Star in the constellation Perseus
36 Persei is a solitary,[ 8] variable star located 121 light years away from the Sun in the northern constellation of Perseus . It is visible to the naked eye as a dim, yellow-white hued point of light with a baseline apparent visual magnitude of 5.32.[ 2] The star is drifting closer to the Sun with a heliocentric radial velocity of −47.5 km/s,[ 4] and may come as close as 36.6 light-years in 661,000 years.[ 5]
The stellar classification of 36 Persei is F4III,[ 3] matching an aging giant star that has used up its core hydrogen . This object is used by astronomers as a spectral standard for stars with a similar class.[ 9] The star is a suspected variable of unknown type, ranging in visual magnitude from 5.29 down to 5.33,[ 10] and is a source of X-ray emission .[ 11] The star is 2.2[ 4] billion years old with a projected rotational velocity of 28 km/s.[ 6] It has an estimated 1.5[ 4] times the mass of the Sun and has not yet expanded significantly, having 2.3[ 1] times the Sun's girth. The star is radiating 8.6[ 1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,546 [ 1]
References
^ a b c d e f g h i j k Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues . 2237 . Bibcode :2002yCat.2237....0D .
^ a b Ljunggren, B.; Oja, T. (1961). "The Uppsala spectral classification". Uppsala Astronomical Observatory Annual . 4 (10): 10. Bibcode :1961UppAn...4j...1L .
^ a b c d e f g h Casagrande, L.; et al. (June 2011). "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey". Astronomy and Astrophysics . 530 : A138. arXiv :1103.4651 . Bibcode :2011A&A...530A.138C . doi :10.1051/0004-6361/201016276 . S2CID 56118016 .
^ a b 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
^ a b De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics . 561 : A126. arXiv :1312.3474 . Bibcode :2014A&A...561A.126D . doi :10.1051/0004-6361/201220762 . S2CID 54046583 . Vizier catalog entry
^ "36 Per" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-07-14 .
^ 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 .
^ Garcia, B. (1989). "A list of MK standard stars". Bulletin d'Information du Centre de Données Stellaires . 36 : 27. Bibcode :1989BICDS..36...27G .
^ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports , 5.1, 61 (1): 80–88, Bibcode :2017ARep...61...80S , doi :10.1134/S1063772917010085 , S2CID 125853869 .
^ Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009). "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources". The Astrophysical Journal Supplement . 184 (1): 138–151. arXiv :0910.3229 . Bibcode :2009ApJS..184..138H . doi :10.1088/0067-0049/184/1/138 . S2CID 119267456 .