| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| OGLE-2018-BLG-0360 | OGLE-2018-BLG-0360 | 2022 | microlente gravitacional | 45,00 MJ |
| OGLE-2018-BLG-1126 b | OGLE-2018-BLG-1126 | 2022 | microlente gravitacional | 0,06 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 |
| KMT-2018-BLG-1976L b | KMT-2018-BLG-1976 | 2021 | microlente gravitacional | 2,22 MJ |
| KMT-2019-BLG-0371 b | EWS 2019-BLG-505 | 2021 | microlente gravitacional | 16,50 MJ |
| OGLE-2018-BLG-0506 b | EWS 2018-BLG-506 | 2021 | microlente gravitacional | 0,05 MJ |
| OGLE-2018-BLG-0962 | EWS 2018-BLG-962 | 2021 | microlente gravitacional | 1,34 MJ |
| OGLE-2018-BLG-0977 b | EWS 2018-BLG-977 | 2021 | microlente gravitacional | 0,02 MJ |
| SMSS J1606-1000 b | SMSS J160639.78-100010.7 | 2021 | — | 60,00 MJ |
| 17 Scorpii b | Chi Scorpii | 2020 | espectroscopia Dopple | 4,32 MJ |
| EWS 2018-BLG-0677b | EWS 2018-BLG-677 | 2020 | microlente gravitacional | 0,01 MJ |
| KMT-2016-BLG-1836L b | KMT-2016-BLG-1836 | 2020 | microlente gravitacional | 2,30 MJ |
| KMT-2018-BLG-0748L b | KMT-2018-BLG-0748 | 2020 | microlente gravitacional | 0,19 MJ |
| KMT-2018-BLG-1292L b | KMT-2018-BLG-1292 | 2020 | microlente gravitacional | 4,42 MJ |
| OGLE-2017-BLG-0604 b | EWS 2017-BLG-604 | 2020 | microlente gravitacional | 0,51 MJ |
| OGLE-2017-BLG-1375 b | EWS 2017-BLG-1375 | 2020 | microlente gravitacional | 13,27 MJ |
| HIP 79098 (AB) b | HIP 79098 | 2019 | — | 20,50 MJ |
| MOA-2016-BLG-231 b | EWS 2016-BLG-864 | 2019 | microlente gravitacional | 9,00 MJ |
| OGLE-2016-BLG-1227L b | KMT-2016-BLG-1089 | 2019 | microlente gravitacional | 4,98 MJ |
| OGLE-2019-BLG-0249L b | EWS 2019-BLG-249 | 2019 | microlente gravitacional | 6,95 MJ |
| V921 Scorpii b | CD-42 11721 | 2019 | — | 60,00 MJ |
| EWS 2014-BLG-1722b | EWS 2014-BLG-1722 | 2018 | microlente gravitacional | 0,17 MJ |
| EWS 2014-BLG-1722c | EWS 2014-BLG-1722 | 2018 | microlente gravitacional | 0,26 MJ |
| EWS 2017-BLG-0373b | EWS 2017-BLG-373 | 2018 | microlente gravitacional | 0,40 MJ |
| EWS 2017-BLG-1434b | EWS 2017-BLG-1434 | 2018 | microlente gravitacional | 0,01 MJ |
| KMT-2017-BLG-1146L b | KMT-2017-BLG-1146 | 2018 | microlente gravitacional | 0,71 MJ |
| MOA 2017-BLG-209L b | MOA 2017-BLG-209 | 2018 | microlente gravitacional | 0,03 MJ |
| OGLE 2017-BLG-0560L b | — | 2018 | microlente gravitacional | 1,90 MJ |
| OGLE-2014-BLG-1186L b | OGLE-2014-BLG-1186 | 2018 | microlente gravitacional | 0,14 MJ |
| AS 205 A b | AS 205 N | 2017 | espectroscopia Dopple | 19,25 MJ |
| HD 147873 c | HD 147873 | 2017 | espectroscopia Dopple | 2,30 MJ |
| MOA 2013-BLG-618L b | MOA 2013-BLG-618 | 2017 | microlente gravitacional | 0,64 MJ |
| MOA-2012-BLG-505L b | MOA 2012-BLG-505 | 2017 | microlente gravitacional | 0,02 MJ |
| OGLE-2016-BLG-1195Lb | EWS 2016-BLG-1195 | 2017 | microlente gravitacional | 0,02 MJ |
| EPIC 2037 c | EPIC 203771098 | 2016 | — | 0,05 MJ |
| HD 147873 Ab | HD 147873 | 2016 | espectroscopia Dopple | 5,14 MJ |
| K2-31 Ab | K2-31 | 2016 | — | 1,77 MJ |
| K2-33 b | K2-33 | 2016 | — | 3,70 MJ |
| K2-37 b | K2-37 | 2016 | — | — |
| K2-37 c | K2-37 | 2016 | — | — |
| K2-37 d | K2-37 | 2016 | — | — |
| K2-38 b | K2-38 | 2016 | — | 0,02 MJ |
| K2-38 c | K2-38 | 2016 | — | 0,03 MJ |
| K2-52 b | K2-52 | 2016 | — | 0,40 MJ |
| K2-53 b | K2-53 | 2016 | — | 0,03 MJ |
| MOA 2014-BLG-175L b | MOA 2014-BLG-175 | 2016 | microlente gravitacional | 3,68 MJ |
| OGLE 2016-BLG-596b | EWS 2016-BLG-596 | 2016 | microlente gravitacional | 12,20 MJ |