This article will address the topic of List of exoplanets discovered in 2019, which has been the subject of debate and interest in different areas. List of exoplanets discovered in 2019 has attracted great attention due to its relevance in today's society and its impact on various aspects of daily life. Throughout history, List of exoplanets discovered in 2019 has played a fundamental role in the evolution of humanity, being the object of study and research in multiple disciplines. In this sense, different perspectives and approaches related to List of exoplanets discovered in 2019 will be analyzed, with the aim of providing a comprehensive and enriching vision on this topic. Through a rigorous and critical analysis, the aim is to delve into the different aspects that characterize List of exoplanets discovered in 2019, as well as its implications and repercussions today.
This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019.
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) | 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 | |||
Beta Pictoris c | 9 | 1200 | 2.7 | radial vel. | 64.43 | 1.76 | ||||
DS Tucanae Ab | 0.509±0.015 | 8.138268±0.000011 | 850 | transit | 143.89±0.22 | 1.01±0.06 | 5428±80 | |||
Epsilon Indi Ab | 3.25 | 16510 | 11.55 | 64.25 | radial vel. | 11.87 | 0.75 | |||
G 9-40 b | 0.1807 | 5.746007 | 0.0385 | 456 | transit | 91.1 | 0.290 | 3348 | ||
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 | |||
Gliese 357 b | 0.00579 | 0.1086 | 3.93072 | 0.035 | 525 | transit | 30.80 | 0.342 | 3505 | |
Gliese 357 c | 0.0107 | 9.1247 | 0.061 | 401.2 | radial vel. | 30.80 | 0.342 | 3505 | ||
Gliese 357 d | 0.019 | 55.661 | 0.204 | 219.6 | radial vel. | 30.80 | 0.342 | 3505 | Potentially habitable exoplanet | |
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 | |||
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 | 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 | |||
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 | ||
Gliese 3512 b | 0.463 | 203.59 | 0.3380 | radial vel. | 30.95 | 0.123 | 3081 | |||
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 | ||
HAT-P-69b | 3.58 | 1.676 | 4.7869491 | 0.06555 | 1930 | transit | 1122 | 1.65 | 7394 | |
HAT-P-70b | <6.78 | 1.87 | 2.74432452 | 0.04739 | 4000 | transit | 1073 | 1.89 | 8450 | |
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 |
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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 | |||
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 |
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 |
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 |
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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 | |
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 | |
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 |
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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 | |||
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 |
|||
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 |
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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 | ||
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 |
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 | |||
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 | |||
HD 97048 b | 2.5 | 130 | imaging | 603 | 2.4 | 10000 | Discovered using study of disk kinematics. 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 |
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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 |
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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 | |||
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 |
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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 |
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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 |
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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 |
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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 |
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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 | |
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 | ||
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 | |
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 | |||
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 |
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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 |
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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 |
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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 |
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HIP 79098 (AB)b | 20.5±4.5 | 345±6 | 2450±150 | imaging | 477.2±8.2 | 3.75±1.25 | Brown dwarf | |||
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 | ||
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 | ||
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 | ||
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 | |
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 | |||
K2-43c | 0.216 | 2.198884 | 1093.7 | transit | 598 | 0.57 | 3841 | |||
K2-50c | 0.089+0.011 −0.01 |
3.96151+0.00046 −0.00051 |
transit | 845.82±10.63 | 0.61±0.06 | |||||
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 | Host star also known as LP 358-499 | |
K2-146c | 0.02358 | 0.195 | 4.00498 | 1093.7 | transit | 259 | 0.33 | 3385 | ||
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 | |||||
K2-168c | 0.105+0.012 −0.009 |
8.0468+0.0024 −0.0025 |
transit | 800.91±13.67 | 0.91±0.03 | |||||
K2-198c | 0.1270 | 3.3596055 | 1229.9 | transit | 362 | 0.80 | 5213 | |||
K2-198d | 0.2175 | 7.4500177 | 943.2 | transit | 362 | 0.80 | 5213 | |||
K2-282c | 0.132+0.012 −0.009 |
0.70531±0.00005 | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | 3rd planet discovered in 2020 | |||
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 | |
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 | ||
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 | Two planets on a retrograde orbit |
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 | Two planets on a retrograde orbit |
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 | ||
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 | |||
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 | |||
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 | ||||
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 | ||||
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 |
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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 | Two more planets in star system discovered in 2020 | |||
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 |
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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 | ||||
K2-302b | 0.08+0.017 −0.018 |
2.25372±0.00047 | transit | 359.49±3.52 | 0.41+0.1 −0.08 |
Two more planets in system discovered in 2020 | ||||
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 |
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K2-304b | 0.118+0.007 −0.008 |
2.28943±0.00019 | transit | 1380.78±23.94 | 0.83+0.09 −0.12 |
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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 |
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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 |
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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 |
Two more planets in system are suspected, second planet in system confirmed in 2021 | |||
K2-308b | 0.884±0.087 | 3.38628±0.00002 | transit | 1.09±0.09 | 6100±263 | |||||
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 | ||
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 | ||
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 | |
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 |
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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 | |||
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 | ||
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 | |||
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 |
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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 |
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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 |
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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 |
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KMT-2017-BLG-1146Lb | 0.710+0.800 −0.420 |
1.6±0.6 | microlensing | 21200.16 | 0.33+0.36 −0.20 |
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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 | ||
LP 791-18 c | 0.206 | 4.989963 | 0.029392 | 370 | transit | 86.41 | 0.14 | 2960 | ||
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 | ||
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 | ||
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 | ||
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 | Refuted in 2022 | ||
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 | Confirmed in 2022 as L 1159-16 b | ||
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 | |||
LTT 1445 Ab | 0.0069 | 0.123 | 5.35882 | 0.03807 | 433 | transit | 22.4 | 0.26 | 3337 | |
MOA-bin-29b | 0.600 | 0.48 | microlensing | 23200 | 0.03 | |||||
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 | |
NGTS-6b | 1.339 | 1.326 | 0.8820590 | 0.01677 | transit | 1010 | 0.77 | 4730 | ||
NGTS-8b | 0.93 | 1.09 | 2.49970 | 0.035 | 1345 | transit | 1420 | 0.89 | 5241 | |
NGTS-9b | 2.90 | 1.07 | 4.43527 | 0.058 | 1448 | transit | 1420 | 1.34 | 6330 | |
NSVS 14256825 b | 14.15±0.16 | 3225±22 | 3.12±0.07 | timing | 2734.2±137.31 | 0.42±0.07 | 40000 | Disputed | ||
NY Virginis c | 5.54 | 8799 | timing | 1800 | Disputed | |||||
OGLE-2013-BLG-0911L b | 9.51+2.72 −1.69 |
microlensing | 10500+1500 −1100 |
0.29+0.07 −0.05 |
||||||
OGLE-2015-BLG-1649L | 2.54 | 2.07 | microlensing | 1380 | 0.34 | |||||
OGLE-2016-BLG-1227 b | 0.79+1.3 −0.39 |
3.4+2.1 −1 |
microlensing | 0.1+0.17 −0.05 |
||||||
OGLE-2018-BLG-0532Lb | 0.02062+0.00285 −0.00254 |
1.103+0.118 −0.107 |
microlensing | |||||||
OGLE-2018-BLG-0596Lb | 0.04383±0.00491 | 0.97±0.13 | microlensing | 18400±2400 | 0.23±0.03 | |||||
OGLE-2018-BLG-0740Lb | 4.8 | 5480 | 6.1 | microlensing | 10400 | 1.0 | 5912 | |||
OGLE-2018-BLG-1011Lb | 1.8 | 6.1 | microlensing | 23000 | 0.18 | |||||
OGLE-2018-BLG-1011Lc | 2.8 | 0.80 | microlensing | 23000 | 0.18 | |||||
PDS 70c | 8.0±4.0 | 34.5±2 | imaging | 369.96±1.7 | 0.76±0.02 | 3972±36 | ||||
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 | |
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 | |
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 | |
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 | |||
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 | |||
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 | |
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 | |
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 | |
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 | |
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 |
|
TOI-163b | 1.22 | 1.489 | 4.231306 | 0.0580 | 1669 | transit | 1359 | 1.44 | 6495 | |
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 | ||
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 | To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique. Host star also known as L 98-59. |
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 |
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 |
TOI-270b | 0.0050 | 0.1112 | 3.360080 | 0.0306 | 528 | transit | 73.23 | 0.40 | 3386 | |
TOI-270c | 0.0193 | 0.216 | 5.660172 | 0.0472 | 424 | transit | 73.23 | 0.40 | 3386 | |
TOI-270d | 0.0150 | 0.190 | 11.38014 | 0.0733 | 340 | transit | 73.23 | 0.40 | 3386 | Hydrogen and steam atmosphere |
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 |
|
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 |
|
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 | ||
V1298 Tauri c | 0.499 | 8.24958 | 0.0825 | 845±27 | transit | 353.9 | 1.10 | 4970 | ||
V1298 Tauri d | 0.572 | 12.4032 | 0.1083 | 677±22 | transit | 353.9 | 1.10 | 4970 | ||
V1298 Tauri e | 0.780 | 60 | 0.308 | 492+66 −104 |
transit | 353.9 | 1.10 | 4970 | ||
WASP-18Ac | 0.174±0.039 | 2.1558 | 0.035 | timing | 404 | 1.22 | 6400 | |||
WASP-126c | 0.202±0.077 | 7.63±0.17 | timing | 763.206±48.9235 | 1.12 | 5800 | False positive | |||
WASP-169b | 0.561 | 1.304 | 5.6114118 | 0.0681 | 1604 | transit | 2080 | 1.34 | 6110 | |
WASP-171b | 1.084 | 0.980 | 3.8186244 | 0.05040 | 1642 | transit | 2530 | 1.17 | 5965 | |
WASP-175b | 0.990 | 1.208 | 3.0652907 | 0.04403 | 1571 | transit | 2080 | 1.21 | 6229 | |
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 | |
WASP-178b | 1.66 | 1.81 | 3.3448285 | 0.0558 | 2470 | transit | 1360 | 2.07 | 9360 | |
WASP-180Ab | 0.9 | 1.24 | 3.409264 | 0.048 | transit | 830 | 1.3 | 6600 | ||
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 | |
WASP-182b | 0.148 | 0.850 | 3.3769848 | 0.0451 | 1479 | transit | 1080 | 1.08 | 5638 | |
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 | |
WASP-184b | 0.57 | 1.33 | 5.18170 | 0.0627 | 1480 | transit | 2090 | 1.23 | 6000 | |
WASP-185b | 0.980 | 1.25 | 9.38755 | 0.0904 | 1160 | transit | 897 | 1.12 | 5900 | |
WASP-192b | 2.30 | 1.23 | 2.8786765 | 0.0408 | 1620 | transit | 1610 | 1.09 | 5910 |