10 Tauri

10 Tauri
Location of 10 Tauri (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 03h 36m 52.38s
Declination +00° 24′ 06.0″
Apparent magnitude (V) 4.29
Characteristics
Evolutionary stage subgiant
Spectral type F9IV-V
U−B color index +0.08
B−V color index +0.58
Astrometry
Radial velocity (Rv)+27.8±0.5 km/s
Proper motion (μ) RA: −232.563 mas/yr
Dec.: −481.472 mas/yr
Parallax (π)71.8370±0.01503 mas
Distance45.402 ± 0.009 ly
(13.920 ± 0.003 pc)
Absolute magnitude (MV)+3.60
Details
Mass1.139±0.016 M
Radius1.622±0.024 R
Luminosity3.042±0.042 L
Surface gravity (log g)4.06±0.03 cgs
Temperature6,000±59 K
Metallicity [Fe/H]−0.08±0.01 dex
Rotation17.6 days
Rotational velocity (v sin i)2.4 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

10 Tauri is a single star in the zodiac constellation of Taurus. It can be seen with the naked eye, having an apparent visual magnitude of 4.29. An annual parallax shift of 71.62 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 and has a relatively high proper motion.

The star has a stellar classification of F9IV-V, indicating that it is an F-type star between main sequence and subgiant. Modles indicate that it is a subgiant, having exhausted its core hydrogen and evolved away from the main sequence. It is around 5.7 billion years old with a rotation period of 17.6 days. 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 6,000 K.

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

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