This is a list of the coolest exoplanets known, specifically those with temperatures lower than −75 °C (198 K). Planets from the Solar System were also included for comparison for purposes.
Discovered in 2006, OGLE-2005-BLG-390Lb is the coldest known exoplanet, and was nicknamed "Hoth" by NASA in reference to the planet from the Star Wars franchise.[1]
↑Dong, Subo; Bond, I. A.; Gould, A.; Kozłowski, Szymon; Miyake, N.; Gaudi, B. S.; Bennett, D. P.; Abe, F. et al. (2009-06-04). "Microlensing Event Moa-2007-BLG-400: Exhuming the Buried Signature of a Cool, Jovian-Mass Planet". The Astrophysical Journal698 (2): 1826–1837. doi:10.1088/0004-637x/698/2/1826. ISSN0004-637X.
↑Grieves, N.; Bouchy, F.; Armstrong, D. J.; Akinsanmi, B.; Psaridi, A.; Ulmer-Moll, S.; Frensch, Y. G. C.; Helled, R. et al. (2025), "Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132", Astronomy & Astrophysics693: A144, doi:10.1051/0004-6361/202348177
↑ 13.013.113.2Giovinazzi, Mark R.; Blake, Cullen H.; Robertson, Paul; Lin, Andrea S. J.; Gupta, Arvind F.; Mahadevan, Suvrath; Fernandes, Rachel B.; Wright, Jason T. et al. (2025). "The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems". The Astronomical Journal170: 52. doi:10.3847/1538-3881/add922.
↑Dedrick, Cayla M.; Fulton, Benjamin J.; Knutson, Heather A.; Howard, Andrew W.; Beatty, Thomas G.; Cargile, Phillip A.; Gaudi, B. Scott; Hirsch, Lea A. et al. (2021-02-01). "Two Planets Straddling the Habitable Zone of the Nearby K Dwarf Gl 414A". The Astronomical Journal161 (2): 86. doi:10.3847/1538-3881/abd0ef. ISSN0004-6256. Bibcode: 2021AJ....161...86D.
↑Chachan, Yayaati; Dalba, Paul A.; Knutson, Heather A.; Fulton, Benjamin J.; Thorngren, Daniel; Beichman, Charles; Ciardi, David R.; Howard, Andrew W. et al. (2022-02-01). "Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths". The Astrophysical Journal926 (1): 62. doi:10.3847/1538-4357/ac3ed6. ISSN0004-637X. Bibcode: 2022ApJ...926...62C.
↑Maciejewski, G. et al. (July 2024). "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N VIII. A wide-orbit planetary companion in the hot-Jupiter system HD 118203". Astronomy & Astrophysics. doi:10.1051/0004-6361/202451084.
↑Moutou, C.; Ould-Elhkim, M.; Donati, J.-F.; Charpentier, P.; Cadieux, C.; Delfosse, X.; Artigau, E.; Arnold, L. et al. (14 June 2024). "Characterising planetary systems with SPIRou: Temperate sub-Neptune exoplanet orbiting the nearby fully convective star GJ 1289 and a candidate around GJ 3378". Astronomy & Astrophysics688: A196. doi:10.1051/0004-6361/202450466. Bibcode: 2024A&A...688A.196M.
↑Fulton, Benjamin J.; Howard, Andrew W.; Weiss, Lauren M.; Sinukoff, Evan; Petigura, Erik A.; Isaacson, Howard; Hirsch, Lea; Marcy, Geoffrey W. et al. (2016-10-10). "Three Temperate Neptunes Orbiting Nearby Stars". The Astrophysical Journal830 (1): 46. doi:10.3847/0004-637x/830/1/46. ISSN1538-4357. Bibcode: 2016ApJ...830...46F.
↑Dreizler, S.; Luque, R.; Ribas, I.; Koseleva, V.; Ruh, H. L.; Nagel, E.; Pozuelos, F. J.; Zechmeister, M. et al. (2024-02-01), Teegarden's Star revisited: A nearby planetary system with at least three planets
↑Blunt, Sarah; Endl, Michael; Weiss, Lauren M.; Cochran, William D.; Howard, Andrew W.; MacQueen, Phillip J.; Fulton, Benjamin J.; Henry, Gregory W. et al. (2019-11-01). "Radial Velocity Discovery of an Eccentric Jovian World Orbiting at 18 au". The Astronomical Journal158 (5): 181. doi:10.3847/1538-3881/ab3e63. ISSN0004-6256. Bibcode: 2019AJ....158..181B.
↑ 27.027.1Ducrot, Elsa; Gillon, M.; Delrez, L.; Agol, E.; Rimmer, P.; Turbet, M.; Günther, M. N.; Demory, B.-O. et al. (August 2020). "TRAPPIST-1: Global Results of the Spitzer Exploration Science Program {\it Red Worlds}". Astronomy & Astrophysics640: A112. doi:10.1051/0004-6361/201937392. ISSN0004-6361.
↑Kunimoto, Michelle; Vanderburg, Andrew; Huang, Chelsea X.; Davis, M. Ryleigh; Affer, Laura; Cameron, Andrew Collier; Charbonneau, David; Cosentino, Rosario et al. (2023-07-01). "TOI-4010: A System of Three Large Short-period Planets with a Massive Long-period Companion". The Astronomical Journal166 (1): 7. doi:10.3847/1538-3881/acd537. ISSN0004-6256. Bibcode: 2023AJ....166....7K.
↑Sarkis, P.; Henning, Th.; Hartman, J. D.; Bakos, G. Á.; Brahm, R.; Jordán, A.; Bayliss, D.; Mancini, L. et al. (2018-11-01). "HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet around a Sun-like Star". The Astronomical Journal156 (5): 216. doi:10.3847/1538-3881/aade54. ISSN0004-6256. Bibcode: 2018AJ....156..216S.
↑Teske, Johanna; Díaz, Matías R.; Luque, Rafael; Močnik, Teo; Seidel, Julia V.; Otegi, Jon Fernández; Feng, Fabo; Jenkins, James S. et al. (2020-08-01). "TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet". The Astronomical Journal160 (2): 96. doi:10.3847/1538-3881/ab9f95. ISSN0004-6256. Bibcode: 2020AJ....160...96T.
↑Pepe, F.; Lovis, C.; Ségransan, D.; Benz, W.; Bouchy, F.; Dumusque, X.; Mayor, M.; Queloz, D. et al. (2011-10-01). "The HARPS search for Earth-like planets in the habitable zone. I. Very low-mass planets around HD 20794, HD 85512, and HD 192310". Astronomy and Astrophysics534: A58. doi:10.1051/0004-6361/201117055. ISSN0004-6361. Bibcode: 2011A&A...534A..58P.
↑ 36.036.1Mary Anne Limbach; Vanderburg, Andrew; MacDonald, Ryan J.; Stevenson, Kevin B.; Jenkins, Sydney; Blouin, Simon; Rauscher, Emily; Bowens-Rubin, Rachel; Gallo, Elena; Mang, James; Morley, Caroline V.; Sing, David K.; O'Connor, Christopher; Venner, Alexander; Xu, Siyi (2025). "Thermal Emission and Confirmation of the Frigid White Dwarf Exoplanet WD 1856+534b". arXiv:2504.16982 [astro-ph.EP].
↑Doyle, Laurance R.; Carter, Joshua A.; Fabrycky, Daniel C.; Slawson, Robert W.; Howell, Steve B.; Winn, Joshua N.; Orosz, Jerome A.; Prsa, Andrej et al. (2011-09-16). "Kepler-16: A Transiting Circumbinary Planet". Science333 (6049): 1602–1606. doi:10.1126/science.1210923. ISSN0036-8075. PMID21921192. Bibcode: 2011Sci...333.1602D.
↑Quintana, Elisa V.; Barclay, Thomas; Raymond, Sean N.; Rowe, Jason F.; Bolmont, Emeline; Caldwell, Douglas A.; Howell, Steve B.; Kane, Stephen R. et al. (2014-04-18). "An Earth-sized Planet in the Habitable Zone of a Cool Star". Science344 (6181): 277–280. doi:10.1126/science.1249403. ISSN0036-8075. PMID24744370. Bibcode: 2014Sci...344..277Q.
↑Mireles, Ismael; Dragomir, Diana; Osborn, Hugh P.; Hesse, Katharine; Collins, Karen A.; Villanueva, Steven; Bieryla, Allyson; Ciardi, David R. et al. (2023-09-01). "TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf". The Astrophysical Journal954 (1): L15. doi:10.3847/2041-8213/aceb69. ISSN0004-637X. Bibcode: 2023ApJ...954L..15M.
↑Teff: Measured effective temperature.
Teq: The temperature of the planet has not been measured, so it is listed with the calculated equilibrium temperature.
↑The melting points of elemental Nitrogen and Oxygen at 1 bar pressure are -210 °C and -218 °C, respectively.[2][3]
↑This was obtained using the CalcTool luminosity converter. Using the apparent magnitude of HIP 11915 and its distance from Earth (using the uncertainty parameter of ±10 light years), this yields a range of 1.03–1.27 L☉. When used in the default 190 light-year distance (with margin of error) is 1.07+0.11 −0.09L☉. When run into simulations using the orbital distance of HIP 11915 and its planet, yields a result of 118 K.
↑This is the surface temperature if GJ 1002 c has no atmosphere.
↑This is the surface temperature if Kepler-186f has no atmosphere.
↑This is the surface temperature if TRAPPIST-1g has no atmosphere.
↑The age is the same as the globular cluster where PSR B1620-26b is located (Messier 4), as all the stars in the cluster formed at the same time, and the planets form together with their host stars.