Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cassiopeia |
Right ascension | 00h 55m 00.15523s[1] |
Declination | +58° 58′ 21.7108″[1] |
Apparent magnitude (V) | +4.86[2] |
Characteristics | |
Spectral type | K1 IIIa[3] |
U−B color index | +1.05[2] |
B−V color index | +1.11[2] |
Variable type | Suspected[4] |
Astrometry | |
Radial velocity (Rv) | −20.48±0.31[5] km/s |
Proper motion (μ) | RA: +60.81±0.19[1] mas/yr Dec.: +56.47±0.17[1] mas/yr |
Parallax (π) | 18.75 ± 0.20 mas[1] |
Distance | 174 ± 2 ly (53.3 ± 0.6 pc) |
Absolute magnitude (MV) | 1.269[6] |
Details | |
Mass | 1.44[7] M☉ |
Radius | 10[5] R☉ |
Luminosity | 40[7] L☉ |
Surface gravity (log g) | 2.50±0.09[8] cgs |
Temperature | 4,617±77[7] K |
Metallicity [Fe/H] | +0.06±0.06[8] dex |
Rotational velocity (v sin i) | 5.9[5] km/s |
Age | 3.90[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Tau Cassiopeiae (τ Cassiopeiae) is a solitary,[10] orange hued star in the northern constellation of Cassiopeia. It is bright enough to be seen with the naked eye, having an apparent visual magnitude of +4.86.[2] Based upon an annual parallax shift of 18.75 mas as seen from Earth,[1] this system is located about 174 light years from the Sun.
The spectrum of this star indicates it is an evolved, K-type giant star with a stellar classification of K1 IIIa.[3] It is a suspected variable star of unknown type.[4][11] Tau Cassiopeiae is 3.9[7] billion years old with about 1.44[7] times the mass of the Sun and 10[5] times the Sun's radius. It is radiating 40[7] times the Sun's luminosity from its expanded photosphere at an effective temperature of around 4,617 K.[7]
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