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] | |
K2-400 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] |
Pi Mensae, also known as HD 39091, is a G-dwarf star in the constellation of Mensa. This star has a high proper motion. The apparent magnitude is 5.67, which can be visible to the naked eye in exceptionally dark, clear skies. It is nearly 60 light-years away. The star is slightly larger than the Sun in terms of mass, size, luminosity, temperature and metallicity, and is about 730 million years younger. It hosts three known planets.
K2-3, also known as EPIC 201367065, is a red dwarf star with three known planets. It is on the borderline of being a late orange dwarf/K-type star, but because of its temperature, it is classified as a red dwarf.
HD 191939 is a single yellow (G-type) main-sequence star, located approximately 174 light-years away in the constellation of Draco, taking its primary name from its Henry Draper Catalogue designation.
HD 108236 is a G-type main-sequence star. Its surface temperature is 5660±61 K. HD 108236 is severely depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.28±0.04, and is probably older than the Sun at an age of 6.7+3.3
−3.4 billion years.
TOI-640 b is an exoplanet that was suspected since 2019. Its discovery has been confirmed by the TESS team in January 2021. It is located 1115 light years away from Earth, orbiting a primary F-class star in a binary star system with red dwarf and has an orbital period of 5 days.
L 98-59 b is an exoplanet having a size between that of the Earth and Mars and a mass only half that of Venus. It orbits L 98-59, a red dwarf 35 light-years away in the constellation Volans. There are at least 3 other planets in the system: L 98-59 c, d, e, and the unconfirmed L 98-59 f. Its discovery was announced on 27 June 2019 on the NASA website. It was the smallest planet discovered by TESS until the discovery of LHS 1678b, and was the lowest-mass planet whose mass has been measured using radial velocities until Proxima Centauri d was found in 2022.
L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs, as measured by the Gaia spacecraft.