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

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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]
82 G. Eridani d | 0.01831±0.00179  |  | 647.6+2.5
−2.7 | 1.354±0.007  |  | radial vel.  | 19.7  | 0.813+0.018
−0.012 | 5490±70  | Orbiting within the habitable zone of its host star.[2][3]
2MASS J05581644–4501559 b  | 6–12  |  |  | 1043  |  | imaging  | 94.5  | 0.259±0.02[4] | 3218±158[4] | [5]
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.[6] Not to be confused with the disproved planet Barnard's Star b of 2018, which shared the same name.
BD+00 444b  | 0.0151±0.0035  | 0.2108±0.0059  | 15.669  | 0.105±0.025  | 519±6  | transit  | 77.99±0.036  | 0.642±0.026  | 4375±65  | [7]
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[8]
BD-14 3065 b  | 12.11+0.95
−0.91 | 1.926±0.094  | 4.3  | 0.0646±0.0026  | 3520±130  | transit  | 1847.4[9][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[10]
BX Trianguli b | 7.5  |  | 3923  | 4.5  |  | timing  | 192±7  | 0.858 (combined)  | 3735 + 3359  | [11][12]
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.[13][14]
CWISE J054129.32–745021.5 b  | 1.8  |  |  | 6576  |  | imaging  | 111  |  |  | Orbits a young red dwarf.[5]
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  | [15]
Gaia20eae b | 6  |  |  | 0.062  |  | episodic accretion outbursts  | 9226+3130
−2021[16] | 1.15  | 4330±300[16] | [17]
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 |  | [18]
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  | [19]
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[20]
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[21]
Gliese 900 b | 10.5  |  | 460,000,000[22] | 12,000  |  | imaging  | 68[23] | 1.08 (combined)  | 3976[24] | Located in a three-star system.[25] It has the longest orbital time of any exoplanet so far at 1.26 million years.[22]
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  | [26]
Gliese 4256 b | 0.00453±0.00044  | 0.0962±0.0058  | 0.238  | 0.0054[27] | 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[28]
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  | [29]
HD 28185 c | 5.68+0.44
−0.36 |  | 9224+332
−223 | 8.54+0.21
−0.14 |  | 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.[30][31]
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  | [32]
HD 48948 c | 0.0229±0.00220  |  | 37.920+0.026
−0.024 | 0.1951±0.0016  | 413±6  | radial vel.  | [32]
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.[32]
HD 57625 b  | 8.43+1.10
−0.91 |  | 4843+306
−167 | 5.70+0.14
−0.13 |  | radial vel. + astrometry  | 144.3  | 1.040+0.078
−0.080 | 5962±43  | True mass revealed using astrometry.[33]
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[34]
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[35] | 1.20±0.02[35] | 6028±110[35] | The dayside temperature can be as high as 1,066 K if the planet is tidally locked.[36]
HD 73344 c | 0.367+0.022
−0.021 |  | 65.936  | 0.3388+0.0042
−0.0043 | 562±4[36] | radial vel.  |

[35]

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.[35]
HD 75898 c | 8.49+0.65
−0.63 |  | 6717±40  | 7.39±0.05  |  | astrometry + radial vel.  | 263  | 1.295±0.015  | 6122±52  | [37][38]
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[39]
HD 101581 b |  | 0.0877  | 4.47  |  |  | transit  | 41.7  | 0.740±0.087  | 4675±53  | Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.[40]
HD 101581 c |  | 0.0925  | 6.21  |  |  | transit  | 41.7  | 0.740±0.087  | 4675±53  | Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.[40]
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  | [41]
HD 111520 b | ≥1 |  | 1,285,900  | ≥200 |  | disk kinematics  | 352.6±0.7  | 1.350±0.215[42] | 6542±131[42] | [43]
HD 115587 b  | 0.7  | 0.49  | 372  |  |  | transit  | 356.2±0.5  | 1.248±0.190  | 6324±129  | [44][45]
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  | [46]
HD 128717 b  | 12.8  |  | 1089.2  | 2.18  |  | astrometry  | 240±0.5  | 1.17+0.06
−0.16 | 6158±115  | [47][48]
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 | [49]
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 | [49]
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.[50] 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[51]
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.[52]
HD 222237 b | 5.19±0.58  |  | 14,890+2120
−1643 | 10.8+1.1
−1.0 |  | astrometry + radial vel.  | 37.31±0.0  | 0.76±0.09  | 4751±139  | [53]
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  | [54]
HIP 11696 b  | 4 to 16  |  |  | 2.5 to 28  |  | astrometry  | 160.8  | 1.40±0.07  | 6298[55] | [56]
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[57] | May be a brown dwarf. Estimates of the mass vary from 13.8 MJ to 30+31
−12 MJ.[58]
HIP 47110 b  | 3 to 10  |  |  | 3 to 30  |  | astrometry  | 126.2  | 0.98±0.05  | 4529[55] | [56]
HIP 67522 c |  | 0.731+0.055
−0.057 | 14.335  | 0.1235  | 915+22
−19 | transit  | 414[59] | 1.2±0.05[59] | 5675±75[59] | [60]
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  | [61]
IRAS 04125+2902 b | 0.3  | 0.955  | 8.83  |  |  | transit  | 520[62] | 0.7  | 3720[63] | [64] The youngest transiting exoplanet discovered to date.[65]
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 ME and a period of 260 days.[66]
Kepler-158d  |  | 0.038±0.004  | 0.645088±0.000002  |  |  | transit  | 1028±7  | 0.656+0.073
−0.049 | 4895.97  | [67]
Kepler-879c  |  | 0.04±0.01  | 0.646716±0.000003  |  |  | transit  | 2618+36
−35 | 0.974+0.127
−0.104 | 5456.75  | [67]
Kepler-963c  |  | 0.05±0.02  | 0.919783±0.000003  |  |  | transit  | 2516+42
−40 | 0.821+0.120
−0.065 | 5169.47  | [67]
Kepler-1489c  |  | 0.045±0.007  | 0.680741±0.000004  |  |  | transit  | 4185+118
−111 | 0.977+0.050
−0.062 | 5565.53  | [67]
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.[67]
K2-360 c | 0.0479±0.0024  |  | 9.797±0.030  | 0.0883±0.0016  | 912±18  | radial vel.  | 762.59±19.05  | 0.958±0.048  | 5679+60
−39 | [68]
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  | [69]
KMT-2016-BLG-2321Lb  | 3.58±1.22  |  |  | 3.58±0.81  |  | microlensing  | 11,670±3980  | 0.73±0.28  |  | [70]
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 |  | [71]
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 |  | [71]
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 |  | [71]
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 |  | [72]
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 |  | [73]
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 |  | [73]
KMT-2022-BLG-0732Lb  | 1.12±0.65  |  |  | 4.11+0.74
−1.14 |  | microlensing  | 21,712+3879
−6000 | 0.54±0.31  |  | [72]
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 |  | [72]
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 |  | [72]
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.[74]
KMT-2023-BLG-0469Lb  | 0.124+0.092
−0.067 |  |  | 2.37±0.9  |  | microlensing  | 23,050+3260
−3910 | 0.47±0.36  |  | [75]
KMT-2023-BLG-0735Lb  | 0.12±0.07  |  |  | 2.75±1  |  | microlensing  | 20,830+3910
−3260 | 0.61±0.34  |  | [75]
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 |  | [76]
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[74]
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 |  | [74]
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.[77]
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.[78]
KMT-2024-BLG-1044L  | 0.0244+0.0378
−0.0127 or 0.0430+0.0479
−0.0211 |  |  |  |  | microlensing  | 21,900+3200
−3400 or 23,300±3100  | 0.069+0.080
−0.036 or 0.131+0.146
−0.064 |  | Host star is either a brown dwarf or a red dwarf.[79]
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  | [80]
M62H b | 2.83  | <0.683 [c][d] | 0.133  | 0.004908  |  | timing  | 21,500[81] | 1.4  |  | Pulsar planet located in the globular cluster Messier 62.[82] Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b.[83]
MOA-2016-BLG-526Lb  | 6.93±0.75  |  |  | 2.07±0.35  |  | microlensing  | 22,490  | 0.4  |  | [70]
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 |  | [75]
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)[84]
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  | [84]
NGTS-29 b  | 0.393  | 0.857  | 69.33  | 0.347  | 414  | transit  | 487±1  | 1.034±0.032  | 5730±80  | [85]
NGTS-30 b | 0.96  | 0.93  | 98.3  | 0.408  | 390  | transit  | 762.5  | 0.94  | 5455  | Also known as TOI-4862 b[86]
NGTS-31 b  | 1.12±0.12  | 1.61±0.16  | 4.162734±0.000004  | 0.064±0.008  | 1410±20  | transit  | 2780+323
−326 | 0.96+0.11
−0.05 | 5710±70  | [87]
NGTS-32 b  | 0.57±0.05  | 1.42±0.03  | 3.31211±0.00002  | 0.044±0.001  | 1750±20  | transit  | 2760+33
−23 | 1.07+0.06
−0.04 | 5680±60  | [87]
NGTS-33 b  | 3.6±0.3  | 1.64±0.07  | 2.828  | 0.048±0.02  | 1991±21  | transit  | 1430±23  | 1.60±0.11  | 7437±72  | [88]
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 |  | [89]
OGLE-2015-BLG-1609Lb  | 0.0059+0.0122
−0.0031 to +0.24
−0.90 |  |  |  |  | microlensing  | 10,100+8500
−6800 | 0.025+0.050
−0.012 to 0.17+0.63
−0.12 |  | [90]
OGLE-2016-BLG-1598Lb | 5.91±1.74  |  |  | 2.5±0.88  |  | microlensing  | 19,270±5670  | 0.55±0.32  |  | [70]
OGLE-2016-BLG-1800Lb  | 2.59±1.46  |  |  | 1.88±0.51  |  | microlensing  | 21,100±3360  | 0.41±0.22  |  | [70]
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 |  | [71] Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11.[83]
OGLE-2017-BLG-0380Lb A  | 10.5  |  |  |  | microlensing  | 6,980  |  | A pair of rogue planets.[91]
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 |  | [92]
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 |  | [92]
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.[92]
OGLE-2023-BLG-0836Lb  | 4.36+2.35
−2.2 |  |  | 3.7+1
−1.2 |  | microlensing  | 16,690+4430
−5250 | [e] |  | The planet is located in a binary star system, and is likely to be orbiting both stars in the system.[93]
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.[94]
SPECULOOS-3 b |  | 0.08716  | 0.719  | 0.00733  | 553  | transit  | 57.9  | 0.1  | 2800  | Ultra-short period planet[95]
Struve 2398 Ab | 0.00875±0.0011  | 0.107–0.178  | 11.2201±0.0051  | 0.068±0.001  |  | radial vel.  | 11.4  | 0.330±0.008  | 3470±31  | [96]
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.[97]
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[98][a] | 1.01±0.03  | 5757+72
−65 | [99]
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  | [100]
TIC 139270665 b  | 0.463  | 0.645  | 23.624  | 0.163  | 700  | transit  | 618  | 1.035+0.052
−0.062 | 5844+84
−82 | [101][102]
TIC 139270665 c  | 4.89+0.66
−0.37 |  | 1010+780
−220 | 2+0.93
−0.31 | 200+18
−35 | radial vel.  | [102]
TIC 241249530 b | 4.98+0.16
−0.18 | 1.19±0.04  | 165.772  |  |  | transit  | 1058±12[45] | 1.271+0.061
−0.068 | 6139±103[45] | A planet on a highly-eccentric (e=0.94) and retrograde orbit.[103]
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)[104]
Also known as TOI-6883 b[105]
TIC 393818343 c | 0.357±0.132  | 0.792±0.018  | 7.8458±0.0023  | 0.079±0.011  | 1027.2089± 0.3717  | transit  | [106]
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.[107]
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  | 222.5±0.2[108] | 0.85  | 6086  | [109]
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  | [110]
TOI-261 b  |  | 0.271  | 3.36  | 0.035  | 1722  | transit  | 370.6±0.9[111] | 0.50  | 5890  | [109]
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.[f][8]
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  | [8]
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☉)[112]
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  | [113]
TOI-406 c  | 0.02067±0.003  | 0.1846±0.0143  | 13.18  | 0.0809±0.003  | 368±14  | transit
TOI-429 b  | 0.8  | 0.8056±0.0196  | 338  |  |  | transit  | 391.5±0.5  | 0.99±0.06  | 5245+25
−67 | [114][115][116]
TOI-480 b  | 0.0654  |  | 6.866  |  |  | transit  | 177.8  | 1.2  | 6212  | [117]
TOI-588 b  |  | 1.459±0.036  | 39.4718[118] |  | 1015  | transit  | 502.9±3.2  | 2.69+0.34
−0.36 | 10,416+254
−220 | [118][119]
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  | [120]
TOI-654 b  |  | 0.211  | 1.53  | 0.021  | 749  | transit  | 188.7±0.18[121] | 0.53  | 3433  | [109]
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  | [122]
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-694 b  |  | 1.146±0.056  | 48.05[118] |  | 479.8  | transit  | 730.2+4.1
−4.0 | 1.042+0.063
−0.038 | 5355+74
−140 | [118][123]
TOI-710 b  |  | 1.66±1.10  | 72.08[118] |  |  | transit  | 514±2  | 1.71+0.39
−0.19 | 7458+146
−123 | [118][124]
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  | [125]
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.[100]
TOI-782 b  | <0.06 | 0.244±0.008  | 8.024  | 0.0578±0.0018  | 398±6–435±6[g] | transit  | 170.2±0.2  | 0.397±0.01  | 3370+29
−32 | [126]
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[127]
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  | 197.5±0.2[128] | 0.81  | 4935  | [109]
TOI-907 b  |  | 0.858  | 4.58  | 0.055  | 1847  | transit  | 989.9±5.0[129] | 1.07  | 6272  | [109]
TOI-1011 b  | 0.01271±0.00186  | 0.1294±0.0045  | 2.47  | 0.0346  |  | transit  | 170.8±0.1[130] | 0.92±0.03  | 5475±84  | [131]
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  | [132]
TOI-1173 Ab | 0.08213±0.00598  | 0.723±0.015  | 7.064  | 0.0702±0.0012  | 863.9±9.8  | transit  | 430.85[133][a] | 0.911+0.028
−0.03 | 5350±340  | Low-density planet located in a wide binary system.[134]
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  | [52]
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  | [135]
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.[136]
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  | [52]
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 | [137]
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  | [138]
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 | [139]
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  | [135]
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  | [52]
TOI-1294 b  | 0.1957±0.016  | 0.8199±0.0277  | 3.915  | 0.0489  |  | transit  | 1052±7  | 1.02±0.13  | 5714±126  | [140]
TOI-1294 c  | 0.467±0.053  |  | 160.1±2.5  | 0.581  |  | radial vel.  | 1052±7  | 1.02±0.13  | 5714±126  | [141]
TOI-1295 b  | 1.42±0.08  | 1.40±0.08  | 3.197  | 0.047±0.002  | 2360±50  | transit  | 1265±16  | 1.38±0.08  | 6280±50  | [142]
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[143]
TOI-1347 c | 0.0088±0.0072  | 0.143±0.009  | 4.842  |  | 1000±25  | transit  | [143]
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 | [144]
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 | [144]
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  | [145]
TOI-1410 b  |  | 0.262  | 1.22  | 0.020  | 1396  | transit  | 236.7±0.2[146] | 0.72  | 4635  | [109]
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[147] | transit + radial vel.  | 336  | 1.10±0.10  | 6008±113  | [148]
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  | [149]
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 | [150]
TOI-1448 b  | <0.0613 | 0.245±0.006  | 8.112  | 0.0567±0.0015  | 389±5–426±6[g] | transit  | 240±0.3  | 0.372±0.009  | 3412+28
−32 | [126]
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.[151]
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.[151]
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  | [52]
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 | [52]
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  | [152]
TOI-1683 b  |  | 0.236  | 3.06  | 0.037  | 929  | transit  | 166.2±0.2[153] | 0.69  | 4402  | [109]
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 | [154]
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 | [155]
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).[156]
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  | [52]
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 | [157]
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  | [52]
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  | [158]
TOI-1798 b  |  | 0.126  | 0.44  | 0.011  | 2122  | transit  | 369.147+1.008
−1.005 | 0.86  | 5165  | [109]
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  | [52]
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 | [159]
TOI-1803 b  | 0.03241±0.00787  | 0.267±0.007  | 6.293287±0.000028  | 0.060±0.001  | 747±11  | transit  | 388.3  | 0.756+0.050
−0.042 | 4687±65  | [160]
TOI-1803 c  | 0.01794±0.00944  | 0.3738+0.0223
−0.0267 | 12.885776±0.000036  | 0.097±0.002  | 561±10  | transit
TOI-1806 b  |  | 0.304  | 15.15  | 0.088  | 337  | transit  | 180.7±0.2[161] | 0.39  | 3272  | [109]
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  | [52]
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.[162]
TOI-1828 b  | 0.1841±0.012  | 0.769±0.017  | 9.09  | 0.0859  |  | transit  | 1208±8  | 1.04±0.13  | 5809±127  | [163]
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 | [164]
TOI-1883 b  |  | 0.4953±0.0460  | 4.506  |  | 524.9  | transit  | 376±3  | 0.492±0.02  | 3477±157  | [165][166]
TOI-1885 b  | 1.624±0.103  | 1.219±0.037  | 6.544060±0.000006  |  |  | transit  | 1826.773+21.464
−20.982 |  | 6527±98  | [149]
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 | [167]
TOI-2019 b  | 0.109±0.0132  | 0.505±0.0250  | 15.3444±0.0055  |  |  | transit  | 645.812+2.684
−2.665 |  | 5590  | [149]
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 | [164]
TOI-2120 b  | <0.02139 | 0.1893±0.0056  | 5.8  | 0.0377±0.0013  | 351±6–384±6[g] | transit  | 104.9  | 0.211±0.005  | 3131±30  | [126]
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 | [168]
TOI-2264 b  |  | 0.3726±0.0355  | 55.08[118] |  | 373.1  | transit  | 617.2+7.1
−6.9 | 1.164+0.146
−0.168 | 6140+129
−128 | [118][169]
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  | [170]
TOI-2274 b  |  |  | 2.679  |  | 771  | transit  | 159.9±0.2  | 0.612±0.02  | 3943±157  | [171][166]
TOI-2286 b  |  | 0.3343±0.0606  | 179.4  |  | 434.7  | transit  | 761.6+3.4
−3.3 | 1.487+0.322
−0.209 | 6863+147
−277 | [118][172]
TOI-2295 b  | 0.875+0.042
−0.041 | 1.47+0.85
−0.53 | 30.03  | 0.1992+0.0039
−0.0041 | 747±24  | transit  | 409.36+0.52
−0.46 | 1.168+0.070
−0.071 | 5730±140  | Radius in unconstrained due to the planet's grazing transit.[173]
TOI-2295 c  | 5.61+0.23
−0.24 |  | 966.5+4.3
−4.2 | 2.018+0.040
−0.042 | 234.9±7.6  | radial vel.  | [173]
TOI-2328 b  | 0.16±0.02  | 0.89±0.04  | 17.102  | 0.127+0.005
−0.006 | 842+20
−21 | transit  | 746.6±4.9  | 0.95±0.06  | 5525+147
−144 | [174]
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 | [164]
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  | [175]
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  | [176]
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  | [177]
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  | [177]
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  | [175]
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  |  | [178]
TOI-2458 b  | 0.04188+0.00311
−0.00302 | 0.252+0.018
−0.016 | 3.73659+0.00044
−0.00047 | 0.0482+0.0025
−0.0027 | 1509+41
−35 | transit  | 368.42+1.76
−1.74 | 1.05±0.03  | 6005±50  | Also known as HD 34562 b.[179]
TOI-2458 c  | 0.03216+0.00538
−0.00598 |  | 16.553+0.059
−0.061 | 0.129±0.002  |  | radial vel.  | [179]
TOI-2477 b  |  | 1.156±0.403  | 34.78[118] |  |  | transit  | 1181.4+16.8
−16.3 | 1.73+0.40
−0.21 | 7505+192
−222 | [118][180]
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  |  | [178]
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  | [175]
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 | [99]
TOI-2537 b  | 1.307+0.091
−0.088 | 1.004+0.059
−0.061 | 94.1022±0.0011  | 0.3715+0.0077
−0.0080 | 338±14  | transit  | 594.97+3.42
−3.03 | 0.771±0.049  | 4870±150  | [173]
TOI-2537 c  | 7.23+0.52
−0.45 |  | 1920+230
−140 | 2.78+0.22
−0.15 | 123.1+6.3
−6.7 | radial vel.
TOI-2580 b  | 0.63±0.08  | 1.55±0.05  | 3.397750±0.000002  | 0.048±0.003  | 2410±60  | transit  | 1236±16  | 1.33±0.08  | 6120±30  | [142]
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  | [181]
TOI-2768 b  |  | 0.2688±0.0313  | 1.508  |  | 855  | transit  | 255.8±0.6  | 0.63+0.06
−0.10 | 4008+124
−137 | [182][166]
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  | [181]
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  | [176]
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[183]
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  | [164]
TOI-3353 b  |  | 0.238  | 4.67  | 0.060  | 1264  | transit  | 257.1±0.2[184] | 1.33  | 6365  | [109]
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  | [185]
TOI-3837 b  | 0.59±0.06  | 0.96±0.05  | 11.889  | 0.098±0.005  | 1182+30
−31 | transit  | 1000.3±18.9  | 0.89±0.05  | 5905+157
−155 | [174]
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  | [164]
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  | [164]
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 | [164]
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.[186]
TOI-4356 b  |  | 0.321±0.198  | 289.92[118] |  |  | transit  | 668.6±3.8  | 1.48+0.32
−0.19 | 6855+140
−127 | [118][187]
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.[188]
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  | [189]
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  | [190]
TOI-4443 b  |  | 0.153  | 1.85  | 0.030  | 1639  | transit  |  | 1.05  | 5834  | [109]
TOI-4468 b  |  | 1.0197±0.0517  | 2.77  |  |  | transit  | 1224.7±8.2  | 0.82  | 4975±122  | [191]
TOI-4468 c  |  | 0.296±0.023  | 7.01  |  |  | transit  | [192]
TOI-4495 b  |  | 0.324  | 5.18  | 0.062  | 1383  | transit  |  | 1.17  | 6156  | [109]
TOI-4504 b  | 0.03272±0.00283  | 0.240±0.017  | 2.426  | 0.03392±0.00068  |  | transit  | 1117.43±5.57  | 0.89+0.06
−0.04 | 5315±60  | [193]
TOI-4504 c  | 3.77±0.18  | 0.9897±0.0092  | 82.97213±0.00013  | 0.3546+0.0073
−0.0077 |  | transit + radial vel.
TOI-4504 d  | 1.417±0.065  |  | 40.5634+0.0365
−0.0368 | 0.2219+0.0041
−0.0043 |  | timing
TOI-4527 b  |  | 0.0812  | 0.40  | 0.008  | 1363  | transit  |  | 0.48  | 3702  | [109]
TOI-4562 c | 5.77+0.37
−0.56 |  | 3990+201
−192 | 5.219±0.002  |  | timing  | 1131±12[194] | 1.218+0.054
−0.048[194] | 6096±32[194] | [195]
TOI-4602 b  |  | 0.227  | 3.98  | 0.051  | 1380  | transit  |  | 1.12  | 6012  | [109]
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[h] | 5600±50 or 5800±50 [h] | Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.[196]
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  | [181]
TOI-4994 b  | 0.280+0.037
−0.034 | 0.762+0.030
−0.027 | 21.491984±0.000023  | 0.1515+0.0032
−0.0031 | 717.6+9.7
−10 | transit  | 1079±8  | 1.005+0.064
−0.061 | 5640±110  | [197]
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  | [198]
TOI-5027 b  | 2.01±0.13  | 0.99+0.07
−0.12 | 10.244  | 0.093±0.004  | 1056+23
−24 | transit  | 659.5±4.9  | 1.02±0.05  | 5909+145
−144 | [174]
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  | [199]
TOI-5082 b  |  | 0.227  | 4.24  | 0.051  | 1165  | transit  |  | 1.00  | 5670  | [109]
TOI-5110 b  | 2.90±0.13  | 1.069+0.054
−0.052 | 30.159  | 0.2157+0.0042
−0.0044 | 976+33
−32 | transit  | 1170.64+5.12
−9.65 | 1.469+0.089
−0.088 | 6160±150  | [173]
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  | [69]
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 | [164]
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  | [164]
TOI-5319 b  |  | 0.33427±0.0551  | 4.079  |  | 695  | transit  | 199.4±0.7  | 0.5±0.1  | 3580+107
−141 | [200][166]
TOI-5388 b  |  | 0.169  | 2.59  | 0.024  | 601  | transit  |  | 0.29  | 3495  | [109]
TOI-5575 b  |  | 0.8459±0.0255  | 32.07[118] |  | 195  | transit  | 184.9±0.6  | 0.21±0.02  | 3176±157  | [118][201]
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  | [69]
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  | [69]
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  | [202]
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  | [203]
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  | [204]
TOI-5723 b  |  | 1.146±0.068  | 56.88[118] |  |  | transit  | 1878+22
−21 | 1.01+0.12
−0.15 | 5695+110
−170 | [118][205]
TOI-5731 b  |  | 0.401±0.046  | 90.1  |  |  | transit  | 358.2±0.8  | 0.697+0.088
−0.077 | 4448+92
−123 | [118][206]
TOI-5975 b  |  | 0.7536±0.0422  | 186.52[118] |  |  | transit  | 1141+7.1
−7.0 | 1.335+0.260
−0.188 | 6508+83
−163 | [118][207]
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 | [203]
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[204]
TOI-6016 b  | 1.17±0.09  | 1.22±0.03  | 4.023687±0.000003  | 0.055±0.002  | 1890±40  | transit  | 1190±13  | 1.31±0.08  | 6110±50  | [142]
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  | [189]
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  | [69]
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  | [204]
TOI-6130 b  | 1.05±0.06  | 1.28±0.03  | 2.392679±0.000002  | 0.036±0.002  | 1750±40  | transit  | 721±10  | 1.16±0.07  | 5940±50  | [142]
TOI-6303 b  | 7.84±0.31  | 1.034+0.054
−0.057 | 9.4852360±0.0000162  | 0.07610±0.00100  | 541±14  | transit  | 495.17±1.37  | 0.644±0.024  | 3977±59  | [208]
TOI-6324 b  | 0.0041±0.0006  | 0.0937  | 0.28  |  |  | transit  | 67.02±0.05  | 0.272±0.020  | 3358±160  | [114]
TOI-6330 b  | 10±0.32  | 0.972+0.033
−0.031 | 6.8500246±0.0000033  | 0.05763+0.00073
−0.00077 | 495±14  | transit  | 468.07±1.79  | 0.531±0.021  | 3539±59  | [208]
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  | [209]
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[210][a] | 1.323+0.050
−0.045 | 5940±110  | [211]
TOI-6628 b  | 0.75±0.06  | 0.98±0.05  | 18.184  | 0.133±0.007  | 836+22
−23 | transit  | 1028±27  | 0.97±0.06  | 5463+143
−142 | [174]
TOI-7041 b  | 0.36±0.16  | 1.02±0.03  | 9.691±0.006  |  |  | transit  | 1431±10  | 1.12±0.02  | 4640±10  | [212]
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[213]
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  | [214]
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[215]

## Specific exoplanet lists

[edit]

Lists of exoplanets

* List of directly imaged exoplanets
* List of exoplanet extremes
* List of exoplanet firsts
* List of exoplanets discovered by the Kepler space telescope
* List of exoplanets observed during Kepler's K2 mission
* List of extrasolar candidates for liquid water
* List of hottest exoplanets
* List of coolest exoplanets
* List of multiplanetary systems
* List of nearest exoplanets
* List of nearest terrestrial exoplanet candidates
* List of potentially habitable exoplanets
* List of proper names of exoplanets
* List of largest exoplanets
* List of smallest exoplanets
* List of transiting exoplanets
* List of exoplanets and planetary debris around white dwarfs
* List of extrasolar planetary collisions

### Lists of exoplanets by year of discovery

[edit]

* List of exoplanets discovered before 2000 (31)
* List of exoplanets discovered between 2000–2009 (377)
* List of exoplanets discovered in 2010 (109)
* List of exoplanets discovered in 2011 (179)
* List of exoplanets discovered in 2012 (149)
* List of exoplanets discovered in 2013 (151)
* List of exoplanets discovered in 2014 (870)
* List of exoplanets discovered in 2015 (144)
* List of exoplanets discovered in 2016 (1497)
* List of exoplanets discovered in 2017 (152)
* List of exoplanets discovered in 2018 (300)
* List of exoplanets discovered in 2019 (170)
* List of exoplanets discovered in 2020 (249)
* List of exoplanets discovered in 2021 (257)
* List of exoplanets discovered in 2022 (313)
* List of exoplanets discovered in 2023 (307)
* List of exoplanets discovered in 2024 (284)
* List of exoplanets discovered in 2025 (9)

## 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. ^ 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
4. ^ Since the density is only a lower limit, the radius is an upper limit.
5. ^ 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.
6. ^ 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.
7. ^ a b c Assuming albedos of 0.3 and 0 respectively.
8. ^ a b It is not known which of the stars the planet orbits.

## References

[edit]

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 (2025). "The NEID Earth Twin Survey. I. Confirmation of a 31-day planet orbiting HD 86728". The Astronomical Journal. 169 (1): 1. arXiv:2409.12315. Bibcode:2025AJ....169....1G. doi:10.3847/1538-3881/ad89bf.
2. ^ "The Extrasolar Planet Encyclopaedia — 82 Eri d". Extrasolar Planets Encyclopaedia. Paris Observatory.
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196. ^ Eisner, Nora L.; Grunblatt, Samuel K.; Barragán, Oscar; Faridani, Thea H.; Lintott, Chris; Aigrain, Suzanne; Johnston, Cole; Mason, Ian R.; Stassun, Keivan G.; Bedell, Megan; Boyle, Andrew W.; Ciardi, David R.; Clark, Catherine A.; Hebrard, Guillaume; Hogg, David W. (1 May 2024). "Planet Hunters TESS V: a planetary system around a binary star, including a mini-Neptune in the habitable zone". The Astronomical Journal. 167 (5): 241. arXiv:2404.18997. Bibcode:2024AJ....167..241E. doi:10.3847/1538-3881/ad1d5c. ISSN 0004-6256.
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Exoplanets

* Planet
* Definition
* IAU
* Planetary science

Main topics|

* Exoplanet
* Exoplanet orbital and physical parameters
* Methods of detecting exoplanets
* Planetary system
* Planet-hosting stars

Sizes
and
types|

| Terrestrial|

* Carbon planet
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* Desert planet
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* Ice planet
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* Lava planet
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Gaseous|

* Eccentric Jupiter
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Other types|

* Blanet
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Formation
and
evolution|

* Accretion
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* Detached object
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* Scattered disc
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Systems|

* Exocomet
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* Rogue planet
* Orbits
* Retrograde
* Trojan
* Mean-motion resonances
* Titius–Bode law

Host stars|

* A
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* Brown dwarfs
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* Herbig Ae/Be
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* Pulsar
* Red giant
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* Subgiant
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Detection|

* Astrometry
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* list
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* list
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* list
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* list
* Transit-timing variation

Habitability|

* Astrobiology
* Astrooceanography
* Circumstellar habitable zone
* Earth analog
* Extraterrestrial liquid water
* Galactic habitable zone
* Habitability of binary star systems
* Habitability of F-type main-sequence star systems
* Habitability of K-type main-sequence star systems
* Habitability of natural satellites
* Habitability of neutron star systems
* Habitability of red dwarf systems
* Habitability of yellow dwarf systems
* Habitable zone for complex life
* List of potentially habitable exoplanets
* Tholin
* Superhabitable planet

Catalogues|

* Nearby Habitable Systems
* Exoplanet Data Explorer
* Extrasolar Planets Encyclopaedia
* NASA Exoplanet Archive
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Lists|

* Exoplanetary systems
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Other|

* Carl Sagan Institute
* Exoplanet naming convention
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* Exoplanetary Circumstellar Environments and Disk Explorer
* Extragalactic planet
* Extrasolar planets in fiction
* Geodynamics of terrestrial exoplanets
* Neptunian desert
* Nexus for Exoplanet System Science
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* Sudarsky's gas giant classification

* Discoveries of exoplanets
* Search projects

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2024 in space

* « 2023

2025 »

Space probe launches |

* Peregrine Mission One (January)
* XPoSat
* Einstein Probe (January)
* DRO A/B (March)
* Chang'e 6 (Sample return from lunar far side, May-June)
* IM-1 / EagleCam
* Queqiao 2 / Tiandu-1 and 2 (March)
* Chang'e 6 / ICUBE-Q (May)
* Space Variable Objects Monitor (June)
* Hera / Milani / Juventas (October)
* Europa Clipper (October)
* PROBA-3 (December)

Impact events|

* 2024 BX1
* 2024 RW1
* 2024 UQ
* 2024 XA1

Selected NEOs|

* Asteroid close approaches
* 2020 BX12
* 2011 MD
* 2022 YO1
* 2024 MK
* 2024 ON
* 2024 PT5
* 2024 YR4

Discoveries|

* QSO J0529-4351
* 1 moon of Uranus
* 2 moons of Neptune
* Gaia BH3
* JADES-GS-z14-0
* Water on asteroids
* Porphyrion (radio galaxy)
* 2019 UO14 (First confirmed Saturnian trojan)

| Exoplanets |

* 82 G. Eridani d
* Barnard's Star b
* BX Trianguli b
* Gliese 12 b
* Gliese 341 b
* Gliese 900 b
* HD 48948#Planetary system
* b
* c
* d
* HD 73344
* b
* c
* d
* HD 101581
* b
* c
* HD 63433 d
* IRAS 04125+2902 b
* Kepler-51e
* LHS 1678 d
* SPECULOOS-3 b
* Struve 2398 Ab
* Teegarden's Star d
* TOI-6883 b
* WASP-132d

|

Comets |

* 144P/Kushida
* 12P/Pons-Brooks
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* C/2023 A3 (Tsuchinshan–ATLAS)
* 333P/LINEAR
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* C/2024 G3 (ATLAS)
* C/2024 S1 (ATLAS)
* C/2024 X1 (Fazekas)

* Outer space portal
* Category:2023 in outer space — Category:2024 in outer space — Category:2025 in outer space

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