List of exoplanets discovered in 2020

Last updated

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.

NameMass (MJ)Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K)Discovery methodDistance (ly)Host star mass (M) Host star temp. (K)Remarks
2MASS J1155-7919 b 10582imaging330 [1] Very young Super-Jupiter on unusually wide orbit. [2]
HD 38677 b 18.57±0.010.1462±0.0012877radial vel.202.2169±3.2615641.21±0.036196±29DMPP-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
1239radial vel.202.2169±3.2615641.21±0.036196±29DMPP-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±0.0010.0422+0.0004
0.0003
1632radial vel.202.2169±3.2615641.21±0.036196±29DMPP-1 [3] Found by Dispersed Matter Planet Project looking for hot ablating planets.
HD 38677 e 5.516+0.002
0.004
0.0651±0.00051314radial vel.202.2169±3.2615641.21±0.036196±29DMPP-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±0.00051000radial vel.437.0495±13.046251.44±0.036500±100DMPP-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±0.0013854radial vel.159.4905±1.9569380.87±0.055138±99DMPP-3 [3] Found by Dispersed Matter Planet Project looking for hot ablating planets.
EPIC 249893012 b  [ ja ]0.02753±0.003430.174±0.0083.5951±0.00030.047+0.005
0.007
1616+150
80
transit1059.03±13.698571.05±0.055430±85 [5]
EPIC 249893012 c  [ ja ]0.04616±0.005950.3274+0.0152
0.0125
15.624±0.0010.13+0.01
0.02
990+68
29
transit1059.03±13.698571.05±0.055430±85 [5]
EPIC 249893012 d  [ ja ]0.03203+0.00774
0.00761
0.3515±0.011635.747±0.0050.22+0.02
0.04
752+69
37
transit1059.03±13.698571.05±0.055430±85 [5] [6]
G 9-40 b 0.18075.7460070.0385456transit91.10.2903348 [7]
Gliese 180 d 7.56±1.07106.341+0.261
0.34
0.31+0.024
0.029
radial vel.39.96±0.010.433371 [8]
Gliese 229 Ac 0.025122.005+0.364
0.382
0.339+0.024
0.029
radial vel.18.78±0.0040.583564 [9] [10]
Gliese 251 b >0.01314.2380.0818351radial vel.18.205±0.0060.360±0.0153451±51False positive in 2019, rediscovered in 2020 [11] [12]
Gliese 433 d 0.01936.052+0.045
0.031
0.178+0.013
0.015
radial vel.29.57±0.010.483600 [13] [14]
Gliese 1061 b 0.00431+0.00050
0.00047
3.204±0.0010.021±0.001radial vel.11.98±0.0030.12±0.012953±98 [15]
Gliese 1061 c 0.00547±0.000726.689±0.0050.035±0.001radial vel.11.98±0.0030.12±0.012953±98 [16]
Gliese 1061 d 0.00516+0.00076
0.00072
13.031+0.025
0.032
0.054±0.001radial vel.11.98±0.0030.12±0.012953±98 [17]
Gliese 1252 b 0.00658±0.001760.1064±0.00660.5182349+0.0000063
0.0000050
0.00916±0.000761089±69transit66.49±0.060.381±0.0193458+140
133
[18]
Gliese 3082 b  [ ja ]0.02759+0.011
0.01334
11.949±0.0220.079+0.006
0.007
radial vel.54.20.47 [19]
HATS-47b 0.3691.1173.9228852.9transit984.01±6.200.674 [20]
HATS-48Ab 0.2430.8003.13170.03769±0.00011954.6transit8650.72794546.0+23
18
[20] [21]
HATS-49b 0.3530.7654.1480834.8transit1058.70±7.180.7133 [20]
HATS-72b 0.12540.72247.3279739.3transit416.37±1.700.7311 [20]
HD 80653 b 0.0176±0.00140.1439±0.00630.719573±0.0000210.0166±0.0003transit358.1197±2.6418671.18±0.04 [22]
HIP 65 Ab  [ ja ]3.213±0.0782.03+0.61
0.49
0.9809761+0.000037
0.000034
0.01782±0.000211411±15transit201.85818±0.26092510.781±0.0274590±49an 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
microlensing23000+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
microlensing23000+3600
4300
0.31+0.37
0.17
[28] [27]
Kepler-1661(AB) b 0.053±0.0380.345±0.005175.06±0.060.633±0.005243transit1355.26±9.560.841±0.0225100±100 [29] [30]
L 168-9b  [ ja ]0.0145±0.001760.124±0.0081.4015±0.000180.02091±0.00024816±160transit82.02833±0.078277530.62±0.033800±70 [31]
OGLE-2018-BLG-0677Lb  [ ja ]0.0125+0.0185
0.0084
0.68+0.27
0.22
microlensing27000±35000.12+0.14
0.08
Milky way bulge [32]
TOI-132 b 0.07048+0.00598
0.00604
0.305±0.0122.1097019+0.000012
0.000011
0.026+0.002
0.003
1395+52
72
transit536.43±89.110.970±0.065397±46 [33]
TOI-257b  [ ja ]0.134±0.0230.626±0.01318.38827±0.000720.1523±0.00171033±19transit251.37±0.0651.38+0.056
0.009
6075±90Host star also called HD 19916. [34] [35] [36]
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
transit101.50.416±0.013480±135 [37]
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
transit101.50.416±0.013480±135 [37]
TOI-700 d 0.00711+0.0022
0.00164
0.1062±0.009837.426+0.0007
0.001
0.163±0.015295±55transit101.50.416±0.013480±135First "Earth sized" discovered by TESS [37] [38]
TOI-732 b 0.0980.1190.76838810.012892transit720.3793360Orbiting primary star of binary LDS 3977 [39] [40]
TOI-732 c 0.0270.20512.250.07673323transit720.3793360Orbiting primary star of binary LDS 3977 [39] [40]
TOI-813 b 0.599±0.03483.8911+0.0027
0.0031
0.423+0.031
0.037
610+28
21
transit864.8192±5.1563791.32±0.065907±150 [41]
TOI-1338 b 0.10382±0.06220.61±0.016995.20.4607724transit1301First circumbinary planet discovered by TESS [42]
HD 191939 b 0.3018.8804110.089778+58
41
transit1750.925400Host star also known as TOI-1339 [43]
HD 191939 c 0.28728.580600.178550±45transit1750.925400Host star also known as TOI-1339 [43]
HD 191939 d 0.28238.35610.216499+12
11
transit1750.925400Host star also known as TOI-1339 [43]
USco1621 b 1628802270imaging4500.363460 [44]
USco1556 b 1535002240imaging4590.333410 [44]
XO-7b 0.7091.3732.86414240.044211743transit7631.4056250 [45]
LHS 1815 b  [ ja ]0.0132±0.00470.0971±0.0053.81433±0.000030.0404±0.0094617±84transit970.5023643±142 [46] [47]
TOI-157 b  [ ja ]1.18±0.131.29±0.022.0845435±0.00000230.03138+0.00025
0.00020
1588+21
20
transit11710.948+0.023
0.018
5404+70
67
[23]
TOI 169 b  [ ja ]0.791+0.064
0.06
1.086+0.081
0.048
2.2554477±0.00000630.03524+0.00069
0.00079
1715+22
20
transit13451.147+0.069
0.075
5880+54
49
[23]
TOI-849 b 0.128±0.0080.308+0.014
0.011
0.7655240±0.00000270.01598±0.000131800transit7350.929±0.0235329±48 Neptunian Desert planet [48]
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
transit1200.76+0.16
0.1
5212+16
11
[49]
HD 332231 b 0.251±0.0170.867+0.027
0.025
18.70173±0.000280.1436+0.0032
0.0033
876±17transit2621.127±0.0776089+97
96
TOI 1456 [50] [51]
TOI-1130 b 0.3256±0.0094.066499±0.0000460.04394+0.00035
0.00038
876±17transit1900.684+0.16
0.17
4250±67 [52] [53]
TOI-1130 c 0.974+0.043
0.044
1.5+0.27
0.22
8.350381±0.0000330.07098+0.00056
0.0006
637±12transit1900.684+0.16
0.17
4250±67 [52] [54]
HD 79211 b 0.032±0.00524.45±0.020.141±0.005345radial vel.20.658±0.0050.64±0.074005±51Orbiting primary star of binary ADS 7251 [55]
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±11transit24221.394+0.07
0.049
6218+49
45
[56]
WASP-176 b 0.855+0.072
0.069
1.505+0.05
0.045
3.899052±0.000050.0535+0.001
0.0019
1721+28
21
transit18831.345+0.08
0.13
5941+77
79
[56]
TOI-1235 b 0.0217±0.000250.155±0.0073.444729+0.000031
0.000028
0.03845+0.00037
0.0004
754±18transit1290.640±0.0163872±70one more suspected planet in system [57]
OGLE-2017-BLG-0406 b 0.41±0.053.5±0.3microlensing17000±16000.56±0.074848High fidelity microlensing event [58]
TOI-421 b 0.051+0.004
0.003
0.461±0.01216.06815+0.00034
0.00035
0.1182+0.0026
0.0027
696.6±12.2transit244.3±1.90.852+0.029
0.021
5325+78
58
Also in system a red dwarf star at 2200 a.u. separation [59]
TOI-421 c 0.0222±0.00220.243±0.0175.19676+0.00049
0.00048
0.0557+0.0012
0.0013
1014.9+17.9
17.6
transit244.3±1.90.852+0.029
0.021
5325+78
58
Also in system a red dwarf star at 2200 a.u. separation [59]
HD108236 b 0.1415±0.00873.79523+0.00047
0.00044
0.0469±0.00171099+19
18
transit2110.975730±50 [60]
HD108236 c 0.1845+0.0089
0.0081
6.2037+0.00064
0.00052
0.0651±0.0024932+17
16
transit2110.975730±50 [60]
HD108236 d 0.2423±0.009714.1756+0.001
0.0011
0.1131±0.004708+13
12
transit2110.975730±50 [60]
HD108236 e 0.279+0.012
0.011
19.592±0.0020.14±0.0052636+12
11
transit2110.975730±50 [60]
WASP-148 b 0.291±0.0250.722±0.0558.80381±0.0000430.22±0.063940±80transit809±51.00±0.085460±130 [61] [62]
WASP-148 c 0.397+0.203
0.044
34.515±0.0290.359±0.086590±50radial vel.809±51.00±0.085460±130 [61] [62]
NGTS-11 b 0.37±0.140.823±0.03535.4553±0.00020.201±0.002440±40transit624±60.862±0.0285050±80 [63]
HIP 67522 b  [ ja ]0.250.894+0.048
0.047
6.9596+0.000016
0.000015
1174±21transit416±41.22±0.055675±75One more candidate planet around very young (age below 20 million years) star [64]
HD 63433 b  [ ru ]0.017±0.0097.10801+0.00046
0.00034
0.0710+0.0033
0.0041
transit73.08±0.070.99±0.035640±74 [65]
HD 63433 c  [ ru ]0.0230.238±0.0120.5455±0.0010.1531+0.0074
0.0092
transit73.08±0.070.99±0.035640±74 [65] [66]
HD 164922 d 0.013±0.00312.458±0.0030.103±0.003radial vel.72.1±0.90.874±0.0125293±32 [67]
OGLE-2006-BLG-284 b 0.45+0.14
0.40
2.2±0.8microlensing13000±49000.35+0.3
0.2
Binary host with 2.1 astronomical unit separation and uncertain, possibly unstable, planetary orbit. [68]
Wendelstein-1b 0.59+0.17
0.13
1.0314+0.00204
0.021
2.663416±0.0000010.0282±0.00091727+78
90
transit1004±100.65±0.13984+152
46
[69]
Wendelstein-2b 0.731+0.541
0.311
1.1592±0.00611.7522239±0.00000080.0234±0.00151852+120
140
transit1875±200.73±0.114288+133
111
Extended gaseous envelope [69]
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
transit3140±600.885471+115
37
Next expected transit in September 2020. [70]
K2-315b 0.085±0.0053.1443189±0.00000490.0234460±5transit185±10.174±0.0043300±30Also called the "Pi Earth" due its orbital period, or EPIC 249631677b [71]
TOI-1266 b  [ ja ]0.2193+0.074
0.066
10.894879+0.00007
0.00007
0.0745+0.0046
0.0069
410+21
15
transit117.4±1.00.437±0.0213563±77 [72]
TOI-1266 c  [ ja ]0.1492+0.077
0.095
18.80152+0.00054
0.00067
0.1037+0.0026
0.0025
347.1+7.9
8
transit117.4±1.00.437±0.0213563±77 [72] Possibly atmosphere of steam [73]
AU Microscopii b 0.180.3758.46321±0.000040.066transit32.3±0.30.313500±100 [74] [75] [76]
TOI-1728 b  [ ja ]0.084+0.017
0.016
0.450±0.0143.491510+0.000062
0.000057
0.0391±0.0009767±8transit198.2±0.50.646+0.023
0.022
3980+31
32
[77]
BD-11 4672 c 0.048±0.00974.2+0.06
0.08
0.30±0.01radial vel.88.63±0.110.651+0.031
0.029
4550±110Habitable zone, highly eccentric orbit. [78]
OGLE-2018-BLG-1269Lb 0.69+0.44
0.22
43834.61+1.70
1.17
microlensing8300+3000
2000
0.35+0.3
0.2
Very high fidelity event [79]
Lacaille 9352 b 0.0132±0.00199.262±0.0010.068±0.002468radial vel.10.721±0.0020.468±0.0123688±86 [80]
Lacaille 9352 c 0.0234±0.003821.789+0.004
0.005
0.120±0.004352radial vel.10.721±0.0020.468±0.0123688±86 [80]
HAT-P-58b 0.372±0.031.332±0.0434.0138379±0.00000240.04994±0.000441622±18transit1690±401.031±0.0286078±48 [81]
HAT-P-59b 1.540±0.0671.123±0.0134.1419771±0.00000120.05064±0.000371278±7transit871±41.008±0.0225678±16 [81]
HAT-P-60b 0.574±0.0381.631±0.0244.7947813±0.00000240.06277±0.000171772±12transit767±71.435±0.0126212±26 [81]
HAT-P-61b 1.057±0.070.899±0.0271.90231289±0.000000770.03010±0.000341505±16transit1120±201.004±0.0125587±45 [81]
HAT-P-62b 0.761±0.0881.073±0.0292.6453235±0.00000390.03772±0.000241512±13transit1150±201.023±0.0205629±48 [81]
HAT-P-63b 0.614±0.0241.119±0.0333.377728±0.0000130.04294±0.000351237±11transit1330±200.925±0.0235400+55
39
[81]
HAT-P-64b 0.58+0.18
0.13
1.703±0.074.0072320±0.00000170.05387±0.000301766+22
16
transit2135±201.298±0.0216457+55
36
[81]
TOI-1899 b 0.66±0.071.37+0.05
0.06
29.02+0.36
0.23
0.1587+0.067
0.075
362±7transit419±10.627+0.026
0.028
3841+54
45
[82]
HATS-37A b 0.099±0.0420.606±0.0164.33150.1587+0.067
0.075
1085+16
12
transit6950.843+0.017
0.012
5247±50One more red dwarf in system [83]
HATS-38 b 0.074±0.0110.614±0.01764.37500.1587+0.067
0.075
1294±10transit11310.890+0.016
0.012
5740±50 [83]
TYC 8998-760-1 c 6±11.1+0.6
0.3
3201240+160
170
imaging309.4±0.94783 [84]
HD 86226 c 0.023±0.0040.193±0.0073.98442±0.000180.049±0.0011311±28transit1491.019+0.061
0.066
5863±88 [85]
Gliese 2056 b 0.444±0.05369.971±0.0610.283±0.0013radial vel.92.80.62±0.08habitable zone [86]
Gliese 480 b 0.042±0.0059.567±0.0050.068±0.001radial vel.46.40.45±0.02 [86]
Gliese 687 c 0.050±0.013728±121.165±0.023radial vel.14.830.40±0.02Second Neptune sized planet discovered in this system [86]
HIP 107772 b  [ ja ]0.049+0.014
0.030
55.259+0.111
0.311
0.243+0.022
0.027
radial vel.77.10.63±0.08habitable zone [86]
HIP 38594 b  [ ja ]0.026+0.012
0.014
60.711+0.426
0.192
0.256+0.006
0.007
radial vel.58.00.61±0.02habitable zone [86]
HIP 38594 c 0.135+0.077
0.035
3525+541
572
3.842+0.399
0.441
radial vel.58.00.61±0.02 [86]
HIP 4845 b 0.053+0.016
0.028
34.151+0.17
0.09
0.177+0.016
0.020
radial vel.68.80.62±0.04 [86]
HIP 48714 b 0.071+0.023
0.020
17.819+0.004
0.009
0.112±0.003radial vel.34.30.58±0.02 [86]
TOI 824 b 0.058±0.0060.261+0.018
0.017
1.392978+0.000018
0.000017
0.02177±0.000321253+38
37
transit2080.69+0.009
0.007
4569±50 Neptunian Desert planet [87]
Proxima Centauri c 0.0179±0.0061928±201.489±0.04939+16
18
radial vel.4.244±0.0010.1221±0.00223042±117 [88] [89] Second planet discovered orbiting nearest star to the Solar System
TOI-763 b 0.031±0.0020.203±0.0105.6057±0.00130.0600±0.00061038±16transit3110.917±0.0285444±110 [90]
TOI-763 c 0.029±0.0030.235±0.01112.2737+0.0053
0.0077
0.1011±0.0010800±12transit3110.917±0.0285444±110 [90]
TOI-763 d 0.030±0.00547.7991±2.73990.2504+0.0093
0.0105
509±12radial vel.3110.917±0.0285444±110 [90]
TOI-561 b 0.0050±0.00110.127±0.0060.446578±0.0000170.01055±0.00008transit279.2±1.60.785±0.0185455+65
47
[91] [92]
TOI-561 c 0.017±0.0030.257±0.00910.779±0.0040.08809±0.0007transit279.2±1.60.785±0.0185455+65
47
[91] [92]
TOI-561 d 0.038±0.0040.226±0.01125.62±0.040.1569±0.0012transit279.2±1.60.785±0.0185455+65
47
[91] [92]
TOI-561 e 0.050±0.0070.238±0.01077.23±0.390.3274+0.0028
0.0027
transit279.2±1.60.785±0.0185455+65
47
[91]
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±20transit117.5±0.10.48±0.13570±100 [93]
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±16transit117.5±0.10.48±0.13570±100 [93]
Gl 414 A b 0.029+0.010
0.008
0.263+0.099
0.081
50.817+0.031
0.03
0.24±0.01303.7±32.5radial vel.38.80.650±0.084120±109Planets orbiting primary star of binary system [94]
Gl 414 A c 0.177+0.033
0.031
0.784+0.360
0.238
748.3+1.3
1.2
1.43±0.06123.3±13.2radial vel.38.80.650±0.084120±109Planets orbiting primary star of binary system [94]
TOI 837 b <1.20.768+0.091
0.072
8.3248762±0.0000157transit466.5±1.21.118±0.0596047±162Belongs to open cluster IC 2602 [95]
TOI-776 b 0.0147±0.00310.163±0.0108.24664+0.00009
0.00006
0.0652±0.0011513±12transit88.6±0.10.544±0.0283709±70 [96]
TOI-776 c 0.0192±0.00470.184±0.01215.6653+0.0008
0.0007
0.1000±0.0017415±10transit88.6±0.10.544±0.0283709±70 [96]
MOA-2009-BLG-319Lb 0.2077±0.02552.03±0.21microlensing22800±23000.514±0.063 [97]
TOI-481 b 1.53±0.030.99±0.0110.33111±0.000020.097±0.0011370±10transit5871.14+0.02
0.01
5735±72 [98]
TOI-892 b 0.95±0.071.07±0.0210.62656±0.000070.092±0.0051397±40transit11201.28+0.03
0.02
6261±80 [98]
GJ 3473 b 0.0059±0.00090.113±0.0041.1980035+0.0000018
0.0000019
0.01589±0.00062773+16
15
transit89.29±0.130.360±0.0163347±54Also called TOI-488 b [99]
GJ 3473 c 0.0233+0.0029
0.0027
15.509±0.0330.0876+0.0035
0.0034
329.1+6.6
6.4
radial vel.89.29±0.130.360±0.0163347±54Also called TOI-488 c [99]
NGTS-12b 0.208±0.0221.048±0.0327.532806±0.0000480.0757±0.00141257±34transit1474±251.021+0.056
0.049
5690±130 [100]
OGLE-2016-BLG-1928 0.001n/amicrolensing30000n/an/a Rogue planet [101]
LTT 9779 b  [ it ]0.092±0.0030.421±0.0210.792054±0.0000140.01679±0.00142000transit262.8±1.01.02+0.02
0.03
5499±50 Neptune desert planet [102]
TOI 540 b  [ ja ]0.081±0.0051.2391491±0.00000170.01223±0.00036611±23transit45.67±0.290.159±0.0143216±83 [103]
HD 238090 b 0.0217+0.0029
0.0030
13.671+0.011
0.010
0.0932±0.0011469.6+2.3
2.6
radial vel.49.68±0.030.578±0.0213933±51Orbiting primary star in binary system Gliese 458 [12]
TIC 237913194b 1.942+0.092
0.091
1.117+0.054
0.047
15.168865±0.0000180.1207±0.0037974transit1009±61.026+0.057
0.055
5788±80Very eccentric orbit [104]
EPIC 201170410 b 0.093416.79870.0349transit437+149
130
0.287+0.101
0.084
3648+172
143
[105]
EPIC 201757695 b 0.081012.04780.0296transit1880±1100.727+0.044
0.053
4520+108
54
[105]
OGLE-2018-BLG-0799Lb 0.22+0.19
0.06
1.27+0.45
0.29
microlensing160000.08+0.08
0.02
[106]
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
transit768.5±8.31.201+0.066
0.064
5710+53
49
[107]
EPIC 246193072 b 0.260+0.020
0.022
0.774+0.026
0.024
12.4551225±0.00000310.1016+0.0018
0.0019
650+53
70
transit760±90.912+0.048
0.049
5282+40
39
[107]
WASP-186 b 4.22±0.181.11±0.035.026799+0.000012
0.000014
0.0600+0.0012
0.0013
1348+23
22
transit913±111.22+0.07
0.08
6361+105
82
Also called TOI-1494 [108]
WASP-187 b 0.80±0.091.64±0.055.147878+0.000005
0.000009
0.0653±0.00131726+31
2
transit1224±211.54±0.096150+92
85
Also called TOI-1493 [108]
TOI 122b 0.028+0.029
0.010
0.243±0.0165.078030±0.0000150.0392±0.0007471transit202.9±0.70.312±0.0073403±100 [109]
TOI 237b 0.009+0.006
0.003
0.128±0.0115.436098±0.0000390.0341±0.0010388transit124.2±0.70.179±0.0043212±100 [109]
HAT-P-68b 0.724±0.0431.072±0.0122.29840551±0.000000520.02996+0.00043
0.00012
1027.8±8.2transit662±30.6785+0.0299
0.0079
4514±50 [110]
LP 714-47 b 0.097±0.0050.420±0.0274.052037±0.0000040.0417±0.0005700+19
24
transit171.8±0.40.59±0.023950±51Host star also known as G 160-62 or TOI 442, planet in Neptune desert [111]
CFHTWIR-Oph 98 B 7.8+0.7
0.8
1.86±0.042001800±40imaging447±130.0152320±40Very young superjovian planet orbiting a brown dwarf known as 2MASS J16274422-2358521 [112]
HD 190007 b 0.052±0.00511.72radial vel.41.47±0.030.77±0.024610±20 [113]
HD 216520 b 0.032±0.00335.45radial vel.63.77±0.030.82±0.045103±20 [113]
HD 216520 c 0.030±0.005154.43radial vel.63.77±0.030.82±0.045103±20 [113]
TOI-519 b <140.75±0.211.2652328±0.00000050.012±0.004760±54transit378±30.369+0.026
0.097
3350+100
200
Very faint 17-magnitude host star [114]
TOI-260 b 0.009+0.013
0.009
0.157±0.02713.478048±0.005188transit65.84±0.07Host star also called HIP 1532 and BD-10 47 [115]
TOI-784 b 0.031±0.0040.171±0.0152.797179±0.000158transit211±0.4Host star also called HD 307842 [115]
TOI-836 b 0.047±0.0110.224±0.0298.592004±0.002328transit89.73±0.10Host star also called HIP 73427 and CD-23 12010 [115]
TOI-836 c 0.018±0.0040.162±0.0243.816514±0.000757transit89.73±0.10Host star also called HIP 73427 and CD-23 12010 [115]
EPIC 201085153 b 0.214±0.0890.25722±0.000039transit3945±386Extremely tight orbit [116]
EPIC 201085153 c 0.125+0.179
0.125
2.259797±0.0008transit3945±386 [116]
EPIC 201427007 b 0.134±0.0180.72091±0.000067transit5633±111 [116]
EPIC 201595106 b 0.116±0.0090.877214±0.000087transit762±95820±20Candidate since 2018 [116]
EPIC 201650711 c 0.036±0.0075.544059±0.00016transit298.8±1.74310±92Ternary star system, and planet b unconfirmed [116]
EPIC 205152172 b 0.107±0.0180.980088±0.000026transit517±20.669±0.0164202±242Candidate since 2016 [116]
K2-299c 0.223±0.08014.648966±0.000031transit1219±165724±72Also known as EPIC 206024342 p2 [116]
K2-299d 0.152±0.0544.507464±0.0000077transit1219±165724±72Also known as EPIC 206024342 p3 [116]
K2-301c 0.152±0.0185.2986±0.00035transit1491±454114±99Also known as EPIC 206042996 p2 [116]
TOI-251b 0.245±0.0164.937770+0.000028
0.000029
0.05741+0.00023
0.00017
transit324.4±1.41.036+0.013
0.009
5875+100
190
[117]
TOI-942b 0.429±0.0184.324190±0.000030.04796+0.00073
0.00065
transit498±20.788+0.037
0.031
4928+125
85
[117] [118] 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
transit498±20.788+0.037
0.031
4928+125
85
[117] [118] Host star TYC 5909-319-1
K2-302c 0.089±0.0092.255438±0.000037transit359.3±3.53297±73Also known as EPIC 206215704 p2 [116]
K2-302d 0.098±0.0092.909216±0.000032transit359.3±3.53297±73Also known as EPIC 206215704 p3 [116]
EPIC 206298289 b 0.078±0.0090.434847±0.000022transit492±63875±157Candidate since 2016 [116]
K2-85 b 0.107±0.0090.684559±0.000026transit317.8±1.24427±48Also known as EPIC 210707130 p1 [116]
EPIC 210801536 b 0.088±0.0270.892592±0.00012transit5304±259Candidate since 2019, one more planet candidate in system [116]
EPIC 212624936 b 0.517+0.098
0.027
0.578657±0.000066transit5765±170 [116] Host star TYC 5557-667-1
EPIC 212624936 c 0.214+0.098
0.057
11.811437±0.00016transit5765±170 [116] Host star TYC 5557-667-1
K2-211c 0.116±0.0182.601404±0.000072transit895±140.882+0.019
0.027
5360±51 [116]
EPIC 220440058 b 0.125±0.0360.626683±0.00005transit3682±217One more planet candidate in system [116]
EPIC 220492298 b 0.085±0.0180.762406±0.00014transit5620±31 [116]
K2-282d 0.232±0.02727.248322±0.00047transit1638.22±25.340.94±0.045499±109 [116]
EPIC 228836835 b 0.089±0.0270.728113±0.00004transit491±63782±152 [116]
K2-106c 0.188±0.01813.334621±0.000068transit803±105613±39Candidate since 2017 [116]
Kepler-1514c 0.1049+0.0051
0.0039
10.514181±0.0000390.0997±0.00181066+16
14
transit12401.196+0.065
0.063
6145+99
80
[119]
OGLE-2017-BLG-1049Lb 5.53+3.62
2.87
3.92+1.10
1.32
microlensing18500+3600
4500
0.55+0.36
0.29
[120]
AU Microscopii c <0.0870.320±0.01418.858991±0.0000100.1101±0.0022454±16transit31.70.50±0.033700±100 [121] Precise radial velocities of giant stars
HD 25723 b 2.51456.781.49radial vel.3752.1±0.3Giant star host [122]
HD 25723 c 1.332369.844.35radial vel.3752.1±0.3Giant star host [122]
Chi Scorpii b 4.32+0.15
0.12
573.4±2.01.45±0.02radial vel.4081.09±0.154157±11Giant star host [122]
HD 60292 b 6.5±1.0495.4±3.01.5±0.1radial vel.1036±101.7±0.24348±28Giant star host [123]
HD 112640 b 5.0±1.0613.2±5.81.7±0.1radial vel.1065±61.8±0.24155±15Giant star host [123]
K2-111 c 0.0356±0.003515.6785+0.0064
0.0063
0.1166±0.0025radial vel.680±600.89±0.025730±50 [124]
K2-316b 0.1191.1330.0147841transit368EPIC 249384674b [125]
K2-316c 0.1635.2600.0582423transit368EPIC 249384674c [125]
K2-317b 0.2616.2200.0542432transit577EPIC 249557502b [125]
K2-318b 0.1487.0100.0911456transit483EPIC 249826231b [125]
K2-319b 0.24926.6800.1516641transit686EPIC 201663879b [125]
K2-320b 0.2341.9950.0142698transit356EPIC 201796690b [125]
K2-321b 0.1742.2980.0410701transit254EPIC 248480671b [125]
K2-322b 0.1718.2050.0594635transit404EPIC 248558190b [125]
K2-323b 0.18724.9300.1275318transit387EPIC 248616368b [125]
K2-324b 0.2173.2620.0331707transit447EPIC 248639308b [125]
K2-325b 0.1966.9300.0419423transit365EPIC 246074965b [125]
K2-326b 0.2031.2560.01981114transit928EPIC 246472939b [125]
KMT-2016-BLG-2397b 2.422.83microlensing160000.62+0.29
0.30
Multiple solutions for planetary parameters [126]
KMT-2016-BLG-2364b 3.932.63microlensing210000.50+0.40
0.22
[126]
OGLE-2017-BLG-1375b 10.332.97microlensing120000.77+0.27
0.23
Multiple solutions for planetary parameters [126]
OGLE-2017-BLG-0604b 0.514.06microlensing130000.70±0.28 [126]
KMT-2018-BLG-0748Lb 0.18+0.29
0.10
0.62±0.09microlensing240000.0870+0.138
0.047
[127]
KMT-2019-BLG-1339Lb 12.2+16.1
6.7
0.67+0.77
0.55
microlensing23000±30000.27+0.366
0.15
Multiple solutions for planetary parameters [128]
KMT-2019-BLG-2073  [ ja ]0.19microlensing12000Free-floating planet [129]
OGLE-2019-BLG-0551 0.0242microlensingPoorly characterized free-floating planet [130]
TVLM 513-46546 b 0.38±0.24221±50.3±0.0036astrometry34.90±0.070.092500 [131]
CD Ceti b  [ es ]0.0124+0.0013
0.0014
2.29070±0.000120.0185+0.0013
0.0013
464±18radial vel.28.070.161±0.0103130±51 [132]
OGLE-2018-BLG-0799Lb 0.22+0.19
0.06
1.27+0.45
0.29
microlensing160000.08+0.08
0.02
[133]
WD 1856+534 b 13.80.93±0.091.4079405±0.00000110.0204±0.0012transit80.737±0.1440.518±0.0554710±60Orbiting a white dwarf star [134]
Kepler-1649c 0.00380.095+0.014
0.010
19.53527±0.000100.0649234±20transit301.6±1.60.1977±0.00513240±61Habitable zone, Earth-like [135]
Kepler-305e 0.1603.20538transit2900±90 [136]
Kepler-385d 0.23356.4159transit4870±160 [136]
Kepler-598c 0.27086.4945transit2260±40FPP=1.0% [136]
Kepler-647c 0.35729.6663transit3660±70 [136]
Kepler-716c 0.1243.96999transit2110±30FPP=0.6% [136]
Kepler-783c 0.2087.05395transit1707±15 [136]
Kepler-1001c 0.1409.18186transit3110±80 [136]
Kepler-1085c 0.29156.7771transit4630±150 [136]
Kepler-1662b 0.2230.790134.4628transit [137] Host star also known as KOI-1783 [138]
Kepler-1663b 0.29417.6046transit1112±11Host star also known as KOI-252 [136]
Kepler-1664b 0.27014.3868transitHost star also known as KOI-349 [136]
Kepler-1665b 0.25311.9548transit1104±5Host star also known as KOI-650 [136]
Kepler-1666b 0.25725.8476transit4680±190Host star also known as KOI-945 [136]
Kepler-1666c 0.25725.8476transit4680±190Host star also known as KOI-945 [136]
Kepler-1667b 0.26683.5781transit2080±20Host star also known as KOI-1311 [136]
Kepler-1668b 0.38815.434transit4500±200Host star also known as KOI-1470 [136]
Kepler-1669b 0.2489.51216transit1800±40Host star also known as KOI-1475 [136]
Kepler-1670b 0.29920.4998transit7200±400Host star also known as KOI-1705 [136]
Kepler-1671b 0.1184.16787transit1176±7Host star also known as KOI-1738 [136]
Kepler-1672b 0.265150.878transit1189±14Host star also known as KOI-1822 [136]
Kepler-1673b 0.26233.7888transit2420±20Host star also known as KOI-1863 [136]
Kepler-1674b 0.28662.5611transit3400±100Host star also known as KOI-1892 [136]
Kepler-1675b 0.27963.0382transit2163±19Host star also known as KOI-1928 [136]
Kepler-1676b 0.30129.9221transitHost star also known as KOI-1943 [136]
Kepler-1677b 0.24122.064transit2250±30Host star also known as KOI-1984, FPP=0.6% [136]
Kepler-1678b 0.295147.974transit2830±70Host star also known as KOI-2066, FPP=0.5% [136]
Kepler-1679b 0.1849.75376transit3040±100Host star also known as KOI-2106 [136]
Kepler-1680b 0.1218.77424transit1020±5Host star also known as KOI-2120 [136]
Kepler-1681b 0.222769.8956transit2100±300Host star also known as KOI-2132 [136]
Kepler-1682b 0.25714.8334transit3900±160Host star also known as KOI-2229 [136]
Kepler-1683b 0.16715.0337transit2440±50Host star also known as KOI-2293 [136]
Kepler-1684b 0.25647.7055transit2060±40Host star also known as KOI-2417 [136]
Kepler-1685b 0.23020.4905transit3840±150Host star also known as KOI-2504 [136]
Kepler-1686b 0.1279.30987transit2430±30Host star also known as KOI-2559 [136]
Kepler-1687b 0.1475.77954transit1375±17Host star also known as KOI-2588 [136]
Kepler-1688b 0.1125.62012transit1850±380Host star also known as KOI-2733 [136]
Kepler-1689b 0.0848.483transit967±5Host star also known as KOI-2755 [136]
Kepler-1690b 0.250234.636transit2340±30Host star also known as KOI-2757 [136]
Kepler-1691b 0.1633.8482transit4290±110Host star also known as KOI-2802 [136]
Kepler-1692b 0.0995.95966transit1960±20Host star also known as KOI-2849 [136]
Kepler-1693b 0.11512.0999transit2530±50Host star also known as KOI-2871 [136]
Kepler-1694b 0.1053.89526transit1698±16Host star also known as KOI-2878, FPP=0.6% [136]
Kepler-1695b 0.0994.7329transit2640±40Host star also known as KOI-3048, FPP=0.5% [136]
Kepler-1696b 0.25065.9409transit5100±200Host star also known as KOI-3361 [136]
Kepler-1697b 0.11233.4969transit813±2Host star also known as KOI-3478 [136]
Kepler-1698b 0.0951.2107transit729±3Host star also known as KOI-3864 [136]
Kepler-1699b 0.1393.49082transitHost star also known as KOI-3933 [136]
Kepler-1701b 0.198169.134transit1940±20Host star also known as KOI-4054, [136] potentially habitable exoplanet
Kepler-1702b 0.14318.5012transit2860±90Host star also known as KOI-4386 [136]


Specific exoplanet lists

Related Research Articles

Exomoon Moon beyond the Solar System

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The Hungarian Automated Telescope Network (HATNet) project is a network of six small fully automated "HAT" telescopes. The scientific goal of the project is to detect and characterize extrasolar planets using the transit method. This network is used also to find and follow bright variable stars. The network is maintained by the Harvard-Smithsonian Center for Astrophysics.

HD 118203 is a star located in the northern circumpolar constellation of Ursa Major. It has the proper name Liesma, which means flame, and it is the name of a character from the Latvian poem Staburags un Liesma. The name was selected in the NameExoWorlds campaign by Latvia, during the 100th anniversary of the IAU.

Transiting Exoplanet Survey Satellite NASA space telescope designed to search for exoplanets

The Transiting Exoplanet Survey Satellite (TESS) is a space telescope for NASA's Explorers program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission. It was launched on April 18, 2018, atop a Falcon 9 rocket and was placed into a highly elliptical 13.7-day orbit around the Earth. The first light image from TESS was taken on August 7, 2018, and released publicly on September 17, 2018.

Kepler-1625 is a 14th-magnitude solar-mass star located in the constellation of Cygnus approximately 8,000 light years away. Its mass is within 5% of that of the Sun, but its radius is approximately 70% larger reflecting its more evolved state. A candidate gas giant exoplanet was detected by the Kepler Mission around the star in 2015, which was later validated as a likely real planet to >99% confidence in 2016. In 2018, the Hunt for Exomoons with Kepler project reported that this exoplanet has evidence for a Neptune-sized exomoon around it, based on observations from NASA’s Kepler Mission. Subsequent observations by the larger Hubble Space Telescope provided compounding evidence for a Neptune-sized satellite, with an on-going debate about the reality of this exomoon candidate.

K2-28 is a metal rich M4-type main sequence star. One confirmed transiting exoplanet is known to orbit this star. There is another star 5.2 arcseconds to the north–east of K2-28 however this star has a different proper motion and is therefore physically unrelated and probably a background star.

TOI 700 is a red dwarf 101.4 light-years away from Earth located in the Dorado constellation that hosts TOI 700 d, the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).

TOI 700 d is a near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf TOI 700, the outermost planet within the system. It is located roughly 101.4 light-years (31.1 pc) away from Earth in the constellation of Dorado. The exoplanet is the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).

TOI 1338 Binary star system in the constellation Pictor found in January 9th, 2020

TOI 1338 is a binary star system located in the constellation Pictor, about 1,320 light-years from Earth. It was discovered by the Transiting Exoplanet Survey Satellite (TESS) and is orbited by the circumbinary planet TOI 1338 b.

LTT 1445 Star system in the constellation Eridanus

LTT 1445 is a triple M-dwarf system about 22 light-years distant in the constellation Eridanus. The primary LTT 1445 A hosts two exoplanets- one discovered in 2019 that transits the star every 5.36 days, and another found in 2021 that transits the star every 3.12 days, close to a 12:7 resonance. As of August 2019 it is the second closest transiting exoplanet system discovered, with the closest being HD 219134 bc.

LTT 3780, also known as TOI 732 or LP 729-54, is the primary of the binary stellar system LDS 3977 in the constellation Hydra.

WASP-72 is the primary of a binary star system. It is an F7 class dwarf star, with an internal structure just on the verge of the Kraft break. It is orbited by a planet WASP-72b. The age of WASP-72 is younger than the Sun at 3.55±0.82 billion years.

KELT-1 is a F-type main-sequence star. Its surface temperature is 6518±50 K. It is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.008±0.073, but is much younger at an age of 1.75±0.25 billion years. The star is rotating very rapidly.

HD 175289 is a binary star system. Its primary star, also known as Kepler-410A, is a F-type subgiant star, orbited by the orange dwarf star Kepler-410B on a wide orbit. The companion star was discovered in 2012.

L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.623 ± 0.003 parsecs, or 34.648 ± 0.01 light-years, as measured by Gaia.

References

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