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Gamma Geminorum

Gamma Geminorum A
Diagram showing star positions and boundaries of the Gemini constellation and its surroundings
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Location of γ Geminorum (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Gemini
Right ascension 06h 37m 42.71050s
Declination +16° 23′ 57.4095″
Apparent magnitude (V) 1.915
Characteristics
Spectral type A1.5IV+
U−B color index +0.137
B−V color index +0.005
Astrometry
Radial velocity (Rv) -12.5 km/s
Proper motion (μ) RA: +13.81 mas/yr
Dec.: -54.96 mas/yr
Parallax (π) 29.84 ± 2.23mas
Distance 109 ± 8 ly
(34 ± 3 pc)
Orbit
Period (P) 4,614.51 days
Eccentricity (e) 0.8933 ± 0.0013
Periastron epoch (T) 244399.13 ± 0.77
Argument of periastron (ω)
(secondary)
312.60 ± 0.60°
Semi-amplitude (K1)
(primary)
11.881 ± 0.068 km/s
Details
Mass 2.81 M
Radius 3.3 R
Luminosity 123 L
Surface gravity (log g) 3.60 cgs
Temperature 9,260 K
Metallicity [Fe/H] –0.12 dex
Rotational velocity (v sin i) 15 km/s
Other designations
Alhena, 24 Geminorum, BD+16°1223, FK5 251, GCTP1539.00, HIP 31681, HD 47105, HR 2421, SAO 95912
Database references
SIMBAD data

Gamma Geminorum (γ Geminorum, abbreviated Gamma Gem, γ Gem), also named Alhena, is the third-brightest star in the constellation of Gemini. It has an apparent visual magnitude of 1.9, making it easily visible to the naked eye even in urban regions. Based upon parallax measurements with the Hipparcos satellite, it is located at a distance of roughly 109 light-years (33 parsecs) from the Sun.

Alhena is an evolving star that is exhausting the supply of hydrogen at its core and has entered the subgiant stage. The spectrum matches a stellar classification of A0 IV. Compared to the Sun it has 2.8 times the mass and 3.3 times the radius. It is radiating around 123 times the luminosity of the Sun from its outer envelope at an effective temperature of 9,260 K. This gives it a white hue typical of an A-class star.

This is a spectroscopic binary system with a period of 12.6 years (4,614.51 days) in a highly eccentric Keplerian orbit.

γ Geminorum (Latinised to Gamma Geminorum) is the star's Bayer designation. The traditional name Alhena is derived from the Arabic الهنعة Al Han'ah, 'the brand' (on the neck of the camel), whilst the alternate name Almeisan is from the Arabic المیسان Al Maisan, 'the shining one.' Al Hanʽah was the name of star association consisting of this star, along with Mu Geminorum (Tejat Posterior), Nu Geminorum, Eta Geminorum (Tejat Prior) and Xi Geminorum (Alzirr). They also were associated in Al Nuḥātai, the dual form of Al Nuḥāt, 'a Camel's Hump'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Alhena for this star.


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Wikipedia

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