List of exoplanets discovered in 2020
Appearance
(Redirected from Kepler-1702b)
This list of exoplanets discovered in 2020 is a list of confirmed exoplanets that were first observed in 2020.
For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.
Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K) | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
2MASS J1155-7919 b | 10 | 582 | imaging | 330 | [1] Very young Super-Jupiter on unusually wide orbit.[2] | |||||
AU Microscopii b | 0.054±0.015 | 0.371±0.016 | 8.463000±0.000002 | 0.0645±0.0013 | 593±21 | transit | 31.718±0.015 | 0.50±0.03 | 3700±100 | [3][4][5][6] |
AU Microscopii c | 0.007 – 0.079 | 0.295±0.014 | 18.859019±0.000016 | 0.1101±0.0022 | 454±16 | transit | 31.718±0.015 | 0.50±0.03 | 3700±100 | [6] Precise radial velocities of giant stars |
BD-11 4672 c | 0.04837+0.00935 −0.00884 |
74.2+0.06 −0.08 |
0.30±0.01 | radial vel. | 88.63±0.11 | 0.651+0.031 −0.029 |
4550±110 | Habitable zone, highly eccentric orbit.[7] | ||
CD Ceti b | 0.0124+0.0013 −0.0014 |
2.29070±0.00012 | 0.0185+0.0013 −0.0013 |
464±18 | radial vel. | 28.07 | 0.161±0.010 | 3130±51 | [8] | |
CFHTWIR-Oph 98 b | 7.8+0.7 −0.8 |
1.86±0.04 | 8,040,000±470,000 | 200 | 1800±40 | imaging | 447±13 | 0.015±0.0008 | 2320±40 | Very young superjovian planet orbiting a brown dwarf known as 2MASS J16274422-2358521[9] |
Chi Scorpii b | 4.32+0.15 −0.12 |
578.38+2.01 −2.09 |
1.45+0.02 −0.02 |
radial vel. | 378.3+16 −15 |
1.22+0.13 −0.14 |
4157+11 −10 |
Giant star host[10][11] | ||
CoRoT-30 b | 2.90±0.22 | 1.009±0.076 | 9.06005±0.00024 | 0.0844±0.0012 | transit | 3130+220 −130 |
0.98+0.03 −0.05 |
5650±100 | [12] | |
CoRoT-31 b | 0.84±0.34 | 1.46±0.30 | 4.62941±0.00075 | 0.0586±0.0034 | transit | 7140±2300 | 1.25+0.22 −0.21 |
5700±120 | [12] | |
EPIC 201085153 b | 0.214±0.089 | 0.25722±0.000039 | transit | 3945±386 | Extremely tight orbit[13][citation needed] | |||||
EPIC 201085153 c | 0.125+0.179 −0.125 |
2.259797±0.0008 | transit | 3945±386 | [13][citation needed] | |||||
EPIC 201170410 b | 0.00362 | 0.09341+0.0246 −0.0229 |
6.7987±0.0001 | 0.0349+0.0027 −0.0022 |
transit | 437+149 −130 |
0.287+0.101 −0.084 |
3648+172 −143 |
[14][15] | |
EPIC 201650711 c | 0.036±0.007 | 5.544059±0.00016 | transit | 298.8±1.7 | 4310±92 | Ternary star system, and planet b unconfirmed[13][citation needed] | ||||
EPIC 201757695 b | 0.00217 | 0.08101+0.0052 −0.0057 |
2.0478±0.0001 | 0.0296±0.0005 | transit | 1880±110 | 0.727+0.044 −0.053 |
4520+108 −54 |
[14][16][17] | |
EPIC 205152172 b | 0.107±0.018 | 0.980088±0.000026 | transit | 517±2 | 0.669±0.016 | 4202±242 | Candidate since 2016[13][citation needed] | |||
EPIC 206298289 b | 0.078±0.009 | 0.434847±0.000022 | transit | 492±6 | 3875±157 | Candidate since 2016[13][citation needed] | ||||
EPIC 210801536 b | 0.088±0.027 | 0.892592±0.00012 | transit | 5304±259 | Candidate since 2019, one more planet candidate in system[13][citation needed] | |||||
EPIC 220440058 b | 0.125±0.036 | 0.626683±0.00005 | transit | 3682±217 | One more planet candidate in system[13][citation needed] | |||||
EPIC 249893012 b | 0.02753±0.00343 | 0.174±0.008 | 3.5951±0.0003 | 0.047+0.005 −0.007 |
1616+150 −80 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18] |
EPIC 249893012 c | 0.04616±0.00595 | 0.3274+0.0152 −0.0125 |
15.624±0.001 | 0.13+0.01 −0.02 |
990+68 −29 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18] |
EPIC 249893012 d | 0.03203+0.00774 −0.00761 |
0.3515±0.0116 | 35.747±0.005 | 0.22+0.02 −0.04 |
752+69 −37 |
transit | 1059.03±13.69857 | 1.05±0.05 | 5430±85 | [18][19] |
GJ 1061 b | 0.00431+0.00050 −0.00047 |
0.098 | 3.204±0.001 | 0.021±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | Potentially rocky world, larger than Earth[20][21][22] | |
GJ 1061 c | 0.00547±0.00072 | 0.105 | 6.689±0.005 | 0.035±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | Potentially rocky world, larger than Earth[23][21][24] | |
GJ 1061 d | 0.00516+0.00076 −0.00072 |
0.104 | 13.031+0.025 −0.032 |
0.054±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | Potentially rocky world, larger than Earth[25][21][26] | |
GJ 1252 b | 0.0042±0.0009 | 0.105±0.007 | 0.5182349+0.0000063 −0.0000050 |
0.00915±0.00015 | 1410+91 −125 |
transit | 66.49±0.06 | 0.381±0.019 | 3458+140 −133 |
[27] Hot rocky planet with no atmosphere, larger than Earth[28][29] |
GJ 2056 b | 0.0510±0.011 | 0.372 | 69.971±0.061 | 0.283±0.0013 | radial vel. | 92.8 | 0.62±0.08 | Neptune-like ice giant in the habitable zone[30][31] | ||
GJ 3082 b | 0.02759+0.011 −0.01334 |
0.249 | 11.949±0.022 | 0.079+0.006 −0.007 |
radial vel. | 54.2 | 0.47 | Neptune-like ice giant.[32][33][34] | ||
GJ 3473 b | 0.0059±0.0009 | 0.113+0.0045 −0.0044 |
1.1980035+0.0000018 −0.0000019 |
0.01589±0.00062 | 773+16 −15 |
transit | 89.29±0.13 | 0.360±0.016 | 3347±54 | Potentially rocky world, larger than Earth, also called TOI-488 b[35] |
GJ 3473 c | 0.0233+0.0029 −0.0027 |
0.235 | 15.509±0.033 | 0.0876+0.0035 −0.0034 |
329.1+6.6 −6.4 |
radial vel. | 89.29±0.13 | 0.360±0.016 | 3347±54 | Neptune-like ice giant also called TOI-488 c[35][36][37] |
GJ 9689 b | 0.0304±0.00444 | 0.274 | 18.27+0.01 −0.01 |
0.1139±0.0039 | 413.88-492.19 | radial vel. | 100 | 0.59±0.06 | 3836±69 | Neptune-like ice giant.[38][39] |
Gliese 180 d | 0.0236+0.00837 −0.00733 |
0.237 | 106.341+0.261 −0.34 |
0.31+0.024 −0.029 |
radial vel. | 39.96±0.01 | 0.43 | 3371 | Neptune-like ice giant.[40][33] | |
Gliese 229 Ac | 0.0250+0.00752 −0.00733 |
0.256 | 122.005+0.364 −0.382 |
0.339+0.024 −0.029 |
radial vel. | 18.78±0.004 | 0.58 | 3564 | Neptune-like ice giant.[41][42][43] | |
Gliese 251 b | 0.0126+0.00126 −0.00126 |
0.163 | 14.238+0.002 −0.002 |
0.0818+0.0011 −0.0012 |
351+1.4 −1.3 |
radial vel. | 18.205±0.006 | 0.360±0.015 | 3451±51 | Potentially rocky world, larger than earth. |
Gliese 317 c | 1.664+0.118 −0.166 |
1.2 | 6718.777+375.180 −282.469 |
radial vel. | 49.25±0.72 | 0.42±0.05 | 3510±50 | Gas giant[30][47] | ||
Gliese 414 Ab | 0.029+0.010 −0.008 |
0.263+0.099 −0.081 |
50.817+0.031 −0.03 |
0.24±0.01 | 303.7±32.5 | radial vel. | 38.8 | 0.650±0.08 | 4120±109 | Planets orbiting primary star of binary system.
Gl 414A is also known as HD 97101 and HIP 54646.[48] |
Gliese 414 Ac | 0.177+0.033 −0.031 |
0.784+0.360 −0.238 |
748.3+1.3 −1.2 |
1.43±0.06 | 123.3±13.2 | radial vel. | 38.8 | 0.650±0.08 | 4120±109 | Planets orbiting primary star of binary system.
Gl 414A is also known as HD 97101 and HIP 54646.[48] |
Gliese 433 d | 0.01643±0.00290 | 0.191 | 36.052+0.045 −0.031 |
0.178+0.013 −0.015 |
radial vel. | 29.57±0.01 | 0.48 | 3600 | Neptune-like ice giant.[49][50][51] | |
Gliese 480 b | 0.042±0.005 | 0.33 | 9.567±0.005 | 0.068±0.001 | radial vel. | 46.4 | 0.45±0.02 | Neptune-like ice giant.[52][53][33] | ||
Gliese 687 c | 0.0503±0.013 | 0.369 | 727.562±12.198 | 1.165±0.023 | radial vel. | 14.83 | 0.40±0.02 | Second Neptune-like ice giant discovered in this system. [53][54] | ||
HAT-P-68b | 0.724±0.043 | 1.072±0.012 | 2.29840551±0.00000052 | 0.02996+0.00043 −0.00012 |
1027.8±8.2 | transit | 662±3 | 0.6785+0.0299 −0.0079 |
4514±50 | Gas giant.[55][56] |
HATS-37A b | 0.099±0.042 | 0.606±0.016 | 4.3315366±0.0000041 | 0.04913+0.00033 −0.00023 |
1085+16 −12 |
transit | 688.5±8.2 | 0.843+0.017 −0.012 |
5247±50 | Hot Neptune-like gas giant with one more red dwarf in system[57][58] |
HATS-38 b | 0.074±0.011 | 0.614±0.0176 | 4.375021±0.000010 | 0.05036+0.00030 −0.00023 |
1294±10 | transit | 1134±17 | 0.890+0.016 −0.012 |
5740±50 | Hot Neptune-like gas giant.[57][59] |
HATS-47 b | 0.369+0.031 −0.021 |
1.117±0.014 | 3.9228038±0.0000022 | 0.04269+0.00033 −0.00025 |
852.9±4.7 | transit | 984.01±6.20 | 0.674+0.016 −0.012 |
4479±51 | Warm gas giant also known as TOI-1073b.[60][61] |
HATS-48 A b | 0.243+0.022 −0.030 |
0.800±0.0015 | 3.1316666±0.000037 | 0.03769±0.00011 | 954.6±4.8 | transit | 865.6±5.5 | 0.7279±0.0066 | 4190±100 | Warm gas giant.[60][62][63] |
HATS-49 b | 0.353+0.038 −0.027 |
0.765±0.013 | 4.1480467±0.0000037 | 0.04515±0.00016 | 834.8±3.6 | transit | 1058.70±7.18 | 0.7133±0.0075 | 4354±70 | Warm gas giant.[60][64] |
HATS-72 b | 0.1254±0.0039 | 0.7224±0.0032 | 7.3279474±0.0000016 | 0.066517±0.000085 | 739.3±1.6 | transit | 416.37±1.70 | 0.7311±0.0028 | 4612±76 | Warm gas giant, also known as WASP-191b or TOI-294b.[60][65] |
HD 11231 b | 0.426+0.038 −0.052 |
5.2072+0.0002 −0.0055 |
0.0664±0.0005 | 1000 | radial vel. | 437.0495±13.04625 | 1.44±0.03 | 6500±100 | DMPP-2[66] Found by Dispersed Matter Planet Project looking for hot ablating planets. | |
HD 25723 b | 2.50+0.14 −0.17 |
457.01+1.29 −1.31 |
1.49+0.04 −0.05 |
radial vel. | 384.5+17.5 −16.1 |
2.12+0.41 −0.55 |
4766+49 −38 |
Gas giant with a giant star host[67][68] | ||
HD 25723 c | 1.34+0.08 −0.11 |
2273.17+151.11 −116.33 |
4.35+0.22 −0.03 |
radial vel. | 384.5+17.5 −16.1 |
2.12+0.41 −0.55 |
4766+49 −38 |
Giant star host[67] | ||
HD 38677 b | 18.57±0.01 | 0.1462±0.0012 | 877 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[66] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 38677 c | 6.584+0.003 −0.002 |
0.0733+0.0006 −0.0007 |
1239 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[66] Found by Dispersed Matter Planet Project looking for hot ablating planets, 2:1 orbital resonance of unconfirmed transiting planet.[69] | ||
HD 38677 d | 2.882±0.001 | 0.0422+0.0004 −0.0003 |
1632 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[66] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 38677 e | 5.516+0.002 −0.004 |
0.0651±0.0005 | 1314 | radial vel. | 202.2169±3.261564 | 1.21±0.03 | 6196±29 | DMPP-1[66] Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
HD 42936 Ab | 2.58+0.35 −0.58 |
6.6732+0.0011 −0.0003 |
0.0662±0.0013 | 854 | radial vel. | 159.4905±1.956938 | 0.87±0.05 | 5138±99 | DMPP-3[66] Found by Dispersed Matter Planet Project looking for hot ablating planets. | |
HD 60292 b | 6.5±1.0 | 1.13 | 495.4±3.0 | 1.5±0.1 | radial vel. | 1036±10 | 1.7±0.2 | 4348±28 | Gas giant with a giant star host[70][71] | |
HD 63433 b | 0.017 | 0.192±0.0089 | 7.10801+0.00046 −0.00034 |
0.0710+0.0033 −0.0041 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | Young mini-Neptune losing mass at a rate of 0.35 Earth masses per billion years.[72][73] | |
HD 63433 c | 0.023 | 0.236±0.011 | 20.5455±0.001 | 0.1531+0.0074 −0.0092 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | Young mini-Neptune losing mass at a rate of 0.11 Earth masses per billion years.[72][73][74][75] | |
HD 79211 b | 0.0334±0.004 | 24.422±0.014 | 0.142±0.005 | 345 | radial vel. | 20.658±0.005 | 0.64±0.07 | 4005±51 | Orbiting primary star of binary ADS 7251[76][77] | |
HD 80653 b | 0.0180+0.0011 −0.0011 |
0.1439±0.0063 | 0.719573±0.000021 | 0.01661±0.00019 | transit | 358.1197±2.641867 | 1.18±0.04 | 5959±61 | Rocky super-Earth also known as K2-312b.[78][79][80] | |
HD 81817 b | 24.128+9.747 −0.691 |
1.07 | 1021.20159+13.88370 −9.89130 |
3.233+0.125 −0.131 |
radial vel. | 877.773+75.789 −64.791 |
4.3±0.5 | 4140±55 | Gas giant.[81][82][83] | |
HD 86226 c | 0.0228+0.0037 −0.0035 |
0.193±0.007 | 3.98442±0.00018 | 0.049±0.001 | 1311±28 | transit | 148.6±0.4 | 1.019+0.061 −0.066 |
5863±88 | Sub-Neptune super-Earth.[84][85] |
HD 95338 b | 0.1335+0.0070 −0.0065 |
0.347+0.017 −0.018 |
55.087+0.020 −0.020 |
0.262+0.002 −0.002 |
385+17 −17 |
transit | 120.6+0.1 −0.1 |
0.83+0.02 −0.02 |
5212+16 −11 |
Gas giant.[86][87] |
HD108236 b | 0.0102 | 0.1415±0.0087 | 3.79523+0.00047 −0.00044 |
0.0469±0.0017 | 1099+19 −18 |
transit | 210±1 | 0.869+0.050 −0.048 |
5660±61 | Potentially rocky super-Earth.[88][89][90] |
HD108236 c | 0.0155 | 0.1845+0.0089 −0.0081 |
6.2037+0.00064 −0.00052 |
0.0651±0.0024 | 932+17 −16 |
transit | 210±1 | 0.869+0.050 −0.048 |
5660±61 | Potentially rocky super-Earth[88][89][91] |
HD108236 d | 0.0220 | 0.2423±0.0097 | 14.1756+0.001 −0.0011 |
0.1131±0.004 | 708+13 −12 |
transit | 210±1 | 0.869+0.050 −0.048 |
5660±61 | Neptune-like exoplanet.[88][89][92] |
HD108236 e | 0.0306 | 0.279+0.012 −0.011 |
19.592±0.002 | 0.14±0.0052 | 636+12 −11 |
transit | 210±1 | 0.869+0.050 −0.048 |
5660±61 | Neptune-like exoplanet.[88][89][93] |
HD 112640 b | 5.0±1.0 | 1.15 | 613.2±5.8 | 1.7±0.1 | radial vel. | 1065±6 | 1.8±0.2 | 4155±15 | Gas giant with a giant star host[70][94] | |
HD 136295 b | 1.79±0.16 | 926.4±12.8 | 2.02±0.02 | radial vel. | 269.0±1.3 | 1.28+0.11 −0.10 |
4891±50 | Red giant host star also known as HIP 75092[95] | ||
HD 158259 b | 0.00698+0.00123 −0.00142 |
0.1146 | 2.17800+0.00009 −0.00010 |
radial vel. | 88.11±0.05 | 1.21+0.03 −0.08 |
6068 | Potentially rocky super-Earth.[96][97][98] | ||
HD 158259 c | 0.0176+0.0019 −0.0019 |
0.1989 | 3.43200+0.00030 −0.00016 |
radial vel. | 88.11±0.05 | 1.21+0.03 −0.08 |
6068 | Neptune-like.[96][99][98] | ||
HD 158259 d | 0.0170+0.0023 −0.0022 |
0.1945 | 5.1980814+0.0008186 −0.0008814 |
radial vel. | 88.11±0.05 | 1.21+0.03 −0.08 |
6068 | Neptune-like.[96][100][98] | ||
HD 158259 e | 0.0191+0.0030 −0.0032 |
0.5424 | 7.9510+0.0022 −0.0021 |
radial vel. | 88.11±0.05 | 1.21+0.03 −0.08 |
6068 | Neptune-like.[96][101][98] | ||
HD 158259 f | 0.0193+0.0041 −0.0043 |
0.5478 | 12.028±0.009 | radial vel. | 88.11±0.05 | 1.21+0.03 −0.08 |
6068 | Neptune-like.[96][102][98] | ||
HD 164922 d | 0.0331+0.0031 −0.00313 |
0.1633 | 12.4584+0.0019 −0.0023 |
0.2292+0.0026 −0.0027 |
radial vel. | 72.1±0.9 | 0.9211±0.0318 | 5393.4305±68.3325 | Super-earth.[103][104][105] | |
HD 190007 b | 0.0488+0.0038 −0.0041 |
0.362 | 11.724128±0.000099 | radial vel. | 41.4679+0.0329 −0.0326 |
0.77±0.02 | 4610±20 | Neptune-like.[106][107][108] | ||
HD 191939 b | 0.03146±0.0220 | 0.3042±0.0067 | 8.8803256±0.0000047 | 0.0804+0.0025 −0.0023 |
880±20 | transit | 174.849+0.0733 −0.0731 |
0.81±0.04 | 5348±100 | Host star also known as TOI-1339[109][110][111] |
HD 191939 c | 0.02518±0.0031 | 0.2850±0.0067 | 28.579743±0.000045 | 0.1752+0.0055 −0.0050 |
600±13 | transit | 174.849+0.0733 −0.0731 |
0.81±0.04 | 5348±100 | Host star also known as TOI-1339[109][110][111] |
HD 191939 d | 0.00881±0.0019 | 0.2672±0.0062 | 38.353037±0.000060 | 0.2132+0.0065 −0.0061 |
540±11 | transit | 174.849+0.0733 −0.0731 |
0.81±0.04 | 5348±100 | Host star also known as TOI-1339[109][110][111] |
HD 219553 b | 1.94±0.17 | 1481.6±61.7 | 2.84±0.08 | radial vel. | 332.9±1.7 | 1.39±0.09 | 4824±60 | Red giant host star also known as HIP 114933[95] | ||
HD 238090 b | 0.0217+0.0029 −0.0030 |
13.671+0.011 −0.010 |
0.0932±0.0011 | 469.6+2.3 −2.6 |
radial vel. | 49.68±0.03 | 0.578±0.021 | 3933±51 | Orbiting primary star in binary system Gliese 458[45] | |
HD 332231 b | 0.251±0.017 | 0.867+0.027 −0.025 |
18.70173±0.00028 | 0.1436+0.0032 −0.0033 |
876±17 | transit | 262 | 1.127±0.077 | 6089+97 −96 |
TOI 1456[112][113] |
HIP 65 Ab | 3.213±0.078 | 2.03+0.61 −0.49 |
0.9809761+0.000037 −0.000034 |
0.01782±0.00021 | 1411±15 | transit | 201.85818±0.2609251 | 0.781±0.027 | 4590±49 | an ultra-short-period Jupiter orbiting a bright (V=11.1 mag) K4-dwarf.[114][115][116][117] |
HIP 38594 b | 0.026+0.012 −0.014 |
60.711+0.426 −0.192 |
0.256+0.006 −0.007 |
radial vel. | 58.0 | 0.61±0.02 | habitable zone[53] | |||
HIP 38594 c | 0.135+0.077 −0.035 |
3525+541 −572 |
3.842+0.399 −0.441 |
radial vel. | 58.0 | 0.61±0.02 | [53] | |||
HIP 4845 b | 0.053+0.016 −0.028 |
34.151+0.17 −0.09 |
0.177+0.016 −0.020 |
radial vel. | 68.8 | 0.62±0.04 | [53] | |||
HIP 48714 b | 0.071+0.023 −0.020 |
17.819+0.004 −0.009 |
0.112±0.003 | radial vel. | 34.3 | 0.58±0.02 | [53] | |||
HIP 67522 b | 0.25 | 0.894+0.048 −0.047 |
6.9596+0.000016 −0.000015 |
1174±21 | transit | 416±4 | 1.22±0.05 | 5675±75 | One more candidate planet around very young (age below 20 million years) star[118] | |
HIP 107772 b | 0.049+0.014 −0.030 |
55.259+0.111 −0.311 |
0.243+0.022 −0.027 |
radial vel. | 77.1 | 0.63±0.08 | habitable zone[53] | |||
K2-85 b | 0.107±0.009 | 0.684559±0.000026 | transit | 317.8±1.2 | 4427±48 | Also known as EPIC 210707130 p1[13] | ||||
K2-106c | 0.188±0.018 | 13.334621±0.000068 | transit | 803±10 | 5613±39 | Candidate since 2017[13] | ||||
K2-111 c | 0.0356±0.0035 | 15.6785+0.0064 −0.0063 |
0.1166±0.0025 | radial vel. | 680±60 | 0.89±0.02 | 5730±50 | [119] | ||
K2-211c | 0.116±0.018 | 2.601404±0.000072 | transit | 895±14 | 0.882+0.019 −0.027 |
5360±51 | [13] | |||
K2-282d | 0.232±0.027 | 27.248322±0.00047 | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | [13] | |||
K2-299c | 0.223±0.080 | 14.648966±0.000031 | transit | 1219±16 | 5724±72 | Also known as EPIC 206024342 p2[13] | ||||
K2-299d | 0.152±0.054 | 4.507464±0.0000077 | transit | 1219±16 | 5724±72 | Also known as EPIC 206024342 p3[13] | ||||
K2-301c | 0.152±0.018 | 5.2986±0.00035 | transit | 1491±45 | 4114±99 | Also known as EPIC 206042996 p2[13] | ||||
K2-302c | 0.089±0.009 | 2.255438±0.000037 | transit | 359.3±3.5 | 3297±73 | Also known as EPIC 206215704 p2[13] | ||||
K2-302d | 0.098±0.009 | 2.909216±0.000032 | transit | 359.3±3.5 | 3297±73 | Also known as EPIC 206215704 p3[13] | ||||
K2-315b | 0.085±0.005 | 3.1443189±0.0000049 | 0.0234 | 460±5 | transit | 185±1 | 0.174±0.004 | 3300±30 | Also called the "Pi Earth" due its orbital period, or EPIC 249631677b[120] | |
K2-316b | 0.119 | 1.133 | 0.0147 | 841 | transit | 368 | EPIC 249384674b[121] | |||
K2-316c | 0.163 | 5.260 | 0.0582 | 423 | transit | 368 | EPIC 249384674c[121] | |||
K2-317b | 0.261 | 6.220 | 0.0542 | 432 | transit | 577 | EPIC 249557502b[121] | |||
K2-318b | 0.148 | 7.010 | 0.0911 | 456 | transit | 483 | EPIC 249826231b[121] | |||
K2-319b | 0.249 | 26.680 | 0.1516 | 641 | transit | 686 | EPIC 201663879b[121] | |||
K2-320b | 0.234 | 1.995 | 0.0142 | 698 | transit | 356 | EPIC 201796690b[121] | |||
K2-321b | 0.174 | 2.298 | 0.0410 | 701 | transit | 254 | EPIC 248480671b[121] | |||
K2-322b | 0.171 | 8.205 | 0.0594 | 635 | transit | 404 | EPIC 248558190b[121] | |||
K2-323b | 0.187 | 24.930 | 0.1275 | 318 | transit | 387 | EPIC 248616368b[121] | |||
K2-324b | 0.217 | 3.262 | 0.0331 | 707 | transit | 447 | EPIC 248639308b[121] | |||
K2-325b | 0.196 | 6.930 | 0.0419 | 423 | transit | 365 | EPIC 246074965b[121] | |||
K2-326b | 0.203 | 1.256 | 0.0198 | 1114 | transit | 928 | EPIC 246472939b[121] | |||
K2-329b | 0.260+0.020 −0.022 |
0.774+0.026 −0.024 |
12.4551225±0.0000031 | 0.1016+0.0018 −0.0019 |
650+53 −70 |
transit | 760±9 | 0.912+0.048 −0.049 |
5282+40 −39 |
Also called EPIC 246193072 b[122] |
KMT-2019-BLG-1953L b | 0.59+0.71 −0.32 |
0.8+0.9 −0.6 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[123][124] | ||||
KMT-2019-BLG-1953L c | 0.28+0.35 −0.15 |
0.8+0.9 −0.7 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[125][124] | ||||
Kepler-160e | 0.170+0.015 −0.012 |
378.417+0.028 −0.025 |
1.089+0.037 −0.073 |
244.8+2.1 −2.9 |
transit | 3140±60 | 0.88 | 5471+115 −37 |
Next expected transit in September 2020.[126] | |
Kepler-385d | 0.233 | 56.4159 | transit | 4870±160 | [127] | |||||
Kepler-305e | 0.160 | 3.20538 | transit | 2900±90 | [127] | |||||
Kepler-598c | 0.270 | 86.4945 | transit | 2260±40 | FPP=1.0%[127] | |||||
Kepler-647c | 0.357 | 29.6663 | transit | 3660±70 | [127] | |||||
Kepler-716c | 0.124 | 3.96999 | transit | 2110±30 | FPP=0.6%[127] | |||||
Kepler-783c | 0.208 | 7.05395 | transit | 1707±15 | [127] | |||||
Kepler-1001c | 0.140 | 9.18186 | transit | 3110±80 | [127] | |||||
Kepler-1085c | 0.291 | 56.7771 | transit | 4630±150 | [127] | |||||
Kepler-1514c | 0.1049+0.0051 −0.0039 |
10.514181±0.000039 | 0.0997±0.0018 | 1066+16 −14 |
transit | 1240 | 1.196+0.065 −0.063 |
6145+99 −80 |
[128] | |
Kepler-1661(AB) b | 0.053±0.038 | 0.345±0.005 | 175.06±0.06 | 0.633±0.005 | 243 | transit | 1355.26±9.56 | 0.841±0.022 | 5100±100 | [129][130] |
Kepler-1649c | 0.0038 | 0.095+0.014 −0.010 |
19.53527±0.00010 | 0.0649 | 234±20 | transit | 301.6±1.6 | 0.1977±0.0051 | 3240±61 | Habitable zone, Earth-like[131] |
Kepler-1662b | 0.223 | 0.790 | 134.4628 | transit | [132] Host star also known as KOI-1783[133] | |||||
Kepler-1663b | 0.294 | 17.6046 | transit | 1112±11 | Host star also known as KOI-252[127] | |||||
Kepler-1664b | 0.270 | 14.3868 | transit | Host star also known as KOI-349[127] | ||||||
Kepler-1665b | 0.253 | 11.9548 | transit | 1104±5 | Host star also known as KOI-650[127] | |||||
Kepler-1666b | 0.257 | 25.8476 | transit | 4680±190 | Host star also known as KOI-945[127] | |||||
Kepler-1666c | 0.257 | 25.8476 | transit | 4680±190 | Host star also known as KOI-945[127] | |||||
Kepler-1667b | 0.266 | 83.5781 | transit | 2080±20 | Host star also known as KOI-1311[127] | |||||
Kepler-1668b | 0.388 | 15.434 | transit | 4500±200 | Host star also known as KOI-1470[127] | |||||
Kepler-1669b | 0.248 | 9.51216 | transit | 1800±40 | Host star also known as KOI-1475[127] | |||||
Kepler-1670b | 0.299 | 20.4998 | transit | 7200±400 | Host star also known as KOI-1705[127] | |||||
Kepler-1671b | 0.118 | 4.16787 | transit | 1176±7 | Host star also known as KOI-1738[127] | |||||
Kepler-1672b | 0.265 | 150.878 | transit | 1189±14 | Host star also known as KOI-1822[127] | |||||
Kepler-1673b | 0.262 | 33.7888 | transit | 2420±20 | Host star also known as KOI-1863[127] | |||||
Kepler-1674b | 0.286 | 62.5611 | transit | 3400±100 | Host star also known as KOI-1892[127] | |||||
Kepler-1675b | 0.279 | 63.0382 | transit | 2163±19 | Host star also known as KOI-1928[127] | |||||
Kepler-1676b | 0.301 | 29.9221 | transit | Host star also known as KOI-1943[127] | ||||||
Kepler-1677b | 0.241 | 22.064 | transit | 2250±30 | Host star also known as KOI-1984, FPP=0.6%[127] | |||||
Kepler-1678b | 0.295 | 147.974 | transit | 2830±70 | Host star also known as KOI-2066, FPP=0.5%[127] | |||||
Kepler-1679b | 0.184 | 9.75376 | transit | 3040±100 | Host star also known as KOI-2106[127] | |||||
Kepler-1680b | 0.121 | 8.77424 | transit | 1020±5 | Host star also known as KOI-2120[127] | |||||
Kepler-1681b | 0.2227 | 69.8956 | transit | 2100±300 | Host star also known as KOI-2132[127] | |||||
Kepler-1682b | 0.257 | 14.8334 | transit | 3900±160 | Host star also known as KOI-2229[127] | |||||
Kepler-1683b | 0.167 | 15.0337 | transit | 2440±50 | Host star also known as KOI-2293[127] | |||||
Kepler-1684b | 0.256 | 47.7055 | transit | 2060±40 | Host star also known as KOI-2417[127] | |||||
Kepler-1685b | 0.230 | 20.4905 | transit | 3840±150 | Host star also known as KOI-2504[127] | |||||
Kepler-1686b | 0.127 | 9.30987 | transit | 2430±30 | Host star also known as KOI-2559[127] | |||||
Kepler-1687b | 0.147 | 5.77954 | transit | 1375±17 | Host star also known as KOI-2588[127] | |||||
Kepler-1688b | 0.112 | 5.62012 | transit | 1850±380 | Host star also known as KOI-2733[127] | |||||
Kepler-1689b | 0.084 | 8.483 | transit | 967±5 | Host star also known as KOI-2755[127] | |||||
Kepler-1690b | 0.250 | 234.636 | transit | 2340±30 | Host star also known as KOI-2757[127] | |||||
Kepler-1691b | 0.163 | 3.8482 | transit | 4290±110 | Host star also known as KOI-2802[127] | |||||
Kepler-1692b | 0.099 | 5.95966 | transit | 1960±20 | Host star also known as KOI-2849[127] | |||||
Kepler-1693b | 0.115 | 12.0999 | transit | 2530±50 | Host star also known as KOI-2871[127] | |||||
Kepler-1694b | 0.105 | 3.89526 | transit | 1698±16 | Host star also known as KOI-2878, FPP=0.6%[127] | |||||
Kepler-1695b | 0.099 | 4.7329 | transit | 2640±40 | Host star also known as KOI-3048, FPP=0.5%[127] | |||||
Kepler-1696b | 0.250 | 65.9409 | transit | 5100±200 | Host star also known as KOI-3361[127] | |||||
Kepler-1697b | 0.112 | 33.4969 | transit | 813±2 | Host star also known as KOI-3478[127] | |||||
Kepler-1698b | 0.095 | 1.2107 | transit | 729±3 | Host star also known as KOI-3864[127] | |||||
Kepler-1699b | 0.139 | 3.49082 | transit | Host star also known as KOI-3933[127] | ||||||
Kepler-1701b | 0.198 | 169.134 | transit | 1940±20 | Host star also known as KOI-4054,[127] potentially habitable exoplanet | |||||
Kepler-1702b | 0.143 | 18.5012 | transit | 2860±90 | Host star also known as KOI-4386[127] | |||||
KMT-2016-BLG-2397b | 2.42 | 2.83 | microlensing | 16000 | 0.62+0.29 −0.30 |
Multiple solutions for planetary parameters[134] | ||||
KMT-2016-BLG-2364b | 3.93 | 2.63 | microlensing | 21000 | 0.50+0.40 −0.22 |
[134] | ||||
KMT-2018-BLG-0748Lb | 0.18+0.29 −0.10 |
0.62±0.09 | microlensing | 24000 | 0.0870+0.138 −0.047 |
[135] | ||||
KMT-2019-BLG-1339Lb | 12.2+16.1 −6.7 |
0.67+0.77 −0.55 |
microlensing | 23000±3000 | 0.27+0.366 −0.15 |
Multiple solutions for planetary parameters[136] | ||||
KMT-2019-BLG-2073 | 0.19 | microlensing | 12000 | Free-floating planet[137] | ||||||
L 168-9b | 0.0145±0.00176 | 0.124±0.008 | 1.4015±0.00018 | 0.02091±0.00024 | 816±160 | transit | 82.02833±0.07827753 | 0.62±0.03 | 3800±70 | [138] |
Lacaille 9352 b | 0.0132±0.0019 | 0.168 | 9.262±0.001 | 0.068±0.002 | 468 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | Potentially rocky world, larger than Earth, also known as GJ 887b[139][140] |
Lacaille 9352 c | 0.0234±0.0038 | 0.238 | 21.789+0.004 −0.005 |
0.120±0.004 | 352 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | Potentially habitable, larger than Earth, also known as GJ 887c[139][141] |
LHS 1815 b | 0.0132±0.0047 | 0.0971±0.005 | 3.81433±0.00003 | 0.0404±0.0094 | 617±84 | transit | 97 | 0.502 | 3643±142 | [142][143] |
LP 714-47 b | 0.097±0.005 | 0.420±0.027 | 4.052037±0.000004 | 0.0417±0.0005 | 700+19 −24 |
transit | 171.8±0.4 | 0.59±0.02 | 3950±51 | Host star also known as G 160-62 or TOI 442, planet in Neptune desert[144] |
LTT 9779 b | 0.092±0.003 | 0.421±0.021 | 0.792054±0.000014 | 0.01679±0.0014 | 2000 | transit | 262.8±1.0 | 1.02+0.02 −0.03 |
5499±50 | Neptune desert planet[145] |
MOA-2009-BLG-319Lb | 0.2077±0.0255 | 2.03±0.21 | microlensing | 22800±2300 | 0.514±0.063 | [146] | ||||
NGTS-11 b | 0.37±0.14 | 0.823±0.035 | 35.4553±0.0002 | 0.201±0.002 | 440±40 | transit | 624±6 | 0.862±0.028 | 5050±80 | [147] |
NGTS-12b | 0.208±0.022 | 1.048±0.032 | 7.532806±0.000048 | 0.0757±0.0014 | 1257±34 | transit | 1474±25 | 1.021+0.056 −0.049 |
5690±130 | [148] |
OGLE-2006-BLG-284 b | 0.45+0.14 −0.40 |
2.2±0.8 | microlensing | 13000±4900 | 0.35+0.3 −0.2 |
Binary host with 2.1 astronomical unit separation and uncertain, possibly unstable, planetary orbit.[149] | ||||
OGLE-2016-BLG-1928 | 0.001 | n/a | microlensing | 30000 | n/a | n/a | Rogue planet[150] | |||
OGLE-2017-BLG-0406 b | 0.41±0.05 | 3.5±0.3 | microlensing | 17000±1600 | 0.56±0.07 | 4848 | High fidelity microlensing event[151] | |||
OGLE-2017-BLG-0604b | 0.51 | 4.06 | microlensing | 13000 | 0.70±0.28 | [134] | ||||
OGLE-2017-BLG-1049Lb | 5.53+3.62 −2.87 |
3.92+1.10 −1.32 |
microlensing | 18500+3600 −4500 |
0.55+0.36 −0.29 |
[152] | ||||
OGLE-2017-BLG-1375b | 10.33 | 2.97 | microlensing | 12000 | 0.77+0.27 −0.23 |
Multiple solutions for planetary parameters[134] | ||||
OGLE-2018-BLG-0677Lb | 0.0125+0.0185 −0.0084 |
0.68+0.27 −0.22 |
microlensing | 27000±3500 | 0.12+0.14 −0.08 |
Milky way bulge[153] | ||||
OGLE-2018-BLG-1269Lb | 0.69+0.44 −0.22 |
4383 | 4.61+1.70 −1.17 |
microlensing | 8300+3000 −2000 |
0.35+0.3 −0.2 |
Very high fidelity event[154] | |||
OGLE-2018-BLG-0799Lb | 0.22+0.19 −0.06 |
1.27+0.45 −0.29 |
microlensing | 16000 | 0.08+0.08 −0.02 |
[155][156] | ||||
OGLE-2019-BLG-0551 | 0.0242 | microlensing | Poorly characterized free-floating planet[157] | |||||||
Proxima Centauri c | 0.0179±0.006 | 1928±20 | 1.489±0.049 | 39+16 −18 |
radial vel. | 4.244±0.001 | 0.1221±0.0022 | 3042±117 | [158][159] Second planet discovered orbiting nearest star to the Solar System | |
TIC 237913194b | 1.942+0.092 −0.091 |
1.117+0.054 −0.047 |
15.168865±0.000018 | 0.1207±0.0037 | 974 | transit | 1009±6 | 1.026+0.057 −0.055 |
5788±80 | Very eccentric orbit[160] |
TOI 122b | 0.028+0.029 −0.010 |
0.243±0.016 | 5.078030±0.000015 | 0.0392±0.0007 | 471 | transit | 202.9±0.7 | 0.312±0.007 | 3403±100 | [161] |
TOI-132 b | 0.07048+0.00598 −0.00604 |
0.305±0.012 | 2.1097019+0.000012 −0.000011 |
0.026+0.002 −0.003 |
1395+52 −72 |
transit | 536.43±89.11 | 0.970±0.06 | 5397±46 | [162] |
TOI-157 b | 1.18±0.13 | 1.29±0.02 | 2.0845435±0.0000023 | 0.03138+0.00025 −0.00020 |
1588+21 −20 |
transit | 1171 | 0.948+0.023 −0.018 |
5404+70 −67 |
[114] |
TOI 169 b | 0.791+0.064 −0.06 |
1.086+0.081 −0.048 |
2.2554477±0.0000063 | 0.03524+0.00069 −0.00079 |
1715+22 −20 |
transit | 1345 | 1.147+0.069 −0.075 |
5880+54 −49 |
[114] |
TOI 237b | 0.009+0.006 −0.003 |
0.128±0.011 | 5.436098±0.000039 | 0.0341±0.0010 | 388 | transit | 124.2±0.7 | 0.179±0.004 | 3212±100 | [161] |
TOI-251b | 0.245±0.016 | 4.937770+0.000028 −0.000029 |
0.05741+0.00023 −0.00017 |
transit | 324.4±1.4 | 1.036+0.013 −0.009 |
5875+100 −190 |
[163] | ||
TOI-257b | 0.134±0.023 | 0.626±0.013 | 18.38827±0.00072 | 0.1523±0.0017 | 1033±19 | transit | 251.37±0.065 | 1.38+0.056 −0.009 |
6075±90 | Host star also called HD 19916.[164][165][166] |
TOI-421 b | 0.051+0.004 −0.003 |
0.461±0.012 | 16.06815+0.00034 −0.00035 |
0.1182+0.0026 −0.0027 |
696.6±12.2 | transit | 244.3±1.9 | 0.852+0.029 −0.021 |
5325+78 −58 |
Also in system a red dwarf star at 2200 a.u. separation[167] |
TOI-421 c | 0.0222±0.0022 | 0.243±0.017 | 5.19676+0.00049 −0.00048 |
0.0557+0.0012 −0.0013 |
1014.9+17.9 −17.6 |
transit | 244.3±1.9 | 0.852+0.029 −0.021 |
5325+78 −58 |
Also in system a red dwarf star at 2200 a.u. separation[167] |
TOI-481 b | 1.53±0.03 | 0.99±0.01 | 10.33111±0.00002 | 0.097±0.001 | 1370±10 | transit | 587 | 1.14+0.02 −0.01 |
5735±72 | [168] |
TOI-519 b | <14 | 0.75±0.21 | 1.2652328±0.0000005 | 0.012±0.004 | 760±54 | transit | 378±3 | 0.369+0.026 −0.097 |
3350+100 −200 |
Very faint 17-magnitude host star[169] |
TOI 540 b | 0.081±0.005 | 1.2391491±0.0000017 | 0.01223±0.00036 | 611±23 | transit | 45.67±0.29 | 0.159±0.014 | 3216±83 | [170] | |
TOI-561 b | 0.0050±0.0011 | 0.127±0.006 | 0.446578±0.000017 | 0.01055±0.00008 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[171][172] | |
TOI-561 c | 0.017±0.003 | 0.257±0.009 | 10.779±0.004 | 0.08809±0.0007 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[171][172] | |
TOI-561 d | 0.038±0.004 | 0.226±0.011 | 25.62±0.04 | 0.1569±0.0012 | transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[171][172] | |
TOI-561 e | 0.050±0.007 | 0.238±0.010 | 77.23±0.39 | 0.3274+0.0028 −0.0027 |
transit | 279.2±1.6 | 0.785±0.018 | 5455+65 −47 |
[171] | |
TOI-700 b | 0.00406+0.003 −0.00116 |
0.0901+0.00839 −0.00776 |
9.97701+0.00024 −0.00028 |
0.0637+0.0064 −0.006 |
transit | 101.5 | 0.416±0.01 | 3480±135 | [173] | |
TOI-700 c | 0.0249+0.0085 −0.0057 |
0.2346+0.0214 −0.0205 |
16.051998+0.000089 −0.000092 |
0.0925+0.0088 −0.0083 |
transit | 101.5 | 0.416±0.01 | 3480±135 | [173] | |
TOI-700 d | 0.00711+0.0022 −0.00164 |
0.1062±0.0098 | 37.426+0.0007 −0.001 |
0.163±0.015 | 295±55 | transit | 101.5 | 0.416±0.01 | 3480±135 | First "Earth sized" discovered by TESS[173][174] |
TOI-732 b | 0.098 | 0.119 | 0.7683881 | 0.012 | 892 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[175][176] |
TOI-732 c | 0.027 | 0.205 | 12.25 | 0.07673 | 323 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[175][176] |
TOI-763 b | 0.031±0.002 | 0.203±0.010 | 5.6057±0.0013 | 0.0600±0.0006 | 1038±16 | transit | 311 | 0.917±0.028 | 5444±110 | [177] |
TOI-763 c | 0.029±0.003 | 0.235±0.011 | 12.2737+0.0053 −0.0077 |
0.1011±0.0010 | 800±12 | transit | 311 | 0.917±0.028 | 5444±110 | [177] |
TOI-763 d | 0.030±0.005 | 47.7991±2.7399 | 0.2504+0.0093 −0.0105 |
509±12 | radial vel. | 311 | 0.917±0.028 | 5444±110 | [177] | |
TOI-776 b | 0.0147±0.0031 | 0.163±0.010 | 8.24664+0.00009 −0.00006 |
0.0652±0.0011 | 513±12 | transit | 88.6±0.1 | 0.544±0.028 | 3709±70 | [178] |
TOI-776 c | 0.0192±0.0047 | 0.184±0.012 | 15.6653+0.0008 −0.0007 |
0.1000±0.0017 | 415±10 | transit | 88.6±0.1 | 0.544±0.028 | 3709±70 | [178] |
TOI-813 b | 0.599±0.034 | 83.8911+0.0027 −0.0031 |
0.423+0.031 −0.037 |
610+28 −21 |
transit | 864.8192±5.156379 | 1.32±0.06 | 5907±150 | [179] | |
TOI 824 b | 0.058±0.006 | 0.261+0.018 −0.017 |
1.392978+0.000018 −0.000017 |
0.02177±0.00032 | 1253+38 −37 |
transit | 208 | 0.69+0.009 −0.007 |
4569±50 | Neptunian desert planet,[180] likely stripped of hydrogen envelope[181] |
TOI-892 b | 0.95±0.07 | 1.07±0.02 | 10.62656±0.00007 | 0.092±0.005 | 1397±40 | transit | 1120 | 1.28+0.03 −0.02 |
6261±80 | [168] |
TOI 837 b | <1.2 | 0.768+0.091 −0.072 |
8.3248762±0.0000157 | transit | 466.5±1.2 | 1.118±0.059 | 6047±162 | Belongs to open cluster IC 2602[182] | ||
TOI-849 b | 0.128±0.008 | 0.308+0.014 −0.011 |
0.7655240±0.0000027 | 0.01598±0.00013 | 1800 | transit | 735 | 0.929±0.023 | 5329±48 | Neptunian desert planet[183] |
TOI-942b | 0.429±0.018 | 4.324190±0.00003 | 0.04796+0.00073 −0.00065 |
transit | 498±2 | 0.788+0.037 −0.031 |
4928+125 −85 |
[163][184] Host star TYC 5909-319-1 | ||
TOI-942c | 0.517+0.017 −0.016 |
10.156430+0.000069 −0.000079 |
0.0847+0.0012 −0.0011 |
transit | 498±2 | 0.788+0.037 −0.031 |
4928+125 −85 |
[163][184] Host star TYC 5909-319-1 | ||
TOI-954 b | 0.174+0.018 −0.017 |
0.852+0.053 −0.062 |
3.6849729+0.0000027 −0.0000028 |
0.04963+0.00089 −0.00090 |
1526+123 −164 |
transit | 768.5±8.3 | 1.201+0.066 −0.064 |
5710+53 −49 |
[122] |
TOI-1130 b | 0.3256±0.009 | 4.066499±0.000046 | 0.04394+0.00035 −0.00038 |
876±17 | transit | 190 | 0.684+0.16 −0.17 |
4250±67 | [185][186] | |
TOI-1130 c | 0.974+0.043 −0.044 |
1.5+0.27 −0.22 |
8.350381±0.000033 | 0.07098+0.00056 −0.0006 |
637±12 | transit | 190 | 0.684+0.16 −0.17 |
4250±67 | [185][187] |
TOI-1235 b | 0.0217±0.00025 | 0.155±0.007 | 3.444729+0.000031 −0.000028 |
0.03845+0.00037 −0.0004 |
754±18 | transit | 129 | 0.640±0.016 | 3872±70 | one more suspected planet in system[188] |
TOI-1266 b | 0.042+0.035 −0.028 |
0.212+0.014 −0.011 |
10.894843+0.000067 −0.000066 |
0.0736+0.0016 −0.0017 |
413±20 | transit | 117.5±0.1 | 0.48±0.1 | 3570±100 | [189][190] |
TOI-1266 c | 0.007+0.006 −0.005 |
0.139+0.013 −0.012 |
18.80151+0.00067 −0.00069 |
0.1058+0.0023 −0.0024 |
344±16 | transit | 117.5±0.1 | 0.48±0.1 | 3570±100 | [189] Possibly atmosphere of steam[191][190] |
TOI-1338 b | 0.10382±0.0622 | 0.61±0.0169 | 95.2 | 0.4607 | 724 | transit | 1301 | First circumbinary planet discovered by TESS[192] | ||
TOI-1728 b | 0.084+0.017 −0.016 |
0.450±0.014 | 3.491510+0.000062 −0.000057 |
0.0391±0.0009 | 767±8 | transit | 198.2±0.5 | 0.646+0.023 −0.022 |
3980+31 −32 |
[193] |
TOI-1899 b | 0.67±0.04 | 0.99±0.03 | 29.090312+0.000036 −0.000035 |
0.1587+0.067 −0.075 |
362±7 | transit | 419±1 | 0.627+0.026 −0.028 |
3841+54 −45 |
[194][195] |
TVLM 513-46546 b | 0.38±0.24 | 221±5 | 0.3±0.0036 | astrometry | 34.90±0.07 | 0.09 | 2500 | [196] | ||
TYC 8998-760-1 c | 6±1 | 1.1+0.6 −0.3 |
320 | 1240+160 −170 |
imaging | 309.4±0.9 | 4783 | [197] | ||
USco1621 b | 16 | 2880 | 2270 | imaging | 450 | 0.36 | 3460 | [198] | ||
USco1556 b | 15 | 3500 | 2240 | imaging | 459 | 0.33 | 3410 | [198] | ||
XO-7b | 0.709 | 1.373 | 2.8641424 | 0.04421 | 1743 | transit | 763 | 1.405 | 6250 | [199] |
WASP-148 b | 0.291±0.025 | 0.722±0.055 | 8.80381±0.000043 | 0.22±0.063 | 940±80 | transit | 809±5 | 1.00±0.08 | 5460±130 | [200][201] |
WASP-148 c | 0.397+0.203 −0.044 |
34.515±0.029 | 0.359±0.086 | 590±50 | radial vel. | 809±5 | 1.00±0.08 | 5460±130 | [200][201] | |
WASP-150 b | 8.46+0.28 −0.2 |
1.07+0.024 −0.025 |
5.644207+0.00003 −0.000004 |
0.0694+0.0011 −0.0008 |
1460±11 | transit | 2422 | 1.394+0.07 −0.049 |
6218+49 −45 |
[202] |
WASP-176 b | 0.855+0.072 −0.069 |
1.505+0.05 −0.045 |
3.899052±0.00005 | 0.0535+0.001 −0.0019 |
1721+28 −21 |
transit | 1883 | 1.345+0.08 −0.13 |
5941+77 −79 |
[202] |
WASP-186 b | 4.22±0.18 | 1.11±0.03 | 5.026799+0.000012 −0.000014 |
0.0600+0.0012 −0.0013 |
1348+23 −22 |
transit | 913±11 | 1.22+0.07 −0.08 |
6361+105 −82 |
Also called TOI-1494[203] |
WASP-187 b | 0.80±0.09 | 1.64±0.05 | 5.147878+0.000005 −0.000009 |
0.0653±0.0013 | 1726+31 −2 |
transit | 1224±21 | 1.54±0.09 | 6150+92 −85 |
Also called TOI-1493[203] |
Wendelstein-1b | 0.59+0.17 −0.13 |
1.0314+0.00204 −0.021 |
2.663416±0.000001 | 0.0282±0.0009 | 1727+78 −90 |
transit | 1004±10 | 0.65±0.1 | 3984+152 −46 |
[204] |
Wendelstein-2b | 0.731+0.541 −0.311 |
1.1592±0.0061 | 1.7522239±0.0000008 | 0.0234±0.0015 | 1852+120 −140 |
transit | 1875±20 | 0.73±0.11 | 4288+133 −111 |
Extended gaseous envelope[204] |
WD 1856+534 b | 13.8 | 0.93±0.09 | 1.4079405±0.0000011 | 0.0204±0.0012 | transit | 80.737±0.144 | 0.518±0.055 | 4710±60 | Orbiting a white dwarf star[205] |
Specific exoplanet lists
[edit]- 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
Lists of exoplanets by year of discovery
[edit]- 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 (150)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (304)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (312)
- List of exoplanets discovered in 2023 (304)
- List of exoplanets discovered in 2024 (176)
References
[edit]- https://exoplanet.eu/catalog/
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- ^ Planet K2-314 d
- ^ GJ 1061 b
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- ^ GJ 1252 b
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- ^ GJ 180 d
- ^ GJ 229 A c
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- ^ GJ 433 d
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- ^ a b Jordán, A.; Bakos, G. Á.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Hartman, J. D.; Henning, Th.; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V.; de Val-Borro, M.; Zhou, G.; Butler, R. P.; Teske, J.; Crane, J.; Shectman, S.; Tan, T. G.; Thompson, I.; Wallace, J. J.; Lázár, J.; Papp, I.; Sári, P. (2020), "HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert", The Astronomical Journal, 160 (5): 222, arXiv:2007.07135, Bibcode:2020AJ....160..222J, doi:10.3847/1538-3881/aba530, S2CID 220514785
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- ^ exoplanet.eu hats-48a b
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