List of exoplanets discovered in 2025
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 | ||||
| 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 |
|||
| Barnard's Star c | 0.00105 | 4.12 | 0.0274±0.0004 | radial vel. | 5.96 | 0.162 | 3,195 | |||
| 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 | 1.3445 | 6,033 | A circumbinary planet. | ||
| 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. |
| 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. | ||||
| 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. | ||
| 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. | ||||
| 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 | |||
| 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 | |||
| 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. | ||
| 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. | ||
| Gliese 536 c | 0.01853±0.0022 | 32.76 | 0.1617±0.003 | 290 | radial vel. | 32.71 | 0.52±0.05 | 3685±68 | ||
| 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 | |||
| 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 | |||
| Gliese 508.2 b | 1.85 | ~5300 | 4.85 | radial vel. | 54.3 | 0.54±0.12 | 3,720±12 | |||
| GJ 9773 b | 0.543 | 2965 | 2.921±0.045 | radial vel. | 51.8 | 0.358±0.011 | 3,528±25 | |||
| HD 85426 c | 0.0324+0.0050 −0.0047 |
35.73+0.09 −0.10 |
0.2118+0.0050 −0.0044 |
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. | |
| 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. | ||
| 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. | ||
| 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 | |||
| 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 | ||
| 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. |
| 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 | |
| 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. |
| 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 | ||
| 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 . | ||||||
| J042705.86+261520.3 b | 3.9 | imaging | 522 | Part of a JuMBO along with J042705.86+261520.3. | ||||||
| J041546.22+280811.4 | 6.0 | imaging | – | Free-floating object of planetary mass. Could also be a sub-brown dwarf. | ||||||
| K2-157 c | 0.0969 | 25.9 | 0.165±0.0018 | 587 | radial vel. | 946.5 | 0.89 ± 0.029 | 5,334 ± 64 | ||
| 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 | ||||
| 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 | |||
| 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 | |||
| Kepler-725 c | 0.031 | 207.5 | 0.674±0.002 | timing | 2474±45 | 0.91 | 5,293±122 | Partially in habitable zone. | ||
| 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 |
|||||
| 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 |
|||||
| 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 |
|||||
| 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 |
|||||
| 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 |
|||||
| 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 | |||||
| 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 |
|||||
| 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 |
|||||
| 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 | |||||
| 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 |
|||||
| 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 | |||||
| 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 | ||||
| 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 |
|||||
| 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 |
|||||
| 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 |
|||||
| 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 | ||
| 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 | ||
| 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 | ||||
| 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 | ||
| 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 |
|||||
| 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 |
|||||
| MP Muscae b | 5.0 | 1 – 3 | astrometry + disk kinematics | 319.3 | 1.3±0.08 | 5000 | ||||
| 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. | ||
| 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 |
|||||
| OGLE-2023-BLG-0524 | 0.0293 or 0.182 | microlensing | – | Free-floating object of planetary mass. | ||||||
| o005 s41280 | 8.4 | 2.3 | 2,162 | imaging | 17,300 | Free-floating object of planetary mass. Could also be a sub-brown dwarf. | ||||
| o006 s00089 | 11.5 | 1.2 | 955 | imaging | 6,520 | Free-floating object of planetary mass. Could also be a sub-brown dwarf. | ||||
| 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 | |
| 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 | ||
| 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 | ||
| 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 | |
| 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. |
| 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 | ||
| TOI-771 c | 0.00903 | 7.61 | 0.046±0.002 | 365 | radial vel. | 82.45 | 0.22±0.024 | 3,201±100 | ||
| 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 | |
| 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. |
| 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 | |||
| 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 | |
| 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 | ||
| 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 |
Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection. | |
| 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 | ||
| TOI-2267 b | 0.0893 or 0.1089 | 2.2891 | 0.0205 or 0.0127 | transit | 73.5 | 0.270 | 3,030±100 | |||
| 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 | ||
| TOI-2427 c | 0.02033 | 5.15±0.01 | 0.05±0.01 | radial vel. | 92.95 | 0.64±0.02 | 4,072±121 | |||
| 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. |
| 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. |
| 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 | |
| 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 | |
| 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 | ||
| TOI-3495 b | 0.3631 | 8.413073±0.000055 | 902 | transit | 562.2 | 1.42±0.17 | 6,400±230 | |||
| 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 | ||
| 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 | |
| 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 | |||
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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. |
| 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 | |
| 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 | |
| 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 | |
| TOI-6695 b | 0.21 | 0.85±0.02 | 80.4 | 0.402±0.002 | 599 | transit | 922 | 1.338 | 6,400 | |
| 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 | |
| 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 | |
| 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. | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| WISPIT 1 b | 10.4+0.7 −0.8 |
338 | imaging | 747 | 4,670+990 −540 |
Circumbinary planets. | ||||
| 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 |