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Exoplanetas
6.229 exoplanetas
| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| KMT-2016-BLG-2142L b | KMT-2016-BLG-2142 | 2018 | microlente gravitacional | 15,49 MJ |
| KMT-2017-BLG-0165L b | KMT-2017-BLG-0165 | 2018 | microlente gravitacional | 0,11 MJ |
| KMT-2017-BLG-1038L b | KMT-2017-BLG-1038 | 2018 | microlente gravitacional | 2,00 MJ |
| KMT-2017-BLG-1146L b | KMT-2017-BLG-1146 | 2018 | microlente gravitacional | 0,71 MJ |
| KOI-1089.02 | TYC 1401-984-1 | 2018 | — | 0,64 MJ |
| KPS-1b | KPS-1 | 2018 | — | 1,09 MJ |
| L 98-59 d | L 98-59 | 2018 | — | 0,01 MJ |
| LHS 1610 b | Wolf 227 | 2018 | espectroscopia Dopple | 52,00 MJ |
| MOA 2011-BLG-133L b | MOA 2011-BLG-133 | 2018 | microlente gravitacional | 0,18 MJ |
| MOA 2011-BLG-291L b | MOA 2011-BLG-291 | 2018 | microlente gravitacional | 0,04 MJ |
| MOA 2015-BLG-337L a | — | 2018 | microlente gravitacional | 9,80 MJ |
| MOA 2015-BLG-337L b | MOA 2015-BLG-337L a | 2018 | microlente gravitacional | 18,00 MJ |
| MOA 2015-BLG-379L b | MOA 2015-BLG-379 | 2018 | microlente gravitacional | 0,06 MJ |
| MOA 2016-BLG-319L b | MOA 2016-BLG-319 | 2018 | microlente gravitacional | 0,65 MJ |
| MOA 2017-BLG-209L b | MOA 2017-BLG-209 | 2018 | microlente gravitacional | 0,03 MJ |
| MOA-2010-BLG-117L b | MOA 2010-BLG-117 | 2018 | microlente gravitacional | 0,54 MJ |
| NAME DE CVn b | DE Canum Venaticorum | 2018 | — | 11,00 MJ |
| NGTS-1b | NGTS-1 | 2018 | espectroscopia Dopple | 0,81 MJ |
| NGTS-2b | NGTS-2 | 2018 | — | 0,74 MJ |
| NGTS-3 A b | NGTS-3 | 2018 | — | 2,38 MJ |
| NGTS-4b | NGTS-4 | 2018 | — | 0,06 MJ |
| OGLE 2017-BLG-0560L b | — | 2018 | microlente gravitacional | 1,90 MJ |
| OGLE-2012-BLG-1323L | — | 2018 | microlente gravitacional | 0,01 MJ |
| OGLE-2014-BLG-1186L b | OGLE-2014-BLG-1186 | 2018 | microlente gravitacional | 0,14 MJ |
| OGLE-2016-BLG-1266L b | — | 2018 | microlente gravitacional | 11,90 MJ |
| OGLE-2016-BLG-1540L | — | 2018 | microlente gravitacional | — |
| OGLE-2017-BLG-1522Lb | EWS 2017-BLG-1522 | 2018 | microlente gravitacional | 0,75 MJ |
| PDS 70 b | PDS 70 | 2018 | — | 3,00 MJ |
| Pi Mensae c | Pi Mensae | 2018 | — | 0,01 MJ |
| PSR J2322-2650 b | PSR J2322−2650 | 2018 | — | 0,79 MJ |
| Ross 128b | Ross 128 | 2018 | espectroscopia Dopple | 0,00 MJ |
| SDSS J1411+2009 b | SDSS J141126.20+200911.1 | 2018 | — | 50,00 MJ |
| TCP J050742+244755 b | Kojima-1L | 2018 | microlente gravitacional | 0,06 MJ |
| TOI-203 b | UPM J0252-6741 | 2018 | — | — |
| UKIRT 2017-BLG-001b | UKIRT 2017-BLG-001 | 2018 | microlente gravitacional | 1,28 MJ |
| WASP-128 b | WASP-128 | 2018 | — | 37,19 MJ |
| WASP-134 c | TYC 552-1060-1 | 2018 | espectroscopia Dopple | 0,70 MJ |
| WASP-134b | TYC 552-1060-1 | 2018 | — | 1,41 MJ |
| WASP-137 b | WASP-137 | 2018 | — | 0,68 MJ |
| WASP-144b | WASP-144 | 2018 | — | 0,44 MJ |
| WASP-146 b | WASP-146 | 2018 | — | 1,11 MJ |
| WASP-160Bb | WASP-160B | 2018 | — | 0,28 MJ |
| WASP-163b | WASP-163 | 2018 | — | 1,87 MJ |
| WASP-164b | WASP-164 | 2018 | — | 2,13 MJ |
| WASP-166b | WASP-166 | 2018 | — | 0,10 MJ |
| WASP-170b | WASP-170 | 2018 | — | 1,60 MJ |
| WASP-174b | WASP-174 | 2018 | — | 0,33 MJ |
| WASP-189b | WASP-189 | 2018 | — | 1,99 MJ |