10 Tauri

10 Tauri is a single[10] star in the zodiac constellation of Taurus. It can be seen with the naked eye, having an apparent visual magnitude of 4.29.[2] An annual parallax shift of 71.62[1] mas provides a distance estimate of 45.5 light years. It is moving further from the Sun with a radial velocity of +28 km/s[4] and has a relatively high proper motion.[2]

10 Tauri
Chart showing the position of the stars in the constellation Taurus
Location of 10 Tauri (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationTaurus
Right ascension03h 36m 52.38s[1]
Declination+00° 24′ 06.0″[1]
Apparent magnitude (V)4.29[2]
Characteristics
Spectral typeF8 V[3]
U−B color index+0.08[2]
B−V color index+0.58[2]
Astrometry
Radial velocity (Rv)+27.8±0.5[4] km/s
Proper motion (μ) RA: −232.60±0.59[1] mas/yr
Dec.: −481.92±0.54[1] mas/yr
Parallax (π)71.62 ± 0.54 mas[1]
Distance45.5 ± 0.3 ly
(14.0 ± 0.1 pc)
Absolute magnitude (MV)+3.60[5]
Details[6]
Mass1.139±0.016 M
Radius1.622±0.024 R
Luminosity3.042±0.042 L
Surface gravity (log g)4.07±0.05[7] cgs
Temperature5,997±44 K
Metallicity [Fe/H]−0.12±0.07[8] dex
Rotation17.6 days[9]
Rotational velocity (v sin i)2.4[5] km/s
Age5.7±0.4 Gyr
Other designations
10 Tau, BD−00° 572, FK5 1101, GJ 147, HD 22484, HIP 16852, HR 1101, SAO 111292, LHS 1569, LTT 11194
Database references
SIMBADdata

The star has a stellar classification of F8 V,[3] indicating that it is an ordinary F-type main-sequence star that is generating energy through hydrogen fusion in its core region. It is around 5.7[6] billion years old with a rotation period of 17.6 days.[9] The star has 1.14 times the mass of the Sun and 1.6 times the Sun's radius. It is radiating three times the Sun's luminosity from its photosphere at an effective temperature of around 5,997 K.[6]

A debris disk has been identified orbiting 10 Tauri, based on excess infrared radiation detected by IRAS/ISO.[11]

10 Tauri was the brightest star in the obsolete constellation Psalterium Georgii (Harpa Georgii).[12]

References