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List of exoplanets discovered in 2024

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This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
20 Leonis Minoris b 0.02882+0.00173
−0.00176 		31.15 0.1916±0.0007 radial vel. 48.64±0.07 0.967±0.01 5610±46 [1]
2MASS J05581644–4501559 b 6–12 1043 imaging 94.5 0.259±0.02[2] 3218±158[2] [3]
Barnard's Star b 0.00116±0.00016 3.153 0.0229 ~400 radial vel. 5.9629±0.0004 0.162±0.007 3195±28 The closest exoplanet around a solitary star. Also located in the second closest star system to the Sun, after Alpha Centauri.[4] Not to be confused with the disproved planet Barnard's Star b of 2018, which shared the same name.
BD-10 47 b 0.0133±0.005 0.1529±0.0007 13.476 0.0943±0.0016 493±12 transit 65.89 0.616±0.032 4026±14 Also known as TOI-260 b[5]
BD-14 3065 b 12.11+0.95
−0.91 		1.926±0.094 4.3 0.0646±0.0026 1957±28 transit 1847.4[6][a] 1.4±0.06 6985±90 Located in a triple star system. It orbits the primary component of the system (BD-14 3065 A), a subgiant star. Also known as TOI-4987 b[7]
CI Tauri c 3.6±0.3 25.2±1.8 0.17 radial vel. 522.6±1.3 0.9±0.02 4250±50 Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.[8][9]
CWISE J054129.32–745021.5 b 1.8 6576 imaging 111 Orbits a young red dwarf.[3]
Gaia-4 b 11.8+0.73
−0.66 		571.3+1.4
−1.3 		astrometry + radial vel. 239.2±0.4 0.644+0.025
−0.023 		4034±77 [10]
Gaia20eae b 6 0.062 disk thermal instability 9226+3130
−2021[11] 		1.15 4330±300[11] First object detected by this method[12]
Gaia22dkvLb 0.15 to 5.67+0.39
−0.38 		219+47
−29 to 964+99
−106 		0.48+0.01
−0.07 to 2.08+0.16
−0.18 		microlensing 3097±130 to 5477+326
−391 		0.219+0.056
−0.039 to 1.3+0.04
−0.05 		[13]
Gliese 12 b 0.002769+0.00123
−0.0008 		0.0892±0.0089[b] 12.7 0.066±0.002 315±5 transit 39.65 0.241±0.006 3253±55 [14]
Gliese 238 b 0.05049±0.0012 1.74 0.02123+0.00016
−0.00017 		758+16
−15 		transit 49.6 0.419±0.01 3485±140 Mars-sized exoplanet, one of the smallest exoplanets currently known[15]
Gliese 341 b 0.00227±0.00044 0.0821±0.045 7.577 540 transit 33.9 0.506 3745 Also known as TOI-741 b[16]
Gliese 900 b 10.5 460,000,000[17] 12,000 imaging 68[18] 1.08 (combined) 3976[19] Located in a three-star system.[20] It has the longest orbital time of any exoplanet so far at 1.4 million years.[21]
Gliese 1289 b 0.01655+0.002958
−0.003052 		111.74 0.27±0.01 150 radial vel. 28.88 0.21±0.02 3296±30 [22]
Gliese 4256 b 0.00453±0.00044 0.0962±0.0058 0.238 0.0107[c] 1340±60 transit 66.46±0.03 0.353±0.015 3421±70 An ultra-short period planet orbiting close to the host star's Roche limit. It is expected to undergo tidal disruption in the next hundred million years. Also known as TOI-6255 b[23]
HD 21520 b 0.02486+0.01007
−0.00944 		0.2409±0.008 25.13 0.1726±0.0071 637+13
−12 		transit 258 1.09±0.07 5871±62 [24]
HD 28185 c 6.0±0.6 9088.5+474.5
−401.5 		8.50+0.29
−0.26 		astrometry + radial vel. 127.8±0.1 0.974±0.018 5602±36 Already known to exist in 2022, but was found to be an exoplanet—as opposed to a brown dwarf, in 2024.[25]
HD 48948 b 0.0154±0.000661 7.34013±0.00040 0.0652±0.0005 715±10 radial vel. 54.915±0.0228 0.686+0.020
−0.013 		4593±60 [26]
HD 48948 c 0.0229±0.00220 37.920+0.026
−0.024 		0.1951±0.0016 413±6 radial vel. [26]
HD 48948 d 0.0333±0.00315 150.95+0.45
−0.41 		0.4894±0.0042 262±4 radial vel. Closest Super Earth in habitable zone around a K-dwarf star.[26]
HD 63433 d 0.09573±0.0141 4.21 0.0503±0.0027 1040±40 transit 71.7 0.99±0.03 5688±28 Hot Earth-sized exoplanet[27]
HD 73344 b 0.00939+0.00787
−0.00599 		0.2573+0.0073
−0.0064 		15.6 0.131 911±7 transit 114.7+0.1
−0.0[28] 		1.20±0.02[28] 6028±110[28] The dayside temperature can be as high as 1,066 K if the planet is tidally locked.[29]
HD 73344 c 0.367+0.022
−0.021 		65.936 0.3388+0.0042
−0.0043 		562±4[29] radial vel.

[28]

HD 73344 d 2.55+0.56
−0.46 		5746+120
−150 		6.70+0.25
−0.26 		radial vel. True mass revealed using astrometry.[28]
HD 75898 c 8.49±0.65 6717±40 7.39±0.05 astrometry + radial vel. 263 1.28±0.13 6021±50 [30]
HD 77946 b 0.02637±0.00415 0.24133+0.00767
−0.0071 		6.527 0.072±0.0012 1248+40
−38 		transit 322.7±1 1.17±0.06 6046.0±50.0 Also known as TOI-1778 b[31]
HD 104067 c 0.0415 13.8992+0.0047
−0.0037 		0.1058±0.0013 radial vel. 66.34±0.03 0.82±0.03 4952±100 [32]
HD 111520 b ≥1 1,285,900 ≥200 disk kinematics 352.6±0.7 1.350±0.215[33] 6542±131[33] [34]
HD 118203 c 11.1+1.3
−1 		5070 6.2±0.2 146±3 astrometry + radial vel. 300±0.5 1.353±0.006 5872±20 [35]
HD 128717 b 12.8 1089.2 2.18 astrometry 240±0.5 1.17+0.06
−0.16 		6158±115 [36][37]
HD 134606 e 0.00726+0.00113
−0.0011 		4.32 0.0527±0.0012 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[38]
HD 134606 f 0.01737+0.00232
−0.00229 		26.915 0.1784±0.004 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[38]
HD 148193 Ab 0.0894±0.0135 0.7476±0.017 20.38 0.1577 transit 626±3 1.261±0.183 6351±119 The host star is orbited by two red dwarfs 157 and 1950 AU away.[39] Also known as TOI-1836 Ab
HD 148193 Ac 0.025 0.232+0.01972
−0.01285 		1.773 0.03089±0.0005 2007.6+35.85
−29 		transit Also known as TOI-1836 Ac[40]
HD 156141 b 0.0305±0.0060 0.211±0.005 21.269 0.154±0.003 694.1+11.2
−11.0 		transit 237.726+0.390
−0.389 		1.09+0.034
−0.033 		5814±137 Also known as TOI-1742 b.[41]
HD 222237 b 5.19±0.58 14,890+2120
−1643 		10.8+1.1
−1.0 		astrometry 37.31±0.0 0.76±0.09 4751±139 [42]
HD 278878 b 0.6963±0.0242 0.9225±0.0571 8.71 0.08258 transit 520.8±4.9 0.989±0.126 5597±147 [43]
HIP 39017 b 23.6+9.1
−7.4 		0.87 30681+18627.8
−9496.5 		22.1+8.0
−4.9 		imaging 214.9±0.3 1.52+0.28
−0.26 		7201+142
−112[44] 		May be a brown dwarf. Estimates of the mass vary from 13.8 MJ to 30+31
−12 MJ.[45]
HIP 67522 c 0.731+0.055
−0.057 		14.335 0.1235 915+22
−19 		transit 414[46] 1.2±0.05[46] 5675±75[46] [47]
HS Piscium b 1.44+0.56
−0.44 		3.986 0.0435±0.0017 radial vel. 122.79+0.12
−0.14 		0.69±0.07 4203±116 [48]
Kepler-51e 0.01572 260 timing 2610±50 1.04 6018 Assuming the 2:1 resonance solution, which is the best-fit one, Kepler-51e has a mass of about 5 M🜨 and a period of 260 days.[49]
Kepler-158d 0.038±0.004 0.645088±0.000002 transit 1028±7 0.656+0.073
−0.049 		4895.97 [50]
Kepler-879c 0.04±0.01 0.646716±0.000003 transit 2618+36
−35 		0.974+0.127
−0.104 		5456.75 [50]
Kepler-963c 0.05±0.02 0.919783±0.000003 transit 2516+42
−40 		0.821+0.120
−0.065 		5169.47 [50]
Kepler-1489c 0.045±0.007 0.680741±0.000004 transit 4185+118
−111 		0.977+0.050
−0.062 		5565.53 [50]
Kepler-2003b 0.06±0.01 0.941967±0.000003 transit 3054+85
−81 		0.859+0.126
−0.065 		5050.28 Also known as KOI-4978 b.[50]
K2-419 Ab 0.617±0.047 0.941±0.034 20.358 0.1208+0.0016
−0.0017 		377±11 transit 860±8 0.562±0.024 3711±88 [51]
KMT-2016-BLG-2321Lb 3.58±1.22 3.58±0.81 microlensing 11,670±3980 0.73±0.28 [52]
KMT-2017-BLG-0849Lb 0.0201+0.0245
−0.0097 		2.73+0.68
−0.62 		microlensing 23,540+2670
−3220 		0.19+0.23
−0.09 		[53]
KMT-2017-BLG-1057Lb 0.0739+0.0472
−0.0378 		2.36+0.69
−0.62 		microlensing 21,190+2640
−5280 		0.57+0.37
−0.29 		[53]
KMT-2017-BLG-2331Lb 0.538+0.431
−0.277 		2.14+0.48
−0.42 		microlensing 26,180+2740
−3420 		0.4+0.32
−0.21 		[53]
KMT-2020-BLG-0157Lb 10.71+6.17
−5.61 		11.54+1.61
−2.25 		microlensing 21,744+3032
−4238 		0.58+0.33
−0.30 		[54]
KMT-2021-BLG-2609Lb 0.032+0.044
−0.018 or 0.112+0.152
−0.061 		2.30+0.32
−0.36 		microlensing 24,380+3420
−3810 		0.20+0.27
−0.11 		[55]
KMT-2022-BLG-0303Lb 0.513+0.410
−0.275 		4.81+0.65
−0.76 		microlensing 21,400+2900
−3400 		0.368+0.294
−0.197 		[55]
KMT-2022-BLG-0732Lb 1.12±0.65 4.11+0.74
−1.14 		microlensing 21,712+3879
−6000 		0.54±0.31 [54]
KMT-2022-BLG-1787Lb 6.64+4.98
−3.64 		6.3+0.75
−1.08 		microlensing 24,613+2901
−4038 		0.42+0.32
−0.23 		[54]
KMT-2022-BLG-1852Lb 4.98+5.42
−2.94 		5.03+0.72
−0.92 		microlensing 20,440+2934
−3749 		0.32+0.34
−0.19 		[54]
KMT-2023-BLG-0416Lb 6.15+3.03
−3.2 		3.73+0.56
−0.8 		microlensing 20,640+3100
−4400 		0.61+0.3
−0.32 		The mass of the planet can be as low as 0.042+0.021
−0.022 MJ.[56]
KMT-2023-BLG-0469Lb 0.124+0.092
−0.067 		2.37±0.9 microlensing 23,050+3260
−3910 		0.47±0.36 [57]
KMT-2023-BLG-0735Lb 0.12±0.07 2.75±1 microlensing 20,830+3910
−3260 		0.61±0.34 [57]
KMT-2023-BLG-1431Lb 0.0428+0.0261
−0.0217 		2.3±0.5 or 3.2+0.7
−0.8 		microlensing 22,500+2610
−5540 		0.57+0.33
−0.29 		[58]
KMT-2023-BLG-1454Lb 0.63+0.71
−0.34 		1.18+0.17
−0.18 		microlensing 23,540+3460
−3590 		0.17+0.19
−0.09 		Estimates of the planet's mass varies between 0.3+0.34
−0.16 MJ and 0.77+0.87
−0.42 MJ[56]
KMT-2023-BLG-1642Lb 1.08+1.53
−0.58 		1.41+0.22
−0.27 		microlensing 22,750+3550
−4370 		0.17+0.24
−0.09 		[56]
KMT-2023-BLG-1866Lb 0.00828+0.00132
−0.00214 		2.63+0.37
−0.34 		microlensing 20,240+2840
−1100 		0.51+0.08
−0.13 		Super-Earth planet detected by microlensing.[59]
KMT-2023-BLG-2669 0.02517 microlensing Candidate rogue planet. Might have a mass ranging from sub-Neptune to Saturn-mass, depending on its distance.[60]
LHS 1678 d 0.00289+0.00208
−0.00107 		0.08752±0.0062 4.965 0.04+0.0018
−0.0017 		transit 65 0.345±0.014 3490±50 [61]
M62H b 2.83 <0.683 [d][e] 0.133 0.004908 timing 21,500[62] 1.4 Pulsar planet located in the globular cluster Messier 62.[63] Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b.[64]
MOA-2016-BLG-526Lb 6.93±0.75 2.07±0.35 microlensing 22,490 0.4 [52]
MOA-2022-BLG-563Lb 0.4+0.31
−0.25 		2.25±0.25 microlensing 21,290+3650
−5220 		0.48+0.36
−0.3 		[57]
NGTS-26 b 0.29+0.07
−0.06 		1.33+0.06
−0.05 		4.52 0.0490+0.0038
−0.0032 		1331+85
−72 		transit 3610±100 0.96+0.04
−0.03 		5550±100 Highly inflated planet (density = 0.153 g/cm3)[65]
NGTS-27 b 0.593+0.095
−0.072 		1.396+0.038
−0.035 		3.37 0.0446+0.0026
−0.0036 		1783+104
−88 		transit 3185±55 1.07±0.06 5700±80 [65]
NGTS-29 b 0.393 0.857 69.33 0.347 414 transit 487±1 1.034±0.032 5730±80 [66]
NGTS-30 b 0.96 0.93 98.3 0.408 390 transit 762.5 0.94 5455 Also known as TOI-4862 b[67]
OGLE-2014-BLG-0221Lb 4.35+1.65
−1.91 		3.76+0.96
−1.07 		microlensing 12,000+3690
−3780 		0.69+0.26
−0.30 		[68]
OGLE-2016-BLG-1598Lb 5.91±1.74 2.5±0.88 microlensing 19,270±5670 0.55±0.32 [52]
OGLE-2016-BLG-1800Lb 2.59±1.46 1.88±0.51 microlensing 21,100±3360 0.41±0.22 [52]
OGLE-2017-BLG-0364Lb 0.0642+0.106
−0.034 to 0.805+0.554
−0.437 		1.27+0.49
−0.3 		microlensing 22,300 to 29,300 0.1+0.16
−0.05 to 0.55+0.38
−0.3 		[53] Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11.[64]
OGLE-2017-BLG-0380Lb A 10.5 microlensing 6,980 A pair of rogue planets.[69]
OGLE-2017-BLG-0380Lb B 3.08 microlensing 6,980
OGLE-2017-BLG-0640Lb 1.62+1.64
−0.94 		1.14±0.38 microlensing 21,600+3550
−4730 		0.32+0.32
−0.18 		[70]
OGLE-2017-BLG-1237Lb 3.8+2.49
−1.99 		2.53+0.5
−0.64 		microlensing 19,660+3060
−4990 		0.46+0.3
−0.24 		[70]
OGLE-2017-BLG-1275Lb 5.9±2.2 1.19±0.36 microlensing 25,070±2930 0.63±0.23 Another solution suggests a larger semi-major axis, of 2.09±0.63 AU.[70]
OGLE-2023-BLG-0836Lb 4.36+2.35
−2.2 		3.7+1
−1.2 		microlensing 16,690+4430
−5250 		[f] The planet is located in a binary star system, and is likely to be orbiting both stars in the system.[71]
S1429 b 1.8±0.2 77.51±0.2 0.384±0.4 683±9 radial vel. 2836±26 1.26±0.04 6000±40 Located in the open cluster Messier 67.[72]
SGR 1935+2154 b 0.0318 – 0.0573 0.125 – 0.223 238 or 398 0.85 or 1.19 x-ray bursts 21,500[73]–28,400 1.4 Has a highly-eccentric orbit (0.992) and is tidally disrupted.[74]
SPECULOOS-3 b 0.08716 0.719 0.00733 553 transit 57.9 0.1 2800 Ultra-short period planet[75]
Teegarden's Star d 0.00258±0.00053 26.13 0.0791 ±0.0027 159±3 radial vel. 12.5 0.097±0.01 3034±45 Orbits beyond the habitable zone of its star. Another planet in the system is suspected.[76]
TIC 4672985 b 12.74±1.01 1.026+0.065
−0.067 		69.05 0.33±0.019 517.2+11.3
−11.2 		transit 823.4[77][a] 1.01±0.03 5757+72
−65 		[78]
TIC 46432937 b 3.2±0.11 1.188±0.03 1.44 0.1951±0.0051 872±14 transit 295.5±0.3 0.563±0.029 3572±57 [79]
TIC 139270665 b 0.463 0.645 23.624 0.163 700 transit 618 1.035+0.052
−0.062 		5844+84
−82 		[80][81]
TIC 139270665 c 4.89+0.66
−0.37 		1010+780
−220 		2+0.93
−0.31 		200+18
−35 		radial vel. [81]
TIC 241249530 b 4.98+0.16
−0.18 		1.19±0.04 165.772 transit 1.271+0.061
−0.068 		A planet on a highly-eccentric (e=0.94) and retrograde orbit.[82]
TIC 393818343 b 4.34±0.15 1.087+0.023
−0.021 		16.25 0.129±0.002 805.5+9.6
−9.4 		transit 306.3±1.1 1.082+0.055
−0.056 		5756+57
−66 		Highly eccentric orbit (e=0.6058)[83]
Also known as TOI-6883 b[84]
TIC 393818343 c 0.357±0.132 0.792±0.018 7.8458±0.0023 0.079±0.011 1027.2089± 0.3717 transit [85]
TIC 434398831 b 0.3131+0.0196
−0.0187 		3.6855 0.04641±0.00017 1250±11 transit 698±6 0.992+0.014
−0.018 		5638±50 Young exoplanet located in the Theia 116 association.[86]
TIC 434398831 c 0.5023+0.0259
−0.025 		6.21 0.06572±0.00024 1050±10 transit
TOI-128 b 0.198 4.94 0.054 1345 transit 0.85 6086 [87]
TOI-238 c 0.0211±0.0035 0.1945±0.0161 8.466 0.0749±0.0013 696±15 transit 261.328±0.312 0.79±0.022 5059±89 [88]
TOI-261 b 0.271 3.36 0.035 1722 transit 0.50 5890 [87]
TOI-286 b 0.01425±0.00245 0.1267±0.0089 4.512 0.0503±0.001 979±31 transit 193 0.832±0.049 5152±12 There are three available models to explain the disagreement between the radial velocity and transit measurements.[g][5]
TOI-286 c 0.01171±0.00698 0.1677±0.0107 39.36 0.213±0.004 475±15 transit 193 0.832±0.049 5152±12 [5]
TOI-329 b 0.1271 5.71 0.064 transit 927.1 0.98 5560 Radius of the host star is significantly larger compared to mass (1.61 R☉)[89]
TOI-406 b 0.00654+0.00072
−0.00069 		0.1178±0.0107 3.307 0.0322±0.0013 584±22 transit 101±0.7 0.408+0.046
−0.042 		3392±44 [90]
TOI-406 c 0.02067±0.003 0.1846±0.0143 13.18 0.0809±0.003 368±14 transit 101±0.7 0.408+0.046
−0.042 		3392±44 [90]
TOI-480 b 0.0654 6.866 transit 177.8 1.2 6,212 [91]
TOI-603 b 0.1495±0.0431 0.7075±0.018 16.18 0.1281 transit 671.3±5.15 1.072±0.136 5901±130 [92]
TOI-654 b 0.211 1.53 0.021 749 transit 0.53 3433 [87]
TOI-663 b 0.0140±0.00204 0.203±0.00892 2.599 0.0295±0.0011 674±30 transit 209.490±0.587 0.514±0.012 3681±70 [93]
TOI-663 c 0.0115±0.00305 0.202±0.00892 4.696 0.0437±0.0016 553±24 transit
TOI-663 d <0.0164 0.171±0.0116 7.103 0.0576+0.0021
−0.0022 		482±21 transit
TOI-757 b 0.033±0.007 0.223±0.001 17.468 0.122±0.002 641±10 transit 196.9+1
−0.7 		0.8±0.04 5278±63 [94]
TOI-762 Ab 0.251±0.042 0.744±0.017 3.472 0.03418 555±6 transit 322±0.7 0.442±0.025 3266±36 Located in a binary star system.[79]
TOI-782 b <0.06 0.244±0.008 8.024 0.0578±0.0018 398±6–435±6[h] transit 170.2±0.2 0.397±0.01 3370+29
−32 		[95]
TOI-815 b 0.0239±0.0047 0.2622±0.0044 11.197 0.0903+0.0018
−0.0019 		686+13
−14 		transit 193.76±0.15 0.776±0.036 4869±77 The host star is part of a binary star system with a red dwarf companion[96]
TOI-815 c 0.0739±0.00755 0.2337+0.0089
−0.008 		34.976 0.193±0.004 469±9 transit
TOI-880 b 0.248 2.57 0.034 1163 transit 0.81 4935 [87]
TOI-907 b 0.858 4.58 0.055 1847 transit 1.07 6272 [87]
TOI-1135 b 0.062+0.033
−0.031 		0.805±0.02 5.13±0.27 0.082±0.003 1198.9±21.3 transit 371.4±0.5 1.125±0.032 6122±25 [97]
TOI-1173 Ab 0.08213±0.00598 0.723±0.015 7.064 0.0702±0.0012 863.9±9.8 transit 430.85[98][a] 0.911+0.028
−0.03 		5350±340 Low-density planet located in a wide binary system.[99]
TOI-1184 b 0.021±0.007 0.215+0.009
−0.013 		5.748 0.056±0.001 715.5+13.7
−14.1 		transit 191.110±0.254 0.73+0.024
−0.025 		4616±104 [41]
TOI-1199 b 0.239±0.02 0.938±0.025 3.671 0.04988±0.0009 1486±20 transit 805±2.6 1.23±0.07 5710±40 [100]
TOI-1224 b 0.1877+0.0084
−0.0081 		4.178 0.0355+0.0017
−0.0034 		541+26
−14 		transit 121.5 0.4±0.01 3326±66 Located in the MELANGE-5 association, which is 200 Myr old. The host star may be binary.[101]
TOI-1224 c 0.2573±0.0087 17.945 transit
TOI-1248 b 0.0862+0.0113
−0.0110 		0.607+0.0104
−0.0107 		4.360 0.051±0.001 952.1+13.5
−14.3 		transit 550.340+1.963
−1.947 		0.90±0.03 5205±120 [41]
TOI-1249 b 0.0374+0.0164
−0.0160 		0.2918+0.0274
−0.0167 		13.079 0.109±0.002 727+12
−11 		transit 455.0+1.8
−1.7 		0.952+0.167
−0.082 		5453+76
−160 		[102]
TOI-1266 d 0.01158+0.00330
−0.00349 		32.5 0.1513±0.0024 288±5 radial vel. + timing 117.4±0.1 0.437±0.021 3563±77 [103]
TOI-1269 b 0.020±0.009 0.2142+0.0134
−0.0066 		4.253 0.0496+0.0009
−0.0010 		1005+15
−14 		transit 561.4±2.3 0.969+0.154
−0.104 		5517+107
−143 		[104]
TOI-1273 b 0.222±0.015 0.99±0.2 4.631 0.0549±0.001 1211±15 transit 574±1.3 1.06±0.06 5690±40 [100]
TOI-1279 b 0.0334±0.0079 0.237+0.0123
−0.0095 		9.61419±0.00004 0.085±0.002 759+11.8
−11.7 		transit 349.167+0.933
−0.926 		0.88±0.03 5457±127 [41]
TOI-1294 b 0.1957±0.016 0.8199±0.0277 3.915 0.0489 transit 1052±7 1.02±0.13 5714±126 [105]
TOI-1294 c 0.467±0.053 160.1±2.5 0.581 radial vel. 1052±7 1.02±0.13 5714±126 [106]
TOI-1347 b 0.0349±0.0038 0.161±0.009 0.847 1400±40 transit 480.8±2 0.913±0.033 5464±100 Ultra-short period planet[107]
TOI-1347 c 0.0088±0.0072 0.143±0.009 4.842 1000±25 transit [107]
TOI-1386 b 0.148+0.019
−0.018 		0.54+0.018
−0.016 		25.838 0.1732+0.0027
−0.0033 		676.4+10
−8.3 		transit 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[108]
TOI-1386 c 0.309±0.038 227.6+4.6
−4 		0.739+0.015
−0.016 		327.4+5.3
−4.6 		radial vel. 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[108]
TOI-1408 c 0.0239±0.0006 0.1981±0.0054 2.1664±0.0001 0.3587±0.0008 timing 435.6±0.7 1.31±0.01 6117±31 [109]
TOI-1410 b 0.262 1.22 0.020 1396 transit 0.72 4635 [87]
TOI-1437 b 0.0302+0.0123
−0.0104 		0.200+0.021
−0.020 		18.841 0.140+0.018
−0.017 		794±14[110] transit + radial vel. 336 1.10±0.10 6008±113 [111]
TOI-1439 b 0.121±0.018 0.379+0.021
−0.015 		27.644 0.192±0.004 748.4+10.9
−13.1 		transit 751.158+7.691
−7.537 		1.24 5857±60 [112]
TOI-1443 b <0.0944 0.2055+0.0113
−0.0090 		23.541 0.147±0.003 521+14
−12 		transit 279.9±0.7 0.89+0.14
−0.09 		5236+111
−140 		[113]
TOI-1448 b <0.0613 0.245±0.006 8.112 0.0567±0.0015 389±5–426±6[h] transit 240±0.3 0.372±0.009 3412+28
−32 		[95]
TOI-1450 Ab 0.00396±0.0004 0.1±0.004 2.04 722±35 transit 73.2±0.1 0.48±0.024 3437±86 Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement.[114]
TOI-1450 Ac 0.0048±0.0006 5.07 533±26 radial vel. Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab.[114]
TOI-1451 b 0.0478±0.0088 0.233+0.0120
−0.0092 		16.538 0.127±0.003 723.3+12.4
−12.2 		transit 299.856+0.710
−0.707 		1.00+0.04
−0.03 		5800±139 [41]
TOI-1472 b 0.0519±0.0160 0.371+0.0140
−0.0113 		6.36381±0.00091 0.065±0.001 811.1+11.2
−10.8 		transit 397.389+4.341
−4.250 		0.92±0.02 5103+119
−144 		[41]
TOI-1669 b <0.0409 0.2049+0.0091
−0.0080 		2.68 0.0376±0.0007 1285+22
−21 		transit 362.9±1.2 1.00±0.05 5542±100 [115]
TOI-1683 b 0.236 3.06 0.037 929 transit 0.69 4402 [87]
TOI-1691 b 0.0459+0.0170
−0.0167 		0.3181+0.0096
−0.0078 		16.737 0.126±0.003 703+13
−12 		transit 363.5±1.2 1.031+0.159
−0.127 		5759+209
−165 		[116]
TOI-1723 b 0.2937+0.0127
−0.0114 		13.72641±0.00046 0.114±0.002 783+15
−14 		transit 328.5±1.0 1.035+0.147
−0.107 		5777+149
−101 		[117]
TOI-1751 b 0.0538±0.0101 0.2489±0.0259 37.468 0.2115±0.0024 820 transit 370.3±0.3 1.15±0.17 6116±22 The host star is metal-poor ([Fe/H] = –0.40 dex).[118]
TOI-1753 b 0.0522±0.0164 0.221+0.009
−0.007 		5.385 0.059±0.001 1005.4+18.3
−17.6 		transit 739.302+8.907
−8.699 		0.95±0.03 5620±134 [41]
TOI-1758 b 0.3174+0.0203
−0.0127 		20.705 0.138±0.003 551+9
−8 		transit 315.1±1.1 0.88+0.12
−0.09 		5169+95
−148 		[119]
TOI-1775 b 0.302±0.047 0.718+0.0128
−0.0114 		10.241 0.080±0.002 707.9+8.6
−8.3 		transit 486.736+3.108
−3.072 		0.92+0.01
−0.02 		5283±116 [41]
TOI-1776 b 0.1085+0.0080
−0.0069 		2.8 0.0378+0.0007
−0.0008 		1269±21 transit 146 1.02+0.11
−0.14 		5724±105 [120]
TOI-1798 b 0.126 0.44 0.011 2122 transit 369.147+1.008
−1.005 		0.86 5165 [87]
TOI-1798 c 0.018+0.003
−0.002 		0.125+0.006
−0.005 		0.438 0.0107±0.0002 1935.8+25.2
−25.9 		transit [41]
TOI-1799 b 0.013+0.005
−0.006 		0.1269+0.0932
−0.0880 		7.085738±0.000083 0.071±0.001 923+15
−14 		transit[ 203 1.01+0.14
−0.12 		5690+121
−124 		[121]
TOI-1806 b 0.304 15.15 0.088 337 transit 0.39 3272 [87]
TOI-1823 b 0.212+0.025
−0.026 		0.673+0.030
−0.022 		38.80±0.01 0.212±0.004 423.6+10.4
−8.7 		transit 233.677+0.375
−0.374 		0.84±0.03 4926±113 [41]
TOI-1824 b 0.0582±0.01 0.2346±0.0133 22.8 0.149±0.003 577±19 transit 192.3 0.85±0.05 5180±110 High-density planet, situated in the small group of "overdense sub-Neptunes". TOI-1824 has also a red dwarf companion named TIC 142387022.[122]
TOI-1828 b 0.1841±0.012 0.769±0.017 9.09 0.0859 transit 1208±8 1.04±0.13 5809±127 [123]
TOI-1855 b 1.133±0.096 1.65+0.52
−0.37 		1.364 0.02398+0.00037
−0.00036 		1700±20 transit + radial vel. 576.3±4.6 0.987+0.058
−0.045 		5359+89
−83 		[124]
TOI-1883 b 0.4953±0.0460 4.506 524.9 transit 376±3 0.492±0.02 3477±157 [125][126]
TOI-1885 b 1.624±0.103 1.219±0.037 6.544060±0.000006 transit 1826.773+21.464
−20.982 		6527±98 [112]
TOI-1898 b 0.4059+0.0220
−0.0252 		0.838+0.021
−0.028 		45.52 0.269±0.005 674.5+11.6
−11.8 		transit 259.7±1.4 1.24+0.22
−0.16 		6304+139
−144 		[127]
TOI-2019 b 0.109±0.0132 0.505±0.0250 15.3444±0.0055 transit 645.812+2.684
−2.665 		5590 [112]
TOI-2107 b 0.83±0.11 1.211±0.035 2.454 0.0315+0.0006
−0.00067 		1397±20 transit + radial vel. 767.4+6.2
−5.9 		0.961+0.049
−0.054 		5627+94
−93 		[124]
TOI-2120 b <0.02139 0.1893±0.0056 5.8 0.0377±0.0013 351±6–384±6[h] transit 104.9 0.211±0.005 3131±30 [95]
TOI-2128 b 0.014±0.006 0.186+0.008
−0.007 		16.341 0.127±0.003 780.5+14.8
−14.4 		transit 119.2±0.1 1.1+0.15
−0.12 		5991+114
−90 		[128]
TOI-2266 b 0.1374±0.008 2.326 0.02±0.002 550±47 transit 168.6±0.2 0.23±0.02 3240±160 [129]
TOI-2274 b 2.679 771 transit 159.9±0.2 0.612±0.02 3943±157 [130][126]
TOI-2368 b 0.65±0.18 0.967+0.036
−0.031 		5.175 0.05649±0.001 1000+44
−30 		transit 685±3.9 0.897+0.048
−0.049 		5360+230
−170 		[124]
TOI-2373 b 9.3±0.2 0.93±0.02 13.337 0.112±0.001 860±10 transit 1617±33 1.041+0.032
−0.028 		5651±180 [131]
TOI-2374 b 0.1782+0.011
−0.0134 		0.6075±0.0268 4.314 0.0471 <885±22 transit 439±3 0.75±0.01 4802±97 [132]
TOI-2379 b 5.76±0.20 1.046±0.023 5.4693827±0.0000023 0.05263±0.00091 624±12 transit 689.5±3.6 0.645±0.033 3707±58 [133]
TOI-2384 b 1.966±0.059 1.025±0.021 2.13570304±0.00000038 0.02793±0.00023 889.7±5.0 transit 609.9±4.9 0.635±0.016 3943±14 [133]
TOI-2416 b 3+0.1
−0.09 		0.88±0.02 8.275 0.0831±0.0007 1080±10 transit 1767±261 1.118+0.029
−0.027 		5808±80 [131]
TOI-2420 b 0.927+0.085
−0.079 		1.340+0.074
−0.072 		5.8426 0.0684+0.0067
−0.0059 		1571.6+60.8
−64 		transit 1450[a] 1.158±0.098 [134]
TOI-2485 b 2.412+0.088
−0.087 		1.083±0.045 11.235 0.1093+0.0055
−0.0057 		1134+27
−25 		transit 1296[a] 1.163±0.053 [134]
TOI-2524 b 0.64±0.04 1+0.02
−0.03 		7.186 0.073±0.0007 1100±20 transit 1399±36 1.007+0.032
−0.029 		5831±80 [131]
TOI-2529 b 2.34±0.2 1.03±0.05 64.5949±0.0003 0.327±0.02 636±15.7 transit 965.8+14
−13.7 		1.11+0.02
−0.02 		5802+60
−52 		[78]
TOI-2714 b 0.717+0.104
−0.101 		1.224+0.0625
−0.0598 		2.499 0.036±0.002 1603±65 transit 1930±16 1.07±0.06 5665±115 [135]
TOI-2768 b 0.2688±0.0313 1.508 855 transit 255.8±0.6 0.63+0.06
−0.10 		4008+124
−137 		[136][126]
TOI-2981 b 2.007±0.104 1.1955±0.0375 3.602 0.048±0.002 1358±39 transit 1741±16 1.03±0.06 5940±75 [135]
TOI-3071 b 0.2146±0.011 0.6388+0.0509
−0.0455 		1.267 0.0249 <2155±40 transit 1582±29 1.29±0.02 6177±62 [132]
TOI-3261 b 0.0953±0.0076 0.3408+0.0375
−0.0312 		0.883 0.01714 1722+26
−18 		transit 972.3+2.3
−3.1 		0.861+0.02
−0.03 		4995±47 Ultra-hot Neptune[137]
TOI-3321 b 0.554±0.076 1.388+0.070
−0.064 		3.652 0.047±0.001 1616±30 transit 928+10.8
−10.4 		1.041+0.084
−0.068 		5850±140 [124]
TOI-3353 b 0.238 4.67 0.060 1264 transit 1.33 6365 [87]
TOI-3568 b 0.083±0.003 0.473±0.024 4.42 0.0485±0.0004 899±12 transit 645±2 0.78±0.02 4969±45 [138]
TOI-3894 b 0.85±0.15 1.358+0.054
−0.052 		4.335 0.0543±0.0014 1519±22 transit 1343+12.7
−12.4 		1.138+0.089
−0.075 		6000±110 [124]
TOI-3919 b 3.88±0.023 1.1±0.05 7.433 0.0795±0.0016 1200±15 transit 1973+28.7
−28.4 		1.208+0.067
−0.07 		6100±110 [124]
TOI-4153 b 1.15±0.38 1.438±0.045 4.617 0.06311+0.00084
−0.00096 		1670+30
−40 		transit 1366±11.4 1.572+0.064
−0.071 		6860+150
−180 		[124]
TOI-4336 Ab 0.017+0.013
−0.007 		0.1891 16.337 0.0872+0.0013
−0.0014 		308±9 transit 73.15 0.331±0.015 3298+75
−73 		Located in a triple hierarchical stellar system.[139]
TOI-4364 b 0.1793+0.0089
−0.0082 		5.424 0.04753+0.00053
−0.00054 		488±4 transit 142.9±0.1 0.487+0.017
−0.016 		3528+33
−20 		Located in the Hyades.[140]
TOI-4379 b 1.113±0.071 1.489±0.079 3.254 transit 2013+38
−39 		1.372+0.037
−0.105 		6020±100 [141]
TOI-4438 b 0.017±0.0035 0.2248±0.0116 7.44 0.0534±0.009 400±50 transit 98 0.368±0.021 3422±81 [142]
TOI-4443 b 0.153 1.85 0.030 1639 transit 1.05 5834 [87]
TOI-4495 b 0.324 5.18 0.062 1383 transit 1.17 6156 [87]
TOI-4527 b 0.0812 0.40 0.008 1363 transit 0.48 3702 [87]
TOI-4562 c 5.77+0.37
−0.56 		3990+201
−192 		5.219±0.002 timing 1131±12[143] 1.218+0.054
−0.048[143] 		6096±32[143] [144]
TOI-4602 b 0.227 3.98 0.051 1380 transit 1.12 6012 [87]
TOI-4633 c 0.15+0.087
−0.075 		0.285+0.018
−0.017 		271.94 0.847±0.061 290 transit 310.4±0.78 1.05±0.06 or 1.1±0.06[i] 5600±50 or 5800±50 [i] Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.[145]
TOI-4914 b 0.714±0.041 1.1482±0.0321 10.6 0.098±0.003 894±20 transit 951±5 1.03±0.06 5805±62 [135]
TOI-5005 b 0.103±0.018 0.558±0.021 6.309 0.06614±0.0045 1040±20 transit 685±2 0.97±0.02 5749±61 [146]
TOI-5076 b 0.0503±0.00629 0.285±0.00892 23.445±0.001 615±20 transit 270.057±0.326 0.80±0.07 5070±143 [147]
TOI-5082 b 0.227 4.24 0.051 1165 transit 1.00 5670 [87]
TOI-5218 b 0.799+0.393
−0.359 		0.879±0.034 4.291 0.0469±0.0006 783±21 transit 1243±11 0.739±0.03 4230±88 [51]
TOI-5232 b 2.34±0.16 1.14+0.05
−0.045 		4.097 0.0599±0.001 1772+40
−45 		transit 1985+28
−27 		1.389+0.068
−0.075 		6500+180
−190 		[124]
TOI-5301 b 3.65±0.4 1.18+0.08
−0.07 		5.859 0.0726+0.0013
−0.0024 		1655±40 transit 1914+59
−55 		1.483+0.081
−0.14 		6240±160 [124]
TOI-5319 b 0.33427±0.0551 4.079 695 transit 199.4±0.7 0.5±0.1 3580+107
−141 		[148][126]
TOI-5388 b 0.169 2.59 0.024 601 transit 0.29 3495 [87]
TOI-5616 b 0.802+0.371
−0.384 		0.961+0.048
−0.042 		2.003 0.0272±0.0003 939±27 transit 1249±14 0.666±0.025 3996±88 [51]
TOI-5634 Ab 0.576+0.406
−0.346 		0.923+0.056
−0.050 		2.2035 0.0272±0.0003 837±34 transit 1051+20
−18 		0.556±0.022 3896±88 [51]
TOI-5688 Ab 0.390+0.074
−0.077 		0.920+0.053
−0.062 		2.948 0.03379+0.00046
−0.00045 		742±18 transit 735.8+4.2
−4.9 		0.60±0.02 3713±59 [149]
TOI-5713 b 0.0135+0.0053
−0.0035 		0.1579+0.0152
−0.0125 		10.44 0.06008±0.00046 347±3 transit 133.7[a] 0.265±0.006 3228±41 [150]
TOI-5720 b 0.0041+0.0029
−0.0015 		0.0972±0.0062 1.434 0.0183±0.0003 708±19 transit 116.9±0.1 0.383±0.019 3325±75 [151]
TOI-6002 b 0.0119+0.005
−0.0031 		0.1454+0.0107
−0.017 		10.905 0.05722±0.00044 321+7
−5 		transit 104.6[a] 0.21 3241+80
−60 		[150]
TOI-6008 b 0.00346+0.0023
−0.0011 		0.0919±0.0045 0.858 0.0108±0.0002 707±19 transit 75.05±0.03 0.23±0.011 3075±75 Ultra-short period planet[151]
TOI-6029 b 1.635±0.032 1.284±0.098 5.7987±0.0004 transit 1946+37
−36 		1.548+0.027
−0.085 		6223±100 [141]
TOI-6034 b 0.798±0.075 1.063±0.042 2.576 0.02949+0.00043
−0.00044 		714±21 transit 385 0.514+0.025
−0.022 		3635±88 [51]
TOI-6086 b 0.00346+0.00362
−0.00176 		0.1053±0.0062 1.389 0.0154±0.0002 634±16 transit 102.6 0.254±0.013 3200±75 [151]
TOI-6383 Ab 1.04±0.094 1.008+0.036
−0.033 		1.791 0.02292±0.00037 745±23 transit 561+3.0
−2.7 		0.458±0.011 3444±88 [152]
TOI-6651 b 0.1919+0.0239
−0.0249 		0.4541+0.0241
−0.0232 		5.057 0.06330+0.00078
−0.00072 		1493+14
−15 		transit 690±3[153][a] 1.323+0.050
−0.045 		5940±110 [154]
TOI-7041 b 0.36±0.16 1.02±0.03 9.691±0.006 transit 1431±10 1.12±0.02 4640±10 [155]
V808 Aurigae b [ru] 6.8±0.7 4109±362 timing 698±13 0.9±0.1 The planet's host star is a polar. The mass value for the planet is only a minimum mass.[156]
VHS J183135.58-551355.9 6.5±1.5 1.42+0.04
−0.03 		1085±60 imaging 180.6±17.9 Free-floating planet[157]
WASP-132d 5.16±0.52 1816.6±44.4 2.71±0.12 107+11
−18 		radial vel. 401.53±1.86 0.789±0.039 4686±99 [158]
Wolf 327 b 0.00796±0.00145 0.1106±0.0054 0.573 0.01 996±22 transit 92.9 0.405±0.019 3542±70 Ultra-short period planet[159]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]


Notes

[edit]
  1. ^ a b c d e f g h Distance calculated from parallax
  2. ^ The radius is the same as that of the Earth, with an uncertainty of 10%
  3. ^ Calculated using a/R⋆ (ratio between Semi-major axis and host star radius)
  4. ^ Radius calculated with mass and lower limit in density in the equation d=(1.89813*10^(30)*m)/((4/3)*π*r3), where d is density (in g/cm3), m is the mass (in MJ and r is the radius (in centimeters). Should be divided by 7.1492×109 to convert from centimeters to RJ
  5. ^ Since the density is only a lower limit, the radius is an upper limit.
  6. ^ The planet is located in a two-star system, with masses of 0.78+0.38
    −0.36     M☉     and 0.56+0.3
    −0.28     M☉    . There is a large chance that it is orbiting both stars in the system, so the "host star mass" would be 0.78+0.38
    −0.36     M☉     + 0.56+0.3
    −0.28     M☉    . However, there is a small chance that is orbiting only one of the stars in the system.
  7. ^ The transit observations of TOI-286 indicate periodic transit signals of 4.5 and 39.4 days. While this, radial velocity measurements with ESPRESSO do not immediately show evidence for periodic signals at either periods.
  8. ^ a b c Assuming albedos of 0.3 and 0 respectively.
  9. ^ a b It is not known which of the stars the planet orbits.


References

[edit]
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