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Exoplanetas
6.229 exoplanetas
| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| KMT-2021-BLG-1689L b | — | 2022 | microlente gravitacional | 0,14 MJ |
| KMT-2021-BLG-1898 b | KMT-2021-BLG-1898 | 2022 | microlente gravitacional | 0,73 MJ |
| KMT-2021-BLG-1931 b | KMT-2021-BLG-1391 | 2022 | microlente gravitacional | 0,01 MJ |
| KMT-2021-BLG-2294 b | KMT-2021-BLG-2294 | 2022 | microlente gravitacional | 0,07 MJ |
| KOI-7913 b | KIC 8873450 | 2022 | — | — |
| KOI-984 c | KOI-984 | 2022 | — | 0,08 MJ |
| Lalande 21185 d | Lalande 21185 | 2022 | — | 0,01 MJ |
| LHS 1678 c | TOI-696 | 2022 | — | 0,00 MJ |
| LP 890-9 b | LP 890-9 | 2022 | — | 0,04 MJ |
| LP 890-9 c | LP 890-9 | 2022 | — | 0,08 MJ |
| LTT 1445A d | BD-17 588A | 2022 | espectroscopia Dopple | 0,01 MJ |
| MAXI J1957+032 b | IGR J19566+0326 | 2022 | — | 17,00 MJ |
| MOA-2019-BLG-008L b | EWS 2019-BLG-11 | 2022 | microlente gravitacional | 25,00 MJ |
| MOA-2020-BLG-135 b | KMT-2020-BLG-0579 | 2022 | microlente gravitacional | 0,04 MJ |
| Mu2 Sco b | Mu2 Scorpii | 2022 | — | 14,40 MJ |
| NGTS-11 c | UCAC2 26590993 | 2022 | — | — |
| NGTS-20 b | TYC 5871-345-1 | 2022 | — | 2,98 MJ |
| NGTS-21 b | UCAC3 110-455458 | 2022 | — | 2,36 MJ |
| NGTS-23 b | NGTS-23 | 2022 | — | 0,61 MJ |
| NGTS-24 b | NGTS-24 | 2022 | — | 0,52 MJ |
| NGTS-25 b | NGTS-25 | 2022 | — | 0,64 MJ |
| NSVS 11868841 c | NSVS 11868841 | 2022 | — | 47,00 MJ |
| OGLE-2014-BLG-0319 b | EWS 2014-BLG-319 | 2022 | microlente gravitacional | 0,57 MJ |
| OGLE-2016-BLG-0890 b | OGLE-2016-BLG-0890 | 2022 | microlente gravitacional | 38,00 MJ |
| OGLE-2016-BLG-1093L b | OGLE BLG508.23 93011 | 2022 | microlente gravitacional | 0,63 MJ |
| OGLE-2017-BLG-0614 b | OGLE-2017-BLG-0614 | 2022 | microlente gravitacional | 31,50 MJ |
| OGLE-2017-BLG-1038 b | — | 2022 | microlente gravitacional | 13,30 MJ |
| OGLE-2017-BLG-1806 b | EWS 2017-BLG-1806 | 2022 | microlente gravitacional | 0,01 MJ |
| OGLE-2018-BLG-0298 b | OGLE-2018-BLG-0298 | 2022 | microlente gravitacional | 0,14 MJ |
| OGLE-2018-BLG-0360 | OGLE-2018-BLG-0360 | 2022 | microlente gravitacional | 45,00 MJ |
| OGLE-2018-BLG-0799Lb | EWS 2018-BLG-799 | 2022 | microlente gravitacional | 0,26 MJ |
| OGLE-2018-BLG-0932 b | EWS 2018-BLG-932 | 2022 | microlente gravitacional | 0,89 MJ |
| OGLE-2018-BLG-1119Lb | OGLE-2018-BLG-1119 | 2022 | microlente gravitacional | 0,86 MJ |
| OGLE-2018-BLG-1126 b | OGLE-2018-BLG-1126 | 2022 | microlente gravitacional | 0,06 MJ |
| OGLE-2018-BLG-1212 b | OGLE-2018-BLG-1212 | 2022 | microlente gravitacional | 0,19 MJ |
| OGLE-2018-BLG-1367 b | OGLE-2018-BLG-1367 | 2022 | microlente gravitacional | 0,99 MJ |
| OGLE-2018-BLG-1489 b | OGLE-2018-BLG-1489 | 2022 | microlente gravitacional | 50,00 MJ |
| OGLE-2018-BLG-1544 b | OGLE-2018-BLG-1544 | 2022 | microlente gravitacional | 11,20 MJ |
| OGLE-2018-BLG-1647 b | OGLE-2018-BLG-1647 | 2022 | microlente gravitacional | 0,97 MJ |
| OGLE-2019-BLG-0362 b | OGLE-2019-BLG-0362 | 2022 | microlente gravitacional | 3,26 MJ |
| OGLE-2019-BLG-0468L c | EWS 2019-BLG-468 | 2022 | microlente gravitacional | 10,14 MJ |
| OGLE-2019-BLG-1470LAB b | — | 2022 | microlente gravitacional | 3,10 MJ |
| Pi Men d | Pi Mensae | 2022 | espectroscopia Dopple | 0,04 MJ |
| PSR J0952-0607 b | PSR J0952–0607 | 2022 | — | 32,00 MJ |
| PSR J1301+0833 b | PSR J1301+0833 | 2022 | — | 36,00 MJ |
| PSR J1653-0158 b | 3EG J1652-0223 | 2022 | — | 14,00 MJ |
| PSR J1748-2021H | PSR J1748-2021H | 2022 | — | 7,54 MJ |
| QZ Ser b | QZ Serpentis | 2022 | — | 0,63 MJ |