List of exoplanets discovered in 2025

Last updated

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.

Contents

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 2.5–93–5astrometry + radial vel.1630.90±0.105188±50 [1]
AT2021uey b1.34+0.45
0.50
4,170+2,910
1,710
4.01+1.68
1.34
microlensing3,390+2,410
1,440
0.49+0.16
0.18
3,680+307
204
[2]
Barnard's Star c 0.001054.120.0274±0.0004radial velocity5.960.1623,195 [3]
Barnard's Star d 0.000832.340.0188±0.0003radial velocity
Barnard's Star e 0.000616.740.0381±0.0005radial velocity
BEBOP-3b0.558+0.051
0.048
547.0+6.2
7.6
1.444±0.017radial vel.385.13±0.58 [4] 1.3445 [a] 6,033 [b] A circumbinary planet. [5]
BD+05 4868 Ab 0.0000630.0281.271870.0208±0.00031,820±45transit142.4±0.10.70±0.024,596+65
64
A disintegrating planet with a comet-like tail. [6]
G 192-15 b0.00324±0.000572.27476+0.00026
0.00028
0.01723+0.00038
0.00039
453.6+8.8
8.5
radial velocity31.09±0.0220.132±0.009Also known as GJ 3380 b. [7]
G 192-15 c0.0450+0.0050
0.0047
1,219+13
11
1.137+0.026
0.027
55.9±1.1radial velocityAlso known as GJ 3380 c. [7]
G 261-6 b0.00431+0.00072
0.00069
5.4536+0.0031
0.0032
0.02971+0.00087
0.00093
322.3+9.9
9.7
radial velocity34.66±0.0210.118±0.011 [7]
G 268-110 b0.00478±0.000791.432630+0.000072
0.000076
0.01283+0.00028
0.00029
534+12
11
radial velocity31.860.137±0.009 [7]
Gliese 410 b0.0249±0.00386.020.0531±0.0007radial velocity38.90.55±0.023,842±31Two additional planets in the same system are suspected. [8]
GJ 2126 b1.3+0.2
0.1
272.70.71±0.03radial velocity124.3±0.40.65+0.09
0.07
4,159±130 [9]
GJ 3998 d 0.0191+0.00315
0.00302
41.78±0.050.189±0.006radial velocity58.056±2.2830.52±0.053726±68 [10]
HD 87816 b 6.744841.618±0.0003radial velocity434.42.41±0.14,989±46Host star also known as R Velorum. [11]
HD 87816 c 12.27,596+1140
535
10.14+1.0
0.5
radial velocity
HD 94890 b 2.138242.07±0.001radial velocity201.21.74±0.204,867±38Host star also known as iota Antliae. [11]
HD 94890 c 8.924924.33±0.02radial velocity
HD 102888 b5.692521.05±0.001radial velocity412.62.42±0.064,990±39 [11]
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
imaging4401.59,540±100 [12]
J042705.86+261520.34.5imaging522Part of a JuMBO along with J042705.86+261520.3 b . [13]
J042705.86+261520.3 b3.9imaging522Part of a JuMBO along with J042705.86+261520.3. [13]
J041546.22+280811.46.0imagingFree-floating object of planetary mass. Could also be a brown dwarf. [13]
K2-157c0.096925.90.165±0.0018587radial velocity946.50.89 ± 0.0295,334 ± 64 [14]
K2-157d0.073366.50.309±0.0038429radial velocity
Kepler-139 f0.113±0.0315355±2radial velocity + timing1,289.78±13.891.085,594±100 [15]
Kepler-279 e0.176+0.0189
0.0154
0.310±0.0482~98.35transit3,487.26±74.071.10+0.16
0.13
6,363±259 [16]
Kepler-289 e 0.0547+0.00409
0.00377
0.286+0.00437
0.00259
~330transit2,283.09±45.661.08±0.025,990±38 [16]
Kepler-725 c 0.031207.50.674±0.002timing2474±450.915,293±122Partially in habitable zone. [17]
KMT-2017-BLG-2197Lb8.84+8.3
4.9
15.9+2.1
2.7
microlensing25,400+3,300
4,300
0.36+0.34
0.2
[18]
KMT-2019-BLG-0578Lb1.2+1.2
0.6
1.2±0.2 or 2.0±0.3microlensing23,810+2,280
2,610
0.28+0.28
0.14
[19]
KMT-2021-BLG-0736Lb0.0661+0.0409
0.0315
4.0+0.9
0.8
microlensing22,830+2,610
4,890
0.60+0.37
0.29
[19]
KMT-2022-BLG-1790Lb1.73+0.95
0.9
5.25+0.75
1.0
microlensing21,100+3,000
4,200
0.58+0.32
0.3
[18]
KMT-2022-BLG-1818Lb1.5+0.6
−0.3
1.5+0.3
−0.2
microlensing9460+2280
−1300
0.3+0.12
−0.06
[20]
KMT-2022-BLG-1818Lc0.35+0.24
−0.17
0.4±0.1microlensing
KMT-2022-BLG-2076Lb0.88±0.465.67±1.58microlensing18,200+4,100
5,000
0.67±0.35 [18]
KMT-2023-BLG-0119Lb0.2634+0.16822
0.14396
3.14+1.32
1.33
or 4.01+1.69
1.70
microlensing10,240+5,510
5,540
0.71+0.45
0.39
[21]
KMT-2023-BLG-1896Lb0.0515+0.03087
0.02656
2.86+1.12
1.02
or 4.62+1.81
1.94
microlensing17,900+7,000
7,500
0.72+0.43
0.37
[21]
KMT-2023-BLG-2209Lb0.80±0.385.31+0.95
1.1
microlensing18,200+5,000
5,700
0.73±0.35 [18]
KMT-2024-BLG-0404L b0.0544+0.0802
0.0277
0.34±0.05microlensing23,510+3,030
3,160
0.09+0.133
0.046
Also a brown dwarf exists in the system [22]
KMT-2024-BLG-1209Lb2.64+1.57
1.16
2.51+1.50
1.10
microlensing12,800+6,600
4,600
0.77+0.46
0.34
[23]
KOBE-1 b0.0277±0.00248.540.07±0.0004594radial velocity77.89±0.040.629±0.0174,135±36 [24]
KOBE-1 c0.039±0.003529.670.161±0.001392radial velocity
KOI-134 b1.08±0.267.590.358588transit37801.176154±26 [25]
KOI-134 c0.22 ± 0.0133.5timing
L 98-59 f 0.0093423.070.1053±0.0024radial velocity34.60.32±0.033,415±135Potentially habitable [26]
MOA-2022-BLG-033Lb0.0382+0.0296
0.0197
2.15+1.17
0.75
or 2.31+1.27
0.81
microlensing6,000+3,260
2,640
0.51+0.39
0.26
[21]
MOA-2022-BLG-091Lb3.59+2.00
1.67
2.67+1.45
1.24
to 3.63+1.30
1.31
microlensing13,900+4,960
4,990
0.75+0.42
0.35
[23]
MP Muscae b 5.01 3astrometry + disk kinematics319.31.3±0.085000 [27]
OGLE-2016-BLG-0007 b 0.00415+0.0028
0.0022
10.1+3.8
3.4
microlensing14,020+3590
4570
0.6+0.4
0.3
[28]
o005 s412808.42.32,162imaging17,300Free-floating object of planetary mass. Could also be a brown dwarf. [29]
o006 s0008911.51.2955imaging6,520Free-floating object of planetary mass. Could also be a brown dwarf. [29]
Ross 176 b0.01438±0.00280.1642±0.00715.00663±0.000080.0464±0.001682transit151.70.58±0.024,061±70 [30]
TIC 88785435 b0.449±0.01910.5088430.08432±0.00068635±16transit398.2±0.80.724±0.0173,998±95 [31]
TOI-201 c14.2±2.00.99±0.0172,800+360
210
4.28+0.36
0.2
timing + transit372.51.316±0.0276,394±75 [32]
TOI-512 b0.01123+0.00167
0.00173
0.1374±0.00897.18886+0.000069
0.000077
1,009±29transit219.16±0.140.74±0.035,277±67 [33]
TOI-771 c0.009037.610.046±0.002365radial velocity82.450.22±0.0243,201±100 [34]
TOI-1117 b0.028±0.0030.219+0.012
0.011
2.22816±0.000010.0330±0.00021,538±21transit546.64±2.940.97±0.025,635±62 [35]
TOI-1117 c0.0276+0.0037
0.0038
4.579±0.0040.0534±0.00031,210±16radial vel.
TOI-1117 d0.0337±0.00508.665±0.0110.0817±0.0006978±13radial vel.
TOI-1453 Ab0.00390+0.00208
0.00204
0.105+0.00526
0.00500
4.3135225+0.0000118
0.0000092
transit257.288±0.2090.715±0.0354,975±68 [36]
TOI-1453 Ac0.00928+0.00261
0.00264
0.198±0.008486.5886982transit
TOI-1846 b0.01385++0.00503
-0.00315
0.15987++0.00580
-0.00607
3.9310.03646+0.00072
0.00074
568.1+6.1
5.9
transit154.09±0.110.40±0.023,568±44 [37]
TOI-2005 b<6.41.07+0.06
0.11
17.305904+0.000023
0.000020
0.16±0.02transit1,072.08+15.00
13.70
1.59+0.016
0.017
7,130±150 [38]
TOI-2015 c0.02803+0.001196
0.001259
5.582796+0.000042
0.000041
0.041232±0.000004448±3timing154.34±0.160.3041+0.0353
0.0312
3,297+14
28
[39] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection. [40]
TOI-2076 e0.12089+0.00901
0.00874
3.0223445±0.00000330.0385+0.0021
0.0049
1138transit136.70.849+0.027
0.026
5,200±100 [41]
TOI-2407 b0.380±0.0232.7030.033±0.001705±12transit300.060.548±0.0163,530±100 [42]
TOI-2431 b0.020±0.0040.137±0.0030.2241960.0063±0.00012,063±30transit1170.661+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 is gone. [43]
TOI-3493 b0.0282+0.00368
0.00377
0.287±0.007148.1594667+0.0000016
0.0000017
1,102+20
14
transit315.59±0.651.023±0.0415,844±42 [44]
TOI-3495 b0.36318.413073±0.000055902transit562.21.42±0.176,400±230 [45]
TOI-5108 b0.101±0.01570.589±0.008926.7530.073±0.0041,180±40transit427.6±2.01.10±0.035,808±40 [46]
TOI-5143 c1.45+0.18
0.12
5.2097118+0.0000032
0.0000039
0.05602+0.00082
0.00079
transit582.42±1.970.864+0.040
0.033
5,183±125 [47]
TOI-5786 b0.230±0.02830.762±0.011612.7790.114±0.0071,040±40transit632.1±1.61.23+0.04
0.03
6,235±50 [46]
TOI-5795 b0.0744+0.0129
0.0145
0.5014±0.00986.140632±0.0000050.064±0.0021137transit526.70.901+0.055
0.037
5,715±55 [48]
TOI-5800 b0.030±0.0060.218±0.0262.62790.0345±0.00141,108±20transit139.4±0.10.778+0.037
0.032
4,850±78 [49]
TOI-5817 b0.03241+0.00441
0.00409
0.275±0.01215.610.1223±0.0060950+21
18
transit262.0±0.50.970+0.072
0.055
5,770±50 [49]
TOI-6038 Ab0.247+0.030
0.031
0.572+0.018
0.014
5.826730.0690+0.0012
0.0011
1,439+25
24
transit577.9±2.01.291+0.066
0.060
6,110±100The host star is part of a binary system with a K-type companion. [50]
TOI-6054 b0.039±0.00530.2364±0.01347.5010.0763±0.00481,360+35
31
transit256.7±0.41.107±0.0406,047±50 [51]
TOI-6054 c0.0289±0.0060.250±0.01612.5640.1077±0.00671,144+29
26
transit
TOI-6478 b 0.03110.411±0.02134.005019±0.0000250.1136±0.0060204.4±4.9transit125.93±0.330.230±0.0073,230±75 [52]
TOI-6695 b0.210.85±0.0280.40.402±0.002599transit9221.3386,400 [53]
TOI-6695 c1.452420.838±0.005415radial velocity
TOI-6894 b 0.168±0.0220.855±0.0223.3710.02604±0.00045417.9±8.6transit237.96±0.950.207±0.0113007±58 [54]
TOI-7149 b0.705±0.0751.180±0.0452.6520.026±0.00076593±21transit415.0±2.40.344±0.0303,363±59 [55]
WASP-154 b0.626±0.1290.96±0.063.811678±0.0000010.044±0.003994±63transit702.87±6.400.80±0.054,774±133 [56]
WASP-188 Ab1.443+0.296
0.298
1.322±0.0515.748916±0.0000030.072±0.0031,666±70transit2,202.47±31.551.50±0.096,850±125 [56]
WASP-195 b0.104+0.03
0.031
0.92±0.055.051928±0.0000040.063±0.0031,522±71transit1,581.38±16.601.30±0.086,300±125 [56]
WASP-197 b1.269±0.2541.289±0.0495.167228±0.0000030.065±0.0021,665±67transit1,577.54±40.081.36±0.086,050±100 [56]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

Notes

  1. Sum of masses of the system
  2. Temperature of component A

References

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