Kappa Cassiopeiae

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Kappa Cassiopeiae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia
Right ascension 00h 32m 59.9917s
Declination +62° 55′ 54.418″
Apparent magnitude (V) 4.189
Characteristics
Spectral type B1Iae
Apparent magnitude (U) 3.50
Apparent magnitude (B) 4.276
Apparent magnitude (J) 4.141
Apparent magnitude (H) 4.148
Apparent magnitude (K) 4.013
U−B color index -0.776
B−V color index +0.0869
J−H color index -0.0069
J−K color index +0.128
Variable type α Cyg
Astrometry
Radial velocity (Rv) -2.3 km/s
Proper motion (μ) RA: 3.99 mas/yr
Dec.: -2.10 mas/yr
Parallax (π) 0.79 ± 0.52 mas
Distance 4126.57 ly
(1265.82 pc)
Absolute magnitude (MV) -6.32
Details
Radius 41.4[1] R
Luminosity 330,000[1] L
Surface gravity (log g) 2.6[1]
Temperature 21,500[1] K
Rotational velocity (v sin i) 91[1] km/s
Other designations
15 Cassiopeiae, HR 130, HD 2905, BD+62°102, FK5 16, HIP 2599, SAO 11256, GC 645
The Bayer-designated stars in Cassiopeia. Kappa Cassiopeiae is circled.

Kappa Cassiopeiae (κ Cas, κ Cassiopeiae) is a star in the constellation Cassiopeia.

κ Cassiopeiae is a blue-white B-type supergiant with a mean apparent magnitude of +4.17. It is approximately 4100 light years from Earth. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude +4.22 to +4.30.

[edit] References

  1. ^ a b c d e Crowther, P. A.; Lennon, D. J.; Walborn, N. R. (January 2006), "Physical parameters and wind properties of galactic early B supergiants", Astronomy and Astrophysics 446 (1): 279–293, Bibcode 2006A&A...446..279C, doi:10.1051/0004-6361:20053685 
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