List of exoplanets discovered in 2012

Short description: None

This is a List of exoplanets discovered in 2012.[1] 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)[2] | Discovery method  | Distance (ly)  | Host star mass (M☉)  | Host star temp. (K)  | Remarks

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75 Ceti b | 3  |  | 691.9  | 2.1  |  | radial vel.  | 266  | 2.49  | 4846  | [3]
BD+20 274 b | 4.2  |  | 578.2  | 1.3  |  | radial vel.  | 4500±300  | 0.8  | 4296  | [4]
BD+48 740 b | 1.7±0.7  |  | 733+5−8 | 1.7±0.1  |  | radial vel.  | 2214±72  | 1.09±0.16  | 4534±8  | [5] Confirmed in 2018.[6]
CoRoT-21b | 2.26  | 1.3  | 2.72  | 0.0417  | 1867  | transit  | 4600±900  | 1.29  | 6200  | [7]
Epsilon Coronae Borealis b | 6.7  |  | 417.9  | 1.3  |  | radial vel.  | 229.7  | 1.7  | 4406  | [8]
Gliese 676 Ad  | 0.014  |  | 3.6005  | 0.0413±0.0014  |  | radial vel.  | 52.29±0.03  | 0.71±0.04  | 3734  | [9]
Gliese 676 Ae  | 0.025  |  | 35.39  | 0.187±0.007  |  | radial vel.  | 52.29±0.03  | 0.71±0.04  | 3734  | [9]
Gliese 3470 b | 0.043  | 0.346  | 3.3366487  | 0.031  |  | radial vel.  | 82  | 0.51  | 3652  | [10]
HAT-P-34b  | 7.01  | 1.35  | 5.45265  | 0.06774  | 1520  | transit  | 818.94  | 4.26  | 6442  | [11] Proper name Ġgantija
HAT-P-35b  | 7.52  | 3.55  | 3.64671  | 0.0498  | 1581  | transit  | 1677  | 23.56  | 6096  | [11]
HAT-P-36b  | 1.8482  | 1.277  | 1.32734683  | 0.0241  | 1781  | transit  | 968.49  | 1.03  | 5620  | [11] Proper name Bran
HAT-P-37b  | 1.169  | 1.178  | 2.797436  | 0.0379  | 1271  | transit  | 1341  | 0.93  | 5500  | [11]Additional planets in system are suspected[12]
HAT-P-38b  | 0.267  | 0.825  | 4.640382  | 0.0523  |  | transit  | 810  | 0.89  | 5330  | [13] Proper name Hiisi
HAT-P-39b  | 0.599  | 1.571  | 3.54387  | 0.0509  |  | transit  | 2090  | 1.4  | 6430  | [14]
HAT-P-40b  | 0.615  | 1.73  | 4.457243  | 0.0608  |  | transit  | 1630  | 1.51  | 6080  | [14] Proper name Vytis
HAT-P-41b | 0.8  | 1.685  | 2.694047  | 0.0426  |  | transit  | 1120  | 1.42  | 6390  | [15][14][16]
HAT-P-42b  | 1.044  | 1.28  | 4.641878  | 0.0575  | 1427  | transit  | 1460  | 1.18  | 5743  | [17] Proper name Iolaus
HAT-P-43b  | 0.662  | 1.281  | 3.332687  | 0.0443  | 1361  | transit  | 1770  | 1.05  | 5645  | [17]
HATS-1b  | 1.855  | 1.302  | 3.446459  | 0.0444  |  | transit  | 990  | 0.99  | 5870  | [18]
HD 142 c | 5.3  |  | 6005  | 6.8  |  | radial vel.  | 83.6  | 1.23  | 6245  | [19]
HD 4732 b  | 2.37  |  | 360.2  | 1.19  |  | radial vel.  | 184  | 1.74  | 4959  | [20]
HD 4732 c  | 2.37  |  | 2732  | 4.6  |  | radial vel.  | 184  | 1.74  | 4959  | [20]
HD 5608 b  | 1.4  |  | 792.6  | 1.9  |  | radial vel.  | 189.7  | 1.55  | 4854  | [3]
HD 24040 b | 4.10±0.12  |  | 3490±25  | 4.637±0.067  |  | radial vel.  | 152.3±0.4  | 1.14±0.02  | 5917±52  | [21] Suspected since 2006
HD 27631 b | 1.45  |  | 2208  | 3.25  |  | radial vel.  | 145.3  | 0.94  | 5737  | [22]
HD 37605 c | 3.366  |  | 2720  | 3.814  |  | radial vel.  | 139.9  | 1  | 5448  | [23]
HD 40307 e | 0.0110±0.0044  |  | 34.62+0.21−0.20 | 0.1886+0.083−0.0104 |  | radial vel.  | 41.8  | 0.77  | 4956  | [24]
HD 40307 f | 0.0164  |  | 51.76  | 0.247  |  | radial vel.  | 41.8  | 0.77  | 4956  | [24]
HD 40307 g | 0.0223  |  | 197.8  | 0.6  |  | radial vel.  | 41.8  | 0.77  | 4956  | [24]
HD 66141 b  | 6  |  | 480.5  | 1.2  |  | radial vel.  | 261.1  | 1.1  | 4323  | [25]
HD 77338b | 0.05  |  | 5.7361  | 0.0614  |  | radial vel.  | 134.6  | 0.93  | 5370  | [26]
HD 79498 b | 1.34  |  | 1807  | 2.98  |  | radial vel.  | 159.89  | 1.08  | 5748  | [27]
HD 98649 b | 6.8  |  | 4951  | 5.6  |  | radial vel.  | 139.5  | 1  | 5759  | [22]
HD 106515 Ab | 9.61  |  | 3630  | 4.59  |  | radial vel.  | 118.6  | 0.97  | 5362  | [22]
HD 150706 b | 2.71  |  | 5894  | 6.7  |  | radial vel.  | 88.8  | 1.17  | 5961  | [21]
HD 159868 c | 0.73  |  | 352.3  | 1  |  | radial vel.  | 171.9  | 1.09  | 5558  | [19]
HD 166724 b | 3.53  |  | 5144  | 5.42  |  | radial vel.  | 140.2  | 0.81  | 5127  | [22]
HD 197037 b | 0.79  |  | 1035.7  | 2.07  |  | radial vel.  | 107.1  | 1.063±0.022  | 6137±20  | [27]
HD 207832 b | 0.56  |  | 161.97  | 0.57  |  | radial vel.  | 180.4  | 0.94  | 5710  | [28] Suspected false positive[29]
HD 207832 c | 0.73  |  | 1155.7  | 2.112  |  | radial vel.  | 180.4  | 0.94  | 5710  | [28] Suspected false positive[29]
HD 208527 b  | 9.9  |  | 875.5  | 2.1  |  | radial vel.  | 1148.4  | 1.6  | 4035  | [30]
HD 219077 b | 10.39  |  | 5501  | 6.22  |  | radial vel.  | 95  | 1.05  | 5362  | [22]
HD 219415 b  | 1  |  | 2093.3  | 3.2  |  | radial vel.  | 553.7  | 1  | 4820  | [4]
HD 220074 b  | 11.1  |  | 672.1  | 1.6  |  | radial vel.  | 942.7  | 1.2  | 3935  | [30]
HD 220689 b | 1.06  |  | 2209  | 3.36  |  | radial vel.  | 147.5  | 1.04  | 5921  | [22]
HD 220773 b | 1.45  |  | 3724.7  | 4.94  |  | radial vel.  | 159.82  | 1.16  | 5940  | [27]
HD 222155 b | 2.12  |  | 3999  | 5.14  |  | radial vel.  | 165.3  | 1.21  | 5701  | [21]
HW Virginis b  | 14.3  |  | 4640  | 4.69  |  | timing  | 590  | 0.485  |  | [31]Likely false positive[32]
Kappa Andromedae b | 13.616  |  |  | 55  | 1850  | imaging  | 169.7  | 2.6  | 10900  | Has a reddish color, and may be a brown dwarf[33]
KELT-1b | 27.23  | 1.11  | 1.217514  | 0.02466  | 2423  | transit  | 850  | 1.32  | 6518  | [34]
KELT-2Ab | 1.522  | 1.286  | 4.1137912  | 0.05496  |  | transit  | 405.2  | 1.31  | 6151  | [35]
Kepler-30b | 0.036  | 0.348  | 29.33434  | 0.18  |  | transit  | 4600  | 0.99  | 5498  | [36]
Kepler-30c | 2.01  | 1.097  | 60.323105  | 0.3  |  | transit  | 4600  | 0.99  | 5498  | [36]
Kepler-30d | 0.073  | 0.785  | 143.34394  | 0.5  |  | transit  | 4600  | 0.99  | 5498  | [36]
Kepler-32d |  | 0.241  | 22.7802  | 0.13  |  | transit  | 990  | 0.58  | 3900  | [36]
Kepler-32e |  | 0.134  | 2.896  | 0.033  |  | transit  | 990  | 0.58  | 3900  | Weak evidence[36]
Kepler-32f |  | 0.073  | 0.74296  | 0.013  |  | transit  | 990  | 0.58  | 3900  | Weak evidence[36]
Kepler-33f | 0.03036  | 0.398  | 41.02902  | 0.2535  |  | transit  | 4086  | 1.29  | 5904  | [37]
Kepler-34b | 0.22  | 0.764  | 288.822  | 1.0896  |  | transit  | 4889  | 1.05  | 5913  | [38]
Kepler-35b | 0.127  | 0.728  | 131.458  | 0.60347  |  | transit  | 5365  | 0.89  | 5606  | [38]
Kepler-36b | 0.014  | 0.133  | 13.83989  | 0.1153  |  | transit  | 1500  | 1.07  | 5911  | [39]
Kepler-36c | 0.025  | 0.328  | 16.23855  | 0.1283  |  | transit  | 1500  | 1.07  | 5911  | [39]
Kepler-38b | 0.384  | 0.384  | 105.599  | 0.4632  |  | transit  | 2000  | 0.94  | 5623  | [40]
Kepler-46b | 6  | 0.808  | 33.60134  | 0.1968  |  | transit  | 2790  | 0.9  | 5309  | [41]
Kepler-46c | 0.376  |  | 57.011  | 0.2799  |  | timing  | 2790  | 0.9  | 5309  | [41]
Kepler-47b | 2  | 0.27  | 49.532  | 0.2962  |  | transit  | 4900  | 1.05  | 5636  | [42]
Kepler-47c | 28  | 0.411  | 303.137  | 0.991  |  | transit  | 4900  | 1.05  | 5636  | [42]
Kepler-48b  | 0.0124  | 0.168  | 4.778  |  |  | transit  | 1009±5  | 0.88  | 5194  | [43][44]
Kepler-48c  | 0.04597  | 0.242  | 9.67395  |  |  | transit  | 1009±5  | 0.88  | 5194  | [43][44]
Kepler-49b  | 0.98  | 0.243  | 7.2037945  |  |  | transit  | 1024±8  | 0.55  | 4252  | [43][44]
Kepler-49c  | 0.72  | 0.227  | 10.9129343  |  |  | transit  | 1024±8  | 0.55  | 4252  | [43][44]
Kepler-50b  |  | 0.153  | 7.81254  | 0.077  |  | transit  | 821±6  | 1.24  | 6225  | [44]
Kepler-50c  |  | 0.194  | 9.37647  | 0.087  |  | transit  | 821±6  | 1.24  | 6225  | [44]
Kepler-51b | 0.007  | 0.633  | 45.154  | 0.2514  | 543  | transit  | 2610±50  | 1.04  | 6018  | [44]
Kepler-51c | 0.013  | 0.803  | 85.312  | 0.384  | 439  | transit  | 2610±50  | 1.04  | 6018  | [44]
Kepler-52b  | 8.7  | 0.187  | 7.8773565  |  |  | transit  | 1058±7  | 0.54  | 4263  | [44]
Kepler-52c  | 10.41  | 0.164  | 16.3850021  |  |  | transit  | 1058±7  | 0.54  | 4263  | [44]
Kepler-53b  | 18.41  | 0.258  | 18.6489525  |  |  | transit  | 4600±200  | 0.98  | 5858  | [43][44]
Kepler-53c  | 15.74  | 0.283  | 38.5583038  |  |  | transit  | 4600±200  | 0.98  | 5858  | [43][44]
Kepler-54b  | 0.92  | 0.187  | 8.0109434  |  |  | transit  | 893±9  | 0.51  | 4252  | [44]
Kepler-54c  | 0.37  | 0.11  | 12.0717249  |  |  | transit  | 893±9  | 0.51  | 4252  | [44]
Kepler-55b  | 1.49  | 0.217  | 27.9481449  |  |  | transit  | 1920±30  | 0.62  | 4503  | [44]
Kepler-55c  | 1.11  | 0.197  | 42.1516418  |  |  | transit  | 1920±30  | 0.62  | 4503  | [44]
Kepler-56b | 0.07  | 0.581  | 10.5016  | 0.1028  |  | transit  | 3060±80  | 1.32  | 4840  | [44]
Kepler-56c | 0.57  | 0.874  | 21.40239  | 0.1652  |  | transit  | 3060±80  | 1.32  | 4840  | [44]
Kepler-57b  | 18.86  | 0.195  | 5.7293196  |  |  | transit  | 3140±30  | 0.83  | 5145  | [43][44]
Kepler-57c  | 6.95  | 0.138  | 11.6092567  |  |  | transit  | 3140±30  | 0.83  | 5145  | [43][44]
Kepler-58b  | 1.39  | 0.248  | 10.2184954  |  |  | transit  | 3250±80  | 0.95  | 6099  | [43][44]
Kepler-58c  | 2.19  | 0.255  | 15.5741568  |  |  | transit  | 3250±80  | 0.95  | 6099  | [43][44]
Kepler-59b | 2.05  | 0.098  | 11.8681707  |  |  | transit  | 3925±75  | 1.04  | 6074  | [44]
Kepler-59c  | 1.37  | 0.177  | 17.9801235  |  |  | transit  | 3925±75  | 1.04  | 6074  | [44]
Kepler-60b  | 0.01318  | 0.153  | 7.1334  |  |  | transit  | 3440±70  | 1.04  | 5905  | [44]
Kepler-60c  | 0.01211  | 0.17  | 8.9187  |  |  | transit  | 3440±70  | 1.04  | 5905  | [44]
Kepler-60d | 0.01309  | 0.178  | 11.8981  |  |  | transit  | 3440±70  | 1.04  | 5905  | [44]
Kepler-64b | 0.531  | 0.551  | 138.317  | 0.652  |  | transit  | 6200±1000  | 1.53  | 6407  | [45] Quadruple star system
Kepler-79b  | 0.0343  | 0.31  | 13.4845  | 0.117  | 868  | transit  | 3430±60  | 1.17  | 6174  | [43]
Kepler-79c  | 0.019  | 0.332  | 27.4029  | 0.187  | 685  | transit  | 3430±60  | 1.17  | 6174  | [43]
Kepler-80b | 0.0218  | 0.238  | 7.05246  | 0.0648  |  | transit  | 1160  | 0.73  | 4540  | [43]
Kepler-80c | 0.02121  | 0.244  | 9.52355  | 0.0792  |  | transit  | 1160  | 0.73  | 4540  | [43]
Kepler-81b  |  | 0.216  | 5.955  |  | 646  | transit  | 1147±10  | 0.64  | 4500  | [43]
Kepler-81c  |  | 0.211  | 12.04  |  | 513  | transit  | 1147±10  | 0.64  | 4500  | [43]
Kepler-82b  |  | 0.357  | 26.444  |  | 581  | transit  | 3030±80  | 0.85  | 5428  | [43]
Kepler-82c  |  | 0.477  | 51.538  |  | 464  | transit  | 3030±80  | 0.85  | 5428  | [43]
Kepler-83b  |  | 0.252  | 9.77  |  |  | transit  | 1320±17  | 0.66  | 4648  | [43][46]
Kepler-83c  |  | 0.211  | 20.09  |  |  | transit  | 1320±17  | 0.66  | 4648  | [43][46]
Kepler-84b  |  | 0.199  | 8.726  |  | 937  | transit  | 4700±500  | 1  | 6031  | [43][46]
Kepler-84c  |  | 0.211  | 12.883  |  | 821  | transit  | 4700±500  | 1  | 6031  | [43][46]
Kepler-85b  |  | 0.176  | 8.306  |  |  | transit  | 2550±50  | 0.92  | 5436  | [43] KOI-2038[47]
Kepler-85c  |  | 0.194  | 12.513  |  |  | transit  | 2550±50  | 0.92  | 5436  | [43] KOI-2038[47]
MOA-2011-BLG-293Lb (ja)  | 2.4+1.4−0.9 |  |  | 1.0±0.1  |  | microlensing  | 23000±2000  | 0.675±0.525  |  | [48]
MOA-2010-BLG-073Lb  | 11  |  |  | 1.21  |  | microlensing  | 9100  | 0.16  |  | Possibly brown dwarf[49]
MOA-2010-BLG-477Lb | 1.4±0.3  |  |  | 2.8±0.5  |  | microlensing  | 7500±2000  | 0.53±0.11  | 5950±150  | [50]White dwarf host star[51]
MOA-bin-1Lb  | 3.7±2.1  |  |  | 8.3+4.5−2.7 |  | microlensing  | 17000  | 0.75+0.33−0.41 |  | [52]
Mu2 Octantis b | 6.9  |  | 3638  | 5.02  |  | radial vel.  | 142.1  | 1.29  | 6017  | [22]
Nu Ophiuchi b | 24  |  | 530.32  | 1.9  |  | radial vel.  | 152.8  | 3.04  | 4928  | Brown dwarf or small star[3]
Nu Ophiuchi c | 27  |  | 3186  | 6.1  |  | radial vel.  | 152.8  | 3.04  | 4928  | Brown dwarf or small star[3]
OGLE-2012-BLG-0026Lb  | 0.145  |  |  | 4  |  | microlensing  | 13110  | 1.06  |  | [53]
OGLE-2012-BLG-0026Lc  | 0.86  |  |  | 4.8  |  | microlensing  | 13110  | 1.06  |  | [53]
Omicron Coronae Borealis b | 1.5  |  | 187.83  | 0.83  |  | radial vel.  | 274.1  | 2.13  | 4749  | [3]
Omicron Ursae Majoris b | 4.1  |  | 1630  | 3.9  |  | radial vel.  | 183.7  | 3.09  | 5242  | [3]
Pr0201 b | 0.54  |  | 4.4264  |  |  | radial vel.  | 610  | 1.23  | 6174  | [54] In Beehive Cluster
Pr0211 b | 1.88  |  | 2.1461  | 0.03176  |  | radial vel.  | 610  | 0.94  | 5300  | [54] Multi-planet system In Beehive Cluster
RR Caeli b | 3.0±0.3  |  | 1900±40  | 5.2±0.1  |  | timing  | 69.10±0.03  | 0.18+0.44  | 3100+7540  | Circumbinary planet around red and white dwarfs.[55][56]
Tau Ceti e | 0.0124  |  | 162.87  | 0.538  |  | radial vel.  | 12  | 0.78  |  | [57] Potentially habitable exoplanet
Tau Ceti f | 0.0124  |  | 636.13  | 1.334  |  | radial vel.  | 12  | 0.78  |  | [57]
WASP-42b | 0.527  | 1.122  | 4.9816819  | 0.0561  | 1021±19  | transit  | 520  | 0.95  | 5315  | [58]
WASP-47b | 1.21  | 1.15  | 4.16071  | 0.052  | 1275  | transit  | 650  | 1.11  | 5576  | [59]
WASP-49b | 0.378  | 1.115  | 2.7817387  | 0.0379  | 1369±39  | transit  | 550  | 0.94  | 5600  | [58]
WASP-52b | 0.46  | 1.27  | 1.7497798  | 0.0272  | 1315±35  | transit  | 460  | 0.87  | 5000  | [60] Proper name Göktürk
WASP-54b | 0.636  | 1.653  | 3.6936411  | 0.04987  | 1742+49−69 | transit  | 650  | 1.21  | 6100  | [61]
WASP-55b | 0.627  | 1.335  | 4.4656291  | 0.0558  | 1290  | transit  | 1100  | 1.16  | 6070  | [59]
WASP-56b | 0.571  | 1.092  | 4.617101  | 0.05458  | 1200  | transit  | 830  | 1.03  | 5600  | [61]
WASP-57b | 0.644  | 1.05  | 2.83891856  | 0.03769  | 1338±29  | transit  | 1480  | 0.89  | 5600  | [61]
WASP-58b | 0.89  | 1.37  | 5.01718  | 0.0561  | 1270±80  | transit  | 980  | 0.94  | 5800  | [60]
WASP-59b | 0.863  | 0.775  | 7.919585  | 0.0697  | 670±35  | transit  | 410  | 0.72  | 4650  | [60]
WASP-60b | 0.514  | 0.86  | 4.3050011  | 0.0531  | 1479±35  | transit  | 1300  | 1.08  | 5900  | [60] Proper name Vlasina
WASP-61b | 2.06  | 1.24  | 3.8559  | 0.0514  | 1565±35  | transit  | 1600  | 1.22  | 6320  | [59]
WASP-62b | 0.57  | 1.39  | 4.411953  | 0.0567  | 1329.6±44.8  | transit  | 520  | 1.25  | 6280  | [59] Proper name Krotoa
WASP-63b | 0.38  | 1.43  | 4.37809  | 0.0574  | 1536±37  | transit  | 1100  | 1.32  | 5570  | [59]
WASP-64b | 1.271  | 1.271  | 1.5732918  | 0.02648  | 1989+87−88 | transit  | 1100  | 1  | 5400  | [62] Proper name Agouto
WASP-66b | 2.32  | 1.39  | 4.086052  | 0.0546  | 1790±60  | transit  | 1200  | 1.3  | 6580  | [59]
WASP-67b | 0.42  | 1.4  | 4.61442  | 0.0517  | 1050  | transit  | 730  | 0.87  | 5240  | [59]
WASP-71b | 2.242  | 1.46  | 2.9036747  | 0.04619  | 2016.1+67.0−52.5 | transit  | 1130  | 1.56  | 6059  | [63] Proper name Tanzanite
WASP-72b | 1.5461  | 1.27  | 2.2167421  | 0.03708  | 2210+120−130 | transit  | 1100  | 1.39  | 6250  | [62] Proper name Cuptor
WASP-77Ab  | 1.76  | 1.21  | 1.3600309  | 0.024  | 1715  | transit  | 300  | 1  | 5500  | Orbiting primary star of binary star system[64]
WASP-78b | 0.89  | 1.7  | 2.17517632  | 0.0362  | 2350  | transit  | 1800  | 1.17  | 6100  | [65]
WASP-79b | 0.9  | 2.09  | 3.6623866  | 0.0535  | 1900±50  | transit  | 780  | 1.38  | 6600  | [65] Proper name Pollera
WISE 1217+1626 B | 22  | 0.934  |  | 8  | 450  | imaging  | 29±3  | 0.03  | 575  | Brown dwarf[66]
WTS-1b  | 4.01  | 1.49  | 3.352057  | 0.047  | 1500±100  | transit  | 8100±1000  | 1.2  | 6250  | [67]

## Specific exoplanet lists

## References

1. ↑ "NASA Exoplanet Archive". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=compositepars.
2. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/.
3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 Sato, Bun'ei et al. (2012). "Substellar Companions to Seven Evolved Intermediate-Mass Stars". Publications of the Astronomical Society of Japan 64 (6): 135. doi:10.1093/pasj/64.6.135. Bibcode: 2012PASJ...64..135S.
4. ↑ 4.0 4.1 Gettel, S.; Wolszczan, A.; Niedzielski, A.; Nowak, G.; Adamów, M.; Zieliński, P.; MacIejewski, G. (2012), "Planets Around the K-Giants Bd+20 274 and Hd 219415", The Astrophysical Journal 756 (1): 53, doi:10.1088/0004-637X/756/1/53, Bibcode: 2012ApJ...756...53G
5. ↑ Adamów, M.; Niedzielski, A.; Villaver, E.; Nowak, G.; Wolszczan, A. (2012). "BD+48 740—Li Overabundant Giant Star with a Planet: A Case of Recent Engulfment?". The Astrophysical Journal 754 (1): L15. doi:10.1088/2041-8205/754/1/L15. Bibcode: 2012ApJ...754L..15A.
6. ↑ Adamów, M.; Niedzielski, A.; Kowalik, K.; Villaver, E.; Wolszczan, A.; MacIejewski, G.; Gromadzki, M. (2018), "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N", Astronomy & Astrophysics 613: A47, doi:10.1051/0004-6361/201732161
7. ↑ Transiting exoplanets from the CoRoT space mission XXIII. CoRoT-21b: a doomed large Jupiter around a faint subgiant star
8. ↑ Lee, B.-C.; Han, I.; Park, M.-G.; Mkrtichian, D. E.; Kim, K.-M. (2012). "A planetary companion around the K giant ɛ Corona Borealis". Astronomy & Astrophysics 546: 5. doi:10.1051/0004-6361/201219347. A5. Bibcode: 2012A&A...546A...5L.
9. ↑ 9.0 9.1 Anglada-Escudé, Guillem; Tuomi, Mikko (2012). "A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems". Astronomy 548: A58. doi:10.1051/0004-6361/201219910. Bibcode: 2012A&A...548A..58A. http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2.
10. ↑ Bonfils, Xavier; Gillon, Michaël; Udry, Stéphane; Armstrong, David; Bouchy, François; Delfosse, Xavier; Forveille, Thierry; Fumel, Aurélie et al. (2012). "A hot Uranus transiting the nearby M dwarf GJ3470. Detected with HARPS velocimetry. Captured in transit with TRAPPIST photometry". Astronomy & Astrophysics 546: A27. doi:10.1051/0004-6361/201219623. Bibcode: 2012A&A...546A..27B. http://orbi.ulg.ac.be/jspui/handle/2268/135085.
11. ↑ 11.0 11.1 11.2 11.3 Bakos, G. Á.; Hartman, J. D.; Torres, G.; Béky, B.; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Kovács, G. et al. (2012), "HAT-P-34b-HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS", The Astronomical Journal 144 (1): 19, doi:10.1088/0004-6256/144/1/19, Bibcode: 2012AJ....144...19B
12. ↑ A-thano, Napaporn; Jiang, Ing-Guey; Awiphan, Supachai; Rattanamala, Ronnakrit; Su, Li-Hsin; Hengpiya, Torik; Sariya, Devesh P.; Yeh, Li-Chin et al. (2022), "The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b", The Astronomical Journal 163 (2): 77, doi:10.3847/1538-3881/ac416d
13. ↑ Sato, Bun'ei; Hartman, Joel D.; Bakos, Gáspár Á.; Béky, Bence; Torres, Guillermo; Latham, David W.; Kovács, Géza; Csubry, Zoltán et al. (2012), "HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star", Publications of the Astronomical Society of Japan 64 (5): 97, doi:10.1093/pasj/64.5.97
14. ↑ 14.0 14.1 14.2 Hartman, J. D. (2012). "HAT-P-39b–HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters". The Astronomical Journal 144 (5): 139. doi:10.1088/0004-6256/144/5/139. Bibcode: 2012AJ....144..139H.
15. ↑ Lewis, N. K. (2020). "Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed". The Astrophysical Journal 902 (1): L19. doi:10.3847/2041-8213/abb77f. Bibcode: 2020ApJ...902L..19L.
16. ↑ Sheppard, Kyle B. (2021). "The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b". The Astronomical Journal 161 (2): 51. doi:10.3847/1538-3881/abc8f4. Bibcode: 2021AJ....161...51S.
17. ↑ 17.0 17.1 Boisse, I.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Csubry, Z.; Béky, B.; Latham, D. W.; Bieryla, A. et al. (2012), "HAT-P-42b and HAT-P-43b", Astronomy & Astrophysics 558: A86, doi:10.1051/0004-6361/201220993
18. ↑ Penev, K.; Bakos, G. Á.; Bayliss, D.; Jordán, A.; Mohler, M.; Zhou, G.; Suc, V.; Rabus, M. et al. (2012), "HATS-1b: THE FIRST TRANSITING PLANET DISCOVERED BY THE HATSouth SURVEY", The Astronomical Journal 145: 5, doi:10.1088/0004-6256/145/1/5
19. ↑ 19.0 19.1 Wittenmyer, Robert A.; Horner, J.; Tuomi, Mikko; Salter, G. S.; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; o'Toole, S. J. et al. (2012), "The Anglo-Australian Planet Search. Xxii. Two New Multi-Planet Systems", The Astrophysical Journal 753 (2): 169, doi:10.1088/0004-637X/753/2/169, Bibcode: 2012ApJ...753..169W
20. ↑ 20.0 20.1 Sato, Bun'ei et al. (2013). "A Double Planetary System around the Evolved Intermediate-mass Star HD 4732". The Astrophysical Journal 762 (1): 9. doi:10.1088/0004-637X/762/1/9. Bibcode: 2013ApJ...762....9S.
21. ↑ 21.0 21.1 21.2 Boisse, Isabelle; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Bonfils, Xavier; Bouchy, François; Santos, Nuno C.; Arnold, Luc et al. (2012), "The SOPHIE search for northern extrasolar planets V. Follow-up of ELODIE candidates: Jupiter-analogs around Sun-like stars", Astronomy and Astrophysics 545: A55, doi:10.1051/0004-6361/201118419, Bibcode: 2012A&A...545A..55B, http://www.aanda.org/articles/aa/full_html/2012/09/aa18419-11/aa18419-11.html
22. ↑ 22.0 22.1 22.2 22.3 22.4 22.5 22.6 Marmier, M. et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics 551: A90. doi:10.1051/0004-6361/201219639. Bibcode: 2013A&A...551A..90M.
23. ↑ Wang Xuesong, Sharon et al. (2012). "The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b". Astrophysical Journal 761 (1): 46. doi:10.1088/0004-637X/761/1/46. Bibcode: 2012ApJ...761...46W.
24. ↑ 24.0 24.1 24.2 Tuomi, M.; Anglada-Escudé, G.; Gerlach, E.; Jones, H. R. A.; Reiners, A.; Rivera, E. J.; Vogt, S. S.; Butler, R. P. (2012), "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307", Astronomy & Astrophysics 549: A48, doi:10.1051/0004-6361/201220268
25. ↑ Lee, B.-C.; Mkrtichian, D. E.; Han, I.; Park, M.-G.; Kim, K.-M. (2012), "Detection of an exoplanet around the evolved K giant HD 66141", Astronomy & Astrophysics 548: A118, doi:10.1051/0004-6361/201118014, Bibcode: 2012A&A...548A.118L
26. ↑ Jenkins, J. S.; Jones, H. R. A.; Tuomi, M.; Murgas, F.; Hoyer, S.; Jones, M. I.; Barnes, J. R.; Pavlenko, Y. V. et al. (2012), "A Hot Uranus Orbiting the Super Metal-Rich Star Hd 77338 and the Metallicity-Mass Connection", The Astrophysical Journal 766 (2): 67, doi:10.1088/0004-637X/766/2/67
27. ↑ 27.0 27.1 27.2 Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Wittenmyer, Robert A.; Horner, J.; Brugamyer, Erik J.; Simon, Attila E. et al. (2012). "The McDonald Observatory Planet Search: New Long-period Giant Planets and Two Interacting Jupiters in the HD 155358 System". The Astrophysical Journal 749 (1): 17 pp. doi:10.1088/0004-637X/749/1/39. Bibcode: 2012ApJ...749...39R.
28. ↑ 28.0 28.1 Haghighipour, Nader; Butler, R. Paul; Rivera, Eugenio J.; Henry, Gregory W.; Vogt, Steven S. (2012), "The Lick-Carnegie Survey: A New Two-Planet System Around the Star Hd 207832", The Astrophysical Journal 756 (1): 91, doi:10.1088/0004-637X/756/1/91, Bibcode: 2012ApJ...756...91H
29. ↑ 29.0 29.1 Luhn, Jacob K.; Wright, Jason T.; Howard, Andrew W.; Isaacson, Howard (2020), "Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars", The Astronomical Journal 159 (5): 235, doi:10.3847/1538-3881/ab855a, Bibcode: 2020AJ....159..235L
30. ↑ 30.0 30.1 Lee, B.-C.; Han, I.; Park, M.-G. (2012), "Planetary companions orbiting M giants HD 208527 and HD 220074", Astronomy & Astrophysics 549: A2, doi:10.1051/0004-6361/201220301
31. ↑ Beuermann, K.; Dreizler, S.; Hessman, F. V.; Deller, J. (2012). "The quest for companions to post-common envelope binaries. III. A reexamination of HW Virginis". Astronomy & Astrophysics 543: id.A138. doi:10.1051/0004-6361/201219391. Bibcode: 2012A&A...543A.138B.
32. ↑ Jonathan Horner; Robert Wittenmyer; Tobias Hinse; Jonathan Marshall; Alex Mustill (2014). "Wobbling Ancient Binaries - Here Be Planets?". arXiv:1401.6742 [astro-ph.EP].
33. ↑ Carson; Thalmann; Janson; Kozakis; Bonnefoy; Biller; Schlieder; Currie et al. (November 15, 2012). "Direct Imaging Discovery of a 'Super-Jupiter' Around the late B-Type Star Kappa And". The Astrophysical Journal 763 (2): L32. doi:10.1088/2041-8205/763/2/L32. Bibcode: 2013ApJ...763L..32C.
34. ↑ Fabrycky, Daniel C. et al. (2012), "Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models", The Astrophysical Journal 750 (2): 114, doi:10.1088/0004-637X/750/2/114, Bibcode: 2012ApJ...750..114F
35. ↑ Beatty, Thomas G. et al. (2012). "KELT-2Ab: A Hot Jupiter Transiting the Bright (V = 8.77) Primary Star of a Binary System". The Astrophysical Journal Letters 756 (2): L39. doi:10.1088/2041-8205/756/2/L39. Bibcode: 2012ApJ...756L..39B.
36. ↑ 36.0 36.1 36.2 36.3 36.4 36.5 Fabrycky, Daniel C. et al. (2012), "Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models", The Astrophysical Journal 750 (2): 114, doi:10.1088/0004-637X/750/2/114, Bibcode: 2012ApJ...750..114F
37. ↑ Lissauer, Jack J.; Marcy, Geoffrey W.; Rowe, Jason F.; Bryson, Stephen T.; Adams, Elisabeth; Buchhave, Lars A.; Ciardi, David R.; Cochran, William D. et al. (10 May 2012). "Almost All of Kepler's Multiple Planet Candidates are Planets". The Astrophysical Journal 750 (2): 112. doi:10.1088/0004-637X/750/2/112. Bibcode: 2012ApJ...750..112L.
38. ↑ 38.0 38.1 Welsh, William F. et al. (2012). "Transiting circumbinary planets Kepler-34 b and Kepler-35 b". Nature 481 (7382): 475–479. doi:10.1038/nature10768. PMID 22237021. Bibcode: 2012Natur.481..475W.
39. ↑ 39.0 39.1 Carter, J. A. et al. (2012). "Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities". Science 337 (6094): 556–559. doi:10.1126/science.1223269. PMID 22722249. Bibcode: 2012Sci...337..556C.
40. ↑ Orosz, Jerome A. et al. (2012), "THE NEPTUNE-SIZED CIRCUMBINARY PLANET KEPLER-38b", The Astrophysical Journal 758 (2): 87, doi:10.1088/0004-637X/758/2/87, Bibcode: 2012ApJ...758...87O
41. ↑ 41.0 41.1 Nesvorny, D. et al. (2012). "The Detection and Characterization of a Nontransiting Planet by Transit Timing Variations". Science 336 (6085): 1133–6. doi:10.1126/science.1221141. PMID 22582018. Bibcode: 2012Sci...336.1133N.
42. ↑ 42.0 42.1 Orosz, Jerome A.; Welsh, William F.; Carter, Joshua A.; Fabrycky, Daniel C.; Cochran, William D.; Endl, Michael; Ford, Eric B.; Haghighipour, Nader et al. (2012). "Kepler-47: A Transiting Circumbinary Multi-Planet System". Science 337 (6101): 1511–4. doi:10.1126/science.1228380. PMID 22933522. Bibcode: 2012Sci...337.1511O.
43. ↑ 43.00 43.01 43.02 43.03 43.04 43.05 43.06 43.07 43.08 43.09 43.10 43.11 43.12 43.13 43.14 43.15 43.16 43.17 43.18 43.19 43.20 43.21 43.22 43.23 Xie, Ji-Wei (2012), "Transit Timing Variation of Near-Resonance Planetary Pairs: Confirmation of 12 Multiple-Planet Systems", The Astrophysical Journal Supplement Series 208 (2): 22, doi:10.1088/0067-0049/208/2/22
44. ↑ 44.00 44.01 44.02 44.03 44.04 44.05 44.06 44.07 44.08 44.09 44.10 44.11 44.12 44.13 44.14 44.15 44.16 44.17 44.18 44.19 44.20 44.21 44.22 44.23 44.24 44.25 44.26 Steffen, Jason H.; Fabrycky, Daniel C.; Agol, Eric; Ford, Eric B.; Morehead, Robert C.; Cochran, William D.; Lissauer, Jack J.; Adams, Elisabeth R. et al. (2012), "Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability", Monthly Notices of the Royal Astronomical Society 428 (2): 1077–1087, doi:10.1093/mnras/sts090
45. ↑ Kostov, V. B.; McCullough, P. R.; Hinse, T. C.; Tsvetanov, Z. I.; Hébrard, G.; Díaz, R. F.; Deleuil, M.; Valenti, J. A. (2013-01-01). "A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the Two Transiting Planets in the Kepler-47 System" (in en). The Astrophysical Journal 770 (1): 52. doi:10.1088/0004-637X/770/1/52. ISSN 0004-637X. Bibcode: 2013ApJ...770...52K.
46. ↑ 46.0 46.1 46.2 46.3 Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard et al. (2014), "Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems", The Astrophysical Journal 784 (1): 45, doi:10.1088/0004-637X/784/1/45, Bibcode: 2014ApJ...784...45R
47. ↑ 47.0 47.1 Yang, Ming; Liu, Hui-Gen; Zhang, Hui; Yang, Jia-Yi; Zhou, Ji-Lin (2013), "Eight Planets in Four Multi-Planet Systems Via Transit Timing Variations in 1350 Days", The Astrophysical Journal 778 (2): 110, doi:10.1088/0004-637X/778/2/110, Bibcode: 2013ApJ...778..110Y
48. ↑ Yee, J. C. et al. (2012), "MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS", The Astrophysical Journal 755 (2): 102, doi:10.1088/0004-637X/755/2/102
49. ↑ Street, R. A. et al. (2012), "Moa-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary", The Astrophysical Journal 763: 67, doi:10.1088/0004-637X/763/1/67
50. ↑ Bachelet, E.; Shin, I.-G.; Han, C.; Fouqué, P.; Gould, A.; Menzies, J. W.; Beaulieu, J.-P.; Bennett, D. P. et al. (2012). "MOA-2010-BLG-477Lb: Constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light". The Astrophysical Journal 754 (1): 73. doi:10.1088/0004-637X/754/1/73. Bibcode: 2012ApJ...754...73B.
51. ↑ Blackman, J. W.; Beaulieu, J. P.; Bennett, D. P.; Danielski, C.; Alard, C.; Cole, A. A.; Vandorou, A.; Ranc, C. et al. (2021), "A Jovian analogue orbiting a white dwarf star", Nature 598 (7880): 272–275, doi:10.1038/s41586-021-03869-6, PMID 34646001, Bibcode: 2021Natur.598..272B
52. ↑ Bennett, D. P.; Sumi, T.; Bond, I. A.; Kamiya, K.; Abe, F.; Botzler, C. S.; Fukui, A.; Furusawa, K. et al. (2012), "Planetary and Other Short Binary Microlensing Events from the Moa Short-Event Analysis", The Astrophysical Journal 757 (2): 119, doi:10.1088/0004-637X/757/2/119, Bibcode: 2012ApJ...757..119B
53. ↑ 53.0 53.1 Han, C. et al. (2012), "THE SECOND MULTIPLE-PLANET SYSTEM DISCOVERED BY MICROLENSING: OGLE-2012-BLG-0026Lb, c—A PAIR OF JOVIAN PLANETS BEYOND THE SNOW LINE", The Astrophysical Journal 762 (2): L28, doi:10.1088/2041-8205/762/2/L28
54. ↑ 54.0 54.1 Quinn, Samuel N.; White, Russel J.; Latham, David W.; Buchhave, Lars A.; Cantrell, Justin R.; Dahm, Scott E.; Fűrész, Gabor; Szentgyorgyi, Andrew H. et al. (2012). "TWO "b"s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER". The Astrophysical Journal 756 (2): L33. doi:10.1088/2041-8205/756/2/L33. Bibcode: 2012ApJ...756L..33Q.
55. ↑ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P. et al. (2021), Two circumbinary planets in RR Cae eclipsing binary system
56. ↑ Qian, S. B.; Liu, L.; Zhu, L. Y.; Dai, Z. B.; Fernández Lajús, E.; Baume, G. L. (2012). "A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR Cae". Monthly Notices of the Royal Astronomical Society: Letters 422 (1): L24–L27. doi:10.1111/j.1745-3933.2012.01228.x. Bibcode: 2012MNRAS.422L..24Q.
57. ↑ 57.0 57.1 Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A et al. (2013). "Signals embedded in the radial velocity noise". Astronomy & Astrophysics 551: A79. doi:10.1051/0004-6361/201220509. Bibcode: 2012yCat..35510079T.
58. ↑ 58.0 58.1 Lendl, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lister, T. A. et al. (2012), "WASP-42 b and WASP-49 b: Two new transiting sub-Jupiters", Astronomy & Astrophysics 544: A72, doi:10.1051/0004-6361/201219585, Bibcode: 2012A&A...544A..72L
59. ↑ 59.0 59.1 59.2 59.3 59.4 59.5 59.6 Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Jehin, E.; Lendl, M. et al. (2012), "Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b and WASP-67b", Monthly Notices of the Royal Astronomical Society 426 (1): 739–750, doi:10.1111/j.1365-2966.2012.21780.x, Bibcode: 2012MNRAS.426..739H
60. ↑ 60.0 60.1 60.2 60.3 Hébrard, G. et al. (2012), "WASP-52b, WASP-58b, WASP-59b, and WASP-60b: Four new transiting close-in giant planets", Astronomy & Astrophysics 549: A134, doi:10.1051/0004-6361/201220363
61. ↑ 61.0 61.1 61.2 Faedi, F. (2013). "WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP". Astronomy & Astrophysics 551: A73. doi:10.1051/0004-6361/201220520. Bibcode: 2013A&A...551A..73F.
62. ↑ 62.0 62.1 Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Hellier, C.; Jehin, E.; Lendl, M. et al. (2012), "WASP-64 b and WASP-72 b: Two new transiting highly irradiated giant planets", Astronomy & Astrophysics 552: A82, doi:10.1051/0004-6361/201220561
63. ↑ Smith, A. M. S.; Anderson, D. R.; Bouchy, F.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hébrard, G. et al. (2013), "WASP-71b: A bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star", Astronomy & Astrophysics 552: A120, doi:10.1051/0004-6361/201220727, Bibcode: 2013A&A...552A.120S
64. ↑ Maxted, P. F. L.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2012), "WASP-77 Ab: A Transiting Hot Jupiter Planet in a Wide Binary System1", Publications of the Astronomical Society of the Pacific 125 (923): 48–55, doi:10.1086/669231
65. ↑ 65.0 65.1 Smalley, B.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2012), "WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus", Astronomy & Astrophysics 547: A61, doi:10.1051/0004-6361/201219731, Bibcode: 2012A&A...547A..61S
66. ↑ Liu, Michael C.; Dupuy, Trent J.; Bowler, Brendan P.; Leggett, S. K.; Best, William M. J. (2012). "Two Extraordinary Substellar Binaries at the T/Y Transition and the Y-band Fluxes of the Coolest Brown Dwarfs". The Astrophysical Journal 758 (1): 57. doi:10.1088/0004-637X/758/1/57. Bibcode: 2012ApJ...758...57L.
67. ↑ The first planet detected in the WTS: An inflated hot Jupiter in a 3.35d orbit around a late F star

* 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
* 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
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* Exozodiacal dust
* Extraterrestrial materials
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* Giant-impact hypothesis
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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
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* 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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