List of exoplanets discovered in 2018

Last updated

This List of exoplanets discovered in 2018 is a list of confirmed exoplanets that were first observed during 2018. [1]

Contents

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) [2] Discovery method Distance (ly) Host star mass (M) Host star temp. (K) Remarks
24 Boötis b 0.91+0.13
0.10
30.3506+0.0078
0.0077
0.190+0.012
0.009
radial vel.313.9±2.10.99+0.19
0.13
4893±15 [3]
40 Eridani Ab 0.0266±0.001542.378±0.0100.2190+0.0073
0.0078
radial vel.16.426±0.0420.78±0.085072±53 [4]
Barnard's Star b 0.0102±0.00130.122+0
0.122
232.8+0.38
0.41
0.404±0.018105±3radial vel.60.1443134 [5] Disproven candidate. In 2021, the existence of Barnard's star b was refuted. [6]
COROT-20c 17±11675+19
17
2.90±0.07radial vel.2819±801.14±0.086050±200 Brown dwarf (possibly) [7]
DE Canum Venaticorum b 12±34098.1±131.55.75±2.02timing99.64±0.090.51 [8]
Gamma Librae b 1.02±0.14415.2+1.8
1.9
1.24±0.10radial vel.154.7±2.91.47±0.204822±15 [3]
Gamma Librae c 4.58+0.45
0.43
964.6±3.12.17±0.10radial vel.154.7±2.91.47±0.204822±15 [3]
Gliese 15 Ac 0.1176005.4radial vel.11.60.383567 [9]
Gliese 96 b 0.06186+0.00761
0.00724
73.94+0.33
0.38
0.291±0.005radial vel.38.929±0.03020.60±0.073785±62 [10]
Gliese 143 b 0.09637+0.00827
0.00840
0.228±0.02835.589+0.006
0.005
0.1932±0.0002transit53.25±0.020.76+0.03
0.02
[11]
Gliese 1132 c 0.00831±0.001388.929±0.0100.0476±0.0017300±5radial vel.41.153±0.0230.181±0.0193270±140 [12]
Gliese 1265 b 0.023±0.0023.6511±0.00120.026±0.001radial vel.33.45±0.020.18±0.023236±51Host star also known as LP 819-052 [13]
Gliese 3779 b 0.025±0.0023.0232±0.00130.026±0.001radial vel.44.84±0.040.27±0.023324±51Host star also known as Ross 1020 [13]
HAT-P-11c 1.60+0.09
0.08
3407+360
190
4.13+0.29
0.16
radial vel.123.31±0.110.809+0.020
0.030
4780±50 [14]
HATS-39b 0.63±0.131.57±0.124.57763480.06007±0.000581645±43transit2910±2401.379±0.0406572±83 [15]
HATS-40b 1.59±0.241.58+0.16
0.12
3.26427360.04997±0.000742101±69transit4550±1101.561±0.0696460±130 [15]
HATS-41b  [ ru ]9.7±1.61.33+0.29
0.20
4.1936490.0583+0.0015
0.0010
1710+170
120
transit2457±471.496+0.115
0.078
6424±91 [15]
HATS-42b 1.88±0.151.40+0.25
0.14
2.29210200.03689±0.000651856+105
75
transit2672±351.273±0.0676060±120 [15]
HATS-54b 0.753±0.0571.015±0.0242.5441765±0.00000240.0370±0.0011429±24transit2350±301.05±0.055621±70 [16] Host star also known as NGTS-22 [17]
HATS-55b 0.9211.2514.20420010.054121367transit20341.206214 [16]
HATS-56b 0.6021.6884.3247990.060431902transit18821.576536 [16]
HATS-57b 3.1471.1392.35062100.034931413.4transit9131.035587 [16]
HATS-58Ab 1.031.0954.21808960.057981721transit16051.467175 [16]
HATS-59b 0.806±0.0691.126±0.0775.416081±0.0000160.06112±0.000761128±40transit2140±501.04±0.045670±91 [18]
HATS-59c 12.70±0.871422±142.504±0.035175.9±6.4radial vel.2140±501.04±0.045670±91 [18]
HATS-60b 0.662±0.0551.153±0.0533.560829±0.0000320.04708+0.00015
0.00023
1528±11transit1609±281.097+0.010
0.016
5688±20 [19]
HATS-61b 3.40±0.141.195±0.0677.817953±0.0000240.07908±0.000331226.1±7.3transit2262±291.08±0.015542±21 [19]
HATS-62b 0.179+0
0.179
1.055±0.0253.2768837±0.00000330.04163+0.00024
0.00016
1237±12transit1731±340.90+0.02
0.01
5416+19
13
[19]
HATS-63b 0.960±0.1201.207±0.0393.0566527±0.00000490.04026±0.000281398.3±9.0transit2070±200.93±0.025627±18 [19]
HATS-64b 0.960±0.2001.679±0.0814.908897±0.0000130.06562±0.000391793±27transit3640±1401.56±0.036554±27 [19]
HATS-65b 0.821±0.0831.501±0.0503.1051610±0.00000160.04497±0.000331634±18transit1631±411.26±0.036277±30 [19]
HATS-66b 5.33±0.681.411±0.0843.1414391±0.00000740.04714±0.000251998±21transit5040±1301.41±0.026625±35 [19]
HATS-67b 1.45±0.121.685±0.0471.6091788±0.00000400.03032±0.000152193±22transit3219±801.44±0.026594±33 [19]
HATS-68b 1.290±0.0591.232+0.039
0.029
3.5862202±0.00000470.05071±0.000181741±12transit2004±341.35±0.016147±22 [19]
HATS-69b 0.577+0
0.577
0.945±0.0222.2252577±0.00000190.03211+0.00014
0.00019
1295.7±6.9transit1368±11.70.89+0.01
-0.02
5137±16 [19]
HATS-70b 12.9+1.8
1.6
1.384+0.079
0.074
1.8882378±0.00000150.03632+0.00074
0.00087
2730+140
160
transit4263+196
202
0.81+0.50
0.33
1.08+0.16
0.14
[20]
HD 1397 b  [ id ]0.415±0.0201.026+0.025
0.027
11.53533+0.00079
0.00080
0.1097+0.0011
0.0013
1228.3+10.0
9.9
transit260.1211.324+0.042
0.046
5521±60 [21] [22]
HD 2685 b  [ id ]1.17±0.121.44±0.054.12688+0.00005
0.00004
0.0568±0.00062061±28transit645.72+2.77
2.28
1.43+0.05
0.04
6801±76 [23]
HD 4917 b 1.615±0.0921.224400.5±1.71.167±0.065radial vel.670.1±8.11.324802Two additional planets in system are suspected [24]
HD 13167 b 3.31±0.161.1672613±174.10±0.34radial vel.487.8±3.51.355671 [24] [25]
HD 14787 b 1.121±0.0691.250676.6±8.11.70±0.19radial vel.389.9±2.51.434946 [24]
HD 18015 b 3.18±0.231.1702278±713.87±0.32radial vel.405.2±2.61.495603 [24]
HD 23472 b 0.05638+0.00444
0.04405
0.179±0.00917.667+0.142
0.095
0.121±0.001543±18transit127.48±0.060.67±0.034684±99 [11] [26]
HD 23472 c 0.05405+0.00337
0.04333
0.167±0.01029.625+0.224
0.171
0.170±0.001467+19
18
transit127.48±0.060.67±0.034684±99 [11] [26]
HD 33142 c 5.97+1.04
0.80
834+29
24
radial vel.37.34±0.181.78±0.315009±15Marginal detection [24]
HD 55696 b 3.87±0.721827±103.18±0.18radial vel.255±11.29±0.206012 [27]
HD 72490 b 1.768±0.0801.218858±121.88±0.21radial vel.413.5±3.61.214934 [24]
HD 72490 c 4.5±1.23878±2615.22±0.58radial vel.224±201.26±0.254867 [24]
HD 89345 b 0.1100.66011.814300.10661089transit433.11.165576 [28] Host star also known as K2-234 [29]
HD 94834 b 1.26±0.171.2421576±762.74±0.18radial vel.321.0±2.11.114798 [24]
HD 98736 b 2.33±0.78968.8±2.21.864±0.091radial vel.106±0.20.92±0.135271 [27]
HD 125390 b 22.161756.23.16radial vel.5031.364850 [24]
HD 148164 b 1.23±0.25328.55±0.410.9930±0.0660radial vel.252±1.01.21±0.246032 [27]
HD 148164 c 5.16±0.825062±1146.15±0.50radial vel.252±1.01.21±0.246032 [27]
HD 148284 b 33.7±5.5339.331±0.0180.9740±0.0790radial vel.400±21.07±0.265572 [24] Brown dwarf [27]
HD 158996 b 14.0±2.3820.2±14.02.1±0.2radial vel.933±151.8±0.34069±30 [30]
HD 180053 b 2.194±0.0641.203213.72±0.470.843±0.063radial vel.448.7±2.01.755131 [24]
HD 180617 b 0.03839+0.00315
0.0044
105.9+0.09
0.1
0.3357+0.0099
0.01
radial vel.19.28±0.070.45±0.043557±51Planetary orbit partly in habitable zone [31]
HD 202772 Ab 1.017+0.070
0.068
1.545+0.052
0.060
3.308958±0.0000830.05208+0.00064
0.00068
2132+28
30
transit480.1+8.2
7.8
1.72+0.06
0.07
6272+77
71
[32]
HD 203473 b 7.8±1.11552.9±3.42.73±0.17radial vel.237±1.01.12±0.215780 [27]
HD 211810 b 0.670±0.4401558±222.656±0.043radial vel.211±0.41.03±0.025652 [27]
HD 215152 b 0.0057+0.0016
0.0020
5.7600+0.0016
0.0018
0.05764+0.00074
0.00076
radial vel.70.48±0.160.770±0.0154935±76 [33]
HD 215152 e 0.0091+0.0033
0.0047
25.197+0.048
0.051
0.1542±0.0020radial vel.70.48±0.160.770±0.0154935±76 [33]
HD 217850 b 21.6±2.63501.3±2.14.56±0.24radial vel.215±31.03±0.165544Likely a brown dwarf [27]
HD 219666 b 0.0552±0.00410.4202±0.01526.03607±0.000640.06356±0.002651073±20transit307.89±0.980.92±0.035527±65 [34] Host star also known as TOI-118 [35]
HD 220197 b 0.2017282.729radial vel.2100.915683 [36]
HD 233832 b 1.7820582.827radial vel.1920.714981 [36]
HD 238914 b 6.041005.7radial vel.9821.474769 [37]
IC 4651 9122 b 6.3±0.5734.0±8.12.038±0.039radial vel.2870±1102.19000 [38] Disputed [39]
K2-80d 0.228+0.025
0.012
28.8673+0.0051
0.0046
0.1778+0.0051
0.0055
transit658.7±5.70.90±0.085441±249 [25]
K2-138b 0.1402.353220.03380transit5970.935378 [40]
K2-138c 0.2253.559870.04454transit5970.935378 [40]
K2-138d 0.2375.404780.05883transit5970.935378 [40]
K2-138e 0.2948.261440.07807transit5970.935378 [40]
K2-138f 0.25112.757590.10430transit5970.935378 [40]
K2-141c 0.023+0
0.023
0.624+0.410
0.250
7.748500.06739+0.00089
0.00091
transit202.16±0.540.708±0.0284599±79 [41]
K2-155b 0.015+0.002
0.001
0.138+0.018
0.015
6.343650.0546+0.0013
0.0014
708+38
31
transit237.94±0.930.65+0.06
0.03
4258±150 [42]
K2-155c 0.020+0.005
0.002
0.174+0.024
0.020
13.854020.0946+0.0031
0.0030
583+52
35
transit237.94±0.930.65+0.06
0.03
4258±150 [42]
K2-155d 0.015+0.005
0.002
0.146+0.016
0.015
40.6835±0.00310.1937+0.0064
0.0059
381+47
25
transit237.94±0.930.65+0.06
0.03
4258±150 [42]
K2-156b 0.103+0.009
0.006
0.8131490.0149±0.00011347+18
19
transit492.0±3.50.66+0.02
0.01
4597±50 [43] [44]
K2-157b 0.0940.365257transit0.945456 [43] [44]
K2-158b 0.236+0.014
0.009
10.0605+0.0013
0.0015
0.0887±0.0008794±11transit647.1±6.70.92+0.03
0.02
5503+51
48
[43]
K2-158c 0.114+0.012
0.009
5.9028+0.0019
0.0023
0.0622±0.0006948±13transit647.1±6.70.92+0.03
0.02
5503+51
48
[45]
K2-159b 0.202+0.015
0.010
12.4221±0.00180.1013+0.0008
0.0009
684±8transit560.4±4.60.90+0.02
0.03
5425±44 [43]
K2-160b 0.284+0.019
0.013
3.7058710.04660+0.00037
0.00041
transit1038±150.983+0.023
0.025
5649±50 [43]
K2-161b 0.546+0.146
0.070
9.2831880.0861+0.0018
0.0023
transit3070±1600.987+0.082
0.060
4972±50 [43]
K2-162b 0.128+0.010
0.006
9.4589+0.0010
0.0011
0.0795±0.0006631±8transit407.3±2.00.75±0.024842+49
45
[43]
K2-163b 0.220+0.023
0.011
6.6731170.06509+0.00050
0.00060
transit684±140.826+0.019
0.023
4937±50 [43]
K2-164b 0.290+0.046
0.037
17.3551+0.0041
0.0038
0.1387+0.0036
0.0025
transit1238±251.181+0.093
0.061
5791±50 [43]
K2-165b 0.1137+0.0129
0.0087
2.354990.03262±0.00040transit440.6±3.90.835+0.031
0.030
5185±50 [43]
K2-165c 0.1386+0.0187
0.0098
4.382750.04935±0.00061transit440.6±3.90.835+0.031
0.030
5185±50 [43]
K2-165d 0.236+0.023
0.013
14.1014±0.00110.1076±0.0013transit440.6±3.90.835+0.031
0.030
5185±50 [43]
K2-166b 0.195+0.018
0.017
8.5272±0.00200.08583+0.00123
0.00076
transit1577±321.16+0.05
0.03
5960+52
53
[43]
K2-167b 0.252+0.046
0.040
9.9775±0.00100.0912+0.0036
0.0029
transit264.5±1.51.02+0.12
0.09
5908±50 [43]
K2-168b 0.191+0.018
0.012
15.8540±0.00140.1195+0.0013
0.0014
transit801±140.907+0.029
0.032
5554±50 [43]
K2-169b 0.1136+0.0096
0.0069
6.380800.06764+0.00063
0.00061
transit774±150.986+0.028
0.026
5548±50 [43]
K2-170b 0.127+0.018
0.012
7.5765+0.0018
0.0017
0.07457+0.00083
0.00086
transit1296±210.964±0.0325748±50 [43]
K2-170c 0.161+0.022
0.014
12.4000+0.0017
0.0019
0.1036+0.0011
0.0012
transit1296±210.964±0.0325748±50 [43]
K2-171b 0.240+0.036
0.030
5.6285+0.0017
0.0015
0.05960+0.00132
0.00062
transit2010±610.892+0.060
0.027
5250±50 [43]
K2-172b 0.1486+0.014
0.0085
14.3169±0.00140.1128+0.0010
0.0011
transit820.3±9.60.934+0.026
0.027
5569±50 [43]
K2-172c 0.286+0.017
0.012
29.6268±0.00160.1832+0.0017
0.0018
transit820.3±9.60.934+0.026
0.027
5569±50 [43]
K2-173b 0.1435+0.0143
0.0094
5.868700.06105+0.00078
0.00085
}
transit750.6±6.40.881+0.034
0.036
5580±70 [43]
K2-174b 0.2223+0.0157
0.0087
19.562740.1242±0.0013transit326.9±1.20.668+0.022
0.021
4500±50 [43]
K2-175b 0.182+0.032
0.024
9.5260+0.0012
0.0013
0.0906+0.0016
0.0011
transit812.2±9.11.095+0.057
0.039
5909±50 [43]
K2-176b 0.1330+0.0110
0.0083
5.329440.05846+0.00042
0.00052
transit812±120.939+0.020
0.025
5428±50 [43]
K2-177b 0.189+0.025
0.014
14.1552+0.0032
0.0030
0.1221+0.0011
0.0013
transit1628±421.211+0.032
0.038
6063±50 [43]
K2-178b 0.317+0.018
0.012
8.747820.08171+0.00066
0.00081
transit704.7±6.00.951+0.023
0.027
5525±50 [43]
K2-179b 0.224+0.015
0.011
5.172190.05488+0.00048
0.00060
transit625.7±6.90.824+0.022
0.027
5015±50 [43]
K2-180b 0.2150+0.0184
0.0098
8.865930.07550+0.00070
0.00075
transit668.9±5.70.730+0.020
0.022
5263±50 [43]
K2-181b 0.241+0.028
0.016
6.894250.07191+0.00055
0.00067
transit1189±171.044+0.024
0.029
5609±50 [43]
K2-182b 0.063±0.0160.2469+0.0152
0.0089
4.7368840.05223+0.00048
0.00064
transit507.2±4.10.847+0.024
0.031
5159±50 [43] [25] Confirmed in 2021. [46]
K2-183b 0.098±0.0900.4692690.011586+0.00010
0.000087
transit1083±140.942+0.021
0.025
5482±50 [43] [44]
K2-183c 0.224+0.024
0.012
10.793470.09371+0.00070
0.00083
transit1083±140.942+0.021
0.025
5482±50 [43] [25] [44]
K2-183d 0.227+0.025
0.013
22.6295+0.0018
0.0019
0.1535+0.0014
0.0012
transit1083±140.942+0.021
0.025
5482±50 [43] [25] [44]
K2-184b 0.1372+0.0134
0.0080
16.993440.1210+0.0014
0.0015
transit247.1±1.10.819+0.028
0.030
5252±50 [43] [25]
K2-185b 0.117+0.020
0.010
10.6166+0.0016
0.0018
0.09378+0.00088
0.00093
transit882±110.976+0.027
0.028
5722±50 [43]
K2-186b 0.283+0.024
0.015
41.4742+0.0033
0.0043
0.2359+0.0018
0.0021
transit1089±181.019+0.023
0.027
5784±50 [43]
K2-187b 0.1230.773981transit0.975477 [43] [25]
K2-187c 0.152+0.022
0.010
2.871790.03910+0.00034
0.00033
transit1089±190.967+0.025
0.024
5477±50 [43] [25]
K2-187d 0.287+0.045
0.022
7.149080.07182+0.00062
0.00061
transit1089±190.967+0.025
0.024
5477±50 [43] [25]
K2-187e 0.201+0.019
0.012
13.6083+0.0017
0.0016
0.11031+0.00096
0.00094
transit1089±190.967+0.025
0.024
5477±50 [43] [25]
K2-188b 0.112+0.015
0.010
1.742980.02932+0.000276
0.000225
transit1476±281.107+0.031
0.025
5982±50 [43] [25]
K2-188c 0.234+0.028
0.016
7.807600.07967+0.00075
0.00061
transit1476±281.107+0.031
0.025
5982±50 [43] [25]
K2-189b 0.1349+0.0136
0.0085
5.176300.05711+0.00049
0.00057
transit795.2±6.30.928+0.024
0.027
5503±50 [43] [25]
K2-189c 0.222+0.028
0.012
6.679340.06769+0.00058
0.00068
transit795.2±6.30.928+0.024
0.027
5503±50 [43] [25]
K2-190b 0.1210+0.0157
0.0091
10.098860.0884+0.0011
0.0012
transit526.5±3.70.905+0.033
0.036
5631±50 [43]
K2-190c 0.0975+0.0135
0.0082
21.5740+0.0057
0.0043
0.1467+0.0018
0.0020
transit526.5±3.70.905+0.033
0.036
5631±50 [43]
K2-191b {{0.141+0.024
0.012
2.858650.03807+0.00036
0.00040
transit944.5±7.80.901+0.026
0.028
5176±50 [43]
K2-192b 0.1405+0.0135
0.0099
4.163220.04840+0.00045
0.00058
transit727.9±5.90.873+0.024
0.031
5252±50 [43] [25]
K2-193b 0.358+0.031
0.018
14.787210.1177±0.0011transit1360±120.994+0.029
0.027
5623±50 [43] Low fidelity [25]
K2-194b 0.325+0.055
0.045
39.7214+0.0057
0.0056
0.2359+0.0032
0.0025
transit2090±611.110+0.046
0.035
5979±52 [43]
K2-195b 0.262+0.018
0.012
15.853540.1220+0.0012
0.0014
transit1037±140.963+0.028
0.031
5712±50 [43] [25]
K2-195c 0.230+0.024
0.013
28.4828+0.0064
0.0073
0.1803+0.0018
0.0020
transit1037±140.963+0.028
0.031
5712±50 [43]
K2-196b 0.321+0.054
0.045
48.3242+0.0085
0.0087
0.2730+0.0058
0.0036
transit1938±731.162+0.075
0.045
6045±50 [43]
K2-197b 0.223+0.017
0.010
8.357950.07992+0.00068
0.00080
transit813.4±7.80.975+0.025
0.029
5675±50 [43] Low fidelity [25]
K2-198b 0.367+0.023
0.015
17.043180.1221±0.0014transit361.7±2.80.836±0.0295262±50 [43]
K2-199b 0.022±0.0060.1679+0.0167
0.0079
3.2254230.03804+0.00043
0.00042
transit351.8±2.00.706+0.024
0.023
4681±50 [43] [25] [46]
K2-199c 0.039±0.0070.253+0.015
0.010
7.374500.06601+0.00075
0.00074
transit351.8±2.00.706+0.024
0.023
4681±50 [43] [25] [46]
K2-200b 0.1217+0.0128
0.0094
2.849880.03741+0.00033
0.00040
transit603.7±6.10.860+0.023
0.027
5233±50 [43]
K2-201b 0.1249+0.0120
0.0069
1.0597900.02004+0.00014
0.00015
transit649.2±5.40.956+0.020
0.021
5507±50 [43]
K2-201c 0.293+0.036
0.016
22.7799+0.0020
0.0019
0.1549+0.0011
0.0012
transit649.2±5.40.956+0.020
0.021
5507±50 [43]
K2-202b 0.205+0.016
0.011
3.405160.04387+0.00044
0.00042
transit988.2±8.70.971+0.030
0.028
5491±58 [43]
K2-203b 0.122+0.025
0.011
9.6951±0.00130.08238+0.00112
0.00098
transit544.5±5.10.794+0.033
0.028
5000±50 [43]
K2-204b 0.272+0.039
0.033
7.055780.07222+0.00074
0.00066
transit1914±581.009+0.031
0.027
5755±50 [43]
K2-205b 0.178+0.024
0.021
26.6723+0.0042
0.0037
0.1718+0.0023
0.0022
transit1337±300.951+0.038
0.036
5890±50 [43]
K2-206b 0.249+0.020
0.014
18.2945+0.0017
0.0016
0.1256+0.0016
0.0015
transit803±100.789+0.030
0.028
5043±50 [43]
K2-207b 0.232+0.033
0.019
12.4875±0.00120.1033±0.0010transit1196±180.942±0.0285522±50 [43]
K2-208b 0.150+0.015
0.011
4.190950.04957+0.00053
0.00054
transit844±100.925±0.0305582±50 [43]
K2-209b 0.0775+0.0094
0.0056
2.080620.02891+0.00033
0.00032
transit250.05±0.990.745+0.026
0.024
4720±50 [43]
K2-210b 0.0730+0.0090
0.0062
0.5702330.01305+0.00011
0.00014
transit578.6±6.00.912+0.023
0.029
5396±50 [43]
K2-211b 0.1226+0.0154
0.0091
0.6695580.01436+0.00011
0.00015
transit895±140.882+0.019
0.027
5221±50 [43] Another planet discovered in 2020 [44]
K2-212b 0.2135+0.0127
0.0082
9.795400.07648+0.00082
0.00075
transit357.3±3.00.622+0.020
0.018
4349±50 [43] [25]
K2-213b 0.135+0.027
0.019
8.1309±0.00180.08093+0.00138
0.00099
transit1285±231.070+0.055
0.038
5794±50 [43]
K2-214b 0.198+0.034
0.023
8.596530.08273+0.00083
0.00076
transit989±141.022+0.031
0.028
5768±50 [43] [25]
K2-215b 0.189+0.023
0.014
8.269650.08003+0.00070
0.00073
transit1333±211.000+0.026
0.027
5704±50 [43]
K2-216b 0.1497+0.0090
0.0068
2.1747890.02916+0.00031
0.00032
transit377.8±2.30.699±0.0234591±50 [43] [25]
K2-217b 0.319+0.062
0.043
14.074520.1179+0.0016
0.0013
transit1259±251.103+0.046
0.037
5967±50 [43]
K2-218b 0.229+0.025
0.014
8.679890.08395+0.00082
0.00075
transit1299±321.048+0.031
0.028
5757±50 [43]
K2-219b 0.120+0.018
0.016
3.90129}}0.04885+0.00054
0.00048
transit1071±161.022+0.034
0.030
5753±50 [43]
K2-219c 0.128+0.019
0.017
6.6677+0.0013
0.0016
0.06982+0.00077
0.00070
transit1071±161.022+0.034
0.030
5753±50 [43]
K2-219d 0.230+0.032
0.029
11.137280.09830+0.00108
0.00097
transit1071±161.022+0.034
0.030
5753±50 [43]
K2-220b 0.198+0.023
0.013
13.682510.11043+0.00099
0.00112
transit766.7±8.90.960+0.026
0.029
5599±50 [43]
K2-221b 0.1498+0.0149
0.0085
2.399090.03520+0.00028
0.00029
transit1049±221.011+0.024
0.025
5716±50 [43]
K2-222b 0.0252±0.00570.210±0.00715.388830.1190+0.0016
0.0015
transit331.4±2.00.950+0.040
0.036
5934±50 [43] [25] [47]
K2-223b 0.0812+0.0088
0.0066
0.5055700.012664+0.000080
0.000081
transit651.3±8.31.06±0.025835+38
40
[43]
K2-223c 0.144+0.010
0.006
4.564170.05491±0.00035transit651.3±8.31.06±0.025835+38
40
[43]
K2-224b 0.139+0.014
0.012
4.478590.05422+0.00034
0.00035
1002±11transit904.8±9.60.91±0.025620+42
45
[43]
K2-224c 0.215+0.014
0.011
10.0949+0.0012
0.0011
0.08858+0.00065
0.00066
764±9transit904.8±9.60.91±0.025620+42
45
[45]
K2-225b 0.311+0.023
0.018
15.8715+0.0017
0.0021
0.13385+0.00140
0.00072
902±13transit1179±191.27+0.02
0.04
5742+49
47
[43]
K2-226b 0.137+0.012
0.008
3.271110.04133+0.00047
0.00048
1120±16transit693±110.88±0.035424+48
46
[43]
K2-227b 0.149+0.109
0.016
13.6218+0.0032
0.0033
0.1098+0.0011
0.0012
transit613.9±6.70.951+0.028
0.030
5673±50 [43]
K2-228b 0.108+0.009
0.005
2.698370.0338±0.0003914+14
13
transit423±130.71±0.024715+48
46
[43]
K2-229b 0.0082±0.00140.102+0.005
0.003
0.5842490.012888±0.000131818+14
15
transit335.5±3.50.87±0.015315+25
31
[43]
K2-229c 0.067+0
0.067
0.181+0.011
0.005
8.328010.0769±0.0003750±6transit335.5±3.50.87±0.015315+25
31
[43] [45]
K2-230b 0.175+0.016
0.014
2.860640.0409+0.0003
0.0002
1529±22transit1791±471.11±0.025945+23
25
[43]
K2-231b 0.22±0.0213.8419±0.00140.1132±0.0011transit1057±141.01±0.035695±50 [48]
K2-232b 0.398±0.0371.000+0.022
0.020
11.1684590.10356+0.00081
0.00077
1001±14transit427.9±2.51.188+0.028
0.026
6154±60 [49] [50]
K2-233b 0.1247+.0055
0.0054
2.467460.03317+0.00044
0.00045
1040+28
26
transit220.60±0.910.800±0.0324950±100 [51]
K2-233c 0.1191+0.0074
0.0069
7.061420.06687728+20
19
transit220.60±0.910.800±0.0324950±100 [51]
K2-233d 0.236±0.01024.3662±0.00210.1527+0.0020
0.0021
482+14
13
transit220.60±0.910.800±0.0324950±100 [51]
K2-236b 0.085+0.044
0.040
0.546±0.00919.492130.148±0.004886±17transit595.7±4.21.18+0.03
0.04
6025±100 [52] First exoplanet discovered by scientists based in India.
K2-237b 1.60±0.111.65+0.07
0.08
2.180560.037±0.0021884+37
36
transit1036±231.28+0.03
0.04
6257±100 [53] [54] Also called EPIC 229426032 b
K2-238b 0.86+0.13
0.12
1.30+0.15
0.14
3.204660.046±1587+75
76
transit22000+13000
50000
1.19±0.085630±78 [53] Also called EPIC 246067459 b
K2-239b 0.0044±0.00130.098±0.0095.240±0.0010.0441±0.0008502+22
18
transit101.48±0.270.40±0.013420±18 [55]
K2-239c 0.0028±0.00090.089±0.0097.775±0.0010.0576±0.0009427+24
19
transit101.48±0.270.40±0.013420±18 [55]
K2-239d 0.0041±0.00130.098±0.00910.115±0.0010.0685±0.0012399+18
15
transit101.48±0.270.40±0.013420±18 [55]
K2-240b 0.016+0.002
0.001
0.18+0.02
0.01
6.034±0.0010.0513±0.0009586+24
18
transit238.3±1.70.58±0.013810±17 [55]
K2-240c 0.014+0.002
0.001
0.16+0.03
0.01
20.523±0.0010.1159±0.0020389+19
17
transit238.3±1.70.58±0.013810±17 [55]
K2-241b 0.227+0.016
0.009
26.8199±0.00250.1567+0.0007
0.0008
507±5transit489.6±3.50.71±0.015262+43
39
[45]
K2-242b 0.227+0.019
0.017
6.513890.0494±0.0004416±8transit357.4±2.00.38±0.013459+65
38
[45]
K2-243b 0.194+0.012
0.011
11.5418+0.0027
0.0022
0.1087±0.00141035+36
35
transit877±111.29+0.04
0.06
6570+269
171
[45]
K2-243c 0.179+0.013
0.012
24.9460+0.0049
0.0056
0.1817+0.0022
0.0024
801+27
28
transit877±111.29+0.04
0.06
6570+269
171
[45]
K2-244b 0.156+0.012
0.009
21.0688+0.0032
0.0033
0.1418+0.0010
0.0011
638±7transit698.6±7.80.86±0.025677+38
39
[45]
K2-245b 0.387+0.017
0.012
11.893070.0959±0.0006923±14transit1507±280.83+0.02
0.01
5793+66
52
[45]
K2-246b 0.311+0.022
0.019
5.769180.0602±0.0004977+19
18
transit2341±890.87±0.025610+32
29
[45]
K2-247b 0.189+0.017
0.014
2.250210.0304±0.0004979+52
51
transit848.1±6.70.74±0.034667+305
183
[45]
K2-247c 0.195+0.022
0.021
6.4942+0.0026
0.0025
0.0615±0.0008688+36
35
transit848.1±6.70.74±0.034667+305
183
[45]
K2-248b 0.229+0.018
0.012
7.1726+0.0015
0.0014
0.0699±0.0010886+19
18
transit1341±160.88+0.04
0.03
5528+97
86
[45]
K2-249b 0.249+0.024
0.020
12.4090+0.0034
0.0028
0.1151+0.0030
0.0031
1061±66transit1726±551.32+0.09
0.12
6504+329
419
[45]
K2-250b 0.218+0.017
0.013
4.014570.0459±0.0005958+14
13
transit1369±210.80+0.03
0.02
5172+46
44
[45]
K2-251b 0.210+0.023
0.019
9.3008+0.0033
0.0032
0.0694±0.0005437±9transit481.6±3.40.52±0.013717+85
50
[45]
K2-252b 0.155+0.015
0.011
13.8151+0.0046
0.0045
0.1041+0.0008
0.0007
639±7transit751.3±6.80.79+0.02
0.01
5152+41
39
[45]
K2-253b 1.130+0.062
0.054
4.001670.0506+0.0010
0.0011
1238+57
53
transit2933±951.08+0.05
0.08
6027+221
240
[45]
K2-254b 0.145+0.025
0.021
4.096390.0448±0.0005791±26transit747.8±4.20.71+0.02
0.03
4629+168
123
[45]
K2-254c 0.195+0.021
0.016
12.1184+0.0030
0.0032
0.0923±0.0010551±18transit747.8±4.20.71+0.02
0.03
4629+168
123
[45]
K2-255b 0.259+0.025
0.010
1.964170.0274±0.00031034±17transit628.4±5.00.71±0.034676+63
61
[45]
K2-256b 0.235+0.022
0.019
5.5201+0.0024
0.0028
0.0578±0.0008845±28transit1871±490.84+0.03
0.04
5219+179
136
[45]
K2-257b 0.074+0.005
0.004
1.605880.0216±0.0002789±14transit209.14±0.840.52±0.013725+80
46
[45]
K2-258b 0.268+0.019
0.018
19.0921+0.0058
0.0063
0.1490+0.0025
0.0026
{831±30transit2201±371.21+0.05
0.08
6351+198
228
[45]
K2-259b 0.207+0.018
0.015
15.4804+0.0033
0.0039
0.1271+0.0010
0.0011
795±13transit1374±271.14±0.036059+62
76
[45]
K2-260b 1.42+0.31
0.32
1.552+0.048
0.057
2.62666570.0404+0.0013
0.0016
1957+78
77
transit2206±631.39+0.05
0.06
6367±250 [56]
K2-261b 0.223±0.0310.850+0.026
0.022
11.633440.102+0.019
0.020
1080+110
100
transit699.9±6.41.10+0.01
0.02
5537±71 [56]
K2-263b 0.0466±0.00980.215±0.01150.818947±0.0000940.2573±0.0029470±10transit532±40.88±0.035368±44 [57]
K2-264b 0.203+0.018
0.014
5.839770+0.000061
0.000063
489+12
13
transit609±70.47±0.013580±70 [58] [59]
K2-264c 0.247+0.018
0.016
19.663650+0.000303
0.000306
326+8
9
transit609±70.47±0.013580±70 [58] [59]
K2-265b 0.0206±0.00260.153±0.0102.369172±0.0000890.03376±0.00021transit454±30.912±0.025477±27 [60] [61]
K2-266b 0.0356+0.0346
0.0205
0.29+0.16
0.12
0.658524±0.0000170.01306+0.00020
0.00021
1515±18transit251.7+1.95
1.92
0.686±0.0334285+49
57
[62]
K2-266c 0.00091+0.00053
0.00035
0.0629+0.0086
0.0076
7.8140+0.0019
0.0016
0.0679±0.0011664.5+8.0
7.7
transit251.7+1.95
1.92
0.686±0.0334285+49
57
[62]
K2-266d 0.0296+0.0091
0.0063
0.261+0.012
0.011
14.69700+0.00034
0.00035
0.1035+0.0016
0.0017
538.3+6.5
6.3
transit251.7+1.95
1.92
0.686±0.0334285+49
57
[62]
K2-266e 0.0261+0.0085
0.0057
0.244+0.012
0.010
19.4820±0.00120.1249+0.0019
0.0020
490.1+5.9
5.7
transit251.7+1.95
1.92
0.686±0.0334285+49
57
Two more planets are suspected [62]
K2-267b 3.0+1.1
1.2
1.051±0.0446.180235±0.0000140.07229+0.00074
0.00075
1401±16transit1098+27
26
1.317+0.041
0.040
6202+52
50
Unconfirmed, host star also known as EPIC 246851721 [63]
K2-268b 0.126±0.0122.151894+0.000393
0.000363
0.0308±0.00021121±14transit1081.1±10.270.84±0.025068±51 [25]
K2-268c 0.240±0.0219.326841+0.001532
0.001617
0.0819±0.0006688±8transit1081.1±10.270.84±0.025068±51 [25]
K2-269b 0.140±0.0114.144965+0.000817
0.000619
0.0531±0.00061429±37transit1180.1±47.01.16±0.046209±88 [25]
K2-270b 0.123±0.0101.543069+0.000189
0.000185
0.0247±0.00021203±17transit924.75±7.600.85±0.024877±58 [25]
K2-270c 0.263±0.0144.400028+0.000169
0.000178
0.0497±0.0004848±12transit924.75±7.600.85±0.024877±58 [25]
K2-271b 0.649±0.0218.562421±0.0001270.0770+0.0008
0.0009
893±17transit1863.9±44.320.83±0.035644±71 [25]
K2-272b 0.260±0.01314.453533+0.001328
0.001360
0.1081+0.0016
0.0017
655±12transit1391.3±17.30.81±0.045419±79 [25]
K2-273b 0.394±0.11411.716332+0.001172
0.001198
0.0974±0.0011672±11transit1013.0±9.390.90±0.035200±67 [25]
K2-274b 0.196±0.01114.129714+0.0021022
0.001876
0.1064+0.0009
0.0008
589±9transit1013.0±9.390.81±0.025065±60 [25]
K2-275b 0.200±0.0113.280961+0.000112
0.000107
0.0400±0.0003905±13transit404.73±2.280.79±0.024812±59 [25]
K2-275c 0.209±0.0098.438756+0.000269
0.000271
0.0750±0.0005660±9transit404.73±2.280.79±0.024812±59 [25]
K2-276b 0.336±0.01918.718269+0.003153
0.003008
0.1291±0.0011583+10
9
transit1597.8±23.90.82±0.025139±62 [25]
K2-277b 0.185±0.0116.326763+0.000355
0.000361
0.0675±0.0006958±14transit370.29±2.281.02±0.035741±65 [25]
K2-278b 0.266±0.0213.334966+0.000701
0.000859
0.0488±0.00091711±101transit2622.7±53.71.40±0.086747±383 [25]
K2-279b 0.108±0.0127.122605+0.001647
0.001601
0.0670+0.0008
0.0009
879±14transit599.48±5.150.79±0.035558±70 [25]
K2-280b 0.684±0.02319.895202+0.000774
0.000753
0.1488+0.0019
0.0020
744±15transit1294.5±2.381.11±0.045742±90 [64] [25] [65] [43]
K2-281b 0.730±0.0198.687721+0.000151
0.000150
0.0773±0.0008665±12transit1520.2±23.60.82±0.034812±72 [25]
K2-282b 0.252±0.0124.169836+0.000279
0.000300
0.0499+0.0006
0.0007
1057±20transit1638.2±25.30.95±0.045523±82 [25] Two more planets discovered in 2019 and 2020 [44]
K2-283b 0.314±0.0141.921036+0.000051
0.000053
0.0291±0.00031186±20transit1331.5±15.70.89±0.035060±70 [25]
K2-284b 0.248+0.012
0.011
4.795069±0.0000860.04771±0.00025653+16
14
transit351.0±1.60.63±0.014140±50Very young host star [66]
K2-285b 0.03046+0.00381
0.00431
0.231±0.0053.471745+0.000044
0.000046
0.03817+0.00095
0.00092
1088.9+22.1
21.9
transit508±40.83±0.024975±95 [67]
K2-285c 0.04933+0.00717
0.00670
0.315±0.0077.138048+0.000072
0.000063
0.0824±0.0018741.4±14.5transit508±40.83±0.024975±95 [67]
K2-285d 0.020±0.0200.221±0.00510.45582+0.00025
0.00023
0.1178±0.0029619.9+12.7
12.5
transit508±40.83±0.024975±95 [67]
K2-285e 0.0337+0
0.0337
0.174±0.00414.76289+0.00065
0.00061
0.18041+0.00420
0.00430
500.9+10.1
9.9
transit508±40.83±0.024975±95 [67]
K2-287b 0.315±0.0270.847±0.01314.893291±0.0000250.1206±0.0008804+8
7
transit518.7±4.21.06±0.025695±58 [68]
K2-292b 0.0771±0.01380.235+0.010
0.009
16.9841±0.00080.13±0.01795+33
28
transit372.76+2.67
2.64
1.00±0.035725±65Host star also known as HD 119130 [69]
K2-295b 0.335±0.062{0.897+0.011
0.005
4.024867±0.0000150.0451+0.0006
0.0014
852+14
6
transit736.1±7.80.74±0.044444±70 [54]
K2-311b 131.11±0.073650+1280
1130
4.5±1.0183+25
18
transit1826.480.90±0.094898±68 [70]
Kepler-730c 0.140±0.0122.8518833800.03997+0.00089
0.00069
1607+27
29
transit6590+254
267
1.05+0.07
0.05
5620+55
59
[71]
Kepler-1654b 0.819+0.019
0.017
1047.8356+0.0018
0.0019
2.026+0.037
0.035
206.0+3.7
3.5
transit1884±131.011+0.056
0.052
5597+95
93
[72]
Kepler-1655b 0.016+0.010
0.009
0.1974±0.007311.872903960.103±0.001transit699.9±3.21.03±0.046148±71Similar to a mini-Neptune [73]
Kepler-1656b 0.153+0.013
0.012
0.448±0.04731.5786590.197±0.021651+51
47
transit610±31.03±0.045731±60Highly eccentric orbit [74]
Kepler-1657b 1.93+0.19
0.21
0.990+0.060
0.070
141.241671±0.0000860.534+0.012
0.030
347±12transit3090±801.01+0.07
0.16
5830±100Also called KOI-3680 b in Exoplanet Archive [75]
KMT-2016-BLG-1397Lb 7.00+5.20
4.30
5.1+1.5
1.7
microlensing22000+3600
4200
0.45+0.33
0.28
[76]
KMT-2016-BLG-1820Lb 4.57+5.03
2.14
1.08+0.22
0.24
microlensing20420+3720
4170
0.039+0.043
0.018
[77]
KMT-2016-BLG-2142Lb 15.49+24.99
8.58
0.830+0.150
0.200
microlensing7010+1010
1160
0.0730+0.1170
0.0400
[77]
KPS-1b 1.090+0.086
0.087
1.03+0.13
0.12
1.7062910.0269±0.00101459±56transit863.3±8.50.892+0.090
0.100
5165±90First transiting exoplanet found by an amateur astronomer [78]
LHS 1140 c 0.00569±0.001230.1144±0.00213.777931±0.0000030.02675±0.00070438±9transit40.67±1.370.18±0.013216±39 [79]
MOA-2011-BLG-291Lb 0.057+0.107
0.038
0.69±0.24microlensing14000±46000.15+0.27
0.10
[80]
MOA-2015-BLG-337Lb  [ ja ]0.1060+0.4059
0.0730
0.24+0.06
0.09
microlensing23000+3600
3300
0.00940+0.03590
0.00650
[81]
MOA-2016-BLG-319Lb 0.620+1.160
0.330
0.950+0.170
0.200
microlensing22000+3900
4600
0.15+0.28
0.08
[82]
NGTS-2b 0.74+0.13
0.12
1.595+0.047
0.045
4.511164±0.0000610.0630+0.0024
0.0030
1468+45
42
transit1174+27
25
1.64+0.19
0.22
6478+94
89
[83] Also known as WASP-179b [84]
NGTS-3Ab 2.38±0.261.48±0.371.67537280.023+0.007
0.005
transit2480±361.017±0.0935600±150 [85]
NGTS-4b  [ it ]0.0648±0.00940.284±0.0231.3373508±0.00000800.019±0.0051650±400transit921.7±5.90.75±0.025143±100 [86]
OGLE-2011-BLG-0173Lb 0.19+0.18
0.11
8microlensing20000+4200
5500
0.41+0.30
0.21
[87] Not the planetary candidate OGLE-2017-BLG-0173Lb!
OGLE-2014-BLG-1722Lb 0.17+0.16
0.10
1512+3715
1029
1.9+1.3
0.8
microlensing20900+4200
5900
0.40+0.36
0.24
3500+1490
470
[88]
OGLE-2014-BLG-1722Lc 0.26+0.27
0.16
2283+7021
1589
2.5+2.2
1.1
microlensing20900+4200
5900
0.40+0.36
0.24
3500+1490
470
[88]
OGLE-2015-BLG-1670Lb 0.0563+0.0302
0.0277
2.62+0.58
0.60
microlensing22000+3300
4200
0.55±0.28 [89]
OGLE-2016-BLG-1067Lb 0.431.7microlensing12165.6330.3 [90]
OGLE-2017-BLG-0373Lb 0.40+0.64
0.26
2768+3343
1704
2.42+0.76
0.78
microlensing19200+4200
6400
0.25+0.27
0.13
3250+500
300
[91]
OGLE-2017-BLG-0482Lb 0.0283+0.028
0.014
1972+1306
2322
1.8+0.6
0.7
microlensing18900+5900
6800
0.20+0.20
0.10
3150+350
300
[92]
OGLE-2017-BLG-1140Lb 1.59+0.35
0.26
819+253
218
1.02±0.15microlensing113000.211+0.032
0.025
3170+60
50
[93]
OGLE-2017-BLG-1522Lb 0.75+1.26
0.40
780+728
431
0.59+0.12
0.11
microlensing3200+3000
1800
0.045+0.076
0.024
1500+1000
500
[94]
OGLE-2017-BLG-1434Lb 0.014±0.002968±691.18±0.10microlensing2800±2900.234±0.0263220+30
70
[95] Planet confirmed in 2021 [96]
PDS 70b 8.0±6.0>1.34350022imaging369.96±1.700.76±0.023972±36 [97]
Pi Mensae c 0.0152+0.0026
0.0027
0.1822±0.00456.26790±0.000460.06839±0.000501169.8+2.8
4.3
transit59.62±0.0731.094±0.0396037±45 [98]
Qatar-7b 1.88±0.251.70±0.03{2.0320460±0.00000970.0352±0.0002transit2364.63371.409±0.0266387±38 [99]
TCP J05074264+2447555 b 0.0289±0.02080.5microlensing12000.25±0.18 [100] Also known as Kojima-1Lb [101]
TYC 3318-1333-1 b 3.42±0.35562.0+4.1
4.0
1.414±0.063radial vel.1622±331.19±0.144776±10 [37]
UKIRT-2017-BLG-001Lb 1.28+0.37
0.44
3468+2324
1300
4.18+0.96
0.88
microlensing20500+5200
6800
0.81+0.21
0.27
5100+700
1300
[102]
WASP-134b 1.40±0.0810.14980.0956±0.0025953±22transit636±70.81±0.045700±100 [103]
WASP-134c 0.70±0.0770.01±0.14radial vel.636±70.81±0.045700±100 [103]
WASP-137b 0.681±0.0541.27±0.113.9080284±0.00000530.0519±0.00181601±65transit943±131.216±0.0666100±140 [103]
WASP-143b 0.725±0.0841.234±0.0423.7788730±0.00000320.0490±0.00141325±30transit1310±201.087±0.0455900±140 [103]
WASP-144b 0.44±0.060.85±0.052.2783152±0.00000130.0316±0.00051260±40transit1170±340.81±0.045200±140 [104]
WASP-145Ab 0.89±0.040.90±0.401.7690381±0.00000080.0261±0.00051200±60transit298±0.80.76±0.044900±150 [104]
WASP-146b 1.11±0.151.228±0.0763.3969440±0.00000360.0451±0.00241486±43transit1610±901.057±0.0856100±140 [103]
WASP-147b 0.275+0.028
0.027
1.115+0.140
0.093
4.602730±0.0000270.0549+0.0012
0.0013
1404+69
43
transit1390±461.044+0.070
0.073
5702±100 [105]
WASP-158b 2.79±0.231.07±0.153.656333±0.0000040.0517±0.00181590±80transit1740±411.38±0.146350±150 [104]
WASP-159b 0.55±0.081.38±0.093.840401±0.0000070.0538±0.00151850±50transit2382±361.41±0.126120±140 [104]
WASP-160Bb 0.278+0.044
0.045
1.090+0.047
0.041
3.7684952±0.00000350.0452±0.00121119+25
23
transit926±169.750±2.2805298±99 [105]
WASP-161b 2.49±0.211.143+0.065
0.058
5.4060425±0.00000480.0673±0.00231557+34
29
transit1130±141.39±0.146400±100 [106] Proper name Isli
WASP-162b 5.2±0.21.00±0.059.62468±0.000010.0871±0.0013910±20transit1023±130.95±0.045300±100 [104]
WASP-163b 1.87±0.211.202±0.0971.6096884±0.00000150.0266±0.00141638±68transit858±120.97±0.155500±200 [106]
WASP-164b 2.13+0.12
0.13
1.128+0.041
0.043
1.7771255±0.00000280.02818+0.00065
0.00072
1610+58
53
transit1050±230.9460+0.0670
0.0710
5806+190
200
[105]
WASP-165b 0.658+0.097
0.092
1.26+0.19
0.17
3.465509±0.0000230.04823+0.00091
0.00092
1624+93
89
transit1900±1101.248+0.072
0.070
5599±150 [105]
WASP-166 b 0.101±0.0050.63±0.035.443540±0.0000040.0641±0.00111270±30transit368.551.19±0.066050±50 [107] [108] [109]
WASP-168b 0.42±0.041.5+0.5
0.3
4.153658±0.0000030.0519±0.00081340±40transit1000±61.08±0.056000±100 [104]
WASP-170b 1.6±0.21.096±0.0852.34478022±0.000003600.0337±0.00181422±42transit1005±120.93±0.155600±150 [106]
WASP-172b 0.47±0.101.57±0.105.477433±0.0000070.0694±0.00111740±60transit1780±501.49±0.076900±140 [104]
WASP-173Ab 3.69±0.181.20±0.061.38665318±0.000000270.0248±0.00061880±55transit235±5.81.05±0.085800±140 [104] Also known as KELT-22Ab [110]
WASP-174b 1.3+0
1.3
1.34.2337000.05591490transit13501.306400 [111]
WASP-190b 1.0±0.11.15±0.095.367753±0.0000040.0663±0.00081500±50transit1796.3231.35±0.056400±100 [112]
Wolf 503b  [ ru ]0.020±0.0020.1811+0.0068
0.0065
6.00118+0.00008
0.00011
0.0571±0.0020805±9transit145.4±0.30.688+0.023
0.016
4716±60 [113] [114]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

Related Research Articles

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 Center for Astrophysics | Harvard & Smithsonian.

<span class="mw-page-title-main">Ruprecht 147</span> Dispersed open cluster

Ruprecht 147 or NGC 6774 is a dispersed star cluster in the Milky Way galaxy. It is about 1,000 light years away, which is close to Earth in comparison with other such clusters. In late summer, it can be seen with binoculars in the constellation of Sagittarius. The stars, bound by gravity, are about 2.5 to 3.25 billion years old. The cluster, discovered in 1830 by John Herschel, was sometimes thought to be an asterism due to its sparseness and location against the background of the richest part of the Milky Way, and also since the brightest stars in this old cluster perished long ago. In 1966 the Czech astronomer Jaroslav Ruprecht classified it as a type III 2 m open cluster under the Trumpler scheme. It received otherwise little attention until 2012, when it was identified as a potentially important reference gauge for stellar and Galactic astrophysics research, particularly the research of Sun-like stars.

GJ 9827 is a star in the constellation of Pisces. It is a K-type main-sequence star with an apparent magnitude of 10.250. It is 97 light-years away, based on parallax.

<span class="mw-page-title-main">HATS-36b</span> Extrasolar planet in the constellation Sagittarius

HATS-36b is a gas giant exoplanet that orbits an F-type star. Its mass is 3.216 Jupiters, it takes 4.2 days to complete one orbit of its star, and is 0.05425 AU from it. It was discovered on June 12, 2017 and was announced in 2018. Its discoverers were 23, namely Daniel Bayliss, Joel Hartman, George Zhou, Gaspar Á. Bakos, Andrew Vanderburg, J. Bento, L. Mancini, S. Ciceri, Rafael Brahm, Andres Jordán, N. Espinoza, M. Rabus, T. G. Tan, K. Penev, W. Bhatti, M. de Val-Borro, V. Suc, Z. Csubry, Th. Henning, P. Sarkis, J. Lázár, I. Papp, P. Sári.

K2-58 is G-type main-sequence star in the constellation of Aquarius, approximately 596 light-years from Solar System. The star is metal-rich, having 155% of Solar abundance of elements heavier than helium. The star is located in the region allowing to see Venus transiting the Sun for hypothetical observer located in K2-58 system.

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.

<span class="mw-page-title-main">K2-18</span> Red dwarf star in the constellation Leo

K2-18, also known as EPIC 201912552, is a red dwarf star with two planetary companions located 124 light-years from Earth, in the constellation of Leo.

<span class="mw-page-title-main">V1298 Tauri</span> Star in the constellation Taurus

V1298 Tauri is a young weakly-lined T Tauri star that is part of the Taurus-Auriga association in the Taurus Molecular Cloud. Alternatively it is part of a proposed moving group, called Group 29 that is slightly older. The system has four transiting exoplanets, discovered with the Kepler space telescope in the K2 mission. One of the planets was discovered in August 2019 and the other three were discovered in November 2019 by the same team.

HAT-P-29, also known as Muspelheim since 2019, is a star about 1,040 light-years away. It is a G-type main-sequence star. The star's age of 2.2±1.0 billion years is less than half that of the Sun. HAT-P-29 is slightly enriched in heavy elements, having 35% more iron than the Sun.

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.

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.

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