This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019.[1][2]
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 | 0.87 | 996.00 | 2.153 | radial vel. | 64.6 | 1.34 | 4826 | [4] | ||
Beta Pictoris c | 9 | 1200 | 2.7 | radial vel. | 64.43 | 1.76 | [5] | |||
DS Tucanae Ab | 0.509±0.015 | 8.138268±0.000011 | 850 | transit | 143.89±0.22 | 1.01±0.06 | 5428±80 | [6] | ||
Epsilon Indi Ab | 3.25 | 16510 | 11.55 | 64.25 | radial vel. | 11.87 | 0.75 | [7] | ||
G 9-40 b | 0.1807 | 5.746007 | 0.0385 | 456 | transit | 91.1 | 0.290 | 3348 | [8][9] | |
Gliese 49 b | 0.0177+0.0021 −0.0021 |
13.8508+0.0053 −0.0051 |
0.0905±0.0011 | radial vel. | 32.145±0.01 | 0.515±0.019 | 3805±51 | [10] | ||
Gliese 357 b | 0.00579 | 0.1086 | 3.93072 | 0.035 | 525 | transit | 30.80 | 0.342 | 3505 | [11] |
Gliese 357 c | 0.0107 | 9.1247 | 0.061 | 401.2 | radial vel. | 30.80 | 0.342 | 3505 | [11] | |
Gliese 357 d | 0.019 | 55.661 | 0.204 | 219.6 | radial vel. | 30.80 | 0.342 | 3505 | Potentially habitable exoplanet[11] | |
Gliese 378 b | 0.04097±0.006 | 3.822±0.001 | 0.082±0.002 | radial vel. | 48.79 | 0.56±0.01 | 3879±67 | [12] | ||
Gliese 411 b | 0.00941±0.00145 | 12.9532±0.0079 | 349.83±0.32 | radial vel. | 8.284 | 0.386±0.039 | 3563±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. | 46.7102 | 0.3816±0.069 | 0.55±0.06 | [14] | ||
Gliese 686 b | 0.022±0.003 | 15.53209+0.00166 −0.00167 |
0.091±0.004 | 379+24 −25 |
radial vel. | 26.612±0.008 | 0.42±0.05 | 3663±68 | [15] | |
Gliese 3512 b | 0.463 | 203.59 | 0.3380 | radial vel. | 30.95 | 0.123 | 3081 | [16] | ||
Gliese 4276 b | 0.05213+0.00296 −0.00299 |
13.352±0.003 | 0.082±0.002 | radial vel. | 69.6±0.1 | 0.41±0.03 | 3387±51 | May be two planwts in 2:1 orbital resonance[17] | ||
HAT-P-69b | 3.58 | 1.676 | 4.7869491 | 0.06555 | 1930 | transit | 1122 | 1.65 | 7394 | [18] |
HAT-P-70b | <6.78 | 1.87 | 2.74432452 | 0.04739 | 4000 | transit | 1073 | 1.89 | 8450 | [18][19] |
HD 8326 b | 0.210±0.062 | 158.991±1.440 | 0.533±0.011 | radial vel. | 100.2 | 0.80±0.05 | 4914+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±0.17 | 0.76±0.71 | 5868±27 | [21] | ||
HD 15337 b | 0.0236+0.0034 −0.0032 |
0.146±0.005 | 4.75615±0.00017 | 0.0522±0.0012 | 1001.0±11.5 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402[22] |
HD 15337 c | 0.0255+0.0057 −0.0053 |
0.213±0.011 | 17.1784±0.0016 | 0.1268±0.0038 | 642±10 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402[22] |
HD 21411 b | 0.207±0.081 | 84.288±0.127 | 0.362±0.007 | radial vel. | ±95.11 | 0.89±0.05 | 5605+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 |
transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | [23] |
HD 21749 c | <0.0116 | 0.0796+0.0057 −0.0052 |
7.78993+0.00051 −0.00044 |
0.0695+0.0021 −0.0023 |
701+25 −23 |
transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | [23] |
HD 24085 b | 0.0371±0.0098 | 2.0455±0.0002 | 0.034±0.001 | radial vel. | 179.4 | 1.22±0.07 | 6034+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±0.22 | 0.86±0.05 | 5160±63 | [21] | ||
HD 39855 b | 0.027±0.005 | 3.2498±0.0004 | 0.041±0.001 | radial vel. | 75.93 | 0.87±0.05 | 5576+50 −46 |
[20] | ||
HD 64114 b | 0.0560±0.0110 | 45.791±0.070 | 0.246±0.005 | radial vel. | 102.9 | 0.95±0.05 | 5676+32 −87 |
[20] | ||
HD 65216c | 1.295±0.062 | 577.6±1.328 | 1.301±0.020 | radial vel. | 114.7±0.1 | 0.95±0.01 | 5718±8 | Rediscovered in 2019 after false positive in 2013[24] | ||
HD 85628 Ab | 1.675±0.241 | 1.515±0.044 | 2.8240932±0.0000046 | 0.0474±0.0013 | 1865±25 | transit | 560±3 | 1.75±0.05 | 7800±200 | Host 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. | 113.1385 | 1.15±0.07 | 5744±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±0.22 | 1.08±0.06 | 5770±36 | [21][29] | ||
HD 97048 b | 2.5 | 130 | imaging | 603 | 2.4 | 10000 | Discovered using study of disk kinematics.[30] Unconfirmed. | |||
HD 102843 b | 0.3584±0.0456 | 3090.942±295.049 | 4.074±0.270 | radial vel. | 205.05 | 0.95±0.05 | 5436+144 −69 |
[20] | ||
HD 103949 b | 0.0352±0.0072 | 120.878±0.446 | 0.439±0.009 | radial vel. | 86.50 | 0.77±0.04 | 4792+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±0.42 | 1.01±0.06 | 5386±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±5.2 | 1.91+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±5.2 | 1.91+0.09 −0.14 |
5040+71 −85 |
[31] | ||
HD 206255 b | 0.108±0.022 | 96.045±0.317 | 0.461±0.009 | radial vel. | 245.9 | 1.42±0.08 | 5635+82 −99 |
[20] | ||
HD 210193 b | 0.4817±0.0733 | 649.918±8.599 | 1.487±0.031 | radial vel. | 137.8 | 1.04±0.06 | 5790+38 −50 |
[20] | ||
HD 211970 b | 0.0409±0.0079 | 25.201±0.025 | 0.143±0.003 | radial vel. | 42.4 | 0.61±0.04 | 4127+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 |
transit | 156.45721±0.4566189 | 1.068+0.020 −0.018 |
5978±50 | A 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±0.4566189 | 1.068+0.020 −0.018 |
5978±50 | [32] | |
HD 221416 b | 0.190±0.018 | 0.836+0.031 −0.028 |
14.2767±0.0037 | 0.1228+0.00025 −0.00026 |
transit | 310.0931 | 1.212±0.074 | 5080±90 | Host star also known as TOI-197 or HIP 116158[33] | |
HD 221420 b | 9.70+1.10 −1.00 |
22482+4200 −4100 |
18.5±2.3 | radial vel. | 101.7±0.12 | 1.67±0.11 | 5830±44 | [29] | ||
HIP 35173 b | 0.0400±0.0085 | 41.516±0.077 | 0.217±0.004 | radial vel. | 108.25 | 0.79±0.05 | 4881+55 −81 |
[20] | ||
HIP 54373 b | 0.02712±0.00579 | 7.760±0.003 | 0.063±0.001 | radial vel. | 61.09 | 0.57±0.03 | 4021+226 −146 |
[20] | ||
HIP 54373 c | 0.03914±0.00664 | 15.144±0.008 | 0.0990±0.0020 | radial vel. | 61.09 | 0.57±0.03 | 4021+226 −146 |
[20] | ||
HIP 71135 b | 0.0592±0.0129 | 87.190±0.381 | 0.335±0.007 | radial vel. | 105.5 | 0.66±0.04 | 4146+107 −110 |
[20] | ||
HIP 79098 (AB)b | 20.5±4.5 | 345±6 | 2450±150 | imaging | 477.2±8.2 | 3.75±1.25 | Brown dwarf[34] | |||
HR 858 b | 0.1860+0.0061 −0.0057 |
3.58599±0.00015 | 0.0480+0.0010 −0.0011 |
1572+22 −19 |
transit | 104.35 | 1.145+0.074 −0.080 |
6201±50 | [35] | |
HR 858 c | 0.1730±0.0062 | 5.97293+0.00060 −0.00053 |
0.0674+0.0014 −0.0016 |
1326+18 −16 |
transit | 104.35 | 1.145+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 |
transit | 104.35 | 1.145+0.074 −0.080 |
6201±50 | [35] | |
HR 5183 b | 3.23 | 27000 | 18 | 171 | radial vel. | 102.7 | 1.07 | 5794 | Exoplanet 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±0.00055 | transit | 516.6±4.2 | 0.856±0.028 | With a radius almost identical to that of the Earth it is almost certainly a terrestrial planet[37] | |||
K2-43c | 0.216 | 2.198884 | 1093.7 | transit | 598 | 0.57 | 3841 | [38] | ||
K2-50c | 0.089+0.011 −0.01 |
3.96151+0.00046 −0.00051 |
transit | 845.82±10.63 | 0.61±0.06 | [39] | ||||
K2-63c | 0.35±0.11 | 25.4556±0.0047 | 0.189±0.011 | transit | 524.414±21 | 1.40±0.25 | 6771±303 | Unconfirmed | ||
K2-133e | 0.154+0.012 −0.012 |
26.5841+0.0018 −0.0017 |
0.1346±0.0011 | 296±10 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | [40]Host star also known as LP 358-499 | |
K2-146c | 0.02358 | 0.195 | 4.00498 | 1093.7 | transit | 259 | 0.33 | 3385 | [41] | |
K2-166c | 0.109+0.019 −0.015 |
3.80464+0.00091 −0.00105 |
transit | 1568.81+31.64 −29.03 |
1.07±0.03 | [39] | ||||
K2-168c | 0.105+0.012 −0.009 |
8.0468+0.0024 −0.0025 |
transit | 800.91±13.67 | 0.91±0.03 | [38][39] | ||||
K2-198c | 0.1270 | 3.3596055 | 1229.9 | transit | 362 | 0.80 | 5213 | [38] | ||
K2-198d | 0.2175 | 7.4500177 | 943.2 | transit | 362 | 0.80 | 5213 | [38] | ||
K2-282c | 0.132+0.012 −0.009 |
0.70531±0.00005 | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | [39]3rd planet discovered in 2020[42] | |||
K2-286b | 0.0214±0.0135 | 0.1873±0.0178 | 27.359±0.005 | 0.1768+0.0175 −0.0205 |
347+21 −11 |
transit | 248.9±0.8 | 0.64±0.02 | 3926±100 | [43] |
K2-288Bb | 0.17±0.03 | 31.393463+0.000067 −0.000069 |
0.164±0.030 | 226.36±22.30 | transit | 214.3±2.8 | 0.33±0.02 | 3341±276 | [44] | |
K2-290b | 0.0664 | 0.273±0.014 | 9.21165+0.00033 −0.00034 |
0.0923±0.0066 | 1230±38 | transit | 897±12 | 1.19+0.07 −0.08 |
6302±120 | [45] Two planets on a retrograde orbit[46] |
K2-290c | 0.774±0.047 | 1.006±0.050 | 48.36685+0.00041 −0.00040 |
0.0923±0.0066 | 676±16 | transit | 897±12 | 1.19+0.07 −0.08 |
6302±120 | [45] Two planets on a retrograde orbit[46] |
K2-291b | 0.0204±0.0036 | 0.1418+0.0085 −0.0064 |
2.225177+0.000066 −0.000068 |
0.03261±0.00044 | transit | 295±2 | 0.93±0.04 | 5520±60 | [47] | |
K2-293b | 0.219+0.031 −0.022 |
13.1225+0.0011 −0.0012 |
750+170 −50 |
transit | 1290±22 | 0.96+0.04 −0.03 |
5532±78 | [48] | ||
K2-294b | 0.148+0.019 −0.017 |
2.50387+0.00022 −0.00023 |
1425+79 −54 |
transit | 1230±20 | 0.99+0.03 −0.03 |
5612±50 | [48] | ||
K2-296b | 0.167+0.018 −0.04 |
28.1656+0.0027 −0.0028 |
transit | 521.78±4.57 | 0.41+0.11 −0.05 |
Host star also known as EPIC 201238110[39] | ||||
K2-297b | 0.062+0.005 −0.004 |
2.13174±0.00022 | transit | 831.31±5.48 | 0.78+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 |
transit | 1441.42±26.65 | 0.8+0.08 −0.16 |
[39] | ||||
K2-299b | 0.152+0.053 −0.028 |
4.50756+0.00062 −0.0006 |
transit | 1219.21±16.28 | 0.93+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 |
transit | 528.67±5.87 | 0.22+0.04 −0.06 |
[39] | ||||
K2-301b | 0.145+0.015 −0.017 |
5.29711+0.00074 −0.0007 |
transit | 1491.42±44.98 | 0.56±0.05 | 4114±99 | [39] | |||
K2-302b | 0.08+0.017 −0.018 |
2.25372±0.00047 | transit | 359.49±3.52 | 0.41+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 |
transit | 1034.57±9.59 | 0.71+0.09 −0.03 |
[39] | ||||
K2-304b | 0.118+0.007 −0.008 |
2.28943±0.00019 | transit | 1380.78±23.94 | 0.83+0.09 −0.12 |
[39] | ||||
K2-305b | 0.194+0.06 −0.037 |
18.0983+0.006 −0.0058 |
transit | 2030.88±33.92 | 1.11+0.14 −0.12 |
[39] | ||||
K2-306b | 0.143+0.012 −0.014 |
34.885+0.011 −0.01 |
transit | 931.54±6.69 | 0.91+0.04 −0.16 |
[39] | ||||
K2-307b | 0.1+0.011 −0.008 |
15.2841+0.0037 −0.0029 |
transit | 1053.09±20.65 | 0.98+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±0.087 | 3.38628±0.00002 | transit | 1.09±0.09 | 6100±263 | [51] | ||||
K2-310b | 0.2307±0.0112 | 13.6030±0.0013 | 0.0980±0.0040 | 536±18 | transit | 1133.22 | 0.690±0.038 | 4684±79 | [52] | |
K2-310c | 0.2400±0.0130 | 65.5500±0.0089 | 0.280±0.006 | 316±10 | transit | 1133.22 | 0.690±0.038 | 4684±79 | [52] | |
KELT-23Ab | 0.938+0.048 −0.044 |
1.323±0.025 | 2.255251+0.000011 −0.000012 |
0.03302+0.00068 −0.00064 |
1561±20 | transit | 409.07±1.14 | 0.94+0.06 −0.05 |
5899±49 | [53] |
KELT-24b | 5.18 | 1.272 | 5.5514926 | 0.06969 | 1459 | transit | 313.2 | 1.46 | 6509 | |
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 |
transit | 4900 | 0.957+0.013 −0.015 |
|||
Kepler-65e | 0.653+0.056 −0.055 |
258.8+1.5 −1.3 |
0.362±0.007 | radial vel. | 999.3±8.8 | 1.25±0.06 | 6211±66 | |||
Kepler-82f | 0.0658±0.0031 | 75.732±0.012 | 0.3395±0.0041 | timing | 3026.64 | 0.91±0.03 | 5401±108 | |||
Kepler-88d | 3.15±0.15 | 1409+14 −13 |
2.45±0.02 | radial vel. | 1243±7 | 1.022+0.023 −0.026 |
5513±67 | [54] | ||
Kepler-411d | 0.0478±0.0160 | 0.2961±0.0093 | 58.02035±0.00056 | 0.279±0.004 | 410±10 | transit | 500.94±1.57 | 0.87±0.04 | [55] | |
Kepler-411e | 0.0340±0.0035 | 31.509728±0.000085 | 0.186±0.003 | 503±9 | timing | 500.94±1.57 | 0.87±0.04 | [55] | ||
Kepler-448c | 22 | 2500 | 4.2 | timing | 1318 | 1.5 | ||||
Kepler-1658b | 5.88 | 1.04 | 3.8494 | 0.0546 | transit | 2629.05 | 2.891+0.130 −0.106 |
6216±78 | First exoplanet candidate detected by Kepler Space Telescope (known as KOI-4.01), confirmed in 2019. | |
Kepler-1659b | 0.028±0.001 | 0.17±0.02 | 13.608±0.00006 | 0.11229 | transit | 3812.7570 | 1.02 | |||
Kepler-1659c | 0.0014±0.001 | 0.17±0.03 | 20.4415±0.0013 | 0.1472 | transit | 3812.7570 | 1.02 | |||
Kepler-1660b | 7.693±0.054 | 237.68977±0.08237 | timing | 4013.68±73.27 | 1.21 | This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler. | ||||
KMT-2016-BLG-0212Lb | 18 | 2.2 | microlensing | 21000 | 0.48 | |||||
KMT-2016-BLG-1107Lb | 3.283+3.468 −1.835 |
0.342+0.070 −0.085 |
microlensing | 21700+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 |
microlensing | 23157.1+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 |
microlensing | 14774.88 | 0.760+0.340 −0.270 |
[57][58] | ||||
KMT-2017-BLG-1038Lb | 2.0+2.0 −1.1 |
1.8+0.6 −0.5 |
microlensing | 19569.3826 | 0.37+0.36 −0.20 |
|||||
KMT-2017-BLG-1146Lb | 0.710+0.800 −0.420 |
1.6±0.6 | microlensing | 21200.16 | 0.33+0.36 −0.20 |
|||||
KMT-2018-BLG-1990Lb | 0.348 | 0.763 | microlensing | 3150 | 0.09 | |||||
LHS 3844 b | 0.1162±0.0020 | 0.46292913±0.00000190 | 0.00622±0.00017 | 805±20 | transit | 48.60±0.03 | 0.15±0.01 | 3036±77 | ||
LP 791-18 b | 0.0999 | 0.9480050 | 0.009690 | 650 | transit | 86.41 | 0.14 | 2960 | [59] | |
LP 791-18 c | 0.206 | 4.989963 | 0.029392 | 370 | transit | 86.41 | 0.14 | 2960 | [59] | |
L 98-59 b | 0.00157+0.00094 −0.00063 |
0.071±0.004 | 2.25314±0.00002 | 0.0233±0.0017 | transit | 34.64 | 0.31±0.01 | 3367±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±0.0023-0.0024 | transit | 34.64 | 0.31±0.01 | 3367±150 | [60] | |
L 98-59 d | 0.0107+0.0085 −0.0044 |
0.14±0.012 | 7.45086+0.00004 −0.00005 |
0.052±0.004 | transit | 34.64 | 0.31±0.01 | 3367±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±0.007 | 0.15 | 3158 | [61][62] Refuted in 2022[63] | ||
L 1159-16 c | 0.23±0.02 | 772.05+2.41 −1.84 |
0.88±0.02 | radial vel. | 14.578±0.005 | 0.15±0.01 | 3154±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±0.07 | 0.43±0.03 | 3475±51 | [64] | ||
LTT 1445 Ab | 0.0069 | 0.123 | 5.35882 | 0.03807 | 433 | transit | 22.4 | 0.26 | 3337 | [65] |
MOA-bin-29b | 0.600 | 0.48 | microlensing | 23200 | 0.03 | [66] | ||||
NGTS-5b | 0.229±0.037 | 1.136±0.023 | 3.3569866±0.0000026 | 0.0382±0.0013 | 952±24 | transit | 309.5±8.5 | 0.66+0.07 −0.06 |
4987±41 | [67] |
NGTS-6b | 1.339 | 1.326 | 0.8820590 | 0.01677 | transit | 1010 | 0.77 | 4730 | [68] | |
NGTS-8b | 0.93 | 1.09 | 2.49970 | 0.035 | 1345 | transit | 1420 | 0.89 | 5241 | [69] |
NGTS-9b | 2.90 | 1.07 | 4.43527 | 0.058 | 1448 | transit | 1420 | 1.34 | 6330 | [69] |
NSVS 14256825 b | 14.15±0.16 | 3225±22 | 3.12±0.07 | timing | 2734.2±137.31 | 0.42±0.07 | 40000 | Disputed[70] | ||
NY Virginis c | 5.54 | 8799 | timing | 1800 | Disputed[71] | |||||
OGLE-2013-BLG-0911L b | 9.51+2.72 −1.69 |
microlensing | 10500+1500 −1100 |
0.29+0.07 −0.05 |
[72] | |||||
OGLE-2015-BLG-1649L | 2.54 | 2.07 | microlensing | 1380 | 0.34 | [73] | ||||
OGLE-2016-BLG-1227 b | 0.79+1.3 −0.39 |
3.4+2.1 −1 |
microlensing | 0.1+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±0.00491 | 0.97±0.13 | microlensing | 18400±2400 | 0.23±0.03 | [76] | ||||
OGLE-2018-BLG-0740Lb | 4.8 | 5480 | 6.1 | microlensing | 10400 | 1.0 | 5912 | [77] | ||
OGLE-2018-BLG-1011Lb | 1.8 | 6.1 | microlensing | 23000 | 0.18 | [78] | ||||
OGLE-2018-BLG-1011Lc | 2.8 | 0.80 | microlensing | 23000 | 0.18 | [78] | ||||
PDS 70c | 8.0±4.0 | 34.5±2 | imaging | 369.96±1.7 | 0.76±0.02 | 3972±36 | [79] | |||
Qatar-8b | 0.371±0.062 | 1.285±0.022 | 3.71495±0.00100 | 0.0474±0.0008 | 1457±14 | transit | 902.5±11 | 1.03±0.05 | 5738±51 | [80] |
Qatar-9b | 1.19±0.16 | 1.009±0.014 | 1.540731±0.000038 | 0.0234±0.0003 | 1134±9 | transit | 689.5±5.2 | 0.72±0.02 | 4309±31 | [80] |
Qatar-10b | 0.736±0.090 | 1.543±0.040 | 1.645321±0.000010 | 0.0286±0.0006 | 1955±25 | transit | 1760±33 | 1.16±0.07 | 6124±46 | [80] |
SDSS J1228+1040 b | 0.0009+0.0045 −0.000758 |
0.0857±0.00021 | 0.0034±0.000009 | 1800 | timing | 413.337977±0.4892346 | 0.705±0.05 | [81] | ||
Teegarden b | 0.00330+0.00041 −0.00038 |
4.9100±0.0014 | 0.0252+0.0008 −0.0009 |
radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | [82] | ||
Teegarden c | 0.00349+0.00050 −0.00047 |
11.409±0.009 | 0.0443+0.0014 −0.0015 |
226 | radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | Potentially habitable exoplanet[82] | |
TOI-125 b | 0.0299±0.00277 | 0.2432±0.00669 | 4.65382±0.00033 | 0.05186+0.00086 −0.00077 |
1037±11 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [83] |
TOI-125 c | 0.02086±0.00311 | 0.24614±0.009 | 9.15059+0.0007 −0.00082 |
0.814±0.0013 | 827.8±8.6 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [83] |
TOI-125 d | 0.0428±0.0038 | 0.2614±0.0152 | 19.98+0.005 −0.0056 |
0.05186+0.00086 −0.00077 |
638.1±6.6 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [84][83] |
TOI-150b | 1.75+0.14 −0.17 |
1.38±0.04 | 5.857342+0.000065 −0.000066 |
0.0583+0.0013 −0.0018 |
1493+29 −32 |
transit | 1095.89±6.52 | 1.25+0.07 −0.12 |
6003+104 −98 |
[85] |
TOI-163b | 1.22 | 1.489 | 4.231306 | 0.0580 | 1669 | transit | 1359 | 1.44 | 6495 | [85] |
TOI-172b | 5.42+0.22 −0.20 |
0.965+0.032 −0.029 |
9.47725+0.00064 −0.00079 |
0.0914±0.0017 | transit | 1097.418 | 1.128+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 |
transit | 34.636±0.010 | 0.273±0.030 | 3415±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±0.002 | 0.714+0.268 −0.179 |
17.1607 | 0.1293+0.0067 −0.0051 |
628+13 −11 |
transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years[90][91][92] |
TOI-216 c | 0.56±0.02 | 0.902±0.018 | 34.525528 | 0.2069+0.0107 −0.0082 |
497+10 −8 |
transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years[90][91][92] |
TOI-270b | 0.0050 | 0.1112 | 3.360080 | 0.0306 | 528 | transit | 73.23 | 0.40 | 3386 | [93][94] |
TOI-270c | 0.0193 | 0.216 | 5.660172 | 0.0472 | 424 | transit | 73.23 | 0.40 | 3386 | [93][94] |
TOI-270d | 0.0150 | 0.190 | 11.38014 | 0.0733 | 340 | transit | 73.23 | 0.40 | 3386 | [93][94]Hydrogen and steam atmosphere[95] |
TOI-564b | 1.463+0.10 −0.096 |
1.02+0.71 −0.29 |
1.651144±0.000018 | 0.02734+0.00061 −0.00053 |
1714+20 −21 |
transit | 643.8±5.9 | 0.998+0.068 −0.057 |
5640+34 −37 |
[96] |
TOI-905b | 0.667+0.042 −0.041 |
1.171+0.052 −0.051 |
3.739494±0.000038 | 0.04666+0.00096 −0.0011 |
1192+39 −36 |
transit | 489.9+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±22 | transit | 353.9±2.3 | 1.10±0.05 | 4970±120 | [97] | |
V1298 Tauri c | 0.499 | 8.24958 | 0.0825 | 845±27 | transit | 353.9 | 1.10 | 4970 | [98] | |
V1298 Tauri d | 0.572 | 12.4032 | 0.1083 | 677±22 | transit | 353.9 | 1.10 | 4970 | [98] | |
V1298 Tauri e | 0.780 | 60 | 0.308 | 492+66 −104 |
transit | 353.9 | 1.10 | 4970 | [98] | |
WASP-18Ac | 0.174±0.039 | 2.1558 | 0.035 | timing | 404 | 1.22 | 6400 | [99] | ||
WASP-126c | 0.202±0.077 | 7.63±0.17 | timing | 763.206±48.9235 | 1.12 | 5800 | [99]False positive[100] | |||
WASP-169b | 0.561 | 1.304 | 5.6114118 | 0.0681 | 1604 | transit | 2080 | 1.34 | 6110 | [101] |
WASP-171b | 1.084 | 0.980 | 3.8186244 | 0.05040 | 1642 | transit | 2530 | 1.17 | 5965 | [101] |
WASP-175b | 0.990 | 1.208 | 3.0652907 | 0.04403 | 1571 | transit | 2080 | 1.21 | 6229 | [101] |
WASP-177b | 0.508±0.038 | 1.58+0.66 −0.83 |
3.071722±0.000001 | 0.03957±0.00058 | 1142±32 | transit | 580.5583 | 0.876±0.038 | 5017±70 | [102] |
WASP-178b | 1.66 | 1.81 | 3.3448285 | 0.0558 | 2470 | transit | 1360 | 2.07 | 9360 | [103] |
WASP-180Ab | 0.9 | 1.24 | 3.409264 | 0.048 | transit | 830 | 1.3 | 6600 | [104] | |
WASP-181b | 0.299±0.034 | 1.184+0.071 −0.059 |
4.159±0.0000034 | 0.00542±0.00069 | 1186+32 −26 |
transit | 1444.872 | 1.04±0.04 | 5839±70 | [102] |
WASP-182b | 0.148 | 0.850 | 3.3769848 | 0.0451 | 1479 | transit | 1080 | 1.08 | 5638 | [101] |
WASP-183b | 0.502±0.047 | 1.47+0.94 −0.33 |
4.11177±0.0000051 | 0.0463±0.00075 | 1111±30 | transit | 1069.79292 | 1.00±0.03 | 0.784±0.038 | [102] |
WASP-184b | 0.57 | 1.33 | 5.18170 | 0.0627 | 1480 | transit | 2090 | 1.23 | 6000 | [103] |
WASP-185b | 0.980 | 1.25 | 9.38755 | 0.0904 | 1160 | transit | 897 | 1.12 | 5900 | [103] |
WASP-192b | 2.30 | 1.23 | 2.8786765 | 0.0408 | 1620 | transit | 1610 | 1.09 | 5910 | [103] |