Star in the constellation Pegasus
ν Pegasi , Latinized as Nu Pegasi is a single star in the northern constellation of Pegasus . It is an orange-hued star that is faintly visible to the naked eye with an apparent visual magnitude of 4.84. The star is located approximately 261 light years away based on parallax , but is drifting closer with a radial velocity of −19 km/s .
This is an aging giant star , most likely (94% chance) on the red giant branch , with a stellar classification of K4III. It is a suspected variable, with a magnitude range observed from 4.83 to 4.86. With the supply of hydrogen at its core exhausted, the star has cooled and expanded to 24.6 times the Sun's radius . It is 13% more massive than the Sun and is radiating 149 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,073 K .
References
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Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331. arXiv :1108.4971 . Bibcode :2012AstL...38..331A . doi :10.1134/S1063773712050015 . S2CID 119257644 . Vizier catalog entry
^ Reffert, Sabine; et al. (2015). "Precise radial velocities of giant stars". Astronomy & Astrophysics . 574 : A116. arXiv :1412.4634 . Bibcode :2015A&A...574A.116R . doi :10.1051/0004-6361/201322360 . hdl :10722/215277 . S2CID 59334290 . Vizier catalog entry
De Medeiros, J. R.; Mayor, M. (1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series . 139 (3): 433. arXiv :astro-ph/0608248 . Bibcode :1999A&AS..139..433D . doi :10.1051/aas:1999401 . Vizier catalog entry
"nu. Peg" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-10-01.
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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