List of exoplanets discovered in 2017

Short description: None

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

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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

1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. https://exoplanet.eu/catalog/.
2. ↑ 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. ↑ 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.
4. ↑ 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. ↑ 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.
6. ↑ 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.
7. ↑ Trifonov, T. et al. (2018), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: A117, doi:10.1051/0004-6361/201731442
8. ↑ Perger, M. et al. (2017), "HADES RV Programme with HARPS-N at TNG", Astronomy & Astrophysics 608: A63, doi:10.1051/0004-6361/201731307
9. ↑ 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
10. ↑ 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. ↑ 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. ↑ 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
13. ↑ 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. ↑ 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. ↑ 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
16. ↑ 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. ↑ 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. ↑ 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. ↑ 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. ↑ 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. ↑ 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
22. ↑ 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
23. ↑ 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
24. ↑ 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
25. ↑ Unger, N. et al. (2021), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics 654: A104, doi:10.1051/0004-6361/202141351
26. ↑ 26.0 26.1 Ferraz, Alvaro; Kochetov, Evgenii (2017), A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315
27. ↑ Reiners, A. et al. (2017), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: L5, doi:10.1051/0004-6361/201732165
28. ↑ 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
29. ↑ 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
30. ↑ 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
31. ↑ 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
32. ↑ "HIP 65426 b - Exoplanet-catalog" (in en). https://exoplanets.nasa.gov/exoplanet-catalog/7220/hip-65426-b/.
33. ↑ 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
34. ↑ 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. ↑ 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
36. ↑ 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
37. ↑ 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. ↑ 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. ↑ 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. ↑ 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
41. ↑ 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
42. ↑ 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. ↑ 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. ↑ 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. ↑ 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
46. ↑ 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
47. ↑ 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
48. ↑ 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
49. ↑ 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
50. ↑ Okoli, Chiamaka (2017), K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours
51. ↑ 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.
52. ↑ 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.
53. ↑ 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
54. ↑ McLeod, Kim K.; Rodriguez, Joseph E.; Oelkers, Ryan J.; Collins, Karen A.; Bieryla, Allyson; Fulton, Benjamin J.; Stassun, Keivan G.; Gaudi, B. Scott et al. (1 June 2017). "KELT-18b: Puffy Planet, Hot Host, Probably Perturbed". The Astronomical Journal 153 (6): 263. doi:10.3847/1538-3881/aa6d5d. ISSN 0004-6256. Bibcode: 2017AJ....153..263M.
55. ↑ 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
56. ↑ Talens, G. J. J et al. (2018). "MASCARA-2 b: A hot Jupiter transiting a mV = 7.6 A-star". Astronomy & Astrophysics A57: 612. doi:10.1051/0004-6361/201731512. Bibcode: 2018A&A...612A..57T.
57. ↑ Rainer, M. et al. (2021), "The GAPS programme at TNG", Astronomy & Astrophysics 649: A29, doi:10.1051/0004-6361/202039247
58. ↑ 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.
59. ↑ 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
60. ↑ 60.0 60.1 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". The Astrophysical Journal 155 (2): 94. doi:10.3847/1538-3881/aa9e09. Bibcode: 2018AJ....155...94S. https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf. Retrieved 2017-12-15.
61. ↑ 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
62. ↑ 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
63. ↑ 63.0 63.1 Mann, Andrew W.; Dupuy, Trent; Muirhead, Philip S.; Johnson, Marshall C.; Liu, Michael C.; Ansdell, Megan; Dalba, Paul A.; Swift, Jonathan J. et al. (2017), "The Gold Standard: Accurate Stellar and Planetary Parameters for EightKeplerM Dwarf Systems Enabled by Parallaxes", The Astronomical Journal 153 (6): 267, doi:10.3847/1538-3881/aa7140
64. ↑ 64.0 64.1 Torres, Guillermo; Kane, Stephen R.; Rowe, Jason F.; Batalha, Natalie M.; Henze, Christopher E.; Ciardi, David R.; Barclay, Thomas; Borucki, William J. et al. (2017), "Validation of SmallKepler Transiting Planet Candidates in or near the Habitable Zone", The Astronomical Journal 154 (6): 264, doi:10.3847/1538-3881/aa984b
65. ↑ 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.
66. ↑ 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. doi:10.1051/0004-6361/201731282. Bibcode: 2017A&A...606A..73T.
67. ↑ Bennett, D. P. et al. (2017), "The First Planetary Microlensing Event with Two Microlensed Source Stars", The Astronomical Journal 155 (3): 141, doi:10.3847/1538-3881/aaadfa
68. ↑ 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
69. ↑ Nagakane, M.; Sumi, T.; Koshimoto, N.; Bennett, D. P.; Bond, I. A.; Rattenbury, N.; Suzuki, D.; Abe, F. et al. (2017), "MOA-2012-BLG-505Lb: A Super-Earth-mass Planet That Probably Resides in the Galactic Bulge", The Astronomical Journal 154: 35, doi:10.3847/1538-3881/aa74b2
70. ↑ Koshimoto, N. et al. (2017), "MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Light-curve Analysis and Keck AO Imaging", The Astronomical Journal 154: 3, doi:10.3847/1538-3881/aa72e0
71. ↑ 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
72. ↑ Bayliss, Danile (31 October 2017). "NGTS-1b: A hot Jupiter transiting an M-dwarf". Monthly Notices of the Royal Astronomical Society 475 (4): 4467–4475. doi:10.1093/mnras/stx2778. Bibcode: 2018MNRAS.475.4467B.
73. ↑ 73.0 73.1 Mróz, Przemek et al. (2017), "OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs", The Astronomical Journal 154 (5): 205, doi:10.3847/1538-3881/aa8f98
74. ↑ Hirao, Y. et al. (2017), "OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf", The Astronomical Journal 154: 1, doi:10.3847/1538-3881/aa73da
75. ↑ 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
76. ↑ Han, C. et al. (2017), "OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System", The Astronomical Journal 154 (6): 223, doi:10.3847/1538-3881/aa9179
77. ↑ Ryu, Y.-H. (27 October 2017). "OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary". The Astronomical Journal 155: 40. doi:10.3847/1538-3881/aa9be4.
78. ↑ Shvartzvald, Y (1 May 2017). "An Earth-mass Planet in a 1 au Orbit around an Ultracool Dwarf". The Astrophysical Journal Letters 840 (L3): L3. doi:10.3847/2041-8213/aa6d09. Bibcode: 2017ApJ...840L...3S.
79. ↑ Vandorou, Aikaterini; Dang, Lisa; Bennett, David P.; Koshimoto, Naoki; Terry, Sean K.; Beaulieu, Jean-Phillipe; Alard, Christophe; Bhattacharya, Aparna et al. (2023), OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-Dwarf Confirmed by Keck AO
80. ↑ Hwang, K.-H. et al. (2017), "OGLE-2017-BLG-0173Lb: Low-mass-ratio Planet in a "Hollywood" Microlensing Event", The Astronomical Journal 155: 20, doi:10.3847/1538-3881/aa992f
81. ↑ Starovoit, E. D.; Rodin, A. E. (2017). "On the existence of planets around the pulsar PSR B0329+54". Astronomy Reports 61 (11): 948–953. doi:10.1134/S1063772917110063. Bibcode: 2017ARep...61..948S.
82. ↑ Spiewak, R.; Bailes, M.; Barr, E. D.; Bhat, N D R.; Burgay, M.; Cameron, A. D.; Champion, D. J.; Flynn, C M L. et al. (2017), "PSR J2322−2650 – a low-luminosity millisecond pulsar with a planetary-mass companion", Monthly Notices of the Royal Astronomical Society 475: 469–477, doi:10.1093/mnras/stx3157
83. ↑ 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
84. ↑ Bonfils, Xavier (2017). "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs". Astronomy and Astrophysics 613: A25. doi:10.1051/0004-6361/201731973. Bibcode: 2018A&A...613A..25B.
85. ↑ 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
86. ↑ 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. ↑ 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. ↑ 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.
89. ↑ 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. ↑ 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. ↑ 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
92. ↑ 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. ↑ 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

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Exoplanetology

* Planet
* Definition
* IAU
* Planetary science

Main topics|

* Exoplanet
* Methods of detecting exoplanets
* Planetary system

Sizes
and types|

| Terrestrial|

* Carbon planet
* Coreless planet
* Desert planet
* Dwarf planet
* Ice planet
* Iron planet
* Lava planet
* Mega-Earth
* Ocean planet
* Sub-Earth
* Super-Earth

|

Gaseous|

* Eccentric Jupiter
* Gas dwarf
* Helium planet
* Hot Jupiter
* Hot Neptune
* Ice giant
* Mini-Neptune
* Super-Neptune
* Super-Jupiter

Other types|

* Brown dwarf
* Chthonian planet
* Circumbinary planet
* Disrupted planet
* Double planet
* Eyeball planet
* Mesoplanet
* Planemo
* Planet/Brown dwarf boundary
* Planetesimal
* Protoplanet
* Pulsar planet
* Sub-brown dwarf
* Ultra-cool dwarf
* Ultra-short period planets (USP)

Formation
and evolution|

* Accretion
* Accretion disk
* Asteroid belt
* Circumplanetary disk
* Circumstellar disc
* Circumstellar envelope
* Cosmic dust
* Debris disk
* Detached object
* Disrupted planet
* Excretion disk
* Exoplanetary Circumstellar Environments and Disk Explorer
* Exozodiacal dust
* Extraterrestrial materials
* Extraterrestrial sample curation
* Giant-impact hypothesis
* Gravitational collapse
* Hills cloud
* Interplanetary dust cloud
* Interplanetary medium
* Interplanetary space
* Interstellar cloud
* Interstellar dust
* Interstellar medium
* Interstellar space
* Kuiper belt
* List of interstellar and circumstellar molecules
* Merging stars
* Molecular cloud
* Nebular hypothesis
* Oort cloud
* Outer space
* Planetary migration
* Planetary system
* Planetesimal
* Planet formation
* Protoplanetary disk
* Ring system
* Rubble pile
* Sample-return mission
* Scattered disc
* Star formation

Systems|

* Exocomet
* Exomoon
* Interstellar comet
* Mean-motion resonances
* Retrograde planet
* Rogue planet
* Tidally detached exomoon
* Titius–Bode laws
* Trojan planet

Host stars|

* A
* B
* Binary star
* Brown dwarfs
* Extragalactic planet
* F/Yellow-white dwarfs
* G/Yellow dwarfs
* Herbig Ae/Be
* K/Orange dwarfs
* M/Red dwarfs
* Planets in globular clusters
* Pulsar
* Red giant
* Subdwarf B
* Subgiant
* T Tauri
* White dwarfs
* Yellow giants

Detection|

* Astrometry
* Direct imaging
* list
* Microlensing
* list
* Polarimetry
* Pulsar timing
* list
* Radial velocity
* list
* Transit method
* list
* Transit-timing variation

Habitability|

* Astrobiology
* Circumstellar habitable zone
* Earth analog
* Extraterrestrial liquid water
* Habitability of natural satellites
* Superhabitable planet

Catalogues|

* Catalog of Nearby Habitable Systems
* Exoplanet Data Explorer
* Extrasolar Planets Encyclopaedia
* NASA Exoplanet Archive
* NASA Star and Exoplanet Database

Lists|

* Exoplanetary systems
* Host stars
* Multiplanetary systems
* Stars with proplyds
* Exoplanets
* Lists of exoplanets
* Discoveries
* Extremes
* Firsts
* Nearest
* Largest
* Most massive
* Terrestrial candidates
* Kepler
* Potentially habitable
* Discovered exoplanets by year
* before 2000
* 2000–2009
* 2010
* 2011
* 2012
* 2013
* 2014
* 2015
* 2016
* 2017
* 2018
* 2019

Other|

* Carl Sagan Institute
* Exoplanet phase curves
* Nexus for Exoplanet System Science
* Planets in science fiction
* Sudarsky's gas giant classification

* Discoveries of exoplanets
* Search projects

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