This is a list of exoplanets discovered in 2017.
For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)
Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K) [1] | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
BD+03 2562 b | 6.4 | 481.9 | 1.3 | radial vel. | 8540 | 1.14 | 4095 | [2] | ||
CoRoT-30 b | 2.90±0.22 | 1.009±0.076 | 9.06005±0.00024 | 0.0844±0.0012 | transit | 3100±200 | 0.98+0.03 −0.05 | 5650±100 | [3] | |
CoRoT-31 b | 0.84±0.34 | 1.46±0.30 | 4.62941±0.00075 | 0.0586±0.0034 | transit | 7000±2000 | 1.25+0.22 −0.21 | 5700±120 | [3] | |
CoRoT-32 b | 0.15 | 0.57 | 6.71837 | 0.071 | 938 | transit | 1.08 | 5970 | Host star also known as CoRoT 223977153 [4] | |
Luyten b | 0.00909 | 18.6498 | 0.091101 | 259 | radial vel. | 12 | 0.29 | 3382 | Potentially habitable exoplanet. [5] | |
Luyten c | 0.00371 | 4.7234 | 0.036467 | radial vel. | 12 | 0.29 | 3382 | [5] | ||
Gliese 625 b | 0.00887 | 14.628 | 0.078361 | radial vel. | 21 | 0.30 | 3499 | [6] | ||
Gliese 1148 c | 0.2141 | 532.58 | 0.912 | radial vel. | 35.98 | 0.357±0.013 | Host star also known as Ross 1003 [7] | |||
Gliese 3138 b | 0.0056 | 1.22003 | 0.0197 | radial vel. | 92.9 | 0.68 | 3717 | [5] | ||
Gliese 3138 c | 0.01315 | 5.974 | 0.057 | radial vel. | 92.9 | 0.68 | 3717 | [5] | ||
Gliese 3138 d | 0.03304 | 257.8 | 0.698 | radial vel. | 92.9 | 0.68 | 3717 | [5] | ||
Gliese 3293 d | 0.02391 | 48.1345 | 0.19394 | radial vel. | 51.4 | 0.42 | 3466 | [5] | ||
Gliese 3293 e | 0.01032 | 13.2543 | 0.08208 | radial vel. | 51.4 | 0.42 | 3466 | [5] | ||
Gliese 3323 b | 0.00636 | 5.3636 | 0.03282 | radial vel. | 17.4 | 0.16 | 3159 | [5] | ||
Gliese 3323 c | 0.00727 | 40.54 | 0.1264 | radial vel. | 17.4 | 0.16 | 3159 | [5] | ||
Gliese 3942 b | 0.0225 | 6.905 | 0.0608 | 590 | radial vel. | 55.3 | 0.63 | 3867 | [8] | |
HAT-P-67b | 0.34 | 2.085 | 4.81010250 | 0.06505 | transit | 1000 | 1.642 | 6406 | [9] | |
HATS-36b | 2.79±0.40 | 1.263±0.045 | 4.1752379±0.0000021 | 0.0529±0.0011 | 1363±40 | transit | 2860±70 | 1.135±0.067 | 5970±160 | Host star also known as K2-145 [10] Host star also known as K2-145 |
HATS-43b | 0.261±0.054 | 1.180±0.050 | 4.3888497 | 0.04944±0.00046 | 1003±27 | transit | 1194.1±7.4 | 0.837±0.023 | 5099±61 | [11] |
HATS-44b | 0.56±0.11 | 1.067+0.125 −0.071 | 2.7439004 | 0.03649±0.00030 | 1161±34 | transit | 1474±11 | 0.860±0.021 | 5080±100 | [11] |
HATS-45b | 0.70±0.15 | 1.286±0.093 | 4.1876244 | 0.05511±0.00069 | 1518±45 | transit | 2575±38 | 1.272±0.048 | 6450±110 | [11] |
HATS-46b | 0.173±0.062 | 0.903+0.058 −0.045 | 4.7423729 | 0.05367±0.00053 | 1054±29 | transit | 1500±13 | 0.917±0.027 | 5495±69 | [11] |
HATS-50b | 0.39 | 1.130 | 3.8297015 | 0.05046 | transit | 2340 | 1.17 | 5990 | [12] | |
HATS-51b | 0.768 | 1.41 | 3.3488702 | 0.04639 | 1553 | transit | 1560 | 1.17 | 5758 | [12] |
HATS-52b | 2.24 | 1.382 | 1.36665436 | 0.02498 | 1834 | transit | 2060 | 1.11 | 6010 | [12] |
HATS-53b | 0.595 | 1.340 | 3.8537768 | 0.04753 | 1312 | transit | 2000 | 0.96 | 5644 | [12] |
HD 3167 d | 0.0217 | 8.509 | 0.07757 | radial vel. | 149 | 0.86 | 5261 | [13] | ||
HD 17674 b | 0.87 | 623.8 | 1.42 | radial vel. | 145 | 0.98 | 5904 | [14] | ||
HD 20781 d | 0.0061+0.0012 −0.0011 | 0.2052 | 5.3135±0.001 | 0.0529+0.0024 −0.0027 | radial vel. | 115.36±4.4 | 0.7 | 5256±29 | [15] | |
HD 20781 e | 0.0168+0.0022 −0.0021 | 0.2183 | 13.8905+0.0033 −0.0034 | 0.1004+0.0046 −0.0051 | radial vel. | 115.36±4.4 | 0.7 | 5256±29 | [15] | |
HD 20794 e | 0.0150 | 147.02 | 0.509 | radial vel. | 19.8 | 0.7 | 5401 | [16] | ||
HD 27894 c | 0.162 | 36.07 | 0.198 | radial vel. | 138.2 | 0.8 | 4875 | [17] | ||
HD 27894 d | 5.415 | 5174 | 5.448 | radial vel. | 138.2 | 0.8 | 4875 | [17] | ||
HD 29021 b | 2.4 | 1362.3 | 2.28 | radial vel. | 100 | 0.85 | 5560 | [14] | ||
HD 34445 c | 0.168 | 214.67 | 0.7181 | radial vel. | 146.8 | 1.07 | 5836 | [18] Likely a false positive [19] | ||
HD 34445 d | 0.0970 | 117.87 | 0.4817 | radial vel. | 146.8 | 1.07 | 5836 | [18] Likely a false positive [19] | ||
HD 34445 e | 0.0529 | 49.175 | 0.2687 | radial vel. | 146.8 | 1.07 | 5836 | [18] Likely a false positive [19] | ||
HD 34445 f | 0.119 | 676.8 | 1.543 | radial vel. | 146.8 | 1.07 | 5836 | [18] Likely a false positive [19] | ||
HD 34445 g | 0.38 | 5700 | 6.36 | radial vel. | 146.8 | 1.07 | 5836 | [18] Likely a false positive [19] | ||
HD 40956 b | 2.7 | 578.6 | 1.4 | radial vel. | 385 | 2.00 | 4869 | [20] | ||
HD 42012 b | 1.6 | 857.5 | 1.67 | radial vel. | 121 | 0.83 | 5405 | [14] | ||
HD 45184 c | 0.0277+0.0034 −0.0032 | 13.1354+0.0026 −0.0025 | 0.11+0.0034 −0.0036 | radial vel. | 71.36±0.62 | 1.03 | 5869±14 | [21] | ||
HD 76920 b | 3.93 | 415.891+0.043 −0.039 | 1.149 | radial vel. | 602.7 | 1.17 | 4698 | Extremely eccentric orbit around an evolved red giant [22] [23] [24] | ||
HD 93385 Ab | 0.0125±0.0015 | 7.3422±0.0014 | 0.0749±0.0017 | 1129±19 | radial vel. | 141.6±0.2 | 1.04±0.01 | 5823±35 | [21] Confirmed in 2021, renamed from HD 93385 d [25] | |
HD 106315 b | 0.0255 | 0.207 | 9.55804 | 0.0905 | 1046 | transit | 358 | 1.08 | 6277 | Host star also known as K2-109 [26] |
HD 106315 c | 0.0560 | 0.385 | 21.05788 | 0.1533 | 804 | transit | 358 | 1.08 | 6277 | Host star also known as K2-109 [26] |
HD 111591 b | 4.4 | 1056.4 | 2.5 | radial vel. | 352 | 1.94 | 4884 | [20] | ||
HD 113996 b | 6.3 | 610.2 | 1.6 | radial vel. | 331.4 | 1.49 | 4181 | [20] | ||
HD 147379 b | 0.0777 | 86.54 | 0.3193 | radial vel. | 35.01 | 0.58 | 4090 | [27] | ||
HD 176986 b | 0.0181 | 6.48980 | 0.06296 | radial vel. | 86.1 | 0.79 | 4931 | [28] | ||
HD 176986 c | 0.02888 | 16.8191 | 0.11878 | radial vel. | 86.1 | 0.79 | 4931 | [28] | ||
HD 177565 b | 0.04751 | 44.505 | 0.246 | radial vel. | 56 | 1.0 | [29] | |||
HD 208897 b | 1.40 | 352.7 | 1.05 | radial vel. | 211 | 1.25 | 4860 | [30] | ||
HIP 65426 b | 9.0±3.0 | 1.5±0.1 | 230,400 | 92 | 1500+100 −200 | imaging | 363.3±12.3 | 1.96±0.05 | 8840±200 | Gas giant orbiting the host star also known as HD 116434 [31] [32] |
K2-18c | 0.0236 | 8.962 | 0.060 | 363 | radial vel. | 110 | 0.36 | 3547 | [33] | |
K2-105b | 0.09439 | 0.369 | 8.266902 | 0.081 | transit | 760 | 1.01 | 5434 | [34] | |
K2-106b | 0.0263 | 0.136 | 0.571292 | 0.0116 | 2333 | transit | 798 | 0.95 | 5470 | [35] Host star also known as EPIC 220674823 |
K2-106c | 0.226 | 13.341245 | transit | 830 | 0.93 | 5590 | [35] Host star also known as EPIC 220674823 | |||
K2-108b | 0.18689 | 0.471 | 4.73401 | 0.0573 | 1446 | transit | 1530 | 1.12 | 5474 | [36] |
K2-111b | 0.0271 | 0.17 | 5.35117 | 0.0621 | 1309 | transit | 680 | 0.88 | 5730 | [37] |
K2-114b | 1.85 | 0.942 | 11.39109 | 0.09309 | 719 | transit | 1570 | 0.83 | 5027 | [38] |
K2-115b | 0.84 | 1.115 | 20.273034 | 0.1367 | 682 | transit | 1360 | 0.83 | 5560 | [38] |
K2-116b | 0.062 | 4.655411 | 0.048 | transit | 183.1 | 0.69 | 4348 | [39] Host star also known as BD-12 6259 | ||
K2-117b | 0.175 | 1.291505 | 0.019 | transit | 333.5 | 0.58 | 3842 | [40] | ||
K2-117c | 0.181 | 5.444820 | 0.051 | transit | 333.5 | 0.58 | 3842 | [40] | ||
K2-118b | 0.227 | 50.92092 | 0.245 | transit | 1057 | 0.76 | 4726 | [39] | ||
K2-119b | 0.204 | 7.728578 | 0.070 | transit | 1180 | 0.76 | 4753 | [39] | ||
K2-120b | 0.179 | 9.562742 | 0.078 | transit | 950 | 0.69 | 4350 | [39] | ||
K2-121b | 0.814 | 5.185754 | 0.052 | transit | 552 | 0.71 | 4471 | [39] | ||
K2-122b | 0.114 | 2.219405 | 0.029 | transit | 236 | 0.63 | 3993 | [39] [40] | ||
K2-123b | 0.236 | 30.956763 | 0.167 | transit | 529 | 0.65 | 4076 | [39] [40] | ||
K2-124b | 0.236 | 6.413539 | 0.051 | transit | 448 | 0.44 | 3561 | [39] | ||
K2-125b | 0.194 | 21.750264 | 0.121 | transit | 415 | 0.49 | 3654 | [39] | ||
K2-126b | 0.164 | 7.387073 | 0.066 | transit | 332 | 0.70 | 4368 | [39] | ||
K2-127b | 0.773 | 3.588165 | 0.041 | transit | 2370 | 0.70 | 4388 | [39] | ||
K2-128b | 0.127 | 5.675819 | 0.056 | transit | 373 | 0.71 | 4470 | [39] | ||
K2-129b | 0.0928 | 8.239493 | 0.057 | transit | 90.19±0.07 | 0.36 | 3459 | [39] Host star also known as LP 868-19 | ||
K2-130b | 0.112 | 2.494120 | 0.032 | transit | 384.4±0.6 | 0.70 | 4356 | [39] | ||
K2-131b | 0.017 | 0.152 | 0.36931 | 0.009500 | 2062 | transit | 501 | 0.84 | 5245 | [41] |
K2-132b | 1.30 | 9.1751 | transit | 568 | 1.08±0.08 | 4840±90 | [42] | |||
K2-133b | 0.117 | 3.0712 | 0.033 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | Host star also known as LP 358–499, 4 planets in system [43] | ||
K2-133c | 0.132 | 4.8682 | 0.045 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | Host star also known as LP 358–499, 4 planets in system [43] | ||
K2-133d | 0.180 | 11.0234 | 0.077 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | Host star also known as LP 358–499, 4 planets in system [43] | ||
K2-135b | 0.156 | 1.208957 | 0.020 | 1043.5 | transit | 98.8 | 0.66 | 4255 | [44] | |
K2-135c | 0.121 | 3.64802 | 0.042 | 721.9 | transit | 98.8 | 0.66 | 4255 | [44] | |
K2-135d | 0.187 | 6.20141 | 0.060 | 604.9 | transit | 98.8 | 0.66 | 4255 | [44] | |
K2-136b | 0.0883 | 7.975292 | 553 | transit | 0.74 | 4499 | [45] | |||
K2-136c | 0.057±0.006 | 0.260 | 17.307137 | 0.11728 | 425 | transit | 0.74 | 4499 | [45] [46] | |
K2-136d | 0.129 | 25.575065 | 373 | transit | 0.74 | 4499 | [45] | |||
K2-137b | 0.5 | 0.079 | 0.179715 | 0.0058 | 1471 | transit | 0.46 | 3492 | [47] | |
K2-139b | 0.387 | 0.808 | 28.38236 | 0.179 | 565 | transit | 496 | 1.8 | 5340 | [48] |
K2-140b | 0.211 | 1.093 | 6.56918 | 0.0687 | 957 | transit | 1110 | 1.00 | 5705 | [49] |
K2-141b | 0.0160±0.0013 | 0.135±0.004 | 0.2803226 | 0.00716+0.00055 −0.00065 | 2039+87 −48 | transit | 202.16±0.54 | 0.708±0.028 | 4599±79 | [50] [51] |
K2-146b | 0.196±0.021 | 2.644646 | 0.0266±0.0010 | transit | 259.2±1.5 | 0.358±0.042 | 3385±70 | [40] | ||
K2-147b | 0.123+0.015 −0.013 | 0.961917 | 0.0159±0.0005 | transit | 296.10±0.90 | 0.583±0.059 | 3672±70 | [40] Also called EPIC 213715787 [52] | ||
K2-148b | 0.119+0.017 −0.016 | 4.38395±0.00080 | 0.0454±0.0014 | transit | 407.4±2.0 | 0.650±0.061 | 4079±70 | [40] | ||
K2-148c | 0.154+0.021 −0.019 | 6.92260±0.00070 | 0.0616±0.0019 | transit | 407.4±2.0 | 0.650±0.061 | 4079±70 | [40] | ||
K2-148d | 0.146+0.021 −0.019 | 9.7579±0.0010 | 0.0774±0.0024 | transit | 407.4±2.0 | 0.650±0.061 | 4079±70 | [40] | ||
K2-149b | 0.146+0.018 −0.016 | 11.3320±0.0013 | 0.0830±0.0027 | transit | 404.8±1.8 | 0.595±0.059 | 3745±70 | [40] | ||
K2-150b | 0.178+0.024 −0.019 | 10.59357±0.00084 | 0.0727±0.0027 | transit | 335.2±2.6 | 0.457±0.051 | 3499±70 | [40] | ||
K2-151b | 0.120+0.014 −0.012 | 3.835592 | 0.0365±0.0014 | transit | 227.07±0.49 | 0.440±0.050 | 3585±70 | [40] | ||
K2-152b | 0.204+0.022 −0.021 | 32.6527±0.0035 | 0.1716±0.0012 | 337±3 | transit | 354.8±1.3 | 0.63±0.01 | 4044+34 −35 | [40] | |
K2-153b | 0.178+0.019 −0.016 | 7.51554 | 0.0614±0.0004 | 497±6 | transit | 468.7±3.0 | 0.55±0.01 | 3845±37 | [40] | |
K2-154b | 0.178+0.019 −0.010 | 3.67635 | 0.0405±0.0003 | 715+9 −8 | transit | 423.5±1.5 | 0.65+0.02 −0.01 | 4097+40 −45 | [40] | |
K2-154c | 0.185+0.016 −0.012 | 7.95478 | 0.0677±0.0005 | 552±7 | transit | 423.5±1.5 | 0.65+0.02 −0.01 | 4097+40 −45 | [40] | |
KELT-9b | 2.88 | 1.891 | 1.4811235 | 0.03462 | 4050 | transit | 615.5 | 2.52 | 10170 | Hottest confirmed exoplanet [53] |
KELT-18b | 1.18 | 1.570 | 2.8717518 | 0.04550 | 2085 | transit | 1.52 | 6670 | [54] | |
KELT-19Ab | <4.07 | 1.91 | 4.6117093 | 0.0637 | 1935 | transit | 950 | 1.62 | 7500 | [55] |
KELT-20b | 1.741 | 3.4741085 | 0.0542 | 2262 | transit | 455.6 | 1.76 | 8720 | [56] Also known as MASCARA-2b [57] | |
KELT-21b | 3.91+0 −3.91 | 1.586+0.039 −0.040 | 3.6127647 | 0.05224+0.00035 −0.00034 | 2051+29 −30 | transit | 1557±21 | 1.458+0.029 −0.028 | 7598+81 −84 | [58] |
Kepler-19d | 0.0708 | 62.95 | radial vel. | 6910 | 0.94 | 5541 | [59] | |||
Kepler-80g | 0.101 | 14.64558 | 418 | transit | 1160 | 0.73 | 4540 | [60] | ||
Kepler-90i | 0.118 | 14.44912 | 709 | transit | 2540 | 1.2 | 6080 | [60] | ||
Kepler-150 f | 0.325 | 637.2093 | 1.24 | transit | 2980±50 | 5560 | [61] | |||
Kepler-1649b | 0.0964 | 8.689090 | 0.0514 | transit | 0.22 | 3240 | [62] | |||
Kepler-1650b | 0.0856 | 1.53818001 | transit | 393 | 0.33 | 3410 | [63] | |||
Kepler-1651b | 0.164 | 9.87863917 | transit | 226 | 0.52 | 3713 | [63] | |||
Kepler-1652b | 0.143 | 38.09722 | 0.1654 | 268 | transit | 822 | 0.40 | 3638 | [64] | |
Kepler-1653b | 0.194 | 140.2524 | 0.4706 | 284 | transit | 2460 | 0.72 | 4807 | [64] | |
LHS 1140 b | 0.0209 | 0.128 | 24.73712 | 0.0875 | 254 | transit | 40.7 | 0.18 | 3216 | Potentially habitable exoplanet [65] |
MASCARA-1b | 3.7 | 1.5 | 2.148780 | 0.043 | 2570 | transit | 615.5 | 1.72 | 7554 | [66] |
MOA-2010-BLG-117Lb | 0.54±0.10 | 2369+835 −2717 | 2.9+1.6 −0.6 | microlensing | 11400±1300 | 0.58±0.11 | 4000+450 −350 | [67] | ||
MOA-2012-BLG-006Lb | 8.40 | 10.2 | microlensing | 17000 | 0.49 | [68] | ||||
MOA-2012-BLG-505Lb | 0.02108 | 0.900 | microlensing | 23500 | 0.10 | [69] | ||||
MOA-2016-BLG-227Lb | 2.8 | 1.67 | microlensing | 21000 | 0.29 | [70] | ||||
MXB 1658-298 b | 23.7 | 760 | 1.613 | timing | 1.98 | Circumbinary planet [71] | ||||
NGTS-1b | 0.812 | 1.33 | 2.647298 | 0.0326 | 790 | transit | 731 | 0.617 | 3916 | Largest exoplanet in relation to its star [72] |
OGLE-2013-BLG-0132Lb | 0.29 | 3.6 | microlensing | 13000 | 0.54 | [73] | ||||
OGLE-2013-BLG-1721Lb | 0.64 | 2.6 | microlensing | 21000 | 0.46 | [73] | ||||
OGLE-2013-BLG-1761Lb | 2.7+2.5 −1.5 | 1.8±0.5 | microlensing | 23000+3300 −3900 | 0.33+0.32 −0.19 | [74] | ||||
OGLE-2016-BLG-0263Lb | 4.10 | 5.4 | microlensing | 21000 | 0.13 | [75] | ||||
OGLE-2016-BLG-0613(AB)b | 4.18 | 6.40 | microlensing | 11100 | 0.72 | [76] | ||||
OGLE-2016-BLG-1190Lb | 13.38 | 1224 | 2.17 | microlensing | 22100 | 0.88 | Extremely massive; possible brown dwarf [77] | |||
OGLE-2016-BLG-1195Lb | 0.031 | 2.62±0.28 | microlensing | 22000±2000 | 0.57±0.06 | [78] [79] | ||||
OGLE-2017-BLG-0173Lb | 0.0103+0.0121 −0.0063 | 4493+3090 −7055 | 3.9±1.6 | microlensing | 15700+4900 −5900 | 0.40+0.39 −0.23 | 3500+1500 −500 | Atypical lensing event [80] Not an OGLE-2011-BLG-0173Lb! | ||
PSR B0329+54 b | 0.00620 | 10140 | 10.26 | timing | 1600 | 1.44 | Dubious [81] | |||
PSR J2322-2650 b | 0.7949 | 0.322963997 | 0.0102 | timing | 750 | 1.4 | [82] | |||
Qatar-6b | 0.668 | 1.062 | 3.506195 | 0.0423 | transit | 330 | 0.822 | 5052 | [83] | |
Ross 128 b | 0.00440 | 9.8658 | 0.0496 | 301 | radial vel. | 11.03 | 0.17 | 3192 | [84] | |
SAND978 b | 2.18 | 511.21 | radial vel. | 2051.3 | 1.37 | 4200 | [85] Red giant host star, belonging to M67, is also known as NGC 2682 108 | |||
TAP 26 b | 1.66 | 10.79 | 0.0968 | radial vel. | 480 | 1.04 | 4620 | Host star also known as V1069 Tauri [86] | ||
Tau Ceti g | 0.00551 | 20.00 | 0.133 | radial vel. | 12 | 0.78 | [87] | |||
Tau Ceti h | 0.00576 | 49.41 | 0.243 | radial vel. | 12 | 0.78 | [87] | |||
TRAPPIST-1e | 0.00195 | 0.082 | 6.099615 | 0.02817 | 251 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet [88] |
TRAPPIST-1f | 0.00214 | 0.093 | 9.20669 | 0.0371 | 219 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet [88] |
TRAPPIST-1g | 0.00422 | 0.101 | 12.35294 | 0.0451 | 199 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet [88] |
TRAPPIST-1h | 0.067 | 20 | 0.063 | 168 | transit | 39 | 0.08 | 2559 | [88] | |
TYC 4282-605-1 b | 10.78 | 101.54 | 0.422 | radial vel. | 2300 | 0.97 | 4300 | [89] | ||
WASP-91b | 1.34 | 1.03 | 2.798581 | 0.037 | 1160 | transit | 490 | 0.84 | 4920 | [90] |
WASP-105b | 1.8 | 0.96 | 7.87288 | 0.075 | 900 | transit | 0.89 | 5070 | [90] | |
WASP-107b | 0.12 | 0.94 | 5.721490 | 0.055 | 770 | transit | 0.69 | 4430 | [90] | |
WASP-151b | 0.31 | 1.13 | 4.533471 | 0.055 | 1290 | transit | 1570 | 1.01 | 5871 | [91] Host star also known as K2-134 |
WASP-153b | 0.39 | 1.55 | 3.332609 | 0.048 | 1700 | transit | 1400 | 1.34 | 5914 | [91] |
WASP-156b | 0.128 | 0.51 | 3.836169 | 0.0453 | 970 | transit | 460 | 0.84 | 4910 | [91] Host star also known as TOI-465 |
WASP-167b | 1.58 | 2.0219596 | 0.0365 | 2329 | transit | 1240 | 1.59 | 7000 | Host star also known as KELT-13 [92] | |
YZ Ceti b | 0.0024 | 1.96876 | 0.01634+0.00035 −0.00041 | radial vel. | 12.122±0.002 | 0.130±0.013 | 3056±60 | [93] | ||
YZ Ceti c | 0.00308 | 3.06008 | 0.02156+0.00046 −0.00054 | radial vel. | 12.122±0.002 | 0.130±0.013 | 3056±60 | [93] | ||
YZ Ceti d | 0.00359 | 4.65627 | 0.02851+0.00061 −0.00071 | radial vel. | 12.122±0.002 | 0.130±0.013 | 3056±60 | [93] |
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.
GJ 9827 is a star in the constellation of Pisces. It is a K-type main-sequence star with an apparent magnitude of 10.250. It is 97 light-years away, based on parallax.
K2-19 is an early K-type or late G-type main sequence star that is magnetically active, and has a light curve that exhibits variations in brightness of ~1%. It is located approximately 976 light-years away in the constellation Virgo. Three confirmed transiting exoplanets are known to orbit this star.
K2-28 is a metal rich M4-type main sequence star. One confirmed transiting exoplanet is known to orbit this star. There is another star 5.2 arcseconds to the north–east of K2-28 however this star has a different proper motion and is therefore physically unrelated and probably a background star.
K2-18, also known as EPIC 201912552, is a red dwarf star with two planetary companions located 124 light-years from Earth, in the constellation of Leo.
K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun. Four confirmed transiting exoplanets are known to orbit this star. A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator.
Kepler-51 is a Sun-like star that is about 500 million years old. It is orbited by three super-puff planets—Kepler-51b, c, and d—which have the lowest known densities of any known exoplanet. The planets are similar in radius to gas giants like Jupiter, but have unusually small masses for their size, only a few times greater than Earth’s.
WASP-75 is a F-type main-sequence star about 980 light-years away. The star is much younger than the Sun at approximately 2.9±0.2 billion years. WASP-75 is similar to the Sun in its concentration of heavy elements.
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 Gaia.