Epoch J2000 Equinox J2000
|Right ascension||01h 53m 31.81479s|
|Declination||+19° 17′ 37.8790″|
|Apparent magnitude (V)||3.86 (4.58/4.64)|
|Spectral type||B9 V + A1p Si|
|U−B color index||–0.12|
|B−V color index||–0.04|
|Radial velocity (Rv)||+3.7 km/s|
|Proper motion (μ)|| RA: +79.20 mas/yr |
Dec.: –97.63 mas/yr
|Parallax (π)||19.88 ± 0.96 mas|
|Distance||164 ± 8 ly |
(50 ± 2 pc)
|Rotational velocity (v sin i)||54 km/s|
|Surface gravity (log g)||4.25 cgs|
|Metallicity [Fe/H]||0.43 ± 0.14 dex|
|Rotational velocity (v sin i)||201 km/s|
|Gam¹ Ari: HD 11502, HR 545, SAO 92680, WDS J01535+1918B.|
|Gam² Ari: HD 11503, HR 546, SAO 92681, WDS J01535+1918A.|
Gamma Arietis (γ Arietis, abbreviated Gamma Ari, γ Ari) is a binary star in the northern constellation of Aries. The two components are designated γ¹ Arietis or Gamma Arietis B and γ² Arietis or Gamma Arietis A (formally named Mesarthim //, the traditional name for the Gamma Arietis system). 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 parallax measurements obtained during the Hipparcos mission, the distance to Gamma Arietis from the Sun is approximately 164 light-years (50 parsecs).
The 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, γ² Arietis, is a Lambda Boötis (chemically peculiar) star with a stellar classification of A1p Si and a magnitude of 4.64. It is classified as an α² CVn type variable star and its brightness varies by 0.04 magnitudes with a period of 2.61 days. The secondary, γ¹ Arietis, is a magnitude 4.58 B-type main-sequence star with a stellar classification of B9 V.
γ Arietis (Latinised to Gamma Arietis) is the system's Bayer designation; γ¹ and γ² Arietis those of its two components. The designation of the two components as Gamma Arietis A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).
Gamma Arietis has been called "the First Star in Aries" as having been at one time the nearest visible star to the equinoctial point.
It bore the traditional name Mesarthim. Originally it had shared the name Sheratan with Beta Arietis. However, this got corrupted to "Sartai" in medieval manuscripts, which Bayer erroneously explained as being the Hebrew grammatical term מְשָׁרְתִים mᵉshārᵉthīm "servants", and later scholars picked up on this term.
In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. It approved the name Mesarthim for the component γ² Arietis on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.
In Chinese, 婁宿 (Lóusù), meaning Bond (asterism), refers to an asterism consisting of Gamma, Beta and Alpha Arietis. Consequently, the Chinese name for Gamma Arietis itself is 婁宿二 (Lóusù Èr, English: the Second Star of Bond).
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