Xi Arietis

Star in the constellation Aries From Wikipedia, the free encyclopedia

Xi Arietis is a binary star[9] system in the northern constellation of Aries. Its name is a Bayer designation that is Latinized from ξ Arietis, and abbreviated Xi Ari or ξ Ari. This system has an apparent visual magnitude of 5.46,[2] and so is dimly visible to the naked eye. Based upon an annual parallax shift of 3.74±0.29 mas as seen from Earth, it is 770 ± 30 light-years (236.1 ± 9.2 parsecs) distant from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.24 due to interstellar dust.[5] The proximity of this system to the ecliptic means it is subject to lunar occultations.[10]

Quick facts Constellation, Right ascension ...
ξ Arietis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aries
Right ascension 02h 24m 49.058s[1]
Declination +10° 36 38.01[1]
Apparent magnitude (V) +5.46[2]
Characteristics
Spectral type B7 IV[3]
U−B color index −0.48[2]
B−V color index −0.10[2]
Astrometry
Radial velocity (Rv)−0.5±2.8[4] km/s
Proper motion (μ) RA: +20.979 mas/yr[1]
Dec.: −15.022 mas/yr[1]
Parallax (π)4.2483±0.1511 mas[1]
Distance770 ± 30 ly
(235 ± 8 pc)
Absolute magnitude (MV)−0.43[5]
Details
Mass4.85±0.13[6] M
Luminosity1,000+186
157
[6] L
Surface gravity (log g)3.897±0.017[7] cgs
Temperature13,627±100[7] K
Rotational velocity (v sin i)164±8[7] km/s
Age195[5] Myr
Other designations
ξ Ari, ψ Ceti, 24 Arietis, BD+09°316, FK5 2164, GC 2901, HD 14951, HIP 11249, HR 702, SAO 92932, PPM 118200[8]
Database references
SIMBADdata
Close

This is a double-lined spectroscopic binary.[9] The spectrum matches a stellar classification of B7 IV,[3] which suggests a subgiant star that has exhausted the supply of hydrogen at its core and is in the process of evolving into a giant star. Xi Arietis was once a designation for Psi Ceti (ψ Cet, ψ Ceti), and was later recognized to be a duplicate by Bayer.[11]

References

Related Articles

Wikiwand AI