List of exoplanets discovered in 2020

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

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

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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 [es] | 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 [ja] | 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 [ja] | 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 [ja] | 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 [ja] | 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.

False positive in 2019, rediscovered in 2020[44][45][46]

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 65Ab | 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 [ja] | 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 [ja] | 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 [ru] |  | 0.119  | 1.133  | 0.0147  | 841  | transit  | 368  |  |  | EPIC 249384674b[121]
K2-316c [ru] |  | 0.163  | 5.260  | 0.0582  | 423  | transit  | 368  |  |  | EPIC 249384674c[121]
K2-317b [ru] |  | 0.261  | 6.220  | 0.0542  | 432  | transit  | 577  |  |  | EPIC 249557502b[121]
K2-318b [ru] |  | 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 [ru] |  | 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 [ru] | 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 [ja] | 0.19  |  |  |  |  | microlensing  | 12000  |  |  | Free-floating planet[137]
L 168-9b [ja] | 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 [ja] | 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 [ja] | 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 [ja] | 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 [ja] | 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 [ja] | 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 [ja] |  | 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 [ja] |  | 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 [ja] | 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 [ru] | 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 [ja] | 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 [ja] | 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 [ja] | 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]

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

[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 (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 (9)

## References

[edit]

* https://exoplanet.eu/catalog/
* https://exoplanetarchive.ipac.caltech.edu/overview/

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10. ^ Precise radial velocities of giant stars XIV. Evidence of planetary companions around HD 25723, 17 Sco, 3 Cnc, and 44 UMa
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19. ^ Planet K2-314 d
20. ^ GJ 1061 b
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23. ^ GJ 1061 c
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25. ^ GJ 1061 d
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27. ^ GJ 1252 b
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189. ^ a b Stefansson, Gudmundur; Kopparapu, Ravi; Lin, Andrea; Mahadevan, Suvrath; Cañas, Caleb; Kanodia, Shubham; Ninan, Joe; Cochran, William; Endl, Michael; Hebb, Leslie; Wisniewski, John; Gupta, Arvind; Everett, Mark; Bender, Chad; Diddams, Scott; Ford, Eric; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Levi, Eric; Maney, Marissa; Metcalf, Andrew; Monson, Andrew; Ramsey, Lawrence; Robertson, Paul; Roy, Arpita; Schwab, Christian; Terrien, Ryan; Wright, Jason (2020), A Mini-Neptune and a Venus-Zone Planet in the Radius Valley Orbiting the Nearby M2-dwarf TOI-1266: Validation with the Habitable-zone Planet Finder, arXiv:2006.11180
190. ^ a b Demory, B.-O.; et al. (2020), "A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266", Astronomy & Astrophysics, 642: A49, arXiv:2009.04317, Bibcode:2020A&A...642A..49D, doi:10.1051/0004-6361/202038616, S2CID 221554586
191. ^ Harman, C. E.; Ravi Kumar Kopparapu; Stefánsson, Guðmundur; Lin, Andrea S. J.; Mahadevan, Suvrath; Hedges, Christina; Batalha, Natasha E. (2021), "A Snowball in Hell: The Potential Steam Atmosphere of TOI-1266c", The Planetary Science Journal, 3 (2): 45, arXiv:2109.10838, Bibcode:2022PSJ.....3...45H, doi:10.3847/PSJ/ac38ac, S2CID 237592960
192. ^ Kostov, Veselin B.; Orosz, Jerome A.; Feinstein, Adina D.; Welsh, William F.; Cukier, Wolf; Haghighipour, Nader; Quarles, Billy; Martin, David V.; Montet, Benjamin T.; Torres, Guillermo; Triaud, Amaury H. M. J.; Barclay, Thomas; Boyd, Patricia; Briceno, Cesar; Andrew Collier Cameron; Correia, Alexandre C. M.; Gilbert, Emily A.; Gill, Samuel; Gillon, Michael; Haqq-Misra, Jacob; Hellier, Coel; Dressing, Courtney; Fabrycky, Daniel C.; Furesz, Gabor; Jenkins, Jon; Kane, Stephen R.; Kopparapu, Ravi; Vedad Kunovac Hodzic; Latham, David W.; et al. (2020). "TOI-1338: TESS' First Transiting Circumbinary Planet". The Astronomical Journal. 159 (6): 253. arXiv:2004.07783. Bibcode:2020AJ....159..253K. doi:10.3847/1538-3881/ab8a48. S2CID 215785933.
193. ^ Kanodia, Shubham; Cañas, Caleb I.; Stefansson, Gudmundur; Ninan, Joe P.; Hebb, Leslie; Lin, Andrea S. J.; Baran, Helen; Maney, Marissa; Terrien, Ryan C.; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Dong, Jiayin; Bender, Chad F.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Metcalf, Andrew J.; Monson, Andrew; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Wright, Jason T. (2020), "TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host", The Astrophysical Journal, 899 (1): 29, arXiv:2006.14546, Bibcode:2020ApJ...899...29K, doi:10.3847/1538-4357/aba0a2, S2CID 220056014
194. ^ Cañas, Caleb I.; Stefansson, Gudmundur; Kanodia, Shubham; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Robertson, Paul; Bender, Chad F.; Ninan, Joe P.; Beard, Corey; Lubin, Jack; Gupta, Arvind F.; Everett, Mark E.; Monson, Andrew; Wilson, Robert F.; Lewis, Hannah M.; Brewer, Mary; Majewski, Steven R.; Hebb, Leslie; Dawson, Rebekah I.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Lin, Andrea S. J.; Metcalf, Andrew J.; Rajagopal, Jayadev; Ramsey, Lawrence W.; et al. (2020), "A Warm Jupiter Transiting an M Dwarf: A TESS Single-transit Event Confirmed with the Habitable-zone Planet Finder", The Astronomical Journal, 160 (3): 147, arXiv:2007.07098, Bibcode:2020AJ....160..147C, doi:10.3847/1538-3881/abac67, S2CID 220514735
195. ^ Lin, Andrea S. J.; et al. (2023), "The Unusual M-dwarf Warm Jupiter TOI-1899 b: Refinement of Orbital and Planetary Parameters", The Astronomical Journal, 166 (3): 90, arXiv:2301.10837, Bibcode:2023AJ....166...90L, doi:10.3847/1538-3881/ace1ef
196. ^ Curiel, Salvador; Ortiz-León, Gisela N.; Mioduszewski, Amy J.; Torres, Rosa M. (2020). "An Astrometric Planetary Companion Candidate to the M9 Dwarf TVLM 513–46546". The Astronomical Journal. 160 (3): 97. arXiv:2008.01595. Bibcode:2020AJ....160...97C. doi:10.3847/1538-3881/ab9e6e. S2CID 220961489.
197. ^ Bohn, Alexander J.; Kenworthy, Matthew A.; Ginski, Christian; Rieder, Steven; Mamajek, Eric E.; Meshkat, Tiffany; Pecaut, Mark J.; Reggiani, Maddalena; De Boer, Jozua; Keller, Christoph U.; Snik, Frans; Southworth, John (2020), "Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1", The Astrophysical Journal, 898 (1): L16, arXiv:2007.10991, Bibcode:2020ApJ...898L..16B, doi:10.3847/2041-8213/aba27e, S2CID 220686536
198. ^ a b Chinchilla, Patricia; et al. (2020). "USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius". Astronomy & Astrophysics. 633: A152. arXiv:1912.04150. Bibcode:2020A&A...633A.152C. doi:10.1051/0004-6361/201936130. S2CID 208910589.
199. ^ Crouzet, Nicolas; et al. (2020). "XO-7 b: A Transiting Hot Jupiter with a Massive Companion on a Wide Orbit". The Astronomical Journal. 159 (2): 44. arXiv:1912.02821. Bibcode:2020AJ....159...44C. doi:10.3847/1538-3881/ab5b12. S2CID 208857410.
200. ^ a b Hebrard, G.; Diaz, R. F.; Correia, A. C. M.; Collier Cameron, A.; Laskar, J.; Pollacco, D.; Almenara, J. -M.; Anderson, D. R.; Barros, S. C. C.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Boue, G.; Boumis, P.; Brown, D. J. A.; Dalal, S.; Deleuil, M.; Demangeon, O.; Doyle, A. P.; Haswell, C. A.; Hellier, C.; Osborn, H.; Kiefer, F.; Kolb, U. C.; Lam, K.; Lecavelier des Etangs, A.; Lopez, T.; Martin-Lagarde, M.; Maxted, P.; et al. (2020). "Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets". Astronomy & Astrophysics. A32: 640. arXiv:2004.14645. Bibcode:2020A&A...640A..32H. doi:10.1051/0004-6361/202038296. S2CID 216867348.
201. ^ a b Maciejewski, G.; Fernández, M.; Sota, A.; Garcìa Segura, A.J. (2020), "A Newtonian Model for the WASP-148 Exoplanetary System Enhanced with TESS and Ground-based Photometric Observations", Acta Astronomica, 70 (3): 203, arXiv:2012.02602, Bibcode:2020AcA....70..203M, doi:10.32023/0001-5237/70.3.3, S2CID 227305904
202. ^ a b Cooke, Benjamin F.; Pollacco, Don; Almleaky, Y.; Barkaoui, K.; Benkhaldoun, Z.; Blake, James A.; Bouchy, François; Boumis, Panos; Brown, D. J. A.; Bruni, Ivan; Burdanov, A.; Andrew Collier Cameron; Chote, Paul; Daassou, A.; D'ago, Giuseppe; Dalal, Shweta; Damasso, Mario; Delrez, L.; Doyle, A. P.; Ducrot, E.; Gillon, M.; Hébrard, G.; Hellier, C.; Henning, Thomas; Jehin, E.; Kiefer, Flavien; King, George W.; Liakos, Alexios; Lopez, Théo; et al. (2020). "Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b". The Astronomical Journal. 159 (6): 255. arXiv:2004.06622. Bibcode:2020AJ....159..255C. doi:10.3847/1538-3881/ab88db. S2CID 215754471.
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* v
* t
* e

Exoplanets

* Planet
* Definition
* IAU
* Planetary science

Main topics|

* Exoplanet
* Exoplanet orbital and physical parameters
* Methods of detecting exoplanets
* Planetary system
* Planet-hosting stars

Sizes
and
types|

| Terrestrial|

* Carbon planet
* Coreless planet
* Desert planet
* Dwarf planet
* Hycean planet
* Ice planet
* Iron planet (Super-Mercury)
* Lava planet
* Ocean world
* Mega-Earth
* Sub-Earth
* Super-Earth

|

Gaseous|

* Eccentric Jupiter
* Mini-Neptune (Gas dwarf)
* Helium planet
* Hot Jupiter
* Hot Neptune
* Gas giant
* Ice giant
* Super-Jupiter
* Super-Neptune
* Super-puff
* Ultra-hot Jupiter
* Ultra-hot Neptune

Other types|

* Blanet
* Brown dwarf
* Chthonian planet
* Circumbinary planet
* Circumtriple planet
* Disrupted planet
* Double planet
* Ecumenopolis
* Eyeball planet
* Giant planet
* Mesoplanet
* Planemo
* Planet/Brown dwarf boundary
* Planetesimal
* Protoplanet
* Pulsar planet
* Sub-brown dwarf
* Sub-Neptune
* Toroidal planet
* Ultra-cool dwarf
* Ultra-short period planet (USP)

Formation
and
evolution|

* Accretion
* Accretion disk
* Asteroid belt
* Circumplanetary disk
* Circumstellar disc
* Circumstellar envelope
* Cosmic dust
* Debris disk
* Detached object
* Disrupted planet
* Excretion disk
* Exozodiacal dust
* Extraterrestrial materials
* Extraterrestrial sample curation
* Giant-impact hypothesis
* Gravitational collapse
* Hills cloud
* Internal structure
* Interplanetary dust cloud
* Interplanetary medium
* Interplanetary space
* Interstellar cloud
* Interstellar dust
* Interstellar medium
* Interstellar space
* Kuiper belt
* List of interstellar and circumstellar molecules
* Merging stars
* Molecular cloud
* Nebular hypothesis
* Oort cloud
* Outer space
* Planetary migration
* Planetary system
* Planetesimal
* Planet formation
* Protoplanetary disk
* Ring system
* Rubble pile
* Sample-return mission
* Scattered disc
* Star formation

Systems|

* Exocomet
* Interstellar
* Exomoon
* Tidally detached
* Rogue planet
* Orbits
* Retrograde
* Trojan
* Mean-motion resonances
* Titius–Bode law

Host stars|

* A
* B
* Binary star
* Brown dwarfs
* F/Yellow-white dwarfs
* G/Yellow dwarfs
* Herbig Ae/Be
* K/Orange dwarfs
* M/Red dwarfs
* Pulsar
* Red giant
* Subdwarf B
* Subgiant
* T Tauri
* White dwarfs
* Yellow giants

Detection|

* Astrometry
* Direct imaging
* list
* Microlensing
* list
* Polarimetry
* Timing
* list
* Radial velocity
* list
* Transit method
* list
* Transit-timing variation

Habitability|

* Astrobiology
* Astrooceanography
* Circumstellar habitable zone
* Earth analog
* Extraterrestrial liquid water
* Galactic habitable zone
* Habitability of binary star systems
* Habitability of F-type main-sequence star systems
* Habitability of K-type main-sequence star systems
* Habitability of natural satellites
* Habitability of neutron star systems
* Habitability of red dwarf systems
* Habitability of yellow dwarf systems
* Habitable zone for complex life
* List of potentially habitable exoplanets
* Tholin
* Superhabitable planet

Catalogues|

* Nearby Habitable Systems
* Exoplanet Data Explorer
* Extrasolar Planets Encyclopaedia
* NASA Exoplanet Archive
* NASA Star and Exoplanet Database
* Open Exoplanet Catalogue

Lists|

* Exoplanetary systems
* Host stars
* Multiplanetary systems
* Stars with proto-planetary discs

* Exoplanets
* Discoveries
* Extremes
* Firsts
* Nearest
* Largest
* Heaviest
* Terrestrial candidates
* Kepler
* 1–500
* 501–1000
* 1001–1500
* 1501–2000
* K2
* Potentially habitable
* Proper names

* Discovered exoplanets by year
* before 2000
* 2000–2009
* 2010
* 2011
* 2012
* 2013
* 2014
* 2015
* 2016
* 2017
* 2018
* 2019
* 2020
* 2021
* 2022
* 2023
* 2024
* 2025

Other|

* Carl Sagan Institute
* Exoplanet naming convention
* Exoplanet phase curves
* Exoplanetary Circumstellar Environments and Disk Explorer
* Extragalactic planet
* Extrasolar planets in fiction
* Geodynamics of terrestrial exoplanets
* Neptunian desert
* Nexus for Exoplanet System Science
* Planets in globular clusters
* Small planet radius gap
* Sudarsky's gas giant classification

* Discoveries of exoplanets
* Search projects

* v
* t
* e

2020 in space

* « 2019

2021 »

Space probe
launches |

* Solar Orbiter (Feb 2020)
* Hope (Jul 2020)
* Tianwen-1 (Jul 2020)
* Mars 2020 (Jul 2020)
* Perseverance rover
* Mars Helicopter Ingenuity
* Chang'e 5 (lunar sample return mission; Nov 2020)

Impact events|

* 2020 China bolide

Selected
NEOs|

* Asteroid close approaches
* 594913 ꞌAylóꞌchaxnim
* 2020 BX12
* 2020 CW
* 2020 CD3 (temporary satellite)
* (52768) 1998 OR2
* 2020 HS7
* 2020 JJ
* 2020 LD
* (163348) 2002 NN4
* 2020 OY4
* 2020 QG
* 2011 ES4
* 2018 VP1
* 2020 SO (space debris)
* 2020 SW
* 2020 SL1
* 2020 UA
* 2020 VV
* 2020 VT4
* (153201) 2000 WO107
* (501647) 2014 SD224
* (614689) 2020 XL5

Exoplanets |

* AU Mic b
* Gliese 229 Ac
* Gliese 414
* Ab
* Ac
* Gliese 433
* b
* c
* d
* GJ 1151 b radio emissions
* K2-315b
* Kepler-1649c
* KOI-456.04
* Lacaille 9352
* b
* c
* M51-ULS-1b
* OGLE-2016-BLG-1928 (rogue planet)
* Tau Ceti j (predicted)
* TOI-561
* b
* c
* d
* e
* TOI-700
* b
* c
* d
* TOI-732
* b
* c
* TOI-1338 b
* TOI-1339
* b
* c
* d
* TYC 8998-760-1 c
* WD 1856+534 b

Discoveries|

* Betelgeuse dimming
* FRB 180916 location and periodicity
* Radcliffe wave
* Ophiuchus Supercluster explosion
* PSO J03094+27 (distant blazar)
* 2MASS J1047+21 wind speed measurements
* SGR 1935+2154 (soft gamma ray repeater)
* HR 6819 black hole hypothesis
* PHL 293B ending of P Cygni profile hydrogen emission lines
* Swift J1818.0–1607 (young magnetar)
* GW190814 (announced)
* South Pole Wall
* GW190521 (announced)
* Phosphine detection in the atmosphere of Venus
* Water detection on the sunlit surface of the Moon

Comets |

* C/2019 Y4 (ATLAS)
* P/2019 LD2 (ATLAS)
* C/2017 T2 (PANSTARRS)
* C/2020 F8 (SWAN)
* C/2019 U6 (LEMMON)
* C/2020 F3 (NEOWISE)
* 2P/Encke
* 88P/Howell
* 156P/Russell–LINEAR

Space
exploration|

* Spitzer retirement (Jan 2020)
* BepiColombo (Earth gravity assist; Apr 2020, Venus gravity assist; Oct 2020)
* OSIRIS-REx (sample collection from asteroid Bennu; Oct 2020)
* Hayabusa2 (sample return from asteroid Ryugu; Dec 2020)
* Chang'e 5 (lunar sample return; Dec 2020)

* Outer space portal
* Category:2019 in outer space — Category:2020 in outer space — Category:2021 in outer space

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