This list of exoplanets discovered in 2022 is a list of confirmed exoplanets that were first reported in 2022. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.
On 31 March 2022, K2-2016-BLG-0005Lb was reported to be the most distant exoplanet found by Kepler to date.[1][2]
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 |
---|---|---|---|---|---|---|---|---|---|---|
HD 22532 b | 2.12±0.09 | 872.6±2.8 | 1.900±0.004 | radial vel. | 526±2 | 1.20±0.05 | 5067+59 −22 |
Giant host star[3] | ||
HD 64121 b | 2.56±0.19 | 623.0±3.4 | 1.510±0.006 | radial vel. | 424.1±1.7 | 1.18±0.05 | 5066+58 −60 |
Giant host star[3] | ||
HD 69123 b | 3.04±0.16 | 1193.3±7.0 | 2.482±0.010 | radial vel. | 245.0±1.3 | 1.43±0.07 | 4787+280 −51 |
Giant host star[3] | ||
HD 29399 b | 1.57±0.11 | 892.7±5.9 | 1.913±0.008 | radial vel. | 144.2±0.3 | 1.15±0.04 | 4845±52 | Giant host star[4] | ||
Kepler-1708b | <4.6 | 0.8886+0.0535 −0.0526 |
737.11310+0.00146 −0.00770 |
1.64±0.10 | transit | 5436+334 −298 |
1.088±0.072 | 6157+231 −202 |
Possible exomoon host[5][6] | |
TOI-1064b | 0.0425±0.0055 | 0.231±0.004 | 6.443868±0.000025 | 0.06152+0.00086 −0.00089 |
784±13 | transit | 224.5±0.2 | 0.748±0.032 | 4734±67 | [7] |
TOI-1064c | 0.0079+0.0057 −0.0063 |
0.237±0.004 | 12.226574+0.000046 −0.000043 |
0.09429+0.00132 −0.00136 |
634±10 | transit | 224.5±0.2 | 0.748±0.032 | 4734±67 | [7] |
TOI-2337b | 1.60±0.15 | 0.9±0.1 | 2.99432±0.00008 | 0.04467 | transit | 1780±20 | 1.325±0.118 | 4780±100 | [8] | |
TOI-4329b | 0.45±0.09 | 1.50±0.19 | 2.9223±0.00015 | transit | 2258±16 | 1.538±0.049 | 6000±100 | [8] | ||
TOI-2669b | 0.61±0.19 | 1.76±0.16 | 6.2034±0.0001 | transit | 1294±9 | 1.19±0.16 | 4800±100 | [8] | ||
TOI-2180 b | 2.755+0.087 −0.081 |
1.010+0.022 −0.019 |
260.79+0.59 −0.58 |
0.828±0.012 | 348.0+3.3 −3.6 |
transit | 379.4±0.8 | 1.111+0.047 −0.046 |
5695+58 −60 |
[9] |
OGLE-2016-BLG-1093Lb | 0.71±0.12 | 2.13±0.33 | microlensing | 26000±2000 | 0.46±0.08 | [10] | ||||
TOI-3714 b | 0.70±0.003 | 1.01±0.03 | 2.154849±0.000001 | 0.027±0.001 | 750±20 | transit | 367.0+0.6 −1.3 |
0.53±0.02 | 3660±90 | [11] |
TOI-3629 b | 0.26±0.02 | 0.74±0.02 | 3.936551+0.000005 −0.000006 |
0.043±0.002 | 690±20 | transit | 423.1±1.0 | 0.63±0.02 | 3870±90 | [11] |
Kepler-1972 b | 0.0064±0.0019 | 0.072±0.004 | 7.54425±0.00054 | transit | 923±3 | 1.12±0.03 | 5818±27 | Very dense planets, additional planet in system suspected[12] | ||
Kepler-1972 c | 0.0066±0.0020 | 0.078±0.005 | 11.3295±0.0011 | transit | 923±3 | 1.12±0.03 | 5818±27 | Very dense planets, additional planet in system suspected[12] | ||
TOI-206 b | 0.116±0.004 | 0.7363104±0.0000003 | 0.0112±0.0001 | 910±36 | transit | 155.9 | 0.35±0.01 | 3383±157 | [13] | |
TOI-500 b | 0.104±0.010 | 0.5481579±0.0000006 | 0.0128±0.0011 | 1693±105 | transit | 154.8 | 0.88±0.25 | 4621±50 | [13] | |
TOI-544 b | 0.181±0.009 | 1.5483510±0.0000015 | 0.0251 ± 0.0019 | 1082±47 | transit | 132.7 | 0.85±0.20 | 4369±100 | [13] | |
TOI-833 b | 0.113±0.006 | 1.0418777±0.0000324 | 0.0171±0.0003 | 1118±49 | transit | 136.3 | 0.61±0.03 | 3920±160 | [13] | |
TOI-1075 b | 0.154±0.007 | 0.6047328±0.0000032 | 0.0118±0.0001 | 1336±56 | transit | 200.9 | 0.60±0.02 | 3921±157 | [13] | |
TOI-1411 b | 0.121±0.013 | 1.4520358±0.0000098 | 0.0230±0.0026 | 1136±59 | transit | 106.0 | 0.59±0.23 | 4266±100 | [13] | |
TOI-1442 b | 0.104±0.005 | 0.4090677±0.0000003 | 0.0071±0.0002 | 1072±54 | transit | 134.5 | 0.29±0.02 | 3330±160 | [13] | |
TOI-1693 b | 0.126±0.009 | 1.7666957±0.0000054 | 0.0226±0.0004 | 764±19 | transit | 100.6 | 0.49±0.03 | 3499±70 | [13] | |
TOI-1860 b | 0.117±0.005 | 1.0662107±0.0000014 | 0.0204±0.0002 | 1885±28 | transit | 149.8 | 0.99±0.03 | 5752±100 | [13] | |
TOI-2260 b | 0.145±0.012 | 0.3524728±0.0000047 | 0.0097±0.0001 | 2609±86 | transit | 331.2 | 0.99±0.04 | 5534±100 | [13] | |
TOI-2411 b | 0.150±0.010 | 0.7826942±0.0000037 | 0.0144±0.0001 | 1355±45 | transit | 194.5 | 0.65±0.02 | 4099±123 | [13] | |
TOI-2427 b | 0.161±0.011 | 1.3060011±0.0000102 | 0.0202±0.0002 | 1117±46 | transit | 93.1 | 0.64±0.02 | 4072±121 | [13] | |
TOI-2445 b | 0.112±0.007 | 0.3711281±0.0000005 | 0.0064±0.0001 | 1060±54 | transit | 158.7 | 0.25±0.01 | 3333±157 | [13] | |
Gliese 3929 b | 0.0038±0.0013 | 0.103±0.004 | 2.6162745±0.000003 | 0.02569±0.00088 | 568.8+9.4 −9.3 |
transit | 51.64±0.02 | 0.309±0.014 | 3369±51 | Another planet in system is suspected[14] |
TOI-1759 b | 0.021±0.06 | 0.279±0.02 | 18.849975±0.000006 | 0.1176±0.0013 | 433±14 | transit | 130.85±0.05 | 0.606±0.020 | 4065±51 | [15][16] |
Kepler-451 c | 1.61±0.14 | 1460±90 | 2.1±0.2 | timing | 1340±20 | 0.48+0.12 | [17] | |||
Kepler-451 d | 1.76±0.18 | 43.0±0.1 | 0.20±0.03 | timing | 1340±20 | 0.48+0.12 | [17] | |||
KMT-2021-BLG-1391b | 0.0143±0.0073 | 2.29+0.56 −0.71 |
microlensing | 19000+3000 −5000 |
0.37±0.19 | [18] | ||||
KMT-2021-BLG-1253b | 0.0599+0.0643 −0.0319 |
1.52+0.57 −0.41 |
microlensing | 22000+3000 −4000 |
0.24+0.26 −0.13 |
[18] | ||||
KMT-2021-BLG-1372b | 0.1928±0.1129 | 2.37±0.77 | microlensing | 19000+5000 −8000 |
0.42±0.25 | [18] | ||||
KMT-2021-BLG-0748b | 0.45+0.40 −0.25 |
2.43±0.67 | microlensing | 20000+3000 −4000 |
0.36+0.32 −0.20 |
[18] | ||||
Proxima Centauri d | 0.0008±0.0002 | 5.122+0.002 −0.0036 |
0.02885+0.00019 −0.00022 |
360 | radial vel. | 4.2465±0.0003 | 0.1221±0.0022 | 2900±100 | [19] | |
TOI-1268 b | 0.303±0.026 | 0.81±0.05 | 8.1577080±0.0000044 | 0.072+0.009 −0.010 |
919 | transit | 359.1±0.4 | 0.92±0.03 | 5290±117 | [20] |
TOI-2136 b | 0.0200+0.0077 −0.0072 |
0.196±0.015 | 7.851928+0.000018 −0.000016 |
0.057±0.006 | 395+24 −22 |
transit | 108.82±0.07 | 0.34±0.02 | 3342±100 | [21][22] |
PSR J2007+3120 b | 0.0072±0.0009 | 723±8 | timing | 22000 | Pulsar planet, another planet in the system is suspected.[23] | |||||
Pi Mensae d | 0.0421±0.0042 | 124.64+0.48 −0.52 |
radial vel. | 59.62±0.07 | 1.11±0.01 | 6013±18 | [24] | |||
K2-365 b | 0.0272±0.0172 | 0.259+0.017 −0.015 |
23.448172+0.00076 −0.00099 |
710 | transit | 0.823+0.369 −0.25 |
5561±138 | [25] | ||
K2-366 b | 0.0199±0.0115 | 0.210+0.016 −0.014 |
15.93703+0.00079 −0.00114 |
770 | transit | 0.825+0.366 −0.255 |
5601±138 | [25] | ||
K2-367 b | 0.0203±0.0126 | 0.215+0.020 −0.017 |
20.64509+0.00099 −0.00137 |
450 | transit | 0.756+0.231 −0.347 |
4348±128 | [25] | ||
K2-368 b | 0.0073±0.0042 | 0.118+0.009 −0.008 |
5.02559+0.00028 −0.00034 |
800 | transit | 0.746+0.334 −0.232 |
4663±138 | [25] | ||
K2-368 c | 0.0078±0.0041 | 0.121+0.010 −0.009 |
9.66018±0.00116 | 650 | transit | 0.746+0.334 −0.232 |
4663±138 | [25] | ||
K2-368 d | 0.0146±0.0085 | 0.173+0.013 −0.012 |
20.20108+0.00235 −0.00273 |
500 | transit | 0.746+0.334 −0.232 |
4663±138 | [25] | ||
K2-369 b | 0.0069±0.0040 | 0.117+0.009 −0.008 |
5.76161+0.00084 −0.00071 |
1080 | transit | 0.735+0.334 −0.224 |
5682±138 | [25] | ||
K2-370 b | 0.0327±0.0207 | 0.286+0.020 −0.048 |
2.14084+0.00003 −0.00004 |
1420 | transit | 0.984+0.428 −0.303 |
5377±138 | [25] | ||
K2-371 b | 4.7±2.2 | 1.162+0.082 −0.077 |
3.11490±0.00001 | 1000 | transit | 0.958+0.44 −0.298 |
4925±138 | [25] | ||
K2-372 b | 0.0289±0.0168 | 0.262±0.006 | 9.84407+0.00056 −0.00057 |
870 | transit | 0.847+0.101 −0.088 |
5479±27 | [25] | ||
K2-373 b | 0.0162±0.0089 | 0.184+0.013 −0.012 |
11.02066+0.00143 −0.00136 |
1130 | transit | 1.158+0.499 −0.349 |
6138±138 | [25] | ||
K2-374 b | 0.0113±0.0058 | 0.142±0.005 | 4.52195+0.00032 −0.00040 |
1210 | transit | 0.731+0.067 −0.061 |
5789±21 | [25] | ||
K2-374 c | 0.0179±0.0109 | 0.197+0.008 −0.007 |
16.43445+0.00237 −0.00270 |
790 | transit | 0.731+0.067 −0.061 |
5789±21 | [25] | ||
K2-375 b | 0.0183±0.0106 | 0.200+0.016 −0.015 |
14.45389+0.00477 −0.00417 |
1000 | transit | 1.119+0.492 −0.344 |
5822±138 | [25] | ||
K2-376 b | 0.0129±0.0074 | 0.155+0.011 −0.010 |
5.77647+0.00026 −0.00023 |
1240 | transit | 0.908+0.394 −0.281 |
5937±138 | [25] | ||
K2-377 b | 0.0123±0.0073 | 0.151+0.013 −0.011 |
12.83223+0.00155 −0.00161 |
530 | transit | 0.821+0.371 −0.258 |
4200±138 | [25] | ||
K2-378 b | 0.0283±0.0173 | 0.257+0.024 −0.020 |
2.06043+0.00011 −0.00007 |
1130 | transit | 0.923+0.425 −0.291 |
4823±138 | [25] | ||
K2-379 b | 0.0175±0.0104 | 0.194+0.032 −0.017 |
8.77724+0.00062 −0.00061 |
680 | transit | 0.856+0.375 −0.265 |
4603±138 | [25] | ||
K2-380 b | 0.0250±0.0144 | 0.243+0.016 −0.015 |
9.40131+0.00046 −0.00050 |
1110 | transit | 0.993+0.416 −0.302 |
5911±138 | [25] | ||
K2-381 b | 0.0040±0.0026 | 0.095+0.012 −0.009 |
7.93893±0.00059 | 670 | transit | 0.754+0.337 −0.239 |
4473±138 | [25] | ||
K2-381 c | 0.0158±0.0094 | 0.178+0.016 −0.013 |
16.03465+0.00184 −0.00157 |
530 | transit | 0.754+0.337 −0.239 |
4473±138 | [25] | ||
K2-381 d | 0.0121±0.0070 | 0.150+0.016 −0.012 |
26.80302+0.00277 −0.00304 |
440 | transit | 0.754+0.337 −0.239 |
4473±138 | [25] | ||
K2-382 b | 0.0162±0.0101 | 0.185+0.013 −0.011 |
21.70015+0.00202 −0.00191 |
610 | transit | 0.922+0.401 −0.284 |
5452±138 | [25] | ||
K2-383 b | 0.0102±0.0052 | 0.139+0.010 −0.009 |
1.86596±0.00001 | 1270 | transit | 1.061+0.459 −0.327 |
5129±138 | [25] | ||
K2-384 b | 0.0040±0.0026 | 0.096+0.020 −0.005 |
2.23152+0.0019 −0.00032 |
600 | transit | 0.330±0.009 | 3623±138 | [25] | ||
K2-384 c | 0.0054±0.0027 | 0.106+0.004 −0.006 |
4.19476+0.00030 −0.00018 |
480 | transit | 0.330±0.009 | 3623±138 | [25] | ||
K2-384 d | 0.0085±0.0044 | 0.124+0.010 −0.006 |
6.67958+0.00071 −0.00049 |
410 | transit | 0.330±0.009 | 3623±138 | [25] | ||
K2-384 e | 0.0075±0.0042 | 0.120+0.012 −0.007 |
9.71504+0.00100 −0.00073 |
370 | transit | 0.330±0.009 | 3623±138 | [25] | ||
K2-384 f | 0.0179±0.0104 | 0.198+0.008 −0.007 |
13.62749+0.00034 −0.00057 |
330 | transit | 0.330±0.009 | 3623±138 | [25] | ||
K2-385 b | 0.0100±0.0056 | 0.137+0.012 −0.011 |
2.38086+0.00016 −0.00021 |
1100 | transit | 1370±20 | 0.9270+0.4120 −0.2860 |
4844±138 | [25] | |
K2-386 b | 0.0195±0.0115 | 0.207+0.006 −0.005 |
7.47322+0.00037 −0.00031 |
1010 | transit | 1400±30 | 0.911+0.088 −0.083 |
5749±22 | [25] | |
K2-387 b | 0.1430±0.0996 | 0.653±0.023 | 28.73532±0.00099 | 340 | transit | 870±12 | 0.570+0.051 −0.048 |
3572±138 | [25] | |
K2-388 b | 0.0412±0.0263 | 0.326+0.029 −0.020 |
6.33906+0.00022 −0.00018 |
970 | transit | 948±13 | 0.8420+0.3760 −0.2590 |
5367±138 | [25] | |
K2-389 b | 0.0177±0.0103 | 0.195±0.010 | 8.58404+0.00088 −0.00202 |
1050 | transit | 846±9 | 0.8020+0.3570 −0.2460 |
5782±138 | [25] | |
K2-389 c | 0.0165±0.0085 | 0.182+0.013 −0.012 |
20.85133+0.00280 −0.00298 |
780 | transit | 846±9 | 0.8020+0.3570 −0.2460 |
5782±138 | [25] | |
K2-390 b | 0.0636±0.0390 | 0.416+0.027 −0.030 |
3.31279±0.00010 | 1310 | transit | 1490±18 | 0.7890+0.3510 −0.2390 |
5558±138 | [25] | |
K2-391 b | 0.0078±0.0053 | 0.122+0.025 −0.016 |
4.62265+0.00022 −0.00025 |
900 | transit | 1660±50 | 0.7570+0.3410 −0.2400 |
5543±138 | [25] | |
K2-392 b | 0.0140±0.0079 | 0.165+0.014 −0.013 |
15.39872+0.00242 −0.00193 |
840 | transit | 1330±30 | 0.8410+0.3700 −0.2580 |
5726±138 | [25] | |
K2-393 b | 0.0199±0.0127 | 0.210+0.015 −0.014 |
10.41318+0.00093 −0.00069 |
950 | transit | 867±9 | 0.8810+0.3810 −0.2690 |
5678±138 | [25] | |
K2-394 b | 0.0123±0.0063 | 0.151+0.012 −0.011 |
5.09571±0.00011 | 890 | transit | 319.7±1.5 | 0.478+0.214 −0.147 |
4938±138 | [25] | |
K2-395 b | 0.0240±0.0141 | 0.231+0.017 −0.015 |
4.80335+0.00035 −0.00046 |
910 | transit | 935±10 | 0.9520+0.4210 −0.2930 |
5007±138 | [25] | |
K2-395 c | 0.0371±0.0220 | 0.303+0.025 −0.022 |
8.49128+0.00033 −0.00030 |
750 | transit | 935±10 | 0.9520+0.4210 −0.2930 |
5007±138 | [25] | |
K2-396 b | 0.0106±0.0061 | 0.140+0.010 −0.009 |
0.6736±0.00001 | 1990 | transit | 897±9 | 0.9540+0.4290 −0.2930 |
5236±138 | [25] | |
K2-396 c | 0.0314±0.0189 | 0.278+0.015 −0.010 |
25.76051+0.00199 −0.00188 |
590 | transit | 897±9 | 0.9540+0.4290 −0.2930 |
5236±138 | [25] | |
K2-397 b | 0.0212±0.0127 | 0.216±0.016 | 3.57232+0.00018 −0.00015 |
1210 | transit | 650±5 | 0.9370+0.4060 −0.2850 |
5387±138 | [25] | |
K2-398 b | 0.0191±0.0112 | 0.203+0.010 −0.009 |
6.39302+0.00113 −0.00075 |
1240 | transit | 1980±40 | 0.9450+0.0900 −0.0830 |
5946±20 | [25] | |
K2-398 c | 0.0736±0.0412 | 0.455±0.013 | 18.78783+0.00087 −0.00099 |
870 | transit | 1980±40 | 0.9450+0.0900 −0.0830 |
5946±20 | [25] | |
K2-399 b | 0.1015±0.0697 | 0.540+0.093 −0.042 |
0.75997±0.00001 | 2780 | transit | 1680±40 | 0.783+0.131 −0.114 |
5690±38 | [25] | |
K2-400 b | 0.0051±0.0025 | 0.103±0.004 | 3.86505±0.00018 | 570 | transit | 203.5±0.8 | 0.374±0.009 | 3578±138 | [25] | |
K2-401 b | 0.0183±0.0117 | 0.201+0.018 −0.017 |
6.29309+0.00057 −0.00070 |
660 | transit | 655±5 | 0.8700+0.3950 −0.2690 |
4213±138 | [25] | |
K2-402 b | 0.0245±0.0149 | 0.239+0.019 −0.017 |
17.27474+0.00259 −0.00317 |
870 | transit | 1710±60 | 0.9440+0.4190 −0.2900 |
5716±138 | [25] | |
K2-403 b | 0.0783±0.0515 | 0.476+0.031 −0.034 |
33.58977±0.00076 | 580 | transit | 804±8 | 0.7840+0.3400 −0.2410 |
5511±138 | [25] | |
K2-404 b | 0.0230±0.0127 | 0.225±0.007 | 13.11536+0.00044 −0.00060 |
450 | transit | 397±2 | 0.552±0.015 | 3748±138 | [25] | |
K2-405 b | 0.0586±0.0342 | 0.407+0.007 −0.010 |
3.43547±0.00003 | 980 | transit | 643±7 | 1.034+0.459 −0.314 |
4927±138 | [25] | |
K2-406 b | 0.063±0.039 | 0.410+0.027 −0.026 |
22.5494+0.00137 −0.00143 |
720 | transit | 278±2 | 0.7980+0.3390 −0.2450 |
5784±138 | [25] | |
K2-407 b | 0.0066±0.0035 | 0.114+0.008 −0.007 |
4.9419+0.00066 −0.00069 |
1110 | transit | [25] | ||||
K2-407 c | 0.0078±0.0044 | 0.121+0.008 −0.007 |
9.22453+0.00132 −0.00091 |
900 | transit | [25] | ||||
K2-408 b | 0.0122±0.0062 | 0.149+0.010 −0.009 |
20.97895+0.00130 −0.00124 |
610 | transit | [25] | ||||
K2-409 b | 0.0212±0.0127 | 0.221+0.015 −0.014 |
1.90808+0.00004 −0.00005 |
1800 | transit | [25] | ||||
EPIC 206317286 c | 0.0168±0.098 | 0.186+0.015 −0.014 |
17.51547+0.00228 −0.00296 |
570 | transit | 0.832+0.253 −0.367 |
4752±138 | [25] | ||
TOI-1696 b | 0.1781 | 0.276±0.010 | 2.500311±0.000004 | 0.0229±0.0002 | 489±13 | transit | 210.8±0.5 | 0.255±0.0066 | 3185±76 | [26][27] |
TOI-1670 b | 0.04±0.03 | 0.184+0.017 −0.013 |
10.98462+0.00046 −0.00051 |
0.103±0.002 | 1062+14 −13 |
transit | 540.6+1.0 −1.2 |
1.21±0.02 | 6170±61 | [28] |
TOI-1670 c | 0.63+0.09 −0.08 |
0.987±0.025 | 40.74976+0.000022 −0.00021 |
0.249±0.005 | 684±9 | transit | 540.6+1.0 −1.2 |
1.21±0.02 | 6170±61 | [28] |
TOI-3757 b | 0.2684±0.0276 | 1.07+0.04 −0.05 |
3.4387530+0.0000039 −0.0000040 |
0.03845±0.00043 | 759±13 | transit | 579±2 | 0.64±0.02 | 3913±56 | [29] |
TYC 2187-512-1 b | 0.33±0.02 | 691.90+8.77 −8.61 |
1.22±0.02 | radial vel. | 50.512±0.016 | 0.498±0.019 | 3734±54 | [30] | ||
KMT-2021-BLG-1077Lb | 0.22+0.31 −0.12 |
1.26+1.41 −1.08 |
microlensing | 27000±3000 | 0.14+0.19 −0.07 |
[31] | ||||
KMT-2021-BLG-1077Lc | 0.25+0.35 −0.13 |
0.93+1.05 −0.80 |
microlensing | 27000±3000 | 0.14+0.19 −0.07 |
[31] | ||||
K2-2016-BLG-0005Lb | 1.1±0.1 | 4.4+1.9 −0.4 |
4700+3300 −700 |
microlensing | 17000±700 | 0.58±0.03 | [1] | |||
KMT-20109-BLG-1042Lb | 0.19+0.21 −0.11 |
1.7±0.5 | microlensing | 22000+3000 −5000 |
0.30+0.34 −0.18 |
[32] | ||||
KMT-20109-BLG-1552Lb | 4.05+1.73 −1.85 |
2.6+0.6 −0.8 |
microlensing | 15000+6000 −5000 |
0.79+0.33 −0.36 |
[32] | ||||
KMT-20109-BLG-2974Lb | 0.28+0.29 −0.18 |
2.0+0.8 −0.7 |
microlensing | 20000+5000 −7000 |
0.47+0.41 −0.28 |
[32] | ||||
TOI-620 b | 5.0988179+0.0000045 −0.0000046 |
0.04825+0.00065 −0.00066 |
603.6+5.5 −5.3 |
transit | 107.81±0.19 | 0.577+0.024 −0.023 |
3708+57 −56 |
[33] | ||
MOA-2020-BLG-135Lb | 0.036+0.060 −0.021 |
1.11+0.23 −0.20 |
microlensing | 26000±3000 | 0.23+0.39 −0.14 |
[34] | ||||
OGLE-2018-BLG-1126b | 0.056+0.033 −0.031 |
3.23+1.29 −1.71 |
microlensing | 19000+6000 −8000 |
0.69+0.41 −0.38 |
[35] | ||||
KMT-2018-BLG-2004b | 0.27±\0.12 | 4.62+0.80 −1.10 |
microlensing | 23000+3000 −4000 |
0.69+0.32 −0.31 |
[35] | ||||
OGLE-2018-BLG-1647b | 0.97+1.78 −0.56 |
1.36+0.20 −0.17 |
microlensing | 26000+4000 −3000 |
0.092+0.170 −0.053 |
[35] | ||||
OGLE-2018-BLG-1367b | 0.95+0.75 −0.44 |
3.63+1.02 −0.96 |
microlensing | 0.28+0.22 −0.13 |
Multiple solutions for frojected separation[35] | |||||
OGLE-2018-BLG-1544b | 11.2+6.3 −5.9 |
6.21+1.32 −2.10 |
microlensing | 21000+4000 −7000 |
0.62+0.38 −0.36 |
Multiple solutions for frojected separation[35] | ||||
OGLE-2018-BLG-0932b | 0.89+0.36 −0.31 |
1.75+0.24 −0.23 |
microlensing | 22000±3000 | 0.72+0.29 −0.25 |
[35] | ||||
OGLE-2018-BLG-1212b | 0.20+0.16 −0.13 |
1.68+1.47 −0.63 |
microlensing | 5100+4100 −1800 |
0.16+0.12 −0.10 |
[35] | ||||
KMT-2018-BLG-2718b | 16.0+11.7 −8.0 |
4.86+2.97 −2.55 |
microlensing | 15000+10000 −7000 |
0.82+0.57 −0.39 |
[35] | ||||
HD 83443 c | 1.5+0.5 −0.2 |
8241+1019 −530 |
8.0±0.8 | radial vel. | 133.6±0.2 | 1.00±0.03 | 5442±17 | Eccentric orbit due to hot Jupiter in system[36] | ||
OGLE-2019-BLG-1470LABc | 2.2+1.8 −1.3 |
3.1+1.2 −1.1 |
microlensing | 20000±4000 | 0.55+0.17 | Circumbinary planet[37] | ||||
Gliese 514b | 0.0164±0.0028 | 140.43±0.41 | 0.422+0.014 −0.015 |
202±11 | radial vel. | 24.850±0.010 | 0.510±0.051 | 3714±51 | Planetary orbit partially in habitable zone[38] | |
TOI-1710 b | 0.0890±0.0148 | 0.477±0.010 | 24.283429±0.00043 | 0.16±0.04 | 687±50 | transit | 264.7±0.2 | 0.984+0.050 −0.059 |
5665±55 | [39] |
HD 260655 b | 0.0067±0.0011 | 0.111±0.002 | 2.76953±0.00003 | 0.02933±0.00024 | 709±4 | transit | 32.63±0.07 | 0.439±0.011 | 3803±10 | Host star also known as TOI-4599[40] |
HD 260655 c | 0.0097±0.0015 | 0.137±0.004 | 5.70588±0.00007 | 0.04749±0.00039 | 557±3 | transit | 32.63±0.07 | 0.439±0.011 | 3803±10 | Host star also known as TOI-4599[40] |
KMT-2021-BLG-0240 b | 0.40+0.07 −0.08 |
2.5+2.8 −1.9 |
microlensing | 23000+3000 −5000 |
0.47+0.33 −0.24 |
Multiple solutions for orbital separation[41] | ||||
KMT-2021-BLG-0240 c | 0.64+0.25 −0.24 |
1.0+1.1 −0.8 |
microlensing | 23000+3000 −5000 |
0.47+0.33 −0.24 |
Multiple solutions for orbital separation[41] | ||||
KMT-2021-BLG-1898 b | 0.73+0.50 −0.40 |
1.9+0.3 −0.5 |
microlensing | 23000+3000 −4000 |
0.48+0.33 −0.26 |
Possibly a binary star system[42] | ||||
TOI-1246 b | 0.0255±0.0035 | 0.269±0.005 | 4.30744±0.00002 | 0.049±0.002 | 955 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | [43] |
TOI-1246 c | 0.0277±0.0038 | 0.224±0.007 | 5.904144±0.000083 | 0.061±0.002 | 860 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | [43] |
TOI-1246 d | 0.0167±0.0053 | 0.313±0.008 | 18.65590±0.00048 | 0.131±0.004 | 586 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | [43] |
TOI-1246 e | 0.0466±0.0072 | 0.338±0.014 | 37.9216±0.0010 | 0.211±0.007 | 462 | transit | 557.9±1.0 | 1.12±0.16 | 5217±50 | [43] |
HIP 94235 b | 0.268±0.027 | 7.713057±0.000021 | 0.07870+0.00056 −0.00017 |
1060±50 | transit | 191.2±0.4 | 1.094+0.024 −0.007 |
5991±50 | Host star also known as TOI-4399, also red dwarf in the system[44] | |
HIP 34269 b | 0.0052±0.0007 | 0.103±0.005 | 0.548177±0.000019 | 0.01188±0.00040 | 1617±41 | transit | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500[45] |
HIP 34269 c | 0.0146±0.0016 | 6.6356±0.0040 | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500[45] | |||
HIP 34269 d | 0.1055±0.0033 | 26.233±0.020 | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500[45] | |||
HIP 34269 e | 0.0376±0.0042 | 61.30±0.28 | radial vel. | 154.81±0.15 | 0.740±0.017 | 4440±100 | Host star also known as TOI-500[45] | |||
TOI-1820 b | 2.3±0.2 | 1.12±0.02 | 4.860700±0.000010 | 0.069±0.005 | 1295±11 | transit | 807±13 | 1.04±0.13 | 5734±50 | [46] |
TOI-2025 b | 4.4±0.4 | 1.120±0.009 | 8.872086±0.000009 | 0.089±0.004 | 1186±11 | transit | 1106±7 | 1.32±0.14 | 5880±53 | [46] |
TOI-2158 b | 0.82±0.08 | 0.960±0.012 | 8.60077±0.00003 | 0.075±0.004 | 1188±10 | transit | 652±3 | 1.12±0.12 | 5673±50 | [46] |
HIP 63374 B | 11±3 | 30.02±0.12 | imaging | 176.4±0.3 | 1.211±0.006 | [47] | ||||
HIP 60584 B | 8±3 | 16.58±0.15 | imaging | 99.60±0.12 | 1.352±0.014 | [47] | ||||
TOI-1181 b | 1.18±0.14 | 1.30±0.08 | 2.103195+0.000012 −0.000011 |
2162 | transit | 1013±3 | 1.38+0.086 −0.082 |
6260±100 | Subjiant host star[48] | |
TOI-1516 b | 3.16±0.12 | 1.36±0.03 | 2.056014±0.000002 | 1820 | transit | 804.6±1.9 | 1.085+0.061 −0.066 |
6420±100 | [48] | |
TOI-2046 b | 2.30±0.08 | 1.44±0.11 | 1.4971842+0.0000031 −0.0000033 |
1998 | transit | 940±3 | 1.153+0.100 −0.093 |
6160±100 | Young host star[48] | |
WASP-132c | 0.165±0.009 | 1.011534±0.000005 | 0.0182±0.0003 | transit | 390 | 0.782±0.034 | 4714+87 −88 |
[49] | ||
TOI-1811 b | 0.974+0.075 −0.076 |
1.002+0.026 −0.024 |
3.7130818±0.0000028 | 0.04393+0.00058 −0.00054 |
961.5±8 | transit | 418±3 | 0.819+0.033 −0.030 |
4753+54 −55 |
[50] |
TOI-2025 b | 3.51+0.36 −0.35 |
1.118+0.031 −0.030 |
8.8720942+0.0000080 −0.0000079 |
0.0886+0.0019 −0.0024 |
1172+18 −17 |
transit | 1095±11 | 1.176+0.079 −0.091 |
5928+76 −75 |
[50] |
TOI-2145 b | 5.35+0.32 −0.35 |
1.103+0.031 −0.029 |
10.261081+0.000026 −0.000027 |
0.1108+0.0012 −0.0015 |
1484+16 −14 |
transit | 733±5 | 1.720+0.057 −0.068 |
6189±67 | Host star also known as HIP 86040[50] |
TOI-2152A b | 2.83+0.38 −0.37 |
1.281+0.050 −0.046 |
3.3773512+0.0000060 −0.0000061 |
0.05064+0.00093 −0.0011 |
1802+60 −54 |
transit | 988±13 | 1.516+0.085 −0.10 |
6630+300 −290 |
Planet orbiting primary of binary star[50] |
TOI-2154 b | 0.92+0.19 −0.18 |
1.453+0.053 −0.048 |
3.8240801±0.0000025 | 0.0513+0.0011 −0.0013 |
1580±27 | transit | 967±10 | 1.233+0.077 −0.090 |
6280±160 | [50] |
TOI-2497 b | 5.21±0.52 | 1.000+0.040 −0.038 |
10.655661±0.000026 | 0.1167+0.0018 −0.0017 |
1596+44 −41 |
transit | 930±14 | 1.861+0.086 −0.081 |
7360+290 −270 |
[50] |
Mu2 Scorpii b | 14.4 | ? | ? | 290 | ? | direct imaging | 474 | 9.1 | 21900 | [51] |
Mu2 Scorpii c | 18.5 | ? | ? | 21 | ? | direct imaging | 474 | 9.1 | 21900 | [51] |
HD 28109 b | 0.058+0.029 −0.024 |
0.196±0.009 | 22.89104+0.00035 −0.00036 |
0.1357±0.0034 | 881.2±7.5 | transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | [52] |
HD 28109 c | 0.025+0.013 −0.010 |
0.378±0.010 | 56.00819+0.00194 −0.00202 |
0.308±0.011 | 585.2+8.7 −8.3 |
transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | [52] |
HD 28109 d | 0.018+0.009 −0.007 |
0.290±0.010 | 84.25999+0.00744 −0.00662 |
0.411±0.016 | 506.5+8.7 −8.0 |
transit | 457.0±0.6 | 1.26±0.08 | 6120±50 | [52] |
TOI-2193 b | 0.94±0.18 | 1.77 | 2.1225735±0.0000016 | 0.03319+0.00052 −0.00051 |
1763+21 −22 |
transit | 1126±3 | 1.082+0.052 −0.049 |
5974±110 | Also Also 0.54M☉ star in the system[53] |
TOI-2207 b | 0.64+0.10 −0.12 |
0.995+0.028 −0.027 |
8.001968+0.000024 −0.000025 |
0.0854+0.0015 −0.0016 |
16|15}} | transit | 1242±9 | 1.296+0.069 −0.072 |
6075±110 | [53] |
TOI-2236 b | 1.58+0.40 −0.39 |
1.282+0.032 −0.031 |
3.5315902±0.0000026 | 0.05009+0.00080 −0.00082 |
1688+19 −21 |
transit | 1149±5 | 1.343+0.066 −0.065 |
6164±50 | [53] |
TOI-2421 b | 0.333±0.079 | 0.925+0.035 −0.034 |
4.3474032+0.0000079 −0.0000078 |
0.0543+0.0021 −0.0010 |
1534+20 −28 |
transit | 1067±7 | 1.131+0.130 −0.064 |
5577±50 | [53] |
TOI-2567 b | 0.201+0.034 −0.031 |
0.975+0.031 −0.029 |
5.983944±0.000013 | 0.0672+0.0024 −0.0012 |
1352+18 −19 |
transit | 1691±8 | 1.130+0.130 −0.059 |
5650±50 | [53] |
TOI-2570 b | 0.820+0.063 −0.065 |
1.217+0.035 −0.034 |
±|0.0000022}} | 0.04145+0.00081 −0.00086 |
1431+24 −23 |
transit | 1179±6 | 1.063+0.063 −0.065 |
5765±50 | [53] |
TOI-3331 b | 2.27±0.16 | 1.158±0.043 | 2.0180231+0.0000043 −0.0000044 |
0.03144+0.00048 −0.00055 |
1488+31 −29 |
transit | 733±4 | 1.016+0.047 −0.052 |
5521±110 | Also Also 0.6M☉ star in the system[53] |
TOI-3540 b | 1.18±0.14 | 2.10 | 3.1199990±0.0000079 | 0.04289+0.00092 −0.00093 |
1498±22 | transit | 921±10 | 1.081+0.071 −0.069 |
5969±50 | Also 0.8M☉ star in the system[53] |
TOI-3693 b | 1.02+0.24 −0.22 |
1.124+0.029 −0.023 |
9.088516+0.000026 −0.000027 |
0.0813+0.0011 −0.0012 |
801+13 −12 |
transit | 576±2 | 0.867+0.036 −0.037 |
5274±50 | [53] |
TOI-4137 b | 1.44+0.17 −0.15 |
1.211+0.040 −0.039 |
3.8016122±0.0000065 | 0.05222+0.00089 −0.00096 |
1570+25 −24 |
transit | 1128±7 | 1.313+0.068 −0.071 |
6134±50 | [53] |
OGLE-2017-BLG-1691Lb | 0.046+0.037 −0.025 |
2.41+0.34 −0.44 |
microlensing | 24000+3000 −4000 |
0.45+0.36 −0.25 |
Host star also known as KMT-2017-BLG-0752[54] | ||||
KMT-2021-BLG-0320Lb | 0.10+0.13 −0.07 |
1.54+0.24 −0.30 |
microlensing | 23000+3000 −4000 |
0.32+0.39 −0.21 |
[54] | ||||
KMT-2021-BLG-1303Lb | 0.38+0.22 −0.20 |
2.89+0.44 −0.66 |
microlensing | 20000+3000 −5000 |
0.57+0.32 −0.29 |
Host star also known as MOA-2021-BLG-182[54] | ||||
KMT-2021-BLG-1554Lb | 0.12+0.20 −0.07 |
0.72+0.13 −0.14 |
microlensing | 25000+3000 −4000 |
0.08+0.13 −0.04 |
[54] | ||||
TOI-1107b | 3.35±0.18 | 1.30±0.05 | 4.0782387+0.0000024 −0.0000025 |
0.0561+0.0024 −0.0025 |
1728±27 | transit | 925±7 | 1.35±0.08 | 6311±98 | [55] |
Ross 508 b | 0.0126±0.0019 | 10.76+0.01 −0.02 |
0.05353+0.00047 −0.00051 |
radial vel. | 36.594±0.011 | 0.1774±0.0045 | 3071+34 −22 |
Host star also known as Gliese 585, planet close to habitable zone.[56] | ||
KMT-2021-BLG-0171Lb | 0.0352+0.0173 −0.0142 |
3.5+1.3 −1.0 |
microlensing | 15000+5000 −4000 |
0.78+0.29 −0.26 |
[57] | ||||
KMT-2021-BLG-1689Lb | 0.145+0.094 −0.072 |
2.5+0.8 −06 |
microlensing | 23000+2000 −4000 |
0.58+0.33 −0.27 |
[57] |
Specific exoplanet lists
- Lists of exoplanets
- List of exoplanets discovered before 2000 (32)
- List of exoplanets discovered between 2000–2009 (379)
- List of exoplanets discovered in 2010 (108)
- List of exoplanets discovered in 2011 (177)
- List of exoplanets discovered in 2012 (148)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (878)
- List of exoplanets discovered in 2015 (151)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (152)
- List of exoplanets discovered in 2018 (314)
- List of exoplanets discovered in 2019 (191)
- List of exoplanets discovered in 2020 (260)
- List of exoplanets discovered in 2021 (243)
- List of exoplanets discovered in 2022 (179)
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered using the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of transiting exoplanets
References
- ^ a b Specht, D.; et al. (31 March 2022). "Kepler K2 Campaign 9: II. First space-based discovery of an exoplanet using microlensing". arxiv. Retrieved 4 April 2022.
- ^ Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert. Retrieved 4 April 2022.
- ^ a b c Ottoni, G.; Udry, S.; Ségransan, D.; et al. (22 December 2021). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy & Astrophysics. EDP Sciences. arXiv:2201.01528. doi:10.1051/0004-6361/202040078. ISSN 0004-6361. S2CID 245440163.
- ^ Pezzotti, C.; Ottoni, G.; Buldgen, G.; et al. (22 April 2021). "Coralie radial-velocity search for companions around evolved stars (CASCADES). III. A new Jupiter host-star: in-depth analysis of HD29399 using TESS data". Astronomy & Astrophysics. EDP Sciences. arXiv:2201.01553. doi:10.1051/0004-6361/202040080. ISSN 0004-6361. S2CID 242974999.
- ^ Kipping, David; Bryson, Steve; et al. (13 January 2022). "An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i". Nature. Retrieved 13 January 2022.
- ^ "Kepler-1708". NASA Exoplanet Archive. Retrieved 13 January 2022.
- ^ a b A pair of Sub-Neptunes transiting the bright K-dwarf TOI-1064 characterised with CHEOPS, 2022, arXiv:2201.03570
- ^ a b c TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars, 2022, arXiv:2201.04140
- ^ The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 day Orbit with the Automated Planet Finder Telescope, 2022, arXiv:2201.04146
- ^ OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in Galactic Bulge, 2022, arXiv:2201.04312
- ^ a b Two gas giants transiting M dwarfs confirmed with HPF and NEID, 2022, arXiv:2201.09963
- ^ a b Alleviating the Transit Timing Variations bias in transit surveys. II. RIVERS: Twin resonant Earth-sized planets around Kepler-1972 recovered from Kepler's false positive, 2022, arXiv:2201.11459
- ^ a b c d e f g h i j k l m Validation of 13 Hot and Potentially Terrestrial TESS Planets, 2022, arXiv:2201.12661
- ^ Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b, 2022, arXiv:2202.00970
- ^ A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS, 2022, arXiv:2202.01240
- ^ TOI-1759 b: a transiting sub-Neptune around a low mass star characterized with SPIRou and TESS, 2022, arXiv:2202.01259
- ^ a b Detection of two additional circumbinary planets around Kepler-451, 2022, arXiv:2202.02118
- ^ a b c d Mass Production of 2021 KMTNet Microlensing Planets I, 2022, arXiv:2202.03022
- ^ A candidate short-period sub-Earth orbiting Proxima Centauri, 2022, arXiv:2202.05188
- ^ TOI-1268b: the youngest hot Saturn-mass transiting exoplanet, 2022, arXiv:2201.13341
- ^ TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136, 2022, arXiv:2202.10024
- ^ Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf, 2022, arXiv:2202.10182
- ^ A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme, 2022, arXiv:2203.01136
- ^ A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125-d Orbit, 2022, arXiv:2203.01018
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18, 2022, arXiv:2203.02087
- ^ TOI-1696: a nearby M4 dwarf with a 3R⊕ planet in the Neptunian desert, 2022, arXiv:2203.02694
- ^ TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF, 2022, arXiv:2204.09063
- ^ a b TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration, 2022, arXiv:2203.04334
- ^ TOI-3757 b: A low density gas giant orbiting a solar-metallicity M dwarf, 2022, arXiv:2203.07178
- ^ The CARMENES search for exoplanets around M dwarfs Two Saturn-mass planets orbiting active stars, 2022, arXiv:2203.16504
- ^ a b KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing, 2022, arXiv:2203.16734
- ^ a b c Systematic KMTNet Planetary Anomaly Search. IV. Complete Statistical Sample of 2019 Prime-Field Microlensing Planets, 2022, arXiv:2204.02017
- ^ A close-in puffy Neptune with hidden friends: The enigma of TOI 620, 2022, arXiv:2204.03108
- ^ MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis, 2022, arXiv:2204.03672
- ^ a b c d e f g h Systematic KMTNet Planetary Anomaly Search. V. Complete Sample of 2018 Prime-Field, 2022, arXiv:2204.04354
- ^ HD 83443c: A highly eccentric giant planet on a 22-year orbit, 2022, arXiv:2204.05711
- ^ OGLE-2019-BLG-1470LABc: Another Microlensing Giant Planet in a Binary System, 2022, arXiv:2204.05606
- ^ A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514 A super-Earth on an eccentric orbit moving in and out of the habitable zone, 2022, arXiv:2204.06376
- ^ A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE and HARPS-N, 2022, arXiv:2204.08984
- ^ a b The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc, 2022, arXiv:2204.10261
- ^ a b KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal, 2022, arXiv:2204.11383
- ^ KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars, 2022, arXiv:2204.11378
- ^ a b c d {{citation|arxiv=2204.11895|year=2022|title=The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
- ^ A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor member HIP 94235, 2022, arXiv:2204.11975
- ^ a b c d A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system, 2022, arXiv:2204.13573
- ^ a b c FIES and Tull confirm and characterise three giant planets delivered by TESS, 2022, arXiv:2204.13956
- ^ a b c TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant and a normal star, 2022, arXiv:2205.01860
- ^ The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b, 2022, arXiv:2205.02501
- ^ a b c d e f Another Shipment of Six Short-Period Giant Planets from TESS, 2022, arXiv:2205.05709
- ^ a b A scaled-up planetary system around a supernova progenitor, 2022, arXiv:2205.02279
- ^ a b c HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica, 2022, arXiv:2205.09046
- ^ a b c d e f g h i j The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets, 2022, arXiv:2205.09728
- ^ a b c d Four sub-Jovian-mass planets detected by high-cadence microlensing surveys, 2022, arXiv:2205.10510
- ^ Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars, 2022, arXiv:2205.10854
- ^ A Super-Earth Orbiting Near the Inner Edge of the Habitable Zone around the M4.5-dwarf Ross 508, 2022, arXiv:2205.11986
- ^ a b KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: Two Microlensing Planets in the KMTNet High-cadence Fields with Followup Observations, 2022, arXiv:2205.12584