# List of exoplanets discovered in 2022

This list of exoplanets discovered in 2022 is a list of confirmed exoplanets that were first reported in 2022. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.
On 31 March 2022, K2-2016-BLG-0005Lb was reported to be the most distant exoplanet found by Kepler to date.
| 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 |
| 29 Cygni b | 13.9$^{+6.1}$ $_{−5.1}$ | | | 16.9$^{+3.4}$ $_{−1.9}$ | | astrometry + imaging | 130.9±0.9 | 2.14±0.15 | 8790$^{+1513}$ $_{−1292}$ | Host star also known as HIP 99770 |
| CoRoT-35b | 1.10±0.37 | 1.68±0.11 | 3.22748±0.00008 | 0.04290±0.00092 | 1747±62 | transit | 3700±200 | 1.01$^{+0.07}$ $_{−0.06}$ | 6390±130 | |
| CoRoT-36b | 0.68$^{+0.47}$ $_{−0.43}$ | 1.41±0.14 | 5.616531±0.000023 | 0.066±0.007 | 1567±35 | transit | 3110±60 | 1.32±0.09 | 6730±140 | |
| EPIC 206317286 c | 0.0168±0.098 | 0.186$^{+0.015}$ $_{−0.014}$ | 17.51547$^{+0.00228}$ $_{−0.00296}$ | | 570 | transit | | 0.832$^{+0.253}$ $_{−0.367}$ | 4752±138 | |
| EPIC 210768568 b | | 0.088±0.004 | 3.2141±0.0002 | 0.0511$^{+0.0021}$ $_{−0.0028}$ | | transit | 965 | 1.018±0.131 | 5711±105 | |
| EPIC 246078343 b | | 0.068±0.007 | 0.8094±0.00003 | 0.0117$^{+0.0009}$ $_{−0.0012}$ | | transit | 954 | 0.808$^{+0.364}$ $_{−0.256}$ | 4116±138 | |
| EPIC 246078343 c | | 0.110±0.006 | 5.3301±0.0003 | 0.0426$^{+0.0016}$ $_{−0.0019}$ | | transit | 954 | 0.808$^{+0.364}$ $_{−0.256}$ | 4116±138 | |
| EPIC 246220667 b | | 0.172±0.006 | 6.6690±0.0002 | 0.0552$^{+0.0017}$ $_{−0.0023}$ | | transit | 835 | 0.814$^{+0.363}$ $_{−0.251}$ | 4343±138 | |
| EPIC 246220667 c | | 0.109±0.006 | 4.3696±0.0001 | 0.0487$^{+0.0027}$ $_{−0.0031}$ | | transit | 835 | 0.814$^{+0.363}$ $_{−0.251}$ | 4343±138 | |
| EPIC 247422570 b | | 0.189±0.009 | 5.9382$^{+0.0006}$ $_{−0.0004}$ | 0.0586$^{+0.0032}$ $_{−0.0033}$ | | transit | 2181 | 0.893$^{+0.406}$ $_{−0.275}$ | 5590±138 | |
| Gaia-1b | 1.68±0.11 | 1.229±0.021 | 3.052524±0.000017 | 0.04047±0.00094 | | transit | 1201±7 | 0.949±0.066 | 5470±110 | First confirmed exoplanet discovered by Gaia, along with Gaia-2b |
| Gaia-2b | 0.817±0.047 | 1.322±0.013 | 3.6915224±0.0000039 | 0.0467±0.0015 | | transit | 676±3 | 1.000±0.095 | 5720±84 | First confirmed exoplanet discovered by Gaia, along with Gaia-1b |
| Gliese 514b | 0.0164±0.0028 | | 140.43±0.41 | 0.422$^{+0.014}$ $_{−0.015}$ | 202±11 | radial vel. | 24.850±0.010 | 0.510±0.051 | 3714±51 | Planetary orbit partially in habitable zone |
| Gliese 1002 b | 0.0034±0.0004 | | 10.3465±0.027 | 0.0457±0.0013 | 230.9±6.7 | radial vel. | 15.808±0.003 | 0.120±0.010 | 3024±52 | Planet in habitable zone |
| Gliese 1002 c | 0.0043±0.0005 | | 21.202±0.013 | 0.0738±0.0021 | 181.7±5.2 | radial vel. | 15.808±0.003 | 0.120±0.010 | 3024±52 | Planet in habitable zone |
| Gliese 3929 b | 0.0055±0.0014 | 0.097±0.004 | 2.6162745±0.000003 | 0.0252±0.0005 | 568±6 | transit | 51.64±0.02 | 0.309±0.014 | 3369±51 | Another planet in system is suspected |
| Gliese 3929 c | 0.0180±0.0029 | | 15.04±0.03 | 0.081±0.002 | 317±3 | radial vel. | 51.64±0.02 | 0.309±0.014 | 3369±51 | |
| GJ 463 b | 3.6±0.4 | | 3448$^{+110}$ $_{−88}$ | 3.53±0.07 | | radial vel. | 59.91±0.03 | 0.49±0.02 | 3540±41 | Host star also known as Ross 690 |
| GJ 3090 b | 0.0105 | 0.19 | 2.8531042±0.0000032 | 0.03165 | 696 | transit | 73.21±0.04 | 0.519±0.013 | 3556±70 | Host star also known as TOI-177 |
| GJ 3090 c | 0.0538 | | 12.734$^{+0.033}$ $_{−0.026}$ | 0.08575 | 421 | radial vel. | 73.21±0.04 | 0.519±0.013 | 3556±70 | Host star also known as TOI-177 |
| HD 3167 e | 0.0306±0.0037 | | 102.09$^{+0.52}$ $_{−0.50}$ | 0.4048$^{+0.0077}$ $_{−0.0074}$ | 375±7 | radial vel. | 154.59±0.13 | 0.852$^{+0.026}$ $_{−0.015}$ | 5300±73 | |
| HD 18599 b | 0.0758$^{+0.0223}$ $_{−0.0242}$ | 0.232±0.012 | 4.1374354$^{+0.0000036}$ $_{−0.0000037}$ | 0.0480±0.0004 | 935±11 | transit | 126.02±0.06 | 0.863±0.020 | 5145±50 | Host star also known as TOI-179, also red dwarf star in the system |
| HD 20329b | 0.0233±0.0034 | 0.154±0.006 | 0.926118$^{+0.000050}$ $_{−0.000043}$ | 0.0180±0.0003 | 2141±27 | transit | 207.7±0.9 | 0.90±0.05 | 5596±50 | |
| HD 22532 b | 2.12±0.09 | | 872.6±2.8 | 1.900±0.004 | | radial vel. | 526±2 | 1.20±0.05 | 5067$^{+59}$ $_{−22}$ | Giant host star |
| HD 22946 b | | 0.154±0.009 | 4.040301$^{+0.000023}$ $_{−0.000042}$ | 0.0528±0.0030 | 1378±36 | transit | 205.08±0.16 | 1.158±0.058 | 6210$^{+173}$ $_{−158}$ | Host star also known as TOI-411, third transiting planet in system is suspected |
| HD 22946 c | | 0.245±0.013 | 9.573096$^{+0.000026}$ $_{−0.000023}$ | 0.0939±0.0054 | 1033±27 | transit | 205.08±0.16 | 1.158±0.058 | 6210$^{+173}$ $_{−158}$ | Host star also known as TOI-411, third transiting planet in system is suspected |
| HD 23472 d | 0.0017±0.0006 | 0.067±0.005 | 3.97664$^{+0.000030}$ $_{−0.000044}$ | 0.04298$^{+0.00063}$ $_{−0.00065}$ | 909$^{+35}$ $_{−32}$ | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | |
| HD 23472 e | 0.0023±0.0009 | 0.073±0.006 | 7.90754±0.00011 | 0.0680±0.0010 | 723$^{+28}$ $_{−25}$ | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | |
| HD 23472 f | 0.0024±0.0013 | 0.102±0.007 | 12.1621839$^{+0.00012}$ $_{−0.000099}$ | 0.0906±0.0014 | 630$^{+27}$ $_{−23}$ | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | |
| HD 28109 b | 0.058$^{+0.029}$ $_{−0.024}$ | 0.196±0.009 | 22.89104$^{+0.00035}$ $_{−0.00036}$ | 0.1357±0.0034 | 881.2±7.5 | transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | |
| HD 28109 c | 0.025$^{+0.013}$ $_{−0.010}$ | 0.378±0.010 | 56.00819$^{+0.00194}$ $_{−0.00202}$ | 0.308±0.011 | 585.2$^{+8.7}$ $_{−8.3}$ | transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | |
| HD 28109 d | 0.018$^{+0.009}$ $_{−0.007}$ | 0.290±0.010 | 84.25999$^{+0.00744}$ $_{−0.00662}$ | 0.411±0.016 | 506.5$^{+8.7}$ $_{−8.0}$ | transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | |
| HD 29399 b | 1.57±0.11 | | 892.7±5.9 | 1.913±0.008 | | radial vel. | 144.2±0.3 | 1.15±0.04 | 4845±52 | Giant host star |
| HD 33142 d | 0.89$^{+0.06}$ $_{−0.05}$ | | 810.2$^{+3.8}$ $_{−4.2}$ | 1.955$^{+0.016}$ $_{−0.012}$ | | radial vel. | 394.3±0.9 | 1.52±0.03 | 5025.4$^{+23.6}$ $_{−15.5}$ | Giant host star |
| HD 56414 b | 0.0944±0.0053 | 0.331±0.018 | 29.04992±0.00021 | 0.229±0.004 | 1133±30 | transit | 873±3 | 1.89±0.11 | 8500±150 | Host star also known as TOI-1228 |
| HD 64121 b | 2.56±0.19 | | 623.0±3.4 | 1.510±0.006 | | radial vel. | 424.1±1.7 | 1.18±0.05 | 5066$^{+58}$ $_{−60}$ | Giant host star |
| HD 69123 b | 3.04±0.16 | | 1193.3±7.0 | 2.482±0.010 | | radial vel. | 245.0±1.3 | 1.43±0.07 | 4787$^{+280}$ $_{−51}$ | Giant host star |
| HD 83443 c | 1.5$^{+0.5}$ $_{−0.2}$ | | 8241$^{+1019}$ $_{−530}$ | 8.0±0.8 | | radial vel. | 133.6±0.2 | 1.00±0.03 | 5442±17 | Eccentric orbit due to hot Jupiter in system |
| HD 93963A b | | 0.121±0.004 | 1.0391353$^{+0.0000049}$ $_{−0.0000045}$ | 0.02085±0.00037 | 2042±27 | transit | 268.6±1.3 | 1.109±0.043 | 5987±64 | Host star also known as TOI-1797 |
| HD 93963A c | | 0.288±0.005 | 3.6451398$^{+0.0000106}$ $_{−0.0000142}$ | 0.04813±0.00085 | 1344±18 | transit | 268.6±1.3 | 1.109±0.043 | 5987±64 | Host star also known as TOI-1797 |
| HD 109833 b | | 0.258$^{+0.014}$ $_{−0.012}$ | 9.188526±0.000026 | | | transit | 259.5±0.2 | 1.08±0.05 | 5881±50 | Young host star also known as TOI-1097 |
| HD 109833 c | | 0.231$^{+0.018}$ $_{−0.016}$ | 13.900148±0.000057 | | | transit | 259.5±0.2 | 1.08±0.05 | 5881±50 | Young host star also known as TOI-1097 |
| HD 114082 b | 8.0±1.0 | 1.00±0.03 | 109.75$^{+0.40}$ $_{−0.37}$ | 0.5109$^{+0.0081}$ $_{−0.0083}$ | | transit | 310.1±0.7 | 1.47±0.07 | 6651±35 | Young star, eccentric planetary orbit |
| HD 167768 b [zh] | 0.85$^{+0.12}$ $_{−0.11}$ | | 20.6532$^{+0.0032}$ $_{−0.0032}$ | 0.1512$^{+0.0058}$ $_{−0.0063}$ | 1874 | radial vel. | 353.5 | 1.08$^{+0.14}$ $_{−0.12}$ | 4830 | Host red giant star also known as HR 6840, other planets in system are suspected |
| HD 191939 g | 0.0425±0.0063 | | 284$^{+10}$ $_{−8}$ | 0.812±0.028 | 278±6 | radial vel. | 174.4±0.1 | 0.81±0.04 | 5348±100 | Habitable zone planet |
| HD 191939 f | >2.1 | | >2200 | >3.2 | <125 | | 174.4±0.1 | 0.81±0.04 | 5348±100 | |
| HD 199981 b | 10.070±2.483 | | 21000±8000 | 13.048±3.073 | | radial vel. | 66.7±2.4 | | | Host star also known as GJ 9714 |
| HD 105618 b | 0.079±0.008 | | 9.9 | 0.091±0.004 | | radial vel. | 227.8±0.4 | | | Also brown dwarf in the system |
| HD 206893 c | 12.3$^{+1.1}$ $_{−1.2}$ | 1.46$^{+0.18}$ $_{−0.06}$ | 2082 | 3.53$^{+0.08}$ $_{−0.07}$ | 1181.9$^{+20.6}$ $_{−53.9}$ | radial vel. | 125.1±2.6 | 1.24 | 6486 | Some deuterium burning despite its low mass, also another brown dwarf is present in the system |
| HD 21019 b [zh] | 0.014±0.002 | | 2.56 | 0.034±0.002 | | radial vel. | 120 | | | Host star also known as GJ 2030 |
| HD 21019 c [zh] | 12.934±2.361 | | 25600±2500 | 16.752±1.312 | | radial vel. | 120 | | | Host star also known as GJ 2030 |
| HD 21175 b | 0.038±0.010 | | 10.6 | 0.091±0.004 | | radial vel. | 57.7 | | | Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system |
| HD 260655 b | 0.0067±0.0011 | 0.111±0.002 | 2.76953±0.00003 | 0.02933±0.00024 | 709±4 | transit | 32.63±0.07 | 0.439±0.011 | 3803±10 | Host star also known as TOI-4599 |
| HD 260655 c | 0.0097±0.0015 | 0.137±0.004 | 5.70588±0.00007 | 0.04749±0.00039 | 557±3 | transit | 32.63±0.07 | 0.439±0.011 | 3803±10 | Host star also known as TOI-4599 |
| HIP 34269 b [ja] | 0.0052±0.0007 | 0.103±0.005 | 0.548177±0.000019 | 0.01188±0.00040 | 1617±41 | transit | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500 |
| HIP 34269 c [ja] | 0.0146±0.0016 | | 6.6356±0.0040 | | | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500 |
| HIP 34269 d [ja] | 0.1055±0.0033 | | 26.233±0.020 | | | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500 |
| HIP 34269 e [ja] | 0.0376±0.0042 | | 61.30±0.28 | | | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500 |
| HIP 94235 b | | 0.268±0.027 | 7.713057±0.000021 | 0.07870$^{+0.00056}$ $_{−0.00017}$ | 1060±50 | transit | 191.2±0.4 | 1.094$^{+0.024}$ $_{−0.007}$ | 5991±50 | Host star also known as TOI-4399, shares system with a red dwarf |
| HR 7321 b | 0.30±0.07 | | 285.1$^{+1.2}$ $_{−1.5}$ | 0.937±0.003 | | radial vel. | 200.2 | 1.35$^{+0.19}$ $_{−0.21}$ | 4971 | Red giant host star also known as HD 184010 |
| HR 7321 c | 0.28$^{+0.08}$ $_{−0.10}$ | | 483.3$^{+3.2}$ $_{−4.0}$ | 1.332$^{+0.006}$ $_{−0.007}$ | | radial vel. | 200.2 | 1.35$^{+0.19}$ $_{−0.21}$ | 4971 | Red giant host star also known as HD 184010 |
| HR 7321 d | 0.46±0.08 | | 837.7$^{+6.4}$ $_{−5.5}$ | 1.922$^{+0.010}$ $_{−0.008}$ | | radial vel. | 200.2 | 1.35$^{+0.19}$ $_{−0.21}$ | 4971 | Red giant host star also known as HD 184010 |
| K2-365 b | 0.0272±0.0172 | 0.259$^{+0.017}$ $_{−0.015}$ | 23.448172$^{+0.00076}$ $_{−0.00099}$ | | 710 | transit | | 0.823$^{+0.369}$ $_{−0.25}$ | 5561±138 | |
| K2-366 b | 0.0199±0.0115 | 0.210$^{+0.016}$ $_{−0.014}$ | 15.93703$^{+0.00079}$ $_{−0.00114}$ | | 770 | transit | | 0.825$^{+0.366}$ $_{−0.255}$ | 5601±138 | |
| K2-367 b | 0.0203±0.0126 | 0.215$^{+0.020}$ $_{−0.017}$ | 20.64509$^{+0.00099}$ $_{−0.00137}$ | | 450 | transit | | 0.756$^{+0.231}$ $_{−0.347}$ | 4348±128 | |
| K2-368 b | 0.0073±0.0042 | 0.118$^{+0.009}$ $_{−0.008}$ | 5.02559$^{+0.00028}$ $_{−0.00034}$ | | 800 | transit | | 0.746$^{+0.334}$ $_{−0.232}$ | 4663±138 | |
| K2-368 c | 0.0078±0.0041 | 0.121$^{+0.010}$ $_{−0.009}$ | 9.66018±0.00116 | | 650 | transit | | 0.746$^{+0.334}$ $_{−0.232}$ | 4663±138 | |
| K2-368 d | 0.0146±0.0085 | 0.173$^{+0.013}$ $_{−0.012}$ | 20.20108$^{+0.00235}$ $_{−0.00273}$ | | 500 | transit | | 0.746$^{+0.334}$ $_{−0.232}$ | 4663±138 | |
| K2-369 b | 0.0069±0.0040 | 0.117$^{+0.009}$ $_{−0.008}$ | 5.76161$^{+0.00084}$ $_{−0.00071}$ | | 1080 | transit | | 0.735$^{+0.334}$ $_{−0.224}$ | 5682±138 | |
| K2-370 b | 0.0327±0.0207 | 0.286$^{+0.020}$ $_{−0.048}$ | 2.14084$^{+0.00003}$ $_{−0.00004}$ | | 1420 | transit | | 0.984$^{+0.428}$ $_{−0.303}$ | 5377±138 | |
| K2-371 b | 4.7±2.2 | 1.162$^{+0.082}$ $_{−0.077}$ | 3.11490±0.00001 | | 1000 | transit | | 0.958$^{+0.44}$ $_{−0.298}$ | 4925±138 | |
| K2-372 b | 0.0289±0.0168 | 0.262±0.006 | 9.84407$^{+0.00056}$ $_{−0.00057}$ | | 870 | transit | | 0.847$^{+0.101}$ $_{−0.088}$ | 5479±27 | |
| K2-373 b | 0.0162±0.0089 | 0.184$^{+0.013}$ $_{−0.012}$ | 11.02066$^{+0.00143}$ $_{−0.00136}$ | | 1130 | transit | | 1.158$^{+0.499}$ $_{−0.349}$ | 6138±138 | |
| K2-374 b | 0.0113±0.0058 | 0.142±0.005 | 4.52195$^{+0.00032}$ $_{−0.00040}$ | | 1210 | transit | | 0.731$^{+0.067}$ $_{−0.061}$ | 5789±21 | |
| K2-374 c | 0.0179±0.0109 | 0.197$^{+0.008}$ $_{−0.007}$ | 16.43445$^{+0.00237}$ $_{−0.00270}$ | | 790 | transit | | 0.731$^{+0.067}$ $_{−0.061}$ | 5789±21 | |
| K2-375 b | 0.0183±0.0106 | 0.200$^{+0.016}$ $_{−0.015}$ | 14.45389$^{+0.00477}$ $_{−0.00417}$ | | 1000 | transit | | 1.119$^{+0.492}$ $_{−0.344}$ | 5822±138 | |
| K2-376 b | 0.0129±0.0074 | 0.155$^{+0.011}$ $_{−0.010}$ | 5.77647$^{+0.00026}$ $_{−0.00023}$ | | 1240 | transit | | 0.908$^{+0.394}$ $_{−0.281}$ | 5937±138 | |
| K2-377 b | 0.0123±0.0073 | 0.151$^{+0.013}$ $_{−0.011}$ | 12.83223$^{+0.00155}$ $_{−0.00161}$ | | 530 | transit | | 0.821$^{+0.371}$ $_{−0.258}$ | 4200±138 | |
| K2-378 b | 0.0283±0.0173 | 0.257$^{+0.024}$ $_{−0.020}$ | 2.06043$^{+0.00011}$ $_{−0.00007}$ | | 1130 | transit | | 0.923$^{+0.425}$ $_{−0.291}$ | 4823±138 | |
| K2-379 b | 0.0175±0.0104 | 0.194$^{+0.032}$ $_{−0.017}$ | 8.77724$^{+0.00062}$ $_{−0.00061}$ | | 680 | transit | | 0.856$^{+0.375}$ $_{−0.265}$ | 4603±138 | |
| K2-380 b | 0.0250±0.0144 | 0.243$^{+0.016}$ $_{−0.015}$ | 9.40131$^{+0.00046}$ $_{−0.00050}$ | | 1110 | transit | | 0.993$^{+0.416}$ $_{−0.302}$ | 5911±138 | |
| K2-381 b | 0.0040±0.0026 | 0.095$^{+0.012}$ $_{−0.009}$ | 7.93893±0.00059 | | 670 | transit | | 0.754$^{+0.337}$ $_{−0.239}$ | 4473±138 | |
| K2-381 c | 0.0158±0.0094 | 0.178$^{+0.016}$ $_{−0.013}$ | 16.03465$^{+0.00184}$ $_{−0.00157}$ | | 530 | transit | | 0.754$^{+0.337}$ $_{−0.239}$ | 4473±138 | |
| K2-381 d | 0.0121±0.0070 | 0.150$^{+0.016}$ $_{−0.012}$ | 26.80302$^{+0.00277}$ $_{−0.00304}$ | | 440 | transit | | 0.754$^{+0.337}$ $_{−0.239}$ | 4473±138 | |
| K2-382 b | 0.0162±0.0101 | 0.185$^{+0.013}$ $_{−0.011}$ | 21.70015$^{+0.00202}$ $_{−0.00191}$ | | 610 | transit | | 0.922$^{+0.401}$ $_{−0.284}$ | 5452±138 | |
| K2-383 b | 0.0102±0.0052 | 0.139$^{+0.010}$ $_{−0.009}$ | 1.86596±0.00001 | | 1270 | transit | | 1.061$^{+0.459}$ $_{−0.327}$ | 5129±138 | |
| K2-384b [ja] | 0.0040±0.0026 | 0.096$^{+0.020}$ $_{−0.005}$ | 2.23152$^{+0.0019}$ $_{−0.00032}$ | | 600 | transit | | 0.330±0.009 | 3623±138 | |
| K2-384c [ja] | 0.0054±0.0027 | 0.106$^{+0.004}$ $_{−0.006}$ | 4.19476$^{+0.00030}$ $_{−0.00018}$ | | 480 | transit | | 0.330±0.009 | 3623±138 | |
| K2-384d [ja] | 0.0085±0.0044 | 0.124$^{+0.010}$ $_{−0.006}$ | 6.67958$^{+0.00071}$ $_{−0.00049}$ | | 410 | transit | | 0.330±0.009 | 3623±138 | |
| K2-384e [ja] | 0.0075±0.0042 | 0.120$^{+0.012}$ $_{−0.007}$ | 9.71504$^{+0.00100}$ $_{−0.00073}$ | | 370 | transit | | 0.330±0.009 | 3623±138 | |
| K2-384f [ja] | 0.0179±0.0104 | 0.198$^{+0.008}$ $_{−0.007}$ | 13.62749$^{+0.00034}$ $_{−0.00057}$ | | 330 | transit | | 0.330±0.009 | 3623±138 | |
| K2-385 b | 0.0100±0.0056 | 0.137$^{+0.012}$ $_{−0.011}$ | 2.38086$^{+0.00016}$ $_{−0.00021}$ | | 1100 | transit | 1370±20 | 0.9270$^{+0.4120}$ $_{−0.2860}$ | 4844±138 | |
| K2-386 b | 0.0195±0.0115 | 0.207$^{+0.006}$ $_{−0.005}$ | 7.47322$^{+0.00037}$ $_{−0.00031}$ | | 1010 | transit | 1400±30 | 0.911$^{+0.088}$ $_{−0.083}$ | 5749±22 | |
| K2-387 b | 0.1430±0.0996 | 0.653±0.023 | 28.73532±0.00099 | | 340 | transit | 870±12 | 0.570$^{+0.051}$ $_{−0.048}$ | 3572±138 | |
| K2-388 b | 0.0412±0.0263 | 0.326$^{+0.029}$ $_{−0.020}$ | 6.33906$^{+0.00022}$ $_{−0.00018}$ | | 970 | transit | 948±13 | 0.8420$^{+0.3760}$ $_{−0.2590}$ | 5367±138 | |
| K2-389 b | 0.0177±0.0103 | 0.195±0.010 | 8.58404$^{+0.00088}$ $_{−0.00202}$ | | 1050 | transit | 846±9 | 0.8020$^{+0.3570}$ $_{−0.2460}$ | 5782±138 | |
| K2-389 c | 0.0165±0.0085 | 0.182$^{+0.013}$ $_{−0.012}$ | 20.85133$^{+0.00280}$ $_{−0.00298}$ | | 780 | transit | 846±9 | 0.8020$^{+0.3570}$ $_{−0.2460}$ | 5782±138 | |
| K2-390 b | 0.0636±0.0390 | 0.416$^{+0.027}$ $_{−0.030}$ | 3.31279±0.00010 | | 1310 | transit | 1490±18 | 0.7890$^{+0.3510}$ $_{−0.2390}$ | 5558±138 | |
| K2-391 b | 0.0078±0.0053 | 0.122$^{+0.025}$ $_{−0.016}$ | 4.62265$^{+0.00022}$ $_{−0.00025}$ | | 900 | transit | 1660±50 | 0.7570$^{+0.3410}$ $_{−0.2400}$ | 5543±138 | |
| K2-392 b | 0.0140±0.0079 | 0.165$^{+0.014}$ $_{−0.013}$ | 15.39872$^{+0.00242}$ $_{−0.00193}$ | | 840 | transit | 1330±30 | 0.8410$^{+0.3700}$ $_{−0.2580}$ | 5726±138 | |
| K2-393 b | 0.0199±0.0127 | 0.210$^{+0.015}$ $_{−0.014}$ | 10.41318$^{+0.00093}$ $_{−0.00069}$ | | 950 | transit | 867±9 | 0.8810$^{+0.3810}$ $_{−0.2690}$ | 5678±138 | |
| K2-394 b | 0.0123±0.0063 | 0.151$^{+0.012}$ $_{−0.011}$ | 5.09571±0.00011 | | 890 | transit | 319.7±1.5 | 0.478$^{+0.214}$ $_{−0.147}$ | 4938±138 | |
| K2-395 b | 0.0240±0.0141 | 0.231$^{+0.017}$ $_{−0.015}$ | 4.80335$^{+0.00035}$ $_{−0.00046}$ | | 910 | transit | 935±10 | 0.9520$^{+0.4210}$ $_{−0.2930}$ | 5007±138 | |
| K2-395 c | 0.0371±0.0220 | 0.303$^{+0.025}$ $_{−0.022}$ | 8.49128$^{+0.00033}$ $_{−0.00030}$ | | 750 | transit | 935±10 | 0.9520$^{+0.4210}$ $_{−0.2930}$ | 5007±138 | |
| K2-396 b | 0.0106±0.0061 | 0.140$^{+0.010}$ $_{−0.009}$ | 0.6736±0.00001 | | 1990 | transit | 897±9 | 0.9540$^{+0.4290}$ $_{−0.2930}$ | 5236±138 | |
| K2-396 c | 0.0314±0.0189 | 0.278$^{+0.015}$ $_{−0.010}$ | 25.76051$^{+0.00199}$ $_{−0.00188}$ | | 590 | transit | 897±9 | 0.9540$^{+0.4290}$ $_{−0.2930}$ | 5236±138 | |
| K2-397 b | 0.0212±0.0127 | 0.216±0.016 | 3.57232$^{+0.00018}$ $_{−0.00015}$ | | 1210 | transit | 650±5 | 0.9370$^{+0.4060}$ $_{−0.2850}$ | 5387±138 | |
| K2-398 b | 0.0191±0.0112 | 0.203$^{+0.010}$ $_{−0.009}$ | 6.39302$^{+0.00113}$ $_{−0.00075}$ | | 1240 | transit | 1980±40 | 0.9450$^{+0.0900}$ $_{−0.0830}$ | 5946±20 | |
| K2-398 c | 0.0736±0.0412 | 0.455±0.013 | 18.78783$^{+0.00087}$ $_{−0.00099}$ | | 870 | transit | 1980±40 | 0.9450$^{+0.0900}$ $_{−0.0830}$ | 5946±20 | |
| K2-400 b | 0.0051±0.0025 | 0.103±0.004 | 3.86505±0.00018 | | 570 | transit | 203.5±0.8 | 0.374±0.009 | 3578±138 | |
| K2-401 b | 0.0183±0.0117 | 0.201$^{+0.018}$ $_{−0.017}$ | 6.29309$^{+0.00057}$ $_{−0.00070}$ | | 660 | transit | 655±5 | 0.8700$^{+0.3950}$ $_{−0.2690}$ | 4213±138 | |
| K2-402 b | 0.0245±0.0149 | 0.239$^{+0.019}$ $_{−0.017}$ | 17.27474$^{+0.00259}$ $_{−0.00317}$ | | 870 | transit | 1710±60 | 0.9440$^{+0.4190}$ $_{−0.2900}$ | 5716±138 | |
| K2-403 b | 0.0783±0.0515 | 0.476$^{+0.031}$ $_{−0.034}$ | 33.58977±0.00076 | | 580 | transit | 804±8 | 0.7840$^{+0.3400}$ $_{−0.2410}$ | 5511±138 | |
| K2-404 b | 0.0230±0.0127 | 0.225±0.007 | 13.11536$^{+0.00044}$ $_{−0.00060}$ | | 450 | transit | 397±2 | 0.552±0.015 | 3748±138 | |
| K2-405 b | 0.0586±0.0342 | 0.407$^{+0.007}$ $_{−0.010}$ | 3.43547±0.00003 | | 980 | transit | 643±7 | 1.034$^{+0.459}$ $_{−0.314}$ | 4927±138 | |
| K2-406 b | 0.063±0.039 | 0.410$^{+0.027}$ $_{−0.026}$ | 22.5494$^{+0.00137}$ $_{−0.00143}$ | | 720 | transit | 278±2 | 0.7980$^{+0.3390}$ $_{−0.2450}$ | 5784±138 | |
| K2-407 b | 0.0066±0.0035 | 0.114$^{+0.008}$ $_{−0.007}$ | 4.9419$^{+0.00066}$ $_{−0.00069}$ | | 1110 | transit | | | | |
| K2-407 c | 0.0078±0.0044 | 0.121$^{+0.008}$ $_{−0.007}$ | 9.22453$^{+0.00132}$ $_{−0.00091}$ | | 900 | transit | | | | |
| K2-408 b | 0.0122±0.0062 | 0.149$^{+0.010}$ $_{−0.009}$ | 20.97895$^{+0.00130}$ $_{−0.00124}$ | | 610 | transit | | | | |
| K2-409 b | 0.0212±0.0127 | 0.221$^{+0.015}$ $_{−0.014}$ | 1.90808$^{+0.00004}$ $_{−0.00005}$ | | 1800 | transit | | | | |
| K2-2016-BLG-0005Lb | 1.1±0.1 | | | 4.4$^{+1.9}$ $_{−0.4}$ | 4700$^{+3300}$ $_{−700}$ | microlensing | 17000±700 | 0.58±0.03 | | |
| Kepler-451 c | 1.61±0.14 | | 1460±90 | 2.1±0.2 | | timing | 1340±20 | 0.48+0.12 | | |
| Kepler-451 d | 1.76±0.18 | | 43.0±0.1 | 0.20±0.03 | | timing | 1340±20 | 0.48+0.12 | | |
| Kepler-1656 c | 0.40±0.09 | | 1919$^{+27}$ $_{−24}$ | 3.053±0.049 | | radial vel. | | 1.03±0.04 | | |
| Kepler-1708b | <4.6 | 0.8886$^{+0.0535}$ $_{−0.0526}$ | 737.11310$^{+0.00146}$ $_{−0.00770}$ | 1.64±0.10 | | transit | 5436$^{+334}$ $_{−298}$ | 1.088±0.072 | 6157$^{+231}$ $_{−202}$ | Possible exomoon host |
| Kepler-1972b [ja] | 0.0064±0.0019 | 0.072±0.004 | 7.54425±0.00054 | | | transit | 923±3 | 1.12±0.03 | 5818±27 | Very dense planets, additional planet in system suspected |
| Kepler-1972c [ja] | 0.0066±0.0020 | 0.078±0.005 | 11.3295±0.0011 | | | transit | 923±3 | 1.12±0.03 | 5818±27 | Very dense planets, additional planet in system suspected |
| KMT-2016-BLG-1105b | 0.007$^{+0.023}$ $_{−0.005}$ | | | 2.44$^{+0.88}$ $_{−0.75}$ | | microlensing | 17000±7000 | 0.41$^{+0.25}$ $_{−0.21}$ | | |
| KMT-2017-BLG-0428b | 0.018$^{+0.011}$ $_{−0.009}$ | | | 1.81$^{+0.55}$ $_{−0.59}$ | | microlensing | 18000$^{+6000}$ $_{−8000}$ | 0.34$^{+0.22}$ $_{−0.17}$ | | |
| KMT-2017-BLG-0673Lb | 3.67$^{+2.17}$ $_{−2.07}$ | | | 2.34$^{+0.56}$ $_{−0.74}$ | | microlensing | 17000$^{+4000}$ $_{−5000}$ | 0.63$^{+0.37}$ $_{−0.35}$ | | |
| KMT-2017-BLG-1003b | 0.016$^{+0.017}$ $_{−0.009}$ | | | 1.38$^{+0.39}$ $_{−0.32}$ | | microlensing | 23000±2000 | 0.32$^{+0.31}$ $_{−0.17}$ | | |
| KMT-2017-BLG-1194b | 0.011±0.006 | | | 1.78$^{+0.45}$ $_{−0.46}$ | | microlensing | 14000±6000 | 0.41$^{+0.23}$ $_{−0.19}$ | | |
| KMT-2018-BLG-0030b | 1.45$^{+1.23}$ $_{−0.88}$ | | | 4.39$^{+2.18}$ $_{−2.40}$ | | microlensing | 21000$^{+4000}$ $_{−6000}$ | 0.51$^{+0.43}$ $_{−0.31}$ | | |
| KMT-2018-BLG-0087b | 0.23$^{+0.32}$ $_{−0.12}$ | | | 0.87$^{+0.24}$ $_{−0.25}$ | | microlensing | 23000$^{+3000}$ $_{−4000}$ | 0.10$^{+0.14}$ $_{−0.05}$ | | |
| KMT-2018-BLG-0247b | 2.11$^{+2.09}$ $_{−1.04}$ | | | 2.46$^{+0.51}$ $_{−0.58}$ | | microlensing | 22000$^{+3000}$ $_{−4000}$ | 0.29$^{+0.28}$ $_{−0.14}$ | | |
| KMT-2018-BLG-2004b | 0.27±\0.12 | | | 4.62$^{+0.80}$ $_{−1.10}$ | | microlensing | 23000$^{+3000}$ $_{−4000}$ | 0.69$^{+0.32}$ $_{−0.31}$ | | |
| KMT-2018-BLG-2602b | 1.15$^{+0.73}$ $_{−0.63}$ | | | 3.81$^{+2.96}$ $_{−2.32}$ | | microlensing | 14000±6000 | 0.66$^{+0.42}$ $_{−0.36}$ | | |
| KMT-2018-BLG-2718b | 16.0$^{+11.7}$ $_{−8.0}$ | | | 4.86$^{+2.97}$ $_{−2.55}$ | | microlensing | 15000$^{+10000}$ $_{−7000}$ | 0.82$^{+0.57}$ $_{−0.39}$ | | |
| KMT-2019-BLG-0414Lb | 4.57$^{+3.74}$ $_{−2.06}$ | | | 1.16$^{+0.47}$ $_{−0.51}$ | | microlensing | 14000$^{+5000}$ $_{−6000}$ | 0.74$^{+0.43}$ $_{−0.38}$ | | |
| KMT-2019-BLG-1042Lb | 0.19$^{+0.21}$ $_{−0.11}$ | | | 1.7±0.5 | | microlensing | 22000$^{+3000}$ $_{−5000}$ | 0.30$^{+0.34}$ $_{−0.18}$ | | |
| KMT-2019-BLG-1367b | 0.013$^{+0.008}$ $_{−0.007}$ | | | 1.70$^{+0.50}$ $_{−0.56}$ | | microlensing | 15000$^{+8000}$ $_{−7000}$ | 0.25$^{+0.16}$ $_{−0.13}$ | | |
| KMT-2019-BLG-1552Lb | 4.05$^{+1.73}$ $_{−1.85}$ | | | 2.6$^{+0.6}$ $_{−0.8}$ | | microlensing | 15000$^{+6000}$ $_{−5000}$ | 0.79$^{+0.33}$ $_{−0.36}$ | | |
| KMT-2019-BLG-1806b | 0.015±0.005 | | | 3.02$^{+0.70}$ $_{−0.73}$ | | microlensing | 22000$^{+2000}$ $_{−7000}$ | 0.74±0.25 | | |
| KMT-2019-BLG-2974Lb | 0.28$^{+0.29}$ $_{−0.18}$ | | | 2.0$^{+0.8}$ $_{−0.7}$ | | microlensing | 20000$^{+5000}$ $_{−7000}$ | 0.47$^{+0.41}$ $_{−0.28}$ | | |
| KMT-2021-BLG-0171Lb | 0.0352$^{+0.0173}$ $_{−0.0142}$ | | | 3.5$^{+1.3}$ $_{−1.0}$ | | microlensing | 15000$^{+5000}$ $_{−4000}$ | 0.78$^{+0.29}$ $_{−0.26}$ | | |
| KMT-2021-BLG-0240 b | 0.40$^{+0.07}$ $_{−0.08}$ | | | 2.5$^{+2.8}$ $_{−1.9}$ | | microlensing | 23000$^{+3000}$ $_{−5000}$ | 0.47$^{+0.33}$ $_{−0.24}$ | | Multiple solutions for orbital separation |
| KMT-2021-BLG-0240 c | 0.64$^{+0.25}$ $_{−0.24}$ | | | 1.0$^{+1.1}$ $_{−0.8}$ | | microlensing | 23000$^{+3000}$ $_{−5000}$ | 0.47$^{+0.33}$ $_{−0.24}$ | | Multiple solutions for orbital separation |
| KMT-2021-BLG-0320Lb | 0.10$^{+0.13}$ $_{−0.07}$ | | | 1.54$^{+0.24}$ $_{−0.30}$ | | microlensing | 23000$^{+3000}$ $_{−4000}$ | 0.32$^{+0.39}$ $_{−0.21}$ | | |
| KMT-2021-BLG-0748b | 0.45$^{+0.40}$ $_{−0.25}$ | | | 2.43±0.67 | | microlensing | 20000$^{+3000}$ $_{−4000}$ | 0.36$^{+0.32}$ $_{−0.20}$ | | |
| KMT-2021-BLG-0119Lb | 5.97$^{+2.94}$ $_{−2.60}$ | | | 3.23$^{+0.76}$ $_{−0.80}$ | | microlensing | 11000$^{+6000}$ $_{−4000}$ | 0.69$^{+0.34}$ $_{−0.30}$ | | Multiple orbital solutions |
| KMT-2021-BLG-0192Lb | 0.19$^{+0.09}$ $_{−0.10}$ | | | 2.07$^{+0.35}$ $_{−0.47}$ | | microlensing | 22000$^{+3000}$ $_{−5000}$ | 0.55$^{+0.26}$ $_{−0.28}$ | | Multiple orbital solutions |
| KMT-2021-BLG-0712b | 0.12$^{+0.06}$ $_{−0.04}$ | | | 2.22$^{+0.66}$ $_{−0.48}$ | | microlensing | 10000$^{+3000}$ $_{−2000}$ | 0.22$^{+0.12}$ $_{−0.07}$ | | |
| KMT-2021-BLG-0909b | 1.26$^{+1.01}$ $_{−0.66}$ | | | 1.75±0.42 | | microlensing | 21000$^{+3000}$ $_{−5000}$ | 0.38$^{+0.30}$ $_{−0.20}$ | | |
| KMT-2021-BLG-1077Lb | 0.22$^{+0.31}$ $_{−0.12}$ | | | 1.26$^{+1.41}$ $_{−1.08}$ | | microlensing | 27000±3000 | 0.14$^{+0.19}$ $_{−0.07}$ | | |
| KMT-2021-BLG-1077Lc | 0.25$^{+0.35}$ $_{−0.13}$ | | | 0.93$^{+1.05}$ $_{−0.80}$ | | microlensing | 27000±3000 | 0.14$^{+0.19}$ $_{−0.07}$ | | |
| KMT-2021-BLG-1105b | 1.30±0.68 | | | 3.54±1.06 | | microlensing | 15000±5000 | 0.63±0.33 | | |
| KMT-2021-BLG-1253b | 0.0599$^{+0.0643}$ $_{−0.0319}$ | | | 1.52$^{+0.57}$ $_{−0.41}$ | | microlensing | 22000$^{+3000}$ $_{−4000}$ | 0.24$^{+0.26}$ $_{−0.13}$ | | |
| KMT-2021-BLG-1303Lb | 0.38$^{+0.22}$ $_{−0.20}$ | | | 2.89$^{+0.44}$ $_{−0.66}$ | | microlensing | 20000$^{+3000}$ $_{−5000}$ | 0.57$^{+0.32}$ $_{−0.29}$ | | Host star also known as MOA-2021-BLG-182 |
| KMT-2021-BLG-1372b | 0.1928±0.1129 | | | 2.37±0.77 | | microlensing | 19000$^{+5000}$ $_{−8000}$ | 0.42±0.25 | | |
| KMT-2021-BLG-1391b | 0.0143±0.0073 | | | 2.29$^{+0.56}$ $_{−0.71}$ | | microlensing | 19000$^{+3000}$ $_{−5000}$ | 0.37±0.19 | | |
| KMT-2021-BLG-1554Lb | 0.12$^{+0.20}$ $_{−0.07}$ | | | 0.72$^{+0.13}$ $_{−0.14}$ | | microlensing | 25000$^{+3000}$ $_{−4000}$ | 0.08$^{+0.13}$ $_{−0.04}$ | | |
| KMT-2021-BLG-1689Lb | 0.145$^{+0.094}$ $_{−0.072}$ | | | 2.5$^{+0.8}$ $_{−06}$ | | microlensing | 23000$^{+2000}$ $_{−4000}$ | 0.58$^{+0.33}$ $_{−0.27}$ | | |
| KMT-2021-BLG-1898 b | 0.73$^{+0.50}$ $_{−0.40}$ | | | 1.9$^{+0.3}$ $_{−0.5}$ | | microlensing | 23000$^{+3000}$ $_{−4000}$ | 0.48$^{+0.33}$ $_{−0.26}$ | | Possibly a binary star system |
| KMT-2021-BLG-2294Lb | 0.07$^{+0.10}$ $_{−0.03}$ | | | 0.94±0.16 | | microlensing | 22000±3000 | 0.11$^{+0.17}$ $_{−0.06}$ | | Multiple orbital solutions |
| KMT-2021-BLG-2478b | 0.80$^{+0.56}$ $_{−0.35}$ | | | 1.38±0.26 | | microlensing | 8000$^{+4000}$ $_{−3000}$ | 0.12$^{+0.09}$ $_{−0.06}$ | | |
| L 363-38 b | 0.0147±0.0014 | | 8.781±0.007 | 0.048±0.006 | 330 | radial vel. | 33.31 | 0.21 | 3129 | Host star also known as Gliese 3049 |
| MOA-2019-BLG-008L b | 30 | | | | | microlensing | 8000±2000 | 0.8 | | |
| MOA-2020-BLG-135Lb | 0.036$^{+0.060}$ $_{−0.021}$ | | | 1.11$^{+0.23}$ $_{−0.20}$ | | microlensing | 26000±3000 | 0.23$^{+0.39}$ $_{−0.14}$ | | |
| MOA-2020-BLG-208Lb | 0.217$^{+0.116}$ $_{−0.106}$ | | | 2.88$^{+0.40}$ $_{−0.41}$ | | microlensing | 25000±3000 | 0.656$^{+0.346}$ $_{−0.322}$ | | |
| Mu2 Scorpii b | 14.4 | | | 290 | | imaging | 474 | 9.1 | 21900 | |
| Mu2 Scorpii c | 18.5 | | | 21 | | imaging | 474 | 9.1 | 21900 | |
| NGTS-20 b | 2.98$^{+0.16}$ $_{−0.15}$ | 1.07±0.04 | 54.18915±0.00015 | 0.313±0.013 | 688$^{+14}$ $_{−13}$ | transit | 1195±8 | 1.47±0.09 | 5980±80 | Planet on eccentric orbit, host star also known as TOI-5152 |
| NGTS-21b | 2.36±0.21 | 1.33±0.03 | 1.5433897±0.0000016 | 0.0236±0.0005 | 1357±15 | transit | 2090$^{+90}$ $_{−80}$ | 0.72±0.04 | 4660±41 | |
| NGTS-23b | 0.613±0.097 | 1.267±0.030 | 4.0764326±0.0000041 | 0.0504±0.012 | 1327$^{+17}$ $_{−16}$ | transit | 3230±70 | 1.01$^{+0.06}$ $_{−0.07}$ | 6057±64 | |
| NGTS-24b | 0.52$^{+0.12}$ $_{−0.11}$ | 1.214$^{+0.058}$ $_{−0.062}$ | 3.4678796±0.0000070 | 0.0479$^{+0.0028}$ $_{−0.0030}$ | 1499$^{+41}$ $_{−36}$ | transit | 2360±80 | 1.26$^{+0.05}$ $_{−0.21}$ | 5820$^{+93}$ $_{−8}$ | |
| NGTS-25b | 0.639$^{+0.058}$ $_{−0.052}$ | 1.023$^{+0.035}$ $_{−0.052}$ | 2.8230930±0.0000033 | 0.0388$^{+0.0014}$ $_{−0.002}$ | 1101$^{+15}$ $_{−14}$ | transit | 2350±30 | 0.91$^{+0.03}$ $_{−0.04}$ | 5321±58 | |
| OGLE-2016-BLG-1093Lb | 0.71±0.12 | | | 2.13±0.33 | | microlensing | 26000±2000 | 0.46±0.08 | | |
| OGLE-2017-BLG-1691Lb | 0.046$^{+0.037}$ $_{−0.025}$ | | | 2.41$^{+0.34}$ $_{−0.44}$ | | microlensing | 24000$^{+3000}$ $_{−4000}$ | 0.45$^{+0.36}$ $_{−0.25}$ | | Host star also known as KMT-2017-BLG-0752 |
| OGLE-2017-BLG-1806b | 0.017$^{+0.015}$ $_{−0.009}$ | | | 1.75$^{+0.46}$ $_{−0.47}$ | | microlensing | 21000$^{+3000}$ $_{−5000}$ | 0.38$^{+0.34}$ $_{−0.20}$ | | |
| OGLE-2018-BLG-0298Lb | 0.14$^{+0.07}$ $_{−0.06}$ | | | 2.86$^{+0.73}$ $_{−0.80}$ | | microlensing | 21000$^{+3000}$ $_{−4000}$ | 0.69$^{+0.34}$ $_{−0.30}$ | | |
| OGLE-2018-BLG-0932b | 0.89$^{+0.36}$ $_{−0.31}$ | | | 1.75$^{+0.24}$ $_{−0.23}$ | | microlensing | 22000±3000 | 0.72$^{+0.29}$ $_{−0.25}$ | | |
| OGLE-2018-BLG-1119Lb | 0.91$^{+0.66}$ $_{−0.52}$ | | | 4.06$^{+2.14}$ $_{−2.58}$ | | microlensing | 19000$^{+5000}$ $_{−8000}$ | 0.48$^{+0.35}$ $_{−0.28}$ | | |
| OGLE-2018-BLG-1126b | 0.056$^{+0.033}$ $_{−0.031}$ | | | 3.23$^{+1.29}$ $_{−1.71}$ | | microlensing | 19000$^{+6000}$ $_{−8000}$ | 0.69$^{+0.41}$ $_{−0.38}$ | | |
| OGLE-2018-BLG-1212b | 0.20$^{+0.16}$ $_{−0.13}$ | | | 1.68$^{+1.47}$ $_{−0.63}$ | | microlensing | 5100$^{+4100}$ $_{−1800}$ | 0.16$^{+0.12}$ $_{−0.10}$ | | |
| OGLE-2018-BLG-1367b | 0.95$^{+0.75}$ $_{−0.44}$ | | | 3.63$^{+1.02}$ $_{−0.96}$ | | microlensing | | 0.28$^{+0.22}$ $_{−0.13}$ | | Multiple solutions for frojected separation |
| OGLE-2018-BLG-1544b | 11.2$^{+6.3}$ $_{−5.9}$ | | | 6.21$^{+1.32}$ $_{−2.10}$ | | microlensing | 21000$^{+4000}$ $_{−7000}$ | 0.62$^{+0.38}$ $_{−0.36}$ | | Multiple solutions for frojected separation |
| OGLE-2018-BLG-1647b | 0.97$^{+1.78}$ $_{−0.56}$ | | | 1.36$^{+0.20}$ $_{−0.17}$ | | microlensing | 26000$^{+4000}$ $_{−3000}$ | 0.092$^{+0.170}$ $_{−0.053}$ | | |
| OGLE-2019-BLG-0362Lb | 3.26$^{+0.83}$ $_{−0.58}$ | | | 2.18$^{+0.58}$ $_{−0.72}$ | | microlensing | 19000±2000 | 0.42$^{+0.34}$ $_{−0.23}$ | | Multiple solutions for planetary parameters |
| OGLE-2019-BLG-1470LABc | 2.2$^{+1.8}$ $_{−1.3}$ | | | 3.1$^{+1.2}$ $_{−1.1}$ | | microlensing | 20000±4000 | 0.55+0.17 | | Circumbinary planet |
| Pi Mensae d | 0.0421±0.0042 | | 124.64$^{+0.48}$ $_{−0.52}$ | | | radial vel. | 59.62±0.07 | 1.11±0.01 | 6013±18 | |
| Proxima Centauri d | 0.0008±0.0002 | | 5.122$^{+0.002}$ $_{−0.0036}$ | 0.02885$^{+0.00019}$ $_{−0.00022}$ | 360 | radial vel. | 4.2465±0.0003 | 0.1221±0.0022 | 2900±100 | |
| PSR J2007+3120 b | 0.0072±0.0009 | | 723±8 | | | timing | 22000 | | | Pulsar planet, another planet in the system is suspected. |
| Ross 508 b | 0.0126±0.0019 | | 10.76$^{+0.01}$ $_{−0.02}$ | 0.05353$^{+0.00047}$ $_{−0.00051}$ | | radial vel. | 36.594±0.011 | 0.1774±0.0045 | 3071$^{+34}$ $_{−22}$ | Host star also known as Gliese 585, planet close to habitable zone. |
| TOI-181b | 0.127891$^{+0.013510}$ $_{−0.025081}$ | 0.631521$^{+0.007554}$ $_{−0.009811}$ | 4.532058$^{+0.000002}$ $_{−0.000002}$ | 0.055780$^{+0.005563}$ $_{−0.003893}$ | 878$^{+32}$ $_{−41}$ | transit | 314±2 | 0.781±0.042 | 4994±50 | |
| TOI-206 b | | 0.116±0.004 | 0.7363104±0.0000003 | 0.0112±0.0001 | 910±36 | transit | 155.9 | 0.35±0.01 | 3383±157 | |
| TOI-277 b | 0.0239$^{+0.0179}$ $_{−0.0098}$ | 0.237±0.016 | 3.9940±0.0004 | 0.0269±0.0011 | | transit | 212.6$^{+0.6}$ $_{−0.3}$ | 0.16±0.01 | 4031$^{+21}$ $_{−23}$ | |
| TOI-500 b | | 0.104±0.010 | 0.5481579±0.0000006 | 0.0128±0.0011 | 1693±105 | transit | 154.8 | 0.88±0.25 | 4621±50 | |
| TOI-544 b | | 0.181±0.009 | 1.5483510±0.0000015 | 0.0251 ± 0.0019 | 1082±47 | transit | 132.7 | 0.85±0.20 | 4369±100 | |
| TOI-620 b | | | 5.0988179$^{+0.0000045}$ $_{−0.0000046}$ | 0.04825$^{+0.00065}$ $_{−0.00066}$ | 603.6$^{+5.5}$ $_{−5.3}$ | transit | 107.81±0.19 | 0.577$^{+0.024}$ $_{−0.023}$ | 3708$^{+57}$ $_{−56}$ | |
| TOI-778 b | 2.76±0.24 | 1.375±0.045 | 4.633611±0.000001 | 0.060±0.003 | 1561$^{+33}$ $_{−32}$ | transit | 530±4 | 1.428±0.094 | 6715±128 | |
| TOI-833 b | | 0.113±0.006 | 1.0418777±0.0000324 | 0.0171±0.0003 | 1118±49 | transit | 136.3 | 0.61±0.03 | 3920±160 | |
| TOI-969 b | 0.0286±0.0031 | 0.247±0.033 | 1.8237305$^{+0.0000020}$ $_{−0.0000021}$ | 0.02636±0.00017 | 941±31 | transit | 253.8±0.5 | 0.730±0.037 | 4550±75 | |
| TOI-969 c | 11.3$^{+1.1}$ $_{−0.9}$ | | 1700$^{+290}$ $_{−280}$ | 2.52$^{+0.27}$ $_{−0.29}$ | 96.4$^{+6.8}$ $_{−5.8}$ | radial vel. | 253.8±0.5 | 0.730±0.037 | 4550±75 | Eccentric orbit |
| TOI-1064b | 0.0425±0.0055 | 0.231±0.004 | 6.443868±0.000025 | 0.06152$^{+0.00086}$ $_{−0.00089}$ | 784±13 | transit | 224.5±0.2 | 0.748±0.032 | 4734±67 | |
| TOI-1064c | 0.0079$^{+0.0057}$ $_{−0.0063}$ | 0.237±0.004 | 12.226574$^{+0.000046}$ $_{−0.000043}$ | 0.09429$^{+0.00132}$ $_{−0.00136}$ | 634±10 | transit | 224.5±0.2 | 0.748±0.032 | 4734±67 | |
| TOI-1075 b | | 0.154±0.007 | 0.6047328±0.0000032 | 0.0118±0.0001 | 1336±56 | transit | 200.9 | 0.60±0.02 | 3921±157 | |
| TOI-1075 b | 0.0313±0.0042 | 0.160$^{+0.010}$ $_{−0.007}$ | 0.6047328±0.0000032 | 0.01159$^{+0.00023}$ $_{−0.00020}$ | 1323±44 | transit | 200.4$^{+0.6}$ $_{−2.2}$ | 0.604±0.030 | 3875±75 | |
| TOI-1107b | 3.35±0.18 | 1.30±0.05 | 4.0782387$^{+0.0000024}$ $_{−0.0000025}$ | 0.0561$^{+0.0024}$ $_{−0.0025}$ | 1728±27 | transit | 925±7 | 1.35±0.08 | 6311±98 | |
| TOI-1136 b | 0.0095$^{+0.0022}$ $_{−0.0028}$ | 0.170$^{+0.019}$ $_{−0.013}$ | 4.1728±0.0002 | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1136 c | 0.0189$^{+0.0041}$ $_{−0.0053}$ | 0.257±0.005 | 6.2573±0.0002 | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1136 d | 0.0252$^{+0.0076}$ $_{−0.0060}$ | 0.413±0.007 | 12.5194±0.0004 | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1136 e | 0.0170±0.0031 | 0.236$^{+0.006}$ $_{−0.008}$ | 18.7992$^{+0.0017}$ $_{−0.0015}$ | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1136 f | 0.0261$^{+0.0088}$ $_{−0.0113}$ | 0.346±0.010 | 26.3162$^{+0.0017}$ $_{−0.0013}$ | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1136 g | 0.0151$^{+0.0148}$ $_{−0.0104}$ | 0.226±0.010 | 39.5387$^{+0.0036}$ $_{−0.0030}$ | | | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | |
| TOI-1181 b | 1.18±0.14 | 1.30±0.08 | 2.103195$^{+0.000012}$ $_{−0.000011}$ | | 2162 | transit | 1013±3 | 1.38$^{+0.086}$ $_{−0.082}$ | 6260±100 | Subgiant host star |
| TOI-1221 b | | 0.259±0.011 | 91.68278$^{+0.00032}$ $_{−0.00041}$ | 0.404$^{+0.026}$ $_{−0.023}$ | 400 | transit | 447.1±0.7 | 1.03±0.06 | 5592±50 | |
| TOI-1246 b [ja] | 0.0255±0.0035 | 0.269±0.005 | 4.30744±0.00002 | 0.049±0.002 | 955 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | |
| TOI-1246 c [ja] | 0.0277±0.0038 | 0.224±0.007 | 5.904144±0.000083 | 0.061±0.002 | 860 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | |
| TOI-1246 d [ja] | 0.0167±0.0053 | 0.313±0.008 | 18.65590±0.00048 | 0.131±0.004 | 586 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | |
| TOI-1246 e [ja] | 0.0466±0.0072 | 0.338±0.014 | 37.9216±0.0010 | 0.211±0.007 | 462 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | |
| TOI-1260 d | 0.0373±0.0245 | 0.276±0.008 | 16.608164±0.000083 | 0.1116±0.0033 | 499±4 | transit | 239.5±0.3 | 0.66±0.01 | 4227±85 | |
| TOI-1268 b | 0.303±0.026 | 0.81±0.05 | 8.1577080±0.0000044 | 0.072$^{+0.009}$ $_{−0.010}$ | 919 | transit | 359.1±0.4 | 0.92±0.03 | 5290±117 | |
| TOI-1272 b | 0.0774±0.0072 | 0.370±0.019 | 3.31599±0.00002 | 0.0412±0.0008 | 961±32 | transit | 450.6±1.3 | 0.851±0.049 | 4985±121 | |
| TOI-1272 c | 0.0840±0.0098 | | 8.689±0.008 | 0.0783±0.0014 | 697±23 | radial vel. | 450.6±1.3 | 0.851±0.049 | 4985±121 | |
| TOI-1288 b | 0.0712$^{+0.0574}$ $_{−0.0304}$ | 0.454±0.010 | 2.69998±0.00015 | 0.0429±0.0006 | | transit | 375.3$^{+1.3}$ $_{−0.5}$ | 1.46±0.06 | 5307$^{+18}$ $_{−16}$ | |
| TOI-1288 c | 0.2643±0.0220 | | 443$^{+11}$ $_{−13}$ | | | radial vel. | 375.3$^{+1.3}$ $_{−0.5}$ | 1.46±0.06 | 5307$^{+18}$ $_{−16}$ | |
| TOI-1411 b | | 0.121±0.013 | 1.4520358±0.0000098 | 0.0230±0.0026 | 1136±59 | transit | 106.0 | 0.59±0.23 | 4266±100 | |
| TOI-1422 b | 0.0283$^{+0.0072}$ $_{−0.0063}$ | 0.354$^{+0.012}$ $_{−0.010}$ | 12.9972±0.0006 | 0.108±0.003 | 867±17 | transit | 504.17$^{+0.12}$ $_{−0.09}$ | 0.981$^{+0.062}$ $_{−0.065}$ | 5840±62 | Another planet in the system is suspected. |
| TOI-1442 b | | 0.104±0.005 | 0.4090677±0.0000003 | 0.0071±0.0002 | 1072±54 | transit | 134.5 | 0.29±0.02 | 3330±160 | |
| TOI-1452 b | 0.0152±0.0041 | 0.149±0.006 | 11.06201±0.00002 | 0.061±0.003 | 326±7 | transit | 99.51±0.04 | 0.249±0.008 | 3185±50 | Also a red dwarf on a 97AU separation in the system |
| TOI-1468 b | 0.0101±0.0008 | 0.114±0.003 | 1.8805136$^{+0.0000024}$ $_{−0.0000026}$ | | 682.2$^{+7.4}$ $_{−6.9}$ | transit | 80.64±0.07 | 0.339±0.011 | 3496±25 | |
| TOI-1468 c | 0.0209±0.0021 | 0.184±0.004 | 15.532482$^{+0.000034}$ $_{−0.000033}$ | | 337.5$^{+3.7}$ $_{−3.4}$ | transit | 80.64±0.07 | 0.339±0.011 | 3496±25 | |
| TOI-1516 b | 3.16±0.12 | 1.36±0.03 | 2.056014±0.000002 | | 1820 | transit | 804.6±1.9 | 1.085$^{+0.061}$ $_{−0.066}$ | 6420±100 | |
| TOI-1669 b | 0.0132±0.0085 | 0.214±0.016 | 2.7 | | | transit | 364.6 | 1.00±0.05 | 5542.3±100.0 | Host star also known as BD+82 71, planet suspected since 2020 |
| TOI-1669 c | 0.602±0.078 | | 501±16 | | | radial vel. | 364.6 | 1.00±0.05 | 5542.3±100.0 | Host star also known as BD+82 71, additional long-period companion is suspected. |
| TOI-1694 b | 0.0979±0.0066 | 0.461±0.016 | 3.8 | | | transit | 405.7 | 0.84±0.03 | 5066±100 | Host star also known as TYC 4108-1434-1, planet suspected since 2020 |
| TOI-1694 c | 0.929±0.037 | | 393.2±4.3 | | | radial vel. | 405.7 | 0.84±0.03 | 5066±100 | Host star also known as TYC 4108-1434-1 |
| TOI-1670 b | 0.04±0.03 | 0.184$^{+0.017}$ $_{−0.013}$ | 10.98462$^{+0.00046}$ $_{−0.00051}$ | 0.103±0.002 | 1062$^{+14}$ $_{−13}$ | transit | 540.6$^{+1.0}$ $_{−1.2}$ | 1.21±0.02 | 6170±61 | |
| TOI-1670 c | 0.63$^{+0.09}$ $_{−0.08}$ | 0.987±0.025 | 40.74976$^{+0.000022}$ $_{−0.00021}$ | 0.249±0.005 | 684±9 | transit | 540.6$^{+1.0}$ $_{−1.2}$ | 1.21±0.02 | 6170±61 | |
| TOI-1693 b | | 0.126±0.009 | 1.7666957±0.0000054 | 0.0226±0.0004 | 764±19 | transit | 100.6 | 0.49±0.03 | 3499±70 | |
| TOI-1695 b | 0.0173±0.0031 | 0.181±0.016 | 3.1342790±0.0000072 | 0.033548$^{+0.000260}$ $_{−0.000268}$ | 590±90 | transit | 147.2±0.2 | 0.51±0.02 | 3627±31 | |
| TOI-1696 b | 0.1781 | 0.276±0.010 | 2.500311±0.000004 | 0.0229±0.0002 | 489±13 | transit | 210.8±0.5 | 0.255±0.0066 | 3185±76 | |
| TOI-1710 b | 0.0890±0.0148 | 0.477±0.010 | 24.283429±0.00043 | 0.16±0.04 | 687±50 | transit | 264.7±0.2 | 0.984$^{+0.050}$ $_{−0.059}$ | 5665±55 | |
| TOI-1759 b | 0.021±0.06 | 0.279±0.02 | 18.849975±0.000006 | 0.1176±0.0013 | 433±14 | transit | 130.85±0.05 | 0.606±0.020 | 4065±51 | |
| TOI-1811 b | 0.974$^{+0.075}$ $_{−0.076}$ | 1.002$^{+0.026}$ $_{−0.024}$ | 3.7130818±0.0000028 | 0.04393$^{+0.00058}$ $_{−0.00054}$ | 961.5±8 | transit | 418±3 | 0.819$^{+0.033}$ $_{−0.030}$ | 4753$^{+54}$ $_{−55}$ | |
| TOI-1820 b | 2.3±0.2 | 1.12±0.02 | 4.860700±0.000010 | 0.069±0.005 | 1295±11 | transit | 807±13 | 1.04±0.13 | 5734±50 | |
| TOI-1860 b | | 0.117±0.005 | 1.0662107±0.0000014 | 0.0204±0.0002 | 1885±28 | transit | 149.8 | 0.99±0.03 | 5752±100 | |
| TOI-1937 b | 2.01$^{+0.17}$ $_{−0.16}$ | 1.247$^{+0.059}$ $_{−0.062}$ | 0.94667944±0.00000047 | 0.01932$^{+0.00035}$ $_{−0.00039}$ | 2097$^{+35}$ $_{−36}$ | transit | 1366±6 | 1.072$^{+0.059}$ $_{−0.064}$ | 5814$^{+91}$ $_{−93}$ | |
| TOI-2000 b | 0.0324±0.0070 | 0.236±0.010 | 3.098331$^{+0.000021}$ $_{−0.000019}$ | 0.04260$^{+0.00076}$ $_{−0.00067}$ | 1475$^{+120}$ $_{−158}$ | transit | 566.3±1.0 | 1.074$^{+0.059}$ $_{−0.050}$ | 5607$^{+86}$ $_{−82}$ | |
| TOI-2000 c | 0.238±0.012 | 0.711±0.011 | 9.1270553±0.0000073 | 0.0875$^{+0.0016}$ $_{−0.0014}$ | 1029$^{+84}$ $_{−111}$ | transit | 566.3±1.0 | 1.074$^{+0.059}$ $_{−0.050}$ | 5607$^{+86}$ $_{−82}$ | |
| TOI-2025 b | 4.4±0.4 | 1.120±0.009 | 8.872086±0.000009 | 0.089±0.004 | 1186±11 | transit | 1106±7 | 1.32±0.14 | 5880±53 | |
| TOI-2025 b | 3.51$^{+0.36}$ $_{−0.35}$ | 1.118$^{+0.031}$ $_{−0.030}$ | 8.8720942$^{+0.0000080}$ $_{−0.0000079}$ | 0.0886$^{+0.0019}$ $_{−0.0024}$ | 1172$^{+18}$ $_{−17}$ | transit | 1095±11 | 1.176$^{+0.079}$ $_{−0.091}$ | 5928$^{+76}$ $_{−75}$ | |
| TOI-2046 b | 2.30±0.08 | 1.44±0.11 | 1.4971842$^{+0.0000031}$ $_{−0.0000033}$ | | 1998 | transit | 940±3 | 1.153$^{+0.100}$ $_{−0.093}$ | 6160±100 | Young host star |
| TOI-2048 b | | 0.184±0.018 | 13.79019$^{+0.00065}$ $_{−0.00084}$ | | 640±20 | transit | 379.7±0.5 | 0.83±0.03 | 5185±60 | Young host star belongs to NGC 3532 |
| TOI-2081 b | 0.0157$^{+0.0151}$ $_{−0.0076}$ | 0.182±0.046 | 10.50534$^{+0.00007}$ $_{−0.00008}$ | 0.0752$^{+0.0047}$ $_{−0.0119}$ | 488$^{+28}$ $_{−52}$ | transit | 203.26±0.16 | 0.540±0.080 | 3800±100 | |
| TOI-2136 b | 0.0200$^{+0.0077}$ $_{−0.0072}$ | 0.196±0.015 | 7.851928$^{+0.000018}$ $_{−0.000016}$ | 0.057±0.006 | 395$^{+24}$ $_{−22}$ | transit | 108.82±0.07 | 0.34±0.02 | 3342±100 | |
| TOI-2145 b | 5.35$^{+0.32}$ $_{−0.35}$ | 1.103$^{+0.031}$ $_{−0.029}$ | 10.261081$^{+0.000026}$ $_{−0.000027}$ | 0.1108$^{+0.0012}$ $_{−0.0015}$ | 1484$^{+16}$ $_{−14}$ | transit | 733±5 | 1.720$^{+0.057}$ $_{−0.068}$ | 6189±67 | Host star also known as HIP 86040 |
| TOI-2152A b | 2.83$^{+0.38}$ $_{−0.37}$ | 1.281$^{+0.050}$ $_{−0.046}$ | 3.3773512$^{+0.0000060}$ $_{−0.0000061}$ | 0.05064$^{+0.00093}$ $_{−0.0011}$ | 1802$^{+60}$ $_{−54}$ | transit | 988±13 | 1.516$^{+0.085}$ $_{−0.10}$ | 6630$^{+300}$ $_{−290}$ | Planet orbiting primary of binary star |
| TOI-2154 b | 0.92$^{+0.19}$ $_{−0.18}$ | 1.453$^{+0.053}$ $_{−0.048}$ | 3.8240801±0.0000025 | 0.0513$^{+0.0011}$ $_{−0.0013}$ | 1580±27 | transit | 967±10 | 1.233$^{+0.077}$ $_{−0.090}$ | 6280±160 | |
| TOI-2180 b | 2.755$^{+0.087}$ $_{−0.081}$ | 1.010$^{+0.022}$ $_{−0.019}$ | 260.79$^{+0.59}$ $_{−0.58}$ | 0.828±0.012 | 348.0$^{+3.3}$ $_{−3.6}$ | transit | 379.4±0.8 | 1.111$^{+0.047}$ $_{−0.046}$ | 5695$^{+58}$ $_{−60}$ | |
| TOI-2158 b | 0.82±0.08 | 0.960±0.012 | 8.60077±0.00003 | 0.075±0.004 | 1188±10 | transit | 652±3 | 1.12±0.12 | 5673±50 | |
| TOI-2193 b | 0.94±0.18 | 1.77 | 2.1225735±0.0000016 | 0.03319$^{+0.00052}$ $_{−0.00051}$ | 1763$^{+21}$ $_{−22}$ | transit | 1126±3 | 1.082$^{+0.052}$ $_{−0.049}$ | 5974±110 | Also 0.54M$_☉$ star in the system |
| TOI-2196 b | 0.0818±0.0041 | 0.313±0.013 | 1.1947268$^{+0.0000079}$ $_{−0.0000093}$ | 0.02234±0.00060 | 1860±20 | transit | 861±3 | 1.032±0.038 | 5634±31 | Neptunian desert planet |
| TOI-2207 b | 0.64$^{+0.10}$ $_{−0.12}$ | 0.995$^{+0.028}$ $_{−0.027}$ | 8.001968$^{+0.000024}$ $_{−0.000025}$ | 0.0854$^{+0.0015}$ $_{−0.0016}$ | 1259$^{+16}$ $_{−15}$ | transit | 1242±9 | 1.296$^{+0.069}$ $_{−0.072}$ | 6075±110 | |
| TOI-2260 b | | 0.145±0.012 | 0.3524728±0.0000047 | 0.0097±0.0001 | 2609±86 | transit | 331.2 | 0.99±0.04 | 5534±100 | |
| TOI-2236 b | 1.58$^{+0.40}$ $_{−0.39}$ | 1.282$^{+0.032}$ $_{−0.031}$ | 3.5315902±0.0000026 | 0.05009$^{+0.00080}$ $_{−0.00082}$ | 1688$^{+19}$ $_{−21}$ | transit | 1149±5 | 1.343$^{+0.066}$ $_{−0.065}$ | 6164±50 | |
| TOI-2337b | 1.60±0.15 | 0.9±0.1 | 2.99432±0.00008 | 0.04467 | | transit | 1780±20 | 1.325±0.118 | 4780±100 | |
| TOI-2364 b | 0.225$^{+0.043}$ $_{−0.049}$ | 0.768$^{+0.023}$ $_{−0.018}$ | 4.0197517±0.0000043 | 0.04871$^{+0.00069}$ $_{−0.00079}$ | 1091$^{+17}$ $_{−14}$ | transit | 713±6 | 0.954$^{+0.041}$ $_{−0.046}$ | 5306$^{+76}$ $_{−68}$ | |
| TOI-2411 b | | 0.150±0.010 | 0.7826942±0.0000037 | 0.0144±0.0001 | 1355±45 | transit | 194.5 | 0.65±0.02 | 4099±123 | |
| TOI-2421 b | 0.333±0.079 | 0.925$^{+0.035}$ $_{−0.034}$ | 4.3474032$^{+0.0000079}$ $_{−0.0000078}$ | 0.0543$^{+0.0021}$ $_{−0.0010}$ | 1534$^{+20}$ $_{−28}$ | transit | 1067±7 | 1.131$^{+0.130}$ $_{−0.064}$ | 5577±50 | |
| TOI-2427 b | | 0.161±0.011 | 1.3060011±0.0000102 | 0.0202±0.0002 | 1117±46 | transit | 93.1 | 0.64±0.02 | 4072±121 | |
| TOI-2445 b | | 0.112±0.007 | 0.3711281±0.0000005 | 0.0064±0.0001 | 1060±54 | transit | 158.7 | 0.25±0.01 | 3333±157 | |
| TOI-2497 b | 5.21±0.52 | 1.000$^{+0.040}$ $_{−0.038}$ | 10.655661±0.000026 | 0.1167$^{+0.0018}$ $_{−0.0017}$ | 1596$^{+44}$ $_{−41}$ | transit | 930±14 | 1.861$^{+0.086}$ $_{−0.081}$ | 7360$^{+290}$ $_{−270}$ | |
| TOI-2567 b | 0.201$^{+0.034}$ $_{−0.031}$ | 0.975$^{+0.031}$ $_{−0.029}$ | 5.983944±0.000013 | 0.0672$^{+0.0024}$ $_{−0.0012}$ | 1352$^{+18}$ $_{−19}$ | transit | 1691±8 | 1.130$^{+0.130}$ $_{−0.059}$ | 5650±50 | |
| TOI-2570 b | 0.820$^{+0.063}$ $_{−0.065}$ | 1.217$^{+0.035}$ $_{−0.034}$ | 2.9887615±0.0000022 | 0.04145$^{+0.00081}$ $_{−0.00086}$ | 1431$^{+24}$ $_{−23}$ | transit | 1179±6 | 1.063$^{+0.063}$ $_{−0.065}$ | 5765±50 | |
| TOI-2583 b | 0.250$^{+0.058}$ $_{−0.056}$ | 1.290$^{+0.040}$ $_{−0.033}$ | 4.5207265±0.0000049 | 0.0571$^{+0.0010}$ $_{−0.0013}$ | 1456$^{+19}$ $_{−16}$ | transit | 1831±9 | 1.215$^{+0.063}$ $_{−0.082}$ | 5936$^{+65}$ $_{−68}$ | |
| TOI-2587 b | 0.218$^{+0.054}$ $_{−0.046}$ | 1.077$^{+0.042}$ $_{−0.040}$ | 5.456640±0.000011 | 0.0635$^{+0.0025}$ $_{−0.0013}$ | 1445$^{+23}$ $_{−26}$ | transit | 1242±10 | 1.15$^{+0.14}$ $_{−0.07}$ | 5760$^{+80}$ $_{−79}$ | |
| TOI-2669b | 0.61±0.19 | 1.76±0.16 | 6.2034±0.0001 | | | transit | 1294±9 | 1.19±0.16 | 4800±100 | |
| TOI-2796 b | 0.44$^{+0.10}$ $_{−0.11}$ | 1.59 | 4.8084983$^{+0.0000057}$ $_{−0.0000056}$ | 0.0569$^{+0.0010}$ $_{−0.0011}$ | 1205$^{+18}$ $_{−17}$ | transit | 1150±6 | 1.063$^{+0.057}$ $_{−0.062}$ | 5764$^{+81}$ $_{−78}$ | |
| TOI-2803 b | 0.975$^{+0.083}$ $_{−0.070}$ | 1.616$^{+0.034}$ $_{−0.032}$ | 1.96229325±0.00000082 | 0.03185±0.00052 | 1893$^{+29}$ $_{−28}$ | transit | 1635±9 | 1.118$^{+0.056}$ $_{−0.054}$ | 6280$^{+99}$ $_{−96}$ | |
| TOI-2818 b | 0.71±0.26 | 1.363$^{+0.046}$ $_{−0.045}$ | 4.0397090$^{+0.0000024}$ $_{−0.0000023}$ | 0.0493$^{+0.0010}$ $_{−0.0008}$ | 1376$^{+26}$ $_{−24}$ | transit | 1028±3 | 0.977$^{+0.063}$ $_{−0.049}$ | 5721$^{+88}$ $_{−83}$ | |
| TOI-2842 b | 0.370$^{+0.052}$ $_{−0.047}$ | 1.146$^{+0.051}$ $_{−0.048}$ | 3.5514058$^{+0.0000077}$ $_{−0.0000078}$ | 0.0475$^{+0.0010}$ $_{−0.0011}$ | 1471$^{+29}$ $_{−27}$ | transit | 1501±8 | 1.135$^{+0.077}$ $_{−0.079}$ | 5910±100 | |
| TOI-2977 b | 1.68$^{+0.26}$ $_{−0.25}$ | 1.174$^{+0.031}$ $_{−0.027}$ | 2.3505614±0.0000025 | 0.03386$^{+0.00067}$ $_{−0.00050}$ | 1544±26 | transit | 1160±30 | 0.936$^{+0.057}$ $_{−0.041}$ | 5691$^{+94}$ $_{−93}$ | |
| TOI-3023 b | 0.62$^{+0.10}$ $_{−0.09}$ | 1.466$^{+0.043}$ $_{−0.032}$ | 3.9014971±0.0000031 | 0.0505$^{+0.0015}$ $_{−0.0009}$ | 1596$^{+24}$ $_{−25}$ | transit | 1281±5 | 1.12$^{+0.11}$ $_{−0.06}$ | 5760$^{+85}$ $_{−88}$ | |
| TOI-3331 b | 2.27±0.16 | 1.158±0.043 | 2.0180231$^{+0.0000043}$ $_{−0.0000044}$ | 0.03144$^{+0.00048}$ $_{−0.00055}$ | 1488$^{+31}$ $_{−29}$ | transit | 733±4 | 1.016$^{+0.047}$ $_{−0.052}$ | 5521±110 | Also 0.6M$_☉$ star in the system |
| TOI-3364 b | 1.67$^{+0.12}$ $_{−0.13}$ | 1.091$^{+0.038}$ $_{−0.032}$ | 5.8768918±0.0000069 | 0.0675$^{+0.0011}$ $_{−0.0016}$ | 1264$^{+22}$ $_{−21}$ | transit | 899±3 | 1.186$^{+0.059}$ $_{−0.083}$ | 5706$^{+95}$ $_{−91}$ | |
| TOI-3540 b | 1.18±0.14 | 2.10 | 3.1199990±0.0000079 | 0.04289$^{+0.00092}$ $_{−0.00093}$ | 1498±22 | transit | 921±10 | 1.081$^{+0.071}$ $_{−0.069}$ | 5969±50 | Also 0.8M$_☉$ star in the system |
| TOI-3629 b | 0.26±0.02 | 0.74±0.02 | 3.936551$^{+0.000005}$ $_{−0.000006}$ | 0.043±0.002 | 690±20 | transit | 423.1±1.0 | 0.63±0.02 | 3870±90 | |
| TOI-3688 b | 0.98$^{+0.10}$ $_{−0.11}$ | 1.167$^{+0.048}$ $_{−0.044}$ | 3.246075±0.000012 | 0.04560$^{+0.00089}$ $_{−0.00098}$ | 1534$^{+29}$ $_{−28}$ | transit | 1308±6 | 1.199$^{+0.072}$ $_{−0.076}$ | 5950±100 | |
| TOI-3693 b | 1.02$^{+0.24}$ $_{−0.22}$ | 1.124$^{+0.029}$ $_{−0.023}$ | 9.088516$^{+0.000026}$ $_{−0.000027}$ | 0.0813$^{+0.0011}$ $_{−0.0012}$ | 801$^{+13}$ $_{−12}$ | transit | 576±2 | 0.867$^{+0.036}$ $_{−0.037}$ | 5274±50 | |
| TOI-3714 b | 0.70±0.003 | 1.01±0.03 | 2.154849±0.000001 | 0.027±0.001 | 750±20 | transit | 367.0$^{+0.6}$ $_{−1.3}$ | 0.53±0.02 | 3660±90 | |
| TOI-3757 b | 0.2684±0.0276 | 1.07$^{+0.04}$ $_{−0.05}$ | 3.4387530$^{+0.0000039}$ $_{−0.0000040}$ | 0.03845±0.00043 | 759±13 | transit | 579±2 | 0.64±0.02 | 3913±56 | |
| TOI-3807 b | 1.04$^{+0.15}$ $_{−0.14}$ | 2.00 | 2.8989727$^{+0.0000038}$ $_{−0.0000039}$ | 0.0421$^{+0.0007}$ $_{−0.0011}$ | 1646$^{+25}$ $_{−24}$ | transit | 1399±7 | 1.181$^{+0.064}$ $_{−0.092}$ | 5772$^{+84}$ $_{−80}$ | |
| TOI-3819 b | 1.11$^{+0.18}$ $_{−0.20}$ | 1.172$^{+0.036}$ $_{−0.035}$ | 3.2443141±0.0000055 | 0.04611$^{+0.00069}$ $_{−0.00096}$ | 1633$^{+21}$ $_{−19}$ | transit | 1834±17 | 1.242$^{+0.057}$ $_{−0.076}$ | 5859$^{+72}$ $_{−71}$ | |
| TOI-3884 b | 0.0519$^{+0.0110}$ $_{−0.0057}$ | 0.563±0.025 | 4.5445697±0.0000094 | 0.0354±0.0014 | 463±12 | transit | 141.37±0.16 | 0.2813±0.0067 | 3269±70 | |
| TOI-3912 b | 0.406$^{+0.071}$ $_{−0.068}$ | 1.274$^{+0.041}$ $_{−0.040}$ | 3.4936264±0.0000038 | 0.0463$^{+0.0012}$ $_{−0.0010}$ | 1512±20 | transit | 1533±9 | 1.088$^{+0.086}$ $_{−0.070}$ | 5725$^{+69}$ $_{−68}$ | |
| TOI-3976 b | 0.175$^{+0.037}$ $_{−0.036}$ | 1.095$^{+0.036}$ $_{−0.035}$ | 6.607662$^{+0.000016}$ $_{−0.000015}$ | 0.0743$^{+0.0013}$ $_{−0.0014}$ | 1295$^{+16}$ $_{−14}$ | transit | 1703±8 | 1.254$^{+0.067}$ $_{−0.072}$ | 5975$^{+70}$ $_{−69}$ | |
| TOI-4087 b | 0.73±0.14 | 1.164$^{+0.025}$ $_{−0.024}$ | 3.17748350±0.00000094 | 0.04469$^{+0.00048}$ $_{−0.00054}$ | 1458$^{+20}$ $_{−17}$ | transit | 1013±4 | 1.178$^{+0.039}$ $_{−0.042}$ | 6060$^{+74}$ $_{−67}$ | |
| TOI-4137 b | 1.44$^{+0.17}$ $_{−0.15}$ | 1.211$^{+0.040}$ $_{−0.039}$ | 3.8016122±0.0000065 | 0.05222$^{+0.00089}$ $_{−0.00096}$ | 1570$^{+25}$ $_{−24}$ | transit | 1128±7 | 1.313$^{+0.068}$ $_{−0.071}$ | 6134±50 | |
| TOI-4145 b | 0.43±0.13 | 1.187$^{+0.032}$ $_{−0.031}$ | 4.0664428±0.0000058 | 0.04823$^{+0.00075}$ $_{−0.00079}$ | 1074$^{+19}$ $_{−16}$ | transit | 668.7±1.3 | 0.905$^{+0.043}$ $_{−0.044}$ | 5281$^{+86}$ $_{−76}$ | |
| TOI-4329b | 0.45±0.09 | 1.50±0.19 | 2.9223±0.00015 | | | transit | 2258±16 | 1.538±0.049 | 6000±100 | |
| TOI-4463 b | 0.794$^{+0.039}$ $_{−0.040}$ | 1.183$^{+0.064}$ $_{−0.045}$ | 2.8807198$^{+0.0000028}$ $_{−0.0000027}$ | 0.04036$^{+0.00074}$ $_{−0.00082}$ | 1395$^{+25}$ $_{−22}$ | transit | 579.5±1.8 | 1.056$^{+0.059}$ $_{−0.063}$ | 5640$^{+89}$ $_{−82}$ | |
| TOI-4479 b | 0.0261$^{+0.0252}$ $_{−0.0126}$ | 0.252±0.057 | 1.15890$^{+0.00001}$ $_{−0.00002}$ | 0.0164$^{+0.0015}$ $_{−0.0029}$ | 861$^{+64}$ $_{−103}$ | transit | 262.9±0.3 | 0.452±0.090 | 3400±100 | |
| TOI-4562 b | 3.29$^{+1.88}$ $_{−0.82}$ | 1.072$^{+0.044}$ $_{−0.043}$ | 225.11757$^{+0.00027}$ $_{−0.00025}$ | 0.771±0.013 | 349±10 | transit | 1131±12 | 1.218$^{+0.054}$ $_{−0.048}$ | 6096±32 | Highly eccentric orbit |
| TOI-4582 b | 0.53±0.05 | 0.94$^{+0.09}$ $_{−0.12}$ | 31.034±0.001 | | | transit | 1242 | 1.34±0.06 | 5190±100 | Evolved star, eccentric planetary orbit |
| TOI-4791 b | 2.31$^{+0.32}$ $_{−0.33}$ | 1.110±0.050 | 4.280880$^{+0.000022}$ $_{−0.000023}$ | 0.0555$^{+0.0011}$ $_{−0.0012}$ | 1472$^{+26}$ $_{−24}$ | transit | 1051±6 | 1.242$^{+0.072}$ $_{−0.077}$ | 6058$^{+99}$ $_{−94}$ | |
| TOI-5153 b | 3.26$^{+0.18}$ $_{−0.17}$ | 1.06±0.04 | 20.33003±0.00007 | 0.158±0.006 | 906±13 | transit | 1272.336±11 | 1.24±0.07 | 6300±80 | |
| TOI-5174 b | 0.07801 | 0.47667 | 12.214 | | | transit | | 1.0±0.125 | | |
| TOI-5205b | 1.08±0.06 | 1.03±0.03 | 1.630757±0.000001 | 0.0199±0.0002 | 737±15 | transit | 283.35±0.16 | 0.392±0.015 | 3430±54 | |
| TOI-5542 b | 1.32±0.10 | 1.009$^{+0.036}$ $_{−0.035}$ | 75.12375$^{+0.00019}$ $_{−0.00018}$ | 0.332±0.016 | 441$^{+48}$ $_{−74}$ | transit | 1154±12 | 0.890$^{+0.056}$ $_{−0.031}$ | 5700±80 | |
| Berry 37a | 0.69$^{+0.47}$ $_{−0.43}$ | 1.41±0.14 | 5.616531±0.000023 | 0.066±0.007 | 961.5±8 | transit | 20±60 | 1.32±0.09 | 4200±140 | |
| TYC 2187-512-1 b | 0.33±0.02 | | 691.90$^{+8.77}$ $_{−8.61}$ | 1.22±0.02 | | radial vel. | 50.512±0.016 | 0.498±0.019 | 3734±54 | |
| WASP-132c | 0.165±0.009 | | 1.011534±0.000005 | 0.0182±0.0003 | | transit | 390 | 0.782±0.034 | 4714$^{+87}$ $_{−88}$ | |

## 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 (17)