List of largest exoplanets

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Template:Short description

Jupiter as seen by Voyager 1 in 1979. It is the largest planet having its surface resolved[1][2][3] and it is the largest planet in the Solar System.[4]

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

Limitations

This list of extrasolar objects may and will change over time due to diverging measurements published between scientific journals, varying methods used to examine these objects, and the notably difficult task of discovering extrasolar objects in general. These objects are not stars, and are quite small on a universal or even stellar scale. Then there is the fact that these objects might be brown dwarfs, sub-brown dwarfs, or not exist at all. Because of this, this list only cites the most certain measurements to date and is prone to change.

List

The sizes are listed in units of Jupiter radii (Template:Jupiter radius, 71 492 km). This list is designed to include all planets that are larger than 1.6 times the size of Jupiter. Some well-known planets that are smaller than Template:Jupiter radius (17.93Template:NbspTemplate:Earth radius or Template:Val Template:Val) have been included for the sake of comparison.

Key (classification)
Template:Asterisk Probably brown dwarfs (≳ 13 Template:Jupiter mass) (based on mass)
Template:Dagger Probably sub-brown dwarfs (based on mass and location)
? Uncertain status (inconsistency in age or mass of planetary system)
! Uncertain status while probably brown dwarfs (≳ 13 Template:Jupiter mass) (based on mass)
← Probably exoplanets (≲ 13 Template:Jupiter mass) (based on mass)
→ Planets with grazing transit, hindering radius determination
Template:Number sign Notable non-exoplanets reported for reference
– Theoretical planet size restrictions
Key (illustration)
Artist's impression
Artist's size comparison
Artist's impression size comparison
Direct imaging telescopic observation
Direct image size comparison
Composite image of direct observations
Transiting telescopic observation
Simulation observation

Template:Sticky header

Illustration Name
(Alternates) 		Radius
(Template:Jupiter radius) 		Key Mass
(Template:Jupiter mass) 		Notes
Sun
(Sol) 		Template:Val
(Template:Val)[5]
(695 700 km) 		Template:Number sign 1047.569
(Template:Val)[5]
(1.988 416 x 1030 kg) 		The only star in the Solar System. Responsible for life on Earth and keeping the planets on orbit. Age: 4.6 Gyr.[6]
Reported for reference.
Toliman
(Alpha Centauri B) 		Template:Val ± 0.035[7]
(0.8591 ± 0.0036 Template:Solar radius) 		Template:Number sign 952.450 ± 2.619[7]
(0.9092 ± 0.0025 Template:Solar mass) 		One of first two stars (other being Rigil Kentaurus / Alpha Centauri A) to have its stellar parallax measured.[8] Nearest binary star system and nearest stellar system to the Sun at the distance of Template:Cvt. A member of Alpha Centauri System, the nearest system to the Sun. Age: 5.3 ± 0.3 Gyr.[9]
Reported for reference.
Maximum size of planetary-mass object 8[10] – ~ 5[10] Maximum theoretical size limit assumed for a ~ 5 Template:Val mass object right after formation, however, for 'arbitrary initial conditions'.
Proplyd 133-353 ≲ 7.82 ± 0.81[11]Template:Efn
(≲ Template:Solar radius calculator) 		Template:Dagger (≲) 13[11] A candidate sub-brown dwarf or rogue planet with a photoevaporating disk, located in the Orion Nebula Cluster. At a probable age younger than 500 000 years, it is one of the youngest free-floating planetary-mass candidates known.[11]
More information about Proplyd 133-353 and estimates of its radius are available:Template:Efn
2M0535-05 A
(V2384 Orionis A) 		6.71 ± 0.11[12]
Template:Nowrap 		Template:Number sign 59.9 ± 3.5[12]
(0.0572 ± 0.0033 Template:Val) 		First eclipsing binary brown dwarf system to be discovered, orbiting around 9.8 days.[13][14] Age: ~1 Myr[15]
Reported for reference.
2M0535-05 B
(V2384 Orionis B) 		5.25 ± 0.09[12]
(0.540 ± 0.009 Template:Val) 		Template:Number sign 38.3 ± 2.3[12]
(0.0366 ± 0.0022 Template:Val)
KPNO-Tau-4 4.1[16][17] Template:Dagger 10.5[16] A member of Taurus-Auriga star-forming region.[17]
GQ Lupi b
(GQ Lupi Ab,
GQ Lupi B) 		3.77[18] Template:Asterisk 20 ± 10;[19]
Template:Nowrap[20] 		First confirmed exoplanet candidate to be directly imaged. GQ Lupi b has a mass of 1 – Template:Val; in the higher half of this range, it may be classified as a young brown dwarf. It should not be confused with the star GQ Lup C (2MASS J15491331), 2400 AU away, sometimes referred to as GQ Lup B.[21] Other sources of the radius include Template:Val Template:Jupiter radius,[22] Template:Val Template:Jupiter radius,[20] Template:Val Template:Jupiter radius,[23] 4.6 ± 1.4 RJ, 6.5 ± 2.0 RJ.[24]
HD 100546 b
(KR Muscae b) 		3.4[25] Template:Asterisk 25[25] Sometimes the initially reported Template:Val Template:± Template:Jupiter radius for the emitting area due to the diffuse dust and gas envelope or debris disk surrounding the planet[26] is confused with the actual radius. Other source of mass: 1.65 Template:Val.[27]
HD 100546 (KR Mus) is the nearest Herbig Be star to the Sun.[28]
2MASS J0437+2331 3.30[29]Template:Efn Template:Dagger 7.1 Template:±[29] May be a sub-brown dwarf or a rogue planet
OTS 44 3.2Template:Snd3.6[30] Template:Dagger 11.5[31] First discovered rogue planet; very likely a brown dwarf[32] or sub-brown dwarf.[33] It is surrounded by a circumstellar disk of dust and particles of rock and ice. The currently preferred radius estimate is done by SED modelling including substellar object and disk model.[30]
2MASS J044144b
(2M 0441+23 Bb) 		3.06[34]Template:Efn Template:Dagger 9.8 ± 1.8[34] Based on the mass ratio to 2M J044145 A (2M 0441+23 Aa) it is likely not a planet according to the IAU's exoplanet working definition.[35] Part of the lowest mass quadruple 2M 0441+23 system of Template:Solar mass.[34]
Kapteyn's Star 2.83 ± 0.24[36]
(0.291 ± 0.025 Template:Solar radius) 		Template:Number sign 294.4 ± 14.7[36]
(0.2810 ± 0.014 Template:Solar mass) 		The closest halo star and nearest red subdwarf, at the distance of Template:Cvt, and second-highest proper motion of any stars of more than 8 arcseconds per year (after the Barnard's Star). Age: 11.5 Template:± Gyr.[37]
Reported for reference.
AB Aurigae b
(AB Aur b) 		< 2.75[38]Template:Efn ! 20 Template:Nowrap,[39]
Template:Nowrap Template:Nowrap,
< 130[38] 		Likely a brown dwarf; Assuming a hot-start evolution model and a planetary mass, AB Aurigae b would be younger than 2 Myr to have its observed large luminosity, which is inconsistent with the age of AB Aurigae of 6.0 Template:± Myr, which could be caused by delayed planet formation in the disk.[40] Other system ages include 1 - 5 Myr,[38] 4 ± 1 Myr[41] and 4 Myr.[42] Another source gives a higher mass of Template:Val in the brown dwarf regime for an age of 4 Myr, arguing since gravitational instability of the disk (preferred formation mechanism in the discovery publication)[38] operates on very short time scales, the object might be as old as AB Aur.[39] A more recent study also support the latter source, given the apparent magnitude was revised upwards.[43]
DH Tauri b
(DH Tau b) 		2.7 ± 0.8[24] ← 11 ± 3[24] First planet to have a confirmed circumplanetary disk, detected with polarimetry at the VLT[44] and youngest confirmed planet at an age of 0.7 Myr.[22] DH Tauri b is suspected to have an exomoon candidate orbiting it every 320 years, with about the same mass as Jupiter.[45]
Other sources give the radii: Template:Val Template:Jupiter radius,[22] 2.49 Template:Jupiter radius[30]Template:Efn and masses: 14.2 Template:± Template:Val,[46] 17 ± 6 Template:Val,[47] 12 ± 4 Template:Val.[22]
CT Chamaeleontis b
(CT Cha b) 		2.6 Template:±[30] Template:Asterisk 17 ± 6[48] Likely a brown dwarf.
CM Draconis A
(Gliese 630.1 Aa) 		2.4437 ± 0.0002[49]
(0.25113 ± 0.00016 Template:Solar radius) 		Template:Number sign 235.8 ± 0.3[49]
Template:Nowrap 		One of the lightest stars with precisely measured masses and radii, orbiting around 1.268 days. Age: 4.1 ± 0.8 Gyr.[50]
Reported for reference.
PZ Telescopii b
(PZ Tel b,
HD 174429 b) 		2.42 Template:±[51] Template:Asterisk 27 Template:±[52] Likely a brown dwarf. First possible extra Jupiter-like planet to be directly imaged[53]
CM Draconis B
(Gliese 630.1 Ab) 		2.3094 ± 0.0001[49]
(0.23732 ± 0.00014 Template:Solar radius) 		Template:Number sign 220.2 ± 0.3[49]
(0.21017 ± 0.00028 Template:Solar mass) 		One of the lightest stars with precisely measured masses and radii, orbiting around 1.268 days. Age: 4.1 ± 0.8 Gyr.[50]
Reported for reference.
o005 s41280 2.30[54] Template:Dagger 8.4[54] May be a sub-brown dwarf or a rogue planet[54]
TWA 29 2.222 Template:±[55] Template:Dagger 6.6 Template:±[55] Rogue planet
Hot Jupiter limit 2.2[56] – > 0 Theoretical limit for hot Jupiters close to a star, that are limited by tidal heating, resulting in 'runaway inflation'
XO-6b 2.17 ± 0.2[57] ← 4.47 ± 0.12[57] A very puffy Hot Jupiter
PSO J077.1+24 2.14[29]Template:Efn Template:Dagger 5.9 Template:±[29] Rogue planet
CAHA Tau 1 2.12[58][59]Template:Efn Template:Dagger 10 ± 5[58][59] Rogue planet
ROXs 42B b 2.10 ± 0.35[22] ← 9 Template:±,[60] 10 ± 4[61] Older estimates include 1.9 – 2.4, 1.3Template:Snd4.7 Template:Jupiter radius[62] and 2.43Template:±, 2.55Template:± Template:Jupiter radius.[63] Other recent sources of masses include 3.2 – 27 Template:Jupiter mass,[64] 13 ± 5 Template:Jupiter mass.[22]
HAT-P-67b 2.038 Template:±,[57]
2.165 Template:±Template:Efn[65] 		← 0.418 ± 0.012[57] A very puffy Hot Jupiter. Was the largest known planet with an accurately and precisely measured radius[66] (2.085 Template:± Template:Jupiter radius),[67] until a new estimate revised its radius in 2024.[65][57]
HATS-15b 2.019 Template:±[68] ← 2.17 ± 0.15[68]
Cha 110913-773444
(Cha 110913) 		2.0Template:Snd2.1[30] Template:Dagger 8 Template:±[69] A rogue planet/sub-brown dwarf that is surrounded by a protoplanetary disk, the first one to be confirmed. It is one of youngest free-floating substellar objects with 0.5–10 Myr. The currently preferred radius estimate is done by SED modelling including substellar object and disk model.[30]
CFHTWIR-Oph 90
(Oph 90) 		2.00 Template:±;[70]
3[71][72] 		Template:Dagger 10.5[71] May be rogue planet or brown dwarf
SSTB213 J041757 A 2[73] Template:Dagger 3.5[73] In a binary with a smaller Template:Jupiter radius planet.
Kepler-435b
(KOI-614 b) 		1.99 ± 0.18[74] ← 0.84 ± 0.15[74]
PDS 70 c 1.98 Template:±[75] ← 7.5 Template:±, Template:Nowrap, Template:Nowrap (total)[76] First confirmed directly imaged exoplanet still embedded in the natal gas and dust from which planets form (protoplanetary disk) and the second protoplanet to have a confirmed circumplanetary disk (after DH Tauri b).[77] PDS 70 is the second multi-planet system to be directly imaged (after HR 8799).
PDS 70 b 1.96 Template:±[75] ← 3.2 Template:±, 7.9 Template:±, Template:Nowrap, Template:Nowrap[76] First protoplanet to have been ever detected. PDS 70 is the second multiplanetary system to be directly imaged (after HR 8799 system). Other source of radius includes 2.7 Template:Jupiter radius.[40]
OGLE2-TR-L9b Template:Val[68] ← Template:Val[68] First discovered planet orbiting a fast-rotating hot star, OGLE2-TR-L9.[78]
CFHTWIR-Oph 98 A 1.95Template:±;[70] 2.14[71][79] Template:Asterisk 15.4 ± 0.8;[80]
10.5[71] 		Either a M-type brown dwarf or sub-brown dwarf with a sub-brown dwarf/planet companion CFHTWIR-Oph 98 b.
Other sources of masses includes: 9.6 – 18.4 Template:Jupiter mass.[80]
WASP-178b
(KELT-26 b,
HD 134004 b) 		1.940 Template:±[81] ← 1.41 Template:±[81] An ultra-hot Jupiter. Initially, the planet's atmosphere was discovered having silicon monoxide, making this exoplanet the first one to have the compound on its atmosphere,[82] now the atmosphere is more likely dominated by ionized magnesium and iron.[83]
WASP-12Ab 1.937 ± 0.056[84] ← 1.47 Template:±[85] This planet is so close to WASP-12 A that its tidal forces are distorting it into an egg-like shape.[86] First planet observed being consumed by its host star;[87] it will be destroyed in 3.16 ± 0.10 Template:Val due to tidal interactions.[88][89]
WASP-12b is suspected to have one exomoon due to a curve of change of shine of the planet observed regular variation of light.[90]
BD-14 3065 b
(TOI-4987 b) 		1.926 ± 0.094[91] Template:Asterisk 12.37 ± 0.92[91] Might be a brown dwarf fusing deuterium at its core, which could explain its anomalous high radius. Also one of the hottest known exoplanets, measuring Template:Convert.[91]
KELT-9b
(HD 195689 b) 		1.891 Template:±[92] ← 2.17 ± 0.56[93] Hottest confirmed exoplanet, with a temperature of Template:Val (3777 ± 180 Template:Val; 6830 ± 324 Template:Val).[94]
TOI-1518 b 1.875 ± 0.053[95] ← < 2.3 (2 σ)[95]
HAT-P-70b 1.87 Template:±[96] ← < 6.78 (3 σ)[96]
2MASS J1935-2846 1.869 ± 0.053[97] Template:Dagger 7.4 Template:±[97] May be a sub-brown dwarf or rogue planet.
HATS-23b 1.86 Template:±[98] → 1.470 ± 0.072[98] Grazing planet.
CFHTWIR-Oph 98 b
(Oph 98 b,
CFHTWIR-Oph 98 B) 		1.86 ± 0.05[99][79] Template:Dagger 7.8 Template:±[80] Its formation as an exoplanet is challenging or impossible.[100] If its formation scenario is known, it may explain the formation of Planet Nine. Planetary migration may explain its formation, or it may be a sub-brown dwarf.
Other sources of mass includes 4.1 – 11.6 Template:Jupiter mass.[80]
KELT-8b 1.86 Template:±[101] ← 0.867 Template:±[101]
KPNO-Tau 12 1.84,[16]
2.22 Template:±[70] 		Template:Dagger 11.5[71] A member of Taurus-Auriga star-forming region.[16]
TrES-4
(GSC 06200-00648 Ab) 		1.838 Template:±[68] ← 0.78 ± 0.19[102] This planet has a density of 0.17 g/cm3,[68] about that of balsa wood, less than Saturn's 0.7 g/cm3.
HAT-P-33b 1.827 ± 0.29,[103]
Template:Val[99] 		← 0.72 Template:±[104]
HAT-P-32b 1.822 Template:±[68] ← 0.941 ± 0.166,
0.860 ± 0.164[105]
KELT-20b
(MASCARA-2b) 		1.821Template:±[106] ← 3.355Template:±[106] An ultra-hot Jupiter.
YSES 1 b
(TYC 8998-760-1 b) 		Template:Nowrap Template:Asterisk 21.8 ± 3[107] Likely a brown dwarf. First substellar object to have an isotope (13C) in its atmosphere.[108][109] First directly imaged planetary system having multiple bodies orbiting a Sun-like star.[110][111]
Barnard's Star 1.82 ± 0.01[112]
(0.187 ± 0.001 Template:Val) 		Template:Number sign 168.7 Template:±[112]
(0.1610 Template:± Template:Val) 		Second nearest planetary system to the Sun at the distance of Template:Cvt and closest star in the northern celestial hemisphere. Also the highest proper motion of any stars of 10.3 arcseconds per year relative to the Sun.
Has a planet, Barnard b (Barnard's Star b).[113]
Reported for reference.
CoRoT-1b 1.805 Template:±[68] ← 1.03 ± 0.12[68] First exoplanet for which optical (as opposed to infrared) observations of phases were reported.[114]
WTS-2b 1.804 Template:±[68] ← 1.12 ± 0.16[68]
WASP-76b 1.802Template:±[106] ← 0.921Template:±[106] WASP-76b is suspected to have an exomoon analogue to Jupiter's Io due to the detection of sodium via absorption spectroscopy.[115]
Saffar
(Template:Nowrap) 		~1.8[116] ← 1.70 Template:±[117] Radius estimated using the phase curve of reflected light. The planet orbits very close to Titawin (υ And A) at the distance of 0.0595 AU, completing an orbit in 4.617 days.[118] First multiple-planet system to be discovered around a main-sequence star, and first multiple-planet system known in a multiple-star system.
HAT-P-40b 1.799 Template:±[68] ← 0.48 ± 0.13[68] A very puffy hot Jupiter
WASP-122b
(KELT-14b) 		1.795 Template:±[68] ← 1.284 ± 0.032[119]
KELT-12b 1.79 Template:±[120] ← 0.95 ± 0.14[120]
Tylos
(WASP-121b) 		1.773 Template:±[121] ← 1.157 ± 0.07[121] First exoplanet found to contain water on its stratosphere. Tylos is suspected to have an exomoon analogous to Jupiter's Io due to the detection of sodium absorption spectroscopy around it.[122]
TOI-640 Ab 1.771 Template:±[123] ← 0.88 ± 0.16[123]
WASP-187b 1.766 ± 0.036[57] ← 0.801 Template:±[57]
WASP-94 Ab 1.761 Template:±[68] ← Template:Val[68]
TOI-2669b 1.76 ± 0.16[124] ← 0.61 ± 0.19[124]
WISE J0528+0901 1.752 Template:±[125] Template:Dagger 13 Template:±[125] Brown dwarf or rogue planet.
HATS-26b 1.75 ± 0.21[126] ← 0.650 ± 0.076[126]
Kepler-12b 1.7454 Template:±[127] ← 0.431 ± 0.041[128] Least-irradiated of four Hot Jupiters at the time of discovery
HAT-P-65b 1.744 Template:±[68] ← 0.527 ± 0.083[129] This planet has been suffering orbital decay due to its close proximity to HAT-P-65; 0.04 AU.[130]
2MASS J2352-1100 1.742 Template:±[97] Template:Dagger 12.4 Template:±[97] Brown dwarf or rogue planet.
KELT-15b 1.74 ± 0.20[102] ← 1.31 ± 0.43[102]
HAT-P-57b 1.74 ± 0.36[102] ← 1.41 ± 1.52[102]
WASP-93b 1.737 Template:±[68] ← 1.47 ± 0.29[68]
WASP-82b Template:Val[68] ← Template:Val[68]
Ditsö̀
(WASP-17b) 		1.720 Template:±,
1.83 ± 0.01[131] 		← 0.512 ± 0.037[132] First planet discovered to have a retrograde orbit[133] and first to have quartz (crystalline silica, SiO2) in its clouds.[134] Template:Nowrap,[135] the lowest of any exoplanet when it was discovered, and was possibly the largest exoplanet at the time of discovery, with a radius of Template:Jupiter radius.[136]
KELT-19 Ab 1.717Template:±[106] ← 3.98Template:±[106]
HAT-P-39b Template:Val[68] ← Template:Val[68]
KELT-4Ab 1.706 Template:±[137] ← 0.878 Template:±[137]
Pollera
(WASP-79b) 		1.704 Template:±[68] ← 0.850 Template:±[68]
HAT-P-64b 1.703 ± 0.070[138] ← 0.58 Template:±[138]
WASP-78b 1.70 ± 0.04,[139]
1.93 ± 0.45[99] 		← 0.89 ± 0.08[139] This planet has likely undergone in the past a migration from the initial highly eccentric orbit.[140]
Qatar-7b 1.70 ± 0.03[99] ← 1.88 ± 0.25[141]
SSTB213 J041757 b 1.70[142] Template:Dagger 1.50[142] In a binary with a larger Template:Jupiter radius planet.
CoRoT-17b 1.694 Template:±[68] ← 2.430Template:±[68]
TOI-615b 1.69Template:±[143] ← 0.43Template:±[143]
TOI-1855 b 1.65 Template:±[144] ← 1.133 ± 0.096[144]
TOI-3807 b >1.65 (95% lower limit)[145] → 1.04 Template:±[145] Grazing planet, a large radius of Template:Jupiter radius derived from transit data is unreliable due to its grazing nature.
NGTS-33 b 1.64 ± 0.07[146] ← 3.6 ± 0.3[146]
KELT-8b 1.62 ± 0.10[102] ← 0.66 ± 0.12[102]
WASP-82b 1.62 ± 0.13 ← 1.17 ± 0.20[102]
WASP-189 b 1.619 ± 0.021[147] ← 1.99 Template:±[147] One of the hottest known exoplanets.
HAT-P-65b 1.611 ± 0.024[148] ← 0.554 Template:±[148]
NGTS-31 b 1.61 ± 0.16[149] ← 1.12 ± 0.12[149]
HATS-11b 1.609 ± 0.064[150] ← 0.85[150]
K2-52b 1.61 ± 0.20[151] ←
KELT-7b 1.60 ± 0.06[102] ← 1.39 ± 0.22[102]
SR 12 c
(SR 12 (AB) b,
SR 12 C) 		~ 1.6,[152]
2.38 Template:±[70] 		? 11 ± 3[152] The planet is at the very edge of the deuterium burning limit. This object orbits around SR 12 AB at the distance of 980 Template:Val but has a circumplanetary disk, detected in sub-mm with ALMA.[152]
Other sources of masses includes 14 Template:± Template:Jupiter mass,[153] 12Template:Snd15 Template:Jupiter mass[154] and 13 ± 2 Template:Jupiter mass.[70]
A few notable examples with radii below 1.6 Template:Jupiter radius (17.93 Template:Earth radius).
Kepler-7b 1.574 Template:±[127] ← 0.433 Template:±[155] One of the first five exoplanets to be confirmed by the Kepler spacecraft, within 34 days of Kepler's science operations,[156] and the first exoplanet to have a crude map of cloud coverage.[157][158][159]
HD 106906 b 1.54 Template:±[160] ← 11 ± 2[161] This planet orbits around HD 106906 at the distance of 738 AU, a distance much larger than what is possible for a planet formed within a protoplanetary disk.[162] It more likely formed on its own, like a star, rather in a protoplanetary disk.[163]
Recent observations made by the Hubble Space Telescope strengthened the case for the planet having an unusual orbit that perturbed it from its host star's debris disk causing NASA and several news outlets to compare to the hypothetical Planet Nine.[164][165]
Proxima Centauri
(Alpha Centauri C) 		1.50 ± 0.04[166]
(0.1542 ± 0.0045 Template:Solar radius) 		Template:Number sign 127.9 ± 2.3[166]
Template:Nowrap 		The nearest star and planetary system to the Sun, at a distance of Template:Cvt, orbiting around Alpha Centauri AB System, the nearest star system to the Sun. Age: 4.85 Gyr.[167]
Has a confirmed planet, Proxima Centauri b,[168] a disputed planet, Proxima Centauri c,[169] and a unconfirmed planet, Proxima Centauri d.
Reported for reference.
Beta Pictoris b
(β Pic b) 		1.46 ± 0.01[170] ← 11.729 Template:±[171] First exoplanet to have its rotation rate measured and fastest-spinning exoplanet known at the time of discovery.[172][173] Beta Pictoris b is suspected to have exomoon due to the former's predicted obliquity misalignment.[174]
Najsakopajk
(HIP 65426 b) 		1.44 ± 0.03[175] ← 7.1 ± 1.2, 9.9 Template:±,
10.9 Template:±[175] 		First exoplanet to be imaged by the James Webb Space Telescope.[176] The JWST direct imaging observations tightly constrained its bolometric luminosity, which provides a robust mass constraint of 7.1 ± 1.2 Template:Jupiter mass. The atmospheric fitting of both temperature and radius are in disagreement with evolutionary models. Moreover, this planet is around 14 million years old which is however not associated with a debris disk, despite its young age,[177][178] causing it to not fit current models for planetary formation.[179]
HD 209458 b
("Osiris") 		1.359 Template:±[180] ← 0.682 Template:±[180] 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[181][182] and the first to have an atmosphere, containing evaporating hydrogen, and oxygen and carbon. First extrasolar gas giant to have its superstorm measured. Nicknamed "Osiris".
Teide 1 1.311 Template:±[97]
(0.1347 Template:± Template:Solar radius) 		Template:Number sign 52 Template:±[97]
(0.0496 Template:± Template:Val) 		The first brown dwarf to be confirmed.[183][184] It is located in the Pleiades and has an age of 70Template:Snd140Myr.[185]
Reported for reference.
OGLE-TR-56b 1.30 ± 0.05 ← 1.29 ± 0.12 First discovered exoplanet using the transit method.[186]
TOI-157b 1.29 ± 0.02[187] ← 1.18 ± 0.13[187] Oldest confirmed planet at the age of 12.9 Template:± Gyr[187]
TrES-2
(Kepler-1 Ab) 		1.265 Template:±[127] ← 1.199 ± 0.052[188] Darkest known exoplanet due to an extremely low geometric albedo of 0.0136, absorbing 99% of light.
Dimidium
(51 Pegasi b) 		1.2 ± 0.1[189] ← 0.46 Template:±[190] First exoplanet to be discovered orbiting a main-sequence star.[191] Prototype of the hot Jupiters.
HR 8799 e 1.17 Template:±[192] ← 9.6 Template:±[193] First exoplanet to be directly observed using optical interferometry. HR 8799 system is also the first directly imaged planetary system having multiple exoplanets.
TRAPPIST-1 1.16 ± 0.01[194]
(0.1192 ± 0.0013 Template:Solar radius) 		Template:Number sign 94.1 ± 2.4[194]
Template:Nowrap 		Coldest and smallest known star hosting exoplanets.[195] All seven exoplanets are rocky planets, orbiting closer to the star than Mercury. Their orbits' inclinations of 0.1 degreesTemplate:Sfn makes TRAPPIST-1 system the flattest planetary system.[196] Age: 7.6 ± 2.2 Gyr.[197]
Reported for reference.
HD 189733 Ab 1.138 ± 0.027[180] ← 1.123 ± 0.045[180] First exoplanet to have its thermal map constructed,[198] its overall color (deep blue) determined,[199][200] its transit viewed in the X-ray spectrum, one of first two exoplanets (other being "Osiris") to be observed spectroscopically[181][182] and first to have carbon dioxide confirmed as being present in its atmosphere.
Such the rich cobalt blue[201][202] colour of HD 189733 Ab may be the result of Rayleigh scattering. The wind can blow up to Template:Convert from the day side to the night side.[203]
2M1207 b
(TWA 27b) 		1.13[204] Template:Dagger 5.5 ± 0.5[204] First planetary body discovered via direct imaging, and the first around a brown dwarf.[205][206] It could be considered a sub-brown dwarf due to its large mass in relation to its host: 2M1207 b is around six times more massive than Jupiter, but orbits a Template:Jupiter mass brown dwarf, a ratio much larger than the 1:1000 of Jupiter and Sun for example. The IAU defined that exoplanets must have a mass ratio to the central object less than 0.04,[207][208] which would make 2M1207b a sub-brown dwarf. Nevertheless, 2M1207b has been considered an exoplanet by press media and websites,[209][210][211] exoplanet databases[212][213] and alternative definitions.[214] It will shrink to a size slightly smaller than Jupiter as it cools over the next few billion years.
2MASS J0523−1403 1.126 ± 0.063[215]
(0.116 ± 0.006 Template:Solar radius) 		Template:Number sign 103 ± 11[215]
(0.0983 ± 0.0011 Template:Solar mass)
or
67.54 ± 12.79[216]
(0.0644 ± 0.0122 Template:Solar mass) 		Coolest main sequence star with effective temperature 1939 K (1666 Template:Val; 3031 Template:Val)[216] and one of the smallest stars, in both radius and mass.[217]
Reported for reference.
Gliese 900 b
(CW2335+0142) 		1.11[218] ← 10.5[219] This exoplanet has the largest observed host star separation of any known exoplanet, at 12 000 AU (0.058 pc; 0.19 ly) and the longest known orbital period, at a duration of 1.27 Myr. First confirmed and third discovered circumtriple planet.
CoRoT-3 Ab 1.08 ± 0.05[220] Template:Asterisk 21.66 ± 1.00[221] Might be considered either a planet or a brown dwarf, depending on the definition chosen for these terms. If the brown dwarf/planet limit is defined by mass regime using the deuterium burning limit as the delimiter (i.e. Template:Val), CoRoT-3b is a brown dwarf.[222] If formation is the criterion, CoRoT-3 Ab may be a planet given that some models of planet formation predict that planets with masses up to 25–30 Jupiter masses can form via core accretion.[223] However, it is unclear which method of formation created CoRoT-3A b.
Kepler-1647 b 1.05932 ± 0.01228[224] ← 1.52 ± 0.65[224] Longest transit orbital period of any confirmed transiting exoplanet discovered at the duration of 1107 days[225] and largest circumbinary planet discovered.[226] This planet is located within the habitable zone of binary star system Kepler-1647 and thus could theoretically have a habitable Earth-like exomoon.[227]
Kepler-90h 1.01 ± 0.09[228] ← 0.639 ± 0.016[229] Located in the Kepler-90 system with eight known exoplanets, whose architecture is similar to that of the Solar System, with rocky planets being closer to the star and gas giants being more distant. This planet is located at 1 AU from its star, which is within the habitable zone of Kepler-90 and thus could theoretically have a habitable Earth-like exomoon.
Ahra
(WD 0806-661 b) 		1.007 – 1.04[230] ← 6.8 – 9.0[230] First exoplanet discovered around a single (as opposed to binary) white dwarf, and the coldest directly imaged exoplanet when discovered.[231]
Possibly formed closer to Maru (WD 0806−661) when it was a main sequence star, this object migrated further away as it reached the end of its life (see stellar evolution), with a current separation of about Template:Val.
Might be considered an exoplanet or a sub-brown dwarf, the dimmest sub-brown dwarf. The IAU considers objects below the Template:Val limiting mass for deuterium fusion that orbit stars (or stellar remnants) to be planets, regardless on how they formed.[232]
Jupiter 1
(Template:Val)[5]
(71 492 km) 		Template:Number sign 1
(Template:Val)[233]
(1.898 125 × 1027 kg) 		Oldest, largest and most massive planet in the Solar System;[234] this planet hosts 95 known moons including the Galilean moons.
Reported for reference.
For smaller exoplanets, see the list of smallest exoplanets or other lists of exoplanets. For exoplanets with milestones, see the list of exoplanet extremes and list of exoplanet firsts.

Notes

Template:Notelist

Candidates for largest exoplanets

Unconfirmed exoplanets

These planets are also larger than 1.6 times the size of the largest planet in the Solar System, Jupiter, but have yet to be confirmed or are disputed.
Note: Some data may be unreliable or incorrect due to unit or conversion errors

Key (Classification)
← Probably planets (≲ 13 Template:Jupiter mass) (based on mass)
‡ Unclassified object (unknown mass)
– Theoretical planet size restrictions
Key (Illustration)
Artist's impression
Composite image of direct observations

Template:Sticky header

Illustration Name
(Alternates)
(Status) 		Radius
(Template:Jupiter radius) 		Key Mass
(Template:Jupiter mass) 		Notes
New born planet limit ~ 30[235] – ≤ 20
Template:Nowrap[235] 		Theoretical size limit of a newly-formed planet.
Young Hot Jupiter limit ~ 20[236] – ≤ 10[236] Theoretical size limit of a newly-formed planet that needed 104 – 105 (Template:Val – Template:Val) years to migrate close to the host star, but has not yet interacted with it beforehand.
Template:Nowrap
(FU Ori Ab)
(unconfirmed) 		~ 9.8[235]
(~ Template:Val) 		← ~ 3[235] Discovered using a variation of disk kinematics.[237] Tidal disruption and extreme evaporation made the planet radius shrink from the beginning of the burst (Template:Jupiter radius) in 1937[236] to the present year by ~30 per cent and its mass is around half of its initial mass of Template:Jupiter mass.[236][235]
UCAC4 174-179953 b
(unclassified) 		8.14 ± 0.40[238]
(0.84 Template:Solar radius) 		‡ Unknown Object cannot be classified as brown dwarf or exoplanet without a mass estimate.
UCAC4 220-040923 b
(unclassified) 		4.65 ± 0.20[238] ‡ Unknown
UCAC4 223-042828 b
(unclassified) 		3.33 ± 0.50[238] ‡ Unknown
UCAC4 185-192986 b
(unclassified) 		3.3 ± 0.2[238] ‡ Unknown
UCAC4 118-126574 b
(unclassified) 		3.12 ± 0.10[238] ‡ Unknown
UCAC4 171-187216 b
(unclassified) 		2.75 ± 0.20[238] ‡ Unknown
KOI-7073 b
(unclassified) 		Template:Nowrap[239] ‡ Unknown
UCAC4 175-188215 b
(unclassified) 		2.69 ± 0.50[238] ‡ Unknown
UCAC4 116-118563 b
(unclassified) 		2.62 ± 0.10[238] ‡ Unknown
19g-2-01326 b
(unclassified) 		Template:Nowrap[240] ‡ Unknown
SOI-2 b
(unclassified) 		2.22[241] ‡ Unknown
TIC 332350266.01
(unclassified) 		2.21Template:±[242] ‡ Unknown
Old Hot Jupiter limit 2.2[56] – > 0 Theoretical limit for hot Jupiters close to a star, that are limited by tidal heating, resulting in 'runaway inflation'
TIC 138664795.01
(unclassified) 		2.16 ± 0.16[242] ‡ Unknown Object cannot be classified as brown dwarf or exoplanet without a mass estimate.
UCAC4 221-041868 b
(unclassified) 		2.1 ± 0.20[238] ‡ Unknown
TOI-496 b
(unclassified) 		2.05 Template:±[243] ‡ Unknown
SOI-7 b
(unclassified) 		1.96[241] ‡ Unknown
UCAC4 121-140615 b
(unclassified) 		1.94 ± 0.20[238] ‡ Unknown
UCAC4 123-150641 b
(unclassified) 		1.93 ± 0.20[238] ‡ Unknown
TIC 274508785.01
(unclassified) 		1.92Template:±[242] ‡ Unknown
W74 b
(Gaia DR2 6045477635223138432 b)
(unclassified) 		1.9[244] ‡ Unknown
TIC 116307482.01
(unclassified) 		1.89 ± 1.46[242] ‡ Unknown
UCAC4 122-142653 b
(unclassified) 		1.85 ± 0.10[238] ‡ Unknown
TIC 77173027.01
(unclassified) 		1.84 ± 1.12[242] ‡ Unknown
TOI-159 Ab
(unclassified) 		1.80 ± 0.77[245] ‡ Unknown
TIC 82205179.01
(TIC 82205179 b)
(unclassified) 		1.76 ± 0.56[242] ‡ Unknown
UCAC4 124-144273 b
(unclassified) 		1.71 ± 0.10[238] ‡ Unknown
TOI-710 b
(unclassified) 		1.66 ± 1.10[246] ‡ Unknown

Exoplanets with uncertain radii

This list contains planets with uncertain radii that could be below or above the adopted cut-off of Template:Jupiter radius, depending on the estimate.

Key (classification)
← Probably planets (≲ 13 Template:Jupiter mass) (based on mass)
? Status uncertain (inconsistency in age or mass of planetary system)
→ Planets with grazing transit, hindering radius determination
Key (illustration)
Direct imaging telescopic observation

Template:Sticky header

Illustration Name
(Alternates) 		Radius
(Template:Jupiter radius) 		Key Mass
(Template:Jupiter mass) 		Notes
AB Pictoris b
(AB Pic b) 		1.57 ± 0.07Template:Snd1.8 ± 0.3[247] ← 10 ± 1[247] Template:Nowrap mass estimates of Template:Val[248] to Template:Val,[249] its mass is now estimated to be Template:Val, with an age of Template:Val million years.[250]
TOI-2193 Ab >Template:Nowrap[251] → Template:Nowrap[251] Grazing planet, a large reported radius of Template:Jupiter radius is unreliable. Whether it is larger than Template:Jupiter radius is unknown.
TOI-3540 b >1.44 (95% lower limit)[251] → 1.18 ± 0.14[251] Grazing planet, a large reported radius of Template:Jupiter radius is unreliable. Whether it is larger than Template:Jupiter radius is unknown.
TOI-1408 b >1, 1.5 (estimate),[252]
2.23 ± 0.36,Template:Efn
2.4 ± 0.5[253] 		→ 1.86 ± 0.02[253] A large radius of Template:Val has been derived from transit photometry,[253] but this value is likely inaccurate due to the grazing transit of TOI-1408 b; it transits only part of the star's surface, thus hindering a precise measurement of planet-to-star size ratio. Only a lower limit of about Template:Jupiter radius can be obtained, whether TOI-1408 b is larger than Template:Jupiter radius is unknown.[252]

Notes

Template:Notelist

Chronological list of largest exoplanets

These exoplanets were the largest at the time of their discovery.

Key (classification)
Template:Asterisk Later identified to be a probable/confirmed brown dwarf (≳ 13 Template:Jupiter mass) or a star (≳ 82.76 Template:Jupiter mass)
Template:Dagger Candidate for largest exoplanet (currently or in time span)
? Status uncertain (inconsistency in age or mass of planetary system) while being candidate for largest exoplanet
→ Assumed largest exoplanet, while unconfirmed, later retracted or later confirmed
← Largest exoplanet (≲ 13 Template:Jupiter mass) at the time
– Largest confirmed exoplanet (in radius and mass), while discovered candidates might be larger
Template:Number sign Non-exoplanets reported for reference
Key (illustration)
Artist's impression
Artist's impression size comparison
Direct Imaging telescopic observation
Transiting telescopic observation
Graphic chart

Template:Sticky header

Years largest discovered Illustration Name
(Alternates) 		Radius
(Template:Jupiter radius) 		Key Mass
(Template:Jupiter mass) 		Notes
2024Template:Sndpresent XO-6b 2.17 ± 0.2[57] – 4.47 ± 0.12[57] A very puffy Hot Jupiter
(2024Template:Snd2024) ROXs 42B b 2.10 ± 0.35[22] Template:Dagger 9 Template:±;[60] 10 ± 4[61] Large size needs confirmation. Other estimates include 1.9 – 2.4 Template:Jupiter radius, 1.3Template:Snd4.7 Template:Jupiter radius.[62] Other recent sources of masses include 3.2 – 27 Template:Jupiter mass,[64] 13 ± 5 Template:Jupiter mass.[22]
2024 – 2024 HAT-P-67b 2.165 Template:±Template:Efn[65] – 0.418 ± 0.012[57] A very puffy Hot Jupiter. Previously the largest known planet with an accurately and precisely measured radius,[66] a new estimate revised its radius.[65][57]
(2022 – 2025) AB Aurigae b
(AB Aur b,
HD 31293 b) 		2.75[38] ? 20 Template:Nowrap[39]
< 130,
Template:Nowrap Template:Nowrap[38] 		The commonly favored model for gas giant planet formation – core accretion – has significant difficulty forming massive gas giant planets at AB Aur b's very large distance from its AB Aur. Instead, AB Aur b may be forming by disk (gravitational) instability,[254] where as a massive disk around a star cools, gravity causes the disk to rapidly break up into one or more planet-mass fragments.[255]
(2022 – present) PDS 70b 2.7[40] Template:Dagger 3.2 Template:±, 7.9 Template:±,
< 10 (2 σ),
≲ 15 (total)[76] 		Has been later measured to have a radius of only Template:Jupiter radius,[75] and then Template:Jupiter radius in 2022.[40] Large size needs confirmation due to this discrepancy.
(2021 – 2022) 1.96[75]
(2020 – 2021) 2.09 Template:±Template:Snd2.72 Template:±[256]
(2020Template:Sndpresent) SR 12 c
(SR 12 (AB) c,
SR 12 C) 		2.38 Template:±[70] ? 13 ± 2[70] The planet is at the very edge of the deuterium burning limit. Mass being below it needs confirmation. Other sources of masses includes 14 Template:± Template:Jupiter mass,[153] 12Template:Snd15 Template:Jupiter mass.[154]
2017 – 2024 HAT-P-67b 2.085 Template:±[67] – 0.34 Template:±[257] A very puffy Hot Jupiter. At discovery the largest known planet with an accurately and precisely measured radius.[66]
2017 – 2017 XO-6b 2.07 ± 0.22[258] – 4.47 ± 0.12[57] A very puffy Hot Jupiter
(2014Template:Snd2024) ROXs 42B b 2.43 ± 0.18 – 2.55 ± 0.2[63] Template:Dagger 9 Template:±;[60] 10 ± 4[61] Large size needs confirmation. Other estimates include 1.9 – 2.4 Template:Jupiter radius, 1.3Template:Snd4.7 Template:Jupiter radius.[62]
(2014Template:Sndpresent) DH Tauri b
(DH Tau b) 		2.7 ± 0.8[24] Template:Dagger 11.5 Template:±[259] Mass being below the deuterium burning limit needs confirmation. Temperature originally given as 2700 – 2800 K.[260] Other sources give the radii: 2.49 Template:Jupiter radius,[30]Template:Efn 2.68 Template:Jupiter radius,[261] and 2.6 ± 0.6 Template:Jupiter radius[22] and masses: 11 ± 3 Template:Jupiter mass,[24] 14.2 Template:± Template:Jupiter mass,[46] 17 ± 6 Template:Jupiter mass[47] and 12 ± 4 Template:Jupiter mass[22]
2010Template:Snd2017 Ditsö̀
(WASP-17b) 		1.74 Template:±[133] – 0.512 ± 0.037[132] First planet discovered to have a retrograde orbit[133] and first to have quartz (crystalline silica, SiO2) in the clouds of an exoplanet.[134] Puffiest and possibly largest exoplanet at the time of discovery.[136] Template:Nowrap[135]
2007Template:Snd2010 TrES-4
(GSC 02620-00648 Ab) 		1.674 ± 0.094[262] – 0.78 ± 0.19[102][68] This planet has a density of 0.2 g/cm3, less than Saturn's 0.7 g/cm3.
(2007Template:Sndpresent) GQ Lupi b
(GQ Lup Ab,
GQ Lup B) 		3.50 Template:±[23] * 1 – 46[263] First confirmed exoplanet candidate to be directly imaged.
(2006Template:Snd2014) DH Tauri b
(DH Tau b) 		1.75[259][260]Template:Efn Template:Dagger 11.5 Template:±[259] Mass being below the deuterium burning limit needs confirmation. Temperature originally given as 2700 – 2800 K.[260]
2006Template:Snd2007 HD 209458 b
("Osiris") 		1.27 ± 0.02[264] – 0.682 Template:±[180] First known transiting exoplanet, first precisely measured planet available, first to have its orbital speed measured, determining its mass directly,[265] one of first two exoplanets (other being HD 189733 Ab) to be observed spectroscopically[181][182] and first to have an atmosphere, containing evaporating hydrogen, and first to have contained oxygen and carbon. First extrasolar gas giant to have its superstorm measured. Nicknamed "Osiris".
(2005Template:Snd2007) GQ Lupi b
(GQ Lup Ab,
GQ Lup B) 		~ 2[266] Template:Dagger 1 – 46[263] First confirmed exoplanet candidate to be directly imaged.
1999Template:Snd2006 HD 209458 b
("Osiris") 		1.27 ± 0.02[264] ← 0.682 Template:±[180] First known transiting exoplanet, first precisely measured radius available, first to have its orbital speed measured, determining its mass directly,[265] and first to have an atmosphere, containing evaporating hydrogen, and first to have contained oxygen and carbon. First extrasolar gas giant to have its superstorm measured. Nicknamed "Osiris".
(1995Template:Snd1999) various Unknown Template:Dagger 0.49Template:Snd8.37 About 20Template:Snd25 planets including Saffar were found within this time span via the radial velocity method, none of them having radius measurements, especially shortly after their discoveries. As expected, Dimidium is larger than Poltergeist, whether one of the additional planets found till 1999 is larger than Dimidium is not clear to this day.
1995Template:Snd1999 Dimidium
(51 Peg b) 		Unknown – 0.46 Template:±[190] First convincing exoplanet discovered orbiting a main-sequence star. Prototype hot Jupiter.
1995Template:Snd1995 Dimidium
(51 Peg b) 		Unknown ← 0.46 Template:±[190] First convincing exoplanet discovered orbiting a main-sequence star. Prototype hot Jupiter.
(1993Template:Snd1995) PSR B1620−26 b
(PSR B1620-26 (AB) b,
"Methuselah") 		Unknown → 2.5 ± 1[267] Likely larger than Poltergeist, but not confirmed as planet until 2003. First circumbinary planet, first planet to be found in a globular cluster and the oldest planet to be discovered (until 2020) at the age of 11.2–12.7 billion years old,[268] hence the nickname, "Methuselah".[267][269]
1992Template:Snd1995 Poltergeist
(Template:Nowrap) 		Unknown ← 0.013 53 ± 0.000 63
(4.3 ± 0.2 Template:Val)[270] 		First confirmed planet ever discovered outside the Solar System together with the less massive Draugr (PSR B1257+12 b), one of three pulsar planets known to be orbiting the pulsar Lich (PSR B1257+12).[271][272] Unclear whether Lich planets are survivors or formed in a second round of planet formation from the remnants of the supernova.
(1989Template:Snd1995) HD 114762 Ab
("Latham's Planet") 		Unknown * Template:Nowrap[273]
~63.2[274] 		Discovered in 1989 by Latham to have a minimum mass of 11.069 ± 0.063 Template:Val (at 90°) and a probable mass of approximately Template:Val (at 10°),[274] making the former planet the first to be spotted,[275] and confirmed in 1991, it was thought to be the first discovered exoplanet until 2019 when it was confirmed to be a low-mass star with the mass of 147.0 Template:± Template:Val,[276] making the planet above the first confirmed exoplanet discovered ever.
(1988Template:Snd1992) Tadmor
(Gamma Cephei Ab,
γ Cep Ab) 		Unknown → 6.6 Template:±[277] First evidence for exoplanet to receive later confirmation. First reported in 1988,[278] making it arguably the first true exoplanet discovered, and independently in 1989,[279] however, retracted in 1992[280] due to the possibility that the stellar activity of the star mimics a planet not allowing a solid discovery claim and then finally confirmed in 2003.[281]
(AntiquityTemplate:Snd1992, 1988 or 1995) Jupiter 1
(Template:Val)[5]
(71 492 km) 		Template:Number sign 1
(Template:Val)[233]
(1.898 125 × 1027 kg) 		Oldest, largest and most massive planet in the Solar System[234] Observations date back to 7th or 8th century BC. Using an early telescope the Galilean moons were discovered in 1610, the planet hosts 95 known moons.
Reported for reference.
For earlier entries, see early speculations and discredited claims.

Notes

Template:Notelist

See also

References

Template:Reflist

Template:Exoplanet

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