HD 176051,又名BD+32 3267,SAO 67612、HR 7162,是一個天琴座的光譜聯星系統[1][2],视星等为5.22,位于銀經63.35,銀緯13.27,其B1900.0坐标为赤經18h 53m 16.6s,赤緯+32° 13.27′ 23″。距離地球約49光年。該聯星系統的週期是22,423日(61.4日),軌道離心率0.25[10]。相較於太陽,這兩顆恆星的金屬量較低[8],兩顆恆星的質量分別是1.07和0.71倍太陽質量[5]。
行星系統
該行星的母恆星是聯星。行星的各項參數是來自質量為0.71倍太陽質量的伴星(Muterspaugh et al. 2010)。如果該行星環繞質量是1.07倍太陽質量的主星,該行星質量是2.26倍木星質量,軌道半長軸2.02天文單位。
参考文献
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- ^ 4.0 4.1 Simbad Query Result: HD 176051 -- Spectroscopic binary. Simbad. Centre de Données astronomiques de Strasbourg. [2009-05-07]. (原始内容存档于2020-02-01).
- ^ 5.0 5.1 5.2 Muterspaugh, Matthew W.; et al. Limits to tertiary astrometric companions in binary systems. The Astrophysical Journal. 2006, 653 (2): 1469–1479. Bibcode:2006ApJ...653.1469M. S2CID 15218103. arXiv:astro-ph/0608640 . doi:10.1086/508743.
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- ^ Wilson, R. E. General Catalogue of Stellar Radial Velocities. Carnegie Institute Washington D.C. Publication (Washington D.C.: Carnegie Institute). 1953. Bibcode:1953GCRV..C......0W.
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- ^ Pourbaix, D.; et al, SB9: The Ninth Catalogue of Spectroscopic Binary Orbits, Astronomy & Astrophysics, 2004, 424: 727–732, Bibcode:2004A&A...424..727P, S2CID 119387088, arXiv:astro-ph/0406573 , doi:10.1051/0004-6361:20041213. VizierR (obsoleted) (页面存档备份,存于互联网档案馆)
- ^ Schneider, J. Notes for star HD 176051 b. The Extrasolar Planets Encyclopaedia. [2010-10-22]. (原始内容存档于2012-01-20).