List of exoplanets discovered in 2019

Last updated

This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019. [1] [2]

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) [3] Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
7 Canis Majoris c 0.87996.002.153radial vel.64.61.344826 [4]
Beta Pictoris c 912002.7radial vel.64.431.76 [5]
DS Tucanae Ab 0.509±0.0158.138268±0.000011850transit143.89±0.221.01±0.065428±80 [6]
Epsilon Indi Ab 3.251651011.5564.25radial vel.11.870.75 [7]
G 9-40 b 0.18075.7460070.0385456transit91.10.2903348 [8] [9]
Gliese 49 b 0.0177+0.0021
−0.0021
13.8508+0.0053
−0.0051
0.0905±0.0011radial vel.32.145±0.010.515±0.0193805±51 [10]
Gliese 357 b 0.005790.10863.930720.035525transit30.800.3423505 [11]
Gliese 357 c 0.01079.12470.061401.2radial vel.30.800.3423505 [11]
Gliese 357 d 0.01955.6610.204219.6radial vel.30.800.3423505Potentially habitable exoplanet [11]
Gliese 378 b  [ id ]0.04097±0.0063.822±0.0010.082±0.002radial vel.48.790.56±0.013879±67 [12]
Gliese 411 b 0.00941±0.0014512.9532±0.0079349.83±0.32radial vel.8.2840.386±0.0393563±60 [13] Host star also known as Lalande 21185
Gliese 685 b 0.028+0.0053
−0.0057
24.160+0.061
−0.047
0.1344+0.0052
−0.0051
radial vel.46.71020.3816±0.0690.55±0.06 [14]
Gliese 686 b 0.022±0.00315.53209+0.00166
−0.00167
0.091±0.004379+24
−25
radial vel.26.612±0.0080.42±0.053663±68 [15]
Gliese 3512 b 0.463203.590.3380radial vel.30.950.1233081 [16]
Gliese 4276 b 0.05213+0.00296
−0.00299
13.352±0.0030.082±0.002radial vel.69.6±0.10.41±0.033387±51May be two planwts in 2:1 orbital resonance [17]
HAT-P-69b  [ id ]3.581.6764.78694910.065551930transit11221.657394 [18]
HAT-P-70b  [ id ]<6.781.872.744324520.047394000transit10731.898450 [18] [19]
HD 8326 b  [ id ]0.210±0.062158.991±1.4400.533±0.011radial vel.100.20.80±0.054914+51
−32
[20]
HD 13724 b 26.77+4.40
−2.20
14763.405+4901.655
−1599.795
12.40+2.60
−0.90
radial vel.141.9±0.170.76±0.715868±27 [21]
HD 15337 b 0.0236+0.0034
−0.0032
0.146±0.0054.75615±0.000170.0522±0.00121001.0±11.5transit146.36±0.230.90±0.035125±50Host star also known as TOI-402 [22]
HD 15337 c 0.0255+0.0057
−0.0053
0.213±0.01117.1784±0.00160.1268±0.0038642±10transit146.36±0.230.90±0.035125±50Host star also known as TOI-402 [22]
HD 21411 b 0.207±0.08184.288±0.1270.362±0.007radial vel.±95.110.89±0.055605+247
−132
[20]
HD 21749 b 0.073+0.007
−0.006
0.254+0.023
−0.020
35.61253+0.00060
−0.00062
0.1915+0.0058
−0.0063
422+15
−14
transit53.261±0.0230.73±0.074640±100 [23]
HD 21749 c <0.01160.0796+0.0057
−0.0052
7.78993+0.00051
−0.00044
0.0695+0.0021
−0.0023
701+25
−23
transit53.261±0.0230.73±0.074640±100 [23]
HD 24085 b 0.0371±0.00982.0455±0.00020.034±0.001radial vel.179.41.22±0.076034+32
−53
[20]
HD 25015 b 4.48+0.30
−0.28
6019.320+679.365
−262.980
6.19+0.45
−0.23
radial vel.122.2±0.220.86±0.055160±63 [21]
HD 39855 b 0.027±0.0053.2498±0.00040.041±0.001radial vel.75.930.87±0.055576+50
−46
[20]
HD 64114 b 0.0560±0.011045.791±0.0700.246±0.005radial vel.102.90.95±0.055676+32
−87
[20]
HD 65216c 1.295±0.062577.6±1.3281.301±0.020radial vel.114.7±0.10.95±0.015718±8Rediscovered in 2019 after false positive in 2013 [24]
HD 85628 Ab 1.675±0.2411.515±0.0442.8240932±0.00000460.0474±0.00131865±25transit560±31.75±0.057800±200Host star also known as MASCARA-4 [25] [26] [27]
HD 92788 c 3.67+0.30
−0.25
11611.2975+5055.06
−905.820
10.50+2.90
−0.55
radial vel.113.13851.15±0.075744±24 [28]
HD 92987 b 16.88+0.69
−0.65
10354.8375+551.5275
−270.2850
9.62+0.36
−0.26
radial vel.142.2±0.221.08±0.065770±36 [21] [29]
HD 97048 b 2.5130imaging6032.410000Discovered using study of disk kinematics. [30]
HD 102843 b 0.3584±0.04563090.942±295.0494.074±0.270radial vel.205.050.95±0.055436+144
−69
[20]
HD 103949 b 0.0352±0.0072120.878±0.4460.439±0.009radial vel.86.500.77±0.044792+66
−54
[20]
HD 181234 b 8.37+0.34
−0.36
7462.0575+80.3550
−76.7025
12.40+2.60
−0.90
radial vel.155.9±0.421.01±0.065386±60 [21]
HD 202696 b 1.996+0.220
−0.100
517.8+8.9
−3.9
1.566+0.016
−0.007
radial vel.618.3±5.21.91+0.09
−0.14
5040+71
−85
[31]
HD 202696 c 1.864+0.177
−0.227
946.6+20.7
−20.9
2.342+0.034
−0.035
radial vel.618.3±5.21.91+0.09
−0.14
5040+71
−85
[31]
HD 206255 b 0.108±0.02296.045±0.3170.461±0.009radial vel.245.91.42±0.085635+82
−99
[20]
HD 210193 b 0.4817±0.0733649.918±8.5991.487±0.031radial vel.137.81.04±0.065790+38
−50
[20]
HD 211970 b 0.0409±0.007925.201±0.0250.143±0.003radial vel.42.40.61±0.044127+149
−94
[20]
HD 213885 b 0.0278+0.0021
−0.0020
0.1557+0.0045
−0.0046
1.008035+0.000021
−0.000020
0.02012+0.00015
−0.00012
transit156.45721±0.45661891.068+0.020
−0.018
5978±50A transiting 1-day-period super-Earth with an Earth-like composition around a bright (V=7.9) star unveiled by TESS [32]
HD 213885 c 0.06277+0.00434
−0.00428
4.78503+0.00056
−0.000051
0.056798+0.00044
−0.00032
1265.4+7.3
−8.4
radial vel.156.45721±0.45661891.068+0.020
−0.018
5978±50 [32]
HD 221416 b 0.190±0.0180.836+0.031
−0.028
14.2767±0.00370.1228+0.00025
−0.00026
transit310.09311.212±0.0745080±90Host star also known as TOI-197 or HIP 116158 [33]
HD 221420 b 9.70+1.10
−1.00
22482+4200
−4100
18.5±2.3radial vel.101.7±0.121.67±0.115830±44 [29]
HIP 35173 b 0.0400±0.008541.516±0.0770.217±0.004radial vel.108.250.79±0.054881+55
−81
[20]
HIP 54373 b 0.02712±0.005797.760±0.0030.063±0.001radial vel.61.090.57±0.034021+226
−146
[20]
HIP 54373 c 0.03914±0.0066415.144±0.0080.0990±0.0020radial vel.61.090.57±0.034021+226
−146
[20]
HIP 71135 b 0.0592±0.012987.190±0.3810.335±0.007radial vel.105.50.66±0.044146+107
−110
[20]
HIP 79098 (AB)b 20.5±4.5345±62450±150imaging477.2±8.23.75±1.25 Brown dwarf [34]
HR 858 b 0.1860+0.0061
−0.0057
3.58599±0.000150.0480+0.0010
−0.0011
1572+22
−19
transit104.351.145+0.074
−0.080
6201±50 [35]
HR 858 c 0.1730±0.00625.97293+0.00060
−0.00053
0.0674+0.0014
−0.0016
1326+18
−16
transit104.351.145+0.074
−0.080
6201±50 [35]
HR 858 d 0.1931+0.0077
−0.0074
11.2300+0.0011
−0.0010
0.1027+0.0022
−0.0025
1075+15
−13
transit104.351.145+0.074
−0.080
6201±50 [35]
HR 5183 b 3.232700018171radial vel.102.71.075794Exoplanet found with one of the most elliptical orbits as of 2019 [36]
K2-32e 0.0901+0.0089
−0.008
4.34882+0.00069
−0.00075
0.04951±0.00055transit516.6±4.20.856±0.028With a radius almost identical to that of the Earth it is almost certainly a terrestrial planet [37]
K2-43c 0.2162.1988841093.7transit5980.573841 [38]
K2-50c 0.089+0.011
−0.01
3.96151+0.00046
−0.00051
transit845.82±10.630.61±0.06 [39]
K2-63c  [ ru ]0.35±0.1125.4556±0.00470.189±0.011transit524.414±211.40±0.256771±303Unconfirmed
K2-133e  [ ru ]0.154+0.012
−0.012
26.5841+0.0018
−0.0017
0.1346±0.0011296±10transit245.3±0.70.46±0.013655±80 [40] Host star also known as LP 358-499
K2-146c 0.023580.1954.004981093.7transit2590.333385 [41]
K2-166c 0.109+0.019
−0.015
3.80464+0.00091
−0.00105
transit1568.81+31.64
−29.03
1.07±0.03 [39]
K2-168c  [ ru ]0.105+0.012
−0.009
8.0468+0.0024
−0.0025
transit800.91±13.670.91±0.03 [38] [39]
K2-198c 0.12703.35960551229.9transit3620.805213 [38]
K2-198d 0.21757.4500177943.2transit3620.805213 [38]
K2-282c 0.132+0.012
−0.009
0.70531±0.00005transit1638.22±25.340.94±0.045499±109 [39] 3rd planet discovered in 2020 [42]
K2-286b  [ ru ]0.0214±0.01350.1873±0.017827.359±0.0050.1768+0.0175
−0.0205
347+21
−11
transit248.9±0.80.64±0.023926±100 [43]
K2-288Bb 0.17±0.0331.393463+0.000067
−0.000069
0.164±0.030226.36±22.30transit214.3±2.80.33±0.023341±276 [44]
K2-290b  [ ru ]0.06640.273±0.0149.21165+0.00033
−0.00034
0.0923±0.00661230±38transit897±121.19+0.07
−0.08
6302±120 [45] Two planets on a retrograde orbit [46]
K2-290c  [ ru ]0.774±0.0471.006±0.05048.36685+0.00041
−0.00040
0.0923±0.0066676±16transit897±121.19+0.07
−0.08
6302±120 [45] Two planets on a retrograde orbit [46]
K2-291b 0.0204±0.00360.1418+0.0085
−0.0064
2.225177+0.000066
−0.000068
0.03261±0.00044transit295±20.93±0.045520±60 [47]
K2-293b  [ ru ]0.219+0.031
−0.022
13.1225+0.0011
−0.0012
750+170
−50
transit1290±220.96+0.04
−0.03
5532±78 [48]
K2-294b  [ ru ]0.148+0.019
−0.017
2.50387+0.00022
−0.00023
1425+79
−54
transit1230±200.99+0.03
−0.03
5612±50 [48]
K2-296b 0.167+0.018
−0.04
28.1656+0.0027
−0.0028
transit521.78±4.570.41+0.11
−0.05
Host star also known as EPIC 201238110 [39]
K2-297b 0.062+0.005
−0.004
2.13174±0.00022transit831.31±5.480.78+0.09
−0.17
Host star also known as EPIC 201497682 [39]
K2-298b 0.098+0.012
−0.011
4.16959+0.00051
−0.00053
transit1441.42±26.650.8+0.08
−0.16
[39]
K2-299b  [ ru ]0.152+0.053
−0.028
4.50756+0.00062
−0.0006
transit1219.21±16.280.93+0.08
−0.1
5724±72 [39] Two more planets in star system discovered in 2020 [42]
K2-300b  [ ru ]0.09+0.021
−0.012
2.87814+0.00023
−0.00026
transit528.67±5.870.22+0.04
−0.06
[39]
K2-301b  [ ru ]0.145+0.015
−0.017
5.29711+0.00074
−0.0007
transit1491.42±44.980.56±0.054114±99 [39]
K2-302b  [ ru ]0.08+0.017
−0.018
2.25372±0.00047transit359.49±3.520.41+0.1
−0.08
[39] Two more planets in system discovered in 2020 [42]
K2-303b  [ ru ]0.086+0.01
−0.013
1.58252+0.00017
−0.00018
transit1034.57±9.590.71+0.09
−0.03
[39]
K2-304b 0.118+0.007
−0.008
2.28943±0.00019transit1380.78±23.940.83+0.09
−0.12
[39]
K2-305b 0.194+0.06
−0.037
18.0983+0.006
−0.0058
transit2030.88±33.921.11+0.14
−0.12
[39]
K2-306b 0.143+0.012
−0.014
34.885+0.011
−0.01
transit931.54±6.690.91+0.04
−0.16
[39]
K2-307b 0.1+0.011
−0.008
15.2841+0.0037
−0.0029
transit1053.09±20.650.98+0.04
−0.03
6004+77
−78
[39] Two more planets in system are suspected, [49] second planet in system confirmed in 2021 [50]
K2-308b 0.884±0.0873.38628±0.00002transit1.09±0.096100±263 [51]
K2-310b 0.2307±0.011213.6030±0.00130.0980±0.0040536±18transit1133.220.690±0.0384684±79 [52]
K2-310c 0.2400±0.013065.5500±0.00890.280±0.006316±10transit1133.220.690±0.0384684±79 [52]
KELT-23Ab 0.938+0.048
−0.044
1.323±0.0252.255251+0.000011
−0.000012
0.03302+0.00068
−0.00064
1561±20transit409.07±1.140.94+0.06
−0.05
5899±49 [53]
KELT-24b 5.181.2725.55149260.069691459transit313.21.466509
Kepler-47d 0.05984+0.07501
−0.03672
0.628+0.059
−0.044
187.366+0.069
−0.051
0.6992+0.0031
−0.0033
transit49000.957+0.013
−0.015
Kepler-65e 0.653+0.056
−0.055
258.8+1.5
−1.3
0.362±0.007radial vel.999.3±8.81.25±0.066211±66
Kepler-82f 0.0658±0.003175.732±0.0120.3395±0.0041timing3026.640.91±0.035401±108
Kepler-88d 3.15±0.151409+14
−13
2.45±0.02radial vel.1243±71.022+0.023
−0.026
5513±67 [54]
Kepler-411d 0.0478±0.01600.2961±0.009358.02035±0.000560.279±0.004410±10transit500.94±1.570.87±0.04 [55]
Kepler-411e 0.0340±0.003531.509728±0.0000850.186±0.003503±9timing500.94±1.570.87±0.04 [55]
Kepler-448c 2225004.2timing13181.5
Kepler-1659b 0.028±0.0010.17±0.0213.608±0.000060.11229transit3812.75701.02
Kepler-1659c 0.0014±0.0010.17±0.0320.4415±0.00130.1472transit3812.75701.02
Kepler-1660b 7.693±0.054237.68977±0.08237timing4013.68±73.271.21This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler.
KMT-2016-BLG-0212Lb 182.2microlensing210000.48
KMT-2016-BLG-1107Lb 3.283+3.468
−1.835
0.342+0.070
−0.085
microlensing21700+3090
−4400
0.087+0.092
−0.049
KMT-2016-BLG-1836L b 2.2+1.9
−1.1
3.5+1.1
−0.9
microlensing23157.1+2609.25
−7827.753
0.49+0.38
−0.25
[56]
KMT-2017-BLG-0165Lb 0.11+0.05
−0.04
3.45+0.98
−0.95
microlensing14774.880.760+0.340
−0.270
[57] [58]
KMT-2017-BLG-1038Lb 2.0+2.0
−1.1
1.8+0.6
−0.5
microlensing19569.38260.37+0.36
−0.20
KMT-2017-BLG-1146Lb 0.710+0.800
−0.420
1.6±0.6microlensing21200.160.33+0.36
−0.20
KMT-2018-BLG-1990Lb 0.3480.763microlensing31500.09
LHS 3844 b 0.1162±0.00200.46292913±0.000001900.00622±0.00017805±20transit48.60±0.030.15±0.013036±77
LP 791-18 b 0.09990.94800500.009690650transit86.410.142960 [59]
LP 791-18 c 0.2064.9899630.029392370transit86.410.142960 [59]
L 98-59 b 0.00157+0.00094
−0.00063
0.071±0.0042.25314±0.000020.0233±0.0017transit34.640.31±0.013367±150 [60]
L 98-59 c 0.00755+0.00566
−0.00252
0.12+0.007
−0.006
3.690621+0.000013
−0.000014
0.0324±0.0023-0.0024transit34.640.31±0.013367±150 [60]
L 98-59 d 0.0107+0.0085
−0.0044
0.14±0.0127.45086+0.00004
−0.00005
0.052±0.004transit34.640.31±0.013367±150 [60]
L 1159-16 c 0.23±0.02772.05+2.41
−1.84
0.88±0.02radial vel.14.578±0.0050.15±0.013154±54 [61] [62] Confirmed in 2022 as L 1159-16 b [63]
LSPM J2116+0234 b 0.04185+0.00315
−0.00346
14.4399+0.0078
−0.0087
0.0876+0.0022
−0.0021
radial vel.57.53±0.070.43±0.033475±51 [64]
LTT 1445 Ab 0.00690.1235.358820.03807433transit22.40.263337 [65]
MOA-bin-29b 0.6000.48microlensing232000.03 [66]
NGTS-5b  [ ja ]0.229±0.0371.136±0.0233.3569866±0.00000260.0382±0.0013952±24transit309.5±8.50.66+0.07
−0.06
4987±41 [67]
NGTS-6b  [ ja ]1.3391.3260.88205900.01677transit10100.774730 [68]
NGTS-8b 0.931.092.499700.0351345transit14200.895241 [69]
NGTS-9b 2.901.074.435270.0581448transit14201.346330 [69]
NSVS 14256825 b 14.15±0.163225±223.12±0.07timing2734.2±137.310.42±0.0740000Disputed [70]
NY Virginis c 5.548799timing1800Disputed [71]
OGLE-2013-BLG-0911L b 9.51+2.72
−1.69
microlensing10500+1500
−1100
0.29+0.07
−0.05
[72]
OGLE-2015-BLG-1649L 2.542.07microlensing13800.34 [73]
OGLE-2016-BLG-1227 b 0.79+1.3
−0.39
3.4+2.1
−1
microlensing0.1+0.17
−0.05
[74]
OGLE-2018-BLG-0532Lb 0.02062+0.00285
−0.00254
1.103+0.118
−0.107
microlensing [75]
OGLE-2018-BLG-0596Lb 0.04383±0.004910.97±0.13microlensing18400±24000.23±0.03 [76]
OGLE-2018-BLG-0740Lb 4.854806.1microlensing104001.05912 [77]
OGLE-2018-BLG-1011Lb 1.86.1microlensing230000.18 [78]
OGLE-2018-BLG-1011Lc 2.80.80microlensing230000.18 [78]
PDS 70c 8.0±4.034.5±2imaging369.96±1.70.76±0.023972±36 [79]
Qatar-8b 0.371±0.0621.285±0.0223.71495±0.001000.0474±0.00081457±14transit902.5±111.03±0.055738±51 [80]
Qatar-9b 1.19±0.161.009±0.0141.540731±0.0000380.0234±0.00031134±9transit689.5±5.20.72±0.024309±31 [80]
Qatar-10b 0.736±0.0901.543±0.0401.645321±0.0000100.0286±0.00061955±25transit1760±331.16±0.076124±46 [80]
SDSS J1228+1040 b 0.0009+0.0045
−0.000758
0.0857±0.000210.0034±0.0000091800timing413.337977±0.48923460.705±0.05 [81]
Teegarden b 0.00330+0.00041
−0.00038
4.9100±0.00140.0252+0.0008
−0.0009
radial vel.12.50±0.0130.09±0.012904±51 [82]
Teegarden c 0.00349+0.00050
−0.00047
11.409±0.0090.0443+0.0014
−0.0015
226radial vel.12.50±0.0130.09±0.012904±51Potentially habitable exoplanet [82]
TOI-125 b 0.0299±0.002770.2432±0.006694.65382±0.000330.05186+0.00086
−0.00077
1037±11transit363.3382±1.4350880.859+0.044
−0.038
5320±39 [83]
TOI-125 c 0.02086±0.003110.24614±0.0099.15059+0.0007
−0.00082
0.814±0.0013827.8±8.6transit363.3382±1.4350880.859+0.044
−0.038
5320±39 [83]
TOI-125 d 0.0428±0.00380.2614±0.015219.98+0.005
−0.0056
0.05186+0.00086
−0.00077
638.1±6.6transit363.3382±1.4350880.859+0.044
−0.038
5320±39 [84] [83]
TOI-150b 1.75+0.14
−0.17
1.38±0.045.857342+0.000065
−0.000066
0.0583+0.0013
−0.0018
1493+29
−32
transit1095.89±6.521.25+0.07
−0.12
6003+104
−98
[85]
TOI-163b 1.221.4894.2313060.05801669transit13591.446495 [85]
TOI-172b 5.42+0.22
−0.20
0.965+0.032
−0.029
9.47725+0.00064
−0.00079
0.0914±0.0017transit1097.4181.128+0.065
−0.061
5645±50 [86]
TOI-175b 0.00126+0.00050
−0.00048
0.0642+0.0046
−0.0035
2.2531136+0.0000012
−0.0000015
0.02191+0.00080
−0.00084
627+33
−36
transit34.636±0.0100.273±0.0303415±135 [87] To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique. [88] Host star also known as L 98-59. [89]
TOI-216 b 0.059±0.0020.714+0.268
−0.179
17.16070.1293+0.0067
−0.0051
628+13
−11
transit583±30.775026±125Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years [90] [91] [92]
TOI-216 c 0.56±0.020.902±0.01834.5255280.2069+0.0107
−0.0082
497+10
−8
transit583±30.775026±125Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years [90] [91] [92]
TOI-270b 0.00500.11123.3600800.0306528transit73.230.403386 [93] [94]
TOI-270c 0.01930.2165.6601720.0472424transit73.230.403386 [93] [94]
TOI-270d 0.01500.19011.380140.0733340transit73.230.403386 [93] [94] Hydrogen and steam atmosphere [95]
TOI-564b 1.463+0.10
−0.096
1.02+0.71
−0.29
1.651144±0.0000180.02734+0.00061
−0.00053
1714+20
−21
transit643.8±5.90.998+0.068
−0.057
5640+34
−37
[96]
TOI-905b 0.667+0.042
−0.041
1.171+0.052
−0.051
3.739494±0.0000380.04666+0.00096
−0.0011
1192+39
−36
transit489.9+23.5
−22.5
0.968+0.061
−0.068
5570+150
−140
[96]
V1298 Tauri b 0.911+0.049
−0.053
24.13861+0.00102
−0.00090
0.1687+0.0025
−0.0026
668±22transit353.9±2.31.10±0.054970±120 [97]
V1298 Tauri c 0.4998.249580.0825845±27transit353.91.104970 [98]
V1298 Tauri d 0.57212.40320.1083677±22transit353.91.104970 [98]
V1298 Tauri e 0.780600.308492+66
−104
transit353.91.104970 [98]
WASP-18Ac 0.174±0.0392.15580.035timing4041.226400 [99]
WASP-169b 0.5611.3045.61141180.06811604transit20801.346110 [100]
WASP-171b 1.0840.9803.81862440.050401642transit25301.175965 [100]
WASP-175b 0.9901.2083.06529070.044031571transit20801.216229 [100]
WASP-177b 0.508±0.0381.58+0.66
−0.83
3.071722±0.0000010.03957±0.000581142±32transit580.55830.876±0.0385017±70 [101]
WASP-178b 1.661.813.34482850.05582470transit13602.079360 [102]
WASP-180Ab 0.91.243.4092640.048transit8301.36600 [103]
WASP-181b 0.299±0.0341.184+0.071
−0.059
4.159±0.00000340.00542±0.000691186+32
−26
transit1444.8721.04±0.045839±70 [101]
WASP-182b 0.1480.8503.37698480.04511479transit10801.085638 [100]
WASP-183b 0.502±0.0471.47+0.94
−0.33
4.11177±0.00000510.0463±0.000751111±30transit1069.792921.00±0.030.784±0.038 [101]
WASP-184b 0.571.335.181700.06271480transit20901.236000 [102]
WASP-185b 0.9801.259.387550.09041160transit8971.125900 [102]
WASP-192b 2.301.232.87867650.04081620transit16101.095910 [102]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

References

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  38. 1 2 3 4 Hedges, Christina; Saunders, Nicholas; Barentsen, Geert; Coughlin, Jeffrey L.; De Miranda Cardoso, Josè Vinícius; Kostov, Veselin B.; Dotson, Jessie; Cody, Ann Marie (2019), "Four Small Planets Buried in K2 Systems: What Can We Learn for TESS?", The Astrophysical Journal, 880 (1): L5, arXiv: 1907.08244 , Bibcode:2019ApJ...880L...5H, doi: 10.3847/2041-8213/ab2a74 , S2CID   197935399
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  40. ↑ Wells, R.; Poppenhaeger, K.; Watson, C. A. (2019), "Validation of a temperate fourth planet in the K2-133 multiplanet system", Monthly Notices of the Royal Astronomical Society, 487 (2): 1865–1873, arXiv: 1905.05206 , doi: 10.1093/mnras/stz1334
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  42. 1 2 3 Adams, Elisabeth R.; Jackson, Brian; Johnson, Samantha; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Furlan, Elise; Howell, Steve B.; Jayanthi, Prasanna; MacQueen, Phillip J.; Matson, Rachel A.; Partyka-Worley, Ciera; Schlieder, Joshua; Scott, Nicholas J.; Stanton, Sevio M.; Ziegler, Carl (2020), Ultra Short Period Planets in K2 III: Neighbors Are Common With 12 New Multi-Planet Systems and 26 Newly Validated Planets in Campaigns 0-8, 10, arXiv: 2011.11698
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