Zeta Arietis

Star in the constellation Aries From Wikipedia, the free encyclopedia

Zeta Arietis is a star in the northern constellation of Aries. Its name is a Bayer designation that is Latinized from ζ Arietis, and abbreviated Zeta Ari or ζ Ari. This star is dimly visible to the naked eye with an apparent visual magnitude of +4.87.[3] Based upon an annual parallax shift of 12.77 mas,[2] the distance to this star is approximately 255 light-years (78 parsecs). It is receding from the Sun with a radial velocity of +7 km/s.[6]

Right ascension03h 14m 54.098s[2]
Declination+21° 02 40.01[2]
Apparentmagnitude(V)+4.874±0.023[3]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
ζ Arietis
Location of ζ Arietis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Aries[1]
Right ascension 03h 14m 54.098s[2]
Declination +21° 02 40.01[2]
Apparent magnitude (V) +4.874±0.023[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A1 V[4]
U−B color index −0.01[5]
B−V color index −0.02[5]
Astrometry
Radial velocity (Rv)+7.3±2.8[6] km/s
Proper motion (μ) RA: −26.276 mas/yr[2]
Dec.: −72.900 mas/yr[2]
Parallax (π)12.7708±0.3734 mas[2]
Distance255 ± 7 ly
(78 ± 2 pc)
Absolute magnitude (MV)+0.35[1]
Details
Mass2.430±0.340[3] M
Radius2.974±0.115[3] R
Luminosity65.7±4.8[3] L
Surface gravity (log g)3.88±0.07[3] cgs
Temperature9,528±117[3] K
Rotational velocity (v sin i)133[7] km/s
Age333[8] Myr
Other designations
ζ Ari, 58 Arietis, BD+20 527, FK5 1089, GC 3872, HD 20150, HIP 15110, HR 972, SAO 75810, PPM 92319[9]
Database references
SIMBADdata
Close

This is an A-type main sequence star with a stellar classification of A1 V.[4] It is an estimated 333[8] million years old and is spinning rapidly with a projected rotational velocity of 133 km/s.[7] Zeta Arietis has 2.4 times the mass of the Sun and 3.0 times the Sun's radius.[3] It is radiating 66 times the luminosity of the Sun from its photosphere at an effective temperature of 9,528 K,[3] giving it the characteristic white-hued glow of an A-type star.[10]

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 was 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, and 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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