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Gamma Arietis

Gamma Arietis
Diagram showing star positions and boundaries of the Aries constellation and its surroundings
Cercle rouge 100%.svg

Location of γ Arietis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 01h 53m 31.81479s
Declination +19° 17′ 37.8790″
Apparent magnitude (V) 3.86 (4.58/4.64)
Characteristics
Spectral type B9 V + A1p Si
U−B color index –0.12
B−V color index –0.04
Astrometry
Radial velocity (Rv) +3.7 km/s
Proper motion (μ) RA: +79.20 mas/yr
Dec.: –97.63 mas/yr
Parallax (π) 19.88 ± 0.96mas
Distance 164 ± 8 ly
(50 ± 2 pc)
Details
Gam1 Ari
Radius 1.9 R
Rotational velocity (v sin i) 54 km/s
Gam2 Ari
Surface gravity (log g) 4.25 cgs
Temperature 10,970 K
Metallicity [Fe/H] 0.43 ± 0.14 dex
Rotational velocity (v sin i) 201 km/s
Other designations
5 Ari, BD+18 243, HIP 8832.
Gam1 Ari: HD 11502, HR 545, SAO 92680.
Gam2 Ari: HD 11503, HR 546, SAO 92681.
Database references
SIMBAD γ Ari
γ1 Ari
γ2 Ari

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 and γ² Arietis, also named Mesarthim. 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 milliarcseconds, 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.


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