ケプラー25
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2020/03/17 08:41 UTC 版)
ケプラー25 (英: Kepler-25) とは、こと座の方向に約799光年離れた場所に存在する恒星である[9]。太陽よりもわずかに大きくて重く、光度は太陽の2.4倍。見かけの等級は10.6で、肉眼で見ることは出来ない[1]。
注釈
出典
- ^ a b Henden, A. A. et al. (2016). “VizieR Online Data Catalog: AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)”. VizieR On-line Data Catalog: II/336. Originally Published in: 2015AAS...22533616H 2336. Bibcode: 2016yCat.2336....0H. Vizier catalog entry
- ^ a b c d 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.
- ^ a b c d e Silva Aguirre, V. et al. (2015). “Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology”. Monthly Notices of the Royal Astronomical Society 452 (2): 2127–2148. arXiv:1504.07992. Bibcode: 2015MNRAS.452.2127S. doi:10.1093/mnras/stv1388.
- ^ a b Marcy, Geoffrey W. et al. (2014). “Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets”. The Astrophysical Journal Supplement Series 210 (2): 20. arXiv:1401.4195. Bibcode: 2014ApJS..210...20M. doi:10.1088/0067-0049/210/2/20.
- ^ McQuillan, A.; Mazeh, T.; Aigrain, S. (2013). “Stellar Rotation Periods of The Kepler objects of Interest: A Dearth of Close-In Planets Around Fast Rotators”. The Astrophysical Journal Letters 775 (1): L11. arXiv:1308.1845. Bibcode: 2013ApJ...775L..11M. doi:10.1088/2041-8205/775/1/L11.
- ^ a b Schneider, Jean, Star: Kepler-25, Paris Observatory, オリジナルの2012-06-16時点におけるアーカイブ。 2013年12月18日閲覧。
- ^ a b Huber, Daniel et al. (2013). “Fundamental Properties of Kepler Planet-candidate Host Stars using Asteroseismology”. The Astrophysical Journal 767 (2): 127. arXiv:1302.2624. Bibcode: 2013ApJ...767..127H. doi:10.1088/0004-637X/767/2/127.
- ^ "Kepler-25". SIMBAD. Centre de données astronomiques de Strasbourg. 2019年10月2日閲覧。
- ^ Roman, Nancy G. (1987). “Identification of a Constellation From a Position”. Publications of the Astronomical Society of the Pacific 99 (617): 695–699. Bibcode: 1987PASP...99..695R. doi:10.1086/132034. Vizier query form
- ^ Borucki, William J. et al. (2011). “Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data”. The Astrophysical Journal 736 (1): 19. arXiv:1102.0541. Bibcode: 2011ApJ...736...19B. doi:10.1088/0004-637X/736/1/19.
- ^ Steffen, Jason H. et al. (2012). “Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations”. Monthly Notices of the Royal Astronomical Society 421 (3): 2342–2354. arXiv:1201.5412. Bibcode: 2012MNRAS.421.2342S. doi:10.1111/j.1365-2966.2012.20467.x.
- ^ Mills, Sean M. et al. (2019). “Long-period Giant Companions to Three Compact, Multiplanet Systems”. The Astronomical Journal 157 (4): 145. arXiv:1903.07186. Bibcode: 2019AJ....157..145M. doi:10.3847/1538-3881/ab0899.
[続きの解説]
「ケプラー25」の続きの解説一覧
- 1 ケプラー25とは
- 2 ケプラー25の概要
- 3 惑星系 
- 4 関連項目
- ケプラー25のページへのリンク
