# List of exoplanets discovered in 2019

This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019.
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 |
| 7 Canis Majoris c | 0.87 | | 996.00 | 2.153 | | radial vel. | 64.6 | 1.34 | 4826 | |
| Beta Pictoris c | 9 | | 1200 | 2.7 | | radial vel. | 64.43 | 1.76 | | |
| DS Tucanae Ab | | 0.509±0.015 | 8.138268±0.000011 | | 850 | transit | 143.89±0.22 | 1.01±0.06 | 5428±80 | |
| Epsilon Indi Ab | 3.25 | | 16510 | 11.55 | 64.25 | radial vel. | 11.87 | 0.75 | | |
| G 9-40 b | | 0.1807 | 5.746007 | 0.0385 | 456 | transit | 91.1 | 0.290 | 3348 | |
| Gliese 49 b | 0.0177$^{+0.0021}$ $_{−0.0021}$ | | 13.8508$^{+0.0053}$ $_{−0.0051}$ | 0.0905±0.0011 | | radial vel. | 32.145±0.01 | 0.515±0.019 | 3805±51 | |
| Gliese 357 b | 0.00579 | 0.1086 | 3.93072 | 0.035 | 525 | transit | 30.80 | 0.342 | 3505 | |
| Gliese 357 c | 0.0107 | | 9.1247 | 0.061 | 401.2 | radial vel. | 30.80 | 0.342 | 3505 | |
| Gliese 357 d | 0.019 | | 55.661 | 0.204 | 219.6 | radial vel. | 30.80 | 0.342 | 3505 | Potentially habitable exoplanet |
| Gliese 378 b [id] | 0.04097±0.006 | | 3.822±0.001 | 0.082±0.002 | | radial vel. | 48.79 | 0.56±0.01 | 3879±67 | |
| Gliese 411 b | 0.00941±0.00145 | | 12.9532±0.0079 | | 349.83±0.32 | radial vel. | 8.284 | 0.386±0.039 | 3563±60 | Host star also known as Lalande 21185 |
| Gliese 685 b | 0.028$^{+0.0053}$ $_{−0.0057}$ | | 24.160$^{+0.061}$ $_{−0.047}$ | 0.1344$^{+0.0052}$ $_{−0.0051}$ | | radial vel. | 46.7102 | 0.3816±0.069 | 0.55±0.06 | |
| Gliese 686 b | 0.022±0.003 | | 15.53209$^{+0.00166}$ $_{−0.00167}$ | 0.091±0.004 | 379$^{+24}$ $_{−25}$ | radial vel. | 26.612±0.008 | 0.42±0.05 | 3663±68 | |
| Gliese 3512 b | 0.463 | | 203.59 | 0.3380 | | radial vel. | 30.95 | 0.123 | 3081 | |
| Gliese 4276 b | 0.05213$^{+0.00296}$ $_{−0.00299}$ | | 13.352±0.003 | 0.082±0.002 | | radial vel. | 69.6±0.1 | 0.41±0.03 | 3387±51 | May be two planwts in 2:1 orbital resonance |
| HAT-P-69b [id] | 3.58 | 1.676 | 4.7869491 | 0.06555 | 1930 | transit | 1122 | 1.65 | 7394 | |
| HAT-P-70b [id] | <6.78 | 1.87 | 2.74432452 | 0.04739 | 4000 | transit | 1073 | 1.89 | 8450 | |
| HD 8326 b [id] | 0.210±0.062 | | 158.991±1.440 | 0.533±0.011 | | radial vel. | 100.2 | 0.80±0.05 | 4914$^{+51}$ $_{−32}$ | |
| HD 13724 b | 26.77$^{+4.40}$ $_{−2.20}$ | | 14763.405$^{+4901.655}$ $_{−1599.795}$ | 12.40$^{+2.60}$ $_{−0.90}$ | | radial vel. | 141.9±0.17 | 0.76±0.71 | 5868±27 | |
| HD 15337 b | 0.0236$^{+0.0034}$ $_{−0.0032}$ | 0.146±0.005 | 4.75615±0.00017 | 0.0522±0.0012 | 1001.0±11.5 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402 |
| HD 15337 c | 0.0255$^{+0.0057}$ $_{−0.0053}$ | 0.213±0.011 | 17.1784±0.0016 | 0.1268±0.0038 | 642±10 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402 |
| HD 21411 b | 0.207±0.081 | | 84.288±0.127 | 0.362±0.007 | | radial vel. | ±95.11 | 0.89±0.05 | 5605$^{+247}$ $_{−132}$ | |
| HD 21749 b | 0.073$^{+0.007}$ $_{−0.006}$ | 0.254$^{+0.023}$ $_{−0.020}$ | 35.61253$^{+0.00060}$ $_{−0.00062}$ | 0.1915$^{+0.0058}$ $_{−0.0063}$ | 422$^{+15}$ $_{−14}$ | transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | |
| HD 21749 c | <0.0116 | 0.0796$^{+0.0057}$ $_{−0.0052}$ | 7.78993$^{+0.00051}$ $_{−0.00044}$ | 0.0695$^{+0.0021}$ $_{−0.0023}$ | 701$^{+25}$ $_{−23}$ | transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | |
| HD 24085 b | 0.0371±0.0098 | | 2.0455±0.0002 | 0.034±0.001 | | radial vel. | 179.4 | 1.22±0.07 | 6034$^{+32}$ $_{−53}$ | |
| HD 25015 b | 4.48$^{+0.30}$ $_{−0.28}$ | | 6019.320$^{+679.365}$ $_{−262.980}$ | 6.19$^{+0.45}$ $_{−0.23}$ | | radial vel. | 122.2±0.22 | 0.86±0.05 | 5160±63 | |
| HD 39855 b | 0.027±0.005 | | 3.2498±0.0004 | 0.041±0.001 | | radial vel. | 75.93 | 0.87±0.05 | 5576$^{+50}$ $_{−46}$ | |
| HD 64114 b | 0.0560±0.0110 | | 45.791±0.070 | 0.246±0.005 | | radial vel. | 102.9 | 0.95±0.05 | 5676$^{+32}$ $_{−87}$ | |
| HD 65216c | 1.295±0.062 | | 577.6±1.328 | 1.301±0.020 | | radial vel. | 114.7±0.1 | 0.95±0.01 | 5718±8 | Rediscovered in 2019 after false positive in 2013 |
| HD 85628 Ab | 1.675±0.241 | 1.515±0.044 | 2.8240932±0.0000046 | 0.0474±0.0013 | 1865±25 | transit | 560±3 | 1.75±0.05 | 7800±200 | Host star also known as MASCARA-4 |
| HD 92788 c | 3.67$^{+0.30}$ $_{−0.25}$ | | 11611.2975$^{+5055.06}$ $_{−905.820}$ | 10.50$^{+2.90}$ $_{−0.55}$ | | radial vel. | 113.1385 | 1.15±0.07 | 5744±24 | |
| HD 92987 b | 16.88$^{+0.69}$ $_{−0.65}$ | | 10354.8375$^{+551.5275}$ $_{−270.2850}$ | 9.62$^{+0.36}$ $_{−0.26}$ | | radial vel. | 142.2±0.22 | 1.08±0.06 | 5770±36 | |
| HD 97048 b | 2.5 | | | 130 | | imaging | 603 | 2.4 | 10000 | Discovered using study of disk kinematics. |
| HD 102843 b | 0.3584±0.0456 | | 3090.942±295.049 | 4.074±0.270 | | radial vel. | 205.05 | 0.95±0.05 | 5436$^{+144}$ $_{−69}$ | |
| HD 103949 b | 0.0352±0.0072 | | 120.878±0.446 | 0.439±0.009 | | radial vel. | 86.50 | 0.77±0.04 | 4792$^{+66}$ $_{−54}$ | |
| HD 181234 b | 8.37$^{+0.34}$ $_{−0.36}$ | | 7462.0575$^{+80.3550}$ $_{−76.7025}$ | 12.40$^{+2.60}$ $_{−0.90}$ | | radial vel. | 155.9±0.42 | 1.01±0.06 | 5386±60 | |
| HD 202696 b | 1.996$^{+0.220}$ $_{−0.100}$ | | 517.8$^{+8.9}$ $_{−3.9}$ | 1.566$^{+0.016}$ $_{−0.007}$ | | radial vel. | 618.3±5.2 | 1.91$^{+0.09}$ $_{−0.14}$ | 5040$^{+71}$ $_{−85}$ | |
| HD 202696 c | 1.864$^{+0.177}$ $_{−0.227}$ | | 946.6$^{+20.7}$ $_{−20.9}$ | 2.342$^{+0.034}$ $_{−0.035}$ | | radial vel. | 618.3±5.2 | 1.91$^{+0.09}$ $_{−0.14}$ | 5040$^{+71}$ $_{−85}$ | |
| HD 206255 b | 0.108±0.022 | | 96.045±0.317 | 0.461±0.009 | | radial vel. | 245.9 | 1.42±0.08 | 5635$^{+82}$ $_{−99}$ | |
| HD 210193 b | 0.4817±0.0733 | | 649.918±8.599 | 1.487±0.031 | | radial vel. | 137.8 | 1.04±0.06 | 5790$^{+38}$ $_{−50}$ | |
| HD 211970 b | 0.0409±0.0079 | | 25.201±0.025 | 0.143±0.003 | | radial vel. | 42.4 | 0.61±0.04 | 4127$^{+149}$ $_{−94}$ | |
| HD 213885 b | 0.0278$^{+0.0021}$ $_{−0.0020}$ | 0.1557$^{+0.0045}$ $_{−0.0046}$ | 1.008035$^{+0.000021}$ $_{−0.000020}$ | 0.02012$^{+0.00015}$ $_{−0.00012}$ | | transit | 156.45721±0.4566189 | 1.068$^{+0.020}$ $_{−0.018}$ | 5978±50 | A transiting 1-day-period super-Earth with an Earth-like composition around a bright (V=7.9) star unveiled by TESS |
| HD 213885 c | 0.06277$^{+0.00434}$ $_{−0.00428}$ | | 4.78503$^{+0.00056}$ $_{−0.000051}$ | 0.056798$^{+0.00044}$ $_{−0.00032}$ | 1265.4$^{+7.3}$ $_{−8.4}$ | radial vel. | 156.45721±0.4566189 | 1.068$^{+0.020}$ $_{−0.018}$ | 5978±50 | |
| HD 221416 b | 0.190±0.018 | 0.836$^{+0.031}$ $_{−0.028}$ | 14.2767±0.0037 | 0.1228$^{+0.00025}$ $_{−0.00026}$ | | transit | 310.0931 | 1.212±0.074 | 5080±90 | Host star also known as TOI-197 or HIP 116158 |
| HD 221420 b | 9.70$^{+1.10}$ $_{−1.00}$ | | 22482$^{+4200}$ $_{−4100}$ | 18.5±2.3 | | radial vel. | 101.7±0.12 | 1.67±0.11 | 5830±44 | |
| HIP 35173 b | 0.0400±0.0085 | | 41.516±0.077 | 0.217±0.004 | | radial vel. | 108.25 | 0.79±0.05 | 4881$^{+55}$ $_{−81}$ | |
| HIP 54373 b | 0.02712±0.00579 | | 7.760±0.003 | 0.063±0.001 | | radial vel. | 61.09 | 0.57±0.03 | 4021$^{+226}$ $_{−146}$ | |
| HIP 54373 c | 0.03914±0.00664 | | 15.144±0.008 | 0.0990±0.0020 | | radial vel. | 61.09 | 0.57±0.03 | 4021$^{+226}$ $_{−146}$ | |
| HIP 71135 b | 0.0592±0.0129 | | 87.190±0.381 | 0.335±0.007 | | radial vel. | 105.5 | 0.66±0.04 | 4146$^{+107}$ $_{−110}$ | |
| HIP 79098 (AB)b | 20.5±4.5 | | | 345±6 | 2450±150 | imaging | 477.2±8.2 | 3.75±1.25 | | Brown dwarf |
| HR 858 b | | 0.1860$^{+0.0061}$ $_{−0.0057}$ | 3.58599±0.00015 | 0.0480$^{+0.0010}$ $_{−0.0011}$ | 1572$^{+22}$ $_{−19}$ | transit | 104.35 | 1.145$^{+0.074}$ $_{−0.080}$ | 6201±50 | |
| HR 858 c | | 0.1730±0.0062 | 5.97293$^{+0.00060}$ $_{−0.00053}$ | 0.0674$^{+0.0014}$ $_{−0.0016}$ | 1326$^{+18}$ $_{−16}$ | transit | 104.35 | 1.145$^{+0.074}$ $_{−0.080}$ | 6201±50 | |
| HR 858 d | | 0.1931$^{+0.0077}$ $_{−0.0074}$ | 11.2300$^{+0.0011}$ $_{−0.0010}$ | 0.1027$^{+0.0022}$ $_{−0.0025}$ | 1075$^{+15}$ $_{−13}$ | transit | 104.35 | 1.145$^{+0.074}$ $_{−0.080}$ | 6201±50 | |
| HR 5183 b | 3.23 | | 27000 | 18 | 171 | radial vel. | 102.7 | 1.07 | 5794 | Exoplanet found with one of the most elliptical orbits as of 2019 |
| K2-32e | | 0.0901$^{+0.0089}$ $_{−0.008}$ | 4.34882$^{+0.00069}$ $_{−0.00075}$ | 0.04951±0.00055 | | transit | 516.6±4.2 | 0.856±0.028 | | With a radius almost identical to that of the Earth it is almost certainly a terrestrial planet |
| K2-43c | | 0.216 | 2.198884 | | 1093.7 | transit | 598 | 0.57 | 3841 | |
| K2-50c | | 0.089$^{+0.011}$ $_{−0.01}$ | 3.96151$^{+0.00046}$ $_{−0.00051}$ | | | transit | 845.82±10.63 | 0.61±0.06 | | |
| K2-63c [ru] | | 0.35±0.11 | 25.4556±0.0047 | 0.189±0.011 | | transit | 524.414±21 | 1.40±0.25 | 6771±303 | Unconfirmed |
| K2-133e [ru] | | 0.154$^{+0.012}$ $_{−0.012}$ | 26.5841$^{+0.0018}$ $_{−0.0017}$ | 0.1346±0.0011 | 296±10 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | Host star also known as LP 358-499 |
| K2-146c | 0.02358 | 0.195 | 4.00498 | | 1093.7 | transit | 259 | 0.33 | 3385 | |
| K2-166c | | 0.109$^{+0.019}$ $_{−0.015}$ | 3.80464$^{+0.00091}$ $_{−0.00105}$ | | | transit | 1568.81$^{+31.64}$ $_{−29.03}$ | 1.07±0.03 | | |
| K2-168c [ru] | | 0.105$^{+0.012}$ $_{−0.009}$ | 8.0468$^{+0.0024}$ $_{−0.0025}$ | | | transit | 800.91±13.67 | 0.91±0.03 | | |
| K2-198c | | 0.1270 | 3.3596055 | | 1229.9 | transit | 362 | 0.80 | 5213 | |
| K2-198d | | 0.2175 | 7.4500177 | | 943.2 | transit | 362 | 0.80 | 5213 | |
| K2-282c | | 0.132$^{+0.012}$ $_{−0.009}$ | 0.70531±0.00005 | | | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | 3rd planet discovered in 2020 |
| K2-286b [ru] | 0.0214±0.0135 | 0.1873±0.0178 | 27.359±0.005 | 0.1768$^{+0.0175}$ $_{−0.0205}$ | 347$^{+21}$ $_{−11}$ | transit | 248.9±0.8 | 0.64±0.02 | 3926±100 | |
| K2-288Bb | | 0.17±0.03 | 31.393463$^{+0.000067}$ $_{−0.000069}$ | 0.164±0.030 | 226.36±22.30 | transit | 214.3±2.8 | 0.33±0.02 | 3341±276 | |
| K2-290b [ru] | 0.0664 | 0.273±0.014 | 9.21165$^{+0.00033}$ $_{−0.00034}$ | 0.0923±0.0066 | 1230±38 | transit | 897±12 | 1.19$^{+0.07}$ $_{−0.08}$ | 6302±120 | Two planets on a retrograde orbit |
| K2-290c [ru] | 0.774±0.047 | 1.006±0.050 | 48.36685$^{+0.00041}$ $_{−0.00040}$ | 0.0923±0.0066 | 676±16 | transit | 897±12 | 1.19$^{+0.07}$ $_{−0.08}$ | 6302±120 | Two planets on a retrograde orbit |
| K2-291b | 0.0204±0.0036 | 0.1418$^{+0.0085}$ $_{−0.0064}$ | 2.225177$^{+0.000066}$ $_{−0.000068}$ | 0.03261±0.00044 | | transit | 295±2 | 0.93±0.04 | 5520±60 | |
| K2-293b [ru] | | 0.219$^{+0.031}$ $_{−0.022}$ | 13.1225$^{+0.0011}$ $_{−0.0012}$ | | 750$^{+170}$ $_{−50}$ | transit | 1290±22 | 0.96$^{+0.04}$ $_{−0.03}$ | 5532±78 | |
| K2-294b [ru] | | 0.148$^{+0.019}$ $_{−0.017}$ | 2.50387$^{+0.00022}$ $_{−0.00023}$ | | 1425$^{+79}$ $_{−54}$ | transit | 1230±20 | 0.99$^{+0.03}$ $_{−0.03}$ | 5612±50 | |
| K2-296b | | 0.167$^{+0.018}$ $_{−0.04}$ | 28.1656$^{+0.0027}$ $_{−0.0028}$ | | | transit | 521.78±4.57 | 0.41$^{+0.11}$ $_{−0.05}$ | | Host star also known as EPIC 201238110 |
| K2-297b | | 0.062$^{+0.005}$ $_{−0.004}$ | 2.13174±0.00022 | | | transit | 831.31±5.48 | 0.78$^{+0.09}$ $_{−0.17}$ | | Host star also known as EPIC 201497682 |
| K2-298b | | 0.098$^{+0.012}$ $_{−0.011}$ | 4.16959$^{+0.00051}$ $_{−0.00053}$ | | | transit | 1441.42±26.65 | 0.8$^{+0.08}$ $_{−0.16}$ | | |
| K2-299b [ru] | | 0.152$^{+0.053}$ $_{−0.028}$ | 4.50756$^{+0.00062}$ $_{−0.0006}$ | | | transit | 1219.21±16.28 | 0.93$^{+0.08}$ $_{−0.1}$ | 5724±72 | Two more planets in star system discovered in 2020 |
| K2-300b [ru] | | 0.09$^{+0.021}$ $_{−0.012}$ | 2.87814$^{+0.00023}$ $_{−0.00026}$ | | | transit | 528.67±5.87 | 0.22$^{+0.04}$ $_{−0.06}$ | | |
| K2-301b [ru] | | 0.145$^{+0.015}$ $_{−0.017}$ | 5.29711$^{+0.00074}$ $_{−0.0007}$ | | | transit | 1491.42±44.98 | 0.56±0.05 | 4114±99 | |
| K2-302b [ru] | | 0.08$^{+0.017}$ $_{−0.018}$ | 2.25372±0.00047 | | | transit | 359.49±3.52 | 0.41$^{+0.1}$ $_{−0.08}$ | | Two more planets in system discovered in 2020 |
| K2-303b [ru] | | 0.086$^{+0.01}$ $_{−0.013}$ | 1.58252$^{+0.00017}$ $_{−0.00018}$ | | | transit | 1034.57±9.59 | 0.71$^{+0.09}$ $_{−0.03}$ | | |
| K2-304b | | 0.118$^{+0.007}$ $_{−0.008}$ | 2.28943±0.00019 | | | transit | 1380.78±23.94 | 0.83$^{+0.09}$ $_{−0.12}$ | | |
| K2-305b | | 0.194$^{+0.06}$ $_{−0.037}$ | 18.0983$^{+0.006}$ $_{−0.0058}$ | | | transit | 2030.88±33.92 | 1.11$^{+0.14}$ $_{−0.12}$ | | |
| K2-306b | | 0.143$^{+0.012}$ $_{−0.014}$ | 34.885$^{+0.011}$ $_{−0.01}$ | | | transit | 931.54±6.69 | 0.91$^{+0.04}$ $_{−0.16}$ | | |
| K2-307b | | 0.1$^{+0.011}$ $_{−0.008}$ | 15.2841$^{+0.0037}$ $_{−0.0029}$ | | | transit | 1053.09±20.65 | 0.98$^{+0.04}$ $_{−0.03}$ | 6004$^{+77}$ $_{−78}$ | Two more planets in system are suspected, second planet in system confirmed in 2021 |
| K2-308b | | 0.884±0.087 | 3.38628±0.00002 | | | transit | | 1.09±0.09 | 6100±263 | |
| K2-310b | | 0.2307±0.0112 | 13.6030±0.0013 | 0.0980±0.0040 | 536±18 | transit | 1133.22 | 0.690±0.038 | 4684±79 | |
| K2-310c | | 0.2400±0.0130 | 65.5500±0.0089 | 0.280±0.006 | 316±10 | transit | 1133.22 | 0.690±0.038 | 4684±79 | |
| KELT-23Ab | 0.938$^{+0.048}$ $_{−0.044}$ | 1.323±0.025 | 2.255251$^{+0.000011}$ $_{−0.000012}$ | 0.03302$^{+0.00068}$ $_{−0.00064}$ | 1561±20 | transit | 409.07±1.14 | 0.94$^{+0.06}$ $_{−0.05}$ | 5899±49 | |
| KELT-24b | 5.18 | 1.272 | 5.5514926 | 0.06969 | 1459 | transit | 313.2 | 1.46 | 6509 | |
| Kepler-47d | 0.05984$^{+0.07501}$ $_{−0.03672}$ | 0.628$^{+0.059}$ $_{−0.044}$ | 187.366$^{+0.069}$ $_{−0.051}$ | 0.6992$^{+0.0031}$ $_{−0.0033}$ | | transit | 4900 | 0.957$^{+0.013}$ $_{−0.015}$ | | |
| Kepler-65e | 0.653$^{+0.056}$ $_{−0.055}$ | | 258.8$^{+1.5}$ $_{−1.3}$ | 0.362±0.007 | | radial vel. | 999.3±8.8 | 1.25±0.06 | 6211±66 | |
| Kepler-82f | 0.0658±0.0031 | | 75.732±0.012 | 0.3395±0.0041 | | timing | 3026.64 | 0.91±0.03 | 5401±108 | |
| Kepler-88d | 3.15±0.15 | | 1409$^{+14}$ $_{−13}$ | 2.45±0.02 | | radial vel. | 1243±7 | 1.022$^{+0.023}$ $_{−0.026}$ | 5513±67 | |
| Kepler-411d | 0.0478±0.0160 | 0.2961±0.0093 | 58.02035±0.00056 | 0.279±0.004 | 410±10 | transit | 500.94±1.57 | 0.87±0.04 | | |
| Kepler-411e | 0.0340±0.0035 | | 31.509728±0.000085 | 0.186±0.003 | 503±9 | timing | 500.94±1.57 | 0.87±0.04 | | |
| Kepler-448c | 22 | | 2500 | 4.2 | | timing | 1318 | 1.5 | | |
| Kepler-1658b | 5.88 | 1.04 | 3.8494 | 0.0546 | | transit | 2629.05 | 2.891$^{+0.130}$ $_{−0.106}$ | 6216±78 | First exoplanet candidate detected by Kepler Space Telescope (known as KOI-4.01), confirmed in 2019. |
| Kepler-1659b | 0.028±0.001 | 0.17±0.02 | 13.608±0.00006 | 0.11229 | | transit | 3812.7570 | 1.02 | | |
| Kepler-1659c | 0.0014±0.001 | 0.17±0.03 | 20.4415±0.0013 | 0.1472 | | transit | 3812.7570 | 1.02 | | |
| Kepler-1660b | 7.693±0.054 | | | 237.68977±0.08237 | | timing | 4013.68±73.27 | 1.21 | | This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler. |
| KMT-2016-BLG-0212Lb | 18 | | | 2.2 | | microlensing | 21000 | 0.48 | | |
| KMT-2016-BLG-1107Lb | 3.283$^{+3.468}$ $_{−1.835}$ | | | 0.342$^{+0.070}$ $_{−0.085}$ | | microlensing | 21700$^{+3090}$ $_{−4400}$ | 0.087$^{+0.092}$ $_{−0.049}$ | | |
| KMT-2016-BLG-1836L b | 2.2$^{+1.9}$ $_{−1.1}$ | | | 3.5$^{+1.1}$ $_{−0.9}$ | | microlensing | 23157.1$^{+2609.25}$ $_{−7827.753}$ | 0.49$^{+0.38}$ $_{−0.25}$ | | |
| KMT-2017-BLG-0165Lb | 0.11$^{+0.05}$ $_{−0.04}$ | | | 3.45$^{+0.98}$ $_{−0.95}$ | | microlensing | 14774.88 | 0.760$^{+0.340}$ $_{−0.270}$ | | |
| KMT-2017-BLG-1038Lb | 2.0$^{+2.0}$ $_{−1.1}$ | | | 1.8$^{+0.6}$ $_{−0.5}$ | | microlensing | 19569.3826 | 0.37$^{+0.36}$ $_{−0.20}$ | | |
| KMT-2017-BLG-1146Lb | 0.710$^{+0.800}$ $_{−0.420}$ | | | 1.6±0.6 | | microlensing | 21200.16 | 0.33$^{+0.36}$ $_{−0.20}$ | | |
| KMT-2018-BLG-1990Lb | 0.348 | | | 0.763 | | microlensing | 3150 | 0.09 | | |
| LHS 3844 b | | 0.1162±0.0020 | 0.46292913±0.00000190 | 0.00622±0.00017 | 805±20 | transit | 48.60±0.03 | 0.15±0.01 | 3036±77 | |
| LP 791-18 b | | 0.0999 | 0.9480050 | 0.009690 | 650 | transit | 86.41 | 0.14 | 2960 | |
| LP 791-18 c | | 0.206 | 4.989963 | 0.029392 | 370 | transit | 86.41 | 0.14 | 2960 | |
| L 98-59 b | 0.00157$^{+0.00094}$ $_{−0.00063}$ | 0.071±0.004 | 2.25314±0.00002 | 0.0233±0.0017 | | transit | 34.64 | 0.31±0.01 | 3367±150 | |
| L 98-59 c | 0.00755$^{+0.00566}$ $_{−0.00252}$ | 0.12$^{+0.007}$ $_{−0.006}$ | 3.690621$^{+0.000013}$ $_{−0.000014}$ | 0.0324±0.0023-0.0024 | | transit | 34.64 | 0.31±0.01 | 3367±150 | |
| L 98-59 d | 0.0107$^{+0.0085}$ $_{−0.0044}$ | 0.14±0.012 | 7.45086$^{+0.00004}$ $_{−0.00005}$ | 0.052±0.004 | | transit | 34.64 | 0.31±0.01 | 3367±150 | |
| L 1159-16 c | 0.23±0.02 | | 772.05$^{+2.41}$ $_{−1.84}$ | 0.88±0.02 | | radial vel. | 14.578±0.005 | 0.15±0.01 | 3154±54 | Confirmed in 2022 as L 1159-16 b |
| LSPM J2116+0234 b | 0.04185$^{+0.00315}$ $_{−0.00346}$ | | 14.4399$^{+0.0078}$ $_{−0.0087}$ | 0.0876$^{+0.0022}$ $_{−0.0021}$ | | radial vel. | 57.53±0.07 | 0.43±0.03 | 3475±51 | |
| LTT 1445 Ab | 0.0069 | 0.123 | 5.35882 | 0.03807 | 433 | transit | 22.4 | 0.26 | 3337 | |
| MOA-bin-29b | 0.600 | | | 0.48 | | microlensing | 23200 | 0.03 | | |
| NGTS-5b [ja] | 0.229±0.037 | 1.136±0.023 | 3.3569866±0.0000026 | 0.0382±0.0013 | 952±24 | transit | 309.5±8.5 | 0.66$^{+0.07}$ $_{−0.06}$ | 4987±41 | |
| NGTS-6b [ja] | 1.339 | 1.326 | 0.8820590 | 0.01677 | | transit | 1010 | 0.77 | 4730 | |
| NGTS-8b | 0.93 | 1.09 | 2.49970 | 0.035 | 1345 | transit | 1420 | 0.89 | 5241 | |
| NGTS-9b | 2.90 | 1.07 | 4.43527 | 0.058 | 1448 | transit | 1420 | 1.34 | 6330 | |
| NSVS 14256825 b | 14.15±0.16 | | 3225±22 | 3.12±0.07 | | timing | 2734.2±137.31 | 0.42±0.07 | 40000 | Disputed |
| NY Virginis c | 5.54 | | 8799 | | | timing | 1800 | | | Disputed |
| OGLE-2013-BLG-0911L b | 9.51$^{+2.72}$ $_{−1.69}$ | | | | | microlensing | 10500$^{+1500}$ $_{−1100}$ | 0.29$^{+0.07}$ $_{−0.05}$ | | |
| OGLE-2015-BLG-1649L | 2.54 | | | 2.07 | | microlensing | 1380 | 0.34 | | |
| OGLE-2016-BLG-1227 b | 0.79$^{+1.3}$ $_{−0.39}$ | | | 3.4$^{+2.1}$ $_{−1}$ | | microlensing | | 0.1$^{+0.17}$ $_{−0.05}$ | | |
| OGLE-2018-BLG-0532Lb | 0.02062$^{+0.00285}$ $_{−0.00254}$ | | | 1.103$^{+0.118}$ $_{−0.107}$ | | microlensing | | | | |
| OGLE-2018-BLG-0596Lb | 0.04383±0.00491 | | | 0.97±0.13 | | microlensing | 18400±2400 | 0.23±0.03 | | |
| OGLE-2018-BLG-0740Lb | 4.8 | | 5480 | 6.1 | | microlensing | 10400 | 1.0 | 5912 | |
| OGLE-2018-BLG-1011Lb | 1.8 | | | 6.1 | | microlensing | 23000 | 0.18 | | |
| OGLE-2018-BLG-1011Lc | 2.8 | | | 0.80 | | microlensing | 23000 | 0.18 | | |
| PDS 70c | 8.0±4.0 | | | 34.5±2 | | imaging | 369.96±1.7 | 0.76±0.02 | 3972±36 | |
| Qatar-8b | 0.371±0.062 | 1.285±0.022 | 3.71495±0.00100 | 0.0474±0.0008 | 1457±14 | transit | 902.5±11 | 1.03±0.05 | 5738±51 | |
| Qatar-9b | 1.19±0.16 | 1.009±0.014 | 1.540731±0.000038 | 0.0234±0.0003 | 1134±9 | transit | 689.5±5.2 | 0.72±0.02 | 4309±31 | |
| Qatar-10b | 0.736±0.090 | 1.543±0.040 | 1.645321±0.000010 | 0.0286±0.0006 | 1955±25 | transit | 1760±33 | 1.16±0.07 | 6124±46 | |
| SDSS J1228+1040 b | | 0.0009$^{+0.0045}$ $_{−0.000758}$ | 0.0857±0.00021 | 0.0034±0.000009 | 1800 | timing | 413.337977±0.4892346 | 0.705±0.05 | | |
| Teegarden b | 0.00330$^{+0.00041}$ $_{−0.00038}$ | | 4.9100±0.0014 | 0.0252$^{+0.0008}$ $_{−0.0009}$ | | radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | |
| Teegarden c | 0.00349$^{+0.00050}$ $_{−0.00047}$ | | 11.409±0.009 | 0.0443$^{+0.0014}$ $_{−0.0015}$ | 226 | radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | Potentially habitable exoplanet |
| TOI-125 b | 0.0299±0.00277 | 0.2432±0.00669 | 4.65382±0.00033 | 0.05186$^{+0.00086}$ $_{−0.00077}$ | 1037±11 | transit | 363.3382±1.435088 | 0.859$^{+0.044}$ $_{−0.038}$ | 5320±39 | |
| TOI-125 c | 0.02086±0.00311 | 0.24614±0.009 | 9.15059$^{+0.0007}$ $_{−0.00082}$ | 0.814±0.0013 | 827.8±8.6 | transit | 363.3382±1.435088 | 0.859$^{+0.044}$ $_{−0.038}$ | 5320±39 | |
| TOI-125 d | 0.0428±0.0038 | 0.2614±0.0152 | 19.98$^{+0.005}$ $_{−0.0056}$ | 0.05186$^{+0.00086}$ $_{−0.00077}$ | 638.1±6.6 | transit | 363.3382±1.435088 | 0.859$^{+0.044}$ $_{−0.038}$ | 5320±39 | |
| TOI-150b | 1.75$^{+0.14}$ $_{−0.17}$ | 1.38±0.04 | 5.857342$^{+0.000065}$ $_{−0.000066}$ | 0.0583$^{+0.0013}$ $_{−0.0018}$ | 1493$^{+29}$ $_{−32}$ | transit | 1095.89±6.52 | 1.25$^{+0.07}$ $_{−0.12}$ | 6003$^{+104}$ $_{−98}$ | |
| TOI-163b | 1.22 | 1.489 | 4.231306 | 0.0580 | 1669 | transit | 1359 | 1.44 | 6495 | |
| TOI-172b | 5.42$^{+0.22}$ $_{−0.20}$ | 0.965$^{+0.032}$ $_{−0.029}$ | 9.47725$^{+0.00064}$ $_{−0.00079}$ | 0.0914±0.0017 | | transit | 1097.418 | 1.128$^{+0.065}$ $_{−0.061}$ | 5645±50 | |
| TOI-175b | 0.00126$^{+0.00050}$ $_{−0.00048}$ | 0.0642$^{+0.0046}$ $_{−0.0035}$ | 2.2531136$^{+0.0000012}$ $_{−0.0000015}$ | 0.02191$^{+0.00080}$ $_{−0.00084}$ | 627$^{+33}$ $_{−36}$ | transit | 34.636±0.010 | 0.273±0.030 | 3415±135 | To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique. Host star also known as L 98-59. |
| TOI-216 b | 0.059±0.002 | 0.714$^{+0.268}$ $_{−0.179}$ | 17.1607 | 0.1293$^{+0.0067}$ $_{−0.0051}$ | 628$^{+13}$ $_{−11}$ | transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years |
| TOI-216 c | 0.56±0.02 | 0.902±0.018 | 34.525528 | 0.2069$^{+0.0107}$ $_{−0.0082}$ | 497$^{+10}$ $_{−8}$ | transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years |
| TOI-270b | 0.0050 | 0.1112 | 3.360080 | 0.0306 | 528 | transit | 73.23 | 0.40 | 3386 | |
| TOI-270c | 0.0193 | 0.216 | 5.660172 | 0.0472 | 424 | transit | 73.23 | 0.40 | 3386 | |
| TOI-270d | 0.0150 | 0.190 | 11.38014 | 0.0733 | 340 | transit | 73.23 | 0.40 | 3386 | Hydrogen and steam atmosphere |
| TOI-564b | 1.463$^{+0.10}$ $_{−0.096}$ | 1.02$^{+0.71}$ $_{−0.29}$ | 1.651144±0.000018 | 0.02734$^{+0.00061}$ $_{−0.00053}$ | 1714$^{+20}$ $_{−21}$ | transit | 643.8±5.9 | 0.998$^{+0.068}$ $_{−0.057}$ | 5640$^{+34}$ $_{−37}$ | |
| TOI-905b | 0.667$^{+0.042}$ $_{−0.041}$ | 1.171$^{+0.052}$ $_{−0.051}$ | 3.739494±0.000038 | 0.04666$^{+0.00096}$ $_{−0.0011}$ | 1192$^{+39}$ $_{−36}$ | transit | 489.9$^{+23.5}$ $_{−22.5}$ | 0.968$^{+0.061}$ $_{−0.068}$ | 5570$^{+150}$ $_{−140}$ | |
| V1298 Tauri b | | 0.911$^{+0.049}$ $_{−0.053}$ | 24.13861$^{+0.00102}$ $_{−0.00090}$ | 0.1687$^{+0.0025}$ $_{−0.0026}$ | 668±22 | transit | 353.9±2.3 | 1.10±0.05 | 4970±120 | |
| V1298 Tauri c | | 0.499 | 8.24958 | 0.0825 | 845±27 | transit | 353.9 | 1.10 | 4970 | |
| V1298 Tauri d | | 0.572 | 12.4032 | 0.1083 | 677±22 | transit | 353.9 | 1.10 | 4970 | |
| V1298 Tauri e | | 0.780 | 60 | 0.308 | 492$^{+66}$ $_{−104}$ | transit | 353.9 | 1.10 | 4970 | |
| WASP-18Ac | 0.174±0.039 | | 2.1558 | 0.035 | | timing | 404 | 1.22 | 6400 | |
| WASP-169b | 0.561 | 1.304 | 5.6114118 | 0.0681 | 1604 | transit | 2080 | 1.34 | 6110 | |
| WASP-171b | 1.084 | 0.980 | 3.8186244 | 0.05040 | 1642 | transit | 2530 | 1.17 | 5965 | |
| WASP-175b | 0.990 | 1.208 | 3.0652907 | 0.04403 | 1571 | transit | 2080 | 1.21 | 6229 | |
| WASP-177b | 0.508±0.038 | 1.58$^{+0.66}$ $_{−0.83}$ | 3.071722±0.000001 | 0.03957±0.00058 | 1142±32 | transit | 580.5583 | 0.876±0.038 | 5017±70 | |
| WASP-178b | 1.66 | 1.81 | 3.3448285 | 0.0558 | 2470 | transit | 1360 | 2.07 | 9360 | |
| WASP-180Ab | 0.9 | 1.24 | 3.409264 | 0.048 | | transit | 830 | 1.3 | 6600 | |
| WASP-181b | 0.299±0.034 | 1.184$^{+0.071}$ $_{−0.059}$ | 4.159±0.0000034 | 0.00542±0.00069 | 1186$^{+32}$ $_{−26}$ | transit | 1444.872 | 1.04±0.04 | 5839±70 | |
| WASP-182b | 0.148 | 0.850 | 3.3769848 | 0.0451 | 1479 | transit | 1080 | 1.08 | 5638 | |
| WASP-183b | 0.502±0.047 | 1.47$^{+0.94}$ $_{−0.33}$ | 4.11177±0.0000051 | 0.0463±0.00075 | 1111±30 | transit | 1069.79292 | 1.00±0.03 | 0.784±0.038 | |
| WASP-184b | 0.57 | 1.33 | 5.18170 | 0.0627 | 1480 | transit | 2090 | 1.23 | 6000 | |
| WASP-185b | 0.980 | 1.25 | 9.38755 | 0.0904 | 1160 | transit | 897 | 1.12 | 5900 | |
| WASP-192b | 2.30 | 1.23 | 2.8786765 | 0.0408 | 1620 | transit | 1610 | 1.09 | 5910 | |

## 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 (870)
* 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 (249)
* 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 (4)