List of exoplanets discovered in 2017
Appearance
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] | |
Gliese 273 b | 0.00909 | 18.6498 | 0.091101 | 259 | radial vel. | 12 | 0.29 | 3382 | Also known as Luyten b, potentially habitable exoplanet.[5] | |
Gliese 273 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 str 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] | ||
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[24] | |
HD 106315 b | 0.0255 | 0.207 | 9.55804 | 0.0905 | 1046 | transit | 358 | 1.08 | 6277 | Host star also known as K2-109[25] |
HD 106315 c | 0.0560 | 0.385 | 21.05788 | 0.1533 | 804 | transit | 358 | 1.08 | 6277 | Host star also known as K2-109[25] |
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 | [26] | ||
HD 176986 b | 0.0181 | 6.48980 | 0.06296 | radial vel. | 86.1 | 0.79 | 4931 | [27] | ||
HD 176986 c | 0.02888 | 16.8191 | 0.11878 | radial vel. | 86.1 | 0.79 | 4931 | [27] | ||
HD 177565 b | 0.04751 | 44.505 | 0.246 | radial vel. | 56 | 1.0 | [28] | |||
HD 208897 b | 1.40 | 352.7 | 1.05 | radial vel. | 211 | 1.25 | 4860 | [29] | ||
HIP 65426 b | 9.0 | 92 | 1450 | imaging | 363 | 1.96 | 8840 | Host star also known as HD 116434[30] | ||
K2-18c | 0.0236 | 8.962 | 0.060 | 363 | radial vel. | 110 | 0.36 | 3547 | [31] | |
K2-105b | 0.09439 | 0.369 | 8.266902 | 0.081 | transit | 760 | 1.01 | 5434 | [32] | |
K2-106b | 0.0263 | 0.136 | 0.571292 | 0.0116 | 2333 | transit | 798 | 0.95 | 5470 | [33] Host star also known as EPIC 220674823 |
K2-106c | 0.226 | 13.341245 | transit | 830 | 0.93 | 5590 | [33] Host star also known as EPIC 220674823 | |||
K2-108b | 0.18689 | 0.471 | 4.73401 | 0.0573 | 1446 | transit | 1530 | 1.12 | 5474 | [34] |
K2-111b | 0.0271 | 0.17 | 5.35117 | 0.0621 | 1309 | transit | 680 | 0.88 | 5730 | [35] |
K2-114b | 1.85 | 0.942 | 11.39109 | 0.09309 | 719 | transit | 1570 | 0.83 | 5027 | [36] |
K2-115b | 0.84 | 1.115 | 20.273034 | 0.1367 | 682 | transit | 1360 | 0.83 | 5560 | [36] |
K2-116b | 0.062 | 4.655411 | 0.048 | transit | 183.1 | 0.69 | 4348 | [37] Host star also known as BD-12 6259 | ||
K2-117b | 0.175 | 1.291505 | 0.019 | transit | 333.5 | 0.58 | 3842 | [38] | ||
K2-117c | 0.181 | 5.444820 | 0.051 | transit | 333.5 | 0.58 | 3842 | [38] | ||
K2-118b | 0.227 | 50.92092 | 0.245 | transit | 1057 | 0.76 | 4726 | [37] | ||
K2-119b | 0.204 | 7.728578 | 0.070 | transit | 1180 | 0.76 | 4753 | [37] | ||
K2-120b | 0.179 | 9.562742 | 0.078 | transit | 950 | 0.69 | 4350 | [37] | ||
K2-121b | 0.814 | 5.185754 | 0.052 | transit | 552 | 0.71 | 4471 | [37] | ||
K2-122b | 0.114 | 2.219405 | 0.029 | transit | 236 | 0.63 | 3993 | [37][38] | ||
K2-123b | 0.236 | 30.956763 | 0.167 | transit | 529 | 0.65 | 4076 | [37][38] | ||
K2-124b | 0.236 | 6.413539 | 0.051 | transit | 448 | 0.44 | 3561 | [37] | ||
K2-125b | 0.194 | 21.750264 | 0.121 | transit | 415 | 0.49 | 3654 | [37] | ||
K2-126b | 0.164 | 7.387073 | 0.066 | transit | 332 | 0.70 | 4368 | [37] | ||
K2-127b | 0.773 | 3.588165 | 0.041 | transit | 2370 | 0.70 | 4388 | [37] | ||
K2-128b | 0.127 | 5.675819 | 0.056 | transit | 373 | 0.71 | 4470 | [37] | ||
K2-129b | 0.0928 | 8.239493 | 0.057 | transit | 90.19±0.07 | 0.36 | 3459 | [37] Host star also known as LP 868-19 | ||
K2-130b | 0.112 | 2.494120 | 0.032 | transit | 384.4±0.6 | 0.70 | 4356 | [37] | ||
K2-131b | 0.017 | 0.152 | 0.36931 | 0.009500 | 2062 | transit | 501 | 0.84 | 5245 | [39] |
K2-132b | 1.30 | 9.1751 | transit | 568 | 1.08±0.08 | 4840±90 | [40] | |||
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[41] | ||
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[41] | ||
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[41] | ||
K2-135b | 0.156 | 1.208957 | 0.020 | 1043.5 | transit | 98.8 | 0.66 | 4255 | [42] | |
K2-135c | 0.121 | 3.64802 | 0.042 | 721.9 | transit | 98.8 | 0.66 | 4255 | [42] | |
K2-135d | 0.187 | 6.20141 | 0.060 | 604.9 | transit | 98.8 | 0.66 | 4255 | [42] | |
K2-136b | 0.0883 | 7.975292 | 553 | transit | 0.74 | 4499 | [43] | |||
K2-136c | 0.260 | 17.307137 | 0.11728 | 425 | transit | 0.74 | 4499 | [43] | ||
K2-136d | 0.129 | 25.575065 | 373 | transit | 0.74 | 4499 | [43] | |||
K2-137b | 0.5 | 0.079 | 0.179715 | 0.0058 | 1471 | transit | 0.46 | 3492 | [44] | |
K2-139b | 0.387 | 0.808 | 28.38236 | 0.179 | 565 | transit | 496 | 1.8 | 5340 | [45] |
K2-140b | 0.211 | 1.093 | 6.56918 | 0.0687 | 957 | transit | 1110 | 1.00 | 5705 | [46] |
K2-146b | 0.196±0.021 | 2.644646 | 0.0266±0.0010 | transit | 259.2±1.5 | 0.358±0.042 | 3385±70 | [38] | ||
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 | [38] Also called EPIC 213715787[47] | ||
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 | [38] | ||
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 | [38] | ||
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 | [38] | ||
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 | [38] | ||
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 | [38] | ||
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 | [38] | ||
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 |
[38] | |
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 | [38] | |
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 |
[38] | |
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 |
[38] | |
KELT-9b | 2.88 | 1.891 | 1.4811235 | 0.03462 | 4050 | transit | 615.5 | 2.52 | 10170 | Hottest confirmed exoplanet[48] |
KELT-18b | 1.18 | 1.570 | 2.8717518 | 0.04550 | 2085 | transit | 1.52 | 6670 | [49] | |
KELT-19Ab | <4.07 | 1.91 | 4.6117093 | 0.0637 | 1935 | transit | 950 | 1.62 | 7500 | [50] |
KELT-20b | 1.741 | 3.4741085 | 0.0542 | 2262 | transit | 455.6 | 1.76 | 8720 | [51] Also known as MASCARA-2b[52] | |
Kepler-19d | 0.0708 | 62.95 | radial vel. | 6910 | 0.94 | 5541 | [53] | |||
Kepler-80g | 0.101 | 14.64558 | 418 | transit | 1160 | 0.73 | 4540 | [54] | ||
Kepler-90i | 0.118 | 14.44912 | 709 | transit | 2540 | 1.2 | 6080 | [54] | ||
Kepler-150 f | 0.325 | 637.2093 | 1.24 | transit | 2980±50 | 5560 | [55] | |||
Kepler-1649b | 0.0964 | 8.689090 | 0.0514 | transit | 0.22 | 3240 | [56] | |||
Kepler-1650b | 0.0856 | 1.53818001 | transit | 393 | 0.33 | 3410 | [57] | |||
Kepler-1651b | 0.164 | 9.87863917 | transit | 226 | 0.52 | 3713 | [57] | |||
Kepler-1652b | 0.143 | 38.09722 | 0.1654 | 268 | transit | 822 | 0.40 | 3638 | [58] | |
Kepler-1653b | 0.194 | 140.2524 | 0.4706 | 284 | transit | 2460 | 0.72 | 4807 | [58] | |
LHS 1140 b | 0.0209 | 0.128 | 24.73712 | 0.0875 | 254 | transit | 40.7 | 0.18 | 3216 | Potentially habitable exoplanet[59] |
MASCARA-1b | 3.7 | 1.5 | 2.148780 | 0.043 | 2570 | transit | 615.5 | 1.72 | 7554 | [60] |
MOA-2012-BLG-006Lb | 8.40 | 10.2 | microlensing | 17000 | 0.49 | [61] | ||||
MOA-2012-BLG-505Lb | 0.02108 | 0.900 | microlensing | 23500 | 0.10 | [62] | ||||
MOA-2016-BLG-227Lb | 2.8 | 1.67 | microlensing | 21000 | 0.29 | [63] | ||||
MXB 1658-298 b | 23.7 | 760 | 1.613 | timing | 1.98 | Circumbinary planet[64] | ||||
NGTS-1b | 0.812 | 1.33 | 2.647298 | 0.0326 | 790 | transit | 731 | 0.617 | 3916 | Largest exoplanet in relation to its star[65] |
OGLE-2013-BLG-0132Lb | 0.29 | 3.6 | microlensing | 13000 | 0.54 | [66] | ||||
OGLE-2013-BLG-1721Lb | 0.64 | 2.6 | microlensing | 21000 | 0.46 | [66] | ||||
OGLE-2016-BLG-0263Lb | 4.10 | 5.4 | microlensing | 21000 | 0.13 | [67] | ||||
OGLE-2016-BLG-0613(AB)b | 4.18 | 6.40 | microlensing | 11100 | 0.72 | [68] | ||||
OGLE-2016-BLG-1190Lb | 13.38 | 1224 | 2.17 | microlensing | 22100 | 0.88 | Extremely massive; possible brown dwarf[69] | |||
OGLE-2016-BLG-1195Lb | 0.00450 | 1.16 | microlensing | 13000 | 0.08 | [70] | ||||
PSR B0329+54 b | 0.00620 | 10140 | 10.26 | timing | 1600 | 1.44 | Dubious[71] | |||
PSR J2322-2650 b | 0.7949 | 0.322963997 | 0.0102 | timing | 750 | 1.4 | [72] | |||
Ross 128 b | 0.00440 | 9.8658 | 0.0496 | 301 | radial vel. | 11.03 | 0.17 | 3192 | [73] | |
SAND978 b | 2.18 | 511.21 | radial vel. | 2051.3 | 1.37 | 4200 | [74]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[75] | ||
Tau Ceti g | 0.00551 | 20.00 | 0.133 | radial vel. | 12 | 0.78 | [76] | |||
Tau Ceti h | 0.00576 | 49.41 | 0.243 | radial vel. | 12 | 0.78 | [76] | |||
TRAPPIST-1e | 0.00195 | 0.082 | 6.099615 | 0.02817 | 251 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet[77] |
TRAPPIST-1f | 0.00214 | 0.093 | 9.20669 | 0.0371 | 219 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet[77] |
TRAPPIST-1g | 0.00422 | 0.101 | 12.35294 | 0.0451 | 199 | transit | 39 | 0.08 | 2559 | Potentially habitable exoplanet[77] |
TRAPPIST-1h | 0.067 | 20 | 0.063 | 168 | transit | 39 | 0.08 | 2559 | [77] | |
TYC 4282-605-1 b | 10.78 | 101.54 | 0.422 | radial vel. | 2300 | 0.97 | 4300 | [78] | ||
WASP-91b | 1.34 | 1.03 | 2.798581 | 0.037 | 1160 | transit | 490 | 0.84 | 4920 | [79] |
WASP-105b | 1.8 | 0.96 | 7.87288 | 0.075 | 900 | transit | 0.89 | 5070 | [79] | |
WASP-107b | 0.12 | 0.94 | 5.721490 | 0.055 | 770 | transit | 0.69 | 4430 | [79] | |
WASP-151b | 0.31 | 1.13 | 4.533471 | 0.055 | 1290 | transit | 1570 | 1.01 | 5871 | [80] Host star also known as K2-134 |
WASP-153b | 0.39 | 1.55 | 3.332609 | 0.048 | 1700 | transit | 1400 | 1.34 | 5914 | [80] |
WASP-156b | 0.128 | 0.51 | 3.836169 | 0.0453 | 970 | transit | 460 | 0.84 | 4910 | [80] 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[81] | |
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 | [82] | ||
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 | [82] | ||
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 | [82] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
- List of exoplanets and planetary debris around white dwarfs
- List of extrasolar planetary collisions
Lists of exoplanets by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (144)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (152)
- List of exoplanets discovered in 2018 (300)
- List of exoplanets discovered in 2019 (170)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (307)
- List of exoplanets discovered in 2024 (284)
- List of exoplanets discovered in 2025 (7)
References
- ^ "The Extrasolar Planets Encyclopaedia". Retrieved 2015-11-09.
- ^ Villaver, E; Niedzielski, A; Wolszczan, A; Nowak, G; Kowalik, K; Adamów, M; MacIejewski, G; Deka-Szymankiewicz, B; Maldonado, J (2017). "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N". Astronomy & Astrophysics. 606: A38. arXiv:1706.01278. Bibcode:2017A&A...606A..38V. doi:10.1051/0004-6361/201730471. S2CID 119228758.
- ^ a b Transiting exoplanets from the CoRoT space mission XXIX. The hot Jupiters CoRoT-30 b and CoRoT-31 b
- ^ 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, arXiv:1709.00351, doi:10.1093/mnras/stx2187
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c d e f g h i 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. arXiv:1703.05386. Bibcode:2017A&A...602A..88A. doi:10.1051/0004-6361/201630153. S2CID 119418595.
- ^ 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. arXiv:1705.06537. Bibcode:2017A&A...605A..92S. doi:10.1051/0004-6361/201730957. S2CID 119003137.
- ^ The CARMENES search for exoplanets around M dwarfs First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems, 2017, arXiv:1710.01595
- ^ HADES RV Programme with HARPS-N at TNG VI. GJ 3942 b behind dominant activity signals, 2017, arXiv:1709.06851
- ^ HAT-P-67b: An Extremely Low Density Saturn Transiting an F-Subgiant Confirmed via Doppler Tomography, 2017, arXiv:1702.00106
- ^ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S.; Brahm, R.; Jordán, A.; Espinoza, N.; Rabus, M.; Tan, T. G.; Penev, K.; Bhatti, W.; De Val-Borro, M.; Suc, V.; Csubry, Z.; Henning, Th.; Sarkis, P.; Lázár, J.; Papp, I.; Sári, P. (2017), "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program", The Astronomical Journal, 155 (3): 119, arXiv:1706.03858, doi:10.3847/1538-3881/aaa8e6, S2CID 119383417
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c d HATS-43b, HATS-44b, HATS-45b, and HATS-46b: Four Short Period Transiting Giant Planets in the Neptune-Jupiter Mass Range, 2017, arXiv:1707.07093
- ^ a b c d HATS-50b THROUGH HATS-53b: FOUR TRANSITING HOT JUPITERS ORBITING G-TYPE STARS DISCOVERED BY THE HATSOUTH SURVEY, 2017, arXiv:1712.04324
- ^ 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, arXiv:1706.01892, Bibcode:2017AJ....154..122C, doi:10.3847/1538-3881/aa832d, S2CID 54196245, 122.
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c The SOPHIE search for northern extrasolar planets XII. Three giant planets suitable for astrometric mass determination with Gaia, 2017, arXiv:1702.06393
- ^ a b Udry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Wyttenbach, A.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (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, arXiv:1705.05153, Bibcode:2019A&A...622A..37U, doi:10.1051/0004-6361/201731173, S2CID 119095511
- ^ 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. arXiv:1705.05124. Bibcode:2017A&A...605A.103F. doi:10.1051/0004-6361/201730406. S2CID 119084078.
- ^ a b Trifonov, T.; Kürster, M.; Zechmeister, M.; Zakhozhay, O. V.; Reffert, S.; Lee, M. H.; Rodler, F.; Vogt, S. S.; Brems, S. S. (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. arXiv:1706.00509. Bibcode:2017A&A...602L...8T. doi:10.1051/0004-6361/201731044. S2CID 119105619.
- ^ a b c d e Vogt, Steven S.; et al. (2017). "A Six-planet System around the Star HD 34445". The Astronomical Journal. 154 (5): 181. arXiv:1710.07337. Bibcode:2017AJ....154..181V. doi:10.3847/1538-3881/aa8b61. S2CID 119182115.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b c d e Rosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C.; Petigura, Erik A.; Knutson, Heather A.; Behmard, Aida; Chontos, Ashley; Crepp, Justin R.; Crossfield, Ian J. M.; Dalba, Paul A.; Fischer, Debra A.; Henry, Gregory W.; Kane, Stephen R.; Kosiarek, Molly; Marcy, Geoffrey W.; Rubenzahl, Ryan A.; Weiss, Lauren M.; Wright, Jason T. (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. arXiv:2105.11583. doi:10.3847/1538-4365/abe23c. S2CID 235186973.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b c Detection of planet candidates around K giants, HD 40956, HD 111591, and HD 113996, 2017, arXiv:1711.07173
- ^ a b Gillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F.; Queloz, D.; Seager, S.; Ségransan, D.; Udry, S. (2017), "The Spitzersearch for the transits of HARPS low-mass planets", Astronomy & Astrophysics, 601: A117, arXiv:1701.01303, doi:10.1051/0004-6361/201629270, S2CID 86862862
- ^ The Pan-Pacific Planet Search VII: The most eccentric planet orbiting a giant star, 2017, arXiv:1711.05378
- ^ HD 76920 b pinned down: a detailed analysis of the most eccentric planetary system around an evolved star, 2021, arXiv:2102.08902
- ^ Unger, N.; et al. (2021), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics, 654: A104, arXiv:2108.10198, doi:10.1051/0004-6361/202141351, S2CID 239033129
- ^ a b A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315, 2017, arXiv:1701.03808
- ^ The CARMENES search for exoplanets around M dwarfs - HD 147379b: A nearby Neptune in the temperate zone of an early-M dwarf, 2017, arXiv:1712.05797
- ^ a b The RoPES project with HARPS and HARPS-N. I. A system of super-Earths orbiting the moderately active K-dwarf HD 176986, 2017, arXiv:1712.01046
- ^ Agatha: disentangling periodic signals from correlated noise in a periodogram framework, 2017, arXiv:1705.03089
- ^ A Jupiter-mass planet around the K0 giant HD 208897, 2017, arXiv:1708.01895
- ^ Discovery of a warm, dusty giant planet around HIP65426, 2017, arXiv:1707.01413
- ^ Characterization of the K2-18 multi-planetary system with HARPS A habitable zone super-Earth and discovery of a second, warm super-Earth on a non-coplanar orbit, 2017, arXiv:1707.04292
- ^ The K2-ESPRINT Project VI: K2-105 b, a Hot-Neptune around a Metal-rich G-dwarf, 2017, arXiv:1701.01294
- ^ a b 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, arXiv:1705.04163, Bibcode:2017A&A...608A..93G, doi:10.1051/0004-6361/201730885, S2CID 55692535
- ^ Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes, 2017, arXiv:1702.00013
- ^ K2-111 b - a short period super-Earth transiting a metal poor, evolved old star, 2017, arXiv:1704.08284
- ^ a b K2-114b and K2-115b: Two Transiting Warm Jupiters, 2017, arXiv:1708.07128
- ^ a b c d e f g h i j k l m n CHARACTERIZING K2 CANDIDATE PLANETARY SYSTEMS ORBITING LOW-MASS STARS II: PLANETARY SYSTEMS OBSERVED DURING CAMPAIGNS 1–7, 2017, arXiv:1703.07416
- ^ a b c d e f g h i j k l m n o p EXOPLANETS AROUND LOW-MASS STARS UNVEILED BY K2, 2017, arXiv:1710.03239
- ^ The discovery and mass measurement of a new ultra-short-period planet: K2-131b, 2017, arXiv:1710.00076
- ^ SEEING DOUBLE WITH K2: TESTING RE-INFLATION WITH TWO REMARKABLY SIMILAR PLANETS AROUND RED GIANT BRANCH STARS, 2017, arXiv:1706.05865
- ^ a b c Three small transiting planets around the M dwarf host star LP 358-499, 2017, arXiv:1709.01025
- ^ a b c 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. arXiv:1709.01957. Bibcode:2018AJ....155...72R. doi:10.3847/1538-3881/aaa292. S2CID 55459523.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b c ZODIACAL EXOPLANETS IN TIME (ZEIT) VI: A THREE-PLANET SYSTEM IN THE HYADES CLUSTER INCLUDING AN EARTH-SIZED PLANET, 2017, arXiv:1709.10328
- ^ K2-137 b: an Earth-sized planet in a 4.3-hour orbit around an M-dwarf, 2017, arXiv:1707.04549
- ^ K2-139 b: a low-mass warm Jupiter on a 29-day orbit transiting an active K0 V star, 2017, arXiv:1702.00691
- ^ K2-140 b - An eccentric 6.57 day transiting hot Jupiter in Virgo, 2017, arXiv:1706.06865
- ^ Adams, Elisabeth R.; et al. (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. arXiv:2011.11698. Bibcode:2021PSJ.....2..152A. doi:10.3847/PSJ/ac0ea0. S2CID 227151802.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host, 2017, arXiv:1706.06723
- ^ McLeod, Kim K.; Rodriguez, Joseph E.; Oelkers, Ryan J.; Collins, Karen A.; Bieryla, Allyson; Fulton, Benjamin J.; Stassun, Keivan G.; Gaudi, B. Scott; Penev, Kaloyan; Stevens, Daniel J.; et al. (1 June 2017). "KELT-18b: Puffy Planet, Hot Host, Probably Perturbed". The Astronomical Journal. 153 (6): 263. arXiv:1702.01657. Bibcode:2017AJ....153..263M. doi:10.3847/1538-3881/aa6d5d. ISSN 0004-6256. S2CID 54667386.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ KELT-19Ab: A P~4.6 Day Hot Jupiter Transiting a Likely Am Star with a Distant Stellar Companion, 2017, arXiv:1709.07010
- ^ Talens, G. J. J; et al. (2018). "MASCARA-2 b: A hot Jupiter transiting a mV = 7.6 A-star". Astronomy & Astrophysics. A57: 612. arXiv:1707.01500. Bibcode:2018A&A...612A..57T. doi:10.1051/0004-6361/201731512. S2CID 119422884.
- ^ Rainer, M.; et al. (2021), "The GAPS programme at TNG", Astronomy & Astrophysics, 649: A29, arXiv:2103.10395, doi:10.1051/0004-6361/202039247, S2CID 232270019
- ^ The Kepler-19 system: a thick-envelope super-Earth with two Neptune-mass companions characterized using Radial Velocities and Transit Timing Variations, 2017, arXiv:1703.06885
- ^ a b Shallue, C. J.; Vanderburg, A. (2017). "Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90" (PDF). The Astrophysical Journal. 155 (2): 94. arXiv:1712.05044. Bibcode:2018AJ....155...94S. doi:10.3847/1538-3881/aa9e09. S2CID 4535051. Retrieved 2017-12-15.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ A Search for Lost Planets in the Kepler Multi-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 f, 2017, arXiv:1703.09229
- ^ Kepler-1649b: An Exo-Venus in the Solar Neighborhood, 2017, arXiv:1704.03136
- ^ a b THE GOLD STANDARD: ACCURATE STELLAR AND PLANETARY PARAMETERS FOR EIGHT Kepler M DWARF SYSTEMS ENABLED BY PARALLAXES, 2017, arXiv:1705.01545
- ^ a b VALIDATION OF SMALL KEPLER TRANSITING PLANET CANDIDATES IN OR NEAR THE HABITABLE ZONE, 2017, arXiv:1711.01267
- ^ 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. arXiv:2005.10318. Bibcode:2020MNRAS.494.5082G. doi:10.1093/mnras/staa1110.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Talens, G. J. J; et al. (2017). "MASCARA-1 b. A hot Jupiter transiting a bright mV = 8.3 A-star in a misaligned orbit". Astronomy & Astrophysics. 606: A73. arXiv:1707.04262. Bibcode:2017A&A...606A..73T. doi:10.1051/0004-6361/201731282. S2CID 119259578.
- ^ A companion on the planet/brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing, 2017, arXiv:1704.01121
- ^ MOA-2012-BLG-505Lb: A super-Earth mass planet probably in the Galactic bulge, 2017, arXiv:1703.10769
- ^ MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Lightcurve Analysis and Keck AO Imaging, 2017, arXiv:1704.01724
- ^ Indication of a massive circumbinary planet orbiting the Low Mass X-ray Binary MXB 1658-298, 2017, arXiv:1703.04433
- ^ Bayliss, Danile; et al. (31 October 2017). "NGTS-1b: A hot Jupiter transiting an M-dwarf". Monthly Notices of the Royal Astronomical Society. 475 (4): 4467–4475. arXiv:1710.11099. Bibcode:2018MNRAS.475.4467B. doi:10.1093/mnras/stx2778. S2CID 39357327.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs, 2017, arXiv:1705.01058
- ^ OGLE-2016-BLG-0263Lb: MICROLENSING DETECTION OF A VERY LOW-MASS BINARY COMPANION THROUGH A REPEATING EVENT CHANNEL, 2017, arXiv:1708.02727
- ^ OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System, 2017, arXiv:1710.00924
- ^ Ryu, Y.-H.; et al. (27 October 2017). "OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary". The Astronomical Journal. 155: 40. arXiv:1710.09974. doi:10.3847/1538-3881/aa9be4. S2CID 54706921.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Shvartzvald, Y; et al. (1 May 2017). "An Earth-mass Planet in a 1 au Orbit around an Ultracool Dwarf". The Astrophysical Journal Letters. 840 (L3): L3. arXiv:1703.08548. Bibcode:2017ApJ...840L...3S. doi:10.3847/2041-8213/aa6d09. hdl:10092/13689.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Starovoit, E. D.; Rodin, A. E. (2017), "On the existence of planets around the pulsar PSR B0329+54", Astronomy Reports, 61 (11): 948–953, arXiv:1710.01153, Bibcode:2017ARep...61..948S, doi:10.1134/S1063772917110063, S2CID 119460916
- ^ PSR J2322−2650 -- A low-luminosity millisecond pulsar with a planetary-mass companion, 2017, arXiv:1712.04445
- ^ Bonfils, Xavier (2017). "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs". Astronomy and Astrophysics. 613: A25. arXiv:1711.06177. Bibcode:2018A&A...613A..25B. doi:10.1051/0004-6361/201731973.
- ^ Search for giant planets in M67 IV: survey results, 2017, arXiv:1703.04296
- ^ A hot Jupiter around the very active weak-line T Tauri star TAP 26, 2017, arXiv:1701.01512
- ^ a b Feng, Fabo; et al. (2017). "Color Difference Makes a Difference: Four Planet Candidates around Tau Ceti". The Astronomical Journal. 154 (4): 135. arXiv:1708.02051. Bibcode:2017AJ....154..135F. doi:10.3847/1538-3881/aa83b4. S2CID 53500995.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b c d 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" (PDF). Nature. 542 (7642): 456–460. arXiv:1703.01424. Bibcode:2017Natur.542..456G. doi:10.1038/nature21360. PMC 5330437. PMID 28230125.
- ^ The GAPS Programme with HARPS-N at TNG XV. A substellar companion around a K giant star identified with quasi-simultaneous HARPS-N and GIANO measurements, 2022, arXiv:1706.06955
- ^ a b c 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, 2017, arXiv:1701.03776
- ^ a b c The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert, 2017, arXiv:1710.06321
- ^ WASP-167b/KELT-13b: Joint discovery of a hot Jupiter transiting a rapidly-rotating F1V star, 2017, arXiv:1704.07771
- ^ a b c The HARPS search for southern extra-solar planets XLII. A system of Earth-mass planets around the nearby M dwarf YZ Ceti, 2017, arXiv:1708.03336