List of exoplanets discovered in 2025

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This list of exoplanets discovered in 2025 is a list of confirmed exoplanets that were first reported in 2025. 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
AB Pictoris c 2.5–9 3–5 astrometry + radial vel. 163 0.90±0.10 5188±50 [1]
AT2021uey b 1.34+0.45
−0.50		 4,170+2,910
−1,710		 4.01+1.68
−1.34		 microlensing 3,390+2,410
−1,440		 0.49+0.16
−0.18		 3,680+307
−204		 [2]
Barnard's Star c 0.00105 4.12 0.0274±0.0004 radial vel. 5.96 0.162 3,195 [3]
Barnard's Star d 0.00083 2.34 0.0188±0.0003 radial vel.
Barnard's Star e 0.00061 6.74 0.0381±0.0005 radial vel.
BEBOP-3b 0.558+0.051
−0.048		 547.0+6.2
−7.6		 1.444±0.017 radial vel. 385.13±0.58[4] 1.3445[a] 6,033[b] A circumbinary planet.[5]
BD+05 4868 Ab 0.000063 0.028 1.27187 0.0208±0.0003 1,820±45 transit 142.4±0.1 0.70±0.02 4,596+65
−64		 A disintegrating planet with a comet-like tail.[6]
Cha 1107-7626 8.0±2.0 2.8 1800 imaging 636 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[7]
G 192-15 b 0.00324±0.00057 2.27476+0.00026
−0.00028		 0.01723+0.00038
−0.00039		 453.6+8.8
−8.5		 radial vel. 31.09±0.022 0.132±0.009 Also known as GJ 3380 b.[8]
G 192-15 c 0.0450+0.0050
−0.0047		 1,219+13
−11		 1.137+0.026
−0.027		 55.9±1.1 radial vel. Also known as GJ 3380 c.[8]
G 261-6 b 0.00431+0.00072
−0.00069		 5.4536+0.0031
−0.0032		 0.02971+0.00087
−0.00093		 322.3+9.9
−9.7		 radial vel. 34.66±0.021 0.118±0.011 [8]
G 268-110 b 0.00478±0.00079 1.432630+0.000072
−0.000076		 0.01283+0.00028
−0.00029		 534+12
−11		 radial vel. 31.86 0.137±0.009 [8]
Gliese 251 c 0.01207 53.647±0.044 0.196±0.014 radial vel. 18.21 0.360±0.015 3342±24 Potentially habitable.[9]
Gliese 410 b 0.0249±0.0038 6.02 0.0531±0.0007 radial vel. 38.9 0.55±0.02 3,842±31 Two additional planets in the same system are suspected.[10]
Gliese 536 c 0.01853±0.0022 32.76 0.1617±0.003 290 radial vel. 32.71 0.52±0.05 3685±68 [11]
GJ 2126 b 1.3+0.2
−0.1		 272.7 0.71±0.03 radial vel. 124.3±0.4 0.65+0.09
−0.07		 4,159±130 [12]
GJ 3998 d 0.0191+0.00315
−0.00302		 41.78±0.05 0.189±0.006 radial vel. 58.056±2.283 0.52±0.05 3726±68 [13]
Gliese 508.2 b 1.85 ~5300 4.85 radial vel. 54.3 0.54±0.12 3,720±12 [14]
GJ 9773 b 0.543 2965 2.921±0.045 radial vel. 51.8 0.358±0.011 3,528±25 [14]
HD 85426 c 0.0324+0.0050
−0.0047		 35.73+0.09
−0.10		 0.2118+0.0050
−0.0044 [c]		 640±9 radial vel. 175.3 0.991+0.027
−0.020		 5,746±59 Star also known as TOI-1774. An additional planet is suspected in the system.[15]
HD 87816 b 6.74 484 1.618±0.0003 radial vel. 434.4 2.41±0.1 4,989±46 Host star also known as R Velorum.[16]
HD 87816 c 12.2 7,596+1140
−535		 10.14+1.0
−0.5		 radial vel.
HD 94890 b 2.13 824 2.07±0.001 radial vel. 201.2 1.74±0.20 4,867±38 Host star also known as iota Antliae.[16]
HD 94890 c 8.9 2492 4.33±0.02 radial vel.
HD 102888 b 5.69 252 1.05±0.001 radial vel. 412.6 2.42±0.06 4,990±39 [16]
HD 135344 Ab 10.0+1.4
−1.9		 1.45+0.06
−0.03		 16.5+2.8
−2.0		 1,585+82
−73		 imaging 440 1.5 9,540±100 [17]
HD 143811 (AB)b 5.6±1.1 1.41±0.03 – 1.7 +0.7
−0.4		 117000 +91000
−31000		 63.88 1042 imaging 446.4 2.5 6,575±325 A circumbinary planet.[18]
HD 224018 b 0.0129±0.0025 0.0812+0.0036
−0.033		 10.64 0.0952±0.002 968 transit 346.0±0.7 1.013+0.069
−0.061		 5,784±60 [19]
HD 224018 c 0.0327+0.0041
−0.0035		 0.2159+0.0062
−0.0071		 36.58 0.217±0.005 641 transit
HD 224018 d 0.0132+0.0057
−0.0050		 0.214±0.009 138.1 0.53+0.06
−0.02		 411 transit
HD 224018 e 0.475+0.041
−0.044		 9129±2499 8.6+1.5
−1.6		 102 radial vel.
HIP 54515 b 17.7+7.6
−4.9		 1.08±0.23 32500+15000
−8800		 24.8+7.2
−4.7		 2,348±218 imaging + astrometry 271.4 1.88±0.11 8,100+500
−340		 Host star also known as 66 Leonis.[20]
HIP 99452 Ab 0.00667±0.00088 2.764 0.03608±0.00045 1201 radial vel. 66.67 0.821±0.032 5,185±80 [21]
HIP 99452 Ac 0.016±0.0016 0.2552±0.0161 12.93 0.1009±0.0013 718 transit
HIP 99452 Ad 0.0135±0.0022 29.65 0.175±0.002 545 radial vel.
HIP 99452 Ae 0.0365±0.003 62.98 0.290±0.004 424 radial vel.
J042705.86+261520.3 4.5 imaging 522 Part of a JuMBO along with J042705.86+261520.3 b .[22]
J042705.86+261520.3 b 3.9 imaging 522 Part of a JuMBO along with J042705.86+261520.3.[22]
J041546.22+280811.4 6.0 imaging – Free-floating object of planetary mass. Could also be a sub-brown dwarf.[22]
K2-157 c 0.0969 25.9 0.165±0.0018 587 radial vel. 946.5 0.89 ± 0.029 5,334 ± 64 [23]
K2-157 d 0.0733 66.5 0.309±0.0038 429 radial vel.
Kepler-139 f 0.113±0.0315 355±2 radial vel. + timing 1,289.78±13.89 1.08 5,594±100 [24]
Kepler-279 e 0.176+0.0189
−0.0154		 0.310±0.0482 ~98.35 transit 3,487.26±74.07 1.10+0.16
−0.13		 6,363±259 [25]
Kepler-289 e 0.0547+0.00409
−0.00377		 0.286+0.00437
−0.00259		 ~330 transit 2,283.09±45.66 1.08±0.02 5,990±38 [25]
Kepler-725 c 0.031 207.5 0.674±0.002 timing 2474±45 0.91 5,293±122 Partially in habitable zone.[26]
KMT-2017-BLG-2197Lb 8.84+8.3
−4.9		 15.9+2.1
−2.7		 microlensing 25,400+3,300
−4,300		 0.36+0.34
−0.2		 [27]
KMT-2019-BLG-0578Lb 1.2+1.2
−0.6		 1.2±0.2 or 2.0±0.3 microlensing 23,810+2,280
−2,610		 0.28+0.28
−0.14		 [28]
KMT-2021-BLG-0736Lb 0.0661+0.0409
−0.0315		 4.0+0.9
−0.8		 microlensing 22,830+2,610
−4,890		 0.60+0.37
−0.29		 [28]
KMT-2022-BLG-1790Lb 1.73+0.95
−0.9		 5.25+0.75
−1.0		 microlensing 21,100+3,000
−4,200		 0.58+0.32
−0.3		 [27]
KMT-2022-BLG-1818Lb 1.5+0.6
−0.3		 1.5+0.3
−0.2		 microlensing 9460+2280
−1300		 0.3+0.12
−0.06		 [29]
KMT-2022-BLG-1818Lc 0.35+0.24
−0.17		 0.4±0.1 microlensing
KMT-2022-BLG-2076Lb 0.88±0.46 5.67±1.58 microlensing 18,200+4,100
−5,000		 0.67±0.35 [27]
KMT-2023-BLG-0119Lb 0.2634+0.16822
−0.14396		 3.14+1.32
−1.33 or 4.01+1.69
−1.70		 microlensing 10,240+5,510
−5,540		 0.71+0.45
−0.39		 [30]
KMT-2023-BLG-1896Lb 0.0515+0.03087
−0.02656		 2.86+1.12
−1.02 or 4.62+1.81
−1.94		 microlensing 17,900+7,000
−7,500		 0.72+0.43
−0.37		 [30]
KMT-2023-BLG-2209Lb 0.80±0.38 5.31+0.95
−1.1		 microlensing 18,200+5,000
−5,700		 0.73±0.35 [27]
KMT-2024-BLG-0176Lb 0.76+1.03
−0.39		 0.75+0.09
−0.10 or 1.32+0.16
−0.18		 microlensing 27201+3294
−3686		 0.103+0.141
−0.054		 [31]
KMT-2024-BLG-0349Lb 11.86+6.56
−6.54		 1.85+0.65
−0.77 or 6.46+2.27
−2.69		 microlensing 18754+6588
−7795		 0.68±0.38 [31]
KMT-2024-BLG-0404Lb 0.0544+0.0802
−0.0277		 0.34±0.05 microlensing 23,510+3,030
−3,160		 0.09+0.133
−0.046		 Also a brown dwarf exists in the system[32]
KMT-2024-BLG-1209Lb 2.64+1.57
−1.16		 2.51+1.50
−1.10		 microlensing 12,800+6,600
−4,600		 0.77+0.46
−0.34		 [33]
KMT-2024-BLG-1870Lb 1.06+0.53
−0.55		 2.57+0.64
−0.97 or 3.15+0.79
−1.19		 microlensing 17873+4468
−6719		 0.67+0.33
−0.34		 [31]
KMT-2024-BLG-2087Lb 4.39+3.07
−2.46		 3.03+0.42
−0.54		 microlensing 23451+3098
−4175		 0.48+0.27
−0.33		 [31]
KOBE-1 b 0.0277±0.0024 8.54 0.07±0.0004 594 radial vel. 77.89±0.04 0.629±0.017 4,135±36 [34]
KOBE-1 c 0.039±0.0035 29.67 0.161±0.001 392 radial vel.
KOI-134 b 1.08±0.2 67.59 0.358 588 transit 3780 1.17 6154±26 [35]
KOI-134 c 0.22 ± 0.01 33.5 timing
KOINTREAU-1 b 10.6±2.5 690±10 imaging 518.6 0.26±0.03 3,551±59 [36]
L 98-59 f 0.00934 23.07 0.1053±0.0024 radial vel. 34.6 0.32±0.03 3,415±135 Potentially habitable[37]
MOA-2022-BLG-033Lb 0.0382+0.0296
−0.0197		 2.15+1.17
−0.75 or 2.31+1.27
−0.81		 microlensing 6,000+3,260
−2,640		 0.51+0.39
−0.26		 [30]
MOA-2022-BLG-091Lb 3.59+2.00
−1.67		 2.67+1.45
−1.24 to 3.63+1.30
−1.31		 microlensing 13,900+4,960
−4,990		 0.75+0.42
−0.35		 [33]
MP Muscae b 5.0 1 – 3 astrometry + disk kinematics 319.3 1.3±0.08 5000 [38]
Mu2 Octantis Ac 0.0318±0.0038 4.60111±0.00024 0.056 radial vel. 130.3 1.330±0.013 6059±52 Also known as HD 196067 c.[39]
OGLE-2016-BLG-0007Lb 0.00415+0.0028
−0.0022		 10.1+3.8
−3.4		 microlensing 14,020+3590
−4570		 0.6+0.4
−0.3		 [40]
OGLE-2023-BLG-0524 0.0293 or 0.182[d] microlensing – Free-floating object of planetary mass.[41]
o005 s41280 8.4 2.3 2,162 imaging 17,300 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[42]
o006 s00089 11.5 1.2 955 imaging 6,520 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[42]
Ross 176 b 0.01438±0.0028 0.1642±0.0071 5.00663±0.00008 0.0464±0.001 682 transit 151.7 0.58±0.02 4,061±70 [43]
TIC 88785435 b 0.449±0.019 10.508843 0.08432±0.00068 635±16 transit 398.2±0.8 0.724±0.017 3,998±95 [44]
TOI-201 c 14.2±2.0 0.99±0.017 2,800+360
−210		 4.28+0.36
−0.2		 timing + transit 372.5 1.316±0.027 6,394±75 [45]
TOI-333 b 0.0632±0.0076 0.3801±0.0098 3.785250±0.000006 0.049±0.001 1445 transit 1132 1.2±0.1 6,241±73 [46]
TOI-375 b 0.745+0.052
−0.053		 0.961+0.044
−0.043		 9.45469±0.00002 0.099±0.002 1,373+47
−45		 transit 1316 1.441+0.076
−0.075		 5,259.9+136.9
−135.3		 The star is a subgiant.[47]
TOI-375 c 2.106+0.223
−0.212		 115.5+2.0
−1.6		 0.524±0.011 596±21 radial vel.
TOI-375 d 1.402+0.311
−0.276		 297.9+28.9
−18.6		 0.984+0.062
−0.044		 434±19 radial vel.
TOI-512 b 0.01123+0.00167
−0.00173		 0.1374±0.0089 7.18886+0.000069
−0.000077		 1,009±29 transit 219.16±0.14 0.74±0.03 5,277±67 [48]
TOI-771 c 0.00903 7.61 0.046±0.002 365 radial vel. 82.45 0.22±0.024 3,201±100 [49]
TOI-1117 b 0.028±0.003 0.219+0.012
−0.011		 2.22816±0.00001 0.0330±0.0002 1,538±21 transit 546.64±2.94 0.97±0.02 5,635±62 [50]
TOI-1117 c 0.0276+0.0037
−0.0038		 4.579±0.004 0.0534±0.0003 1,210±16 radial vel.
TOI-1117 d 0.0337±0.0050 8.665±0.011 0.0817±0.0006 978±13 radial vel.
TOI-1203 b 0.0110±0.0010 0.1356+0.0040
−0.0041		 4.1572888 0.04869+0.00094
−−0.00095		 1361.2+18.8
−18.4		 transit 211.9 0.886±0.036 5,737±62 An old thick disk star. The fourth planet in the system, TOI-1203 d, was already validated in 2020.[51]
TOI-1203 c 0.0172±0.0016 13.0766+0.0079
−0.0072		 radial vel.
TOI-1203 e 0.1325+0.0058
−0.0056		 204.59+0.67
−0.63		 radial vel.
TOI-1453 Ab 0.00390+0.00208
−0.00204		 0.105+0.00526
−0.00500		 4.3135225+0.0000118
−0.0000092		 transit 257.288±0.209 0.715±0.035 4,975±68 [52]
TOI-1453 Ac 0.00928+0.00261
−0.00264		 0.198±0.00848 6.5886982 transit
TOI-1846 b 0.01385+0.00503
−0.00315		 0.15987+0.00580
−0.00607		 3.931 0.03646+0.00072
−0.00074		 568.1+6.1
−5.9		 transit 154.09±0.11 0.40±0.02 3,568±44 [53]
TOI-2005 b <6.4 1.07+0.06
−0.11		 17.305904+0.000023
−0.000020		 0.16±0.02 transit 1,072.08+15.00
−13.70		 1.59+0.016
−0.017		 7,130±150 [54]
TOI-2015 c 0.02803+0.001196
−0.001259		 5.582796+0.000042
−0.000041		 0.041232±0.000004 448±3 timing 154.34±0.16 0.3041+0.0353
−0.0312		 3,297+14
−28		 [55] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.[56]
TOI-2076 e 0.12089+0.00901
−0.00874		 3.0223445±0.0000033 0.0385+0.0021
−0.0049		 1138 transit 136.7 0.849+0.027
−0.026		 5,200±100 [57]
TOI-2267 b 0.0893 or 0.1089 2.2891 0.0205 or 0.0127 transit 73.5 0.270[e] 3,030±100[f] [58][59]
TOI-2267 c 0.1018 or 0.1214 3.4950 0.0263 or 0.0145 transit
TOI-2267 d 0.0875 or 0.1580 2.0345 0.0174 or 0.0145 transit
TOI-2407 b 0.380±0.023 2.703 0.033±0.001 705±12 transit 300.06 0.548±0.016 3,530±100 [60]
TOI-2427 c 0.02033 5.15±0.01 0.05±0.01 radial vel. 92.95 0.64±0.02 4,072±121 [61]
TOI-2431 b 0.020±0.004 0.137±0.003 0.224196 0.0063±0.0001 2,063±30 transit 117 0.661+0.021
−0.024		 4,109+28
−27		 Has one of the shortest orbital periods of any exoplanet. In just 31 million years the planet will have been destroyed.[62]
TOI-2449 b 0.7±0.04 1.0±0.01 106.1447 0.45±0.01 400 transit 505.5 1.079+0.045
−0.048		 6,021±62 Also known as NGTS-36 b.[63]
TOI-2969 b 1.16±0.04 1.1±0.08 1.8237146±0.0000002 0.0261±0.0002 1186 transit 530.0 0.71±0.02 4738±100 [64]
TOI-2989 b 3.0±0.2 1.12±0.05 3.122832±0.000001 0.0384±0.0003 1000 transit 635.7 0.77±0.02 4672±170 [64]
TOI-3493 b 0.0282+0.00368
−0.00377		 0.287±0.00714 8.1594667+0.0000016
−0.0000017		 1,102+20
−14		 transit 315.59±0.65 1.023±0.041 5,844±42 [65]
TOI-3495 b 0.3631 8.413073±0.000055 902 transit 562.2 1.42±0.17 6,400±230 [66]
TOI-4507 b <0.094 0.7333±0.0071 104.61595±0.00004 0.449±0.003 transit 580.6 1.15±0.07 6,235±100 [67]
TOI-5108 b 0.101±0.0157 0.589±0.00892 6.753 0.073±0.004 1,180±40 transit 427.6±2.0 1.10±0.03 5,808±40 [68]
TOI-5143 c 1.45+0.18
−0.12		 5.2097118+0.0000032
−0.0000039		 0.05602+0.00082
−0.00079		 transit 582.42±1.97 0.864+0.040
−0.033		 5,183±125 [69]
TOI-5300 b 0.6±0.1 0.88±0.08 2.262196±0.000003 0.0295±0.0003 1043 transit 530.6 0.67±0.02 4610±207 [64]
TOI-5349 b 0.40±0.02 0.91±0.02 3.317921 0.0369±0.0004 719±15 transit 620 0.61±0.02 3,751±59 [70]
TOI-5573 b 0.35±0.06 0.87±0.04 8.79759±0.00001 0.0712±0.0008 528 transit 606.0 0.619±0.023 3,790±59 [71]
TOI-5786 b 0.230±0.0283 0.762±0.0116 12.779 0.114±0.007 1,040±40 transit 632.1±1.6 1.23+0.04
−0.03		 6,235±50 [68]
TOI-5795 b 0.0744+0.0129
−0.0145		 0.5014±0.0098 6.140632±0.000005 0.064±0.002 1137 transit 526.7 0.901+0.055
−0.037		 5,715±55 [72]
TOI-5800 b 0.030±0.006 0.218±0.026 2.6279 0.0345±0.0014 1,108±20 transit 139.4±0.1 0.778+0.037
−0.032		 4,850±78 [73]
TOI-5817 b 0.03241+0.00441
−0.00409		 0.275±0.012 15.61 0.1223±0.0060 950+21
−18		 transit 262.0±0.5 0.970+0.072
−0.055		 5,770±50 [73]
TOI-6038 Ab 0.247+0.030
−0.031		 0.572+0.018
−0.014		 5.82673 0.0690+0.0012
−0.0011		 1,439+25
−24		 transit 577.9±2.0 1.291+0.066
−0.060		 6,110±100 The host star is part of a binary system with a K-type companion.[74]
TOI-6041 b <0.03401 0.4059±0.018 26.0494 0.1651±0.002 605 transit 236 0.89±0.04 5,417±50 [75]
TOI-6041 c 0.2451 88.0 0.3721±0.0067 403 radial vel.
TOI-6054 b 0.039±0.0053 0.2364±0.0134 7.501 0.0763±0.0048 1,360+35
−31		 transit 256.7±0.4 1.107±0.040 6,047±50 [76]
TOI-6054 c 0.0289±0.006 0.250±0.016 12.564 0.1077±0.0067 1,144+29
−26		 transit
TOI-6478 b 0.0311 0.411±0.021 34.005019±0.000025 0.1136±0.0060 204.4±4.9 transit 125.93±0.33 0.230±0.007 3,230±75 [77]
TOI-6695 b 0.21 0.85±0.02 80.4 0.402±0.002 599 transit 922 1.338 6,400 [78]
TOI-6695 c 1.45 242 0.838±0.005 415 radial vel.
TOI-6894 b 0.168±0.022 0.855±0.022 3.371 0.02604±0.00045 417.9±8.6 transit 237.96±0.95 0.207±0.011 3007±58 [79]
TOI-7149 b 0.705±0.075 1.180±0.045 2.652 0.026±0.00076 593±21 transit 415.0±2.4 0.344±0.030 3,363±59 [80]
TOI-7166 b 0.1793±0.0054 12.920636±0.000001 0.06191±0.00044 249 transit 114.9 0.19±0.004 3,099±51 Located in habitable zone.[81]
TOI-7510 b 0.0569±0.0053 0.651±0.018 11.5309 0.102±0.002 878 transit 789 1.02±0.03 5,820±80 [82]
TOI-7510 c 0.41±0.04 0.964±0.027 22.5687 0.159±0.003 702 transit
TOI-7510 d 0.56±0.04 0.94±0.03 48.8645 0.267±0.005 542 transit
WASP-154 b 0.626±0.129 0.96±0.06 3.811678±0.000001 0.044±0.003 994±63 transit 702.87±6.40 0.80±0.05 4,774±133 [83]
WASP-188 Ab 1.443+0.296
−0.298		 1.322±0.051 5.748916±0.000003 0.072±0.003 1,666±70 transit 2,202.47±31.55 1.50±0.09 6,850±125 [83]
WASP-195 b 0.104+0.03
−0.031		 0.92±0.05 5.051928±0.000004 0.063±0.003 1,522±71 transit 1,581.38±16.60 1.30±0.08 6,300±125 [83]
WASP-197 b 1.269±0.254 1.289±0.049 5.167228±0.000003 0.065±0.002 1,665±67 transit 1,577.54±40.08 1.36±0.08 6,050±100 [83]
WISPIT 1 b 10.4+0.7
−0.8		 338 imaging 747 4,670+990
−540[g]		 Circumbinary planets.[84]
WISPIT 1 c 5.3+0.8
−0.6		 840 imaging
WISPIT 2 b 5.3±1.0 1.6±0.2 15.0 imaging 435 1.08+0.06
−0.17		 4,400±50 [85][86]

Lists of exoplanets by year of discovery

Notes

References

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