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] |
HD 187123 is a single, yellow-hued star with two exoplanetary companions in the northern constellation of Cygnus. It has an apparent visual magnitude of 7.83, making it an 8th magnitude star that is too faint to be visible with the naked eye. However, it should be easy target with binoculars or small telescope. The system is located at a distance of 150 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −17 km/s.
HD 86226 is a star with a pair of orbiting exoplanet companions, found in the constellation of Hydra. With an apparent visual magnitude of 7.93, it is too dim to be visible with the naked eye. The distance to this system has been determined by the parallax method, yielding a range of 149 light years. It is receding with a heliocentric radial velocity of +19.6 km/s. A survey in 2015 has ruled out the existence of any stellar companions at projected distances above 12 astronomical units.
HD 86226 b is a gas giant exoplanet discovered by the Magellan Planet Search Program in 2010. It was confirmed in data collected by the CORALIE spectrograph on the Swiss 1.2-metre Leonhard Euler Telescope in 2012. It takes about 4.6 years to orbit its G-type star and was initially believed to have a minimal mass of 0.92 Jupiters. Discovery of the second planet in the system has led to the revised mass of HD 86226 b in 2020, now estimated to be 0.45+0.04
−0.05MJ.
HD 97658 is a star with an exoplanetary companion in the equatorial constellation of Leo. The star is too dim to be seen with the naked eye, having an apparent visual magnitude of 7.76. It is located at a distance of 70 light years based on parallax, but is slowly drifting closer with a radial velocity of −1.6 km/s.
Gliese 880 is a red dwarf star in the northern constellation of Pegasus that may host an exoplanetary companion. No stellar companions to Gliese 880 have been discovered as of 2020.
HD 222155 is a star in the northern constellation of Andromeda. It is a yellow star that can be viewed with binoculars or a small telescope, but is too faint to be seen with the naked eye at an apparent visual magnitude of 7.1. The imaging survey in 2017 did not detect any stellar companions to HD 222155.
HD 179070, also known as Kepler-21, is a star with a closely orbiting exoplanet in the northern constellation of Lyra. At an apparent visual magnitude of 8.25 this was the brightest star observed by the Kepler spacecraft to host a validated planet until the discovery of an exoplanet orbiting HD 212657 in 2018. This system is located at a distance of 354 light-years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −18.2 km/s.
HD 191939 is a single yellow (G-type) main-sequence star, located approximately 174 light-years away in the constellation of Draco, taking its primary name from its Henry Draper Catalogue designation.
HD 164509 is a binary star system in the constellation of Ophiuchus. The primary component has an orbiting exoplanet companion. This system is located at a distance of 175 light years based on parallax measurements, and is drifting further away with a radial velocity of 13.7 km/s. It has an absolute magnitude of 4.64, but at that distance the system has an apparent visual magnitude of 8.10, which is too faint to be seen with the naked eye.
HD 217786 is a binary star system in the equatorial constellation of Pisces. With an apparent visual magnitude of 7.78, it requires binoculars or a small telescope to view. The system is located at a distance of 181 light-years from the Sun based on parallax, and is drifting further away with a radial velocity of +10 km/s. Kinematically, the star system belongs to the thin disk population of the Milky Way.
HD 93396 is a solitary star located in the equatorial constellation Sextans. It has an apparent magnitude of 8.04, making it readily visible in binoculars, but not to the naked eye. The object is located relatively close at a distance of 326 light-years based on Gaia DR3 parallax measurements, but it is receding with a heliocentric radial velocity of 34.96 km/s. At its current distance, HD 93396's brightness is diminished by an interstellar extinction of 0.17 magnitudes and it has an absolute magnitude of +3.01.