| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| Estrela de Barnard b | Estrela de Barnard | 2024 | espectroscopia Dopple | 0,01 MJ |
| KMT-2016-BLG-2321 b | — | 2024 | microlente gravitacional | 3,58 MJ |
| KMT-2023-BLG-1642 b | KMT-2023-BLG-1642 | 2024 | microlente gravitacional | 1,08 MJ |
| M62H b | PSR J1701-3006H | 2024 | — | 2,47 MJ |
| KMT-2017-BLG-1003 b | KMT-2017-BLG-1003 | 2023 | microlente gravitacional | 0,02 MJ |
| KMT-2019-BLG-0298 b | EWS 2019-BLG-445 | 2023 | microlente gravitacional | 1,81 MJ |
| KMT-2019-BLG-0298L b | — | 2023 | microlente gravitacional | 1,81 MJ |
| KMT-2019-BLG-0335 b | KMT-2019-BLG-0335 | 2023 | microlente gravitacional | 20,00 MJ |
| KMT-2021-BLG-0909 b | KMT-2021-BLG-0909 | 2023 | microlente gravitacional | 1,26 MJ |
| KMT-2022-BLG-1013 b | KMT-2022-BLG-1013 | 2023 | microlente gravitacional | 0,31 MJ |
| OGLE-2019-BLG-0679L b | EWS 2019-BLG-679 | 2023 | microlente gravitacional | 3,34 MJ |
| PSR J1720-0534 b | — | 2023 | — | 31,50 MJ |
| BLG-1691L b | OGLE BLG654.31 22909 | 2022 | microlente gravitacional | 0,05 MJ |
| CoRoT-36 b | UCAC2 34324554 | 2022 | — | 0,68 MJ |
| DANCe J16255679-2113354 | — | 2022 | — | 12,00 MJ |
| HD 149086 Ab | HD 149806 | 2022 | — | 12,60 MJ |
| HD 149806 b | HD 149806 | 2022 | espectroscopia Dopple | 12,60 MJ |
| HD 151450 b | HD 151450 | 2022 | espectroscopia Dopple | 0,12 MJ |
| HD 151450 c | HD 151450 | 2022 | espectroscopia Dopple | 5,15 MJ |
| KMT-2018-BLG-0030 b | KMT-2018-BLG-0030 | 2022 | microlente gravitacional | 1,45 MJ |
| KMT-2018-BLG-0087 b | KMT-2018-BLG-0087 | 2022 | microlente gravitacional | 0,32 MJ |
| KMT-2018-BLG-0247 b | EWS 2018-BLG-1219 | 2022 | microlente gravitacional | 2,04 MJ |
| KMT-2021-BLG-1105 b | KMT-2021-BLG-1105 | 2022 | microlente gravitacional | 1,28 MJ |
| KMT-2021-BLG-1372 b | KMT-2021-BLG-1372 | 2022 | microlente gravitacional | 0,20 MJ |
| KMT-2021-BLG-1898 b | KMT-2021-BLG-1898 | 2022 | microlente gravitacional | 0,73 MJ |
| OGLE-2016-BLG-0890 b | OGLE-2016-BLG-0890 | 2022 | microlente gravitacional | 38,00 MJ |
| OGLE-2018-BLG-0298 b | OGLE-2018-BLG-0298 | 2022 | microlente gravitacional | 0,14 MJ |
| OGLE-2019-BLG-0362 b | OGLE-2019-BLG-0362 | 2022 | microlente gravitacional | 3,26 MJ |
| PSR J1653-0158 b | 3EG J1652-0223 | 2022 | — | 14,00 MJ |
| [BHB2007]-1 b | 2MASS J17110392-2722551 | 2021 | espectroscopia Dopple | 42,00 MJ |
| HAT-P-63 b | HAT-P-63 | 2021 | — | 0,61 MJ |
| HD 154088 b | HD 154088 | 2021 | espectroscopia Dopple | 0,02 MJ |
| HD 155193 b | HD 155193 | 2021 | espectroscopia Dopple | 0,75 MJ |
| KMT-2017-BLG-2509 b | KMT-2017-BLG-2509 | 2021 | microlente gravitacional | 2,09 MJ |
| OGLE-2017-BLG-0114 b | — | 2021 | microlente gravitacional | — |
| OGLE-2017-BLG-1099 b | EWS 2017-BLG-1099 | 2021 | microlente gravitacional | 3,02 MJ |
| OGLE-2018-BLG-1428L b | EWS 2018-BLG-1428 | 2021 | microlente gravitacional | 0,77 MJ |
| OGLE-2019-BLG-0304 b | EWS 2019-BLG-304 | 2021 | microlente gravitacional | 0,51 MJ |
| TYC 0434-04538-1 b | TYC 434-4538-1 | 2021 | espectroscopia Dopple | — |
| CoRoT-30 b | CoRoT-30 | 2020 | — | 2,90 MJ |
| KMT-2016-BLG-2364 b | KMT-2016-BLG-2364 | 2020 | microlente gravitacional | 3,93 MJ |
| KMT-2017-BLG-2820L | — | 2020 | microlente gravitacional | — |
| KMT-2019-BLG-1339 b | EWS 2019-BLG-1019 | 2020 | microlente gravitacional | 12,20 MJ |
| Oph 98 b | CFHTWIR-Oph 98 A | 2020 | — | 7,80 MJ |
| DoAr 21 b | EPIC 203924493 | 2019 | Astrometria | 35,60 MJ |
| DoAr 21 c | EPIC 203924493 | 2019 | Astrometria | 44,00 MJ |
| K2-289 b | K2-289 | 2019 | — | 0,15 MJ |
| K2-32e | K2-32 | 2019 | — | 0,01 MJ |