List of exoplanets discovered in 2020
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] | |||||
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[3]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[3]Found by Dispersed Matter Planet Project looking for hot ablating planets, 2:1 orbital resonance of unconfirmed transiting planet.[4] | ||
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[3]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[3]Found by Dispersed Matter Planet Project looking for hot ablating planets. | ||
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[3]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[3]Found by Dispersed Matter Planet Project looking for hot ablating planets. | |
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 | [5] |
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 | [5] |
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 | [5][6] |
G 9-40 b | 0.1807 | 5.746007 | 0.0385 | 456 | transit | 91.1 | 0.290 | 3348 | [7] | |
Gliese 180 d | 7.56±1.07 | 106.341+0.261 −0.34 |
0.31+0.024 −0.029 |
radial vel. | 39.96±0.01 | 0.43 | 3371 | [8] | ||
Gliese 229 Ac | 0.025 | 122.005+0.364 −0.382 |
0.339+0.024 −0.029 |
radial vel. | 18.78±0.004 | 0.58 | 3564 | [9][10] | ||
Gliese 433 d | 0.019 | 36.052+0.045 −0.031 |
0.178+0.013 −0.015 |
radial vel. | 29.57±0.01 | 0.48 | 3600 | [11][12] | ||
Gliese 1061 b | 0.00431+0.00050 −0.00047 |
3.204±0.001 | 0.021±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [13] | ||
Gliese 1061 c | 0.00547±0.00072 | 6.689±0.005 | 0.035±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [14] | ||
Gliese 1061 d | 0.00516+0.00076 −0.00072 |
13.031+0.025 −0.032 |
0.054±0.001 | radial vel. | 11.98±0.003 | 0.12±0.01 | 2953±98 | [15] | ||
Gliese 1252 b | 0.00658±0.00176 | 0.1064±0.0066 | 0.5182349+0.0000063 −0.0000050 |
0.00916±0.00076 | 1089±69 | transit | 66.49±0.06 | 0.381±0.019 | 3458+140 −133 |
[16] |
Gliese 3082 b | 0.02759+0.011 −0.01334 |
11.949±0.022 | 0.079+0.006 −0.007 |
radial vel. | 54.2 | 0.47 | [17] | |||
HATS-47b | 0.369 | 1.117 | 3.9228 | 852.9 | transit | 0.674 | [18] | |||
HATS-48Ab | 0.243 | 0.800 | 3.1317 | 0.03769±0.00011 | 954.6 | transit | 865 | 0.7279 | 4546.0+23 −18 |
[18][19] |
HATS-49b | 0.353 | 0.765 | 4.1480 | 834.8 | transit | 0.7133 | [18] | |||
HATS-72b | 0.1254 | 0.7224 | 7.3279 | 739.3 | transit | 0.7311 | [18] | |||
HD 80653 b | 0.0176±0.0014 | 0.1439±0.0063 | 0.719573±0.000021 | 0.0166±0.0003 | transit | 358.1197±2.641867 | 1.18±0.04 | [20] | ||
HD 285507 b | 0.92±0.03 | 6.0962±0.0002 | radial vel. | 153 | 0.73±0.03 | 4503+85 −61 |
[21][22]member of Hyades (star cluster), suspected since 2013 | |||
HIP 65A b | 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.[23][24][25] |
KELT-2019-BLG-1953 b | 0.59+0.71 −0.32 |
0.8+0.9 −0.6 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[26][27] | ||||
KELT-2019-BLG-1953 c | 0.28+0.35 −0.15 |
0.8+0.9 −0.7 |
microlensing | 23000+3600 −4300 |
0.31+0.37 −0.17 |
[28][27] | ||||
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 | [29][30] |
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 | [31] |
OGLE-2018-BLG-0677L b | 0.0125+0.0185 −0.0084 |
0.68+0.27 −0.22 |
microlensing | 27000±3500 | 0.12+0.14 −0.08 |
Milky way bulge[32] | ||||
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 | [33] |
TOI-257 b | 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 | [34] |
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 | [35] | |
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 | [35] | |
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[35][36] |
TOI-732 b | 0.098 | 0.119 | 0.7683881 | 0.012 | 892 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[37][38] |
TOI-732 c | 0.027 | 0.205 | 12.25 | 0.07673 | 323 | transit | 72 | 0.379 | 3360 | Orbiting primary star of binary LDS 3977[37][38] |
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 | [39] | |
TOI-1338 b | 0.616 | 94.5 | 724 | transit | 1301 | First circumbinary planet discovered by TESS[40] | ||||
TOI-1339 b | 0.301 | 8.880411 | 0.089 | 778+58 −41 |
transit | 175 | 0.92 | 5400 | [41] | |
TOI-1339 c | 0.287 | 28.58060 | 0.178 | 550±45 | transit | 175 | 0.92 | 5400 | [41] | |
TOI-1339 d | 0.282 | 38.3561 | 0.216 | 499+12 −11 |
transit | 175 | 0.92 | 5400 | [41] | |
USco1621 b | 16 | 2880 | 2270 | imaging | 450 | 0.36 | 3460 | [42] | ||
USco1556 b | 15 | 3500 | 2240 | imaging | 459 | 0.33 | 3410 | [42] | ||
XO-7b | 0.709 | 1.373 | 2.8641424 | 0.04421 | 1743 | transit | 763 | 1.405 | 6250 | [43] |
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 | [44][45] |
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 |
[23] |
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 |
[23] |
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[46] |
HD 95338 b | 0.124+0.019 −0.013 |
0.355+0.008 −0.007 |
55.086+0.018 −0.019 |
0.231+0.005 −0.009 |
402+6 −9 |
transit | 120 | 0.76+0.16 −0.1 |
5212+16 −11 |
[47] |
HD 332231 b | 0.244±0.021 | 0.867+0.027 −0.025 |
18.71204±0.00043 | 0.1436+0.0032 −0.0033 |
876±17 | transit | 262 | 1.127±0.077 | 6089+97 −96 |
TOI 1456[48] |
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 | [49][50] | |
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 | [49][51] |
HD 78211 b | 0.032±0.005 | 24.45±0.02 | 0.141±0.005 | 345 | radial vel. | 20.658±0.005 | 0.64±0.07 | 4005±51 | [52] | |
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 |
[53] |
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 |
[53] |
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[54] |
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[55] | |||
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[56] |
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[56] |
HD 108236 b | 0.1415±0.0087 | 3.79523+0.00047 −0.00044 |
0.0469±0.0017 | 1099+19 −18 |
transit | 211 | 0.97 | 5730±50 | [57] | |
HD 108236 c | 0.1845+0.0089 −0.0081 |
6.2037+0.00064 −0.00052 |
0.0651±0.0024 | 932+17 −16 |
transit | 211 | 0.97 | 5730±50 | [57] | |
HD 108236 d | 0.2423±0.0097 | 14.1756+0.001 −0.0011 |
0.1131±0.004 | 708+13 −12 |
transit | 211 | 0.97 | 5730±50 | [57] | |
HD 108236 e | 0.279+0.012 −0.011 |
19.592±0.002 | 0.14±0.0052 | 636+12 −11 |
transit | 211 | 0.97 | 5730±50 | [57] | |
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 | [58] |
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 | [58] | |
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 | [59] |
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[60] | |
HD 63433 b | 0.017 | ±0.009 | 7.10801+0.00046 −0.00034 |
0.0710+0.0033 −0.0041 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | [61] | |
HD 63433 c | 0.023 | 0.238±0.01 | 20.5455±0.001 | 0.1531+0.0074 −0.0092 |
transit | 73.08±0.07 | 0.99±0.03 | 5640±74 | [61] | |
HD 164922 d | 0.013±0.003 | 12.458±0.003 | 0.103±0.003 | radial vel. | 72.1±0.9 | 0.874±0.012 | 5293±32 | [62] | ||
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.[63] | ||||
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 |
[64] |
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[64] |
Kepler-160d | 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.[65] | |
EPIC 249631677b | 0.085±0.005 | 3.1443189±0.0000049 | 0.0234 | 460±5 | transit | 185±1 | 0.174±0.004 | 3300±30 | Also called "pi Earth" due its orbital period[66] | |
TOI-1266 b | 0.2193+0.074 −0.066 |
10.894879+0.00007 −0.00007 |
0.0745+0.0046 −0.0069 |
410+21 −15 |
transit | 117.4±1.0 | 0.437±0.021 | 3563±77 | [67] | |
TOI-1266 c | 0.1492+0.077 −0.095 |
18.80152+0.00054 −0.00067 |
0.1037+0.0026 −0.0025 |
347.1+7.9 −8 |
transit | 117.4±1.0 | 0.437±0.021 | 3563±77 | [67] | |
AU Microscopii b | 0.18 | 0.375 | 8.46321±0.00004 | 0.066 | transit | 32.3±0.3 | 0.31 | 3500±100 | [68][69][70] | |
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 |
[71] |
BD-11 4672 c | 0.048±0.009 | 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.[72] | ||
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[73] | |||
Lacaille 9352 b | 0.0132±0.0019 | 9.262±0.001 | 0.068±0.002 | 468 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | [74] | |
Lacaille 9352 c | 0.0234±0.0038 | 21.789+0.004 −0.005 |
0.120±0.004 | 352 | radial vel. | 10.721±0.002 | 0.468±0.012 | 3688±86 | [74] | |
HAT-P-58b | 0.372±0.03 | 1.332±0.043 | 4.0138379±0.0000024 | 0.04994±0.00044 | 1622±18 | transit | 1690±40 | 1.031±0.028 | 6078±48 | [75] |
HAT-P-59b | 1.540±0.067 | 1.123±0.013 | 4.1419771±0.0000012 | 0.05064±0.00037 | 1278±7 | transit | 871±4 | 1.008±0.022 | 5678±16 | [75] |
HAT-P-60b | 0.574±0.038 | 1.631±0.024 | 4.7947813±0.0000024 | 0.06277±0.00017 | 1772±12 | transit | 767±7 | 1.435±0.012 | 6212±26 | [75] |
HAT-P-61b | 1.057±0.07 | 0.899±0.027 | 1.90231289±0.00000077 | 0.03010±0.00034 | 1505±16 | transit | 1120±20 | 1.004±0.012 | 5587±45 | [75] |
HAT-P-62b | 0.761±0.088 | 1.073±0.029 | 2.6453235±0.0000039 | 0.03772±0.00024 | 1512±13 | transit | 1150±20 | 1.023±0.020 | 5629±48 | [75] |
HAT-P-63b | 0.614±0.024 | 1.119±0.033 | 3.377728±0.000013 | 0.04294±0.00035 | 1237±11 | transit | 1330±20 | 0.925±0.023 | 5400+55 −39 |
[75] |
HAT-P-64b | 0.58+0.18 −0.13 |
1.703±0.07 | 4.0072320±0.0000017 | 0.05387±0.00030 | 1766+22 −16 |
transit | 2135±20 | 1.298±0.021 | 6457+55 −36 |
[75] |
TOI-1899 b | 0.66±0.07 | 1.37+0.05 −0.06 |
29.02+0.36 −0.23 |
0.1587+0.067 −0.075 |
362±7 | transit | 419±1 | 0.627+0.026 −0.028 |
3841+54 −45 |
[76] |
HATS-37A b | 0.099±0.042 | 0.606±0.016 | 4.3315 | 0.1587+0.067 −0.075 |
1085+16 −12 |
transit | 695 | 0.843+0.017 −0.012 |
5247±50 | One more red dwarf in system[77] |
HATS-38 b | 0.074±0.011 | 0.614±0.0176 | 4.3750 | 0.1587+0.067 −0.075 |
1294±10 | transit | 1131 | 0.890+0.016 −0.012 |
5740±50 | [77] |
TYC 8998-760-1 c | 6±1 | 1.1+0.6 −0.3 |
320 | 1240+160 −170 |
imaging | 309.4±0.9 | 4783 | [78] | ||
HD 86226 c | 0.023±0.004 | 0.193±0.007 | 3.98442±0.00018 | 0.049±0.001 | 1311±28 | transit | 149 | 1.019+0.061 −0.066 |
5863±88 | [79] |
Specific exoplanet lists
- Lists of exoplanets
- List of exoplanets discovered before 2000 (30)
- List of exoplanets discovered between 2000–2009 (381)
- List of exoplanets discovered in 2010 (97)
- List of exoplanets discovered in 2011 (144)
- List of exoplanets discovered in 2012 (139)
- List of exoplanets discovered in 2013 (125)
- List of exoplanets discovered in 2014 (872)
- List of exoplanets discovered in 2015 (164)
- List of exoplanets discovered in 2016 (1508)
- List of exoplanets discovered in 2017 (149)
- List of exoplanets discovered in 2018 (311)
- List of exoplanets discovered in 2019 (200)
- List of exoplanets discovered in 2020 (97)
- List of potentially habitable exoplanets
- List of proper names of exoplanets
References
- exoplanet.eu Planet 2MASS J1155-7919 b
- www.sci-news.com Astronomers Discover Nearest-Known Newborn Gas Giant
- Haswell, Carole A.; et al. (2019). "Dispersed Matter Planet Project discoveries of ablating planets orbiting nearby bright stars". Nature Astronomy. 4 (4): 408–418. arXiv:1912.10874. Bibcode:2020NatAs...4..408H. doi:10.1038/s41550-019-0973-y.
- Jones, Mark H.; Haswell, Carole A.; Barnes, John R.; Staab, Daniel; Heller, René (2020). "A possible transit of a disintegrating exoplanet in the nearby multiplanet system DMPP-1". arXiv:2005.07086 [astro-ph.EP].
- Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M⊕ super-Earth and two warm 14.7 and 10.2-M⊕ sub-Neptunes, 2020, arXiv:2002.01755v1
- exoplanet.eu Planet EPIC 249893012 d
- G 9-40 b
- GJ 180 d
- GJ 229 A c
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- www.sci-news.com Astronomers Discover Five New Planets around Nearby Red Dwarfs
- GJ 433 d
- GJ 1061 b
- GJ 1061 c
- GJ 1061 d
- GJ 1252 b
- exoplanet.eu Planet GJ 3082 b
- Hartman, J. D.; et al. (2020). "HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs". The Astronomical Journal. 159 (4): 173. arXiv:2002.05776. Bibcode:2020AJ....159..173H. doi:10.3847/1538-3881/ab7821.
- exoplanet.eu hats-48a b
- exoplanet.eu HD 80653 b
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- Open exoplanet catalogue HD 285507
- Nielsen, L.; et al. (2020). "Three Short Period Jupiters from TESS". arXiv:2003.05932 [astro-ph.EP].
- exoplanet.eu HIP 65A b
- Wong, Ian; et al. (2020). "Systematic Phase Curve Study of Known Transiting Systems from Year 1 of the TESS Mission". arXiv:2003.06407 [astro-ph.EP].
- exoplanet.eu Planet KELT-2019-BLG-1953 b
- Han, Cheongho; et al. (2020). "One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953". arXiv:2002.05310 [astro-ph.EP].
- exoplanet.eu Planet KELT-2019-BLG-1953 c
- Kepler-1661 b
- Socia, Quentin J.; et al. (2020). "Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary". The Astronomical Journal. 159 (3): 94. arXiv:2001.02840. Bibcode:2020AJ....159...94S. doi:10.3847/1538-3881/ab665b.
- exoplanet.eu L 168-9 b
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- TOI-132 b
- exoplanet.eu toi-257_b
- Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet; et al. (2020). "The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 System". arXiv:2001.00952 [astro-ph.EP].
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- exoplanet.eu toi-813_b
- 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.
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- exoplanet.eu LHS 1815 b
- Armstrong, David J.; et al. (2020). "A remnant planetary core in the hot Neptunian desert". arXiv:2003.10314 [astro-ph.EP].
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- exoplanet.eu toi-1130 b
- exoplanet.eu toi-1130 c
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