Astronomy:List of exoplanets discovered in 2017
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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] | |||
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] | |||
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] | |||
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] | |
0.0883 | 7.975292 | 553 | transit | 0.74 | 4499 | [45] | ||||
0.057±0.006 | 0.260 | 17.307137 | 0.11728 | 425 | transit | 0.74 | 4499 | [45][46] | ||
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] | |
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] |
Specific exoplanet lists
References
- ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. https://exoplanet.eu/catalog/.
- ↑ Villaver, E; Niedzielski, A; Wolszczan, A; Nowak, G; Kowalik, K; Adamów, M; MacIejewski, G; Deka-Szymankiewicz, B et al. (2017). "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N". Astronomy & Astrophysics 606: A38. doi:10.1051/0004-6361/201730471. Bibcode: 2017A&A...606A..38V.
- ↑ 3.0 3.1 "Transiting exoplanets from the CoRoT space mission XXIX. The hot Jupiters CoRoT-30 b and CoRoT-31 b". Astronomy & Astrophysics 635: A122. March 2020. doi:10.1051/0004-6361/201732393. https://www.aanda.org/articles/aa/full_html/2020/03/aa32393-17/aa32393-17.html. Retrieved 2021-09-01.
- ↑ Boufleur, Rodrigo C.; Emilio, Marcelo; Janot-Pacheco, Eduardo; Andrade, Laerte; Ferraz-Mello, Sylvio; Do Nascimento Jr, José-Dias; de la Reza, Ramiro (2017), "A modified CoRoT detrend algorithm and the discovery of a new planetary companion", Monthly Notices of the Royal Astronomical Society 473: 710–720, doi:10.1093/mnras/stx2187
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 5.8 Astudillo-Defru, Nicola; Forveille, Thierry; Bonfils, Xavier; Ségransan, Damien; Bouchy, François; Delfosse, Xavier et al. (2017). "The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293". Astronomy and Astrophysics 602: A88. doi:10.1051/0004-6361/201630153. Bibcode: 2017A&A...602A..88A. https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html.
- ↑ Suárez Mascareño, A. et al. (2017). "HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625". Astronomy and Astrophysics 605: A92. doi:10.1051/0004-6361/201730957. Bibcode: 2017A&A...605A..92S. https://www.aanda.org/articles/aa/full_html/2017/09/aa30957-17/aa30957-17.html.
- ↑ Trifonov, T. et al. (2018), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: A117, doi:10.1051/0004-6361/201731442
- ↑ Perger, M. et al. (2017), "HADES RV Programme with HARPS-N at TNG", Astronomy & Astrophysics 608: A63, doi:10.1051/0004-6361/201731307
- ↑ Zhou, G. et al. (2017), "HAT-P-67b: An Extremely Low Density Saturn Transiting an F-subgiant Confirmed via Doppler Tomography", The Astronomical Journal 153 (5): 211, doi:10.3847/1538-3881/aa674a
- ↑ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S. et al. (2017), "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program", The Astronomical Journal 155 (3): 119, doi:10.3847/1538-3881/aaa8e6
- ↑ 11.0 11.1 11.2 11.3 Brahm, R.; Hartman, J. D.; Jordán, A.; Bakos, G. Á.; Espinoza, N.; Rabus, M.; Bhatti, W.; Penev, K. et al. (2017), "HATS-43b, HATS-44b, HATS-45b, and HATS-46b: Four Short-period Transiting Giant Planets in the Neptune–Jupiter Mass Range", The Astronomical Journal 155 (3): 112, doi:10.3847/1538-3881/aaa898
- ↑ 12.0 12.1 12.2 12.3 Henning, Th.; Mancini, L.; Sarkis, P.; Bakos, G. Á.; Hartman, J. D.; Bayliss, D.; Bento, J.; Bhatti, W. et al. (2018), "HATS-50b through HATS-53b: Four Transiting Hot Jupiters Orbiting G-type Stars Discovered by the HATSouth Survey", The Astronomical Journal 155 (2): 79, doi:10.3847/1538-3881/aaa254
- ↑ Christiansen, Jessie L.; Vanderburg, Andrew et al. (September 2017), "Three's Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets", The Astronomical Journal 154 (3): 17, doi:10.3847/1538-3881/aa832d, 122, Bibcode: 2017AJ....154..122C.
- ↑ 14.0 14.1 14.2 Rey, J.; Hébrard, G.; Bouchy, F.; Bourrier, V.; Boisse, I.; Santos, N. C.; Arnold, L.; Astudillo-Defru, N. et al. (2017), "The SOPHIE search for northern extrasolar planets", Astronomy & Astrophysics 601: A9, doi:10.1051/0004-6361/201630089
- ↑ 15.0 15.1 Udry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A. et al. (2019), "The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions", Astronomy & Astrophysics A37: 622, doi:10.1051/0004-6361/201731173, Bibcode: 2019A&A...622A..37U
- ↑ Feng, F.; Tuomi, M.; Jones, H.R.A. (September 2017). "Evidence for at least three planet candidates orbiting HD 20794". Astronomy and Astrophysics 605 (103): 11. doi:10.1051/0004-6361/201730406. Bibcode: 2017A&A...605A.103F.
- ↑ 17.0 17.1 Trifonov, T.; Kürster, M.; Zechmeister, M.; Zakhozhay, O. V.; Reffert, S.; Lee, M. H.; Rodler, F.; Vogt, S. S. et al. (2017). "Three planets around HD 27894. A close-in pair with a 2:1 period ratio and an eccentric Jovian planet at 5.4 AU". Astronomy & Astrophysics 602: L8. doi:10.1051/0004-6361/201731044. Bibcode: 2017A&A...602L...8T.
- ↑ 18.0 18.1 18.2 18.3 18.4 Vogt, Steven S. et al. (2017). "A Six-planet System around the Star HD 34445". The Astronomical Journal 154 (5): 181. doi:10.3847/1538-3881/aa8b61. Bibcode: 2017AJ....154..181V.
- ↑ 19.0 19.1 19.2 19.3 19.4 Rosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C. et al. (2021). "The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades". The Astrophysical Journal Supplement Series 255: 8. doi:10.3847/1538-4365/abe23c.
- ↑ 20.0 20.1 20.2 Jeong, G.; Lee, B.-C.; Han, I.; Omiya, M.; Izumiura, H.; Sato, B.; Harakawa, H.; Kambe, E. et al. (2017), "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996", Astronomy & Astrophysics 610: A3, doi:10.1051/0004-6361/201629185
- ↑ 21.0 21.1 Gillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F. et al. (2017), "The Spitzersearch for the transits of HARPS low-mass planets", Astronomy & Astrophysics 601: A117, doi:10.1051/0004-6361/201629270
- ↑ Wittenmyer, Robert A.; Jones, M. I.; Horner, Jonathan; Kane, Stephen R.; Marshall, J. P.; Mustill, A. J.; Jenkins, J. S.; Rojas, P. A. Pena et al. (2017), "The Pan-Pacific Planet Search. VII. The Most Eccentric Planet Orbiting a Giant Star", The Astronomical Journal 154 (6): 274, doi:10.3847/1538-3881/aa9894
- ↑ Bergmann, C.; Jones, M. I.; Zhao, J.; Mustill, A. J.; Brahm, R.; Torres, P.; Wittenmyer, R. A.; Gunn, F. et al. (2021), "HD 76920 b pinned down: A detailed analysis of the most eccentric planetary system around an evolved star", Publications of the Astronomical Society of Australia 38, doi:10.1017/pasa.2021.8
- ↑ Jiang, Chen et al. (2023), "TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting an Extremely Eccentric Exoplanet", The Astrophysical Journal 945: 20, doi:10.3847/1538-4357/acb8ac
- ↑ Unger, N. et al. (2021), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics 654: A104, doi:10.1051/0004-6361/202141351
- ↑ 26.0 26.1 Ferraz, Alvaro; Kochetov, Evgenii (2017), A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315
- ↑ Reiners, A. et al. (2017), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: L5, doi:10.1051/0004-6361/201732165
- ↑ 28.0 28.1 Suárez Mascareño, A.; González Hernández, J. I.; Rebolo, R.; Velasco, S.; Toledo-Padrón, B.; Udry, S.; Motalebi, F.; Ségrasan, D. et al. (2018), "The RoPES project with HARPS and HARPS-N", Astronomy & Astrophysics 612: A41, doi:10.1051/0004-6361/201732042
- ↑ Feng, F.; Tuomi, M.; Jones, H. R. A. (2017), "Agatha: Disentangling periodic signals from correlated noise in a periodogram framework", Monthly Notices of the Royal Astronomical Society 470 (4): 4794–4814, doi:10.1093/mnras/stx1126
- ↑ Yılmaz, M.; Sato, B.; Bikmaev, I.; Selam, S. O.; Izumiura, H.; Keskin, V.; Kambe, E.; Melnikov, S. S. et al. (2017), "A Jupiter-mass planet around the K0 giant HD 208897", Astronomy & Astrophysics 608: A14, doi:10.1051/0004-6361/201731184
- ↑ Chauvin, G. et al. (2017), "Discovery of a warm, dusty giant planet around HIP 65426", Astronomy & Astrophysics 605: L9, doi:10.1051/0004-6361/201731152
- ↑ "HIP 65426 b - Exoplanet-catalog" (in en). https://exoplanets.nasa.gov/exoplanet-catalog/7220/hip-65426-b/.
- ↑ Cloutier, R.; Astudillo-Defru, N.; Doyon, R.; Bonfils, X.; Almenara, J.-M.; Benneke, B.; Bouchy, F.; Delfosse, X. et al. (2017), "Characterization of the K2-18 multi-planetary system with HARPS", Astronomy & Astrophysics 608: A35, doi:10.1051/0004-6361/201731558
- ↑ Narita, Norio; Hirano, Teruyuki; Fukui, Akihiko; Hori, Yasunori; Dai, Fei; Yu, Liang; Livingston, John; Ryu, Tsuguru et al. (2017), "The K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf", Publications of the Astronomical Society of Japan 69 (2), doi:10.1093/pasj/psx002
- ↑ 35.0 35.1 Guenther, E. W. et al. (2017), "K2-106, a system containing a metal-rich planet and a planet of lower density", Astronomy & Astrophysics 608: A93, doi:10.1051/0004-6361/201730885, Bibcode: 2017A&A...608A..93G
- ↑ Petigura, Erik A.; Sinukoff, Evan; Lopez, Eric D.; Crossfield, Ian J. M.; Howard, Andrew W.; Brewer, John M.; Fulton, Benjamin J.; Isaacson, Howard T. et al. (2017), "Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes", The Astronomical Journal 153 (4): 142, doi:10.3847/1538-3881/aa5ea5
- ↑ Fridlund, Malcolm et al. (2017), "K2-111 b − a short period super-Earth transiting a metal poor, evolved old star", Astronomy & Astrophysics 604: A16, doi:10.1051/0004-6361/201730822
- ↑ 38.0 38.1 Shporer, Avi; Zhou, George; Fulton, Benjamin J.; Vanderburg, Andrew; Espinoza, Nestor; Collins, Karen; Ciardi, David; Bayliss, Daniel et al. (2017), "K2-114b and K2-115b: Two Transiting Warm Jupiters", The Astronomical Journal 154 (5): 188, doi:10.3847/1538-3881/aa8bb9
- ↑ 39.00 39.01 39.02 39.03 39.04 39.05 39.06 39.07 39.08 39.09 39.10 39.11 39.12 39.13 Dressing, Courtney D.; Vanderburg, Andrew; Schlieder, Joshua E.; Crossfield, Ian J. M.; Knutson, Heather A.; Newton, Elisabeth R.; Ciardi, David R.; Fulton, Benjamin J. et al. (2017), "Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. II. Planetary Systems Observed During Campaigns 1–7", The Astronomical Journal 154 (5): 207, doi:10.3847/1538-3881/aa89f2
- ↑ 40.00 40.01 40.02 40.03 40.04 40.05 40.06 40.07 40.08 40.09 40.10 40.11 40.12 40.13 40.14 40.15 Hirano, Teruyuki et al. (2017), "Exoplanets around Low-mass Stars Unveiled byK2", The Astronomical Journal 155 (3): 127, doi:10.3847/1538-3881/aaa9c1
- ↑ Dai, Fei et al. (2017), "The Discovery and Mass Measurement of a New Ultra-short-period Planet: K2-131b", The Astronomical Journal 154 (6): 226, doi:10.3847/1538-3881/aa9065
- ↑ Grunblatt, Samuel K.; Huber, Daniel; Gaidos, Eric; Lopez, Eric D.; Howard, Andrew W.; Isaacson, Howard T.; Sinukoff, Evan; Vanderburg, Andrew et al. (2017), "Seeing Double withK2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars", The Astronomical Journal 154 (6): 254, doi:10.3847/1538-3881/aa932d
- ↑ 43.0 43.1 43.2 Wells, R.; Poppenhaeger, K.; Watson, C. A. (2017), "Three small transiting planets around the M-dwarf host star LP 358-499", Monthly Notices of the Royal Astronomical Society: Letters 473: L131–L135, doi:10.1093/mnrasl/slx171
- ↑ 44.0 44.1 44.2 Rodriguez, Joseph E; Vanderburg, Andrew; Eastman, Jason D; Mann, Andrew W; Crossfield, Ian J. M; Ciardi, David R; Latham, David W; Quinn, Samuel N (2018). "A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc". The Astronomical Journal 155 (2): 72. doi:10.3847/1538-3881/aaa292. Bibcode: 2018AJ....155...72R.
- ↑ 45.0 45.1 45.2 Mann, Andrew W.; Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A. et al. (2017), "Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet", The Astronomical Journal 155: 4, doi:10.3847/1538-3881/aa9791
- ↑ Mayo, Andrew W. et al. (2023), "Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass", The Astronomical Journal 165 (6): 235, doi:10.3847/1538-3881/acca1c
- ↑ Smith, A M S. et al. (2018), "K2-137 b: An Earth-sized planet in a 4.3-h orbit around an M-dwarf", Monthly Notices of the Royal Astronomical Society 474 (4): 5523–5533, doi:10.1093/mnras/stx2891
- ↑ Barragán, O.; Gandolfi, D.; Smith, A M S.; Deeg, H. J.; Fridlund, M C V.; Persson, C. M.; Donati, P.; Endl, M. et al. (2017), "K2-139 b: A low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star", Monthly Notices of the Royal Astronomical Society 475 (2): 1765–1776, doi:10.1093/mnras/stx3207
- ↑ Giles, H A C.; Bayliss, D.; Espinoza, N.; Brahm, R.; Blanco-Cuaresma, S.; Shporer, A.; Armstrong, D.; Lovis, C. et al. (2017), "K2-140b – an eccentric 6.57 d transiting hot Jupiter in Virgo", Monthly Notices of the Royal Astronomical Society 475 (2): 1809–1818, doi:10.1093/mnras/stx3300
- ↑ Okoli, Chiamaka (2017), K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours
- ↑ Malavolta, Luca et al. (2018). "An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141". The Astronomical Journal 155 (3): 107. doi:10.3847/1538-3881/aaa5b5. Bibcode: 2018AJ....155..107M.
- ↑ Adams, Elisabeth R. (2020). "Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10". The Planetary Science Journal 2 (4): 152. doi:10.3847/PSJ/ac0ea0. Bibcode: 2021PSJ.....2..152A.
- ↑ Gaudi, B. Scott et al. (2017), "A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host", Nature 546 (7659): 514–518, doi:10.1038/nature22392, PMID 28582774
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- ↑ Siverd, Robert J. et al. (2017), "KELT-19Ab: AP~ 4.6-day Hot Jupiter Transiting a Likely Am Star with a Distant Stellar Companion", The Astronomical Journal 155: 35, doi:10.3847/1538-3881/aa9e4d
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- ↑ Rainer, M. et al. (2021), "The GAPS programme at TNG", Astronomy & Astrophysics 649: A29, doi:10.1051/0004-6361/202039247
- ↑ Johnson, Marshall C; Rodriguez, Joseph E; Zhou, George; Gonzales, Erica J; Cargile, Phillip A; Crepp, Justin R; Penev, Kaloyan; Stassun, Keivan G et al. (2018). "KELT-21b: A Hot Jupiter Transiting the Rapidly Rotating Metal-poor Late-A Primary of a Likely Hierarchical Triple System". The Astronomical Journal 155 (2): 100. doi:10.3847/1538-3881/aaa5af. Bibcode: 2018AJ....155..100J.
- ↑ Malavolta, Luca et al. (2017), "The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations", The Astronomical Journal 153 (5): 224, doi:10.3847/1538-3881/aa6897
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- ↑ Schmitt, Joseph R.; Jenkins, Jon M.; Fischer, Debra A. (2017), "A Search for Lost Planets in theKepler Multi-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 F", The Astronomical Journal 153 (4): 180, doi:10.3847/1538-3881/aa62ad, PMID 29375142
- ↑ Angelo, Isabel; Rowe, Jason F.; Howell, Steve B.; Quintana, Elisa V.; Still, Martin; Mann, Andrew W.; Burningham, Ben; Barclay, Thomas et al. (2017), "Kepler-1649b: An Exo-Venus in the Solar Neighborhood", The Astronomical Journal 153 (4): 162, doi:10.3847/1538-3881/aa615f
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- ↑ Ferraz-Mello, S.; Gomes, G. O. (2020). "Tidal evolution of exoplanetary systems hosting potentially habitable exoplanets. The cases of LHS-1140 b-c and K2-18 b-c". Monthly Notices of the Royal Astronomical Society 494 (4): 5082–5090. doi:10.1093/mnras/staa1110. Bibcode: 2020MNRAS.494.5082G.
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- ↑ Poleski, R. et al. (2017), "A companion on the planet/Brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing", Astronomy & Astrophysics 604: A103, doi:10.1051/0004-6361/201730928
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- ↑ Jain, Chetana; Paul, Biswajit; Sharma, Rahul; Jaleel, Abdul; Dutta, Anjan (2017), "Indication of a massive circumbinary planet orbiting the low-mass X-ray binary MXB 1658−298", Monthly Notices of the Royal Astronomical Society: Letters 468: L118–L122, doi:10.1093/mnrasl/slx039
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- ↑ Han, C. et al. (2017), "OGLE-2016-BLG-0263Lb: Microlensing Detection of a Very Low-mass Binary Companion through a Repeating Event Channel", The Astronomical Journal 154 (4): 133, doi:10.3847/1538-3881/aa859a
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- ↑ Alsubai, Khalid; Tsvetanov, Zlatan I.; Latham, David W.; Bieryla, Allyson; Esquerdo, Gilbert A.; Mislis, Dimitris; Pyrzas, Stylianos; Foxell, Emma et al. (2017), "Qatar Exoplanet Survey: Qatar-6b—A Grazing Transiting Hot Jupiter", The Astronomical Journal 155 (2): 52, doi:10.3847/1538-3881/aaa000
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- ↑ Brucalassi, A.; Koppenhoefer, J.; Saglia, R.; Pasquini, L.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Libralato, M. et al. (2017), "Search for giant planets in M 67", Astronomy & Astrophysics 603: A85, doi:10.1051/0004-6361/201527562
- ↑ Yu, L.; Donati, J.-F.; Hébrard, E. M.; Moutou, C.; Malo, L.; Grankin, K.; Hussain, G.; Collier Cameron, A. et al. (2017), "A hot Jupiter around the very active weak-line T Tauri star TAP 26", Monthly Notices of the Royal Astronomical Society: stx009, doi:10.1093/mnras/stx009
- ↑ 87.0 87.1 Feng, Fabo et al. (2017). "Color Difference Makes a Difference: Four Planet Candidates around Tau Ceti". The Astronomical Journal 154 (4): 135. doi:10.3847/1538-3881/aa83b4. Bibcode: 2017AJ....154..135F.
- ↑ 88.0 88.1 88.2 88.3 Gillon, M.; Triaud, A. H. M. J.; Demory, B.-O. et al. (February 2017). "Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1". Nature 542 (7642): 456–460. doi:10.1038/nature21360. PMID 28230125. PMC 5330437. Bibcode: 2017Natur.542..456G. http://www.eso.org/public/archives/releases/sciencepapers/eso1706/eso1706a.pdf.
- ↑ González-Álvarez, E. et al. (2022), "The GAPS Programme with HARPS-N at TNG", Astronomy & Astrophysics 606: A51, doi:10.1051/0004-6361/201731124
- ↑ 90.0 90.1 90.2 Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M. et al. (2017), "The discoveries of WASP-91b, WASP-105b and WASP-107b: Two warm Jupiters and a planet in the transition region between ice giants and gas giants", Astronomy & Astrophysics 604: A110, doi:10.1051/0004-6361/201730439
- ↑ 91.0 91.1 91.2 Demangeon, O. D. S. et al. (2018), "The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert", Astronomy & Astrophysics 610: A63, doi:10.1051/0004-6361/201731735
- ↑ Temple, L. Y. et al. (2017), "WASP-167b/KELT-13b: Joint discovery of a hot Jupiter transiting a rapidly rotating F1V star", Monthly Notices of the Royal Astronomical Society 471 (3): 2743–2752, doi:10.1093/mnras/stx1729
- ↑ 93.0 93.1 93.2 Astudillo-Defru, N.; Díaz, R. F.; Bonfils, X.; Almenara, J. M.; Delisle, J.-B.; Bouchy, F.; Delfosse, X.; Forveille, T. et al. (2017), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics 605: L11, doi:10.1051/0004-6361/201731581
![]() | Original source: https://en.wikipedia.org/wiki/List of exoplanets discovered in 2017.
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