| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| KMT-2023-BLG-0416 b | KMT-2023-BLG-0416 | 2024 | microlente gravitacional | 0,04 MJ |
| KMT-2023-BLG-0469 b | KMT-2023-BLG-0469 | 2024 | microlente gravitacional | 0,12 MJ |
| KMT-2023-BLG-0735 b | KMT-2023-BLG-0735 | 2024 | microlente gravitacional | 0,12 MJ |
| KMT-2023-BLG-1454 b | KMT-2023-BLG-1454 | 2024 | microlente gravitacional | 0,63 MJ |
| KMT-2023-BLG-1866L b | — | 2024 | microlente gravitacional | 0,01 MJ |
| MOA-2022-BLG-563 b | — | 2024 | microlente gravitacional | 0,40 MJ |
| OGLE-2014-BLG-0221L b | MOA 2014-BLG-69 | 2024 | microlente gravitacional | 4,35 MJ |
| OGLE-2016-BLG-1598 b | KMT-2016-BLG-0696 | 2024 | microlente gravitacional | 5,91 MJ |
| OGLE-2016-BLG-1800 b | KMT-2016-BLG-0781 | 2024 | microlente gravitacional | 2,59 MJ |
| OGLE-2017-BLG-1237 b | KMT-2017-BLG-0422 | 2024 | microlente gravitacional | 3,80 MJ |
| OGLE-2017-BLG-1275 b | KMT-2017-BLG-0314 | 2024 | microlente gravitacional | 5,90 MJ |
| OGLE-2023-BLG-0836L b | KMT-2023-BLG-1144 | 2024 | microlente gravitacional | 4,36 MJ |
| HD 165131 b | HD 165131 | 2023 | espectroscopia Dopple | 18,70 MJ |
| KMT-2016-BLG-0625 b | KMT-2016-BLG-0625 | 2023 | microlente gravitacional | 0,05 MJ |
| KMT-2016-BLG-1105 b | KMT-2016-BLG-1105 | 2023 | microlente gravitacional | 0,00 MJ |
| KMT-2017-BLG-0428 b | KMT-2017-BLG-0428 | 2023 | microlente gravitacional | 0,02 MJ |
| KMT-2018-BLG-0885 b | KMT-2018-BLG-0885 | 2023 | microlente gravitacional | 31,00 MJ |
| KMT-2019-BLG-0297 b | KMT-2019-BLG-0297 | 2023 | microlente gravitacional | 19,00 MJ |
| KMT-2019-BLG-1806 | EWS 2019-BLG-1250 | 2023 | microlente gravitacional | 0,01 MJ |
| KMT-2021-BLG-0588 b | KMT-2021-BLG-0588 | 2023 | microlente gravitacional | 53,00 MJ |
| KMT-2021-BLG-1547L b | — | 2023 | microlente gravitacional | 1,47 MJ |
| KMT-2021-BLG-1643 b | KMT-2021-BLG-1643 | 2023 | microlente gravitacional | 61,00 MJ |
| KMT-2021-BLG-1770 b | KMT-2021-BLG-1770 | 2023 | microlente gravitacional | 21,00 MJ |
| KMT-2021-BLG-2478 b | KMT-2021-BLG-2478 | 2023 | microlente gravitacional | 0,91 MJ |
| KMT-2022-BLG-0440L b | — | 2023 | microlente gravitacional | 0,05 MJ |
| KMT-2022-BLG-0475 b | KMT-2022-BLG-0475 | 2023 | microlente gravitacional | 0,08 MJ |
| KMT-2022-BLG-1480 b | KMT-2022-BLG-1480 | 2023 | microlente gravitacional | 0,08 MJ |
| KMT-2023-BLG-1431L b | — | 2023 | microlente gravitacional | 13,50 MJ |
| MOA-2016-BLG-532 b | OGLE-2016-BLG-1749 | 2023 | microlente gravitacional | 0,41 MJ |
| MOA-2019-BLG-421 b | — | 2023 | microlente gravitacional | 0,54 MJ |
| MOA-2022-BLG-249L b | — | 2023 | microlente gravitacional | 0,02 MJ |
| MOA-9y-5919 | — | 2023 | microlente gravitacional | 0,00 MJ |
| OGLE-2017-BLG-0640 b | KMT-2017-BLG-1726 | 2023 | microlente gravitacional | 1,62 MJ |
| OGLE-2019-BLG-1180L b | OGLE BLG504.22 34811 | 2023 | microlente gravitacional | 1,75 MJ |
| TOI-2194 b | HD 188474 | 2023 | — | 0,01 MJ |
| HD 168863 b | HD 168863 | 2022 | espectroscopia Dopple | 6,78 MJ |
| HD 188641 b | HD 188641 | 2022 | espectroscopia Dopple | 29,36 MJ |
| K2-2016-BLG-0005L b | — | 2022 | microlente gravitacional | 1,10 MJ |
| K2-379 b | K2-379 | 2022 | — | 0,02 MJ |
| K2-380 b | K2-380N | 2022 | — | 0,03 MJ |
| K2-381 b | K2-381 | 2022 | — | — |
| K2-381 c | K2-381 | 2022 | — | — |
| K2-382 b | K2-382 | 2022 | — | 0,02 MJ |
| K2-383 b | K2-383 | 2022 | — | 0,01 MJ |
| KMT-2017-BLG-1194L b | KMT-2017-BLG-1194 | 2022 | microlente gravitacional | 0,01 MJ |
| KMT-2018-BLG-2119 b | — | 2022 | microlente gravitacional | 12,00 MJ |
| KMT-2018-BLG-2602 b | KMT-2018-BLG-2602 | 2022 | microlente gravitacional | 1,15 MJ |
| KMT-2019-BLG-0414L b | KMT-2019-BLG-0414 | 2022 | microlente gravitacional | 2,14 MJ |