Binary star in the constellation Capricornus
Eta Capricorni , Latinized from η Capricorni, is a binary star [ 6] system in the southern constellation of Capricornus . It can be seen with the naked eye, having a combined apparent visual magnitude of +4.84.[ 2] Based upon an annual parallax shift of 20.20 mas as seen from the Earth,[ 1] the star is located about 161 light years from the Sun .
The pair orbit each other with a period of 27.85 years, a semimajor axis of 0.265 arc seconds , an eccentricity of 0.410.[ 6] The primary member, component A, is a white-hued A-type main sequence star with an apparent magnitude of +5.02.[ 3] Its companion, component B, has an apparent magnitude of +7.39.[ 3]
Nomenclature
η Capricorni (Latinised to Eta Capricorni ) is the system's Bayer designation . It also has the Flamsteed designation 22 Capricorni.
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 η Capricorni, φ Capricorni , ι Capricorni , 38 Capricorni , 35 Capricorni , 36 Capricorni , χ Capricorni , θ Capricorni , 30 Capricorni , 33 Capricorni , ζ Capricorni , 19 Capricorni , 26 Capricorni , 27 Capricorni , 20 Capricorni and 21 Capricorni .[ 8] Consequently, the Chinese name for η Capricorni itself is 周一 (Zhou yī , English: the First Star of Zhou ), meaning that this star (together with 21 Capricorni and β Serpentis in Right Wall of Heavenly Market Enclosure (asterism)[ 9] ) represent Zhou (周 ) (possibly Chow , the dynasty in China).[ 10]
Sometimes, this star is called by the name Armus in an astrological context.[ 11]
References
^ a b c d e f 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 .
^ a b c d Nicolet, B. (1978), "Catalogue of homogeneous data in the UBV photoelectric photometric system", Astronomy and Astrophysics , 34 : 1, Bibcode :1978A&AS...34....1N .
^ a b c 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 .
^ ten Brummelaar, Theo; et al. (May 2000), "Binary Star Differential Photometry Using the Adaptive Optics System at Mount Wilson Observatory", The Astronomical Journal , 119 (5): 2403–2414, Bibcode :2000AJ....119.2403T , doi :10.1086/301338 .
^ a b c 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 .
^ a b c d e Docobo, J. A.; Andrade, M. (2013), "Dynamical and physical properties of 22 binaries discovered by W. S. Finsen", Monthly Notices of the Royal Astronomical Society , 428 (1): 321–339, Bibcode :2013MNRAS.428..321D , doi :10.1093/mnras/sts045 .
^ "eta Cap" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-05-15 .{{cite web }}
: CS1 maint: postscript (link )
^ (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 .
^ "LacusCurtius • Allen's Star Names — Serpens" .
^ Allen, Richard Hinckley (1963), "Capricornus" , Star Names, Their Lore and Meaning , Dover, retrieved 2017-05-09 .
^ Armus , constellationsofwords.com, retrieved 2017-05-16 .