(Redirected from Al Kalb al Rai )
Star in the constellation Cepheus
For other stars with this Bayer designation , see ρ Cephei .
Rho Cephei , Latinized from ρ Cephei, or simply ρ Cephei, is a solitary star in the northern constellation of Cepheus . With an apparent visual magnitude of 5.50, it is faintly visible to the naked eye, forming an optical pair with Rho Cephei . Based upon an annual parallax shift of 13.31 mas as seen from the Earth, it is located about 245 light years from the Sun .
Rho Cephei is an A-type main sequence star with a stellar classification of A3 V, estimated to be 85 million years old. It has a high rate of rotation, showing a projected rotational velocity of 133 km/s. The effective temperature of its photosphere is 8,511 K and its bolometric luminosity , the total amount of radiation it emits at all wavelengths, is 32 L ☉ .
References
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^ Gullikson, Kevin; Kraus, Adam; Dodson-Robinson, Sarah (2016). "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars" . The Astronomical Journal . 152 (2): 40. arXiv :1604.06456 . Bibcode :2016AJ....152...40G . doi :10.3847/0004-6256/152/2/40 . S2CID 119179065 .
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"rho Cep -- Star" , SIMBAD Astronomical Database , Centre de Données astronomiques de Strasbourg, retrieved 2017-05-05.
Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
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