List of exoplanets discovered in 2022
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 |
---|---|---|---|---|---|---|---|---|---|---|
29 Cygni b | 13.9+6.1 −5.1 | 16.9+3.4 −1.9 | astrometry + imaging | 130.9±0.9 | 2.14±0.15 | 8790+1513 −1292 | Host star also known as HIP 99770[3] | |||
CoRoT-35b | 1.10±0.37 | 1.68±0.11 | 3.22748±0.00008 | 0.04290±0.00092 | 1747±62 | transit | 3700±200 | 1.01+0.07 −0.06 | 6390±130 | [4] |
CoRoT-36b | 0.68+0.47 −0.43 | 1.41±0.14 | 5.616531±0.000023 | 0.066±0.007 | 1567±35 | transit | 3110±60 | 1.32±0.09 | 6730±140 | [4] |
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 | [5] | ||
EPIC 210768568 b | 0.088±0.004 | 3.2141±0.0002 | 0.0511+0.0021 −0.0028 | transit | 965 | 1.018±0.131 | 5711±105 | [6] | ||
EPIC 246078343 b | 0.068±0.007 | 0.8094±0.00003 | 0.0117+0.0009 −0.0012 | transit | 954 | 0.808+0.364 −0.256 | 4116±138 | [6] | ||
EPIC 246078343 c | 0.110±0.006 | 5.3301±0.0003 | 0.0426+0.0016 −0.0019 | transit | 954 | 0.808+0.364 −0.256 | 4116±138 | [6] | ||
EPIC 246220667 b | 0.172±0.006 | 6.6690±0.0002 | 0.0552+0.0017 −0.0023 | transit | 835 | 0.814+0.363 −0.251 | 4343±138 | [6] | ||
EPIC 246220667 c | 0.109±0.006 | 4.3696±0.0001 | 0.0487+0.0027 −0.0031 | transit | 835 | 0.814+0.363 −0.251 | 4343±138 | [6] | ||
EPIC 247422570 b | 0.189±0.009 | 5.9382+0.0006 −0.0004 | 0.0586+0.0032 −0.0033 | transit | 2181 | 0.893+0.406 −0.275 | 5590±138 | [6] | ||
Gaia-1b | 1.68±0.11 | 1.229±0.021 | 3.052524±0.000017 | 0.04047±0.00094 | transit | 1201±7 | 0.949±0.066 | 5470±110 | First confirmed exoplanet discovered by Gaia, along with Gaia-2b[7] | |
Gaia-2b | 0.817±0.047 | 1.322±0.013 | 3.6915224±0.0000039 | 0.0467±0.0015 | transit | 676±3 | 1.000±0.095 | 5720±84 | First confirmed exoplanet discovered by Gaia, along with Gaia-1b[7] | |
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[8] | |
Gliese 1002 b | 0.0034±0.0004 | 10.3465±0.027 | 0.0457±0.0013 | 230.9±6.7 | radial vel. | 15.808±0.003 | 0.120±0.010 | 3024±52 | Planet in habitable zone[9] | |
Gliese 1002 c | 0.0043±0.0005 | 21.202±0.013 | 0.0738±0.0021 | 181.7±5.2 | radial vel. | 15.808±0.003 | 0.120±0.010 | 3024±52 | Planet in habitable zone[9] | |
Gliese 3929 b | 0.0055±0.0014 | 0.097±0.004 | 2.6162745±0.000003 | 0.0252±0.0005 | 568±6 | transit | 51.64±0.02 | 0.309±0.014 | 3369±51 | Another planet in system is suspected[10][11] |
Gliese 3929 c | 0.0180±0.0029 | 15.04±0.03 | 0.081±0.002 | 317±3 | radial vel. | 51.64±0.02 | 0.309±0.014 | 3369±51 | [11] | |
GJ 463 b | 3.6±0.4 | 3448+110 −88 | 3.53±0.07 | radial vel. | 59.91±0.03 | 0.49±0.02 | 3540±41 | Host star also known as Ross 690[12][13] | ||
GJ 3090 b | 0.0105 | 0.19 | 2.8531042±0.0000032 | 0.03165 | 696 | transit | 73.21±0.04 | 0.519±0.013 | 3556±70 | Host star also known as TOI-177[14] |
GJ 3090 c | 0.0538 | 12.734+0.033 −0.026 | 0.08575 | 421 | radial vel. | 73.21±0.04 | 0.519±0.013 | 3556±70 | Host star also known as TOI-177[14] | |
HD 3167 e | 0.0306±0.0037 | 102.09+0.52 −0.50 | 0.4048+0.0077 −0.0074 | 375±7 | radial vel. | 154.59±0.13 | 0.852+0.026 −0.015 | 5300±73 | [15] | |
HD 18599 b | 0.0758+0.0223 −0.0242 | 0.232±0.012 | 4.1374354+0.0000036 −0.0000037 | 0.0480±0.0004 | 935±11 | transit | 126.02±0.06 | 0.863±0.020 | 5145±50 | Host star also known as TOI-179, also red dwarf star in the system[16][17][18] |
HD 20329b | 0.0233±0.0034 | 0.154±0.006 | 0.926118+0.000050 −0.000043 | 0.0180±0.0003 | 2141±27 | transit | 207.7±0.9 | 0.90±0.05 | 5596±50 | [19] |
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[20] | ||
HD 22946 b | 0.154±0.009 | 4.040301+0.000023 −0.000042 | 0.0528±0.0030 | 1378±36 | transit | 205.08±0.16 | 1.158±0.058 | 6210+173 −158 | Host star also known as TOI-411, third transiting planet in system is suspected[21] | |
HD 22946 c | 0.245±0.013 | 9.573096+0.000026 −0.000023 | 0.0939±0.0054 | 1033±27 | transit | 205.08±0.16 | 1.158±0.058 | 6210+173 −158 | Host star also known as TOI-411, third transiting planet in system is suspected[21] | |
HD 23472 d | 0.0017±0.0006 | 0.067±0.005 | 3.97664+0.000030 −0.000044 | 0.04298+0.00063 −0.00065 | 909+35 −32 | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | [22] |
HD 23472 e | 0.0023±0.0009 | 0.073±0.006 | 7.90754±0.00011 | 0.0680±0.0010 | 723+28 −25 | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | [22] |
HD 23472 f | 0.0024±0.0013 | 0.102±0.007 | 12.1621839+0.00012 −0.000099 | 0.0906±0.0014 | 630+27 −23 | transit | 127.48±0.06 | 0.67±0.03 | 4684±99 | [22] |
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 | [23] |
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 | [23] |
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 | [23] |
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[24] | ||
HD 33142 d | 0.89+0.06 −0.05 | 810.2+3.8 −4.2 | 1.955+0.016 −0.012 | radial vel. | 394.3±0.9 | 1.52±0.03 | 5025.4+23.6 −15.5 | Giant host star[25] | ||
HD 56414 b | 0.0944±0.0053 | 0.331±0.018 | 29.04992±0.00021 | 0.229±0.004 | 1133±30 | transit | 873±3 | 1.89±0.11 | 8500±150 | Host star also known as TOI-1228[26] |
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[20] | ||
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[20] | ||
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[27] | ||
HD 93963A b | 0.121±0.004 | 1.0391353+0.0000049 −0.0000045 | 0.02085±0.00037 | 2042±27 | transit | 268.6±1.3 | 1.109±0.043 | 5987±64 | Host star also known as TOI-1797[28] | |
HD 93963A c | 0.288±0.005 | 3.6451398+0.0000106 −0.0000142 | 0.04813±0.00085 | 1344±18 | transit | 268.6±1.3 | 1.109±0.043 | 5987±64 | Host star also known as TOI-1797[28] | |
HD 109833 b | 0.258+0.014 −0.012 | 9.188526±0.000026 | transit | 259.5±0.2 | 1.08±0.05 | 5881±50 | Young host star also known as TOI-1097[29] | |||
HD 109833 c | 0.231+0.018 −0.016 | 13.900148±0.000057 | transit | 259.5±0.2 | 1.08±0.05 | 5881±50 | Young host star also known as TOI-1097[29] | |||
HD 114082 b | 8.0±1.0 | 1.00±0.03 | 109.75+0.40 −0.37 | 0.5109+0.0081 −0.0083 | transit | 310.1±0.7 | 1.47±0.07 | 6651±35 | Young star, eccentric planetary orbit[30][31] | |
HD 167768 b | 0.85+0.12 −0.11 | 20.6532+0.0032 −0.0032 | 0.1512+0.0058 −0.0063 | 1874 | radial vel. | 353.5 | 1.08+0.14 −0.12 | 4830 | Host red giant star also known as HR 8640, other planets in system are suspected[32] | |
HD 191939 g | 0.0425±0.0063 | 284+10 −8 | 0.812±0.028 | 278±6 | radial vel. | 174.4±0.1 | 0.81±0.04 | 5348±100 | Habitable zone planet[33] | |
HD 191939 f | >2.1 | >2200 | >3.2 | <125 | 174.4±0.1 | 0.81±0.04 | 5348±100 | [33] | ||
HD 199981 b | 10.070±2.483 | 21000±8000 | 13.048±3.073 | radial vel. | 66.7±2.4 | Host star also known as GJ 9714[34] | ||||
HD 105618 b | 0.079±0.008 | 9.9 | 0.091±0.004 | radial vel. | 227.8±0.4 | Also brown dwarf in the system[34] | ||||
HD 206893 c | 12.3+1.1 −1.2 | 1.46+0.18 −0.06 | 2082 | 3.53+0.08 −0.07 | 1181.9+20.6 −53.9 | radial vel. | 125.1±2.6 | 1.24 | 6486 | Some deuterium burning despite its low mass, also another brown dwarf is present in the system[35] |
HD 21019 b | 0.014±0.002 | 2.56 | 0.034±0.002 | radial vel. | 120 | Host star also known as GJ 2030[34] | ||||
HD 21019 c | 12.934±2.361 | 25600±2500 | 16.752±1.312 | radial vel. | 120 | Host star also known as GJ 2030[34] | ||||
HD 21175 b | 0.038±0.010 | 10.6 | 0.091±0.004 | radial vel. | 57.7 | Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system[34] | ||||
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[36] |
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[36] |
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[37] |
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[37] | |||
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[37] | |||
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[37] | |||
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, shares system with a red dwarf[38] | |
HR 7321 b | 0.30±0.07 | 285.1+1.2 −1.5 | 0.937±0.003 | radial vel. | 200.2 | 1.35+0.19 −0.21 | 4971 | Red giant host star also known as HD 184010[39] | ||
HR 7321 c | 0.28+0.08 −0.10 | 483.3+3.2 −4.0 | 1.332+0.006 −0.007 | radial vel. | 200.2 | 1.35+0.19 −0.21 | 4971 | Red giant host star also known as HD 184010[39] | ||
HR 7321 d | 0.46±0.08 | 837.7+6.4 −5.5 | 1.922+0.010 −0.008 | radial vel. | 200.2 | 1.35+0.19 −0.21 | 4971 | Red giant host star also known as HD 184010[39] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
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 | [5] | ||
K2-384b | 0.0040±0.0026 | 0.096+0.020 −0.005 | 2.23152+0.0019 −0.00032 | 600 | transit | 0.330±0.009 | 3623±138 | [5] | ||
K2-384c | 0.0054±0.0027 | 0.106+0.004 −0.006 | 4.19476+0.00030 −0.00018 | 480 | transit | 0.330±0.009 | 3623±138 | [5] | ||
K2-384d | 0.0085±0.0044 | 0.124+0.010 −0.006 | 6.67958+0.00071 −0.00049 | 410 | transit | 0.330±0.009 | 3623±138 | [5] | ||
K2-384e | 0.0075±0.0042 | 0.120+0.012 −0.007 | 9.71504+0.00100 −0.00073 | 370 | transit | 0.330±0.009 | 3623±138 | [5] | ||
K2-384f | 0.0179±0.0104 | 0.198+0.008 −0.007 | 13.62749+0.00034 −0.00057 | 330 | transit | 0.330±0.009 | 3623±138 | [5] | ||
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
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 | [5] | |
K2-407 b | 0.0066±0.0035 | 0.114+0.008 −0.007 | 4.9419+0.00066 −0.00069 | 1110 | transit | [5] | ||||
K2-407 c | 0.0078±0.0044 | 0.121+0.008 −0.007 | 9.22453+0.00132 −0.00091 | 900 | transit | [5] | ||||
K2-408 b | 0.0122±0.0062 | 0.149+0.010 −0.009 | 20.97895+0.00130 −0.00124 | 610 | transit | [5] | ||||
K2-409 b | 0.0212±0.0127 | 0.221+0.015 −0.014 | 1.90808+0.00004 −0.00005 | 1800 | transit | [5] | ||||
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] | |||
Kepler-451 c | 1.61±0.14 | 1460±90 | 2.1±0.2 | timing | 1340±20 | 0.48+0.12 | [40] | |||
Kepler-451 d | 1.76±0.18 | 43.0±0.1 | 0.20±0.03 | timing | 1340±20 | 0.48+0.12 | [40] | |||
Kepler-1656 c | 0.40±0.09 | 1919+27 −24 | 3.053±0.049 | radial vel. | 1.03±0.04 | [41] | ||||
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[42][43] | |
Kepler-1972b | 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[44] | ||
Kepler-1972c | 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[44] | ||
KMT-2016-BLG-1105b | 0.007+0.023 −0.005 | 2.44+0.88 −0.75 | microlensing | 17000±7000 | 0.41+0.25 −0.21 | [45] | ||||
KMT-2017-BLG-0428b | 0.018+0.011 −0.009 | 1.81+0.55 −0.59 | microlensing | 18000+6000 −8000 | 0.34+0.22 −0.17 | [45] | ||||
KMT-2017-BLG-0673Lb | 3.67+2.17 −2.07 | 2.34+0.56 −0.74 | microlensing | 17000+4000 −5000 | 0.63+0.37 −0.35 | [46] | ||||
KMT-2017-BLG-1003b | 0.016+0.017 −0.009 | 1.38+0.39 −0.32 | microlensing | 23000±2000 | 0.32+0.31 −0.17 | [45] | ||||
KMT-2017-BLG-1194b | 0.011±0.006 | 1.78+0.45 −0.46 | microlensing | 14000±6000 | 0.41+0.23 −0.19 | [45] | ||||
KMT-2018-BLG-0030b | 1.45+1.23 −0.88 | 4.39+2.18 −2.40 | microlensing | 21000+4000 −6000 | 0.51+0.43 −0.31 | [47] | ||||
KMT-2018-BLG-0087b | 0.23+0.32 −0.12 | 0.87+0.24 −0.25 | microlensing | 23000+3000 −4000 | 0.10+0.14 −0.05 | [47] | ||||
KMT-2018-BLG-0247b | 2.11+2.09 −1.04 | 2.46+0.51 −0.58 | microlensing | 22000+3000 −4000 | 0.29+0.28 −0.14 | [47] | ||||
KMT-2018-BLG-2004b | 0.27±\0.12 | 4.62+0.80 −1.10 | microlensing | 23000+3000 −4000 | 0.69+0.32 −0.31 | [48] | ||||
KMT-2018-BLG-2602b | 1.15+0.73 −0.63 | 3.81+2.96 −2.32 | microlensing | 14000±6000 | 0.66+0.42 −0.36 | [47] | ||||
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 | [48] | ||||
KMT-2019-BLG-0414Lb | 4.57+3.74 −2.06 | 1.16+0.47 −0.51 | microlensing | 14000+5000 −6000 | 0.74+0.43 −0.38 | [46] | ||||
KMT-2019-BLG-1042Lb | 0.19+0.21 −0.11 | 1.7±0.5 | microlensing | 22000+3000 −5000 | 0.30+0.34 −0.18 | [49] | ||||
KMT-2019-BLG-1367b | 0.013+0.008 −0.007 | 1.70+0.50 −0.56 | microlensing | 15000+8000 −7000 | 0.25+0.16 −0.13 | [45] | ||||
KMT-2019-BLG-1552Lb | 4.05+1.73 −1.85 | 2.6+0.6 −0.8 | microlensing | 15000+6000 −5000 | 0.79+0.33 −0.36 | [49] | ||||
KMT-2019-BLG-1806b | 0.015±0.005 | 3.02+0.70 −0.73 | microlensing | 22000+2000 −7000 | 0.74±0.25 | [45] | ||||
KMT-2019-BLG-2974Lb | 0.28+0.29 −0.18 | 2.0+0.8 −0.7 | microlensing | 20000+5000 −7000 | 0.47+0.41 −0.28 | [49] | ||||
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 | [50] | ||||
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[51] | ||||
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[51] | ||||
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 | [52] | ||||
KMT-2021-BLG-0748b | 0.45+0.40 −0.25 | 2.43±0.67 | microlensing | 20000+3000 −4000 | 0.36+0.32 −0.20 | [53] | ||||
KMT-2021-BLG-0119Lb | 5.97+2.94 −2.60 | 3.23+0.76 −0.80 | microlensing | 11000+6000 −4000 | 0.69+0.34 −0.30 | Multiple orbital solutions[54] | ||||
KMT-2021-BLG-0192Lb | 0.19+0.09 −0.10 | 2.07+0.35 −0.47 | microlensing | 22000+3000 −5000 | 0.55+0.26 −0.28 | Multiple orbital solutions[54] | ||||
KMT-2021-BLG-0712b | 0.12+0.06 −0.04 | 2.22+0.66 −0.48 | microlensing | 10000+3000 −2000 | 0.22+0.12 −0.07 | [55] | ||||
KMT-2021-BLG-0909b | 1.26+1.01 −0.66 | 1.75±0.42 | microlensing | 21000+3000 −5000 | 0.38+0.30 −0.20 | [55] | ||||
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 | [56] | ||||
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 | [56] | ||||
KMT-2021-BLG-1105b | 1.30±0.68 | 3.54±1.06 | microlensing | 15000±5000 | 0.63±0.33 | [55] | ||||
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 | [53] | ||||
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[52] | ||||
KMT-2021-BLG-1372b | 0.1928±0.1129 | 2.37±0.77 | microlensing | 19000+5000 −8000 | 0.42±0.25 | [53] | ||||
KMT-2021-BLG-1391b | 0.0143±0.0073 | 2.29+0.56 −0.71 | microlensing | 19000+3000 −5000 | 0.37±0.19 | [53] | ||||
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 | [52] | ||||
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 | [50] | ||||
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[57] | ||||
KMT-2021-BLG-2294Lb | 0.07+0.10 −0.03 | 0.94±0.16 | microlensing | 22000±3000 | 0.11+0.17 −0.06 | Multiple orbital solutions[54] | ||||
KMT-2021-BLG-2478b | 0.80+0.56 −0.35 | 1.38±0.26 | microlensing | 8000+4000 −3000 | 0.12+0.09 −0.06 | [55] | ||||
L 363-38 b | 0.0147±0.0014 | 8.781±0.007 | 0.048±0.006 | 330 | radial vel. | 33.31 | 0.21 | 3129 | Host star also known as Gliese 3049[58] | |
MOA-2019-BLG-008L b | 30 | microlensing | 8000±2000 | 0.8 | [59] | |||||
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 | [60] | ||||
MOA-2020-BLG-208Lb | 0.217+0.116 −0.106 | 2.88+0.40 −0.41 | microlensing | 25000±3000 | 0.656+0.346 −0.322 | [61] | ||||
Mu2 Scorpii b | 14.4 | 290 | imaging | 474 | 9.1 | 21900 | [62] | |||
Mu2 Scorpii c | 18.5 | 21 | imaging | 474 | 9.1 | 21900 | [62] | |||
NGTS-20 b | 2.98+0.16 −0.15 | 1.07±0.04 | 54.18915±0.00015 | 0.313±0.013 | 688+14 −13 | transit | 1195±8 | 1.47±0.09 | 5980±80 | Planet on eccentric orbit, host star also known as TOI-5152[63] |
NGTS-21b | 2.36±0.21 | 1.33±0.03 | 1.5433897±0.0000016 | 0.0236±0.0005 | 1357±15 | transit | 2090+90 −80 | 0.72±0.04 | 4660±41 | [64] |
NGTS-23b | 0.613±0.097 | 1.267±0.030 | 4.0764326±0.0000041 | 0.0504±0.012 | 1327+17 −16 | transit | 3230±70 | 1.01+0.06 −0.07 | 6057±64 | [65] |
NGTS-24b | 0.52+0.12 −0.11 | 1.214+0.058 −0.062 | 3.4678796±0.0000070 | 0.0479+0.0028 −0.0030 | 1499+41 −36 | transit | 2360±80 | 1.26+0.05 −0.21 | 5820+93 −8 | [65] |
NGTS-25b | 0.639+0.058 −0.052 | 1.023+0.035 −0.052 | 2.8230930±0.0000033 | 0.0388+0.0014 −0.002 | 1101+15 −14 | transit | 2350±30 | 0.91+0.03 −0.04 | 5321±58 | [65] |
OGLE-2016-BLG-1093Lb | 0.71±0.12 | 2.13±0.33 | microlensing | 26000±2000 | 0.46±0.08 | [66] | ||||
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[52] | ||||
OGLE-2017-BLG-1806b | 0.017+0.015 −0.009 | 1.75+0.46 −0.47 | microlensing | 21000+3000 −5000 | 0.38+0.34 −0.20 | [45] | ||||
OGLE-2018-BLG-0298Lb | 0.14+0.07 −0.06 | 2.86+0.73 −0.80 | microlensing | 21000+3000 −4000 | 0.69+0.34 −0.30 | [47] | ||||
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 | [48] | ||||
OGLE-2018-BLG-1119Lb | 0.91+0.66 −0.52 | 4.06+2.14 −2.58 | microlensing | 19000+5000 −8000 | 0.48+0.35 −0.28 | [47] | ||||
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 | [48] | ||||
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 | [48] | ||||
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[48] | |||||
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[48] | ||||
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 | [48] | ||||
OGLE-2019-BLG-0362Lb | 3.26+0.83 −0.58 | 2.18+0.58 −0.72 | microlensing | 19000±2000 | 0.42+0.34 −0.23 | Multiple solutions for planetary parameters[67] | ||||
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[68] | ||||
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 | [69] | |||
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 | [70] | |
PSR J2007+3120 b | 0.0072±0.0009 | 723±8 | timing | 22000 | Pulsar planet, another planet in the system is suspected.[71] | |||||
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.[72] | ||
TOI-181b | 0.127891+0.013510 −0.025081 | 0.631521+0.007554 −0.009811 | 4.532058+0.000002 −0.000002 | 0.055780+0.005563 −0.003893 | 878+32 −41 | transit | 314±2 | 0.781±0.042 | 4994±50 | [73] |
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 | [74] | |
TOI-277 b | 0.0239+0.0179 −0.0098 | 0.237±0.016 | 3.9940±0.0004 | 0.0269±0.0011 | transit | 212.6+0.6 −0.3 | 0.16±0.01 | 4031+21 −23 | [75] | |
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 | [74] | |
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 | [74] | |
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 | [76] | ||
TOI-778 b | 2.76±0.24 | 1.375±0.045 | 4.633611±0.000001 | 0.060±0.003 | 1561+33 −32 | transit | 530±4 | 1.428±0.094 | 6715±128 | [77] |
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 | [74] | |
TOI-969 b | 0.0286±0.0031 | 0.247±0.033 | 1.8237305+0.0000020 −0.0000021 | 0.02636±0.00017 | 941±31 | transit | 253.8±0.5 | 0.730±0.037 | 4550±75 | [78] |
TOI-969 c | 11.3+1.1 −0.9 | 1700+290 −280 | 2.52+0.27 −0.29 | 96.4+6.8 −5.8 | radial vel. | 253.8±0.5 | 0.730±0.037 | 4550±75 | Eccentric orbit[78] | |
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 | [79] |
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 | [79] |
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 | [74] | |
TOI-1075 b | 0.0313±0.0042 | 0.160+0.010 −0.007 | 0.6047328±0.0000032 | 0.01159+0.00023 −0.00020 | 1323±44 | transit | 200.4+0.6 −2.2 | 0.604±0.030 | 3875±75 | [80] |
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 | [81] |
TOI-1136 b | 0.0095+0.0022 −0.0028 | 0.170+0.019 −0.013 | 4.1728±0.0002 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
TOI-1136 c | 0.0189+0.0041 −0.0053 | 0.257±0.005 | 6.2573±0.0002 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
TOI-1136 d | 0.0252+0.0076 −0.0060 | 0.413±0.007 | 12.5194±0.0004 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
TOI-1136 e | 0.0170±0.0031 | 0.236+0.006 −0.008 | 18.7992+0.0017 −0.0015 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
TOI-1136 f | 0.0261+0.0088 −0.0113 | 0.346±0.010 | 26.3162+0.0017 −0.0013 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
TOI-1136 g | 0.0151+0.0148 −0.0104 | 0.226±0.010 | 39.5387+0.0036 −0.0030 | transit | 275.8±0.5 | 1.022±0.027 | 5770±50 | [82] | ||
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 | Subgiant host star[83] | |
TOI-1221 b | 0.259±0.011 | 91.68278+0.00032 −0.00041 | 0.404+0.026 −0.023 | 400 | transit | 447.1±0.7 | 1.03±0.06 | 5592±50 | [84] | |
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 | [85] |
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 | [85] |
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 | [85] |
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 | [85] |
TOI-1260 d | 0.0373±0.0245 | 0.276±0.008 | 16.608164±0.000083 | 0.1116±0.0033 | 499±4 | transit | 239.5±0.3 | 0.66±0.01 | 4227±85 | [86] |
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 | [87] |
TOI-1272 b | 0.0774±0.0072 | 0.370±0.019 | 3.31599±0.00002 | 0.0412±0.0008 | 961±32 | transit | 450.6±1.3 | 0.851±0.049 | 4985±121 | [88] |
TOI-1272 c | 0.0840±0.0098 | 8.689±0.008 | 0.0783±0.0014 | 697±23 | radial vel. | 450.6±1.3 | 0.851±0.049 | 4985±121 | [88] | |
TOI-1288 b | 0.0712+0.0574 −0.0304 | 0.454±0.010 | 2.69998±0.00015 | 0.0429±0.0006 | transit | 375.3+1.3 −0.5 | 1.46±0.06 | 5307+18 −16 | [75] | |
TOI-1288 c | 0.2643±0.0220 | 443+11 −13 | radial vel. | 375.3+1.3 −0.5 | 1.46±0.06 | 5307+18 −16 | [89] | |||
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 | [74] | |
TOI-1422 b | 0.0283+0.0072 −0.0063 | 0.354+0.012 −0.010 | 12.9972±0.0006 | 0.108±0.003 | 867±17 | transit | 504.17+0.12 −0.09 | 0.981+0.062 −0.065 | 5840±62 | Another planet in the system is suspected.[90] |
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 | [74] | |
TOI-1452 b | 0.0152±0.0041 | 0.149±0.006 | 11.06201±0.00002 | 0.061±0.003 | 326±7 | transit | 99.51±0.04 | 0.249±0.008 | 3185±50 | Also a red dwarf on a 97AU separation in the system[91] |
TOI-1468 b | 0.0101±0.0008 | 0.114±0.003 | 1.8805136+0.0000024 −0.0000026 | 682.2+7.4 −6.9 | transit | 80.64±0.07 | 0.339±0.011 | 3496±25 | [92] | |
TOI-1468 c | 0.0209±0.0021 | 0.184±0.004 | 15.532482+0.000034 −0.000033 | 337.5+3.7 −3.4 | transit | 80.64±0.07 | 0.339±0.011 | 3496±25 | [92] | |
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 | [83] | |
TOI-1669 b | 0.0132±0.0085 | 0.214±0.016 | 2.7 | transit | 364.6 | 1.00±0.05 | 5542.3±100.0 | [93] Host star also known as BD+82 71, planet suspected since 2020[94] | ||
TOI-1669 c | 0.602±0.078 | 501±16 | radial vel. | 364.6 | 1.00±0.05 | 5542.3±100.0 | [93] Host star also known as BD+82 71, additional long-period companion is suspected. | |||
TOI-1694 b | 0.0979±0.0066 | 0.461±0.016 | 3.8 | transit | 405.7 | 0.84±0.03 | 5066±100 | [93] Host star also known as TYC 4108-1434-1, planet suspected since 2020[94] | ||
TOI-1694 c | 0.929±0.037 | 393.2±4.3 | radial vel. | 405.7 | 0.84±0.03 | 5066±100 | [93] Host star also known as TYC 4108-1434-1 | |||
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 | [95] |
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 | [95] |
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 | [74] | |
TOI-1695 b | 0.0173±0.0031 | 0.181±0.016 | 3.1342790±0.0000072 | 0.033548+0.000260 −0.000268 | 590±90 | transit | 147.2±0.2 | 0.51±0.02 | 3627±31 | [96][97] |
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 | [98][99] |
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 | [100] |
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 | [101][102] |
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 | [103] |
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 | [104] |
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 | [74] | |
TOI-1937 b | 2.01+0.17 −0.16 | 1.247+0.059 −0.062 | 0.94667944±0.00000047 | 0.01932+0.00035 −0.00039 | 2097+35 −36 | transit | 1366±6 | 1.072+0.059 −0.064 | 5814+91 −93 | [105] |
TOI-2000 b | 0.0324±0.0070 | 0.236±0.010 | 3.098331+0.000021 −0.000019 | 0.04260+0.00076 −0.00067 | 1475+120 −158 | transit | 566.3±1.0 | 1.074+0.059 −0.050 | 5607+86 −82 | [106] |
TOI-2000 c | 0.238±0.012 | 0.711±0.011 | 9.1270553±0.0000073 | 0.0875+0.0016 −0.0014 | 1029+84 −111 | transit | 566.3±1.0 | 1.074+0.059 −0.050 | 5607+86 −82 | [106] |
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 | [104] |
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 | [103] |
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[83] | |
TOI-2048 b | 0.184±0.018 | 13.79019+0.00065 −0.00084 | 640±20 | transit | 379.7±0.5 | 0.83±0.03 | 5185±60 | Young host star belongs to NGC 3532[107] | ||
TOI-2081 b | 0.0157+0.0151 −0.0076 | 0.182±0.046 | 10.50534+0.00007 −0.00008 | 0.0752+0.0047 −0.0119 | 488+28 −52 | transit | 203.26±0.16 | 0.540±0.080 | 3800±100 | [108] |
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 | [109][110] |
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[103] |
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[103] |
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 | [103] |
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 | [111] |
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 | [104] |
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 0.54M☉ star in the system[112] |
TOI-2196 b | 0.0818±0.0041 | 0.313±0.013 | 1.1947268+0.0000079 −0.0000093 | 0.02234±0.00060 | 1860±20 | transit | 861±3 | 1.032±0.038 | 5634±31 | Neptunian desert planet[113] |
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 | 1259+16 −15 | transit | 1242±9 | 1.296+0.069 −0.072 | 6075±110 | [112] |
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 | [74] | |
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 | [112] |
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 | [114] | |
TOI-2364 b | 0.225+0.043 −0.049 | 0.768+0.023 −0.018 | 4.0197517±0.0000043 | 0.04871+0.00069 −0.00079 | 1091+17 −14 | transit | 713±6 | 0.954+0.041 −0.046 | 5306+76 −68 | [105] |
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 | [74] | |
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 | [112] |
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 | [74] | |
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 | [74] | |
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 | [103] |
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 | [112] |
TOI-2570 b | 0.820+0.063 −0.065 | 1.217+0.035 −0.034 | 2.9887615±0.0000022 | 0.04145+0.00081 −0.00086 | 1431+24 −23 | transit | 1179±6 | 1.063+0.063 −0.065 | 5765±50 | [112] |
TOI-2583 b | 0.250+0.058 −0.056 | 1.290+0.040 −0.033 | 4.5207265±0.0000049 | 0.0571+0.0010 −0.0013 | 1456+19 −16 | transit | 1831±9 | 1.215+0.063 −0.082 | 5936+65 −68 | [105] |
TOI-2587 b | 0.218+0.054 −0.046 | 1.077+0.042 −0.040 | 5.456640±0.000011 | 0.0635+0.0025 −0.0013 | 1445+23 −26 | transit | 1242±10 | 1.15+0.14 −0.07 | 5760+80 −79 | [105] |
TOI-2669b | 0.61±0.19 | 1.76±0.16 | 6.2034±0.0001 | transit | 1294±9 | 1.19±0.16 | 4800±100 | [114] | ||
TOI-2796 b | 0.44+0.10 −0.11 | 1.59 | 4.8084983+0.0000057 −0.0000056 | 0.0569+0.0010 −0.0011 | 1205+18 −17 | transit | 1150±6 | 1.063+0.057 −0.062 | 5764+81 −78 | [105] |
TOI-2803 b | 0.975+0.083 −0.070 | 1.616+0.034 −0.032 | 1.96229325±0.00000082 | 0.03185±0.00052 | 1893+29 −28 | transit | 1635±9 | 1.118+0.056 −0.054 | 6280+99 −96 | [105] |
TOI-2818 b | 0.71±0.26 | 1.363+0.046 −0.045 | 4.0397090+0.0000024 −0.0000023 | 0.0493+0.0010 −0.0008 | 1376+26 −24 | transit | 1028±3 | 0.977+0.063 −0.049 | 5721+88 −83 | [105] |
TOI-2842 b | 0.370+0.052 −0.047 | 1.146+0.051 −0.048 | 3.5514058+0.0000077 −0.0000078 | 0.0475+0.0010 −0.0011 | 1471+29 −27 | transit | 1501±8 | 1.135+0.077 −0.079 | 5910±100 | [105] |
TOI-2977 b | 1.68+0.26 −0.25 | 1.174+0.031 −0.027 | 2.3505614±0.0000025 | 0.03386+0.00067 −0.00050 | 1544±26 | transit | 1160±30 | 0.936+0.057 −0.041 | 5691+94 −93 | [105] |
TOI-3023 b | 0.62+0.10 −0.09 | 1.466+0.043 −0.032 | 3.9014971±0.0000031 | 0.0505+0.0015 −0.0009 | 1596+24 −25 | transit | 1281±5 | 1.12+0.11 −0.06 | 5760+85 −88 | [105] |
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 0.6M☉ star in the system[112] |
TOI-3364 b | 1.67+0.12 −0.13 | 1.091+0.038 −0.032 | 5.8768918±0.0000069 | 0.0675+0.0011 −0.0016 | 1264+22 −21 | transit | 899±3 | 1.186+0.059 −0.083 | 5706+95 −91 | [105] |
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[112] |
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 | [115] |
TOI-3688 b | 0.98+0.10 −0.11 | 1.167+0.048 −0.044 | 3.246075±0.000012 | 0.04560+0.00089 −0.00098 | 1534+29 −28 | transit | 1308±6 | 1.199+0.072 −0.076 | 5950±100 | [105] |
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 | [112] |
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 | [115] |
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 | [116] |
TOI-3807 b | 1.04+0.15 −0.14 | 2.00 | 2.8989727+0.0000038 −0.0000039 | 0.0421+0.0007 −0.0011 | 1646+25 −24 | transit | 1399±7 | 1.181+0.064 −0.092 | 5772+84 −80 | [105] |
TOI-3819 b | 1.11+0.18 −0.20 | 1.172+0.036 −0.035 | 3.2443141±0.0000055 | 0.04611+0.00069 −0.00096 | 1633+21 −19 | transit | 1834±17 | 1.242+0.057 −0.076 | 5859+72 −71 | [105] |
TOI-3884 b | 0.0519+0.0110 −0.0057 | 0.563±0.025 | 4.5445697±0.0000094 | 0.0354±0.0014 | 463±12 | transit | 141.37±0.16 | 0.2813±0.0067 | 3269±70 | [117][118] |
TOI-3912 b | 0.406+0.071 −0.068 | 1.274+0.041 −0.040 | 3.4936264±0.0000038 | 0.0463+0.0012 −0.0010 | 1512±20 | transit | 1533±9 | 1.088+0.086 −0.070 | 5725+69 −68 | [105] |
TOI-3976 b | 0.175+0.037 −0.036 | 1.095+0.036 −0.035 | 6.607662+0.000016 −0.000015 | 0.0743+0.0013 −0.0014 | 1295+16 −14 | transit | 1703±8 | 1.254+0.067 −0.072 | 5975+70 −69 | [105] |
TOI-4087 b | 0.73±0.14 | 1.164+0.025 −0.024 | 3.17748350±0.00000094 | 0.04469+0.00048 −0.00054 | 1458+20 −17 | transit | 1013±4 | 1.178+0.039 −0.042 | 6060+74 −67 | [105] |
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 | [112] |
TOI-4145 b | 0.43±0.13 | 1.187+0.032 −0.031 | 4.0664428±0.0000058 | 0.04823+0.00075 −0.00079 | 1074+19 −16 | transit | 668.7±1.3 | 0.905+0.043 −0.044 | 5281+86 −76 | [105] |
TOI-4329b | 0.45±0.09 | 1.50±0.19 | 2.9223±0.00015 | transit | 2258±16 | 1.538±0.049 | 6000±100 | [114] | ||
TOI-4463 b | 0.794+0.039 −0.040 | 1.183+0.064 −0.045 | 2.8807198+0.0000028 −0.0000027 | 0.04036+0.00074 −0.00082 | 1395+25 −22 | transit | 579.5±1.8 | 1.056+0.059 −0.063 | 5640+89 −82 | [105] |
TOI-4479 b | 0.0261+0.0252 −0.0126 | 0.252±0.057 | 1.15890+0.00001 −0.00002 | 0.0164+0.0015 −0.0029 | 861+64 −103 | transit | 262.9±0.3 | 0.452±0.090 | 3400±100 | [108] |
TOI-4562 b | 3.29+1.88 −0.82 | 1.072+0.044 −0.043 | 225.11757+0.00027 −0.00025 | 0.771±0.013 | 349±10 | transit | 1131±12 | 1.218+0.054 −0.048 | 6096±32 | Highly eccentric orbit[119] |
TOI-4582 b | 0.53±0.05 | 0.94+0.09 −0.12 | 31.034±0.001 | transit | 1242 | 1.34±0.06 | 5190±100 | Evolved star, eccentric planetary orbit[120] | ||
TOI-4791 b | 2.31+0.32 −0.33 | 1.110±0.050 | 4.280880+0.000022 −0.000023 | 0.0555+0.0011 −0.0012 | 1472+26 −24 | transit | 1051±6 | 1.242+0.072 −0.077 | 6058+99 −94 | [105] |
TOI-5153 b | 3.26+0.18 −0.17 | 1.06±0.04 | 20.33003±0.00007 | 0.158±0.006 | 906±13 | transit | 1272.336±11 | 1.24±0.07 | 6300±80 | [63] |
TOI-5174 b | 0.07801 | 0.47667 | 12.214 | transit | 1.0±0.125 | [121][122] | ||||
TOI-5205b | 1.08±0.06 | 1.03±0.03 | 1.630757±0.000001 | 0.0199±0.0002 | 737±15 | transit | 283.35±0.16 | 0.392±0.015 | 3430±54 | [123] |
TOI-5542 b | 1.32±0.10 | 1.009+0.036 −0.035 | 75.12375+0.00019 −0.00018 | 0.332±0.016 | 441+48 −74 | transit | 1154±12 | 0.890+0.056 −0.031 | 5700±80 | [124] |
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 | [125] | ||
WASP-132c | 0.165±0.009 | 1.011534±0.000005 | 0.0182±0.0003 | transit | 390 | 0.782±0.034 | 4714+87 −88 | [126] |
Specific exoplanet lists
[edit]- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- 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 largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
Lists of exoplanets by year of discovery
[edit]- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (150)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (304)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (304)
- List of exoplanets discovered in 2024 (176)
References
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- ^ Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert. Retrieved 4 April 2022.
- ^ Currie, Thayne; et al. (2023), "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star", Science, 380 (6641): 198–203, arXiv:2212.00034, Bibcode:2023Sci...380..198C, doi:10.1126/science.abo6192, PMID 37053312, S2CID 258108042
- ^ a b Sebastian, D.; Guenther, E. W.; Deleuil, M.; Dorsch, M.; Heber, U.; Heuser, C.; Gandolfi, D.; Grziwa, S.; Deeg, H. J.; Alonso, R.; Bouchy, F.; Csizmadia, Sz; Cusano, F.; Fridlund, M.; Geier, S.; Irrgang, A.; Korth, J.; Nespral, D.; Rauer, H.; Tal-Or, L. (2022), "Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b", Monthly Notices of the Royal Astronomical Society, 516: 636–655, arXiv:2207.08742, doi:10.1093/mnras/stac2131
- ^ 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 Christiansen, Jessie L.; et al. (2022), "Scaling K2. V. Statistical Validation of 60 New Exoplanets from K2 Campaigns 2–18", The Astronomical Journal, 163 (6): 244, arXiv:2203.02087, Bibcode:2022AJ....163..244C, doi:10.3847/1538-3881/ac5c4c, S2CID 247244871
- ^ a b c d e f Del Ser, D.; Fors, O.; Del Alcázar, M.; Dyachenko, V.; Horch, E. P.; Tokovinin, A.; Ziegler, C.; Van Belle, G. T.; Clark, C. A.; Hartman, Z. D. (2023), "TFAW survey II: Six newly validated planets and 13 planet candidates from K2", Monthly Notices of the Royal Astronomical Society, 518: 669–690, arXiv:2210.10805, doi:10.1093/mnras/stac3087
- ^ a b Panahi, Aviad; Zucker, Shay; Clementini, Gisella; Audard, Marc; Binnenfeld, Avraham; Cusano, Felice; Evans, Dafydd Wyn; Gomel, Roy; Holl, Berry; Ilyin, Ilya; De Fombelle, Grégory Jevardat; Mazeh, Tsevi; Mowlavi, Nami; Nienartowicz, Krzysztof; Rimoldini, Lorenzo; Shahaf, Sahar; Eyer, Laurent (2022). "The detection of transiting exoplanets by Gaia". Astronomy & Astrophysics. 663: A101. arXiv:2205.10197. Bibcode:2022A&A...663A.101P. doi:10.1051/0004-6361/202243497. S2CID 248965147.
- ^ Damasso, M.; et al. (2022), "A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514", Astronomy & Astrophysics, 666: A187, arXiv:2204.06376, doi:10.1051/0004-6361/202243522, S2CID 248157318
- ^ a b Suárez Mascareño, A.; et al. (2022), "Two temperate Earth-mass planets orbiting the nearby star GJ 1002", Astronomy & Astrophysics, 670: A5, arXiv:2212.07332, doi:10.1051/0004-6361/202244991, S2CID 254353639
- ^ Kemmer, J.; et al. (2022), "Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 B", Astronomy & Astrophysics, 659: A17, arXiv:2202.00970, Bibcode:2022A&A...659A..17K, doi:10.1051/0004-6361/202142653, S2CID 246473345
- ^ a b Beard, Corey; et al. (2022), "GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion", The Astrophysical Journal, 936 (1): 55, arXiv:2207.10672, Bibcode:2022ApJ...936...55B, doi:10.3847/1538-4357/ac8480, S2CID 251018402
- ^ A Jupiter Analog Orbiting The Nearby M Dwarf GJ 463
- ^ Sozzetti, A. (2023), "A dynamical mass for GJ 463 b: A massive super-Jupiter companion beyond the snow line of a nearby M dwarf", Astronomy & Astrophysics, 670: L17, arXiv:2302.00413, Bibcode:2023A&A...670L..17S, doi:10.1051/0004-6361/202245454, S2CID 256253670
- ^ a b Almenara, J. M.; et al. (2022), "GJ 3090 b: One of the most favourable mini-Neptune for atmospheric characterisation", Astronomy & Astrophysics, 665: A91, arXiv:2207.14121, Bibcode:2022A&A...665A..91A, doi:10.1051/0004-6361/202243975, S2CID 252367299
- ^ Bourrier, V.; et al. (2022), "A CHEOPS-enhanced view of the HD 3167 system", Astronomy & Astrophysics, 668: A31, arXiv:2209.06937, Bibcode:2022A&A...668A..31B, doi:10.1051/0004-6361/202243778, S2CID 251861892
- ^ Desidera, S.; et al. (2023), "TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit", Astronomy & Astrophysics, 675: A158, arXiv:2210.07933, Bibcode:2023A&A...675A.158D, doi:10.1051/0004-6361/202244611, S2CID 252907692
- ^ de Leon, Jerome P.; et al. (2023), "A sub-Neptune transiting the young field star HD 18599 at 40 pc", Monthly Notices of the Royal Astronomical Society, 522: 750–766, arXiv:2210.08179, doi:10.1093/mnras/stad894
- ^ Vines, Jose I.; Jenkins, James S.; Berdiñas, Zaira; Soto, Maritza G.; Díaz, Matías R.; Alves, Douglas R.; Tuomi, Mikko; Wittenmyer, Robert A.; De Leon, Jerome Pitogo; Peña, Pablo; Lissauer, Jack J.; Ballard, Sarah; Bedding, Timothy; Bowler, Brendan P.; Horner, Jonathan; Jones, Hugh R A.; Kane, Stephen R.; Kielkopf, John; Plavchan, Peter; Shporer, Avi; Tinney, C. G.; Wright, Hui Zhang Duncan J.; Addison, Brett; Mengel, Matthew W.; Okumura, Jack; Samadi-Ghadim, Anya (2022), "A dense mini-Neptune orbiting the bright young star HD 18599", Monthly Notices of the Royal Astronomical Society, 518 (2): 2627–2639, arXiv:2210.07945, doi:10.1093/mnras/stac2845
- ^ Murgas, F.; et al. (2022), "HD 20329b: An ultra-short-period planet around a solar-type star found by TESS", Astronomy & Astrophysics, 668: A158, arXiv:2211.02547, Bibcode:2022A&A...668A.158M, doi:10.1051/0004-6361/202244459, S2CID 253370507
- ^ a b c Ottoni, G.; Udry, S.; Ségransan, D.; et al. (2022). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars".