| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
|---|
| HIP 77900 b | HD 142250 | 2024 | — | 21,00 MJ |
| MOA-2016-BLG-526 b | — | 2024 | microlente gravitacional | 6,93 MJ |
| HIP 81208 C b | HD 149274C | 2023 | — | 14,80 MJ |
| KMT-2016-BLG-1751 | KMT-2016-BLG-1751 | 2023 | microlente gravitacional | 1,20 MJ |
| KMT-2019-BLG-1216L b | EWS 2019-BLG-1033 | 2023 | microlente gravitacional | 0,09 MJ |
| KMT-2019-BLG-2783L b | — | 2023 | microlente gravitacional | 1,16 MJ |
| KMT-2021-BLG-1110 b | KMT-2021-BLG-1110 | 2023 | microlente gravitacional | 55,00 MJ |
| KMT-2021-BLG-1150L b | — | 2023 | microlente gravitacional | 0,88 MJ |
| KMT-2021-BLG-2010 b | KMT-2021-BLG-2010 | 2023 | microlente gravitacional | 1,07 MJ |
| KMT-2022-BLG-0371 b | KMT-2022-BLG-0371 | 2023 | microlente gravitacional | 0,26 MJ |
| MOA-2020-BLG-208 b | — | 2023 | microlente gravitacional | 0,22 MJ |
| MOA-9y-770 | — | 2023 | microlente gravitacional | 0,07 MJ |
| OGLE-2016-BLG-1635 b | OGLE-2016-BLG-1635 | 2023 | microlente gravitacional | 11,49 MJ |
| OGLE-2016-BLG-1850 b | OGLE BLG535.21 11771 | 2023 | microlente gravitacional | 0,03 MJ |
| OGLE-2017-BLG- 0448 b | OGLE-2017-BLG-0448 | 2023 | microlente gravitacional | 7,30 MJ |
| OGLE-2019-BLG-0825 b | OGLE-2019-BLG-0825 | 2023 | microlente gravitacional | 50,00 MJ |
| DANCe J15481655-2307430 | — | 2022 | — | 12,00 MJ |
| DANCe J15582895-2530319 | — | 2022 | — | 7,00 MJ |
| DANCe J16041234-2127472 | — | 2022 | — | 10,00 MJ |
| DANCe J16053908-2403330 | — | 2022 | — | 11,00 MJ |
| DANCe J16064467-2033428 | — | 2022 | — | 12,00 MJ |
| DANCe J16064553-2121595 | — | 2022 | — | 10,00 MJ |
| DANCe J16081299-2304316 | — | 2022 | — | 4,00 MJ |
| DANCe J16091010-1930376 | — | 2022 | — | 8,00 MJ |
| DANCe J16123953-2614510 | — | 2022 | — | 12,00 MJ |
| DANCe J16134589-2442310 | — | 2022 | — | 10,00 MJ |
| DANCe J16135217-2443562 | — | 2022 | — | 10,00 MJ |
| DANCe J16140756-2211524 | — | 2022 | — | 11,00 MJ |
| DANCe J16393029-2454135 | — | 2022 | — | 11,00 MJ |
| HD 149790 b | HD 149790 | 2022 | espectroscopia Dopple | 42,00 MJ |
| HD 156098 b | HD 156098 | 2022 | espectroscopia Dopple | 0,05 MJ |
| HD 156098 c | HD 156098 | 2022 | espectroscopia Dopple | 5,23 MJ |
| K2-365 b | TYC 6199-1529-1 | 2022 | — | 0,03 MJ |
| K2-366 b | EPIC 205111664 | 2022 | — | 0,02 MJ |
| KMT-2017-BLG-0673L b | — | 2022 | microlente gravitacional | 3,67 MJ |
| KMT-2018-BLG-1988L b | KMT-2018-BLG-1988 | 2022 | microlente gravitacional | 0,02 MJ |
| KMT-2018-BLG-2004 b | KMT-2018-BLG-2004 | 2022 | microlente gravitacional | 0,27 MJ |
| KMT-2018-BLG-2718 b | KMT-2018-BLG-2718 | 2022 | microlente gravitacional | 16,00 MJ |
| KMT-2021-BLG-0171L b | KMT-2021-BLG-0171 | 2022 | microlente gravitacional | 0,04 MJ |
| KMT-2021-BLG-0320 b | KMT-2021-BLG-0320 | 2022 | microlente gravitacional | 0,10 MJ |
| KMT-2021-BLG-0712 b | KMT-2021-BLG-0712 | 2022 | microlente gravitacional | 0,12 MJ |
| KMT-2021-BLG-1077L b | KMT-2021-BLG-1077 | 2022 | microlente gravitacional | 0,22 MJ |
| KMT-2021-BLG-1077L c | KMT-2021-BLG-1077 | 2022 | microlente gravitacional | 0,25 MJ |
| KMT-2021-BLG-1554 b | KMT-2021-BLG-1554 | 2022 | microlente gravitacional | 0,12 MJ |
| Mu2 Sco b | Mu2 Scorpii | 2022 | — | 14,40 MJ |
| OGLE-2014-BLG-0319 b | EWS 2014-BLG-319 | 2022 | microlente gravitacional | 0,57 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 |