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^ Sharp, A. G.; Moses, J. I.; Friedson, A. J.; Fegley, B.; Marley, M. S.; Lodders, K. (2004). ⇒“Predicting the Atmospheric Composition of Extrasolar Giant Planets”. 35th Lunar and Planetary Science Conference (Lunar and Planetary Science Conference) 35: 1152. Bibcode: 2004LPI....35.1152S. ⇒http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1152.pdf
^ Darling, David. “epistellar jovians”. The Internet Encyclopedia of Science. 2019年4月4日閲覧。
^ .mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation.cs-ja1 q,.mw-parser-output .citation.cs-ja2 q{quotes:"「""」""『""』"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free a,.mw-parser-output .citation .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited a,.mw-parser-output .id-lock-registration a,.mw-parser-output .citation .cs1-lock-limited a,.mw-parser-output .citation .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription a,.mw-parser-output .citation .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:#d33}.mw-parser-output .cs1-visible-error{color:#d33}.mw-parser-output .cs1-maint{display:none;color:#3a3;margin-left:0.3em}.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit} ⇒"Interiors of extrasolar planets: A first step" (PDF) (Press release). Astronomy & Astrophysics. 30 May 2006. 2019年4月4日閲覧。
^ Than, Ker (2006年6月5日). “ ⇒Inside Exoplanets: Motley Crew of Worlds Share Common Thread”. Space.com. 2019年4月4日閲覧。
^ “ ⇒天文学辞典 ≫ 灼熱巨大惑星”. 天文学辞典. 日本天文学会. 2019年2月14日閲覧。
^ a b c 井田茂 2016, p. 8-9.
^ 井田茂 2016, p. 24-25.
^ “ ⇒Hot Jupiter with hidden Water”. spacetelescope.org. ESA/Hubble. 2017年1月6日閲覧。
^ a b c d e f Winn, Joshua N.; Fabrycky, Daniel; Albrecht, Simon; Johnson, John Asher (2010-01-01). ⇒“Hot Stars with Hot Jupiters Have High Obliquities” (英語). The Astrophysical Journal Letters 718 (2): L145. arXiv:1006.4161. Bibcode: 2010ApJ...718L.145W. doi:10.1088/2041-8205/718/2/L145. ISSN 2041-8205. ⇒http://stacks.iop.org/2041-8205/718/i=2/a=L145
^ Chauvin, G. et al. (2005). “A companion to AB Pic at the planet/brown dwarf boundary”. Astronomy and Astrophysics 438 (3): L29-L32. arXiv:astro-ph/0504658. doi:10.1051/0004-6361:200500111. ISSN 0004-6361. 
^ a b Fabrycky, D.; Tremaine, S. (2007-11-10). “Shrinking Binary and Planetary Orbits by Kozai Cycles with Tidal Friction”. Astrophysical Journal 669 (2): 1298-1315. arXiv:0705.4285. Bibcode: 2007ApJ...669.1298F. doi:10.1086/521702. 
^ a b c Mandushev, Georgi et al. (2007). “TrES-4: A Transiting Hot Jupiter of Very Low Density”. The Astrophysical Journal 667 (2): L195-L198. arXiv:0708.0834v1. Bibcode: 2007ApJ...667L.195M. doi:10.1086/522115. ISSN 0004-637X. 
^ Zhou, G.; Bakos, G. A.; Hartman, J. D.; Latham, D. W.; Torres, G.; Bhatti, W.; Penev, K.; Buchhave, L. et al. (2017). “HAT-P-67b: An Extremely Low Density Saturn Transiting an F-subgiant Confirmed via Doppler Tomography”. The Astronomical Journal 153 (5): 211. arXiv:1702.00106. Bibcode: 2017AJ....153..211Z. doi:10.3847/1538-3881/aa674a. ISSN 1538-3881. 
^ a b c d Baraffe, I; Chabrier, G; Barman, T (2010). “The physical properties of extra-solar planets”. Reports on Progress in Physics 73 (1): 016901. arXiv:1001.3577. Bibcode: 2010RPPh...73a6901B. doi:10.1088/0034-4885/73/1/016901. ISSN 0034-4885. 
^ a b c d Burrows, A.; Hubeny, I.; Budaj, J.; Hubbard, W. B. (2007). “Possible Solutions to the Radius Anomalies of Transiting Giant Planets”. The Astrophysical Journal 661 (1): 502?514. arXiv:astro-ph/0612703. Bibcode: 2007ApJ...661..502B. doi:10.1086/514326. ISSN 0004-637X. 
^ Michelle Starr (2018年4月23日). “Astronomers Just Found a 'Hot Jupiter' So Dark, It Absorbs Nearly 99% of Light”. sciencealert. 2019年4月4日閲覧。
^ Cooper, Curtis S.; Showman, Adam P. (2005-01-01). ⇒“Dynamic Meteorology at the Photosphere of HD 209458b” (英語). The Astrophysical Journal Letters 629 (1): L45. arXiv:astro-ph/0502476. Bibcode: 2005ApJ...629L..45C. doi:10.1086/444354. ISSN 1538-4357. ⇒http://stacks.iop.org/1538-4357/629/i=1/a=L45
^ a b Rauscher, Emily; Menou, Kristen (2010-01-01). ⇒“Three-dimensional Modeling of Hot Jupiter Atmospheric Flows” (英語). The Astrophysical Journal 714 (2): 1334?1342. arXiv:0907.2692. Bibcode: 2010ApJ...714.1334R. doi:10.1088/0004-637X/714/2/1334. ISSN 0004-637X. ⇒http://stacks.iop.org/0004-637X/714/i=2/a=1334
^ Wittenmyer, R. A. et al. (2020). “Cool Jupiters greatly outnumber their toasty siblings: occurrence rates from the Anglo-Australian Planet Search”. MNRAS 492: 377. Bibcode: 2020MNRAS.492..377W. doi:10.1093/mnras/stz3436. 

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