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 velocity | 5.96 | 0.162 | 3,195 | [3] | ||
Barnard's Star d | 0.00083 | 2.34 | 0.0188±0.0003 | radial velocity | ||||||
Barnard's Star e | 0.00061 | 6.74 | 0.0381±0.0005 | radial velocity | ||||||
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] |
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 velocity | 31.09±0.022 | 0.132±0.009 | Also known as GJ 3380 b. [7] | ||
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 velocity | Also known as GJ 3380 c. [7] | ||||
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 velocity | 34.66±0.021 | 0.118±0.011 | [7] | ||
G 268-110 b | 0.00478±0.00079 | 1.432630+0.000072 −0.000076 | 0.01283+0.00028 −0.00029 | 534+12 −11 | radial velocity | 31.86 | 0.137±0.009 | [7] | ||
Gliese 410 b | 0.0249±0.0038 | 6.02 | 0.0531±0.0007 | radial velocity | 38.9 | 0.55±0.02 | 3,842±31 | Two additional planets in the same system are suspected. [8] | ||
GJ 2126 b | 1.3+0.2 −0.1 | 272.7 | 0.71±0.03 | radial velocity | 124.3±0.4 | 0.65+0.09 −0.07 | 4,159±130 | [9] | ||
GJ 3998 d | 0.0191+0.00315 −0.00302 | 41.78±0.05 | 0.189±0.006 | radial velocity | 58.056±2.283 | 0.52±0.05 | 3726±68 | [10] | ||
HD 87816 b | 6.74 | 484 | 1.618±0.0003 | radial velocity | 434.4 | 2.41±0.1 | 4,989±46 | Host star also known as R Velorum. [11] | ||
HD 87816 c | 12.2 | 7,596+1140 −535 | 10.14+1.0 −0.5 | radial velocity | ||||||
HD 94890 b | 2.13 | 824 | 2.07±0.001 | radial velocity | 201.2 | 1.74±0.20 | 4,867±38 | Host star also known as iota Antliae. [11] | ||
HD 94890 c | 8.9 | 2492 | 4.33±0.02 | radial velocity | ||||||
HD 102888 b | 5.69 | 252 | 1.05±0.001 | radial velocity | 412.6 | 2.42±0.06 | 4,990±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 | imaging | 440 | 1.5 | 9,540±100 | [12] | |
J042705.86+261520.3 | 4.5 | imaging | 522 | Part of a JuMBO along with J042705.86+261520.3 b . [13] | ||||||
J042705.86+261520.3 b | 3.9 | imaging | 522 | Part of a JuMBO along with J042705.86+261520.3. [13] | ||||||
J041546.22+280811.4 | 6.0 | imaging | – | Free-floating object of planetary mass. Could also be a brown dwarf. [13] | ||||||
K2-157c | 0.0969 | 25.9 | 0.165±0.0018 | 587 | radial velocity | 946.5 | 0.89 ± 0.029 | 5,334 ± 64 | [14] | |
K2-157d | 0.0733 | 66.5 | 0.309±0.0038 | 429 | radial velocity | |||||
Kepler-139 f | 0.113±0.0315 | 355±2 | radial velocity + timing | 1,289.78±13.89 | 1.08 | 5,594±100 | [15] | |||
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 | [16] | ||
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 | [16] | ||
Kepler-725 c | 0.031 | 207.5 | 0.674±0.002 | timing | 2474±45 | 0.91 | 5,293±122 | Partially in habitable zone. [17] | ||
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 | [18] | ||||
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 | [19] | ||||
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 | [19] | ||||
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 | [18] | ||||
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 | [20] | ||||
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 | [18] | ||||
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 | [21] | ||||
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 | [21] | ||||
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 | [18] | ||||
KMT-2024-BLG-0404L b | 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 [22] | ||||
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 | [23] | ||||
KOBE-1 b | 0.0277±0.0024 | 8.54 | 0.07±0.0004 | 594 | radial velocity | 77.89±0.04 | 0.629±0.017 | 4,135±36 | [24] | |
KOBE-1 c | 0.039±0.0035 | 29.67 | 0.161±0.001 | 392 | radial velocity | |||||
KOI-134 b | 1.08±0.2 | 67.59 | 0.358 | 588 | transit | 3780 | 1.17 | 6154±26 | [25] | |
KOI-134 c | 0.22 ± 0.01 | 33.5 | timing | |||||||
L 98-59 f | 0.00934 | 23.07 | 0.1053±0.0024 | radial velocity | 34.6 | 0.32±0.03 | 3,415±135 | Potentially habitable [26] | ||
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 | [21] | ||||
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 | [23] | ||||
MP Muscae b | 5.0 | 1 –3 | astrometry + disk kinematics | 319.3 | 1.3±0.08 | 5000 | [27] | |||
OGLE-2016-BLG-0007 b | 0.00415+0.0028 −0.0022 | 10.1+3.8 −3.4 | microlensing | 14,020+3590 −4570 | 0.6+0.4 −0.3 | [28] | ||||
o005 s41280 | 8.4 | 2.3 | 2,162 | imaging | 17,300 | Free-floating object of planetary mass. Could also be a brown dwarf. [29] | ||||
o006 s00089 | 11.5 | 1.2 | 955 | imaging | 6,520 | Free-floating object of planetary mass. Could also be a brown dwarf. [29] | ||||
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 | [30] |
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 | [31] | |
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 | [32] | |
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 | [33] | |
TOI-771 c | 0.00903 | 7.61 | 0.046±0.002 | 365 | radial velocity | 82.45 | 0.22±0.024 | 3,201±100 | [34] | |
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 | [35] |
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-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 | [36] | ||
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 | [37] |
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 | [38] | |
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 | [39] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection. [40] | |
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 | [41] | |
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 | [42] | |
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 is gone. [43] |
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 | [44] | |
TOI-3495 b | 0.3631 | 8.413073±0.000055 | 902 | transit | 562.2 | 1.42±0.17 | 6,400±230 | [45] | ||
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 | [46] |
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 | [47] | ||
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 | [46] |
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 | [48] |
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 | [49] |
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 | [49] |
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. [50] |
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 | [51] |
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 | [52] |
TOI-6695 b | 0.21 | 0.85±0.02 | 80.4 | 0.402±0.002 | 599 | transit | 922 | 1.338 | 6,400 | [53] |
TOI-6695 c | 1.45 | 242 | 0.838±0.005 | 415 | radial velocity | |||||
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 | [54] |
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 | [55] |
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 | [56] |
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 | [56] |
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 | [56] |
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 | [56] |
{{cite journal}}
: CS1 maint: bibcode (link){{cite journal}}
: CS1 maint: bibcode (link){{cite journal}}
: CS1 maint: bibcode (link)