Sigma2 Tauri

Star in the constellation Taurus From Wikipedia, the free encyclopedia

Sigma2 Tauri2 Tauri) is the Bayer designation for a white-hued star in the zodiac constellation of Taurus. It has an apparent visual magnitude of +4.70,[2] which indicates it is visible to the naked eye. Based upon parallax measurements, σ2 Tauri is about 156 light-years distant.

Right ascension04h 39m 16.50230s[1]
Declination+15° 55 04.7029[1]
Quick facts Constellation, Right ascension ...
Sigma2 Tauri
Location of σ2 Tauri (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Taurus
Right ascension 04h 39m 16.50230s[1]
Declination +15° 55 04.7029[1]
Apparent magnitude (V) 4.70[2]
Characteristics
Spectral type A5 Vn[3]
U−B color index +0.13[2]
B−V color index +0.14[2]
Astrometry
Radial velocity (Rv)+40.8±1.2[4] km/s
Proper motion (μ) RA: +83.17[1] mas/yr
Dec.: −20.97[1] mas/yr
Parallax (π)20.97±0.27 mas[1]
Distance156 ± 2 ly
(47.7 ± 0.6 pc)
Details
Mass1.71[5] M
Radius1.9[6] R
Luminosity22.5[7] L
Surface gravity (log g)3.96[5] cgs
Temperature8,165±278[5] K
Metallicity [Fe/H]0.10±0.11[8] dex
Rotational velocity (v sin i)128[3] km/s
Age258[5] Myr
Other designations
92 Tauri, BD+15°666, FK5 2345, HD 29488, HIP 21683, HR 1479, SAO 94054, WDS J04393+1555A[9]
Database references
SIMBADdata
Close

σ2 Tauri is a solitary[10] A-type main sequence star with a stellar classification of A5 Vn.[3] The 'n' suffix indicates the lines are "nebulous" due to rapid rotation, and indeed it is spinning with a projected rotational velocity of 128 km/s.[3] The star is an estimated 258[5] million years old, with 1.7[5] times the mass of the Sun. It is radiating 22.5[7] times the Sun's luminosity from its photosphere at an effective temperature of around 8,165 K.[5] The star is considered a member of the Hyades cluster.[6]

In Chinese astronomy, σ2 Tauri is called 附耳, Pinyin: Fùěr, meaning Whisper, because this star is marking itself and stands alone in the Whisper asterism of the Net mansion (see: Chinese constellation).[11]

References

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