximately 185 light years from Earth. The brighter component is an orange K-type giant with an apparent magnitude of +4.55. The companion is an eighth magnitude star located 3.1 arcseconds away.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Gamma Caeli, HIP 23595B, SAO 195532, HD 32831B, GC 6212, HR 1652, DM CD-35  2089, TYC 7053-2046-2",
	"group" : { "key" : "Caelum" },
	"Common" : "Gamma1 Caeli",
	"OType" : "Star",
	"Distance" : "55.55",
	"RA_S" : 76.100437,
	"DEC_S" : -35.482344,
	"X" : 406,
	"Y" : 439,
	"Constellation" : "Caelum ",
	"AMag" : 8.167,
	"key" : 68990,
	"title" : "Gamma1 Caeli"
	},
{
	"Index" : "48989",
	"Description" : "Gamma1 Caeli (\u03B31 Cae, \u03B31 Caeli) is a double star in the constellation Caelum. It is approximately 185 light years from Earth. The brighter component is an orange K-type giant with an apparent magnitude of +4.55. The companion is an eighth magnitude star located 3.1 arcseconds away.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Gamma Caeli, HIP 23595A, SAO 195532, HD 32831A, GC 6212, HR 1652, DM CD-35  2089, TYC 7053-2046-1",
	"group" : { "key" : "Caelum" },
	"Common" : "Gamma1 Caeli",
	"OType" : "Star",
	"Distance" : "55.55",
	"RA_S" : 76.10167971,
	"DEC_S" : -35.48297548,
	"X" : 406,
	"Y" : 439,
	"Constellation" : "Caelum ",
	"AMag" : 4.711,
	"key" : 68989,
	"title" : "Gamma1 Caeli"
	},
{
	"Index" : "26126",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 15520, SAO 12704, HD 20336, GC 3947, HR 985, DM BD+65  340, TYC 4061-1593-1",
	"group" : { "backgroundImage" : "images/Alignment/11.png",
		"description" : "Camelopardalis (pron.: /k\u0259\u02CCm\u025Bl\u0259\u02C8p\u0251rd\u0259l\u0268s/) is a large but faint constellation in the northern sky. The constellation was introduced in 1612 (or 1613) by Petrus Plancius. Some older astronomy books give an alternative spelling of the name, Camelopardus.\r\rFirst attested in English in 1785, the word camelopardalis comes from Latin, and it is the romanisation of the Greek \u0022\u03BA\u03B1\u03BC\u03B7\u03BB\u03BF\u03C0\u03AC\u03C1\u03B4\u03B1\u03BB\u03B9\u03C2\u0022 meaning \u0022giraffe\u0022, from \u0022\u03BA\u03AC\u03BC\u03B7\u03BB\u03BF\u03C2\u0022 (kam\u0113los), \u0022camel\u0022 + \u0022\u03C0\u03AC\u03C1\u03B4\u03B1\u03BB\u03B9\u03C2\u0022 (pardalis), \u0022leopard\u0022, due to its having a long neck like a camel and spots like a leopard.",
		"key" : "Camelopardalis",
		"grouptype" : "Camelopardalis",
		"Meaning" : "giraffe",
		"Family" : "Ursa Major",
		"Origin" : "1613, Plancius[6]",
		"shortTitle" : "Camelopardalis",
		"title" : "Camelopardalis Objects Group" },
	"Common" : "HR 985",
	"OType" : "Be Star",
	"Distance" : "230.17",
	"RA_S" : 49.99697752,
	"DEC_S" : 65.65228816,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.712,
	"key" : 46126,
	"title" : "HR 985"
	},
{
	"Index" : "26101",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 15890, SAO 12743, HD 20797, GC 4034, HR 1009, DM BD+64  391, TYC 4057-2594-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "V* CQ Cam",
	"OType" : "Long-period variable star",
	"Distance" : "628.9308",
	"RA_S" : 51.16898977,
	"DEC_S" : 64.58599735,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.398,
	"key" : 46101,
	"title" : "V* CQ Cam"
	},
{
	"Index" : "23160",
	"Description" : "CS Camelopardalis (CS Cam) is a binary star in reflection nebulae vdB 14, in the constellation Camelopardalis. It was designated B Cam or 2H.Cam.\r\rThe primary component, CS Camelopardalis A, is a blue-white B-type supergiant with a mean apparent magnitude of 4.21m. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude 4.19m to 4.23m. Its companion, CS Camelopardalis B, is a magnitude 8.7m star located 2.9 arcseconds from the primary.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 16228A, SAO 24054, HD 21291, GC 4113, HR 1035, DM BD+59  660, TYC 3715-1248-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "CS Camelopardalis",
	"OType" : "Pulsating variable Star",
	"Distance" : "595.2381",
	"RA_S" : 52.26721649,
	"DEC_S" : 59.94033249,
	"X" : 456,
	"Y" : 466,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.233,
	"key" : 43160,
	"title" : "CS Camelopardalis"
	},
{
	"Index" : "23161",
	"Description" : "CS Camelopardalis (CS Cam) is a binary star in reflection nebulae vdB 14, in the constellation Camelopardalis. It was designated B Cam or 2H.Cam.\r\rThe primary component, CS Camelopardalis A, is a blue-white B-type supergiant with a mean apparent magnitude of 4.21m. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude 4.19m to 4.23m. Its companion, CS Camelopardalis B, is a magnitude 8.7m star located 2.9 arcseconds from the primary.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 16228B, SAO 24054, HD 21291, HR 1035, DM BD+59  660, TYC 3715-1248-2",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "CS Camelopardalis",
	"OType" : "Pulsating variable Star",
	"Distance" : "595.2381",
	"RA_S" : 52.26721649,
	"DEC_S" : 59.94033249,
	"X" : 456,
	"Y" : 466,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.21,
	"key" : 43161,
	"title" : "CS Camelopardalis"
	},
{
	"Index" : "23164",
	"Description" : "CE Camelopardalis is a variable star in reflection nebula VDB 15, in the constellation Camelopardalis. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 16281, SAO 24061, HD 21389, GC 4140, HR 1040, DM BD+58  607, TYC 3715-1250-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "CE Camelopardalis",
	"OType" : "Evolved supergiant star",
	"Distance" : "769.2308",
	"RA_S" : 52.47810052,
	"DEC_S" : 58.87874987,
	"X" : 460,
	"Y" : 479,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.642,
	"key" : 43164,
	"title" : "CE Camelopardalis"
	},
{
	"Index" : "23102",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 16292, SAO 24064, HD 21447, GC 4146, HR 1046, DM BD+54  684, TYC 3707-802-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1046",
	"OType" : "High proper-motion Star",
	"Distance" : "60.88",
	"RA_S" : 52.50076258,
	"DEC_S" : 55.45180995,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.103,
	"key" : 43102,
	"title" : "HR 1046"
	},
{
	"Index" : "26166",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 17296, SAO 12874, HD 22649, GC 4383, HR 1105, DM BD+62  597, TYC 4066-1732-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "V* BD Cam",
	"OType" : "Symbiotic Star",
	"Distance" : "158.68",
	"RA_S" : 55.53884942,
	"DEC_S" : 63.21680745,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.284,
	"key" : 46166,
	"title" : "V* BD Cam"
	},
{
	"Index" : "26174",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 17587, SAO 12891, HD 23089, GC 4470, HR 1129, DM BD+62  604, TYC 4067-1935-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1129",
	"OType" : "Star",
	"Distance" : "301.51",
	"RA_S" : 56.5097184,
	"DEC_S" : 63.34504678,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.894,
	"key" : 46174,
	"title" : "HR 1129"
	},
{
	"Index" : "28317",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 17854, SAO 5000, HD 23277, GC 4530, HR 1138, DM BD+70  257, TYC 4331-1936-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1138",
	"OType" : "Spectroscopic binary",
	"Distance" : "106.29",
	"RA_S" : 57.30723198,
	"DEC_S" : 70.87104592,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.405,
	"key" : 48317,
	"title" : "HR 1138"
	},
{
	"Index" : "26214",
	"Description" : "BE Camelopardalis (BE Cam) is a star in the constellation Camelopardalis.\r\rBE Camelopardalis is a red M-type bright giant with a mean apparent magnitude of +4.39. It is approximately 965 light years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +4.35 to +4.48.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 17884, SAO 12916, HD 23475, GC 4553, HR 1155, DM BD+65  369, TYC 4071-1894-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "BE Camelopardalis",
	"OType" : "Long-period variable star",
	"Distance" : "240.27",
	"RA_S" : 57.38034525,
	"DEC_S" : 65.52597221,
	"X" : 400,
	"Y" : 410,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.625,
	"key" : 46214,
	"title" : "BE Camelopardalis"
	},
{
	"Index" : "28354",
	"Description" : "Gamma Camelopardalis (\u03B3 Cam / \u03B3 Camelopardalis) is a star in the constellation Camelopardalis.\r\r\u03B3 Camelopardalis is a white A-type subgiant with an apparent magnitude of +4.59. It is approximately 335 light years from Earth.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "Gamma Camelopardalis, HIP 17959, SAO 5006, HD 23401, GC 4557, HR 1148, DM BD+70   259, TYC 4335-2106-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Gamma Camelopardalis",
	"OType" : "Star",
	"Distance" : "109.96",
	"RA_S" : 57.58962116,
	"DEC_S" : 71.33226447,
	"X" : 373,
	"Y" : 339,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.611,
	"key" : 48354,
	"title" : "Gamma Camelopardalis"
	},
{
	"Index" : "26147",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 18488A, TYC 4063-1714-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1205",
	"OType" : "Star",
	"Distance" : "448.4305",
	"RA_S" : 59.28467694,
	"DEC_S" : 61.10894213,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.248,
	"key" : 46147,
	"title" : "HR 1205"
	},
{
	"Index" : "26176",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 18505, SAO 12969, HD 24479, GC 4730, HR 1204, DM BD+62  628, TYC 4067-1937-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1204",
	"OType" : "Be Star",
	"Distance" : "110.48",
	"RA_S" : 59.35601583,
	"DEC_S" : 63.07226227,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.943,
	"key" : 46176,
	"title" : "HR 1204"
	},
{
	"Index" : "23275",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 19018, SAO 24384, HD 25291, GC 4858, HR 1242, DM BD+58  690, TYC 3730-1595-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1242",
	"OType" : "Star",
	"Distance" : "604.35",
	"RA_S" : 61.1131755,
	"DEC_S" : 59.15550714,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.086,
	"key" : 43275,
	"title" : "HR 1242"
	},
{
	"Index" : "23192",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 19949, SAO 24512, HD 26764, GC 5132, HR 1314, DM BD+53  750, TYC 3719-1538-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1314",
	"OType" : "Star",
	"Distance" : "99.75",
	"RA_S" : 64.17953927,
	"DEC_S" : 53.61179812,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.193,
	"key" : 43192,
	"title" : "HR 1314"
	},
{
	"Index" : "26229",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 20266, SAO 13098, HD 27022, GC 5199, HR 1327, DM BD+64  433, TYC 4073-1392-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 1327",
	"OType" : "Star",
	"Distance" : "97.79",
	"RA_S" : 65.16802447,
	"DEC_S" : 65.14044005,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.344,
	"key" : 46229,
	"title" : "HR 1327"
	},
{
	"Index" : "23290",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "3 Camelopardalis, HIP 21727, SAO 24743, HD 29317, GC 5658, HR 1467, DM BD+52   865, TYC 3732-1029-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "3 Camelopardalis",
	"OType" : "Cepheid variable Star",
	"Distance" : "128.27",
	"RA_S" : 69.97783736,
	"DEC_S" : 53.07953438,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.194,
	"key" : 43290,
	"title" : "3 Camelopardalis"
	},
{
	"Index" : "23291",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "2 Camelopardalis, HIP 21730ABC, SAO 24744, HD 29316, GC 5659, HR 1466, DM BD+53   794, TYC 3732-1030-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "2 Camelopardalis",
	"OType" : "Double or multiple star",
	"Distance" : "84.49",
	"RA_S" : 69.991821,
	"DEC_S" : 53.473228,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.451,
	"key" : 43291,
	"title" : "2 Camelopardalis"
	},
{
	"Index" : "23355",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "4 Camelopardalis, HIP 22287AD, SAO 24829, HD 30121, GC 5811, HR 1511, DM BD+56   973, TYC 3741-1602-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "4 Camelopardalis",
	"OType" : "Double or multiple star",
	"Distance" : "52.72",
	"RA_S" : 72.00111995,
	"DEC_S" : 56.75717769,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.306,
	"key" : 43355,
	"title" : "4 Camelopardalis"
	},
{
	"Index" : "26348",
	"Description" : "Alpha Camelopardalis (Alpha Cam, \u03B1 Camelopardalis, \u03B1 Cam) is a star in the constellation Camelopardalis, with an apparent visual magnitude of 4.301. It is the third brightest star in this not very prominent circumpolar constellation, the first and second brightest stars being \u03B2 Camelopardalis and CS Camelopardalis, respectively.It is the farthest constellational star, with a distance of 6000 light-years from Earth.\r\rThis star has a stellar classification of O9.5Iae, with the \u0027Ia\u0027 indicating that it is an O-type luminous supergiant and the \u0027e\u0027 showing that there are emission lines in its spectrum. It is a massive star with 43 times the mass of the Sun and 37 times the Sun\u0027s radius. The effective temperature of the outer envelope is 27,700 K; much hotter than the Sun\u0027s effective temperature of 5,778 K, giving it the characteristic blue hue of an O-type star. It is emitting 680,000 times the luminosity of the Sun and is a weak X-ray emitter.\r\rThis star shows multiple patterns of variability. It may be a non-radial pulsating variable star, which is causing changes in the spectrum being emitted by the photosphere. The absorption lines in the optical spectrum show radial velocity variations, although there is significant uncertainty about the period. Estimates range from a period as low as 0.36 days up to 2.93 days. The stellar wind from this star is not smooth and continuous, but instead shows a behavior indicating clumping at both large and small scales. This star is losing mass rapidly through its stellar wind at a rate of approximately 6.3 \u00D7 10\u22126 solar masses per year, or the equivalent of the mass of the Sun every 160,000 years.\r\rIn 1968, this star was classified as a spectroscopic binary, indicating that it has an orbiting stellar companion with a period of 3.68 days and an orbital eccentricity of 0.45. Subsequent studies refined the period to 3.24 days. However, in 2006 it was recognized that the changes in the spectrum were probably the result of changes in the atmosphere or stellar wind, so it is more likely a single star. Speckle interferometery observations with the 3.67 m Advanced Electro Optical System Telescope at the Haleakala Observatory failed to detect a secondary component.\r\rIn 1961, based on the criteria that the proper motion of this star indicates a space velocity of greater than 30 km/s, Alpha Camelopardalis was suggested as a candidate runaway star that had been ejected from the cluster NGC 1502. This was based upon the kinematic properties of the star and cluster, as well as the location of this star at a high galactic latitude in an area otherwise lacking in stellar associations. Over the course of a million years, this star should have moved only 1.4\u00B0 across the sky, while it was estimated as being only two million years old. It has been suggested as a runaway star ejected from the OB association Camelopardalis OB1, but subsequent observations cast doubt on this.\r\rRunaway stars such as this with a stellar wind that is moving at supersonic velocity through the interstellar medium have their wind confined by a bow shock due to ram pressure. The dust in this bow shock can be detected using an infrared telescope. Just such a bow shock was observed with NASA\u0027s Wide-field Infrared Survey Explorer, or WISE. The star is traveling at a rate of somewhere between 680 and 4,200 kilometers per second: between 1.5 and 9.4 million mph.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "9 Camelopardalis, Alpha Camelopardalis, HIP 22783, SAO 13298, HD 30614, GC 5924, HR 1542, DM BD+66   358, TYC 4091-2094-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Alpha Camelopardalis",
	"OType" : "Blue supergiant star",
	"RA_S" : 73.51254332,
	"DEC_S" : 66.3426768,
	"X" : 315,
	"Y" : 419,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.292,
	"key" : 46348,
	"title" : "Alpha Camelopardalis"
	},
{
	"Index" : "23305",
	"Description" : "7 Camelopardalis is a triple star system in the constellation Camelopardalis. It is approximately 376 light years from Earth.\r\rThe primary component, 7 Camelopardalis A, is a white A-type main sequence dwarf with an apparent magnitude of +4.43. Orbiting the primary with a period of 284 years is 7 Camelopardalis B, a magnitude +7.8 star which is only 0.78 arcseconds from the primary. The third component, 7 Camelopardalis C, is an eleventh magnitude star 26 arcseconds distant.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "7 Camelopardalis, HIP 23040AB, SAO 24929, HD 31278, GC 6017, HR 1568, DM BD+53   829, TYC 3734-2320-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "7 Camelopardalis",
	"OType" : "Spectroscopic binary",
	"Distance" : "113.39",
	"RA_S" : 74.321668,
	"DEC_S" : 53.75210262,
	"X" : 322,
	"Y" : 583,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.43,
	"key" : 43305,
	"title" : "7 Camelopardalis"
	},
{
	"Index" : "26264",
	"Description" : "Beta Camelopardalis (\u03B2 Cam / \u03B2 Camelopardalis) is a star in the constellation Camelopardalis.\r\r\u03B2 Camelopardalis is a yellow G-type supergiant with an apparent magnitude of +4.03. This is a double star, with components of magnitudes 4.0 and 7.4. It is approximately 1000 light years from Earth.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "10 Camelopardalis, Beta Camelopardalis, HIP 23522, SAO 13351, HD 31910, GC 6136, HR 1603, DM BD+60   856, TYC 4079-2478-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Beta Camelopardalis",
	"OType" : "Star",
	"Distance" : "266.37",
	"RA_S" : 75.85454684,
	"DEC_S" : 60.44224417,
	"X" : 306,
	"Y" : 496,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.123,
	"key" : 46264,
	"title" : "Beta Camelopardalis"
	},
{
	"Index" : "23388",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "11 Camelopardalis, HIP 23734, SAO 25001, HD 32343, GC 6193, HR 1622, DM BD+58   804, TYC 3746-2216-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "11 Camelopardalis",
	"OType" : "Be Star",
	"Distance" : "209.02",
	"RA_S" : 76.53521493,
	"DEC_S" : 58.97237189,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.197,
	"key" : 43388,
	"title" : "11 Camelopardalis"
	},
{
	"Index" : "28527",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 24254, SAO 5455, HD 32650, GC 6288, HR 1643, DM BD+73  274, TYC 4355-1445-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "V* BN Cam",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "115.46",
	"RA_S" : 78.09358069,
	"DEC_S" : 73.94667936,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.404,
	"key" : 48527,
	"title" : "V* BN Cam"
	},
{
	"Index" : "29900",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 25110, SAO 5496, HD 33564, GC 6455, HR 1686, DM BD+79  169, TYC 4532-2096-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Gliese 196 (HR 1686)",
	"OType" : "Star",
	"Distance" : "20.89",
	"RA_S" : 80.6397249,
	"DEC_S" : 79.23114744,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.14,
	"key" : 49900,
	"title" : "Gliese 196 (HR 1686)"
	},
{
	"Index" : "23457",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "16 Camelopardalis, HIP 25197, SAO 25161, HD 34787, GC 6578, HR 1751, DM BD+57   879, TYC 3756-1653-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "16 Camelopardalis",
	"OType" : "Star",
	"Distance" : "102.97",
	"RA_S" : 80.86601579,
	"DEC_S" : 57.54439793,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.232,
	"key" : 43457,
	"title" : "16 Camelopardalis"
	},
{
	"Index" : "23495",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "31 Camelopardalis, HIP 27971, SAO 25447, HD 39220, GC 7402, HR 2027, DM BD+59   920, TYC 3762-2640-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "31 Camelopardalis",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "142.76",
	"RA_S" : 88.74095045,
	"DEC_S" : 59.88836738,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.21,
	"key" : 43495,
	"title" : "31 Camelopardalis"
	},
{
	"Index" : "23501",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "37 Camelopardalis, HIP 29246, SAO 25597, HD 41597, GC 7796, HR 2152, DM BD+58   897, TYC 3763-2582-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "37 Camelopardalis",
	"OType" : "Star",
	"Distance" : "116.61",
	"RA_S" : 92.49589407,
	"DEC_S" : 58.93569418,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.477,
	"key" : 43501,
	"title" : "37 Camelopardalis"
	},
{
	"Index" : "26447",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "36 Camelopardalis, HIP 29490, SAO 13756, HD 41927, GC 7856, HR 2165, DM BD+65   517, TYC 4107-1558-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "36 Camelopardalis",
	"OType" : "Star",
	"Distance" : "218.24",
	"RA_S" : 93.21275175,
	"DEC_S" : 65.71842257,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.499,
	"key" : 46447,
	"title" : "36 Camelopardalis"
	},
{
	"Index" : "28444",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 29997, SAO 13788, HD 42818, GC 8020, HR 2209, DM BD+69  371, TYC 4345-2051-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 2209",
	"OType" : "Star",
	"Distance" : "53.64",
	"RA_S" : 94.71158481,
	"DEC_S" : 69.31978165,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.758,
	"key" : 48444,
	"title" : "HR 2209"
	},
{
	"Index" : "29921",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 32439, SAO 5946, HD 46588, GC 8711, HR 2401, DM BD+79  212, TYC 4534-1837-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Gliese 240.1",
	"OType" : "Star",
	"Distance" : "17.87",
	"RA_S" : 101.5589676,
	"DEC_S" : 79.56481005,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.493,
	"key" : 49921,
	"title" : "Gliese 240.1"
	},
{
	"Index" : "28549",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "42 Camelopardalis, HIP 32864, SAO 13973, HD 48879, GC 8902, HR 2490, DM BD+67   454, TYC 4359-2044-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "42 Camelopardalis",
	"OType" : "Star",
	"Distance" : "281.16",
	"RA_S" : 102.73786858,
	"DEC_S" : 67.57194062,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.096,
	"key" : 48549,
	"title" : "42 Camelopardalis"
	},
{
	"Index" : "28548",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "43 Camelopardalis, HIP 33104, SAO 13986, HD 49340, GC 8957, HR 2511, DM BD+69   394, TYC 4359-2043-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "43 Camelopardalis",
	"OType" : "Star",
	"Distance" : "297.77",
	"RA_S" : 103.42603029,
	"DEC_S" : 68.88831037,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.077,
	"key" : 48548,
	"title" : "43 Camelopardalis"
	},
{
	"Index" : "29886",
	"Description" : "M Camelopardalis is a star in the constellation Camelopardalis.\r\rM Camelopardalis is an orange K-type giant with an apparent magnitude of +4.55. It is approximately 187 light years from Earth.",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 33694, SAO 6022, HD 49878, GC 9073, HR 2527, DM BD+77  266, TYC 4530-2010-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "M Camelopardalis",
	"OType" : "Star",
	"Distance" : "56.33",
	"RA_S" : 105.01681496,
	"DEC_S" : 76.97740739,
	"X" : 211,
	"Y" : 266,
	"Constellation" : "Camelopardalis ",
	"AMag" : 4.699,
	"key" : 49886,
	"title" : "M Camelopardalis"
	},
{
	"Index" : "29939",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "VZ Camelopardalis, HIP 36547, SAO 1179, HD 55966, GC 9851, HR 2742, DM BD+82   201, TYC 4539-1189-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "VZ Camelopardalis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "152.87",
	"RA_S" : 112.76858948,
	"DEC_S" : 82.41146515,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.088,
	"key" : 49939,
	"title" : "VZ Camelopardalis"
	},
{
	"Index" : "29989",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 39538, TYC 4543-3120-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 3082",
	"OType" : "Star",
	"Distance" : "98.94",
	"RA_S" : 121.19617967,
	"DEC_S" : 79.47960973,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.379,
	"key" : 49989,
	"title" : "HR 3082"
	},
{
	"Index" : "30707",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 51502, SAO 1714, HD 90089, GC 14367, HR 4084, DM BD+83  297, TYC 4632-2151-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "Gliese 392.1 (HR 4084)",
	"OType" : "Variable Star",
	"Distance" : "21.48",
	"RA_S" : 157.76938229,
	"DEC_S" : 82.55859795,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.297,
	"key" : 50707,
	"title" : "Gliese 392.1 (HR 4084)"
	},
{
	"Index" : "30082",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 59504, SAO 7522, HD 106112, GC 16672, HR 4646, DM BD+78  412, TYC 4553-1680-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "V* CO Cam",
	"OType" : "Spectroscopic binary",
	"Distance" : "33.38",
	"RA_S" : 183.04976587,
	"DEC_S" : 77.61624402,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.178,
	"key" : 50082,
	"title" : "V* CO Cam"
	},
{
	"Index" : "30713",
	"MapNum" : "11",
	"ImageNum" : "11",
	"Desig" : "HIP 62572A, SAO 2102, HD 112028, GC 17443, HR 4893, DM BD+84  290, TYC 4633-1785-1",
	"group" : { "key" : "Camelopardalis" },
	"Common" : "HR 4893",
	"OType" : "Star",
	"Distance" : "90.19",
	"RA_S" : 192.30693758,
	"DEC_S" : 83.41290442,
	"Constellation" : "Camelopardalis ",
	"AMag" : 5.288,
	"key" : 50713,
	"title" : "HR 4893"
	},
{
	"Index" : "56377",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "8 Cancri, HIP 39567, SAO 97542, HD 66664, GC 10959, HR 3163, DM BD+13  1831, TYC 789-1806-1",
	"group" : { "backgroundImage" : "images/Alignment/18.png",
		"description" : "Cancer is one of the twelve constellations of the zodiac. Its name is Latin for crab and it is commonly represented as such. Its astrological symbol is \u264B. Cancer is relatively small among the constellations with an area of only 505 square degrees and its stars are rather faint. It lies between Gemini to the west and Leo to the east, Lynx to the north and Canis Minor and Hydra to the south.\r\rCancer is said to have been the place for the Akkadian Sun of the South, perhaps from its position at the summer solstice in very remote antiquity. But afterwards it was associated with the fourth month Duzu (June\u2013July in the modern western calendar), and was known as the Northern Gate of Sun.\r\rShowing but few stars, and its brightest stars being of only 4th magnitude, Cancer was often considered the \u0022Dark Sign\u0022, quaintly described as black and without eyes. Dante, alluding to this faintness and position of heavens, wrote in Paradiso:\r\rThen a light among them brightened,\rSo that, if Cancer one such crystal had,\rWinter would have a month of one sole day.\r\rCancer was the location of the Sun\u0027s most northerly position in the sky (the summer solstice) in ancient times, though this position now occurs in Taurus due to the precession of the equinoxes, around June 21. This is also the time that the sun is directly overhead at 23.5\u00B0N, a parallel now known as the Tropic of Cancer.",
		"key" : "Cancer",
		"grouptype" : "Cancer",
		"Meaning" : "crab",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Cancer",
		"title" : "Cancer Objects Group" },
	"Common" : "8 Cancri",
	"OType" : "Star",
	"Distance" : "65.75",
	"RA_S" : 121.26870313,
	"DEC_S" : 13.11821194,
	"Constellation" : "Cancer ",
	"AMag" : 5.136,
	"key" : 76377,
	"title" : "8 Cancri"
	},
{
	"Index" : "3180",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "10 Cancri, Mu Cancri, HIP 39780, SAO 79959, HD 67228, GC 11021, HR 3176, DM BD+22  1862, TYC 1388-1791-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Mu Cancri",
	"OType" : "Star",
	"Distance" : "23.29",
	"RA_S" : 121.94106421,
	"DEC_S" : 21.58181577,
	"Constellation" : "Cancer ",
	"AMag" : 5.361,
	"key" : 23180,
	"title" : "Mu Cancri"
	},
{
	"Index" : "3136",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "16 Cancri, Zeta01 Cancri, HIP 40167A, SAO 97645, HD 68257, GC 11141, HR 3208, DM BD+18  1867A, TYC 1381-1638-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Tegmen",
	"OType" : "Star",
	"Distance" : "25.07",
	"RA_S" : 123.05319049,
	"DEC_S" : 17.64774942,
	"Constellation" : "Cancer ",
	"AMag" : 5.302,
	"key" : 23136,
	"shortTitle" : "Tegmine",
	"title" : "Tegmen"
	},
{
	"Index" : "56837",
	"Description" : "Beta Cancri (\u03B2 Cnc, \u03B2 Cancri) is the brightest star in the constellation Cancer. It has the traditional name Tarf or Al Tarf (Altarf), certainly a derivation from Arabic \u0627\u0644\u0637\u0631\u0641 a\u1E6D-\u1E6Darf \u0022the eye\u0022 or \u0637\u0631\u0641\u0629 a\u1E6D-\u1E6Darfah \u0022the glance (of Leo)\u0022. It is approximately 290 light years from Earth.\r\rThis is an orange K-type giant,about 49 times the radius of the Sun, with an apparent magnitude of +3.50 and absolute magnitude of -1.25 (visual). It has a faint, fourteenth magnitude, red dwarf companion star located 29 arcseconds away.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "17 Cancri, Beta Cancri, HIP 40526, SAO 116569, HD 69267, GC 11254, HR 3249, DM BD+09  1917, TYC 794-1622-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Tarf / Al Tarf",
	"OType" : "Variable Star",
	"Distance" : "92.99",
	"RA_S" : 124.12883577,
	"DEC_S" : 9.1855446,
	"X" : 387,
	"Y" : 457,
	"Constellation" : "Cancer ",
	"AMag" : 3.684,
	"key" : 76837,
	"shortTitle" : "Al Tarf; Tarf",
	"title" : "Tarf / Al Tarf"
	},
{
	"Index" : "7736",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "18 Cancri, Chi Cancri, HIP 40843, SAO 80104, HD 69897, GC 11348, HR 3262, DM BD+27  1589, TYC 1936-1174-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Chi Cancri",
	"OType" : "High proper-motion Star",
	"Distance" : "18.27",
	"RA_S" : 125.01608634,
	"DEC_S" : 27.21770692,
	"Constellation" : "Cancer ",
	"AMag" : 5.179,
	"key" : 27736,
	"title" : "Chi Cancri"
	},
{
	"Index" : "56964",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "HIP 41325, SAO 116752, HD 71115, GC 11505, HR 3306, DM BD+08 2053, TYC 796-1827-1",
	"group" : { "key" : "Cancer" },
	"Common" : "HR 3306",
	"OType" : "Star",
	"Distance" : "120.85",
	"RA_S" : 126.47819543,
	"DEC_S" : 7.56450525,
	"Constellation" : "Cancer ",
	"AMag" : 5.225,
	"key" : 76964,
	"title" : "HR 3306"
	},
{
	"Index" : "3304",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "33 Cancri, Eta Cancri, HIP 41909, SAO 80243, HD 72292, GC 11687, HR 3366, DM BD+20  2109, TYC 1398-3161-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Eta Cancri",
	"OType" : "Star",
	"Distance" : "91.34",
	"RA_S" : 128.17707186,
	"DEC_S" : 20.4411613,
	"Constellation" : "Cancer ",
	"AMag" : 5.467,
	"key" : 23304,
	"title" : "Eta Cancri"
	},
{
	"Index" : "3312",
	"Description" : "Gamma Cancri (\u03B3 Cnc, \u03B3 Cancri) is a star system in the constellation Cancer. It has the traditional name Asellus Borealis (Latin for \u0022northern donkey colt\u0022).\r\rIn Chinese, \u9B3C\u5BBF (Gu\u01D0 Su), meaning Ghost (asterism), refers to an asterism consisting of \u03B3 Cancri, \u03B8 Cancri, \u03B7 Cancri and \u03B4 Cancri. Consequently, \u03B3 Cancri itself is known as \u9B3C\u5BBF\u4E09 (Gu\u01D0 Su s\u0101n, English: the Third Star of Ghost.)\r\r\u03B3 Cancri is a white A-type subgiant with an apparent magnitude of +4.66. It is approximately 158 light years from Earth. Since it is near the ecliptic, it can be occulted by the Moon and, very rarely, by planets. It will die in about 510 million years.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "43 Cancri, Gamma Cancri, HIP 42806, SAO 80378, HD 74198, GC 11982, HR 3449, DM BD+21  1895, TYC 1399-2905-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Asellus Borealis",
	"OType" : "Star",
	"Distance" : "55.55",
	"RA_S" : 130.8214428,
	"DEC_S" : 21.46849861,
	"X" : 302,
	"Y" : 299,
	"Constellation" : "Cancer ",
	"AMag" : 4.654,
	"key" : 23312,
	"shortTitle" : "Severnyj Oslenok",
	"title" : "Asellus Borealis"
	},
{
	"Index" : "3283",
	"Description" : "Delta Cancri (\u03B4 Cnc, \u03B4 Cancri) is an orange giant star approximately 180 light-years away in the constellation Cancer. It has the traditional name Asellus Australis which in Latin means \u0022southern donkey colt\u0022. It also has the longest of all known star names, Arkushanangarushashutu, derived from ancient Babylonian[clarification needed] which means \u0022the southeast star in the Crab\u0022.\r\rIn Chinese, \u9B3C\u5BBF (Gu\u01D0 Su), meaning Ghost (asterism), refers to an asterism consisting of \u03B4 Cancri, \u03B8 Cancri, \u03B7 Cancri and \u03B3 Cancri. Consequently, \u03B4 Cancri itself is known as \u9B3C\u5BBF\u56DB (Gu\u01D0 Su s\u00EC, English: the Fourth Star of Ghost.)\r\rSince it is near the ecliptic, it can be occulted by the Moon and very rarely by planets.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "47 Cancri, Delta Cancri, HIP 42911, SAO 98087, HD 74442, GC 12022, HR 3461, DM BD+18  2027, TYC 1396-2758-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Asellus Australis / Arkushanangarushashutu",
	"OType" : "Double or multiple star",
	"Distance" : "40.03",
	"RA_S" : 131.17125265,
	"DEC_S" : 18.15430914,
	"X" : 297,
	"Y" : 342,
	"Constellation" : "Cancer ",
	"AMag" : 4.048,
	"key" : 23283,
	"shortTitle" : "Juzhnyj Oslenok",
	"title" : "Asellus Australis / Arkushanangarushashutu"
	},
{
	"Index" : "7823",
	"Description" : "Iota Cancri (\u03B9 Cnc, \u03B9 Cancri) is a double star in the constellation Cancer. The brighter component is approximately 298 light years from Earth.\r\rThe brighter star is a yellow G-type bright giant with an apparent magnitude of +4.02. The companion is a white A-type main sequence dwarf with an apparent magnitude of +6.58. The two stars are separated by 30.5 arcseconds on the sky, and are resolvable through a small telescope.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "48 Cancri, Iota Cancri, HIP 43103A, SAO 80416, HD 74739, GC 12083, HR 3475, DM BD+29  1824, TYC 1949-2011-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Iota Cancri",
	"OType" : "High proper-motion Star",
	"Distance" : "101.06",
	"RA_S" : 131.67424592,
	"DEC_S" : 28.75990042,
	"X" : 293,
	"Y" : 204,
	"Constellation" : "Cancer ",
	"AMag" : 4.126,
	"key" : 27823,
	"title" : "Iota Cancri"
	},
{
	"Index" : "7826",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "58 Cancri, Rho02 Cancri, HIP 43834, SAO 80511, HD 76219, GC 12326, HR 3540, DM BD+28  1666, TYC 1949-2014-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Rho02 Cancri",
	"OType" : "Star",
	"Distance" : "148.85",
	"RA_S" : 133.91533071,
	"DEC_S" : 27.92748595,
	"Constellation" : "Cancer ",
	"AMag" : 5.336,
	"key" : 27826,
	"title" : "Rho02 Cancri"
	},
{
	"Index" : "12097",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "59 Cancri, Sigma02 Cancri, HIP 43932, SAO 61146, HD 76398, GC 12358, HR 3555, DM BD+33  1785, TYC 2488-1707-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Sigma02 Cancri",
	"OType" : "Star",
	"Distance" : "59.54",
	"RA_S" : 134.2358245,
	"DEC_S" : 32.91043008,
	"Constellation" : "Cancer ",
	"AMag" : 5.457,
	"key" : 32097,
	"title" : "Sigma02 Cancri"
	},
{
	"Index" : "3236",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "62 Cancri, Omicron01 Cancri, HIP 43970, SAO 98247, HD 76543, GC 12373, HR 3561, DM BD+15  1945, TYC 1394-2122-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Omicron01 Cancri",
	"OType" : "Star",
	"Distance" : "45.72",
	"RA_S" : 134.31229058,
	"DEC_S" : 15.32276375,
	"Constellation" : "Cancer ",
	"AMag" : 5.241,
	"key" : 23236,
	"title" : "Omicron01 Cancri"
	},
{
	"Index" : "58431",
	"Description" : "Alpha Cancri (\u03B1 Cnc, \u03B1 Cancri) is a star system in the constellation Cancer. It has the traditional name Acubens (A\u00E7ubens). Acubens is a fourth-magnitude star with an apparent magnitude of 4.20, making it barely visible to the naked eye under good lighting conditions. Nevertheless, it is 23 times more luminous than the Sun. Its stellar classification is A5m. The Hipparcos mission estimated the distance of Acubens to be roughly 53 parsecs from Earth, or approximately 174 light years away.\r\rSince it is near the ecliptic, it can be occulted by the Moon and very rarely by planets.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "65 Cancri, Alpha Cancri, HIP 44066, SAO 98267, HD 76756, GC 12406, HR 3572, DM BD+12  1948, TYC 814-3029-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Acubens",
	"OType" : "Variable Star",
	"Distance" : "57.52",
	"RA_S" : 134.62174055,
	"DEC_S" : 11.85768694,
	"X" : 253,
	"Y" : 423,
	"Constellation" : "Cancer ",
	"AMag" : 4.268,
	"key" : 78431,
	"shortTitle" : "Sertan; Sartan; Akubens",
	"title" : "Acubens"
	},
{
	"Index" : "12068",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "64 Cancri, Sigma03 Cancri, HIP 44154, SAO 61177, HD 76813, GC 12417, HR 3575, DM BD+32  1821, TYC 2485-2095-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Sigma03 Cancri",
	"OType" : "Star",
	"Distance" : "90.59",
	"RA_S" : 134.88605507,
	"DEC_S" : 32.41855781,
	"Constellation" : "Cancer ",
	"AMag" : 5.321,
	"key" : 32068,
	"title" : "Sigma03 Cancri"
	},
{
	"Index" : "7837",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "69 Cancri, Nu Cancri, HIP 44405, SAO 80595, HD 77350, GC 12496, HR 3595, DM BD+25  2029, TYC 1950-2323-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Nu Cancri",
	"OType" : "Spectroscopic binary",
	"Distance" : "120.08",
	"RA_S" : 135.6844411,
	"DEC_S" : 24.45291226,
	"Constellation" : "Cancer ",
	"AMag" : 5.44,
	"key" : 27837,
	"title" : "Nu Cancri"
	},
{
	"Index" : "58566",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "76 Cancri, Kappa Cancri, HIP 44798, SAO 98378, HD 78316, GC 12596, HR 3623, DM BD+11  1984, TYC 815-2146-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Kappa Cancri",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "162.52",
	"RA_S" : 136.93671785,
	"DEC_S" : 10.66818893,
	"Constellation" : "Cancer ",
	"AMag" : 5.202,
	"key" : 78566,
	"title" : "Kappa Cancri"
	},
{
	"Index" : "3388",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "77 Cancri, Xi Cancri, HIP 44946, SAO 80666, HD 78515, GC 12635, HR 3627, DM BD+22  2061, TYC 1407-1989-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Xi Cancri",
	"OType" : "Spectroscopic binary",
	"Distance" : "113.99",
	"RA_S" : 137.33973063,
	"DEC_S" : 22.04545887,
	"Constellation" : "Cancer ",
	"AMag" : 5.257,
	"key" : 23388,
	"title" : "Xi Cancri"
	},
{
	"Index" : "59623",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "82 Cancri, Pi Cancri, HIP 45410, SAO 98456, HD 79554, GC 12758, HR 3669, DM BD+15  2009, TYC 825-1545-1",
	"group" : { "key" : "Cancer" },
	"Common" : "Pi Cancri",
	"OType" : "Star",
	"Distance" : "185.33",
	"RA_S" : 138.80771946,
	"DEC_S" : 14.94150911,
	"Constellation" : "Cancer ",
	"AMag" : 5.498,
	"key" : 79623,
	"title" : "Pi Cancri"
	},
{
	"Index" : "20640",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "3 Canum Venaticorum, HIP 60122, SAO 44127, HD 107274, GC 16814, HR 4690, DM BD+49  2130, TYC 3457-1877-1",
	"group" : { "backgroundImage" : "images/Alignment/21.png",
		"description" : "Canes Venatici (pron.: /\u02C8ke\u026Ani\u02D0z v\u0268\u02C8n\u00E6t\u0268sa\u026A/) is one of the 88 official modern constellations. It is a small northern constellation that was created by Johannes Hevelius in the 17th century. Its name is Latin for \u0022hunting dogs\u0022, and the constellation is often depicted in illustrations as representing the dogs of Bootes the Herdsman, a neighboring constellation.\r\rThe stars of Canes Venatici are not bright. In classical times, they were included by Ptolemy within the constellation Ursa Major in his star catalogue. \u03B1 CVn was Ptolemy\u0027s \u002228th of Ursa Major\u0022, and \u03B2 CVn was his \u002229th of Ursa Major\u0022.\r\rIn the medieval times, the identification of these stars with the dogs of Bootes arose through a mistranslation. Some of Bootes\u0027 stars were traditionally described as representing the club (Greek, \u039A\u03BF\u03BB\u03BB\u03BF\u03C1\u03BF\u03B2\u03BF\u03C2) of Bootes. When the Greek astronomer Ptolemy\u0027s Almagest was translated from Greek to Arabic, the translator Johannitius (following Alberuni) did not know the Greek word and rendered it as the nearest-looking Arabic word, writing \u0627\u0644\u0639\u0635\u0649 \u0630\u0627\u062A \u0627\u0644\u0643\u0644\u0627\u0628 in ordinary unvowelled Arabic text \u0022al-`a\u015F\u0101 dh\u0101t al-kull\u0101b\u0022, which means \u0022the spearshaft having a hook\u0022. When the Arabic text was translated into Latin, the translator Gerard of Cremona (probably in Spain) mistook the Arabic word \u0643\u0644\u0627\u0628 for kil\u0101b (the plural of \u0643\u0644\u0628 kalb), meaning \u0022dogs\u0022, writing hastile habens canes (\u0022spearshaft having dogs\u0022).\r\r In 1533, the German astronomer Peter Apian depicted Bootes as having two dogs with him.\r\rThese spurious dogs floated about the astronomical literature until Hevelius decided to specify their presence in the sky by making them a separate constellation in 1687. Hevelius chose the name Asterion (from the Greek \u0027\u03B1\u03C3\u03C4\u03AD\u03C1\u03B9\u03BF\u03BD, meaning the \u0022little star\u0022, the diminutive of \u0027\u03B1\u03C3\u03C4\u03B7\u03C1 the \u0022star\u0022, or adjective meaning \u0022starry\u0022) for the northern dog and Chara (from the Greek \u03C7\u03B1\u03C1\u03AC, meaning \u0022joy\u0022) for the southern dog, as Canes Venatici, the Hunting Dogs, in his star atlas. In his star catalogue, the Czech astronomer Becvar assigned Asterion to \u03B2 CVn and Chara to \u03B1 CVn.",
		"key" : "Canes Venatici",
		"grouptype" : "Canes Venatici",
		"Meaning" : "hunting dogs",
		"Family" : "Ursa Major",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Canes Venatici",
		"title" : "Canes Venatici Objects Group" },
	"Common" : "3 Canum Venaticorum",
	"OType" : "Variable Star",
	"Distance" : "180.28",
	"RA_S" : 184.95296009,
	"DEC_S" : 48.98414896,
	"Constellation" : "Canes Venatici ",
	"AMag" : 5.471,
	"key" : 40640,
	"title" : "3 Canum Venaticorum"
	},
{
	"Index" : "20651",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "5 Canum Venaticorum, HIP 60485, SAO 28366, HD 107950, GC 16906, HR 4716, DM BD+52  1626, TYC 3458-2328-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "5 Canum Venaticorum",
	"OType" : "Star",
	"Distance" : "118.37",
	"RA_S" : 186.00623486,
	"DEC_S" : 51.56225799,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.859,
	"key" : 40651,
	"title" : "5 Canum Venaticorum"
	},
{
	"Index" : "16778",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "6 Canum Venaticorum, HIP 60646, SAO 63000, HD 108225, GC 16948, HR 4728, DM BD+39  2521, TYC 3018-2755-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "6 Canum Venaticorum",
	"OType" : "Star",
	"Distance" : "80.15",
	"RA_S" : 186.46223826,
	"DEC_S" : 39.01861677,
	"Constellation" : "Canes Venatici ",
	"AMag" : 5.117,
	"key" : 36778,
	"title" : "6 Canum Venaticorum"
	},
{
	"Index" : "16804",
	"Description" : "Beta Canum Venaticorum (\u03B2 CVn, \u03B2 Canum Venaticorum) is the Bayer designation for a G-type main sequence star in the northern constellation Canes Venatici. At an apparent visual magnitude of 4.26, it is the second-brightest star in this relatively faint constellation. Based upon an annual parallax shift of 118.49 mas, this star is 27.53 light-years (8.44 parsecs) distant from the Earth.\r\rAlong with the brighter star Cor Caroli, the pair form the \u0022southern dog\u0022 in this constellation that represents hunting dogs. The name Chara was originally applied to the \u0022southern dog\u0022, but it later became used specifically to refer to Beta Canum Venaticorum. Chara (\u03C7\u03B1\u03C1\u03AC) means Joy in Greek.\r\rIn Chinese, \u5E38\u9673 (Ch\u00E1ng Ch\u00E9n), meaning Imperial Guards, refers to an asterism consisting of \u03B2 Canum Venaticorum, \u03B1 Canum Venaticorum, 10 Canum Venaticorum, 6 Canum Venaticorum, 2 Canum Venaticorum, and 67 Ursae Majoris. Consequently, \u03B2 Canum Venaticorum itself is known as \u5E38\u9673\u56DB (Ch\u00E1ng Ch\u00E9n s\u00EC, English: the Fourth Star of Imperial Guards.)",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "8 Canum Venaticorum, Beta Canum Venaticorum, HIP 61317, SAO 44230, HD 109358, GC 17127, HR 4785, DM BD+42  2321, TYC 3020-2541-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "Chara",
	"OType" : "Spectroscopic binary",
	"Distance" : "8.44",
	"RA_S" : 188.43560242,
	"DEC_S" : 41.35747839,
	"X" : 406,
	"Y" : 227,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.309,
	"key" : 36804,
	"shortTitle" : "Asterion (the \"northen hound\" of the CVn); Venatici",
	"title" : "Chara"
	},
{
	"Index" : "16820",
	"Description" : "Cor Caroli (\u03B1 CVn, \u03B1 Canum Venaticorum, Alpha Canum Venaticorum) is the brightest star in the northern constellation Canes Venatici. It is a binary star consisting of two distantly separated components. The name Cor Caroli means \u0022Charles\u0027 Heart\u0022, and was named in the 17th century to honour the murdered King Charles I of England. In the western world the star had no name until the 17th century, when it was named Cor Caroli, which means \u0022Charles\u0027s Heart\u0022. There has been some uncertainty whether it was named in honour of King Charles I of England, who was executed in 1649 during the English Civil War, or to his son, Charles II, who restored the English monarchy to the throne in 1660. The name was coined in 1660 by Sir Charles Scarborough, physician to Charles II, who claimed the star seemed to shine exceptionally brightly on the night of Charles II\u0027s return to England. In Star Names, R.H. Allen claimed that Scarborough suggested the name to Edmund Halley and intended it to refer to Charles II. However, Robert Burnham Jr. notes that \u0022the attribution of the name to Halley appears in a report published by J. E. Bode at Berlin in 1801, but seems to have no other verification\u0022. In Star Tales, Ian Ridpath points out that the name\u0027s first appearance on a star map was in the 1673 chart of Francis Lamb, who labelled it Cor Caroli Regis Martyris (\u0022the heart of Charles the martyred king\u0022), clearly indicating that it was seen as referring to Charles I.\r\rIn Chinese, \u5E38\u9673 (Ch\u00E1ng Ch\u00E9n), meaning Imperial Guards, refers to an asterism consisting of \u03B1 Canum Venaticorum, 10 Canum Venaticorum, \u03B2 Canum Venaticorum, 6 Canum Venaticorum, 2 Canum Venaticorum, 67 Ursae Majoris. Consequently, \u03B1 Canum Venaticorum itself is known as \u5E38\u9673\u4E00 (Ch\u00E1ng Ch\u00E9n y\u012B, English: the First Star of Imperial Guards.) From this Chinese name, the name Chang Chen was appeared.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "12 Canum Venaticorum, Alpha02 Canum Venaticorum, HIP 63125A, SAO 63257, HD 112413, GC 17557, HR 4915, DM BD+39  2580A, TYC 3021-2645-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "Cor Caroli",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "35.16",
	"RA_S" : 194.00694257,
	"DEC_S" : 38.31837614,
	"X" : 353,
	"Y" : 270,
	"Constellation" : "Canes Venatici ",
	"AMag" : 2.845,
	"key" : 36820,
	"shortTitle" : "Chara; Serdtse Karla; Kor Karoli; Khara",
	"title" : "Cor Caroli"
	},
{
	"Index" : "12579",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "14 Canum Venaticorum, HIP 63901, SAO 63338, HD 113797, GC 17751, HR 4943, DM BD+36  2337, TYC 2534-304-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "14 Canum Venaticorum",
	"OType" : "Variable Star",
	"Distance" : "104.34",
	"RA_S" : 196.43514926,
	"DEC_S" : 35.79889929,
	"Constellation" : "Canes Venatici ",
	"AMag" : 5.185,
	"key" : 32579,
	"title" : "14 Canum Venaticorum"
	},
{
	"Index" : "16834",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "HIP 64540, SAO 44519, HD 115004, GC 17916, HR 4997, DM BD+40 2633, TYC 3022-2307-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "HR 4997",
	"OType" : "Star",
	"Distance" : "140.65",
	"RA_S" : 198.42892214,
	"DEC_S" : 40.15288514,
	"Constellation" : "Canes Venatici ",
	"AMag" : 5.048,
	"key" : 36834,
	"title" : "HR 4997"
	},
{
	"Index" : "16833",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "20 Canum Venaticorum, HIP 64844, SAO 44549, HD 115604, GC 18000, HR 5017, DM BD+41  2380, TYC 3022-2306-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "20 Canum Venaticorum",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "81.01",
	"RA_S" : 199.38558526,
	"DEC_S" : 40.57260979,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.737,
	"key" : 36833,
	"title" : "20 Canum Venaticorum"
	},
{
	"Index" : "20700",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "21 Canum Venaticorum, HIP 64906, SAO 44556, HD 115735, GC 18009, HR 5023, DM BD+50  1994, TYC 3462-2651-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "21 Canum Venaticorum",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "84.21",
	"RA_S" : 199.56045975,
	"DEC_S" : 49.68205999,
	"Constellation" : "Canes Venatici ",
	"AMag" : 5.13,
	"key" : 40700,
	"title" : "21 Canum Venaticorum"
	},
{
	"Index" : "20722",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "24 Canum Venaticorum, HIP 66234, SAO 44668, HD 118232, GC 18356, HR 5112, DM BD+49  2227, TYC 3466-1270-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "24 Canum Venaticorum",
	"OType" : "High proper-motion Star",
	"Distance" : "55.27",
	"RA_S" : 203.61358531,
	"DEC_S" : 49.01597692,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.685,
	"key" : 40722,
	"title" : "24 Canum Venaticorum"
	},
{
	"Index" : "12632",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "HIP 66257, SAO 63623, HD 118216, GC 18359, HR 5110, DM BD+37 2426, TYC 2542-1094-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "HR 5110",
	"OType" : "Variable of RS CVn type",
	"Distance" : "45.66",
	"RA_S" : 203.69920192,
	"DEC_S" : 37.18241443,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.978,
	"key" : 32632,
	"title" : "HR 5110"
	},
{
	"Index" : "12640",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "25 Canum Venaticorum, HIP 66458A, SAO 63648, HD 118623A, GC 18421, HR 5127, DM BD+37  2433, TYC 2543-1189-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "25 Canum Venaticorum",
	"OType" : "Star",
	"Distance" : "60.83",
	"RA_S" : 204.365388,
	"DEC_S" : 36.294842,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.98,
	"key" : 32640,
	"title" : "25 Canum Venaticorum"
	},
{
	"Index" : "12666",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "HIP 67665, SAO 63793, HD 120933, GC 18741, HR 5219, DM BD+35 2496, TYC 2547-1181-1",
	"group" : { "key" : "Canes Venatici" },
	"Common" : "HR 5219",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "183.86",
	"RA_S" : 207.94781625,
	"DEC_S" : 34.44424002,
	"Constellation" : "Canes Venatici ",
	"AMag" : 4.94,
	"key" : 32666,
	"title" : "HR 5219"
	},
{
	"Index" : "36411",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 29735, SAO 151283, HD 43445, GC 8024, HR 2244, DM BD-13 1411, TYC 5375-2589-1",
	"group" : { "backgroundImage" : "images/Alignment/17.png",
		"description" : "Canis Major (pron.: /\u02CCke\u026An\u0268s \u02C8me\u026Ad\u0292\u0259r/) is one of the 88 modern constellations, and was included in the 2nd-century astronomer Ptolemy\u0027s 48 constellations. Its name is Latin for \u0027greater dog\u0027, and is commonly represented as one of the dogs following Orion the hunter (see also Canis Minor the \u0027lesser dog\u0027). Canis Major contains Sirius, the brightest star in the night sky, known as the \u0027dog star\u0027. It is bright because of its proximity to our Solar System. In contrast, the other bright stars of the constellation are distant luminous bright giants and supergiants. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second brightest star of the constellation, followed by Delta (Wezen) at 1.8, Beta (Mirzam) at 2.0 and Eta (Aludra) at 2.4. The red supergiant VY Canis Majoris is one of the largest stars known.\r\rCanis Major is a constellation in the southern hemisphere\u0027s summer (or northern hemisphere\u0027s winter) sky, bordered by Monoceros (which lies between it and Canis Minor) to the north, Puppis to the east and southeast, Columba to the southwest, and Lepus to the west. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027CMa\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 4 sides. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 06h 12.5m and 07h 27.5m, while the declination coordinates are between -11.03\u00B0 and \u221233.25\u00B0. Covering 380 square degrees, it ranks 43rd of the 88 constellations in size. Canis Major culminates each year at 9 p.m. on 4 April.\r\rIn early classical Europe, Canis Major represented the dog Laelaps, a gift from Zeus to Europa; or sometimes the hound of Procris, Diana\u0027s nymph; or the one given by Aurora to Cephalus, so famed for its speed that Zeus elevated it to the sky.\r\rIt was also considered to represent one of Orion\u0027s hunting dogs, pursuing Lepus the Hare or helping Orion fight Taurus the Bull; and is referred to in this way by Aratos, Homer and Hesiod. The ancient Greeks refer only to one dog, but by Roman times, Canis Minor appears as Orion\u0027s second dog.\r\rSirius was considered a dog in its own right; early Greek mythology sometimes tells that the constellation represents a two-headed dog. As such, together with the area of the sky that is deserted (now considered as the new and extremely faint constellations Camelopardalis and Lynx), and the other features of the area in the Zodiac sign of Gemini (i.e. the Milky Way, and the constellations Gemini, Orion, Auriga, and Canis Minor), this may be the origin of the myth of the cattle of Geryon, which forms one of The Twelve Labours of Heracles.[original research?]\r\rRoman myth refers to Canis Major as Custos Europae, the dog guarding Europa but failing to prevent her abduction by Jupiter in the form of a bull; and as Janitor Lethaeus, the watchdog.\r\rIn Chinese astronomy, the modern constellation of Canis Major lies in The Vermillion Bird of the South (\u5357\u65B9\u6731\u96C0, N\u00E1n F\u0101ng Zh\u016B Qu\u00E8).\r\rBoth the Maori people and the people of the Tuamotus recognized the figure of Canis Major as a distinct entity, though it was sometimes absorbed into other constellations. Te Huinga-o-Rehua, also called Te Putahi-nui-o-Rehua and Te Kahui-Takurua, (\u0022The Assembly of Rehua\u0022 or \u0022The Assembly of Sirius\u0022) was a Maori constellation that included both Canis Minor and Canis Major, along with some surrounding stars. Related was Taumata-o-Rehua, also called Pukawanui, the Mirror of Rehua, formed from an undefined group of stars in Canis Major. They called Sirius Rehua and Takarua, corresponding to two of the names for the constellation, though Rehua was a name applied to other stars in various Maori groups and other Polynesian cosmologies. The Tuamotu people called Canis Major Muihanga-hetika-o-Takurua, \u0022the abiding assemblage of Takurua\u0022. In their cosmology, Sirius had various names, including Takurua-te-upuupu, Te Kaha (\u0022coconut fiber\u0022), Te Upuupu, Taranga, and Vero-ma-torutoru (\u0022flaming and diminishing\u0022). Beta Canis Majoris was called Oupo. Sirius itself was named by several other Polynesian cultures. The Hawaiian people had many names for Sirius, including Aa (\u0022glowing\u0022), Hoku-kauopae, Kau-ano-meha (also Kaulanomeha), \u0022Standing-alone-and-sacred\u0022, Hiki-kauelia or Hiki-kauilia (the navigational name), Hiki-kau-lono-meha (\u0022star of solitary Lono\u0022, the astrological name), Kaulua (also Kaulua-ihai-mohai, \u0022flower of the heavens\u0022), Hiki-kauelia, Hoku-hoo-kele-waa (\u0022star which causes the canoe to sail\u0022, a marine navigation name), and Kaulua-lena (\u0022yellow star\u0022). The people of the Society Islands called Sirius variously Taurua-fau-papa, Taurua-nui-te-amo-aha, and Taurua-e-hiti-i-tara-te-feiai. Other names for Sirius included Palolo-mua (Futuna), Mere (Mangaia), Apura (Manihiki), Taku-ua (Marquesas Islands), and Tokiva (Pukapuka).",
		"key" : "Canis Major",
		"grouptype" : "Canis Major",
		"Meaning" : "greater dog",
		"Family" : "Orion",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Canis Major",
		"title" : "Canis Major Objects Group" },
	"Common" : "HR 2244",
	"OType" : "Star",
	"Distance" : "124.82",
	"RA_S" : 93.93702411,
	"DEC_S" : -13.71841714,
	"Constellation" : "Canis Major ",
	"AMag" : 4.987,
	"key" : 56411,
	"title" : "HR 2244"
	},
{
	"Index" : "40501",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 29895, SAO 151322, HD 43827, GC 8080, HR 2260, DM BD-16 1426, TYC 5934-2741-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2260",
	"OType" : "Variable Star",
	"Distance" : "188.81",
	"RA_S" : 94.42384963,
	"DEC_S" : -16.81590792,
	"Constellation" : "Canis Major ",
	"AMag" : 5.292,
	"key" : 60501,
	"title" : "HR 2260"
	},
{
	"Index" : "40572",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 29941, SAO 151334, HD 43955, GC 8099, HR 2266, DM BD-19 1407, TYC 5942-2406-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2266",
	"OType" : "Star",
	"Distance" : "242.54",
	"RA_S" : 94.55720364,
	"DEC_S" : -19.96697454,
	"Constellation" : "Canis Major ",
	"AMag" : 5.473,
	"key" : 60572,
	"title" : "HR 2266"
	},
{
	"Index" : "49133",
	"Description" : "Zeta Canis Majoris (\u03B6 CMa, \u03B6 Canis Majoris) is a spectroscopic binary in the constellation Canis Major. It has the traditional name Furud or Phurud, from the Arabic \u0623\u0644\u0641\u0631\u062F al-furud meaning the bright single ones or, perhaps by a transcriber\u0027s error, from Al \u1E32ur\u016Bd (\u0623\u0644\u0642\u0631\u062F - al-qird), the Apes, or Al Agribah (\u0623\u0644 \u0623\u063A\u0631\u0628\u0629), the Raven by Al Sufi, referring to the surrounding small stars with some of those of Columba (\u03B6 CMa, \u03BB CMa, \u03B3 Col, \u03B4 Col, \u03B8 Col, \u03BA Col, \u03BB Col, \u03BC Col and \u03BE Col). The Bayer designation Zeta Canis Majoris was assigned by German astronomer Johann Bayer in 1603.\r\rThis star system has an apparent visual magnitude of +3.0, making it one of the brighter stars in the constellation and hence readily visible to the naked eye. Parallax measurements from the Hipparcos mission yield a distance estimate of around 362 ly (111 pc) from Earth. This is a single-lined spectroscopic binary system, which means that the pair have not been individually resolved with a telescope, but the gravitational perturbations of an unseen astrometric companion can be discerned by shifts in the spectrum of the primary caused by the Doppler effect. The pair orbit around their common center of mass once every 675 days with an eccentricity of 0.57.\r\rThe primary component is a large star with nearly four times the Sun\u0027s radius and almost eight times the mass of the Sun. It has a stellar classification of B2.5 V, which means it is a B-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. It is emitting 3,603 times the luminosity of the Sun and is a suspected Beta Cephei variable. This energy is being radiated from its outer envelope at an effective temperature of about 18,700 K, giving it the blue-white hue of a B-type star. It is relatively young for a star, with an estimated age of 32 million years.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "1 Canis Majoris, Zeta Canis Majoris, HIP 30122, SAO 196698, HD 44402, GC 8170, HR 2282, DM CD-30  3038, TYC 7073-2426-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Furud / Phurud",
	"OType" : "Cepheid variable Star",
	"Distance" : "111.08",
	"RA_S" : 95.07830017,
	"DEC_S" : -30.06336673,
	"X" : 479,
	"Y" : 332,
	"Constellation" : "Canis Major ",
	"AMag" : 2.961,
	"key" : 69133,
	"shortTitle" : "Phurud",
	"title" : "Furud / Phurud"
	},
{
	"Index" : "36381",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 30457, SAO 151458, HD 44951, GC 8265, HR 2305, DM BD-11 1478, TYC 5372-2524-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2305",
	"OType" : "Star",
	"Distance" : "106.62",
	"RA_S" : 96.04300022,
	"DEC_S" : -11.53008774,
	"Constellation" : "Canis Major ",
	"AMag" : 5.345,
	"key" : 56381,
	"title" : "HR 2305"
	},
{
	"Index" : "49168",
	"Description" : "Lambda Canis Majoris (\u03BB CMa, \u03BB Canis Majoris) is a star in the constellation Canis Major. This star, along with \u03B6 CMa, \u03B3 Col, \u03B4 Col, \u03B8 Col, \u03BA Col, \u03BB Col, \u03BC Col and \u03BE Col, were Al \u1E32ur\u016Bd (\u0623\u0644\u0642\u0631\u062F - al-qird), the Apes.\r\r\u03BB Canis Majoris is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.47. It is approximately 406 light years from Earth.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Lambda Canis Majoris, HIP 30788, SAO 196857, HD 45813, GC 8410, HR 2361, DM CD-32  3066, TYC 7078-2130-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Lambda Canis Majoris",
	"OType" : "Star",
	"Distance" : "129.8",
	"RA_S" : 97.04253279,
	"DEC_S" : -32.58007046,
	"X" : 453,
	"Y" : 362,
	"Constellation" : "Canis Major ",
	"AMag" : 4.436,
	"key" : 69168,
	"title" : "Lambda Canis Majoris"
	},
{
	"Index" : "36396",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 31084, SAO 151602, HD 46184, GC 8470, HR 2379, DM BD-12 1518, TYC 5373-2863-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2379",
	"OType" : "High proper-motion Star",
	"Distance" : "111.95",
	"RA_S" : 97.84602215,
	"DEC_S" : -12.39197252,
	"Constellation" : "Canis Major ",
	"AMag" : 5.297,
	"key" : 56396,
	"title" : "HR 2379"
	},
{
	"Index" : "44857",
	"Description" : "Xi1 Canis Majoris (\u03BE1 CMa, \u03BE1 Canis Majoris) is a star in the constellation Canis Major. It is approximately 2051 light years from Earth.\r\r\u03BE1 Canis Majoris is a blue-white B-type subgiant with a mean apparent magnitude of +4.34. It is classified as a Beta Cephei type variable star and its brightness varies from magnitude +4.33 to +4.36 with a period of 5.03 hours.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "4 Canis Majoris, Xi01 Canis Majoris, HIP 31125, SAO 171895, HD 46328, GC 8496, HR 2387, DM CD-23  3991, TYC 6507-2920-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Xi1 Canis Majoris",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "420.11",
	"RA_S" : 97.96402649,
	"DEC_S" : -23.41842169,
	"X" : 457,
	"Y" : 241,
	"Constellation" : "Canis Major ",
	"AMag" : 4.286,
	"key" : 64857,
	"title" : "Xi1 Canis Majoris"
	},
{
	"Index" : "44862",
	"Description" : "Xi2 Canis Majoris (\u03BE2 CMa, \u03BE2 Canis Majoris) is a star in the constellation Canis Major.\r\r\u03BE2 Canis Majoris is a white A-type main sequence dwarf with an apparent magnitude of +4.54. It is approximately 412 light years from Earth.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "5 Canis Majoris, Xi02 Canis Majoris, HIP 31416, SAO 171982, HD 46933, GC 8577, HR 2414, DM BD-22  1458, TYC 6508-2872-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Xi2 Canis Majoris",
	"OType" : "Star",
	"Distance" : "134.33",
	"RA_S" : 98.76411952,
	"DEC_S" : -22.9647882,
	"X" : 447,
	"Y" : 234,
	"Constellation" : "Canis Major ",
	"AMag" : 4.517,
	"key" : 64862,
	"title" : "Xi2 Canis Majoris"
	},
{
	"Index" : "40723",
	"Description" : "Nu2 Canis Majoris (\u03BD2 CMa, \u03BD2 Canis Majoris) is a star in the constellation Canis Major. It is an evolved K-type giant approximately 65 light years away, seen below Sirius. In 2011, it was discovered to have a planet.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "7 Canis Majoris, Nu02 Canis Majoris, HIP 31592, SAO 151702, HD 47205, GC 8624, HR 2429, DM BD-19  1502, TYC 5956-2621-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Nu2 Canis Majoris",
	"OType" : "Variable Star",
	"Distance" : "19.75",
	"RA_S" : 99.17099216,
	"DEC_S" : -19.25587721,
	"X" : 447,
	"Y" : 186,
	"Constellation" : "Canis Major ",
	"AMag" : 4.068,
	"key" : 60723,
	"title" : "Nu2 Canis Majoris"
	},
{
	"Index" : "49305",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 31688, SAO 197019, HD 47536, GC 8667, HR 2447, DM CD-32 3216, TYC 7091-1257-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2447",
	"OType" : "Star",
	"Distance" : "123.19",
	"RA_S" : 99.44841121,
	"DEC_S" : -32.33972878,
	"Constellation" : "Canis Major ",
	"AMag" : 5.389,
	"key" : 69305,
	"title" : "HR 2447"
	},
{
	"Index" : "40676",
	"Description" : "Nu3 Canis Majoris (\u03BD3 CMa, \u03BD3 Canis Majoris) is a binary star in the constellation Canis Major. It is approximately 464 light years from Earth.\r\rThe primary component, \u03BD3 Canis Majoris A, is an orange K-type bright giant with an apparent magnitude of +4.42. Its companion, \u03BD3 Canis Majoris A, is 1.04 arcseconds distant and has an apparent magnitude of +8.4.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "8 Canis Majoris, Nu03 Canis Majoris, HIP 31700A, SAO 151730, HD 47442A, GC 8660, HR 2443, DM BD-18  1492, TYC 5952-2800-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Nu3 Canis Majoris",
	"OType" : "Star",
	"Distance" : "128.72",
	"RA_S" : 99.47258804,
	"DEC_S" : -18.23747545,
	"X" : 444,
	"Y" : 172,
	"Constellation" : "Canis Major ",
	"AMag" : 4.564,
	"key" : 60676,
	"title" : "Nu3 Canis Majoris"
	},
{
	"Index" : "36576",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 31827, SAO 151751, HD 47667, GC 8694, HR 2450, DM BD-14 1525, TYC 5390-2169-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2450",
	"OType" : "Star",
	"Distance" : "298.99",
	"RA_S" : 99.81966047,
	"DEC_S" : -14.14576059,
	"Constellation" : "Canis Major ",
	"AMag" : 4.986,
	"key" : 56576,
	"title" : "HR 2450"
	},
{
	"Index" : "49258",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "10 Canis Majoris, HIP 32292, SAO 197149, HD 48917, GC 8827, HR 2492, DM CD-30  3484, TYC 7087-1384-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "10 Canis Majoris",
	"OType" : "Be Star",
	"RA_S" : 101.11861,
	"DEC_S" : -31.07052337,
	"Constellation" : "Canis Major ",
	"AMag" : 5.214,
	"key" : 69258,
	"title" : "10 Canis Majoris"
	},
{
	"Index" : "36590",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 32411, SAO 151895, HD 49048, GC 8852, HR 2498, DM BD-14 1573, TYC 5391-3303-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2498",
	"OType" : "Star",
	"Distance" : "129.73",
	"RA_S" : 101.4974688,
	"DEC_S" : -14.7961269,
	"Constellation" : "Canis Major ",
	"AMag" : 5.306,
	"key" : 56590,
	"title" : "HR 2498"
	},
{
	"Index" : "36591",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "11 Canis Majoris, HIP 32492, SAO 151919, HD 49229, GC 8879, HR 2504, DM BD-14  1584, TYC 5391-3304-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "11 Canis Majoris",
	"OType" : "Star",
	"Distance" : "241.28",
	"RA_S" : 101.71288257,
	"DEC_S" : -14.42597216,
	"Constellation" : "Canis Major ",
	"AMag" : 5.267,
	"key" : 56591,
	"title" : "11 Canis Majoris"
	},
{
	"Index" : "40653",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 32677AB, SAO 151962, HD 49662, GC 8922, HR 2522, DM BD-14 1599, TYC 5950-2337-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR  2522",
	"OType" : "Star",
	"Distance" : "159.25",
	"RA_S" : 102.24056488,
	"DEC_S" : -15.14471225,
	"Constellation" : "Canis Major ",
	"AMag" : 5.389,
	"key" : 60653,
	"title" : "HR  2522"
	},
{
	"Index" : "49319",
	"Description" : "Kappa Canis Majoris (\u03BA CMa, \u03BA Canis Majoris) is a star in the constellation Canis Major. It is approximately 790 light years from Earth.\r\r\u03BA Canis Majoris is a blue-white B-type subgiant with a mean apparent magnitude of +3.50. This is a rapidly rotating Be star with 5.9 times the radius of the Sun. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +3.78 to +3.97.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "13 Canis Majoris, Kappa Canis Majoris, HIP 32759, SAO 197258, HD 50013, GC 8946, HR 2538, DM CD-32  3404, TYC 7092-2576-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Kappa Canis Majoris",
	"OType" : "Be Star",
	"Distance" : "201.88",
	"RA_S" : 102.46024719,
	"DEC_S" : -32.50847846,
	"X" : 394,
	"Y" : 355,
	"Constellation" : "Canis Major ",
	"AMag" : 3.486,
	"key" : 69319,
	"title" : "Kappa Canis Majoris"
	},
{
	"Index" : "40746",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "15 Canis Majoris, HIP 33092, SAO 172520, HD 50707, GC 9034, HR 2571, DM BD-20  1616, TYC 5958-3292-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "15 Canis Majoris",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "369.58",
	"RA_S" : 103.38711328,
	"DEC_S" : -20.22425492,
	"Constellation" : "Canis Major ",
	"AMag" : 4.773,
	"key" : 60746,
	"title" : "15 Canis Majoris"
	},
{
	"Index" : "45014",
	"Description" : "Omicron1 Canis Majoris (\u03BF1 CMa, \u03BF1 Canis Majoris) is a star in the constellation Canis Major.\r\r\u03BF1 Canis Majoris is an orange K-type supergiant with a mean apparent magnitude of +3.89. It is approximately 1980 light years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +3.78 to +3.99.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "16 Canis Majoris, Omicron01 Canis Majoris, HIP 33152, SAO 172542, HD 50877, GC 9059, HR 2580, DM CD-24  4567, TYC 6522-3271-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Omicron1 Canis Majoris",
	"OType" : "Red supergiant star",
	"RA_S" : 103.53314221,
	"DEC_S" : -24.18421182,
	"X" : 390,
	"Y" : 246,
	"Constellation" : "Canis Major ",
	"AMag" : 4.041,
	"key" : 65014,
	"title" : "Omicron1 Canis Majoris"
	},
{
	"Index" : "36544",
	"Description" : "Theta Canis Majoris (\u03B8 CMa, \u03B8 Canis Majoris) is a star in the constellation Canis Major.\r\r\u03B8 Canis Majoris is an orange K-type giant with an apparent magnitude of +4.08. This star is about the same mass as the Sun, but it has 30 times the Sun\u0027s radius. It is approximately 252 light years from Earth.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "14 Canis Majoris, Theta Canis Majoris, HIP 33160, SAO 152071, HD 50778, GC 9051, HR 2574, DM BD-11  1681, TYC 5388-2234-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Theta Canis Majoris",
	"OType" : "Star",
	"Distance" : "79.7",
	"RA_S" : 103.54748861,
	"DEC_S" : -12.03863013,
	"X" : 398,
	"Y" : 88,
	"Constellation" : "Canis Major ",
	"AMag" : 4.23,
	"key" : 56544,
	"title" : "Theta Canis Majoris"
	},
{
	"Index" : "40745",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "19 Canis Majoris, Pi Canis Majoris, HIP 33302, SAO 172579, HD 51199, GC 9096, HR 2590, DM BD-19  1610, TYC 5958-3291-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Pi Canis Majoris",
	"OType" : "Variable Star",
	"Distance" : "29.58",
	"RA_S" : 103.90595884,
	"DEC_S" : -20.13649738,
	"Constellation" : "Canis Major ",
	"AMag" : 4.708,
	"key" : 60745,
	"title" : "Pi Canis Majoris"
	},
{
	"Index" : "45012",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 33316, SAO 172588, HD 51283, GC 9099, HR 2595, DM BD-22 1602, TYC 6522-3269-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2595",
	"OType" : "Star in Cluster",
	"RA_S" : 103.94553422,
	"DEC_S" : -22.94144148,
	"Constellation" : "Canis Major ",
	"AMag" : 5.272,
	"key" : 65012,
	"title" : "HR 2595"
	},
{
	"Index" : "36601",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "18 Canis Majoris, Mu Canis Majoris, HIP 33345B, SAO 152123, HD 51250, GC 9103, HR 2593, DM BD-13  1741, TYC 5392-2413-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Isida",
	"OType" : "Star in double system",
	"Distance" : "381.6794",
	"RA_S" : 104.02769123,
	"DEC_S" : -14.04343111,
	"Constellation" : "Canis Major ",
	"AMag" : 5,
	"key" : 56601,
	"title" : "Isida"
	},
{
	"Index" : "36611",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "18 Canis Majoris, Mu Canis Majoris, HIP 33345A, TYC 5392-913-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "18 Mu Canis Majoris (Isida)",
	"OType" : "Star in double system",
	"Distance" : "381.6794",
	"RA_S" : 104.02769375,
	"DEC_S" : -14.0434681,
	"Constellation" : "Canis Major ",
	"AMag" : 5.271,
	"key" : 56611,
	"title" : "18 Mu Canis Majoris (Isida)"
	},
{
	"Index" : "40864",
	"Description" : "Iota Canis Majoris (\u03B9 CMa, \u03B9 Canis Majoris) is a star in the constellation Canis Major.\r\r\u03B9 Canis Majoris is a blue-white B-type bright giant with a mean apparent magnitude of +4.36. It is approximately 3100 light years from Earth. This star has 24.9 times the radius of the Sun. It is classified as a Beta Cephei type variable star and its brightness varies from magnitude +4.36 to +4.40 with a period of 1.92 hours.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "20 Canis Majoris, Iota Canis Majoris, HIP 33347, SAO 152126, HD 51309, GC 9107, HR 2596, DM BD-16  1661, TYC 5967-2618-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Iota Canis Majoris",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "747.99",
	"RA_S" : 104.03427079,
	"DEC_S" : -17.05423768,
	"X" : 388,
	"Y" : 152,
	"Constellation" : "Canis Major ",
	"AMag" : 4.371,
	"key" : 60864,
	"title" : "Iota Canis Majoris"
	},
{
	"Index" : "45153",
	"Description" : "Sigma Canis Majoris (\u03C3 CMa, \u03C3 Canis Majoris) is a star in the southern constellation of Canis Major. It is approximately 1,120 light-years (340 parsecs) from Earth and has an average apparent visual magnitude of +3.41.\r\r\u03C3 CMa is a supergiant star with a stellar classification of M1.5 Iab. This is a type of star that is in the late stages of its evolution, having consumed the hydrogen at its core and ballooned out to 420 times the Sun\u0027s radius. At 1.95 Astronomical Units, this is radius nearly double the average distance of the Earth from the Sun. It is currently radiating about 32,000 times the luminosity of the Sun from its outer envelope at an effective temperature of around 3,877 K. This gives it the cool orange-red hue of an M-type star.\r\rIt is classified as an irregular variable star and its brightness varies from magnitude +3.43 to +3.51. The magnetic field of this star has a strength below 1 G. It is suspected of being a member of the Collider 121 stellar association of co-moving stars, but this is disputed.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "22 Canis Majoris, Sigma Canis Majoris, HIP 33856, SAO 172797, HD 52877, GC 9276, HR 2646, DM CD-27  3544, TYC 6531-3793-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Sigma Canis Majoris",
	"OType" : "Long-period variable star",
	"Distance" : "341.89",
	"RA_S" : 105.42978085,
	"DEC_S" : -27.93483318,
	"X" : 365,
	"Y" : 293,
	"Constellation" : "Canis Major ",
	"AMag" : 3.656,
	"key" : 65153,
	"title" : "Sigma Canis Majoris"
	},
{
	"Index" : "45033",
	"Description" : "Omicron2 Canis Majoris (\u03BF\u00B2 CMa, \u03BF\u00B2 Canis Majoris) is a star in the constellation Canis Major. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It has an apparent visual magnitude of 3.043, making it one of the brighter members of the constellation. The distance to this star is roughly 2,800 light years (800 parsecs), with a 34% margin of error.\r\rThis is a massive supergiant star with a stellar classification of B3 Ia, indicating that, at the age of around 7 million years, it has exhausted the supply of hydrogen at its core and is now undergoing nuclear fusion of helium to generate energy. It has about 21 times the mass of the Sun and 65 times the Sun\u0027s radius. In all likelihood, it will end its life as a Type II supernova.\r\rOmicron2 Canis Majoris is one of the most luminous stars known, as it radiates about 220,000 times as much luminosity as the Sun from its outer envelope at a temperature of 15,500 K. At this heat, the star is glowing with the blue-white hue of a B-type star. This star is classified as an Alpha Cygni-type variable star that undergoes periodic non-radial pulsations, which cause its brightness to cycle from magnitude +2.93 to +3.08 over a 24.44 day interval. It is losing mass from its stellar wind at the rate of around 2 \u00D7 10\u20139 times the mass of the Sun per year, or the equivalent of the Sun\u0027s mass every 500 million years.\r\rWhile this star lies in the field of view of the open cluster named Collinder 121, it is unlikely to be a member. In fact, its optical neighbor, \u03BF1 Canis Majoris has a much higher likelihood of 23.1% based upon its proper motion being a closer match to the motion of the cluster. Although they are located near each other on the celestial sphere, \u03BF1 CMa and \u03BF2 CMa are most likely not gravitationally bound to each other as they appear to lie many light",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "24 Canis Majoris, Omicron02 Canis Majoris, HIP 33977, SAO 172839, HD 53138, GC 9307, HR 2653, DM CD-23  4797, TYC 6523-3722-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Omicron2 Canis Majoris",
	"OType" : "Pulsating variable Star",
	"Distance" : "847.4576",
	"RA_S" : 105.75613209,
	"DEC_S" : -23.83329149,
	"X" : 363,
	"Y" : 239,
	"Constellation" : "Canis Major ",
	"AMag" : 2.999,
	"key" : 65033,
	"title" : "Omicron2 Canis Majoris"
	},
{
	"Index" : "40821",
	"Description" : "Gamma Canis Majoris (\u03B3 CMa, \u03B3 Canis Majoris) is a star in the constellation Canis Major. It has the traditional name Muliphein, not to be confused with Muhlifain, which is Gamma Centauri; both names derive from the same Arabic root, \u0645\u062D\u0644\u0641\u064A\u0646 mu\u0127lifayn.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "23 Canis Majoris, Gamma Canis Majoris, HIP 34045, SAO 152303, HD 53244, GC 9320, HR 2657, DM BD-15  1625, TYC 5963-1938-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Muliphein",
	"OType" : "Star in Cluster",
	"Distance" : "135.37",
	"RA_S" : 105.93955264,
	"DEC_S" : -15.63328488,
	"X" : 365,
	"Y" : 133,
	"Constellation" : "Canis Major ",
	"AMag" : 4.078,
	"key" : 60821,
	"shortTitle" : "Muliphen; Isis; Mirza (also HD44743,116656)",
	"title" : "Muliphein"
	},
{
	"Index" : "36563",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 34301AB, SAO 152394, HD 53974, GC 9389, HR 2678, DM BD-11 1790, TYC 5389-3064-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "V* FN CMa",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "934.5794",
	"RA_S" : 106.66988935,
	"DEC_S" : -11.29402842,
	"Constellation" : "Canis Major ",
	"AMag" : 5.439,
	"key" : 56563,
	"title" : "V* FN CMa"
	},
{
	"Index" : "45168",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "27 Canis Majoris, HIP 34981AB, SAO 173264, HD 56014, GC 9608, HR 2745, DM CD-26  4057, TYC 6532-5000-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "27 Canis Majoris",
	"OType" : "Be Star",
	"Distance" : "514.04",
	"RA_S" : 108.56338299,
	"DEC_S" : -26.35250867,
	"Constellation" : "Canis Major ",
	"AMag" : 4.415,
	"key" : 65168,
	"title" : "27 Canis Majoris"
	},
{
	"Index" : "45171",
	"Description" : "Omega Canis Majoris (\u03C9 CMa, \u03C9 Canis Majoris) is a star in the constellation Canis Major.\r\r\u03C9 Canis Majoris is a blue-white B-type subgiant with a mean apparent magnitude of +4.01. It is approximately 920 light years from Earth. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +3.60 to +4.18.\r\rThis star has 6.2 times the radius of the Sun and its outer atmosphere has an effective temperature of 21,019 K.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "28 Canis Majoris, Omega Canis Majoris, HIP 35037, SAO 173282, HD 56139, GC 9625, HR 2749, DM CD-26  4073, TYC 6532-5003-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Omega Canis Majoris",
	"OType" : "Be Star",
	"Distance" : "278.58",
	"RA_S" : 108.7027253,
	"DEC_S" : -26.77266733,
	"X" : 328,
	"Y" : 277,
	"Constellation" : "Canis Major ",
	"AMag" : 4.004,
	"key" : 65171,
	"title" : "Omega Canis Majoris"
	},
{
	"Index" : "49422",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35083, SAO 197756, HD 56342, GC 9639, HR 2756, DM CD-30 4184, TYC 7103-2651-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2756",
	"OType" : "Star in Cluster",
	"Distance" : "192.26",
	"RA_S" : 108.83779294,
	"DEC_S" : -30.68644312,
	"Constellation" : "Canis Major ",
	"AMag" : 5.312,
	"key" : 69422,
	"title" : "HR 2756"
	},
{
	"Index" : "40844",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35180, SAO 152641, HD 56405, GC 9657, HR 2758, DM BD-15 1734, TYC 5965-363-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Gliese 9228 (HR 2758)",
	"OType" : "Star",
	"Distance" : "82.4",
	"RA_S" : 109.06063735,
	"DEC_S" : -15.58569158,
	"Constellation" : "Canis Major ",
	"AMag" : 5.457,
	"key" : 60844,
	"title" : "Gliese 9228 (HR 2758)"
	},
{
	"Index" : "45345",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35205, SAO 173360, HD 56618, GC 9678, HR 2766, DM CD-27 3852, TYC 6545-482-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2766",
	"OType" : "Star in Cluster",
	"Distance" : "123.84",
	"RA_S" : 109.14580496,
	"DEC_S" : -27.88117707,
	"Constellation" : "Canis Major ",
	"AMag" : 4.857,
	"key" : 65345,
	"title" : "HR 2766"
	},
{
	"Index" : "45236",
	"Description" : "HD 56577 is a star in the constellation Canis Major. Its apparent magnitude is 4.84.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "145 Canis Majoris, HIP 35210A, SAO 173349, HD 56577, GC 9675, HR 2764, DM CD-23  5189, TYC 6537-3290-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HD 56577",
	"OType" : "Star",
	"Distance" : "434.7826",
	"RA_S" : 109.15348398,
	"DEC_S" : -23.31559164,
	"X" : 323,
	"Y" : 231,
	"Constellation" : "Canis Major ",
	"AMag" : 5.001,
	"key" : 65236,
	"title" : "HD 56577"
	},
{
	"Index" : "45294",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "29 Canis Majoris, UW Canis Majoris, HIP 35412, SAO 173444, HD 57060, GC 9734, HR 2781, DM CD-24  5173, TYC 6541-4202-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "UW Canis Majoris",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "567.81",
	"RA_S" : 109.66824346,
	"DEC_S" : -24.55870067,
	"Constellation" : "Canis Major ",
	"AMag" : 4.927,
	"key" : 65294,
	"title" : "UW Canis Majoris"
	},
{
	"Index" : "45295",
	"Description" : "Tau Canis Majoris (\u03C4 CMa, \u03C4 Canis Majoris) is an eclipsing spectroscopic binary in the constellation Canis Major and the brightest star of an open cluster designated NGC 2362. It is approximately 3200 light years from Earth.\r\rThis star is sometimes known as the \u0027Mexican Jumping Star\u0027 by amateur astronomers, because it can appear to \u0027jump around\u0027 with respect to the other stars in the cluster because of its marked contrast in brightness.\r\r\u03C4 Canis Majoris is classified as an O-type blue supergiant with a mean apparent magnitude of +4.37. It is a Beta Lyrae type variable star with a period of 1.28 days, over which time its brightness varies from magnitude +4.32 to +4.37.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "30 Canis Majoris, Tau Canis Majoris, HIP 35415AP, SAO 173446, HD 57061, GC 9736, HR 2782, DM CD-24  5176, TYC 6541-4204-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "Tau Canis Majoris",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "917.4312",
	"RA_S" : 109.67702675,
	"DEC_S" : -24.95437258,
	"X" : 316,
	"Y" : 252,
	"Constellation" : "Canis Major ",
	"AMag" : 4.383,
	"key" : 65295,
	"title" : "Tau Canis Majoris"
	},
{
	"Index" : "45344",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35427, SAO 173453, HD 57146, GC 9740, HR 2786, DM CD-26 4164, TYC 6545-3167-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2786",
	"OType" : "Star",
	"Distance" : "378.96",
	"RA_S" : 109.71363822,
	"DEC_S" : -26.58585198,
	"Constellation" : "Canis Major ",
	"AMag" : 5.395,
	"key" : 65344,
	"title" : "HR 2786"
	},
{
	"Index" : "40932",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35727, SAO 152776, HD 57821, GC 9836, HR 2812, DM BD-18 1806, TYC 5974-3954-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2812",
	"OType" : "Star",
	"Distance" : "147.23",
	"RA_S" : 110.5563729,
	"DEC_S" : -19.01659949,
	"Constellation" : "Canis Major ",
	"AMag" : 4.941,
	"key" : 60932,
	"title" : "HR 2812"
	},
{
	"Index" : "49490",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35795, SAO 197925, HD 58155, GC 9862, HR 2819, DM CD-31 4437, TYC 7108-4764-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2819",
	"OType" : "Be Star",
	"Distance" : "388.43",
	"RA_S" : 110.75290267,
	"DEC_S" : -31.92378176,
	"Constellation" : "Canis Major ",
	"AMag" : 5.38,
	"key" : 69490,
	"title" : "HR 2819"
	},
{
	"Index" : "49491",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35855, SAO 197938, HD 58286, GC 9877, HR 2823, DM CD-31 4454, TYC 7108-4765-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2823",
	"OType" : "Star in Cluster",
	"Distance" : "386.48",
	"RA_S" : 110.88289431,
	"DEC_S" : -32.20207136,
	"Constellation" : "Canis Major ",
	"AMag" : 5.365,
	"key" : 69491,
	"title" : "HR 2823"
	},
{
	"Index" : "40849",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35951, SAO 152834, HD 58343, GC 9893, HR 2825, DM BD-15 1810, TYC 5966-1288-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2825",
	"OType" : "Be Star",
	"Distance" : "278.09",
	"RA_S" : 111.1674496,
	"DEC_S" : -16.20147468,
	"Constellation" : "Canis Major ",
	"AMag" : 5.208,
	"key" : 60849,
	"title" : "HR 2825"
	},
{
	"Index" : "49441",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35957A, SAO 197964, HD 58535, GC 9903, HR 2834, DM CD-31 4482, TYC 7104-3985-1",
	"group" : { "key" : "Canis Major" },
	"Common" : "HR 2834",
	"OType" : "Double or multiple star",
	"Distance" : "201",
	"RA_S" : 111.18272594,
	"DEC_S" : -31.80890234,
	"Constellation" : "Canis Major ",
	"AMag" : 5.4,
	"key" : 69441,
	"title" : "HR 2834"
	},
{
	"Index" : "5731",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "HIP 34987, SAO 115119, HD 55751, GC 9590, HR 2729, DM BD+03 1609, TYC 167-4147-1",
	"group" : { "backgroundImage" : "images/Alignment/18.png",
		"description" : "Canis Minor (pron.: /\u02CCke\u026An\u0268s \u02C8ma\u026An\u0259r/) is a small constellation in the northern celestial hemisphere. In the second century, it was included as an asterism, or pattern, of two stars in Ptolemy\u0027s 48 constellations, and is counted among the 88 modern constellations. Its name is Latin for \u0022lesser dog\u0022 in contrast to Canis Major, the \u0022greater dog\u0022; both figures are commonly represented as following the constellation of Orion the hunter.\r\rCanis Minor contains only two stars brighter than the fourth magnitude, Procyon (Alpha Canis Minoris), with a magnitude of 0.34, and Gomeisa (Beta Canis Minoris), with a magnitude of 2.9. The constellation\u0027s dimmer stars were noted by Johann Bayer, who named eight stars including Alpha and Beta, and John Flamsteed, who numbered fourteen. Procyon is the seventh-brightest star in the night sky, as well as one of the closest. A yellow-white main sequence star, it has a white dwarf companion. Gomeisa is a blue-white main sequence star. Luyten\u0027s Star is a ninth-magnitude red dwarf and the Solar System\u0027s next closest stellar neighbour in the constellation after Procyon. The fourth-magnitude HD 66141, which has evolved into an orange giant towards the end of its life cycle, was discovered to have a planet in 2012. There are two faint deep sky objects within the constellation\u0027s borders. The 11 Canis-Minorids are a meteor shower that can be seen in early December.\r\rThough strongly associated with the Classical Greek uranographic tradition, Canis Minor originates from ancient Mesopotamia. Procyon and Gomeisa were called MASH.TAB.BA or \u0022twins\u0022 in the Three Stars Each tablets, dating to around 1100 BC. In the later MUL.APIN, this name was also applied to the pairs of Pi3 and Pi4 Orionis and Zeta and Xi Orionis. The meaning of MASH.TAB.BA evolved as well, becoming the twin deities Lulal and Latarak, who are on the opposite side of the sky from Papsukal, the True Shepherd of Heaven in Babylonian mythology. Canis Minor was also given the name DAR.LUGAL, which translates to \u0022the star which stands behind it\u0022, in the MUL.APIN; the constellation represents a rooster. This name may have also referred to the constellation Lepus. DAR.LUGAL was also denoted DAR.MU\u0160EN and DAR.LUGAL.MU\u0160EN in Babylonia. Canis Minor was then called tarlugallu in Akkadian astronomy.\r\rCanis Minor was one of the original 48 constellations formulated by Ptolemy in his second-century Almagest, in which it was defined as a specific pattern (asterism) of stars; Ptolemy identified only two stars and hence no depiction was possible. The Ancient Greeks called the constellation \u03C0\u03C1\u03BF\u03BA\u03C5\u03C9\u03BD/Procyon, \u0022coming before the dog\u0022, transliterated into Latin as Antecanis, Praecanis, or variations thereof, by Cicero and others. Roman writers also appended the descriptors parvus, minor or minusculus (\u0022small\u0022 or \u0022lesser\u0022, for its faintness), septentrionalis (\u0022northerly\u0022, for its position in relation to Canis Major), primus (rising \u0022first\u0022) or sinister (rising to the \u0022left\u0022) to its name Canis. In Greek mythology, Canis Minor was sometimes connected with the Teumessian Fox, a beast turned into stone with its hunter, Laelaps, by Zeus, who placed them in heaven as Canis Major (Laelaps) and Canis Minor (Teumessian Fox). Eratosthenes accompanied the Little Dog with Orion, while Hyginus linked the constellation with Maera, a dog owned by Icarius of Athens. On discovering the latter\u0027s death, the dog and Icarius\u0027 daughter Erigone took their lives and all three were placed in the sky\u2014Erigone as Virgo and Icarius as Bootes.\r\rThe medieval Arabic astronomers maintained the depiction of Canis Minor (al-Kalb al-Asghar in Arabic) as a dog; in his Book of the Fixed Stars, Abd al-Rahman al-Sufi included a diagram of the constellation with a canine figure superimposed. There was one slight difference between the Ptolemaic vision of Canis Minor and the Arabic; al-Sufi claims Mirzam, now assigned to Orion, as part of both Canis Minor\u2014the collar of the dog\u2014and its modern home. The Arabic names for both Procyon and Gomeisa alluded to their proximity and resemblance to Sirius, though they were not direct translations of the Greek; Procyon was called ash-Shi\u0027ra ash-Shamiya, the \u0022Syrian Sirius\u0022 and Gomeisa was called ash-Shira al-Ghamisa, the Sirius with bleary eyes. Among the Merazig of Tunisia, shepherds note six constellations that mark the passage of the dry, hot season. One of them, called Merzem, includes the stars of Canis Minor and Canis Major and is the herald of two weeks of hot weather.\r\rAlternative names have been proposed: Johann Bayer in the early 17th century termed the constellation Fovea \u0022The Pit\u0022, and Morus \u0022Sycamine Tree\u0022. Seventeenth-century German poet and author Philippus Caesius linked it to the dog of Tobias from the Apocrypha. Richard A. Proctor gave the constellation the name Felis \u0022the Cat\u0022 in 1870 (contrasting with Canis Major, which he had abbreviated to Canis \u0022the Dog\u0022), explaining that he sought to shorten the constellation names to make them more manageable on celestial charts. Occasionally, Canis Minor is confused with Canis Major and given the name Canis Orionis (\u0022Orion\u0027s Dog\u0022).",
		"key" : "Canis Minor",
		"grouptype" : "Canis Minor",
		"Meaning" : "lesser dog",
		"Family" : "Orion",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Canis Minor",
		"title" : "Canis Minor Objects Group" },
	"Common" : "HR 2729",
	"OType" : "Star",
	"Distance" : "226.01",
	"RA_S" : 108.58359346,
	"DEC_S" : 3.11141805,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.48,
	"key" : 25731,
	"title" : "HR 2729"
	},
{
	"Index" : "54897",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "1 Canis Minoris, HIP 35987, SAO 96871, HD 58187, GC 9891, HR 2820, DM BD+11  1578, TYC 772-1776-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "1 Canis Minoris",
	"OType" : "Star",
	"Distance" : "96.92",
	"RA_S" : 111.24241522,
	"DEC_S" : 11.66952121,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.375,
	"key" : 74897,
	"title" : "1 Canis Minoris"
	},
{
	"Index" : "53950",
	"Description" : "Epsilon Canis Minoris (\u03B5 CMi, \u03B5 Canis Minoris) is a star in the constellation Canis Minor.\r\r\u03B5 Canis Minoris is a yellow G-type bright giant with an apparent magnitude of +4.99. It is approximately 990 light years from Earth.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "2 Canis Minoris, Epsilon Canis Minoris, HIP 36041, SAO 115425, HD 58367, GC 9908, HR 2828, DM BD+09  1643, TYC 764-2771-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Epsilon Canis Minoris",
	"OType" : "Star",
	"Distance" : "316.01",
	"RA_S" : 111.41207182,
	"DEC_S" : 9.27609612,
	"X" : 551,
	"Y" : 446,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.097,
	"key" : 73950,
	"title" : "Epsilon Canis Minoris"
	},
{
	"Index" : "53952",
	"Description" : "Beta Canis Minoris (\u03B2 CMi, \u03B2 Canis Minoris) is a star in the constellation of Canis Minor. In the night sky it is notable for its proximity to the prominent star Procyon. It has the traditional name Gomeisa, which comes from the Arabic al-ghumaisa\u0027 \u0022the bleary-eyed (woman)\u0022, short for \u0645\u0631\u0632\u0645 \u0627\u0644\u063A\u0645\u064A\u0635\u0627\u0621 mirzam al-ghumaisa\u0027 \u0022girdle of the bleary-eyed one\u0022. In Arabic, the short form would be identical with the name of Procyon.\r\rIn Chinese, \u5357\u6CB3 (N\u00E1n H\u00E9), meaning South River, refers to an asterism consisting of \u03B2 Canis Minoris, Procyon and \u03B5 Canis Minoris. Consequently, \u03B2 Canis Minoris itself is known as \u5357\u6CB3\u4E8C (N\u00E1n H\u00E9 \u00E8r, English: the Second Star of South River.)",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "3 Canis Minoris, Beta Canis Minoris, HIP 36188, SAO 115456, HD 58715, GC 9947, HR 2845, DM BD+08  1774, TYC 764-2774-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Gomeisa",
	"OType" : "Be Star",
	"Distance" : "49.57",
	"RA_S" : 111.78767391,
	"DEC_S" : 8.28931576,
	"X" : 547,
	"Y" : 460,
	"Constellation" : "Canis Minor ",
	"AMag" : 2.838,
	"key" : 73952,
	"shortTitle" : "Algomeyla; Gomelza; Gomejsa; Gomejza",
	"title" : "Gomeisa"
	},
{
	"Index" : "6485",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "5 Canis Minoris, Eta Canis Minoris, HIP 36265, SAO 115477, HD 58923, GC 9970, HR 2851, DM BD+07  1729, TYC 177-2986-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Eta Canis Minoris",
	"OType" : "Star",
	"Distance" : "97.49",
	"RA_S" : 112.00864271,
	"DEC_S" : 6.94197237,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.255,
	"key" : 26485,
	"title" : "Eta Canis Minoris"
	},
{
	"Index" : "53951",
	"Description" : "Gamma Canis Minoris (\u03B3 CMi, \u03B3 Canis Minoris) is a binary star in the constellation Canis Minor. It is approximately 398 light years from Earth.\r\r\u03B3 Canis Minoris is an orange K-type giant with an apparent magnitude of +4.34. It is a spectroscopic binary, and it has an unresolved companion which has an orbital period of 389 days.\r\rIts orange colour is obvious when seen through binoculars.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "4 Canis Minoris, Gamma Canis Minoris, HIP 36284, SAO 115478, HD 58972, GC 9974, HR 2854, DM BD+09  1660, TYC 764-2772-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Gamma Canis Minoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "97.32",
	"RA_S" : 112.04081045,
	"DEC_S" : 8.92553211,
	"X" : 543,
	"Y" : 452,
	"Constellation" : "Canis Minor ",
	"AMag" : 4.48,
	"key" : 73951,
	"title" : "Gamma Canis Minoris"
	},
{
	"Index" : "54896",
	"Description" : "6 Canis Minoris is a star in the constellation Canis Minor.\r\r6 Canis Minoris is an orange K-type giant with an apparent magnitude of +4.55. It is approximately 560 light years from Earth. It has four times the mass of the Sun.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "6 Canis Minoris, HIP 36425, SAO 96952, HD 59294, GC 10024, HR 2864, DM BD+12  1567, TYC 772-1775-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "6 Canis Minoris",
	"OType" : "Variable Star",
	"Distance" : "175.15",
	"RA_S" : 112.449097,
	"DEC_S" : 12.00656121,
	"X" : 535,
	"Y" : 411,
	"Constellation" : "Canis Minor ",
	"AMag" : 4.676,
	"key" : 74896,
	"title" : "6 Canis Minoris"
	},
{
	"Index" : "6864",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "7 Canis Minoris, Delta01 Canis Minoris, HIP 36641, SAO 115581, HD 59881, GC 10085, HR 2880, DM BD+02  1691, TYC 182-2739-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Delta01 Canis Minoris",
	"OType" : "Star",
	"Distance" : "232",
	"RA_S" : 113.02478384,
	"DEC_S" : 1.91447711,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.261,
	"key" : 26864,
	"title" : "Delta01 Canis Minoris"
	},
{
	"Index" : "55669",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "11 Canis Minoris, HIP 37921, SAO 97224, HD 62832, GC 10463, HR 3008, DM BD+11  1670, TYC 782-542-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "11 Canis Minoris",
	"OType" : "Variable Star",
	"Distance" : "92.37",
	"RA_S" : 116.56750237,
	"DEC_S" : 10.76825481,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.238,
	"key" : 75669,
	"title" : "11 Canis Minoris"
	},
{
	"Index" : "6698",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "13 Canis Minoris, Zeta Canis Minoris, HIP 38373, SAO 116043, HD 63975, GC 10622, HR 3059, DM BD+02  1808, TYC 180-2565-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "Zeta Canis Minoris",
	"OType" : "Star",
	"Distance" : "190.12",
	"RA_S" : 117.92494572,
	"DEC_S" : 1.7668666,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.092,
	"key" : 26698,
	"title" : "Zeta Canis Minoris"
	},
{
	"Index" : "7019",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "14 Canis Minoris, HIP 38962, SAO 116182, HD 65345, GC 10776, HR 3110, DM BD+02  1833, TYC 185-2499-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "14 Canis Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "74.02",
	"RA_S" : 119.58606168,
	"DEC_S" : 2.22476425,
	"Constellation" : "Canis Minor ",
	"AMag" : 5.407,
	"key" : 27019,
	"title" : "14 Canis Minoris"
	},
{
	"Index" : "8123",
	"Description" : "HD 66141, also known as HR 3145 and 50 G. Canis Minoris, is the main star of a binary system in the constellation Canis Minor. It is an orange K-type giant, approximately 254 light years from Earth. Its apparent magnitude is +4.39.\r\rWhen first catalogued it was in the Puppis constellation and was designated \u002213 Puppis\u0022, but it subsequently migrated to Canis Minor. Bode gave it the Bayer designation of Lambda Canis Minoris.\r\rOver 2003 to 2012 a starspot was periodically dimming its light.",
	"MapNum" : "18",
	"ImageNum" : "18",
	"Desig" : "G Canis Minoris, HIP 39311, SAO 116260, HD 66141, GC 10891, HR 3145, DM BD+02  1854, TYC 198-2137-1",
	"group" : { "key" : "Canis Minor" },
	"Common" : "HD 66141",
	"OType" : "Star",
	"Distance" : "77.85",
	"RA_S" : 120.56640053,
	"DEC_S" : 2.33457164,
	"X" : 436,
	"Y" : 545,
	"Constellation" : "Canis Minor ",
	"AMag" : 4.524,
	"key" : 28123,
	"title" : "HD 66141"
	},
{
	"Index" : "39007",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "5 Capricorni, Alpha01 Capricorni, HIP 100027AE, SAO 163422, HD 192876, GC 28189, HR 7747, DM BD-12  5683, TYC 5748-2598-1",
	"group" : { "backgroundImage" : "images/Alignment/12.png",
		"description" : "Capricornus (pron.: /\u02CCk\u00E6pr\u0268\u02C8k\u0254rn\u0259s/) is one of the constellations of the zodiac; it is often called Capricorn, especially when referring to the corresponding astrological sign. Its name is Latin for \u0022horned goat\u0022 or \u0022goat horn\u0022, and it is commonly represented in the form of a sea-goat: a mythical creature that is half goat, half fish. Its symbol is \u2651.\r\rCapricornus is one of the 88 modern constellations, and was also one of the 48 constellations listed by the 2nd century astronomer Ptolemy. Under its modern boundaries it is bordered by Aquila, Sagittarius, Microscopium, Piscis Austrinus and Aquarius. The constellation is located in an area of sky called the Sea or the Water, consisting of many water-related constellations such as Aquarius, Pisces and Eridanus. It is the second faintest constellation in the zodiac after Cancer, and it is the smallest constellation in the zodiac.\r\rDespite its faintness, Capricornus has one of the oldest mythological associations, having been consistently represented as a hybrid of a goat and a fish since the Middle Bronze Age. First attested in depictions on a cylinder-seal from around the 21st century BC, it was explicitly recorded in the Babylonian star catalogues as MULSU\u1E2AUR.MA\u0160 \u0022The Goat-Fish\u0022 before 1000 BC. The constellation was a symbol of the god Ea and in the Early Bronze Age marked the winter solstice.\r\rDue to the precession of the equinoxes the December solstice no longer takes place while the sun is in the constellation Capricornus, as it did until 130 BCE, but the astrological sign called Capricorn begins with the solstice. The solstice now takes place when the Sun is in Sagittarius. The sun\u0027s most southerly position, which is attained at the northern hemisphere\u0027s winter solstice, is now called the Tropic of Capricorn, a term which also applies to the line on the Earth at which the sun is directly overhead at noon on that solstice. The Sun is now in Capricorn from late January through mid-February.\r\rIn Greek mythology, the constellation is sometimes identified as Amalthea, the goat that suckled the infant Zeus after his mother Rhea saved him from being devoured by his father Cronos (in Greek mythology). The goat\u0027s broken horn was transformed into the cornucopia or horn of plenty. Capricornus is also sometimes identified as Pan, the god with a goat\u0027s head, who saved himself from the monster Typhon by giving himself a fish\u0027s tail and diving into a river.\r\rThe planet Neptune was discovered in Capricornus by German astronomer Johann Galle, near Deneb Algedi (\u03B4 Capricorni) on September 23, 1846, which is appropriate as Capricornus can be seen best from Europe at 4:00am in September.",
		"key" : "Capricornus",
		"grouptype" : "Capricornus",
		"Meaning" : "sea goat",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Capricornus",
		"title" : "Capricornus Objects Group" },
	"Common" : "Prima Giedi",
	"OType" : "Double or multiple star",
	"Distance" : "173.83",
	"RA_S" : 304.41195507,
	"DEC_S" : -12.50821473,
	"Constellation" : "Capricornus ",
	"AMag" : 4.342,
	"key" : 59007,
	"shortTitle" : "Algiedi Prima; Algedi (with HD192947)",
	"title" : "Prima Giedi"
	},
{
	"Index" : "39012",
	"Description" : "Alpha2 Capricorni (\u03B12 Cap, \u03B12 Capricorni) is a star in the constellation Capricornus. It also has the traditional star name Secunda Giedi or Algiedi Secunda, and shares the name Algedi (from \u0627\u0644\u062C\u062F\u064A - al-jadii, meaning the goat) with \u03B1\u00B9 Capricorni.\r\rIn Chinese, \u725B\u5BBF (Ni\u00FA Su), meaning Ox (asterism), refers to an asterism consisting of \u03B1\u00B2 Capricorni, \u03B2 Capricorni, \u03BE2 Capricorni, \u03C0 Capricorni, \u03BF Capricorni and \u03C1 Capricorni. Consequently, \u03B1\u00B2 Capricorni itself is known as \u725B\u5BBF\u4E8C (Ni\u00FA Su \u00E8r, English: the Second Star of Ox.)\r\r\u03B12 Capricorni is a yellow G-type giant with an apparent magnitude of +3.58. It is approximately 109 light years from Earth.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "6 Capricorni, Alpha02 Capricorni, HIP 100064, SAO 163427, HD 192947, GC 28200, HR 7754, DM BD-12  5685, TYC 5749-2530-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Secunda Giedi / Algiedi Secunda",
	"OType" : "Star",
	"Distance" : "32.44",
	"RA_S" : 304.51356645,
	"DEC_S" : -12.54485232,
	"X" : 482,
	"Y" : 162,
	"Constellation" : "Capricornus ",
	"AMag" : 3.665,
	"key" : 59012,
	"shortTitle" : "Algedi (with HD192876); Secunda Giedi; Algiedi Secunda; Deneb Al'gedi; Gnedi",
	"title" : "Secunda Giedi / Algiedi Secunda"
	},
{
	"Index" : "43558",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "7 Capricorni, Sigma Capricorni, HIP 100195, SAO 163445, HD 193150, GC 28233, HR 7761, DM BD-19  5776, TYC 6336-1995-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Sigma Capricorni",
	"OType" : "Star",
	"Distance" : "339.87",
	"RA_S" : 304.84835007,
	"DEC_S" : -19.11853278,
	"Constellation" : "Capricornus ",
	"AMag" : 5.427,
	"key" : 63558,
	"title" : "Sigma Capricorni"
	},
{
	"Index" : "39013",
	"Description" : "Nu Capricorni (\u03BD Cap, \u03BD Capricorni) is a binary star in the constellation Capricornus. It has the traditional name Alshat, from the Arabic \u0627\u0644\u0634\u0627\u0629 a\u0161-\u0161\u0101, meaning the sheep that was to be slaughtered by the adjacent Dabih . It is approximately 272 light years from Earth.\r\rThe primary component, \u03BD Capricorni A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.77. Its companion, \u03BD Capricorni B, is a twelfth magnitude star located 54 arcseconds or at least 4000 AU from the primary.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "8 Capricorni, Nu Capricorni, HIP 100310, SAO 163468, HD 193432, GC 28282, HR 7773, DM BD-13  5642, TYC 5749-2531-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Alshat",
	"OType" : "Star",
	"Distance" : "77.6",
	"RA_S" : 305.16589961,
	"DEC_S" : -12.75908049,
	"X" : 479,
	"Y" : 164,
	"Constellation" : "Capricornus ",
	"AMag" : 4.741,
	"key" : 59013,
	"title" : "Alshat"
	},
{
	"Index" : "39034",
	"Description" : "Beta Capricorni (\u03B2 Cap, \u03B2 Capricorni) is a star system in the constellation Capricornus. It has the traditional name Dabih, which comes from the Arabic \u0627\u0644\u0630\u0627\u0628\u062D al-dh\u0101bi\u1E25, meaning \u0022the butcher\u0022. The \u03B2 Capricorni system is located 328 light years from Earth. Because it is near the ecliptic, \u03B2 Capricorni can be occulted by the Moon, and also (rarely) by planets.\r\rIn Chinese, \u725B\u5BBF (Ni\u00FA Su), meaning Ox (asterism), refers to an asterism consisting of \u03B2 Capricorni, \u03B12 Capricorni, \u03BE2 Capricorni, \u03C0 Capricorni, \u03BF Capricorni and \u03C1 Capricorni. Consequently, \u03B2 Capricorni itself is known as \u725B\u5BBF\u4E00 (Ni\u00FA Su y\u012B, English: the First Star of Ox.)",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "9 Capricorni, Beta Capricorni, HIP 100345, SAO 163481, HD 193496, GC 28295, HR 7776, DM BD-15  5629A, TYC 5753-2281-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Dabih",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.23",
	"RA_S" : 305.25280077,
	"DEC_S" : -14.78140739,
	"X" : 469,
	"Y" : 192,
	"Constellation" : "Capricornus ",
	"AMag" : 3.151,
	"key" : 59034,
	"title" : "Dabih"
	},
{
	"Index" : "43539",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "10 Capricorni, Pi Capricorni, HIP 100881A, SAO 163592, HD 194636, GC 28442, HR 7814, DM BD-18  5685, TYC 6333-2129-2",
	"group" : { "key" : "Capricornus" },
	"Common" : "Okul",
	"OType" : "Spectroscopic binary",
	"Distance" : "165.36",
	"RA_S" : 306.83004169,
	"DEC_S" : -18.21172389,
	"Constellation" : "Capricornus ",
	"AMag" : 5.13,
	"key" : 63539,
	"title" : "Okul"
	},
{
	"Index" : "43537",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "11 Capricorni, Rho Capricorni, HIP 101027A, SAO 163614, HD 194943A, GC 28481, HR 7822, DM BD-18  5689, TYC 6333-2128-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Rho Capricorni",
	"OType" : "Star",
	"Distance" : "30.26",
	"RA_S" : 307.21508142,
	"DEC_S" : -17.8137256,
	"Constellation" : "Capricornus ",
	"AMag" : 4.967,
	"key" : 63537,
	"title" : "Rho Capricorni"
	},
{
	"Index" : "39128",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "14 Capricorni, Tau Capricorni, HIP 101923AB, SAO 163771, HD 196662, GC 28748, HR 7889, DM BD-15  5743, TYC 5767-2439-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Tau Capricorni",
	"OType" : "Star",
	"Distance" : "348.4321",
	"RA_S" : 309.81802376,
	"DEC_S" : -14.95477825,
	"Constellation" : "Capricornus ",
	"AMag" : 5.231,
	"key" : 59128,
	"title" : "Tau Capricorni"
	},
{
	"Index" : "43549",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "15 Capricorni, Upsilon Capricorni, HIP 101984, SAO 163779, HD 196777, GC 28777, HR 7900, DM BD-18  5738, TYC 6335-1121-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Upsilon Capricorni",
	"OType" : "Variable Star",
	"Distance" : "177.37",
	"RA_S" : 310.01227116,
	"DEC_S" : -18.13866131,
	"Constellation" : "Capricornus ",
	"AMag" : 5.337,
	"key" : 63549,
	"title" : "Upsilon Capricorni"
	},
{
	"Index" : "47934",
	"Description" : "Psi Capricorni (\u03C8 Cap, \u03C8 Capricorni) is a star in the constellation Capricornus. \u03C8 Capricorni is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.13. It is approximately 47.9 light years from Earth. The measured rotational velocity of this star is approximately 37 km/s (the Sun has an equatorial rotation velocity of 2 km/s).\r\rIn Chinese, \u5929\u7530 (Ti\u0101n Ti\u00E1n), meaning Celestial Farmland, refers to an asterism consisting of \u03C8 Capricorni, \u03C9 Capricorni, 3 Piscis Austrini, and 24 Capricorni. Consequently, \u03C9 Capricorni itself is known as \u5929\u7530\u56DB (Ti\u0101n Ti\u00E1n s\u00EC, English: the Fourth Star of Celestial Farmland.)\r\rIn R. H. Allen\u0027s version, this star was represent the state Yue.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "16 Capricorni, Psi Capricorni, HIP 102485, SAO 189664, HD 197692, GC 28929, HR 7936, DM CD-25 15018, TYC 6925-1576-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Psi Capricorni",
	"OType" : "Star",
	"Distance" : "14.68",
	"RA_S" : 311.52388594,
	"DEC_S" : -25.27089755,
	"X" : 387,
	"Y" : 326,
	"Constellation" : "Capricornus ",
	"AMag" : 4.172,
	"key" : 67934,
	"title" : "Psi Capricorni"
	},
{
	"Index" : "47969",
	"Description" : "Omega Capricorni (\u03C9 Cap, \u03C9 Capricorni) is a star in the constellation Capricornus, with the traditional but seldom used name Baten Algiedi, which is Arabic for \u0022belly of the goat\u0022.\r\rIn Chinese, \u5929\u7530 (Ti\u0101n Ti\u00E1n), meaning Celestial Farmland, refers to an asterism consisting of \u03C9 Capricorni, 3 Piscis Austrini, 24 Capricorni and \u03C8 Capricorni. Consequently, \u03C9 Capricorni itself is known as \u5929\u7530\u4E8C (Ti\u0101n Ti\u00E1n \u00E8r, English: the First Star of Celestial Farmland.)\r\r\u03C9 Capricorni is a M-type red giant with an apparent magnitude of +4.12. It is also classed as a variable star because of its regular fluctuations in luminosity and absolute magnitude. It is approximately 630 light years from Earth.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "18 Capricorni, Omega Capricorni, HIP 102978, SAO 189781, HD 198542, GC 29079, HR 7980, DM CD-27 15082, TYC 6930-987-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Baten Algiedi",
	"OType" : "Variable Star",
	"Distance" : "249.17",
	"RA_S" : 312.9553789,
	"DEC_S" : -26.91913232,
	"X" : 370,
	"Y" : 347,
	"Constellation" : "Capricornus ",
	"AMag" : 4.289,
	"key" : 67969,
	"title" : "Baten Algiedi"
	},
{
	"Index" : "43670",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "22 Capricorni, Eta Capricorni, HIP 104019AB, SAO 189986, HD 200499, GC 29419, HR 8060, DM BD-20  6115, TYC 6354-1492-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Arm",
	"OType" : "Double or multiple star",
	"Distance" : "49.41",
	"RA_S" : 316.10125551,
	"DEC_S" : -19.85499196,
	"Constellation" : "Capricornus ",
	"AMag" : 4.868,
	"key" : 63670,
	"title" : "Arm"
	},
{
	"Index" : "43647",
	"Description" : "Theta Capricorni (\u03B8 Cap, \u03B8 Capricorni) is a star in the constellation Capricornus. \u03B8 Capricorni is a white A-type main sequence dwarf with an apparent magnitude of +4.08. It is approximately 158 light years from Earth.\r\rSometimes, this star is called by the name Dorsum, meaning the back (of the goat) in Latin.\r\rIn Chinese, \u5341\u4E8C\u570B (Sh\u00EDer Gu\u00F3), meaning Twelve States, refers to an asterism which is represent twelve ancient states in the Spring and Autumn Period and the Warring States Period, consisting of \u03B8 Capricorni, \u03C6 Capricorni, \u03B9 Capricorni, 38 Capricorni, 35 Capricorni, 36 Capricorni, \u03C7 Capricorni, 30 Capricorni, 33 Capricorni, \u03B6 Capricorni, 19 Capricorni, 26 Capricorni, 27 Capricorni, 20 Capricorni, \u03B7 Capricorni and 21 Capricorni,. Consequently, \u03B8 Capricorni itself is known as \u79E6\u4E00 (Qin y\u012B, English: the First Star of Qin), meaning that this star (together with 30 Capricorni and \u03B4 Serpentis in Right Wall of Heavenly Market Enclosure (asterism)) represent the state Qin (\u79E6) (or Tsin)",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "23 Capricorni, Theta Capricorni, HIP 104139, SAO 164132, HD 200761, GC 29460, HR 8075, DM BD-17  6174, TYC 6350-1499-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Dorsum",
	"OType" : "Star",
	"Distance" : "49.71",
	"RA_S" : 316.48678263,
	"DEC_S" : -17.23286169,
	"X" : 328,
	"Y" : 221,
	"Constellation" : "Capricornus ",
	"AMag" : 4.07,
	"key" : 63647,
	"title" : "Dorsum"
	},
{
	"Index" : "47948",
	"Description" : "24 Capricorni is a star in the constellation Capricornus. 24 Capricorni is a M-type red giant with an apparent magnitude of +4.49. It is approximately 523 light years from Earth.\r\rIn R.H.Allen\u0027s version, this star was represent the state Chu (or Tsoo).",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "24 Capricorni, A Capricorni, HIP 104234, SAO 190025, HD 200914, GC 29490, HR 8080, DM CD-25 15235, TYC 6928-335-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "24 Capricorni",
	"OType" : "Star",
	"Distance" : "139.7",
	"RA_S" : 316.78195142,
	"DEC_S" : -25.00585286,
	"X" : 325,
	"Y" : 322,
	"Constellation" : "Capricornus ",
	"AMag" : 4.692,
	"key" : 67948,
	"title" : "24 Capricorni"
	},
{
	"Index" : "43694",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "25 Capricorni, Chi Capricorni, HIP 104365, SAO 190050, HD 201184, GC 29543, HR 8087, DM BD-21  5933, TYC 6358-1841-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Chi Capricorni",
	"OType" : "Star",
	"Distance" : "55.11",
	"RA_S" : 317.14010537,
	"DEC_S" : -21.19367159,
	"Constellation" : "Capricornus ",
	"AMag" : 5.316,
	"key" : 63694,
	"title" : "Chi Capricorni"
	},
{
	"Index" : "43703",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "28 Capricorni, Phi Capricorni, HIP 104963, SAO 190173, HD 202320, GC 29722, HR 8127, DM BD-21  5974, TYC 6359-1519-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Phi Capricorni",
	"OType" : "Star",
	"Distance" : "196.66",
	"RA_S" : 318.9079168,
	"DEC_S" : -20.65169723,
	"Constellation" : "Capricornus ",
	"AMag" : 5.282,
	"key" : 63703,
	"title" : "Phi Capricorni"
	},
{
	"Index" : "43653",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "30 Capricorni, HIP 105143, SAO 164286, HD 202671, GC 29781, HR 8137, DM BD-18  5903, TYC 6351-1446-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "30 Capricorni",
	"OType" : "Star",
	"Distance" : "163.16",
	"RA_S" : 319.4886916,
	"DEC_S" : -17.98513813,
	"Constellation" : "Capricornus ",
	"AMag" : 5.364,
	"key" : 63653,
	"title" : "30 Capricorni"
	},
{
	"Index" : "43711",
	"Description" : "Iota Capricorni (\u03B9 Cap, \u03B9 Capricorni) is a star in the constellation Capricornus.\r\r\u03B9 Capricorni is a yellow G-type giant with a mean apparent magnitude of +4.28. It is approximately 216 light years from Earth. It is classified as a BY Draconis type variable star and its brightness varies by 0.06 magnitudes.\r\rIn Chinese, \u5341\u4E8C\u570B (Sh\u00EDer Gu\u00F3), meaning Twelve States, refers to an asterism which is represent twelve ancient states in the Spring and Autumn Period and the Warring States Period, consisting of \u03B9 Capricorni, \u03C6 Capricorni, 38 Capricorni, 35 Capricorni, 36 Capricorni, \u03C7 Capricorni, \u03B8 Capricorni, 30 Capricorni, 33 Capricorni, \u03B6 Capricorni, 19 Capricorni, 26 Capricorni, 27 Capricorni, 20 Capricorni, \u03B7 Capricorni and 21 Capricorni. Consequently, \u03B9 Capricorni itself is known as \u4EE3\u4E00 (D\u00E0i y\u012B, English: the First Star of Dai), meaning that this star (together with 37 Capricorni) represent the state Dai (or Tae)(\u4EE3).",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "32 Capricorni, Iota Capricorni, HIP 105515, SAO 164346, HD 203387, GC 29903, HR 8167, DM BD-17  6245, TYC 6360-1220-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Iota Capricorni",
	"OType" : "Variable of BY Dra type",
	"Distance" : "60.29",
	"RA_S" : 320.56164914,
	"DEC_S" : -16.83454194,
	"X" : 277,
	"Y" : 216,
	"Constellation" : "Capricornus ",
	"AMag" : 4.377,
	"key" : 63711,
	"title" : "Iota Capricorni"
	},
{
	"Index" : "43773",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "33 Capricorni, HIP 105665, SAO 190295, HD 203638, GC 29953, HR 8183, DM BD-21  6007, TYC 6372-1276-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "33 Capricorni",
	"OType" : "Variable Star",
	"Distance" : "73.29",
	"RA_S" : 321.03997058,
	"DEC_S" : -20.85187098,
	"Constellation" : "Capricornus ",
	"AMag" : 5.496,
	"key" : 63773,
	"title" : "33 Capricorni"
	},
{
	"Index" : "43775",
	"Description" : "Zeta Capricorni, (\u03B6 Cap, \u03B6 Capricorni), is a fourth-magnitude star in the constellation Capricornus. \u03B6 Capricorni is a binary star, with the primary component \u03B6 Capricorni A being a yellow G-type supergiant with an apparent magnitude of +3.77. It is considered one of the prototypical examples of a Barium star, properties of which include overabundances of carbon molecules (such as C2) and s-process elements. Zeta Capricorni has an overabundance of the s-process element praseodymium.\r\rIts companion, \u03B6 Capricorni B is a white dwarf.\r\rThe \u03B6 Capricorni binary system is approximately 398 light years from Earth.\r\rIn Chinese, \u5341\u4E8C\u570B (Sh\u00EDer Gu\u00F3), meaning Twelve States, refers to an asterism which represents twelve ancient states in the Spring and Autumn Period and the Warring States Period, consisting of \u03B6 Capricorni, \u03C6 Capricorni, \u03B9 Capricorni, 38 Capricorni, 35 Capricorni, 36 Capricorni, \u03C7 Capricorni, \u03B8 Capricorni, 30 Capricorni, 33 Capricorni, 19 Capricorni, 26 Capricorni, 27 Capricorni, 20 Capricorni, \u03B7 Capricorni and 21 Capricorni. Consequently, \u03B6 Capricorni itself represents the state of Yan (\u71D5)., together with \u03BD Ophiuchi in Left Wall of Heavenly Market Enclosure (asterism).",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "34 Capricorni, Zeta Capricorni, HIP 105881, SAO 190341, HD 204075, GC 30020, HR 8204, DM CD-22 15388, TYC 6372-1278-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Zeta Capricorni",
	"OType" : "Spectroscopic binary",
	"Distance" : "118.12",
	"RA_S" : 321.66677642,
	"DEC_S" : -22.4113345,
	"X" : 266,
	"Y" : 289,
	"Constellation" : "Capricornus ",
	"AMag" : 3.841,
	"key" : 63775,
	"title" : "Zeta Capricorni"
	},
{
	"Index" : "43780",
	"Description" : "36 Capricorni is a star in the constellation Capricornus. 36 Capricorni is an orange K-type giant with an apparent magnitude of +4.50. It is approximately 179 light years from Earth and has 3.46 times the mass of the Sun.\r\rIn Chinese, \u5341\u4E8C\u570B (Sh\u00EDer Gu\u00F3), meaning Twelve States, refers to an asterism which is represent twelve ancient states in the Spring and Autumn Period and the Warring States Period, consisting of 36 Capricorni, \u03C6 Capricorni, \u03B9 Capricorni, 37 Capricorni, 35 Capricorni, \u03C7 Capricorni, \u03B8 Capricorni, 30 Capricorni, 33 Capricorni, \u03B6 Capricorni, 19 Capricorni, 26 Capricorni, 27 Capricorni, 20 Capricorni, \u03B7 Capricorni and 21 Capricorni. Consequently, 36 Capricorni itself is represent the state Jin (\u6649)(or Tsin)., together with \u03BA Herculis in Right Wall of Heavenly Market Enclosure (asterism)",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "36 Capricorni, b Capricorni, HIP 106039, SAO 190374, HD 204381, GC 30059, HR 8213, DM BD-22  5692, TYC 6373-1203-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "36 Capricorni",
	"OType" : "Star",
	"Distance" : "52.45",
	"RA_S" : 322.18083351,
	"DEC_S" : -21.80718172,
	"X" : 260,
	"Y" : 282,
	"Constellation" : "Capricornus ",
	"AMag" : 4.602,
	"key" : 63780,
	"title" : "36 Capricorni"
	},
{
	"Index" : "43759",
	"Description" : "Epsilon Capricorni (\u03B5 Cap, \u03B5 Capricorni) is a triple star system in the constellation Capricornus. It also has the traditional star name Castra or Kastra, meaning \u0022fort\u0022 or \u0022military camp\u0022 in Latin. It is approximately 660 light years from Earth.\r\rIn Chinese, \u58D8\u58C1\u9663 (L\u011Bi B\u00EC Zh\u00E8n), meaning Line of Ramparts, refers to an asterism consisting of \u03B5 Capricorni, \u03BA Capricorni, \u03B3 Capricorni, \u03B4 Capricorni, \u03B9 Aquarii, \u03C3 Aquarii, \u03BB Aquarii, \u03C6 Aquarii, 27 Piscium, 29 Piscium, 33 Piscium and 30 Piscium. Consequently, \u03B5 Capricorni itself is known as \u58D8\u58C1\u9663\u4E8C (L\u011Bi B\u00EC Zh\u00E8n \u00E8r, English: the Second Star of Line of Ramparts.)\r\rThe primary component, \u03B5 Capricorni A, is a blue-white B-type main sequence dwarf with a mean apparent magnitude of +4.51. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.48 to +4.72. It is a spectroscopic binary, and the two subcomponents have apparent magnitudes of +5.0 and +6.3 and are separated by 0.0047 arcseconds (1 AU).\r\rFurther out, 68 arcseconds away, is \u03B5 Capricorni B which is at least 13,000 AU, or 0.22 light years away from the close binary. It is an orange K-type giant with an apparent magnitude of +9.5.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "39 Capricorni, Epsilon Capricorni, HIP 106723, SAO 164520, HD 205637, GC 30252, HR 8260, DM BD-20  6251, TYC 6370-1176-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Castra / Kastra",
	"OType" : "Be Star",
	"Distance" : "322.31",
	"RA_S" : 324.27012783,
	"DEC_S" : -19.46601288,
	"X" : 233,
	"Y" : 253,
	"Constellation" : "Capricornus ",
	"AMag" : 4.486,
	"key" : 63759,
	"title" : "Castra / Kastra"
	},
{
	"Index" : "43715",
	"Description" : "Gamma Capricorni (\u03B3 Cap, \u03B3 Capricorni) is a giant star in the constellation Capricornus. It has the traditional name Nashira, which comes from the Arabic \u0633\u0639\u062F \u0646\u0627\u0634\u0631\u0629 - sa\u0027d nashirah for \u0022the lucky one\u0022 or \u0022bearer of good news\u0022.\r\rIn Chinese, \u58D8\u58C1\u9663 (L\u011Bi B\u00EC Zh\u00E8n), meaning Line of Ramparts, refers to an asterism consisting of \u03B3 Capricorni, \u03BA Capricorni, \u03B5 Capricorni, \u03B4 Capricorni, \u03B9 Aquarii, \u03C3 Aquarii, \u03BB Aquarii, \u03C6 Aquarii, 27 Piscium, 29 Piscium, 33 Piscium and 30 Piscium. Consequently, \u03B3 Capricorni itself is known as \u58D8\u58C1\u9663\u4E09 (L\u011Bi B\u00EC Zh\u00E8n s\u0101n, English: the Third Star of Line of Ramparts.)\r\rBecause it is near the ecliptic, \u03B3 Capricorni can be occulted by the Moon, and (rarely) by planets.\r\r\u03B3 Capricorni is a blue-white A-type (A7III) giant star with a mean apparent magnitude of +3.69. It is approximately 139 light years from Earth. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies by 0.03 magnitudes.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "40 Capricorni, Gamma Capricorni, HIP 106985, SAO 164560, HD 206088, GC 30320, HR 8278, DM BD-17  6340, TYC 6362-1078-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Nashira",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "48.08",
	"RA_S" : 325.02273533,
	"DEC_S" : -16.66230756,
	"X" : 222,
	"Y" : 216,
	"Constellation" : "Capricornus ",
	"AMag" : 3.704,
	"key" : 63715,
	"title" : "Nashira"
	},
{
	"Index" : "39313",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "42 Capricorni, HIP 107095, SAO 164580, HD 206301, GC 30354, HR 8283, DM BD-14  6102, TYC 5799-1135-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "42 Capricorni",
	"OType" : "Variable of RS CVn type",
	"Distance" : "33.23",
	"RA_S" : 325.38691906,
	"DEC_S" : -14.04761146,
	"Constellation" : "Capricornus ",
	"AMag" : 5.233,
	"key" : 59313,
	"title" : "42 Capricorni"
	},
{
	"Index" : "48022",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "41 Capricorni, HIP 107128, SAO 190559, HD 206356, GC 30365, HR 8285, DM CD-23 17057, TYC 6940-1032-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "41 Capricorni",
	"OType" : "Star",
	"Distance" : "70.69",
	"RA_S" : 325.50290863,
	"DEC_S" : -23.26285875,
	"Constellation" : "Capricornus ",
	"AMag" : 5.349,
	"key" : 68022,
	"title" : "41 Capricorni"
	},
{
	"Index" : "43758",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "43 Capricorni, Kappa Capricorni, HIP 107188, SAO 164593, HD 206453, GC 30382, HR 8288, DM BD-19  6152, TYC 6370-1175-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Kappa Capricorni",
	"OType" : "Star",
	"Distance" : "90.1",
	"RA_S" : 325.66461527,
	"DEC_S" : -18.86632186,
	"Constellation" : "Capricornus ",
	"AMag" : 4.823,
	"key" : 63758,
	"title" : "Kappa Capricorni"
	},
{
	"Index" : "39248",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "46 Capricorni, c Capricorni, HIP 107382, SAO 145637, HD 206834, GC 30448, HR 8311, DM BD-09  5829, TYC 5788-1167-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "c Capricorni",
	"OType" : "Star",
	"Distance" : "241.08",
	"RA_S" : 326.25105618,
	"DEC_S" : -9.08243042,
	"Constellation" : "Capricornus ",
	"AMag" : 5.203,
	"key" : 59248,
	"title" : "c Capricorni"
	},
{
	"Index" : "43720",
	"Description" : "Delta Capricorni (\u03B4 Cap, \u03B4 Capricorni), also traditionally named Deneb Algedi and Scheddi, is a binary star system approximately 39 light-years away in the constellation of Capricornus (the Sea Goat). The primary star in the system is a white giant star and the combined light of its members makes it the brightest \u0022single\u0022 star within the constellation.\r\rBecause it is near the ecliptic, Delta Capricorni can be occulted by the Moon, and also (rarely) by planets. Delta Capricorni is an eclipsing binary star system similar to Algol, with an orbital period of 1.022768 days and an inclination close to the line of sight from the Earth. The peak apparent visual magnitude of the pair is 2.81. During an eclipse of the primary, this magnitude drops by 0.24. When the primary is eclipsing the secondary, the magnitude decreases by 0.09.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "49 Capricorni, Delta Capricorni, HIP 107556, SAO 164644, HD 207098, GC 30491, HR 8322, DM BD-16  5943, TYC 6363-1044-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Deneb Algedi / Scheddi",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "11.87",
	"RA_S" : 326.76018434,
	"DEC_S" : -16.12728709,
	"X" : 199,
	"Y" : 211,
	"Constellation" : "Capricornus ",
	"AMag" : 2.85,
	"key" : 63720,
	"shortTitle" : "Deneb Algiedi; Scheddi; Sheddi; Deneb Al'gedi",
	"title" : "Deneb Algedi / Scheddi"
	},
{
	"Index" : "39320",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "51 Capricorni, Mu Capricorni, HIP 108036, SAO 164713, HD 207958, GC 30631, HR 8351, DM BD-14  6149, TYC 5801-1017-1",
	"group" : { "key" : "Capricornus" },
	"Common" : "Mu Capricorni",
	"OType" : "High proper-motion Star",
	"Distance" : "26.61",
	"RA_S" : 328.32404834,
	"DEC_S" : -13.5517694,
	"Constellation" : "Capricornus ",
	"AMag" : 5.12,
	"key" : 59320,
	"title" : "Mu Capricorni"
	},
{
	"Index" : "62083",
	"Description" : "N Carinae (N Car) is a star in the constellation Carina. It is a white A-type bright giant with an apparent magnitude of +4.35 and is approximately 1760 light years from Earth.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "N Carinae, HIP 31407, SAO 234589, HD 47306, GC 8604, HR 2435, DM CP-52   953, TYC 8535-2126-1",
	"group" : { "backgroundImage" : "images/Alignment/13.png",
		"description" : "Carina (pron.: /k\u0259\u02C8ra\u026An\u0259/) is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was formerly part of the larger constellation of Argo Navis (the ship Argo) until that constellation was divided into three pieces, the other two being Puppis (the poop deck), and Vela (the sails of the ship).\r\rCarina was once a part of Argo Navis, the great ship of Jason and the Argonauts who searched for the Golden Fleece. The constellation of Argo was introduced in ancient Greece. However, Nicolas Louis de Lacaille divided the Argo into three component constellations in 1763, including Carina, the Keel.\r\rDespite the division, Lacaille kept Argo\u0027s Bayer designations. Therefore Carina has the \u03B1, \u03B2 and \u03B5, Vela has \u03B3 and \u03B4, Puppis has \u03B6, and so on.",
		"key" : "Carina",
		"grouptype" : "Carina",
		"Meaning" : "keel",
		"Family" : "Heavenly Waters",
		"Origin" : "1763, Lacaille, split from Argo Navis",
		"shortTitle" : "Carina",
		"title" : "Carina Objects Group" },
	"Common" : "N Carinae",
	"OType" : "Star",
	"Distance" : "416.93",
	"RA_S" : 98.74407995,
	"DEC_S" : -52.97560661,
	"X" : 609,
	"Y" : 227,
	"Constellation" : "Carina ",
	"AMag" : 4.363,
	"key" : 82083,
	"title" : "N Carinae"
	},
{
	"Index" : "62092",
	"Description" : "V415 Carinae (V415 Car or A Carinae) is an eclipsing spectroscopic binary of the Algol type in the constellation of Carina whose apparent visual magnitude varies by 0.06 magnitudes and is approximately 4.39 at maximum brightness. Its primary is a G-type bright giant star and its secondary is an A-type main sequence star. It is 2approximately 553 light years from Earth. A Carinae has two components in orbit around each other, making it a binary star. The semi-major axis of the secondary\u0027s orbit is 2.17 arcseconds. The two components regularly eclipse each other, making A Carinae a variable star. Its brightness varies by 0.06 magnitudes with a period equal to its orbital period of 195 days.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "A Carinae, HIP 32761, SAO 234737, HD 50337, GC 8972, HR 2554, DM CP-53  1168, TYC 8536-794-1",
	"group" : { "key" : "Carina" },
	"Common" : "V415 Carinae",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "166.76",
	"RA_S" : 102.46381353,
	"DEC_S" : -53.62244777,
	"X" : 579,
	"Y" : 222,
	"Constellation" : "Carina ",
	"AMag" : 4.51,
	"key" : 82092,
	"title" : "V415 Carinae"
	},
{
	"Index" : "58230",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "23 Carinae, HIP 33779, SAO 234854, HD 53047, GC 9273, HR 2652, DM CD-51  2224, TYC 8130-2235-1",
	"group" : { "key" : "Carina" },
	"Common" : "23 Carinae",
	"OType" : "Variable Star",
	"Distance" : "197.65",
	"RA_S" : 105.21453213,
	"DEC_S" : -51.4025886,
	"Constellation" : "Carina ",
	"AMag" : 5.35,
	"key" : 78230,
	"title" : "23 Carinae"
	},
{
	"Index" : "62156",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 34105, SAO 234902, HD 54118, GC 9368, HR 2683, DM CP-56 1232, TYC 8545-2238-1",
	"group" : { "key" : "Carina" },
	"Common" : "V* V386 Car",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "92.08",
	"RA_S" : 106.07636068,
	"DEC_S" : -56.74972316,
	"Constellation" : "Carina ",
	"AMag" : 5.135,
	"key" : 82156,
	"title" : "V* V386 Car"
	},
{
	"Index" : "58247",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 35589, SAO 235116, HD 57917, GC 9818, HR 2815, DM CD-51 2445, TYC 8132-2087-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 2815",
	"OType" : "Star",
	"Distance" : "147.14",
	"RA_S" : 110.16169862,
	"DEC_S" : -52.08592559,
	"Constellation" : "Carina ",
	"AMag" : 5.355,
	"key" : 78247,
	"title" : "HR 2815"
	},
{
	"Index" : "58248",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 36114, SAO 235192, HD 59219, GC 9964, HR 2862, DM CD-50 2761, TYC 8132-2109-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 2862",
	"OType" : "Star",
	"Distance" : "185.22",
	"RA_S" : 111.59104186,
	"DEC_S" : -51.01848056,
	"Constellation" : "Carina ",
	"AMag" : 5.196,
	"key" : 78248,
	"title" : "HR 2862"
	},
{
	"Index" : "62216",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Q Carinae, HIP 36942, SAO 235336, HD 61248, GC 10206, HR 2934, DM CP-52  1231, TYC 8552-1360-1",
	"group" : { "key" : "Carina" },
	"Common" : "Q Carinae",
	"OType" : "Variable Star",
	"Distance" : "120.26",
	"RA_S" : 113.91551609,
	"DEC_S" : -52.53383268,
	"Constellation" : "Carina ",
	"AMag" : 5.082,
	"key" : 82216,
	"title" : "Q Carinae"
	},
{
	"Index" : "62242",
	"Description" : "Chi Carinae (\u03C7 Car, \u03C7 Carinae) is a star in the southern constellation of Carina. It is a third-magnitude star and is one of the brighter members of the constellation. The distance to Chi Carinae can be determined directly through parallax measurements, yielding an estimate of roughly 450 light-years (140 parsecs) with a 6.7% margin of error. This star is a suspected astrometric binary, although nothing is known about the companion.\r\rThis is a massive star, with about seven times the mass of the Sun. It is about 40 million years old and rotating rapidly; the projected rotational velocity has been measured as high as 110 km s\u20131. The spectrum of this star matches a stellar classification of B3 IV, with the luminosity class of IV indicates this is likely a subgiant star that has nearly exhausted the supply of hydrogen at its core and is in the process of evolving into a giant star.\r\rIn 1969, Chi Carinae was classified as chemically peculiar Ap star because its absorption lines of silicon appeared unusually strong relative to the lines for helium. However, subsequent examination in the ultraviolet band showed the silicon bands were as expected and it was determined the spectra is normal for a star of its type. There is no indication of variability in the star\u0027s spectrum. Observation during the Hipparcos mission showed no photometric variability down to a limit of \u00B10.003 magnitudes. For this reason, the star has been ruled out as a Beta Cephei type variable star.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Chi Carinae, HIP 38827, SAO 235635, HD 65575, GC 10770, HR 3117, DM CP-52  1343, TYC 8553-2883-1",
	"group" : { "key" : "Carina" },
	"Common" : "Chi Carinae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "138.75",
	"RA_S" : 119.19464243,
	"DEC_S" : -52.98235073,
	"X" : 456,
	"Y" : 176,
	"Constellation" : "Carina ",
	"AMag" : 3.404,
	"key" : 82242,
	"title" : "Chi Carinae"
	},
{
	"Index" : "65885",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 39070, SAO 250063, HD 66342, GC 10873, HR 3153, DM CP-60 1018, TYC 8911-3387-1",
	"group" : { "key" : "Carina" },
	"Common" : "V* V460 Car",
	"OType" : "Long-period variable star",
	"Distance" : "382.96",
	"RA_S" : 119.90642674,
	"DEC_S" : -60.58706264,
	"Constellation" : "Carina ",
	"AMag" : 5.392,
	"key" : 85885,
	"title" : "V* V460 Car"
	},
{
	"Index" : "66040",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "D Carinae, HIP 39138, SAO 250069, HD 66591, GC 10893, HR 3159, DM CP-63   866, TYC 8928-3018-1",
	"group" : { "key" : "Carina" },
	"Common" : "D Carinae",
	"OType" : "Star",
	"Distance" : "153.07",
	"RA_S" : 120.08319492,
	"DEC_S" : -63.56745613,
	"Constellation" : "Carina ",
	"AMag" : 4.778,
	"key" : 86040,
	"title" : "D Carinae"
	},
{
	"Index" : "65996",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "B Carinae, HIP 39903, SAO 250131, HD 68456, GC 11115, HR 3220, DM CP-60  1074, TYC 8924-2780-1",
	"group" : { "key" : "Carina" },
	"Common" : "B Carinae",
	"OType" : "Blue Straggler Star",
	"Distance" : "19.91",
	"RA_S" : 122.25277417,
	"DEC_S" : -61.30240874,
	"Constellation" : "Carina ",
	"AMag" : 4.792,
	"key" : 85996,
	"title" : "B Carinae"
	},
{
	"Index" : "66037",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "C Carinae, HIP 40429A, SAO 250164, HD 69863A, GC 11275, HR 3260, DM CP-62   985, TYC 8928-2911-1",
	"group" : { "key" : "Carina" },
	"Common" : "C Carinae",
	"OType" : "Star",
	"Distance" : "77.45",
	"RA_S" : 123.81628389,
	"DEC_S" : -62.91561919,
	"Constellation" : "Carina ",
	"AMag" : 5.267,
	"key" : 86037,
	"title" : "C Carinae"
	},
{
	"Index" : "62526",
	"Description" : "Epsilon Carinae (\u03B5 Car, \u03B5 Carinae) is a star in the southern constellation of Carina. It is also known by the name Avior. At apparent magnitude +1.86 it is one of the brightest stars in the night sky, but is not visible from the northern hemisphere. Epsilon Carinae is a double star located roughly 560\u2013660 light-years (170\u2013200 parsecs) away from the Earth. Measurements during the Hipparcos mission give the pair an angular separation of 0.46 arcseconds with a difference in magnitude of 2.0. At their estimated distance, this angle is equivalent to a physical separation of around 4 Astronomical Units. This pair may form an eclipsing binary system with a period of 785 days (2.15 years), resulting in a magnitude change of 0.12 during each eclipse.\r\rThe primary component has an apparent visual magnitude of 2.2, which by itself would still make it the third brightest star in the constellation. It is an evolved giant star with a stellar classification of K0 III. However, examination of the ultraviolet flux from this star suggests it may instead be of spectral type K7. The fainter secondary companion has an apparent visual magnitude of 4.1, which, if it were a solitary star, would be bright enough to be seen with the naked eye. This is a hot, core hydrogen-fusing B-type main sequence star of spectral class B2 Vp. The secondary may itself have an orbiting stellar companion of spectral class F8:.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Epsilon Carinae, HIP 41037B, SAO 235932, HD 71129, GC 11463, HR 3307, DM CP-59  1032A, TYC 8579-2692-2",
	"group" : { "key" : "Carina" },
	"Common" : "Avior",
	"OType" : "Double or multiple star",
	"Distance" : "184.19",
	"RA_S" : 125.62848024,
	"DEC_S" : -59.50948419,
	"X" : 401,
	"Y" : 255,
	"Constellation" : "Carina ",
	"AMag" : 1.86,
	"key" : 82526,
	"title" : "Avior"
	},
{
	"Index" : "62532",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "e01 Carinae, HIP 42129AB, SAO 236105, HD 73390, GC 11796, HR 3415, DM CP-57  1590, TYC 8580-3313-1",
	"group" : { "key" : "Carina" },
	"Common" : "e01 Carinae",
	"OType" : "Star",
	"Distance" : "272.65",
	"RA_S" : 128.81481519,
	"DEC_S" : -58.22473476,
	"Constellation" : "Carina ",
	"AMag" : 5.212,
	"key" : 82532,
	"title" : "e01 Carinae"
	},
{
	"Index" : "62491",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "e02 Carinae, HIP 42134AB, SAO 236106, HD 73389, GC 11797, HR 3414, DM CP-57  1591, TYC 8576-2426-1",
	"group" : { "key" : "Carina" },
	"Common" : "e02 Carinae",
	"OType" : "Star",
	"Distance" : "68.04",
	"RA_S" : 128.83211608,
	"DEC_S" : -58.00923266,
	"Constellation" : "Carina ",
	"AMag" : 4.957,
	"key" : 82491,
	"title" : "e02 Carinae"
	},
{
	"Index" : "62544",
	"Description" : "V343 Carinae (d Car / d Carinae) is a binary star in the constellation Carina. It is approximately 1410 light years from Earth.\r\rV343 Carinae is a blue-white B-type giant with a mean apparent magnitude of +4.31. It is classified as a Beta Cephei type variable star and its brightness varies from magnitude +4.30 to +4.33. It is a spectroscopic binary with an orbital period of 134 days.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "d Carinae, HIP 42568, SAO 236181, HD 74375, GC 11964, HR 3457, DM CP-59  1080, TYC 8581-3010-1",
	"group" : { "key" : "Carina" },
	"Common" : "V343 Carinae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "441.22",
	"RA_S" : 130.15427627,
	"DEC_S" : -59.76100058,
	"X" : 371,
	"Y" : 257,
	"Constellation" : "Carina ",
	"AMag" : 4.292,
	"key" : 82544,
	"title" : "V343 Carinae"
	},
{
	"Index" : "62506",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "f Carinae, HIP 43105, SAO 236268, HD 75311, GC 12138, HR 3498, DM CP-56  1865, TYC 8577-3017-1",
	"group" : { "key" : "Carina" },
	"Common" : "f Carinae",
	"OType" : "Be Star",
	"Distance" : "185.38",
	"RA_S" : 131.67728788,
	"DEC_S" : -56.76978077,
	"Constellation" : "Carina ",
	"AMag" : 4.454,
	"key" : 82506,
	"title" : "f Carinae"
	},
{
	"Index" : "66029",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "c Carinae, HIP 43783, SAO 250374, HD 76728, GC 12359, HR 3571, DM CP-60  1243, TYC 8927-3658-1",
	"group" : { "key" : "Carina" },
	"Common" : "c Carinae",
	"OType" : "Star",
	"Distance" : "98.03",
	"RA_S" : 133.76180187,
	"DEC_S" : -60.64461452,
	"Constellation" : "Carina ",
	"AMag" : 3.802,
	"key" : 86029,
	"title" : "c Carinae"
	},
{
	"Index" : "62760",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "b01 Carinae, HIP 43937, SAO 236436, HD 77002, GC 12405, HR 3582, DM CP-58  1301, TYC 8594-3179-1",
	"group" : { "key" : "Carina" },
	"Common" : "b01 Carinae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "206.15",
	"RA_S" : 134.24340311,
	"DEC_S" : -59.22933668,
	"Constellation" : "Carina ",
	"AMag" : 4.866,
	"key" : 82760,
	"title" : "b01 Carinae"
	},
{
	"Index" : "62758",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "b02 Carinae, HIP 44143, SAO 236475, HD 77370, GC 12449, HR 3598, DM CP-58  1327, TYC 8594-3177-1",
	"group" : { "key" : "Carina" },
	"Common" : "b02 Carinae",
	"OType" : "High proper-motion Star",
	"Distance" : "26.42",
	"RA_S" : 134.85075636,
	"DEC_S" : -59.08371314,
	"Constellation" : "Carina ",
	"AMag" : 5.212,
	"key" : 82758,
	"title" : "b02 Carinae"
	},
{
	"Index" : "68931",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "G Carinae, HIP 44599, SAO 256582, HD 78791, GC 12595, HR 3643, DM CP-72   779, TYC 9203-2759-1",
	"group" : { "key" : "Carina" },
	"Common" : "G Carinae",
	"OType" : "Spectroscopic binary",
	"Distance" : "122.8",
	"RA_S" : 136.28671152,
	"DEC_S" : -72.60270412,
	"Constellation" : "Carina ",
	"AMag" : 4.536,
	"key" : 88931,
	"title" : "G Carinae"
	},
{
	"Index" : "68898",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "E Carinae, HIP 44626, SAO 256583, HD 78764, GC 12602, HR 3642, DM CP-70   861, TYC 9199-2885-1",
	"group" : { "key" : "Carina" },
	"Common" : "E Carinae",
	"OType" : "Be Star",
	"Distance" : "292.28",
	"RA_S" : 136.40989945,
	"DEC_S" : -70.53850019,
	"Constellation" : "Carina ",
	"AMag" : 4.627,
	"key" : 88898,
	"title" : "E Carinae"
	},
{
	"Index" : "62771",
	"Description" : "V357 Carinae (a Car, a Carinae) is a spectroscopic binary in the constellation Carina. It is approximately 419 light years from Earth. The mean apparent magnitude of the system is +3.43.\r\rV357 Carinae is composed of two similar blue-white B-type subgiants. This star has five times the radius of the Sun. It is an eclipsing binary. Due to the eclipses, it is a variable star and its brightness varies from magnitude +3.41 to +3.44 with a period of 6.75 days, which is its orbital period.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "a Carinae, HIP 45080, SAO 236693, HD 79351, GC 12696, HR 3659, DM CP-58  1419, TYC 8595-3311-1",
	"group" : { "key" : "Carina" },
	"Common" : "V357 Carinae",
	"OType" : "Spectroscopic binary",
	"Distance" : "136.61",
	"RA_S" : 137.74204034,
	"DEC_S" : -58.96689247,
	"X" : 320,
	"Y" : 250,
	"Constellation" : "Carina ",
	"AMag" : 3.381,
	"key" : 82771,
	"title" : "V357 Carinae"
	},
{
	"Index" : "66213",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "i Carinae, HIP 45101, SAO 250471, HD 79447, GC 12707, HR 3663, DM CP-61  1201, TYC 8944-3281-1",
	"group" : { "key" : "Carina" },
	"Common" : "i Carinae",
	"OType" : "Star",
	"Distance" : "166.31",
	"RA_S" : 137.81966453,
	"DEC_S" : -62.3169797,
	"Constellation" : "Carina ",
	"AMag" : 3.915,
	"key" : 86213,
	"title" : "i Carinae"
	},
{
	"Index" : "62702",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "g Carinae, HIP 45496, SAO 236787, HD 80230, GC 12813, HR 3696, DM CP-57  1961, TYC 8591-1279-1",
	"group" : { "key" : "Carina" },
	"Common" : "g Carinae",
	"OType" : "Variable Star",
	"Distance" : "149.61",
	"RA_S" : 139.05030064,
	"DEC_S" : -57.54147386,
	"Constellation" : "Carina ",
	"AMag" : 4.518,
	"key" : 82702,
	"title" : "g Carinae"
	},
{
	"Index" : "68867",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 45571AB, SAO 250526, HD 80671, GC 12848, HR 3712, DM CP-68  918, TYC 9196-198-1",
	"group" : { "key" : "Carina" },
	"Common" : "* 128 Car",
	"OType" : "Double or multiple star",
	"Distance" : "33.51",
	"RA_S" : 139.32181901,
	"DEC_S" : -68.68964556,
	"Constellation" : "Carina ",
	"AMag" : 5.437,
	"key" : 88867,
	"title" : "* 128 Car"
	},
{
	"Index" : "68974",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 45581AB, TYC 9208-2718-1",
	"group" : { "key" : "Carina" },
	"Common" : "NAME HD 80951AB",
	"OType" : "Star",
	"Distance" : "216.04",
	"RA_S" : 139.35490066,
	"DEC_S" : -74.89432591,
	"Constellation" : "Carina ",
	"AMag" : 5.322,
	"key" : 88974,
	"title" : "NAME HD 80951AB"
	},
{
	"Index" : "66214",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "k Carinae, HIP 45856, SAO 250544, HD 81101, GC 12923, HR 3728, DM CP-61  1242, TYC 8944-3282-1",
	"group" : { "key" : "Carina" },
	"Common" : "k Carinae",
	"OType" : "Star",
	"Distance" : "71.62",
	"RA_S" : 140.23671784,
	"DEC_S" : -62.4046329,
	"Constellation" : "Carina ",
	"AMag" : 4.903,
	"key" : 86214,
	"title" : "k Carinae"
	},
{
	"Index" : "62802",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "h Carinae, HIP 46974, SAO 237117, HD 83183, GC 13246, HR 3825, DM CP-58  1576, TYC 8597-2340-1",
	"group" : { "key" : "Carina" },
	"Common" : "h Carinae",
	"OType" : "Star",
	"Distance" : "405.7",
	"RA_S" : 143.61104296,
	"DEC_S" : -59.22975471,
	"Constellation" : "Carina ",
	"AMag" : 4.078,
	"key" : 82802,
	"title" : "h Carinae"
	},
{
	"Index" : "66156",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "m Carinae, HIP 47391, SAO 250653, HD 83944, GC 13355, HR 3856, DM CP-60  1477, TYC 8941-2077-1",
	"group" : { "key" : "Carina" },
	"Common" : "m Carinae",
	"OType" : "Variable Star",
	"Distance" : "69.2",
	"RA_S" : 144.8374828,
	"DEC_S" : -61.32806004,
	"Constellation" : "Carina ",
	"AMag" : 4.487,
	"key" : 86156,
	"title" : "m Carinae"
	},
{
	"Index" : "62738",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 47479AB, SAO 237221, HD 84121, GC 13376, HR 3863, DM CP-57 2228, TYC 8593-1420-1",
	"group" : { "key" : "Carina" },
	"Common" : "Gliese 9305",
	"OType" : "Double or multiple star",
	"Distance" : "72.49",
	"RA_S" : 145.17736951,
	"DEC_S" : -57.98355239,
	"Constellation" : "Carina ",
	"AMag" : 5.332,
	"key" : 82738,
	"title" : "Gliese 9305"
	},
{
	"Index" : "66239",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "l Carinae, HIP 47854, SAO 250683, HD 84810, GC 13462, HR 3884, DM CP-61  1333, TYC 8946-3219-1",
	"group" : { "key" : "Carina" },
	"Common" : "l Carinae",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "467.66",
	"RA_S" : 146.31172215,
	"DEC_S" : -62.50790124,
	"Constellation" : "Carina ",
	"AMag" : 3.905,
	"key" : 86239,
	"title" : "l Carinae"
	},
{
	"Index" : "66286",
	"Description" : "Upsilon Carinae (\u03C5 Car, \u03C5 Carinae) is a double star in the southern constellation of Carina. It is part of the Diamond Cross asterism in southern Carina. The Upsilon Carinae system has a combined apparent magnitude of +2.97 and is approximately 1,400 light years (440 parsecs) from Earth.\r\rIn Chinese, \u6D77\u77F3 (H\u01CEi D\u00E0n), meaning Sea Rock, refers to an asterism consisting of \u03C5 Carinae, \u03B5 Carinae, \u03B9 Carinae, HD 83183 and HD 84810. Consequently, \u03C5 Carinae itself is known as \u6D77\u77F3\u4E94 (H\u01CEi D\u00E0n w\u01D4, English: the Fifth Star of Sea Rock.)\r\rThe primary component, \u03C5 Carinae A, has a stellar classification of A8 Ib, making it a supergiant star that has exhausted the hydrogen at its core and evolved away from its brief main sequence lifetime as a O9 V star. With an apparent magnitude of +3.08, it has an effective temperature of about 7,600 K, giving it a white hue. The companion, \u03C5 Carinae B, is a giant star with a classification of B7 III, although Mandrini and Niemela (1986) suggested it may be a subgiant star with a classification of B4\u20135 IV. The outer envelope of this star has an effective temperature of around 23,000 K, resulting in the blue-white hue of a B-type star.\r\rThe two stars have an angular separation of 5.030 arcseconds. As a binary star system, they would have an estimated orbital period of at least 19,500 years and a present day separation of around 2,000 Astronomical Units. This system is roughly 12 million years old.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Upsilon Carinae, HIP 48002B, SAO 250695, HD 85123J, GC 13506, HR 3890, DM CP-64  1084A, TYC 8950-2272-2",
	"group" : { "key" : "Carina" },
	"Common" : "Upsilon Carinae",
	"OType" : "Double or multiple star",
	"Distance" : "432.63",
	"RA_S" : 146.77550706,
	"DEC_S" : -65.07200742,
	"X" : 281,
	"Y" : 338,
	"Constellation" : "Carina ",
	"AMag" : 2.92,
	"key" : 86286,
	"title" : "Upsilon Carinae"
	},
{
	"Index" : "66285",
	"Description" : "Upsilon Carinae (\u03C5 Car, \u03C5 Carinae) is a double star in the southern constellation of Carina. It is part of the Diamond Cross asterism in southern Carina. The Upsilon Carinae system has a combined apparent magnitude of +2.97 and is approximately 1,400 light years (440 parsecs) from Earth.\r\rIn Chinese, \u6D77\u77F3 (H\u01CEi D\u00E0n), meaning Sea Rock, refers to an asterism consisting of \u03C5 Carinae, \u03B5 Carinae, \u03B9 Carinae, HD 83183 and HD 84810. Consequently, \u03C5 Carinae itself is known as \u6D77\u77F3\u4E94 (H\u01CEi D\u00E0n w\u01D4, English: the Fifth Star of Sea Rock.)\r\rThe primary component, \u03C5 Carinae A, has a stellar classification of A8 Ib, making it a supergiant star that has exhausted the hydrogen at its core and evolved away from its brief main sequence lifetime as a O9 V star. With an apparent magnitude of +3.08, it has an effective temperature of about 7,600 K, giving it a white hue. The companion, \u03C5 Carinae B, is a giant star with a classification of B7 III, although Mandrini and Niemela (1986) suggested it may be a subgiant star with a classification of B4\u20135 IV. The outer envelope of this star has an effective temperature of around 23,000 K, resulting in the blue-white hue of a B-type star.\r\rThe two stars have an angular separation of 5.030 arcseconds. As a binary star system, they would have an estimated orbital period of at least 19,500 years and a present day separation of around 2,000 Astronomical Units. This system is roughly 12 million years old.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Upsilon Carinae, HIP 48002A, TYC 8950-2272-1",
	"group" : { "key" : "Carina" },
	"Common" : "Upsilon Carinae",
	"OType" : "Double or multiple star",
	"Distance" : "432.63",
	"RA_S" : 146.77551194,
	"DEC_S" : -65.07200514,
	"X" : 281,
	"Y" : 338,
	"Constellation" : "Carina ",
	"AMag" : 3.025,
	"key" : 86285,
	"title" : "Upsilon Carinae"
	},
{
	"Index" : "66339",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 49698, SAO 250836, HD 88323, GC 13960, HR 3995, DM CP-65 1248, TYC 8955-1325-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 3995",
	"OType" : "Star",
	"Distance" : "112.97",
	"RA_S" : 152.17811681,
	"DEC_S" : -65.81543305,
	"Constellation" : "Carina ",
	"AMag" : 5.364,
	"key" : 86339,
	"title" : "HR 3995"
	},
{
	"Index" : "66340",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "M Carinae, HIP 50083, SAO 250880, HD 88981, GC 14066, HR 4025, DM CP-65  1273, TYC 8955-1326-1",
	"group" : { "key" : "Carina" },
	"Common" : "M Carinae",
	"OType" : "Star",
	"Distance" : "94.31",
	"RA_S" : 153.37763701,
	"DEC_S" : -66.37281028,
	"Constellation" : "Carina ",
	"AMag" : 5.17,
	"key" : 86340,
	"title" : "M Carinae"
	},
{
	"Index" : "69057",
	"Description" : "Omega Carinae (\u03C9 Car, \u03C9 Carinae) is a star in the constellation Carina. With a declination greater than 70 degrees south of the celestial equator, it is the most southerly of the bright stars of Carina (third-magnitude or brighter), and it is part of a southern asterism known as the Diamond Cross. This star has an apparent visual magnitude of 3.3 and is located at a distance of about 342 light-years (105 parsecs) from Earth.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Omega Carinae, HIP 50099, SAO 250885, HD 89080, GC 14074, HR 4037, DM CP-69  1178, TYC 9214-2842-1",
	"group" : { "key" : "Carina" },
	"Common" : "Omega Carinae",
	"OType" : "Be Star",
	"Distance" : "104.81",
	"RA_S" : 153.43423521,
	"DEC_S" : -70.03789684,
	"X" : 270,
	"Y" : 410,
	"Constellation" : "Carina ",
	"AMag" : 3.271,
	"key" : 89057,
	"title" : "Omega Carinae"
	},
{
	"Index" : "66199",
	"Description" : "V337 Carinae (V337 Car, q Carinae) is a K-type bright giant star in the constellation of Carina. It is an irregular variable and has an apparent visual magnitude which varies between 3.36 and 3.44.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "q Carinae, HIP 50371, SAO 250905, HD 89388, GC 14133, HR 4050, DM CP-60  1817, TYC 8943-3447-1",
	"group" : { "key" : "Carina" },
	"Common" : "V337 Carinae",
	"OType" : "Long-period variable star",
	"Distance" : "201.53",
	"RA_S" : 154.27073517,
	"DEC_S" : -61.3323077,
	"X" : 224,
	"Y" : 306,
	"Constellation" : "Carina ",
	"AMag" : 3.536,
	"key" : 86199,
	"title" : "V337 Carinae"
	},
{
	"Index" : "66572",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "L Carinae, HIP 50847, SAO 250940, HD 90264, GC 14283, HR 4089, DM CP-66  1243, TYC 8968-1393-1",
	"group" : { "key" : "Carina" },
	"Common" : "L Carinae",
	"OType" : "Star",
	"Distance" : "123.08",
	"RA_S" : 155.74227801,
	"DEC_S" : -66.90149527,
	"Constellation" : "Carina ",
	"AMag" : 4.938,
	"key" : 86572,
	"title" : "L Carinae"
	},
{
	"Index" : "69140",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "I Carinae, HIP 50954, SAO 256710, HD 90589, GC 14323, HR 4102, DM CP-73   733, TYC 9223-2880-1",
	"group" : { "key" : "Carina" },
	"Common" : "I Carinae",
	"OType" : "Variable Star",
	"Distance" : "16.22",
	"RA_S" : 156.0987793,
	"DEC_S" : -74.03161376,
	"Constellation" : "Carina ",
	"AMag" : 4.02,
	"key" : 89140,
	"title" : "I Carinae"
	},
{
	"Index" : "62990",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "P Carinae, HIP 51192, SAO 238077, HD 90772, GC 14373, HR 4110, DM CP-57  3256, TYC 8609-3069-1",
	"group" : { "key" : "Carina" },
	"Common" : "P Carinae",
	"OType" : "Cepheid variable Star",
	"Distance" : "2483.88",
	"RA_S" : 156.85195718,
	"DEC_S" : -57.63880666,
	"Constellation" : "Carina ",
	"AMag" : 4.736,
	"key" : 82990,
	"title" : "P Carinae"
	},
{
	"Index" : "63076",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "s Carinae, HIP 51232, SAO 238085, HD 90853, GC 14388, HR 4114, DM CP-58  2227, TYC 8613-3363-1",
	"group" : { "key" : "Carina" },
	"Common" : "s Carinae",
	"OType" : "Variable Star",
	"Distance" : "445.78",
	"RA_S" : 156.96971516,
	"DEC_S" : -58.73940351,
	"Constellation" : "Carina ",
	"AMag" : 3.848,
	"key" : 83076,
	"title" : "s Carinae"
	},
{
	"Index" : "69110",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "K Carinae, HIP 51438, SAO 256722, HD 91375, GC 14457, HR 4138, DM CP-71  1034, TYC 9219-3722-1",
	"group" : { "key" : "Carina" },
	"Common" : "K Carinae",
	"OType" : "Star",
	"Distance" : "79.85",
	"RA_S" : 157.5838721,
	"DEC_S" : -71.99279102,
	"Constellation" : "Carina ",
	"AMag" : 4.715,
	"key" : 89110,
	"title" : "K Carinae"
	},
{
	"Index" : "69138",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 51495, SAO 256723, HD 91496, GC 14480, HR 4142, DM CP-72  981, TYC 9223-255-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4142",
	"OType" : "Variable Star",
	"Distance" : "315.23",
	"RA_S" : 157.75857706,
	"DEC_S" : -73.2214912,
	"Constellation" : "Carina ",
	"AMag" : 5.128,
	"key" : 89138,
	"title" : "HR 4142"
	},
{
	"Index" : "66368",
	"Description" : "PP Carinae is the variable star designation for a star in the southern constellation of Carina. It has the Bayer designation p Carinae (p Car) and, at an apparent visual magnitude of +3.30, is readily visible to the naked eye from the southern hemisphere. From the observed parallax shift of this star as the Earth orbits the Sun, its distance can be estimated as roughly 480 light-years (150 parsecs) with a 6% margin of error.\r\rPP Carinae is a B-type main sequence star with a stellar classification of B4 Vne. The \u0027ne\u0027 suffix indicates it is a rapidly rotating Be star that is surrounded by hot circumstellar gas. This material adds emission lines to the spectrum of the star. It has a projected rotational velocity of 325 km s\u20131, with about 7.6 times the mass and 6 times the radius of the Sun. This star is classified as a Gamma Cassiopeiae type variable and its brightness varies from magnitude +3.27 to +3.37.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "p Carinae, HIP 51576, SAO 251006, HD 91465, GC 14489, HR 4140, DM CP-61  1704, TYC 8956-4324-1",
	"group" : { "key" : "Carina" },
	"Common" : "PP Carinae",
	"OType" : "Be Star",
	"Distance" : "148.54",
	"RA_S" : 158.00609569,
	"DEC_S" : -61.68533231,
	"X" : 204,
	"Y" : 319,
	"Constellation" : "Carina ",
	"AMag" : 3.341,
	"key" : 86368,
	"title" : "PP Carinae"
	},
{
	"Index" : "62986",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "r Carinae, HIP 51849, SAO 238222, HD 91942, GC 14570, HR 4159, DM CP-56  3544, TYC 8609-2378-1",
	"group" : { "key" : "Carina" },
	"Common" : "r Carinae",
	"OType" : "Variable Star",
	"Distance" : "440.66",
	"RA_S" : 158.89708031,
	"DEC_S" : -57.55763043,
	"Constellation" : "Carina ",
	"AMag" : 4.628,
	"key" : 82986,
	"title" : "r Carinae"
	},
{
	"Index" : "63079",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "t01 Carinae, HIP 51912, SAO 238242, HD 92063, GC 14594, HR 4164, DM CP-58  2371, TYC 8613-3366-1",
	"group" : { "key" : "Carina" },
	"Common" : "t01 Carinae",
	"OType" : "Variable Star",
	"Distance" : "80.47",
	"RA_S" : 159.08549367,
	"DEC_S" : -59.56439388,
	"Constellation" : "Carina ",
	"AMag" : 5.217,
	"key" : 83079,
	"title" : "t01 Carinae"
	},
{
	"Index" : "63078",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "t02 Carinae, HIP 52102A, SAO 238295, HD 92397, GC 14647, HR 4177, DM CP-58  2460A, TYC 8613-3365-1",
	"group" : { "key" : "Carina" },
	"Common" : "t02 Carinae",
	"OType" : "Star",
	"Distance" : "467.46",
	"RA_S" : 159.68748047,
	"DEC_S" : -59.18299597,
	"Constellation" : "Carina ",
	"AMag" : 4.894,
	"key" : 83078,
	"title" : "t02 Carinae"
	},
{
	"Index" : "66535",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52221, SAO 251059, HD 92664, GC 14685, HR 4185, DM CP-64 1403, TYC 8965-542-1",
	"group" : { "key" : "Carina" },
	"Common" : "V* V364 Car",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "151.05",
	"RA_S" : 160.0476702,
	"DEC_S" : -65.10020917,
	"Constellation" : "Carina ",
	"AMag" : 5.474,
	"key" : 86535,
	"title" : "V* V364 Car"
	},
{
	"Index" : "66521",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52370, SAO 251078, HD 92938, GC 14733, HR 4196, DM CP-63 1589, TYC 8965-1766-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4196",
	"OType" : "Be Star",
	"Distance" : "146.82",
	"RA_S" : 160.55883095,
	"DEC_S" : -64.46642672,
	"Constellation" : "Carina ",
	"AMag" : 4.714,
	"key" : 86521,
	"title" : "HR 4196"
	},
{
	"Index" : "63274",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52405, SAO 238379, HD 92964, GC 14743, HR 4198, DM CP-58 2581, TYC 8626-2804-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4198",
	"OType" : "Blue supergiant star",
	"Distance" : "2492.27",
	"RA_S" : 160.66902081,
	"DEC_S" : -59.21576017,
	"Constellation" : "Carina ",
	"AMag" : 5.416,
	"key" : 83274,
	"title" : "HR 4198"
	},
{
	"Index" : "66520",
	"Description" : "Theta Carinae (\u03B8 Car, \u03B8 Carinae) is a star in the southern constellation of Carina. With an apparent visual magnitude of 2.76, it is the brightest star in the open star cluster IC 2602. It marks the northeastern end of the Diamond Cross asterism. Parallax measurements from the Hipparcos mission place this star at a distance of about 460 light-years (140 parsecs) from Earth.\r\rIn Chinese, \u5357\u8239 (N\u00E1n Chu\u00E1n), meaning Southern Boat, refers to an asterism consisting of \u03B8 Carinae, V337 Carinae, PP Carinae, \u03B2 Carinae and \u03C9 Carinae. Consequently, \u03B8 Carinae itself is known as \u5357\u8239\u4E09 (N\u00E1n Chu\u00E1n s\u0101n, English: the Third Star of Southern Boat.)\r\rThe stellar classification of this star is B0.5 Vp, which indicates this is a B-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. The \u0027p\u0027 suffix means it displays peculiar features in its spectrum, which have been observed in both the optical and ultraviolet band. This might be explained by a magnetic field, yet no such measurable field has been observed. Theta Carinae is actually a single-lined spectroscopic binary with a period of 2.2 days; the shortest known orbital period among massive stars. The close orbit means that a mass transfer between the two components may have occurred, which could explain the peculiarities of the spectrum.\r\rThe primary component in this system is a blue straggler, which is a type of star that is created by the interaction between two or more stars. Most likely the source of this mass transfer was the secondary member of the system, and what is now the primary star was probably once the secondary component. At an estimated age of 4 million years, this star is much younger than the age of the surrounding IC 2602 cluster, which is consistent with it being a straggler. At present the primary star has about 15 times the mass of the Sun and five times the Sun\u0027s radius. It has an intensely hot outer envelope that is radiating more than 25,000 the Sun\u0027s luminosity at an effective temperature of 31,000 K, giving it a blue-white glow. When the primary reaches the age of around 11 million years, it will expand to the point where it will begin to transfer part of its mass back to its companion. Little is known about this secondary component, but it may be an F-type star with a luminosity less than 1% of the primary.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Theta Carinae, HIP 52419, SAO 251083, HD 93030, GC 14755, HR 4199, DM CP-63  1599, TYC 8965-1765-1",
	"group" : { "key" : "Carina" },
	"Common" : "Theta Carinae",
	"OType" : "Spectroscopic binary",
	"Distance" : "146.93",
	"RA_S" : 160.73917486,
	"DEC_S" : -64.39445022,
	"X" : 206,
	"Y" : 358,
	"Constellation" : "Carina ",
	"AMag" : 2.67,
	"key" : 86520,
	"title" : "Theta Carinae"
	},
{
	"Index" : "66399",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "w Carinae, HIP 52468, SAO 251090, HD 93070, GC 14762, HR 4200, DM CP-59  2532, TYC 8957-4262-1",
	"group" : { "key" : "Carina" },
	"Common" : "w Carinae",
	"OType" : "Long Period Variable candidate",
	"Distance" : "439.53",
	"RA_S" : 160.88455459,
	"DEC_S" : -60.56661767,
	"Constellation" : "Carina ",
	"AMag" : 4.754,
	"key" : 86399,
	"title" : "w Carinae"
	},
{
	"Index" : "66517",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52502, SAO 251096, HD 93194, GC 14778, HR 4205, DM CP-63 1623, TYC 8965-1762-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4205",
	"OType" : "Star in Cluster",
	"Distance" : "149.15",
	"RA_S" : 161.02881454,
	"DEC_S" : -63.9610704,
	"Constellation" : "Carina ",
	"AMag" : 4.767,
	"key" : 86517,
	"title" : "HR 4205"
	},
{
	"Index" : "66522",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52678, SAO 251115, HD 93540, GC 14837, HR 4219, DM CP-63 1646, TYC 8965-1767-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4219",
	"OType" : "Star in Cluster",
	"Distance" : "148.18",
	"RA_S" : 161.56897154,
	"DEC_S" : -64.5145634,
	"Constellation" : "Carina ",
	"AMag" : 5.303,
	"key" : 86522,
	"title" : "HR 4219"
	},
{
	"Index" : "66518",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52701, SAO 251117, HD 93549, GC 14844, HR 4220, DM CP-63 1649, TYC 8965-1763-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4220",
	"OType" : "Spectroscopic binary",
	"Distance" : "148.15",
	"RA_S" : 161.62328556,
	"DEC_S" : -64.26324036,
	"Constellation" : "Carina ",
	"AMag" : 5.214,
	"key" : 86518,
	"title" : "HR 4220"
	},
{
	"Index" : "66519",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 52736, SAO 251120, HD 93607, GC 14850, HR 4222, DM CP-63 1655, TYC 8965-1764-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4222",
	"OType" : "Star in Cluster",
	"Distance" : "148.45",
	"RA_S" : 161.71341662,
	"DEC_S" : -64.38347342,
	"Constellation" : "Carina ",
	"AMag" : 4.814,
	"key" : 86519,
	"title" : "HR 4222"
	},
{
	"Index" : "63193",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 53154, SAO 238557, HD 94367, GC 14960, HR 4250, DM CP-56 3947, TYC 8622-3780-1",
	"group" : { "key" : "Carina" },
	"Common" : "V* V524 Car",
	"OType" : "Pulsating variable Star",
	"RA_S" : 163.12852499,
	"DEC_S" : -57.24040283,
	"Constellation" : "Carina ",
	"AMag" : 5.284,
	"key" : 83193,
	"title" : "V* V524 Car"
	},
{
	"Index" : "63322",
	"Description" : "HD 94510 (u Car, u Carinae) is a star in the constellation Carina. It is an orange K-type giant with an apparent magnitude of +3.79 and is approximately 96.8 light years from Earth. It has about 22.3 times the sun\u0027s luminosity.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "u Carinae, HIP 53253, SAO 238574, HD 94510, GC 14980, HR 4257, DM CP-58  2834, TYC 8627-3091-1",
	"group" : { "key" : "Carina" },
	"Common" : "u Carinae",
	"OType" : "Variable Star",
	"Distance" : "29.13",
	"RA_S" : 163.37356391,
	"DEC_S" : -58.85317313,
	"X" : 157,
	"Y" : 302,
	"Constellation" : "Carina ",
	"AMag" : 3.882,
	"key" : 83322,
	"title" : "u Carinae"
	},
{
	"Index" : "66486",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "z Carinae, HIP 54301, SAO 251269, HD 96566, GC 15288, HR 4325, DM CP-61  2067, TYC 8962-2641-1",
	"group" : { "key" : "Carina" },
	"Common" : "z Carinae",
	"OType" : "Star",
	"Distance" : "122.04",
	"RA_S" : 166.63511877,
	"DEC_S" : -62.42411235,
	"Constellation" : "Carina ",
	"AMag" : 4.719,
	"key" : 86486,
	"title" : "z Carinae"
	},
{
	"Index" : "66485",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "z02 Carinae, HIP 54461, SAO 251286, HD 96919, GC 15331, HR 4338, DM CP-61  2075, TYC 8962-2640-1",
	"group" : { "key" : "Carina" },
	"Common" : "z02 Carinae",
	"OType" : "Pulsating variable Star",
	"RA_S" : 167.14165893,
	"DEC_S" : -61.9471782,
	"Constellation" : "Carina ",
	"AMag" : 5.163,
	"key" : 86485,
	"title" : "z02 Carinae"
	},
{
	"Index" : "63356",
	"Description" : "V382 Carinae, also known as x Carinae (x Car), is a star in the constellation Carina.\r\rV382 Carinae is a yellow G-type hypergiant with a mean apparent magnitude of +3.93. It is 8,900 light years from Earth. It is a variable star of low amplitude, and is 700 times the size of our Sun.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "x Carinae, HIP 54463, SAO 238813, HD 96918, GC 15329, HR 4337, DM CP-58  3189, TYC 8628-2484-1",
	"group" : { "key" : "Carina" },
	"Common" : "x Carinae",
	"OType" : "Classical Cepheid (delta Cep type)",
	"RA_S" : 167.14745997,
	"DEC_S" : -58.97503773,
	"X" : 136,
	"Y" : 317,
	"Constellation" : "Carina ",
	"AMag" : 4.052,
	"key" : 83356,
	"title" : "x Carinae"
	},
{
	"Index" : "66451",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "y Carinae, HIP 54751, SAO 251316, HD 97534, GC 15415, HR 4352, DM CP-59  3190, TYC 8959-2615-1",
	"group" : { "key" : "Carina" },
	"Common" : "y Carinae",
	"OType" : "Pulsating variable Star",
	"RA_S" : 168.15005741,
	"DEC_S" : -60.31762926,
	"Constellation" : "Carina ",
	"AMag" : 4.679,
	"key" : 86451,
	"title" : "y Carinae"
	},
{
	"Index" : "66556",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 54767, SAO 251320, HD 97583, GC 15421, HR 4355, DM CP-63 1860, TYC 8967-1169-1",
	"group" : { "key" : "Carina" },
	"Common" : "HR 4355",
	"OType" : "Star",
	"Distance" : "95.84",
	"RA_S" : 168.18836055,
	"DEC_S" : -64.16976994,
	"Constellation" : "Carina ",
	"AMag" : 5.206,
	"key" : 86556,
	"title" : "HR 4355"
	},
{
	"Index" : "25685",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "12 Cassiopeiae, HIP 1960, SAO 11172, HD 2011, GC 481, HR 93, DM BD+61    69, TYC 4015-3523-1",
	"group" : { "backgroundImage" : "images/Alignment/14.png",
		"description" : "Cassiopeia is a constellation in the northern sky, named after the vain queen Cassiopeia in Greek mythology, who boasted about her unrivalled beauty. Cassiopeia was one of the 48 constellations listed by the 2nd century Greek astronomer Ptolemy, and it remains one of the 88 modern constellations today. It is easily recognizable due to its distinctive \u0027W\u0027 shape, formed by five bright stars. It is bordered by Andromeda to the south, Perseus to the southeast, and Cepheus to the north. She is opposite the Big Dipper, and from northern latitudes can be seen at her clearest in early November.\r\rThe constellation is named after Cassiopeia, the queen of Aethiopia. Cassiopeia was the wife of Cepheus, King of Aethiopia and mother of Princess Andromeda. Cepheus and Cassiopeia were placed next to each other among the stars, along with Andromeda. She was placed in the sky as a punishment for her boast that Andromeda was more beautiful than the Nereids; she was forced to wheel around the North Celestial Pole on her throne, spending half of her time clinging to it so she does not fall off.\r\rCassiopeia has been variously portrayed throughout her history as a constellation. In Persia, she was drawn by al-Sufi as a queen holding a staff with a crescent moon in her right hand, wearing a crown. In France, she was portrayed as having a marble throne and a palm leaf in her left hand, holding her robe in her right hand. This depiction is from Augustin Royer\u0027s 1679 atlas.",
		"key" : "Cassiopeia",
		"grouptype" : "Cassiopeia",
		"Meaning" : "Cassiopeia (mythological character)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Cassiopeia",
		"title" : "Cassiopeia Objects Group" },
	"Common" : "12 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "214.19",
	"RA_S" : 6.19793679,
	"DEC_S" : 61.83105925,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.376,
	"key" : 45685,
	"title" : "12 Cassiopeiae"
	},
{
	"Index" : "22553",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "14 Cassiopeiae, Lambda Cassiopeiae, HIP 2505AB, SAO 21489, HD 2772, GC 618, HR 123, DM BD+53    82, TYC 3658-2414-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Lambda Cassiopeiae",
	"OType" : "Double or multiple star",
	"Distance" : "115.4",
	"RA_S" : 7.94316395,
	"DEC_S" : 54.52228492,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.756,
	"key" : 42553,
	"title" : "Lambda Cassiopeiae"
	},
{
	"Index" : "25739",
	"Description" : "Kappa Cassiopeiae (\u03BA Cas, \u03BA Cassiopeiae) is a star in the constellation Cassiopeia.\r\r\u03BA Cassiopeiae is a blue-white B-type supergiant with a mean apparent magnitude of +4.17. It is approximately 4100 light years from Earth. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude +4.22 to +4.30.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "15 Cassiopeiae, Kappa Cassiopeiae, HIP 2599, SAO 11256, HD 2905, GC 645, HR 130, DM BD+62   102, TYC 4019-3949-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Kappa Cassiopeiae",
	"OType" : "Blue supergiant star",
	"RA_S" : 8.24996332,
	"DEC_S" : 62.93178261,
	"X" : 292,
	"Y" : 427,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.183,
	"key" : 45739,
	"title" : "Kappa Cassiopeiae"
	},
{
	"Index" : "22512",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 2854, SAO 21551, HD 3240, GC 708, HR 144, DM BD+53  102, TYC 3654-2131-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 144",
	"OType" : "Star",
	"Distance" : "164.06",
	"RA_S" : 9.03462489,
	"DEC_S" : 54.16844835,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.059,
	"key" : 42512,
	"title" : "HR 144"
	},
{
	"Index" : "22513",
	"Description" : "Zeta Cassiopeiae (\u03B6 Cas, \u03B6 Cassiopeiae) is a star in the constellation Cassiopeia. It has a blue-white hue and is classified as a B-type subgiant with an apparent magnitude of +3.67. It is approximately 590 light years from Earth.\r\r\u03B6 Cas is a member of an unusual group of variable stars known as \u0022Slowly Pulsating B\u0022 (SPB) stars. It shows a pulsation frequency of 0.64 per day (or once every 1.56 days) and displays a weak magnetic field with a strength of roughly 3.35 \u00D7 10\u20132 T, which varies with a period of 5.37 days. This likely matches the rotation rate of the star, which, when combined with the low projected rotational velocity, indicates the star may be seen nearly pole-on. Zeta Cassiopeiae is a candidate magnetic Bp star that shows an overabundance of helium. The star contains a randomly oriented fossil magnetic field, which impacts the outflow of the stellar wind. Collisions between streams from this stellar wind creates a shock front, with cooling particles settling toward a co-rotating disk.\r\rIn Chinese astronomy, Zeta Cassiopeiae is called \u9644\u8DEF, Pinyin: F\u00F9l\u00F9, meaning Auxiliary Road, because this star is marking itself and stand alone in Auxiliary Road asterism, Legs (mansion) (see : Chinese constellation). \u9644\u8DEF (F\u00F9l\u00F9) is westernized into Foo Loo, but the name Foo Loo was designated not only for Zeta Cassiopeiae, but also for \u03B7 Cassiopeiae (Achird) by R.H. Allen, with the meaning is \u0022a by-path",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "17 Cassiopeiae, Zeta Cassiopeiae, HIP 2920, SAO 21566, HD 3360, GC 727, HR 153, DM BD+53   105, TYC 3654-2132-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Zeta Cassiopeiae",
	"OType" : "Pulsating variable Star",
	"Distance" : "181.63",
	"RA_S" : 9.24285078,
	"DEC_S" : 53.89690758,
	"X" : 276,
	"Y" : 544,
	"Constellation" : "Cassiopeia ",
	"AMag" : 3.628,
	"key" : 42513,
	"title" : "Zeta Cassiopeiae"
	},
{
	"Index" : "18971",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "19 Cassiopeiae, Xi Cassiopeiae, HIP 3300, SAO 21637, HD 3901, GC 828, HR 179, DM BD+49   164, TYC 3257-2189-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Xi Cassiopeiae",
	"OType" : "Spectroscopic binary",
	"Distance" : "438.5965",
	"RA_S" : 10.5162233,
	"DEC_S" : 50.51252059,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.775,
	"key" : 38971,
	"title" : "Xi Cassiopeiae"
	},
{
	"Index" : "18930",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "20 Cassiopeiae, Pi Cassiopeiae, HIP 3414, SAO 36602, HD 4058, GC 856, HR 184, DM BD+46   146, TYC 3253-1987-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Pi Cassiopeiae",
	"OType" : "Spectroscopic binary",
	"Distance" : "53.66",
	"RA_S" : 10.86696078,
	"DEC_S" : 47.02454596,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.972,
	"key" : 38930,
	"title" : "Pi Cassiopeiae"
	},
{
	"Index" : "18931",
	"Description" : "Omicron Cassiopeiae (\u03BF Cas, \u03BF Cassiopeiae) is a triple star system in the constellation Cassiopeia. It is approximately 910 light years from Earth.\r\rThe primary component, \u03BF Cassiopeiae A, is a blue-white B-type giant with a mean apparent magnitude of +4.54. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.50 to +4.62. The primary is a spectroscopic binary, and its close companion completes one orbit every 2.83 years. A more distant companion, \u03BF Cassiopeiae B, lies 33.6 arcseconds away. It is an eleventh magnitude, yellow-white F-type main sequence dwarf.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "22 Cassiopeiae, Omicron Cassiopeiae, HIP 3504, SAO 36620, HD 4180, GC 882, HR 193, DM BD+47   183, TYC 3253-1988-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Omicron Cassiopeiae",
	"OType" : "Be Star",
	"Distance" : "213.8",
	"RA_S" : 11.18132777,
	"DEC_S" : 48.28436488,
	"X" : 253,
	"Y" : 615,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.463,
	"key" : 38931,
	"title" : "Omicron Cassiopeiae"
	},
{
	"Index" : "22563",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 3544, SAO 21677, HD 4222, GC 894, HR 196, DM BD+54  143, TYC 3659-2174-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Lalande 1171",
	"OType" : "Star",
	"Distance" : "98.67",
	"RA_S" : 11.32155672,
	"DEC_S" : 55.22139921,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.411,
	"key" : 42563,
	"title" : "Lalande 1171"
	},
{
	"Index" : "28131",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "23 Cassiopeiae, HIP 3721, SAO 4226, HD 4382, GC 934, HR 208, DM BD+74    29, TYC 4307-2166-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "23 Cassiopeiae",
	"OType" : "Spectroscopic binary",
	"Distance" : "235.64",
	"RA_S" : 11.94189354,
	"DEC_S" : 74.8475728,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.401,
	"key" : 48131,
	"title" : "23 Cassiopeiae"
	},
{
	"Index" : "19161",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "25 Cassiopeiae, Nu Cassiopeiae, HIP 3801, SAO 21729, HD 4636, GC 961, HR 223, DM BD+50   147, TYC 3274-2090-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Nu Cassiopeiae",
	"OType" : "Variable Star",
	"Distance" : "126.02",
	"RA_S" : 12.20842455,
	"DEC_S" : 50.96816716,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.875,
	"key" : 39161,
	"title" : "Nu Cassiopeiae"
	},
{
	"Index" : "22617",
	"Description" : "Eta Cassiopeiae (\u03B7 Cas, \u03B7 Cassiopeiae) is a star system in the northern circumpolar constellation of Cassiopeia. It has the traditional name Achird. Based upon parallax measurements, the distance to this system is 19.42 light-years (5.95 parsecs) from Earth.\r\rIn Chinese, \u738B\u826F (W\u00E1ng Li\u00E1ng), meaning Wang Liang, refers to an asterism consisting of \u03B7 Cassiopeiae, \u03B2 Cassiopeiae, \u03BA Cassiopeiae, \u03B1 Cassiopeiae and \u03BB Cassiopeiae. Consequently, \u03B7 Cassiopeiae itself is known as \u738B\u826F\u4E09 (W\u00E1ng Li\u00E1ng s\u0101n, English: the Third Star of Wang Liang.)",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "24 Cassiopeiae, Eta Cassiopeiae, HIP 3821A, TYC 3663-2669-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Achird",
	"OType" : "Star",
	"Distance" : "5.95",
	"RA_S" : 12.271438,
	"DEC_S" : 57.8165,
	"X" : 260,
	"Y" : 491,
	"Constellation" : "Cassiopeia ",
	"AMag" : 3.518,
	"key" : 42617,
	"title" : "Achird"
	},
{
	"Index" : "22618",
	"Description" : "Eta Cassiopeiae (\u03B7 Cas, \u03B7 Cassiopeiae) is a star system in the northern circumpolar constellation of Cassiopeia. It has the traditional name Achird. Based upon parallax measurements, the distance to this system is 19.42 light-years (5.95 parsecs) from Earth.\r\rIn Chinese, \u738B\u826F (W\u00E1ng Li\u00E1ng), meaning Wang Liang, refers to an asterism consisting of \u03B7 Cassiopeiae, \u03B2 Cassiopeiae, \u03BA Cassiopeiae, \u03B1 Cassiopeiae and \u03BB Cassiopeiae. Consequently, \u03B7 Cassiopeiae itself is known as \u738B\u826F\u4E09 (W\u00E1ng Li\u00E1ng s\u0101n, English: the Third Star of Wang Liang.)",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "24 Cassiopeiae, Eta Cassiopeiae, HIP 3821B, SAO 21732, HD 4614B, GC 962, HR 219, DM BD+57   150, TYC 3663-2669-2",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Achird",
	"OType" : "High proper-motion Star",
	"Distance" : "5.95",
	"RA_S" : 12.271529,
	"DEC_S" : 57.817714,
	"X" : 260,
	"Y" : 491,
	"Constellation" : "Cassiopeia ",
	"AMag" : 7.365,
	"key" : 42618,
	"title" : "Achird"
	},
{
	"Index" : "25788",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 3951, SAO 11424, HD 4775, GC 1004, HR 233, DM BD+63   99, TYC 4024-2330-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 233",
	"OType" : "Spectroscopic binary",
	"Distance" : "195.47",
	"RA_S" : 12.68172011,
	"DEC_S" : 64.24755193,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.421,
	"key" : 45788,
	"title" : "HR 233"
	},
{
	"Index" : "25709",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 4151, SAO 11444, HD 5015, GC 1047, HR 244, DM BD+60  124, TYC 4017-2318-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Gliese 41 (HR 244)",
	"OType" : "Star",
	"Distance" : "18.74",
	"RA_S" : 13.26748341,
	"DEC_S" : 61.1239707,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.848,
	"key" : 45709,
	"title" : "Gliese 41 (HR 244)"
	},
{
	"Index" : "22789",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "26 Cassiopeiae, Upsilon01 Cassiopeiae, HIP 4292, SAO 21832, HD 5234, GC 1086, HR 253, DM BD+58   134, TYC 3680-1840-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Upsilon01 Cassiopeiae",
	"OType" : "High proper-motion Star",
	"Distance" : "100.41",
	"RA_S" : 13.75065293,
	"DEC_S" : 58.97269068,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.957,
	"key" : 42789,
	"title" : "Upsilon01 Cassiopeiae"
	},
{
	"Index" : "22788",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "28 Cassiopeiae, Upsilon02 Cassiopeiae, HIP 4422, SAO 21855, HD 5395, GC 1115, HR 265, DM BD+58   138, TYC 3680-1839-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Upsilon02 Cassiopeiae",
	"OType" : "Peculiar Star",
	"Distance" : "61.26",
	"RA_S" : 14.16627596,
	"DEC_S" : 59.18105467,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.728,
	"key" : 42788,
	"title" : "Upsilon02 Cassiopeiae"
	},
{
	"Index" : "22714",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "30 Cassiopeiae, Mu Cassiopeiae, HIP 5336, SAO 22024, HD 6582, GC 1360, HR 321, DM BD+54   223, TYC 3673-1929-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Marfak (with HD6961)",
	"OType" : "Spectroscopic binary",
	"Distance" : "7.55",
	"RA_S" : 17.0681861,
	"DEC_S" : 54.92029007,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.23,
	"key" : 42714,
	"title" : "Marfak (with HD6961)"
	},
{
	"Index" : "28043",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "31 Cassiopeiae, HIP 5518, SAO 11612, HD 6829, GC 1406, HR 336, DM BD+68    77, TYC 4296-1459-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "31 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "84.84",
	"RA_S" : 17.66383767,
	"DEC_S" : 68.77861435,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.304,
	"key" : 48043,
	"title" : "31 Cassiopeiae"
	},
{
	"Index" : "22713",
	"Description" : "Theta Cassiopeiae (\u03B8 Cas, \u03B8 Cassiopeiae) is a star in the constellation Cassiopeia. It has the traditional name Marfark or Marfak, which it shares with \u03BC Cassiopeiae, and the name was from Al Marfik or Al Mirfaq (\u0627\u0644\u0645\u0631\u0641\u0642), meaning \u0022the elbow\u0022.\r\rIn Chinese, \u95A3\u9053 (G\u00E9 D\u00E0o), meaning Flying Corridor, refers to an asterism consisting of \u03B8 Cassiopeiae, \u03B9 Cassiopeiae, \u03B5 Cassiopeiae, \u03B4 Cassiopeiae, \u03BD Cassiopeiae and \u03BF Cassiopeiae. Consequently, \u03B8 Cassiopeiae itself is known as \u95A3\u9053\u56DB (G\u00E9 D\u00E0o s\u00EC, English: the Fourth Star of Flying Corridor.)\r\r\u03B8 Cassiopeiae is a white A-type main sequence dwarf with an apparent magnitude of +4.34. It is approximately 137 light years from Earth.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "33 Cassiopeiae, Theta Cassiopeiae, HIP 5542, SAO 22070, HD 6961, GC 1424, HR 343, DM BD+54   236, TYC 3673-1923-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Marfark",
	"OType" : "Variable Star",
	"Distance" : "40.95",
	"RA_S" : 17.77567602,
	"DEC_S" : 55.14990201,
	"X" : 215,
	"Y" : 518,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.343,
	"key" : 42713,
	"title" : "Marfark"
	},
{
	"Index" : "22812",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "34 Cassiopeiae, Phi Cassiopeiae, HIP 6242, SAO 22191, HD 7927, GC 1594, HR 382, DM BD+57   260, TYC 3682-2389-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Phi Cassiopeiae",
	"OType" : "Star",
	"RA_S" : 20.02048923,
	"DEC_S" : 58.23161207,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.069,
	"key" : 42812,
	"title" : "Phi Cassiopeiae"
	},
{
	"Index" : "25866",
	"Description" : "Delta Cassiopeiae (\u03B4 Cas, \u03B4 Cassiopeiae) is a star in the northern circumpolar constellation of Cassiopeia. It has the traditional names Ksora and Ruchbah, derived from the Arabic word \u0631\u0643\u0628\u0629 rukbah meaning \u0022knee\u0022. It is not to be confused with Alpha Sagittarii, which also is called Ruchbah or Rukbat.\r\rIn Chinese, \u95A3\u9053 (G\u00E9 D\u00E0o), meaning Flying Corridor, refers to an asterism consisting of \u03B4 Cassiopeiae, \u03B9 Cassiopeiae, \u03B5 Cassiopeiae, \u03B8 Cassiopeiae, \u03BD Cassiopeiae and \u03BF Cassiopeiae. Consequently, \u03B4 Cassiopeiae itself is known as \u95A3\u9053\u4E09 (G\u00E9 D\u00E0o s\u0101n, English: the Third Star of Flying Corridor.)",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "37 Cassiopeiae, Delta Cassiopeiae, HIP 6686, SAO 22268, HD 8538, GC 1715, HR 403, DM BD+59   248, TYC 4031-3289-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Ksora / Ruchbah",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "30.48",
	"RA_S" : 21.45396446,
	"DEC_S" : 60.23528403,
	"X" : 206,
	"Y" : 448,
	"Constellation" : "Cassiopeia ",
	"AMag" : 2.66,
	"key" : 45866,
	"shortTitle" : "Ksora; Rucha; Rucba (also HD181869); Rukba",
	"title" : "Ksora / Ruchbah"
	},
{
	"Index" : "28057",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "36 Cassiopeiae, Psi Cassiopeiae, HIP 6692, SAO 11751, HD 8491, GC 1707, HR 399, DM BD+67   123, TYC 4297-1685-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Psi Cassiopeiae",
	"OType" : "Double or multiple star",
	"Distance" : "59.8",
	"RA_S" : 21.48342486,
	"DEC_S" : 68.13001598,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.844,
	"key" : 48057,
	"title" : "Psi Cassiopeiae"
	},
{
	"Index" : "22822",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "39 Cassiopeiae, Chi Cassiopeiae, HIP 7294, SAO 22397, HD 9408, GC 1879, HR 442, DM BD+58   260, TYC 3683-2185-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Chi Cassiopeiae",
	"OType" : "Star",
	"Distance" : "63.77",
	"RA_S" : 23.48281891,
	"DEC_S" : 59.23204329,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.791,
	"key" : 42822,
	"title" : "Chi Cassiopeiae"
	},
{
	"Index" : "28221",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "40 Cassiopeiae, HIP 7650, SAO 4453, HD 9774, GC 1955, HR 456, DM BD+72    86, TYC 4318-2488-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "40 Cassiopeiae",
	"OType" : "Variable Star",
	"Distance" : "140.13",
	"RA_S" : 24.62882142,
	"DEC_S" : 73.04003806,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.389,
	"key" : 48221,
	"title" : "40 Cassiopeiae"
	},
{
	"Index" : "28195",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "42 Cassiopeiae, HIP 8016, SAO 4470, HD 10250, GC 2059, HR 480, DM BD+69   114, TYC 4314-2021-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "42 Cassiopeiae",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "85.07",
	"RA_S" : 25.73275206,
	"DEC_S" : 70.62252745,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.169,
	"key" : 48195,
	"title" : "42 Cassiopeiae"
	},
{
	"Index" : "25923",
	"Description" : "Epsilon Cassiopeiae (\u03B5 Cas, \u03B5 Cassiopeiae) is a star system in the constellation Cassiopeia. It has the traditional name Segin. With an apparent visual magnitude of 3.4, this is one of the brightest stars in the constellation. The distance to this star has been determined directly using parallax measurements, yielding a value of around 390\u2013430 light-years (120\u2013130 parsecs).",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "45 Cassiopeiae, Epsilon Cassiopeiae, HIP 8886, SAO 12031, HD 11415, GC 2289, HR 542, DM BD+62   320, TYC 4036-2834-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Segin",
	"OType" : "Be Star",
	"Distance" : "125.82",
	"RA_S" : 28.59885697,
	"DEC_S" : 63.67010079,
	"X" : 179,
	"Y" : 392,
	"Constellation" : "Cassiopeia ",
	"AMag" : 3.313,
	"key" : 45923,
	"shortTitle" : "Ruchbah (Allen,see HD8538)",
	"title" : "Segin"
	},
{
	"Index" : "28160",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "46 Cassiopeiae, Omega Cassiopeiae, HIP 9009, SAO 12038, HD 11529, GC 2313, HR 548, DM BD+67   169, TYC 4310-902-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Omega Cassiopeiae",
	"OType" : "Spectroscopic binary",
	"Distance" : "214.37",
	"RA_S" : 29.00009851,
	"DEC_S" : 68.68524096,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.953,
	"key" : 48160,
	"title" : "Omega Cassiopeiae"
	},
{
	"Index" : "25953",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 9312, SAO 12076, HD 11946, GC 2379, HR 567, DM BD+63  265, TYC 4040-2022-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 567",
	"OType" : "Star",
	"Distance" : "75.27",
	"RA_S" : 29.90850432,
	"DEC_S" : 64.62160223,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.277,
	"key" : 45953,
	"title" : "HR 567"
	},
{
	"Index" : "28200",
	"Description" : "48 Cassiopeiae is a star system in the constellation Cassiopeia. It is approximately 116.9 light years from Earth.\r\rThe primary component, 48 Cassiopeiae A, is a white A-type subgiant with an apparent magnitude of +4.71. It has an astrometric companion, 48 Cassiopeiae B, which is a F-type main sequence dwarf with an apparent magnitude of +6.41. These two stars orbit around their common centre of mass once every 60.5 years. Component B has a semi-major axis of 0.62 arcseconds, or 22 AU. A third companion, 48 Cassiopeiae C, is a fourteenth magnitude star located 24 arcseconds, or at least 850 AU, away. The primary is also a spectroscopic binary, and has an unresolved companion, meaning the system has at least four components.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "48 Cassiopeiae, A Cassiopeiae, HIP 9480A, SAO 4554, HD 12111, GC 2424, HR 575, DM BD+70   153, TYC 4315-2126-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "48 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "35.25",
	"RA_S" : 30.48928821,
	"DEC_S" : 70.90705771,
	"X" : 207,
	"Y" : 301,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.647,
	"key" : 48200,
	"title" : "48 Cassiopeiae"
	},
{
	"Index" : "28201",
	"Description" : "48 Cassiopeiae is a star system in the constellation Cassiopeia. It is approximately 116.9 light years from Earth.\r\rThe primary component, 48 Cassiopeiae A, is a white A-type subgiant with an apparent magnitude of +4.71. It has an astrometric companion, 48 Cassiopeiae B, which is a F-type main sequence dwarf with an apparent magnitude of +6.41. These two stars orbit around their common centre of mass once every 60.5 years. Component B has a semi-major axis of 0.62 arcseconds, or 22 AU. A third companion, 48 Cassiopeiae C, is a fourteenth magnitude star located 24 arcseconds, or at least 850 AU, away. The primary is also a spectroscopic binary, and has an unresolved companion, meaning the system has at least four components.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "48 Cassiopeiae, A Cassiopeiae, HIP 9480B, SAO 4554, HD 12111, GC 2424, HR 575, DM BD+70   153, TYC 4315-2126-2",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "48 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "35.25",
	"RA_S" : 30.48928821,
	"DEC_S" : 70.90705771,
	"X" : 207,
	"Y" : 301,
	"Constellation" : "Cassiopeia ",
	"AMag" : 6.744,
	"key" : 48201,
	"title" : "48 Cassiopeiae"
	},
{
	"Index" : "28225",
	"Description" : "50 Cassiopeiae is a star in the constellation Cassiopeia. In the past, it had been misidentified as a suspected nebula, and given the number NGC 771.\r\r50 Cassiopeiae is a white A-type main sequence dwarf with an apparent magnitude of +3.95. It is approximately 162.1 light years from Earth.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "50 Cassiopeiae, HIP 9598, SAO 4560, HD 12216, GC 2445, HR 580, DM BD+71   117, TYC 4319-1847-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "50 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "48.17",
	"RA_S" : 30.85877576,
	"DEC_S" : 72.42129382,
	"X" : 214,
	"Y" : 283,
	"Constellation" : "Cassiopeia ",
	"AMag" : 3.94,
	"key" : 48225,
	"title" : "50 Cassiopeiae"
	},
{
	"Index" : "29649",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "47 Cassiopeiae, HIP 9727, SAO 4562, HD 12230, GC 2459, HR 581, DM BD+76    63, TYC 4499-2252-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "47 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "33.15",
	"RA_S" : 31.28073848,
	"DEC_S" : 77.28131341,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.308,
	"key" : 49649,
	"title" : "47 Cassiopeiae"
	},
{
	"Index" : "29626",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "49 Cassiopeiae, HIP 9763, SAO 4565, HD 12339, GC 2475, HR 592, DM BD+75    86, TYC 4495-1881-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "49 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "122.56",
	"RA_S" : 31.38146671,
	"DEC_S" : 76.1150589,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.322,
	"key" : 49626,
	"title" : "49 Cassiopeiae"
	},
{
	"Index" : "26111",
	"Description" : "Iota Cassiopeiae (\u03B9 Cas, \u03B9 Cassiopeiae) is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth.\r\rThe primary component, \u03B9 Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an \u03B1\u00B2 Canum Venaticorum type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days. Component A is a spectroscopic binary. Its unresolved companion has an orbital period of 52.4 years and is separated from the primary by 0.113 arcseconds, or at least 5 AU.\r\rThe second astrometric component, \u03B9 Cassiopeiae B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.89. It is 2.27 arcseconds, or at least 100 AU, from the primary. It has an orbital period of 840 years. The third astrometric component, \u03B9 Cassiopeiae C, is a yellow G-type dwarf, with an apparent magnitude of +8.40. It is 7.3 arcseconds (at least 300 AU) from the primary.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "Iota Cassiopeiae, HIP 11569A, SAO 12298, HD 15089A, GC 2952, HR 707, DM BD+66   213, TYC 4058-1504-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Iota Cassiopeiae",
	"OType" : "Double or multiple star",
	"Distance" : "43.34",
	"RA_S" : 37.2664289,
	"DEC_S" : 67.4023957,
	"X" : 158,
	"Y" : 328,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.627,
	"key" : 46111,
	"title" : "Iota Cassiopeiae"
	},
{
	"Index" : "26112",
	"Description" : "Iota Cassiopeiae (\u03B9 Cas, \u03B9 Cassiopeiae) is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth.\r\rThe primary component, \u03B9 Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an \u03B1\u00B2 Canum Venaticorum type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days. Component A is a spectroscopic binary. Its unresolved companion has an orbital period of 52.4 years and is separated from the primary by 0.113 arcseconds, or at least 5 AU.\r\rThe second astrometric component, \u03B9 Cassiopeiae B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.89. It is 2.27 arcseconds, or at least 100 AU, from the primary. It has an orbital period of 840 years. The third astrometric component, \u03B9 Cassiopeiae C, is a yellow G-type dwarf, with an apparent magnitude of +8.40. It is 7.3 arcseconds (at least 300 AU) from the primary.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "Iota Cassiopeiae, HIP 11569B, SAO 12298, HD 15089B, GC 2952, HR 707, DM BD+66   213, TYC 4058-1504-2",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Iota Cassiopeiae",
	"OType" : "Star",
	"Distance" : "43.34",
	"RA_S" : 37.2664289,
	"DEC_S" : 67.4023957,
	"X" : 158,
	"Y" : 328,
	"Constellation" : "Cassiopeia ",
	"AMag" : 6.919,
	"key" : 46112,
	"title" : "Iota Cassiopeiae"
	},
{
	"Index" : "28232",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 12273, SAO 4694, HD 15920, GC 3116, HR 743, DM BD+72  140, TYC 4320-2109-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 743",
	"OType" : "Star",
	"Distance" : "78.4",
	"RA_S" : 39.50846879,
	"DEC_S" : 72.81825148,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.266,
	"key" : 48232,
	"title" : "HR 743"
	},
{
	"Index" : "28263",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 14862, SAO 4840, HD 19275, GC 3759, HR 932, DM BD+73  168, TYC 4325-1562-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 932",
	"OType" : "Star",
	"Distance" : "50.7",
	"RA_S" : 47.98442933,
	"DEC_S" : 74.39366357,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.84,
	"key" : 48263,
	"title" : "HR 932"
	},
{
	"Index" : "25436",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 113561, SAO 35039, HD 217476, GC 32063, HR 8752, DM BD+56 2923, TYC 3993-2269-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "HR 8752",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 345.02125881,
	"DEC_S" : 56.94537539,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.21,
	"key" : 45436,
	"title" : "HR 8752"
	},
{
	"Index" : "25472",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "1 Cassiopeiae, HIP 114104, SAO 35147, HD 218376, GC 32197, HR 8797, DM BD+58  2545, TYC 3997-2306-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "1 Cassiopeiae",
	"OType" : "Star",
	"Distance" : "345.18",
	"RA_S" : 346.65340774,
	"DEC_S" : 59.41975992,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.829,
	"key" : 45472,
	"title" : "1 Cassiopeiae"
	},
{
	"Index" : "27913",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "4 Cassiopeiae, HIP 115590, SAO 20614, HD 220652, GC 32582, HR 8904, DM BD+61  2444, TYC 4283-1498-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "4 Cassiopeiae",
	"OType" : "Variable Star",
	"Distance" : "240.23",
	"RA_S" : 351.20942839,
	"DEC_S" : 62.2828071,
	"Constellation" : "Cassiopeia ",
	"AMag" : 5.157,
	"key" : 47913,
	"title" : "4 Cassiopeiae"
	},
{
	"Index" : "25626",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "AR Cassiopeiae, HIP 115990, SAO 35478, HD 221253, GC 32683, HR 8926, DM BD+57  2748, TYC 4011-1296-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "AR Cassiopeiae",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "188.26",
	"RA_S" : 352.50808109,
	"DEC_S" : 58.54892001,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.866,
	"key" : 45626,
	"title" : "AR Cassiopeiae"
	},
{
	"Index" : "25653",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "5 Cassiopeiae, Tau Cassiopeiae, HIP 117301, SAO 35763, HD 223165, GC 33010, HR 9008, DM BD+57  2804, TYC 4013-1825-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Tau Cassiopeiae",
	"OType" : "Variable Star",
	"Distance" : "53.33",
	"RA_S" : 356.76439588,
	"DEC_S" : 58.6519874,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.998,
	"key" : 45653,
	"title" : "Tau Cassiopeiae"
	},
{
	"Index" : "25612",
	"Description" : "Rho Cassiopeiae (pron.: /\u02CCro\u028A k\u00E6si\u0259\u02C8pi\u02D0.i\u02D0/; \u03C1 Cas, \u03C1 Cassiopeiae) is a yellow hypergiant star in the constellation Cassiopeia. It is about 8,200 light-years (2,500 pc) away from Earth, yet can still be seen by the naked eye (in the Northern Hemisphere only), as it is 500,000 times more luminous than the Sun. On average, it has an absolute magnitude of \u22129.5, making it one of the most luminous stars known. Its surface diameter measures 450 times that of the Sun, or approximately 630,000,000 kilometers. Being a yellow hypergiant, it is one of the rarest types of stars, one of only twelve in the Milky Way that are currently known, though it is not the only one in its constellation, which also includes V509 Cassiopeiae. Rho Cassiopeiae is a single star, and is categorized as a semiregular variable.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "7 Cassiopeiae, Rho Cassiopeiae, HIP 117863, SAO 35879, HD 224014, GC 33160, HR 9045, DM BD+56  3111, TYC 4009-2605-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "Rho Cassiopeiae",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 358.59596168,
	"DEC_S" : 57.49938359,
	"X" : 354,
	"Y" : 498,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.628,
	"key" : 45612,
	"title" : "Rho Cassiopeiae"
	},
{
	"Index" : "22473",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "R Cassiopeiae, HIP 118188, SAO 35938, HD 224490, GC 33244, HR 9066, DM BD+50  4202, TYC 3651-470-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "R Cassiopeiae",
	"OType" : "Variable Star of Mira Cet type",
	"Distance" : "123.35",
	"RA_S" : 359.60363898,
	"DEC_S" : 51.38880585,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.8,
	"key" : 42473,
	"title" : "R Cassiopeiae"
	},
{
	"Index" : "25563",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "8 Cassiopeiae, Sigma Cassiopeiae, HIP 118243A, TYC 4005-2471-1",
	"group" : { "key" : "Cassiopeia" },
	"Common" : "8 Sigma Cassiopeiae (HR 9071)",
	"OType" : "Star",
	"RA_S" : 359.752208,
	"DEC_S" : 55.754939,
	"Constellation" : "Cassiopeia ",
	"AMag" : 4.991,
	"key" : 45563,
	"title" : "8 Sigma Cassiopeiae (HR 9071)"
	},
{
	"Index" : "54991",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 54360A, SAO 222581, HD 96616, GC 15300, HR 4327, DM CD-41 6343, TYC 7733-2500-1",
	"group" : { "backgroundImage" : "images/Alignment/15.png",
		"description" : "Centaurus (pron.: /s\u025Bn\u02C8t\u0254r\u0259s/) is a bright constellation in the southern sky. One of the largest constellations, Centaurus was included among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. In Greek mythology, Centaurus represents a centaur; a creature that is half man, half horse. (Another constellation named after a centaur is one from the zodiac: Sagittarius.)\r\rWhile Centaurus now has a high southern latitude, at the dawn of civilization it was an equatorial constellation. Precession has been slowly shifting it southward for millennia, and it is now close to its maximal southern declination. Thousands of years from now Centaurus will, once again, be at lower latitudes and be visible worldwide.\r\rThe figure of Centaurus can be traced back to a Babylonian constellation known as the Bison-man (MUL.GUD.ALIM). This being was depicted in two major forms: firstly, as a 4-legged bison with a human head, and secondly, as a being with a man\u0027s head and torso attached to the rear legs and tail of a bull or bison. It has been closely associated with the Sun god Utu-Shamash from very early times.\r\rThe Greeks depicted the constellation as a centaur and gave it its current name. It was mentioned by Eudoxus in the 4th century BCE and Aratus in the 3rd century BCE. In the 2nd century AD, Claudius Ptolemy catalogued 37 stars in Centaurus. Large as it is now, in earlier times it was even larger, as the constellation Lupus was treated as an asterism within Centaurus, portrayed in illustrations as an unspecified animal either in the centaur\u0027s grasp or impaled on its spear. The Southern Cross, which is now regarded as a separate constellation, was treated by the ancients as a mere asterism formed of the stars composing the centaur\u0027s legs. Additionally, what is now the minor constellation Circinus was treated as undefined stars under the centaur\u0027s front hooves.\r\rAccording to the Roman poet Ovid (Fasti v.379), the constellation honors the centaur Chiron, who was tutor to many of the earlier Greek heroes including Heracles (Hercules), Theseus, and Jason, the leader of the Argonauts. However, most authorities consider Sagittarius to be the civilized Chiron, while Centaurus represents a more uncouth member of the species. The legend associated with Chiron says that he was accidentally poisoned with an arrow shot by Hercules, and was subsequently placed in the heavens.",
		"key" : "Centaurus",
		"grouptype" : "Centaurus",
		"Meaning" : "centaur",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Centaurus",
		"title" : "Centaurus Objects Group" },
	"Common" : "*  46 Cen",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "84",
	"RA_S" : 166.81951816,
	"DEC_S" : -42.63868077,
	"Constellation" : "Centaurus ",
	"AMag" : 5.237,
	"key" : 74991,
	"title" : "*  46 Cen"
	},
{
	"Index" : "59227",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 54746, SAO 222639, HD 97495, GC 15411, HR 4350, DM CD-48 6263, TYC 8208-2153-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4350",
	"OType" : "Double or multiple star",
	"Distance" : "50.29",
	"RA_S" : 168.13773602,
	"DEC_S" : -49.10099454,
	"Constellation" : "Centaurus ",
	"AMag" : 5.388,
	"key" : 79227,
	"title" : "HR 4350"
	},
{
	"Index" : "63179",
	"Description" : "Pi Centauri (\u03C0 Cen, \u03C0 Centauri) is a binary star in the constellation Centaurus. It is approximately 360 light years from Earth.\r\rBoth components are blue-white B-type main sequence dwarfs. The primary \u03C0 Centauri A, has an apparent magnitude of +4.3, while the apparent magnitude of its companion, \u03C0 Centauri B, is +5.0. The two stars orbit around their common centre of mass once every 39.18 years. The semi-major axis of the companion is 0.23 arcseconds on the sky.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Pi Centauri, HIP 55425AB, SAO 238986, HD 98718A, GC 15601, HR 4390, DM CP-53  4498, TYC 8621-2002-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Pi Centauri",
	"OType" : "Star",
	"Distance" : "109.5",
	"RA_S" : 170.25170677,
	"DEC_S" : -54.49103279,
	"X" : 557,
	"Y" : 390,
	"Constellation" : "Centaurus ",
	"AMag" : 3.873,
	"key" : 83179,
	"title" : "Pi Centauri"
	},
{
	"Index" : "50518",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 55588, SAO 202391, HD 98993, GC 15641, HR 4396, DM CD-35 7163, TYC 7214-353-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4396",
	"OType" : "Star",
	"Distance" : "310.06",
	"RA_S" : 170.8028543,
	"DEC_S" : -36.16477108,
	"Constellation" : "Centaurus ",
	"AMag" : 5.161,
	"key" : 70518,
	"title" : "HR 4396"
	},
{
	"Index" : "50599",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 55756, SAO 202428, HD 99322, GC 15680, HR 4409, DM CD-35 7189, TYC 7227-1664-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4409",
	"OType" : "Star",
	"Distance" : "83.96",
	"RA_S" : 171.37272382,
	"DEC_S" : -36.06306414,
	"Constellation" : "Centaurus ",
	"AMag" : 5.328,
	"key" : 70599,
	"title" : "HR 4409"
	},
{
	"Index" : "66810",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 55779, SAO 251402, HD 99453, GC 15693, HR 4413, DM CP-63 1893, TYC 8980-2291-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 3663",
	"OType" : "Spectroscopic binary",
	"Distance" : "27.22",
	"RA_S" : 171.42977755,
	"DEC_S" : -63.97247626,
	"Constellation" : "Centaurus ",
	"AMag" : 5.224,
	"key" : 86810,
	"title" : "Gliese 3663"
	},
{
	"Index" : "66605",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 55831, SAO 251406, HD 99556, GC 15708, HR 4415, DM CP-60 2941, TYC 8972-1221-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4415",
	"OType" : "Star",
	"Distance" : "413.81",
	"RA_S" : 171.64757824,
	"DEC_S" : -61.11517037,
	"Constellation" : "Centaurus ",
	"AMag" : 5.259,
	"key" : 86605,
	"title" : "HR 4415"
	},
{
	"Index" : "55104",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 56000A, SAO 222813, HD 99803, GC 15744, HR 4423, DM CD-41 6565, TYC 7747-2546-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4423",
	"OType" : "Star",
	"Distance" : "208.93",
	"RA_S" : 172.14615322,
	"DEC_S" : -42.67420441,
	"Constellation" : "Centaurus ",
	"AMag" : 5.131,
	"key" : 75104,
	"title" : "HR 4423"
	},
{
	"Index" : "63376",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Omicron01 Centauri, HIP 56243, SAO 239145, HD 100261, GC 15818, HR 4441, DM CP-58  3692, TYC 8629-1712-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Omicron01 Centauri",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 172.94194495,
	"DEC_S" : -59.44205936,
	"Constellation" : "Centaurus ",
	"AMag" : 5.212,
	"key" : 83376,
	"title" : "Omicron01 Centauri"
	},
{
	"Index" : "63377",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Omicron02 Centauri, HIP 56250, SAO 239146, HD 100262, GC 15820, HR 4442, DM CP-58  3693, TYC 8629-1713-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Omicron02 Centauri",
	"OType" : "Pulsating variable Star",
	"RA_S" : 172.95333213,
	"DEC_S" : -59.51564911,
	"Constellation" : "Centaurus ",
	"AMag" : 5.224,
	"key" : 83377,
	"title" : "Omicron02 Centauri"
	},
{
	"Index" : "63405",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "A Centauri, HIP 56480, SAO 239189, HD 100673, GC 15877, HR 4460, DM CP-53  4637, TYC 8630-2190-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "A Centauri",
	"OType" : "Be Star",
	"Distance" : "130.59",
	"RA_S" : 173.69023526,
	"DEC_S" : -54.26409128,
	"Constellation" : "Centaurus ",
	"AMag" : 4.595,
	"key" : 83405,
	"title" : "A Centauri"
	},
{
	"Index" : "66738",
	"Description" : "Lambda Centauri (\u03BB Cen, \u03BB Centauri) is a star in the southern circumpolar constellation of Centaurus. It has an apparent visual magnitude of +3.13, which is bright enough to be seen with the naked eye from the southern hemisphere and places it among the brighter members of this constellation. The star is close enough that its distance can be determined directly using the parallax technique, which gives a value of roughly 420 light-years (130 parsecs) from Earth, with a 5% margin of error. Although a putative solitary star, it has a candidate proper motion companion at an angular separation of 0.73 arcseconds along a position angle of 135\u00B0.\r\r\u03BB Centauri is a B-type giant star with a stellar classification of B9 III. (Although it has also been classified as A1 III.) It has about 5.5 times the radius of the Sun and is rotating rapidly with a projected rotational velocity of 183 km s\u20131. The star\u0027s outer atmosphere has an effective temperature of 9,880 K, giving it a blue-white hue.\r\rBased upon the position and movement of this star through space, it is a likely member of the Gould Belt. In particular, it belongs to the Lower Centaurus-Crux (LCC) group of the Scorpius-Centaurus Association, which is the nearest OB association to the Sun. This is a loose grouping of stars that share a common motion through space and therefore formed in the same molecular cloud. The LCC group has an estimated age of 16\u201320 million years and is centered around a mean distance of 380 light-years (120 parsecs) from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Lambda Centauri, HIP 56561, SAO 251472, HD 100841, GC 15899, HR 4467, DM CP-62  2127, TYC 8976-5383-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Lambda Centauri",
	"OType" : "Star",
	"Distance" : "128.41",
	"RA_S" : 173.94534186,
	"DEC_S" : -63.019845,
	"X" : 493,
	"Y" : 486,
	"Constellation" : "Centaurus ",
	"AMag" : 3.092,
	"key" : 86738,
	"title" : "Lambda Centauri"
	},
{
	"Index" : "59337",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "C02 Centauri, HIP 56573, SAO 222895, HD 100825, GC 15901, HR 4466, DM CD-46  7205, TYC 8218-1882-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "C02 Centauri",
	"OType" : "Star",
	"Distance" : "61.78",
	"RA_S" : 173.98160411,
	"DEC_S" : -47.64163733,
	"Constellation" : "Centaurus ",
	"AMag" : 5.283,
	"key" : 79337,
	"title" : "C02 Centauri"
	},
{
	"Index" : "66631",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 56656, SAO 251486, HD 101021, GC 15935, HR 4475, DM CP-60 3182, TYC 8972-2817-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 101021",
	"OType" : "High proper-motion Star",
	"Distance" : "71.65",
	"RA_S" : 174.25219264,
	"DEC_S" : -61.28344122,
	"Constellation" : "Centaurus ",
	"AMag" : 5.251,
	"key" : 86631,
	"title" : "HD 101021"
	},
{
	"Index" : "66632",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 56754, SAO 251505, HD 101189, GC 15965, HR 4487, DM CP-61 2463, TYC 8972-2819-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4487",
	"OType" : "Star in Cluster",
	"Distance" : "87.27",
	"RA_S" : 174.53038312,
	"DEC_S" : -61.82653113,
	"Constellation" : "Centaurus ",
	"AMag" : 5.129,
	"key" : 86632,
	"title" : "HR 4487"
	},
{
	"Index" : "66737",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 56986, SAO 251535, HD 101570, GC 16037, HR 4499, DM CP-61 2514, TYC 8976-5382-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4499",
	"OType" : "Star",
	"Distance" : "271.2",
	"RA_S" : 175.22347505,
	"DEC_S" : -62.09010277,
	"Constellation" : "Centaurus ",
	"AMag" : 5.062,
	"key" : 86737,
	"title" : "HR 4499"
	},
{
	"Index" : "66762",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57175, SAO 251555, HD 101947, GC 16092, HR 4511, DM CP-61 2559, TYC 8977-9437-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "V* V810 Cen",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 175.87996552,
	"DEC_S" : -62.48939602,
	"Constellation" : "Centaurus ",
	"AMag" : 5.103,
	"key" : 86762,
	"title" : "V* V810 Cen"
	},
{
	"Index" : "59309",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57371, SAO 223009, HD 102232, GC 16133, HR 4519, DM CD-44 7564, TYC 8215-2314-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4519",
	"OType" : "Variable Star",
	"Distance" : "211.1",
	"RA_S" : 176.43320336,
	"DEC_S" : -45.69013472,
	"Constellation" : "Centaurus ",
	"AMag" : 5.252,
	"key" : 79309,
	"title" : "HR 4519"
	},
{
	"Index" : "66664",
	"Description" : "HD 102350 is a star in the constellation Centaurus. Its apparent magnitude is 4.10.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57439, SAO 251579, HD 102350, GC 16147, HR 4522, DM CP-60 3325, TYC 8973-2923-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 102350",
	"OType" : "Cepheid variable Star",
	"Distance" : "119.42",
	"RA_S" : 176.62842921,
	"DEC_S" : -61.17839713,
	"X" : 485,
	"Y" : 458,
	"Constellation" : "Centaurus ",
	"AMag" : 4.199,
	"key" : 86664,
	"title" : "HD 102350"
	},
{
	"Index" : "55088",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57443, SAO 223020, HD 102365, GC 16149, HR 4523, DM CD-39 7301, TYC 7745-1381-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 442 A",
	"OType" : "High proper-motion Star",
	"Distance" : "9.22",
	"RA_S" : 176.6294711,
	"DEC_S" : -40.50035427,
	"Constellation" : "Centaurus ",
	"AMag" : 4.962,
	"key" : 75088,
	"title" : "Gliese 442 A"
	},
{
	"Index" : "66821",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "j Centauri, HIP 57669, SAO 251602, HD 102776, GC 16201, HR 4537, DM CP-63  1988, TYC 8981-4409-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "j Centauri",
	"OType" : "Be Star",
	"Distance" : "179.98",
	"RA_S" : 177.42108582,
	"DEC_S" : -63.78847913,
	"Constellation" : "Centaurus ",
	"AMag" : 4.284,
	"key" : 86821,
	"title" : "j Centauri"
	},
{
	"Index" : "59314",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "B Centauri, HIP 57803, SAO 223062, HD 102964, GC 16226, HR 4546, DM CD-44  7614, TYC 8216-2577-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "B Centauri",
	"OType" : "Star",
	"Distance" : "132.67",
	"RA_S" : 177.78621136,
	"DEC_S" : -45.17347025,
	"Constellation" : "Centaurus ",
	"AMag" : 4.609,
	"key" : 79314,
	"title" : "B Centauri"
	},
{
	"Index" : "55210",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 58803, SAO 223193, HD 104731, GC 16472, HR 4600, DM CD-41 6938, TYC 7763-1047-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 3701",
	"OType" : "High proper-motion Star",
	"Distance" : "25.32",
	"RA_S" : 180.91488294,
	"DEC_S" : -42.4340575,
	"Constellation" : "Centaurus ",
	"AMag" : 5.196,
	"key" : 75210,
	"title" : "Gliese 3701"
	},
{
	"Index" : "59528",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 59173, SAO 239687, HD 105382, GC 16576, HR 4618, DM CD-49 6813, TYC 8241-3234-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4618",
	"OType" : "Be Star",
	"Distance" : "133.33",
	"RA_S" : 182.02176936,
	"DEC_S" : -50.66127675,
	"Constellation" : "Centaurus ",
	"AMag" : 4.419,
	"key" : 79528,
	"title" : "HR 4618"
	},
{
	"Index" : "59463",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "E Centauri, HIP 59184, SAO 223235, HD 105416, GC 16581, HR 4620, DM CD-47  7396, TYC 8233-3212-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "E Centauri",
	"OType" : "Star",
	"Distance" : "183.16",
	"RA_S" : 182.06129315,
	"DEC_S" : -48.69248683,
	"Constellation" : "Centaurus ",
	"AMag" : 5.328,
	"key" : 79463,
	"title" : "E Centauri"
	},
{
	"Index" : "59529",
	"Description" : "Delta Centauri (\u03B4 Cen, \u03B4 Centauri) is a star in the southern constellation of Centaurus. The apparent visual magnitude of this star is +2.57, making it readily visible to the naked eye. Based upon parallax measurements, it is located at a distance of about 410 light-years (130 parsecs) from the Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Delta Centauri, HIP 59196, SAO 239689, HD 105435, GC 16584, HR 4621, DM CD-50  6697, TYC 8241-3235-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Delta Centauri",
	"OType" : "Be Star",
	"Distance" : "126.78",
	"RA_S" : 182.08963142,
	"DEC_S" : -50.72242738,
	"X" : 481,
	"Y" : 316,
	"Constellation" : "Centaurus ",
	"AMag" : 2.515,
	"key" : 79529,
	"title" : "Delta Centauri"
	},
{
	"Index" : "55181",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 59232, SAO 223242, HD 105521, GC 16593, HR 4625, DM CD-40 7128, TYC 7759-1305-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4625",
	"OType" : "Be Star",
	"Distance" : "479.25",
	"RA_S" : 182.22745412,
	"DEC_S" : -41.23160479,
	"Constellation" : "Centaurus ",
	"AMag" : 5.483,
	"key" : 75181,
	"title" : "HR 4625"
	},
{
	"Index" : "59547",
	"Description" : "Rho Centauri (\u03C1 Cen, \u03C1 Centauri) is a star in the southern constellation of Centaurus. \u03C1 Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +3.98. It is approximately 380 light years from Earth.\r\rThis star is a proper motion member of the Lower-Centaurus Crux sub-group in the Scorpius-Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Rho Centauri, HIP 59449, SAO 239737, HD 105937, GC 16651, HR 4638, DM CD-51  6455, TYC 8242-3478-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Rho Centauri",
	"OType" : "Star",
	"Distance" : "115.07",
	"RA_S" : 182.91297782,
	"DEC_S" : -52.36845068,
	"X" : 470,
	"Y" : 336,
	"Constellation" : "Centaurus ",
	"AMag" : 3.918,
	"key" : 79547,
	"title" : "Rho Centauri"
	},
{
	"Index" : "63466",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "F Centauri, HIP 60059, SAO 239838, HD 107079, GC 16792, HR 4682, DM CP-54  5113, TYC 8637-1766-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "F Centauri",
	"OType" : "Variable Star",
	"Distance" : "149.93",
	"RA_S" : 184.74897505,
	"DEC_S" : -55.14300541,
	"Constellation" : "Centaurus ",
	"AMag" : 5.195,
	"key" : 83466,
	"title" : "F Centauri"
	},
{
	"Index" : "50710",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "x01 Centauri, HIP 60449, SAO 203420, HD 107832, GC 16892, HR 4712, DM CD-34  8117, TYC 7241-1795-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "x01 Centauri",
	"OType" : "Star",
	"Distance" : "136.03",
	"RA_S" : 185.89758473,
	"DEC_S" : -35.41267857,
	"Constellation" : "Centaurus ",
	"AMag" : 5.3,
	"key" : 70710,
	"title" : "x01 Centauri"
	},
{
	"Index" : "59554",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "G Centauri, HIP 60710, SAO 239948, HD 108257, GC 16954, HR 4732, DM CD-50  6975, TYC 8243-3043-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "G Centauri",
	"OType" : "Star",
	"Distance" : "137.21",
	"RA_S" : 186.63233084,
	"DEC_S" : -51.4506369,
	"Constellation" : "Centaurus ",
	"AMag" : 4.783,
	"key" : 79554,
	"title" : "G Centauri"
	},
{
	"Index" : "59503",
	"Description" : "Sigma Centauri (\u03C3 Cen, \u03C3 Centauri) is a star in the constellation Centaurus. \u03C3 Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +3.91. It is approximately 412 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Sigma Centauri, HIP 60823, SAO 223454, HD 108483, GC 16990, HR 4743, DM CD-49  7115, TYC 8239-2420-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Sigma Centauri",
	"OType" : "Double or multiple star",
	"Distance" : "126.2",
	"RA_S" : 187.00992401,
	"DEC_S" : -50.23063622,
	"X" : 442,
	"Y" : 303,
	"Constellation" : "Centaurus ",
	"AMag" : 3.864,
	"key" : 79503,
	"title" : "Sigma Centauri"
	},
{
	"Index" : "55170",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "u Centauri, HIP 60855, SAO 203508, HD 108541, GC 17001, HR 4748, DM CD-38  7753, TYC 7757-2015-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "u Centauri",
	"OType" : "Star",
	"Distance" : "133.68",
	"RA_S" : 187.09360963,
	"DEC_S" : -39.04116998,
	"Constellation" : "Centaurus ",
	"AMag" : 5.429,
	"key" : 75170,
	"title" : "u Centauri"
	},
{
	"Index" : "55206",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 61468, SAO 223542, HD 109536, GC 17158, HR 4794, DM CD-40 7376, TYC 7762-1974-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4794",
	"OType" : "Star",
	"Distance" : "35.52",
	"RA_S" : 188.93971287,
	"DEC_S" : -41.02194433,
	"Constellation" : "Centaurus ",
	"AMag" : 5.143,
	"key" : 75206,
	"title" : "HR 4794"
	},
{
	"Index" : "59483",
	"Description" : "Tau Centauri (\u03C4 Cen, \u03C4 Centauri) is a star in the constellation Centaurus. It is a white A-type main sequence dwarf with an apparent magnitude of +3.85 and is approximately 131 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Tau Centauri, HIP 61622, SAO 223560, HD 109787, GC 17194, HR 4802, DM CD-47  7745, TYC 8236-3158-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Tau Centauri",
	"OType" : "High proper-motion Star",
	"Distance" : "40.22",
	"RA_S" : 189.42568602,
	"DEC_S" : -48.54130499,
	"X" : 425,
	"Y" : 279,
	"Constellation" : "Centaurus ",
	"AMag" : 3.848,
	"key" : 79483,
	"title" : "Tau Centauri"
	},
{
	"Index" : "55207",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "l Centauri, HIP 61789, SAO 203681, HD 110073, GC 17236, HR 4817, DM CD-39  7748, TYC 7762-1975-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "l Centauri",
	"OType" : "Star",
	"Distance" : "111.76",
	"RA_S" : 189.96887239,
	"DEC_S" : -39.98730167,
	"Constellation" : "Centaurus ",
	"AMag" : 4.613,
	"key" : 75207,
	"title" : "l Centauri"
	},
{
	"Index" : "59514",
	"Description" : "Gamma Centauri (\u03B3 Cen, \u03B3 Centauri) is a star in the southern constellation Centaurus. It has the proper name Muhlifain, not to be confused with Muliphein, which is \u03B3 Canis Majoris; both names derive from the same Arabic root.\r\rGamma Centauri is a double star located about 130 light-years (40 parsecs) from Earth. The combined apparent visual magnitude of the pair is +2.17, although individually they are third magnitude stars. The stellar classification of the pair is A1IV+, suggesting they are A-type subgiant stars in the process of becoming giants. Individually, their stellar classifications are sometimes listed as A0III, which would mean they have already become giants.\r\rIn 2000, the pair had an angular separation of 1.217 arcseconds with a position angle of 351.9\u00B0. Their positions have been observed since 1897, which is long enough to estimate an orbital period of 84.5 years and a semimajor axis of 0.93 arcseconds. At the distance of this system, this is equivalent to a linear distance of about 93 Astronomical Units. The star Tau Centauri is relatively close to Gamma Centauri, with an estimated separation of 1.72 light-years (0.53 pc).",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Gamma Centauri, HIP 61932B, SAO 223603, HD 110304, GC 17262, HR 4819, DM CD-48  7597, TYC 8240-2724-2",
	"group" : { "key" : "Centaurus" },
	"Common" : "Muhlifain",
	"OType" : "Star",
	"Distance" : "39.9",
	"RA_S" : 190.3792717,
	"DEC_S" : -48.95975694,
	"X" : 416,
	"Y" : 284,
	"Constellation" : "Centaurus ",
	"AMag" : 2.881,
	"key" : 79514,
	"title" : "Muhlifain"
	},
{
	"Index" : "59511",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "w Centauri, HIP 62012, SAO 223614, HD 110458, GC 17282, HR 4831, DM CD-48  7608, TYC 8240-2722-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "w Centauri",
	"OType" : "Star",
	"Distance" : "58.43",
	"RA_S" : 190.64771473,
	"DEC_S" : -48.81310586,
	"Constellation" : "Centaurus ",
	"AMag" : 4.77,
	"key" : 79511,
	"title" : "w Centauri"
	},
{
	"Index" : "50800",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "p Centauri, HIP 62683, SAO 203863, HD 111597, GC 17433, HR 4874, DM CD-33  8653, TYC 7256-1650-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "p Centauri",
	"OType" : "Star",
	"Distance" : "121.95",
	"RA_S" : 192.67152716,
	"DEC_S" : -33.99930731,
	"Constellation" : "Centaurus ",
	"AMag" : 4.889,
	"key" : 70800,
	"title" : "p Centauri"
	},
{
	"Index" : "59636",
	"Description" : "HD 111915, also known by the Bayer designation e Centauri (e Cen), is a star in the constellation Centaurus.\r\re Centauri is an orange K-type giant with an apparent magnitude of +4.33. It is approximately 294 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "e Centauri, HIP 62867, SAO 223731, HD 111915, GC 17473, HR 4888, DM CD-48  7753, TYC 8253-1778-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 111915",
	"OType" : "Star",
	"Distance" : "90.22",
	"RA_S" : 193.27877435,
	"DEC_S" : -48.94331067,
	"X" : 391,
	"Y" : 281,
	"Constellation" : "Centaurus ",
	"AMag" : 4.475,
	"key" : 79636,
	"title" : "HD 111915"
	},
{
	"Index" : "55295",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "n Centauri, HIP 62896, SAO 203907, HD 111968, GC 17489, HR 4889, DM CD-39  7893, TYC 7776-1664-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 488.1",
	"OType" : "Star",
	"Distance" : "45.55",
	"RA_S" : 193.35915723,
	"DEC_S" : -40.17886835,
	"X" : 397,
	"Y" : 168,
	"Constellation" : "Centaurus ",
	"AMag" : 4.276,
	"key" : 75295,
	"title" : "Gliese 488.1"
	},
{
	"Index" : "59673",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "H Centauri, HIP 63210, SAO 240407, HD 112409, GC 17569, HR 4913, DM CD-50  7394, TYC 8258-1469-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "H Centauri",
	"OType" : "Pulsating variable Star",
	"Distance" : "112.87",
	"RA_S" : 194.26814334,
	"DEC_S" : -51.19875254,
	"Constellation" : "Centaurus ",
	"AMag" : 5.148,
	"key" : 79673,
	"title" : "H Centauri"
	},
{
	"Index" : "59643",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Xi01 Centauri, HIP 63724, SAO 223870, HD 113314, GC 17704, HR 4933, DM CD-48  7887, TYC 8254-2207-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Xi01 Centauri",
	"OType" : "Star",
	"Distance" : "67.59",
	"RA_S" : 195.88877792,
	"DEC_S" : -49.5272638,
	"Constellation" : "Centaurus ",
	"AMag" : 4.828,
	"key" : 79643,
	"title" : "Xi01 Centauri"
	},
{
	"Index" : "59613",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "f Centauri, HIP 63945, SAO 223900, HD 113703, GC 17750, HR 4940, DM CD-47  8088, TYC 8250-3266-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "f Centauri",
	"OType" : "Star",
	"Distance" : "119.51",
	"RA_S" : 196.56959425,
	"DEC_S" : -48.46329751,
	"Constellation" : "Centaurus ",
	"AMag" : 4.669,
	"key" : 79613,
	"title" : "f Centauri"
	},
{
	"Index" : "59644",
	"Description" : "Xi2 Centauri (\u03BE2 Cen, \u03BE2 Centauri) is a double star in the constellation Centaurus. It is approximately 470 light years from Earth.\r\rThe primary component, \u03BE2 Centauri A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.27. Its companion, \u03BE2 Centauri B, is a tenth magnitude yellow-white F-type dwarf. The two stars share a common proper motion, indicating they may be gravitationally bound.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Xi02 Centauri, HIP 64004, SAO 223909, HD 113791, GC 17773, HR 4942, DM CD-49  7644, TYC 8254-2208-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Xi2 Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "143.06",
	"RA_S" : 196.72766418,
	"DEC_S" : -49.90624735,
	"X" : 361,
	"Y" : 293,
	"Constellation" : "Centaurus ",
	"AMag" : 4.228,
	"key" : 79644,
	"title" : "Xi2 Centauri"
	},
{
	"Index" : "55363",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 64348, SAO 223966, HD 114474, GC 17850, HR 4973, DM CD-42 8175, TYC 7786-2675-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4973",
	"OType" : "Star",
	"Distance" : "68.13",
	"RA_S" : 197.84673584,
	"DEC_S" : -43.36855809,
	"Constellation" : "Centaurus ",
	"AMag" : 5.348,
	"key" : 75363,
	"title" : "HR 4973"
	},
{
	"Index" : "55282",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 64408, SAO 204227, HD 114613, GC 17869, HR 4979, DM CD-37 8437, TYC 7774-1925-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 501.2 (HR 4979)",
	"OType" : "Star",
	"Distance" : "20.67",
	"RA_S" : 198.01327123,
	"DEC_S" : -37.80302414,
	"Constellation" : "Centaurus ",
	"AMag" : 4.922,
	"key" : 75282,
	"title" : "Gliese 501.2 (HR 4979)"
	},
{
	"Index" : "63738",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 64425, SAO 240645, HD 114529, GC 17866, HR 4975, DM CP-59 4815, TYC 8661-2284-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 4975",
	"OType" : "Ellipsoidal variable Star",
	"Distance" : "115.03",
	"RA_S" : 198.0732832,
	"DEC_S" : -59.9205756,
	"Constellation" : "Centaurus ",
	"AMag" : 4.578,
	"key" : 83738,
	"title" : "HR 4975"
	},
{
	"Index" : "63737",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 64583, SAO 240666, HD 114837A, HR 4989, DM CP-58 4740, TYC 8661-2282-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Gliese 503 (HR 4989)",
	"OType" : "Star",
	"Distance" : "18.2",
	"RA_S" : 198.564221,
	"DEC_S" : -59.102883,
	"Constellation" : "Centaurus ",
	"AMag" : 4.963,
	"key" : 83737,
	"title" : "Gliese 503 (HR 4989)"
	},
{
	"Index" : "50844",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "r Centauri, HIP 64803, SAO 204312, HD 115310, GC 17968, HR 5006, DM CD-30 10457, TYC 7263-2070-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "r Centauri",
	"OType" : "Red Giant Branch star",
	"Distance" : "78.94",
	"RA_S" : 199.22139518,
	"DEC_S" : -31.50619715,
	"Constellation" : "Centaurus ",
	"AMag" : 5.216,
	"key" : 70844,
	"title" : "r Centauri"
	},
{
	"Index" : "50918",
	"Description" : "Iota Centauri (\u03B9 Cen, \u03B9 Centauri) is a star in the southern constellation of Centaurus. It carries the rarely applied traditional name Alhakim (\u0022The Wise One\u0022), dervived from the Arabic title Kentaurus al-Hakeem (\u0642\u0646\u0637\u0648\u0631\u0633 \u0627\u0644\u062D\u0643\u064A\u0645), meaning \u0022The Wise Centaur\u0022. Based upon parallax measurements, it lies at a distance of approximately 58.6 light-years (18.0 parsecs) from Earth. Iota Centauri has an apparent visual magnitude of +2.73, making it easily visible to the naked eye.\r\rIn Chinese, \u67F1 (Zh\u01D4), meaning Pillars, refers to an asterism consisting of \u03B9 Centauri, \u03C52 Centauri, \u03C51 Centauri, a Centauri, \u03C8 Centauri, 4 Centauri, 3 Centauri and 1 Centauri. Consequently, \u03B9 Centauri itself is known as \u67F1\u5341\u4E00 (Zh\u01D4 sh\u00EDy\u012B, English: the Eleventh Star of Pillars.)\r\rThe spectrum of \u03B9 Centauri matches a stellar classification of A2 V. It is an A-type main sequence star that is generating energy by the nuclear fusion of hydrogen in its core region. This energy is being radiated from the outer envelope of the star at an effective temperature of 8,600 K, giving the star a white hue. It has about 2.5 times the Sun\u0027s mass and is roughly 350 million years old. The abundance of elements other than hydrogen and helium, what astronomers term the metallicity, is only 35% of the abundance in the Sun. A weak magnetic field has been tentatively identified with a strength of \u221277 \u00B1 30 G.\r\rThis star has an excess emission of infrared indicating it is surrounded by a circumstellar disk of dust, known as a debris disk. The disk is located within an orbital radius of six Astronomical Units from the star. The dust is unusually luminous for a star this age, suggesting that some process may have recently increased the amount of debris, such as collisions between planetesimals. Alternatively, the planetesimals in this system may have unusual physical properties. As of 2011, a search for planets in this system has thus far been unsuccessful.\r\rIota Centauri appears to belong to the stellar stellar kinematic group known as IC 2391. This is a group of around 16 co-moving stars that most likely originated in the same molecular cloud at least 45 million years ago.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Iota Centauri, HIP 65109, SAO 204371, HD 115892, GC 18039, HR 5028, DM CD-36  8497, TYC 7275-2074-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Alhakim",
	"OType" : "High proper-motion Star",
	"Distance" : "18.02",
	"RA_S" : 200.14923763,
	"DEC_S" : -36.71229344,
	"X" : 327,
	"Y" : 122,
	"Constellation" : "Centaurus ",
	"AMag" : 2.732,
	"key" : 70918,
	"title" : "Alhakim"
	},
{
	"Index" : "63748",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 65112, SAO 240762, HD 115823, GC 18034, HR 5026, DM CP-52 6405, TYC 8662-1710-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5026",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "125.06",
	"RA_S" : 200.15760346,
	"DEC_S" : -52.74782513,
	"Constellation" : "Centaurus ",
	"AMag" : 5.423,
	"key" : 83748,
	"title" : "HR 5026"
	},
{
	"Index" : "66969",
	"Description" : "J Centauri (J Cen) is a star in the constellation Centaurus. It is approximately 350 light years from Earth.\r\rJ Centauri is a spectral class B3V main sequence star with a mean apparent magnitude of 4.5 and a luminosity 500 times that of the Sun. The temperature of the star\u0027s photosphere is nearly 24,000 K. The rotation velocity at the equator is at least 223 km/s. It is believed to be a binary star system.\r\rThis star may be a member of the Scorpio-Centaurus OB association (Sco OB2). This is one of the nearest regions of recent star formation.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "J Centauri, HIP 65271, SAO 252284, HD 116087, GC 18087, HR 5035, DM CD-60  4640, TYC 8990-3680-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "J Centauri",
	"OType" : "Double or multiple star",
	"Distance" : "108.63",
	"RA_S" : 200.65807557,
	"DEC_S" : -60.98840339,
	"X" : 335,
	"Y" : 437,
	"Constellation" : "Centaurus ",
	"AMag" : 4.487,
	"key" : 86969,
	"title" : "J Centauri"
	},
{
	"Index" : "67063",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "m Centauri, HIP 65387, SAO 252293, HD 116243, GC 18107, HR 5041, DM CP-63  2732, TYC 8998-3189-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "m Centauri",
	"OType" : "Star",
	"Distance" : "79.78",
	"RA_S" : 201.00201286,
	"DEC_S" : -64.53566699,
	"Constellation" : "Centaurus ",
	"AMag" : 4.619,
	"key" : 87063,
	"title" : "m Centauri"
	},
{
	"Index" : "67062",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 65479, SAO 252304, HD 116457, GC 18132, HR 5048, DM CP-63 2743, TYC 8998-3188-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5048",
	"OType" : "Star",
	"Distance" : "39.2",
	"RA_S" : 201.30802908,
	"DEC_S" : -64.48514651,
	"Constellation" : "Centaurus ",
	"AMag" : 5.359,
	"key" : 87062,
	"title" : "HR 5048"
	},
{
	"Index" : "55400",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 65535, SAO 204465, HD 116713, GC 18153, HR 5058, DM CD-39 8246, TYC 7791-2183-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5058",
	"OType" : "Peculiar Star",
	"Distance" : "62.24",
	"RA_S" : 201.53241224,
	"DEC_S" : -39.75509201,
	"Constellation" : "Centaurus ",
	"AMag" : 5.245,
	"key" : 75400,
	"title" : "HR 5058"
	},
{
	"Index" : "59694",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "K Centauri, HIP 65810, SAO 240883, HD 117150, GC 18220, HR 5071, DM CD-50  7812, TYC 8260-2661-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "K Centauri",
	"OType" : "Star",
	"Distance" : "155.17",
	"RA_S" : 202.35522565,
	"DEC_S" : -51.16513641,
	"Constellation" : "Centaurus ",
	"AMag" : 5.037,
	"key" : 79694,
	"title" : "K Centauri"
	},
{
	"Index" : "55406",
	"Description" : "HD 117440, also known by its Bayer designation d Centauri (d Cen), is a binary star in the constellation Centaurus. It is approximately 900 light years from Earth.\r\rBoth components are yellow G-type giant stars. The primary, d Centauri A, has an apparent magnitude of +4.5, while the secondary, d Centauri B, has an apparent magnitude of +4.7. The two stars orbit around their common centre of mass once every 78.7 years and the secondary has a semi-major axis of 0.165 arcseconds.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "d Centauri, HIP 65936AB, SAO 204545, HD 117440, GC 18254, HR 5089, DM CD-38  8592, TYC 7792-2393-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 117440",
	"OType" : "Star",
	"Distance" : "271.74",
	"RA_S" : 202.76107277,
	"DEC_S" : -39.40730757,
	"X" : 302,
	"Y" : 158,
	"Constellation" : "Centaurus ",
	"AMag" : 4.027,
	"key" : 75406,
	"title" : "HD 117440"
	},
{
	"Index" : "63806",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Q Centauri, HIP 66821A, SAO 241076, HD 118991A, GC 18495, HR 5141, DM CP-53  5725, TYC 8667-432-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Q Centauri",
	"OType" : "Star",
	"Distance" : "82.87",
	"RA_S" : 205.43651256,
	"DEC_S" : -54.55937774,
	"Constellation" : "Centaurus ",
	"AMag" : 5.204,
	"key" : 83806,
	"title" : "Q Centauri"
	},
{
	"Index" : "63885",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 66849, SAO 241080, HD 118978, GC 18500, HR 5140, DM CP-58 5059, TYC 8675-3299-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5140",
	"OType" : "Star",
	"Distance" : "234.55",
	"RA_S" : 205.50453936,
	"DEC_S" : -58.78707588,
	"Constellation" : "Centaurus ",
	"AMag" : 5.366,
	"key" : 83885,
	"title" : "HR 5140"
	},
{
	"Index" : "50876",
	"Description" : "1 Centauri is a star in the constellation Centaurus.\r\r1 Centauri is a yellow-white F-type subgiant with an apparent magnitude of +4.23. It is approximately 63 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "1 Centauri, i Centauri, HIP 67153, SAO 204812, HD 119756, GC 18593, HR 5168, DM CD-32  9603, TYC 7270-2399-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "1 Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "19.4",
	"RA_S" : 206.42185669,
	"DEC_S" : -33.04372296,
	"X" : 257,
	"Y" : 79,
	"Constellation" : "Centaurus ",
	"AMag" : 4.272,
	"key" : 70876,
	"title" : "1 Centauri"
	},
{
	"Index" : "59849",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "M Centauri, HIP 67234, SAO 241157, HD 119834, GC 18607, HR 5172, DM CD-50  8017, TYC 8274-2554-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "M Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "80.37",
	"RA_S" : 206.66408134,
	"DEC_S" : -51.43276374,
	"Constellation" : "Centaurus ",
	"AMag" : 4.738,
	"key" : 79849,
	"title" : "M Centauri"
	},
{
	"Index" : "50936",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "z Centauri, HIP 67244, SAO 204835, HD 119921, GC 18618, HR 5174, DM CD-35  8995, TYC 7278-2043-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "z Centauri",
	"OType" : "Star",
	"Distance" : "133.63",
	"RA_S" : 206.73480417,
	"DEC_S" : -36.25193049,
	"Constellation" : "Centaurus ",
	"AMag" : 5.145,
	"key" : 70936,
	"title" : "z Centauri"
	},
{
	"Index" : "51008",
	"Description" : "2 Centauri is a star in the constellation Centaurus.\r\r2 Centauri is a M-type red giant with a mean apparent magnitude of +4.19. It is approximately 183 light years from Earth. It is classified as a semiregular variable star and its brightness varies from magnitude +4.16 to +4.26 with a period of 12. days.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "2 Centauri, g Centauri, HIP 67457, SAO 204875, HD 120323, GC 18666, HR 5192, DM CD-33  9358, TYC 7287-1891-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "2 Centauri",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "56.11",
	"RA_S" : 207.36133376,
	"DEC_S" : -34.45077493,
	"X" : 249,
	"Y" : 99,
	"Constellation" : "Centaurus ",
	"AMag" : 4.416,
	"key" : 71008,
	"title" : "2 Centauri"
	},
{
	"Index" : "55450",
	"Description" : "Nu Centauri (\u03BD Cen, \u03BD Centauri) is a binary star system in the southern constellation of Centaurus. The combined apparent visual magnitude of the pair is +3.41, making this one of the brightest members of the constellation. Based upon parallax measurements made during the Hipparcos mission, this star system is located at a distance of roughly 437 light-years (134 parsecs) from Earth. The margin of error for this distance is about 2%, which is enough to give an error in distance of \u00B110 light years.\r\rThis is a single-lined spectroscopic binary system, which means that the two stellar components have not been individually resolved with a telescope. Instead, their orbital motion can be tracked through periodic shifts in the spectrum of the primary. The gravitational perturbation of the hidden secondary component upon the primary is causing the latter to first move toward and then away from the Earth, creating Doppler shift changes in the spectrum. From these subtle shifts, the orbital elements of the pair can be extracted. The pair are orbiting their common center of mass in a circular orbit with a period of only 2.622 days, indicating that they are in a relatively tight orbit.\r\rThe interaction between the two components of this system appears to be creating emission lines in the spectrum, turning the primary into a Be star. It has a stellar classification of B2 IV, which matches a massive B-type subgiant star. The primary has 8.5 times the mass of the Sun and 6.4 times the Sun\u0027s radius. It is a Beta Cephei type variable star with a brightness that periodically varies from magnitude +3.38 to +3.41 over an interval of 0.17 days. The tidal interaction with the secondary component has turned it into a rotating ellipsoidal variable.\r\rThis star system is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Nu Centauri, HIP 67464, SAO 224469, HD 120307, GC 18665, HR 5190, DM CD-41  8171, TYC 7797-2744-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Nu Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "133.79",
	"RA_S" : 207.37615861,
	"DEC_S" : -41.68770854,
	"X" : 259,
	"Y" : 192,
	"Constellation" : "Centaurus ",
	"AMag" : 3.352,
	"key" : 75450,
	"title" : "Nu Centauri"
	},
{
	"Index" : "55449",
	"Description" : "Mu Centauri (\u03BC Cen, \u03BC Centauri) is a third-magnitude star in the southern constellation of Centaurus. With the stars \u03BD and \u03C6 Centauri, it marks what has been traditionally portrayed as \u0022dextro Latere\u0022 (the right side) of the Centaur. The apparent visual magnitude of this star is 3.42, making it one of the brighter members of the constellation. The distance to this star can be estimated directly using parallax measurements, which yield a value of roughly 510 light years (155 parsecs) from Earth.\r\rThe spectrum of Mu Centauri matches a stellar classification of B2 IV-Ve. The \u0027e\u0027 suffix is used to mark the presence of emission lines, which indicates this is a Be star surrounded by a circumstellar disk of hot gas that was formed from material ejected from the star. Mu Centauri is a pulsating variable star that has multiple non-radial cycles with a primary period of 0.503 days. Three other pulsation cycles have a similar period, while two have a shorter interval of about 0.28 days. It undergoes outburst events that result in the transfer of additional material to the surrounding disk. During these outbursts, the star can experience transient periodicities. Mu Centauri is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +2.75 to +3.25.\r\rThis star is spinning rapidly, with a projected rotational velocity of 194, km s\u20131 and is completing a full rotation in about 11.615 hours. The equatorial azimuthal velocity is around 85% of the critical velocity where the star would start to break up, resulting a pronounced equatorial bulge that is about 26% wider than the radius at the poles. Because of the oblate spheroidal shape of this star, the polar region is at a higher temperature than the equator\u201423,000 K versus 17,600 K respectively. Likewise, the gravitational force at the poles is greater than along the equator. The axis of rotation of the star is tilted by an angle of about (19 \u00B1 3)\u00B0 to the line of sight from the Earth.\r\rAt an estimated age of nearly 20 million years, this star is around 55\u201365% of the way through its evolutionary period on the main sequence of core hydrogen burning stars. It has around nine times the mass of the Sun and four times the Sun\u0027s radius, but emits over 2,000 times as much energy as the Sun. The outer atmosphere has a mean effective temperature of 22,410 K, giving the star a blue-white hue.\r\rThis star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Mu Centauri, HIP 67472, SAO 224471, HD 120324, GC 18667, HR 5193, DM CD-41  8172, TYC 7797-2743-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Mu Centauri",
	"OType" : "Be Star",
	"Distance" : "154.92",
	"RA_S" : 207.40411849,
	"DEC_S" : -42.47373038,
	"X" : 260,
	"Y" : 202,
	"Constellation" : "Centaurus ",
	"AMag" : 3.415,
	"key" : 75449,
	"title" : "Mu Centauri"
	},
{
	"Index" : "50985",
	"Description" : "3 Centauri is a binary star in the constellation Centaurus. It is approximately 340 light years from Earth.\r\rThe primary component, 3 Centauri A, is a blue-white B-type giant with a mean apparent magnitude of +4.56. It is a variable star, and its brightness varies from magnitude +4.27 to +4.32 It is suspected the variations in luminosity are a result of the primary being an eclipsing binary, which would mean the system would consist of at least three objects. Its more distant companion, 3 Centauri B, is located 7.9 arcseconds away. It is a blue-white B-type main sequence dwarf and has an apparent magnitude of +6.06.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "3 Centauri, HIP 67669A, TYC 7283-2100-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "3 Centauri",
	"OType" : "Star",
	"Distance" : "90.54",
	"RA_S" : 207.95657568,
	"DEC_S" : -32.99406889,
	"X" : 240,
	"Y" : 80,
	"Constellation" : "Centaurus ",
	"AMag" : 4.497,
	"key" : 70985,
	"title" : "3 Centauri"
	},
{
	"Index" : "50986",
	"Description" : "3 Centauri is a binary star in the constellation Centaurus. It is approximately 340 light years from Earth.\r\rThe primary component, 3 Centauri A, is a blue-white B-type giant with a mean apparent magnitude of +4.56. It is a variable star, and its brightness varies from magnitude +4.27 to +4.32 It is suspected the variations in luminosity are a result of the primary being an eclipsing binary, which would mean the system would consist of at least three objects. Its more distant companion, 3 Centauri B, is located 7.9 arcseconds away. It is a blue-white B-type main sequence dwarf and has an apparent magnitude of +6.06.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "3 Centauri, k Centauri, HIP 67669B, SAO 204916, HD 120709, GC 18724, HR 5210, DM CD-32  9676A, TYC 7283-2101-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "3 Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "90.54",
	"RA_S" : 207.95667234,
	"DEC_S" : -32.99408521,
	"X" : 240,
	"Y" : 80,
	"Constellation" : "Centaurus ",
	"AMag" : 4.32,
	"key" : 70986,
	"title" : "3 Centauri"
	},
{
	"Index" : "63774",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "N Centauri, HIP 67703A, SAO 241239, HD 120642, GC 18720, HR 5207, DM CP-52  6787A, TYC 8664-669-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "N Centauri",
	"OType" : "Star",
	"Distance" : "79.3",
	"RA_S" : 208.02026814,
	"DEC_S" : -52.81153174,
	"Constellation" : "Centaurus ",
	"AMag" : 5.242,
	"key" : 83774,
	"title" : "N Centauri"
	},
{
	"Index" : "50984",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "4 Centauri, h Centauri, HIP 67786A, SAO 204944, HD 120955, GC 18755, HR 5221, DM CD-31 10729, TYC 7283-2099-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "h Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "191.03",
	"RA_S" : 208.30225363,
	"DEC_S" : -31.9276129,
	"Constellation" : "Centaurus ",
	"AMag" : 4.717,
	"key" : 70984,
	"title" : "h Centauri"
	},
{
	"Index" : "59778",
	"Description" : "Zeta Centauri (\u03B6 Centauri, \u03B6 Cen) is a binary star system in the southern constellation of Centaurus. It has the proper name Alnair, from the scientific-Arabic Nayyir Badan Qan\u1E6D\u016Bris (\u0623\u0644\u0646\u0627\u064A\u0631 \u0623\u0644\u0628\u0637\u0646 \u0623\u0644\u0642\u0646\u062A\u0648\u0631\u0633), meaning \u0022The Bright (Star) of the Body of the Centaur\u0022. With a combined apparent visual magnitude of +2.55, it is one of the brighter members of the constellation. This system is close enough to the Earth that its distance can be measured directly using the parallax technique. This yields a value of roughly 382 light-years (117 parsecs), with a 1.6% margin of error.\r\rIn Chinese, \u5EAB\u6A13 (K\u00F9 L\u00F3u), meaning Arsenal, refers to an asterism consisting of \u03B6 Centauri, \u03B7 Centauri, \u03B8 Centauri, 2 Centauri, HD 117440, \u03BE1 Centauri, \u03B3 Centauri, \u03C4 Centauri, D Centauri and \u03C3 Centauri. Consequently, \u03B6 Centauri itself is known as \u5EAB\u6A13\u4E00 (K\u00F9 L\u00F3u y\u012B, English: the First Star of Arsenal.)\r\r\u03B6 Cen is a double-lined spectroscopic binary system, which indicates that the orbital motion was detected by shifts in the absorption lines of their combined spectra caused by the Doppler effect. The two stars orbit each other over a period of slightly more than eight days with an orbital eccentricity of about 0.5. The estimated angular separation of the pair is 1.4 mas.\r\rAt an estimated age of 40 million years, the primary component of this system appears to be in the subgiant stage of its evolution with a stellar classification of B2.5 IV. It is a large star with nearly 8 times the mass of the Sun and close to 6 times the Sun\u0027s radius. This star is rotating rapidly with a projected rotational velocity of 235 km s\u20131.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Zeta Centauri, HIP 68002, SAO 224538, HD 121263, GC 18809, HR 5231, DM CD-46  8949, TYC 8267-3545-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Alnair",
	"OType" : "Spectroscopic binary",
	"Distance" : "117.06",
	"RA_S" : 208.8849402,
	"DEC_S" : -47.28837451,
	"X" : 255,
	"Y" : 266,
	"Constellation" : "Centaurus ",
	"AMag" : 2.497,
	"key" : 79778,
	"title" : "Alnair"
	},
{
	"Index" : "67198",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 68191, SAO 252531, HD 121474, GC 18845, HR 5241, DM CP-63 3070, TYC 9008-4454-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5241",
	"OType" : "Star",
	"Distance" : "64.24",
	"RA_S" : 209.41201595,
	"DEC_S" : -63.68669457,
	"Constellation" : "Centaurus ",
	"AMag" : 4.824,
	"key" : 87198,
	"title" : "HR 5241"
	},
{
	"Index" : "55456",
	"Description" : "Phi Centauri (\u03C6 Cen, \u03C6 Centauri) is a star in the constellation Centaurus. \u03C6 Centauri is a blue-white B-type subgiant with an apparent magnitude of +3.83. It is approximately 530 light years from Earth.\r\rThis star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Phi Centauri, HIP 68245, SAO 224577, HD 121743, GC 18874, HR 5248, DM CD-41  8329, TYC 7798-2848-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Phi Centauri",
	"OType" : "Variable Star",
	"Distance" : "160.89",
	"RA_S" : 209.5677746,
	"DEC_S" : -42.10075401,
	"X" : 239,
	"Y" : 200,
	"Constellation" : "Centaurus ",
	"AMag" : 3.769,
	"key" : 75456,
	"title" : "Phi Centauri"
	},
{
	"Index" : "55488",
	"Description" : "Upsilon1 Centauri (\u03C51 Cen, \u03C51 Centauri) is the Bayer designation for a star in the constellation Centaurus.\r\r\u03C51 Centauri is a blue-white B-type subgiant with an apparent magnitude of +3.87. It is approximately 427 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Upsilon01 Centauri, HIP 68282, SAO 224585, HD 121790, GC 18883, HR 5249, DM CD-44  9010, TYC 7802-2736-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Upsilon1 Centauri",
	"OType" : "Variable Star",
	"Distance" : "131",
	"RA_S" : 209.66978384,
	"DEC_S" : -44.80358591,
	"X" : 243,
	"Y" : 235,
	"Constellation" : "Centaurus ",
	"AMag" : 3.811,
	"key" : 75488,
	"title" : "Upsilon1 Centauri"
	},
{
	"Index" : "59726",
	"Description" : "Upsilon2 Centauri (\u03C52 Cen, \u03C52 Centauri) is a star in the constellation Centaurus. \u03C52 Centauri is a yellow-white F-type bright giant with an apparent magnitude of +4.34. It is approximately 1300 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Upsilon02 Centauri, HIP 68523, SAO 224621, HD 122223, GC 18939, HR 5260, DM CD-44  9040, TYC 8263-3419-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Upsilon2 Centauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "389.1051",
	"RA_S" : 210.43125759,
	"DEC_S" : -45.60341726,
	"X" : 238,
	"Y" : 247,
	"Constellation" : "Centaurus ",
	"AMag" : 4.405,
	"key" : 79726,
	"title" : "Upsilon2 Centauri"
	},
{
	"Index" : "67147",
	"Description" : "eta Centauri (\u03B2 Cen, \u03B2 Centauri) is a star system in the southern constellation of Centaurus. With an apparent visual magnitude of 0.60, it is the second brightest star in the constellation Centaurus and the tenth brightest star in the night sky. It has the traditional names Hadar and Agena. The name Hadar comes from the Arabic word for \u0022ground / soil / earth\u0022 (from \u0623\u0644 \u0623\u0631\u0636 - al ardh) or \u0022civilization\u0022 (from \u0623\u0644\u062D\u0636\u0627\u0631\u0629 - al hidaara), while the name Agena comes from Latin words for \u0022the knee\u0022. The Chinese name for the star is \u9A6C\u8179\u4E00 (Mandarin: m\u01CE f\u00F9 y\u012B, the First Star of the Horse\u0027s Abdomen).",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Beta Centauri, HIP 68702B, SAO 252582, HD 122451, GC 18971, HR 5267, DM CP-59  5365, TYC 9005-3919-2",
	"group" : { "key" : "Centaurus" },
	"Common" : "Hadar / Agena",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "119.76",
	"RA_S" : 210.95585562,
	"DEC_S" : -60.37303516,
	"X" : 269,
	"Y" : 437,
	"Constellation" : "Centaurus ",
	"AMag" : 0.61,
	"key" : 87147,
	"shortTitle" : "Hadar; Khadar",
	"title" : "Hadar / Agena"
	},
{
	"Index" : "55521",
	"Description" : "Chi Centauri (\u03C7 Cen, \u03C7 Centauri) is a star in the constellation Centaurus.\r\r\u03C7 Centauri is a blue-white B-type main sequence dwarf with a mean apparent magnitude of +4.36. It is approximately 510 light years from Earth. It is classified as a Beta Cephei type variable star and its brightness varies by 0.02 magnitudes with a period of 50.40 minutes.\r\rThis star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Chi Centauri, HIP 68862, SAO 224673, HD 122980, GC 19017, HR 5285, DM CD-40  8405, TYC 7807-2674-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Chi Centauri",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "156.29",
	"RA_S" : 211.51153013,
	"DEC_S" : -41.17963189,
	"X" : 219,
	"Y" : 191,
	"Constellation" : "Centaurus ",
	"AMag" : 4.311,
	"key" : 75521,
	"title" : "Chi Centauri"
	},
{
	"Index" : "63783",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 69191, SAO 241496, HD 123569, GC 19099, HR 5297, DM CP-52 7028, TYC 8665-2921-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5297",
	"OType" : "Star",
	"Distance" : "55.91",
	"RA_S" : 212.47839238,
	"DEC_S" : -53.43894633,
	"Constellation" : "Centaurus ",
	"AMag" : 4.84,
	"key" : 83783,
	"title" : "HR 5297"
	},
{
	"Index" : "63991",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 69618, SAO 241563, HD 124367, GC 19199, HR 5316, DM CP-56 6206, TYC 8686-3021-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5316",
	"OType" : "Be Star",
	"Distance" : "147.49",
	"RA_S" : 213.73807364,
	"DEC_S" : -57.08612682,
	"Constellation" : "Centaurus ",
	"AMag" : 5.032,
	"key" : 83991,
	"title" : "HR 5316"
	},
{
	"Index" : "67162",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 70035, SAO 252703, HD 125158, GC 19302, HR 5349, DM CP-60 5294, TYC 9006-5415-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5349",
	"OType" : "Star",
	"Distance" : "48.34",
	"RA_S" : 214.96459649,
	"DEC_S" : -61.27297145,
	"Constellation" : "Centaurus ",
	"AMag" : 5.242,
	"key" : 87162,
	"title" : "HR 5349"
	},
{
	"Index" : "63990",
	"Description" : "HD 125288 (Bayer designation v Cen / v Centauri) is a star in the constellation Centaurus.\r\rHD 125288 is a blue-white B-type supergiant with an apparent magnitude of +4.30. It is approximately 1230 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "v Centauri, HIP 70069, SAO 241641, HD 125288, GC 19318, HR 5358, DM CP-55  5984, TYC 8686-3020-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 125288",
	"OType" : "Star",
	"Distance" : "373.41",
	"RA_S" : 215.08142783,
	"DEC_S" : -56.38649515,
	"X" : 229,
	"Y" : 392,
	"Constellation" : "Centaurus ",
	"AMag" : 4.347,
	"key" : 83990,
	"title" : "HD 125288"
	},
{
	"Index" : "55508",
	"Description" : "Psi Centauri (\u03C8 Cen, \u03C8 Centauri) is a star in the constellation Centaurus. \u03C8 Centauri is a white A-type subgiant with an apparent magnitude of +4.05. It is approximately 259 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Psi Centauri, HIP 70090, SAO 205453, HD 125473, GC 19337, HR 5367, DM CD-37  9336, TYC 7805-2696-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Psi Centauri",
	"OType" : "Star",
	"Distance" : "79.34",
	"RA_S" : 215.13929774,
	"DEC_S" : -37.88529327,
	"X" : 174,
	"Y" : 157,
	"Constellation" : "Centaurus ",
	"AMag" : 4.029,
	"key" : 75508,
	"title" : "Psi Centauri"
	},
{
	"Index" : "64037",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 70264A, TYC 8690-3219-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5371",
	"OType" : "Star",
	"Distance" : "115.16",
	"RA_S" : 215.65448702,
	"DEC_S" : -58.45911009,
	"Constellation" : "Centaurus ",
	"AMag" : 5.028,
	"key" : 84037,
	"title" : "HR 5371"
	},
{
	"Index" : "55536",
	"Description" : "V761 Centauri (a Centauri) is a star in the constellation Centaurus.\r\rV761 Centauri is a blue-white B-type giant with a mean apparent magnitude of +4.41. It is approximately 460 light years from Earth. It is classified as an SX Arietis type variable star and its brightness varies from magnitude +4.38 to +4.43 with a period of 8.82 days.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "a Centauri, HIP 70300, SAO 205497, HD 125823, GC 19377, HR 5378, DM CD-38  9329, TYC 7809-2783-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "761 Centauri",
	"OType" : "Rotationally variable Star",
	"Distance" : "140.18",
	"RA_S" : 215.75933285,
	"DEC_S" : -39.51181573,
	"X" : 173,
	"Y" : 178,
	"Constellation" : "Centaurus ",
	"AMag" : 4.371,
	"key" : 75536,
	"title" : "761 Centauri"
	},
{
	"Index" : "67174",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Alpha Centauri, HIP 71681B, HD 128621, HR 5460, DM CP-60  5483B, TYC 9007-5848-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Proksima Kentavra",
	"OType" : "High proper-motion Star",
	"Distance" : "1.35",
	"RA_S" : 219.89609629,
	"DEC_S" : -60.83752757,
	"Constellation" : "Centaurus ",
	"AMag" : 1.243,
	"key" : 87174,
	"title" : "Proksima Kentavra"
	},
{
	"Index" : "55613",
	"Description" : "HD 129116, also known by its Bayer designation b Centauri (b Cen), is a star in the constellation Centaurus.\r\rb Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.01. It is approximately 339 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "b Centauri, HIP 71865, SAO 205839, HD 129116, GC 19779, HR 5471, DM CD-37  9618, TYC 7819-2819-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 129116",
	"OType" : "Star",
	"Distance" : "103.91",
	"RA_S" : 220.48996424,
	"DEC_S" : -37.79349398,
	"X" : 108,
	"Y" : 137,
	"Constellation" : "Centaurus ",
	"AMag" : 3.958,
	"key" : 75613,
	"title" : "HD 129116"
	},
{
	"Index" : "51145",
	"Description" : "HD 129456, also known by its Bayer designation c\u00B9 Centauri (c\u00B9 Cen), is a star in the constellation Centaurus. c\u00B9 Centauri is an orange K-type giant with an apparent magnitude of +4.06. It is approximately 209 light years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "c01 Centauri, HIP 72010, SAO 205871, HD 129456, GC 19820, HR 5485, DM CD-34  9868, TYC 7305-2442-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HD 129456",
	"OType" : "High proper-motion Star",
	"Distance" : "64.22",
	"RA_S" : 220.91433358,
	"DEC_S" : -35.1736592,
	"X" : 65,
	"Y" : 50,
	"Constellation" : "Centaurus ",
	"AMag" : 4.201,
	"key" : 71145,
	"title" : "HD 129456"
	},
{
	"Index" : "51146",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "c02 Centauri, HIP 72104, SAO 205899, HD 129685, GC 19845, HR 5489, DM CD-34  9888, TYC 7305-2443-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "c02 Centauri",
	"OType" : "Star",
	"Distance" : "65.69",
	"RA_S" : 221.24667613,
	"DEC_S" : -35.19182826,
	"Constellation" : "Centaurus ",
	"AMag" : 4.924,
	"key" : 71146,
	"title" : "c02 Centauri"
	},
{
	"Index" : "55621",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 72800, SAO 206037, HD 131120, GC 20000, HR 5543, DM CD-37 9760, TYC 7820-3238-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5543",
	"OType" : "Double or multiple star",
	"Distance" : "150.63",
	"RA_S" : 223.21280849,
	"DEC_S" : -37.80316481,
	"Constellation" : "Centaurus ",
	"AMag" : 4.989,
	"key" : 75621,
	"title" : "HR 5543"
	},
{
	"Index" : "51150",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 73049, SAO 206099, HD 131625, GC 20066, HR 5558, DM CD-3310169, TYC 7306-2614-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "HR 5558",
	"OType" : "Star",
	"Distance" : "77.78",
	"RA_S" : 223.93628407,
	"DEC_S" : -33.85578491,
	"Constellation" : "Centaurus ",
	"AMag" : 5.317,
	"key" : 71150,
	"title" : "HR 5558"
	},
{
	"Index" : "55691",
	"Description" : "Kappa Centauri (\u03BA Cen, \u03BA Centauri) is a binary star in the southern constellation of Centaurus. With an apparent visual magnitude of +3.14, it can be viewed with the naked eye on a dark night. Parallax measurements place it at an estimated distance of 380 light-years (120 parsecs) from Earth.\r\rThis is a spectroscopic binary system where the presence of an orbiting companion is revealed by shifts in the absorption lines caused by the Doppler effect. The primary component is a huge star, with about seven times the Sun\u0027s mass and four times the Sun\u0027s radius. It has a stellar classification of B2 IV, indicating that it is in the subgiant stage of its stellar evolution. An effective temperature of 19,800 K in the outer envelope is what gives it the blue-white hue of a B-type star.\r\rThe primary is a candidate Beta Cephei variable that shows line-profile variations in its spectrum. However, the nature of the variability remains uncertain because of the binary nature of the system. As of 2007, the secondary component was separated from the primary by 0.128 arcseconds at a position angle of 156\u00B0. It has about 68% of the mass of the primary. This system is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.\r\rIn Chinese, \u9A0E\u5B98 (Q\u00ED Gu\u0101n), meaning Imperial Guards, refers to an asterism consisting of \u03BA Centauri, \u03B3 Lupi, \u03B4 Lupi, \u03B2 Lupi, \u03BB Lupi, \u03B5 Lupi, \u03BC Lup, \u03C0 Lupi, \u03BF Lupi and \u03B1 Lupi. Consequently, \u03BA Centauri itself is known as \u9A0E\u5B98\u4E09 (Q\u00ED Gu\u0101n s\u0101n, English: the Third Star of Imperial Guards.). From this Chinese name, the name Ke Kwan was appeared.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Kappa Centauri, HIP 73334AC, SAO 225344, HD 132200, GC 20146, HR 5576, DM CD-41  9342, TYC 7828-3520-1",
	"group" : { "key" : "Centaurus" },
	"Common" : "Ke Kwan",
	"OType" : "Variable Star",
	"Distance" : "116.94",
	"RA_S" : 224.79034661,
	"DEC_S" : -42.1042044,
	"X" : 96,
	"Y" : 236,
	"Constellation" : "Centaurus ",
	"AMag" : 3.078,
	"key" : 75691,
	"title" : "Ke Kwan"
	},
{
	"Index" : "30657",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "2 Ursae Minoris, HIP 5372, SAO 181, HD 5848, GC 1288, HR 285, DM BD+85    19, TYC 4623-1236-1",
	"group" : { "backgroundImage" : "images/Alignment/14.png",
		"description" : "Cepheus is a constellation in the northern sky. It is named after Cepheus, King of Aethiopia in Greek mythology. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations.\r\rCepheus was the King of Aethiopia. He was married to Cassiopeia and was the father of Andromeda, both of whom are immortalized as modern day constellations along with Cepheus.",
		"key" : "Cepheus",
		"grouptype" : "Cepheus",
		"Meaning" : "Cepheus (mythological character)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Cepheus",
		"title" : "Cepheus Objects Group" },
	"Common" : "2 Ursae Minoris",
	"OType" : "Star",
	"Distance" : "85.89",
	"RA_S" : 17.18696647,
	"DEC_S" : 86.25709194,
	"Constellation" : "Cepheus ",
	"AMag" : 4.364,
	"key" : 50657,
	"title" : "2 Ursae Minoris"
	},
{
	"Index" : "29759",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 15547, SAO 4875, HD 19978, GC 3912, HR 961, DM BD+77  115, TYC 4513-2820-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 961",
	"OType" : "Variable Star",
	"Distance" : "81.11",
	"RA_S" : 50.08225028,
	"DEC_S" : 77.73475159,
	"Constellation" : "Cepheus ",
	"AMag" : 5.471,
	"key" : 49759,
	"title" : "HR 961"
	},
{
	"Index" : "29808",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 19461AB, SAO 650, HD 25007, HR 1230, DM BD+80  125, TYC 4522-1564-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HD  25007",
	"OType" : "Star",
	"Distance" : "115.8",
	"RA_S" : 62.51181939,
	"DEC_S" : 80.69863086,
	"Constellation" : "Cepheus ",
	"AMag" : 5.264,
	"key" : 49808,
	"title" : "HD  25007"
	},
{
	"Index" : "30610",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 20860AB, SAO 685, HD 26356, GC 5208, HR 1289, DM BD+83  104, TYC 4617-2855-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HD  26356",
	"OType" : "Be Star",
	"Distance" : "229.53",
	"RA_S" : 67.05526515,
	"DEC_S" : 83.80778826,
	"Constellation" : "Cepheus ",
	"AMag" : 5.488,
	"key" : 50610,
	"title" : "HD  26356"
	},
{
	"Index" : "29819",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 23265, SAO 783, HD 30338, GC 5962, HR 1523, DM BD+80  155, TYC 4523-1181-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 1523",
	"OType" : "Star",
	"Distance" : "117.65",
	"RA_S" : 75.08633807,
	"DEC_S" : 81.19408681,
	"Constellation" : "Cepheus ",
	"AMag" : 5.236,
	"key" : 49819,
	"title" : "HR 1523"
	},
{
	"Index" : "30675",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 37391, SAO 1168, HD 51802, GC 9772, HR 2609, DM BD+87   51, TYC 4626-748-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "V* OV Cep",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "139.19",
	"RA_S" : 115.12717047,
	"DEC_S" : 87.02009101,
	"Constellation" : "Cepheus ",
	"AMag" : 5.227,
	"key" : 50675,
	"title" : "V* OV Cep"
	},
{
	"Index" : "30370",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "1 Cephei, Kappa Cephei, HIP 99255A, SAO 9665, HD 192907, GC 28066, HR 7750, DM BD+77   764, TYC 4589-3106-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Kappa Cephei",
	"OType" : "Star",
	"Distance" : "96.43",
	"RA_S" : 302.22229298,
	"DEC_S" : 77.71142163,
	"Constellation" : "Cepheus ",
	"AMag" : 4.391,
	"key" : 50370,
	"title" : "Kappa Cephei"
	},
{
	"Index" : "27446",
	"Description" : "Theta Cephei (\u03B8 Cep, \u03B8 Cephei) is a Class A7, fourth-magnitude star in the constellation Cepheus. Theta Cephei is a white spectroscopic binary star, located about 135 light-years from Earth. Shared with \u03B7 Cep, this star have the title Al Kidr, meaning unknown\r\rIn Chinese, \u5929\u920E (Ti\u0101n G\u014Du), meaning Celestial Hook, refers to an asterism consisting of 4 Cephei, HD 194298, \u03B7 Cephei, \u03B1 Cephei, \u03BE Cephei, 26 Cephei, \u03B9 Cephei and \u03BF Cephei. Consequently, \u03B8 Cephei itself is known as \u5929\u920E\u4E09 (Ti\u0101n G\u014Du s\u0101n, English: the Third Star of Celestial Hook.).",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "2 Cephei, Theta Cephei, HIP 101093, SAO 18897, HD 195725, GC 28541, HR 7850, DM BD+62  1821, TYC 4237-2168-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Al Kidr (Theta)",
	"OType" : "Spectroscopic binary",
	"Distance" : "41.57",
	"RA_S" : 307.39535443,
	"DEC_S" : 62.99410654,
	"X" : 610,
	"Y" : 290,
	"Constellation" : "Cepheus ",
	"AMag" : 4.228,
	"key" : 47446,
	"title" : "Al Kidr (Theta)"
	},
{
	"Index" : "27509",
	"Description" : "Eta Cephei (\u03B7 Cep, \u03B7 Cephei) is a star in the northern circumpolar constellation of Cepheus. It shares the name Al Kidr with \u03B8 Cep, although the meaning of this name is unknown. This star, along with \u03B1 Cep (Alderamin) and \u03B2 Cep (Alfirk), were identified as Al Kaw\u0101kib al Fir\u1E33 (\u0627\u0644\u0643\u0648\u0643\u0628 \u0627\u0644\u0641\u0631\u0642), meaning \u0022the Stars of The Flock\u0022 by Ulug Beg. With an apparent visual magnitude of 3.4, this is a third magnitude star that, according to the Bortle Dark-Sky Scale, is readily visible to the naked eye. Parallax measurements put it at a distance of 46.53 light-years (14.27 parsecs) from Earth.\r\rIn Chinese, \u5929\u920E (Ti\u0101n G\u014Du), meaning Celestial Hook, refers to an asterism consisting of \u03B7 Cephei, 4 Cephei, HD 194298, \u03B8 Cephei, \u03B1 Cephei, \u03BE Cephei, 26 Cephei, \u03B9 Cephei and \u03BF Cephei. Consequently, \u03B7 Cephei itself is known as \u5929\u920E\u56DB (Ti\u0101n G\u014Du s\u00EC, English: the Fourth Star of Celestial Hook.).\r\rEta Cephei is a subgiant star with a stellar classification of K0 IV, which indicates it is exhausting the supply of hydrogen at its core and is in the process of evolving into a giant star. With 1.6 times the Sun\u0027s mass, at an age of 2.5 billion years it has reached a radius four times larger than the Sun and a luminosity ten times greater. It is radiating this energy from its outer atmosphere at an effective temperature of 4,950 K, giving it the orange-hued glow of a K-type star. Eta Cephei has a high proper motion across the celestial sphere and a large peculiar velocity of 112 km s\u20131.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "3 Cephei, Eta Cephei, HIP 102422, SAO 19019, HD 198149, GC 28962, HR 7957, DM BD+61  2050, TYC 4246-1967-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Al Kidr (Eta)",
	"OType" : "High proper-motion Star",
	"Distance" : "14.27",
	"RA_S" : 311.32240361,
	"DEC_S" : 61.83878016,
	"X" : 606,
	"Y" : 318,
	"Constellation" : "Cepheus ",
	"AMag" : 3.511,
	"key" : 47509,
	"title" : "Al Kidr (Eta)"
	},
{
	"Index" : "25056",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "Upsilon01 Cephei, HIP 102431, SAO 32862, HD 198084, GC 28956, HR 7955, DM BD+57  2240, TYC 3959-1685-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Upsilon01 Cephei",
	"OType" : "Spectroscopic binary",
	"Distance" : "27.12",
	"RA_S" : 311.33803256,
	"DEC_S" : 57.5797272,
	"Constellation" : "Cepheus ",
	"AMag" : 4.571,
	"key" : 45056,
	"title" : "Upsilon01 Cephei"
	},
{
	"Index" : "27604",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "6 Cephei, HIP 105268, SAO 19313, HD 203467, GC 29875, HR 8171, DM BD+64  1527, TYC 4256-3042-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "6 Cephei",
	"OType" : "Be Star",
	"Distance" : "601.99",
	"RA_S" : 319.84256849,
	"DEC_S" : 64.8718543,
	"Constellation" : "Cepheus ",
	"AMag" : 5.169,
	"key" : 47604,
	"title" : "6 Cephei"
	},
{
	"Index" : "27642",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "7 Cephei, HIP 105972, SAO 19432, HD 204770, GC 30081, HR 8227, DM BD+66  1405, TYC 4261-1792-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "7 Cephei",
	"OType" : "Star",
	"Distance" : "246.12",
	"RA_S" : 321.94225999,
	"DEC_S" : 66.80909587,
	"Constellation" : "Cepheus ",
	"AMag" : 5.392,
	"key" : 47642,
	"title" : "7 Cephei"
	},
{
	"Index" : "29380",
	"Description" : "Beta Cephei (\u03B2 Cep, \u03B2 Cephei) is a third magnitude star in the constellation Cepheus. It has the traditional name Alfirk (Arabic \u0627\u0644\u0641\u0631\u0642\u0629 al-firqah), meaning \u0022The Flock\u0022 (referring to a flock of sheep) This star, along with \u03B1 Cep (Alderamin) and \u03B7 Cep (Alkidr), were Al Kaw\u0101kib al Fir\u1E33 (\u0627\u0644\u0643\u0648\u0643\u0628 \u0627\u0644\u0641\u0631\u0642), meaning \u0022the Stars of The Flock\u0022 by Ulug Beg. Beta Cephei is the prototype of the Beta Cephei variable stars.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "8 Cephei, Beta Cephei, HIP 106032, SAO 10057, HD 205021, GC 30118, HR 8238, DM BD+69  1173, TYC 4465-2643-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Alfirk",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "209.09",
	"RA_S" : 322.16498688,
	"DEC_S" : 70.56071519,
	"X" : 486,
	"Y" : 271,
	"Constellation" : "Cepheus ",
	"AMag" : 3.173,
	"key" : 49380,
	"shortTitle" : "Alphirk; Al'firk",
	"title" : "Alfirk"
	},
{
	"Index" : "27583",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "9 Cephei, HIP 106801, SAO 19541, HD 206165, GC 30302, HR 8279, DM BD+61  2169, TYC 4253-2243-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "9 Cephei",
	"OType" : "Pulsating variable Star",
	"RA_S" : 324.48010288,
	"DEC_S" : 62.08193957,
	"Constellation" : "Cepheus ",
	"AMag" : 4.807,
	"key" : 47583,
	"title" : "9 Cephei"
	},
{
	"Index" : "29427",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "11 Cephei, HIP 107119, SAO 10126, HD 206952, GC 30415, HR 8317, DM BD+70  1193, TYC 4470-1875-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "11 Cephei",
	"OType" : "High proper-motion Star",
	"Distance" : "55.89",
	"RA_S" : 325.48038452,
	"DEC_S" : 71.31141939,
	"Constellation" : "Cepheus ",
	"AMag" : 4.659,
	"key" : 49427,
	"title" : "11 Cephei"
	},
{
	"Index" : "29426",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "78 Draconis, HIP 107230, SAO 10131, HD 207130, GC 30452, HR 8324, DM BD+71  1082, TYC 4470-1874-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "78 Draconis",
	"OType" : "Star",
	"Distance" : "74.94",
	"RA_S" : 325.76684247,
	"DEC_S" : 72.32008433,
	"Constellation" : "Cepheus ",
	"AMag" : 5.291,
	"key" : 49426,
	"title" : "78 Draconis"
	},
{
	"Index" : "25267",
	"Description" : "Mu Cephei (\u03BC Cep, \u03BC Cephei), also known as Herschel\u0027s Garnet Star, is a red supergiant star in the constellation Cepheus. It is one of the largest and most luminous stars known in the Milky Way. It appears garnet red and is given the spectral class of M2 Ia. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. The deep red color of Mu Cephei was noted by William Herschel, who described it as \u0022a very fine deep garnet colour, such as the periodical star \u03BF Ceti\u0022, and it is thus commonly known as Herschel\u0027s \u0022Garnet Star\u0022. Giuseppe Piazzi called it Garnet sidus in his catalogue. An alternative name, Erakis, used in Anton\u00EDn Be\u010Dv\u00E1\u0159\u0027s star catalogue, is probably due to confusion with Mu Draconis, which was previously called al-R\u0101qis [ar\u02C8ra\u02D0qis] in Arabic.\r\rIn 1848, English astronomer John Russell Hind discovered that it was variable. This variability was quickly confirmed by German astronomer Friedrich Wilhelm Argelander. Almost continual records of the star\u0027s variability have been maintained since 1881.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "Mu Cephei, HIP 107259, SAO 33693, HD 206936, GC 30440, HR 8316, DM BD+58  2316, TYC 3979-1616-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Herschel's Garnet Star",
	"OType" : "Semi-regular pulsating Star",
	"RA_S" : 325.87692062,
	"DEC_S" : 58.78004333,
	"X" : 560,
	"Y" : 411,
	"Constellation" : "Cepheus ",
	"AMag" : 4.267,
	"key" : 45267,
	"shortTitle" : "Granatovaya; Ehrakis",
	"title" : "Herschel's Garnet Star"
	},
{
	"Index" : "27661",
	"Description" : "Nu Cephei (\u03BD Cep, \u03BD Cep) is a Class A2, fourth-magnitude star in the constellation Cepheus. Nu Cephei is a white pulsating variable star and multiple star system, located about 5100 light-years from Earth.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "10 Cephei, Nu Cephei, HIP 107418, SAO 19624, HD 207260, GC 30483, HR 8334, DM BD+60  2288, TYC 4262-2279-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Nu Cephei",
	"OType" : "Pulsating variable Star",
	"RA_S" : 326.36218658,
	"DEC_S" : 61.12080553,
	"X" : 541,
	"Y" : 386,
	"Constellation" : "Cepheus ",
	"AMag" : 4.349,
	"key" : 47661,
	"title" : "Nu Cephei"
	},
{
	"Index" : "27714",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "VV Cephei, HIP 108317, SAO 19753, HD 208816, GC 30731, HR 8383, DM BD+62  2007, TYC 4266-3252-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "VV Cephei",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "670.17",
	"RA_S" : 329.16307992,
	"DEC_S" : 63.62556024,
	"Constellation" : "Cepheus ",
	"AMag" : 5.363,
	"key" : 47714,
	"title" : "VV Cephei"
	},
{
	"Index" : "29453",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "16 Cephei, HIP 108535, SAO 10216, HD 209369, GC 30800, HR 8400, DM BD+72  1009, TYC 4474-1757-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "16 Cephei",
	"OType" : "Star",
	"Distance" : "36.72",
	"RA_S" : 329.81236084,
	"DEC_S" : 73.17989435,
	"Constellation" : "Cepheus ",
	"AMag" : 5.088,
	"key" : 49453,
	"title" : "16 Cephei"
	},
{
	"Index" : "27770",
	"Description" : "Xi Cephei (\u03BE Cep, \u03BE Cephei) is a star in the constellation Cepheus. It has the traditional name Kurhah or Alkirdah or Al Kirduh, and the name was from Al \u1E32ur\u1E25a\u1E25 (\u0627\u0644\u0642\u0631\u062D\u0629 - al-qurhah), an Arabic word that translated as a white spot, or blaze, in the face of a horse and other suggestion was Al \u1E32irdah (\u0623\u0644\u0642\u0631\u062F\u0629 - al q\u00EDrada), the Ape. Xi Cephei belongs to spectral class A3/6Vm and has apparent magnitude +4.29. It is approximately 100 light years from Earth.\r\rIt is a spectroscopic binary.\r\rIn Chinese, \u5929\u920E (Ti\u0101n G\u014Du), meaning Celestial Hook, refers to an asterism consisting of \u03BE Cephei, 4 Cephei, HD 194298, \u03B7 Cephei, \u03B8 Cephei, \u03B1 Cephei, 26 Cephei, \u03B9 Cephei and \u03BF Cephei. Consequently, \u03BE Cephei itself is known as \u5929\u920E\u516D (Ti\u0101n G\u014Du li\u00F9, English: the Sixth Star of Celestial Hook.).",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "17 Cephei, Xi Cephei, HIP 108917B, SAO 19826, HD 209791, GC 30876, DM BD+63  1802B, TYC 4271-2619-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Kurhah / Alkirdah",
	"OType" : "Spectroscopic binary",
	"Distance" : "31.16",
	"RA_S" : 330.942579,
	"DEC_S" : 64.628194,
	"X" : 494,
	"Y" : 361,
	"Constellation" : "Cepheus ",
	"AMag" : 6.403,
	"key" : 47770,
	"title" : "Kurhah / Alkirdah"
	},
{
	"Index" : "27771",
	"Description" : "Xi Cephei (\u03BE Cep, \u03BE Cephei) is a star in the constellation Cepheus. It has the traditional name Kurhah or Alkirdah or Al Kirduh, and the name was from Al \u1E32ur\u1E25a\u1E25 (\u0627\u0644\u0642\u0631\u062D\u0629 - al-qurhah), an Arabic word that translated as a white spot, or blaze, in the face of a horse and other suggestion was Al \u1E32irdah (\u0623\u0644\u0642\u0631\u062F\u0629 - al q\u00EDrada), the Ape. Xi Cephei belongs to spectral class A3/6Vm and has apparent magnitude +4.29. It is approximately 100 light years from Earth.\r\rIt is a spectroscopic binary.\r\rIn Chinese, \u5929\u920E (Ti\u0101n G\u014Du), meaning Celestial Hook, refers to an asterism consisting of \u03BE Cephei, 4 Cephei, HD 194298, \u03B7 Cephei, \u03B8 Cephei, \u03B1 Cephei, 26 Cephei, \u03B9 Cephei and \u03BF Cephei. Consequently, \u03BE Cephei itself is known as \u5929\u920E\u516D (Ti\u0101n G\u014Du li\u00F9, English: the Sixth Star of Celestial Hook.).",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "17 Cephei, Xi Cephei, HIP 108917A, SAO 19827, HD 209790, GC 30877, HR 8417, DM BD+63  1802A, TYC 4271-2620-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Kurhah / Alkirdah",
	"OType" : "Spectroscopic binary",
	"Distance" : "31.16",
	"RA_S" : 330.94771793,
	"DEC_S" : 64.62796997,
	"X" : 494,
	"Y" : 361,
	"Constellation" : "Cepheus ",
	"AMag" : 4.446,
	"key" : 47771,
	"shortTitle" : "Al Kirdah; Kurhah",
	"title" : "Kurhah / Alkirdah"
	},
{
	"Index" : "27733",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "18 Cephei, HIP 108924, SAO 19828, HD 209772, GC 30880, HR 8416, DM BD+62  2028, TYC 4267-2755-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "18 Cephei",
	"OType" : "Long Period Variable candidate",
	"Distance" : "129.92",
	"RA_S" : 330.9707415,
	"DEC_S" : 63.11991736,
	"Constellation" : "Cepheus ",
	"AMag" : 5.473,
	"key" : 47733,
	"title" : "18 Cephei"
	},
{
	"Index" : "27734",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "20 Cephei, HIP 109005, SAO 19847, HD 209960, GC 30904, HR 8426, DM BD+62  2029, TYC 4267-2756-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "20 Cephei",
	"OType" : "Variable Star",
	"Distance" : "92.89",
	"RA_S" : 331.25207766,
	"DEC_S" : 62.78567019,
	"Constellation" : "Cepheus ",
	"AMag" : 5.432,
	"key" : 47734,
	"title" : "20 Cephei"
	},
{
	"Index" : "27735",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "19 Cephei, HIP 109017, SAO 19849, HD 209975, GC 30907, HR 8428, DM BD+61  2246, TYC 4267-2757-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "19 Cephei",
	"OType" : "Double or multiple star",
	"Distance" : "622.12",
	"RA_S" : 331.2866248,
	"DEC_S" : 62.27981393,
	"Constellation" : "Cepheus ",
	"AMag" : 5.109,
	"key" : 47735,
	"title" : "19 Cephei"
	},
{
	"Index" : "29432",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "24 Cephei, HIP 109400, SAO 10265, HD 210807, GC 31037, HR 8468, DM BD+71  1111, TYC 4471-1685-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "24 Cephei",
	"OType" : "Star",
	"Distance" : "120.86",
	"RA_S" : 332.45179393,
	"DEC_S" : 72.34120543,
	"Constellation" : "Cepheus ",
	"AMag" : 4.888,
	"key" : 49432,
	"title" : "24 Cephei"
	},
{
	"Index" : "25296",
	"Description" : "Zeta Cephei (\u03B6 Cep, \u03B6 Cephei) is a star in the constellation of Cepheus. Zeta Cephei marks the left shoulder of Cepheus, the King of Joppa (Ethiopia).\r\rZeta Cephei is an orange supergiant star of spectral type K1.5 Ib, with a surface temperature of 3,853 K and eight times more massive then the Sun. The luminosity of Zeta Cephei is approximately 3600 times that of the Sun. At a distance of about 726 light-years, Zeta Cephei has an apparent magnitude (m) of 3.39 and an absolute magnitude (M) of -3.35. The star has a metallicity approximately 1.6 times that of the Sun; i.e., it contains 1.6 times as much heavy-element material as the sun.\r\rAt the edge of the 8 to 10 solar mass limit at which stars develop iron cores and then explode as supernovae, Zeta Cephei\u0027s most likely fate is to produce a very massive white dwarf near the Chandrasekhar limit (1.4 solar mass) at which such dense remnants can survive. If Zeta Cephei is a binary star; i.e., if there is a stellar companion, and it is close enough to feed sufficient matter to the white-dwarf-to-be, it is marginally possible that the limit could be overflowed, resulting in the white dwarf\u0027s collapse and a Type Ia supernova explosion.\r\rHekkel et al. (2008) have detected a periodicity of 533 days, hinting at the possible presence of an as yet unseen companion.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "21 Cephei, Zeta Cephei, HIP 109492, SAO 34137, HD 210745, GC 31044, HR 8465, DM BD+57  2475, TYC 3981-1590-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Zeta Cephei",
	"OType" : "Eclipsing binary",
	"Distance" : "256.21",
	"RA_S" : 332.71364908,
	"DEC_S" : 58.20125999,
	"X" : 524,
	"Y" : 442,
	"Constellation" : "Cepheus ",
	"AMag" : 3.51,
	"key" : 45296,
	"title" : "Zeta Cephei"
	},
{
	"Index" : "25290",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "22 Cephei, Lambda Cephei, HIP 109556, SAO 34149, HD 210839, GC 31066, HR 8469, DM BD+58  2402, TYC 3981-1585-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Lambda Cephei",
	"OType" : "Blue supergiant star",
	"Distance" : "593.4",
	"RA_S" : 332.87739877,
	"DEC_S" : 59.4144874,
	"Constellation" : "Cepheus ",
	"AMag" : 5.099,
	"key" : 45290,
	"title" : "Lambda Cephei"
	},
{
	"Index" : "25247",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 109572, SAO 34151, HD 210855, GC 31070, HR 8472, DM BD+56 2727, TYC 3977-2051-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8472",
	"OType" : "High proper-motion Star",
	"Distance" : "37.35",
	"RA_S" : 332.95320103,
	"DEC_S" : 56.83935792,
	"Constellation" : "Cepheus ",
	"AMag" : 5.305,
	"key" : 45247,
	"title" : "HR 8472"
	},
{
	"Index" : "27678",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 109592, SAO 19932, HD 210939, GC 31077, HR 8479, DM BD+60 2358, TYC 4263-2407-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8479",
	"OType" : "Star",
	"Distance" : "112",
	"RA_S" : 333.00838977,
	"DEC_S" : 60.75910568,
	"Constellation" : "Cepheus ",
	"AMag" : 5.491,
	"key" : 47678,
	"title" : "HR 8479"
	},
{
	"Index" : "30870",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 109693, SAO 3721, HD 212710, GC 31223, HR 8546, DM BD+85  383, TYC 4654-1613-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8546",
	"OType" : "Star",
	"Distance" : "78.62",
	"RA_S" : 333.29423939,
	"DEC_S" : 86.10796795,
	"Constellation" : "Cepheus ",
	"AMag" : 5.254,
	"key" : 50870,
	"title" : "HR 8546"
	},
{
	"Index" : "25399",
	"Description" : "Epsilon Cephei (\u03B5 Cep, \u03B5 Cep) is a Class F0, fourth-magnitude star in the constellation Cepheus. Epsilon Cephei is a yellow-white, Delta Scuti variable star, located about 85 light-years from Earth.\r\rIn Chinese, \u87A3\u86C7 (T\u00E9ng Sh\u00E9), meaning Flying Serpent, refers to an asterism consisting of \u03B5 Cephei, \u03B1 Lacertae, 4 Lacertae, \u03C02 Cygni, \u03C01 Cygni, HD 206267, \u03B2 Lacertae, \u03C3 Cassiopeiae, \u03C1 Cassiopeiae, \u03C4 Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, \u03BB Andromedae, \u03BA Andromedae, \u03B9 Andromedae, and \u03C8 Andromedae. Consequently, \u03B5 Cephei itself is known as \u87A3\u86C7\u4E5D (T\u00E9ng Sh\u00E9 ji\u01D4, English: the Ninth Star of Flying Serpent)",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "23 Cephei, Epsilon Cephei, HIP 109857, SAO 34227, HD 211336, GC 31135, HR 8494, DM BD+56  2741, TYC 3990-2431-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Epsilon Cephei",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "25.73",
	"RA_S" : 333.75914709,
	"DEC_S" : 57.04357698,
	"X" : 524,
	"Y" : 459,
	"Constellation" : "Cepheus ",
	"AMag" : 4.208,
	"key" : 45399,
	"title" : "Epsilon Cephei"
	},
{
	"Index" : "25448",
	"Description" : "Delta Cephei (\u03B4 Cep, \u03B4 Cephei) is the Bayer designation for a binary star system located approximately 887 light-years away in the northern circumpolar constellation of Cepheus, the King. At this distance, the visual magnitude of the star is diminished by 0.23 as a result of extinction caused by gas and dust along the line of sight. It is the prototype of the Cepheid variable stars that undergo periodic changes in luminosity.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "27 Cephei, Delta Cephei, HIP 110991, SAO 34508, HD 213306, GC 31421, HR 8571, DM BD+57  2548, TYC 3995-1479-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Delta Cephei",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "264.68",
	"RA_S" : 337.29276758,
	"DEC_S" : 58.4152036,
	"X" : 494,
	"Y" : 452,
	"Constellation" : "Cepheus ",
	"AMag" : 4.207,
	"key" : 45448,
	"title" : "Delta Cephei"
	},
{
	"Index" : "30535",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "29 Cephei, Rho Cephei, HIP 111056, SAO 10402, HD 213798, GC 31474, HR 8591, DM BD+78   801, TYC 4608-2417-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Al Kalb al Rai",
	"OType" : "Star",
	"Distance" : "75.11",
	"RA_S" : 337.47074611,
	"DEC_S" : 78.82428226,
	"Constellation" : "Cepheus ",
	"AMag" : 5.466,
	"key" : 50535,
	"title" : "Al Kalb al Rai"
	},
{
	"Index" : "29568",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "31 Cephei, HIP 111532, SAO 10425, HD 214470, GC 31567, HR 8615, DM BD+72  1049, TYC 4488-872-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "31 Cephei",
	"OType" : "High proper-motion Star",
	"Distance" : "54.88",
	"RA_S" : 338.94222934,
	"DEC_S" : 73.64318931,
	"Constellation" : "Cepheus ",
	"AMag" : 5.109,
	"key" : 49568,
	"title" : "31 Cephei"
	},
{
	"Index" : "27756",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "30 Cephei, HIP 111797, SAO 20190, HD 214734, GC 31620, HR 8627, DM BD+62  2102, TYC 4269-809-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "30 Cephei",
	"OType" : "Star",
	"Distance" : "87.99",
	"RA_S" : 339.66271111,
	"DEC_S" : 63.58447528,
	"Constellation" : "Cepheus ",
	"AMag" : 5.197,
	"key" : 47756,
	"title" : "30 Cephei"
	},
{
	"Index" : "30839",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 112519, SAO 3794, HD 216446, GC 31855, HR 8702, DM BD+82  703, TYC 4650-3037-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8702",
	"OType" : "Star",
	"Distance" : "96.02",
	"RA_S" : 341.87107561,
	"DEC_S" : 83.15383207,
	"Constellation" : "Cepheus ",
	"AMag" : 4.916,
	"key" : 50839,
	"title" : "HR 8702"
	},
{
	"Index" : "27830",
	"Description" : "Iota Cephei (\u03B9 Cep, \u03B9 Cep) is a Class K0, third-magnitude star in the constellation Cepheus. Iota Cephei is an orange giant star located about 115 light-years from Earth. This star has 10.05 \u00B1 0.18 times the Sun\u0027s radius and about 1.8\u20132.2 times the mass of the Sun. It is emitting 49.6 \u00B1 2.5 as much luminosity as the Sun, which is being radiated from its outer atmosphere at an effective temperature of 4,831 \u00B1 74 K. Due to precession of the equinoxes, it will become the pole star some time around 5200 CE.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "32 Cephei, Iota Cephei, HIP 112724, SAO 20268, HD 216228, GC 31857, HR 8694, DM BD+65  1814, TYC 4277-1102-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Iota Cephei",
	"OType" : "Variable Star",
	"Distance" : "35.35",
	"RA_S" : 342.42007037,
	"DEC_S" : 66.20040964,
	"X" : 429,
	"Y" : 367,
	"Constellation" : "Cepheus ",
	"AMag" : 3.611,
	"key" : 47830,
	"title" : "Iota Cephei"
	},
{
	"Index" : "30838",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 113116, SAO 3816, HD 217382, GC 31999, HR 8748, DM BD+83  640, TYC 4650-3036-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8748",
	"OType" : "Star",
	"Distance" : "109",
	"RA_S" : 343.60400919,
	"DEC_S" : 84.34617707,
	"Constellation" : "Cepheus ",
	"AMag" : 4.85,
	"key" : 50838,
	"title" : "HR 8748"
	},
{
	"Index" : "27990",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 113864, SAO 20398, HD 218029, GC 32142, HR 8779, DM BD+66 1575, TYC 4290-1302-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 8779",
	"OType" : "Star",
	"Distance" : "126.62",
	"RA_S" : 345.8870026,
	"DEC_S" : 67.20921049,
	"Constellation" : "Cepheus ",
	"AMag" : 5.371,
	"key" : 47990,
	"title" : "HR 8779"
	},
{
	"Index" : "30475",
	"Description" : "Pi Cephei (\u03C0 Cep) is a trinary star located in the constellation Cepheus.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "33 Cephei, Pi Cephei, HIP 114222B, SAO 10629, HD 218658, GC 32237, HR 8819, DM BD+74  1006, TYC 4601-3531-2",
	"group" : { "key" : "Cepheus" },
	"Common" : "Pi Cephei",
	"OType" : "Star",
	"Distance" : "67.29",
	"RA_S" : 346.97433962,
	"DEC_S" : 75.38753356,
	"X" : 373,
	"Y" : 259,
	"Constellation" : "Cepheus ",
	"AMag" : 6.798,
	"key" : 50475,
	"title" : "Pi Cephei"
	},
{
	"Index" : "30474",
	"Description" : "Pi Cephei (\u03C0 Cep) is a trinary star located in the constellation Cepheus.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "33 Cephei, Pi Cephei, HIP 114222A, SAO 10629, HD 218658, GC 32237, HR 8819, DM BD+74  1006, TYC 4601-3531-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Pi Cephei",
	"OType" : "Spectroscopic binary",
	"Distance" : "67.29",
	"RA_S" : 346.97433962,
	"DEC_S" : 75.38753356,
	"X" : 373,
	"Y" : 259,
	"Constellation" : "Cepheus ",
	"AMag" : 4.609,
	"key" : 50474,
	"title" : "Pi Cephei"
	},
{
	"Index" : "29486",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "34 Cephei, Omicron Cephei, HIP 115088A, SAO 20554, HD 219916, GC 32463, HR 8872, DM BD+67  1514, TYC 4478-1361-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Omicron Cephei",
	"OType" : "Double or multiple star",
	"Distance" : "62.23",
	"RA_S" : 349.65620785,
	"DEC_S" : 68.11147467,
	"Constellation" : "Cepheus ",
	"AMag" : 4.971,
	"key" : 49486,
	"title" : "Omicron Cephei"
	},
{
	"Index" : "29487",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "34 Cephei, Omicron Cephei, HIP 115088B, SAO 20554, HD 219916, GC 32463, HR 8872, DM BD+67  1514, TYC 4478-1361-2",
	"group" : { "key" : "Cepheus" },
	"Common" : "Omicron Cephei",
	"OType" : "Double or multiple star",
	"Distance" : "62.23",
	"RA_S" : 349.65621622,
	"DEC_S" : 68.11144271,
	"Constellation" : "Cepheus ",
	"AMag" : 4.75,
	"key" : 49487,
	"title" : "Omicron Cephei"
	},
{
	"Index" : "30522",
	"Description" : "Gamma Cephei (\u03B3 Cep, \u03B3 Cephei), traditionally named Errai, Er Rai, and or Alrai, is a binary star system approximately 45 light-years away in the constellation of Cepheus. Gamma Cephei contains an apparent magnitude of 3.22. The visible part of the system is a stellar class K1III-IV orange subgiant star on its first ascent off the main sequence. It is about 6.6 billion years old (based on Fe/H metallicity). Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.\r\rGamma Cephei is the naked-eye star that will succeed Polaris as the Earth\u0027s northern pole star, due to the precession of the equinoxes. It will be closer to the northern celestial pole than Polaris around 3000 CE and will make its closest approach around 4000 CE. The \u0022title\u0022 will pass to \u03B9 Cephei some time around 5200 CE.\r\rThe star has a companion star with a mass approximately 0.409 times that of our Sun. Gamma Cephei B is of stellar mass and is assumed to be of similar age to its primary. It is probably a red dwarf of class M4, 6.2 degrees of magnitude fainter than the K-type primary star.",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "35 Cephei, Gamma Cephei, HIP 116727, SAO 10818, HD 222404, GC 32875, HR 8974, DM BD+76   928, TYC 4606-3584-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "Errai / Er Rai, and / Alrai",
	"OType" : "Spectroscopic binary",
	"Distance" : "14.1",
	"RA_S" : 354.836665,
	"DEC_S" : 77.6323124,
	"X" : 342,
	"Y" : 235,
	"Constellation" : "Cepheus ",
	"AMag" : 3.322,
	"key" : 50522,
	"shortTitle" : "Errai; Arrai; Er Rai; Al'rai",
	"title" : "Errai / Er Rai, and / Alrai"
	},
{
	"Index" : "29488",
	"MapNum" : "14",
	"ImageNum" : "14",
	"Desig" : "HIP 117371, SAO 20853, HD 223274, GC 33031, HR 9013, DM BD+67 1562, TYC 4479-1760-1",
	"group" : { "key" : "Cepheus" },
	"Common" : "HR 9013",
	"OType" : "Star",
	"Distance" : "92.9",
	"RA_S" : 356.97820766,
	"DEC_S" : 67.80680778,
	"Constellation" : "Cepheus ",
	"AMag" : 5.043,
	"key" : 49488,
	"title" : "HR 9013"
	},
{
	"Index" : "39630",
	"Description" : "2 Ceti (2 Cet) is a star in the constellation Cetus. Its apparent magnitude is 4.54.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "2 Ceti, HIP 301, SAO 147059, HD 225132, GC 23, HR 9098, DM BD-18  6417, TYC 5838-1288-1",
	"group" : { "backgroundImage" : "images/Alignment/16.png",
		"description" : "Cetus (pron.: /\u02C8si\u02D0t\u0259s/) is a constellation. Its name refers to Cetus, a sea monster in Greek mythology, although it is often called \u0027the whale\u0027 today. Cetus is located in the region of the sky that contains other water-related constellations such as Aquarius, Pisces, and Eridanus.\r\rCetus may have originally been associated with a whale, which would have had mythic status amongst Mesopotamian cultures. It is often now called the Whale, though it is most strongly associated with Cetus the sea-monster, who was slain by Perseus as he saved the princess Andromeda from Poseidon\u0027s wrath. Cetus is located in a region of the sky called \u0022The Sea\u0022 because many water-associated constellations are placed there, including Eridanus, Pisces, Piscis Austrinus, Capricornus, and Aquarius.\r\rCetus has been depicted many ways throughout its history. In the 17th century, Cetus was depicted as a \u0022dragon fish\u0022 by Johannes Bayer. Both Willem Jansson Blaeu and Cellarius[disambiguation needed] depicted Cetus as a whale-like creature in the same century. However, Cetus has also been variously depicted with animal heads attached to a piscine body.",
		"key" : "Cetus",
		"grouptype" : "Cetus",
		"Meaning" : "sea monster (later interpreted as a whale)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Cetus",
		"title" : "Cetus Objects Group" },
	"Common" : "2 Ceti",
	"OType" : "Star",
	"Distance" : "83.43",
	"RA_S" : 0.93494934,
	"DEC_S" : -17.3359922,
	"X" : 666,
	"Y" : 480,
	"Constellation" : "Cetus ",
	"AMag" : 4.527,
	"key" : 59630,
	"title" : "2 Ceti"
	},
{
	"Index" : "35324",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "3 Ceti, HIP 355, SAO 147066, HD 225212, GC 36, HR 9103, DM BD-11  6194, TYC 5263-1049-1",
	"group" : { "key" : "Cetus" },
	"Common" : "3 Ceti",
	"OType" : "Variable Star",
	"Distance" : "612.02",
	"RA_S" : 1.12549591,
	"DEC_S" : -10.50952282,
	"Constellation" : "Cetus ",
	"AMag" : 5.123,
	"key" : 55324,
	"title" : "3 Ceti"
	},
{
	"Index" : "39635",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "6 Ceti, HIP 910, SAO 147133, HD 693, GC 190, HR 33, DM BD-16    17, TYC 5839-1081-1",
	"group" : { "key" : "Cetus" },
	"Common" : "6 Ceti",
	"OType" : "High proper-motion Star",
	"Distance" : "18.74",
	"RA_S" : 2.81607642,
	"DEC_S" : -15.46798074,
	"Constellation" : "Cetus ",
	"AMag" : 4.95,
	"key" : 59635,
	"title" : "6 Ceti"
	},
{
	"Index" : "39655",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 983, SAO 147144, HD 787, GC 214, HR 37, DM BD-18   14, TYC 5842-1161-1",
	"group" : { "key" : "Cetus" },
	"Common" : "HR 37",
	"OType" : "Star",
	"Distance" : "187.06",
	"RA_S" : 3.0416001,
	"DEC_S" : -17.93828415,
	"Constellation" : "Cetus ",
	"AMag" : 5.439,
	"key" : 59655,
	"title" : "HR 37"
	},
{
	"Index" : "35308",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 1158, SAO 128655, HD 1014, GC 265, HR 46, DM BD-08   26, TYC 5261-219-1",
	"group" : { "key" : "Cetus" },
	"Common" : "V* AD Cet",
	"OType" : "Long Period Variable candidate",
	"Distance" : "177.96",
	"RA_S" : 3.61511659,
	"DEC_S" : -7.78052668,
	"Constellation" : "Cetus ",
	"AMag" : 5.333,
	"key" : 55308,
	"title" : "V* AD Cet"
	},
{
	"Index" : "39657",
	"Description" : "7 Ceti (7 Cet) is a star in the constellation Cetus. Its apparent magnitude is 4.44.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "7 Ceti, HIP 1170, SAO 147169, HD 1038, GC 272, HR 48, DM BD-19    21, TYC 5842-1163-1",
	"group" : { "key" : "Cetus" },
	"Common" : "7 Ceti",
	"OType" : "Long Period Variable candidate",
	"Distance" : "136.93",
	"RA_S" : 3.66006788,
	"DEC_S" : -18.93286794,
	"X" : 630,
	"Y" : 498,
	"Constellation" : "Cetus ",
	"AMag" : 4.629,
	"key" : 59657,
	"title" : "7 Ceti"
	},
{
	"Index" : "35306",
	"Description" : "Iota Ceti (\u03B9 Cet, \u03B9 Ceti) is a star in the constellation Cetus. It has the traditional name Deneb Kaitos Shemali. The name was from the Arabian word \u0630\u0646\u0628 \u0623\u0644\u0634\u0645\u0627\u0644\u064A - \u00F0\u00E1nab al sham\u0101liyy, meaning the northern tail of the sea monster.\r\rIn Chinese, \u5929\u5009 (Ti\u0101n C\u0101ng), meaning Square Celestial Granary, refers to an asterism consisting of \u03B9 Ceti, \u03B7 Ceti, \u03B8 Ceti, \u03B6 Ceti, \u03C4 Ceti and 57 Ceti. Consequently, \u03B9 Ceti itself is known as \u5929\u5009\u4E00 (Ti\u0101n C\u0101ng y\u012B, English: the First Star of Square Celestial Granary.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "8 Ceti, Iota Ceti, HIP 1562, SAO 128694, HD 1522, GC 388, HR 74, DM BD-09    48, TYC 5261-1084-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Deneb Kaitos Shemali",
	"OType" : "High proper-motion Star",
	"Distance" : "84.15",
	"RA_S" : 4.85697636,
	"DEC_S" : -8.82392118,
	"X" : 626,
	"Y" : 364,
	"Constellation" : "Cetus ",
	"AMag" : 3.674,
	"key" : 55306,
	"shortTitle" : "Deneb Kaitos Al Shamaliyy; Deneb al' Shemali",
	"title" : "Deneb Kaitos Shemali"
	},
{
	"Index" : "44056",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 2381, SAO 166318, HD 2696, GC 590, HR 118, DM CD-24  179, TYC 6414-1077-1",
	"group" : { "key" : "Cetus" },
	"Common" : "HR 118",
	"OType" : "Double or multiple star",
	"Distance" : "53.09",
	"RA_S" : 7.59439436,
	"DEC_S" : -23.78768058,
	"Constellation" : "Cetus ",
	"AMag" : 5.18,
	"key" : 64056,
	"title" : "HR 118"
	},
{
	"Index" : "30996",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "13 Ceti, HIP 2762AB, SAO 128839, HD 3196, GC 696, HR 142, DM BD-04    62, TYC 4675-1216-3",
	"group" : { "key" : "Cetus" },
	"Common" : "13 Ceti",
	"OType" : "Variable of RS CVn type",
	"Distance" : "21.25",
	"RA_S" : 8.81201635,
	"DEC_S" : -3.59281795,
	"Constellation" : "Cetus ",
	"AMag" : 5.265,
	"key" : 50996,
	"title" : "13 Ceti"
	},
{
	"Index" : "35377",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "17 Ceti, Phi01 Ceti, HIP 3455, SAO 147423, HD 4188, GC 875, HR 194, DM BD-11   128, TYC 5269-2450-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Phi01 Ceti",
	"OType" : "Variable Star",
	"Distance" : "71.61",
	"RA_S" : 11.04750234,
	"DEC_S" : -10.60955016,
	"Constellation" : "Cetus ",
	"AMag" : 4.878,
	"key" : 55377,
	"title" : "Phi01 Ceti"
	},
{
	"Index" : "39726",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 3505, SAO 166528, HD 4247, GC 889, HR 197, DM BD-22  127, TYC 5849-2437-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Gliese 31.3 (HR 197)",
	"OType" : "Star",
	"Distance" : "26.74",
	"RA_S" : 11.18497822,
	"DEC_S" : -22.00613698,
	"Constellation" : "Cetus ",
	"AMag" : 5.26,
	"key" : 59726,
	"title" : "Gliese 31.3 (HR 197)"
	},
{
	"Index" : "35385",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "19 Ceti, Phi02 Ceti, HIP 3909, SAO 147470, HD 4813, GC 1003, HR 235, DM BD-11   153, TYC 5270-1139-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Phi02 Ceti",
	"OType" : "Star",
	"Distance" : "15.75",
	"RA_S" : 12.53162863,
	"DEC_S" : -10.64432723,
	"Constellation" : "Cetus ",
	"AMag" : 5.224,
	"key" : 55385,
	"title" : "Phi02 Ceti"
	},
{
	"Index" : "30990",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "20 Ceti, HIP 4147, SAO 129009, HD 5112, GC 1055, HR 248, DM BD-01   114, TYC 4674-1183-1",
	"group" : { "key" : "Cetus" },
	"Common" : "20 Ceti",
	"OType" : "Star",
	"Distance" : "179.52",
	"RA_S" : 13.25206001,
	"DEC_S" : -1.14425879,
	"Constellation" : "Cetus ",
	"AMag" : 4.941,
	"key" : 50990,
	"title" : "20 Ceti"
	},
{
	"Index" : "35444",
	"Description" : "Eta Ceti (\u03B7 Cet, \u03B7 Ceti) is a star in the equatorial constellation of Cetus, the whale. It has the traditional name Deneb Algenubi or Algenudi. The apparent visual magnitude of this star is +3.4, making it the fourth brightest star in this otherwise relatively faint constellation. The distance to this star can be measured directly using the parallax technique, yielding a value of 123.9 light-years (38.0 parsecs).\r\rThis is a giant star with a stellar classification of K1 III, having exhausted the hydrogen at its core and evolved away from the main sequence of stars like the Sun. (The classification is sometimes listed as K1.5 IIICN1Fe0.5, indicating a higher than normal abundance of cyanogen and iron relative to other stars of its class.) It is a red clump star that is generating energy through the nuclear fusion of helium at its core.\r\rEta Ceti may have slightly more mass than the Sun and its outer envelope has expanded to 15 times the Sun\u0027s radius. It is radiating 74 times as much luminosity as the Sun from its outer atmosphere at an effective temperature of 4,356 K. This heat gives the star the orange-hued glow of a K-type star.\r\rThe name Deneb Algenubi was from Arabic \u0630\u0646\u0628 \u0623\u0644\u062C\u0646\u0628\u064A - \u00F0\u00E1nab al-jan\u016Bbii, meaning the southern tail of the sea monster. In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Aoul al Naamat (\u0623\u0648\u0644 \u0623\u0644\u0646\u0639\u0645\u0629 - awwil al na\u02BD\u0101m\u0101t), which was translated into Latin as Prima Struthionum, meaning the first ostrich. This star, along with \u03B8 Cet (Thanih al Naamat), \u03C4 Cet (Thalath Al Naamat), \u03B6 Cet (Baten Kaitos) and \u03C5 Cet, were Al Na\u02BD\u0101m\u0101t (\u0623\u0644\u0646\u0639\u0645\u0629), the Hen Ostriches.\r\rIn Chinese, \u5929\u5009 (Ti\u0101n C\u0101ng), meaning Square Celestial Granary, refers to an asterism consisting of \u03B7 Ceti, \u03B9 Ceti, \u03B8 Ceti, \u03B6 Ceti, \u03C4 Ceti and 57 Ceti. Consequently, \u03B7 Ceti itself is known as \u5929\u5009\u4E8C (Ti\u0101n C\u0101ng \u00E8r, English: the Second Star of Square Celestial Granary.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "31 Ceti, Eta Ceti, HIP 5364, SAO 147632, HD 6805, GC 1384, HR 334, DM BD-10   240, TYC 5273-2657-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Deneb Algenubi / Algenudi",
	"OType" : "Horizontal Branch Star",
	"Distance" : "37.99",
	"RA_S" : 17.14746688,
	"DEC_S" : -10.18226477,
	"X" : 468,
	"Y" : 375,
	"Constellation" : "Cetus ",
	"AMag" : 3.573,
	"key" : 55444,
	"shortTitle" : "Deneb; Deneb Algenubi",
	"title" : "Deneb Algenubi / Algenudi"
	},
{
	"Index" : "35440",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "37 Ceti, HIP 5799, SAO 129193, HD 7439, GC 1491, HR 366, DM BD-08   216, TYC 5273-2653-1",
	"group" : { "key" : "Cetus" },
	"Common" : "37 Ceti",
	"OType" : "Double or multiple star",
	"Distance" : "23.38",
	"RA_S" : 18.60016957,
	"DEC_S" : -7.92282222,
	"Constellation" : "Cetus ",
	"AMag" : 5.188,
	"key" : 55440,
	"title" : "37 Ceti"
	},
{
	"Index" : "35456",
	"Description" : "Theta Ceti (\u03B8 Ceti, \u03B8 Cet) is a Class K0, fourth-magnitude star in the constellation Cetus. Theta Ceti is an orange giant star located about 115 light-years from Earth.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Thanih al Naamat (\u062A\u0627\u0646\u064A \u0623\u0644\u0646\u0639\u0627\u0645\u0629 - taanii al na\u02BD\u0101m\u0101t), which was translated into Latin as Secunda Struthionum, meaning the second ostrich. This star, along with \u03B7 Cet (Deneb Algenubi), \u03C4 Cet (Thalath Al Naamat), \u03B6 Cet (Baten Kaitos)and \u03C5 Cet, were Al Na\u02BD\u0101m\u0101t (\u0623\u0644\u0646\u0639\u0627\u0645\u0629), the Hen Ostriches.\r\rIn Chinese, \u5929\u5009 (Ti\u0101n C\u0101ng), meaning Square Celestial Granary, refers to an asterism consisting of \u03B8 Ceti, \u03B9 Ceti, \u03B7 Ceti, \u03B6 Ceti, \u03C4 Ceti and 57 Ceti. Consequently, \u03B8 Ceti itself is known as \u5929\u5009\u4E09 (Ti\u0101n C\u0101ng s\u0101n, English: the Third Star of Square Celestial Granary.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "45 Ceti, Theta Ceti, HIP 6537, SAO 129274, HD 8512, GC 1695, HR 402, DM BD-08   244, TYC 5274-1984-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Theta Ceti",
	"OType" : "Horizontal Branch Star",
	"Distance" : "34.89",
	"RA_S" : 21.00585534,
	"DEC_S" : -8.1832559,
	"X" : 418,
	"Y" : 348,
	"Constellation" : "Cetus ",
	"AMag" : 3.722,
	"key" : 55456,
	"title" : "Theta Ceti"
	},
{
	"Index" : "35493",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "46 Ceti, HIP 6670, SAO 147803, HD 8705, GC 1725, HR 412, DM BD-15   266, TYC 5276-2116-1",
	"group" : { "key" : "Cetus" },
	"Common" : "46 Ceti",
	"OType" : "Star",
	"Distance" : "87.62",
	"RA_S" : 21.40514481,
	"DEC_S" : -14.59879184,
	"Constellation" : "Cetus ",
	"AMag" : 5.045,
	"key" : 55493,
	"title" : "46 Ceti"
	},
{
	"Index" : "39794",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "48 Ceti, HIP 6960, SAO 167086, HD 9132, GC 1808, HR 433, DM BD-22   254, TYC 5854-2047-1",
	"group" : { "key" : "Cetus" },
	"Common" : "48 Ceti",
	"OType" : "Star",
	"Distance" : "71.34",
	"RA_S" : 22.40056441,
	"DEC_S" : -21.62933815,
	"Constellation" : "Cetus ",
	"AMag" : 5.107,
	"key" : 59794,
	"title" : "48 Ceti"
	},
{
	"Index" : "31114",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 7999, SAO 129465, HD 10550, GC 2093, HR 500, DM BD-04  260, TYC 4685-2579-1",
	"group" : { "key" : "Cetus" },
	"Common" : "HR 500",
	"OType" : "Variable Star",
	"Distance" : "362.41",
	"RA_S" : 25.68129396,
	"DEC_S" : -3.6901993,
	"Constellation" : "Cetus ",
	"AMag" : 5.142,
	"key" : 51114,
	"title" : "HR 500"
	},
{
	"Index" : "39815",
	"Description" : "Tau Ceti (\u03C4 Cet, \u03C4 Ceti) is a star in the constellation Cetus that is spectrally similar to the Sun, although it has only about 78% of the Sun\u0027s mass. At a distance of just under 12 light-years from the Solar System, it is a relatively nearby star, and is the closest solitary G-class star.[nb 1] The star appears stable, with little stellar variation.\r\rTau Ceti is metal-deficient, which deficiency is usually correlated with no giant planets and few rocky planets. Observations have however detected more than ten times as much dust surrounding Tau Ceti as is present in the Solar System.\r\rSince December 2012, there has been evidence of possibly five planets orbiting Tau Ceti, with one of these being potentially in the habitable zone. Because of its debris disk, any planet orbiting Tau Ceti would face far more impact events than the Earth. Despite this hurdle to habitability, its solar analog (Sun-like) characteristics have led to widespread interest in the star. Given its stability, similarity and relative proximity to the Sun, Tau Ceti is consistently listed as a target for the Search for Extra-Terrestrial Intelligence (SETI), and it appears in some science fiction literature.\r\rIt can be seen with the unaided eye as a third-magnitude star.[nb 2] As seen from Tau Ceti, the Sun would be a third-magnitude star in the constellation Bootes.[nb 3]",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "52 Ceti, Tau Ceti, HIP 8102, SAO 147986, HD 10700, GC 2123, HR 509, DM BD-16   295, TYC 5855-2292-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Tau Ceti",
	"OType" : "Star",
	"Distance" : "3.65",
	"RA_S" : 26.021158,
	"DEC_S" : -15.939506,
	"X" : 354,
	"Y" : 448,
	"Constellation" : "Cetus ",
	"AMag" : 3.572,
	"key" : 59815,
	"title" : "Tau Ceti"
	},
{
	"Index" : "35519",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "53 Ceti, Chi Ceti, HIP 8497, SAO 148036, HD 11171, GC 2212, HR 531, DM BD-11   352, TYC 5278-2438-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Chi Ceti",
	"OType" : "Star",
	"Distance" : "23.18",
	"RA_S" : 27.39626495,
	"DEC_S" : -10.68641272,
	"Constellation" : "Cetus ",
	"AMag" : 4.694,
	"key" : 55519,
	"title" : "Chi Ceti"
	},
{
	"Index" : "35518",
	"Description" : "Zeta Ceti (\u03B6 Cet, \u03B6 Ceti) is a star in the constellation Cetus. It has the traditional name Baten Kaitos (Arabic batn qaytus \u0628\u0637\u0646 \u0642\u064A\u062A\u0648\u0633 - \u0022belly of the sea monster\u0022).\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Rabah al Naamat (\u0631\u0627\u0628\u0639 \u0623\u0644\u0646\u0639\u0627\u0645\u0629 - raabi3 al na\u02BD\u0101m\u0101t), which was translated into Latin as Quarta Struthionum, meaning the fourth ostrich. This star, along with \u03B7 Cet (Deneb Algenubi), \u03B8 Cet (Thanih Al Naamat), \u03C4 Cet (Thalath Al Naamat), and \u03C5 Cet, were Al Na\u02BD\u0101m\u0101t (\u0623\u0644\u0646\u0639\u0627\u0645\u0629), the Hen Ostriches.\r\rIn Chinese, \u5929\u5009 (Ti\u0101n C\u0101ng), meaning Square Celestial Granary, refers to an asterism consisting of \u03B6 Ceti, \u03B9 Ceti, \u03B8 Ceti, \u03B7 Ceti, \u03C4 Ceti and 57 Ceti. Consequently, \u03B6 Ceti itself is known as \u5929\u5009\u56DB (Ti\u0101n C\u0101ng s\u00EC, English: the Second Star of Square Celestial Granary.)\r\rZeta Ceti is a yellowish star of spectral class K0 IIIBa0.1 and is approximately 260 light years from the Earth. Its apparent magnitude is +3.9.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "55 Ceti, Zeta Ceti, HIP 8645, SAO 148059, HD 11353, GC 2249, HR 539, DM BD-11   359, TYC 5278-2437-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Baten Kaitos",
	"OType" : "Spectroscopic binary",
	"Distance" : "71.9",
	"RA_S" : 27.86513636,
	"DEC_S" : -10.33504177,
	"X" : 331,
	"Y" : 375,
	"Constellation" : "Cetus ",
	"AMag" : 3.851,
	"key" : 55518,
	"shortTitle" : "Baten Kajtos",
	"title" : "Baten Kaitos"
	},
{
	"Index" : "44241",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "56 Ceti, HIP 9061, SAO 167416, HD 11930, GC 2343, HR 565, DM CD-23   721, TYC 6429-656-1",
	"group" : { "key" : "Cetus" },
	"Common" : "56 Ceti",
	"OType" : "Star",
	"Distance" : "107.99",
	"RA_S" : 29.16749111,
	"DEC_S" : -22.52678333,
	"Constellation" : "Cetus ",
	"AMag" : 5.057,
	"key" : 64241,
	"title" : "56 Ceti"
	},
{
	"Index" : "39856",
	"Description" : "Upsilon Ceti (\u03C5 Ceti, \u03C5 Cet) is a Class K5, fourth-magnitude star in the constellation Cetus. Upsilon Ceti is a red-orange giant star located about 300 light-years from Earth.\r\rThis star with \u03B7 Cet (Deneb Algenubi), \u03B8 Cet (Thanih al Naamat), \u03C4 Cet (Durre Menthor) and \u03B6 Cet (Baten Kaitos), were Al Na\u02BD\u0101m\u0101t (\u0623\u0644\u0646\u0639\u0627\u0645\u0629), the Hen Ostriches\r\rIn Chinese, \u9207\u9455 (F\u016B Zh\u00EC), meaning Sickle, refers to an asterism consisting of \u03C5 Ceti, 48 Ceti and 56 Ceti. Consequently, \u03C5 Ceti itself is known as \u9207\u9455\u56DB (F\u016B Zh\u00EC s\u00EC, English: the Fourth Star of Sickle.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "59 Ceti, Upsilon Ceti, HIP 9347, SAO 167471, HD 12274, GC 2419, HR 585, DM BD-21   358, TYC 5858-2053-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Upsilon Ceti",
	"OType" : "Star",
	"Distance" : "89.74",
	"RA_S" : 30.00128716,
	"DEC_S" : -21.07782992,
	"X" : 306,
	"Y" : 516,
	"Constellation" : "Cetus ",
	"AMag" : 4.167,
	"key" : 59856,
	"title" : "Upsilon Ceti"
	},
{
	"Index" : "23142",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "60 Ceti, HIP 9589, SAO 129655, HD 12573, GC 2474, HR 607, DM BD-00   307, TYC 37-1318-1",
	"group" : { "key" : "Cetus" },
	"Common" : "60 Ceti",
	"OType" : "Star",
	"Distance" : "86.08",
	"RA_S" : 30.79854556,
	"Constellation" : "Cetus ",
	"AMag" : 5.444,
	"key" : 43142,
	"title" : "60 Ceti"
	},
{
	"Index" : "43409",
	"Description" : "Xi1 Ceti (\u03BE1 Ceti), is a binary system located in the constellation Cetus, suspected as a ternary.\r\rIn Chinese, \u5929\u56F7 (Ti\u0101n Q\u016Bn), meaning Circular Celestial Granary, refers to an asterism consisting of \u03B1 Ceti, \u03BA1 Ceti, \u03BB Ceti, \u03BC Ceti, \u03BE1 Ceti, \u03BE2 Ceti, \u03BD Ceti, \u03B3 Ceti, \u03B4 Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, Xi1 Ceti itself is known as the Fifth Star of Circular Celestial Granary, Ti\u0101n Q\u016Bn Wu.\r\rXi1 Ceti A is an G6III or G8III clump-giant star. Xi1 Ceti B is a spectroscopic binary to the primary. It is an A2V dwarf of about 2 solar masses and 30 luminosity. It is separated at 0.012 arcsec so in an orbit of 4.2 AU, smaller than the distance between Jupiter and the Sun.\r\rXi1 Ceti A exhibits characteristics similar to an eclipsing binary, with a small white dwarf companion. Occultations with the moon have not yet confirmed the existence of the second suspected companion.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "65 Ceti, Xi01 Ceti, HIP 10324, SAO 110408, HD 13611, GC 2656, HR 649, DM BD+08   345, TYC 631-1493-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Xi1 Ceti",
	"OType" : "Eclipsing binary",
	"Distance" : "117",
	"RA_S" : 33.24998635,
	"DEC_S" : 8.84672997,
	"X" : 259,
	"Y" : 126,
	"Constellation" : "Cetus ",
	"AMag" : 4.453,
	"key" : 63409,
	"title" : "Xi1 Ceti"
	},
{
	"Index" : "24646",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "69 Ceti, HIP 11021, SAO 110495, HD 14652, GC 2846, HR 689, DM BD-00   355, TYC 39-1275-1",
	"group" : { "key" : "Cetus" },
	"Common" : "69 Ceti",
	"OType" : "Variable Star",
	"Distance" : "327.14",
	"RA_S" : 35.48595042,
	"Constellation" : "Cetus ",
	"AMag" : 5.489,
	"key" : 44646,
	"title" : "69 Ceti"
	},
{
	"Index" : "35579",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 11029, SAO 148354, HD 14691, GC 2849, HR 692, DM BD-11  448, TYC 5282-2511-1",
	"group" : { "key" : "Cetus" },
	"Common" : "HR 692",
	"OType" : "Star",
	"Distance" : "29.65",
	"RA_S" : 35.50638671,
	"DEC_S" : -10.77753306,
	"Constellation" : "Cetus ",
	"AMag" : 5.465,
	"key" : 55579,
	"title" : "HR 692"
	},
{
	"Index" : "31180",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "70 Ceti, HIP 11046, SAO 129858, HD 14690, GC 2850, HR 691, DM BD-01   322, TYC 4691-1115-1",
	"group" : { "key" : "Cetus" },
	"Common" : "70 Ceti",
	"OType" : "Star",
	"Distance" : "80.07",
	"RA_S" : 35.55164999,
	"DEC_S" : -0.88485452,
	"Constellation" : "Cetus ",
	"AMag" : 5.459,
	"key" : 51180,
	"title" : "70 Ceti"
	},
{
	"Index" : "35604",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "72 Ceti, Rho Ceti, HIP 11345, SAO 148385, HD 15130, GC 2932, HR 708, DM BD-12   451, TYC 5284-2546-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Rho Ceti",
	"OType" : "Star",
	"Distance" : "139.64",
	"RA_S" : 36.48752289,
	"DEC_S" : -12.29047913,
	"Constellation" : "Cetus ",
	"AMag" : 4.862,
	"key" : 55604,
	"title" : "Rho Ceti"
	},
{
	"Index" : "43463",
	"Description" : "Xi2 Ceti (\u03BE2 Ceti), is a star located in the constellation Cetus.\r\rIn Chinese, \u5929\u56F7 (Ti\u0101n Q\u016Bn), meaning Circular Celestial Granary, refers to an asterism consisting of \u03B1 Ceti, \u03BA1 Ceti, \u03BB Ceti, \u03BC Ceti, \u03BE1 Ceti, \u03BE2 Ceti, \u03BD Ceti, \u03B3 Ceti, \u03B4 Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, Xi2 Ceti itself is known as the Sixth Star of Circular Celestial Granary, Ti\u0101n Q\u016Bn Li\u00F9.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "73 Ceti, Xi02 Ceti, HIP 11484, SAO 110543, HD 15318, GC 2960, HR 718, DM BD+07   388, TYC 632-1491-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Xi2 Ceti",
	"OType" : "Star",
	"Distance" : "58.84",
	"RA_S" : 37.03975201,
	"DEC_S" : 8.46007064,
	"X" : 209,
	"Y" : 133,
	"Constellation" : "Cetus ",
	"AMag" : 4.261,
	"key" : 63463,
	"title" : "Xi2 Ceti"
	},
{
	"Index" : "30595",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "HIP 11738, SAO 110589, HD 15694, GC 3029, HR 737, DM BD+01  438, TYC 46-1631-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Gliese 9083 (HR 737)",
	"OType" : "Star",
	"Distance" : "140.41",
	"RA_S" : 37.87540008,
	"DEC_S" : 2.26718375,
	"Constellation" : "Cetus ",
	"AMag" : 5.411,
	"key" : 50595,
	"title" : "Gliese 9083 (HR 737)"
	},
{
	"Index" : "39884",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "76 Ceti, Sigma Ceti, HIP 11783, SAO 148445, HD 15798, GC 3045, HR 740, DM BD-15   449, TYC 5860-2587-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Sigma Ceti",
	"OType" : "Double or multiple star",
	"Distance" : "26.69",
	"RA_S" : 38.021805,
	"DEC_S" : -15.2446155,
	"Constellation" : "Cetus ",
	"AMag" : 4.792,
	"key" : 59884,
	"title" : "Sigma Ceti"
	},
{
	"Index" : "31230",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "75 Ceti, HIP 11791, SAO 129959, HD 15779, GC 3043, HR 739, DM BD-01   353, TYC 4698-1302-1",
	"group" : { "key" : "Cetus" },
	"Common" : "75 Ceti",
	"OType" : "Horizontal Branch Star",
	"Distance" : "81.3",
	"RA_S" : 38.03926272,
	"DEC_S" : -1.03489431,
	"Constellation" : "Cetus ",
	"AMag" : 5.47,
	"key" : 51230,
	"title" : "75 Ceti"
	},
{
	"Index" : "34994",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "78 Ceti, Nu Ceti, HIP 12093, SAO 110635, HD 16161, GC 3117, HR 754, DM BD+04   418, TYC 52-1681-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Nu Ceti",
	"OType" : "Star",
	"Distance" : "104.2",
	"RA_S" : 38.96863357,
	"DEC_S" : 5.59324309,
	"Constellation" : "Cetus ",
	"AMag" : 4.968,
	"key" : 54994,
	"title" : "Nu Ceti"
	},
{
	"Index" : "30599",
	"Description" : "Delta Ceti (\u03B4 Ceti, \u03B4 Cet) is a Class B2, fourth-magnitude star in the constellation Cetus.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "82 Ceti, Delta Ceti, HIP 12387, SAO 110665, HD 16582, GC 3192, HR 779, DM BD-00   406, TYC 46-1633-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Delta Ceti",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "198.99",
	"RA_S" : 39.87064912,
	"X" : 173,
	"Y" : 240,
	"Constellation" : "Cetus ",
	"AMag" : 4.029,
	"key" : 50599,
	"title" : "Delta Ceti"
	},
{
	"Index" : "35632",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "83 Ceti, Epsilon Ceti, HIP 12390AB, SAO 148528, HD 16620, GC 3199, HR 781, DM BD-12   501, TYC 5288-1093-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Epsilon Ceti",
	"OType" : "Spectroscopic binary",
	"Distance" : "26.96",
	"RA_S" : 39.89091111,
	"DEC_S" : -11.87216242,
	"Constellation" : "Cetus ",
	"AMag" : 4.874,
	"key" : 55632,
	"title" : "Epsilon Ceti"
	},
{
	"Index" : "33894",
	"Description" : "Gamma Ceti (\u03B3 Cet, \u03B3 Ceti) is a star system in the equatorial constellation Cetus. It has the traditional name Kaffaljidhma and has an apparent visual magnitude of 3.47. Based upon parallax measurements, this star is located at a distance of about 80 light years (24.4 parsecs) from Earth.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "86 Ceti, Gamma Ceti, HIP 12706B, SAO 110707, HD 16970B, GC 3276, HR 804, DM BD+02   422, TYC 50-1721-2",
	"group" : { "key" : "Cetus" },
	"Common" : "Kaffaljidhma",
	"OType" : "High proper-motion Star",
	"Distance" : "24.4",
	"RA_S" : 40.824883,
	"DEC_S" : 3.236472,
	"X" : 159,
	"Y" : 202,
	"Constellation" : "Cetus ",
	"AMag" : 6.175,
	"key" : 53894,
	"shortTitle" : "Al Kaff al Jidhmah; Kaffalidma",
	"title" : "Kaffaljidhma"
	},
{
	"Index" : "33893",
	"Description" : "Gamma Ceti (\u03B3 Cet, \u03B3 Ceti) is a star system in the equatorial constellation Cetus. It has the traditional name Kaffaljidhma and has an apparent visual magnitude of 3.47. Based upon parallax measurements, this star is located at a distance of about 80 light years (24.4 parsecs) from Earth.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "86 Ceti, Gamma Ceti, HIP 12706A, SAO 110707, HD 16970A, GC 3276, HR 804, DM BD+02   422, TYC 50-1721-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Kaffaljidhma",
	"OType" : "High proper-motion Star",
	"Distance" : "24.4",
	"RA_S" : 40.8255,
	"DEC_S" : 3.236167,
	"X" : 159,
	"Y" : 202,
	"Constellation" : "Cetus ",
	"AMag" : 3.551,
	"key" : 53893,
	"shortTitle" : "Al Kaff al Jidhmah; Kaffalidma",
	"title" : "Kaffaljidhma"
	},
{
	"Index" : "35671",
	"Description" : "Pi Ceti (\u03C0 Ceti, \u03C0 Cet) is a Class B7, fourth-magnitude star in the constellation Cetus. Pi Ceti is a blue main-sequence star located about 440 light-years from Earth. It has about 8.1 times the radius of the Sun.\r\rThis star, along with \u03B5 Cet, \u03C1 Cet and \u03C3 Cet, was Al Sufi\u0027s Al Sadr al \u1E32ai\u1E6Dos, the Whale\u0027s Breast\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Sadr al \u1E32ai\u1E6Dos were the title for four stars :\u03C1 Cet as Al Sadr al \u1E32ai\u1E6Dos I, \u03C3 Cet as Al Sadr al \u1E32ai\u1E6Dos II, \u03B5 Cet as Al Sadr al \u1E32ai\u1E6Dos III and \u03C0 Cet as Al Sadr al \u1E32ai\u1E6Dos IV\r\rIn Chinese, \u5929\u82D1 (Ti\u0101n Yu\u00E0n), meaning Celestial Meadows, refers to an asterism consisting of \u03C0 Ceti, \u03B3 Eridani, \u03C0 Eridani, \u03B4 Eridani, \u03B5 Eridani, \u03B6 Eridani, \u03B7 Eridani, \u03C41 Eridani, \u03C42 Eridani, \u03C43 Eridani, \u03C44 Eridani, \u03C45 Eridani, \u03C46 Eridani, \u03C47 Eridani, \u03C48 Eridani and \u03C49 Eridani. Consequently, \u03B4 Ceti itself is known as \u5929\u82D1\u4E03 (Ti\u0101n Yu\u00E0n q\u012B, English: the Seventh Star of Celestial Meadows.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "89 Ceti, Pi Ceti, HIP 12770, SAO 148575, HD 17081, GC 3300, HR 811, DM BD-14   519, TYC 5292-970-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Pi Ceti",
	"OType" : "Spectroscopic binary",
	"Distance" : "120.39",
	"RA_S" : 41.03062246,
	"DEC_S" : -13.85870626,
	"X" : 164,
	"Y" : 427,
	"Constellation" : "Cetus ",
	"AMag" : 4.216,
	"key" : 55671,
	"title" : "Pi Ceti"
	},
{
	"Index" : "44378",
	"Description" : "Mu Ceti (\u03BC Ceti) is a binary system located in the constellation Cetus. Mu Ceti is a quadruple visual star system. The combined apparent magnitude of the system is +4.27, and is located 84 light years from the Sun.\r\rIn Chinese, \u5929\u56F7 (Ti\u0101n Q\u016Bn), meaning Circular Celestial Granary, refers to an asterism consisting of \u03B1 Ceti, \u03BA1 Ceti, \u03BB Ceti, \u03BC Ceti, \u03BE1 Ceti, \u03BE2 Ceti, \u03BD Ceti, \u03B3 Ceti, \u03B4 Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, Mu Ceti itself is known as the Fourth Star of Circular Celestial Granary.\r\rMu Ceti A is an F0V subgiant, believed to be a Delta Scuti variable star.\r\rThe other components, Mu Ceti B, C and D are G3V, G2V and G6V respectively. The dimmer components were all discovered during occultations of Mu Ceti by the Moon. One of them orbits at a period of 1202 days.",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "87 Ceti, Mu Ceti, HIP 12828, SAO 110723, HD 17094, GC 3309, HR 813, DM BD+09   359, TYC 643-937-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Mu Ceti",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "25.77",
	"RA_S" : 41.23559196,
	"DEC_S" : 10.11414303,
	"X" : 155,
	"Y" : 111,
	"Constellation" : "Cetus ",
	"AMag" : 4.305,
	"key" : 64378,
	"title" : "Mu Ceti"
	},
{
	"Index" : "44101",
	"Description" : "Lambda Ceti (\u03BB Cet, \u03BB Ceti) is Class B star of fifth-magnitude star located in the constellation Cetus. Historically, the star bore the traditional name Menkar, although today that name is more commonly associated with \u03B1 Ceti.\r\rThis star, along with \u03B1 Cet (Menkar), \u03B3 Cet (Kaffaljidhma), \u03B4 Cet, \u03BC Cet, \u03BE1 Cet and \u03BE2 Cet were Al Kaff al Jidhmah, \u0022the Part of a Hand\u0022.\r\rIn Chinese, \u5929\u56F7 (Ti\u0101n Q\u016Bn), meaning Circular Celestial Granary, refers to an asterism consisting of \u03BB Ceti, \u03B1 Ceti, \u03BA1 Ceti, \u03BC Ceti, \u03BE1 Ceti, \u03BE2 Ceti, \u03BD Ceti, \u03B3 Ceti, \u03B4 Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, \u03BB Ceti itself is known as \u5929\u56F7\u4E09 (Ti\u0101n Q\u016Bn s\u0101n, English: the Third Star of Circular Celestial Granary.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "91 Ceti, Lambda Ceti, HIP 13954, SAO 110889, HD 18604, GC 3595, HR 896, DM BD+08   455, TYC 641-985-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Lambda Ceti",
	"OType" : "Star",
	"Distance" : "176.3",
	"RA_S" : 44.92874947,
	"DEC_S" : 8.9073583,
	"X" : 106,
	"Y" : 128,
	"Constellation" : "Cetus ",
	"AMag" : 4.681,
	"key" : 64101,
	"title" : "Lambda Ceti"
	},
{
	"Index" : "39451",
	"Description" : "Alpha Ceti (\u03B1 Cet, \u03B1 Ceti) is a star in the constellation of Cetus. It has the traditional name Menkar or Menkab. The name Menkar derives from the Arabic word \u0645\u0646\u062E\u0631 man\u0127ar \u0022nostril\u0022 (of Cetus).\r\rThis star, along with \u03B3 Cet (Kaffaljidhma), \u03B4 Cet, \u03BB Cet (Menkar), \u03BC Cet, \u03BE1 Cet and \u03BE2 Cet were Al Kaff al Jidhmah, \u0022the Part of a Hand\u0022.\r\rIn Chinese, \u5929\u56F7 (Ti\u0101n Q\u016Bn), meaning Circular Celestial Granary, refers to an asterism consisting of \u03B1 Ceti, \u03BA1 Ceti, \u03BB Ceti, \u03BC Ceti, \u03BE1 Ceti, \u03BE2 Ceti, \u03BD Ceti, \u03B3 Ceti, \u03B4 Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, \u03B1 Ceti itself is known as \u5929\u56F7\u4E00 (Ti\u0101n Q\u016Bn y\u012B, English: the First Star of Circular Celestial Granary.)",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "92 Ceti, Alpha Ceti, HIP 14135, SAO 110920, HD 18884, GC 3643, HR 911, DM BD+03   419, TYC 58-1618-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Menkar / Menkab",
	"OType" : "Long Period Variable candidate",
	"Distance" : "76.29",
	"RA_S" : 45.56988422,
	"DEC_S" : 4.08973824,
	"X" : 98,
	"Y" : 192,
	"Constellation" : "Cetus ",
	"AMag" : 2.716,
	"key" : 59451,
	"shortTitle" : "Mekab; Menkab; Monkar; Mentar",
	"title" : "Menkar / Menkab"
	},
{
	"Index" : "31311",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "94 Ceti, HIP 14954, SAO 130355, HD 19994, GC 3838, HR 962, DM BD-01   457, TYC 4708-1423-1",
	"group" : { "key" : "Cetus" },
	"Common" : "94 Ceti",
	"OType" : "Double or multiple star",
	"Distance" : "22.58",
	"RA_S" : 48.19348407,
	"DEC_S" : -1.19610464,
	"Constellation" : "Cetus ",
	"AMag" : 5.135,
	"key" : 51311,
	"title" : "94 Ceti"
	},
{
	"Index" : "40361",
	"MapNum" : "16",
	"ImageNum" : "16",
	"Desig" : "96 Ceti, Kappa Ceti, HIP 15457, SAO 111120, HD 20630, GC 3969, HR 996, DM BD+02   518, TYC 59-1947-1",
	"group" : { "key" : "Cetus" },
	"Common" : "Kappa Ceti",
	"OType" : "Variable of BY Dra type",
	"Distance" : "9.14",
	"RA_S" : 49.84040284,
	"DEC_S" : 3.37019796,
	"Constellation" : "Cetus ",
	"AMag" : 4.919,
	"key" : 60361,
	"title" : "Kappa Ceti"
	},
{
	"Index" : "70447",
	"Description" : "Alpha Chamaeleontis (\u03B1 Cha, \u03B1 Chamaeleontis) is a star in the constellation Chamaeleon. It has about the same mass as the Sun.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Alpha Chamaeleontis, HIP 40702, SAO 256496, HD 71243, GC 11419, HR 3318, DM CP-76   507, TYC 9398-2714-1",
	"group" : { "backgroundImage" : "images/Alignment/13.png",
		"description" : "Chamaeleon (/k\u0259\u02C8mi\u02D0li\u0259n/) is a small constellation in the southern sky. It is named after the chameleon, a form of lizard. It was first defined in the 16th century.\r\rChamaeleon was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. It first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius and Jodocus Hondius. Johann Bayer was the first uranographer to put Chamaeleon in a celestial atlas. It was one of many constellations created by European explorers in the 15th and 16th centuries out of unfamiliar Southern Hemisphere stars.",
		"key" : "Chamaeleon",
		"grouptype" : "Chamaeleon",
		"Meaning" : "chameleon",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Chamaeleon",
		"title" : "Chamaeleon Objects Group" },
	"Common" : "Alpha Chamaeleontis",
	"OType" : "Star",
	"Distance" : "19.56",
	"RA_S" : 124.63146692,
	"DEC_S" : -76.91972218,
	"X" : 388,
	"Y" : 481,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.095,
	"key" : 90447,
	"title" : "Alpha Chamaeleontis"
	},
{
	"Index" : "70448",
	"Description" : "Theta Chamaeleontis (t Cha), is a star located in the constellation Chamaeleon. Theta Chamaeleontis is also known as HR 3340, and HD 71701. Theta Chamaeleontis is located at Right Ascension 08h 20m 38 sec and Declination -77 deg 29 arcmin 04 arcsec. Theta Chamaeleontis is a binary star system.\r\rTheta Chamaeleontis A is an K0III giant star with an effective temperature of 5000 Kelvin. It has an apparent visual magnitude of +4.35, an absolute magnitude of +.974 and a mass of 3 solar masses. It is located 47 pc (153 light years) from the Sun.\r\rTheta Chamaeleontis B is a white dwarf star with apparent visual magnitude of 12.05. The angular separation between Theta A and Theta B is 31 arcsec.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Theta Chamaeleontis, HIP 40888, SAO 256503, HD 71701, GC 11481, HR 3340, DM CP-77   383, TYC 9398-2715-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Theta Chamaeleontis",
	"OType" : "Star",
	"Distance" : "47.62",
	"RA_S" : 125.16057901,
	"DEC_S" : -77.48447572,
	"X" : 386,
	"Y" : 488,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.467,
	"key" : 90448,
	"title" : "Theta Chamaeleontis"
	},
{
	"Index" : "70476",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Eta Chamaeleontis, HIP 42637, SAO 256543, HD 75416, GC 12063, HR 3502, DM CP-78   372, TYC 9403-1986-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Eta Chamaeleontis",
	"OType" : "Star",
	"Distance" : "94.94",
	"RA_S" : 130.33131377,
	"DEC_S" : -78.96335963,
	"Constellation" : "Chamaeleon ",
	"AMag" : 5.437,
	"key" : 90476,
	"title" : "Eta Chamaeleontis"
	},
{
	"Index" : "70501",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Iota Chamaeleontis, HIP 46107, SAO 258530, HD 82554, GC 13066, HR 3795, DM CP-80   350, TYC 9408-1798-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Iota Chamaeleontis",
	"OType" : "High proper-motion Star",
	"Distance" : "58.13",
	"RA_S" : 141.03842815,
	"DEC_S" : -80.7868751,
	"Constellation" : "Chamaeleon ",
	"AMag" : 5.39,
	"key" : 90501,
	"title" : "Iota Chamaeleontis"
	},
{
	"Index" : "70502",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Zeta Chamaeleontis, HIP 46928, SAO 258538, HD 83979, GC 13308, HR 3860, DM CP-80   365, TYC 9408-1799-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Zeta Chamaeleontis",
	"OType" : "Variable Star",
	"Distance" : "175.29",
	"RA_S" : 143.4723918,
	"DEC_S" : -80.9412587,
	"Constellation" : "Chamaeleon ",
	"AMag" : 5.037,
	"key" : 90502,
	"title" : "Zeta Chamaeleontis"
	},
{
	"Index" : "70464",
	"Description" : "Gamma Chamaeleonitis (y Cha), is a star located in the constellation Chamaeleon. Gamma Chamaeleontis is also known as HR 4174, and HD 92305. The star is located at Right Ascension 10h 35m 28.l sec and Declination -78 deg 38 arcmin 28 arcsec.\r\rGamma Chamaeleontis is an M0III Giant star with an effective temperature of 3700 Kelvin. It has an apparent visual magnitude of +4.11, and an absolute visual magnitude of -1.4. It is located 127 parsecs, (413 light years) from the sun and has a mass of 1.2 solar masses. Gamma Chamaeleontis is an irregular variable star.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Gamma Chamaeleontis, HIP 51839, SAO 256731, HD 92305, GC 14604, HR 4174, DM CP-77   622, TYC 9401-1714-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Gamma Chamaeleontis",
	"OType" : "Variable Star",
	"Distance" : "128",
	"RA_S" : 158.86711446,
	"DEC_S" : -78.60778663,
	"X" : 300,
	"Y" : 519,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.277,
	"key" : 90464,
	"title" : "Gamma Chamaeleontis"
	},
{
	"Index" : "70576",
	"Description" : "Delta2 Chamaeleontis (d2 Cha), is a star located in the constellation Chamaeleon. Delta2 Chamaeleontis is also known as HR 4234, and HD 93845. Delta2 Chamaeleontis is located at Right Ascension 10h 45m 46.8 sec and Declination -80 deg 32 arcmin 25 arcsec.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Delta02 Chamaeleontis, HIP 52633, SAO 258593, HD 93845, GC 14863, HR 4234, DM CP-79   556, TYC 9418-2653-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Delta2 Chamaeleontis",
	"OType" : "Star",
	"Distance" : "107.5",
	"RA_S" : 161.44584864,
	"DEC_S" : -80.5401905,
	"X" : 307,
	"Y" : 544,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.404,
	"key" : 90576,
	"title" : "Delta2 Chamaeleontis"
	},
{
	"Index" : "70560",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Epsilon Chamaeleontis, HIP 58484AB, SAO 256894, HD 104174, GC 16402, HR 4583, DM CP-77   772, TYC 9415-3217-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Epsilon Chamaeleontis",
	"OType" : "Star",
	"Distance" : "110.8",
	"RA_S" : 179.90650682,
	"DEC_S" : -78.22185407,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.908,
	"key" : 90560,
	"title" : "Epsilon Chamaeleontis"
	},
{
	"Index" : "70540",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Kappa Chamaeleontis, HIP 58905, SAO 256899, HD 104902, GC 16497, HR 4605, DM CP-75   777, TYC 9412-2483-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Kappa Chamaeleontis",
	"OType" : "Star",
	"Distance" : "146",
	"RA_S" : 181.19363066,
	"DEC_S" : -76.51906023,
	"Constellation" : "Chamaeleon ",
	"AMag" : 5.201,
	"key" : 90540,
	"title" : "Kappa Chamaeleontis"
	},
{
	"Index" : "70585",
	"Description" : "Beta Chamaeleontis (Beta Cha, \u03B2 Chamaeleontis, \u03B2 Cha) is a B-type main sequence star and is the third brightest star in the constellation of Chamaeleon. It has an apparent visual magnitude which varies between 4.24 and 4.30.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Beta Chamaeleontis, HIP 60000, SAO 256924, HD 106911, GC 16775, HR 4674, DM CP-78   741, TYC 9420-1543-1",
	"group" : { "key" : "Chamaeleon" },
	"Common" : "Beta Chamaeleontis",
	"OType" : "Variable Star",
	"Distance" : "91.47",
	"RA_S" : 184.58676993,
	"DEC_S" : -79.31223842,
	"X" : 257,
	"Y" : 567,
	"Constellation" : "Chamaeleon ",
	"AMag" : 4.209,
	"key" : 90585,
	"title" : "Beta Chamaeleontis"
	},
{
	"Index" : "67274",
	"Description" : "Alpha Circini (\u03B1 Cir, \u03B1 Circini) is a variable star in the faint, southern, circumpolar constellation of Circinus. At an apparent visual magnitude of 3.19, it is the brightest star in the constellation and can be readily seen with the naked eye from the southern hemisphere. Parallax measurements of this star yield an estimated distance of 54.0 light-years (16.6 parsecs) from the Earth.\r\rThis star belongs to a class of variables known as rapidly oscillating Ap stars. It oscillates with multiple, non-radial pulsation cycles and a dominant cycle of 6.8 minutes. The spectrum shows peculiar features caused by chemical stratification of the outer atmosphere. It displays a moderate deficiency of carbon, nitrogen and oxygen, while there is an overabundance of chromium (Cr). The stellar classification of A7 Vp SrCrEu indicates that this is a main sequence star with enhanced levels of strontium (Sr), chromium, and europium (Eu) in its atmosphere (compared to a typical star like the Sun).\r\rThe mass of Alpha Circini is about 150% to 170% the mass of the Sun and it has double the Sun\u0027s radius, while the luminosity is more than 10 times that of the Sun. The effective temperature of the outer envelope is about 7,500 K, giving it the white hue typical of A-type stars. It is rotating with a period of 4.5 days and the pole is inclined by about 37 \u00B1 4\u00B0 to the line of sight from the Earth.\r\rBased upon its location and motion through space, Alpha Circini is a candidate member of a stellar kinematic group known as the Beta Pictoris moving group. This group shares a common origin and has an estimated age of about 12 million years. At the birth of this group, Alpha Circini was estimated to be located at a distance of about 91 ly (28 pc) from the center of the assemblage.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Alpha Circini, HIP 71908, SAO 252853, HD 128898, GC 19772, HR 5463, DM CP-64  2977, TYC 9015-1445-1",
	"group" : { "backgroundImage" : "images/Alignment/03.png",
		"description" : "Circinus is a small and faint constellation in the southern sky, first defined in 1756 by French astronomer Nicolas Louis de Lacaille. Its name is Latin for compass, referring to the drafting tool used for drawing circles (it should not be confused with Pyxis, a constellation that represents a mariner\u0027s compass). Its brightest star is Alpha Circini, with an apparent magnitude of 3.19. Slightly variable, it is the brightest rapidly oscillating Ap star in the night sky. Theta and AX Circini are the most prominent variable stars in the constellation. Two sun-like stars have planetary systems: HD 134060 has two small planets, and HD 129445 has a Jupiter-like planet. Supernova SN 185 appeared in Circinus in 185 AD and was recorded by Chinese observers. Two novae were observed more recently, in the 20th century.\r\rThe Milky Way runs through the constellation, featuring prominent objects such as the open cluster NGC 5823 and the planetary nebula NGC 5315. Circinus hosts one notable spiral galaxy, the Circinus Galaxy, which was discovered in 1977 and is the closest Seyfert galaxy to the Milky Way. The Alpha Circinids (ACI), a meteor shower also discovered in 1977, radiate from this constellation.\r\rIn 1756, French astronomer Nicolas Louis de Lacaille introduced the constellation of Circinus with the French name le Compas, representing a pair of dividing compasses. It had first been depicted on one of Lacaille\u0027s maps in 1754, but it was unnamed. Lacaille portrayed the constellations of Norma, Circinus and Triangulum Australe, respectively, as a set square and ruler, a compass, and a surveyor\u0027s level in a set of draughtsman instruments, in his 1756 map of the southern stars. Circinus was given its current name in 1763, when Lacaille published an updated sky map with Latin names for the constellations he introduced.",
		"key" : "Circinus",
		"grouptype" : "Circinus",
		"Meaning" : "compass (drawing tool)",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Circinus",
		"title" : "Circinus Objects Group" },
	"Common" : "Alpha Circini",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "16.57",
	"RA_S" : 220.62675238,
	"DEC_S" : -64.97513751,
	"X" : 441,
	"Y" : 378,
	"Constellation" : "Circinus ",
	"AMag" : 3.189,
	"key" : 87274,
	"title" : "Alpha Circini"
	},
{
	"Index" : "67243",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 72131, SAO 252869, HD 129422, GC 19832, HR 5482, DM CP-62 4275, TYC 9011-5652-1",
	"group" : { "key" : "Circinus" },
	"Common" : "HR 5482",
	"OType" : "Star",
	"Distance" : "48.44",
	"RA_S" : 221.32222718,
	"DEC_S" : -62.87564935,
	"Constellation" : "Circinus ",
	"AMag" : 5.396,
	"key" : 87243,
	"title" : "HR 5482"
	},
{
	"Index" : "67343",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 73036, SAO 242111, HD 131342, GC 20054, HR 5546, DM CP-59 5753, TYC 9020-2567-1",
	"group" : { "key" : "Circinus" },
	"Common" : "HR 5546",
	"OType" : "Star",
	"Distance" : "49.41",
	"RA_S" : 223.894002,
	"DEC_S" : -60.11416394,
	"Constellation" : "Circinus ",
	"AMag" : 5.31,
	"key" : 87343,
	"title" : "HR 5546"
	},
{
	"Index" : "67397",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Theta Circini, HIP 73129, SAO 252965, HD 131492, GC 20067, HR 5551, DM CP-62  4337, TYC 9024-1862-1",
	"group" : { "key" : "Circinus" },
	"Common" : "Theta Circini",
	"OType" : "Be Star",
	"Distance" : "453.16",
	"RA_S" : 224.18328451,
	"DEC_S" : -62.78101019,
	"Constellation" : "Circinus ",
	"AMag" : 5.028,
	"key" : 87397,
	"title" : "Theta Circini"
	},
{
	"Index" : "67439",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Eta Circini, HIP 73776, SAO 253005, HD 132905, GC 20242, HR 5593, DM CP-63  3493, TYC 9028-336-1",
	"group" : { "key" : "Circinus" },
	"Common" : "Eta Circini",
	"OType" : "Star",
	"Distance" : "84.54",
	"RA_S" : 226.20077486,
	"DEC_S" : -64.03134878,
	"Constellation" : "Circinus ",
	"AMag" : 5.272,
	"key" : 87439,
	"title" : "Eta Circini"
	},
{
	"Index" : "67363",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Delta Circini, HIP 74778, SAO 253084, HD 135240, GC 20507, HR 5664, DM CP-60  5701, TYC 9021-2243-1",
	"group" : { "key" : "Circinus" },
	"Common" : "Delta Circini",
	"OType" : "Spectroscopic binary",
	"RA_S" : 229.23705765,
	"DEC_S" : -60.95725531,
	"Constellation" : "Circinus ",
	"AMag" : 5.072,
	"key" : 87363,
	"title" : "Delta Circini"
	},
{
	"Index" : "64210",
	"Description" : "Beta Circini (Beta Cir, \u03B2 Circini, \u03B2 Cir) is an A-type main sequence star and is the second brightest star in the constellation of Circinus. It has an apparent visual magnitude of approximately 4.069.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Beta Circini, HIP 74824, SAO 242384, HD 135379, GC 20526, HR 5670, DM CP-58  5875, TYC 8706-1061-1",
	"group" : { "key" : "Circinus" },
	"Common" : "Beta Circini",
	"OType" : "Star",
	"Distance" : "30.55",
	"RA_S" : 229.37854232,
	"DEC_S" : -58.80120481,
	"X" : 392,
	"Y" : 295,
	"Constellation" : "Circinus ",
	"AMag" : 4.071,
	"key" : 84210,
	"title" : "Beta Circini"
	},
{
	"Index" : "67417",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Epsilon Circini, HIP 74837, SAO 253088, HD 135291, GC 20519, HR 5666, DM CP-63  3544, TYC 9025-910-1",
	"group" : { "key" : "Circinus" },
	"Common" : "Epsilon Circini",
	"OType" : "Star",
	"Distance" : "124.46",
	"RA_S" : 229.41205229,
	"DEC_S" : -63.61046633,
	"Constellation" : "Circinus ",
	"AMag" : 4.99,
	"key" : 87417,
	"title" : "Epsilon Circini"
	},
{
	"Index" : "67362",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 74941, SAO 253101, HD 135591, GC 20549, HR 5680, DM CP-60 5720, TYC 9021-2242-1",
	"group" : { "key" : "Circinus" },
	"Common" : "HR 5680",
	"OType" : "Star",
	"RA_S" : 229.70475714,
	"DEC_S" : -60.49633415,
	"Constellation" : "Circinus ",
	"AMag" : 5.418,
	"key" : 87362,
	"title" : "HR 5680"
	},
{
	"Index" : "64224",
	"Description" : "Gamma Circini (y Cir), is a star located in the constellation Circinus. Gamma Circini is also known as HR 5704, and HD 136415. Gamma Circini is a spectroscopic binary. The system is located at Right Ascension 15h 23m 23s and Declination -59 deg 19 arcmin 15 arcsec. The system has a combined apparent visual magnitude of +4.48, and is located at a distance of 156 pc (509 ly) from the Sun.\r\rGamma Circini A is a B5IV subgiant star, with an effective temperature of 15000 Kelvin. It has an apparent visual magnitude +5.1, an absolute magnitude of -1.49 and a mass of 5 solar masses. Gamma Circini A is a Be Lacertae variable star.\r\rGamma Circini B, also known as HD 136416, is a F8V dwarf star, with an effective temperature of 6000 Kelvin. It has an apparent visual magnitude of +5.5, and a mass of 1.2 solar masses.\r\rThe angular separation between A and B is approximately 2 arcsec.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma Circini, HIP 75323B, SAO 242463, HD 136415J, GC 20663, HR 5704, DM CP-58  5908A, TYC 8707-1990-2",
	"group" : { "key" : "Circinus" },
	"Common" : "HR 5704",
	"OType" : "Double or multiple star",
	"Distance" : "135.53",
	"RA_S" : 230.84434558,
	"DEC_S" : -59.32078142,
	"X" : 382,
	"Y" : 301,
	"Constellation" : "Circinus ",
	"AMag" : 4.48,
	"key" : 84224,
	"title" : "HR 5704"
	},
{
	"Index" : "64223",
	"Description" : "Gamma Circini (y Cir), is a star located in the constellation Circinus. Gamma Circini is also known as HR 5704, and HD 136415. Gamma Circini is a spectroscopic binary. The system is located at Right Ascension 15h 23m 23s and Declination -59 deg 19 arcmin 15 arcsec. The system has a combined apparent visual magnitude of +4.48, and is located at a distance of 156 pc (509 ly) from the Sun.\r\rGamma Circini A is a B5IV subgiant star, with an effective temperature of 15000 Kelvin. It has an apparent visual magnitude +5.1, an absolute magnitude of -1.49 and a mass of 5 solar masses. Gamma Circini A is a Be Lacertae variable star.\r\rGamma Circini B, also known as HD 136416, is a F8V dwarf star, with an effective temperature of 6000 Kelvin. It has an apparent visual magnitude of +5.5, and a mass of 1.2 solar masses.\r\rThe angular separation between A and B is approximately 2 arcsec.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma Circini, HIP 75323A, SAO 242463, HD 136415, GC 20663, HR 5704, DM CP-58  5908A, TYC 8707-1990-1",
	"group" : { "key" : "Circinus" },
	"Common" : "HR 5704",
	"OType" : "Star",
	"Distance" : "135.53",
	"RA_S" : 230.844404,
	"DEC_S" : -59.320703,
	"X" : 382,
	"Y" : 301,
	"Constellation" : "Circinus ",
	"AMag" : 4.937,
	"key" : 84223,
	"title" : "HR 5704"
	},
{
	"Index" : "48962",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Omicron Columbae, HIP 24659, SAO 195721, HD 34642, GC 6495, HR 1743, DM CD-35  2214, TYC 7051-2305-1",
	"group" : { "backgroundImage" : "images/Alignment/10.png",
		"description" : "Columba is a small, faint constellation created in the late sixteenth century. Its name is Latin for dove. It is located just south of Canis Major and Lepus.\r\rColumba was created by Dutch astronomer Petrus Plancius in 1592 in order to differentiate the \u0027unformed stars\u0027 of the large constellation Canis Major. Plancius first depicted Columba on the small celestial planispheres of his large wall map of 1592. It is also shown on his smaller world map of 1594 and on early Dutch celestial globes.\r\rPlancius originally named the constellation Columba Noachi (\u0022Noah\u0027s Dove\u0022), referring to the dove that gave Noah the information that the Great Flood was receding. This name is found on early 17th-century celestial globes and star atlases (such as Bayer\u0027s Uranometria of 1603). Columba may also represent the dove released by Jason and the Argonauts at the Black Sea\u0027s mouth; it helped them navigate the dangerous Symplegades.\r\rIn the Society Islands, Alpha Columbae (Phaet) was called Ana-iva.",
		"key" : "Columba",
		"grouptype" : "Columba",
		"Meaning" : "dove",
		"Family" : "Heavenly Waters",
		"Origin" : "1592, Plancius, split from Canis Major",
		"shortTitle" : "Columba",
		"title" : "Columba Objects Group" },
	"Common" : "Omicron Columbae",
	"OType" : "High proper-motion Star",
	"Distance" : "32.44",
	"RA_S" : 79.37120592,
	"DEC_S" : -34.8952067,
	"Constellation" : "Columba ",
	"AMag" : 4.931,
	"key" : 68962,
	"title" : "Omicron Columbae"
	},
{
	"Index" : "49058",
	"Description" : "Epsilon Columbae, also known as Adeline\u0027s star is a giant star in the constellation Columba. It is approximately 531 light years from Earth.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Epsilon Columbae, HIP 25859, SAO 195924, HD 36597, GC 6846, HR 1862, DM CD-35  2348, TYC 7063-1179-1",
	"group" : { "key" : "Columba" },
	"Common" : "Epsilon Columbae",
	"OType" : "Star",
	"Distance" : "80.6",
	"RA_S" : 82.80314024,
	"DEC_S" : -35.4705184,
	"X" : 335,
	"Y" : 433,
	"Constellation" : "Columba ",
	"AMag" : 3.983,
	"key" : 69058,
	"title" : "Epsilon Columbae"
	},
{
	"Index" : "44794",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Nu02 Columbae, HIP 26460, SAO 170613, HD 37495, GC 7013, HR 1935, DM CD-28  2321, TYC 6501-1434-1",
	"group" : { "key" : "Columba" },
	"Common" : "Nu02 Columbae",
	"OType" : "Star",
	"Distance" : "40.79",
	"RA_S" : 84.43590859,
	"DEC_S" : -28.68969279,
	"Constellation" : "Columba ",
	"AMag" : 5.33,
	"key" : 64794,
	"title" : "Nu02 Columbae"
	},
{
	"Index" : "49067",
	"Description" : "Alpha Columbae (\u03B1 Columbae, \u03B1 Col) is the Bayer designation for a third magnitude star in the southern constellation of Columba. It has the traditional name of Phact, which is derived from the Arabic term for \u0022ring dove\u0022. It has an apparent visual magnitude of 2.6, making it the brightest member of Columba. Based upon parallax measurements made during the Hipparcos mission, Alpha Columbae is located at a distance of around 261 light-years (80 parsecs).",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Alpha Columbae, HIP 26634, SAO 196059, HD 37795, GC 7078, HR 1956, DM CD-34  2375, TYC 7064-1357-1",
	"group" : { "key" : "Columba" },
	"Common" : "Phact",
	"OType" : "Be Star",
	"Distance" : "80.05",
	"RA_S" : 84.9122543,
	"DEC_S" : -34.07410972,
	"X" : 313,
	"Y" : 414,
	"Constellation" : "Columba ",
	"AMag" : 2.608,
	"key" : 69067,
	"shortTitle" : "Phact; Phaet; Phad (also HD103287); Fakt",
	"title" : "Phact"
	},
{
	"Index" : "49074",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 26868, SAO 196098, HD 38170, GC 7150, HR 1973, DM CD-34 2401, TYC 7065-1558-1",
	"group" : { "key" : "Columba" },
	"Common" : "V* WZ Col",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "131.3",
	"RA_S" : 85.56330956,
	"DEC_S" : -34.66781547,
	"Constellation" : "Columba ",
	"AMag" : 5.276,
	"key" : 69074,
	"title" : "V* WZ Col"
	},
{
	"Index" : "49040",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Mu Columbae, HIP 27204, SAO 196149, HD 38666, GC 7230, HR 1996, DM CD-32  2538, TYC 7061-1617-1",
	"group" : { "key" : "Columba" },
	"Common" : "Mu Columbae",
	"OType" : "Variable Star",
	"Distance" : "404.93",
	"RA_S" : 86.49956186,
	"DEC_S" : -32.30643822,
	"Constellation" : "Columba ",
	"AMag" : 5.114,
	"key" : 69040,
	"title" : "Mu Columbae"
	},
{
	"Index" : "49101",
	"Description" : "Beta Columbae (\u03B2 Columbae, \u03B2 Col) is the second brightest star in the southern constellation of Columba. It has the traditional name Wezn (or Wazn), from the Arabic \u0648\u0632\u0646 \u0022weight\u0022. It has an apparent visual magnitude of 3.1, which is bright enough to be viewed with the naked eye even from an urban location. Parallax measurements place it at a distance of about 87.2 light-years (26.7 parsecs) from Earth.\r\rIn Chinese, \u5B50 (Z\u01D0), meaning Son, refers to an asterism consisting of \u03B2 Columbae and \u03BB Columbae. Consequently, \u03B2 Columbae itself is known as \u5B50\u4E8C (Z\u01D0 \u00E8r, English: the Second Star of Son.)",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Beta Columbae, HIP 27628, SAO 196240, HD 39425, GC 7364, HR 2040, DM CD-35  2546, TYC 7069-1482-1",
	"group" : { "key" : "Columba" },
	"Common" : "Wezn",
	"OType" : "High proper-motion Star",
	"Distance" : "26.73",
	"RA_S" : 87.73997009,
	"DEC_S" : -35.76830949,
	"X" : 283,
	"Y" : 436,
	"Constellation" : "Columba ",
	"AMag" : 3.231,
	"key" : 69101,
	"shortTitle" : "Wezn",
	"title" : "Wezn"
	},
{
	"Index" : "49083",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Lambda Columbae, HIP 27810, SAO 196276, HD 39764, GC 7416, HR 2056, DM CD-33  2599, TYC 7066-2023-1",
	"group" : { "key" : "Columba" },
	"Common" : "Lambda Columbae",
	"OType" : "Ellipsoidal variable Star",
	"Distance" : "102.51",
	"RA_S" : 88.27867161,
	"DEC_S" : -33.80136396,
	"Constellation" : "Columba ",
	"AMag" : 4.845,
	"key" : 69083,
	"title" : "Lambda Columbae"
	},
{
	"Index" : "49106",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Xi Columbae, HIP 28010, SAO 196316, HD 40176, GC 7481, HR 2087, DM CD-37  2487, TYC 7070-1723-1",
	"group" : { "key" : "Columba" },
	"Common" : "Xi Columbae",
	"OType" : "Star",
	"Distance" : "101.87",
	"RA_S" : 88.87464804,
	"DEC_S" : -37.12066004,
	"Constellation" : "Columba ",
	"AMag" : 5.083,
	"key" : 69106,
	"title" : "Xi Columbae"
	},
{
	"Index" : "49084",
	"Description" : "Gamma Columbae is a blue subgiant star in the constellation Columba. It is approximately 854 light years from Earth. This star, along with \u03B6 CMa, \u03BB CMa, \u03B4 Col, \u03B8 Col, \u03BA Col, \u03BB Col, \u03BC Col and \u03BE Col, were Al \u1E32ur\u016Bd (\u0623\u0644\u0642\u0631\u062F - al-qird), the Apes.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Gamma Columbae, HIP 28199, SAO 196352, HD 40494, GC 7536, HR 2106, DM CD-35  2612, TYC 7066-2024-1",
	"group" : { "key" : "Columba" },
	"Common" : "Gamma Columbae",
	"OType" : "Variable Star",
	"Distance" : "265.93",
	"RA_S" : 89.38420824,
	"DEC_S" : -35.28328064,
	"X" : 265,
	"Y" : 430,
	"Constellation" : "Columba ",
	"AMag" : 4.32,
	"key" : 69084,
	"title" : "Gamma Columbae"
	},
{
	"Index" : "53637",
	"Description" : "Eta Columbae is a yellow-orange giant star in the constellation Columba.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Eta Columbae, HIP 28328, SAO 217650, HD 40808, GC 7591, HR 2120, DM CD-42  2266, TYC 7606-989-1",
	"group" : { "key" : "Columba" },
	"Common" : "Eta Columbae",
	"OType" : "Star",
	"Distance" : "144.67",
	"RA_S" : 89.78668801,
	"DEC_S" : -42.81513142,
	"X" : 263,
	"Y" : 528,
	"Constellation" : "Columba ",
	"AMag" : 4.057,
	"key" : 73637,
	"title" : "Eta Columbae"
	},
{
	"Index" : "49223",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Theta Columbae, HIP 29034, SAO 196514, HD 42167, GC 7805, HR 2177, DM CD-37  2609, TYC 7083-1772-1",
	"group" : { "key" : "Columba" },
	"Common" : "Theta Columbae",
	"OType" : "Star",
	"Distance" : "220.91",
	"RA_S" : 91.88180092,
	"DEC_S" : -37.25292059,
	"Constellation" : "Columba ",
	"AMag" : 4.977,
	"key" : 69223,
	"title" : "Theta Columbae"
	},
{
	"Index" : "53735",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Pi02 Columbae, HIP 29064, SAO 217730, HD 42303, GC 7816, HR 2181, DM CD-42  2351, TYC 7619-9-1",
	"group" : { "key" : "Columba" },
	"Common" : "Pi02 Columbae",
	"OType" : "Double or multiple star",
	"Distance" : "74.43",
	"RA_S" : 91.97024116,
	"DEC_S" : -42.15404143,
	"Constellation" : "Columba ",
	"AMag" : 5.491,
	"key" : 73735,
	"title" : "Pi02 Columbae"
	},
{
	"Index" : "49192",
	"Description" : "Kappa Columbae is a giant star in the constellation Columba.\r\rThis star, along with \u03B6 CMa, \u03BB CMa, \u03B3 Col, \u03B4 Col, \u03B8 Col, \u03BB Col, \u03BC Col and \u03BE Col, were Al \u1E32ur\u016Bd (\u0623\u0644\u0642\u0631\u062F - al-qird), the Apes.\r\rIn Chinese, \u5B6B (S\u016Bn), meaning Grandson, refers to an asterism consisting of \u03BA Columbae and \u03B8 Columbae. Consequently, \u03BA Columbae itself is known as \u5B6B\u4E00 (S\u016Bn y\u012B, English: the First Star of Grandson.).",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Kappa Columbae, HIP 29807, SAO 196643, HD 43785, GC 8062, HR 2256, DM CD-35  2800, TYC 7080-2123-1",
	"group" : { "key" : "Columba" },
	"Common" : "Kappa Columbae",
	"OType" : "Variable Star",
	"Distance" : "55.95",
	"RA_S" : 94.13806878,
	"DEC_S" : -35.14051763,
	"X" : 215,
	"Y" : 430,
	"Constellation" : "Columba ",
	"AMag" : 4.472,
	"key" : 69192,
	"title" : "Kappa Columbae"
	},
{
	"Index" : "49199",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 30143, SAO 196707, HD 44506, GC 8180, HR 2288, DM CD-34 2806, TYC 7081-1572-1",
	"group" : { "key" : "Columba" },
	"Common" : "HR 2288",
	"OType" : "Be Star",
	"Distance" : "583.24",
	"RA_S" : 95.1509975,
	"DEC_S" : -34.14414635,
	"Constellation" : "Columba ",
	"AMag" : 5.49,
	"key" : 69199,
	"title" : "HR 2288"
	},
{
	"Index" : "49158",
	"Description" : "Delta Columbae is a spectroscopic binary yellow giant star in the constellation Columba. It has the uncommon traditional name Ghusn al Zaitun, from the Arabic \u0627\u0644\u063A\u0635\u0646 \u0627\u0644\u0632\u064A\u062A\u0648\u0646 al-ghu\u015Fn al-zait\u016Bn \u0022the olive branch\u0022..\r\rThis star, along with \u03B6 CMa, \u03BB CMa, \u03B3 Col, \u03B8 Col, \u03BA Col, \u03BB Col, \u03BC Col and \u03BE Col, were Al \u1E32ur\u016Bd (\u0623\u0644\u0642\u0631\u062F - al-qird), the Apes.\r\rDelta Columbae was a latter designation of 3 Canis Majoris.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "Delta Columbae, HIP 30277, SAO 196735, HD 44762, GC 8214, HR 2296, DM CD-33  2927, TYC 7077-2060-1",
	"group" : { "key" : "Columba" },
	"Common" : "Ghusn al Zaitu",
	"OType" : "Spectroscopic binary",
	"Distance" : "71.62",
	"RA_S" : 95.52844658,
	"DEC_S" : -33.43640196,
	"X" : 198,
	"Y" : 409,
	"Constellation" : "Columba ",
	"AMag" : 3.93,
	"key" : 69158,
	"title" : "Ghusn al Zaitu"
	},
{
	"Index" : "53691",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 31165, SAO 196917, HD 46568, GC 8514, HR 2399, DM CD-37 2889, TYC 7614-1951-1",
	"group" : { "key" : "Columba" },
	"Common" : "HR 2399",
	"OType" : "Star",
	"Distance" : "83.72",
	"RA_S" : 98.08911065,
	"DEC_S" : -37.69670001,
	"Constellation" : "Columba ",
	"AMag" : 5.361,
	"key" : 73691,
	"title" : "HR 2399"
	},
{
	"Index" : "64995",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "6 Comae Berenices, HIP 59819, SAO 100012, HD 106661, GC 16747, HR 4663, DM BD+15  2436, TYC 879-919-1",
	"group" : { "backgroundImage" : "images/Alignment/21.png",
		"description" : "Coma Berenices is a traditional asterism that has since been defined as one of the 88 modern constellations. It is located near Leo, to which it formerly belonged, and accommodates the North Galactic Pole. Its name means \u0022Berenice\u0027s Hair\u0022 (in Greek, via Latin), and refers to the legend of Queen Berenice II of Egypt, who sacrificed her long hair.\r\rComa Berenices is one of the few constellations to owe its name to a historical figure, in this case Queen Berenice II of Egypt, wife of Ptolemy III Euergetes (fl. 246 BC\u2013221 BC), the king under whom Alexandria became an important cultural center.\r\rIn 243 BC, during the Third Syrian War, Ptolemy undertook a dangerous expedition against the Seleucids, who had murdered his sister. His newlywed bride, Berenice, swore to the goddess Aphrodite to sacrifice her long, blonde hair, of which she was extremely proud, if her husband returned safely. He did, so she cut her hair and placed it in the goddess\u0027s temple. By the next morning the hair had disappeared. To appease the furious king the court astronomer, Conon, announced that the offering had so pleased the goddess that she had placed it in the sky. He indicated a cluster of stars that have since been called Berenice\u0027s Hair.\r\rThis incident inspired the court poet Callimachus of Cyrene to write a poem entitled \u0392\u03B5\u03C1\u03B5\u03BD\u03AF\u03BA\u03B7\u03C2 \u03C0\u03BB\u03CC\u03BA\u03B1\u03BC\u03BF\u03C2 (Greek \u0022Berenice\u0027s braid\u0022). About 2/3 of the Greek original is now lost, but the full version was translated to Latin by the Roman poet Catullus, and his version exists to this day.\r\rComa Berenices consists of a number of stars close together, and has been recognized as a distinct asterism since the Hellenistic period. Eratosthenes referred to it as both \u0022Ariadne\u0027s Hair\u0022 and \u0022Berenice\u0027s Hair\u0022. Ptolemy referred to it as \u0022the lock\u0022 of hair; however, he did not list it as one of his 48 constellations, considering it to be a part of Leo, specifically, the tuft at the end of the lion\u0027s tail.\r\rTycho Brahe, who is usually given credit for Coma\u0027s promotion to constellation status, listed it in his star catalogue of 1602, but it originally occurred on a celestial globe by the cartographer Caspar Vopel from 1536. Gerardus Mercator has also been credited as its promoter in 1551.\r\rIt appeared in Johann Bayer\u0027s Uranometria of 1603, and during the 17th century, a few other maps that were made of the sky followed suit.",
		"key" : "Coma Berenices",
		"grouptype" : "Coma Berenices",
		"Meaning" : "Berenice's hair",
		"Family" : "Ursa Major",
		"Origin" : "1603, Uranometria, split from Leo",
		"shortTitle" : "Coma Berenices",
		"title" : "Coma Berenices Objects Group" },
	"Common" : "6 Comae Berenices",
	"OType" : "Star",
	"Distance" : "60.89",
	"RA_S" : 184.00077813,
	"DEC_S" : 14.89906906,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.092,
	"key" : 84995,
	"title" : "6 Comae Berenices"
	},
{
	"Index" : "8183",
	"Description" : "7 Comae Berenices (7 Com) is a star in the constellation Coma Berenices. Its apparent magnitude is 4.86.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "7 Comae Berenices, HIP 59847, SAO 82211, HD 106714, GC 16752, HR 4667, DM BD+24  2443, TYC 1986-2432-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "7 Comae Berenices",
	"OType" : "Star in Cluster",
	"Distance" : "76.4",
	"RA_S" : 184.08557628,
	"DEC_S" : 23.94541234,
	"X" : 479,
	"Y" : 447,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.033,
	"key" : 28183,
	"title" : "7 Comae Berenices"
	},
{
	"Index" : "12490",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "HIP 59856, SAO 62928, HD 106760, GC 16754, HR 4668, DM BD+33 2213, TYC 2527-2202-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "HR 4668",
	"OType" : "Spectroscopic binary",
	"Distance" : "96.84",
	"RA_S" : 184.12556852,
	"DEC_S" : 33.06152753,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.122,
	"key" : 32490,
	"title" : "HR 4668"
	},
{
	"Index" : "3730",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "11 Comae Berenices, HIP 60202, SAO 100053, HD 107383, GC 16835, HR 4697, DM BD+18  2592, TYC 1445-2560-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "11 Comae Berenices",
	"OType" : "Star",
	"Distance" : "88.85",
	"RA_S" : 185.17927905,
	"DEC_S" : 17.79287347,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.835,
	"key" : 23730,
	"title" : "11 Comae Berenices"
	},
{
	"Index" : "8242",
	"Description" : "12 Comae Berenices (12 Com) is a star in the constellation Coma Berenices. Its apparent magnitude is 4.80.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "12 Comae Berenices, HIP 60351, SAO 82273, HD 107700, GC 16873, HR 4707, DM BD+26  2337, TYC 1989-3210-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "12 Comae Berenices",
	"OType" : "Spectroscopic binary",
	"Distance" : "94.59",
	"RA_S" : 185.62630134,
	"DEC_S" : 25.8461567,
	"X" : 458,
	"Y" : 424,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.859,
	"key" : 28242,
	"title" : "12 Comae Berenices"
	},
{
	"Index" : "8235",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "13 Comae Berenices, HIP 60514, SAO 82291, HD 107966, GC 16910, HR 4717, DM BD+26  2344, TYC 1989-3203-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "13 Comae Berenices",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "90.74",
	"RA_S" : 186.07721149,
	"DEC_S" : 26.09858356,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.157,
	"key" : 28235,
	"title" : "13 Comae Berenices"
	},
{
	"Index" : "8283",
	"Description" : "14 Comae Berenices (14 Com) is a star in the constellation Coma Berenices. Its apparent magnitude is 4.92.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "14 Comae Berenices, HIP 60697, SAO 82310, HD 108283, GC 16955, HR 4733, DM BD+28  2115, TYC 1991-1897-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "14 Comae Berenices",
	"OType" : "Star in Cluster",
	"Distance" : "92.35",
	"RA_S" : 186.60027028,
	"DEC_S" : 27.26823928,
	"X" : 444,
	"Y" : 407,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.948,
	"key" : 28283,
	"title" : "14 Comae Berenices"
	},
{
	"Index" : "8281",
	"Description" : "Gamma Comae Berenices (Gamma Com, \u03B3 Comae Berenices, \u03B3 Com) is a K-type giant star in the constellation of Coma Berenices. It has an apparent visual magnitude of approximately 4.350. It appears as part of the cluster Melotte 111, although it is probably not actually in this cluster.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "15 Comae Berenices, Gamma Comae Berenices, HIP 60742, SAO 82313, HD 108381, GC 16964, HR 4737, DM BD+29  2288, TYC 1991-1895-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "Gamma Comae Berenices",
	"OType" : "Star in Cluster",
	"Distance" : "51.28",
	"RA_S" : 186.73447237,
	"DEC_S" : 28.26842484,
	"X" : 441,
	"Y" : 395,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.466,
	"key" : 28281,
	"title" : "Gamma Comae Berenices"
	},
{
	"Index" : "8286",
	"Description" : "16 Comae Berenices (16 Com) is a star in the constellation Coma Berenices. Its apparent magnitude is 4.97.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "16 Comae Berenices, HIP 60746, SAO 82314, HD 108382, GC 16965, HR 4738, DM BD+27  2134, TYC 1991-1901-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "16 Comae Berenices",
	"OType" : "Star in Cluster",
	"Distance" : "92.58",
	"RA_S" : 186.74706742,
	"DEC_S" : 26.82570069,
	"X" : 443,
	"Y" : 413,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.971,
	"key" : 28286,
	"title" : "16 Comae Berenices"
	},
{
	"Index" : "8238",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "17 Comae Berenices, HIP 60904, SAO 82330, HD 108662, GC 17012, HR 4752, DM BD+26  2354, TYC 1989-3206-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "17 Comae Berenices",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "72.86",
	"RA_S" : 187.2279271,
	"DEC_S" : 25.91284986,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.231,
	"key" : 28238,
	"title" : "17 Comae Berenices"
	},
{
	"Index" : "8246",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "21 Comae Berenices, HIP 61071, SAO 82346, HD 108945, GC 17056, HR 4766, DM BD+25  2517, TYC 1989-3213-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "21 Comae Berenices",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "91.61",
	"RA_S" : 187.75233742,
	"DEC_S" : 24.56716766,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.444,
	"key" : 28246,
	"title" : "21 Comae Berenices"
	},
{
	"Index" : "8273",
	"Description" : "23 Comae Berenices (23 Com) is a star in the constellation Coma Berenices. Its apparent magnitude is 4.79.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "23 Comae Berenices, HIP 61394AB, SAO 82390, HD 109485, GC 17142, HR 4789, DM BD+23  2475, TYC 1990-3784-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "23 Comae Berenices",
	"OType" : "Star",
	"Distance" : "94.78",
	"RA_S" : 188.7128287,
	"DEC_S" : 22.62924164,
	"X" : 424,
	"Y" : 470,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.773,
	"key" : 28273,
	"title" : "23 Comae Berenices"
	},
{
	"Index" : "3739",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "24 Comae Berenices, HIP 61418A, SAO 100160, HD 109511, GC 17147, HR 4792, DM BD+19  2584A, TYC 1446-2469-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "24 Comae Berenices",
	"OType" : "Variable Star",
	"Distance" : "138.1215",
	"RA_S" : 188.7823313,
	"DEC_S" : 18.3770576,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.109,
	"key" : 23739,
	"title" : "24 Comae Berenices"
	},
{
	"Index" : "3741",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "27 Comae Berenices, HIP 62356, SAO 100252, HD 111067, GC 17363, HR 4851, DM BD+17  2533, TYC 1446-2471-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "27 Comae Berenices",
	"OType" : "Star",
	"Distance" : "104.05",
	"RA_S" : 191.66150904,
	"DEC_S" : 16.57768995,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.265,
	"key" : 23741,
	"title" : "27 Comae Berenices"
	},
{
	"Index" : "8337",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "31 Comae Berenices, HIP 62763, SAO 82537, HD 111812, GC 17455, HR 4883, DM BD+28  2156, TYC 1995-2586-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "31 Comae Berenices",
	"OType" : "Rotationally variable Star",
	"Distance" : "94.12",
	"RA_S" : 192.92467317,
	"DEC_S" : 27.54071548,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.999,
	"key" : 28337,
	"title" : "31 Comae Berenices"
	},
{
	"Index" : "3829",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "35 Comae Berenices, HIP 62886A, SAO 82550, HD 112033A, GC 17493, HR 4894, DM BD+22  2519, TYC 1455-1412-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "35 Comae Berenices",
	"OType" : "Star",
	"Distance" : "86.22",
	"RA_S" : 193.32392316,
	"DEC_S" : 21.24490755,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.148,
	"key" : 23829,
	"title" : "35 Comae Berenices"
	},
{
	"Index" : "3776",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "36 Comae Berenices, HIP 63355, SAO 100357, HD 112769, GC 17616, HR 4920, DM BD+18  2682, TYC 1450-1133-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "36 Comae Berenices",
	"OType" : "Variable Star",
	"Distance" : "99.31",
	"RA_S" : 194.73101062,
	"DEC_S" : 17.40944591,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.922,
	"key" : 23776,
	"title" : "36 Comae Berenices"
	},
{
	"Index" : "12552",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "37 Comae Berenices, HIP 63462AC, SAO 63288, HD 112989, GC 17647, HR 4924, DM BD+31  2434, TYC 2532-2226-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "37 Comae Berenices",
	"OType" : "Variable of RS CVn type",
	"Distance" : "199.46",
	"RA_S" : 195.068629,
	"DEC_S" : 30.78501699,
	"Constellation" : "Coma Berenices ",
	"AMag" : 5.018,
	"key" : 32552,
	"title" : "37 Comae Berenices"
	},
{
	"Index" : "8350",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "41 Comae Berenices, HIP 64022, SAO 82659, HD 113996, GC 17787, HR 4954, DM BD+28  2185, TYC 1996-2401-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "41 Comae Berenices",
	"OType" : "Star",
	"Distance" : "101.57",
	"RA_S" : 196.79470976,
	"DEC_S" : 27.62474074,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.952,
	"key" : 28350,
	"title" : "41 Comae Berenices"
	},
{
	"Index" : "3815",
	"Description" : "Alpha Comae Berenices (Alpha Com, \u03B1 Com, \u03B1 Comae Berenices) is a star in the constellation Coma Berenices (Berenice\u0027s Hair). Although it has the Bayer designation \u0022alpha\u0022, at magnitude 4.32 it is actually fainter than Beta Comae Berenices. It has the traditional name Diadem. It is said to represent the crown worn by Queen Berenice. A name occasionally seen is Al Dafirah, from the Arabic \u0627\u0644\u0636\u0641\u064A\u0631\u0629 a\u0111\u0327-\u0111\u0327af\u012Brah \u0022the braid\u0022.\r\rIn Chinese, \u592A\u5FAE\u5DE6\u57A3 (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n), meaning Left Wall of Supreme Palace Enclosure, refers to an asterism consisting of \u03B1 Comae Berenices, \u03B7 Virginis, \u03B3 Virginis, \u03B4 Virginis and \u03B5 Virginis. Consequently, \u03B1 Comae Berenices itself is known as \u592A\u5FAE\u5DE6\u57A3\u4E94 (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n w\u01D4, English: the Fifth Star of Left Wall of Supreme Palace Enclosure.), representing \u6771\u4E0A\u5C07 (D\u014Dngsh\u01CEngji\u0101ng), meaning The First Eastern General. \u6771\u4E0A\u5C07 (D\u014Dngsh\u01CEngji\u0101ng), westernized into Shang Tseang, but the name Shang Tseang was designated for \u0022v Comae Berenices\u0022 by R.H. Allen and the meaning is \u0022a Higher General",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "42 Comae Berenices, Alpha Comae Berenices, HIP 64241, SAO 100443, HD 114378, GC 17833, HR 4968, DM BD+18  2697A, TYC 1454-1134-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "Al Dafirah",
	"OType" : "High proper-motion Star",
	"Distance" : "17.82",
	"RA_S" : 197.49702877,
	"DEC_S" : 17.52944436,
	"X" : 318,
	"Y" : 541,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.427,
	"key" : 23815,
	"title" : "Al Dafirah"
	},
{
	"Index" : "8349",
	"Description" : "Beta Comae Berenices (\u03B2 Comae Berenices, \u03B2 Com) is a main sequence dwarf star in the northern constellation of Coma Berenices. It is located at a distance of about 29.78 light-years (9.13 parsecs) from Earth. The Greek letter beta (\u03B2) usually indicates that the star has the second highest visual magnitude in the constellation. However, with an apparent visual magnitude of 4.3, this star is slightly brighter than \u03B1 Comae Berenices. It can be seen with the naked eye, but may be too dim to be viewed from a built-up urban area.\r\rThis star is similar to our own Sun, being only slightly larger and brighter in absolute magnitude. It has a stellar classification of G0 V, compared to G2 V for the Sun. The effective temperature of the outer envelope is 5,936 K, giving it a yellow hue of a G-type star. In terms of age it is younger than the Sun, being about 3 billion years old.\r\rObservations of short term variations in the chromatic activity suggest that the star undergoes differential rotation, with a rotation period of about 11\u201313 days. Its surface has a measured activity cycle of 16.6 years, compared to 11 years on our Sun. It may also have a secondary activity cycle of 9.6 years. At one time it was thought that this star might have a spectroscopic companion. However, this was ruled out by means of more accurate radial velocity measurements. No planets have yet been detected around it, and there is no evidence of a dusty disk.",
	"MapNum" : "21",
	"ImageNum" : "21",
	"Desig" : "43 Comae Berenices, Beta Comae Berenices, HIP 64394, SAO 82706, HD 114710, GC 17874, HR 4983, DM BD+28  2193, TYC 1996-2400-1",
	"group" : { "key" : "Coma Berenices" },
	"Common" : "Beta Comae Berenices",
	"OType" : "High proper-motion Star",
	"Distance" : "9.13",
	"RA_S" : 197.96830985,
	"DEC_S" : 27.87818125,
	"X" : 312,
	"Y" : 406,
	"Constellation" : "Coma Berenices ",
	"AMag" : 4.304,
	"key" : 28349,
	"title" : "Beta Comae Berenices"
	},
{
	"Index" : "56574",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 89290, SAO 228815, HD 166596, GC 24824, HR 6804, DM CD-4112534, TYC 7908-4299-1",
	"group" : { "backgroundImage" : "images/Alignment/19.png",
		"description" : "Corona Australis (pron.: /k\u0275\u02C8ro\u028An\u0259 \u0252\u02C8stre\u026Al\u0268s/) or Corona Austrina (pron.: /k\u0275\u02C8ro\u028An\u0259 \u0252\u02C8stra\u026An\u0259/) is a constellation in the Southern Hemisphere. Its Latin name means \u0022southern crown\u0022, and it is the southern counterpart of Corona Borealis, the northern crown. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The Ancient Greeks saw Corona Australis as a wreath rather than a crown and associated it with Sagittarius or Centaurus. Other cultures have likened the pattern to a turtle, ostrich nest, a tent, or even a hut belonging to a rock hyrax.\r\rAlthough fainter than its namesake, the oval- or horseshoe-shaped pattern of its brighter stars renders it distinctive. Alpha and Beta Coronae Australis are the two brightest stars with an apparent magnitude of around 4.1. Epsilon Coronae Australis is the brightest example of a W Ursae Majoris variable in the southern sky. Lying alongside the Milky Way, Corona Australis contains one of the closest star-forming regions to our Solar System\u2014a dusty dark nebula known as the Corona Australis Molecular Cloud, lying about 430 light years away. Within it are stars at the earliest stages of their lifespan. The variable stars R and TY Coronae Australis light up parts of the nebula, which varies in brightness accordingly.\r\rCorona Australis is a small constellation bordered by Sagittarius to the north, Scorpius to the west, Telescopium to the south, and Ara to the southwest. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027CrA\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of four segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 17h 58.3m and 19h 19.0m, while the declination coordinates are between \u221236.77\u00B0 and \u221245.52\u00B0. Covering 128 square degrees, Corona Australis culminates at midnight around the 30th of June and ranks 80th in area. Only visible at latitudes south of 53\u00B0 north, Corona Australis cannot be seen from the British Isles as it lies too far south, but it can be seen from southern Europe and readily from the southern United States.\r\rCorona Australis may have been recorded by ancient Mesopotamians in the MUL.APIN, as a constellation called MA.GUR (\u0022The Bark\u0022). However, this constellation, adjacent to SUHUR.MASH (\u0022The Goat-Fish\u0022, modern Capricornus), may instead have been modern Epsilon Sagittarii. As a part of the southern sky, MA.GUR was one of the fifteen \u0022stars of Ea\u0022.\r\rIn the 3rd century BC, the Greek didactic poet Aratus wrote of, but did not name the constellation, instead calling the two crowns \u03A3\u03C4\u03B5\u03C6\u03AC\u03BD\u03BF\u03B9 (Stephanoi). The Greek astronomer Ptolemy described the constellation in the 2nd century AD, though with the inclusion of Alpha Telescopii, since transferred to Telescopium. Ascribing 13 stars to the constellation, he named it \u03A3\u03C4\u03B5\u03C6\u03AC\u03BD\u03BF\u03C2 \u03BD\u03BF\u03C4\u03B9\u03BF\u03C2 (Stephanos notios), \u0022Southern Wreath\u0022, while other authors associated it with either Sagittarius (having fallen off his head) or Centaurus; with the former, it was called Corona Sagittarii. Similarly, the Romans called Corona Australis the \u0022Golden Crown of Sagittarius\u0022. It was known as Parvum Coelum (\u0022Canopy\u0022, \u0022Little Sky\u0022) in the 5th century. The 18th-century French astronomer J\u00E9r\u00F4me Lalande gave it the names Sertum Australe (\u0022Southern Garland\u0022) and Orbiculus Capitis, while German poet and author Philippus Caesius called it Corolla (\u0022Little Crown\u0022) or Spira Australis (\u0022Southern Coil\u0022), and linked it with the Crown of Eternal Life from the New Testament. Seventeenth-century celestial cartographer Julius Schiller linked it to the Diadem of Solomon. Sometimes, Corona Australis was not the wreath of Sagittarius but arrows held in his hand.\r\rCorona Australis has been associated with the myth of Bacchus and Semele. Jupiter had impregnated Semele, causing Juno to become jealous. Juno convinced Semele to ask Jupiter to appear in his full splendor, which the mortal woman could not handle, causing her to burn. After Bacchus, Semele\u0027s unborn child, became an adult and the god of wine, he honored his deceased mother by placing a wreath in the sky.\r\rIn Chinese astronomy, the stars of Corona Australis are located within the Black Tortoise of the North (\u5317\u65B9\u7384\u6B66, B\u011Bi F\u0101ng Xu\u00E1n W\u01D4). The constellation itself was known as ti\u0027en pieh (\u0022Heavenly Turtle\u0022) and during the Western Zhou period, marked the beginning of winter. However, precession over time has meant that the \u0022Heavenly River\u0022 (Milky Way) became the more accurate marker to the ancient Chinese and hence supplanted the turtle in this role. Arabic names for Corona Australis include Al \u0136ubbah \u0022the Tortoise\u0022, Al \u0124ib\u0101 \u0022the Tent\u0022 or Al Ud\u1E25\u0101 al Na\u0027\u0101m \u0022the Ostrich Nest\u0022. It was later given the name Al Ikl\u012Bl al Jan\u016Bbiyyah, which the European authors Chilmead, Riccioli and Caesius transliterated as Alachil Elgenubi, Elkleil Elgenubi and Aladil Algenubi respectively.\r\rThe \u01C0Xam speaking Bushmen of South Africa knew the constellation as \u2260nabbe ta !nu \u0022house of branches\u0022\u2014owned originally by the Dassie (rock hyrax), and the star pattern depicting people sitting in a semicircle around a fire.\r\rThe indigenous Boorong people of northwestern Victoria saw it as Won, a boomerang thrown by Totyarguil (Altair). The Aranda people of Central Australia saw Corona Australis as a coolamon carrying a baby, which was accidentally dropped to earth by a group of sky-women dancing in the Milky Way. The impact of the coolamon created Gosses Bluff crater, 175 km west of Alice Springs. The Torres Strait Islanders saw Corona Australis as part of a larger constellation encompassing part of Sagittarius and the tip of Scorpius\u0027s tail; the Pleiades and Orion were also associated. This constellation was Tagai\u0027s canoe, crewed by the Pleiades, called the Usiam, and Orion, called the Seg. The myth of Tagai says that he was in charge of this canoe, but his crewmen consumed all of the supplies onboard without asking permission. Enraged, Tagai bound the Usiam with a rope and tied them to the side of the boat, then threw them overboard. Scorpius\u0027s tail represents a suckerfish, while Eta Sagittarii and Theta Coronae Australis mark the bottom of the canoe. On the island of Futuna, the figure of Corona Australis was called Tanuma and in the Tuamotus, it was called Na Kaua-ki-Tonga.",
		"key" : "Corona Australis",
		"grouptype" : "Corona Australis",
		"Meaning" : "southern crown",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Corona Australis",
		"title" : "Corona Australis Objects Group" },
	"Common" : "HR 6804",
	"OType" : "Rotationally variable Star",
	"Distance" : "351.63",
	"RA_S" : 273.30291035,
	"DEC_S" : -41.33611529,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.435,
	"key" : 76574,
	"title" : "HR 6804"
	},
{
	"Index" : "56508",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90037, SAO 210048, HD 168592, GC 25051, HR 6862, DM CD-3812729, TYC 7901-3102-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "HR 6862",
	"OType" : "Star",
	"Distance" : "147.86",
	"RA_S" : 275.57738163,
	"DEC_S" : -38.65689718,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.252,
	"key" : 76508,
	"title" : "HR 6862"
	},
{
	"Index" : "56617",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90200, SAO 228982, HD 168905, GC 25094, HR 6875, DM CD-4412569, TYC 7913-205-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "HR 6875",
	"OType" : "Variable Star",
	"Distance" : "148.96",
	"RA_S" : 276.07600231,
	"DEC_S" : -44.11025647,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.2,
	"key" : 76617,
	"title" : "HR 6875"
	},
{
	"Index" : "56551",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90887, SAO 210277, HD 170642, GC 25285, HR 6942, DM CD-3912696, TYC 7906-1557-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "HR 6942",
	"OType" : "Star",
	"Distance" : "70.25",
	"RA_S" : 278.08887754,
	"DEC_S" : -39.70400154,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.166,
	"key" : 76551,
	"title" : "HR 6942"
	},
{
	"Index" : "56591",
	"Description" : "Theta Coronae Australis (t CrA), is a star located in the constellation Corona Australis. Theta Coronae Australis is also known as HR 6951, and HD 170845. The star is located at Right Ascension 18h 33m 30s and Declination -42 deg 18 arcmin 45 arcsec.\r\rTheta Coronae Australis is a G8III giant star with an effective temperature of 5000 Kelvin. It has an apparent visual magnitude of +4.64, an absolute magnitude of -2.5, and a mass of 1.1 solar masses. The star is located at a distance of 265 pc, (866 light years).",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Theta Coronae Australis, HIP 90982, SAO 229111, HD 170845, GC 25313, HR 6951, DM CD-42 13378, TYC 7910-1570-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Theta Coronae Australis",
	"OType" : "Star",
	"Distance" : "170.5",
	"RA_S" : 278.37577028,
	"DEC_S" : -42.31250882,
	"X" : 389,
	"Y" : 429,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.725,
	"key" : 76591,
	"title" : "Theta Coronae Australis"
	},
{
	"Index" : "56634",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Lambda Coronae Australis, HIP 91875, SAO 210501, HD 172777, GC 25599, HR 7021, DM CD-38 13036, TYC 7915-1673-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Lambda Coronae Australis",
	"OType" : "Star",
	"Distance" : "62.9",
	"RA_S" : 280.94559597,
	"DEC_S" : -38.32344263,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.121,
	"key" : 76634,
	"title" : "Lambda Coronae Australis"
	},
{
	"Index" : "56673",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Mu Coronae Australis, HIP 92226, SAO 229285, HD 173540, GC 25722, HR 7050, DM CD-40 12807, TYC 7919-1424-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Mu Coronae Australis",
	"OType" : "Star",
	"Distance" : "121.14",
	"RA_S" : 281.93591272,
	"DEC_S" : -40.40616238,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.303,
	"key" : 76673,
	"title" : "Mu Coronae Australis"
	},
{
	"Index" : "56756",
	"Description" : "Eta1 Coronae Australis (n1 CrA), is a star located in the constellation Corona Australis. Eta1 Coronae Australis is also known as HR 7062, and HD 173715. The star is located at Right Ascension 18h 48m 53s and Declination -43 deg 40 arcmin 48 arcsec.\r\rEta1 Coronae Australis is an A3V dwarf star with an effective temperature of 9000 Kelvin. It has an apparent visual magnitude of +5.49, an absolute magnitude of +0.326, and a mass of 2.4 solar masses. The star is located at a distance of 106 pc, (346 light years).\r\rEta1 Coronae Australis has broad spectrum absorption lines associated with its rotation period.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Eta01 Coronae Australis, HIP 92308, SAO 229299, HD 173715, GC 25748, HR 7062, DM CD-43 12841, TYC 7927-522-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Eta1 Coronae Australis",
	"OType" : "Star",
	"Distance" : "102.43",
	"RA_S" : 282.21037372,
	"DEC_S" : -43.68003818,
	"X" : 352,
	"Y" : 447,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.472,
	"key" : 76756,
	"title" : "Eta1 Coronae Australis"
	},
{
	"Index" : "56725",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 92953, SAO 229383, HD 175219, GC 25956, HR 7122, DM CD-4213761, TYC 7924-1192-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "HR 7122",
	"OType" : "Star",
	"Distance" : "90.4",
	"RA_S" : 284.07063266,
	"DEC_S" : -42.71067127,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.456,
	"key" : 76725,
	"title" : "HR 7122"
	},
{
	"Index" : "52258",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 92989, SAO 210734, HD 175362, GC 25973, HR 7129, DM CD-3712982, TYC 7421-2297-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "HR 7129",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "131.73",
	"RA_S" : 284.16873224,
	"DEC_S" : -37.34324617,
	"Constellation" : "Corona Australis ",
	"AMag" : 5.332,
	"key" : 72258,
	"title" : "HR 7129"
	},
{
	"Index" : "52257",
	"Description" : "Epsilon Coronae Australis (e CrA), is a star located in the constellation Corona Australis. Epsilon Coronae Australis is also known as HR 7152, and HD 175813. The star is located at Right Ascension 19h 08m 21s and Declination -40 deg 29 arcmin 48 arcsec.\r\rEpsilon Coronae Australis is an F4V dwarf star with an effective temperature of 6000 Kelvin. It has an apparent visual magnitude of +4.83, an absolute magnitude of +2.45, and a mass of 1.1 solar masses. Epsilon Coronae Australis is an W Ursae Majoris variable, indicating that it has a contact companion within the Roche Limit of the primary. The star is located at a distance of 30 pc (97 light years) from the Sun.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Epsilon Coronae Australis, HIP 93174, SAO 210781, HD 175813, GC 26038, HR 7152, DM CD-37 13001, TYC 7421-2296-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Epsilon Coronae Australis",
	"OType" : "Eclipsing binary of W UMa type (contact binary)",
	"Distance" : "30.18",
	"RA_S" : 284.68073584,
	"DEC_S" : -37.10734814,
	"X" : 325,
	"Y" : 362,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.903,
	"key" : 72257,
	"title" : "Epsilon Coronae Australis"
	},
{
	"Index" : "56738",
	"Description" : "Zeta Coronae Australis (z CrA), is a star located in the constellation Corona Australis. Zeta Coronae Australis is also known as HR 7188, and HD 176638. The star is located at Right Ascension 19h 03m 07s and Declination -42 deg 05 arcmin 43 arcsec.\r\rZeta Coronae Australis is a B9V dwarf star with an effective temperature of 9800 Kelvin. It has an apparent visual magnitude of +4.75, an absolute magnitude of +0.986, and a mass of 2.9 solar masses. The star is located at a distance of 56 pc, (183 light years).\r\rZeta Coronae Australis has broad spectrum absorption lines associated with its rotation period.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Zeta Coronae Australis, HIP 93542, SAO 229461, HD 176638, GC 26165, HR 7188, DM CD-42 13855, TYC 7925-2795-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Zeta Coronae Australis",
	"OType" : "High proper-motion Star",
	"Distance" : "59.19",
	"RA_S" : 285.77865864,
	"DEC_S" : -42.09510289,
	"X" : 317,
	"Y" : 428,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.721,
	"key" : 76738,
	"title" : "Zeta Coronae Australis"
	},
{
	"Index" : "52276",
	"Description" : "Gamma Coronae Australis (y CrA), is a star located in the constellation Corona Australis. Gamma Coronae Australis is also known as HR 7226, and HD 177474. The star is a spectroscopic binary. The system is located at Right Ascension 19h 06m 25s and Declination -37 deg 03 arcmin 48 arcsec. The system has a combined apparent visual magnitude of +4.26 is located 18 pc (58 light years) from the Sun.\r\rGamma Coronae Australis A is an F8V dwarf star with an effective temperature of 5500 Kelvin. It has an apparent visual magnitude of +4.9, an absolute magnitude of +2.97, and a mass of 1.2 solar masses.\r\rGamma Coronae Australis B, also known as HR 7227, and HD 177475 is an F8V dwarf star with an effective temperature of 5500 Kelvin. It has an apparent visual magnitude of +5, an absolute magnitude of +2.97, and a mass of 1.2 solar masses.\r\rThe angular separation of A and B is just 4.5 arcsec.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Gamma Coronae Australis, HIP 93825AB, SAO 210928, HD 177474, GC 26263, HR 7226, DM CD-37 13048A, TYC 7422-1737-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Gamma Coronae Australis",
	"OType" : "Star",
	"Distance" : "17.3",
	"RA_S" : 286.60479182,
	"DEC_S" : -37.06349317,
	"X" : 305,
	"Y" : 363,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.409,
	"key" : 72276,
	"title" : "Gamma Coronae Australis"
	},
{
	"Index" : "56701",
	"Description" : "Delta Coronae Australis (d CrA), is a star located in the constellation Corona Australis. Delta Coronae Australis is also known as HR 7242, and HD 177873. The star is located at Right Ascension 19h 08m 21s and Declination -40 deg 29 arcmin 48 arcsec.\r\rDelta Coronae Australis is a K1III giant star with an effective temperature of 4500 Kelvin. It has an apparent visual magnitude of +4.59, an absolute magnitude of +0.926, and a mass of 1.1 solar masses. The star is located at a distance of 53 pc (174.5 light years) from the Sun.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Delta Coronae Australis, HIP 94005, SAO 229513, HD 177873, GC 26322, HR 7242, DM CD-40 13061, TYC 7921-2856-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Delta Coronae Australis",
	"OType" : "Star",
	"Distance" : "54.71",
	"RA_S" : 287.08737612,
	"DEC_S" : -40.49669605,
	"X" : 303,
	"Y" : 408,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.693,
	"key" : 76701,
	"title" : "Delta Coronae Australis"
	},
{
	"Index" : "56651",
	"Description" : "Alpha Coronae Australis (\u03B1 CrA, \u03B1 Coronae Australis) is a star in the constellation Corona Australis. It is the only star in the constellation with a proper name, Alphekka Meridiana (Alphekka South), after the brightest star in Corona Borealis, Alphecca. In Chinese astronomy, it is known as \u9C49\u516D (the Sixth Star of the River Turtle). It is a Class A star like Vega, rotating extremely fast on its axis, close to its breakup velocity. Alpha Coronae Australis belongs to the spectral class A2Va and has apparent magnitude +4.10. Located about 125 light years from Earth, the star\u0027s mass and radius are estimated at 2.3 times solar. With an effective temperature of roughly 9,100 K, the star radiates a total luminosity of about 31 times solar. This star is roughly 254 million years old. A rapidly rotating star, it spins at almost 200 km per second at the equator, making a complete revolution in approximately 14 hours. Like the star Vega, it has excess infrared radiation, which indicates it may be ringed by a disk of dust.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Alpha Coronae Australis, HIP 94114, SAO 210990, HD 178253, GC 26360, HR 7254, DM CD-38 13350, TYC 7917-2653-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Alphekka Meridiana",
	"OType" : "Star",
	"Distance" : "38.43",
	"RA_S" : 287.36808863,
	"DEC_S" : -37.90447819,
	"X" : 298,
	"Y" : 375,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.095,
	"key" : 76651,
	"title" : "Alphekka Meridiana"
	},
{
	"Index" : "56658",
	"Description" : "Beta Coronae Australis (Beta CrA, \u03B2 Coronae Australis, \u03B2 CrA) is a K-type bright giant star in the constellation of Corona Australis. It has an apparent visual magnitude of approximately 4.117.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Beta Coronae Australis, HIP 94160, SAO 211005, HD 178345, GC 26380, HR 7259, DM CD-39 13146, TYC 7918-1524-1",
	"group" : { "key" : "Corona Australis" },
	"Common" : "Beta Coronae Australis",
	"OType" : "Star",
	"Distance" : "145.12",
	"RA_S" : 287.50732387,
	"DEC_S" : -39.34079447,
	"X" : 298,
	"Y" : 394,
	"Constellation" : "Corona Australis ",
	"AMag" : 4.227,
	"key" : 76658,
	"title" : "Beta Coronae Australis"
	},
{
	"Index" : "8599",
	"Description" : "Beta Coronae Borealis (Beta CrB, \u03B2 Coronae Borealis, \u03B2 CrB), which has the traditional name Nusakan, is the second brightest star in the constellation of Corona Borealis. Although it appears to the naked eye to be a single star, it is actually a binary star system. It is approximately 114 light-years away and has an apparent visual magnitude which varies between 3.65 and 3.72.\r\rIn Chinese, \u8CAB\u7D22 (Gu\u00E0n Su\u01D2), meaning Coiled Thong, refers to an asterism consisting of \u03B2 Coronae Borealis, \u03C0 Coronae Borealis, \u03B8 Coronae Borealis, \u03B1 Coronae Borealis, \u03B3 Coronae Borealis, \u03B4 Coronae Borealis, \u03B5 Coronae Borealis, \u03B9 Coronae Borealis and \u03C1 Coronae Borealis. Consequently, \u03B2 Coronae Borealis itself is known as \u8CAB\u7D22\u4E09 (Gu\u00E0n Su\u01D2 s\u0101n, English: the Third Star of Coiled Thong.).",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "3 Coronae Borealis, Beta Coronae Borealis, HIP 75695, SAO 83831, HD 137909, GC 20795, HR 5747, DM BD+29  2670, TYC 2032-1605-1",
	"group" : { "backgroundImage" : "images/Alignment/09.png",
		"description" : "Corona Borealis (pron.: /k\u0275\u02C8ro\u028An\u0259 b\u0252ri\u02C8\u00E6l\u0268s/) is a small constellation in the northern sky. Its name is Latin for \u0022northern crown\u0022, a name inspired by its shape; its main stars form a semicircular arc. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy and remains one of the 88 modern constellations.\r\rIn Greek mythology, Corona Borealis was sometimes considered to represent a crown that was given by Dionysus to Ariadne, the daughter of Minos of Crete. When she wore the crown to her wedding, where she married Dionysus, he placed her crown in the heavens to commemorate the wedding. In Welsh mythology, it was called Caer Arianrhod, \u0022the Castle of the Silver Circle\u0022, and was the heavenly abode of the Lady Arianrhod (Squire, 2000:154\u2013155). In Arabic mythology, the constellation was known as \u0022the bowl of the poor people\u0022 from the Arabic name \u0642\u0635\u0639\u0629 \u0627\u0644\u0645\u0633\u0627\u0643\u064A\u0646, since the stars form an unsymmetrical pattern with an indent in one side, similar to the bowl of the poor. The Arabs also called the constellation Alphecca (a name later given to Alpha Corona Borealis), which means separated or broken up since the stars of Corona Borealis resembles a loose string of jewels.",
		"key" : "Corona Borealis",
		"grouptype" : "Corona Borealis",
		"Meaning" : "northern crown",
		"Family" : "Ursa Major",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Corona Borealis",
		"title" : "Corona Borealis Objects Group" },
	"Common" : "Nusakan",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "34.94",
	"RA_S" : 231.95721428,
	"DEC_S" : 29.10569774,
	"X" : 265,
	"Y" : 373,
	"Constellation" : "Corona Borealis ",
	"AMag" : 3.672,
	"key" : 28599,
	"title" : "Nusakan"
	},
{
	"Index" : "12778",
	"Description" : "Theta Coronae Borealis (\u03B8 CrB) is a star in the constellation Corona Borealis. Its apparent magnitude is 4.15.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "4 Coronae Borealis, Theta Coronae Borealis, HIP 76127AB, SAO 64769, HD 138749A, GC 20908, HR 5778, DM BD+31  2750, TYC 2564-1629-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Theta Coronae Borealis",
	"OType" : "Star",
	"Distance" : "114.69",
	"RA_S" : 233.23242458,
	"DEC_S" : 31.35912981,
	"X" : 255,
	"Y" : 342,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.143,
	"key" : 32778,
	"title" : "Theta Coronae Borealis"
	},
{
	"Index" : "17044",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "6 Coronae Borealis, Mu Coronae Borealis, HIP 76307, SAO 64790, HD 139153, GC 20964, HR 5800, DM BD+39  2889, TYC 3053-2219-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Mu Coronae Borealis",
	"OType" : "Variable Star",
	"Distance" : "189.28",
	"RA_S" : 233.81216348,
	"DEC_S" : 39.01006635,
	"Constellation" : "Corona Borealis ",
	"AMag" : 5.322,
	"key" : 37044,
	"title" : "Mu Coronae Borealis"
	},
{
	"Index" : "12869",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "7 Coronae Borealis, Zeta02 Coronae Borealis, HIP 76669A, SAO 64834, HD 139892, GC 21064, HR 5834, DM BD+37  2665A, TYC 2577-1754-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Zeta02 Coronae Borealis",
	"OType" : "Spectroscopic binary",
	"Distance" : "144.15",
	"RA_S" : 234.84447155,
	"DEC_S" : 36.63581655,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.962,
	"key" : 32869,
	"title" : "Zeta02 Coronae Borealis"
	},
{
	"Index" : "12868",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "7 Coronae Borealis, Zeta02 Coronae Borealis, HIP 76669B, SAO 64834, HD 139892, GC 21064, HR 5834, DM BD+37  2665A, TYC 2577-1753-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Zeta02 Coronae Borealis",
	"OType" : "Spectroscopic binary",
	"Distance" : "144.15",
	"RA_S" : 234.84447155,
	"DEC_S" : 36.63581655,
	"Constellation" : "Corona Borealis ",
	"AMag" : 5.07,
	"key" : 32868,
	"title" : "Zeta02 Coronae Borealis"
	},
{
	"Index" : "8617",
	"Description" : "Gamma Coronae Borealis (\u03B3 CrB) is a star in the constellation Corona Borealis. Its apparent magnitude is 3.84.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "8 Coronae Borealis, Gamma Coronae Borealis, HIP 76952AB, SAO 83958, HD 140436A, GC 21130, HR 5849, DM BD+26  2722, TYC 2036-1674-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Gamma Coronae Borealis",
	"OType" : "Star",
	"Distance" : "44.76",
	"RA_S" : 235.68572161,
	"DEC_S" : 26.29562122,
	"X" : 218,
	"Y" : 404,
	"Constellation" : "Corona Borealis ",
	"AMag" : 3.851,
	"key" : 28617,
	"title" : "Gamma Coronae Borealis"
	},
{
	"Index" : "8627",
	"Description" : "Delta Coronae Borealis (\u03B4 CrB) is a star in the constellation Corona Borealis. Its apparent magnitude is 4.60.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "10 Coronae Borealis, Delta Coronae Borealis, HIP 77512, SAO 84019, HD 141714, GC 21276, HR 5889, DM BD+26  2737, TYC 2037-1827-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Delta Coronae Borealis",
	"OType" : "Variable of RS CVn type",
	"Distance" : "52.13",
	"RA_S" : 237.39852975,
	"DEC_S" : 26.068393,
	"X" : 198,
	"Y" : 404,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.685,
	"key" : 28627,
	"title" : "Delta Coronae Borealis"
	},
{
	"Index" : "12879",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "11 Coronae Borealis, Kappa Coronae Borealis, HIP 77655, SAO 64948, HD 142091, GC 21319, HR 5901, DM BD+36  2652, TYC 2578-1609-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Kappa Coronae Borealis",
	"OType" : "High proper-motion Star",
	"Distance" : "30.5",
	"RA_S" : 237.80804851,
	"DEC_S" : 35.65738425,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.908,
	"key" : 32879,
	"title" : "Kappa Coronae Borealis"
	},
{
	"Index" : "17056",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "12 Coronae Borealis, Lambda Coronae Borealis, HIP 78012, SAO 64974, HD 142908, GC 21402, HR 5936, DM BD+38  2712, TYC 3054-2094-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Lambda Coronae Borealis",
	"OType" : "Star",
	"Distance" : "41.56",
	"RA_S" : 238.94828019,
	"DEC_S" : 37.94695678,
	"Constellation" : "Corona Borealis ",
	"AMag" : 5.466,
	"key" : 37056,
	"title" : "Lambda Coronae Borealis"
	},
{
	"Index" : "8626",
	"Description" : "Epsilon Coronae Borealis (\u03B5 CrB) is a star in the constellation Corona Borealis. Its apparent magnitude is 4.13.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "13 Coronae Borealis, Epsilon Coronae Borealis, HIP 78159, SAO 84098, HD 143107, GC 21440, HR 5947, DM BD+27  2558, TYC 2037-1826-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Epsilon Coronae Borealis",
	"OType" : "Double or multiple star",
	"Distance" : "67.87",
	"RA_S" : 239.39687489,
	"DEC_S" : 26.87787278,
	"X" : 176,
	"Y" : 389,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.274,
	"key" : 28626,
	"title" : "Epsilon Coronae Borealis"
	},
{
	"Index" : "12856",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "15 Coronae Borealis, Rho Coronae Borealis, HIP 78459, SAO 65024, HD 143761, GC 21527, HR 5968, DM BD+33  2663, TYC 2576-2228-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Rho Coronae Borealis",
	"OType" : "High proper-motion Star",
	"Distance" : "17.23",
	"RA_S" : 240.26108486,
	"DEC_S" : 33.30350761,
	"Constellation" : "Corona Borealis ",
	"AMag" : 5.471,
	"key" : 32856,
	"title" : "Rho Coronae Borealis"
	},
{
	"Index" : "8663",
	"Description" : "Iota Coronae Borealis (\u03B9 CrB) is a star in the constellation Corona Borealis. Its apparent magnitude is 4.98.",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "14 Coronae Borealis, Iota Coronae Borealis, HIP 78493, SAO 84152, HD 143807, GC 21534, HR 5971, DM BD+30  2738, TYC 2041-1805-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Iota Coronae Borealis",
	"OType" : "Spectroscopic binary",
	"Distance" : "95.54",
	"RA_S" : 240.36068895,
	"DEC_S" : 29.85105897,
	"X" : 173,
	"Y" : 348,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.963,
	"key" : 28663,
	"title" : "Iota Coronae Borealis"
	},
{
	"Index" : "12887",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "16 Coronae Borealis, Tau Coronae Borealis, HIP 79119, SAO 65108, HD 145328, GC 21733, HR 6018, DM BD+36  2699, TYC 2579-2094-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Tau Coronae Borealis",
	"OType" : "Double or multiple star",
	"Distance" : "34.66",
	"RA_S" : 242.24287372,
	"DEC_S" : 36.49092289,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.845,
	"key" : 32887,
	"title" : "Tau Coronae Borealis"
	},
{
	"Index" : "12892",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "19 Coronae Borealis, Xi Coronae Borealis, HIP 80181, SAO 65254, HD 147677, GC 22020, HR 6103, DM BD+31  2845, TYC 2580-2438-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Xi Coronae Borealis",
	"OType" : "Double or multiple star",
	"Distance" : "56.23",
	"RA_S" : 245.52426025,
	"DEC_S" : 30.89199456,
	"Constellation" : "Corona Borealis ",
	"AMag" : 4.958,
	"key" : 32892,
	"title" : "Xi Coronae Borealis"
	},
{
	"Index" : "12914",
	"MapNum" : "09",
	"ImageNum" : "09",
	"Desig" : "20 Coronae Borealis, Nu01 Coronae Borealis, HIP 80197, SAO 65257, HD 147749, GC 22026, HR 6107, DM BD+34  2773, TYC 2583-1993-1",
	"group" : { "key" : "Corona Borealis" },
	"Common" : "Nu01 Coronae Borealis",
	"OType" : "Variable Star",
	"Distance" : "196.02",
	"RA_S" : 245.58926746,
	"DEC_S" : 33.79905099,
	"Constellation" : "Corona Borealis ",
	"AMag" : 5.39,
	"key" : 32914,
	"title" : "Nu01 Coronae Borealis"
	},
{
	"Index" : "41916",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "31 Crateris, HIP 58587, SAO 157042, HD 104337, GC 16423, HR 4590, DM BD-18  3295, TYC 6097-1648-1",
	"group" : { "backgroundImage" : "images/Alignment/20.png",
		"description" : "Corvus is a small constellation in the southern sky. Its name is Latin for raven or crow. It includes only 11 stars visible to the naked eye (brighter than magnitude 5.5). It was one of the 48 constellations listed by Ptolemy, who only counted 7 stars, and it remains one of the 88 modern constellations.\r\rThe Greek figure of Corvus is modeled on the Babylonian Raven (MUL.UGA.MUSHEN), which was similarly placed sitting on the tail of the Serpent (Greek Hydra). The Babylonian constellation was sacred to Adad, the god of rain and storm; in the second Millennium it would have risen just before the start of the autumnal rainy season.\r\rOne myth associated with Corvus is that of Apollo and Coronis. Coronis had been unfaithful to her lover, who learned this information from a pure white crow. Apollo then turned its feathers black in a fit of rage.\r\rAnother legend associated with Corvus is that a crow stopped on his way to fetch water for Apollo, in order to eat figs. Instead of telling the truth to Apollo, he lied and said that a snake, Hydra, kept him from the water, while holding a snake in his talons as proof. Apollo saw this to be a lie, however, and flung the crow (Corvus), cup (Crater), and the snake (Hydra) into the sky. He further punished the wayward bird by making sure that it would forever be thirsty, both in real life and in the heavens, where the Cup is barely out of reach.",
		"key" : "Corvus",
		"grouptype" : "Corvus",
		"Meaning" : "crow",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Corvus",
		"title" : "Corvus Objects Group" },
	"Common" : "31 Crateris",
	"OType" : "Spectroscopic binary",
	"Distance" : "970.8738",
	"RA_S" : 180.21316354,
	"DEC_S" : -19.6589841,
	"Constellation" : "Corvus ",
	"AMag" : 5.233,
	"key" : 61916,
	"title" : "31 Crateris"
	},
{
	"Index" : "46297",
	"Description" : "Alpha Corvi (\u03B1 Crv, \u03B1 Corvi) is a star in the constellation Corvus. It has the traditional names Alchiba (Arabic \u0623\u0644\u062E\u0628\u0627 al-xib\u0101 \u0022tent\u0022) or Al Minliar al Ghurab.\r\rAl Minliar al Ghurab (Arabic \u0623\u0644\u0645\u0646\u062E\u0631 \u0623\u0644\u063A\u0631\u0628 al-manxar al-ghurab) or Minkar al Ghyrab appeared in the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, which was translated into Latin as Rostrum Corvi [beak of the crow].\r\rIn Chinese astronomy, Alchiba is called \u53F3\u8F44, Pinyin: Y\u00F2uxi\u00E1, meaning Right Linchpin, because this star is marking itself and stand alone in Right Linchpin asterism, Chariot mansion (see : Chinese constellation). \u53F3\u8F44 (Y\u00F2uxi\u00E1), westernized into Yew Hea by R.H. Allen.\r\rAlchiba belongs to the spectral class F0 and has apparent magnitude +4.00. It is 48 light years from Earth. This star is suspected of being a spectroscopic binary, although this has not yet been confirmed.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "1 Corvi, Alpha Corvi, HIP 59199, SAO 180505, HD 105452, GC 16586, HR 4623, DM CD-24 10174, TYC 6672-995-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Alchiba / Al Minliar al Ghurab",
	"OType" : "High proper-motion Star",
	"Distance" : "14.94",
	"RA_S" : 182.10340218,
	"DEC_S" : -24.7288751,
	"X" : 187,
	"Y" : 551,
	"Constellation" : "Corvus ",
	"AMag" : 4.054,
	"key" : 66297,
	"shortTitle" : "Alchiba; Al Minliar al Ghurab; Al Chiba; Al'chiba",
	"title" : "Alchiba / Al Minliar al Ghurab"
	},
{
	"Index" : "46279",
	"Description" : "Epsilon Corvi (\u03B5 Crv, \u03B5 Corvi) is a star in the southern constellation of Corvus. It has the traditional name Minkar, from Arabian \u0623\u0644\u0645\u0646\u062E\u0631 alm\u00E1nxar meaning \u0022the nostril of the crow\u0022 The apparent visual magnitude is +3.0 and it is located at a distance of 318 light-years (97 parsecs) from Earth.\r\rIn Chinese, \u8EEB\u5BBF (Zh\u011Bn S\u00F9), meaning Chariot (asterism), refers to an asterism consisting of \u03B5 Corvi, \u03B3 Corvi, \u03B4 Corvi and \u03B2 Corvi. Consequently, \u03B5 Corvi itself is known as \u8EEB\u5BBF\u4E8C (Zh\u011Bn S\u00F9 \u00E8r, English: the Second Star of Chariot.).\r\rEpsilon Corvi is a giant star with a stellar classification of K2 III, having consumed the hydrogen at its core and evolved away from the main sequence. It has about three times the Sun\u0027s mass. The interferometry-measured angular diameter of this star is about 4.99 mas, which, at its estimated distance, equates to a physical radius of about 52 times the radius of the Sun. The effective temperature of the outer envelope is 4,320 K, giving it an orange hue that is characteristic of a K-type star.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "2 Corvi, Epsilon Corvi, HIP 59316, SAO 180531, HD 105707, GC 16618, HR 4630, DM BD-21  3487, TYC 6668-992-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Minkar",
	"OType" : "Variable Star",
	"Distance" : "97.44",
	"RA_S" : 182.53116909,
	"DEC_S" : -22.61976722,
	"X" : 180,
	"Y" : 524,
	"Constellation" : "Corvus ",
	"AMag" : 3.138,
	"key" : 66279,
	"title" : "Minkar"
	},
{
	"Index" : "46280",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "3 Corvi, HIP 59394, SAO 180546, HD 105850, GC 16638, HR 4635, DM BD-22  3305, TYC 6668-993-1",
	"group" : { "key" : "Corvus" },
	"Common" : "3 Corvi",
	"OType" : "High proper-motion Star",
	"Distance" : "58.75",
	"RA_S" : 182.76600101,
	"DEC_S" : -23.60242334,
	"Constellation" : "Corvus ",
	"AMag" : 5.452,
	"key" : 66280,
	"title" : "3 Corvi"
	},
{
	"Index" : "41924",
	"Description" : "Gamma Corvi (\u03B3 Crv, \u03B3 Corvi) is the brightest star in the southern constellation of Corvus, having an apparent visual magnitude of 2.6. Its traditional name is Gienah, which it shares with Epsilon Cygni. The name \u0022Gienah Corvi\u0022, or \u0022Gienah Ghurab\u0022, may be used to distinguish it from this star in Cygnus. The distance to this star has been measured directly using the parallax technique, yielding an estimated 154 light-years (47 parsecs) from Earth.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "4 Corvi, Gamma Corvi, HIP 59803, SAO 157176, HD 106625, GC 16740, HR 4662, DM BD-16  3424, TYC 6098-1754-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Gienah",
	"OType" : "Variable Star",
	"Distance" : "47.1",
	"RA_S" : 183.95154504,
	"DEC_S" : -17.54193046,
	"X" : 158,
	"Y" : 459,
	"Constellation" : "Corvus ",
	"AMag" : 2.532,
	"key" : 61924,
	"shortTitle" : "Gienah Ghurab; Dzhanakh; Giena",
	"title" : "Gienah"
	},
{
	"Index" : "42020",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "5 Corvi, Zeta Corvi, HIP 60189, SAO 180700, HD 107348, GC 16830, HR 4696, DM BD-21  3514, TYC 6108-1477-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Zeta Corvi",
	"OType" : "Be Star",
	"Distance" : "127.27",
	"RA_S" : 185.140175,
	"DEC_S" : -22.21590028,
	"Constellation" : "Corvus ",
	"AMag" : 5.173,
	"key" : 62020,
	"title" : "Zeta Corvi"
	},
{
	"Index" : "37720",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "HIP 60221, SAO 157226, HD 107418, GC 16841, HR 4699, DM BD-12 3614, TYC 5532-1649-1",
	"group" : { "key" : "Corvus" },
	"Common" : "HR 4699",
	"OType" : "Variable Star",
	"Distance" : "61.67",
	"RA_S" : 185.23213798,
	"DEC_S" : -13.56572344,
	"Constellation" : "Corvus ",
	"AMag" : 5.256,
	"key" : 57720,
	"title" : "HR 4699"
	},
{
	"Index" : "41976",
	"Description" : "Delta Corvi (\u03B4 Crv, \u03B4 Corvi) is a star in the southern constellation of Corvus. It has the traditional name Algorab (from Arabian \u0623\u0644\u063A\u0631\u0627\u0628 al-ghuraab, meaning \u0022the crow\u0022). This is a third magnitude star at a distance of 86.9 light-years (26.6 parsecs) from Earth. In 1823, it was found to be a wide double star by British astronomers James South and John Herschel. Since that time, the position of the two stars with respect to each other has not changed.\r\rThis star has more than 2.7 times the mass of the Sun, which is causing it to radiate a much higher energy output\u2014roughly 69 times the Sun\u0027s luminosity. The effective temperature of the outer atmosphere is 10,400 K, giving it the white hue of an A-type star. The spectrum matches a stellar classification of A0 IV(n) kB9. Although it is only around 260 million years old, the luminosity class of \u0027IV\u0027 indicates this is a subgiant star that has nearly exhausted the supply of hydrogen at its core and is in the process of evolving away from the main sequence of stars like the Sun.\r\rAlgorab displays no excess infrared emission that would otherwise suggest the presence of circumstellar matter. It has a magnitude 9.3 companion, HR 4757 B, with a classification of K2Ve at an angular separation of 24.2 arcseconds along a position angle of 214\u00B0. Although the two stars share a common proper motion, the significant differences in their estimated ages suggests that they may not be physically connected.\r\rIn Chinese, \u8EEB\u5BBF (Zh\u011Bn S\u00F9), meaning Chariot (asterism), refers to an asterism consisting of \u03B4 Corvi, \u03B3 Corvi, \u03B5 Corvi and \u03B2 Corvi. Consequently, \u03B4 Corvi itself is known as \u8EEB\u5BBF\u4E09 (Zh\u011Bn S\u00F9 s\u0101n, English: the Third Star of Chariot.).",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "7 Corvi, Delta Corvi, HIP 60965, SAO 157323, HD 108767, GC 17029, HR 4757, DM BD-15  3482, TYC 6103-2395-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Algorab",
	"OType" : "High proper-motion Star",
	"Distance" : "26.63",
	"RA_S" : 187.46606319,
	"DEC_S" : -16.51543126,
	"X" : 113,
	"Y" : 449,
	"Constellation" : "Corvus ",
	"AMag" : 2.926,
	"key" : 61976,
	"shortTitle" : "Algores; Algoral; Algorel; Al'gorab",
	"title" : "Algorab"
	},
{
	"Index" : "41975",
	"Description" : "Eta Corvi (Eta Crv, \u03B7 Corvi, \u03B7 Crv) is an F-type main sequence star, the sixth-brightest star in the constellation of Corvus. Two debris disks have been detected orbiting this star, one warm within a few AU and another out at ~150 AU.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "8 Corvi, Eta Corvi, HIP 61174, SAO 157345, HD 109085, GC 17087, HR 4775, DM BD-15  3489, TYC 6103-2394-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Eta Corvi",
	"OType" : "Variable Star",
	"Distance" : "18.28",
	"RA_S" : 188.01761108,
	"DEC_S" : -16.19600226,
	"X" : 106,
	"Y" : 445,
	"Constellation" : "Corvus ",
	"AMag" : 4.338,
	"key" : 61975,
	"title" : "Eta Corvi"
	},
{
	"Index" : "46345",
	"Description" : "Beta Corvi (Beta Crv, \u03B2 Corvi, \u03B2 Crv) is the second brightest star in the southern constellation of Corvus. It has the traditional name Kraz. The origin and meaning of this name remains uncertain.\r\rIn Chinese, \u8EEB\u5BBF (Zh\u011Bn S\u00F9), meaning Chariot (asterism), refers to an asterism consisting of \u03B2 Corvi, \u03B3 Corvi, \u03B5 Corvi and \u03B4 Corvi. Consequently, \u03B2 Corvi itself is known as \u8EEB\u5BBF\u56DB (Zh\u011Bn S\u00F9 s\u00EC, English: the Fourth Star of Chariot.). Beta Corvi has about 3.7 times the Sun\u0027s mass and is roughly 206 million years in age, which is old enough for a star of this mass to consume the hydrogen at its core and evolve away from the main sequence. The stellar classification is G5 II, with the luminosity class of \u0027II\u0027 indicating this is a bright giant. The effective temperature of the star\u0027s outer envelope is about 5,100 K, which produces a yellow hue common to G-type stars.\r\rThe measured angular diameter of this star is 3.30 \u00B1 0.17 mas. At an estimated distance of 146 light-years (45 parsecs), this yields a physical size of about 16 times the radius of the Sun. Because of the star\u0027s mass and radius, it is emitting about 164 times the luminosity of the Sun. The abundance of elements other than hydrogen or helium, what astronomers term metallicity, is similar to the proportions in the Sun.\r\rThis is a variable star that ranges in apparent visual magnitude from a low of 2.66 to a high of 2.60.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "9 Corvi, Beta Corvi, HIP 61359, SAO 180915, HD 109379, GC 17133, HR 4786, DM BD-22  3401, TYC 6683-1116-1",
	"group" : { "key" : "Corvus" },
	"Common" : "Kraz",
	"OType" : "Variable Star",
	"Distance" : "44.66",
	"RA_S" : 188.59681183,
	"DEC_S" : -23.3967604,
	"X" : 109,
	"Y" : 540,
	"Constellation" : "Corvus ",
	"AMag" : 2.721,
	"key" : 66345,
	"shortTitle" : "Krats",
	"title" : "Kraz"
	},
{
	"Index" : "41762",
	"Description" : "Alpha Crateris (\u03B1 Crt, \u03B1 Crateris) is a star in the constellation Crater. It has the traditional name Alkes, from the Arabic \u0627\u0644\u0643\u0627\u0633 alk\u0101s or \u0627\u0644\u0643\u0623\u0633 alka\u0027s \u0022the cup\u0022.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Aoul al Batjna (\u0623\u0648\u0644 \u0623\u0644\u0628\u062C\u0646 awwil albajna), which was translated into Latin as Prima Crateris, meaning the first cup.\r\rIn Chinese, \u7FFC\u5BBF (Y\u00EC S\u00F9), meaning Wings (asterism), refers to an asterism consisting of \u03B1 Crateris, \u03B3 Crateris, \u03B6 Crateris, \u03BB Crateris, \u03BD Hydrae, \u03B7 Crateris, \u03B4 Crateris, \u03B9 Crateris, \u03BA Crateris, \u03B5 Crateris, HD 95808, HD 93833, \u03B8 Crateris, HD 102574, HD 100219, \u03B2 Crateris, HD 99922, HD 100307, HD 96819, \u03C71 Hydrae, HD 102620 and HD 103462. Consequently, \u03B1 Crateris itself is known as \u7FFC\u5BBF\u4E00 (Y\u00EC S\u00F9 y\u012B, English: the First Star of Wings.).",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "7 Crateris, Alpha Crateris, HIP 53740, SAO 156375, HD 95272, GC 15106, HR 4287, DM BD-17  3273, TYC 6079-1901-1",
	"group" : { "backgroundImage" : "images/Alignment/20.png",
		"description" : "Crater is a constellation. Its name is Latin for cup, and in Greek mythology it is identified with the cup of the god Apollo. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is faint, with no star brighter than third magnitude.\r\rCrater is identified with a story from Greek mythology in which a crow or raven serves Apollo, and is sent to fetch water, but it rests lazily on the journey, and after finally obtaining the water in a cup, takes back a water snake as an excuse. According to the myth, Apollo saw through the fraud, and angrily cast the crow, cup, and snake, into the sky. The constellations of Corvus the crow and Hydra the water-snake are also identified with this myth.",
		"key" : "Crater",
		"grouptype" : "Crater",
		"Meaning" : "cup",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Crater",
		"title" : "Crater Objects Group" },
	"Common" : "Alkes",
	"OType" : "High proper-motion Star",
	"Distance" : "48.79",
	"RA_S" : 164.94360402,
	"DEC_S" : -18.29878471,
	"X" : 393,
	"Y" : 463,
	"Constellation" : "Crater ",
	"AMag" : 4.195,
	"key" : 61762,
	"shortTitle" : "Al'kes",
	"title" : "Alkes"
	},
{
	"Index" : "46173",
	"Description" : "Beta Crateris (\u03B2 Crt, \u03B2 Crateris) is a star in the constellation Crater. Beta Crateris is a white sub-giant belonging to the spectral class A2, has apparent magnitude 4.48, and is about 265 light years from Earth.\r\rShared with \u03BA Hya, this star was Al Tizini\u0027s Al Shar\u0101s\u012Bf (\u0623\u0644\u0635\u0631\u0633\u0649\u0641), the Ribs, \u2014 i.e. of the Hydra, \u2014 and the first of the set\r\rIn Chinese, \u7FFC\u5BBF (Y\u00EC S\u00F9), meaning Wings (asterism), refers to an asterism consisting of \u03B2 Crateris, \u03B1 Crateris, \u03B3 Crateris, \u03B6 Crateris, \u03BB Crateris, \u03BD Hydrae, \u03B7 Crateris, \u03B4 Crateris, \u03B9 Crateris, \u03BA Crateris, \u03B5 Crateris, HD 95808, HD 93833, \u03B8 Crateris, HD 102574, HD 100219, HD 99922, HD 100307, HD 96819, \u03C71 Hydrae, HD 102620 and HD 103462. Consequently, \u03B2 Crateris itself is known as \u7FFC\u5BBF\u5341\u516D (Y\u00EC S\u00F9 sh\u00EDli\u00F9, English: the Sixteenth Star of Wings.)",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "11 Crateris, Beta Crateris, HIP 54682, SAO 179624, HD 97277, GC 15385, HR 4343, DM BD-22  3095, TYC 6649-1274-1",
	"group" : { "key" : "Crater" },
	"Common" : "Beta Crateris",
	"OType" : "Spectroscopic binary",
	"Distance" : "103.69",
	"RA_S" : 167.91453265,
	"DEC_S" : -22.82584981,
	"X" : 356,
	"Y" : 522,
	"Constellation" : "Crater ",
	"AMag" : 4.452,
	"key" : 66173,
	"title" : "Beta Crateris"
	},
{
	"Index" : "37598",
	"Description" : "Delta Crateris (\u03B4 Crt, \u03B4 Crateris) is a star in the constellation Crater. Delta Crateris is an orange giant belonging to the spectral class K0, has apparent magnitude 3.56, and is 195 light years from Earth. This star has 22.44 \u00B1 0.28 times the radius of the Sun and 1.0\u20131.4 times the Sun\u0027s mass. It is radiating 171.4 \u00B1 9.0 as much luminosity as the Sun from its outer envelope at an effective temperature of 4,408 \u00B1 57 K.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "12 Crateris, Delta Crateris, HIP 55282, SAO 156605, HD 98430, GC 15567, HR 4382, DM BD-13  3345, TYC 5514-1423-1",
	"group" : { "key" : "Crater" },
	"Common" : "Delta Crateris",
	"OType" : "High proper-motion Star",
	"Distance" : "56.94",
	"RA_S" : 169.83519818,
	"DEC_S" : -14.77853925,
	"X" : 333,
	"Y" : 417,
	"Constellation" : "Crater ",
	"AMag" : 3.674,
	"key" : 57598,
	"title" : "Delta Crateris"
	},
{
	"Index" : "41836",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "13 Crateris, Lambda Crateris, HIP 55598, SAO 156646, HD 98991, GC 15644, HR 4395, DM BD-17  3367, TYC 6088-2156-1",
	"group" : { "key" : "Crater" },
	"Common" : "Lambda Crateris",
	"OType" : "Star",
	"Distance" : "42.82",
	"RA_S" : 170.84116339,
	"DEC_S" : -18.77997839,
	"Constellation" : "Crater ",
	"AMag" : 5.121,
	"key" : 61836,
	"title" : "Lambda Crateris"
	},
{
	"Index" : "37578",
	"Description" : "Epsilon Crateris (\u03B5 Crt) is a K5III orange giant star in the constellation of Crater, that shines with an apparent magnitude of ~4.82 from a distance of 376 light years.\r\rEpsilon Crateris is located in the sky above Beta Crateris (Labr), and slightly to the left, or east, marking the lower right edge of the rim of the bowl and is somewhat closer to Theta Crateris, which is further east at the top of the bowl.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "14 Crateris, Epsilon Crateris, HIP 55687, SAO 156658, HD 99167, GC 15665, HR 4402, DM BD-10  3260, TYC 5512-1389-1",
	"group" : { "key" : "Crater" },
	"Common" : "Epsilon Crateris",
	"OType" : "Star",
	"Distance" : "115.25",
	"RA_S" : 171.15246302,
	"DEC_S" : -10.85932411,
	"X" : 316,
	"Y" : 366,
	"Constellation" : "Crater ",
	"AMag" : 4.986,
	"key" : 57578,
	"title" : "Epsilon Crateris"
	},
{
	"Index" : "41835",
	"Description" : "Gamma Crateris is a double star system, divisible with a small amateur telescope, and located at the center of the constellation Crater. The primary is a white A-type main sequence star of apparent magnitude 4.1, while the secondary is a small companion of magnitude 9.6. The system is located 84 light years away from the Earth.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "15 Crateris, Gamma Crateris, HIP 55705, SAO 156661, HD 99211, GC 15669, HR 4405, DM BD-16  3244, TYC 6088-2155-1",
	"group" : { "key" : "Crater" },
	"Common" : "Gamma Crateris",
	"OType" : "Double or multiple star",
	"Distance" : "25.24",
	"RA_S" : 171.22051508,
	"DEC_S" : -17.68400833,
	"X" : 315,
	"Y" : 454,
	"Constellation" : "Crater ",
	"AMag" : 4.091,
	"key" : 61835,
	"title" : "Gamma Crateris"
	},
{
	"Index" : "37563",
	"Description" : "Theta Crateris (\u03B8 Crt) is a B9V blue dwarf star in the constellation Crater that sines with an apparent magnitude of 4.68 from a distance of 280 ly. \u03B8 Crt is a low metallicity star with an iron abundance about 54% that of the sun.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "21 Crateris, Theta Crateris, HIP 56633, SAO 138296, HD 100889, GC 15921, HR 4468, DM BD-08  3202, TYC 5510-1508-1",
	"group" : { "key" : "Crater" },
	"Common" : "Theta Crateris",
	"OType" : "Star",
	"Distance" : "85.94",
	"RA_S" : 174.17046972,
	"DEC_S" : -9.8022421,
	"X" : 277,
	"Y" : 353,
	"Constellation" : "Crater ",
	"AMag" : 4.662,
	"key" : 57563,
	"title" : "Theta Crateris"
	},
{
	"Index" : "41913",
	"Description" : "Zeta Crateris (\u03B6 Crt)is a G8III yellow giant star in the constellation Crater with an apparent magnitude of 4.72, shining from a distance of 351 light years.\r\rZeta Crateris appears to be about half way between Epsilon Corvi to the southeast and Beta Crateris to the northwest, and marks the lower left corner of the rim of the bowl. Eta Crateris lies somewhat less than half way from Zeta Crateris to Gamma Corvi, the bright star above, (north) of Epsilon Corvi.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "27 Crateris, Zeta Crateris, HIP 57283AB, SAO 156869, HD 102070, GC 16112, HR 4514, DM BD-17  3460, TYC 6096-2032-1",
	"group" : { "key" : "Crater" },
	"Common" : "Zeta Crateris",
	"OType" : "Double or multiple star",
	"Distance" : "107.7",
	"RA_S" : 176.19073974,
	"DEC_S" : -18.35068448,
	"X" : 254,
	"Y" : 464,
	"Constellation" : "Crater ",
	"AMag" : 4.813,
	"key" : 61913,
	"title" : "Zeta Crateris"
	},
{
	"Index" : "41896",
	"Description" : "Eta Crateris (\u03B7 Crt) is a 5.17 vmag, A1III white giant star, 251 ly from Earth that marks the lip of the tilted bowl on the left side in the constellation Crater. Eta Crateris lies in the sky NE of Zeta Crateris and NNW of 31 Crateris, the three stars forming an almost perfect right triangle with Eta at the right angle and 31 and Zeta the ends of the hypotenuse. Eta Crateris also lies to the right (west) of the bright star Gamma Corvi.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "30 Crateris, Eta Crateris, HIP 58188, SAO 156988, HD 103632, GC 16319, HR 4567, DM BD-16  3358, TYC 6094-1532-1",
	"group" : { "key" : "Crater" },
	"Common" : "Eta Crateris",
	"OType" : "Variable Star",
	"Distance" : "77.07",
	"RA_S" : 179.00397634,
	"DEC_S" : -17.15082944,
	"X" : 218,
	"Y" : 450,
	"Constellation" : "Crater ",
	"AMag" : 5.156,
	"key" : 61896,
	"title" : "Eta Crateris"
	},
{
	"Index" : "63495",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 58379, SAO 239533, HD 103961, GC 16371, HR 4576, DM CP-55 4751, TYC 8639-3562-1",
	"group" : { "backgroundImage" : "images/Alignment/15.png",
		"description" : "Crux (pron.: /\u02C8kr\u028Cks/) is the smallest of the 88 modern constellations, but is one of the most distinctive. Its name is Latin for cross, and it is dominated by a cross-shaped asterism that is commonly known as the Southern Cross.\r\rCrux is easily visible from the southern hemisphere at practically any time of year. It is also visible near the horizon from tropical latitudes of the northern hemisphere for a few hours every night during the northern winter and spring. For instance, it is visible from Cancun or any other place at latitude 25\u00B0 N or less at around 10 pm at the end of April.\r\rCrux was visible to the Ancient Greeks; Ptolemy regarded it as part of the constellation Centaurus. It was entirely visible as far north as Britain in the fourth millennium BC. However, the precession of the equinoxes gradually lowered its stars below the European horizon, and they were eventually forgotten by the inhabitants of northern latitudes. By AD 400, most of the constellation never rose above the horizon for Athenians.\r\rThe 15th century Venetian navigator Alvise Cadamosto made note of what was probably the Southern Cross on exiting the Gambia River in 1455, calling it the carro dell\u0027ostro (\u0022southern chariot\u0022). However, Cadamosto\u0027s constellation had too many stars and was tilted incorrectly. Historians generally credit Jo\u00E3o Faras - astronomer and physician of King Manuel I of Portugal who accompanied Pedro \u00C1lvares Cabral in the discovery of Brazil in 1500 - for being the first European to depict it correctly. Faras sketched and described the constellation (calling it \u0022Las Guardas\u0022) in a letter written on the beaches of Brazil on May 1, 1500, to the Portuguese monarch. \u00C9merie Mollineux has also been cited as the first uranographer to distinguish Crux; his illustration dates to 1592. Later adopters of the constellation included Jakob Bartsch in 1624 and Augustin Royer in 1679. Royer is also sometimes cited as initially distinguishing Crux. Explorer Amerigo Vespucci depicted Crux as an almond, called \u0022Mandorla\u0022.\r\rThe separation of Crux from Centaurus is generally attributed to the French astronomer Augustin Royer in 1679, but other historians attribute the invention of Crux to Petrus Plancius in 1613. However, Crux was later published by Jakob Bartsch in 1624.[1",
		"key" : "Crux",
		"grouptype" : "Crux",
		"Meaning" : "southern cross",
		"Family" : "Hercules",
		"Origin" : "1603, Uranometria, split from Centaurus",
		"shortTitle" : "Crux",
		"title" : "Crux Objects Group" },
	"Common" : "HR 4576",
	"OType" : "Variable Star",
	"Distance" : "231.89",
	"RA_S" : 179.56343709,
	"DEC_S" : -56.31731219,
	"Constellation" : "Crux ",
	"AMag" : 5.424,
	"key" : 83495,
	"title" : "HR 4576"
	},
{
	"Index" : "66789",
	"Description" : "Theta1 Crucis (\u03B81 Cru, Theta1 Crucis) is a spectroscopic binary star in the constellation Crux. It has an apparent magnitude of 4.32m. The spectral class of the star is Am. Theta1 Crucis is located at 230 light-years from the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Theta01 Crucis, HIP 58758, SAO 251705, HD 104671, GC 16463, HR 4599, DM CP-62  2543, TYC 8978-6112-1",
	"group" : { "key" : "Crux" },
	"Common" : "Theta1 Crucis",
	"OType" : "Spectroscopic binary",
	"Distance" : "72.04",
	"RA_S" : 180.75625643,
	"DEC_S" : -63.31293112,
	"X" : 453,
	"Y" : 479,
	"Constellation" : "Crux ",
	"AMag" : 4.348,
	"key" : 86789,
	"title" : "Theta1 Crucis"
	},
{
	"Index" : "66788",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Theta02 Crucis, HIP 58867, SAO 251717, HD 104841, GC 16490, HR 4603, DM CP-62  2561, TYC 8978-6111-1",
	"group" : { "key" : "Crux" },
	"Common" : "Theta02 Crucis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "259.59",
	"RA_S" : 181.08007422,
	"DEC_S" : -63.16571068,
	"Constellation" : "Crux ",
	"AMag" : 4.7,
	"key" : 86788,
	"title" : "Theta02 Crucis"
	},
{
	"Index" : "66846",
	"Description" : "\u03B7 Crucis (\u03B7 Cru, Eta Crucis) is a star in the constellation Crux. It has an apparent magnitude of 4.14m. The star is classified as a yellow-white giant (spectral class F2 III). \u03B7 Crucis is located at 64 light-years from the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Eta Crucis, HIP 59072, SAO 251742, HD 105211, GC 16551, HR 4616, DM CP-63  2145, TYC 8982-4970-1",
	"group" : { "key" : "Crux" },
	"Common" : "Eta Crucis",
	"OType" : "Spectroscopic binary",
	"Distance" : "19.75",
	"RA_S" : 181.72041604,
	"DEC_S" : -64.61373057,
	"X" : 470,
	"Y" : 490,
	"Constellation" : "Crux ",
	"AMag" : 4.177,
	"key" : 86846,
	"title" : "Eta Crucis"
	},
{
	"Index" : "63568",
	"Description" : "Delta Crucis (\u03B4 Cru, \u03B4 Crucis) is a star in the southern circumpolar constellation of Crux. It is sometimes called P\u00E1lida (Pale [one]) in Portuguese. This star is of apparent magnitude 2.79 and is located at a distance of about 345 light-years (106 parsecs) from Earth, the faintest of the four bright stars that form the prominent asterism known as the Southern Cross. Delta Crucis is massive, hot and rapidly rotating star that is in the process of evolving into a giant.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Delta Crucis, HIP 59747, SAO 239791, HD 106490, GC 16724, HR 4656, DM CP-58  4189, TYC 8645-2263-1",
	"group" : { "key" : "Crux" },
	"Common" : "Delta Crucis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "105.79",
	"RA_S" : 183.78631757,
	"DEC_S" : -58.74892829,
	"X" : 448,
	"Y" : 417,
	"Constellation" : "Crux ",
	"AMag" : 2.721,
	"key" : 83568,
	"title" : "Delta Crucis"
	},
{
	"Index" : "66863",
	"Description" : "\u03B6 Crucis (\u03B6 Cru, Zeta Crucis) is a binary star in the constellation Crux. It has an apparent magnitude of 4.06m. The primary star is classified as a blue-white dwarf (spectral class B2.5 V). The secondary component is much fainter, with an apparent magnitude of 12.49. \u03B6 Crucis is located at about 360 light-years from the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Zeta Crucis, HIP 60009, SAO 251841, HD 106983, GC 16785, HR 4679, DM CP-63  2235, TYC 8983-2258-1",
	"group" : { "key" : "Crux" },
	"Common" : "Zeta Crucis",
	"OType" : "Star",
	"Distance" : "109.33",
	"RA_S" : 184.60934991,
	"DEC_S" : -64.00307083,
	"X" : 429,
	"Y" : 483,
	"Constellation" : "Crux ",
	"AMag" : 4.011,
	"key" : 86863,
	"title" : "Zeta Crucis"
	},
{
	"Index" : "66709",
	"Description" : "Epsilon Crucis (\u03B5 Cru, \u03B5 Crucis) is a Class K3III, fourth-magnitude star in the constellation Crux. It is sometimes called Intrometida (intrusive) in Portuguese. This star is an orange giant, located about 228 light-years from Earth.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Epsilon Crucis, HIP 60260, SAO 251862, HD 107446, GC 16849, HR 4700, DM CP-59  4188, TYC 8975-4125-1",
	"group" : { "key" : "Crux" },
	"Common" : "Epsilon Crucis",
	"OType" : "Variable Star",
	"Distance" : "70.46",
	"RA_S" : 185.34003799,
	"DEC_S" : -60.40114907,
	"X" : 433,
	"Y" : 436,
	"Constellation" : "Crux ",
	"AMag" : 3.734,
	"key" : 86709,
	"title" : "Epsilon Crucis"
	},
{
	"Index" : "63527",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 60379, SAO 239901, HD 107696, GC 16877, HR 4706, DM CP-56 5202, TYC 8641-2593-1",
	"group" : { "key" : "Crux" },
	"Common" : "HR 4706",
	"OType" : "Star",
	"Distance" : "110.73",
	"RA_S" : 185.70596296,
	"DEC_S" : -57.67613118,
	"Constellation" : "Crux ",
	"AMag" : 5.351,
	"key" : 83527,
	"title" : "HR 4706"
	},
{
	"Index" : "66800",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "256 Crucis, SAO 251903, HD 108250, GC 16951, HR 4729, DM CP-62  2742, TYC 8979-3466-1",
	"group" : { "key" : "Crux" },
	"Common" : "256 Crucis",
	"OType" : "Star",
	"RA_S" : 186.62868845,
	"DEC_S" : -63.12223768,
	"Constellation" : "Crux ",
	"AMag" : 4.799,
	"key" : 86800,
	"title" : "256 Crucis"
	},
{
	"Index" : "66799",
	"Description" : "Alpha Crucis (\u03B1 Cru, \u03B1 Crucis, also Acrux, HD 108248) is the brightest star in the constellation Crux, the Southern Cross, and, at a combined visual magnitude 0.77, is the twelfth brightest star in the night sky. Acrux is the southernmost first-magnitude star, just a bit more southerly than Alpha Centauri.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Alpha01 Crucis, HIP 60718B, SAO 251904, HD 108248J, GC 16952, HR 4730, DM CP-62  2745A, TYC 8979-3465-1",
	"group" : { "key" : "Crux" },
	"Common" : "Acrux",
	"OType" : "Spectroscopic binary",
	"Distance" : "98.48",
	"RA_S" : 186.6495634,
	"DEC_S" : -63.09909286,
	"X" : 420,
	"Y" : 469,
	"Constellation" : "Crux ",
	"AMag" : 0.77,
	"key" : 86799,
	"shortTitle" : "Akruks",
	"title" : "Acrux"
	},
{
	"Index" : "63713",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "39 Crucis, HIP 61966, SAO 240161, HD 110335, GC 17268, HR 4823, DM CP-59  4393, TYC 8659-3106-1",
	"group" : { "key" : "Crux" },
	"Common" : "39 Crucis",
	"OType" : "Be Star",
	"Distance" : "291.38",
	"RA_S" : 190.48570127,
	"DEC_S" : -59.6858208,
	"Constellation" : "Crux ",
	"AMag" : 4.904,
	"key" : 83713,
	"title" : "39 Crucis"
	},
{
	"Index" : "66993",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 62027, SAO 252002, HD 110432, GC 17286, HR 4830, DM CP-62 2898, TYC 8992-1861-1",
	"group" : { "key" : "Crux" },
	"Common" : "HR 4830",
	"OType" : "Be Star",
	"Distance" : "367.61",
	"RA_S" : 190.70944482,
	"DEC_S" : -63.05862211,
	"Constellation" : "Crux ",
	"AMag" : 5.332,
	"key" : 86993,
	"title" : "HR 4830"
	},
{
	"Index" : "66916",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Iota Crucis, HIP 62268, SAO 252016, HD 110829, GC 17339, HR 4842, DM CP-60  4273, TYC 8988-2172-1",
	"group" : { "key" : "Crux" },
	"Common" : "Iota Crucis",
	"OType" : "Star",
	"Distance" : "36.8",
	"RA_S" : 191.40854771,
	"DEC_S" : -60.98131765,
	"Constellation" : "Crux ",
	"AMag" : 4.803,
	"key" : 86916,
	"title" : "Iota Crucis"
	},
{
	"Index" : "63672",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 62327, SAO 240235, HD 110956, GC 17352, HR 4848, DM CP-55 5215, TYC 8655-4100-1",
	"group" : { "key" : "Crux" },
	"Common" : "HR 4848",
	"OType" : "Star",
	"Distance" : "117.83",
	"RA_S" : 191.59464529,
	"DEC_S" : -56.48880994,
	"Constellation" : "Crux ",
	"AMag" : 4.594,
	"key" : 83672,
	"title" : "HR 4848"
	},
{
	"Index" : "63683",
	"Description" : "Mu Crucis (\u03BC Cru, \u03BC Crucis) the 7th brightest star in the constellation Crux, or Southern Cross. It is a wide binary of spectral class B stars, each of magnitude 4.0 and 5.1. They lie about 360\u2212380 light years away.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Mu01 Crucis, HIP 63003, SAO 240366, HD 112092, GC 17512, HR 4898, DM CP-56  5487A, TYC 8656-3488-1",
	"group" : { "key" : "Crux" },
	"Common" : "Mu Crucis",
	"OType" : "Variable Star",
	"Distance" : "126.99",
	"RA_S" : 193.64843978,
	"DEC_S" : -57.17791894,
	"X" : 382,
	"Y" : 388,
	"Constellation" : "Crux ",
	"AMag" : 3.938,
	"key" : 83683,
	"title" : "Mu Crucis"
	},
{
	"Index" : "63682",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Mu02 Crucis, HIP 63005, SAO 240367, HD 112091, GC 17513, HR 4899, DM CP-56  5487B, TYC 8656-3487-1",
	"group" : { "key" : "Crux" },
	"Common" : "Mu02 Crucis",
	"OType" : "Be Star",
	"Distance" : "124.68",
	"RA_S" : 193.65372053,
	"DEC_S" : -57.16868306,
	"Constellation" : "Crux ",
	"AMag" : 4.951,
	"key" : 83682,
	"title" : "Mu02 Crucis"
	},
{
	"Index" : "63724",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Lambda Crucis, HIP 63007, SAO 240368, HD 112078, GC 17514, HR 4897, DM CP-58  4584, TYC 8660-2695-1",
	"group" : { "key" : "Crux" },
	"Common" : "Lambda Crucis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "117.58",
	"RA_S" : 193.66326199,
	"DEC_S" : -59.14670296,
	"Constellation" : "Crux ",
	"AMag" : 4.578,
	"key" : 83724,
	"title" : "Lambda Crucis"
	},
{
	"Index" : "63680",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 63117, SAO 240385, HD 112244, GC 17540, HR 4908, DM CP-56 5498, TYC 8656-3196-1",
	"group" : { "key" : "Crux" },
	"Common" : "HR 4908",
	"OType" : "Blue supergiant star",
	"RA_S" : 193.98805955,
	"DEC_S" : -56.83580345,
	"Constellation" : "Crux ",
	"AMag" : 5.366,
	"key" : 83680,
	"title" : "HR 4908"
	},
{
	"Index" : "24691",
	"Description" : "Kappa Cygni (\u03BA Cyg) is a star in the northern constellation of Cygnus. It has an apparent visual magnitude of 3.8, which is bright enough to be seen with the naked eye. In the constellation, it forms the tip of Cygnus the swan\u0027s left wing. The radiant of the minor Kappa Cygnids meteor shower is located about 5\u00B0 north of this star.\r\rExamination of this star\u0027s spectrum show it to match a stellar classification of G9 III, with the \u0027III\u0027 luminosity class revealing that it has consumed the hydrogen fuel at its core and expanded into the giant star stage of its stellar evolution. It is known to vary in luminosity, but only by about 0.01 to 0.02 magnitudes. The measured angular diameter of this star, after correction for limb darkening, is 2.07 \u00B1 0.09 mas. At an estimated distance of 124.2 light-years (38.1 parsecs) based on parallax measurements, this yields a physical size of about 8\u20139 times the radius of the Sun. The outer envelope has an effective temperature of 4,920 K, giving it the yellow-orange hue of a star near the transition from a G- to a K-type classification.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "1 Cygni, Kappa Cygni, HIP 94779, SAO 31537, HD 181276, GC 26621, HR 7328, DM BD+53  2216, TYC 3920-1971-1",
	"group" : { "backgroundImage" : "images/Alignment/22.png",
		"description" : "Cygnus (pron.: /\u02C8s\u026A\u0261n\u0259s/) is a northern constellation lying on the plane of the Milky Way. Its name is the Latinized Hellenic (Greek) word for swan. One of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross (in contrast to the Southern Cross). Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.\r\rIn Greek mythology, Cygnus has been identified with several different legendary swans. Zeus disguised himself as a swan to seduce Leda, Spartan king Tyndareus\u0027s wife, who gave birth to the Gemini, Helen of Troy and Clytemnestra; Orpheus was transformed into a swan after his murder, and was said to have been placed in the sky next to his lyre (Lyra); and the King Cycnus was transformed into a swan.\r\rIn Ovid\u0027s Metamorphoses, there are three people named Cygnus, all of whom are transformed into swans. Alongside Cycnus, noted above, he mentions a boy from Tempe who commits suicide when Phyllius refuses to give him a tamed bull that he demands, but is transformed into a swan and flies away. He also mentions a son of Neptune who is an invulnerable warrior in the Trojan War who is eventually defeated by Achilles, but Neptune saves him by transforming him into a swan.\r\rCygnus, together with other avian constellations near the summer solstice, Vultur cadens and Aquila, may be a significant part of the origin of the myth of the Stymphalian Birds, one of The Twelve Labours of Hercules.\r\rNormally, Cygnus is depicted with Delta and Epsilon Cygni as its wings, Deneb as its tail, and Albireo as the tip of its beak.",
		"key" : "Cygnus",
		"grouptype" : "Cygnus",
		"Meaning" : "swan or Northern Cross",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Cygnus",
		"title" : "Cygnus Objects Group" },
	"Common" : "Kappa Cygni",
	"OType" : "Variable Star",
	"Distance" : "38.07",
	"RA_S" : 289.27570408,
	"DEC_S" : 53.36845789,
	"X" : 523,
	"Y" : 94,
	"Constellation" : "Cygnus ",
	"AMag" : 3.884,
	"key" : 44691,
	"title" : "Kappa Cygni"
	},
{
	"Index" : "9383",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "2 Cygni, HIP 95372, SAO 87159, HD 182568, GC 26785, HR 7372, DM BD+29  3584, TYC 2137-3101-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "2 Cygni",
	"OType" : "Star",
	"Distance" : "257.49",
	"RA_S" : 291.03158017,
	"DEC_S" : 29.62134672,
	"Constellation" : "Cygnus ",
	"AMag" : 4.957,
	"key" : 29383,
	"title" : "2 Cygni"
	},
{
	"Index" : "13702",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "4 Cygni, HIP 95556, SAO 68301, HD 183056, GC 26846, HR 7395, DM BD+36  3557, TYC 2666-2297-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "4 Cygni",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "216.33",
	"RA_S" : 291.53802269,
	"DEC_S" : 36.3178979,
	"Constellation" : "Cygnus ",
	"AMag" : 5.143,
	"key" : 33702,
	"title" : "4 Cygni"
	},
{
	"Index" : "21410",
	"Description" : "The Bayer designation Iota Cygni (\u03B9 Cyg / \u03B9 Cygni) is shared by two stars, in the constellation Cygnus. Iota1 Cygni (\u03B91 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 5.75. Iota2 Cygni (\u03B92 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.76.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "10 Cygni, Iota Cygni, HIP 95853, SAO 31702, HD 184006, GC 26947, HR 7420, DM BD+51  2605, TYC 3555-2112-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Iota Cygni",
	"OType" : "Star",
	"Distance" : "37.2",
	"RA_S" : 292.42649498,
	"DEC_S" : 51.72978175,
	"X" : 504,
	"Y" : 121,
	"Constellation" : "Cygnus ",
	"AMag" : 3.775,
	"key" : 41410,
	"title" : "Iota Cygni"
	},
{
	"Index" : "9344",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "6 Cygni, Beta02 Cygni, HIP 95951, SAO 87302, HD 183914, GC 26956, HR 7418, DM BD+27  3411, TYC 2133-2963-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Beta02 Cygni",
	"OType" : "Be Star",
	"Distance" : "122.41",
	"RA_S" : 292.6891415,
	"DEC_S" : 27.96526807,
	"Constellation" : "Cygnus ",
	"AMag" : 4.683,
	"key" : 29344,
	"title" : "Beta02 Cygni"
	},
{
	"Index" : "13649",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "8 Cygni, HIP 96052, SAO 68447, HD 184171, GC 26988, HR 7426, DM BD+34  3590, TYC 2663-1148-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "8 Cygni",
	"OType" : "Star",
	"Distance" : "263.29",
	"RA_S" : 292.94300702,
	"DEC_S" : 34.45296571,
	"Constellation" : "Cygnus ",
	"AMag" : 4.709,
	"key" : 33649,
	"title" : "8 Cygni"
	},
{
	"Index" : "17778",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 96288, SAO 48601, HD 184875, GC 27070, HR 7444, DM BD+42 3386, TYC 3143-2179-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7444",
	"OType" : "Star",
	"Distance" : "176.44",
	"RA_S" : 293.67191352,
	"DEC_S" : 42.41250848,
	"Constellation" : "Cygnus ",
	"AMag" : 5.344,
	"key" : 37778,
	"title" : "HR 7444"
	},
{
	"Index" : "9561",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "9 Cygni, HIP 96302, SAO 87385, HD 184759, GC 27062, HR 7441, DM BD+29  3651A, TYC 2150-5010-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "9 Cygni",
	"OType" : "Star",
	"Distance" : "170.66",
	"RA_S" : 293.71219918,
	"DEC_S" : 29.46295717,
	"Constellation" : "Cygnus ",
	"AMag" : 5.471,
	"key" : 29561,
	"title" : "9 Cygni"
	},
{
	"Index" : "21517",
	"Description" : "Theta Cygni (\u03B8 Cygni, \u03B8 Cyg) is a star in the northern constellation of Cygnus. It has an apparent visual magnitude of 4.5, so it can be seen from the northern hemisphere with the naked eye in sufficiently dark skies. Based upon parallax measurements, it is at a distance of about 59.8 light-years (18.3 parsecs) from the Earth. It is suspected of hosting an extrasolar planet.\r\rThe spectrum of this star matches a stellar classification of F3 V. The luminosity class \u0027V\u0027 is associated with a category of stars called main sequence, which, like the Sun, are generating energy through the nuclear fusion of hydrogen at their cores. The outer envelope of this star is radiating 4.2 times the luminosity of the Sun at an effective temperature of about 6,381 K, which gives it the yellow-white hue typical of F-type stars. Theta Cygni is larger than the Sun, with about 38% more mass and a 58% greater radius. The estimated age of this star is probably in the range of 0.6\u20131.9 billion years.\r\rTheta Cygni has a faint companion star at an angular separation of about three arcseconds and a position angle of 56\u00B0. This star has an apparent visual magnitude of 13.03, which is too faint to be seen without a telescope. It is a red dwarf star with a stellar classification of M3 V and an estimated mass of about 0.33 times the mass of the Sun. Both components of this system are traveling together through space with a high proper motion of 0.261 arcseconds per year, or 0.4\u00B0 per century.\r\rRadial velocity variations of Theta Cygni have been detected by the ELODIE team while searching of extrasolar planets. Desort et al. (2009) infer these variations are not caused by a dim stellar companion roughly 80 Astronomical Units away from the star, but suggest instead the presence of a perturbing planetary object, twice as massive as Jupiter and orbiting around the primary star in less than half a year. This extrasolar planet has yet to be confirmed.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "13 Cygni, Theta Cygni, HIP 96441, SAO 31815, HD 185395, GC 27141, HR 7469, DM BD+49  3062, TYC 3564-3157-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Theta Cygni",
	"OType" : "High proper-motion Star",
	"Distance" : "18.34",
	"RA_S" : 294.11055588,
	"DEC_S" : 50.22109911,
	"X" : 495,
	"Y" : 144,
	"Constellation" : "Cygnus ",
	"AMag" : 4.534,
	"key" : 41517,
	"title" : "Theta Cygni"
	},
{
	"Index" : "17814",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 96459, SAO 48649, HD 185351, GC 27140, HR 7468, DM BD+44 3185, TYC 3147-1921-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7468",
	"OType" : "Star",
	"Distance" : "40.83",
	"RA_S" : 294.15823492,
	"DEC_S" : 44.69493523,
	"Constellation" : "Cygnus ",
	"AMag" : 5.273,
	"key" : 37814,
	"title" : "HR 7468"
	},
{
	"Index" : "13570",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "12 Cygni, Phi Cygni, HIP 96683, SAO 68637, HD 185734, GC 27203, HR 7478, DM BD+29  3684, TYC 2656-5248-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Phi Cygni",
	"OType" : "Spectroscopic binary",
	"Distance" : "81.6",
	"RA_S" : 294.84419106,
	"DEC_S" : 30.1533234,
	"Constellation" : "Cygnus ",
	"AMag" : 4.78,
	"key" : 33570,
	"title" : "Phi Cygni"
	},
{
	"Index" : "17777",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "14 Cygni, HIP 96693, SAO 48691, HD 185872, GC 27213, HR 7483, DM BD+42  3413, TYC 3143-2178-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "14 Cygni",
	"OType" : "Star",
	"Distance" : "199.65",
	"RA_S" : 294.86034812,
	"DEC_S" : 42.81828148,
	"Constellation" : "Cygnus ",
	"AMag" : 5.388,
	"key" : 37777,
	"title" : "14 Cygni"
	},
{
	"Index" : "21424",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 96825, SAO 48718, HD 186155, GC 27249, HR 7495, DM BD+45 2949, TYC 3556-3772-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7495",
	"OType" : "Variable Star",
	"Distance" : "49.62",
	"RA_S" : 295.20909667,
	"DEC_S" : 45.52494249,
	"Constellation" : "Cygnus ",
	"AMag" : 5.105,
	"key" : 41424,
	"title" : "HR 7495"
	},
{
	"Index" : "13726",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "15 Cygni, HIP 97118, SAO 68778, HD 186675, GC 27328, HR 7517, DM BD+37  3586, TYC 2668-995-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "15 Cygni",
	"OType" : "Star",
	"Distance" : "88.62",
	"RA_S" : 296.06918753,
	"DEC_S" : 37.35435889,
	"Constellation" : "Cygnus ",
	"AMag" : 4.991,
	"key" : 33726,
	"title" : "15 Cygni"
	},
{
	"Index" : "21433",
	"Description" : "Delta Cygni (\u03B4 Cygni, \u03B4 Cyg) is the third-magnitude star in the constellation Cygnus. It has the traditional name Rukh. It will be the \u0022North Star\u0022 for at least four centuries around 11,250.\r\rThis star belonged to the Arabic asterism al-Faw\u0101ris (\u0627\u0644\u0641\u0648\u0627\u0631\u0633), meaning \u0022the Riders\u0022 in indigenous Arabic., together with \u03B6, \u03B5, and \u03B3 Cyg, the transverse of the Northern Cross.\r\rIn Chinese, \u5929\u6D25 (Ti\u0101n J\u012Bn), meaning Celestial Ford, refers to an asterism consisting of \u03B4 Cygni, \u03B3 Cygni, 30 Cygni, \u03B1 Cygni, \u03BD Cygni, \u03C4 Cygni, \u03C5 Cygni, \u03B6 Cygni and \u03B5 Cygni. Consequently, \u03B4 Cygni itself is known as \u5929\u6D25\u4E8C (Ti\u0101n J\u012Bn \u00E8r, English: the Second Star of Celestial Ford.)",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "18 Cygni, Delta Cygni, HIP 97165B, SAO 48796, HD 186882, GC 27347, HR 7528, DM BD+44  3234, TYC 3557-2486-2",
	"group" : { "key" : "Cygnus" },
	"Common" : "Rukh",
	"OType" : "Star",
	"Distance" : "52.4",
	"RA_S" : 296.24366059,
	"DEC_S" : 45.13081002,
	"X" : 489,
	"Y" : 212,
	"Constellation" : "Cygnus ",
	"AMag" : 2.86,
	"key" : 41433,
	"title" : "Rukh"
	},
{
	"Index" : "21432",
	"Description" : "Delta Cygni (\u03B4 Cygni, \u03B4 Cyg) is the third-magnitude star in the constellation Cygnus. It has the traditional name Rukh. It will be the \u0022North Star\u0022 for at least four centuries around 11,250.\r\rThis star belonged to the Arabic asterism al-Faw\u0101ris (\u0627\u0644\u0641\u0648\u0627\u0631\u0633), meaning \u0022the Riders\u0022 in indigenous Arabic., together with \u03B6, \u03B5, and \u03B3 Cyg, the transverse of the Northern Cross.\r\rIn Chinese, \u5929\u6D25 (Ti\u0101n J\u012Bn), meaning Celestial Ford, refers to an asterism consisting of \u03B4 Cygni, \u03B3 Cygni, 30 Cygni, \u03B1 Cygni, \u03BD Cygni, \u03C4 Cygni, \u03C5 Cygni, \u03B6 Cygni and \u03B5 Cygni. Consequently, \u03B4 Cygni itself is known as \u5929\u6D25\u4E8C (Ti\u0101n J\u012Bn \u00E8r, English: the Second Star of Celestial Ford.)",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "18 Cygni, Delta Cygni, HIP 97165A, SAO 48796, HD 186882, GC 27347, HR 7528, DM BD+44  3234, TYC 3557-2486-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Rukh",
	"OType" : "Star",
	"Distance" : "52.4",
	"RA_S" : 296.24366059,
	"DEC_S" : 45.13081002,
	"X" : 489,
	"Y" : 212,
	"Constellation" : "Cygnus ",
	"AMag" : 2.893,
	"key" : 41432,
	"title" : "Rukh"
	},
{
	"Index" : "13619",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "17 Cygni, HIP 97295, SAO 68827, HD 187013, GC 27369, HR 7534, DM BD+33  3587, TYC 2660-4227-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "17 Cygni",
	"OType" : "Star",
	"Distance" : "21.23",
	"RA_S" : 296.60666492,
	"DEC_S" : 33.72759409,
	"Constellation" : "Cygnus ",
	"AMag" : 5.056,
	"key" : 33619,
	"title" : "17 Cygni"
	},
{
	"Index" : "17701",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "19 Cygni, HIP 97630, SAO 68947, HD 187849, GC 27486, HR 7566, DM BD+38  3780, TYC 3137-3764-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "19 Cygni",
	"OType" : "Long-period variable star",
	"Distance" : "211.76",
	"RA_S" : 297.64164935,
	"DEC_S" : 38.72241828,
	"Constellation" : "Cygnus ",
	"AMag" : 5.376,
	"key" : 37701,
	"title" : "19 Cygni"
	},
{
	"Index" : "24816",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "20 Cygni, d Cygni, HIP 97635, SAO 32042, HD 188056, GC 27506, HR 7576, DM BD+52  2547, TYC 3935-2415-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "d Cygni",
	"OType" : "Variable Star",
	"Distance" : "62.07",
	"RA_S" : 297.65718065,
	"DEC_S" : 52.98800313,
	"Constellation" : "Cygnus ",
	"AMag" : 5.161,
	"key" : 44816,
	"title" : "d Cygni"
	},
{
	"Index" : "24907",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "23 Cygni, HIP 97870, SAO 32085, HD 188665, GC 27571, HR 7608, DM BD+57  2084, TYC 3943-2323-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "23 Cygni",
	"OType" : "Star",
	"Distance" : "193.82",
	"RA_S" : 298.32240687,
	"DEC_S" : 57.52348029,
	"Constellation" : "Cygnus ",
	"AMag" : 5.111,
	"key" : 44907,
	"title" : "23 Cygni"
	},
{
	"Index" : "21566",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "24 Cygni, Psi Cygni, HIP 98055A, TYC 3570-2426-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "24 Psi Cygni (HR 7619)",
	"OType" : "Double or multiple star",
	"Distance" : "86.17",
	"RA_S" : 298.90746511,
	"DEC_S" : 52.43896872,
	"Constellation" : "Cygnus ",
	"AMag" : 5.032,
	"key" : 41566,
	"title" : "24 Psi Cygni (HR 7619)"
	},
{
	"Index" : "17702",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "22 Cygni, HIP 98068, SAO 69101, HD 188892, GC 27613, HR 7613, DM BD+38  3817, TYC 3137-3765-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "22 Cygni",
	"OType" : "Star",
	"Distance" : "423.23",
	"RA_S" : 298.96567714,
	"DEC_S" : 38.48670686,
	"Constellation" : "Cygnus ",
	"AMag" : 4.93,
	"key" : 37702,
	"title" : "22 Cygni"
	},
{
	"Index" : "24940",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 98073, SAO 32122, HD 189276, GC 27635, HR 7633, DM BD+58 2013, TYC 3947-2622-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7633",
	"OType" : "Star",
	"Distance" : "279.73",
	"RA_S" : 298.98074169,
	"DEC_S" : 58.84596771,
	"Constellation" : "Cygnus ",
	"AMag" : 5.15,
	"key" : 44940,
	"title" : "HR 7633"
	},
{
	"Index" : "13871",
	"Description" : "Eta Cygni (\u03B7 Cyg) is a star in the constellation Cygnus. It is located about 137 light years from the Sun and is categorized as an orange giant star of spectral class K0III.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "21 Cygni, Eta Cygni, HIP 98110, SAO 69116, HD 188947, GC 27622, HR 7615, DM BD+34  3798, TYC 2677-1816-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Eta Cygni",
	"OType" : "Star",
	"Distance" : "41.37",
	"RA_S" : 299.07655211,
	"DEC_S" : 35.08342314,
	"X" : 480,
	"Y" : 346,
	"Constellation" : "Cygnus ",
	"AMag" : 4.008,
	"key" : 33871,
	"title" : "Eta Cygni"
	},
{
	"Index" : "17760",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 98194, SAO 49011, HD 189178, GC 27649, HR 7628, DM BD+39 3968, TYC 3141-3693-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7628",
	"OType" : "Spectroscopic binary",
	"Distance" : "338.44",
	"RA_S" : 299.30778185,
	"DEC_S" : 40.36783048,
	"Constellation" : "Cygnus ",
	"AMag" : 5.439,
	"key" : 37760,
	"title" : "HR 7628"
	},
{
	"Index" : "13759",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 98325, SAO 69188, HD 189395, GC 27677, HR 7640, DM BD+30 3837, TYC 2670-4761-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7640",
	"OType" : "Star",
	"Distance" : "142.38",
	"RA_S" : 299.65826056,
	"DEC_S" : 30.98367529,
	"Constellation" : "Cygnus ",
	"AMag" : 5.492,
	"key" : 33759,
	"title" : "HR 7640"
	},
{
	"Index" : "13971",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "25 Cygni, HIP 98425, SAO 69231, HD 189687, GC 27724, HR 7647, DM BD+36  3806, TYC 2682-3762-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "25 Cygni",
	"OType" : "Be Star",
	"Distance" : "402",
	"RA_S" : 299.97998101,
	"DEC_S" : 37.04288613,
	"Constellation" : "Cygnus ",
	"AMag" : 5.12,
	"key" : 33971,
	"title" : "25 Cygni"
	},
{
	"Index" : "21534",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "26 Cygni, e Cygni, HIP 98571, SAO 49098, HD 190147, GC 27770, HR 7660, DM BD+49  3158, TYC 3566-1919-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "e Cygni",
	"OType" : "Star",
	"Distance" : "133.03",
	"RA_S" : 300.33984942,
	"DEC_S" : 50.10469424,
	"Constellation" : "Cygnus ",
	"AMag" : 5.173,
	"key" : 41534,
	"title" : "e Cygni"
	},
{
	"Index" : "13999",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "27 Cygni, b01 Cygni, HIP 99031, SAO 69413, HD 191026, GC 27904, HR 7689, DM BD+35  3959, TYC 2683-3963-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "b01 Cygni",
	"OType" : "Variable of RS CVn type",
	"Distance" : "23.94",
	"RA_S" : 301.59069282,
	"DEC_S" : 35.97246924,
	"Constellation" : "Cygnus ",
	"AMag" : 5.48,
	"key" : 33999,
	"title" : "b01 Cygni"
	},
{
	"Index" : "13997",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "28 Cygni, b02 Cygni, HIP 99303, SAO 69518, HD 191610, GC 27980, HR 7708, DM BD+36  3907, TYC 2683-3961-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "b02 Cygni",
	"OType" : "Be Star",
	"Distance" : "315.44",
	"RA_S" : 302.356746,
	"DEC_S" : 36.83961894,
	"Constellation" : "Cygnus ",
	"AMag" : 4.904,
	"key" : 33997,
	"title" : "b02 Cygni"
	},
{
	"Index" : "21456",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "30 Cygni, HIP 99639, SAO 49332, HD 192514, GC 28091, HR 7730, DM BD+46  2881, TYC 3559-2796-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "30 Cygni",
	"OType" : "Variable Star",
	"Distance" : "186.41",
	"RA_S" : 303.3252237,
	"DEC_S" : 46.81567203,
	"Constellation" : "Cygnus ",
	"AMag" : 4.832,
	"key" : 41456,
	"title" : "30 Cygni"
	},
{
	"Index" : "24928",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "33 Cygni, HIP 99655, SAO 32378, HD 192696, GC 28108, HR 7740, DM BD+56  2376, TYC 3945-1798-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "33 Cygni",
	"OType" : "Variable Star",
	"Distance" : "48.83",
	"RA_S" : 303.34944491,
	"DEC_S" : 56.56772172,
	"Constellation" : "Cygnus ",
	"AMag" : 4.287,
	"key" : 44928,
	"title" : "33 Cygni"
	},
{
	"Index" : "21457",
	"Description" : "Omicron1 Cygni (\u03BF1 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.76.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "31 Cygni, Omicron01 Cygni, HIP 99675, SAO 49337, HD 192577, GC 28099, HR 7735, DM BD+46  2882A, TYC 3559-2797-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Omicron1 Cygni",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "267.05",
	"RA_S" : 303.40794312,
	"DEC_S" : 46.74133072,
	"X" : 423,
	"Y" : 199,
	"Constellation" : "Cygnus ",
	"AMag" : 3.929,
	"key" : 41457,
	"title" : "Omicron1 Cygni"
	},
{
	"Index" : "13998",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "29 Cygni, b03 Cygni, HIP 99770, SAO 69678, HD 192640, GC 28124, HR 7736, DM BD+36  3955, TYC 2683-3962-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "b03 Cygni",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "42.69",
	"RA_S" : 303.63346892,
	"DEC_S" : 36.80630735,
	"Constellation" : "Cygnus ",
	"AMag" : 4.962,
	"key" : 33998,
	"title" : "b03 Cygni"
	},
{
	"Index" : "21653",
	"Description" : "Omicron2 Cygni (\u03BF2 Cyg, 2 Cyg) is the Bayer designation for a binary star system in the Cygnus constellation. It is a 4th magnitude star, which can be seen with the naked eye under suitably dark skies. Parallax measurements give an estimated distance of 1,100 light-years (320 parsecs) from the Earth. However, Schroder et al. (2007) suggest the actual value, after correcting for Malmquist bias, may be closer to 1,174 light-years (360 parsecs).\r\rThe primary component in this system, \u03BF2 Cygni A, has a stellar classification of K4\u20135 Ib, indicating that it is a lower luminosity supergiant star. Its effective temperature of 3,840 K lies in the range for K-type stars, giving it an orange hue. This star has more than times the mass of the Sun and the outer envelope has expanded to about 184 times the Sun\u0027s radius. It is radiating 6,600 times the luminosity of the Sun.\r\rThe companion star, \u03BF2 Cygni B, is smaller than the primary, with four times the Sun\u0027s mass and three times the Sun\u0027s radius. It has a much higher effective temperature of 16,200 K and is radiating over 300 times the Sun\u0027s luminosity. This star has the blue-white hue of a B-type star, with a stellar classification of B6\u20137 IV\u2013V. The luminosity class \u0027IV\u2013V\u0027 fits a star that has nearly exhausted the hydrogen at its core and begun to evolve off the main sequence to become a subgiant star.\r\rThe two stars form an eclipsing binary system similar to Algol. The orbital plane of the two stars is nearly aligned with the line of sight from the Earth, so that the giant star eclipses the secondary component once per orbit. During an eclipse, emission lines can be seen in the spectrum of this system. These originate in the stellar wind escaping from the giant star. In a volume around the B star, this wind becomes ionized, resulting in a circumstellar H II region. The giant star is losing mass at the rate of 1.3 \u00D7 10\u20138 times the mass of the Sun per year, or the equivalent of the Sun\u0027s mass every 77 million years.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "32 Cygni, HIP 99848, SAO 49385, HD 192910, GC 28160, HR 7751, DM BD+47  3059A, TYC 3576-2157-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Omicron2 Cygni",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "319.15",
	"RA_S" : 303.86799842,
	"DEC_S" : 47.71421473,
	"X" : 418,
	"Y" : 188,
	"Constellation" : "Cygnus ",
	"AMag" : 4.157,
	"key" : 41653,
	"title" : "Omicron2 Cygni"
	},
{
	"Index" : "17947",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 99968, SAO 49410, HD 193092, GC 28197, HR 7759, DM BD+39 4114, TYC 3155-2323-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 7759",
	"OType" : "Variable Star",
	"Distance" : "474.78",
	"RA_S" : 304.23036364,
	"DEC_S" : 40.36506871,
	"Constellation" : "Cygnus ",
	"AMag" : 5.438,
	"key" : 37947,
	"title" : "HR 7759"
	},
{
	"Index" : "17880",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "34 Cygni, P Cygni, HIP 100044, SAO 69773, HD 193237, GC 28218, HR 7763, DM BD+37  3871, TYC 3151-3442-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "P Cygni",
	"OType" : "Blue supergiant star",
	"RA_S" : 304.44666974,
	"DEC_S" : 38.03292997,
	"Constellation" : "Cygnus ",
	"AMag" : 4.837,
	"key" : 37880,
	"title" : "P Cygni"
	},
{
	"Index" : "13932",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "35 Cygni, HIP 100122, SAO 69806, HD 193370, GC 28242, HR 7770, DM BD+34  3967, TYC 2680-1628-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "35 Cygni",
	"OType" : "Spectroscopic binary",
	"Distance" : "531.34",
	"RA_S" : 304.66278838,
	"DEC_S" : 34.98277945,
	"Constellation" : "Cygnus ",
	"AMag" : 5.235,
	"key" : 33932,
	"title" : "35 Cygni"
	},
{
	"Index" : "13861",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "39 Cygni, HIP 100587, SAO 69950, HD 194317, GC 28378, HR 7806, DM BD+31  4062, TYC 2676-1688-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "39 Cygni",
	"OType" : "Spectroscopic binary",
	"Distance" : "76.61",
	"RA_S" : 305.96510065,
	"DEC_S" : 32.19018145,
	"Constellation" : "Cygnus ",
	"AMag" : 4.574,
	"key" : 33861,
	"title" : "39 Cygni"
	},
{
	"Index" : "14032",
	"Description" : "41 Cygni (41 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.99.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "41 Cygni, HIP 101076, SAO 70095, HD 195295, GC 28513, HR 7834, DM BD+29  4057, TYC 2685-1920-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "41 Cygni",
	"OType" : "Variable Star",
	"Distance" : "235.45",
	"RA_S" : 307.34889446,
	"DEC_S" : 30.368555,
	"X" : 394,
	"Y" : 415,
	"Constellation" : "Cygnus ",
	"AMag" : 4.044,
	"key" : 34032,
	"title" : "41 Cygni"
	},
{
	"Index" : "21713",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "45 Cygni, Omega01 Cygni, HIP 101138, SAO 49712, HD 195556, GC 28537, HR 7844, DM BD+48  3142, TYC 3581-2031-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Ruchba (see HD195774)",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "277.71",
	"RA_S" : 307.51475117,
	"DEC_S" : 48.95156859,
	"Constellation" : "Cygnus ",
	"AMag" : 4.92,
	"key" : 41713,
	"title" : "Ruchba (see HD195774)"
	},
{
	"Index" : "14129",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "47 Cygni, HIP 101474AB, SAO 70203, HD 196093, GC 28630, HR 7866, DM BD+34  4079A, TYC 2694-2168-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "47 Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "847.4576",
	"RA_S" : 308.47577649,
	"DEC_S" : 35.25085332,
	"Constellation" : "Cygnus ",
	"AMag" : 4.815,
	"key" : 34129,
	"title" : "47 Cygni"
	},
{
	"Index" : "21726",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "51 Cygni, HIP 102177, SAO 32809, HD 197511, GC 28865, HR 7929, DM BD+49  3353, TYC 3582-2132-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "51 Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "377.25",
	"RA_S" : 310.55262568,
	"DEC_S" : 50.3400275,
	"Constellation" : "Cygnus ",
	"AMag" : 5.383,
	"key" : 41726,
	"title" : "51 Cygni"
	},
{
	"Index" : "14063",
	"Description" : "52 Cygni is a binary star system in the Veil Nebula.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "52 Cygni, HIP 102453, SAO 70467, HD 197912, GC 28942, HR 7942, DM BD+30  4167, TYC 2687-2651-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "52 Cygni",
	"OType" : "Star",
	"Distance" : "61.64",
	"RA_S" : 311.41564175,
	"DEC_S" : 30.71971549,
	"X" : 348,
	"Y" : 410,
	"Constellation" : "Cygnus ",
	"AMag" : 4.334,
	"key" : 34063,
	"title" : "52 Cygni"
	},
{
	"Index" : "14146",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "T Cygni, HIP 102571, SAO 70499, HD 198134, GC 28981, HR 7956, DM BD+33  4028, TYC 2695-4138-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "T Cygni",
	"OType" : "Long Period Variable candidate",
	"Distance" : "136.25",
	"RA_S" : 311.79480577,
	"DEC_S" : 34.37413032,
	"Constellation" : "Cygnus ",
	"AMag" : 5.077,
	"key" : 34146,
	"title" : "T Cygni"
	},
{
	"Index" : "14196",
	"Description" : "Lambda Cygni (\u03BB Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 4.53.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "54 Cygni, Lambda Cygni, HIP 102589A, SAO 70505, HD 198183A, GC 28994, HR 7963, DM BD+35  4267, TYC 2699-3425-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Lambda Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "232.97",
	"RA_S" : 311.852196,
	"DEC_S" : 36.490739,
	"X" : 344,
	"Y" : 335,
	"Constellation" : "Cygnus ",
	"AMag" : 4.734,
	"key" : 34196,
	"title" : "Lambda Cygni"
	},
{
	"Index" : "14197",
	"Description" : "Lambda Cygni (\u03BB Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 4.53.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "54 Cygni, Lambda Cygni, HIP 102589B, SAO 70505, HD 198183B, GC 28994, HR 7963, DM BD+35  4267, TYC 2699-3425-2",
	"group" : { "key" : "Cygnus" },
	"Common" : "Lambda Cygni",
	"OType" : "Star",
	"Distance" : "232.97",
	"RA_S" : 311.852258,
	"DEC_S" : 36.490978,
	"X" : 344,
	"Y" : 335,
	"Constellation" : "Cygnus ",
	"AMag" : 6.263,
	"key" : 34197,
	"title" : "Lambda Cygni"
	},
{
	"Index" : "21646",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "55 Cygni, HIP 102724, SAO 50099, HD 198478, GC 29036, HR 7977, DM BD+45  3291, TYC 3575-6709-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "55 Cygni",
	"OType" : "Blue supergiant star",
	"Distance" : "701.87",
	"RA_S" : 312.23454368,
	"DEC_S" : 46.11413556,
	"Constellation" : "Cygnus ",
	"AMag" : 4.89,
	"key" : 41646,
	"title" : "55 Cygni"
	},
{
	"Index" : "18239",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "56 Cygni, HIP 102843, SAO 50121, HD 198639, GC 29066, HR 7984, DM BD+43  3739, TYC 3179-1248-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "56 Cygni",
	"OType" : "Star",
	"Distance" : "40.96",
	"RA_S" : 312.52054655,
	"DEC_S" : 44.05930639,
	"Constellation" : "Cygnus ",
	"AMag" : 5.074,
	"key" : 38239,
	"title" : "56 Cygni"
	},
{
	"Index" : "18243",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "57 Cygni, HIP 103089, SAO 50180, HD 199081, GC 29150, HR 8001, DM BD+43  3755, TYC 3179-1354-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "57 Cygni",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "160.79",
	"RA_S" : 313.31148109,
	"DEC_S" : 44.38726677,
	"Constellation" : "Cygnus ",
	"AMag" : 4.749,
	"key" : 38243,
	"title" : "57 Cygni"
	},
{
	"Index" : "18155",
	"Description" : "Nu Cygni (\u03BD Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.92.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "58 Cygni, Nu Cygni, HIP 103413AB, SAO 50274, HD 199629, GC 29251, HR 8028, DM BD+40  4364, TYC 3171-2186-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Nu Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "114.6",
	"RA_S" : 314.29342003,
	"DEC_S" : 41.16715777,
	"X" : 321,
	"Y" : 274,
	"Constellation" : "Cygnus ",
	"AMag" : 3.932,
	"key" : 38155,
	"title" : "Nu Cygni"
	},
{
	"Index" : "21691",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "59 Cygni, f01 Cygni, HIP 103632AE, SAO 50335, HD 200120, GC 29327, HR 8047, DM BD+46  3133, TYC 3579-4461-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "f01 Cygni",
	"OType" : "Be Star",
	"Distance" : "418.05",
	"RA_S" : 314.9564716,
	"DEC_S" : 47.52094498,
	"Constellation" : "Cygnus ",
	"AMag" : 4.735,
	"key" : 41691,
	"title" : "f01 Cygni"
	},
{
	"Index" : "21782",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "60 Cygni, HIP 103732A, SAO 50359, HD 200310, GC 29354, HR 8053, DM BD+45  3364, TYC 3588-12112-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "60 Cygni",
	"OType" : "Be Star",
	"Distance" : "451.11",
	"RA_S" : 315.29552563,
	"DEC_S" : 46.15577396,
	"Constellation" : "Cygnus ",
	"AMag" : 5.397,
	"key" : 41782,
	"title" : "60 Cygni"
	},
{
	"Index" : "18268",
	"Description" : "Xi Cygni (\u03BE Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.70.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "62 Cygni, Xi Cygni, HIP 104060, SAO 50424, HD 200905, GC 29459, HR 8079, DM BD+43  3800, TYC 3180-2696-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Xi Cygni",
	"OType" : "Peculiar Star",
	"Distance" : "257.87",
	"RA_S" : 316.23276236,
	"DEC_S" : 43.92785195,
	"X" : 305,
	"Y" : 236,
	"Constellation" : "Cygnus ",
	"AMag" : 3.88,
	"key" : 38268,
	"title" : "Xi Cygni"
	},
{
	"Index" : "21856",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "63 Cygni, f02 Cygni, HIP 104194, SAO 50456, HD 201251, GC 29519, HR 8089, DM BD+47  3292, TYC 3592-7443-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "f02 Cygni",
	"OType" : "Star",
	"Distance" : "314.46",
	"RA_S" : 316.65039033,
	"DEC_S" : 47.648404,
	"Constellation" : "Cygnus ",
	"AMag" : 4.703,
	"key" : 41856,
	"title" : "f02 Cygni"
	},
{
	"Index" : "18118",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "61 Cygni, HIP 104214, SAO 70919, HD 201091, GC 29509, HR 8085, DM BD+38  4343, TYC 3168-2800-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "61 Cygni",
	"OType" : "Variable of BY Dra type",
	"Distance" : "3.48",
	"RA_S" : 316.72480205,
	"DEC_S" : 38.74944038,
	"Constellation" : "Cygnus ",
	"AMag" : 5.349,
	"key" : 38118,
	"title" : "61 Cygni"
	},
{
	"Index" : "14220",
	"Description" : "Zeta Cygni (\u03B6 Cyg) is a binary star system in the northern constellation of Cygnus, the swan. It has an apparent visual magnitude of 3.26, making it one of the brighter members of the constellation. Based upon parallax measurements, the distance to this star is about 143 light-years (44 parsecs).\r\rThe primary component is a giant star with a stellar classification of G8 IIIp. Its most likely status is as a core-helium fusing giant star, although it could be in transition to gianthood with a tranquil helium core. This star has around three times the mass of the Sun and has expanded to about 15 times the Sun\u0027s radius. It is radiating 112 times the brightness of the Sun from its outer atmosphere at an effective temperature of 4,910 K. At this temperature, the star glows with the yellow hue of a G-type star.\r\rZeta Cygni has an overabundance of barium, as well as other heavy chemical elements in its atmosphere, making it a so-called \u0022mild\u0022 barium star. These elements were synthesized by the other member of the system as it passed through the asymptotic giant branch (AGB) stage of its evolution, then ejected in its stellar wind and accreted onto the current primary component. Prior to acquiring this additional mass, Zeta Cygni had about 2.5 times the mass of the Sun, while the more evolved AGB star had three solar masses.\r\rThe secondary component of this system is a white dwarf. The pair orbit each other every 6,489 days, or every 17.8 years, with an eccentricity of 0.22.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "64 Cygni, Zeta Cygni, HIP 104732, SAO 71070, HD 202109, GC 29661, HR 8115, DM BD+29  4348, TYC 2702-2764-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Zeta Cygni",
	"OType" : "Spectroscopic binary",
	"Distance" : "43.87",
	"RA_S" : 318.23408465,
	"DEC_S" : 30.22694106,
	"X" : 270,
	"Y" : 412,
	"Constellation" : "Cygnus ",
	"AMag" : 3.3,
	"key" : 34220,
	"title" : "Zeta Cygni"
	},
{
	"Index" : "18132",
	"Description" : "Tau Cygni (\u03C4 Cyg) is a binary star system in the constellation Cygnus, approximately 69 light years away from Earth. This visual binary system has a period of 49.6 years.\r\rThe main star, 4th magnitude GJ 822.1 A, is a yellowish white subgiant star of the spectral type F2IV. It therefore has a surface temperature of 6,000 to 7,500 kelvins and is larger, hotter, and several times as bright as our Sun. Its companion, 6th magnitude GJ 822.1 B, is a yellow main sequence star of the spectral type G0V. It is similar to our Sun in size, surface temperature, and luminosity.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "65 Cygni, Tau Cygni, HIP 104887AB, SAO 71121, HD 202444, GC 29723, HR 8130, DM BD+37  4240, TYC 3169-3876-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Tau Cygni",
	"OType" : "Star",
	"Distance" : "20.34",
	"RA_S" : 318.69775875,
	"DEC_S" : 38.04538156,
	"X" : 275,
	"Y" : 310,
	"Constellation" : "Cygnus ",
	"AMag" : 3.776,
	"key" : 38132,
	"title" : "Tau Cygni"
	},
{
	"Index" : "18183",
	"Description" : "Sigma Cygni (\u03C3 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 4.21.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "67 Cygni, Sigma Cygni, HIP 105102, SAO 71165, HD 202850, GC 29786, HR 8143, DM BD+38  4431, TYC 3173-3151-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Sigma Cygni",
	"OType" : "Star",
	"Distance" : "802.69",
	"RA_S" : 319.3539699,
	"DEC_S" : 39.39468006,
	"X" : 270,
	"Y" : 292,
	"Constellation" : "Cygnus ",
	"AMag" : 4.248,
	"key" : 38183,
	"title" : "Sigma Cygni"
	},
{
	"Index" : "14307",
	"Description" : "Upsilon Cygni (\u03C5 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 4.21.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "66 Cygni, Upsilon Cygni, HIP 105138, SAO 71173, HD 202904, GC 29802, HR 8146, DM BD+34  4371, TYC 2710-2647-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Upsilon Cygni",
	"OType" : "Be Star",
	"Distance" : "194.12",
	"RA_S" : 319.4794794,
	"DEC_S" : 34.89689692,
	"X" : 262,
	"Y" : 350,
	"Constellation" : "Cygnus ",
	"AMag" : 4.361,
	"key" : 34307,
	"title" : "Upsilon Cygni"
	},
{
	"Index" : "18280",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "68 Cygni, A Cygni, HIP 105186, SAO 50690, HD 203064, GC 29823, HR 8154, DM BD+43  3877, TYC 3181-836-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "A Cygni",
	"OType" : "Spectroscopic binary",
	"RA_S" : 319.61327752,
	"DEC_S" : 43.94594383,
	"Constellation" : "Cygnus ",
	"AMag" : 5.023,
	"key" : 38280,
	"title" : "A Cygni"
	},
{
	"Index" : "21941",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 105898, SAO 50867, HD 204411, GC 30040, HR 8216, DM BD+48 3390, TYC 3598-2172-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "HR 8216",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "125.96",
	"RA_S" : 321.71509773,
	"DEC_S" : 48.83516687,
	"Constellation" : "Cygnus ",
	"AMag" : 5.302,
	"key" : 41941,
	"title" : "HR 8216"
	},
{
	"Index" : "14373",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "70 Cygni, HIP 105942, SAO 71358, HD 204403, GC 30044, HR 8215, DM BD+36  4568, TYC 2716-2883-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "70 Cygni",
	"OType" : "Star",
	"Distance" : "395.62",
	"RA_S" : 321.83901785,
	"DEC_S" : 37.11679933,
	"Constellation" : "Cygnus ",
	"AMag" : 5.269,
	"key" : 34373,
	"title" : "70 Cygni"
	},
{
	"Index" : "21822",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "71 Cygni, g Cygni, HIP 106093, SAO 50934, HD 204771, GC 30108, HR 8228, DM BD+45  3558, TYC 3590-3349-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "g Cygni",
	"OType" : "Star",
	"Distance" : "66.42",
	"RA_S" : 322.36229177,
	"DEC_S" : 46.54058824,
	"Constellation" : "Cygnus ",
	"AMag" : 5.324,
	"key" : 41822,
	"title" : "g Cygni"
	},
{
	"Index" : "21832",
	"Description" : "Rho Cygni (\u03C1 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 3.98.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "73 Cygni, Rho Cygni, HIP 106481, SAO 51035, HD 205435, GC 30207, HR 8252, DM BD+44  3865, TYC 3591-3421-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Rho Cygni",
	"OType" : "Variable Star",
	"Distance" : "37.89",
	"RA_S" : 323.49521648,
	"DEC_S" : 45.59183521,
	"X" : 242,
	"Y" : 207,
	"Constellation" : "Cygnus ",
	"AMag" : 4.082,
	"key" : 41832,
	"title" : "Rho Cygni"
	},
{
	"Index" : "18296",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "72 Cygni, HIP 106551, SAO 71480, HD 205512, GC 30219, HR 8255, DM BD+37  4359, TYC 3183-3283-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "72 Cygni",
	"OType" : "High proper-motion Star",
	"Distance" : "70.9",
	"RA_S" : 323.69402909,
	"DEC_S" : 38.53405887,
	"Constellation" : "Cygnus ",
	"AMag" : 4.99,
	"key" : 38296,
	"title" : "72 Cygni"
	},
{
	"Index" : "18337",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "74 Cygni, HIP 106711, SAO 51101, HD 205835, GC 30263, HR 8266, DM BD+39  4612, TYC 3187-2159-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "74 Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "65.79",
	"RA_S" : 324.23739513,
	"DEC_S" : 40.41352152,
	"Constellation" : "Cygnus ",
	"AMag" : 5.06,
	"key" : 38337,
	"title" : "74 Cygni"
	},
{
	"Index" : "18433",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "75 Cygni, HIP 106999, SAO 51167, HD 206330, GC 30338, HR 8284, DM BD+42  4177, TYC 3196-2204-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "75 Cygni",
	"OType" : "Double or multiple star",
	"Distance" : "123.13",
	"RA_S" : 325.04629665,
	"DEC_S" : 43.27383202,
	"Constellation" : "Cygnus ",
	"AMag" : 5.28,
	"key" : 38433,
	"title" : "75 Cygni"
	},
{
	"Index" : "21995",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "80 Cygni, Pi01 Cygni, HIP 107136, SAO 33665, HD 206672, GC 30391, HR 8301, DM BD+50  3410, TYC 3603-3215-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Azelfafage",
	"OType" : "Spectroscopic binary",
	"Distance" : "525.13",
	"RA_S" : 325.52359559,
	"DEC_S" : 51.18961817,
	"Constellation" : "Cygnus ",
	"AMag" : 4.648,
	"key" : 41995,
	"title" : "Azelfafage"
	},
{
	"Index" : "10061",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "78 Cygni, Mu01 Cygni, HIP 107310A, SAO 89940, HD 206826, GC 30438, HR 8309, DM BD+28  4169A, TYC 2201-2078-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Mu01 Cygni",
	"OType" : "High proper-motion Star",
	"Distance" : "22.23",
	"RA_S" : 326.03572417,
	"DEC_S" : 28.74264837,
	"Constellation" : "Cygnus ",
	"AMag" : 4.745,
	"key" : 30061,
	"title" : "Mu01 Cygni"
	},
{
	"Index" : "22084",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "81 Cygni, Pi02 Cygni, HIP 107533AB, SAO 51293, HD 207330, GC 30512, HR 8335, DM BD+48  3504, TYC 3612-3062-1",
	"group" : { "key" : "Cygnus" },
	"Common" : "Pi02 Cygni",
	"OType" : "Spectroscopic binary",
	"Distance" : "333.66",
	"RA_S" : 326.69836799,
	"DEC_S" : 49.30956975,
	"Constellation" : "Cygnus ",
	"AMag" : 4.208,
	"key" : 42084,
	"title" : "Pi02 Cygni"
	},
{
	"Index" : "5179",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "67 Aquilae, Rho Aquilae, HIP 99742, SAO 105878, HD 192425, GC 28097, HR 7724, DM BD+14  4227, TYC 1618-2331-1",
	"group" : { "backgroundImage" : "images/Alignment/04.png",
		"description" : "Delphinus (pron.: /d\u025Bl\u02C8fa\u026An\u0259s/) is a constellation in the northern sky, close to the celestial equator. Its name is Latin for dolphin. Delphinus was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains among the 88 modern constellations recognized by the International Astronomical Union. It is one of the smaller constellations, ranked 69th in size.\r\rDelphinus\u0027 brightest stars form a distinctive asterism that can easily be recognized. It is bordered (clockwise from north) by Vulpecula the fox, Sagitta the arrow, Aquila the eagle, Aquarius the water-carrier, Equuleus the foal and Pegasus the flying horse.\r\rDelphinus is associated with two stories from Greek mythology.\r\rAccording to the first one, the Greek god Poseidon wanted to marry Amphitrite, a beautiful nereid. She, however, wanting to protect her virginity, fled to the Atlas mountains. Her suitor then sent out several searchers, among them a certain Delphinus. Delphinus accidentally stumbled upon her and was able to persuade Amphitrite to accept Poseidon\u0027s wooing. Out of gratitude the god placed the image of a dolphin among the stars.\r\rThe second story tells of the Greek poet Arion of Lesbos (7th century BC), who was saved by a dolphin. He was a court musician at the palace of Periander, ruler of Corinth. Arion had amassed a fortune during his travels to Sicily and Italy. On his way home from Tarentum his wealth caused the crew of his ship to conspire against him. Threatened with death, Arion asked to be granted a last wish which the crew granted: he wanted to sing a dirge. This he did, and while doing so, flung himself into the sea. There, he was rescued by a dolphin which had been charmed by Arion\u0027s music. The dolphin carried Arion to the coast of Greece and left.",
		"key" : "Delphinus",
		"grouptype" : "Delphinus",
		"Meaning" : "dolphin",
		"Family" : "Heavenly Waters",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Delphinus",
		"title" : "Delphinus Objects Group" },
	"Common" : "Rho Aquilae",
	"OType" : "High proper-motion Star",
	"Distance" : "45.97",
	"RA_S" : 303.56924523,
	"DEC_S" : 15.19760993,
	"Constellation" : "Delphinus ",
	"AMag" : 4.954,
	"key" : 25179,
	"title" : "Rho Aquilae"
	},
{
	"Index" : "845",
	"Description" : "Epsilon Delphini (\u03B5 Del, \u03B5 Delphini) is a blue-white giant star approximately 358 light-years away in the constellation Delphinus. It has the traditional name Deneb Dulfim (occasianally Deneb or Al Dhanab al Dulfim), from the Arabic \u0630\u0646\u0628 \u0627\u0644\u062F\u0644\u0641\u064A\u0646 \u00F0anab ad-dulf\u012Bn \u0022tail of the dolphin.\r\rThe term \u00F0anab ad-dulf\u012Bn or Dzaneb al Delphin was appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, which was translated into Latin as Cauda Delphini, meaning the dolphin\u0027s tail.\r\rIn Chinese, \u6557\u74DC (B\u00E0i Gu\u0101), meaning Rotten Gourd, refers to an asterism consisting of \u03B5 Delphini, \u03B7 Delphini, \u03B8 Delphini, \u03B9 Delphini and \u03BA Delphini. Consequently, \u03B5 Delphini itself is known as \u6557\u74DC\u4E00 (B\u00E0i Gu\u0101 y\u012B, English: the First Star of Rotten Gourd.). From this Chinese name, the name Pae Chaou was appeared\r\rThe star is slightly variable, occasionally brightening to magnitude 3.95.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "2 Delphini, Epsilon Delphini, HIP 101421, SAO 106230, HD 195810, GC 28593, HR 7852, DM BD+10  4321, TYC 1096-1684-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Deneb Dulfim",
	"OType" : "Variable Star",
	"Distance" : "101.26",
	"RA_S" : 308.30321633,
	"DEC_S" : 11.30326144,
	"X" : 238,
	"Y" : 221,
	"Constellation" : "Delphinus ",
	"AMag" : 4.002,
	"key" : 20845,
	"shortTitle" : "Deneb el Delphinus; Deneb ehl' Del'fini",
	"title" : "Deneb Dulfim"
	},
{
	"Index" : "843",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "3 Delphini, Eta Delphini, HIP 101483, SAO 106248, HD 195943, GC 28617, HR 7858, DM BD+12  4378, TYC 1096-1682-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Eta Delphini",
	"OType" : "Variable Star",
	"Distance" : "71.79",
	"RA_S" : 308.48766729,
	"DEC_S" : 13.02727179,
	"Constellation" : "Delphinus ",
	"AMag" : 5.39,
	"key" : 20843,
	"title" : "Eta Delphini"
	},
{
	"Index" : "886",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "4 Delphini, Zeta Delphini, HIP 101589, SAO 106274, HD 196180, GC 28659, HR 7871, DM BD+14  4353, TYC 1100-1719-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Zeta Delphini",
	"OType" : "Star",
	"Distance" : "67.46",
	"RA_S" : 308.82723526,
	"DEC_S" : 14.67421103,
	"Constellation" : "Delphinus ",
	"AMag" : 4.66,
	"key" : 20886,
	"title" : "Zeta Delphini"
	},
{
	"Index" : "887",
	"Description" : "Beta Delphini (Beta Del, \u03B2 Delphini, \u03B2 Del) is a binary star in the constellation of Delphinus. As a practical joke, the astronomer Niccol\u00F2 Cacciatore gave it the name Rotanev, which is a reversal of his Latinized family name, Venator. The name first appeared in Giuseppe Piazzi\u0027s Palermo Catalogue, published in 1814. Beta Delphini was found to be a binary star system in 1873 by the American astronomer S. W. Burnham.\r\rIn Chinese, \u74E0\u74DC (H\u00F9 Gu\u0101), meaning Good Gourd, refers to an asterism consisting of \u03B2 Delphini, \u03B1 Delphini, \u03B32 Delphini, \u03B4 Delphini, and \u03B6 Delphini. Consequently, \u03B2 Delphini itself is known as \u74E0\u74DC\u56DB (H\u00F9 Gu\u0101 y\u012B, English: the Second Star of Good Gourd.).\r\rThis system consists of a pair of F-type stars stars that orbit each other with a period of 26.66 years and an eccentricity of 0.36. The plane of the orbit is inclined by an angle of 61\u00B0 to the line of sight from the Earth. The two stars have an angular separation of about 0.44 arcseconds, making them a challenge to resolve with a telescope. The larger member of the pair is a giant star with 1.75 times the mass and 24 times the luminosity of the Sun, while the secondary component is a subgiant star that has 1.47 times the Sun\u0027s mass and around 8 times the Sun\u0027s luminosity. The system is around 1.8 billion years old.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "6 Delphini, Beta Delphini, HIP 101769AB, SAO 106316, HD 196524, GC 28709, HR 7882, DM BD+14  4369, TYC 1100-1720-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Rotanev",
	"OType" : "Spectroscopic binary",
	"Distance" : "30.92",
	"RA_S" : 309.38723308,
	"DEC_S" : 14.59511021,
	"X" : 225,
	"Y" : 177,
	"Constellation" : "Delphinus ",
	"AMag" : 3.677,
	"key" : 20887,
	"shortTitle" : "Rotanen; Venator",
	"title" : "Rotanev"
	},
{
	"Index" : "844",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "5 Delphini, Iota Delphini, HIP 101800, SAO 106322, HD 196544, GC 28711, HR 7883, DM BD+10  4339, TYC 1096-1683-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Iota Delphini",
	"OType" : "Spectroscopic binary",
	"Distance" : "57.91",
	"RA_S" : 309.45466091,
	"DEC_S" : 11.37767251,
	"Constellation" : "Delphinus ",
	"AMag" : 5.424,
	"key" : 20844,
	"title" : "Iota Delphini"
	},
{
	"Index" : "812",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "7 Delphini, Kappa Delphini, HIP 101916, SAO 126059, HD 196755, GC 28756, HR 7896, DM BD+09  4600, TYC 1092-1776-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Kappa Delphini",
	"OType" : "High proper-motion Star",
	"Distance" : "30.12",
	"RA_S" : 309.78243022,
	"DEC_S" : 10.08620498,
	"Constellation" : "Delphinus ",
	"AMag" : 5.149,
	"key" : 20812,
	"title" : "Kappa Delphini"
	},
{
	"Index" : "5374",
	"Description" : "Alpha Delphini (\u03B1 Del, \u03B1 Delphini) is a multiple star in the constellation Delphinus. It also has the name Sualocin, which was given to it as a practical joke by the astronomer Niccol\u00F2 Cacciatore; the name is the Latinized version (Nicolaus) of his given name, spelled backwards.\r\rIn Chinese, \u74E0\u74DC (H\u00F9 Gu\u0101), meaning Good Gourd, refers to an asterism consisting of \u03B1 Delphini, \u03B32 Delphini, \u03B4 Delphini, \u03B2 Delphini and \u03B6 Delphini. Consequently, \u03B1 Delphini itself is known as \u74E0\u74DC\u4E00 (H\u00F9 Gu\u0101 y\u012B, English: the First Star of Good Gourd.).",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "9 Delphini, Alpha Delphini, HIP 101958AG, SAO 106357, HD 196867, GC 28780, HR 7906, DM BD+15  4222, TYC 1633-2442-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Sualocin",
	"OType" : "Double or multiple star",
	"Distance" : "77.71",
	"RA_S" : 309.90953,
	"DEC_S" : 15.91207326,
	"X" : 220,
	"Y" : 160,
	"Constellation" : "Delphinus ",
	"AMag" : 3.753,
	"key" : 25374,
	"shortTitle" : "Sualocin; Scalovin; Nicolaus; Sualotsin",
	"title" : "Sualocin"
	},
{
	"Index" : "5385",
	"Description" : "Delta Delphini is a giant star in the constellation Delphinus.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "11 Delphini, Delta Delphini, HIP 102281, SAO 106425, HD 197461, GC 28873, HR 7928, DM BD+14  4403, TYC 1634-3055-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Delta Delphini",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "68.43",
	"RA_S" : 310.86472592,
	"DEC_S" : 15.07457822,
	"X" : 208,
	"Y" : 170,
	"Constellation" : "Delphinus ",
	"AMag" : 4.453,
	"key" : 25385,
	"title" : "Delta Delphini"
	},
{
	"Index" : "5387",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "12 Delphini, Gamma01 Delphini, HIP 102531B, SAO 106475, HD 197963, GC 28965, HR 7947, DM BD+15  4255B, TYC 1634-3057-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Gamma01 Delphini",
	"OType" : "Star",
	"Distance" : "37.87",
	"RA_S" : 311.66195431,
	"DEC_S" : 16.12412538,
	"Constellation" : "Delphinus ",
	"AMag" : 5.028,
	"key" : 25387,
	"title" : "Gamma01 Delphini"
	},
{
	"Index" : "5386",
	"Description" : "Gamma Delphini (\u03B3 Del, \u03B3 Delphini) is a binary star system approximately 101 light-years away in the constellation of Delphinus. The star marks one corner of the asterism \u0022Job\u0027s Coffin\u0022. It is one of the best known double stars in the sky, with the primary star being a yellow-white dwarf star, while the secondary star is an orange subgiant star.\r\rThe primary star (catalogued as Gamma1 Delphini) is a yellow-white dwarf star of spectral type \u0022F7V\u0022 and an apparent magnitude of 5.14. The star is thought to have about 7 times more luminosity than the Sun. The secondary star (Gamma2 Delphini) is an orange subgiant star of spectral type \u0022K1IV\u0022 and an apparent magnitude of 4.27. This star is thought to have about 20.6 times more luminosity than the Sun. Nevertheless the cooler component (Gamma2) is more massive than Gamma1 and according to the hierarchy of masses and brightness, Gamma2 should be the primary star of the system.\r\rBack in 1999 the presence of a planetary companion was inferred around Gamma2 Delphini, an evolved orange subgiant star. Such a planet would yield a minimum mass of 0.7 Jupiter masses, orbital period of 1.44 years and separation of nearly 1.5 astronomical units (almost the orbital separation of Mars from the Sun).\r\rSo far the planetary candidate has not been confirmed. McDonald Observatory researches have set mass limits for potential planetary companions in orbit around the star Gamma2 Delphini.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "12 Delphini, Gamma02 Delphini, HIP 102532A, SAO 106476, HD 197964, GC 28966, HR 7948, DM BD+15  4255A, TYC 1634-3056-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "Gamma Delphini",
	"OType" : "Star",
	"Distance" : "31.06",
	"RA_S" : 311.66458324,
	"DEC_S" : 16.12429081,
	"X" : 198,
	"Y" : 156,
	"Constellation" : "Delphinus ",
	"AMag" : 4.356,
	"key" : 25386,
	"title" : "Gamma Delphini"
	},
{
	"Index" : "905",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "17 Delphini, HIP 103294, SAO 106665, HD 199253, GC 29201, HR 8011, DM BD+13  4572, TYC 1102-2546-1",
	"group" : { "key" : "Delphinus" },
	"Common" : "17 Delphini",
	"OType" : "Variable Star",
	"Distance" : "146.8",
	"RA_S" : 313.90287358,
	"DEC_S" : 13.72153343,
	"Constellation" : "Delphinus ",
	"AMag" : 5.306,
	"key" : 20905,
	"title" : "17 Delphini"
	},
{
	"Index" : "57786",
	"Description" : "Gamma Doradus (Gamma Dor, \u03B3 Doradus, \u03B3 Dor) is the third brightest star in the constellation of Dorado. It has an apparent visual magnitude of approximately 4.25 and is a variable star, the type star of the class of Gamma Doradus variables. These stars, like \u03B3 Doradus, are pulsating variables which vary in brightness by less than a tenth of a magnitude owing to nonradial gravity wave oscillations. The magnitude of \u03B3 Doradus itself has been observed to have two sinusoidal variations with periods of approximately 17.6 and 18.2 hours. There is also some additional unexplained, apparently random fluctuation.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Gamma Doradus, HIP 19893, SAO 233457, HD 27290, GC 5179, HR 1338, DM CD-51  1066, TYC 8075-1796-1",
	"group" : { "backgroundImage" : "images/Alignment/23.png",
		"description" : "Dorado (pron.: /d\u0252\u02C8re\u026Ado\u028A/) is a constellation in the southern sky. It was named in the late 16th century and is now one of the 88 modern constellations. Its name refers to the dolphinfish (Coryphaena hippurus), which is known as dorado in Spanish, although it has also been depicted as a swordfish. Dorado is notable for containing most of the Large Magellanic Cloud, the remainder being in the constellation Mensa. The South ecliptic pole also lies within this constellation.\r\rEven though the name Dorado is not Latin but Spanish, astronomers give it the Latin genitive form Doradus when naming its stars; they are treating it (like the adjacent constellation Argo Navis) as if it were a feminine proper name of Greek origin ending in -\u014D (like Io or Callisto or Argo), names that have a genitive ending in -\u016Bs.\r\rDorado was one of twelve constellations named by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman, and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. Its first depiction in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603 where it was also named Dorado. Dorado has been represented historically as a dolphinfish and a swordfish; the latter depiction is inaccurate. It has also been represented as a goldfish. The constellation was also known in the 17th and 18th century as Xiphias, the swordfish, first attested in Johannes Kepler\u0027s edition of Tycho Brahe\u0027s star list in the Rudolphine Tables of 1627. The name Dorado ultimately become dominant and was adopted by the IAU.",
		"key" : "Dorado",
		"grouptype" : "Dorado",
		"Meaning" : "goldfish",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Dorado",
		"title" : "Dorado Objects Group" },
	"Common" : "Gamma Doradus",
	"OType" : "Variable Star of gamma Dor type",
	"Distance" : "20.46",
	"RA_S" : 64.00661109,
	"DEC_S" : -51.48664753,
	"X" : 399,
	"Y" : 272,
	"Constellation" : "Dorado ",
	"AMag" : 4.285,
	"key" : 77786,
	"title" : "Gamma Doradus"
	},
{
	"Index" : "61906",
	"Description" : "Alpha Doradus (Alpha Dor, \u03B1 Doradus, \u03B1 Dor) is the brightest star in the southern constellation of Dorado. The distance to this system, as measured using the parallax method, is about 169 light-years (52 parsecs).\r\rThis is a binary star system with an overall apparent visual magnitude that varies between 3.26 and 3.30, making this one of the brightest binary stars. The system consists of a subgiant star of spectral type B revolving around a giant star with spectral type A in an eccentric orbit with a period of about 12 years. The orbital separation varies from 2 astronomical units at periastron to 17.5 astronomical units at apastron. The primary, \u03B1 Doradus A, is a chemically peculiar star whose atmosphere displays an abnormally high abundance of silicon, making this an Si star.\r\rAlpha Doradus has an optical companion, CCDM J04340-5503C, located 77 arcseconds away along a position angle of 94\u00B0. It has no physical relation to the other two stars.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Alpha Doradus, HIP 21281AB, SAO 233564, HD 29305, GC 5600, HR 1465, DM CP-55   663, TYC 8512-2115-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Alpha Doradus",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "51.69",
	"RA_S" : 68.49907161,
	"DEC_S" : -55.04497896,
	"X" : 358,
	"Y" : 313,
	"Constellation" : "Dorado ",
	"AMag" : 3.243,
	"key" : 81906,
	"title" : "Alpha Doradus"
	},
{
	"Index" : "61938",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Kappa Doradus, HIP 22040, SAO 233664, HD 30478, GC 5810, HR 1530, DM CP-59   376, TYC 8515-1847-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Kappa Doradus",
	"OType" : "Star",
	"Distance" : "67.01",
	"RA_S" : 71.0881432,
	"DEC_S" : -59.73273338,
	"Constellation" : "Dorado ",
	"AMag" : 5.307,
	"key" : 81938,
	"title" : "Kappa Doradus"
	},
{
	"Index" : "61928",
	"Description" : "Zeta Doradus (\u03B6 Dor) is a young star system that lies approximately 38 light-years away. The system consists of two widely separated stars, with the primary being bright enough to be observed with the naked eye but the secondary being much a much fainter star that requires telescopic equipment to be observed. Zeta Doradus A is a bright, high proper motion star with a spectral type of F7V, meaning that it is a main sequence star that is hotter and brighter than the Sun. With an apparent magnitude of 4.82, it is approximately the eight brightest star in the constellation of Dorado.\r\rThough it has been known that Zeta Doradus B is a nearby star since at least the Gliese Catalogue of Nearby Stars, the connection that it is a common proper motion companion to Zeta Doradus A was only made much more recently thanks to HIPPARCOS data. The two stars form a wide binary, with a physical separation between the components of about 0.018 parsecs (0.06 light-years) which is approximately 12400 AU. This is comparable to the 15000 AU separation between Alpha Centauri AB and Proxima Centauri.\r\rBoth components of the system show considerable activity: The log R\u0027HK of the stars are -4.373 and -4.575, respectively, whereas a star is \u0022quiet\u0022 when it has a Log R\u0027HK of <-4.8. This indicates that the system is young; indeed, the estimated age for Zeta Doradus A is only 0.58 Gigayears, about an eighth of the solar age.\r\rIt is not unusual for a young star to possess a debris disk; Zeta Doradus A is no exception, as it has been found to have an infra-red excess indicative of a disk of small bodies like comets re-emitting absorbed light at a redder wavelength. For Zeta Doradus A, the dust disk has a luminosity of 6.0 x 10-6 times the solar luminosity and a temperature of 91 \u00B1 12 Kelvin, indicating that it lies at a separation of several AU.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Zeta Doradus, HIP 23693, SAO 233822, HD 33262, GC 6258, HR 1674, DM CP-57   735, TYC 8514-2291-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Zeta Doradus",
	"OType" : "High proper-motion Star",
	"Distance" : "11.65",
	"RA_S" : 76.37773168,
	"DEC_S" : -57.4727021,
	"X" : 300,
	"Y" : 342,
	"Constellation" : "Dorado ",
	"AMag" : 4.767,
	"key" : 81928,
	"title" : "Zeta Doradus"
	},
{
	"Index" : "65660",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 23840, SAO 249198, HD 33684, GC 6314, HR 1695, DM CP-63  420, TYC 8881-1505-1",
	"group" : { "key" : "Dorado" },
	"Common" : "V* WZ Dor",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "173.11",
	"RA_S" : 76.89177287,
	"DEC_S" : -63.39967955,
	"Constellation" : "Dorado ",
	"AMag" : 5.395,
	"key" : 85660,
	"title" : "V* WZ Dor"
	},
{
	"Index" : "65708",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Theta Doradus, HIP 24372, SAO 249225, HD 34649, GC 6444, HR 1744, DM CP-67   401, TYC 8890-1116-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Theta Doradus",
	"OType" : "Star",
	"Distance" : "150.51",
	"RA_S" : 78.43939333,
	"DEC_S" : -67.18525422,
	"Constellation" : "Dorado ",
	"AMag" : 4.948,
	"key" : 85708,
	"title" : "Theta Doradus"
	},
{
	"Index" : "62049",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Lambda Doradus, HIP 25429, SAO 233981, HD 36189, GC 6749, HR 1836, DM CP-59   472, TYC 8530-1337-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Lambda Doradus",
	"OType" : "Star",
	"Distance" : "140.34",
	"RA_S" : 81.58027649,
	"DEC_S" : -58.91251862,
	"Constellation" : "Dorado ",
	"AMag" : 5.237,
	"key" : 82049,
	"title" : "Lambda Doradus"
	},
{
	"Index" : "65698",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "28 Doradus, HIP 26001, SAO 249309, HD 37297, GC 6927, HR 1917, DM CP-64   456, TYC 8887-1168-1",
	"group" : { "key" : "Dorado" },
	"Common" : "28 Doradus",
	"OType" : "Spectroscopic binary",
	"Distance" : "70.99",
	"RA_S" : 83.24823249,
	"DEC_S" : -64.22752846,
	"Constellation" : "Dorado ",
	"AMag" : 5.455,
	"key" : 85698,
	"title" : "28 Doradus"
	},
{
	"Index" : "65680",
	"Description" : "Beta Doradus (Beta Dor, \u03B2 Doradus, \u03B2 Dor) is the second brightest star in the southern constellation of Dorado. It has an apparent visual magnitude of 3.63, making it visible to the naked eye from the southern hemisphere. Based upon parallax measurements with the Hubble Space Telescope, it is located at a distance of 1,040 light-years (320 parsecs) from Earth.\r\rBeta Doradus is a Cepheid variable that regularly changes magnitude from a low of 4.05 to a high of 3.45 over a period of 9.842 days. The light curve of this magnitude change follows a regular saw-tooth pattern. During each radial pulsation cycle, the radius of the star varies by \u00B13.9 times the Sun\u0027s radius around a mean of 67.8. Its spectral type and luminosity class are likewise variable, from F-type to G-type and from a supergiant to a bright giant.\r\rFar ultraviolet emissions have been detected from this star with the Far Ultraviolet Spectroscopic Explorer, while X-ray emissions were detected with the XMM-Newton space telescope. The X-ray luminosity is about 1 \u00D7 1029 ergs/sec and the emission varies with the pulsation period, suggesting a connection with the pulsation process. The peak X-ray emissions are in the 0.6\u20130.8 keV energy range, which occurs for plasmas with temperatures of 7\u201310 million K.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Beta Doradus, HIP 26069, SAO 249311, HD 37350, GC 6944, HR 1922, DM CP-62   487, TYC 8883-1641-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Beta Doradus",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "304.14",
	"RA_S" : 83.40633428,
	"DEC_S" : -62.48982734,
	"X" : 259,
	"Y" : 410,
	"Constellation" : "Dorado ",
	"AMag" : 3.911,
	"key" : 85680,
	"title" : "Beta Doradus"
	},
{
	"Index" : "65820",
	"Description" : "\u03B4 Doradus is a faint star in the Dorado constellation that has the distinction of being the Moon\u0027s south pole star. It is better aligned than Earth\u0027s Polaris (\u03B1 Ursae Minoris), but much fainter.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Delta Doradus, HIP 27100, SAO 249346, HD 39014, GC 7246, HR 2015, DM CP-65   496, TYC 8904-1522-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Delta Doradus",
	"OType" : "Star",
	"Distance" : "45.87",
	"RA_S" : 86.19323818,
	"DEC_S" : -65.73552235,
	"X" : 250,
	"Y" : 455,
	"Constellation" : "Dorado ",
	"AMag" : 4.353,
	"key" : 85820,
	"title" : "Delta Doradus"
	},
{
	"Index" : "65821",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Epsilon Doradus, HIP 27534, SAO 249368, HD 39844, GC 7384, HR 2064, DM CP-66   463, TYC 8904-1523-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Epsilon Doradus",
	"OType" : "Variable Star",
	"Distance" : "175.91",
	"RA_S" : 87.47300482,
	"DEC_S" : -66.90118487,
	"Constellation" : "Dorado ",
	"AMag" : 5.071,
	"key" : 85821,
	"title" : "Epsilon Doradus"
	},
{
	"Index" : "65761",
	"Description" : "HD 40409 is a star in the constellation Dorado. Its apparent magnitude is 4.66.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "36 Doradus, HIP 27890, SAO 249390, HD 40409, GC 7477, HR 2102, DM CP-63   498, TYC 8896-1535-1",
	"group" : { "key" : "Dorado" },
	"Common" : "HD 40409",
	"OType" : "High proper-motion Star",
	"Distance" : "26.24",
	"RA_S" : 88.52534214,
	"DEC_S" : -63.0896879,
	"X" : 231,
	"Y" : 423,
	"Constellation" : "Dorado ",
	"AMag" : 4.759,
	"key" : 85761,
	"title" : "HD 40409"
	},
{
	"Index" : "68624",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Nu Doradus, HIP 29134, SAO 249461, HD 43107, GC 7886, HR 2221, DM CP-68   474, TYC 9164-2122-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Nu Doradus",
	"OType" : "Star",
	"Distance" : "91.9",
	"RA_S" : 92.18442737,
	"DEC_S" : -68.84341216,
	"Constellation" : "Dorado ",
	"AMag" : 5.028,
	"key" : 88624,
	"title" : "Nu Doradus"
	},
{
	"Index" : "65787",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Eta02 Doradus, HIP 29353, SAO 249469, HD 43455, GC 7946, HR 2245, DM CP-65   561, TYC 8901-1098-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Eta02 Doradus",
	"OType" : "Variable Star",
	"Distance" : "195.98",
	"RA_S" : 92.81243016,
	"DEC_S" : -65.58941681,
	"Constellation" : "Dorado ",
	"AMag" : 5.207,
	"key" : 85787,
	"title" : "Eta02 Doradus"
	},
{
	"Index" : "68748",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Pi02 Doradus, HIP 30565, SAO 249550, HD 46116, GC 8390, HR 2377, DM CP-69   614, TYC 9181-404-1",
	"group" : { "key" : "Dorado" },
	"Common" : "Pi02 Doradus",
	"OType" : "High proper-motion Star",
	"Distance" : "82.76",
	"RA_S" : 96.36928458,
	"DEC_S" : -69.69030199,
	"Constellation" : "Dorado ",
	"AMag" : 5.478,
	"key" : 88748,
	"title" : "Pi02 Doradus"
	},
{
	"Index" : "30020",
	"Description" : "HD 81817 is a star in the constellation Draco. Its apparent magnitude is 4.27.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 47193, SAO 1551, HD 81817, GC 13174, HR 3751, DM BD+81  302, TYC 4547-2323-1",
	"group" : { "backgroundImage" : "images/Alignment/24.png",
		"description" : "Draco is a constellation in the far northern sky. Its name is Latin for dragon. Draco is circumpolar (that is, never setting) for many observers in the northern hemisphere. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations today. The north pole of the ecliptic is in Draco.\r\rDragons in Greek mythology that may have inspired the constellation\u0027s name include Ladon, the dragon who guarded the golden apples of the Hesperides. Hercules killed Ladon during his 12 labors; he was tasked with stealing the golden apples. the constellation of Hercules is depicted near Draco.\r\rIn Greco- Roman legend, Draco was a dragon killed by the goddess Minerva and tossed into the sky upon his defeat. The dragon was one of the Giant Titans, who battled the Olympic gods for ten years. As Minerva threw the dragon, it became twisted on itself and froze at the cold North Celestial Pole before it could right itself.\r\rSometimes, Draco is represented as the demon son of Gaia, Typhon.\r\rTraditional Arabic astronomy does not depict a dragon in modern-day Draco, which is called the Mother Camels. Instead, two hyenas, represented by Eta Draconis and Zeta Draconis are seen attacking a baby camel (a dim star near Beta Draconis), which is protected by four female camels, represented by Beta Draconis, Gamma Draconis, Nu Draconis, and Xi Draconis. The nomads who own the camels are camped nearby, represented by a cooking tripod composed of Upsilon, Tau, and Sigma Draconis.",
		"key" : "Draco",
		"grouptype" : "Draco",
		"Meaning" : "dragon",
		"Family" : "Ursa Major",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Draco",
		"title" : "Draco Objects Group" },
	"Common" : "HD 81817",
	"OType" : "Spectroscopic binary",
	"Distance" : "304.11",
	"RA_S" : 144.27204346,
	"DEC_S" : 81.32638272,
	"X" : 486,
	"Y" : 83,
	"Constellation" : "Draco ",
	"AMag" : 4.43,
	"key" : 50020,
	"title" : "HD 81817"
	},
{
	"Index" : "29979",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 51808, SAO 7164, HD 91190, GC 14507, HR 4126, DM BD+76  393, TYC 4542-2796-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 4126",
	"OType" : "Star",
	"Distance" : "75.74",
	"RA_S" : 158.77288411,
	"DEC_S" : 75.71295573,
	"Constellation" : "Draco ",
	"AMag" : 4.959,
	"key" : 49979,
	"title" : "HR 4126"
	},
{
	"Index" : "28794",
	"Description" : "Lambda Draconis (\u03BB Dra, \u03BB Draconis) is a star in the constellation Draco. It has the traditional names Gianfar, Giansar, Juza, Giausar or Giauzar.\r\rIn Chinese, \u7D2B\u5FAE\u53F3\u57A3 (Z\u01D0 W\u0113i Y\u00F2u Yu\u00E1n), meaning Right Wall of Purple Forbidden Enclosure, refers to an asterism consisting of \u03BB Draconis, \u03B1 Draconis, \u03BA Draconis, 24 Ursae Majoris, 43 Camelopardalis, \u03B1 Camelopardalis and BK Camelopardalis. Consequently, \u03BB Draconis itself is known as \u7D2B\u5FAE\u53F3\u57A3\u4E09 (Z\u01D0 W\u0113i Y\u00F2u Yu\u00E1n s\u0101n, English: the Third Star of Right Wall of Purple Forbidden Enclosure.), representing \u4E0A\u8F14 (Sh\u01CEngf\u01D4), meaning First Minister. \u4E0A\u8F14 (Sh\u01CEngf\u01D4) is westernized into Sang Poo or Shaou Poo by R.H. Allen.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "1 Draconis, Lambda Draconis, HIP 56211, SAO 15532, HD 100029, GC 15799, HR 4434, DM BD+70   665, TYC 4392-1805-1",
	"group" : { "key" : "Draco" },
	"Common" : "Lambda Draconis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "102.12",
	"RA_S" : 172.85091634,
	"DEC_S" : 69.33107562,
	"X" : 631,
	"Y" : 194,
	"Constellation" : "Draco ",
	"AMag" : 3.987,
	"key" : 48794,
	"shortTitle" : "Giausar; Giansar; Gaiusar; Giauzar; Juza",
	"title" : "Lambda Draconis"
	},
{
	"Index" : "28789",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "2 Draconis, HIP 56583, SAO 15567, HD 100696, GC 15893, HR 4461, DM BD+70   670, TYC 4392-141-1",
	"group" : { "key" : "Draco" },
	"Common" : "2 Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "72.81",
	"RA_S" : 174.01164175,
	"DEC_S" : 69.32295609,
	"Constellation" : "Draco ",
	"AMag" : 5.296,
	"key" : 48789,
	"title" : "2 Draconis"
	},
{
	"Index" : "26840",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "3 Draconis, HIP 57111, SAO 15606, HD 101673, GC 16072, HR 4504, DM BD+67   714, TYC 4159-1359-1",
	"group" : { "key" : "Draco" },
	"Common" : "3 Draconis",
	"OType" : "Star",
	"Distance" : "183.91",
	"RA_S" : 175.61817789,
	"DEC_S" : 66.7449041,
	"Constellation" : "Draco ",
	"AMag" : 5.452,
	"key" : 46840,
	"title" : "3 Draconis"
	},
{
	"Index" : "30053",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 60044, SAO 7540, HD 107193, GC 16797, HR 4687, DM BD+75  470, TYC 4550-2114-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 4687",
	"OType" : "Star",
	"Distance" : "97.81",
	"RA_S" : 184.70826575,
	"DEC_S" : 75.16055352,
	"Constellation" : "Draco ",
	"AMag" : 5.466,
	"key" : 50053,
	"title" : "HR 4687"
	},
{
	"Index" : "28819",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "4 Draconis, HIP 60998, SAO 15816, HD 108907, GC 17046, HR 4765, DM BD+70   700, TYC 4394-1871-1",
	"group" : { "key" : "Draco" },
	"Common" : "4 Draconis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "188.58",
	"RA_S" : 187.52776177,
	"DEC_S" : 69.20112924,
	"Constellation" : "Draco ",
	"AMag" : 5.203,
	"key" : 48819,
	"title" : "4 Draconis"
	},
{
	"Index" : "28818",
	"Description" : "Kappa Draconis (\u03BA Draconis, \u03BA Dra) is a blue giant star located in the northern circumpolar constellation of Draco. At an apparent magnitude of 3.88, it is barely visible to the naked eye when artificial lighting from cities is present. Nevertheless, it is a powerful star, approximately five time as massive as the Sun. It is about 490 light-years away, and is 1,400 times brighter than the Sun.\r\rKappa is thought[weasel words] to be just entering its red giant phase, having exhausted the supply of hydrogen in its core. Over the next several thousand years, the star will expand, becoming more powerful but with a much cooler surface temperature. Tens of thousands of years from now, Kappa Draconis will appear much brighter, probably shining with a reddish hue.\r\rThe star is currently located at declination 69\u00B0 47\u0027 18\u0022 North (RA 12h 33m 29.0s), but due to the effects of precession, Kappa Draconis was the nearest star to the North Celestial Pole visible to the naked eye from 1793 BC to approximately 1000 BC. However, because it is so much dimmer than nearby Kochab, Kochab was considered the pole star during that time instead.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "5 Draconis, Kappa Draconis, HIP 61281, SAO 7593, HD 109387, GC 17126, HR 4787, DM BD+70   703, TYC 4394-1870-1",
	"group" : { "key" : "Draco" },
	"Common" : "Kappa Draconis",
	"OType" : "Be Star",
	"Distance" : "149.91",
	"RA_S" : 188.37059686,
	"DEC_S" : 69.78823584,
	"X" : 592,
	"Y" : 254,
	"Constellation" : "Draco ",
	"AMag" : 3.849,
	"key" : 48818,
	"title" : "Kappa Draconis"
	},
{
	"Index" : "28839",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "6 Draconis, HIP 61384, SAO 7600, HD 109551, GC 17148, HR 4795, DM BD+70   705, TYC 4397-1799-1",
	"group" : { "key" : "Draco" },
	"Common" : "6 Draconis",
	"OType" : "Star",
	"Distance" : "182.33",
	"RA_S" : 188.68337656,
	"DEC_S" : 70.02177076,
	"Constellation" : "Draco ",
	"AMag" : 5.095,
	"key" : 48839,
	"title" : "6 Draconis"
	},
{
	"Index" : "26908",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "8 Draconis, HIP 63076, SAO 15941, HD 112429, GC 17554, HR 4916, DM BD+66   778, TYC 4168-930-1",
	"group" : { "key" : "Draco" },
	"Common" : "8 Draconis",
	"OType" : "Variable Star of gamma Dor type",
	"Distance" : "29.29",
	"RA_S" : 193.86894577,
	"DEC_S" : 65.43847425,
	"Constellation" : "Draco ",
	"AMag" : 5.262,
	"key" : 46908,
	"title" : "8 Draconis"
	},
{
	"Index" : "26951",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "10 Draconis, i Draconis, HIP 67627, SAO 16199, HD 121130, GC 18750, HR 5226, DM BD+65   963, TYC 4174-1261-1",
	"group" : { "key" : "Draco" },
	"Common" : "i Draconis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "113.82",
	"RA_S" : 207.85808367,
	"DEC_S" : 64.72327274,
	"Constellation" : "Draco ",
	"AMag" : 4.783,
	"key" : 46951,
	"title" : "i Draconis"
	},
{
	"Index" : "26952",
	"Description" : "Thuban also known by its Bayer designation Alpha Draconis (\u03B1 Draconis, \u03B1 Dra) is a star (or star system) in the constellation of Draco. A relatively inconspicuous star in the night sky of the Northern Hemisphere, it is historically significant as having been the north pole star in ancient times. Thuban is an Arabic word for snake \u062B\u0639\u0628\u0627\u0646 thu\u02BFb\u0101n.\r\rEven though Johann Bayer gave Thuban the designation Alpha, its apparent magnitude of 3.65 is 3.7 times fainter than the brightest star in the constellation, Gamma Draconis (Eltanin), whose apparent magnitude is 2.24.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "11 Draconis, Alpha Draconis, HIP 68756, SAO 16273, HD 123299, GC 19019, HR 5291, DM BD+65   978, TYC 4174-1262-1",
	"group" : { "key" : "Draco" },
	"Common" : "Thuban",
	"OType" : "Spectroscopic binary",
	"Distance" : "92.91",
	"RA_S" : 211.09729148,
	"DEC_S" : 64.37585053,
	"X" : 555,
	"Y" : 383,
	"Constellation" : "Draco ",
	"AMag" : 3.628,
	"key" : 46952,
	"shortTitle" : "Adib; Dragon's Tail; Tuban",
	"title" : "Thuban"
	},
{
	"Index" : "24412",
	"Description" : "Iota Draconis (\u03B9 Dra, \u03B9 Draconis) is a star in the northern circumpolar constellation of Draco. It has the traditional name Edasich, a name that comes from the Arabic Al \u1E0Chiba\u0027 of Ulug Beg and the Dresden Globe, or Al dh\u012Bl\u012B \u0027Male hyena\u0027 by Kazwini, with Eldsich being recorded in the Century Cyclopedia. A visually unremarkable star of apparent magnitude 3.3, in 2002 it was discovered to have a planet. From parallax measurements, this star is located at a distance of about 101.2 light-years (31.0 parsecs) from Earth.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "12 Draconis, Iota Draconis, HIP 75458, SAO 29520, HD 137759, GC 20747, HR 5744, DM BD+59  1654, TYC 3875-1620-1",
	"group" : { "key" : "Draco" },
	"Common" : "Edasich",
	"OType" : "Variable Star",
	"Distance" : "31.03",
	"RA_S" : 231.23239349,
	"DEC_S" : 58.96606176,
	"X" : 467,
	"Y" : 495,
	"Constellation" : "Draco ",
	"AMag" : 3.421,
	"key" : 44412,
	"shortTitle" : "Eldsich; Al Dhiba; Al Dhihi; Edasich",
	"title" : "Edasich"
	},
{
	"Index" : "27054",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 77277, SAO 16848, HD 141653, GC 21246, HR 5886, DM BD+63 1225, TYC 4185-1959-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 5886",
	"OType" : "Star",
	"Distance" : "87.69",
	"RA_S" : 236.6666899,
	"DEC_S" : 62.59955885,
	"Constellation" : "Draco ",
	"AMag" : 5.2,
	"key" : 47054,
	"title" : "HR 5886"
	},
{
	"Index" : "24376",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 78180, SAO 29727, HD 143466, GC 21467, HR 5960, DM BD+55 1793, TYC 3870-1962-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 5960",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "33.58",
	"RA_S" : 239.44767341,
	"DEC_S" : 54.74976585,
	"Constellation" : "Draco ",
	"AMag" : 4.987,
	"key" : 44376,
	"title" : "HR 5960"
	},
{
	"Index" : "24482",
	"Description" : "Theta Draconis (\u03B8 Dra / \u03B8 Draconis) is a fourth-magnitude star in the northern circumpolar constellation of Draco. Parallax measurements place it at an estimated distance of 68.6 light-years (21.0 parsecs) from Earth.\r\rThis star is 21% more massive than the Sun and has a radius 2.5 times the Sun\u0027s. It is radiating 8.7 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 6,290 K. This temperature is what gives it the yellow-white hue of an F-type main sequence star with a stellar classification of F9 V.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "13 Draconis, Theta Draconis, HIP 78527, SAO 29765, HD 144284, GC 21572, HR 5986, DM BD+58  1608, TYC 3883-1543-1",
	"group" : { "key" : "Draco" },
	"Common" : "Theta Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "21.03",
	"RA_S" : 240.47227953,
	"DEC_S" : 58.5652533,
	"X" : 405,
	"Y" : 510,
	"Constellation" : "Draco ",
	"AMag" : 4.055,
	"key" : 44482,
	"title" : "Theta Draconis"
	},
{
	"Index" : "29020",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 78893, SAO 16962, HD 145454, GC 21705, HR 6025, DM BD+68  864, TYC 4419-2888-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 6025",
	"OType" : "Star",
	"Distance" : "77.8",
	"RA_S" : 241.58198798,
	"DEC_S" : 67.81013528,
	"Constellation" : "Draco ",
	"AMag" : 5.435,
	"key" : 49020,
	"title" : "HR 6025"
	},
{
	"Index" : "29017",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 80161, SAO 17062, HD 148293, GC 22062, HR 6126, DM BD+69  845, TYC 4419-2885-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 6126",
	"OType" : "Star",
	"Distance" : "89.89",
	"RA_S" : 245.45296277,
	"DEC_S" : 69.10939609,
	"Constellation" : "Draco ",
	"AMag" : 5.388,
	"key" : 49017,
	"title" : "HR 6126"
	},
{
	"Index" : "27097",
	"Description" : "Eta Draconis (\u03B7 Dra, \u03B7 Draconis) is a star in the northern circumpolar constellation of Draco. Despite having an apparent visual magnitude of only +2.73, it is the second brightest star in this generally faint constellation. Based upon parallax measurements collected during the Hipparcos mission, this star is located at a distance of about 92.1 light-years (28.2 parsecs) from Earth.\r\rEta Draconis is a large star with 2.55 times the mass of the Sun. The spectrum matches a stellar classification of G8 III, with the luminosity class III indicating this is an evolved giant star that has exhausted the supply of hydrogen at its core. It reached this stage in only 550 million years because higher mass stars such as this consume the supply of hydrogen more rapidly than the Sun. The measured angular diameter of this star, after correction for limb darkening, is 3.72 \u00B1 0.07 mas. At the estimated distance of Eta Draconis, this yields a physical size of about 11 times the radius of the Sun. From its extended envelope, it is radiating around 60 times the luminosity of the Sun at an effective temperature of 5,055 K, giving it the yellow glow of a G-type star.\r\rA nearby stellar companion is located at an angular separation of 5.1 arcseconds from Eta Draconis. This is an 8.8 magnitude K-type main sequence star with a stellar classification of K2 V. At the estimated distance of this star system, the two stars are separated by a physical distance of at least 140 AU and require at least a millennium to complete an orbit.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "14 Draconis, Eta Draconis, HIP 80331, SAO 17074, HD 148387, GC 22101, HR 6132, DM BD+61  1591, TYC 4190-2568-1",
	"group" : { "key" : "Draco" },
	"Common" : "Eta Draconis",
	"OType" : "Variable Star",
	"Distance" : "28.23",
	"RA_S" : 245.99785807,
	"DEC_S" : 61.51421387,
	"X" : 368,
	"Y" : 472,
	"Constellation" : "Draco ",
	"AMag" : 2.801,
	"key" : 47097,
	"title" : "Eta Draconis"
	},
{
	"Index" : "29018",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "15 Draconis, A Draconis, HIP 80650, SAO 17107, HD 149212, GC 22194, HR 6161, DM BD+69   850, TYC 4419-2886-1",
	"group" : { "key" : "Draco" },
	"Common" : "A Draconis",
	"OType" : "Star",
	"Distance" : "149.15",
	"RA_S" : 246.99589369,
	"DEC_S" : 68.76813869,
	"Constellation" : "Draco ",
	"AMag" : 4.942,
	"key" : 49018,
	"title" : "A Draconis"
	},
{
	"Index" : "24446",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "16 Draconis, HIP 81290, SAO 30012, HD 150100, GC 22351, HR 6184, DM BD+53  1875, TYC 3879-2961-1",
	"group" : { "key" : "Draco" },
	"Common" : "16 Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "130.81",
	"RA_S" : 249.04758842,
	"DEC_S" : 52.9000481,
	"Constellation" : "Draco ",
	"AMag" : 5.498,
	"key" : 44446,
	"title" : "16 Draconis"
	},
{
	"Index" : "24445",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "17 Draconis, HIP 81292A, SAO 30013, HD 150117, GC 22352, HR 6185, DM BD+53  1876A, TYC 3879-2960-2",
	"group" : { "key" : "Draco" },
	"Common" : "17 Draconis",
	"OType" : "Star",
	"Distance" : "126.2",
	"RA_S" : 249.0571691,
	"DEC_S" : 52.92441435,
	"Constellation" : "Draco ",
	"AMag" : 5.376,
	"key" : 44445,
	"title" : "17 Draconis"
	},
{
	"Index" : "24474",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 81437, SAO 30026, HD 150449, GC 22398, HR 6199, DM BD+56 1907, TYC 3882-2598-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 6199",
	"OType" : "Star",
	"Distance" : "82.94",
	"RA_S" : 249.50192005,
	"DEC_S" : 56.01555196,
	"Constellation" : "Draco ",
	"AMag" : 5.397,
	"key" : 44474,
	"title" : "HR 6199"
	},
{
	"Index" : "27134",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "18 Draconis, g Draconis, HIP 81660, SAO 17188, HD 151101, GC 22489, HR 6223, DM BD+64  1145, TYC 4193-2534-1",
	"group" : { "key" : "Draco" },
	"Common" : "g Draconis",
	"OType" : "Star",
	"Distance" : "225.34",
	"RA_S" : 250.2296655,
	"DEC_S" : 64.58904572,
	"Constellation" : "Draco ",
	"AMag" : 4.977,
	"key" : 47134,
	"title" : "g Draconis"
	},
{
	"Index" : "24473",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 82020, SAO 30076, HD 151613, GC 22584, HR 6237, DM BD+57 1702, TYC 3882-2597-1",
	"group" : { "key" : "Draco" },
	"Common" : "Gliese 9578 (HR 6237)",
	"OType" : "Spectroscopic binary",
	"Distance" : "26.73",
	"RA_S" : 251.32419808,
	"DEC_S" : 56.78184947,
	"Constellation" : "Draco ",
	"AMag" : 4.881,
	"key" : 44473,
	"title" : "Gliese 9578 (HR 6237)"
	},
{
	"Index" : "27162",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "19 Draconis, h Draconis, HIP 82860, SAO 17281, HD 153597, GC 22871, HR 6315, DM BD+65  1157, TYC 4197-2429-1",
	"group" : { "key" : "Draco" },
	"Common" : "h Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "15.26",
	"RA_S" : 254.00704229,
	"DEC_S" : 65.13480035,
	"Constellation" : "Draco ",
	"AMag" : 4.937,
	"key" : 47162,
	"title" : "h Draconis"
	},
{
	"Index" : "27241",
	"Description" : "Zeta Draconis (\u03B6 Dra, \u03B6 Draconis) is the Bayer designation for a star in the northern circumpolar constellation of Draco. It shares the Arabic name Al dhi\u0027bah (\u0027the hyenas\u0027) with several other stars in the constellation, and shares the name Al dhibain with Eta Draconis. It is known as Nodus III (Third Knot, the knot being a loop in the tail of Draco). With an apparent visual magnitude of +3.17,  it is the fifth brightest member of this generally faint constellation. The distance to Zeta Draconis has been measured using the parallax technique, yielding an estimate of roughly 330 light-years (100 parsecs) away.\r\rIn Chinese, \u7D2B\u5FAE\u5DE6\u57A3 (Z\u01D0 W\u0113i Zu\u01D2 Yu\u00E1n), meaning Left Wall of Purple Forbidden Enclosure, refers to an asterism consisting of \u03B6 Draconis, \u03B9 Draconis, \u03B7 Draconis, \u03B8 Draconis, \u03C5 Draconis, 73 Draconis, \u03B3 Cephei and 23 Cassiopeiae. Consequently, \u03B6 Draconis itself is known as \u7D2B\u5FAE\u5DE6\u57A3\u56DB (Z\u01D0 W\u0113i Zu\u01D2 Yu\u00E1n s\u00EC, English: the Fourth Star of Left Wall of Purple Forbidden Enclosure.), representing \u4E0A\u5F3C (Sh\u01CEngb\u00EC), meaning The First Minister. \u4E0A\u5F3C (Sh\u01CEngb\u00EC) is westernized into Shang Pih by R.H. Allen with meaning \u0022the Higher Minister\u0022.\r\rZeta Draconis is a giant star with a stellar classification of B6 III. Compared to the Sun, this star is about 2.5 times larger, 3.5 times more massive, and is radiating 148 times as much luminosity. This energy is being emitted from the star\u0027s outer envelope at an effective temperature of nearly 13,400 K. The azimuthal rotation velocity along the equator is at least 55 km/s.\r\rThe north ecliptic pole is located at right ascension 18h and declination +66.5\u00B0. This is located roughly mid-way between Delta Draconis and Zeta Draconis.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "22 Draconis, Zeta Draconis, HIP 83895, SAO 17365, HD 155763, GC 23182, HR 6396, DM BD+65  1170, TYC 4210-1048-1",
	"group" : { "key" : "Draco" },
	"Common" : "Zeta Draconis",
	"OType" : "Star",
	"Distance" : "100.56",
	"RA_S" : 257.19664984,
	"DEC_S" : 65.71468427,
	"X" : 309,
	"Y" : 412,
	"Constellation" : "Draco ",
	"AMag" : 3.132,
	"key" : 47241,
	"shortTitle" : "Eldsib; Nodus I (also HD163588); Nod",
	"title" : "Zeta Draconis"
	},
{
	"Index" : "21129",
	"Description" : "Beta Draconis (\u03B2 Draconis, \u03B2 Dra) is the third brightest star in the northern circumpolar constellation of Draco. It has the traditional name Rastaban, which has also been used for Gamma Draconis. With an apparent visual magnitude of 2.79, it is bright enough to be easily seen with the naked eye. Based upon parallax measurements from the Hipparcos astrometry satellite, it lies at a distance of about 380 light-years (120 parsecs) from Earth.\r\rCompared to the Sun, this is an enormous star with six times the mass and roughly 40 times the radius. At this size, Beta Draconis is emitting about 950 times the luminosity of the Sun from its outer envelope at an effective temperature of 5,160 K, giving it the yellow hue of a G-type star. The spectrum matches a stellar classification of G2 Ib\u2013IIa, with the luminosity class notation Ib\u2013IIa indicating it lies part way between the bright giant and supergiant stages of its stellar evolution. It is about 67 million years old.\r\rThis is a binary star system, with a binary star designation of ADS 10611, in which the supergiant is orbited by a dwarf companion once every four millennia or so.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "23 Draconis, Beta Draconis, HIP 85670, SAO 30429, HD 159181, GC 23741, HR 6536, DM BD+52  2065, TYC 3521-1800-1",
	"group" : { "key" : "Draco" },
	"Common" : "Rastaban",
	"OType" : "Star",
	"Distance" : "116.53",
	"RA_S" : 262.60817373,
	"DEC_S" : 52.30138871,
	"X" : 235,
	"Y" : 574,
	"Constellation" : "Draco ",
	"AMag" : 2.874,
	"key" : 41129,
	"shortTitle" : "Alwaid; Asuia; Rastaben",
	"title" : "Rastaban"
	},
{
	"Index" : "29048",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "27 Draconis, f Draconis, HIP 85805, SAO 17526, HD 159966, GC 23821, HR 6566, DM BD+68   938, TYC 4421-2880-1",
	"group" : { "key" : "Draco" },
	"Common" : "f Draconis",
	"OType" : "Star",
	"Distance" : "64.67",
	"RA_S" : 262.99112096,
	"DEC_S" : 68.1350229,
	"Constellation" : "Draco ",
	"AMag" : 5.192,
	"key" : 49048,
	"title" : "f Draconis"
	},
{
	"Index" : "24543",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "24 Draconis, Nu01 Draconis, HIP 85819, SAO 30447, HD 159541, GC 23797, HR 6554, DM BD+55  1944, TYC 3892-1620-1",
	"group" : { "key" : "Draco" },
	"Common" : "Kuma",
	"OType" : "Star",
	"Distance" : "30.25",
	"RA_S" : 263.04403565,
	"DEC_S" : 55.18424274,
	"Constellation" : "Draco ",
	"AMag" : 4.899,
	"key" : 44543,
	"title" : "Kuma"
	},
{
	"Index" : "24544",
	"Description" : "Nu Draconis (also known as \u03BD Dra, \u03BD Draconis, or Kuma) is a double star in the constellation Draco. The respective components are designated \u03BD1 Draconis and \u03BD2 Draconis. The second component is a spectroscopic binary star system.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "25 Draconis, Nu02 Draconis, HIP 85829, SAO 30450, HD 159560, GC 23801, HR 6555, DM BD+55  1945, TYC 3892-1621-1",
	"group" : { "key" : "Draco" },
	"Common" : "Nu Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "30.49",
	"RA_S" : 263.06676933,
	"DEC_S" : 55.17295844,
	"X" : 241,
	"Y" : 537,
	"Constellation" : "Draco ",
	"AMag" : 4.87,
	"key" : 44544,
	"title" : "Nu Draconis"
	},
{
	"Index" : "27173",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "26 Draconis, HIP 86036A, SAO 17546, HD 160269A, GC 23874, HR 6573, DM BD+61  1678, TYC 4199-1513-1",
	"group" : { "key" : "Draco" },
	"Common" : "26 Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "14.19",
	"RA_S" : 263.7482476,
	"DEC_S" : 61.87456936,
	"Constellation" : "Draco ",
	"AMag" : 5.281,
	"key" : 47173,
	"title" : "26 Draconis"
	},
{
	"Index" : "29125",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "28 Draconis, Omega Draconis, HIP 86201, SAO 17576, HD 160922, GC 23944, HR 6596, DM BD+68   949, TYC 4428-1960-1",
	"group" : { "key" : "Draco" },
	"Common" : "Omega Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "23.16",
	"RA_S" : 264.2378931,
	"DEC_S" : 68.75796949,
	"Constellation" : "Draco ",
	"AMag" : 4.821,
	"key" : 49125,
	"title" : "Omega Draconis"
	},
{
	"Index" : "29172",
	"Description" : "Psi Draconis (\u03C8\u00B9 Dra, \u03C8\u00B9 Draconis) is a star in the constellation Draco. It also has the traditional name Dziban, from the Arabic Adh-Dhi\u0027ban, meaning \u0022The two wolves\u0022 or \u0022The two jackals\u0022. The primary component of the binary system is suspected to host a substellar companion.\r\rIn Chinese astronomy, Dziban is called \u5973\u53F2, Pinyin: N\u01DAsh\u01D0, meaning Female Protocol, because this star is marking itself and stand alone in Female Protocol asterism, Purple Forbidden enclosure (see : Chinese constellation). \u5973\u53F2 (N\u01DAsh\u01D0) westernized into Niu She by R.H. Allen, with the meaning is \u0022the Palace Governess\u0022, or \u0022a Literary Woman",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "31 Draconis, Psi Draconis, HIP 86614A, SAO 8890, HD 162003, GC 24089, HR 6636, DM BD+72   804, TYC 4436-1425-1",
	"group" : { "key" : "Draco" },
	"Common" : "Psi Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "22.83",
	"RA_S" : 265.48480656,
	"DEC_S" : 72.148847,
	"X" : 294,
	"Y" : 321,
	"Constellation" : "Draco ",
	"AMag" : 4.6,
	"key" : 49172,
	"shortTitle" : "Dsiban",
	"title" : "Psi Draconis"
	},
{
	"Index" : "21146",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "30 Draconis, HIP 87212, SAO 30591, HD 162579, GC 24221, HR 6656, DM BD+50  2468, TYC 3523-1685-1",
	"group" : { "key" : "Draco" },
	"Common" : "30 Draconis",
	"OType" : "Double or multiple star",
	"Distance" : "66.47",
	"RA_S" : 267.26786456,
	"DEC_S" : 50.78105385,
	"Constellation" : "Draco ",
	"AMag" : 5.022,
	"key" : 41146,
	"title" : "30 Draconis"
	},
{
	"Index" : "30250",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "35 Draconis, HIP 87234, SAO 8939, HD 163989, GC 24343, HR 6701, DM BD+76   667, TYC 4573-1916-1",
	"group" : { "key" : "Draco" },
	"Common" : "35 Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "31.76",
	"RA_S" : 267.36263476,
	"DEC_S" : 76.9628803,
	"Constellation" : "Draco ",
	"AMag" : 5.075,
	"key" : 50250,
	"title" : "35 Draconis"
	},
{
	"Index" : "24623",
	"Description" : "Xi Draconis (\u03BE Dra, \u03BE Draconis) is the Bayer designation for a star in the northern circumpolar constellation of Draco. It has the traditional name Grumium or Genam. This star, along with \u03B2 Dra (Rastaban), \u03B3 Dra (Eltanin), \u03BC Dra (Erakis) and \u03BD Dra (Kuma) were Al \u02BDAw\u0101\u00EFd, \u0022the Mother Camels\u0022, which was later known as the Quinque Dromedarii. This star has an apparent visual magnitude of 3.75. Based upon parallax measurements, it is located at a distance of 112.5 light-years (34.5 parsecs) from Earth. At this distance, the apparent magnitude is diminished by 0.03 from extinction caused by intervening gas and dust.\r\rIn Chinese, \u5929\u68D3 (Ti\u0101n B\u00E0ng), meaning Celestial Flail, refers to an asterism consisting of \u03BE Draconis, \u03BD Draconis, \u03B2 Draconis, \u03B3 Draconis and \u03B9 Herculis. Consequently, \u03B4 Draconis itself is known as \u5929\u68D3\u4E00 (Ti\u0101n B\u00E0ng y\u012B, English: the First Star of Celestial Flail.)",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "32 Draconis, Xi Draconis, HIP 87585, SAO 30631, HD 163588, GC 24364, HR 6688, DM BD+56  2033, TYC 3910-1710-1",
	"group" : { "key" : "Draco" },
	"Common" : "Xi Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "34.51",
	"RA_S" : 268.38220999,
	"DEC_S" : 56.8726474,
	"X" : 211,
	"Y" : 503,
	"Constellation" : "Draco ",
	"AMag" : 3.853,
	"key" : 44623,
	"shortTitle" : "Genam; Nodus I (also HD155763)",
	"title" : "Xi Draconis"
	},
{
	"Index" : "29173",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "34 Draconis, Psi02 Draconis, HIP 87728, SAO 8961, HD 164613, GC 24459, HR 6725, DM BD+72   818, TYC 4436-1426-1",
	"group" : { "key" : "Draco" },
	"Common" : "Psi02 Draconis",
	"OType" : "Star",
	"Distance" : "322.01",
	"RA_S" : 268.79646358,
	"DEC_S" : 72.00512635,
	"Constellation" : "Draco ",
	"AMag" : 5.453,
	"key" : 49173,
	"title" : "Psi02 Draconis"
	},
{
	"Index" : "27236",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "36 Draconis, HIP 89348, SAO 17828, HD 168151, GC 24916, HR 6850, DM BD+64  1252, TYC 4209-2018-1",
	"group" : { "key" : "Draco" },
	"Common" : "36 Draconis",
	"OType" : "High proper-motion Star",
	"Distance" : "22.92",
	"RA_S" : 273.4742987,
	"DEC_S" : 64.39728774,
	"Constellation" : "Draco ",
	"AMag" : 5.037,
	"key" : 47236,
	"title" : "36 Draconis"
	},
{
	"Index" : "29182",
	"Description" : "Phi Draconis (\u03C6 Dra / \u03C6 Draconis) is a fourth-magnitude star in the constellation Draco. It has the Flamsteed designation 43 Draconis.\r\rIn Chinese astronomy, Phi Draconis is called \u67F1\u53F2, Pinyin: Zh\u00F9sh\u01D0, meaning Official of Royal Archives, because this star is marking itself and stand alone in Official of Royal Archives asterism, Purple Forbidden enclosure (see : Chinese constellation). Possibly, \u67F1\u53F2 (Zh\u00F9sh\u01D0) westernized into Kwei She by R.H. Allen, with the unknown meaning, but it was for \u03C7 Dra",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "43 Draconis, Phi Draconis, HIP 89908AB, SAO 9084, HD 170000, GC 25114, HR 6920, DM BD+71   889, TYC 4437-1492-1",
	"group" : { "key" : "Draco" },
	"Common" : "Phi Draconis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "92.71",
	"RA_S" : 275.18923586,
	"DEC_S" : 71.33780684,
	"X" : 253,
	"Y" : 315,
	"Constellation" : "Draco ",
	"AMag" : 4.21,
	"key" : 49182,
	"title" : "Phi Draconis"
	},
{
	"Index" : "29181",
	"Description" : "Chi Draconis (\u03C7 Dra, \u03C7 Draconis, Chi Draconis) is a star system in the constellation Draco.\r\rThe first companion is a yellow-white (class F) fourth-magnitude star with a mass approximately equal to that of the sun, but it is nearly twice as luminous. The second companion is an orange (class K) sixth-magnitude star, that is less massive and of lesser luminosity than the sun. In 1898 this system was reported to be a spectroscopic binary system, with an orbital period of 280.55 days. The two stars have an average separation of nearly an astronomical unit, which would disrupt the orbit of any Earth-like planet that was close enough to the primary to support liquid water. The two stars have less than half the abundance of heavy elements as the Sun and are approximately a billion years older.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "44 Draconis, Chi Draconis, HIP 89937, SAO 9087, HD 170153, GC 25122, HR 6927, DM BD+72   839, TYC 4437-1491-1",
	"group" : { "key" : "Draco" },
	"Common" : "Chi Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "8.06",
	"RA_S" : 275.26409395,
	"DEC_S" : 72.73284772,
	"X" : 262,
	"Y" : 299,
	"Constellation" : "Draco ",
	"AMag" : 3.614,
	"key" : 49181,
	"title" : "Chi Draconis"
	},
{
	"Index" : "21230",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 89981, SAO 47417, HD 169305, GC 25085, HR 6891, DM BD+49 2782, TYC 3533-2577-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 6891",
	"OType" : "Variable Star",
	"Distance" : "198.5",
	"RA_S" : 275.38609184,
	"DEC_S" : 49.12159199,
	"Constellation" : "Draco ",
	"AMag" : 5.219,
	"key" : 41230,
	"title" : "HR 6891"
	},
{
	"Index" : "24665",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "39 Draconis, b Draconis, HIP 90156A, SAO 30949, HD 170073A, GC 25151, HR 6923, DM BD+58  1809, TYC 3916-1982-1",
	"group" : { "key" : "Draco" },
	"Common" : "b Draconis",
	"OType" : "Star",
	"Distance" : "56.44",
	"RA_S" : 275.977696,
	"DEC_S" : 58.800586,
	"Constellation" : "Draco ",
	"AMag" : 5.058,
	"key" : 44665,
	"title" : "b Draconis"
	},
{
	"Index" : "27333",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "42 Draconis, HIP 90344, SAO 17888, HD 170693, GC 25212, HR 6945, DM BD+65  1271, TYC 4222-2311-1",
	"group" : { "key" : "Draco" },
	"Common" : "42 Draconis",
	"OType" : "Star",
	"Distance" : "96.48",
	"RA_S" : 276.4964052,
	"DEC_S" : 65.56348038,
	"Constellation" : "Draco ",
	"AMag" : 4.955,
	"key" : 47333,
	"title" : "42 Draconis"
	},
{
	"Index" : "24654",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "45 Draconis, d Draconis, HIP 90905, SAO 31039, HD 171635, GC 25362, HR 6978, DM BD+56  2113, TYC 3913-2269-1",
	"group" : { "key" : "Draco" },
	"Common" : "d Draconis",
	"OType" : "Star",
	"Distance" : "638.88",
	"RA_S" : 278.14385203,
	"DEC_S" : 57.0455989,
	"Constellation" : "Draco ",
	"AMag" : 4.832,
	"key" : 44654,
	"title" : "d Draconis"
	},
{
	"Index" : "24709",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "46 Draconis, c Draconis, HIP 91755, SAO 31119, HD 173524, GC 25635, HR 7049, DM BD+55  2107, TYC 3922-2095-1",
	"group" : { "key" : "Draco" },
	"Common" : "c Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.35",
	"RA_S" : 280.65813791,
	"DEC_S" : 55.5394565,
	"Constellation" : "Draco ",
	"AMag" : 5.013,
	"key" : 44709,
	"title" : "c Draconis"
	},
{
	"Index" : "29212",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 92056, SAO 9241, HD 174980, GC 25803, HR 7117, DM BD+73  835, TYC 4442-1877-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 7117",
	"OType" : "Star",
	"Distance" : "96.76",
	"RA_S" : 281.44486116,
	"DEC_S" : 74.08555318,
	"Constellation" : "Draco ",
	"AMag" : 5.351,
	"key" : 49212,
	"title" : "HR 7117"
	},
{
	"Index" : "30322",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "50 Draconis, HIP 92112, SAO 9250, HD 175286, GC 25839, HR 7124, DM BD+75   682, TYC 4583-2839-1",
	"group" : { "key" : "Draco" },
	"Common" : "50 Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "85.8",
	"RA_S" : 281.59263237,
	"DEC_S" : 75.43396705,
	"Constellation" : "Draco ",
	"AMag" : 5.365,
	"key" : 50322,
	"title" : "50 Draconis"
	},
{
	"Index" : "24782",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "47 Draconis, Omicron Draconis, HIP 92512, SAO 31219, HD 175306, GC 25905, HR 7125, DM BD+59  1925, TYC 3930-1790-1",
	"group" : { "key" : "Draco" },
	"Common" : "Omicron Draconis",
	"OType" : "Variable of RS CVn type",
	"Distance" : "104.76",
	"RA_S" : 282.8004092,
	"DEC_S" : 59.38834934,
	"Constellation" : "Draco ",
	"AMag" : 4.765,
	"key" : 44782,
	"title" : "Omicron Draconis"
	},
{
	"Index" : "21389",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 92689, SAO 31241, HD 175535, GC 25935, HR 7137, DM BD+50 2686, TYC 3552-2018-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 7137",
	"OType" : "Star",
	"Distance" : "137.89",
	"RA_S" : 283.30642972,
	"DEC_S" : 50.70822961,
	"Constellation" : "Draco ",
	"AMag" : 5.011,
	"key" : 41389,
	"title" : "HR 7137"
	},
{
	"Index" : "29194",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "52 Draconis, Upsilon Draconis, HIP 92782, SAO 9283, HD 176524, GC 26024, HR 7180, DM BD+71   915, TYC 4439-1995-1",
	"group" : { "key" : "Draco" },
	"Common" : "Upsilon Draconis",
	"OType" : "Spectroscopic binary",
	"Distance" : "105.2",
	"RA_S" : 283.59940931,
	"DEC_S" : 71.29719057,
	"Constellation" : "Draco ",
	"AMag" : 4.942,
	"key" : 49194,
	"title" : "Upsilon Draconis"
	},
{
	"Index" : "21354",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 93299, SAO 31311, HD 177003, GC 26138, HR 7210, DM BD+50 2708, TYC 3549-2883-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 7210",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "205.42",
	"RA_S" : 285.05698503,
	"DEC_S" : 50.53346487,
	"Constellation" : "Draco ",
	"AMag" : 5.348,
	"key" : 41354,
	"title" : "HR 7210"
	},
{
	"Index" : "24682",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "51 Draconis, HIP 93713, SAO 31371, HD 178207, GC 26290, HR 7251, DM BD+53  2178, TYC 3919-1316-1",
	"group" : { "key" : "Draco" },
	"Common" : "51 Draconis",
	"OType" : "Star",
	"Distance" : "111.05",
	"RA_S" : 286.22985368,
	"DEC_S" : 53.39665719,
	"Constellation" : "Draco ",
	"AMag" : 5.393,
	"key" : 44682,
	"title" : "51 Draconis"
	},
{
	"Index" : "30319",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "59 Draconis, HIP 94083, SAO 9341, HD 180777, GC 26484, HR 7312, DM BD+76   717, TYC 4583-2836-1",
	"group" : { "key" : "Draco" },
	"Common" : "59 Draconis",
	"OType" : "Variable Star",
	"Distance" : "27.3",
	"RA_S" : 287.29114499,
	"DEC_S" : 76.56050147,
	"Constellation" : "Draco ",
	"AMag" : 5.144,
	"key" : 50319,
	"title" : "59 Draconis"
	},
{
	"Index" : "24765",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "53 Draconis, HIP 94302, SAO 31468, HD 180006, GC 26475, HR 7295, DM BD+56  2209, TYC 3928-1045-1",
	"group" : { "key" : "Draco" },
	"Common" : "53 Draconis",
	"OType" : "Variable Star",
	"Distance" : "105.4",
	"RA_S" : 287.91903489,
	"DEC_S" : 56.85921466,
	"Constellation" : "Draco ",
	"AMag" : 5.236,
	"key" : 44765,
	"title" : "53 Draconis"
	},
{
	"Index" : "29227",
	"Description" : "Delta Draconis (\u03B4 Dra, \u03B4 Draconis) is a yellow star in the constellation Draco. It has the traditional names Aldib, Altais (the goat) and Nodus Secundus. This star has an apparent visual magnitude of 3.0, making it easily visible to the naked eye. Parallax measurements with the Hipparcos satellite yield a distance estimate of 97.4 light-years (29.9 parsecs) from Earth.Delta Draconis is a giant star with a stellar classification of G9 III. This indicates that, at an estimated age of 800 million years, this star has exhausted the supply of hydrogen at its core and entered a later stage in its evolution. The angular diameter of the star is estimated as 3.37 \u00B1 0.06 mas. At a parallax of 32.54 mas, this corresponds to a physical radius equal to 11 times the solar radius. It is radiating 59 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,820 K. At this temperature, it is giving off the yellow-hued glow of a G-type star. With a mass 2.32 times that of the Sun, this star will end its life as a white dwarf.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "57 Draconis, Delta Draconis, HIP 94376, SAO 18222, HD 180711, GC 26520, HR 7310, DM BD+67  1129, TYC 4444-2239-1",
	"group" : { "key" : "Draco" },
	"Common" : "Aldib / Altais / Nodus Secundus",
	"OType" : "High proper-motion Star",
	"Distance" : "29.87",
	"RA_S" : 288.1387485,
	"DEC_S" : 67.66154123,
	"X" : 178,
	"Y" : 321,
	"Constellation" : "Draco ",
	"AMag" : 3.165,
	"key" : 49227,
	"shortTitle" : "Aldib; Nodus Secundus; Nodus II; Al'tais",
	"title" : "Aldib / Altais / Nodus Secundus"
	},
{
	"Index" : "24766",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "54 Draconis, HIP 94490, SAO 31497, HD 180610, GC 26537, HR 7309, DM BD+57  1968, TYC 3928-1728-1",
	"group" : { "key" : "Draco" },
	"Common" : "54 Draconis",
	"OType" : "Star",
	"Distance" : "50.65",
	"RA_S" : 288.47977904,
	"DEC_S" : 57.70509492,
	"Constellation" : "Draco ",
	"AMag" : 5.131,
	"key" : 44766,
	"title" : "54 Draconis"
	},
{
	"Index" : "29322",
	"Description" : "Tau Draconis (\u03C4 Dra) is a star in the constellation Draco. Its apparent magnitude is 4.45.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "60 Draconis, Tau Draconis, HIP 94648, SAO 9366, HD 181984, GC 26638, HR 7352, DM BD+73   857, TYC 4456-2107-1",
	"group" : { "key" : "Draco" },
	"Common" : "Tau Draconis",
	"OType" : "Variable Star",
	"Distance" : "44.86",
	"RA_S" : 288.88754691,
	"DEC_S" : 73.3554735,
	"X" : 224,
	"Y" : 262,
	"Constellation" : "Draco ",
	"AMag" : 4.593,
	"key" : 49322,
	"title" : "Tau Draconis"
	},
{
	"Index" : "27366",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "58 Draconis, Pi Draconis, HIP 95081, SAO 18299, HD 182564, GC 26735, HR 7371, DM BD+65  1345, TYC 4229-1852-1",
	"group" : { "key" : "Draco" },
	"Common" : "Pi Draconis",
	"OType" : "Star",
	"Distance" : "70.17",
	"RA_S" : 290.16704378,
	"DEC_S" : 65.71452899,
	"Constellation" : "Draco ",
	"AMag" : 4.58,
	"key" : 47366,
	"title" : "Pi Draconis"
	},
{
	"Index" : "29255",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "61 Draconis, Sigma Draconis, HIP 96100, SAO 18396, HD 185144, GC 27050, HR 7462, DM BD+69  1053, TYC 4448-2481-1",
	"group" : { "key" : "Draco" },
	"Common" : "Alsafi",
	"OType" : "Star",
	"Distance" : "5.75",
	"RA_S" : 293.08996735,
	"DEC_S" : 69.6611839,
	"Constellation" : "Draco ",
	"AMag" : 4.757,
	"key" : 49255,
	"shortTitle" : "Athafi",
	"title" : "Alsafi"
	},
{
	"Index" : "29263",
	"Description" : "Epsilon Draconis (\u03B5 Dra, \u03B5 Draconis) is a fourth-magnitude star in the constellation Draco. It has the traditional name Tyl. This star along with Delta Draconis (Altais), Pi Draconis and Rho Draconis forms an asterism known as Al T\u0101is, meaning \u0022the Goat\u0022.\r\rIn Chinese astronomy, \u5929\u5EDA (Ti\u0101n Ch\u00FA), meaning the Celestial Kitchen, refers to an asterism consisting of Epsilon Draconis, Delta Draconis, Sigma Draconis, Rho Draconis, 64 Draconis and Pi Draconis. Consequently, Epsilon Draconis itself is known as \u5929\u5EDA\u4E09 (Ti\u0101n Ch\u00FA s\u0101n, English: the Third Star of the Celestial Kitchen.)",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "63 Draconis, Epsilon Draconis, HIP 97433A, SAO 9540, HD 188119, GC 27471, HR 7582, DM BD+69  1070, TYC 4449-2652-1",
	"group" : { "key" : "Draco" },
	"Common" : "Epsilon Draconis",
	"OType" : "Variable Star",
	"Distance" : "45.36",
	"RA_S" : 297.04311623,
	"DEC_S" : 70.26792937,
	"X" : 172,
	"Y" : 267,
	"Constellation" : "Draco ",
	"AMag" : 4.01,
	"key" : 49263,
	"title" : "Epsilon Draconis"
	},
{
	"Index" : "29262",
	"Description" : "Epsilon Draconis (\u03B5 Dra, \u03B5 Draconis) is a fourth-magnitude star in the constellation Draco. It has the traditional name Tyl. This star along with Delta Draconis (Altais), Pi Draconis and Rho Draconis forms an asterism known as Al T\u0101is, meaning \u0022the Goat\u0022.\r\rIn Chinese astronomy, \u5929\u5EDA (Ti\u0101n Ch\u00FA), meaning the Celestial Kitchen, refers to an asterism consisting of Epsilon Draconis, Delta Draconis, Sigma Draconis, Rho Draconis, 64 Draconis and Pi Draconis. Consequently, Epsilon Draconis itself is known as \u5929\u5EDA\u4E09 (Ti\u0101n Ch\u00FA s\u0101n, English: the Third Star of the Celestial Kitchen.)",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "63 Draconis, Eps Draconis, HIP 97433B, TYC 4449-2651-1",
	"group" : { "key" : "Draco" },
	"Common" : "Epsilon Draconis",
	"OType" : "Star",
	"Distance" : "45.36",
	"RA_S" : 297.043371,
	"DEC_S" : 70.268678,
	"X" : 172,
	"Y" : 267,
	"Constellation" : "Draco ",
	"AMag" : 6.872,
	"key" : 49262,
	"title" : "Epsilon Draconis"
	},
{
	"Index" : "27466",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "64 Draconis, e Draconis, HIP 98583, SAO 18658, HD 190544, GC 27806, HR 7676, DM BD+64  1405, TYC 4240-471-1",
	"group" : { "key" : "Draco" },
	"Common" : "e Draconis",
	"OType" : "Star",
	"Distance" : "179.42",
	"RA_S" : 300.36892556,
	"DEC_S" : 64.82097234,
	"Constellation" : "Draco ",
	"AMag" : 5.408,
	"key" : 47466,
	"title" : "e Draconis"
	},
{
	"Index" : "29241",
	"Description" : "Rho Draconis (\u03C1 Dra) is a star in the constellation Draco. Its apparent magnitude is 4.50.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "67 Draconis, Rho Draconis, HIP 98702, SAO 18676, HD 190940, GC 27856, HR 7685, DM BD+67  1222, TYC 4446-1736-1",
	"group" : { "key" : "Draco" },
	"Common" : "Rho Draconis",
	"OType" : "Star",
	"Distance" : "131.33",
	"RA_S" : 300.70446338,
	"DEC_S" : 67.87356441,
	"X" : 138,
	"Y" : 274,
	"Constellation" : "Draco ",
	"AMag" : 4.653,
	"key" : 49241,
	"title" : "Rho Draconis"
	},
{
	"Index" : "30429",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "75 Draconis, HIP 100965, SAO 3408, HD 196787, GC 28611, HR 7901, DM BD+80   659, TYC 4597-1693-1",
	"group" : { "key" : "Draco" },
	"Common" : "75 Draconis",
	"OType" : "Star",
	"Distance" : "139.56",
	"RA_S" : 307.06077459,
	"DEC_S" : 81.42270933,
	"Constellation" : "Draco ",
	"AMag" : 5.48,
	"key" : 50429,
	"title" : "75 Draconis"
	},
{
	"Index" : "29332",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "73 Draconis, HIP 101260, SAO 9802, HD 196502, GC 28639, HR 7879, DM BD+74   872, TYC 4459-947-1",
	"group" : { "key" : "Draco" },
	"Common" : "73 Draconis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "120.89",
	"RA_S" : 307.87673911,
	"DEC_S" : 74.9546214,
	"Constellation" : "Draco ",
	"AMag" : 5.197,
	"key" : 49332,
	"title" : "73 Draconis"
	},
{
	"Index" : "30410",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 102599, SAO 3467, HD 199437, GC 29107, HR 8016, DM BD+80  672, TYC 4594-2182-1",
	"group" : { "key" : "Draco" },
	"Common" : "HR 8016",
	"OType" : "Variable Star",
	"Distance" : "122.18",
	"RA_S" : 311.88940438,
	"DEC_S" : 80.55226046,
	"Constellation" : "Draco ",
	"AMag" : 5.498,
	"key" : 50410,
	"title" : "HR 8016"
	},
{
	"Index" : "34970",
	"Description" : "Equulei Epsilon is a star system of apparent magnitude +5.23 in the constellation of Equuleus . It is located 176 light years away from the Solar System .\r\rThe two stars brighter Equulei Epsilon, Epsilon Equulei called A and B, are subgiants of spectral type of F7IV and F5IV respectively. The first has a surface temperature of about 6500 K and its luminosity is 11.1 times that of the Sun . Has a radius larger than 2.6 times the solar radius and a 60% greater mass than the Sun The projected rotation speed measured in the km/s- -42 probably corresponds to this star. Meanwhile, Epsilon Equulei B has a temperature of 6300 K and is 7.8 times more luminous than the Sun Its radius is 2.3 times larger than the Sun, and may have a mass of about 1.55 solar masses .\r\rThe orbital period of this binary is 101.5 years. Although the average separation between the two stars is 35 AU, the orbit is remarkably eccentric so that the separation between the two varies between 10 and 60 AU. The last periastron was in 1920 and the next will be in 2121.\r\rFinally, it is thought that the Epsilon Equulei A may be, in turn, a spectroscopic binary. The orbital period of the latter would be of 2.03 days.\r\rApproximately 10 seconds of arc A,B torque can see a star, though this star makes the second star system called Epsilon Equulei C (HIP 103571 / BD +03 4473C), of magnitude 7.3. Type is a star G0V whose binary separation is equal to or greater than 665 AU, implying an orbital period of over 7500 years.\r\rA fifth star, Epsilon Equulei D (BD +03 4473D), completes the star system. 12.4 magnitude, its separation from the bright AB pair is over 4300 AU.\r\rThe system Equulei Epsilon has an approximate age of 2200 million year",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "1 Equulei, Epsilon Equulei, HIP 103569B, SAO 126428, HD 199766B, GC 29276, HR 8034, DM BD+03  4473, TYC 521-2814-2",
	"group" : { "backgroundImage" : "images/Alignment/04.png",
		"description" : "Equuleus (pron.: /\u0268\u02C8kwu\u02D0li\u0259s/) is a constellation. Its name is Latin for \u0027little horse\u0027, a foal. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is the second smallest of the modern constellations (after Crux), spanning only 72 square degrees. It is also very faint, having no stars brighter than the fourth magnitude.\r\rIn Greek mythology, one myth associates Equuleus with the foal Celeris (meaning \u0022swiftness\u0022 or \u0022speed\u0022), who was the offspring or brother of the winged horse Pegasus. Celeris was given to Castor by Mercury. Other myths say that Equuleus is the horse struck from Poseidon\u0027s trident, during the contest between him and Athena when deciding which would be the superior. Because this section of stars rises before Pegasus, it is often called Equus Primus, or the First Horse. Equuleus is also linked to the story of Philyra and Saturn.\r\rCreated by Ptolemy, it abuts Pegasus; unlike the larger horse it is depicted as a horse\u0027s head alone.",
		"key" : "Equuleus",
		"grouptype" : "Equuleus",
		"Meaning" : "pony",
		"Family" : "Heavenly Waters",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Equuleus",
		"title" : "Equuleus Objects Group" },
	"Common" : "Epsilon Equulei",
	"OType" : "Star",
	"Distance" : "53.74",
	"RA_S" : 314.76857872,
	"DEC_S" : 4.29350516,
	"X" : 153,
	"Y" : 312,
	"Constellation" : "Equuleus ",
	"AMag" : 6.313,
	"key" : 54970,
	"title" : "Epsilon Equulei"
	},
{
	"Index" : "34969",
	"Description" : "Equulei Epsilon is a star system of apparent magnitude +5.23 in the constellation of Equuleus . It is located 176 light years away from the Solar System .\r\rThe two stars brighter Equulei Epsilon, Epsilon Equulei called A and B, are subgiants of spectral type of F7IV and F5IV respectively. The first has a surface temperature of about 6500 K and its luminosity is 11.1 times that of the Sun . Has a radius larger than 2.6 times the solar radius and a 60% greater mass than the Sun The projected rotation speed measured in the km/s- -42 probably corresponds to this star. Meanwhile, Epsilon Equulei B has a temperature of 6300 K and is 7.8 times more luminous than the Sun Its radius is 2.3 times larger than the Sun, and may have a mass of about 1.55 solar masses .\r\rThe orbital period of this binary is 101.5 years. Although the average separation between the two stars is 35 AU, the orbit is remarkably eccentric so that the separation between the two varies between 10 and 60 AU. The last periastron was in 1920 and the next will be in 2121.\r\rFinally, it is thought that the Epsilon Equulei A may be, in turn, a spectroscopic binary. The orbital period of the latter would be of 2.03 days.\r\rApproximately 10 seconds of arc A,B torque can see a star, though this star makes the second star system called Epsilon Equulei C (HIP 103571 / BD +03 4473C), of magnitude 7.3. Type is a star G0V whose binary separation is equal to or greater than 665 AU, implying an orbital period of over 7500 years.\r\rA fifth star, Epsilon Equulei D (BD +03 4473D), completes the star system. 12.4 magnitude, its separation from the bright AB pair is over 4300 AU.\r\rThe system Equulei Epsilon has an approximate age of 2200 million year",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "1 Equulei, Epsilon Equulei, HIP 103569A, SAO 126428, HD 199766A, GC 29276, HR 8034, DM BD+03  4473, TYC 521-2814-1",
	"group" : { "key" : "Equuleus" },
	"Common" : "Epsilon Equulei",
	"OType" : "Star",
	"Distance" : "53.74",
	"RA_S" : 314.76857872,
	"DEC_S" : 4.29350516,
	"X" : 153,
	"Y" : 312,
	"Constellation" : "Equuleus ",
	"AMag" : 5.963,
	"key" : 54969,
	"title" : "Epsilon Equulei"
	},
{
	"Index" : "947",
	"Description" : "Gamma Equulei (5 Equulei) is the Bayer designation for a double star in the northern constellation of Equuleus. It is located at a distance of around 118 light-years (36 parsecs) from Earth and has an apparent visual magnitude of 4.7.\r\rThe primary component is a chemically peculiar star with a stellar classification of A9 Sr Eu and an apparent magnitude of 4.80. Gamma Equulei undergoes periodic pulsations in luminosity, which places it among the category of roAp stars. The surface magnetic field undergoes long term variation with a period of 91.1 \u00B1 3.6 years, ranging from +577 G to \u20131,101 G. It has a magnitude 9.05 companion at an angular separation of 1.26 arcseconds.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "5 Equulei, Gamma Equulei, HIP 104521A, SAO 126593, HD 201601A, GC 29591, HR 8097, DM BD+09  4732, TYC 1108-2583-1",
	"group" : { "key" : "Equuleus" },
	"Common" : "Gamma Equulei",
	"OType" : "Star",
	"Distance" : "36.28",
	"RA_S" : 317.58542098,
	"DEC_S" : 10.13157595,
	"X" : 118,
	"Y" : 234,
	"Constellation" : "Equuleus ",
	"AMag" : 4.703,
	"key" : 20947,
	"title" : "Gamma Equulei"
	},
{
	"Index" : "957",
	"Description" : "Delta Equulei is the second brightest star in the constellation Equuleus. Delta Equulei is a binary star system about 60 light years away, with components of class G0 and F5. Their combined magnitude is 4.47, and their absolute magnitude is 3.142. There is controversy as to the exact masses of the stars. One study puts the larger at 1.22 solar masses and the smaller at 1.17, while another pegs them at 1.66 and 1.593. The luminosity of the larger star is calculated to be 2.23 solar, and the smaller to be 2.17.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "7 Equulei, Delta Equulei, HIP 104858AB, SAO 126643, HD 202275, GC 29697, HR 8123, DM BD+09  4746, TYC 1109-2583-1",
	"group" : { "key" : "Equuleus" },
	"Common" : "Delta Equulei",
	"OType" : "Spectroscopic binary",
	"Distance" : "18.48",
	"RA_S" : 318.62005755,
	"DEC_S" : 10.0069808,
	"X" : 105,
	"Y" : 235,
	"Constellation" : "Equuleus ",
	"AMag" : 4.544,
	"key" : 20957,
	"title" : "Delta Equulei"
	},
{
	"Index" : "36294",
	"Description" : "Alpha Equulei (\u03B1 Equ, \u03B1 Equulei) is a star in the constellation Equuleus. It has the traditional name Kitalpha (rarely Kitel Phard or Kitalphar), a contraction of the Arabic name \u0642\u0637\u0639\u0629 \u0627\u0644\u0641\u0631\u0633 qi\u1E6D\u0027a(t) al-faras \u0022a piece of the horse\u0022.\r\rIn Chinese, \u865A\u5BBF (X\u016B S\u00F9), meaning Emptiness (asterism), refers to an asterism consisting of \u03B1 Equulei and \u03B2 Aquarii. Consequently, \u03B1 Equulei itself is known as \u865B\u5BBF\u4E8C (X\u016B S\u00F9 \u00E8r, English: the Second Star of Emptiness.)\r\rAlpha Equulei collectively belongs to spectral class G0III and has apparent magnitude +3.92 and a luminosity approximately 75 times that of the Sun. Alpha Equulei is a unique spectroscopic binary star consisting of two components. Kitalpha is approximately 186 light years from Earth.\r\rThis star has 2.72 times the mass of the Sun, with a projected rotational velocity of 20.0 km s\u20131 and an estimated rotation period of 98.8 days.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "8 Equulei, Alpha Equulei, HIP 104987, SAO 126662, HD 202448, GC 29735, HR 8131, DM BD+04  4635A, TYC 536-2354-1",
	"group" : { "key" : "Equuleus" },
	"Common" : "Kitalpha",
	"OType" : "Spectroscopic binary",
	"Distance" : "58.33",
	"RA_S" : 318.95595026,
	"DEC_S" : 5.24786527,
	"X" : 98,
	"Y" : 299,
	"Constellation" : "Equuleus ",
	"AMag" : 3.993,
	"key" : 56294,
	"title" : "Kitalpha"
	},
{
	"Index" : "36824",
	"Description" : "Beta Equulei (Beta Equ, \u03B2 Equulei, \u03B2 Equ) is an A-type main sequence star in the constellation of Equuleus. It has an overall apparent visual magnitude of approximately 5.159.\r\r\u03B2 Equulei has four optical visual companions. They are not physically related to the star described above.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "10 Equulei, Beta Equulei, HIP 105570, SAO 126749, HD 203562, GC 29931, HR 8178, DM BD+06  4811, TYC 541-1932-1",
	"group" : { "key" : "Equuleus" },
	"Common" : "Beta Equulei",
	"OType" : "Star",
	"Distance" : "101.31",
	"RA_S" : 320.72338597,
	"DEC_S" : 6.81114101,
	"X" : 76,
	"Y" : 277,
	"Constellation" : "Equuleus ",
	"AMag" : 5.156,
	"key" : 56824,
	"title" : "Beta Equulei"
	},
{
	"Index" : "61594",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "q02 Eridani, HIP 8241, SAO 232520, HD 10939, GC 2165, HR 520, DM CP-54   377, TYC 8475-1390-1",
	"group" : { "backgroundImage" : "images/Alignment/25.png",
		"description" : "Eridanus /\u0268\u02C8r\u026Ad\u0259n\u0259s/ is a constellation. It is represented as a river; its name is the Ancient Greek name for the Po River. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. It is the sixth largest of the modern constellations.\r\rThe Eridanus Supervoid is the largest supervoid (an area of the universe devoid of galaxies) discovered as of 2007. At a diameter of about one billion light years it is much larger than any other known void and represents a challenge for current theories of the origins of the universe to explain. It was discovered by linking a \u0022cold spot\u0022 in the cosmic microwave background to an absence of radio galaxies in data of the United States National Radio Astronomy Observatory\u0027s Very Large Array Sky Survey. There is some speculation that the void may be due to quantum entanglement between our universe and another.\r\rThe name Eridanus refers to the Po River, the main river of northern Italy. Its association with a river comes from the way its stars trace a tortuous path. In some star maps, Eridanus is depicted as a river flowing from the waters poured by Aquarius. In such maps, Aquarius is visualized as facing Eridanus, requiring a different perspective and a redesign of how the stars of Aquarius connect, so the water pours onto the same side as Eridanus.\r\rAccording to one theory, the Greek constellation takes its name from the Babylonian constellation known as the Star of Eridu (MUL.NUN.KI). Eridu was an ancient city in the extreme south of Babylonia; situated in the marshy regions it was held sacred to the god Enki-Ea who ruled the cosmic domain of the Abyss - a mythical conception of the fresh-water reservoir below the Earth\u0027s surface.\r\rEridanus is connected to the myth of Pha\u00EBton, who took over the reins of his father Helios\u0027 sky chariot (i.e., the Sun), but didn\u0027t have the strength to control it and so veered wildly in different directions, scorching both earth and heaven. Zeus intervened by striking Pha\u00EBton dead with a thunderbolt and casting him to earth. The constellation was supposed to be the path Pha\u00EBton drove along; in later times, it was considered a path of souls. Since Eridanos was also a Greek name for the Po (Latin Padus), in which the burning body of Pha\u00EBton is said by Ovid to have extinguished, the mythic geography of the celestial and earthly Eridanus is complex.\r\rAnother association with Eridanus is a series of rivers all around the world. First conflated with the Nile River in Egypt, the constellation was also identified with the Po River in Italy. The stars of the modern constellation Fornax were formerly a part of Eridanus.",
		"key" : "Eridanus",
		"grouptype" : "Eridanus",
		"Meaning" : "river Eridanus (mythology)",
		"Family" : "Heavenly Waters",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Eridanus",
		"title" : "Eridanus Objects Group" },
	"Common" : "q02 Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "62.03",
	"RA_S" : 26.52609853,
	"DEC_S" : -53.52203884,
	"Constellation" : "Eridanus ",
	"AMag" : 5.037,
	"key" : 81594,
	"title" : "q02 Eridani"
	},
{
	"Index" : "57572",
	"Description" : "Chi Eridani (\u03C7 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 3.70.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Chi Eridani, HIP 9007, SAO 232573, HD 11937, GC 2339, HR 566, DM CP-52   241, TYC 8047-1321-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Chi Eridani",
	"OType" : "Pre-main sequence Star",
	"Distance" : "17.85",
	"RA_S" : 28.98944698,
	"DEC_S" : -51.60887338,
	"X" : 581,
	"Y" : 606,
	"Constellation" : "Eridanus ",
	"AMag" : 3.798,
	"key" : 77572,
	"title" : "Chi Eridani"
	},
{
	"Index" : "57629",
	"Description" : "Phi Eridani (\u03C6 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 3.55.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Phi Eridani, HIP 10602, SAO 232696, HD 14228, GC 2756, HR 674, DM CP-52   285, TYC 8055-1270-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Phi Eridani",
	"OType" : "Star",
	"Distance" : "47.12",
	"RA_S" : 34.12744736,
	"DEC_S" : -51.51216991,
	"X" : 543,
	"Y" : 601,
	"Constellation" : "Eridanus ",
	"AMag" : 3.52,
	"key" : 77629,
	"title" : "Phi Eridani"
	},
{
	"Index" : "57606",
	"Description" : "Kappa Eridani (\u03BA Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.23.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Kappa Eridani, HIP 11407, SAO 215906, HD 15371, GC 2954, HR 721, DM CD-48   637, TYC 8052-1380-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Kappa Eridani",
	"OType" : "Star",
	"Distance" : "155.66",
	"RA_S" : 36.74633395,
	"DEC_S" : -47.70384099,
	"X" : 527,
	"Y" : 555,
	"Constellation" : "Eridanus ",
	"AMag" : 4.208,
	"key" : 77606,
	"title" : "Kappa Eridani"
	},
{
	"Index" : "53256",
	"Description" : "HD 16754 is a star in the constellation Eridanus. Its apparent magnitude is 4.75.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "s Eridani, HIP 12413, SAO 215996, HD 16754, GC 3217, HR 789, DM CD-43   814, TYC 7558-987-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 16754",
	"OType" : "Spectroscopic binary",
	"Distance" : "39.73",
	"RA_S" : 39.95001032,
	"DEC_S" : -42.89168783,
	"X" : 503,
	"Y" : 497,
	"Constellation" : "Eridanus ",
	"AMag" : 4.736,
	"key" : 73256,
	"title" : "HD 16754"
	},
{
	"Index" : "53259",
	"Description" : "Iota Eridani (\u03B9 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.12.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Iota Eridani, HIP 12486, SAO 215999, HD 16815, GC 3237, HR 794, DM CD-40   689, TYC 7559-1160-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Iota Eridani",
	"OType" : "Star",
	"Distance" : "46.19",
	"RA_S" : 40.1668128,
	"DEC_S" : -39.85537772,
	"X" : 502,
	"Y" : 461,
	"Constellation" : "Eridanus ",
	"AMag" : 4.226,
	"key" : 73259,
	"title" : "Iota Eridani"
	},
{
	"Index" : "39947",
	"Description" : "Tau1 Eridani (\u03C41 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.50.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "1 Eridani, Tau01 Eridani, HIP 12843, SAO 148584, HD 17206, GC 3318, HR 818, DM BD-19   518, TYC 5866-1050-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau1 Eridani",
	"OType" : "Spectroscopic binary",
	"Distance" : "14.21",
	"RA_S" : 41.27576976,
	"DEC_S" : -18.57256937,
	"X" : 495,
	"Y" : 212,
	"Constellation" : "Eridanus ",
	"AMag" : 4.521,
	"key" : 59947,
	"title" : "Tau1 Eridani"
	},
{
	"Index" : "39973",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "2 Eridani, Tau02 Eridani, HIP 13288, SAO 168094, HD 17824, GC 3429, HR 850, DM BD-21   509, TYC 5870-1028-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Angetenar",
	"OType" : "Star",
	"Distance" : "57.3",
	"RA_S" : 42.75966558,
	"DEC_S" : -21.00402309,
	"Constellation" : "Eridanus ",
	"AMag" : 4.871,
	"key" : 59973,
	"shortTitle" : "Al Anchat al Nahr; Anchat",
	"title" : "Angetenar"
	},
{
	"Index" : "35626",
	"Description" : "Eta Eridani (\u03B7 Eri, \u03B7 Eridani) is a star in the constellation Eridanus. It has the traditional name Azha (\u0022the breeding place\u0022). The word Azha is a corruption of Persian \u0622\u0634\u064A\u0627\u0646\u0647 \u0101\u0161iy\u0101ne The (ostrich) nest.\r\rIn Chinese, \u5929\u82D1 (Ti\u0101n Yu\u00E0n), meaning Celestial Meadows, refers to an asterism consisting of \u03B7 Eridani, \u03B3 Eridani, \u03C0 Eridani, \u03B4 Eridani, \u03B5 Eridani, \u03B6 Eridani, \u03C0 Ceti, \u03C41 Eridani, \u03C42 Eridani, \u03C43 Eridani, \u03C44 Eridani, \u03C45 Eridani \u03C46 Eridani, \u03C47 Eridani, \u03C48 Eridani and \u03C49 Eridani. Consequently, \u03B7 Eridani itself is known as \u5929\u82D1\u516D (Ti\u0101n Yu\u00E0n li\u00F9, English: the Sixth Star of Celestial Meadows.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "3 Eridani, Eta Eridani, HIP 13701, SAO 130197, HD 18322, GC 3539, HR 874, DM BD-09   553, TYC 5287-1076-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Eta Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "41.86",
	"RA_S" : 44.10687285,
	"DEC_S" : -8.89814503,
	"X" : 462,
	"Y" : 99,
	"Constellation" : "Eridanus ",
	"AMag" : 4.013,
	"key" : 55626,
	"title" : "Eta Eridani"
	},
{
	"Index" : "31270",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 13717, SAO 130199, HD 18331, GC 3541, HR 875, DM BD-04  502, TYC 4703-1166-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR 875",
	"OType" : "Star",
	"Distance" : "57.16",
	"RA_S" : 44.15592956,
	"DEC_S" : -3.71231655,
	"Constellation" : "Eridanus ",
	"AMag" : 5.172,
	"key" : 51270,
	"title" : "HR 875"
	},
{
	"Index" : "44367",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "4 Eridani, HIP 13782, SAO 168183, HD 18454, GC 3561, HR 883, DM CD-24  1336, TYC 6437-957-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "4 Eridani",
	"OType" : "Star",
	"Distance" : "47.67",
	"RA_S" : 44.34902771,
	"DEC_S" : -23.86216697,
	"Constellation" : "Eridanus ",
	"AMag" : 5.464,
	"key" : 64367,
	"title" : "4 Eridani"
	},
{
	"Index" : "53305",
	"Description" : "Theta Eridani (\u03B8 Eri, \u03B8 Eridani) is a star in the constellation Eridanus. It has the traditional name Acamar from the Arabic \u0622\u062E\u0650\u0631 \u0627\u0644\u0646\u064E\u0651\u0647\u0652\u0631Empty citation\u200E (help) \u0100khir an-nahr which means \u0022the end of the river\u0022. Historically, Acamar represented the end of the constellation Eridanus. Now that distinction is held by the star Achernar, a star which shares the same Arabic etymology. Achernar is not visible from the Greek isles (latitudes > 33\u00B0 North), hence the choice of Acamar as the river\u0027s end during the time of Hipparchus and later Ptolemy.\r\rThe term \u0100khir an-nahr or Achr al Nahr was appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, which was translated into Latin as Postrema Fluminis.\r\rIn Chinese, \u5929\u5712 (Ti\u0101n Yu\u00E1n), meaning Celestial Orchard, refers to an asterism consisting of \u03B8 Eridani, \u03C7 Eridani, \u03C6 Eridani, \u03BA Eridani, HD 16754, HD 23319, HD 24072, HD 24160, \u03C54 Eridani, 43 Eridani, \u03C52 Eridani and \u03C51 Eridani. Consequently, \u03B8 Eridani itself is known as \u5929\u5712\u516D (Ti\u0101n Yu\u00E1n li\u00F9, English: the Sixth Star of Celestial Orchard.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Theta01 Eridani, HIP 13847A, SAO 216113, HD 18622J, GC 3584, HR 897, DM CD-40   771A, TYC 7563-1016-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Theta Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "49.41",
	"RA_S" : 44.56531355,
	"DEC_S" : -40.30468123,
	"X" : 463,
	"Y" : 467,
	"Constellation" : "Eridanus ",
	"AMag" : 2.88,
	"key" : 73305,
	"shortTitle" : "Akamar",
	"title" : "Theta Eridani"
	},
{
	"Index" : "53306",
	"Description" : "Theta Eridani (\u03B8 Eri, \u03B8 Eridani) is a star in the constellation Eridanus. It has the traditional name Acamar from the Arabic \u0622\u062E\u0650\u0631 \u0627\u0644\u0646\u064E\u0651\u0647\u0652\u0631Empty citation\u200E (help) \u0100khir an-nahr which means \u0022the end of the river\u0022. Historically, Acamar represented the end of the constellation Eridanus. Now that distinction is held by the star Achernar, a star which shares the same Arabic etymology. Achernar is not visible from the Greek isles (latitudes > 33\u00B0 North), hence the choice of Acamar as the river\u0027s end during the time of Hipparchus and later Ptolemy.\r\rThe term \u0100khir an-nahr or Achr al Nahr was appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, which was translated into Latin as Postrema Fluminis.\r\rIn Chinese, \u5929\u5712 (Ti\u0101n Yu\u00E1n), meaning Celestial Orchard, refers to an asterism consisting of \u03B8 Eridani, \u03C7 Eridani, \u03C6 Eridani, \u03BA Eridani, HD 16754, HD 23319, HD 24072, HD 24160, \u03C54 Eridani, 43 Eridani, \u03C52 Eridani and \u03C51 Eridani. Consequently, \u03B8 Eridani itself is known as \u5929\u5712\u516D (Ti\u0101n Yu\u00E1n li\u00F9, English: the Sixth Star of Celestial Orchard.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Theta01 Eridani, HIP 13847B, TYC 7563-1017-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Theta Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "49.41",
	"RA_S" : 44.56848739,
	"DEC_S" : -40.30471666,
	"X" : 463,
	"Y" : 467,
	"Constellation" : "Eridanus ",
	"AMag" : 4.119,
	"key" : 73306,
	"title" : "Theta Eridani"
	},
{
	"Index" : "31269",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 13874, SAO 130215, HD 18543, GC 3580, HR 892, DM BD-03  470, TYC 4703-1165-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR   892",
	"OType" : "Star",
	"Distance" : "110.15",
	"RA_S" : 44.67532316,
	"DEC_S" : -2.78288569,
	"Constellation" : "Eridanus ",
	"AMag" : 5.226,
	"key" : 51269,
	"title" : "HR   892"
	},
{
	"Index" : "44372",
	"Description" : "Tau3 Eridani (\u03C43 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.10.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "11 Eridani, Tau03 Eridani, HIP 14146, SAO 168249, HD 18978, GC 3649, HR 919, DM CD-24  1387, TYC 6438-1110-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau3 Eridani",
	"OType" : "Star",
	"Distance" : "27.17",
	"RA_S" : 45.59791413,
	"DEC_S" : -23.62447044,
	"X" : 448,
	"Y" : 272,
	"Constellation" : "Eridanus ",
	"AMag" : 4.092,
	"key" : 64372,
	"title" : "Tau3 Eridani"
	},
{
	"Index" : "35625",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "9 Eridani, Rho02 Eridani, HIP 14168, SAO 130254, HD 18953, GC 3651, HR 917, DM BD-08   568, TYC 5287-1075-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Rho02 Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "78.58",
	"RA_S" : 45.67617576,
	"DEC_S" : -7.68547124,
	"Constellation" : "Eridanus ",
	"AMag" : 5.442,
	"key" : 55625,
	"title" : "Rho02 Eridani"
	},
{
	"Index" : "35680",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "10 Eridani, Rho03 Eridani, HIP 14293, SAO 130269, HD 19107, GC 3677, HR 925, DM BD-08   572, TYC 5294-1195-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Rho03 Eridani",
	"OType" : "Star",
	"Distance" : "41.55",
	"RA_S" : 46.06881392,
	"DEC_S" : -7.60085634,
	"Constellation" : "Eridanus ",
	"AMag" : 5.281,
	"key" : 55680,
	"title" : "Rho03 Eridani"
	},
{
	"Index" : "31345",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 14456, SAO 130284, HD 19349, GC 3718, HR 935, DM BD-06  606, TYC 4713-1122-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR 935",
	"OType" : "Star",
	"Distance" : "139.31",
	"RA_S" : 46.63955062,
	"DEC_S" : -6.08855335,
	"Constellation" : "Eridanus ",
	"AMag" : 5.443,
	"key" : 51345,
	"title" : "HR 935"
	},
{
	"Index" : "35689",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "13 Eridani, Zeta Eridani, HIP 15197, SAO 130387, HD 20320, GC 3899, HR 984, DM BD-09   624, TYC 5295-1259-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Zibal",
	"OType" : "Spectroscopic binary",
	"Distance" : "33.64",
	"RA_S" : 48.95843436,
	"DEC_S" : -8.81973052,
	"Constellation" : "Eridanus ",
	"AMag" : 4.821,
	"key" : 55689,
	"title" : "Zibal"
	},
{
	"Index" : "44375",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "15 Eridani, HIP 15382AB, SAO 168452, HD 20610, GC 3955, HR 994, DM CD-22  1146, TYC 6439-1171-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "15 Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "77.86",
	"RA_S" : 49.59209599,
	"DEC_S" : -22.51111332,
	"Constellation" : "Eridanus ",
	"AMag" : 4.976,
	"key" : 64375,
	"title" : "15 Eridani"
	},
{
	"Index" : "40035",
	"Description" : "Tau4 Eridani (\u03C44 Eri, \u03C44 Eri) is a Class M3.5III, fourth-magnitude star in the constellation Eridanus. Tau4 Eridani is a binary star system consisting primarily of Class M components, the brightest component being a Class M giant of apparent magnitude 3.66, having a mass and luminosity many times greater than that of the Sun. It is occasionally eclipsed by other stellar components within the system in ways similar to Algol. The entire star system is located about 260 light-years from Earth.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "16 Eridani, Tau04 Eridani, HIP 15474, SAO 168460, HD 20720, GC 3979, HR 1003, DM BD-22   584, TYC 5878-1292-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau4 Eridani",
	"OType" : "Long-period variable star",
	"Distance" : "93.09",
	"RA_S" : 49.87917285,
	"DEC_S" : -21.75786579,
	"X" : 401,
	"Y" : 252,
	"Constellation" : "Eridanus ",
	"AMag" : 3.91,
	"key" : 60035,
	"title" : "Tau4 Eridani"
	},
{
	"Index" : "53334",
	"Description" : "82 G. Eridani (HD 20794, HR 1008, e Eridani) is a star about 20 light years away from Earth in the constellation Eridanus. It is a main-sequence star with a stellar classification of G8. In the southern-sky catalog Uranometria Argentina, 82 G. Eridani (sometimes abbreviated to \u002282 Eridani\u0022) is the 82nd star listed in the constellation Eridanus. The Argentina catalog, compiled by the 19th-century astronomer Benjamin Gould, is a southern celestial hemisphere analog of the more famous Flamsteed catalog, and uses a similar numbering scheme. 82 G. Eridani, like other stars near the Sun, has held on to its Gould designation, even while other more distant stars have not.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "82 Eridani, e Eridani, HIP 15510, SAO 216263, HD 20794, GC 4000, HR 1008, DM CD-43  1028, TYC 7567-1183-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "82 G. Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "6.04",
	"RA_S" : 49.98187897,
	"DEC_S" : -43.06978094,
	"X" : 417,
	"Y" : 501,
	"Constellation" : "Eridanus ",
	"AMag" : 4.336,
	"key" : 73334,
	"title" : "82 G. Eridani"
	},
{
	"Index" : "31434",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "17 Eridani, v Eridani, HIP 16341, SAO 130528, HD 21790, GC 4185, HR 1070, DM BD-05   674, TYC 4722-1534-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "v Eridani",
	"OType" : "Star",
	"Distance" : "123.82",
	"RA_S" : 52.65440929,
	"DEC_S" : -5.07514552,
	"Constellation" : "Eridanus ",
	"AMag" : 4.71,
	"key" : 51434,
	"title" : "v Eridani"
	},
{
	"Index" : "35696",
	"Description" : "Epsilon Eridani (\u03B5 Eri, \u03B5 Eridani) is a star in the southern constellation Eridanus, along a declination 9.46\u00B0 south of the celestial equator. This allows the star to be viewed from most of the Earth\u0027s surface. At a distance of 10.5 light years (ly), it has an apparent magnitude of 3.73. It is the third closest of the individual stars or star systems visible to the unaided eye and was the closest star known to host a planet until the discovery of Alpha Centauri Bb. Its age is estimated at less than a billion years. Because of its youth, Epsilon Eridani has a higher level of magnetic activity than the present-day Sun, with a stellar wind 30 times as strong. Its rotation period is 11.2 days at the equator. Epsilon Eridani is smaller and less massive than the Sun, and has a comparatively lower level of elements heavier than helium. Astronomers categorize it as a main-sequence star of spectral class K2, which means that energy generated at the core through nuclear fusion of hydrogen is emitted from the surface at a temperature of about 5,000 K, giving the star an orange hue.\r\rThe motion of this star along the line of sight to the Earth, known as the radial velocity, has been regularly observed for more than twenty years. Periodic changes in this data yielded evidence of a giant planet orbiting Epsilon Eridani, making it one of the nearest extrasolar system with a candidate exoplanet. This object, Epsilon Eridani b, was formally announced in 2000 by a team of astronomers led by Artie Hatzes. Current data indicate that this planet orbits with a period of about 7 years at a mean separation of 3.4 astronomical units (AU), where 1 AU is the mean distance between the Earth and the Sun. Although this discovery has been controversial because of the amount of background noise in the radial velocity data, many astronomers now regard the planet as confirmed.\r\rThe system includes two belts of rocky asteroids: one at about 3 AU and a second at about 20 AU, whose structure may be maintained by a hypothetical second planet, Epsilon Eridani c. Epsilon Eridani harbors an extensive outer debris disk of remnant planetesimals left over from the system\u0027s formation.\r\rThe designation for this star was established in 1603 by Johann Bayer. It may be a member of the Ursa Major Moving Group of stars that share a similar motion through the Milky Way, implying these stars shared a common origin in an open cluster. Its nearest neighbor, the binary star system Luyten 726-8, will have a close encounter with Epsilon Eridani in approximately 31,500 years when they will be separated by about 0.93 ly. As one of the nearest Sun-like stars with the potential for a planet that may harbor life, Epsilon Eridani has been the target of SETI searches. The star appears in science fiction stories and has been suggested as a destination for interstellar travel.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "18 Eridani, Epsilon Eridani, HIP 16537, SAO 130564, HD 22049, GC 4244, HR 1084, DM BD-09   697, TYC 5296-1533-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Epsilon Eridani",
	"OType" : "Variable of BY Dra type",
	"Distance" : "3.22",
	"RA_S" : 53.23268481,
	"DEC_S" : -9.458263,
	"X" : 354,
	"Y" : 111,
	"Constellation" : "Eridanus ",
	"AMag" : 3.814,
	"key" : 55696,
	"title" : "Epsilon Eridani"
	},
{
	"Index" : "40045",
	"Description" : "Tau5 Eridani (\u03C45 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.30.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "19 Eridani, Tau05 Eridani, HIP 16611, SAO 168634, HD 22203, GC 4258, HR 1088, DM BD-22   628, TYC 5880-1266-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau5 Eridani",
	"OType" : "Spectroscopic binary",
	"Distance" : "89.89",
	"RA_S" : 53.44698387,
	"DEC_S" : -21.63288417,
	"X" : 362,
	"Y" : 254,
	"Constellation" : "Eridanus ",
	"AMag" : 4.233,
	"key" : 60045,
	"title" : "Tau5 Eridani"
	},
{
	"Index" : "40003",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "20 Eridani, HIP 16803AB, SAO 149063, HD 22470, GC 4305, HR 1100, DM BD-17   699, TYC 5874-1098-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "20 Eridani",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "148.22",
	"RA_S" : 54.0725401,
	"DEC_S" : -17.46706696,
	"Constellation" : "Eridanus ",
	"AMag" : 5.218,
	"key" : 60003,
	"title" : "20 Eridani"
	},
{
	"Index" : "53372",
	"Description" : "HD 22663 is a star in the constellation Eridanus. Its apparent magnitude is 4.59.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "y Eridani, HIP 16870, SAO 216405, HD 22663, GC 4329, HR 1106, DM CD-40  1008, TYC 7572-1748-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 22663",
	"OType" : "Star",
	"Distance" : "70.65",
	"RA_S" : 54.27363462,
	"DEC_S" : -40.27457056,
	"X" : 376,
	"Y" : 473,
	"Constellation" : "Eridanus ",
	"AMag" : 4.689,
	"key" : 73372,
	"title" : "HD 22663"
	},
{
	"Index" : "31445",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "22 Eridani, HIP 17167, SAO 130652, HD 22920, GC 4395, HR 1121, DM BD-05   715, TYC 4723-1351-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "22 Eridani",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "151.28",
	"RA_S" : 55.15972103,
	"DEC_S" : -5.21070837,
	"Constellation" : "Eridanus ",
	"AMag" : 5.494,
	"key" : 51445,
	"title" : "22 Eridani"
	},
{
	"Index" : "48801",
	"Description" : "HD 23319 is a star in the constellation Eridanus. Its apparent magnitude is 4.60.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "h Eridani, HIP 17351, SAO 194475, HD 23319, GC 4455, HR 1143, DM CD-37  1415, TYC 7034-1311-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 23319",
	"OType" : "Horizontal Branch Star",
	"Distance" : "56.49",
	"RA_S" : 55.70856423,
	"DEC_S" : -37.31352025,
	"X" : 358,
	"Y" : 439,
	"Constellation" : "Eridanus ",
	"AMag" : 4.717,
	"key" : 68801,
	"title" : "HD 23319"
	},
{
	"Index" : "35749",
	"Description" : "Delta Eridani (\u03B4 Eri, \u03B4 Eridani) is a 3.54 magnitude star in the constellation of Eridanus. It is also called Rana. The name Rana means \u0022the frog\u0022 in Latin\r\rIn Chinese, \u5929\u82D1 (Ti\u0101n Yu\u00E0n), meaning Celestial Meadows, refers to an asterism consisting of \u03B4 Eridani, \u03B3 Eridani, \u03C0 Eridani, \u03B5 Eridani, \u03B6 Eridani, \u03B7 Eridani, \u03C0 Ceti, \u03C41 Eridani, \u03C42 Eridani, \u03C43 Eridani, \u03C44 Eridani, \u03C45 Eridani, \u03C46 Eridani, \u03C47 Eridani, \u03C48 Eridani and \u03C49 Eridani. Consequently, \u03B4 Eridani itself is known as \u5929\u82D1\u4E09 (Ti\u0101n Yu\u00E0n s\u0101n, English: the Third Star of Celestial Meadows.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "23 Eridani, Delta Eridani, HIP 17378, SAO 130686, HD 23249, GC 4450, HR 1136, DM BD-10   728, TYC 5303-1320-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Rana",
	"OType" : "Variable of RS CVn type",
	"Distance" : "9.04",
	"RA_S" : 55.81208985,
	"DEC_S" : -9.76339431,
	"X" : 324,
	"Y" : 117,
	"Constellation" : "Eridanus ",
	"AMag" : 3.622,
	"key" : 55749,
	"title" : "Rana"
	},
{
	"Index" : "31379",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "24 Eridani, HIP 17457, SAO 130698, HD 23363, GC 4481, HR 1146, DM BD-01   526, TYC 4717-1350-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "24 Eridani",
	"OType" : "Star",
	"Distance" : "200.29",
	"RA_S" : 56.1271246,
	"DEC_S" : -1.16309127,
	"Constellation" : "Eridanus ",
	"AMag" : 5.209,
	"key" : 51379,
	"title" : "24 Eridani"
	},
{
	"Index" : "35791",
	"Description" : "Pi Eridani (\u03C0 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.44.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "26 Eridani, Pi Eridani, HIP 17593, SAO 149158, HD 23614, GC 4525, HR 1162, DM BD-12   707, TYC 5307-1357-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Pi Eridani",
	"OType" : "Long Period Variable candidate",
	"Distance" : "146.42",
	"RA_S" : 56.53556566,
	"DEC_S" : -12.10159007,
	"X" : 318,
	"Y" : 145,
	"Constellation" : "Eridanus ",
	"AMag" : 4.613,
	"key" : 55791,
	"title" : "Pi Eridani"
	},
{
	"Index" : "44446",
	"Description" : "Tau6 Eridani (\u03C46 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.20.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "27 Eridani, Tau06 Eridani, HIP 17651, SAO 168827, HD 23754, GC 4547, HR 1173, DM CD-23  1565, TYC 6448-1370-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau6 Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "17.63",
	"RA_S" : 56.71203254,
	"DEC_S" : -23.24972535,
	"X" : 328,
	"Y" : 277,
	"Constellation" : "Eridanus ",
	"AMag" : 4.266,
	"key" : 64446,
	"title" : "Tau6 Eridani"
	},
{
	"Index" : "44447",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "28 Eridani, Tau07 Eridani, HIP 17717, SAO 168836, HD 23878, GC 4566, HR 1181, DM CD-24  1877, TYC 6448-1371-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau07 Eridani",
	"OType" : "Star",
	"Distance" : "76.88",
	"RA_S" : 56.9152152,
	"DEC_S" : -23.87467618,
	"Constellation" : "Eridanus ",
	"AMag" : 5.244,
	"key" : 64447,
	"title" : "Tau07 Eridani"
	},
{
	"Index" : "53351",
	"Description" : "HD 24071 is a star in the constellation Eridanus. Its apparent magnitude is 4.26.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "f Eridani, HIP 17797B, SAO 194550, HD 24071, GC 4601, HR 1189, DM CD-38  1297B, TYC 7570-1586-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 24071",
	"OType" : "Star",
	"Distance" : "49.33",
	"RA_S" : 57.14784795,
	"DEC_S" : -37.62201025,
	"X" : 346,
	"Y" : 445,
	"Constellation" : "Eridanus ",
	"AMag" : 5.247,
	"key" : 73351,
	"title" : "HD 24071"
	},
{
	"Index" : "53350",
	"Description" : "HD 24071 is a star in the constellation Eridanus. Its apparent magnitude is 4.26.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "f Eridani, HIP 17797A, SAO 194551, HD 24072, GC 4602, HR 1190, DM CD-38  1297A, TYC 7570-1585-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 24071",
	"OType" : "Variable Star",
	"Distance" : "49.33",
	"RA_S" : 57.14949957,
	"DEC_S" : -37.62015638,
	"X" : 346,
	"Y" : 445,
	"Constellation" : "Eridanus ",
	"AMag" : 4.717,
	"key" : 73350,
	"title" : "HD 24071"
	},
{
	"Index" : "48811",
	"Description" : "HD 24160 is a star in the constellation Eridanus. Its apparent magnitude is 4.17.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "g Eridani, HIP 17874, SAO 194559, HD 24160, GC 4624, HR 1195, DM CD-36  1467, TYC 7035-1374-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HD 24160",
	"OType" : "Star",
	"Distance" : "64.34",
	"RA_S" : 57.36351801,
	"DEC_S" : -36.20024346,
	"X" : 341,
	"Y" : 429,
	"Constellation" : "Eridanus ",
	"AMag" : 4.267,
	"key" : 68811,
	"title" : "HD 24160"
	},
{
	"Index" : "31454",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "30 Eridani, HIP 18141, SAO 130789, HD 24388, GC 4675, HR 1202, DM BD-05   769, TYC 4724-1421-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "30 Eridani",
	"OType" : "Star",
	"Distance" : "178.54",
	"RA_S" : 58.17355611,
	"DEC_S" : -5.36124711,
	"Constellation" : "Eridanus ",
	"AMag" : 5.46,
	"key" : 51454,
	"title" : "30 Eridani"
	},
{
	"Index" : "48787",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "i Eridani, HIP 18213, SAO 194608, HD 24626, GC 4701, HR 1214, DM CD-35  1455, TYC 7032-1403-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "i Eridani",
	"OType" : "Star",
	"Distance" : "106.09",
	"RA_S" : 58.41227504,
	"DEC_S" : -34.73229983,
	"Constellation" : "Eridanus ",
	"AMag" : 5.071,
	"key" : 68787,
	"title" : "i Eridani"
	},
{
	"Index" : "44448",
	"Description" : "Tau8 Eridani (\u03C48 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.63.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "33 Eridani, Tau08 Eridani, HIP 18216, SAO 168925, HD 24587, GC 4698, HR 1213, DM CD-24  1945, TYC 6448-1372-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau8 Eridani",
	"OType" : "Rotationally variable Star",
	"Distance" : "115.44",
	"RA_S" : 58.42793366,
	"DEC_S" : -24.61222349,
	"X" : 312,
	"Y" : 295,
	"Constellation" : "Eridanus ",
	"AMag" : 4.603,
	"key" : 64448,
	"title" : "Tau8 Eridani"
	},
{
	"Index" : "31416",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "32 Eridani, w Eridani, HIP 18255B, SAO 130805, HD 24554, GC 4705, HR 1211, DM BD-03   631B, TYC 4721-1217-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "32 Eridani",
	"OType" : "Star",
	"Distance" : "95.31",
	"RA_S" : 58.572471,
	"DEC_S" : -2.952861,
	"X" : 286,
	"Y" : 40,
	"Constellation" : "Eridanus ",
	"AMag" : 5.887,
	"key" : 51416,
	"title" : "32 Eridani"
	},
{
	"Index" : "31417",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "32 Eridani, HIP 18255A, TYC 4721-1218-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "32 Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "95.31",
	"RA_S" : 58.57292417,
	"DEC_S" : -2.9547343,
	"X" : 286,
	"Y" : 40,
	"Constellation" : "Eridanus ",
	"AMag" : 4.46,
	"key" : 51417,
	"title" : "32 Eridani"
	},
{
	"Index" : "35825",
	"Description" : "Gamma Eridani (\u03B3 Eri, \u03B3 Eridani) is a star in the constellation Eridanus. It has the traditional name Zaurak, which means \u0022the boat.\r\rIn Chinese, \u5929\u82D1 (Ti\u0101n Yu\u00E0n), meaning Celestial Meadows, refers to an asterism consisting of \u03B3 Eridani, \u03B4 Eridani, \u03C0 Eridani, \u03B5 Eridani, \u03B6 Eridani, \u03B7 Eridani, \u03C0 Ceti, \u03C41 Eridani, \u03C42 Eridani, \u03C43 Eridani, \u03C44 Eridani, \u03C45 Eridani, \u03C46 Eridani, \u03C47 Eridani, \u03C48 Eridani and \u03C49 Eridani. Consequently, \u03B3 Eridani itself is known as \u5929\u82D1\u4E00 (Ti\u0101n Yu\u00E0n y\u012B, English: the First Star of Celestial Meadows.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "34 Eridani, Gamma Eridani, HIP 18543, SAO 149283, HD 25025, GC 4778, HR 1231, DM BD-13   781, TYC 5311-1285-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Zaurak",
	"OType" : "Long Period Variable candidate",
	"Distance" : "62.25",
	"RA_S" : 59.50736224,
	"DEC_S" : -13.50851619,
	"X" : 285,
	"Y" : 166,
	"Constellation" : "Eridanus ",
	"AMag" : 3.129,
	"key" : 55825,
	"shortTitle" : "Zaurac; Zaurack",
	"title" : "Zaurak"
	},
{
	"Index" : "44497",
	"Description" : "Tau9 Eridani (\u03C49 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.62.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "36 Eridani, Tau09 Eridani, HIP 18673, SAO 169017, HD 25267, GC 4801, HR 1240, DM CD-24  2022, TYC 6455-1268-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Tau9 Eridani",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "100.34",
	"RA_S" : 59.98118254,
	"DEC_S" : -24.01621661,
	"X" : 295,
	"Y" : 290,
	"Constellation" : "Eridanus ",
	"AMag" : 4.602,
	"key" : 64497,
	"title" : "Tau9 Eridani"
	},
{
	"Index" : "31468",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "35 Eridani, HIP 18788, SAO 130878, HD 25340, GC 4828, HR 1244, DM BD-01   572, TYC 4725-1278-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "35 Eridani",
	"OType" : "Star",
	"Distance" : "126.73",
	"RA_S" : 60.38354148,
	"DEC_S" : -1.54965781,
	"Constellation" : "Eridanus ",
	"AMag" : 5.241,
	"key" : 51468,
	"title" : "35 Eridani"
	},
{
	"Index" : "31466",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 18859, SAO 130893, HD 25457, GC 4851, HR 1249, DM BD-00  632, TYC 4725-1276-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Gliese 159",
	"OType" : "T Tau-type Star",
	"Distance" : "18.83",
	"RA_S" : 60.65310298,
	"Constellation" : "Eridanus ",
	"AMag" : 5.437,
	"key" : 51466,
	"title" : "Gliese 159"
	},
{
	"Index" : "40070",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 19398, SAO 149412, HD 26326, GC 5009, HR 1288, DM BD-16  796, TYC 5883-1617-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR  1288",
	"OType" : "Pulsating variable Star",
	"Distance" : "199.25",
	"RA_S" : 62.32431387,
	"DEC_S" : -16.38586904,
	"Constellation" : "Eridanus ",
	"AMag" : 5.411,
	"key" : 60070,
	"title" : "HR  1288"
	},
{
	"Index" : "31537",
	"Description" : "Omicron1 Eridani (also known as Beid) is a star of visual magnitude 4.04. It lies approximately 125 light-years from Earth in the Eridanus constellation and is a class F (F2) giant with a surface temperature of 7100 K and a luminosity 28 times that of the Sun. In 1971 it was discovered to be a Delta Scuti variable star, with a variation of just a few hundredths of a magnitude with periods of 1.8 and 3.5 days.\r\rIn Chinese, \u4E5D\u5DDE\u6B8A\u53E3 (Ji\u01D4 Zh\u014Du Sh\u016B K\u01D2u), meaning Interpreters of Nine Dialects, refers to an asterism consisting of \u03BF1 Eridani, 39 Eridani, \u03BE Eridani, \u03BD Eridani, 56 Eridani and 55 Eri. Consequently, \u03BF1 Eridani itself is known as \u4E5D\u5DDE\u6B8A\u53E3\u4E8C (Ji\u01D4 Zh\u014Du Sh\u016B K\u01D2u \u00E8r, English: the Second Star of Interpreters of Nine Dialects.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "38 Eridani, Omicron01 Eridani, HIP 19587, SAO 131019, HD 26574, GC 5056, HR 1298, DM BD-07   764, TYC 4732-1970-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Omicron1 Eridani",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "37.31",
	"RA_S" : 62.96641409,
	"DEC_S" : -6.83757967,
	"X" : 236,
	"Y" : 93,
	"Constellation" : "Eridanus ",
	"AMag" : 4.067,
	"key" : 51537,
	"title" : "Omicron1 Eridani"
	},
{
	"Index" : "35871",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "39 Eridani, A Eridani, HIP 19777A, SAO 149478, HD 26846, GC 5114, HR 1318, DM BD-10   867, TYC 5315-2290-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "A Eridani",
	"OType" : "Star",
	"Distance" : "74.12",
	"RA_S" : 63.59869527,
	"DEC_S" : -10.25627447,
	"Constellation" : "Eridanus ",
	"AMag" : 5.028,
	"key" : 55871,
	"title" : "A Eridani"
	},
{
	"Index" : "35845",
	"Description" : "40 Eridani (also known as Omicron2 Eridani, or Keid, from the Arabic word qayd, (egg) shells) is a triple star system less than 16.5 light years away from Earth. It is in the constellation Eridanus. The primary star of the system, 40 Eridani A, is easily visible to the naked eye. The pair 40 Eridani B/C was discovered on January 31, 1783, by William Herschel., p. 73 It was again observed by Friedrich Georg Wilhelm Struve in 1825 and by Otto Wilhelm von Struve in 1851. In 1910, it was discovered that although component B was a faint star, it was white in color. This meant that it had to be a small star; in fact it was a white dwarf, the first discovered. 40 Eridani A is a main-sequence dwarf of spectral type K1. Its two companion stars, 40 Eridani B and 40 Eridani C, are a 9th magnitude white dwarf (spectral type DA4) and an 11th magnitude red dwarf flare star (spectral type M4.5e) which has the variable star designation DY Eridani. Presumably, while B was a main-sequence star, it was the most massive member of the system, but ejected most of its mass before it became a white dwarf. B and C orbit each other approximately 400 astronomical units from the primary star, A. Their orbit has a semimajor axis of 35 AU (which is also the approximate average distance between B and C) and is rather elliptical (eccentricity 0.410).\r\rAlthough 40 Eridani B is neither the closest white dwarf, nor the brightest in the night sky, it is by far the easiest to observe; it is nearly three magnitudes brighter than Van Maanen\u0027s Star (the nearest solitary white dwarf), and unlike the companions of Procyon and Sirius it is not swamped in the glare of a much brighter primary.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "40 Eridani, Omicron02 Eridani, HIP 19849, SAO 131063, HD 26965, GC 5138, HR 1325, DM BD-07   780, TYC 5312-2325-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Keid",
	"OType" : "Flare Star",
	"Distance" : "4.98",
	"RA_S" : 63.81799845,
	"DEC_S" : -7.65287232,
	"X" : 226,
	"Y" : 103,
	"Constellation" : "Eridanus ",
	"AMag" : 4.506,
	"key" : 55845,
	"shortTitle" : "Kied",
	"title" : "Keid"
	},
{
	"Index" : "48857",
	"Description" : "Upsilon4 Eridani (\u03C54 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 3.55.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "41 Eridani, Upsilon04 Eridani, HIP 20042, SAO 194902, HD 27376, GC 5201, HR 1347, DM CD-34  1614, TYC 7040-1534-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Upsilon4 Eridani",
	"OType" : "Spectroscopic binary",
	"Distance" : "54.55",
	"RA_S" : 64.47359336,
	"DEC_S" : -33.79834914,
	"X" : 269,
	"Y" : 412,
	"Constellation" : "Eridanus ",
	"AMag" : 3.516,
	"key" : 68857,
	"title" : "Upsilon4 Eridani"
	},
{
	"Index" : "40194",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 20264, SAO 169354, HD 27616, GC 5270, HR 1367, DM BD-20  831, TYC 5896-1722-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR 1367",
	"OType" : "Star",
	"Distance" : "145.46",
	"RA_S" : 65.16255516,
	"DEC_S" : -20.63962404,
	"Constellation" : "Eridanus ",
	"AMag" : 5.364,
	"key" : 60194,
	"title" : "HR 1367"
	},
{
	"Index" : "31520",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "42 Eridani, Xi Eridani, HIP 20507, SAO 131176, HD 27861, GC 5327, HR 1383, DM BD-04   818, TYC 4730-1947-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Xi Eridani",
	"OType" : "Star",
	"Distance" : "64.08",
	"RA_S" : 65.92021771,
	"DEC_S" : -3.74547168,
	"Constellation" : "Eridanus ",
	"AMag" : 5.175,
	"key" : 51520,
	"title" : "Xi Eridani"
	},
{
	"Index" : "48868",
	"Description" : "Upsilon3 Eridani (\u03C53 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 3.97.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "43 Eridani, d Eridani, HIP 20535, SAO 194984, HD 28028, GC 5349, HR 1393, DM CD-34  1664, TYC 7041-1605-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Upsilon3 Eridani",
	"OType" : "Star",
	"Distance" : "90.7",
	"RA_S" : 66.00923129,
	"DEC_S" : -34.01685264,
	"X" : 255,
	"Y" : 418,
	"Constellation" : "Eridanus ",
	"AMag" : 4.123,
	"key" : 68868,
	"title" : "Upsilon3 Eridani"
	},
{
	"Index" : "31553",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "45 Eridani, HIP 21139, SAO 131270, HD 28749, GC 5528, HR 1437, DM BD-00   713, TYC 4734-1338-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "45 Eridani",
	"OType" : "Star",
	"Distance" : "199.81",
	"RA_S" : 67.96944566,
	"Constellation" : "Eridanus ",
	"AMag" : 5.047,
	"key" : 51553,
	"title" : "45 Eridani"
	},
{
	"Index" : "44614",
	"Description" : "Upsilon1 Eridani (\u03C51 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.51.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "50 Eridani, Upsilon01 Eridani, HIP 21248, SAO 169570, HD 29085, GC 5572, HR 1453, DM CD-30  1883, TYC 6470-1242-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Upsilon1 Eridani",
	"OType" : "Variable Star",
	"Distance" : "38.95",
	"RA_S" : 68.37730394,
	"DEC_S" : -29.76648879,
	"X" : 221,
	"Y" : 374,
	"Constellation" : "Eridanus ",
	"AMag" : 4.612,
	"key" : 64614,
	"title" : "Upsilon1 Eridani"
	},
{
	"Index" : "35858",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "47 Eridani, HIP 21296, SAO 131315, HD 29064, GC 5576, HR 1451, DM BD-08   887, TYC 5314-3037-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "47 Eridani",
	"OType" : "Long Period Variable candidate",
	"Distance" : "302.6",
	"RA_S" : 68.54845342,
	"DEC_S" : -8.2313524,
	"Constellation" : "Eridanus ",
	"AMag" : 5.395,
	"key" : 55858,
	"title" : "47 Eridani"
	},
{
	"Index" : "35860",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 21297, SAO 131316, HD 29065, GC 5577, HR 1452, DM BD-09  930, TYC 5314-3039-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR 1452",
	"OType" : "Star",
	"Distance" : "230.81",
	"RA_S" : 68.54904522,
	"DEC_S" : -8.97025902,
	"Constellation" : "Eridanus ",
	"AMag" : 5.403,
	"key" : 55860,
	"title" : "HR 1452"
	},
{
	"Index" : "48840",
	"Description" : "Upsilon2 Eridani (Upsilon2 Eri, \u03C52 Eridani, \u03C52 Eri) is a G-type giant star in the constellation of Eridanus. It has an apparent visual magnitude of approximately 3.817 and is approximately 209 light-years from the Earth. It also has the names Theemim (also Theemin) and Beemin.\r\rIn Chinese, \u5929\u5712 (Ti\u0101n Yu\u00E1n), meaning Celestial Orchard, refers to an asterism consisting of \u03C52 Eridani, \u03C7 Eridani, \u03C6 Eridani, \u03BA Eridani, HD 16754, HD 23319, \u03B8 Eridani, HD 24072, HD 24160, \u03C54 Eridani, 43 Eridani and \u03C51 Eridani. Consequently, \u03C52 Eridani itself is known as \u5929\u5712\u5341\u4E8C (Ti\u0101n Yu\u00E1n sh\u00ED\u00E8r, English: the Twelfth Star of Celestial Orchard.)",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "52 Eridani, Upsilon02 Eridani, HIP 21393, SAO 195148, HD 29291, GC 5614, HR 1464, DM CD-30  1901, TYC 7038-1509-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Upsilon2 Eridani",
	"OType" : "Star",
	"Distance" : "65.56",
	"RA_S" : 68.88766298,
	"DEC_S" : -30.56233717,
	"X" : 218,
	"Y" : 385,
	"Constellation" : "Eridanus ",
	"AMag" : 3.908,
	"key" : 68840,
	"shortTitle" : "Beemin; Theemin",
	"title" : "Upsilon2 Eridani"
	},
{
	"Index" : "31579",
	"Description" : "Nu Eridani (\u03BD Eri) is a star in the constellation Eridanus. Its apparent magnitude is 3.92.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "48 Eridani, Nu Eridani, HIP 21444, SAO 131346, HD 29248, GC 5617, HR 1463, DM BD-03   834, TYC 4738-1484-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Nu Eridani",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "206.66",
	"RA_S" : 69.07975601,
	"DEC_S" : -3.35246019,
	"X" : 159,
	"Y" : 64,
	"Constellation" : "Eridanus ",
	"AMag" : 3.896,
	"key" : 51579,
	"title" : "Nu Eridani"
	},
{
	"Index" : "31585",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "51 Eridani, c Eridani, HIP 21547, SAO 131358, HD 29391, GC 5635, HR 1474, DM BD-02   963, TYC 4739-1551-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "c Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "29.43",
	"RA_S" : 69.40054879,
	"DEC_S" : -2.47354766,
	"Constellation" : "Eridanus ",
	"AMag" : 5.244,
	"key" : 51585,
	"title" : "c Eridani"
	},
{
	"Index" : "35991",
	"Description" : "53 Eridani (53 Eri) is a star in the constellation Eridanus. It has the traditional name Sceptrum (Latin \u0022scepter\u0022). 53 Eridani was one of the brighter stars, designated \u0022p Sceptri (Brandenburgici)\u0022, in the obsolete constellation Sceptrum Brandenburgicum.\r\r53 Eridani belongs to the spectral class K2IIIb and has apparent magnitude +3.87. It is approximately 109 light-years from Earth.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "53 Eridani, l Eridani, HIP 21594A, SAO 149781, HD 29503A, GC 5657, HR 1481, DM BD-14   933, TYC 5327-1434-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Sceptrum",
	"OType" : "High proper-motion Star",
	"Distance" : "33.68",
	"RA_S" : 69.54509942,
	"DEC_S" : -14.30397756,
	"X" : 172,
	"Y" : 195,
	"Constellation" : "Eridanus ",
	"AMag" : 4.023,
	"key" : 55991,
	"title" : "Sceptrum"
	},
{
	"Index" : "35992",
	"Description" : "53 Eridani (53 Eri) is a star in the constellation Eridanus. It has the traditional name Sceptrum (Latin \u0022scepter\u0022). 53 Eridani was one of the brighter stars, designated \u0022p Sceptri (Brandenburgici)\u0022, in the obsolete constellation Sceptrum Brandenburgicum.\r\r53 Eridani belongs to the spectral class K2IIIb and has apparent magnitude +3.87. It is approximately 109 light-years from Earth.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "53 Eridani, l Eridani, HIP 21594B, SAO 149781, HD 29503B, GC 5657, HR 1481, DM BD-14   933, TYC 5327-1434-2",
	"group" : { "key" : "Eridanus" },
	"Common" : "Sceptrum",
	"OType" : "High proper-motion Star",
	"Distance" : "33.68",
	"RA_S" : 69.54509942,
	"DEC_S" : -14.30397756,
	"X" : 172,
	"Y" : 195,
	"Constellation" : "Eridanus ",
	"AMag" : 6.952,
	"key" : 55992,
	"title" : "Sceptrum"
	},
{
	"Index" : "35958",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "HIP 21644AB, SAO 149789, HD 29573, GC 5669, HR 1483, DM BD-12  955, TYC 5324-1900-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "HR 1483",
	"OType" : "Double or multiple star",
	"Distance" : "71.2",
	"RA_S" : 69.72314822,
	"DEC_S" : -12.12312359,
	"Constellation" : "Eridanus ",
	"AMag" : 5.011,
	"key" : 55958,
	"title" : "HR 1483"
	},
{
	"Index" : "40187",
	"Description" : "54 Eridani (54 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.36.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "54 Eridani, HIP 21763, SAO 149818, HD 29755, GC 5695, HR 1496, DM BD-19   988, TYC 5895-1948-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "54 Eridani",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "112.37",
	"RA_S" : 70.11045293,
	"DEC_S" : -19.67148449,
	"X" : 177,
	"Y" : 260,
	"Constellation" : "Eridanus ",
	"AMag" : 4.528,
	"key" : 60187,
	"title" : "54 Eridani"
	},
{
	"Index" : "31591",
	"Description" : "Mu Eridani (\u03BC Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.00.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "57 Eridani, Mu Eridani, HIP 22109, SAO 131468, HD 30211, GC 5796, HR 1520, DM BD-03   876, TYC 4740-1916-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Mu Eridani",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "159.82",
	"RA_S" : 71.3756266,
	"DEC_S" : -3.25466015,
	"X" : 131,
	"Y" : 68,
	"Constellation" : "Eridanus ",
	"AMag" : 3.981,
	"key" : 51591,
	"title" : "Mu Eridani"
	},
{
	"Index" : "40221",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "60 Eridani, HIP 22479, SAO 149924, HD 30814, GC 5894, HR 1549, DM BD-16   964, TYC 5899-1192-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "60 Eridani",
	"OType" : "Red Giant Branch star",
	"Distance" : "72.27",
	"RA_S" : 72.54840153,
	"DEC_S" : -16.21715493,
	"Constellation" : "Eridanus ",
	"AMag" : 5.139,
	"key" : 60221,
	"title" : "60 Eridani"
	},
{
	"Index" : "31626",
	"Description" : "Omega Eridani (\u03C9 Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.40.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "61 Eridani, Omega Eridani, HIP 22701, SAO 131568, HD 31109, GC 5954, HR 1560, DM BD-05  1068, TYC 4745-1841-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Omega Eridani",
	"OType" : "Spectroscopic binary",
	"Distance" : "72.02",
	"RA_S" : 73.22362271,
	"DEC_S" : -5.45269885,
	"X" : 113,
	"Y" : 99,
	"Constellation" : "Eridanus ",
	"AMag" : 4.395,
	"key" : 51626,
	"title" : "Omega Eridani"
	},
{
	"Index" : "31625",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "62 Eridani, b Eridani, HIP 22958AC, SAO 131614, HD 31512, GC 6032, HR 1582, DM BD-05  1091, TYC 4745-1840-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "b Eridani",
	"OType" : "Double or multiple star",
	"Distance" : "221.82",
	"RA_S" : 74.10078188,
	"DEC_S" : -5.17135532,
	"Constellation" : "Eridanus ",
	"AMag" : 5.461,
	"key" : 51625,
	"title" : "b Eridani"
	},
{
	"Index" : "35980",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "63 Eridani, HIP 23221, SAO 150060, HD 32008, GC 6098, HR 1608, DM BD-10  1066, TYC 5326-1952-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "63 Eridani",
	"OType" : "Spectroscopic binary",
	"Distance" : "53.83",
	"RA_S" : 74.96022522,
	"DEC_S" : -10.26331972,
	"Constellation" : "Eridanus ",
	"AMag" : 5.478,
	"key" : 55980,
	"title" : "63 Eridani"
	},
{
	"Index" : "36013",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "64 Eridani, S Eridani, HIP 23231, SAO 150064, HD 32045, GC 6104, HR 1611, DM BD-12  1047, TYC 5329-2016-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "S Eridani",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "88.92",
	"RA_S" : 74.9822378,
	"DEC_S" : -12.53741696,
	"Constellation" : "Eridanus ",
	"AMag" : 4.804,
	"key" : 56013,
	"title" : "S Eridani"
	},
{
	"Index" : "31782",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "65 Eridani, Psi Eridani, HIP 23364, SAO 131700, HD 32249, GC 6138, HR 1617, DM BD-07   948, TYC 4762-1492-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Psi Eridani",
	"OType" : "Star",
	"Distance" : "226.02",
	"RA_S" : 75.35976715,
	"DEC_S" : -7.17396699,
	"Constellation" : "Eridanus ",
	"AMag" : 4.752,
	"key" : 51782,
	"title" : "Psi Eridani"
	},
{
	"Index" : "31748",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "66 Eridani, HIP 23794, SAO 131777, HD 32964, GC 6246, HR 1657, DM BD-04  1044, TYC 4758-1506-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "66 Eridani",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "94.58",
	"RA_S" : 76.6902214,
	"DEC_S" : -4.65516497,
	"Constellation" : "Eridanus ",
	"AMag" : 5.088,
	"key" : 51748,
	"title" : "66 Eridani"
	},
{
	"Index" : "31756",
	"Description" : "Beta Eridani (Beta Eri, \u03B2 Eridani, \u03B2 Eri) is the second brightest star in the constellation of Eridanus, located in the northeast end of this constellation near the shared border with Orion. It has the traditional names Cursa. The apparent visual magnitude of this star is 2.796, so it can be viewed with the naked eye in dark skies. Parallax measurements yield an estimated distance of about 89 light-years (27 parsecs) from the Earth. \u03B2 Eridani has a spectral type of A3 III, with the III luminosity class indicating this is a giant star that has consumed the hydrogen at its core and evolved away from the main sequence. The effective temperature of the outer envelope is about 8,104 K, which gives the star a white hue typical of A-type stars. The projected rotational velocity is a rapid 196 km s\u20131, compared to 2 km s\u20131 along the Sun\u0027s equator. The star is known to vary in apparent visual magnitude, ranging between 2.72 and 2.80. A particularly strong flare up was reported in 1985.\r\rThe location and trajectory of this star suggest that it is a member of the Ursa Major supergroup, an association of stars that share a common origin and motion though space. However, its photometric properties indicate that it may instead be an interloper. Beta Eridani has an optical companion star with an apparent magnitude 10.90 at an angular separation of 120 arcseconds and a position angle of 148\u00B0. It has the catalogue identifier CCDM J05079-0506B.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "67 Eridani, Beta Eridani, HIP 23875, SAO 131794, HD 33111, GC 6274, HR 1666, DM BD-05  1162, TYC 4759-1671-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Beta Eridani",
	"OType" : "High proper-motion Star",
	"Distance" : "27.39",
	"RA_S" : 76.96243955,
	"DEC_S" : -5.08644597,
	"X" : 68,
	"Y" : 105,
	"Constellation" : "Eridanus ",
	"AMag" : 2.779,
	"key" : 51756,
	"shortTitle" : "Dhalim; Kursa",
	"title" : "Beta Eridani"
	},
{
	"Index" : "31755",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "68 Eridani, HIP 23941, SAO 131813, HD 33256, GC 6292, HR 1673, DM BD-04  1056, TYC 4759-1670-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "68 Eridani",
	"OType" : "Star",
	"Distance" : "25.46",
	"RA_S" : 77.18207545,
	"DEC_S" : -4.45621143,
	"Constellation" : "Eridanus ",
	"AMag" : 5.17,
	"key" : 51755,
	"title" : "68 Eridani"
	},
{
	"Index" : "36030",
	"Description" : "Lambda Eridani (\u03BB Eri) is a star in the constellation Eridanus. Its apparent magnitude is 4.25.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "69 Eridani, Lambda Eridani, HIP 23972, SAO 131824, HD 33328, GC 6304, HR 1679, DM BD-08  1040, TYC 5330-1723-1",
	"group" : { "key" : "Eridanus" },
	"Common" : "Lamda Eridani",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "248.16",
	"RA_S" : 77.28659901,
	"DEC_S" : -8.75408248,
	"X" : 71,
	"Y" : 150,
	"Constellation" : "Eridanus ",
	"AMag" : 4.211,
	"key" : 56030,
	"title" : "Lamda Eridani"
	},
{
	"Index" : "48543",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Pi Fornacis, HIP 9440, SAO 193455, HD 12438, GC 2443, HR 594, DM CD-30   703, TYC 7006-2299-1",
	"group" : { "backgroundImage" : "images/Alignment/25.png",
		"description" : "Fornax (pron.: /\u02C8f\u0254rn\u00E6ks/) is a constellation in the southern sky. Its name is Latin for furnace. It was named by French astronomer Nicolas Louis de Lacaille in 1756. Fornax is one of the 88 modern constellations.\r\rde Lacaille originally called the constellation \u0022Fornax Chemica\u0022 (the chemical furnace), representing a small solid fuel vessel used for heating chemical experiments.",
		"key" : "Fornax",
		"grouptype" : "Fornax",
		"Meaning" : "chemical furnace",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Fornax",
		"title" : "Fornax Objects Group" },
	"Common" : "Pi Fornacis",
	"OType" : "Star",
	"Distance" : "90.18",
	"RA_S" : 30.31134285,
	"DEC_S" : -30.00183186,
	"Constellation" : "Fornax ",
	"AMag" : 5.445,
	"key" : 68543,
	"title" : "Pi Fornacis"
	},
{
	"Index" : "44277",
	"Description" : "Nu Fornacis (\u03BD For) is a type B5V star in the constellation Fornax 371 ly from here that shines with an apparent magnitude of 4.68.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Nu Fornacis, HIP 9677, SAO 167532, HD 12767, GC 2506, HR 612, DM CD-29   706, TYC 6432-2329-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Nu Fornacis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "113.65",
	"RA_S" : 31.1226565,
	"DEC_S" : -29.29682018,
	"X" : 597,
	"Y" : 344,
	"Constellation" : "Fornax ",
	"AMag" : 4.659,
	"key" : 64277,
	"title" : "Nu Fornacis"
	},
{
	"Index" : "48558",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Mu Fornacis, HIP 10320, SAO 193573, HD 13709, GC 2663, HR 652, DM CD-31   882, TYC 7007-2243-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Mu Fornacis",
	"OType" : "Star",
	"Distance" : "98.17",
	"RA_S" : 33.22695751,
	"DEC_S" : -30.72382563,
	"Constellation" : "Fornax ",
	"AMag" : 5.257,
	"key" : 68558,
	"title" : "Mu Fornacis"
	},
{
	"Index" : "44296",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Kappa Fornacis, HIP 11072, SAO 167736, HD 14802, GC 2862, HR 695, DM CD-24  1038, TYC 6433-2550-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Kappa Fornacis",
	"OType" : "Double or multiple star",
	"Distance" : "21.95",
	"RA_S" : 35.63561004,
	"DEC_S" : -23.81632753,
	"Constellation" : "Fornax ",
	"AMag" : 5.267,
	"key" : 64296,
	"title" : "Kappa Fornacis"
	},
{
	"Index" : "48624",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Phi Fornacis, HIP 11477, SAO 193723, HD 15427, GC 2967, HR 724, DM CD-34   905, TYC 7013-1037-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Phi Fornacis",
	"OType" : "Star",
	"Distance" : "46.59",
	"RA_S" : 37.00709623,
	"DEC_S" : -33.81103858,
	"Constellation" : "Fornax ",
	"AMag" : 5.135,
	"key" : 68624,
	"title" : "Phi Fornacis"
	},
{
	"Index" : "44347",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Omega Fornacis, HIP 11918A, TYC 6436-2246-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Omega Fornacis",
	"OType" : "Star",
	"Distance" : "146.42",
	"RA_S" : 38.46129103,
	"DEC_S" : -28.23234541,
	"Constellation" : "Fornax ",
	"AMag" : 4.95,
	"key" : 64347,
	"title" : "Omega Fornacis"
	},
{
	"Index" : "48611",
	"Description" : "Beta Fornacis (Beta For, \u03B2 Fornacis, \u03B2 For) is a G-type giant star in the constellation of Fornax. It has an apparent visual magnitude of approximately 4.465.\r\r\u03B2 Fornacis has a visual companion, CCDM J02491-3224B, which has an apparent visual magnitude of approximately 14.0.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Beta Fornacis, HIP 13147, SAO 193931, HD 17652, GC 3387, HR 841, DM CD-32  1025, TYC 7012-1019-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Beta Fornacis",
	"OType" : "Red Giant Branch star",
	"Distance" : "52.93",
	"RA_S" : 42.27257987,
	"DEC_S" : -32.40589655,
	"X" : 484,
	"Y" : 374,
	"Constellation" : "Fornax ",
	"AMag" : 4.565,
	"key" : 68611,
	"title" : "Beta Fornacis"
	},
{
	"Index" : "44407",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Gamma02 Fornacis, HIP 13202, SAO 168082, HD 17729, GC 3405, HR 845, DM CD-28   903, TYC 6443-914-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Gamma02 Fornacis",
	"OType" : "Star",
	"Distance" : "140.39",
	"RA_S" : 42.47576006,
	"DEC_S" : -27.94198354,
	"Constellation" : "Fornax ",
	"AMag" : 5.378,
	"key" : 64407,
	"title" : "Gamma02 Fornacis"
	},
{
	"Index" : "44428",
	"Description" : "Alpha Fornacis (\u03B1 Fornacis, \u03B1 For) is the brightest star in the constellation Fornax, its only star brighter than magnitude 4.0. It has the proper names Dalim (in Piazzi\u0027s Palermo Catalogue) and Fornacis (in Burritt\u0027s Atlas). This star was formally identical with 12 Eridani.\r\rThe stellar classification of Alpha Fornacis is F8IV, where the luminosity class IV indicates this is a subgiant star that has just evolved off the main sequence. It has 33% more mass than the Sun and is an estimated 2.9 billion years old. Alpha Fornacis is a binary star and has a high proper motion. This system displays an excess of infrared emission, which may indicate the presence of circumstellar material such as a debris disk.\r\rThe space velocity components of this star are (U, V, W) = (\u201335, +20, +30) km/s. Approximately 350,000 years ago, Alpha Fornacis experienced a close encounter with the A-type main sequence star HD 17848. The two came within an estimated 0.265 ly (0.081 pc) of each other.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Alpha Fornacis, HIP 14879B, SAO 168373, HD 20010B, GC 3831, HR 963, DM CD-29  1177, TYC 6445-990-2",
	"group" : { "key" : "Fornax" },
	"Common" : "Alpha Fornacis",
	"OType" : "High proper-motion Star",
	"Distance" : "14.24",
	"RA_S" : 48.017546,
	"DEC_S" : -28.986944,
	"X" : 425,
	"Y" : 335,
	"Constellation" : "Fornax ",
	"AMag" : 7.192,
	"key" : 64428,
	"title" : "Alpha Fornacis"
	},
{
	"Index" : "44427",
	"Description" : "Alpha Fornacis (\u03B1 Fornacis, \u03B1 For) is the brightest star in the constellation Fornax, its only star brighter than magnitude 4.0. It has the proper names Dalim (in Piazzi\u0027s Palermo Catalogue) and Fornacis (in Burritt\u0027s Atlas). This star was formally identical with 12 Eridani.\r\rThe stellar classification of Alpha Fornacis is F8IV, where the luminosity class IV indicates this is a subgiant star that has just evolved off the main sequence. It has 33% more mass than the Sun and is an estimated 2.9 billion years old. Alpha Fornacis is a binary star and has a high proper motion. This system displays an excess of infrared emission, which may indicate the presence of circumstellar material such as a debris disk.\r\rThe space velocity components of this star are (U, V, W) = (\u201335, +20, +30) km/s. Approximately 350,000 years ago, Alpha Fornacis experienced a close encounter with the A-type main sequence star HD 17848. The two came within an estimated 0.265 ly (0.081 pc) of each other.",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Alpha Fornacis, HIP 14879A, SAO 168373, HD 20010A, GC 3831, HR 963, DM CD-29  1177, TYC 6445-990-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Alpha Fornacis",
	"OType" : "High proper-motion Star",
	"Distance" : "14.24",
	"RA_S" : 48.017892,
	"DEC_S" : -28.989006,
	"X" : 425,
	"Y" : 335,
	"Constellation" : "Fornax ",
	"AMag" : 3.976,
	"key" : 64427,
	"title" : "Alpha Fornacis"
	},
{
	"Index" : "48757",
	"MapNum" : "25",
	"ImageNum" : "25",
	"Desig" : "Delta Fornacis, HIP 17304, SAO 194467, HD 23227, GC 4439, HR 1134, DM CD-32  1430, TYC 7028-1395-1",
	"group" : { "key" : "Fornax" },
	"Common" : "Delta Fornacis",
	"OType" : "Star",
	"Distance" : "258.43",
	"RA_S" : 55.56209208,
	"DEC_S" : -31.93836125,
	"Constellation" : "Fornax ",
	"AMag" : 4.947,
	"key" : 68757,
	"title" : "Delta Fornacis"
	},
{
	"Index" : "7114",
	"Description" : "1 Geminorum (1 Gem) is a star in the constellation Gemini. Its apparent magnitude is 4.15.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "1 Geminorum, HIP 28734AB, SAO 77915, HD 41116, GC 7676, HR 2134, DM BD+23  1170, TYC 1864-2011-1",
	"group" : { "backgroundImage" : "images/Alignment/08.png",
		"description" : "Gemini is one of the constellations of the zodiac. It was one of the 48 constellations described by the 2nd century AD astronomer Ptolemy and it remains one of the 88 modern constellations today. Its name is Latin for \u0022twins,\u0022 and it is associated with the twins Castor and Pollux in Greek mythology. Its symbol is \u264A.\r\rGemini lies between Taurus to the west and Cancer to the east, with Auriga and Lynx to the north and Monoceros and Canis Minor to the south.\r\rThe Sun resides in the astrological sign of Gemini from May 21st to June 20th each year. By mid August, Gemini will appear along the eastern horizon in the morning sky prior to sunrise. The best time to observe Gemini at night is overhead during the months of January and February. By April and May, the constellation will be visible soon after sunset in the west.\r\rThe easiest way to locate the constellation is to find its two brightest stars Castor and Pollux eastward from the familiar \u0022V\u0022 shaped asterism of Taurus and the three stars of Orion\u0027s belt. Another way is to mentally draw a line from the Pleiades star cluster located in Taurus and the brightest star in Leo, Regulus. In doing so, you are drawing an imaginary line that is relatively close to the ecliptic, a line which intersects Gemini roughly at the midpoint of the constellation, just below Castor and Pollux.\r\rIn Babylonian astronomy, the stars Castor and Pollux were known as the Great Twins (MUL.MASH.TAB.BA.GAL.GAL). The Twins were regarded as minor gods and were called Meshlamtaea and Lugalirra, meaning respectively \u0027The One who has arisen from the Underworld\u0027 and the \u0027Mighty King\u0027. Both names can be understood as titles of Nergal, the major Babylonian god of plague and pestilence, who was king of the Underworld.\r\rIn Greek mythology, Gemini was associated with the myth of Castor and Pollux, the children of Leda and Argonauts both. Pollux was the son of Zeus, who seduced Leda, while Castor was the son of Tyndareus, king of Sparta and Leda\u0027s husband. Castor and Pollux were also mythologically associated with St. Elmo\u0027s fire in their role as the protectors of sailors. When Castor died, because he was mortal, Pollux begged his father Zeus to give Castor immortality, and he did, by uniting them together in the heavens.\r\rThe constellation contains 85 stars visible to observation on Earth without a telescope.\r\rGemini is dominated by Castor and Pollux, two bright stars that appear relatively close together, encouraging the mythological link between the constellation and twinship. The twin above and to the right (as seem from the Northern Hemisphere) is Castor, whose brightest star is \u03B1 Geminorum (more commonly called Castor); it is a second magnitude star and represents Castor\u0027s head. The twin below and to the left is Pollux, whose brightest star is \u03B2 Geminorum (more commonly called Pollux); it is of the first magnitude and represents Pollux\u0027s head. Furthermore, the other stars can be visualized as two parallel lines descending from the two main stars, making it look like two figures.\r\rH.A. Rey has suggested an alternative to the traditional visualization that connected the stars of Gemini to show twins holding hands. Pollux\u0027s torso is represented by the star \u03C5 Geminorum, Pollux\u0027s right hand by \u03B9 Geminorum, Pollux\u0027s left hand by \u03BA Geminorum; all three of these stars are of the fourth magnitude. Pollux\u0027s pelvis is represented by the star \u03B4 Geminorum, Pollux\u0027s right knee by \u03B6 Geminorum, Pollux\u0027s right foot by \u03B3 Geminorum, Pollux\u0027s left knee by \u03BB Geminorum, and Pollux\u0027s left foot by \u03BE Geminorum. Gamma Geminorum is of the second magnitude, while Delta and Xi Geminorum are of the third magnitude. Castor\u0027s torso is represented by the star \u03C4 Geminorum, Castor\u0027s left hand by \u03B9 Geminorum (which he shares with Pollux), Castor\u0027s right hand by \u03B8 Geminorum; all three of these stars are of the fourth magnitude. Castor\u0027s pelvis is represented by the star \u03B5 Geminorum, Castor\u0027s left foot by \u03BD Geminorum, and Castor\u0027s right foot by \u03BC Geminorum and \u03B7 Geminorum; \u03B5, \u03BC, and \u03B7 Geminorum are of the third magnitude. The brightest star in this constellation is Pollux.\r\rIn Meteorologica (1 343b30) Aristotle mentions that he observed Jupiter in conjunction with and then occulting a star in Gemini. This is the earliest known observation of this nature. A study published in 1990 suggests the star involved was 1 Geminorum and the event took place on 5 December 337 BC.\r\rWhen William Herschel discovered Uranus on 13 March 1781 it was located near Eta Geminorum. In 1930 Clyde Tombaugh exposed a series of photographic plates centred on Delta Geminorum and discovered Pluto.",
		"key" : "Gemini",
		"grouptype" : "Gemini",
		"Meaning" : "twins",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Gemini",
		"title" : "Gemini Objects Group" },
	"Common" : "1 Geminorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.45",
	"RA_S" : 91.03006433,
	"DEC_S" : 23.26334447,
	"X" : 410,
	"Y" : 448,
	"Constellation" : "Gemini ",
	"AMag" : 4.261,
	"key" : 27114,
	"title" : "1 Geminorum"
	},
{
	"Index" : "7266",
	"Description" : "Eta Geminorum (\u03B7 Gem, \u03B7 Geminorum) is a triple star system in the constellation Gemini. It has the traditional names Tejat Prior, Propus and Praepes and Pish Pai (from the Persian P\u012Bshp\u0101y, \u067E\u06CC\u0634\u067E\u0627\u06CC, meaning foreleg).\r\rThis star, along with \u03B3 Gem (Alhena), \u03BC Gem (Tejat Posterior), \u03BD Gem and \u03BE Gem (Alzirr) were Al Han\u0027ah, \u0022the brand\u0022 (on the neck of the camel). They also were associated in Al Nu\u1E25\u0101tai, the dual form of Al Nu\u1E25\u0101t, \u0022a Camel\u0027s Hump\u0022.\r\rIn Chinese astronomy, Tejat Prior is called \u94BA, Pinyin: Yu\u00E8, meaning Battle Axe, because this star is marking itself and stand alone in Battle Axe asterism, Well mansion. (see : Chinese constellation)\r\rEta Geminorum A is a spectroscopic binary. The primary is a semiregular variable star of type SRA whose brightness changes with a period of 234 days between magnitude +3.15 and +3.9. It is located 350 light years from the Sun and is a red giant of the spectral type M3. The secondary, probably a class B, orbits with a period of 8.2 years. Eta Geminorum B, a class G dwarf, orbits the pair with a period of at least 700 years.,\r\rEta Geminorum is near the ecliptic, so it can be occulted by the Moon and, very rarely, by planets. The last occultation by a planet took place on July 27, 1910, by Venus, and the next to last on July 11, 1837, by Mercury.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "7 Geminorum, Eta Geminorum, HIP 29655B, SAO 78135, HD 42995B, GC 7969, HR 2216, DM BD+22  1241, TYC 1877-1716-2",
	"group" : { "key" : "Gemini" },
	"Common" : "Tejat Prior / Propus / Praepes / Pish Pai",
	"OType" : "Star",
	"Distance" : "115.02",
	"RA_S" : 93.719038,
	"DEC_S" : 22.506753,
	"X" : 377,
	"Y" : 457,
	"Constellation" : "Gemini ",
	"AMag" : 6.154,
	"key" : 27266,
	"shortTitle" : "Propus (also HD41116,58207); Praepes; Teyat Prior; Prop",
	"title" : "Tejat Prior / Propus / Praepes / Pish Pai"
	},
{
	"Index" : "7265",
	"Description" : "Eta Geminorum (\u03B7 Gem, \u03B7 Geminorum) is a triple star system in the constellation Gemini. It has the traditional names Tejat Prior, Propus and Praepes and Pish Pai (from the Persian P\u012Bshp\u0101y, \u067E\u06CC\u0634\u067E\u0627\u06CC, meaning foreleg).\r\rThis star, along with \u03B3 Gem (Alhena), \u03BC Gem (Tejat Posterior), \u03BD Gem and \u03BE Gem (Alzirr) were Al Han\u0027ah, \u0022the brand\u0022 (on the neck of the camel). They also were associated in Al Nu\u1E25\u0101tai, the dual form of Al Nu\u1E25\u0101t, \u0022a Camel\u0027s Hump\u0022.\r\rIn Chinese astronomy, Tejat Prior is called \u94BA, Pinyin: Yu\u00E8, meaning Battle Axe, because this star is marking itself and stand alone in Battle Axe asterism, Well mansion. (see : Chinese constellation)\r\rEta Geminorum A is a spectroscopic binary. The primary is a semiregular variable star of type SRA whose brightness changes with a period of 234 days between magnitude +3.15 and +3.9. It is located 350 light years from the Sun and is a red giant of the spectral type M3. The secondary, probably a class B, orbits with a period of 8.2 years. Eta Geminorum B, a class G dwarf, orbits the pair with a period of at least 700 years.,\r\rEta Geminorum is near the ecliptic, so it can be occulted by the Moon and, very rarely, by planets. The last occultation by a planet took place on July 27, 1910, by Venus, and the next to last on July 11, 1837, by Mercury.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "7 Geminorum, Eta Geminorum, HIP 29655A, SAO 78135, HD 42995A, GC 7969, HR 2216, DM BD+22  1241, TYC 1877-1716-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Tejat Prior / Propus / Praepes / Pish Pai",
	"OType" : "Star",
	"Distance" : "115.02",
	"RA_S" : 93.719562,
	"DEC_S" : 22.506822,
	"X" : 377,
	"Y" : 457,
	"Constellation" : "Gemini ",
	"AMag" : 3.519,
	"key" : 27265,
	"shortTitle" : "Propus (also HD41116,58207); Praepes; Teyat Prior; Prop",
	"title" : "Tejat Prior / Propus / Praepes / Pish Pai"
	},
{
	"Index" : "7276",
	"Description" : "Mu Geminorum (\u03BC Gem, \u03BC Geminorum) is the Bayer designation for a star in the northern constellation of Gemini. It has the traditional name Tejat Posterior, which means back foot, because it is the foot of Castor, one of the Gemini twins. This name was formerly applied to an asterism consisting of this star, along with \u03B3 Gem (Alhena), \u03BD Gem, \u03B7 Gem (Tejat Prior), and \u03BE Gem (Alzirr). The names Calx (Latin, meaning heel), Pish Pai (from the Persian P\u012Bshp\u0101y, \u067E\u06CC\u0634\u067E\u0627\u06CC, meaning foreleg), and Nuhatai (from Arabic Al Nu\u1E25\u0101tai, the dual form of Al Nu\u1E25\u0101t, \u0022a Camel\u0027s Hump\u0022) have also been applied to Mu Geminorum.\r\rIn Chinese, \u4E95\u5BBF (J\u01D0ng Su), meaning Well (asterism), refers to an asterism consisting of \u03BC Geminorum, \u03B3 Geminorum, \u03BD Geminorum, \u03BE Geminorum, \u03B5 Geminorum, 36 Geminorum, \u03B6 Geminorum and \u03BB Geminorum. Consequently, \u03BC Geminorum itself is known as \u4E95\u5BBF\u4E00 (J\u01D0ng Su y\u012B, English: the First Star of Well.)\r\rMu Geminorum has an average apparent visual magnitude of 2.9, which makes it the fourth brightest member of Gemini. From parallax measurements made during the Hipparcos mission, the distance to this star is roughly 230 light-years (71 parsecs). Its visual magnitude is diminished by 0.07 as a result of extinction from intervening gas and dust.\r\rThis star is a slow irregular variable of type LB. Its brightness varies between magnitude +2.75 and +3.02 over a 72 day period, along with a 2,000 day period of long term variation. It is a red giant at a stellar classification of M3 III, with a surface temperature of 3,773 K, meaning it is brighter, yet cooler than our Sun. The star is currently on the asymptotic giant branch and is generating energy through the nuclear fusion of hydrogen and helium along concentric shells surrounding an inert core of carbon and oxygen.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "13 Geminorum, Mu Geminorum, HIP 30343, SAO 78297, HD 44478, GC 8208, HR 2286, DM BD+22  1304, TYC 1878-1429-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Tejat Posterior",
	"OType" : "Long-period variable star",
	"Distance" : "70.81",
	"RA_S" : 95.74011193,
	"DEC_S" : 22.51358275,
	"X" : 352,
	"Y" : 456,
	"Constellation" : "Gemini ",
	"AMag" : 3.064,
	"key" : 27276,
	"shortTitle" : "Calx; Pish Pai; Teyat Posterior; Dirakh",
	"title" : "Tejat Posterior"
	},
{
	"Index" : "2744",
	"Description" : "Nu Geminorum (\u03BD Gem) is a star in the constellation Gemini. Its apparent magnitude is 4.14.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "18 Geminorum, Nu Geminorum, HIP 30883, SAO 78423, HD 45542, GC 8394, HR 2343, DM BD+20  1441, TYC 1336-1812-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Nu Geminorum",
	"OType" : "Be Star",
	"Distance" : "166.51",
	"RA_S" : 97.24078288,
	"DEC_S" : 20.2121344,
	"X" : 332,
	"Y" : 485,
	"Constellation" : "Gemini ",
	"AMag" : 4.102,
	"key" : 22744,
	"title" : "Nu Geminorum"
	},
{
	"Index" : "2724",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "26 Geminorum, HIP 32104, SAO 96015, HD 48097, GC 8755, HR 2466, DM BD+17  1357, TYC 1334-2419-1",
	"group" : { "key" : "Gemini" },
	"Common" : "26 Geminorum",
	"OType" : "Star",
	"Distance" : "43.59",
	"RA_S" : 100.60136359,
	"DEC_S" : 17.64530612,
	"Constellation" : "Gemini ",
	"AMag" : 5.225,
	"key" : 22724,
	"title" : "26 Geminorum"
	},
{
	"Index" : "7453",
	"Description" : "Epsilon Geminorum (\u03B5 Gem, \u03B5 Geminorum) is a star in the constellation of Gemini. It has the traditional name Mebsuta (also Melboula or Melucta). Epsilon Geminorum is located on the outstretched right \u0022leg\u0022 of the twin Castor. The apparent visual magnitude of +3.06 makes it one of the brighter stars in this constellation.\r\rThe distance to this star can be determined directly using parallax measurements, yielding a value of 840 light-years (260 parsecs), although this result has a relatively large margin of error of 40 ly (12 pc). Because Epsilon Geminorum is located near the ecliptic it can be occulted by the Moon or a planet. Just such an occultation took place on April 8, 1976 by Mars, which allowed the oblateness of the planet\u0027s outer atmosphere to be measured. Prior to that, the star was occulted by Mercury on June 10, 1940.\r\rThe spectrum of this star matches a stellar classification of G8 Ib, where the luminosity class of Ib indicates this is a lower luminosity supergiant star. Alternatively, it may be a star that has passed through the asymptotic giant branch stage and possesses a detached shell of dust. The estimated mass of this star is over 19 times the mass of the Sun, and it has expanded to a radius measured at around 105\u2013175 times that of the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.\r\rEpsilon Geminorum is radiating around 8,500 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,662 K. It is this temperature that gives it the yellow-hued glow of a G-type star. A surface magnetic field with a strength of \u20130.14 \u00B1 0.19 G has been detected on this star. This topologically complex field is most likely generated by a dynamo formed from the deep convection zone in the star\u0027s outer envelope.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "27 Geminorum, Epsilon Geminorum, HIP 32246, SAO 78682, HD 48329, GC 8786, HR 2473, DM BD+25  1406, TYC 1897-1639-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Mebsuta",
	"OType" : "Variable Star",
	"Distance" : "258.47",
	"RA_S" : 100.98302446,
	"DEC_S" : 25.13112434,
	"X" : 291,
	"Y" : 417,
	"Constellation" : "Gemini ",
	"AMag" : 3.138,
	"key" : 27453,
	"shortTitle" : "Melucta; Meboula",
	"title" : "Mebsuta"
	},
{
	"Index" : "53458",
	"Description" : "30 Geminorum (30 Gem) is a star in the constellation Gemini. Its apparent magnitude is 4.50.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "30 Geminorum, HIP 32249, SAO 96051, HD 48433, GC 8793, HR 2478, DM BD+13  1390, TYC 758-2357-1",
	"group" : { "key" : "Gemini" },
	"Common" : "30 Geminorum",
	"OType" : "High proper-motion Star",
	"Distance" : "88.53",
	"RA_S" : 100.9970525,
	"DEC_S" : 13.22800619,
	"X" : 278,
	"Y" : 571,
	"Constellation" : "Gemini ",
	"AMag" : 4.618,
	"key" : 73458,
	"title" : "30 Geminorum"
	},
{
	"Index" : "53142",
	"Description" : "Xi Geminorum (\u03BE Gem) is a star in the zodiac constellation Gemini with the traditional name Alzirr. It forms one of the four feet of the outline demarcating the Gemini twins. The star has an apparent visual magnitude of 3.35, which is bright enough for it to be seen with the naked eye. From parallax measurements, its distance from the Earth can be estimated as 58.7 light-years (18.0 parsecs).\r\rAlzirr has a stellar classification of F5 IV, which is subgiant star that is in the process of evolving away from the main sequence of stars like the Sun. It has about 162% of the Sun\u0027s mass and is radiating more than 11 times the luminosity of the Sun. This energy is being emitted from the outer envelope of the star at an effective temperature of 6,464 K. This causes the star to take on the yellow-white hue common to F-type stars.\r\rX-ray emission has been detected from this star, which has an estimated X-ray luminosity of 1.06 \u00D7 1029 erg s\u20131. It has the spectroscopic signature of a rapidly rotating star, with a projected rotational velocity of about 66 km s\u20131. Although generally considered a single star, there is some evidence that it may instead be a spectroscopic binary system consisting of two component stars of equal mass.\r\rThe proper name of Xi Geminorum is Alzirr, meaning \u0022the button\u0022 in Arabic. This star, along with \u03B3 Gem (Alhena), \u03BC Gem (Tejat Posterior), \u03BD Gem and \u03B7 Gem (Tejat Prior) were Al Han\u0027ah, \u0022the brand\u0022 (on the neck of the camel). They also were associated in Al Nu\u1E25\u0101tai, the dual form of Al Nu\u1E25\u0101t, \u0022a Camel\u0027s Hump\u0022.\r\rIn Chinese, \u4E95\u5BBF (J\u01D0ng Su), meaning Well (asterism), refers to an asterism consisting of \u03BE Geminorum, \u03BC Geminorum, \u03BD Geminorum, \u03B3 Geminorum, \u03B5 Geminorum, 36 Geminorum, \u03B6 Geminorum and \u03BB Geminorum. Consequently, \u03BE Geminorum itself is known as \u4E95\u5BBF\u56DB (J\u01D0ng Su s\u00EC, English: the Fourth Star of Well.)",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "31 Geminorum, Xi Geminorum, HIP 32362, SAO 96074, HD 48737, GC 8823, HR 2484, DM BD+13  1396, TYC 754-2356-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Alzirr",
	"OType" : "Variable Star",
	"Distance" : "18",
	"RA_S" : 101.32235246,
	"DEC_S" : 12.89558957,
	"X" : 273,
	"Y" : 575,
	"Constellation" : "Gemini ",
	"AMag" : 3.377,
	"key" : 73142,
	"title" : "Alzirr"
	},
{
	"Index" : "2816",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "36 Geminorum, d Geminorum, HIP 32921, SAO 78805, HD 49908, GC 8965, HR 2529, DM BD+21  1405, TYC 1343-2919-1",
	"group" : { "key" : "Gemini" },
	"Common" : "d Geminorum",
	"OType" : "Star",
	"Distance" : "150.26",
	"RA_S" : 102.88768972,
	"DEC_S" : 21.7611431,
	"Constellation" : "Gemini ",
	"AMag" : 5.259,
	"key" : 22816,
	"title" : "d Geminorum"
	},
{
	"Index" : "11807",
	"Description" : "Theta Geminorum (\u03B8 Gem, \u03B8 Geminorum) is a Class A3, fourth-magnitude star in the constellation Gemini. Theta Geminorum is a binary star with components of magnitudes 3.60 and 5.18, separated by 2.9 arcseconds. This stellar system is located about 200 light-years from Earth.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "34 Geminorum, Theta Geminorum, HIP 33018, SAO 59570, HD 50019, GC 8989, HR 2540, DM BD+34  1481, TYC 2444-1113-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Theta Geminorum",
	"OType" : "Star",
	"Distance" : "57.96",
	"RA_S" : 103.19724379,
	"DEC_S" : 33.96125471,
	"X" : 280,
	"Y" : 299,
	"Constellation" : "Gemini ",
	"AMag" : 3.605,
	"key" : 31807,
	"title" : "Theta Geminorum"
	},
{
	"Index" : "53617",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "38 Geminorum, e Geminorum, HIP 33202A, SAO 96265, HD 50635A, GC 9049, HR 2564, DM BD+13  1462, TYC 760-2586-1",
	"group" : { "key" : "Gemini" },
	"Common" : "e Geminorum",
	"OType" : "Star",
	"Distance" : "27.91",
	"RA_S" : 103.66098164,
	"DEC_S" : 13.17782101,
	"Constellation" : "Gemini ",
	"AMag" : 4.751,
	"key" : 73617,
	"title" : "e Geminorum"
	},
{
	"Index" : "7441",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "42 Geminorum, Omega Geminorum, HIP 33927, SAO 78999, HD 52497, GC 9263, HR 2630, DM BD+24  1502, TYC 1895-2276-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Omega Geminorum",
	"OType" : "Cepheid variable Star",
	"Distance" : "449.03",
	"RA_S" : 105.60325314,
	"DEC_S" : 24.21544539,
	"Constellation" : "Gemini ",
	"AMag" : 5.287,
	"key" : 27441,
	"title" : "Omega Geminorum"
	},
{
	"Index" : "53070",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "HIP 34033, SAO 96429, HD 52960, GC 9303, HR 2649, DM BD+11 1428, TYC 753-2754-1",
	"group" : { "key" : "Gemini" },
	"Common" : "HR 2649",
	"OType" : "Star",
	"Distance" : "181.54",
	"RA_S" : 105.90863731,
	"DEC_S" : 10.95181799,
	"Constellation" : "Gemini ",
	"AMag" : 5.278,
	"key" : 73070,
	"title" : "HR 2649"
	},
{
	"Index" : "2934",
	"Description" : "Zeta Geminorum (\u03B6 Gem, \u03B6 Geminorum) is the Bayer designation for a star in the zodiac constellation Gemini, on the outstretched left \u0027leg\u0027 of the twin Pollux. It has the traditional name Mekbuda, meaning the lion\u0027s folded paw. As a member of the category of variable stars known as classical Cepheids, it has a regular pulsation frequency that is determined by its mass. Because the mass allows the luminosity to be directly determined, the star serves as an important calibrator for the cosmic distance ladder.\r\rIn 1825, German astronomer Julius Schmidt discovered that this star varies in brightness with a period of about 10 days, although it had been suspected of variability as early as 1790. In 1899, American astronomer W. W. Campbell announced that Zeta Geminorum has a variable radial velocity. (This variation was independently discovered by Russian astronomer Aristarkh Belopolsky, published in 1901.) Based on his observations, Campbell later published orbital elements for the binary. However, he found that the curve departed from a keplerian orbit and even suggested that it was a triple star system in order to explain the irregularities. The periodic variation in radial velocity was subsequently explained as the result of radial pulsations that occur in a class of variable stars known as Cepheid variables\u2014named after Delta Cephei.\r\rThe periodicity of the star is itself variable, a trend first noted by German astronomer Paul Guthnick in 1920, who suspected that the period change was the result of an orbiting companion. In 1930, Danish astronomer Axel Nielsen suggested that the change was instead the result in a steady decrease of about 3.6 seconds per year in the period.\r\rThis star is a Classical Cepheid variable that undergoes regular, periodic variation in luminosity because of radial pulsations. In the V band, the apparent magnitude varies between a high of 3.68 and a low of 4.16 (with a mean of 3.93) over a period of 10.148 days. This period of variation is decreasing at the rate of 3.1 seconds per year, or 0.085 seconds per cycle. It has a nominal stellar classification of G0 Ibv, with the luminosity class of Ib indicating that this is an intermediate luminous supergiant. The \u0027v\u0027 suffix means that it has variable spectral features, with the actual classification changing between F7Ib and G3Ib over the course of a pulsation cycle. Likewise the effective temperature of the outer envelope varies between 5,780 K and 5,260 K, while the radius varies from 61 to 69 times the Sun\u0027s radius. On average, it is radiating about 2,900 times the luminosity of the Sun.\r\rThere is no evidence of a stellar companion to Zeta Geminorum. However, the star was recently discovered to belong to a star cluster. Delta Cephei, the prototypical classical Cepheid variables, is also a member of a star cluster. The Cepheid\u0027s cluster membership, along with recent Hubble Space Telescope and Hipparcos parallaxes, place strong constraints on the star\u0027s distance: 363 \u00B1 9(\u03C32) \u00B1 26(\u03C3) parsecs. Zeta Geminorum is thus an important calibrator for establishing the cosmic distance ladder.\r\rThis star has the traditional name Mekbuda, which comes from ancient Arabic where it and the star Mebsuta (Epsilon Geminorum) were the paws of a lion. Mekbuda comes from a phrase meaning the lion\u0027s folded paw. In Chinese, \u4E95\u5BBF (J\u01D0ng Su), meaning Well (asterism), refers to an asterism consisting of \u03B6 Geminorum, \u03BC Geminorum, \u03B3 Geminorum, \u03BD Geminorum, \u03BE Geminorum, \u03B5 Geminorum, 36 Geminorum and \u03BB Geminorum. Consequently, \u03B6 Geminorum itself is known as \u4E95\u5BBF\u4E03 (J\u01D0ng Su q\u012B, English: the Seventh Star of Well.)",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "43 Geminorum, Zeta Geminorum, HIP 34088, SAO 79031, HD 52973, GC 9313, HR 2650, DM BD+20  1687, TYC 1353-1550-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Mekbuda",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "413.98",
	"RA_S" : 106.02721351,
	"DEC_S" : 20.57029288,
	"X" : 224,
	"Y" : 467,
	"Constellation" : "Gemini ",
	"AMag" : 4.05,
	"key" : 22934,
	"title" : "Mekbuda"
	},
{
	"Index" : "11752",
	"Description" : "Tau Geminorum (\u03C4 Gem) is a star in the northern zodiac constellation of Gemini. It has the apparent visual magnitude of +4.42, making it visible to the naked eye under suitably good seeing conditions. This star is close enough to the Earth that its distance can be measured using the parallax technique, which yields a value of roughly 321 light-years (98 parsecs).\r\rIt is an evolved giant star of the spectral type K2 III, meaning it is probably fusing carbon and oxygen in its core to form iron and nickel. It has double the mass of the Sun and has expanded to 27 times the Sun\u0027s radius. Tau Geminorum is radiating 224 as much luminosity as the Sun from its expanded outer atmosphere at an effective temperature of 4,528 K, giving it the characteristic orange-hued glow of a K-type star. It appears to be rotating slowly with a projected rotational velocity of 5.8 km s\u20131.\r\rThis star has a brown dwarf companion Tau Geminorum b, whose mass is 18.1 Jupiter masses, and which was discovered in 2004 by Mitchell et al., who also discovered Nu Ophiuchi b at the same time. This brown dwarf takes 305 days or 0.84 years or 26.4 megaseconds to revolve around Tau Gem.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "46 Geminorum, Tau Geminorum, HIP 34693, SAO 59858, HD 54719, GC 9484, HR 2697, DM BD+30  1439, TYC 2438-1059-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Tau Geminorum",
	"OType" : "Double or multiple star",
	"Distance" : "98.35",
	"RA_S" : 107.78486986,
	"DEC_S" : 30.24516353,
	"X" : 222,
	"Y" : 339,
	"Constellation" : "Gemini ",
	"AMag" : 4.533,
	"key" : 31752,
	"title" : "Tau Geminorum"
	},
{
	"Index" : "2852",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "51 Geminorum, HIP 34909AD, SAO 96638, HD 55383, GC 9551, HR 2717, DM BD+16  1417, TYC 1346-1397-1",
	"group" : { "key" : "Gemini" },
	"Common" : "51 Geminorum",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "162.81",
	"RA_S" : 108.34280995,
	"DEC_S" : 16.15896481,
	"Constellation" : "Gemini ",
	"AMag" : 5.261,
	"key" : 22852,
	"title" : "51 Geminorum"
	},
{
	"Index" : "2851",
	"Description" : "Lambda Geminorum (\u03BB Gem, \u03BB Geminorum) is a Class A3, fourth-magnitude star in the constellation Gemini. Lambda Geminorum is a variable star located about 95 light-years from Earth. It has 2.8 times the radius of the Sun and is radiating 28 times the Sun\u0027s luminosity. It has 2.1 times the mass of the Sun and is around 800 million years old.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "54 Geminorum, Lambda Geminorum, HIP 35350, SAO 96746, HD 56537A, GC 9701, HR 2763, DM BD+16  1443, TYC 1346-1396-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Lambda Geminorum",
	"OType" : "Star",
	"Distance" : "30.93",
	"RA_S" : 109.52324564,
	"DEC_S" : 16.54038384,
	"X" : 172,
	"Y" : 512,
	"Constellation" : "Gemini ",
	"AMag" : 3.575,
	"key" : 22851,
	"title" : "Lambda Geminorum"
	},
{
	"Index" : "2993",
	"Description" : "Delta Geminorum (\u03B4 Gem, \u03B4 Geminorum) is a star in the constellation Gemini. It has the traditional name Wasat. The traditional name comes from the Arabic word for \u0022middle\u0022. It has an apparent visual magnitude of +3.53, allowing it to be seen with the naked eye. Wasat is only two-tenths of a degree south of the ecliptic, and therefore is occasionally occulted by the Moon and, more rarely, by a planet. The last occultation by a planet was by Saturn on June 30, 1857, and the next will be by Venus on August 12, 2420. In 1930, the dwarf planet Pluto was discovered about 0.5\u00B0 to the east of this star by American astronomer Clyde Tombaugh.\r\rIn Chinese, \u5929\u6A3D (Ti\u0101n Z\u016Bn), meaning Celestial Wine Cup, refers to an asterism consisting of \u03B4 Geminorum, 57 Geminorum and \u03C9 Geminorum. Consequently, \u03B4 Geminorum itself is known as \u5929\u6A3D\u4E8C (Ti\u0101n Z\u016Bn \u00E8r, English: the Second Star of Celestial Wine Cup.). From this Chinese name, the name Ta Tsun was appeared.\r\rDelta Geminorum is a subgiant star with the stellar classification F0 IV. It is about 60.5 light-years (18.5 parsecs) distant. This star has 1.57 times the mass of the Sun and is rotating rapidly with a projected rotational velocity of 129.7 km s\u20131. The estimated age is 1.6 billion years.\r\rWasat is a member of a triple star system. The inner components form a spectroscopic binary with a period of 6.1 years (2,238.7 days) and an orbital eccentricity of 0.3530. A cooler class K companion is not apparent to the naked eye but clearly visible in a small telescope. It orbits the inner pair with a period of 1,200 years and an eccentricity of 0.11. Although according to  its radial velocity is away from the Sun, it is actually approching the Solar System. In about 1.1 million years, it will make its closest approach at a separation of roughly 6.7 ly (2.1 pc).",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "55 Geminorum, Delta Geminorum, HIP 35550, SAO 79294, HD 56986, GC 9755, HR 2777, DM BD+22  1645, TYC 1359-2672-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Wasat",
	"OType" : "Star",
	"Distance" : "18.54",
	"RA_S" : 110.030788,
	"DEC_S" : 21.982339,
	"X" : 177,
	"Y" : 440,
	"Constellation" : "Gemini ",
	"AMag" : 3.559,
	"key" : 22993,
	"shortTitle" : "Wesat; Vasat; Vazad",
	"title" : "Wasat"
	},
{
	"Index" : "2951",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "56 Geminorum, HIP 35699, SAO 79328, HD 57423, GC 9808, HR 2795, DM BD+20  1775, TYC 1355-1288-1",
	"group" : { "key" : "Gemini" },
	"Common" : "56 Geminorum",
	"OType" : "Variable Star",
	"Distance" : "135.76",
	"RA_S" : 110.48692306,
	"DEC_S" : 20.44365905,
	"Constellation" : "Gemini ",
	"AMag" : 5.266,
	"key" : 22951,
	"title" : "56 Geminorum"
	},
{
	"Index" : "7584",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "57 Geminorum, A Geminorum, HIP 35846, SAO 79352, HD 57727, GC 9843, HR 2808, DM BD+25  1660, TYC 1913-2400-1",
	"group" : { "key" : "Gemini" },
	"Common" : "A Geminorum",
	"OType" : "Star",
	"Distance" : "48.71",
	"RA_S" : 110.86880153,
	"DEC_S" : 25.05053145,
	"Constellation" : "Gemini ",
	"AMag" : 5.123,
	"key" : 27584,
	"title" : "A Geminorum"
	},
{
	"Index" : "7623",
	"Description" : "Iota Geminorum (\u03B9 Gem, \u03B9 Geminorum) is a Class G9, fourth-magnitude star in the constellation Gemini. It is called by the proper name Propus, meaning \u0022forefoot\u0022 in Latin.\r\rIn Chinese, \u4E94\u8AF8\u4FAF (Wu Zh\u016B H\u00F3u), meaning Five Feudal Kings, refers to an asterism consisting of \u03B9 Geminorum, \u03B8 Geminorum, \u03C4 Geminorum, \u03C5 Geminorum and \u03C6 Geminorum. Consequently, \u03B9 Geminorum itself is known as \u4E94\u8AF8\u4FAF\u4E09 (Wu Zh\u016B H\u00F3u s\u0101n, English: the Third Star of Five Feudal Kings.).\r\rIota Geminorum is a variable star located about 325 light-years from Earth. It forms an unequal pair with 59 Geminorum (app. Mag. 5.77; Class F4III), which is more or less the same distance away.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "60 Geminorum, Iota Geminorum, HIP 36046, SAO 79374, HD 58207, GC 9897, HR 2821, DM BD+28  1385, TYC 1918-2339-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Propus",
	"OType" : "Double or multiple star",
	"Distance" : "36.9",
	"RA_S" : 111.43164963,
	"DEC_S" : 27.79808119,
	"X" : 176,
	"Y" : 362,
	"Constellation" : "Gemini ",
	"AMag" : 3.888,
	"key" : 27623,
	"title" : "Propus"
	},
{
	"Index" : "2994",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "63 Geminorum, HIP 36238A, SAO 79403, HD 58728, GC 9957, HR 2846, DM BD+21  1602, TYC 1359-2673-1",
	"group" : { "key" : "Gemini" },
	"Common" : "63 Geminorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "33.95",
	"RA_S" : 111.93481979,
	"DEC_S" : 21.4452599,
	"Constellation" : "Gemini ",
	"AMag" : 5.283,
	"key" : 22994,
	"title" : "63 Geminorum"
	},
{
	"Index" : "11863",
	"Description" : "Rho Geminorum (\u03C1 Gem) is a star system that lies approximately 59 light-years away in the constellation of Gemini, about 5 arcseconds east of Castor. The system consists of a primary bright enough to be seen with the naked eye, a faint secondary which has rarely been observed even professionally, and a distant semi-bright tertiary which requires telescopic equipment for observation.\r\rRho Geminorum A is a bright star with a spectral type F0V, meaning that it is a main sequence that is over a thousand degrees kelvin hotter, one-third more massive, two-thirds larger and five-and-a-half times more luminous than the Sun. With an apparent magnitude of 4.25, it is approximately the seventeenth-brightest star in the constellation of Gemini. Though there are some sources indicating that the star is a spectroscopic binary, including the Washington Double Star Catalog (WDS) and the Gliese Catalogue of Nearby Stars, no orbit has been provided.\r\rThe WDS lists four companions to Rho Geminorum. Of these, surprisingly little is known about the closest companion, the magnitude 12.5 Rho Geminorum B. The most recent measurement lists a separation of 3.4 arcseconds, corresponding to a separation perpendicular to the line of sight of approximately 85 AU. The spectral type listed in SIMBAD is M5, though this is without a source. Plotting the star\u0027s absolute magnitude on the Hertzsprung-Russell diagram (see left) indicates a B-V of 1.53, a value closer to that of an M3V star.\r\rPeculiarly, the five observations recorded in the WDS date between 1910 and 1935 and none have been made since; even in literature, more recent attempts to resolve Rho Geminorum B have been unsuccessful. The WDS measurements are inconsistent with the star being in the background, so the reasons for the failure to observe Rho Geminorum B is unclear.\r\rThe next-closest companion, the magnitude 11.59 WDS 07291+3147 C, had a much larger separation of 211.6 arcseconds in 1886. However, this separation increased by 10 arcseconds by 2001, indicating that it is a background star that is unrelated to Rho Geminorum. Correcting for Rho Geminorum A\u0027s proper motion, this star\u0027s proper motion is RA = -19 mas/yr and Dec = -55 mas/yr. This is a modestly large value, consistent with a distance of a few hundred light-years.\r\rWDS 07291+3147 C is listed as having a companion, the magnitude 13.20 WDS 07291+3147 D. Relative to WDS 07291+3147 C its separation has remained at about 100 arcseconds between 1909 and 2001, indicating similar proper motion. While this would indicate that the two stars are bound, at their distance this separation would indicate a separation of several hundred thousand AU at the very least and their mutual separation has not been entirely consistent (the position angle has increased from 267 to 270\u00B0, and the separation has decreased from 104.1 to 102.3 arcseconds). It is therefore possible that the two background stars are bound, but it is not certain.\r\rThe final companion in the WDS, the magnitude 7.86 WDS 07291+3147 E (Rho Geminorum C), has a larger still separation of 756 arcseconds, translating to a separation perpendicular to the line of sight of about 18600 AU. The position of this star relative to the primary has remained consistent over decades, indicating that it has a common proper motion and is therefore a wide tertiary component. The wide separation has also facilitated for observations without contamination from Rho Geminorum A, and as of such Rho Geminorum C has its own Gliese catalogue number (273.1) and HIPPARCOS catalogue number (36357). The HIPPARCOS parallax is consistent with that of the primary to 1\u03C3, leading to a probability that they are bound of approximately 100%. The star is also known to be a BY Draconis variable with a period of 11.63 days, caused by varying brightness as starspots move across the stellar surface across its rotation period. While the derived age for Rho Geminorum A of 2.1 Gigayears is not excessively young, Rho Geminorum C is still very active: It has an S\u0027HK of about 0.5, a value similar to that of the near-analogous Epsilon Eridani whose Log R\u0027HK is -4.45. This is much higher than a \u0022quiet\u0022 value of <-4.8, so Rho Geminorum C is unusually active for its age.\r\rThe Rho Geminorum system is an interesting look into an architecture similar to the 40 Eridani system while the most massive component is on the main sequence, before it becomes a white dwarf.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "62 Geminorum, Rho Geminorum, HIP 36366, SAO 60118, HD 58946, GC 9987, HR 2852, DM BD+32  1562, TYC 2452-2167-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Rho Geminorum",
	"OType" : "Double or multiple star",
	"Distance" : "18.05",
	"RA_S" : 112.27798875,
	"DEC_S" : 31.78453362,
	"X" : 177,
	"Y" : 308,
	"Constellation" : "Gemini ",
	"AMag" : 4.198,
	"key" : 31863,
	"title" : "Rho Geminorum"
	},
{
	"Index" : "7621",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "64 Geminorum, HIP 36393, SAO 79427, HD 59037, GC 9997, HR 2857, DM BD+28  1396, TYC 1918-2337-1",
	"group" : { "key" : "Gemini" },
	"Common" : "64 Geminorum",
	"OType" : "Star",
	"Distance" : "54.01",
	"RA_S" : 112.33516871,
	"DEC_S" : 28.11827478,
	"Constellation" : "Gemini ",
	"AMag" : 5.08,
	"key" : 27621,
	"title" : "64 Geminorum"
	},
{
	"Index" : "7622",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "65 Geminorum, b Geminorum, HIP 36429, SAO 79434, HD 59148, GC 10015, HR 2861, DM BD+28  1400, TYC 1918-2338-1",
	"group" : { "key" : "Gemini" },
	"Common" : "b Geminorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "146.63",
	"RA_S" : 112.45317419,
	"DEC_S" : 27.916139,
	"Constellation" : "Gemini ",
	"AMag" : 5.134,
	"key" : 27622,
	"title" : "b Geminorum"
	},
{
	"Index" : "3002",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "68 Geminorum, HIP 36760, SAO 97016, HD 60107, GC 10106, HR 2886, DM BD+16  1510, TYC 1360-2332-1",
	"group" : { "key" : "Gemini" },
	"Common" : "68 Geminorum",
	"OType" : "Star",
	"Distance" : "129.68",
	"RA_S" : 113.40202205,
	"DEC_S" : 15.82666229,
	"Constellation" : "Gemini ",
	"AMag" : 5.269,
	"key" : 23002,
	"title" : "68 Geminorum"
	},
{
	"Index" : "11899",
	"Description" : "Castor (\u03B1 Gem, \u03B1 Geminorum, Alpha Geminorum) is the second brightest star in the constellation Gemini and one of the brightest stars in the night sky. Although it has the Bayer designation \u0022alpha\u0022, it is actually fainter than Beta Geminorum (Pollux). Castor is 49.8 light years away from Earth.\r\rCastor was discovered to be a visual binary in 1678, with the magnitude of its components being 2.0 and 2.9 (the combined magnitude is 1.58). The separation of the components is about 6\u0022, and the period of revolution is around 467 years. Each of the components of Castor is itself a spectroscopic binary, making Castor a quadruple star system. Castor has a faint companion separated from it by about 72\u0022 but having the same parallax and proper motion; this companion is an eclipsing binary system with a period slightly less than 1 day, and it is one of only a few known eclipsing binary systems where both companions are class M dwarf stars. Castor can thus be considered to be a sextuple star system, with six individual stars gravitationally bound together. Component C has the variable star designation YY Geminorum.\r\rCastor and Pollux are the two \u0022heavenly twin\u0022 stars that give the constellation Gemini (meaning twins in Latin) its name. The name Castor refers specifically to Castor, one of the twin sons of Zeus and Leda. The star was annotated by the Arabic description Al-Ras al-Taum al-Muqadim, which translates as the head of the foremost twin. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Aoul al Dzira, which was translated into Latin as Prima Brachii, meaning the first in the paw.\r\rIn Chinese, \u5317\u6CB3 (B\u011Bi H\u00E9), meaning North River, refers to an asterism consisting of Castor, \u03C1 Geminorum, and Pollux. Consequently, Castor itself is known as \u5317\u6CB3\u4E8C (B\u011Bi H\u00E9 \u00E8r, English: the Second Star of North River.) The Chinese recognized Castor as Yin, which is, according to the Chinese, one of the two fundamental principles upon which all things depend.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "66 Geminorum, Alpha Geminorum, HIP 36850B, SAO 60198, HD 60178, GC 10120, HR 2890, DM BD+32  1581B, TYC 2457-2407-2",
	"group" : { "key" : "Gemini" },
	"Common" : "Castor",
	"OType" : "Spectroscopic binary",
	"Distance" : "15.8",
	"RA_S" : 113.650417,
	"DEC_S" : 31.888492,
	"X" : 162,
	"Y" : 303,
	"Constellation" : "Gemini ",
	"AMag" : 2.972,
	"key" : 31899,
	"shortTitle" : "Kastor",
	"title" : "Castor"
	},
{
	"Index" : "11867",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "HIP 36896AB, SAO 60204, HD 60318, GC 10137, HR 2896, DM BD+31 1620, TYC 2453-1917-1",
	"group" : { "key" : "Gemini" },
	"Common" : "HR  2896",
	"OType" : "Star",
	"Distance" : "113.08",
	"RA_S" : 113.78665939,
	"DEC_S" : 30.96093371,
	"Constellation" : "Gemini ",
	"AMag" : 5.46,
	"key" : 31867,
	"title" : "HR  2896"
	},
{
	"Index" : "7630",
	"Description" : "Upsilon Geminorum (\u03C5 Gem) is a star in the constellation Gemini. Its apparent magnitude is 4.08.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "69 Geminorum, Upsilon Geminorum, HIP 36962, SAO 79533, HD 60522, GC 10167, HR 2905, DM BD+27  1424, TYC 1919-2109-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Upsilon Geminorum",
	"OType" : "Variable Star",
	"Distance" : "82.74",
	"RA_S" : 113.980627,
	"DEC_S" : 26.89574745,
	"X" : 144,
	"Y" : 366,
	"Constellation" : "Gemini ",
	"AMag" : 4.227,
	"key" : 27630,
	"title" : "Upsilon Geminorum"
	},
{
	"Index" : "11928",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "71 Geminorum, Omicron Geminorum, HIP 37265, SAO 60247, HD 61110, GC 10257, HR 2930, DM BD+34  1649, TYC 2462-2103-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Omicron Geminorum",
	"OType" : "Star",
	"Distance" : "50.98",
	"RA_S" : 114.79138281,
	"DEC_S" : 34.58435476,
	"Constellation" : "Gemini ",
	"AMag" : 4.928,
	"key" : 31928,
	"title" : "Omicron Geminorum"
	},
{
	"Index" : "3040",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "74 Geminorum, f Geminorum, HIP 37300, SAO 97120, HD 61338, GC 10276, HR 2938, DM BD+18  1701, TYC 1365-2474-1",
	"group" : { "key" : "Gemini" },
	"Common" : "f Geminorum",
	"OType" : "Double or multiple star",
	"Distance" : "160.61",
	"RA_S" : 114.86913565,
	"DEC_S" : 17.67451547,
	"Constellation" : "Gemini ",
	"AMag" : 5.217,
	"key" : 23040,
	"title" : "f Geminorum"
	},
{
	"Index" : "7659",
	"Description" : "Sigma Geminorum (\u03C3 Gem) is a star in the constellation Gemini. Its apparent magnitude is 4.28.",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "75 Geminorum, Sigma Geminorum, HIP 37629, SAO 79638, HD 62044, GC 10373, HR 2973, DM BD+29  1590, TYC 1924-2022-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Sigma Geminorum",
	"OType" : "Variable of RS CVn type",
	"Distance" : "38.34",
	"RA_S" : 115.82802764,
	"DEC_S" : 28.88351125,
	"X" : 129,
	"Y" : 335,
	"Constellation" : "Gemini ",
	"AMag" : 4.369,
	"key" : 27659,
	"title" : "Sigma Geminorum"
	},
{
	"Index" : "7599",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "76 Geminorum, c Geminorum, HIP 37704, SAO 79650, HD 62285, GC 10392, HR 2983, DM BD+26  1633, TYC 1916-2155-1",
	"group" : { "key" : "Gemini" },
	"Common" : "c Geminorum",
	"OType" : "Variable Star",
	"Distance" : "193.65",
	"RA_S" : 116.02880967,
	"DEC_S" : 25.78415832,
	"Constellation" : "Gemini ",
	"AMag" : 5.474,
	"key" : 27599,
	"title" : "c Geminorum"
	},
{
	"Index" : "7600",
	"Description" : "Kappa Geminorum (\u03BA Gem, \u03BA Geminorum) is a Class G8, fourth-magnitude star in the constellation Gemini. It is a multiple star system located about 140 light-years from Earth. This star is radiating about 78 times the luminosity of the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.\r\rIn Chinese astronomy, Kappa Geminorum is called \u7A4D\u85AA, Pinyin: J\u012Bx\u012Bn, meaning Pile of Firewood, because this star is marking itself and stand alone in Pile of Firewood asterism, Well mansion (see : Chinese constellation). \u7A4D\u85AA (J\u012Bx\u012Bn) westernized into Tseih Tsing, but the name Tseih Tsing was designated for \u03C7 Gem and \u03BC Cnc by R.H. Allen, with the meaning is \u0022piled-up fuel",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "77 Geminorum, Kappa Geminorum, HIP 37740, SAO 79653, HD 62345, GC 10403, HR 2985, DM BD+24  1759, TYC 1916-2156-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Kappa Geminorum",
	"OType" : "Double or multiple star",
	"Distance" : "43.34",
	"RA_S" : 116.11187744,
	"DEC_S" : 24.39799681,
	"X" : 112,
	"Y" : 392,
	"Constellation" : "Gemini ",
	"AMag" : 3.662,
	"key" : 27600,
	"title" : "Kappa Geminorum"
	},
{
	"Index" : "3048",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "81 Geminorum, g Geminorum, HIP 37908, SAO 97221, HD 62721, GC 10456, HR 3003, DM BD+18  1733, TYC 1366-2455-1",
	"group" : { "key" : "Gemini" },
	"Common" : "g Geminorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "103.94",
	"RA_S" : 116.53102986,
	"DEC_S" : 18.51003847,
	"Constellation" : "Gemini ",
	"AMag" : 5.036,
	"key" : 23048,
	"title" : "g Geminorum"
	},
{
	"Index" : "11903",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "80 Geminorum, Pi Geminorum, HIP 38016, SAO 60340, HD 62898, GC 10482, HR 3013, DM BD+33  1585, TYC 2458-2151-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Pi Geminorum",
	"OType" : "Variable Star",
	"Distance" : "201.82",
	"RA_S" : 116.87634874,
	"DEC_S" : 33.41569943,
	"Constellation" : "Gemini ",
	"AMag" : 5.317,
	"key" : 31903,
	"title" : "Pi Geminorum"
	},
{
	"Index" : "7717",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "83 Geminorum, Phi Geminorum, HIP 38538, SAO 79774, HD 64145, GC 10653, HR 3067, DM BD+27  1499, TYC 1933-2000-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Phi Geminorum",
	"OType" : "High proper-motion Star",
	"Distance" : "68.01",
	"RA_S" : 118.37423405,
	"DEC_S" : 26.76578861,
	"Constellation" : "Gemini ",
	"AMag" : 4.977,
	"key" : 27717,
	"title" : "Phi Geminorum"
	},
{
	"Index" : "3074",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "85 Geminorum, HIP 38722, SAO 79799, HD 64648, GC 10707, HR 3086, DM BD+20  1946, TYC 1371-2373-1",
	"group" : { "key" : "Gemini" },
	"Common" : "85 Geminorum",
	"OType" : "Star",
	"Distance" : "114.67",
	"RA_S" : 118.91622898,
	"DEC_S" : 19.88396975,
	"Constellation" : "Gemini ",
	"AMag" : 5.359,
	"key" : 23074,
	"title" : "85 Geminorum"
	},
{
	"Index" : "7723",
	"MapNum" : "08",
	"ImageNum" : "08",
	"Desig" : "Chi Geminorum, HIP 39424, SAO 79896, HD 66216, GC 10912, HR 3149, DM BD+28  1532, TYC 1934-1889-1",
	"group" : { "key" : "Gemini" },
	"Common" : "Chi Geminorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "78.63",
	"RA_S" : 120.87951898,
	"DEC_S" : 27.79431875,
	"Constellation" : "Gemini ",
	"AMag" : 5.064,
	"key" : 27723,
	"title" : "Chi Geminorum"
	},
{
	"Index" : "57103",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Xi Gruis, HIP 106327, SAO 230726, HD 204783, GC 30138, HR 8229, DM CD-41 14550, TYC 7984-883-1",
	"group" : { "backgroundImage" : "images/Alignment/26.png",
		"description" : "Grus (pron.: /\u02C8\u0261r\u028Cs/, or colloquially /\u02C8\u0261ru\u02D0s/) is a constellation in the southern sky. Its name is Latin for the crane, a species of bird. It was introduced in the late 16th century.\r\rThe stars that form Grus were originally considered part of Piscis Austrinus (the southern fish). The Arabic name of Gamma Gruis (al-dhanab, \u0022the tail\u0022) reflects this origins.\r\rThe stars were first defined as a separate constellation by Petrus Plancius, who created twelve new constellations based on the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. Grus first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. Its first depiction in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rAn alternative name for the constellation, Phoenicopterus (Latin for flamingo), was used briefly during the early 17th century.\r\rGrus represents a crane, though it is sometimes seen as a flamingo. There are no ancient myths associated with Grus.",
		"key" : "Grus",
		"grouptype" : "Grus",
		"Meaning" : "Crane",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Grus",
		"title" : "Grus Objects Group" },
	"Common" : "Xi Gruis",
	"OType" : "Star",
	"Distance" : "142.15",
	"RA_S" : 323.0244862,
	"DEC_S" : -41.17930886,
	"Constellation" : "Grus ",
	"AMag" : 5.41,
	"key" : 77103,
	"title" : "Xi Gruis"
	},
{
	"Index" : "52779",
	"Description" : "Gamma Gruis (Gamma Gru, \u03B3 Gruis, \u03B3 Gru) is a star in the southern constellation of Grus. It is known as Al Dhanab, \u0022the Tail (of the constellation of the Southern Fish)\u0022 and once belonged to the Ptolemaic constellation Piscis Austrinus. With an apparent visual magnitude of 3.0, it is the third brightest star in the constellation.\r\rIn Chinese, \u6557\u81FC (B\u00E0i Ji\u00F9), meaning Decayed Mortar, refers to an asterism consisting of \u03B3 Gruis, \u03BB Gruis, \u03B3 Piscis Austrini and 19 Piscis Austrini. Consequently, \u03B3 Gruis itself is known as \u6557\u81FC\u4E00 (B\u00E0i Ji\u00F9 y\u012B, English: the First Star of Decayed Mortar.) \r\rBased upon parallax measurements, this star is located at a distance of roughly 211 light-years (65 parsecs) from Earth. Analysis of the spectrum shows it to match a stellar classification of B8 III, with the luminosity class of III indicating this is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The luminosity of Gamma Gruis is around 390 times that of the Sun, with a significant portion of the energy emission being in the ultraviolet. Its outer envelope has an effective temperature of 12,520 K, which give the star a blue-white hue. Gamma Gruis is rotating relatively rapidly with a projected rotational velocity of 57 km s\u20131. By way of comparison, the Sun has an azimuthal velocity along its equator of just 2 km s\u20131.\r\rBased upon analysis of data collected during the Hipparcos mission, this star may have a proper motion companion that is causing gravitational perturbation of Gamma Gruis.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Gamma Gruis, HIP 108085, SAO 213374, HD 207971, GC 30640, HR 8353, DM CD-37 14536, TYC 7494-1748-1",
	"group" : { "key" : "Grus" },
	"Common" : "Al Dhanab",
	"OType" : "Star",
	"Distance" : "64.58",
	"RA_S" : 328.48220445,
	"DEC_S" : -37.3648735,
	"X" : 380,
	"Y" : 145,
	"Constellation" : "Grus ",
	"AMag" : 2.971,
	"key" : 72779,
	"title" : "Al Dhanab"
	},
{
	"Index" : "52778",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "HIP 108294, SAO 213414, HD 208321, GC 30696, HR 8366, DM CD-3714565, TYC 7494-1747-1",
	"group" : { "key" : "Grus" },
	"Common" : "HR 8366",
	"OType" : "Star",
	"Distance" : "102.87",
	"RA_S" : 329.09487465,
	"DEC_S" : -37.25365453,
	"Constellation" : "Grus ",
	"AMag" : 5.454,
	"key" : 72778,
	"title" : "HR 8366"
	},
{
	"Index" : "57157",
	"Description" : "Lambda Gruis (\u03BB Gru) is a star in the constellation Grus. Its apparent magnitude is 4.48.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Lambda Gruis, HIP 109111, SAO 213543, HD 209688, GC 30892, HR 8411, DM CD-40 14639, TYC 7995-1343-1",
	"group" : { "key" : "Grus" },
	"Common" : "Lambda Gruis",
	"OType" : "Star",
	"Distance" : "74.22",
	"RA_S" : 331.52869067,
	"DEC_S" : -39.54335163,
	"X" : 347,
	"Y" : 171,
	"Constellation" : "Grus ",
	"AMag" : 4.618,
	"key" : 77157,
	"title" : "Lambda Gruis"
	},
{
	"Index" : "57191",
	"Description" : "Mu1 Gruis (\u03BC1 Gru) is a star in the constellation Grus. Its apparent magnitude is 4.81.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Mu01 Gruis, HIP 109908AB, SAO 231055, HD 211088, GC 31125, HR 8486, DM CD-41 14810, TYC 7999-1569-1",
	"group" : { "key" : "Grus" },
	"Common" : "Mu1 Gruis",
	"OType" : "Double or multiple star",
	"Distance" : "84.11",
	"RA_S" : 333.90383186,
	"DEC_S" : -41.34669335,
	"X" : 322,
	"Y" : 193,
	"Constellation" : "Grus ",
	"AMag" : 4.887,
	"key" : 77191,
	"title" : "Mu1 Gruis"
	},
{
	"Index" : "57193",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Mu02 Gruis, HIP 109973, SAO 231063, HD 211202, GC 31138, HR 8488, DM CD-42 15846, TYC 7999-1572-1",
	"group" : { "key" : "Grus" },
	"Common" : "Mu2 Gruis",
	"OType" : "Star",
	"Distance" : "81.1",
	"RA_S" : 334.11064175,
	"DEC_S" : -41.62721764,
	"X" : 320,
	"Y" : 197,
	"Constellation" : "Grus ",
	"AMag" : 5.219,
	"key" : 77193,
	"title" : "Mu2 Gruis"
	},
{
	"Index" : "65126",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "HIP 110109, SAO 247400, HD 211415, GC 31178, HR 8501, DM CP-5410055, TYC 8822-1455-1",
	"group" : { "key" : "Grus" },
	"Common" : "Gliese 853 A (HR 8501)",
	"OType" : "Double or multiple star",
	"Distance" : "13.79",
	"RA_S" : 334.56505009,
	"DEC_S" : -53.62707393,
	"Constellation" : "Grus ",
	"AMag" : 5.459,
	"key" : 85126,
	"title" : "Gliese 853 A (HR 8501)"
	},
{
	"Index" : "57224",
	"Description" : "Delta1 Gruis (\u03B41 Gru) is a star in the constellation Grus. Its apparent magnitude is 3.97.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Delta01 Gruis, HIP 110997, SAO 231154, HD 213009, GC 31400, HR 8556, DM CD-44 14931, TYC 8003-1372-1",
	"group" : { "key" : "Grus" },
	"Common" : "Delta1 Gruis",
	"OType" : "Star",
	"Distance" : "94.83",
	"RA_S" : 337.31739355,
	"DEC_S" : -43.49556021,
	"X" : 288,
	"Y" : 220,
	"Constellation" : "Grus ",
	"AMag" : 4.077,
	"key" : 77224,
	"title" : "Delta1 Gruis"
	},
{
	"Index" : "57225",
	"Description" : "Delta2 Gruis (\u03B42 Gru) is a star in the constellation Grus. Its apparent magnitude is 4.17.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Delta02 Gruis, HIP 111043, SAO 231161, HD 213080, GC 31412, HR 8560, DM CD-44 14935, TYC 8003-1373-1",
	"group" : { "key" : "Grus" },
	"Common" : "Delta2 Gruis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "101.15",
	"RA_S" : 337.43931758,
	"DEC_S" : -43.74921705,
	"X" : 287,
	"Y" : 223,
	"Constellation" : "Grus ",
	"AMag" : 4.33,
	"key" : 77225,
	"title" : "Delta2 Gruis"
	},
{
	"Index" : "57263",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Rho Gruis, HIP 112203, SAO 231265, HD 215104, GC 31701, HR 8644, DM CD-42 16049, TYC 8007-205-1",
	"group" : { "key" : "Grus" },
	"Common" : "Rho Gruis",
	"OType" : "Star",
	"Distance" : "70.61",
	"RA_S" : 340.87490495,
	"DEC_S" : -41.41434573,
	"Constellation" : "Grus ",
	"AMag" : 4.948,
	"key" : 77263,
	"title" : "Rho Gruis"
	},
{
	"Index" : "65135",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Eta Gruis, HIP 112374, SAO 247570, HD 215369, GC 31744, HR 8655, DM CP-54 10123, TYC 8823-1609-1",
	"group" : { "key" : "Grus" },
	"Common" : "Eta Gruis",
	"OType" : "Star",
	"Distance" : "127.1",
	"RA_S" : 341.40783731,
	"DEC_S" : -53.50012248,
	"Constellation" : "Grus ",
	"AMag" : 4.977,
	"key" : 85135,
	"title" : "Eta Gruis"
	},
{
	"Index" : "61433",
	"Description" : "Epsilon Gruis (\u03B5 Gru) is a star in the constellation Grus. Its apparent magnitude is 3.49.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Epsilon Gruis, HIP 112623, SAO 247593, HD 215789, GC 31813, HR 8675, DM CD-51 13389, TYC 8453-1499-1",
	"group" : { "key" : "Grus" },
	"Common" : "Epsilon Gruis",
	"OType" : "Spectroscopic binary",
	"Distance" : "39.51",
	"RA_S" : 342.13873951,
	"DEC_S" : -51.31687677,
	"X" : 249,
	"Y" : 323,
	"Constellation" : "Grus ",
	"AMag" : 3.479,
	"key" : 81433,
	"title" : "Epsilon Gruis"
	},
{
	"Index" : "65142",
	"Description" : "Zeta Gruis (\u03B6 Gru) is a star in the constellation Grus. Its apparent magnitude is 4.13.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Zeta Gruis, HIP 113638, SAO 247680, HD 217364, GC 32061, HR 8747, DM CP-53 10382, TYC 8824-1503-1",
	"group" : { "key" : "Grus" },
	"Common" : "Zeta Gruis",
	"OType" : "Star",
	"Distance" : "33.35",
	"RA_S" : 345.22003445,
	"DEC_S" : -52.75413675,
	"X" : 226,
	"Y" : 344,
	"Constellation" : "Grus ",
	"AMag" : 4.222,
	"key" : 85142,
	"title" : "Zeta Gruis"
	},
{
	"Index" : "57306",
	"Description" : "Theta Gruis (\u03B8 Gru) is a star in the constellation Grus. Its apparent magnitude is 4.33.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Theta Gruis, HIP 114131A, SAO 231444, HD 218227A, GC 32184, HR 8787, DM CD-44 15149, TYC 8012-1248-1",
	"group" : { "key" : "Grus" },
	"Common" : "Theta Gruis",
	"OType" : "Star",
	"Distance" : "40.42",
	"RA_S" : 346.71974505,
	"DEC_S" : -43.52035831,
	"X" : 201,
	"Y" : 226,
	"Constellation" : "Grus ",
	"AMag" : 4.452,
	"key" : 77306,
	"title" : "Theta Gruis"
	},
{
	"Index" : "57307",
	"Description" : "Theta Gruis (\u03B8 Gru) is a star in the constellation Grus. Its apparent magnitude is 4.33.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Theta Gruis, HIP 114131B, SAO 231444, HD 218227B, GC 32184, HR 8787, DM CD-44 15149, TYC 8012-1248-2",
	"group" : { "key" : "Grus" },
	"Common" : "Theta Gruis",
	"OType" : "Star",
	"Distance" : "40.42",
	"RA_S" : 346.71974505,
	"DEC_S" : -43.52035831,
	"X" : 201,
	"Y" : 226,
	"Constellation" : "Grus ",
	"AMag" : 6.596,
	"key" : 77307,
	"title" : "Theta Gruis"
	},
{
	"Index" : "61385",
	"Description" : "Iota Gruis (\u03B9 Gru) is a star in the constellation Grus. Its apparent magnitude is 3.89.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Iota Gruis, HIP 114421, SAO 231468, HD 218670, GC 32270, HR 8820, DM CD-45 14947, TYC 8448-1362-1",
	"group" : { "key" : "Grus" },
	"Common" : "Iota Gruis",
	"OType" : "Spectroscopic binary",
	"Distance" : "56.16",
	"RA_S" : 347.58974039,
	"DEC_S" : -45.24671916,
	"X" : 195,
	"Y" : 249,
	"Constellation" : "Grus ",
	"AMag" : 3.988,
	"key" : 81385,
	"title" : "Iota Gruis"
	},
{
	"Index" : "17074",
	"Description" : "Chi Herculis (\u03C7 Her) is a star in the constellation Hercules. Its apparent magnitude is 4.62. It is a yellow class F dwarf star, with a temperature of around 5840 \u00B0K. It is about 3 solar luminosities, 1.7 solar radii, and about 15% more massive than the sun. It is near the end of its life as a main-sequence star that fuses hydrogen.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "1 Herculis, Chi Herculis, HIP 77760, SAO 45772, HD 142373, GC 21340, HR 5914, DM BD+42  2648, TYC 3057-2021-1",
	"group" : { "backgroundImage" : "images/Alignment/27.png",
		"description" : "Hercules is a constellation named after Hercules, the Roman mythological hero adapted from the Greek hero Heracles. Hercules was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations today. It is the fifth largest of the modern constellations.\r\rThe traditional visualization imagines \u03B1 Herculis as Hercules\u0027s head; its name, Ras Algethi, literally means \u0022head of the kneeling one\u0022. Hercules\u0027s left hand then points toward Lyra from his shoulder (Delta Herculis), and Beta Herculis forms his other shoulder. His narrow waist is formed by Epsilon and Zeta Herculis. Finally, his left leg (with Theta as the knee and Iota the foot) is stepping on Draco\u0027s head, the dragon/snake who Hercules has vanquished and perpetually gloats over for eternities.\r\rA common form found in modern star charts uses the quadrangle formed by \u03C0 Her, \u03B7 Her, \u03B6 Her and \u03B5 Her (known as the \u0022Keystone\u0022 asterism) as Hercules\u0027s torso.\r\rH.A. Rey has suggested an alternative visualization in which the \u0022Keystone\u0022 becomes Hercules\u0027s head. This quadrangle lies between two very bright stars: Vega in the constellation Lyra and \u03B1 CrB (Gemma, or Alphecca) in the constellation Corona Borealis. The hero\u0027s right leg contains two bright stars of the third magnitude: \u03B1 Her (Ras Algethi) and \u03B4 Her (Sarin). The latter is the right knee. The hero\u0027s left leg contains dimmer stars of the fourth magnitude which do not have Bayer designations but which do have Flamsteed numbers. The star \u03B2 Her belongs to the hero\u0027s outstretched right hand, and is also called Kornephoros.\r\rAccording to Gavin White, the Greek constellation of Hercules is a distorted version of the Babylonian constellation known as the \u0022Standing Gods\u0022 (MUL.DINGIR.GUB.BA.MESH). White argues that this figure was, like the similarly named \u0022Sitting Gods\u0022, depicted as a man with a serpent\u0027s body instead of legs (the serpent element now being represented on the Greek star map by the figure of Draco that Hercules crushes beneath his feet). He further argues that the original name of Hercules - the \u0027Kneeler\u0027 (see below) - is a conflation of the two Babylonian constellations of the Sitting and Standing Gods.\r\rThe earliest Greek references to the constellation do not refer to it as Hercules. Aratus describes it as follows:\r\rRight there in its [Draco\u0027s] orbit wheels a Phantom form, like to a man that strives at a task. That sign no man knows how to read clearly, nor what task he is bent, but men simply call him On His Knees [\u1F18\u03B3\u03B3\u03CC\u03BD\u03B1\u03C3\u03B9\u03BD \u0022the Kneeler\u0022].\r\rNow that Phantom, that toils on his knees, seems to sit on bended knee, and from both his shoulders his hands are upraised and stretch, one this way, one that, a fathom\u0027s length. Over the middle of the head of the crooked Dragon, he has the tip of his right foot. Here too that Crown [Corona], which glorious Dionysus set to be memorial of the dead Ariadne, wheels beneath the back of the toil-spent Phantom. To the Phantom\u0027s back the Crown is near, but by his head mark near at hand the head of Ophiuchus [...] Yonder, too, is the tiny Tortoise, which, while still beside his cradle, Hermes pierced for stings and bade it be called the Lyre [Lyra]: and he brought it into heaven and set it in front of the unknown Phantom. That Croucher on his Knees comes near the Lyre with his left knee, but the top of the Bird\u0027s head wheels on the other side, and between the Bird\u0027s head and the Phantom\u0027s knee is enstarred the Lyre.\r\rThe story connecting Hercules with the constellation is recounted by Dionysius of Halicarnassus:\r\rOn his way back to Mycenae from Iberia having obtained the Cattle of Geryon as his tenth labour Heracles came to Liguria in North-Western Italy where he engaged in battle with two giants, Albion and Bergion or Dercynus. The opponents were strong; Hercules was in a difficult position so he prayed to his father Zeus for help. With the aegis of Zeus, Heracles won the battle. It was this kneeling position of Heracles when prayed to his father Zeus that gave the name \u0022the Kneeler\u0022. and Hyginus\r\rHercules is also sometimes associated with Gilgamesh, a Sumerian mythological hero.",
		"key" : "Hercules",
		"grouptype" : "Hercules",
		"Meaning" : "Hercules (mythological character)",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Hercules",
		"title" : "Hercules Objects Group" },
	"Common" : "Chi Herculis",
	"OType" : "High proper-motion Star",
	"Distance" : "15.89",
	"RA_S" : 238.16892772,
	"DEC_S" : 42.45151818,
	"X" : 585,
	"Y" : 150,
	"Constellation" : "Hercules ",
	"AMag" : 4.664,
	"key" : 37074,
	"title" : "Chi Herculis"
	},
{
	"Index" : "4223",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "5 Herculis, r Herculis, HIP 78481, SAO 101879, HD 143666, GC 21525, HR 5966, DM BD+18  3101, TYC 1507-1114-1",
	"group" : { "key" : "Hercules" },
	"Common" : "r Herculis",
	"OType" : "Spectroscopic binary",
	"Distance" : "76.5",
	"RA_S" : 240.30965418,
	"DEC_S" : 17.81840469,
	"Constellation" : "Hercules ",
	"AMag" : 5.212,
	"key" : 24223,
	"title" : "r Herculis"
	},
{
	"Index" : "20903",
	"Description" : "Upsilon Herculis (\u03C5 Her) is a star in the constellation Hercules. Its apparent magnitude is 4.71.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "6 Herculis, Upsilon Herculis, HIP 78592, SAO 45865, HD 144206, GC 21580, HR 5982, DM BD+46  2142, TYC 3491-1859-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Upsilon Herculis",
	"OType" : "Star",
	"Distance" : "113.84",
	"RA_S" : 240.69956865,
	"DEC_S" : 46.03669958,
	"X" : 550,
	"Y" : 109,
	"Constellation" : "Hercules ",
	"AMag" : 4.694,
	"key" : 40903,
	"title" : "Upsilon Herculis"
	},
{
	"Index" : "4229",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "7 Herculis, Kappa Herculis, HIP 79043A, SAO 101951, HD 145001, GC 21696, HR 6008, DM BD+17  2964, TYC 1508-1273-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Marsik",
	"OType" : "Star",
	"Distance" : "112.22",
	"RA_S" : 242.01885587,
	"DEC_S" : 17.04697981,
	"Constellation" : "Hercules ",
	"AMag" : 5.097,
	"key" : 24229,
	"shortTitle" : "Marfik; Mirfak (also HD20902); Marfak",
	"title" : "Marsik"
	},
{
	"Index" : "17157",
	"Description" : "Phi Herculis (\u03C6 Her) is a star in the constellation Hercules. Its apparent magnitude is 4.23.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "11 Herculis, Phi Herculis, HIP 79101, SAO 45911, HD 145389, GC 21736, HR 6023, DM BD+45  2376, TYC 3067-1842-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Phi Herculis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "62.48",
	"RA_S" : 242.19240346,
	"DEC_S" : 44.9349181,
	"X" : 540,
	"Y" : 126,
	"Constellation" : "Hercules ",
	"AMag" : 4.216,
	"key" : 37157,
	"title" : "Phi Herculis"
	},
{
	"Index" : "20913",
	"Description" : "Tau Herculis (\u03C4 Her, \u03C4 Herculis) is a fourth-magnitude star in the constellation Hercules. Its traditional name Rukbalgethi Shemali, though seldom used today in scientific journals, means the \u0022northern knee\u0022. It is a blue subgiant star, seven hundred times more luminous than the Sun. Tau Herculis is a blue subgiant star with stellar classification B5IV. Its mass is 4.9 times solar. Though its apparent magnitude is only 3.89, like all B-class stars, it is very luminous boasting a total bolometric luminosity that is 700 times solar. Hipparcos estimated its distance at roughly 96 parsecs from Earth, or 310 \u00B1 20 light years away.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "22 Herculis, Tau Herculis, HIP 79992, SAO 46028, HD 147394, GC 21987, HR 6092, DM BD+46  2169, TYC 3492-1909-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Rukbalgethi Shemali",
	"OType" : "Star",
	"Distance" : "94.24",
	"RA_S" : 244.93515629,
	"DEC_S" : 46.31336906,
	"X" : 511,
	"Y" : 113,
	"Constellation" : "Hercules ",
	"AMag" : 3.854,
	"key" : 40913,
	"title" : "Rukbalgethi Shemali"
	},
{
	"Index" : "4261",
	"Description" : "Gamma Herculis (\u03B3 Herculis, \u03B3 Her) is a magnitude 3.74 binary star system in the northern constellation of Hercules.This is known to be a spectroscopic binary system, although there is no information about the secondary component. Based upon parallax measurements, this system is located at a distance of about 193 light-years (59 parsecs) from the Earth. The spectrum of the primary star matches a stellar classification of A9III, which indicates this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. The effective temperature is about 7,031 K, giving the star a white hue characteristic of A-type stars. It is rotating rapidly with a projected rotational velocity of 135 km s\u20131. The interferometry-measured angular diameter of this star is 0.95 \u00B1 0.04 mas, which, at its estimated distance, equates to a physical radius of about six times the radius of the Sun.\r\rObservations by German astronomer Ernst Zinner in 1929 gave indications that this may be a variable star. It was listed in the New Catalogue of Suspected Variable Stars (1981) with a magnitude range of 3.74 to 3.81. Further observations up to 1991 showed a pattern of small, slow variations with a magnitude variation of 0.05. These appeared to repeat semi-regularly with a period of 183.6 days, although the spectroscopic data presented a longer period of 165.9 days.\r\rIt was a member of indigenous Arabic asterism al-Nasaq al-Sha\u0027\u0101m\u012B, \u0022the Northern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022, along with \u03B2 Her (Kornephoros), \u03B3 Ser (Zheng, Ching) and \u03B2 Ser (Chow).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Sha\u0027\u0101m\u012B or Nasak Shamiya were the title for three stars :\u03B2 Ser as Nasak Shamiya I, \u03B3 Ser as Nasak Shamiya II, \u03B3 Her as Nasak Shamiya III (exclude \u03B2 Her)\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B3 Herculis, \u03B2 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B2 Serpentis, \u03B4 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B3 Herculis itself is known as \u5929\u5E02\u53F3\u57A3\u4E8C (Ti\u0101n Sh\u00EC Zu\u01D2 Y\u00F2u \u00E8r, English: the Second Star of Right Wall of Heavenly Market Enclosure), represent H\u00E9ji\u0101n (\u6CB3\u9593), possibly Hejian states (located in roughly modern Cangzhou, Hebei) or Hejian Commandery (located in roughly modern Baoding, Hebei), (see : Sima Yong, the Prince of Hejian \u6CB3\u9593\u738B and Liu Wuzhou). H\u00E9ji\u0101n (\u6CB3\u9593) was westernized into Ho Keen by R.H. Allen, which was the meaning \u0022between the river\u0022.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "20 Herculis, Gamma Herculis, HIP 80170, SAO 102107, HD 147547A, GC 22012, HR 6095, DM BD+19  3086, TYC 1513-1261-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Gamma Herculis",
	"OType" : "Star",
	"Distance" : "59.05",
	"RA_S" : 245.480175,
	"DEC_S" : 19.153022,
	"X" : 562,
	"Y" : 467,
	"Constellation" : "Hercules ",
	"AMag" : 3.761,
	"key" : 24261,
	"title" : "Gamma Herculis"
	},
{
	"Index" : "71384",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "24 Herculis, Omega Herculis, HIP 80463, SAO 102153, HD 148112, GC 22090, HR 6117, DM BD+14  3049, TYC 971-1433-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Kajam",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "76.47",
	"RA_S" : 246.35397884,
	"DEC_S" : 14.03327273,
	"Constellation" : "Hercules ",
	"AMag" : 4.565,
	"key" : 91384,
	"shortTitle" : "Cujam; Cajam; Caiam",
	"title" : "Kajam"
	},
{
	"Index" : "17150",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "30 Herculis, g Herculis, HIP 80704, SAO 46108, HD 148783, GC 22172, HR 6146, DM BD+42  2714, TYC 3066-2214-1",
	"group" : { "key" : "Hercules" },
	"Common" : "g Herculis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "108.53",
	"RA_S" : 247.1606199,
	"DEC_S" : 41.88167735,
	"Constellation" : "Hercules ",
	"AMag" : 5.047,
	"key" : 37150,
	"title" : "g Herculis"
	},
{
	"Index" : "4293",
	"Description" : "Beta Herculis (Beta Her, \u03B2 Herculis, \u03B2 Her), which has the traditional name Kornephoros, is the brightest star in the northern constellation of Hercules at a base apparent visual magnitude of 2.81. This is a suspected variable star with an apparent magnitude that may rise as high as 2.76. Based upon parallax measurements, it is located at a distance of 139 light-years (43 parsecs) from Earth.\r\rAlthough \u03B2 Herculis appears to the naked eye to be a single star, in July 1899 the American astronomer W. W. Campbell discovered from spectroscopic measurements that its radial velocity varies, and concluded that it is a binary system. An orbit for the binary was computed in 1908 based upon additional spectroscopic measurements.\r\rAt Palomar Observatory, Antoine Labeyrie and others used speckle interferometry with the Hale Telescope to resolve the system in 1977. The Hipparcos satellite observed the orbital motion of the primary relative to other stars, and an orbit was computed in 2005 using spectroscopic data together with these measurements. The period of the system is around 410 days. They have a high orbital eccentricity of 0.55 and the orbital plane is inclined 53.8\u00B0 to the line of sight from the Earth.\r\rThe primary star in this binary system has a stellar classification of G7 IIIa, indicating that it is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. It has a mass nearly three times the mass of the Sun, and has expanded to 17 times the Sun\u0027s radius. The effective temperature of the star\u0027s outer envelope is about 4,887 K, which gives it the yellow hue of a G-type star. The secondary star has a mass only 90% that of the Sun.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "27 Herculis, Beta Herculis, HIP 80816, SAO 84411, HD 148856, GC 22193, HR 6148, DM BD+21  2934, TYC 1518-1442-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Kornephoros",
	"OType" : "Spectroscopic binary",
	"Distance" : "42.63",
	"RA_S" : 247.55499811,
	"DEC_S" : 21.48961132,
	"X" : 534,
	"Y" : 439,
	"Constellation" : "Hercules ",
	"AMag" : 2.86,
	"key" : 24293,
	"shortTitle" : "Rutilicus; Korneforos",
	"title" : "Kornephoros"
	},
{
	"Index" : "4266",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "s Herculis, HIP 80843, SAO 84416, HD 148897, GC 22202, HR 6152, DM BD+20  3283, TYC 1514-1249-1",
	"group" : { "key" : "Hercules" },
	"Common" : "s Herculis",
	"OType" : "Variable Star",
	"Distance" : "191.1",
	"RA_S" : 247.6397858,
	"DEC_S" : 20.47918822,
	"Constellation" : "Hercules ",
	"AMag" : 5.383,
	"key" : 24266,
	"title" : "s Herculis"
	},
{
	"Index" : "71368",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "29 Herculis, h Herculis, HIP 81008, SAO 102234, HD 149161, GC 22250, HR 6159, DM BD+11  3008, TYC 968-1712-1",
	"group" : { "key" : "Hercules" },
	"Common" : "h Herculis",
	"OType" : "Variable Star",
	"Distance" : "107.54",
	"RA_S" : 248.15121646,
	"DEC_S" : 11.48804267,
	"Constellation" : "Hercules ",
	"AMag" : 5.004,
	"key" : 91368,
	"title" : "h Herculis"
	},
{
	"Index" : "17149",
	"Description" : "Sigma Herculis (\u03C3 Her) is a star in the constellation Hercules. Its apparent magnitude is 4.20.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "35 Herculis, Sigma Herculis, HIP 81126, SAO 46161, HD 149630, GC 22296, HR 6168, DM BD+42  2724, TYC 3066-2213-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Sigma Herculis",
	"OType" : "Double or multiple star",
	"Distance" : "96.3",
	"RA_S" : 248.52575146,
	"DEC_S" : 42.43702714,
	"X" : 487,
	"Y" : 168,
	"Constellation" : "Hercules ",
	"AMag" : 4.193,
	"key" : 37149,
	"title" : "Sigma Herculis"
	},
{
	"Index" : "20993",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "42 Herculis, HIP 81497, SAO 46210, HD 150450, GC 22412, HR 6200, DM BD+49  2531, TYC 3502-2258-1",
	"group" : { "key" : "Hercules" },
	"Common" : "42 Herculis",
	"OType" : "Variable Star",
	"Distance" : "126.75",
	"RA_S" : 249.68685896,
	"DEC_S" : 48.92834608,
	"Constellation" : "Hercules ",
	"AMag" : 5.07,
	"key" : 40993,
	"title" : "42 Herculis"
	},
{
	"Index" : "12902",
	"Description" : "Zeta Herculis (\u03B6 Her, \u03B6 Herculis) is a multiple star system in the constellation Hercules. It has a combined apparent visual magnitude of 2.81, which is readily visible to the naked eye. Parallax measurements put it at a distance of about 35.0 light-years (10.7 parsecs) from Earth.\r\rThe primary member is a subgiant star that is somewhat larger than the Sun and has just begun to evolve away from the main sequence as the supply of hydrogen at its core becomes exhausted. It is orbited by a smaller companion star at a mean angular separation of 1.5 arcseconds, which corresponds to a physical separation of 150 Astronomical Units. This distance is large enough so that the two stars do not have a significant tidal effect on each other. The stars orbit each other over a period of 34.45 years, with a semi-major axis of 1.33\u0022 and an eccentricity of 0.46.\r\rComponent A has a stellar classification of F9 IV. It has about 2.6 times the radius of the Sun and 1.45 times the Sun\u0027s mass. This star is radiating more than six times the luminosity of the Sun at an effective temperature of 5,820 K. The secondary component is about the same size and mass as the Sun, with an effective temperature of 5,300 K. Both stars are rotating slowly. There may be a faint third member of this system, although little is known about it.\r\rThis system forms part of the Zeta Herculis moving group of stars. This group includes: \u03C62 Pavonis, \u03B6 Reticuli, 1 Hydrae, Gl 456, Gl 678, and Gl 9079.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "40 Herculis, Zeta Herculis, HIP 81693A, SAO 65485, HD 150680, GC 22464, HR 6212, DM BD+31  2884, TYC 2582-3158-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Zeta Herculis",
	"OType" : "Star",
	"Distance" : "10.72",
	"RA_S" : 250.322771,
	"DEC_S" : 31.601936,
	"X" : 487,
	"Y" : 311,
	"Constellation" : "Hercules ",
	"AMag" : 2.952,
	"key" : 32902,
	"title" : "Zeta Herculis"
	},
{
	"Index" : "12903",
	"Description" : "Zeta Herculis (\u03B6 Her, \u03B6 Herculis) is a multiple star system in the constellation Hercules. It has a combined apparent visual magnitude of 2.81, which is readily visible to the naked eye. Parallax measurements put it at a distance of about 35.0 light-years (10.7 parsecs) from Earth.\r\rThe primary member is a subgiant star that is somewhat larger than the Sun and has just begun to evolve away from the main sequence as the supply of hydrogen at its core becomes exhausted. It is orbited by a smaller companion star at a mean angular separation of 1.5 arcseconds, which corresponds to a physical separation of 150 Astronomical Units. This distance is large enough so that the two stars do not have a significant tidal effect on each other. The stars orbit each other over a period of 34.45 years, with a semi-major axis of 1.33\u0022 and an eccentricity of 0.46.\r\rComponent A has a stellar classification of F9 IV. It has about 2.6 times the radius of the Sun and 1.45 times the Sun\u0027s mass. This star is radiating more than six times the luminosity of the Sun at an effective temperature of 5,820 K. The secondary component is about the same size and mass as the Sun, with an effective temperature of 5,300 K. Both stars are rotating slowly. There may be a faint third member of this system, although little is known about it.\r\rThis system forms part of the Zeta Herculis moving group of stars. This group includes: \u03C62 Pavonis, \u03B6 Reticuli, 1 Hydrae, Gl 456, Gl 678, and Gl 9079.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "40 Herculis, Zeta Herculis, HIP 81693B, SAO 65485, HD 150680, GC 22464, HR 6212, DM BD+31  2884, TYC 2582-3158-2",
	"group" : { "key" : "Hercules" },
	"Common" : "Zeta Herculis",
	"OType" : "Star",
	"Distance" : "10.72",
	"RA_S" : 250.323275,
	"DEC_S" : 31.602031,
	"X" : 487,
	"Y" : 311,
	"Constellation" : "Hercules ",
	"AMag" : 5.4,
	"key" : 32903,
	"title" : "Zeta Herculis"
	},
{
	"Index" : "17176",
	"Description" : "Eta Herculis (\u03B7 Her, \u03B7 Herculis) is a fourth-magnitude star in the constellation Hercules. It has the traditional name Sophian, possibly from the Arabic \u0646\u0642\u064A meaning \u0022pure\u0022 or from the Greek \u03C3\u03BF\u03C6\u03AF\u03B1 meaning \u0022wisdom\u0022.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "44 Herculis, Eta Herculis, HIP 81833, SAO 65504, HD 150997, GC 22502, HR 6220, DM BD+39  3029, TYC 3070-1595-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Sophian",
	"OType" : "Star",
	"Distance" : "33.31",
	"RA_S" : 250.72402056,
	"DEC_S" : 38.92225677,
	"X" : 472,
	"Y" : 217,
	"Constellation" : "Hercules ",
	"AMag" : 3.577,
	"key" : 37176,
	"title" : "Sophian"
	},
{
	"Index" : "71338",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "43 Herculis, i Herculis, HIP 82073, SAO 121843, HD 151217, GC 22560, HR 6228, DM BD+08  3271, TYC 962-2225-1",
	"group" : { "key" : "Hercules" },
	"Common" : "i Herculis",
	"OType" : "Variable Star",
	"Distance" : "108.32",
	"RA_S" : 251.45788094,
	"DEC_S" : 8.58261485,
	"Constellation" : "Hercules ",
	"AMag" : 5.329,
	"key" : 91338,
	"title" : "i Herculis"
	},
{
	"Index" : "24711",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "45 Herculis, l Herculis, HIP 82216, SAO 121865, HD 151525, GC 22605, HR 6234, DM BD+05  3272, TYC 392-2704-1",
	"group" : { "key" : "Hercules" },
	"Common" : "l Herculis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "120.47",
	"RA_S" : 251.94341118,
	"DEC_S" : 5.24674443,
	"Constellation" : "Hercules ",
	"AMag" : 5.217,
	"key" : 44711,
	"title" : "l Herculis"
	},
{
	"Index" : "20973",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "52 Herculis, HIP 82321A, SAO 46305, HD 152107A, GC 22662, HR 6254, DM BD+46  2220, TYC 3500-2419-1",
	"group" : { "key" : "Hercules" },
	"Common" : "52 Herculis",
	"OType" : "Star",
	"Distance" : "55.23",
	"RA_S" : 252.3092414,
	"DEC_S" : 45.98331218,
	"Constellation" : "Hercules ",
	"AMag" : 4.838,
	"key" : 40973,
	"title" : "52 Herculis"
	},
{
	"Index" : "25087",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "47 Herculis, k Herculis, HIP 82402, SAO 121895, HD 151956, GC 22664, HR 6250, DM BD+07  3256, TYC 396-2346-1",
	"group" : { "key" : "Hercules" },
	"Common" : "k Herculis",
	"OType" : "Variable Star",
	"Distance" : "54.39",
	"RA_S" : 252.58075506,
	"DEC_S" : 7.24768382,
	"Constellation" : "Hercules ",
	"AMag" : 5.484,
	"key" : 45087,
	"title" : "k Herculis"
	},
{
	"Index" : "8763",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "51 Herculis, HIP 82504, SAO 84651, HD 152326, GC 22708, HR 6270, DM BD+24  3069, TYC 2062-1253-1",
	"group" : { "key" : "Hercules" },
	"Common" : "51 Herculis",
	"OType" : "Star",
	"Distance" : "213.51",
	"RA_S" : 252.93859387,
	"DEC_S" : 24.65643027,
	"Constellation" : "Hercules ",
	"AMag" : 5.17,
	"key" : 28763,
	"title" : "51 Herculis"
	},
{
	"Index" : "12969",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "53 Herculis, HIP 82587, SAO 65627, HD 152598, GC 22752, HR 6279, DM BD+31  2925, TYC 2589-1303-1",
	"group" : { "key" : "Hercules" },
	"Common" : "53 Herculis",
	"OType" : "High proper-motion Star",
	"Distance" : "29.19",
	"RA_S" : 253.24190807,
	"DEC_S" : 31.70167563,
	"Constellation" : "Hercules ",
	"AMag" : 5.371,
	"key" : 32969,
	"title" : "53 Herculis"
	},
{
	"Index" : "4394",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 82764, SAO 84687, HD 152815, GC 22802, HR 6287, DM BD+21 3002, TYC 1533-1175-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6287",
	"OType" : "Star",
	"Distance" : "82.68",
	"RA_S" : 253.72987851,
	"DEC_S" : 20.95849089,
	"Constellation" : "Hercules ",
	"AMag" : 5.494,
	"key" : 24394,
	"title" : "HR 6287"
	},
{
	"Index" : "12972",
	"Description" : "Epsilon Herculis (\u03B5 Her, \u03B5 Herculis) is a fourth-magnitude spectroscopic binary star in the constellation Hercules. It has the traditional name Cujam.\r\rIn Chinese, \u5929\u7D00 (Ti\u0101n J\u00EC), meaning Celestial Discipline, refers to an asterism consisting of \u03B5 Herculis, \u03BE Coronae Borealis, \u03B6 Herculis, 59 Herculis, 61 Herculis, 68 Herculis, HD 160054 and \u03B8 Herculis. Consequently, \u03B5 Herculis itself is known as \u5929\u7D00\u4E09 (Ti\u0101n J\u00EC s\u0101n, English: the Third Star of Celestial Discipline.)",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "58 Herculis, Epsilon Herculis, HIP 83207, SAO 65716, HD 153808, GC 22935, HR 6324, DM BD+31  2947, TYC 2590-1412-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Cujam",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.53",
	"RA_S" : 255.07239077,
	"DEC_S" : 30.92640766,
	"X" : 435,
	"Y" : 325,
	"Constellation" : "Hercules ",
	"AMag" : 3.895,
	"key" : 32972,
	"title" : "Cujam"
	},
{
	"Index" : "12998",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "59 Herculis, d Herculis, HIP 83313, SAO 65736, HD 154029, GC 22975, HR 6332, DM BD+33  2817, TYC 2594-1823-1",
	"group" : { "key" : "Hercules" },
	"Common" : "d Herculis",
	"OType" : "Star",
	"Distance" : "98.77",
	"RA_S" : 255.40150518,
	"DEC_S" : 33.56826917,
	"Constellation" : "Hercules ",
	"AMag" : 5.269,
	"key" : 32998,
	"title" : "d Herculis"
	},
{
	"Index" : "71482",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "32 Ophiuchi, HIP 83430, SAO 102553, HD 154143, GC 23002, HR 6337, DM BD+14  3179, TYC 988-1951-1",
	"group" : { "key" : "Hercules" },
	"Common" : "32 Ophiuchi",
	"OType" : "Variable Star",
	"Distance" : "120.92",
	"RA_S" : 255.78279907,
	"DEC_S" : 14.09194848,
	"Constellation" : "Hercules ",
	"AMag" : 5.171,
	"key" : 91482,
	"title" : "32 Ophiuchi"
	},
{
	"Index" : "71459",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "60 Herculis, HIP 83613, SAO 102584, HD 154494, GC 23061, HR 6355, DM BD+12  3142, TYC 984-2436-1",
	"group" : { "key" : "Hercules" },
	"Common" : "60 Herculis",
	"OType" : "Star",
	"Distance" : "40.85",
	"RA_S" : 256.3445431,
	"DEC_S" : 12.7408249,
	"Constellation" : "Hercules ",
	"AMag" : 4.889,
	"key" : 91459,
	"title" : "60 Herculis"
	},
{
	"Index" : "13053",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "c Herculis, HIP 83838, SAO 65812, HD 155103, GC 23132, HR 6377, DM BD+36  2827, TYC 2603-1829-1",
	"group" : { "key" : "Hercules" },
	"Common" : "c Herculis",
	"OType" : "Double or multiple star",
	"Distance" : "54.24",
	"RA_S" : 257.00860522,
	"DEC_S" : 35.93517397,
	"Constellation" : "Hercules ",
	"AMag" : 5.436,
	"key" : 33053,
	"title" : "c Herculis"
	},
{
	"Index" : "17195",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 83947, SAO 46524, HD 155410, GC 23172, HR 6388, DM BD+40 3109, TYC 3076-1566-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6388",
	"OType" : "Spectroscopic binary",
	"Distance" : "86.46",
	"RA_S" : 257.38853534,
	"DEC_S" : 40.77702932,
	"Constellation" : "Hercules ",
	"AMag" : 5.209,
	"key" : 37195,
	"title" : "HR 6388"
	},
{
	"Index" : "71496",
	"Description" : "Alpha Herculis (\u03B1 Her, \u03B1 Herculis) is a multiple star system in the constellation Hercules. It has the traditional name Rasalgethi or Ras Algethi (Arabic: \u0631\u0623\u0633 \u0627\u0644\u062C\u0627\u062B\u064A ra\u0027s al-ja\u03B8iyy\u200E Head of the Kneeler), and the Flamsteed designation 64 Herculis. The traditional name \u0022Head\u0022 comes from the fact that in antiquity Hercules was depicted upside down on the constellation maps.\r\rThe term ra\u0027s al-ja\u03B8iyy or Ras al Djathi was appeared in the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, which was translated into Latin as Caput Ingeniculi.\r\rIn Chinese astronomy, Rasalgethi is called \u5E1D\u5EA7, Pinyin: D\u00ECzu\u00F2, meaning Emperor\u0027s Seat, because this star is marking itself and stand alone in Emperor\u0027s Seat asterism, Heavenly Market enclosure (see : Chinese constellation). \u5E1D\u5EA7 (D\u00ECzu\u00F2) was westernized into Ti Tso by R.H. Allen, with the same meaning",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "64 Herculis, Alpha01 Herculis, HIP 84345A, TYC 990-2133-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Ras Algethi",
	"OType" : "Spectroscopic binary",
	"Distance" : "107.52",
	"RA_S" : 258.66188627,
	"DEC_S" : 14.39036763,
	"X" : 401,
	"Y" : 541,
	"Constellation" : "Hercules ",
	"AMag" : 3.48,
	"key" : 91496,
	"title" : "Ras Algethi"
	},
{
	"Index" : "71497",
	"Description" : "Alpha Herculis (\u03B1 Her, \u03B1 Herculis) is a multiple star system in the constellation Hercules. It has the traditional name Rasalgethi or Ras Algethi (Arabic: \u0631\u0623\u0633 \u0627\u0644\u062C\u0627\u062B\u064A ra\u0027s al-ja\u03B8iyy\u200E Head of the Kneeler), and the Flamsteed designation 64 Herculis. The traditional name \u0022Head\u0022 comes from the fact that in antiquity Hercules was depicted upside down on the constellation maps.\r\rThe term ra\u0027s al-ja\u03B8iyy or Ras al Djathi was appeared in the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, which was translated into Latin as Caput Ingeniculi.\r\rIn Chinese astronomy, Rasalgethi is called \u5E1D\u5EA7, Pinyin: D\u00ECzu\u00F2, meaning Emperor\u0027s Seat, because this star is marking itself and stand alone in Emperor\u0027s Seat asterism, Heavenly Market enclosure (see : Chinese constellation). \u5E1D\u5EA7 (D\u00ECzu\u00F2) was westernized into Ti Tso by R.H. Allen, with the same meaning",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "64 Herculis, Alpha01 Herculis, HIP 84345B, SAO 102680, HD 156014J, GC 23277, HR 6406, DM BD+14  3207A, TYC 990-2134-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Ras Algethi",
	"OType" : "Spectroscopic binary",
	"Distance" : "107.52",
	"RA_S" : 258.66190909,
	"DEC_S" : 14.39034061,
	"X" : 401,
	"Y" : 541,
	"Constellation" : "Hercules ",
	"AMag" : 2.78,
	"key" : 91497,
	"shortTitle" : "Ras Algethi; Rasalegti; Ras Al'geti",
	"title" : "Ras Algethi"
	},
{
	"Index" : "8784",
	"Description" : "Delta Herculis (\u03B4 Her, \u03B4 Herculis) is a fourth-magnitude star in the constellation Hercules. It has the traditional name Sarin.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "65 Herculis, Delta Herculis, HIP 84379, SAO 84951, HD 156164A, GC 23294, HR 6410, DM BD+25  3221, TYC 2065-1930-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Sarin",
	"OType" : "Double or multiple star",
	"Distance" : "23.04",
	"RA_S" : 258.75796339,
	"DEC_S" : 24.83920293,
	"X" : 397,
	"Y" : 406,
	"Constellation" : "Hercules ",
	"AMag" : 3.115,
	"key" : 28784,
	"title" : "Sarin"
	},
{
	"Index" : "13060",
	"Description" : "Pi Herculis (\u03C0 Her, \u03C0 Herculis) is a third-magnitude star in the constellation Hercules. As one of the four stars in the Keystone asterism (see yellow quadrangle) is one of the more easily recognized in the constellation. It has an apparent visual magnitude of +3.2, which is visible to the naked eye and makes it one of the brighter members of the constellation. The Hipparcos satellite mission estimated its distance at roughly 115 parsecs from Earth, or about 377 light years away. The overall reduction in the star\u0027s visual magnitude due to extinction from the intervening matter is 0.11.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "67 Herculis, Pi Herculis, HIP 84380, SAO 65890, HD 156283, GC 23302, HR 6418, DM BD+36  2844, TYC 2604-1774-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Pi Herculis",
	"OType" : "Variable Star",
	"Distance" : "115.45",
	"RA_S" : 258.76180626,
	"DEC_S" : 36.80916352,
	"X" : 391,
	"Y" : 250,
	"Constellation" : "Hercules ",
	"AMag" : 3.292,
	"key" : 33060,
	"title" : "Pi Herculis"
	},
{
	"Index" : "13008",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "68 Herculis, u Herculis, HIP 84573, SAO 65913, HD 156633, GC 23359, HR 6431, DM BD+33  2864, TYC 2596-1318-1",
	"group" : { "key" : "Hercules" },
	"Common" : "u Herculis",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "202.3",
	"RA_S" : 259.33152881,
	"DEC_S" : 33.10010172,
	"Constellation" : "Hercules ",
	"AMag" : 4.823,
	"key" : 33008,
	"title" : "u Herculis"
	},
{
	"Index" : "13061",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "69 Herculis, e Herculis, HIP 84606A, SAO 65921, HD 156729, GC 23374, HR 6436, DM BD+37  2864, TYC 2604-1775-1",
	"group" : { "key" : "Hercules" },
	"Common" : "e Herculis",
	"OType" : "Star",
	"Distance" : "53.77",
	"RA_S" : 259.41772651,
	"DEC_S" : 37.29149097,
	"Constellation" : "Hercules ",
	"AMag" : 4.623,
	"key" : 33061,
	"title" : "e Herculis"
	},
{
	"Index" : "8865",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 84821, SAO 85016, HD 157087, GC 23427, HR 6455, DM BD+25 3246, TYC 2078-1802-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6455",
	"OType" : "Star",
	"Distance" : "135.92",
	"RA_S" : 260.04099527,
	"DEC_S" : 25.53760929,
	"Constellation" : "Hercules ",
	"AMag" : 5.364,
	"key" : 28865,
	"title" : "HR 6455"
	},
{
	"Index" : "4449",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 84833, SAO 102757, HD 157049, GC 23426, HR 6452, DM BD+18 3351, TYC 1541-2807-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6452",
	"OType" : "Long Period Variable candidate",
	"Distance" : "146.57",
	"RA_S" : 260.07862929,
	"DEC_S" : 18.05707872,
	"Constellation" : "Hercules ",
	"AMag" : 5.2,
	"key" : 24449,
	"title" : "HR 6452"
	},
{
	"Index" : "13007",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "72 Herculis, w Herculis, HIP 84862, SAO 65963, HD 157214, GC 23446, HR 6458, DM BD+32  2896, TYC 2596-1317-1",
	"group" : { "key" : "Hercules" },
	"Common" : "w Herculis",
	"OType" : "Variable Star",
	"Distance" : "14.33",
	"RA_S" : 260.16486288,
	"DEC_S" : 32.46774663,
	"Constellation" : "Hercules ",
	"AMag" : 5.453,
	"key" : 33007,
	"title" : "w Herculis"
	},
{
	"Index" : "8866",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "70 Herculis, HIP 84887, SAO 85021, HD 157198, GC 23447, HR 6457, DM BD+24  3167, TYC 2078-1803-1",
	"group" : { "key" : "Hercules" },
	"Common" : "70 Herculis",
	"OType" : "Star",
	"Distance" : "130.82",
	"RA_S" : 260.22585693,
	"DEC_S" : 24.49943372,
	"Constellation" : "Hercules ",
	"AMag" : 5.122,
	"key" : 28866,
	"title" : "70 Herculis"
	},
{
	"Index" : "13062",
	"Description" : "Rho Herculis (\u03C1 Her, \u03C1 Herculis) is a binary star in the constellation Hercules consisting of the components rho1 Herculis and rho2 Herculis.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "75 Herculis, Rho Herculis, HIP 85112B, SAO 66000, HD 157778, GC 23543, HR 6484, DM BD+37  2878B, TYC 2604-1776-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Rho Herculis",
	"OType" : "Star",
	"Distance" : "120.4",
	"RA_S" : 260.919658,
	"DEC_S" : 37.146789,
	"X" : 369,
	"Y" : 246,
	"Constellation" : "Hercules ",
	"AMag" : 5.397,
	"key" : 33062,
	"title" : "Rho Herculis"
	},
{
	"Index" : "13063",
	"Description" : "Rho Herculis (\u03C1 Her, \u03C1 Herculis) is a binary star in the constellation Hercules consisting of the components rho1 Herculis and rho2 Herculis.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "75 Herculis, Rho Herculis, HIP 85112A, SAO 66001, HD 157779, GC 23544, HR 6485, DM BD+37  2878A, TYC 2604-1777-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Rho Herculis",
	"OType" : "Double or multiple star",
	"Distance" : "120.4",
	"RA_S" : 260.920717,
	"DEC_S" : 37.145925,
	"X" : 369,
	"Y" : 246,
	"Constellation" : "Hercules ",
	"AMag" : 4.504,
	"key" : 33063,
	"title" : "Rho Herculis"
	},
{
	"Index" : "4483",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 85385, SAO 85095, HD 158148, GC 23641, HR 6502, DM BD+20 3481, TYC 1545-2527-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6502",
	"OType" : "Star",
	"Distance" : "177.63",
	"RA_S" : 261.70470304,
	"DEC_S" : 20.08097207,
	"Constellation" : "Hercules ",
	"AMag" : 5.494,
	"key" : 24483,
	"title" : "HR 6502"
	},
{
	"Index" : "8871",
	"Description" : "Lambda Herculis (\u03BB Her, \u03BB Herculis) is a star in the constellation Hercules. It has the traditional name Maasym (\u0022wrist\u0022).\r\rIn Chinese, \u5929\u5E02\u5DE6\u57A3 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the left borderline of the enclosure, consisting of \u03BB Herculis, \u03B4 Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B6 Aquilae, \u03B81 Serpentis, \u03B7 Serpentis, \u03BD Ophiuchi, \u03BE Serpentis and \u03B7 Ophiuchi. Consequently, \u03BB Herculis itself is known as \u5929\u5E02\u5DE6\u57A3\u4E8C (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n \u00E8r, English: the Second Star of Left Wall of Heavenly Market Enclosure), represent the state Zhao (or Chaou (\u8D99))., together with 26 Capricorni and 27 Capricorni (\u0022m Capricorni\u0022 in R.H.Allen version) in Twelve States (asterism).",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "76 Herculis, Lambda Herculis, HIP 85693, SAO 85163, HD 158899, GC 23726, HR 6526, DM BD+26  3034, TYC 2079-2057-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Maasym",
	"OType" : "Variable Star",
	"Distance" : "113.17",
	"RA_S" : 262.68462423,
	"DEC_S" : 26.1106477,
	"X" : 350,
	"Y" : 390,
	"Constellation" : "Hercules ",
	"AMag" : 4.552,
	"key" : 28871,
	"shortTitle" : "Masym; Misam (also HD13994,19476)",
	"title" : "Maasym"
	},
{
	"Index" : "21078",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "82 Herculis, y Herculis, HIP 86182, SAO 46838, HD 160290, GC 23894, HR 6574, DM BD+48  2542, TYC 3513-423-1",
	"group" : { "key" : "Hercules" },
	"Common" : "y Herculis",
	"OType" : "Star",
	"Distance" : "108.28",
	"RA_S" : 264.15689042,
	"DEC_S" : 48.58563313,
	"Constellation" : "Hercules ",
	"AMag" : 5.481,
	"key" : 41078,
	"title" : "y Herculis"
	},
{
	"Index" : "21059",
	"Description" : "Iota Herculis (\u03B9 Her, \u03B9 Herculis) is a fourth-magnitude star in the constellation Hercules. The luminary shares an etymological similarity with the star Rigel in the constellation of Orion, as both stars refer to one of the feet of each mythological hero.\r\rIn Chinese, \u5929\u68D3 (Ti\u0101n B\u00E0ng), meaning Celestial Flail, refers to an asterism consisting of \u03B9 Herculis, \u03BE Draconis, \u03BD Draconis, \u03B2 Draconis and \u03B3 Draconis. Consequently, \u03B9 Herculis itself is known as \u5929\u68D3\u4E94 (Ti\u0101n B\u00E0ng wu, English: the Fifth Star of Celestial Flail.)",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "85 Herculis, Iota Herculis, HIP 86414, SAO 46872, HD 160762, GC 23965, HR 6588, DM BD+46  2349, TYC 3510-1876-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Iota Herculis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "139.42",
	"RA_S" : 264.86618548,
	"DEC_S" : 46.00632921,
	"X" : 331,
	"Y" : 131,
	"Constellation" : "Hercules ",
	"AMag" : 3.763,
	"key" : 41059,
	"title" : "Iota Herculis"
	},
{
	"Index" : "8912",
	"Description" : "Mu Herculis is a nearby star system about 27.1 light years from Earth in the constellation Hercules. Its main star, Mu Herculis A is fairly similar to the Sun although more highly evolved with a stellar classification of G5 IV. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Its mass is about 1.1 times that of the Sun, and it is beginning to expand to become a giant.\r\rThe secondary component consists of a pair of stars that orbit about each other with a period of 43.2 years. Mu Herculis A and the binary pair B-C are separated by 286 AUs. The stars B-C are separated from each other by 11.4 AUs. Their orbit is quite elliptic (e=0.18) and both stars swing each other between 9.4 and 13.5 AUs.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "86 Herculis, Mu Herculis, HIP 86974, SAO 85397, HD 161797, GC 24138, HR 6623, DM BD+27  2888, TYC 2085-3062-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Mu Herculis",
	"OType" : "Double or multiple star",
	"Distance" : "8.31",
	"RA_S" : 266.61464422,
	"DEC_S" : 27.72067433,
	"X" : 305,
	"Y" : 368,
	"Constellation" : "Hercules ",
	"AMag" : 3.49,
	"key" : 28912,
	"title" : "Mu Herculis"
	},
{
	"Index" : "8887",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "87 Herculis, HIP 87194, SAO 85437, HD 162211, GC 24199, HR 6644, DM BD+25  3353, TYC 2081-3674-1",
	"group" : { "key" : "Hercules" },
	"Common" : "87 Herculis",
	"OType" : "Star",
	"Distance" : "64.96",
	"RA_S" : 267.20478143,
	"DEC_S" : 25.62286878,
	"Constellation" : "Hercules ",
	"AMag" : 5.227,
	"key" : 28887,
	"title" : "87 Herculis"
	},
{
	"Index" : "17300",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "90 Herculis, f Herculis, HIP 87563A, SAO 47037, HD 163217, GC 24342, HR 6677, DM BD+40  3233, TYC 3093-1947-1",
	"group" : { "key" : "Hercules" },
	"Common" : "f Herculis",
	"OType" : "Star",
	"Distance" : "108.27",
	"RA_S" : 268.32513192,
	"DEC_S" : 40.00794243,
	"Constellation" : "Hercules ",
	"AMag" : 5.278,
	"key" : 37300,
	"title" : "f Herculis"
	},
{
	"Index" : "13186",
	"Description" : "Theta Herculis (\u03B8 Her, \u03B8 Herculis) is a fourth-magnitude star in the constellation Hercules. It has the traditional name Rukbalgethi Genubi. Theta Her is a variable K-type giant star with stellar classification K1IIaCN. In 1935, French astronomer P. Muller identified Theta Herculis as an irregular variable with a range of magnitudes between 3.7 and 4.1 and a periodicity of roughly 8\u20139 days.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "91 Herculis, Theta Herculis, HIP 87808, SAO 66485, HD 163770, GC 24415, HR 6695, DM BD+37  2982, TYC 2620-2298-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Rukbalgethi Genubi",
	"OType" : "Variable Star",
	"Distance" : "230.7",
	"RA_S" : 269.06325342,
	"DEC_S" : 37.2505392,
	"X" : 285,
	"Y" : 243,
	"Constellation" : "Hercules ",
	"AMag" : 3.985,
	"key" : 33186,
	"title" : "Rukbalgethi Genubi"
	},
{
	"Index" : "9051",
	"Description" : "Xi Herculis (92 Her, HD 163993, SAO 85590, HR 6703) is a star located within the constellation of Hercules. Its declination is 29\u00B0 15\u2032, its right ascension is 17h 58m, and its apparent magnitude is 3.7. Xi Herculis is about 160 light-years from Earth.\r\rThis star has 2.26 times the mass of the Sun, with a projected rotational velocity of 3.2 km s\u22121. it is radiating 62 times the luminosity of the Sun from the outer atmosphere at an effective temperature of 4,963 K.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "92 Herculis, Xi Herculis, HIP 87933, SAO 85590, HD 163993, GC 24448, HR 6703, DM BD+29  3156, TYC 2102-2772-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Xi Herculis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "41.94",
	"RA_S" : 269.44119603,
	"DEC_S" : 29.24787829,
	"X" : 274,
	"Y" : 347,
	"Constellation" : "Hercules ",
	"AMag" : 3.794,
	"key" : 29051,
	"title" : "Xi Herculis"
	},
{
	"Index" : "13094",
	"Description" : "Nu Herculis (v Her, v Herculis) star in the constellation Hercules. Nu Herculis is a F2II star approximately 243 pc from the Earth. It has an apparent magnitude of 4.41, and an absolute magnitude of -2.53. The star burns yellowish-white, and has a luminosity approximately 8,000x as bright as the sun. Nu Herculis is 5 solar masses.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "94 Herculis, Nu Herculis, HIP 87998AB, SAO 66524, HD 164136, GC 24478, HR 6707, DM BD+30  3093, TYC 2608-2411-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Nu Herculis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "260.54",
	"RA_S" : 269.62562215,
	"DEC_S" : 30.18928273,
	"X" : 272,
	"Y" : 334,
	"Constellation" : "Hercules ",
	"AMag" : 4.454,
	"key" : 33094,
	"title" : "Nu Herculis"
	},
{
	"Index" : "4565",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "93 Herculis, HIP 88128, SAO 103285, HD 164349, GC 24502, HR 6713, DM BD+16  3335, TYC 1554-2021-1",
	"group" : { "key" : "Hercules" },
	"Common" : "93 Herculis",
	"OType" : "Star",
	"Distance" : "201.31",
	"RA_S" : 270.01423021,
	"DEC_S" : 16.75091743,
	"Constellation" : "Hercules ",
	"AMag" : 4.806,
	"key" : 24565,
	"title" : "93 Herculis"
	},
{
	"Index" : "4655",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "95 Herculis, HIP 88267A, SAO 85647, HD 164668, GC 24538, HR 6729, DM BD+21  3280B, TYC 1566-3674-1",
	"group" : { "key" : "Hercules" },
	"Common" : "95 Herculis",
	"OType" : "Star",
	"Distance" : "126.25",
	"RA_S" : 270.37669898,
	"DEC_S" : 21.5957774,
	"X" : 257,
	"Y" : 446,
	"Constellation" : "Hercules ",
	"AMag" : 4.852,
	"key" : 24655,
	"title" : "95 Herculis"
	},
{
	"Index" : "4656",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "95 Herculis, HIP 88267B, SAO 85648, HD 164669, GC 24539, HR 6730, DM BD+21  3280A, TYC 1566-3675-1",
	"group" : { "key" : "Hercules" },
	"Common" : "95 Herculis",
	"OType" : "Star",
	"Distance" : "126.25",
	"RA_S" : 270.37670051,
	"DEC_S" : 21.59578012,
	"X" : 257,
	"Y" : 446,
	"Constellation" : "Hercules ",
	"AMag" : 4.96,
	"key" : 24656,
	"title" : "95 Herculis"
	},
{
	"Index" : "4657",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "96 Herculis, HIP 88331, SAO 85672, HD 164852, GC 24563, HR 6738, DM BD+20  3649, TYC 1566-3676-1",
	"group" : { "key" : "Hercules" },
	"Common" : "96 Herculis",
	"OType" : "Spectroscopic binary",
	"Distance" : "285.45",
	"RA_S" : 270.59604077,
	"DEC_S" : 20.83362848,
	"Constellation" : "Hercules ",
	"AMag" : 5.232,
	"key" : 24657,
	"title" : "96 Herculis"
	},
{
	"Index" : "4654",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "98 Herculis, HIP 88657, SAO 85725, HD 165625, GC 24670, HR 6765, DM BD+22  3273, TYC 1566-3673-1",
	"group" : { "key" : "Hercules" },
	"Common" : "98 Herculis",
	"OType" : "Variable Star",
	"Distance" : "222.82",
	"RA_S" : 271.50791627,
	"DEC_S" : 22.21888054,
	"Constellation" : "Hercules ",
	"AMag" : 5.187,
	"key" : 24654,
	"title" : "98 Herculis"
	},
{
	"Index" : "13197",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "99 Herculis, b Herculis, HIP 88745A, SAO 66648, HD 165908A, GC 24700, HR 6775, DM BD+30  3128, TYC 2621-2683-1",
	"group" : { "key" : "Hercules" },
	"Common" : "b Herculis",
	"OType" : "Double or multiple star",
	"Distance" : "15.64",
	"RA_S" : 271.756692,
	"DEC_S" : 30.561881,
	"Constellation" : "Hercules ",
	"AMag" : 5.125,
	"key" : 33197,
	"title" : "b Herculis"
	},
{
	"Index" : "17457",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 88788, SAO 47237, HD 166208, GC 24724, HR 6791, DM BD+43 2892, TYC 3114-1637-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6791",
	"OType" : "Spectroscopic binary",
	"Distance" : "124.72",
	"RA_S" : 271.86972521,
	"DEC_S" : 43.46189559,
	"Constellation" : "Hercules ",
	"AMag" : 5.099,
	"key" : 37457,
	"title" : "HR 6791"
	},
{
	"Index" : "9059",
	"Description" : "Omicron Herculis (o Her, o Herculis) is a multiple star system in the constellation Hercules. It has the traditional name Atia and the Flamsteed designation 103 Herculis.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "103 Herculis, Omicron Herculis, HIP 88794, SAO 85750, HD 166014, GC 24711, HR 6779, DM BD+28  2925, TYC 2103-3078-1",
	"group" : { "key" : "Hercules" },
	"Common" : "Atia",
	"OType" : "Be Star",
	"Distance" : "103.59",
	"RA_S" : 271.88562981,
	"DEC_S" : 28.76248822,
	"X" : 246,
	"Y" : 351,
	"Constellation" : "Hercules ",
	"AMag" : 3.823,
	"key" : 29059,
	"title" : "Atia"
	},
{
	"Index" : "4763",
	"Description" : "102 Herculis (102 Her) is a star in the constellation Hercules. Its apparent magnitude is 4.36.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "102 Herculis, HIP 88886, SAO 85769, HD 166182, GC 24740, HR 6787, DM BD+20  3674, TYC 1579-1852-1",
	"group" : { "key" : "Hercules" },
	"Common" : "102 Herculis",
	"OType" : "Star",
	"Distance" : "279.94",
	"RA_S" : 272.18954515,
	"DEC_S" : 20.81455574,
	"X" : 234,
	"Y" : 454,
	"Constellation" : "Hercules ",
	"AMag" : 4.319,
	"key" : 24763,
	"title" : "102 Herculis"
	},
{
	"Index" : "4735",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "101 Herculis, HIP 88899, SAO 85770, HD 166230, GC 24743, HR 6794, DM BD+20  3675, TYC 1575-1960-1",
	"group" : { "key" : "Hercules" },
	"Common" : "101 Herculis",
	"OType" : "Star",
	"Distance" : "100.71",
	"RA_S" : 272.22027012,
	"DEC_S" : 20.0452338,
	"Constellation" : "Hercules ",
	"AMag" : 5.121,
	"key" : 24735,
	"title" : "101 Herculis"
	},
{
	"Index" : "13205",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "104 Herculis, A Herculis, HIP 89172, SAO 66737, HD 167006, GC 24831, HR 6815, DM BD+31  3199, TYC 2622-1995-1",
	"group" : { "key" : "Hercules" },
	"Common" : "A Herculis",
	"OType" : "Variable Star",
	"Distance" : "166.68",
	"RA_S" : 272.97565424,
	"DEC_S" : 31.40535096,
	"Constellation" : "Hercules ",
	"AMag" : 5.164,
	"key" : 33205,
	"title" : "A Herculis"
	},
{
	"Index" : "9015",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "105 Herculis, HIP 89773, SAO 85921, HD 168532, GC 25003, HR 6860, DM BD+24  3381, TYC 2097-634-1",
	"group" : { "key" : "Hercules" },
	"Common" : "105 Herculis",
	"OType" : "Spectroscopic binary",
	"Distance" : "293.97",
	"RA_S" : 274.79450155,
	"DEC_S" : 24.4460597,
	"Constellation" : "Hercules ",
	"AMag" : 5.462,
	"key" : 29015,
	"title" : "105 Herculis"
	},
{
	"Index" : "4772",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "106 Herculis, HIP 89861, SAO 85941, HD 168720, GC 25033, HR 6868, DM BD+21  3390, TYC 1580-2157-1",
	"group" : { "key" : "Hercules" },
	"Common" : "106 Herculis",
	"OType" : "Variable Star",
	"Distance" : "120.02",
	"RA_S" : 275.07464627,
	"DEC_S" : 21.96129974,
	"Constellation" : "Hercules ",
	"AMag" : 5.112,
	"key" : 24772,
	"title" : "106 Herculis"
	},
{
	"Index" : "9075",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "107 Herculis, t Herculis, HIP 89935, SAO 85957, HD 168914, GC 25057, HR 6877, DM BD+28  2981, TYC 2105-2586-1",
	"group" : { "key" : "Hercules" },
	"Common" : "t Herculis",
	"OType" : "Star",
	"Distance" : "80.61",
	"RA_S" : 275.25424869,
	"DEC_S" : 28.86995524,
	"Constellation" : "Hercules ",
	"AMag" : 5.142,
	"key" : 29075,
	"title" : "t Herculis"
	},
{
	"Index" : "4708",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 90067, SAO 103655, HD 169191, GC 25093, HR 6885, DM BD+17 3555, TYC 1572-2438-1",
	"group" : { "key" : "Hercules" },
	"Common" : "HR 6885",
	"OType" : "Star",
	"Distance" : "111.08",
	"RA_S" : 275.7043321,
	"DEC_S" : 17.82661676,
	"Constellation" : "Hercules ",
	"AMag" : 5.39,
	"key" : 24708,
	"title" : "HR 6885"
	},
{
	"Index" : "4773",
	"Description" : "109 Herculis (109 Her) is a K2III orange giant star in the constellation Hercules with an apparent magnitude of 3.84 from a distance of 119 light years.\r\r109 Herculis is the lone, moderately bright, orange-red star about halfway between Vega in Lyra and Rasalhauge in Ophiuchus.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "109 Herculis, HIP 90139, SAO 86003, HD 169414, GC 25116, HR 6895, DM BD+21  3411, TYC 1580-2158-1",
	"group" : { "key" : "Hercules" },
	"Common" : "109 Herculis",
	"OType" : "Variable Star",
	"Distance" : "36.46",
	"RA_S" : 275.92454518,
	"DEC_S" : 21.76974973,
	"X" : 190,
	"Y" : 438,
	"Constellation" : "Hercules ",
	"AMag" : 3.975,
	"key" : 24773,
	"title" : "109 Herculis"
	},
{
	"Index" : "4883",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "110 Herculis, HIP 92043, SAO 86406, HD 173667, GC 25698, HR 7061, DM BD+20  3926, TYC 1591-1918-1",
	"group" : { "key" : "Hercules" },
	"Common" : "110 Herculis",
	"OType" : "Variable Star",
	"Distance" : "19.21",
	"RA_S" : 281.41552299,
	"DEC_S" : 20.54630642,
	"Constellation" : "Hercules ",
	"AMag" : 4.243,
	"key" : 24883,
	"title" : "110 Herculis"
	},
{
	"Index" : "4849",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "111 Herculis, HIP 92161, SAO 104093, HD 173880, GC 25734, HR 7069, DM BD+18  3823, TYC 1587-2067-1",
	"group" : { "key" : "Hercules" },
	"Common" : "111 Herculis",
	"OType" : "Star",
	"Distance" : "28.89",
	"RA_S" : 281.75527926,
	"DEC_S" : 18.18151474,
	"Constellation" : "Hercules ",
	"AMag" : 4.356,
	"key" : 24849,
	"title" : "111 Herculis"
	},
{
	"Index" : "4932",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "112 Herculis, HIP 92614, SAO 86521, HD 174933, GC 25895, HR 7113, DM BD+21  3582, TYC 1596-2751-1",
	"group" : { "key" : "Hercules" },
	"Common" : "112 Herculis",
	"OType" : "Spectroscopic binary",
	"Distance" : "124.1",
	"RA_S" : 283.06845073,
	"DEC_S" : 21.4251427,
	"Constellation" : "Hercules ",
	"AMag" : 5.379,
	"key" : 24932,
	"title" : "112 Herculis"
	},
{
	"Index" : "9113",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "113 Herculis, HIP 92818, SAO 86567, HD 175492J, GC 25954, HR 7133, DM BD+22  3524A, TYC 2109-2837-1",
	"group" : { "key" : "Hercules" },
	"Common" : "113 Herculis",
	"OType" : "Spectroscopic binary",
	"Distance" : "144.41",
	"RA_S" : 283.6870179,
	"DEC_S" : 22.64507578,
	"Constellation" : "Hercules ",
	"AMag" : 4.667,
	"key" : 29113,
	"title" : "113 Herculis"
	},
{
	"Index" : "65449",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Lambda Horologii, HIP 11258, SAO 248555, HD 15233, GC 2931, HR 714, DM CP-60   199, TYC 8858-1696-1",
	"group" : { "backgroundImage" : "images/Alignment/23.png",
		"description" : "Horologium is a small and faint constellation in the southern sky (declination around \u221260 degrees). Its name is Latin for clock.\r\rHorologium was created in the 18th century by Abb\u00E9 Nicolas Louis de Lacaille, who originally named it Horologium Oscillitorium after the pendulum clock to honour its inventor, Christiaan Huygens. The name has since been shortened to be less cumbersome.",
		"key" : "Horologium",
		"grouptype" : "Horologium",
		"Meaning" : "pendulum clock",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Horologium",
		"title" : "Horologium Objects Group" },
	"Common" : "Lambda Horologii",
	"OType" : "Star",
	"Distance" : "49.38",
	"RA_S" : 36.22462743,
	"DEC_S" : -60.31194697,
	"Constellation" : "Horologium ",
	"AMag" : 5.4,
	"key" : 85449,
	"title" : "Lambda Horologii"
	},
{
	"Index" : "61667",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Eta Horologii, HIP 12225, SAO 232835, HD 16555, GC 3166, HR 778, DM CP-53   457, TYC 8484-1504-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Eta Horologii",
	"OType" : "Double or multiple star",
	"Distance" : "45.42",
	"RA_S" : 39.35148879,
	"DEC_S" : -52.54312195,
	"X" : 580,
	"Y" : 351,
	"Constellation" : "Horologium ",
	"AMag" : 5.328,
	"key" : 81667,
	"title" : "Eta Horologii"
	},
{
	"Index" : "61719",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Zeta Horologii, HIP 12484, SAO 232857, HD 16920, GC 3246, HR 802, DM CP-55   446, TYC 8491-1600-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Zeta Horologii",
	"OType" : "Spectroscopic binary",
	"Distance" : "49.09",
	"RA_S" : 40.1650497,
	"DEC_S" : -54.54991192,
	"X" : 562,
	"Y" : 371,
	"Constellation" : "Horologium ",
	"AMag" : 5.257,
	"key" : 81719,
	"title" : "Zeta Horologii"
	},
{
	"Index" : "57634",
	"Description" : "Iota Horologii (\u03B9 Hor, \u03B9 Horologii) is a solar twin, yellow dwarf star approximately 56 light-years away in the constellation of Horologium (the Pendulum Clock). The star is classified as a G0Vp yellow dwarf (it has previously been classified as G3 and a subgiant [IV]). It has a mass and radius larger than the Sun, and is about 50% more luminous.\r\rAs of 1999, a single extrasolar planet is known orbiting Iota Horologii. Because the planet orbits in a near Earth orbit, Iota Horologii was ranked 69th in the list of candidates for NASA\u0027s planned Terrestrial Planet Finder mission. In 2000, a dust disc was announced around the star, but this was later determined to be an instrumental artifact.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Iota Horologii, HIP 12653, SAO 232864, HD 17051, GC 3279, HR 810, DM CD-51   641, TYC 8056-1164-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Iota Horologii",
	"OType" : "High proper-motion Star",
	"Distance" : "17.17",
	"RA_S" : 40.63944179,
	"DEC_S" : -50.8002928,
	"X" : 581,
	"Y" : 326,
	"Constellation" : "Horologium ",
	"AMag" : 5.455,
	"key" : 77634,
	"title" : "Iota Horologii"
	},
{
	"Index" : "65493",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Nu Horologii, HIP 13141, SAO 248656, HD 17848, GC 3412, HR 852, DM CP-63   188, TYC 8862-243-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Nu Horologii",
	"OType" : "High proper-motion Star",
	"Distance" : "50.45",
	"RA_S" : 42.2561957,
	"DEC_S" : -62.80652554,
	"Constellation" : "Horologium ",
	"AMag" : 5.267,
	"key" : 85493,
	"title" : "Nu Horologii"
	},
{
	"Index" : "65492",
	"Description" : "Beta Horologii (Beta Hor, \u03B2 Horologii, \u03B2 Hor) is the third brightest star in the constellation of Horologium. It is an A-type giant star with an apparent visual magnitude of approximately 4.979, and is a chemically peculiar star of the metallic-line type.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Beta Horologii, HIP 13884, SAO 248701, HD 18866, GC 3611, HR 909, DM CP-64   215, TYC 8862-1490-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Beta Horologii",
	"OType" : "Star",
	"Distance" : "90.3",
	"RA_S" : 44.6991483,
	"DEC_S" : -64.07128778,
	"X" : 496,
	"Y" : 459,
	"Constellation" : "Horologium ",
	"AMag" : 4.986,
	"key" : 85492,
	"title" : "Beta Horologii"
	},
{
	"Index" : "61762",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Mu Horologii, HIP 14240, SAO 232981, HD 19319, GC 3694, HR 934, DM CP-60   236, TYC 8498-1351-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Mu Horologii",
	"OType" : "Star",
	"Distance" : "43.4",
	"RA_S" : 45.90341868,
	"DEC_S" : -59.73777581,
	"X" : 494,
	"Y" : 413,
	"Constellation" : "Horologium ",
	"AMag" : 5.163,
	"key" : 81762,
	"title" : "Mu Horologii"
	},
{
	"Index" : "53436",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Delta Horologii, HIP 19515AB, SAO 216682, HD 26612, GC 5051, HR 1302, DM CD-42  1400, TYC 7580-1257-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Delta Horologii",
	"OType" : "Double or multiple star",
	"Distance" : "54.79",
	"RA_S" : 62.71076282,
	"DEC_S" : -41.99357969,
	"Constellation" : "Horologium ",
	"AMag" : 4.97,
	"key" : 73436,
	"title" : "Delta Horologii"
	},
{
	"Index" : "53442",
	"Description" : "Alpha Horologii (\u03B1 Hor, \u03B1 Horologii) is a giant yellow star in the constellation Horologium.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Alpha Horologii, HIP 19747, SAO 216710, HD 26967, GC 5121, HR 1326, DM CD-42  1425, TYC 7581-1600-1",
	"group" : { "key" : "Horologium" },
	"Common" : "Alpha Horologii",
	"OType" : "High proper-motion Star",
	"Distance" : "35.26",
	"RA_S" : 63.50047329,
	"DEC_S" : -42.2943709,
	"X" : 422,
	"Y" : 154,
	"Constellation" : "Horologium ",
	"AMag" : 3.966,
	"key" : 73442,
	"title" : "Alpha Horologii"
	},
{
	"Index" : "53476",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 20161, SAO 216749, HD 27588, GC 5250, HR 1364, DM CD-44 1503, TYC 7584-1675-1",
	"group" : { "key" : "Horologium" },
	"Common" : "HR 1364",
	"OType" : "Star",
	"Distance" : "77.26",
	"RA_S" : 64.81957142,
	"DEC_S" : -44.2679168,
	"Constellation" : "Horologium ",
	"AMag" : 5.451,
	"key" : 73476,
	"title" : "HR 1364"
	},
{
	"Index" : "36946",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 40107, SAO 135611, HD 68312, GC 11138, HR 3212, DM BD-07 2378, TYC 5426-3213-1",
	"group" : { "backgroundImage" : "images/Alignment/28.png",
		"description" : "Hydra is the largest of the 88 modern constellations, measuring 1303 square degrees. Also one of the longest at over 100 degrees, its southern end abuts Libra and Centaurus and its northern end borders Cancer. It has a long history, having been included among the 48 constellations listed by the 2nd century astronomer Ptolemy. It is commonly represented as a water snake. It should not be confused with the similarly named constellation of Hydrus.\r\rThe Greek constellation of Hydra is an adaptation of a Babylonian constellation: the MUL.APIN includes a \u0022serpent\u0022 constellation (MUL.DINGIR.MU\u0160) that loosely corresponds to Hydra. It is one of two Babylonian \u0022serpent\u0022 constellations (the other being the origin of the Greek Serpens), a mythological hybrid of serpent, lion and bird.\r\rThe shape of Hydra resembles a twisting snake, and features as such in some Greek myths. One myth associates it with a water snake that a crow served Apollo in a cup when it was sent to fetch water; Apollo saw through the fraud, and angrily cast the crow, cup, and snake, into the sky. It is also associated with the monster Hydra, with its many heads, killed by Hercules, represented in another constellation.",
		"key" : "Hydra",
		"grouptype" : "Hydra",
		"Meaning" : "Hydra (mythological creature)",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Hydra",
		"title" : "Hydra Objects Group" },
	"Common" : "HR 3212",
	"OType" : "Star",
	"Distance" : "89.06",
	"RA_S" : 122.88751671,
	"DEC_S" : -7.77253689,
	"Constellation" : "Hydra ",
	"AMag" : 5.455,
	"key" : 56946,
	"title" : "HR 3212"
	},
{
	"Index" : "32823",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "C Hydrae, HIP 41307, SAO 135896, HD 71155, GC 11499, HR 3314, DM BD-03  2339, TYC 4857-2151-1",
	"group" : { "key" : "Hydra" },
	"Common" : "C Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "37.51",
	"RA_S" : 126.41513338,
	"DEC_S" : -3.90642162,
	"Constellation" : "Hydra ",
	"AMag" : 3.876,
	"key" : 52823,
	"title" : "C Hydrae"
	},
{
	"Index" : "10264",
	"Description" : "Delta Hydrae (\u03B4 Hya, \u03B4 Hydrae) is a Class A1, fourth-magnitude star in the constellation Hydra. Delta Hydrae is a binary double star, located about 180 light-years from Earth. It has 2.2 times the mass of the Sun, 1.5 times the Sun\u0027s radius and is radiating 17 times the luminosity of the Sun.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Lisan al Shudja, which was translated into Latin as Lingua Hydri, meaning the snake\u0027s tongue. This star, along with \u03B5 Hya, \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija), were Ulugh Beg\u0027s Min al Az\u02BDal, \u0022Belonging to the Uninhabited Spot\u0022.\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Min al Az\u02BDal or Minazal were the title for five stars :\u03B4 Hya as Minazal I, \u03B7 Hya as Minazal II, \u03B5 Hya as Minazal III, \u03C1 Hya as Minazal IV and \u03B6 Hya as Minazal V (exclude \u03C3 Hya)\r\rIn Chinese, \u67F3\u5BBF (Li\u01D4 S\u00F9), meaning Willow (asterism), refers to an asterism consisting of \u03B4 Hydrae, \u03C3 Hydrae, \u03B7 Hydrae, \u03C1 Hydrae, \u03B5 Hydrae, \u03B6 Hydrae, \u03C9 Hydrae and \u03B8 Hydrae Consequently, \u03B4 Hydrae itself is known as \u67F3\u5BBF\u4E00 (Li\u01D4 S\u00F9 y\u012B, English: the First Star of Willow.)\r\rThe people of Groote Eylandt called Unwala, \u0022The Crab\u0022, for the star cluster including this star, \u03B5 Hya, \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija).",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "4 Hydrae, Delta Hydrae, HIP 42313, SAO 116965, HD 73262, GC 11823, HR 3410, DM BD+06  2001, TYC 223-1795-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Delta Hydrae",
	"OType" : "Double or multiple star",
	"Distance" : "49.11",
	"RA_S" : 129.41403201,
	"DEC_S" : 5.70378462,
	"X" : 602,
	"Y" : 94,
	"Constellation" : "Hydra ",
	"AMag" : 4.132,
	"key" : 30264,
	"title" : "Delta Hydrae"
	},
{
	"Index" : "9579",
	"Description" : "Sigma Hydrae (\u03C3 Hydrae, \u03C3 Hya) is the 4th-magnitude star in the constellation Hydra. Sigma Hydrae belongs to spectral class K1+III and has apparent magnitude +4.44. It is approximately 353 light years from Earth\r\rIt is also known by the proper name Minchir, and appears as Minchir es-schudscha\u0027 on Bode\u0027s large star atlas, Uranographia, which is derived from the Arabic Minkhir al-Shuja\u0027, \u0022the Nostril of Hydra\u0022, for this star. The name is erroneously spelt as Al Minliar al Shuja in the Yale Bright Star Catalogue..\r\rThis star, along with \u03B4 Hya (Lisan al Shudja), \u03B5 Hya, \u03B6 Hya, \u03B7 Hya and \u03C1 Hya, were Ulug Beg\u0027s Min al Az\u02BDal, \u0022Belonging to the Uninhabited Spot\u0022.\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Min al Az\u02BDal or Minazal were the title for five stars : \u03B4 Hya as Minazal I, \u03B7 Hya as Minazal II, \u03B5 Hya as Minazal III, \u03C1 Hya as Minazal IV and \u03B6 Hya as Minazal V (exclude this star)\r\rIn Chinese, \u67F3\u5BBF (Li\u01D4 S\u00F9), meaning Willow (asterism), refers to an asterism consisting of \u03C3 Hydrae, \u03B4 Hydrae, \u03B7 Hydrae, \u03C1 Hydrae, \u03B5 Hydrae, \u03B6 Hydrae, \u03C9 Hydrae and \u03B8 Hydrae Consequently, \u03C3 Hydrae itself is known as \u67F3\u5BBF\u4E8C (Li\u01D4 S\u00F9 \u00E8r, English: the Second Star of Willow.).\r\rThe people of Groote Eylandt, called Unwala, \u0022The Crab\u0022, for the star cluster including this star, \u03B4 Hya (Lisan al Shudja), \u03B5 Hya, \u03B6 Hya, \u03B7 Hya and \u03C1 Hya.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "5 Hydrae, Sigma Hydrae, HIP 42402, SAO 116988, HD 73471, GC 11856, HR 3418, DM BD+03  2026, TYC 215-2022-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Minchir",
	"OType" : "Star",
	"Distance" : "114.17",
	"RA_S" : 129.68932288,
	"DEC_S" : 3.34143606,
	"X" : 607,
	"Y" : 116,
	"Constellation" : "Hydra ",
	"AMag" : 4.577,
	"key" : 29579,
	"shortTitle" : "Minchir",
	"title" : "Minchir"
	},
{
	"Index" : "37039",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "6 Hydrae, a Hydrae, HIP 42509, SAO 154515, HD 73840, GC 11908, HR 3431, DM BD-11  2420, TYC 5437-2459-1",
	"group" : { "key" : "Hydra" },
	"Common" : "a Hydrae",
	"OType" : "Star",
	"Distance" : "118.9",
	"RA_S" : 130.00613293,
	"DEC_S" : -12.47537354,
	"Constellation" : "Hydra ",
	"AMag" : 5.135,
	"key" : 57039,
	"title" : "a Hydrae"
	},
{
	"Index" : "41324",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "9 Hydrae, HIP 42662, SAO 154552, HD 74137, GC 11959, HR 3441, DM BD-15  2554, TYC 6012-1921-1",
	"group" : { "key" : "Hydra" },
	"Common" : "9 Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "64.92",
	"RA_S" : 130.43056815,
	"DEC_S" : -15.9433864,
	"Constellation" : "Hydra ",
	"AMag" : 4.983,
	"key" : 61324,
	"title" : "9 Hydrae"
	},
{
	"Index" : "9578",
	"Description" : "Eta Hydrae (\u03B7 Hya) is a star in the constellation Hydra. Its apparent magnitude is 4.30.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "7 Hydrae, Eta Hydrae, HIP 42799, SAO 117050, HD 74280, GC 11987, HR 3454, DM BD+03  2039, TYC 215-2021-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Eta Hydrae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "179.45",
	"RA_S" : 130.80614591,
	"DEC_S" : 3.39866074,
	"X" : 597,
	"Y" : 117,
	"Constellation" : "Hydra ",
	"AMag" : 4.248,
	"key" : 29578,
	"title" : "Eta Hydrae"
	},
{
	"Index" : "32952",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "F Hydrae, HIP 42835, SAO 136221, HD 74395, GC 12006, HR 3459, DM BD-06  2708, TYC 4875-1585-1",
	"group" : { "key" : "Hydra" },
	"Common" : "F Hydrae",
	"OType" : "Star",
	"Distance" : "234.71",
	"RA_S" : 130.91821969,
	"DEC_S" : -7.23372719,
	"Constellation" : "Hydra ",
	"AMag" : 4.716,
	"key" : 52952,
	"title" : "F Hydrae"
	},
{
	"Index" : "37180",
	"Description" : "12 Hydrae (12 Hya) is a star in the constellation Hydra. Its apparent magnitude is 4.33.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "12 Hydrae, D Hydrae, HIP 43067, SAO 154622, HD 74918, GC 12097, HR 3484, DM BD-13  2673, TYC 5454-1870-1",
	"group" : { "key" : "Hydra" },
	"Common" : "12 Hydrae",
	"OType" : "Star",
	"Distance" : "74.76",
	"RA_S" : 131.59391378,
	"DEC_S" : -13.54773459,
	"X" : 625,
	"Y" : 269,
	"Constellation" : "Hydra ",
	"AMag" : 4.402,
	"key" : 57180,
	"title" : "12 Hydrae"
	},
{
	"Index" : "10327",
	"Description" : "Epsilon Hydrae (\u03B5 Hya, \u03B5 Hydrae) is a Class G5, third-magnitude star system in the constellation Hydra. This stellar system is located about 129 light-years (40 parsecs) 135 light-years from Earth.\r\rIt is a multiple star system having at least four stellar components. The pair \u03B5 Hya AB form a binary star with an orbital period of 15 years and an angular separation of 0.2 arcseconds. Component \u03B5 Hya C is separated from the AB pair by 3 arcseconds. It is a spectroscopic binary system with a period of 9.9047 days and an orbital eccentricity of 0.62, while simultaneously orbiting \u03B5 Hya AB with a period of 870 years. The fourth component, \u03B5 Hya D, shares a common proper motion with the other components and thus is most likely a gravitationally-bound member of the system. It is separated from the AB pair by 19 arcseconds and has an estimated orbital period of around 10,000 years.\r\rThe primary, \u03B5 Hya A, is a giant star that is shining with 67 times the luminosity of the Sun. This energy is being radiated from the star\u0027s outer atmosphere at an effective temperature of 5,620 K, giving it the yellow hue of a G-type star. It is rotating rapidly with a projected rotational velocity of 19 km s\u20131. It has an X-ray luminosity of 2.8 \u00D7 1029 erg s\u20131.\r\rThis star, along with \u03B4 Hya (Lisan al Sudja), \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija), were Ulug Beg\u0027s Min al Az\u02BDal, \u0022Belonging to the Uninhabited Spot\u0022.\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Min al Az\u02BDal or Minazal were the title for five stars:\u03B4 Hya as Minazal I, \u03B7 Hya as Minazal II, \u03B5 Hya as Minazal III, \u03C1 Hya as Minazal IV and \u03B6 Hya as Minazal V (exclude \u03C3 Hya)\r\rIn Chinese, \u67F3\u5BBF (Li\u01D4 S\u00F9), meaning Willow (asterism), refers to an asterism consisting of \u03B5 Hydrae, \u03B4 Hydra, \u03C3 Hydrae, \u03B7 Hydrae, \u03C1 Hydrae, \u03B6 Hydrae, \u03C9 Hydrae and \u03B8 Hydrae Consequently, \u03B5 Hydrae itself is known as \u67F3\u5BBF\u4E94 (Li\u01D4 S\u00F9 w\u01D4, English: the Fifth Star of Willow.)\r\rIn ancient Indian astronomy, the five-star cluster of Hydrae is collectively called Ashlesha (Ayilyam in southern India) Nakshatras\r\rThe people of Groote Eylandt called Unwala, \u0022The Crab\u0022, for the star cluster including this star, \u03B4 Hya (Lisan al Sudja), \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija).",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "11 Hydrae, Epsilon Hydrae, HIP 43109C, SAO 117112, HD 74874, GC 12102, HR 3482, DM BD+06  2036, TYC 224-1333-2",
	"group" : { "key" : "Hydra" },
	"Common" : "Epsilon Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "39.56",
	"RA_S" : 131.692971,
	"DEC_S" : 6.419231,
	"X" : 581,
	"Y" : 92,
	"Constellation" : "Hydra ",
	"AMag" : 6.665,
	"key" : 30327,
	"title" : "Epsilon Hydrae"
	},
{
	"Index" : "10326",
	"Description" : "Epsilon Hydrae (\u03B5 Hya, \u03B5 Hydrae) is a Class G5, third-magnitude star system in the constellation Hydra. This stellar system is located about 129 light-years (40 parsecs) 135 light-years from Earth.\r\rIt is a multiple star system having at least four stellar components. The pair \u03B5 Hya AB form a binary star with an orbital period of 15 years and an angular separation of 0.2 arcseconds. Component \u03B5 Hya C is separated from the AB pair by 3 arcseconds. It is a spectroscopic binary system with a period of 9.9047 days and an orbital eccentricity of 0.62, while simultaneously orbiting \u03B5 Hya AB with a period of 870 years. The fourth component, \u03B5 Hya D, shares a common proper motion with the other components and thus is most likely a gravitationally-bound member of the system. It is separated from the AB pair by 19 arcseconds and has an estimated orbital period of around 10,000 years.\r\rThe primary, \u03B5 Hya A, is a giant star that is shining with 67 times the luminosity of the Sun. This energy is being radiated from the star\u0027s outer atmosphere at an effective temperature of 5,620 K, giving it the yellow hue of a G-type star. It is rotating rapidly with a projected rotational velocity of 19 km s\u20131. It has an X-ray luminosity of 2.8 \u00D7 1029 erg s\u20131.\r\rThis star, along with \u03B4 Hya (Lisan al Sudja), \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija), were Ulug Beg\u0027s Min al Az\u02BDal, \u0022Belonging to the Uninhabited Spot\u0022.\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Min al Az\u02BDal or Minazal were the title for five stars:\u03B4 Hya as Minazal I, \u03B7 Hya as Minazal II, \u03B5 Hya as Minazal III, \u03C1 Hya as Minazal IV and \u03B6 Hya as Minazal V (exclude \u03C3 Hya)\r\rIn Chinese, \u67F3\u5BBF (Li\u01D4 S\u00F9), meaning Willow (asterism), refers to an asterism consisting of \u03B5 Hydrae, \u03B4 Hydra, \u03C3 Hydrae, \u03B7 Hydrae, \u03C1 Hydrae, \u03B6 Hydrae, \u03C9 Hydrae and \u03B8 Hydrae Consequently, \u03B5 Hydrae itself is known as \u67F3\u5BBF\u4E94 (Li\u01D4 S\u00F9 w\u01D4, English: the Fifth Star of Willow.)\r\rIn ancient Indian astronomy, the five-star cluster of Hydrae is collectively called Ashlesha (Ayilyam in southern India) Nakshatras\r\rThe people of Groote Eylandt called Unwala, \u0022The Crab\u0022, for the star cluster including this star, \u03B4 Hya (Lisan al Sudja), \u03B6 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija).",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "11 Hydrae, Epsilon Hydrae, HIP 43109A, SAO 117112, HD 74874, GC 12102, HR 3482, DM BD+06  2036, TYC 224-1333-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Epsilon Hydrae",
	"OType" : "Star",
	"Distance" : "39.56",
	"RA_S" : 131.69386615,
	"DEC_S" : 6.41877721,
	"X" : 581,
	"Y" : 92,
	"Constellation" : "Hydra ",
	"AMag" : 3.488,
	"key" : 30326,
	"title" : "Epsilon Hydrae"
	},
{
	"Index" : "32896",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 43142, SAO 136276, HD 74988, GC 12122, HR 3486, DM BD-01 2130, TYC 4868-1766-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 3486",
	"OType" : "Star",
	"Distance" : "122.38",
	"RA_S" : 131.81244213,
	"DEC_S" : -1.89703965,
	"Constellation" : "Hydra ",
	"AMag" : 5.284,
	"key" : 52896,
	"title" : "HR 3486"
	},
{
	"Index" : "10328",
	"Description" : "Rho Hydrae (\u03C1 Hya) is a star in the constellation Hydra. Its apparent magnitude is 4.34.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "13 Hydrae, Rho Hydrae, HIP 43234, SAO 117146, HD 75137, GC 12148, HR 3492, DM BD+06  2040, TYC 224-1334-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Rho Hydrae",
	"OType" : "Star",
	"Distance" : "108.51",
	"RA_S" : 132.10820769,
	"DEC_S" : 5.83781082,
	"X" : 579,
	"Y" : 98,
	"Constellation" : "Hydra ",
	"AMag" : 4.332,
	"key" : 30328,
	"title" : "Rho Hydrae"
	},
{
	"Index" : "32897",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "14 Hydrae, HIP 43305, SAO 136308, HD 75333, GC 12172, HR 3500, DM BD-02  2699, TYC 4868-1768-1",
	"group" : { "key" : "Hydra" },
	"Common" : "14 Hydrae",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "137.94",
	"RA_S" : 132.34052389,
	"DEC_S" : -3.44302426,
	"Constellation" : "Hydra ",
	"AMag" : 5.272,
	"key" : 52897,
	"title" : "14 Hydrae"
	},
{
	"Index" : "10381",
	"Description" : "Zeta Hydrae (\u03B6 Hya, \u03B6 Hydrae) is a solitary star in the equatorial constellation of Hydra. This is a generally faint constellation, so, at an apparent visual magnitude of +3.10, this is the third brightest member after Alphard and Gamma Hydrae. The distance to this star has been measured using the parallax technique, yielding a value of roughly 167 light-years (51 parsecs). At this distance, the visual magnitude of the star is diminished by 0.03 as a result of extinction from intervening gas and dust. The star Delta Hydrae is located 12.9 light-years (4.0 parsecs) from Zeta Hydrae and may be a co-moving companion.\r\rWith a stellar classification of G9 II-III, this is an evolved giant star that is radiating 132 times the luminosity of the Sun from its outer envelope at an effective temperature of 4,925 K. At this heat, the star glows with the yellow hue of a G-type star. The radius of this star, as measured using interferometry, is about 18 times the Sun\u0027s radius. It has an estimated 4.2 times the mass of the Sun and is around 400 million years old.\r\rThis star, along with \u03B4 Hya (Lisan al Sudja), \u03B5 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija), were Ulug Beg\u0027s Min al Az\u02BDal, \u0022Belonging to the Uninhabited Spot\u0022. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Min al Az\u02BDal or Minazal were the title for five stars:\u03B4 Hya as Minazal I, \u03B7 Hya as Minazal II, \u03B5 Hya as Minazal III, \u03C1 Hya as Minazal IV and \u03B6 Hya as Minazal V (exclude \u03C3 Hya).\r\rIn Chinese, \u67F3\u5BBF (Li\u01D4 S\u00F9), meaning Willow, refers to an asterism consisting of \u03B6 Hydrae, \u03B4 Hydra, \u03C3 Hydrae, \u03B7 Hydrae, \u03C1 Hydrae, \u03B5 Hydrae, \u03C9 Hydrae and \u03B8 Hydrae Consequently, \u03B6 Hydrae itself is known as \u67F3\u5BBF\u516D (Li\u01D4 S\u00F9 li\u00F9, English: the Sixth Star of Willow).\r\rThe people of Groote Eylandt called Unwala, \u0022The Crab\u0022, for the star cluster including this star, \u03B4 Hya (Lisan al Sudja), \u03B5 Hya, \u03B7 Hya, \u03C1 Hya and \u03C3 Hya (Minhar al Shija).",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "16 Hydrae, Zeta Hydrae, HIP 43813, SAO 117264, HD 76294, GC 12327, HR 3547, DM BD+06  2060, TYC 225-1116-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Zeta Hydrae",
	"OType" : "Star",
	"Distance" : "51.25",
	"RA_S" : 133.8484958,
	"DEC_S" : 5.94550965,
	"X" : 564,
	"Y" : 100,
	"Constellation" : "Hydra ",
	"AMag" : 3.21,
	"key" : 30381,
	"title" : "Zeta Hydrae"
	},
{
	"Index" : "10894",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "18 Hydrae, Omega Hydrae, HIP 44659, SAO 117420, HD 77996, GC 12564, HR 3613, DM BD+05  2116, TYC 232-2195-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Omega Hydrae",
	"OType" : "Star",
	"Distance" : "272.35",
	"RA_S" : 136.49319291,
	"DEC_S" : 5.09231801,
	"Constellation" : "Hydra ",
	"AMag" : 5.12,
	"key" : 30894,
	"title" : "Omega Hydrae"
	},
{
	"Index" : "10548",
	"Description" : "Theta Hydrae (\u03B8 Hya) is a star in the constellation Hydra. Its apparent magnitude is 3.88.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "22 Hydrae, Theta Hydrae, HIP 45336, SAO 117527, HD 79469, GC 12743, HR 3665, DM BD+02  2167, TYC 227-2544-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Theta Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "39.39",
	"RA_S" : 138.59111115,
	"DEC_S" : 2.31427285,
	"X" : 534,
	"Y" : 141,
	"Constellation" : "Hydra ",
	"AMag" : 3.853,
	"key" : 30548,
	"title" : "Theta Hydrae"
	},
{
	"Index" : "37214",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "24 Hydrae, HIP 45526, SAO 136728, HD 79931, GC 12802, HR 3683, DM BD-08  2623, TYC 5458-1843-1",
	"group" : { "key" : "Hydra" },
	"Common" : "24 Hydrae",
	"OType" : "Star",
	"Distance" : "206.44",
	"RA_S" : 139.17236562,
	"DEC_S" : -8.74475686,
	"Constellation" : "Hydra ",
	"AMag" : 5.456,
	"key" : 57214,
	"title" : "24 Hydrae"
	},
{
	"Index" : "33059",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "23 Hydrae, HIP 45527, SAO 136725, HD 79910, GC 12800, HR 3681, DM BD-05  2762, TYC 4892-1405-1",
	"group" : { "key" : "Hydra" },
	"Common" : "23 Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "75.1",
	"RA_S" : 139.17389971,
	"DEC_S" : -6.35314797,
	"Constellation" : "Hydra ",
	"AMag" : 5.362,
	"key" : 53059,
	"title" : "23 Hydrae"
	},
{
	"Index" : "37275",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "26 Hydrae, HIP 45751, SAO 155096, HD 80499, GC 12867, HR 3706, DM BD-11  2609, TYC 5467-1858-1",
	"group" : { "key" : "Hydra" },
	"Common" : "26 Hydrae",
	"OType" : "Double or multiple star",
	"Distance" : "102.91",
	"RA_S" : 139.94325847,
	"DEC_S" : -11.9748508,
	"Constellation" : "Hydra ",
	"AMag" : 4.873,
	"key" : 57275,
	"title" : "26 Hydrae"
	},
{
	"Index" : "37245",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "27 Hydrae, P Hydrae, HIP 45811, SAO 136768, HD 80586, GC 12881, HR 3709, DM BD-08  2643, TYC 5463-1514-1",
	"group" : { "key" : "Hydra" },
	"Common" : "P Hydrae",
	"OType" : "Star",
	"Distance" : "68.18",
	"RA_S" : 140.12091052,
	"DEC_S" : -9.55569885,
	"Constellation" : "Hydra ",
	"AMag" : 4.915,
	"key" : 57245,
	"title" : "P Hydrae"
	},
{
	"Index" : "41504",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "G Hydrae, HIP 46371, SAO 177469, HD 81799, GC 13043, HR 3749, DM BD-21  2802, TYC 6041-1680-1",
	"group" : { "key" : "Hydra" },
	"Common" : "G Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "47.76",
	"RA_S" : 141.82671753,
	"DEC_S" : -22.3438022,
	"Constellation" : "Hydra ",
	"AMag" : 4.849,
	"key" : 61504,
	"title" : "G Hydrae"
	},
{
	"Index" : "33066",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 46404AB, SAO 136872, HD 81809A, HR 3750, DM BD-05 2802, TYC 4893-1379-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 3750",
	"OType" : "High proper-motion Star",
	"Distance" : "30.39",
	"RA_S" : 141.94494627,
	"DEC_S" : -6.07123431,
	"Constellation" : "Hydra ",
	"AMag" : 5.483,
	"key" : 53066,
	"title" : "HR 3750"
	},
{
	"Index" : "33025",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "31 Hydrae, Tau01 Hydrae, HIP 46509, SAO 136895, HD 81997, GC 13080, HR 3759, DM BD-02  2901, TYC 4885-1568-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Tau01 Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "17.31",
	"RA_S" : 142.28706895,
	"DEC_S" : -2.76896247,
	"Constellation" : "Hydra ",
	"AMag" : 4.64,
	"key" : 53025,
	"title" : "Tau01 Hydrae"
	},
{
	"Index" : "33073",
	"Description" : "The Bayer designation Tau Hydrae (\u03C4 Hya, \u03C4 Hydrae) is shared by two star systems, \u03C4\u00B9 Hydrae and \u03C4\u00B2 Hydrae, in the constellation Hydra. The two stars are separated by 1.74\u00B0 in the sky.\r\rThis star (\u03C4\u00B9 Hya and \u03C4\u00B2 Hya), along with \u03B9 Hya and the 5th\u2011magnitude 33 Hya (A Hydrae}, were Ptolemy\u0027s \u039A\u03B1\u03BC\u03C0\u03AE (Kamp\u0113); but Kazwini knew them as \u02BDU\u1E33dah, the Knot. Tau-2 Hydrae is a spectral type A3 main sequence star which has an apparent magnitude of +4.54. It is about 460 light years from Earth.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "32 Hydrae, Tau02 Hydrae, HIP 46776, SAO 136932, HD 82446, GC 13153, HR 3787, DM BD-00  2211, TYC 4894-2528-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Tau2 Hydrae",
	"OType" : "Star",
	"Distance" : "156.28",
	"RA_S" : 142.99552229,
	"DEC_S" : -1.18466713,
	"X" : 506,
	"Y" : 179,
	"Constellation" : "Hydra ",
	"AMag" : 4.562,
	"key" : 53073,
	"title" : "Tau2 Hydrae"
	},
{
	"Index" : "41516",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 46880, SAO 177642, HD 82734, GC 13191, HR 3808, DM BD-20 2936, TYC 6042-1585-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Gliese 355.2 (HR 3808)",
	"OType" : "Star",
	"Distance" : "111.01",
	"RA_S" : 143.30191698,
	"DEC_S" : -21.11572169,
	"Constellation" : "Hydra ",
	"AMag" : 5.117,
	"key" : 61516,
	"title" : "Gliese 355.2 (HR 3808)"
	},
{
	"Index" : "11277",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "2 Sextantis, HIP 47310, SAO 117821, HD 83425, GC 13316, HR 3834, DM BD+05  2207, TYC 238-2476-1",
	"group" : { "key" : "Hydra" },
	"Common" : "2 Sextantis",
	"OType" : "High proper-motion Star",
	"Distance" : "90.51",
	"RA_S" : 144.61369721,
	"DEC_S" : 4.64929342,
	"Constellation" : "Hydra ",
	"AMag" : 4.818,
	"key" : 31277,
	"title" : "2 Sextantis"
	},
{
	"Index" : "33074",
	"Description" : "Iota Hydrae (\u03B9 Hya) is a star in the constellation Hydra. Its apparent magnitude is 3.91.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "35 Hydrae, Iota Hydrae, HIP 47431, SAO 137035, HD 83618, GC 13341, HR 3845, DM BD-00  2231, TYC 4894-2529-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Iota Hydrae",
	"OType" : "Variable Star",
	"Distance" : "80.7",
	"RA_S" : 144.96400696,
	"DEC_S" : -1.14280908,
	"X" : 489,
	"Y" : 183,
	"Constellation" : "Hydra ",
	"AMag" : 4.036,
	"key" : 53074,
	"title" : "Iota Hydrae"
	},
{
	"Index" : "37305",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "38 Hydrae, Kappa Hydrae, HIP 47452, SAO 155388, HD 83754, GC 13354, HR 3849, DM BD-13  2917, TYC 5473-1229-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Kappa Hydrae",
	"OType" : "Variable Star",
	"Distance" : "133.43",
	"RA_S" : 145.07651319,
	"DEC_S" : -14.33229143,
	"Constellation" : "Hydra ",
	"AMag" : 5.029,
	"key" : 57305,
	"title" : "Kappa Hydrae"
	},
{
	"Index" : "45876",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "I Hydrae, HIP 47522, SAO 177840, HD 83953, GC 13373, HR 3858, DM BD-22  2684, TYC 6602-2080-1",
	"group" : { "key" : "Hydra" },
	"Common" : "I Hydrae",
	"OType" : "Be Star",
	"Distance" : "155.1",
	"RA_S" : 145.32086139,
	"DEC_S" : -23.59151217,
	"Constellation" : "Hydra ",
	"AMag" : 4.736,
	"key" : 65876,
	"title" : "I Hydrae"
	},
{
	"Index" : "45877",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 47592, SAO 177866, HD 84117, GC 13394, HR 3862, DM CD-23 8646, TYC 6602-2081-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Gliese 364.0",
	"OType" : "High proper-motion Star",
	"Distance" : "15.01",
	"RA_S" : 145.56006694,
	"DEC_S" : -23.91556854,
	"Constellation" : "Hydra ",
	"AMag" : 4.984,
	"key" : 65877,
	"title" : "Gliese 364.0"
	},
{
	"Index" : "37374",
	"Description" : "Upsilon1 Hydrae is a yellow giant star in the constellation of Hydra. The star is one of Okayama Planet Search\u0027s main target for planet search and has turned out to host a substellar companion.\r\rThe Okayama Planet Search team published a paper in 2005 reporting investigations on radial velocity variations observed for a set of orange giant stars and announcing the detection of a brown dwarf companion in an eccentric orbit around Upsilon1 Hydrae. The orbital period is roughly 4.1 years.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "39 Hydrae, Upsilon01 Hydrae, HIP 48356, SAO 155542, HD 85444, GC 13570, HR 3903, DM BD-14  2963, TYC 5487-1653-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Upsilon1 Hydrae",
	"OType" : "Star",
	"Distance" : "80.86",
	"RA_S" : 147.8695551,
	"DEC_S" : -14.84661184,
	"X" : 496,
	"Y" : 304,
	"Constellation" : "Hydra ",
	"AMag" : 4.21,
	"key" : 57374,
	"title" : "Upsilon1 Hydrae"
	},
{
	"Index" : "45908",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 48559, SAO 178158, HD 85859, GC 13627, HR 3919, DM CD-25 7585, TYC 6607-1795-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HD  85859",
	"OType" : "High proper-motion Star",
	"Distance" : "104.66",
	"RA_S" : 148.55133199,
	"DEC_S" : -25.93234583,
	"Constellation" : "Hydra ",
	"AMag" : 5.009,
	"key" : 65908,
	"title" : "HD  85859"
	},
{
	"Index" : "41594",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 48615, SAO 155588, HD 85951, GC 13644, HR 3923, DM BD-18 2810, TYC 6053-693-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 3923",
	"OType" : "Star",
	"Distance" : "187.7",
	"RA_S" : 148.71753436,
	"DEC_S" : -19.00935839,
	"Constellation" : "Hydra ",
	"AMag" : 5.107,
	"key" : 61594,
	"title" : "HR 3923"
	},
{
	"Index" : "37362",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "40 Hydrae, Upsilon02 Hydrae, HIP 49402, SAO 155713, HD 87504, GC 13861, HR 3970, DM BD-12  3073, TYC 5485-1309-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Upsilon02 Hydrae",
	"OType" : "Variable Star",
	"Distance" : "96.1",
	"RA_S" : 151.28111999,
	"DEC_S" : -13.06462501,
	"Constellation" : "Hydra ",
	"AMag" : 4.574,
	"key" : 57362,
	"title" : "Upsilon02 Hydrae"
	},
{
	"Index" : "37361",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 49809, SAO 155780, HD 88215, GC 13970, HR 3991, DM BD-12 3101, TYC 5485-1226-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 3991",
	"OType" : "Spectroscopic binary",
	"Distance" : "27.73",
	"RA_S" : 152.52452506,
	"DEC_S" : -12.81592239,
	"Constellation" : "Hydra ",
	"AMag" : 5.338,
	"key" : 57361,
	"title" : "HR 3991"
	},
{
	"Index" : "37363",
	"Description" : "Lambda Hydrae (\u03BB Hya) is a star in the constellation Hydra. Its apparent magnitude is 3.61.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "41 Hydrae, Lambda Hydrae, HIP 49841, SAO 155785, HD 88284, GC 13982, HR 3994, DM BD-11  2820, TYC 5485-1310-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Lambda Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "34.47",
	"RA_S" : 152.64698251,
	"DEC_S" : -12.35405115,
	"X" : 453,
	"Y" : 292,
	"Constellation" : "Hydra ",
	"AMag" : 3.707,
	"key" : 57363,
	"title" : "Lambda Hydrae"
	},
{
	"Index" : "41637",
	"Description" : "Mu Hydrae (\u03BC Hya) is a star in the constellation Hydra. Its apparent magnitude is 3.83.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "42 Hydrae, Mu Hydrae, HIP 51069, SAO 155980, HD 90432, GC 14326, HR 4094, DM BD-16  3052, TYC 6061-1134-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Mu Hydrae",
	"OType" : "Variable Star",
	"Distance" : "71.77",
	"RA_S" : 156.52260728,
	"DEC_S" : -16.83628952,
	"X" : 432,
	"Y" : 337,
	"Constellation" : "Hydra ",
	"AMag" : 3.985,
	"key" : 61637,
	"title" : "Mu Hydrae"
	},
{
	"Index" : "46005",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "44 Hydrae, HIP 51718, SAO 178979, HD 91550, GC 14524, HR 4145, DM BD-22  2946, TYC 6620-1355-1",
	"group" : { "key" : "Hydra" },
	"Common" : "44 Hydrae",
	"OType" : "Star",
	"Distance" : "243.49",
	"RA_S" : 158.50368558,
	"DEC_S" : -23.74516511,
	"Constellation" : "Hydra ",
	"AMag" : 5.252,
	"key" : 66005,
	"title" : "44 Hydrae"
	},
{
	"Index" : "46128",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 51979, SAO 179041, HD 92036, GC 14603, HR 4162, DM CD-26 8033, TYC 6641-1479-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4162",
	"OType" : "Variable Star",
	"Distance" : "149.12",
	"RA_S" : 159.30718835,
	"DEC_S" : -27.41263773,
	"Constellation" : "Hydra ",
	"AMag" : 5.065,
	"key" : 66128,
	"title" : "HR 4162"
	},
{
	"Index" : "37457",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "U Hydrae, HIP 52009, SAO 156110, HD 92055, GC 14611, HR 4163, DM BD-12  3218, TYC 5498-264-1",
	"group" : { "key" : "Hydra" },
	"Common" : "U Hydrae",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "207.76",
	"RA_S" : 159.38863405,
	"DEC_S" : -13.38454335,
	"Constellation" : "Hydra ",
	"AMag" : 5.217,
	"key" : 57457,
	"title" : "U Hydrae"
	},
{
	"Index" : "41663",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Phi Hydrae, HIP 52085, SAO 156122, HD 92214, GC 14631, HR 4171, DM BD-16  3100, TYC 6066-1101-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Phi Hydrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "64.45",
	"RA_S" : 159.64562725,
	"DEC_S" : -16.87656933,
	"Constellation" : "Hydra ",
	"AMag" : 5.005,
	"key" : 61663,
	"title" : "Phi Hydrae"
	},
{
	"Index" : "41723",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "b01 Hydrae, HIP 52737, SAO 156221, HD 93397, GC 14835, HR 4214, DM BD-16  3124, TYC 6075-1832-1",
	"group" : { "key" : "Hydra" },
	"Common" : "b01 Hydrae",
	"OType" : "Star",
	"Distance" : "62.92",
	"RA_S" : 161.71689517,
	"DEC_S" : -17.29688174,
	"Constellation" : "Hydra ",
	"AMag" : 5.443,
	"key" : 61723,
	"title" : "b01 Hydrae"
	},
{
	"Index" : "41722",
	"Description" : "Nu Hydrae (\u03BD Hya, \u03BD Hydrae) is a star in the constellation Hydra, near the border with the neighboring constellation of Crater. It has an apparent visual magnitude of 3.115, which is bright enough to be seen with the naked eye. Based upon parallax measurements, this star is located at a distance of about 144 light-years (44 parsecs) from the Earth.\r\rThe spectrum of this star matches a stellar classification of K0/K1 III, where the luminosity class of \u0027III\u0027 indicates this is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The radius of this star has expanded to 21 times the Sun\u0027s radius with an emission of about 151 times the luminosity of the Sun. This expanded outer envelope has an effective temperature of about 4,335 K, giving it the characteristic orange hue of a K-type star.\r\rNu Hydrae is an X-ray emitter with an estimated luminosity of 6.6 \u00D7 1028 erg s\u20131 in the X-ray band. The abundance of elements other than hydrogen and helium, what astronomers term the star\u0027s metallicity, is about half that in the Sun. It has a relatively high proper motion across the celestial sphere, suggesting that is has a peculiar velocity roughly three times higher than its neighbors.\r\rNu Hydrae was a latter designation of 4 Crateris.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Nu Hydrae, HIP 52943, SAO 156256, HD 93813, GC 14898, HR 4232, DM BD-15  3138, TYC 6075-1831-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Nu Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "44.07",
	"RA_S" : 162.40620311,
	"DEC_S" : -16.19364888,
	"X" : 385,
	"Y" : 345,
	"Constellation" : "Hydra ",
	"AMag" : 3.234,
	"key" : 61722,
	"title" : "Nu Hydrae"
	},
{
	"Index" : "41779",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "b03 Hydrae, HIP 53252, SAO 156301, HD 94388, GC 14971, HR 4251, DM BD-19  3125, TYC 6082-2054-1",
	"group" : { "key" : "Hydra" },
	"Common" : "b03 Hydrae",
	"OType" : "Variable Star",
	"Distance" : "30.8",
	"RA_S" : 163.37305094,
	"DEC_S" : -20.13873046,
	"Constellation" : "Hydra ",
	"AMag" : 5.287,
	"key" : 61779,
	"title" : "b03 Hydrae"
	},
{
	"Index" : "46150",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Chi01 Hydrae, HIP 54204, SAO 179514, HD 96202, GC 15248, HR 4314, DM CD-26  8338, TYC 6644-1331-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Chi01 Hydrae",
	"OType" : "Star",
	"Distance" : "43.23",
	"RA_S" : 166.33294636,
	"DEC_S" : -27.29361407,
	"Constellation" : "Hydra ",
	"AMag" : 4.956,
	"key" : 66150,
	"title" : "Chi01 Hydrae"
	},
{
	"Index" : "46151",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 54477, SAO 179577, HD 96819, GC 15325, HR 4334, DM CD-27 7886, TYC 6644-1332-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4334",
	"OType" : "Variable Star",
	"Distance" : "55.59",
	"RA_S" : 167.18332899,
	"DEC_S" : -28.08066766,
	"Constellation" : "Hydra ",
	"AMag" : 5.43,
	"key" : 66151,
	"title" : "HR 4334"
	},
{
	"Index" : "50524",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 56332, SAO 202554, HD 100393, GC 15844, HR 4449, DM CD-30 9303, TYC 7215-490-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4449",
	"OType" : "Variable Star",
	"Distance" : "119.06",
	"RA_S" : 173.22554548,
	"DEC_S" : -31.08722282,
	"Constellation" : "Hydra ",
	"AMag" : 5.313,
	"key" : 70524,
	"title" : "HR 4449"
	},
{
	"Index" : "50526",
	"Description" : "Xi Hydrae (\u03BE Hya, \u03BE Hydrae) is a fourth-magnitude star in the constellation Hydra. The star is situated 130 light-years from Earth and has a radius about 10 times that of the Sun. It is radiating 58 times as much luminosity as the Sun. The star is now approaching the end of its life, and has expanded its outer envelope to become a red giant star.\r\rThe star Xi Hya was particularly interesting in the field of asteroseismology when an international group of astronomers discovered that it behaves like a giant sub-ultra-bass musical instrument.\r\rXi Hydrae was a latter designation of 19 Crateris.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Xi Hydrae, HIP 56343, SAO 202558, HD 100407, GC 15845, HR 4450, DM CD-31  9083, TYC 7216-1261-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Xi Hydrae",
	"OType" : "Double or multiple star",
	"Distance" : "39.74",
	"RA_S" : 173.25048333,
	"DEC_S" : -31.857625,
	"X" : 347,
	"Y" : 497,
	"Constellation" : "Hydra ",
	"AMag" : 3.632,
	"key" : 70526,
	"title" : "Xi Hydrae"
	},
{
	"Index" : "50580",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Omicron Hydrae, HIP 56922, SAO 202695, HD 101431, GC 16019, HR 4494, DM CD-34  7610, TYC 7224-1785-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Omicron Hydrae",
	"OType" : "Star",
	"Distance" : "137.47",
	"RA_S" : 175.05329004,
	"DEC_S" : -34.74466153,
	"Constellation" : "Hydra ",
	"AMag" : 4.674,
	"key" : 70580,
	"title" : "Omicron Hydrae"
	},
{
	"Index" : "50551",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 57047, SAO 202717, HD 101666, GC 16055, HR 4503, DM CD-31 9181, TYC 7220-132-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4503",
	"OType" : "Star",
	"Distance" : "123.54",
	"RA_S" : 175.43311977,
	"DEC_S" : -32.4994051,
	"Constellation" : "Hydra ",
	"AMag" : 5.374,
	"key" : 70551,
	"title" : "HR 4503"
	},
{
	"Index" : "46302",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 57613, SAO 180208, HD 102620, GC 16183, HR 4532, DM CD-26 8789, TYC 6673-912-1",
	"group" : { "key" : "Hydra" },
	"Common" : "V* II Hya",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "166.82",
	"RA_S" : 177.1878447,
	"DEC_S" : -26.74977661,
	"Constellation" : "Hydra ",
	"AMag" : 5.287,
	"key" : 66302,
	"title" : "V* II Hya"
	},
{
	"Index" : "50594",
	"Description" : "Beta Hydrae (Beta Hya, \u03B2 Hydrae, \u03B2 Hya) is a double star in the constellation of Hydra. Its overall apparent visual magnitude varies by 0.04 magnitudes with a period of 2.344 days, and is approximately 4.27 at maximum brightness. The brighter star in the double is a giant Bp star which has been classified as an \u03B12 Canum Venaticorum variable.\r\rBeta Hydrae was a latter designation of 28 Crateris.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "Beta Hydrae, HIP 57936AB, SAO 202901, HD 103192, GC 16258, HR 4552, DM CD-33  8018, TYC 7226-1650-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Beta Hydrae",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "94.6",
	"RA_S" : 178.22719726,
	"DEC_S" : -33.90809452,
	"X" : 320,
	"Y" : 526,
	"Constellation" : "Hydra ",
	"AMag" : 4.345,
	"key" : 70594,
	"title" : "Beta Hydrae"
	},
{
	"Index" : "46291",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 58082, SAO 180288, HD 103462, GC 16286, HR 4558, DM CD-25 8930, TYC 6670-980-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4558",
	"OType" : "Star",
	"Distance" : "87.67",
	"RA_S" : 178.6772489,
	"DEC_S" : -25.71388759,
	"Constellation" : "Hydra ",
	"AMag" : 5.37,
	"key" : 66291,
	"title" : "HR 4558"
	},
{
	"Index" : "46385",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "HIP 61621, SAO 180965, HD 109799, GC 17198, HR 4803, DM CD-26 9233, TYC 6691-1465-1",
	"group" : { "key" : "Hydra" },
	"Common" : "HR 4803",
	"OType" : "Star",
	"Distance" : "34.33",
	"RA_S" : 189.42616681,
	"DEC_S" : -27.13888683,
	"Constellation" : "Hydra ",
	"AMag" : 5.45,
	"key" : 66385,
	"title" : "HR 4803"
	},
{
	"Index" : "46413",
	"Description" : "Psi Hydrae (\u03C8 Hya) is a star in the constellation Hydra. Its apparent magnitude is 4.94.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "45 Hydrae, Psi Hydrae, HIP 64166, SAO 181410, HD 114149, GC 17813, HR 4958, DM BD-22  3515, TYC 6699-1369-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Psi Hydrae",
	"OType" : "Star",
	"Distance" : "70.87",
	"RA_S" : 197.26361539,
	"DEC_S" : -23.11806651,
	"X" : 135,
	"Y" : 515,
	"Constellation" : "Hydra ",
	"AMag" : 5.05,
	"key" : 66413,
	"title" : "Psi Hydrae"
	},
{
	"Index" : "46426",
	"Description" : "Gamma Hydrae (\u03B3 Hya, \u03B3 Hydrae) is a star in the equatorial constellation of Hydra. It has an apparent visual magnitude of 3.0, placing it second in brightness among the members of this generally faint constellation. Based upon parallax measurements made during the Hipparcos mission, this star is at a distance of around 133.8 light-years (41.0 parsecs) from Earth.\r\rThe spectrum of this star matches a stellar classification of G8 III, with the luminosity class of III indicating it has evolved into a giant star after exhausting the supply of hydrogen at its core. The interferometry-measured uniform disk angular diameter of this star is 2.96 \u00B1 0.15 mas, which, at its estimated distance, equates to a physical radius of roughly 13 times the radius of the Sun. It has nearly three times the mass of the Sun and is radiating 115 times the Sun\u0027s luminosity from its outer atmosphere at an effective temperature of 5,019 K. This heat gives it the yellow glow of a K-type star. Despite having reached an advanced stage in its evolution, it is considerably younger than the Sun with an age of around 372 million years. This is because higher mass stars consume their nuclear fuel at a more rapid rate.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "46 Hydrae, Gamma Hydrae, HIP 64962, SAO 181543, HD 115659, GC 18012, HR 5020, DM BD-22  3554, TYC 6700-1436-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Gamma Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "41.03",
	"RA_S" : 199.73040494,
	"DEC_S" : -23.17151428,
	"X" : 118,
	"Y" : 526,
	"Constellation" : "Hydra ",
	"AMag" : 3.078,
	"key" : 66426,
	"title" : "Gamma Hydrae"
	},
{
	"Index" : "46593",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "47 Hydrae, HIP 68269, SAO 182134, HD 121847, GC 18887, HR 5250, DM CD-24 11202, TYC 6733-1509-1",
	"group" : { "key" : "Hydra" },
	"Common" : "47 Hydrae",
	"OType" : "Star",
	"Distance" : "101.99",
	"RA_S" : 209.62977675,
	"DEC_S" : -24.97224942,
	"Constellation" : "Hydra ",
	"AMag" : 5.184,
	"key" : 66593,
	"title" : "47 Hydrae"
	},
{
	"Index" : "46627",
	"Description" : "Pi Hydrae (\u03C0 Hya, \u03C0 Hydrae) is a star in the constellation Hydra with an apparent visual magnitude of 3.3, making it visible to the naked eye. Parallax measurements put this star at a distance of about 101 light-years (31 parsecs) from the Earth.\r\rThe spectrum of this star shows it to have a stellar classification of K1 III-IV, with the luminosity class of \u0027III-IV\u0027 suggesting it is in an evolutionary transition stage somewhere between a subgiant and a giant star. It has a low projected rotational velocity of 2.25 km s\u20131. Pi Hydrae is radiating energy from its outer envelope with an effective temperature of 4,670 K, giving it the orange hue of a K-type star.\r\rPi Hydrae is a type of giant known as a cyanogen-weak star, which means that its spectrum displays weak absorption lines of CN\u2013 relative to the metallicity. (The last is a term astronomers use when describing the abundance of elements other than hydrogen and helium.) Otherwise, it appears to be a normal star of its evolutionary class, having undergone first dredge-up of nuclear fusion by-products onto its surface layers. The measured angular diameter of this star, after correction for limb darkening, is 3.76 \u00B1 0.04 mas. At its estimated distance, this yields a physical size of about 12\u201313 times the radius of the Sun. It has an estimated mass of 2.45 times the mass of the Sun.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "49 Hydrae, Pi Hydrae, HIP 68895, SAO 182244, HD 123123, GC 19029, HR 5287, DM CD-26 10095, TYC 6738-1381-1",
	"group" : { "key" : "Hydra" },
	"Common" : "Pi Hydrae",
	"OType" : "Star",
	"Distance" : "30.96",
	"RA_S" : 211.59290604,
	"DEC_S" : -26.68236072,
	"X" : 75,
	"Y" : 589,
	"Constellation" : "Hydra ",
	"AMag" : 3.368,
	"key" : 66627,
	"title" : "Pi Hydrae"
	},
{
	"Index" : "46631",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "50 Hydrae, HIP 69415, SAO 182349, HD 124206, GC 19163, HR 5312, DM CD-26 10158, TYC 6738-710-1",
	"group" : { "key" : "Hydra" },
	"Common" : "50 Hydrae",
	"OType" : "Star",
	"Distance" : "66.67",
	"RA_S" : 213.1917674,
	"DEC_S" : -27.26118424,
	"Constellation" : "Hydra ",
	"AMag" : 5.202,
	"key" : 66631,
	"title" : "50 Hydrae"
	},
{
	"Index" : "46649",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "51 Hydrae, k Hydrae, HIP 70306, SAO 182483, HD 125932, GC 19389, HR 5381, DM CD-27  9803, TYC 6740-785-1",
	"group" : { "key" : "Hydra" },
	"Common" : "k Hydrae",
	"OType" : "Variable Star",
	"Distance" : "48.25",
	"RA_S" : 215.7740597,
	"DEC_S" : -27.75401574,
	"Constellation" : "Hydra ",
	"AMag" : 4.937,
	"key" : 66649,
	"title" : "k Hydrae"
	},
{
	"Index" : "46672",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "52 Hydrae, l Hydrae, HIP 70753, SAO 182570, HD 126769, GC 19499, HR 5407, DM CD-28 10712, TYC 6744-1753-1",
	"group" : { "key" : "Hydra" },
	"Common" : "l Hydrae",
	"OType" : "Double or multiple star",
	"Distance" : "120.46",
	"RA_S" : 217.043488,
	"DEC_S" : -29.491658,
	"Constellation" : "Hydra ",
	"AMag" : 4.959,
	"key" : 66672,
	"title" : "l Hydrae"
	},
{
	"Index" : "46703",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "54 Hydrae, m Hydrae, HIP 72197A, SAO 182855, HD 129926A, GC 19864, HR 5497, DM CD-24 11661, TYC 6750-1743-1",
	"group" : { "key" : "Hydra" },
	"Common" : "m Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "30.26",
	"RA_S" : 221.50033479,
	"DEC_S" : -25.44317839,
	"Constellation" : "Hydra ",
	"AMag" : 5.125,
	"key" : 66703,
	"title" : "m Hydrae"
	},
{
	"Index" : "46709",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "56 Hydrae, HIP 72357, SAO 182882, HD 130259, GC 19904, HR 5516, DM CD-25 10537, TYC 6751-1895-1",
	"group" : { "key" : "Hydra" },
	"Common" : "56 Hydrae",
	"OType" : "Star",
	"Distance" : "109.63",
	"RA_S" : 221.93669406,
	"DEC_S" : -26.0874994,
	"Constellation" : "Hydra ",
	"AMag" : 5.333,
	"key" : 66709,
	"title" : "56 Hydrae"
	},
{
	"Index" : "46734",
	"Description" : "58 Hydrae (58 Hya) is a star in the constellation Hydra. Its apparent magnitude is 4.42.",
	"MapNum" : "28",
	"ImageNum" : "28",
	"Desig" : "58 Hydrae, E Hydrae, HIP 72571, SAO 182911, HD 130694, GC 19954, HR 5526, DM CD-27 10073, TYC 6755-2085-1",
	"group" : { "key" : "Hydra" },
	"Common" : "58 Hydrae",
	"OType" : "High proper-motion Star",
	"Distance" : "100.93",
	"RA_S" : 222.57212122,
	"DEC_S" : -27.96037002,
	"X" : 17,
	"Y" : 649,
	"Constellation" : "Hydra ",
	"AMag" : 4.573,
	"key" : 66734,
	"title" : "58 Hydrae"
	},
{
	"Index" : "70190",
	"Description" : "Beta Hydri (\u03B2 Hyi, \u03B2 Hydri) is a star in the southern circumpolar constellation of Hydrus. (Note that Hydrus is not the same as Hydra.) With an apparent visual magnitude of 2.8, this is the brightest star the constellation. Based upon parallax measurements the distance to this star is about 24.33 light-years (7.46 parsecs).\r\rThis star has about 108% of the mass of the Sun and 181% of the Sun\u0027s radius, with more than three times the Sun\u0027s luminosity. The spectrum of this star matches a stellar classification of G2 IV, with the luminosity class of \u0027IV\u0027 indicating this is a subgiant star. As such, it is a slightly more evolved star than the Sun, with the supply at its core becoming exhausted. It is the nearest subgiant star to the Sun and one of the oldest stars in the solar neighborhood. This star bears some resemblance to what the Sun may look like in the far distant future, making it an object of interest to astronomers.\r\rAt around 150 BC, this star was two degrees away from the southern celestial pole. It is currently the nearest relatively bright star to the southern pole.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Beta Hydri, HIP 2021, SAO 255670, HD 2151, GC 503, HR 98, DM CP-77    16, TYC 9350-1626-1",
	"group" : { "backgroundImage" : "images/Alignment/29.png",
		"description" : "Hydrus (pron.: /\u02C8ha\u026Adr\u0259s/) is a small constellation in the southern sky, created in the sixteenth century. Its name means \u0022male water snake\u0022, and it should not be confused with Hydra, a much larger constellation which represents a female water snake.\r\rHydrus was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603. The companion to Hydra, the female water snake, he is forced to journey through Eridanus, Orion, and the Milky Way to visit his lover.",
		"key" : "Hydrus",
		"grouptype" : "Hydrus",
		"Meaning" : "lesser water snake",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Hydrus",
		"title" : "Hydrus Objects Group" },
	"Common" : "Beta Hydri",
	"OType" : "Variable Star",
	"Distance" : "7.46",
	"RA_S" : 6.43782906,
	"DEC_S" : -77.25425174,
	"X" : 328,
	"Y" : 378,
	"Constellation" : "Hydrus ",
	"AMag" : 2.855,
	"key" : 90190,
	"title" : "Beta Hydri"
	},
{
	"Index" : "68420",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Lambda Hydri, HIP 3781, SAO 255710, HD 4815, GC 983, HR 236, DM CP-75    64, TYC 9141-7804-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Lambda Hydri",
	"OType" : "Star",
	"Distance" : "64.92",
	"RA_S" : 12.14755649,
	"DEC_S" : -74.9234348,
	"Constellation" : "Hydrus ",
	"AMag" : 5.241,
	"key" : 88420,
	"title" : "Lambda Hydri"
	},
{
	"Index" : "68436",
	"Description" : "Eta2 Hydri (\u03B72 Hyi, \u03B72 Hydri), often catalogued as HD 11977, is a giant yellow star approximately 219 light-years away in the constellation of Hydrus. Based on its mass, it was probably a class A star (similar to Vega or Fomalhaut) when it was on the main sequence, though it is now in the giant stage of its evolution. As of 2005, an extrasolar planet was confirmed to be orbiting the star.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Eta02 Hydri, HIP 8928, SAO 248460, HD 11977, GC 2331, HR 570, DM CP-68   101, TYC 9143-238-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Eta2 Hydri",
	"OType" : "Star",
	"Distance" : "67.06",
	"RA_S" : 28.73387237,
	"DEC_S" : -67.64730307,
	"X" : 280,
	"Y" : 236,
	"Constellation" : "Hydrus ",
	"AMag" : 4.789,
	"key" : 88436,
	"title" : "Eta2 Hydri"
	},
{
	"Index" : "65390",
	"Description" : "Alpha Hydri (\u03B1 Hyi, \u03B1 Hydri) is the second brightest star in the southern circumpolar constellation of Hydrus. It is readily visible to the named eye with an apparent visual magnitude of +2.9. It is sometimes informally known as the Head of Hydrus. This should not be confused with Alpha Hydrae (Alphard) in the constellation Hydra. Alpha Hydri is one of only three stars in the constellation Hydrus that are above the fourth visual magnitude. This star can be readily located as it lies to the south and west of the prominent star Achernar in the constellation Eridanus.\r\rBased upon parallax measurements from the Hipparcos mission, Alpha Hydri is located at a distance of about 71.8 light-years (22.0 parsecs) from Earth. This subgiant star is 80% larger and twice as massive as the Sun, with a stellar classification of F0 IV. It is about 810 million years old and is radiating 32 times the Sun\u0027s luminosity from its outer atmosphere at an effective temperature of 7,077 K. Alpha Hydri emits X-rays similar to Altair. The space velocity components of this star are [U, V, W] = [\u221214, \u221214, -2] km/s.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u86C7\u9996 (Sh\u00E9 Sh\u01D2u), meaning Snake\u0027s Head, refers to an asterism consisting of \u03B1 Hydri and \u03B2 Reticuli. Consequently, \u03B1 Hydri itself is known as \u86C7\u9996\u4E00 (Sh\u00E9 Sh\u01D2u y\u012B, English: the First Star of Snake\u0027s Head.)",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Alpha Hydri, HIP 9236, SAO 248474, HD 12311, GC 2405, HR 591, DM CP-62   162, TYC 8851-2027-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Alpha Hydri",
	"OType" : "High proper-motion Star",
	"Distance" : "22.01",
	"RA_S" : 29.69247778,
	"DEC_S" : -61.56985966,
	"X" : 282,
	"Y" : 156,
	"Constellation" : "Hydrus ",
	"AMag" : 2.871,
	"key" : 85390,
	"title" : "Alpha Hydri"
	},
{
	"Index" : "68447",
	"Description" : "Delta Hydri (\u03B4 Hyi) is a star in the constellation Hydrus. Its apparent magnitude is 4.08.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Delta Hydri, HIP 11001, SAO 248545, HD 15008, GC 2872, HR 705, DM CP-69   113, TYC 9144-1688-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Delta Hydri",
	"OType" : "Star",
	"Distance" : "42.82",
	"RA_S" : 35.43726665,
	"DEC_S" : -68.65942135,
	"X" : 247,
	"Y" : 247,
	"Constellation" : "Hydrus ",
	"AMag" : 4.075,
	"key" : 88447,
	"title" : "Delta Hydri"
	},
{
	"Index" : "70230",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Mu Hydri, HIP 11757, SAO 255898, HD 16522, GC 3102, HR 776, DM CP-79    66, TYC 9357-1339-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Mu Hydri",
	"OType" : "Star",
	"Distance" : "86.94",
	"RA_S" : 37.91878832,
	"DEC_S" : -79.109391,
	"Constellation" : "Hydrus ",
	"AMag" : 5.383,
	"key" : 90230,
	"title" : "Mu Hydri"
	},
{
	"Index" : "68445",
	"Description" : "Epsilon Hydri (\u03B5 Hyi) is a star in the constellation Hydrus. Its apparent magnitude is 4.06.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Epsilon Hydri, HIP 12394, SAO 248621, HD 16978, GC 3240, HR 806, DM CP-68   161, TYC 9144-1686-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Epsilon Hydri",
	"OType" : "Star",
	"Distance" : "46.55",
	"RA_S" : 39.89732264,
	"DEC_S" : -68.26694641,
	"X" : 226,
	"Y" : 243,
	"Constellation" : "Hydrus ",
	"AMag" : 4.088,
	"key" : 88445,
	"title" : "Epsilon Hydri"
	},
{
	"Index" : "68462",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Zeta Hydri, HIP 12876, SAO 248644, HD 17566, GC 3354, HR 837, DM CP-68   169, TYC 9145-2046-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Zeta Hydri",
	"OType" : "Star",
	"Distance" : "87.16",
	"RA_S" : 41.38597824,
	"DEC_S" : -67.61661821,
	"Constellation" : "Hydrus ",
	"AMag" : 4.829,
	"key" : 88462,
	"title" : "Zeta Hydri"
	},
{
	"Index" : "70247",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Nu Hydri, HIP 13244, SAO 255929, HD 18293, GC 3463, HR 872, DM CP-75   204, TYC 9362-1344-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Nu Hydri",
	"OType" : "Star",
	"Distance" : "104.02",
	"RA_S" : 42.6185785,
	"DEC_S" : -75.06694515,
	"Constellation" : "Hydrus ",
	"AMag" : 4.895,
	"key" : 90247,
	"title" : "Nu Hydri"
	},
{
	"Index" : "68487",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Theta Hydri, HIP 14131, SAO 255945, HD 19400, GC 3687, HR 939, DM CP-72   219, TYC 9148-1834-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Theta Hydri",
	"OType" : "Double or multiple star",
	"Distance" : "157.54",
	"RA_S" : 45.56436283,
	"DEC_S" : -71.90246002,
	"Constellation" : "Hydrus ",
	"AMag" : 5.478,
	"key" : 88487,
	"title" : "Theta Hydri"
	},
{
	"Index" : "68587",
	"Description" : "Gamma Hydri (\u03B3 Hyi) is a star in the constellation Hydrus. Its apparent magnitude is 3.24.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Gamma Hydri, HIP 17678, SAO 256029, HD 24512, GC 4633, HR 1208, DM CP-74   276, TYC 9159-1634-1",
	"group" : { "key" : "Hydrus" },
	"Common" : "Gamma Hydri",
	"OType" : "Variable Star",
	"Distance" : "65.61",
	"RA_S" : 56.80975228,
	"DEC_S" : -74.23896428,
	"X" : 174,
	"Y" : 334,
	"Constellation" : "Hydrus ",
	"AMag" : 3.436,
	"key" : 88587,
	"title" : "Gamma Hydri"
	},
{
	"Index" : "61125",
	"Description" : "Alpha Indi (\u03B1 Ind, \u03B1 Indi) is a third magnitude giant star in the constellation Indus, located about 98 light years from the Earth. The stellar classification of this star is K0 III-IV, so it has exhausted the hydrogen at its core and evolved away from the main sequence. It has about double the mass of the Sun and is an estimated billion years old. As a giant star it has expanded to about 12 times the radius of the Sun. The effective temperature of the photosphere is 4,893 K, giving it the characteristic orange hue of a K-type star. It may have two nearby M-type companion stars, which are located at least 2,000 Astronomical Units from the primary.\r\rIn China, this star is called Pe Sze where it also was known as the Persian, a title from the Jesuit missionaries. The term Pe Sze is from the name of asterism \u6CE2\u65AF (B\u014D S\u012B, English: Persia). In Chinese astronomy, consequently, \u03B1 Indi itself is known as \u6CE2\u65AF\u4E8C (B\u014D S\u012B \u00E8r, English: the Second Star of Persia)",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Alpha Indi, HIP 101772, SAO 230300, HD 196171, GC 28682, HR 7869, DM CD-47 13477, TYC 8411-1822-1",
	"group" : { "backgroundImage" : "images/Alignment/26.png",
		"description" : "Indus is a constellation in the southern sky. Created in the late sixteenth century, it represents an Indian, a word that could refer at the time to any native of Asia or the Americas.\r\rIndus does not contain any bright stars. Alpha Indi is the brightest star in Indus. It is an orange giant of magnitude 3.1, 101 light-years from Earth. Beta Indi is an orange giant of magnitude 3.7, 600 light-years from Earth. Delta Indi is a white star of magnitude 4.4, 185 light-years from Earth.\r\rEpsilon Indi is one of the closest stars to Earth, approximately 11.8 light years away. It is an orange dwarf of magnitude 4.7, meaning that the yellow dwarf Sun is slightly hotter and larger. The system has been discovered to contain a pair of binary brown dwarfs, and has long been a prime candidate in SETI studies.\r\rIndus is home to one bright binary star. Theta Indi is a binary star divisible in small amateur telescopes, 97 light-years from Earth. Its primary is a white star of magnitude 4.5 and its secondary is a white star of magnitude 7.0.\r\rT Indi is the only bright variable star in Indus. It is a semi-regular, deeply-coloured red giant with a period of 11 months, 1900 light-years from Earth. Its minimum magnitude is 7 and its maximum magnitude is 5.\r\rThe constellation was one of twelve created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603. Plancius portrayed the figure as a nude male with arrows in both hands but no bow.",
		"key" : "Indus",
		"grouptype" : "Indus",
		"Meaning" : "Indian (American indigenous)",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Indus",
		"title" : "Indus Objects Group" },
	"Common" : "Alpha Indi",
	"OType" : "Star",
	"Distance" : "30.15",
	"RA_S" : 309.39180731,
	"DEC_S" : -47.29150209,
	"X" : 529,
	"Y" : 314,
	"Constellation" : "Indus ",
	"AMag" : 3.203,
	"key" : 81125,
	"title" : "Alpha Indi"
	},
{
	"Index" : "61173",
	"Description" : "Eta Indi (\u03B7 Ind) is a star in the constellation Indus. Its apparent magnitude is 4.52.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Eta Indi, HIP 102333, SAO 246709, HD 197157, GC 28860, HR 7920, DM CP-52 11752, TYC 8419-1619-1",
	"group" : { "key" : "Indus" },
	"Common" : "Eta Indi",
	"OType" : "Star",
	"Distance" : "24.17",
	"RA_S" : 311.00971869,
	"DEC_S" : -51.9209739,
	"X" : 496,
	"Y" : 366,
	"Constellation" : "Indus ",
	"AMag" : 4.53,
	"key" : 81173,
	"title" : "Eta Indi"
	},
{
	"Index" : "61109",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Zeta Indi, HIP 102790, SAO 230391, HD 198048, GC 29008, HR 7952, DM CD-46 13718, TYC 8408-532-1",
	"group" : { "key" : "Indus" },
	"Common" : "Zeta Indi",
	"OType" : "Star",
	"Distance" : "126.33",
	"RA_S" : 312.37067654,
	"DEC_S" : -46.22682865,
	"Constellation" : "Indus ",
	"AMag" : 5.061,
	"key" : 81109,
	"title" : "Zeta Indi"
	},
{
	"Index" : "61178",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Iota Indi, HIP 102950, SAO 246762, HD 198308, GC 29055, HR 7968, DM CP-52 11782, TYC 8420-1431-1",
	"group" : { "key" : "Indus" },
	"Common" : "Iota Indi",
	"OType" : "Star",
	"Distance" : "142.79",
	"RA_S" : 312.87520804,
	"DEC_S" : -51.60818118,
	"X" : 482,
	"Y" : 358,
	"Constellation" : "Indus ",
	"AMag" : 5.168,
	"key" : 81178,
	"title" : "Iota Indi"
	},
{
	"Index" : "65020",
	"Description" : "Beta Indi (Beta Ind, \u03B2 Indi, \u03B2 Ind) is a K-type bright giant star in the constellation of Indus. It has an apparent visual magnitude of approximately 3.658.\r\r\u03B2 Indi has a visual companion, CCDM J20548-5827B, with an apparent visual magnitude of approximately 12.5.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Beta Indi, HIP 103227, SAO 246784, HD 198700, GC 29133, HR 7986, DM CP-58  7788, TYC 8804-1375-1",
	"group" : { "key" : "Indus" },
	"Common" : "Beta Indi",
	"OType" : "Star",
	"Distance" : "187.41",
	"RA_S" : 313.70251081,
	"DEC_S" : -58.45415412,
	"X" : 447,
	"Y" : 440,
	"Constellation" : "Indus ",
	"AMag" : 3.778,
	"key" : 85020,
	"title" : "Beta Indi"
	},
{
	"Index" : "64980",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Mu Indi, HIP 104085, SAO 246854, HD 200365, GC 29420, HR 8055, DM CP-55  9509, TYC 8796-1244-1",
	"group" : { "key" : "Indus" },
	"Common" : "Mu Indi",
	"OType" : "Star",
	"Distance" : "111.98",
	"RA_S" : 316.30937138,
	"DEC_S" : -54.72703897,
	"Constellation" : "Indus ",
	"AMag" : 5.298,
	"key" : 84980,
	"title" : "Mu Indi"
	},
{
	"Index" : "64972",
	"Description" : "Theta Indi (\u03B8 Ind) is a star in the constellation Indus. Its apparent magnitude is 4.40.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Theta Indi, HIP 105319B, SAO 246964, HD 202730, GC 29819, HR 8140, DM CP-53 10037, TYC 8793-1479-1",
	"group" : { "key" : "Indus" },
	"Common" : "Theta Indi",
	"OType" : "High proper-motion Star",
	"Distance" : "30.28",
	"RA_S" : 319.963429,
	"DEC_S" : -53.449403,
	"X" : 422,
	"Y" : 365,
	"Constellation" : "Indus ",
	"AMag" : 6.932,
	"key" : 84972,
	"title" : "Theta Indi"
	},
{
	"Index" : "64971",
	"Description" : "Theta Indi (\u03B8 Ind) is a star in the constellation Indus. Its apparent magnitude is 4.40.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Theta Indi, HIP 105319A, SAO 246965, HD 202730, GC 29819, HR 8140, DM CP-53 10037, TYC 8793-1478-1",
	"group" : { "key" : "Indus" },
	"Common" : "Theta Indi",
	"OType" : "Double or multiple star",
	"Distance" : "30.28",
	"RA_S" : 319.966196,
	"DEC_S" : -53.449267,
	"X" : 422,
	"Y" : 365,
	"Constellation" : "Indus ",
	"AMag" : 4.504,
	"key" : 84971,
	"title" : "Theta Indi"
	},
{
	"Index" : "65061",
	"Description" : "Delta Indi (\u03B4 Ind) is a star in the constellation Indus. Its apparent magnitude is 4.40.",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Delta Indi, HIP 108431AB, SAO 247244, HD 208450, GC 30720, HR 8368, DM CP-55  9733, TYC 8812-1257-1",
	"group" : { "key" : "Indus" },
	"Common" : "Delta Indi",
	"OType" : "Double or multiple star",
	"Distance" : "57.62",
	"RA_S" : 329.4794954,
	"DEC_S" : -54.99257315,
	"X" : 347,
	"Y" : 373,
	"Constellation" : "Indus ",
	"AMag" : 4.43,
	"key" : 85061,
	"title" : "Delta Indi"
	},
{
	"Index" : "65101",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Epsilon Indi, HIP 108870, SAO 247287, HD 209100, GC 30817, HR 8387, DM CP-57 10015, TYC 8817-984-1",
	"group" : { "key" : "Indus" },
	"Common" : "Epsilon Indi",
	"OType" : "Pre-main sequence Star",
	"Distance" : "3.62",
	"RA_S" : 330.84023065,
	"DEC_S" : -56.78597448,
	"Constellation" : "Indus ",
	"AMag" : 4.826,
	"key" : 85101,
	"title" : "Epsilon Indi"
	},
{
	"Index" : "70109",
	"MapNum" : "26",
	"ImageNum" : "26",
	"Desig" : "Nu Indi, HIP 110618, SAO 258033, HD 211998, GC 31284, HR 8515, DM CP-72  2690, TYC 9340-2962-1",
	"group" : { "key" : "Indus" },
	"Common" : "Nu Indi",
	"OType" : "Double or multiple star",
	"Distance" : "28.7",
	"RA_S" : 336.15370803,
	"DEC_S" : -72.25541086,
	"Constellation" : "Indus ",
	"AMag" : 5.351,
	"key" : 90109,
	"title" : "Nu Indi"
	},
{
	"Index" : "22012",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 109102, SAO 51650, HD 209945, GC 30919, HR 8424, DM BD+44 4043, TYC 3605-2847-1",
	"group" : { "backgroundImage" : "images/Alignment/22.png",
		"description" : "Lacerta is one of the 88 modern constellations defined by the International Astronomical Union. Its name is Latin for lizard. A small, faint constellation, it was created in 1687 by the astronomer Johannes Hevelius. Its brightest stars form a \u0022W\u0022 shape similar to that of Cassiopeia, and it is thus sometimes referred to as \u0027Little Cassiopeia\u0027. It is located between Cygnus, Cassiopeia and Andromeda on the northern celestial sphere. The northern part lies on the Milky Way.\r\rLacerta is typical of Milky Way constellations: no bright galaxies, nor globular clusters, but instead open clusters, for example NGC 7243, the faint planetary nebula IC 5271 and quite a few double stars. It also contains the prototypic blazar BL Lacertae. Lacerta contains no Messier objects.\r\rCentred on a region of the sky without apparently bright stars, Lacerta was not regarded as a constellation by ancient astronomers. Johannes Hevelius created the constellation in 1687, though Augustin Royer created Sceptrum (the Hand of Justice and Sceptre) to honor Louis XIV in 1670 and Johann Elert Bode created Frederici Honores (Frederick\u0027s Glory) to honor Frederick the Great in 1787. Both Sceptrum and Frederici Honores are now obsolete, while Lacerta still survives.",
		"key" : "Lacerta",
		"grouptype" : "Lacerta",
		"Meaning" : "lizard",
		"Family" : "Perseus",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Lacerta",
		"title" : "Lacerta Objects Group" },
	"Common" : "HR 8424",
	"OType" : "Variable Star",
	"Distance" : "186.04",
	"RA_S" : 331.5081344,
	"DEC_S" : 45.01434906,
	"Constellation" : "Lacerta ",
	"AMag" : 5.261,
	"key" : 42012,
	"title" : "HR 8424"
	},
{
	"Index" : "22150",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 109521, SAO 34143, HD 210715, GC 31046, HR 8463, DM BD+50 3602, TYC 3618-4103-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "HR 8463",
	"OType" : "Star",
	"Distance" : "54.76",
	"RA_S" : 332.79127296,
	"DEC_S" : 50.82338662,
	"Constellation" : "Lacerta ",
	"AMag" : 5.396,
	"key" : 42150,
	"title" : "HR 8463"
	},
{
	"Index" : "18494",
	"Description" : "HD 211073 is a star in the constellation Lacerta. Its apparent magnitude is 4.51.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 109754AD, SAO 72155, HD 211073, GC 31104, HR 8485, DM BD+38 4711, TYC 3203-2402-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "HD 211073",
	"OType" : "Star",
	"Distance" : "147.08",
	"RA_S" : 333.46970605,
	"DEC_S" : 39.71492837,
	"X" : 132,
	"Y" : 261,
	"Constellation" : "Lacerta ",
	"AMag" : 4.657,
	"key" : 38494,
	"title" : "HD 211073"
	},
{
	"Index" : "18465",
	"Description" : "1 Lacertae (1 Lac) is a star in the constellation Lacerta. Its apparent magnitude is 4.13.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "1 Lacertae, HIP 109937, SAO 72191, HD 211388, GC 31143, HR 8498, DM BD+37  4526, TYC 3199-3591-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "1 Lacertae",
	"OType" : "Variable Star",
	"Distance" : "190.04",
	"RA_S" : 333.9923998,
	"DEC_S" : 37.74874008,
	"X" : 120,
	"Y" : 284,
	"Constellation" : "Lacerta ",
	"AMag" : 4.277,
	"key" : 38465,
	"title" : "1 Lacertae"
	},
{
	"Index" : "22029",
	"Description" : "2 Lacertae (2 Lac) is a fairly faint star at magnitude 4.57.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "2 Lacertae, HIP 110351, SAO 51904, HD 212120, GC 31252, HR 8523, DM BD+45  3894, TYC 3607-2600-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "2 Lacertae",
	"OType" : "Spectroscopic binary",
	"Distance" : "169.95",
	"RA_S" : 335.25644987,
	"DEC_S" : 46.53656838,
	"X" : 141,
	"Y" : 169,
	"Constellation" : "Lacerta ",
	"AMag" : 4.523,
	"key" : 42029,
	"title" : "2 Lacertae"
	},
{
	"Index" : "22163",
	"Description" : "Beta Lacertae (Beta Lac, \u03B2 Lacertae, \u03B2 Lac) is the fourth brightest star in the constellation of Lacerta. It is a G-type giant with an apparent visual magnitude of approximately 4.43.\r\rIn Chinese, \u87A3\u86C7 (T\u00E9ng Sh\u00E9), meaning Flying Serpent, refers to an asterism consisting of \u03B2 Lacertae, \u03B1 Lacertae, 4 Lacertae, \u03C02 Cygni, \u03C01 Cygni, HD 206267, \u03B5 Cephei, \u03C3 Cassiopeiae, \u03C1 Cassiopeiae, \u03C4 Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, \u03BB Andromedae, \u03BA Andromedae, \u03B9 Andromedae, and \u03C8 Andromedae. Consequently, \u03B2 Lacertae itself is known as \u87A3\u86C7\u5341 (T\u00E9ng Sh\u00E9 sh\u00ED, English: the Tenth Star of Flying Serpent)",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "3 Lacertae, Beta Lacertae, HIP 110538, SAO 34395, HD 212496, GC 31310, HR 8538, DM BD+51  3358, TYC 3619-4081-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "Beta Lacertae",
	"OType" : "Double or multiple star",
	"Distance" : "52.11",
	"RA_S" : 335.89009757,
	"DEC_S" : 52.22904846,
	"X" : 161,
	"Y" : 96,
	"Constellation" : "Lacerta ",
	"AMag" : 4.542,
	"key" : 42163,
	"title" : "Beta Lacertae"
	},
{
	"Index" : "22120",
	"Description" : "4 Lacertae (4 Lac) is a star in the constellation Lacerta. Its apparent magnitude is 4.60.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "4 Lacertae, HIP 110609, SAO 51970, HD 212593, GC 31326, HR 8541, DM BD+48  3715, TYC 3615-3021-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "4 Lacertae",
	"OType" : "Star",
	"Distance" : "689.6552",
	"RA_S" : 336.12912665,
	"DEC_S" : 49.47639824,
	"X" : 147,
	"Y" : 130,
	"Constellation" : "Lacerta ",
	"AMag" : 4.591,
	"key" : 42120,
	"title" : "4 Lacertae"
	},
{
	"Index" : "22074",
	"Description" : "5 Lacertae (5 Lac) is a star in the constellation Lacerta. Its apparent magnitude is 4.37.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "5 Lacertae, HIP 111022, SAO 52055, HD 213311, GC 31426, HR 8572, DM BD+46  3719A, TYC 3611-2304-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "5 Lacertae",
	"OType" : "Red supergiant star",
	"Distance" : "500.09",
	"RA_S" : 337.38258661,
	"DEC_S" : 47.70688812,
	"X" : 129,
	"Y" : 149,
	"Constellation" : "Lacerta ",
	"AMag" : 4.546,
	"key" : 42074,
	"title" : "5 Lacertae"
	},
{
	"Index" : "18548",
	"Description" : "6 Lacertae (6 Lac) is a star in the constellation Lacerta. Its apparent magnitude is 4.52.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "6 Lacertae, HIP 111104, SAO 52079, HD 213420, GC 31449, HR 8579, DM BD+42  4420, TYC 3209-2260-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "6 Lacertae",
	"OType" : "Spectroscopic binary",
	"Distance" : "459.21",
	"RA_S" : 337.62191686,
	"DEC_S" : 43.12337679,
	"X" : 106,
	"Y" : 206,
	"Constellation" : "Lacerta ",
	"AMag" : 4.493,
	"key" : 38548,
	"title" : "6 Lacertae"
	},
{
	"Index" : "22246",
	"Description" : "Alpha Lacertae (Alpha Lac, \u03B1 Lacertae, \u03B1 Lac) is an A-type main sequence star in the constellation of Lacerta. It is the brightest star in Lacerta and has an apparent visual magnitude of approximately 3.777.\r\rThe star has a visual companion, CCDM J22313+5017B, of spectral type A and apparent visual magnitude 11.8, approximately 36 arcseconds away. The companion is optical, a chance line-of-sight coincidence.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "7 Lacertae, Alpha Lacertae, HIP 111169, SAO 34542, HD 213558, GC 31471, HR 8585, DM BD+49  3875, TYC 3628-3193-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "Alpha Lacertae",
	"OType" : "Star",
	"Distance" : "31.46",
	"RA_S" : 337.82292212,
	"DEC_S" : 50.28249116,
	"X" : 137,
	"Y" : 116,
	"Constellation" : "Lacerta ",
	"AMag" : 3.758,
	"key" : 42246,
	"title" : "Alpha Lacertae"
	},
{
	"Index" : "22301",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "9 Lacertae, HIP 111674, SAO 34628, HD 214454, GC 31586, HR 8613, DM BD+50  3770, TYC 3632-3260-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "9 Lacertae",
	"OType" : "High proper-motion Star",
	"Distance" : "52.63",
	"RA_S" : 339.34340468,
	"DEC_S" : 51.54511916,
	"Constellation" : "Lacerta ",
	"AMag" : 4.662,
	"key" : 42301,
	"title" : "9 Lacertae"
	},
{
	"Index" : "25407",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 111795, SAO 34651, HD 214665, GC 31615, HR 8621, DM BD+56 2821, TYC 3991-3192-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "HR 8621",
	"OType" : "Long-period variable star",
	"Distance" : "138.13",
	"RA_S" : 339.65802005,
	"DEC_S" : 56.79563023,
	"Constellation" : "Lacerta ",
	"AMag" : 5.348,
	"key" : 45407,
	"title" : "HR 8621"
	},
{
	"Index" : "18483",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "10 Lacertae, HIP 111841, SAO 72575, HD 214680, GC 31626, HR 8622, DM BD+38  4826, TYC 3201-94-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "10 Lacertae",
	"OType" : "Double or multiple star",
	"Distance" : "459.38",
	"RA_S" : 339.81532766,
	"DEC_S" : 39.05026977,
	"Constellation" : "Lacerta ",
	"AMag" : 4.839,
	"key" : 38483,
	"title" : "10 Lacertae"
	},
{
	"Index" : "18710",
	"Description" : "11 Lacertae (11 Lac) is a star in the constellation Lacerta. 11 Lacertae is a giant star with a stellar classification of K2III, an apparent magnitude of 4.50 and absolute magnitude -0.33. It lies at a distance of about 300 light years.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "11 Lacertae, HIP 111944, SAO 52251, HD 214868, GC 31652, HR 8632, DM BD+43  4266, TYC 3226-2285-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "11 Lacertae",
	"OType" : "Star",
	"Distance" : "101.95",
	"RA_S" : 340.12857743,
	"DEC_S" : 44.27630691,
	"X" : 89,
	"Y" : 183,
	"Constellation" : "Lacerta ",
	"AMag" : 4.64,
	"key" : 38710,
	"title" : "11 Lacertae"
	},
{
	"Index" : "18640",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "12 Lacertae, HIP 112031, SAO 72627, HD 214993, GC 31670, HR 8640, DM BD+39  4912, TYC 3218-2413-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "12 Lacertae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "450.26",
	"RA_S" : 340.36937561,
	"DEC_S" : 40.22545188,
	"Constellation" : "Lacerta ",
	"AMag" : 5.205,
	"key" : 38640,
	"title" : "12 Lacertae"
	},
{
	"Index" : "18668",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "13 Lacertae, HIP 112242, SAO 52317, HD 215373, GC 31732, HR 8656, DM BD+41  4594, TYC 3222-1934-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "13 Lacertae",
	"OType" : "Star",
	"Distance" : "78.64",
	"RA_S" : 341.02282713,
	"DEC_S" : 41.81923469,
	"Constellation" : "Lacerta ",
	"AMag" : 5.213,
	"key" : 38668,
	"title" : "13 Lacertae"
	},
{
	"Index" : "18724",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "15 Lacertae, HIP 112917, SAO 52436, HD 216397, GC 31896, HR 8699, DM BD+42  4521, TYC 3227-3865-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "15 Lacertae",
	"OType" : "Star",
	"Distance" : "99.63",
	"RA_S" : 343.00848015,
	"DEC_S" : 43.31242075,
	"Constellation" : "Lacerta ",
	"AMag" : 5.126,
	"key" : 38724,
	"title" : "15 Lacertae"
	},
{
	"Index" : "22271",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 113288, SAO 52516, HD 216946, GC 31989, HR 8726, DM BD+48 3887, TYC 3630-2520-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "HR 8726",
	"OType" : "Long-period variable star",
	"Distance" : "480.82",
	"RA_S" : 344.10832555,
	"DEC_S" : 49.73354575,
	"Constellation" : "Lacerta ",
	"AMag" : 5.178,
	"key" : 42271,
	"title" : "HR 8726"
	},
{
	"Index" : "22228",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "EW Lacertae, HIP 113327, SAO 52526, HD 217050, GC 31998, HR 8731, DM BD+47  3985, TYC 3626-1877-1",
	"group" : { "key" : "Lacerta" },
	"Common" : "EW Lacertae",
	"OType" : "Be Star",
	"Distance" : "250.39",
	"RA_S" : 344.26876188,
	"DEC_S" : 48.68406511,
	"Constellation" : "Lacerta ",
	"AMag" : 5.323,
	"key" : 42228,
	"title" : "EW Lacertae"
	},
{
	"Index" : "7893",
	"Description" : "Kappa Leonis (\u03BA Leonis, \u03BA Leo) is a 4th-magnitude double star in the constellation Leo. It was known as Minchir el-asad on Bode\u0027s large star atlas, Uranographia. This name is derived from the Arabic Minkhir al-Asad, \u0022the Muzzle of (the constellation of) the Lion\u0022 for this star. The name is erroneously spelt as Al Minliar al Asad in the Yale Bright Star Catalogue.\r\rKappa Leonis has apparent magnitude +4.46 and has a stellar classification of K2III. It is approximately 210 light years from Earth.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "1 Leonis, Kappa Leonis, HIP 46146, SAO 80807, HD 81146, GC 12972, HR 3731, DM BD+26  1939, TYC 1955-1904-1",
	"group" : { "backgroundImage" : "images/Alignment/30.png",
		"description" : "Leo (pron.: /\u02C8li\u02D0o\u028A/) is one of the constellations of the zodiac, lying between Cancer to the west and Virgo to the east. Its name is Latin for lion. Its symbol is\u264C. One of the 48 constellations described by the 2nd century astronomer Ptolemy, Leo remains one of the 88 modern constellations today.\r\rLeo was one of the earliest recognized constellations, with archaeological evidence that the Mesopotamians had a similar constellation as early as 4000 BCE. The Persians called Leo Ser or Shir; the Turks, Artan; the Syrians, Aryo; the Jewish, Arye; the Indians, Simha, all meaning \u0022lion\u0022. In Babylonian astronomy, the constellation was called UR.GU.LA, the \u0022Great Lion\u0022; the bright star Regulus was known as \u0022the star that stands at the Lion\u0027s breast.\u0022 Regulus also had distinctly regal associations, as it was known as the King Star.\r\rIn Greek mythology, Leo was identified as the Nemean Lion which was killed by Hercules during one of his twelve labours, and next put into the sky.\r\rThe Roman poet Ovid called it Herculeus Leo and Violentus Leo. Bacchi Sidus (star of Bacchus) was another of its titles, the god Bacchus always being identified with this animal. However, Manilius called it Jovis et Junonis Sidus (Star of Jupiter and Juno).\r\rEarly Hindu astronomers knew it as Asleha and as Sinha, the Tamil Simham.\r\rLeo is commonly represented as if the sickle-shaped asterism of stars is the back of the Lion\u0027s head. The sickle is marked by six stars: Epsilon Leonis, Mu Leonis, Zeta Leonis, Gamma Leonis, Eta Leonis, and Alpha Leonis. The lion\u0027s tail is marked by Beta Leonis (Denebola) and the rest of his body is delineated by Delta Leonis and Theta Leonis.\r\rH.A. Rey has suggested an alternative way to connect the stars, which graphically shows a lion walking. The stars delta Leonis, gamma Leonis, eta Leonis, and theta Leonis form the body of the lion, with gamma Leonis being of the second magnitude and delta Leonis and theta Leonis being of the third magnitude. The stars gamma Leonis, zeta Leonis, mu Leonis, epsilon Leonis, and eta Leonis form the lion\u0027s neck, with epsilon Leonis being of the third magnitude. The stars mu Leonis, kappa Leonis, lambda Leonis, and epsilon Leonis form the head of the lion. Delta Leonis and beta Leonis form the lion\u0027s tail: beta Leonis, also known as Denebola, is the bright tip of the tail with a magnitude of two. The stars theta Leonis, iota Leonis, and sigma Leonis form the left hind leg of the lion, with sigma Leonis being the foot. The stars theta Leonis and rho Leonis form the right hind leg, with rho Leonis being the foot. The stars eta Leonis and alpha Leonis mark the lion\u0027s heart, with alpha Leonis, also known as Regulus, being the bright star of magnitude one. The stars eta Leonis and omicron Leonis form the right front foot of the Lion.",
		"key" : "Leo",
		"grouptype" : "Leo",
		"Meaning" : "lion",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Leo",
		"title" : "Leo Objects Group" },
	"Common" : "Kappa Leonis",
	"OType" : "Double or multiple star",
	"Distance" : "61.72",
	"RA_S" : 141.16357534,
	"DEC_S" : 26.18232599,
	"X" : 580,
	"Y" : 197,
	"Constellation" : "Leo ",
	"AMag" : 4.599,
	"key" : 27893,
	"title" : "Kappa Leonis"
	},
{
	"Index" : "7920",
	"Description" : "Lambda Leonis (\u03BB Leo, \u03BB Leonis) is a star in the constellation Leo. It has the traditional name Alterf, from the Arabic \u0627\u0644\u0637\u0631\u0641 a\u1E6D-\u1E6Darf \u0022the view (of the lion)\u0022.\r\rThis star, along with \u03BE Cnc, were the Persian Nahn, \u0022the Nose\u0022, and the Coptic Piautos, \u0022the Eye\u0022, both lunar asterisms.\r\rLambda Leonis is of spectral class K5 and apparent magnitude +4.32. It is approximately 336 light years from Earth.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "4 Leonis, Lambda Leonis, HIP 46750, SAO 80885, HD 82308, GC 13143, HR 3773, DM BD+23  2107, TYC 1959-1582-1",
	"group" : { "key" : "Leo" },
	"Common" : "Alterf",
	"OType" : "Variable Star",
	"Distance" : "100.87",
	"RA_S" : 142.93011451,
	"DEC_S" : 22.96797209,
	"X" : 564,
	"Y" : 242,
	"Constellation" : "Leo ",
	"AMag" : 4.475,
	"key" : 27920,
	"title" : "Alterf"
	},
{
	"Index" : "59537",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "5 Leonis, Xi Leonis, HIP 46771, SAO 98627, HD 82395, GC 13149, HR 3782, DM BD+11  2053, TYC 824-1978-1",
	"group" : { "key" : "Leo" },
	"Common" : "Xi Leonis",
	"OType" : "Variable Star",
	"Distance" : "66.06",
	"RA_S" : 142.98640503,
	"DEC_S" : 11.29982727,
	"Constellation" : "Leo ",
	"AMag" : 5.08,
	"key" : 79537,
	"title" : "Xi Leonis"
	},
{
	"Index" : "59275",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "6 Leonis, h Leonis, HIP 46774, SAO 117751, HD 82381, GC 13150, HR 3779, DM BD+10  2014, TYC 821-2131-1",
	"group" : { "key" : "Leo" },
	"Common" : "h Leonis",
	"OType" : "Star",
	"Distance" : "152.75",
	"RA_S" : 142.98990442,
	"DEC_S" : 9.71576409,
	"Constellation" : "Leo ",
	"AMag" : 5.216,
	"key" : 79275,
	"title" : "h Leonis"
	},
{
	"Index" : "11542",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "10 Leonis, HIP 47205, SAO 117807, HD 83240, GC 13283, HR 3827, DM BD+07  2160, TYC 241-2399-1",
	"group" : { "key" : "Leo" },
	"Common" : "10 Leonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "75.09",
	"RA_S" : 144.30280318,
	"DEC_S" : 6.83578162,
	"Constellation" : "Leo ",
	"AMag" : 5.125,
	"key" : 31542,
	"title" : "10 Leonis"
	},
{
	"Index" : "59274",
	"Description" : "Omicron Leonis (\u03BF Leo, \u03BF Leonis), known also by its traditional name, Subra, is a binary star in the constellation of Leo, west of Regulus, some 130 light years from here, where it marks one of the lion\u0027s forepaws.\r\rThe two stars of Omicron Leonis (Subra-A and Subra-B) are given variably as type F9III giant for the primary and A5mV dwarf for the secondary and subsequently as an F6II bright giant with a companion A7V dwarf star according to Kaler and others. Their combined apparent magnitude is +3.53.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "14 Leonis, Omicron Leonis, HIP 47508, SAO 98709, HD 83808, GC 13366, HR 3852, DM BD+10  2044A, TYC 821-2130-1",
	"group" : { "key" : "Leo" },
	"Common" : "Omicron Leonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "39.95",
	"RA_S" : 145.28764248,
	"DEC_S" : 9.89230752,
	"X" : 548,
	"Y" : 416,
	"Constellation" : "Leo ",
	"AMag" : 3.562,
	"key" : 79274,
	"title" : "Omicron Leonis"
	},
{
	"Index" : "7925",
	"Description" : "Epsilon Leonis (\u03B5 Leo, \u03B5 Leonis) is the fifth brightest star in the constellation Leo, consistent with its Bayer designation Epsilon. The star has the traditional names Ras Elased (Australis), Asad Australis and Algenubi, all of which derive from the Arabic \u0631\u0623\u0633 \u0627\u0644\u0623\u0633\u062F \u0627\u0644\u062C\u0646\u0648\u0628\u064A r\u0101s al-\u0027asad al-jan\u016Bb\u012B, which means \u0022the southern (star) of the lion\u0027s head\u0022; australis is Latin for \u0022southern\u0022.Epsilon Leonis has a stellar classification of G1 II, with the luminosity class of II indicating that, at an age of 162 million years, it has evolved into a bright giant. It is much larger and brighter than the Sun with a luminosity 288 times and a radius 21 times solar. Consequently, its absolute magnitude is actually \u20131.49, making it one of the more luminous stars in the constellation, significantly more than its alpha star, Regulus. Algenubi\u0027s apparent brightness, though, is only 2.98. Given its distance of about 247 light-years (76 parsecs), the star is more than 3 times the distance from the Sun than Regulus. At this distance, the visual magnitude of Epsilon Leonis is reduced by 0.03 as a result of extinction caused by intervening gas and dust.\r\rAlgenubi exhibits the characteristics of a Cepheid-like variable, changing by an amplitude of 0.3 magnitude every few days. It has around four times the mass of the Sun and a projected rotational velocity of 8.1 km s\u20131. Based upon its iron abundance, the metallicity of this star\u0027s outer atmosphere is only around 52% of the Sun\u0027s. That is, the abundance of elements other than hydrogen and helium is about half that in the Sun.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "17 Leonis, Epsilon Leonis, HIP 47908, SAO 81004, HD 84441, GC 13443, HR 3873, DM BD+24  2129, TYC 1960-1550-1",
	"group" : { "key" : "Leo" },
	"Common" : "Ras Elased / Asad Australis / Algenubi",
	"OType" : "Variable Star",
	"Distance" : "75.63",
	"RA_S" : 146.46280605,
	"DEC_S" : 23.77425356,
	"X" : 520,
	"Y" : 235,
	"Constellation" : "Leo ",
	"AMag" : 3.042,
	"key" : 27925,
	"shortTitle" : "Al Ras al Asad al Janubiyyah; Algenubi; Al Ashfar (with HD85503); Al'genubi",
	"title" : "Ras Elased / Asad Australis / Algenubi"
	},
{
	"Index" : "7934",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "22 Leonis, g Leonis, HIP 48390, SAO 81054, HD 85376, GC 13569, HR 3900, DM BD+25  2169, TYC 1961-1429-1",
	"group" : { "key" : "Leo" },
	"Common" : "g Leonis",
	"OType" : "High proper-motion Star",
	"Distance" : "41.29",
	"RA_S" : 147.97096591,
	"DEC_S" : 24.39536395,
	"Constellation" : "Leo ",
	"AMag" : 5.319,
	"key" : 27934,
	"title" : "g Leonis"
	},
{
	"Index" : "7960",
	"Description" : "Mu Leonis (\u03BC Leo, \u03BC Leonis) is a star in the constellation Leo. It has the traditional names Rasalas (Ras Elased Borealis) and Alshemali, abbreviations of Ras al Asad al Shamaliyy, from the Arabic \u0631\u0623\u0633 \u0627\u0644\u0623\u0633\u062F \u0627\u0644\u0634\u0645\u0627\u0644\u064A ra\u0027s al-\u0027asad a\u0161-\u0161am\u0101l\u012B \u0022the northern (star) of the lion\u0027s head\u0022.\r\rMu Leonis is of spectral class K3 and apparent magnitude +4.1. It is approximately 133 light years from Earth.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "24 Leonis, Mu Leonis, HIP 48455, SAO 81064, HD 85503, GC 13590, HR 3905, DM BD+26  2019, TYC 1964-1473-1",
	"group" : { "key" : "Leo" },
	"Common" : "Rasalas / Alshemali",
	"OType" : "High proper-motion Star",
	"Distance" : "38.05",
	"RA_S" : 148.19090555,
	"DEC_S" : 26.00695148,
	"X" : 498,
	"Y" : 207,
	"Constellation" : "Leo ",
	"AMag" : 4.013,
	"key" : 27960,
	"shortTitle" : "Rasalas; Ras al Asad al Shamaliyy; Alshemali; Al Ashfar (with HD84441)",
	"title" : "Rasalas / Alshemali"
	},
{
	"Index" : "60306",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "27 Leonis, Nu Leonis, HIP 48883, SAO 98876, HD 86360, GC 13724, HR 3937, DM BD+13  2183, TYC 832-1658-1",
	"group" : { "key" : "Leo" },
	"Common" : "Nu Leonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "152.89",
	"RA_S" : 149.5557335,
	"DEC_S" : 12.44479925,
	"Constellation" : "Leo ",
	"AMag" : 5.252,
	"key" : 80306,
	"title" : "Nu Leonis"
	},
{
	"Index" : "60009",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "29 Leonis, Pi Leonis, HIP 49029, SAO 118044, HD 86663, GC 13755, HR 3950, DM BD+08  2301, TYC 829-1744-1",
	"group" : { "key" : "Leo" },
	"Common" : "Pi Leonis",
	"OType" : "Variable Star",
	"Distance" : "124.34",
	"RA_S" : 150.05335881,
	"DEC_S" : 8.04422465,
	"Constellation" : "Leo ",
	"AMag" : 4.859,
	"key" : 80009,
	"title" : "Pi Leonis"
	},
{
	"Index" : "3427",
	"Description" : "Eta Leonis (\u03B7 Leo, \u03B7 Leonis) is a fourth-magnitude star in the constellation Leo. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "30 Leonis, Eta Leonis, HIP 49583, SAO 98955, HD 87737, GC 13899, HR 3975, DM BD+17  2171, TYC 1412-1695-1",
	"group" : { "key" : "Leo" },
	"Common" : "Eta Leonis",
	"OType" : "Star",
	"Distance" : "387.3",
	"RA_S" : 151.83313275,
	"DEC_S" : 16.76266119,
	"X" : 460,
	"Y" : 330,
	"Constellation" : "Leo ",
	"AMag" : 3.49,
	"key" : 23427,
	"title" : "Eta Leonis"
	},
{
	"Index" : "60105",
	"Description" : "31 Leonis (31 Leo) is a star in the constellation Leo. Its apparent magnitude is 4.38.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "31 Leonis, A Leonis, HIP 49637, SAO 98964, HD 87837, GC 13911, HR 3980, DM BD+10  2112, TYC 830-1496-1",
	"group" : { "key" : "Leo" },
	"Common" : "31 Leonis",
	"OType" : "Star",
	"Distance" : "90.53",
	"RA_S" : 151.97612751,
	"DEC_S" : 9.99750678,
	"X" : 462,
	"Y" : 418,
	"Constellation" : "Leo ",
	"AMag" : 4.532,
	"key" : 80105,
	"title" : "31 Leonis"
	},
{
	"Index" : "7998",
	"Description" : "Zeta Leonis (\u03B6 Leo, \u03B6 Leonis) is a third-magnitude star in the constellation Leo, the lion. It has the traditional name Adhafera (Aldhafera, Adhafara), from the Arabic \u0627\u0644\u0636\u0641\u064A\u0631\u0629 al-\u00F0af\u012Brah \u0022the braid/curl\u0022, a reference to its position in the lion\u0027s mane. It forms the second star (after Gamma Leonis) in the blade of \u0022The Sickle\u0022, which is an asterism formed from the head of Leo.Adhafera is a giant star with a stellar classification of F0 III. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Its apparent magnitude is +3.44, making it relatively faint for a star that is visible to the naked eye. Nevertheless, it shines with 85 times the luminosity of the Sun. Adhafera has about three times the Sun\u0027s mass and six times the radius of the Sun. Parallax measurements from the Hipparcos satellite yield an estimated distance to Adhafera of 274 light-years (84 parsecs) from Earth.\r\rAdhafera forms a double star with an optical companion that has an apparent magnitude of 5.90. Known as 35 Leo, this star is separated from Adhafera by 325.9 arcseconds along a position angle of 340\u00B0. The two stars do not form a binary star system as 35 Leo is only 100 light years from Earth.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "36 Leonis, Zeta Leonis, HIP 50335, SAO 81265, HD 89025, GC 14107, HR 4031, DM BD+24  2209, TYC 1969-1261-1",
	"group" : { "key" : "Leo" },
	"Common" : "Adhafera",
	"OType" : "Variable Star",
	"Distance" : "84.01",
	"RA_S" : 154.17256653,
	"DEC_S" : 23.41731168,
	"X" : 429,
	"Y" : 244,
	"Constellation" : "Leo ",
	"AMag" : 3.455,
	"key" : 27998,
	"shortTitle" : "Aldhafara; Aldhafera; Adkhafera",
	"title" : "Adhafera"
	},
{
	"Index" : "3512",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "40 Leonis, HIP 50564, SAO 99065, HD 89449, GC 14170, HR 4054, DM BD+20  2466, TYC 1423-1351-1",
	"group" : { "key" : "Leo" },
	"Common" : "40 Leonis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "21.37",
	"RA_S" : 154.93403667,
	"DEC_S" : 19.47091207,
	"Constellation" : "Leo ",
	"AMag" : 4.834,
	"key" : 23512,
	"title" : "40 Leonis"
	},
{
	"Index" : "3511",
	"Description" : "Gamma Leonis (\u03B3 Leo, \u03B3 Leonis) is a binary star system in the constellation Leo. It has the traditional name Algieba or Al Gieba. The name Algieba originates from the Arabic \u0627\u0644\u062C\u0628\u0647\u0629 Al-Jabhah, meaning the forehead. Despite this meaning, the star actually appears in the mane of Leo. The star\u0027s Latin name is Juba. Algieba, as a binary system, consists of two stars. The brighter component has an apparent magnitude of +2.28 and is of spectral class K1-IIIbCN-0.5. The giant K star has a surface temperature of 4,470 K, a luminosity 180 times that of Earth\u0027s Sun, and a diameter 23 times that of the Sun. The companion star has an apparent magnitude of +3.51 and belongs to the spectral class G7IIICN-I. The giant G star has a temperature of 4,980 K, a luminosity of 50 times that of the Sun, and a diameter 10 times that of the Sun. With angular separation of just over 4\u0022, the two stars are at least 170 AU apart (four times the distance between Pluto and the Sun), and have an orbital period of over 500 years. Because the orbital period is so long, only a fraction of the full path has been observed since discovery.\r\rBoth stars are almost certainly true giants, meaning that they have stopped fusing hydrogen to helium in their cores and have expanded to great proportions. Although there has been too little observation of their orbit to calculate their masses, comparison with evolutionary calculations suggests that each are about double the mass of the Sun. Originating from the same interstellar cloud some two billion years ago, the stars have iron contents about a third that of the Sun. It is hard to tell how far along they might be in their life cycle. They both may be fusing helium in their cores, or they could be giants in development, with quiet helium cores that are waiting to fire up. The chemical composition at the surface, which is influenced by age, suggests the former.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "41 Leonis, Gamma02 Leonis, HIP 50583B, SAO 81299, HD 89485, GC 14178, HR 4058, DM BD+20  2467B, TYC 1423-1349-2",
	"group" : { "key" : "Leo" },
	"Common" : "Algieba / Al Gieba",
	"OType" : "High proper-motion Star",
	"Distance" : "39.87",
	"RA_S" : 154.99425,
	"DEC_S" : 19.84075,
	"X" : 421,
	"Y" : 291,
	"Constellation" : "Leo ",
	"AMag" : 3.644,
	"key" : 23511,
	"title" : "Algieba / Al Gieba"
	},
{
	"Index" : "60942",
	"Description" : "Rho Leonis (\u03C1 Leo) is a binary star in the zodiac constellation of Leo, and, like the prominent nearby star Regulus, it is located near the ecliptic. With an apparent visual magnitude of 3.9, this star can be readily seen with the naked eye at night. Parallax measurements give a distance estimate of about 5,400 light-years (1,700 parsecs) from the Earth.\r\rThis is an enormous star with about 21 times the Sun\u0027s mass and 37 times the Sun\u0027s radius. Its spectrum matches a stellar classification of B1 Iab, with the \u0027Iab\u0027 luminosity class indicating that it is in the supergiant stage of its evolution. Rho Leonis is radiating about 295,000 times the Sun\u0027s luminosity at an effective temperature of 24,200 K, giving it the blue-white hue typical of a B-type star. A strong stellar wind is expelling mass from the outer envelope at a rate of 3.5 \u00D7 10\u20137 times the Sun\u0027s mass per year, or the equivalent of a solar mass every 2.8 million years. The rotation rate is probably about once per 7 days, with an upper limit of 47 days.\r\rRho Leonis is classified as a runaway star, which means it has a peculiar velocity of at least 30 km s\u20131 relative to the surrounding stars. It has radial velocity of 42 km s\u20131 away from the Sun and a proper motion that is carrying it about 1.56 Astronomical Units per year, equivalent to 7 km s\u20131, in a transverse direction. The star is situated about 2,300 light-years (710 parsecs) above the galactic plane.\r\rThis is a binary star system with a magnitude 4.8 companion at an angular separation of 0.11 arcseconds.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "47 Leonis, Rho Leonis, HIP 51624, SAO 118355, HD 91316, GC 14487, HR 4133, DM BD+10  2166, TYC 838-1485-1",
	"group" : { "key" : "Leo" },
	"Common" : "Rho Leonis",
	"OType" : "Blue supergiant star",
	"RA_S" : 158.20279801,
	"DEC_S" : 9.306586,
	"X" : 382,
	"Y" : 429,
	"Constellation" : "Leo ",
	"AMag" : 3.806,
	"key" : 80942,
	"title" : "Rho Leonis"
	},
{
	"Index" : "12982",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "48 Leonis, HIP 51775, SAO 118376, HD 91612, GC 14533, HR 4146, DM BD+07  2330, TYC 259-1552-1",
	"group" : { "key" : "Leo" },
	"Common" : "48 Leonis",
	"OType" : "Star",
	"Distance" : "81.52",
	"RA_S" : 158.70005804,
	"DEC_S" : 6.9537457,
	"Constellation" : "Leo ",
	"AMag" : 5.174,
	"key" : 32982,
	"title" : "48 Leonis"
	},
{
	"Index" : "61726",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "53 Leonis, l Leonis, HIP 52911, SAO 99305, HD 93702, GC 14889, HR 4227, DM BD+11  2283, TYC 849-1444-1",
	"group" : { "key" : "Leo" },
	"Common" : "l Leonis",
	"OType" : "Star",
	"Distance" : "116.51",
	"RA_S" : 162.31429385,
	"DEC_S" : 10.54520104,
	"Constellation" : "Leo ",
	"AMag" : 5.315,
	"key" : 81726,
	"title" : "l Leonis"
	},
{
	"Index" : "8076",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "54 Leonis, HIP 53417A, SAO 81583, HD 94601, GC 15016, HR 4259, DM BD+25  2314A, TYC 1978-2295-1",
	"group" : { "key" : "Leo" },
	"Common" : "54 Leonis",
	"OType" : "Star",
	"Distance" : "87.65",
	"RA_S" : 163.90333907,
	"DEC_S" : 24.74972237,
	"Constellation" : "Leo ",
	"AMag" : 4.477,
	"key" : 28076,
	"title" : "54 Leonis"
	},
{
	"Index" : "13490",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "58 Leonis, d Leonis, HIP 53807, SAO 118610, HD 95345, GC 15125, HR 4291, DM BD+04  2407, TYC 265-1270-1",
	"group" : { "key" : "Leo" },
	"Common" : "d Leonis",
	"OType" : "Double or multiple star",
	"Distance" : "110.43",
	"RA_S" : 165.14019851,
	"DEC_S" : 3.61749809,
	"Constellation" : "Leo ",
	"AMag" : 4.968,
	"key" : 33490,
	"title" : "d Leonis"
	},
{
	"Index" : "13940",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "59 Leonis, c Leonis, HIP 53824, SAO 118615, HD 95382, GC 15130, HR 4294, DM BD+06  2384, TYC 268-1064-1",
	"group" : { "key" : "Leo" },
	"Common" : "c Leonis",
	"OType" : "Star",
	"Distance" : "46.35",
	"RA_S" : 165.18667868,
	"DEC_S" : 6.10144912,
	"Constellation" : "Leo ",
	"AMag" : 4.998,
	"key" : 33940,
	"title" : "c Leonis"
	},
{
	"Index" : "33311",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "61 Leonis, p02 Leonis, HIP 53907, SAO 137947, HD 95578, GC 15151, HR 4299, DM BD-01  2471, TYC 4921-1207-1",
	"group" : { "key" : "Leo" },
	"Common" : "p02 Leonis",
	"OType" : "Variable Star",
	"Distance" : "178.81",
	"RA_S" : 165.45698129,
	"DEC_S" : -2.48458683,
	"Constellation" : "Leo ",
	"AMag" : 4.912,
	"key" : 53311,
	"title" : "p02 Leonis"
	},
{
	"Index" : "3599",
	"Description" : "60 Leonis (60 Leo) is a star in the constellation Leo. Its apparent magnitude is 4.41.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "60 Leonis, b Leonis, HIP 53954, SAO 81637, HD 95608, GC 15162, HR 4300, DM BD+20  2547, TYC 1436-1306-1",
	"group" : { "key" : "Leo" },
	"Common" : "60 Leonis",
	"OType" : "Variable Star",
	"Distance" : "38.86",
	"RA_S" : 165.58239885,
	"DEC_S" : 20.17984033,
	"X" : 291,
	"Y" : 286,
	"Constellation" : "Leo ",
	"AMag" : 4.405,
	"key" : 23599,
	"title" : "60 Leonis"
	},
{
	"Index" : "13941",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "63 Leonis, Chi Leonis, HIP 54182, SAO 118648, HD 96097, GC 15235, HR 4310, DM BD+08  2455, TYC 268-1067-1",
	"group" : { "key" : "Leo" },
	"Common" : "Chi Leonis",
	"OType" : "Variable Star",
	"Distance" : "28.99",
	"RA_S" : 166.2542855,
	"DEC_S" : 7.33600866,
	"Constellation" : "Leo ",
	"AMag" : 4.66,
	"key" : 33941,
	"title" : "Chi Leonis"
	},
{
	"Index" : "33322",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "69 Leonis, p05 Leonis, HIP 54849, SAO 118731, HD 97585, GC 15430, HR 4356, DM BD+00  2761, TYC 4922-1217-1",
	"group" : { "key" : "Leo" },
	"Common" : "p05 Leonis",
	"OType" : "Star",
	"Distance" : "161.39",
	"RA_S" : 168.43980088,
	"Constellation" : "Leo ",
	"AMag" : 5.399,
	"key" : 53322,
	"title" : "p05 Leonis"
	},
{
	"Index" : "3643",
	"Description" : "Delta Leonis (\u03B4 Leo, \u03B4 Leonis) is a star in the zodiac constellation of Leo. It has the traditional names Zosma (or Zozma) and Duhr. Rare spellings include Zozca, Zosca, Zubra, and Dhur. The name Zosma means girdle in ancient Greek, referring to the star\u0027s location in its constellation, on the hip of the lion. Based upon parallax measurements, it lies at a distance of about 58.4 light-years (17.9 parsecs) from the Earth.Zosma is a relatively ordinary main sequence star with a stellar classification of A4 V, making it is somewhat larger and hotter than the Sun. It is a fairly well-studied star, allowing relatively accurate measurements of its age and size. The radius of the star, as measured directly using an interferometer, is about 214% of the Sun\u0027s radius and it is emitting more than 15 times as much luminosity as the Sun. The energy is being emitted from the outer envelope with an effective temperature 8,296 K, giving it the white hue characteristic of an A-type star. Having a larger mass than the Sun it will have a shorter lifespan, and in another 600 million years or so will swell into an orange or red giant star before decaying quietly into a white dwarf.\r\rThis star is rotating rapidly, with a projected rotational velocity of 180 km s\u20131. The inclination of the axis of rotation to the line of sight from the Earth is estimated at 38.1\u00B0, which would mean the azimuthal velocity along the equator is about 280 180 km s\u20131. This rotation is producing an equatorial bulge, giving the star a pronounced oblate spheroidal shape. The polar radius is about 84% of the radius along the equator.\r\rBased upon the location and trajectory of this star through space, it may be a member of the Ursa Major Moving Group, a type of stellar kinematics group that share a common origin and motion through space. The age of this group is about 500 million years.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "68 Leonis, Delta Leonis, HIP 54872, SAO 81727, HD 97603, GC 15438, HR 4357, DM BD+21  2298, TYC 1439-2479-1",
	"group" : { "key" : "Leo" },
	"Common" : "Zosma / Duhr",
	"OType" : "High proper-motion Star",
	"Distance" : "17.91",
	"RA_S" : 168.52708927,
	"DEC_S" : 20.52371814,
	"X" : 255,
	"Y" : 281,
	"Constellation" : "Leo ",
	"AMag" : 2.544,
	"key" : 23643,
	"shortTitle" : "Zozma; Zosca; Zozca; Duhr; Dhur; Zubra; Tsolma",
	"title" : "Zosma / Duhr"
	},
{
	"Index" : "3617",
	"Description" : "Theta Leonis (\u03B8 Leo, \u03B8 Leonis) is a star in the constellation Leo. It has the traditional names Chertan, Chort and Coxa. With an apparent visual magnitude of +3.324 it is visible to the naked eye and forms one of the brighter stars in the constellation. The distance from Earth can be directly determined from parallax measurements, yielding a value of about 165 light-years (51 parsecs).\r\rThis is a large star with 2.5 times the mass of the Sun. The spectrum matches a stellar classification of A2 V, making this a seemingly typical A-type main sequence star. However, the spectrum shows enhanced absorption lines of metals, marking this as a chemically peculiar Am star. The abundance of elements other than hydrogen and helium, what astronomers term the star\u0027s metallicity, appears around 12% higher than in the Sun. It is radiating 141 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 9,350 K, literally giving it a white-hot glow.\r\rTheta Leonis is much younger than the Sun, with an estimated age of around 550 million years. It has a moderately high rate of rotation, with a projected rotational velocity of 23 km s\u20131. Measurements in the infrared band show an excess of emission from the star and its surroundings, suggesting the presence of a circumstellar disk of dust. The temperature of this emission indicates the disk has an orbital radius of 36 AU.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "70 Leonis, Theta Leonis, HIP 54879, SAO 99512, HD 97633, GC 15441, HR 4359, DM BD+16  2234, TYC 1437-2847-1",
	"group" : { "key" : "Leo" },
	"Common" : "Theta Leonis",
	"OType" : "Variable Star",
	"Distance" : "50.6",
	"RA_S" : 168.56002313,
	"DEC_S" : 15.4295709,
	"X" : 252,
	"Y" : 347,
	"Constellation" : "Leo ",
	"AMag" : 3.304,
	"key" : 23617,
	"shortTitle" : "Coxa; Chort; Khort",
	"title" : "Theta Leonis"
	},
{
	"Index" : "8115",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "72 Leonis, HIP 54951, SAO 81736, HD 97778, GC 15460, HR 4362, DM BD+23  2322, TYC 1981-2471-1",
	"group" : { "key" : "Leo" },
	"Common" : "72 Leonis",
	"OType" : "Long-period variable star",
	"Distance" : "281.76",
	"RA_S" : 168.80094818,
	"DEC_S" : 23.09551311,
	"Constellation" : "Leo ",
	"AMag" : 4.74,
	"key" : 28115,
	"title" : "72 Leonis"
	},
{
	"Index" : "63028",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "73 Leonis, n Leonis, HIP 55016, SAO 99525, HD 97907, GC 15487, HR 4365, DM BD+14  2367, TYC 861-1283-1",
	"group" : { "key" : "Leo" },
	"Common" : "n Leonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "117.49",
	"RA_S" : 168.96622432,
	"DEC_S" : 13.30756743,
	"Constellation" : "Leo ",
	"AMag" : 5.45,
	"key" : 83028,
	"title" : "n Leonis"
	},
{
	"Index" : "33352",
	"Description" : "Phi Leonis (\u03C6 Leo) is a star in the constellation Leo. Its apparent magnitude is 4.47.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "74 Leonis, Phi Leonis, HIP 55084, SAO 138102, HD 98058, GC 15511, HR 4368, DM BD-02  3315, TYC 4925-1610-1",
	"group" : { "key" : "Leo" },
	"Common" : "Phi Leonis",
	"OType" : "Star",
	"Distance" : "56.45",
	"RA_S" : 169.16541928,
	"DEC_S" : -3.65160365,
	"X" : 238,
	"Y" : 595,
	"Constellation" : "Leo ",
	"AMag" : 4.477,
	"key" : 53352,
	"title" : "Phi Leonis"
	},
{
	"Index" : "13273",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "75 Leonis, HIP 55137, SAO 118764, HD 98118, GC 15520, HR 4371, DM BD+02  2409, TYC 263-1171-1",
	"group" : { "key" : "Leo" },
	"Common" : "75 Leonis",
	"OType" : "High proper-motion Star",
	"Distance" : "101.75",
	"RA_S" : 169.32249985,
	"DEC_S" : 2.01055696,
	"Constellation" : "Leo ",
	"AMag" : 5.344,
	"key" : 33273,
	"title" : "75 Leonis"
	},
{
	"Index" : "14205",
	"Description" : "Sigma Leonis (\u03C3 Leo) is a blue-white 4th-magnitude star in the constellation Leo.\r\rSigma Leonis is of the spectral class B9.5Vs and has an apparent magnitude of +4.04.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "77 Leonis, Sigma Leonis, HIP 55434, SAO 118804, HD 98664, GC 15600, HR 4386, DM BD+06  2437, TYC 270-1148-1",
	"group" : { "key" : "Leo" },
	"Common" : "Sigma Leonis",
	"OType" : "Star",
	"Distance" : "67.46",
	"RA_S" : 170.28413935,
	"DEC_S" : 6.02932234,
	"X" : 226,
	"Y" : 469,
	"Constellation" : "Leo ",
	"AMag" : 4.031,
	"key" : 34205,
	"title" : "Sigma Leonis"
	},
{
	"Index" : "62539",
	"Description" : "Iota Leonis is a star in the constellation Leo.\r\rIt was known as \u592A\u5FAE\u53F3\u57A3\u4E09, \u0022the Third (Star) of the Right Wall of the Supreme Palace Enclosure\u0022 or \u6B21\u5C07 (Tsze Tseang, Mandarin c\u00ECji\u00E0ng), \u0022the Vice-General\u0022, in traditional Chinese astronomy\r\rIota Leonis is of stellar classification F3 V and apparent visual magnitude +3.94. It is a spectroscopic binary, which means it is a binary star with components that are too close together to be able to resolve individually through a telescope.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "78 Leonis, Iota Leonis, HIP 55642A, SAO 99587, HD 99028, GC 15652, HR 4399, DM BD+11  2348, TYC 858-1221-1",
	"group" : { "key" : "Leo" },
	"Common" : "Iota Leonis",
	"OType" : "Star",
	"Distance" : "23.66",
	"RA_S" : 170.98108722,
	"DEC_S" : 10.52953361,
	"X" : 218,
	"Y" : 409,
	"Constellation" : "Leo ",
	"AMag" : 4.056,
	"key" : 82539,
	"title" : "Iota Leonis"
	},
{
	"Index" : "62540",
	"Description" : "Iota Leonis is a star in the constellation Leo.\r\rIt was known as \u592A\u5FAE\u53F3\u57A3\u4E09, \u0022the Third (Star) of the Right Wall of the Supreme Palace Enclosure\u0022 or \u6B21\u5C07 (Tsze Tseang, Mandarin c\u00ECji\u00E0ng), \u0022the Vice-General\u0022, in traditional Chinese astronomy\r\rIota Leonis is of stellar classification F3 V and apparent visual magnitude +3.94. It is a spectroscopic binary, which means it is a binary star with components that are too close together to be able to resolve individually through a telescope.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "78 Leonis, Iota Leonis, HIP 55642B, SAO 99587, HD 99028, GC 15652, HR 4399, DM BD+11  2348, TYC 858-1221-2",
	"group" : { "key" : "Leo" },
	"Common" : "Iota Leonis",
	"OType" : "Star",
	"Distance" : "23.66",
	"RA_S" : 170.98108722,
	"DEC_S" : 10.52953361,
	"X" : 218,
	"Y" : 409,
	"Constellation" : "Leo ",
	"AMag" : 6.708,
	"key" : 82540,
	"title" : "Iota Leonis"
	},
{
	"Index" : "13364",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "79 Leonis, HIP 55650, SAO 118831, HD 99055, GC 15656, HR 4400, DM BD+02  2418, TYC 264-1157-1",
	"group" : { "key" : "Leo" },
	"Common" : "79 Leonis",
	"OType" : "Star",
	"Distance" : "108.33",
	"RA_S" : 171.00969423,
	"DEC_S" : 1.40776211,
	"Constellation" : "Leo ",
	"AMag" : 5.49,
	"key" : 33364,
	"title" : "79 Leonis"
	},
{
	"Index" : "13773",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "84 Leonis, Tau Leonis, HIP 55945, SAO 118875, HD 99648, GC 15729, HR 4418, DM BD+03  2504, TYC 267-1193-1",
	"group" : { "key" : "Leo" },
	"Common" : "Tau Leonis",
	"OType" : "Star",
	"Distance" : "171.75",
	"RA_S" : 171.98433197,
	"DEC_S" : 2.85626784,
	"Constellation" : "Leo ",
	"AMag" : 5.053,
	"key" : 33773,
	"title" : "Tau Leonis"
	},
{
	"Index" : "33399",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "87 Leonis, e Leonis, HIP 56127, SAO 138238, HD 99998, GC 15779, HR 4432, DM BD-02  3360, TYC 4933-1387-1",
	"group" : { "key" : "Leo" },
	"Common" : "e Leonis",
	"OType" : "Star",
	"Distance" : "184.46",
	"RA_S" : 172.57871795,
	"DEC_S" : -3.00349814,
	"Constellation" : "Leo ",
	"AMag" : 4.929,
	"key" : 53399,
	"title" : "e Leonis"
	},
{
	"Index" : "33374",
	"Description" : "Upsilon Leonis (\u03C5 Leo) is a star in the constellation Leo. Its apparent magnitude is 4.31.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "91 Leonis, Upsilon Leonis, HIP 56647, SAO 138298, HD 100920, GC 15927, HR 4471, DM BD-00  2458, TYC 4930-1093-1",
	"group" : { "key" : "Leo" },
	"Common" : "Upsilon Leonis",
	"OType" : "Star",
	"Distance" : "55.64",
	"RA_S" : 174.23721238,
	"DEC_S" : -0.82374681,
	"X" : 172,
	"Y" : 557,
	"Constellation" : "Leo ",
	"AMag" : 4.414,
	"key" : 53374,
	"title" : "Upsilon Leonis"
	},
{
	"Index" : "3655",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "92 Leonis, HIP 56975, SAO 81941, HD 101484, GC 16030, HR 4495, DM BD+22  2391, TYC 1440-2596-1",
	"group" : { "key" : "Leo" },
	"Common" : "92 Leonis",
	"OType" : "Star",
	"Distance" : "82.68",
	"RA_S" : 175.19611478,
	"DEC_S" : 21.35272392,
	"Constellation" : "Leo ",
	"AMag" : 5.363,
	"key" : 23655,
	"title" : "92 Leonis"
	},
{
	"Index" : "3698",
	"Description" : "93 Leonis (93 Leo) is a star in the constellation Leo. Its apparent magnitude is 4.54.",
	"MapNum" : "30",
	"ImageNum" : "30",
	"Desig" : "93 Leonis, HIP 57565, SAO 81998, HD 102509, GC 16173, HR 4527, DM BD+21  2358, TYC 1443-2662-1",
	"group" : { "key" : "Leo" },
	"Common" : "93 Leonis",
	"OType" : "Variable of RS CVn type",
	"Distance" : "71.3",
	"RA_S" : 176.99639963,
	"DEC_S" : 20.21893252,
	"X" : 152,
	"Y" : 278,
	"Constellation" : "Leo ",
	"AMag" : 4.585,
	"key" : 23698,
	"title" : "93 Leonis"
	},
{
	"Index" : "12229",
	"Description" : "10 Leonis Minoris (10 LMi) is a star in the constellation Leo Minor. Its apparent magnitude is 4.60.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "10 Leonis Minoris, HIP 46952, SAO 61570, HD 82635, GC 13203, HR 3800, DM BD+37  2004, TYC 2500-1532-1",
	"group" : { "backgroundImage" : "images/Alignment/32.png",
		"description" : "Leo Minor is a small and faint constellation in the northern celestial hemisphere. Its name is Latin for \u0022the smaller lion\u0022, in contrast to Leo, the larger lion. It lies between the larger and more recognizable Ursa Major to the north and Leo to the south. Leo Minor was not regarded as a separate constellation by classical astronomers; it was designated by Johannes Hevelius in 1687.\r\rThere are 37 stars brighter than apparent magnitude 6.5 in the constellation; three are brighter than magnitude 4.5. 46 Leonis Minoris, an orange giant of magnitude 3.8, is located some 95 light years from Earth. At magnitude 4.4, Beta Leonis Minoris is the second brightest star and the only one in the constellation with a Bayer designation. It is a binary star, the brighter component of which is an orange giant and the fainter a yellow-white main sequence star. The third brightest star is 21 Leonis Minoris, a rapidly rotating white main sequence star of average magnitude 4.5. The constellation also includes two stars with planetary systems, two pairs of interacting galaxies, and the unique deep-sky object Hanny\u0027s Voorwerp.\r\rThe classical astronomers Aratus and Ptolemy had noted the region of what is now Leo Minor to be undefined and not containing any distinctive pattern; Ptolemy classified the stars in this area as amorph\u014Dtoi (not belonging to a constellation outline) within the constellation Leo. Johannes Hevelius first depicted Leo Minor in 1687 when he outlined ten new constellations in his star atlas Firmamentum Sobiescianum, and included 18 of its objects in the accompanying Catalogus Stellarum Fixarum. Hevelius decided upon Leo Minor or Leo Junior as a depiction that would align with its beastly neighbours the Lion and the Great Bear. In 1845, English astronomer Francis Baily revised the catalogue of Hevelius\u0027s new constellations, and assigned a Greek letter known as Bayer designation to stars brighter than apparent magnitude 4.5. Richard A. Proctor gave the constellation the name Leaena \u0022the Lioness\u0022 in 1870, explaining that he sought to shorten the constellation names to make them more manageable on celestial charts.\r\rGerman astronomer Christian Ludwig Ideler posited that the stars of Leo Minor had been termed Al Thib\u0101\u0027 wa-Aul\u0101duh\u0101 \u0022Gazelle with her Young\u0022 on a 13th-century Arabic celestial globe, recovered by Cardinal Stefano Borgia and housed in the prelate\u0027s museum at Velletri. Arabist Friedrich Wilhelm Lach describes a different view, noting that they had been seen as Al Haud \u0022the Pond\u0022, which the Gazelle jumps into. In Chinese astronomy, the stars Beta, 30, 37 and 46 Leonis Minoris made up Neiping, a \u0022Court of Judge or Mediator\u0022, or Shi \u0022Court Eunuch\u0022 or were combined with stars of the neighbouring Leo to make up a large celestial dragon or State Chariot. A line of four stars was known as Shaowei; it represented four Imperial advisors and may have been located in Leo Minor, Leo or adjacent regions.\r\rA dark area of the sky with a triangle of brighter stars just visible to the naked eye in good conditions, Leo Minor has been described by Patrick Moore as having \u0022dubious claims to a separate identity\u0022. It is a small constellation bordered by Ursa Major to the north, Lynx to the west, Leo to the south, and touching the corner of Cancer to the southwest. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027LMi\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 16 sides. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 9h 22.4m and 11h 06.5m, while the declination coordinates are between 22.84\u00B0 and 41.43\u00B0. Ranked 64th out of 88 constellations in size, Leo Minor covers an area of 232.0 square degrees, or 0.562 percent of the sky. It culminates each year at midnight on February 24, and at 9 p.m. on May 24.",
		"key" : "Leo Minor",
		"grouptype" : "Leo Minor",
		"Meaning" : "lesser lion",
		"Family" : "Ursa Major",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Leo Minor",
		"title" : "Leo Minor Objects Group" },
	"Common" : "10 Leonis Minoris",
	"OType" : "Variable of RS CVn type",
	"Distance" : "56.71",
	"RA_S" : 143.55575614,
	"DEC_S" : 36.39755932,
	"X" : 292,
	"Y" : 424,
	"Constellation" : "Leo Minor ",
	"AMag" : 4.64,
	"key" : 32229,
	"title" : "10 Leonis Minoris"
	},
{
	"Index" : "12230",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "11 Leonis Minoris, HIP 47080, SAO 61586, HD 82885A, GC 13242, HR 3815, DM BD+36  1979, TYC 2500-1533-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "11 Leonis Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "11.37",
	"RA_S" : 143.91461051,
	"DEC_S" : 35.8101674,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.478,
	"key" : 32230,
	"title" : "11 Leonis Minoris"
	},
{
	"Index" : "16512",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "19 Leonis Minoris, HIP 48833, SAO 43115, HD 86146, GC 13700, HR 3928, DM BD+41  2033, TYC 2996-1547-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "19 Leonis Minoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "28.13",
	"RA_S" : 149.42105684,
	"DEC_S" : 41.05563156,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.157,
	"key" : 36512,
	"title" : "19 Leonis Minoris"
	},
{
	"Index" : "12260",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "20 Leonis Minoris, HIP 49081, SAO 61808, HD 86728, GC 13763, HR 3951, DM BD+32  1964, TYC 2503-1516-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "20 Leonis Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "15.05",
	"RA_S" : 150.252735,
	"DEC_S" : 31.92366903,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.451,
	"key" : 32260,
	"title" : "20 Leonis Minoris"
	},
{
	"Index" : "12300",
	"Description" : "21 Leonis Minoris (21 LMi) is a white main sequence star in the constellation Leo Minor with an apparent magnitude of 4.49.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "21 Leonis Minoris, HIP 49593, SAO 61874, HD 87696, GC 13896, HR 3974, DM BD+35  2110, TYC 2509-1343-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "21 Leonis Minoris",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "28.24",
	"RA_S" : 151.85733873,
	"DEC_S" : 35.24469466,
	"X" : 203,
	"Y" : 425,
	"Constellation" : "Leo Minor ",
	"AMag" : 4.498,
	"key" : 32300,
	"title" : "21 Leonis Minoris"
	},
{
	"Index" : "8042",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "23 Leonis Minoris, HIP 50303, SAO 81258, HD 88960, GC 14086, HR 4024, DM BD+30  1981, TYC 1975-1399-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "23 Leonis Minoris",
	"OType" : "Star",
	"Distance" : "79.9",
	"RA_S" : 154.06013364,
	"DEC_S" : 29.31050105,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.489,
	"key" : 28042,
	"title" : "23 Leonis Minoris"
	},
{
	"Index" : "12339",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "30 Leonis Minoris, HIP 51056, SAO 62038, HD 90277, GC 14315, HR 4090, DM BD+34  2128, TYC 2514-1294-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "30 Leonis Minoris",
	"OType" : "Star",
	"Distance" : "71.51",
	"RA_S" : 156.47839085,
	"DEC_S" : 33.79612051,
	"Constellation" : "Leo Minor ",
	"AMag" : 4.751,
	"key" : 32339,
	"title" : "30 Leonis Minoris"
	},
{
	"Index" : "12357",
	"Description" : "Beta Leonis Minoris (Beta LMi, \u03B2 Leonis Minoris, \u03B2 LMi) is a binary star in the constellation of Leo Minor. It has an overall apparent visual magnitude of approximately 4.215. Although it is the only star in Leo Minor with a Bayer designation, it is only the second brightest star in the constellation (the brightest is 46 Leonis Minoris.)",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "31 Leonis Minoris, Beta Leonis Minoris, HIP 51233AB, SAO 62053, HD 90537, GC 14358, HR 4100, DM BD+37  2080, TYC 2517-1209-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "Beta Leonis Minoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.16",
	"RA_S" : 156.97085298,
	"DEC_S" : 36.70722132,
	"X" : 154,
	"Y" : 392,
	"Constellation" : "Leo Minor ",
	"AMag" : 4.304,
	"key" : 32357,
	"title" : "Beta Leonis Minoris"
	},
{
	"Index" : "12324",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "37 Leonis Minoris, HIP 52098, SAO 62173, HD 92125, GC 14624, HR 4166, DM BD+32  2061, TYC 2512-1144-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "37 Leonis Minoris",
	"OType" : "Star",
	"Distance" : "176.89",
	"RA_S" : 159.68005495,
	"DEC_S" : 31.97623934,
	"Constellation" : "Leo Minor ",
	"AMag" : 4.768,
	"key" : 32324,
	"title" : "37 Leonis Minoris"
	},
{
	"Index" : "8063",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "41 Leonis Minoris, HIP 52457, SAO 81490, HD 92825, GC 14740, HR 4192, DM BD+23  2253, TYC 1977-2632-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "41 Leonis Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "70.25",
	"RA_S" : 160.85398394,
	"DEC_S" : 23.18840286,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.075,
	"key" : 28063,
	"title" : "41 Leonis Minoris"
	},
{
	"Index" : "12326",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "42 Leonis Minoris, HIP 52638, SAO 62236, HD 93152, GC 14798, HR 4203, DM BD+31  2180, TYC 2512-1146-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "42 Leonis Minoris",
	"OType" : "Star",
	"Distance" : "117.07",
	"RA_S" : 161.46623003,
	"DEC_S" : 30.68231211,
	"Constellation" : "Leo Minor ",
	"AMag" : 5.343,
	"key" : 32326,
	"title" : "42 Leonis Minoris"
	},
{
	"Index" : "12406",
	"Description" : "46 Leonis Minoris (46 LMi) is the brightest star in the constellation Leo Minor. It is sometimes known as \u0022o LMi\u0022 (not \u0022\u03BF LMi\u0022), from Bode\u0027s catalogue of 1801. It was presumably intended to be designated \u03B1, as Francis Baily decided to letter each star brighter than magnitude 4.5, but the designation was missing from his catalogue, even though the dimmer \u03B2 was included.\r\rIt has the proper name Praecipua, the Latin \u0022the Chief (Star of Leo Minor)\u0022. The name may originally have referred to 37 Leonis Minoris, and later mistransfered to this star.\r\rIt is known as \u52E2\u56DB, \u0022the Fourth (Star) of the Eunuch\u0022, in traditional Chinese astronomy.\r\r46 LMi has spectral class K0+III-IV and is of magnitude 3.83. Its distance from Earth is approximately 95 light years.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "46 Leonis Minoris, HIP 53229, SAO 62297, HD 94264, GC 14961, HR 4247, DM BD+34  2172, TYC 2521-2271-1",
	"group" : { "key" : "Leo Minor" },
	"Common" : "46 Leonis Minoris",
	"OType" : "Variable Star",
	"Distance" : "29.09",
	"RA_S" : 163.32793148,
	"DEC_S" : 34.21487888,
	"X" : 80,
	"Y" : 403,
	"Constellation" : "Leo Minor ",
	"AMag" : 3.905,
	"key" : 32406,
	"title" : "46 Leonis Minoris"
	},
{
	"Index" : "40287",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 23362, SAO 169981, HD 32309, GC 6142, HR 1621, DM BD-20  990, TYC 5908-1410-1",
	"group" : { "backgroundImage" : "images/Alignment/10.png",
		"description" : "Lepus (pron.: /\u02C8li\u02D0p\u0259s/, colloquially /\u02C8l\u025Bp\u0259s/) is a constellation lying just south of the celestial equator, immediately south of Orion. Its name is Latin for hare. Although the hare does not represent any particular figure in Greek mythology, Lepus was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. It is located below the constellation Orion (the hunter), and is sometimes represented as a hare being chased by Orion or, alternatively, by Orion\u0027s hunting dogs.\r\rThis constellation should not be confused with Lupus, the wolf.\r\rLepus is most often represented as a rabbit being hunted by Orion, whose hunting dogs (Canis Major and Canis Minor) pursue it. The constellation is also associated with some lunar mythology, including the Moon rabbit.\r\rFour stars of this constellation (\u03B1, \u03B2, \u03B3, \u03B4 Lep) form a quadrilateral and are known as \u0027Arsh al-Jawz\u0101\u0027, \u0022the Throne of Jawz\u0101\u0027\u0022 or Kursiyy al-Jawz\u0101\u0027 al-Mu\u0027akhkhar, \u0022the Hindmost Chair of Jawz\u0101\u0027\u0022 and al-Nih\u0101l, \u0022the Camels Quenching Their Thirst\u0022 in Arabic.",
		"key" : "Lepus",
		"grouptype" : "Lepus",
		"Meaning" : "hare",
		"Family" : "Orion",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Lepus",
		"title" : "Lepus Objects Group" },
	"Common" : "HR 1621",
	"OType" : "Star",
	"Distance" : "60.66",
	"RA_S" : 75.35658552,
	"DEC_S" : -20.05191858,
	"Constellation" : "Lepus ",
	"AMag" : 4.877,
	"key" : 60287,
	"title" : "HR 1621"
	},
{
	"Index" : "44682",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 23430, SAO 169997, HD 32436, GC 6160, HR 1628, DM CD-26 1975, TYC 6481-1318-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 1628",
	"OType" : "Star",
	"Distance" : "71.44",
	"RA_S" : 75.54092328,
	"DEC_S" : -26.27503082,
	"Constellation" : "Lepus ",
	"AMag" : 5.12,
	"key" : 64682,
	"title" : "HR 1628"
	},
{
	"Index" : "40312",
	"Description" : "Epsilon Leporis (\u03B5 Lep, \u03B5 Lep) is a third-magnitude star in the southern constellation Lepus. The apparent visual magnitude of +3.166 places it third in brightness among the stars in this constellation. Based upon parallax measurements, it is located at a distance of around 213 light-years (65 parsecs) from Earth.\r\rThis is an evolved giant star with a stellar classification of K4 III that has expanded to 40 times the Sun\u0027s radius. It is about 1.72 billion years old and has 1.70 times the mass of the Sun, with a luminosity 372 times as great. The outer atmosphere is cooler than the Sun\u0027s with an effective temperature of 4,131 K, giving it the orange hue of a K-type star. In terms of its composition, this star shows a similar abundance of elements other than hydrogen and helium to the Sun.\r\rThe envelope of this star is undergoing oscillations that show up as changes in the star\u0027s radial velocity. Over long durations these follow a linear trend, in combination with shorter period oscillations occurring over a few days. These oscillations are unlikely to be the result of rotational module as that would imply a high rotation rate, which would display itself through strong X-ray emissions. Instead, they may be the result of solar-like and Mira-like oscillations.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "2 Leporis, Epsilon Leporis, HIP 23685, SAO 170051, HD 32887, GC 6231, HR 1654, DM BD-22  1000, TYC 5913-1374-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Epsilon Leporis",
	"OType" : "Variable Star",
	"Distance" : "65.39",
	"RA_S" : 76.36527121,
	"DEC_S" : -22.37103582,
	"X" : 420,
	"Y" : 269,
	"Constellation" : "Lepus ",
	"AMag" : 3.334,
	"key" : 60312,
	"title" : "Epsilon Leporis"
	},
{
	"Index" : "36083",
	"Description" : "Iota Leporis (\u03B9 Lep) is a star in the constellation Lepus. Its apparent magnitude is 4.46.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "3 Leporis, Iota Leporis, HIP 24244, SAO 150223, HD 33802, GC 6374, HR 1696, DM BD-12  1095, TYC 5338-1445-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Iota Leporis",
	"OType" : "Double or multiple star",
	"Distance" : "71.06",
	"RA_S" : 78.07460084,
	"DEC_S" : -11.86920905,
	"X" : 408,
	"Y" : 130,
	"Constellation" : "Lepus ",
	"AMag" : 4.436,
	"key" : 56083,
	"title" : "Iota Leporis"
	},
{
	"Index" : "40252",
	"Description" : "Mu Leporis (\u03BC Lep, \u03BC Lep) is a star in the southern constellation of Lepus. The apparent visual magnitude is 3.259, making the star visible to the naked eye at night from the southern hemisphere. Parallax measurements yield an estimated distance of 186 light-years (57 parsecs) from the Earth.\r\rThe stellar classification of this star is B9 IV:HgMn, although the \u0027:\u0027 indicates an uncertain spectral value. The luminosity class of IV indicates that this is a subgiant that has exhausted the hydrogen at its core and it is in the process of evolving into a giant star. At present it has about 3.4 times the Sun\u0027s radius and an effective temperature of 12,800 K in its outer envelope.\r\rMu Leporis is a suspected Alpha\u00B2 Canum Venaticorum variable with a period of about two days, although this has not been confirmed. The spectrum of this star shows overabundances of mercury and manganese, as indicated by the HgMn in the stellar class. X-ray emission has been detected coming from a location at an angular separation of 0.93 arcseconds from this star. At the estimated distance of Mu Leporis, this equals a projected distance of 52 Astronomical Units. The source source may be a stellar companion: either a star that has not yet reached the main sequence or a small, low-temperature star. The X-ray luminosity of this object is (4.4 \u00B1 0.1) \u00D7 10 29 erg s\u20131.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "5 Leporis, Mu Leporis, HIP 24305, SAO 150237, HD 33904, GC 6382, HR 1702, DM BD-16  1072, TYC 5902-1721-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Mu Leporis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "56.95",
	"RA_S" : 78.23292366,
	"DEC_S" : -16.20546904,
	"X" : 403,
	"Y" : 186,
	"Constellation" : "Lepus ",
	"AMag" : 3.247,
	"key" : 60252,
	"title" : "Mu Leporis"
	},
{
	"Index" : "36086",
	"Description" : "Kappa Leporis (\u03BA Lep) is a star in the constellation Lepus. Its apparent magnitude is 4.42.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "4 Leporis, Kappa Leporis, HIP 24327B, TYC 5338-1447-2",
	"group" : { "key" : "Lepus" },
	"Common" : "Kappa Leporis",
	"OType" : "Star",
	"Distance" : "218.81",
	"RA_S" : 78.307821,
	"DEC_S" : -12.940681,
	"X" : 404,
	"Y" : 144,
	"Constellation" : "Lepus ",
	"AMag" : 6.765,
	"key" : 56086,
	"title" : "Kappa Leporis"
	},
{
	"Index" : "36085",
	"Description" : "Kappa Leporis (\u03BA Lep) is a star in the constellation Lepus. Its apparent magnitude is 4.42.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "4 Leporis, Kappa Leporis, HIP 24327A, SAO 150239, HD 33949, GC 6387, HR 1705, DM BD-13  1092, TYC 5338-1447-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Kappa Leporis",
	"OType" : "Double or multiple star",
	"Distance" : "218.81",
	"RA_S" : 78.30782339,
	"DEC_S" : -12.94129312,
	"X" : 404,
	"Y" : 144,
	"Constellation" : "Lepus ",
	"AMag" : 4.434,
	"key" : 56085,
	"title" : "Kappa Leporis"
	},
{
	"Index" : "44686",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 24505, SAO 170238, HD 34310, GC 6438, HR 1723, DM CD-27 2161, TYC 6482-1406-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 1723",
	"OType" : "Star",
	"Distance" : "85.2",
	"RA_S" : 78.85155292,
	"DEC_S" : -26.94350923,
	"Constellation" : "Lepus ",
	"AMag" : 5.042,
	"key" : 64686,
	"title" : "HR 1723"
	},
{
	"Index" : "36125",
	"Description" : "Lambda Leporis (\u03BB Lep) is a star in the constellation Lepus. Its apparent magnitude is 4.27.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "6 Leporis, Lambda Leporis, HIP 24845, SAO 150340, HD 34816, GC 6531, HR 1756, DM BD-13  1127, TYC 5343-1529-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Lambda Leporis",
	"OType" : "Star",
	"Distance" : "259.87",
	"RA_S" : 79.89385415,
	"DEC_S" : -13.17678544,
	"X" : 384,
	"Y" : 146,
	"Constellation" : "Lepus ",
	"AMag" : 4.239,
	"key" : 56125,
	"title" : "Lambda Leporis"
	},
{
	"Index" : "36100",
	"Description" : "Nu Leporis is a star in the constellation Lepus. Its apparent magnitude is 5.29.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "7 Leporis, Nu Leporis, HIP 24873, SAO 150345, HD 34863, GC 6538, HR 1757, DM BD-12  1132, TYC 5339-1784-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Nu Leporis",
	"OType" : "Star",
	"Distance" : "102.07",
	"RA_S" : 79.99593041,
	"DEC_S" : -12.3155969,
	"X" : 383,
	"Y" : 134,
	"Constellation" : "Lepus ",
	"AMag" : 5.266,
	"key" : 56100,
	"title" : "Nu Leporis"
	},
{
	"Index" : "40425",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 24927A, TYC 5927-1581-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 1762",
	"OType" : "Star",
	"Distance" : "126.91",
	"RA_S" : 80.112133,
	"DEC_S" : -21.239739,
	"Constellation" : "Lepus ",
	"AMag" : 4.723,
	"key" : 60425,
	"title" : "HR 1762"
	},
{
	"Index" : "44673",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 25045A, TYC 6479-1781-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 1771",
	"OType" : "Star in double system",
	"Distance" : "107.45",
	"RA_S" : 80.44268184,
	"DEC_S" : -24.77297825,
	"Constellation" : "Lepus ",
	"AMag" : 5.443,
	"key" : 64673,
	"title" : "HR 1771"
	},
{
	"Index" : "36139",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "8 Leporis, HIP 25202, SAO 150396, HD 35337, GC 6635, HR 1783, DM BD-14  1119, TYC 5344-1536-1",
	"group" : { "key" : "Lepus" },
	"Common" : "8 Leporis",
	"OType" : "Star",
	"Distance" : "489.7",
	"RA_S" : 80.87565849,
	"DEC_S" : -13.92735787,
	"Constellation" : "Lepus ",
	"AMag" : 5.194,
	"key" : 56139,
	"title" : "8 Leporis"
	},
{
	"Index" : "40436",
	"Description" : "Beta Leporis (Beta Lep, \u03B2 Leporis, \u03B2 Lep) is the second brightest star in the constellation of Lepus. It is also known as Nihal,\u0022quenching their thirst\u0022. The occasional spelling Nibal appears to be due to a misreading.\r\rBased on parallax measurements from the Hipparcos astrometry satellite, this star is located about 160 light-years (49 parsecs) from the Earth. It has an apparent visual magnitude of 2.84 and a stellar classification of G5 II. The mass of this star is 3.5 times the mass of the Sun and it is about 240 million years old, which is sufficient time for a star this massive to consume the hydrogen at its core and evolve away from the main sequence, becoming a G-type bright giant.\r\rThis is a double star system and may be a binary. Using adaptive optics on the AEOS telescope at Haleakala Observatory, the pair was found to be separated by an angle of 2.58 arcseconds at a position angle of 1.4\u00B0. Component B has been observed to fluctuate in brightness and is catalogued as suspected variable star NSV 2008.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "9 Leporis, Beta Leporis, HIP 25606, SAO 170457, HD 36079, GC 6762, HR 1829, DM BD-20  1096, TYC 5928-1657-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Nihal",
	"OType" : "Double or multiple star",
	"Distance" : "49.16",
	"RA_S" : 82.06134649,
	"DEC_S" : -20.75944105,
	"X" : 352,
	"Y" : 242,
	"Constellation" : "Lepus ",
	"AMag" : 2.901,
	"key" : 60436,
	"shortTitle" : "Nibal; Nikhal'",
	"title" : "Nihal"
	},
{
	"Index" : "40366",
	"Description" : "Alpha Leporis (\u03B1 Lep, \u03B1 Leporis) is the brightest star in the constellation Lepus. It has the traditional name Arneb, from the Arabic \u0623\u0631\u0646\u0628 \u0027arnab \u0022hare\u0022.\r\rThis is a massive star with about 14 times the mass of the Sun. The interferometer-measured angular diameter of this star, after correction for limb darkening, is 1.77 \u00B1 0.09 mas. At an estimated distance of 2,218 light-years (680 parsecs), this yields a physical size of about 129 times the radius of the Sun. Alpha Leporis has a stellar classification of F0 Ib, with the Ib luminosity class indicating that it is a lower luminosity supergiant star. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. The effective temperature of the outer envelope is about 6,850 K, which gives the star a yellow-white hue that is typical of F-type stars. It is an estimated 13 million years old.\r\rAlpha Leporis is an older, dying star that may have already passed through a supergiant phase and is now contracting and heating up in the latter phases of stellar evolution, or perhaps is still expanding into the supergiant phase. Based upon its estimated mass, it is expected to end its life in a spectacular stellar explosion known as a supernova.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "11 Leporis, Alpha Leporis, HIP 25985, SAO 150547, HD 36673, GC 6875, HR 1865, DM BD-17  1166, TYC 5920-1685-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Arneb",
	"OType" : "Variable Star",
	"Distance" : "672.95",
	"RA_S" : 83.18256716,
	"DEC_S" : -17.82228927,
	"X" : 339,
	"Y" : 204,
	"Constellation" : "Lepus ",
	"AMag" : 2.587,
	"key" : 60366,
	"title" : "Arneb"
	},
{
	"Index" : "40451",
	"Description" : "Gamma Leporis (\u03B3 Lep, \u03B3 Leporis) is a star that is located at a distance of about 29 light-years from Earth. Gamma Leporis lies in the south central part of the constellation Lepus, southeast of Beta Leporis and southwest of Delta Leporis. It has a common proper motion companion, AK Leporis, which is a variable star of the BY Draconis type. The star is a member of the Ursa Major Moving Group.\r\rThis star is larger than the Sun with 1.2 times the radius of the Sun and 1.3 times the Sun\u0027s mass. Based upon its stellar characteristics and distance from Earth, Gamma Leporis is considered a high-priority target for NASA\u0027s Terrestrial Planet Finder mission.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "13 Leporis, Gamma Leporis, HIP 27072, SAO 170759, HD 38393, GC 7197, HR 1983, DM BD-22  1211, TYC 5930-2197-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Gamma Leporis",
	"OType" : "High proper-motion Star",
	"Distance" : "8.93",
	"RA_S" : 86.11579539,
	"DEC_S" : -22.44838356,
	"X" : 302,
	"Y" : 263,
	"Constellation" : "Lepus ",
	"AMag" : 3.638,
	"key" : 60451,
	"title" : "Gamma Leporis"
	},
{
	"Index" : "36260",
	"Description" : "Zeta Leporis (\u03B6 Lep, \u03B6 Leporis) is a star approximately 70.5 light-years (21.6 parsecs) away in the southern constellation of Lepus. It has an apparent visual magnitude of 3.5, which is bright enough to be seen with the naked eye. In 2001, an asteroid belt was confirmed to orbit the star.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "14 Leporis, Zeta Leporis, HIP 27288, SAO 150801, HD 38678, GC 7247, HR 1998, DM BD-14  1232, TYC 5359-1778-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Zeta Leporis",
	"OType" : "Star",
	"Distance" : "21.61",
	"RA_S" : 86.73892066,
	"DEC_S" : -14.82194998,
	"X" : 295,
	"Y" : 164,
	"Constellation" : "Lepus ",
	"AMag" : 3.541,
	"key" : 56260,
	"title" : "Zeta Leporis"
	},
{
	"Index" : "40449",
	"Description" : "Delta Leporis (\u03B4 Lep) is a star in the constellation Lepus. Its apparent magnitude is 3.81.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "15 Leporis, Delta Leporis, HIP 27654, SAO 170926, HD 39364, GC 7362, HR 2035, DM BD-20  1211, TYC 5930-2195-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Delta Leporis",
	"OType" : "High proper-motion Star",
	"Distance" : "34.87",
	"RA_S" : 87.83040013,
	"DEC_S" : -20.87908925,
	"X" : 281,
	"Y" : 242,
	"Constellation" : "Lepus ",
	"AMag" : 3.879,
	"key" : 60449,
	"title" : "Delta Leporis"
	},
{
	"Index" : "36265",
	"Description" : "Eta Leporis (Eta Lep, \u03B7 Leporis, \u03B7 Lep) is a F-type main sequence star in the constellation of Lepus. It has an apparent visual magnitude of approximately 3.719. Using the IRS instrument on the Spitzer Space Telescope, excess infrared emission has been observed from the star, which can be modelled by a dust disk extending from 1 to 16 astronomical units from the star.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "16 Leporis, Eta Leporis, HIP 28103, SAO 150957, HD 40136, GC 7492, HR 2085, DM BD-14  1286, TYC 5360-1370-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Eta Leporis",
	"OType" : "Star",
	"Distance" : "14.88",
	"RA_S" : 89.10122085,
	"DEC_S" : -14.16769969,
	"X" : 265,
	"Y" : 156,
	"Constellation" : "Lepus ",
	"AMag" : 3.738,
	"key" : 56265,
	"title" : "Eta Leporis"
	},
{
	"Index" : "44788",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 28675, SAO 171180, HD 41312, GC 7680, HR 2140, DM CD-26 2675, TYC 6500-2453-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HD  41312",
	"OType" : "Double or multiple star",
	"Distance" : "124.51",
	"RA_S" : 90.81501445,
	"DEC_S" : -26.28454181,
	"Constellation" : "Lepus ",
	"AMag" : 5.188,
	"key" : 64788,
	"title" : "HD  41312"
	},
{
	"Index" : "40476",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "17 Leporis, HIP 28816, SAO 151093, HD 41511, GC 7711, HR 2148, DM BD-16  1349, TYC 5932-1539-1",
	"group" : { "key" : "Lepus" },
	"Common" : "17 Leporis",
	"OType" : "Symbiotic Star",
	"Distance" : "276.08",
	"RA_S" : 91.24636968,
	"DEC_S" : -16.48443605,
	"Constellation" : "Lepus ",
	"AMag" : 4.988,
	"key" : 60476,
	"title" : "17 Leporis"
	},
{
	"Index" : "36275",
	"Description" : "Theta Leporis (\u03B8 Lep) is a star in the constellation Lepus. Its apparent magnitude is 4.67.",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "18 Leporis, Theta Leporis, HIP 28910, SAO 151110, HD 41695, GC 7742, HR 2155, DM BD-14  1331, TYC 5361-1758-1",
	"group" : { "key" : "Lepus" },
	"Common" : "Theta Leporis",
	"OType" : "Star",
	"Distance" : "52.91",
	"RA_S" : 91.53884997,
	"DEC_S" : -14.93525379,
	"X" : 234,
	"Y" : 166,
	"Constellation" : "Lepus ",
	"AMag" : 4.669,
	"key" : 56275,
	"title" : "Theta Leporis"
	},
{
	"Index" : "44739",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 28943, SAO 171236, HD 41841, GC 7763, HR 2163, DM CD-23 3431, TYC 6492-2566-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 2163",
	"OType" : "Star",
	"Distance" : "139.88",
	"RA_S" : 91.63374185,
	"DEC_S" : -23.11084284,
	"Constellation" : "Lepus ",
	"AMag" : 5.468,
	"key" : 64739,
	"title" : "HR 2163"
	},
{
	"Index" : "40553",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "19 Leporis, HIP 29048, SAO 151142, HD 42042, GC 7794, HR 2168, DM BD-19  1361, TYC 5940-2448-1",
	"group" : { "key" : "Lepus" },
	"Common" : "19 Leporis",
	"OType" : "Variable Star",
	"Distance" : "254.87",
	"RA_S" : 91.92349422,
	"DEC_S" : -19.16586133,
	"Constellation" : "Lepus ",
	"AMag" : 5.48,
	"key" : 60553,
	"title" : "19 Leporis"
	},
{
	"Index" : "40598",
	"MapNum" : "10",
	"ImageNum" : "10",
	"Desig" : "HIP 29150, SAO 171293, HD 42301, GC 7830, HR 2180, DM BD-22 1327, TYC 5945-2604-1",
	"group" : { "key" : "Lepus" },
	"Common" : "HR 2180",
	"OType" : "Star",
	"Distance" : "75.34",
	"RA_S" : 92.241122,
	"DEC_S" : -22.42738775,
	"Constellation" : "Lepus ",
	"AMag" : 5.478,
	"key" : 60598,
	"title" : "HR 2180"
	},
{
	"Index" : "46611",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 70469, SAO 182517, HD 126218, GC 19435, HR 5390, DM CD-2411469, TYC 6736-1472-1",
	"group" : { "backgroundImage" : "images/Alignment/31.png",
		"description" : "Libra (pron.: /\u02C8li\u02D0br\u0259/) is a constellation of the zodiac. Its name is Latin for weighing scales, and its symbol is\u264E. It is fairly faint, with no first magnitude stars, and lies between Virgo to the west and Scorpius to the east.\r\rLibra was known in Babylonian astronomy as MUL Zibanu (\u0022the scales\u0022), or alternatively as the Claws of the Scorpion. The scales were held sacred to the sun god Shamash, who was also the patron of truth and justice. It was also seen as the Scorpion\u0027s Claws in ancient Greece. Since these times, Libra has been associated with law, fairness and civility. In Arabic zub\u0101n\u0101 means \u0022scorpion\u0027s claws\u0022, and likely similarly in other Semitic languages: this resemblance of words may be why the Scorpion\u0027s claws became the Scales. It has also been suggested that the scales are in allusion to the fact that when the sun entered this part of the ecliptic at the autumnal equinox, the days and nights are equal. Libra\u0027s status as the location of the equinox earned the equinox the name \u0022First Point of Libra\u0022, though its position ended in 730 because of the precession of the equinoxes.\r\rLibra is a constellation not mentioned by Eudoxus or Aratus. In Roman mythology, Libra is considered to depict the scales held by Astraea (identified as Virgo), the goddess of justice. Libra is mentioned by Manetho (3rd century B.C.) and Geminus (1st century B.C.), and included by Ptolemy in his 48 asterisms. Ptolemy catalogued 17 stars, Tycho Brahe 10, and Johannes Hevelius 20. It only became a constellation in ancient Rome, when it began to represent the scales held by Astraea, associated with Virgo.\r\rLibra is the only zodiac sign that does not symbolize a living creature.\r\rThe family of candidate habitable planets was extended in late September 2010 to include exoplanets around red dwarf stars because of Gliese 581 g, which is a tidally locked planet in the middle of the habitable zone. Weather studies show that tidally locked planets may still have the ability to support life.\r\rTraditionally, \u03B1 and \u03B2 Librae are considered to represent the scales\u0027 balance beam, and \u03B3 and \u03C3 are the weighing pans.\r\rH.A. Rey has suggested a way to connect the stars more fully to graphically show a balance. Beta Librae represents the top of the balance, Gamma Librae and Alpha Librae represent the balance beam. Upsilon Librae and Tau Librae represent the left plate of the balance, while Sigma Librae represents the right plate. All these stars are of the third magnitude.",
		"key" : "Libra",
		"grouptype" : "Libra",
		"Meaning" : "balance",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Libra",
		"title" : "Libra Objects Group" },
	"Common" : "HR 5390",
	"OType" : "Star",
	"Distance" : "140.44",
	"RA_S" : 216.20261017,
	"DEC_S" : -24.80631279,
	"Constellation" : "Libra ",
	"AMag" : 5.439,
	"key" : 66611,
	"title" : "HR 5390"
	},
{
	"Index" : "42297",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "8 Librae, Alpha01 Librae, HIP 72603, SAO 158836, HD 130819, GC 19970, HR 5530, DM BD-15  3965, TYC 6155-1209-1",
	"group" : { "key" : "Libra" },
	"Common" : "Alpha01 Librae",
	"OType" : "Spectroscopic binary",
	"Distance" : "22.98",
	"RA_S" : 222.67158737,
	"DEC_S" : -15.99723561,
	"Constellation" : "Libra ",
	"AMag" : 5.194,
	"key" : 62297,
	"title" : "Alpha01 Librae"
	},
{
	"Index" : "42298",
	"Description" : "Alpha Librae (\u03B1 Lib, \u03B1 Librae) is the Bayer designation for the second brightest star in the constellation Libra (despite its Bayer designation as alpha). It has the traditional name Zubenelgenubi (pronounced \u0022zoo-BEN-el-je-NEW-bee\u0022). The name, from Arabic \u0627\u0644\u0632\u0628\u0646 \u0627\u0644\u062C\u0646\u0648\u0628\u064A (al-zuban al-jan\u016Bbiyy), means \u0022southern claw\u0022 and was coined before Libra was recognized as distinct from Scorpius. The alternate names Kiffa Australis and Elkhiffa Australis, partial Latin translations of Arabic al-kiffah al-jan\u016Bbiyy, mean \u0022southern pan (of the scales)\u0022. Another name used in older astronomy texts, equivalent to \u0022southern scale or pan\u0022, was Lanx Australis.\r\rAlpha Librae is close to the ecliptic so it can be easily occulted by the Moon and (very rarely) by planets. The next occultation by a planet will be by Mercury on 10 November 2052.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "9 Librae, Alpha02 Librae, HIP 72622, SAO 158840, HD 130841, GC 19975, HR 5531, DM BD-15  3966, TYC 6155-1210-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zubenelgenubi",
	"OType" : "Spectroscopic binary",
	"Distance" : "23.24",
	"RA_S" : 222.71963908,
	"DEC_S" : -16.04177696,
	"X" : 413,
	"Y" : 180,
	"Constellation" : "Libra ",
	"AMag" : 2.742,
	"key" : 62298,
	"shortTitle" : "Kiffa Australis; Zubenelgenubi; Elkhiffa Australis; Zuben Ehl'genubi; Kiffa Australis; Zuben ehl' Genubi",
	"title" : "Zubenelgenubi"
	},
{
	"Index" : "33770",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "11 Librae, HIP 72631, SAO 140176, HD 130952, GC 19978, HR 5535, DM BD-01  2991, TYC 4990-776-1",
	"group" : { "key" : "Libra" },
	"Common" : "11 Librae",
	"OType" : "Star",
	"Distance" : "66.97",
	"RA_S" : 222.7544704,
	"DEC_S" : -2.2991505,
	"Constellation" : "Libra ",
	"AMag" : 5.041,
	"key" : 53770,
	"title" : "11 Librae"
	},
{
	"Index" : "46710",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "12 Librae, HIP 72929, SAO 182983, HD 131430, GC 20047, HR 5548, DM CD-24 11735, TYC 6751-1896-1",
	"group" : { "key" : "Libra" },
	"Common" : "12 Librae",
	"OType" : "Star",
	"Distance" : "127.6",
	"RA_S" : 223.58387706,
	"DEC_S" : -24.64220598,
	"Constellation" : "Libra ",
	"AMag" : 5.42,
	"key" : 66710,
	"title" : "12 Librae"
	},
{
	"Index" : "33793",
	"Description" : "16 Librae (16 Lib) is a star in the constellation Libra. Its apparent magnitude is 4.48.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "16 Librae, HIP 73165, SAO 140240, HD 132052, GC 20115, HR 5570, DM BD-03  3696, TYC 4995-951-1",
	"group" : { "key" : "Libra" },
	"Common" : "16 Librae",
	"OType" : "High proper-motion Star",
	"Distance" : "26.9",
	"RA_S" : 224.29582696,
	"DEC_S" : -4.34645575,
	"X" : 397,
	"Y" : 28,
	"Constellation" : "Libra ",
	"AMag" : 4.503,
	"key" : 53793,
	"title" : "16 Librae"
	},
{
	"Index" : "38065",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "19 Librae, Delta Librae, HIP 73473, SAO 140270, HD 132742, GC 20195, HR 5586, DM BD-07  3938, TYC 5579-1166-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zuben Elakribi",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "89.7",
	"RA_S" : 225.2431216,
	"DEC_S" : -8.51894413,
	"Constellation" : "Libra ",
	"AMag" : 4.963,
	"key" : 58065,
	"title" : "Zuben Elakribi"
	},
{
	"Index" : "46714",
	"Description" : "Sigma Librae (\u03C3 Lib, \u03C3 Librae) is a star in the constellation Libra. It has the traditional names Brachium (\u0022Arm\u0022Latin), Cornu (\u0022Horn\u0022Latin), and Zubenalgubi (\u0022Southern Claw\u0022Arabic). The apparent visual magnitude is +3.29, making it a third magnitude star that is visible to the naked eye. Based upon parallax measurements, this star is at a distance of roughly 288 light-years (88 parsecs) from Earth, with a 2% margin of error. At that distance, the visual magnitude of the star is diminished by 0.20 \u00B1 0.17 from extinction caused by intervening gas and dust.\r\rThis star was originally given the Bayer designation \u0022Gamma Scorpii\u0022 (\u03B3 Sco) despite the fact that it is well within the constellation Libra and far from the boundary with Scorpius. It did not receive its current Bayer designation as Sigma Librae until the 19th century. The new name was agreed upon by Commission 3 of the International Astronomical Union on July 31, 1930.\r\rSigma Librae has a spectral class M3/M4 III, which places it in the red giant stage of its evolution. This is a semi-regular variable star with a single pulsation period of 20 days. It shows small amplitude variations in magnitude of 0.10\u20130.15 on time scales as brief as 15\u201320 minutes, with cycles of repetition over intervals of 2.5\u20133.0 hours. This form of variability indicates that the star is on the asymptotic giant branch and is generating energy through the nuclear fusion of hydrogen and helium along concentric shells surrounding an inert core of carbon and oxygen.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "20 Librae, Sigma Librae, HIP 73714, SAO 183139, HD 133216, GC 20253, HR 5603, DM CD-24 11834, TYC 6752-1455-1",
	"group" : { "key" : "Libra" },
	"Common" : "Brachium / Cornu / Zubenalgubi",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "88.37",
	"RA_S" : 226.01756423,
	"DEC_S" : -25.28196292,
	"X" : 369,
	"Y" : 299,
	"Constellation" : "Libra ",
	"AMag" : 3.459,
	"key" : 66714,
	"shortTitle" : "Cornu; Zuben el Genubi; Zuban al Akrab; Zuben Hakrabi (also HD133774)",
	"title" : "Brachium / Cornu / Zubenalgubi"
	},
{
	"Index" : "42375",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "21 Librae, Nu Librae, HIP 73945, SAO 159028, HD 133774, GC 20311, HR 5622, DM BD-15  4026, TYC 6169-1314-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zuben Hakrabi (also HD133216)",
	"OType" : "Star",
	"Distance" : "212.37",
	"RA_S" : 226.65664984,
	"DEC_S" : -16.25681541,
	"Constellation" : "Libra ",
	"AMag" : 5.366,
	"key" : 62375,
	"title" : "Zuben Hakrabi (also HD133216)"
	},
{
	"Index" : "42426",
	"Description" : "Iota Librae (\u03B9 Lib) is a star in the constellation Libra. Its apparent magnitude is 4.54.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "24 Librae, Iota Librae, HIP 74392, SAO 159090, HD 134759, GC 20433, HR 5652, DM BD-19  4047, TYC 6178-1225-1",
	"group" : { "key" : "Libra" },
	"Common" : "Iota Librae",
	"OType" : "Spectroscopic binary",
	"Distance" : "116.3",
	"RA_S" : 228.05537606,
	"DEC_S" : -19.7917109,
	"X" : 346,
	"Y" : 228,
	"Constellation" : "Libra ",
	"AMag" : 4.529,
	"key" : 62426,
	"title" : "Iota Librae"
	},
{
	"Index" : "38100",
	"Description" : "Beta Librae (\u03B2 Lib, \u03B2 Librae) is the Bayer designation for a star in the zodiac constellation of Libra. It has the traditional name Zubeneschamali (pron.: /\u02CCzu\u02D0b\u0259n\u02CC\u025B\u0283\u0259\u02C8me\u026Ali/) and the Latin name Lanx Borealis, meaning \u0022the northern scale [of the Balance]\u0022. The name Zubeneschamali is derived from the Arabic \u0627\u0644\u0632\u0628\u0646 \u0627\u0644\u0634\u0645\u0627\u0644\u064A\u0629 (al-zuban al-\u0161am\u0101liyya) meaning \u0022The Northern Claw\u0022. The apparent visual magnitude of this star is 2.6, making it the brightest member of Libra. From parallax measurements, its distance can be estimated as 185 light-years (57 parsecs) from Earth.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "27 Librae, Beta Librae, HIP 74785, SAO 140430, HD 135742, GC 20539, HR 5685, DM BD-08  3935, TYC 5585-1014-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zubeneschamali",
	"OType" : "Variable Star",
	"Distance" : "56.75",
	"RA_S" : 229.25172425,
	"DEC_S" : -9.38291441,
	"X" : 332,
	"Y" : 92,
	"Constellation" : "Libra ",
	"AMag" : 2.568,
	"key" : 58100,
	"shortTitle" : "Kiffa Borealis; Zubeneschamali; Zuben Eschamali; Zuben el Chamali; Zubenesch; Zubenelg; Zuben Ehl'shemali; Kiffa Borealis; Zubenish",
	"title" : "Zubeneschamali"
	},
{
	"Index" : "38184",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "31 Librae, Epsilon Librae, HIP 75379, SAO 159234, HD 137052, GC 20699, HR 5723, DM BD-09  4138, TYC 5598-1052-1",
	"group" : { "key" : "Libra" },
	"Common" : "Epsilon Librae",
	"OType" : "Spectroscopic binary",
	"Distance" : "31.21",
	"RA_S" : 231.04952917,
	"DEC_S" : -10.32226004,
	"Constellation" : "Libra ",
	"AMag" : 4.972,
	"key" : 58184,
	"title" : "Epsilon Librae"
	},
{
	"Index" : "42460",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "35 Librae, Zeta Librae, HIP 76126, SAO 159335, HD 138485, GC 20887, HR 5764, DM BD-16  4110, TYC 6184-1407-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zeta Librae",
	"OType" : "Variable Star",
	"Distance" : "200.02",
	"RA_S" : 233.23009123,
	"DEC_S" : -16.8528434,
	"Constellation" : "Libra ",
	"AMag" : 5.476,
	"key" : 62460,
	"title" : "Zeta Librae"
	},
{
	"Index" : "38192",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "37 Librae, HIP 76219, SAO 140609, HD 138716, GC 20914, HR 5777, DM BD-09  4171, TYC 5599-955-1",
	"group" : { "key" : "Libra" },
	"Common" : "37 Librae",
	"OType" : "High proper-motion Star",
	"Distance" : "28.93",
	"RA_S" : 233.54459133,
	"DEC_S" : -10.06452979,
	"Constellation" : "Libra ",
	"AMag" : 4.722,
	"key" : 58192,
	"title" : "37 Librae"
	},
{
	"Index" : "38160",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 76243, SAO 140614, HD 138764, GC 20923, HR 5780, DM BD-08 4010, TYC 5595-1155-1",
	"group" : { "key" : "Libra" },
	"Common" : "HR 5780",
	"OType" : "Pulsating variable Star",
	"Distance" : "121.66",
	"RA_S" : 233.6104701,
	"DEC_S" : -9.18342084,
	"Constellation" : "Libra ",
	"AMag" : 5.127,
	"key" : 58160,
	"title" : "HR 5780"
	},
{
	"Index" : "46844",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "36 Librae, HIP 76259, SAO 183580, HD 138688, GC 20918, HR 5775, DM CD-27 10443, TYC 6772-1895-1",
	"group" : { "key" : "Libra" },
	"Common" : "36 Librae",
	"OType" : "Star",
	"Distance" : "96.25",
	"RA_S" : 233.65548772,
	"DEC_S" : -28.04699619,
	"Constellation" : "Libra ",
	"AMag" : 5.285,
	"key" : 66844,
	"title" : "36 Librae"
	},
{
	"Index" : "38227",
	"Description" : "Gamma Librae (\u03B3 Lib, \u03B3 Librae) is a star in the constellation Libra. It has the traditional name Zuben-el-Akrab, meaning \u0022Shears of the Scorpion\u0022. The name is a modification of the Arabic al-Zuban al-Aqrab (\u0627\u0644\u0632\u0628\u0646 \u0627\u0644\u0639\u0642\u0631\u0628). Alternate modifications of the phrase include Zuben el Hakrabi and Zuben Hakraki.\r\rGamma Librae belongs to the spectral class K0III, and is of the fourth-magnitude, having apparent magnitude +3.91. It is approximately 152 light years from the Earth. This star has 2.15 times the mass of the Sun and is radiating around 71 times the luminosity of the Sun at an effective temperature of 4,822 K.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "38 Librae, Gamma Librae, HIP 76333, SAO 159370, HD 138905, GC 20949, HR 5787, DM BD-14  4237, TYC 5608-1381-1",
	"group" : { "key" : "Libra" },
	"Common" : "Zuben-el-Akrab",
	"OType" : "Double or multiple star",
	"Distance" : "50.02",
	"RA_S" : 233.88157836,
	"DEC_S" : -14.78953551,
	"X" : 273,
	"Y" : 163,
	"Constellation" : "Libra ",
	"AMag" : 4.015,
	"key" : 58227,
	"shortTitle" : "Zuben Hakraki; Zuben el Hakrabi",
	"title" : "Zuben-el-Akrab"
	},
{
	"Index" : "46858",
	"Description" : "Upsilon Librae (\u03C5 Lib, \u03C5 Librae) is a Class K3, fourth-magnitude star in the constellation Libra. Upsilon Librae is a double or multiple stellar system located about 195 light-years from Earth.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "39 Librae, Upsilon Librae, HIP 76470, SAO 183619, HD 139063, GC 20979, HR 5794, DM CD-27 10464, TYC 6776-1590-1",
	"group" : { "key" : "Libra" },
	"Common" : "Upsilon Librae",
	"OType" : "Star",
	"Distance" : "68.57",
	"RA_S" : 234.25604314,
	"DEC_S" : -28.13507606,
	"X" : 273,
	"Y" : 337,
	"Constellation" : "Libra ",
	"AMag" : 3.75,
	"key" : 66858,
	"title" : "Upsilon Librae"
	},
{
	"Index" : "46964",
	"Description" : "Tau Librae (\u03C4 Lib, \u03C4 Librae) is a Class B2.5, fourth-magnitude star in the constellation Libra. Tau Librae is a stellar system located about 445 light-years from Earth. This star has 3.2 times the radius of the Sun and its outer atmosphere has an effective temperature of 20,911 K.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "40 Librae, Tau Librae, HIP 76600, SAO 183649, HD 139365, GC 21019, HR 5812, DM CD-29 11837, TYC 6789-1800-1",
	"group" : { "key" : "Libra" },
	"Common" : "Tau Librae",
	"OType" : "Spectroscopic binary",
	"Distance" : "112.42",
	"RA_S" : 234.66403957,
	"DEC_S" : -29.77774878,
	"X" : 269,
	"Y" : 358,
	"Constellation" : "Libra ",
	"AMag" : 3.616,
	"key" : 66964,
	"title" : "Tau Librae"
	},
{
	"Index" : "42508",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "41 Librae, HIP 76628AB, SAO 159411, HD 139446, GC 21031, HR 5814, DM BD-18  4118, TYC 6193-766-1",
	"group" : { "key" : "Libra" },
	"Common" : "41 Librae",
	"OType" : "Variable Star",
	"Distance" : "94.71",
	"RA_S" : 234.72733712,
	"DEC_S" : -19.30189584,
	"Constellation" : "Libra ",
	"AMag" : 5.456,
	"key" : 62508,
	"title" : "41 Librae"
	},
{
	"Index" : "46872",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "42 Librae, HIP 76742, SAO 183686, HD 139663, GC 21057, HR 5824, DM CD-23 12458, TYC 6777-1627-1",
	"group" : { "key" : "Libra" },
	"Common" : "42 Librae",
	"OType" : "Star",
	"Distance" : "117.04",
	"RA_S" : 235.07039849,
	"DEC_S" : -23.81808486,
	"Constellation" : "Libra ",
	"AMag" : 5.103,
	"key" : 66872,
	"title" : "42 Librae"
	},
{
	"Index" : "42507",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "43 Librae, Kappa Librae, HIP 76880, SAO 159442, HD 139997, GC 21094, HR 5838, DM BD-19  4188, TYC 6193-631-1",
	"group" : { "key" : "Libra" },
	"Common" : "Kappa Librae",
	"OType" : "Variable Star",
	"Distance" : "118.98",
	"RA_S" : 235.48664874,
	"DEC_S" : -19.67882583,
	"Constellation" : "Libra ",
	"AMag" : 4.924,
	"key" : 62507,
	"title" : "Kappa Librae"
	},
{
	"Index" : "42468",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "44 Librae, Eta Librae, HIP 77060, SAO 159466, HD 140417, GC 21146, HR 5848, DM BD-15  4171, TYC 6186-1662-1",
	"group" : { "key" : "Libra" },
	"Common" : "Eta Librae",
	"OType" : "Star",
	"Distance" : "45.74",
	"RA_S" : 236.01833092,
	"DEC_S" : -15.67283385,
	"Constellation" : "Libra ",
	"AMag" : 5.44,
	"key" : 62468,
	"title" : "Eta Librae"
	},
{
	"Index" : "42518",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "45 Librae, Lambda Librae, HIP 77811, SAO 183895, HD 142096, GC 21327, HR 5902, DM BD-19  4249, TYC 6195-1763-1",
	"group" : { "key" : "Libra" },
	"Common" : "Lambda Librae",
	"OType" : "Spectroscopic binary",
	"Distance" : "111.57",
	"RA_S" : 238.33356098,
	"DEC_S" : -20.16706048,
	"Constellation" : "Libra ",
	"AMag" : 5.022,
	"key" : 62518,
	"title" : "Lambda Librae"
	},
{
	"Index" : "42476",
	"Description" : "Theta Librae is a giant star in the southern zodiac constellation of Libra. It is located about 163 light-years (50 parsecs) from the Earth and has an estimated mass about 84% greater than the Sun. This star is radiating about 35 times the luminosity of the Sun from its outer atmosphere at an effective temperature of about 4,700 K.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "46 Librae, Theta Librae, HIP 77853, SAO 159563, HD 142198, GC 21342, HR 5908, DM BD-16  4174, TYC 6187-1544-1",
	"group" : { "key" : "Libra" },
	"Common" : "Theta Librae",
	"OType" : "Star",
	"Distance" : "51.65",
	"RA_S" : 238.45641011,
	"DEC_S" : -16.72929324,
	"X" : 217,
	"Y" : 190,
	"Constellation" : "Libra ",
	"AMag" : 4.24,
	"key" : 62476,
	"title" : "Theta Librae"
	},
{
	"Index" : "38308",
	"Description" : "48 Librae (48 Lib) is a star in the constellation Libra. Its apparent magnitude is 4.94.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "48 Librae, HIP 78207, SAO 159607, HD 142983, GC 21439, HR 5941, DM BD-13  4302, TYC 5623-1368-1",
	"group" : { "key" : "Libra" },
	"Common" : "48 Librae",
	"OType" : "Be Star",
	"Distance" : "143.27",
	"RA_S" : 239.54737295,
	"DEC_S" : -14.2793582,
	"X" : 202,
	"Y" : 158,
	"Constellation" : "Libra ",
	"AMag" : 4.927,
	"key" : 58308,
	"title" : "48 Librae"
	},
{
	"Index" : "59880",
	"Description" : "Iota Lupi (\u03B9 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.54.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Iota Lupi, HIP 69996, SAO 224833, HD 125238, GC 19304, HR 5354, DM CD-45  9084, TYC 8277-3277-1",
	"group" : { "backgroundImage" : "images/Alignment/31.png",
		"description" : "Lupus (pron.: /\u02C8lju\u02D0p\u0259s/) is a constellation in the southern sky. Its name is Latin for wolf. Lupus was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. It lies between Centaurus and Scorpius.\r\rIn ancient times, the constellation was considered an asterism within Centaurus, and was considered to have been an arbitrary animal, killed, or about to be killed, on behalf of, or for, Centaurus. It was not separated from Centaurus until Hipparchus of Bithynia named it Therion (meaning beast) in the 200s BCE. No particular animal was associated with it until the Latin translation of Ptolemy\u0027s work identified it with the wolf.\r\rThe Greek constellation is probably based on the Babylonian figure known as the Mad Dog (UR.IDIM). This was a strange hybrid creature that combined the head and torso of a man with the legs and tail of a lion (the cuneiform sign \u0027UR\u0027 simply refers to a large carnivore; lions, wolves and dogs are all included). It is often found in association with the sun god and another mythical being called the Bison-man, which is supposedly related to the Greek constellation of Centaurus.",
		"key" : "Lupus",
		"grouptype" : "Lupus",
		"Meaning" : "wolf",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Lupus",
		"title" : "Lupus Objects Group" },
	"Common" : "Iota Lupi",
	"OType" : "Variable Star",
	"Distance" : "103.57",
	"RA_S" : 214.85091498,
	"DEC_S" : -46.05809697,
	"X" : 465,
	"Y" : 577,
	"Constellation" : "Lupus ",
	"AMag" : 3.5,
	"key" : 79880,
	"title" : "Iota Lupi"
	},
{
	"Index" : "59879",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 70104, SAO 224843, HD 125442, GC 19336, HR 5364, DM CD-44 9236, TYC 8277-3276-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5364",
	"OType" : "Star",
	"Distance" : "43.54",
	"RA_S" : 215.17741909,
	"DEC_S" : -45.18706343,
	"Constellation" : "Lupus ",
	"AMag" : 4.807,
	"key" : 79879,
	"title" : "HR 5364"
	},
{
	"Index" : "59883",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Tau01 Lupi, HIP 70574, SAO 224919, HD 126341, GC 19453, HR 5395, DM CD-44  9322, TYC 8277-3280-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Tau01 Lupi",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "332.48",
	"RA_S" : 216.53425743,
	"DEC_S" : -45.22142437,
	"Constellation" : "Lupus ",
	"AMag" : 4.527,
	"key" : 79883,
	"title" : "Tau01 Lupi"
	},
{
	"Index" : "59884",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Tau02 Lupi, HIP 70576AB, SAO 224920, HD 126354, GC 19454, HR 5396, DM CD-44  9323, TYC 8277-3281-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Tau02 Lupi",
	"OType" : "Double or multiple star",
	"Distance" : "97.74",
	"RA_S" : 216.54505012,
	"DEC_S" : -45.37926984,
	"Constellation" : "Lupus ",
	"AMag" : 4.401,
	"key" : 79884,
	"title" : "Tau02 Lupi"
	},
{
	"Index" : "59889",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 70915, SAO 224969, HD 126981, GC 19533, HR 5412, DM CD-44 9383, TYC 8278-3072-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5412",
	"OType" : "Star",
	"Distance" : "145.57",
	"RA_S" : 217.53595213,
	"DEC_S" : -45.32135967,
	"Constellation" : "Lupus ",
	"AMag" : 5.487,
	"key" : 79889,
	"title" : "HR 5412"
	},
{
	"Index" : "59970",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 70931, SAO 224972, HD 126983, GC 19539, HR 5413, DM CD-48 9098, TYC 8286-1678-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5413",
	"OType" : "Spectroscopic binary",
	"Distance" : "62.2",
	"RA_S" : 217.58729284,
	"DEC_S" : -49.51902628,
	"Constellation" : "Lupus ",
	"AMag" : 5.382,
	"key" : 79970,
	"title" : "HR 5413"
	},
{
	"Index" : "59971",
	"Description" : "Sigma Lupi (\u03C3 Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.42.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Sigma Lupi, HIP 71121, SAO 241781, HD 127381, GC 19590, HR 5425, DM CD-49  8831, TYC 8286-1831-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Sigma Lupi",
	"OType" : "Ellipsoidal variable Star",
	"Distance" : "176.13",
	"RA_S" : 218.15440271,
	"DEC_S" : -50.45716322,
	"X" : 427,
	"Y" : 631,
	"Constellation" : "Lupus ",
	"AMag" : 4.392,
	"key" : 79971,
	"title" : "Sigma Lupi"
	},
{
	"Index" : "59980",
	"Description" : "Rho Lupi (\u03C1 Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.03.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Rho Lupi, HIP 71536, SAO 225071, HD 128345, GC 19698, HR 5453, DM CD-48  9198, TYC 8287-2475-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Rho Lupi",
	"OType" : "Variable Star",
	"Distance" : "96.87",
	"RA_S" : 219.47177815,
	"DEC_S" : -49.4258314,
	"X" : 417,
	"Y" : 617,
	"Constellation" : "Lupus ",
	"AMag" : 4.007,
	"key" : 79980,
	"title" : "Rho Lupi"
	},
{
	"Index" : "60004",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "b Lupi, HIP 72290, SAO 241992, HD 129893, GC 19876, HR 5495, DM CD-51  8457, TYC 8291-2249-1",
	"group" : { "key" : "Lupus" },
	"Common" : "b Lupi",
	"OType" : "Star",
	"Distance" : "79.64",
	"RA_S" : 221.75539465,
	"DEC_S" : -52.38351631,
	"Constellation" : "Lupus ",
	"AMag" : 5.331,
	"key" : 80004,
	"title" : "b Lupi"
	},
{
	"Index" : "55725",
	"Description" : "Omicron Lupi (\u03BF Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.31.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Omicron Lupi, HIP 72683AS, SAO 225248, HD 130807, GC 19977, HR 5528, DM CD-43  9391, TYC 7832-2492-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Omicron Lupi",
	"OType" : "Star",
	"Distance" : "123.13",
	"RA_S" : 222.90958987,
	"DEC_S" : -43.57535769,
	"X" : 392,
	"Y" : 538,
	"Constellation" : "Lupus ",
	"AMag" : 4.289,
	"key" : 75725,
	"title" : "Omicron Lupi"
	},
{
	"Index" : "63945",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "c Lupi, HIP 73095, SAO 242120, HD 131562, GC 20068, HR 5556, DM CP-52  7634, TYC 8681-3328-1",
	"group" : { "key" : "Lupus" },
	"Common" : "c Lupi",
	"OType" : "Star",
	"Distance" : "61.47",
	"RA_S" : 224.07188631,
	"DEC_S" : -52.8095511,
	"Constellation" : "Lupus ",
	"AMag" : 5.403,
	"key" : 83945,
	"title" : "c Lupi"
	},
{
	"Index" : "55723",
	"Description" : "Beta Lupi (\u03B2 Lupi, \u03B2 Lup) is a star in the southern constellation of Lupus. It has an apparent visual magnitude of 2.7, making it readily visible to the naked eye. Based upon parallax measurements, this star is located at a distance of about 383 light-years (117 parsecs) from Earth. The stellar classification of B2 III indicates this is a giant star. The effective temperature of the star\u0027s outer envelope is 24,090 K, giving it the blue-white hue of a B-type star. With an age of around 25 million years, it is near the end of its hydrogen phase, where hydrogen is fused into the element helium, and transferring into a red supergiant star. At about 8.8 solar masses, it may have enough mass to end its life as a Type II supernova, but there is the possibility of Beta Lupi becoming a white dwarf.\r\rThis is a multi-period Beta Cephei variable with a dominant oscillation period of 0.232 days. It is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. Beta Lupi has a high proper motion of more than 50 mas per year, suggesting a significant transverse velocity.\r\rIt lies close to the supernova remnant SN 1006. In Chinese, \u9A0E\u5B98 (Q\u00ED Gu\u0101n), meaning Imperial Guards, refers to an asterism consisting of \u03B2 Lupi, \u03B3 Lupi, \u03B4 Lupi, \u03BA Centauri, \u03BB Lupi, \u03B5 Lupi, \u03BC Lup, \u03C0 Lupi, \u03BF Lupi and \u03B1 Lupi. Consequently, \u03B2 Lupi itself is known as \u9A0E\u5B98\u56DB (Q\u00ED Gu\u0101n s\u00EC, English: the Fourth Star of Imperial Guards.). From this Chinese name, the name Ke Kwan was appeared.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Beta Lupi, HIP 73273, SAO 225335, HD 132058, GC 20128, HR 5571, DM CD-42  9853, TYC 7832-2490-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Beta Lupi",
	"OType" : "Variable Star",
	"Distance" : "117.31",
	"RA_S" : 224.63302487,
	"DEC_S" : -43.13396021,
	"X" : 375,
	"Y" : 532,
	"Constellation" : "Lupus ",
	"AMag" : 2.603,
	"key" : 75723,
	"title" : "Beta Lupi"
	},
{
	"Index" : "51208",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 73624, SAO 206239, HD 132955, GC 20225, HR 5595, DM CD-3210560, TYC 7315-2056-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5595",
	"OType" : "Star",
	"Distance" : "118.77",
	"RA_S" : 225.74698681,
	"DEC_S" : -32.64329244,
	"Constellation" : "Lupus ",
	"AMag" : 5.418,
	"key" : 71208,
	"title" : "HR 5595"
	},
{
	"Index" : "60056",
	"Description" : "\u03C0 Lupi is a star in a double system.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Pi Lupi, HIP 73807B, SAO 225426, HD 133242, GC 20271, HR 5605, DM CD-46  9773A, TYC 8297-4705-2",
	"group" : { "key" : "Lupus" },
	"Common" : "Pi Lupi",
	"OType" : "Double or multiple star",
	"Distance" : "134.97",
	"RA_S" : 226.27982833,
	"DEC_S" : -47.05118067,
	"X" : 357,
	"Y" : 583,
	"Constellation" : "Lupus ",
	"AMag" : 4.598,
	"key" : 80056,
	"title" : "Pi Lupi"
	},
{
	"Index" : "60055",
	"Description" : "\u03C0 Lupi is a star in a double system.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Pi Lupi, HIP 73807A, SAO 225426, HD 133242, GC 20271, HR 5605, DM CD-46  9773A, TYC 8297-4705-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Pi Lupi",
	"OType" : "Double or multiple star",
	"Distance" : "134.97",
	"RA_S" : 226.27982833,
	"DEC_S" : -47.05118067,
	"X" : 357,
	"Y" : 583,
	"Constellation" : "Lupus ",
	"AMag" : 4.561,
	"key" : 80055,
	"title" : "Pi Lupi"
	},
{
	"Index" : "55668",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 73826, SAO 225435, HD 133340, GC 20278, HR 5607, DM CD-40 9257, TYC 7825-2663-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5607",
	"OType" : "Star",
	"Distance" : "108.06",
	"RA_S" : 226.32986012,
	"DEC_S" : -41.06723543,
	"Constellation" : "Lupus ",
	"AMag" : 5.239,
	"key" : 75668,
	"title" : "HR 5607"
	},
{
	"Index" : "60023",
	"Description" : "Lambda Lupi (\u03BB Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.07.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Lambda Lupi, HIP 74117AB, SAO 225483, HD 133955, GC 20356, HR 5626, DM CD-44  9889, TYC 8293-3877-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Lambda Lupi",
	"OType" : "Spectroscopic binary",
	"Distance" : "231.24",
	"RA_S" : 227.21091634,
	"DEC_S" : -45.27984571,
	"X" : 349,
	"Y" : 560,
	"Constellation" : "Lupus ",
	"AMag" : 4.021,
	"key" : 80023,
	"title" : "Lambda Lupi"
	},
{
	"Index" : "60070",
	"Description" : "Kappa1 Lupi (\u03BA1 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.85.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Kappa01 Lupi, HIP 74376A, SAO 225525, HD 134481, GC 20409, HR 5646, DM CD-48  9704, TYC 8298-4184-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Kappa Lupi",
	"OType" : "Be Star",
	"Distance" : "55.14",
	"RA_S" : 227.98364019,
	"DEC_S" : -48.73782139,
	"X" : 340,
	"Y" : 604,
	"Constellation" : "Lupus ",
	"AMag" : 3.833,
	"key" : 80070,
	"title" : "Kappa Lupi"
	},
{
	"Index" : "60142",
	"Description" : "Zeta Lupi (\u03B6 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.41.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Zeta Lupi, HIP 74395, SAO 242304, HD 134505, GC 20418, HR 5649, DM CD-51  8830, TYC 8306-3362-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Zeta Lupi",
	"OType" : "Star",
	"Distance" : "35.97",
	"RA_S" : 228.07123478,
	"DEC_S" : -52.09924858,
	"X" : 339,
	"Y" : 647,
	"Constellation" : "Lupus ",
	"AMag" : 3.5,
	"key" : 80142,
	"title" : "Zeta Lupi"
	},
{
	"Index" : "55750",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "e Lupi, HIP 74449, SAO 225539, HD 134687, GC 20435, HR 5651, DM CD-44  9932, TYC 7834-3136-1",
	"group" : { "key" : "Lupus" },
	"Common" : "e Lupi",
	"OType" : "Spectroscopic binary",
	"Distance" : "154.36",
	"RA_S" : 228.20662296,
	"DEC_S" : -44.50041892,
	"Constellation" : "Lupus ",
	"AMag" : 4.778,
	"key" : 75750,
	"title" : "e Lupi"
	},
{
	"Index" : "51197",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "1 Lupi, i Lupi, HIP 74604, SAO 206445, HD 135153, GC 20480, HR 5660, DM CD-31 11813, TYC 7312-1422-1",
	"group" : { "key" : "Lupus" },
	"Common" : "i Lupi",
	"OType" : "Star",
	"Distance" : "586.59",
	"RA_S" : 228.65549813,
	"DEC_S" : -31.51912559,
	"Constellation" : "Lupus ",
	"AMag" : 4.961,
	"key" : 71197,
	"title" : "i Lupi"
	},
{
	"Index" : "55709",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 74707AB, SAO 225600, HD 135345, GC 20503, HR 5667, DM CD-41 9682, TYC 7830-3399-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5667",
	"OType" : "Star",
	"Distance" : "540.5405",
	"RA_S" : 229.01677814,
	"DEC_S" : -41.49114915,
	"Constellation" : "Lupus ",
	"AMag" : 5.236,
	"key" : 75709,
	"title" : "HR 5667"
	},
{
	"Index" : "51196",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "2 Lupi, f Lupi, HIP 74857, SAO 183346, HD 135758, GC 20550, HR 5686, DM CD-29 11630, TYC 7312-1421-1",
	"group" : { "key" : "Lupus" },
	"Common" : "f Lupi",
	"OType" : "Variable Star",
	"Distance" : "99.85",
	"RA_S" : 229.45765861,
	"DEC_S" : -30.14867667,
	"Constellation" : "Lupus ",
	"AMag" : 4.47,
	"key" : 71196,
	"title" : "f Lupi"
	},
{
	"Index" : "60068",
	"Description" : "Mu Lupi (\u03BC Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.27.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Mu Lupi, HIP 74911A, SAO 225638, HD 135734, GC 20556, HR 5683, DM CD-47  9860, TYC 8298-4182-2",
	"group" : { "key" : "Lupus" },
	"Common" : "Mu Lupi",
	"OType" : "Star",
	"Distance" : "102.23",
	"RA_S" : 229.63329247,
	"DEC_S" : -47.87519956,
	"X" : 326,
	"Y" : 593,
	"Constellation" : "Lupus ",
	"AMag" : 4.994,
	"key" : 80068,
	"title" : "Mu Lupi"
	},
{
	"Index" : "60067",
	"Description" : "Mu Lupi (\u03BC Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.27.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Mu Lupi, HIP 74911B, SAO 225638, HD 135734, GC 20556, HR 5683, DM CD-47  9860, TYC 8298-4182-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Mu Lupi",
	"OType" : "Star",
	"Distance" : "102.23",
	"RA_S" : 229.63329247,
	"DEC_S" : -47.87519956,
	"X" : 326,
	"Y" : 593,
	"Constellation" : "Lupus ",
	"AMag" : 4.928,
	"key" : 80067,
	"title" : "Mu Lupi"
	},
{
	"Index" : "55794",
	"Description" : "Delta Lupi (\u03B4 Lupi, \u03B4 Lup) is a star in the southern circumpolar constellation of Lupus. It is \u9A0E\u5B98\u4E8C, \u0022the 2nd (star) of the Cavalry Officer\u0022, in traditional Chinese astronomy. With an apparent visual magnitude of 3.22, it is the fourth brightest star in the constellation. The distance to this star has been measured using the parallax technique, yielding an estimate of roughly 900 light years with a 15% margin of error.\r\rThe spectrum of this star matches a stellar classification of B1.5 IV, which indicates this star has entered the subgiant stage and is in the process of evolving into a giant star. It is radiating around 10,000 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 23,000 K, giving it a blue-white hue. This star has nearly 12 times the mass of the Sun and is roughly 15 million years old.\r\rDelta Lupi is a Beta Cephei variable star that undergoes periodic pulsations. It has a single period of variability lasting 0.1655 days, or six cycles per day. This is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Delta Lupi, HIP 75141, SAO 225691, HD 136298, GC 20620, HR 5695, DM CD-40  9538, TYC 7839-2803-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Delta Lupi",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "264.21",
	"RA_S" : 230.34302291,
	"DEC_S" : -40.6475107,
	"X" : 319,
	"Y" : 499,
	"Constellation" : "Lupus ",
	"AMag" : 3.157,
	"key" : 75794,
	"title" : "Delta Lupi"
	},
{
	"Index" : "51270",
	"Description" : "Phi1 Lupi (\u03C61 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.58.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Phi01 Lupi, HIP 75177, SAO 206552, HD 136422, GC 20643, HR 5705, DM CD-35 10236, TYC 7325-1691-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Phi1 Lupi",
	"OType" : "Star",
	"Distance" : "84.3",
	"RA_S" : 230.45154242,
	"DEC_S" : -36.26137509,
	"X" : 317,
	"Y" : 441,
	"Constellation" : "Lupus ",
	"AMag" : 3.729,
	"key" : 71270,
	"title" : "Phi1 Lupi"
	},
{
	"Index" : "60073",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Nu01 Lupi, HIP 75206, SAO 225703, HD 136351, GC 20644, HR 5698, DM CD-47  9922, TYC 8298-907-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Nu01 Lupi",
	"OType" : "High proper-motion Star",
	"Distance" : "35.85",
	"RA_S" : 230.53446009,
	"DEC_S" : -47.92779162,
	"Constellation" : "Lupus ",
	"AMag" : 5.048,
	"key" : 80073,
	"title" : "Nu01 Lupi"
	},
{
	"Index" : "55874",
	"Description" : "Epsilon Lupi (\u03B5 Lup) is a multiple star system in the southern constellation of Lupus. At an apparent visual magnitude of 3.41, Epsilon Lupi can be readily viewed from the southern hemisphere with sufficiently dark skies. It is the fifth brightest star or star system in the constellation. Parallax measurements give a distance to this system of roughly 510 light-years (160 parsecs).\r\rThis system is what astronomers term a double-lined spectroscopic binary. When the spectrum is examined, the absorption line features of both stars can be viewed. As a result of the Doppler effect, these lines shift back and forth in frequency as the two stars orbit around each other. This allows some of their orbital elements to be deduced, even though the individual stars have not been resolved with a telescope. The pair share a close, elliptical orbit with a period of 4.55970 days. The orbital eccentricity is 0.277, which means that at the separation at closest approach, or periapsis, is only 57% of the distance at their greatest separation, or apoapsis. There is a third, more distant companion at an angular separation of 26.5 arcseconds that may be orbiting the pair with a period of about 64 years.\r\rThe pair that share the close orbit, Epsilon Lupi A and Epsilon Lupi a, have estimated masses of 13.24 and 11.46 times the mass of the Sun, respectively. The more distant component, Epsilon Lupi B, has a mass of about 7.64 times the Sun. The combined stellar classification of the system is B2 IV-V, while the individual components may have spectral classes of B3 IV, B3 V, and A5 V, in order of decreasing mass. The inner A-a pair appear to have their rate of spin synchronized with their orbit, so that the same face of each star always faces its partner. The secondary, Epsilon Lupi a, shows regular variation in luminosity of the type that occurs with Beta Cephei variables, at a periodicity of 10.36 cycles per day.\r\rThis star system is a probable member of the Scorpius-Centaurus Association, a moving group of stars that originated together and share a similar trajectory through space.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Epsilon Lupi, HIP 75264AB, SAO 225712, HD 136504, GC 20659, HR 5708, DM CD-44 10066, TYC 7847-2505-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Epsilon Lupi",
	"OType" : "Spectroscopic binary",
	"Distance" : "152.93",
	"RA_S" : 230.67030565,
	"DEC_S" : -44.68962812,
	"X" : 315,
	"Y" : 551,
	"Constellation" : "Lupus ",
	"AMag" : 3.337,
	"key" : 75874,
	"title" : "Epsilon Lupi"
	},
{
	"Index" : "51271",
	"Description" : "Phi2 Lupi (\u03C62 Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.52.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Phi02 Lupi, HIP 75304, SAO 206580, HD 136664, GC 20676, HR 5712, DM CD-36 10103, TYC 7325-1692-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Phi2 Lupi",
	"OType" : "Star",
	"Distance" : "159.08",
	"RA_S" : 230.78896097,
	"DEC_S" : -36.85849088,
	"X" : 314,
	"Y" : 450,
	"Constellation" : "Lupus ",
	"AMag" : 4.499,
	"key" : 71271,
	"title" : "Phi2 Lupi"
	},
{
	"Index" : "55793",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Upsilon Lupi, HIP 75439, SAO 206597, HD 136933, GC 20698, HR 5719, DM CD-39  9827, TYC 7839-2802-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Upsilon Lupi",
	"OType" : "Star",
	"Distance" : "123.8",
	"RA_S" : 231.18753123,
	"DEC_S" : -39.71025508,
	"Constellation" : "Lupus ",
	"AMag" : 5.351,
	"key" : 75793,
	"title" : "Upsilon Lupi"
	},
{
	"Index" : "55758",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "k Lupi, HIP 75501, SAO 206616, HD 137058, GC 20714, HR 5724, DM CD-38 10289, TYC 7835-2634-1",
	"group" : { "key" : "Lupus" },
	"Common" : "k Lupi",
	"OType" : "Star",
	"Distance" : "117.81",
	"RA_S" : 231.33423626,
	"DEC_S" : -38.73362687,
	"Constellation" : "Lupus ",
	"AMag" : 4.592,
	"key" : 75758,
	"title" : "k Lupi"
	},
{
	"Index" : "51281",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 75647, SAO 206660, HD 137432, GC 20756, HR 5736, DM CD-3610161, TYC 7326-922-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5736",
	"OType" : "Spectroscopic binary",
	"Distance" : "130.89",
	"RA_S" : 231.82554154,
	"DEC_S" : -36.76756325,
	"Constellation" : "Lupus ",
	"AMag" : 5.416,
	"key" : 71281,
	"title" : "HR 5736"
	},
{
	"Index" : "60040",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 75828, SAO 225825, HD 137709, GC 20799, HR 5742, DM CD-4610100, TYC 8295-181-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5742",
	"OType" : "Star",
	"Distance" : "330.99",
	"RA_S" : 232.35112423,
	"DEC_S" : -46.73270438,
	"Constellation" : "Lupus ",
	"AMag" : 5.441,
	"key" : 80040,
	"title" : "HR 5742"
	},
{
	"Index" : "55805",
	"Description" : "Gamma Lupi (\u03B3 Lupi, \u03B3 Lup) is a 3rd-magnitude, B-type blue giant star in the constellation of Lupus. It is also known in ancient Chinese astronomy as \u9A0E\u5B98\u4E00 or \u0022the 1st (star) of the Cavalry Officer\u0022. With a telescope, Gamma Lupi can be resolved into a binary star system in close orbit. This is known as the Gamma Lupi AB system, often abbreviated as \u03B3 Lupi AB or \u03B3 Lup AB. Gamma Lupi A is itself a spectroscopic binary with a period of 2.8081 days.\r\rThis star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Gamma Lupi, HIP 76297B, SAO 225938, HD 138690B, GC 20926, HR 5776, DM CD-40  9760, TYC 7840-1432-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Gamma Lupi",
	"OType" : "Star",
	"Distance" : "128.39",
	"RA_S" : 233.78503305,
	"DEC_S" : -41.16678306,
	"X" : 284,
	"Y" : 506,
	"Constellation" : "Lupus ",
	"AMag" : 2.954,
	"key" : 75805,
	"title" : "Gamma Lupi"
	},
{
	"Index" : "55806",
	"Description" : "Gamma Lupi (\u03B3 Lupi, \u03B3 Lup) is a 3rd-magnitude, B-type blue giant star in the constellation of Lupus. It is also known in ancient Chinese astronomy as \u9A0E\u5B98\u4E00 or \u0022the 1st (star) of the Cavalry Officer\u0022. With a telescope, Gamma Lupi can be resolved into a binary star system in close orbit. This is known as the Gamma Lupi AB system, often abbreviated as \u03B3 Lupi AB or \u03B3 Lup AB. Gamma Lupi A is itself a spectroscopic binary with a period of 2.8081 days.\r\rThis star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Gamma Lupi, HIP 76297A, SAO 225938, HD 138690A, GC 20926, HR 5776, DM CD-40  9760, TYC 7840-1432-2",
	"group" : { "key" : "Lupus" },
	"Common" : "Gamma Lupi",
	"OType" : "Star",
	"Distance" : "128.39",
	"RA_S" : 233.78503305,
	"DEC_S" : -41.16678306,
	"X" : 284,
	"Y" : 506,
	"Constellation" : "Lupus ",
	"AMag" : 4.451,
	"key" : 75806,
	"title" : "Gamma Lupi"
	},
{
	"Index" : "55890",
	"Description" : "KT Lupi (KT Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.54.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 76371B, TYC 7848-2378-2",
	"group" : { "key" : "Lupus" },
	"Common" : "KT Lupi",
	"OType" : "Be Star",
	"Distance" : "130.73",
	"RA_S" : 233.97187331,
	"DEC_S" : -44.9583459,
	"X" : 284,
	"Y" : 555,
	"Constellation" : "Lupus ",
	"AMag" : 6.509,
	"key" : 75890,
	"title" : "KT Lupi"
	},
{
	"Index" : "55889",
	"Description" : "KT Lupi (KT Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.54.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "d Lupi, HIP 76371A, SAO 225950, HD 138769, GC 20943, HR 5781, DM CD-44 10239, TYC 7848-2378-1",
	"group" : { "key" : "Lupus" },
	"Common" : "KT Lupi",
	"OType" : "Be Star",
	"Distance" : "130.73",
	"RA_S" : 233.97187331,
	"DEC_S" : -44.9583459,
	"X" : 284,
	"Y" : 555,
	"Constellation" : "Lupus ",
	"AMag" : 4.676,
	"key" : 75889,
	"title" : "KT Lupi"
	},
{
	"Index" : "55847",
	"Description" : "Omega Lupi (\u03C9 Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.35.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Omega Lupi, HIP 76552, SAO 226004, HD 139127, GC 21001, HR 5797, DM CD-42 10601, TYC 7844-198-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Omega Lupi",
	"OType" : "Star",
	"Distance" : "67",
	"RA_S" : 234.51334783,
	"DEC_S" : -42.56734635,
	"X" : 277,
	"Y" : 524,
	"Constellation" : "Lupus ",
	"AMag" : 4.497,
	"key" : 75847,
	"title" : "Omega Lupi"
	},
{
	"Index" : "51362",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "3 Lupi, Psi01 Lupi, HIP 76705, SAO 206843, HD 139521, GC 21042, HR 5820, DM CD-33 10631, TYC 7335-935-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Psi01 Lupi",
	"OType" : "Star",
	"Distance" : "67.31",
	"RA_S" : 234.94157258,
	"DEC_S" : -34.41192278,
	"Constellation" : "Lupus ",
	"AMag" : 4.769,
	"key" : 71362,
	"title" : "Psi01 Lupi"
	},
{
	"Index" : "55907",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "g Lupi, HIP 76829, SAO 226064, HD 139664, GC 21070, HR 5825, DM CD-44 10310, TYC 7849-3219-1",
	"group" : { "key" : "Lupus" },
	"Common" : "g Lupi",
	"OType" : "High proper-motion Star",
	"Distance" : "17.44",
	"RA_S" : 235.29740559,
	"DEC_S" : -44.66120584,
	"Constellation" : "Lupus ",
	"AMag" : 4.681,
	"key" : 75907,
	"title" : "g Lupi"
	},
{
	"Index" : "51381",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "h Lupi, HIP 76939, SAO 206887, HD 139980, GC 21103, HR 5837, DM CD-37 10441, TYC 7339-1215-1",
	"group" : { "key" : "Lupus" },
	"Common" : "h Lupi",
	"OType" : "Star",
	"Distance" : "79.89",
	"RA_S" : 235.65964827,
	"DEC_S" : -37.4249345,
	"Constellation" : "Lupus ",
	"AMag" : 5.348,
	"key" : 71381,
	"title" : "h Lupi"
	},
{
	"Index" : "51363",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "4 Lupi, Psi02 Lupi, HIP 76945, SAO 206889, HD 140008, GC 21106, HR 5839, DM CD-34 10494, TYC 7335-936-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Psi02 Lupi",
	"OType" : "Spectroscopic binary",
	"Distance" : "111.36",
	"RA_S" : 235.67091548,
	"DEC_S" : -34.71040422,
	"Constellation" : "Lupus ",
	"AMag" : 4.698,
	"key" : 71363,
	"title" : "Psi02 Lupi"
	},
{
	"Index" : "51332",
	"Description" : "Phi1 Lupi (\u03C61 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.58.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "5 Lupi, Chi Lupi, HIP 77634, SAO 207040, HD 141556, GC 21281, HR 5883, DM CD-33 10754, TYC 7332-2512-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Chi Lupi",
	"OType" : "Spectroscopic binary",
	"Distance" : "59.83",
	"RA_S" : 237.73973648,
	"DEC_S" : -33.62717361,
	"X" : 237,
	"Y" : 410,
	"Constellation" : "Lupus ",
	"AMag" : 3.94,
	"key" : 71332,
	"title" : "Chi Lupi"
	},
{
	"Index" : "51372",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Xi01 Lupi, HIP 78105A, SAO 207144, HD 142629, GC 21395, HR 5925, DM CD-33 10826A, TYC 7337-1461-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Xi01 Lupi",
	"OType" : "Star",
	"Distance" : "60.04",
	"RA_S" : 239.22287453,
	"DEC_S" : -33.9661125,
	"Constellation" : "Lupus ",
	"AMag" : 5.091,
	"key" : 71372,
	"title" : "Xi01 Lupi"
	},
{
	"Index" : "55862",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 78323, SAO 226425, HD 143009, GC 21451, HR 5943, DM CD-4110478, TYC 7846-1632-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5943",
	"OType" : "Star",
	"Distance" : "133.41",
	"RA_S" : 239.87611505,
	"DEC_S" : -41.74444011,
	"Constellation" : "Lupus ",
	"AMag" : 5.092,
	"key" : 75862,
	"title" : "HR 5943"
	},
{
	"Index" : "55926",
	"Description" : "Eta Lupi (\u03B7 Lup) is a star in the constellation Lupus. Its apparent magnitude is 3.41.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Eta Lupi, HIP 78384, SAO 207208, HD 143118, GC 21478, HR 5948, DM CD-38 10797, TYC 7851-1814-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Eta Lupi",
	"OType" : "Star",
	"Distance" : "135.4",
	"RA_S" : 240.03053121,
	"DEC_S" : -38.3967029,
	"X" : 217,
	"Y" : 473,
	"Constellation" : "Lupus ",
	"AMag" : 3.367,
	"key" : 75926,
	"title" : "Eta Lupi"
	},
{
	"Index" : "55927",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "HIP 78655, SAO 207276, HD 143699, GC 21548, HR 5967, DM CD-3810832, TYC 7851-1815-1",
	"group" : { "key" : "Lupus" },
	"Common" : "HR 5967",
	"OType" : "Star",
	"Distance" : "122.38",
	"RA_S" : 240.85078776,
	"DEC_S" : -38.60254099,
	"Constellation" : "Lupus ",
	"AMag" : 4.857,
	"key" : 75927,
	"title" : "HR 5967"
	},
{
	"Index" : "51406",
	"Description" : "Theta Lupi (\u03B8 Lup) is a star in the constellation Lupus. Its apparent magnitude is 4.21.",
	"MapNum" : "31",
	"ImageNum" : "31",
	"Desig" : "Theta Lupi, HIP 78918, SAO 207332, HD 144294, GC 21625, HR 5987, DM CD-36 10642, TYC 7342-1315-1",
	"group" : { "key" : "Lupus" },
	"Common" : "Theta Lupi",
	"OType" : "Star",
	"Distance" : "126.52",
	"RA_S" : 241.64809564,
	"DEC_S" : -36.80228417,
	"X" : 198,
	"Y" : 453,
	"Constellation" : "Lupus ",
	"AMag" : 4.172,
	"key" : 71406,
	"title" : "Theta Lupi"
	},
{
	"Index" : "26377",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "1 Lyncis, HIP 29919, SAO 13787, HD 42973, GC 8016, HR 2215, DM BD+61   869, TYC 4096-2358-1",
	"group" : { "backgroundImage" : "images/Alignment/32.png",
		"description" : "Lynx is a constellation in the northern sky, introduced in the 17th century by Johannes Hevelius. It is named after the lynx, a genus of cat. It is a very faint constellation; its brightest stars form a zigzag line.\r\rJohannes Hevelius defined the constellation in the 17th century because he wanted to fill the open gap between the constellations Ursa Major and Auriga. He supposedly named it Lynx because of its faintness: only the lynx-eyed (or those of good sight) would have been able to recognise it.\r\rThe only named star in this constellation is Alsciaukat (from the Arabic for thorn), also known as 31 Lyncis, or \u03BA Lyncis.\r\rLynx\u0027s most notable deep sky object is the Intergalactic Tramp NGC 2419, also called the \u0022Intergalactic Wanderer\u0022, a globular cluster that is one of the most distant known of its kind at a distance of 300,000 light-years from Earth. It is likely that NGC 2419 is in a highly elliptical orbit around the Milky Way. It has a magnitude of 10.3 and is a Shapley class II cluster; the classification indicates that it is extremely concentrated at its center. Originally thought to be a star, NGC 2419 was discovered to be a globular cluster by Carl Lampland.",
		"key" : "Lynx",
		"grouptype" : "Lynx",
		"Meaning" : "lynx",
		"Family" : "Ursa Major",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Lynx",
		"title" : "Lynx Objects Group" },
	"Common" : "1 Lyncis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "194.72",
	"RA_S" : 94.478417,
	"DEC_S" : 61.51528548,
	"Constellation" : "Lynx ",
	"AMag" : 5.236,
	"key" : 46377,
	"title" : "1 Lyncis"
	},
{
	"Index" : "23615",
	"Description" : "2 Lyncis (2 Lyn) is a star in the constellation Lynx. Its apparent magnitude is 4.45.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "2 Lyncis, HIP 30060, SAO 25665, HD 43378, GC 8068, HR 2238, DM BD+59   959, TYC 3776-2465-1",
	"group" : { "key" : "Lynx" },
	"Common" : "2 Lyncis",
	"OType" : "Eclipsing binary",
	"Distance" : "47.99",
	"RA_S" : 94.90576908,
	"DEC_S" : 59.01096341,
	"X" : 647,
	"Y" : 69,
	"Constellation" : "Lynx ",
	"AMag" : 4.437,
	"key" : 43615,
	"title" : "2 Lyncis"
	},
{
	"Index" : "23625",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "5 Lyncis, HIP 30679, SAO 25733, HD 44708, GC 8287, HR 2293, DM BD+58   927, TYC 3777-2070-1",
	"group" : { "key" : "Lynx" },
	"Common" : "5 Lyncis",
	"OType" : "Star",
	"Distance" : "191.28",
	"RA_S" : 96.7036394,
	"DEC_S" : 58.41740826,
	"Constellation" : "Lynx ",
	"AMag" : 5.381,
	"key" : 43625,
	"title" : "5 Lyncis"
	},
{
	"Index" : "23636",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "12 Lyncis, HIP 32438A, SAO 25939, HD 48250, GC 8805, HR 2470, DM BD+59  1015, TYC 3778-1985-1",
	"group" : { "key" : "Lynx" },
	"Common" : "12 Lyncis",
	"OType" : "Double or multiple star",
	"Distance" : "65.63",
	"RA_S" : 101.55912626,
	"DEC_S" : 59.44168551,
	"Constellation" : "Lynx ",
	"AMag" : 5.44,
	"key" : 43636,
	"title" : "12 Lyncis"
	},
{
	"Index" : "23595",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "13 Lyncis, HIP 32489, SAO 25947, HD 48432, GC 8826, HR 2477, DM BD+57  1004, TYC 3774-2113-1",
	"group" : { "key" : "Lynx" },
	"Common" : "13 Lyncis",
	"OType" : "Star",
	"Distance" : "64.65",
	"RA_S" : 101.7062844,
	"DEC_S" : 57.16917667,
	"Constellation" : "Lynx ",
	"AMag" : 5.443,
	"key" : 43595,
	"title" : "13 Lyncis"
	},
{
	"Index" : "23634",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "14 Lyncis, HIP 33048AB, SAO 26012, HD 49618, GC 8968, HR 2520, DM BD+59  1028A, TYC 3778-1982-1",
	"group" : { "key" : "Lynx" },
	"Common" : "14 Lyncis",
	"OType" : "Star",
	"Distance" : "133.08",
	"RA_S" : 103.2710312,
	"DEC_S" : 59.44854633,
	"Constellation" : "Lynx ",
	"AMag" : 5.445,
	"key" : 43634,
	"title" : "14 Lyncis"
	},
{
	"Index" : "23645",
	"Description" : "15 Lyncis (15 Lyn) is a star in the constellation Lynx. Its apparent magnitude is 4.35.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "15 Lyncis, HIP 33449, SAO 26051, HD 50522, GC 9082, HR 2560, DM BD+58   982, TYC 3779-1730-1",
	"group" : { "key" : "Lynx" },
	"Common" : "15 Lyncis",
	"OType" : "Star",
	"Distance" : "54.66",
	"RA_S" : 104.31916384,
	"DEC_S" : 58.42274437,
	"X" : 592,
	"Y" : 103,
	"Constellation" : "Lynx ",
	"AMag" : 4.448,
	"key" : 43645,
	"title" : "15 Lyncis"
	},
{
	"Index" : "20097",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "16 Lyncis, HIP 33485, SAO 41463, HD 50973, GC 9113, HR 2585, DM BD+45  1367, TYC 3391-2640-1",
	"group" : { "key" : "Lynx" },
	"Common" : "16 Lyncis",
	"OType" : "Variable Star",
	"Distance" : "73.83",
	"RA_S" : 104.4046109,
	"DEC_S" : 45.0940984,
	"Constellation" : "Lynx ",
	"AMag" : 4.896,
	"key" : 40097,
	"title" : "16 Lyncis"
	},
{
	"Index" : "23725",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "18 Lyncis, HIP 35146, SAO 26248, HD 55280, GC 9581, HR 2715, DM BD+59  1065, TYC 3792-2513-1",
	"group" : { "key" : "Lynx" },
	"Common" : "18 Lyncis",
	"OType" : "High proper-motion Star",
	"Distance" : "60.99",
	"RA_S" : 108.97876813,
	"DEC_S" : 59.63746828,
	"Constellation" : "Lynx ",
	"AMag" : 5.322,
	"key" : 43725,
	"title" : "18 Lyncis"
	},
{
	"Index" : "20171",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "HIP 35384, SAO 41681, HD 56169, GC 9681, HR 2751, DM BD+49 1612, TYC 3400-2010-1",
	"group" : { "key" : "Lynx" },
	"Common" : "HR 2751",
	"OType" : "Star",
	"Distance" : "106.81",
	"RA_S" : 109.63323201,
	"DEC_S" : 49.46475229,
	"Constellation" : "Lynx ",
	"AMag" : 5.024,
	"key" : 40171,
	"title" : "HR 2751"
	},
{
	"Index" : "20178",
	"Description" : "21 Lyncis (21 Lyn) is a star in the constellation Lynx. Its apparent magnitude is 4.61.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "21 Lyncis, HIP 36145, SAO 41764, HD 58142, GC 9909, HR 2818, DM BD+49  1623, TYC 3401-1648-1",
	"group" : { "key" : "Lynx" },
	"Common" : "21 Lyncis",
	"OType" : "Star",
	"Distance" : "83.85",
	"RA_S" : 111.6785505,
	"DEC_S" : 49.21152216,
	"X" : 579,
	"Y" : 235,
	"Constellation" : "Lynx ",
	"AMag" : 4.607,
	"key" : 40178,
	"title" : "21 Lyncis"
	},
{
	"Index" : "20177",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "22 Lyncis, HIP 36439, SAO 41808, HD 58855, GC 9992, HR 2849, DM BD+49  1630, TYC 3401-1647-1",
	"group" : { "key" : "Lynx" },
	"Common" : "22 Lyncis",
	"OType" : "Star",
	"Distance" : "20.24",
	"RA_S" : 112.48314826,
	"DEC_S" : 49.6724587,
	"Constellation" : "Lynx ",
	"AMag" : 5.409,
	"key" : 40177,
	"title" : "22 Lyncis"
	},
{
	"Index" : "23731",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "24 Lyncis, HIP 37609, SAO 26474, HD 61497, GC 10343, HR 2946, DM BD+59  1103, TYC 3794-1738-1",
	"group" : { "key" : "Lynx" },
	"Common" : "24 Lyncis",
	"OType" : "High proper-motion Star",
	"Distance" : "81.81",
	"RA_S" : 115.75173128,
	"DEC_S" : 58.71035973,
	"Constellation" : "Lynx ",
	"AMag" : 4.958,
	"key" : 43731,
	"title" : "24 Lyncis"
	},
{
	"Index" : "20268",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "HIP 37701A, SAO 26488, HD 61931, GC 10377, HR 2969, DM BD+50 1460, TYC 3412-2662-1",
	"group" : { "key" : "Lynx" },
	"Common" : "HR 2969",
	"OType" : "Star",
	"Distance" : "219.15",
	"RA_S" : 116.01741809,
	"DEC_S" : 50.43379644,
	"Constellation" : "Lynx ",
	"AMag" : 5.329,
	"key" : 40268,
	"title" : "HR 2969"
	},
{
	"Index" : "16266",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "HIP 37946, SAO 60328, HD 62647, GC 10460, HR 2999, DM BD+37 1769, TYC 2959-1907-1",
	"group" : { "key" : "Lynx" },
	"Common" : "V* DU Lyn",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "132.35",
	"RA_S" : 116.66367995,
	"DEC_S" : 37.51739466,
	"Constellation" : "Lynx ",
	"AMag" : 5.343,
	"key" : 36266,
	"title" : "V* DU Lyn"
	},
{
	"Index" : "20281",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "27 Lyncis, HIP 39847, SAO 26687, HD 67006, GC 11018, HR 3173, DM BD+51  1391, TYC 3414-2496-1",
	"group" : { "key" : "Lynx" },
	"Common" : "27 Lyncis",
	"OType" : "High proper-motion Star",
	"Distance" : "76.64",
	"RA_S" : 122.11436221,
	"DEC_S" : 51.5066692,
	"Constellation" : "Lynx ",
	"AMag" : 4.8,
	"key" : 40281,
	"title" : "27 Lyncis"
	},
{
	"Index" : "16401",
	"Description" : "31 Lyncis is the fourth-brightest star in the constellation Lynx. Its apparent magnitude is +4.25 and it belongs to the spectral class K4.5III-IIIb. This star has the traditional names Alsciaukat, from Arabic \u0627\u0644\u0634\u0648\u0643\u0629 a\u0161-\u0161awkat \u0022the thorn\u0022, and Mabsuthat (Arabic \u0627\u0644\u0645\u0628\u0633\u0648\u0637\u0629 al-mabs\u016Btah) \u0022the outstretched (paw)\u0022.\r\r31 Lyncis is an orange giant star located about 390 light years from Earth.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "31 Lyncis, HIP 41075, SAO 42319, HD 70272, GC 11401, HR 3275, DM BD+43  1815, TYC 2980-2184-1",
	"group" : { "key" : "Lynx" },
	"Common" : "Alsciaukat / Mabsuthat",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "117.11",
	"RA_S" : 125.70879565,
	"DEC_S" : 43.18813268,
	"X" : 470,
	"Y" : 336,
	"Constellation" : "Lynx ",
	"AMag" : 4.415,
	"key" : 36401,
	"shortTitle" : "Mabsuthat",
	"title" : "Alsciaukat / Mabsuthat"
	},
{
	"Index" : "20298",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "34 Lyncis, HIP 42604, SAO 42490, HD 73593, GC 11903, HR 3422, DM BD+46  1422, TYC 3416-2267-1",
	"group" : { "key" : "Lynx" },
	"Common" : "34 Lyncis",
	"OType" : "Star",
	"Distance" : "55.26",
	"RA_S" : 130.2544584,
	"DEC_S" : 45.83401209,
	"Constellation" : "Lynx ",
	"AMag" : 5.468,
	"key" : 40298,
	"title" : "34 Lyncis"
	},
{
	"Index" : "16460",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "35 Lyncis, HIP 43531, SAO 42576, HD 75506, GC 12221, HR 3508, DM BD+44  1794, TYC 2988-1628-1",
	"group" : { "key" : "Lynx" },
	"Common" : "35 Lyncis",
	"OType" : "Star",
	"Distance" : "81.18",
	"RA_S" : 132.98679751,
	"DEC_S" : 43.72660265,
	"Constellation" : "Lynx ",
	"AMag" : 5.255,
	"key" : 36460,
	"title" : "35 Lyncis"
	},
{
	"Index" : "16445",
	"Description" : "10 Ursae Majoris (10 UMa) is a star in the constellation Lynx. Its apparent magnitude is 3.96.\r\rHR 3579 is a tight double that consists of a fourth magnitude (4.11) class F (F5) dwarf in mutual orbit with near-solar clone, a sixth magnitude (6.18) class G (G5) dwarf. The average separation of 10.6 Astronomical Units (about half a second of arc as seen on the sky) coupled with an orbital period of 21.78 years leads to a total system mass of 2.54 solar masses, and an estimate of the mass ratio tells that the primary class F component carries 1.44 solar, while the lesser class G star carries 1.1 solar.\r\rA modest eccentricity varies the separation between 12.2 and 9.0 AU. The distance, brightnesses, and temperatures (respectively 6500 and 5600 Kelvin) lead to respective luminosities of 4.8 and 0.8 solar and (with application of stellar structure theory) masses of 1.4 and 1.0 solar, the sum of which is very close to that inferred from the binary orbit. A rotation velocity for the primary (10 UMa A) of at least 34 kilometers per second yields a rotation period less than 2.6 days. The class G star (10 UMa B) closely resembles what the Sun looked like in its younger days, when it was but 2 billion years old (it is now 4.6 billion) and slightly dimmer, something to contemplate as we gaze into the otherwise obscure stars of the Lynx.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "10 Ursae Majoris, HIP 44248AB, SAO 42642, HD 76943, GC 12434, HR 3579, DM BD+42  1956, TYC 2986-1978-1",
	"group" : { "key" : "Lynx" },
	"Common" : "10 Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "16.07",
	"RA_S" : 135.15991945,
	"DEC_S" : 41.78294587,
	"X" : 380,
	"Y" : 358,
	"Constellation" : "Lynx ",
	"AMag" : 4.026,
	"key" : 36445,
	"title" : "10 Ursae Majoris"
	},
{
	"Index" : "16424",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "HIP 44700, SAO 61254, HD 77912, GC 12565, HR 3612, DM BD+39 2200, TYC 2983-1983-1",
	"group" : { "key" : "Lynx" },
	"Common" : "HR 3612",
	"OType" : "Peculiar Star",
	"Distance" : "249.45",
	"RA_S" : 136.63236308,
	"DEC_S" : 38.45221297,
	"Constellation" : "Lynx ",
	"AMag" : 4.653,
	"key" : 36424,
	"title" : "HR 3612"
	},
{
	"Index" : "16479",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "36 Lyncis, HIP 45290, SAO 42759, HD 79158, GC 12716, HR 3652, DM BD+43  1893, TYC 2990-1662-1",
	"group" : { "key" : "Lynx" },
	"Common" : "36 Lyncis",
	"OType" : "Rotationally variable Star",
	"Distance" : "177.6",
	"RA_S" : 138.45086523,
	"DEC_S" : 43.21782641,
	"Constellation" : "Lynx ",
	"AMag" : 5.261,
	"key" : 36479,
	"title" : "36 Lyncis"
	},
{
	"Index" : "12217",
	"Description" : "38 Lyncis (38 Lyn, 38 Lyncis) is a Class A1, fourth-magnitude star in the constellation Lynx. Johannes Hevelius was referring to the Eurasian lynx, which he and others perceived as being spotted like a leopard. 38 Lyncis is a binary double star located about 120 light-years from Earth.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "38 Lyncis, HIP 45688B, SAO 61391, HD 80081B, GC 12830, HR 3690, DM BD+37  1965, TYC 2499-1655-2",
	"group" : { "key" : "Lynx" },
	"Common" : "38 Lyncis",
	"OType" : "Double or multiple star",
	"Distance" : "38.23",
	"RA_S" : 139.710454,
	"DEC_S" : 36.802356,
	"X" : 332,
	"Y" : 421,
	"Constellation" : "Lynx ",
	"AMag" : 6.093,
	"key" : 32217,
	"title" : "38 Lyncis"
	},
{
	"Index" : "12216",
	"Description" : "38 Lyncis (38 Lyn, 38 Lyncis) is a Class A1, fourth-magnitude star in the constellation Lynx. Johannes Hevelius was referring to the Eurasian lynx, which he and others perceived as being spotted like a leopard. 38 Lyncis is a binary double star located about 120 light-years from Earth.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "38 Lyncis, HIP 45688A, SAO 61391, HD 80081A, GC 12830, HR 3690, DM BD+37  1965, TYC 2499-1655-1",
	"group" : { "key" : "Lynx" },
	"Common" : "38 Lyncis",
	"OType" : "Star",
	"Distance" : "38.23",
	"RA_S" : 139.711108,
	"DEC_S" : 36.802875,
	"X" : 332,
	"Y" : 421,
	"Constellation" : "Lynx ",
	"AMag" : 3.916,
	"key" : 32216,
	"title" : "38 Lyncis"
	},
{
	"Index" : "12187",
	"Description" : "Alpha Lyncis (\u03B1 Lyn, \u03B1 Lyncis) is the brightest star in the northern constellation of Lynx with an apparent magnitude of +3.13. Unusually, it is the only star in the constellation that has a Bayer designation. Based upon parallax measurements, this star is located about 203 light-years (62 parsecs) from the Earth.\r\rThis is a giant star that has exhausted the hydrogen at its core and has evolved away from the main sequence. It has expanded to about 55 times the Sun\u0027s radius and it is presently emitting roughly 673 times the luminosity of the Sun. The estimated effective temperature of the star\u0027s outer envelope is 3,882 K, which is lower than the Sun\u0027s effective temperature of 5,778 K, and is giving Alpha Lyncis an orange hue that is characteristic of K-type stars.\r\rAlpha Lyncis is a suspected small-amplitude red variable star that changes apparent magnitude from +3.17 up to +3.12. This variability pattern typically occurs in stars that have developed an inert carbon core surrounded by a helium-fusing shell, and suggests that Alpha Lyncis is starting to evolve into a Mira-type variable.",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "40 Lyncis, Alpha Lyncis, HIP 45860, SAO 61414, HD 80493, GC 12880, HR 3705, DM BD+35  1979, TYC 2496-1728-1",
	"group" : { "key" : "Lynx" },
	"Common" : "Alpha Lyncis",
	"OType" : "High proper-motion Star",
	"Distance" : "62.26",
	"RA_S" : 140.26376269,
	"DEC_S" : 34.39256508,
	"X" : 325,
	"Y" : 453,
	"Constellation" : "Lynx ",
	"AMag" : 3.291,
	"key" : 32187,
	"title" : "Alpha Lyncis"
	},
{
	"Index" : "16495",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "HIP 47029, SAO 61578, HD 82741, GC 13221, HR 3809, DM BD+40 2224, TYC 2992-1689-1",
	"group" : { "key" : "Lynx" },
	"Common" : "HR 3809",
	"OType" : "Star",
	"Distance" : "66.03",
	"RA_S" : 143.76595818,
	"DEC_S" : 39.62149299,
	"Constellation" : "Lynx ",
	"AMag" : 4.909,
	"key" : 36495,
	"title" : "HR 3809"
	},
{
	"Index" : "16506",
	"MapNum" : "32",
	"ImageNum" : "32",
	"Desig" : "42 Lyncis, HIP 47300, SAO 42958, HD 83287, GC 13301, HR 3829, DM BD+40  2232, TYC 2995-1482-1",
	"group" : { "key" : "Lynx" },
	"Common" : "42 Lyncis",
	"OType" : "Star",
	"Distance" : "37.57",
	"RA_S" : 144.59072988,
	"DEC_S" : 40.23979341,
	"Constellation" : "Lynx ",
	"AMag" : 5.304,
	"key" : 36506,
	"title" : "42 Lyncis"
	},
{
	"Index" : "13296",
	"Description" : "Kappa Lyrae (\u03BA Lyr) is a 4th magnitude star approximately 238 light years away from Earth, in the constellation Lyra. It is an orange giant star of the spectral type is K2III, meaning it possesses a surface temperature of 3,500 to 5,000 kelvins. It is cooler, yet larger and brighter, than our Sun. It is also a variable star.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "1 Lyrae, Kappa Lyrae, HIP 89826, SAO 66869, HD 168775, GC 25032, HR 6872, DM BD+36  3094, TYC 2635-1483-1",
	"group" : { "backgroundImage" : "images/Alignment/27.png",
		"description" : "Lyra (pron.: /\u02C8la\u026A\u0259r\u0259/; Latin for lyre, from Greek \u03BB\u03CD\u03C1\u03B1) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Its principal star, Vega (Abhijit in Sanskrit), a corner of the Summer Triangle, is one of the brightest stars in the sky. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus.\r\rLyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.\r\rIn the past, Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, either enclosed in its wings, or in its beak. It was sometimes referred to as Aquila Cadens or Vultur Cadens (falling eagle or falling vulture).\r\rIn Greek mythology, Lyra was associated with the myth of Orpheus, the musician who was killed by the Bacchantes. After his death, his lyre was thrown into the river; Zeus sent an eagle to retrieve the lyre, and ordered both of them to be placed in the sky. In Wales, Lyra is known as King Arthur\u0027s Harp (Talyn Arthur), and King David\u0027s harp . The Persian Hafiz called it the Lyre of Zurah. It has been called the Manger of the Infant Saviour, Praesepe Salvatoris .",
		"key" : "Lyra",
		"grouptype" : "Lyra",
		"Meaning" : "lyre / harp",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Lyra",
		"title" : "Lyra Objects Group" },
	"Common" : "Kappa Lyrae",
	"OType" : "Variable Star",
	"Distance" : "77.15",
	"RA_S" : 274.96545761,
	"DEC_S" : 36.0645453,
	"X" : 222,
	"Y" : 253,
	"Constellation" : "Lyra ",
	"AMag" : 4.446,
	"key" : 33296,
	"title" : "Kappa Lyrae"
	},
{
	"Index" : "17408",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "2 Lyrae, Mu Lyrae, HIP 90191, SAO 66943, HD 169702, GC 25137, HR 6903, DM BD+39  3410, TYC 3108-2592-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Alathfar",
	"OType" : "Star",
	"Distance" : "134.51",
	"RA_S" : 276.05743609,
	"DEC_S" : 39.50723859,
	"Constellation" : "Lyra ",
	"AMag" : 5.111,
	"key" : 37408,
	"shortTitle" : "Al Athfar",
	"title" : "Alathfar"
	},
{
	"Index" : "13222",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 90923, SAO 67090, HD 171301, GC 25340, HR 6968, DM BD+30 3223, TYC 2624-2539-1",
	"group" : { "key" : "Lyra" },
	"Common" : "HR 6968",
	"OType" : "Star",
	"Distance" : "109.56",
	"RA_S" : 278.2081527,
	"DEC_S" : 30.55420683,
	"Constellation" : "Lyra ",
	"AMag" : 5.454,
	"key" : 33222,
	"title" : "HR 6968"
	},
{
	"Index" : "13368",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 91235, SAO 67164, HD 172044, GC 25443, HR 6997, DM BD+33 3154, TYC 2641-2396-1",
	"group" : { "key" : "Lyra" },
	"Common" : "HR 6997",
	"OType" : "Spectroscopic binary",
	"Distance" : "154.35",
	"RA_S" : 279.15560431,
	"DEC_S" : 33.46903861,
	"Constellation" : "Lyra ",
	"AMag" : 5.393,
	"key" : 33368,
	"title" : "HR 6997"
	},
{
	"Index" : "17543",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "4 Lyrae, Epsilon01 Lyrae, HIP 91919A, SAO 67310, HD 173582, GC 25667, HR 7051, DM BD+39  3509A, TYC 3122-3438-2",
	"group" : { "key" : "Lyra" },
	"Common" : "Epsilon01 Lyrae",
	"OType" : "Star",
	"Distance" : "49.67",
	"RA_S" : 281.08477158,
	"DEC_S" : 39.67012519,
	"Constellation" : "Lyra ",
	"AMag" : 5.008,
	"key" : 37543,
	"title" : "Epsilon01 Lyrae"
	},
{
	"Index" : "17544",
	"Description" : "Epsilon Lyrae (\u03B5 Lyr, \u03B5 Lyrae), also known as the Double Double, is a multiple star system approximately 162 light-years away in the constellation of Lyra. The widest two components of the system are easily separated when viewed through binoculars, or even with the naked eye under excellent conditions. The northern star is called \u03B51 and the southern one is called \u03B52; they both lie around 162 light years from Earth and orbit each other. When viewed at higher magnifications, both stars of the binary can be further split into binaries; that is, the system contains two binary stars orbiting each other. Being able to view the components of each is a common benchmark for the resolving power of telescopes, since the individual doubles are so close together: the stars of \u03B51 were 2.35 arc-seconds apart in 2006, those of \u03B52 were separated by about the same amount in that year. Since the first high-precision measurements of their orbit in the 1980s, both binaries have moved only a few degrees in position angle.\r\rThe component stars of \u03B51 have magnitudes of 4.7 and 6.2 separated by 2.6\u0022 and have an orbital period that can only be crudely estimated at 1200 years, which places them at roughly 140 AU apart. The component stars of \u03B52 have magnitudes 5.1 and 5.5 separated by 2.3\u0022, and orbit in perhaps half that period. \u03B51 and \u03B52 themselves are not closer than 0.16 light years apart, and would take hundreds of thousands of years to complete an orbit. An observer at one pair would see the other pair shining with the light of a quarter Moon (which is about mv = -5.0), less than a degree away from each other.\r\rA fifth component of this system, orbiting one of the \u03B52 pair, was detected by speckle interferometry in 1985 and confirmed in two subsequent observations. No orbit can be prepared from such limited data, but its rapid motion suggests a period of a few tens of years. Its maximum observed separation of 0.2 arc-seconds precludes direct visual observation.\r\rA number of other nearby stars may also be part of the system, bringing the system to a total of ten stars.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "5 Lyrae, Epsilon02 Lyrae, HIP 91926C, SAO 67315, HD 173607, GC 25668, HR 7053, DM BD+39  3510C, TYC 3122-3439-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Double Double",
	"OType" : "Double or multiple star",
	"Distance" : "47.65",
	"RA_S" : 281.09527752,
	"DEC_S" : 39.6127459,
	"X" : 166,
	"Y" : 198,
	"Constellation" : "Lyra ",
	"AMag" : 5.246,
	"key" : 37544,
	"title" : "Double Double"
	},
{
	"Index" : "17545",
	"Description" : "Epsilon Lyrae (\u03B5 Lyr, \u03B5 Lyrae), also known as the Double Double, is a multiple star system approximately 162 light-years away in the constellation of Lyra. The widest two components of the system are easily separated when viewed through binoculars, or even with the naked eye under excellent conditions. The northern star is called \u03B51 and the southern one is called \u03B52; they both lie around 162 light years from Earth and orbit each other. When viewed at higher magnifications, both stars of the binary can be further split into binaries; that is, the system contains two binary stars orbiting each other. Being able to view the components of each is a common benchmark for the resolving power of telescopes, since the individual doubles are so close together: the stars of \u03B51 were 2.35 arc-seconds apart in 2006, those of \u03B52 were separated by about the same amount in that year. Since the first high-precision measurements of their orbit in the 1980s, both binaries have moved only a few degrees in position angle.\r\rThe component stars of \u03B51 have magnitudes of 4.7 and 6.2 separated by 2.6\u0022 and have an orbital period that can only be crudely estimated at 1200 years, which places them at roughly 140 AU apart. The component stars of \u03B52 have magnitudes 5.1 and 5.5 separated by 2.3\u0022, and orbit in perhaps half that period. \u03B51 and \u03B52 themselves are not closer than 0.16 light years apart, and would take hundreds of thousands of years to complete an orbit. An observer at one pair would see the other pair shining with the light of a quarter Moon (which is about mv = -5.0), less than a degree away from each other.\r\rA fifth component of this system, orbiting one of the \u03B52 pair, was detected by speckle interferometry in 1985 and confirmed in two subsequent observations. No orbit can be prepared from such limited data, but its rapid motion suggests a period of a few tens of years. Its maximum observed separation of 0.2 arc-seconds precludes direct visual observation.\r\rA number of other nearby stars may also be part of the system, bringing the system to a total of ten stars.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "5 Lyrae, Epsilon02 Lyrae, HIP 91926D, HD 173608, HR 7054, DM BD+39  3510D, TYC 3122-3439-2",
	"group" : { "key" : "Lyra" },
	"Common" : "Double Double",
	"OType" : "Star",
	"Distance" : "47.65",
	"RA_S" : 281.09527752,
	"DEC_S" : 39.6127459,
	"X" : 166,
	"Y" : 198,
	"Constellation" : "Lyra ",
	"AMag" : 5.383,
	"key" : 37545,
	"title" : "Double Double"
	},
{
	"Index" : "17485",
	"Description" : "Zeta1 Lyrae (\u03B61 Lyr) is a star in the constellation Lyra. Its apparent magnitude is 4.34.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "6 Lyrae, Zeta01 Lyrae, HIP 91971, SAO 67321, HD 173648, GC 25676, HR 7056, DM BD+37  3222, TYC 3118-2080-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Zeta Lyrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.87",
	"RA_S" : 281.19314347,
	"DEC_S" : 37.60511039,
	"X" : 161,
	"Y" : 224,
	"Constellation" : "Lyra ",
	"AMag" : 4.342,
	"key" : 37485,
	"title" : "Zeta Lyrae"
	},
{
	"Index" : "9173",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 92088, SAO 86418, HD 173780, GC 25721, HR 7064, DM BD+26 3349, TYC 2116-2764-1",
	"group" : { "key" : "Lyra" },
	"Common" : "HR 7064",
	"OType" : "Star",
	"Distance" : "78.09",
	"RA_S" : 281.51866667,
	"DEC_S" : 26.66213209,
	"Constellation" : "Lyra ",
	"AMag" : 4.958,
	"key" : 29173,
	"title" : "HR 7064"
	},
{
	"Index" : "13381",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "9 Lyrae, Nu Lyrae, HIP 92405, SAO 67446, HD 174602, GC 25841, HR 7102, DM BD+32  3228, TYC 2642-2932-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Nu Lyrae",
	"OType" : "Star",
	"Distance" : "70.95",
	"RA_S" : 282.47048591,
	"DEC_S" : 32.55106181,
	"Constellation" : "Lyra ",
	"AMag" : 5.239,
	"key" : 33381,
	"title" : "Nu Lyrae"
	},
{
	"Index" : "13378",
	"Description" : "Beta Lyrae (\u03B2 Lyr, \u03B2 Lyrae) is a binary star system approximately 960 light-years (290 parsecs) away in the constellation Lyra. Beta Lyrae has the traditional name Sheliak (occasionally Shelyak), from \u0627\u0644\u0634\u0644\u064A\u0627\u0642 \u0161iliy\u0101q, the Arabic name of the constellation Lyra. The Bayer designation for this star was given by the German astronomer Johann Bayer with the publication of his star atlas Uranometria in 1603. It was given the Flamsteed designation 10 Lyrae by John Flamsteed in 1712 with the first publication of his star catalogue. The variable luminosity of this system was discovered in 1784 by the British amateur astronomer John Goodricke.\r\rBeta Lyrae is a semidetached binary system made up of a stellar class B7II primary star and a secondary that is probably also a B-type star. The brighter, less massive star (B7II) in the system was once the more massive member of the pair, which caused it to evolve away from the main sequence first and become a giant star. Because the pair are in a close orbit, as this star expanded into a giant it filled its Roche lobe and transferred most of its mass over to its companion. The secondary, now more massive star is surrounded by an accretion disk from this mass transfer, with bipolar, jet-like features projecting perpendicular to the disk. This accretion disk blocks our view of the secondary star, lowering its apparent luminosity and making it difficult for astronomers to pinpoint what its stellar type is. The amount of mass being transferred between the two stars is about 2 \u00D7 10\u20135 solar masses per year, or the equivalent of the Sun\u0027s mass every 50,000 years, which results in an increase in orbital period of about 19 seconds each year. The orbital plane of this system is nearly aligned with the line of sight from the Earth, so the two stars periodically eclipse each other. This causes Beta Lyrae to regularly change its apparent magnitude from +3.4 to +4.6 over an orbital period of 12.9414 days. The two components are so close together that they cannot be resolved with optical telescopes, forming a spectroscopic binary. In 2008, the primary star and the accretion disk of the secondary star were resolved and imaged using the CHARA Array interferometer and the Michigan InfraRed Combiner (MIRC) in the near infrared H band (see video below), allowing the orbital elements to be computed for the first time.\r\rTwo other stars appear close to the line of sight of Beta Lyrae, but are not part of the binary system. One, at an angular distance of 45.7\u0022, is of spectral type B7V, has an apparent magnitude of +7.2, and can easily be seen with binoculars. It is about 80 times as luminous as the Sun and is also a spectroscopic binary with a period of 4.34 days. The other is magnitude 9.9v separation 86\u0022 and with a luminosity 7 times that of the Sun.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "10 Lyrae, Beta Lyrae, HIP 92420, SAO 67452, HD 174638, GC 25847, HR 7106, DM BD+33  3223A, TYC 2642-2929-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Sheliak",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "294.1",
	"RA_S" : 282.51997683,
	"DEC_S" : 33.36266874,
	"X" : 136,
	"Y" : 276,
	"Constellation" : "Lyra ",
	"AMag" : 3.631,
	"key" : 33378,
	"shortTitle" : "Shelyak; Shiliak",
	"title" : "Sheliak"
	},
{
	"Index" : "13489",
	"Description" : "Delta2 Lyrae (\u03B42 Lyr) is a 4th magnitude star in the constellation Lyra, approximately 900 light years away from Earth. It is one of the M4II spectral standard stars, meaning it is a bright giant star with a surface temperature around 3,600 kelvins. It puts out more energy than 10,000 suns, although more than 90% of it at longer than visual wavelengths. Direct angular measurements, combined with the Hipparcos parallax, give a radius of 1.1 - 1.3 astronomical units, comparable to the size calculated from other observed data.\r\rIt began life as a hot blue main sequence star, but now is a large cool asymptotic giant branch star with a degenerate helium core. It is a semi-regular variable star that has its brightness change by 0.2 magnitudes over an ill-defined period. Delta2 Lyrae was once thought to form a visual binary with the star Delta1 Lyrae, but it does not, only appearing to do so to the naked eye.\r\rThe spectral type of the nearby star system CCDM J18545+3654BC suggests that they are at the same distance as Delta2 Lyrae, which could mean that the three stars form a triple star system. In this case, CCDM J18545+3654BC would be 24,000 AU away from Delta2 Lyrae, and it would take 24,000 years for it to make an orbit. The two stars in the CCDM J18545+3654BC system take at least 10,500 years to make an orbit and are separated by 600AU.\r\rDelta2 Lyrae is the brightest member of the scattered open cluster Stephenson 1.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "12 Lyrae, Delta02 Lyrae, HIP 92791, SAO 67559, HD 175588, GC 25959, HR 7139, DM BD+36  3319, TYC 2651-2548-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Delta Lyrae",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "261.76",
	"RA_S" : 283.62618203,
	"DEC_S" : 36.89861113,
	"X" : 134,
	"Y" : 228,
	"Constellation" : "Lyra ",
	"AMag" : 4.464,
	"key" : 33489,
	"title" : "Delta Lyrae"
	},
{
	"Index" : "17645",
	"Description" : "R Lyrae is a 4th magnitude star in the constellation Lyra, approximately 350 light years away from Earth. It is a red giant star of the spectral type M5III, meaning it has a surface temperature of under 3,500 kelvins. It is much larger and brighter, yet cooler, than our Sun. It is a semiregular pulsating star. In the near-infrared J band, it is brighter than Vega.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "13 Lyrae, R Lyrae, HIP 92862, SAO 47919, HD 175865, GC 25996, HR 7157, DM BD+43  3117, TYC 3131-2155-1",
	"group" : { "key" : "Lyra" },
	"Common" : "R Lyrae",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "91.39",
	"RA_S" : 283.83375594,
	"DEC_S" : 43.94609071,
	"X" : 152,
	"Y" : 137,
	"Constellation" : "Lyra ",
	"AMag" : 4.355,
	"key" : 37645,
	"title" : "R Lyrae"
	},
{
	"Index" : "13398",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 93017A, SAO 67612, HD 176051A, HR 7162, DM BD+32 3267, TYC 2643-3345-1",
	"group" : { "key" : "Lyra" },
	"Common" : "HR 7162",
	"OType" : "High proper-motion Star",
	"Distance" : "14.87",
	"RA_S" : 284.256125,
	"DEC_S" : 32.901603,
	"Constellation" : "Lyra ",
	"AMag" : 5.342,
	"key" : 33398,
	"title" : "HR 7162"
	},
{
	"Index" : "13400",
	"Description" : "Gamma Lyrae (\u03B3 Lyr, \u03B3 Lyrae) is the second brightest star in the northern constellation of Lyra. It has the traditional names Sulafat (Sulaphat), from the Arabic \u0627\u0644\u0633\u0644\u062D\u0641\u0627\u0629 al-sul\u1E25af\u0101t \u0022turtle\u0022, and Jugum, from the Latin iugum \u0022yoke\u0022. The connection with turtles is that fine harps were traditionally made of tortoiseshell. The apparent visual magnitude of Sulafat is 3.3, which is readily visible to the naked eye. Parallax measurements yield an estimated distance of 620 light-years (190 parsecs) from the Earth.\r\rThis is a giant star with a stellar classification of B9 III, indicating it has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The effective temperature of the outer envelope of this star is 10,080 K, giving it the blue-white hue typical of a B-type star. The interferometry-measured angular diameter of this star is 0.74 \u00B1 0.10 mas, which, at its estimated distance, equates to a physical radius of roughly 15 times the radius of the Sun.\r\rIn 1909, Canadian astronomer Samuel A. Mitchell identified this star as a spectroscopic binary, although he was unable to split the absorption lines of the components. He found that a period of 25.6 days matched his measurements. It was reported as a spectroscopic binary as recently as 2001, but is now believed to be a single star with a high rate of rotation for stars of this type.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "14 Lyrae, Gamma Lyrae, HIP 93194, SAO 67663, HD 176437, GC 26086, HR 7178, DM BD+32  3286, TYC 2643-3346-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Sulafat / Jugum",
	"OType" : "Star",
	"Distance" : "189.51",
	"RA_S" : 284.73592752,
	"DEC_S" : 32.68955708,
	"X" : 111,
	"Y" : 280,
	"Constellation" : "Lyra ",
	"AMag" : 3.217,
	"key" : 33400,
	"shortTitle" : "Sulaphat",
	"title" : "Sulafat / Jugum"
	},
{
	"Index" : "9263",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "HIP 93256, SAO 86673, HD 176527, GC 26101, HR 7181, DM BD+26 3418, TYC 2126-2370-1",
	"group" : { "key" : "Lyra" },
	"Common" : "HR 7181",
	"OType" : "Star",
	"Distance" : "99.09",
	"RA_S" : 284.93951748,
	"DEC_S" : 26.23040713,
	"Constellation" : "Lyra ",
	"AMag" : 5.399,
	"key" : 29263,
	"title" : "HR 7181"
	},
{
	"Index" : "13401",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "15 Lyrae, Lambda Lyrae, HIP 93279, SAO 67682, HD 176670, GC 26115, HR 7192, DM BD+31  3424, TYC 2643-3347-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Lambda Lyrae",
	"OType" : "Variable Star",
	"Distance" : "336.09",
	"RA_S" : 285.00343495,
	"DEC_S" : 32.1455074,
	"Constellation" : "Lyra ",
	"AMag" : 5.103,
	"key" : 33401,
	"title" : "Lambda Lyrae"
	},
{
	"Index" : "21311",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "16 Lyrae, HIP 93408, SAO 48011, HD 177196, GC 26181, HR 7215, DM BD+46  2602, TYC 3545-3041-1",
	"group" : { "key" : "Lyra" },
	"Common" : "16 Lyrae",
	"OType" : "Variable Star",
	"Distance" : "37.44",
	"RA_S" : 285.359902,
	"DEC_S" : 46.93482327,
	"Constellation" : "Lyra ",
	"AMag" : 5.03,
	"key" : 41311,
	"title" : "16 Lyrae"
	},
{
	"Index" : "13497",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "18 Lyrae, Iota Lyrae, HIP 93903, SAO 67834, HD 178475, GC 26338, HR 7262, DM BD+35  3485, TYC 2652-1709-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Iota Lyrae",
	"OType" : "Be Star",
	"Distance" : "273.73",
	"RA_S" : 286.82553819,
	"DEC_S" : 36.10015915,
	"Constellation" : "Lyra ",
	"AMag" : 5.235,
	"key" : 33497,
	"title" : "Iota Lyrae"
	},
{
	"Index" : "13412",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "17 Lyrae, HIP 93917, SAO 67835, HD 178449, GC 26340, HR 7261, DM BD+32  3326, TYC 2644-2411-1",
	"group" : { "key" : "Lyra" },
	"Common" : "17 Lyrae",
	"OType" : "Spectroscopic binary",
	"Distance" : "41.57",
	"RA_S" : 286.85658901,
	"DEC_S" : 32.50173295,
	"Constellation" : "Lyra ",
	"AMag" : 5.264,
	"key" : 33412,
	"title" : "17 Lyrae"
	},
{
	"Index" : "17526",
	"Description" : "Eta Lyrae (\u03B7 Lyr, \u03B7 Lyrae) is a star in the constellation Lyra. It has the traditional name Aladfar, from the Arabic \u0627\u0644\u0623\u0638\u0641\u0631 al-\u0027uz\u0327fur \u0022the talons (of the swooping eagle)\u0022, a name it shares with Mu Lyrae (though the latter is typically spelled Alathfar in English).\r\rEta Lyrae belongs to spectral class B2.5IV and has apparent magnitude of +4.39. It is approximately 1040 light years from Earth.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "20 Lyrae, Eta Lyrae, HIP 94481, SAO 68010, HD 180163, GC 26507, HR 7298, DM BD+38  3490, TYC 3121-2285-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Aladfar",
	"OType" : "Spectroscopic binary",
	"Distance" : "423.97",
	"RA_S" : 288.43953049,
	"DEC_S" : 39.14596968,
	"X" : 93,
	"Y" : 188,
	"Constellation" : "Lyra ",
	"AMag" : 4.373,
	"key" : 37526,
	"title" : "Aladfar"
	},
{
	"Index" : "17528",
	"Description" : "Theta Lyrae (\u03B8 Lyr) is a star in a trinary star system, in the constellation Lyra, approximately 770 light years away from Earth. Theta Lyrae is an orange bright giant star of the spectral type K0II, meaning it possesses a surface temperature of about 5,000 kelvins, and is many times bigger and brighter, yet cooler, than our Sun.\r\rIt is orbited by a subsystem composed of BD+37\u00B0 3399 and BD+37\u00B0 3399B. 10th magnitude BD+37\u00B0 3399 is a giant star with a spectral type of K2III. It is therefore almost the same temperature as Theta Lyrae, but smaller and dimmer. BD+37\u00B0 3399B is an 11th magnitude star of an unknown spectral type.",
	"MapNum" : "27",
	"ImageNum" : "27",
	"Desig" : "21 Lyrae, Theta Lyrae, HIP 94713, SAO 68065, HD 180809, GC 26585, HR 7314, DM BD+37  3398, TYC 3121-2287-1",
	"group" : { "key" : "Lyra" },
	"Common" : "Theta Lyrae",
	"OType" : "Star",
	"Distance" : "254.53",
	"RA_S" : 289.09205674,
	"DEC_S" : 38.13373018,
	"X" : 83,
	"Y" : 199,
	"Constellation" : "Lyra ",
	"AMag" : 4.476,
	"key" : 37528,
	"title" : "Theta Lyrae"
	},
{
	"Index" : "68567",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Mu Mensae, HIP 21949, SAO 256122, HD 30612, GC 5809, HR 1541, DM CP-71   282, TYC 9157-1971-1",
	"group" : { "backgroundImage" : "images/Alignment/13.png",
		"description" : "Mensa is a constellation in the southern sky, created in the 18th century. Its name is Latin for table. It covers a keystone-shaped wedge of sky stretching from approximately 4h to 7.5h of right ascension, and \u221271 to \u221285.5 degrees of declination. Other than the south polar constellation of Octans, it is the most southerly of constellations. As a result, it is essentially unobservable from the Northern Hemisphere. Besides those already mentioned, its other neighbouring constellations are Chamaeleon, Dorado, Hydrus and Volans.\r\rMensa was created by Nicolas Louis de Lacaille out of dim Southern Hemisphere stars in honor of Table Mountain, a South African mountain. Though the stars of Mensa do not feature in any ancient mythology, the mountain it is named after has a rich mythology. Called \u0022Tafelberg\u0022 in Dutch and German, the mesa has two neighboring mountains called \u0022Devil\u0027s Peak\u0022 and \u0022Lion\u0027s Head\u0022. Table Mountain features in the mythology of the Cape of Good Hope, notorious for its storms\u2014the explorer Bartolomeu Dias saw the mesa as a mythical anvil for storms. Another myth relating to its dangers comes from Sinbad the Sailor, an Arabic folk hero who saw the mountain as a magnet pulling his ships to the bottom of the sea.",
		"key" : "Mensa",
		"grouptype" : "Mensa",
		"Meaning" : "Table Mountain (South Africa)",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Mensa",
		"title" : "Mensa Objects Group" },
	"Common" : "Mu Mensae",
	"OType" : "Star",
	"Distance" : "150.39",
	"RA_S" : 70.76650682,
	"DEC_S" : -70.93102716,
	"Constellation" : "Mensa ",
	"AMag" : 5.492,
	"key" : 88567,
	"title" : "Mu Mensae"
	},
{
	"Index" : "68689",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Eta Mensae, HIP 22871, SAO 256145, HD 32440, GC 6078, HR 1629, DM CP-75   290, TYC 9173-1001-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Eta Mensae",
	"OType" : "Star",
	"Distance" : "204.42",
	"RA_S" : 73.79667378,
	"DEC_S" : -74.93685357,
	"X" : 536,
	"Y" : 536,
	"Constellation" : "Mensa ",
	"AMag" : 5.63,
	"key" : 88689,
	"title" : "Eta Mensae"
	},
{
	"Index" : "68659",
	"Description" : "Beta Mensae (Beta Men, \u03B2 Mensae, \u03B2 Men) is the third brightest star in the constellation of Mensa. It is a G-type giant with an apparent visual magnitude of approximately 5.302.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Beta Mensae, HIP 23467, SAO 256154, HD 33285, GC 6232, HR 1677, DM CP-71   309, TYC 9169-1591-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Beta Mensae",
	"OType" : "Star",
	"Distance" : "242.48",
	"RA_S" : 75.67915009,
	"DEC_S" : -71.3143001,
	"X" : 570,
	"Y" : 501,
	"Constellation" : "Mensa ",
	"AMag" : 5.405,
	"key" : 88659,
	"title" : "Beta Mensae"
	},
{
	"Index" : "70328",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Gamma Mensae, HIP 25918, SAO 256201, HD 37763, GC 6966, HR 1953, DM CP-76   333, TYC 9378-1692-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Gamma Mensae",
	"OType" : "Star",
	"Distance" : "31.33",
	"RA_S" : 82.97062046,
	"DEC_S" : -76.34097434,
	"X" : 502,
	"Y" : 526,
	"Constellation" : "Mensa ",
	"AMag" : 5.307,
	"key" : 90328,
	"title" : "Gamma Mensae"
	},
{
	"Index" : "70379",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Kappa Mensae, HIP 27566, SAO 256248, HD 40953, GC 7476, HR 2125, DM CP-79   202, TYC 9386-2611-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Kappa Mensae",
	"OType" : "Star",
	"Distance" : "87.38",
	"RA_S" : 87.56993226,
	"DEC_S" : -79.36136177,
	"Constellation" : "Mensa ",
	"AMag" : 5.439,
	"key" : 90379,
	"title" : "Kappa Mensae"
	},
{
	"Index" : "68708",
	"Description" : "Alpha Mensae is the brightest star in the constellation Mensa. At a magnitude of 5.09, it is the dimmest lucida (a constellation\u0027s brightest star) in the sky. It is a main sequence dwarf star only slightly smaller and cooler in temperature than the Sun. Due to its declination, on Earth it is best visible from higher latitudes of the southern hemisphere, yet can also be seen, though low in the sky, from just north of the Equator when near its daily arc\u0027s highest point, the culmination.\r\rAlpha Mensae has a relatively high proper motion across the sky, and it is located about 33 light years distant from the Sun. No planetary companions have yet been discovered around it. It has a red dwarf companion star at a distance of 3.05 arcseconds (a projected separation of roughly 30 AU).",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Alpha Mensae, HIP 29271, SAO 256274, HD 43834, GC 7962, HR 2261, DM CP-74   374, TYC 9176-987-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Alpha Mensae",
	"OType" : "High proper-motion Star",
	"Distance" : "10.2",
	"RA_S" : 92.56030926,
	"DEC_S" : -74.7530456,
	"X" : 492,
	"Y" : 489,
	"Constellation" : "Mensa ",
	"AMag" : 5.151,
	"key" : 88708,
	"title" : "Alpha Mensae"
	},
{
	"Index" : "70384",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Theta Mensae, HIP 33384, SAO 256355, HD 54239, GC 9278, HR 2689, DM CP-79   238, TYC 9388-1630-1",
	"group" : { "key" : "Mensa" },
	"Common" : "Theta Mensae",
	"OType" : "Star",
	"Distance" : "107.93",
	"RA_S" : 104.14364246,
	"DEC_S" : -79.42019279,
	"Constellation" : "Mensa ",
	"AMag" : 5.454,
	"key" : 90384,
	"title" : "Theta Mensae"
	},
{
	"Index" : "56966",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Nu Microscopii, HIP 101477, SAO 230276, HD 195569, GC 28588, HR 7846, DM CD-44 14020, TYC 7962-1389-1",
	"group" : { "backgroundImage" : "images/Alignment/12.png",
		"description" : "Microscopium (pron.: /\u02CCma\u026Akr\u0259\u02C8sk\u0252pi\u0259m/) is a small constellation in the southern sky, defined in the 18th century by Nicolas Louis de Lacaille. Its name is Latin for microscope; it was called this due to its visual similarity to 18th century microscope. Its stars are very faint and hardly visible from most of the non-tropical northern hemisphere.\r\rThe former constellation Neper, representing an auger, may have been located in or near modern-day Microscopium. However, this connection is disputed.\r\rMicroscopium is a small constellation bordered by Capricornus to the north, Piscis Austrinus and Grus to the west, Sagittarius to the east, Indus to the south, and touching on Telescopium to the southeast. The recommended three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027Mic\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 4 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 20h 27.3m and 21h 28.4m, while the declination coordinates are between \u221227.45\u00B0 and \u221245.09\u00B0. Given that its brightest stars are of fifth magnitude, the constellation is invisible to the naked eye in areas with polluted skies.",
		"key" : "Microscopium",
		"grouptype" : "Microscopium",
		"Meaning" : "microscope",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Microscopium",
		"title" : "Microscopium Objects Group" },
	"Common" : "Nu Microscopii",
	"OType" : "Red Giant Branch star",
	"Distance" : "71.68",
	"RA_S" : 308.47946288,
	"DEC_S" : -44.51604942,
	"Constellation" : "Microscopium ",
	"AMag" : 5.228,
	"key" : 76966,
	"title" : "Nu Microscopii"
	},
{
	"Index" : "56976",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "HIP 102497, SAO 212416, HD 197630, GC 28927, HR 7933, DM CD-3913960, TYC 7963-1586-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "HR 7933",
	"OType" : "Star",
	"Distance" : "99.37",
	"RA_S" : 311.58362559,
	"DEC_S" : -39.19926485,
	"Constellation" : "Microscopium ",
	"AMag" : 5.456,
	"key" : 76976,
	"title" : "HR 7933"
	},
{
	"Index" : "57040",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Iota Microscopii, HIP 102693, SAO 230379, HD 197937, GC 28980, HR 7943, DM CD-44 14145, TYC 7975-1347-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Iota Microscopii",
	"OType" : "Star",
	"Distance" : "41",
	"RA_S" : 312.12143928,
	"DEC_S" : -43.98853195,
	"Constellation" : "Microscopium ",
	"AMag" : 5.138,
	"key" : 77040,
	"title" : "Iota Microscopii"
	},
{
	"Index" : "52567",
	"Description" : "Alpha Microscopii (Alpha Mic, \u03B1 Microscopii, \u03B1 Mic) is a G-type giant star in the constellation of Microscopium. It has an apparent visual magnitude which varies between 4.88 and 4.94.\r\rThis star has an optical visual companion, CCDM J20500-3347B, of apparent visual magnitude 10.0 approximately 20.4 arcseconds away at a position angle of 166\u00B0. It has no physical connection to the star described above.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Alpha Microscopii, HIP 102831, SAO 212472, HD 198232, GC 29026, HR 7965, DM CD-34 14660, TYC 7465-1445-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Alpha Microscopii",
	"OType" : "Star",
	"Distance" : "115.07",
	"RA_S" : 312.49202586,
	"DEC_S" : -33.7797206,
	"X" : 373,
	"Y" : 436,
	"Constellation" : "Microscopium ",
	"AMag" : 4.999,
	"key" : 72567,
	"title" : "Alpha Microscopii"
	},
{
	"Index" : "57002",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "HIP 103127, SAO 212522, HD 198716, GC 29127, HR 7987, DM CD-4014078, TYC 7968-239-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "HR 7987",
	"OType" : "Star",
	"Distance" : "122.47",
	"RA_S" : 313.41744157,
	"DEC_S" : -39.80986309,
	"Constellation" : "Microscopium ",
	"AMag" : 5.484,
	"key" : 77002,
	"title" : "HR 7987"
	},
{
	"Index" : "52637",
	"Description" : "Gamma Microscopii (\u03B3 Microscopii, \u03B3 Mic) is the brightest star in the faint southern constellation of Microscopium. It has an apparent visual magnitude of 4.68, which is too dim to be viewed from city skies. The distance to this star has been determined using parallax measurements made during the Hipparcos mission, which place it around 229 light-years (70 parsecs) away with a 2% margin of error.\r\rBased upon a stellar classification of G6 III, this is a G-type giant star. It is a core helium fusing star that is classified as a member of the red clump evolutionary branch, although the metallicity of this star\u2014meaning the abundance of elements other than hydrogen and helium\u2014is anomalously low for a member of this group. The effective temperature of the star\u0027s outer envelope is 5,050 K, giving it the yellow-hued glow typical of G-type stars.\r\rIn the galactic coordinate system, this star has space velocity components of [U, V, W] = [+13.75, +3.47, \u201310.50] km s\u20131. The peculiar velocity of this star, relative to its neighbors, is 1.2 km s\u20131. It has been listed as likely member of the Ursa Major Moving Group of stars that share a similar location and a common trajectory through space. Backwards extrapolation of the motion of \u03B3 Microscopii has shown that approximately 3.8 million years ago, it was only around 6 light-years from the Sun. It would then have had an apparent magnitude of \u22123 and have been brighter than Sirius is now.\r\rGamma Microscopii has a visual companion, CCDM J21013-3215B at an angular separation of 26 arcseconds along a position angle of 94\u00B0, with an apparent visual magnitude of approximately 13.7. Most likely this star is not gravitationally bound to \u03B3 Microscopii, but is merely a line of sight companion.\r\rGamma Microscopii was a later designation of 1 Piscis Austrini.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Gamma Microscopii, HIP 103738, SAO 212636, HD 199951, GC 29331, HR 8039, DM CD-32 16353, TYC 7475-1129-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Gamma Microscopii",
	"OType" : "Star",
	"Distance" : "70.2",
	"RA_S" : 315.32274739,
	"DEC_S" : -32.25776111,
	"X" : 343,
	"Y" : 416,
	"Constellation" : "Microscopium ",
	"AMag" : 4.752,
	"key" : 72637,
	"title" : "Gamma Microscopii"
	},
{
	"Index" : "56989",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Zeta Microscopii, HIP 103882, SAO 212666, HD 200163, GC 29363, HR 8048, DM CD-39 14089, TYC 7965-765-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Zeta Microscopii",
	"OType" : "Star",
	"Distance" : "35.37",
	"RA_S" : 315.74147017,
	"DEC_S" : -38.6314474,
	"Constellation" : "Microscopium ",
	"AMag" : 5.354,
	"key" : 76989,
	"title" : "Zeta Microscopii"
	},
{
	"Index" : "52636",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "2 Piscis Austrini, HIP 104174, SAO 212716, HD 200763, GC 29465, HR 8076, DM CD-32 16398, TYC 7475-1108-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "2 Piscis Austrini",
	"OType" : "Star",
	"Distance" : "100.53",
	"RA_S" : 316.60282649,
	"DEC_S" : -32.34162054,
	"Constellation" : "Microscopium ",
	"AMag" : 5.319,
	"key" : 72636,
	"title" : "2 Piscis Austrini"
	},
{
	"Index" : "57011",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "HIP 104738, SAO 212793, HD 201772, GC 29640, HR 8104, DM CD-3914152, TYC 7970-1275-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "HR 8104",
	"OType" : "High proper-motion Star",
	"Distance" : "32.95",
	"RA_S" : 318.26278122,
	"DEC_S" : -39.4249239,
	"Constellation" : "Microscopium ",
	"AMag" : 5.296,
	"key" : 77011,
	"title" : "HR 8104"
	},
{
	"Index" : "52646",
	"Description" : "Epsilon Microscopii (\u03B5 Mic) is a star in the constellation Microscopium. Its apparent magnitude is 4.72.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Epsilon Microscopii, HIP 105140, SAO 212874, HD 202627, GC 29774, HR 8135, DM CD-32 16498, TYC 7476-923-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Epsilon Microscopii",
	"OType" : "Star",
	"Distance" : "55.85",
	"RA_S" : 319.48452117,
	"DEC_S" : -32.17254439,
	"X" : 297,
	"Y" : 415,
	"Constellation" : "Microscopium ",
	"AMag" : 4.717,
	"key" : 72646,
	"title" : "Epsilon Microscopii"
	},
{
	"Index" : "57091",
	"Description" : "Theta1 Microscopii (\u03B81 Mic) is a star in the constellation Microscopium. Its apparent magnitude is 4.81.",
	"MapNum" : "12",
	"ImageNum" : "12",
	"Desig" : "Theta01 Microscopii, HIP 105382AB, SAO 230644, HD 203006, GC 29854, HR 8151, DM CD-41 14475, TYC 7983-1200-1",
	"group" : { "key" : "Microscopium" },
	"Common" : "Theta1 Microscopii",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "57",
	"RA_S" : 320.19015481,
	"DEC_S" : -40.80950379,
	"X" : 294,
	"Y" : 528,
	"Constellation" : "Microscopium ",
	"AMag" : 4.806,
	"key" : 77091,
	"title" : "Theta1 Microscopii"
	},
{
	"Index" : "36205",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "2 Monocerotis, HIP 28325, SAO 132715, HD 40536, GC 7565, HR 2108, DM BD-09  1285, TYC 5352-933-1",
	"group" : { "backgroundImage" : "images/Alignment/33.png",
		"description" : "Monoceros (Greek: \u039C\u03BF\u03BD\u03CC\u03BA\u03B5\u03C1\u03C9\u03C2) is a faint constellation on the celestial equator. Its name is Greek for unicorn. Its definition is attributed to the 17th-century Dutch cartographer Petrus Plancius. It is bordered by Orion to the west, Gemini to the north, Canis Major to the south and Hydra to the east. Other bordering constellations include Canis Minor, Lepus and Puppis.\r\rMonoceros is a relatively modern constellation. Its first certain appearance was on a globe created by the Dutch cartographer Petrus Plancius in 1612 or 1613 and it was later charted by Jakob Bartsch as Unicornus in his star chart of 1624.\r\rHeinrich Wilhelm Olbers and Ludwig Ideler indicate (according to Richard Hinkley Allen\u0027s allegations) that the constellation may be older, quoting an astrological work from 1564 that mentioned \u0022the second horse between the Twins and the Crab has many stars, but not very bright\u0022; these references may ultimately be due to Michael Scot of the 13th century, but refer to a horse and not a unicorn, and its position does not quite match. Joseph Scaliger is reported to have found Monoceros on an ancient Persian sphere.",
		"key" : "Monoceros",
		"grouptype" : "Monoceros",
		"Meaning" : "unicorn",
		"Family" : "Orion",
		"Origin" : "1613, Plancius",
		"shortTitle" : "Monoceros",
		"title" : "Monoceros Objects Group" },
	"Common" : "2 Monocerotis",
	"OType" : "Spectroscopic binary",
	"Distance" : "87.72",
	"RA_S" : 89.76797057,
	"DEC_S" : -9.55825367,
	"Constellation" : "Monoceros ",
	"AMag" : 5.053,
	"key" : 56205,
	"title" : "2 Monocerotis"
	},
{
	"Index" : "36209",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "3 Monocerotis, HIP 28574A, SAO 151037, HD 40967, GC 7631, HR 2128, DM BD-10  1349, TYC 5353-1318-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "3 Monocerotis",
	"OType" : "Double or multiple star",
	"Distance" : "235.45",
	"RA_S" : 90.46008496,
	"DEC_S" : -10.59793171,
	"Constellation" : "Monoceros ",
	"AMag" : 4.992,
	"key" : 56209,
	"title" : "3 Monocerotis"
	},
{
	"Index" : "32206",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 28744AB, SAO 132793, HD 41335, GC 7691, HR 2142, DM BD-06 1391, TYC 4794-1530-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2142",
	"OType" : "Be Star",
	"Distance" : "403.2258",
	"RA_S" : 91.05625789,
	"DEC_S" : -6.70894165,
	"Constellation" : "Monoceros ",
	"AMag" : 5.222,
	"key" : 52206,
	"title" : "HR 2142"
	},
{
	"Index" : "32146",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 28949, SAO 132841, HD 41692, GC 7750, HR 2154, DM BD-04 1362, TYC 4790-1829-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2154",
	"OType" : "Star",
	"Distance" : "320",
	"RA_S" : 91.66140458,
	"DEC_S" : -4.19383698,
	"Constellation" : "Monoceros ",
	"AMag" : 5.341,
	"key" : 52146,
	"title" : "HR 2154"
	},
{
	"Index" : "32217",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 29417, SAO 132944, HD 42690, GC 7899, HR 2205, DM BD-06 1446, TYC 4795-1771-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2205",
	"OType" : "Star",
	"Distance" : "362.05",
	"RA_S" : 92.96589403,
	"DEC_S" : -6.55028685,
	"Constellation" : "Monoceros ",
	"AMag" : 5.007,
	"key" : 52217,
	"title" : "HR 2205"
	},
{
	"Index" : "32215",
	"Description" : "Gamma Monocerotis is a star in the constellation of Monocerotis.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "5 Monocerotis, Gamma Monocerotis, HIP 29651, SAO 133012, HD 43232, GC 7986, HR 2227, DM BD-06  1469, TYC 4795-1769-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Tempestris",
	"OType" : "Star",
	"Distance" : "152.52",
	"RA_S" : 93.71388533,
	"DEC_S" : -6.27477334,
	"X" : 392,
	"Y" : 484,
	"Constellation" : "Monoceros ",
	"AMag" : 4.117,
	"key" : 52215,
	"title" : "Tempestris"
	},
{
	"Index" : "36339",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 29996, SAO 133091, HD 43993, GC 8107, HR 2267, DM BD-09 1411, TYC 5367-1742-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2267",
	"OType" : "Star",
	"Distance" : "143.79",
	"RA_S" : 94.71076109,
	"DEC_S" : -9.39001814,
	"Constellation" : "Monoceros ",
	"AMag" : 5.491,
	"key" : 56339,
	"title" : "HR 2267"
	},
{
	"Index" : "36300",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "7 Monocerotis, HIP 30073, SAO 133114, HD 44112, GC 8132, HR 2273, DM BD-07  1373, TYC 5363-2397-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "7 Monocerotis",
	"OType" : "Double or multiple star",
	"Distance" : "265.46",
	"RA_S" : 94.92832467,
	"DEC_S" : -7.8229084,
	"Constellation" : "Monoceros ",
	"AMag" : 5.221,
	"key" : 56300,
	"title" : "7 Monocerotis"
	},
{
	"Index" : "3434",
	"Description" : "Epsilon Monocerotis is a star in the constellation of Monocerotis.\r\rIts location is guide for sky navigation toward Rosette nebula\r\rRight Ascension 6 hours 28 minutes 8 seconds, Declination 4 degrees 36 minutes, Magnitude 4.5, 6.5 Separation 13,4\u0022, Position Angle 27 degrees\r\rWhite giant (A)( spectral classification ), Catalogue number: 8 Mon, Brightness + 4.4, Distance in light years is 130 light years\r\rBayer classification - \u03B5, Flamsteed classification - 8, Henry Draper Catalogue(HD)-44769, Smithsonian Astronomical Observatory Star Catalogue (SAO)-113810,FK5 -244, RA J2000 6 23 46.1,DEC J2000 +4 35\u0027 34\u0022, Proper motion in RA arcsec/y -0.018, Proper motion in DEC arcsec/y -0.011, parallax arcsec -0.025,mag 4.44, MK spectral class A5IV",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "8 Monocerotis, Epsilon Monocerotis, HIP 30419A, SAO 113810, HD 44769, GC 8240, HR 2298, DM BD+04  1236, TYC 141-2452-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Epsilon Monocerotis",
	"OType" : "Star",
	"Distance" : "37.44",
	"RA_S" : 95.94203484,
	"DEC_S" : 4.59286794,
	"X" : 363,
	"Y" : 342,
	"Constellation" : "Monoceros ",
	"AMag" : 4.423,
	"key" : 23434,
	"title" : "Epsilon Monocerotis"
	},
{
	"Index" : "2689",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "77 Orionis, HIP 30717, SAO 113905, HD 45416, GC 8355, HR 2334, DM BD+00  1426, TYC 133-2047-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "77 Orionis",
	"OType" : "Star",
	"Distance" : "257.23",
	"RA_S" : 96.80733367,
	"Constellation" : "Monoceros ",
	"AMag" : 5.318,
	"key" : 22689,
	"title" : "77 Orionis"
	},
{
	"Index" : "32193",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "10 Monocerotis, HIP 30772, SAO 133290, HD 45546, GC 8378, HR 2344, DM BD-04  1526, TYC 4793-2716-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "10 Monocerotis",
	"OType" : "Variable Star",
	"Distance" : "321.89",
	"RA_S" : 96.98987238,
	"DEC_S" : -4.76215246,
	"Constellation" : "Monoceros ",
	"AMag" : 5.011,
	"key" : 52193,
	"title" : "10 Monocerotis"
	},
{
	"Index" : "32244",
	"Description" : "Beta Monocerotis (Beta Mon, \u03B2 Monocerotis, \u03B2 Mon) is a triple star system in the constellation of Monoceros. To the naked eye, it appears as a single star with an apparent visual magnitude of approximately 3.74, making it the brightest visible star in the constellation. A telescope shows a curved line of three pale blue stars (or pale yellow stars, depending on your scope\u0027s focus). The star system consists of three Be stars, \u03B2 Monocerotis A, \u03B2 Monocerotis B, and \u03B2 Monocerotis C. There is also an additional visual companion star that is probably not physically close to the other three stars.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "11 Monocerotis, Beta Monocerotis, HIP 30867A, SAO 133316, HD 45725, GC 8412, HR 2356, DM BD-06  1574, TYC 4797-1880-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Beta Monocerotis",
	"OType" : "Be Star",
	"Distance" : "207.4689",
	"RA_S" : 97.20445713,
	"DEC_S" : -7.03305836,
	"X" : 347,
	"Y" : 494,
	"Constellation" : "Monoceros ",
	"AMag" : 4.616,
	"key" : 52244,
	"title" : "Beta Monocerotis"
	},
{
	"Index" : "32245",
	"Description" : "Beta Monocerotis (Beta Mon, \u03B2 Monocerotis, \u03B2 Mon) is a triple star system in the constellation of Monoceros. To the naked eye, it appears as a single star with an apparent visual magnitude of approximately 3.74, making it the brightest visible star in the constellation. A telescope shows a curved line of three pale blue stars (or pale yellow stars, depending on your scope\u0027s focus). The star system consists of three Be stars, \u03B2 Monocerotis A, \u03B2 Monocerotis B, and \u03B2 Monocerotis C. There is also an additional visual companion star that is probably not physically close to the other three stars.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "11 Monocerotis, Beta Monocerotis, HIP 30867B, SAO 133317, HD 45726, GC 8413, HR 2357, DM BD-06  1575A, TYC 4797-1881-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Beta Monocerotis",
	"OType" : "Star",
	"Distance" : "207.4689",
	"RA_S" : 97.20593766,
	"DEC_S" : -7.0344483,
	"X" : 347,
	"Y" : 494,
	"Constellation" : "Monoceros ",
	"AMag" : 5.004,
	"key" : 52245,
	"title" : "Beta Monocerotis"
	},
{
	"Index" : "32246",
	"Description" : "Beta Monocerotis (Beta Mon, \u03B2 Monocerotis, \u03B2 Mon) is a triple star system in the constellation of Monoceros. To the naked eye, it appears as a single star with an apparent visual magnitude of approximately 3.74, making it the brightest visible star in the constellation. A telescope shows a curved line of three pale blue stars (or pale yellow stars, depending on your scope\u0027s focus). The star system consists of three Be stars, \u03B2 Monocerotis A, \u03B2 Monocerotis B, and \u03B2 Monocerotis C. There is also an additional visual companion star that is probably not physically close to the other three stars.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "11 Monocerotis, Beta Monocerotis, HIP 30867C, HD 45727, HR 2358, DM BD-06  1575B, TYC 4797-1882-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Beta Monocerotis",
	"OType" : "Emission-line Star",
	"Distance" : "207.4689",
	"RA_S" : 97.2067372,
	"DEC_S" : -7.0346443,
	"X" : 347,
	"Y" : 494,
	"Constellation" : "Monoceros ",
	"AMag" : 5.319,
	"key" : 52246,
	"title" : "Beta Monocerotis"
	},
{
	"Index" : "52153",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 31119, SAO 95788, HD 46089, GC 8468, HR 2375, DM BD+11 1209, TYC 741-1572-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2375",
	"OType" : "Star",
	"Distance" : "63.61",
	"RA_S" : 97.9512484,
	"DEC_S" : 11.54441004,
	"Constellation" : "Monoceros ",
	"AMag" : 5.234,
	"key" : 72153,
	"title" : "HR 2375"
	},
{
	"Index" : "4814",
	"Description" : "13 Monocerotis (13 Mon) is a star in the constellation Monoceros. Its apparent magnitude is 4.50.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "13 Monocerotis, HIP 31216, SAO 114034, HD 46300, GC 8506, HR 2385, DM BD+07  1337, TYC 158-3394-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "13 Monocerotis",
	"OType" : "Star in Nebula",
	"RA_S" : 98.22594981,
	"DEC_S" : 7.33296586,
	"X" : 334,
	"Y" : 306,
	"Constellation" : "Monoceros ",
	"AMag" : 4.486,
	"key" : 24814,
	"title" : "13 Monocerotis"
	},
{
	"Index" : "32253",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 31278, SAO 133404, HD 46487, GC 8527, HR 2395, DM BD-01 1274, TYC 4798-1735-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2395",
	"OType" : "Star",
	"Distance" : "169.44",
	"RA_S" : 98.40800518,
	"DEC_S" : -1.2201571,
	"Constellation" : "Monoceros ",
	"AMag" : 5.056,
	"key" : 52253,
	"title" : "HR 2395"
	},
{
	"Index" : "32340",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 31583, SAO 133469, HD 47054, GC 8609, HR 2418, DM BD-05 1710, TYC 4806-3516-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2418",
	"OType" : "Be Star",
	"Distance" : "229.62",
	"RA_S" : 99.14721397,
	"DEC_S" : -5.21114187,
	"Constellation" : "Monoceros ",
	"AMag" : 5.498,
	"key" : 52340,
	"title" : "HR 2418"
	},
{
	"Index" : "52851",
	"Description" : "S Monocerotis, also known as 15 Monocerotis, is a massive variable star system located in the constellation Monoceros. It is a spectroscopic binary system with an orbital period of 25 years. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is a type O main sequence dwarf with a stellar classification of O7Ve, and is about 8,500 times as luminous as the Sun, while varying in between magnitude 4.2 and 4.6. The star lies at the base of the Christmas Tree Cluster in NGC 2264.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "15 Monocerotis, S Monocerotis, HIP 31978B, SAO 114258, HD 47839, GC 8720, HR 2456, DM BD+10  1220, TYC 750-1880-2",
	"group" : { "key" : "Monoceros" },
	"Common" : "S Monocerotis",
	"OType" : "Star",
	"Distance" : "275.14",
	"RA_S" : 100.244025,
	"DEC_S" : 9.895056,
	"X" : 309,
	"Y" : 272,
	"Constellation" : "Monoceros ",
	"AMag" : 7.788,
	"key" : 72851,
	"title" : "S Monocerotis"
	},
{
	"Index" : "52850",
	"Description" : "S Monocerotis, also known as 15 Monocerotis, is a massive variable star system located in the constellation Monoceros. It is a spectroscopic binary system with an orbital period of 25 years. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is a type O main sequence dwarf with a stellar classification of O7Ve, and is about 8,500 times as luminous as the Sun, while varying in between magnitude 4.2 and 4.6. The star lies at the base of the Christmas Tree Cluster in NGC 2264.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "15 Monocerotis, S Monocerotis, HIP 31978A, SAO 114258, HD 47839, GC 8720, HR 2456, DM BD+10  1220, TYC 750-1880-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "S Monocerotis",
	"OType" : "Double or multiple star",
	"Distance" : "275.14",
	"RA_S" : 100.24440064,
	"DEC_S" : 9.89575245,
	"X" : 309,
	"Y" : 272,
	"Constellation" : "Monoceros ",
	"AMag" : 4.642,
	"key" : 72850,
	"title" : "S Monocerotis"
	},
{
	"Index" : "36435",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 32064, SAO 133585, HD 48217, GC 8756, HR 2469, DM BD-09 1601, TYC 5378-2317-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2469",
	"OType" : "Star",
	"Distance" : "105.44",
	"RA_S" : 100.48494144,
	"DEC_S" : -9.16753313,
	"Constellation" : "Monoceros ",
	"AMag" : 5.376,
	"key" : 56435,
	"title" : "HR 2469"
	},
{
	"Index" : "52616",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "17 Monocerotis, HIP 32533, SAO 114410, HD 49161, GC 8880, HR 2503, DM BD+08  1496, TYC 747-2464-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "17 Monocerotis",
	"OType" : "Star",
	"Distance" : "150.8",
	"RA_S" : 101.83262719,
	"DEC_S" : 8.03725286,
	"Constellation" : "Monoceros ",
	"AMag" : 4.923,
	"key" : 72616,
	"title" : "17 Monocerotis"
	},
{
	"Index" : "36445",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 32558, SAO 133679, HD 49331, GC 8891, HR 2508, DM BD-08 1558, TYC 5379-2816-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Lalande 13100 (HR 2508)",
	"OType" : "Variable Star",
	"Distance" : "424.87",
	"RA_S" : 101.90509055,
	"DEC_S" : -8.99849968,
	"Constellation" : "Monoceros ",
	"AMag" : 5.293,
	"key" : 56445,
	"title" : "Lalande 13100 (HR 2508)"
	},
{
	"Index" : "4326",
	"Description" : "18 Monocerotis (18 Mon) is a star in the constellation Monoceros. Its apparent magnitude is 4.48.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "18 Monocerotis, HIP 32578, SAO 114428, HD 49293, GC 8892, HR 2506, DM BD+02  1397, TYC 152-2580-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "18 Monocerotis",
	"OType" : "Spectroscopic binary",
	"Distance" : "112.59",
	"RA_S" : 101.96520108,
	"DEC_S" : 2.41216003,
	"X" : 284,
	"Y" : 370,
	"Constellation" : "Monoceros ",
	"AMag" : 4.593,
	"key" : 24326,
	"title" : "18 Monocerotis"
	},
{
	"Index" : "32287",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 33184, SAO 133870, HD 50747, GC 9052, HR 2572, DM BD-00 1487, TYC 4801-4454-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2572",
	"OType" : "Star",
	"Distance" : "166",
	"RA_S" : 103.6027571,
	"DEC_S" : -1.1269843,
	"Constellation" : "Monoceros ",
	"AMag" : 5.457,
	"key" : 52287,
	"title" : "HR 2572"
	},
{
	"Index" : "32573",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 33878, SAO 134076, HD 52666, GC 9269, HR 2639, DM BD-05 1926, TYC 4826-3284-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "HR 2639",
	"OType" : "Variable Star",
	"Distance" : "174.63",
	"RA_S" : 105.48493721,
	"DEC_S" : -5.72205904,
	"Constellation" : "Monoceros ",
	"AMag" : 5.398,
	"key" : 52573,
	"title" : "HR 2639"
	},
{
	"Index" : "32516",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "19 Monocerotis, HIP 33971, SAO 134106, HD 52918, GC 9293, HR 2648, DM BD-04  1788, TYC 4822-3679-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "19 Monocerotis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "370.14",
	"RA_S" : 105.72823613,
	"DEC_S" : -4.23923269,
	"Constellation" : "Monoceros ",
	"AMag" : 4.937,
	"key" : 52516,
	"title" : "19 Monocerotis"
	},
{
	"Index" : "32535",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "20 Monocerotis, HIP 34622, SAO 134282, HD 54810, GC 9477, HR 2701, DM BD-04  1840, TYC 4823-4552-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "20 Monocerotis",
	"OType" : "High proper-motion Star",
	"Distance" : "62.17",
	"RA_S" : 107.55700602,
	"DEC_S" : -4.23710687,
	"Constellation" : "Monoceros ",
	"AMag" : 5.026,
	"key" : 52535,
	"title" : "20 Monocerotis"
	},
{
	"Index" : "32434",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "21 Monocerotis, HIP 34724, SAO 134316, HD 55057, GC 9505, HR 2707, DM BD-00  1634, TYC 4815-3815-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "21 Monocerotis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "87.13",
	"RA_S" : 107.84839858,
	"Constellation" : "Monoceros ",
	"AMag" : 5.464,
	"key" : 52434,
	"title" : "21 Monocerotis"
	},
{
	"Index" : "32435",
	"Description" : "Delta Monocerotis (\u03B4 Mon) is a star in the constellation Monoceros. Its apparent magnitude is 4.15.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "22 Monocerotis, Delta Monocerotis, HIP 34769, SAO 134330, HD 55185, GC 9518, HR 2714, DM BD-00  1636, TYC 4815-3816-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Delta Monocerotis",
	"OType" : "Star",
	"Distance" : "117.73",
	"RA_S" : 107.96608397,
	"X" : 206,
	"Y" : 409,
	"Constellation" : "Monoceros ",
	"AMag" : 4.136,
	"key" : 52435,
	"title" : "Delta Monocerotis"
	},
{
	"Index" : "32666",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "25 Monocerotis, HIP 37088, SAO 134899, HD 61064, GC 10217, HR 2927, DM BD-03  1979, TYC 4838-3344-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "25 Monocerotis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "67.49",
	"RA_S" : 114.31954575,
	"DEC_S" : -4.11098095,
	"Constellation" : "Monoceros ",
	"AMag" : 5.183,
	"key" : 52666,
	"title" : "25 Monocerotis"
	},
{
	"Index" : "36847",
	"Description" : "Alpha Monocerotis (\u03B1 Mon, \u03B1 Monocerotis) is the Bayer designation for a star in the equatorial constellation of Monoceros.\r\rAlpha Monocerotis is the brightest star in the constellation Monoceros ,It is nearing the end of its life. Internal changes have caused the star to puff up gas.\r\rIt is a giant star with a stellar classification of K0 III and is of apparent magnitude 3.93. It is approximately 144 light years from Earth.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "26 Monocerotis, Alpha Monocerotis, HIP 37447, SAO 134986, HD 61935, GC 10345, HR 2970, DM BD-09  2172, TYC 5414-2746-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Alpha Monocerotis",
	"OType" : "Star",
	"Distance" : "45.31",
	"RA_S" : 115.31180305,
	"DEC_S" : -9.55112894,
	"X" : 115,
	"Y" : 533,
	"Constellation" : "Monoceros ",
	"AMag" : 4.039,
	"key" : 56847,
	"title" : "Alpha Monocerotis"
	},
{
	"Index" : "32658",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "27 Monocerotis, HIP 39079, SAO 135345, HD 65695, GC 10811, HR 3122, DM BD-03  2157, TYC 4837-3335-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "27 Monocerotis",
	"OType" : "Star",
	"Distance" : "84.19",
	"RA_S" : 119.93396926,
	"DEC_S" : -3.67958251,
	"Constellation" : "Monoceros ",
	"AMag" : 5.069,
	"key" : 52658,
	"title" : "27 Monocerotis"
	},
{
	"Index" : "32740",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "28 Monocerotis, HIP 39211, SAO 135380, HD 65953, GC 10870, HR 3141, DM BD-00  1882, TYC 4846-2652-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "28 Monocerotis",
	"OType" : "Rotationally variable Star",
	"Distance" : "137.65",
	"RA_S" : 120.30556612,
	"DEC_S" : -1.39261026,
	"Constellation" : "Monoceros ",
	"AMag" : 4.853,
	"key" : 52740,
	"title" : "28 Monocerotis"
	},
{
	"Index" : "32783",
	"Description" : "Zeta Monocerotis (\u03B6 Mon) is a star in the constellation Monoceros. Its apparent magnitude is 4.37.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "29 Monocerotis, Zeta Monocerotis, HIP 39863, SAO 135551, HD 67594, GC 11051, HR 3188, DM BD-02  2450, TYC 4851-2878-1",
	"group" : { "key" : "Monoceros" },
	"Common" : "Zeta Monocerotis",
	"OType" : "Star",
	"Distance" : "321.71",
	"RA_S" : 122.14853588,
	"DEC_S" : -2.98378544,
	"X" : 22,
	"Y" : 444,
	"Constellation" : "Monoceros ",
	"AMag" : 4.456,
	"key" : 52783,
	"title" : "Zeta Monocerotis"
	},
{
	"Index" : "66557",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 55597A, SAO 251382, HD 99103, GC 15648, TYC 8967-1170-1",
	"group" : { "backgroundImage" : "images/Alignment/15.png",
		"description" : "Musca (Latin: fly) is one of the minor southern constellations. The constellation was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Petrus Plancius and Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rMusca, under its original name Apis \u2013 the Bee, was introduced in the late 16th century by Isaac Bautista to fill the previously uncharted area around the southern pole and to provide nourishment for the nearby constellation Chamaeleon (17th-century celestial maps clearly show the chameleon\u0027s tongue trying to catch the insect). In 1752 Nicolas Louis de Lacaille renamed it to Musca Australis, the Southern Fly \u2013 Australis, since it counterparted the now discarded constellation of Musca Borealis composed of a few stars in Aries, and to avoid confusion with Apus. Today the name is simply Musca.",
		"key" : "Musca",
		"grouptype" : "Musca",
		"Meaning" : "fly",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Musca",
		"title" : "Musca Objects Group" },
	"Common" : "HR 4401",
	"OType" : "Star",
	"Distance" : "123.43",
	"RA_S" : 170.83902603,
	"DEC_S" : -64.95464259,
	"Constellation" : "Musca ",
	"AMag" : 5.37,
	"key" : 86557,
	"title" : "HR 4401"
	},
{
	"Index" : "66811",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 56862AS, SAO 251522, HD 101379J, GC 16004, HR 4492, DM CP-64 1685, TYC 8980-2292-1",
	"group" : { "key" : "Musca" },
	"Common" : "*  12 Mus",
	"OType" : "Eclipsing binary",
	"Distance" : "152.39",
	"RA_S" : 174.87329169,
	"DEC_S" : -65.39776073,
	"Constellation" : "Musca ",
	"AMag" : 5.181,
	"key" : 86811,
	"title" : "*  12 Mus"
	},
{
	"Index" : "66885",
	"Description" : "Lambda Muscae (\u03BB Mus, \u03BB Muscae), often catalogued HD 102249 or HIP 57363, is the fourth brightest star in the southern hemisphere constellation of Musca (the Fly). Lambda Muscae visibly makes up the far end of the tail of the visual Musca constellation. It is a star in a dual system according to studies, and one of the stars catalogued in astronomer Johann Bayer\u0027s 1603 publications Uranometria. Lambda Muscae more recently has been recorded as having a stellar classification of A7III. Thus, Lambda Muscae has a white tint and burns significantly hotter than our own sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Lambda Muscae, HIP 57363, SAO 251575, HD 102249, GC 16131, HR 4520, DM CP-66  1640, TYC 8985-3045-1",
	"group" : { "key" : "Musca" },
	"Common" : "Lambda Muscae",
	"OType" : "Star",
	"Distance" : "38.98",
	"RA_S" : 176.40176103,
	"DEC_S" : -66.72876145,
	"X" : 464,
	"Y" : 528,
	"Constellation" : "Musca ",
	"AMag" : 3.638,
	"key" : 86885,
	"title" : "Lambda Muscae"
	},
{
	"Index" : "66886",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Mu Muscae, HIP 57581, SAO 251597, HD 102584, GC 16176, HR 4530, DM CP-66  1649, TYC 8985-3046-1",
	"group" : { "key" : "Musca" },
	"Common" : "Mu Muscae",
	"OType" : "Long-period variable star",
	"Distance" : "131.65",
	"RA_S" : 177.06056315,
	"DEC_S" : -66.81490926,
	"Constellation" : "Musca ",
	"AMag" : 4.915,
	"key" : 86886,
	"title" : "Mu Muscae"
	},
{
	"Index" : "69226",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57696, SAO 251604, HD 102839, GC 16206, HR 4538, DM CP-69 1595, TYC 9230-2344-1",
	"group" : { "key" : "Musca" },
	"Common" : "HR 4538",
	"OType" : "Star",
	"Distance" : "289.4",
	"RA_S" : 177.48588606,
	"DEC_S" : -70.22579164,
	"Constellation" : "Musca ",
	"AMag" : 5.122,
	"key" : 89226,
	"title" : "HR 4538"
	},
{
	"Index" : "66823",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 57851A, SAO 251617, HD 103079, GC 16241, HR 4549, DM CP-64 1724, TYC 8981-4411-1",
	"group" : { "key" : "Musca" },
	"Common" : "HR  4549",
	"OType" : "Star",
	"Distance" : "110.75",
	"RA_S" : 177.96349455,
	"DEC_S" : -65.20591736,
	"Constellation" : "Musca ",
	"AMag" : 4.968,
	"key" : 86823,
	"title" : "HR  4549"
	},
{
	"Index" : "69176",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 58884AB, SAO 251720, HD 104878, GC 16493, HR 4604, DM CP-67 1896, TYC 9227-1544-1",
	"group" : { "key" : "Musca" },
	"Common" : "HR 4604",
	"OType" : "Star",
	"Distance" : "106.28",
	"RA_S" : 181.16204047,
	"DEC_S" : -68.32892447,
	"Constellation" : "Musca ",
	"AMag" : 5.37,
	"key" : 89176,
	"title" : "HR 4604"
	},
{
	"Index" : "70539",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 59151, SAO 256905, HD 105340, GC 16572, HR 4617, DM CP-74  880, TYC 9412-2399-1",
	"group" : { "key" : "Musca" },
	"Common" : "HR 4617",
	"OType" : "Star",
	"Distance" : "130.07",
	"RA_S" : 181.9578334,
	"DEC_S" : -75.36702124,
	"Constellation" : "Musca ",
	"AMag" : 5.311,
	"key" : 90539,
	"title" : "HR 4617"
	},
{
	"Index" : "69188",
	"Description" : "Epsilon Muscae (\u03B5 Mus) is a star in the constellation Musca. Its apparent magnitude is 4.11.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Epsilon Muscae, HIP 59929, SAO 251830, HD 106849, GC 16764, HR 4671, DM CP-67  1931, TYC 9227-2705-1",
	"group" : { "key" : "Musca" },
	"Common" : "Epsilon Muscae",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "92.39",
	"RA_S" : 184.39282557,
	"DEC_S" : -67.96073518,
	"X" : 420,
	"Y" : 534,
	"Constellation" : "Musca ",
	"AMag" : 4.332,
	"key" : 89188,
	"title" : "Epsilon Muscae"
	},
{
	"Index" : "69179",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Zeta02 Muscae, HIP 60320AC, SAO 251866, HD 107566, GC 16857, HR 4703, DM CP-66  1747, TYC 9227-1699-1",
	"group" : { "key" : "Musca" },
	"Common" : "Zeta02 Muscae",
	"OType" : "Star",
	"Distance" : "100.97",
	"RA_S" : 185.53061206,
	"DEC_S" : -67.5221065,
	"Constellation" : "Musca ",
	"AMag" : 5.17,
	"key" : 89179,
	"title" : "Zeta02 Muscae"
	},
{
	"Index" : "69293",
	"Description" : "Gamma Muscae is a star in the southern circumpolar constellation of Musca, or the Fly. As a Bayer object in the constellation it is one of the brightest, and thus most visible, stars.\r\rThis star is a proper motion member of the Lower-Centaurus Crux sub-group in the Scorpius-Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Gamma Muscae, HIP 61199, SAO 256955, HD 109026, GC 17086, HR 4773, DM CP-71  1336, TYC 9236-2907-1",
	"group" : { "key" : "Musca" },
	"Common" : "Gamma Muscae",
	"OType" : "Pulsating variable Star",
	"Distance" : "99.58",
	"RA_S" : 188.11673226,
	"DEC_S" : -72.13298676,
	"X" : 393,
	"Y" : 584,
	"Constellation" : "Musca ",
	"AMag" : 3.804,
	"key" : 89293,
	"title" : "Gamma Muscae"
	},
{
	"Index" : "69200",
	"Description" : "Alpha Muscae (\u03B1 Muscae, \u03B1 Mus) is a star in the southern circumpolar constellation of Musca. With an apparent visual magnitude of +2.7, it is the brightest star in the constellation. The distance to this star has been determined using parallax measurements, giving an estimate of about 315 light-years (97 parsecs) from Earth.\r\rWith a stellar classification of B2 IV-V, this star appears to be in the process of evolving away from the main sequence of stars like the Sun and turning a subgiant star, as the supply of hydrogen at its core becomes exhausted. It is larger than the Sun, with nearly nine times the mass and almost five times the radius. This star is radiating around 4,000 times as much luminosity as the Sun from its outer atmosphere at an effective temperature of 21,400 K, giving it the blue-white hue of a B-type star.\r\rAlpha Muscae appears to be a Beta Cephei variable star. Telting et al. (2006) report it as a Beta Cephei with a high degree of confidence, although Stankov and Handler (2005) listed it as a poor or rejected candidate in their Catalog of Galactic \u03B2 Cephei Stars. It is rotating rapidly with a projected rotational velocity of 114 km s\u20131 and has an estimated age of about 18 million years.\r\rThis star is a proper motion member of the Lower-Centaurus Crux sub-group in the Scorpius-Centaurus OB association, the nearest such association of co-moving massive stars to the Sun. Alpha Muscae has a peculiar velocity of 10 km s\u22121, which, while high, is not enough for it to be considered a runaway star.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Alpha Muscae, HIP 61585, SAO 251974, HD 109668, GC 17179, HR 4798, DM CP-68  1702, TYC 9228-3049-1",
	"group" : { "key" : "Musca" },
	"Common" : "Alpha Muscae",
	"OType" : "Double or multiple star",
	"Distance" : "96.7",
	"RA_S" : 189.2959858,
	"DEC_S" : -69.13561311,
	"X" : 394,
	"Y" : 545,
	"Constellation" : "Musca ",
	"AMag" : 2.622,
	"key" : 89200,
	"title" : "Alpha Muscae"
	},
{
	"Index" : "69198",
	"Description" : "Beta Muscae (\u03B2 Muscae, \u03B2 Mus) is a binary star in the southern circumpolar constellation of Musca. With a combined apparent visual magnitude of 3.07, it is the second brightest star (or star system) in the constellation. Judging by the parallax results, it is located at a distance of roughly 330\u2013350 light-years (100\u2013110 parsecs) from the Earth.\r\rThis is a binary star system with a period of about 194 years at an orbital eccentricity of 0.6. As of 2007, the two stars had an angular separation of 1.206 arcseconds at a position angle of 35\u00B0. The components are main sequence stars of similar size and appearance. The primary component, \u03B2 Muscae A, has an apparent magnitude of 3.51, a stellar classification of B2 V, and about 7.35 times the Sun\u0027s mass. The secondary component, \u03B2 Muscae B, has an apparent magnitude of 4.01, a stellar classification of B3 V, and is about 6.40 times the mass of the Sun.\r\rThis is a confirmed member of the Scorpius-Centaurus Association, which is a group of stars with similar ages, locations, and trajectories through space, implying that they formed together in the same molecular cloud. Beta Muscae is considered a runaway star system as it has a high peculiar velocity of 43.9 km s\u20131 relative to the normal galactic rotation. Runaway stars can be produced through several means, such as through an encounter with another binary star system. Binary systems form a relatively small fraction of the total population of runaway stars.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Beta Muscae, HIP 62322A, SAO 252019, HD 110879, GC 17348, HR 4844, DM CP-67  2064, TYC 9228-3047-1",
	"group" : { "key" : "Musca" },
	"Common" : "Beta Muscae",
	"OType" : "Double or multiple star",
	"Distance" : "104.48",
	"RA_S" : 191.57001709,
	"DEC_S" : -68.10811567,
	"X" : 385,
	"Y" : 531,
	"Constellation" : "Musca ",
	"AMag" : 3.518,
	"key" : 89198,
	"title" : "Beta Muscae"
	},
{
	"Index" : "69199",
	"Description" : "Beta Muscae (\u03B2 Muscae, \u03B2 Mus) is a binary star in the southern circumpolar constellation of Musca. With a combined apparent visual magnitude of 3.07, it is the second brightest star (or star system) in the constellation. Judging by the parallax results, it is located at a distance of roughly 330\u2013350 light-years (100\u2013110 parsecs) from the Earth.\r\rThis is a binary star system with a period of about 194 years at an orbital eccentricity of 0.6. As of 2007, the two stars had an angular separation of 1.206 arcseconds at a position angle of 35\u00B0. The components are main sequence stars of similar size and appearance. The primary component, \u03B2 Muscae A, has an apparent magnitude of 3.51, a stellar classification of B2 V, and about 7.35 times the Sun\u0027s mass. The secondary component, \u03B2 Muscae B, has an apparent magnitude of 4.01, a stellar classification of B3 V, and is about 6.40 times the mass of the Sun.\r\rThis is a confirmed member of the Scorpius-Centaurus Association, which is a group of stars with similar ages, locations, and trajectories through space, implying that they formed together in the same molecular cloud. Beta Muscae is considered a runaway star system as it has a high peculiar velocity of 43.9 km s\u20131 relative to the normal galactic rotation. Runaway stars can be produced through several means, such as through an encounter with another binary star system. Binary systems form a relatively small fraction of the total population of runaway stars.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Beta Muscae, HIP 62322B, SAO 252019, HD 110879, GC 17348, HR 4844, DM CP-67  2064, TYC 9228-3047-2",
	"group" : { "key" : "Musca" },
	"Common" : "Beta Muscae",
	"OType" : "Double or multiple star",
	"Distance" : "104.48",
	"RA_S" : 191.57001709,
	"DEC_S" : -68.10811567,
	"X" : 385,
	"Y" : 531,
	"Constellation" : "Musca ",
	"AMag" : 3.04,
	"key" : 89199,
	"title" : "Beta Muscae"
	},
{
	"Index" : "69422",
	"Description" : "Delta Muscae (\u03B4 Mus, \u03B4 Muscae), often catalogued as HD 112985, is a spectroscopic binary star system and the closest to the Earth in the southern hemisphere constellation of Musca (the Fly) at a distance of approximately 27.8 parsecs (91.0 light years). The main star is classified as a giant star with an orange tint. It is one of the stars given a Bayer designation by astronomer Johann Bayer. It was recorded in Bayer\u0027s 1603 publication Uranometria. In addition it is one of the main stars used in the visual formation of the Musca constellation.",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Delta Muscae, HIP 63613, SAO 257000, HD 112985, GC 17672, HR 4923, DM CP-70  1548, TYC 9249-2380-1",
	"group" : { "key" : "Musca" },
	"Common" : "Delta Muscae",
	"OType" : "Spectroscopic binary",
	"Distance" : "27.87",
	"RA_S" : 195.56771577,
	"DEC_S" : -71.54885423,
	"X" : 363,
	"Y" : 575,
	"Constellation" : "Musca ",
	"AMag" : 3.736,
	"key" : 89422,
	"title" : "Delta Muscae"
	},
{
	"Index" : "69335",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Eta Muscae, HIP 64661, SAO 252224, HD 114911A, GC 17927, HR 4993, DM CP-67  2224, TYC 9242-1816-1",
	"group" : { "key" : "Musca" },
	"Common" : "Eta Muscae",
	"OType" : "Star",
	"Distance" : "117.3",
	"RA_S" : 198.81225576,
	"DEC_S" : -67.89458602,
	"Constellation" : "Musca ",
	"AMag" : 4.765,
	"key" : 89335,
	"title" : "Eta Muscae"
	},
{
	"Index" : "67107",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "HIP 64820, SAO 252240, HD 115211, GC 17959, HR 5002, DM CP-66 2142, TYC 9002-2135-1",
	"group" : { "key" : "Musca" },
	"Common" : "HR 5002",
	"OType" : "Variable Star",
	"Distance" : "362.65",
	"RA_S" : 199.30421545,
	"DEC_S" : -66.78343773,
	"Constellation" : "Musca ",
	"AMag" : 5.021,
	"key" : 87107,
	"title" : "HR 5002"
	},
{
	"Index" : "69463",
	"MapNum" : "15",
	"ImageNum" : "15",
	"Desig" : "Iota01 Muscae, HIP 65468, SAO 257041, HD 116244, GC 18116, HR 5042, DM CP-74  1057, TYC 9254-2970-1",
	"group" : { "key" : "Musca" },
	"Common" : "Iota01 Muscae",
	"OType" : "Star",
	"Distance" : "67.78",
	"RA_S" : 201.27966241,
	"DEC_S" : -74.88781707,
	"Constellation" : "Musca ",
	"AMag" : 5.163,
	"key" : 89463,
	"title" : "Iota01 Muscae"
	},
{
	"Index" : "60174",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 76618, SAO 242793, HD 139129, GC 21007, HR 5798, DM CD-51 9324, TYC 8308-2515-1",
	"group" : { "backgroundImage" : "images/Alignment/03.png",
		"description" : "Norma is a small and inconspicuous constellation in the southern hemisphere between Scorpius and Centaurus. Its name is Latin for normal, referring to a right angle, and is variously considered to represent a rule, a carpenter\u0027s square, a set square or a level.\r\rNorma, originally named l\u0027Equerre et la Regle in French, was one of the constellations invented by Abb\u00E9 de Lacaille in the middle of the 1750s, when he was measuring about 10,000 stars at the Cape of Good Hope. Norma represents a carpenter\u0027s square, used in the Age of Exploration by carpenters on exploratory vessels.",
		"key" : "Norma",
		"grouptype" : "Norma",
		"Meaning" : "carpenter's level",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Norma",
		"title" : "Norma Objects Group" },
	"Common" : "HR 5798",
	"OType" : "Star",
	"Distance" : "125.17",
	"RA_S" : 234.70613611,
	"DEC_S" : -52.37269558,
	"Constellation" : "Norma ",
	"AMag" : 5.422,
	"key" : 80174,
	"title" : "HR 5798"
	},
{
	"Index" : "60261",
	"Description" : "Eta Normae (\u03B7 Nor) is a star in the constellation Norma. Its apparent magnitude is 4.65.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Eta Normae, HIP 78639, SAO 226466, HD 143546, GC 21539, HR 5962, DM CD-48 10512, TYC 8318-1128-1",
	"group" : { "key" : "Norma" },
	"Common" : "Eta Normae",
	"OType" : "Star",
	"Distance" : "67.27",
	"RA_S" : 240.80374166,
	"DEC_S" : -49.22969901,
	"X" : 292,
	"Y" : 180,
	"Constellation" : "Norma ",
	"AMag" : 4.746,
	"key" : 80261,
	"title" : "Eta Normae"
	},
{
	"Index" : "64370",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Iota01 Normae, HIP 78662AB, SAO 243279, HD 143474, GC 21535, HR 5961, DM CP-57  7500, TYC 8718-2860-1",
	"group" : { "key" : "Norma" },
	"Common" : "Iota01 Normae",
	"OType" : "Double or multiple star",
	"Distance" : "42.9",
	"RA_S" : 240.8837229,
	"DEC_S" : -57.77506378,
	"Constellation" : "Norma ",
	"AMag" : 4.697,
	"key" : 84370,
	"title" : "Iota01 Normae"
	},
{
	"Index" : "60184",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Delta Normae, HIP 78914, SAO 226500, HD 144197, GC 21615, HR 5980, DM CD-44 10625, TYC 8310-1489-1",
	"group" : { "key" : "Norma" },
	"Common" : "Delta Normae",
	"OType" : "Star",
	"Distance" : "37.47",
	"RA_S" : 241.62260435,
	"DEC_S" : -45.17321012,
	"Constellation" : "Norma ",
	"AMag" : 4.743,
	"key" : 80184,
	"title" : "Delta Normae"
	},
{
	"Index" : "64342",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Kappa Normae, HIP 79509, SAO 243454, HD 145397, GC 21787, HR 6024, DM CP-54  7245, TYC 8715-2592-1",
	"group" : { "key" : "Norma" },
	"Common" : "Kappa Normae",
	"OType" : "Star",
	"Distance" : "131.05",
	"RA_S" : 243.36970178,
	"DEC_S" : -54.63046557,
	"Constellation" : "Norma ",
	"AMag" : 5.062,
	"key" : 84342,
	"title" : "Kappa Normae"
	},
{
	"Index" : "60228",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Theta Normae, HIP 79653, SAO 226600, HD 145842, GC 21836, HR 6045, DM CD-47 10611, TYC 8315-1750-1",
	"group" : { "key" : "Norma" },
	"Common" : "Theta Normae",
	"OType" : "Star",
	"Distance" : "118.07",
	"RA_S" : 243.81381189,
	"DEC_S" : -47.37202573,
	"Constellation" : "Norma ",
	"AMag" : 5.105,
	"key" : 80228,
	"title" : "Theta Normae"
	},
{
	"Index" : "60272",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma01 Normae, HIP 79790, SAO 226619, HD 146143, GC 21871, HR 6058, DM CD-49 10474, TYC 8319-1759-1",
	"group" : { "key" : "Norma" },
	"Common" : "Gamma01 Normae",
	"OType" : "Star",
	"Distance" : "442.59",
	"RA_S" : 244.25389411,
	"DEC_S" : -50.06812195,
	"Constellation" : "Norma ",
	"AMag" : 5.056,
	"key" : 80272,
	"title" : "Gamma01 Normae"
	},
{
	"Index" : "55988",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Lambda Normae, HIP 79963AS, SAO 226650, HD 146667, GC 21923, HR 6071, DM CD-42 11188, TYC 7860-1591-1",
	"group" : { "key" : "Norma" },
	"Common" : "Lambda Normae",
	"OType" : "Star",
	"Distance" : "106.11",
	"RA_S" : 244.82353438,
	"DEC_S" : -42.67396919,
	"Constellation" : "Norma ",
	"AMag" : 5.453,
	"key" : 75988,
	"title" : "Lambda Normae"
	},
{
	"Index" : "60290",
	"Description" : "Gamma2 Normae (\u03B32 Nor) is a star in the constellation Norma. Its apparent magnitude is 4.02.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma02 Normae, HIP 80000, SAO 243643, HD 146686, GC 21933, HR 6072, DM CD-49 10536, TYC 8320-2290-1",
	"group" : { "key" : "Norma" },
	"Common" : "Gamma2 Normae",
	"OType" : "Star",
	"Distance" : "39.48",
	"RA_S" : 244.96009758,
	"DEC_S" : -50.15550924,
	"X" : 261,
	"Y" : 199,
	"Constellation" : "Norma ",
	"AMag" : 4.122,
	"key" : 80290,
	"title" : "Gamma2 Normae"
	},
{
	"Index" : "60289",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 80208, SAO 226693, HD 147152, GC 21997, HR 6083, DM CD-4910591, TYC 8320-2258-1",
	"group" : { "key" : "Norma" },
	"Common" : "HR 6083",
	"OType" : "Star",
	"Distance" : "141.49",
	"RA_S" : 245.61664616,
	"DEC_S" : -49.57235741,
	"Constellation" : "Norma ",
	"AMag" : 5.308,
	"key" : 80289,
	"title" : "HR 6083"
	},
{
	"Index" : "60238",
	"Description" : "Epsilon Normae (\u03B5 Nor) is a star in the constellation Norma. Its apparent magnitude is 4.53.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Epsilon Normae, HIP 80582, SAO 226773, HD 147971, GC 22106, HR 6115, DM CD-47 10765, TYC 8316-4441-1",
	"group" : { "key" : "Norma" },
	"Common" : "Epsilon Normae",
	"OType" : "Spectroscopic binary",
	"Distance" : "162.2",
	"RA_S" : 246.79598304,
	"DEC_S" : -47.55479139,
	"X" : 237,
	"Y" : 171,
	"Constellation" : "Norma ",
	"AMag" : 4.508,
	"key" : 80238,
	"title" : "Epsilon Normae"
	},
{
	"Index" : "60210",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 80782, SAO 226813, HD 148379, GC 22150, HR 6131, DM CD-4510697, TYC 8312-3982-1",
	"group" : { "key" : "Norma" },
	"Common" : "HR 6131",
	"OType" : "Be Star",
	"Distance" : "558.6592",
	"RA_S" : 247.42636271,
	"DEC_S" : -46.24323255,
	"Constellation" : "Norma ",
	"AMag" : 5.41,
	"key" : 80210,
	"title" : "HR 6131"
	},
{
	"Index" : "56023",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Mu Normae, HIP 81122, SAO 226900, HD 149038, GC 22258, HR 6155, DM CD-43 10900, TYC 7866-3007-1",
	"group" : { "key" : "Norma" },
	"Common" : "Mu Normae",
	"OType" : "Pulsating variable Star",
	"RA_S" : 248.52092772,
	"DEC_S" : -44.04531723,
	"Constellation" : "Norma ",
	"AMag" : 4.91,
	"key" : 76023,
	"title" : "Mu Normae"
	},
{
	"Index" : "70192",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Theta Octantis, HIP 122, SAO 258207, HD 224889, GC 33321, HR 9084, DM CP-77  1596, TYC 9350-450-1",
	"group" : { "backgroundImage" : "images/Alignment/29.png",
		"description" : "Octans (pron.: /\u02C8\u0252kt\u00E6nz/) is a faint constellation the southern sky. Its name is Latin for the eighth part of a circle, but it is named after the octant, a navigational instrument. The constellation was devised by Nicolas Louis de Lacaille in the eighteenth century.\r\rOctans is notable as the location of the south celestial pole. Unlike the north pole, it has no bright pole star: Sigma Octantis (\u03C3 Oct) is a naked-eye star very close to the pole, but it is so faint (mag. 5.6) that it is practically useless for navigation purposes. Conveniently for navigators, the constellation Crux, the Southern Cross, points toward the pole.\r\rThe constellation is circumpolar to the south celestial pole, so it can be seen in Southern Hemisphere skies during the evening in any month of the year. The Right Ascension and month of best visibility given are for the three brightest stars, which are at their highest in the sky during the evening in November.\r\rOctans was created by Nicolas Louis de Lacaille in 1752 out of faint circumpolar stars. Originally, it was known as \u0022Octans Hadleianus\u0022 in honor of the octant\u0027s inventor, John Hadley, who devised it in 1730. There is no real mythology related to Octans, partially due to its extreme southerly latitude.",
		"key" : "Octans",
		"grouptype" : "Octans",
		"Meaning" : "octant (instrument)",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Octans",
		"title" : "Octans Objects Group" },
	"Common" : "Theta Octantis",
	"OType" : "Star",
	"Distance" : "66.57",
	"DEC_S" : -77.06569263,
	"Constellation" : "Octans ",
	"AMag" : 4.926,
	"key" : 90192,
	"title" : "Theta Octantis"
	},
{
	"Index" : "70235",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Gamma03 Octantis, HIP 814, SAO 258215, HD 636, GC 173, HR 30, DM CP-82     4, TYC 9358-208-1",
	"group" : { "key" : "Octans" },
	"Common" : "Gamma03 Octantis",
	"OType" : "Star",
	"Distance" : "78.04",
	"RA_S" : 2.50906179,
	"DEC_S" : -82.22404825,
	"Constellation" : "Octans ",
	"AMag" : 5.399,
	"key" : 90235,
	"title" : "Gamma03 Octantis"
	},
{
	"Index" : "71109",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Zeta Octantis, HIP 43908, SAO 258515, HD 79837, GC 12580, HR 3678, DM CP-85   183, TYC 9510-2752-1",
	"group" : { "key" : "Octans" },
	"Common" : "Zeta Octantis",
	"OType" : "Star",
	"Distance" : "49.75",
	"RA_S" : 134.17078978,
	"DEC_S" : -85.66315116,
	"Constellation" : "Octans ",
	"AMag" : 5.456,
	"key" : 91109,
	"title" : "Zeta Octantis"
	},
{
	"Index" : "71103",
	"Description" : "Delta Octantis has the distinction of being Saturn\u0027s southern pole star. It has 1.2 times the mass of the Sun and about 25 times the Sun\u0027s radius. This star is about 4.3 billion years old; the same age as the Sun.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u7570\u96C0 (Y\u00EC Qu\u00E8), meaning Exotic Bird, refers to an asterism consisting of \u03B4 Octantis, \u03B6 Apodis, \u03B9 Apodis, \u03B2 Apodis, \u03B3 Apodis, \u03B41 Apodis, \u03B7 Apodis, \u03B1 Apodis and \u03B5 Apodis. Consequently, \u03B4 Octantis itself is known as \u7570\u96C0\u4E94 (Y\u00EC Qu\u00E8 w\u01D4, English: the Fifth Star of Exotic Bird.)",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Delta Octantis, HIP 70638, SAO 258698, HD 124882, GC 19349, HR 5339, DM CP-83   557, TYC 9509-3854-1",
	"group" : { "key" : "Octans" },
	"Common" : "Delta Octantis",
	"OType" : "Variable Star",
	"Distance" : "91.64",
	"RA_S" : 216.73013364,
	"DEC_S" : -83.66788522,
	"X" : 252,
	"Y" : 607,
	"Constellation" : "Octans ",
	"AMag" : 4.453,
	"key" : 91103,
	"title" : "Delta Octantis"
	},
{
	"Index" : "70765",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Phi Octantis, HIP 90133, SAO 257584, HD 167468, GC 24999, HR 6829, DM CP-75  1417, TYC 9445-2572-1",
	"group" : { "key" : "Octans" },
	"Common" : "Phi Octantis",
	"OType" : "Star",
	"Distance" : "59.47",
	"RA_S" : 275.90187348,
	"DEC_S" : -75.04427574,
	"Constellation" : "Octans ",
	"AMag" : 5.461,
	"key" : 90765,
	"title" : "Phi Octantis"
	},
{
	"Index" : "71271",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Chi Octantis, HIP 92824, SAO 258799, HD 164461, GC 25207, HR 6721, DM CP-87   274, TYC 9531-934-1",
	"group" : { "key" : "Octans" },
	"Common" : "Chi Octantis",
	"OType" : "Star",
	"Distance" : "78.71",
	"RA_S" : 283.69636371,
	"DEC_S" : -87.60584344,
	"Constellation" : "Octans ",
	"AMag" : 5.426,
	"key" : 91271,
	"title" : "Chi Octantis"
	},
{
	"Index" : "70878",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Alpha Octantis, HIP 104043, SAO 257879, HD 199532, GC 29343, HR 8021, DM CP-77  1474, TYC 9465-412-1",
	"group" : { "key" : "Octans" },
	"Common" : "Alpha Octantis",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "43.53",
	"RA_S" : 316.17942543,
	"DEC_S" : -77.02376733,
	"Constellation" : "Octans ",
	"AMag" : 5.182,
	"key" : 90878,
	"title" : "Alpha Octantis"
	},
{
	"Index" : "71288",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Sigma Octantis, HIP 104382, SAO 258857, HD 177482, GC 28194, HR 7228, DM CP-89    47, TYC 9536-384-1",
	"group" : { "key" : "Octans" },
	"Common" : "Polaris Australis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "86.06",
	"RA_S" : 317.19522281,
	"DEC_S" : -88.95649871,
	"Constellation" : "Octans ",
	"AMag" : 5.475,
	"key" : 91288,
	"title" : "Polaris Australis"
	},
{
	"Index" : "70946",
	"Description" : "Nu Octantis (\u03BD Oct) is a star in the constellation Octans. Its apparent magnitude is 3.76.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Nu Octantis, HIP 107089, SAO 257948, HD 205478, GC 30289, HR 8254, DM CP-77  1510, TYC 9478-1483-1",
	"group" : { "key" : "Octans" },
	"Common" : "Nu Octantis",
	"OType" : "Spectroscopic binary",
	"Distance" : "21.16",
	"RA_S" : 325.36937405,
	"DEC_S" : -77.39004341,
	"X" : 405,
	"Y" : 464,
	"Constellation" : "Octans ",
	"AMag" : 3.73,
	"key" : 90946,
	"title" : "Nu Octantis"
	},
{
	"Index" : "70972",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Epsilon Octantis, HIP 110256, SAO 258928, HD 210967, GC 31166, HR 8481, DM CP-81   995, TYC 9483-1157-1",
	"group" : { "key" : "Octans" },
	"Common" : "Epsilon Octantis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "89.08",
	"RA_S" : 335.0069699,
	"DEC_S" : -80.43974779,
	"Constellation" : "Octans ",
	"AMag" : 5.319,
	"key" : 90972,
	"title" : "Epsilon Octantis"
	},
{
	"Index" : "70989",
	"Description" : "Beta Octantis (\u03B2 Oct) is a star in the constellation Octans. Its apparent magnitude is 4.14.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Beta Octantis, HIP 112405, SAO 258941, HD 214846, GC 31712, HR 8630, DM CP-82   889, TYC 9488-1053-1",
	"group" : { "key" : "Octans" },
	"Common" : "Beta Octantis",
	"OType" : "Star",
	"Distance" : "45.75",
	"RA_S" : 341.51455096,
	"DEC_S" : -81.38161865,
	"X" : 340,
	"Y" : 457,
	"Constellation" : "Octans ",
	"AMag" : 4.155,
	"key" : 90989,
	"title" : "Beta Octantis"
	},
{
	"Index" : "70977",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Xi Octantis, HIP 112781, SAO 258946, HD 215573, GC 31821, HR 8663, DM CP-80  1055, TYC 9484-1164-1",
	"group" : { "key" : "Octans" },
	"Common" : "Xi Octantis",
	"OType" : "Pulsating variable Star",
	"Distance" : "150.91",
	"RA_S" : 342.59505196,
	"DEC_S" : -80.12384567,
	"Constellation" : "Octans ",
	"AMag" : 5.29,
	"key" : 90977,
	"title" : "Xi Octantis"
	},
{
	"Index" : "70994",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Gamma01 Octantis, HIP 117689, SAO 258989, HD 223647, GC 33107, HR 9032, DM CP-82   905, TYC 9489-785-1",
	"group" : { "key" : "Octans" },
	"Common" : "Gamma01 Octantis",
	"OType" : "Star",
	"Distance" : "81.28",
	"RA_S" : 358.02702882,
	"DEC_S" : -82.01881778,
	"Constellation" : "Octans ",
	"AMag" : 5.21,
	"key" : 90994,
	"title" : "Gamma01 Octantis"
	},
{
	"Index" : "33985",
	"Description" : "Delta Ophiuchi (\u03B4 Oph, \u03B4 Ophiuchi) is a star in the constellation Ophiuchus. It has the traditional name Yed Prior. The star Epsilon Ophiuchi, with which it forms a naked eye optical double, is Yed Posterior. The apparent visual magnitude is 2.75, making this a third-magnitude star and the fourth brightest in the constellation. Parallax measurements from the Hipparcos spacecraft yield a distance estimate of around 171 light-years (52 parsecs) from Earth. Delta Ophiuchi is 170 light years from Earth, while Epsilon is 108; hence they are a mere optical double. This star has a stellar classification of M0.5 III, making this a red giant star that has undergone expansion of its outer envelope after exhausting the supply of hydrogen at its core. The measured angular diameter of this star, after correction for limb darkening, is 10.47 \u00B1 0.12 mas. At the estimated distance of Delta Ophiuchi, this yields a physical size of about 59 times the radius of the Sun. In spite of its enlarged size, this star has only 1.5 times the mass of the Sun and hence a much lower density. The effective temperature of the outer atmosphere of Delta Ophiuchi is a relatively cool 3,679 K, which is what gives it the orange-red hue of an M-type star.\r\rYed Prior is listed as a suspected variable star that may change by 0.03 in visual magnitude. It has a low projected rotational velocity of 7.0 km s\u20131, which gives a minimum value for the azimuthal velocity along the star\u0027s equator. The abundance of elements other than hydrogen and helium, what astronomers term the star\u0027s metallicity, is more than double the abundance in the Sun\u0027s photosphere.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "1 Ophiuchi, Delta Ophiuchi, HIP 79593, SAO 141052, HD 146051, GC 21838, HR 6056, DM BD-03  3903, TYC 5037-1068-1",
	"group" : { "backgroundImage" : "images/Alignment/34.png",
		"description" : "Ophiuchus (pron.: /\u02CC\u0252fi\u02D0\u02C8ju\u02D0k\u0259s/) is a large constellation located around the celestial equator. Its name is from the Greek \u1F48\u03C6\u03B9\u03BF\u1FE6\u03C7\u03BF\u03C2 \u0022serpent-bearer\u0022, and it is commonly represented as a man grasping the snake that is represented by the constellation Serpens. Ophiuchus was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and it remains one of the 88 modern constellations. It was formerly referred to as Serpentarius (/\u02CCs\u025Crp\u0259n\u02C8t\u025B\u0259ri\u0259s/; also Anguitenens), a Latin word meaning the same as its current name.\r\rOphiuchus is located between Aquila, Serpens and Hercules, northwest of the center of the Milky Way. The southern part lies between Scorpius to the west and Sagittarius to the east. In the northern hemisphere, it is best visible in summer. It is located opposite Orion in the sky. Ophiuchus is depicted as a man grasping a serpent; the interposition of his body divides the snake constellation Serpens into two parts, Serpens Caput and Serpens Cauda, which are nonetheless counted as one constellation.\r\rOphiuchus straddles the equator but lies predominately to its south. Rasalhague, a fairly conspicuous star in its north, is circumpolar north of 78\u00B0 north latitude and invisible south of 78\u00B0 south latitude. The constellation extends southward to -30\u00B0 declination, so the constellation can never be seen in full even in such places as Anchorage, Reykjav\u00EDk, and Helsinki north of 60\u00B0 north latitude. Segments of the ecliptic that lie within Ophiuchus lie south of -20\u00B0 declination and are thus invisible north of 70\u00B0 north latitude.\r\rIn contrast to Orion, it is in the period November\u2013January (summer in the Southern Hemisphere, winter in the Northern Hemisphere) when Ophiuchus is in the daytime sky and thus not visible at most latitudes. However for much of the Arctic Circle in the Northern Hemisphere\u0027s winter months, the Sun is below the horizon even at midday. Stars (and thus parts of Ophiuchus, especially Rasalhague) are then visible at twilight for a few hours around local noon, low in the South. In the Northern Hemisphere\u0027s summer months, when Ophiuchus is normally visible in the night sky, the constellation is actually not visible in the Arctic Circle because the sun does not set at that time of year north of the Arctic Circle. In countries close to the equator Ophiuchus appears overhead in June around midnight and in the October evening sky.\r\rThere is no evidence of the constellation preceding the classical era, and in Babylonian astronomy, a \u0022Sitting Gods\u0022 constellation seems to have been located in the general area of Ophiuchus. However, Gavin White proposes that Ophiuchus may in fact be remotely descended from this Babylonian constellation, representing Nirah, a serpent-god who was sometimes depicted with his upper half human but with serpents for legs.\r\rThe earliest mention of the constellation is in Aratus, informed by the lost catalogue of Eudoxus of Cnidus (4th century BC):\r\rTo the Phantom\u0027s back the Crown is near, but by his head mark near at hand the head of Ophiuchus, and then from it you can trace the starlit Ophiuchus himself: so brightly set beneath his head appear his gleaming shoulders. They would be clear to mark even at the midmonth moon, but his hands are not at all so bright; for faint runs the gleam of stars along on this side and on that. Yet they too can be seen, for they are not feeble. Both firmly clutch the Serpent, which encircles the waist of Ophiuchus, but he, steadfast with both his feet well set, tramples a huge monster, even the Scorpion, standing upright on his eye and breast. Now the Serpent is wreathed about his two hands \u2013 a little above his right hand, but in many folds high above his left.\r\rAccording to Roman era mythography, the figure represents the healer Asclepius, who learned the secrets of keeping death at bay after observing one serpent bringing another healing herbs. To prevent the entire human race from becoming immortal under Asclepius\u0027 care, Zeus killed him with a bolt of lightning, but later placed his image in the heavens to honor his good works.\r\rIn medieval Islamic astronomy (Azophi\u0027s Uranometry, 10th century), the constellation was known as Al-\u1E24awwa\u02BE \u0022the snake-charmer\u0022.\r\rAratus describes Ophiuchus as trampling on Scorpio with his feet. This is depicted in Renaissance to Early Modern star charts, beginning with Albrecht D\u00FCrer in 1515; in some depictions (such as that of Johannes Kepler, 1604), Scorpio also seems to threaten to sting Serpentarius in the foot. This is consistent with Azophi, who already included \u03C8 Oph and \u03C9 Oph as the snake-charmer\u0027s \u0022left foot\u0022, and \u03B8 Oph and \u03BF Oph as his \u0022right foot\u0022, making Ophiuchus a zodiacal constellation at least as regards his feet. This arrangement has been taken as symbolic in later literature, and placed in relation to the words spoken by God to the serpent in the Garden of Eden (Genesis 3:15).\r\rJohn Milton used Opiuchus as the vehicle for an epic simile in Book 2 of Paradise Lost, comparing Satan to a comet burning across the length of Opiuchus (lines 706-10): \u0027on th\u0027 other side / Incensed with indignation Satan stood / Unterrified, and like a comet burned / That fires the length of Opiuchus huge / In th\u0027 arctic sky\u0027.",
		"key" : "Ophiuchus",
		"grouptype" : "Ophiuchus",
		"Meaning" : "serpent-bearer",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Ophiuchus",
		"title" : "Ophiuchus Objects Group" },
	"Common" : "Yed Prior",
	"OType" : "Variable Star",
	"Distance" : "52.46",
	"RA_S" : 243.58641053,
	"DEC_S" : -3.69432256,
	"X" : 524,
	"Y" : 362,
	"Constellation" : "Ophiuchus ",
	"AMag" : 2.896,
	"key" : 53985,
	"shortTitle" : "Yad; Yed; Jed; Jed Prior",
	"title" : "Yed Prior"
	},
{
	"Index" : "34010",
	"Description" : "Epsilon Ophiuchi (\u03B5 Oph, \u03B5 Ophiuchi) is a red giant star in the constellation Ophiuchus. It has the traditional name Yed Posterior. The star Delta Ophiuchi, with which it forms a naked eye optical double, is named Yed Prior. The name Yed comes from Arabic for \u0022the hand\u0022. Epsilon Ophiuchi is located less than five degrees south of the celestial equator in the eastern part of the constellation. With an apparent visual magnitude of 3.220, this allows the star to be seen with the naked eye from most of the Earth under suitably dark skies. Parallax measurements yield an estimated distance of 106.4 light-years (32.6 parsecs). It has a stellar classification of G9.5 IIIb, with the luminosity class of III indicating that this is a giant star that has exhausted the hydrogen and evolved away from the main sequence. This red giant has nearly double the Sun\u0027s mass and has expanded to an estimated radius of over ten times the radius of the Sun, giving it a luminosity of about 54 times the Sun. It is about a billion years old.\r\rUnusually for a class G giant, it is cyanogen-deficient and carbon-deficient. The outer envelope of this star displays solar-type oscillations with a period of 0.19 days, allowing the methods of asteroseismology to be applied. However, the models for this star have not been able to distinguish whether this star is generating energy by the thermonuclear fusion of hydrogen along a shell, or the fusion of helium at its core. Either mode produces a good fit to the star\u0027s physical properties. The projected rotational velocity of the star is 5.7 km s\u22121, and the inclination of the rotation axis to the line of sight from the Earth lies in the range of 41\u201373\u00B0.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "2 Ophiuchi, Epsilon Ophiuchi, HIP 79882, SAO 141086, HD 146791, GC 21920, HR 6075, DM BD-04  4086, TYC 5042-999-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Yed Posterior",
	"OType" : "Star",
	"Distance" : "32.64",
	"RA_S" : 244.58037393,
	"DEC_S" : -4.69250958,
	"X" : 512,
	"Y" : 374,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.321,
	"key" : 54010,
	"shortTitle" : "Jed Posterior",
	"title" : "Yed Posterior"
	},
{
	"Index" : "42605",
	"Description" : "Psi Ophiuchi (\u03C8 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.49.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "4 Ophiuchi, Psi Ophiuchi, HIP 80343, SAO 159892, HD 147700, GC 22042, HR 6104, DM BD-19  4365, TYC 6211-510-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Psi Ophiuchi",
	"OType" : "Star",
	"Distance" : "61.14",
	"RA_S" : 246.02575955,
	"DEC_S" : -20.03732496,
	"X" : 485,
	"Y" : 565,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.591,
	"key" : 62605,
	"title" : "Psi Ophiuchi"
	},
{
	"Index" : "46996",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "5 Ophiuchi, Rho Ophiuchi, HIP 80473B, SAO 184382, HD 147933, GC 22079, HR 6112, DM CD-23 12861A, TYC 6794-549-2",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Rho Ophiuchi",
	"OType" : "Double or multiple star",
	"Distance" : "109.44",
	"RA_S" : 246.39632359,
	"DEC_S" : -23.44717083,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.57,
	"key" : 66996,
	"title" : "Rho Ophiuchi"
	},
{
	"Index" : "46995",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "5 Ophiuchi, Rho Ophiuchi, HIP 80473A, SAO 184382, HD 147933, GC 22079, HR 6112, DM CD-23 12861A, TYC 6794-549-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Rho Ophiuchi",
	"OType" : "Double or multiple star",
	"Distance" : "109.44",
	"RA_S" : 246.39642649,
	"DEC_S" : -23.44719629,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.067,
	"key" : 66995,
	"title" : "Rho Ophiuchi"
	},
{
	"Index" : "42576",
	"Description" : "Chi Ophiuchi (Chi Oph / \u03C7 Ophiuchi / \u03C7 Oph) is a Be star in the constellation of Ophiuchus. It has an apparent visual magnitude which varies between 4.18 and 5.0.\r\rThis star is a proper motion member of the Upper Scorpius sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "7 Ophiuchi, Chi Ophiuchi, HIP 80569, SAO 159918, HD 148184, GC 22117, HR 6118, DM BD-18  4282, TYC 6207-1170-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Chi Ophiuchi",
	"OType" : "Be Star",
	"Distance" : "160.77",
	"RA_S" : 246.75597912,
	"DEC_S" : -18.45624827,
	"X" : 478,
	"Y" : 544,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.281,
	"key" : 62576,
	"title" : "Chi Ophiuchi"
	},
{
	"Index" : "38325",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "HIP 80620, SAO 141186, HD 148349, GC 22133, HR 6128, DM BD-07 4292, TYC 5626-124-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "HR 6128",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "175.98",
	"RA_S" : 246.93106756,
	"DEC_S" : -7.5979333,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.444,
	"key" : 58325,
	"title" : "HR 6128"
	},
{
	"Index" : "38328",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "3 Ophiuchi, Upsilon Ophiuchi, HIP 80628AB, SAO 141187, HD 148367, GC 22134, HR 6129, DM BD-08  4243, TYC 5626-1388-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Upsilon Ophiuchi",
	"OType" : "Spectroscopic binary",
	"Distance" : "37.45",
	"RA_S" : 246.95075196,
	"DEC_S" : -8.37167379,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.653,
	"key" : 58328,
	"title" : "Upsilon Ophiuchi"
	},
{
	"Index" : "24311",
	"Description" : "Lambda Ophiuchi (\u03BB Oph, \u03BB Ophiuchi) is a binary star system in the constellation Ophiuchus. It has the traditional name Marfik (or \u0022Marsik\u0022).\r\rLambda Ophiuchi belongs to spectral class A1V+A and has apparent magnitude +3.82. It is approximately 166 light years from Earth.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "10 Ophiuchi, Lambda Ophiuchi, HIP 80883B, SAO 121658, HD 148857, GC 22203, HR 6149, DM BD+02  3118, TYC 386-2062-2",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Lambda Ophiuchi",
	"OType" : "High proper-motion Star",
	"Distance" : "53.02",
	"RA_S" : 247.7284781,
	"DEC_S" : 1.98395581,
	"X" : 474,
	"Y" : 290,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.152,
	"key" : 44311,
	"shortTitle" : "Marfik; Marsic",
	"title" : "Lambda Ophiuchi"
	},
{
	"Index" : "24310",
	"Description" : "Lambda Ophiuchi (\u03BB Oph, \u03BB Ophiuchi) is a binary star system in the constellation Ophiuchus. It has the traditional name Marfik (or \u0022Marsik\u0022).\r\rLambda Ophiuchi belongs to spectral class A1V+A and has apparent magnitude +3.82. It is approximately 166 light years from Earth.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "10 Ophiuchi, Lambda Ophiuchi, HIP 80883A, SAO 121658, HD 148857, GC 22203, HR 6149, DM BD+02  3118, TYC 386-2062-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Lambda Ophiuchi",
	"OType" : "High proper-motion Star",
	"Distance" : "53.02",
	"RA_S" : 247.7284781,
	"DEC_S" : 1.98395581,
	"X" : 474,
	"Y" : 290,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.147,
	"key" : 44310,
	"shortTitle" : "Marfik; Marsic",
	"title" : "Lambda Ophiuchi"
	},
{
	"Index" : "42556",
	"Description" : "Phi Ophiuchi (\u03C6 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.29.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "8 Ophiuchi, Phi Ophiuchi, HIP 80894, SAO 159963, HD 148786, GC 22200, HR 6147, DM BD-16  4298, TYC 6203-806-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Phi Ophiuchi",
	"OType" : "Star",
	"Distance" : "74.65",
	"RA_S" : 247.7848649,
	"DEC_S" : -16.61273106,
	"X" : 467,
	"Y" : 521,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.378,
	"key" : 62556,
	"title" : "Phi Ophiuchi"
	},
{
	"Index" : "42689",
	"Description" : "Omega Ophiuchi (\u03C9 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.44.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "9 Ophiuchi, Omega Ophiuchi, HIP 80975, SAO 184450, HD 148898, GC 22221, HR 6153, DM BD-21  4381, TYC 6228-1489-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Omega Ophiuchi",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "51.7",
	"RA_S" : 248.03416595,
	"DEC_S" : -21.46639223,
	"X" : 461,
	"Y" : 581,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.449,
	"key" : 62689,
	"title" : "Omega Ophiuchi"
	},
{
	"Index" : "38356",
	"Description" : "Zeta Ophiuchi (\u03B6 Oph, \u03B6 Ophiuchi) is a star located in the constellation of Ophiuchus. It has an apparent visual magnitude of 2.57, making it the third brightest star in the constellation. Parallax measurements give an estimated distance of roughly 366 light-years (112 parsecs) from the Earth.\u03B6 Ophiuchi is an enormous star with more than 19 times the Sun\u0027s mass and eight times its radius. The stellar classification of this star is O9.5 V, with the luminosity class of V indicating that it is generating energy in its core by the nuclear fusion of hydrogen. This energy is being emitted from the outer envelope at an effective temperature of 34,000K, giving the star the blue hue of an O-type star. It is rotating rapidly and may be close to the velocity at which it would begin to break up. The projected rotational velocity may be as high as 400 km s\u20131 and it may be rotating at a rate of once per day.\r\rThis is a young star with an age of only three million years. Its luminosity is varying in a periodic manner similar to a Beta Cephei variable. This periodicity has a dozen or more frequencies ranging between 1\u201310 cycles per day. In 1979, examination of the spectrum of this star found \u0022moving bumps\u0022 in its helium line profiles. This feature has since been found in other stars, which have come to be called \u03B6 Oph stars. These spectral properties are likely the result of non-radial pulsations.\r\rThis star is roughly half way through the initial phase of its stellar evolution and will, within the next few million years, expand into a red supergiant star wider than the orbit of Jupiter before ending its life in a supernova explosion leaving behind a Neutron Star or Pulsar. From the Earth, a significant fraction of the light from this star is absorbed by interstellar dust, particularly at the blue end of the spectrum. In fact, were it not for this dust, \u03B6 Ophiuchi would shine several times brighter and be among the very brightest stars visible.\r\rX-ray emissions have been detected from Zeta Ophiuchi that vary periodically. The net X-ray flux is estimated at 1.2 \u00D7 1031 erg s\u20131. In the energy range of 0.5\u201310 keV, this flux varies by about 20% over a period of 0.77 days. This behavior may be the result of a magnetic field in the star. The measured average strength of the longitudinal field is about 141 \u00B1 45 G. \u03B6 Ophiuchi is moving through space with a peculiar velocity of 30 km s\u20131. Based upon the age and direction of motion of this star, it is a member of the Upper Scorpius sub-group of the Scorpius-Centaurus Association of stars that share a common origin and space velocity. Such runaway stars may be ejected by dynamic interactions between three or four stars. However, in this case the star may be a former component of a binary star system in which the more massive primary was destroyed in a Type II supernova explosion. The pulsar PSR B1929+10 may be the leftover remnant of this supernova, as it too was ejected from the association with a velocity vector that fits the scenario.\r\rDue to the high space velocity of Zeta Ophiuchi, in combination with high intrinsic brightness and its current location in a dust-rich area of the galaxy, the star is creating a bow-shock in the direction of motion. This shock has been made visible via NASA\u0027s Wide-field Infrared Survey Explorer. The formation of this bow shock can be explained by a mass loss rate of about 1.1 \u00D7 10\u22127 times the Mass of the Sun per year, which equals the mass of the Sun every nine million years.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "13 Ophiuchi, Zeta Ophiuchi, HIP 81377, SAO 160006, HD 149757, GC 22332, HR 6175, DM BD-10  4350, TYC 5632-1042-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Zeta Ophiuchi",
	"OType" : "Be Star",
	"Distance" : "112.17",
	"RA_S" : 249.28974606,
	"DEC_S" : -10.56709152,
	"X" : 452,
	"Y" : 446,
	"Constellation" : "Ophiuchus ",
	"AMag" : 2.546,
	"key" : 58356,
	"title" : "Zeta Ophiuchi"
	},
{
	"Index" : "42661",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "24 Scorpii, HIP 81724, SAO 160046, HD 150416, GC 22449, HR 6196, DM BD-17  4618, TYC 6221-904-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "24 Scorpii",
	"OType" : "Star in Nebula",
	"Distance" : "126.2",
	"RA_S" : 250.39326332,
	"DEC_S" : -17.74216611,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.042,
	"key" : 62661,
	"title" : "24 Scorpii"
	},
{
	"Index" : "38363",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "20 Ophiuchi, HIP 82369, SAO 160118, HD 151769, GC 22643, HR 6243, DM BD-10  4394, TYC 5633-777-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "20 Ophiuchi",
	"OType" : "Star",
	"Distance" : "31.8",
	"RA_S" : 252.45845297,
	"DEC_S" : -10.78303255,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.687,
	"key" : 58363,
	"title" : "20 Ophiuchi"
	},
{
	"Index" : "71426",
	"Description" : "Iota Ophiuchi (\u03B9 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.38.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "25 Ophiuchi, Iota Ophiuchi, HIP 82673, SAO 102458, HD 152614, GC 22775, HR 6281, DM BD+10  3092, TYC 979-2199-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Iota Ophiuchi",
	"OType" : "Star",
	"Distance" : "75.16",
	"RA_S" : 253.50196535,
	"DEC_S" : 10.16536115,
	"X" : 402,
	"Y" : 188,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.347,
	"key" : 91426,
	"title" : "Iota Ophiuchi"
	},
{
	"Index" : "34102",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "23 Ophiuchi, HIP 82730, SAO 141431, HD 152601, GC 22783, HR 6280, DM BD-05  4374, TYC 5063-1633-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "23 Ophiuchi",
	"OType" : "Star",
	"Distance" : "73.66",
	"RA_S" : 253.64872257,
	"DEC_S" : -6.15397998,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.352,
	"key" : 54102,
	"title" : "23 Ophiuchi"
	},
{
	"Index" : "71425",
	"Description" : "Kappa Ophiuchi (\u03BA Oph, \u03BA Ophiuchi) is a star in the equatorial constellation Ophiuchus. It is a suspected variable star with an average apparent visual magnitude of 3.20, making it visible to the naked eye and one of the brighter members of this constellation. Based upon parallax measurements made during the Hipparcos mission, it is situated at a distance of around 91.5 light-years (28.1 parsecs) from Earth. The overall brightness of the star is diminished by 0.11 magnitudes due to extinction from intervening matter along the line of sight.\r\rThe spectrum of this star matches a stellar classification of A2 III, with the luminosity class of \u0027III\u0027 indicating this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence of stars like the Sun. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is 19% more massive than the Sun, but the outer envelope has expanded to around 11 times the Sun\u0027s radius. With its enlarged size, it is radiating 46 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,529 K. This is cooler than the Sun\u0027s surface and gives Kappa Ophiuchi the orange-hued glow of a K-type star.\r\rAlthough designated as a variable star, observations with the Hipparcos satellite showed a variation of no more than 0.02 in magnitude. In designating this as a suspected variable star, it is possible that Kappa Ophiuchi was mistaken for Chi Ophiuchi, which is a variable star. Kappa Ophiuchi belongs to an evolutionary branch known as the red clump, making it a clump giant. The surface abundance of elements other than hydrogen and helium, what astronomers term the star\u0027s metallicity, is similar to the abundances of those elements in the Sun.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "27 Ophiuchi, Kappa Ophiuchi, HIP 83000, SAO 121962, HD 153210, GC 22862, HR 6299, DM BD+09  3298, TYC 979-2198-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Kappa Ophiuchi",
	"OType" : "Long Period Variable candidate",
	"Distance" : "28.04",
	"RA_S" : 254.41707145,
	"DEC_S" : 9.37503097,
	"X" : 391,
	"Y" : 197,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.31,
	"key" : 91425,
	"title" : "Kappa Ophiuchi"
	},
{
	"Index" : "34138",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "30 Ophiuchi, HIP 83262, SAO 141483, HD 153687, GC 22937, HR 6318, DM BD-04  4215, TYC 5072-1228-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "30 Ophiuchi",
	"OType" : "Star",
	"Distance" : "123.97",
	"RA_S" : 255.26500639,
	"DEC_S" : -4.22264404,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.988,
	"key" : 54138,
	"title" : "30 Ophiuchi"
	},
{
	"Index" : "38409",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "HIP 83962, SAO 160324, HD 155078, GC 23145, HR 6375, DM BD-10 4445, TYC 5648-1672-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Lalande 31188 (HR 6375)",
	"OType" : "Star",
	"Distance" : "41.31",
	"RA_S" : 257.44979611,
	"DEC_S" : -10.52330063,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.483,
	"key" : 58409,
	"title" : "Lalande 31188 (HR 6375)"
	},
{
	"Index" : "42702",
	"Description" : "Eta Ophiuchi, also known as \u03B7 Oph or \u03B7 Ophiuchi, is a star in the constellation Ophiuchus. It has the traditional name Sabik.\u03B7 Oph is actually a binary star system that is difficult to resolve in amateur telescopes but whose true nature has been determined through use of more advanced techniques. The \u0022primary\u0022 star (whose observational data make up the table in this article), which could nominally be referred to as \u03B7 Oph A, is actually only slightly larger and warmer than its companion, \u03B7 Oph B. Individually each star is a fairly unremarkable A class main sequence star, but as a binary pair they are unusual. Each star orbits around a common center in a close and highly elliptical orbit, making planetary formation impossible in this system and some stellar data imprecise.\r\r\u03B7 Oph is the northern pole star of the planet Uranus.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "35 Ophiuchi, Eta Ophiuchi, HIP 84012B, SAO 160332, HD 155125, GC 23158, HR 6378, DM BD-15  4467, TYC 6232-1333-2",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Sabik",
	"OType" : "High proper-motion Star",
	"Distance" : "27.08",
	"RA_S" : 257.594167,
	"DEC_S" : -15.725236,
	"X" : 351,
	"Y" : 507,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.706,
	"key" : 62702,
	"shortTitle" : "Al'sabik",
	"title" : "Sabik"
	},
{
	"Index" : "42701",
	"Description" : "Eta Ophiuchi, also known as \u03B7 Oph or \u03B7 Ophiuchi, is a star in the constellation Ophiuchus. It has the traditional name Sabik.\u03B7 Oph is actually a binary star system that is difficult to resolve in amateur telescopes but whose true nature has been determined through use of more advanced techniques. The \u0022primary\u0022 star (whose observational data make up the table in this article), which could nominally be referred to as \u03B7 Oph A, is actually only slightly larger and warmer than its companion, \u03B7 Oph B. Individually each star is a fairly unremarkable A class main sequence star, but as a binary pair they are unusual. Each star orbits around a common center in a close and highly elliptical orbit, making planetary formation impossible in this system and some stellar data imprecise.\r\r\u03B7 Oph is the northern pole star of the planet Uranus.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "35 Ophiuchi, Eta Ophiuchi, HIP 84012A, SAO 160332, HD 155125, GC 23158, HR 6378, DM BD-15  4467, TYC 6232-1333-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Sabik",
	"OType" : "High proper-motion Star",
	"Distance" : "27.08",
	"RA_S" : 257.594388,
	"DEC_S" : -15.725158,
	"X" : 351,
	"Y" : 507,
	"Constellation" : "Ophiuchus ",
	"AMag" : 2.477,
	"key" : 62701,
	"shortTitle" : "Al'sabik",
	"title" : "Sabik"
	},
{
	"Index" : "47188",
	"Description" : "36 Ophiuchi is a triple star system 19.5 light years away from Earth. It is in the constellation Ophiuchus.\r\rThe primary and secondary stars are nearly identical orange main sequence dwarves of spectral type K0/K1 and the tertiary star is an orange main sequence dwarf of spectral type K5.\r\rStar C is separated from the A-B pair by 700 arc seconds, compared to a minimum of 4.6 arcsec for A-B, so it has a negligible effect on the movements of the A-B pair. Both A and B have active chromospheres.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "36 Ophiuchi, A Ophiuchi, HIP 84405A, SAO 185199, HD 155885, GC 23274, HR 6401, DM CD-26 12026B, TYC 6820-326-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "36 Ophiuchi",
	"OType" : "Double or multiple star",
	"Distance" : "5.93",
	"RA_S" : 258.83743307,
	"DEC_S" : -26.60282143,
	"X" : 335,
	"Y" : 642,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.33,
	"key" : 67188,
	"title" : "36 Ophiuchi"
	},
{
	"Index" : "47189",
	"Description" : "36 Ophiuchi is a triple star system 19.5 light years away from Earth. It is in the constellation Ophiuchus.\r\rThe primary and secondary stars are nearly identical orange main sequence dwarves of spectral type K0/K1 and the tertiary star is an orange main sequence dwarf of spectral type K5.\r\rStar C is separated from the A-B pair by 700 arc seconds, compared to a minimum of 4.6 arcsec for A-B, so it has a negligible effect on the movements of the A-B pair. Both A and B have active chromospheres.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "36 Ophiuchi, A Ophiuchi, HIP 84405B, SAO 185199, HD 155885, GC 23274, HR 6401, DM CD-26 12026B, TYC 6820-326-2",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "36 Ophiuchi",
	"OType" : "Double or multiple star",
	"Distance" : "5.93",
	"RA_S" : 258.83743307,
	"DEC_S" : -26.60282143,
	"X" : 335,
	"Y" : 642,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.33,
	"key" : 67189,
	"title" : "36 Ophiuchi"
	},
{
	"Index" : "34117",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "41 Ophiuchi, HIP 84514A, SAO 141586, HD 156266, GC 23320, HR 6415, DM BD-00  3255, TYC 5066-1267-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "41 Ophiuchi",
	"OType" : "Double or multiple star",
	"Distance" : "62.99",
	"RA_S" : 259.15286365,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.915,
	"key" : 54117,
	"title" : "41 Ophiuchi"
	},
{
	"Index" : "47111",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "39 Ophiuchi, Omicron Ophiuchi, HIP 84626A, SAO 185238, HD 156349, GC 23344, HR 6424, DM CD-24 13255A, TYC 6812-592-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Omicron Ophiuchi",
	"OType" : "Star",
	"Distance" : "89.37",
	"RA_S" : 259.50283629,
	"DEC_S" : -24.28690589,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.23,
	"key" : 67111,
	"title" : "Omicron Ophiuchi"
	},
{
	"Index" : "71445",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "66 Herculis, e Ophiuchi, HIP 84671, SAO 102725, HD 156681, GC 23382, HR 6433, DM BD+11  3156, TYC 982-2322-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "e Ophiuchi",
	"OType" : "Variable Star",
	"Distance" : "150.55",
	"RA_S" : 259.65412797,
	"DEC_S" : 10.86447427,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.203,
	"key" : 91445,
	"title" : "e Ophiuchi"
	},
{
	"Index" : "42797",
	"Description" : "Xi Ophiuchi (\u03BE Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.39.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "40 Ophiuchi, Xi Ophiuchi, HIP 84893, SAO 185296, HD 156897, GC 23423, HR 6445, DM BD-20  4731, TYC 6246-664-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Xi Ophiuchi",
	"OType" : "Star",
	"Distance" : "17.35",
	"RA_S" : 260.250921,
	"DEC_S" : -21.112433,
	"X" : 319,
	"Y" : 574,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.431,
	"key" : 62797,
	"title" : "Xi Ophiuchi"
	},
{
	"Index" : "47252",
	"Description" : "Theta Ophiuchi (\u03B8 Oph, \u03B8 Ophiuchi) is a multiple star system in the equatorial constellation of Ophiuchus. It lies on the \u0022right foot\u0022 of the serpent-bearer, and is only a little to the southwest of the Kepler\u0027s Star, the nova of 1604. According to Richard H. Allen\u0027s, Star Names: Their Lore and Meaning (1899), \u03B8 Oph together with \u03BE Oph formed the Sogdian Wajrik \u0022the Magician\u0022, the Khorasmian Markhashik \u0022the Serpent-bitten\u0022 and with \u03B7 Oph the Coptic Tshi\u014D, \u0022the Snake\u0022, and Aggia, \u0022the Magician\u0022. This star has an apparent visual magnitude of +3.26, making it readily visible to the naked eye. Based upon parallax measurements from the Hipparcos mission, it is located at a distance of roughly 436 light-years (134 parsecs) from Earth.\r\rTheta Ophiuchi appears to be a triple star system. The brightest component is a spectroscopic binary with an orbital period of 56.71 days and an eccentricity of 0.17. The tertiary component is 5.5 magnitude star with a stellar classification of B5. It is located at an angular separation of 0.15 arcseconds from the binary pair. This system is a proper motion member of the Upper Scorpius sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.\r\rThe primary component of this system is a variable star of the Beta Cephei type with a short period of just 3h 22m. It has nearly nine times the mass of the Sun and more than six times the Sun\u0027s radius. Although only 21 million years old, it has begun to evolve away from the main sequence and has become a subgiant star with a stellar classification of B2 IV. This massive star is radiating around 5,000 times the luminosity of the Sun from its outer atmosphere at an effective temperature of about 22,260 K, giving it the blue-white hue of a B-type star.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "42 Ophiuchi, Theta Ophiuchi, HIP 84970, SAO 185320, HD 157056, GC 23451, HR 6453, DM CD-24 13292, TYC 6829-577-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Theta Ophiuchi",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "133.61",
	"RA_S" : 260.50241395,
	"DEC_S" : -24.99954638,
	"X" : 316,
	"Y" : 622,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.212,
	"key" : 67252,
	"title" : "Theta Ophiuchi"
	},
{
	"Index" : "47294",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "43 Ophiuchi, HIP 85084, SAO 185350, HD 157236, GC 23492, HR 6459, DM CD-28 13081, TYC 6837-698-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "43 Ophiuchi",
	"OType" : "Star",
	"Distance" : "248.25",
	"RA_S" : 260.83996101,
	"DEC_S" : -28.14283193,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.475,
	"key" : 67294,
	"title" : "43 Ophiuchi"
	},
{
	"Index" : "47230",
	"Description" : "44 Ophiuchi (44 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.17.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "44 Ophiuchi, b Ophiuchi, HIP 85340, SAO 185401, HD 157792, GC 23597, HR 6486, DM CD-24 13337, TYC 6825-462-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "44 Ophiuchi",
	"OType" : "Variable Star",
	"Distance" : "25.5",
	"RA_S" : 261.59256959,
	"DEC_S" : -24.17530784,
	"X" : 304,
	"Y" : 611,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.189,
	"key" : 67230,
	"title" : "44 Ophiuchi"
	},
{
	"Index" : "26352",
	"Description" : "Sigma Ophiuchi (\u03C3 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.34.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "49 Ophiuchi, Sigma Ophiuchi, HIP 85355, SAO 122387, HD 157999, GC 23621, HR 6498, DM BD+04  3422, TYC 409-1922-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Sigma Ophiuchi",
	"OType" : "Variable Star",
	"Distance" : "274.13",
	"RA_S" : 261.62866868,
	"DEC_S" : 4.14035686,
	"X" : 302,
	"Y" : 262,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.496,
	"key" : 46352,
	"title" : "Sigma Ophiuchi"
	},
{
	"Index" : "34148",
	"Description" : "47 Ophiuchi (47 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.50.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "47 Ophiuchi, HIP 85365, SAO 141665, HD 157950, GC 23617, HR 6493, DM BD-04  4275, TYC 5075-717-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "47 Ophiuchi",
	"OType" : "Spectroscopic binary",
	"Distance" : "30.07",
	"RA_S" : 261.65783725,
	"DEC_S" : -5.08659722,
	"X" : 301,
	"Y" : 375,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.569,
	"key" : 54148,
	"title" : "47 Ophiuchi"
	},
{
	"Index" : "47297",
	"Description" : "45 Ophiuchi (45 Oph) is a star in the constellation Ophiuchus. Its apparent magnitude is 4.29.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "45 Ophiuchi, d Ophiuchi, HIP 85423, SAO 185412, HD 157919, GC 23627, HR 6492, DM CD-29 13557, TYC 6838-1112-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "45 Ophiuchi",
	"OType" : "Star",
	"Distance" : "34.21",
	"RA_S" : 261.83864112,
	"DEC_S" : -29.86703242,
	"X" : 301,
	"Y" : 682,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.317,
	"key" : 67297,
	"title" : "45 Ophiuchi"
	},
{
	"Index" : "25641",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "HIP 85537, SAO 122418, HD 158352, GC 23677, HR 6507, DM BD+00 3697, TYC 401-2211-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "HR 6507",
	"OType" : "High proper-motion Star",
	"Distance" : "59.61",
	"RA_S" : 262.20689477,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.442,
	"key" : 45641,
	"title" : "HR 6507"
	},
{
	"Index" : "47236",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "51 Ophiuchi, c Ophiuchi, HIP 85755, SAO 185470, HD 158643, GC 23717, HR 6519, DM CD-23 13412, TYC 6826-368-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "c Ophiuchi",
	"OType" : "Be Star",
	"Distance" : "124.25",
	"RA_S" : 262.85397159,
	"DEC_S" : -23.96264277,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.795,
	"key" : 67236,
	"title" : "c Ophiuchi"
	},
{
	"Index" : "38467",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "57 Ophiuchi, Mu Ophiuchi, HIP 86284, SAO 141772, HD 159975, GC 23889, HR 6567, DM BD-08  4472, TYC 5660-589-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Mu Ophiuchi",
	"OType" : "Star",
	"Distance" : "230.89",
	"RA_S" : 264.46130695,
	"DEC_S" : -8.11876693,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.616,
	"key" : 58467,
	"title" : "Mu Ophiuchi"
	},
{
	"Index" : "42875",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "58 Ophiuchi, HIP 86736, SAO 185660, HD 160915, GC 24030, HR 6595, DM BD-21  4712, TYC 6260-2072-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "58 Ophiuchi",
	"OType" : "Star",
	"Distance" : "17.65",
	"RA_S" : 265.85747375,
	"DEC_S" : -21.68319388,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.914,
	"key" : 62875,
	"title" : "58 Ophiuchi"
	},
{
	"Index" : "27389",
	"Description" : "Beta Ophiuchi (\u03B2 Oph, \u03B2 Ophiuchi) is a star in the equatorial constellation of Ophiuchus. It has the traditional names Celbalrai, which comes from the Arabic \u0643\u0644\u0628 \u0627\u0644\u0631\u0627\u0639\u064A kalb al-r\u0101\u0027\u012B meaning \u0022shepherd dog\u0022. It is also called Cheleb, Kelb Alrai, or sometimes just Alrai. the apparent visual magnitude of this star is 2.7, which is readily visible to the naked eye even from urban skies. The distance to this star can be estimated using parallax measurements, yielding a value of 81.8 light-years (25.1 parsecs).\r\rThis is a giant star with a stellar classification of K2 III. Although it is only 13% greater in mass than the Sun, it has reached a stage in its evolution where the atmosphere has expanded to about 12 times the Sun\u0027s radius and is radiating 63 times the luminosity of the Sun. Its outer envelope is relatively cool with an effective temperature of 4,467 K, giving it the orange hue typical of K-type stars. Like some other K-type giants, \u03B2 Ophiuchi has been found to vary very slightly (0.02 magnitudes) in brightness.,\r\rCebalrai is a member of the thin disk population. It is following a low eccentricity orbit through the Milky Way galaxy that carries it between a distance of 27.3\u201330.9 kly (8.4\u20139.5 kpc) from the Galactic Center and up to 0.62 kly (0.19 kpc) above or below the galactic plane.\r\rRadial velocity variations with a period of 142 days hint about the possible presence of a planetary companion orbiting Beta Ophiuchi. Thus far, no planetary object has been confirmed; while periodic radial pulsations caused by intrinsic stellar variability could explain the observed variations.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "60 Ophiuchi, Beta Ophiuchi, HIP 86742, SAO 122671, HD 161096, GC 24048, HR 6603, DM BD+04  3489, TYC 423-1724-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Celbalrai",
	"OType" : "Variable Star",
	"Distance" : "25.09",
	"RA_S" : 265.86813614,
	"DEC_S" : 4.56730027,
	"X" : 249,
	"Y" : 257,
	"Constellation" : "Ophiuchus ",
	"AMag" : 2.879,
	"key" : 47389,
	"shortTitle" : "Kelb Alrai; Kabalrai; Cheleb; Celb-al-Rai; Tsel'bal'raj; Tsebal'raj",
	"title" : "Celbalrai"
	},
{
	"Index" : "27186",
	"Description" : "Gamma Ophiuchi (\u03B3 Oph, \u03B3 Ophiuchi) is a fourth-magnitude star in the constellation Ophiuchus. It is located about 95 light-years from Earth. The system has an age of roughly 184 million years.\r\rThis is an A-type main sequence star with a stellar classification of A0 V. It has nearly three times the mass of the Sun and 1.8 times the Sun\u0027s radius. The star shines with 29 times the luminosity of the Sun, which is being emitted from its outer atmosphere at an effective temperature of 9,506 K. It is radiating an excess emission of infrared, suggesting the presence of a circumstellar disk of dust at an orbital radius of 64 AU from the host star.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "62 Ophiuchi, Gamma Ophiuchi, HIP 87108, SAO 122754, HD 161868, GC 24162, HR 6629, DM BD+02  3403, TYC 420-1962-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Gamma Ophiuchi",
	"OType" : "High proper-motion Star",
	"Distance" : "31.51",
	"RA_S" : 266.97316954,
	"DEC_S" : 2.70727672,
	"X" : 236,
	"Y" : 280,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.737,
	"key" : 47186,
	"title" : "Gamma Ophiuchi"
	},
{
	"Index" : "38556",
	"Description" : "Nu Ophiuchi (\u03BD Oph, \u03BD Ophiuchi) is a star in the equatorial constellation of Ophiuchus. This star is sometimes called by the name Sinistra, meaning left side in Latin. The apparent visual magnitude is +3.3, making it one of the brighter members of this constellation. Based upon parallax measurements made during the Hipparcos mission, this star is located about 151 light-years (46 parsecs) from Earth.\r\rIn China, the star is part of \u5929\u5E02\u5DE6\u57A3 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n), meaning Left Wall of Heavenly Market Enclosure. The stars in this group include \u03BD Ophiuchi, \u03B4 Herculis, \u03BB Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B6 Aquilae, \u03B81 Serpentis, \u03B7 Serpentis, \u03BE Serpentis and \u03B7 Ophiuchi. Consequently, \u03BD Ophiuchi itself is known as \u5929\u5E02\u5DE6\u57A3\u4E5D (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n ji\u01D4, English: the Ninth Star of Left Wall of Heavenly Market Enclosure), and together with \u03B6 Capricorni represents the state Yan (\u71D5) in the Twelve States constellation. Nu Ophiuchi has about three times the mass of the Sun and is roughly 330 million years old. The spectrum of the star matches a stellar classification of K0 IIIa, indicating it is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence of stars like the Sun. Unusually, it displays an anomalously low abundance of cyanogen for a star of its type. The star\u0027s outer envelope has expanded to around 14 times the Sun\u0027s radius and now radiates 123 times as much luminosity of the Sun. This energy is being emitted from its outer envelope at an effective temperature of 4,928 K, giving it the cool, orange hue of a K-type star.\r\rThis is not a binary star system in the sense of having a gravitationally-bound stellar companion. However, in early 2004, a brown dwarf companion Nu Ophiuchi b was discovered. This sub-stellar companion has at least 21.9 times the mass of Jupiter and takes 536 days (1.47 years) to complete an orbit. A second brown dwarf companion was discovered in 2010, orbiting further from the star with a period of 3,169 days (8.68 years). These have been confirmed in 2012.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "64 Ophiuchi, Nu Ophiuchi, HIP 88048, SAO 142004, HD 163917, GC 24468, HR 6698, DM BD-09  4632, TYC 5678-956-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Nu Ophiuchi",
	"OType" : "Star",
	"Distance" : "46.2",
	"RA_S" : 269.75663133,
	"DEC_S" : -9.7736295,
	"X" : 203,
	"Y" : 435,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.42,
	"key" : 58556,
	"title" : "Nu Ophiuchi"
	},
{
	"Index" : "28705",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "66 Ophiuchi, HIP 88149, SAO 123005, HD 164284, GC 24500, HR 6712, DM BD+04  3570, TYC 438-2741-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "66 Ophiuchi",
	"OType" : "Be Star",
	"Distance" : "288.92",
	"RA_S" : 270.06582784,
	"DEC_S" : 4.36861876,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.742,
	"key" : 48705,
	"title" : "66 Ophiuchi"
	},
{
	"Index" : "28442",
	"Description" : "67 Ophiuchi (67 Oph) is a Class B5 fourth-magnitude star in the constellation Ophiuchus. It is considered to be a member of the open cluster Collinder 359 (Melotte 186).",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "67 Ophiuchi, HIP 88192, SAO 123013, HD 164353, GC 24509, HR 6714, DM BD+02  3458, TYC 434-5198-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "67 Ophiuchi",
	"OType" : "Star",
	"Distance" : "305.94",
	"RA_S" : 270.16131625,
	"DEC_S" : 2.93156477,
	"X" : 196,
	"Y" : 278,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.959,
	"key" : 48442,
	"title" : "67 Ophiuchi"
	},
{
	"Index" : "28105",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "68 Ophiuchi, HIP 88290AB, SAO 123035, HD 164577, GC 24534, HR 6723, DM BD+01  3560, TYC 430-3748-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "68 Ophiuchi",
	"OType" : "Star",
	"Distance" : "89.38",
	"RA_S" : 270.43832947,
	"DEC_S" : 1.30506816,
	"X" : 192,
	"Y" : 298,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.432,
	"key" : 48105,
	"title" : "68 Ophiuchi"
	},
{
	"Index" : "38539",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "69 Ophiuchi, Tau Ophiuchi, HIP 88404A, SAO 142050, HD 164765, GC 24565, HR 6734, DM BD-08  4549B, TYC 5675-662-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "Tau Ophiuchi",
	"OType" : "Spectroscopic binary",
	"Distance" : "51.26",
	"RA_S" : 270.77033367,
	"DEC_S" : -8.18034956,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.269,
	"key" : 58539,
	"title" : "Tau Ophiuchi"
	},
{
	"Index" : "28446",
	"Description" : "70 Ophiuchi a binary star system located 16.6 light years away from the Earth. It is in the constellation Ophiuchus. At magnitude 4 it is a typical less bright star usually visible to the unaided eye away from city lights. The primary star is a yellow-orange main sequence dwarf BY Draconis variable of spectral type K0, and the secondary star is an orange main sequence dwarf of spectral type K4. The two stars orbit each other at an average distance of 23.2 AUs. But since the orbit is highly elliptical (at e=0.499), the separation between the two varies from 11.4 to 34.8 AUs, with one orbit taking 83.38 years to complete.\r\rThis star system was first cataloged by William Herschel in the late 18th century in his study of binary stars. Herschel proved that this system as a gravitationally bound binary system where the two stars orbited around a common center of mass. This was an important contribution to the proof that Newton\u0027s law of universal gravitation applied to objects beyond the solar system. He commented at the time that there was a possible third unseen companion affecting the orbit of the two visible stars.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "70 Ophiuchi, p Ophiuchi, HIP 88601A, SAO 123107, HD 165341A, GC 24641, HR 6752, DM BD+02  3482, TYC 434-5213-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "70 Ophiuchi",
	"OType" : "High proper-motion Star",
	"Distance" : "5.08",
	"RA_S" : 271.36404409,
	"DEC_S" : 2.49979492,
	"X" : 181,
	"Y" : 283,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.217,
	"key" : 48446,
	"title" : "70 Ophiuchi"
	},
{
	"Index" : "28445",
	"Description" : "70 Ophiuchi a binary star system located 16.6 light years away from the Earth. It is in the constellation Ophiuchus. At magnitude 4 it is a typical less bright star usually visible to the unaided eye away from city lights. The primary star is a yellow-orange main sequence dwarf BY Draconis variable of spectral type K0, and the secondary star is an orange main sequence dwarf of spectral type K4. The two stars orbit each other at an average distance of 23.2 AUs. But since the orbit is highly elliptical (at e=0.499), the separation between the two varies from 11.4 to 34.8 AUs, with one orbit taking 83.38 years to complete.\r\rThis star system was first cataloged by William Herschel in the late 18th century in his study of binary stars. Herschel proved that this system as a gravitationally bound binary system where the two stars orbited around a common center of mass. This was an important contribution to the proof that Newton\u0027s law of universal gravitation applied to objects beyond the solar system. He commented at the time that there was a possible third unseen companion affecting the orbit of the two visible stars.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "70 Ophiuchi, p Ophiuchi, HIP 88601B, SAO 123107, HD 165341B, GC 24641, HR 6752, DM BD+02  3482, TYC 434-5212-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "70 Ophiuchi",
	"OType" : "High proper-motion Star",
	"Distance" : "5.08",
	"RA_S" : 271.364254,
	"DEC_S" : 2.499006,
	"X" : 181,
	"Y" : 283,
	"Constellation" : "Ophiuchus ",
	"AMag" : 6.17,
	"key" : 48445,
	"title" : "70 Ophiuchi"
	},
{
	"Index" : "56",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "71 Ophiuchi, HIP 88765, SAO 123140, HD 165760, GC 24693, HR 6770, DM BD+08  3582, TYC 1008-1945-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "71 Ophiuchi",
	"OType" : "Star",
	"Distance" : "83.56",
	"RA_S" : 271.82649942,
	"DEC_S" : 8.7338679,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.745,
	"key" : 20056,
	"title" : "71 Ophiuchi"
	},
{
	"Index" : "88",
	"Description" : "72 Ophiuchi (72 Oph) is a Class A4, fourth-magnitude star in the constellation Ophiuchus. 72 Ophiuchi is a multiple star system of several components, located about 85 light-years from Earth.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "72 Ophiuchi, HIP 88771, SAO 123142, HD 165777, GC 24695, HR 6771, DM BD+09  3564, TYC 1012-1661-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "72 Ophiuchi",
	"OType" : "Star",
	"Distance" : "26.63",
	"RA_S" : 271.83743304,
	"DEC_S" : 9.56384725,
	"X" : 176,
	"Y" : 195,
	"Constellation" : "Ophiuchus ",
	"AMag" : 3.722,
	"key" : 20088,
	"title" : "72 Ophiuchi"
	},
{
	"Index" : "28577",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "74 Ophiuchi, HIP 89918, SAO 123377, HD 168656, GC 25036, HR 6866, DM BD+03  3680, TYC 436-3545-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "74 Ophiuchi",
	"OType" : "Star",
	"Distance" : "79.81",
	"RA_S" : 275.21692256,
	"DEC_S" : 3.37716851,
	"Constellation" : "Ophiuchus ",
	"AMag" : 4.957,
	"key" : 48577,
	"title" : "74 Ophiuchi"
	},
{
	"Index" : "187",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "HIP 91217, SAO 123690, HD 171802, GC 25422, HR 6985, DM BD+09 3783, TYC 1024-3216-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "HR 6985",
	"OType" : "Spectroscopic binary",
	"Distance" : "38.49",
	"RA_S" : 279.11598158,
	"DEC_S" : 9.12249652,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.419,
	"key" : 20187,
	"title" : "HR 6985"
	},
{
	"Index" : "30307",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "HIP 91237, SAO 123693, HD 171834, GC 25427, HR 6987, DM BD+06 3855, TYC 458-1851-1",
	"group" : { "key" : "Ophiuchus" },
	"Common" : "HR 6987",
	"OType" : "Variable Star of gamma Dor type",
	"Distance" : "33.08",
	"RA_S" : 279.16281192,
	"DEC_S" : 6.67180631,
	"Constellation" : "Ophiuchus ",
	"AMag" : 5.469,
	"key" : 50307,
	"title" : "HR 6987"
	},
{
	"Index" : "47623",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 22044, SAO 94095, HD 30034, GC 5767, HR 1507, DM BD+10  621, TYC 687-1627-1",
	"group" : { "backgroundImage" : "images/Alignment/33.png",
		"description" : "Orion, representing the Hunter, is a prominent constellation located on the celestial equator and visible throughout the world. It is one of the most conspicuous and most recognizable constellations in the night sky. Its name refers to Orion, a hunter in Greek mythology. Its brightest stars are Beta (Rigel) and Alpha (Betelgeuse), a blue-white and red supergiant respectively. Many other of the brightest stars in the constellation are hot blue supergiant stars.\r\rThe distinctive pattern of Orion has been recognized in numerous cultures around the world, and many myths have been associated with it. It has also been used as a symbol in the modern world.\r\rThe Babylonian star catalogues of the Late Bronze Age name Orion MULSIPA.ZI.AN.NA,[note 1] \u0022The Heavenly Shepherd\u0022 or \u0022True Shepherd of Anu\u0022 - Anu being the chief god of the heavenly realms. The Babylonian constellation was sacred to Papshukal and Ninshubur, both minor gods fulfilling the role of \u0027messenger to the gods\u0027. Papshukal was closely associated with the figure of a walking bird on Babylonian boundary stones, and on the star map the figure of the Rooster was located below and behind the figure of the True Shepherd\u2014both constellations represent the herald of the gods, in his bird and human forms respectively.\r\rThe stars of Orion were associated with Osiris, the sun-god of rebirth and afterlife, by the ancient Egyptians.\r\rOrion has also been identified with the Egyptian Pharaoh of the Fifth Dynasty called Unas who, according to the Pyramid Texts, became great by eating the flesh of his mortal enemies and then slaying and devouring the gods themselves. This was based on a belief in contiguous magic whereby consuming the flesh of great people would bring inheritance of their power. After devouring the gods and absorbing their spirits and powers, Unas journeys through the day and night sky to become the star Sahu, or Orion. The Pyramid Texts also show that the dead Pharaoh was identified with the god Osiris, whose form in the stars was often said to be the constellation Orion.\r\rThe Armenians identified their forefather Hayk with Orion. Hayk is also the name of the Orion constellation in the Armenian translation of the Bible.\r\rThe Bible mentions Orion three times, naming it \u0022Kesil\u0022 (\u05DB\u05E1\u05D9\u05DC, literally - fool). Though, this name perhaps is etymologically connected with \u0022Kislev\u0022, the name for the ninth month of the Hebrew calendar (i.e. November\u2013December), which, in turn, may derive from the Hebrew root K-S-L as in the words \u0022kesel, kisla\u0022 (\u05DB\u05B5\u05BC\u05E1\u05B6\u05DC, \u05DB\u05B4\u05BC\u05E1\u05B0\u05DC\u05B8\u05D4, hope, positiveness), i.e. hope for winter rains.): Job 9:9 (\u0022He is the maker of the Bear and Orion\u0022), Job 38:31 (\u0022Can you loosen Orion`s belt?\u0022), and Amos 5:8 (\u0022He who made the Pleiades and Orion\u0022). In ancient Aram, the constellation was known as Neph\u00EEl\u0101\u2032, the Nephilim may have been Orion\u0027s descendants.\r\rOrion\u0027s current name derives from Greek mythology, in which Orion was a gigantic, supernaturally strong hunter of primordial times, born to Euryale, a nymph, and Poseidon (Neptune), god of the sea in the Greco-Roman tradition. One myth recounts Gaia\u0027s rage at Orion, who dared to say that he would kill every animal on the planet. The angry goddess tried to dispatch Orion with a scorpion, the reason that the constellations of Scorpius and Orion are never in the sky at the same time. However, Ophiuchus (disambiguation), the Serpent Bearer, revived Orion with an antidote, the reason that the constellation of Ophiuchus stands midway between the Scorpion and the Hunter in the sky.\r\rThe constellation is mentioned in Horace\u0027s Odes (Ode 3.27.18), Homer\u0027s Odyssey (Book 5, line 283) and Iliad, and Virgil\u0027s Aeneid (Book 1, line 535)\r\rIn ancient Egypt, the constellation of Orion was known to represent Osiris, who, after being killed by his evil brother Set, was revived by his wife Isis to live immortal among the stars.",
		"key" : "Orion",
		"grouptype" : "Orion",
		"Meaning" : "Orion (mythological character)",
		"Family" : "Orion",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Orion",
		"title" : "Orion Objects Group" },
	"Common" : "HR 1507",
	"OType" : "Variable Star",
	"Distance" : "45.82",
	"RA_S" : 71.1076161,
	"DEC_S" : 11.14613604,
	"Constellation" : "Orion ",
	"AMag" : 5.41,
	"key" : 67623,
	"title" : "HR 1507"
	},
{
	"Index" : "47861",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 22157, SAO 94111, HD 30210, GC 5802, HR 1519, DM BD+11  646, TYC 691-1509-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1519",
	"OType" : "High proper-motion Star",
	"Distance" : "72.09",
	"RA_S" : 71.5072524,
	"DEC_S" : 11.70558946,
	"Constellation" : "Orion ",
	"AMag" : 5.367,
	"key" : 67861,
	"title" : "HR 1519"
	},
{
	"Index" : "71332",
	"Description" : "Pi3 Orionis (\u03C03 Ori, \u03C03 Orionis) is the Bayer designation for a star in the equatorial constellation of Orion. It has the traditional name of Tabit and the Flamsteed designation 1 Orionis. At an apparent visual magnitude of 3.16, it is readily visible to the naked eye. Pi3 Orionis is the brightest star in the lion\u0027s hide (or shield) that Orion is holding. The distance to this star, as measured using the parallax technique, is 26.32 light-years (8.07 parsecs). Though no extrasolar planets have been observed around Pi3 Orionis, the star is considered[who?] a prime location for planets as small as the Earth.\r\rPi3 Orionis is a main-sequence star of spectral type F6 V. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Compared to the Sun, it has about 124% of the mass, 132% of the radius, and nearly 3 times the luminosity. This energy is being radiated from the star\u0027s outer atmosphere at an effective temperature of 6,516 K, giving it the yellow-white glow of an F-type star. Pi3 Orionis is most likely single; a nearby star is probably an optical companion.\r\rAlthough a periodicity of 73.26 days has been observed in the star\u0027s radial velocity, it seems likely to be bound more to stellar activity than to a planetary object in close orbit. No substellar companion has been detected so far around Pi3 Orionis and the McDonald Observatory team has set limits to the presence of one or more planets with masses between 0.84 and 46.7 Jupiter masses and average separations spanning between 0.05 and 5.2 astronomical units. Thus, so far it appears that an Earth-like planet could easily orbit the star without any complications caused by a gravitationally perturbing body.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "1 Orionis, Pi03 Orionis, HIP 22449, SAO 112106, HD 30652, GC 5875, HR 1543, DM BD+06   762, TYC 96-1462-1",
	"group" : { "key" : "Orion" },
	"Common" : "Tabit",
	"OType" : "Variable Star",
	"Distance" : "8.07",
	"RA_S" : 72.46004311,
	"DEC_S" : 6.96127723,
	"X" : 667,
	"Y" : 311,
	"Constellation" : "Orion ",
	"AMag" : 3.222,
	"key" : 91332,
	"title" : "Tabit"
	},
{
	"Index" : "47258",
	"Description" : "Pi2 Orionis (\u03C02 Ori, \u03C02 Orionis), also known as Tabit (1544), is a star in the constellation Orion.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "2 Orionis, Pi02 Orionis, HIP 22509, SAO 112124, HD 30739, GC 5892, HR 1544, DM BD+08   777, TYC 683-1217-1",
	"group" : { "key" : "Orion" },
	"Common" : "Tabit (1544)",
	"OType" : "Star",
	"Distance" : "68.77",
	"RA_S" : 72.6530041,
	"DEC_S" : 8.90017727,
	"X" : 664,
	"Y" : 286,
	"Constellation" : "Orion ",
	"AMag" : 4.343,
	"key" : 67258,
	"title" : "Tabit (1544)"
	},
{
	"Index" : "69141",
	"Description" : "Pi4 Orionis (\u03C04 Ori, \u03C04 Orionis) is a spectroscopic binary star in the constellation Orion. It is about 1,300 light years away and is one of the most luminous stars known. It is one of a series of stars that share the Bayer designation Pi Orionis.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "3 Orionis, Pi04 Orionis, HIP 22549, SAO 112142, HD 30836, GC 5911, HR 1552, DM BD+05   745, TYC 92-2345-1",
	"group" : { "key" : "Orion" },
	"Common" : "Pi4 Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "321.28",
	"RA_S" : 72.80151656,
	"DEC_S" : 5.60510315,
	"X" : 663,
	"Y" : 329,
	"Constellation" : "Orion ",
	"AMag" : 3.638,
	"key" : 89141,
	"title" : "Pi4 Orionis"
	},
{
	"Index" : "48167",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "4 Orionis, Omicron01 Orionis, HIP 22667, SAO 94176, HD 30959, GC 5942, HR 1556, DM BD+14   777, TYC 696-1788-1",
	"group" : { "key" : "Orion" },
	"Common" : "Omicron01 Orionis",
	"OType" : "S Star",
	"Distance" : "194.9",
	"RA_S" : 73.1331831,
	"DEC_S" : 14.25064331,
	"Constellation" : "Orion ",
	"AMag" : 4.941,
	"key" : 68167,
	"title" : "Omicron01 Orionis"
	},
{
	"Index" : "66008",
	"Description" : "Pi5 Orionis (\u03C05 Ori, \u03C05 Orionis) is a star in the constellation Orion.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "8 Orionis, Pi05 Orionis, HIP 22797, SAO 112197, HD 31237, GC 5978, HR 1567, DM BD+02   810, TYC 89-2558-1",
	"group" : { "key" : "Orion" },
	"Common" : "Pi5 Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "399.18",
	"RA_S" : 73.56290018,
	"DEC_S" : 2.44067308,
	"X" : 653,
	"Y" : 370,
	"Constellation" : "Orion ",
	"AMag" : 3.657,
	"key" : 86008,
	"title" : "Pi5 Orionis"
	},
{
	"Index" : "47913",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "6 Orionis, g Orionis, HIP 22833, SAO 94197, HD 31283, GC 5983, HR 1569, DM BD+11   675, TYC 692-1664-1",
	"group" : { "key" : "Orion" },
	"Common" : "g Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "69.93",
	"RA_S" : 73.69540173,
	"DEC_S" : 11.42601608,
	"Constellation" : "Orion ",
	"AMag" : 5.199,
	"key" : 67913,
	"title" : "g Orionis"
	},
{
	"Index" : "47406",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 22834, SAO 112203, HD 31296, GC 5986, HR 1571, DM BD+07  755, TYC 684-906-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1571",
	"OType" : "Variable Star",
	"Distance" : "147.36",
	"RA_S" : 73.69908844,
	"DEC_S" : 7.77909863,
	"Constellation" : "Orion ",
	"AMag" : 5.46,
	"key" : 67406,
	"title" : "HR 1571"
	},
{
	"Index" : "47706",
	"Description" : "Pi1 Orionis (\u03C01 Ori, \u03C01 Orionis), also known as Tabit (1570), is a star in the constellation Orion.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "7 Orionis, Pi01 Orionis, HIP 22845, SAO 94201, HD 31295, GC 5987, HR 1570, DM BD+09   683, TYC 688-1867-1",
	"group" : { "key" : "Orion" },
	"Common" : "Tabit (1570)",
	"OType" : "High proper-motion Star",
	"Distance" : "35.66",
	"RA_S" : 73.72386559,
	"DEC_S" : 10.15083236,
	"X" : 650,
	"Y" : 270,
	"Constellation" : "Orion ",
	"AMag" : 4.659,
	"key" : 67706,
	"title" : "Tabit (1570)"
	},
{
	"Index" : "48169",
	"Description" : "Omicron2 Orionis (\u03BF2 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.09.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "9 Orionis, Omicron02 Orionis, HIP 22957, SAO 94218, HD 31421, GC 6025, HR 1580, DM BD+13   740, TYC 696-1790-1",
	"group" : { "key" : "Orion" },
	"Common" : "Omicron2 Orionis",
	"OType" : "Star",
	"Distance" : "57",
	"RA_S" : 74.09281277,
	"DEC_S" : 13.51446669,
	"X" : 644,
	"Y" : 225,
	"Constellation" : "Orion ",
	"AMag" : 4.2,
	"key" : 68169,
	"title" : "Omicron2 Orionis"
	},
{
	"Index" : "62010",
	"Description" : "Pi6 Orionis (\u03C06 Ori, \u03C06 Orionis) is a star in the constellation Orion.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "10 Orionis, Pi06 Orionis, HIP 23123, SAO 112281, HD 31767, GC 6068, HR 1601, DM BD+01   872, TYC 85-2362-1",
	"group" : { "key" : "Orion" },
	"Common" : "Pi6 Orionis",
	"OType" : "Variable Star",
	"Distance" : "287.25",
	"RA_S" : 74.63708788,
	"DEC_S" : 1.71401474,
	"X" : 639,
	"Y" : 379,
	"Constellation" : "Orion ",
	"AMag" : 4.62,
	"key" : 82010,
	"title" : "Pi6 Orionis"
	},
{
	"Index" : "2232",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "11 Orionis, HIP 23607, SAO 94290, HD 32549, GC 6191, HR 1638, DM BD+15   732, TYC 1282-2292-1",
	"group" : { "key" : "Orion" },
	"Common" : "11 Orionis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "111.89",
	"RA_S" : 76.14228976,
	"DEC_S" : 15.40410506,
	"Constellation" : "Orion ",
	"AMag" : 4.652,
	"key" : 22232,
	"title" : "11 Orionis"
	},
{
	"Index" : "48340",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "14 Orionis, i Orionis, HIP 23879AB, SAO 112440, HD 33054, GC 6269, HR 1664, DM BD+08   866, TYC 698-2328-1",
	"group" : { "key" : "Orion" },
	"Common" : "i Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "58.95",
	"RA_S" : 76.97034709,
	"DEC_S" : 8.49846569,
	"Constellation" : "Orion ",
	"AMag" : 5.475,
	"key" : 68340,
	"title" : "i Orionis"
	},
{
	"Index" : "48719",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "16 Orionis, h Orionis, HIP 23983, SAO 112467, HD 33254, GC 6300, HR 1672, DM BD+09   743, TYC 702-2789-1",
	"group" : { "key" : "Orion" },
	"Common" : "h Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "54.68",
	"RA_S" : 77.33184259,
	"DEC_S" : 9.82958059,
	"Constellation" : "Orion ",
	"AMag" : 5.452,
	"key" : 68719,
	"title" : "h Orionis"
	},
{
	"Index" : "2231",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "15 Orionis, HIP 24010, SAO 94359, HD 33276, GC 6306, HR 1676, DM BD+15   752, TYC 1282-2291-1",
	"group" : { "key" : "Orion" },
	"Common" : "15 Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "96.64",
	"RA_S" : 77.42483871,
	"DEC_S" : 15.59723483,
	"Constellation" : "Orion ",
	"AMag" : 4.85,
	"key" : 22231,
	"title" : "15 Orionis"
	},
{
	"Index" : "2230",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 24197, SAO 94377, HD 33554, GC 6350, HR 1684, DM BD+15  759, TYC 1282-2290-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1684",
	"OType" : "Star",
	"Distance" : "105.15",
	"RA_S" : 77.92318236,
	"DEC_S" : 16.04567266,
	"Constellation" : "Orion ",
	"AMag" : 5.348,
	"key" : 22230,
	"title" : "HR 1684"
	},
{
	"Index" : "262",
	"Description" : "Rho Orionis (\u03C1 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.48.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "17 Orionis, Rho Orionis, HIP 24331A, SAO 112528, HD 33856A, GC 6381, HR 1698, DM BD+02   888, TYC 103-2863-1",
	"group" : { "key" : "Orion" },
	"Common" : "Rho Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.44",
	"RA_S" : 78.3228378,
	"DEC_S" : 2.8612555,
	"X" : 592,
	"Y" : 365,
	"Constellation" : "Orion ",
	"AMag" : 4.62,
	"key" : 20262,
	"title" : "Rho Orionis"
	},
{
	"Index" : "265",
	"Description" : "Rho Orionis (\u03C1 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.48.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "17 Orionis, Rho Orionis, HIP 24331B, SAO 112528, HD 33856B, GC 6381, HR 1698, DM BD+02   888, TYC 103-2874-1",
	"group" : { "key" : "Orion" },
	"Common" : "Rho Orionis",
	"OType" : "Star",
	"Distance" : "104.44",
	"RA_S" : 78.324558,
	"DEC_S" : 2.862125,
	"X" : 592,
	"Y" : 365,
	"Constellation" : "Orion ",
	"AMag" : 8.498,
	"key" : 20265,
	"title" : "Rho Orionis"
	},
{
	"Index" : "31797",
	"Description" : "Tau Orionis (\u03C4 Ori, \u03C4 Orionis) is a star in the constellation Orion.\r\rThis star, along with \u03B2 Eri, \u03BB Eri and \u03C8 Eri were Al Kursiyy al Jauzah, \u0022the Chair (or \u0022Footstool\u0022) of the Central One\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Kursiyy al Jauzah were the title for three stars :\u03B2 Eri as Cursa, \u03C8 Eri as Al Kursiyy al Jauzah I and \u03BB Eri as Al Kursiyy al Jauzah II (exclude this star)\r\rIn Chinese, \u7389\u4E95 (Y\u00F9 J\u01D0ng), meaning Jade Well, refers to an asterism consisting of \u03C4 Orionis, \u03B2 Eridani, \u03BB Eridani and \u03C8 Eridani. Consequently, \u03C4 Orionis itself is known as \u7389\u4E95\u56DB (Y\u00F9 J\u01D0ng s\u00EC, English: the Fourth Star of Jade Well.). From this Chinese name, the name Yuh Tsing was appeared",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "20 Orionis, Tau Orionis, HIP 24674, SAO 131952, HD 34503, GC 6480, HR 1735, DM BD-07  1028, TYC 4764-1639-1",
	"group" : { "key" : "Orion" },
	"Common" : "Tau Orionis",
	"OType" : "Star",
	"Distance" : "151.42",
	"RA_S" : 79.40162482,
	"DEC_S" : -6.84440489,
	"X" : 577,
	"Y" : 491,
	"Constellation" : "Orion ",
	"AMag" : 3.556,
	"key" : 51797,
	"title" : "Tau Orionis"
	},
{
	"Index" : "352",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "21 Orionis, HIP 24817, SAO 112624, HD 34658, GC 6509, HR 1746, DM BD+02   916, TYC 104-3169-1",
	"group" : { "key" : "Orion" },
	"Common" : "21 Orionis",
	"OType" : "Variable Star",
	"Distance" : "61.91",
	"RA_S" : 79.79673986,
	"DEC_S" : 2.59580838,
	"Constellation" : "Orion ",
	"AMag" : 5.375,
	"key" : 20352,
	"title" : "21 Orionis"
	},
{
	"Index" : "31675",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "22 Orionis, o Orionis, HIP 25044, SAO 132028, HD 35039, GC 6579, HR 1765, DM BD-00   930, TYC 4752-1608-1",
	"group" : { "key" : "Orion" },
	"Common" : "o Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "347",
	"RA_S" : 80.44061154,
	"Constellation" : "Orion ",
	"AMag" : 4.678,
	"key" : 51675,
	"title" : "o Orionis"
	},
{
	"Index" : "451",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "23 Orionis, m Orionis, HIP 25142, SAO 112697, HD 35149, GC 6607, HR 1770, DM BD+03   871, TYC 105-2800-1",
	"group" : { "key" : "Orion" },
	"Common" : "m Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "384.02",
	"RA_S" : 80.70833914,
	"DEC_S" : 3.54444725,
	"Constellation" : "Orion ",
	"AMag" : 4.951,
	"key" : 20451,
	"title" : "m Orionis"
	},
{
	"Index" : "36047",
	"Description" : "29 Orionis (29 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.14.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "29 Orionis, e Orionis, HIP 25247, SAO 132067, HD 35369, GC 6646, HR 1784, DM BD-07  1064, TYC 5332-1832-1",
	"group" : { "key" : "Orion" },
	"Common" : "29 Orionis",
	"OType" : "Star",
	"Distance" : "48.24",
	"RA_S" : 80.98678228,
	"DEC_S" : -7.80805735,
	"X" : 557,
	"Y" : 504,
	"Constellation" : "Orion ",
	"AMag" : 4.237,
	"key" : 56047,
	"title" : "29 Orionis"
	},
{
	"Index" : "31736",
	"Description" : "Eta Orionis (\u03B7 Ori, \u03B7 Orionis) is a star in the constellation Orion. Other names are Saiph (Arabic for \u0022sword\u0022), Algjebbah (Arabic for \u0022scutum\u0022), and Ensis (Latin for \u0022sword\u0022, since the star is taken to represent Orion\u0027s sheathed weapon). Eta Orionis lies a little to the west of Orion\u0027s belt between Delta Orionis and Rigel, being closer to Delta Orionis than to Rigel. It lies at a distance of around 1,000 light years from Earth and is part of the Orion Arm.\r\rThis is a quadruple star system, of which three members can be resolved with a telescope. The primary component is an eclipsing binary star in a triple-star grouping. These stars have orbital periods of 8 days and 9.2 years. It includes a variable star with a pulsation period of around 8 hours. Three of the components are B-type main sequence stars with stellar classifications of B1 V, B3 V and B2 V.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "28 Orionis, Eta Orionis, HIP 25281A, SAO 132071, HD 35411, GC 6655, HR 1788, DM BD-02  1235, TYC 4757-1588-1",
	"group" : { "key" : "Orion" },
	"Common" : "Saiph / Algjebbah / Ensis",
	"OType" : "Spectroscopic binary",
	"Distance" : "341.3",
	"RA_S" : 81.119238,
	"DEC_S" : -2.397136,
	"X" : 555,
	"Y" : 433,
	"Constellation" : "Orion ",
	"AMag" : 3.564,
	"key" : 51736,
	"title" : "Saiph / Algjebbah / Ensis"
	},
{
	"Index" : "31737",
	"Description" : "Eta Orionis (\u03B7 Ori, \u03B7 Orionis) is a star in the constellation Orion. Other names are Saiph (Arabic for \u0022sword\u0022), Algjebbah (Arabic for \u0022scutum\u0022), and Ensis (Latin for \u0022sword\u0022, since the star is taken to represent Orion\u0027s sheathed weapon). Eta Orionis lies a little to the west of Orion\u0027s belt between Delta Orionis and Rigel, being closer to Delta Orionis than to Rigel. It lies at a distance of around 1,000 light years from Earth and is part of the Orion Arm.\r\rThis is a quadruple star system, of which three members can be resolved with a telescope. The primary component is an eclipsing binary star in a triple-star grouping. These stars have orbital periods of 8 days and 9.2 years. It includes a variable star with a pulsation period of around 8 hours. Three of the components are B-type main sequence stars with stellar classifications of B1 V, B3 V and B2 V.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "28 Orionis, Eta Orionis, HIP 25281B, SAO 132071, HD 35411, GC 6655, HR 1788, DM BD-02  1235, TYC 4757-1588-2",
	"group" : { "key" : "Orion" },
	"Common" : "Saiph / Algjebbah / Ensis",
	"OType" : "Spectroscopic binary",
	"Distance" : "341.3",
	"RA_S" : 81.119704,
	"DEC_S" : -2.397033,
	"X" : 555,
	"Y" : 433,
	"Constellation" : "Orion ",
	"AMag" : 4.871,
	"key" : 51737,
	"title" : "Saiph / Algjebbah / Ensis"
	},
{
	"Index" : "31696",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "27 Orionis, p Orionis, HIP 25282, SAO 132070, HD 35410, GC 6654, HR 1787, DM BD-01   886, TYC 4753-1893-1",
	"group" : { "key" : "Orion" },
	"Common" : "p Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "57.03",
	"RA_S" : 81.12043571,
	"DEC_S" : -0.89133988,
	"Constellation" : "Orion ",
	"AMag" : 5.178,
	"key" : 51696,
	"title" : "p Orionis"
	},
{
	"Index" : "96",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "25 Orionis, Psi01 Orionis, HIP 25302, SAO 112734, HD 35439, GC 6660, HR 1789, DM BD+01  1005, TYC 101-2568-1",
	"group" : { "key" : "Orion" },
	"Common" : "Psi01 Orionis",
	"OType" : "Be Star",
	"Distance" : "351.13",
	"RA_S" : 81.18678122,
	"DEC_S" : 1.84644655,
	"Constellation" : "Orion ",
	"AMag" : 4.837,
	"key" : 20096,
	"title" : "Psi01 Orionis"
	},
{
	"Index" : "452",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "30 Orionis, Psi Orionis, HIP 25473A, SAO 112775, HD 35715, GC 6713, HR 1811, DM BD+02   962, TYC 105-2801-1",
	"group" : { "key" : "Orion" },
	"Common" : "Psi Orionis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "348.4321",
	"RA_S" : 81.70927011,
	"DEC_S" : 3.095646,
	"Constellation" : "Orion ",
	"AMag" : 4.574,
	"key" : 20452,
	"title" : "Psi Orionis"
	},
{
	"Index" : "31697",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "31 Orionis, HIP 25737, SAO 132176, HD 36167, GC 6792, HR 1834, DM BD-01   913, TYC 4753-1894-1",
	"group" : { "key" : "Orion" },
	"Common" : "31 Orionis",
	"OType" : "Variable Star",
	"Distance" : "154.09",
	"RA_S" : 82.43325925,
	"DEC_S" : -1.09223719,
	"Constellation" : "Orion ",
	"AMag" : 4.884,
	"key" : 51697,
	"title" : "31 Orionis"
	},
{
	"Index" : "2054",
	"Description" : "32 Orionis (32 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.20.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "32 Orionis, A Orionis, HIP 25813A, SAO 112849, HD 36267, GC 6813, HR 1839, DM BD+05   939, TYC 126-1899-1",
	"group" : { "key" : "Orion" },
	"Common" : "32 Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "92.46",
	"RA_S" : 82.69607778,
	"DEC_S" : 5.94814616,
	"X" : 534,
	"Y" : 325,
	"Constellation" : "Orion ",
	"AMag" : 4.439,
	"key" : 22054,
	"title" : "32 Orionis"
	},
{
	"Index" : "2055",
	"Description" : "32 Orionis (32 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.20.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "32 Orionis, HIP 25813B, TYC 126-1899-2",
	"group" : { "key" : "Orion" },
	"Common" : "32 Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "92.46",
	"RA_S" : 82.69607778,
	"DEC_S" : 5.94814616,
	"X" : 534,
	"Y" : 325,
	"Constellation" : "Orion ",
	"AMag" : 5.751,
	"key" : 22055,
	"title" : "32 Orionis"
	},
{
	"Index" : "32014",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "36 Orionis, Upsilon Orionis, HIP 25923, SAO 132222, HD 36512, GC 6850, HR 1855, DM BD-07  1106, TYC 4778-1407-1",
	"group" : { "key" : "Orion" },
	"Common" : "Thabit",
	"OType" : "Variable Star",
	"Distance" : "877.193",
	"RA_S" : 82.98274925,
	"DEC_S" : -7.30154281,
	"Constellation" : "Orion ",
	"AMag" : 4.565,
	"key" : 52014,
	"shortTitle" : "Tabit (see HD30652)",
	"title" : "Thabit"
	},
{
	"Index" : "31828",
	"Description" : "Mintaka (\u03B4 Orionis, 34 Orionis) is a star some 900 light years distant in the constellation Orion. The name Mintaka comes from \u0645\u0646\u0637\u0642\u0629 man\u0163aqah, which means \u0022the belt\u0022 in Arabic. Together with Alnitak (Zeta Orionis) and Alnilam (Epsilon Orionis), the three stars make up the belt of Orion, known by many names among ancient cultures. When Orion is close to the meridian, Mintaka is the right-most of the belt\u0027s stars as seen by an observer in the Northern Hemisphere facing south. Mintaka is actually a multiple star at the western end of Orion\u0027s belt, with a magnitude 7 star about 52\u0022 away from the main component and an even fainter star in between. The main component itself is also double, consisting of a class B giant and a smaller but hotter class O. The stars orbit each other every 5.73 days. These two stars are both about 90,000 times as luminous as the Sun with a mass of some 20 solar masses.\r\rIn 1904, Johannes Hartmann discovered that interstellar space contains a thin gas, the interstellar medium, by using Mintaka as a background source.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "34 Orionis, Delta Orionis, HIP 25930D, SAO 132220, HD 36486, GC 6847, HR 1852, DM BD-00   983, TYC 4766-2445-2",
	"group" : { "key" : "Orion" },
	"Common" : "Mintaka",
	"OType" : "Star",
	"Distance" : "331.14",
	"RA_S" : 83.001708,
	"X" : 531,
	"Y" : 406,
	"Constellation" : "Orion ",
	"AMag" : 3.763,
	"key" : 51828,
	"shortTitle" : "Mintika",
	"title" : "Mintaka"
	},
{
	"Index" : "31835",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 25980, SAO 132234, HD 36591, GC 6863, HR 1861, DM BD-01  935, TYC 4766-2452-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1861",
	"OType" : "Variable Star",
	"Distance" : "378.16",
	"RA_S" : 83.17230579,
	"DEC_S" : -1.59183657,
	"Constellation" : "Orion ",
	"AMag" : 5.314,
	"key" : 51835,
	"title" : "HR 1861"
	},
{
	"Index" : "31832",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "VV Orionis, HIP 26063, SAO 132255, HD 36695, GC 6884, HR 1868, DM BD-01   943, TYC 4766-2449-1",
	"group" : { "key" : "Orion" },
	"Common" : "VV Orionis",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "383.09",
	"RA_S" : 83.38103274,
	"DEC_S" : -1.15607415,
	"Constellation" : "Orion ",
	"AMag" : 5.34,
	"key" : 51832,
	"title" : "VV Orionis"
	},
{
	"Index" : "1778",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "38 Orionis, n02 Orionis, HIP 26126, SAO 112904, HD 36777, GC 6896, HR 1872, DM BD+03   964, TYC 122-2409-1",
	"group" : { "key" : "Orion" },
	"Common" : "n02 Orionis",
	"OType" : "Double or multiple star",
	"Distance" : "84.31",
	"RA_S" : 83.56989621,
	"DEC_S" : 3.76688998,
	"Constellation" : "Orion ",
	"AMag" : 5.334,
	"key" : 21778,
	"title" : "n02 Orionis"
	},
{
	"Index" : "48980",
	"Description" : "The Bayer designation Phi Orionis (\u03C6 Ori, \u03C6 Orionis) is shared by two star systems, \u03C6\u00B9 Orionis and \u03C6\u00B2 Orionis, in the constellation Orion. The two stars are separated by approximately 0.71\u00B0 in the sky. Phi-1 Orionis, is a binary star lying about 1000 light years from Earth. Phi-1 Orionis is a spectral type B0 main sequence star which has an apparent magnitude of +4.39.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "37 Orionis, Phi01 Orionis, HIP 26176, SAO 112914, HD 36822, GC 6907, HR 1876, DM BD+09   877, TYC 705-2401-1",
	"group" : { "key" : "Orion" },
	"Common" : "Phi1 Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "358.62",
	"RA_S" : 83.70515583,
	"DEC_S" : 9.48957657,
	"X" : 521,
	"Y" : 279,
	"Constellation" : "Orion ",
	"AMag" : 4.367,
	"key" : 68980,
	"title" : "Phi1 Orionis"
	},
{
	"Index" : "32010",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 26199, SAO 132301, HD 36960, GC 6926, HR 1887, DM BD-06 1234, TYC 4778-1403-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1887",
	"OType" : "Young Stellar Object",
	"Distance" : "393.04",
	"RA_S" : 83.76117628,
	"DEC_S" : -6.0020161,
	"Constellation" : "Orion ",
	"AMag" : 4.702,
	"key" : 52010,
	"title" : "HR 1887"
	},
{
	"Index" : "48978",
	"Description" : "Meissa (Lambda Orionis, \u03BB Orionis) is a star in the constellation Orion. \u0022Meissa\u0022 derives from the Arabic \u0022Al-Maisan\u0022 which means \u0022The Shining One\u0022. This term was used for Gamma Gemini (Alhena), but was somehow also mistakenly applied to Meissa and the name stuck. The original Arabic name for this star, \u0022Al Hakah\u0022 (the source for another name for it, \u0022Heka\u0022) refers to the Arabic lunar mansion that includes this star and the two of \u03C6 Ori (Al Ha\u1E33\u02BDah, \u0022a White Spot\u0022).\r\rIn Chinese, \u89DC\u5BBF (Z\u012B S\u00F9), meaning Turtle Beak (asterism), refers to an asterism consisting of Meissa and both of \u03C6 Ori Consequently, Meissa itself is known as \u89DC\u5BBF\u4E00 (Z\u012B S\u00F9 y\u012B, English: the First Star of Turtle Beak.)\r\rMeissa is a giant star with a stellar classification of O8 III and an apparent visible magnitude 3.54. It is an enormous star with about 28 times the mass of the Sun and 10 times the Sun\u0027s radius. The outer atmosphere has an effective temperature of around 35,000 K, giving it the characteristic blue glow of a hot O-type star. Meissa is a soft X-ray source with a luminosity of 1032 erg s\u22121 and peak emission in the energy range of 0.2\u20130.3 keV, which suggests the X-rays are probably being generated by the stellar wind.\r\rThis star is the dominant member of a 5 million year old star-forming region known as the \u03BB-Orionis cluster, or Collinder 69. The intense ultraviolet energy being radiated by this star is creating the S 264 H II region in the neighboring volume of space, which in turn is surrounded by an expanding ring of cool gas that has an age of about 2\u20136 million years. The expansion of this gaseous ring may be explained by a former binary companion of Meissa that became a Type II supernova. Such an event would also explain the star\u0027s peculiar velocity with respect to the center of the expanding ring, as the explosion and resulting mass loss could have kicked Meissa out of the system. A potential candidate for the supernova remnant is the neutron star Geminga. However, the last is unlikely given the distance between Geminga and the cluster.\r\rMeissa is actually a double star with a companion at an angular separation of 4.41 arcseconds along a position angle of 43.12\u00B0 (as of 1937). This fainter component is of magnitude 5.61 and it has a stellar classification of B0.5 V, making it a B-type main sequence star. There is an outlying component, Meissa C, which is an F-type main sequence star with a classification of F8 V. This star in turn may have a very low mass companion that is probably a brown dwarf.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "39 Orionis, Lambda Orionis, HIP 26207A, SAO 112921, HD 36861, GC 6915, HR 1879, DM BD+09   879A, TYC 705-2400-1",
	"group" : { "key" : "Orion" },
	"Common" : "Meissa",
	"OType" : "Emission-line Star",
	"Distance" : "357.4",
	"RA_S" : 83.7844872,
	"DEC_S" : 9.93415437,
	"X" : 521,
	"Y" : 273,
	"Constellation" : "Orion ",
	"AMag" : 3.509,
	"key" : 68978,
	"shortTitle" : "Meissa; Kheka; Al'kheka; Mejssa",
	"title" : "Meissa"
	},
{
	"Index" : "48979",
	"Description" : "Meissa (Lambda Orionis, \u03BB Orionis) is a star in the constellation Orion. \u0022Meissa\u0022 derives from the Arabic \u0022Al-Maisan\u0022 which means \u0022The Shining One\u0022. This term was used for Gamma Gemini (Alhena), but was somehow also mistakenly applied to Meissa and the name stuck. The original Arabic name for this star, \u0022Al Hakah\u0022 (the source for another name for it, \u0022Heka\u0022) refers to the Arabic lunar mansion that includes this star and the two of \u03C6 Ori (Al Ha\u1E33\u02BDah, \u0022a White Spot\u0022).\r\rIn Chinese, \u89DC\u5BBF (Z\u012B S\u00F9), meaning Turtle Beak (asterism), refers to an asterism consisting of Meissa and both of \u03C6 Ori Consequently, Meissa itself is known as \u89DC\u5BBF\u4E00 (Z\u012B S\u00F9 y\u012B, English: the First Star of Turtle Beak.)\r\rMeissa is a giant star with a stellar classification of O8 III and an apparent visible magnitude 3.54. It is an enormous star with about 28 times the mass of the Sun and 10 times the Sun\u0027s radius. The outer atmosphere has an effective temperature of around 35,000 K, giving it the characteristic blue glow of a hot O-type star. Meissa is a soft X-ray source with a luminosity of 1032 erg s\u22121 and peak emission in the energy range of 0.2\u20130.3 keV, which suggests the X-rays are probably being generated by the stellar wind.\r\rThis star is the dominant member of a 5 million year old star-forming region known as the \u03BB-Orionis cluster, or Collinder 69. The intense ultraviolet energy being radiated by this star is creating the S 264 H II region in the neighboring volume of space, which in turn is surrounded by an expanding ring of cool gas that has an age of about 2\u20136 million years. The expansion of this gaseous ring may be explained by a former binary companion of Meissa that became a Type II supernova. Such an event would also explain the star\u0027s peculiar velocity with respect to the center of the expanding ring, as the explosion and resulting mass loss could have kicked Meissa out of the system. A potential candidate for the supernova remnant is the neutron star Geminga. However, the last is unlikely given the distance between Geminga and the cluster.\r\rMeissa is actually a double star with a companion at an angular separation of 4.41 arcseconds along a position angle of 43.12\u00B0 (as of 1937). This fainter component is of magnitude 5.61 and it has a stellar classification of B0.5 V, making it a B-type main sequence star. There is an outlying component, Meissa C, which is an F-type main sequence star with a classification of F8 V. This star in turn may have a very low mass companion that is probably a brown dwarf.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "39 Orionis, Lambda Orionis, HIP 26207B, HD 36862, HR 1880, DM BD+09   879B, TYC 705-2400-2",
	"group" : { "key" : "Orion" },
	"Common" : "Meissa",
	"OType" : "Star",
	"Distance" : "357.4",
	"RA_S" : 83.785333,
	"DEC_S" : 9.935028,
	"X" : 521,
	"Y" : 273,
	"Constellation" : "Orion ",
	"AMag" : 5.452,
	"key" : 68979,
	"title" : "Meissa"
	},
{
	"Index" : "31969",
	"Description" : "Theta Orionis (tet Ori, Theta Ori, \u03B8 Orionis, \u03B8 Ori) is the name of several astronomical objects, located at RA 05h 35.3m DEC -05\u00B0 24\u2032. The Theta Orionis set of objects are located within the NGC 1977 nebula.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "41 Orionis, Theta01 Orionis, HIP 26220B, HD 37020, HR 1893, DM BD-05  1315, TYC 4774-953-1",
	"group" : { "key" : "Orion" },
	"Common" : "Theta1 Orionis",
	"OType" : "Herbig Ae/Be star",
	"Distance" : "621.91",
	"RA_S" : 83.815954,
	"DEC_S" : -5.387322,
	"X" : 520,
	"Y" : 472,
	"Constellation" : "Orion ",
	"AMag" : 6.55,
	"key" : 51969,
	"title" : "Theta1 Orionis"
	},
{
	"Index" : "31970",
	"Description" : "Theta Orionis (tet Ori, Theta Ori, \u03B8 Orionis, \u03B8 Ori) is the name of several astronomical objects, located at RA 05h 35.3m DEC -05\u00B0 24\u2032. The Theta Orionis set of objects are located within the NGC 1977 nebula.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "41 Orionis, Theta01 Orionis, HIP 26220D, HD 37021, HR 1894, DM BD-05  1315B, TYC 4774-954-1",
	"group" : { "key" : "Orion" },
	"Common" : "Theta1 Orionis",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "621.91",
	"RA_S" : 83.817133,
	"DEC_S" : -5.385247,
	"X" : 520,
	"Y" : 472,
	"Constellation" : "Orion ",
	"AMag" : 7.492,
	"key" : 51970,
	"title" : "Theta1 Orionis"
	},
{
	"Index" : "31964",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "41 Orionis, Theta01 Orionis, HIP 26221A, SAO 132314, HD 37022, GC 6931, HR 1895, DM BD-05  1315C, TYC 4774-931-1",
	"group" : { "key" : "Orion" },
	"Common" : "Theta01 Orionis",
	"OType" : "Double or multiple star",
	"RA_S" : 83.81859643,
	"DEC_S" : -5.38977294,
	"Constellation" : "Orion ",
	"AMag" : 5.061,
	"key" : 51964,
	"title" : "Theta01 Orionis"
	},
{
	"Index" : "31965",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "43 Orionis, Theta02 Orionis, HIP 26235EN, SAO 132321, HD 37041, GC 6935, HR 1897, DM BD-05  1319, TYC 4774-933-1",
	"group" : { "key" : "Orion" },
	"Common" : "Theta02 Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "484.86",
	"RA_S" : 83.84541789,
	"DEC_S" : -5.41605396,
	"Constellation" : "Orion ",
	"AMag" : 5.027,
	"key" : 51965,
	"title" : "Theta02 Orionis"
	},
{
	"Index" : "31960",
	"Description" : "42 Orionis (42 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.59.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "42 Orionis, c Orionis, HIP 26237, SAO 132320, HD 37018, GC 6934, HR 1892, DM BD-04  1185, TYC 4774-928-1",
	"group" : { "key" : "Orion" },
	"Common" : "42 Orionis",
	"OType" : "Young Stellar Object",
	"Distance" : "271.0027",
	"RA_S" : 83.84648287,
	"DEC_S" : -4.83835095,
	"X" : 520,
	"Y" : 465,
	"Constellation" : "Orion ",
	"AMag" : 4.607,
	"key" : 51960,
	"title" : "42 Orionis"
	},
{
	"Index" : "32009",
	"Description" : "Iota Orionis (\u03B9 Ori, \u03B9 Orionis) is a star in the equatorial constellation of Orion the hunter. The apparent visual magnitude of Iota Orionis is 2.77, making it the eighth brightest member of Orion. It is the brightest star in an asterism known as Orion\u0027s sword. Iota Orionis has the traditional names Hatsya (sometimes with the typographic error Hatysa) and in Arabic, Na\u0027ir al Saif, which means simply \u0022the Bright One of the Sword.\u0022 From parallax measurements, it is located at a distance of roughly 2,330 light-years (710 parsecs) from Earth.\r\rIota Orionis is a quadruple system dominated by a massive spectroscopic binary with an eccentric (e=0.764), 29-day orbit. The binary is composed of a stellar class O9 III star (blue giant) and a class B0.8 III/IV star, with the secondary being about 2 magnitudes fainter. The collision of the stellar winds from this pair makes the system a strong X-ray source. Oddly, the two objects of this system appear to have different ages, with the secondary being about double the age of the primary. In combination with the high eccentricity of their orbit, this suggests that the binary system was created through a capture, rather than by being formed together and undergoing a mass transfer. This capture may have occurred, for example, through an encounter between two binary systems.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "44 Orionis, Iota Orionis, HIP 26241, SAO 132323, HD 37043, GC 6937, HR 1899, DM BD-06  1241, TYC 4778-1401-1",
	"group" : { "key" : "Orion" },
	"Common" : "Hatsya",
	"OType" : "Spectroscopic binary",
	"Distance" : "441.15",
	"RA_S" : 83.85825795,
	"DEC_S" : -5.90990098,
	"X" : 519,
	"Y" : 479,
	"Constellation" : "Orion ",
	"AMag" : 2.715,
	"key" : 52009,
	"shortTitle" : "Nair al Saif",
	"title" : "Hatsya"
	},
{
	"Index" : "31962",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "45 Orionis, HIP 26268, SAO 132336, HD 37077, GC 6945, HR 1901, DM BD-04  1188, TYC 4774-929-1",
	"group" : { "key" : "Orion" },
	"Common" : "45 Orionis",
	"OType" : "Star",
	"Distance" : "110",
	"RA_S" : 83.91451689,
	"DEC_S" : -4.85606611,
	"Constellation" : "Orion ",
	"AMag" : 5.266,
	"key" : 51962,
	"title" : "45 Orionis"
	},
{
	"Index" : "48610",
	"Description" : "The Bayer designation Phi Orionis (\u03C6 Ori, \u03C6 Orionis) is shared by two star systems, \u03C6\u00B9 Orionis and \u03C6\u00B2 Orionis, in the constellation Orion. The two stars are separated by approximately 0.71\u00B0 in the sky. Phi-2 Orionis, is a spectral type K0 giant which has an apparent magnitude of +4.09. It is about 115 light years from Earth.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "40 Orionis, Phi02 Orionis, HIP 26366, SAO 112958, HD 37160, GC 6972, HR 1907, DM BD+09   898, TYC 701-2047-1",
	"group" : { "key" : "Orion" },
	"Common" : "Phi2 Orionis",
	"OType" : "High proper-motion Star",
	"Distance" : "36.02",
	"RA_S" : 84.22662092,
	"DEC_S" : 9.29067066,
	"X" : 515,
	"Y" : 282,
	"Constellation" : "Orion ",
	"AMag" : 4.187,
	"key" : 68610,
	"title" : "Phi2 Orionis"
	},
{
	"Index" : "31916",
	"Description" : "Sigma Orionis or Sigma Ori (\u03C3 Orionis, \u03C3 Ori) is a five-star system in the constellation Orion, just to the southwest of Alnitak. It is approximately 1,150 light years from Earth.\r\rThe primary component is the binary Sigma Orionis AB, with the two stars being a mere 0.25 arcseconds apart. Both stars are hydrogen-fusing dwarfs only a few million years old. The brighter one, Sigma Orionis A, is a blue O-type star with an apparent visual magnitude of +4.2. Sigma Orionis B is a B-type star with an apparent visual magnitude of +5.1. The pair orbit each other every 170 years at a distance of about 90 AU. A and B have very hot surfaces, around 32,000 and 29,600 kelvins, radiating at about 35,000 and 30,000 solar luminosities, respectively. Temperature and luminosity give masses of 18 and 13.5 solar masses, making the close AB pair among the most massive of visual binaries.\r\rThe next brightest stars in the system are Sigma Orionis D and E, which lie about 4,600 and 15,000 AU respectively from the AB pair. Both are seven solar mass B-type dwarf stars with magnitudes of 6.62 and 6.66. Sigma Orionis E is a prototype of the strange \u0022helium-rich\u0022 stars, which have significantly large amounts of helium.\r\rThe last star in the system is Sigma Orionis C, an A-type dwarf star. C is the closest to the AB pair, about 3,900 AU away.\r\rWhile the orbit of the AB pair is stable, the orbits of the other three are not, and long before they die they will probably be gravitationally sped up and forced out of the system.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "48 Orionis, Sigma Orionis, HIP 26549AB, SAO 132406, HD 37468, GC 7031, HR 1931, DM BD-02  1326, TYC 4771-1196-1",
	"group" : { "key" : "Orion" },
	"Common" : "Sigma Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "291.36",
	"RA_S" : 84.68658057,
	"DEC_S" : -2.60003294,
	"X" : 509,
	"Y" : 436,
	"Constellation" : "Orion ",
	"AMag" : 3.763,
	"key" : 51916,
	"title" : "Sigma Orionis"
	},
{
	"Index" : "32033",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "49 Orionis, d Orionis, HIP 26563, SAO 132411, HD 37507, GC 7039, HR 1937, DM BD-07  1142, TYC 4779-700-1",
	"group" : { "key" : "Orion" },
	"Common" : "d Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "44.58",
	"RA_S" : 84.72117914,
	"DEC_S" : -7.21283158,
	"Constellation" : "Orion ",
	"AMag" : 4.79,
	"key" : 52033,
	"title" : "d Orionis"
	},
{
	"Index" : "1879",
	"Description" : "Omega Orionis (\u03C9 Ori) is a star in the constellation Orion. Its apparent magnitude is 4.57.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "47 Orionis, Omega Orionis, HIP 26594, SAO 113001, HD 37490, GC 7042, HR 1934, DM BD+04  1002, TYC 123-2200-1",
	"group" : { "key" : "Orion" },
	"Common" : "Omega Orionis",
	"OType" : "Be Star",
	"Distance" : "378.1",
	"RA_S" : 84.79644125,
	"DEC_S" : 4.12146379,
	"X" : 508,
	"Y" : 348,
	"Constellation" : "Orion ",
	"AMag" : 4.503,
	"key" : 21879,
	"title" : "Omega Orionis"
	},
{
	"Index" : "31908",
	"Description" : "Alnitak (Arabic: \u0627\u0644\u0646\u0637\u0627\u0642 an-ni\u1E6D\u0101q\u200E) is a triple star some 736 light years distant in the constellation Orion. It is part of Orion\u0027s Belt along with Alnilam and Mintaka, and has a Bayer designation of Zeta Orionis.\r\rThe primary star is a hot blue supergiant with an absolute magnitude of -5.25, and is the brightest class O star in the night sky with a visual magnitude of +2.04. It has two bluish 4th magnitude companions, producing a combined magnitude for the trio of +1.72. The stars are members of the Orion OB1 association and the Collinder 70 association. Alnitak has been known since antiquity and, as a component of Orion\u0027s belt, has been of widespread cultural significance. It was reported to be a double star by amateur German astronomer George K. Kunowsky in 1819. Much more recently, in 1998, the bright primary was found by a team from the Lowell Observatory to have a close companion; this had been suspected from observations made with the Narrabri Stellar Intensity Interferometer in the 1970s. Initially thought to be around 1500 light years distant, the Alnitak system\u0027s distance was determined to be roughly half that via measurement of its stellar parallax by the Hipparcos satellite.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "50 Orionis, Zeta Orionis, HIP 26727B, HD 37743, HR 1949, DM BD-02  1338B, TYC 4771-1188-2",
	"group" : { "key" : "Orion" },
	"Common" : "Alnitak",
	"OType" : "Star",
	"Distance" : "333.85",
	"RA_S" : 85.189879,
	"DEC_S" : -1.943219,
	"X" : 502,
	"Y" : 427,
	"Constellation" : "Orion ",
	"AMag" : 3.699,
	"key" : 51908,
	"title" : "Alnitak"
	},
{
	"Index" : "31850",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 26736, SAO 132445, HD 37756, GC 7091, HR 1952, DM BD-01 1004, TYC 4767-1404-1",
	"group" : { "key" : "Orion" },
	"Common" : "HR 1952",
	"OType" : "Spectroscopic binary",
	"Distance" : "345.46",
	"RA_S" : 85.2113089,
	"DEC_S" : -1.12878491,
	"Constellation" : "Orion ",
	"AMag" : 4.9,
	"key" : 51850,
	"title" : "HR 1952"
	},
{
	"Index" : "1243",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "51 Orionis, b Orionis, HIP 26885, SAO 113056, HD 37984, GC 7136, HR 1963, DM BD+01  1105, TYC 115-2299-1",
	"group" : { "key" : "Orion" },
	"Common" : "b Orionis",
	"OType" : "Star",
	"Distance" : "89.89",
	"RA_S" : 85.61929695,
	"DEC_S" : 1.47462815,
	"Constellation" : "Orion ",
	"AMag" : 5.03,
	"key" : 21243,
	"title" : "b Orionis"
	},
{
	"Index" : "36155",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "55 Orionis, HIP 27658, SAO 132591, HD 39291, GC 7354, HR 2031, DM BD-07  1187, TYC 5347-905-1",
	"group" : { "key" : "Orion" },
	"Common" : "55 Orionis",
	"OType" : "Variable Star",
	"Distance" : "318.66",
	"RA_S" : 87.84159899,
	"DEC_S" : -7.5180025,
	"Constellation" : "Orion ",
	"AMag" : 5.308,
	"key" : 56155,
	"title" : "55 Orionis"
	},
{
	"Index" : "1323",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "56 Orionis, HIP 27750, SAO 113220, HD 39400, GC 7380, HR 2037, DM BD+01  1151, TYC 116-1329-1",
	"group" : { "key" : "Orion" },
	"Common" : "56 Orionis",
	"OType" : "Variable Star",
	"Distance" : "379.98",
	"RA_S" : 88.11016412,
	"DEC_S" : 1.85513956,
	"Constellation" : "Orion ",
	"AMag" : 4.909,
	"key" : 21323,
	"title" : "56 Orionis"
	},
{
	"Index" : "2552",
	"Description" : "Chi1 Orionis (\u03C71 Ori, \u03C71 Orionis) is a star about 28 light years away. It is in the constellation Orion.\r\r\u03C71 Ori is a G0V main-sequence star. It has a faint companion with a mass estimated at about 15% of the mass of the Sun, an orbital period of 14.1 years, and an estimated stellar class of M6. The companion orbits an average distance of 6.1 AU from the primary, but has a fairly high orbital eccentricity, ranging from 3.3 AU out to 8.9 AU from the primary. Because of this red dwarf companion, the likelihood of habitable planets in this system is low.\r\r\u03C71 Ori is a candidate stream star member of the Ursa Major Moving Group, although there is some evidence to the contrary.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "54 Orionis, Chi01 Orionis, HIP 27913, SAO 77705, HD 39587, GC 7419, HR 2047, DM BD+20  1162, TYC 1320-2118-1",
	"group" : { "key" : "Orion" },
	"Common" : "Chi1 Orionis",
	"OType" : "Variable of RS CVn type",
	"Distance" : "8.66",
	"RA_S" : 88.59573271,
	"DEC_S" : 20.27619413,
	"X" : 461,
	"Y" : 138,
	"Constellation" : "Orion ",
	"AMag" : 4.462,
	"key" : 22552,
	"title" : "Chi1 Orionis"
	},
{
	"Index" : "1394",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "60 Orionis, HIP 28296, SAO 113321, HD 40446, GC 7556, HR 2103, DM BD+00  1239, TYC 117-1471-1",
	"group" : { "key" : "Orion" },
	"Common" : "60 Orionis",
	"OType" : "Star",
	"Distance" : "134.54",
	"RA_S" : 89.70655414,
	"DEC_S" : 0.55297829,
	"Constellation" : "Orion ",
	"AMag" : 5.202,
	"key" : 21394,
	"title" : "60 Orionis"
	},
{
	"Index" : "32107",
	"Description" : "HD 40657 is a star in the constellation Orion. Its apparent magnitude is 4.54.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 28413, SAO 132732, HD 40657, GC 7587, HR 2113, DM BD-03 1256, TYC 4786-2368-1",
	"group" : { "key" : "Orion" },
	"Common" : "HD 40657",
	"OType" : "Variable Star",
	"Distance" : "127.36",
	"RA_S" : 90.01396016,
	"DEC_S" : -3.07425864,
	"X" : 439,
	"Y" : 442,
	"Constellation" : "Orion ",
	"AMag" : 4.669,
	"key" : 52107,
	"title" : "HD 40657"
	},
{
	"Index" : "50507",
	"Description" : "Mu Orionis is a quadruple star system in the constellation Orion, similar to Mizar and Epsilon Lyrae with combined visual magnitude of 4.13. The four stars are known as Mu Orionis Aa, Mu Orionis Ab, Mu Orionis Ba, and Mu Orionis Bb. All four components are spectroscopic, with A and B systems only several tenths of an arcsec apart. The entire system is located approximately 155 ly from the Sun.\r\rMu Orionis Aa is an A5V dwarf and metallic line star, of effective temperature 8350 Kelvin, and apparent magnitude of +4.31. Mu Orionis Aa has 2.1 solar masses, and a radius of 2.9 solar radii and a luminosity 32x that of the Sun.\r\rMu Orionis Ab is a G5V dwarf orbiting Aa at a distance of 0.077 AU, .2x the orbit of mercury.\r\rMu Orionis Ba and Bb are F5V dwarfs with 1.4 solar masses and apparent magnitudes of 6.91. They are separated from eacu other by 0.078 AU.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "61 Orionis, Mu Orionis, HIP 28614AB, SAO 113389, HD 40932A, GC 7635, HR 2124, DM BD+09  1064, TYC 721-2468-1",
	"group" : { "key" : "Orion" },
	"Common" : "Mu Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.45",
	"RA_S" : 90.59582367,
	"DEC_S" : 9.64729514,
	"X" : 433,
	"Y" : 276,
	"Constellation" : "Orion ",
	"AMag" : 4.152,
	"key" : 70507,
	"title" : "Mu Orionis"
	},
{
	"Index" : "2565",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "64 Orionis, HIP 28691, SAO 95166, HD 41040, GC 7662, HR 2130, DM BD+19  1186, TYC 1321-1516-1",
	"group" : { "key" : "Orion" },
	"Common" : "64 Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "219.19",
	"RA_S" : 90.86402655,
	"DEC_S" : 19.69055971,
	"Constellation" : "Orion ",
	"AMag" : 5.113,
	"key" : 22565,
	"title" : "64 Orionis"
	},
{
	"Index" : "2564",
	"Description" : "Chi2 Orionis (Chi2 Ori / \u03C72 Orionis / \u03C72 Ori) is a B-type supergiant star in the constellation of Orion. It has an apparent visual magnitude of approximately 4.646. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "62 Orionis, Chi02 Orionis, HIP 28716, SAO 77911, HD 41117, GC 7675, HR 2135, DM BD+20  1233, TYC 1321-1515-1",
	"group" : { "key" : "Orion" },
	"Common" : "Chi2 Orionis",
	"OType" : "Blue supergiant star",
	"Distance" : "537.06",
	"RA_S" : 90.97994038,
	"DEC_S" : 20.13844671,
	"X" : 431,
	"Y" : 140,
	"Constellation" : "Orion ",
	"AMag" : 4.662,
	"key" : 22564,
	"title" : "Chi2 Orionis"
	},
{
	"Index" : "51045",
	"Description" : "Nu Orionis (\u03BD Orionis) is a triple star system located 514 light years from here in the northeastern part of the constellation Orion, well above Betelgeuse and next to the somewhat further Xi Orionis\r\rThe primary, Nu Orionis A, is a blue, B4V, main-sequence dwarf with a mass 9.2 times solar. It shines with an apparent magnitude of 4.42 and has an absolute magnitude of -1.64.\r\rThe star is a member of the Pleiades moving group.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "67 Orionis, Nu Orionis, HIP 29038, SAO 95259, HD 41753, GC 7772, HR 2159, DM BD+14  1152, TYC 729-1980-1",
	"group" : { "key" : "Orion" },
	"Common" : "Nu Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "157.71",
	"RA_S" : 91.89302608,
	"DEC_S" : 14.76847246,
	"X" : 418,
	"Y" : 210,
	"Constellation" : "Orion ",
	"AMag" : 4.371,
	"key" : 71045,
	"title" : "Nu Orionis"
	},
{
	"Index" : "52279",
	"Description" : "Xi Orionis (\u03BE Orionis) is a blue main-sequence star, spectral type B3V, located some 606 light years from here in the northeastern part of the constellation of Orion, well above the red giant star, Betelgeuse in the sky. It lies next to another blue main-sequence star, Nu Orionis which is somewhat closer at 514 light years.\r\rXi Orionis shines with an apparent visual magnitide of 4.45; its absolute magnitude is -2.0, effective temperature 21000K, and mass 9.2 (times solar). The B3 star is the primary component of a multiple-star system which has also been classified as a B3IV subgiant, although at a somewhat further distance of nearly 634 ly.",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "70 Orionis, Xi Orionis, HIP 29426, SAO 95362, HD 42560, GC 7889, HR 2199, DM BD+14  1187, TYC 742-2472-1",
	"group" : { "key" : "Orion" },
	"Common" : "Xi Orionis",
	"OType" : "Spectroscopic binary",
	"Distance" : "185.81",
	"RA_S" : 92.984985,
	"DEC_S" : 14.20876552,
	"X" : 403,
	"Y" : 217,
	"Constellation" : "Orion ",
	"AMag" : 4.413,
	"key" : 72279,
	"title" : "Xi Orionis"
	},
{
	"Index" : "2485",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "69 Orionis, f01 Orionis, HIP 29434, SAO 95365, HD 42545, GC 7891, HR 2198, DM BD+16  1035, TYC 1314-1954-1",
	"group" : { "key" : "Orion" },
	"Common" : "f01 Orionis",
	"OType" : "Emission-line Star",
	"Distance" : "161.76",
	"RA_S" : 93.01366765,
	"DEC_S" : 16.13040337,
	"Constellation" : "Orion ",
	"AMag" : 4.923,
	"key" : 22485,
	"title" : "f01 Orionis"
	},
{
	"Index" : "2583",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "71 Orionis, HIP 29650, SAO 95432, HD 43042, GC 7971, HR 2220, DM BD+19  1270, TYC 1322-1496-1",
	"group" : { "key" : "Orion" },
	"Common" : "71 Orionis",
	"OType" : "High proper-motion Star",
	"Distance" : "20.81",
	"RA_S" : 93.71198415,
	"DEC_S" : 19.15644872,
	"Constellation" : "Orion ",
	"AMag" : 5.245,
	"key" : 22583,
	"title" : "71 Orionis"
	},
{
	"Index" : "2484",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "72 Orionis, f02 Orionis, HIP 29704, SAO 95447, HD 43153, GC 7987, HR 2223, DM BD+16  1060, TYC 1314-1953-1",
	"group" : { "key" : "Orion" },
	"Common" : "f02 Orionis",
	"OType" : "Star",
	"Distance" : "158",
	"RA_S" : 93.8547028,
	"DEC_S" : 16.1431797,
	"Constellation" : "Orion ",
	"AMag" : 5.309,
	"key" : 22484,
	"title" : "f02 Orionis"
	},
{
	"Index" : "51944",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "73 Orionis, HIP 29736, SAO 95457, HD 43247, GC 7996, HR 2229, DM BD+12  1081, TYC 739-2616-1",
	"group" : { "key" : "Orion" },
	"Common" : "73 Orionis",
	"OType" : "Star",
	"Distance" : "351.97",
	"RA_S" : 93.93735022,
	"DEC_S" : 12.5510665,
	"Constellation" : "Orion ",
	"AMag" : 5.466,
	"key" : 71944,
	"title" : "73 Orionis"
	},
{
	"Index" : "51945",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "74 Orionis, k Orionis, HIP 29800, SAO 95476, HD 43386, GC 8033, HR 2241, DM BD+12  1084, TYC 739-2617-1",
	"group" : { "key" : "Orion" },
	"Common" : "k Orionis",
	"OType" : "Star",
	"Distance" : "19.25",
	"RA_S" : 94.11091061,
	"DEC_S" : 12.27216283,
	"Constellation" : "Orion ",
	"AMag" : 5.084,
	"key" : 71945,
	"title" : "k Orionis"
	},
{
	"Index" : "51478",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "75 Orionis, l Orionis, HIP 29850, SAO 113675, HD 43525, GC 8051, HR 2247, DM BD+09  1173, TYC 735-3442-1",
	"group" : { "key" : "Orion" },
	"Common" : "l Orionis",
	"OType" : "Star",
	"Distance" : "69.06",
	"RA_S" : 94.27759134,
	"DEC_S" : 9.94238992,
	"Constellation" : "Orion ",
	"AMag" : 5.4,
	"key" : 71478,
	"title" : "l Orionis"
	},
{
	"Index" : "32129",
	"MapNum" : "33",
	"ImageNum" : "33",
	"Desig" : "HIP 30093, SAO 133118, HD 44131, GC 8137, HR 2275, DM BD-02 1564, TYC 4788-3059-1",
	"group" : { "key" : "Orion" },
	"Common" : "Lalande 12104 (HR 2275)",
	"OType" : "Variable Star",
	"Distance" : "142.27",
	"RA_S" : 94.99833367,
	"DEC_S" : -2.94449313,
	"Constellation" : "Orion ",
	"AMag" : 5.094,
	"key" : 52129,
	"title" : "Lalande 12104 (HR 2275)"
	},
{
	"Index" : "67797",
	"Description" : "Eta Pavonis (\u03B7 Pav) is a star in the constellation Pavo. Its apparent magnitude is 3.60.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Eta Pavonis, HIP 86929, SAO 254020, HD 160635, GC 24044, HR 6582, DM CP-64  3662, TYC 9062-3615-1",
	"group" : { "backgroundImage" : "images/Alignment/06.png",
		"description" : "Pavo is a constellation in the southern sky. Its name is Latin for peacock. It is one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rThe Peacock\u0027s mythology dates to Greco-Roman times and the story of Jason and the Argonauts. The Argo was named for its creator, Argos, who was transmuted to a peacock by Juno upon his death and honored eternally as a constellation. She honored him further by locating his constellation close to Argo Navis, the constellation representing the Argo.\r\rHowever, there are other myths that prominently feature a peacock. Argus was a creature with one hundred eyes, who guarded the pregnant Io\u2014changed into a heifer. Jupiter entreated Mercury to save Io; Mercury lulled Argus to sleep by playing instruments and talking repetitively; after Argus fell asleep Mercury beheaded him. Juno, who had asked Argus to guard Io, made the peacock\u0027s tail ornaments with all of his eyes in his honor.\r\rPavo was created by Johann Bayer out of faint southern polar stars.",
		"key" : "Pavo",
		"grouptype" : "Pavo",
		"Meaning" : "peacock",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Pavo",
		"title" : "Pavo Objects Group" },
	"Common" : "Eta Pavonis",
	"OType" : "Star",
	"Distance" : "107.94",
	"RA_S" : 266.43327575,
	"DEC_S" : -64.72387503,
	"X" : 398,
	"Y" : 382,
	"Constellation" : "Pavo ",
	"AMag" : 3.714,
	"key" : 87797,
	"title" : "Eta Pavonis"
	},
{
	"Index" : "67774",
	"Description" : "Pi Pavonis (\u03C0 Pav) is a star in the constellation Pavo. Its apparent magnitude is 4.33.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Pi Pavonis, HIP 88866, SAO 254147, HD 165040, GC 24665, HR 6745, DM CP-63  4292, TYC 9059-3655-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Pi Pavonis",
	"OType" : "Star",
	"Distance" : "39.85",
	"RA_S" : 272.1450547,
	"DEC_S" : -63.66853771,
	"X" : 369,
	"Y" : 362,
	"Constellation" : "Pavo ",
	"AMag" : 4.359,
	"key" : 87774,
	"title" : "Pi Pavonis"
	},
{
	"Index" : "67848",
	"Description" : "Xi Pavonis (\u03BE Pav) is a star in the constellation Pavo. Its apparent magnitude is 4.38.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Xi Pavonis, HIP 90098, SAO 254226, HD 168339, GC 25045, HR 6855, DM CP-61  6140, TYC 9068-2823-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Xi Pavonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "127.36",
	"RA_S" : 275.80677423,
	"DEC_S" : -61.4939018,
	"X" : 352,
	"Y" : 331,
	"Constellation" : "Pavo ",
	"AMag" : 4.54,
	"key" : 87848,
	"title" : "Xi Pavonis"
	},
{
	"Index" : "67879",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Nu Pavonis, HIP 90797, SAO 254273, HD 169978, GC 25227, HR 6916, DM CP-62  5879, TYC 9072-3028-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Nu Pavonis",
	"OType" : "Spectroscopic binary",
	"Distance" : "134.42",
	"RA_S" : 277.84344241,
	"DEC_S" : -62.27830805,
	"Constellation" : "Pavo ",
	"AMag" : 4.593,
	"key" : 87879,
	"title" : "Nu Pavonis"
	},
{
	"Index" : "69840",
	"Description" : "Zeta Pavonis (\u03B6 Pav) is a star in the constellation Pavo. Its apparent magnitude is 4.01.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Zeta Pavonis, HIP 91792, SAO 257620, HD 171759, GC 25522, HR 6982, DM CP-71  2353, TYC 9299-2361-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Zeta Pavonis",
	"OType" : "Star",
	"Distance" : "66.97",
	"RA_S" : 280.75889847,
	"DEC_S" : -71.4281107,
	"X" : 316,
	"Y" : 457,
	"Constellation" : "Pavo ",
	"AMag" : 4.129,
	"key" : 89840,
	"title" : "Zeta Pavonis"
	},
{
	"Index" : "67923",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 92024, SAO 254358, HD 172555, GC 25604, HR 7012, DM CP-64 3948, TYC 9077-2487-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7012",
	"OType" : "High proper-motion Star",
	"Distance" : "28.55",
	"RA_S" : 281.36209273,
	"DEC_S" : -64.87125755,
	"Constellation" : "Pavo ",
	"AMag" : 4.793,
	"key" : 87923,
	"title" : "HR 7012"
	},
{
	"Index" : "67894",
	"Description" : "Lambda Pavonis (\u03BB Pav), also known as HD 173948 or HIP 92609, is a star in the constellation Pavo. Its apparent magnitude is 4.21. It is a Be star, a rapidly rotating hot blue star which has developed a gas disk around it. It is a member of the Scorpius-Centaurus Association. It is a Gamma Cassiopeae variable or shell star which has brightened to magnitude 4.0.\r\rVariations in signals coming from Lambda Pavonis have led to debate on whether it is a binary, single or pulsating variable star.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Lambda Pavonis, HIP 92609, SAO 254393, HD 173948, GC 25823, HR 7074, DM CP-62  5983, TYC 9074-2203-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Lambda Pavonis",
	"OType" : "Be Star",
	"Distance" : "435.34",
	"RA_S" : 283.05430944,
	"DEC_S" : -62.18759233,
	"X" : 307,
	"Y" : 338,
	"Constellation" : "Pavo ",
	"AMag" : 4.181,
	"key" : 87894,
	"title" : "Lambda Pavonis"
	},
{
	"Index" : "67959",
	"Description" : "Kappa Pavonis (\u03BA Pav) is a star in the constellation Pavo. Its apparent magnitude is 4.40.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Kappa Pavonis, HIP 93015, SAO 254413, HD 174694, GC 25930, HR 7107, DM CP-67  3603, TYC 9082-1890-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Kappa Pavonis",
	"OType" : "Variable Star of W Vir type",
	"Distance" : "150.85",
	"RA_S" : 284.23761857,
	"DEC_S" : -67.23349812,
	"X" : 301,
	"Y" : 403,
	"Constellation" : "Pavo ",
	"AMag" : 4.439,
	"key" : 87959,
	"title" : "Kappa Pavonis"
	},
{
	"Index" : "67860",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Omega Pavonis, HIP 93163, SAO 254423, HD 175329, GC 26008, HR 7127, DM CP-60  7213, TYC 9070-2106-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Omega Pavonis",
	"OType" : "Star",
	"Distance" : "172.04",
	"RA_S" : 284.65186551,
	"DEC_S" : -60.20054835,
	"Constellation" : "Pavo ",
	"AMag" : 5.279,
	"key" : 87860,
	"title" : "Omega Pavonis"
	},
{
	"Index" : "69786",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 94150, SAO 254475, HD 177389, GC 26313, HR 7221, DM CP-68 3185, TYC 9292-2324-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7221",
	"OType" : "Star",
	"Distance" : "37.38",
	"RA_S" : 287.47028321,
	"DEC_S" : -68.42444704,
	"Constellation" : "Pavo ",
	"AMag" : 5.405,
	"key" : 89786,
	"title" : "HR 7221"
	},
{
	"Index" : "69955",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 97534, SAO 257736, HD 186219, GC 27351, HR 7498, DM CP-72 2445, TYC 9314-780-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7498",
	"OType" : "Star",
	"Distance" : "43.62",
	"RA_S" : 297.35544015,
	"DEC_S" : -72.50337656,
	"Constellation" : "Pavo ",
	"AMag" : 5.422,
	"key" : 89955,
	"title" : "HR 7498"
	},
{
	"Index" : "64940",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 97646AB, SAO 246293, HD 186957, GC 27424, HR 7531, DM CP-59 7534, TYC 8787-2077-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7531",
	"OType" : "Star",
	"Distance" : "84.76",
	"RA_S" : 297.68668917,
	"DEC_S" : -59.19368413,
	"Constellation" : "Pavo ",
	"AMag" : 5.478,
	"key" : 84940,
	"title" : "HR 7531"
	},
{
	"Index" : "64939",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 98174, SAO 246349, HD 188162, GC 27588, HR 7587, DM CP-59 7550, TYC 8787-2076-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7587",
	"OType" : "Star",
	"Distance" : "85.27",
	"RA_S" : 299.27629055,
	"DEC_S" : -58.90134985,
	"Constellation" : "Pavo ",
	"AMag" : 5.242,
	"key" : 84939,
	"title" : "HR 7587"
	},
{
	"Index" : "69958",
	"Description" : "Epsilon Pavonis (\u03B5 Pav) is a star in the constellation Pavo. Its apparent magnitude is 3.95.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Epsilon Pavonis, HIP 98495, SAO 257757, HD 188228, GC 27631, HR 7590, DM CP-73  2086, TYC 9315-1893-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Epsilon Pavonis",
	"OType" : "Variable Star",
	"Distance" : "32.22",
	"RA_S" : 300.14812488,
	"DEC_S" : -72.91050438,
	"X" : 242,
	"Y" : 486,
	"Constellation" : "Pavo ",
	"AMag" : 3.938,
	"key" : 89958,
	"title" : "Epsilon Pavonis"
	},
{
	"Index" : "64948",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "HIP 98608, SAO 246389, HD 189124, GC 27704, HR 7625, DM CP-59 7564, TYC 8788-1765-1",
	"group" : { "key" : "Pavo" },
	"Common" : "HR 7625",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "145.52",
	"RA_S" : 300.43644321,
	"DEC_S" : -59.37589062,
	"Constellation" : "Pavo ",
	"AMag" : 5.235,
	"key" : 84948,
	"title" : "HR 7625"
	},
{
	"Index" : "68059",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Mu02 Pavonis, HIP 98624, SAO 254707, HD 188887, GC 27687, HR 7612, DM CP-67  3698, TYC 9098-1914-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Mu02 Pavonis",
	"OType" : "Star",
	"Distance" : "72.41",
	"RA_S" : 300.46859089,
	"DEC_S" : -66.9439675,
	"Constellation" : "Pavo ",
	"AMag" : 5.467,
	"key" : 88059,
	"title" : "Mu02 Pavonis"
	},
{
	"Index" : "68061",
	"Description" : "Delta Pavonis (\u03B4 Pav, \u03B4 Pavonis) is a star in the southern circumpolar constellation of Pavo. It has an apparent visual magnitude of 3.56, making it a fourth-magnitude star that is visible to the naked eye from the southern hemisphere. Parallax measurements from the Hipparcos satellite yield an estimated distance of 19.92 light-years (6.11 parsecs) from Earth. This makes it one of the nearest bright stars to the Solar System.\r\rIt is a subgiant of spectral type G8 IV, meaning it is about to stop fusing hydrogen in its core and is starting the process of becoming a red giant. Because of that, Delta Pavonis is 22% brighter than the Sun even though the effective temperature of its outer atmosphere is lower, at 5,604 K. It has 99.1% of the Sun\u0027s mass and 122% of the Sun\u0027s radius. The surface convection zone extends downward to about 43.1% of the star\u0027s radius, but only contains 4.8% of the star\u0027s mass.\r\rSpectroscopic examination of this star shows that it has a higher abundance of elements heavier than helium (or metallicity, as astronomers call it) than does the Sun. This value is typically given in terms of the relative ratio of iron (chemical symbol Fe) to hydrogen (H) as compared to the Sun\u0027s atmosphere (iron being a relatively easy element to detect in a stellar atmosphere). For Delta Pavonis, the metallicity is about:\r\r[Fe/H] = 0.33\r\r(This notation gives the logarithm of the iron-to-hydrogen ratio relative to the Sun.) This corresponds to a 214% abundance of iron in this star\u0027s atmosphere compared to the solar abundance. Past studies have shown a correlation between the heavy element abundance in stars and the presence of a planetary system, suggesting Delta Pavonis has a greater than average probability of harboring planets. However, no planetary companions have yet been discovered in orbit around this star.\r\rThe age of this star is in the range of 6.6\u20136.9 billion years old, and the star\u0027s luminosity has increased 60% since it was a zero-age main-sequence star. It appears to be rotating slowly with a projected rotational velocity of 1.0 km s\u20131.\r\rIt has been identified by Maggie Turnbull and Jill Tarter of the SETI Institute as the \u0022Best SETI target\u0022 among the list of the 100 nearest G-type stars. Properties in its favor include a high metallicity, minimal level of magnetic activity, low rotation rate, and kinematic membership in the thin disk population of the Milky Way. The lack of detected radial velocity variation suggests that there are no gas giant planets orbiting near the star\u0027s habitable zone, which may otherwise destabilize a hypothetical Earth-like planet in that orbital zone. As of 1999, no radio source of technological origin has been detected coming from this star. Delta Pavonis is the nearest solar analog that is not a member of a binary or multiple star system. This is a type of star that is a close photometric match to the Sun.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Delta Pavonis, HIP 99240, SAO 254733, HD 190248, GC 27886, HR 7665, DM CP-66  3474, TYC 9098-1918-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Delta Pavonis",
	"OType" : "Variable Star",
	"Distance" : "6.11",
	"RA_S" : 302.18170173,
	"DEC_S" : -66.18206983,
	"X" : 208,
	"Y" : 405,
	"Constellation" : "Pavo ",
	"AMag" : 3.616,
	"key" : 88061,
	"title" : "Delta Pavonis"
	},
{
	"Index" : "68080",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Phi01 Pavonis, HIP 101612, SAO 254823, HD 195627, GC 28609, HR 7848, DM CP-61  6492, TYC 9100-1712-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Phi01 Pavonis",
	"OType" : "Star",
	"Distance" : "27.79",
	"RA_S" : 308.89521314,
	"DEC_S" : -60.58174899,
	"Constellation" : "Pavo ",
	"AMag" : 4.782,
	"key" : 88080,
	"title" : "Phi01 Pavonis"
	},
{
	"Index" : "68076",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Rho Pavonis, HIP 101773, SAO 254835, HD 195961, GC 28668, HR 7859, DM CP-61  6495, TYC 9100-1263-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Rho Pavonis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "58.13",
	"RA_S" : 309.39713643,
	"DEC_S" : -61.52991906,
	"Constellation" : "Pavo ",
	"AMag" : 4.901,
	"key" : 88076,
	"title" : "Rho Pavonis"
	},
{
	"Index" : "68075",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Phi02 Pavonis, HIP 101983, SAO 254846, HD 196378, GC 28730, HR 7875, DM CP-60  7419, TYC 9100-1218-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Phi02 Pavonis",
	"OType" : "High proper-motion Star",
	"Distance" : "24.66",
	"RA_S" : 310.01098847,
	"DEC_S" : -60.54889126,
	"Constellation" : "Pavo ",
	"AMag" : 5.181,
	"key" : 88075,
	"title" : "Phi02 Pavonis"
	},
{
	"Index" : "68155",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Upsilon Pavonis, HIP 102157, SAO 254854, HD 196519, GC 28782, HR 7881, DM CP-67  3754, TYC 9112-1600-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Upsilon Pavonis",
	"OType" : "Star",
	"Distance" : "239.75",
	"RA_S" : 310.4878144,
	"DEC_S" : -66.76068201,
	"Constellation" : "Pavo ",
	"AMag" : 5.123,
	"key" : 88155,
	"title" : "Upsilon Pavonis"
	},
{
	"Index" : "68156",
	"Description" : "Beta Pavonis (\u03B2 Pav) is a star in the constellation Pavo. Its apparent magnitude is 3.43.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Beta Pavonis, HIP 102395, SAO 254862, HD 197051, GC 28862, HR 7913, DM CP-66  3501, TYC 9112-1605-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Beta Pavonis",
	"OType" : "Star",
	"Distance" : "41.42",
	"RA_S" : 311.23955932,
	"DEC_S" : -66.20321518,
	"X" : 164,
	"Y" : 423,
	"Constellation" : "Pavo ",
	"AMag" : 3.431,
	"key" : 88156,
	"title" : "Beta Pavonis"
	},
{
	"Index" : "70024",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Omicron Pavonis, HIP 104755, SAO 257896, HD 201371, GC 29606, HR 8092, DM CP-70  2835, TYC 9326-1-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Omicron Pavonis",
	"OType" : "Variable Star",
	"Distance" : "263.33",
	"RA_S" : 318.33546094,
	"DEC_S" : -70.12626542,
	"Constellation" : "Pavo ",
	"AMag" : 5.256,
	"key" : 90024,
	"title" : "Omicron Pavonis"
	},
{
	"Index" : "68142",
	"Description" : "Gamma Pavonis (\u03B3 Pav, \u03B3 Pavonis) is a star in the southern circumpolar constellation of Pavo. With an apparent visual magnitude of 4.22, it is a fourth-magnitude star and thereby visible to the naked eye. From parallax observations with the Hipparcos satellite, the distance to this star has been estimated at 30.21 light-years (9.26 parsecs).\r\rCompared to the Sun, this star has a 21% greater mass and a 15% larger radius. It is a brighter star with 152% of the Sun\u0027s luminosity, which is it radiating from the outer envelope at an effective temperature of 6,112 K. The stellar classification of F9 V puts it in the class of F-type main sequence stars that generate energy through the nuclear fusion of hydrogen at the core. It is a metal-poor star, which means it has a low abundance of elements heavier than helium. Gamma Pavonis is orbiting through the Milky Way at an unusually high peculiar velocity relative to nearby stars.\r\rThis star has rank 14 on TPC-F\u0027s top 100 target stars to search for a rocky planet in the Habitable Zone, approximately 1.2 AU, or a little beyond an Earth-like orbit.",
	"MapNum" : "06",
	"ImageNum" : "06",
	"Desig" : "Gamma Pavonis, HIP 105858, SAO 254999, HD 203608, GC 29979, HR 8181, DM CP-65  3918, TYC 9111-1423-1",
	"group" : { "key" : "Pavo" },
	"Common" : "Gamma Pavonis",
	"OType" : "Variable Star",
	"Distance" : "9.26",
	"RA_S" : 321.61085348,
	"DEC_S" : -65.36619847,
	"X" : 111,
	"Y" : 442,
	"Constellation" : "Pavo ",
	"AMag" : 4.21,
	"key" : 88142,
	"title" : "Gamma Pavonis"
	},
{
	"Index" : "1442",
	"Description" : "Gamma Pegasi (\u03B3 Peg) is a star in the constellation of Pegasus, located at the lower left-hand corner of the asterism known as the Great Square. It also has the traditional name Algenib; confusingly however, this name is also used for Alpha Persei. The average apparent visual magnitude of +2.84 puts this at fourth place among the brightest stars in the constellation. The distance to this star has been measured using the parallax technique, yielding a value of roughly 390 light-years (120 parsecs) with a margin of error of 5%.\r\rThe asterism of \u03B3 Pegasi and \u03B1 Andromedae, in Hindu astronomy, is called Uttara Bh\u0101drapad\u0101 (\u0909\u0924\u094D\u0924\u0930\u092D\u093E\u0926\u094D\u0930\u092A\u0926\u093E) or Utt\u1E5B\u1E6D\u1E6D\u0101ti. It is the 26th nakshatra. In Chinese, \u58C1\u5BBF (B\u00EC S\u00F9), meaning Wall (asterism) refers to an asterism consisting of \u03B3 Pegasi and \u03B1 Andromedae . Consequently, \u03B3 Pegasi itself is known as \u58C1\u5BBF\u4E00 (B\u00EC S\u00F9 y\u012B, English: the First Star of Wall.)\r\rIn 1911, American astronomer Keivin Burns discovered that the radial velocity of this star varied slightly. This was confirmed in 1953 by American astronomer D. Harold McNamara, who identified it as a Beta Cephei variable. (At the time he actually identified is as a Beta Canis Majoris star, which was subsequently designated a Beta Cephei variable.) It has a radial pulsation period of 0.15175 days (3.642 hours), but also shows the behavior of a slowing pulsating B star (SPB) with three additional pulsational frequencies. Its magnitude varies between +2.78 and +2.89 over the course of each pulsation cycle.\r\rThis is a large star with almost nine times the mass of the Sun and close to five times the Sun\u0027s radius. The stellar classification of B2 IV suggests this is a subgiant star that is exhausting the hydrogen at its core and is in the process of evolving away from the main sequence. It is either rotating very slowly with no measurable rotational velocity or else it is being viewed from nearly pole-on. Gamma Pegasi has a total luminosity of 5,840 times that of the Sun, which is being radiated from its outer atmosphere at an effective temperature of more than 21,000 K. At this temperature, the star glows with a blue-white hue.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "88 Pegasi, Gamma Pegasi, HIP 1067, SAO 91781, HD 886, GC 238, HR 39, DM BD+14    14, TYC 1179-1775-1",
	"group" : { "backgroundImage" : "images/Alignment/35.png",
		"description" : "Pegasus is a constellation in the northern sky, named after the winged horse Pegasus in Greek mythology. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations.\r\rThe Babylonian constellation IKU (field) had four stars of which three were later part of the Greek constellation Hippos (Pegasus). Pegasus, in Greek mythology, was a winged horse with magical powers. One myth regarding his powers says that his hooves dug out a spring, Hippocrene, which blessed those who drank its water with the ability to write poetry. Pegasus was the one who delivered Medusa\u0027s head to Polydectes, after which he travelled to Mount Olympus in order to be the bearer of thunder and lightning for Zeus. Eventually, he became the horse to Bellerophon, who was asked to kill the Chimera and succeeded with the help of Athena and Pegasus. Despite this success, after the death of his children, Bellerophon asked Pegasus to take him to Mount Olympus. Though Pegasus agreed, he plummeted back to Earth after Zeus either threw a thunderbolt at him or made Pegasus buck him off.\r\rIn ancient Persia, Pegasus was depicted by al-Sufi as a complete horse facing east, unlike most other uranographers, who had depicted Pegasus as half of a horse, rising out of the ocean. In al-Sufi\u0027s depiction, Pegasus\u0027s head is made up of the stars of Lacerta the lizard. Its right foreleg is represented by \u03B2 Peg and its left foreleg is represented by \u03B7 Peg, \u03BC Peg, and \u03BB Peg; its hind legs are marked by 9 Peg. The back is represented by \u03C0 Peg and \u03BC Cyg, and the belly is represented by \u03B9 Peg and \u03BA Peg.\r\rPegasus is dominated by an asterism in the shape of a rough square, although one of the stars, Delta Pegasi or Sirrah, is now officially considered to be part of Andromeda, (\u03B1 Andromedae) and is more usually called \u0022Alpheratz\u0022. Traditionally, the body of the horse consists of a quadrilateral formed by the stars \u03B1 Peg, \u03B2 Peg, \u03B3 Peg, and \u03B1 And. The front legs of the winged horse are formed by two crooked lines of stars, one leading from \u03B7 Peg to \u03BA Peg and the other from \u03BC Peg to 1 Pegasi. Another crooked line of stars from \u03B1 Peg via \u03B8 Peg to \u03B5 Peg forms the neck and head; \u03B5 is the snout.\r\rH.A. Rey has suggested an alternative way to connect the stars into the shape of a winged horse, as seen in the diagram at right. In this visualization, the Square of Pegasus is broken into a triangle, representing the horse\u0027s wings, by the removal of Alpha Andromedae.",
		"key" : "Pegasus",
		"grouptype" : "Pegasus",
		"Meaning" : "Pegasus (mythological winged horse)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Pegasus",
		"title" : "Pegasus Objects Group" },
	"Common" : "Algenib",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "119.47",
	"RA_S" : 3.30896346,
	"DEC_S" : 15.18359354,
	"X" : 58,
	"Y" : 417,
	"Constellation" : "Pegasus ",
	"AMag" : 2.769,
	"key" : 21442,
	"shortTitle" : "Al'genib",
	"title" : "Algenib"
	},
{
	"Index" : "1495",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "89 Pegasi, Chi Pegasi, HIP 1168, SAO 91792, HD 1013, GC 270, HR 45, DM BD+19    27, TYC 1185-2319-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Chi Pegasi",
	"OType" : "Variable Star",
	"Distance" : "112.78",
	"RA_S" : 3.65068367,
	"DEC_S" : 20.20669856,
	"Constellation" : "Pegasus ",
	"AMag" : 4.983,
	"key" : 21495,
	"title" : "Chi Pegasi"
	},
{
	"Index" : "5709",
	"Description" : "1 Pegasi (1 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.09.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "1 Pegasi, HIP 105502, SAO 107073, HD 203504, GC 29914, HR 8173, DM BD+19  4691, TYC 1671-986-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "1 Pegasi",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.77",
	"RA_S" : 320.5216682,
	"DEC_S" : 19.80450879,
	"X" : 588,
	"Y" : 362,
	"Constellation" : "Pegasus ",
	"AMag" : 4.2,
	"key" : 25709,
	"title" : "1 Pegasi"
	},
{
	"Index" : "9961",
	"Description" : "2 Pegasi (2 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.54.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "2 Pegasi, HIP 106140, SAO 89752, HD 204724, GC 30109, HR 8225, DM BD+23  4325, TYC 2188-2203-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "2 Pegasi",
	"OType" : "Star",
	"Distance" : "120.7",
	"RA_S" : 322.48706197,
	"DEC_S" : 23.63883727,
	"X" : 558,
	"Y" : 315,
	"Constellation" : "Pegasus ",
	"AMag" : 4.7,
	"key" : 29961,
	"title" : "2 Pegasi"
	},
{
	"Index" : "5729",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "5 Pegasi, HIP 106787, SAO 107288, HD 205852, GC 30274, HR 8267, DM BD+18  4827, TYC 1673-930-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "5 Pegasi",
	"OType" : "Star",
	"Distance" : "98.29",
	"RA_S" : 324.4392916,
	"DEC_S" : 19.31861057,
	"Constellation" : "Pegasus ",
	"AMag" : 5.486,
	"key" : 25729,
	"title" : "5 Pegasi"
	},
{
	"Index" : "5698",
	"Description" : "9 Pegasi (9 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.34.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "9 Pegasi, HIP 107348, SAO 107365, HD 206859, GC 30444, HR 8313, DM BD+16  4582, TYC 1670-918-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "9 Pegasi",
	"OType" : "Variable Star",
	"Distance" : "282.77",
	"RA_S" : 326.12789848,
	"DEC_S" : 17.35001622,
	"X" : 521,
	"Y" : 402,
	"Constellation" : "Pegasus ",
	"AMag" : 4.454,
	"key" : 25698,
	"title" : "9 Pegasi"
	},
{
	"Index" : "10005",
	"Description" : "Kappa Pegasi is a triple star system in the constellation Pegasus. It has an apparent brightness of +4.13 magnitude and belongs to the spectral class F5IV; a subgiant star. The star has also the traditional name Jih.\r\rThis system consists of two components, designated Kappa Pegasi A and B, that are separated by an angular distance of 0.235 arcseconds. The binary nature of this pair was discovered by Sherburne W. Burnham in 1880. They orbit around each other every 11.6 years with a semimajor axis of 0.4 arcseconds. The brighter member of the pair, Kappa Pegasi B, is actually a spectroscopic binary, with the components designated Kappa Pegasi Ba and Kappa Pegasi Bb. They orbit about each other every six days. There is a fourth component, Kappa Pegasi C, which may be an optical companion.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "10 Pegasi, Kappa Pegasi, HIP 107354AB, SAO 89949, HD 206901, GC 30450, HR 8315, DM BD+24  4463, TYC 2193-2017-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Jih",
	"OType" : "Spectroscopic binary",
	"Distance" : "34.2",
	"RA_S" : 326.16136464,
	"DEC_S" : 25.645031,
	"X" : 512,
	"Y" : 293,
	"Constellation" : "Pegasus ",
	"AMag" : 4.185,
	"key" : 30005,
	"title" : "Jih"
	},
{
	"Index" : "10074",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "12 Pegasi, HIP 107472, SAO 89972, HD 207089, GC 30479, HR 8321, DM BD+22  4472, TYC 2202-1719-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "12 Pegasi",
	"OType" : "Star",
	"Distance" : "417.39",
	"RA_S" : 326.51818443,
	"DEC_S" : 22.94888042,
	"Constellation" : "Pegasus ",
	"AMag" : 5.422,
	"key" : 30074,
	"title" : "12 Pegasi"
	},
{
	"Index" : "14386",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "14 Pegasi, HIP 107763, SAO 90040, HD 207650, GC 30565, HR 8343, DM BD+29  4525, TYC 2718-2224-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "14 Pegasi",
	"OType" : "Spectroscopic binary",
	"Distance" : "84.21",
	"RA_S" : 327.46122816,
	"DEC_S" : 30.17421474,
	"Constellation" : "Pegasus ",
	"AMag" : 5.069,
	"key" : 34386,
	"title" : "14 Pegasi"
	},
{
	"Index" : "5699",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "13 Pegasi, HIP 107788AB, SAO 107425, HD 207652, GC 30569, HR 8344, DM BD+16  4612, TYC 1670-919-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "13 Pegasi",
	"OType" : "Flare Star",
	"Distance" : "33.41",
	"RA_S" : 327.53624965,
	"DEC_S" : 17.28584969,
	"Constellation" : "Pegasus ",
	"AMag" : 5.382,
	"key" : 25699,
	"title" : "13 Pegasi"
	},
{
	"Index" : "10104",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "16 Pegasi, HIP 108022, SAO 90075, HD 208057, GC 30635, HR 8356, DM BD+25  4635, TYC 2206-1964-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "16 Pegasi",
	"OType" : "Be Star",
	"Distance" : "193.3",
	"RA_S" : 328.26570276,
	"DEC_S" : 25.92513943,
	"Constellation" : "Pegasus ",
	"AMag" : 5.055,
	"key" : 30104,
	"title" : "16 Pegasi"
	},
{
	"Index" : "38394",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "22 Pegasi, Nu Pegasi, HIP 109068, SAO 127285, HD 209747, GC 30894, HR 8413, DM BD+04  4800, TYC 564-2591-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Nu Pegasi",
	"OType" : "Variable Star",
	"Distance" : "83.15",
	"RA_S" : 331.41979522,
	"DEC_S" : 5.05853081,
	"Constellation" : "Pegasus ",
	"AMag" : 5.018,
	"key" : 58394,
	"title" : "Nu Pegasi"
	},
{
	"Index" : "10120",
	"Description" : "Iota Pegasi (24 Peg, HD 210027) is a star located within the constellation Pegasus. It is about 40 light-years from Earth. It is a binary star system.\r\rIota Pegasi A is a yellowish-white star somewhat brighter than the sun. It and the dimmer Iota Pegasi B orbit each other with a period of about 10 days. In about four billion years from now, component A will evolve off the main sequence into a giant. In the process it will overflow its Roche lobe and begin to transfer mass onto the secondary. This may cause the secondary to acquire enough mass to become the primary component. After both stars have passed through the giant star stage, the end result will be a pair of co-orbiting white dwarfs in about eight billion years.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "24 Pegasi, Iota Pegasi, HIP 109176, SAO 90238, HD 210027, GC 30932, HR 8430, DM BD+24  4533, TYC 2208-2471-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Iota Pegasi",
	"OType" : "Spectroscopic binary",
	"Distance" : "11.73",
	"RA_S" : 331.75277679,
	"DEC_S" : 25.34511025,
	"X" : 446,
	"Y" : 302,
	"Constellation" : "Pegasus ",
	"AMag" : 3.809,
	"key" : 30120,
	"title" : "Iota Pegasi"
	},
{
	"Index" : "14441",
	"Description" : "Pi2 Pegasi (\u03C02 Peg, \u03C02 Pegasi) is a star in the constellation Pegasus.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "29 Pegasi, Pi Pegasi, HIP 109410, SAO 72077, HD 210459, GC 31016, HR 8454, DM BD+32  4352, TYC 2724-2354-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Pi2 Pegasi",
	"OType" : "Star",
	"Distance" : "80.63",
	"RA_S" : 332.49684589,
	"DEC_S" : 33.17822027,
	"X" : 432,
	"Y" : 200,
	"Constellation" : "Pegasus ",
	"AMag" : 4.325,
	"key" : 34441,
	"title" : "Pi2 Pegasi"
	},
{
	"Index" : "38428",
	"Description" : "Theta Pegasi (\u03B8 Peg) is a star in the constellation Pegasus. It has the traditional name Baham (\u0022the livestocks\u0022).\r\rIn Chinese, \u5371\u5BBF (W\u0113i S\u00F9), meaning Rooftop, refers to an asterism consisting of \u03B8 Pegasi, \u03B1 Aquarii and \u03B5 Pegasi. Consequently, \u03B8 Pegasi itself is known as \u5371\u5BBF\u4E8C (W\u0113i S\u00F9 \u00E8r, English: the Second Star of Rooftop.)\r\rTheta Pegasi is of spectral class A2 and has apparent magnitude +3.53. It is approximately 67 light years from Earth. This star has 2.6 times the Sun\u0027s radius and it is radiating 25 times the luminosity of the Sun from its outer envelope at an effective temperature of 7,951 K.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "26 Pegasi, Theta Pegasi, HIP 109427, SAO 127340, HD 210418, GC 31013, HR 8450, DM BD+05  4961, TYC 565-1999-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Baham",
	"OType" : "Variable Star",
	"Distance" : "28.28",
	"RA_S" : 332.54993865,
	"DEC_S" : 6.19786326,
	"X" : 446,
	"Y" : 551,
	"Constellation" : "Pegasus ",
	"AMag" : 3.519,
	"key" : 58428,
	"shortTitle" : "Baham; Bakham",
	"title" : "Baham"
	},
{
	"Index" : "14555",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "HIP 109654, SAO 72132, HD 210889, GC 31081, HR 8475, DM BD+33 4456, TYC 2741-2741-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "HR 8475",
	"OType" : "Star",
	"Distance" : "79.07",
	"RA_S" : 333.19926575,
	"DEC_S" : 34.60458821,
	"Constellation" : "Pegasus ",
	"AMag" : 5.47,
	"key" : 34555,
	"title" : "HR 8475"
	},
{
	"Index" : "38468",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "30 Pegasi, HIP 110298, SAO 127453, HD 211924, GC 31230, HR 8513, DM BD+05  4998, TYC 566-1004-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "30 Pegasi",
	"OType" : "Variable Star",
	"Distance" : "384.29",
	"RA_S" : 335.11490173,
	"DEC_S" : 5.78949685,
	"Constellation" : "Pegasus ",
	"AMag" : 5.363,
	"key" : 58468,
	"title" : "30 Pegasi"
	},
{
	"Index" : "10250",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "32 Pegasi, HIP 110371AF, SAO 90440, HD 212097, GC 31253, HR 8522, DM BD+27  4299, TYC 2230-2066-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "32 Pegasi",
	"OType" : "Double or multiple star",
	"Distance" : "208.84",
	"RA_S" : 335.33057367,
	"DEC_S" : 28.33052742,
	"Constellation" : "Pegasus ",
	"AMag" : 4.792,
	"key" : 30250,
	"title" : "32 Pegasi"
	},
{
	"Index" : "1203",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "31 Pegasi, HIP 110386, SAO 107854, HD 212076, GC 31255, HR 8520, DM BD+11  4784, TYC 1146-1242-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "31 Pegasi",
	"OType" : "Be Star",
	"Distance" : "486.19",
	"RA_S" : 335.37947949,
	"DEC_S" : 12.20518618,
	"Constellation" : "Pegasus ",
	"AMag" : 4.789,
	"key" : 21203,
	"title" : "31 Pegasi"
	},
{
	"Index" : "38355",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "35 Pegasi, HIP 110882, SAO 127540, HD 212943, GC 31377, HR 8551, DM BD+03  4710, TYC 563-1818-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "35 Pegasi",
	"OType" : "High proper-motion Star",
	"Distance" : "45.46",
	"RA_S" : 336.96467549,
	"DEC_S" : 4.69566169,
	"Constellation" : "Pegasus ",
	"AMag" : 4.906,
	"key" : 58355,
	"title" : "35 Pegasi"
	},
{
	"Index" : "1264",
	"Description" : "Zeta Pegasi (\u03B6 Peg) is a single star in the northern constellation of Pegasus. It has the traditional name, Homam, meaning \u0022Man of High Spirit\u0022 or \u0022Lucky Star of High Minded\u0022. With an apparent visual magnitude of +3.4, this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus. Parallax measurements place it at a distance of around 204 light-years (63 parsecs) from Earth.\r\rThis star has a stellar classification of B8 V, which identifies it as a large B-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. The radius of this star is about four times that of the Sun. It is a slowly pulsating B star that varies slightly in luminosity with a period of 22.952 \u00B1 0.804 hours, completing 1.04566 cycles per day. Zeta Pegasi is about 120 million years old and is rotating rapidly with a projected rotational velocity in the range of 140\u2013210 km s\u20131. The effective temperature of its outer envelope is around 11,190 K, giving it the characteristic blue-white glow of a B-type star.\r\rZeta Pegasi has been examined for infrared excess that may indicate the presence of circumstellar matter, but none was found. This star does have two optical companions. The first is a magnitude 11.6 star at an angular separation of 68 arcseconds along a position angle of 139\u00B0, as of 1997. The second is an 11th magnitude star at a separation of 177 arcseconds with a position angle of 5\u00B0. Zeta Pegasi is not known to be a member of a stellar association.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "42 Pegasi, Zeta Pegasi, HIP 112029, SAO 108103, HD 214923, GC 31664, HR 8634, DM BD+10  4797, TYC 1155-2187-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Homam",
	"OType" : "Star",
	"Distance" : "62.65",
	"RA_S" : 340.36555,
	"DEC_S" : 10.831289,
	"X" : 345,
	"Y" : 493,
	"Constellation" : "Pegasus ",
	"AMag" : 3.378,
	"key" : 21264,
	"shortTitle" : "Homan; Humam; Al Hammam; Khomam",
	"title" : "Homam"
	},
{
	"Index" : "10269",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "43 Pegasi, Omicron Pegasi, HIP 112051, SAO 90717, HD 214994, GC 31674, HR 8641, DM BD+28  4436, TYC 2232-1590-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Omicron Pegasi",
	"OType" : "Star",
	"Distance" : "91.16",
	"RA_S" : 340.43919248,
	"DEC_S" : 29.307631,
	"Constellation" : "Pegasus ",
	"AMag" : 4.789,
	"key" : 30269,
	"title" : "Omicron Pegasi"
	},
{
	"Index" : "14519",
	"Description" : "Eta Pegasi (\u03B7 Peg) is a binary star in the constellation Pegasus. It has the traditional name Matar, which comes from the Arabic Al Sa\u02BDd al Ma\u1E6Dar (\u0633\u0639\u062F \u0627\u0644\u0645\u0637\u0631) meaning lucky star of rain. The apparent visual magnitude of this star is +2.95, making this the fifth brightest member of Pegasus. Based upon parallax measurements, the distance to this star is about 167 light-years (51 parsecs).\r\rThis system consists of a pair of stars in a binary orbit with a period of 813 days and an eccentricity of 0.183. The primary component is a bright giant star with a stellar classification of G2 II and about four times the mass of the Sun. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is 3.26 \u00B1 0.07 mas, which, at its estimated distance, equates to a physical radius of nearly 18 times the radius of the Sun. It is radiating 247 times the luminosity of the Sun from its expanded outer envelope at an effective temperature of 5,450 K. The rotation rate of the star slowed as it expanded, so it has a projected rotational velocity of 1.7 km s\u20131 with an estimated rotation period of 818 days.\r\rThe secondary component is an F-type main sequence star with a classification of F0 V. There are also 2 class G stars further away that may or may not be physically related to the main pair.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "44 Pegasi, Eta Pegasi, HIP 112158, SAO 90734, HD 215182, GC 31706, HR 8650, DM BD+29  4741, TYC 2736-1823-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Eta Pegasi",
	"OType" : "Spectroscopic binary",
	"Distance" : "65.53",
	"RA_S" : 340.75057944,
	"DEC_S" : 30.22124754,
	"X" : 341,
	"Y" : 241,
	"Constellation" : "Pegasus ",
	"AMag" : 3.016,
	"key" : 34519,
	"title" : "Eta Pegasi"
	},
{
	"Index" : "10204",
	"Description" : "Lambda Pegasi (\u03BB Peg, \u03BB Pegasi) is a fourth-magnitude star in the constellation Pegasus. It has the traditional name Sadalpheretz, sometimes spelled Sadalpheris or Sad Al Faris, from the Arabic \u0633\u0639\u062F \u0627\u0644\u0641\u0631\u0633 meaning \u0022Luck of the Stallion\u0022, its etymology similar to that of the star Alpheratz, with both referring to the mythological winged-horse Pegasus.\r\rSadalpheretz is a yellow giant with stellar classification G8II-III. With a mass of 1.5 M\u2609 and radius that is 28.5 R\u2609, the star boasts a bolometric luminosity that is roughly 390 L\u2609. Its apparent magnitude was calibrated in 1983 at 3.96, yielding an intrinsic brightness of -1.45. Parallax calculations place the star at a distance of roughly 112 parsecs from Earth, or 365 \u00B1 10 light years away, about three times the distance of its line-of-sight double Sadalbari.\r\rIn the constellation, Lambda and Mu lie to the southwest of Beta Pegasi, the nearest bright star.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "47 Pegasi, Lambda Pegasi, HIP 112440, SAO 90775, HD 215665, GC 31776, HR 8667, DM BD+22  4709, TYC 2221-1666-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Sadalpheretz",
	"OType" : "Star",
	"Distance" : "111.89",
	"RA_S" : 341.63282442,
	"DEC_S" : 23.56565448,
	"X" : 330,
	"Y" : 327,
	"Constellation" : "Pegasus ",
	"AMag" : 4.068,
	"key" : 30204,
	"title" : "Sadalpheretz"
	},
{
	"Index" : "1263",
	"Description" : "Xi Pegasi (\u03BE Peg, \u03BE Pegasi) is a star in the constellation Pegasus.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "46 Pegasi, Xi Pegasi, HIP 112447, SAO 108165, HD 215648, GC 31778, HR 8665, DM BD+11  4875, TYC 1155-2186-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Xi Pegasi",
	"OType" : "High proper-motion Star",
	"Distance" : "16.3",
	"RA_S" : 341.67325688,
	"DEC_S" : 12.17288835,
	"X" : 328,
	"Y" : 475,
	"Constellation" : "Pegasus ",
	"AMag" : 4.251,
	"key" : 21263,
	"title" : "Xi Pegasi"
	},
{
	"Index" : "10225",
	"Description" : "Mu Pegasi (\u03BC Peg, \u03BC Pegasi) is a star in the northern constellation of Pegasus. It has the traditional name Sadalbari, which derives from the Arabic term for \u0022luck star of the splendid one\u0022. The apparent visual magnitude of this star is 3.5, which is bright enough to be seen with the naked eye even on a moonlit night. The distance to this star can be determined with parallax measurements, which yields a value of 106.1 light-years (32.5 parsecs).\r\rThe spectrum of this star matches a stellar classification of G8 III. The luminosity class of \u0027III\u0027 means that it has exhausted the hydrogen fuel at its core and evolved into a giant star. It is slightly more massive than the Sun, but has expanded to nearly ten times the Sun\u0027s radius. (Mishenina et al (2006) list it with an estimated 2.7 times the mass of the Sun.) The effective temperature of the outer atmosphere is about 4,950 K, which is cooler than the Sun and gives it the yellow hue of a G-type star. The abundance of elements other than hydrogen and helium, what astronomers term the metallicity, is similar to the abundance in the Sun.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "48 Pegasi, Mu Pegasi, HIP 112748, SAO 90816, HD 216131, GC 31851, HR 8684, DM BD+23  4615, TYC 2225-1821-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Sadalbari",
	"OType" : "High proper-motion Star",
	"Distance" : "32.53",
	"RA_S" : 342.50080903,
	"DEC_S" : 24.60157698,
	"X" : 320,
	"Y" : 314,
	"Constellation" : "Pegasus ",
	"AMag" : 3.604,
	"key" : 30225,
	"title" : "Sadalbari"
	},
{
	"Index" : "1252",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "49 Pegasi, Sigma Pegasi, HIP 112935, SAO 127810, HD 216385, GC 31899, HR 8697, DM BD+09  5122, TYC 1153-1558-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Sigma Pegasi",
	"OType" : "High proper-motion Star",
	"Distance" : "27.28",
	"RA_S" : 343.10031546,
	"DEC_S" : 9.83566698,
	"Constellation" : "Pegasus ",
	"AMag" : 5.213,
	"key" : 21252,
	"title" : "Sigma Pegasi"
	},
{
	"Index" : "1253",
	"Description" : "Rho Pegasi (\u03C1 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.91.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "50 Pegasi, Rho Pegasi, HIP 113186, SAO 127839, HD 216735, GC 31963, HR 8717, DM BD+08  4961, TYC 1153-1559-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Rho Pegasi",
	"OType" : "Star",
	"Distance" : "95.59",
	"RA_S" : 343.80696167,
	"DEC_S" : 8.81615347,
	"X" : 262,
	"Y" : 510,
	"Constellation" : "Pegasus ",
	"AMag" : 4.902,
	"key" : 21253,
	"title" : "Rho Pegasi"
	},
{
	"Index" : "1313",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "55 Pegasi, HIP 114144, SAO 127976, HD 218329, GC 32196, HR 8795, DM BD+08  4997, TYC 1160-1745-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "55 Pegasi",
	"OType" : "Variable Star",
	"Distance" : "100.7",
	"RA_S" : 346.75108748,
	"DEC_S" : 9.40949244,
	"Constellation" : "Pegasus ",
	"AMag" : 4.715,
	"key" : 21313,
	"title" : "55 Pegasi"
	},
{
	"Index" : "10308",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "56 Pegasi, HIP 114155, SAO 91019, HD 218356, GC 32201, HR 8796, DM BD+24  4716, TYC 2239-1475-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "56 Pegasi",
	"OType" : "Spectroscopic binary",
	"Distance" : "181.11",
	"RA_S" : 346.77808169,
	"DEC_S" : 25.46826185,
	"Constellation" : "Pegasus ",
	"AMag" : 4.9,
	"key" : 30308,
	"title" : "56 Pegasi"
	},
{
	"Index" : "1321",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "57 Pegasi, HIP 114347, SAO 128001, HD 218634, GC 32252, HR 8815, DM BD+07  4981, TYC 1161-1796-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "57 Pegasi",
	"OType" : "S Star",
	"Distance" : "237.91",
	"RA_S" : 347.38107087,
	"DEC_S" : 8.67716555,
	"Constellation" : "Pegasus ",
	"AMag" : 5.294,
	"key" : 21321,
	"title" : "57 Pegasi"
	},
{
	"Index" : "1319",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "58 Pegasi, HIP 114389, SAO 128007, HD 218700, GC 32267, HR 8821, DM BD+09  5170, TYC 1161-1794-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "58 Pegasi",
	"OType" : "Star",
	"Distance" : "246.39",
	"RA_S" : 347.50609036,
	"DEC_S" : 9.82208892,
	"Constellation" : "Pegasus ",
	"AMag" : 5.373,
	"key" : 21319,
	"title" : "58 Pegasi"
	},
{
	"Index" : "1320",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "59 Pegasi, HIP 114520, SAO 128022, HD 218918, GC 32302, HR 8826, DM BD+07  4991, TYC 1161-1795-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "59 Pegasi",
	"OType" : "Star",
	"Distance" : "74.18",
	"RA_S" : 347.93412575,
	"DEC_S" : 8.72011319,
	"Constellation" : "Pegasus ",
	"AMag" : 5.17,
	"key" : 21320,
	"title" : "59 Pegasi"
	},
{
	"Index" : "10298",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "62 Pegasi, Tau Pegasi, HIP 115250, SAO 91186, HD 220061, GC 32503, HR 8880, DM BD+22  4810, TYC 2237-1659-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Kerb",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "49.56",
	"RA_S" : 350.15934509,
	"DEC_S" : 23.74033926,
	"Constellation" : "Pegasus ",
	"AMag" : 4.602,
	"key" : 30298,
	"shortTitle" : "Salm; Markab (also HD218045); El khereb",
	"title" : "Kerb"
	},
{
	"Index" : "14625",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "64 Pegasi, HIP 115355AB, SAO 73205, HD 220222, GC 32522, HR 8887, DM BD+31  4897, TYC 2752-2219-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "64 Pegasi",
	"OType" : "Double or multiple star",
	"Distance" : "247.75",
	"RA_S" : 350.4788879,
	"DEC_S" : 31.81245495,
	"Constellation" : "Pegasus ",
	"AMag" : 5.33,
	"key" : 34625,
	"title" : "64 Pegasi"
	},
{
	"Index" : "1352",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "66 Pegasi, HIP 115444, SAO 108580, HD 220363, GC 32543, HR 8893, DM BD+11  4993, TYC 1165-1549-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "66 Pegasi",
	"OType" : "Star",
	"Distance" : "118.9",
	"RA_S" : 350.76904628,
	"DEC_S" : 12.31391783,
	"Constellation" : "Pegasus ",
	"AMag" : 5.232,
	"key" : 21352,
	"title" : "66 Pegasi"
	},
{
	"Index" : "10299",
	"Description" : "Upsilon Pegasi (\u03C5 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.40.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "68 Pegasi, Upsilon Pegasi, HIP 115623, SAO 91253, HD 220657, GC 32585, HR 8905, DM BD+22  4833, TYC 2237-1660-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Upsilon Pegasi",
	"OType" : "High proper-motion Star",
	"Distance" : "52.24",
	"RA_S" : 351.34493244,
	"DEC_S" : 23.40410164,
	"X" : 214,
	"Y" : 325,
	"Constellation" : "Pegasus ",
	"AMag" : 4.49,
	"key" : 30299,
	"title" : "Upsilon Pegasi"
	},
{
	"Index" : "1367",
	"Description" : "70 Pegasi (70 Peg) is a star in the constellation Pegasus. Its apparent magnitude is 4.55.",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "70 Pegasi, HIP 115919, SAO 108638, HD 221115, GC 32667, HR 8923, DM BD+11  5009, TYC 1168-1611-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "70 Pegasi",
	"OType" : "Star",
	"Distance" : "53.51",
	"RA_S" : 352.28874138,
	"DEC_S" : 12.76055418,
	"X" : 193,
	"Y" : 463,
	"Constellation" : "Pegasus ",
	"AMag" : 4.638,
	"key" : 21367,
	"title" : "70 Pegasi"
	},
{
	"Index" : "14723",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "72 Pegasi, HIP 116310AB, SAO 73341, HD 221673, GC 32772, HR 8943, DM BD+30  4978, TYC 2766-1925-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "72 Pegasi",
	"OType" : "Double or multiple star",
	"Distance" : "167.2",
	"RA_S" : 353.48834402,
	"DEC_S" : 31.32528185,
	"Constellation" : "Pegasus ",
	"AMag" : 5.167,
	"key" : 34723,
	"title" : "72 Pegasi"
	},
{
	"Index" : "6068",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "75 Pegasi, HIP 116611, SAO 108732, HD 222133, GC 32842, HR 8963, DM BD+17  4952, TYC 1723-2166-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "75 Pegasi",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "71.35",
	"RA_S" : 354.48667695,
	"DEC_S" : 18.40067093,
	"Constellation" : "Pegasus ",
	"AMag" : 5.481,
	"key" : 26068,
	"title" : "75 Pegasi"
	},
{
	"Index" : "1410",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "77 Pegasi, HIP 117020, SAO 108789, HD 222764, GC 32945, HR 8991, DM BD+09  5268, TYC 1173-1740-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "77 Pegasi",
	"OType" : "Variable Star",
	"Distance" : "188.86",
	"RA_S" : 355.84316193,
	"DEC_S" : 10.33153625,
	"Constellation" : "Pegasus ",
	"AMag" : 5.276,
	"key" : 21410,
	"title" : "77 Pegasi"
	},
{
	"Index" : "10434",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "78 Pegasi, HIP 117073A, SAO 91457, HD 222842, GC 32954, HR 8997, DM BD+28  4627, TYC 2257-2521-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "78 Pegasi",
	"OType" : "Double or multiple star",
	"Distance" : "68.65",
	"RA_S" : 355.99783892,
	"DEC_S" : 29.36145541,
	"Constellation" : "Pegasus ",
	"AMag" : 5.067,
	"key" : 30434,
	"title" : "78 Pegasi"
	},
{
	"Index" : "6079",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "81 Pegasi, Phi Pegasi, HIP 117718, SAO 108878, HD 223768, GC 33119, HR 9036, DM BD+18  5231, TYC 1725-2097-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Phi Pegasi",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "141.59",
	"RA_S" : 358.1220291,
	"DEC_S" : 19.12028556,
	"Constellation" : "Pegasus ",
	"AMag" : 5.258,
	"key" : 26079,
	"title" : "Phi Pegasi"
	},
{
	"Index" : "1416",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "82 Pegasi, HIP 117730, SAO 108879, HD 223781, GC 33122, HR 9039, DM BD+10  5004, TYC 1174-1713-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "82 Pegasi",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "55.83",
	"RA_S" : 358.15458888,
	"DEC_S" : 10.94732487,
	"Constellation" : "Pegasus ",
	"AMag" : 5.335,
	"key" : 21416,
	"title" : "82 Pegasi"
	},
{
	"Index" : "10421",
	"MapNum" : "35",
	"ImageNum" : "35",
	"Desig" : "84 Pegasi, Psi Pegasi, HIP 118131, SAO 91611, HD 224427, GC 33230, HR 9064, DM BD+24  4865, TYC 2255-2883-1",
	"group" : { "key" : "Pegasus" },
	"Common" : "Psi Pegasi",
	"OType" : "Double or multiple star",
	"Distance" : "145.77",
	"RA_S" : 359.4396949,
	"DEC_S" : 25.1414001,
	"Constellation" : "Pegasus ",
	"AMag" : 4.832,
	"key" : 30421,
	"title" : "Psi Pegasi"
	},
{
	"Index" : "19312",
	"Description" : "Phi Persei (Phi Per, \u03C6 Persei, \u03C6 Per) is a Class B2Vpe, fourth-magnitude star in the constellation Perseus. Due to its isolation and distance from Cassiopeia, Andromeda and the rest of Perseus, John Flamsteed never took thought to assign a number and constellation to Phi Persei.\r\rPhi Persei is binary consisting of a blue main sequence primary of class B2 and an apparent magnitude of 4.01 and a hot subdwarf secondary. The primary has 9.3 times the radius of the Sun. Phi Persei is also a variable star with rapid variations in its brightness and spectrum. The Phi Persei stellar system is located about 716 light-years from Earth.\r\rPhi Persei was a latter designation of 54 Andromedae.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "Phi Persei, HIP 8068, SAO 22554, HD 10516, GC 2102, HR 496, DM BD+49   444, TYC 3291-2118-1",
	"group" : { "backgroundImage" : "images/Alignment/07.png",
		"description" : "Perseus is a constellation in the northern sky, named after the Greek hero Perseus. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations defined by the International Astronomical Union. Located in the northern celestial hemisphere, it lies nearby several other constellations from the legend of Perseus, including Andromeda (the maiden he rescued), Cetus (the sea monster he slew) and Cepheus and Cassiopeia (Andromeda\u0027s royal parents).\r\rIts brightest star is the yellow-white supergiant Alpha Persei, or Mirfak, which shines with a magnitude of 1.79. The most notable star, however, is the famous variable star Algol (Beta Persei), linked with ominous legends on account of its apparent variability. GK Persei was a nova which brightened to magnitude 0.2 in 1901, making it briefly one of the brightest stars in the sky. The constellation also gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. The constellation also hosts the annual Perseids meteor shower, one of the most prominent.\r\rThe Greek constellation may be an adaptation of the Babylonian constellation known as the Old Man (MUL.SHU.GI) which is associated with East (as a cardinal direction) in the MUL.APIN, an astronomical compilation dating to around 1000 BCE.\r\rIn Greek mythology, Perseus was the son of Danae, who became the hero who slayed Medusa. He later used the Gorgon\u0027s head to rescue the princess Andromeda from the monster Cetus.\r\rFour Chinese constellations existed in the area of the sky now assigned to Perseus. T\u0027ien-tchouen, translated as the \u0022Celestial Boat\u0022, was the third paranatellon of the third house of the White Tiger of the West. It represented the boats that Chinese people were reminded to build in case of a catastrophic flood season. Tsi-choui, translated as the \u0022Swollen Waters\u0022, was the fourth paranatellon of the third house of the White Tiger of the West. It represented the potential of unusually high floods during the beginning of the flood season, which commenced at the end of August and beginning of September. Ta-ling, translated as the \u0022Great Trench\u0022, was the fifth paranatellon of the third house of the White Tiger of the West. It represented the trenches where criminals executed en masse in August were interred. The pile of corpses prior to their interment was represented by Tsi-chi (Algol), the sixth paranatellon of the third house of the White Tiger.\r\rThe Double Cluster, h and \u03C7 Persei, had special significance in Chinese astronomy. Known as Hsi and Ho, the two clusters represented two astronomers who failed to predict a total solar eclipse and were beheaded thereafter.\r\rIn Polynesia, Perseus was not commonly recognized as a separate constellation; the only people that named it were the people of the Society Islands, who called it Faa-iti, meaning \u0022Little Valley\u0022. Algol may have been named Matohi by the Maori people, but the evidence for this identification is disputed. Matohi (\u0022Split\u0022) occasionally came into conflict with Tangaroa-whakapau over which of them should appear in the sky, the outcome affecting the tides. It matches the Maori description of a blue-white star near Aldebaran but does not disappear as the myth would indicate.",
		"key" : "Perseus",
		"grouptype" : "Perseus",
		"Meaning" : "Perseus (mythological character)",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Perseus",
		"title" : "Perseus Objects Group" },
	"Common" : "Phi Persei",
	"OType" : "Be Star",
	"Distance" : "219.75",
	"RA_S" : 25.91515198,
	"DEC_S" : 50.68873018,
	"X" : 485,
	"Y" : 116,
	"Constellation" : "Perseus ",
	"AMag" : 4.011,
	"key" : 39312,
	"title" : "Phi Persei"
	},
{
	"Index" : "22873",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "1 Persei, HIP 8704, SAO 22690, HD 11241, GC 2241, HR 533, DM BD+54   396, TYC 3688-2149-1",
	"group" : { "key" : "Perseus" },
	"Common" : "1 Persei",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "388.82",
	"RA_S" : 27.99716507,
	"DEC_S" : 55.14738243,
	"Constellation" : "Perseus ",
	"AMag" : 5.497,
	"key" : 42873,
	"title" : "1 Persei"
	},
{
	"Index" : "22880",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "4 Persei, g Persei, HIP 9505, SAO 22859, HD 12303, GC 2442, HR 590, DM BD+53   439, TYC 3689-131-1",
	"group" : { "key" : "Perseus" },
	"Common" : "g Persei",
	"OType" : "Star",
	"Distance" : "222.51",
	"RA_S" : 30.57545287,
	"DEC_S" : 54.48754132,
	"Constellation" : "Perseus ",
	"AMag" : 4.98,
	"key" : 42880,
	"title" : "g Persei"
	},
{
	"Index" : "22896",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "9 Persei, i Persei, HIP 11060, SAO 23256, HD 14489, GC 2836, HR 685, DM BD+55   598, TYC 3690-2172-1",
	"group" : { "key" : "Perseus" },
	"Common" : "i Persei",
	"OType" : "Pulsating variable Star",
	"RA_S" : 35.58930972,
	"DEC_S" : 55.84565729,
	"Constellation" : "Perseus ",
	"AMag" : 5.237,
	"key" : 42896,
	"title" : "i Persei"
	},
{
	"Index" : "15348",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "12 Persei, HIP 12623, SAO 55793, HD 16739, GC 3245, HR 788, DM BD+39   610, TYC 2849-2054-1",
	"group" : { "key" : "Perseus" },
	"Common" : "12 Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "24.19",
	"RA_S" : 40.5621436,
	"DEC_S" : 40.19394211,
	"Constellation" : "Perseus ",
	"AMag" : 4.961,
	"key" : 35348,
	"title" : "12 Persei"
	},
{
	"Index" : "19429",
	"Description" : "Theta Persei (Theta Per, \u03B8 Persei, \u03B8 Per) is a star system 37 light years away from Earth, in the constellation Perseus. The primary star is a yellowish dwarf (main sequence) star of spectral type F7V, which is somewhat larger and brighter than our sun, but still within the range considered to have the potential for Earth-like planets. There is also a red dwarf companion of spectral type M1V, orbiting about 250 AU from the primary. The star\u0027s age is estimated to be 2.8 billion years but is certainly no less than 1.7 billion years and no greater than 3.9 billion years.\r\rTheta Persei is moving through the Galaxy at a speed of 30.5 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,700 and 34,200 light years from the center of the Galaxy.\r\rTheta Persei came closest to the Sun 285,000 years ago when it had brightened to magnitude 2.99 from a distance of 21.7 light years.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "13 Persei, Theta Persei, HIP 12777, SAO 38288, HD 16895, GC 3277, HR 799, DM BD+48   746, TYC 3304-2737-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Theta Persei",
	"OType" : "High proper-motion Star",
	"Distance" : "11.13",
	"RA_S" : 41.04994601,
	"DEC_S" : 49.22844754,
	"X" : 365,
	"Y" : 161,
	"Constellation" : "Perseus ",
	"AMag" : 4.155,
	"key" : 39429,
	"title" : "Theta Persei"
	},
{
	"Index" : "15315",
	"Description" : "16 Persei (16 Per) is a star in the constellation Perseus.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "16 Persei, HIP 13254, SAO 55928, HD 17584, GC 3401, HR 840, DM BD+37   646, TYC 2846-1429-1",
	"group" : { "key" : "Perseus" },
	"Common" : "16 Persei",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "37.02",
	"RA_S" : 42.64608807,
	"DEC_S" : 38.31865113,
	"X" : 364,
	"Y" : 303,
	"Constellation" : "Perseus ",
	"AMag" : 4.253,
	"key" : 35315,
	"title" : "16 Persei"
	},
{
	"Index" : "23078",
	"Description" : "Eta Persei (Eta Per, \u03B7 Persei, \u03B7 Per) is a star in the constellation Perseus. It also has the traditional name Miram. Miram belongs to spectral class K3 and has an apparent magnitude of +3.76. It is approximately 1331 light years away from Earth. This star is radiating 35,000 times the luminosity of the Sun.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "15 Persei, Eta Persei, HIP 13268, SAO 23655, HD 17506, GC 3390, HR 834, DM BD+55   714, TYC 3704-1332-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Miram",
	"OType" : "Star",
	"Distance" : "268.51",
	"RA_S" : 42.67421136,
	"DEC_S" : 55.8954932,
	"X" : 343,
	"Y" : 76,
	"Constellation" : "Perseus ",
	"AMag" : 3.942,
	"key" : 43078,
	"title" : "Miram"
	},
{
	"Index" : "11003",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "17 Persei, HIP 13328, SAO 55946, HD 17709, GC 3419, HR 843, DM BD+34   527, TYC 2334-1042-1",
	"group" : { "key" : "Perseus" },
	"Common" : "17 Persei",
	"OType" : "Variable Star",
	"Distance" : "142.59",
	"RA_S" : 42.87848766,
	"DEC_S" : 35.05974318,
	"Constellation" : "Perseus ",
	"AMag" : 4.735,
	"key" : 31003,
	"title" : "17 Persei"
	},
{
	"Index" : "15314",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "20 Persei, HIP 13490AB, SAO 55975, HD 17904, GC 3459, HR 855, DM BD+37   655, TYC 2846-1428-1",
	"group" : { "key" : "Perseus" },
	"Common" : "20 Persei",
	"OType" : "Double or multiple star",
	"Distance" : "70.45",
	"RA_S" : 43.42756675,
	"DEC_S" : 38.33748295,
	"Constellation" : "Perseus ",
	"AMag" : 5.391,
	"key" : 35314,
	"title" : "20 Persei"
	},
{
	"Index" : "23056",
	"Description" : "Tau Persei (Tau Per, \u03C4 Persei, \u03C4 Per) is multiple star system in constellation of Perseus, with an apparent magnitude of +3.93. The primary component is a yellow G-type giant. It is approximately 248 light years from Earth.\r\rTau Persei is moving through the Galaxy at a speed of 2.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,100 and 34,200 light years from the center of the Galaxy.\r\rIn Chinese, \u5927\u9675 (D\u00E0 L\u00EDng), meaning Mausoleum, refers to an asterism consisting of \u03C4 Persei, 9 Persei, \u03B9 Persei, \u03BA Persei, \u03B2 Persei, \u03C1 Persei, 16 Persei and 12 Persei. Consequently, \u03C4 Persei itself is known as \u5927\u9675\u4E8C (D\u00E0 L\u00EDng \u00E8r, English: the Second Star of Mausoleum.).",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "18 Persei, Tau Persei, HIP 13531, SAO 23685, HD 17879, GC 3462, HR 854, DM BD+52   641B, TYC 3701-1394-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Tau Persei",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "77.87",
	"RA_S" : 43.56442116,
	"DEC_S" : 52.76247888,
	"X" : 340,
	"Y" : 117,
	"Constellation" : "Perseus ",
	"AMag" : 4.013,
	"key" : 43056,
	"title" : "Tau Persei"
	},
{
	"Index" : "10959",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "21 Persei, HIP 13775, SAO 56031, HD 18296, GC 3544, HR 873, DM BD+31   509, TYC 2330-2043-1",
	"group" : { "key" : "Perseus" },
	"Common" : "21 Persei",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "97.96",
	"RA_S" : 44.3220073,
	"DEC_S" : 31.93421934,
	"Constellation" : "Perseus ",
	"AMag" : 5.091,
	"key" : 30959,
	"title" : "21 Persei"
	},
{
	"Index" : "15355",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "22 Persei, Pi Persei, HIP 13879, SAO 56047, HD 18411, GC 3567, HR 879, DM BD+39   681, TYC 2850-2115-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Gorgonea Secunda",
	"OType" : "Star",
	"Distance" : "94.89",
	"RA_S" : 44.69029797,
	"DEC_S" : 39.66272904,
	"Constellation" : "Perseus ",
	"AMag" : 4.69,
	"key" : 35355,
	"title" : "Gorgonea Secunda"
	},
{
	"Index" : "11002",
	"Description" : "24 Persei (24 Per) is a star in the constellation Perseus. Its apparent magnitude is 4.93.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "24 Persei, HIP 13905, SAO 56052, HD 18449, GC 3575, HR 882, DM BD+34   550, TYC 2334-1041-1",
	"group" : { "key" : "Perseus" },
	"Common" : "24 Persei",
	"OType" : "Star",
	"Distance" : "112.68",
	"RA_S" : 44.76532082,
	"DEC_S" : 35.18312749,
	"X" : 365,
	"Y" : 346,
	"Constellation" : "Perseus ",
	"AMag" : 5.073,
	"key" : 31002,
	"title" : "24 Persei"
	},
{
	"Index" : "19612",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 14043A, SAO 23763, HD 18537, GC 3600, HR 890, DM BD+51  665, TYC 3322-1409-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 890",
	"OType" : "Star",
	"Distance" : "136.29",
	"RA_S" : 45.21755402,
	"DEC_S" : 52.3517284,
	"Constellation" : "Perseus ",
	"AMag" : 5.209,
	"key" : 39612,
	"title" : "HR 890"
	},
{
	"Index" : "23055",
	"Description" : "Gamma Persei (Gamma Per, \u03B3 Persei, \u03B3 Per) is a binary star system in the constellation Perseus. The combined apparent visual magnitude of the pair is +2.9, making it the fourth brightest member of the constellation. The distance to this system has been measured using the parallax technique, giving an estimate of roughly 243 light-years (75 parsecs) with a 4% margin of error. About 4\u00B0 to the north of Gamma Persei is the radiance point for the annual Perseid meteor shower.\r\rThis is a wide eclipsing binary system with an orbital period of 5,329.8 days (14.6 years). This eclipse was first observed in 1990 and lasted for two weeks. During an eclipse, the primary passes in front of the secondary, causing the magnitude of the system to decrease by 0.55. The primary component of this system is a giant star with a stellar classification of G9 III. It has a projected rotational velocity of 50.0 km s\u22121 and a lengthy estimated rotation period of 14.6 years. The classification of the secondary remains tentative, with assignments of A3 V and A2(III).\r\rMass estimates for the two stars remain disparate. Using speckle interferometery, McAlister (1982) obtained mass estimates of 4.73 M\u2609 for the primary and 2.75 M\u2609 for the secondary, where M\u2609 is the mass of the Sun. He noted that the mass estimate was too high for the given classification of the primary. Martin and Mignard (1998) determined masses for both components based on data from the Hipparcos mission: 5.036 \u00B1 0.951 M\u2609 for the primary and 2.295 \u00B1 0.453 M\u2609 for the secondary. They admit that the high inclination of the orbit resulted in a large margin of error. Prieto and Lambert (1999) came up with a mass estimate of 3.81 M\u2609 for the primary, while Pizzolato and Maggio (2000) obtained 4.34 M\u2609. Ling et al. (2001) obtained estimates of 2.7 M\u2609 for the primary and 1.65 M\u2609 for the secondary, while Kaler (2001) obtained 2.5 and 1.9, respectively.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "23 Persei, Gamma Persei, HIP 14328, SAO 23789, HD 18925, GC 3664, HR 915, DM BD+52   654A, TYC 3701-1393-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Gamma Persei",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "74.44",
	"RA_S" : 46.19912808,
	"DEC_S" : 53.50643576,
	"X" : 319,
	"Y" : 109,
	"Constellation" : "Perseus ",
	"AMag" : 2.992,
	"key" : 43055,
	"title" : "Gamma Persei"
	},
{
	"Index" : "15319",
	"Description" : "Rho Persei (Rho Per, \u03C1 Persei, \u03C1 Per) is a star in the northern constellation of Perseus. It has the traditional name Gorgonea Tertia, being the third member of the quartet called the Gorgonea in reference to the Gorgons from the legend of Perseus. An apparent visual magnitude of +3.39 makes it visible to the naked eye, but a challenge to view from a well-lit urban environment. Based upon parallax measurements, it is located at a distance of roughly 308 light-years (94 pc) from Earth.\r\rRho Persei is a semiregular variable star of the \u03BC Cephei type, whose apparent magnitude varies between 3.3 and 4.0 with periods of 50, 120 and 250 days. The star has reached the asymptotic giant branch of its evolution. It is presently near the tip of the red giant branch with a stellar classification of M4 II. The outer envelope has an effective temperature of 4,111 K, giving it the red-orange hue of an M-type star.\r\rThis star has a mass five times the mass of the Sun, while its radius has expanded to 150 times solar. It is radiating some 2,290 times the Sun\u0027s luminosity. Rho Persei is losing mass at the rate of 1.2 \u00D7 10\u22128 solar masses per year, or the equivalent of the Sun\u0027s mass every 83 million years. It is about 440 million years in age.\r\rIn Chinese, \u5927\u9675 (D\u00E0 L\u00EDng), meaning Mausoleum, refers to an asterism consisting of \u03C1 Persei, 9 Persei, \u03C4 Persei, \u03B9 Persei, \u03BA Persei, \u03B2 Persei, 16 Persei and 12 Persei. Consequently, \u03C1 Persei itself is known as \u5927\u9675\u516D (D\u00E0 L\u00EDng li\u00F9, English: the Sixth Star of Mausoleum.).",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "25 Persei, Rho Persei, HIP 14354, SAO 56138, HD 19058, GC 3682, HR 921, DM BD+38   630, TYC 2847-1572-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Gorgonea Tertia",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "94.28",
	"RA_S" : 46.29413731,
	"DEC_S" : 38.84027493,
	"X" : 327,
	"Y" : 299,
	"Constellation" : "Perseus ",
	"AMag" : 3.539,
	"key" : 35319,
	"title" : "Gorgonea Tertia"
	},
{
	"Index" : "23114",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "k Persei, HIP 14382, SAO 23791, HD 18970, GC 3674, HR 918, DM BD+56   767, TYC 3709-1135-1",
	"group" : { "key" : "Perseus" },
	"Common" : "k Persei",
	"OType" : "Star",
	"Distance" : "64.7",
	"RA_S" : 46.38504777,
	"DEC_S" : 56.70571786,
	"Constellation" : "Perseus ",
	"AMag" : 4.88,
	"key" : 43114,
	"title" : "k Persei"
	},
{
	"Index" : "19563",
	"Description" : "Iota Persei (Iota Per, \u03B9 Persei, \u03B9 Per) is a main sequence dwarf star in the constellation Perseus. It is somewhat larger and greater in mass than the Sun, and is located about 34 light years distant. Iota Persei has a relatively high proper motion across the sky, and moves at a net velocity of 92 km/s, relative to the Sun.\r\rNo sub-stellar companions to this star have yet been found. There is a 12th-magnitude line-of-sight companion star that is not believed to be gravitationally associated with Iota Persei.\r\rIn Chinese, \u5927\u9675 (D\u00E0 L\u00EDng), meaning Mausoleum, refers to an asterism consisting of \u03B9 Persei, 9 Persei, \u03C4 Persei, \u03BA Persei, \u03B2 Persei, \u03C1 Persei, 16 Persei and 12 Persei. Consequently, \u03B9 Persei itself is known as \u5927\u9675\u4E09 (D\u00E0 L\u00EDng s\u0101n, English: the Third Star of Mausoleum.).",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "Iota Persei, HIP 14632, SAO 38597, HD 19373, GC 3740, HR 937, DM BD+49   857, TYC 3318-1840-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Iota Persei",
	"OType" : "High proper-motion Star",
	"Distance" : "10.54",
	"RA_S" : 47.26674916,
	"DEC_S" : 49.61327841,
	"X" : 312,
	"Y" : 160,
	"Constellation" : "Perseus ",
	"AMag" : 4.107,
	"key" : 39563,
	"title" : "Iota Persei"
	},
{
	"Index" : "15439",
	"Description" : "Kappa Persei (Kappa Per, \u03BA Persei, \u03BA Per) is a star in the constellation Perseus.\r\rThis star belongs to the spectral class K0 and has apparent magnitude +3.8. It is 112 light years from Earth. Kappa Persei is a triple star system consisting of a spectroscopic double star with a wider companion.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "27 Persei, Kappa Persei, HIP 14668, SAO 38609, HD 19476, GC 3755, HR 941, DM BD+44   631, TYC 2859-2274-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Kappa Persei",
	"OType" : "Variable Star",
	"Distance" : "34.56",
	"RA_S" : 47.37406045,
	"DEC_S" : 44.85753454,
	"X" : 314,
	"Y" : 220,
	"Constellation" : "Perseus ",
	"AMag" : 3.889,
	"key" : 35439,
	"title" : "Kappa Persei"
	},
{
	"Index" : "15372",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "28 Persei, Omega Persei, HIP 14817, SAO 56224, HD 19656, GC 3791, HR 947, DM BD+39   724, TYC 2852-2474-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Gorgonea Quarta",
	"OType" : "Star",
	"Distance" : "88.3",
	"RA_S" : 47.822421,
	"DEC_S" : 39.61158947,
	"Constellation" : "Perseus ",
	"AMag" : 4.732,
	"key" : 35372,
	"title" : "Gorgonea Quarta"
	},
{
	"Index" : "19622",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 15219, SAO 23914, HD 20123, GC 3883, HR 969, DM BD+50  729, TYC 3323-1510-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 969",
	"OType" : "Star in Cluster",
	"Distance" : "240.98",
	"RA_S" : 49.05084338,
	"DEC_S" : 50.93766153,
	"Constellation" : "Perseus ",
	"AMag" : 5.17,
	"key" : 39622,
	"title" : "HR 969"
	},
{
	"Index" : "15445",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "30 Persei, HIP 15338, SAO 38704, HD 20315, GC 3923, HR 982, DM BD+43   674, TYC 2860-2382-1",
	"group" : { "key" : "Perseus" },
	"Common" : "30 Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "195.29",
	"RA_S" : 49.44730921,
	"DEC_S" : 44.02502492,
	"Constellation" : "Perseus ",
	"AMag" : 5.465,
	"key" : 35445,
	"title" : "30 Persei"
	},
{
	"Index" : "19569",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "29 Persei, HIP 15404, SAO 23944, HD 20365, GC 3934, HR 987, DM BD+49   899, TYC 3319-2073-1",
	"group" : { "key" : "Perseus" },
	"Common" : "29 Persei",
	"OType" : "Star in Cluster",
	"Distance" : "188.58",
	"RA_S" : 49.65725362,
	"DEC_S" : 50.22217115,
	"Constellation" : "Perseus ",
	"AMag" : 5.144,
	"key" : 39569,
	"title" : "29 Persei"
	},
{
	"Index" : "11104",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 15416, SAO 56340, HD 20468, GC 3948, HR 991, DM BD+33  619, TYC 2349-1954-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 991",
	"OType" : "Star",
	"Distance" : "358.05",
	"RA_S" : 49.6826104,
	"DEC_S" : 34.22265255,
	"Constellation" : "Perseus ",
	"AMag" : 4.993,
	"key" : 31104,
	"title" : "HR 991"
	},
{
	"Index" : "19570",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "31 Persei, HIP 15444, SAO 38714, HD 20418, GC 3945, HR 989, DM BD+49   902, TYC 3319-2074-1",
	"group" : { "key" : "Perseus" },
	"Common" : "31 Persei",
	"OType" : "Star in Cluster",
	"Distance" : "182.96",
	"RA_S" : 49.78182486,
	"DEC_S" : 50.09496312,
	"Constellation" : "Perseus ",
	"AMag" : 5.021,
	"key" : 39570,
	"title" : "31 Persei"
	},
{
	"Index" : "15543",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "32 Persei, l Persei, HIP 15648, SAO 38750, HD 20677, GC 4004, HR 1002, DM BD+42   750, TYC 2873-3762-1",
	"group" : { "key" : "Perseus" },
	"Common" : "l Persei",
	"OType" : "Variable Star",
	"Distance" : "46.16",
	"RA_S" : 50.3606571,
	"DEC_S" : 43.32965275,
	"Constellation" : "Perseus ",
	"AMag" : 4.954,
	"key" : 35543,
	"title" : "l Persei"
	},
{
	"Index" : "19589",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 15770, SAO 38768, HD 20809, GC 4024, HR 1011, DM BD+48  899, TYC 3320-2812-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR  1011",
	"OType" : "Star in Cluster",
	"Distance" : "181.57",
	"RA_S" : 50.80497592,
	"DEC_S" : 49.21326436,
	"Constellation" : "Perseus ",
	"AMag" : 5.295,
	"key" : 39589,
	"title" : "HR  1011"
	},
{
	"Index" : "19592",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 16147, SAO 38849, HD 21278, GC 4108, HR 1034, DM BD+48  920, TYC 3320-2815-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 1034",
	"OType" : "Spectroscopic binary",
	"Distance" : "180.33",
	"RA_S" : 52.01279081,
	"DEC_S" : 49.06286921,
	"Constellation" : "Perseus ",
	"AMag" : 4.962,
	"key" : 39592,
	"title" : "HR 1034"
	},
{
	"Index" : "19586",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "34 Persei, HIP 16244A, SAO 38872, HD 21428, GC 4133, HR 1044, DM BD+49   945, TYC 3320-2810-1",
	"group" : { "key" : "Perseus" },
	"Common" : "34 Persei",
	"OType" : "Double or multiple star",
	"Distance" : "181.35",
	"RA_S" : 52.34187782,
	"DEC_S" : 49.50895109,
	"Constellation" : "Perseus ",
	"AMag" : 4.715,
	"key" : 39586,
	"title" : "34 Persei"
	},
{
	"Index" : "19540",
	"Description" : "Sigma Persei (Sigma Per, \u03C3 Persei, \u03C3 Per) is an orange K-type giant with an apparent magnitude of +4.36. It is approximately 353 light years from Earth.\r\rSigma Persei is moving through the Galaxy at a speed of 17.4 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,400 and 43,600 light years from the center of the Galaxy. It came closest to the Sun 5.1 million years ago when it had brightened to magnitude 3.11 from a distance of 202 light years.\r\rThis star, together with \u03B4 Per, \u03C8 Per, \u03B1 Per, \u03B3 Per and \u03B7 Per, has been called the Segment of Perseus.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "35 Persei, Sigma Persei, HIP 16335, SAO 38890, HD 21552, GC 4158, HR 1052, DM BD+47   843, TYC 3316-2308-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Sigma Persei",
	"OType" : "Variable Star",
	"Distance" : "110.14",
	"RA_S" : 52.64368819,
	"DEC_S" : 47.99521392,
	"X" : 266,
	"Y" : 181,
	"Constellation" : "Perseus ",
	"AMag" : 4.492,
	"key" : 39540,
	"title" : "Sigma Persei"
	},
{
	"Index" : "19539",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 16470, SAO 38917, HD 21699, GC 4205, HR 1063, DM BD+47  847, TYC 3316-2307-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HD  21699",
	"OType" : "Rotationally variable Star",
	"Distance" : "186.23",
	"RA_S" : 53.03583725,
	"DEC_S" : 48.02347518,
	"Constellation" : "Perseus ",
	"AMag" : 5.444,
	"key" : 39539,
	"title" : "HD  21699"
	},
{
	"Index" : "19485",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "36 Persei, HIP 16499, SAO 38924, HD 21770, GC 4210, HR 1069, DM BD+45   778, TYC 3312-3022-1",
	"group" : { "key" : "Perseus" },
	"Common" : "36 Persei",
	"OType" : "Variable Star",
	"Distance" : "36.32",
	"RA_S" : 53.10941328,
	"DEC_S" : 46.05686053,
	"Constellation" : "Perseus ",
	"AMag" : 5.343,
	"key" : 39485,
	"title" : "36 Persei"
	},
{
	"Index" : "19557",
	"Description" : "Psi Persei (Psi Per, \u03C8 Persei, \u03C8 Per) is a Be star in the northern constellation of Perseus. It has an apparent visual magnitude of 4.31, so it is visible to the naked eye at night under suitably dark skies. Based on parallax measurements, it is located at a distance of roughly 580 light-years (180 parsecs) from the Earth.\r\rThis star has a stellar classification of B5Ve, which indicates it is a B-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. It is a shell star with a circumstellar disc of gas surrounding the equator and extending out to about 11 times the radius of the star. As a result of this disc, the spectrum of this star shows emission lines (as indicated by the \u0027e\u0027 in the stellar class) and its magnitude varies over a period of about a day.\r\rPsi Persei is rotating rapidly with a projected rotational velocity (v sin i) along the equator of 390 km/s or more. The axis of rotation is inclined about 75\u00B0 \u00B1 8\u00B0 to the line of sight from the Earth, so this velocity is close to the actual azimuthal velocity along the star\u0027s equator. It is expelling mass at the rate of about 5.0 \u00D7 10\u20138 times the mass of the Sun per year, or the equivalent of the Sun\u0027s mass every 20 million years. This star may be a member of the Alpha Persei Cluster, although its proper motion is high compared to other members.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "37 Persei, Psi Persei, HIP 16826, SAO 38980, HD 22192, GC 4287, HR 1087, DM BD+47   857, TYC 3317-3033-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Psi Persei",
	"OType" : "Be Star",
	"Distance" : "184.71",
	"RA_S" : 54.12240631,
	"DEC_S" : 48.19262969,
	"X" : 253,
	"Y" : 177,
	"Constellation" : "Perseus ",
	"AMag" : 4.295,
	"key" : 39557,
	"title" : "Psi Persei"
	},
{
	"Index" : "11190",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "40 Persei, o Persei, HIP 17313, SAO 56646, HD 22951, GC 4420, HR 1123, DM BD+33   698, TYC 2363-2185-1",
	"group" : { "key" : "Perseus" },
	"Common" : "o Persei",
	"OType" : "Star",
	"Distance" : "279.73",
	"RA_S" : 55.59435755,
	"DEC_S" : 33.96502764,
	"Constellation" : "Perseus ",
	"AMag" : 4.962,
	"key" : 31190,
	"title" : "o Persei"
	},
{
	"Index" : "19558",
	"Description" : "Delta Persei (Delta Per, \u03B4 Persei, \u03B4 Per) is a double star in the northern constellation of Perseus. It has an apparent visual magnitude of 3.01, making it readily visible with the naked eye. Parallax measurements give it a distance of about 520 light-years (160 parsecs) from the Earth.\r\rThe spectrum of this star matches a stellar classification of B5 III, which indicates it is a giant star that has evolved away from the main sequence after exhausting the hydrogen at its core. It has about seven times the Sun\u0027s mass and has an estimated age of 6.8 million years. The effective temperature of the outer envelope is 14,890 K, with the energy being emitted at this temperature giving it the blue-white hue that is a characteristic of a B-type star. It is rotating rapidly with a projected rotational velocity of 190 km s\u22121, which gives a lower bound for the actual azimuthal velocity along the star\u0027s equator.\r\rThis is most probably a binary star and may be a triple star system. It has an optical companion with an apparent magnitude of +6.17 at an angular separation of 0.330 arcseconds and a position angle of 221\u00B0, but it is uncertain whether this is an optical double star or a gravitationally bound companion. The star has also been categorized as a spectroscopic binary, indicating that it has an orbiting companion that has not been separately resolved with a telescope. Finally, this star may be a member of the Melotte 20 open cluster, which would make it the second brightest member after Mirfak.\r\rObservation with the IRAS shows an extended, ring-like feature that may be a bow wave driven by radiation pressure from the star, rather than a bubble being generated by the stellar wind. This feature has an angular size of 15 \u00D7 25 arcminutes and a peak temperature of 38 K. It has an estimated peculiar velocity of more than 30 km s\u22121, making it a runaway star.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "39 Persei, Delta Persei, HIP 17358AC, SAO 39053, HD 22928, GC 4427, HR 1122, DM BD+47   876, TYC 3317-3034-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Delta Persei",
	"OType" : "Be Star",
	"Distance" : "157.18",
	"RA_S" : 55.73126774,
	"DEC_S" : 47.78754851,
	"X" : 239,
	"Y" : 182,
	"Constellation" : "Perseus ",
	"AMag" : 2.963,
	"key" : 39558,
	"title" : "Delta Persei"
	},
{
	"Index" : "11156",
	"Description" : "Omicron Persei (\u03BF Per) is a star in the constellation Perseus. It has the traditional name Atik (also Ati, Al Atik, Arabic for \u0022the shoulder\u0022).\r\rAtik is a spectroscopic binary star consisting of a spectral type B1 giant and a type B3 dwarf orbiting each other every 4.5 days.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "38 Persei, Omicron Persei, HIP 17448A, SAO 56673, HD 23180, GC 4461, HR 1131, DM BD+31   642, TYC 2359-1258-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Atik",
	"OType" : "Star",
	"Distance" : "343.6426",
	"RA_S" : 56.07972678,
	"DEC_S" : 32.28824964,
	"X" : 222,
	"Y" : 382,
	"Constellation" : "Perseus ",
	"AMag" : 3.906,
	"key" : 31156,
	"shortTitle" : "Ati; Al Atik; Atiks; Atik",
	"title" : "Atik"
	},
{
	"Index" : "11157",
	"Description" : "Omicron Persei (\u03BF Per) is a star in the constellation Perseus. It has the traditional name Atik (also Ati, Al Atik, Arabic for \u0022the shoulder\u0022).\r\rAtik is a spectroscopic binary star consisting of a spectral type B1 giant and a type B3 dwarf orbiting each other every 4.5 days.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "38 Persei, Omicron Persei, HIP 17448B, SAO 56673, HD 23180, GC 4461, HR 1131, DM BD+31   642, TYC 2359-1258-2",
	"group" : { "key" : "Perseus" },
	"Common" : "Atik",
	"OType" : "Star",
	"Distance" : "343.6426",
	"RA_S" : 56.07972678,
	"DEC_S" : 32.28824964,
	"X" : 222,
	"Y" : 382,
	"Constellation" : "Perseus ",
	"AMag" : 6.696,
	"key" : 31157,
	"shortTitle" : "Ati; Al Atik; Atiks; Atik",
	"title" : "Atik"
	},
{
	"Index" : "15532",
	"Description" : "Nu Persei (\u03BD Per, \u03BD Persei) is a Class F5, fourth-magnitude star in the constellation Perseus. Nu Persei is a highly luminous yellow-white giant located about 555 light-years from Earth.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "41 Persei, Nu Persei, HIP 17529, SAO 39078, HD 23230, GC 4474, HR 1135, DM BD+42   815, TYC 2871-2573-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Nu Persei",
	"OType" : "Variable Star of RR Lyr type",
	"Distance" : "170.36",
	"RA_S" : 56.298463,
	"DEC_S" : 42.57855004,
	"X" : 229,
	"Y" : 249,
	"Constellation" : "Perseus ",
	"AMag" : 3.813,
	"key" : 35532,
	"title" : "Nu Persei"
	},
{
	"Index" : "11162",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "42 Persei, n Persei, HIP 17886, SAO 56727, HD 23848, GC 4592, HR 1177, DM BD+32   667, TYC 2360-1949-1",
	"group" : { "key" : "Perseus" },
	"Common" : "n Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "81.98",
	"RA_S" : 57.38620369,
	"DEC_S" : 33.09138818,
	"Constellation" : "Perseus ",
	"AMag" : 5.141,
	"key" : 31162,
	"title" : "n Persei"
	},
{
	"Index" : "11171",
	"Description" : "Zeta Persei (\u03B6 Per, \u03B6 Persei) is a star in the northern constellation of Perseus. With an apparent visual magnitude of 2.9, it can be readily seen with the naked eye. Parallax measurements place it at a distance of about 750 light-years (230 parsecs) from Earth.\r\rThis is a lower luminosity supergiant star with a stellar classification of B1 Ib. This is an enormous star, with an estimated 26\u201327 times the Sun\u0027s radius and 13\u201316 times the Sun\u0027s mass. It has about 47,000 times the luminosity of the Sun and it is radiating this energy at an effective temperature of 20,800 K, giving it the blue-white hue of a B-type star. The spectrum displays anomalously high levels of carbon. Zeta Persei has a strong stellar wind that is expelling 0.23 \u00D7 10\u20136 times the mass of the Sun per year, or the equivalent of the Sun\u0027s mass every 4.3 million years.\r\rZeta Persei has a 9th magnitude companion at an angular separation of 12.9 arcseconds. The two stars have the same proper motion, so they may be physically associated. If so, they are separated by at least 4,000 Astronomical Units. Zeta Persei is a confirmed member of the Perseus OB2 association (Per OB2), also called the Zeta Persei association, which is a moving group of stars that includes 17 massive, high luminosity members with spectral types of O or B, giving them a blue hue. These stars have a similar trajectory through space, suggesting they originated in the same molecular cloud and are about the same age.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "44 Persei, Zeta Persei, HIP 18246, SAO 56799, HD 24398, GC 4688, HR 1203, DM BD+31   666, TYC 2361-2820-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Zeta Persei",
	"OType" : "Variable Star",
	"Distance" : "269.14",
	"RA_S" : 58.53300785,
	"DEC_S" : 31.88363844,
	"X" : 195,
	"Y" : 386,
	"Constellation" : "Perseus ",
	"AMag" : 2.858,
	"key" : 31171,
	"shortTitle" : "Menkhib (also HD24912)",
	"title" : "Zeta Persei"
	},
{
	"Index" : "19670",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 18396, SAO 39195, HD 24504, GC 4721, HR 1207, DM BD+47  912, TYC 3330-3020-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 1207",
	"OType" : "Star",
	"Distance" : "195.38",
	"RA_S" : 58.99239324,
	"DEC_S" : 47.8714155,
	"Constellation" : "Perseus ",
	"AMag" : 5.366,
	"key" : 39670,
	"title" : "HR 1207"
	},
{
	"Index" : "11199",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 18434, SAO 56824, HD 24640, GC 4734, HR 1215, DM BD+34  768, TYC 2365-1420-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 1215",
	"OType" : "Cepheid variable Star",
	"Distance" : "273.02",
	"RA_S" : 59.11953951,
	"DEC_S" : 35.08090238,
	"Constellation" : "Perseus ",
	"AMag" : 5.478,
	"key" : 31199,
	"title" : "HR 1215"
	},
{
	"Index" : "19738",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "43 Persei, A Persei, HIP 18453, SAO 24314, HD 24546, GC 4728, HR 1210, DM BD+50   860, TYC 3339-1703-1",
	"group" : { "key" : "Perseus" },
	"Common" : "A Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "40.74",
	"RA_S" : 59.1521725,
	"DEC_S" : 50.69537389,
	"Constellation" : "Perseus ",
	"AMag" : 5.32,
	"key" : 39738,
	"title" : "A Persei"
	},
{
	"Index" : "15505",
	"Description" : "Epsilon Persei (\u03B5 Persei, \u03B5 Per) is a multiple star system in the northern constellation of Perseus. It has a combined apparent visual magnitude of +2.88, which is bright enough to be viewed with the naked eye. Based upon parallax measurements, this system is located at a distance of roughly 640 light-years (196 parsecs) from Earth.\r\rThis is a spectroscopic binary system, which means that the presence of an orbiting companion has been revealed by radial velocity variations in the spectrum of the primary. The two components are orbiting each other with a period of 14 days at a high orbital eccentricity of 0.55. The secondary component has about 6\u201313% of the primary\u0027s mass and may have a stellar classification in the range from A6 V to K1 V. There may be a third component to this system with an orbital period of roughly 9,428 days (25.8 years), although this has not been conclusively demonstrated. If this component exists, it would have about 51\u2013139% of the primary\u0027s mass. This high level of uncertainty is because the inclination of the orbit is not known.\r\rThe primary component of this system, Epsilon Persei A, is a massive star with 12\u201316 times the Sun\u0027s mass and near eight times the radius of the Sun. It has a stellar classification of B0.5 V, making it a B-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. Component A is radiating over 28,000 times the Sun\u0027s luminosity from its outer envelope at an effective temperature of 26,500 K. This gives the star the blue-white hue that is typical of B-type stars.\r\rEpsilon Persei A is a Beta Cephei variable star with a primary pulsation period of 0.1603 days, or 6.24 cycles per day. It may have multiple pulsation frequencies.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "45 Persei, Epsilon Persei, HIP 18532, SAO 56840, HD 24760, GC 4759, HR 1220, DM BD+39   895, TYC 2868-1623-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Epsilon Persei",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "195.22",
	"RA_S" : 59.46346687,
	"DEC_S" : 40.01021532,
	"X" : 195,
	"Y" : 280,
	"Constellation" : "Perseus ",
	"AMag" : 2.854,
	"key" : 35505,
	"title" : "Epsilon Persei"
	},
{
	"Index" : "11213",
	"Description" : "Xi Persei (\u03BE Per) is a star in the constellation Perseus. It has the traditional name Menkib (Menchib, Menkhib, Al Mankib from Mankib al Thurayya (Arabic for \u0022shoulder\u0022 [of the Pleiades]). Menkib has an apparent magnitude of +4.06 and is classified as a blue giant (spectral class O7.5III). It is approximately 1800 light years from Earth.\r\rIt is visually 12,700 times brighter than the Sun with absolute magnitude -5.5. If we include the ultraviolet light that emanates from Menkib its total, bolometric, luminosity is 263,000 times that of the Sun.\r\rThe star has a mass of some 30 solar masses and a surface temperature of 35,000 kelvins, making it one of the hottest stars that can be seen with the naked eye.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "46 Persei, Xi Persei, HIP 18614, SAO 56856, HD 24912, GC 4779, HR 1228, DM BD+35   775, TYC 2369-2273-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Menkib",
	"OType" : "Double or multiple star",
	"Distance" : "365.08",
	"RA_S" : 59.74125101,
	"DEC_S" : 35.79103224,
	"X" : 186,
	"Y" : 334,
	"Constellation" : "Perseus ",
	"AMag" : 4.026,
	"key" : 31213,
	"shortTitle" : "Menkhib (also HD24398); Menchib",
	"title" : "Menkib"
	},
{
	"Index" : "19706",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "47 Persei, Lambda Persei, HIP 19167, SAO 24412, HD 25642, GC 4924, HR 1261, DM BD+49  1101, TYC 3335-2097-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Lambda Persei",
	"OType" : "Star",
	"Distance" : "129.24",
	"RA_S" : 61.6459775,
	"DEC_S" : 50.35123808,
	"Constellation" : "Perseus ",
	"AMag" : 4.263,
	"key" : 39706,
	"title" : "Lambda Persei"
	},
{
	"Index" : "19690",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "48 Persei, c Persei, HIP 19343, SAO 39336, HD 25940, GC 4967, HR 1273, DM BD+47   939, TYC 3332-2427-1",
	"group" : { "key" : "Perseus" },
	"Common" : "c Persei",
	"OType" : "Be Star",
	"Distance" : "146.1",
	"RA_S" : 62.165384,
	"DEC_S" : 47.71251193,
	"Constellation" : "Perseus ",
	"AMag" : 3.982,
	"key" : 39690,
	"title" : "c Persei"
	},
{
	"Index" : "15616",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "52 Persei, f Persei, HIP 19811, SAO 39409, HD 26673, GC 5103, HR 1306, DM BD+40   912A, TYC 2882-2046-1",
	"group" : { "key" : "Perseus" },
	"Common" : "f Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "291.5452",
	"RA_S" : 63.72214846,
	"DEC_S" : 40.48365426,
	"Constellation" : "Perseus ",
	"AMag" : 4.797,
	"key" : 35616,
	"title" : "f Persei"
	},
{
	"Index" : "19689",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "51 Persei, Mu Persei, HIP 19812, SAO 39404, HD 26630, GC 5099, HR 1303, DM BD+48  1063, TYC 3332-2426-1",
	"group" : { "key" : "Perseus" },
	"Common" : "Mu Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "275.23",
	"RA_S" : 63.72442609,
	"DEC_S" : 48.4093281,
	"Constellation" : "Perseus ",
	"AMag" : 4.238,
	"key" : 39689,
	"title" : "Mu Persei"
	},
{
	"Index" : "19711",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "b Persei, HIP 20070, SAO 24531, HD 26961, GC 5174, HR 1324, DM BD+49  1150, TYC 3336-2435-1",
	"group" : { "key" : "Perseus" },
	"Common" : "b Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "96.02",
	"RA_S" : 64.56090705,
	"DEC_S" : 50.29549581,
	"Constellation" : "Perseus ",
	"AMag" : 4.6,
	"key" : 39711,
	"title" : "b Persei"
	},
{
	"Index" : "19718",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 20156, SAO 39457, HD 27084, GC 5191, HR 1330, DM BD+49 1155, TYC 3337-195-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 1330",
	"OType" : "Star in Cluster",
	"Distance" : "74.39",
	"RA_S" : 64.80515814,
	"DEC_S" : 50.04869045,
	"Constellation" : "Perseus ",
	"AMag" : 5.483,
	"key" : 39718,
	"title" : "HR 1330"
	},
{
	"Index" : "11254",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "54 Persei, HIP 20252, SAO 57171, HD 27348, GC 5235, HR 1343, DM BD+34   860, TYC 2379-2589-1",
	"group" : { "key" : "Perseus" },
	"Common" : "54 Persei",
	"OType" : "Star",
	"Distance" : "66.91",
	"RA_S" : 65.10266258,
	"DEC_S" : 34.56672423,
	"Constellation" : "Perseus ",
	"AMag" : 5.033,
	"key" : 31254,
	"title" : "54 Persei"
	},
{
	"Index" : "19662",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "53 Persei, d Persei, HIP 20354, SAO 39483, HD 27396, GC 5256, HR 1350, DM BD+46   872, TYC 3329-2516-1",
	"group" : { "key" : "Perseus" },
	"Common" : "d Persei",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "155.17",
	"RA_S" : 65.38819181,
	"DEC_S" : 46.4988827,
	"Constellation" : "Perseus ",
	"AMag" : 4.803,
	"key" : 39662,
	"title" : "d Persei"
	},
{
	"Index" : "11232",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "HIP 20704, SAO 57229, HD 27971, GC 5359, HR 1390, DM BD+31  776, TYC 2372-2099-1",
	"group" : { "key" : "Perseus" },
	"Common" : "HR 1390",
	"OType" : "Star",
	"Distance" : "77.58",
	"RA_S" : 66.52628957,
	"DEC_S" : 31.43891786,
	"Constellation" : "Perseus ",
	"AMag" : 5.393,
	"key" : 31232,
	"title" : "HR 1390"
	},
{
	"Index" : "15672",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "58 Persei, e Persei, HIP 21476, SAO 39639, HD 29094, GC 5609, HR 1454, DM BD+40  1000A, TYC 2888-2054-1",
	"group" : { "key" : "Perseus" },
	"Common" : "e Persei",
	"OType" : "Spectroscopic binary",
	"Distance" : "241.99",
	"RA_S" : 69.17262533,
	"DEC_S" : 41.26481622,
	"Constellation" : "Perseus ",
	"AMag" : 4.374,
	"key" : 35672,
	"title" : "e Persei"
	},
{
	"Index" : "15815",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "59 Persei, HIP 21928, SAO 39699, HD 29722, GC 5719, HR 1494, DM BD+43  1043, TYC 2905-1947-1",
	"group" : { "key" : "Perseus" },
	"Common" : "59 Persei",
	"OType" : "Star",
	"Distance" : "72.92",
	"RA_S" : 70.72637691,
	"DEC_S" : 43.36513597,
	"Constellation" : "Perseus ",
	"AMag" : 5.3,
	"key" : 35815,
	"title" : "59 Persei"
	},
{
	"Index" : "11391",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "1 Aurigae, HIP 22453, SAO 57447, HD 30504, GC 5868, HR 1533, DM BD+37   969, TYC 2399-1844-1",
	"group" : { "key" : "Perseus" },
	"Common" : "1 Aurigae",
	"OType" : "Star",
	"Distance" : "153.47",
	"RA_S" : 72.47765716,
	"DEC_S" : 37.48827429,
	"Constellation" : "Perseus ",
	"AMag" : 5.036,
	"key" : 31391,
	"title" : "1 Aurigae"
	},
{
	"Index" : "57382",
	"Description" : "Epsilon Phoenicis (\u03B5 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 3.88.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Epsilon Phoenicis, HIP 765, SAO 214983, HD 496, GC 158, HR 25, DM CD-46    18, TYC 8022-1240-1",
	"group" : { "backgroundImage" : "images/Alignment/36.png",
		"description" : "Phoenix is a minor constellation in the southern sky. It is named after the Phoenix, a mythical bird. The constellation stretches from roughly \u221239\u00B0 to \u221257\u00B0 declination, and from 23.5h to 2.5h of right ascension. The brightest star, Alpha Phoenicis is named Ankaa, an Arabic word meaning \u0027the Phoenix\u0027. It is an orange giant of apparent magnitude 2.4. Next is Beta Phoenicis, actually a binary system composed of two yellow giants with a combined apparent magnitude of 3.3. The constellation boasts several stars with planets, and the recently discovered Phoenix galaxy cluster \u2013 one of the largest objects in the universe.\r\rPhoenix is a small constellation bordered by Fornax and Sculptor to the north, Grus to the west, Tucana to the south, touching on the corner of Hydrus to the south, and Eridanus to the southeast. The bright star Achernar is nearby. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027Phe\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 10 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 23h 26.5m and 02h 25.0m, while the declination coordinates are between \u221239.31\u00B0 and \u221257.84\u00B0. This means it is generally invisible to anyone living north of the 40th parallel in the Northern Hemisphere, and remains low in the sky for anyone living north of the equator. It is easily visible from locations such as Australia and South Africa during Southern Hemisphere summer.\r\rPhoenix was the largest of the twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rThe same group of stars was imagined by the Arabs as a boat, Al Zaurak, on the nearby river Eridanus. It was also seen to represent Young Ostriches Al Ri\u0027\u0101l, or as a griffin or eagle. Phoenix and the neighbouring constellation of Grus together were seen to portray Aaron the High Priest by Julius Schiller.",
		"key" : "Phoenix",
		"grouptype" : "Phoenix",
		"Meaning" : "phoenix",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Phoenix",
		"title" : "Phoenix Objects Group" },
	"Common" : "Epsilon Phoenicis",
	"OType" : "High proper-motion Star",
	"Distance" : "44.19",
	"RA_S" : 2.35265739,
	"DEC_S" : -45.74742469,
	"X" : 405,
	"Y" : 422,
	"Constellation" : "Phoenix ",
	"AMag" : 3.99,
	"key" : 77382,
	"title" : "Epsilon Phoenicis"
	},
{
	"Index" : "53055",
	"Description" : "Kappa Phoenicis (\u03BA Phe) is a star in the constellation Phoenix. Its apparent magnitude is 3.90.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Kappa Phoenicis, HIP 2072, SAO 215092, HD 2262, GC 516, HR 100, DM CD-44   101, TYC 7530-978-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Kappa Phoenicis",
	"OType" : "Star",
	"Distance" : "23.81",
	"RA_S" : 6.55084105,
	"DEC_S" : -43.67983206,
	"X" : 369,
	"Y" : 391,
	"Constellation" : "Phoenix ",
	"AMag" : 3.953,
	"key" : 73055,
	"title" : "Kappa Phoenicis"
	},
{
	"Index" : "57416",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Lambda01 Phoenicis, HIP 2472, SAO 215131, HD 2834, GC 619, HR 125, DM CD-49   115, TYC 8027-1305-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Lambda01 Phoenicis",
	"OType" : "High proper-motion Star",
	"Distance" : "52.96",
	"RA_S" : 7.85408789,
	"DEC_S" : -48.8035133,
	"Constellation" : "Phoenix ",
	"AMag" : 4.755,
	"key" : 77416,
	"title" : "Lambda01 Phoenicis"
	},
{
	"Index" : "57393",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Mu Phoenicis, HIP 3245, SAO 215194, HD 3919, GC 823, HR 180, DM CD-46   180, TYC 8024-1169-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Mu Phoenicis",
	"OType" : "Star",
	"Distance" : "75.33",
	"RA_S" : 10.3314842,
	"DEC_S" : -46.08500948,
	"Constellation" : "Phoenix ",
	"AMag" : 4.706,
	"key" : 77393,
	"title" : "Mu Phoenicis"
	},
{
	"Index" : "61557",
	"Description" : "Eta Phoenicis (\u03B7 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 4.37.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Eta Phoenicis, HIP 3405, SAO 232162, HD 4150, GC 866, HR 191, DM CP-58    42, TYC 8469-1596-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Eta Phoenicis",
	"OType" : "Star",
	"Distance" : "75.47",
	"RA_S" : 10.83849872,
	"DEC_S" : -57.46306909,
	"X" : 322,
	"Y" : 567,
	"Constellation" : "Phoenix ",
	"AMag" : 4.359,
	"key" : 81557,
	"title" : "Eta Phoenicis"
	},
{
	"Index" : "57484",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Rho Phoenicis, HIP 3949, SAO 232203, HD 4919, GC 1019, HR 242, DM CD-51   209, TYC 8037-1153-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Rho Phoenicis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "74.22",
	"RA_S" : 12.6716104,
	"DEC_S" : -50.98681445,
	"Constellation" : "Phoenix ",
	"AMag" : 5.269,
	"key" : 77484,
	"title" : "Rho Phoenicis"
	},
{
	"Index" : "57447",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "HIP 4890, SAO 215343, HD 6245, GC 1266, HR 299, DM CD-47  313, TYC 8032-1071-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "HR 299",
	"OType" : "Star",
	"Distance" : "73.07",
	"RA_S" : 15.70495372,
	"DEC_S" : -46.39731193,
	"Constellation" : "Phoenix ",
	"AMag" : 5.487,
	"key" : 77447,
	"title" : "HR 299"
	},
{
	"Index" : "57451",
	"Description" : "Beta Phoenicis (\u03B2 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 3.32.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Beta Phoenicis, HIP 5165, SAO 215365, HD 6595A, GC 1335, HR 322, DM CD-47   324, TYC 8032-1228-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Beta Phoenicis",
	"OType" : "Star",
	"RA_S" : 16.5211354,
	"DEC_S" : -46.71845453,
	"X" : 277,
	"Y" : 427,
	"Constellation" : "Phoenix ",
	"AMag" : 3.459,
	"key" : 77451,
	"title" : "Beta Phoenicis"
	},
{
	"Index" : "53103",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Upsilon Phoenicis, HIP 5300AB, SAO 215374, HD 6767, GC 1378, HR 331, DM CD-42   391, TYC 7537-994-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Upsilon Phoenicis",
	"OType" : "Double or multiple star",
	"Distance" : "60.58",
	"RA_S" : 16.94938081,
	"DEC_S" : -41.48689922,
	"Constellation" : "Phoenix ",
	"AMag" : 5.228,
	"key" : 73103,
	"title" : "Upsilon Phoenicis"
	},
{
	"Index" : "61601",
	"Description" : "Zeta Phoenicis (\u03B6 Phe, \u03B6 Phoenicis) is a 280 light-year distant star in the constellation Phoenix. It is an Algol-type eclipsing binary star and its apparent magnitude fluctuates between 3.9 and 4.4 with a period of 1.66977 days. Zeta Phoenicis is a four-star system: it has two other telescopic components with an apparent magnitude of 7.2 and 8.2 at a distance of 0.8 and 6.4 arcseconds from the main star.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Zeta Phoenicis, HIP 5348C, SAO 232306, HD 6882C, GC 1387, HR 338, DM CP-55   241, TYC 8476-1304-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Zeta Phoenicis",
	"OType" : "High proper-motion Star",
	"Distance" : "91.44",
	"RA_S" : 17.09335,
	"DEC_S" : -55.246642,
	"X" : 277,
	"Y" : 538,
	"Constellation" : "Phoenix ",
	"AMag" : 8.233,
	"key" : 81601,
	"title" : "Zeta Phoenicis"
	},
{
	"Index" : "61600",
	"Description" : "Zeta Phoenicis (\u03B6 Phe, \u03B6 Phoenicis) is a 280 light-year distant star in the constellation Phoenix. It is an Algol-type eclipsing binary star and its apparent magnitude fluctuates between 3.9 and 4.4 with a period of 1.66977 days. Zeta Phoenicis is a four-star system: it has two other telescopic components with an apparent magnitude of 7.2 and 8.2 at a distance of 0.8 and 6.4 arcseconds from the main star.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Zeta Phoenicis, HIP 5348AB, SAO 232306, HD 6882, GC 1387, HR 338, DM CP-55   241, TYC 8476-1302-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Zeta Phoenicis",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "91.44",
	"RA_S" : 17.09619765,
	"DEC_S" : -55.24575773,
	"X" : 277,
	"Y" : 538,
	"Constellation" : "Phoenix ",
	"AMag" : 3.997,
	"key" : 81600,
	"title" : "Zeta Phoenicis"
	},
{
	"Index" : "57456",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Nu Phoenicis, HIP 5862, SAO 215428, HD 7570, GC 1510, HR 370, DM CD-46   346, TYC 8033-1232-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Nu Phoenicis",
	"OType" : "High proper-motion Star",
	"Distance" : "15.11",
	"RA_S" : 18.79633866,
	"DEC_S" : -45.53166556,
	"Constellation" : "Phoenix ",
	"AMag" : 5.023,
	"key" : 77456,
	"title" : "Nu Phoenicis"
	},
{
	"Index" : "53176",
	"Description" : "Gamma Phoenicis (\u03B3 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 3.41.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Gamma Phoenicis, HIP 6867, SAO 215516, HD 9053, GC 1787, HR 429, DM CD-43   449, TYC 7547-1134-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Gamma Phoenicis",
	"OType" : "Spectroscopic binary",
	"Distance" : "71.58",
	"RA_S" : 22.0913625,
	"DEC_S" : -43.31823589,
	"X" : 223,
	"Y" : 387,
	"Constellation" : "Phoenix ",
	"AMag" : 3.613,
	"key" : 73176,
	"title" : "Gamma Phoenicis"
	},
{
	"Index" : "57531",
	"Description" : "Delta Phoenicis (\u03B4 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 3.95.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Delta Phoenicis, HIP 7083, SAO 215536, HD 9362, GC 1847, HR 440, DM CD-49   425, TYC 8043-1179-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Delta Phoenicis",
	"OType" : "High proper-motion Star",
	"Distance" : "43.57",
	"RA_S" : 22.81293687,
	"DEC_S" : -49.07270501,
	"X" : 225,
	"Y" : 462,
	"Constellation" : "Phoenix ",
	"AMag" : 4.044,
	"key" : 77531,
	"title" : "Delta Phoenicis"
	},
{
	"Index" : "57511",
	"Description" : "Psi Phoenicis (\u03C8 Phe) is a star in the constellation Phoenix. Its apparent magnitude is 4.44.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Psi Phoenicis, HIP 8837, SAO 215696, HD 11695, GC 2303, HR 555, DM CD-46   552, TYC 8041-1199-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Psi Phoenicis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "104.77",
	"RA_S" : 28.41142963,
	"DEC_S" : -46.30266629,
	"X" : 171,
	"Y" : 434,
	"Constellation" : "Phoenix ",
	"AMag" : 4.598,
	"key" : 77511,
	"title" : "Psi Phoenicis"
	},
{
	"Index" : "53171",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Phi Phoenicis, HIP 8882, SAO 215697, HD 11753, GC 2315, HR 558, DM CD-43   583, TYC 7546-1195-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Phi Phoenicis",
	"OType" : "Spectroscopic binary",
	"Distance" : "93.94",
	"RA_S" : 28.59180729,
	"DEC_S" : -42.49694548,
	"Constellation" : "Phoenix ",
	"AMag" : 5.1,
	"key" : 73171,
	"title" : "Phi Phoenicis"
	},
{
	"Index" : "57512",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "HIP 9095, SAO 215715, HD 12055, GC 2369, HR 574, DM CD-47  597, TYC 8041-1200-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "HR 574",
	"OType" : "Star",
	"Distance" : "75.82",
	"RA_S" : 29.29201027,
	"DEC_S" : -47.38528101,
	"Constellation" : "Phoenix ",
	"AMag" : 4.93,
	"key" : 77512,
	"title" : "HR 574"
	},
{
	"Index" : "53240",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Chi Phoenicis, HIP 9459, SAO 215739, HD 12524, GC 2455, HR 602, DM CD-45   659, TYC 7556-1058-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Chi Phoenicis",
	"OType" : "Star",
	"Distance" : "114.92",
	"RA_S" : 30.42656568,
	"DEC_S" : -44.71350768,
	"Constellation" : "Phoenix ",
	"AMag" : 5.313,
	"key" : 73240,
	"title" : "Chi Phoenicis"
	},
{
	"Index" : "57376",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Iota Phoenicis, HIP 116389, SAO 231675, HD 221760, GC 32787, HR 8949, DM CD-43 15420, TYC 8020-969-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Iota Phoenicis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "76.13",
	"RA_S" : 353.76902011,
	"DEC_S" : -42.61508989,
	"Constellation" : "Phoenix ",
	"AMag" : 4.705,
	"key" : 77376,
	"title" : "Iota Phoenicis"
	},
{
	"Index" : "61465",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "HIP 116602, SAO 231707, HD 222095, GC 32836, HR 8959, DM CD-4614720, TYC 8456-967-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "HR 8959",
	"OType" : "Star",
	"Distance" : "61.37",
	"RA_S" : 354.46247574,
	"DEC_S" : -45.49234598,
	"Constellation" : "Phoenix ",
	"AMag" : 4.736,
	"key" : 81465,
	"title" : "HR 8959"
	},
{
	"Index" : "61502",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Sigma Phoenicis, HIP 117315, SAO 248018, HD 223145, GC 33012, HR 9006, DM CD-50 14047, TYC 8463-1212-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Sigma Phoenicis",
	"OType" : "Star",
	"Distance" : "184.71",
	"RA_S" : 356.81665044,
	"DEC_S" : -50.2264582,
	"Constellation" : "Phoenix ",
	"AMag" : 5.139,
	"key" : 81502,
	"title" : "Sigma Phoenicis"
	},
{
	"Index" : "65228",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Pi Phoenicis, HIP 118234, SAO 248087, HD 224554, GC 33256, HR 9069, DM CP-53 10561, TYC 8833-221-1",
	"group" : { "key" : "Phoenix" },
	"Common" : "Pi Phoenicis",
	"OType" : "Star",
	"Distance" : "88.02",
	"RA_S" : 359.7324063,
	"DEC_S" : -52.74580552,
	"Constellation" : "Phoenix ",
	"AMag" : 5.258,
	"key" : 85228,
	"title" : "Pi Phoenicis"
	},
{
	"Index" : "57842",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Lambda Pictoris, HIP 21914, SAO 233638, HD 30185, GC 5764, HR 1516, DM CD-50  1471, TYC 8082-1842-1",
	"group" : { "backgroundImage" : "images/Alignment/23.png",
		"description" : "Pictor is a small and faint constellation in the southern sky (declination \u221250\u00B0 to \u221260\u00B0), located between the brilliant star Canopus and the Large Magellanic Cloud. Its name is Latin for painter, but it is in fact an abbreviation of its original name Equuleus Pictoris, the \u0027painter\u0027s easel\u0027, and it is normally represented as an easel. It was invented and named by Abb\u00E9 Nicolas Louis de Lacaille in the 18th century.\r\rPictor has attracted attention in recent years because of its second-brightest star Beta Pictoris, 63.4 light-years distant, which is surrounded by an unusual dust disk rich in carbon, as well as an extrasolar planet. Another four stars have been found to have extrasolar planets. The constellation also hosts RR Pictoris, a nova which brightened to magnitude 1.2 in 1925.\r\rThe French astronomer Nicolas Louis de Lacaille first described the constellation as le Chevalet et la Palette (the easel and palette) in 1756, and gave Bayer designations to ten stars now named Alpha to Nu Pictoris (he erred in naming the wrong star with the Greek letter epsilon, which is now not used). He labelled it Equuleus Pictorius on his 1763 chart. Johann Bode called it Pluteum Pictoris. The name was shortened to Pictor in 1845 by Francis Baily on the suggestion of Sir John Herschel.\r\rPictor is a small constellation bordered by Columba to the north, Puppis and Carina to the east, Caelum to the northwest, Dorado to the southwest and Volans to the south. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027Pic\u0027.\r\rThe official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 18 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 04h 32.5m and 06h 52.0m, while the declination coordinates are between \u221242.79\u00B0 and \u221264.15\u00B0. Pictor culminates each year at 9 p.m. on 17 March.",
		"key" : "Pictor",
		"grouptype" : "Pictor",
		"Meaning" : "easel",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Pictor",
		"title" : "Pictor Objects Group" },
	"Common" : "Lambda Pictoris",
	"OType" : "Star",
	"Distance" : "114.75",
	"RA_S" : 70.69343051,
	"DEC_S" : -50.48133339,
	"Constellation" : "Pictor ",
	"AMag" : 5.406,
	"key" : 77842,
	"title" : "Lambda Pictoris"
	},
{
	"Index" : "57827",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Eta01 Pictoris, HIP 23482, SAO 217140, HD 32743, GC 6185, HR 1649, DM CD-49  1541, TYC 8081-1280-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Eta01 Pictoris",
	"OType" : "Star",
	"Distance" : "26.07",
	"RA_S" : 75.7028598,
	"DEC_S" : -49.15140577,
	"Constellation" : "Pictor ",
	"AMag" : 5.422,
	"key" : 77827,
	"title" : "Eta01 Pictoris"
	},
{
	"Index" : "57826",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Eta02 Pictoris, HIP 23649, SAO 217164, HD 33042, GC 6234, HR 1663, DM CD-49  1562, TYC 8081-1231-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Eta02 Pictoris",
	"OType" : "Variable Star",
	"Distance" : "135.97",
	"RA_S" : 76.24172278,
	"DEC_S" : -49.577836,
	"Constellation" : "Pictor ",
	"AMag" : 5.221,
	"key" : 77826,
	"title" : "Eta02 Pictoris"
	},
{
	"Index" : "57928",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Zeta Pictoris, HIP 24829, SAO 233926, HD 35072, GC 6553, HR 1767, DM CD-50  1723, TYC 8093-1067-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Zeta Pictoris",
	"OType" : "High proper-motion Star",
	"Distance" : "35.71",
	"RA_S" : 79.84222882,
	"DEC_S" : -50.60596688,
	"Constellation" : "Pictor ",
	"AMag" : 5.495,
	"key" : 77928,
	"title" : "Zeta Pictoris"
	},
{
	"Index" : "57878",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 27243, SAO 217521, HD 38871, GC 7257, HR 2008, DM CD-46 1999, TYC 8087-1675-1",
	"group" : { "key" : "Pictor" },
	"Common" : "HR 2008",
	"OType" : "Red Giant Branch star",
	"Distance" : "143.76",
	"RA_S" : 86.61405472,
	"DEC_S" : -46.59717925,
	"Constellation" : "Pictor ",
	"AMag" : 5.418,
	"key" : 77878,
	"title" : "HR 2008"
	},
{
	"Index" : "57966",
	"Description" : "Beta Pictoris (\u03B2 Pic, \u03B2 Pictoris) is the second brightest star in the constellation Pictor. It is located 63.4 light years from our solar system, and is 1.75 times as massive and 8.7 times as luminous as the Sun. The Beta Pictoris system is very young, only 8\u201320 million years old, although it is already in the main sequence stage of its evolution. Beta Pictoris is the title member of the Beta Pictoris moving group, an association of young stars which share the same motion through space and have the same age.\r\rBeta Pictoris shows an excess of infrared emission compared to normal stars of its type, which is caused by large quantities of dust near the star. Detailed observations reveal a large disk of dust and gas orbiting the star, which was the first debris disk to be imaged around another star. In addition to the presence of several planetesimal belts and cometary activity, there are indications that planets have formed within this disk and that the processes of planet formation may still be ongoing. Material from the Beta Pictoris debris disk is thought to be the dominant source of interstellar meteoroids in our solar system.\r\rThe European Southern Observatory (ESO) has confirmed the presence of a planet, matching previous predictions, through the use of direct imagery, orbiting in the plane of the debris disk surrounding the star. This planet is currently the closest extrasolar planet to its star ever photographed: the observed separation is roughly the same as the distance between Saturn and the Sun.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Beta Pictoris, HIP 27321, SAO 234134, HD 39060, GC 7287, HR 2020, DM CD-51  1620, TYC 8099-1392-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Beta Pictoris",
	"OType" : "Star",
	"Distance" : "19.44",
	"RA_S" : 86.82119562,
	"DEC_S" : -51.06651205,
	"X" : 213,
	"Y" : 267,
	"Constellation" : "Pictor ",
	"AMag" : 3.87,
	"key" : 77966,
	"title" : "Beta Pictoris"
	},
{
	"Index" : "62014",
	"Description" : "Gamma Pictoris (\u03B3 Pic) is a star in the constellation Pictor. Its apparent magnitude is 4.50.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Gamma Pictoris, HIP 27530, SAO 234154, HD 39523, GC 7353, HR 2042, DM CP-56   946, TYC 8524-1280-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Gamma Pictoris",
	"OType" : "Star",
	"Distance" : "54.2",
	"RA_S" : 87.45692541,
	"DEC_S" : -56.16666692,
	"X" : 220,
	"Y" : 334,
	"Constellation" : "Pictor ",
	"AMag" : 4.616,
	"key" : 82014,
	"title" : "Gamma Pictoris"
	},
{
	"Index" : "57971",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 27621, SAO 234169, HD 39640, GC 7377, HR 2049, DM CP-52  794, TYC 8100-1465-1",
	"group" : { "key" : "Pictor" },
	"Common" : "HR 2049",
	"OType" : "Star",
	"Distance" : "78.6",
	"RA_S" : 87.7217543,
	"DEC_S" : -52.10887334,
	"Constellation" : "Pictor ",
	"AMag" : 5.274,
	"key" : 77971,
	"title" : "HR 2049"
	},
{
	"Index" : "61987",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 27947, SAO 234199, HD 40292, GC 7479, HR 2094, DM CP-52  805, TYC 8520-704-1",
	"group" : { "key" : "Pictor" },
	"Common" : "HD  40292",
	"OType" : "High proper-motion Star",
	"Distance" : "34.7",
	"RA_S" : 88.70871703,
	"DEC_S" : -52.63548125,
	"Constellation" : "Pictor ",
	"AMag" : 5.316,
	"key" : 81987,
	"title" : "HD  40292"
	},
{
	"Index" : "65768",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "HIP 28991, SAO 249451, HD 42540, GC 7825, HR 2196, DM CP-62  582, TYC 8897-788-1",
	"group" : { "key" : "Pictor" },
	"Common" : "HR 2196",
	"OType" : "Variable Star",
	"Distance" : "110.82",
	"RA_S" : 91.7641167,
	"DEC_S" : -62.15458046,
	"Constellation" : "Pictor ",
	"AMag" : 5.182,
	"key" : 85768,
	"title" : "HR 2196"
	},
{
	"Index" : "62021",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Delta Pictoris, HIP 29276, SAO 234359, HD 42933, GC 7898, HR 2212, DM CP-54   980, TYC 8525-1313-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Delta Pictoris",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "396.71",
	"RA_S" : 92.5746196,
	"DEC_S" : -54.96864591,
	"Constellation" : "Pictor ",
	"AMag" : 4.685,
	"key" : 82021,
	"title" : "Delta Pictoris"
	},
{
	"Index" : "62142",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "61 Pictoris, HIP 30932, SAO 234541, HD 46355, GC 8459, HR 2389, DM CP-56  1095, TYC 8543-1756-1",
	"group" : { "key" : "Pictor" },
	"Common" : "61 Pictoris",
	"OType" : "Variable Star",
	"Distance" : "93.23",
	"RA_S" : 97.36874772,
	"DEC_S" : -56.85276884,
	"Constellation" : "Pictor ",
	"AMag" : 5.318,
	"key" : 82142,
	"title" : "61 Pictoris"
	},
{
	"Index" : "65778",
	"Description" : "Alpha Pictoris (\u03B1 Pic, \u03B1 Pictoris) is the brightest star in the southern constellation of Pictor. It has an apparent visual magnitude of 3.27, which is bright enough to be viewed from urban areas in the southern hemisphere. This star is close enough for its distance to be measured using parallax shifts, which yields a value of roughly 97 light-years (30 parsecs) from the Sun, with a 5% margin of error. Alpha Pictoris has the distinction of being the south pole star of the planet Mercury.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Alpha Pictoris, HIP 32607, SAO 249647, HD 50241, GC 8941, HR 2550, DM CP-61   720, TYC 8899-2202-1",
	"group" : { "key" : "Pictor" },
	"Common" : "Alpha Pictoris",
	"OType" : "High proper-motion Star",
	"Distance" : "29.51",
	"RA_S" : 102.04772601,
	"DEC_S" : -61.94132165,
	"X" : 149,
	"Y" : 434,
	"Constellation" : "Pictor ",
	"AMag" : 3.262,
	"key" : 85778,
	"title" : "Alpha Pictoris"
	},
{
	"Index" : "30942",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "29 Piscium, HIP 145, SAO 147041, HD 224926, GC 33327, HR 9087, DM BD-03  5749, TYC 4666-935-1",
	"group" : { "backgroundImage" : "images/Alignment/37.png",
		"description" : "Pisces (pron.: /\u02C8pa\u026Asi\u02D0z/) is a constellation of the zodiac. Its name is the Latin plural for fish, and its symbol is\u2653. It lies between Aquarius to the west and Aries to the east. The ecliptic and the celestial equator intersect within this constellation and in Virgo.\r\rPisces originates from some composition of the Babylonian constellations Zibatti-me\u0161 (maybe \u0160inunutu4 \u0022the great swallow\u0022 in current eastern Pisces) and KU6 (\u0022the fish, Ea\u0022, Piscis Austrinus). In the first Millennium BCE texts known as the Astronomical Diaries, part of the constellation was also called DU.NU.NU (Rikis-nu.mi, \u0022the fish cord or ribbon\u0022). Rogers thinks this constellation was somehow misinterpreted and turned around so that the current northern fish is on the border of Andromeda, instead of being constituted by Piscis Austrinus.\r\rPisces is associated with the Roman legend of Venus and Cupid, who escaped the monster Typhon by transforming into fish and tying themselves together with rope. The knot of the rope is marked by alpha Piscium, also called Al-Rischa (\u0022the cord\u0022 in Arabic).\r\rThe Fishes are also associated with the German legend of Antenteh, who owned just a tub and a crude cabin when he met a magical fish. They offered him a wish, which he refused. However, his wife begged him to return to the fish and ask for a beautiful furnished home. This wish was granted, but her desires were not satisfied. She then asked to be a queen and have a palace, but when she asked to become a goddess, the fish became angry and took the palace and home, leaving the couple with the tub and cabin once again. The tub in the story is sometimes recognized as the Great Square of Pegasus.",
		"key" : "Pisces",
		"grouptype" : "Pisces",
		"Meaning" : "fishes",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Pisces",
		"title" : "Pisces Objects Group" },
	"Common" : "29 Piscium",
	"OType" : "Variable Star",
	"Distance" : "138.98",
	"DEC_S" : -3.02750332,
	"Constellation" : "Pisces ",
	"AMag" : 5.082,
	"key" : 50942,
	"title" : "29 Piscium"
	},
{
	"Index" : "30962",
	"Description" : "30 Piscium (30 Psc) is a star in the constellation Pisces. Its apparent magnitude is 4.41.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "30 Piscium, HIP 154, SAO 147042, HD 224935, GC 33330, HR 9089, DM BD-06  6345, TYC 4669-997-1",
	"group" : { "key" : "Pisces" },
	"Common" : "30 Piscium",
	"OType" : "Long Period Variable candidate",
	"Distance" : "131.49",
	"DEC_S" : -6.0140715,
	"X" : 441,
	"Y" : 604,
	"Constellation" : "Pisces ",
	"AMag" : 4.576,
	"key" : 50962,
	"title" : "30 Piscium"
	},
{
	"Index" : "30961",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "33 Piscium, HIP 443, SAO 128572, HD 28, GC 59, HR 3, DM BD-06  6357, TYC 4669-996-1",
	"group" : { "key" : "Pisces" },
	"Common" : "33 Piscium",
	"OType" : "Variable of RS CVn type",
	"Distance" : "39.47",
	"RA_S" : 1.33390735,
	"DEC_S" : -5.70761634,
	"Constellation" : "Pisces ",
	"AMag" : 4.727,
	"key" : 50961,
	"title" : "33 Piscium"
	},
{
	"Index" : "1485",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "47 Piscium, TV Piscium, HIP 2219, SAO 91910, HD 2411, GC 543, HR 103, DM BD+17    55, TYC 1183-1805-1",
	"group" : { "key" : "Pisces" },
	"Common" : "TV Piscium",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "160.32",
	"RA_S" : 7.01214503,
	"DEC_S" : 17.8931235,
	"Constellation" : "Pisces ",
	"AMag" : 5.243,
	"key" : 21485,
	"title" : "TV Piscium"
	},
{
	"Index" : "1560",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "52 Piscium, HIP 2568, SAO 74084, HD 2910, GC 641, HR 131, DM BD+19    79, TYC 1193-2069-1",
	"group" : { "key" : "Pisces" },
	"Common" : "52 Piscium",
	"OType" : "Star",
	"Distance" : "79.95",
	"RA_S" : 8.14785803,
	"DEC_S" : 20.29431945,
	"Constellation" : "Pisces ",
	"AMag" : 5.489,
	"key" : 21560,
	"title" : "52 Piscium"
	},
{
	"Index" : "1561",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "55 Piscium, HIP 3138B, SAO 74182, HD 3690, GC 784, HR 167, DM BD+20    87, TYC 1193-2070-1",
	"group" : { "key" : "Pisces" },
	"Common" : "55 Piscium",
	"OType" : "Double or multiple star",
	"Distance" : "126.67",
	"RA_S" : 9.98154959,
	"DEC_S" : 21.43849567,
	"Constellation" : "Pisces ",
	"AMag" : 5.36,
	"key" : 21561,
	"title" : "55 Piscium"
	},
{
	"Index" : "41508",
	"Description" : "Delta Piscium (Delta Psc, \u03B4 Piscium, \u03B4 Psc) is a binary star in the constellation Pisces, with an apparent magnitude of +4.43. The primary component is an orange K-type giant. It is approximately 305 light years from Earth. The temperature seems well-defined at 3975 Kelvin, which (to account for a lot of infrared radiation) with distance tells of a luminosity 380 times that of the Sun.\r\rDelta Piscium is moving through the Galaxy at a speed of 54.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 21,700 and 26,100 light years from the center of the Galaxy.\r\rDelta Piscium came closest to the Sun 1.0 million years ago when it had brightened to magnitude 3.96 from a distance of 249 light years.\r\rIn Chinese, \u5916\u5C4F (W\u00E0i P\u00EDng), meaning Outer Fence, refers to an asterism consisting of refers to an asterism consisting of \u03B4 Piscium, \u03B5 Piscium, \u03B6 Piscium, \u03BC Piscium, \u03BD Piscium, \u03BE Piscium and \u03B1 Piscium. Consequently, \u03B4 Piscium itself is known as \u5916\u5C4F\u4E00 (W\u00E0i P\u00EDng y\u012B, English: the First Star of Outer Fence.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "63 Piscium, Delta Piscium, HIP 3786, SAO 109474, HD 4656, GC 963, HR 224, DM BD+06   107, TYC 604-1301-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Linteum",
	"OType" : "High proper-motion Star",
	"Distance" : "95.37",
	"RA_S" : 12.1706003,
	"DEC_S" : 7.58508166,
	"X" : 288,
	"Y" : 427,
	"Constellation" : "Pisces ",
	"AMag" : 4.594,
	"key" : 61508,
	"title" : "Linteum"
	},
{
	"Index" : "1519",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "64 Piscium, HIP 3810, SAO 92099, HD 4676, GC 968, HR 225, DM BD+16    76, TYC 1188-1686-1",
	"group" : { "key" : "Pisces" },
	"Common" : "64 Piscium",
	"OType" : "Spectroscopic binary",
	"Distance" : "23.45",
	"RA_S" : 12.24462066,
	"DEC_S" : 16.94064534,
	"Constellation" : "Pisces ",
	"AMag" : 5.12,
	"key" : 21519,
	"title" : "64 Piscium"
	},
{
	"Index" : "10582",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "69 Piscium, Sigma Piscium, HIP 4889, SAO 54374, HD 6118, GC 1253, HR 291, DM BD+31   168, TYC 2277-843-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Sigma Piscium",
	"OType" : "Spectroscopic binary",
	"Distance" : "132.79",
	"RA_S" : 15.70456843,
	"DEC_S" : 31.80425941,
	"Constellation" : "Pisces ",
	"AMag" : 5.486,
	"key" : 30582,
	"title" : "Sigma Piscium"
	},
{
	"Index" : "42137",
	"Description" : "Epsilon Piscium (Epsilon Psc, \u03B5 Piscium, \u03B5 Psc) is the Bayer designation for a star approximately 182 light-years (56 parsecs) away from the Earth, in the constellation Pisces. It is a yellow-orange star of the G9 III or K0 III spectral type, meaning it has a surface temperature around 5,000 Kelvin. This is a normal giant star, slightly cooler in surface temperature, yet brighter and larger than our Sun. It is a suspected occultation double, with both stars having the same magnitude, separated by 0.25 arcsecond.\r\rIn Chinese, \u5916\u5C4F (W\u00E0i P\u00EDng), meaning Outer Fence, refers to an asterism consisting of refers to an asterism consisting of \u03B5 Piscium, \u03B4 Piscium, \u03B6 Piscium, \u03BC Piscium, \u03BD Piscium, \u03BE Piscium and \u03B1 Piscium. Consequently, \u03B5 Piscium itself is known as \u5916\u5C4F\u4E8C (W\u00E0i P\u00EDng \u00E8r, English: the Second Star of Outer Fence.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "71 Piscium, Epsilon Piscium, HIP 4906, SAO 109627, HD 6186, GC 1258, HR 294, DM BD+07   153, TYC 612-1446-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Kaht",
	"OType" : "Double or multiple star",
	"Distance" : "55.73",
	"RA_S" : 15.73586996,
	"DEC_S" : 7.89013507,
	"X" : 242,
	"Y" : 422,
	"Constellation" : "Pisces ",
	"AMag" : 4.364,
	"key" : 62137,
	"title" : "Kaht"
	},
{
	"Index" : "1636",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "74 Piscium, Psi01 Piscium, HIP 5131A, SAO 74482, HD 6456, GC 1309, HR 310, DM BD+20   156, TYC 1202-2124-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Psi01 Piscium",
	"OType" : "Double or multiple star",
	"Distance" : "83.99",
	"RA_S" : 16.42066726,
	"DEC_S" : 21.47316687,
	"Constellation" : "Pisces ",
	"AMag" : 5.271,
	"key" : 21636,
	"title" : "Psi01 Piscium"
	},
{
	"Index" : "1637",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "74 Piscium, Psi01 Piscium, HIP 5132B, SAO 74483, HD 6457, GC 1310, HR 311, DM BD+20   157, TYC 1202-2125-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Psi01 Piscium",
	"OType" : "Star",
	"Distance" : "85.56",
	"RA_S" : 16.42379184,
	"DEC_S" : 21.46545729,
	"Constellation" : "Pisces ",
	"AMag" : 5.447,
	"key" : 21637,
	"title" : "Psi01 Piscium"
	},
{
	"Index" : "10584",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "82 Piscium, g Piscium, HIP 5544, SAO 54493, HD 7034, GC 1431, HR 349, DM BD+30   181, TYC 2278-1259-1",
	"group" : { "key" : "Pisces" },
	"Common" : "g Piscium",
	"OType" : "Double or multiple star",
	"Distance" : "146.81",
	"RA_S" : 17.77819301,
	"DEC_S" : 31.42473908,
	"Constellation" : "Pisces ",
	"AMag" : 5.184,
	"key" : 30584,
	"title" : "g Piscium"
	},
{
	"Index" : "1638",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "84 Piscium, Chi Piscium, HIP 5571, SAO 74544, HD 7087, GC 1437, HR 351, DM BD+20   172, TYC 1202-2126-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Chi Piscium",
	"OType" : "Star",
	"Distance" : "117.56",
	"RA_S" : 17.86341594,
	"DEC_S" : 21.03465245,
	"Constellation" : "Pisces ",
	"AMag" : 4.771,
	"key" : 21638,
	"title" : "Chi Piscium"
	},
{
	"Index" : "10585",
	"Description" : "Tau Piscium (Tau Psc, \u03C4 Piscium, \u03C4 Psc) is an orange K-type giant with an apparent magnitude of +4.51. It is approximately 162 light years from Earth.\r\rTau Piscium is moving through the Galaxy at a speed of 40.5 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,900 and 40,900 light years from the center of the Galaxy.\r\rTau Piscium came closest to the Sun 1.1 million years ago when it had brightened to magnitude 2.97 from a distance of 83 light years.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of refers to an asterism consisting of \u03C4 Piscium, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, 91 Piscium, \u03C5 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03C4 Piscium itself is known as \u594E\u5BBF\u5341\u4E00 (Ku\u00ED S\u00F9 sh\u00EDy\u012B, English: the Eleventh Star of Legs.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "83 Piscium, Tau Piscium, HIP 5586, SAO 74546, HD 7106, GC 1441, HR 352, DM BD+29   190, TYC 2278-1260-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Tau Piscium",
	"OType" : "Star",
	"Distance" : "51.75",
	"RA_S" : 17.91514824,
	"DEC_S" : 30.0896432,
	"X" : 230,
	"Y" : 131,
	"Constellation" : "Pisces ",
	"AMag" : 4.633,
	"key" : 30585,
	"title" : "Tau Piscium"
	},
{
	"Index" : "42198",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "86 Piscium, Zeta Piscium, HIP 5737A, SAO 109739, HD 7344, GC 1476, HR 361, DM BD+06   174, TYC 613-1249-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Zeta Piscium",
	"OType" : "High proper-motion Star",
	"Distance" : "44.81",
	"RA_S" : 18.43286091,
	"DEC_S" : 7.57535872,
	"Constellation" : "Pisces ",
	"AMag" : 5.221,
	"key" : 62198,
	"title" : "Zeta Piscium"
	},
{
	"Index" : "6290",
	"Description" : "Phi Piscium (Phi Psc, \u03C6 Piscium, \u03C6 Psc) is a binary star system approximately 380 light years away in the constellation Pisces. It consists of Phi Piscium A, with a spectral type of K0III, and Phi Piscium B. Phi Piscium A possesses a surface temperature of 3,500 to 5,000 kelvins. Some suggest the only visible companion in the Phi Piscium B sub-system is a late F dwarf star, while others suggest it is a K0 star. The invisible component of the Phi Piscium B sub-system is proposed to have a spectral type of M2V. The star system has a period of about 20\u00BD years and has a notably high eccentricity of 0.815.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of refers to an asterism consisting of \u03C6 Piscium, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C5 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03C6 Piscium itself is known as \u594E\u5BBF\u5341\u56DB (Ku\u00ED S\u00F9 sh\u00ED s\u00EC, English: the Fourteenth Star of Legs.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "85 Piscium, Phi Piscium, HIP 5742, SAO 74571, HD 7318, GC 1474, HR 360, DM BD+23   158, TYC 1747-2263-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Phi Piscium",
	"OType" : "Double or multiple star",
	"Distance" : "136.52",
	"RA_S" : 18.43728157,
	"DEC_S" : 24.58370895,
	"X" : 218,
	"Y" : 203,
	"Constellation" : "Pisces ",
	"AMag" : 4.786,
	"key" : 26290,
	"title" : "Phi Piscium"
	},
{
	"Index" : "10827",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "89 Piscium, f Piscium, HIP 6061, SAO 109793, HD 7804, GC 1566, HR 378, DM BD+02   185, TYC 23-1341-1",
	"group" : { "key" : "Pisces" },
	"Common" : "f Piscium",
	"OType" : "Star",
	"Distance" : "75.25",
	"RA_S" : 19.44981811,
	"DEC_S" : 3.61446437,
	"Constellation" : "Pisces ",
	"AMag" : 5.147,
	"key" : 30827,
	"title" : "f Piscium"
	},
{
	"Index" : "6322",
	"Description" : "Upsilon Piscium (Upsilon Psc, \u03C5 Piscium, \u03C5 Psc) is a star approximately 310 light years away from Earth, in the constellation Pisces. It is bluish-white star of the spectral type A3V. It has a surface temperature of 7,500 to 11,000 kelvins, and is approximately the same size as our Sun, yet is much hotter and brighter. It has a rotational velocity of 93 kilometers per second at the equator.\r\rIn Chinese, \u594E\u5BBF (Ku\u00ED S\u00F9), meaning Legs (asterism), refers to an asterism consisting of refers to an asterism consisting of \u03C5 Piscium, \u03B7 Andromedae, 65 Piscium, \u03B6 Andromedae, \u03B5 Andromedae, \u03B4 Andromedae, \u03C0 Andromedae, \u03BD Andromedae, \u03BC Andromedae, \u03B2 Andromedae, \u03C3 Piscium, \u03C4 Piscium, 91 Piscium, \u03C6 Piscium, \u03C7 Piscium and \u03C8\u00B9 Piscium. Consequently, \u03C5 Piscium itself is known as \u594E\u5BBF\u5341\u4E09 (Ku\u00ED S\u00F9 sh\u00ED s\u0101n, English: the Thirteenth Star of Legs.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "90 Piscium, Upsilon Piscium, HIP 6193, SAO 74637, HD 7964, GC 1591, HR 383, DM BD+26   220, TYC 1751-2178-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Upsilon Piscium",
	"OType" : "Star",
	"Distance" : "94.37",
	"RA_S" : 19.86664165,
	"DEC_S" : 27.26405675,
	"X" : 205,
	"Y" : 167,
	"Constellation" : "Pisces ",
	"AMag" : 4.753,
	"key" : 26322,
	"title" : "Upsilon Piscium"
	},
{
	"Index" : "6341",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "91 Piscium, l Piscium, HIP 6315, SAO 74647, HD 8126, GC 1630, HR 389, DM BD+27   215, TYC 1754-2321-1",
	"group" : { "key" : "Pisces" },
	"Common" : "l Piscium",
	"OType" : "Star",
	"Distance" : "107.29",
	"RA_S" : 20.28072019,
	"DEC_S" : 28.73820688,
	"Constellation" : "Pisces ",
	"AMag" : 5.386,
	"key" : 26341,
	"title" : "l Piscium"
	},
{
	"Index" : "1630",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "93 Piscium, Rho Piscium, HIP 6706, SAO 92436, HD 8723, GC 1733, HR 413, DM BD+18   187, TYC 1201-1725-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Rho Piscium",
	"OType" : "Variable Star",
	"Distance" : "25.21",
	"RA_S" : 21.56360024,
	"DEC_S" : 19.17234281,
	"Constellation" : "Pisces ",
	"AMag" : 5.389,
	"key" : 21630,
	"title" : "Rho Piscium"
	},
{
	"Index" : "20271",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "98 Piscium, Mu Piscium, HIP 7007, SAO 109926, HD 9138, GC 1819, HR 434, DM BD+05   194, TYC 34-1287-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Mu Piscium",
	"OType" : "High proper-motion Star",
	"Distance" : "93.16",
	"RA_S" : 22.54631213,
	"DEC_S" : 6.14382228,
	"Constellation" : "Pisces ",
	"AMag" : 4.995,
	"key" : 40271,
	"title" : "Mu Piscium"
	},
{
	"Index" : "1607",
	"Description" : "Eta Piscium (Eta Psc, \u03B7 Piscium, \u03B7 Psc) is the brightest star in the constellation Pisces. Eta Piscium is located at a distance of about 294 light years from Earth and shines at magnitude +3.62. It is of Spectral type G7 III.\r\rThe total luminosity of this star is 316 times that of the Sun while its surface temperature is 4930 kelvins. The star has a radius of 26 \u00B1 2 times solar while its mass is 3.5 to 4 solar masses.\r\rEta Piscium has a faint companion star with a separation of about 1\u0022.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "99 Piscium, Eta Piscium, HIP 7097AB, SAO 92484, HD 9270, GC 1839, HR 437, DM BD+14   231, TYC 1198-1597-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Alpherg",
	"OType" : "Double or multiple star",
	"Distance" : "106.42",
	"RA_S" : 22.87087592,
	"DEC_S" : 15.34582789,
	"X" : 156,
	"Y" : 320,
	"Constellation" : "Pisces ",
	"AMag" : 3.712,
	"key" : 21607,
	"title" : "Alpherg"
	},
{
	"Index" : "21304",
	"Description" : "Nu Piscium (Nu Psc, \u03BD Piscium, \u03BD Psc) is a star approximately 368 light years away from Earth, in the constellation Pisces. It is an orange star of the spectral type K3IIIb, meaning it possesses a surface temperature between 3,500 and 5,000 kelvins. It is a giant star, cooler in surface temperature than our Sun, yet larger and brighter.\r\rNu Piscium was a latter designation of 51 Ceti.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "106 Piscium, Nu Piscium, HIP 7884, SAO 110065, HD 10380, GC 2055, HR 489, DM BD+04   293, TYC 35-435-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Nu Piscium",
	"OType" : "Star",
	"Distance" : "111.27",
	"RA_S" : 25.35789226,
	"DEC_S" : 5.48760831,
	"X" : 117,
	"Y" : 448,
	"Constellation" : "Pisces ",
	"AMag" : 4.587,
	"key" : 41304,
	"title" : "Nu Piscium"
	},
{
	"Index" : "1705",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "107 Piscium, HIP 7981, SAO 74883, HD 10476, GC 2080, HR 493, DM BD+19   279, TYC 1211-1733-1",
	"group" : { "key" : "Pisces" },
	"Common" : "107 Piscium",
	"OType" : "Variable Star",
	"Distance" : "7.53",
	"RA_S" : 25.62401387,
	"DEC_S" : 20.26851628,
	"Constellation" : "Pisces ",
	"AMag" : 5.337,
	"key" : 21705,
	"title" : "107 Piscium"
	},
{
	"Index" : "42673",
	"Description" : "Omicron Piscium (Omicron Psc, \u03BF Piscium, \u03BF Psc) is a star in the constellation Pisces, located about 142 light years from Earth.\r\rIt has an apparent magnitude of +4.26 and belongs to spectral type G8.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "110 Piscium, Omicron Piscium, HIP 8198, SAO 110110, HD 10761, GC 2139, HR 510, DM BD+08   273, TYC 622-574-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Omicron Piscium",
	"OType" : "Variable Star",
	"Distance" : "85.35",
	"RA_S" : 26.34846273,
	"DEC_S" : 9.15774949,
	"X" : 107,
	"Y" : 398,
	"Constellation" : "Pisces ",
	"AMag" : 4.368,
	"key" : 62673,
	"title" : "Omicron Piscium"
	},
{
	"Index" : "19482",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "111 Piscium, Xi Piscium, HIP 8833, SAO 110206, HD 11559, GC 2293, HR 549, DM BD+02   290, TYC 33-1213-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Xi Piscium",
	"OType" : "Spectroscopic binary",
	"Distance" : "58.3",
	"RA_S" : 28.38895755,
	"DEC_S" : 3.18753055,
	"Constellation" : "Pisces ",
	"AMag" : 4.709,
	"key" : 39482,
	"title" : "Xi Piscium"
	},
{
	"Index" : "25658",
	"Description" : "Alpha Piscium (Alpha Psc, \u03B1 Piscium, \u03B1 Psc) is the Bayer designation for a star in the equatorial constellation of Pisces. It has the traditional name Alrescha (Al Rescha, Alrischa, Alrisha).\r\rThe distance to \u03B1 Psc is about 139 light years. The system comprises a close double star with angular separation of presently 1.8\u0022 between the components. The main star is of magnitude +4.33 and spectral type A0p, while the companion is magnitude 5.23 and belongs to spectral class A3m. The two stars take more than 700 years to orbit one another and they will make their closest approach to each other around 2060. One or both of the stars may be a spectroscopic binary as well. The stars have masses of 2.3 and 1.8 solar masses respectively and shine with a total luminosity of 31 and 12 times that of the Sun.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "113 Piscium, Alpha Piscium, HIP 9487A, SAO 110291, HD 12447, GC 2452, HR 596, DM BD+02   317A, TYC 40-1338-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Alrescha",
	"OType" : "Star",
	"Distance" : "46.04",
	"RA_S" : 30.51169807,
	"DEC_S" : 2.76374242,
	"X" : 48,
	"Y" : 479,
	"Constellation" : "Pisces ",
	"AMag" : 4.1,
	"key" : 45658,
	"shortTitle" : "Alrischa; Alrescha; El Rischa; Al Richa; Rescha; Okda; Kaitain; Al'risha; Okda; Kantajn; Resha",
	"title" : "Alrescha"
	},
{
	"Index" : "25659",
	"Description" : "Alpha Piscium (Alpha Psc, \u03B1 Piscium, \u03B1 Psc) is the Bayer designation for a star in the equatorial constellation of Pisces. It has the traditional name Alrescha (Al Rescha, Alrischa, Alrisha).\r\rThe distance to \u03B1 Psc is about 139 light years. The system comprises a close double star with angular separation of presently 1.8\u0022 between the components. The main star is of magnitude +4.33 and spectral type A0p, while the companion is magnitude 5.23 and belongs to spectral class A3m. The two stars take more than 700 years to orbit one another and they will make their closest approach to each other around 2060. One or both of the stars may be a spectroscopic binary as well. The stars have masses of 2.3 and 1.8 solar masses respectively and shine with a total luminosity of 31 and 12 times that of the Sun.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "113 Piscium, Alpha Piscium, HIP 9487B, HD 12446, GC 2452, HR 595, DM BD+02   317B, TYC 40-1338-2",
	"group" : { "key" : "Pisces" },
	"Common" : "Alrescha",
	"OType" : "Star",
	"Distance" : "46.04",
	"RA_S" : 30.51169807,
	"DEC_S" : 2.76374242,
	"X" : 48,
	"Y" : 479,
	"Constellation" : "Pisces ",
	"AMag" : 5.167,
	"key" : 45659,
	"shortTitle" : "Kaitain; Okda; Rescha; Al'risha; Okda; Kantajn; Resha",
	"title" : "Alrescha"
	},
{
	"Index" : "39271",
	"Description" : "Beta Piscium (Beta Psc, \u03B2 Piscium, \u03B2 Psc) is a star in the constellation Pisces. It has the traditional name Fum al Samakah.\r\rBeta Piscium belongs to the spectral class B6Ve and is of magnitude +4.53m. It is approximately 492 light-years from the Sun.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "4 Piscium, Beta Piscium, HIP 113889, SAO 127934, HD 217891, GC 32134, HR 8773, DM BD+03  4818, TYC 579-1834-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Fum al Samakah",
	"OType" : "Be Star",
	"Distance" : "125.04",
	"RA_S" : 345.9692259,
	"DEC_S" : 3.82004928,
	"X" : 629,
	"Y" : 467,
	"Constellation" : "Pisces ",
	"AMag" : 4.461,
	"key" : 59271,
	"title" : "Fum al Samakah"
	},
{
	"Index" : "39324",
	"Description" : "Gamma Piscium (Gamma Psc, \u03B3 Piscium, \u03B3 Psc) is a star approximately 138 light years away from Earth, in the zodiac constellation of Pisces.It lets out gas every 56 years that scientists call star pheses. It is a yellow star with a spectral type of G9 III, meaning it has a surface temperature of 4,885 K and is a giant star. It is slightly cooler than our Sun, yet it is 10 solar radii in size and shines with the light of 61 Suns. At an apparent magnitude of 3.7, it is the second brightest star in the constellation Pisces, between Eta and Alpha. Once a white A2 star, it is 5.5 billion years old.\r\rGamma Piscium moves across the sky at three-quarters of an arcsecond per year, which at 138 light years corresponds to 153 kilometers per second. This suggests it is a visitor from another part of the Milky Way Galaxy; in astronomical terms, it will quickly leave the vicinity of the Sun. Its metallicity is only one-fourth that of the Sun, and visitors from outside the thin disk that composes the Milky Way tend to be metal-poor. It also has a low carbon-nitrogen content. Gamma Piscium lies inside an asterism known as the \u0022circlet of Pisces.\r\rIn Chinese, \u9739\u9742 (P\u012B L\u00EC), meaning Thunderbolt, refers to an asterism consisting of refers to an asterism consisting of \u03B3 Piscium, \u03B2 Piscium, \u03B8 Piscium, \u03B9 Piscium and \u03C9 Piscium. Consequently, \u03B3 Piscium itself is known as \u9739\u9742\u4E8C (P\u012B L\u00EC \u00E8r, English: the Second Star of Thunderbolt.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "6 Piscium, Gamma Piscium, HIP 114971, SAO 128085, HD 219615, GC 32415, HR 8852, DM BD+02  4648, TYC 580-1884-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Simmah",
	"OType" : "High proper-motion Star",
	"Distance" : "42.3",
	"RA_S" : 349.29140639,
	"DEC_S" : 3.28228654,
	"X" : 586,
	"Y" : 477,
	"Constellation" : "Pisces ",
	"AMag" : 3.798,
	"key" : 59324,
	"title" : "Simmah"
	},
{
	"Index" : "39651",
	"Description" : "7 Piscium (also known as 7 Psc or HR 8878) is a metal-deficient giant star in the constellation Pisces.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "7 Piscium, b Piscium, HIP 115227, SAO 128126, HD 220009, GC 32491, HR 8878, DM BD+04  4997, TYC 584-1516-1",
	"group" : { "key" : "Pisces" },
	"Common" : "7 Piscium",
	"OType" : "Star",
	"Distance" : "132.18",
	"RA_S" : 350.08576619,
	"DEC_S" : 5.38130566,
	"X" : 575,
	"Y" : 450,
	"Constellation" : "Pisces ",
	"AMag" : 5.202,
	"key" : 59651,
	"title" : "7 Piscium"
	},
{
	"Index" : "39206",
	"Description" : "Kappa Piscium (Kappa Psc, \u03BA Piscium, \u03BA Psc) is a multiple star approximately 162 light years away from Earth, in the constellation Pisces. Appearing as a single point in the sky, it is easily split when viewed with a pair of binoculars, and consists of three components. One star has an apparent magnitude of 4.87 at maximum brightness and 4.95 at minimum brightness, while the other has an apparent magnitude of 11.9.\r\rThe brighter component is a variable star, meaning its brightness fluctuates by a magnitude of 0.01 to 0.1. Specifically, it is an Alpha\u00B2 Canum Venaticorum variable, a star with strong magnetic fields and strong silicon, strontium, and chromium spectral lines. It also shows many lines of uranium, and possibly the rare element holmium. Its uranium and osmium content could have been caused by a nearby supernova. It is deficient in oxygen relative to magnesium.\r\rThe star rotates approximately once every 48 hours at a velocity of about 41 km/s. As it is a class A star, it possesses a surface temperature between 7,500 to 11,000 kelvins.\r\rIn Chinese, \u96F2\u96E8 (Y\u00FAn Y\u01D4), meaning Cloud and Rain, refers to an asterism consisting of refers to an asterism consisting of \u03BA Piscium, 12 Piscium, 21 Piscium and \u03BB Piscium. Consequently, \u03BA Piscium itself is known as \u96F2\u96E8\u4E00 (Y\u00FAn Y\u01D4 y\u012B, English: the First Star of Cloud and Rain.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "8 Piscium, Kappa Piscium, HIP 115738, SAO 128186, HD 220825, GC 32620, HR 8911, DM BD+00  4998, TYC 578-1415-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Kappa Piscium",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "47.05",
	"RA_S" : 351.73314848,
	"DEC_S" : 1.2556063,
	"X" : 555,
	"Y" : 505,
	"Constellation" : "Pisces ",
	"AMag" : 4.923,
	"key" : 59206,
	"title" : "Kappa Piscium"
	},
{
	"Index" : "39650",
	"Description" : "Theta Piscium (Theta Psc, \u03B8 Piscium, \u03B8 Psc) is a star approximately 159 light years away from Earth in the constellation Pisces. It is an orange-red star of the spectral type K1III, meaning it is a normal giant star with a surface temperature of 3,500 to 5,000 kelvins, and is brighter yet cooler than our sun.\r\rIn Chinese, \u9739\u9742 (P\u012B L\u00EC), meaning Thunderbolt, refers to an asterism consisting of refers to an asterism consisting of \u03B8 Piscium, \u03B2 Piscium, \u03B3 Piscium, \u03B9 Piscium and \u03C9 Piscium. Consequently, \u03B8 Piscium itself is known as \u9739\u9742\u4E09 (P\u012B L\u00EC s\u0101n, English: the Third Star of Thunderbolt.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "10 Piscium, Theta Piscium, HIP 115830, SAO 128196, HD 220954, GC 32647, HR 8916, DM BD+05  5173, TYC 584-1515-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Theta Piscium",
	"OType" : "Star",
	"Distance" : "45.53",
	"RA_S" : 351.99206551,
	"DEC_S" : 6.37898978,
	"X" : 549,
	"Y" : 438,
	"Constellation" : "Pisces ",
	"AMag" : 4.394,
	"key" : 59650,
	"title" : "Theta Piscium"
	},
{
	"Index" : "40305",
	"Description" : "Iota Piscium (Iota Psc, \u03B9 Piscium, \u03B9 Psc) is a star 45 light years away from Earth, in the constellation Pisces. The star is a yellowish dwarf (main sequence) star of spectral type F7V, which is somewhat larger and brighter than our sun, but still within the range considered to have the potential for Earth-like planets. It has a surface temperature of about 6,000 to 7,500 kelvin. Iota Piscium is a suspected variable star, and was once thought to have one or two stellar companions, but both are line-of-sight coincidences.\r\rIn Chinese, \u9739\u9742 (P\u012B L\u00EC), meaning Thunderbolt, refers to an asterism consisting of refers to an asterism consisting of \u03B9 Piscium, \u03B2 Piscium, \u03B3 Piscium, \u03B8 Piscium, and \u03C9 Piscium. Consequently, \u03B9 Piscium itself is known as \u9739\u9742\u56DB (P\u012B L\u00EC s\u00EC, English: the Fourth Star of Thunderbolt.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "17 Piscium, Iota Piscium, HIP 116771, SAO 128310, HD 222368, GC 32879, HR 8969, DM BD+04  5035, TYC 591-1744-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Iota Piscium",
	"OType" : "Variable Star",
	"Distance" : "13.71",
	"RA_S" : 354.98767175,
	"DEC_S" : 5.62629106,
	"X" : 511,
	"Y" : 450,
	"Constellation" : "Pisces ",
	"AMag" : 4.176,
	"key" : 60305,
	"title" : "Iota Piscium"
	},
{
	"Index" : "39905",
	"Description" : "Lambda Piscium (Lambda Psc, \u03BB Piscium, \u03BB Psc) is a star approximately 101 light years away from Earth in the constellation Pisces. It is a bluish-white star of A7V spectral classification, meaning it has a surface temperature of 7,500 to 11,000 kelvins. It is much brighter and hotter in surface temperature than our sun, yet is approximately the same size. Lambda Piscium forms the southeast corner of the \u0022Circlet\u0022 in Pisces.\r\rIn Chinese, \u96F2\u96E8 (Y\u00FAn Y\u01D4), meaning Cloud and Rain, refers to an asterism consisting of refers to an asterism consisting of \u03BB Piscium, \u03BA Piscium, 12 Piscium and 21 Piscium. Consequently, \u03BB Piscium itself is known as \u96F2\u96E8\u56DB (Y\u00FAn Y\u01D4 s\u00EC, English: the Fourth Star of Cloud and Rain.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "18 Piscium, Lambda Piscium, HIP 116928, SAO 128336, HD 222603, GC 32917, HR 8984, DM BD+00  5037, TYC 586-1458-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Lambda Piscium",
	"OType" : "High proper-motion Star",
	"Distance" : "32.69",
	"RA_S" : 355.51169435,
	"DEC_S" : 1.78004045,
	"X" : 505,
	"Y" : 500,
	"Constellation" : "Pisces ",
	"AMag" : 4.514,
	"key" : 59905,
	"title" : "Lambda Piscium"
	},
{
	"Index" : "40150",
	"Description" : "TX Piscium (aka 19 Psc) is a variable carbon star in the constellation Pisces. It is amongst the reddest stars known, with a significant reddish hue when seen in binoculars.\r\rTX Piscium is of spectral class C5 and its apparent magnitude varies from +4.9 to +5.5 in an irregular manner. It is approximately 760 light years from Earth.",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "19 Piscium, TX Piscium, HIP 117245, SAO 128374, HD 223075, GC 32995, HR 9004, DM BD+02  4709, TYC 589-1671-1",
	"group" : { "key" : "Pisces" },
	"Common" : "TX Piscium",
	"OType" : "Carbon Star",
	"Distance" : "271.72",
	"RA_S" : 356.59798581,
	"DEC_S" : 3.48680914,
	"X" : 491,
	"Y" : 478,
	"Constellation" : "Pisces ",
	"AMag" : 5.306,
	"key" : 60150,
	"title" : "TX Piscium"
	},
{
	"Index" : "35278",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "27 Piscium, HIP 118209, SAO 147008, HD 224533, GC 33248, HR 9067, DM BD-04  5996, TYC 5256-1131-1",
	"group" : { "key" : "Pisces" },
	"Common" : "27 Piscium",
	"OType" : "Double or multiple star",
	"Distance" : "71.86",
	"RA_S" : 359.66824021,
	"DEC_S" : -3.55598079,
	"Constellation" : "Pisces ",
	"AMag" : 4.989,
	"key" : 55278,
	"title" : "27 Piscium"
	},
{
	"Index" : "40471",
	"Description" : "Omega Piscium (Omega Psc, \u03C9 Piscium, \u03C9 Psc) is a star approximately 106 light years away from Earth, in the constellation Pisces. It has a spectral type of F4IV, meaning it is a subgiant/dwarf star, and it has a temperature of 6,600 kelvins. It may or may not be a close binary star system. Variations in its spectrum were once interpreted as giving it an orbital period of 2.16 days, but this claim was later debunked as false. It is 20 times brighter than our Sun and is 1.8 times greater in mass, if it is a single star.\r\rCounting stars with Flamsteed numbers, Greek letters, and proper names, Omega Piscium is the named star with the highest right ascension (akin to terrestrial longitude). Due to the 26,000-year wobble of the Earth\u0027s axis, this will change in 2013, when its right ascension will reset to 0 hours. It is the first star to the east of the Circlet of Pisces, which represents the head of the western fish in the constellation.\r\rIn Chinese, \u9739\u9742 (P\u012B L\u00EC), meaning Thunderbolt, refers to an asterism consisting of refers to an asterism consisting of \u03C9 Piscium, \u03B2 Piscium, \u03B3 Piscium, \u03B8 Piscium and \u03B9 Piscium. Consequently, \u03C9 Piscium itself is known as \u9739\u9742\u4E94 (P\u012B L\u00EC wu, English: the Fifth Star of Thunderbolt.)",
	"MapNum" : "37",
	"ImageNum" : "37",
	"Desig" : "28 Piscium, Omega Piscium, HIP 118268, SAO 128513, HD 224617, GC 33262, HR 9072, DM BD+06  5227, TYC 593-1697-1",
	"group" : { "key" : "Pisces" },
	"Common" : "Vernalis",
	"OType" : "Star",
	"Distance" : "31.99",
	"RA_S" : 359.82787316,
	"DEC_S" : 6.86331901,
	"X" : 448,
	"Y" : 436,
	"Constellation" : "Pisces ",
	"AMag" : 4.06,
	"key" : 60471,
	"title" : "Vernalis"
	},
{
	"Index" : "52728",
	"Description" : "Iota Piscis Austrini (Iota PsA, \u03B9 Piscis Austrini, \u03B9 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +4.35. The primary component is a white B-type subgiant. It is approximately 205 light years from Earth.\r\rIota Piscis Austrini is moving through the Galaxy at a speed of 29.7 km/s relative to the Sun. Its projected Galactic orbit carries it between 18,400 and 24,300 light years from the center of the Galaxy. \r\rIn Chinese, \u5929\u9322 (Ti\u0101n Qi\u00E1n), meaning Celestial Money, refers to an asterism consisting of refers to an asterism consisting of \u03B9 Piscis Austrini 13 Piscis Austrini, \u03B8 Piscis Austrini, \u03BC Piscis Austrini and \u03C4 Piscis Austrini. Consequently, \u03B9 Piscis Austrini itself is known as \u5929\u9322\u4E09 (Ti\u0101n Qi\u00E1n s\u0101n, English: the Third Star of Celestial Money.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "9 Piscis Austrini, Iota Piscis Austrini, HIP 107380, SAO 213258, HD 206742, GC 30439, HR 8305, DM CD-33 15734, TYC 7490-1839-1",
	"group" : { "backgroundImage" : "images/Alignment/05.png",
		"description" : "Piscis Austrinus (also known as Piscis Australis) is a constellation in the southern celestial hemisphere. The name is Latin for \u0022the southern fish\u0022, in contrast with the larger constellation Pisces, which represents a pair of fishes. Prior to the 20th century, it was also known as Piscis Notius. Its only star brighter than 4th magnitude is Fomalhaut, which is a first-magnitude star and is the 18th brightest star in the night sky.\r\rPiscis Austrinus was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. The stars of the modern constellation Grus once formed part of Piscis Austrinus. In 1597 (or 1598), Petrus Plancius carved out a separate constellation and named it after the crane.\r\rIn Greek mythology, this constellation is known as the Great Fish and it is portrayed as swallowing the water being poured out by Aquarius, the water-bearer constellation. The two fish of the constellation Pisces are said to be the offspring of the Great Fish. In Egyptian mythology, this fish saved the life of the Egyptian goddess Isis, so she placed this fish and its descendants into the heavens as constellations of stars.\r\rPisces Austrinus originated with the Babylonian constellation simply known as the Fish (MUL.KU).",
		"key" : "Piscis Austrinus",
		"grouptype" : "Piscis Austrinus",
		"Meaning" : "southern fish",
		"Family" : "Heavenly Waters",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Piscis Austrinus",
		"title" : "Piscis Austrinus Objects Group" },
	"Common" : "Iota Piscis Austrini",
	"OType" : "Star",
	"Distance" : "62.61",
	"RA_S" : 326.23670919,
	"DEC_S" : -33.02578052,
	"X" : 432,
	"Y" : 581,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.323,
	"key" : 72728,
	"title" : "Iota Piscis Austrini"
	},
{
	"Index" : "52707",
	"Description" : "Theta Piscis Austrini (Theta PsA, \u03B8 Piscis Austrini, \u03B8 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +5.02. The primary component is a white A-type main sequence star. It is approximately 339 light years from Earth.\r\rTheta Piscis Austrini is moving through the Galaxy at a speed of 21.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 22,600 and 38,300 light years from the center of the Galaxy.\r\rTheta Piscis Austrini came closest to the Sun 2.7 million years ago when it had brightened to magnitude 4.54 from a distance of 256 light years.\r\rIn Chinese, \u5929\u9322 (Ti\u0101n Qi\u00E1n), meaning Celestial Money, refers to an asterism consisting of refers to an asterism consisting of \u03B8 Piscis Austrini, 13 Piscis Austrini, \u03B9 Piscis Austrini, \u03BC Piscis Austrini and \u03C4 Piscis Austrini. Consequently, \u03B8 Piscis Austrini itself is known as \u5929\u9322\u4E8C (Ti\u0101n Qi\u00E1n \u00E8r, English: the Second Star of Celestial Money.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "10 Piscis Austrini, Theta Piscis Austrini, HIP 107608, SAO 213292, HD 207155, GC 30509, HR 8326, DM CD-31 18466, TYC 7487-1984-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Theta Piscis Austrini",
	"OType" : "Double or multiple star",
	"Distance" : "98.24",
	"RA_S" : 326.93394969,
	"DEC_S" : -30.89830014,
	"X" : 426,
	"Y" : 553,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.022,
	"key" : 72707,
	"title" : "Theta Piscis Austrini"
	},
{
	"Index" : "48158",
	"Description" : "Eta Piscis Austrini (Eta PsA, \u03B7 Piscis Austrini, \u03B7 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +5.43. The primary component is a blue B-type subgiant. It is approximately 1012 light years from Earth.\r\rEta Piscis Austrini is moving through the Galaxy at a speed of 11.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,600 and 30,800 light years from the center of the Galaxy.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "12 Piscis Austrini, Eta Piscis Austrini, HIP 108661B, TYC 6960-1866-2",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Eta Piscis Austrini",
	"OType" : "Be Star",
	"Distance" : "246.35",
	"RA_S" : 330.20935288,
	"DEC_S" : -28.45377033,
	"X" : 389,
	"Y" : 520,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 6.766,
	"key" : 68158,
	"title" : "Eta Piscis Austrini"
	},
{
	"Index" : "48157",
	"Description" : "Eta Piscis Austrini (Eta PsA, \u03B7 Piscis Austrini, \u03B7 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +5.43. The primary component is a blue B-type subgiant. It is approximately 1012 light years from Earth.\r\rEta Piscis Austrini is moving through the Galaxy at a speed of 11.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,600 and 30,800 light years from the center of the Galaxy.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "12 Piscis Austrini, Eta Piscis Austrini, HIP 108661A, SAO 190822, HD 209014, GC 30785, HR 8386, DM CD-29 18119, TYC 6960-1866-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Eta Piscis Austrini",
	"OType" : "Be Star",
	"Distance" : "246.35",
	"RA_S" : 330.20935288,
	"DEC_S" : -28.45377033,
	"X" : 389,
	"Y" : 520,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.696,
	"key" : 68157,
	"title" : "Eta Piscis Austrini"
	},
{
	"Index" : "52751",
	"Description" : "Mu Piscis Austrini (Mu PsA, \u03BC Piscis Austrini, \u03BC PsA) is a white A-type main sequence star with an apparent magnitude of +4.50. It is approximately 130 light years from Earth.\r\rMu Piscis Austrini is moving through the Galaxy at a speed of 20 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 28,500 light years from the center of the Galaxy.\r\rMu Piscis Austrini came closest to the Sun 1.2 million years ago when it had brightened to magnitude 4.06 from a distance of 111 light years.\r\rIn Chinese, \u5929\u9322 (Ti\u0101n Qi\u00E1n), meaning Celestial Money, refers to an asterism consisting of refers to an asterism consisting of \u03BC Piscis Austrini, 13 Piscis Austrini, \u03B8 Piscis Austrini, \u03B9 Piscis Austrini and \u03C4 Piscis Austrini. Consequently, \u03BC Piscis Austrini itself is known as \u5929\u9322\u56DB (Ti\u0101n Qi\u00E1n s\u00EC, English: the Fifth Star of Celestial Money.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "14 Piscis Austrini, Mu Piscis Austrini, HIP 109285, SAO 213576, HD 210049, GC 30954, HR 8431, DM CD-33 15922, TYC 7492-1466-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Mu Piscis Austrini",
	"OType" : "Variable Star",
	"Distance" : "41.57",
	"RA_S" : 332.09586308,
	"DEC_S" : -32.98846662,
	"X" : 366,
	"Y" : 579,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.502,
	"key" : 72751,
	"title" : "Mu Piscis Austrini"
	},
{
	"Index" : "52753",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "Upsilon Piscis Austrini, HIP 109289, SAO 213577, HD 210066, GC 30957, HR 8433, DM CD-34 15421, TYC 7492-1468-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Upsilon Piscis Austrini",
	"OType" : "Star",
	"Distance" : "129.91",
	"RA_S" : 332.10804877,
	"DEC_S" : -34.04383939,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.149,
	"key" : 72753,
	"title" : "Upsilon Piscis Austrini"
	},
{
	"Index" : "52752",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "HIP 109404, SAO 213599, HD 210271, GC 30996, HR 8444, DM CD-3415430, TYC 7492-1467-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "HR 8444",
	"OType" : "Variable Star",
	"Distance" : "63.34",
	"RA_S" : 332.48208947,
	"DEC_S" : -34.01496867,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.399,
	"key" : 72752,
	"title" : "HR 8444"
	},
{
	"Index" : "52750",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "15 Piscis Austrini, Tau Piscis Austrini, HIP 109422, SAO 213602, HD 210302, GC 31003, HR 8447, DM CD-33 15941, TYC 7492-1465-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Tau Piscis Austrini",
	"OType" : "High proper-motion Star",
	"Distance" : "18.28",
	"RA_S" : 332.5365834,
	"DEC_S" : -32.54840635,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.988,
	"key" : 72750,
	"title" : "Tau Piscis Austrini"
	},
{
	"Index" : "48164",
	"Description" : "Lambda Piscis Austrini (Lambda PsA, \u03BB Piscis Austrini, \u03BB PsA) is a blue B-type main sequence star with an apparent magnitude of +5.45. It is approximately 508 light years from Earth.\r\rLambda Piscis Austrini is moving through the Galaxy at a speed of 18.1 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 29,300 light years from the center of the Galaxy.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "16 Piscis Austrini, Lambda Piscis Austrini, HIP 109789, SAO 190985, HD 210934, GC 31095, HR 8478, DM CD-28 17653, TYC 6961-1626-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Lambda Piscis Austrini",
	"OType" : "Star",
	"Distance" : "153.14",
	"RA_S" : 333.5781279,
	"DEC_S" : -27.7669083,
	"X" : 350,
	"Y" : 511,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.412,
	"key" : 68164,
	"title" : "Lambda Piscis Austrini"
	},
{
	"Index" : "52798",
	"Description" : "Beta Piscis Austrini (Beta PsA, \u03B2 Piscis Austrini, \u03B2 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +4.29. The primary component is a white A-type subgiant. It is approximately 148 light years from Earth.\r\rBeta Piscis Austrini is moving through the Galaxy at a speed of 14.4 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,900 and 28,300 light years from the center of the Galaxy.\r\rWith Delta and Zeta it constituted Tien Kang (\u0022heavenly rope\u0022) in China.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "17 Piscis Austrini, Beta Piscis Austrini, HIP 111188, SAO 213883, HD 213398, GC 31459, HR 8576, DM CD-32 17126, TYC 7497-1511-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Beta Piscis Austrini",
	"OType" : "High proper-motion Star",
	"Distance" : "43.78",
	"RA_S" : 337.87637951,
	"DEC_S" : -32.34607797,
	"X" : 301,
	"Y" : 570,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.28,
	"key" : 72798,
	"title" : "Beta Piscis Austrini"
	},
{
	"Index" : "48197",
	"Description" : "Epsilon Piscis Austrini (Epsilon PsA, \u03B5 Piscis Austrini, \u03B5 PsA) is a blue B-type main sequence star with an apparent magnitude of +4.18. It is approximately 744 light years from Earth.\r\rEpsilon Piscis Austrini is moving through the Galaxy at a speed of 18.7 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,900 and 28,100 light years from the center of the Galaxy.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "18 Piscis Austrini, Epsilon Piscis Austrini, HIP 111954, SAO 191318, HD 214748, GC 31646, HR 8628, DM CD-27 16010, TYC 6966-1509-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Epsilon Piscis Austrini",
	"OType" : "Be Star",
	"Distance" : "147.54",
	"RA_S" : 340.16392911,
	"DEC_S" : -27.04361888,
	"X" : 273,
	"Y" : 502,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.16,
	"key" : 68197,
	"title" : "Epsilon Piscis Austrini"
	},
{
	"Index" : "52896",
	"Description" : "Gamma Piscis Austrini (Gamma PsA, \u03B3 Piscis Austrini, \u03B3 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +4.46. The primary component is a white A-type giant. It is approximately 222 light years from Earth. With a temperature estimated at 10,600 Kelvin, the star shines with a rather decent luminosity of 81 times that of the Sun.\r\rGamma Piscis Austrini is moving through the Galaxy at a speed of 24.1 km/s relative to the Sun. Its projected Galactic orbit carries it between 21,600 and 30,800 light years from the center of the Galaxy.\r\rGamma Piscis Austrini came closest to the Sun 1.8 million years ago when it had brightened to magnitude 3.78 from a distance of 157 light years.\r\rIn Chinese, \u6557\u81FC (B\u00E0i Ji\u00F9), meaning Decayed Mortar, refers to an asterism consisting of refers to an asterism consisting of \u03B3 Piscis Austrini, \u03B3 Gruis, \u03BB Gruis and 19 Piscis Austrini. Consequently, \u03B3 Piscis Austrini itself is known as \u6557\u81FC\u4E09 (B\u00E0i Ji\u00F9 s\u0101n, English: the Third Star of Decayed Mortar.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "22 Piscis Austrini, Gamma Piscis Austrini, HIP 112948B, SAO 214153, HD 216336, GC 31895, HR 8695, DM CD-33 16270, TYC 7508-1315-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Gamma Piscis Austrini",
	"OType" : "Star",
	"Distance" : "65.94",
	"RA_S" : 343.130067,
	"DEC_S" : -32.875742,
	"X" : 243,
	"Y" : 579,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.026,
	"key" : 72896,
	"title" : "Gamma Piscis Austrini"
	},
{
	"Index" : "52895",
	"Description" : "Gamma Piscis Austrini (Gamma PsA, \u03B3 Piscis Austrini, \u03B3 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +4.46. The primary component is a white A-type giant. It is approximately 222 light years from Earth. With a temperature estimated at 10,600 Kelvin, the star shines with a rather decent luminosity of 81 times that of the Sun.\r\rGamma Piscis Austrini is moving through the Galaxy at a speed of 24.1 km/s relative to the Sun. Its projected Galactic orbit carries it between 21,600 and 30,800 light years from the center of the Galaxy.\r\rGamma Piscis Austrini came closest to the Sun 1.8 million years ago when it had brightened to magnitude 3.78 from a distance of 157 light years.\r\rIn Chinese, \u6557\u81FC (B\u00E0i Ji\u00F9), meaning Decayed Mortar, refers to an asterism consisting of refers to an asterism consisting of \u03B3 Piscis Austrini, \u03B3 Gruis, \u03BB Gruis and 19 Piscis Austrini. Consequently, \u03B3 Piscis Austrini itself is known as \u6557\u81FC\u4E09 (B\u00E0i Ji\u00F9 s\u0101n, English: the Third Star of Decayed Mortar.)",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "22 Piscis Austrini, Gamma Piscis Austrini, HIP 112948A, SAO 214153, HD 216336, GC 31895, HR 8695, DM CD-33 16270, TYC 7508-1313-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Gamma Piscis Austrini",
	"OType" : "Star",
	"Distance" : "65.94",
	"RA_S" : 343.13138489,
	"DEC_S" : -32.87555453,
	"X" : 243,
	"Y" : 579,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.502,
	"key" : 72895,
	"title" : "Gamma Piscis Austrini"
	},
{
	"Index" : "52894",
	"Description" : "Delta Piscis Austrini (Delta PsA, \u03B4 Piscis Austrini, \u03B4 PsA) is multiple star system in constellation of Piscis Austrinus, with an apparent magnitude of +4.20. The primary component is a yellow G-type giant. It is approximately 170 light years from Earth.\r\rDelta Piscis Austrini is moving through the Galaxy at a speed of 13.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,000 and 35,300 light years from the center of the Galaxy.\r\rDelta Piscis Austrini will come closest to the Sun 2.8 million years from now when it will brighten to magnitude 2.87 from a distance of 83 light years.\r\rThe Chinese name for Delta Piscis Austrini is \u5929\u7DB1 (Ti\u0101n G\u0101ng) meaning Materials for Making Tents, because this star is marking itself and stand alone in Materials for Making Tents asterism, Well mansion (see : Chinese constellation). \u5929\u7DB1 (Ti\u0101n G\u0101ng) westernized into Tien Kang, meaning \u0022the Heavenly Rope\u0022 in R.H. Allen\u0027s work, but the name is for the asterism consisting this star, \u03B2 PsA and \u03B6 PsA.",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "23 Piscis Austrini, Delta Piscis Austrini, HIP 113246, SAO 214189, HD 216763, GC 31974, HR 8720, DM CD-33 16303, TYC 7508-1312-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Delta Piscis Austrini",
	"OType" : "Star",
	"Distance" : "47.25",
	"RA_S" : 343.98709154,
	"DEC_S" : -32.53962916,
	"X" : 233,
	"Y" : 575,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 4.315,
	"key" : 72894,
	"title" : "Delta Piscis Austrini"
	},
{
	"Index" : "52904",
	"MapNum" : "05",
	"ImageNum" : "05",
	"Desig" : "Pi Piscis Austrini, HIP 113860, SAO 214275, HD 217792, GC 32122, HR 8767, DM CD-35 15630, TYC 7509-1264-1",
	"group" : { "key" : "Piscis Austrinus" },
	"Common" : "Pi Piscis Austrini",
	"OType" : "Cepheid variable Star",
	"Distance" : "29.4",
	"RA_S" : 345.87422707,
	"DEC_S" : -34.74942143,
	"Constellation" : "Piscis Austrinus ",
	"AMag" : 5.159,
	"key" : 72904,
	"title" : "Pi Piscis Austrini"
	},
{
	"Index" : "58058",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 30953AB, TYC 8111-2007-1",
	"group" : { "backgroundImage" : "images/Alignment/17.png",
		"description" : "Puppis (pron.: /\u02C8p\u028Cp\u0268s/) is a constellation in the southern sky. Its name is the Latin word for the poop deck of a ship, and Puppis represents the deck of the ship and its deckhouses. Puppis was originally part of an over-large constellation, the ship of \u0022Jason and the Argonauts\u0022, Argo Navis, which was centuries later divided into three parts, the other two being Carina (the keel and hull), and Vela (the sails of the ship). Puppis is the largest of the three constellations in square degrees. It is one of the 88 modern constellations recognized by the International Astronomical Union.\r\rArgo Navis was sub-divided in 1752 by the French astronomer Nicolas Louis de Lacaille, forming Puppis. Despite the division, Lacaille kept Argo\u0027s Bayer designations. Therefore Carina has the \u03B1, \u03B2 and \u03B5, Vela has \u03B3 and \u03B4, Puppis has \u03B6, and so on.",
		"key" : "Puppis",
		"grouptype" : "Puppis",
		"Meaning" : "poop deck",
		"Family" : "Heavenly Waters",
		"Origin" : "1763, Lacaille, split from Argo Navis",
		"shortTitle" : "Puppis",
		"title" : "Puppis Objects Group" },
	"Common" : "TYC 8111-2007-1",
	"OType" : "Star",
	"Distance" : "51.37",
	"RA_S" : 97.45428926,
	"DEC_S" : -50.2390828,
	"Constellation" : "Puppis ",
	"AMag" : 5.424,
	"key" : 78058,
	"title" : "TYC 8111-2007-1"
	},
{
	"Index" : "53793",
	"Description" : "Nu Puppis (Nu Pup, \u03BD Puppis, \u03BD Pup) is a blue B-type giant with an apparent magnitude of +3.17. It is the fifth brightest star in Puppis. At a distance of 423 light years, this class B (B8) giant, with a measured temperature of 12,000 Kelvin, shines with a luminosity (after allowance for ultraviolet radiation) of 1340 times that of Sun.\r\rNu Puppis is moving through the Galaxy at a speed of 31 km/s relative to the Sun. Its projected Galactic orbit carries it between 19,000 and 24,400 light years from the center of the Galaxy. It came closest to the Sun 3.6 million years ago when it had brightened to magnitude -2.57 from a distance of 26 light years.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Nu Puppis, HIP 31685, SAO 218071, HD 47670, GC 8675, HR 2451, DM CD-43  2576, TYC 7626-2203-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Nu Puppis",
	"OType" : "Cepheid variable Star",
	"Distance" : "113.78",
	"RA_S" : 99.4402973,
	"DEC_S" : -43.19593498,
	"X" : 411,
	"Y" : 496,
	"Constellation" : "Puppis ",
	"AMag" : 3.138,
	"key" : 73793,
	"title" : "Nu Puppis"
	},
{
	"Index" : "58038",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Y Puppis, HIP 31765B, SAO 218093, HD 47973, GC 8704, HR 2462, DM CD-48  2417, TYC 8108-2223-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Y Puppis",
	"OType" : "Variable Star",
	"Distance" : "132.76",
	"RA_S" : 99.65680783,
	"DEC_S" : -48.22018526,
	"Constellation" : "Puppis ",
	"AMag" : 5.05,
	"key" : 78038,
	"title" : "Y Puppis"
	},
{
	"Index" : "58039",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 31765A, TYC 8108-2224-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Y Puppis (HR 2462)",
	"OType" : "Variable Star",
	"Distance" : "132.76",
	"RA_S" : 99.65681768,
	"DEC_S" : -48.22017638,
	"Constellation" : "Puppis ",
	"AMag" : 5.141,
	"key" : 78039,
	"title" : "Y Puppis (HR 2462)"
	},
{
	"Index" : "53808",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "x Puppis, HIP 32537, SAO 197215, HD 49591, GC 8899, HR 2518, DM CD-37  3080, TYC 7627-2519-1",
	"group" : { "key" : "Puppis" },
	"Common" : "x Puppis",
	"OType" : "Star",
	"Distance" : "99.37",
	"RA_S" : 101.83916764,
	"DEC_S" : -37.92969838,
	"Constellation" : "Puppis ",
	"AMag" : 5.247,
	"key" : 73808,
	"title" : "x Puppis"
	},
{
	"Index" : "58107",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "X Puppis, HIP 32765, SAO 218235, HD 50223, GC 8960, HR 2548, DM CD-46  2703, TYC 8117-1539-1",
	"group" : { "key" : "Puppis" },
	"Common" : "X Puppis",
	"OType" : "High proper-motion Star",
	"Distance" : "25.26",
	"RA_S" : 102.47756436,
	"DEC_S" : -46.61456092,
	"Constellation" : "Puppis ",
	"AMag" : 5.187,
	"key" : 78107,
	"title" : "X Puppis"
	},
{
	"Index" : "58184",
	"Description" : "Tau Puppis (Tau Pup, \u03C4 Puppis, \u03C4 Pup) is a star in the southern constellation of Puppis. It has an apparent visual magnitude of +2.95 and is located at a distance of about 182 light-years (56 parsecs) from Earth. This is a spectroscopic binary star system, with the presence of the secondary component being revealed by the shifts of absorption lines in the spectrum resulting from the Doppler effect. The two components orbit each other with a period of 1,066.0 days (2.9 years) and a low eccentricity of 0.090.\r\rThe primary component of this system has a stellar classification of K1 III. A luminosity class \u0027III\u0027 indicates this has expanded into a giant star after exhausting the supply of hydrogen at its core and evolving away from the main sequence of stars like the Sun. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is 4.49 \u00B1 0.07 mas, which, at its estimated distance, equates to a physical radius of about 27 times the radius of the Sun. It appears to be rotating slowly, with a projected rotational velocity of 2.2 km s\u20131. This gives a lower bound on the azimuthal velocity of rotation along the star\u0027s equator. Tau Puppis is radiating energy from its outer envelope at an effective temperature of around 4,500, giving it the orange hue of a cool, K-type star.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Tau Puppis, HIP 32768, SAO 234735, HD 50310, GC 8969, HR 2553, DM CD-50  2415, TYC 8125-2314-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Tau Puppis",
	"OType" : "Spectroscopic binary",
	"Distance" : "55.77",
	"RA_S" : 102.48403588,
	"DEC_S" : -50.61455277,
	"X" : 372,
	"Y" : 589,
	"Constellation" : "Puppis ",
	"AMag" : 3.05,
	"key" : 78184,
	"title" : "Tau Puppis"
	},
{
	"Index" : "49349",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 32855, SAO 197277, HD 50235, GC 8979, HR 2549, DM CD-34 3140, TYC 7096-2300-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2549",
	"OType" : "Star",
	"Distance" : "248.83",
	"RA_S" : 102.7181318,
	"DEC_S" : -34.36731945,
	"Constellation" : "Puppis ",
	"AMag" : 5.149,
	"key" : 69349,
	"title" : "HR 2549"
	},
{
	"Index" : "58156",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 33357, SAO 218324, HD 51799, GC 9137, HR 2608, DM CD-48 2601, TYC 8122-1697-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2608",
	"OType" : "Variable Star",
	"Distance" : "263.36",
	"RA_S" : 104.06662787,
	"DEC_S" : -48.72114192,
	"Constellation" : "Puppis ",
	"AMag" : 5.137,
	"key" : 78156,
	"title" : "HR 2608"
	},
{
	"Index" : "49357",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "t Puppis, HIP 33558AB, SAO 197427, HD 52092, GC 9184, HR 2619, DM CD-33  3389, TYC 7097-2515-1",
	"group" : { "key" : "Puppis" },
	"Common" : "t Puppis",
	"OType" : "Double or multiple star",
	"Distance" : "179.53",
	"RA_S" : 104.60456463,
	"DEC_S" : -34.11170467,
	"Constellation" : "Puppis ",
	"AMag" : 5.042,
	"key" : 69357,
	"title" : "t Puppis"
	},
{
	"Index" : "58195",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "H Puppis, HIP 34059, SAO 218427, HD 53811, GC 9348, HR 2672, DM CD-49  2587, TYC 8126-2550-1",
	"group" : { "key" : "Puppis" },
	"Common" : "H Puppis",
	"OType" : "Star",
	"Distance" : "60.52",
	"RA_S" : 105.97334792,
	"DEC_S" : -49.58391765,
	"Constellation" : "Puppis ",
	"AMag" : 4.942,
	"key" : 78195,
	"title" : "H Puppis"
	},
{
	"Index" : "53906",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "C Puppis, HIP 34081AB, SAO 218424, HD 53704, GC 9342, HR 2666, DM CD-42  2929, TYC 7637-2648-1",
	"group" : { "key" : "Puppis" },
	"Common" : "C Puppis",
	"OType" : "Double or multiple star",
	"Distance" : "106.74",
	"RA_S" : 106.01165009,
	"DEC_S" : -42.33727655,
	"Constellation" : "Puppis ",
	"AMag" : 5.218,
	"key" : 73906,
	"title" : "C Puppis"
	},
{
	"Index" : "53868",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "A Puppis, HIP 34495, SAO 197632, HD 54893, GC 9463, HR 2702, DM CD-39  3105, TYC 7633-2708-1",
	"group" : { "key" : "Puppis" },
	"Common" : "A Puppis",
	"OType" : "Cepheid variable Star",
	"Distance" : "237.56",
	"RA_S" : 107.21278319,
	"DEC_S" : -39.65565278,
	"Constellation" : "Puppis ",
	"AMag" : 4.787,
	"key" : 73868,
	"title" : "A Puppis"
	},
{
	"Index" : "58201",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 34670, SAO 218513, HD 55526, GC 9523, HR 2719, DM CD-48 2765, TYC 8127-1731-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Gliese 3434",
	"OType" : "High proper-motion Star",
	"Distance" : "96.87",
	"RA_S" : 107.69784313,
	"DEC_S" : -48.93209745,
	"Constellation" : "Puppis ",
	"AMag" : 5.259,
	"key" : 78201,
	"title" : "Gliese 3434"
	},
{
	"Index" : "53874",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "E Puppis, HIP 34802A, SAO 218525, HD 55719A, GC 9554, HR 2727, DM CD-40  2987, TYC 7634-1222-1",
	"group" : { "key" : "Puppis" },
	"Common" : "E Puppis",
	"OType" : "Star",
	"Distance" : "125.76",
	"RA_S" : 108.06586541,
	"DEC_S" : -40.49880674,
	"Constellation" : "Puppis ",
	"AMag" : 5.314,
	"key" : 73874,
	"title" : "E Puppis"
	},
{
	"Index" : "58132",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "I Puppis, HIP 34834, SAO 218537, HD 55892, GC 9569, HR 2740, DM CD-46  2977, TYC 8119-2547-1",
	"group" : { "key" : "Puppis" },
	"Common" : "I Puppis",
	"OType" : "Variable Star of gamma Dor type",
	"Distance" : "21.43",
	"RA_S" : 108.1401073,
	"DEC_S" : -46.75930683,
	"Constellation" : "Puppis ",
	"AMag" : 4.518,
	"key" : 78132,
	"title" : "I Puppis"
	},
{
	"Index" : "58128",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "L01 Puppis, HIP 34899, SAO 218546, HD 56022, GC 9591, HR 2746, DM CD-44  3223, TYC 8119-1757-1",
	"group" : { "key" : "Puppis" },
	"Common" : "L01 Puppis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "56.52",
	"RA_S" : 108.30562795,
	"DEC_S" : -45.18274543,
	"Constellation" : "Puppis ",
	"AMag" : 4.871,
	"key" : 78128,
	"title" : "L01 Puppis"
	},
{
	"Index" : "53943",
	"Description" : "L\u00B2 Puppis (also known as HD 56096) is a giant star in the constellation of Puppis and is located between the bright stars Canopus and Sirius. It is a semi-regular pulsating star that varies in apparent magnitude from 2.60 down to 6.00 with a period of 140.83 days. The variation in light may be caused by a combination of radial pulsations in the star\u0027s atmosphere and by dimming from circumstellar dust. This is most likely an asymptotic giant branch star that has passed through the main sequence and is evolving to become a white dwarf. It is shedding mass at the rate of about 2.2 \u00D7 10\u22129 solar masses per year. Recently the star has had an apparent magnitude range of about 6.9 to 8.\r\rL2 Puppis has a visual 10th magnitude companion about a minute of arc away.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "L02 Puppis, HIP 34922, SAO 218549, HD 56096, GC 9604, HR 2748, DM CD-44  3227, TYC 7642-1461-1",
	"group" : { "key" : "Puppis" },
	"Common" : "L2 Puppis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "63.75",
	"RA_S" : 108.38466803,
	"DEC_S" : -44.6397414,
	"X" : 325,
	"Y" : 509,
	"Constellation" : "Puppis ",
	"AMag" : 4.767,
	"key" : 73943,
	"title" : "L2 Puppis"
	},
{
	"Index" : "58163",
	"Description" : "HD 56456 is a star in the constellation Puppis. Its apparent magnitude is 4.74.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35020, SAO 218567, HD 56456, GC 9635, HR 2762, DM CD-48 2807, TYC 8123-2767-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 56456",
	"OType" : "Star",
	"Distance" : "115.42",
	"RA_S" : 108.65892079,
	"DEC_S" : -48.2719316,
	"X" : 327,
	"Y" : 536,
	"Constellation" : "Puppis ",
	"AMag" : 4.731,
	"key" : 78163,
	"title" : "HD 56456"
	},
{
	"Index" : "49568",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 35226, SAO 197790, HD 56779, GC 9696, HR 2770, DM CD-36 3485, TYC 7115-3015-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2770",
	"OType" : "Star in Cluster",
	"Distance" : "240.52",
	"RA_S" : 109.20586267,
	"DEC_S" : -36.5926326,
	"Constellation" : "Puppis ",
	"AMag" : 4.983,
	"key" : 69568,
	"title" : "HR 2770"
	},
{
	"Index" : "49571",
	"Description" : "Pi Puppis (Pi Pup, \u03C0 Puppis, \u03C0 Pup) is the second brightest star in the southern constellation of Puppis. It has an apparent visual magnitude of 2.733, so it can be viewed with the naked eye at night. Parallax measurements yield an estimated distance of roughly 810 light-years (250 pc) from the Earth. This is a double star with a magnitude 6.86 companion at an angular separation of 0.72 arcsecond and a position angle of 148\u00B0.\r\rThe spectrum of Pi Puppis matches a stellar classification of K3 Ib. The Ib luminosity class indicates this a lower luminosity supergiant star that has consumed the hydrogen fuel at its core, evolved away from the main sequence, and expanded to about 290 times the Sun\u0027s radius. The effective temperature of the star\u0027s outer envelope is about 4,000 K, which gives it the orange hue of a K-type star. It is a semiregular variable star that varies in apparent magnitude from a high of 2.70 down to 2.85. Pi Puppis is the brightest star in the open cluster Collinder 135.\r\rIn Chinese, \u5F27\u77E2 (H\u00FA Sh\u01D0), meaning Bow and Arrow, refers to an asterism consisting of \u03C0 Puppis, \u03B4 Canis Majoris, \u03B7 Canis Majoris, HD 63032, HD 65456, \u03BF Puppis, k Puppis, \u03B5 Canis Majoris and \u03BA Canis Majoris. Consequently, \u03C0 Puppis itself is known as \u5F27\u77E2\u4E5D (H\u00FA Sh\u01D0 ji\u01D4, English: the Ninth Star of Bow and Arrow.)",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Pi Puppis, HIP 35264AC, SAO 197795, HD 56855Aa, GC 9706, HR 2773, DM CD-36  3489, TYC 7115-3019-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Tureis",
	"OType" : "Star",
	"Distance" : "246.72",
	"RA_S" : 109.28565491,
	"DEC_S" : -37.09747668,
	"X" : 318,
	"Y" : 410,
	"Constellation" : "Puppis ",
	"AMag" : 2.866,
	"key" : 69571,
	"title" : "Tureis"
	},
{
	"Index" : "49569",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "v01 Puppis, HIP 35363, SAO 197824, HD 57150, GC 9733, HR 2787, DM CD-36  3512, TYC 7115-3016-1",
	"group" : { "key" : "Puppis" },
	"Common" : "v01 Puppis",
	"OType" : "Be Star",
	"Distance" : "246.7",
	"RA_S" : 109.5766325,
	"DEC_S" : -36.7339557,
	"Constellation" : "Puppis ",
	"AMag" : 4.659,
	"key" : 69569,
	"title" : "v01 Puppis"
	},
{
	"Index" : "53837",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "F Puppis, HIP 35393, SAO 197836, HD 57240, GC 9743, HR 2791, DM CD-38  3309, TYC 7630-2343-1",
	"group" : { "key" : "Puppis" },
	"Common" : "F Puppis",
	"OType" : "Star",
	"Distance" : "141.68",
	"RA_S" : 109.63963772,
	"DEC_S" : -39.21027996,
	"Constellation" : "Puppis ",
	"AMag" : 5.245,
	"key" : 73837,
	"title" : "F Puppis"
	},
{
	"Index" : "49570",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "v02 Puppis, HIP 35406, SAO 197837, HD 57219, GC 9746, HR 2790, DM CD-36  3519, TYC 7115-3017-1",
	"group" : { "key" : "Puppis" },
	"Common" : "v02 Puppis",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "240.91",
	"RA_S" : 109.65910407,
	"DEC_S" : -36.74274007,
	"Constellation" : "Puppis ",
	"AMag" : 5.07,
	"key" : 69570,
	"title" : "v02 Puppis"
	},
{
	"Index" : "53958",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "y Puppis, HIP 36363, SAO 198045, HD 59635, GC 10033, HR 2875, DM CD-38  3400, TYC 7643-2149-1",
	"group" : { "key" : "Puppis" },
	"Common" : "y Puppis",
	"OType" : "X-ray Binary",
	"Distance" : "179.79",
	"RA_S" : 112.27373127,
	"DEC_S" : -38.81206705,
	"Constellation" : "Puppis ",
	"AMag" : 5.37,
	"key" : 73958,
	"title" : "y Puppis"
	},
{
	"Index" : "54126",
	"Description" : "Sigma Puppis (Sigma Pup, \u03C3 Puppis, \u03C3 Pup) is a binary star system in the southern constellation of Puppis. It has an apparent visual magnitude of 3.25, which is bright enough to be visible to the naked eye at night from the southern hemisphere. Through a telescope, it appears as an bright, orange-hued star with a nearby white companion. Parallax measurements indicate this star is located at a distance of about 194 light-years (59 parsecs) from Earth.\r\rThis is a spectroscopic binary system, consisting of an orbiting pair of stars that have not been individually resolved with a telescope. Their orbital period is 257.8 days and the eccentricity is 0.17. The pair form an eclipsing binary of the Beta Lyrae type and a period of 130.5 days, or one half of their orbital period. The eclipse of the primary component causes a decline of 0.04 magnitudes, while the secondary eclipse reduces the magnitude by 0.03.\r\rThe combined stellar classification is K5 III, which matches the spectrum of a giant star. The measured angular diameter of the primary star is 16.71 \u00B1 2.84 mas. At the estimated distance of this system, this yields a physical size of about 107 times the radius of the Sun. The primary component shows the behavior of a slow irregular variable.\r\rIn addition to its binary components, Sigma Puppis has a more distant companion that has a matching proper motion, suggesting that it may be gravitationally bound to the binary. This magnitude 8.5 star is at an angular separation of 22.4 arcseconds with a position angle of 74\u00B0 from Sigma Puppis, which is equivalent to a projected separation of 1,200 Astronomical Units. In 1970, American astronomer Olin J. Eggen suggested that Sigma Puppis belonged to a moving group of stars that share a similar motion through space, and thereby a common origin. It served as the eponym for this, the \u03C3 Puppis group. The existence of this group was later brought into question.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Sigma Puppis, HIP 36377, SAO 218755, HD 59717, GC 10040, HR 2878, DM CD-43  3260, TYC 7655-2687-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Hadir",
	"OType" : "Spectroscopic binary",
	"Distance" : "56.32",
	"RA_S" : 112.30762743,
	"DEC_S" : -43.30143311,
	"X" : 288,
	"Y" : 491,
	"Constellation" : "Puppis ",
	"AMag" : 3.418,
	"key" : 74126,
	"title" : "Hadir"
	},
{
	"Index" : "45249",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 36431, SAO 173864, HD 59612, GC 10043, HR 2874, DM BD-22 1897, TYC 6538-3324-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2874",
	"OType" : "Star",
	"Distance" : "952.381",
	"RA_S" : 112.46421661,
	"DEC_S" : -23.02428659,
	"Constellation" : "Puppis ",
	"AMag" : 4.88,
	"key" : 65249,
	"title" : "HR 2874"
	},
{
	"Index" : "49453",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 36514, SAO 198064, HD 59890, GC 10071, HR 2881, DM CD-30 4620, TYC 7105-3516-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2881",
	"OType" : "Star",
	"Distance" : "454.16",
	"RA_S" : 112.67750963,
	"DEC_S" : -30.96228158,
	"Constellation" : "Puppis ",
	"AMag" : 4.738,
	"key" : 69453,
	"title" : "HR 2881"
	},
{
	"Index" : "36794",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 36773, SAO 153072, HD 60414, GC 10122, HR 2902, DM BD-14 1971, TYC 5409-1859-1",
	"group" : { "key" : "Puppis" },
	"Common" : "V* KQ Pup",
	"OType" : "Long-period variable star",
	"Distance" : "399.98",
	"RA_S" : 113.44984739,
	"DEC_S" : -14.5238965,
	"Constellation" : "Puppis ",
	"AMag" : 5.11,
	"key" : 56794,
	"title" : "V* KQ Pup"
	},
{
	"Index" : "49599",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "z Puppis, HIP 36778, SAO 198130, HD 60606, GC 10139, HR 2911, DM CD-36  3715, TYC 7117-2765-1",
	"group" : { "key" : "Puppis" },
	"Common" : "z Puppis",
	"OType" : "Be Star",
	"Distance" : "360.34",
	"RA_S" : 113.46267724,
	"DEC_S" : -36.3383938,
	"Constellation" : "Puppis ",
	"AMag" : 5.406,
	"key" : 69599,
	"title" : "z Puppis"
	},
{
	"Index" : "41115",
	"Description" : "HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as our Sun (2.7 Gyr) and has metallicity of only 38% that of our Sun. In 2008, two extrasolar planets were discovered in orbit around it.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 36795, SAO 174009, HD 60532, GC 10134, HR 2906, DM BD-21 2007, TYC 5991-217-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 60532",
	"OType" : "Star",
	"Distance" : "25.3",
	"RA_S" : 113.5132535,
	"DEC_S" : -22.29606662,
	"X" : 271,
	"Y" : 218,
	"Constellation" : "Puppis ",
	"AMag" : 4.493,
	"key" : 61115,
	"title" : "HD 60532"
	},
{
	"Index" : "45422",
	"Description" : "HD 60863 is a star in the constellation Puppis. Its apparent magnitude is 4.63.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "p Puppis, HIP 36917, SAO 174058, HD 60863, GC 10178, HR 2922, DM CD-28  4566, TYC 6551-3461-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 60863",
	"OType" : "Star",
	"Distance" : "68.81",
	"RA_S" : 113.84540663,
	"DEC_S" : -28.36931859,
	"X" : 269,
	"Y" : 297,
	"Constellation" : "Puppis ",
	"AMag" : 4.617,
	"key" : 65422,
	"title" : "HD 60863"
	},
{
	"Index" : "49548",
	"Description" : "HD 61330 is a star in the constellation Puppis. Its apparent magnitude is 4.52.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "f Puppis, HIP 37096AC, SAO 198195, HD 61330, GC 10246, HR 2937, DM CD-34  3755, TYC 7113-3280-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 61330",
	"OType" : "Double or multiple star",
	"Distance" : "110.24",
	"RA_S" : 114.34211882,
	"DEC_S" : -34.96852245,
	"X" : 265,
	"Y" : 383,
	"Constellation" : "Puppis ",
	"AMag" : 4.527,
	"key" : 69548,
	"title" : "HD 61330"
	},
{
	"Index" : "45323",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "m Puppis, HIP 37173, SAO 174175, HD 61429, GC 10266, HR 2944, DM CD-25  4828, TYC 6543-3376-1",
	"group" : { "key" : "Puppis" },
	"Common" : "m Puppis",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "189.2",
	"RA_S" : 114.57518921,
	"DEC_S" : -25.36480601,
	"Constellation" : "Puppis ",
	"AMag" : 4.664,
	"key" : 65323,
	"title" : "m Puppis"
	},
{
	"Index" : "45372",
	"Description" : "k Puppis (k Pup, k Puppis) is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis. Note that the designation here is \u0022k\u0022 not \u0022kappa\u0022 (\u03BA) as some astronomers teach. Many of Puppis\u0027 stellar designations are English labels. This pair of stars is given the traditional Arabic name Markeb or Markab.\r\rBoth k1 Puppis and k2 Puppis are bright blue B-type giant stars of nearly equal brightness, +4.50 and +4.62, respectively. To the naked eye, the pair has a combined magnitude of +3.80. On the sky, the two stars are separated by approximately 9.9 seconds of arc along PA 318\u00BA. The optical pair can be distinguished easily with a small telescope. The component k1 Puppis is a binary star system in its own right, while k2 Puppis is a variable star. Each star within the k Puppis optical pair is between 450 and 470 light years from Earth.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Kappa01 Puppis, HIP 37229B, SAO 174198, HD 61555, GC 10281, HR 2948, DM CD-26  4707B, TYC 6547-2626-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Markeb / Markab",
	"OType" : "Star",
	"Distance" : "105.36",
	"RA_S" : 114.70575036,
	"DEC_S" : -26.80180356,
	"X" : 258,
	"Y" : 277,
	"Constellation" : "Puppis ",
	"AMag" : 4.616,
	"key" : 65372,
	"shortTitle" : "Markab",
	"title" : "Markeb / Markab"
	},
{
	"Index" : "45373",
	"Description" : "k Puppis (k Pup, k Puppis) is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis. Note that the designation here is \u0022k\u0022 not \u0022kappa\u0022 (\u03BA) as some astronomers teach. Many of Puppis\u0027 stellar designations are English labels. This pair of stars is given the traditional Arabic name Markeb or Markab.\r\rBoth k1 Puppis and k2 Puppis are bright blue B-type giant stars of nearly equal brightness, +4.50 and +4.62, respectively. To the naked eye, the pair has a combined magnitude of +3.80. On the sky, the two stars are separated by approximately 9.9 seconds of arc along PA 318\u00BA. The optical pair can be distinguished easily with a small telescope. The component k1 Puppis is a binary star system in its own right, while k2 Puppis is a variable star. Each star within the k Puppis optical pair is between 450 and 470 light years from Earth.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Kappa02 Puppis, HIP 37229A, SAO 174199, HD 61556, GC 10283, HR 2949, DM CD-26  4707A, TYC 6547-2627-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Markeb / Markab",
	"OType" : "Variable Star",
	"Distance" : "105.36",
	"RA_S" : 114.70778595,
	"DEC_S" : -26.80383507,
	"X" : 258,
	"Y" : 277,
	"Constellation" : "Puppis ",
	"AMag" : 4.401,
	"key" : 65373,
	"title" : "Markeb / Markab"
	},
{
	"Index" : "53969",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "d01 Puppis, HIP 37297, SAO 198253, HD 61831, GC 10311, HR 2961, DM CD-38  3531, TYC 7644-2700-1",
	"group" : { "key" : "Puppis" },
	"Common" : "d01 Puppis",
	"OType" : "Star in Cluster",
	"Distance" : "181.38",
	"RA_S" : 114.86390636,
	"DEC_S" : -38.30802555,
	"Constellation" : "Puppis ",
	"AMag" : 4.788,
	"key" : 73969,
	"title" : "d01 Puppis"
	},
{
	"Index" : "41001",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "140 Puppis, HIP 37379, SAO 153227, HD 61772, GC 10328, HR 2959, DM BD-14  2082, TYC 5980-1606-1",
	"group" : { "key" : "Puppis" },
	"Common" : "140 Puppis",
	"OType" : "Star",
	"Distance" : "211.96",
	"RA_S" : 115.09670883,
	"DEC_S" : -15.26392361,
	"Constellation" : "Puppis ",
	"AMag" : 5.138,
	"key" : 61001,
	"title" : "140 Puppis"
	},
{
	"Index" : "53997",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 37450, SAO 198298, HD 62226, GC 10355, HR 2981, DM CD-38 3556, TYC 7645-3249-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 2981",
	"OType" : "Spectroscopic binary",
	"Distance" : "184.69",
	"RA_S" : 115.3158836,
	"DEC_S" : -38.53353302,
	"Constellation" : "Puppis ",
	"AMag" : 5.371,
	"key" : 73997,
	"title" : "HR 2981"
	},
{
	"Index" : "58282",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 37606, SAO 218923, HD 62644, GC 10402, HR 2998, DM CD-44 3675, TYC 8134-800-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Gliese 284",
	"OType" : "High proper-motion Star",
	"Distance" : "24.67",
	"RA_S" : 115.73790132,
	"DEC_S" : -45.17311909,
	"Constellation" : "Puppis ",
	"AMag" : 5.126,
	"key" : 78282,
	"title" : "Gliese 284"
	},
{
	"Index" : "45433",
	"Description" : "1 Puppis (1 Pup) is a red giant star in the constellation of Puppis, its vis mag 4.62.\r\r1 Puppis lies in the northern part of the constellation at a distance of 770 ly, east of Aludra in Canis Major and just above the white supergiant, 3 Puppis.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "1 Puppis, HIP 37648, SAO 174391, HD 62576, GC 10409, HR 2993, DM CD-28  4767, TYC 6552-3227-1",
	"group" : { "key" : "Puppis" },
	"Common" : "1 Puppis",
	"OType" : "Variable Star",
	"Distance" : "236.13",
	"RA_S" : 115.88494408,
	"DEC_S" : -28.41088421,
	"X" : 245,
	"Y" : 305,
	"Constellation" : "Puppis ",
	"AMag" : 4.803,
	"key" : 65433,
	"title" : "1 Puppis"
	},
{
	"Index" : "54049",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "W Puppis, HIP 37664, SAO 218932, HD 62713, GC 10425, HR 3002, DM CD-40  3377, TYC 7649-2744-1",
	"group" : { "key" : "Puppis" },
	"Common" : "W Puppis",
	"OType" : "High proper-motion Star",
	"Distance" : "66.52",
	"RA_S" : 115.92470406,
	"DEC_S" : -40.93374591,
	"Constellation" : "Puppis ",
	"AMag" : 5.241,
	"key" : 74049,
	"title" : "W Puppis"
	},
{
	"Index" : "45434",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "3 Puppis, l Puppis, HIP 37677, SAO 174400, HD 62623, GC 10417, HR 2996, DM CD-28  4774, TYC 6552-3228-1",
	"group" : { "key" : "Puppis" },
	"Common" : "l Puppis",
	"OType" : "Evolved supergiant star",
	"RA_S" : 115.95195301,
	"DEC_S" : -28.95482556,
	"Constellation" : "Puppis ",
	"AMag" : 3.987,
	"key" : 65434,
	"title" : "l Puppis"
	},
{
	"Index" : "53994",
	"Description" : "c Puppis (HD 63032, HR 3017) is a K4III orange giant star in the constellation Puppis with an apparent visual magnitude of 3.62 that lies at a distance of some 1,085 light years. c Puppis, which is found in the night sky between Naos and Nu Puppis, is the 335th brightest star in the Earth\u0027s sky, and 8th brightest in its constellation. It is located in the open cluster NGC 2451.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "c Puppis, HIP 37819, SAO 198398, HD 63032, GC 10462, HR 3017, DM CD-37  3863, TYC 7645-3246-1",
	"group" : { "key" : "Puppis" },
	"Common" : "C Puppis",
	"OType" : "Star",
	"Distance" : "332.96",
	"RA_S" : 116.31373632,
	"DEC_S" : -37.96858216,
	"X" : 246,
	"Y" : 423,
	"Constellation" : "Puppis ",
	"AMag" : 3.806,
	"key" : 73994,
	"title" : "C Puppis"
	},
{
	"Index" : "49555",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "171 Puppis, HIP 37853, SAO 198404, HD 63077, GC 10473, HR 3018, DM CD-33  4113, TYC 7114-2950-1",
	"group" : { "key" : "Puppis" },
	"Common" : "171 Puppis",
	"OType" : "Double or multiple star",
	"Distance" : "15.21",
	"RA_S" : 116.39577259,
	"DEC_S" : -34.17244838,
	"Constellation" : "Puppis ",
	"AMag" : 5.426,
	"key" : 69555,
	"title" : "171 Puppis"
	},
{
	"Index" : "36912",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "4 Puppis, HIP 37891, SAO 153372, HD 62952, GC 10469, HR 3015, DM BD-14  2199, TYC 5422-3293-1",
	"group" : { "key" : "Puppis" },
	"Common" : "4 Puppis",
	"OType" : "Star",
	"Distance" : "71.91",
	"RA_S" : 116.48696206,
	"DEC_S" : -14.56380459,
	"Constellation" : "Puppis ",
	"AMag" : 5.065,
	"key" : 56912,
	"title" : "4 Puppis"
	},
{
	"Index" : "53995",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 38010, SAO 198442, HD 63465, GC 10523, HR 3035, DM CD-38 3650, TYC 7645-3247-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3035",
	"OType" : "Star",
	"Distance" : "329.33",
	"RA_S" : 116.85413308,
	"DEC_S" : -38.51114117,
	"Constellation" : "Puppis ",
	"AMag" : 5.05,
	"key" : 73995,
	"title" : "HR 3035"
	},
{
	"Index" : "58279",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 38020, SAO 219000, HD 63578, GC 10533, HR 3037, DM CD-46 3435, TYC 8134-3516-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3037",
	"OType" : "Spectroscopic binary",
	"Distance" : "476.49",
	"RA_S" : 116.881278,
	"DEC_S" : -46.6084904,
	"Constellation" : "Puppis ",
	"AMag" : 5.183,
	"key" : 78279,
	"title" : "HR 3037"
	},
{
	"Index" : "45334",
	"Description" : "Omicron Puppis (Omicron Pup, \u03BF Puppis, \u03BF Pup) is multiple star system in constellation of Puppis, with an apparent magnitude of +4.40. The primary component is a blue B-type subgiant. It is approximately 2470 light years from Earth.\r\rOmicron Puppis is moving through the Galaxy at a speed of 26.9 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,800 and 32,000 light years from the center of the Galaxy.\r\rOmicron Puppis came closest to the Sun 8.7 million years ago when it had brightened to magnitude 3.99 from a distance of 1,162 light years.\r\rOmicron Puppis (Omicron Pup, \u03BF Puppis, \u03BF Pup) is multiple star system in constellation of Puppis, with an apparent magnitude of +4.40. The primary component is a blue B-type subgiant. It is approximately 2470 light years from Earth.\r\rOmicron Puppis is moving through the Galaxy at a speed of 26.9 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,800 and 32,000 light years from the center of the Galaxy.\r\rOmicron Puppis came closest to the Sun 8.7 million years ago when it had brightened to magnitude 3.99 from a distance of 1,162 light years.\r\rIn Chinese, \u5F27\u77E2 (H\u00FA Sh\u01D0), meaning Bow and Arrow, refers to an asterism consisting of \u03BF Puppis, \u03B4 Canis Majoris, \u03B7 Canis Majoris, HD 63032, HD 65456, k Puppis, \u03B5 Canis Majoris, \u03BA Canis Majoris and \u03C0 Puppis. Consequently, \u03BF Puppis itself is known as \u5F27\u77E2\u4E94 (H\u00FA Sh\u01D0 w\u01D4, English: the Fifth Star of Bow and Arrow.)",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Omicron Puppis, HIP 38070, SAO 174558, HD 63462, GC 10532, HR 3034, DM CD-25  5081, TYC 6544-4213-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Omicron Puppis",
	"OType" : "Be Star",
	"Distance" : "429.63",
	"RA_S" : 117.02153497,
	"DEC_S" : -25.93717008,
	"X" : 230,
	"Y" : 267,
	"Constellation" : "Puppis ",
	"AMag" : 4.468,
	"key" : 65334,
	"title" : "Omicron Puppis"
	},
{
	"Index" : "58355",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Q Puppis, HIP 38089, SAO 219018, HD 63744, GC 10553, HR 3046, DM CD-46  3451, TYC 8138-3767-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Q Puppis",
	"OType" : "Star",
	"Distance" : "71.21",
	"RA_S" : 117.08400588,
	"DEC_S" : -47.07772394,
	"Constellation" : "Puppis ",
	"AMag" : 4.803,
	"key" : 78355,
	"title" : "Q Puppis"
	},
{
	"Index" : "45488",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "188 Puppis, HIP 38146, SAO 174592, HD 63660, GC 10556, HR 3043, DM CD-24  6022, TYC 6557-4523-1",
	"group" : { "key" : "Puppis" },
	"Common" : "188 Puppis",
	"OType" : "Double or multiple star",
	"Distance" : "85.24",
	"RA_S" : 117.2569858,
	"DEC_S" : -24.91220326,
	"Constellation" : "Puppis ",
	"AMag" : 5.397,
	"key" : 65488,
	"title" : "188 Puppis"
	},
{
	"Index" : "58278",
	"Description" : "HD 63922 is a blue giant star in the constellation Puppis. Its apparent magnitude is 4.09.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "P Puppis, HIP 38164AC, SAO 219035, HD 63922, GC 10576, HR 3055, DM CD-46  3458, TYC 8134-3515-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 63922",
	"OType" : "Double or multiple star",
	"Distance" : "493.21",
	"RA_S" : 117.30957174,
	"DEC_S" : -46.37320694,
	"X" : 243,
	"Y" : 532,
	"Constellation" : "Puppis ",
	"AMag" : 4.056,
	"key" : 78278,
	"title" : "HD 63922"
	},
{
	"Index" : "45487",
	"Description" : "Xi Puppis (Xi Pup, \u03BE Puppis, \u03BE Pup) is a star in the southern constellation of Puppis. With an apparent visual magnitude of 3.35, it is one of the brighter members of this constellation. It is a yellow supergiant. It has the traditional name Asmidiske (Azmidiske), a misplacement and mistransliteration of Aspidiske, the traditional name of \u03B9 Carinae. Based on parallax measurements made during the Hipparcos mission, it is located approximately 1,200 light-years (370 parsecs) away, with a 7.5% margin of error. Because of the distance of this star from the Earth, its visual magnitude is reduced by 0.73 as a result of extinction from the intervening gas and dust.\r\rAsmidiske has a 13th magnitude companion at an apparent distance of 5\u0022.1 while it may also be a spectroscopic binary.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "7 Puppis, Xi Puppis, HIP 38170, SAO 174601, HD 63700, GC 10562, HR 3045, DM CD-24  6030, TYC 6557-4522-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Asmidiske",
	"OType" : "Star",
	"Distance" : "365.04",
	"RA_S" : 117.32356494,
	"DEC_S" : -24.85978712,
	"X" : 227,
	"Y" : 253,
	"Constellation" : "Puppis ",
	"AMag" : 3.452,
	"key" : 65487,
	"shortTitle" : "Asmidiske (also applied to HD80404)",
	"title" : "Asmidiske"
	},
{
	"Index" : "41058",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "6 Puppis, HIP 38211, SAO 153454, HD 63697, GC 10569, HR 3044, DM BD-16  2146, TYC 5985-1590-1",
	"group" : { "key" : "Puppis" },
	"Common" : "6 Puppis",
	"OType" : "Star",
	"Distance" : "78.02",
	"RA_S" : 117.42167172,
	"DEC_S" : -17.22840648,
	"Constellation" : "Puppis ",
	"AMag" : 5.309,
	"key" : 61058,
	"title" : "6 Puppis"
	},
{
	"Index" : "36923",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "9 Puppis, HIP 38382AB, SAO 153500, HD 64096A, GC 10629, HR 3064, DM BD-13  2267, TYC 5423-3227-1",
	"group" : { "key" : "Puppis" },
	"Common" : "9 Puppis",
	"OType" : "Star",
	"Distance" : "16.5",
	"RA_S" : 117.94291196,
	"DEC_S" : -13.89799605,
	"Constellation" : "Puppis ",
	"AMag" : 5.263,
	"key" : 56923,
	"title" : "9 Puppis"
	},
{
	"Index" : "54066",
	"Description" : "HD 64440 (a Puppis, a Pup) is a multiple star system in the constellation Puppis. Its apparent magnitude is 3.72. Based on parallax measurements, it is around 352 light-years away. It is the 364th brightest star in the sky and the 9th brightest star in Puppis.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "a Puppis, HIP 38414, SAO 219082, HD 64440, GC 10655, HR 3080, DM CD-40  3579, TYC 7650-3052-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 64440",
	"OType" : "Spectroscopic binary",
	"Distance" : "107.07",
	"RA_S" : 118.05431952,
	"DEC_S" : -40.57578007,
	"X" : 230,
	"Y" : 458,
	"Constellation" : "Puppis ",
	"AMag" : 3.809,
	"key" : 74066,
	"title" : "HD 64440"
	},
{
	"Index" : "49720",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "212 Puppis, HIP 38423A, SAO 198540, HD 64379A, GC 10651, HR 3079, DM CD-34  4036, TYC 7127-2092-2",
	"group" : { "key" : "Puppis" },
	"Common" : "212 Puppis",
	"OType" : "Star",
	"Distance" : "17.94",
	"RA_S" : 118.0652769,
	"DEC_S" : -34.70544353,
	"Constellation" : "Puppis ",
	"AMag" : 5.118,
	"key" : 69720,
	"title" : "212 Puppis"
	},
{
	"Index" : "54015",
	"Description" : "QZ Puppis (QZ Pup, b Pup) is a star in the constellation Puppis. Its apparent magnitude is 4.48.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "b Puppis, HIP 38455, SAO 198545, HD 64503, GC 10661, HR 3084, DM CD-38  3769, TYC 7646-3591-1",
	"group" : { "key" : "Puppis" },
	"Common" : "QZ Puppis",
	"OType" : "Spectroscopic binary",
	"Distance" : "198.47",
	"RA_S" : 118.16102426,
	"DEC_S" : -38.86281541,
	"X" : 228,
	"Y" : 436,
	"Constellation" : "Puppis ",
	"AMag" : 4.445,
	"key" : 74015,
	"title" : "QZ Puppis"
	},
{
	"Index" : "58446",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 38500, SAO 219106, HD 64740, GC 10686, HR 3089, DM CD-49 3137, TYC 8143-3240-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3089",
	"OType" : "Star",
	"Distance" : "232.22",
	"RA_S" : 118.2651371,
	"DEC_S" : -49.613046,
	"Constellation" : "Puppis ",
	"AMag" : 4.574,
	"key" : 78446,
	"title" : "HR 3089"
	},
{
	"Index" : "58375",
	"Description" : "HD 64760 (J Puppis) is a star in the constellation Puppis. Its apparent magnitude is 4.23. It is a blue supergiant with a spectral type of B0.5Ib.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "J Puppis, HIP 38518, SAO 219111, HD 64760, GC 10689, HR 3090, DM CD-47  3396, TYC 8139-4578-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 64760",
	"OType" : "Star",
	"Distance" : "506.05",
	"RA_S" : 118.32565801,
	"DEC_S" : -48.10294218,
	"X" : 236,
	"Y" : 556,
	"Constellation" : "Puppis ",
	"AMag" : 4.203,
	"key" : 78375,
	"title" : "HD 64760"
	},
{
	"Index" : "49776",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 38593, SAO 198575, HD 64802, GC 10695, HR 3091, DM CD-35 4002, TYC 7131-2155-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3091",
	"OType" : "Star",
	"Distance" : "207.33",
	"RA_S" : 118.54586995,
	"DEC_S" : -35.87729007,
	"Constellation" : "Puppis ",
	"AMag" : 5.434,
	"key" : 69776,
	"title" : "HR 3091"
	},
{
	"Index" : "45447",
	"Description" : "11 Puppis (11 Pup) is a star in the constellation Puppis. Its apparent magnitude is 4.20.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "11 Puppis, j Puppis, HIP 38835, SAO 174852, HD 65228, GC 10756, HR 3102, DM BD-22  2087, TYC 6553-3890-1",
	"group" : { "key" : "Puppis" },
	"Common" : "11 Puppis",
	"OType" : "Star",
	"Distance" : "159.74",
	"RA_S" : 119.21474706,
	"DEC_S" : -22.88012318,
	"X" : 202,
	"Y" : 229,
	"Constellation" : "Puppis ",
	"AMag" : 4.265,
	"key" : 65447,
	"title" : "11 Puppis"
	},
{
	"Index" : "54166",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 38846, SAO 219189, HD 65460, GC 10765, HR 3114, DM CD-43 3758, TYC 7658-4642-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3114",
	"OType" : "Star",
	"Distance" : "462.26",
	"RA_S" : 119.24083553,
	"DEC_S" : -43.50040488,
	"Constellation" : "Puppis ",
	"AMag" : 5.319,
	"key" : 74166,
	"title" : "HR 3114"
	},
{
	"Index" : "54167",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "N Puppis, HIP 38872, SAO 219197, HD 65551, GC 10775, HR 3116, DM CD-43  3766, TYC 7658-4643-1",
	"group" : { "key" : "Puppis" },
	"Common" : "N Puppis",
	"OType" : "Star",
	"Distance" : "334.27",
	"RA_S" : 119.32676236,
	"DEC_S" : -44.1098649,
	"Constellation" : "Puppis ",
	"AMag" : 5.037,
	"key" : 74167,
	"title" : "N Puppis"
	},
{
	"Index" : "49639",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "Chi Puppis, HIP 38901, SAO 198636, HD 65456, GC 10774, HR 3113, DM CD-29  5236, TYC 7120-2422-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Chi Puppis",
	"OType" : "Variable Star",
	"Distance" : "368.79",
	"RA_S" : 119.41710751,
	"DEC_S" : -30.33456726,
	"Constellation" : "Puppis ",
	"AMag" : 4.793,
	"key" : 69639,
	"title" : "Chi Puppis"
	},
{
	"Index" : "58295",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "O Puppis, HIP 38917, SAO 219218, HD 65685, GC 10790, HR 3121, DM CD-45  3611, TYC 8135-3065-1",
	"group" : { "key" : "Puppis" },
	"Common" : "O Puppis",
	"OType" : "Star",
	"Distance" : "89.08",
	"RA_S" : 119.46549938,
	"DEC_S" : -45.57766701,
	"Constellation" : "Puppis ",
	"AMag" : 5.266,
	"key" : 78295,
	"title" : "O Puppis"
	},
{
	"Index" : "58445",
	"Description" : "V Puppis (V Pup) is a star system in the constellation Puppis. Its apparent magnitude is 4.45. There is a binary star system at the center with a B1 dwarf orbiting a B3 subgiant star. They have an orbital period of 1.45 days and a distance of only 15 solar radii apart. However, the system moves back and forth, indicating that there is a massive object orbiting them. Based on Kepler\u0027s Laws and the fact that the object is not visible, it is probably a black hole.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "V Puppis, HIP 38957, SAO 219226, HD 65818, GC 10802, HR 3129, DM CD-48  3349, TYC 8143-3239-1",
	"group" : { "key" : "Puppis" },
	"Common" : "V Puppis",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "404.25",
	"RA_S" : 119.56014788,
	"DEC_S" : -49.24491439,
	"X" : 227,
	"Y" : 571,
	"Constellation" : "Puppis ",
	"AMag" : 4.472,
	"key" : 78445,
	"title" : "V Puppis"
	},
{
	"Index" : "45457",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "12 Puppis, HIP 39023, SAO 174932, HD 65699, GC 10805, HR 3123, DM BD-22  2104, TYC 6554-3065-1",
	"group" : { "key" : "Puppis" },
	"Common" : "12 Puppis",
	"OType" : "Peculiar Star",
	"Distance" : "261.75",
	"RA_S" : 119.77380948,
	"DEC_S" : -23.31039419,
	"Constellation" : "Puppis ",
	"AMag" : 5.204,
	"key" : 65457,
	"title" : "12 Puppis"
	},
{
	"Index" : "54016",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 39061AB, SAO 198668, HD 65925, GC 10830, HR 3140, DM CD-38 3908, TYC 7646-3592-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3140",
	"OType" : "Star",
	"Distance" : "55.51",
	"RA_S" : 119.8681567,
	"DEC_S" : -39.2969253,
	"Constellation" : "Puppis ",
	"AMag" : 5.27,
	"key" : 74016,
	"title" : "HR 3140"
	},
{
	"Index" : "41070",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 39095, SAO 153687, HD 65810, GC 10825, HR 3131, DM BD-18 2118, TYC 5986-3435-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3131",
	"OType" : "Star",
	"Distance" : "73.77",
	"RA_S" : 119.96688603,
	"DEC_S" : -18.39922887,
	"Constellation" : "Puppis ",
	"AMag" : 4.618,
	"key" : 61070,
	"title" : "HR 3131"
	},
{
	"Index" : "54301",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 39360, SAO 219339, HD 66624, GC 10932, HR 3162, DM CD-40 3776, TYC 7667-5593-1",
	"group" : { "key" : "Puppis" },
	"Common" : "V* V336 Pup",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "146.84",
	"RA_S" : 120.68660027,
	"DEC_S" : -41.30982725,
	"Constellation" : "Puppis ",
	"AMag" : 5.475,
	"key" : 74301,
	"title" : "V* V336 Pup"
	},
{
	"Index" : "49686",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 39487, SAO 198764, HD 66888, GC 10960, HR 3170, DM CD-32 4796, TYC 7124-3767-1",
	"group" : { "key" : "Puppis" },
	"Common" : "V* MZ Pup",
	"OType" : "Red supergiant star",
	"Distance" : "623.32",
	"RA_S" : 121.06745437,
	"DEC_S" : -32.67483085,
	"Constellation" : "Puppis ",
	"AMag" : 5.432,
	"key" : 69686,
	"title" : "V* MZ Pup"
	},
{
	"Index" : "41236",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 39734, SAO 175206, HD 67456, GC 11027, HR 3183, DM BD-20 2395, TYC 6003-2954-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3183",
	"OType" : "Star",
	"Distance" : "461.2",
	"RA_S" : 121.82516728,
	"DEC_S" : -20.55434294,
	"Constellation" : "Puppis ",
	"AMag" : 5.35,
	"key" : 61236,
	"title" : "HR 3183"
	},
{
	"Index" : "45464",
	"Description" : "Rho Puppis (Rho Pup, \u03C1 Puppis, \u03C1 Pup) is a star in the southern constellation of Puppis, which according to British astronomy author Patrick Moore, has the traditional name Turais. With an average apparent visual magnitude of 2.78, it is the third brightest member of this generally faint constellation. Based upon parallax measurements made during the Hipparcos mission, Rho Puppis is located at a distance of 63.5 light-years (19.5 parsecs) from Earth. At present it is moving away from the Sun with a radial velocity of +46.1 km s\u20131. The closest approach occurred about 394,000 years ago when Rho Puppis came within roughly 11.6 ly (3.6 pc) of the Solar System; about the same distance as Procyon in the present era.\r\rThe variability of this star was announced in 1956 by American astronomer Olin J. Eggen. It was determined to be a Delta Scuti-type variable star, making it one of the first stars of that type to be identified. Photometric observations dating back to 1946 provide a lengthy record of its pattern of pulsation; it undergoes periodic pulsations with a single period of 0.14088143(3) days, or 7.1 cycles per day. During each cycle, the star\u0027s magnitude varies with an amplitude of 0.15 and the radial velocity varies by 10 km s\u20131. The peak brightness occurs 28.8 minutes following the minimum radial velocity. The outer atmosphere\u0027s effective temperature of 6,920 K is one of the lowest known for a Delta Scuti variable.\r\rRho Puppis has an estimated age of about 2 billion years and it has 3.4 times the Sun\u0027s radius. It has a stellar classification of F2mF5IIp, which matches the spectrum of an F-type bright giant star. It shows stronger than normal absorption lines of metals\u2014a term astronomers use for any element other than hydrogen and helium. The \u0027p\u0027 suffix indicates chemical peculiarities that mark it as a cooler temperature Am star. Most such stars are found in binary star systems, but this appears to be an exception as no companion has been discovered. Evolved stars that show this combination of Delta Scuti variability with Am-like peculiarities of abundance have come to be known as \u03C1 Pup stars. The star\u0027s metallicity is more than double that in the Sun.\r\rThis star shows an excess emission of infrared radiation, suggesting that there is a circumstellar disk of dust orbiting this star. The mean temperature of the emission is 85 K, corresponding to an orbital separation from the host star of 50 AU.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "15 Puppis, Rho Puppis, HIP 39757, SAO 175217, HD 67523, GC 11034, HR 3185, DM CD-23  6828, TYC 6555-3245-1",
	"group" : { "key" : "Puppis" },
	"Common" : "Turais",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "19.48",
	"RA_S" : 121.88603676,
	"DEC_S" : -24.30432443,
	"X" : 172,
	"Y" : 249,
	"Constellation" : "Puppis ",
	"AMag" : 2.842,
	"key" : 65464,
	"title" : "Turais"
	},
{
	"Index" : "41246",
	"Description" : "16 Puppis (16 Pup) is a blue (B4IV) subgiant star in the constellation of Puppis at 464 light years that shines with an vis mag of 4.39.\r\r16 Puppis is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "16 Puppis, HIP 39906, SAO 153890, HD 67797, GC 11071, HR 3192, DM BD-18  2190, TYC 6004-3719-1",
	"group" : { "key" : "Puppis" },
	"Common" : "16 Puppis",
	"OType" : "Star",
	"Distance" : "142.48",
	"RA_S" : 122.25681287,
	"DEC_S" : -19.24501484,
	"X" : 162,
	"Y" : 184,
	"Constellation" : "Puppis ",
	"AMag" : 4.368,
	"key" : 61246,
	"title" : "16 Puppis"
	},
{
	"Index" : "37012",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "19 Puppis, HIP 40084, SAO 153942, HD 68290, GC 11134, HR 3211, DM BD-12  2385, TYC 5434-3731-1",
	"group" : { "key" : "Puppis" },
	"Common" : "19 Puppis",
	"OType" : "Double or multiple star",
	"Distance" : "54.16",
	"RA_S" : 122.81794651,
	"DEC_S" : -12.92699606,
	"Constellation" : "Puppis ",
	"AMag" : 4.82,
	"key" : 57012,
	"title" : "19 Puppis"
	},
{
	"Index" : "54248",
	"Description" : "NS Puppis (NS Pup) is a star in the constellation Puppis. Its apparent magnitude is 4.44.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "h01 Puppis, HIP 40091, SAO 198908, HD 68553, GC 11149, HR 3225, DM CD-39  4084, TYC 7664-2481-1",
	"group" : { "key" : "Puppis" },
	"Common" : "NS Puppis",
	"OType" : "Long-period variable star",
	"Distance" : "500.86",
	"RA_S" : 122.83955809,
	"DEC_S" : -39.61854641,
	"X" : 182,
	"Y" : 450,
	"Constellation" : "Puppis ",
	"AMag" : 4.6,
	"key" : 74248,
	"title" : "NS Puppis"
	},
{
	"Index" : "54314",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 40096, SAO 219569, HD 68601, GC 11155, HR 3226, DM CD-42 3979, TYC 7668-3980-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3226",
	"OType" : "Star",
	"Distance" : "1234.33",
	"RA_S" : 122.85788828,
	"DEC_S" : -42.9872758,
	"Constellation" : "Puppis ",
	"AMag" : 4.768,
	"key" : 74314,
	"title" : "HR 3226"
	},
{
	"Index" : "41174",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "20 Puppis, HIP 40259, SAO 153993, HD 68752, GC 11184, HR 3229, DM BD-15  2324, TYC 5996-2764-1",
	"group" : { "key" : "Puppis" },
	"Common" : "20 Puppis",
	"OType" : "Star",
	"Distance" : "264.63",
	"RA_S" : 123.33319906,
	"DEC_S" : -15.78822208,
	"Constellation" : "Puppis ",
	"AMag" : 5.107,
	"key" : 61174,
	"title" : "20 Puppis"
	},
{
	"Index" : "49830",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "r Puppis, HIP 40274, SAO 198957, HD 68980, GC 11197, HR 3237, DM CD-35  4349, TYC 7133-4588-1",
	"group" : { "key" : "Puppis" },
	"Common" : "r Puppis",
	"OType" : "Be Star",
	"Distance" : "354.15",
	"RA_S" : 123.372991,
	"DEC_S" : -35.89951463,
	"Constellation" : "Puppis ",
	"AMag" : 4.744,
	"key" : 69830,
	"title" : "r Puppis"
	},
{
	"Index" : "49819",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 40321, SAO 198969, HD 69081, GC 11208, HR 3240, DM CD-35 4358, TYC 7133-4552-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR  3240",
	"OType" : "Be Star",
	"Distance" : "354.99",
	"RA_S" : 123.49296824,
	"DEC_S" : -36.32227843,
	"Constellation" : "Puppis ",
	"AMag" : 5.032,
	"key" : 69819,
	"title" : "HR  3240"
	},
{
	"Index" : "54249",
	"Description" : "HD 69142 is an orange giant star in the constellation Puppis. Its apparent magnitude is 4.43.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "h02 Puppis, HIP 40326, SAO 219635, HD 69142, GC 11215, HR 3243, DM CD-39  4128, TYC 7664-2482-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 69142",
	"OType" : "Spectroscopic binary",
	"Distance" : "91.28",
	"RA_S" : 123.51217475,
	"DEC_S" : -40.34789127,
	"X" : 176,
	"Y" : 459,
	"Constellation" : "Puppis ",
	"AMag" : 4.55,
	"key" : 74249,
	"title" : "HD 69142"
	},
{
	"Index" : "49850",
	"Description" : "HD 70060 is a star in the constellation Puppis. Its apparent magnitude is 4.40.",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "q Puppis, HIP 40706, SAO 199070, HD 70060, GC 11343, HR 3270, DM CD-36  4449, TYC 7134-2967-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HD 70060",
	"OType" : "Star",
	"Distance" : "28.63",
	"RA_S" : 124.63880469,
	"DEC_S" : -36.65928895,
	"X" : 159,
	"Y" : 413,
	"Constellation" : "Puppis ",
	"AMag" : 4.46,
	"key" : 69850,
	"title" : "HD 70060"
	},
{
	"Index" : "49844",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 40943, SAO 199119, HD 70556, GC 11402, HR 3283, DM CD-36 4513, TYC 7134-2734-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3283",
	"OType" : "Star",
	"Distance" : "478.33",
	"RA_S" : 125.33769047,
	"DEC_S" : -36.48417813,
	"Constellation" : "Puppis ",
	"AMag" : 5.144,
	"key" : 69844,
	"title" : "HR 3283"
	},
{
	"Index" : "49715",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "w Puppis, HIP 40945, SAO 199118, HD 70555, GC 11400, HR 3282, DM CD-32  5185, TYC 7126-3938-1",
	"group" : { "key" : "Puppis" },
	"Common" : "w Puppis",
	"OType" : "Star",
	"Distance" : "306.45",
	"RA_S" : 125.3459427,
	"DEC_S" : -33.05436579,
	"Constellation" : "Puppis ",
	"AMag" : 4.983,
	"key" : 69715,
	"title" : "w Puppis"
	},
{
	"Index" : "45603",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 41260, SAO 175783, HD 71176, GC 11491, HR 3315, DM CD-23 7277, TYC 6569-4890-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3315",
	"OType" : "Star",
	"Distance" : "143.15",
	"RA_S" : 126.26557883,
	"DEC_S" : -24.04620819,
	"Constellation" : "Puppis ",
	"AMag" : 5.479,
	"key" : 65603,
	"title" : "HR 3315"
	},
{
	"Index" : "54332",
	"MapNum" : "17",
	"ImageNum" : "17",
	"Desig" : "HIP 41323, SAO 219910, HD 71459, GC 11532, HR 3326, DM CD-41 4119, TYC 7669-3846-1",
	"group" : { "key" : "Puppis" },
	"Common" : "HR 3326",
	"OType" : "Star",
	"Distance" : "219.75",
	"RA_S" : 126.46629224,
	"DEC_S" : -42.1530747,
	"Constellation" : "Puppis ",
	"AMag" : 5.415,
	"key" : 74332,
	"title" : "HR 3326"
	},
{
	"Index" : "41263",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 41817AB, SAO 154359, HD 72310, GC 11679, HR 3367, DM BD-19 2438, TYC 6006-4297-1",
	"group" : { "backgroundImage" : "images/Alignment/02.png",
		"description" : "Pyxis (pron.: /\u02C8p\u026Aks\u0268s/; Greek: box) is a small and faint constellation in the southern sky. Its name is Latin for a mariner\u0027s compass (it should not be confused with Circinus, which represents a draftsman\u0027s compasses). Pyxis is completely visible from latitudes south of 53 degrees north, with its best evening-sky visibility in January through March. The brightest star is Alpha Pyxidis at magnitude 3.68.\r\rPyxis was introduced by Nicolas Louis de Lacaille in the 18th century; he called it Pyxis Nautica, but the name was shortened. The constellation is located close to those forming the old constellation of Argo Navis (the ship Argo), and in the 19th century astronomer John Herschel suggested renaming Pyxis to \u0027Malus, the mast\u0027, but the suggestion was not followed.\r\rThe French astronomer Nicolas Louis de Lacaille first described the constellation as la Boussole (the Marine Compass) and gave Bayer designations to ten stars now named Alpha to Lambda Pyxidis (he skipped the Greek letter iota). Contrary to popular belief, these stars were not eked out of the old large constellation Argo Navis. He labelled it Pyxis Nautica on his 1763 chart. Francis Baily renamed it Malus the mast, but Benjamin Gould restored its original name. Johann Bode created the constellation Lochium Funis, the Log and Line, around Pyxis but this did not survive.\r\rIn ancient Chinese astronomy, Alpha, Beta and Gamma Pyxidis formed part of Tianmiao a Celestial Temple honouring the ancestors of the Emperor, along with stars from neighbouring Antlia.",
		"key" : "Pyxis",
		"grouptype" : "Pyxis",
		"Meaning" : "mariner's compass",
		"Family" : "Heavenly Waters",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Pyxis",
		"title" : "Pyxis Objects Group" },
	"Common" : "HR  3367",
	"OType" : "Star",
	"Distance" : "105.31",
	"RA_S" : 127.87884188,
	"DEC_S" : -19.57746987,
	"Constellation" : "Pyxis ",
	"AMag" : 5.415,
	"key" : 61263,
	"title" : "HR  3367"
	},
{
	"Index" : "45668",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Eta Pyxidis, HIP 42334, SAO 176189, HD 73495, GC 11848, HR 3420, DM CD-25  6356, TYC 6578-2618-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Eta Pyxidis",
	"OType" : "Star",
	"Distance" : "71.05",
	"RA_S" : 129.46729961,
	"DEC_S" : -26.255002,
	"Constellation" : "Pyxis ",
	"AMag" : 5.235,
	"key" : 65668,
	"title" : "Eta Pyxidis"
	},
{
	"Index" : "45613",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42430A, SAO 176226, HD 73752A, HR 3430, DM BD-22 2345, TYC 6571-3298-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "HD  73752A",
	"OType" : "High proper-motion Star",
	"Distance" : "19.4",
	"RA_S" : 129.78295342,
	"DEC_S" : -22.66183371,
	"Constellation" : "Pyxis ",
	"AMag" : 5.372,
	"key" : 65613,
	"title" : "HD  73752A"
	},
{
	"Index" : "45727",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Zeta Pyxidis, HIP 42483, SAO 176253, HD 73898, GC 11907, HR 3433, DM CD-29  6544, TYC 6583-2588-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Zeta Pyxidis",
	"OType" : "High proper-motion Star",
	"Distance" : "74.88",
	"RA_S" : 129.92697575,
	"DEC_S" : -29.5610888,
	"Constellation" : "Pyxis ",
	"AMag" : 4.973,
	"key" : 65727,
	"title" : "Zeta Pyxidis"
	},
{
	"Index" : "49961",
	"Description" : "Beta Pyxidis (Beta Pyx, \u03B2 Pyxidis, \u03B2 Pyx) is a double star located in the southern constellation Pyxis. It has an apparent visual magnitude of 3.954, making it the second brightest star in this faint constellation.\r\rBased upon parallax measurements, this star is an estimated 420 light-years (128 parsecs) from the Earth. The spectrum matches a bright giant or supergiant star of stellar classification G7Ib-II. The interferometer-measured angular diameter of this star is 2.05 \u00B1 0.14 mas. At its estimated distance, this yields a physical size of about 28 times the radius of the Sun. The effective temperature of the star\u0027s outer envelope is about 5,400 K, giving it the characteristic yellow hue of a G-type star.\r\rIn 2010, this star was among a survey of massive, lower effective temperature supergiants in an attempt to detect a magnetic field. This star may have a longitudinal magnetic field with a strength of less than a Gauss. It is a young disk star system with space velocity components, [U, V, W] = [\u201311.0, +11.8, \u20132.2] km/s. There is a magnitude 12.5 optical companion, located at an angular separation of 12.7 arcseconds and a position angle of 118\u00B0 as of the year 1943.\r\rIn Chinese, \u5929\u72D7 (Ti\u0101n G\u01D2u), meaning Celestial Dog, refers to an asterism consisting of \u03B2 Pyxidis, e Velorum, f Velorum, \u03B1 Pyxidis, \u03B3 Pyxidis and \u03B4 Pyxidis. Consequently, \u03B2 Pyxidis itself is known as \u5929\u72D7\u56DB (Ti\u0101n G\u01D2u s\u00EC, English: the Fourth Star of Celestial Dog.)",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Beta Pyxidis, HIP 42515, SAO 199490, HD 74006, GC 11923, HR 3438, DM CD-34  5128, TYC 7144-3639-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Beta Pyxidi",
	"OType" : "Star",
	"Distance" : "127.46",
	"RA_S" : 130.02559453,
	"DEC_S" : -35.30835275,
	"X" : 483,
	"Y" : 267,
	"Constellation" : "Pyxis ",
	"AMag" : 4.057,
	"key" : 69961,
	"title" : "Beta Pyxidi"
	},
{
	"Index" : "49924",
	"Description" : "Alpha Pyxidis (Alpha Pyx, \u03B1 Pyxidis, \u03B1 Pyx) is a giant star in the constellation Pyxis. It has a stellar classification of B1.5III and is a Beta Cephei variable. This star has more than ten times the mass of the Sun and is more than six times the Sun\u0027s radius. The surface temperature is 24,300 K and the star is about 10,000 times as luminous as the Sun. Stars such as this with more than 10 solar masses are expected to end their life by exploding as a supernova.\r\rIn Chinese, \u5929\u72D7 (Ti\u0101n G\u01D2u), meaning Celestial Dog, refers to an asterism consisting of \u03B1 Pyxidis, e Velorum, f Velorum, \u03B2 Pyxidis, \u03B3 Pyxidis and \u03B4 Pyxidis. Consequently, \u03B1 Pyxidis itself is known as \u5929\u72D7\u4E94 (Ti\u0101n G\u01D2u w\u01D4, English: the Fifth Star of Celestial Dog.)",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Alpha Pyxidis, HIP 42828, SAO 199546, HD 74575, GC 12018, HR 3468, DM CD-32  5651, TYC 7141-2725-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Alpha Pyxidis",
	"OType" : "Variable Star",
	"Distance" : "269.08",
	"RA_S" : 130.89807119,
	"DEC_S" : -33.18638549,
	"X" : 478,
	"Y" : 238,
	"Constellation" : "Pyxis ",
	"AMag" : 3.631,
	"key" : 69924,
	"title" : "Alpha Pyxidis"
	},
{
	"Index" : "49920",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 43352, SAO 199678, HD 75605, GC 12195, HR 3512, DM CD-32 5770, TYC 7141-2513-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "HR 3512",
	"OType" : "Variable Star",
	"Distance" : "68.34",
	"RA_S" : 132.4645885,
	"DEC_S" : -32.78052461,
	"Constellation" : "Pyxis ",
	"AMag" : 5.29,
	"key" : 69920,
	"title" : "HR 3512"
	},
{
	"Index" : "45687",
	"Description" : "Gamma Pyxidis (Gamma Pyx, \u03B3 Pyxidis, \u03B3 Pyx) is a 4th magnitude star in the constellation Pyxis. It is classified as a giant star of composition similar to the Sun and is located an estimated 209 light years from the Solar System.\r\rGamma Pyxidis is moving through the Galaxy at a speed of 54.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 21,300 and 30,700 light years from the center of the Galaxy.\r\rIn Chinese, \u5929\u72D7 (Ti\u0101n G\u01D2u), meaning Celestial Dog, refers to an asterism consisting of \u03B3 Pyxidis, e Velorum, f Velorum, \u03B2 Pyxidis, \u03B1 Pyxidis and \u03B4 Pyxidis. Consequently, \u03B3 Pyxidis itself is known as \u5929\u72D7\u516D (Ti\u0101n G\u01D2u li\u00F9, English: the Sixth Star of Celestial Dog.)",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Gamma Pyxidis, HIP 43409, SAO 176559, HD 75691, GC 12216, HR 3518, DM CD-27  5986, TYC 6580-2781-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Gamma Pyxidis",
	"OType" : "Star",
	"Distance" : "63.56",
	"RA_S" : 132.63301493,
	"DEC_S" : -27.7098454,
	"X" : 467,
	"Y" : 165,
	"Constellation" : "Pyxis ",
	"AMag" : 4.158,
	"key" : 65687,
	"title" : "Gamma Pyxidis"
	},
{
	"Index" : "45686",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Delta Pyxidis, HIP 43825, SAO 176697, HD 76483, GC 12343, HR 3556, DM CD-27  6072, TYC 6580-2780-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Delta Pyxidis",
	"OType" : "Star",
	"Distance" : "69.27",
	"RA_S" : 133.88153371,
	"DEC_S" : -27.68186339,
	"Constellation" : "Pyxis ",
	"AMag" : 4.884,
	"key" : 65686,
	"title" : "Delta Pyxidis"
	},
{
	"Index" : "45779",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Kappa Pyxidis, HIP 44824, SAO 177002, HD 78541, GC 12614, HR 3628, DM CD-25  6895, TYC 6590-2180-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Kappa Pyxidis",
	"OType" : "Star",
	"Distance" : "170",
	"RA_S" : 137.01200535,
	"DEC_S" : -25.85853921,
	"Constellation" : "Pyxis ",
	"AMag" : 4.784,
	"key" : 65779,
	"title" : "Kappa Pyxidis"
	},
{
	"Index" : "45795",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Theta Pyxidis, HIP 45902, SAO 177322, HD 80874, GC 12916, HR 3718, DM CD-25  7114, TYC 6592-2420-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Theta Pyxidis",
	"OType" : "Star",
	"Distance" : "153.2",
	"RA_S" : 140.37329667,
	"DEC_S" : -25.96543915,
	"Constellation" : "Pyxis ",
	"AMag" : 4.905,
	"key" : 65795,
	"title" : "Theta Pyxidis"
	},
{
	"Index" : "45857",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Lambda Pyxidis, HIP 46026, SAO 177374, HD 81169, GC 12952, HR 3733, DM CD-28  7196, TYC 6600-2227-1",
	"group" : { "key" : "Pyxis" },
	"Common" : "Lambda Pyxidis",
	"OType" : "Star",
	"Distance" : "58.88",
	"RA_S" : 140.80106324,
	"DEC_S" : -28.83388113,
	"Constellation" : "Pyxis ",
	"AMag" : 4.814,
	"key" : 65857,
	"title" : "Lambda Pyxidis"
	},
{
	"Index" : "65513",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Zeta02 Reticuli, HIP 15371, SAO 248774, HD 20807, GC 3975, HR 1010, DM CP-62   265, TYC 8863-1557-1",
	"group" : { "backgroundImage" : "images/Alignment/23.png",
		"description" : "Reticulum is a small, faint constellation in the southern sky. Its name is Latin for a small net, or reticle\u2014a net of crosshairs at the focus of a telescope eyepiece that is used to measure star positions. The constellation is best viewed between October and December, but cannot be seen from middle to northern latitudes.\r\rThis constellation was introduced by Isaac Habrecht II in his celestial globe in 1621, who named it Rhombus. It was later renamed by the French astronomer Nicolas Louis de Lacaille in the eighteenth century; during his stay at the Cape of Good Hope, he named the constellation le R\u00E9ticule Rhomboide to commemorate the reticle in his telescope eyepiece. It was later Latinized to Reticulum in his star catalogue Coelum Australe Stelliferum. In 1810, the stars of Reticulum were used by William Croswell to produce the constellation Marmor Sculptile, which represented the bust of Christopher Columbus, but this did not catch on among astronomers.\r\rThe constellation Reticulum became officially recognized during the First General Assembly of the International Astronomical Union in 1922. The boundary for this and other constellations was drawn up by Belgian astronomer Eug\u00E8ne Delporte along arcs of right ascension and declination for epoch 1875. These were published in 1930 in the Delimination Scientifique des Constellations at the behest of the IAU.",
		"key" : "Reticulum",
		"grouptype" : "Reticulum",
		"Meaning" : "eyepiece graticule",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Reticulum",
		"title" : "Reticulum Objects Group" },
	"Common" : "Zeta02 Reticuli",
	"OType" : "Double or multiple star",
	"Distance" : "12.03",
	"RA_S" : 49.55341052,
	"DEC_S" : -62.50636244,
	"Constellation" : "Reticulum ",
	"AMag" : 5.296,
	"key" : 85513,
	"title" : "Zeta02 Reticuli"
	},
{
	"Index" : "65573",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Kappa Reticuli, HIP 16245, SAO 248819, HD 22001, GC 4200, HR 1083, DM CP-63   234, TYC 8870-1384-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Kappa Reticuli",
	"OType" : "High proper-motion Star",
	"Distance" : "21.68",
	"RA_S" : 52.34448534,
	"DEC_S" : -62.93752503,
	"Constellation" : "Reticulum ",
	"AMag" : 4.75,
	"key" : 85573,
	"title" : "Kappa Reticuli"
	},
{
	"Index" : "65574",
	"Description" : "Beta Reticuli (Beta Ret, \u03B2 Reticuli, \u03B2 Ret) is triple star system and spectroscopic binary in constellation of Reticulum, with an apparent magnitude of +3.84. The primary component is an orange K-type giant. It is approximately 100 light years from Earth.\r\rBeta Reticuli is moving through the Galaxy at a speed of 69.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 10,100 and 24,200 light years from the center of the Galaxy.\r\rBeta Reticuli came closest to the Sun 319,000 years ago when it had brightened to magnitude 2.98 from a distance of 67 light years.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Beta Reticuli, HIP 17440, SAO 248877, HD 23817, GC 4517, HR 1175, DM CP-65   263, TYC 8870-1385-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Beta Reticuli",
	"OType" : "Spectroscopic binary",
	"Distance" : "30.56",
	"RA_S" : 56.04991539,
	"DEC_S" : -64.80689293,
	"X" : 413,
	"Y" : 453,
	"Constellation" : "Reticulum ",
	"AMag" : 3.959,
	"key" : 85574,
	"title" : "Beta Reticuli"
	},
{
	"Index" : "65551",
	"Description" : "Delta Reticuli (Delta Ret, \u03B4 Reticuli, \u03B4 Ret) is a red M-type giant with an apparent magnitude of +4.56. It is approximately 530 light years from Earth.\r\rDelta Reticuli is moving through the Galaxy at a speed of 13.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 22,700 and 30,400 light years from the center of the Galaxy.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Delta Reticuli, HIP 18597, SAO 248918, HD 25422, GC 4808, HR 1247, DM CP-61   290, TYC 8868-1318-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Delta Reticuli",
	"OType" : "Variable Star",
	"Distance" : "160.98",
	"RA_S" : 59.68645509,
	"DEC_S" : -61.40018254,
	"X" : 404,
	"Y" : 404,
	"Constellation" : "Reticulum ",
	"AMag" : 4.74,
	"key" : 85551,
	"title" : "Delta Reticuli"
	},
{
	"Index" : "65560",
	"Description" : "Gamma Reticuli (Gamma Ret, \u03B3 Reticuli, \u03B3 Ret) is a red M-type giant with an apparent magnitude of +4.48. It is approximately 490 light years from Earth.\r\rGamma Reticuli is moving through the Galaxy at a speed of 24.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,100 and 39,200 light years from the center of the Galaxy.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Gamma Reticuli, HIP 18744, SAO 248925, HD 25705, GC 4855, HR 1264, DM CP-62   312, TYC 8868-2193-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Gamma Reticuli",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "143.84",
	"RA_S" : 60.22419433,
	"DEC_S" : -62.15927854,
	"X" : 399,
	"Y" : 413,
	"Constellation" : "Reticulum ",
	"AMag" : 4.7,
	"key" : 85560,
	"title" : "Gamma Reticuli"
	},
{
	"Index" : "65561",
	"Description" : "Iota Reticuli (Iota Ret, \u03B9 Reticuli, \u03B9 Ret) is an orange K-type giant with an apparent magnitude of +4.97. It is approximately 331 light years from Earth.\r\rIota Reticuli is moving through the Galaxy at a speed of 80.9 km/s relative to the Sun. Its projected Galactic orbit carries it between 12,300 and 25,100 light years from the center of the Galaxy.\r\rIota Reticuli came closest to the Sun 883,000 years ago when it had brightened to magnitude 4.08 from a distance of 212 light years.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Iota Reticuli, HIP 18772, SAO 248927, HD 25728, GC 4861, HR 1266, DM CP-61   293, TYC 8868-2221-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Iota Reticuli",
	"OType" : "Star",
	"Distance" : "97.82",
	"RA_S" : 60.32562661,
	"DEC_S" : -61.07882052,
	"X" : 401,
	"Y" : 399,
	"Constellation" : "Reticulum ",
	"AMag" : 5.12,
	"key" : 85561,
	"title" : "Iota Reticuli"
	},
{
	"Index" : "65567",
	"Description" : "Alpha Reticuli (Alpha Ret, \u03B1 Reticuli, \u03B1 Ret) is the Bayer designation the brightest star in the southern circumpolar constellation of Reticulum, with an apparent visual magnitude of 3.3. This appears to be a solitary star located at a distance of 162 light-years from Earth. Although it is bright enough to be seen with the naked eye, the declination of this star means that it is best viewed from the southern hemisphere and is only readily visible below the tropic of cancer.\r\rThis star has more than three times the mass of the Sun and is about 330 million years old. The spectrum of this star matches a stellar classification of G8 II-III, with the luminosity class notation \u0027II-III\u0027 indicating it shows some traits of both a giant star and a bright giant. At this evolutionary stage, the atmosphere has expanded to almost thirteen times the radius of the Sun and the outer envelope has an effective temperature of 5,196 K. X-ray emission has been detected from this star, with an estimated luminosity of 3 \u00D7 1029 erg s\u20131.\r\rAlpha Reticuli has a 12th-magnitude visual companion, CCDM J04144-6228B, at an angular separation of 48 arcseconds away along a position angle of 355\u00B0. Since the two stars share a common proper motion across the celestial sphere, it is possible that Alpha Reticuli, rather than being solitary, may instead be the primary component of a binary star system with an orbital period is at least 60,000 years.\r\rIn Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, \u593E\u767D (Ji\u00E1 B\u00E1i), meaning White Patches Attached, refers to an asterism consisting of \u03B1 Reticuli and \u03B8 Doradus. Consequently, \u03B1 Reticuli itself is known as \u593E\u767D\u4E8C (Ji\u00E1 B\u00E1i \u00E8r, English: the Second Star of White Patches Attached.)",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Alpha Reticuli, HIP 19780, SAO 248969, HD 27256, GC 5164, HR 1336, DM CP-62   332, TYC 8869-2461-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Alpha Reticuli",
	"OType" : "Star",
	"Distance" : "49.55",
	"RA_S" : 63.60618243,
	"DEC_S" : -62.47386074,
	"X" : 378,
	"Y" : 413,
	"Constellation" : "Reticulum ",
	"AMag" : 3.425,
	"key" : 85567,
	"title" : "Alpha Reticuli"
	},
{
	"Index" : "61861",
	"Description" : "Epsilon Reticuli (Epsilon Ret, \u03B5 Reticuli, \u03B5 Ret) is a double star approximately 59 light-years away in the constellation of Reticulum. The primary component is an orange subgiant star, while the secondary is a white dwarf star. The two stars share a common motion through space and hence most likely form a binary star system. The brighter star should be easily visible without optical aid under dark skies in the southern hemisphere. In 2000, an extrasolar planet was confirmed to be orbiting the primary star in the system.",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Epsilon Reticuli, HIP 19921, SAO 233463, HD 27442A, GC 5194, HR 1355, DM CP-59   324, TYC 8508-2041-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Epsilon Reticuli",
	"OType" : "Star",
	"Distance" : "18.24",
	"RA_S" : 64.12095133,
	"DEC_S" : -59.30215392,
	"X" : 382,
	"Y" : 372,
	"Constellation" : "Reticulum ",
	"AMag" : 4.554,
	"key" : 81861,
	"title" : "Epsilon Reticuli"
	},
{
	"Index" : "65594",
	"MapNum" : "23",
	"ImageNum" : "23",
	"Desig" : "Eta Reticuli, HIP 20384, SAO 249009, HD 28093, GC 5333, HR 1395, DM CP-63   324, TYC 8872-1983-1",
	"group" : { "key" : "Reticulum" },
	"Common" : "Eta Reticuli",
	"OType" : "High proper-motion Star",
	"Distance" : "117.86",
	"RA_S" : 65.47218705,
	"DEC_S" : -63.38639156,
	"Constellation" : "Reticulum ",
	"AMag" : 5.341,
	"key" : 85594,
	"title" : "Eta Reticuli"
	},
{
	"Index" : "5020",
	"Description" : "Alpha Sagittae (Alpha Sge, \u03B1 Sagittae, \u03B1 Sge) is a star in the constellation Sagitta. It has the traditional name Sham or Alsahm which comes to us from Arabic \u0633\u0647\u0645 sahm and means Arrow, the name formerly having been applied to the whole constellation. Alpha Sagittae is the third brightest star and is four times more massive and 340 times brighter than the Sun.\r\rIn Chinese, \u5DE6\u65D7 (Zu\u01D2 Q\u00ED), meaning Left Flag, refers to an asterism consisting of \u03B1 Sagittae, \u03B2 Sagittae, \u03B4 Sagittae, \u03B6 Sagittae, \u03B3 Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and \u03C1 Aquilae. Consequently, \u03B1 Sagittae itself is known as \u5DE6\u65D7\u4E00 (Zu\u01D2 Q\u00ED y\u012B, English: the First Star of Left Flag.)\r\r\u03B1 Sge is a yellow bright giant star of apparent magnitude +4.37 and spectral class G1 II about 475 light years from Earth. It has a luminosity 340 times that of the Sun with a surface temperature of 5,333 K. The star\u0027s radius is roughly 20 times solar while its mass is 4 times the solar mass.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "5 Sagittae, Alpha Sagittae, HIP 96757, SAO 105120, HD 185758, GC 27215, HR 7479, DM BD+17  4042, TYC 1606-2341-1",
	"group" : { "backgroundImage" : "images/Alignment/22.png",
		"description" : "Sagitta is a constellation. Its name is Latin for \u0022arrow\u0022, and it should not be confused with the larger constellation Sagittarius, the archer. Although Sagitta is an ancient constellation, it has no star brighter than 3rd magnitude and has the third-smallest area of all constellations (only Equuleus and Crux are smaller). It was included among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations defined by the International Astronomical Union. Located to the north of the equator, Sagitta can be seen from every location on Earth except within the Antarctic circle.\r\rSagitta lies within the Milky Way and is bordered by the following constellations (beginning at the north and then continuing clockwise): the little fox Vulpecula, the mythological hero Hercules, the eagle Aquila and the dolphin Delphinus.\r\rThe Greeks who may have originally identified this constellation called it Oistos. The Romans named it Sagitta.\r\rJohann Bayer chose to name the stars in Sagitta in a non-brightness order, in this case giving the brightest star a designation of \u03B3. Another example of such a deviation from the usual brightness order is the constellation Sagittarius.\r\rIn ancient Greece, Sagitta was regarded as the weapon that Hercules used to kill the eagle (Aquila) of Jove that perpetually gnawed Prometheus\u0027 liver. The Arrow is located beyond the north border of Aquila, the Eagle. Others believe the Arrow to be the one shot by Hercules towards the adjacent Stymphalian birds (6th labor) who had claws, beaks and wings of iron, and who lived on human flesh in the marshes of Arcadia - Aquila the Eagle and Cygnus the Swan, and the Vulture - and still lying between them, whence the title Herculea. Eratosthenes claimed it as the arrow with which Apollo exterminated the Cyclopes.",
		"key" : "Sagitta",
		"grouptype" : "Sagitta",
		"Meaning" : "arrow",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Sagitta",
		"title" : "Sagitta Objects Group" },
	"Common" : "Sham / Alsahm",
	"OType" : "Star",
	"Distance" : "130.23",
	"RA_S" : 295.02413159,
	"DEC_S" : 18.01389215,
	"X" : 555,
	"Y" : 561,
	"Constellation" : "Sagitta ",
	"AMag" : 4.458,
	"key" : 25020,
	"shortTitle" : "Alsahm",
	"title" : "Sham / Alsahm"
	},
{
	"Index" : "5021",
	"Description" : "Beta Sagittae (Beta Sge, \u03B2 Sagittae, \u03B2 Sge) is a G-type giant star in the constellation of Sagitta. It has an apparent visual magnitude of approximately 4.387.\r\rBeta Sagittae projected Galactic orbit carries it between 18,400 and 24,100 light years from the center of the Galaxy.\r\rBeta Sagittae will come closest to the Sun 3.0 million years from now when it will brighten to magnitude 3.64 from a distance of 310 light years.\r\rIn Chinese, \u5DE6\u65D7 (Zu\u01D2 Q\u00ED), meaning Left Flag, refers to an asterism consisting of \u03B2 Sagittae, \u03B1 Sagittae, \u03B4 Sagittae, \u03B6 Sagittae, \u03B3 Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and \u03C1 Aquilae. Consequently, \u03B2 Sagittae itself is known as \u5DE6\u65D7\u4E8C (Zu\u01D2 Q\u00ED \u00E8r, English: the Second Star of Left Flag.)",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "6 Sagittae, Beta Sagittae, HIP 96837, SAO 105133, HD 185958, GC 27236, HR 7488, DM BD+17  4048, TYC 1606-2342-1",
	"group" : { "key" : "Sagitta" },
	"Common" : "Beta Sagittae",
	"OType" : "Star",
	"Distance" : "134.57",
	"RA_S" : 295.26224442,
	"DEC_S" : 17.47604483,
	"X" : 552,
	"Y" : 568,
	"Constellation" : "Sagitta ",
	"AMag" : 4.488,
	"key" : 25021,
	"title" : "Beta Sagittae"
	},
{
	"Index" : "5199",
	"Description" : "Delta Sagittae (Delta Sge, \u03B4 Sagittae, \u03B4 Sge) is a multiple star system in the constellation of Sagitta, with an apparent magnitude of +3.68. The primary component is a red M-type bright giant. It is approximately 448 light years from Earth.\r\rDelta Sagittae is moving through the Galaxy at a speed of 9.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 35,300 light years from the center of the Galaxy.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "7 Sagittae, Delta Sagittae, HIP 97365AB, SAO 105259, HD 187076J, GC 27391, HR 7536, DM BD+18  4240A, TYC 1619-3542-1",
	"group" : { "key" : "Sagitta" },
	"Common" : "Delta Sagittae",
	"OType" : "Spectroscopic binary",
	"Distance" : "178.47",
	"RA_S" : 296.8469495,
	"DEC_S" : 18.53428307,
	"X" : 530,
	"Y" : 557,
	"Constellation" : "Sagitta ",
	"AMag" : 3.956,
	"key" : 25199,
	"title" : "Delta Sagittae"
	},
{
	"Index" : "5255",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "8 Sagittae, Zeta Sagittae, HIP 97496AB, SAO 105298, HD 187362, GC 27431, HR 7546, DM BD+18  4254, TYC 1623-2647-1",
	"group" : { "key" : "Sagitta" },
	"Common" : "Zeta Sagittae",
	"OType" : "Double or multiple star",
	"Distance" : "77.93",
	"RA_S" : 297.24441561,
	"DEC_S" : 19.14204156,
	"Constellation" : "Sagitta ",
	"AMag" : 5.044,
	"key" : 25255,
	"title" : "Zeta Sagittae"
	},
{
	"Index" : "5277",
	"Description" : "Gamma Sagittae (Gamma Sge, \u03B3 Sagittae, \u03B3 Sge) is the brightest star in constellation Sagitta and is an orange K-type giant with an apparent magnitude of +3.51. It is approximately 274 light years from Earth and radiates at a power 640 times that of Sun. With a mass of 2.5 times that of the Sun, Gamma Sagittae began life 750 million years ago as a white class B9 star.\r\rGamma Sagittae is moving through the Galaxy at a speed of 42.9 km/s relative to the Sun. It is projected Galactic orbit carries it between 20,300 and 25,900 light years from the center of the Galaxy.\r\rGamma Sagittae will come closest to the Sun 1.4 million years from now when it will brighten to magnitude 2.44 from a distance of 158 light years.\r\rIn Chinese, \u5DE6\u65D7 (Zu\u01D2 Q\u00ED), meaning Left Flag, refers to an asterism consisting of \u03B3 Sagittae, \u03B1 Sagittae, \u03B2 Sagittae, \u03B4 Sagittae, \u03B6 Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and \u03C1 Aquilae. Consequently, \u03B3 Sagittae itself is known as \u5DE6\u65D7\u4E94 (Zu\u01D2 Q\u00ED w\u01D4, English: the Fifth Star of Left Flag.)",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "12 Sagittae, Gamma Sagittae, HIP 98337, SAO 105500, HD 189319, GC 27672, HR 7635, DM BD+19  4229, TYC 1624-3414-1",
	"group" : { "key" : "Sagitta" },
	"Common" : "Gamma Sagittae",
	"OType" : "Variable Star",
	"Distance" : "79.22",
	"RA_S" : 299.68928618,
	"DEC_S" : 19.49214977,
	"X" : 494,
	"Y" : 549,
	"Constellation" : "Sagitta ",
	"AMag" : 3.668,
	"key" : 25277,
	"title" : "Gamma Sagittae"
	},
{
	"Index" : "5281",
	"Description" : "Eta Sagittae (Eta Sge, \u03B7 Sagittae, \u03B7 Sge) is an orange K-type giant with an apparent magnitude of +3.51. It is approximately 162 light years from Earth.\r\rEta Sagittae is moving through the Galaxy at a speed of 45.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 19,100 and 25,500 light years from the center of the Galaxy. It will come closest to the Sun 953,000 years from now when it will brighten to magnitude 3.30 from a distance of 70 light years.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "16 Sagittae, Eta Sagittae, HIP 98920, SAO 105659, HD 190608, GC 27868, HR 7679, DM BD+19  4277, TYC 1625-1053-1",
	"group" : { "key" : "Sagitta" },
	"Common" : "Eta Sagittae",
	"OType" : "Star",
	"Distance" : "49.14",
	"RA_S" : 301.2895611,
	"DEC_S" : 19.99106987,
	"X" : 473,
	"Y" : 545,
	"Constellation" : "Sagitta ",
	"AMag" : 5.209,
	"key" : 25281,
	"title" : "Eta Sagittae"
	},
{
	"Index" : "47276",
	"Description" : "X Sagittarii is a Cepheid variable star in the constellation Sagittarius.\r\rThis variable star changes in apparent magnitude from +4.24 to +4.84 with a period of 7.01 days. Its change in brightness is accompanied by a change in spectral classification, from G2 to F5.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "3 Sagittarii, X Sagittarii, HIP 87072, SAO 185755, HD 161592, GC 24135, HR 6616, DM CD-27 11930, TYC 6836-118-1",
	"group" : { "backgroundImage" : "images/Alignment/19.png",
		"description" : "Sagittarius is a constellation of the zodiac, the one containing the galactic center. Its name is Latin for the archer, and its symbol is \u2650, a stylized arrow. Sagittarius is commonly represented as a centaur drawing a bow. It lies between Ophiuchus to the west and Capricornus to the east.\r\rThe constellation\u0027s brighter stars (from left to right on the map: \u03C4, \u03B6, \u03C3, \u03C6, \u03BB, \u03B5, \u03B4, and \u03B32 Sagittarii) form an easily recognizable asterism known as \u0027the Teapot\u0027. The stars \u03B4 Sgr (Kaus Media), \u03B5 Sgr (Kaus Australis), \u03B6 Sgr (Ascella), and \u03C6 Sgr form the body of the pot; \u03BB Sgr (Kaus Borealis) is the point of the lid; \u03B32 Sgr (Alnasl) is the tip of the spout; and \u03C3 Sgr (Nunki) and \u03C4 Sgr the handle.\r\rThe constellation as a whole is often depicted as having the rough appearance of a stick-figure archer drawing its bow, with the fainter stars providing its horse body.\r\rThe Babylonians identified Sagittarius as the god Nerigal or Nergal, a strange centaur-like creature firing an arrow from a bow. It is generally depicted with wings, with two heads, one panther head and one human head, as well as a scorpion\u0027s stinger raised above its more conventional horse\u0027s tail. The Sumerian name Pabilsag is composed of two elements \u2013 Pabil, meaning \u0027elder paternal kinsman\u0027 and Sag, meaning \u0027chief, head\u0027. The name may thus be translated as the \u0027Forefather\u0027 or \u0027Chief Ancestor\u0027. The figure is reminiscent of modern depictions of Sagittarius.\r\rIn Greek mythology, Sagittarius is identified as a centaur: half human, half horse. In some legends, the Centaur Chiron was the son of Philyra and Saturn, who was said to have changed himself into a horse to escape his jealous wife, Rhea. Chiron was eventually immortalised in the constellation of Centaurus or in some version, Sagittarius.\r\rThe arrow of this constellation points towards the star Antares, the \u0022heart of the scorpion.\u0022",
		"key" : "Sagittarius",
		"grouptype" : "Sagittarius",
		"Meaning" : "archer",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Sagittarius",
		"title" : "Sagittarius Objects Group" },
	"Common" : "X Sagittarii",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "299.89",
	"RA_S" : 266.89010248,
	"DEC_S" : -27.83079164,
	"X" : 525,
	"Y" : 251,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.656,
	"key" : 67276,
	"title" : "X Sagittarii"
	},
{
	"Index" : "51706",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 88060A, HD 163755, GC 24451, HR 6693, DM CD-3015035, TYC 7378-3132-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HD 163755",
	"OType" : "Star",
	"Distance" : "310.559",
	"RA_S" : 269.77200341,
	"DEC_S" : -30.25302294,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.391,
	"key" : 71706,
	"title" : "HD 163755"
	},
{
	"Index" : "47320",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "4 Sagittarii, HIP 88116, SAO 186061, HD 163955, GC 24483, HR 6700, DM CD-23 13731, TYC 6841-1403-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "4 Sagittarii",
	"OType" : "Star",
	"Distance" : "126.62",
	"RA_S" : 269.94814164,
	"DEC_S" : -23.81612685,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.72,
	"key" : 67320,
	"title" : "4 Sagittarii"
	},
{
	"Index" : "47340",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "7 Sagittarii, HIP 88380, SAO 186163, HD 164584, GC 24555, HR 6724, DM CD-24 13793, TYC 6842-1740-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "7 Sagittarii",
	"OType" : "Star in Cluster",
	"Distance" : "327.75",
	"RA_S" : 270.71291573,
	"DEC_S" : -24.28246659,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.448,
	"key" : 67340,
	"title" : "7 Sagittarii"
	},
{
	"Index" : "47485",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "W Sagittarii, HIP 88567, SAO 186237, HD 164975, GC 24605, HR 6742, DM CD-29 14447, TYC 6854-4373-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Nash",
	"OType" : "Classical Cepheid (delta Cep type)",
	"Distance" : "266.6667",
	"RA_S" : 271.25510345,
	"DEC_S" : -29.58008828,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.781,
	"key" : 67485,
	"shortTitle" : "Alnasl; Alwazl; Zujj al Nushshabah; Nushaba (see HD165135)",
	"title" : "Nash"
	},
{
	"Index" : "51923",
	"Description" : "Gamma Sagittarii (Gamma Sgr, \u03B3 Sagittarii, \u03B3 Sgr) is a 3rd-magnitude star in the zodiac constellation Sagittarius. The location of this star forms the tip of the arrow in the bow of Sagittarius the Centaur. It has the proper names Alnasl (Nasl, El Nasl), Nushaba (Nash) and Warida.\r\rThis star is close enough to the Earth that its distance can be determined using parallax, yielding a value of about 96.9 light-years (29.7 parsecs). It has an apparent visual magnitude of +2.98, making it the seventh brightest star in the constellation. A stellar classification of K1 III reveals that this is a giant star, having expanded to an estimated 12 times the Sun\u0027s radius. This means it has exhausted the hydrogen in its core and evolved away from the main sequence. The abundance of elements other than hydrogen and helium in this star, what astronomers term the star\u0027s metallicity, is lower than in the Sun. Gamma Sagittarii has an effective temperature of 4,760 K, compared to 5,778 K for the Sun. It is this lower temperature that gives Gamma Sagittarii the orange hue that is a characteristic of K-type stars.\r\rThere is a fainter optical companion located about 50 arcminutes north of this star. It is magnitude 4.7 Cepheid variable star designated W Sagittarii.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "10 Sagittarii, Gamma Sagittarii, HIP 88635, SAO 209696, HD 165135, GC 24632, HR 6746, DM CD-30 15215, TYC 7391-2710-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Alnasl / Nushaba / Warida",
	"OType" : "High proper-motion Star",
	"Distance" : "29.7",
	"RA_S" : 271.45202735,
	"DEC_S" : -30.42409858,
	"X" : 470,
	"Y" : 279,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.066,
	"key" : 71923,
	"shortTitle" : "Nushaba (see HD164975); Alnasl; Alwazl; Zujj al Nushshabah",
	"title" : "Alnasl / Nushaba / Warida"
	},
{
	"Index" : "47484",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 88839, SAO 186328, HD 165634, GC 24694, HR 6766, DM CD-2814174, TYC 6854-4372-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6766",
	"OType" : "Star",
	"Distance" : "103.86",
	"RA_S" : 272.02074305,
	"DEC_S" : -28.45709441,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.661,
	"key" : 67484,
	"title" : "HR 6766"
	},
{
	"Index" : "47355",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "11 Sagittarii, HIP 89153, SAO 186437, HD 166464, GC 24799, HR 6801, DM CD-23 14047, TYC 6843-1347-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "11 Sagittarii",
	"OType" : "Star",
	"Distance" : "78.44",
	"RA_S" : 272.93056136,
	"DEC_S" : -23.701234,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.081,
	"key" : 67355,
	"title" : "11 Sagittarii"
	},
{
	"Index" : "43080",
	"Description" : "Mu Sagittarii (Mu Sgr, \u03BC Sagittarii, \u03BC Sgr) is a star system in the constellation Sagittarius. It also has the traditional name Polis.\r\rThe stars in the Polis system are designated Polis A through Polis E. Polis is more than 3000 light years from Earth.\r\rThe primary component in this system, Polis A, is a type B giant star with a total luminosity of 180,000 times that of the Sun and a radius of 115 times solar. Its mass is 23 times the solar mass while it has a surface temperature of 11,100 kelvins.\r\rPolis A is an eclipsing binary, bringing the total of stars in the system to six. The primary component is a spectral type B8 supergiant and the companion is a type B2 giant. The orbital period of the binary is 180.55 days. Due to occultation of the primary by the companion, the apparent magnitude of Polis A varies between +3.84 and +3.96.\r\rThe remaining components are very weakly bound to the Polis system.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "13 Sagittarii, Mu Sagittarii, HIP 89341, SAO 186497, HD 166937, GC 24856, HR 6812, DM BD-21  4908, TYC 6276-3093-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Polis",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"RA_S" : 273.44087017,
	"DEC_S" : -21.05883169,
	"X" : 454,
	"Y" : 155,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.845,
	"key" : 63080,
	"title" : "Polis"
	},
{
	"Index" : "43072",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "15 Sagittarii, HIP 89439, SAO 186543, HD 167264, GC 24893, HR 6822, DM BD-20  5054, TYC 6276-1023-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "15 Sagittarii",
	"OType" : "Blue supergiant star",
	"RA_S" : 273.80377669,
	"DEC_S" : -20.72827049,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.339,
	"key" : 63072,
	"title" : "15 Sagittarii"
	},
{
	"Index" : "52083",
	"Description" : "Eta Sagittarii (Eta Sgr, \u03B7 Sagittarii, \u03B7 Sgr) is a binary star system in the southern zodiac constellation of Sagittarius. Based upon parallax measurements, it is located at a distance of 146 light-years (45 parsecs) from Earth. It was formerly known as \u0022Beta Telescopii\u0022 (\u03B2 Tel). In India, where part of the constellation of Sagittarius represents an Elephant, this star forms the creature\u0027s tail.\r\rThe primary component, \u03B7 Sagittarii A, is a red giant star with a stellar classification of M2 III. It is an evolved star that is currently at a stage called the asymptotic giant branch, having exhausted both the hydrogen and the helium at its core. This star is classified as an oxygen-rich irregular variable, as it undergoes small magnitude fluctuations between +3.08 and 3.12. The measured angular diameter of this star is 11.9 \u00B1 2.1 mas. At the estimated distance of Eta Draconis, this yields a physical size of about 57 times the radius of the Sun.\r\rThe companion, \u03B7 Sagittarii B, was first noted by American astronomer S. W. Burnham in 1879. The two stars share a common proper motion and hence are probably gravitationally bound to each other. The secondary is likely an F-type main sequence star with an apparent magnitude of +7.77. It located at an angular separation of 3.6 arcseconds from the primary, along a position angle of 108\u00B0. This star is at a projected distance of 165 Astronomical Units from the red giant primary and the pair take a minimum of 1,270 years to complete an orbit.\r\rWithin the context of the Milky Way galaxy, this system is a member of the faint old disk group. Because of proper motion, this star will move into constellation Corona Australis around 6300 CE. Eta Sagittarii has two optical companions that are not physically associated with the system. The first is a 10th magnitude star at an angular separation of 93 arcseconds with a position angle of 303\u00B0. There is a fainter, 13th magnitude star at an angular separation of 33 arcseconds along a position angle of 276\u00B0.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Eta Sagittarii, HIP 89642, SAO 209957, HD 167618, GC 24944, HR 6832, DM CD-36 12423, TYC 7404-7057-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Eta Sagittarii",
	"OType" : "Long Period Variable candidate",
	"Distance" : "44.74",
	"RA_S" : 274.40680477,
	"DEC_S" : -36.76168819,
	"X" : 432,
	"Y" : 358,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.298,
	"key" : 72083,
	"title" : "Eta Sagittarii"
	},
{
	"Index" : "47454",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 89678, SAO 186612, HD 167818, GC 24961, HR 6842, DM CD-2712684, TYC 6852-5204-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6842",
	"OType" : "Star",
	"Distance" : "231.99",
	"RA_S" : 274.51330204,
	"DEC_S" : -27.04264383,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.829,
	"key" : 67454,
	"title" : "HR 6842"
	},
{
	"Index" : "47510",
	"Description" : "Delta Sagittarii (Delta Sgr, \u03B4 Sagittarii, \u03B4 Sgr) is a double star in the southern zodiac constellation of Sagittarius. It has the traditional names Kaus Media, Kaus Meridionalis, and Media.The apparent visual magnitude of this star is +2.70, making it easily visible to the naked eye. Parallax measurements place the distance at roughly 348 light-years (107 parsecs) from Earth.\r\rThis is a giant star with a stellar classification K3 III. It has a mass of about 3.4 times that of the Sun, while the outer envelope has expanded to 129 times the Sun\u0027s radius. With an effective temperature of roughly 3,600 K, it is radiating 2,500 times the luminosity of the Sun.\r\rIt has three dim companions",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "19 Sagittarii, Delta Sagittarii, HIP 89931, SAO 186681, HD 168454, GC 25024, HR 6859, DM CD-29 14834, TYC 6856-2170-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Kaus Media / Kaus Meridionalis / Media",
	"OType" : "High proper-motion Star",
	"Distance" : "106.56",
	"RA_S" : 275.24850706,
	"DEC_S" : -29.8281024,
	"X" : 427,
	"Y" : 268,
	"Constellation" : "Sagittarius ",
	"AMag" : 2.83,
	"key" : 67510,
	"shortTitle" : "Kaus Medius; Kaus Meridionalis; Media; Kaus Meridianalis",
	"title" : "Kaus Media / Kaus Meridionalis / Media"
	},
{
	"Index" : "52093",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90074, SAO 210061, HD 168733, GC 25067, HR 6870, DM CD-3612524, TYC 7405-3486-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6870",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "170",
	"RA_S" : 275.72115209,
	"DEC_S" : -36.66955555,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.31,
	"key" : 72093,
	"title" : "HR 6870"
	},
{
	"Index" : "43046",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "21 Sagittarii, HIP 90289A, SAO 186794, HD 169420, GC 25132, HR 6896, DM BD-20  5134A, TYC 6274-1663-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "21 Sagittarii",
	"OType" : "Star",
	"Distance" : "124.56",
	"RA_S" : 276.33759697,
	"DEC_S" : -20.54164289,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.029,
	"key" : 63046,
	"title" : "21 Sagittarii"
	},
{
	"Index" : "47555",
	"Description" : "Lambda Sagittarii (Lambda Sgr, \u03BB Sagittarii, \u03BB Sgr) is the Bayer designation for a star within the southern constellation of Sagittarius. The star marks the top of the Archer\u0027s bow, whence its traditional name Kaus Borealis.\r\rWith an apparent visual magnitude of +2.82, this is one of the brighter members of the constellation and, accordingly to the Bortle Dark-Sky Scale, it is readily visible to the naked eye. Based upon parallax measurements, it is located at a distance of 78.2 light-years (24.0 parsecs) from Earth. Being near the ecliptic, Lambda Sgr is sometimes occulted by the Moon and, more rarely, by a planet. The last planet to pass in front of it was Venus, on 19 November 1984. The previous occasion was on 5 December 1865, when it was occulted by the planet Mercury.\r\rKaus Borealis is a subgiant star with a stellar classification of K0 IV. It has a mass 2.6 times that of the Sun. The interferometry-measured angular diameter of this star, after correction for limb darkening, is 4.24 \u00B1 0.05 mas. At the estimated distance of Lambda Sagittarii, this yields a physical size of about 11 times the radius of the Sun. This expanded outer envelope is radiating energy at an effective temperature of 4,770 K, causing it to glow with the cool orange hue of a K-type star. It appears to be rotating at a leisurely rate, with a projected rotational velocity of 3.81 km s\u20131.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "22 Sagittarii, Lambda Sagittarii, HIP 90496, SAO 186841, HD 169916, GC 25180, HR 6913, DM CD-25 13149, TYC 6861-3180-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Kaus Borealis",
	"OType" : "Star",
	"Distance" : "23.97",
	"RA_S" : 276.99266925,
	"DEC_S" : -25.42170006,
	"X" : 409,
	"Y" : 210,
	"Constellation" : "Sagittarius ",
	"AMag" : 2.924,
	"key" : 67555,
	"title" : "Kaus Borealis"
	},
{
	"Index" : "51991",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90763A, SAO 210257, HD 170479, GC 25263, HR 6936, DM CD-3313281, TYC 7398-1220-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6936",
	"OType" : "Star",
	"Distance" : "88.35",
	"RA_S" : 277.77018386,
	"DEC_S" : -32.98910218,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.41,
	"key" : 71991,
	"title" : "HR 6936"
	},
{
	"Index" : "42989",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 90806, SAO 161564, HD 170680, GC 25279, HR 6944, DM BD-18 4988, TYC 6270-2456-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6944",
	"OType" : "Star",
	"Distance" : "68.37",
	"RA_S" : 277.85956944,
	"DEC_S" : -18.40269738,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.118,
	"key" : 62989,
	"title" : "HR 6944"
	},
{
	"Index" : "51992",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 91014, SAO 210312, HD 171034, GC 25327, HR 6960, DM CD-3313338, TYC 7398-1312-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 6960",
	"OType" : "Variable Star",
	"Distance" : "399.94",
	"RA_S" : 278.49069225,
	"DEC_S" : -33.01656315,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.256,
	"key" : 71992,
	"title" : "HR 6960"
	},
{
	"Index" : "52235",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 91918, SAO 210509, HD 172910, GC 25613, HR 7029, DM CD-3512876, TYC 7419-3077-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 7029",
	"OType" : "Star",
	"Distance" : "142.88",
	"RA_S" : 281.08067365,
	"DEC_S" : -35.64199177,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.816,
	"key" : 72235,
	"title" : "HR 7029"
	},
{
	"Index" : "47590",
	"Description" : "Phi Sagittarii (Phi Sgr, \u03C6 Sagittarii, \u03C6 Sgr) is a star in the southern constellation of Sagittarius. With an apparent visual magnitude of 3.17, it is the ninth brightest star in the constellation and is readily visible to the naked eye. Parallax measurements place it at a distance of roughly 239 light-years (73 pc) from the Earth.\r\rThe stellar classification of this star has been rated at B8.5 III and B7 IV, with a luminosity class of III indicating it is a giant star, while a class of IV suggests it is still a subgiant star. Both represent stages in the evolution of a star after it has exhausted the hydrogen at its core. This energy is being radiated from the star\u0027s outer envelope at an effective temperature of 14,990 K, which produces the blue-white hue typical of B-type stars.\r\rIn the past, this star catalogued as a spectroscopic binary and a companion was apparently detected through lunar occultation. However, it is most likely a solitary star and any nearby stars are merely optical companions.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "27 Sagittarii, Phi Sagittarii, HIP 92041, SAO 187239, HD 173300, GC 25661, HR 7039, DM CD-27 13170, TYC 6867-2428-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Phi Sagittarii",
	"OType" : "Star",
	"Distance" : "73.35",
	"RA_S" : 281.41411125,
	"DEC_S" : -26.99077697,
	"X" : 357,
	"Y" : 229,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.126,
	"key" : 67590,
	"title" : "Phi Sagittarii"
	},
{
	"Index" : "43196",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "29 Sagittarii, HIP 92390, SAO 187324, HD 174116, GC 25785, HR 7078, DM BD-20  5277, TYC 6289-3134-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "29 Sagittarii",
	"OType" : "Variable Star",
	"Distance" : "281.17",
	"RA_S" : 282.41711186,
	"DEC_S" : -20.32465569,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.373,
	"key" : 63196,
	"title" : "29 Sagittarii"
	},
{
	"Index" : "47547",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "32 Sagittarii, Nu01 Sagittarii, HIP 92761, SAO 187426, HD 174974, GC 25918, HR 7116, DM BD-22  4907, TYC 6860-863-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Ain al Rami",
	"OType" : "Star",
	"Distance" : "340.46",
	"RA_S" : 283.54240275,
	"DEC_S" : -22.74483882,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.008,
	"key" : 67547,
	"title" : "Ain al Rami"
	},
{
	"Index" : "47544",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "35 Sagittarii, Nu02 Sagittarii, HIP 92845, SAO 187445, HD 175190, GC 25939, HR 7120, DM BD-22  4915, TYC 6860-304-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Nu02 Sagittarii",
	"OType" : "Star",
	"Distance" : "83.77",
	"RA_S" : 283.77973683,
	"DEC_S" : -22.67131098,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.149,
	"key" : 67544,
	"title" : "Nu02 Sagittarii"
	},
{
	"Index" : "43243",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "36 Sagittarii, Xi01 Sagittarii, HIP 93057, SAO 187498, HD 175687, GC 26012, HR 7145, DM BD-20  5339, TYC 6294-1245-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Xi01 Sagittarii",
	"OType" : "Star",
	"Distance" : "612.99",
	"RA_S" : 284.33532049,
	"DEC_S" : -20.65634646,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.066,
	"key" : 63243,
	"title" : "Xi01 Sagittarii"
	},
{
	"Index" : "43244",
	"Description" : "The Bayer designation Xi Sagittarii (Xi Sgr, \u03BE Sagittarii, \u03BE Sgr) is shared by two stars, \u03BE\u00B9 Sagittarii and \u03BE\u00B2 Sagittarii, in the constellation Sagittarius, separated by 0.46\u00B0 in the sky. Because they are close to the ecliptic, they can be occulted by the Moon and, very rarely, by planets. The last occultation of \u03BE\u00B2 Sagittarii by a planet took place on 22 December 1810, when it was occulted by Venus.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "37 Sagittarii, Xi02 Sagittarii, HIP 93085, SAO 187504, HD 175775, GC 26019, HR 7150, DM BD-21  5201, TYC 6294-2507-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Xi Sagittarii",
	"OType" : "Star",
	"Distance" : "111.51",
	"RA_S" : 284.43250499,
	"DEC_S" : -21.10665345,
	"X" : 319,
	"Y" : 155,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.636,
	"key" : 63244,
	"title" : "Xi Sagittarii"
	},
{
	"Index" : "47719",
	"Description" : "Zeta Sagittarii (Zeta Sgr, \u03B6 Sagittarii, \u03B6 Sgr) is the third brightest star system in the constellation Sagittarius, with an apparent visual magnitude of +2.59. It has the traditional name Ascella. Based upon parallax measurements, the distance to Ascella is about 88 ly (27 pc). Ascella is moving away from the Solar System with a radial velocity of 22 km s\u22121. Some 1.0\u20131.4 million years ago, this system came within 7.5 \u00B1 1.8 ly (2.3 \u00B1 0.55 pc) of the Sun.\r\rThis is a binary star system, with the two components orbiting each other over a period of 21 years at an eccentricity of 0.211. The combined mass of the system is 5.26 \u00B1 0.37 times the mass of the Sun and their blended stellar classification is A2.5 Va.\r\rThe system consists of a spectral class A2 giant with an apparent magnitude of +3.27, and an A4 subgiant with apparent magnitude of +3.48. The pair have a mean separation of 13.4 astronomical units (AU). Ascella has a faint, 10th magnitude companion, separated from the primary by a distance of 75 arcseconds.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "38 Sagittarii, Zeta Sagittarii, HIP 93506AB, SAO 187600, HD 176687, GC 26161, HR 7194, DM CD-30 16575, TYC 6885-2837-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Ascella",
	"OType" : "Double or multiple star",
	"Distance" : "27.02",
	"RA_S" : 285.65304266,
	"DEC_S" : -29.8800633,
	"X" : 309,
	"Y" : 269,
	"Constellation" : "Sagittarius ",
	"AMag" : 2.599,
	"key" : 67719,
	"shortTitle" : "Askela; Astsella",
	"title" : "Ascella"
	},
{
	"Index" : "52136",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 93667, SAO 210883, HD 177074, GC 26209, HR 7211, DM CD-3116306, TYC 7410-3044-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 7211",
	"OType" : "Star",
	"Distance" : "146.64",
	"RA_S" : 286.10440563,
	"DEC_S" : -31.0470795,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.486,
	"key" : 72136,
	"title" : "HR 7211"
	},
{
	"Index" : "43251",
	"Description" : "Omicron Sagittarii (Omicron Sgr, \u03BF Sagittarii, \u03BF Sgr) is a binary star in the constellation Sagittarius. \u03BF Sagittarii is located 142 light years from Earth and is a spectral type K0 orange giant with an apparent magnitude of +3.77. It has a faint, 13th magnitude companion, \u03BF Sagittarii B, 36 arc seconds away.\r\rBecause it is close to the ecliptic, \u03BF Sagittarii can be occulted by the Moon and very rarely by planets. The last occultation of \u03BF Sagittarii by a planet took place on 24 December 1937, when it was occulted by Mercury.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "39 Sagittarii, Omicron Sagittarii, HIP 93683, SAO 187643, HD 177241, GC 26224, HR 7217, DM BD-21  5237, TYC 6295-2492-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Manubrium of Manubrij",
	"OType" : "Star",
	"Distance" : "43.55",
	"RA_S" : 286.1707572,
	"DEC_S" : -21.7414935,
	"X" : 297,
	"Y" : 164,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.861,
	"key" : 63251,
	"title" : "Manubrium of Manubrij"
	},
{
	"Index" : "47703",
	"Description" : "Tau Sagittarii (Tau Sgr, \u03C4 Sagittarii, \u03C4 Sgr) is a star in the southern zodiac constellation of Sagittarius. With an apparent visual magnitude of +3.3, this is one of the brighter members of the constellation. The distance of this star from Earth is roughly 122 light-years (37 parsecs), based upon parallax measurements.\r\rThis is a spectral type K1 giant star with 1.5 - 2 Solar masses. The stellar envelope is slightly cooler than the Sun, with an effective temperature of 4,860 K, giving the star a light orange color. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is 3.93 \u00B1 0.04 mas, which, at its estimated distance, equates to a physical radius of about 16 times the radius of the Sun. Tau Sagittarii is a suspected double star although no companion has been confirmed yet. A lower metal content (Fe to H ratio is 70%) and a high peculiar velocity (64 km/s, 4x the local average) relative to the Sun suggest the star is a visitor from a different part of the Galaxy.\r\rTau Sagittarii is the closest visible star in the night sky to the origin of the 1977 Wow! signal, the only radio signal that has been received that may be a sign of extraterrestrial intelligence.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "40 Sagittarii, Tau Sagittarii, HIP 93864, SAO 187683, HD 177716, GC 26291, HR 7234, DM CD-27 13564, TYC 6881-1777-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Tau Sagittarii",
	"OType" : "High proper-motion Star",
	"Distance" : "37.24",
	"RA_S" : 286.73502439,
	"DEC_S" : -27.67042392,
	"X" : 295,
	"Y" : 241,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.427,
	"key" : 67703,
	"title" : "Tau Sagittarii"
	},
{
	"Index" : "43252",
	"Description" : "Pi Sagittarii (Pi Sgr, \u03C0 Sagittarii, \u03C0 Sgr) is a triple star system in the zodiac constellation Sagittarius. It has the traditional name Albaldah.\r\rAlbaldah has an apparent visual magnitude of +2.89, which is sufficiently bright to be readily seen with the naked eye. Based upon parallax measurements, this star is located at a distance of roughly 510 light-years (160 parsecs) from Earth. Because it is close to the ecliptic, Albaldah can sometimes be occulted by the Moon, and, very rarely, planets of the Solar System. The next occultation by a planet takes place on February 17, 2035, when it will be occulted by Venus.\r\rThe spectrum of this star matches a stellar classification of F2 II. The \u0027II\u0027 luminosity class is for a bright giant star that has exhausted the hydrogen at its core and has followed an evolutionary track away from the main sequence of stars like the Sun. Because it has nearly six times the mass of the Sun, it reached this stage in a mere 67 million years. The outer envelope is radiating energy at an effective temperature of about 6,590 K, giving it the yellow-white hue of an F-type star.\r\rPi Sagittarii has two nearby companions. The first is located at an angular separation of 0.1 arcseconds from Albaldah, or at least 13 Astronomical Units (AU). The second is 0.4 arcseconds away, which is 40 AU or more. Nothing is known about the orbits of these stars.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "41 Sagittarii, Pi Sagittarii, HIP 94141, SAO 187756, HD 178524, GC 26386, HR 7264, DM BD-21  5275, TYC 6295-282-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Albaldah",
	"OType" : "Double or multiple star",
	"Distance" : "155.41",
	"RA_S" : 287.44097053,
	"DEC_S" : -21.02361398,
	"X" : 281,
	"Y" : 155,
	"Constellation" : "Sagittarius ",
	"AMag" : 2.903,
	"key" : 63252,
	"shortTitle" : "Al Baldah",
	"title" : "Albaldah"
	},
{
	"Index" : "47691",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "42 Sagittarii, Psi Sagittarii, HIP 94643, SAO 187882, HD 179950, GC 26516, HR 7292, DM CD-25 13866, TYC 6879-2498-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Psi Sagittarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "91.4",
	"RA_S" : 288.88510541,
	"DEC_S" : -25.25668133,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.924,
	"key" : 67691,
	"title" : "Psi Sagittarii"
	},
{
	"Index" : "43344",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "43 Sagittarii, d Sagittarii, HIP 94820, SAO 162413, HD 180540, GC 26589, HR 7304, DM BD-19  5379, TYC 6304-334-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "d Sagittarii",
	"OType" : "Star",
	"Distance" : "147.43",
	"RA_S" : 289.40866184,
	"DEC_S" : -18.95291023,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.991,
	"key" : 63344,
	"title" : "d Sagittarii"
	},
{
	"Index" : "43320",
	"Description" : "The Bayer designation Rho Sagittarii (Rho Sgr, \u03C1 Sagittarii, \u03C1 Sgr) is shared by two stars, \u03C1\u00B9 Sagittarii and \u03C1\u00B2 Sagittarii, in the constellation Sagittarius. The two stars are separated by 0.46\u00B0 in the sky. Because they are close to the ecliptic, they can be occulted by the Moon and, very rarely, by planets. The next occultation of \u03C1\u00B9 Sagittarii by a planet will take place on 23 February 2046, when it will be occulted by Venus.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "44 Sagittarii, Rho01 Sagittarii, HIP 95168, SAO 162512, HD 181577, GC 26694, HR 7340, DM BD-18  5322, TYC 6301-2457-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Rho Sagittarii",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "38.92",
	"RA_S" : 290.41816275,
	"DEC_S" : -17.84720025,
	"X" : 241,
	"Y" : 117,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.935,
	"key" : 63320,
	"title" : "Rho Sagittarii"
	},
{
	"Index" : "43273",
	"Description" : "Upsilon Sagittarii (Upsilon Sgr, \u03C5 Sagittarii, \u03C5 Sgr) is a spectroscopic binary star system in the constellation Sagittarius. Upsilon Sagittarii is the prototypical hydrogen-deficient binary (HdB), and one of only four such systems known. The unusual spectrum of hydrogen-deficient binaries has made stellar classification of Upsilon Sagittarii difficult.\r\rThe primary component, Upsilon Sagittarii A, is most probably an A type supergiant. The radius of the primary is estimated at 60 solar radii, and its mass is estimated to be 25 solar masses. A is classified as an irregular variable and experiences apparent magnitude fluctuations between +4.51 and +4.65 with a period of approximately 20 days. Its mean apparent magnitude is +4.52.\r\rThe companion, Upsilon Sagittarii B, is more massive, but so dim at visible frequencies as to be undetectable by optical telescopes. It is probably an O or B type main sequence dwarf, which has accreted much of the original mass of the primary. It is estimated to have a mass of 19 solar masses.\r\rThe binary system has an orbital period of 137.939 days and is approximately 1672 light years from Earth. It is predicted that Upsilon Sagittarii will end its life in a supernova.\r\rIn Chinese, \u5EFA (Ji\u00E0n), meaning Establishment, refers to an asterism consisting of \u03C5 Sagittarii, \u03BE\u00B2 Sagittarii, \u03BF Sagittarii, \u03C0 Sagittarii, 43 Sagittarii and \u03C1\u00B9 Sagittarii . Consequently, \u03C5 Sagittarii itself is known as \u5EFA\u516D (Ji\u00E0n li\u00F9, English: the Sixth Star of Establishment.)",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "46 Sagittarii, Upsilon Sagittarii, HIP 95176, SAO 162518, HD 181615, GC 26697, HR 7342, DM BD-16  5283A, TYC 6297-1419-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Upsilon Sagittarii",
	"OType" : "Be Star",
	"Distance" : "536.28",
	"RA_S" : 290.43176503,
	"DEC_S" : -15.95501735,
	"X" : 239,
	"Y" : 93,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.579,
	"key" : 63273,
	"title" : "Upsilon Sagittarii"
	},
{
	"Index" : "56851",
	"Description" : "The Bayer designation Beta Sagittarii (Beta Sgr, \u03B2 Sagittarii, \u03B2 Sgr) is shared by two star systems, \u03B2\u00B9 Sagittarii and \u03B2\u00B2 Sagittarii, in the constellation Sagittarius. The two stars are separated by 0.36\u00B0 in the sky. Beta Sagittarii also has the traditional name Arkab. Beta\u00B9 Sagittarii (Beta\u00B9 Sgr, \u03B2\u00B9 Sagittarii, \u03B2\u00B9 Sgr), also called Arkab Prior since it leads \u03B2\u00B2 across the sky, is a binary star lying 378 light years from Earth. Arkab Prior A is a spectral type B9 main sequence dwarf which has an apparent magnitude of +3.96. Arkab Prior B is a type A3 dwarf with an apparent magnitude of +7.4. The two stars are separated in the sky by 28 arcseconds, which puts them at least 3300 astronomical units apart.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Beta01 Sagittarii, HIP 95241, SAO 229646, HD 181454, GC 26703, HR 7337, DM CD-44 13277, TYC 7943-2105-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Arkab Prior",
	"OType" : "Star",
	"Distance" : "114.34",
	"RA_S" : 290.65954946,
	"DEC_S" : -44.45896074,
	"X" : 274,
	"Y" : 463,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.935,
	"key" : 76851,
	"shortTitle" : "Arkab; Urkab (with HD181623)",
	"title" : "Arkab Prior"
	},
{
	"Index" : "56852",
	"Description" : "The Bayer designation Beta Sagittarii (Beta Sgr, \u03B2 Sagittarii, \u03B2 Sgr) is shared by two star systems, \u03B2\u00B9 Sagittarii and \u03B2\u00B2 Sagittarii, in the constellation Sagittarius. The two stars are separated by 0.36\u00B0 in the sky. Beta Sagittarii also has the traditional name Arkab. Beta\u00B2 Sagittarii (Beta\u00B2 Sgr, \u03B2\u00B2 Sagittarii, \u03B2\u00B2 Sgr), also called Arkab Posterior since it trails \u03B2\u00B9 across the sky, is a spectral type F2 giant which has an apparent magnitude of +4.27. It is 137 light years from Earth.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Beta02 Sagittarii, HIP 95294, SAO 229654, HD 181623, GC 26718, HR 7343, DM CD-45 13171, TYC 7943-2106-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Arkab Posterior",
	"OType" : "Star",
	"Distance" : "41.13",
	"RA_S" : 290.80473648,
	"DEC_S" : -44.79978637,
	"X" : 274,
	"Y" : 467,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.311,
	"key" : 76852,
	"shortTitle" : "Arkab; Urkab (with HD181454)",
	"title" : "Arkab Posterior"
	},
{
	"Index" : "56797",
	"Description" : "Alpha Sagittarii (Alpha Sgr, \u03B1 Sagittarii, \u03B1 Sgr) is a star in the Sagittarius constellation. It has the traditional names Alrami and Rukbat.\r\rAlpha Sagittarii is a blue, class B dwarf star. It does not appear particularly bright in the sky to the naked eye, with a visual apparent magnitude of +3.97. However, this is due to its distance; in reality, the star is twice as hot as the Sun and considerably more massive, with a luminosity in visible wavelengths about 40 times greater than that of the Sun. Based on an excess emission of infrared radiation, it may have a debris disk, much like Vega. It is unclear why Bayer designated this star as the alpha, rather than \u03B5 Sgr or \u03C3 Sgr. This led some old star charts to occasionally depict Alpha and Beta Sgr as much brighter than they are in reality, as they are invisible from northern Europe, being too far south to see there.\r\rThis is a single-lined spectroscopic binary system. The ROSAT All Sky Survey discovered that Alpha Sagittarii is emitting an excess flux of X-rays, which is not expected to originate from a star of this spectral class. The most likely explanation is that the companion is an active pre-main sequence star or else a star that has just reached the main sequence.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Alpha Sagittarii, HIP 95347, SAO 229659, HD 181869, GC 26737, HR 7348, DM CD-40 13245, TYC 7935-2139-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Alrami / Rukbat",
	"OType" : "Star",
	"Distance" : "55.73",
	"RA_S" : 290.9715706,
	"DEC_S" : -40.61593839,
	"X" : 265,
	"Y" : 413,
	"Constellation" : "Sagittarius ",
	"AMag" : 3.927,
	"key" : 76797,
	"shortTitle" : "Alrami; Rucba (also HD8538); Rukbat al Rami",
	"title" : "Alrami / Rukbat"
	},
{
	"Index" : "47697",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "47 Sagittarii, Chi01 Sagittarii, HIP 95477, SAO 188101, HD 182369, GC 26789, HR 7362, DM CD-24 15303, TYC 6880-2342-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Chi01 Sagittarii",
	"OType" : "Double or multiple star",
	"Distance" : "77.08",
	"RA_S" : 291.31868176,
	"DEC_S" : -24.50857986,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.038,
	"key" : 67697,
	"title" : "Chi01 Sagittarii"
	},
{
	"Index" : "47770",
	"Description" : "52 Sagittarii (52 Sgr) is a star in the constellation Sagittarius. Its apparent magnitude is 4.59.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "52 Sagittarii, h02 Sagittarii, HIP 96465, SAO 188337, HD 184707, GC 27089, HR 7440, DM CD-25 14184, TYC 6893-2132-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "52 Sagittarii",
	"OType" : "Star",
	"Distance" : "58.13",
	"RA_S" : 294.17680369,
	"DEC_S" : -24.88361911,
	"X" : 205,
	"Y" : 214,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.587,
	"key" : 67770,
	"title" : "52 Sagittarii"
	},
{
	"Index" : "43299",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "54 Sagittarii, e01 Sagittarii, HIP 96808, SAO 162883, HD 185644, GC 27214, HR 7476, DM BD-16  5399, TYC 6299-2609-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "e01 Sagittarii",
	"OType" : "Star",
	"Distance" : "73.71",
	"RA_S" : 295.18076628,
	"DEC_S" : -16.29326879,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.421,
	"key" : 63299,
	"title" : "e01 Sagittarii"
	},
{
	"Index" : "43297",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "55 Sagittarii, e02 Sagittarii, HIP 96950, SAO 162915, HD 186005, GC 27255, HR 7489, DM BD-16  5413, TYC 6299-2607-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "e02 Sagittarii",
	"OType" : "Star",
	"Distance" : "54.31",
	"RA_S" : 295.62972218,
	"DEC_S" : -16.12399283,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.084,
	"key" : 63297,
	"title" : "e02 Sagittarii"
	},
{
	"Index" : "43455",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "56 Sagittarii, f Sagittarii, HIP 97290, SAO 162964, HD 186648, GC 27349, HR 7515, DM BD-20  5698, TYC 6320-2845-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "f Sagittarii",
	"OType" : "Star",
	"Distance" : "63.64",
	"RA_S" : 296.59058382,
	"DEC_S" : -19.76111302,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.99,
	"key" : 63455,
	"title" : "f Sagittarii"
	},
{
	"Index" : "56820",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 97749, SAO 229903, HD 187474, GC 27474, HR 7552, DM CD-4013514, TYC 7938-3655-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 7552",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "91.69",
	"RA_S" : 297.96085541,
	"DEC_S" : -39.87437082,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.31,
	"key" : 76820,
	"title" : "HR 7552"
	},
{
	"Index" : "56845",
	"Description" : "Iota Sagittarii (Iota Sgr, \u03B9 Sagittarii, \u03B9 Sgr) is a star in the constellation Sagittarius.\r\rIota Sagittarii is a spectral type K0 giant and has an apparent magnitude of +4.12. It is 189 light years from Earth. It is moving through the Galaxy at a speed of 39.3 km/s relative to the Sun. Its projected Galactic orbit carries it between 22,500 and 50,100 light years from the center of the Galaxy.\r\rIt came closest to the Sun 1.3 million years ago when it had brightened to magnitude 2.21 from a distance of 75 light years.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Iota Sagittarii, HIP 98032, SAO 229927, HD 188114, GC 27557, HR 7581, DM CD-42 14549, TYC 7942-3241-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Iota Sagittarii",
	"OType" : "Star",
	"Distance" : "55.73",
	"RA_S" : 298.81540493,
	"DEC_S" : -41.86827352,
	"X" : 193,
	"Y" : 442,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.235,
	"key" : 76845,
	"title" : "Iota Sagittarii"
	},
{
	"Index" : "47803",
	"Description" : "Omega Sagittarii (Omega Sgr, \u03C9 Sagittarii, \u03C9 Sgr) is a G-type subgiant star in the constellation of Sagittarius. It has an apparent visual magnitude of approximately 4.70.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "58 Sagittarii, Omega Sagittarii, HIP 98066, SAO 188722, HD 188376, GC 27583, HR 7597, DM CD-26 14637, TYC 6899-2595-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Omega Sagittarii",
	"OType" : "High proper-motion Star",
	"Distance" : "25.84",
	"RA_S" : 298.95982747,
	"DEC_S" : -26.29949408,
	"X" : 150,
	"Y" : 254,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.773,
	"key" : 67803,
	"shortTitle" : "Terebell",
	"title" : "Omega Sagittarii"
	},
{
	"Index" : "47804",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "59 Sagittarii, b01 Sagittarii, HIP 98162, SAO 188742, HD 188603, GC 27605, HR 7604, DM CD-27 14399, TYC 6899-2596-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Terebellum (see HD188376,189005,189763)",
	"OType" : "Star",
	"Distance" : "253.55",
	"RA_S" : 299.23679853,
	"DEC_S" : -27.16990026,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.698,
	"key" : 67804,
	"title" : "Terebellum (see HD188376,189005,189763)"
	},
{
	"Index" : "43417",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "61 Sagittarii, g Sagittarii, HIP 98258, SAO 163141, HD 188899, GC 27637, HR 7614, DM BD-15  5516, TYC 6313-2321-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "g Sagittarii",
	"OType" : "Star",
	"Distance" : "81.28",
	"RA_S" : 299.48762683,
	"DEC_S" : -15.49150531,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.006,
	"key" : 63417,
	"title" : "g Sagittarii"
	},
{
	"Index" : "47785",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "60 Sagittarii, A Sagittarii, HIP 98353, SAO 188778, HD 189005, GC 27658, HR 7618, DM CD-26 14682, TYC 6896-2102-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Terebellum (see HD188376)",
	"OType" : "Star",
	"Distance" : "95.98",
	"RA_S" : 299.73832094,
	"DEC_S" : -26.19576704,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.945,
	"key" : 67785,
	"title" : "Terebellum (see HD188376)"
	},
{
	"Index" : "52454",
	"Description" : "The Bayer designation Theta Sagittarii (Theta Sgr, \u03B8 Sagittarii, \u03B8 Sgr) is shared by two star systems, \u03B8\u00B9 Sagittarii and \u03B8\u00B2 Sagittarii, in the constellation Sagittarius. The two stars are separated by 0.58\u00B0 in the sky.\r\r\u03B8\u00B9 Sagittarii\r\rTheta\u00B9 Sagittarii (Theta\u00B9 Sgr, \u03B8\u00B9 Sagittarii, \u03B8\u00B9 Sgr) is a spectroscopic binary lying 617 light years from Earth. The primary star, \u03B8\u00B9 Sagittarii A, is a spectral type B2.5 subgiant which has an apparent magnitude of +4.37. The companion star, \u03B8\u00B9 Sagittarii B, is approximately 0.2 arcseconds from the primary, which puts them 31 astronomical units (AU) apart (a Sun-Neptune distance).\r\rTheta\u00B9 Sagittarii is moving through the Galaxy at a speed of 19.9 km/s relative to the Sun. Its projected Galactic orbit carries it between 20,900 and 24,300 light years from the center of the Galaxy.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Theta01 Sagittarii, HIP 98412, SAO 211716, HD 189103, GC 27670, HR 7623, DM CD-35 13831, TYC 7448-1357-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Theta Sagittarii",
	"OType" : "Spectroscopic binary",
	"Distance" : "158.77",
	"RA_S" : 299.93407933,
	"DEC_S" : -35.27630705,
	"X" : 163,
	"Y" : 360,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.325,
	"key" : 72454,
	"title" : "Theta Sagittarii"
	},
{
	"Index" : "52453",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Theta02 Sagittarii, HIP 98421, SAO 211717, HD 189118, GC 27676, HR 7624, DM CD-35 13832, TYC 7448-1356-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Theta02 Sagittarii",
	"OType" : "Star",
	"Distance" : "48.49",
	"RA_S" : 299.96398574,
	"DEC_S" : -34.69780779,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.321,
	"key" : 72453,
	"title" : "Theta02 Sagittarii"
	},
{
	"Index" : "47811",
	"Description" : "62 Sagittarii (62 Sgr) or c Sagittarii (c Sgr) is an M-type giant star in the constellation of Sagittarius. It is the southwest corner of the asterism called the Terebellum. It is an irregular variable whose apparent visual magnitude varies between 4.45 and 4.64, and, at its brightest, it is the brightest of the four stars in the Terebellum. It is approximately 450 light-years from Earth. 62 Sagittarii is the star in the Terebellum which is most distant from its centre; it is 1.72\u00B0 from its northwest corner, 60 Sagittarii, and 1.37\u00B0 from its southeast corner, 59 Sagittarii.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "62 Sagittarii, c Sagittarii, HIP 98688, SAO 188844, HD 189763, GC 27763, HR 7650, DM CD-28 16355, TYC 6900-2236-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "62 Sagittarii",
	"OType" : "Long-period variable star",
	"Distance" : "137.45",
	"RA_S" : 300.66449858,
	"DEC_S" : -27.70984656,
	"X" : 136,
	"Y" : 264,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.676,
	"key" : 67811,
	"title" : "62 Sagittarii"
	},
{
	"Index" : "56871",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 98761, SAO 211767, HD 189831, GC 27779, HR 7652, DM CD-3813828, TYC 7947-3890-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 7652",
	"OType" : "Star",
	"Distance" : "112.22",
	"RA_S" : 300.88940613,
	"DEC_S" : -37.94070715,
	"Constellation" : "Sagittarius ",
	"AMag" : 4.928,
	"key" : 76871,
	"title" : "HR 7652"
	},
{
	"Index" : "52433",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 98842, SAO 211782, HD 190056, GC 27811, HR 7659, DM CD-3215682, TYC 7444-1508-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "HR 7659",
	"OType" : "Variable Star",
	"Distance" : "89.07",
	"RA_S" : 301.08163884,
	"DEC_S" : -32.05629774,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.123,
	"key" : 72433,
	"title" : "HR 7659"
	},
{
	"Index" : "52496",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 99461, SAO 211885, HD 191408A, GC 27992, HR 7703, DM CD-3613940, TYC 7453-1391-1",
	"group" : { "key" : "Sagittarius" },
	"Common" : "Gliese 783 A (HR 7703)",
	"OType" : "High proper-motion Star",
	"Distance" : "6.02",
	"RA_S" : 302.79974601,
	"DEC_S" : -36.10119781,
	"Constellation" : "Sagittarius ",
	"AMag" : 5.413,
	"key" : 72496,
	"title" : "Gliese 783 A (HR 7703)"
	},
{
	"Index" : "46913",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "1 Scorpii, b Scorpii, HIP 77635, SAO 183854, HD 141637, GC 21285, HR 5885, DM CD-25 11131, TYC 6782-2148-1",
	"group" : { "backgroundImage" : "images/Alignment/38.png",
		"description" : "Scorpius, sometimes known as Scorpio, is one of the constellations of the zodiac. Its name is Latin for scorpion, and its symbol is \u264F. It lies between Libra to the west and Sagittarius to the east. It is a large constellation located in the southern hemisphere near the center of the Milky Way.\r\rIn Greek Mythology the myths associated with Scorpio almost invariably also contain a reference to Orion. According to one of these myths it is written that Orion boasted to goddess Artemis and her mother, Leto, that he would kill every animal on the earth. Although Artemis was known to be a hunter herself she offered protection to all creatures. Artemis and her mother Leto sent a scorpion to deal with Orion. The pair battled and the scorpion killed Orion. However, the contest was apparently a lively one that caught the attention of the king of the gods Zeus, who later raised the scorpion to heaven and afterwards, at the request of Artemis, did the same for Orion to serve as a reminder for mortals to curb their excessive pride. There is also a version that Orion was better than the goddess Artemis but said that Artemis was better than he and so Artemis took a liking to Orion. The god Apollo, Artemis\u0027s twin brother, grew angry and sent a scorpion to attack Orion. After Orion was killed, Artemis asked Zeus to put Orion up in the sky. So every winter Orion hunts in the sky, but every summer he flees as the constellation of the scorpion comes.\r\rIn another Greek story involving Scorpio without Orion, Phaeton (the mortal male offspring of Helios) went to his father, who had earlier sworn by the River Styx to give Phaeton anything he should ask for. Phaeton wanted to drive his father\u0027s Sun Chariot for a day. Although Helios tried to dissuade his son, Phaeton was adamant. However, when the day arrived, Phaeton panicked and lost control of the white horses that drew the chariot. First, the Earth grew chill as Phaeton flew too high and encountered the celestial scorpion, its deadly sting raised to strike. Alarmed, he dipped the chariot too close, causing the vegetation to burn. By accident, Phaeton turned most of Africa into desert and darkened the skin of the Ethiopian nation until it was black. Eventually, Zeus was forced to intervene by striking the runaway chariot and Phaeton with a lightning bolt to put an end to its rampage and Phaeton plunged into the River Eridanos.\r\rThe Babylonians called this constellation MUL.GIR.TAB - the \u0027Scorpion\u0027, the signs can be literally read as \u0027the (creature with) a burning sting\u0027. The Claws of the Scorpion were also known as the Scales in Babylonia.",
		"key" : "Scorpius",
		"grouptype" : "Scorpius",
		"Meaning" : "scorpion",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Scorpius",
		"title" : "Scorpius Objects Group" },
	"Common" : "b Scorpii",
	"OType" : "Star",
	"Distance" : "151.44",
	"RA_S" : 237.74476794,
	"DEC_S" : -25.75129441,
	"Constellation" : "Scorpius ",
	"AMag" : 4.622,
	"key" : 66913,
	"title" : "b Scorpii"
	},
{
	"Index" : "46911",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "2 Scorpii, HIP 77840A, TYC 6782-2147-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "2 A Scorpii (HR 5904)",
	"OType" : "Double or multiple star",
	"Distance" : "152.95",
	"RA_S" : 238.40299219,
	"DEC_S" : -25.32713753,
	"Constellation" : "Scorpius ",
	"AMag" : 4.694,
	"key" : 66911,
	"title" : "2 A Scorpii (HR 5904)"
	},
{
	"Index" : "46912",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "2 Scorpii, A Scorpii, HIP 77840B, SAO 183896, HD 142114, GC 21329, HR 5904, DM CD-24 12352, TYC 6782-2147-2",
	"group" : { "key" : "Scorpius" },
	"Common" : "A Scorpii",
	"OType" : "Double or multiple star",
	"Distance" : "152.95",
	"RA_S" : 238.402995,
	"DEC_S" : -25.32714131,
	"Constellation" : "Scorpius ",
	"AMag" : 4.59,
	"key" : 66912,
	"title" : "A Scorpii"
	},
{
	"Index" : "46909",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 77858, SAO 183900, HD 142165, GC 21339, HR 5906, DM CD-2412354, TYC 6782-2145-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 5906",
	"OType" : "Spectroscopic binary",
	"Distance" : "128.18",
	"RA_S" : 238.474641,
	"DEC_S" : -24.53315764,
	"Constellation" : "Scorpius ",
	"AMag" : 5.368,
	"key" : 66909,
	"title" : "HR 5906"
	},
{
	"Index" : "46878",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 77859, SAO 183901, HD 142184, GC 21341, HR 5907, DM CD-2312569, TYC 6778-1980-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 5907",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "130.52",
	"RA_S" : 238.48276445,
	"DEC_S" : -23.97809846,
	"Constellation" : "Scorpius ",
	"AMag" : 5.394,
	"key" : 66878,
	"title" : "HR 5907"
	},
{
	"Index" : "46977",
	"Description" : "Rho Scorpii (\u03C1 Sco, \u03C1 Scorpii) is a binary star in the constellation Scorpius. It is approximately 409 light years from Earth.\r\rThe primary component, Rho Scorpii A, is a blue-white B-type subgiant with an apparent magnitude of +3.87. Orbiting it with a separation of 38 arcseconds is the magnitude +12.8 Rho Scorpii B.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "5 Scorpii, Rho Scorpii, HIP 78104, SAO 183957, HD 142669, GC 21398, HR 5928, DM CD-28 11714, TYC 6791-2509-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Rho Scorpii",
	"OType" : "Spectroscopic binary",
	"Distance" : "144.59",
	"RA_S" : 239.22114797,
	"DEC_S" : -29.21407343,
	"X" : 486,
	"Y" : 381,
	"Constellation" : "Scorpius ",
	"AMag" : 3.833,
	"key" : 66977,
	"title" : "Rho Scorpii"
	},
{
	"Index" : "46921",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 78246, SAO 183982, HD 142990, GC 21442, HR 5942, DM CD-2412427, TYC 6783-2695-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 5942",
	"OType" : "Rotationally variable Star",
	"Distance" : "170.02",
	"RA_S" : 239.64527921,
	"DEC_S" : -24.83149237,
	"Constellation" : "Scorpius ",
	"AMag" : 5.405,
	"key" : 66921,
	"title" : "HR 5942"
	},
{
	"Index" : "46923",
	"Description" : "Pi Scorpii is a triple star system in the southern constellation Scorpius. With a combined apparent magnitude of 2.9, it can be easily seen with the naked eye. Parallax measurements yield an estimated distance of around 590 light-years (180 parsecs) from the Earth.\r\rThe name Pi Scorpii was assigned to this star by the German astronomer Johann Bayer in 1603. In 1712, it received the catalogue identifier 6 Scorpii with the publication of the star catalogue of English astronomer John Flamsteed. The binary nature of this star remained unknown until 1899, when it was announced by American astronomer Edward Charles Pickering. Two years later, an orbital period of 1.571 days was found by American astronomer Solon Irving Bailey, but it would not be until 1927 that the orbit of this spectroscopic binary was determined by Russian astronomer Otto Struve and American astrophysicist Christian T. Elvey.\r\rThe main components of this system form an eclipsing binary of the Beta Lyrae type. Both its members are hot, B-type main sequence stars with a blue-white hue. They display an ellipsoidal variation of 0.03 in magnitude. The two stars are rotating rapidly, with projected rotational velocities of 108 and 87 km s\u22121, respectively. Their orbital period is 1.57 days and they are separated by an estimated distance of only 15 solar radii along a circular orbit. The binary system is orbited by a smaller, more distant companion, which has an apparent magnitude of +12.2. This component is separated from the pair by 50 arcseconds, putting it at least 7000 Astronomical Units away.\r\rThe Pi Scorpii system is a kinematic member of the Upper Scorpius subgroup of the Scorpius-Centaurus Association, a group of thousands of young stars with mean age 11 million years at distance 470 light years (145 parsecs). A recent analysis of the HR diagram position for the primary star Pi Scorpii A estimates its effective temperature to be 25,230 Kelvin with a luminosity of 21,900 Suns, consistent with an isochronal age of 12-14 million years and an estimated mass of 12-13 solar masses.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "6 Scorpii, Pi Scorpii, HIP 78265, SAO 183987, HD 143018, GC 21447, HR 5944, DM CD-25 11228, TYC 6783-2697-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Pi Scorpii",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "176.73",
	"RA_S" : 239.71297183,
	"DEC_S" : -26.11410794,
	"X" : 485,
	"Y" : 340,
	"Constellation" : "Scorpius ",
	"AMag" : 2.832,
	"key" : 66923,
	"title" : "Pi Scorpii"
	},
{
	"Index" : "46930",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 78650, SAO 184068, HD 143787, GC 21556, HR 5969, DM CD-2511295, TYC 6784-1424-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 5969",
	"OType" : "Star",
	"Distance" : "63.63",
	"RA_S" : 240.83592886,
	"DEC_S" : -25.86524237,
	"Constellation" : "Scorpius ",
	"AMag" : 5.105,
	"key" : 66930,
	"title" : "HR 5969"
	},
{
	"Index" : "38284",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Xi Scorpii, SAO 159665, HD 144070, HR 5978, DM BD-10  4237B, TYC 5619-1257-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Grafias (see HD144217,152334)",
	"OType" : "Star",
	"RA_S" : 241.09222735,
	"DEC_S" : -11.37310381,
	"Constellation" : "Scorpius ",
	"AMag" : 4.363,
	"key" : 58284,
	"title" : "Grafias (see HD144217,152334)"
	},
{
	"Index" : "71561",
	"Description" : "Xi Scorpii (\u03BE Sco, \u03BE Scorpii) is a star system in the constellation Scorpius. It was also 51 Lib.\r\rThe Xi Scorpii system consists of at least five stars in two groups separated by 4.67 arcminutes (or 0.08\u00B0) on the sky, corresponding to a distance of at least 8000 astronomical units (AU).\r\rThe brighter group contains Xi Scorpii A, B, and C. A and B are both yellow-white F-type stars. A is a slightly brighter and warmer magnitude +4.8 subgiant, while B is a magnitude +5.1 main sequence dwarf. They are separated by 0.76 arcseconds, or at least 21 AU, roughly a Sun\u2013Uranus distance, and orbit around a common centre once every 46 years. The magnitude +7.6 Xi Scorpii C orbits this pair at ten times the distance, having a separation of 7.6 arcseconds.\r\rThe second group contains Xi Scorpii D and E. Both D and E are K-type stars, which are separated by 11.5 arcseconds, more than 320 AU.\r\rXi Scorpii also possesses a sixth component, the 11th magnitude Xi Scorpii F, located 81 arcseconds from D. It is not known to be gravitationally bound to the other five components.\r\rXi Scorpii was a latter designation of 51 Librae.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Xi Scorpii, HIP 78727, SAO 159665, HD 144069J, GC 21593, HR 5977, DM BD-10 4237A",
	"group" : { "key" : "Scorpius" },
	"Common" : "Xi Scorpii",
	"OType" : "Spectroscopic binary",
	"RA_S" : 241.092462,
	"DEC_S" : -11.372944,
	"X" : 484,
	"Y" : 146,
	"Constellation" : "Scorpius ",
	"AMag" : 4.16,
	"key" : 91561,
	"title" : "Xi Scorpii"
	},
{
	"Index" : "42586",
	"Description" : "Beta Scorpii (\u03B2 Sco, \u03B2 Scorpii) is a multiple star system in the southern zodiac constellation of Scorpius. It has the traditional names Acrab, Akrab or Elacrab, all come from (Arabic: \u0627\u0644\u0639\u0642\u0631\u0628\u200E) al-\u0027Aqrab, the Scorpion, for the whole constellation, as well as Graffias, a name it shares with Xi Scorpii. It was known as \u623F\u5BBF\u56DB (the Fourth Star of the Room) in Chinese. Observed through a small telescope, Beta Scorpii appears as a binary star with a separation between the two components of 13.5 arcseconds. This pair, \u03B21 and \u03B22, form the top branches of the hierarchy of orbiting components in this system. \u03B21 Scorpii, the brighter of the pair, consists of two sub-components, \u03B2 Sco A and \u03B2 Sco B, orbiting at an angular separation of 3.9 arcseconds with an orbital period of 610 years. \u03B2 Sco A is itself a spectroscopic binary with the components \u03B2 Sco Aa and \u03B2 Sco Ab separated by 1.42 milliarcseconds and an orbital period of 6.82 days.\r\rThe second visual component, \u03B22 Scorpii, has two sub-components, \u03B2 Sco C and \u03B2 Sco E, orbiting at an angular separation of 0.1328 arcseconds with an orbital period of 39 years. \u03B2 Sco E is a spectroscopic binary with the components \u03B2 Sco Aa and \u03B2 Sco Ab having an orbital period of 10.7 days. This brings the total number of stars in the system to six. There is no D component; this is now an artifact of earlier system models.\r\rThe two most massive members of the system have the spectrum of B-type main sequence stars. Component C has a stellar classification of B2V. They are both hot stars at least 10 times as massive as our own Sun, and will have short lives. Both are expected to end their stellar evolution with massive Type II supernova explosions.\r\rThe Beta Scorpii system is a kinematic member of the Upper Scorpius subgroup of the Scorpius-Centaurus Association, a group of thousands of young stars with mean age 11 million years at distance 470 light years (145 parsecs). A recent analysis of the HR diagram position for the most massive star Beta-1 Scorpii A estimates its effective temperature to be 26,240 Kelvin with a luminosity of 19,500 Suns, consistent with an isochronal age of 11 million years and an estimated mass of 12 solar masses.\r\rBecause it is close to the ecliptic, Beta Scorpii can be occulted by the Moon and, very rarely, by planets. The last occultation by a planet took place on 13 May 1971, by Jupiter.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "8 Scorpii, Beta01 Scorpii, HIP 78820A, SAO 159682, HD 144217, GC 21609, HR 5984, DM BD-19  4307, TYC 6208-1623-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Acrab / Akrab / Elacrab",
	"OType" : "Spectroscopic binary",
	"Distance" : "122.54",
	"RA_S" : 241.35929993,
	"DEC_S" : -19.80545278,
	"X" : 473,
	"Y" : 255,
	"Constellation" : "Scorpius ",
	"AMag" : 2.592,
	"key" : 62586,
	"shortTitle" : "Acrab; Elacrab; Grafias (also HD144070,152334); Grassias; Akrab; Akrab; Ehlyakrab",
	"title" : "Acrab / Akrab / Elacrab"
	},
{
	"Index" : "42585",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "8 Scorpii, Beta02 Scorpii, HIP 78821C, SAO 159683, HD 144218, GC 21610, HR 5985, DM BD-19  4308, TYC 6208-1622-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Beta02 Scorpii",
	"OType" : "Spectroscopic binary",
	"Distance" : "119.18",
	"RA_S" : 241.36071368,
	"DEC_S" : -19.80190433,
	"Constellation" : "Scorpius ",
	"AMag" : 4.517,
	"key" : 62585,
	"title" : "Beta02 Scorpii"
	},
{
	"Index" : "42607",
	"Description" : "The Bayer designation Omega Scorpii (\u03C9 Sco, \u03C9 Scorpii) is shared by two stars, \u03C9\u00B9 Scorpii and \u03C9\u00B2 Scorpii, in the constellation Scorpius. They are separated by 0.24\u00B0 on the sky. Omega Scorpii also has the traditional name Jabhat al Akrab, which is derived from the Arabic \u062C\u0628\u0647\u0629 \u0627\u0644\u0639\u0642\u0631\u0628 jabhat al-caqrab meaning \u0022[The] forehead of the scorpion\u0022. Omega-1 Scorpii is a blue-white B-type dwarf with an apparent magnitude of +3.93. It is approximately 424 light years from Earth.\r\rOmega-1 Sco is one of the most massive members of the Upper Scorpius subgroup of the Scorpius-Centaurus Association, a group of thousands of young stars with mean age 11 million years at distance 470 light years (145 parsecs). A recent analysis of the HR diagram position for the star estimates its effective temperature to be 26,550 Kelvin with a luminosity of 9,120 Suns, consistent with an isochronal age of 5 million years and an estimated mass of 11 solar masses.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "9 Scorpii, Omega01 Scorpii, HIP 78933, SAO 184123, HD 144470, GC 21639, HR 5993, DM BD-20  4405, TYC 6212-1711-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Omega1 Scorpii",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "144.26",
	"RA_S" : 241.70177884,
	"DEC_S" : -20.66919173,
	"X" : 468,
	"Y" : 267,
	"Constellation" : "Scorpius ",
	"AMag" : 3.929,
	"key" : 62607,
	"title" : "Omega1 Scorpii"
	},
{
	"Index" : "42608",
	"Description" : "The Bayer designation Omega Scorpii (\u03C9 Sco, \u03C9 Scorpii) is shared by two stars, \u03C9\u00B9 Scorpii and \u03C9\u00B2 Scorpii, in the constellation Scorpius. They are separated by 0.24\u00B0 on the sky. Omega Scorpii also has the traditional name Jabhat al Akrab, which is derived from the Arabic \u062C\u0628\u0647\u0629 \u0627\u0644\u0639\u0642\u0631\u0628 jabhat al-caqrab meaning \u0022[The] forehead of the scorpion\u0022. Omega-2 Scorpii is a yellow G-type bright giant with an apparent magnitude of +4.31. It is approximately 265 light years from Earth.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "10 Scorpii, Omega02 Scorpii, HIP 78990, SAO 184135, HD 144608, GC 21659, HR 5997, DM BD-20  4408, TYC 6212-1712-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Omega2 Scorpii",
	"OType" : "Variable Star",
	"Distance" : "89.04",
	"RA_S" : 241.85136395,
	"DEC_S" : -20.86876363,
	"X" : 466,
	"Y" : 269,
	"Constellation" : "Scorpius ",
	"AMag" : 4.404,
	"key" : 62608,
	"title" : "Omega2 Scorpii"
	},
{
	"Index" : "51355",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 79199, SAO 207403, HD 144987, GC 21722, HR 6007, DM CD-3310961, TYC 7334-2611-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6007",
	"OType" : "Star",
	"Distance" : "124.76",
	"RA_S" : 242.4691256,
	"DEC_S" : -33.54580332,
	"Constellation" : "Scorpius ",
	"AMag" : 5.483,
	"key" : 71355,
	"title" : "HR 6007"
	},
{
	"Index" : "46982",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 79302, SAO 184197, HD 145250, GC 21749, HR 6017, DM CD-2912343, TYC 6792-2274-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6017",
	"OType" : "Star",
	"Distance" : "97.32",
	"RA_S" : 242.75862713,
	"DEC_S" : -29.41621848,
	"Constellation" : "Scorpius ",
	"AMag" : 5.227,
	"key" : 66982,
	"title" : "HR 6017"
	},
{
	"Index" : "42592",
	"Description" : "Nu Scorpii (\u03BD Sco, 14 Scorpii) is a star system in the constellation Scorpius.\r\rIt is at least a quintuple star, probably a septuple, consisting of two close groups that are separated by 41 arcseconds. The brighter group, Nu Scorpii A and B, is split by 1.3\u0022 and composed of spectral type B2 subgiants. The fainter pair, Nu Scorpii C and D, are spectral type B8 and B9 main sequence dwarfs split by 2.4\u0022. Nu Scorpii A is itself a semi-detached spectroscopic binary, having a fainter B-type companion separated by approximately 0.3 mas.\r\rSince it is near the ecliptic, Nu Scorpii can be occulted by the Moon and, very rarely, by planets. Mercury occulted it on 14 December 1821, but will not occult it again until 2 December 2031. The last occultation by Venus took place on 27 December 1852 and the next will take place on 30 December 2095. On 29 July 1808 there was an occultation by Neptune.\r\rNu Scorpii is the star which causes the reflection nebula cataloged as IC 4592. Reflection nebulae are actually made up of very fine dust that normally appears dark but can look quite blue when reflecting the light of energetic nearby stars.\r\rIn Chinese astronomy, Nu Scorpii is called \u9375\u9589, Pinyin: Ji\u00E0nb\u00EC, meaning Door Bolt, because this star is marking itself and stand alone in Door Bolt asterism, Room mansion (see : Chinese constellation). \u9375\u9589 (Ji\u00E0nb\u00EC), westernized into Keen Pi, but the name Keen Pi was designated for the formation of \u03BB Sco (Shaula) and \u03C5 Sco (Lesath) by R.H. Allen and the meaning is \u0022the Two Parts of a Lock.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "14 Scorpii, Nu Scorpii, HIP 79374A, SAO 159764, HD 145502A, GC 21773, HR 6027, DM BD-19  4333, TYC 6209-1537-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Nu Scorpii",
	"OType" : "Double or multiple star",
	"Distance" : "143.25",
	"RA_S" : 242.998917,
	"DEC_S" : -19.460647,
	"X" : 453,
	"Y" : 250,
	"Constellation" : "Scorpius ",
	"AMag" : 4.35,
	"key" : 62592,
	"shortTitle" : "Lesath (also HD158408)",
	"title" : "Nu Scorpii"
	},
{
	"Index" : "42593",
	"Description" : "Nu Scorpii (\u03BD Sco, 14 Scorpii) is a star system in the constellation Scorpius.\r\rIt is at least a quintuple star, probably a septuple, consisting of two close groups that are separated by 41 arcseconds. The brighter group, Nu Scorpii A and B, is split by 1.3\u0022 and composed of spectral type B2 subgiants. The fainter pair, Nu Scorpii C and D, are spectral type B8 and B9 main sequence dwarfs split by 2.4\u0022. Nu Scorpii A is itself a semi-detached spectroscopic binary, having a fainter B-type companion separated by approximately 0.3 mas.\r\rSince it is near the ecliptic, Nu Scorpii can be occulted by the Moon and, very rarely, by planets. Mercury occulted it on 14 December 1821, but will not occult it again until 2 December 2031. The last occultation by Venus took place on 27 December 1852 and the next will take place on 30 December 2095. On 29 July 1808 there was an occultation by Neptune.\r\rNu Scorpii is the star which causes the reflection nebula cataloged as IC 4592. Reflection nebulae are actually made up of very fine dust that normally appears dark but can look quite blue when reflecting the light of energetic nearby stars.\r\rIn Chinese astronomy, Nu Scorpii is called \u9375\u9589, Pinyin: Ji\u00E0nb\u00EC, meaning Door Bolt, because this star is marking itself and stand alone in Door Bolt asterism, Room mansion (see : Chinese constellation). \u9375\u9589 (Ji\u00E0nb\u00EC), westernized into Keen Pi, but the name Keen Pi was designated for the formation of \u03BB Sco (Shaula) and \u03C5 Sco (Lesath) by R.H. Allen and the meaning is \u0022the Two Parts of a Lock.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "14 Scorpii, Nu Scorpii, HIP 79374B, SAO 159764, HD 145502B, GC 21773, HR 6027, DM BD-19  4333, TYC 6209-1537-2",
	"group" : { "key" : "Scorpius" },
	"Common" : "Nu Scorpii",
	"OType" : "Star",
	"Distance" : "143.25",
	"RA_S" : 242.998942,
	"DEC_S" : -19.460261,
	"X" : 453,
	"Y" : 250,
	"Constellation" : "Scorpius ",
	"AMag" : 5.309,
	"key" : 62593,
	"shortTitle" : "Lesath (also HD158408)",
	"title" : "Nu Scorpii"
	},
{
	"Index" : "38271",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "15 Scorpii, Psi Scorpii, HIP 79375, SAO 141022, HD 145570, GC 21780, HR 6031, DM BD-09  4324, TYC 5616-1294-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Psi Scorpii",
	"OType" : "Star",
	"Distance" : "47.47",
	"RA_S" : 242.9999829,
	"DEC_S" : -10.06422024,
	"Constellation" : "Scorpius ",
	"AMag" : 4.942,
	"key" : 58271,
	"title" : "Psi Scorpii"
	},
{
	"Index" : "38251",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "16 Scorpii, HIP 79387, SAO 141024, HD 145607, GC 21784, HR 6033, DM BD-08  4180, TYC 5612-1227-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "16 Scorpii",
	"OType" : "Star",
	"Distance" : "77.22",
	"RA_S" : 243.03047693,
	"DEC_S" : -8.54757962,
	"Constellation" : "Scorpius ",
	"AMag" : 5.441,
	"key" : 58251,
	"title" : "16 Scorpii"
	},
{
	"Index" : "47031",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "13 Scorpii, c02 Scorpii, HIP 79404, SAO 184221, HD 145482, GC 21778, HR 6028, DM CD-27 10841, TYC 6801-1004-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "c02 Scorpii",
	"OType" : "Spectroscopic binary",
	"Distance" : "146.75",
	"RA_S" : 243.07585418,
	"DEC_S" : -27.92637613,
	"Constellation" : "Scorpius ",
	"AMag" : 4.543,
	"key" : 67031,
	"title" : "c02 Scorpii"
	},
{
	"Index" : "38296",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "17 Scorpii, Chi Scorpii, HIP 79540, SAO 159793, HD 145897, GC 21828, HR 6048, DM BD-11  4096, TYC 5621-1388-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Chi Scorpii",
	"OType" : "Star",
	"Distance" : "115.78",
	"RA_S" : 243.4621078,
	"DEC_S" : -11.83774529,
	"Constellation" : "Scorpius ",
	"AMag" : 5.398,
	"key" : 58296,
	"title" : "Chi Scorpii"
	},
{
	"Index" : "47062",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "d Scorpii, HIP 79881, SAO 184301, HD 146624, GC 21910, HR 6070, DM CD-28 12037, TYC 6805-1909-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "d Scorpii",
	"OType" : "High proper-motion Star",
	"Distance" : "41.28",
	"RA_S" : 244.57458134,
	"DEC_S" : -28.61401816,
	"Constellation" : "Scorpius ",
	"AMag" : 4.785,
	"key" : 67062,
	"title" : "d Scorpii"
	},
{
	"Index" : "46999",
	"Description" : "Omicron Scorpii (\u03BF Sco, \u03BF Scorpii) is a star in the constellation Scorpius. It is a white A-type bright giant with an apparent magnitude of +4.57 located approximately 1,200 light years from Earth. This star has about eight times the mass of the Sun and is roughly 40 million years old.\r\rThe star is radiating around 3,200 times the luminosity of the Sun from its outer atmosphere at an effective temperature of about 8,100 K. While it was occasionally mentioned as a possible member of the Upper Scorpius sub-group in the Scorpius-Centaurus OB association during the 20th century, it does not appear in more recent membership lists for this group due to its small proper motion and small trigonometric parallax as measured by Hipparcos, which is suggestive that it is a background star unrelated to Scorpius-Centaurus.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "19 Scorpii, Omicron Scorpii, HIP 80079, SAO 184329, HD 147084, GC 21969, HR 6081, DM CD-23 12849, TYC 6794-552-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Omicron Scorpii",
	"OType" : "Variable Star",
	"Distance" : "262.86",
	"RA_S" : 245.15908172,
	"DEC_S" : -24.16932398,
	"X" : 423,
	"Y" : 309,
	"Constellation" : "Scorpius ",
	"AMag" : 4.665,
	"key" : 66999,
	"title" : "Omicron Scorpii"
	},
{
	"Index" : "47018",
	"Description" : "Sigma Scorpii (\u03C3 Sco, \u03C3 Scorpii) is a star system in the constellation Scorpius. It has the traditional name Al Niyat, although this name is sometimes also applied to Tau Scorpii, or to the asterism formed by both Sigma and Tau. This system has a combined apparent visual magnitude of +2.88, making it one of the brighter members of the constellation, although greatly outshone by its neighbor Antares. Based upon parallax measurements made during the Hipparcos mission, the distance to Sigma Scorpii is roughly 696 light years (214 parsecs). North et al. (2007) computed a more accurate estimate of 568+75\u221259 light years (174+23\u221218 parsecs). The brightest component of the system is a double-lined spectroscopic binary, which means that the pair has not been resolved using a telescope. Instead, their orbit is determined by changes in their combined spectrum caused by the Doppler shift. This indicates that the pair complete an orbit every 33.01 days and have an orbital eccentricity of 0.32.\r\rThe primary component of the spectroscopic binary, \u03C3 Scorpii A, is an evolved giant star with a stellar classification of B1 III. It has around 18 times the mass of the Sun and 12 times the Sun\u0027s radius. This star is radiating about 29,000 times the luminosity of the Sun from its outer envelope at an effective temperature of 26,150 K. This is a variable star of the Beta Cephei type, causing the apparent magnitude to vary between +2.86 and +2.94 with multiple periods of 0.2468429, 0.239671, and 8.2 days. During each pulsation cycle, the temperature of the star varies by 4,000 \u00B1 2,000 K.\r\rThe other member of the core pair, \u03C3 Scorpii B, is a main sequence star with a classification of B1 V. Orbiting this binary at a separation half an arcsecond, or at least 120 Astronomical Units (AU), four times the Sun\u2013Neptune distance, is the magnitude +5.2 \u03C3 Scorpii C, which has an orbital period of over a hundred years. Even farther out at 20 arcseconds, or more than 4500 AU, is \u03C3 Scorpii D with a magnitude of +8.7. It is classified as a B9 dwarf.\r\rGiven its position, youth, and space velocity, the Sigma Scorpii system is a likely member of the Gould Belt, and in particular the Upper Scorpius subgroup of the Scorpius-Centaurus Association (Sco OB2). Recent isochronal age estimates for the Sigma Scorpii system yield ages of 8\u201310 million years through comparison of the HR diagram positions for the stars to modern evolutionary tracks. This agrees well with mean age for the Upper Scorpius group which is approximately 11 million years.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "20 Scorpii, Sigma Scorpii, HIP 80112AC, SAO 184336, HD 147165, GC 21982, HR 6084, DM CD-25 11485, TYC 6798-540-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Al Niyat",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "209.54",
	"RA_S" : 245.29713575,
	"DEC_S" : -25.59280657,
	"X" : 420,
	"Y" : 328,
	"Constellation" : "Scorpius ",
	"AMag" : 2.911,
	"key" : 67018,
	"shortTitle" : "Al Niyat (with HD149438)",
	"title" : "Al Niyat"
	},
{
	"Index" : "55942",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 80337, SAO 207622, HD 147513, GC 22030, HR 6094, DM CD-3810983, TYC 7853-621-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Gliese 620.1 A (HR 6094)",
	"OType" : "Pre-main sequence Star",
	"Distance" : "12.78",
	"RA_S" : 246.00537232,
	"DEC_S" : -39.19297957,
	"Constellation" : "Scorpius ",
	"AMag" : 5.441,
	"key" : 75942,
	"title" : "Gliese 620.1 A (HR 6094)"
	},
{
	"Index" : "55943",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 80390, SAO 207637, HD 147628, GC 22043, HR 6100, DM CD-3710778, TYC 7853-675-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6100",
	"OType" : "Double or multiple star",
	"Distance" : "128.87",
	"RA_S" : 246.13230965,
	"DEC_S" : -37.56604698,
	"Constellation" : "Scorpius ",
	"AMag" : 5.397,
	"key" : 75943,
	"title" : "HR 6100"
	},
{
	"Index" : "47024",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "22 Scorpii, i Scorpii, HIP 80815, SAO 184429, HD 148605, GC 22179, HR 6141, DM CD-24 12695, TYC 6799-932-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "i Scorpii",
	"OType" : "Star in Nebula",
	"Distance" : "126.6",
	"RA_S" : 247.55198134,
	"DEC_S" : -25.11522081,
	"Constellation" : "Scorpius ",
	"AMag" : 4.759,
	"key" : 67024,
	"title" : "i Scorpii"
	},
{
	"Index" : "51475",
	"Description" : "N Scorpii (N Sco) is a blue giant star in the constellation Scorpius. Its apparent magnitude is 4.22.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "N Scorpii, HIP 80911, SAO 207732, HD 148703, GC 22195, HR 6143, DM CD-34 11044, TYC 7353-3152-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "N Scorpii",
	"OType" : "Variable Star",
	"Distance" : "169.86",
	"RA_S" : 247.84555582,
	"DEC_S" : -34.70436902,
	"X" : 386,
	"Y" : 444,
	"Constellation" : "Scorpius ",
	"AMag" : 4.202,
	"key" : 71475,
	"title" : "N Scorpii"
	},
{
	"Index" : "55996",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 80945, SAO 226855, HD 148688, GC 22198, HR 6142, DM CD-4110695, TYC 7862-1036-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6142",
	"OType" : "Blue supergiant star",
	"Distance" : "833.3333",
	"RA_S" : 247.92403496,
	"DEC_S" : -41.81714208,
	"Constellation" : "Scorpius ",
	"AMag" : 5.355,
	"key" : 75996,
	"title" : "HR 6142"
	},
{
	"Index" : "47074",
	"Description" : "Tau Scorpii is a star in the southern zodiac constellation of Scorpius. It has the traditional name Alniyat or Al Niyat, which it shares with \u03C3 Scorpii. The name derives from the Arabic \u0627\u0644\u0646\u064A\u0627\u0637 an-niy\u0101\u0163 meaning \u0022the arteries\u0022. The apparent visual magnitude of Tau Scorpii is +2.8, while parallax measurements yield a distance estimate of roughly 470 light-years (150 parsecs) from Earth.  The spectrum of this star shows triply-ionized oxygen (O IV) that is being generated by X-rays and the Auger ionization effect. Observations with the ROSAT space telescope showed it has a higher energy (harder) X-ray spectrum than is usual for B0 V stars. Over the energy range 0.8\u20131.2 keV, its X-ray luminosity is Lx = 1.8 \u00D7 1031 erg s\u20131 with a large Lx to Lbol of log Lx/Lbol = \u20136.53 from ASCA measurements. ROSAT measurements showed a log Lx/Lbol \u2243 \u20135.93 for the range 0.1-2.4 keV. The hard component of the X-ray spectrum from \u03C4 Sco as studied with XMM-Newton supports the presence of in-falling clumps of plasma in \u03C4 Sco.\r\rThis star is a proper motion member of the Upper Scorpius subgroup of the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. The Upper Scorpius subgroup contains thousands of young stars with mean age 11 million years at average distance of 470 light years (145 parsecs) A more recent analysis of the HR diagram position for Tau Scorpii estimates its effective temperature to be 29,850 Kelvin with a luminosity of 20,400 Suns, consistent with an isochronal age of 5 million years and an estimated mass of 14.5-14.7 solar masses.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "23 Scorpii, Tau Scorpii, HIP 81266, SAO 184481, HD 149438, GC 22303, HR 6165, DM CD-27 11015, TYC 6807-1012-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Alniyat",
	"OType" : "Star",
	"Distance" : "137.13",
	"RA_S" : 248.97063838,
	"DEC_S" : -28.21601356,
	"X" : 376,
	"Y" : 360,
	"Constellation" : "Scorpius ",
	"AMag" : 2.759,
	"key" : 67074,
	"shortTitle" : "Al Niyat (with HD147165)",
	"title" : "Alniyat"
	},
{
	"Index" : "51476",
	"Description" : "H Scorpii (H Sco) is a star in the constellation Scorpius. Its apparent magnitude is 4.18.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "H Scorpii, HIP 81304, SAO 207814, HD 149447, GC 22311, HR 6166, DM CD-34 11112, TYC 7353-3153-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "H Scorpii",
	"OType" : "Variable Star",
	"Distance" : "105.01",
	"RA_S" : 249.09363443,
	"DEC_S" : -35.2553257,
	"X" : 372,
	"Y" : 451,
	"Constellation" : "Scorpius ",
	"AMag" : 4.346,
	"key" : 71476,
	"title" : "H Scorpii"
	},
{
	"Index" : "56120",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 82493, SAO 227313, HD 151804, GC 22669, HR 6245, DM CD-4110957, TYC 7872-2284-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6245",
	"OType" : "Pulsating variable Star",
	"RA_S" : 252.89050688,
	"DEC_S" : -41.23053271,
	"Constellation" : "Scorpius ",
	"AMag" : 5.249,
	"key" : 76120,
	"title" : "HR 6245"
	},
{
	"Index" : "56045",
	"Description" : "Mu1 Scorpii (\u03BC1 Sco, \u03BC1 Scorpii) is a binary star system in the southern zodiac constellation of Scorpius. The combined apparent visual magnitude of the pair is +3.04, making it one of the brighter members of Scorpius. Based upon parallax measurements, the distance of this system from the Earth is roughly 500 light years (150 parsecs). This system is a member of the Scorpius-Centaurus Association, the nearest OB association of co-moving stars to the Sun.\r\r\u03BC1 Scorpii is an eclipsing binary of the Beta Lyrae type. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. The two stars revolve each other along a circular orbit with the components separated by 12.9 times the radius of the Sun. Due to occultation of each component by the other, the apparent magnitude of the system decreased by 0.3 and 0.4 magnitudes over the course of the binary\u0027s orbit, which takes 34 hours 42.6 minutes to complete.\r\rThe primary component is a B-type main sequence star with a stellar classification of B1.5 V. It has 8.5 times the mass of the Sun and 4.1 times the Sun\u0027s radius. The secondary member is a smaller B-type main sequence star with a classification of about B6.5 V, having 5.3 times the Sun\u0027s mass and 4.4 times the radius of the Sun. The effective temperature of the outer atmosphere for each star is 23,725 K for the primary and 16,850 K for the secondary. At these temperatures, the two stars glow with a blue-white hue.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Mu01 Scorpii, HIP 82514, SAO 208102, HD 151890, GC 22677, HR 6247, DM CD-37 11033, TYC 7868-1821-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Mu1 Scorpii",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "150.09",
	"RA_S" : 252.96762965,
	"DEC_S" : -38.04738039,
	"X" : 331,
	"Y" : 487,
	"Constellation" : "Scorpius ",
	"AMag" : 2.971,
	"key" : 76045,
	"title" : "Mu1 Scorpii"
	},
{
	"Index" : "56044",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Mu02 Scorpii, HIP 82545, SAO 208116, HD 151985, GC 22691, HR 6252, DM CD-37 11037, TYC 7868-1820-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Mu02 Scorpii",
	"OType" : "Variable Star",
	"Distance" : "145.3",
	"RA_S" : 253.0839355,
	"DEC_S" : -38.01753493,
	"Constellation" : "Scorpius ",
	"AMag" : 3.508,
	"key" : 76044,
	"title" : "Mu02 Scorpii"
	},
{
	"Index" : "56183",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Zeta01 Scorpii, HIP 82671, SAO 227375, HD 152236, GC 22730, HR 6262, DM CD-42 11633, TYC 7876-2743-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Zeta01 Scorpii",
	"OType" : "Blue supergiant star",
	"Distance" : "752.41",
	"RA_S" : 253.49886066,
	"DEC_S" : -42.36202508,
	"Constellation" : "Scorpius ",
	"AMag" : 4.817,
	"key" : 76183,
	"title" : "Zeta01 Scorpii"
	},
{
	"Index" : "56165",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 82676AB, SAO 227377, HD 152234, GC 22733, HR 6260, DM CD-4111024, TYC 7876-2191-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6260",
	"OType" : "Spectroscopic binary",
	"Distance" : "793.6508",
	"RA_S" : 253.5076655,
	"DEC_S" : -41.80638311,
	"Constellation" : "Scorpius ",
	"AMag" : 5.466,
	"key" : 76165,
	"title" : "HR 6260"
	},
{
	"Index" : "56186",
	"Description" : "Zeta2 Scorpii (Zeta2 Sco, \u03B62 Scorpii, \u03B62 Sco) is a K-type orange giant star in the constellation of Scorpius. It has an apparent visual magnitude which varies between 3.59 and 3.65, and is located near the blue-white supergiant star Zeta-1 Scorpii in our sky, although it is, in astronomical terms, far more distant and unrelated to Zeta-1 Scorpii except for line-of sight co-incidence. Zeta-1 is 5,700 light-years away and probably an outlying member of open star cluster NGC 6231, also known as the \u0022northern jewel box\u0022 cluster, whereas Zeta-2 is a mere 151 lightyears distant and thus much less luminous in real terms. Zeta-2 Scorpii can also be distinguished from its optical partner, Zeta-1, because of Zeta-2\u0027s orangish colour especially in long-exposure astrophographs.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Zeta02 Scorpii, HIP 82729, SAO 227402, HD 152334, GC 22751, HR 6271, DM CD-42 11646, TYC 7876-2871-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Zeta2 Scorpii",
	"OType" : "Variable Star",
	"Distance" : "40.56",
	"RA_S" : 253.64585971,
	"DEC_S" : -42.36131128,
	"X" : 325,
	"Y" : 543,
	"Constellation" : "Scorpius ",
	"AMag" : 3.764,
	"key" : 76186,
	"title" : "Zeta2 Scorpii"
	},
{
	"Index" : "51575",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 83336, SAO 208324, HD 153613, GC 22942, HR 6316, DM CD-3113473, TYC 7364-2287-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6316",
	"OType" : "Star",
	"Distance" : "136.55",
	"RA_S" : 255.46934373,
	"DEC_S" : -32.14352536,
	"Constellation" : "Scorpius ",
	"AMag" : 4.995,
	"key" : 71575,
	"title" : "HR 6316"
	},
{
	"Index" : "51611",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "k Scorpii, HIP 83574, SAO 208377, HD 154090, GC 23019, HR 6334, DM CD-33 11706, TYC 7368-1546-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "k Scorpii",
	"OType" : "Blue supergiant star",
	"RA_S" : 256.20563325,
	"DEC_S" : -34.12292923,
	"Constellation" : "Scorpius ",
	"AMag" : 4.886,
	"key" : 71611,
	"title" : "k Scorpii"
	},
{
	"Index" : "56251",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 84033, SAO 227688, HD 154948, GC 23148, HR 6371, DM CD-4411502, TYC 7882-570-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6371",
	"OType" : "Star",
	"Distance" : "96.73",
	"RA_S" : 257.67634366,
	"DEC_S" : -44.55770735,
	"Constellation" : "Scorpius ",
	"AMag" : 5.157,
	"key" : 76251,
	"title" : "HR 6371"
	},
{
	"Index" : "56250",
	"Description" : "Eta Scorpii (\u03B7 Sco, \u03B7 Scorpii) is a star in the southern zodiac constellation of Scorpius. With an apparent visual magnitude of 3.33, this is one of the brighter members of the Scorpius and is the furthest south of the constellation stars with a Bayer designation. The distance to this star can be estimated using parallax measurements, yielding a value of 73.5 light-years (22.5 parsecs) with a 0.4% margin of error.\r\rThe stellar classification of this star has undergone some revision over time, with the star being classified anywhere from an F-type main sequence star to a giant star. In 2006, the NStars program assigned it a class of F5 IV, where the luminosity class of \u0027IV\u0027 indicates this is a subgiant star that is exhausting the supply of hydrogen at its core and is in the process of evolving into a giant star. It has around 175% of the Sun\u0027s mass with an estimated age of 1.1 billion years. The star is radiating about 18 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 6,519 K. It is this heat that gives it a yellow-white hue that is typical for an F-type star.\r\rEta Scorpii is rotating rapidly, with a projected rotational velocity of 150 km s\u20131. This is causing the star to spin on its axis with a period of less than a day. It is an X-ray emitter with its stellar corona giving off an X-ray luminosity of 4.4 \u00D7 1028 ergs s\u20131. In 1991 it was identified as a possible barium star, as it displays an enhanced abundance of the element barium in its spectrum. Overall, the abundance of elements other than hydrogen and helium, what astronomers term the star\u0027s metallicity, is similar to the abundance in the Sun.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Eta Scorpii, HIP 84143, SAO 227707, HD 155203, GC 23180, HR 6380, DM CD-43 11485, TYC 7882-569-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Eta Scorpii",
	"OType" : "High proper-motion Star",
	"Distance" : "22.53",
	"RA_S" : 258.03830303,
	"DEC_S" : -43.2391912,
	"X" : 283,
	"Y" : 555,
	"Constellation" : "Scorpius ",
	"AMag" : 3.359,
	"key" : 76250,
	"title" : "Eta Scorpii"
	},
{
	"Index" : "56429",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 85162, SAO 227911, HD 157243, GC 23503, HR 6460, DM CD-4411669, TYC 7895-5293-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6460",
	"OType" : "Star",
	"Distance" : "225.51",
	"RA_S" : 261.05453461,
	"DEC_S" : -44.16257102,
	"Constellation" : "Scorpius ",
	"AMag" : 5.097,
	"key" : 76429,
	"title" : "HR 6460"
	},
{
	"Index" : "51861",
	"Description" : "Upsilon Scorpii (\u03C5 Sco, \u03C5 Scorpii) is a star located in the \u0022stinger\u0022 of the southern zodiac constellation of Scorpius, the scorpion. It has the traditional name Lesath (alternative spellings Leschath, Lesuth), from Arabic las\u0027a = \u0022pass (or bite) of a poisonous animal\u0022; but this is a miscorrection by Scaliger (a European astronomer who knew Arabic) for earlier \u0022Alascha\u0022, which came from Arabic al la\u0163kha = \u0022the foggy patch\u0022, referring to the nearby open cluster M7. On the night sky it lies near the 1.6 magnitude star Lambda Scorpii, so the two form an optical pair that is sometimes called the \u0022Cat\u0027s Eyes\u0022.\r\rThis star has apparent magnitude +2.7 and belongs to spectral class B2 IV, with the luminosity class of \u0027IV\u0027 indicating it is a subgiant star. From parallax measurements, it is approximately 580 light years from Earth. The star\u0027s luminosity is 12,300 times that of the Sun, while its surface temperature is 22,831 kelvins. The star has a radius of 6.1 times solar and 11 times the mass of the Sun.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "34 Scorpii, Upsilon Scorpii, HIP 85696, SAO 208896, HD 158408, GC 23693, HR 6508, DM CD-37 11638, TYC 7387-1249-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Lesath",
	"OType" : "Star",
	"Distance" : "176.46",
	"RA_S" : 262.69097937,
	"DEC_S" : -37.29581257,
	"X" : 231,
	"Y" : 482,
	"Constellation" : "Scorpius ",
	"AMag" : 2.624,
	"key" : 71861,
	"shortTitle" : "Lesuth; Lezat; Lezakh",
	"title" : "Lesath"
	},
{
	"Index" : "56273",
	"Description" : "Q Scorpii (Q Sco) is a star in the constellation Scorpius. Its apparent magnitude is 4.27.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Q Scorpii, HIP 86170, SAO 209019, HD 159433, GC 23846, HR 6546, DM CD-38 12044, TYC 7884-2876-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Q Scorpii",
	"OType" : "High proper-motion Star",
	"Distance" : "50.21",
	"RA_S" : 264.13683545,
	"DEC_S" : -38.635355,
	"X" : 218,
	"Y" : 501,
	"Constellation" : "Scorpius ",
	"AMag" : 4.388,
	"key" : 76273,
	"title" : "Q Scorpii"
	},
{
	"Index" : "56394",
	"Description" : "Theta Scorpii (\u03B8 Sco, \u03B8 Scorpii) is a star in the southern zodiac constellation of Scorpius. It has the traditional name Sargas, of Sumerian origin. In Chinese, it is referred to as \u5C3E\u5BBF\u4E94 (Mandarin: w\u011Bi xi\u00F9 w\u01D4), the Fifth Star of the Tail. The apparent visual magnitude of this star is +1.87, making it readily visible to the naked eye and one of the brightest stars in the night sky. It is sufficiently near that the distance can be measured directly using the parallax technique, which yields an estimate of roughly 300 light years (90 parsecs).\r\rThis is an evolved bright giant star with a stellar classification of F0 II. With a mass 5.7 times that of the Sun, it has expanded to about 26 times the Sun\u0027s radius. It is radiating 1,834 times as much luminosity as the Sun from its outer envelope at an effective temperature of 7,268, giving it the yellow-white hued glow of an F-type star.\r\rIt has a magnitude 5.36 companion at an angular separation of 6.470 arcseconds.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Theta Scorpii, HIP 86228B, SAO 228201, HD 159532B, GC 23857, HR 6553, DM CD-42 12312, TYC 7892-7679-2",
	"group" : { "key" : "Scorpius" },
	"Common" : "Sargas",
	"OType" : "Star",
	"Distance" : "82.91",
	"RA_S" : 264.327967,
	"DEC_S" : -42.996561,
	"X" : 223,
	"Y" : 558,
	"Constellation" : "Scorpius ",
	"AMag" : 5.363,
	"key" : 76394,
	"title" : "Sargas"
	},
{
	"Index" : "56343",
	"Description" : "Iota1 Scorpii (\u03B91 Scorpii) is star in the southern constellation of Scorpius. With an apparent visual magnitude of 3.03, this star can be seen with the naked eye. It is sometimes called by the proper name Apollyon. Parallax measurements place it at a distance of roughly 1,930 light-years (590 parsecs) from Earth, with a 9% margin of error.\r\rThis star has a stellar classification of F2 Ia, with the \u0027Ia\u0027 luminosity class indicating this is an evolved star that has expanded to become a supergiant. It has about 12 times the Sun\u0027s mass and is radiating about 35,070 times the Sun\u0027s luminosity. The radius is uncertain, with estimates ranging from 125 to 400 times that of the Sun. The effective temperature of the outer envelope is about 7,000 K, which gives it a yellow-white hue typical of an F-type star.\r\rIota1 Scorpii has a 10th magnitude companion at an angular separation of 37.5 arcseconds, which, at the distance of this star, gives it a projected physical separation of 20,000 Astronomical Units (AU). As the relative separation of the two stars along the line of sight to the Earth is not known, however, this distance represents only a minimum value for their separation.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Iota01 Scorpii, HIP 87073, SAO 228420, HD 161471, GC 24125, HR 6615, DM CD-40 11838, TYC 7889-2669-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Apollyon",
	"OType" : "Emission-line Star",
	"Distance" : "586.17",
	"RA_S" : 266.89617172,
	"DEC_S" : -40.12699529,
	"X" : 193,
	"Y" : 524,
	"Constellation" : "Scorpius ",
	"AMag" : 3.05,
	"key" : 76343,
	"title" : "Apollyon"
	},
{
	"Index" : "51690",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 87220, SAO 209303, HD 161840, GC 24176, HR 6628, DM CD-3114609, TYC 7377-1056-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6628",
	"OType" : "Star",
	"Distance" : "170.25",
	"RA_S" : 267.29365427,
	"DEC_S" : -31.70320547,
	"Constellation" : "Scorpius ",
	"AMag" : 4.79,
	"key" : 71690,
	"title" : "HR 6628"
	},
{
	"Index" : "51894",
	"Description" : "G Scorpii (G Sco) is a star in the constellation Scorpius. It is an orange K-type giant with an apparent magnitude of +3.19. It is approximately 126 light years from Earth. The measured angular diameter of the primary star is 3.94 \u00B1 0.21 mas. At the estimated distance of this system, this yields a physical size of about 16 times the radius of the Sun.\r\rJust 8.5 arcminutes to the east is the globular cluster NGC 6441.\r\rIt was formerly known as \u0022Gamma Telescopii\u0022 (\u03B3 Tel) and \u0022Fuyue\u0022 \uFF08\u5085\u8AAA\uFF09 in ancient China.",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "G Scorpii, HIP 87261, SAO 209318, HD 161892, GC 24188, HR 6630, DM CD-37 11907, TYC 7389-2159-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "G Scorpii",
	"OType" : "Star",
	"Distance" : "38.58",
	"RA_S" : 267.46451837,
	"DEC_S" : -37.04330034,
	"X" : 181,
	"Y" : 485,
	"Constellation" : "Scorpius ",
	"AMag" : 3.315,
	"key" : 71894,
	"title" : "G Scorpii"
	},
{
	"Index" : "56363",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "Iota02 Scorpii, HIP 87294, SAO 228466, HD 161912, GC 24197, HR 6631, DM CD-40 11886, TYC 7890-2436-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "Iota02 Scorpii",
	"OType" : "Star",
	"Distance" : "749.63",
	"RA_S" : 267.54629866,
	"DEC_S" : -40.090434,
	"Constellation" : "Scorpius ",
	"AMag" : 4.833,
	"key" : 76363,
	"title" : "Iota02 Scorpii"
	},
{
	"Index" : "56469",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 87846, SAO 228562, HD 163145, GC 24374, HR 6675, DM CD-4412201, TYC 7898-2022-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6675",
	"OType" : "Star",
	"Distance" : "88.48",
	"RA_S" : 269.19758923,
	"DEC_S" : -44.34224252,
	"Constellation" : "Scorpius ",
	"AMag" : 4.982,
	"key" : 76469,
	"title" : "HR 6675"
	},
{
	"Index" : "56418",
	"MapNum" : "38",
	"ImageNum" : "38",
	"Desig" : "HIP 87936, SAO 228578, HD 163376, GC 24402, HR 6682, DM CD-4112231, TYC 7894-3355-1",
	"group" : { "key" : "Scorpius" },
	"Common" : "HR 6682",
	"OType" : "Variable Star",
	"Distance" : "138.27",
	"RA_S" : 269.44918043,
	"DEC_S" : -41.71629653,
	"Constellation" : "Scorpius ",
	"AMag" : 5.066,
	"key" : 76418,
	"title" : "HR 6682"
	},
{
	"Index" : "44088",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Zeta Sculptoris, HIP 183, HD 224990, GC 33337, HR 9091, DM CD-30 19790, TYC 6418-1221-1",
	"group" : { "backgroundImage" : "images/Alignment/36.png",
		"description" : "Sculptor is a small and faint constellation in the southern sky. It represents a sculptor. It was introduced by Nicolas Louis de Lacaille in the 18th century. He originally named it Apparatus Sculptoris (the sculptor\u0027s studio), but the name was later shortened.\r\rNo stars brighter than 3rd magnitude are located in Sculptor. This is explained by the fact that Sculptor contains the south galactic pole where stellar density is very low.\r\rThe brightest is \u03B1 Sculptoris, an SX Arietis-type variable star with the magnitude of only 4.31m. The constellation also contains the Sculptor Dwarf, a dwarf galaxy which is a member of the Local Group, as well as the Sculptor Group, the group of galaxies closest to the Local Group. The Sculptor Galaxy (NGC 253), a barred spiral galaxy and the largest member of the group, lies near the border between Sculptor and Cetus. Another prominent member of the group is the irregular galaxy NGC 55.\r\rOne unique galaxy in Sculptor is the Cartwheel Galaxy, at a distance of 500 million light-years. The result of a merger around 300 million years ago, the Cartwheel Galaxy has a core of older, yellow stars, and an outer ring of younger, blue stars, which has a diameter of 100,000 light-years. The smaller galaxy in the collision is now incorporated into the core, after moving from a distance of 250,000 light-years. The shock waves from the collision sparked extensive star formation in the outer ring.",
		"key" : "Sculptor",
		"grouptype" : "Sculptor",
		"Meaning" : "sculptor",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Sculptor",
		"title" : "Sculptor Objects Group" },
	"Common" : "Zeta Sculptoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "153.81",
	"RA_S" : 0.58301191,
	"DEC_S" : -29.72041312,
	"Constellation" : "Sculptor ",
	"AMag" : 4.999,
	"key" : 64088,
	"title" : "Zeta Sculptoris"
	},
{
	"Index" : "48429",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Theta Sculptoris, HIP 950, SAO 192388, HD 739, GC 202, HR 35, DM CD-35    42, TYC 6995-1262-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Theta Sculptoris",
	"OType" : "High proper-motion Star",
	"Distance" : "21.28",
	"RA_S" : 2.93337139,
	"DEC_S" : -35.13311562,
	"Constellation" : "Sculptor ",
	"AMag" : 5.289,
	"key" : 68429,
	"title" : "Theta Sculptoris"
	},
{
	"Index" : "44097",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Iota Sculptoris, HIP 1708, SAO 166207, HD 1737, GC 433, HR 84, DM CD-29    86, TYC 6419-1055-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Iota Sculptoris",
	"OType" : "Red Giant Branch star",
	"Distance" : "101.11",
	"RA_S" : 5.37999326,
	"DEC_S" : -28.98146943,
	"Constellation" : "Sculptor ",
	"AMag" : 5.278,
	"key" : 64097,
	"title" : "Iota Sculptoris"
	},
{
	"Index" : "48421",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Eta Sculptoris, HIP 2210, SAO 192545, HD 2429, GC 544, HR 105, DM CD-33   152, TYC 6994-1104-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Eta Sculptoris",
	"OType" : "Long-period variable star",
	"Distance" : "137.68",
	"RA_S" : 6.98207067,
	"DEC_S" : -33.00716675,
	"Constellation" : "Sculptor ",
	"AMag" : 5.062,
	"key" : 68421,
	"title" : "Eta Sculptoris"
	},
{
	"Index" : "44168",
	"Description" : "Alpha Sculptoris (\u03B1 Scl, \u03B1 Sculptoris) is the Bayer designation for a star in the southern constellation of Sculptor. It has an apparent visual magnitude of +4.30, which makes it the brightest star in this generally faint constellation. Parallax measurements collected during the Hipparcos mission provide a distance estimate for this star, placing it at roughly 780 light-years (240 parsecs), with a 4% margin of error.\r\rAlpha Sculptoris is a blue-white B-type giant. It is classified as an SX Arietis type variable star and its magnitude varies by 0.01.\r\rThe luminosity of \u03B1 Scl is around 1700 times that of the Sun while its surface temperature is 14,000 kelvins. The radius of Alpha Sculptoris is calculated to be 7 times solar while its mass is 5.5 times that of our own star. Spectral variations observed in this star where once believed to be caused by an orbiting black hole but are now known to be the result of chemical variations in its atmosphere.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Alpha Sculptoris, HIP 4577, SAO 166716, HD 5737, GC 1172, HR 280, DM CD-30   297, TYC 6424-2270-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Alpha Sculptoris",
	"OType" : "Rotationally variable Star",
	"Distance" : "237.57",
	"RA_S" : 14.65150219,
	"DEC_S" : -29.35744807,
	"X" : 291,
	"Y" : 201,
	"Constellation" : "Sculptor ",
	"AMag" : 4.274,
	"key" : 64168,
	"title" : "Alpha Sculptoris"
	},
{
	"Index" : "48505",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Pi Sculptoris, HIP 7955, SAO 193263, HD 10537, GC 2085, HR 497, DM CD-32   666, TYC 7003-2207-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Pi Sculptoris",
	"OType" : "Star",
	"Distance" : "65.71",
	"RA_S" : 25.53583543,
	"DEC_S" : -32.32692048,
	"Constellation" : "Sculptor ",
	"AMag" : 5.371,
	"key" : 68505,
	"title" : "Pi Sculptoris"
	},
{
	"Index" : "44238",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Epsilon Sculptoris, HIP 8209A, SAO 167275, HD 10830A, GC 2145, HR 514, DM CD-25   704, TYC 6429-2283-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Epsilon Sculptoris",
	"OType" : "Star",
	"Distance" : "28.11",
	"RA_S" : 26.411087,
	"DEC_S" : -25.052439,
	"Constellation" : "Sculptor ",
	"AMag" : 5.384,
	"key" : 64238,
	"title" : "Epsilon Sculptoris"
	},
{
	"Index" : "52911",
	"Description" : "Gamma Sculptoris (\u03B3 Scl, \u03B3 Sculptoris) is a star in the constellation Sculptor.\r\rGamma Sculptoris is an orange K-type giant with an apparent magnitude of +4.41. It is approximately 179 light years from Earth.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Gamma Sculptoris, HIP 115102, SAO 214444, HD 219784, GC 32450, HR 8863, DM CD-33 16476, TYC 7510-1089-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Gamma Sculptoris",
	"OType" : "Star",
	"Distance" : "55.86",
	"RA_S" : 349.70599725,
	"DEC_S" : -32.53202066,
	"X" : 565,
	"Y" : 281,
	"Constellation" : "Sculptor ",
	"AMag" : 4.531,
	"key" : 72911,
	"title" : "Gamma Sculptoris"
	},
{
	"Index" : "57316",
	"Description" : "Beta Sculptoris (\u03B2 Scl, \u03B2 Sculptoris) is a star in the constellation Sculptor.\r\rBeta Sculptoris is a blue-white B-type subgiant with an apparent magnitude of +4.38. It is approximately 178 light years from Earth.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Beta Sculptoris, HIP 116231, SAO 214615, HD 221507, GC 32744, HR 8937, DM CD-38 15527, TYC 8013-1357-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Beta Sculptoris",
	"OType" : "Star",
	"Distance" : "53.36",
	"RA_S" : 353.24272496,
	"DEC_S" : -37.81827844,
	"X" : 511,
	"Y" : 338,
	"Constellation" : "Sculptor ",
	"AMag" : 4.352,
	"key" : 77316,
	"title" : "Beta Sculptoris"
	},
{
	"Index" : "52944",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Mu Sculptoris, HIP 116820, SAO 214701, HD 222433, GC 32888, HR 8975, DM CD-32 17621, TYC 7515-1148-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Mu Sculptoris",
	"OType" : "Variable Star",
	"Distance" : "89.37",
	"RA_S" : 355.15895713,
	"DEC_S" : -32.07312821,
	"Constellation" : "Sculptor ",
	"AMag" : 5.41,
	"key" : 72944,
	"title" : "Mu Sculptoris"
	},
{
	"Index" : "48379",
	"Description" : "Delta Sculptoris (\u03B4 Scl, \u03B4 Sculptoris) is a triple star system in the constellation Sculptor. It is approximately 143 light years from Earth.\r\rThe primary component, Delta Sculptoris A, is a white A-type main sequence dwarf with an apparent magnitude of +4.59. It has a faint, 11th magnitude companion, Delta Sculptoris B, 4 arcseconds, or more than 175 astronomical units, away from it. Orbiting this pair at the much greater separation of 74 arcseconds, is the yellow G-type Delta Sculptoris C, which has an apparent magnitude of +9.4.",
	"MapNum" : "36",
	"ImageNum" : "36",
	"Desig" : "Delta Sculptoris, HIP 117452, SAO 192167, HD 223352, GC 33050, HR 9016, DM CD-28 18353, TYC 6988-1337-1",
	"group" : { "key" : "Sculptor" },
	"Common" : "Delta Sculptoris",
	"OType" : "Double or multiple star",
	"Distance" : "42.14",
	"RA_S" : 357.2314421,
	"DEC_S" : -28.13026985,
	"X" : 494,
	"Y" : 204,
	"Constellation" : "Sculptor ",
	"AMag" : 4.572,
	"key" : 68379,
	"title" : "Delta Sculptoris"
	},
{
	"Index" : "38617",
	"Description" : "Zeta Scuti (\u03B6 Sct, \u03B6 Scuti) is the Bayer designation for a star in the southern constellation of Scutum. It is a G-type giant star with an apparent magnitude of +4.68, approximately 207 light years from Earth. This is an astrometric binary system with a period of 6.5 years (2,374 days) and an orbital eccentricity of 0.10.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Zeta Scuti, HIP 90135, SAO 142267, HD 169156, GC 25101, HR 6884, DM BD-09  4712, TYC 5690-1263-1",
	"group" : { "backgroundImage" : "images/Alignment/04.png",
		"description" : "Scutum is a small constellation introduced in the seventeenth century. Its name is Latin for shield.\r\rScutum is the only constellation that owes its name to a non-classical historical figure. It was created in 1684 by Polish astronomer Johannes Hevelius (Jan Heweliusz), who originally named it Scutum Sobiescianum (Shield of Sobieski) to commemorate the victory of the Polish forces led by King John III Sobieski (Jan III Sobieski) in the Battle of Vienna in 1683. Later, the name was shortened to Scutum.\r\rFive bright stars of Scutum (\u03B1 Sct, \u03B2 Sct, \u03B4 Sct, \u03B5 Sct and \u03B7 Sct) was a latter designation of 1,6,2,3 and 9 Aquilae\r\rScutum contains several open clusters, as well as a globular cluster and a planetary nebula. The two best known deep sky objects in Scutum are M11 (the Wild Duck Cluster) and the open cluster M26 (NGC 6694). The globular cluster NGC 6712 and the planetary nebula IC 1295 can be found in the eastern part of the constellation, only 24 arcminutes apart.\r\rThe most prominent open cluster in Scutum is the Wild Duck Cluster, M11. It was named by William H. Smyth in 1844 for its resemblance in the eyepiece to a flock of ducks in flight. The cluster, 6200 light-years from Earth and 20 light-years in diameter, contains approximately 3000 stars, making it a particularly rich cluster. It is 220 million years old.",
		"key" : "Scutum",
		"grouptype" : "Scutum",
		"Meaning" : "shield (of Sobieski)",
		"Family" : "Hercules",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Scutum",
		"title" : "Scutum Objects Group" },
	"Common" : "Zeta Scuti",
	"OType" : "Spectroscopic binary",
	"Distance" : "63.06",
	"RA_S" : 275.91492828,
	"DEC_S" : -8.93440847,
	"X" : 655,
	"Y" : 487,
	"Constellation" : "Scutum ",
	"AMag" : 4.77,
	"key" : 58617,
	"title" : "Zeta Scuti"
	},
{
	"Index" : "38698",
	"Description" : "Gamma Scuti (\u03B3 Sct, \u03B3 Scuti) is a star in the constellation Scutum.\r\rGamma Scuti is a white A-type subgiant with an apparent magnitude of +4.67. It is approximately 291 light years from Earth.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Gamma Scuti, HIP 90595, SAO 161520, HD 170296, GC 25220, HR 6930, DM BD-14  5071, TYC 5702-2882-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Gamma Scuti",
	"OType" : "Star",
	"Distance" : "97.88",
	"RA_S" : 277.29938875,
	"DEC_S" : -14.56581214,
	"X" : 634,
	"Y" : 561,
	"Constellation" : "Scutum ",
	"AMag" : 4.684,
	"key" : 58698,
	"title" : "Gamma Scuti"
	},
{
	"Index" : "38649",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "HIP 91105, SAO 161632, HD 171391, GC 25374, HR 6970, DM BD-11 4681, TYC 5695-1028-1",
	"group" : { "key" : "Scutum" },
	"Common" : "HR 6970",
	"OType" : "Star",
	"Distance" : "100.82",
	"RA_S" : 278.75996949,
	"DEC_S" : -10.97720758,
	"Constellation" : "Scutum ",
	"AMag" : 5.22,
	"key" : 58649,
	"title" : "HR 6970"
	},
{
	"Index" : "38623",
	"Description" : "Alpha Scuti (\u03B1 Sct, \u03B1 Scuti) is a fourth-magnitude star in the constellation Scutum. Alpha Scuti is an orange K-type giant with an apparent magnitude of +3.85. Alpha Scuti is a known variable star. It is approximately 174 light years from Earth.\r\rAlpha Scuti was a latter designation of 1 Aquilae.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Alpha Scuti, HIP 91117, SAO 142408, HD 171443, GC 25385, HR 6973, DM BD-08  4638, TYC 5691-1338-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Alpha Scuti",
	"OType" : "Variable Star",
	"Distance" : "61.04",
	"RA_S" : 278.80177754,
	"DEC_S" : -8.24406995,
	"X" : 618,
	"Y" : 477,
	"Constellation" : "Scutum ",
	"AMag" : 3.991,
	"key" : 58623,
	"title" : "Alpha Scuti"
	},
{
	"Index" : "38634",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Delta Scuti, HIP 91726, SAO 142515, HD 172748, GC 25580, HR 7020, DM BD-09  4796, TYC 5692-2505-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Delta Scuti",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "62.05",
	"RA_S" : 280.56844679,
	"DEC_S" : -9.0525494,
	"Constellation" : "Scutum ",
	"AMag" : 4.734,
	"key" : 58634,
	"title" : "Delta Scuti"
	},
{
	"Index" : "38633",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Epsilon Scuti, HIP 91845, SAO 142546, HD 173009, GC 25610, HR 7032, DM BD-08  4686, TYC 5692-2504-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Epsilon Scuti",
	"OType" : "Star",
	"Distance" : "162.84",
	"RA_S" : 280.8802172,
	"DEC_S" : -8.27522293,
	"Constellation" : "Scutum ",
	"AMag" : 5.013,
	"key" : 58633,
	"title" : "Epsilon Scuti"
	},
{
	"Index" : "34387",
	"Description" : "Beta Scuti (\u03B2 Sct, \u03B2 Scuti) is a star in the constellation Scutum. It is approximately 690 light years from Earth. The primary star is radiating about 1,270 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,622 K. The star is a yellow G-type bright giant with an apparent magnitude of +4.22.\r\rBeta Scuti was a latter designation of 6 Aquilae.",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Beta Scuti, HIP 92175, SAO 142618, HD 173764, GC 25730, HR 7063, DM BD-04  4582, TYC 5122-1426-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Beta Scuti",
	"OType" : "Spectroscopic binary",
	"Distance" : "276.07",
	"RA_S" : 281.79363848,
	"DEC_S" : -4.74786905,
	"X" : 580,
	"Y" : 431,
	"Constellation" : "Scutum ",
	"AMag" : 4.337,
	"key" : 54387,
	"title" : "Beta Scuti"
	},
{
	"Index" : "43113",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "HIP 92814, SAO 161964, HD 175156, GC 25931, HR 7119, DM BD-15 5143, TYC 6281-2005-1",
	"group" : { "key" : "Scutum" },
	"Common" : "HR 7119",
	"OType" : "Star",
	"Distance" : "423.79",
	"RA_S" : 283.67964085,
	"DEC_S" : -15.60304096,
	"Constellation" : "Scutum ",
	"AMag" : 5.103,
	"key" : 63113,
	"title" : "HR 7119"
	},
{
	"Index" : "34426",
	"MapNum" : "04",
	"ImageNum" : "04",
	"Desig" : "Eta Scuti, HIP 93026, SAO 142838, HD 175751, GC 26013, HR 7149, DM BD-06  4976, TYC 5127-7358-1",
	"group" : { "key" : "Scutum" },
	"Common" : "Eta Scuti",
	"OType" : "Star",
	"Distance" : "62.01",
	"RA_S" : 284.26528832,
	"DEC_S" : -5.84630936,
	"Constellation" : "Scutum ",
	"AMag" : 4.939,
	"key" : 54426,
	"title" : "Eta Scuti"
	},
{
	"Index" : "20498",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "3 Serpentis, HIP 74649AB, SAO 120916, HD 135482, GC 20501, HR 5675, DM BD+05  2985, TYC 344-1146-1",
	"group" : { "backgroundImage" : "images/Alignment/34.png",
		"description" : "Serpens (\u0022the Serpent\u0022, Greek \u1F4C\u03C6\u03B9\u03C2) is a constellation of the northern hemisphere. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy and it remains one of the 88 modern constellations defined by the International Astronomical Union.\r\rIt is unique among the modern constellations in being split into two non-contiguous parts, Serpens Caput (Serpent\u0027s Head) to the west and Serpens Cauda (Serpent\u0027s Tail) to the east. Between these two halves lies the constellation of Ophiuchus, the \u0022Serpent-Bearer\u0022. In figurative representations, the body of the serpent is represented as passing behind Ophiuchus between \u03BC Ser in Serpens Caput and \u03BD Ser in Serpens Cauda. The brightest star in Serpens is Unukalhai or Cor Serpentis \u0022Serpent\u0027s Heart\u0022, with an apparent magnitude of 2.63.\r\rAratus describes the constellation as follows:\r\rBoth [hands of Ophiuchus] firmly clutch the Serpent, which encircles the waist of Ophiuchus, but he, steadfast with both his feet well set, tramples a huge monster, even the Scorpion, standing upright on his eye and breast. Now the Serpent is wreathed about his two hands \u2013 a little above his right hand, but in many folds high above his left. ... Toward the Crown leans the Serpent\u0027s jaw, but beneath his coiling form seek thou for the mighty Claws [Libra]\r\rThere were two \u0022serpent\u0022 constellations in Babylonian astronomy, known as Mu\u0161\u1E2Bu\u0161\u0161u and Ba\u0161mu. It appears that Mu\u0161\u1E2Bu\u0161\u0161u was depicted as a hybrid of dragon, lion and bird, and loosely corresponds to Hydra. Ba\u0161mu was a horned serpent (c.f. Ningishzida) and loosely corresponds to the \u1F4C\u03C6\u03B9\u03C2 constellation of Eudoxus of Cnidus on which the \u1F4C\u03C6\u03B9\u03C2 (Serpens) of Ptolemy is based.",
		"key" : "Serpens",
		"grouptype" : "Serpens",
		"Meaning" : "snake",
		"Family" : "Hercules",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Serpens",
		"title" : "Serpens Objects Group" },
	"Common" : "3 Serpentis",
	"OType" : "Star",
	"Distance" : "113.41",
	"RA_S" : 228.79730569,
	"DEC_S" : 4.93936037,
	"Constellation" : "Serpens ",
	"AMag" : 5.457,
	"key" : 40498,
	"title" : "3 Serpentis"
	},
{
	"Index" : "19872",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "5 Serpentis, HIP 74975, SAO 120946, HD 136202, GC 20591, HR 5694, DM BD+02  2944, TYC 336-1027-1",
	"group" : { "key" : "Serpens" },
	"Common" : "5 Serpentis",
	"OType" : "Variable of BY Dra type",
	"Distance" : "25.38",
	"RA_S" : 229.82832621,
	"DEC_S" : 1.76540542,
	"Constellation" : "Serpens ",
	"AMag" : 5.118,
	"key" : 39872,
	"title" : "5 Serpentis"
	},
{
	"Index" : "4074",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "9 Serpentis, Tau01 Serpentis, HIP 75530, SAO 101545, HD 137471, GC 20740, HR 5739, DM BD+15  2858, TYC 1487-1430-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Tau01 Serpentis",
	"OType" : "Variable Star",
	"Distance" : "210.04",
	"RA_S" : 231.44748452,
	"DEC_S" : 15.42803736,
	"Constellation" : "Serpens ",
	"AMag" : 5.34,
	"key" : 24074,
	"title" : "Tau01 Serpentis"
	},
{
	"Index" : "20007",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "10 Serpentis, HIP 75761, SAO 121020, HD 137898, GC 20805, HR 5746, DM BD+02  2965, TYC 337-843-1",
	"group" : { "key" : "Serpens" },
	"Common" : "10 Serpentis",
	"OType" : "Star",
	"Distance" : "39.74",
	"RA_S" : 232.15932111,
	"DEC_S" : 1.84208399,
	"Constellation" : "Serpens ",
	"AMag" : 5.178,
	"key" : 40007,
	"title" : "10 Serpentis"
	},
{
	"Index" : "70058",
	"Description" : "Delta Serpentis (\u03B4 Serpentis, \u03B4 Ser) is a star system in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Yam\u0101n\u012B, \u0022the Southern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022., along with \u03B1 Ser (Unukalhai), \u03B5 Ser (Ba, Pa), \u03B4 Oph (Yed Prior), \u03B5 Oph (Yed Posterior), \u03B6 Oph (Han) and \u03B3 Oph (Tsung Ching).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Yam\u0101n\u012B or Nasak Yamani were the title for two stars :\u03B4 Ser as Nasak Yamani I and \u03B5 Ser as Nasak Yamani II (exclude \u03B1 Ser, \u03B4 Oph, \u03B5 Oph, \u03B6 Oph and \u03B3 Oph)\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B4 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B2 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B4 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u516D (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n li\u00F9, English: the Sixth Star of Right Wall of Heavenly Market Enclosure), represent the state Qin (\u79E6) (or Tsin), together with \u03B8 Capricorni and 30 Capricorni in Twelve States (asterism).",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "13 Serpentis, Delta Serpentis, HIP 76276A, TYC 933-1238-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Delta Serpentis",
	"OType" : "Double or multiple star",
	"Distance" : "69.7",
	"RA_S" : 233.70061048,
	"DEC_S" : 10.53889165,
	"X" : 646,
	"Y" : 184,
	"Constellation" : "Serpens ",
	"AMag" : 4.171,
	"key" : 90058,
	"title" : "Delta Serpentis"
	},
{
	"Index" : "70059",
	"Description" : "Delta Serpentis (\u03B4 Serpentis, \u03B4 Ser) is a star system in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Yam\u0101n\u012B, \u0022the Southern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022., along with \u03B1 Ser (Unukalhai), \u03B5 Ser (Ba, Pa), \u03B4 Oph (Yed Prior), \u03B5 Oph (Yed Posterior), \u03B6 Oph (Han) and \u03B3 Oph (Tsung Ching).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Yam\u0101n\u012B or Nasak Yamani were the title for two stars :\u03B4 Ser as Nasak Yamani I and \u03B5 Ser as Nasak Yamani II (exclude \u03B1 Ser, \u03B4 Oph, \u03B5 Oph, \u03B6 Oph and \u03B3 Oph)\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B4 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B2 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B4 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u516D (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n li\u00F9, English: the Sixth Star of Right Wall of Heavenly Market Enclosure), represent the state Qin (\u79E6) (or Tsin), together with \u03B8 Capricorni and 30 Capricorni in Twelve States (asterism).",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "13 Serpentis, Delta Serpentis, HIP 76276B, SAO 101623, HD 138917J, GC 20941, HR 5788, DM BD+11  2821B, TYC 933-1239-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Delta Serpentis",
	"OType" : "Double or multiple star",
	"Distance" : "69.7",
	"RA_S" : 233.70061506,
	"DEC_S" : 10.538868,
	"X" : 646,
	"Y" : 184,
	"Constellation" : "Serpens ",
	"AMag" : 3.8,
	"key" : 90059,
	"title" : "Delta Serpentis"
	},
{
	"Index" : "70060",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "16 Serpentis, HIP 76425, SAO 101640, HD 139195, GC 20981, HR 5802, DM BD+10  2884, TYC 933-1240-1",
	"group" : { "key" : "Serpens" },
	"Common" : "16 Serpentis",
	"OType" : "Spectroscopic binary",
	"Distance" : "70.83",
	"RA_S" : 234.12324591,
	"DEC_S" : 10.01016535,
	"Constellation" : "Serpens ",
	"AMag" : 5.36,
	"key" : 90060,
	"title" : "16 Serpentis"
	},
{
	"Index" : "4164",
	"Description" : "Iota Serpentis (\u03B9 Ser, \u03B9 Serpentis) is a star system in the constellation Serpens, in its head (Serpens Caput). It is approximately 192 light years from Earth.\r\rAt the centre of the system is a spectroscopic binary, Iota Serpentis A and B. These are both white A-type main sequence dwarfs and both have apparent magnitudes of +5.3. This binary appears to have an orbital period of 11 years; spectroscopic evidence indicates a third companion of A and B. A and B also have two distant companions, Iota Serpentis C, a 13th magnitude star 143 arcseconds away and Iota Serpentis D, a 12th magnitude star 151 arcseconds distant.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "21 Serpentis, Iota Serpentis, HIP 76852AB, SAO 101682, HD 140159, GC 21102, HR 5842, DM BD+20  3138, TYC 1498-1787-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Iota Serpentis",
	"OType" : "Star",
	"Distance" : "58.17",
	"RA_S" : 235.38773106,
	"DEC_S" : 19.67040458,
	"X" : 619,
	"Y" : 68,
	"Constellation" : "Serpens ",
	"AMag" : 4.513,
	"key" : 24164,
	"title" : "Iota Serpentis"
	},
{
	"Index" : "70297",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "20 Serpentis, Chi Serpentis, HIP 76866, SAO 101683, HD 140160, GC 21105, HR 5843, DM BD+13  2982, TYC 937-1118-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Chi Serpentis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "67.32",
	"RA_S" : 235.44756867,
	"DEC_S" : 12.8475302,
	"Constellation" : "Serpens ",
	"AMag" : 5.322,
	"key" : 90297,
	"title" : "Chi Serpentis"
	},
{
	"Index" : "22279",
	"Description" : "Alpha Serpentis (\u03B1 Serpentis, \u03B1 Ser) is a double star in the head (Serpens Caput) of the equatorial constellation Serpens. It has the traditional name Unukalhai. With an apparent visual magnitude of 2.6, this star is the brightest in the constellation and it can be viewed with the naked eye from most of the Earth. Parallax measurements yield an estimated distance of about 74 light-years (23 parsecs) from Earth.Alpha Serpentis is a giant star with a stellar classification of K2 III, having consumed the hydrogen at its core and evolved away from the main sequence. The interferometry-measured angular diameter of this star, after correcting for limb darkening, is 4.85 \u00B1 0.05 mas, which, at its estimated distance, equates to a physical radius of about 12 times the radius of the Sun. The effective temperature of the outer envelope is 4,498 K, giving it an orange hue that is characteristic of a K-type star.\r\rThis star is radiating about 38 times the luminosity of the Sun, while a further 32 times the Sun\u0027s luminosity is being emitted in the infrared, for 70-fold total. A magnitude +11.8 companion is at an angular separation of 58 arcseconds from Alpha Serpentis, while a 13th magnitude star lies 2.3 arcminutes distant.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "24 Serpentis, Alpha Serpentis, HIP 77070, SAO 121157, HD 140573, GC 21158, HR 5854, DM BD+06  3088, TYC 363-1135-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Unukalhai",
	"OType" : "Variable Star",
	"Distance" : "22.68",
	"RA_S" : 236.06697631,
	"DEC_S" : 6.42562868,
	"X" : 619,
	"Y" : 236,
	"Constellation" : "Serpens ",
	"AMag" : 2.739,
	"key" : 42279,
	"shortTitle" : "Unuk Elhaia; Cor Serpentis; Unuk al Hay; Unuk; Unukalhay; Unuk Ehl'khaja; Unuk alb Khaj; Unuk-Ehl'khaja; Unuk al' Khaj",
	"title" : "Unukalhai"
	},
{
	"Index" : "33900",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "25 Serpentis, A02 Serpentis, HIP 77227, SAO 140740, HD 140873, GC 21187, HR 5863, DM BD-01  3092, TYC 5018-1142-1",
	"group" : { "key" : "Serpens" },
	"Common" : "A02 Serpentis",
	"OType" : "Spectroscopic binary",
	"Distance" : "137.63",
	"RA_S" : 236.5234907,
	"DEC_S" : -1.80419091,
	"Constellation" : "Serpens ",
	"AMag" : 5.379,
	"key" : 53900,
	"title" : "A02 Serpentis"
	},
{
	"Index" : "4141",
	"Description" : "Beta Serpentis (\u03B2 Ser, \u03B2 Serpentis) is a star system in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Sha\u0027\u0101m\u012B, \u0022the Northern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022, along with \u03B2 Her (Kornephoros), \u03B3 Her (Hejian, Ho Keen) and \u03B3 Ser (Zheng, Ching).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Sha\u0027\u0101m\u012B or Nasak Shamiya were the title for three stars :\u03B2 Ser as Nasak Shamiya I, \u03B3 Ser as Nasak Shamiya II, \u03B3 Her as Nasak Shamiya III (exclude \u03B2 Her)\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B2 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B4 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B2 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u4E94 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n wu, English: the Fifth Star of Right Wall of Heavenly Market Enclosure), represent Zhou (\u912D) (possibly Chow, the dynasty in China), together with \u03B7 Capricorni and 21 Capricorni in Twelve States (asterism).Beta Serpentis is approximately 150 light years from Earth and is a member of the Ursa Major Moving Group.\r\rThe primary component, Beta Serpentis A, is a white A-type main sequence dwarf with an apparent magnitude of +3.65. It has two companions, the magnitude +9.9 B, 31 arcseconds distant, and the magnitude +10.7 C, 201 arcseconds away.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "28 Serpentis, Beta Serpentis, HIP 77233, SAO 101725, HD 141003, GC 21194, HR 5867, DM BD+15  2911, TYC 1495-1994-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Beta Serpentis",
	"OType" : "Star",
	"Distance" : "47.54",
	"RA_S" : 236.5468981,
	"DEC_S" : 15.42181924,
	"X" : 608,
	"Y" : 122,
	"Constellation" : "Serpens ",
	"AMag" : 3.653,
	"key" : 24141,
	"title" : "Beta Serpentis"
	},
{
	"Index" : "22388",
	"Description" : "Lambda Serpentis (\u03BB Ser, \u03BB Serpentis) is a star in the constellation Serpens, in its head (Serpens Caput). It has an apparent visual magnitude of 4.43, making it visible to the naked eye. Based upon parallax measurements from the Hipparcos satellite, this star lies at a distance of about 38.3 light-years (11.7 parsecs) from Earth. This star is larger and more massive than the Sun, although it has a similar stellar classification. It is shining with nearly double the Sun\u0027s luminosity and this energy is being radiated from the star\u0027s outer atmosphere at an effective temperature of 5,884 K.\r\rLambda Serpentis is moving toward the Solar System with a radial velocity of 66.4 km s\u20131. In about 166,000 years, this system will make its closest approach of the Sun at a distance of 7.371 \u00B1 0.258 light-years (2.260 \u00B1 0.079 parsecs), before moving away thereafter.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "27 Serpentis, Lambda Serpentis, HIP 77257, SAO 121186, HD 141004, GC 21201, HR 5868, DM BD+07  3023, TYC 364-1224-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Lambda Serpentis",
	"OType" : "Spectroscopic binary",
	"Distance" : "12.12",
	"RA_S" : 236.61088938,
	"DEC_S" : 7.3530724,
	"X" : 611,
	"Y" : 224,
	"Constellation" : "Serpens ",
	"AMag" : 4.482,
	"key" : 42388,
	"title" : "Lambda Serpentis"
	},
{
	"Index" : "4166",
	"Description" : "Kappa Serpentis (\u03BA Ser, \u03BA Serpentis) is a star in the constellation Serpens, in its head (Serpens Caput).\r\rKappa Serpentis is a red M-type giant with an apparent magnitude of +4.09. It is approximately 348 light years from Earth.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "35 Serpentis, Kappa Serpentis, HIP 77450, SAO 101752, HD 141477, GC 21255, HR 5879, DM BD+18  3074, TYC 1498-1789-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Kappa Serpentis",
	"OType" : "Variable Star",
	"Distance" : "116.99",
	"RA_S" : 237.18490292,
	"DEC_S" : 18.14156492,
	"X" : 598,
	"Y" : 87,
	"Constellation" : "Serpens ",
	"AMag" : 4.273,
	"key" : 24166,
	"title" : "Kappa Serpentis"
	},
{
	"Index" : "33920",
	"Description" : "Mu Serpentis (\u03BC Ser, \u03BC Serpentis) is a star in the constellation Serpens, in its head (Serpens Caput). Mu Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +3.54. It is approximately 156 light years from Earth.\r\rIn Chinese astronomy, Mu Serpentis is called \u5929\u4E73, Pinyin: Ti\u0101nr\u01D4, meaning Celestial Milk, because this star is marking itself and stand alone in Celestial Milk asterism, Root mansion (see : Chinese constellation).",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "32 Serpentis, Mu Serpentis, HIP 77516, SAO 140787, HD 141513, GC 21269, HR 5881, DM BD-02  4052, TYC 5022-936-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Mu Serpentis",
	"OType" : "Star",
	"Distance" : "51.98",
	"RA_S" : 237.40502902,
	"DEC_S" : -3.43020438,
	"X" : 601,
	"Y" : 361,
	"Constellation" : "Serpens ",
	"AMag" : 3.535,
	"key" : 53920,
	"title" : "Mu Serpentis"
	},
{
	"Index" : "21480",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "34 Serpentis, Omega Serpentis, HIP 77578, SAO 121215, HD 141680, GC 21280, HR 5888, DM BD+02  3007, TYC 356-1276-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Omega Serpentis",
	"OType" : "Star",
	"Distance" : "83.77",
	"RA_S" : 237.57311334,
	"DEC_S" : 2.19651263,
	"Constellation" : "Serpens ",
	"AMag" : 5.33,
	"key" : 41480,
	"title" : "Omega Serpentis"
	},
{
	"Index" : "21971",
	"Description" : "Epsilon Serpentis (\u03B5 Ser, \u03B5 Serpentis) is a star in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Yam\u0101n\u012B, \u0022the Southern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022., along with \u03B1 Ser (Unukalhai), \u03B4 Ser (Qin, Tsin), \u03B4 Oph (Yed Prior), \u03B5 Oph (Yed Posterior), \u03B6 Oph (Han) and \u03B3 Oph (Tsung Ching).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Yam\u0101n\u012B or Nasak Yamani were the title for two stars :\u03B4 Ser as Nasak Yamani I and \u03B5 Ser as Nasak Yamani II (exclude \u03B1 Ser, \u03B4 Oph, \u03B5 Oph, \u03B6 Oph and \u03B3 Oph)\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B5 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B3 Serpentis, \u03B2 Serpentis, \u03B1 Serpentis, \u03B4 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B5 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u516B (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n b\u0101, English: the Eighth Star of Right Wall of Heavenly Market Enclosure), represent the state Ba (\u5DF4) (or Pa).Epsilon Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +3.71. It is approximately 70.3 light years from Earth. This star has 1.8 times the Sun\u0027s radius and it is radiating 12 times the luminosity of the Sun from its outer envelope at an effective temperature of 8,084 K.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "37 Serpentis, Epsilon Serpentis, HIP 77622, SAO 121218, HD 141795, GC 21288, HR 5892, DM BD+04  3069, TYC 360-1226-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Epsilon Serpentis",
	"OType" : "Star",
	"Distance" : "21.6",
	"RA_S" : 237.70402752,
	"DEC_S" : 4.47773211,
	"X" : 598,
	"Y" : 261,
	"Constellation" : "Serpens ",
	"AMag" : 3.714,
	"key" : 41971,
	"title" : "Epsilon Serpentis"
	},
{
	"Index" : "33919",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "36 Serpentis, b Serpentis, HIP 77660, SAO 140801, HD 141851, GC 21301, HR 5895, DM BD-02  4058, TYC 5022-935-1",
	"group" : { "key" : "Serpens" },
	"Common" : "b Serpentis",
	"OType" : "Double or multiple star",
	"Distance" : "49.74",
	"RA_S" : 237.8149806,
	"DEC_S" : -3.09049186,
	"Constellation" : "Serpens ",
	"AMag" : 5.106,
	"key" : 53919,
	"title" : "b Serpentis"
	},
{
	"Index" : "4197",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "38 Serpentis, Rho Serpentis, HIP 77661, SAO 84037, HD 141992, GC 21311, HR 5899, DM BD+21  2829, TYC 1502-1782-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Rho Serpentis",
	"OType" : "Variable Star",
	"Distance" : "114.78",
	"RA_S" : 237.81628762,
	"DEC_S" : 20.97791955,
	"Constellation" : "Serpens ",
	"AMag" : 4.914,
	"key" : 24197,
	"title" : "Rho Serpentis"
	},
{
	"Index" : "4150",
	"Description" : "Gamma Serpentis (\u03B3 Serpentis, \u03B3 Ser) is a star in the constellation Serpens, in its head (Serpens Caput). It was a member of indigenous Arabic asterism al-Nasaq al-Sha\u0027\u0101m\u012B, \u0022the Northern Line\u0022 of al-Nasaq\u0101n \u0022the Two Lines\u0022, along with \u03B2 Her (Kornephoros), \u03B3 Her (Hejian, Ho Keen) and \u03B2 Ser (Chow).\r\rAccording to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Sha\u0027\u0101m\u012B or Nasak Shamiya were the title for three stars :\u03B2 Ser as Nasak Shamiya I, \u03B3 Ser as Nasak Shamiya II, \u03B3 Her as Nasak Shamiya III (exclude \u03B2 Her). The star was later given the proper name Ainalhai, from the Arabic \u0639\u064A\u0646 \u0627\u0644\u062D\u064A\u0629 \u0027Ayn al-\u1E24ayyah \u0022the Serpent\u0027s Eye\u0022.\r\rIn Chinese, \u5929\u5E02\u53F3\u57A3 (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of \u03B3 Serpentis, \u03B2 Herculis, \u03B3 Herculis, \u03BA Herculis, \u03B2 Serpentis, \u03B4 Serpentis, \u03B1 Serpentis, \u03B5 Serpentis, \u03B4 Ophiuchi, \u03B5 Ophiuchi and \u03B6 Ophiuchi. Consequently, \u03B3 Serpentis itself is known as \u5929\u5E02\u53F3\u57A3\u56DB (Ti\u0101n Sh\u00EC Y\u00F2u Yu\u00E1n s\u00EC, English: the Fourth Star of Right Wall of Heavenly Market Enclosure), represent the state Zheng (\u912D) (or Ching), together with 20 Capricorni in Twelve States (asterism).Gamma Serpentis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +3.85. Occasionally Gamma Serpentis is listed as having two 10th magnitude companions, but it appears that these stars are just optical neighbours. The Gamma Serpentis system is approximately 36.3 light years from Earth.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "41 Serpentis, Gamma Serpentis, HIP 78072, SAO 101826, HD 142860, GC 21408, HR 5933, DM BD+16  2849, TYC 1496-2119-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Gamma Serpentis",
	"OType" : "Variable Star",
	"Distance" : "11.25",
	"RA_S" : 239.11326123,
	"DEC_S" : 15.66161682,
	"X" : 577,
	"Y" : 119,
	"Constellation" : "Serpens ",
	"AMag" : 3.882,
	"key" : 24150,
	"title" : "Gamma Serpentis"
	},
{
	"Index" : "8612",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "44 Serpentis, Pi Serpentis, HIP 78554, SAO 84155, HD 143894, GC 21552, HR 5972, DM BD+23  2886, TYC 2035-1749-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Pi Serpentis",
	"OType" : "Star",
	"Distance" : "54.87",
	"RA_S" : 240.57371524,
	"DEC_S" : 22.80445158,
	"Constellation" : "Serpens ",
	"AMag" : 4.827,
	"key" : 28612,
	"title" : "Pi Serpentis"
	},
{
	"Index" : "22801",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "50 Serpentis, Sigma Serpentis, HIP 80179, SAO 121540, HD 147449, GC 22007, HR 6093, DM BD+01  3215, TYC 368-1592-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Sigma Serpentis",
	"OType" : "High proper-motion Star",
	"Distance" : "27.27",
	"RA_S" : 245.51811977,
	"DEC_S" : 1.02904029,
	"Constellation" : "Serpens ",
	"AMag" : 4.858,
	"key" : 42801,
	"title" : "Sigma Serpentis"
	},
{
	"Index" : "38435",
	"Description" : "Nu Serpentis (\u03BD Ser, \u03BD Serpentis) is a binary star in the constellation Serpens. It is approximately 193 light years from Earth.\r\rThe primary component, Nu Serpentis A, is a white A-type main sequence dwarf with an apparent magnitude of +4.32. It is separated from Nu Serpentis B, a magnitude +8.4 companion, by 46 arcseconds.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "53 Serpentis, Nu Serpentis, HIP 84880, SAO 160479, HD 156928, GC 23424, HR 6446, DM BD-12  4722, TYC 5653-1431-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Nu Serpentis",
	"OType" : "Star",
	"Distance" : "62.29",
	"RA_S" : 260.20691879,
	"DEC_S" : -12.84688063,
	"X" : 319,
	"Y" : 472,
	"Constellation" : "Serpens ",
	"AMag" : 4.329,
	"key" : 58435,
	"title" : "Nu Serpentis"
	},
{
	"Index" : "42804",
	"Description" : "Xi Serpentis (\u03BE Ser, \u03BE Serpentis) is a triple star system in the constellation Serpens. The primary star, Xi Serpentis A, is a yellow-white F-type giant with an apparent magnitude of +3.54. It is a spectroscopic binary with an orbital period of 2.29 days. A 13th magnitude companion, Xi Serpentis B, is located 25 arcseconds from the primary pair. Xi Serpentis is approximately 105 light years from Earth.\r\rIn Chinese, Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n (\u5929\u5E02\u5DE6\u57A3), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states (and region) in China which is marking the left borderline of the enclosure, consisting of \u03BE Serpentis, \u03B4 Herculis, \u03BB Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B6 Aquilae, \u03B7 Serpentis, \u03B81 Serpentis, \u03BD Ophiuchi and \u03B7 Ophiuchi. Consequently, \u03BE Serpentis itself is known as Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n sh\u00ED (\u5929\u5E02\u5DE6\u57A3\u5341, English: the Tenth Star of Left Wall of Heavenly Market Enclosure), representing the region of Nanhai (\u5357\u6D77, lit. meaning southern sea)",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "55 Serpentis, Xi Serpentis, HIP 86263, SAO 160700, HD 159876, GC 23881, HR 6561, DM BD-15  4621, TYC 6248-1369-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Xi Serpentis",
	"OType" : "Spectroscopic binary",
	"Distance" : "32.28",
	"RA_S" : 264.39667267,
	"DEC_S" : -15.39855661,
	"X" : 269,
	"Y" : 504,
	"Constellation" : "Serpens ",
	"AMag" : 3.553,
	"key" : 62804,
	"title" : "Xi Serpentis"
	},
{
	"Index" : "38497",
	"Description" : "Omicron Serpentis (\u03BF Ser, \u03BF Serpentis) is a star in the constellation Serpens.\r\rOmicron Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +4.24. It is approximately 168 light years from Earth. It is classified as a Delta Scuti type variable star and its apparent magnitude varies by 0.01 with a period of 76 minutes.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "56 Serpentis, Omicron Serpentis, HIP 86565, SAO 160747, HD 160613, GC 23978, HR 6581, DM BD-12  4808, TYC 5668-1486-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Omicron Serpentis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "53.1",
	"RA_S" : 265.35363573,
	"DEC_S" : -12.87530581,
	"X" : 257,
	"Y" : 472,
	"Constellation" : "Serpens ",
	"AMag" : 4.24,
	"key" : 58497,
	"title" : "Omicron Serpentis"
	},
{
	"Index" : "34268",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "57 Serpentis, Zeta Serpentis, HIP 88175, SAO 142025, HD 164259, GC 24503, HR 6710, DM BD-03  4217, TYC 5100-600-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Zeta Serpentis",
	"OType" : "Star",
	"Distance" : "23.55",
	"RA_S" : 270.12087711,
	"DEC_S" : -3.69027123,
	"Constellation" : "Serpens ",
	"AMag" : 4.66,
	"key" : 54268,
	"title" : "Zeta Serpentis"
	},
{
	"Index" : "34285",
	"Description" : "Eta Serpentis (\u03B7 Ser, \u03B7 Serpentis) is a star in the constellation Serpens. In particular, it lies in Serpens Cauda, the snake\u0027s tail. The star has an apparent visual magnitude of 3.260, making it visible to the naked eye. Parallax measurements give a distance estimate of 60.5 light-years (18.5 parsecs) from the Earth.\r\rThis star is larger than the Sun, with twice the mass and almost six times the radius. The spectrum matches a stellar classification of K0 III-IV, with the luminosity class of III-IV corresponding to an evolved star that lies between the subgiant and giant stages. The expanded outer envelope star is radiating about 19 times the luminosity of the Sun at an effective temperature of 4,890 K. At this temperature, it has an orange hue typical of a K-type star. Eta Serpentis displays solar-like oscillations with a period of 0.09 days.\r\rIn Chinese astronomy, the star is known as \u5929\u5E02\u5DE6\u57A3 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n), meaning \u0027Left Wall of Heavenly Market Enclosure\u0027; the name refers to an asterism that represents eleven old states in China. The leftmost borderline of the enclosure consists of \u03B7 Serpentis, \u03B4 Herculis, \u03BB Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B7 Ophiuchi, \u03B6 Aquilae, \u03B81 Serpentis, \u03BD Ophiuchi and \u03BE Serpentis. Consequently, \u03B7 Serpentis itself is known as \u5929\u5E02\u5DE6\u57A3\u516B (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n b\u0101, the Eighth Star of Left Wall of Heavenly Market Enclosure, representing the region of Donghai (\u6771\u6D77, lit. meaning \u0027eastern sea\u0027), possibly a reference to the East China Sea.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "58 Serpentis, Eta Serpentis, HIP 89962, SAO 142241, HD 168723, GC 25046, HR 6869, DM BD-02  4599, TYC 5102-416-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Eta Serpentis",
	"OType" : "Variable Star",
	"Distance" : "18.54",
	"RA_S" : 275.32750215,
	"DEC_S" : -2.89882468,
	"X" : 132,
	"Y" : 351,
	"Constellation" : "Serpens ",
	"AMag" : 3.337,
	"key" : 54285,
	"title" : "Eta Serpentis"
	},
{
	"Index" : "28357",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "59 Serpentis, d Serpentis, HIP 90441A, SAO 123497, HD 169985, GC 25176, HR 6918, DM BD+00  3936A, TYC 433-595-1",
	"group" : { "key" : "Serpens" },
	"Common" : "d Serpentis",
	"OType" : "Spectroscopic binary",
	"Distance" : "142.48",
	"RA_S" : 276.80214785,
	"Constellation" : "Serpens ",
	"AMag" : 5.382,
	"key" : 48357,
	"title" : "d Serpentis"
	},
{
	"Index" : "34288",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "60 Serpentis, c Serpentis, HIP 90642, SAO 142348, HD 170474, GC 25234, HR 6935, DM BD-02  4641, TYC 5103-302-1",
	"group" : { "key" : "Serpens" },
	"Common" : "c Serpentis",
	"OType" : "Star",
	"Distance" : "70.36",
	"RA_S" : 277.42074776,
	"DEC_S" : -1.98530811,
	"Constellation" : "Serpens ",
	"AMag" : 5.475,
	"key" : 54288,
	"title" : "c Serpentis"
	},
{
	"Index" : "30274",
	"Description" : "Theta Serpentis (\u03B8 Ser, \u03B8 Serpentis) is a star system in the constellation Serpens. It is approximately 132 light years from Earth. Theta Serpentis also has the traditional name Alya, or Alga, from the Arabic \u0627\u0644\u064A\u0629 \u0027alyah \u0022fat tail (of a sheep)\u0022.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Dzaneb al Haiyet, which was translated into Latin as Cauda Serpentis, meaning the serpent\u0027s tail.\r\rIn Chinese, \u5929\u5E02\u5DE6\u57A3 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n), meaning Left Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China, consisting of \u03B8 Serpentis, \u03B4 Herculis, \u03BB Herculis, \u03BC Herculis, \u03BF Herculis, 112 Herculis, \u03B6 Aquilae, \u03B7 Serpentis, \u03BD Ophiuchi, \u03BE Serpentis and \u03B7 Ophiuchi. Consequently, \u03B8 Serpentis itself is known as \u5929\u5E02\u5DE6\u57A3\u4E03 (Ti\u0101n Sh\u00EC Zu\u01D2 Yu\u00E1n q\u012B, English: the Seventh Star of Left Wall of Heavenly Market Enclosure), represent the state Xu (\u5F90).\r\rBoth Theta-1 Serpentis and Theta-2 Serpentis are white A-type main sequence dwarfs. \u03B8\u00B9 has an apparent magnitude of +4.62 while the slightly dimmer \u03B8\u00B2 has a magnitude of +4.98. These two stars are 22 arcseconds apart on the sky, putting them at least 900 astronomical units apart with an orbital period of at least 14,000 years. Both stars are similar to each other in all respects, having luminosities of 18 and 13 times solar respectively, radii of about twice solar and also masses of roughly 2 times that of our Sun. Both star have a surface temperature of 8,000 kelvins.\r\rThe third star in the system, Theta Serpentis C, is a yellow G-type star with an apparent magnitude of +6.71. It is separated by 7 arcminutes from \u03B8\u00B2.",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "63 Serpentis, Theta01 Serpentis, HIP 92946A, SAO 124068, HD 175638, GC 25991, HR 7141, DM BD+04  3916, TYC 457-687-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Theta Serpentis",
	"OType" : "Star",
	"Distance" : "40.23",
	"RA_S" : 284.0549455,
	"DEC_S" : 4.20359728,
	"X" : 24,
	"Y" : 265,
	"Constellation" : "Serpens ",
	"AMag" : 4.592,
	"key" : 50274,
	"shortTitle" : "Alga",
	"title" : "Theta Serpentis"
	},
{
	"Index" : "30275",
	"MapNum" : "34",
	"ImageNum" : "34",
	"Desig" : "63 Serpentis, Theta02 Serpentis, HIP 92951B, SAO 124070, HD 175639, GC 25993, HR 7142, DM BD+04  3917, TYC 457-688-1",
	"group" : { "key" : "Serpens" },
	"Common" : "Theta02 Serpentis",
	"OType" : "Star",
	"Distance" : "49.89",
	"RA_S" : 284.06098815,
	"DEC_S" : 4.20209847,
	"Constellation" : "Serpens ",
	"AMag" : 4.93,
	"key" : 50275,
	"title" : "Theta02 Serpentis"
	},
{
	"Index" : "37311",
	"Description" : "Gamma Sextantis (\u03B3 Sex, \u03B3 Sextantis) is a triple star system in the constellation Sextans. It is approximately 262 light years from Earth. The combined apparent magnitude of the system is +5.07.\r\rThe system is composed of a close binary star, Gamma Sextantis A and B, which is given the stellar classification A1. The two component stars are approximately 0.38 arcseconds apart, or approximately 30 Astronomical Units, and have apparent magnitudes of +5.8 and +6.2. They complete one orbit every 77.6 years. Orbiting the binary star, at a distance of 36 arcseconds, roughly a hundred times farther out, is Gamma Sextantis C, a 12th magnitude companion.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "8 Sextantis, Gamma Sextantis, HIP 48437AB, SAO 137199, HD 85558, GC 13593, HR 3909, DM BD-07  2909, TYC 5475-1379-1",
	"group" : { "backgroundImage" : "images/Alignment/20.png",
		"description" : "Sextans is a minor equatorial constellation which was introduced in 1687 by Johannes Hevelius. Its name is Latin for the astronomical sextant, an instrument that Hevelius made frequent use of in his observations.\r\rSextans as a constellation covers a rather dim, sparse region of the sky. It has only one star above the fifth magnitude, namely \u03B1 Sextantis at 4.49m. The constellation contains a few double stars, including \u03B3, 35, and 40 Sextantis. There are a few notable variable stars, including \u03B2, 25, 23 Sextantis, and LHS 292. NGC 3115, an edge-on lenticular galaxy, is the only noteworthy deep-sky object. It also lies near the ecliptic, which causes the Moon, and some of the planets to occasionally pass through it for brief periods of time.\r\rThe constellation is the location of the field studied by the COSMOS project, undertaken by the Hubble Space Telescope.\r\rSextans B is a fairly bright dwarf irregular galaxy at magnitude 6.6, 4.3 million light-years from Earth. It is part of the Local Group of galaxies.",
		"key" : "Sextans",
		"grouptype" : "Sextans",
		"Meaning" : "sextant",
		"Family" : "Hercules",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Sextans",
		"title" : "Sextans Objects Group" },
	"Common" : "Gamma Sextantis",
	"OType" : "Star",
	"Distance" : "84.81",
	"RA_S" : 148.12687824,
	"DEC_S" : -8.10499898,
	"X" : 613,
	"Y" : 343,
	"Constellation" : "Sextans ",
	"AMag" : 5.112,
	"key" : 57311,
	"title" : "Gamma Sextantis"
	},
{
	"Index" : "33158",
	"Description" : "Alpha Sextantis (\u03B1 Sex, \u03B1 Sextantis) is the brightest star in the constellation Sextans. It is a white A-type giant with an apparent magnitude of +4.48. It is approximately 287 light years from Earth.\r\rAlpha Sextantis is considered an informal \u0022equator star\u0022, as it lies less than a quarter of a degree south of the celestial equator. In 1900, it was 7 minutes of arc north of the equator. As a result of movement of the Earth\u0027s axial tilt, it crossed over to the Southern Hemisphere in December 1923.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "15 Sextantis, Alpha Sextantis, HIP 49641, SAO 137366, HD 87887, GC 13916, HR 3981, DM BD+00  2615, TYC 4903-1750-1",
	"group" : { "key" : "Sextans" },
	"Common" : "Alpha Sextantis",
	"OType" : "Star",
	"Distance" : "86.13",
	"RA_S" : 151.98452808,
	"X" : 567,
	"Y" : 237,
	"Constellation" : "Sextans ",
	"AMag" : 4.473,
	"key" : 53158,
	"title" : "Alpha Sextantis"
	},
{
	"Index" : "37392",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "22 Sextantis, Epsilon Sextantis, HIP 50414, SAO 137469, HD 89254, GC 14129, HR 4042, DM BD-07  3001, TYC 5490-1694-1",
	"group" : { "key" : "Sextans" },
	"Common" : "Epsilon Sextantis",
	"OType" : "Star",
	"Distance" : "59.29",
	"RA_S" : 154.40750979,
	"DEC_S" : -8.06891415,
	"Constellation" : "Sextans ",
	"AMag" : 5.279,
	"key" : 57392,
	"title" : "Epsilon Sextantis"
	},
{
	"Index" : "33211",
	"Description" : "Delta Sextantis (\u03B4 Sex, \u03B4 Sextantis) is a star in the constellation Sextans.\r\rDelta Sextantis is a blue-white B-type main sequence dwarf with an apparent magnitude of +5.19. It is approximately 300 light years from Earth.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "29 Sextantis, Delta Sextantis, HIP 51362, SAO 137600, HD 90882, GC 14403, HR 4116, DM BD-02  3155, TYC 4908-1773-1",
	"group" : { "key" : "Sextans" },
	"Common" : "Delta Sextantis",
	"OType" : "Star",
	"Distance" : "98.66",
	"RA_S" : 157.36959314,
	"DEC_S" : -2.73907657,
	"X" : 496,
	"Y" : 264,
	"Constellation" : "Sextans ",
	"AMag" : 5.172,
	"key" : 53211,
	"title" : "Delta Sextantis"
	},
{
	"Index" : "33249",
	"Description" : "Beta Sextantis (\u03B2 Sex, \u03B2 Sextantis) is a variable star in the constellation Sextans. Beta Sextantis is a blue-white B-type main sequence dwarf. It is approximately 345 light years from Earth. It is classified as an Alpha2 Canum Venaticorum variable and its brightness varies from magnitude +5.00 to +5.10. The period of this variability is unclear but may be around 15.4 days.",
	"MapNum" : "20",
	"ImageNum" : "20",
	"Desig" : "30 Sextantis, Beta Sextantis, HIP 51437, SAO 137608, HD 90994, GC 14431, HR 4119, DM BD+00  2663, TYC 4912-1381-1",
	"group" : { "key" : "Sextans" },
	"Common" : "Beta Sextantis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "123.77",
	"RA_S" : 157.57283706,
	"DEC_S" : -0.63703152,
	"X" : 494,
	"Y" : 237,
	"Constellation" : "Sextans ",
	"AMag" : 5.039,
	"key" : 53249,
	"title" : "Beta Sextantis"
	},
{
	"Index" : "44800",
	"Description" : "Omicron Tauri (\u03BF Tau, \u03BF Tauri) is a star in the constellation Taurus. Omicron Tauri is a yellow G-type giant with an apparent magnitude of +3.61. This star has three times the mass of the Sun and fifteen to eighteen times the Sun\u0027s radius. Based on the latter, interferometry-measured radius, it is rotating once every 533 days. It is approximately 212 light years from Earth and is radiating 155 times the luminosity of the Sun.\r\rThis is a binary star system with the two components orbiting each other over a period of 1,655 days at an eccentricity of 0.263.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "1 Tauri, Omicron Tauri, HIP 15900, SAO 111172, HD 21120, GC 4070, HR 1030, DM BD+08   511, TYC 650-1471-1",
	"group" : { "backgroundImage" : "images/Alignment/39.png",
		"description" : "Taurus is one of the constellations of the zodiac, which means it is crossed by the plane of the ecliptic. Its name is a Latin word meaning \u0022bull\u0022, and its astrological symbol is a stylized bull\u0027s head: \u2649. Taurus is a large and prominent constellation in the northern hemisphere\u0027s winter sky. It is one of the oldest constellations, dating back to at least the Early Bronze Age when it marked the location of the Sun during the spring equinox. Taurus came to symbolize the bull in the mythologies of Ancient Babylon, Egypt and Greece.\r\rThere are a number of features of interest to astronomers. Taurus hosts two of the nearest open clusters to Earth, the Pleiades and the Hyades, both of which are visible to the naked eye. At first magnitude, the red giant Aldebaran is the brightest star in the constellation. In the northwest part of Taurus is the supernova remnant Messier 1, more commonly known as the Crab Nebula. One of the closest regions of active star location, the Taurus-Auriga complex, crosses into the northern part of the constellation. The variable star T Tauri is the prototype of a class of pre-main-sequence stars.\r\rTaurus is a large and prominent constellation in the northern hemisphere\u0027s winter sky, between Aries to the west and Gemini to the east; to the north lie Perseus and Auriga, to the southeast Orion, to the south Eridanus, and to the southwest Cetus. In September and October, Taurus is visible in the evening along the eastern horizon. The most favorable time to observe Taurus in the night sky is during the months of December and January. By March and April, the constellation will appear to the west during the evening twilight.\r\rThis constellation forms part of the zodiac, and hence is intersected by the ecliptic. This circle across the celestial sphere forms the apparent path of the Sun as the Earth completes its annual orbit. As the orbital plane of the Moon and the planets lie near the ecliptic, they can usually be found in the constellation Taurus during some part of each year. The galactic plane of the Milky Way intersects the northeast corner of the constellation and the galactic anticenter is located near the border between Taurus and Auriga. Taurus is the only constellation crossed by all three of the galactic equator, celestial equator, and ecliptic. A ring-like galactic structure known as the Gould\u0027s Belt passes through the Taurus constellation.\r\rThe recommended three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0022Tau\u0022. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 26 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 03h 23.4m and 05h 53.3m, while the declination coordinates are between 31.10\u00B0 and \u22121.35\u00B0. Because a small part of the constellation lies to the south of the celestial equator, this can not be a completely circumpolar constellation at any latitude.\r\rThe identification of the constellation of Taurus with a bull is very old, certainly dating to the Chalcolithic, and perhaps even to the Upper Paleolithic. Michael Rappengl\u00FCck of the University of Munich believes that Taurus is represented in a cave painting at the Hall of the Bulls in the caves at Lascaux (dated to roughly 15,000 BC), which he believes is accompanied by a depiction of the Pleiades. The name \u0022seven sisters\u0022 has been used for the Pleiades in the languages of many cultures, including indigenous groups of Australia, North America and Siberia. This suggests that the name may have a common ancient origin.\r\rTaurus marked the point of vernal (spring) equinox in the Chalcolithic and the Early Bronze Age (the \u0022Age of Taurus\u0022), from about 4000 BC to 1700 BC, after which it moved into the neighboring constellation Aries. The Pleiades were closest to the Sun at vernal equinox around the 23rd century BC. In Babylonian astronomy, the constellation was listed in the MUL.APIN as GU4.AN.NA, \u0022The Heavenly Bull\u0022. As this constellation marked the vernal equinox, it was also the first constellation in the Babylonian zodiac and they described it as \u0022The Bull in Front\u0022. The Akkadian name was Alu.\r\rIn the Mesopotamian Epic of Gilgamesh, one of the earliest works of literature, the goddess Ishtar sends Taurus, the Bull of Heaven, to kill Gilgamesh for spurning her advances. Gilgamesh is depicted as the neighboring constellation of Orion, and in the sky they face each other as if engaged in combat. In early Mesopotamian art, the Bull of Heaven was closely associated with Inanna, the Sumerian goddess of sexual love, fertility, and warfare. One of the oldest depictions shows the bull standing before the goddess\u0027 standard; since it has 3 stars depicted on its back (the cuneiform sign for \u0022star-constellation\u0022), there is good reason to regard this as the constellation later known as Taurus.\r\rThe same iconic representation of the Heavenly Bull was depicted in the Dendera zodiac, an Egyptian bas-relief carving in a ceiling that depicted the celestial hemisphere using a planisphere. In these ancient cultures, the orientation of the horns was portrayed as upward or backward. This differed from the later Greek depiction where the horns pointed forward. To the Egyptians, the constellation Taurus was a sacred bull that was associated with the renewal of life in spring. When the spring equinox entered Taurus, the constellation would become covered by the Sun in the western sky as spring began. This \u0022sacrifice\u0022 led to the renewal of the land. To the early Hebrews, Taurus was the first constellation in their zodiac and consequently it was represented by the first letter in their alphabet, Aleph.\r\rIn Greek mythology, Taurus was identified with Zeus, who assumed the form of a magnificent white bull to abduct Europa, a legendary Phoenician princess. In illustrations of Greek mythology, only the front portion of this constellation are depicted; this was sometimes explained as Taurus being partly submerged as he carried Europa out to sea. A second Greek myth portrays Taurus as Io, a mistress of Zeus. To hide his lover from his wife Hera, Zeus changed Io into the form of a heifer. Greek mythographer Acusilaus marks the bull Taurus as the same that formed the myth of the Cretan Bull, one of The Twelve Labors of Heracles.\r\rTaurus became an important object of worship among the Druids. Their Tauric religious festival was held while the Sun passed through the constellation. In Buddhism, legends hold that Gautama Buddha was born when the Full Moon was in Vaisakha, or Taurus. Buddha\u0027s birthday is celebrated with the Wesak Festival, or Ves\u0101kha, which occurs on the first or second Full Moon when the Sun is in Taurus.",
		"key" : "Taurus",
		"grouptype" : "Taurus",
		"Meaning" : "bull",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Taurus",
		"title" : "Taurus Objects Group" },
	"Common" : "Omicron Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "88.57",
	"RA_S" : 51.20332798,
	"DEC_S" : 9.02887505,
	"X" : 590,
	"Y" : 439,
	"Constellation" : "Taurus ",
	"AMag" : 3.705,
	"key" : 64800,
	"title" : "Omicron Tauri"
	},
{
	"Index" : "44797",
	"Description" : "Xi Tauri (\u03BE Tau, \u03BE Tauri) is a triple star system in the constellation Taurus. It carries the proper name Ushakaron or Yshakaron, which is Akkadian for \u0022Exacter of Justice and Retribution\u0022 or \u0022The Avenger\u0022 or \u0022The Vindicator\u0022.\r\rXi Tauri a spectroscopic and eclipsing triple star. It consists of three blue-white B-type main sequence dwarfs. Two of the stars are in a close orbit and revolve around each other once every 7.15 days. These in turn orbit the third star once every 145 days. The mean combined apparent magnitude of the system is +3.73 but, because the stars eclipse one another during their orbits, it is classified as a variable star, and its brightness varies from magnitude +3.70 to +3.79. Xi Tauri is approximately 222 light years from Earth.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "2 Tauri, Xi Tauri, HIP 16083AB, SAO 111195, HD 21364, GC 4107, HR 1038, DM BD+09   439, TYC 650-1469-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Ushakaron",
	"OType" : "Eclipsing binary",
	"Distance" : "67.74",
	"RA_S" : 51.79229464,
	"DEC_S" : 9.73267621,
	"X" : 581,
	"Y" : 431,
	"Constellation" : "Taurus ",
	"AMag" : 3.715,
	"key" : 64797,
	"title" : "Ushakaron"
	},
{
	"Index" : "45150",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "4 Tauri, s Tauri, HIP 16322, SAO 93463, HD 21686, GC 4173, HR 1061, DM BD+10   452, TYC 653-1366-1",
	"group" : { "key" : "Taurus" },
	"Common" : "s Tauri",
	"OType" : "Star",
	"Distance" : "110.61",
	"RA_S" : 52.60195434,
	"DEC_S" : 11.33643928,
	"Constellation" : "Taurus ",
	"AMag" : 5.118,
	"key" : 65150,
	"title" : "s Tauri"
	},
{
	"Index" : "45529",
	"Description" : "5 Tauri (5 Tau) is a star in the constellation Taurus. 5 Tauri is an orange K-type giant, a spectroscopic binary, with an apparent magnitude of +4.14. It is approximately 360 light years from Earth.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "5 Tauri, f Tauri, HIP 16369, SAO 93469, HD 21754, GC 4184, HR 1066, DM BD+12   486, TYC 656-1725-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Birhan Isat",
	"OType" : "Spectroscopic binary",
	"Distance" : "104.68",
	"RA_S" : 52.71824103,
	"DEC_S" : 12.93667724,
	"X" : 568,
	"Y" : 390,
	"Constellation" : "Taurus ",
	"AMag" : 4.246,
	"key" : 65529,
	"title" : "Birhan Isat"
	},
{
	"Index" : "44067",
	"Description" : "10 Tauri is a star in the constellation Taurus. Located about 45 light years from the Sun, it is slightly more massive and luminous, and about the same age or older. Spectral classification places it between a dwarf and sub-giant, so it appears to be a well-evolved star that may be near the end of its time on the main sequence. It is a suspected spectroscopic binary, although this has not been confirmed. When viewed through a telescope, there is also a line-of-sight companion.\r\rA debris disk has been identified around 10 Tauri, based on excess infrared radiation detected by IRAS/ISO.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "10 Tauri, HIP 16852, SAO 111292, HD 22484, GC 4313, HR 1101, DM BD-00   572, TYC 64-1569-1",
	"group" : { "key" : "Taurus" },
	"Common" : "10 Tauri",
	"OType" : "High proper-motion Star",
	"Distance" : "13.96",
	"RA_S" : 54.21826305,
	"X" : 555,
	"Y" : 555,
	"Constellation" : "Taurus ",
	"AMag" : 4.353,
	"key" : 64067,
	"title" : "10 Tauri"
	},
{
	"Index" : "6645",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "16 Tauri, HIP 17489, SAO 76126, HD 23288, GC 4475, HR 1140, DM BD+23   505, TYC 1799-1440-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Celaeno",
	"OType" : "Variable Star",
	"Distance" : "121.88",
	"RA_S" : 56.2008923,
	"DEC_S" : 24.28946632,
	"Constellation" : "Taurus ",
	"AMag" : 5.441,
	"key" : 26645,
	"shortTitle" : "Celieno; Celeno; \"Lost Pleiad\"; Tselano; Tselena",
	"title" : "Celaeno"
	},
{
	"Index" : "6646",
	"Description" : "Electra, also cataloged as 17 Tauri, is a blue-white giant star in the constellation of Taurus. The star is one of the nine brightest stars in the Pleiades open cluster. The most visible stars in this group are named for the Seven Sisters of Greek mythology.\r\rThe star has an apparent brightness of 3.72, the third brightest of the stars in the group. Electra belongs to the spectral class B6 IIIe and is approximately 370 light years from the Sun. Electra is one of the four Pleiades stars that is classed as a giant; one that is starting to expand as the internal hydrogen fuel in the core is exhausted.\r\rThe projected rotational velocity of this star is 181 km/s, making it a fast rotator. This is the velocity component of the star\u0027s equatorial rotation along the line of sight to the Earth. The estimated inclination of the star\u0027s pole is 46.8\u00B0 \u00B1 1.6, giving it a true equatorial rotational velocity of 320 \u00B1 18 km/s. The rapid rotation rate of this star flattens the poles and stretch the equator. This makes the surface gravity of the star non-uniform and causes temperature variation. This effect is known as gravity darkening, because it results in a variation of radiation by latitude. The rapid rotation extends the life span of the star by increasing the core density and reducing the radiation output.\r\rThis is classified as a Be star, which is a B-type star with prominent emission lines of hydrogen in its spectrum. The Be stars have a rotation rate that is 1.5\u20132 times the rotation of normal B-type stars. This high rate of rotation may allow mass loss during even minor prominences. Changes in the radial velocity measurements indicate that this star may have a companion, which would make Electra a spectroscopic binary.\r\rInfrared observations of this star showed an excess level of radiation equal to about 0.5 magnitudes. This emission is probably from a gaseous disk created by radiation-driven mass loss and rapid rotation of the star. These disks are created by an ejection of material roughly every ten years, which then settles into the equatorial plane about the star. However, the bright nebulosity that surrounds this star makes the observation uncertain.\r\rElectra is periodically occulted by the Moon and occasionally by other planets in our solar system. The last planetary occultation took place on May 9, 1841, when it was occulted by Venus.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "17 Tauri, HIP 17499, SAO 76131, HD 23302, GC 4477, HR 1142, DM BD+23   507, TYC 1799-1441-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Electra",
	"OType" : "Be Star",
	"Distance" : "124.05",
	"RA_S" : 56.21890368,
	"DEC_S" : 24.11333645,
	"X" : 516,
	"Y" : 246,
	"Constellation" : "Taurus ",
	"AMag" : 3.674,
	"key" : 26646,
	"shortTitle" : "Ehlektra",
	"title" : "Electra"
	},
{
	"Index" : "6708",
	"Description" : "Taygeta is a triple star system in the constellation Taurus and a member of the Pleiades star cluster. It is approximately 440 light years from Earth.\r\rThe primary component, Taygeta A, is a blue-white B-type subgiant with an apparent magnitude of +4.30. It is a spectroscopic binary, whose component stars have magnitudes of +4.6 and +6.1. They are separated by 0.012 arcseconds and complete one orbit every 1313 days. They have an 8th magnitude companion, Taygeta B, 69 arcseconds away.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "19 Tauri, q Tauri, HIP 17531, SAO 76140, HD 23338, GC 4486, HR 1145, DM BD+24   547, TYC 1803-1585-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Taygeta",
	"OType" : "Star",
	"Distance" : "124.39",
	"RA_S" : 56.30206106,
	"DEC_S" : 24.46726881,
	"X" : 515,
	"Y" : 241,
	"Constellation" : "Taurus ",
	"AMag" : 4.272,
	"key" : 26708,
	"shortTitle" : "Taygete; Tajgeta",
	"title" : "Taygeta"
	},
{
	"Index" : "49528",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "29 Tauri, u Tauri, HIP 17563, SAO 111400, HD 23466, GC 4505, HR 1153, DM BD+05   539, TYC 71-1224-1",
	"group" : { "key" : "Taurus" },
	"Common" : "u Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "163.22",
	"RA_S" : 56.4185134,
	"DEC_S" : 6.04999463,
	"Constellation" : "Taurus ",
	"AMag" : 5.319,
	"key" : 69528,
	"title" : "u Tauri"
	},
{
	"Index" : "6644",
	"Description" : "Maia (20 Tauri) is a star in the constellation Taurus. It is the fourth brightest star in the Pleiades open star cluster (M45), after Alcyone, Atlas and Electra, in that order. The name Maia originates with the Greek: \u039C\u03B1\u1FD6\u03B1 and Latin: Maia. She is one of the seven daughters of Atlas and Pleione in Greek mythology\u2014stars which are also included in the Pleaides star cluster (see map). Maia is a blue giant of spectral type B8 III, and a mercury-manganese star. Maia\u0027s visual magnitude is 3.871, requiring darker skies to be seen. Its total bolometric luminosity is 660 times solar, mostly in the ultraviolet, thus suggesting a radius that is 5.5 times that of the Sun and a mass that is slightly more than 4 times solar. Maia is one of the stars in the Maia Nebula (also known as NGC 1432), a bright emission or reflection nebula within the Pleiades star cluster.\r\rMaia was thought to be a variable star by astronomer Otto Struve. A class of stars known as Maia variables was proposed, which included Gamma Ursae Minoris, but Maia and some others in the class have since been found to be stable.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "20 Tauri, HIP 17573, SAO 76155, HD 23408, GC 4500, HR 1149, DM BD+23   516, TYC 1799-1439-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Maia",
	"OType" : "Star",
	"Distance" : "122.38",
	"RA_S" : 56.45669538,
	"DEC_S" : 24.36775119,
	"X" : 512,
	"Y" : 242,
	"Constellation" : "Taurus ",
	"AMag" : 3.849,
	"key" : 26644,
	"shortTitle" : "Majya",
	"title" : "Maia"
	},
{
	"Index" : "6677",
	"Description" : "Merope (23 Tauri) is a star in the constellation Taurus and a member of the Pleiades star cluster. It is approximately 360 light years from Earth.\r\rMerope is a blue-white B-type subgiant with a mean apparent magnitude of +4.14. Richard Hinckley Allen described the star as lucid white and violet. It has a luminosity of 630 times that of the Sun and a surface temperature of 14,000 kelvins. Merope\u0027s mass is roughly 4.5 solar masses and has a radius more than 4 times as great as the Sun\u0027s. It is classified as a Beta Cephei type variable star and its brightness varies by 0.01 magnitudes.\r\rSurrounding Merope is the Merope Nebula. Part of the nebula that the Pleiades Cluster is currently passing through, it appears brightest around Merope and is listed in the Index Catalogue as number IC 349.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "23 Tauri, HIP 17608, SAO 76172, HD 23480, GC 4512, HR 1156, DM BD+23   522, TYC 1800-2204-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Merope",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "122.12",
	"RA_S" : 56.58155286,
	"DEC_S" : 23.94834792,
	"X" : 511,
	"Y" : 249,
	"Constellation" : "Taurus ",
	"AMag" : 4.152,
	"key" : 26677,
	"shortTitle" : "Meropa",
	"title" : "Merope"
	},
{
	"Index" : "6675",
	"Description" : "Alcyone (\u03B7 Tau, \u03B7 Tauri, Eta Tauri) is a star system in the constellation Taurus. It is the brightest star in the Pleiades open cluster, which is a young cluster, aged at less than 50 million years. Alcyone is approximately 370 light years from Earth. It is named after the mythological figure Alcyone, one of the mythological Pleiades. It is known as \u6634\u5BBF\u516D (the Sixth Star of the Hairy Head) in Chinese. The main star, known as Alcyone A, is a blue-white B-type giant similar to many of the other B-type stars in the Pleiades cluster. It has an apparent magnitude of +2.87 (absolute magnitude = \u22122.39), and a radius almost 10 times that of the Sun. Its temperature is approximately 13,000 K giving it a total luminosity that is 2,400 times solar. The spectral type of B7IIIe indicates that emission lines are present in its spectrum. Like many Be stars, Alcyone A has a high rotational velocity of 215 km/s, which has created a gaseous disk flung into orbit around the star from its equator.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "25 Tauri, Eta Tauri, HIP 17702, SAO 76199, HD 23630, GC 4541, HR 1165, DM BD+23   541, TYC 1800-2202-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Alcyone",
	"OType" : "Be Star",
	"Distance" : "123.88",
	"RA_S" : 56.87115231,
	"DEC_S" : 24.10513565,
	"X" : 506,
	"Y" : 247,
	"Constellation" : "Taurus ",
	"AMag" : 2.834,
	"key" : 26675,
	"shortTitle" : "Al'tsiona; Al'tsione",
	"title" : "Alcyone"
	},
{
	"Index" : "45940",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "30 Tauri, e Tauri, HIP 17771, SAO 93611, HD 23793, GC 4568, HR 1174, DM BD+10   486, TYC 661-1403-1",
	"group" : { "key" : "Taurus" },
	"Common" : "e Tauri",
	"OType" : "Variable Star",
	"Distance" : "137.24",
	"RA_S" : 57.06777385,
	"DEC_S" : 11.14329982,
	"Constellation" : "Taurus ",
	"AMag" : 5.055,
	"key" : 65940,
	"title" : "e Tauri"
	},
{
	"Index" : "6680",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 17776, SAO 76215, HD 23753, GC 4564, HR 1172, DM BD+22  563, TYC 1800-2207-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HR 1172",
	"OType" : "Variable Star",
	"Distance" : "122.56",
	"RA_S" : 57.08673343,
	"DEC_S" : 23.42124898,
	"Constellation" : "Taurus ",
	"AMag" : 5.427,
	"key" : 26680,
	"title" : "HR 1172"
	},
{
	"Index" : "6676",
	"Description" : "Atlas is a triple star system in the Pleiades open cluster (M45). It is also known as 27 Tauri.\r\rThe primary component, Atlas A, is a blue-white B-type giant with an apparent magnitude of +3.62. It is a spectroscopic binary whose components have magnitudes of +4.1 and +5.6. The binary makes one orbit every 1250 days. Atlas also has a dimmer magnitude +6.8 companion, Atlas B, at a separation of 0.4 arcseconds or at least 52 astronomical units away.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "27 Tauri, HIP 17847, SAO 76228, HD 23850, GC 4586, HR 1178, DM BD+23   557, TYC 1800-2203-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Atlas",
	"OType" : "Spectroscopic binary",
	"Distance" : "122.28",
	"RA_S" : 57.29059475,
	"DEC_S" : 24.05341343,
	"X" : 500,
	"Y" : 248,
	"Constellation" : "Taurus ",
	"AMag" : 3.601,
	"key" : 26676,
	"title" : "Atlas"
	},
{
	"Index" : "6673",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "28 Tauri, HIP 17851, SAO 76229, HD 23862, GC 4587, HR 1180, DM BD+23   558, TYC 1800-2200-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Pleione",
	"OType" : "Be Star",
	"Distance" : "122.27",
	"RA_S" : 57.29673613,
	"DEC_S" : 24.13670934,
	"Constellation" : "Taurus ",
	"AMag" : 5.028,
	"key" : 26673,
	"shortTitle" : "Plejona; Plejone",
	"title" : "Pleione"
	},
{
	"Index" : "6728",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 17954AB, SAO 76256, HD 23985, GC 4616, HR 1188, DM BD+25  624, TYC 1804-2519-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HR 1188",
	"OType" : "Double or multiple star",
	"Distance" : "56.4",
	"RA_S" : 57.57893316,
	"DEC_S" : 25.57938512,
	"Constellation" : "Taurus ",
	"AMag" : 5.262,
	"key" : 26728,
	"title" : "HR 1188"
	},
{
	"Index" : "46017",
	"Description" : "Lambda Tauri (\u03BB Tau, \u03BB Tauri) is a triple star system in the constellation Taurus. In the Calendarium of Al Achsasi Al Mouakket, this star was designated Sadr al Tauri, which was translated into Latin as Pectus Tauri, meaning \u0022the bull chest\u0022. In 1848, the light from this system was found to vary periodically and it was determined to be an eclipsing binary system\u2014the third such discovered. The components of this system have a combined apparent visual magnitude of +3.47, making it one of the brighter members of the constellation. Based upon parallax measurements from the Hipparcos mission, the distance to this system is approximately 480 light-years (150 parsecs).\r\rThe inner pair of this triple star system, Lambda Tauri AB, orbit around each other with a period of 3.95 days and a low eccentricity of about 0.025. Their orbital plane is inclined by around 76\u00B0 to the line of sight from the Earth, so it is being viewed from nearly edge on and the two stars form an Algol-like eclipsing binary system. The combined brightness of the pair varies from magnitude +3.37 to +3.91 as first one star and then the other pass in front of its companion. The primary member, \u03BB Tau A, undergoes a decrease of 0.435 \u00B1 0.050 in magnitude during an eclipse, while the secondary component, \u03BB Tau B, decreases by 0.09\u20130.10 in magnitude. The mean physical separation between these two stars is estimated at 21.91 times the radius of the Sun, or 0.1 Astronomical Units.\r\rThe primary component has a stellar classification of B3 V, making this a massive B-type main sequence star. It has over seven times the mass of the Sun and 6.4 times the Sun\u0027s radius. This star is the brightest member of the system, radiating about 5,801 times the luminosity of the Sun from its outer envelope at an effective temperature of 18,700 K, which gives it a blue-white hue common to the B-type stars. Lambda Tauri A is rotating rapidly with a projected rotational velocity of 85 km s\u20131. It, along with \u03B4 Librae, were the first stars on which rotational line broadening was observed, by Frank Schlesinger in 1909.\r\rThe spectrum of Lambda Tauri A shows an under abundance of carbon relative to the norm for this category of star. A possible explanation for this is a mass of loss by the star some time in the past. An inner region of the star became depleted by the conversion of carbon into nitrogen during the nuclear fusion process, and this region was later exposed when the outer envelope of the star was lost. Alternatively, the star may have undergone a period of convective mixing, bringing the carbon-depleted material to the surface. However, the cause of such a fully convective behavior in a main sequence star of this mass is unclear.\r\rThe secondary companion has a stellar classification of A4 IV, suggesting that it is a subgiant star that has nearly exhausted the supply of hydrogen at its core and is in the process of evolving into a giant star. It has nearly 1.9 times the mass of the Sun, 5.3 times the Sun\u0027s radius, and is radiating 128 times the Sun\u0027s luminosity at an effective temperature of 8,405 K. As with the primary, this star is spinning rapidly with a projected rotational velocity of 76 km s\u20131. The side of the secondary facing the more massive star is being heated by an additional 1,440 K, which produces a rotational effect that causes the strength of the secondary\u0027s spectral lines to vary over the course of its orbit.\r\rA conundrum with this system is the large radius of the secondary star. In stellar evolutionary terms, the more massive primary should be the first to reach the subgiant stage. Hence the enlarged radius of the secondary must be caused by a means other than the star\u0027s age. This suggests that the pair Lambda Tauri AB form a semidetached binary with the secondary filling its Roche lobe, giving it a distorted shape.\r\rThe third component, \u03BB Tau C, is orbiting the inner pair over a 33.025 day period with an eccentricity of roughly 0.15. The orbital plane of this component is nearly coplanar with the orbit of Lambda Tauri AB, differing by no more than 7\u00B0. It has about half the mass of the Sun. The orbit of this star causes perturbation effects on the orbit of the AB pair, resulting in periodic changes in their orbital eccentricity and other orbital elements.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "35 Tauri, Lambda Tauri, HIP 18724, SAO 93719, HD 25204, GC 4805, HR 1239, DM BD+12   539, TYC 662-1546-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Lambda Tauri",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "148.25",
	"RA_S" : 60.17006453,
	"DEC_S" : 12.49034684,
	"X" : 473,
	"Y" : 399,
	"Constellation" : "Taurus ",
	"AMag" : 3.388,
	"key" : 66017,
	"title" : "Lambda Tauri"
	},
{
	"Index" : "56640",
	"Description" : "Nu Tauri (\u03BD Tau, \u03BD Tauri) is a star in the constellation Taurus. Nu Tauri is a white A-type main sequence dwarf with an apparent magnitude of +3.91. It is approximately 129 light years from Earth. This star is 2.2 times the mass of the Sun, nearly double the Sun\u0027s radius, and is radiating roughly 26 times the Sun\u0027s luminosity.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "38 Tauri, Nu Tauri, HIP 18907, SAO 111579, HD 25490, GC 4862, HR 1251, DM BD+05   581, TYC 79-1585-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Nu Tauri",
	"OType" : "Star",
	"Distance" : "35.85",
	"RA_S" : 60.78908349,
	"DEC_S" : 5.98930391,
	"X" : 467,
	"Y" : 484,
	"Constellation" : "Taurus ",
	"AMag" : 3.888,
	"key" : 76640,
	"title" : "Nu Tauri"
	},
{
	"Index" : "57087",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "40 Tauri, HIP 18957, SAO 111585, HD 25558, GC 4876, HR 1253, DM BD+05   584, TYC 79-826-1",
	"group" : { "key" : "Taurus" },
	"Common" : "40 Tauri",
	"OType" : "Pulsating variable Star",
	"Distance" : "195.54",
	"RA_S" : 60.93585655,
	"DEC_S" : 5.43562248,
	"Constellation" : "Taurus ",
	"AMag" : 5.293,
	"key" : 77087,
	"title" : "40 Tauri"
	},
{
	"Index" : "45785",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 18975, SAO 111586, HD 25570, GC 4883, HR 1254, DM BD+07  592, TYC 659-1274-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HR 1254",
	"OType" : "Star in Cluster",
	"Distance" : "34.85",
	"RA_S" : 60.98584547,
	"DEC_S" : 8.19726924,
	"Constellation" : "Taurus ",
	"AMag" : 5.48,
	"key" : 65785,
	"title" : "HR 1254"
	},
{
	"Index" : "53704",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 18993, SAO 111590, HD 25621, GC 4892, HR 1257, DM BD+02  645, TYC 76-1563-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HD  25621",
	"OType" : "High proper-motion Star",
	"Distance" : "35.39",
	"RA_S" : 61.04114295,
	"DEC_S" : 2.82694308,
	"Constellation" : "Taurus ",
	"AMag" : 5.399,
	"key" : 73704,
	"title" : "HD  25621"
	},
{
	"Index" : "2058",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "37 Tauri, A01 Tauri, HIP 19038, SAO 76430, HD 25604, GC 4897, HR 1256, DM BD+21   585, TYC 1262-1645-1",
	"group" : { "key" : "Taurus" },
	"Common" : "A01 Tauri",
	"OType" : "Star",
	"Distance" : "57.36",
	"RA_S" : 61.17381933,
	"DEC_S" : 22.08192654,
	"Constellation" : "Taurus ",
	"AMag" : 4.463,
	"key" : 22058,
	"title" : "A01 Tauri"
	},
{
	"Index" : "6858",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "41 Tauri, HIP 19171, SAO 76455, HD 25823, GC 4937, HR 1268, DM BD+27   633, TYC 1822-2314-1",
	"group" : { "key" : "Taurus" },
	"Common" : "41 Tauri",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "125.23",
	"RA_S" : 61.6517163,
	"DEC_S" : 27.59990174,
	"Constellation" : "Taurus ",
	"AMag" : 5.151,
	"key" : 26858,
	"title" : "41 Tauri"
	},
{
	"Index" : "6880",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "42 Tauri, Psi Tauri, HIP 19205, SAO 76461, HD 25867, GC 4944, HR 1269, DM BD+28   619, TYC 1826-1575-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Psi Tauri",
	"OType" : "Star",
	"Distance" : "27.6",
	"RA_S" : 61.75189871,
	"DEC_S" : 29.00130375,
	"Constellation" : "Taurus ",
	"AMag" : 5.245,
	"key" : 26880,
	"title" : "Psi Tauri"
	},
{
	"Index" : "6859",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "44 Tauri, p Tauri, HIP 19513, SAO 76485, HD 26322, GC 5020, HR 1287, DM BD+26   686, TYC 1822-2315-1",
	"group" : { "key" : "Taurus" },
	"Common" : "p Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "62.88",
	"RA_S" : 62.70775126,
	"DEC_S" : 26.4809523,
	"Constellation" : "Taurus ",
	"AMag" : 5.427,
	"key" : 26859,
	"title" : "p Tauri"
	},
{
	"Index" : "46307",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "46 Tauri, HIP 19719, SAO 111672, HD 26690, GC 5089, HR 1309, DM BD+07   617, TYC 667-495-1",
	"group" : { "key" : "Taurus" },
	"Common" : "46 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "36.32",
	"RA_S" : 63.38793562,
	"DEC_S" : 7.71604986,
	"Constellation" : "Taurus ",
	"AMag" : 5.332,
	"key" : 66307,
	"title" : "46 Tauri"
	},
{
	"Index" : "46325",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "47 Tauri, HIP 19740A, SAO 111674, HD 26722A, GC 5100, HR 1311, DM BD+08   652, TYC 667-840-1",
	"group" : { "key" : "Taurus" },
	"Common" : "47 Tauri",
	"OType" : "Star",
	"Distance" : "101.21",
	"RA_S" : 63.48492054,
	"DEC_S" : 9.26385629,
	"Constellation" : "Taurus ",
	"AMag" : 5.048,
	"key" : 66325,
	"title" : "47 Tauri"
	},
{
	"Index" : "46513",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 19799, SAO 111680, HD 26793, GC 5111, HR 1315, DM BD+09  550, TYC 671-912-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HR 1315",
	"OType" : "Star",
	"Distance" : "119.75",
	"RA_S" : 63.65097246,
	"DEC_S" : 10.01140764,
	"Constellation" : "Taurus ",
	"AMag" : 5.202,
	"key" : 66513,
	"title" : "HR 1315"
	},
{
	"Index" : "46324",
	"Description" : "Mu Tauri (\u03BC Tau, \u03BC Tauri) is a star in the constellation Taurus. Mu Tauri is a blue-white B-type subgiant with an apparent magnitude of +4.27. It is approximately 435 light years from Earth.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "49 Tauri, Mu Tauri, HIP 19860, SAO 111696, HD 26912, GC 5134, HR 1320, DM BD+08   657, TYC 667-839-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Mu Tauri",
	"OType" : "Star",
	"Distance" : "139.29",
	"RA_S" : 63.88357331,
	"DEC_S" : 8.89235728,
	"X" : 427,
	"Y" : 447,
	"Constellation" : "Taurus ",
	"AMag" : 4.267,
	"key" : 66324,
	"title" : "Mu Tauri"
	},
{
	"Index" : "2153",
	"Description" : "The Bayer designation Omega Tauri (\u03C9 Tau, \u03C9 Tauri) is shared by two star systems, \u03C9\u00B9 Tauri and \u03C9\u00B2 Tauri, in the constellation Taurus. They are separated by 2.13\u00B0 on the sky. Omega-2 Tauri is a white A-type spectroscopic binary star with an apparent magnitude of +4.93. It is approximately 93.5 light years from Earth. Its two components are separated by 0.05 arcseconds, or at least 1.4 astronomical units, and have an orbital period in excess of 14 years.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "50 Tauri, Omega Tauri, HIP 19990, SAO 76532, HD 27045, GC 5172, HR 1329, DM BD+20   724, TYC 1272-1126-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Omega2 Tauri",
	"OType" : "Star",
	"Distance" : "28.94",
	"RA_S" : 64.31525576,
	"DEC_S" : 20.57859111,
	"X" : 457,
	"Y" : 275,
	"Constellation" : "Taurus ",
	"AMag" : 4.947,
	"key" : 22153,
	"title" : "Omega2 Tauri"
	},
{
	"Index" : "2179",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "53 Tauri, HIP 20171, SAO 76548, HD 27295, GC 5210, HR 1339, DM BD+20   733, TYC 1276-1623-1",
	"group" : { "key" : "Taurus" },
	"Common" : "53 Tauri",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "82.69",
	"RA_S" : 64.85873785,
	"DEC_S" : 21.14230744,
	"Constellation" : "Taurus ",
	"AMag" : 5.471,
	"key" : 22179,
	"title" : "53 Tauri"
	},
{
	"Index" : "2177",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "56 Tauri, HIP 20186, SAO 76551, HD 27309, GC 5216, HR 1341, DM BD+21   623, TYC 1276-1621-1",
	"group" : { "key" : "Taurus" },
	"Common" : "56 Tauri",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "99.91",
	"RA_S" : 64.90294288,
	"DEC_S" : 21.77349081,
	"Constellation" : "Taurus ",
	"AMag" : 5.328,
	"key" : 22177,
	"title" : "56 Tauri"
	},
{
	"Index" : "2067",
	"Description" : "Gamma Tauri (\u03B3 Tau, \u03B3 Tauri) is a star in the constellation Taurus and a member of the Hyades star cluster. It has the traditional name Hyadum I, which is Latin for \u0022First Hyad\u0022.\r\rGamma Tauri is a spectral class G8 or K0 giant star with an apparent magnitude of +3.65. It is located within about 2.5 parsecs of the center of the Hyades cluster\u2014the nearest open cluster to the Sun. This star has passed through the main sequence phase is now on the red giant branch where it is using nuclear fusion of helium at its core to provide energy. Age estimates for Gamma Tauri range from 430 million to 530 million years. By comparison, the age of the Hyades cluster is about 625 million years with an error margin of 50 million years.\r\rBased upon parallax measurements, Gamma Tauri is approximately 154 light years from Earth. The angular diameter of this star has been measured using the CHARA array to 2% accuracy. After correcting for limb darkening, this gives the stellar radius as 13.4 times the radius of the Sun. The star is radiating about 85 times the luminosity of the Sun and has 2.7 times the Sun\u0027s mass. With its large size and low projected rotational velocity of 4 km s\u20131, it takes about 253 days to complete a rotation.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "54 Tauri, Gamma Tauri, HIP 20205, SAO 93868, HD 27371, GC 5226, HR 1346, DM BD+15   612, TYC 1264-1009-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Hyadum I",
	"OType" : "Double or multiple star",
	"Distance" : "49.51",
	"RA_S" : 64.9483497,
	"DEC_S" : 15.6276446,
	"X" : 412,
	"Y" : 360,
	"Constellation" : "Taurus ",
	"AMag" : 3.75,
	"key" : 22067,
	"title" : "Hyadum I"
	},
{
	"Index" : "6869",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "52 Tauri, Phi Tauri, HIP 20250, SAO 76558, HD 27382, GC 5240, HR 1348, DM BD+27   655, TYC 1824-1167-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Phi Tauri",
	"OType" : "Star",
	"Distance" : "98.35",
	"RA_S" : 65.08839863,
	"DEC_S" : 27.35075106,
	"Constellation" : "Taurus ",
	"AMag" : 5.079,
	"key" : 26869,
	"title" : "Phi Tauri"
	},
{
	"Index" : "2068",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "58 Tauri, HIP 20261, SAO 93876, HD 27459, GC 5252, HR 1356, DM BD+14   682, TYC 1264-1010-1",
	"group" : { "key" : "Taurus" },
	"Common" : "58 Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "46.93",
	"RA_S" : 65.15129201,
	"DEC_S" : 15.09544997,
	"Constellation" : "Taurus ",
	"AMag" : 5.276,
	"key" : 22068,
	"title" : "58 Tauri"
	},
{
	"Index" : "6840",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "59 Tauri, Chi Tauri, HIP 20430, SAO 76573, HD 27638, GC 5292, HR 1369, DM BD+25   707, TYC 1820-1416-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Chi Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "89.22",
	"RA_S" : 65.64559588,
	"DEC_S" : 25.62931476,
	"Constellation" : "Taurus ",
	"AMag" : 5.372,
	"key" : 26840,
	"title" : "Chi Tauri"
	},
{
	"Index" : "2115",
	"Description" : "The Bayer designation Delta Tauri (\u03B4 Tau, \u03B4 Tauri) is shared by three star systems in the constellation Taurus. They are all members of the Hyades star cluster.\r\rBecause they are close to the ecliptic, these stars can be occulted by the Moon and, very rarely, by planets. The last occultation of \u03B4\u00B9 Tauri by a planet took place on 3 January 1818, when it was occulted by Venus. \u03B4\u00B9 Tauri is a triple star approximately 153 light years from Earth and has the traditional name Hyadum II, which is Latin for \u0022Second Hyad\u0022, and the name Eudora (Greek \u0395\u03C5\u03B4\u03C9\u03C1\u03B7), who was one of the Hyades sisters.\r\rThe primary component, Delta-1 Tauri A, is an orange K-type giant with an apparent magnitude of +3.77. Delta-1 has a luminosity of 74 times that of the Sun and a radius of 11.6 times solar. Its mass is calculated to be 2.6 solar masses. The surface temperature of this star is 4965 kelvins. Its companion, Delta-1 Tauri B, is a 12th magnitude star separated by 107 arcseconds from the primary. It is most likely not physically related to the main star. However, observations of lunar occultations of this star has revealed a much closer, physically related, star that orbits the main star in an eccentric orbit with an average distance of 1.76 AU. This companion takes about 530 days to orbit the main star.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "61 Tauri, Delta Tauri, HIP 20455, SAO 93897, HD 27697, GC 5304, HR 1373, DM BD+17   712, TYC 1268-1267-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Delta1 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.67",
	"RA_S" : 65.73371968,
	"DEC_S" : 17.54251527,
	"X" : 402,
	"Y" : 335,
	"Constellation" : "Taurus ",
	"AMag" : 3.86,
	"key" : 22115,
	"title" : "Delta1 Tauri"
	},
{
	"Index" : "46529",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "66 Tauri, r Tauri, HIP 20522, SAO 111791, HD 27820, GC 5325, HR 1381, DM BD+09   570, TYC 672-1284-1",
	"group" : { "key" : "Taurus" },
	"Common" : "r Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "121.15",
	"RA_S" : 65.96593538,
	"DEC_S" : 9.46096563,
	"Constellation" : "Taurus ",
	"AMag" : 5.109,
	"key" : 66529,
	"title" : "r Tauri"
	},
{
	"Index" : "2125",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "64 Tauri, Delta02 Tauri, HIP 20542, SAO 93907, HD 27819, GC 5328, HR 1380, DM BD+17   714, TYC 1269-1244-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Delta02 Tauri",
	"OType" : "Star",
	"Distance" : "49.46",
	"RA_S" : 66.0240013,
	"DEC_S" : 17.44413435,
	"Constellation" : "Taurus ",
	"AMag" : 4.81,
	"key" : 22125,
	"title" : "Delta02 Tauri"
	},
{
	"Index" : "2188",
	"Description" : "Kappa Tauri (\u03BA Tau, \u03BA Tauri) is a star system in the constellation Taurus and a member of the Hyades open cluster. It is approximately 153 light years from Earth.\r\rThe system is dominated by a visual double star, \u03BA\u00B9 Tauri and \u03BA\u00B2 Tauri. \u03BA\u00B9 Tauri is a white A-type subgiant with an apparent magnitude of +4.21. \u03BA\u00B2 Tauri is a white A-type main sequence dwarf with an apparent magnitude of +5.27. They are 5.8 arcminutes, or at least a quarter light year apart.\r\rBetween the two bright stars is a binary star made up of two 9th magnitude stars, Kappa Tauri C and Kappa Tauri D, which are 5.3 arcseconds from each other and 183 arcseconds from \u03BA\u00B9 Tau. Two more 12th magnitude companions fill out the star system, Kappa Tauri E, which is 136 arcseconds from \u03BA\u00B9 Tau, and Kappa Tauri F, 340 arcseconds away from \u03BA\u00B2 Tau.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "65 Tauri, Kappa Tauri, HIP 20635, SAO 76601, HD 27934, GC 5350, HR 1387, DM BD+21   642, TYC 1277-1626-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Kappa Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "47.19",
	"RA_S" : 66.34236228,
	"DEC_S" : 22.29387398,
	"X" : 394,
	"Y" : 273,
	"Constellation" : "Taurus ",
	"AMag" : 4.215,
	"key" : 22188,
	"title" : "Kappa Tauri"
	},
{
	"Index" : "2189",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "67 Tauri, Kappa02 Tauri, HIP 20641, SAO 76602, HD 27946, GC 5351, HR 1388, DM BD+21   643, TYC 1277-1627-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Kappa02 Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "45.38",
	"RA_S" : 66.35423433,
	"DEC_S" : 22.20000213,
	"Constellation" : "Taurus ",
	"AMag" : 5.294,
	"key" : 22189,
	"title" : "Kappa02 Tauri"
	},
{
	"Index" : "2128",
	"Description" : "The Bayer designation Delta Tauri (\u03B4 Tau, \u03B4 Tauri) is shared by three star systems in the constellation Taurus. They are all members of the Hyades star cluster.\r\rBecause they are close to the ecliptic, these stars can be occulted by the Moon and, very rarely, by planets. The last occultation of \u03B4\u00B9 Tauri by a planet took place on 3 January 1818, when it was occulted by Venus. \u03B4\u00B3 Tauri is a triple star system in the constellation Taurus. It is approximately 148 light years from Earth and is separated from \u03B4\u00B9 Tauri by 0.72\u00B0 on the sky. This star also has the traditional name Cleeia or Kleeia (Greek \u039A\u03BB\u03B5\u03B5\u03B9\u03B1), who was one of the Hyades sisters.\r\rThe primary component, \u03B4\u00B3 Tauri A, is a white A-type subgiant with a mean apparent magnitude of +4.30. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +4.29 to +4.32 with a period of 57.25 days. It has a close, 8th magnitude binary companion, \u03B4\u00B3 Tauri B, 1.4 arcseconds, or at least 64 AU, away. At 77 arcseconds away is the third component, the 11th magnitude \u03B4\u00B3 Tauri C.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "68 Tauri, Delta03 Tauri, HIP 20648B, SAO 93923, HD 27962B, GC 5354, HR 1389, DM BD+17   719, TYC 1269-1246-2",
	"group" : { "key" : "Taurus" },
	"Common" : "Delta3 Tauri",
	"OType" : "High proper-motion Star",
	"Distance" : "45.51",
	"RA_S" : 66.372242,
	"DEC_S" : 17.928361,
	"X" : 394,
	"Y" : 330,
	"Constellation" : "Taurus ",
	"AMag" : 8.366,
	"key" : 22128,
	"title" : "Delta3 Tauri"
	},
{
	"Index" : "2127",
	"Description" : "The Bayer designation Delta Tauri (\u03B4 Tau, \u03B4 Tauri) is shared by three star systems in the constellation Taurus. They are all members of the Hyades star cluster.\r\rBecause they are close to the ecliptic, these stars can be occulted by the Moon and, very rarely, by planets. The last occultation of \u03B4\u00B9 Tauri by a planet took place on 3 January 1818, when it was occulted by Venus. \u03B4\u00B3 Tauri is a triple star system in the constellation Taurus. It is approximately 148 light years from Earth and is separated from \u03B4\u00B9 Tauri by 0.72\u00B0 on the sky. This star also has the traditional name Cleeia or Kleeia (Greek \u039A\u03BB\u03B5\u03B5\u03B9\u03B1), who was one of the Hyades sisters.\r\rThe primary component, \u03B4\u00B3 Tauri A, is a white A-type subgiant with a mean apparent magnitude of +4.30. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +4.29 to +4.32 with a period of 57.25 days. It has a close, 8th magnitude binary companion, \u03B4\u00B3 Tauri B, 1.4 arcseconds, or at least 64 AU, away. At 77 arcseconds away is the third component, the 11th magnitude \u03B4\u00B3 Tauri C.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "68 Tauri, Delta03 Tauri, HIP 20648A, SAO 93923, HD 27962A, GC 5354, HR 1389, DM BD+17   719, TYC 1269-1246-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Delta3 Tauri",
	"OType" : "High proper-motion Star",
	"Distance" : "45.51",
	"RA_S" : 66.37244991,
	"DEC_S" : 17.92790534,
	"X" : 394,
	"Y" : 330,
	"Constellation" : "Taurus ",
	"AMag" : 4.262,
	"key" : 22127,
	"title" : "Delta3 Tauri"
	},
{
	"Index" : "6823",
	"Description" : "Upsilon Tauri (\u03C5 Tau, \u03C5 Tauri) is a triple star system in the constellation Taurus and a member of the Hyades star cluster. It is approximately 155 light years from Earth.\r\rThe primary component, Upsilon Tauri A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.28. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +4.28 to +4.31 with a period of 3.56 hours. It is also a spectroscopic binary, and is composed of two stars with apparent magnitudes of +4.4 and +6.5 which are separated by 0.02 arcseconds, or at least 1 Astronomical Unit. A third star, 12th magnitude in brightness, orbits the pair with a separation of 110 arcseconds.\r\rOccasionally this star system shares the Bayer designation \u03C5 Tauri with 72 Tauri, which is separated from it by 0.29\u00B0 in the sky. 72 Tauri is not a member of the Hyades cluster, being three times farther away from Earth.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "69 Tauri, Upsilon Tauri, HIP 20711, SAO 76608, HD 28024, GC 5370, HR 1392, DM BD+22   696, TYC 1816-1893-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Upsilon Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "47.14",
	"RA_S" : 66.57693588,
	"DEC_S" : 22.81357951,
	"X" : 391,
	"Y" : 267,
	"Constellation" : "Taurus ",
	"AMag" : 4.303,
	"key" : 26823,
	"title" : "Upsilon Tauri"
	},
{
	"Index" : "2085",
	"Description" : "71 Tauri (71 Tau) is a faint star in the constellation Taurus. It is a yellow-white F-type main sequence star with an apparent magnitude of +4.48. It is approximately 156 light years from Earth.\r\rThis star has about 1.94 times the mass of the Sun. It has a projected rotational velocity of 192 km s\u20131, for an estimated rotation period of 14.2 years.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "71 Tauri, HIP 20713, SAO 93932, HD 28052, GC 5375, HR 1394, DM BD+15   625, TYC 1265-1176-1",
	"group" : { "key" : "Taurus" },
	"Common" : "71 Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "49.04",
	"RA_S" : 66.58641399,
	"DEC_S" : 15.61828259,
	"X" : 392,
	"Y" : 360,
	"Constellation" : "Taurus ",
	"AMag" : 4.504,
	"key" : 22085,
	"title" : "71 Tauri"
	},
{
	"Index" : "47091",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "73 Tauri, Pi Tauri, HIP 20732, SAO 93935, HD 28100, GC 5383, HR 1396, DM BD+14   697, TYC 680-993-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Pi Tauri",
	"OType" : "Star",
	"Distance" : "127.59",
	"RA_S" : 66.65155384,
	"DEC_S" : 14.71378525,
	"Constellation" : "Taurus ",
	"AMag" : 4.794,
	"key" : 67091,
	"title" : "Pi Tauri"
	},
{
	"Index" : "6822",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "72 Tauri, HIP 20789, SAO 76613, HD 28149, GC 5396, HR 1399, DM BD+22   699, TYC 1816-1892-1",
	"group" : { "key" : "Taurus" },
	"Common" : "72 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "115.66",
	"RA_S" : 66.82270096,
	"DEC_S" : 22.9963333,
	"Constellation" : "Taurus ",
	"AMag" : 5.498,
	"key" : 26822,
	"title" : "72 Tauri"
	},
{
	"Index" : "2076",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "75 Tauri, HIP 20877, SAO 93950, HD 28292, GC 5427, HR 1407, DM BD+16   605, TYC 1265-1168-1",
	"group" : { "key" : "Taurus" },
	"Common" : "75 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "57.2",
	"RA_S" : 67.10986989,
	"DEC_S" : 16.35967857,
	"Constellation" : "Taurus ",
	"AMag" : 5.095,
	"key" : 22076,
	"title" : "75 Tauri"
	},
{
	"Index" : "2078",
	"Description" : "Theta Tauri (\u03B8 Tau, \u03B8 Tauri) is a double star in the constellation Taurus and a member of the Hyades open cluster. It dominated by two 3rd magnitude stars, \u03B8\u00B9 Tauri and \u03B8\u00B2 Tauri, which are separated by 5.62 arcminutes (0.094\u00B0) on the sky. Based upon parallax measurements, the first component, \u03B8\u00B9 Tauri, is located at a distance of 154.4 ly (47.3 pc), while the second component, \u03B8\u00B2 Tauri is at a distance of 150.4 light-years (46.1 parsecs). If these estimates are correct, then the two components are separated by about four light years and hence are unlikely to form a binary star system.\r\r\u03B8\u00B9 Tauri is the dimmer star, an orange K-type giant with an apparent magnitude of +3.84. \u03B8\u00B2 Tauri is a white A-type giant with a mean apparent magnitude of +3.40. \u03B8\u00B2 Tauri is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.35 to +3.42 with a period of 1.82 hours.\r\rBoth bright stars are spectroscopic binaries and have at least one closer companion. \u03B8\u00B9 Tauri has a 7th magnitude companion 0.082 arcseconds, or at least 4 astronomical units (AU), away from the primary. \u03B8\u00B2 has a 6th magnitude companion 0.005 arcseconds, or at least 2 AU, distant. It completes an orbit once every 141 days.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "77 Tauri, Theta01 Tauri, HIP 20885, SAO 93955, HD 28307, GC 5433, HR 1411, DM BD+15   631, TYC 1265-1170-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Theta1 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "47.32",
	"RA_S" : 67.14374055,
	"DEC_S" : 15.96215799,
	"X" : 385,
	"Y" : 354,
	"Constellation" : "Taurus ",
	"AMag" : 3.936,
	"key" : 22078,
	"title" : "Theta1 Tauri"
	},
{
	"Index" : "2159",
	"Description" : "Epsilon Tauri (\u03B5 Tau, \u03B5 Tauri) is an orange giant star, spectral type of K0 III, located approximately 147 light-years away from the Sun in the constellation of Taurus. It is a member of the Hyades open cluster. It has the traditional names Ain (Arabic \u0639\u064A\u0646), or Oculus Borealis, both of which mean \u0022eye\u0022.\r\rIt has an 11th magnitude companion 182 arcseconds from the primary.\r\rSince Epsilon Tauri lies near the plane of the ecliptic, it is sometimes occulted by the Moon and (very rarely) by planets.\r\rAs a member of the Hyades cluster, Epsilon Tauri\u0027s age is well constrained at 625 million years. Given its large mass, this star was formerly a member of spectral type A that has now evolved off the main sequence into the giant phase. It is regarded as a red clump that burns helium at its core.\r\rIn 2007 a massive extrasolar planet was reported orbiting the star. The planet orbits Epsilon Tauri every 1.6 years in a somewhat eccentric orbit. At the time of the discovery it was the only known planet in an open cluster. No other planets have yet been detected in the Hyades cluster, but another planetary system\u2014Iota Horologii\u2014 belongs to the Hyades stream and may be an escaped member of the cluster.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "74 Tauri, Epsilon Tauri, HIP 20889, SAO 93954, HD 28305, GC 5430, HR 1409, DM BD+18   640, TYC 1273-1104-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Ain / Oculus Borealis",
	"OType" : "Double or multiple star",
	"Distance" : "44.96",
	"RA_S" : 67.1541614,
	"DEC_S" : 19.18043252,
	"X" : 384,
	"Y" : 314,
	"Constellation" : "Taurus ",
	"AMag" : 3.635,
	"key" : 22159,
	"shortTitle" : "Oculus Boreus",
	"title" : "Ain / Oculus Borealis"
	},
{
	"Index" : "2080",
	"Description" : "Theta Tauri (\u03B8 Tau, \u03B8 Tauri) is a double star in the constellation Taurus and a member of the Hyades open cluster. It dominated by two 3rd magnitude stars, \u03B8\u00B9 Tauri and \u03B8\u00B2 Tauri, which are separated by 5.62 arcminutes (0.094\u00B0) on the sky. Based upon parallax measurements, the first component, \u03B8\u00B9 Tauri, is located at a distance of 154.4 ly (47.3 pc), while the second component, \u03B8\u00B2 Tauri is at a distance of 150.4 light-years (46.1 parsecs). If these estimates are correct, then the two components are separated by about four light years and hence are unlikely to form a binary star system.\r\r\u03B8\u00B9 Tauri is the dimmer star, an orange K-type giant with an apparent magnitude of +3.84. \u03B8\u00B2 Tauri is a white A-type giant with a mean apparent magnitude of +3.40. \u03B8\u00B2 Tauri is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.35 to +3.42 with a period of 1.82 hours.\r\rBoth bright stars are spectroscopic binaries and have at least one closer companion. \u03B8\u00B9 Tauri has a 7th magnitude companion 0.082 arcseconds, or at least 4 astronomical units (AU), away from the primary. \u03B8\u00B2 has a 6th magnitude companion 0.005 arcseconds, or at least 2 AU, distant. It completes an orbit once every 141 days.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "78 Tauri, Theta02 Tauri, HIP 20894, SAO 93957, HD 28319, GC 5436, HR 1412, DM BD+15   632, TYC 1265-1172-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Theta2 Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "46.08",
	"RA_S" : 67.16558706,
	"DEC_S" : 15.87088179,
	"X" : 384,
	"Y" : 357,
	"Constellation" : "Taurus ",
	"AMag" : 3.407,
	"key" : 22080,
	"title" : "Theta2 Tauri"
	},
{
	"Index" : "46832",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "79 Tauri, b Tauri, HIP 20901, SAO 93960, HD 28355, GC 5443, HR 1414, DM BD+12   598, TYC 677-1116-1",
	"group" : { "key" : "Taurus" },
	"Common" : "b Tauri",
	"OType" : "High proper-motion Star",
	"Distance" : "48.84",
	"RA_S" : 67.20901646,
	"DEC_S" : 13.04760369,
	"Constellation" : "Taurus ",
	"AMag" : 5.034,
	"key" : 66832,
	"title" : "b Tauri"
	},
{
	"Index" : "2077",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 21029, SAO 93975, HD 28527, GC 5480, HR 1427, DM BD+15  637, TYC 1265-1169-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Gliese 170.1 (HR 1427)",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "43.19",
	"RA_S" : 67.64013379,
	"DEC_S" : 16.19401556,
	"Constellation" : "Taurus ",
	"AMag" : 4.785,
	"key" : 22077,
	"title" : "Gliese 170.1 (HR 1427)"
	},
{
	"Index" : "47101",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "83 Tauri, HIP 21036, SAO 93979, HD 28556, GC 5483, HR 1430, DM BD+13   690, TYC 681-1153-1",
	"group" : { "key" : "Taurus" },
	"Common" : "83 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "45.19",
	"RA_S" : 67.65568259,
	"DEC_S" : 13.72440177,
	"Constellation" : "Taurus ",
	"AMag" : 5.42,
	"key" : 67101,
	"title" : "83 Tauri"
	},
{
	"Index" : "2082",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "81 Tauri, HIP 21039, SAO 93978, HD 28546, GC 5482, HR 1428, DM BD+15   639, TYC 1265-1174-1",
	"group" : { "key" : "Taurus" },
	"Common" : "81 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "44.9",
	"RA_S" : 67.66204197,
	"DEC_S" : 15.69187376,
	"Constellation" : "Taurus ",
	"AMag" : 5.482,
	"key" : 22082,
	"title" : "81 Tauri"
	},
{
	"Index" : "47099",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "86 Tauri, Rho Tauri, HIP 21273, SAO 94007, HD 28910, GC 5558, HR 1444, DM BD+14   720, TYC 681-1151-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Rho Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "48.48",
	"RA_S" : 68.46215695,
	"DEC_S" : 14.84442457,
	"Constellation" : "Taurus ",
	"AMag" : 4.67,
	"key" : 67099,
	"title" : "Rho Tauri"
	},
{
	"Index" : "46589",
	"Description" : "88 Tauri is a multiple star system in the Taurus constellation consisting of a total of six stars.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "88 Tauri, d Tauri, HIP 21402AC, SAO 94026, HD 29140, GC 5599, HR 1458, DM BD+09   607, TYC 673-1488-1",
	"group" : { "key" : "Taurus" },
	"Common" : "88 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "46.05",
	"RA_S" : 68.91360147,
	"DEC_S" : 10.16079261,
	"X" : 362,
	"Y" : 431,
	"Constellation" : "Taurus ",
	"AMag" : 4.272,
	"key" : 66589,
	"title" : "88 Tauri"
	},
{
	"Index" : "59331",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "49 Eridani, HIP 21515, SAO 111928, HD 29335, GC 5627, HR 1469, DM BD+00   798, TYC 82-1777-1",
	"group" : { "key" : "Taurus" },
	"Common" : "49 Eridani",
	"OType" : "Variable Star",
	"Distance" : "258.51",
	"RA_S" : 69.30697047,
	"DEC_S" : 0.99831341,
	"Constellation" : "Taurus ",
	"AMag" : 5.296,
	"key" : 79331,
	"title" : "49 Eridani"
	},
{
	"Index" : "47817",
	"Description" : "90 Tauri (90 Tau) is a star in the constellation Taurus.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "90 Tauri, c01 Tauri, HIP 21589, SAO 94044, HD 29388, GC 5645, HR 1473, DM BD+12   618, TYC 690-1547-1",
	"group" : { "key" : "Taurus" },
	"Common" : "90 Tauri",
	"OType" : "Star",
	"Distance" : "47.04",
	"RA_S" : 69.539426,
	"DEC_S" : 12.51083729,
	"X" : 354,
	"Y" : 401,
	"Constellation" : "Taurus ",
	"AMag" : 4.277,
	"key" : 67817,
	"title" : "90 Tauri"
	},
{
	"Index" : "47210",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "HIP 21670, SAO 111954, HD 29499, GC 5665, HR 1480, DM BD+07  681, TYC 682-1726-1",
	"group" : { "key" : "Taurus" },
	"Common" : "HR 1480",
	"OType" : "Star",
	"Distance" : "49.15",
	"RA_S" : 69.77565747,
	"DEC_S" : 7.87098038,
	"Constellation" : "Taurus ",
	"AMag" : 5.399,
	"key" : 67210,
	"title" : "HR 1480"
	},
{
	"Index" : "2105",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "91 Tauri, Sigma01 Tauri, HIP 21673, SAO 94051, HD 29479, GC 5662, HR 1478, DM BD+15   665, TYC 1266-1419-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Sigma01 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "44.99",
	"RA_S" : 69.78841102,
	"DEC_S" : 15.79986376,
	"Constellation" : "Taurus ",
	"AMag" : 5.093,
	"key" : 22105,
	"title" : "Sigma01 Tauri"
	},
{
	"Index" : "2104",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "92 Tauri, Sigma02 Tauri, HIP 21683, SAO 94054, HD 29488, GC 5666, HR 1479, DM BD+15   666, TYC 1266-1418-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Sigma02 Tauri",
	"OType" : "Star",
	"Distance" : "47.68",
	"RA_S" : 69.81876109,
	"DEC_S" : 15.91797839,
	"Constellation" : "Taurus ",
	"AMag" : 4.686,
	"key" : 22104,
	"title" : "Sigma02 Tauri"
	},
{
	"Index" : "47818",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "93 Tauri, HIP 21735, SAO 94063, HD 29589, GC 5684, HR 1484, DM BD+11   639, TYC 690-1548-1",
	"group" : { "key" : "Taurus" },
	"Common" : "93 Tauri",
	"OType" : "Star",
	"Distance" : "127.46",
	"RA_S" : 70.01423784,
	"DEC_S" : 12.19760374,
	"Constellation" : "Taurus ",
	"AMag" : 5.425,
	"key" : 67818,
	"title" : "93 Tauri"
	},
{
	"Index" : "6901",
	"Description" : "Tau Tauri (\u03C4 Tau, \u03C4 Tauri) is a triple star system in the constellation Taurus. It is approximately 401 light years from Earth.\r\rThe primary component, Tau Tauri A, is a blue-white B-type main sequence dwarf with an apparent V magnitude of +4.26. It has a close companion 0.1 arcseconds away which has a magnitude of +8.9. At a separation of 63 arcseconds is the third component of the system, Tau Tauri C, which is classified as a white A-type star and has a V magnitude of +7.10.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "94 Tauri, Tau Tauri, HIP 21881AS, SAO 76721, HD 29763, GC 5716, HR 1497, DM BD+22   739, TYC 1830-2129-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Tau Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "121.51",
	"RA_S" : 70.56125872,
	"DEC_S" : 22.95694022,
	"X" : 344,
	"Y" : 265,
	"Constellation" : "Taurus ",
	"AMag" : 4.239,
	"key" : 26901,
	"title" : "Tau Tauri"
	},
{
	"Index" : "2257",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "97 Tauri, i Tauri, HIP 22565, SAO 94164, HD 30780, GC 5907, HR 1547, DM BD+18   743, TYC 1288-1706-1",
	"group" : { "key" : "Taurus" },
	"Common" : "i Tauri",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "51.17",
	"RA_S" : 72.84358959,
	"DEC_S" : 18.83986323,
	"Constellation" : "Taurus ",
	"AMag" : 5.115,
	"key" : 22257,
	"title" : "i Tauri"
	},
{
	"Index" : "2289",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "102 Tauri, Iota Tauri, HIP 23497, SAO 76920, HD 32301, GC 6158, HR 1620, DM BD+21   751, TYC 1293-2747-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Iota Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "52.95",
	"RA_S" : 75.77394436,
	"DEC_S" : 21.58996112,
	"Constellation" : "Taurus ",
	"AMag" : 4.633,
	"key" : 22289,
	"title" : "Iota Tauri"
	},
{
	"Index" : "2249",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "104 Tauri, m Tauri, HIP 23835, SAO 94332, HD 32923, GC 6255, HR 1656, DM BD+18   779, TYC 1286-403-1",
	"group" : { "key" : "Taurus" },
	"Common" : "m Tauri",
	"OType" : "Star",
	"Distance" : "15.43",
	"RA_S" : 76.86252944,
	"DEC_S" : 18.64505359,
	"Constellation" : "Taurus ",
	"AMag" : 4.986,
	"key" : 22249,
	"title" : "m Tauri"
	},
{
	"Index" : "2263",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "106 Tauri, l Tauri, HIP 23871, SAO 76971, HD 32977, GC 6259, HR 1658, DM BD+20   885, TYC 1290-1638-1",
	"group" : { "key" : "Taurus" },
	"Common" : "l Tauri",
	"OType" : "High proper-motion Star",
	"Distance" : "58.07",
	"RA_S" : 76.95166816,
	"DEC_S" : 20.41837464,
	"Constellation" : "Taurus ",
	"AMag" : 5.304,
	"key" : 22263,
	"title" : "l Tauri"
	},
{
	"Index" : "2301",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "109 Tauri, n Tauri, HIP 24822, SAO 77097, HD 34559, GC 6506, HR 1739, DM BD+21   816, TYC 1295-1998-1",
	"group" : { "key" : "Taurus" },
	"Common" : "n Tauri",
	"OType" : "Star",
	"Distance" : "75.77",
	"RA_S" : 79.81917315,
	"DEC_S" : 22.09649646,
	"Constellation" : "Taurus ",
	"AMag" : 5.053,
	"key" : 22301,
	"title" : "n Tauri"
	},
{
	"Index" : "2351",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "111 Tauri, HIP 25278, SAO 94526, HD 35296, GC 6645, HR 1780, DM BD+17   920, TYC 1300-2225-1",
	"group" : { "key" : "Taurus" },
	"Common" : "111 Tauri",
	"OType" : "Variable of BY Dra type",
	"Distance" : "14.39",
	"RA_S" : 81.10609841,
	"DEC_S" : 17.38353466,
	"Constellation" : "Taurus ",
	"AMag" : 5.06,
	"key" : 22351,
	"title" : "111 Tauri"
	},
{
	"Index" : "2350",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "115 Tauri, HIP 25499, SAO 94554, HD 35671, GC 6714, HR 1808, DM BD+17   928, TYC 1300-2224-1",
	"group" : { "key" : "Taurus" },
	"Common" : "115 Tauri",
	"OType" : "Star",
	"Distance" : "167.69",
	"RA_S" : 81.79205763,
	"DEC_S" : 17.96221804,
	"Constellation" : "Taurus ",
	"AMag" : 5.388,
	"key" : 22350,
	"title" : "115 Tauri"
	},
{
	"Index" : "2427",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "114 Tauri, o Tauri, HIP 25539, SAO 77184, HD 35708, GC 6723, HR 1810, DM BD+21   847, TYC 1308-2240-1",
	"group" : { "key" : "Taurus" },
	"Common" : "o Tauri",
	"OType" : "Star",
	"Distance" : "191.2",
	"RA_S" : 81.90869034,
	"DEC_S" : 21.9369655,
	"Constellation" : "Taurus ",
	"AMag" : 4.844,
	"key" : 22427,
	"title" : "o Tauri"
	},
{
	"Index" : "7016",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "118 Tauri, HIP 25695B, SAO 77201, HD 35943, GC 6764, HR 1821, DM BD+25   839, TYC 1852-1862-1",
	"group" : { "key" : "Taurus" },
	"Common" : "118 Tauri",
	"OType" : "Star in double system",
	"Distance" : "128.98",
	"RA_S" : 82.31875034,
	"DEC_S" : 25.15021613,
	"Constellation" : "Taurus ",
	"AMag" : 5.47,
	"key" : 27016,
	"title" : "118 Tauri"
	},
{
	"Index" : "2369",
	"Description" : "119 Tauri is a star in the constellation Taurus. It is one of the largest stars known, having a diameter about 600 times that of the Sun. Because it is near the ecliptic, CE Tau is periodically occulted by the moon and its angular diameter can be measured very accurately. It is also close enough that its distance can be determined accurately by parallax and so the actual diameter can be determined directly.\r\r119 Tauri is a M-type red supergiant with a mean apparent magnitude of +4.32. It is approximately 1,800 light years from Earth. The star is classified as a semiregular variable star and its brightness varies from magnitude +4.23 to +4.54 with a period of 165 days. With a colour index of +2.07, this star has been identified as the second reddest in the night sky to shine consistently at a naked eye brightness well above the 5th magnitude. Down to a limiting magnitude of +5, it is superseded in redness only by the Garnet Star (Mu Cephei). 119 Tauri lies 4.6 degrees off the ecliptic. This makes it a candidate for occultations by the Moon and (extremely rarely) by one of the bright planets. The star\u0027s angular diameter and a linear radius of 450 Solar radii have been measured in three colors by lunar occultation.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "119 Tauri, CE Tauri, HIP 25945, SAO 94628, HD 36389, GC 6841, HR 1845, DM BD+18   875, TYC 1301-707-1",
	"group" : { "key" : "Taurus" },
	"Common" : "119 Tauri",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "536.32",
	"RA_S" : 83.05313167,
	"DEC_S" : 18.59423706,
	"X" : 189,
	"Y" : 315,
	"Constellation" : "Taurus ",
	"AMag" : 4.639,
	"key" : 22369,
	"title" : "119 Tauri"
	},
{
	"Index" : "7076",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "121 Tauri, HIP 26248, SAO 77285, HD 36819, GC 6916, HR 1875, DM BD+23   954, TYC 1861-2149-1",
	"group" : { "key" : "Taurus" },
	"Common" : "121 Tauri",
	"OType" : "Star",
	"Distance" : "169.21",
	"RA_S" : 83.86303444,
	"DEC_S" : 24.03959138,
	"Constellation" : "Taurus ",
	"AMag" : 5.355,
	"key" : 27076,
	"title" : "121 Tauri"
	},
{
	"Index" : "2439",
	"Description" : "Zeta Tauri (\u03B6 Tau, \u03B6 Tauri) is a binary star in the zodiac constellation Taurus, the Bull. It has an apparent visual magnitude of 3.0, which is bright enough to be seen with the naked eye. Parallax measurements place it at a distance of roughly 440 light-years from the Earth.\r\rIn Chinese astronomy, Zeta Tauri is called \u5929\u95DC, Pinyin: Ti\u0101ngu\u0101n, meaning Celestial Gate, because this star is marking itself and stand alone in Celestial Gate asterism, Net (mansion) (see : Chinese constellation). \u5929\u95DC (Ti\u0101ngu\u0101n) is westernized into Tien Kwan, but the name Tien Kwan was designated not only for Zeta Tauri, but also for the stars near by, with the meaning is \u0022the Heavenly Gate\u0022 This is a single-lined spectroscopic binary system, which means the two components are orbiting so close to each other that they can not be resolved with a telescope. Instead, the orbital motion of the primary component is indicated by Doppler effect shifts in the absorption lines in its spectrum. The two components are separated by an estimated distance of about 1.17 Astronomical Units, or 117% of the distance from the Earth to the Sun. They are following circular orbits with a period of nearly 133 days.\r\rCompared to the Sun, the primary is an enormous star with more than 11 times the mass and 5\u20136 times the radius. It is rotating rapidly with a projected rotational velocity of 125 km s\u20131. The companion has about 94% the mass of the Sun, although it is unknown whether this is a main sequence star, a neutron star, or a white dwarf. If it is a main sequence star, then the mass indicates it may have a stellar classification of G4.\r\rThe spectrum of the primary component has a stellar classification of B2 IIIpe. A luminosity class of \u0027III\u0027 indicates this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. The \u0027e\u0027 suffix is used for stars that show emission lines in their spectrum. For Be stars such as this, the emission lines are produced by a rotating circumstellar disk of gas, made of material that has been ejected from the star\u0027s outer envelope. An oscillatory pattern in this spectrum is being caused by a single-armed spiral density wave in the disk. The disk may be precessing from the gravitational influence of the secondary component.",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "123 Tauri, Zeta Tauri, HIP 26451, SAO 77336, HD 37202, GC 6985, HR 1910, DM BD+21   908, TYC 1310-2697-1",
	"group" : { "key" : "Taurus" },
	"Common" : "Zeta Tauri",
	"OType" : "Be Star",
	"Distance" : "134.41",
	"RA_S" : 84.41118926,
	"DEC_S" : 21.14254411,
	"X" : 175,
	"Y" : 280,
	"Constellation" : "Taurus ",
	"AMag" : 2.931,
	"key" : 22439,
	"title" : "Zeta Tauri"
	},
{
	"Index" : "7125",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "125 Tauri, HIP 26640, SAO 77360, HD 37438, GC 7047, HR 1928, DM BD+25   902, TYC 1865-2865-1",
	"group" : { "key" : "Taurus" },
	"Common" : "125 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "130.77",
	"RA_S" : 84.93416784,
	"DEC_S" : 25.89709329,
	"Constellation" : "Taurus ",
	"AMag" : 5.142,
	"key" : 27125,
	"title" : "125 Tauri"
	},
{
	"Index" : "2338",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "126 Tauri, HIP 26777AB, SAO 94759, HD 37711, GC 7094, HR 1946, DM BD+16   841, TYC 1298-373-1",
	"group" : { "key" : "Taurus" },
	"Common" : "126 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "189.27",
	"RA_S" : 85.32381687,
	"DEC_S" : 16.53414321,
	"Constellation" : "Taurus ",
	"AMag" : 4.816,
	"key" : 22338,
	"title" : "126 Tauri"
	},
{
	"Index" : "2382",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "130 Tauri, HIP 27338, SAO 94858, HD 38558, GC 7241, HR 1990, DM BD+17  1004, TYC 1303-16-1",
	"group" : { "key" : "Taurus" },
	"Common" : "130 Tauri",
	"OType" : "Star",
	"Distance" : "546.4481",
	"RA_S" : 86.85914986,
	"DEC_S" : 17.72914255,
	"Constellation" : "Taurus ",
	"AMag" : 5.493,
	"key" : 22382,
	"title" : "130 Tauri"
	},
{
	"Index" : "50888",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "133 Tauri, HIP 27364, SAO 94864, HD 38622, GC 7249, HR 1993, DM BD+13   979, TYC 727-1686-1",
	"group" : { "key" : "Taurus" },
	"Common" : "133 Tauri",
	"OType" : "Variable Star",
	"Distance" : "193.04",
	"RA_S" : 86.92878125,
	"DEC_S" : 13.89960445,
	"Constellation" : "Taurus ",
	"AMag" : 5.243,
	"key" : 70888,
	"title" : "133 Tauri"
	},
{
	"Index" : "7138",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "132 Tauri, HIP 27468A, SAO 77592, HD 38751, GC 7283, HR 2002, DM BD+24   970, TYC 1866-2598-1",
	"group" : { "key" : "Taurus" },
	"Common" : "132 Tauri",
	"OType" : "Double or multiple star",
	"Distance" : "111.4827",
	"RA_S" : 87.25399547,
	"DEC_S" : 24.56749571,
	"Constellation" : "Taurus ",
	"AMag" : 4.987,
	"key" : 27138,
	"title" : "132 Tauri"
	},
{
	"Index" : "50631",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "134 Tauri, HIP 27511, SAO 94888, HD 38899, GC 7306, HR 2010, DM BD+12   912, TYC 723-1241-1",
	"group" : { "key" : "Taurus" },
	"Common" : "134 Tauri",
	"OType" : "Star",
	"Distance" : "76.22",
	"RA_S" : 87.38721365,
	"DEC_S" : 12.65132162,
	"Constellation" : "Taurus ",
	"AMag" : 4.865,
	"key" : 70631,
	"title" : "134 Tauri"
	},
{
	"Index" : "7197",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "136 Tauri, HIP 27830, SAO 77675, HD 39357, GC 7389, HR 2034, DM BD+27   899, TYC 1871-2618-1",
	"group" : { "key" : "Taurus" },
	"Common" : "136 Tauri",
	"OType" : "Spectroscopic binary",
	"Distance" : "129.58",
	"RA_S" : 88.33186065,
	"DEC_S" : 27.61226179,
	"Constellation" : "Taurus ",
	"AMag" : 4.55,
	"key" : 27197,
	"title" : "136 Tauri"
	},
{
	"Index" : "7153",
	"MapNum" : "39",
	"ImageNum" : "39",
	"Desig" : "139 Tauri, HIP 28237, SAO 77775, HD 40111, GC 7507, HR 2084, DM BD+25  1052, TYC 1867-3204-1",
	"group" : { "key" : "Taurus" },
	"Common" : "139 Tauri",
	"OType" : "Emission-line Star",
	"Distance" : "471.56",
	"RA_S" : 89.49856803,
	"DEC_S" : 25.95391053,
	"Constellation" : "Taurus ",
	"AMag" : 4.806,
	"key" : 27153,
	"title" : "139 Tauri"
	},
{
	"Index" : "60709",
	"Description" : "Epsilon Telescopii (\u03B5 Tel, \u03B5 Telescopii) is a binary star in the constellation Telescopium. It is approximately 420 light years from Earth.\r\rThe primary component, Epsilon Telescopii A, is an orange K-type giant with an apparent magnitude of +4.52. It has a 13th magnitude companion, Epsilon Telescopii B, 21 arcseconds away from the primary.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Epsilon Telescopii, HIP 89112, SAO 228777, HD 166063, GC 24767, HR 6783, DM CD-45 12251, TYC 8357-3862-1",
	"group" : { "backgroundImage" : "images/Alignment/19.png",
		"description" : "Telescopium is a minor southern constellation created in the 18th century by Nicolas Louis de Lacaille, a French astronomer and student of the southern skies. Its name is a Latinized form of the Greek word for telescope. It was created in honor of the telescope\u0027s invention.\r\rThere are no European names for stars in this constellation. The Chinese did assign names to \u03B1 Tel (We, meaning danger), and \u03B3 Tel (the present-day G Scorpii) as Chuen Shwo, with a mythological meaning.\r\rTelescopium was periodically called \u0022Tubus Astronomicus\u0022; this name is now deprecated.\r\rTelescopium was introduced in 1751-52 by Nicolas Louis de Lacaille with the French name le Telescope, depicting an aerial telescope. It stretched out northwards between Sagittarius and Scorpio. Johann Bode called it the Astronomische Fernrohr in his 1805 Gestirne and kept its size, but Baily and Gould subsequently shrank its boundaries. The much reduced constellation lost several brighter stars to neighbouring constellations: Beta Telescopii became Eta Sagittarii, which it had been before Lacaille placed it in Telescopium, Gamma was placed in Scorpio and renamed G Scorpii by Benjamin Gould, Theta Telescopii reverted to its old appellation of d Ophiuchi, and Sigma Telescopii was placed in Corona Australis. Initially unnamed, it is now known as HR 6875.",
		"key" : "Telescopium",
		"grouptype" : "Telescopium",
		"Meaning" : "telescope",
		"Family" : "La Caille",
		"Origin" : "1763, Lacaille",
		"shortTitle" : "Telescopium",
		"title" : "Telescopium Objects Group" },
	"Common" : "Epsilon Telescopii",
	"OType" : "Star",
	"Distance" : "127.33",
	"RA_S" : 272.80733434,
	"DEC_S" : -45.95441762,
	"X" : 438,
	"Y" : 479,
	"Constellation" : "Telescopium ",
	"AMag" : 4.62,
	"key" : 80709,
	"title" : "Epsilon Telescopii"
	},
{
	"Index" : "64670",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "HIP 89605, SAO 245369, HD 167128, GC 24906, HR 6819, DM CP-56 8706, TYC 8748-2276-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "HR 6819",
	"OType" : "Be Star",
	"Distance" : "232",
	"RA_S" : 274.28138384,
	"DEC_S" : -56.02335146,
	"Constellation" : "Telescopium ",
	"AMag" : 5.353,
	"key" : 84670,
	"title" : "HR 6819"
	},
{
	"Index" : "60730",
	"Description" : "Alpha Telescopii (\u03B1 Tel, \u03B1 Telescopii) is the brightest star in the constellation Telescopium, with an apparent visual magnitude of 3.5. Ptolemy included it in constellation Corona Australis, but it was moved to Telescopium when that constellation was created by Nicolas Louis de Lacaille in the 18th century. Parallax measurements put it at a distance of 278 light-years (85 parsecs) from Earth.\r\rThis star is much larger than the Sun, with about five times the mass and three times the radius. The spectrum of the star matches a stellar classification of B3 IV, where the luminosity class of \u0027IV\u0027 indicates this is a subgiant star that has nearly exhausted the supply of hydrogen at its core and is evolving away from the main sequence. Alpha Telescopii is a bright star that is radiating nearly 800 times the Sun\u0027s luminosity. This energy is being emitted from the star\u0027s outer envelope at an effective temperature of around 16,700 K, giving it the characteristic blue-white hue of a B-type star.\r\rThis is a type of variable star known as a slowly pulsating B star. It has a longitudinal magnetic field with a mean strength of \u2013233 \u00B1 43 G. A projected stellar rotation velocity of about 14 km s\u20131 is considered low for a star of this type, which may indicate it is being viewed from nearly pole-on.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Alpha Telescopii, HIP 90422, SAO 229023, HD 169467, GC 25154, HR 6897, DM CD-46 12379, TYC 8359-3650-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Alpha Telescopii",
	"OType" : "Star",
	"Distance" : "85.16",
	"RA_S" : 276.74339772,
	"DEC_S" : -45.96846635,
	"X" : 403,
	"Y" : 477,
	"Constellation" : "Telescopium ",
	"AMag" : 3.436,
	"key" : 80730,
	"title" : "Alpha Telescopii"
	},
{
	"Index" : "60817",
	"Description" : "Zeta Telescopii (\u03B6 Tel, \u03B6 Telescopii) is the second brightest star in the constellation Telescopium.\r\rZeta Telescopii is a yellow G-type giant with an apparent magnitude of +4.10. It is approximately 127 light years from Earth.",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Zeta Telescopii, HIP 90568, SAO 229047, HD 169767, GC 25183, HR 6905, DM CD-49 12153, TYC 8367-2755-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Zeta Telescopii",
	"OType" : "High proper-motion Star",
	"Distance" : "38.7",
	"RA_S" : 277.2077471,
	"DEC_S" : -49.07058505,
	"X" : 397,
	"Y" : 517,
	"Constellation" : "Telescopium ",
	"AMag" : 4.22,
	"key" : 80817,
	"title" : "Zeta Telescopii"
	},
{
	"Index" : "60729",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Delta01 Telescopii, HIP 90830, SAO 229092, HD 170465, GC 25269, HR 6934, DM CD-45 12550, TYC 8359-3649-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Delta01 Telescopii",
	"OType" : "Spectroscopic binary",
	"Distance" : "216.48",
	"RA_S" : 277.93930781,
	"DEC_S" : -45.91481266,
	"Constellation" : "Telescopium ",
	"AMag" : 4.902,
	"key" : 80729,
	"title" : "Delta01 Telescopii"
	},
{
	"Index" : "60728",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Delta02 Telescopii, HIP 90853, SAO 229095, HD 170523, GC 25273, HR 6938, DM CD-45 12556, TYC 8359-3648-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Delta02 Telescopii",
	"OType" : "Spectroscopic binary",
	"Distance" : "362.36",
	"RA_S" : 278.00810878,
	"DEC_S" : -45.75738358,
	"Constellation" : "Telescopium ",
	"AMag" : 5.048,
	"key" : 80728,
	"title" : "Delta02 Telescopii"
	},
{
	"Index" : "60972",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Kappa Telescopii, HIP 92646, SAO 245772, HD 174295, GC 25859, HR 7087, DM CP-52 11268, TYC 8385-1198-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Kappa Telescopii",
	"OType" : "Star",
	"Distance" : "83.28",
	"RA_S" : 283.16518017,
	"DEC_S" : -52.107373,
	"Constellation" : "Telescopium ",
	"AMag" : 5.28,
	"key" : 80972,
	"title" : "Kappa Telescopii"
	},
{
	"Index" : "64754",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Lambda Telescopii, HIP 93148, SAO 245834, HD 175510, GC 26016, HR 7134, DM CP-53  9402, TYC 8759-2961-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Lambda Telescopii",
	"OType" : "Star",
	"Distance" : "187.12",
	"RA_S" : 284.61569182,
	"DEC_S" : -52.93863011,
	"Constellation" : "Telescopium ",
	"AMag" : 4.829,
	"key" : 84754,
	"title" : "Lambda Telescopii"
	},
{
	"Index" : "60986",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Rho Telescopii, HIP 93815, SAO 245921, HD 177171, GC 26240, HR 7213, DM CP-52 11356, TYC 8386-2339-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Rho Telescopii",
	"OType" : "Star",
	"Distance" : "56.65",
	"RA_S" : 286.58314501,
	"DEC_S" : -52.34091201,
	"Constellation" : "Telescopium ",
	"AMag" : 5.235,
	"key" : 80986,
	"title" : "Rho Telescopii"
	},
{
	"Index" : "64804",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Eta Telescopii, HIP 95261, SAO 246055, HD 181296, GC 26696, HR 7329, DM CP-54  9339, TYC 8765-2571-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Eta Telescopii",
	"OType" : "Double or multiple star",
	"Distance" : "48.21",
	"RA_S" : 290.71335627,
	"DEC_S" : -54.42393097,
	"Constellation" : "Telescopium ",
	"AMag" : 5.022,
	"key" : 84804,
	"title" : "Eta Telescopii"
	},
{
	"Index" : "61037",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Iota Telescopii, HIP 96341, SAO 229751, HD 184127, GC 27025, HR 7424, DM CD-48 13161, TYC 8393-1808-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Iota Telescopii",
	"OType" : "Star",
	"Distance" : "113.46",
	"RA_S" : 293.80411398,
	"DEC_S" : -48.09920243,
	"Constellation" : "Telescopium ",
	"AMag" : 5.001,
	"key" : 81037,
	"title" : "Iota Telescopii"
	},
{
	"Index" : "64921",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Nu Telescopii, HIP 97421, SAO 246271, HD 186543, GC 27358, HR 7510, DM CP-56  9290, TYC 8783-720-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Nu Telescopii",
	"OType" : "Star",
	"Distance" : "49.54",
	"RA_S" : 297.00499213,
	"DEC_S" : -56.36260803,
	"Constellation" : "Telescopium ",
	"AMag" : 5.355,
	"key" : 84921,
	"title" : "Nu Telescopii"
	},
{
	"Index" : "64865",
	"MapNum" : "19",
	"ImageNum" : "19",
	"Desig" : "Xi Telescopii, HIP 99120, SAO 246443, HD 190421, GC 27879, HR 7673, DM CP-53  9794, TYC 8776-1343-1",
	"group" : { "key" : "Telescopium" },
	"Common" : "Xi Telescopii",
	"OType" : "Variable Star",
	"Distance" : "325.87",
	"RA_S" : 301.84648427,
	"DEC_S" : -52.88079032,
	"Constellation" : "Telescopium ",
	"AMag" : 5.1,
	"key" : 84865,
	"title" : "Xi Telescopii"
	},
{
	"Index" : "6431",
	"Description" : "Alpha Trianguli (Alpha Tri, \u03B1 Trianguli, \u03B1 Tri) is the Bayer designation for a binary star in the constellation Triangulum. It has the traditional names Ras al Muthallah (or Mothallah) and Caput Trianguli.\r\rEstimates of the combined stellar classification for this system range from F5III to F6IV, with the luminosity class of \u0027IV\u0027 or \u0027III\u0027 indicating the primary component is a subgiant or giant star, respectively. It is a member of a close binary system\u2014a spectroscopic binary\u2014whose components complete an orbit about their center of mass once every 1.736 days. Because the primary star is rotating rapidly, it has assumed the shape of an oblate spheroid. The ellipsoidal profile of the star, as viewed from Earth, varies over the course of an orbit causing the luminosity to vary in magnitude during the same period. Such stars are termed ellipsoidal variables. Within a few million years, as the primary continues to evolve into a red giant star, the system may become a semi-detached binary with the Roche lobe becoming filled to overflowing.\r\rThe mean apparent magnitude of +3.42 for this pair is bright enough to be readily seen with the naked eye. It forms the second brightest star or star system in this generally faint constellation, following Beta Trianguli. Parallax measurements place this system at a distance of 63.3 light-years (19.4 parsecs) from the Earth. The effective temperature of the primary\u0027s outer envelope is 6,288 K, giving it a yellow-white hue typical of F-type stars. It has a mean radius about three times the radius of the Sun. The system is an estimated 1.6 billion years old.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "2 Trianguli, Alpha Trianguli, HIP 8796, SAO 74996, HD 11443, GC 2272, HR 544, DM BD+28   312, TYC 1763-3028-1",
	"group" : { "backgroundImage" : "images/Alignment/07.png",
		"description" : "Triangulum is a small constellation in the northern sky. Its name is Latin for triangle, which distinguishes it from Triangulum Australe in the southern sky. Its name derives from its three brightest stars, of third and fourth magnitude, which form a nearly isosceles long and narrow triangle. Triangulum was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations.\r\rIn the Babylonian star catalogues, Triangulum together with \u03B3 And formed the constellation known as MULAPIN (\uD808\uDC2F\uD808\uDC33) \u0022The Plough\u0022. It is notable as the first constellation listed in the pair of tablets containing the canonical star lists compiled around 1000 BC, which are thus known as the MUL.APIN by their incipit. The Plough was the first constellation of the \u0022Way of Enlil\u0022, i.e. northernmost quarter of the Sun\u0027s path, corresponding to the 45 days on either side of summer solstice.\r\rAn early name of the constellation was Sicilia, because Ceres, patron goddess of Sicily, was claimed to have begged Jupiter that the island be placed in the heavens.\r\rThe Greeks called Triangulum \u0394\u03B5\u03BB\u03C4\u03C9\u03C4\u03CC\u03BD, as the constellation resembled an upper-case Greek letter delta (\u0394) to the earlier Greeks. It was transliterated into Deltoton by Roman writers. Later, it became the Latin Deltotum. Greek astronomers called it as \u03A4\u03C1\u03AF\u03B3\u03C9\u03BF\u03BD. And later, it became Trigonum. Originally, it represented an equilateral triangle, but is now depicted as a scalene triangle.\r\rIn Chinese astronomy, the stars of Triangulum along with several in Andromeda were incorporated into T\u0027ien-ta-tsiang-kiun (the \u0022Great Celestial General\u0022), the fifth paranatellon of the second house of the White Tiger of the West. Gamma Trianguli represented the General itself, while 14 Trianguli and Upsilon Andromedae represented his standard-bearers. The rest of the stars in Triangulum represented other officers.",
		"key" : "Triangulum",
		"grouptype" : "Triangulum",
		"Meaning" : "triangle",
		"Family" : "Perseus",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Triangulum",
		"title" : "Triangulum Objects Group" },
	"Common" : "Ras al Muthallah",
	"OType" : "Spectroscopic binary",
	"Distance" : "19.42",
	"RA_S" : 28.27045048,
	"DEC_S" : 29.57882527,
	"X" : 535,
	"Y" : 390,
	"Constellation" : "Triangulum ",
	"AMag" : 3.457,
	"key" : 26431,
	"shortTitle" : "Mothallah; Atria (see HD150798); Ras al Muthallah; Elmuthalleth; Caput Trianguli; Metallakh; Motallakh",
	"title" : "Ras al Muthallah"
	},
{
	"Index" : "10852",
	"Description" : "Beta Trianguli (Beta Tri, \u03B2 Trianguli, \u03B2 Tri) is the Bayer designation for a binary star system in the constellation Triangulum, located about 127 light years from Earth. Although the apparent magnitude is only 3.0, it is the brightest star in the constellation Triangulum.\r\rThe star Beta Trianguli has a stellar classification of A5III, indicating that it has evolved away from the main sequence and is now a giant star. It is among the least variable of the stars that were observed by the Hipparcos spacecraft, with a magnitude varying by only 0.0005. This is a probable spectroscopic binary star system with an orbital period of 31.39 days and an eccentricity of 0.43. They are separated by a distance of less than 5 AU.\r\rBased on observations using the Spitzer Space Telescope, as reported in 2005, this system is emitting an excess of infrared radiation. This emission can be explained by a circumbinary ring of dust orbiting at a distance of about 10\u201320 AU from the stars. The dust is emitting infrared radiation at a blackbody temperature of 100 K.",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "4 Trianguli, Beta Trianguli, HIP 10064, SAO 55306, HD 13161, GC 2572, HR 622, DM BD+34   381, TYC 2317-1647-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "Beta Trianguli",
	"OType" : "Spectroscopic binary",
	"Distance" : "38.89",
	"RA_S" : 32.38594355,
	"DEC_S" : 34.98729435,
	"X" : 476,
	"Y" : 331,
	"Constellation" : "Triangulum ",
	"AMag" : 3.017,
	"key" : 30852,
	"title" : "Beta Trianguli"
	},
{
	"Index" : "10797",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "6 Trianguli, HIP 10280A, SAO 55347, HD 13480A, GC 2633, HR 642, DM BD+29   371, TYC 2309-1821-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "6 Trianguli",
	"OType" : "Spectroscopic binary",
	"Distance" : "88.71",
	"RA_S" : 33.09282345,
	"DEC_S" : 30.30307391,
	"Constellation" : "Triangulum ",
	"AMag" : 5.259,
	"key" : 30797,
	"title" : "6 Trianguli"
	},
{
	"Index" : "10837",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "7 Trianguli, HIP 10559, SAO 55397, HD 13869, GC 2710, HR 655, DM BD+32   409, TYC 2314-1819-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "7 Trianguli",
	"OType" : "Star",
	"Distance" : "85.94",
	"RA_S" : 33.98451829,
	"DEC_S" : 33.35889664,
	"Constellation" : "Triangulum ",
	"AMag" : 5.247,
	"key" : 30837,
	"title" : "7 Trianguli"
	},
{
	"Index" : "10859",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "8 Trianguli, Delta Trianguli, HIP 10644, SAO 55420, HD 13974, GC 2733, HR 660, DM BD+33   395, TYC 2318-1874-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "Delta Trianguli",
	"OType" : "Spectroscopic binary",
	"Distance" : "10.78",
	"RA_S" : 34.26346537,
	"DEC_S" : 34.22423504,
	"Constellation" : "Triangulum ",
	"AMag" : 4.933,
	"key" : 30859,
	"title" : "Delta Trianguli"
	},
{
	"Index" : "10860",
	"Description" : "Gamma Trianguli (Gamma Tri, \u03B3 Trianguli, \u03B3 Tri) is a star in the constellation Triangulum located approximately 112 light years from Earth. It has an apparent magnitude of +4.03 and forms an optical (line-of-sight) triple with Delta Trianguli and 7 Trianguli.\r\rThis star has a stellar classification of A1Vnn, which indicates it is an A-type main sequence star. It has 2.7 times the mass of the Sun and nearly double the Sun\u0027s radius. Gamma Trianguli is radiating about 33 times the luminosity of the Sun from its outer envelope at an effective temperature of 9,440 K, giving the star a white hue. The star is roughly 300 million years old.\r\rIt is rotating rapidly, with a projected rotational velocity of 254 km/s along the equator, which causes the star to take the pronounced shape of an oblate spheroid like Altair. Because the inclination of the star\u0027s axial tilt is unknown, this means that the azimuthal equatorial velocity is at least this amount and possibly higher. By comparison, the Sun is a slow rotator with an equatorial azimuthal velocity of 2 km/s. The doppler shift from the rapid rotation results in very diffuse absorption lines in the star\u0027s spectrum, as indicated by the \u0027nn\u0027 in the classification.\r\rOrbiting the star is a dusty debris disk with a combined mass of about 2.9 \u00D7 10\u20132 times the mass of the Earth. This disk can be detected because it is being heated to a temperature of about 75 K by Gamma Trianguli and is radiating this as infrared energy. The disk is separated from the host star by an angle of 2.24 arcseconds, corresponding to a physical radius of 80 AU, or 80 times the separation of the Earth from the Sun.\r\rIn Chinese, \u5929\u5927\u5C07\u8ECD (Ti\u0101n D\u00E0 Ji\u0101ng J\u016Bn), meaning Heaven\u0027s Great General, refers to an asterism consisting of \u03B3 Trianguli, \u03B3 Andromedae, \u03C6 Persei, 51 Andromedae, 49 Andromedae, \u03C7 Andromedae, \u03C5 Andromedae, \u03C4 Andromedae, 56 Andromedae, \u03B2 Trianguli, and \u03B4 Trianguli. Consequently, \u03B3 Trianguli itself is known as \u5929\u5927\u5C07\u8ECD\u5341 (Ti\u0101n D\u00E0 Ji\u0101ng J\u016Bn sh\u00ED, English: the Tenth Star of Heaven\u0027s Great General.).",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "9 Trianguli, Gamma Trianguli, HIP 10670, SAO 55427, HD 14055, GC 2742, HR 664, DM BD+33   397, TYC 2318-1875-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "Gamma Trianguli",
	"OType" : "High proper-motion Star",
	"Distance" : "34.43",
	"RA_S" : 34.32861366,
	"DEC_S" : 33.84719231,
	"X" : 458,
	"Y" : 349,
	"Constellation" : "Triangulum ",
	"AMag" : 3.999,
	"key" : 30860,
	"title" : "Gamma Trianguli"
	},
{
	"Index" : "6510",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "10 Trianguli, HIP 10793, SAO 75276, HD 14252, GC 2781, HR 675, DM BD+27   360, TYC 1777-1481-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "10 Trianguli",
	"OType" : "Star",
	"Distance" : "115.27",
	"RA_S" : 34.73747496,
	"DEC_S" : 28.64267444,
	"Constellation" : "Triangulum ",
	"AMag" : 5.293,
	"key" : 26510,
	"title" : "10 Trianguli"
	},
{
	"Index" : "6521",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "12 Trianguli, HIP 11486, SAO 75382, HD 15257, GC 2956, HR 717, DM BD+29   417, TYC 1778-1522-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "12 Trianguli",
	"OType" : "Star",
	"Distance" : "49.81",
	"RA_S" : 37.0415862,
	"DEC_S" : 29.66933261,
	"Constellation" : "Triangulum ",
	"AMag" : 5.323,
	"key" : 26521,
	"title" : "12 Trianguli"
	},
{
	"Index" : "11014",
	"MapNum" : "07",
	"ImageNum" : "07",
	"Desig" : "14 Trianguli, HIP 11784, SAO 55635, HD 15656, GC 3032, HR 736, DM BD+35   497, TYC 2335-442-1",
	"group" : { "key" : "Triangulum" },
	"Common" : "14 Trianguli",
	"OType" : "Star",
	"Distance" : "132.46",
	"RA_S" : 38.02571095,
	"DEC_S" : 36.14726687,
	"Constellation" : "Triangulum ",
	"AMag" : 5.319,
	"key" : 31014,
	"title" : "14 Trianguli"
	},
{
	"Index" : "69521",
	"Description" : "Gamma Trianguli Australis (\u03B3 TrA, \u03B3 Trianguli Australis) is a star in the constellation Triangulum Australe. Along with Alpha and Beta Trianguli Australis it forms a prominent triangular asterism that gives the constellation its name (Latin for southern triangle). It is the third brightest member of this constellation with an apparent visual magnitude of +2.87. based upon parallax measurements, Gamma Trianguli Australis is located at a distance of about 184 light-years (56 parsecs) from Earth.\r\rThe spectrum of this star matches a stellar classification of A1 V, which identifies it as an A-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. An unusual abundance of the element europium demonstrates it to be a peculiar, or Ap star. Most stars of this type are slow rotators, but Gamma Trianguli Australis displays a very high rate of rotation with a projected rotational velocity of 199 km s\u20131. It has an estimated age of 260 million years.\r\rThis system shows an excess emission of infrared radiation, suggesting that there is a circumstellar disk of dust orbiting this star. The mean temperature of the emission is 50 K, corresponding to a separation from the star of 481 AU.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Gamma Trianguli Australis, HIP 74946, SAO 253097, HD 135382, GC 20538, HR 5671, DM CP-68  2383, TYC 9259-4905-1",
	"group" : { "backgroundImage" : "images/Alignment/03.png",
		"description" : "Triangulum Australe is a small constellation in the far southern celestial hemisphere. Its name is Latin for \u0022the southern triangle\u0022, which distinguishes it from Triangulum in the northern sky and is derived from the almost equilateral pattern of its three brightest stars. It was first depicted on a celestial globe as Triangulus Antarcticus by Petrus Plancius in 1589, and later with more accuracy and its current name by Johann Bayer in his 1603 Uranometria. The French explorer and astronomer Nicolas Louis de Lacaille charted and gave the brighter stars their Bayer designations in 1756.\r\rAlpha Trianguli Australis, known as Atria, is a second magnitude orange giant and the brightest star in the constellation. Completing the triangle are the two white main sequence stars Beta and Gamma Trianguli Australis. Although the constellation lies in the Milky Way and contains many stars, deep-sky objects are not prominent. Notable features include the open cluster NGC 6025 and planetary nebula NGC 5979.\r\rItalian navigator Amerigo Vespucci explored the New World at the beginning of the 16th century. He learnt to recognize the stars in the southern hemisphere and made a catalogue for his patron king Manuel I of Portugal, which is now lost. As well as the catalogue, Vespucci wrote descriptions of the southern stars, including a triangle which may be either Triangulum Australe or Apus. This was sent to his patron in Florence, Lorenzo di Pierfrancesco de\u0027 Medici, and published as Mundus Novus in 1504. The first depiction of the constellation was provided in 1589 by Flemish astronomer and clergyman Petrus Plancius on a 32\u00BD-cm diameter celestial globe published in Amsterdam by Dutch cartographer Jacob Floris van Langren, where it was called Triangulus Antarcticus and incorrectly portrayed to the south of Argo Navis. His student Petrus Keyzer, along with Dutch explorer Frederick de Houtman, coined the name Den Zuyden Trianghel. Triangulum Australe was more accurately depicted in Johann Bayer\u0027s celestial atlas Uranometria in 1603, where it was also given its current name.\r\rNicolas Louis de Lacaille portrayed the constellations of Norma, Circinus and Triangulum Australe as a set square and ruler, a compass, and a surveyor\u0027s level respectively in a set of draughtsman\u0027s instruments in his 1756 map of the southern stars. Also depicting it as a surveyor\u0027s level, German Johann Bode gave it the alternate name of Libella in his Uranographia.\r\rGerman poet and author Philippus Caesius saw the three main stars as representing the Three Patriarchs, Abraham, Isaac and Jacob (with Atria as Abraham). The Wardaman people of the Northern Territory in Australia perceived the stars of Triangulum Australe as the tail of the Rainbow Serpent, which stretched out from near Crux across to Scorpius. Overhead in October, the Rainbow Serpent \u0022gives Lightning a nudge\u0022 to bring on the wet season rains in November.",
		"key" : "Triangulum Australe",
		"grouptype" : "Triangulum Australe",
		"Meaning" : "southern triangle",
		"Family" : "Hercules",
		"Origin" : "1603 Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Triangulum Australe",
		"title" : "Triangulum Australe Objects Group" },
	"Common" : "Gamma Trianguli Australis",
	"OType" : "Variable Star",
	"Distance" : "56.37",
	"RA_S" : 229.72743233,
	"DEC_S" : -68.67954332,
	"X" : 391,
	"Y" : 423,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 2.849,
	"key" : 89521,
	"title" : "Gamma Trianguli Australis"
	},
{
	"Index" : "67504",
	"Description" : "Epsilon Trianguli Australis (\u03B5 TrA, \u03B5 Trianguli Australis) is a wide double star in the southern constellation Triangulum Australe. It is approximately 216 light years from Earth.\r\rThe primary component, Epsilon Trianguli Australis A, is an orange K-type sub-giant with an apparent magnitude of +4.11V. The companion, Epsilon Trianguli Australis B, is a white A-type main sequence dwarf which has an apparent magnitude of +9.32v, and is separated from the primary by 82.1 arcseconds in position angle 218\u00B0 (2001).",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Epsilon Trianguli Australis, HIP 76440, SAO 253226, HD 138538, GC 20932, HR 5771, DM CP-65  3102, TYC 9034-3741-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Epsilon Trianguli Australis",
	"OType" : "Star",
	"Distance" : "61.83",
	"RA_S" : 234.18009209,
	"DEC_S" : -66.31703907,
	"X" : 368,
	"Y" : 393,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 4.234,
	"key" : 87504,
	"title" : "Epsilon Trianguli Australis"
	},
{
	"Index" : "67431",
	"Description" : "Beta Trianguli Australis (\u03B2 TrA, \u03B2 Trianguli Australis) is a double star in the southern circumpolar constellation of Triangulum Australe. It is approximately 40.37 light-years (12.38 parsecs) from Earth and has an apparent visual magnitude of +2.85. This star has a relatively high rate of proper motion across the celestial sphere. It is a F-type main-sequence star with a stellar classification of F1 V. Beta TrA has a 14th magnitude optical companion at an angular separation of 155 arcseconds.\r\rObservation with the Spitzer Space Telescope reveals what appears to be an excess infrared emission from this star. This suggests the presence of circumstellar material in this system, making it a debris disk candidate. This star may be a member of the Beta Pictoris moving group, an association of about 17 stars that share a common origin and a similar motion through space. If it is a member of this group, this would put the age of \u03B2 TrA at about 12 million years; the same as the group itself.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Beta Trianguli Australis, HIP 77952, SAO 253346, HD 141891, GC 21332, HR 5897, DM CP-63  3723, TYC 9027-5712-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Beta Trianguli Australis",
	"OType" : "High proper-motion Star",
	"Distance" : "12.38",
	"RA_S" : 238.78567527,
	"DEC_S" : -63.43072653,
	"X" : 338,
	"Y" : 359,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 2.851,
	"key" : 87431,
	"title" : "Beta Trianguli Australis"
	},
{
	"Index" : "69524",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Kappa Trianguli Australis, HIP 77982, SAO 253342, HD 141767, GC 21328, HR 5891, DM CP-68  2585, TYC 9260-1772-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Kappa Trianguli Australis",
	"OType" : "Star",
	"Distance" : "366.29",
	"RA_S" : 238.87333751,
	"DEC_S" : -68.60299876,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 5.22,
	"key" : 89524,
	"title" : "Kappa Trianguli Australis"
	},
{
	"Index" : "67572",
	"Description" : "Delta Trianguli Australis (\u03B4 TrA, \u03B4 Trianguli Australis) is a binary star in the constellation Triangulum Australe. It is approximately 606 light years (182 parsecs) from Earth.\r\rThe primary component, Delta Trianguli Australis A, is a yellow G-type supergiant with an apparent magnitude of +3.86. The companion, Delta Trianguli Australis B, is a 12th magnitude star separated by 30 arcseconds from the primary.",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Delta Trianguli Australis, HIP 79664, SAO 253474, HD 145544, GC 21819, HR 6030, DM CP-63  3854, TYC 9040-4790-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Delta Trianguli Australis",
	"OType" : "Star",
	"Distance" : "186",
	"RA_S" : 243.85946202,
	"DEC_S" : -63.6856802,
	"X" : 310,
	"Y" : 368,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 3.962,
	"key" : 87572,
	"title" : "Delta Trianguli Australis"
	},
{
	"Index" : "67624",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Iota Trianguli Australis, HIP 80645, SAO 253555, HD 147787, GC 22100, HR 6109, DM CP-63  3923, TYC 9045-2767-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Iota Trianguli Australis",
	"OType" : "Variable Star of gamma Dor type",
	"Distance" : "38.79",
	"RA_S" : 246.98894314,
	"DEC_S" : -64.05794152,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 5.326,
	"key" : 87624,
	"title" : "Iota Trianguli Australis"
	},
{
	"Index" : "69684",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "Zeta Trianguli Australis, HIP 80686, SAO 253554, HD 147584, GC 22089, HR 6098, DM CP-69  2558, TYC 9278-2951-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "Zeta Trianguli Australis",
	"OType" : "Spectroscopic binary",
	"Distance" : "12.12",
	"RA_S" : 247.11725275,
	"DEC_S" : -70.08439912,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 4.963,
	"key" : 89684,
	"title" : "Zeta Trianguli Australis"
	},
{
	"Index" : "67535",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 80874, SAO 253582, HD 148291, GC 22159, HR 6125, DM CP-61 5701, TYC 9037-4020-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "HR 6125",
	"OType" : "Star",
	"Distance" : "239.04",
	"RA_S" : 247.70566837,
	"DEC_S" : -61.63350031,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 5.321,
	"key" : 87535,
	"title" : "HR 6125"
	},
{
	"Index" : "67683",
	"MapNum" : "03",
	"ImageNum" : "03",
	"Desig" : "HIP 82129, SAO 253688, HD 150549, GC 22513, HR 6204, DM CP-66 3009, TYC 9050-2573-1",
	"group" : { "key" : "Triangulum Australe" },
	"Common" : "HR 6204",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "212.83",
	"RA_S" : 251.66662769,
	"DEC_S" : -67.10968925,
	"Constellation" : "Triangulum Australe ",
	"AMag" : 5.084,
	"key" : 87683,
	"title" : "HR 6204"
	},
{
	"Index" : "65325",
	"Description" : "Zeta Tucanae (\u03B6 Tuc, \u03B6 Tucanae) is a star in the constellation Tucana. It is a spectral class F9.5 main sequence star with an apparent magnitude of +4.23. Despite having a slightly lower mass, this star is more luminous than the Sun. Based upon parallax measurements by the Hipparcos spacecraft, it is approximately 28.0 light years from Earth. This is one of the least variable stars observed during the Hipparcos mission.\r\rThe composition and mass of this star are very similar to the Sun, with a slightly lower mass and an estimated age of three billion years. The solar-like qualities make it a target of interest for investigating the possible existence of a life-bearing planet.\r\rBased upon an excess emission of infrared radiation at 70 micrometres, this system is believed to have a debris disk. The disk is orbiting the star at a minimum radius of 2.3 astronomical units. It is radiating with a maximum temperature of 218 K. As of 2009, no planet has been discovered in orbit around this star.\r\rThe components of this star\u0027s space velocity are U = \u221260, V = \u22124 and W = \u221238 km/s. These correspond to the velocity toward the galactic center, the velocity along the direction of galactic rotation, and the velocity toward the north galactic pole, respectively. It is orbiting through the galaxy at a mean distance of 8.4 kpc from the galactic center and with an orbital eccentricity of 0.16.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Zeta Tucanae, HIP 1599, SAO 248163, HD 1581, GC 401, HR 77, DM CP-65    13, TYC 8843-1706-1",
	"group" : { "backgroundImage" : "images/Alignment/29.png",
		"description" : "Tucana is a constellation of stars in the southern sky, created in the late sixteenth century. Its name is Latin for the toucan, a South American bird. This is not a prominent constellation as all of its stars are third magnitude or fainter; the brightest is Alpha Tucanae at apparent visual magnitude 2.87.\r\rThe recommended three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is \u0027Tuc\u0027. The official constellation boundaries, as set by Eug\u00E8ne Delporte in 1930, are defined by a polygon of 10 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 22h 08.45m and 01h 24.82m, while the declination coordinates are between \u201356.31\u00B0 and -75.35\u00B0.\r\rThe constellation was one of twelve created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. It first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rIn 1998, part of the constellation was the subject of a two-week observation program by the Hubble Space Telescope, which resulted in the Hubble Deep Field South.",
		"key" : "Tucana",
		"grouptype" : "Tucana",
		"Meaning" : "toucan",
		"Family" : "Bayer",
		"Origin" : "1603 Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Tucana",
		"title" : "Tucana Objects Group" },
	"Common" : "Zeta Tucanae",
	"OType" : "High proper-motion Star",
	"Distance" : "8.59",
	"RA_S" : 5.01775866,
	"DEC_S" : -64.87479253,
	"X" : 408,
	"Y" : 237,
	"Constellation" : "Tucana ",
	"AMag" : 4.286,
	"key" : 85325,
	"title" : "Zeta Tucanae"
	},
{
	"Index" : "68361",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Pi Tucanae, HIP 1647, SAO 248167, HD 1685, GC 420, HR 83, DM CP-70    12, TYC 9134-2059-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Pi Tucanae",
	"OType" : "Double or multiple star",
	"Distance" : "97.51",
	"RA_S" : 5.16265735,
	"DEC_S" : -69.62491407,
	"Constellation" : "Tucana ",
	"AMag" : 5.491,
	"key" : 88361,
	"title" : "Pi Tucanae"
	},
{
	"Index" : "65334",
	"Description" : "Beta Tucanae (\u03B2 Tuc, \u03B2 Tucanae) is a group of six stars which appear to be at least loosely bound into a system in the constellation Tucana. Three of the stars are luminous enough to have been given their own Bayer designations, \u03B2\u00B9 Tucanae through \u03B2\u00B3 Tucanae. The system is approximately 140 light years from Earth.\r\r\u03B2\u00B9,\u00B2 Tucanae\r\rThe two brightest stars, Beta-1 Tucanae and Beta-2 Tucanae, also referred to as Beta Tucanae A and Beta Tucanae C, are 27 arcseconds, or at least 1100 astronomical units (AU) apart. They are both main sequence dwarfs, Beta-1 a blue-white B-type star with an apparent magnitude of +4.36, and Beta-2 a white A-type star with an apparent magnitude of +4.53.\r\rBoth of these bright stars have at least one closer main sequence companion. Beta Tucanae B is a magnitude +13.5 A-type star which is a close companion to Beta-1, being 2.4 arcseconds, or at least 100 AU away. Beta-2\u0027s companion, the 6th magnitude Beta Tucanae D, is another A-type star which is separated by approximately 0.38 arcseconds (16 AU) from Beta-2.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Beta01 Tucanae, HIP 2484, SAO 248201, HD 2884, GC 625, HR 126, DM CP-63    50A, TYC 8844-1519-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Beta Tucanae",
	"OType" : "Double or multiple star",
	"Distance" : "41.4",
	"RA_S" : 7.88611748,
	"DEC_S" : -62.95822506,
	"X" : 405,
	"Y" : 208,
	"Constellation" : "Tucana ",
	"AMag" : 4.282,
	"key" : 85334,
	"title" : "Beta Tucanae"
	},
{
	"Index" : "65335",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Beta02 Tucanae, HIP 2487, SAO 248202, HD 2885C, GC 626, HR 127, DM CP-63    50C, TYC 8844-1520-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Beta02 Tucanae",
	"OType" : "Star",
	"Distance" : "50.23",
	"RA_S" : 7.8894511,
	"DEC_S" : -62.96556401,
	"Constellation" : "Tucana ",
	"AMag" : 4.505,
	"key" : 85335,
	"title" : "Beta02 Tucanae"
	},
{
	"Index" : "65336",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Beta03 Tucanae, HIP 2578, SAO 248208, HD 3003, GC 651, HR 136, DM CP-63    52, TYC 8844-1521-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Beta03 Tucanae",
	"OType" : "Double or multiple star",
	"Distance" : "45.55",
	"RA_S" : 8.18293856,
	"DEC_S" : -63.03150422,
	"Constellation" : "Tucana ",
	"AMag" : 5.069,
	"key" : 85336,
	"title" : "Beta03 Tucanae"
	},
{
	"Index" : "65361",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Rho Tucanae, HIP 3330, SAO 248237, HD 4089, GC 851, HR 187, DM CP-66    47, TYC 8847-1489-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Rho Tucanae",
	"OType" : "Spectroscopic binary",
	"Distance" : "41.03",
	"RA_S" : 10.61822093,
	"DEC_S" : -65.4680317,
	"Constellation" : "Tucana ",
	"AMag" : 5.439,
	"key" : 85361,
	"title" : "Rho Tucanae"
	},
{
	"Index" : "65315",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Iota Tucanae, HIP 5268, SAO 248324, HD 6793, GC 1372, HR 332, DM CP-62    89, TYC 8842-1781-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Iota Tucanae",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "93.23",
	"RA_S" : 16.82776168,
	"DEC_S" : -61.7752927,
	"Constellation" : "Tucana ",
	"AMag" : 5.439,
	"key" : 85315,
	"title" : "Iota Tucanae"
	},
{
	"Index" : "68380",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Kappa Tucanae, HIP 5896A, SAO 248346, HD 7788, GC 1536, HR 377, DM CP-69    45, TYC 9136-1759-2",
	"group" : { "key" : "Tucana" },
	"Common" : "Kappa Tucanae",
	"OType" : "High proper-motion Star",
	"Distance" : "20.95",
	"RA_S" : 18.94229509,
	"DEC_S" : -68.87597322,
	"Constellation" : "Tucana ",
	"AMag" : 4.997,
	"key" : 88380,
	"title" : "Kappa Tucanae"
	},
{
	"Index" : "68188",
	"Description" : "Alpha Tucanae (\u03B1 Tuc, \u03B1 Tucanae) is a binary star system in the southern circumpolar constellation of Tucana. With an apparent visual magnitude of 2.86, it can be seen with the naked eye from the southern hemisphere. Using parallax measurements, the distance to this system can be estimated as 200 light-years (61 parsecs).\r\rThis is a spectroscopic binary, which means that the two stars have not been individually resolved using a telescope, but the presence of the companion has been inferred from measuring changes in the spectrum of the primary. The orbital period of the binary system is 4197.7 days (11.5 years). The primary component has a stellar classification of K3 III, which indicates it is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence. It has the characteristic orange hue of a K-type star.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Alpha Tucanae, HIP 110130, SAO 255193, HD 211416, GC 31183, HR 8502, DM CP-60  7561, TYC 9117-1947-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Alpha Tucanae",
	"OType" : "Spectroscopic binary",
	"Distance" : "61.14",
	"RA_S" : 334.62539861,
	"DEC_S" : -60.25959646,
	"X" : 581,
	"Y" : 315,
	"Constellation" : "Tucana ",
	"AMag" : 2.998,
	"key" : 88188,
	"title" : "Alpha Tucanae"
	},
{
	"Index" : "65183",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "HIP 110649, SAO 247441, HD 212330, GC 31311, HR 8531, DM CP-58 7954, TYC 8828-1420-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Gliese 857 (HR 8531)",
	"OType" : "Spectroscopic binary",
	"Distance" : "20.56",
	"RA_S" : 336.23482997,
	"DEC_S" : -57.79744484,
	"Constellation" : "Tucana ",
	"AMag" : 5.387,
	"key" : 85183,
	"title" : "Gliese 857 (HR 8531)"
	},
{
	"Index" : "68216",
	"Description" : "Delta Tucanae (\u03B4 Tuc, \u03B4 Tucanae) is a binary star in the constellation Tucana. It is approximately 267 light years from Earth.\r\rThe primary component, Delta Tucanae A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.51. The companion star is a magnitude +9.3 star 7 arcseconds from the primary.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Delta Tucanae, HIP 110838A, SAO 255222, HD 212581, GC 31346, HR 8540, DM CP-65  4044, TYC 9120-1918-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Delta Tucanae",
	"OType" : "Double or multiple star",
	"Distance" : "76.8",
	"RA_S" : 336.83319647,
	"DEC_S" : -64.96635976,
	"X" : 523,
	"Y" : 341,
	"Constellation" : "Tucana ",
	"AMag" : 4.494,
	"key" : 88216,
	"title" : "Delta Tucanae"
	},
{
	"Index" : "68193",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Nu Tucanae, HIP 111310, SAO 255247, HD 213442, GC 31478, HR 8582, DM CP-62  6348, TYC 9118-1191-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Nu Tucanae",
	"OType" : "Long Period Variable candidate",
	"Distance" : "88.92",
	"RA_S" : 338.25026961,
	"DEC_S" : -61.9821241,
	"Constellation" : "Tucana ",
	"AMag" : 5.127,
	"key" : 88193,
	"title" : "Nu Tucanae"
	},
{
	"Index" : "65265",
	"Description" : "Gamma Tucanae (\u03B3 Tuc, \u03B3 Tucanae) is a star in the constellation Tucana.\r\rGamma Tucanae is a yellow-white F-type giant with an apparent magnitude of +3.99. It is approximately 75.3 light years from Earth.\r\rThis star has 1.55 times the mass of the Sun.",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Gamma Tucanae, HIP 114996, SAO 247814, HD 219571, GC 32413, HR 8848, DM CP-58  8062, TYC 8837-1297-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Gamma Tucanae",
	"OType" : "Star",
	"Distance" : "23.05",
	"RA_S" : 349.3574272,
	"DEC_S" : -58.23573669,
	"X" : 537,
	"Y" : 223,
	"Constellation" : "Tucana ",
	"AMag" : 4.033,
	"key" : 85265,
	"title" : "Gamma Tucanae"
	},
{
	"Index" : "68317",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Eta Tucanae, HIP 118121, SAO 255609, HD 224392, GC 33223, HR 9062, DM CP-64  4391, TYC 9130-1766-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Eta Tucanae",
	"OType" : "Star",
	"Distance" : "47.41",
	"RA_S" : 359.39614963,
	"DEC_S" : -64.29822447,
	"Constellation" : "Tucana ",
	"AMag" : 4.997,
	"key" : 88317,
	"title" : "Eta Tucanae"
	},
{
	"Index" : "68347",
	"Description" : "Epsilon Tucanae (\u03B5 Tuc, \u03B5 Tucanae) is a star in the constellation Tucana.\r\rEpsilon Tucanae is a blue-white B-type subgiant with an apparent magnitude of +4.49. It is approximately 374 light years from Earth.\r\rIt is the last star in the Hipparcos catalog, HIP 118322, from the Hipparcos (1989-1993) astrometry satellite (see List of stars in the Hipparcos Catalogue).",
	"MapNum" : "29",
	"ImageNum" : "29",
	"Desig" : "Epsilon Tucanae, HIP 118322, SAO 255619, HD 224686, GC 33280, HR 9076, DM CP-66  3819, TYC 9133-1652-1",
	"group" : { "key" : "Tucana" },
	"Common" : "Epsilon Tucanae",
	"OType" : "Be Star",
	"Distance" : "114.36",
	"RA_S" : 359.979082,
	"DEC_S" : -65.57713312,
	"X" : 428,
	"Y" : 259,
	"Constellation" : "Tucana ",
	"AMag" : 4.473,
	"key" : 88347,
	"title" : "Epsilon Tucanae"
	},
{
	"Index" : "28636",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "55 Camelopardalis, HIP 40215, SAO 14456, HD 67447, GC 11100, HR 3182, DM BD+68   524, TYC 4374-2926-1",
	"group" : { "backgroundImage" : "images/Alignment/40.png",
		"description" : "Ursa Major (Latin: \u0022Larger Bear\u0022), also known as the Great Bear, is a constellation visible throughout the year in most of the northern hemisphere. It can best be seen in April. It is dominated by the widely recognized asterism known as the Big Dipper or Plough, which is a useful pointer toward north, and which has mythological significance in numerous world cultures.\r\rUrsa Major was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy. It is mentioned by such poets as Homer, Spenser, Shakespeare, Tennyson and Bertrand Cantat. The Finnish epic Kalevala mentions it, Vincent van Gogh painted it and Federico Garcia Lorca mentions in his poem \u0022Song for the Moon\u0022 written August 1920. In 2009, the American rock band Third Eye Blind named their fourth album, Ursa Major, after the constellation.\r\rThe constellation of Ursa Major has been seen as a bear by many distinct civilizations. This may stem from a common oral tradition stretching back more than 13,000 years.\r\rIn Burmese, Pucwan T\u0101r\u0101 (pronounced \u0022bazun taja\u0022) is the name of a constellation comprising stars from the head and forelegs of Ursa Major; pucwan is a general term for a crustacean, such as prawn, shrimp, crab, lobster, etc.\r\rIn Greek mythology, Zeus (the king of the gods) lusts after a young woman named Callisto, a nymph of Artemis. Hera, Zeus\u0027 jealous wife, transforms the beautiful Callisto into a bear. Callisto, while in bear form, later encounters her son Arcas. Arcas almost shoots the bear, but to avert the tragedy, Zeus turns them into bears and puts them in the sky, forming Ursa Major and Ursa Minor. Callisto is Ursa Major and her son, Arcas is Ursa Minor. In ancient times the name of the constellation was Helike, (\u0022turning\u0022), because it turns around the Pole. In Book Two of Lucan it is called Parrhasian Helice, since Callisto came from Parrhasia in Arcadia, where the story is set. The Odyssey notes that it is the sole constellation that never sinks below the horizon and \u0022bathes in the Ocean\u0027s waves\u0022. It is also referred to as the \u0022Wain\u0022.\r\rOne of the few star groups mentioned in the Bible (Job 9:9; 38:32; \u2014 Orion and the Pleiades being others), Ursa Major was also pictured as a bear by the Jewish peoples. (\u0022The Bear\u0022 was translated as \u0022Arcturus\u0022 in the Vulgate and it persisted in the KJV.)\r\rIn Finnish language, the asterism is sometimes called with its old Finnish name, Otava. The meaning of the name has been almost forgotten in Modern Finnish; it means a salmon weir.\r\rThe Iroquois Native Americans interpreted Alioth, Mizar, and Alkaid as three hunters pursuing the Great Bear. According to one version of their myth, the first hunter (Alioth) is carrying a bow and arrow to strike down the bear. The second hunter (Mizar) carries a large pot \u2014 the star Alcor \u2014 on his shoulder in which to cook the bear while the third hunter (Alkaid) hauls a pile of firewood to light a fire beneath the pot.\r\rIn Hinduism, Ursa Major is known as Saptarshi, each of the stars representing one of the Saptarshis or Seven Sages viz. Bhrigu, Atri, Angirasa, Vasishta, Pulastya, Pulalaha and Kratu. The fact that the two front stars of the constellations point to the pole star is explained as the boon given to the boy sage Dhruva by Lord Vishnu.\r\rIn Javanese, the brightest seven stars are known as Lintang Wuluh, literally means \u0022seven stars\u0022.\r\rIn South Korea, the constellation is referred to as \u0022the seven stars of the north\u0022. In the related myth, a widow with seven sons found comfort with a widower, but to get to his house required crossing a stream. The seven sons, sympathetic to their mother, placed stepping stones in the river. Their mother, not knowing who put the stones in place, blessed them and, when they died, they became the constellation.\r\rIn Shinto, the 7 largest stars of Ursa Major belong to Amenominakanushi, the oldest and most powerful of all kami.\r\rIn Theosophy, it is believed the Seven Stars of the Pleiades focus the spiritual energy of the Seven Rays from the Galactic Logos to the Seven Stars of the Great Bear, then to Sirius, then to the Sun, then to the god of Earth (Sanat Kumara), and finally through the seven Masters of the Seven Rays to the human race.\r\rIn European star charts, the constellation was visualized with the \u0027square\u0027 of the Big Dipper forming the bear\u0027s body and the chain of stars as a long tail. However, bears do not have long tails, and Jewish astronomers considered Alioth, Mizar, and Alkaid instead to be either three cubs following their mother, and the Native Americans as three hunters.\r\rNoted children\u0027s book author H. A. Rey, in his 1952 book The Stars: A New Way to See Them, (ISBN 0-395-24830-2) instead had the \u0022bear\u0022 image of the constellation, much as Johannes Hevelius had done (as far as the figure of the bear facing \u0022left\u0022), oriented with Alkaid as the tip of the bear\u0027s nose, and the \u0022handle\u0022 of the Big Dipper part of the constellation forming the outline of the top of the bear\u0027s head and neck, rearwards to the shoulder. Because of Rey\u0027s book, many amateur astronomers[who?] have come to accept Rey\u0027s star chart interpretation of Ursa Major, dropping the idea of the Big Dipper\u0027s \u0022handle\u0022 as being the hind end of the bear, with a non-natural \u0022tail\u0022 extending rearwards.",
		"key" : "Ursa Major",
		"grouptype" : "Ursa Major",
		"Meaning" : "great bear",
		"Family" : "Ursa Major",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Ursa Major",
		"title" : "Ursa Major Objects Group" },
	"Common" : "55 Camelopardalis",
	"OType" : "Peculiar Star",
	"Distance" : "229.43",
	"RA_S" : 123.20327842,
	"DEC_S" : 68.47406976,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.443,
	"key" : 48636,
	"title" : "55 Camelopardalis"
	},
{
	"Index" : "26582",
	"Description" : "Omicron Ursae Majoris (Omicron UMa, \u03BF Ursae Majoris, \u03BF UMa) is a star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of +3.35 and is located at a distance of around 179 light-years (55 parsecs) from Earth. This star has the traditional name Muscida, which it shares with the optical double star Pi Ursae Majoris.\r\rThe stellar classification of this star, G4 II\u2013III, places it midway between the giant and bright giant stages of its evolution. The interferometry-measured angular diameter of this star is about 2.42 mas, which, at its estimated distance, equates to a physical radius of about 14 times the radius of the Sun. It has about three times the mass of the Sun and radiates 138 times the Sun\u0027s luminosity from its outer atmosphere at an effective temperature of 5,282 K, giving it the yellowish hue of a G-type star.\r\rIn 1963, East German astronomer Gerhard Jakisch reported this star as a variable with a period of 358 days and an amplitude of 0.08 magnitude. The 1982 edition of the New Catalogue of Suspected Variable Stars listed it with a variability from 3.30 to 3.36 in the visual band. However, in 1992 American astronomer Dorrit Hoffleit noted that the two comparison stars used to determine the variability may themselves be variable. Hence the actual variability of this star may be suspect.\r\rMuscida has a magnitude 15.2 common proper motion companion at an angular separation of 7.1 arcseconds. With a probability of 99.4%, this companion is the source for the X-ray emission from the system. Omicron Ursae Majoris is sometimes listed with two more companions, but, based on proper motion data, these appear to be optical companions.\r\rThis system is a member of the thin disk population and is following an orbit through the Milky Way galaxy with an eccentricity of 0.12. It comes as close to the Galactic Center as 23.5 kly (7.2 kpc) and as distant as 30.2 kly (9.3 kpc). This orbit carries it no more than about 330 ly (100 pc) above the galactic plane. It is considered a runaway star because it has a high peculiar velocity of 35.5 km s\u22121 relative to the typical motion of stars in its vicinity.\r\rIn 2012, extrasolar planet Omicron Ursae Majoris Ab orbiting the primary at 3.9 astronomical units, was found. This gas giant (4.1 times as massive as Jupiter) completes orbit in 1630 days.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "1 Ursae Majoris, Omicron Ursae Majoris, HIP 41704, SAO 14573, HD 71369, GC 11593, HR 3323, DM BD+61  1054, TYC 4127-2431-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Muscida",
	"OType" : "Variable Star",
	"Distance" : "54.91",
	"RA_S" : 127.56612767,
	"DEC_S" : 60.71816987,
	"X" : 603,
	"Y" : 177,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.436,
	"key" : 46582,
	"title" : "Muscida"
	},
{
	"Index" : "26625",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "2 Ursae Majoris, A Ursae Majoris, HIP 42080, SAO 14590, HD 72037, GC 11700, HR 3354, DM BD+65   638, TYC 4133-1970-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "A Ursae Majoris",
	"OType" : "Star",
	"Distance" : "46.73",
	"RA_S" : 128.65048299,
	"DEC_S" : 65.14512876,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.479,
	"key" : 46625,
	"title" : "A Ursae Majoris"
	},
{
	"Index" : "26605",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "4 Ursae Majoris, Pi02 Ursae Majoris, HIP 42527, SAO 14616, HD 73108, GC 11850, HR 3403, DM BD+64   698, TYC 4130-2355-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Muscida (also HD71369,72905)",
	"OType" : "Star",
	"Distance" : "78.45",
	"RA_S" : 130.05342959,
	"DEC_S" : 64.32793567,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.722,
	"key" : 46605,
	"title" : "Muscida (also HD71369,72905)"
	},
{
	"Index" : "20329",
	"Description" : "Iota Ursae Majoris (Iota UMa, \u03B9 Ursae Majoris, \u03B9 UMa) is a star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 3.14, making it visible to the naked eye and placing it among the brighter members of this constellation. Based upon parallax measurements, it is located at a distance of 47.3 light-years (14.5 parsecs) from Earth. It has the traditional names Talitha, Talitha Borealis and Alphikra Borealis, and was also dubbed Dnoces (\u0022Second,\u0022 backwards) after Edward H. White II, an Apollo 1 astronaut. The name was invented by his fellow astronaut Gus Grissom as a practical joke.\r\rThe Iota Ursae Majoris system is composed of two binary stars. The brightest component is a white A-type subgiant. It is a spectroscopic binary whose components have an orbital period of 4028 days. The companion binary is composed of the 9th magnitude and 10th magnitude stars. These two stars orbit around each other with a period of 39.7 years, and are separated by roughly 0.7 arcseconds, or at least 10 AU. This pair may be the source of the X-ray emission detected from this system.\r\rThe two binary systems orbit around each other once every 818 years. The apparent separation between the two binaries is rapidly decreasing as they follow their orbits. In 1841 when the B component was first discovered, they had a separation of 10.7 arcseconds, or at least 156 AU. By 1971 their separation had decreased to 4.5 arcseconds, or at least 66 AU. This system appears to be dynamically unstable with a high likelihood and may become disrupted on a time scale on the order of 105 years.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "9 Ursae Majoris, Iota Ursae Majoris, HIP 44127, SAO 42630, HD 76644, GC 12407, HR 3569, DM BD+48  1707, TYC 3420-2149-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Talitha / Talitha Borealis / Alphikra Borealis / Dnoces",
	"OType" : "Spectroscopic binary",
	"Distance" : "14.51",
	"RA_S" : 134.803387,
	"DEC_S" : 48.042314,
	"X" : 645,
	"Y" : 351,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.128,
	"key" : 40329,
	"shortTitle" : "Talita",
	"title" : "Talitha / Talitha Borealis / Alphikra Borealis / Dnoces"
	},
{
	"Index" : "28643",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "8 Ursae Majoris, Rho Ursae Majoris, HIP 44390, SAO 14742, HD 76827, GC 12447, HR 3576, DM BD+68   551, TYC 4375-2458-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Rho Ursae Majoris",
	"OType" : "Variable Star",
	"Distance" : "96.36",
	"RA_S" : 135.63621989,
	"DEC_S" : 67.62961701,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.942,
	"key" : 48643,
	"title" : "Rho Ursae Majoris"
	},
{
	"Index" : "20352",
	"Description" : "Kappa Ursae Majoris (Kappa UMa, \u03BA Ursae Majoris, \u03BA UMa) is a binary star in the constellation Ursa Major. It is approximately 358 light years from Earth and has the traditional names Talitha Australis, Al Kaprah, and Alphikra Australis.\r\rBoth components of the binary star are a white A-type main sequence dwarfs. They have apparent magnitudes of +4.2 and +4.4, which gives the system a combined apparent magnitude of +3.60. The orbital period of the binary is 35.6 years (13,007.2 days), and the two stars are separated by 0.18 arcseconds.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "12 Ursae Majoris, Kappa Ursae Majoris, HIP 44471AB, SAO 42661, HD 77327, GC 12503, HR 3594, DM BD+47  1633, TYC 3424-1626-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Talitha Australis / Al Kaprah / Alphikra Australis",
	"OType" : "Star",
	"Distance" : "109.49",
	"RA_S" : 135.90636507,
	"DEC_S" : 47.15652473,
	"X" : 642,
	"Y" : 365,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.547,
	"key" : 40352,
	"title" : "Talitha Australis / Al Kaprah / Alphikra Australis"
	},
{
	"Index" : "26633",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "11 Ursae Majoris, Sigma01 Ursae Majoris, HIP 44857, SAO 14769, HD 77800, GC 12576, HR 3609, DM BD+67   573, TYC 4134-1397-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Sigma01 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "159.31",
	"RA_S" : 137.09791984,
	"DEC_S" : 66.87323708,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.317,
	"key" : 46633,
	"title" : "Sigma01 Ursae Majoris"
	},
{
	"Index" : "20409",
	"Description" : "15 Ursae Majoris (15 UMa) is a star in the constellation Ursa Major. Its apparent magnitude is 4.50.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "15 Ursae Majoris, f Ursae Majoris, HIP 44901, SAO 27136, HD 78209, GC 12604, HR 3619, DM BD+52  1365, TYC 3430-1673-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "15 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "28.82",
	"RA_S" : 137.21774014,
	"DEC_S" : 51.60464804,
	"X" : 606,
	"Y" : 317,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.479,
	"key" : 40409,
	"title" : "15 Ursae Majoris"
	},
{
	"Index" : "26686",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "13 Ursae Majoris, Sigma02 Ursae Majoris, HIP 45038A, SAO 14788, HD 78154, GC 12619, HR 3616, DM BD+67   577, TYC 4141-1496-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Sigma02 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "20.38",
	"RA_S" : 137.5980745,
	"DEC_S" : 67.13400723,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.869,
	"key" : 46686,
	"title" : "Sigma02 Ursae Majoris"
	},
{
	"Index" : "26661",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "14 Ursae Majoris, Tau Ursae Majoris, HIP 45075, SAO 14796, HD 78362, GC 12646, HR 3624, DM BD+64   723A, TYC 4138-1687-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Tau Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "38.71",
	"RA_S" : 137.72940686,
	"DEC_S" : 63.51363249,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.684,
	"key" : 46661,
	"title" : "Tau Ursae Majoris"
	},
{
	"Index" : "26645",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "16 Ursae Majoris, c Ursae Majoris, HIP 45333, SAO 14819, HD 79028, GC 12713, HR 3648, DM BD+62  1058, TYC 4135-1915-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "c Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "19.57",
	"RA_S" : 138.58557798,
	"DEC_S" : 61.42331982,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.255,
	"key" : 46645,
	"title" : "c Ursae Majoris"
	},
{
	"Index" : "23879",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "17 Ursae Majoris, HIP 45455, SAO 27185, HD 79354, GC 12748, HR 3660, DM BD+57  1211, TYC 3809-1867-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "17 Ursae Majoris",
	"OType" : "Variable Star",
	"Distance" : "219.44",
	"RA_S" : 138.95743045,
	"DEC_S" : 56.74140732,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.457,
	"key" : 43879,
	"title" : "17 Ursae Majoris"
	},
{
	"Index" : "23853",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "18 Ursae Majoris, e Ursae Majoris, HIP 45493, SAO 27191, HD 79439, GC 12761, HR 3662, DM BD+54  1285, TYC 3806-1813-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "e Ursae Majoris",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "35.84",
	"RA_S" : 139.04720364,
	"DEC_S" : 54.02185653,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.83,
	"key" : 43853,
	"title" : "e Ursae Majoris"
	},
{
	"Index" : "26664",
	"Description" : "23 Ursae Majoris, or 23 UMa, is a binary star system in the constellation Ursa Major. It is approximately 75.5 light years from Earth.\r\rThe primary component is a yellow-white F-type subgiant with an apparent magnitude of +3.65. It has 2.9 times the Sun\u0027s radius and is emitting 15 times the luminosity of the Sun. Orbiting at an angular separation of 22.7 arcseconds is the 9th magnitude secondary companion. There is a magnitude +10.5 optical companion at an angular separation of 99.6 arcseconds.\r\rWith \u03C6, \u03C5, \u03B8, \u03C4, e, and f, it composed the Arabic asterism Sar\u012Br Ban\u0101t al-Na\u0027sh, the Throne of the daughters of Na\u0027sh, and al-Haud, the Pond,",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "23 Ursae Majoris, h Ursae Majoris, HIP 46733, SAO 14908, HD 81937, GC 13109, HR 3757, DM BD+63   845, TYC 4139-1304-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "23 Ursae Majoris",
	"OType" : "Variable Star",
	"Distance" : "23.81",
	"RA_S" : 142.88211972,
	"DEC_S" : 63.06186148,
	"X" : 507,
	"Y" : 196,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.679,
	"key" : 46664,
	"title" : "23 Ursae Majoris"
	},
{
	"Index" : "20424",
	"Description" : "Theta Ursae Majoris (Theta UMa, \u03B8 Ursae Majoris, \u03B8 UMa) is a suspected spectroscopic binary star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 3.17, placing it among the brighter members of this constellation. The distance to this star has been measured directly using the parallax method, yielding an estimated value of 43.96 light-years (13.48 parsecs).\r\rIn 1976, this was reported as a spectroscopic binary system by Helmut A. Abt and Saul G. Levy, giving it an orbital period of 371 days. This has been listed as a spectroscopic binary system with an orbital period of 371 days. However, this was brought into question by Christopher L. Morbey and Roger F. Griffin in 1987, who suggested that the data could be explained by random chance. Further observations in 2009 with observations with the Bok Telescope in Arizona did show changes of 180 m/s in radial velocity, although there was not sufficient evidence to support a Keplerian orbit. There is a 14th-magnitude common proper motion companion to Theta Ursae Majoris at an angular separation of 4.1 arcseconds, so this may potentially be a triple star system.\r\rThe primary component of this putative system has a published stellar classification of F6 IV, indicating it is a subgiant star that is evolving away from the main sequence. In 2009, Helmut A. Abt listed it with a stellar classification of F7 V, suggesting that it is still on the main sequence. It is larger than the Sun with 141% of the Sun\u0027s mass and 250% of the Sun\u0027s radius. Consequently it is shining brighter and evolving more rapidly than the Sun, with a luminosity nearly eight times the Sun\u0027s at an age of 2.2 billion years. This energy is being radiated from the star\u0027s outer atmosphere at an effective temperature of 6,300 K. At this heat, the star glows with the yellow-white hue of an F-type star.\r\rThe McDonald Observatory team has set limits to the hypothetical presence of one or more planets around the primary with masses between 0.24 and 4.6 Jupiter masses and average separations spanning between 0.05 and 5.2 AU.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "25 Ursae Majoris, Theta Ursae Majoris, HIP 46853, SAO 27289, HD 82328, GC 13157, HR 3775, DM BD+52  1401, TYC 3432-1451-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Theta Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "13.48",
	"RA_S" : 143.21430793,
	"DEC_S" : 51.67730032,
	"X" : 562,
	"Y" : 336,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.214,
	"key" : 40424,
	"title" : "Theta Ursae Majoris"
	},
{
	"Index" : "28649",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "24 Ursae Majoris, d Ursae Majoris, HIP 46977, SAO 6897, HD 82210, GC 13171, HR 3771, DM BD+70   565, TYC 4376-2052-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "d Ursae Majoris",
	"OType" : "Variable of RS CVn type",
	"Distance" : "31.93",
	"RA_S" : 143.62025424,
	"DEC_S" : 69.83034343,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.633,
	"key" : 48649,
	"title" : "d Ursae Majoris"
	},
{
	"Index" : "20423",
	"Description" : "26 Ursae Majoris (26 UMa) is a star in the constellation Ursa Major. Its apparent magnitude is 4.48.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "26 Ursae Majoris, HIP 47006, SAO 27298, HD 82621, GC 13212, HR 3799, DM BD+52  1402, TYC 3432-1450-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "26 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "80.36",
	"RA_S" : 143.70597897,
	"DEC_S" : 52.05147831,
	"X" : 556,
	"Y" : 333,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.468,
	"key" : 40423,
	"title" : "26 Ursae Majoris"
	},
{
	"Index" : "28745",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "27 Ursae Majoris, HIP 47654, SAO 6936, HD 83506, GC 13364, HR 3839, DM BD+72   466, TYC 4386-1897-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "27 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "146.43",
	"RA_S" : 145.73827929,
	"DEC_S" : 72.25262039,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.257,
	"key" : 48745,
	"title" : "27 Ursae Majoris"
	},
{
	"Index" : "23890",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "44 Lyncis, HIP 47965, SAO 27377, HD 84335, GC 13442, HR 3870, DM BD+57  1231, TYC 3810-1602-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "44 Lyncis",
	"OType" : "Long Period Variable candidate",
	"Distance" : "168.32",
	"RA_S" : 146.63193508,
	"DEC_S" : 57.12807191,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.311,
	"key" : 43890,
	"title" : "44 Lyncis"
	},
{
	"Index" : "20431",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "15 Leonis Minoris, HIP 48113, SAO 43046, HD 84737, GC 13497, HR 3881, DM BD+46  1551, TYC 3433-1531-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "15 Leonis Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "18.37",
	"RA_S" : 147.14738212,
	"DEC_S" : 46.0210054,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.141,
	"key" : 40431,
	"title" : "15 Leonis Minoris"
	},
{
	"Index" : "23975",
	"Description" : "Upsilon Ursae Majoris (Upsilon UMa, \u03C5 Ursae Majoris, \u03C5 UMa) is a binary star in the constellation Ursa Major. It is approximately 115 light years from Earth.\r\rThe primary component, Upsilon Ursae Majoris A, is a yellow-white F-type subgiant with a mean apparent magnitude of +3.78. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.68 to +3.86 with a period of 3.18 hours.[dubious \u2013 discuss] It has a projected rotational velocity of 110 km s\u20131, an effective temperature of 7,080 K, and a luminosity 29\u201330 times that of the Sun.\r\rThe companion, Upsilon Ursae Majoris B, is a magnitude +11.5 star, 11.3 arcseconds away from the primary.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "29 Ursae Majoris, Upsilon Ursae Majoris, HIP 48319, SAO 27401, HD 84999, GC 13540, HR 3888, DM BD+59  1268, TYC 3820-1522-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Upsilon Ursae Majoris",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "35.64",
	"RA_S" : 147.74732084,
	"DEC_S" : 59.03873572,
	"X" : 497,
	"Y" : 257,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.797,
	"key" : 43975,
	"title" : "Upsilon Ursae Majoris"
	},
{
	"Index" : "23920",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "30 Ursae Majoris, Phi Ursae Majoris, HIP 48402AB, SAO 27408, HD 85235, GC 13559, HR 3894, DM BD+54  1331, TYC 3814-1752-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Phi Ursae Majoris",
	"OType" : "Star",
	"Distance" : "154.44",
	"RA_S" : 148.02650542,
	"DEC_S" : 54.06433787,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.563,
	"key" : 43920,
	"title" : "Phi Ursae Majoris"
	},
{
	"Index" : "20458",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "31 Ursae Majoris, HIP 48682, SAO 27430, HD 85795, GC 13643, HR 3917, DM BD+50  1698, TYC 3436-1469-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "31 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "63.76",
	"RA_S" : 148.92917764,
	"DEC_S" : 49.81984578,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.278,
	"key" : 40458,
	"title" : "31 Ursae Majoris"
	},
{
	"Index" : "16598",
	"Description" : "Lambda Ursae Majoris (Lambda UMa, \u03BB Ursae Majoris, \u03BB UMa) is a star in the northern circumpolar constellation of Ursa Major. It has the proper names Tania Borealis (former Tania borealis).\r\rThis star has an apparent visual magnitude of +3.45, making it one of the brighter members of the constellation. The distance to this star has been measured directly using the parallax technique, which yields a value of roughly 138 light-years (42 parsecs) with a 4% margin of error. The stellar classification of Lambda Ursae Majoris is A2 IV, with the luminosity class of \u0027IV\u0027 indicating that, after 410 million years on the main sequence, this star is in the process of evolving into a giant star as the supply of hydrogen at its core becomes exhausted. Compared to the Sun it has 240% of the mass and 230% of the Sun\u0027s radius, but is radiating 37 times as much luminosity. This energy is being emitted from the star\u0027s outer atmosphere at an effective temperature of 9,280 K, giving it the characteristic white-hot glow of an A-type star.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "33 Ursae Majoris, Lambda Ursae Majoris, HIP 50372, SAO 43268, HD 89021, GC 14113, HR 4033, DM BD+43  2005, TYC 3007-1286-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Tania Borealis",
	"OType" : "High proper-motion Star",
	"Distance" : "42.1",
	"RA_S" : 154.27409528,
	"DEC_S" : 42.91435577,
	"X" : 500,
	"Y" : 474,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.428,
	"key" : 36598,
	"shortTitle" : "Al Kafzah al Thaniyah (with HD89758)",
	"title" : "Tania Borealis"
	},
{
	"Index" : "16579",
	"Description" : "Mu Ursae Majoris (Mu UMa, \u03BC Ursae Majoris, \u03BC UMa) is a star in the constellation Ursa Major. An apparent visual magnitude of +3.06 places it among the brighter members of the constellation. Parallax measurements give an estimated distance of roughly 230 light-years (71 parsecs) from Earth, with a margin of error of 4%. This star has the proper name Tania Australis (formerly Tania australis)\r\rMu Ursae Majoris is an evolved star that is currently in the red giant stage with a stellar classification of M0 IIIab. It has expanded to 75 times the radius of the Sun whilst the outer atmosphere has cooled to an effective temperature of 3,899 K, giving it the orange-red hued glow of an M-type star. Estimates of the luminosity range from 977\u20131,200 times that of the Sun. It is classified as a semiregular variable star and its brightness varies from magnitude 2.99m to 3.33m.\r\rThis is a spectroscopic binary star system with a companion a mere 1.5 AU from the primary with an orbital period of 230 days.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "34 Ursae Majoris, Mu Ursae Majoris, HIP 50801, SAO 43310, HD 89758, GC 14232, HR 4069, DM BD+42  2115, TYC 3004-1418-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Tania Australis",
	"OType" : "Spectroscopic binary",
	"Distance" : "70.5",
	"RA_S" : 155.58225403,
	"DEC_S" : 41.4995165,
	"X" : 491,
	"Y" : 495,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.216,
	"key" : 36579,
	"shortTitle" : "Al Kafzah al Thaniyah (with HD89021)",
	"title" : "Tania Australis"
	},
{
	"Index" : "26758",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 50933, SAO 15163, HD 89822, GC 14260, HR 4072, DM BD+66  664, TYC 4150-1302-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "V* ET UMa",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "104",
	"RA_S" : 156.03269124,
	"DEC_S" : 65.56642121,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.923,
	"key" : 46758,
	"title" : "V* ET UMa"
	},
{
	"Index" : "23966",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "36 Ursae Majoris, HIP 51459, SAO 27670, HD 90839, GC 14427, HR 4112, DM BD+56  1459, TYC 3819-1373-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "36 Ursae Majoris",
	"OType" : "High proper-motion Star",
	"Distance" : "12.78",
	"RA_S" : 157.65657878,
	"DEC_S" : 55.98053929,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.88,
	"key" : 43966,
	"title" : "36 Ursae Majoris"
	},
{
	"Index" : "16589",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 51658, SAO 43379, HD 91312, GC 14491, HR 4132, DM BD+41 2101, TYC 3005-1206-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "HR 4132",
	"OType" : "Spectroscopic binary",
	"Distance" : "34.61",
	"RA_S" : 158.30787094,
	"DEC_S" : 40.42555611,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.742,
	"key" : 36589,
	"title" : "HR 4132"
	},
{
	"Index" : "23965",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "37 Ursae Majoris, HIP 51814, SAO 27695, HD 91480, GC 14527, HR 4141, DM BD+57  1277, TYC 3819-1372-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "37 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "26.52",
	"RA_S" : 158.79039196,
	"DEC_S" : 57.08263526,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.189,
	"key" : 43965,
	"title" : "37 Ursae Majoris"
	},
{
	"Index" : "26765",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "38 Ursae Majoris, HIP 52353, SAO 15261, HD 92424, GC 14688, HR 4178, DM BD+66   678, TYC 4151-1450-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "38 Ursae Majoris",
	"OType" : "Variable Star",
	"Distance" : "69.51",
	"RA_S" : 160.4856156,
	"DEC_S" : 65.71628508,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.244,
	"key" : 46765,
	"title" : "38 Ursae Majoris"
	},
{
	"Index" : "28731",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 52425, SAO 15269, HD 92523, GC 14713, HR 4181, DM BD+69  586, TYC 4385-1959-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "HR 4181",
	"OType" : "Star",
	"Distance" : "127.9",
	"RA_S" : 160.76682215,
	"DEC_S" : 69.07621341,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.155,
	"key" : 48731,
	"title" : "HR 4181"
	},
{
	"Index" : "20500",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 52469, SAO 43444, HD 92787, GC 14737, HR 4191, DM BD+46 1657, TYC 3442-1254-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "HD  92787",
	"OType" : "High proper-motion Star",
	"Distance" : "37.09",
	"RA_S" : 160.8870395,
	"DEC_S" : 46.2038717,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.213,
	"key" : 40500,
	"title" : "HD  92787"
	},
{
	"Index" : "23997",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "44 Ursae Majoris, HIP 53261, SAO 27815, HD 94247, GC 14962, HR 4246, DM BD+55  1418, TYC 3823-1032-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "44 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "199.35",
	"RA_S" : 163.39355626,
	"DEC_S" : 54.58512957,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.264,
	"key" : 43997,
	"title" : "44 Ursae Majoris"
	},
{
	"Index" : "16655",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "45 Ursae Majoris, Omega Ursae Majoris, HIP 53295, SAO 43512, HD 94334, GC 14974, HR 4248, DM BD+43  2058, TYC 3011-2549-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Omega Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "75.4",
	"RA_S" : 163.4947529,
	"DEC_S" : 43.18995877,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.659,
	"key" : 36655,
	"title" : "Omega Ursae Majoris"
	},
{
	"Index" : "12383",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "46 Ursae Majoris, HIP 53426, SAO 62314, HD 94600, GC 15018, HR 4258, DM BD+34  2181, TYC 2519-2586-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "46 Ursae Majoris",
	"OType" : "High proper-motion Star",
	"Distance" : "72.59",
	"RA_S" : 163.93493426,
	"DEC_S" : 33.5069282,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.155,
	"key" : 32383,
	"title" : "46 Ursae Majoris"
	},
{
	"Index" : "16621",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "47 Ursae Majoris, HIP 53721, SAO 43557, HD 95128, GC 15087, HR 4277, DM BD+41  2147, TYC 3009-2703-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "47 Ursae Majoris",
	"OType" : "High proper-motion Star",
	"Distance" : "14.06",
	"RA_S" : 164.86655304,
	"DEC_S" : 40.43026,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.102,
	"key" : 36621,
	"title" : "47 Ursae Majoris"
	},
{
	"Index" : "16635",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "49 Ursae Majoris, HIP 53838, SAO 62354, HD 95310, GC 15128, HR 4288, DM BD+39  2400, TYC 3010-2498-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "49 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "115.36",
	"RA_S" : 165.21009721,
	"DEC_S" : 39.21208797,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.093,
	"key" : 36635,
	"title" : "49 Ursae Majoris"
	},
{
	"Index" : "26725",
	"Description" : "Alpha Ursae Majoris (Alpha UMa, \u03B1 Ursae Majoris, \u03B1 UMa) is the second-brightest star in the constellation of Ursa Major (despite its Bayer designation of \u0022alpha\u0022). It has the traditional name Dubhe, and a rarer name Ak.\r\rThis star forms part of the Big Dipper (also known as the Plough or the Great Bear), and is the northern of the \u0027pointers\u0027 (or \u0027guards\u0027), the two stars of Ursa Major which point towards Polaris, the North Star. Dubhe is about 123 light years away and is a giant star that has evolved away from the main sequence after consuming the hydrogen at its core. It is a spectroscopic binary with a main sequence companion \u03B1 UMa B that has a stellar classification of F0V. This star orbiting at a mean separation of about 23 astronomical units (AU) and completes an orbit every 44.4 years. More than 90,000 AU distant from this pair is a second binary system that includes an F-type star, making this a four star system.\r\rAlthough it is part of the constellation of Ursa Major, it does not form part of the Ursa Major Moving Group of stars that have a common motion through space..",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "50 Ursae Majoris, Alpha Ursae Majoris, HIP 54061B, SAO 15384, HD 95689B, GC 15185, HR 4301, DM BD+62  1161, TYC 4146-1274-2",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Dubhe",
	"OType" : "Star",
	"Distance" : "37.66",
	"RA_S" : 165.931663,
	"DEC_S" : 61.750872,
	"X" : 376,
	"Y" : 244,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.945,
	"key" : 46725,
	"shortTitle" : "Dubb; Ak; Dubkhe; Dube; Kaffa (see HD106591)",
	"title" : "Dubhe"
	},
{
	"Index" : "16677",
	"Description" : "Psi Ursae Majoris (Psi UMa, \u03C8 Ursae Majoris, \u03C8 UMa) is a star in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of +3.01, making it a third magnitude star and one of the brighter members of the constellation. Parallax measurements place it at a distance of 144.5 light-years (44.3 parsecs) from Earth. This is sufficiently close that the magnitude of the star is only reduced by 0.05 due to extinction. In Chinese astronomy, Psi Ursae Majoris is called Tien Tsan or Ta Tsun, \u0022Extremely Honorable\u0022. The name was possibly derived from the word \u592A\u5C0A, Pinyin: T\u00E0iz\u016Bn, meaning Royals, because this star is marking itself and stand alone in Royals asterism, Purple Forbidden enclosure (see Chinese constellation).\r\rThe spectrum of this star matches a stellar classification of K1 III, with the luminosity class of \u0027III\u0027 indicating this is an evolved giant star that has exhausted the supply of hydrogen at its core. As a consequence, it has expanded to around 20 times the radius of the Sun. It is radiating roughly 148 times the luminosity of the Sun from its enlarged outer envelope at an effective temperature of 4,520 K. At this heat, the star glows with the orange hue of a K-type star.\r\rPsi Ursae Majoris is a member of the thin disk population of the Milky Way. It is following an orbit through the galaxy with a low eccentricity of 0.02 that will carry it between 26.5\u201327.8 kly (8.1\u20138.5 kpc) from the Galactic Center. The low inclination of its orbit means the star will only stray 130 ly (40 pc) from the galactic plane.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "52 Ursae Majoris, Psi Ursae Majoris, HIP 54539, SAO 43629, HD 96833, GC 15340, HR 4335, DM BD+45  1897, TYC 3012-2519-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Psi Ursae Majoris",
	"OType" : "Star",
	"Distance" : "44.3",
	"RA_S" : 167.41586628,
	"DEC_S" : 44.49848342,
	"X" : 375,
	"Y" : 469,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.11,
	"key" : 36677,
	"title" : "Psi Ursae Majoris"
	},
{
	"Index" : "12393",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "53 Ursae Majoris, Xi Ursae Majoris, SAO 62484, HD 98231, HR 4375, DM BD+32  2132A, TYC 2520-2634-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alula Australis",
	"OType" : "Spectroscopic binary",
	"RA_S" : 169.54548201,
	"DEC_S" : 31.52919433,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.327,
	"key" : 32393,
	"title" : "Alula Australis"
	},
{
	"Index" : "12394",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "53 Ursae Majoris, Xi Ursae Majoris, SAO 62484, HD 98230, GC 15537, HR 4374, DM BD+32  2132B, TYC 2520-2634-2",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alula Australe",
	"OType" : "Spectroscopic binary",
	"RA_S" : 169.54548201,
	"DEC_S" : 31.52919433,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.804,
	"key" : 32394,
	"title" : "Alula Australe"
	},
{
	"Index" : "71562",
	"Description" : "Xi Ursae Majoris (Xi UMa, \u03BE Ursae Majoris, \u03BE UMa) is a star system in the constellation Ursa Major. On May 2, 1780, Sir William Herschel discovered that this was a binary star system, making it the first such system ever discovered. It was the first visual double star for which an orbit was calculated, when it was computed by F\u00E9lix Savary in 1828.\r\rThe two components are yellow G-type main-sequence stars. The brighter component, Xi Ursae Majoris A, has a mean apparent magnitude of +4.41. It is classified as an RS Canum Venaticorum type variable star and its brightness varies by 0.01 magnitudes. The companion star, Xi Ursae Majoris B has an apparent magnitude of +4.87. The orbital period of the two stars is 59.84 years, and they are currently separated by 1.2 arcseconds, or at least 10 AUs.\r\rEach component of this double star is itself a spectroscopic binary. B\u0027s binary companion, denoted Xi Ursae Majoris Bb, is unresolved, but the binary star is known to have an orbital period of 3.98 days. The masses of both A and B\u0027s companions (Ab and Bb) (deduced by the sum total mass of the system minus the likely masses of Aa and Ba determined by their class) indicate that they are probably MV stars (red dwarfs), Bb being on the cool end of the M spectrum, not much hotter than a brown dwarf.\r\rIt also has the proper name Alula Australis (and erroneously Alula Australe).",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "53 Ursae Majoris, Xi Ursae Majoris, HIP 55203, SAO 62484, HD 98230J, GC 15537, HR 4374, DM BD+32 2132",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alula Australis",
	"OType" : "Variable of RS CVn type",
	"Distance" : "10.4167",
	"RA_S" : 169.54555,
	"DEC_S" : 31.529289,
	"X" : 356,
	"Y" : 638,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.79,
	"key" : 91562,
	"title" : "Alula Australis"
	},
{
	"Index" : "12391",
	"Description" : "Nu Ursae Majoris (Nu UMa, \u03BD Ursae Majoris, \u03BD UMa) is a double star in the northern circumpolar constellation of Ursa Major. The traditional name of this star is Alula Borealis. At an apparent visual magnitude of +3.490, it is bright enough to be seen with the naked eye. Based upon parallax measurements, the distance to \u03BD Ursae Majoris is about 399 light-years (122 parsecs).\r\rThis is a giant star with a stellar classification of K3 III. It has expanded to about 57 times the radius of the Sun and is radiating 775 times the Sun\u0027s luminosity. The effective temperature of the outer envelope is 4,070 K; cool enough to give it an orange hue typical of a K-type star. It has a 10th-magnitude optical companion at an angular separation of 7.1 arcseconds.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "54 Ursae Majoris, Nu Ursae Majoris, HIP 55219, SAO 62486, HD 98262, GC 15547, HR 4377, DM BD+33  2098, TYC 2520-2631-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alula Borealis",
	"OType" : "Star",
	"Distance" : "122.34",
	"RA_S" : 169.61973721,
	"DEC_S" : 33.09430465,
	"X" : 355,
	"Y" : 617,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.635,
	"key" : 32391,
	"shortTitle" : "Alula Boreale",
	"title" : "Alula Borealis"
	},
{
	"Index" : "16638",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "55 Ursae Majoris, HIP 55266, SAO 62491, HD 98353, GC 15558, HR 4380, DM BD+38  2225, TYC 3010-2501-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "55 Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "58.8",
	"RA_S" : 169.7829152,
	"DEC_S" : 38.18556347,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.773,
	"key" : 36638,
	"title" : "55 Ursae Majoris"
	},
{
	"Index" : "16734",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "56 Ursae Majoris, HIP 55560, SAO 43719, HD 98839, GC 15625, HR 4392, DM BD+44  2083, TYC 3015-2321-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "56 Ursae Majoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "163.02",
	"RA_S" : 170.70660284,
	"DEC_S" : 43.48270463,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.092,
	"key" : 36734,
	"title" : "56 Ursae Majoris"
	},
{
	"Index" : "16701",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "57 Ursae Majoris, HIP 56034A, SAO 62572, HD 99787A, GC 15751, HR 4422, DM BD+40  2433, TYC 3013-2482-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "57 Ursae Majoris",
	"OType" : "High proper-motion Star",
	"Distance" : "65.13",
	"RA_S" : 172.26717357,
	"DEC_S" : 39.33697101,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.353,
	"key" : 36701,
	"title" : "57 Ursae Majoris"
	},
{
	"Index" : "12463",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "61 Ursae Majoris, HIP 56997, SAO 62655, HD 101501, GC 16035, HR 4496, DM BD+35  2270, TYC 2525-2445-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "61 Ursae Majoris",
	"OType" : "Variable Star",
	"Distance" : "9.61",
	"RA_S" : 175.26256758,
	"DEC_S" : 34.20163504,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.39,
	"key" : 32463,
	"title" : "61 Ursae Majoris"
	},
{
	"Index" : "20581",
	"Description" : "Chi Ursae Majoris (Chi UMa, \u03C7 Ursae Majoris, \u03C7 UMa) is a star in the constellation Ursa Major. It has the traditional names Alkafzah, Alkaphrah, and El Koprah.\r\rChi Ursae Majoris is an orange K-type giant with an apparent magnitude of +3.69. It is approximately 196 light years from Earth. This star has 20.8 \u00B1 0.8 times the radius of the Sun.\r\rIn Chinese astronomy, Alkafzah is called Tae Yang Show, \u0022the Sun Governor\u0022. The name was possibly derived from the word \u592A\u967D\u5B88, Pinyin: T\u00E0iy\u00E1ngsh\u01D2u, meaning Guard of the Sun, because this star is marking itself and stand alone in Guard of the Sun asterism, Purple Forbidden enclosure (see : Chinese constellation).\r\rThe Spiral Galaxy in Ursa Major, NGC 3877 (= H I.201), type Sc, is best found from Chi Ursae Majoris, which is almost exactly 15 arc minutes north of the galaxy.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "63 Ursae Majoris, Chi Ursae Majoris, HIP 57399, SAO 43886, HD 102224, GC 16137, HR 4518, DM BD+48  1966, TYC 3452-2140-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alkafzah / Alkaphrah / El Koprah",
	"OType" : "Variable Star",
	"Distance" : "56.3",
	"RA_S" : 176.51255662,
	"DEC_S" : 47.77940553,
	"X" : 293,
	"Y" : 424,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.818,
	"key" : 40581,
	"shortTitle" : "El Koprah",
	"title" : "Alkafzah / Alkaphrah / El Koprah"
	},
{
	"Index" : "24105",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 57477, SAO 28142, HD 102328, GC 16153, HR 4521, DM BD+56 1544, TYC 3835-1057-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "HR 4521",
	"OType" : "Star",
	"Distance" : "66.06",
	"RA_S" : 176.73176118,
	"DEC_S" : 55.62819024,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.398,
	"key" : 44105,
	"title" : "HR 4521"
	},
{
	"Index" : "16793",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "67 Ursae Majoris, HIP 58684, SAO 44002, HD 104513, GC 16445, HR 4594, DM BD+43  2179, TYC 3019-2030-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "67 Ursae Majoris",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "34.24",
	"RA_S" : 180.5283411,
	"DEC_S" : 43.04564026,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.241,
	"key" : 36793,
	"title" : "67 Ursae Majoris"
	},
{
	"Index" : "24120",
	"Description" : "Delta Ursae Majoris (Delta UMa, \u03B4 Ursae Majoris, \u03B4 UMa) is the Bayer designation for a star in the northern circumpolar constellation of Ursa Major. It has the traditional names Megrez /\u02C8m\u025B\u0261r\u025Bz/, and Kaffa. Megrez has an apparent magnitude of +3.3, making it the dimmest of the seven stars in the Big Dipper asterism. Parallax measurements yield a distance estimate of 58.4 light-years (17.9 parsecs) from Earth.\r\rMegrez has 63% more mass of the Sun and is about 1.4 times the Sun\u0027s radius. It has a stellar classification of A3 V, which means it is an A-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. It shines at 14 times the luminosity of the Sun, with this energy being emitted from its outer envelope at an effective temperature of 9,480 K. This gives it the white hue typical of an A-type star.\r\rThis star has an excess emission of infrared radiation, indicating the presence of circumstellar matter. This forms a debris disk around an orbital radius of 16 Astronomical Units from the star. This radius is unusually small for the estimated age of the disk, which may be explained by drag from the Poynting\u2013Robertson effect causing the dust to spiral inward.\r\rIt has two faint companions, an 11th magnitude star at an angular separation of 190 arcseconds, and a 10th magnitude star 186 arcseconds away.\r\rMegrez is a marginally outlying member of the Ursa Major moving group, an association of stars that share a common motion through space and likely formed in the same molecular cloud. The space velocity components of Delta Ursae Majoris in the galactic coordinate system are [U, V, W] = [+15.35, +1.17, \u201311.52] km s\u20131.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "69 Ursae Majoris, Delta Ursae Majoris, HIP 59774, SAO 28315, HD 106591, GC 16736, HR 4660, DM BD+57  1363, TYC 3837-1070-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Megrez",
	"OType" : "Variable Star",
	"Distance" : "24.68",
	"RA_S" : 183.85650264,
	"DEC_S" : 57.03261544,
	"X" : 253,
	"Y" : 297,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.298,
	"key" : 44120,
	"shortTitle" : "Kaffa; Megrets",
	"title" : "Megrez"
	},
{
	"Index" : "24191",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "74 Ursae Majoris, HIP 60978, SAO 28405, HD 108844, GC 17038, HR 4760, DM BD+59  1444, TYC 3847-1128-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "74 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "83.39",
	"RA_S" : 187.48887565,
	"DEC_S" : 58.40574408,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.374,
	"key" : 44191,
	"title" : "74 Ursae Majoris"
	},
{
	"Index" : "24177",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "78 Ursae Majoris, HIP 63503A, SAO 28601, HD 113139A, GC 17664, HR 4931, DM BD+57  1408, TYC 3845-1189-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "78 Ursae Majoris",
	"OType" : "Star",
	"Distance" : "25.44",
	"RA_S" : 195.181625,
	"DEC_S" : 56.366333,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.023,
	"key" : 44177,
	"title" : "78 Ursae Majoris"
	},
{
	"Index" : "24220",
	"Description" : "The Mizar\u2013Alcor stellar sextuple system consists of the quadruple system Mizar and the binary system Alcor. Mizar (Zeta Ursae Majoris, Zeta UMa, \u03B6 Ursae Majoris, \u03B6 UMa) in Arabic known as \u0022\u0633\u0647\u0627 \u0627\u0644\u062D\u064A\u0648\u0627\u0646\u0629\u0022 is a quadruple system of two binary stars in the constellation Ursa Major and is the second star from the end of the Big Dipper\u0027s handle. Its apparent magnitude is 2.23 and its spectral class is A1V. Mizar\u0027s name comes from the Arabic \u0645\u0626\u0632\u0631 m\u012Bzar, meaning a waistband or girdle.\r\rWith normal eyesight one can make out a faint companion just to the east, named Alcor or 80 Ursae Majoris. Alcor is of magnitude 3.99 and spectral class A5V.\r\rMizar and Alcor together are sometimes called the \u0022Horse and Rider,\u0022 and the ability to resolve the two stars with the naked eye is often quoted as a test of eyesight, although even people with quite poor eyesight can see the two stars. Arabic literature says that only those with the sharpest eyesight can see the companion of Mizar. Astronomer Sir Patrick Moore has suggested that this in fact refers to another star which lies visually between Mizar and Alcor. The name the Arabs used for Alcor was \u0633\u0647\u0627 (suha), meaning either the \u0027forgotten\u0027 or \u0027neglected\u0027 one.\r\rAs of 2007, the best estimates of Mizar and Alcor\u0027s respective distances place them 1.1 light-years and 4 minutes of arc apart, and though their proper motions show they move together (they are both members of the Ursa Major Moving Group), it was long believed that they did not form a true binary star system, but simply a double star. However, in 2009, it was independently reported by two groups of astronomers (Eric Mamajek et al., and Zimmerman et al.) that Alcor actually is itself a binary, consisting of Alcor A and Alcor B, and that this binary system is most likely gravitationally bound to Mizar, bringing the full count of stars in this complex system to six. These studies also demonstrated that the Alcor binary and Mizar quadruple are somewhat closer together than previously thought: approximately 74,000 \u00B1 39,000 astronomical units or 0.5\u20131.5 light years.\r\rThe whole six-star system lies about 83 light-years away from Earth, as measured by the Hipparcos astrometry satellite. The components are all members of the Ursa Major moving group, a mostly dispersed group of stars sharing a common birth, as determined by proper motion. The other stars of the Big Dipper, except Dubhe and Alkaid, belong to this group as well.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "79 Ursae Majoris, Zeta Ursae Majoris, HIP 65378C, SAO 28738, HD 116657, GC 18134, HR 5055, DM BD+55  1598B, TYC 3850-1386-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Mizar",
	"OType" : "Spectroscopic binary",
	"Distance" : "23.96",
	"RA_S" : 200.984708,
	"DEC_S" : 54.921822,
	"X" : 126,
	"Y" : 284,
	"Constellation" : "Ursa Major ",
	"AMag" : 3.878,
	"key" : 44220,
	"title" : "Mizar"
	},
{
	"Index" : "24218",
	"Description" : "The Mizar\u2013Alcor stellar sextuple system consists of the quadruple system Mizar and the binary system Alcor. Mizar (Zeta Ursae Majoris, Zeta UMa, \u03B6 Ursae Majoris, \u03B6 UMa) in Arabic known as \u0022\u0633\u0647\u0627 \u0627\u0644\u062D\u064A\u0648\u0627\u0646\u0629\u0022 is a quadruple system of two binary stars in the constellation Ursa Major and is the second star from the end of the Big Dipper\u0027s handle. Its apparent magnitude is 2.23 and its spectral class is A1V. Mizar\u0027s name comes from the Arabic \u0645\u0626\u0632\u0631 m\u012Bzar, meaning a waistband or girdle.\r\rWith normal eyesight one can make out a faint companion just to the east, named Alcor or 80 Ursae Majoris. Alcor is of magnitude 3.99 and spectral class A5V.\r\rMizar and Alcor together are sometimes called the \u0022Horse and Rider,\u0022 and the ability to resolve the two stars with the naked eye is often quoted as a test of eyesight, although even people with quite poor eyesight can see the two stars. Arabic literature says that only those with the sharpest eyesight can see the companion of Mizar. Astronomer Sir Patrick Moore has suggested that this in fact refers to another star which lies visually between Mizar and Alcor. The name the Arabs used for Alcor was \u0633\u0647\u0627 (suha), meaning either the \u0027forgotten\u0027 or \u0027neglected\u0027 one.\r\rAs of 2007, the best estimates of Mizar and Alcor\u0027s respective distances place them 1.1 light-years and 4 minutes of arc apart, and though their proper motions show they move together (they are both members of the Ursa Major Moving Group), it was long believed that they did not form a true binary star system, but simply a double star. However, in 2009, it was independently reported by two groups of astronomers (Eric Mamajek et al., and Zimmerman et al.) that Alcor actually is itself a binary, consisting of Alcor A and Alcor B, and that this binary system is most likely gravitationally bound to Mizar, bringing the full count of stars in this complex system to six. These studies also demonstrated that the Alcor binary and Mizar quadruple are somewhat closer together than previously thought: approximately 74,000 \u00B1 39,000 astronomical units or 0.5\u20131.5 light years.\r\rThe whole six-star system lies about 83 light-years away from Earth, as measured by the Hipparcos astrometry satellite. The components are all members of the Ursa Major moving group, a mostly dispersed group of stars sharing a common birth, as determined by proper motion. The other stars of the Big Dipper, except Dubhe and Alkaid, belong to this group as well.",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "80 Ursae Majoris, g Ursae Majoris, HIP 65477, SAO 28751, HD 116842, GC 18155, HR 5062, DM BD+55  1603, TYC 3850-1384-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "Alcor",
	"OType" : "Double or multiple star",
	"Distance" : "25.06",
	"RA_S" : 201.3064015,
	"DEC_S" : 54.98795585,
	"X" : 124,
	"Y" : 280,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.007,
	"key" : 44218,
	"shortTitle" : "Saidak; Al'cor",
	"title" : "Alcor"
	},
{
	"Index" : "24268",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "HIP 65728, SAO 16080, HD 117376, GC 18226, HR 5085, DM BD+60 1461, TYC 3856-621-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "HR 5085",
	"OType" : "High proper-motion Star",
	"Distance" : "71.36",
	"RA_S" : 202.11286402,
	"DEC_S" : 59.94578626,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.458,
	"key" : 44268,
	"title" : "HR 5085"
	},
{
	"Index" : "24229",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "82 Ursae Majoris, HIP 66634, SAO 28832, HD 119024, GC 18473, HR 5142, DM BD+53  1640, TYC 3851-126-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "82 Ursae Majoris",
	"OType" : "High proper-motion Star",
	"Distance" : "53.58",
	"RA_S" : 204.87687428,
	"DEC_S" : 52.92120313,
	"Constellation" : "Ursa Major ",
	"AMag" : 5.472,
	"key" : 44229,
	"title" : "82 Ursae Majoris"
	},
{
	"Index" : "24232",
	"MapNum" : "40",
	"ImageNum" : "40",
	"Desig" : "83 Ursae Majoris, HIP 66738, SAO 28843, HD 119228, GC 18504, HR 5154, DM BD+55  1625, TYC 3851-1506-1",
	"group" : { "key" : "Ursa Major" },
	"Common" : "83 Ursae Majoris",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "160.27",
	"RA_S" : 205.18446983,
	"DEC_S" : 54.68163243,
	"Constellation" : "Ursa Major ",
	"AMag" : 4.828,
	"key" : 44232,
	"title" : "83 Ursae Majoris"
	},
{
	"Index" : "30166",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "4 Ursae Minoris, HIP 69112, SAO 7958, HD 124547, GC 19142, HR 5321, DM BD+78   478, TYC 4561-2317-1",
	"group" : { "backgroundImage" : "images/Alignment/24.png",
		"description" : "Ursa Minor (Latin: \u0022Smaller Bear\u0022, contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor is notable as the location of the north celestial pole, although this will change after some centuries due to the precession of the equinoxes.\r\rUrsa Minor is commonly visualized as a baby bear with an unusually long tail.\r\rUrsa Minor and Ursa Major were related by the Greeks to the myth of Callisto and Arcas. However, in a variant of the story, in which it is Bootes that represents Arcas, Ursa Minor represents a dog. This is the older tradition, which sensibly explains both the length of the tail and the obsolete alternate name of Cynosura (the dog\u0027s tail) for Polaris, the North Star.\r\rPreviously, Ursa Minor was considered just seven close stars, mythologically regarded as sisters. In early Greek mythology, the seven stars of the Little Dipper were the Hesperides, daughters of Atlas. Together with the nearby constellations of Bootes, Ursa Major, and Draco, it may have formed the origin of the myth of the apples of the Hesperides, which forms part of the Labours of Hercules.[original research?] Ursa Minor with its modern associations was invented by Thales of Miletus in approximately 600 BCE, from what had previously represented the wings of Draco, the Dragon. He did so out of a desire to commemorate the location of the North Celestial Pole, then near Beta and Gamma Ursae Minoris.\r\rIn Hungarian mythology the constellation is called \u0027Little Goncol cart\u0027 (Goncol szek\u00E9r) after a legendary shaman. (Ursa Major is \u0027Big Goncol cart.\u0027) The shaman\u0027s knowledge knew no limit. He invented the cart: His nation was wandering, so the cart was the biggest gift of the Gods to the country. Legends claim he knew everything about the world. Nobody saw his death; his body simply disappeared among the stars.\r\rBecause Ursa Minor consists of seven stars, the Latin word for \u0022North\u0022 (i.e. where Polaris points) is septentrio, from septem (seven) and triones (oxen), from seven oxen driving a plow, which the seven stars also resemble.",
		"key" : "Ursa Minor",
		"grouptype" : "Ursa Minor",
		"Meaning" : "lesser bear",
		"Family" : "Ursa Major",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Ursa Minor",
		"title" : "Ursa Minor Objects Group" },
	"Common" : "4 Ursae Minoris",
	"OType" : "Spectroscopic binary",
	"Distance" : "139.48",
	"RA_S" : 212.21219993,
	"DEC_S" : 77.54751495,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.963,
	"key" : 50166,
	"title" : "4 Ursae Minoris"
	},
{
	"Index" : "28887",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 69373, SAO 16305, HD 124730, GC 19189, HR 5334, DM BD+70  778, TYC 4403-2218-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "HR 5334",
	"OType" : "Variable Star",
	"Distance" : "131.14",
	"RA_S" : 213.01671094,
	"DEC_S" : 69.43254398,
	"Constellation" : "Ursa Minor ",
	"AMag" : 5.366,
	"key" : 48887,
	"title" : "HR 5334"
	},
{
	"Index" : "30136",
	"Description" : "5 Ursae Minoris (5 UMi) is a star in the constellation Ursa Minor. Its apparent magnitude is 4.25.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "5 Ursae Minoris, HIP 70692, SAO 8024, HD 127700, GC 19548, HR 5430, DM BD+76   527, TYC 4559-3017-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "5 Ursae Minoris",
	"OType" : "Variable Star",
	"Distance" : "109.98",
	"RA_S" : 216.88142333,
	"DEC_S" : 75.69599492,
	"X" : 461,
	"Y" : 267,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.401,
	"key" : 50136,
	"title" : "5 Ursae Minoris"
	},
{
	"Index" : "27059",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "RR Ursae Minoris, HIP 73199, SAO 16558, HD 132813, GC 20170, HR 5589, DM BD+66   878, TYC 4186-1373-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "RR Ursae Minoris",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "140.39",
	"RA_S" : 224.39585498,
	"DEC_S" : 65.93246407,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.865,
	"key" : 47059,
	"title" : "RR Ursae Minoris"
	},
{
	"Index" : "27068",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "HIP 74605, SAO 16660, HD 136064, GC 20532, HR 5691, DM BD+67  876, TYC 4187-1365-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Gliese 580.2 (HR 5691)",
	"OType" : "High proper-motion Star",
	"Distance" : "25.34",
	"RA_S" : 228.65974157,
	"DEC_S" : 67.34672278,
	"Constellation" : "Ursa Minor ",
	"AMag" : 5.21,
	"key" : 47068,
	"title" : "Gliese 580.2 (HR 5691)"
	},
{
	"Index" : "28985",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "11 Ursae Minoris, HIP 74793, SAO 8207, HD 136726, GC 20598, HR 5714, DM BD+72   678, TYC 4414-2315-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Pherkad Minor (see HD131873)",
	"OType" : "Star",
	"Distance" : "122.02",
	"RA_S" : 229.2745561,
	"DEC_S" : 71.82389796,
	"Constellation" : "Ursa Minor ",
	"AMag" : 5.173,
	"key" : 48985,
	"title" : "Pherkad Minor (see HD131873)"
	},
{
	"Index" : "28984",
	"Description" : "Gamma Ursae Minoris (\u03B3 UMi, \u03B3 Ursae Minoris; also 13 UMi) is a star in the northern circumpolar constellation of Ursa Minor. It has the traditional name Pherkad, which derives from the Arabic \u0641\u0631\u0642\u062F farqad \u0022calf\u0022, short for a\u1E2Bfa al farkadayn \u0022the dim one of the two calves\u0022, Pherkad and Kochab. (The full name Ahfa al Farkadain is now applied to Zeta Ursae Minoris.) Gamma Ursae Minoris is sometimes called Pherkad Major to distinguish it from 11 Ursae Minoris Pherkad Minor. Together with Beta Ursae Minoris, or Kochab, Gamma forms the end of the dipper pan of the \u0022Little Dipper\u0022, which is a colloquial name for the constellation. Pherkad and Kochab are sometimes called the \u0022Guardians of the Pole\u0022, as they appear to circle around the north star Polaris as the Earth rotates.\r\rIn Chinese, \u5317\u6975 (B\u011Bi J\u00ED), meaning North Pole, refers to an asterism consisting of \u03B3 Ursae Minoris, \u03B2 Ursae Minoris, 5 Ursae Minoris, 4 Ursae Minoris and \u03A3 1694. Consequently, \u03B3 Ursae Minoris itself is known as \u5317\u6975\u4E00 (B\u011Bi J\u00ED y\u012B, English: the First Star of North Pole.), representing \u592A\u5B50 (T\u00E0iz\u01D0), meaning Crown Prince\r\rGamma Ursae Minoris has apparent magnitude +3.05 and can be readily observed with the naked eye even in a city-lit night sky. Based upon parallax measurements, it is approximately 487 light-years (149 parsecs) from Earth, giving it an absolute magnitude of \u20132.84. Measurement of the star\u0027s spectrum resulted in a stellar classification of A3 Iab, with the luminosity class of \u0027Iab\u0027 indicating this is an intermediate luminosity supergiant star. The effective temperature of the star\u0027s outer envelope is 8,280 K, giving it the typical white hue of an A-type star. It is rotating rapidly, with the projected rotational velocity of 180 km s\u20131 providing a lower limit on the azimuthal velocity along the star\u0027s equator.\r\rThis is classified as a shell star that has a circumstellar disk of gas around the star\u0027s equator, which may be causing it to vary in magnitude. It is 1100 times more luminous than the Sun, and possesses a radius 15 times that of the Sun.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "13 Ursae Minoris, Gamma Ursae Minoris, HIP 75097, SAO 8220, HD 137422, GC 20692, HR 5735, DM BD+72   679, TYC 4414-2314-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Pherkad",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "149.21",
	"RA_S" : 230.18215017,
	"DEC_S" : 71.83401655,
	"X" : 433,
	"Y" : 331,
	"Constellation" : "Ursa Minor ",
	"AMag" : 3.011,
	"key" : 48984,
	"shortTitle" : "Pherkad Major (see HD131873); Ferkad",
	"title" : "Pherkad"
	},
{
	"Index" : "30155",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "15 Ursae Minoris, Theta Ursae Minoris, HIP 76008, SAO 8274, HD 139669, GC 20952, HR 5826, DM BD+77   592, TYC 4560-3065-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Theta Ursae Minoris",
	"OType" : "Variable Star",
	"Distance" : "259.53",
	"RA_S" : 232.85385883,
	"DEC_S" : 77.34936187,
	"Constellation" : "Ursa Minor ",
	"AMag" : 5.169,
	"key" : 50155,
	"title" : "Theta Ursae Minoris"
	},
{
	"Index" : "30181",
	"Description" : "Zeta Ursae Minoris (\u03B6 UMi, \u03B6 Ursae Minoris) is a star in the constellation Ursa Minor. It has the traditional name Akhfa al Farkadain, from the Arabic \u0623\u062E\u0641\u0649 \u0627\u0644\u0641\u0631\u0642\u062F\u064A\u0646 a\u1E2Bfa al-farqadayn \u0022the dimmer of the two calves\u0022, as opposed to Anwar al Farkadain (\u03B7 UMi) \u0022the brighter of the two calves\u0022. These names were originally applied to Pherkad and Kochab, respectively, the other two stars in the rectangle of Ursa Minor.\r\rZeta Ursae Minoris is a white stellar class A-type main sequence star with an apparent magnitude of +4.32. It is approximately 380 light years from Earth.\r\rDespite its classification as a main sequence dwarf star, Zeta UMi is 3.4 times the mass of the sun and its luminosity is about 200 solar luminosities. At a surface temperature of 8,700 kelvins, this star is actually on the verge of becoming a giant star. Zeta UMi may also be a variable of the Delta Scuti type.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "16 Ursae Minoris, Zeta Ursae Minoris, HIP 77055, SAO 8328, HD 142105, GC 21243, HR 5903, DM BD+78   527, TYC 4563-2708-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Akhfa al Farkadain",
	"OType" : "Variable Star",
	"Distance" : "113.1",
	"RA_S" : 236.01466214,
	"DEC_S" : 77.79449412,
	"X" : 398,
	"Y" : 259,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.279,
	"key" : 50181,
	"title" : "Akhfa al Farkadain"
	},
{
	"Index" : "30205",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "19 Ursae Minoris, HIP 79280, SAO 8446, HD 146926, GC 21851, HR 6079, DM BD+76   594, TYC 4567-1411-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "19 Ursae Minoris",
	"OType" : "Star",
	"Distance" : "189.13",
	"RA_S" : 242.70634963,
	"DEC_S" : 75.87756111,
	"Constellation" : "Ursa Minor ",
	"AMag" : 5.457,
	"key" : 50205,
	"title" : "19 Ursae Minoris"
	},
{
	"Index" : "30209",
	"Description" : "Eta Ursae Minoris (\u03B7 UMi, \u03B7 Ursae Minoris) is a star in the constellation Ursa Minor. It has the traditional names Anwar al Farkadain and Alasco. The first is from the Arabic \u0623\u0646\u0648\u0631 \u0627\u0644\u0641\u0631\u0642\u062F\u064A\u0646 \u0027anwar al-farqadayn \u0022the brighter of the two calves\u0022, as opposed to Ahfa al Farkadain (\u03B6 UMi) \u0022the dimmer of the two calves\u0022; these names were originally applied to Kochab, and Pherkad, respectively, the other two stars in the rectangle of Ursa Minor.\r\rEta Ursae Minoris is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.95, making it visible to the naked eye. It is approximately 97.3 light years from Earth.\r\rThis star has 1.41 times the mass of the Sun, with a projected rotational velocity of 76.0 km s\u22121.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "21 Ursae Minoris, Eta Ursae Minoris, HIP 79822, SAO 8470, HD 148048, GC 21999, HR 6116, DM BD+76   596, TYC 4567-1764-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Eta Ursae Minoris",
	"OType" : "High proper-motion Star",
	"Distance" : "29.73",
	"RA_S" : 244.37620882,
	"DEC_S" : 75.75532538,
	"X" : 375,
	"Y" : 288,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.991,
	"key" : 50209,
	"title" : "Eta Ursae Minoris"
	},
{
	"Index" : "30298",
	"Description" : "Epsilon Ursae Minoris (\u03B5 UMi, \u03B5 Ursae Minoris) is a triple star system in the constellation Ursa Minor. It is approximately 347 light years from Earth.\r\rThe primary component, Epsilon Ursae Minoris A, is an eclipsing spectroscopic binary. It is classified as a yellow G-type giant with a mean apparent magnitude of +4.21. In addition to light changes due to eclipses, the system is also classified as an RS Canum Venaticorum type variable star and its brightness varies from magnitude +4.19 to +4.23 with a period of 39.48 days, which is also the orbital period of the binary. The binary is orbited by a third component, Epsilon Ursae Minoris B, which is an 11th magnitude star, 77 arcseconds away in the sky.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "22 Ursae Minoris, Epsilon Ursae Minoris, HIP 82080, SAO 2770, HD 153751, GC 22749, HR 6322, DM BD+82   498, TYC 4580-1154-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Epsilon Ursae Minoris",
	"OType" : "Variable of RS CVn type",
	"Distance" : "93.05",
	"RA_S" : 251.49270461,
	"DEC_S" : 82.03725358,
	"X" : 361,
	"Y" : 205,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.312,
	"key" : 50298,
	"title" : "Epsilon Ursae Minoris"
	},
{
	"Index" : "30882",
	"Description" : "Delta Ursae Minoris (\u03B4 UMi, \u03B4 Ursae Minoris; also 23 UMi) is a star in the constellation Ursa Minor. It has the traditional name Yildun (also spelled Vildiur, Jildun, Gildun, and Yilduz), from the Turkish y\u0131ld\u0131z \u0022star\u0022. It may also have been called Pherkard, an alternate spelling of Pherkad, used for \u03B3 UMi and 11 UMi.\r\rDelta Ursae Minoris is a white A-type main sequence dwarf with an apparent magnitude of +4.35. It is approximately 183 light years from Earth.",
	"MapNum" : "24",
	"ImageNum" : "24",
	"Desig" : "23 Ursae Minoris, Delta Ursae Minoris, HIP 85822, SAO 2937, HD 166205, GC 24236, HR 6789, DM BD+86   269, TYC 4655-1053-1",
	"group" : { "key" : "Ursa Minor" },
	"Common" : "Yildun",
	"OType" : "Double or multiple star",
	"Distance" : "52.77",
	"RA_S" : 263.05411524,
	"DEC_S" : 86.58646256,
	"X" : 359,
	"Y" : 145,
	"Constellation" : "Ursa Minor ",
	"AMag" : 4.34,
	"key" : 50882,
	"shortTitle" : "Vildiur; Gildun; Pherkard; Jildun",
	"title" : "Yildun"
	},
{
	"Index" : "58314",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 39690, SAO 219422, HD 67582, GC 11026, HR 3187, DM CD-44 4051, TYC 8136-1795-1",
	"group" : { "backgroundImage" : "images/Alignment/02.png",
		"description" : "Vela is a constellation in the southern sky. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis.\r\rArgo was sub-divided in 1752 by the French astronomer Nicolas Louis de Lacaille, forming Vela. Despite the division, Lacaille kept Argo\u0027s Bayer designations. Therefore Carina has the \u03B1, \u03B2 and \u03B5, Vela has \u03B3 and \u03B4, Puppis has \u03B6, and so on.",
		"key" : "Vela",
		"grouptype" : "Vela",
		"Meaning" : "sails",
		"Family" : "Heavenly Waters",
		"Origin" : "1763, Lacaille, split from Argo Navis",
		"shortTitle" : "Vela",
		"title" : "Vela Objects Group" },
	"Common" : "HR 3187",
	"OType" : "Variable Star",
	"Distance" : "424.75",
	"RA_S" : 121.66808141,
	"DEC_S" : -45.26601489,
	"Constellation" : "Vela ",
	"AMag" : 5.196,
	"key" : 78314,
	"title" : "HR 3187"
	},
{
	"Index" : "58397",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Gamma01 Velorum, SAO 219501, HD 68243, GC 11103, HR 3206, DM CD-46  3846, TYC 8140-6534-1",
	"group" : { "key" : "Vela" },
	"Common" : "Gamma01 Velorum",
	"OType" : "Spectroscopic binary",
	"RA_S" : 122.37218,
	"DEC_S" : -47.34527805,
	"Constellation" : "Vela ",
	"AMag" : 4.143,
	"key" : 78397,
	"title" : "Gamma01 Velorum"
	},
{
	"Index" : "54361",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 39961, SAO 219502, HD 68217, GC 11104, HR 3204, DM CD-43 3998, TYC 7671-5701-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3204",
	"OType" : "Star",
	"Distance" : "380.72",
	"RA_S" : 122.39964246,
	"DEC_S" : -44.12277167,
	"Constellation" : "Vela ",
	"AMag" : 5.154,
	"key" : 74361,
	"title" : "HR 3204"
	},
{
	"Index" : "58399",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 39970, SAO 219515, HD 68324, GC 11117, HR 3213, DM CD-47 3653, TYC 8140-6536-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* IS Vel",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "385.24",
	"RA_S" : 122.42981614,
	"DEC_S" : -47.93719166,
	"Constellation" : "Vela ",
	"AMag" : 5.183,
	"key" : 78399,
	"title" : "V* IS Vel"
	},
{
	"Index" : "58394",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 40285, SAO 219629, HD 69144, GC 11207, HR 3244, DM CD-46 3929, TYC 8140-6531-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* NO Vel",
	"OType" : "Eclipsing binary of beta Lyr type (semi-detached)",
	"Distance" : "423.77",
	"RA_S" : 123.40065644,
	"DEC_S" : -46.99163168,
	"Constellation" : "Vela ",
	"AMag" : 5.104,
	"key" : 78394,
	"title" : "V* NO Vel"
	},
{
	"Index" : "58594",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "B Velorum, HIP 41039AB, SAO 219848, HD 70930, GC 11450, HR 3294, DM CD-48  3734, TYC 8153-4761-1",
	"group" : { "key" : "Vela" },
	"Common" : "B Velorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "508.99",
	"RA_S" : 125.63209789,
	"DEC_S" : -48.49041887,
	"Constellation" : "Vela ",
	"AMag" : 4.846,
	"key" : 78594,
	"title" : "B Velorum"
	},
{
	"Index" : "58705",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 41296, SAO 235959, HD 71510, GC 11531, HR 3330, DM CD-51 3004, TYC 8161-1767-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3330",
	"OType" : "Be Star",
	"Distance" : "212.66",
	"RA_S" : 126.38052331,
	"DEC_S" : -51.72741816,
	"Constellation" : "Vela ",
	"AMag" : 5.141,
	"key" : 78705,
	"title" : "HR 3330"
	},
{
	"Index" : "62388",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "F Velorum, HIP 41483, SAO 236002, HD 71935, GC 11595, HR 3350, DM CP-52  1484, TYC 8568-3119-1",
	"group" : { "key" : "Vela" },
	"Common" : "F Velorum",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "61.04",
	"RA_S" : 126.90243199,
	"DEC_S" : -53.08848315,
	"Constellation" : "Vela ",
	"AMag" : 5.105,
	"key" : 82388,
	"title" : "F Velorum"
	},
{
	"Index" : "54395",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 41639A, SAO 219996, HD 72127A, GC 11635, HR 3359, DM CD-44 4462, TYC 7673-2998-1",
	"group" : { "key" : "Vela" },
	"Common" : "TYC 7673-2998-1",
	"OType" : "Star",
	"Distance" : "800",
	"RA_S" : 127.36451935,
	"DEC_S" : -44.72482057,
	"Constellation" : "Vela ",
	"AMag" : 5.159,
	"key" : 74395,
	"title" : "TYC 7673-2998-1"
	},
{
	"Index" : "58682",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "C Velorum, HIP 42088, SAO 220138, HD 73155, GC 11783, HR 3407, DM CD-49  3646, TYC 8158-2683-1",
	"group" : { "key" : "Vela" },
	"Common" : "C Velorum",
	"OType" : "Star",
	"Distance" : "259.65",
	"RA_S" : 128.68164872,
	"DEC_S" : -49.94420094,
	"Constellation" : "Vela ",
	"AMag" : 5.133,
	"key" : 78682,
	"title" : "C Velorum"
	},
{
	"Index" : "54347",
	"Description" : "HD 73634 is a star in the constellation Vela. Its apparent magnitude is 4.14.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "e Velorum, HIP 42312, SAO 220204, HD 73634, GC 11852, HR 3426, DM CD-42  4451, TYC 7670-866-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 73634",
	"OType" : "Star",
	"Distance" : "553.99",
	"RA_S" : 129.410967,
	"DEC_S" : -42.98908214,
	"X" : 473,
	"Y" : 368,
	"Constellation" : "Vela ",
	"AMag" : 4.136,
	"key" : 74347,
	"title" : "HD 73634"
	},
{
	"Index" : "62392",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42459, SAO 236151, HD 74071, GC 11917, HR 3440, DM CP-53 1796, TYC 8568-3122-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* HW Vel",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "163.4",
	"RA_S" : 129.84933603,
	"DEC_S" : -53.43976777,
	"Constellation" : "Vela ",
	"AMag" : 5.415,
	"key" : 82392,
	"title" : "V* HW Vel"
	},
{
	"Index" : "62386",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42504, SAO 236157, HD 74146, GC 11933, HR 3442, DM CP-52 1579, TYC 8568-3117-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD  74146",
	"OType" : "Spectroscopic binary",
	"Distance" : "163.33",
	"RA_S" : 129.98998976,
	"DEC_S" : -53.05472894,
	"Constellation" : "Vela ",
	"AMag" : 5.143,
	"key" : 82386,
	"title" : "HD  74146"
	},
{
	"Index" : "62413",
	"Description" : "Omicron Velorum (\u03BF Vel, \u03BF Velorum) is a star in the constellation Vela.\r\rOmicron Velorum is a blue-white B-type subgiant with a mean apparent magnitude of +3.60. It is approximately 495 light years from Earth. It is a variable star and its brightness varies from magnitude +3.55 to +3.67 with a period of 2.78 days.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Omicron Velorum, HIP 42536, SAO 236164, HD 74195, GC 11943, HR 3447, DM CP-52  1583, TYC 8569-4018-1",
	"group" : { "key" : "Vela" },
	"Common" : "Omicron Velorum",
	"OType" : "Pulsating variable Star",
	"Distance" : "164.5",
	"RA_S" : 130.07327092,
	"DEC_S" : -52.92191154,
	"X" : 444,
	"Y" : 494,
	"Constellation" : "Vela ",
	"AMag" : 3.545,
	"key" : 82413,
	"title" : "Omicron Velorum"
	},
{
	"Index" : "54475",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42540A, SAO 220252, HD 74067, GC 11931, HR 3439, DM CD-39 4653, TYC 7679-2117-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* NY Vel",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "85.43",
	"RA_S" : 130.0798728,
	"DEC_S" : -40.2638801,
	"Constellation" : "Vela ",
	"AMag" : 5.206,
	"key" : 74475,
	"title" : "V* NY Vel"
	},
{
	"Index" : "58556",
	"Description" : "HD 74180 is a binary star in the constellation Vela. It is approximately 3100 light years from Earth.\r\rThe primary component is a yellow-white F-type supergiant with a mean apparent magnitude of +3.77. It is classified as an irregular variable star and its brightness varies from magnitude +3.77 to +3.91. It has a 10th magnitude companion, 37.5 arcseconds distant.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "b Velorum, HIP 42570, SAO 220265, HD 74180, GC 11951, HR 3445, DM CD-46  4438, TYC 8151-5000-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 74180",
	"OType" : "Variable Star",
	"RA_S" : 130.15654223,
	"DEC_S" : -46.6487452,
	"X" : 458,
	"Y" : 413,
	"Constellation" : "Vela ",
	"AMag" : 3.88,
	"key" : 78556,
	"title" : "HD 74180"
	},
{
	"Index" : "58638",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "n Velorum, HIP 42624, SAO 220284, HD 74272, GC 11966, HR 3452, DM CD-46  4448, TYC 8155-3647-1",
	"group" : { "key" : "Vela" },
	"Common" : "n Velorum",
	"OType" : "Star",
	"Distance" : "763.14",
	"RA_S" : 130.30472176,
	"DEC_S" : -47.31712261,
	"Constellation" : "Vela ",
	"AMag" : 4.779,
	"key" : 78638,
	"title" : "n Velorum"
	},
{
	"Index" : "58536",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42679, SAO 220300, HD 74371, GC 11978, HR 3456, DM CD-44 4704, TYC 8151-179-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* LN Vel",
	"OType" : "Pulsating variable Star",
	"RA_S" : 130.48712087,
	"DEC_S" : -45.41071353,
	"Constellation" : "Vela ",
	"AMag" : 5.248,
	"key" : 78536,
	"title" : "V* LN Vel"
	},
{
	"Index" : "58627",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42712AB, SAO 220313, HD 74455, GC 11988, HR 3462, DM CD-47 4251, TYC 8155-2250-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* HX Vel",
	"OType" : "Ellipsoidal variable Star",
	"RA_S" : 130.56747262,
	"DEC_S" : -48.09909192,
	"Constellation" : "Vela ",
	"AMag" : 5.438,
	"key" : 78627,
	"title" : "V* HX Vel"
	},
{
	"Index" : "62410",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42715BC, SAO 236202, HD 74535, GC 11992, HR 3466, DM CP-52 1605, TYC 8569-3934-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* KT Vel",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "164.66",
	"RA_S" : 130.579143,
	"DEC_S" : -53.10006997,
	"Constellation" : "Vela ",
	"AMag" : 5.453,
	"key" : 82410,
	"title" : "V* KT Vel"
	},
{
	"Index" : "62411",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 42726, SAO 236205, HD 74560, GC 11997, HR 3467, DM CP-52 1607, TYC 8569-3954-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* HY Vel",
	"OType" : "Spectroscopic binary",
	"Distance" : "164.32",
	"RA_S" : 130.60577674,
	"DEC_S" : -53.11398217,
	"Constellation" : "Vela ",
	"AMag" : 4.789,
	"key" : 82411,
	"title" : "V* HY Vel"
	},
{
	"Index" : "58692",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "D Velorum, HIP 42834, SAO 220361, HD 74753, GC 12031, HR 3476, DM CD-49  3761, TYC 8159-2763-1",
	"group" : { "key" : "Vela" },
	"Common" : "D Velorum",
	"OType" : "Variable Star",
	"Distance" : "559.51",
	"RA_S" : 130.91779676,
	"DEC_S" : -49.82280209,
	"Constellation" : "Vela ",
	"AMag" : 5.101,
	"key" : 78692,
	"title" : "D Velorum"
	},
{
	"Index" : "54523",
	"Description" : "HD 74772 is a star in the constellation Vela. Itsapparent magnitude is 4.06.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "d Velorum, HIP 42884, SAO 220371, HD 74772, GC 12050, HR 3477, DM CD-42  4569, TYC 7683-2233-1",
	"group" : { "key" : "Vela" },
	"Common" : "Gliese 321.1",
	"OType" : "Star",
	"Distance" : "70.12",
	"RA_S" : 131.09977719,
	"DEC_S" : -42.64927754,
	"X" : 458,
	"Y" : 360,
	"Constellation" : "Vela ",
	"AMag" : 4.143,
	"key" : 74523,
	"title" : "Gliese 321.1"
	},
{
	"Index" : "62472",
	"Description" : "Delta Velorum (\u03B4 Vel, \u03B4 Velorum) is a star system in the southern constellation Vela, near the border with Carina. From parallax measurements, it is approximately 80.6 light-years (24.7 parsecs) from Earth. This star is sometimes given the name Koo She, Chinese for \u0027Bow and Arrows\u0027, along with \u03C9 Velorum and stars in Canis Major.\r\rDelta Velorum is a triple star system. The outward components A and B have a wide orbit with a 142 year orbital period. The primary component A has an apparent magnitude of 1.97, while the secondary component B is magnitude 5.55. In 1978 the primary component was reported to be a spectroscopic binary in the Proceeding of the Australian Astronomical observatory, and this was confirmed by the Hipparcos satellite. Observations of variability in the \u03B4 Velorum system were made independently by ground-based astronomers and the Galileo spaceprobe at Jupiter.\r\rIn 2000 it was announced that the components Aa and Ab form an eclipsing binary, having an orbital period of 45.15 days and an eccentricity of 0.230. Delta Velorum is the brightest known eclipsing binary, although Algol has a deeper minimum and is easier to observe visually. Only the primary component \u03B4 Velorum A is sufficiently bright to explain such variation.\r\rBoth members of the spectroscopic binary \u03B4 Vel A are evolved stars that have left the main sequence. Component Aa has 2.5 times the mass of the Sun, 2.6 times the Sun\u0027s radius, and is radiating 56 times the luminosity of the Sun at an effective temperature of 9,470. Component Ab is only slightly smaller, with 2.4 times the Sun\u0027s mass and radius, with a luminosity of 47 times the Sun and an effective temperature of 9,370 K. The two stars are spinning rapidly and are about 400 million years old.\r\rBecause of precession, \u03B4 Velorum will be the south polar star around 9000 AD.\r\rA second binary system is located at an angular separation of 69 arcseconds. It is composed of an 11th magnitude and 13th magnitude pair, which are 6 arcseconds apart.\r\rThe Chinese name Koo She \u5F27\u77E2 (Mandarin h\u00FAsh\u01D0) \u0022Bow and Arrow\u0022, originally assigned for some[which?] stars among Canis Major, Puppis, and Vela, was introduced by Robson for this star.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Delta Velorum, HIP 42913B, SAO 236232, HD 74956B, GC 12069, HR 3485, DM CP-54  1788, TYC 8573-3571-2",
	"group" : { "key" : "Vela" },
	"Common" : "Koo She",
	"OType" : "Star",
	"Distance" : "24.45",
	"RA_S" : 131.175846,
	"DEC_S" : -54.7085,
	"X" : 432,
	"Y" : 515,
	"Constellation" : "Vela ",
	"AMag" : 5.57,
	"key" : 82472,
	"title" : "Koo She"
	},
{
	"Index" : "58560",
	"Description" : "HD 75063 (a Vel, a Velorum) is a star in the constellation Vela.\r\rHD 75063 is a white A-type giant with an apparent magnitude of +3.87. It is approximately 1500 light years from Earth.\r\rThis star, a Velorum, should not be confused with A Velorum\u2014note capitalization.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "a Velorum, HIP 43023, SAO 220422, HD 75063, GC 12109, HR 3487, DM CD-45  4517, TYC 8151-6254-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 75063",
	"OType" : "Star",
	"Distance" : "563.9",
	"RA_S" : 131.50684886,
	"DEC_S" : -46.04153102,
	"X" : 447,
	"Y" : 403,
	"Constellation" : "Vela ",
	"AMag" : 3.877,
	"key" : 78560,
	"title" : "HD 75063"
	},
{
	"Index" : "58548",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 43082, SAO 220442, HD 75149, GC 12125, HR 3494, DM CD-45 4526, TYC 8151-3667-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* OP Vel",
	"OType" : "Pulsating variable Star",
	"RA_S" : 131.6272731,
	"DEC_S" : -45.9125064,
	"Constellation" : "Vela ",
	"AMag" : 5.487,
	"key" : 78548,
	"title" : "V* OP Vel"
	},
{
	"Index" : "54469",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "h Velorum, HIP 43325, SAO 220531, HD 75630, GC 12193, HR 3514, DM CD-39  4838, TYC 7679-1755-1",
	"group" : { "key" : "Vela" },
	"Common" : "h Velorum",
	"OType" : "Star",
	"Distance" : "384.54",
	"RA_S" : 132.41316493,
	"DEC_S" : -40.32015732,
	"Constellation" : "Vela ",
	"AMag" : 5.474,
	"key" : 74469,
	"title" : "h Velorum"
	},
{
	"Index" : "58568",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "g Velorum, HIP 43347, SAO 220540, HD 75710, GC 12204, HR 3520, DM CD-44  4861, TYC 8152-2275-1",
	"group" : { "key" : "Vela" },
	"Common" : "g Velorum",
	"OType" : "Star",
	"Distance" : "338.44",
	"RA_S" : 132.44848991,
	"DEC_S" : -45.30787599,
	"Constellation" : "Vela ",
	"AMag" : 4.94,
	"key" : 78568,
	"title" : "g Velorum"
	},
{
	"Index" : "58564",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "f Velorum, HIP 43413, SAO 220561, HD 75821, GC 12227, HR 3527, DM CD-46  4661, TYC 8152-1394-1",
	"group" : { "key" : "Vela" },
	"Common" : "f Velorum",
	"OType" : "Eclipsing binary",
	"RA_S" : 132.63942123,
	"DEC_S" : -46.52918926,
	"Constellation" : "Vela ",
	"AMag" : 5.07,
	"key" : 78564,
	"title" : "f Velorum"
	},
{
	"Index" : "58656",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 43671, SAO 220636, HD 76360, GC 12314, HR 3551, DM CD-47 4480, TYC 8156-3114-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD  76360",
	"OType" : "Star",
	"Distance" : "77.14",
	"RA_S" : 133.46080728,
	"DEC_S" : -47.52076482,
	"Constellation" : "Vela ",
	"AMag" : 5.336,
	"key" : 78656,
	"title" : "HD  76360"
	},
{
	"Index" : "62558",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "H Velorum, HIP 43878A, SAO 236417, HD 76805, GC 12381, HR 3574, DM CP-52  1788, TYC 8582-4212-1",
	"group" : { "key" : "Vela" },
	"Common" : "H Velorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "108.16",
	"RA_S" : 134.08026375,
	"DEC_S" : -52.72348443,
	"Constellation" : "Vela ",
	"AMag" : 4.702,
	"key" : 82558,
	"title" : "H Velorum"
	},
{
	"Index" : "58655",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 44093, SAO 220717, HD 77140, GC 12431, HR 3588, DM CD-46 4810, TYC 8156-3113-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* FZ Vel",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "68.9",
	"RA_S" : 134.71814492,
	"DEC_S" : -47.23469014,
	"Constellation" : "Vela ",
	"AMag" : 5.178,
	"key" : 78655,
	"title" : "V* FZ Vel"
	},
{
	"Index" : "54547",
	"Description" : "HD 77258 is a star in the constellation Vela. Its apparent magnitude is 4.47.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "w Velorum, HIP 44191, SAO 220730, HD 77258, GC 12451, HR 3591, DM CD-40  4810, TYC 7685-2720-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 77258",
	"OType" : "Spectroscopic binary",
	"Distance" : "64.51",
	"RA_S" : 135.02253235,
	"DEC_S" : -41.25360954,
	"X" : 422,
	"Y" : 337,
	"Constellation" : "Vela ",
	"AMag" : 4.519,
	"key" : 74547,
	"title" : "HD 77258"
	},
{
	"Index" : "58896",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 44337AB, SAO 236518, HD 77653, GC 12501, HR 3605, DM CD-51 3430, TYC 8177-1874-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* OY Vel",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "112.69",
	"RA_S" : 135.43568592,
	"DEC_S" : -52.18871539,
	"Constellation" : "Vela ",
	"AMag" : 5.275,
	"key" : 78896,
	"title" : "V* OY Vel"
	},
{
	"Index" : "58795",
	"Description" : "HD 78004 (c Vel, c Velorum) is a star in the constellation Vela.\r\rHD 78004 is an orange K-type giant with an apparent magnitude of +3.75. It is approximately 309 light years from Earth.\r\rThe star should not be confused with C Velorum.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "c Velorum, HIP 44511, SAO 220803, HD 78004, GC 12545, HR 3614, DM CD-46  4883, TYC 8169-1192-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 78004",
	"OType" : "Star",
	"Distance" : "91.82",
	"RA_S" : 136.03867203,
	"DEC_S" : -47.09773947,
	"X" : 405,
	"Y" : 412,
	"Constellation" : "Vela ",
	"AMag" : 3.867,
	"key" : 78795,
	"title" : "HD 78004"
	},
{
	"Index" : "54621",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 45085, SAO 220928, HD 79186, GC 12688, HR 3654, DM CD-44 5206, TYC 7690-536-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* GX Vel",
	"OType" : "Pulsating variable Star",
	"RA_S" : 137.7683277,
	"DEC_S" : -44.86790328,
	"Constellation" : "Vela ",
	"AMag" : 5.035,
	"key" : 74621,
	"title" : "V* GX Vel"
	},
{
	"Index" : "62644",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 45328, SAO 236749, HD 79846, GC 12767, HR 3679, DM CP-55 2035, TYC 8587-2116-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3679",
	"OType" : "Variable Star",
	"Distance" : "195.72",
	"RA_S" : 138.57495788,
	"DEC_S" : -55.56962546,
	"Constellation" : "Vela ",
	"AMag" : 5.362,
	"key" : 82644,
	"title" : "HR 3679"
	},
{
	"Index" : "54613",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "z Velorum, HIP 45344, SAO 220978, HD 79735, GC 12759, HR 3674, DM CD-42  5086, TYC 7690-2858-1",
	"group" : { "key" : "Vela" },
	"Common" : "z Velorum",
	"OType" : "Star",
	"Distance" : "181.78",
	"RA_S" : 138.60202491,
	"DEC_S" : -43.22749899,
	"Constellation" : "Vela ",
	"AMag" : 5.218,
	"key" : 74613,
	"title" : "z Velorum"
	},
{
	"Index" : "54460",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "l Velorum, HIP 45439, SAO 200159, HD 79917, GC 12784, HR 3682, DM CD-38  5408, TYC 7678-4341-1",
	"group" : { "key" : "Vela" },
	"Common" : "l Velorum",
	"OType" : "Star",
	"Distance" : "68.85",
	"RA_S" : 138.9029532,
	"DEC_S" : -38.56994143,
	"Constellation" : "Vela ",
	"AMag" : 5.036,
	"key" : 74460,
	"title" : "l Velorum"
	},
{
	"Index" : "50135",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "k Velorum, HIP 45448, SAO 200163, HD 79940, GC 12787, HR 3684, DM CD-36  5505, TYC 7164-4049-1",
	"group" : { "key" : "Vela" },
	"Common" : "Markeb (see HD61555)",
	"OType" : "Star",
	"Distance" : "50.46",
	"RA_S" : 138.93783556,
	"DEC_S" : -37.41314858,
	"Constellation" : "Vela ",
	"AMag" : 4.668,
	"key" : 70135,
	"title" : "Markeb (see HD61555)"
	},
{
	"Index" : "54618",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 45505, SAO 221014, HD 80108, GC 12808, HR 3692, DM CD-43 5103, TYC 7690-2863-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3692",
	"OType" : "Variable Star",
	"RA_S" : 139.09598092,
	"DEC_S" : -44.26573453,
	"Constellation" : "Vela ",
	"AMag" : 5.302,
	"key" : 74618,
	"title" : "HR 3692"
	},
{
	"Index" : "54511",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 45544, SAO 200185, HD 80170, GC 12821, HR 3694, DM CD-38 5430, TYC 7682-3456-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3694",
	"OType" : "Star",
	"Distance" : "105.72",
	"RA_S" : 139.23781423,
	"DEC_S" : -39.40154088,
	"Constellation" : "Vela ",
	"AMag" : 5.434,
	"key" : 74511,
	"title" : "HR 3694"
	},
{
	"Index" : "58905",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "K Velorum, HIP 45631, SAO 236824, HD 80456, GC 12844, HR 3703, DM CD-50  4001, TYC 8178-3063-1",
	"group" : { "key" : "Vela" },
	"Common" : "K Velorum",
	"OType" : "Star",
	"Distance" : "134.13",
	"RA_S" : 139.52446059,
	"DEC_S" : -51.05085934,
	"Constellation" : "Vela ",
	"AMag" : 5.243,
	"key" : 78905,
	"title" : "K Velorum"
	},
{
	"Index" : "62599",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "I Velorum, HIP 46283, SAO 236972, HD 81848, GC 13035, HR 3753, DM CP-52  2360, TYC 8584-5050-1",
	"group" : { "key" : "Vela" },
	"Common" : "I Velorum",
	"OType" : "Star",
	"Distance" : "131.49",
	"RA_S" : 141.57482944,
	"DEC_S" : -53.37890578,
	"Constellation" : "Vela ",
	"AMag" : 5.071,
	"key" : 82599,
	"title" : "I Velorum"
	},
{
	"Index" : "58918",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 46594, SAO 237042, HD 82419, GC 13129, HR 3784, DM CD-50 4204, TYC 8179-3633-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 3784",
	"OType" : "Star",
	"Distance" : "132.51",
	"RA_S" : 142.52128967,
	"DEC_S" : -51.51716652,
	"Constellation" : "Vela ",
	"AMag" : 5.425,
	"key" : 78918,
	"title" : "HR 3784"
	},
{
	"Index" : "54678",
	"Description" : "Psi Velorum (\u03C8 Vel, \u03C8 Velorum) is a binary star in the constellation Vela. It is approximately 60.5 light years from Earth, making it the nearest star of the constellation.\r\rThe primary component, Psi Velorum A, is a yellow-white F-type subgiant with an apparent magnitude of +4.1. The companion, Psi Velorum B, is a yellow-white F-type main sequence dwarf, with an apparent magnitude of +4.6. The two stars are 0.68 arcseconds, or at least 12 astronomical units, apart and complete one orbit every 33.99 years.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Psi Velorum, HIP 46651AB, SAO 221234, HD 82434A, GC 13140, HR 3786, DM CD-39  5580, TYC 7696-2620-1",
	"group" : { "key" : "Vela" },
	"Common" : "Tseen Ke",
	"OType" : "Star",
	"Distance" : "18.81",
	"RA_S" : 142.67486821,
	"DEC_S" : -40.46674196,
	"X" : 348,
	"Y" : 323,
	"Constellation" : "Vela ",
	"AMag" : 3.66,
	"key" : 74678,
	"title" : "Tseen Ke"
	},
{
	"Index" : "62729",
	"Description" : "HR 3803 or N Velorum (N Vel) is a 3rd-magnitude star on the border between the southern constellations Carina and Vela. Based upon parallax measurements, it is approximately 239 light-years (73 parsecs) from Earth. It is an orange-hued K-type giant star and has twice the mass of the Sun. The measured angular diameter of this star, after correction for limb darkening, is 7.13 \u00B1 0.08 mas. At the estimated distance of Eta Draconis, this yields a physical size of about 29 times the radius of the Sun.\r\rIn 1752, French astronomer Nicolas Louis de Lacaille divided the former constellation Argo Navis into three separate constellations, and then referenced its stars by extending Bayer\u0027s system of star nomenclature; this star was given the designation N Velorum. In 1871 Benjamin Apthorp Gould discovered this star to be variable, but this occurred prior to the standardization of variable star nomenclature by German astronomer Friedrich Wilhelm Argelander during the nineteenth century, so it does not fall into the standard range of variable star designations.\r\rThe star should not be confused with n Velorum.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "N Velorum, HIP 46701, SAO 237067, HD 82668, GC 13160, HR 3803, DM CP-56  2270, TYC 8592-2561-1",
	"group" : { "key" : "Vela" },
	"Common" : "N Velorum",
	"OType" : "Variable Star",
	"Distance" : "73.26",
	"RA_S" : 142.80549361,
	"DEC_S" : -57.03437817,
	"X" : 344,
	"Y" : 538,
	"Constellation" : "Vela ",
	"AMag" : 3.326,
	"key" : 82729,
	"title" : "N Velorum"
	},
{
	"Index" : "54679",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 46811A, SAO 221262, HD 82694, GC 13180, HR 3807, DM CD-40 5284, TYC 7696-2621-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR  3807",
	"OType" : "Star",
	"Distance" : "129.47",
	"RA_S" : 143.08035552,
	"DEC_S" : -40.64933164,
	"Constellation" : "Vela ",
	"AMag" : 5.496,
	"key" : 74679,
	"title" : "HR  3807"
	},
{
	"Index" : "58925",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "L Velorum, HIP 46950, SAO 237107, HD 83058, GC 13234, HR 3819, DM CD-50  4270, TYC 8180-2997-1",
	"group" : { "key" : "Vela" },
	"Common" : "L Velorum",
	"OType" : "Star",
	"Distance" : "276.18",
	"RA_S" : 143.53663967,
	"DEC_S" : -51.25526601,
	"Constellation" : "Vela ",
	"AMag" : 4.966,
	"key" : 78925,
	"title" : "L Velorum"
	},
{
	"Index" : "58886",
	"Description" : "HD 83446 is a star in the constellation Vela. Its apparent magnitude is 4.35.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "M Velorum, HIP 47175, SAO 221344, HD 83446, GC 13293, HR 3836, DM CD-48  4836, TYC 8176-2817-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 83446",
	"OType" : "Star",
	"Distance" : "32.32",
	"RA_S" : 144.20641263,
	"DEC_S" : -49.35503644,
	"X" : 333,
	"Y" : 438,
	"Constellation" : "Vela ",
	"AMag" : 4.358,
	"key" : 78886,
	"title" : "HD 83446"
	},
{
	"Index" : "58942",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "u Velorum, HIP 48224, SAO 221523, HD 85355, GC 13547, HR 3898, DM CD-45  5470, TYC 8181-3013-1",
	"group" : { "key" : "Vela" },
	"Common" : "u Velorum",
	"OType" : "Star",
	"Distance" : "257.01",
	"RA_S" : 147.48807687,
	"DEC_S" : -45.73273585,
	"Constellation" : "Vela ",
	"AMag" : 5.068,
	"key" : 78942,
	"title" : "u Velorum"
	},
{
	"Index" : "58944",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "m Velorum, HIP 48374, SAO 221553, HD 85622, GC 13587, HR 3912, DM CD-45  5508, TYC 8181-868-1",
	"group" : { "key" : "Vela" },
	"Common" : "m Velorum",
	"OType" : "Spectroscopic binary",
	"Distance" : "322.01",
	"RA_S" : 147.91944504,
	"DEC_S" : -46.54761854,
	"Constellation" : "Vela ",
	"AMag" : 4.702,
	"key" : 78944,
	"title" : "m Velorum"
	},
{
	"Index" : "62864",
	"Description" : "Phi Velorum (\u03C6 Vel, \u03C6 Velorum) is a star in the constellation Vela. It has the traditional name Tseen Ke, from Chinese \u5929\u7D00 (Mandarin ti\u0101nj\u00EC) \u0022star chart\u0022. (lit. \u0022Record of Heaven\u0022).\r\rPhi Velorum is a blue-white B-type supergiant with an apparent magnitude of +3.52. It is approximately 1590 light years from Earth.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Phi Velorum, HIP 48774, SAO 237522, HD 86440, GC 13711, HR 3940, DM CP-53  3075, TYC 8602-2024-1",
	"group" : { "key" : "Vela" },
	"Common" : "Phi Velorum",
	"OType" : "Star",
	"Distance" : "486.13",
	"RA_S" : 149.21558969,
	"DEC_S" : -54.56779331,
	"X" : 296,
	"Y" : 507,
	"Constellation" : "Vela ",
	"AMag" : 3.5,
	"key" : 82864,
	"title" : "Phi Velorum"
	},
{
	"Index" : "58994",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 49485A, SAO 221773, HD 87783, GC 13890, HR 3976, DM CD-46 5806, TYC 8186-2960-1",
	"group" : { "key" : "Vela" },
	"Common" : "CCDM J10062-4722AB",
	"OType" : "Double or multiple star",
	"Distance" : "73.61",
	"RA_S" : 151.54675042,
	"DEC_S" : -47.36996955,
	"Constellation" : "Vela ",
	"AMag" : 5.321,
	"key" : 78994,
	"title" : "CCDM J10062-4722AB"
	},
{
	"Index" : "59101",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Q Velorum, HIP 49712, SAO 237736, HD 88206, GC 13953, HR 3990, DM CD-51  4507, TYC 8195-4554-1",
	"group" : { "key" : "Vela" },
	"Common" : "Q Velorum",
	"OType" : "Star",
	"Distance" : "405.24",
	"RA_S" : 152.23432891,
	"DEC_S" : -51.81126308,
	"Constellation" : "Vela ",
	"AMag" : 4.824,
	"key" : 79101,
	"title" : "Q Velorum"
	},
{
	"Index" : "59099",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 50070, SAO 237804, HD 88824, GC 14047, HR 4017, DM CD-50 4924, TYC 8195-4552-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* LW Vel",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "51.89",
	"RA_S" : 153.34518204,
	"DEC_S" : -51.23297322,
	"Constellation" : "Vela ",
	"AMag" : 5.297,
	"key" : 79099,
	"title" : "V* LW Vel"
	},
{
	"Index" : "54851",
	"Description" : "HD 88955 is a star in the constellation Vela. This is a white A-type main sequence star with an apparent magnitude of +3.85. It is approximately 103 light years from Earth. This star has 1.8 times the Sun\u0027s radius and 2.2 times the mass of the Sun. It is radiating 22 times the Sun\u0027s luminosity from its outer atmosphere at an effective temperature of 9,460 K.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "q Velorum, HIP 50191, SAO 221895, HD 88955, GC 14076, HR 4023, DM CD-41  5713, TYC 7716-3704-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 88955",
	"OType" : "Star",
	"Distance" : "31.07",
	"RA_S" : 153.68397941,
	"DEC_S" : -42.12193872,
	"X" : 241,
	"Y" : 349,
	"Constellation" : "Vela ",
	"AMag" : 3.836,
	"key" : 74851,
	"title" : "HD 88955"
	},
{
	"Index" : "62896",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 50555, SAO 237916, HD 89682, GC 14185, HR 4063, DM CP-54 3474, TYC 8604-2441-1",
	"group" : { "key" : "Vela" },
	"Common" : "V* GZ Vel",
	"OType" : "Long-period variable star",
	"Distance" : "562.6",
	"RA_S" : 154.90312793,
	"DEC_S" : -55.02930088,
	"Constellation" : "Vela ",
	"AMag" : 4.739,
	"key" : 82896,
	"title" : "V* GZ Vel"
	},
{
	"Index" : "62907",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "J Velorum, HIP 50676A, SAO 237959, HD 89890, GC 14220, HR 4074, DM CP-55  3286, TYC 8604-975-1",
	"group" : { "key" : "Vela" },
	"Common" : "J Velorum",
	"OType" : "Double or multiple star",
	"Distance" : "348.05",
	"RA_S" : 155.2283049,
	"DEC_S" : -56.04321873,
	"Constellation" : "Vela ",
	"AMag" : 4.49,
	"key" : 82907,
	"title" : "J Velorum"
	},
{
	"Index" : "54864",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "r Velorum, HIP 50799, SAO 221998, HD 89998, GC 14248, HR 4080, DM CD-41  5809, TYC 7717-3167-1",
	"group" : { "key" : "Vela" },
	"Common" : "r Velorum",
	"OType" : "Variable Star",
	"Distance" : "62.48",
	"RA_S" : 155.58160198,
	"DEC_S" : -41.64996002,
	"Constellation" : "Vela ",
	"AMag" : 4.938,
	"key" : 74864,
	"title" : "r Velorum"
	},
{
	"Index" : "62851",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Y Velorum, HIP 51523, SAO 238146, HD 91324, GC 14464, HR 4134, DM CP-53  3909, TYC 8601-4516-1",
	"group" : { "key" : "Vela" },
	"Common" : "Y Velorum",
	"OType" : "High proper-motion Star",
	"Distance" : "21.81",
	"RA_S" : 157.84092252,
	"DEC_S" : -53.7154822,
	"Constellation" : "Vela ",
	"AMag" : 4.946,
	"key" : 82851,
	"title" : "Y Velorum"
	},
{
	"Index" : "59157",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "t Velorum, HIP 51635AC, SAO 222136, HD 91504, GC 14505, HR 4143, DM CD-46  6205, TYC 8201-3334-1",
	"group" : { "key" : "Vela" },
	"Common" : "t Velorum",
	"OType" : "Star",
	"Distance" : "383.77",
	"RA_S" : 158.2369322,
	"DEC_S" : -47.00335326,
	"Constellation" : "Vela ",
	"AMag" : 5.148,
	"key" : 79157,
	"title" : "t Velorum"
	},
{
	"Index" : "59159",
	"Description" : "HD 92139 is a triple star system in the constellation Vela. It is approximately 86.5 light years from Earth.\r\rThe primary component is a yellow-white F-type subgiant with an apparent magnitude of +4.5. It is a spectroscopic binary whose components have an orbital period of 10.21 days. The companion star is a white A-type main sequence dwarf with an apparent magnitude of +5.1. It is located 0.3 arcseconds from the primary and has an orbital period of 16.3 years. The system has a combined apparent magnitude of +3.84.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "p Velorum, HIP 51986AB, SAO 222199, HD 92139, GC 14614, HR 4167, DM CD-47  6042A, TYC 8201-3337-1",
	"group" : { "key" : "Vela" },
	"Common" : "HD 92139",
	"OType" : "Spectroscopic binary",
	"Distance" : "26.84",
	"RA_S" : 159.32558311,
	"DEC_S" : -48.22562079,
	"X" : 203,
	"Y" : 437,
	"Constellation" : "Vela ",
	"AMag" : 3.872,
	"key" : 79159,
	"title" : "HD 92139"
	},
{
	"Index" : "62910",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "x Velorum, HIP 52154, SAO 238309, HD 92449, GC 14662, HR 4180, DM CP-54  3915, TYC 8605-1196-1",
	"group" : { "key" : "Vela" },
	"Common" : "x Velorum",
	"OType" : "Star",
	"Distance" : "257.21",
	"RA_S" : 159.82663889,
	"DEC_S" : -55.60326723,
	"Constellation" : "Vela ",
	"AMag" : 4.379,
	"key" : 82910,
	"title" : "x Velorum"
	},
{
	"Index" : "59208",
	"Description" : "Mu Velorum (\u03BC Vel, \u03BC Velorum) is a binary star system in the southern constellation Vela. The two stars orbit each other with a semi-major axis of 1.437 arcseconds and a period of 116.24 years. (Wulff-Dieter Heintz (1986) lists a period of 138 years with his orbital elements.) The pair have a combined apparent visual magnitude of 2.69, making the system readily visible to the naked eye. From parallax measurements, the distance to this system is estimated to be 117 light-years (36 parsecs). The system is about 360 million years old.\r\rThe primary component is a giant star with an apparent magnitude of 2.7 and a stellar classification of G5 III. It is radiating about 107 times the luminosity of the Sun from an expanded atmosphere about 13 times the Sun\u0027s radius. The mass of this star is 3.3 times that of the Sun. In 1998, the Extreme Ultraviolet Explorer space telescope detected a strong flare that released an X-ray emission nearly equal to the output of the entire star. The quiescent X-ray luminosity of Mu Velorum A is about 1.7 \u00D7 1030 erg s\u20131.\r\rThe fainter companion, Mu Velorum B, is a main sequence star with an apparent magnitude of 6.4 and an assigned stellar classification of G2V. However, this classification is suspect. Closer examination of the spectrum suggests the star may actually have a classification of F4V or F5V, which suggests a mass of about 1.5 times the mass of the Sun. Such stars typically do not show a marked level of magnetic activity.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Mu Velorum, HIP 52727A, SAO 222321, HD 93497, GC 14842, HR 4216, DM CD-48  5913, TYC 8206-3033-1",
	"group" : { "key" : "Vela" },
	"Common" : "Mu Velorum",
	"OType" : "Star",
	"Distance" : "35.91",
	"RA_S" : 161.69248947,
	"DEC_S" : -49.42023604,
	"X" : 187,
	"Y" : 456,
	"Constellation" : "Vela ",
	"AMag" : 2.815,
	"key" : 79208,
	"title" : "Mu Velorum"
	},
{
	"Index" : "59209",
	"Description" : "Mu Velorum (\u03BC Vel, \u03BC Velorum) is a binary star system in the southern constellation Vela. The two stars orbit each other with a semi-major axis of 1.437 arcseconds and a period of 116.24 years. (Wulff-Dieter Heintz (1986) lists a period of 138 years with his orbital elements.) The pair have a combined apparent visual magnitude of 2.69, making the system readily visible to the naked eye. From parallax measurements, the distance to this system is estimated to be 117 light-years (36 parsecs). The system is about 360 million years old.\r\rThe primary component is a giant star with an apparent magnitude of 2.7 and a stellar classification of G5 III. It is radiating about 107 times the luminosity of the Sun from an expanded atmosphere about 13 times the Sun\u0027s radius. The mass of this star is 3.3 times that of the Sun. In 1998, the Extreme Ultraviolet Explorer space telescope detected a strong flare that released an X-ray emission nearly equal to the output of the entire star. The quiescent X-ray luminosity of Mu Velorum A is about 1.7 \u00D7 1030 erg s\u20131.\r\rThe fainter companion, Mu Velorum B, is a main sequence star with an apparent magnitude of 6.4 and an assigned stellar classification of G2V. However, this classification is suspect. Closer examination of the spectrum suggests the star may actually have a classification of F4V or F5V, which suggests a mass of about 1.5 times the mass of the Sun. Such stars typically do not show a marked level of magnetic activity.",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "Mu Velorum, HIP 52727B, TYC 8206-3033-2",
	"group" : { "key" : "Vela" },
	"Common" : "Mu Velorum",
	"OType" : "Star",
	"Distance" : "35.91",
	"RA_S" : 161.69248947,
	"DEC_S" : -49.42023604,
	"X" : 187,
	"Y" : 456,
	"Constellation" : "Vela ",
	"AMag" : 5.645,
	"key" : 79209,
	"title" : "Mu Velorum"
	},
{
	"Index" : "63192",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "HIP 52742, SAO 238468, HD 93563, GC 14849, HR 4221, DM CP-56 3800, TYC 8622-3779-1",
	"group" : { "key" : "Vela" },
	"Common" : "HR 4221",
	"OType" : "Be Star",
	"Distance" : "161.11",
	"RA_S" : 161.73946509,
	"DEC_S" : -56.7571888,
	"Constellation" : "Vela ",
	"AMag" : 5.117,
	"key" : 83192,
	"title" : "HR 4221"
	},
{
	"Index" : "54990",
	"MapNum" : "02",
	"ImageNum" : "02",
	"Desig" : "i Velorum, HIP 53773, SAO 222487, HD 95370, GC 15118, HR 4293, DM CD-41  6276, TYC 7733-2499-1",
	"group" : { "key" : "Vela" },
	"Common" : "i Velorum",
	"OType" : "Star",
	"Distance" : "60.16",
	"RA_S" : 165.03860361,
	"DEC_S" : -42.22585363,
	"Constellation" : "Vela ",
	"AMag" : 4.383,
	"key" : 74990,
	"title" : "i Velorum"
	},
{
	"Index" : "62528",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "1 Virginis, Omega Virginis, HIP 56779, SAO 118965, HD 101153, GC 15971, HR 4483, DM BD+08  2532, TYC 857-983-1",
	"group" : { "backgroundImage" : "images/Alignment/41.png",
		"description" : "Virgo is one of the constellations of the zodiac. Its name is Latin for virgin, and its symbol is \u264D. Lying between Leo to the west and Libra to the east, it is the second largest constellation in the sky (after Hydra). It can be easily found through its brightest star, Spica.\r\rThe bright Spica makes it easy to locate Virgo, as it can be found by following the curve of the Big Dipper to Arcturus in Bootes and continuing from there in the same curve (\u0022follow the arc to Arcturus and speed on to Spica\u0022).\r\rDue to the effects of precession, the First Point of Libra, (also known as the autumn equinox point) lies within the boundaries of Virgo very close to \u03B2 Virginis. This is one of the two points in the sky where the celestial equator crosses the ecliptic (the other being the First Point of Aries, now in the constellation of Pisces.) This point will pass into the neighbouring constellation of Leo around the year 2440.\r\rAccording to the Babylonian Mul.Apin, which dates between 1000 BC and 686 BC, this constellation was known as \u0022The Furrow\u0022, representing the goddess Shala\u0027s ear of grain or corn. One star in this constellation, Spica, retains this tradition as it is Latin for \u0022ear of grain\u0022, one of the major products of the Mesopotamian furrow. The constellation was also known as AB.SIN and absinnu. For this reason the constellation became associated with fertility. According to Gavin White the figure of Virgo corresponds to two Babylonian constellations - the \u0027Furrow\u0027 in the eastern sector of Virgo and the \u0027Frond of Erua\u0027 in the western sector. The Frond of Erua was depicted as a goddess holding a palm-frond - a motif that still occasionally appears in much later depictions of Virgo.\r\rThe Greeks and Romans associated Virgo with their goddess of wheat/agriculture, Demeter-Ceres who is the mother of Persephone-Proserpina. Alternatively, she was sometimes identified as the virgin goddess Iustitia or Astraea, holding the scales of justice in her hand as the constellation Libra. In the Middle Ages, Virgo was sometimes associated with the Blessed Virgin Mary.",
		"key" : "Virgo",
		"grouptype" : "Virgo",
		"Meaning" : "virgin or maiden",
		"Family" : "Zodiac",
		"Origin" : "ancient (Ptolemy)",
		"shortTitle" : "Virgo",
		"title" : "Virgo Objects Group" },
	"Common" : "Omega Virginis",
	"OType" : "Long-period variable star",
	"Distance" : "151.89",
	"RA_S" : 174.61503068,
	"DEC_S" : 8.13429773,
	"Constellation" : "Virgo ",
	"AMag" : 5.487,
	"key" : 82528,
	"title" : "Omega Virginis"
	},
{
	"Index" : "63523",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "2 Virginis, Xi Virginis, HIP 57328, SAO 119029, HD 102124, GC 16118, HR 4515, DM BD+09  2545, TYC 864-1209-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Xi Virginis",
	"OType" : "Star",
	"Distance" : "37.41",
	"RA_S" : 176.32099858,
	"DEC_S" : 8.25812036,
	"Constellation" : "Virgo ",
	"AMag" : 4.864,
	"key" : 83523,
	"title" : "Xi Virginis"
	},
{
	"Index" : "14875",
	"Description" : "Nu Virginis (\u03BD Vir, \u03BD Virginis) is a star in the constellation Virgo.\r\rNu Virginis is a M-type red giant with a mean apparent magnitude of +4.04. It is approximately 313 light years from Earth. It is classified as a semiregular variable star and its brightness varies by 0.06 magnitudes. This star has about 1.6 times the mass of the sun and an effective temperature of 3,795 K.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "3 Virginis, Nu Virginis, HIP 57380, SAO 119035, HD 102212, GC 16135, HR 4517, DM BD+07  2479, TYC 278-925-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Nu Virginis",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "90.06",
	"RA_S" : 176.4648432,
	"DEC_S" : 6.52938127,
	"X" : 665,
	"Y" : 216,
	"Constellation" : "Virgo ",
	"AMag" : 4.209,
	"key" : 34875,
	"title" : "Nu Virginis"
	},
{
	"Index" : "63524",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "4 Virginis, A01 Virginis, HIP 57562, SAO 119058, HD 102510, GC 16171, HR 4528, DM BD+09  2549, TYC 864-1210-1",
	"group" : { "key" : "Virgo" },
	"Common" : "A01 Virginis",
	"OType" : "Double or multiple star",
	"Distance" : "59.15",
	"RA_S" : 176.97874644,
	"DEC_S" : 8.24588835,
	"Constellation" : "Virgo ",
	"AMag" : 5.319,
	"key" : 83524,
	"title" : "A01 Virginis"
	},
{
	"Index" : "14540",
	"Description" : "Beta Virginis (\u03B2 Vir, \u03B2 Virginis) is a star in the constellation Virgo. It has the traditional names Zavijava (also Zavijah) and Alaraph. Despite being the beta star of the constellation Virgo it is only the fifth star in order of brightness.\r\rPhysically, Beta Virginis is larger and more massive than the Sun, and is comparatively metal-rich (that is, it has a higher preponderance of elements heavier than helium).\r\rSince it is close to the ecliptic, it can be occulted by the Moon and (very rarely) by planets. The next planetary occultation of Zavijava will take place on 11 August 2069, by Venus.\r\rThis was the star Einstein used during the solar eclipse of September 21, 1922, to determine the speed of light in space,[dubious \u2013 discuss] as it was close to the Sun.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "5 Virginis, Beta Virginis, HIP 57757, SAO 119076, HD 102870, GC 16215, HR 4540, DM BD+02  2489, TYC 273-924-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Zavijava / Zavijah / Alaraph",
	"OType" : "High proper-motion Star",
	"Distance" : "10.93",
	"RA_S" : 177.67382586,
	"DEC_S" : 1.76471731,
	"X" : 650,
	"Y" : 281,
	"Constellation" : "Virgo ",
	"AMag" : 3.649,
	"key" : 34540,
	"shortTitle" : "Alaraph (see HD113226,116658); Zavijava; Zavyava; Zawijah; Zarijan; Minelauva (also HD112300); Zavidzhava; Alaraf; Al'araf",
	"title" : "Zavijava / Zavijah / Alaraph"
	},
{
	"Index" : "14686",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "7 Virginis, b Virginis, HIP 58510, SAO 119156, HD 104181, GC 16406, HR 4585, DM BD+04  2556, TYC 276-1189-1",
	"group" : { "key" : "Virgo" },
	"Common" : "b Virginis",
	"OType" : "Star",
	"Distance" : "93.59",
	"RA_S" : 179.98713609,
	"DEC_S" : 3.65519708,
	"Constellation" : "Virgo ",
	"AMag" : 5.345,
	"key" : 34686,
	"title" : "b Virginis"
	},
{
	"Index" : "15448",
	"Description" : "Pi Virginis (\u03C0 Vir, \u03C0 Virginis) is a binary star in the constellation Virgo.\r\rPi Virginis is a spectroscopic binary which has a stellar classification of A5V and a combined apparent magnitude of +4.65. It is approximately 356 light years from Earth. The two components have apparent magnitudes 5.0 and 7.0 and are separated by 0.011 arcseconds. They have an orbital period of 309.67 days.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "8 Virginis, Pi Virginis, HIP 58590, SAO 119164, HD 104321, GC 16425, HR 4589, DM BD+07  2502, TYC 286-1022-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Pi Virginis",
	"OType" : "Spectroscopic binary",
	"Distance" : "117.49",
	"RA_S" : 180.21829452,
	"DEC_S" : 6.61433025,
	"X" : 616,
	"Y" : 216,
	"Constellation" : "Virgo ",
	"AMag" : 4.658,
	"key" : 35448,
	"title" : "Pi Virginis"
	},
{
	"Index" : "63733",
	"Description" : "Omicron Virginis (\u03BF Vir, \u03BF Virginis) is a star in the constellation Virgo.\r\rOmicron Virginis is a yellow G-type giant with an apparent magnitude of +4.12. It is approximately 171 light years from Earth. This star is radiating about 70 times the luminosity of the Sun and has 2.12 times the Sun\u0027s mass. It is around a billion years old.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "9 Virginis, Omicron Virginis, HIP 58948, SAO 119213, HD 104979, GC 16512, HR 4608, DM BD+09  2583, TYC 866-1180-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Omicron Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "50.04",
	"RA_S" : 181.30224957,
	"DEC_S" : 8.73297201,
	"X" : 601,
	"Y" : 188,
	"Constellation" : "Virgo ",
	"AMag" : 4.212,
	"key" : 83733,
	"title" : "Omicron Virginis"
	},
{
	"Index" : "33443",
	"Description" : "Eta Virginis (\u03B7 Vir, \u03B7 Virginis) is a multiple star system in the zodiac constellation of Virgo. It has the traditional name Zaniah pron.: /z\u0259\u02C8na\u026A.\u0259/. From parallax measurements, the distance to this star was found to be roughly 265 light-years (81 parsecs). It has an apparent visual magnitude of 3.89, which is bright enough for the system to be seen with the naked eye in dark skies.\r\rAlthough the star looks single, lunar occultations have shown this star to be a very close triple star system consisting of two stars only 0.5 AU apart with a third slightly more distant star. The inner pair is a spectroscopic binary that completes an orbit with a period of 72 days. The inclination of this orbit was determined through interferometer observations to be 45.5\u00B0, which allowed the individual masses of the two stars to be estimated. The primary star, \u03B7 Vir Aa, has a mass of about 2.5 times the Sun\u0027s mass, while the secondary, \u03B7 Vir Ab, has 1.9 solar masses. The faint tertiary star, \u03B7 Vir B, orbits the inner group in a wider orbit over a period of 13.1 years.\r\rBecause Zaniah is near the ecliptic, it can be occulted by the Moon and (very rarely) by planets. On October 12, 272 BC, the ancient Greek astronomer Timocharis observed a conjunction of the star with Venus. The last occultation by a planet took place on September 27, 1843, also by Venus, which will occult it again on November 19, 2445.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "15 Virginis, Eta Virginis, HIP 60129, SAO 138721, HD 107259, GC 16813, HR 4689, DM BD+00  2926, TYC 4940-1158-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Zaniah",
	"OType" : "Spectroscopic binary",
	"Distance" : "81.24",
	"RA_S" : 184.97647537,
	"DEC_S" : -0.66679342,
	"X" : 555,
	"Y" : 312,
	"Constellation" : "Virgo ",
	"AMag" : 3.874,
	"key" : 53443,
	"shortTitle" : "Zannakh",
	"title" : "Zaniah"
	},
{
	"Index" : "15362",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "16 Virginis, c Virginis, HIP 60172, SAO 119341, HD 107328, GC 16828, HR 4695, DM BD+04  2604, TYC 285-1247-1",
	"group" : { "key" : "Virgo" },
	"Common" : "c Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "94.37",
	"RA_S" : 185.0874191,
	"DEC_S" : 3.31257122,
	"Constellation" : "Virgo ",
	"AMag" : 5.093,
	"key" : 35362,
	"title" : "c Virginis"
	},
{
	"Index" : "37690",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "21 Virginis, q Virginis, HIP 61318, SAO 138845, HD 109309, GC 17122, HR 4781, DM BD-08  3372, TYC 5527-1966-1",
	"group" : { "key" : "Virgo" },
	"Common" : "q Virginis",
	"OType" : "Star",
	"Distance" : "79.19",
	"RA_S" : 188.44478881,
	"DEC_S" : -9.45207689,
	"Constellation" : "Virgo ",
	"AMag" : 5.469,
	"key" : 57690,
	"title" : "q Virginis"
	},
{
	"Index" : "37695",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "26 Virginis, Chi Virginis, HIP 61740, SAO 138892, HD 110014, GC 17227, HR 4813, DM BD-07  3452, TYC 5528-1471-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Chi Virginis",
	"OType" : "Double or multiple star",
	"Distance" : "89.94",
	"RA_S" : 189.81152926,
	"DEC_S" : -7.9955635,
	"Constellation" : "Virgo ",
	"AMag" : 4.783,
	"key" : 57695,
	"title" : "Chi Virginis"
	},
{
	"Index" : "33513",
	"Description" : "Gamma Virginis (\u03B3 Vir, \u03B3 Virginis) is a binary star system in the constellation Virgo. This star system has the traditional names Porrima, Postvarta and Arich. Porrima was the names of two ancient goddesses of prophecy \u2013 the Carmenae, sisters and assistants of Carmenta or Carmentis, worshiped and at times invoked by their women.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Laouiyet al Aoua, which was translated into Latin as Angulus Latratoris, meaning the angle of the barker. This star, along with \u03B2 Vir(Zavijava), \u03B7 Vir (Zaniah), \u03B4 Vir (Auva) and \u03B5 Vir (Vindemiatrix), were Al \u02BDAww\u0101\u02BC, the Barker.\r\rIn Chinese, \u592A\u5FAE\u5DE6\u57A3 (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n), meaning Left Wall of Supreme Palace Enclosure, refers to an asterism consisting of \u03B3 Virginis, \u03B7 Virginis, \u03B4 Virginis, \u03B5 Virginis and \u03B1 Comae Berenices. Consequently, \u03B3 Virginis itself is known as \u592A\u5FAE\u5DE6\u57A3\u4E8C (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n \u00E8r, English: the Second Star of Left Wall of Supreme Palace Enclosure.), representing \u6771\u4E0A\u76F8 (D\u014Dngsh\u01CEngxi\u0101ng), meaning The First Eastern Minister. \u6771\u4E0A\u76F8 (D\u014Dngsh\u01CEngxi\u0101ng), westernized into Shang Seang by R.H. Allen and the meaning is \u0022the High Minister of State\u0022.Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3.65 and 3.56, and of spectral type F0V. With an orbital period of 168.93 years, it was an easy object for amateur astronomers until the beginning of the 1990s, but in 2011 the smaller apparent distance between the stars requires a larger telescope. The last time they were at periapsis was in 1836. The distance will again be wide enough in 2020 to view with a small telescope. The star system has a combined apparent magnitude of 2.9. The system is 39 light years away from the Sun.\r\rAs Gamma Virginis is close to the ecliptic, it can be occulted by the Moon and (extremely rarely) by planets. In June 2011, Saturn came within a quarter of a degree from Porrima.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "29 Virginis, Gamma Virginis, HIP 61941B, SAO 138917, HD 110380, HR 4826, DM BD-00  2601B, TYC 4949-1120-2",
	"group" : { "key" : "Virgo" },
	"Common" : "Porrima / Postvarta / Arich",
	"OType" : "Star",
	"Distance" : "11.68",
	"RA_S" : 190.415887,
	"DEC_S" : -1.449342,
	"X" : 484,
	"Y" : 323,
	"Constellation" : "Virgo ",
	"AMag" : 3.528,
	"key" : 53513,
	"title" : "Porrima / Postvarta / Arich"
	},
{
	"Index" : "33512",
	"Description" : "Gamma Virginis (\u03B3 Vir, \u03B3 Virginis) is a binary star system in the constellation Virgo. This star system has the traditional names Porrima, Postvarta and Arich. Porrima was the names of two ancient goddesses of prophecy \u2013 the Carmenae, sisters and assistants of Carmenta or Carmentis, worshiped and at times invoked by their women.\r\rIn the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Laouiyet al Aoua, which was translated into Latin as Angulus Latratoris, meaning the angle of the barker. This star, along with \u03B2 Vir(Zavijava), \u03B7 Vir (Zaniah), \u03B4 Vir (Auva) and \u03B5 Vir (Vindemiatrix), were Al \u02BDAww\u0101\u02BC, the Barker.\r\rIn Chinese, \u592A\u5FAE\u5DE6\u57A3 (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n), meaning Left Wall of Supreme Palace Enclosure, refers to an asterism consisting of \u03B3 Virginis, \u03B7 Virginis, \u03B4 Virginis, \u03B5 Virginis and \u03B1 Comae Berenices. Consequently, \u03B3 Virginis itself is known as \u592A\u5FAE\u5DE6\u57A3\u4E8C (T\u00E0i W\u0113i Zu\u01D2 Yu\u00E1n \u00E8r, English: the Second Star of Left Wall of Supreme Palace Enclosure.), representing \u6771\u4E0A\u76F8 (D\u014Dngsh\u01CEngxi\u0101ng), meaning The First Eastern Minister. \u6771\u4E0A\u76F8 (D\u014Dngsh\u01CEngxi\u0101ng), westernized into Shang Seang by R.H. Allen and the meaning is \u0022the High Minister of State\u0022.Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3.65 and 3.56, and of spectral type F0V. With an orbital period of 168.93 years, it was an easy object for amateur astronomers until the beginning of the 1990s, but in 2011 the smaller apparent distance between the stars requires a larger telescope. The last time they were at periapsis was in 1836. The distance will again be wide enough in 2020 to view with a small telescope. The star system has a combined apparent magnitude of 2.9. The system is 39 light years away from the Sun.\r\rAs Gamma Virginis is close to the ecliptic, it can be occulted by the Moon and (extremely rarely) by planets. In June 2011, Saturn came within a quarter of a degree from Porrima.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "29 Virginis, Gamma Virginis, HIP 61941A, SAO 138917, HD 110379, GC 17270, HR 4825, DM BD-00  2601A, TYC 4949-1120-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Porrima / Postvarta / Arich",
	"OType" : "Star",
	"Distance" : "11.68",
	"RA_S" : 190.416596,
	"DEC_S" : -1.449514,
	"X" : 484,
	"Y" : 323,
	"Constellation" : "Virgo ",
	"AMag" : 3.484,
	"key" : 53512,
	"shortTitle" : "Arich",
	"title" : "Porrima / Postvarta / Arich"
	},
{
	"Index" : "64902",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "30 Virginis, Rho Virginis, HIP 61960, SAO 100211, HD 110411, GC 17276, HR 4828, DM BD+11  2485, TYC 878-1102-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Rho Virginis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "36.27",
	"RA_S" : 190.47106628,
	"DEC_S" : 10.23562633,
	"Constellation" : "Virgo ",
	"AMag" : 4.877,
	"key" : 84902,
	"title" : "Rho Virginis"
	},
{
	"Index" : "64755",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "32 Virginis, d02 Virginis, HIP 62267, SAO 119574, HD 110951, GC 17346, HR 4847, DM BD+08  2639, TYC 875-998-1",
	"group" : { "key" : "Virgo" },
	"Common" : "d02 Virginis",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "77.42",
	"RA_S" : 191.40440876,
	"DEC_S" : 7.67332584,
	"Constellation" : "Virgo ",
	"AMag" : 5.246,
	"key" : 84755,
	"title" : "d02 Virginis"
	},
{
	"Index" : "37744",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "40 Virginis, Psi Virginis, HIP 62985, SAO 139033, HD 112142, GC 17516, HR 4902, DM BD-08  3449, TYC 5535-1713-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Psi Virginis",
	"OType" : "Long-period variable star",
	"Distance" : "166.65",
	"RA_S" : 193.58817121,
	"DEC_S" : -9.53898928,
	"Constellation" : "Virgo ",
	"AMag" : 4.975,
	"key" : 57744,
	"title" : "Psi Virginis"
	},
{
	"Index" : "16125",
	"Description" : "Delta Virginis (\u03B4 Vir, \u03B4 Virginis) is a star in the zodiac constellation of Virgo. It has the traditional name Auva. With an apparent visual magnitude of 3.4, this star is bright enough to be seen with the naked eye. Based upon parallax measurements, it is located at a distance of about 198 light-years (61 parsecs) from Earth. The spectrum of this star matches a stellar classification of M3 III, which places it among the category of evolved stars called red giants. Indeed, the outer atmosphere of this star has expanded to around 48 times the radius of the Sun. Even though it has just 1.4 times the mass of the Sun, this wide envelope gives it a luminosity of roughly 468 times the Sun\u0027s. This energy is being radiated from a relatively cool outer atmosphere that has an effective temperature of nearly 4,000 K. It is this cool temperature that gives it the orange-red glow of an M-type star.\r\rThe outer envelope of this star is undergoing a type of pulsation that occurs in a class of variable stars known as semiregular variables and its brightness varies from magnitude +3.32 to +3.40. Based upon frequency analysis of the observed light curve, the star\u0027s variability exhibits multiple periods of pulsation. The detected periods are 13.0, 17.2, 25.6, 110.1 and 125.8 days. This is a high-velocity star with a peculiar velocity of more than 30 km s\u20131 relative to the mean motion of other stars in the vicinity.\r\rDelta Virginis is a possible binary star, as an 11th magnitude star is located at an angular separation of 80 arcseconds. This K-type dwarf may have an orbital period of over 200,000 years, but this has not been confirmed.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "43 Virginis, Delta Virginis, HIP 63090, SAO 119674, HD 112300, GC 17543, HR 4910, DM BD+04  2669, TYC 294-1032-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Auva",
	"OType" : "Red Giant Branch star",
	"Distance" : "60.81",
	"RA_S" : 193.90086808,
	"DEC_S" : 3.39747144,
	"X" : 439,
	"Y" : 259,
	"Constellation" : "Virgo ",
	"AMag" : 3.577,
	"key" : 36125,
	"shortTitle" : "Minelauva (also HD102870)",
	"title" : "Auva"
	},
{
	"Index" : "65482",
	"Description" : "Epsilon Virginis (\u03B5 Vir, \u03B5 Virginis) is the Bayer designation for a star in the zodiac constellation of Virgo. It has the traditional name Vindemiatrix, which comes from Greek through Latin and means Grape Gatherer. The apparent visual magnitude of this star is +2.8, making it the third brightest member of Virgo. Based upon parallax measurements made during the Hipparcos mission, Vindemiatrix lies at a distance of about 109.6 light-years (33.6 parsecs) from Earth, give or take a half light year.\r\rVindemiatrix is a giant star with a stellar classification of G8 III. With 2.6 times the mass of the Sun, it has reached a stage in its evolution where the hydrogen fuel in its core is exhausted. As a result, it has expanded to over ten times the Sun\u0027s girth and is now radiating around 77 times as much luminosity as the Sun. This energy is being emitted from its outer atmosphere at an effective temperature of 5,086 K, which gives it the yellow-hued glow of a G-type star. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.\r\rThis star is following an orbit through the Milky Way with an eccentricity of 0.11. This will carry it as close as 7.25 kpc (23.6 kly) to the Galactic Center, and take it as far as 8.95 kpc (29.2 kly). It is a likely member of the thin disk population and the orbit departs by no more than 60 pc (200 ly) from the galactic plane.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "47 Virginis, Epsilon Virginis, HIP 63608, SAO 100384, HD 113226, GC 17687, HR 4932, DM BD+11  2529, TYC 886-1326-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Vindemiatrix",
	"OType" : "High proper-motion Star",
	"Distance" : "33.6",
	"RA_S" : 195.54415972,
	"DEC_S" : 10.95914863,
	"X" : 417,
	"Y" : 162,
	"Constellation" : "Virgo ",
	"AMag" : 2.917,
	"key" : 85482,
	"shortTitle" : "Vindemiator; Vendemiatrix; Almuredin; Provindemiator; Protrigetrix; Protrygetor; Alaraph (see HD102870,116658); Vinde-Miatriks; Vindemiatriks",
	"title" : "Vindemiatrix"
	},
{
	"Index" : "37778",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "49 Virginis, HIP 64078, SAO 157739, HD 114038, GC 17794, HR 4955, DM BD-09  3628, TYC 5540-1439-1",
	"group" : { "key" : "Virgo" },
	"Common" : "49 Virginis",
	"OType" : "Star",
	"Distance" : "94.21",
	"RA_S" : 196.97421748,
	"DEC_S" : -10.74040422,
	"Constellation" : "Virgo ",
	"AMag" : 5.277,
	"key" : 57778,
	"title" : "49 Virginis"
	},
{
	"Index" : "33609",
	"Description" : "Theta Virginis (\u03B8 Vir, \u03B8 Virginis) is a star system in the constellation Virgo. It is approximately 415 light years from Earth.\r\rThe primary component, Theta Virginis A, is a white A-type subgiant with an apparent magnitude of +4.38. It is a spectroscopic binary whose components have magnitudes +4.6 and +6.8. The system has an orbital period of about 14 years. The separation of the components is 0.48 arcseconds. The binary star is orbited by the 9th magnitude A- or F-type Theta Virginis B, which is 7.1 arcseconds distant. A fourth component, Theta Virginis C, is 69.6 arcseconds away and has an apparent magnitude of 10.4.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "51 Virginis, Theta Virginis, HIP 64238AD, SAO 139189, HD 114330, GC 17828, HR 4963, DM BD-04  3430, TYC 4963-1316-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Theta Virginis",
	"OType" : "Star",
	"Distance" : "95.53",
	"RA_S" : 197.48746111,
	"DEC_S" : -5.53900515,
	"X" : 392,
	"Y" : 376,
	"Constellation" : "Virgo ",
	"AMag" : 4.395,
	"key" : 53609,
	"title" : "Theta Virginis"
	},
{
	"Index" : "42074",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "53 Virginis, HIP 64407, SAO 157788, HD 114642, GC 17870, HR 4981, DM BD-15  3613, TYC 6113-1726-1",
	"group" : { "key" : "Virgo" },
	"Common" : "53 Virginis",
	"OType" : "Variable Star",
	"Distance" : "33.91",
	"RA_S" : 198.01475876,
	"DEC_S" : -16.19860137,
	"Constellation" : "Virgo ",
	"AMag" : 5.084,
	"key" : 62074,
	"title" : "53 Virginis"
	},
{
	"Index" : "42099",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "55 Virginis, HIP 64577, SAO 157806, HD 114946, GC 17918, HR 4995, DM BD-19  3651, TYC 6116-1514-1",
	"group" : { "key" : "Virgo" },
	"Common" : "55 Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "38.97",
	"RA_S" : 198.54539807,
	"DEC_S" : -19.93094761,
	"Constellation" : "Virgo ",
	"AMag" : 5.418,
	"key" : 62099,
	"title" : "55 Virginis"
	},
{
	"Index" : "42097",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "57 Virginis, HIP 64725, SAO 157823, HD 115202, GC 17951, HR 5001, DM BD-19  3653, TYC 6116-1050-1",
	"group" : { "key" : "Virgo" },
	"Common" : "57 Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "38.47",
	"RA_S" : 198.99488425,
	"DEC_S" : -19.94310164,
	"Constellation" : "Virgo ",
	"AMag" : 5.333,
	"key" : 62097,
	"title" : "57 Virginis"
	},
{
	"Index" : "65939",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "59 Virginis, e Virginis, HIP 64792, SAO 119847, HD 115383, GC 17975, HR 5011, DM BD+10  2531, TYC 891-624-1",
	"group" : { "key" : "Virgo" },
	"Common" : "e Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "17.56",
	"RA_S" : 199.193814,
	"DEC_S" : 9.42415796,
	"Constellation" : "Virgo ",
	"AMag" : 5.249,
	"key" : 85939,
	"title" : "e Virginis"
	},
{
	"Index" : "66712",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "HIP 64823, SAO 100497, HD 115478, GC 17988, HR 5013, DM BD+14 2591, TYC 897-595-1",
	"group" : { "key" : "Virgo" },
	"Common" : "HR 5013",
	"OType" : "Star",
	"Distance" : "99.35",
	"RA_S" : 199.31511869,
	"DEC_S" : 13.67575284,
	"Constellation" : "Virgo ",
	"AMag" : 5.468,
	"key" : 86712,
	"title" : "HR 5013"
	},
{
	"Index" : "17091",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "60 Virginis, Sigma Virginis, HIP 64852, SAO 119855, HD 115521, GC 17995, HR 5015, DM BD+06  2722, TYC 305-948-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Sigma Virginis",
	"OType" : "Variable Star",
	"Distance" : "206.66",
	"RA_S" : 199.40117797,
	"DEC_S" : 5.46987345,
	"Constellation" : "Virgo ",
	"AMag" : 4.976,
	"key" : 37091,
	"title" : "Sigma Virginis"
	},
{
	"Index" : "42100",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "61 Virginis, HIP 64924, SAO 157844, HD 115617, GC 18007, HR 5019, DM BD-17  3813, TYC 6116-1517-1",
	"group" : { "key" : "Virgo" },
	"Common" : "61 Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "8.56",
	"RA_S" : 199.60130946,
	"DEC_S" : -18.31119576,
	"Constellation" : "Virgo ",
	"AMag" : 4.81,
	"key" : 62100,
	"title" : "61 Virginis"
	},
{
	"Index" : "42163",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "63 Virginis, HIP 65301, SAO 157899, HD 116292, GC 18104, HR 5044, DM BD-16  3650, TYC 6124-836-1",
	"group" : { "key" : "Virgo" },
	"Common" : "63 Virginis",
	"OType" : "Variable Star",
	"Distance" : "93.74",
	"RA_S" : 200.7546398,
	"DEC_S" : -17.73527571,
	"Constellation" : "Virgo ",
	"AMag" : 5.464,
	"key" : 62163,
	"title" : "63 Virginis"
	},
{
	"Index" : "37869",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "68 Virginis, i Virginis, HIP 65581, SAO 157938, HD 116870, GC 18168, HR 5064, DM BD-11  3516, TYC 5550-1597-1",
	"group" : { "key" : "Virgo" },
	"Common" : "i Virginis",
	"OType" : "Variable Star",
	"Distance" : "134.72",
	"RA_S" : 201.6798637,
	"DEC_S" : -12.70766245,
	"Constellation" : "Virgo ",
	"AMag" : 5.438,
	"key" : 57869,
	"title" : "i Virginis"
	},
{
	"Index" : "42133",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "69 Virginis, HIP 65639, SAO 157946, HD 116976, GC 18181, HR 5068, DM BD-15  3668, TYC 6120-921-1",
	"group" : { "key" : "Virgo" },
	"Common" : "69 Virginis",
	"OType" : "Variable Star",
	"Distance" : "85.86",
	"RA_S" : 201.86318368,
	"DEC_S" : -15.97357817,
	"Constellation" : "Virgo ",
	"AMag" : 4.873,
	"key" : 62133,
	"title" : "69 Virginis"
	},
{
	"Index" : "66813",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "70 Virginis, HIP 65721, SAO 100582, HD 117176, GC 18212, HR 5072, DM BD+14  2621, TYC 898-1042-1",
	"group" : { "key" : "Virgo" },
	"Common" : "70 Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "17.99",
	"RA_S" : 202.10754314,
	"DEC_S" : 13.77878712,
	"Constellation" : "Virgo ",
	"AMag" : 5.045,
	"key" : 86813,
	"title" : "70 Virginis"
	},
{
	"Index" : "33660",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "74 Virginis, l Virginis, HIP 66006, SAO 139390, HD 117675, GC 18288, HR 5095, DM BD-05  3714, TYC 4972-1456-1",
	"group" : { "key" : "Virgo" },
	"Common" : "l Virginis",
	"OType" : "Variable Star",
	"Distance" : "122.47",
	"RA_S" : 202.99118726,
	"DEC_S" : -6.25581602,
	"Constellation" : "Virgo ",
	"AMag" : 4.897,
	"key" : 53660,
	"title" : "l Virginis"
	},
{
	"Index" : "37853",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "76 Virginis, h Virginis, HIP 66098, SAO 139401, HD 117818, GC 18309, HR 5100, DM BD-09  3711, TYC 5548-1546-1",
	"group" : { "key" : "Virgo" },
	"Common" : "h Virginis",
	"OType" : "Star",
	"Distance" : "72.06",
	"RA_S" : 203.24196978,
	"DEC_S" : -10.16500048,
	"Constellation" : "Virgo ",
	"AMag" : 5.323,
	"key" : 57853,
	"title" : "h Virginis"
	},
{
	"Index" : "17351",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "78 Virginis, o Virginis, HIP 66200, SAO 120004, HD 118022, GC 18335, HR 5105, DM BD+04  2764, TYC 310-1430-1",
	"group" : { "key" : "Virgo" },
	"Common" : "o Virginis",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "56.65",
	"RA_S" : 203.53304921,
	"DEC_S" : 3.65896576,
	"Constellation" : "Virgo ",
	"AMag" : 4.916,
	"key" : 37351,
	"title" : "o Virginis"
	},
{
	"Index" : "33628",
	"Description" : "Zeta Virginis (\u03B6 Vir, \u03B6 Virginis) is a star in the zodiac constellation of Virgo. Zeta Virginis has the proper name Heze, which is of unclear origin. The star is known as Horn 2 (\u89D2\u5BBF\u4E8C) in Chinese astronomy. It is visible to the naked eye with has an apparent visual magnitude is +3.376  and is located about a half degree south of the celestial equator at a distance of 74.1 light-years (22.7 parsecs) from Earth.\r\r\u03B6 Virginis is a main sequence star with a spectral class A3 V, indicating that it is generating energy through the nuclear fusion of hydrogen at its core. This energy is being radiated from its outer envelope at an effective temperature of 8,247 K, giving Zeta Virginis the white hue of an A-type star. It has twice the mass and double the radius of the Sun and is about a half billion years old.\r\rIn 2010, a low mass stellar companion was discovered, \u03B6 Virginis B. The object has not been under observation for a sufficient length of time to determine accurate orbital elements. However, the pair are estimated to be orbiting at an average separation of at least 24.9 Astronomical Units and an orbital eccentricity of 0.16 or more. Their orbital period is a minimum of 124 years. This companion may be a red dwarf star, which would explain the observed X-ray flux from this system.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "79 Virginis, Zeta Virginis, HIP 66249, SAO 139420, HD 118098, GC 18351, HR 5107, DM BD+00  3076, TYC 4966-1366-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Heze",
	"OType" : "High proper-motion Star",
	"Distance" : "22.71",
	"RA_S" : 203.673937,
	"DEC_S" : -0.595939,
	"X" : 312,
	"Y" : 312,
	"Constellation" : "Virgo ",
	"AMag" : 3.38,
	"key" : 53628,
	"shortTitle" : "Kheze",
	"title" : "Heze"
	},
{
	"Index" : "37831",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "82 Virginis, m Virginis, HIP 66803, SAO 139490, HD 119149, GC 18509, HR 5150, DM BD-07  3674, TYC 5546-1582-1",
	"group" : { "key" : "Virgo" },
	"Common" : "m Virginis",
	"OType" : "Variable Star",
	"Distance" : "155.92",
	"RA_S" : 205.40323329,
	"DEC_S" : -8.70298216,
	"Constellation" : "Virgo ",
	"AMag" : 5.227,
	"key" : 57831,
	"title" : "m Virginis"
	},
{
	"Index" : "42183",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "89 Virginis, HIP 67494, SAO 158186, HD 120452, GC 18676, HR 5196, DM BD-17  3937, TYC 6127-879-1",
	"group" : { "key" : "Virgo" },
	"Common" : "89 Virginis",
	"OType" : "Star",
	"Distance" : "74.85",
	"RA_S" : 207.46784883,
	"DEC_S" : -18.1341664,
	"Constellation" : "Virgo ",
	"AMag" : 5.077,
	"key" : 62183,
	"title" : "89 Virginis"
	},
{
	"Index" : "33638",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "90 Virginis, p Virginis, HIP 67929, SAO 139613, HD 121299, GC 18800, HR 5232, DM BD-00  2758, TYC 4968-1517-1",
	"group" : { "key" : "Virgo" },
	"Common" : "p Virginis",
	"OType" : "Star",
	"Distance" : "75.5",
	"RA_S" : 208.67561264,
	"DEC_S" : -1.50312263,
	"Constellation" : "Virgo ",
	"AMag" : 5.281,
	"key" : 53638,
	"title" : "p Virginis"
	},
{
	"Index" : "18045",
	"Description" : "Tau Virginis (\u03C4 Vir, \u03C4 Virginis) is a star system in the constellation Virgo. It is approximately 218 light years from Earth.\r\rThe primary component, Tau Virginis A, is a white A-type main sequence dwarf with an apparent magnitude of +4.23. It has a 9th magnitude companion, Tau Virginis B, 80 arcseconds from the primary.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "93 Virginis, Tau Virginis, HIP 68520, SAO 120238, HD 122408, GC 18945, HR 5264, DM BD+02  2761, TYC 316-1271-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Tau Virginis",
	"OType" : "Star",
	"Distance" : "68.95",
	"RA_S" : 210.41163573,
	"DEC_S" : 1.54453325,
	"X" : 225,
	"Y" : 284,
	"Constellation" : "Virgo ",
	"AMag" : 4.25,
	"key" : 38045,
	"title" : "Tau Virginis"
	},
{
	"Index" : "37917",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "95 Virginis, HIP 68940, SAO 139736, HD 123255, GC 19041, HR 5290, DM BD-08  3697, TYC 5554-1682-1",
	"group" : { "key" : "Virgo" },
	"Common" : "95 Virginis",
	"OType" : "Star",
	"Distance" : "58.01",
	"RA_S" : 211.67842979,
	"DEC_S" : -9.31351601,
	"Constellation" : "Virgo ",
	"AMag" : 5.496,
	"key" : 57917,
	"title" : "95 Virginis"
	},
{
	"Index" : "42227",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "HIP 69269, SAO 158401, HD 123934, GC 19125, HR 5301, DM BD-15 3817, TYC 6138-15-1",
	"group" : { "key" : "Virgo" },
	"Common" : "HR 5301",
	"OType" : "Semi-regular pulsating Star",
	"Distance" : "140.9",
	"RA_S" : 212.71035724,
	"DEC_S" : -16.30203102,
	"Constellation" : "Virgo ",
	"AMag" : 5.136,
	"key" : 62227,
	"title" : "HR 5301"
	},
{
	"Index" : "18162",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "HIP 69389, SAO 120339, HD 124224, GC 19157, HR 5313, DM BD+03 2867, TYC 317-1590-1",
	"group" : { "key" : "Virgo" },
	"Common" : "HR 5313",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "79.15",
	"RA_S" : 213.06585278,
	"DEC_S" : 2.40943027,
	"Constellation" : "Virgo ",
	"AMag" : 4.964,
	"key" : 38162,
	"title" : "HR 5313"
	},
{
	"Index" : "37953",
	"Description" : "Kappa Virginis (\u03BA Vir, \u03BA Virginis) is a star in the constellation Virgo.\r\rKappa Virginis is an orange K-type giant with an apparent magnitude of +4.18. It is approximately 224 light years from Earth.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "98 Virginis, Kappa Virginis, HIP 69427, SAO 158427, HD 124294, GC 19168, HR 5315, DM BD-09  3878, TYC 5558-1738-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Kappa Virginis",
	"OType" : "Variable Star",
	"Distance" : "78.09",
	"RA_S" : 213.22393914,
	"DEC_S" : -10.2737004,
	"X" : 190,
	"Y" : 438,
	"Constellation" : "Virgo ",
	"AMag" : 4.325,
	"key" : 57953,
	"title" : "Kappa Virginis"
	},
{
	"Index" : "33723",
	"Description" : "Iota Virginis (\u03B9 Vir, \u03B9 Virginis) is a star in the constellation Virgo. It has the traditional name Syrma.\r\rSyrma is a yellow star of apparent magnitude 4.08 and spectral class F6 III about 70 light years from Earth. This star has 1.52 times the mass of the Sun, with a projected rotational velocity of 14.8 km s\u20131. It is radiating 8.6 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 6,282 K. The radius is about 2.5 times that of the Sun.\r\rThe name Syrma is from the Arabic (\u0633\u0631\u0645\u0627 (\u062A\u0637\u0631\u064A\u0632 sirm\u0101 \u0022train\u0022 (of a garment).",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "99 Virginis, Iota Virginis, HIP 69701, SAO 139824, HD 124850, GC 19244, HR 5338, DM BD-05  3843, TYC 4982-1645-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Syrma",
	"OType" : "Variable Star",
	"Distance" : "22.24",
	"RA_S" : 214.00362294,
	"DEC_S" : -6.00054537,
	"X" : 178,
	"Y" : 382,
	"Constellation" : "Virgo ",
	"AMag" : 4.126,
	"key" : 53723,
	"title" : "Syrma"
	},
{
	"Index" : "38044",
	"Description" : "Lambda Virginis (\u03BB Vir, \u03BB Virginis) is a binary star in the constellation Virgo. It also has the traditional name Khambalia (from old Coptic meaning \u0027Crooked Claw\u0027).\r\rLambda Virginis is a spectroscopic binary. The combined spectra of the components is classified as A2 and the system has an apparent magnitude of +4.52. It is approximately 187 light years from Earth. The two components have magnitudes of +5.3 and +5.4 and are separated by 0.0002 arcseconds. They have an orbital period of 206.64 days.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "100 Virginis, Lambda Virginis, HIP 69974, SAO 158489, HD 125337, GC 19311, HR 5359, DM BD-12  4018, TYC 5574-824-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Khambalia",
	"OType" : "Spectroscopic binary",
	"Distance" : "57.16",
	"RA_S" : 214.77746671,
	"DEC_S" : -13.37109165,
	"X" : 171,
	"Y" : 479,
	"Constellation" : "Virgo ",
	"AMag" : 4.532,
	"key" : 58044,
	"title" : "Khambalia"
	},
{
	"Index" : "33689",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "102 Virginis, Upsilon Virginis, HIP 70012, SAO 139866, HD 125454, GC 19323, HR 5366, DM BD-01  2938, TYC 4976-1278-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Upsilon Virginis",
	"OType" : "Variable Star",
	"Distance" : "80.13",
	"RA_S" : 214.88533681,
	"DEC_S" : -2.26552131,
	"Constellation" : "Virgo ",
	"AMag" : 5.256,
	"key" : 53689,
	"title" : "Upsilon Virginis"
	},
{
	"Index" : "18836",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "HIP 70400, SAO 120434, HD 126248, GC 19428, HR 5392, DM BD+06 2875, TYC 324-1444-1",
	"group" : { "key" : "Virgo" },
	"Common" : "HR 5392",
	"OType" : "Double or multiple star",
	"Distance" : "48.75",
	"RA_S" : 216.04726847,
	"DEC_S" : 5.82013268,
	"Constellation" : "Virgo ",
	"AMag" : 5.112,
	"key" : 38836,
	"title" : "HR 5392"
	},
{
	"Index" : "33693",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "105 Virginis, Phi Virginis, HIP 70755A, SAO 139951, HD 126868A, GC 19504, HR 5409, DM BD-01  2957, TYC 4977-1458-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Phi Virginis",
	"OType" : "High proper-motion Star",
	"Distance" : "41.32",
	"RA_S" : 217.05057347,
	"DEC_S" : -2.22795257,
	"Constellation" : "Virgo ",
	"AMag" : 4.918,
	"key" : 53693,
	"title" : "Phi Virginis"
	},
{
	"Index" : "33806",
	"Description" : "Mu Virginis (\u03BC Vir, \u03BC Virginis) is a star in the constellation Virgo. It has the traditional name Rijl al Awwa.\r\rRijl al Awwa is a yellow star of apparent magnitude 3.88 and spectral class F2 III about 61 light years from Earth. This star has 1.7 times the mass of the Sun and 2.1 times the Sun\u0027s radius. It is shining with 9.8 times the Sun\u0027s luminosity, which it is radiating from its outer atmosphere at an effective temperature of 7,140 K.\r\rThe medieval name Rijl al Awwa is from the Arabic \u0631\u062C\u0644 \u0627\u0644\u0639\u0648\u0649 rijl al-\u0027awwa\u0027 \u0022The foot of the barking (dog)\u0022.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "107 Virginis, Mu Virginis, HIP 71957, SAO 140090, HD 129502, GC 19816, HR 5487, DM BD-05  3936, TYC 4997-942-1",
	"group" : { "key" : "Virgo" },
	"Common" : "Rijl al Awwa",
	"OType" : "High proper-motion Star",
	"Distance" : "18.27",
	"RA_S" : 220.76509509,
	"DEC_S" : -5.65820353,
	"X" : 91,
	"Y" : 379,
	"Constellation" : "Virgo ",
	"AMag" : 3.907,
	"key" : 53806,
	"title" : "Rijl al Awwa"
	},
{
	"Index" : "19012",
	"Description" : "109 Virginis is the seventh brightest star in the constellation Virgo.\r\r109 Virginis is a white A-type main sequence dwarf with an apparent magnitude of +3.73. It is approximately 129 light years from Earth. This star has 2.3 times the mass of the Sun and 1.7 times the Sun\u0027s radius. It shines with 23 times the luminosity of the Sun, with the energy being radiated from its outer atmosphere at an effective temperature of 9,820 K.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "109 Virginis, HIP 72220, SAO 120648, HD 130109, GC 19884, HR 5511, DM BD+02  2862, TYC 326-1426-1",
	"group" : { "key" : "Virgo" },
	"Common" : "109 Virginis",
	"OType" : "Variable Star",
	"Distance" : "41.23",
	"RA_S" : 221.56218328,
	"DEC_S" : 1.89288176,
	"X" : 80,
	"Y" : 279,
	"Constellation" : "Virgo ",
	"AMag" : 3.716,
	"key" : 39012,
	"title" : "109 Virginis"
	},
{
	"Index" : "20024",
	"Description" : "110 Virginis is a star in the constellation Virgo.\r\r110 Virginis is an orange K-type giant with an apparent magnitude of +4.39. It is approximately 183 light years from Earth.",
	"MapNum" : "41",
	"ImageNum" : "41",
	"Desig" : "110 Virginis, HIP 73620, SAO 120809, HD 133165, GC 20237, HR 5601, DM BD+02  2905, TYC 338-1145-1",
	"group" : { "key" : "Virgo" },
	"Common" : "110 Virginis",
	"OType" : "Variable Star",
	"Distance" : "59.9",
	"RA_S" : 225.72516114,
	"DEC_S" : 2.09130414,
	"X" : 26,
	"Y" : 276,
	"Constellation" : "Virgo ",
	"AMag" : 4.513,
	"key" : 40024,
	"title" : "110 Virginis"
	},
{
	"Index" : "68764",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Iota Volantis, HIP 32912, SAO 256344, HD 51557, GC 9057, HR 2602, DM CP-70   572, TYC 9182-1412-1",
	"group" : { "backgroundImage" : "images/Alignment/13.png",
		"description" : "Volans is a constellation in the southern sky. It represents a flying fish; its name is a shortened form of its original name, Piscis Volans. Volans was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm diameter celestial globe published in 1597 (or 1598) in Amsterdam by Plancius with Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer\u0027s Uranometria of 1603.\r\rThere are two double stars within the constellation which can be observed using a small telescope, Gamma Volantis and Epsilon Volantis, along with two galaxies which may be more difficult to see clearly, NGC 2442 and NGC 2434. The magnitudes of the Gamma Volantis stars are fourth and sixth, and of Epsilon Volantis fourth and eighth.",
		"key" : "Volans",
		"grouptype" : "Volans",
		"Meaning" : "flying fish",
		"Family" : "Bayer",
		"Origin" : "1603, Uranometria, created by Keyser and de Houtman",
		"shortTitle" : "Volans",
		"title" : "Volans Objects Group" },
	"Common" : "Iota Volantis",
	"OType" : "Star",
	"Distance" : "172.49",
	"RA_S" : 102.86244405,
	"DEC_S" : -70.96341027,
	"Constellation" : "Volans ",
	"AMag" : 5.378,
	"key" : 88764,
	"title" : "Iota Volantis"
	},
{
	"Index" : "68720",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 33682, SAO 249704, HD 53501, GC 9280, HR 2662, DM CP-67  686, TYC 9178-929-1",
	"group" : { "key" : "Volans" },
	"Common" : "Gliese 3422",
	"OType" : "High proper-motion Star",
	"Distance" : "89.57",
	"RA_S" : 104.9605638,
	"DEC_S" : -67.91644449,
	"Constellation" : "Volans ",
	"AMag" : 5.326,
	"key" : 88720,
	"title" : "Gliese 3422"
	},
{
	"Index" : "68762",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Gamma01 Volantis, HIP 34473B, SAO 256373, HD 55864, GC 9513, HR 2735, DM CP-70   600B, TYC 9182-1410-1",
	"group" : { "key" : "Volans" },
	"Common" : "Gamma01 Volantis",
	"OType" : "Star",
	"Distance" : "49.26",
	"RA_S" : 107.17657779,
	"DEC_S" : -70.49710667,
	"Constellation" : "Volans ",
	"AMag" : 5.429,
	"key" : 88762,
	"title" : "Gamma01 Volantis"
	},
{
	"Index" : "68763",
	"Description" : "Gamma Volantis (\u03B3 Vol, \u03B3 Volantis) is a binary star in the constellation Volans. It is approximately 142 light years from Earth.\r\rThe primary component, designated \u03B3\u00B2 Volantis, is an orange K-type giant with an apparent magnitude of +3.78. Its companion, \u03B3\u00B9 Volantis, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +5.68. The two stars are 14.1 arcseconds apart in the sky.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Gamma02 Volantis, HIP 34481A, SAO 256374, HD 55865, GC 9514, HR 2736, DM CP-70   600A, TYC 9182-1411-1",
	"group" : { "key" : "Volans" },
	"Common" : "Gamma Volantis",
	"OType" : "Star",
	"Distance" : "43.39",
	"RA_S" : 107.18693308,
	"DEC_S" : -70.49892452,
	"X" : 469,
	"Y" : 414,
	"Constellation" : "Volans ",
	"AMag" : 3.86,
	"key" : 88763,
	"title" : "Gamma Volantis"
	},
{
	"Index" : "68727",
	"Description" : "Delta Volantis (\u03B4 Vol, \u03B4 Volantis) is a star in the constellation Volans.\r\rDelta Volantis is a yellow-white F-type bright giant with an apparent magnitude of +3.97. It is approximately 660 light years from Earth.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Delta Volantis, HIP 35228, SAO 249809, HD 57623, GC 9747, HR 2803, DM CP-67   730, TYC 9179-2107-1",
	"group" : { "key" : "Volans" },
	"Common" : "Delta Volantis",
	"OType" : "Star",
	"Distance" : "226.08",
	"RA_S" : 109.20760662,
	"DEC_S" : -67.9571512,
	"X" : 471,
	"Y" : 380,
	"Constellation" : "Volans ",
	"AMag" : 4.051,
	"key" : 88727,
	"title" : "Delta Volantis"
	},
{
	"Index" : "68811",
	"Description" : "Zeta Volantis (\u03B6 Vol, \u03B6 Volantis) is a binary star in the constellation Volans. It is approximately 134 light years from Earth.\r\rThe primary component, \u03B6 Volantis A, is an orange K-type giant with an apparent magnitude of +3.93. Its companion, the 10th magnitude \u03B6 Volantis B, lies 16.7 arcseconds away.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Zeta Volantis, HIP 37504, SAO 256438, HD 63295, GC 10444, HR 3024, DM CP-72   627, TYC 9188-1864-1",
	"group" : { "key" : "Volans" },
	"Common" : "Zeta Volantis",
	"OType" : "High proper-motion Star",
	"Distance" : "43.23",
	"RA_S" : 115.4552576,
	"DEC_S" : -72.60609618,
	"X" : 428,
	"Y" : 430,
	"Constellation" : "Volans ",
	"AMag" : 4.059,
	"key" : 88811,
	"title" : "Zeta Volantis"
	},
{
	"Index" : "68840",
	"Description" : "Epsilon Volantis (\u03B5 Vol, \u03B5 Volantis) is a triple star system in the constellation Volans. It is approximately 642 light years from Earth.\r\rThe primary component, Epsilon Volantis A, is a spectroscopic binary. It is classified a blue-white B-type subgiant and has an apparent magnitude of +4.35. The binary system has an orbital period of 14.17 days. The binary\u0027s companion, Epsilon Volantis B, is 6.05 arcseconds away and has an apparent magnitude of +8.1.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Epsilon Volantis, HIP 39794B, SAO 250128, HD 68520, GC 11098, HR 3223, DM CP-68   736, TYC 9193-3090-2",
	"group" : { "key" : "Volans" },
	"Common" : "Epsilon Volantis",
	"OType" : "Spectroscopic binary",
	"Distance" : "171.48",
	"RA_S" : 121.98247583,
	"DEC_S" : -68.61706528,
	"X" : 410,
	"Y" : 374,
	"Constellation" : "Volans ",
	"AMag" : 4.35,
	"key" : 88840,
	"title" : "Epsilon Volantis"
	},
{
	"Index" : "68839",
	"Description" : "Epsilon Volantis (\u03B5 Vol, \u03B5 Volantis) is a triple star system in the constellation Volans. It is approximately 642 light years from Earth.\r\rThe primary component, Epsilon Volantis A, is a spectroscopic binary. It is classified a blue-white B-type subgiant and has an apparent magnitude of +4.35. The binary system has an orbital period of 14.17 days. The binary\u0027s companion, Epsilon Volantis B, is 6.05 arcseconds away and has an apparent magnitude of +8.1.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Eps Volantis, HIP 39794A, TYC 9193-3090-1",
	"group" : { "key" : "Volans" },
	"Common" : "Epsilon Volantis",
	"OType" : "Spectroscopic binary",
	"Distance" : "171.48",
	"RA_S" : 121.98250612,
	"DEC_S" : -68.61706563,
	"X" : 410,
	"Y" : 374,
	"Constellation" : "Volans ",
	"AMag" : 4.378,
	"key" : 88839,
	"title" : "Epsilon Volantis"
	},
{
	"Index" : "66091",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 40680, SAO 250186, HD 70514, GC 11366, HR 3280, DM CP-65  907, TYC 8933-3031-1",
	"group" : { "key" : "Volans" },
	"Common" : "HR 3280",
	"OType" : "Star",
	"Distance" : "91.05",
	"RA_S" : 124.57836447,
	"DEC_S" : -65.61319104,
	"Constellation" : "Volans ",
	"AMag" : 5.184,
	"key" : 86091,
	"title" : "HR 3280"
	},
{
	"Index" : "68913",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Kappa01 Volantis, HIP 40817, SAO 256497, HD 71046, GC 11421, HR 3301, DM CP-71   677, TYC 9201-2149-1",
	"group" : { "key" : "Volans" },
	"Common" : "Kappa01 Volantis",
	"OType" : "Star",
	"Distance" : "132.99",
	"RA_S" : 124.95401146,
	"DEC_S" : -71.51490885,
	"Constellation" : "Volans ",
	"AMag" : 5.306,
	"key" : 88913,
	"title" : "Kappa01 Volantis"
	},
{
	"Index" : "68945",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Eta Volantis, HIP 41003, SAO 256505, HD 71576, GC 11485, HR 3334, DM CP-72   694, TYC 9205-1959-1",
	"group" : { "key" : "Volans" },
	"Common" : "Eta Volantis",
	"OType" : "Star",
	"Distance" : "116.77",
	"RA_S" : 125.51857573,
	"DEC_S" : -73.3999852,
	"Constellation" : "Volans ",
	"AMag" : 5.279,
	"key" : 88945,
	"title" : "Eta Volantis"
	},
{
	"Index" : "66121",
	"Description" : "Beta Volantis (\u03B2 Vol, \u03B2 Volantis) is the brightest star of the constellation Volans. Its distance is about 108 light years and spectral class is K1III.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Beta Volantis, HIP 41312, SAO 250228, HD 71878, GC 11567, HR 3347, DM CP-65   933, TYC 8937-2820-1",
	"group" : { "key" : "Volans" },
	"Common" : "Beta Volantis",
	"OType" : "Variable Star",
	"Distance" : "32.97",
	"RA_S" : 126.43414912,
	"DEC_S" : -66.1368911,
	"X" : 391,
	"Y" : 340,
	"Constellation" : "Volans ",
	"AMag" : 3.886,
	"key" : 86121,
	"title" : "Beta Volantis"
	},
{
	"Index" : "68890",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Theta Volantis, HIP 42425, SAO 256535, HD 74405, GC 11947, HR 3460, DM CP-69   946, TYC 9198-2243-1",
	"group" : { "key" : "Volans" },
	"Common" : "Theta Volantis",
	"OType" : "Star",
	"Distance" : "73.62",
	"RA_S" : 129.77151386,
	"DEC_S" : -70.38674584,
	"Constellation" : "Volans ",
	"AMag" : 5.184,
	"key" : 88890,
	"title" : "Theta Volantis"
	},
{
	"Index" : "66122",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "HIP 43414, SAO 250347, HD 76143, GC 12253, HR 3537, DM CP-66  927, TYC 8938-1028-1",
	"group" : { "key" : "Volans" },
	"Common" : "HR 3537",
	"OType" : "High proper-motion Star",
	"Distance" : "51.92",
	"RA_S" : 132.6450677,
	"DEC_S" : -66.7929839,
	"Constellation" : "Volans ",
	"AMag" : 5.378,
	"key" : 86122,
	"title" : "HR 3537"
	},
{
	"Index" : "66133",
	"Description" : "Alpha Volantis (\u03B1 Vol, \u03B1 Volantis) is a star in the constellation Volans.\r\rAlpha Volantis is an Am star with a stellar classification of kA3hA5mA5 V and an apparent magnitude of +4.00. It is approximately 125 light years from Earth. This star has an estimated age of 427 million years.",
	"MapNum" : "13",
	"ImageNum" : "13",
	"Desig" : "Alpha Volantis, HIP 44382, SAO 250422, HD 78045, GC 12532, HR 3615, DM CP-65  1065, TYC 8939-2729-1",
	"group" : { "key" : "Volans" },
	"Common" : "Alpha Volantis",
	"OType" : "Double or multiple star",
	"Distance" : "38.3",
	"RA_S" : 135.61164787,
	"DEC_S" : -66.39606826,
	"X" : 343,
	"Y" : 344,
	"Constellation" : "Volans ",
	"AMag" : 4.011,
	"key" : 86133,
	"title" : "Alpha Volantis"
	},
{
	"Index" : "5078",
	"Description" : "1 Vulpeculae (1 Vul) is a star in the constellation Vulpecula.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "1 Vulpeculae, HIP 94703, SAO 87010, HD 180554, GC 26569, HR 7306, DM BD+21  3713, TYC 1611-2043-1",
	"group" : { "backgroundImage" : "images/Alignment/22.png",
		"description" : "Vulpecula (pron.: /v\u028Cl\u02C8p\u025Bkj\u028Al\u0259/) is a faint constellation in the northern sky. Its name is Latin for \u0022little fox\u0022, although it is commonly known simply as the fox. It was identified in the seventeenth century, and is located in the middle of the Summer Triangle (an asterism consisting of the bright stars Deneb, Vega and Altair).\r\rIn the late 17th century, the astronomer Johannes Hevelius created Vulpecula. It was originally known as Vulpecula cum ansere (\u0022the little fox with the goose\u0022 or Vulpecula et Anser (\u0022the little fox and the goose\u0022), and was illustrated with a goose in the jaws of a fox. Hevelius did not regard the fox and the goose to be two separate constellations, but later the stars were divided into a separate Anser and Vulpecula. Today, they have been merged again under the name of the fox, but the goose is remembered by the name of the star \u03B1 Vulpeculae: Anser.\r\r",
		"key" : "Vulpecula",
		"grouptype" : "Vulpecula",
		"Meaning" : "fox",
		"Family" : "Hercules",
		"Origin" : "1690, Firmamentum Sobiescianum, Hevelius",
		"shortTitle" : "Vulpecula",
		"title" : "Vulpecula Objects Group" },
	"Common" : "1 Vulpeculae",
	"OType" : "Spectroscopic binary",
	"Distance" : "246.25",
	"RA_S" : 289.05433625,
	"DEC_S" : 21.3904264,
	"X" : 622,
	"Y" : 503,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.739,
	"key" : 25078,
	"title" : "1 Vulpeculae"
	},
{
	"Index" : "9245",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "2 Vulpeculae, HIP 94827A, SAO 87036, HD 180968, GC 26613, HR 7318, DM BD+22  3648, TYC 2124-2557-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "2 Vulpeculae",
	"OType" : "Variable Star of beta Cep type",
	"Distance" : "365.23",
	"RA_S" : 289.43182603,
	"DEC_S" : 23.02551713,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.434,
	"key" : 29245,
	"title" : "2 Vulpeculae"
	},
{
	"Index" : "9334",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "3 Vulpeculae, HIP 95260, SAO 87136, HD 182255, GC 26748, HR 7358, DM BD+25  3811, TYC 2132-3895-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "3 Vulpeculae",
	"OType" : "Pulsating variable Star",
	"Distance" : "119.73",
	"RA_S" : 290.71202099,
	"DEC_S" : 26.26240815,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.172,
	"key" : 29334,
	"title" : "3 Vulpeculae"
	},
{
	"Index" : "5045",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "4 Vulpeculae, HIP 95498, SAO 104818, HD 182762, GC 26821, HR 7385, DM BD+19  4010, TYC 1608-1202-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "4 Vulpeculae",
	"OType" : "Star",
	"Distance" : "83.19",
	"RA_S" : 291.36917392,
	"DEC_S" : 19.79836718,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.247,
	"key" : 25045,
	"title" : "4 Vulpeculae"
	},
{
	"Index" : "9297",
	"Description" : "Alpha Vulpeculae (Alpha Vul, \u03B1 Vulpeculae, \u03B1 Vul) is the brightest star in the constellation Vulpecula. It has a traditional name, variously represented as Lukida, Lucida Anseris, or Anser, a tradition kept from when the constellation had the name Vulpecula et Anser \u0027the fox and the goose\u0027.\r\rAlpha Vulpeculae is a red giant of spectral class M0 and has apparent magnitude +4.44. It is approximately 297 light years from Earth. It forms a wide optical binary with 8 Vulpeculae.\r\rIt has been analysed as a member of the Arcturus stream, a group of stars with high proper motion and metal-poor properties thought to be the remnants of a small galaxy consumed by the Milky Way.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "6 Vulpeculae, Alpha Vulpeculae, HIP 95771, SAO 87261, HD 183439, GC 26904, HR 7405, DM BD+24  3759, TYC 2129-2772-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "Lukida / Lucida Anseris / Anser",
	"OType" : "High proper-motion Star",
	"Distance" : "91.09",
	"RA_S" : 292.17637095,
	"DEC_S" : 24.66490581,
	"X" : 577,
	"Y" : 468,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.61,
	"key" : 29297,
	"title" : "Lukida / Lucida Anseris / Anser"
	},
{
	"Index" : "5061",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "9 Vulpeculae, HIP 96275, SAO 104990, HD 184606, GC 27047, HR 7437, DM BD+19  4063, TYC 1609-2082-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "9 Vulpeculae",
	"OType" : "Variable Star",
	"Distance" : "169.18",
	"RA_S" : 293.64540303,
	"DEC_S" : 19.77340131,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.974,
	"key" : 25061,
	"title" : "9 Vulpeculae"
	},
{
	"Index" : "9419",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "12 Vulpeculae, HIP 97679, SAO 87813, HD 187811, GC 27493, HR 7565, DM BD+22  3833, TYC 2140-3054-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "12 Vulpeculae",
	"OType" : "Be Star",
	"Distance" : "192.51",
	"RA_S" : 297.76712269,
	"DEC_S" : 22.61004685,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.86,
	"key" : 29419,
	"title" : "12 Vulpeculae"
	},
{
	"Index" : "9416",
	"Description" : "13 Vulpeculae (13 Vul) is a star in the constellation Vulpecula.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "13 Vulpeculae, HIP 97886B, SAO 87883, HD 188260B, GC 27544, HR 7592, DM BD+23  3820, TYC 2140-3051-2",
	"group" : { "key" : "Vulpecula" },
	"Common" : "13 Vulpeculae",
	"OType" : "Star",
	"Distance" : "102.19",
	"RA_S" : 298.36538185,
	"DEC_S" : 24.07959907,
	"X" : 504,
	"Y" : 488,
	"Constellation" : "Vulpecula ",
	"AMag" : 7.373,
	"key" : 29416,
	"title" : "13 Vulpeculae"
	},
{
	"Index" : "9415",
	"Description" : "13 Vulpeculae (13 Vul) is a star in the constellation Vulpecula.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "13 Vulpeculae, HIP 97886A, SAO 87883, HD 188260A, GC 27544, HR 7592, DM BD+23  3820, TYC 2140-3051-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "13 Vulpeculae",
	"OType" : "Star",
	"Distance" : "102.19",
	"RA_S" : 298.36538185,
	"DEC_S" : 24.07959907,
	"X" : 504,
	"Y" : 488,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.631,
	"key" : 29415,
	"title" : "13 Vulpeculae"
	},
{
	"Index" : "9546",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "15 Vulpeculae, HIP 98543, SAO 88071, HD 189849, GC 27753, HR 7653, DM BD+27  3587, TYC 2149-1880-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "15 Vulpeculae",
	"OType" : "Variable Star of alpha2 CVn type",
	"Distance" : "72.45",
	"RA_S" : 300.27520265,
	"DEC_S" : 27.75357235,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.675,
	"key" : 29546,
	"title" : "15 Vulpeculae"
	},
{
	"Index" : "9630",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "17 Vulpeculae, HIP 99080, SAO 88212, HD 190993, GC 27910, HR 7688, DM BD+23  3896, TYC 2154-4100-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "17 Vulpeculae",
	"OType" : "Star",
	"Distance" : "154.24",
	"RA_S" : 301.72253515,
	"DEC_S" : 23.61442289,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.029,
	"key" : 29630,
	"title" : "17 Vulpeculae"
	},
{
	"Index" : "9779",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "21 Vulpeculae, HIP 99738, SAO 88391, HD 192518, GC 28105, HR 7731, DM BD+28  3675, TYC 2167-1352-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "21 Vulpeculae",
	"OType" : "Variable Star of delta Sct type",
	"Distance" : "91.11",
	"RA_S" : 303.56053909,
	"DEC_S" : 28.69481596,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.213,
	"key" : 29779,
	"title" : "21 Vulpeculae"
	},
{
	"Index" : "9677",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "HIP 99824AB, SAO 88410, HD 192685, GC 28140, HR 7739, DM BD+25 4165, TYC 2159-2068-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "HR 7739",
	"OType" : "Be Star",
	"Distance" : "295.43",
	"RA_S" : 303.81622768,
	"DEC_S" : 25.59194889,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.725,
	"key" : 29677,
	"title" : "HR 7739"
	},
{
	"Index" : "9638",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "22 Vulpeculae, HIP 99853, SAO 88416, HD 192713, GC 28144, HR 7741, DM BD+23  3944, TYC 2155-2337-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "22 Vulpeculae",
	"OType" : "Eclipsing binary of Algol type (detached)",
	"Distance" : "588.2353",
	"RA_S" : 303.87599338,
	"DEC_S" : 23.50890841,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.289,
	"key" : 29638,
	"title" : "22 Vulpeculae"
	},
{
	"Index" : "9728",
	"Description" : "23 Vulpeculae (23 Vul) is a star in a double star system in the constellation Vulpecula.",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "23 Vulpeculae, HIP 99874AC, SAO 88428, HD 192806, GC 28152, HR 7744, DM BD+27  3666, TYC 2163-1794-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "23 Vulpeculae",
	"OType" : "Double or multiple star",
	"Distance" : "103.56",
	"RA_S" : 303.94222413,
	"DEC_S" : 27.81424753,
	"X" : 434,
	"Y" : 446,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.656,
	"key" : 29728,
	"title" : "23 Vulpeculae"
	},
{
	"Index" : "9678",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "24 Vulpeculae, HIP 99951, SAO 88451, HD 192944, GC 28183, HR 7753, DM BD+24  4075, TYC 2159-2069-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "24 Vulpeculae",
	"OType" : "Star",
	"Distance" : "134.02",
	"RA_S" : 304.19619486,
	"DEC_S" : 24.6710989,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.407,
	"key" : 29678,
	"title" : "24 Vulpeculae"
	},
{
	"Index" : "5516",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "29 Vulpeculae, HIP 101867, SAO 88944, HD 196724, GC 28740, HR 7891, DM BD+20  4658, TYC 1645-2169-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "29 Vulpeculae",
	"OType" : "Star",
	"Distance" : "70.95",
	"RA_S" : 309.63056858,
	"DEC_S" : 21.20118746,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.798,
	"key" : 25516,
	"title" : "29 Vulpeculae"
	},
{
	"Index" : "9655",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "28 Vulpeculae, HIP 101868, SAO 88945, HD 196740, GC 28741, HR 7894, DM BD+23  4084, TYC 2157-1647-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "28 Vulpeculae",
	"OType" : "Star",
	"Distance" : "159.97",
	"RA_S" : 309.63297618,
	"DEC_S" : 24.11595778,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.028,
	"key" : 29655,
	"title" : "28 Vulpeculae"
	},
{
	"Index" : "9855",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "30 Vulpeculae, HIP 102388, SAO 89084, HD 197752, GC 28920, HR 7939, DM BD+24  4229, TYC 2174-2867-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "30 Vulpeculae",
	"OType" : "Spectroscopic binary",
	"Distance" : "99.34",
	"RA_S" : 311.21875712,
	"DEC_S" : 25.2706023,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.046,
	"key" : 29855,
	"title" : "30 Vulpeculae"
	},
{
	"Index" : "9886",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "31 Vulpeculae, HIP 103004, SAO 89228, HD 198809, GC 29112, HR 7995, DM BD+26  4017, TYC 2179-2496-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "31 Vulpeculae",
	"OType" : "Variable Star",
	"Distance" : "57.7",
	"RA_S" : 313.03200577,
	"DEC_S" : 27.09697503,
	"Constellation" : "Vulpecula ",
	"AMag" : 4.66,
	"key" : 29886,
	"title" : "31 Vulpeculae"
	},
{
	"Index" : "9885",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "32 Vulpeculae, HIP 103200, SAO 89272, HD 199169, GC 29178, HR 8008, DM BD+27  3911, TYC 2179-2495-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "32 Vulpeculae",
	"OType" : "Variable Star",
	"Distance" : "177.32",
	"RA_S" : 313.64015621,
	"DEC_S" : 28.05762242,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.176,
	"key" : 29885,
	"title" : "32 Vulpeculae"
	},
{
	"Index" : "5626",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "33 Vulpeculae, HIP 103511, SAO 89332, HD 199697, GC 29267, HR 8032, DM BD+21  4424, TYC 1660-1962-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "33 Vulpeculae",
	"OType" : "Star",
	"Distance" : "138.43",
	"RA_S" : 314.56813293,
	"DEC_S" : 22.32590963,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.453,
	"key" : 25626,
	"title" : "33 Vulpeculae"
	},
{
	"Index" : "10023",
	"MapNum" : "22",
	"ImageNum" : "22",
	"Desig" : "35 Vulpeculae, HIP 105966, SAO 89720, HD 204414, GC 30048, HR 8217, DM BD+26  4164, TYC 2195-2392-1",
	"group" : { "key" : "Vulpecula" },
	"Common" : "35 Vulpeculae",
	"OType" : "High proper-motion Star",
	"Distance" : "58.32",
	"RA_S" : 321.91690692,
	"DEC_S" : 27.60859255,
	"Constellation" : "Vulpecula ",
	"AMag" : 5.384,
	"key" : 30023,
	"title" : "35 Vulpeculae"
	}
]
