Kappa Cephei

Kappa Cephei
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 20h 08m 53.348s[1]
Declination +77° 42 41.12[1]
Apparent magnitude (V) 4.395[2]
Characteristics
Spectral type B9III[2] + A7V
U−B color index -0.12
B−V color index -0.04
Astrometry
Radial velocity (Rv)−22.8 ± 0.9[2] km/s
Proper motion (μ) RA: 11.57 ± 0.29[1] mas/yr
Dec.: 24.34 ± 0.33[1] mas/yr
Parallax (π)10.36 ± 0.29[1] mas
Distance315 ± 9 ly
(97 ± 3 pc)
Absolute magnitude (MV)-0.53
Details
Radius4.45 ± 0.22[3] R
Surface gravity (log g)3.66 ± 0.03[3] cgs
Temperature10,174 ± 55[3] K
Other designations
kap Cep, 1 Cep, BD+77° 764, GSC 04589-03106, HD 192907, HIP 99255, HR 7750, SAO 9665.

Kappa Cephei (κ Cep) is a binary star[4] in the constellation Cepheus. Its apparent magnitude is 4.395.[2] Located approximately 96.53 parsecs (314.8 ly) distant,[1] the primary is a blue giant of spectral type B9III,[2] a star that has used up its core hydrogen and is likely expanding to become a supergiant. The secondary is a main sequence star of spectral type A7V. It has an apparent magnitude of 8.34 and lies 7.38 arc seconds distant.[5]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry
  2. 2.0 2.1 2.2 2.3 2.4 "Kappa Cephei". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 12 October 2014.
  3. 3.0 3.1 3.2 Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal 129 (3): 1642–1662, arXiv:astro-ph/0412542, Bibcode:2005AJ....129.1642F, doi:10.1086/427855
  4. Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society 389 (2): 869. doi:10.1111/j.1365-2966.2008.13596.x.