Chi Cassiopeiae

χ Cassiopeiae
Location of χ Cassiopeiae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cassiopeia
Right ascension 01h 33m 55.881s
Declination +59° 13′ 55.39″
Apparent magnitude (V) +4.696
Characteristics
Evolutionary stage red clump
Spectral type G9 IIIb
U−B color index +0.762
B−V color index +0.997
Astrometry
Radial velocity (Rv)+6.66±0.14 km/s
Proper motion (μ) RA: −44.188 mas/yr
Dec.: −18.538 mas/yr
Parallax (π)16.2553±0.095 mas
Distance201 ± 1 ly
(61.5 ± 0.4 pc)
Absolute magnitude (MV)+0.52
Details
Mass2.04 M
Radius10.27±0.32 R
Luminosity67.6 L
Surface gravity (log g)2.21 cgs
Temperature4,746 K
Metallicity [Fe/H]−0.34 dex
Rotational velocity (v sin i)0.44±0.45 km/s
Age1.0 Gyr
Other designations
χ Cas, 39 Cas, BD+58°260, HD 9408, HIP 7294, HR 442, SAO 22397
Database references
SIMBADdata

Chi Cassiopeiae is a solitary, yellow-hued star in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from χ Cassiopeiae, and is abbreviated Chi Cas or χ Cas. This star is visible to the naked eye with an apparent visual magnitude of +4.7. Based upon an annual parallax shift of 16.26 mas as seen from Earth, this system is located approximately 201 light-years (62 pc) from the Sun. At that distance, the visual magnitude is diminished by an extinction of 0.18 due to interstellar dust.

With a stellar classification of G9 IIIb, it has the spectrum of an evolved, G-type giant star. It is a red clump star that it is generating energy through helium fusion at its core, with an estimated age of a billion years. The star has about double the mass of the Sun and has expanded to 10.3 times the Sun's radius. It is radiating 67.6 times the Sun's luminosity from its photosphere at an effective temperature of 4,746 K.