List of exoplanets discovered in 2024

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

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

Lists of exoplanets

Lists of exoplanets by year of discovery


Notes

  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

  1. ^ Gupta, Arvind F.; Luhn, Jacob K.; Wright, Jason T.; Mahadevan, Suvrath; Robertson, Paul; Krolikowski, Daniel M.; Ford, Eric B.; Cañas, Caleb I.; Halverson, Samuel (18 September 2024), The NEID Earth Twin Survey. I. Confirmation of a 31-day planet orbiting HD 86728, arXiv:2409.12315
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