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Star in the constellation Capricornus
This article is about b Capricorni. Not to be confused with β Capricorni .
36 Capricorni is a single, yellow-hued star in the southern constellation of Capricornus . It is visible to the naked eye with an apparent visual magnitude of +4.50. The distance to this star, as determined from an annual parallax shift of 19.06±0.29 mas , is around 171 light years . It is currently moving closer with a heliocentric radial velocity of −21 km/s, and will come within 145 ly (44.58 pc) in about 685,000 years ago.
This is an evolved G-type giant star with a stellar classification of G7IIIb Fe–1, where the suffix notation indicates an underabundance of iron found in the spectrum . At the age of 770 million years it has become a red clump giant, meaning it is generating energy through helium fusion at its core . It has 2.26 times the mass of the Sun , but has expanded to 8.6 times its radius . It is radiating 43 times the Sun's luminosity from its photosphere at an effective temperature of 5,047 K.
Chinese name
In Chinese , 十二國 (Shíer Guó ), meaning Twelve States , refers to an asterism which is represent twelve ancient states in the Spring and Autumn period and the Warring States period , consisting of 36 Capricorni, φ Capricorni , ι Capricorni , 37 Capricorni , 35 Capricorni , χ Capricorni , θ Capricorni , 30 Capricorni , 33 Capricorni , ζ Capricorni , 19 Capricorni , 26 Capricorni , 27 Capricorni , 20 Capricorni , η Capricorni and 21 Capricorni . Consequently, 36 Capricorni itself is represent the state Jin (晉)(or Tsin ), together with κ Herculis in Right Wall of Heavenly Market Enclosure (asterism)
References
^ 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 , S2CID 18759600 .
^ Hekker, S.; et al. (August 2006), "Precise radial velocities of giant stars. I. Stable stars", Astronomy and Astrophysics , 454 (3): 943–949, arXiv :astro-ph/0604502 , Bibcode :2006A&A...454..943H , doi :10.1051/0004-6361:20064946 , S2CID 119529768 .
^ Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series , 71 : 245, Bibcode :1989ApJS...71..245K , doi :10.1086/191373 .
^ 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 .
Liu, Y. J.; et al. (2007), "The abundances of nearby red clump giants", Monthly Notices of the Royal Astronomical Society , 382 (2): 553–66, Bibcode :2007MNRAS.382..553L , doi :10.1111/j.1365-2966.2007.11852.x .
^ Gallenne, A.; Pietrzyński, G.; Graczyk, D.; Nardetto, N.; Mérand, A.; Kervella, P.; Gieren, W.; Villanova, S.; Mennickent, R. E.; Pilecki, B. (2018-08-01), "Fundamental properties of red-clump stars from long-baseline H-band interferometry", Astronomy & Astrophysics , 616 : A68, arXiv :1806.09572 , doi :10.1051/0004-6361/201833341 , ISSN 0004-6361
"24 Cap" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2018-06-15.
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 .
(in Chinese) 中國星座神話 , written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7 .
Ian Ridpath's Startales - Capricornus the Sea Goat
Richard Hinckley Allen: Star Names — Their Lore and Meaning: Capricornus
(in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 24 日 Archived 2011-05-22 at the Wayback Machine
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