List of exoplanets discovered in 2013

Short description: None

This is a List of exoplanets discovered in 2013.

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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2MASS J01225093-2439505 b  | 24.5  |  |  | 52  |  | imaging  | 120  | 0.4  | 3530  | [2]
BD+15 2940 b  | 1.11  |  | 137.48  | 0.539  |  | radial vel.  | 572.2  | 1.1  | 4796  | [3]
CoRoT-25b | 0.27  | 1.08  | 4.86069  | 0.0578  |  | transit  | 3300  | 1.09  | 6040  | [4]
CoRoT-26b | 0.52  | 1.26  | 4.20474  | 0.0526  |  | transit  | 5400  | 1.09  | 5590  | [4]
DENIS-P J082303.1-491201 b | 28.5  |  | 246.36  | 0.36  |  | astrometry  | 67.7  | 0.07  | 2150  | [5]
Gliese 163 b | 0.03335  |  | 8.63182  | 0.0607  |  | radial vel.  | 48.8  | 0.4  | 3500  | [6]
Gliese 163 c | 0.0214  |  | 25.63058  | 0.1254  |  | radial vel.  | 48.8  | 0.4  | 3500  | [6]
Gliese 163 d | 0.0925  |  | 603.95116  | 1.0304  |  | radial vel.  | 48.8  | 0.4  | 3500  | [6]
Gliese 221b  | 0.027  |  | 3.8728  | 0.0428  |  | radial vel.  | 66  | 0.7  | 4324  | [7][8]Disputed[9]
Gliese 221 c | 0.17  |  | 125.94  | 0.435  |  | radial vel.  | 66  | 0.7  | 4324  | [7][8]
Gliese 328b | 2.3  |  | 4100  | 4.5  |  | radial vel.  | 65.3  | 0.69  | 3900  | [10]
Gliese 504 b | 4  |  |  | 43.5  |  | imaging  | 58.5  | 1.22  | 6234  | [11]
HAT-P-44b  | 0.352  | 1.242  | 4.301219  | 0.0507  |  | transit  | 1180  | 0.94  | 5295  | [12]
HAT-P-44c  | 4  |  | 872.2  | 1.752  |  | radial vel.  | 1180  | 0.94  | 5295  | Period is ambiguous[12]
HAT-P-45b  | 0.892  | 1.426  | 3.128992  | 0.0452  |  | transit  | 990  | 1.26  | 6330  | [12]
HAT-P-46b  | 0.493  | 1.284  | 4.463129  | 0.0577  |  | transit  | 970  | 1.28  | 6120  | [12]
HATS-2b  | 1.345  | 1.168  | 1.354133  | 0.023  |  | transit  | 1200  | 0.88  | 5227  | [13]
HATS-3b | 1.071  | 1.381  | 3.547851  | 0.0485  | 1648  | transit  | 1480  | 1.21  | 6351  | [14]
HD 2952 b (ru)  | 1.6  |  | 311.6  | 1.2  |  | radial vel.  | 375.8  | 2.54  | 4844  | [15]
HD 13908 b (fr)  | 0.865  |  | 19.382  | 0.154  |  | radial vel.  | 218.2  | 1.29  | 6255  | [16]
HD 13908 c (fr)  | 5.13  |  | 931  | 2.03  |  | radial vel.  | 218.2  | 1.29  | 6255  | [16]
HD 65216c | 0.17  |  | 152.6  | 0.54  |  | radial vel.  | 116.1  | 0.92  | 5666  | [17]False positive, another planet with same assigned name discovered in 2019.[18]
HD 95086 b | 5  |  |  | 55.7  |  | imaging  | 298.7  | 1.6  |  | [19]
HD 103774 b | 0.367  |  | 5.8881  | 0.07  |  | radial vel.  | 173.1  | 1.33  | 6489  | [7]
HD 106906 b | 11  |  |  | 650  |  | imaging  | 299.5  | 1.5  | 6516  | [20]
HD 109271 b | 0.054  |  | 7.8543  | 0.079  |  | radial vel.  | 185.6  | 1.05  | 5783  | [7]
HD 109271 c | 0.076  |  | 30.93  | 0.196  |  | radial vel.  | 185.6  | 1.05  | 5783  | [7]
HD 113337 b | 2.83  |  | 324  | 0.92  |  | radial vel.  | 122.0  | 1.4  | 6576.6  | [21]
HD 120084 b | 4.5  |  | 2082  | 4.3  |  | radial vel.  | 318.5  | 2.39  | 4892  | [15]
HD 159243 b  | 1.13  |  | 12.62  | 0.11  |  | radial vel.  | 223.7  | 1.12  | 6123  | [16]
HD 159243 c (fr)  | 1.9  |  | 248.4  | 0.8  |  | radial vel.  | 223.7  | 1.12  | 6123  | [16]
HD 233604 b  | 6.575  |  | 192  | 0.747  |  | radial vel.  | 2830±90  | 1.5  | 4791  | [3]
HD 285507 b  | 0.92±0.03  |  | 6.0962±0.0002  |  |  | radial vel.  | 153  | 0.73±0.03  | 4503+85−61 | member of Hyades (star cluster)[22][23]
HD 112410 b | 9.18  |  | 124.6  | 0.565  |  | radial vel.  | 486.8  | 1.54  | 4830  | [24]
HIP 91258 b (fr)  | 1.068  |  | 5.0505  | 0.057  |  | radial vel.  | 145.0  | 0.95  | 5519  | [16]
KELT-3b | 1.477  | 1.345  | 2.7033904  | 0.04122  |  | transit  | 580  | 1.28  | 6306  | [25]
KELT-6b | 0.442  | 1.18  | 7.8455821  | 0.08  |  | transit  | 720  | 1.13  | 6272  | [26]
Kepler-37b | 0.03146  | 0.029  | 13.3675  |  |  | transit  | 220  | 0.8  | 5417  | [27]
Kepler-37c | 0.03776  | 0.067  | 21.302  |  |  | transit  | 220  | 0.8  | 5417  | [27]
Kepler-37d | 0.03839  | 0.173  | 39.7922  |  |  | transit  | 220  | 0.8  | 5417  | [27]
Kepler-61b |  | 0.192  | 59.87756  |  |  | transit  | 1103±16  | 0.64  | 4017  | [28]
Kepler-62b | 0.03  | 0.117  | 5.714932  | 0.0553  |  | transit  | 1200  | 0.69  | 4925  | [29]
Kepler-62c | 0.013  | 0.048  | 12.4417  | 0.0929  |  | transit  | 1200  | 0.69  | 4925  | [29]
Kepler-62d | 0.044  | 0.174  | 18.16406  | 0.12  |  | transit  | 1200  | 0.69  | 4925  | [29]
Kepler-62e | 0.113  | 0.144  | 122.3874  | 0.427  |  | transit  | 1200  | 0.69  | 4925  | Potentially habitable exoplanet[29]
Kepler-62f | 0.11  | 0.126  | 267.291  | 0.718  |  | transit  | 1200  | 0.69  | 4925  | Potentially habitable exoplanet[29]
Kepler-63b | 0.378  | 0.545  | 9.4341505  | 0.08  |  | transit  | 650  | 0.98  | 5576  | [30]
Kepler-65b |  | 0.127  | 2.15491  | 0.035  |  | transit  | 999±8  | 1.25  | 6211  | [31]
Kepler-65c |  | 0.23  | 5.859944  | 0.068  |  | transit  | 999±8  | 1.25  | 6211  | [31]
Kepler-65d |  | 0.136  | 8.13123  | 0.084  |  | transit  | 999±8  | 1.25  | 6211  | [31]
Kepler-66b |  | 0.25  | 17.815815  | 0.1352  |  | transit  | 3610  | 1.04  | 5962  | Belongs to open cluster NGC 6811[32]
Kepler-67b |  | 0.262  | 15.7259  | 0.1171  |  | transit  | 3610  | 0.86  | 5331  | Belongs to open cluster NGC 6811[32]
Kepler-68b | 0.01878  | 0.208  | 5.39875  |  | 1280  | transit  | 440  | 1.08  | 5793  | [33]
Kepler-68c | 0.02265  | 0.089  | 9.60504  |  |  | transit  | 440  | 1.08  | 5793  | [33]
Kepler-68d | 0.84007  |  | 625  |  |  | radial vel.  | 440  | 1.08  | 5793  | [33]
Kepler-69b |  | 0.2  | 13.722341  | 0.094  |  | transit  | 2430±30  | 0.81  | 5638  | [34]
Kepler-69c |  | 0.153  | 242.4613  | 0.64  |  | transit  | 2430±30  | 0.81  | 5638  | [34][35]
Kepler-74b (es)  | 0.63  | 0.96  | 7.340711  | 0.0781  |  | transit  | 4300  | 1.18  | 6000  | [36]
Kepler-75b (es)  | 10.1  | 1.05  | 8.8849116  | 0.0818  |  | transit  | 3700  | 0.91  | 5200  | [36]
Kepler-76b | 2.01  | 1.36  | 1.5449298  | 0.0274  |  | orbital brightness modulation  | 2750±30  | 1.2  | 6409  | [37]
Kepler-77b (es)  | 0.43  | 0.96  | 3.57878087  | 0.04501  |  | transit  | 1900  | 0.95  | 5520  | [38]
Kepler-78b | 0.006  | 0.105  | 0.355  |  | 2330  | transit  | 407.1±1.1  | 0.76  | 5058  | [39]
Kepler-87b | 1.02  | 1.204  | 114.73635  | 0.481  | 478  | transit  | 4170±90  | 1.1  | 5600  | Two more unconfirmed planets in the system[40]
Kepler-87c | 0.02  | 0.548  | 191.2318  | 0.676  | 403  | transit  | 4170±90  | 1.1  | 5600  | Two more unconfirmed planets in the system[40]
Kepler-88b | 0.027  | 0.337  | 10.95416  |  |  | transit  | 1110  | 0.96  | 5471  | [41]
Kepler-88c | 0.626  |  | 22.3395  | 0.15525  |  | timing  | 1110  | 0.96  | 5471  | [41][42]
Kepler-89b | 0.033  | 0.153  | 3.743208  | 0.05119  |  | transit  | 1577±16  | 1.28  | 6182  | [43]
Kepler-89c | 0.049  | 0.385  | 10.423648  | 0.1013  |  | transit  | 1577±16  | 1.28  | 6182  | [43]
Kepler-89d | 0.334  | 1.005  | 22.342989  | 0.1684  |  | transit  | 1577±16  | 1.28  | 6182  | [43]
Kepler-89e | 0.11  | 0.585  | 54.32031  | 0.3046  |  | transit  | 1577±16  | 1.28  | 6182  | [43]
Kepler-90b  |  | 0.117  | 7.008151  | 0.074  | 1056  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90c  |  | 0.106  | 8.719375  | 0.089  | 981  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90d  |  | 0.256  | 59.73667  | 0.32  | 518  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90e |  | 0.237  | 91.93913  | 0.42  | 448  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90f |  | 0.257  | 124.9144  | 0.48  | 592  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90g |  | 0.723  | 210.60697  | 0.71  | 340  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-90h |  | 1.008  | 331.60059  | 1.01  | 292  | transit  | 2500  | 1.2  | 6080  | [44]
Kepler-91b | 0.81  | 1.367  | 6.24658  | 0.0731  |  | transit  | 3400  | 1.31  | 4550  | [45]
Kepler-92b  | 0.202  | 0.313  | 13.749  |  |  | transit  | 1580±17  | 1.21  | 5883  | [46]
Kepler-92c  | 0.019  | 0.232  | 26.723  |  |  | transit  | 1580±17  | 1.21  | 5883  | [46]
Kepler-102e | 0.028  | 0.198  | 16.1457  |  | 579  | transit  | 352.7±0.7  | 0.81  | 4909  | [47]
Kepler-105b  |  | 0.429  | 5.4122  | 0.066  |  | transit  | 1517±18  | 0.96  | 5827  | [47]
Kepler-114c  | 0.009  | 0.143  | 8.041  |  | 623  | transit  | 852±4  | 0.56  | 4605  | [46]
Kepler-114d  | 0.012  | 0.226  | 11.776  |  | 549  | transit  | 852±4  | 0.56  | 4605  | [46]
Kepler-128b  | 0.097  | 0.101  | 15.09  |  |  | transit  | 1307±12  | 1.18  | 6090  | [46]
Kepler-128c  | 0.105  | 0.101  | 22.804  |  |  | transit  | 1307±12  | 1.18  | 6090  | [46]
Kepler-130b  |  | 0.091  | 8.457458  | 0.079  |  | transit  | 1042±7  | 1  | 5884  | [47]
Kepler-145b  | 0.117  | 0.236  | 22.951  |  |  | transit  | 1880±30  | 1.32  | 6022  | [46]
Kepler-145c  | 0.25  | 0.385  | 42.882  |  |  | transit  | 1880±30  | 1.32  | 6022  | [46]
Kepler-177b  | 0.006  | 0.259  | 36.855  |  |  | transit  | 4880±140  | 1.07  | 5942  | [46]
Kepler-177c  | 0.024  | 0.633  | 49.412  |  |  | transit  | 4880±140  | 1.07  | 5942  | [46]
Kepler-238e  | 0.534  | 0.5  | 23.654  |  |  | transit  | 6200±300  | 1.06  | 5751  | [46]
Kepler-238f  | 0.042  | 0.178  | 50.447  |  |  | transit  | 6200±300  | 1.06  | 5751  | [46]
Kepler-276c  | 0.052  | 0.259  | 31.884  |  |  | transit  | 3850±150  | 1.1  | 6105  | [46]
Kepler-276d  | 0.051  | 0.25  | 48.648  |  |  | transit  | 3850±150  | 1.1  | 6105  | [46]
Kepler-277b | 0.275  | 0.261  | 17.324  |  |  | transit  | 3280±50  | 1.12  | 5946  | [46]
Kepler-277c | 0.202  | 0.3  | 33.006  |  |  | transit  | 3280±50  | 1.12  | 5946  | [46]
Kepler-279b  |  | 0.323  | 12.309681  | 0.112  |  | transit  | 3480±70  | 1.1  | 6363  | KOI-1236.01[48]
Kepler-279c  | 0.155  | 0.384  | 35.736  |  |  | transit  | 3490±70  | 1.1  | 6363  | KOI-1236.02[48][46]
Kepler-279d  | 0.118  | 0.277  | 54.414  |  |  | transit  | 3490±70  | 1.1  | 6363  | [46]
Kepler-282d  | 0.192  | 0.219  | 24.806  |  |  | transit  | 4540±150  | 0.97  | 5602  | [46]
Kepler-282e  | 0.177  | 0.277  | 44.347  |  |  | transit  | 4540±150  | 0.97  | 5602  | [46]
Kepler-305b  | 0.033  | 0.321  | 5.487  |  |  | transit  | 2900±90  | 0.76  | 5100  | [46]KOI-1563.01[48]
Kepler-305c  | 0.019  | 0.294  | 8.291  |  |  | transit  | 2900±90  | 0.76  | 5100  | [46]KOI-1563.02[48]
Kepler-307b  | 0.02341  | 0.217  | 10.4208  |  |  | transit  | 1908±17  | 0.91  | 5367  | [46]
Kepler-307c  | 0.01145  | 0.196  | 13.0729  |  |  | transit  | 1908±17  | 0.91  | 5367  | [46]
Kepler-328b  | 0.09  | 0.205  | 34.921  |  |  | transit  | 7700±500  | 1.15  | 5914  | [46]
Kepler-328c  | 0.124  | 0.482  | 71.312  |  |  | transit  | 7700±500  | 1.15  | 5914  | [46]
Kepler-350c  | 0.019  | 0.277  | 17.849  |  |  | transit  | 3210±70  | 1  | 6186  | [46]
Kepler-350d  | 0.047  | 0.25  | 26.136  |  |  | transit  | 3210±70  | 1  | 6186  | [46]
Kepler-396b  | 0.238  | 0.312  | 42.994  |  |  | transit  | 734±5  | 0.85  | 5384  | [46]KOI-2672.01[48]
Kepler-396c  | 0.056  | 0.473  | 88.505  |  |  | transit  | 734±5  | 0.85  | 5384  | [46]KOI-2672.02[48]
Kepler-410Ab |  | 0.253  | 17.833648  | 0.1226  |  | transit  | 430  | 1.21  | 6273  | [49]
Kepler-411b |  | 0.168  | 3.00516  | 0.038  | 1040  | transit  | 503.5±1.5  | 0.83  | 4974  | [47]
Kepler-1359c  |  | 0.3711+0.12−0.06 | 505.46+0.05−0.04 | 1.143±0.018  |  | transit  | 2182+81−82 | 0.78+0.03−0.04 | 4709+46−56 | [44]Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.[50]
MOA-2008-BLG-379Lb  | 4.1  |  |  | 3.3  |  | microlensing  | 11000  | 0.56  |  | [51]
MOA-2010-BLG-328Lb  | 0.02895  |  |  | 0.92  |  | microlensing  | 2600  | 0.11  |  | [52]
MOA-2011-BLG-262Lb | 0.056634  | 0.383  |  | 1  |  | microlensing  | 22830  | 0.1  | 3300  | Host star may be a rogue planet, planet may be an exomoon[53]
MOA-2011-BLG-262L | 4  |  |  | N/A |  | microlensing  | 22830  |  | 3300  | Host star may be a rogue planet, planet may be an exomoon[53]
MOA-2011-BLG-293Lb  | 4.8  |  |  | 1.1  |  | microlensing  | 25200  | 0.86  |  | [54]
MOA-2011-BLG-322Lb  | 11.6  |  |  | 4.3  |  | microlensing  | 24700  | 0.39  |  | [55]
OGLE-2011-BLG-0251Lb  | 0.53  |  |  | 2.72  |  | microlensing  | 8400  | 0.26  |  | [56]
OGLE-2012-BLG-358Lb  | 1.85  |  |  | 0.87  |  | microlensing  | 5700  | 0.02  |  | Orbiting a brown dwarf[57]
OGLE-2012-BLG-406Lb  | 2.73  |  |  | 3.45  |  | microlensing  | 16200  | 0.44  |  | [58]
Omega Serpentis b | 1.7  |  | 277.02  | 1.1  |  | radial vel.  | 263.0  | 2.17  | 4770  | [15]
PH2b |  | 0.903  | 282.5255  | 0.828  | 281  | transit  | 1130±10  | 0.94  | 5629  | [59]Also called Kepler-86b
POTS-1b  | 2.31  | 0.941  | 3.1606296  | 0.03734  |  | transit  | 3900  | 0.69  | 4400  | [60]
PSO J318.5−22 | 6.5  | 1.53  | N/A | N/A | 1160  | imaging  | 80  | N/A | N/A | Rogue planet[61]
ROXs 12b | 16  |  |  | 210  |  | imaging  | 390  | 0.87  | 3850  | [62]
ROXs 42Bb | 9  |  |  | 157  |  | imaging  | 440  | 1  |  | [62]
WASP-8c | 9.45  |  | 4323  | 5.28  |  | radial vel.  | 280  | 1.03  | 5600  | [63]
WASP-65b  | 1.55  | 1.112  | 2.3114243  | 0.0334  |  | transit  | 1000  | 0.93  | 5600  | [64]
WASP-68b  | 0.95  | 1.24  | 5.084298  | 0.06206  |  | transit  | 962±8  | 1.24  | 5911  | [65]
WASP-69b | 0.26  | 1.057  | 3.8681382  | 0.04525  | 963  | transit  | 160  | 0.83  | 4715  | [66]
WASP-70Ab  | 0.59  | 1.164  | 3.7130203  | 0.04853  | 1387  | transit  | 800  | 1.11  | 5763  | [66]
WASP-73b  | 1.88  | 1.16  | 4.08722  | 0.05512  | 1790  | transit  | 1042±9  | 1.34  | 6036  | [65]
WASP-75b | 1.07  | 1.27  | 2.484193  | 0.0375  |  | transit  | 850  | 1.14  | 6100  | [64][67]
WASP-76b | 0.92  | 1.83  | 1.809886  | 0.033  | 2190  | transit  | 390  | 1.46  | 6250  | [68]
WASP-80b | 0.538  | 0.999  | 3.06785234  | 0.0344  |  | transit  | 200  | 0.58  | 4143  | [69]Proper name Wadirum
WASP-82#Planetary system (fr)  | 1.24  | 1.67  | 2.705782  | 0.0447  | 2190  | transit  | 650  | 1.63  | 6490  | [68]
WASP-84b | 0.694  | 0.942  | 8.5234865  | 0.0771  | 797  | transit  | 410  | 0.84  | 5314  | [66]
WASP-88b | 0.56  | 1.7  | 4.954  | 0.06431  | 1775  | transit  | 1730±30  | 1.45  | 6431  | [65]
WASP-90b | 0.63±0.07  | 1.63±0.09  | 3.916243±0.000003  | 0.0562±0.0012  | 1840±50  | transit  | 1100±200  | 1.55±0.10  | 6440±130  | [68]
WASP-95b | 1.13+0.1−0.04 | 1.21±0.06  | 2.184673±0.0000014  | 0.03416±0.00083  | 1570±50  | transit  | 450±2  | 1.11±0.09  | 5630±130  | [70]
WASP-96b | 0.48±0.03  | 1.2±0.06  | 3.4252602±0.0000027  | 0.0453±0.0013  | 1285±40  | transit  | 1161±15  | 1.06±0.09  | 5540±140  | [70]
WASP-97b  | 1.32±0.05  | 1.13±0.06  | 2.07276±0.000001  | 0.03303±0.00056  | 1555±40  | transit  | 494.9±1.7  | 1.12±0.06  | 5640±100  | [70]
WASP-98b  | 0.83±0.07  | 1.10±0.04  | 2.96264036±0.0000013  | 0.03762±0.001  | 1180±30  | transit  | 926±5  | 0.69±0.06  | 5525±130  | [70]
WASP-99b  | 2.78±0.13  | 1.10+0.08−0.05 | 5.75251±0.00004  | 0.0717±0.0016  | 1480±40  | transit  | 519±2  | 1.48±0.10  | 6180±100  | [70]
WASP-100b  | 2.03±0.12  | 1.69±0.29  | 2.849375±0.000008  | 0.0457±0.0010  | 2190±140  | transit  | 1201±9  | 1.57±0.10  | 6900±120  | [70]
WASP-101b  | 0.50±0.04  | 1.41±0.05  | 3.585722±0.000004  | 0.0506±0.0009  | 1560±35  | transit  | 660±3  | 1.34±0.07  | 6400±110  | [70]
WTS-2b  | 1.12  | 1.363  | 1.0187068  | 0.01855  | 2000  | transit  | 3300  | 0.82  | 5000  | [71][72]

## Specific exoplanet lists

## References

1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/.
2. ↑ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
3. ↑ 3.0 3.1 BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
4. ↑ 4.0 4.1 Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
5. ↑ Sahlmann, J.; Lazorenko, P. F.; Ségransan, D.; Martín, Eduardo L.; Queloz, D.; Mayor, M.; Udry, S. (2013), "Astrometric orbit of a low-mass companion to an ultracool dwarf", Astronomy & Astrophysics 556: A133, doi:10.1051/0004-6361/201321871, Bibcode: 2013A&A...556A.133S
6. ↑ 6.0 6.1 6.2 Tuomi, M.; Anglada-Escudé, G. (2013). "Up to four planets around the M dwarf GJ 163". Astronomy & Astrophysics 556: A111. doi:10.1051/0004-6361/201321174.
7. ↑ 7.0 7.1 7.2 7.3 7.4 Lo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D. et al. (2013). "The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone". Astronomy & Astrophysics 551: 7. doi:10.1051/0004-6361/201220415. A59. Bibcode: 2013A&A...551A..59L.
8. ↑ 8.0 8.1 Arriagada, Pamela; Anglada-Escudé, Guillem; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian; Wende, Sebastian; Minniti, Dante (2013), "Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range", The Astrophysical Journal 771 (1): 42, doi:10.1088/0004-637X/771/1/42, Bibcode: 2013ApJ...771...42A
9. ↑ Simpson, Emilie R.; Fetherolf, Tara; Kane, Stephen R.; Li, Zhexing; Pepper, Joshua; Močnik, Teo (2022), "Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity", The Astronomical Journal 163 (5): 215, doi:10.3847/1538-3881/ac5d41, Bibcode: 2022AJ....163..215S
10. ↑ Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Boss, Alan P. (2013), "Secretly Eccentric: The Giant Planet and Activity Cycle of GJ 328", The Astrophysical Journal 774 (2): 147, doi:10.1088/0004-637X/774/2/147, Bibcode: 2013ApJ...774..147R
11. ↑ Kuzuhara, M.; Tamura, M.; Kudo, T.; Janson, M.; Kandori, R.; Brandt, T. D.; Thalmann, C.; Spiegel, D. et al. (2013). "Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504". The Astrophysical Journal 774 (11): 11. doi:10.1088/0004-637X/774/1/11. Bibcode: 2013ApJ...774...11K.
12. ↑ 12.0 12.1 12.2 12.3 Hartman, J. D.; Bakos, G. Á.; Torres, G.; Kovács, G.; Johnson, J. A.; Howard, A. W.; Marcy, G. W.; Latham, D. W. et al. (2013), "HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS", The Astronomical Journal 147 (6): 128, doi:10.1088/0004-6256/147/6/128
13. ↑ Mohler-Fischer, M.; Mancini, L.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Bayliss, D.; Jordán, A.; Csubry, Z. et al. (2013), "HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity", Astronomy & Astrophysics 558: A55, doi:10.1051/0004-6361/201321663, Bibcode: 2013A&A...558A..55M
14. ↑ Bayliss, D.; Zhou, G.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler-Fischer, M. et al. (2013), "HATS-3b: An inflated hot Jupiter transiting an F-type star", The Astronomical Journal 146 (5): 113, doi:10.1088/0004-6256/146/5/113, Bibcode: 2013AJ....146..113B
15. ↑ 15.0 15.1 15.2 Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi et al. (2013), "Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, andωSerpentis", Publications of the Astronomical Society of Japan 65 (4): 85, doi:10.1093/pasj/65.4.85
16. ↑ 16.0 16.1 16.2 16.3 16.4 Moutou, Claire; Hébrard, Guillaume; Bouchy, François; Arnold, Luc; Santos, Nuno C.; Astudillo-Defru, Nicola; Boisse, Isabelle; Bonfils, Xavier et al. (2013), The SOPHIE search for northern extrasolar planets VI. Three new hot Jupiters in multi-planet extrasolar systems, doi:10.1051/0004-6361/201322067
17. ↑ Wittenmyer, Robert A.; Wang, Songhu; Horner, Jonathan; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; O'Toole, S. J.; Bailey, J. et al. (2013), "Forever Alone? Testing Single Eccentric Planetary Systems for Multiple Companions", The Astrophysical Journal Supplement Series 208 (1): 2, doi:10.1088/0067-0049/208/1/2, Bibcode: 2013ApJS..208....2W
18. ↑ Wittenmyer, Robert A. et al. (2019). "Truly eccentric – I. Revisiting eight single-eccentric planetary systems". Monthly Notices of the Royal Astronomical Society 484 (4): 5859–5867. doi:10.1093/mnras/stz290. Bibcode: 2019MNRAS.484.5859W.
19. ↑ Rameau, J., Chauvin, G., Lagrange, A.-M., Boccaletti, A., Quanz, S. P., Currie, T., Mawet, D., Girard, J. H., Bonnefoy, M., Kenworthy, M. (2013). "Confirmation of the planet around HD 95086 by direct imaging". The Astrophysical Journal 779 (2): L26. doi:10.1088/2041-8205/779/2/L26. Bibcode: 2013ApJ...779L..26R.
20. ↑ Bailey, Vanessa et al. (January 2014). "HD 106906 b: A planetary-mass companion outside a massive debris disk". The Astrophysical Journal Letters 780 (1): L4. doi:10.1088/2041-8205/780/1/L4. Bibcode: 2014ApJ...780L...4B.
21. ↑ Borgniet, Simon; Boisse, Isabelle; Lagrange, Anne-Marie; Bouchy, François; Arnold, Luc; Díaz, Rodrigo F.; Galland, Franck; Delorme, Philippe et al. (2013), "Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337", Astronomy & Astrophysics 561: A65, doi:10.1051/0004-6361/201321783
22. ↑ Carleo, I. (2020). "The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: Confirmation of HD 285507 b and refutation of AD Leo B". Astronomy & Astrophysics A5: 638. doi:10.1051/0004-6361/201937369. Bibcode: 2020A&A...638A...5C.
23. ↑ Open exoplanet catalogue HD 285507
24. ↑ Jones, M. I. et al. (2013). "Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242". Astronomy & Astrophysics 556 (A78): 5. doi:10.1051/0004-6361/201321660. Bibcode: 2013A&A...556A..78J.
25. ↑ Pepper, Joshua; Siverd, Robert J.; Beatty, Thomas G.; Gaudi, B. Scott; Stassun, Keivan G.; Eastman, Jason; Collins, Karen; Latham, David W. et al. (2013-08-01). "KELT-3b: A Hot Jupiter Transiting a V = 9.8 Late-F Star". The Astrophysical Journal 773 (1): 64. doi:10.1088/0004-637X/773/1/64. ISSN 0004-637X. Bibcode: 2013ApJ...773...64P. http://adsabs.harvard.edu/abs/2013ApJ...773...64P.
26. ↑ Collins, Karen A. et al. (2013), "KELT-6b: AP~ 7.9 DAY HOT SATURN TRANSITING a METAL-POOR STAR WITH a LONG-PERIOD COMPANION", The Astronomical Journal 147 (2): 39, doi:10.1088/0004-6256/147/2/39
27. ↑ 27.0 27.1 27.2 Barclay, Thomas et al. (2013), "A sub-Mercury-sized exoplanet", Nature 494 (7438): 452–454, doi:10.1038/nature11914, PMID 23426260, Bibcode: 2013Natur.494..452B
28. ↑ Exoplanet Characterization by Proxy: a Transiting 2.15 R Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61 Sarah Ballard, David Charbonneau, Francois Fressin, Guillermo Torres, Jonathan Irwin, Jean-Michel Desert, Elisabeth Newton, Andrew W. Mann, David R. Ciardi, Justin R. Crepp, Christopher E. Henze, Stephen T. Bryson, Steven B. Howell, Elliott P. Horch, Mark E. Everett, Avi Shporer et al. April 26, 2013
29. ↑ 29.0 29.1 29.2 29.3 29.4 Borucki, William J. et al. (2013), "Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone", Science 340 (6132): 587–590, doi:10.1126/science.1234702, PMID 23599262, Bibcode: 2013Sci...340..587B
30. ↑ Sanchis-Ojeda, Roberto; Winn, Joshua N.; Marcy, Geoffrey W.; Howard, Andrew W.; Isaacson, Howard; Johnson, John Asher; Torres, Guillermo; Albrecht, Simon et al. (2013), "KEPLER-63b: A GIANT PLANET IN a POLAR ORBIT AROUND a YOUNG SUN-LIKE STAR", The Astrophysical Journal 775 (1): 54, doi:10.1088/0004-637X/775/1/54, Bibcode: 2013ApJ...775...54S
31. ↑ 31.0 31.1 31.2 Chaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J. et al. (2013), "Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65", The Astrophysical Journal 766 (2): 101, doi:10.1088/0004-637X/766/2/101, Bibcode: 2013ApJ...766..101C
32. ↑ 32.0 32.1 The same frequency of planets inside and outside open clusters of stars
33. ↑ 33.0 33.1 33.2 Gilliland, Ronald L. et al. (2013). "Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants". The Astrophysical Journal 766 (1): 40. doi:10.1088/0004-637X/766/1/40. Bibcode: 2013ApJ...766...40G.
34. ↑ 34.0 34.1 Barclay, Thomas et al. (2013), "A Super-Earth-Sized Planet Orbiting in or Near the Habitable Zone Around a Sun-Like Star", The Astrophysical Journal 768 (2): 101, doi:10.1088/0004-637X/768/2/101, Bibcode: 2013ApJ...768..101B
35. ↑ Kane, Stephen R.; Barclay, Thomas; Gelino, Dawn M. (2013), "A Potential Super-Venus in the Kepler-69 System", The Astrophysical Journal 770 (2): L20, doi:10.1088/2041-8205/770/2/L20, Bibcode: 2013ApJ...770L..20K
36. ↑ 36.0 36.1 Hébrard, G.; Almenara, J.-M.; Santerne, A.; Deleuil, M.; Damiani, C.; Bonomo, A. S.; Bouchy, F.; Bruno, G. et al. (2013), "KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N", Astronomy & Astrophysics 554: A114, doi:10.1051/0004-6361/201321394, Bibcode: 2013A&A...554A.114H
37. ↑ Faigler, S. et al. (2013). "BEER Analysis of Kepler and CoRoT Light Curves. I. Discovery of Kepler-76b: A Hot Jupiter with Evidence for Superrotation". The Astrophysical Journal 771 (1): 26. doi:10.1088/0004-637X/771/1/26. Bibcode: 2013ApJ...771...26F.
38. ↑ Gandolfi, D.; Parviainen, H.; Fridlund, M.; Hatzes, A. P.; Deeg, H. J.; Frasca, A.; Lanza, A. F.; Prada Moroni, P. G. et al. (2013), "Kepler-77b: A very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star", Astronomy & Astrophysics 557: A74, doi:10.1051/0004-6361/201321901, Bibcode: 2013A&A...557A..74G
39. ↑ Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in the Keplerdataset", Astronomy & Astrophysics 561: A103, doi:10.1051/0004-6361/201220935
40. ↑ 40.0 40.1 Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in the Keplerdataset", Astronomy & Astrophysics 561: A103, doi:10.1051/0004-6361/201220935
41. ↑ 41.0 41.1 Nesvorný, David; Kipping, David; Terrell, Dirk; Hartman, Joel; Bakos, Gáspár Á.; Buchhave, Lars A. (2013), "Koi-142, the King of Transit Variations, is a Pair of Planets Near the 2:1 Resonance", The Astrophysical Journal 777 (1): 3, doi:10.1088/0004-637X/777/1/3, Bibcode: 2013ApJ...777....3N
42. ↑ Barros, S. C. C.; Díaz, R. F.; Santerne, A.; Bruno, G.; Deleuil, M.; Almenara, J.-M.; Bonomo, A. S.; Bouchy, F. et al. (2013), "SOPHIE velocimetry of Keplertransit candidates", Astronomy & Astrophysics 561: L1, doi:10.1051/0004-6361/201323067
43. ↑ 43.0 43.1 43.2 43.3 Masuda, Kento et al. (2013). "Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse". The Astrophysical Journal 778 (2): 185. doi:10.1088/0004-637X/778/2/185. Bibcode: 2013ApJ...778..185M.
44. ↑ 44.0 44.1 44.2 44.3 44.4 44.5 44.6 44.7 Schmitt, Joseph R. et al. (2013), "Planet Hunters. Vi. An Independent Characterization of Koi-351 and Several Long Period Planet Candidates from Thekeplerarchival Data", The Astronomical Journal 148 (2): 28, doi:10.1088/0004-6256/148/2/28
45. ↑ Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C. et al. (2013). "Kepler-91b: A planet at the end of its life. Planet and giant host star properties via light-curve variations". Astronomy & Astrophysics 562: A109. doi:10.1051/0004-6361/201322001. Bibcode: 2014A&A...562A.109L.
46. ↑ 46.00 46.01 46.02 46.03 46.04 46.05 46.06 46.07 46.08 46.09 46.10 46.11 46.12 46.13 46.14 46.15 46.16 46.17 46.18 46.19 46.20 46.21 46.22 46.23 46.24 46.25 46.26 46.27 46.28 46.29 Xie, Ji-Wei (2013), "Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems", The Astrophysical Journal Supplement Series 210 (2): 25, doi:10.1088/0067-0049/210/2/25
47. ↑ 47.0 47.1 47.2 47.3 Wang, Ji; Xie, Ji-Wei; Barclay, Thomas; Fischer, Debra A. (2013), "Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation Due to Stellar Companions within 20 Au and Validation of Four Planets from Thekeplermultiple Planet Candidates", The Astrophysical Journal 783: 4, doi:10.1088/0004-637X/783/1/4, Bibcode: 2014ApJ...783....4W
48. ↑ 48.0 48.1 48.2 48.3 48.4 48.5 Yang, Ming; Liu, Hui-Gen; Zhang, Hui; Zhou, Ji-Lin (2013), "8 Planets in 4 Multi-planet Systems via TTVs in 1350 Days", The Astrophysical Journal 778 (2): 110, doi:10.1088/0004-637X/778/2/110, Bibcode: 2013ApJ...778..110Y
49. ↑ Van Eylen, V.; Lund, M. N.; Aguirre, V. Silva; Arentoft, T.; Kjeldsen, H.; Albrecht, S.; Chaplin, W. J.; Isaacson, H. et al. (2013), "WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS a SMALL NEPTUNE AROUND a BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY", The Astrophysical Journal 782: 14, doi:10.1088/0004-637X/782/1/14, Bibcode: 2014ApJ...782...14V
50. ↑ Wang, Ji et al. (2015), "Planet Hunters. Viii. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data", The Astrophysical Journal 815 (2): 127, doi:10.1088/0004-637X/815/2/127, Bibcode: 2015ApJ...815..127W
51. ↑ Suzuki, D. et al. (2013), "MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM a HIGH MAGNIFICATION EVENT WITH a FAINT SOURCE", The Astrophysical Journal 780 (2): 123, doi:10.1088/0004-637X/780/2/123
52. ↑ Furusawa, K. et al. (2013), "MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?", The Astrophysical Journal 779 (2): 91, doi:10.1088/0004-637X/779/2/91, Bibcode: 2013ApJ...779...91F
53. ↑ 53.0 53.1 MOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE
54. ↑ Batista, V.; Beaulieu, J. -P.; Gould, A.; Bennett, D. P.; Yee, J. C.; Fukui, A.; Gaudi, B. S.; Sumi, T. et al. (2013), "MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone", The Astrophysical Journal 780: 54, doi:10.1088/0004-637X/780/1/54
55. ↑ Shvartzvald, Y. et al. (2013), "MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet", Monthly Notices of the Royal Astronomical Society 439: 604–610, doi:10.1093/mnras/stt2477
56. ↑ Kains, N.; Street, R. A.; Choi, J.-Y.; Han, C.; Udalski, A.; Almeida, L. A.; Jablonski, F.; Tristram, P. J. et al. (2013), "A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251", Astronomy & Astrophysics 552: A70, doi:10.1051/0004-6361/201220626, Bibcode: 2013A&A...552A..70K
57. ↑ Han, C. et al. (2013), "Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf", The Astrophysical Journal 778 (1): 38, doi:10.1088/0004-637X/778/1/38, Bibcode: 2013ApJ...778...38H
58. ↑ Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon et al. (2014), "SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb", The Astrophysical Journal 782 (1): 47, doi:10.1088/0004-637X/782/1/47, Bibcode: 2014ApJ...782...47P
59. ↑ Wang, Ji (January 3, 2013). "Planet Hunters. V. A Confirmed Jupiter-Size Planet in the Habitable Zone and 42 Planet Candidates from the Kepler Archive Data". arXiv:1301.0644v1 [astro-ph].
60. ↑ Koppenhoefer, J.; Saglia, R. P.; Fossati, L.; Lyubchik, Y.; Mugrauer, M.; Bender, R.; Lee, C.- H.; Riffeser, A. et al. (2013), "A hot Jupiter transiting a mid-K dwarf found in the pre-Omega Cam Transit Survey", Monthly Notices of the Royal Astronomical Society 435 (4): 3133–3147, doi:10.1093/mnras/stt1512
61. ↑ Michael C. Liu; Eugene A. Magnier; Niall R. Deacon; Katelyn N. Allers et al. (1 October 2013). "The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets". Astrophysical Journal Letters 777 (2). doi:10.1088/2041-8205/777/2/L20. Bibcode: 2013ApJ...777L..20L.
62. ↑ 62.0 62.1 Kraus, Adam L.; Ireland, Michael J.; Cieza, Lucas A.; Hinkley, Sasha; Dupuy, Trent J.; Bowler, Brendan P.; Liu, Michael C. (2013), "THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B", The Astrophysical Journal 781: 20, doi:10.1088/0004-637X/781/1/20
63. ↑ Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha et al. (2013), "Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets", The Astrophysical Journal 785 (2): 126, doi:10.1088/0004-637X/785/2/126
64. ↑ 64.0 64.1 Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M. et al. (2013), "Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii", Astronomy & Astrophysics 559: A36, doi:10.1051/0004-6361/201322314, Bibcode: 2013A&A...559A..36G
65. ↑ 65.0 65.1 65.2 Delrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C. et al. (2013), "Transiting planets from WASP-South, Euler and TRAPPIST:WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars", Astronomy and Astrophysics 563, doi:10.1051/0004-6361/201323204, Bibcode: 2014A&A...563A.143D
66. ↑ 66.0 66.1 66.2 Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y. et al. (2013), Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary, doi:10.1093/mnras/stu1737
67. ↑ Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2013), "An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b", Publications of the Astronomical Society of the Pacific 130 (985): 034401, doi:10.1088/1538-3873/aaa33e
68. ↑ 68.0 68.1 68.2 West, R. G.; Hellier, C.; Almenara, J.-M.; Anderson, D. R.; Barros, S. C. C.; Bouchy, F.; Brown, D. J. A.; Collier Cameron, A. et al. (2016), "Three irradiated and bloated hot Jupiters", Astronomy & Astrophysics 585: A126, doi:10.1051/0004-6361/201527276, Bibcode: 2016A&A...585A.126W
69. ↑ Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2013), "WASP-80b: a gas giant transiting a cool dwarf", Astronomy & Astrophysics 551: A80, doi:10.1051/0004-6361/201220900, Bibcode: 2013A&A...551A..80T
70. ↑ 70.0 70.1 70.2 70.3 70.4 70.5 70.6 Hellier, Coel; Anderson, D. R.; Cameron, A. Collier; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L. et al. (2013), "Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b", Monthly Notices of the Royal Astronomical Society 440 (3): 1982–1992, doi:10.1093/mnras/stu410
71. ↑ WTS-2 b: Too close for comfort?
72. ↑ Birkby, J. L. et al. (2014), "WTS-2 b: A hot Jupiter orbiting near its tidal destruction radius around a K dwarf", Monthly Notices of the Royal Astronomical Society 440 (2): 1470–1489, doi:10.1093/mnras/stu343

* v
* t
* e

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
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* 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
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* Giant-impact hypothesis
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* 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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