HD 92063 – Wikipedia

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Star in the constellation Carina

This article is about t1 Carinae. For t2 Carinae, see HD 92397.

HD 92063 is a single[8]star in the southern constellation of Carina. It has the Bayer designation t1 Carinae, while HD 92063 is the star’s identifier from the Henry Draper Catalogue. This is a suspected variable star[4] and is visible to the naked eye with an apparent visual magnitude of 5.08.[2] The star is located at a distance of approximately 246 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −10 km/s.[1] Although it appears at the edge of the Carina Nebula, it is much closer than the nebula. It is also not considered a member of the nearby Alessi 5 open cluster of stars.[9]

This is an aging K-type giant star with a stellar classification of K1III,[3] having exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence. At present it has 14[1] times the radius of the Sun. The star is radiating 72[1] times the Sun’s luminosity from its enlarged photosphere at an effective temperature of 4,520 K.[1]

References[edit]

  1. ^ a b c d e f g h i j k l m 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.
  2. ^ a b c d 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.
  3. ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1975mcts.book…..H.
  4. ^ a b Samus’, N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N (2017), “General catalogue of variable stars: Version GCVS 5.1”, Astronomy Reports, 61 (1): 80, Bibcode:2017ARep…61…80S, doi:10.1134/S1063772917010085, S2CID 125853869.
  5. ^ a b c Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019), “Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18”, Astronomy and Astrophysics, 628: A94, arXiv:1904.11302, Bibcode:2019A&A…628A..94A, doi:10.1051/0004-6361/201935765, S2CID 131780028.
  6. ^ 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.
  7. ^ “HD 92063”. SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-12.
  8. ^ 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  9. ^ Cantat-Gaudin, T.; et al. (July 2018), “Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution”, Astronomy & Astrophysics, 615: 15, arXiv:1801.10042, Bibcode:2018A&A…615A..49C, doi:10.1051/0004-6361/201731251, S2CID 56324345, A49.

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