List of largest exoplanets

Image of the outer dust around the young star HD 100546. The position of HD 100546 b was indicated by an orange dot.

Below is a list of the largest exoplanets so far discovered, in terms of physical size, ordered by radius.

List

The sizes are listed in units of Jupiter radii (RJ, R♃)(71,492km). All planets listed are larger than two times the size of the largest planet in the Solar System, Jupiter. Some planets that are smaller than 1.7 RJ have been included for comparison.

This list is incomplete; you can help by expanding it.
Exoplanet name Radius (RJ)
(Jupiter = 1) 		Notes
Sun (Sol) 9.95[1][2]
(1,391,400 km)		 The largest object in the Solar System.
Reported for reference
HD 100546 b's surrounding disk 6.9+2.7
−2.9[3]		 Largest exoplanet in the NASA Exoplanet Archive, although because of flux from the planet and the disk that are superimposed, the exact size of this planet cannot be determined and the emitting area has this size, composed of the planet and including its disk, not to be mistaken as a single planet radius. Over time, it will shrink to the size of Jupiter. 20 MJ; is likely a brown dwarf.
Reported for reference
GQ Lupi b 4.6±1.4,[4] 3.0[5]–6.5[4] Currently the largest exoplanet discovered. 1 - 36 MJ; at the highest end of this range, it may be classified as a young brown dwarf.
DH Tauri b 2.7±0.8[4] 11+10
−3 MJ; at its largest, it would be classified as a brown dwarf
ROXs 42Bb 2.5[6] This massive hot jupiter (9+6
−3 MJ) varies from 0.9 RJ to 3 RJ.[6]
OTS 44 2.3[7]–5.7[8] Very likely a sub-brown dwarf, which it may be the lowest-mass free-floating substellar objects. It is surrounded by a circumstellar disk of dust and particles of rock and ice
Kepler-13 Ab (KOI-13b) 2.216±0.087[9] Lisa et al gives also radii of 1.512±0.035 RJ and 2.63+1.04
−0.82 RJ. Natalie et al calculate 2.03 RJ.[10]
CT Chamaeleontis b 2.2+0.81
−0.6[11]		 17 MJ; is likely a brown dwarf.
KOI-368.01 2.1±0.2[12]
WASP-79b 2.09±0.14[13]
HAT-P-67b 2.085+0.096
−0.071[14]		 0.34+0.25
−0.19 MJ; a very puffy Hot Jupiter
XO-6b 2.07±0.22[15] 4.4 MJ; a very puffy Hot Jupiter
HAT-P-32b 2.037±0.999[15] 0.941 (± 0.166) MJ; a very puffy Hot Jupiter. Other estimates give 1.789±0.025 RJ.[16]
KOI-3681.01 2.0+0.7
−1[12]		 Orbits fairly close to its 1.1+0.2
−0.2 M☉ star, with 217 day-long years.
WASP-17b 1.991+0.08
−0.58[17]		 Was the largest known planet in 2012. At only 0.486 MJ, this Hot Jupiter is extremely low density. This estimate gives also a range from 1.411 RJ to 2.071 RJ.[17]
Kepler-435b 1.99±0.18[18]
KOI-680 b 1.99[12]
KELT-19 Ab 1.91[19]
CVSO 30b 1.91[20]
51 Pegasi b (Bellerophon) 1.9±0.3[21] First exoplanet to be discovered orbiting a main-sequence star. Prototype hot Jupiters.
WASP-12b ("Pitch black") 1.900+0.057
−0.055,[22] 1.736±0.056[23]		 This planet is so close to its parent star that its tidal forces are distorting it into an egg shape. As of September 2017, it has been described as "black as asphalt", and as a "pitch black" hot Jupiter as it absorbs 94% of the light that shines on its surface.
KELT-9b 1.891+0.061
−0.055[24]		 One of the hottest exoplanets known.
HAT-P-65b 1.89±0.13[25]
WASP-121b 1.865±0.044[26]
KELT-8b 1.86+0.18
−0.16[27]
HATS-23b 1.86+0.3
−0.4[28]
WASP-76b 1.83+0.06
−0.04[29]
HAT-P-33b 1.827±0.29[30]
Cha 110913-773444 1.8[31] A rogue planet (Likely a sub-brown dwarf) that is surrounded by a protoplanetary disk. It is one of youngest free-floating substellar objects with 0.5–10 Myr.
TrES-4 1.799±0.063[32] This planet has a density of 0.2 g/cm3, about that of balsa wood, less than Jupiter's 1.3g/cm3
WASP-122b 1.792±0.069[33]
KELT-12b 1.78+0.17
−0.16[34]
HATS-26b 1.75±0.21[35]
KELT-14b 1.743±0.047[33]
KELT-20b 1.735+0.07
−0.075[36]
HAT-P-40b 1.730±0.062[37]
WASP-94 Ab 1.72+0.06
−0.05[38]
KELT-4 Ab 1.706+0.085
−0.076[39]
WASP-88b 1.7+0.13
−0.07[40]
WASP-78b 1.70±0.04[13]
1RXS 1609b 1.7[41] 14+2.0
−3.0 MJ; is likely a brown dwarf.

A few additional examples with radii lower than 1.7 RJ.

Exoplanet name Radius (RJ)
(Jupiter = 1) 		Notes
Kepler-12b 1.695+0.032
−0.032[42]
beta Pic b 1.65
PSO J318.5-22 1.53 A rogue planet, which is an extrasolar object of planetary mass that does not appear to have a host star.
Kepler-7b 1.478
HD 209458 b (Osiris) 1.35 The first exoplanet whose size was determined.
TrES-2b (Kepler-1b) 1.272 Darkest known exoplanet due to an extremely low geometric albedo. It absorbs 99% of light.
Kepler-39b 1.22 One of the most massive exoplanets known.
HR 2562 b 1.11 Most massive planet with a mass of 30 MJ, although according to most definitions of planet, it may be too massive to be a planet, and may be a brown dwarf instead.
Jupiter 69,911 km [43] Largest planet in the Solar System, by radius and mass.[44]
Reported for reference

Timeline of largest exoplanet recordholders

Planet Size (RJ) Date Notes
Kepler-1656 b 5.02 2018—
GQ Lupi b 3.0[5] 2015—2018 The emitting area of the extremely young HD 100546 b, including planet and disk, indicates that there is a large amount of heat left from formation. Over time, the planet will shrink to approximately the size of Jupiter. This candidate could be larger.
HAT-P-32b 2.037 2013—2015 CT Cha b may be larger at 2.2 Jupiter radii, but its status as a planet or brown dwarf is unconfirmed.
WASP-17b 1.991 2012—2013
WASP-12b 2.15 to 1.83 2009—2012
TRES-4b 1.799 2007—2009 This planet has a density of 0.2 g/cm3, about that of balsa wood, less than Jupiter's 1.3g/cm3 It was succeeded by WASP-17b as the largest exoplanet.[45][46]
HD 209458 b 1.35 1999—2007 This was the first exoplanet whose size was determined.[47]
Jupiter 1 —1999 Largest planet of Solar System.

See also

References

  1. ↑ Mamajek, E.E.; Prsa, A.; Torres, G.; et, al. (2015), "IAU 2015 Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties", arXiv:1510.07674 [astro-ph.SR]
  2. ↑ Emilio, Marcelo; Kuhn, Jeff R.; Bush, Rock I.; Scholl, Isabelle F. (2012), "Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits", The Astrophysical Journal, 750 (2): 135, arXiv:1203.4898, Bibcode:2012ApJ...750..135E, doi:10.1088/0004-637X/750/2/135
  3. ↑ Quanz, Sasch P.; Amara, Adam; Meyer, Michael P.; Kenworthy, Matthew P.; et al. (2014). "Confirmation and characterization of the protoplanet HD100546 b - Direct evidence for gas giant planet formation at 50 au". Astrophysical Journal. 807: 64. arXiv:1412.5173. Bibcode:2015ApJ...807...64Q. doi:10.1088/0004-637X/807/1/64.
  4. 1 2 3 Zhou, Yifan; Herczeg, Gregory J; Kraus, Adam L; Metchev, Stanimir; Cruz, Kelle L (2014). "Accretion onto Planetary Mass Companions of Low-mass Young Stars". The Astrophysical Journal Letters. 783: L17. arXiv:1401.6545. Bibcode:2014ApJ...783L..17Z. doi:10.1088/2041-8205/783/1/L17.
  5. 1 2 Astrometric and photometric monitoring of GQ Lupi and its sub-stellar companion, Ralph Neuhäuser, Markus Mugrauer, Andreas Seifahrt, Tobias Schmidt, and Nikolaus Vogt, Astronomy and Astrophysics 484, #1 (2008), pp. 281–291. doi:10.1051/0004-6361:20078493. Bibcode: 2008A&A...484..281N
  6. 1 2 Currie, Thayne; Burrows, Adam; Daemgen, Sebastian (2014). "A First-Look Atmospheric Modeling Study of the Young Directly-Imaged Planet-Mass Companion, ROXs 42Bb". The Astrophysical Journal. 787 (2): 104. arXiv:1404.0131 [astro-ph.SR]. Bibcode:2014ApJ...787..104C. doi:10.1088/0004-637X/787/2/104. Cite uses deprecated parameter |class= (help)
  7. ↑ Luhman, K. L.; et al. (February 2005), "Spitzer Identification of the Least Massive Known Brown Dwarf with a Circumstellar Disk", The Astrophysical Journal, 620 (1): L51–L54, arXiv:astro-ph/0502100, Bibcode:2005ApJ...620L..51L, doi:10.1086/428613
  8. ↑ Joergens, V.; Bonnefoy, M.; Liu, Y.; Bayo, A.; Wolf, S.; Chauvin, G.; Rojo, P. (2013). "OTS 44: Disk and accretion at the planetary border". Astronomy & Astrophysics. 558 (7): L7. arXiv:1310.1936. Bibcode:2013A&A...558L...7J. doi:10.1051/0004-6361/201322432.
  9. ↑ Esteves, Lisa J; De Mooij, Ernst J. W; 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.
  10. ↑ Batalha, Natalie M; Rowe, Jason F; Bryson, Stephen T; Barclay, Thomas; Burke, Christopher J; Caldwell, Douglas A; Christiansen, Jessie L; Mullally, Fergal; Thompson, Susan E; Brown, Timothy M; Dupree, Andrea K; Fabrycky, Daniel C; Ford, Eric B; Fortney, Jonathan J; Gilliland, Ronald L; Isaacson, Howard; Latham, David W; Marcy, Geoffrey W; Quinn, Samuel; Ragozzine, Darin; Shporer, Avi; Borucki, William J; Ciardi, David R; Gautier III, Thomas N; Haas, Michael R; Jenkins, Jon M; Koch, David G; Lissauer, Jack J; Rapin, William; et al. (2012). "Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data". The Astrophysical Journal Supplement Series. 204 (2): 24. arXiv:1202.5852. Bibcode:2013ApJS..204...24B. doi:10.1088/0067-0049/204/2/24.
  11. ↑ Direct evidence of a sub-stellar companion around CT Cha, T. O. B. Schmidt et al., accepted for publication in Astronomy and Astrophysics, Bibcode: 2008arXiv0809.2812S, arXiv:0809.2812.
  12. 1 2 3 "All extrasolar planets". Open Exoplanet Catalogue.
  13. 1 2 Smalley, B; Anderson, D. R; Collier-Cameron, A; Doyle, A. P; Fumel, A; Gillon, M; Hellier, C; Jehin, E; Lendl, M; Maxted, P. F. L; Pepe, F; Pollacco, D; Queloz, D; Ségransan, D; Smith, A. M. S; Southworth, J; Triaud, A. H. M. J; Udry, S; West, R. G (2012). "WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus". Astronomy & Astrophysics. 547: A61. arXiv:1206.1177. Bibcode:2012A&A...547A..61S. doi:10.1051/0004-6361/201219731.
  14. ↑ Zhou, G; Bakos, G. Á; Hartman, J. D; Latham, D. W; Torres, G; Bhatti, W; Penev, K; Buchhave, L; Kovács, G; Bieryla, A; Quinn, S; Isaacson, H; Fulton, B. J; Falco, E; Csubry, Z; Everett, M; Szklenar, T; Esquerdo, G; Berlind, P; Calkins, M. L; Béky, B; Knox, R. P; Hinz, P; Horch, E. P; Hirsch, L; Howell, S. B; Noyes, R. W; Marcy, G; De Val-Borro, M; 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.
  15. 1 2 Crouzet, N; McCullough, P. R; Long, D; Montanes Rodriguez, P; Lecavelier Des Etangs, A; Ribas, I; Bourrier, V; Hébrard, G; Vilardell, F; Deleuil, M; Herrero, E; Garcia-Melendo, E; Akhenak, L; Foote, J; Gary, B; Benni, P; Guillot, T; Conjat, M; Mékarnia, D; Garlitz, J; Burke, C. J; Courcol, B; Demangeon, O (2017). "Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit". The Astronomical Journal. 153 (3): 94. arXiv:1612.02776. Bibcode:2017AJ....153...94C. doi:10.3847/1538-3881/153/3/94.
  16. ↑ Hartman, J. D; Bakos, G. Á; Torres, G; Latham, D. W; Kovács, Géza; Béky, B; Quinn, S. N; Mazeh, T; Shporer, A; Marcy, G. W; Howard, A. W; Fischer, D. A; Johnson, J. A; Esquerdo, G. A; Noyes, R. W; Sasselov, D. D; Stefanik, R. P; Fernandez, J. M; Szklenár, T; Lázár, J; Papp, I; Sári, P (2011). "HAT-P-32b and HAT-P-33b: Two Highly Inflated Hot Jupiters Transiting High-jitter Stars". The Astrophysical Journal. 742: 59. arXiv:1106.1212. Bibcode:2011ApJ...742...59H. doi:10.1088/0004-637X/742/1/59.
  17. 1 2 Anderson, D. R.; et al. (2010). "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.
  18. ↑ Almenara, J. M; Damiani, C; Bouchy, F; Havel, M; Bruno, G; Hébrard, G; Diaz, R. F; Deleuil, M; Barros, S. C. C; Boisse, I; Bonomo, A. S; Montagnier, G; Santerne, A (2015). "SOPHIE velocimetry of Kepler transit candidates. XV. KOI-614b, KOI-206b, and KOI-680b: A massive warm Jupiter orbiting a G0 metallic dwarf and two highly inflated planets with a distant companion around evolved F-type stars". Astronomy & Astrophysics. 575: A71. arXiv:1501.01486. Bibcode:2015A&A...575A..71A. doi:10.1051/0004-6361/201424291.
  19. ↑ Siverd, Robert J; Collins, Karen A; Zhou, George; Quinn, Samuel N; Scott Gaudi, B; Stassun, Keivan G; Johnson, Marshall C; Bieryla, Allyson; Latham, David W; Ciardi, David R; Rodriguez, Joseph E; Penev, Kaloyan; Pinsonneault, Marc; Pepper, Joshua; Eastman, Jason D; Relles, Howard; Kielkopf, John F; Gregorio, Joao; Oberst, Thomas E; Giulio Francesco Aldi; Esquerdo, Gilbert A; Calkins, Michael L; Berlind, Perry; Dressing, Courtney D; Patel, Rahul; Stevens, Daniel J; Beatty, Thomas G; Lund, Michael B; Labadie-Bartz, Jonathan; et al. (2017). "KELT-19Ab: A P~4.6 Day Hot Jupiter Transiting a Likely Am Star with a Distant Stellar Companion". The Astronomical Journal. 155 (155): 35. arXiv:1709.07010. Bibcode:2018AJ....155...35S. doi:10.3847/1538-3881/aa9e4d.
  20. ↑ van Eyken, Julian C; Ciardi, David R; Kaspar von Braun; Kane, Stephen R; Plavchan, Peter; Bender, Chad F; Brown, Timothy M; Crepp, Justin R; Fulton, Benjamin J; Howard, Andrew W; Howell, Steve B; Mahadevan, Suvrath; Marcy, Geoffrey W; Shporer, Avi; Szkody, Paula; Akeson, Rachel L; Beichman, Charles A; Boden, Andrew F; Gelino, Dawn M; Hoard, D. W; Ramírez, Solange V; Rebull, Luisa M; Stauffer, John R; Bloom, Joshua S; Bradley Cenko, S; Kasliwal, Mansi M; Kulkarni, Shrinivas R; Law, Nicholas M; Nugent, Peter E; et al. (2012). "The PTF Orion Project: A Possible Planet Transiting a T-Tauri Star". The Astrophysical Journal. 755 (2012): 42. arXiv:1206.1510. Bibcode:2012ApJ...755...42V. doi:10.1088/0004-637X/755/1/42.
  21. ↑ 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.
  22. ↑ Collins, Karen A; Kielkopf, John F; Stassun, Keivan G (2015). "Transit Timing Variation Measurements of WASP-12b and Qatar-1b: No Evidence for Additional Planets". 1512: arXiv:1512.00464. arXiv:1512.00464 [astro-ph.EP]. Bibcode:2015arXiv151200464C. Cite uses deprecated parameter |class= (help)
  23. ↑ Chan, Tucker; Ingemyr, Mikael; Winn, Joshua N; Holman, Matthew J; Sanchis-Ojeda, Roberto; Esquerdo, Gil; Everett, Mark (2011). "The Transit Light Curve project. XIV. Confirmation of Anomalous Radii for the Exoplanets TrES-4b, HAT-P-3b, and WASP-12b". The Astronomical Journal. 141 (6): 179. arXiv:1103.3078. Bibcode:2011AJ....141..179C. doi:10.1088/0004-6256/141/6/179.
  24. ↑ Gaudi, B. Scott; Stassun, Keivan G; Collins, Karen A; Beatty, Thomas G; Zhou, George; Latham, David W; Bieryla, Allyson; Eastman, Jason D; Siverd, Robert J; Crepp, Justin R; Gonzales, Erica J; Stevens, Daniel J; Buchhave, Lars A; Pepper, Joshua; Johnson, Marshall C; Colon, Knicole D; Jensen, Eric L. N; Rodriguez, Joseph E; Bozza, Valerio; Novati, Sebastiano Calchi; d'Ago, Giuseppe; Dumont, Mary T; Ellis, Tyler; Gaillard, Clement; Jang-Condell, Hannah; Kasper, David H; Fukui, Akihiko; Gregorio, Joao; Ito, Ayaka; et al. (2017). "A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host". Nature. 546 (7659): 514–518. arXiv:1706.06723. Bibcode:2017Natur.546..514G. doi:10.1038/nature22392. PMID 28582774.
  25. ↑ Hartman, J. D; Bakos, G. Á; Bhatti, W; Penev, K; Bieryla, A; Latham, D. W; Kovács, G; Torres, G; Csubry, Z; De Val-Borro, M; Buchhave, L; Kovács, T; Quinn, S; Howard, A. W; Isaacson, H; Fulton, B. J; Everett, M. E; Esquerdo, G; Béky, B; Szklenar, T; Falco, E; Santerne, A; Boisse, I; Hébrard, G; Burrows, A; Lázár, J; Papp, I; Sári, P (2016). "HAT-P-65b and HAT-P-66b: Two Transiting Inflated Hot Jupiters and Observational Evidence for the Reinflation of Close-in Giant Planets". The Astronomical Journal. 152 (6): 182. arXiv:1609.02767. Bibcode:2016AJ....152..182H. doi:10.3847/0004-6256/152/6/182.
  26. ↑ Delrez, L; Santerne, A; Almenara, J.-M; Anderson, D. R; Collier-Cameron, A; Díaz, R. F; Gillon, M; Hellier, C; Jehin, E; Lendl, M; Maxted, P. F. L; Neveu-Vanmalle, M; Pepe, F; Pollacco, D; Queloz, D; Ségransan, D; Smalley, B; Smith, A. M. S; Triaud, A. H. M. J; Udry, S; Van Grootel, V; West, R. G (2016). "WASP-121 b: A hot Jupiter close to tidal disruption transiting an active F star". Monthly Notices of the Royal Astronomical Society. 458 (4): 4025. arXiv:1506.02471. Bibcode:2016MNRAS.458.4025D. doi:10.1093/mnras/stw522.
  27. ↑ Fulton, Benjamin J; Collins, Karen A; Gaudi, B. Scott; Stassun, Keivan G; Pepper, Joshua; Beatty, Thomas G; Siverd, Robert J; Penev, Kaloyan; Howard, Andrew W; Baranec, Christoph; Corfini, Giorgio; Eastman, Jason D; Gregorio, Joao; Law, Nicholas M; Lund, Michael B; Oberst, Thomas E; Penny, Matthew T; Riddle, Reed; Rodriguez, Joseph E; Stevens, Daniel J; Zambelli, Roberto; Ziegler, Carl; Bieryla, Allyson; d'Ago, Giuseppe; Depoy, Darren L; Jensen, Eric L. N; Kielkopf, John F; Latham, David W; Manner, Mark; et al. (2015). "KELT-8b: A Highly Inflated Transiting Hot Jupiter and a New Technique for Extracting High-precision Radial Velocities from Noisy Spectra". The Astrophysical Journal. 810: 30. arXiv:1505.06738. Bibcode:2015ApJ...810...30F. doi:10.1088/0004-637X/810/1/30.
  28. ↑ Bento, J; Schmidt, B; Hartman, J. D; Bakos, G. Á; Ciceri, S; Brahm, R; Bayliss, D; Espinoza, N; Zhou, G; Rabus, M; Bhatti, W; Penev, K; Csubry, Z; Jordán, A; Mancini, L; Henning, T; De Val-Borro, M; Tinney, C. G; Wright, D. J; Durkan, S; Suc, V; Noyes, R; Lázár, J; Papp, I; Sári, P (2017). "HATS-22b, HATS-23b and HATS-24b: Three new transiting super-Jupiters from the HATSouth project". Monthly Notices of the Royal Astronomical Society. 468: 835. arXiv:1607.00688. Bibcode:2017MNRAS.468..835B. doi:10.1093/mnras/stx500.
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  30. ↑ Hartman, J. D; Bakos, G. Á; Torres, G; Latham, D. W; Kovács, G; Béky, B; Quinn, S. N; Mazeh, T; Shporer, A; Marcy, G. W; Howard, A. W; Fischer, D. A; Johnson, J. A; Esquerdo, G. A; Noyes, R. W; Sasselov, D. D; Stefanik, R. P; Fernandez, J. M; Szklenár, T; Lázár, J; Papp, I; Sári, P (2011). "HAT-P-32b and HAT-P-33b: Two Highly Inflated Hot Jupiters Transiting High-Jitter Stars". The Astrophysical Journal. 742: 59. arXiv:1106.1212. Bibcode:2011ApJ...742...59H. doi:10.1088/0004-637X/742/1/59.
  31. ↑ Luhman, K. L; Adame, Lucía; d'Alessio, Paola; Calvet, Nuria; Hartmann, Lee; Megeath, S. T; Fazio, G. G (2005). "Discovery of a Planetary-Mass Brown Dwarf with a Circumstellar Disk". The Astrophysical Journal. 635: L93. arXiv:astro-ph/0511807. Bibcode:2005ApJ...635L..93L. doi:10.1086/498868.
  32. ↑ Daemgen, S.; Hormuth, F.; Brandner, W.; Bergfors, C.; Janson, M.; Hippler, S.; Henning, T. (200). "Binarity of transit host stars - Implications for planetary parameters" (PDF). Astronomy and Astrophysics. 498 (2): 567–574. arXiv:0902.2179. Bibcode:2009A&A...498..567D. doi:10.1051/0004-6361/200810988.
  33. 1 2 Turner, O. D; Anderson, D. R; Collier Cameron, A; Delrez, L; Evans, D. F; Gillon, M; Hellier, C; Jehin, E; Lendl, M; Maxted, P. F. L; Pepe, F; Pollacco, D; Queloz, D; Ségransan, D; Smalley, B; Smith, A. M. S; Triaud, A. H. M. J; Udry, S; West, R. G (2016). "WASP-120 b, WASP-122 b, AND WASP-123 b: Three Newly Discovered Planets from the WASP-South Survey". Publications of the Astronomical Society of the Pacific. 128 (964): 064401. arXiv:1509.02210. Bibcode:2016PASP..128f4401T. doi:10.1088/1538-3873/128/964/064401.
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  36. ↑ Lund, Michael B; Rodriguez, Joseph E; Zhou, George; Scott Gaudi, B; Stassun, Keivan G; Johnson, Marshall C; Bieryla, Allyson; Oelkers, Ryan J; Stevens, Daniel J; Collins, Karen A; Penev, Kaloyan; Quinn, Samuel N; Latham, David W; Steven Villanueva Jr; Eastman, Jason D; Kielkopf, John F; Oberst, Thomas E; Jensen, Eric L. N; Cohen, David H; Joner, Michael D; Stephens, Denise C; Relles, Howard; Corfini, Giorgio; Gregorio, Joao; Zambelli, Roberto; Esquerdo, Gilbert A; Calkins, Michael L; Berlind, Perry; Ciardi, David R; et al. (2017). "KELT-20b: A giant planet with a period of P~ 3.5 days transiting the V~ 7.6 early a star HD 185603". The Astronomical Journal. 154 (5): 194. arXiv:1707.01518. Bibcode:2017AJ....154..194L. doi:10.3847/1538-3881/aa8f95.
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  38. ↑ Neveu-VanMalle, M; Queloz, D; Anderson, D. R; Charbonnel, C; Collier Cameron, A; Delrez, L; Gillon, M; Hellier, C; Jehin, E; Lendl, M; Maxted, P. F. L; Pepe, F; Pollacco, D; Segransan, D; Smalley, B; Smith, A. M. S; Southworth, J; Triaud, A. H. M. J; Udry, S; West, R. G (2014). "WASP-94 a and B planets: Hot-Jupiter cousins in a twin-star system". Astronomy & Astrophysics. 572 (49): A49. arXiv:1409.7566. Bibcode:2014A&A...572A..49N. doi:10.1051/0004-6361/201424744.
  39. ↑ Eastman, Jason D; Beatty, Thomas G; Siverd, Robert J; Antognini, Joseph M. O; Penny, Matthew T; Gonzales, Erica J; Crepp, Justin R; Howard, Andrew W; Avril, Ryan L; Bieryla, Allyson; Collins, Karen; Fulton, Benjamin J; Ge, Jian; Gregorio, Joao; Ma, Bo; Mellon, Samuel N; Oberst, Thomas E; Wang, Ji; Gaudi, B. Scott; Pepper, Joshua; Stassun, Keivan G; Buchhave, Lars A; Jensen, Eric L. N; Latham, David W; Berlind, Perry; Calkins, Michael L; Cargile, Phillip A; Colón, Knicole D; Dhital, Saurav; et al. (2016). "KELT-4Ab: An Inflated Hot Jupiter Transiting the Bright (V ˜ 10) Component of a Hierarchical Triple". The Astronomical Journal. 151 (2): 45. arXiv:1510.00015. Bibcode:2016AJ....151...45E. doi:10.3847/0004-6256/151/2/45.
  40. ↑ Delrez, L; Van Grootel, V; Anderson, D. R; Collier-Cameron, A; Doyle, A. P; Fumel, A; Gillon, M; Hellier, C; Jehin, E; Lendl, M; Neveu-VanMalle, M; Maxted, P. F. L; Pepe, F; Pollacco, D; Queloz, D; Ségransan, D; Smalley, B; Smith, A. M. S; Southworth, J; Triaud, A. H. M. J; Udry, S; West, R. G (2013). "Transiting planets from WASP-South, Euler and TRAPPIST: WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars". Astronomy & Astrophysics. 563: A143. arXiv:1312.1827. Bibcode:2014A&A...563A.143D. doi:10.1051/0004-6361/201323204.
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  43. ↑ Elizabeth Howell (21 April 2014). "The Planets in Our Solar System in Order of Size". Universe Today.
  44. ↑ Jerry Coffey (8 July 2008). "What is the Biggest Planet in the Solar System?". Universe Today.
  45. ↑ Ker Than (6 August 2007). "Largest Known Exoplanet Discovered". Space.com.
  46. ↑ California Institute of Technology (6 August 2007). "Keck Confirms Largest Exoplanet To Date". W.M. Keck Observatory.
  47. ↑ Laurance R. Doyle; Hans-Jörg Deeg; Timothy M. Brown (September 2000). "Searching for Shadows of Other Earths" (PDF). Scientific American. 283 (3): 59–65. doi:10.1038/scientificamerican0900-58. PMID 10976467.
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