Tau Geminorum

Tau Geminorum
Location of τ Geminorum (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Gemini
Right ascension 07h 11m 08.3703s
Declination +30° 14 42.590
Apparent magnitude (V) +4.42
Characteristics
Spectral type K2 III
U−B color index +1.41
B−V color index +1.261
Astrometry
Radial velocity (Rv)+22.02±0.07 km/s
Proper motion (μ) RA: −30.725(167) mas/yr
Dec.: −48.515(166) mas/yr
Parallax (π)8.3261±0.1591 mas
Distance392 ± 7 ly
(120 ± 2 pc)
Absolute magnitude (MV)−0.56±0.05
Details
Mass2.3±0.3 M
Radius30.27+1.08
−1.09
 R
Luminosity364±14 L
Surface gravity (log g)1.96±0.08 cgs
Temperature4,583±70 K
Metallicity [Fe/H]0.14±0.10 dex
Rotational velocity (v sin i)5.8 km/s
Age1.22±0.76 Gyr
Other designations
τ Gem, 46 Gem, BD+30 1439, HD 54719, HIP 34693, HR 2697, SAO 59858
Database references
SIMBADdata

Tau Geminorum, Latinized from τ Geminorum, is a star in the northern zodiac constellation of Gemini. It has the apparent visual magnitude of +4.42, making it visible to the naked eye under suitably good seeing conditions. This star is close enough to the Earth that its distance can be measured using the parallax technique, which yields a value of roughly 392 light-years (120 parsecs).

It is an evolved giant star of the spectral type K2 III. It has double the mass of the Sun and has expanded to 30 times the Sun's radius. Tau Geminorum is radiating 364 times as much radiation as the Sun from its expanded outer atmosphere at an effective temperature of 4,583 K, giving it the characteristic orange-hued glow of a K-type star. It appears to be rotating slowly with a projected rotational velocity of 5.8 km/s.