List of hottest exoplanets
Appearance
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).
List of hottest exoplanets irradiated by a nearby star
[edit]Methods for finding temperature:
- Teff: Measured effective temperature.
- Teq: The temperature of the planet has not been measured, so it is listed with the calculated equilibrium temperature.
Image
(Or artistic representation) |
Name | Temperature (K) | Mass | Method | Notes |
---|---|---|---|---|---|
![]() |
KELT-9b | 4643±26[1] | 2.17±0.56 MJ[2] | Teff | Hottest known exoplanet, with a temperature comparable to K-type stars. |
![]() |
55 Cancri e (Janssen) | 3771+669 −520[3] |
7.99 M🜨[3] | Hottest confirmed rocky exoplanet. | |
![]() |
TOI-2109b | 3631±69[4] | 5.02±0.75 MJ[4] | Has the shortest orbital period among the hot Jupiters in 0.6725 days (16.14 hours).[4] | |
BD-14 3065b | 3520±130[5] | 12.37±0.92 MJ[5] | |||
WASP-189b | 3435±27[6] | 1.99+0.16 −0.14 MJ[6] |
|||
TOI-1518b | 3237±59[7] | <2.3 MJ[7] | |||
![]() |
WASP-103b | 3205±136[8] | 1.455+0.090 −0.091 MJ[8] |
First exoplanet to have a deformation detected.[9] (see Jacobi ellipsoid) | |
KELT-16b | 3190±61[10] | 2.75 MJ[10] | |||
![]() |
WASP-12b | 3128±66[11] | 1.476+0.076 −0.069 MJ[12] |
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] | |
![]() |
WASP-33b | 3108±113[8] | 2.81±0.53 MJ[16] | First planet discovered to orbit a Delta Scuti variable star | |
![]() |
WASP-18b | 3067±104[8] | 10.20±0.35 MJ[8] | ||
MASCARA-1b | 3062±67[17] | 3.7 MJ[17] | |||
HATS-70b | 2730+140 −160[18] |
12.9 MJ[18] | Teq | ||
WASP-100b | 2710[19] | 2.03 MJ[19] | Teff | ||
MASCARA-5b | 2700[20] | 3.12 MJ[20] | |||
![]() |
WASP-76b | 2670 (dayside)[21] | 0.92±0.032 MJ[22] | 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] | |
![]() |
HAT-P-7b | 2667±57[25] | 1.806±0.036 MJ[26] | First exoplanet to have a crude map of cloud coverage | |
TOI-2260 b | 2609±86[18] | 0.011 +0.0079 −0.0041 MJ[27] |
Teq | ||
HAT-P-70b | 2562+43 −52[18] |
6.78 MJ[18] | Teq | ||
![]() |
Kepler-13b | 2550±80 (2277 °C)[18] | 9.28(16) MJ[28] | Discovered by Kepler in first four months of Kepler data.[29] | |
The following well-known planets are listed for the purpose of comparison. | |||||
![]() |
Kepler-10b | 2130+60 −120 (1857 °C)[30] |
3.58±0.33 M🜨[31] | Teq | First confirmed terrestrial planet to have been discovered outside the Solar System |
![]() |
TrES-4b | 1782±29 (1509 °C)[32] | 0.78±0.19 MJ[33] | Largest confirmed exoplanet ever found at the time of discovery.[34] This planet has a density of 0.17 g/cm3, comparable to that of balsa wood, less than Saturn's 0.7 g/cm3.[35] | |
![]() |
CoRoT-7b | 1756±27 (1483 °C)[36] | 5.74 M🜨[36] | Smallest exoplanet to have its diameter measured at the time of discovery and first potential extrasolar terrestrial planet to be found. | |
![]() |
Upsilon Andromedae b (Saffar) | 1673 (1400 °C)[37] | 1.70+0.33 −0.24 MJ[38] |
Teff | First multiple-planet system to be discovered around a main-sequence star, and first multiple-planet system known in a multiple-star system. |
![]() |
WASP-17b (Ditsö̀) | 1550+170 −200 (1277 °C)[26] |
0.512±0.037 MJ[26] | With a density of about 0.08 g/cm3,[39] it is one of the puffiest exoplanets known. | |
![]() |
HD 209458 b ("Osiris") | 1499±15 (1226 °C)[40] | 0.682+0.014 −0.015 MJ[26] |
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". | |
![]() |
TrES-2b | 1466±9 (1193 °C)[45] | 1.253 MJ[45] | Teq | The darkest exoplanet known, reflecting less than 1% its star's light. |
![]() |
51 Pegasi b (Dimidium) | 1265 (992 °C) | 0.46+0.06 −0.01 MJ[46] |
Teq | The first exoplanet discovered orbiting a main-sequence star. |
![]() |
Kepler-20e | 1004±14 (735 °C)[47] | <0.76 M🜨[47] | The first planet smaller than Earth discovered after PSR B1257+12 b. | |
![]() |
Venus (for reference) | 735 (462 °C)[48] | 0.815 M🜨[48] | Hottest planet in the Solar System. |
List of hottest self-luminous exoplanets
[edit]All these are measured temperatures.
Image (Or artistic representation) |
Name | Temperature (K) |
Mass (MJ) |
Notes |
---|---|---|---|---|
HIP 78530 b | 2700±100[49] | 28 ± 10[50] | Likely a brown dwarf. | |
![]() |
GQ Lupi b | 2650±100[51] | ~ 20 (1 – 39)[51] | Likely a brown dwarf. First confirmed exoplanet candidate to be directly imaged. |
![]() |
CT Chamaelontis b (CT Cha b) |
2600±250[52] | 17 ± 6[52] | Likely a brown dwarf. Furthest planet to be directly imaged at the distance of 622 ly (190.71 pc). |
![]() |
DH Tauri b | 2400±100[53] | 11 ± 3[53] | First planet to have a confirmed circumplanetary disk[54] and youngest confirmed planet at an age of 0.7 Myr.[55] |
The following well-known planets are listed for the purpose of comparison. | ||||
![]() |
Beta Pictoris b | 1724±15 (1451 °C)[56] | 11.729 +2.337 −2.135[57] |
First exoplanet to have its rotation rate measured[58] 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).[59] |
Unconfirmed candidates
[edit]These planet candidates have not been confirmed.
Image
(Or artistic representation) |
Name | Temperature (K) | Mass | Method |
---|---|---|---|---|
![]() |
Kepler-70b | 7662 [a] | 0.44 M🜨 | Teq |
Kepler-70c | 6807 [b] | 0.655 M🜨 | ||
WD 2226-210 b | 4970[60] | |||
![]() |
Vega b | 3250 [61][c] | 21.9 M🜨 |
Notes
[edit]- ^ Assuming albedo of 0.1
- ^ Assuming albedo of 0.1
- ^ Assuming bond albedo of 0.25
References
[edit]- ^ Jones, K.; Morris, B. M.; et al. (October 2022). "The stable climate of KELT-9b". Astronomy & Astrophysics. 666: A118. arXiv:2208.04818. Bibcode:2022A&A...666A.118J. doi:10.1051/0004-6361/202243823. S2CID 251442580.
- ^ 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 Journal. 163 (2): 40. arXiv:2110.15275. Bibcode:2022AJ....163...40P. doi:10.3847/1538-3881/ac32c7. ISSN 0004-6256.
- ^ a b Mercier, Samson J.; Dang, Lisa; et al. (November 2022). "Revisiting the Iconic Spitzer Phase Curve of 55 Cancri e: Hotter Dayside, Cooler Nightside, and Smaller Phase Offset". The Astronomical Journal. 164 (5): 204. arXiv:2209.02090. Bibcode:2022AJ....164..204M. doi:10.3847/1538-3881/ac8f22.
- ^ a b c Wong, Ian; Shporer, Avi; et al. (December 2021). "TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit". The Astronomical Journal. 162 (6): 256. arXiv:2111.12074. Bibcode:2021AJ....162..256W. doi:10.3847/1538-3881/ac26bd.
- ^ a b Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike; Janík, Jan; Kabáth, Petr; Vanzi, Leonardo; Caballero, José A.; Jenkins, Jon M.; Mireles, Ismael; Seager, Sara (August 2024). "BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?". Astronomy & Astrophysics. 688: A120. arXiv:2403.12311. doi:10.1051/0004-6361/202349028. ISSN 0004-6361.
- ^ a b Lendl, M.; Csizmadia, Sz.; et al. (November 2020). "The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS". Astronomy & Astrophysics. 643: A94. arXiv:2009.13403. Bibcode:2020A&A...643A..94L. doi:10.1051/0004-6361/202038677. S2CID 221970130.
- ^ a b Cabot, Samuel H. C.; Bello-Arufe, Aaron; et al. (November 2021). "TOI-1518b: A Misaligned Ultra-hot Jupiter with Iron in Its Atmosphere". The Astronomical Journal. 162 (5): 218. arXiv:2108.11403. Bibcode:2021AJ....162..218C. doi:10.3847/1538-3881/ac1ba3.
- ^ a b c d e Pass, Emily K.; Cowan, Nicolas B.; et al. (October 2019). "Estimating dayside effective temperatures of hot Jupiters and associated uncertainties through Gaussian process regression". Monthly Notices of the Royal Astronomical Society. 489 (1): 941–950. arXiv:1908.02631. Bibcode:2019MNRAS.489..941P. doi:10.1093/mnras/stz2226.
- ^ Barros, S. C. C.; Akinsanmi, B.; Boué, G.; Smith, A. M. S.; Laskar, J.; Ulmer-Moll, S.; Lillo-Box, J.; Queloz, D.; Cameron, A. Collier; Sousa, S. G.; Ehrenreich, D.; Hooton, M. J.; Bruno, G.; Demory, B.-O.; Correia, A. C. M. (January 2022). "Detection of the tidal deformation of WASP-103b at 3 σ with CHEOPS". Astronomy & Astrophysics. 657: A52. arXiv:2201.03328. Bibcode:2022A&A...657A..52B. doi:10.1051/0004-6361/202142196. ISSN 0004-6361.
- ^ a b Mancini, L.; Southworth, J.; et al. (January 2022). "The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties". Monthly Notices of the Royal Astronomical Society. 509 (1): 1447–1464. arXiv:2105.00889. Bibcode:2022MNRAS.509.1447M. doi:10.1093/mnras/stab2691.
- ^ Owens, Niall; de Mooij, E. J. W.; et al. (May 2021). "Phase curve and variability analysis of WASP-12b using TESS photometry". Monthly Notices of the Royal Astronomical Society: Letters. 503 (1): L38 – L46. arXiv:2102.00052. Bibcode:2021MNRAS.503L..38O. doi:10.1093/mnrasl/slab014.
- ^ 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 Journal. 153 (2): 78. arXiv:1512.00464. Bibcode:2017AJ....153...78C. doi:10.3847/1538-3881/153/2/78. S2CID 55191644.
- ^ Hubble Finds a Star Eating a Planet nasa.gov. 2010-05-20. Retrieved on 2010-12-10.
- ^ waspplanets (2019-11-26). "The orbit of WASP-12b is decaying". WASP Planets. Retrieved 2020-01-01.
- ^ 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 Journal. 163 (4): 175. arXiv:2201.08370. Bibcode:2022AJ....163..175W. doi:10.3847/1538-3881/ac5680. S2CID 246063389.
- ^ 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 & Astrophysics. A34: 639. arXiv:2004.10767. Bibcode:2020A&A...639A..34V. doi:10.1051/0004-6361/202037905. S2CID 216080995.
- ^ a b Hooton, M. J.; Hoyer, S.; et al. (February 2022). "Spi-OPS: Spitzer and CHEOPS confirm the near-polar orbit of MASCARA-1 b and reveal a hint of dayside reflection". Astronomy & Astrophysics. 658: A75. arXiv:2109.05031. Bibcode:2022A&A...658A..75H. doi:10.1051/0004-6361/202141645. S2CID 237490820.
- ^ a b c d e f "Planetary Systems". exoplanetarchive.ipac.caltech.edu. Retrieved 2023-11-17.
- ^ a b Martin, Pierre-Yves (1995). "Catalogue of Exoplanets". Extrasolar Planets Encyclopaedia. Retrieved 2023-11-17.
- ^ a b "Scientists uncover a 'hellish' planet so hot it could vaporize most metals". CNET. April 27, 2021. Retrieved April 27, 2021.
- ^ "WASP 76b – A World with Iron Rain". CosmoQuest. March 17, 2020. Retrieved January 3, 2024.
- ^ Saha, Suman (August 2023). "Precise Transit Photometry Using TESS: Updated Physical Properties for 28 Exoplanets around Bright Stars". The Astrophysical Journal Supplement Series. 268 (1): 2. arXiv:2306.02951. Bibcode:2023ApJS..268....2S. doi:10.3847/1538-4365/acdb6b. ISSN 0067-0049.
- ^ European Space Agency (April 5, 2024). "Astronomers detect potential 'glory effect' on a hellish distant world for the first time". phys.org. Retrieved 2024-04-07.
- ^ Strickland, Ashley (19 April 2024). "Scientists spot 'glory effect' on a world beyond our solar system for the first time". CNN. Archived from the original on 19 April 2024. Retrieved 20 April 2024.
- ^ Wong, Ian; Knutson, Heather A.; Kataria, Tiffany; Lewis, Nikole K.; Burrows, Adam; Fortney, Jonathan J.; Schwartz, Joel; Shporer, Avi; Agol, Eric; Cowan, Nicolas B.; Deming, Drake; Désert, Jean-Michel; Fulton, Benjamin J.; Howard, Andrew W.; Langton, Jonathan (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 Journal. 823 (2): 122. arXiv:1512.09342. Bibcode:2016ApJ...823..122W. doi:10.3847/0004-637X/823/2/122. ISSN 0004-637X.
- ^ a b c d Bonomo, A. S.; Desidera, S.; Benatti, S.; Borsa, F.; Crespi, S.; Damasso, M.; Lanza, A. F.; Sozzetti, A.; Lodato, G.; Marzari, F.; Boccato, C.; Claudi, R. U.; Cosentino, R.; Covino, E.; Gratton, R. (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 & Astrophysics. 602: A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. ISSN 0004-6361. S2CID 118923163.
- ^ Giacalone, Steven. "Validation of 13 Hot and Potentially Terrestrial TESS Planets". Earth and Planetary Astrophysics. arXiv:2201.12661v2. doi:10.48550/arXiv.2201.12661.
- ^ 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 Journal. 804 (2) 150. arXiv:1407.2245. Bibcode:2015ApJ...804..150E. doi:10.1088/0004-637X/804/2/150.
- ^ 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.
- ^ 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 Journal. 804 (2): 150. arXiv:1407.2245. Bibcode:2015ApJ...804..150E. doi:10.1088/0004-637X/804/2/150. ISSN 1538-4357. S2CID 117798959.
- ^ Brinkman, Casey L.; Weiss, Lauren M.; Huber, Daniel; Lee, Rena A.; Kolecki, Jared; Tenn, Gwyneth; Zhang, Jingwen; Narayanan, Suchitra; Polanski, Alex S. (2024-09-30). "The Compositions of Rocky Planets in Close-in Orbits Tend to be Earth-Like". arXiv:2410.00213 [astro-ph.EP].
- ^ Daemgen, S.; Hormuth, F.; Brandner, W.; Bergfors, C.; Janson, M.; Hippler, S.; Henning, Th (May 2009). "Binarity of Transit Host Stars - Implications on Planetary Parameters". Astronomy & Astrophysics. 498 (2): 567–574. arXiv:0902.2179. Bibcode:2009A&A...498..567D. doi:10.1051/0004-6361/200810988. ISSN 0004-6361. S2CID 9893376.
- ^ 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 Journal. 153 (3): 136. arXiv:1609.04389. Bibcode:2017AJ....153..136S. doi:10.3847/1538-3881/aa5df3. ISSN 0004-6256.
- ^ Mandushev, Georgi; O'Donovan, Francis T.; Charbonneau, David; Torres, Guillermo; Latham, David W.; Bakos, Gáspár Á.; Dunham, Edward W.; Sozzetti, Alessandro; Fernández, José M.; Esquerdo, Gilbert A.; Everett, Mark E.; Brown, Timothy M.; Rabus, Markus; Belmonte, Juan A.; Hillenbrand, Lynne A. (2007-10-01). "TrES-4: A Transiting Hot Jupiter of Very Low Density". The Astrophysical Journal. 667 (2): L195 – L198. arXiv:0708.0834. Bibcode:2007ApJ...667L.195M. doi:10.1086/522115. ISSN 0004-637X.
- ^ Johns, Daniel; Marti, Connor; Huff, Madison; McCann, Jacob; Wittenmyer, Robert A.; Horner, Jonathan; Wright, Duncan J. (2018-11-01). "Revised Exoplanet Radii and Habitability Using Gaia Data Release 2". The Astrophysical Journal Supplement Series. 239 (1): 14. arXiv:1808.04533. Bibcode:2018ApJS..239...14J. doi:10.3847/1538-4365/aae5fb. ISSN 0067-0049.
- ^ a b Barros, S. C. C.; Almenara, J. M.; Deleuil, M.; Diaz, R. F.; Csizmadia, Sz.; Cabrera, J.; Chaintreuil, S.; Collier Cameron, A.; Hatzes, A.; Haywood, R.; Lanza, A. F.; Aigrain, S.; Alonso, R.; Bordé, P.; Bouchy, F. (2014-09-01). "Revisiting the transits of CoRoT-7b at a lower activity level". Astronomy and Astrophysics. 569: A74. arXiv:1407.8099. Bibcode:2014A&A...569A..74B. doi:10.1051/0004-6361/201423939. ISSN 0004-6361. S2CID 59495602.
- ^ Piskorz, Danielle; Benneke, Björn; Crockett, Nathan R.; Lockwood, Alexandra C.; Blake, Geoffrey A.; Barman, Travis S.; Bender, Chad F.; Carr, John S.; Johnson, John A. (2017-08-01). "Detection of Water Vapor in the Thermal Spectrum of the Non-transiting Hot Jupiter Upsilon Andromedae b". The Astronomical Journal. 154 (2): 78. arXiv:1707.01534. Bibcode:2017AJ....154...78P. doi:10.3847/1538-3881/aa7dd8. ISSN 1538-3881.
- ^ 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". Science. 314 (5799): 623–626. arXiv:astro-ph/0610491. Bibcode:2006Sci...314..623H. doi:10.1126/science.1133904. ISSN 0036-8075. PMID 17038587. S2CID 20549014.
- ^ Anderson, D. R.; Hellier, C.; Gillon, M.; Triaud, A. H. M. J.; Smalley, B.; Hebb, L.; Cameron, A. Collier; Maxted, P. F. L.; Queloz, D.; West, R. G.; Bentley, S. J.; Enoch, B.; Horne, K.; Lister, T. A.; Mayor, M. (2010-01-20). "WASP-17b: an ultra-low density planet in a probable retrograde orbit". The Astrophysical Journal. 709 (1): 159–167. arXiv:0908.1553. Bibcode:2010ApJ...709..159A. doi:10.1088/0004-637X/709/1/159. ISSN 0004-637X. S2CID 53628741.
- ^ Zellem, Robert T.; Lewis, Nikole K.; Knutson, Heather A.; Griffith, Caitlin A.; Showman, Adam P.; Fortney, Jonathan J.; Cowan, Nicolas B.; Agol, Eric; Burrows, Adam; Charbonneau, David; Deming, Drake; Laughlin, Gregory; Langton, Jonathan (2014-07-02). "The 4.5 μm full-orbit phase curve of the hot Jupiter HD 209458b". The Astrophysical Journal. 790 (1): 53. arXiv:1405.5923. Bibcode:2014ApJ...790...53Z. doi:10.1088/0004-637X/790/1/53. ISSN 0004-637X. S2CID 18882576.
- ^ "NASA's Spitzer First To Crack Open Light of Faraway Worlds". Archived from the original on July 15, 2007.
- ^ Richardson, L. Jeremy; Deming, D; Horning, K; Seager, S; Harrington, J; et al. (2007). "A spectrum of an extrasolar planet". Nature. 445 (7130): 892–895. arXiv:astro-ph/0702507. Bibcode:2007Natur.445..892R. doi:10.1038/nature05636. PMID 17314975. S2CID 4415500.
- ^ Rincon, Paul (23 June 2010). "'Superstorm' rages on exoplanet". BBC News London. Retrieved 2010-06-24.
- ^ 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". Science. 346 (6212): 981–4. arXiv:1411.6875. Bibcode:2014Sci...346..981K. doi:10.1126/science.1257829. PMID 25414310. S2CID 206560188.
- ^ a b Öztürk, 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 Society. 486 (2): 2290–2307. Bibcode:2019MNRAS.486.2290O. doi:10.1093/mnras/stz747. ISSN 0035-8711.
- ^ Martins, J. H. C; Santos, N. C; Figueira, P; Faria, J. P; Montalto, M; Boisse, I; Ehrenreich, D; Lovis, C; Mayor, M; Melo, C; Pepe, F; Sousa, S. G; Udry, S; Cunha, D (2015). "Evidence for a spectroscopic direct detection of reflected light from 51 Pegasi b". Astronomy & Astrophysics. 576: A134. arXiv:1504.05962. Bibcode:2015A&A...576A.134M. doi:10.1051/0004-6361/201425298. S2CID 119224213.
- ^ a b Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A.; Damasso, M.; Haywood, R. D.; Morbidelli, A.; Latham, D. W.; Molinari, E.; Pepe, F.; Poretti, E. (2023-09-01). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems". Astronomy and Astrophysics. 677: A33. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211. ISSN 0004-6361.
- ^ a b "Planet Compare". NASA Solar System Exploration. Retrieved 2023-12-10.
- ^ Lachapelle, François-René; Lafrenière, David; et al. (March 2015). "Characterization of Low-mass, Wide-separation Substellar Companions to Stars in Upper Scorpius: Near-infrared Photometry and Spectroscopy". The Astrophysical Journal. 802 (1): 61. arXiv:1503.07586. Bibcode:2015ApJ...802...61L. doi:10.1088/0004-637X/802/1/61. S2CID 54762786.
- ^ Petrus, S.; Bonnefoy, M.; Chauvin, G.; Babusiaux, C.; Delorme, P.; Lagrange, A.-M.; Florent, N.; Bayo, A.; Janson, M.; Biller, B.; Manjavacas, E.; Marleau, G.-D.; Kopytova, T. (January 2020). "A new take on the low-mass brown dwarf companions on wide orbits in Upper-Scorpius". Astronomy & Astrophysics. 633: A124. arXiv:1910.00347. Bibcode:2020A&A...633A.124P. doi:10.1051/0004-6361/201935732. ISSN 0004-6361.
- ^ a b Neuhäuser, R.; Mugrauer, M.; et al. (June 2008). "Astrometric and photometric monitoring of GQ Lupi and its sub-stellar companion". Astronomy and Astrophysics. 484 (1): 281–291. arXiv:0801.2287. Bibcode:2008A&A...484..281N. doi:10.1051/0004-6361:20078493. S2CID 5358020.
- ^ a b Schmidt, T. O. B.; Neuhäuser, R.; et al. (November 2008). "Direct evidence of a sub-stellar companion around CT Chamaeleontis". Astronomy and Astrophysics. 491 (1): 311–320. arXiv:0809.2812. Bibcode:2008A&A...491..311S. doi:10.1051/0004-6361:20078840. S2CID 17161561.
- ^ a b Bonnefoy, M.; Chauvin, G.; Lagrange, A.-M.; Rojo, P.; Allard, F.; Pinte, C.; Dumas, C.; Homeier, D. (February 2014). "A library of near-infrared integral field spectra of young M–L dwarfs". Astronomy & Astrophysics. 562: A127. arXiv:1306.3709. Bibcode:2014A&A...562A.127B. doi:10.1051/0004-6361/201118270. ISSN 0004-6361.
- ^ van Holstein, R.G.; Stolker, T.; Jensen-Clem, R.; Ginski, C.; Milli, J.; de Boer, J.; Girard, J.H.; Wahhaj, Z.; Bohn, A.J.; Millar-Blanchaer, M.A.; Benisty, M.; Bonnefoy, M.; Chauvin, G.; Dominik, C.; Hinkley, S. (March 2021). "A survey of the linear polarization of directly imaged exoplanets and brown dwarf companions with SPHERE-IRDIS: First polarimetric detections revealing disks around DH Tau B and GSC 6214-210 B". Astronomy & Astrophysics. 647: A21. arXiv:2101.04033. Bibcode:2021A&A...647A..21V. doi:10.1051/0004-6361/202039290. ISSN 0004-6361.
- ^ Xuan, Jerry W.; Hsu, Chih-Chun; Finnerty, Luke; Wang, Jason; Ruffio, Jean-Baptiste; Zhang, Yapeng; Knutson, Heather A.; Mawet, Dimitri; Mamajek, Eric E.; Inglis, Julie; Wallack, Nicole L.; Bryan, Marta L.; Blake, Geoffrey A.; Mollière, Paul; Hejazi, Neda (2024-07-01). "Are These Planets or Brown Dwarfs? Broadly Solar Compositions from High-resolution Atmospheric Retrievals of ∼10–30 M Jup Companions". The Astrophysical Journal. 970 (1): 71. arXiv:2405.13128. Bibcode:2024ApJ...970...71X. doi:10.3847/1538-4357/ad4796. ISSN 0004-637X.
- ^ Chilcote, Jeffrey; Pueyo, Laurent; Rosa, Robert J. De; Vargas, Jeffrey; Macintosh, Bruce; Bailey, Vanessa P.; Barman, Travis; Bauman, Brian; Bruzzone, Sebastian; Bulger, Joanna; Burrows, Adam S.; Cardwell, Andrew; Chen, Christine H.; Cotten, Tara; Dillon, Daren (2017-03-28). "1–2.4μm Near-IR Spectrum of the Giant PlanetβPictoris b Obtained with the Gemini Planet Imager". The Astronomical Journal. 153 (4): 182. arXiv:1703.00011. Bibcode:2017AJ....153..182C. doi:10.3847/1538-3881/aa63e9. ISSN 1538-3881.
- ^ Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo (2022-09-01). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (1): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. ISSN 0067-0049.
- ^ "Length of Exoplanet Day Measured for First Time / VLT measures the spin of Beta Pictoris b". April 30, 2014.
- ^ Landman, R.; Stolker, T.; et al. (February 2024). "β Pictoris b through the eyes of the upgraded CRIRES+. Atmospheric composition, spin rotation, and radial velocity". Astronomy & Astrophysics. 682: A48. arXiv:2311.13527. Bibcode:2024A&A...682A..48L. doi:10.1051/0004-6361/202347846.
- ^ Iskandarli, Leyla; Farihi, Jay; et al. (October 2024). "Novel Constraints on Companions to the Helix Nebula Central Star". Monthly Notices of the Royal Astronomical Society. 534 (4): 3498–3505. arXiv:2410.03288. Bibcode:2024MNRAS.534.3498I. doi:10.1093/mnras/stae2286.
- ^ Hurt, Spencer A.; Quinn, Samuel N.; Latham, David W.; Vanderburg, Andrew; Esquerdo, Gilbert A.; Calkins, Michael L.; Berlind, Perry; Angus, Ruth; Latham, Christian A.; Zhou, George (2021-04-01). "A decade of radial-velocity monitoring of Vega and new limits on the presence of planets". The Astronomical Journal. 161 (4): 157. arXiv:2101.08801. Bibcode:2021AJ....161..157H. doi:10.3847/1538-3881/abdec8. ISSN 0004-6256.