Zeta Arietis, Latinized from ζ Arietis, is a star in the northern constellation of Aries. It is dimly visible to the naked eye with an apparent visual magnitude of +4.89.[2] Based upon an annual parallax shift of 12.77 mas,[1] the distance to this star is 255 ± 7 light-years (78 ± 2 parsecs). This is an A-type main sequence star with a stellar classification of A1 V.[3] It has a high rate of rotation with a projected rotational velocity of 133 km/s.[8] The star is shining at an effective temperature of 9,500 K,[7] giving it the characteristic white-hued glow of an A-type star.[10]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 03h 14m 54.09143s[1] |
Declination | +21° 02′ 39.9952″[1] |
Apparent magnitude (V) | +4.89[2] |
Characteristics | |
Spectral type | A1 V[3] |
U−B color index | –0.01[2] |
B−V color index | –0.02[2] |
Astrometry | |
Radial velocity (Rv) | +7.0[4] km/s |
Proper motion (μ) | RA: –19.930[1] mas/yr Dec.: –72.900[1] mas/yr |
Parallax (π) | 12.7708 ± 0.3734 mas[1] |
Distance | 255 ± 7 ly (78 ± 2 pc) |
Absolute magnitude (MV) | +0.35[5] |
Details | |
Mass | 2.66±0.07[6] M☉ |
Luminosity | 73[5] L☉ |
Temperature | 9,500[7] K |
Rotational velocity (v sin i) | 133[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Name
This star, along with δ Ari, ε Ari, π Ari, and ρ3 Ari, were Al Bīrūnī's Al Buṭain (ألبطين), the dual of Al Baṭn, the Belly.[11] According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Buṭain were the title for five stars : δ Ari as Botein, π Ari as Al Buṭain I, ρ3 Ari as Al Buṭain II, ε Ari as Al Buṭain III dan ζ Ari as Al Buṭain IV.[12]
In Chinese, 天陰 (Tiān Yīn), meaning Yin Force, refers to an asterism consisting of ζ Arietis, 63 Arietis, δ Arietis, τ Arietis and 65 Arietis.[13] Consequently, the Chinese name for ζ Arietis itself is 天陰二 (Lóu Su èr, English: the Second Star of Yin Force.)[14]
References
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