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HD 222582 b
太陽系外行星 来自维基百科,自由的百科全书
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HD 222582 b是一個質量超過木星7倍的太陽系外行星,母恆星是HD 222582。它的公轉週期是572日,軌道半長軸1.35天文單位,是目前已知軌道離心率最高的行星之一。
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參考資料
- Gimenez A. ubvy Photometry of stars with planets. Astronomy and Astrophysics. 2000, 356: 213 [2012-07-12]. Bibcode:2000A&A...356..213G. (原始內容存檔於2011-09-28).
- Han; Black, David C.; Gatewood, George. Preliminary astrometric masses for proposed exrasolar planetary companions. The Astrophysical Journal Letters. 2001, 548 (1): L57–L60. Bibcode:2001ApJ...548L..57H. doi:10.1086/318927.
- S.S. Vogt; et al. Six New Planets from the Keck Precision Velocity Survey. The Astrophysical Journal. 2000, 536 (2): 902–914. Bibcode:2000ApJ...536..902V. arXiv:astro-ph/9911506
. doi:10.1086/308981.
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外部連結
- Notes for planet HD 222582 b. The Extrasolar Planets Encyclopaedia. [2012-07-12]. (原始內容存檔於2012-06-01).
- HD 222582. Exoplanets. [2012-07-12]. (原始內容存檔於2010-03-17). Simulation
- Location. planetquest1.jpl.nasa.gov. [2012-07-12]. (原始內容存檔於2006-09-30).
- Curve. http://exoplanets.org. [2012-07-12]. (原始內容存檔於2008-09-25). 外部連結存在於
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(幫助) - Notes for planet HD 222582 b. www.astrocosmos.net. [2012-07-12]. (原始內容存檔於2012-12-09).
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