# List of exoplanets discovered in 2024

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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 (M$_J$) | Radius (R$_J$) | Period (days) | Semi-major axis (AU) | Temp. (K) | Discovery method | Distance (ly) | Host star mass (M$_☉$) | Host star temp. (K) | Remarks |
| 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 | |
| 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. |
| 2MASS J05581644–4501559 b | 6–12 | | | 1043 | | imaging | 94.5 | 0.259±0.02 | 3218±158 | |
| 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. 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 | |
| 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 |
| 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 | 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 |
| BX Trianguli b | 7.5 | | 3923 | 4.5 | | timing | 192±7 | 0.858 (combined) | 3735 + 3359 | |
| 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. |
| CWISE J054129.32–745021.5 b | 1.8 | | | 6576 | | imaging | 111 | | | Orbits a young red dwarf. |
| 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 | |
| Gaia20eae b | 6 | | | 0.062 | | episodic accretion outbursts | 9226$^{+3130}$ $_{−2021}$ | 1.15 | 4330±300 | |
| 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$^{+0.04}$ $_{−0.05}$ | | |
| Gliese 12 b | 0.002769$^{+0.00123}$ $_{−0.0008}$ | 0.0892±0.0089 | 12.7 | 0.066±0.002 | 315±5 | transit | 39.65 | 0.241±0.006 | 3253±55 | |
| 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 |
| 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 |
| Gliese 900 b | 10.5 | | 460,000,000 | 12,000 | | imaging | 68 | 1.08 (combined) | 3976 | Located in a three-star system. It has the longest orbital time of any exoplanet so far at 1.26 million years. |
| 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 | |
| Gliese 4256 b | 0.00453±0.00044 | 0.0962±0.0058 | 0.238 | 0.0054 | 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 |
| 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 | |
| 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. |
| 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 | |
| HD 48948 c | 0.0229±0.00220 | | 37.920$^{+0.026}$ $_{−0.024}$ | 0.1951±0.0016 | 413±6 | radial vel. | 54.915±0.0228 | 0.686$^{+0.020}$ $_{−0.013}$ | 4593±60 | |
| HD 48948 d | 0.0333±0.00315 | | 150.95$^{+0.45}$ $_{−0.41}$ | 0.4894±0.0042 | 262±4 | radial vel. | 54.915±0.0228 | 0.686$^{+0.020}$ $_{−0.013}$ | 4593±60 | Closest Super Earth in habitable zone around a K-dwarf star. |
| 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. |
| 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 |
| HD 73344 b | 0.00939$^{+0.00787}$ $_{−0.00599}$ | 0.2573$^{+0.0073}$ $_{−0.0064}$ | 15.6 | 0.131 | 911±7 | transit | 114.7$^{+0.1}$ $_{−0.0}$ | 1.20±0.02 | 6028±110 | The dayside temperature can be as high as 1,066 K if the planet is tidally locked. |
| HD 73344 c | 0.367$^{+0.022}$ $_{−0.021}$ | | 65.936 | 0.3388$^{+0.0042}$ $_{−0.0043}$ | 562±4 | radial vel. | 114.7$^{+0.1}$ $_{−0.0}$ | 1.20±0.02 | 6028±110 | |
| HD 73344 d | 2.55$^{+0.56}$ $_{−0.46}$ | | 5746$^{+120}$ $_{−150}$ | 6.70$^{+0.25}$ $_{−0.26}$ | | radial vel. | 114.7$^{+0.1}$ $_{−0.0}$ | 1.20±0.02 | 6028±110 | True mass revealed using astrometry. |
| 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 | |
| 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 |
| 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. |
| 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. |
| 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 | |
| HD 111520 b | ≥1 | | 1,285,900 | ≥200 | | disk kinematics | 352.6±0.7 | 1.350±0.215 | 6542±131 | |
| HD 115587 b | 0.7 | 0.49 | 372 | | | transit | 356.2±0.5 | 1.248±0.190 | 6324±129 | |
| 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 | |
| HD 128717 b | 12.8 | | 1089.2 | 2.18 | | astrometry | 240±0.5 | 1.17$^{+0.06}$ $_{−0.16}$ | 6158±115 | |
| 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$^{+86}$ $_{−85}$ | |
| 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$^{+86}$ $_{−85}$ | |
| 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. 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 | 626±3 | 1.261±0.183 | 6351±119 | Also known as TOI-1836 Ac |
| 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. |
| 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 | |
| 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 | |
| HIP 11696 b | 4 to 16 | | | 2.5 to 28 | | astrometry | 160.8 | 1.40±0.07 | 6298 | |
| 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$^{+142}$ $_{−112}$ | May be a brown dwarf. Estimates of the mass vary from 13.8 M$_J$ to 30+31 −12 M$_J$. |
| HIP 47110 b | 3 to 10 | | | 3 to 30 | | astrometry | 126.2 | 0.98±0.05 | 4529 | |
| HIP 67522 c | | 0.731$^{+0.055}$ $_{−0.057}$ | 14.335 | 0.1235 | 915$^{+22}$ $_{−19}$ | transit | 414 | 1.2±0.05 | 5675±75 | |
| 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 | |
| IRAS 04125+2902 b | 0.3 | 0.955 | 8.83 | | | transit | 520 | 0.7 | 3720 | The youngest transiting exoplanet discovered to date. |
| 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 M$_E$ and a period of 260 days. |
| Kepler-158d | | 0.038±0.004 | 0.645088±0.000002 | | | transit | 1028±7 | 0.656$^{+0.073}$ $_{−0.049}$ | 4895.97 | |
| Kepler-879c | | 0.04±0.01 | 0.646716±0.000003 | | | transit | 2618$^{+36}$ $_{−35}$ | 0.974$^{+0.127}$ $_{−0.104}$ | 5456.75 | |
| Kepler-963c | | 0.05±0.02 | 0.919783±0.000003 | | | transit | 2516$^{+42}$ $_{−40}$ | 0.821$^{+0.120}$ $_{−0.065}$ | 5169.47 | |
| Kepler-1489c | | 0.045±0.007 | 0.680741±0.000004 | | | transit | 4185$^{+118}$ $_{−111}$ | 0.977$^{+0.050}$ $_{−0.062}$ | 5565.53 | |
| 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. |
| 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$^{+60}$ $_{−39}$ | |
| 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 | |
| KMT-2016-BLG-2321Lb | 3.58±1.22 | | | 3.58±0.81 | | microlensing | 11,670±3980 | 0.73±0.28 | | |
| KMT-2017-BLG-0849Lb | 0.0201$^{+0.0245}$ $_{−0.0097}$ | | | 2.73$^{+0.68}$ $_{−0.62}$ | | microlensing | 23,540$^{+2670}$ $_{−3220}$ | 0.19$^{+0.23}$ $_{−0.09}$ | | |
| KMT-2017-BLG-1057Lb | 0.0739$^{+0.0472}$ $_{−0.0378}$ | | | 2.36$^{+0.69}$ $_{−0.62}$ | | microlensing | 21,190$^{+2640}$ $_{−5280}$ | 0.57$^{+0.37}$ $_{−0.29}$ | | |
| KMT-2017-BLG-2331Lb | 0.538$^{+0.431}$ $_{−0.277}$ | | | 2.14$^{+0.48}$ $_{−0.42}$ | | microlensing | 26,180$^{+2740}$ $_{−3420}$ | 0.4$^{+0.32}$ $_{−0.21}$ | | |
| KMT-2020-BLG-0157Lb | 10.71$^{+6.17}$ $_{−5.61}$ | | | 11.54$^{+1.61}$ $_{−2.25}$ | | microlensing | 21,744$^{+3032}$ $_{−4238}$ | 0.58$^{+0.33}$ $_{−0.30}$ | | |
| 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$^{+0.27}$ $_{−0.11}$ | | |
| KMT-2022-BLG-0303Lb | 0.513$^{+0.410}$ $_{−0.275}$ | | | 4.81$^{+0.65}$ $_{−0.76}$ | | microlensing | 21,400$^{+2900}$ $_{−3400}$ | 0.368$^{+0.294}$ $_{−0.197}$ | | |
| KMT-2022-BLG-0732Lb | 1.12±0.65 | | | 4.11$^{+0.74}$ $_{−1.14}$ | | microlensing | 21,712$^{+3879}$ $_{−6000}$ | 0.54±0.31 | | |
| KMT-2022-BLG-1787Lb | 6.64$^{+4.98}$ $_{−3.64}$ | | | 6.3$^{+0.75}$ $_{−1.08}$ | | microlensing | 24,613$^{+2901}$ $_{−4038}$ | 0.42$^{+0.32}$ $_{−0.23}$ | | |
| KMT-2022-BLG-1852Lb | 4.98$^{+5.42}$ $_{−2.94}$ | | | 5.03$^{+0.72}$ $_{−0.92}$ | | microlensing | 20,440$^{+2934}$ $_{−3749}$ | 0.32$^{+0.34}$ $_{−0.19}$ | | |
| 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 M$_J$. |
| KMT-2023-BLG-0469Lb | 0.124$^{+0.092}$ $_{−0.067}$ | | | 2.37±0.9 | | microlensing | 23,050$^{+3260}$ $_{−3910}$ | 0.47±0.36 | | |
| KMT-2023-BLG-0735Lb | 0.12±0.07 | | | 2.75±1 | | microlensing | 20,830$^{+3910}$ $_{−3260}$ | 0.61±0.34 | | |
| 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$^{+0.33}$ $_{−0.29}$ | | |
| 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 M$_J$ and 0.77+0.87 −0.42 M$_J$ |
| KMT-2023-BLG-1642Lb | 1.08$^{+1.53}$ $_{−0.58}$ | | | 1.41$^{+0.22}$ $_{−0.27}$ | | microlensing | 22,750$^{+3550}$ $_{−4370}$ | 0.17$^{+0.24}$ $_{−0.09}$ | | |
| 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. |
| 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. |
| 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. |
| 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 | |
| M62H b | 2.83 | <0.683 | 0.133 | 0.004908 | | timing | 21,500 | 1.4 | | Pulsar planet located in the globular cluster Messier 62. Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b. |
| MOA-2016-BLG-526Lb | 6.93±0.75 | | | 2.07±0.35 | | microlensing | 22,490 | 0.4 | | |
| MOA-2022-BLG-563Lb | 0.4$^{+0.31}$ $_{−0.25}$ | | | 2.25±0.25 | | microlensing | 21,290$^{+3650}$ $_{−5220}$ | 0.48$^{+0.36}$ $_{−0.3}$ | | |
| 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/cm$^3$) |
| 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 | |
| NGTS-29 b | 0.393 | 0.857 | 69.33 | 0.347 | 414 | transit | 487±1 | 1.034±0.032 | 5730±80 | |
| NGTS-30 b | 0.96 | 0.93 | 98.3 | 0.408 | 390 | transit | 762.5 | 0.94 | 5455 | Also known as TOI-4862 b |
| 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 | |
| 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 | |
| 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 | |
| OGLE-2014-BLG-0221Lb | 4.35$^{+1.65}$ $_{−1.91}$ | | | 3.76$^{+0.96}$ $_{−1.07}$ | | microlensing | 12,000$^{+3690}$ $_{−3780}$ | 0.69$^{+0.26}$ $_{−0.30}$ | | |
| 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$^{+0.63}$ $_{−0.12}$ | | |
| OGLE-2016-BLG-1598Lb | 5.91±1.74 | | | 2.5±0.88 | | microlensing | 19,270±5670 | 0.55±0.32 | | |
| OGLE-2016-BLG-1800Lb | 2.59±1.46 | | | 1.88±0.51 | | microlensing | 21,100±3360 | 0.41±0.22 | | |
| 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$^{+0.38}$ $_{−0.3}$ | | Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11. |
| OGLE-2017-BLG-0380Lb A | 10.5 | | | | | microlensing | 6,980 | | | A pair of rogue planets. |
| OGLE-2017-BLG-0380Lb B | 3.08 | | | | | microlensing | 6,980 | | | | A pair of rogue planets. |
| OGLE-2017-BLG-0640Lb | 1.62$^{+1.64}$ $_{−0.94}$ | | | 1.14±0.38 | | microlensing | 21,600$^{+3550}$ $_{−4730}$ | 0.32$^{+0.32}$ $_{−0.18}$ | | |
| OGLE-2017-BLG-1237Lb | 3.8$^{+2.49}$ $_{−1.99}$ | | | 2.53$^{+0.5}$ $_{−0.64}$ | | microlensing | 19,660$^{+3060}$ $_{−4990}$ | 0.46$^{+0.3}$ $_{−0.24}$ | | |
| 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. |
| OGLE-2023-BLG-0836Lb | 4.36$^{+2.35}$ $_{−2.2}$ | | | 3.7$^{+1}$ $_{−1.2}$ | | microlensing | 16,690$^{+4430}$ $_{−5250}$ | | | The planet is located in a binary star system, and is likely to be orbiting both stars in the system. |
| 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. |
| SPECULOOS-3 b | | 0.08716 | 0.719 | 0.00733 | 553 | transit | 57.9 | 0.1 | 2800 | Ultra-short period planet |
| 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 | |
| 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. |
| 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 | 1.01±0.03 | 5757$^{+72}$ $_{−65}$ | |
| 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 | |
| TIC 139270665 b | 0.463 | 0.645 | 23.624 | 0.163 | 700 | transit | 618 | 1.035$^{+0.052}$ $_{−0.062}$ | 5844$^{+84}$ $_{−82}$ | |
| TIC 139270665 c | 4.89$^{+0.66}$ $_{−0.37}$ | | 1010$^{+780}$ $_{−220}$ | 2$^{+0.93}$ $_{−0.31}$ | 200$^{+18}$ $_{−35}$ | radial vel. | 618 | 1.035$^{+0.052}$ $_{−0.062}$ | 5844$^{+84}$ $_{−82}$ | |
| TIC 241249530 b | 4.98$^{+0.16}$ $_{−0.18}$ | 1.19±0.04 | 165.772 | | | transit | 1058±12 | 1.271$^{+0.061}$ $_{−0.068}$ | 6139±103 | A planet on a highly-eccentric (e=0.94) and retrograde orbit. |
| 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) Also known as TOI-6883 b |
| TIC 393818343 c | 0.357±0.132 | 0.792±0.018 | 7.8458±0.0023 | 0.079±0.011 | 1027.2089± 0.3717 | transit | 306.3±1.1 | 1.082$^{+0.055}$ $_{−0.056}$ | 5756$^{+57}$ $_{−66}$ | |
| 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. |
| TIC 434398831 c | | 0.5023$^{+0.0259}$ $_{−0.025}$ | 6.21 | 0.06572±0.00024 | 1050±10 | transit | 698±6 | 0.992$^{+0.014}$ $_{−0.018}$ | 5638±50 | Young exoplanet located in the Theia 116 association. |
| TOI-128 b | | 0.198 | 4.94 | 0.054 | 1345 | transit | 222.5±0.2 | 0.85 | 6086 | |
| 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 | |
| TOI-261 b | | 0.271 | 3.36 | 0.035 | 1722 | transit | 370.6±0.9 | 0.50 | 5890 | |
| 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. |
| 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 | |
| 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$_☉$) |
| 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 | |
| TOI-406 c | 0.02067±0.003 | 0.1846±0.0143 | 13.18 | 0.0809±0.003 | 368±14 | transit | 101±0.7 | 0.408$^{+0.046}$ $_{−0.042}$ | 3392±44 | |
| TOI-429 b | 0.8 | 0.8056±0.0196 | 338 | | | transit | 391.5±0.5 | 0.99±0.06 | 5245$^{+25}$ $_{−67}$ | |
| TOI-480 b | 0.0654 | | 6.866 | | | transit | 177.8 | 1.2 | 6212 | |
| TOI-588 b | | 1.459±0.036 | 39.4718 | | 1015 | transit | 502.9±3.2 | 2.69$^{+0.34}$ $_{−0.36}$ | 10,416$^{+254}$ $_{−220}$ | |
| 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 | |
| TOI-654 b | | 0.211 | 1.53 | 0.021 | 749 | transit | 188.7±0.18 | 0.53 | 3433 | |
| 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 | |
| TOI-663 c | 0.0115±0.00305 | 0.202±0.00892 | 4.696 | 0.0437±0.0016 | 553±24 | transit | 209.490±0.587 | 0.514±0.012 | 3681±70 | |
| TOI-663 d | <0.0164 | 0.171±0.0116 | 7.103 | 0.0576$^{+0.0021}$ $_{−0.0022}$ | 482±21 | transit | 209.490±0.587 | 0.514±0.012 | 3681±70 | |
| TOI-694 b | | 1.146±0.056 | 48.05 | | 479.8 | transit | 730.2$^{+4.1}$ $_{−4.0}$ | 1.042$^{+0.063}$ $_{−0.038}$ | 5355$^{+74}$ $_{−140}$ | |
| TOI-710 b | | 1.66±1.10 | 72.08 | | | transit | 514±2 | 1.71$^{+0.39}$ $_{−0.19}$ | 7458$^{+146}$ $_{−123}$ | |
| 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 | |
| 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. |
| TOI-782 b | <0.06 | 0.244±0.008 | 8.024 | 0.0578±0.0018 | 398±6–435±6 | transit | 170.2±0.2 | 0.397±0.01 | 3370$^{+29}$ $_{−32}$ | |
| 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 |
| TOI-815 c | 0.0739±0.00755 | 0.2337$^{+0.0089}$ $_{−0.008}$ | 34.976 | 0.193±0.004 | 469±9 | 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 |
| TOI-880 b | | 0.248 | 2.57 | 0.034 | 1163 | transit | 197.5±0.2 | 0.81 | 4935 | |
| TOI-907 b | | 0.858 | 4.58 | 0.055 | 1847 | transit | 989.9±5.0 | 1.07 | 6272 | |
| TOI-1011 b | 0.01271±0.00186 | 0.1294±0.0045 | 2.47 | 0.0346 | | transit | 170.8±0.1 | 0.92±0.03 | 5475±84 | |
| 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 | |
| TOI-1173 Ab | 0.08213±0.00598 | 0.723±0.015 | 7.064 | 0.0702±0.0012 | 863.9±9.8 | transit | 430.85 | 0.911$^{+0.028}$ $_{−0.03}$ | 5350±340 | Low-density planet located in a wide binary system. |
| 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 | |
| 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 | |
| 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. |
| TOI-1224 c | | 0.2573±0.0087 | 17.945 | | | 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. |
| 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 | |
| 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$^{+76}$ $_{−160}$ | |
| 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 | |
| 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$^{+107}$ $_{−143}$ | |
| 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 | |
| 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 | |
| TOI-1294 b | 0.1957±0.016 | 0.8199±0.0277 | 3.915 | 0.0489 | | transit | 1052±7 | 1.02±0.13 | 5714±126 | |
| TOI-1294 c | 0.467±0.053 | | 160.1±2.5 | 0.581 | | radial vel. | 1052±7 | 1.02±0.13 | 5714±126 | |
| 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 | |
| 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 |
| TOI-1347 c | 0.0088±0.0072 | 0.143±0.009 | 4.842 | | 1000±25 | transit | 480.8±2 | 0.913±0.033 | 5464±100 | |
| 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$^{+76}$ $_{−73}$ | |
| 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$^{+76}$ $_{−73}$ | |
| 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 | |
| TOI-1410 b | | 0.262 | 1.22 | 0.020 | 1396 | transit | 236.7±0.2 | 0.72 | 4635 | |
| 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 | transit + radial vel. | 336 | 1.10±0.10 | 6008±113 | |
| 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 | |
| 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$^{+111}$ $_{−140}$ | |
| TOI-1448 b | <0.0613 | 0.245±0.006 | 8.112 | 0.0567±0.0015 | 389±5–426±6 | transit | 240±0.3 | 0.372±0.009 | 3412$^{+28}$ $_{−32}$ | |
| 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. |
| TOI-1450 Ac | 0.0048±0.0006 | | 5.07 | | 533±26 | radial vel. | 73.2±0.1 | 0.48±0.024 | 3437±86 | Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab. |
| 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 | |
| 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$^{+119}$ $_{−144}$ | |
| 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 | |
| TOI-1683 b | | 0.236 | 3.06 | 0.037 | 929 | transit | 166.2±0.2 | 0.69 | 4402 | |
| 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$^{+209}$ $_{−165}$ | |
| 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$^{+149}$ $_{−101}$ | |
| 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). |
| 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 | |
| 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$^{+95}$ $_{−148}$ | |
| 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 | |
| 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 | |
| TOI-1798 b | | 0.126 | 0.44 | 0.011 | 2122 | transit | 369.147$^{+1.008}$ $_{−1.005}$ | 0.86 | 5165 | |
| 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 | 369.147$^{+1.008}$ $_{−1.005}$ | 0.86 | 5165 | |
| 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$^{+121}$ $_{−124}$ | |
| 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 | |
| TOI-1803 c | 0.01794±0.00944 | 0.3738$^{+0.0223}$ $_{−0.0267}$ | 12.885776±0.000036 | 0.097±0.002 | 561±10 | transit | 388.3 | 0.756$^{+0.050}$ $_{−0.042}$ | 4687±65 | |
| TOI-1806 b | | 0.304 | 15.15 | 0.088 | 337 | transit | 180.7±0.2 | 0.39 | 3272 | |
| 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 | |
| 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. |
| TOI-1828 b | 0.1841±0.012 | 0.769±0.017 | 9.09 | 0.0859 | | transit | 1208±8 | 1.04±0.13 | 5809±127 | |
| 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$^{+89}$ $_{−83}$ | |
| TOI-1883 b | | 0.4953±0.0460 | 4.506 | | 524.9 | transit | 376±3 | 0.492±0.02 | 3477±157 | |
| TOI-1885 b | 1.624±0.103 | 1.219±0.037 | 6.544060±0.000006 | | | transit | 1826.773$^{+21.464}$ $_{−20.982}$ | | 6527±98 | |
| 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$^{+139}$ $_{−144}$ | |
| TOI-2019 b | 0.109±0.0132 | 0.505±0.0250 | 15.3444±0.0055 | | | transit | 645.812$^{+2.684}$ $_{−2.665}$ | | 5590 | |
| 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$^{+94}$ $_{−93}$ | |
| TOI-2120 b | <0.02139 | 0.1893±0.0056 | 5.8 | 0.0377±0.0013 | 351±6–384±6 | transit | 104.9 | 0.211±0.005 | 3131±30 | |
| 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$^{+114}$ $_{−90}$ | |
| TOI-2264 b | | 0.3726±0.0355 | 55.08 | | 373.1 | transit | 617.2$^{+7.1}$ $_{−6.9}$ | 1.164$^{+0.146}$ $_{−0.168}$ | 6140$^{+129}$ $_{−128}$ | |
| 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 | |
| TOI-2274 b | | | 2.679 | | 771 | transit | 159.9±0.2 | 0.612±0.02 | 3943±157 | |
| 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$^{+147}$ $_{−277}$ | |
| 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. |
| 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. | 409.36$^{+0.52}$ $_{−0.46}$ | 1.168$^{+0.070}$ $_{−0.071}$ | 5730±140 | |
| 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$^{+147}$ $_{−144}$ | |
| 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$^{+230}$ $_{−170}$ | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | 1.158±0.098 | | |
| 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. |
| TOI-2458 c | 0.03216$^{+0.00538}$ $_{−0.00598}$ | | 16.553$^{+0.059}$ $_{−0.061}$ | 0.129±0.002 | | radial vel. | 368.42$^{+1.76}$ $_{−1.74}$ | 1.05±0.03 | 6005±50 | |
| TOI-2477 b | | 1.156±0.403 | 34.78 | | | transit | 1181.4$^{+16.8}$ $_{−16.3}$ | 1.73$^{+0.40}$ $_{−0.21}$ | 7505$^{+192}$ $_{−222}$ | |
| 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 | 1.163±0.053 | | |
| 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 | |
| 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$^{+60}$ $_{−52}$ | |
| 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 | |
| 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. | 594.97$^{+3.42}$ $_{−3.03}$ | 0.771±0.049 | 4870±150 | |
| 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 | |
| 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 | |
| TOI-2768 b | | 0.2688±0.0313 | 1.508 | | 855 | transit | 255.8±0.6 | 0.63$^{+0.06}$ $_{−0.10}$ | 4008$^{+124}$ $_{−137}$ | |
| 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 | |
| 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 | |
| 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 |
| 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 | |
| TOI-3353 b | | 0.238 | 4.67 | 0.060 | 1264 | transit | 257.1±0.2 | 1.33 | 6365 | |
| 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 | |
| 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$^{+157}$ $_{−155}$ | |
| 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 | |
| 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 | |
| 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$^{+150}$ $_{−180}$ | |
| 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. |
| TOI-4356 b | | 0.321±0.198 | 289.92 | | | transit | 668.6±3.8 | 1.48$^{+0.32}$ $_{−0.19}$ | 6855$^{+140}$ $_{−127}$ | |
| 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. |
| 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 | |
| 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 | |
| TOI-4443 b | | 0.153 | 1.85 | 0.030 | 1639 | transit | | 1.05 | 5834 | |
| TOI-4468 b | | 1.0197±0.0517 | 2.77 | | | transit | 1224.7±8.2 | 0.82 | 4975±122 | |
| TOI-4468 c | | 0.296±0.023 | 7.01 | | | transit | 1224.7±8.2 | 0.82 | 4975±122 | |
| TOI-4495 b | | 0.324 | 5.18 | 0.062 | 1383 | transit | | 1.17 | 6156 | |
| 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 | |
| TOI-4504 c | 3.77±0.18 | 0.9897±0.0092 | 82.97213±0.00013 | 0.3546$^{+0.0073}$ $_{−0.0077}$ | | transit + radial vel. | 1117.43±5.57 | 0.89$^{+0.06}$ $_{−0.04}$ | 5315±60 | |
| TOI-4504 d | 1.417±0.065 | | 40.5634$^{+0.0365}$ $_{−0.0368}$ | 0.2219$^{+0.0041}$ $_{−0.0043}$ | | timing | 1117.43±5.57 | 0.89$^{+0.06}$ $_{−0.04}$ | 5315±60 | |
| TOI-4527 b | | 0.0812 | 0.40 | 0.008 | 1363 | transit | | 0.48 | 3702 | |
| TOI-4562 c | 5.77$^{+0.37}$ $_{−0.56}$ | | 3990$^{+201}$ $_{−192}$ | 5.219±0.002 | | timing | 1131±12 | 1.218$^{+0.054}$ $_{−0.048}$ | 6096±32 | |
| TOI-4602 b | | 0.227 | 3.98 | 0.051 | 1380 | transit | | 1.12 | 6012 | |
| 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 | 5600±50 or 5800±50 | Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron. |
| 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 | |
| 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 | |
| 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 | |
| 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$^{+145}$ $_{−144}$ | |
| 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 | |
| TOI-5082 b | | 0.227 | 4.24 | 0.051 | 1165 | transit | | 1.00 | 5670 | |
| 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 | |
| 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 | |
| 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$^{+180}$ $_{−190}$ | |
| 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 | |
| TOI-5319 b | | 0.33427±0.0551 | 4.079 | | 695 | transit | 199.4±0.7 | 0.5±0.1 | 3580$^{+107}$ $_{−141}$ | |
| TOI-5388 b | | 0.169 | 2.59 | 0.024 | 601 | transit | | 0.29 | 3495 | |
| TOI-5575 b | | 0.8459±0.0255 | 32.07 | | 195 | transit | 184.9±0.6 | 0.21±0.02 | 3176±157 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | 0.265±0.006 | 3228±41 | |
| 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 | |
| TOI-5723 b | | 1.146±0.068 | 56.88 | | | transit | 1878$^{+22}$ $_{−21}$ | 1.01$^{+0.12}$ $_{−0.15}$ | 5695$^{+110}$ $_{−170}$ | |
| TOI-5731 b | | 0.401±0.046 | 90.1 | | | transit | 358.2±0.8 | 0.697$^{+0.088}$ $_{−0.077}$ | 4448$^{+92}$ $_{−123}$ | |
| TOI-5975 b | | 0.7536±0.0422 | 186.52 | | | transit | 1141$^{+7.1}$ $_{−7.0}$ | 1.335$^{+0.260}$ $_{−0.188}$ | 6508$^{+83}$ $_{−163}$ | |
| 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 | 0.21 | 3241$^{+80}$ $_{−60}$ | |
| 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 |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| 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 | |
| TOI-6324 b | 0.0041±0.0006 | 0.0937 | 0.28 | | | transit | 67.02±0.05 | 0.272±0.020 | 3358±160 | |
| 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 | |
| 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 | |
| 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 | 1.323$^{+0.050}$ $_{−0.045}$ | 5940±110 | |
| 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$^{+143}$ $_{−142}$ | |
| TOI-7041 b | 0.36±0.16 | 1.02±0.03 | 9.691±0.006 | | | transit | 1431±10 | 1.12±0.02 | 4640±10 | |
| 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 |
| 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 | |
| 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 |

## Specific exoplanet lists

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

* 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 (869)
* 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 (248)
* 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 (18)