Sigma Cassiopeiae

σ Cassiopeiae
Location of σ Cassiopeiae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia
σ Cas A
Right ascension 23h 59m 00.538s
Declination +55° 45 17.75
Apparent magnitude (V) 5.01
σ Cas B
Right ascension 23h 59m 00.331s
Declination +55° 45 20.37
Apparent magnitude (V) 7.24
Characteristics
σ Cas A
Spectral type B2 IV
U−B color index −0.82
B−V color index −0.07
Variable type β Cep
σ Cas B
Spectral type B3 V
Astrometry
σ Cas A
Radial velocity (Rv)−12.6 km/s
Proper motion (μ) RA: +9.956 mas/yr
Dec.: −4.492 mas/yr
Parallax (π)2.7419±0.1491 mas
Distance1,190 ± 60 ly
(360 ± 20 pc)
Absolute magnitude (MV)−3.90
Radial velocity (Rv)−5.0 km/s
Proper motion (μ) RA: +8.651 mas/yr
Dec.: −3.739 mas/yr
Parallax (π)2.2572 ± 0.0558 mas
Distance1,440 ± 40 ly
(440 ± 10 pc)
Absolute magnitude (MV)−1.7
Details
A
Mass12 M
Radius11.3 R
Luminosity25,000 L
Surface gravity (log g)3.6 cgs
Temperature21,000 K
Rotational velocity (v sin i)170 km/s
Age15.8 Myr
Other designations
8 Cassiopeiae, HR 9071, HD 224572, BD+54°3082, HIP 118243, SAO 35947, ADS 17140, CCDM J23591+5546
Database references
SIMBADdata

Sigma Cassiopeiae (σ Cas, σ Cassiopeiae) is a binary star in the constellation Cassiopeia. It is 1,200 to 1,400 light years from Earth and has a combined apparent magnitude of +4.88, making it visible to the naked eye.

The primary component, σ Cassiopeiae A, is a B2 subgiant with an apparent magnitude of +5.0. Its companion, σ Cassiopeiae B, is a B5 main sequence dwarf with an apparent magnitude of +7.1. The two stars are three arcseconds apart.