Tau Cassiopeiae

τ Cassiopeiae
Location of τ Cassiopeiae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cassiopeia
Right ascension 23h 47m 03.454s
Declination +58° 39′ 07.17″
Apparent magnitude (V) +4.86
Characteristics
Spectral type K1 IIIa
U−B color index +1.05
B−V color index +1.11
Variable type Suspected
Astrometry
Radial velocity (Rv)−20.48±0.31 km/s
Proper motion (μ) RA: +60.379 mas/yr
Dec.: +56.828 mas/yr
Parallax (π)18.7789±0.0802 mas
Distance173.7 ± 0.7 ly
(53.3 ± 0.2 pc)
Absolute magnitude (MV)1.269
Details
Mass1.44 M
Radius10 R
Luminosity40 L
Surface gravity (log g)2.50±0.09 cgs
Temperature4,617±77 K
Metallicity [Fe/H]+0.06±0.06 dex
Rotational velocity (v sin i)5.9 km/s
Age3.90 Gyr
Other designations
τ Cas, 5 Cas, BD+57°2804, FK5 3909, GC 33010, HD 223165, HIP 117301, HR 9008, SAO 35763
Database references
SIMBADdata

Tau Cassiopeiae is a solitary, orange hued star in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from τ Cassiopeiae, and abbreviated Tau Cas or τ Cas. This star is bright enough to be seen with the naked eye, having an apparent visual magnitude of +4.86. Based upon an annual parallax shift of 18.78 mas as seen from Earth, this star is located about 173.7 light-years (53.3 pc) from the Sun. It is drifting closer with a radial velocity of −20 km/s.

The spectrum of this star indicates it is an evolved, K-type giant star with a stellar classification of K1 IIIa. It is a suspected variable star of unknown type. Tau Cassiopeiae is 3.9 billion years old with about 1.44 times the mass of the Sun and 10 times the Sun's radius. It is radiating 40 times the Sun's luminosity from its expanded photosphere at an effective temperature of around 4,617 K.