Xi2 Ceti

Star in the constellation Cetus From Wikipedia, the free encyclopedia

Xi2 Ceti is a star located in the equatorial constellation of Cetus. Its name is a Bayer designation that is Latinized from ξ2 Ceti, and abbreviated Xi2 Cet or ξ2 Cet. This star is visible to the naked eye with an apparent visual magnitude of +4.3.[3] This star is located at a distance of approximately 197 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of 12 km/s.[6] It made its closest approach some 2.7 million years ago at a distance of around 128 light-years.[1]

Right ascension02h 28m 09.55706s[2]
Declination+08° 27 36.2168[2]
Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
Xi2 Ceti
Location of ξ2 Ceti (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus[1]
Right ascension 02h 28m 09.55706s[2]
Declination +08° 27 36.2168[2]
Apparent magnitude (V) +4.279[3]
Characteristics
Spectral type B9.5III[4] or A0III-[5]
U−B color index −0.137[1]
B−V color index −0.053±0.003[1]
Astrometry
Radial velocity (Rv)11.90±1.3[6] km/s
Proper motion (μ) RA: 23.707±0.844 mas/yr[2]
Dec.: −4.787±0.778 mas/yr[2]
Parallax (π)16.5681±0.4608 mas[2]
Distance197 ± 5 ly
(60 ± 2 pc)
Absolute magnitude (MV)+0.45[1]
Details
Mass2.45[7] M
Radius2.60±0.17[8] R
Luminosity80.13[1] L
Surface gravity (log g)4.00±0.25[8] cgs
Temperature10,630±400[9] K
Metallicity [Fe/H]−0.43±0.04[1] dex
Rotational velocity (v sin i)55[7] km/s
Age127[7] Myr
Other designations
ξ2 Cet, 73 Ceti, BD+07°388, HD 15318, HIP 11484, HR 718, SAO 110543[10]
Database references
SIMBADdata
Close

Xi2 Ceti is a spectrophotometric standard star.[3] It displays a stellar classification of B9.5III,[4] which suggests it has exhausted its core hydrogen, evolved away from the main sequence, and expanded to become a giant star, although still only 127 million years old.[7] It has 2.45[7] times the mass and 2.6[8] times the radius of the Sun. The star is radiating 80[1] times the Sun's luminosity from its photosphere at an effective temperature of 10,630.[9] It has a high rate of spin, showing a projected rotational velocity of 55 km/s.[7]

In Chinese, 天囷 (Tiān Qūn), meaning Circular Celestial Granary, refers to an asterism consisting of α Ceti, κ1 Ceti, λ Ceti, μ Ceti, ξ1 Ceti, ξ2 Ceti, ν Ceti, γ Ceti, δ Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, the Chinese name for Xi2 Ceti itself is "the Sixth Star of Circular Celestial Granary", Tiān Qūn Liù.[11]

References

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