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] Unconfirmed.
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 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 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 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 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 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 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 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 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 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 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 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-1658b 5.881.043.84940.0546transit2629.052.891+0.130
0.106
6216±78First exoplanet candidate detected by Kepler Space Telescope (known as KOI-4.01), confirmed in 2019.
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 b 0.088+0.060
0.035
241.59+4.6
4.0
0.403+0.039
0.047
radial vel.14.584±0.0070.153158 [61] [62] Refuted in 2022 [63]
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-126c 0.202±0.0777.63±0.17timing763.206±48.92351.125800 [99] False positive [100]
WASP-169b 0.5611.3045.61141180.06811604transit20801.346110 [101]
WASP-171b 1.0840.9803.81862440.050401642transit25301.175965 [101]
WASP-175b 0.9901.2083.06529070.044031571transit20801.216229 [101]
WASP-177b 0.508±0.0381.58+0.66
0.83
3.071722±0.0000010.03957±0.000581142±32transit580.55830.876±0.0385017±70 [102]
WASP-178b 1.661.813.34482850.05582470transit13602.079360 [103]
WASP-180Ab 0.91.243.4092640.048transit8301.36600 [104]
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 [102]
WASP-182b 0.1480.8503.37698480.04511479transit10801.085638 [101]
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 [102]
WASP-184b 0.571.335.181700.06271480transit20901.236000 [103]
WASP-185b 0.9801.259.387550.09041160transit8971.125900 [103]
WASP-192b 2.301.232.87867650.04081620transit16101.095910 [103]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

Related Research Articles

HD 101930, also known as Gliese 3683, is an orange hued star with an orbiting exoplanet located in the southern constellation Centaurus. It has an apparent magnitude of 8.21, making it faintly visible in binoculars but not to the naked eye. The system is located relatively close at a distance of 98 light years but is receding with a heliocentric radial velocity of 18.4 km/s. It has a relatively large proper motion, traversing the celestial sphere with an angular velocity of 0.320″·yr−1.

<span class="mw-page-title-main">WASP-4b</span> Extrasolar planet in the constellation Phoenix

WASP-4b is an exoplanet, specifically a hot Jupiter, approximately 891 light-years away in the constellation of Phoenix.

Gliese 179 is a small red dwarf star with an exoplanetary companion in the equatorial constellation of Orion. It is much too faint to be visible to the naked eye with an apparent visual magnitude of 11.94. The system is located at a distance of 40.5 light-years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of –9 km/s. It is a high proper motion star, traversing the celestial sphere at an angular rate of 0.370″·yr−1.

K2-3, also known as EPIC 201367065, is a red dwarf star with three known planets. It is on the borderline of being a late orange dwarf/K-type star, but because of its temperature, it is classified as a red dwarf.

Kepler-421 is a yellow main sequence star, being of spectral class G7V. Orange star of spectral class K9V, projected on sky plane just 1.085″ away, is not physically associated to it. The distance to star KOI-1274 A is approximately 1150 light-years, and to KOI-1274 B is about 1900 light-years.

Kepler-51 is a Sun-like star that is about 500 million years old. It is orbited by three super-puff planets—Kepler-51b, c, and d—which have the lowest known densities of any known exoplanet. The planets are similar in radius to gas giants like Jupiter, but have unusually small masses for their size, only a few times greater than Earth’s.

<span class="mw-page-title-main">LTT 1445</span> Star system in the constellation Eridanus

LTT 1445 is a triple M-dwarf system 22.4 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 October 2022 it is the second closest transiting exoplanet system discovered, with the closest being HD 219134 bc.

WASP-50 is a G-type main-sequence star about 610 light-years away. The star is older than the Sun and slightly depleted in heavy elements compared to the Sun, and has a close to average starspot activity. Despite its advanced age, the star is rotating rapidly, being spun up by the tides raised by giant planet on close orbit.

WASP-80 is a K-type main-sequence star about 162 light-years away. The star's age is much younger than the Sun's at 1.352±0.222 billion years. WASP-80 is similar to the Sun in concentration of heavy elements, although this measurement is highly uncertain.

L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs, as measured by Gaia.

<span class="mw-page-title-main">Wolf 1069</span> Red dwarf star in the constellation Cygnus

Wolf 1069 is a red dwarf star located 31.2 light-years away from the Solar System in the constellation of Cygnus. The star has 17% the mass and 18% the radius of the Sun, a temperature of 3,158 K, and a slow rotation period of 150–170 days. It hosts one known exoplanet called Wolf 1069 b which could possibly sustain life.

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