This is a list of the hottest exoplanets so far discovered, specifically those with temperatures greater than 2500 K (2230 °C; 4040 °F) for exoplanets irradiated by a nearby star and greater than 2000 K (1730 °C; 3140 °F) for self-luminous exoplanets. For comparison, the hottest planet in the Solar System is Venus, with a temperature of 737 K (464 °C; 867 °F).
This planet is so close to its parent star that its tidal forces are distorting it into an egg shape. First planet observed being consumed by its host star;[13] it will be destroyed in 3.16 ± 0.10 Ma due to tidal interactions.[14][15]
A glory effect in the atmosphere of WASP-76b might be responsible for the observed increase in brightness of its eastern terminator zone which if confirmed, it would become the first exoplanet to have its glory-like phenomenon to be discovered.[23][24]
Represents multiple milestones in exoplanetary discovery, such as the first exoplanet known observed to transit its host star, the first exoplanet with a precisely measured radius, one of first two exoplanets (other being HD 189733 Ab) to be observed spectroscopically[41][42] and the first to have an atmosphere detected, containing evaporating hydrogen, and oxygen and carbon. First extrasolar gas giant to have its superstorm measured.[43] Also first (indirect) detection of a magnetic field on an exoplanet.[44] Nicknamed "Osiris".
First exoplanet to have its rotation rate measured[56] and fastest-spinning planet discovered at the equator speed of 19.9 ± 1.0 km/s (12.37 ± 0.62 mi/s) or 71,640 ± 3,600 km/h (44,520 ± 2,240 mph).[57]
↑Pai Asnodkar, Anusha; Wang 王, Ji 吉; Gaudi, B. Scott; Cauley, P. Wilson; Eastman, Jason D.; Ilyin, Ilya; Strassmeier, Klaus; Beatty, Thomas (2022-02-01). "KELT-9 as an Eclipsing Double-lined Spectroscopic Binary: A Unique and Self-consistent Solution to the System". The Astronomical Journal163 (2): 40. doi:10.3847/1538-3881/ac32c7. ISSN0004-6256. Bibcode: 2022AJ....163...40P.
↑ 5.05.1Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike et al. (August 2024). "BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?". Astronomy & Astrophysics688: A120. doi:10.1051/0004-6361/202349028. ISSN0004-6361.
↑Owens, Niall et al. (May 2021). "Phase curve and variability analysis of WASP-12b using TESS photometry". Monthly Notices of the Royal Astronomical Society: Letters503 (1): L38–L46. doi:10.1093/mnrasl/slab014. Bibcode: 2021MNRAS.503L..38O.
↑Collins, Karen A; Kielkopf, John F; Stassun, Keivan G (2017). "Transit Timing Variation Measurements of WASP-12b and Qatar-1b: No Evidence for Additional Planets". The Astronomical Journal153 (2): 78. doi:10.3847/1538-3881/153/2/78. Bibcode: 2017AJ....153...78C.
↑Wong, Ian; Shporer, Avi; Vissapragada, Shreyas; Greklek-McKeon, Michael; Knutson, Heather A.; Winn, Joshua N.; Benneke, Björn (20 January 2022). "TESS Revisits WASP-12: Updated Orbital Decay Rate and Constraints on Atmospheric Variability". The Astronomical Journal163 (4): 175. doi:10.3847/1538-3881/ac5680. Bibcode: 2022AJ....163..175W.
↑von Essen, C.; Mallonn, M.; Borre, C. C.; Antoci, V.; Stassun, K. G.; Khalafinejad, S.; Tautvaivsiene, G. (2020). "TESS unveils the phase curve of WASP-33b. Characterization of the planetary atmosphere and the pulsations from the star". Astronomy & AstrophysicsA34: 639. doi:10.1051/0004-6361/202037905. Bibcode: 2020A&A...639A..34V.
↑Wong, Ian; Knutson, Heather A.; Kataria, Tiffany; Lewis, Nikole K.; Burrows, Adam; Fortney, Jonathan J.; Schwartz, Joel; Shporer, Avi et al. (2016-06-01). "3.6 and 4.5 μm Spitzer Phase Curves of the Highly Irradiated Hot Jupiters WASP-19b and HAT-P-7b". The Astrophysical Journal823 (2): 122. doi:10.3847/0004-637X/823/2/122. ISSN0004-637X. Bibcode: 2016ApJ...823..122W.
↑ 26.026.126.226.3Bonomo, A. S.; Desidera, S.; Benatti, S.; Borsa, F.; Crespi, S.; Damasso, M.; Lanza, A. F.; Sozzetti, A. et al. (June 2017). "The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy & Astrophysics602: A107. doi:10.1051/0004-6361/201629882. ISSN0004-6361. Bibcode: 2017A&A...602A.107B.
↑Esteves, Lisa J.; Mooij, Ernst J. W. De; Jayawardhana, Ray (2015). "Changing Phases of Alien Worlds: Probing Atmospheres Of Kepler planets with High-Precision Photometry". The Astrophysical Journal804 (2). doi:10.1088/0004-637X/804/2/150. Bibcode: 2015ApJ...804..150E.
↑Borucki, William J. et al. (2011). "Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data". The Astrophysical Journal736 (1). doi:10.1088/0004-637X/736/1/19. Bibcode: 2011ApJ...736...19B.
↑Esteves, Lisa J.; De Mooij, Ernst J. W.; Jayawardhana, Ray (2015-05-12). "Changing Phases of Alien Worlds: Probing Atmospheres of Kepler Planets with High-Precision Photometry". The Astrophysical Journal804 (2): 150. doi:10.1088/0004-637X/804/2/150. ISSN1538-4357. Bibcode: 2015ApJ...804..150E.
↑Brinkman, Casey L.; Weiss, Lauren M.; Huber, Daniel; Lee, Rena A.; Kolecki, Jared; Tenn, Gwyneth; Zhang, Jingwen; Narayanan, Suchitra et al. (2024-09-30). "The Compositions of Rocky Planets in Close-in Orbits Tend to be Earth-Like". The Astronomical Journal170 (2): 109. doi:10.3847/1538-3881/ade677. Bibcode: 2025AJ....170..109B.
↑Stassun, Keivan G.; Collins, Karen A.; Gaudi, B. Scott (2017-03-01). "Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes". The Astronomical Journal153 (3): 136. doi:10.3847/1538-3881/aa5df3. ISSN0004-6256. Bibcode: 2017AJ....153..136S.
↑Piskorz, Danielle; Benneke, Björn; Crockett, Nathan R.; Lockwood, Alexandra C.; Blake, Geoffrey A.; Barman, Travis S.; Bender, Chad F.; Carr, John S. et al. (2017-08-01). "Detection of Water Vapor in the Thermal Spectrum of the Non-transiting Hot Jupiter Upsilon Andromedae b". The Astronomical Journal154 (2): 78. doi:10.3847/1538-3881/aa7dd8. ISSN1538-3881. Bibcode: 2017AJ....154...78P.
↑Harrington, J.; Hansen, B.; Luszcz, S.; Seager, S.; Deming, D.; Menou, K.; Cho, J.; Richardson, L. J. (2006-10-27). "The phase-dependent Infrared brightness of the extrasolar planet upsilon Andromedae b". Science314 (5799): 623–626. doi:10.1126/science.1133904. ISSN0036-8075. PMID17038587. Bibcode: 2006Sci...314..623H.
↑Anderson, D. R.; Hellier, C.; Gillon, M.; Triaud, A. H. M. J.; Smalley, B.; Hebb, L.; Cameron, A. Collier; Maxted, P. F. L. et al. (2010-01-20). "WASP-17b: an ultra-low density planet in a probable retrograde orbit". The Astrophysical Journal709 (1): 159–167. doi:10.1088/0004-637X/709/1/159. ISSN0004-637X. Bibcode: 2010ApJ...709..159A.
↑Zellem, Robert T.; Lewis, Nikole K.; Knutson, Heather A.; Griffith, Caitlin A.; Showman, Adam P.; Fortney, Jonathan J.; Cowan, Nicolas B.; Agol, Eric et al. (2014-07-02). "The 4.5 μm full-orbit phase curve of the hot Jupiter HD 209458b". The Astrophysical Journal790 (1): 53. doi:10.1088/0004-637X/790/1/53. ISSN0004-637X. Bibcode: 2014ApJ...790...53Z.
↑Kislyakova, K. G.; Holmstrom, M.; Lammer, H.; Odert, P.; Khodachenko, M. L. (2014). "Magnetic moment and plasma environment of HD 209458b as determined from Ly observations". Science346 (6212): 981–4. doi:10.1126/science.1257829. PMID25414310. Bibcode: 2014Sci...346..981K.
↑ 45.045.1Öztürk, Oǧuz; Erdem, Ahmet (2019-06-01). "New photometric analysis of five exoplanets: CoRoT-2b, HAT-P-12b, TrES-2b, WASP-12b, and WASP-52b". Monthly Notices of the Royal Astronomical Society486 (2): 2290–2307. doi:10.1093/mnras/stz747. ISSN0035-8711. Bibcode: 2019MNRAS.486.2290O.
↑Martins, J. H. C; Santos, N. C; Figueira, P; Faria, J. P; Montalto, M; Boisse, I; Ehrenreich, D; Lovis, C et al. (2015). "Evidence for a spectroscopic direct detection of reflected light from 51 Pegasi b". Astronomy & Astrophysics576: A134. doi:10.1051/0004-6361/201425298. Bibcode: 2015A&A...576A.134M.
↑Chilcote, Jeffrey; Pueyo, Laurent; Rosa, Robert J. De; Vargas, Jeffrey; Macintosh, Bruce; Bailey, Vanessa P.; Barman, Travis; Bauman, Brian et al. (2017-03-28). "1–2.4μm Near-IR Spectrum of the Giant PlanetβPictoris b Obtained with the Gemini Planet Imager". The Astronomical Journal153 (4): 182. doi:10.3847/1538-3881/aa63e9. ISSN1538-3881. Bibcode: 2017AJ....153..182C.
↑Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A. et al. (2022-09-01). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series262 (1): 21. doi:10.3847/1538-4365/ac7e57. ISSN0067-0049. Bibcode: 2022ApJS..262...21F.
↑Hurt, Spencer A.; Quinn, Samuel N.; Latham, David W.; Vanderburg, Andrew; Esquerdo, Gilbert A.; Calkins, Michael L.; Berlind, Perry; Angus, Ruth et al. (2021-04-01). "A decade of radial-velocity monitoring of Vega and new limits on the presence of planets". The Astronomical Journal161 (4): 157. doi:10.3847/1538-3881/abdec8. ISSN0004-6256. Bibcode: 2021AJ....161..157H.