| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
| HD 167677 b | HD 167677 | 2023 | espectroscopia Dopple | 2,85 MJ |
| NN Ser e | NN Serpentis | 2023 | — | 9,43 MJ |
| HD 167768 b | HD 167768 | 2022 | espectroscopia Dopple | 0,85 MJ |
| QZ Ser b | QZ Serpentis | 2022 | — | 0,63 MJ |
| Ross 508 b | Ross 508 | 2022 | espectroscopia Dopple | 0,01 MJ |
| Gliese 740 b | HD 176029 | 2021 | espectroscopia Dopple | 0,01 MJ |
| HD 136925 b | HD 136925 | 2021 | espectroscopia Dopple | 0,84 MJ |
| HIP 77257 b | Lambda Serpentis | 2021 | espectroscopia Dopple | 0,04 MJ |
| SDSS 1604+1000 b | SDSS J160429.12+100002.2 | 2020 | — | 50,00 MJ |
| CoRoT-28 b | CoRoT-28 | 2015 | — | 0,48 MJ |
| BD+15°2940 b | BD+15°2940 | 2013 | espectroscopia Dopple | 1,11 MJ |
| HAT-P-45 b | HAT-P-45 | 2013 | — | 0,86 MJ |
| HAT-P-46 b | HAT-P-46 | 2013 | — | 0,49 MJ |
| HAT-P-46 c | HAT-P-46 | 2013 | — | 2,00 MJ |
| Omega Serpentis b | Omega Serpentis | 2013 | espectroscopia Dopple | 1,70 MJ |
| CoRoT-23 b | COROT-23 | 2012 | — | 3,09 MJ |
| COROT-27 b | CoRoT-27 | 2012 | — | 10,30 MJ |
| HD 175679 b | HD 175679 | 2012 | espectroscopia Dopple | 59,90 MJ |
| COROT-22b | CoRoT-22 | 2011 | — | 0,04 MJ |
| HD 142245 b | HD 142245 | 2011 | espectroscopia Dopple | 1,90 MJ |
| PSR J1719-1438 b | PSR J1719-1438 | 2011 | — | 1,20 MJ |
| CoRoT-11 b | COROT-11 | 2010 | — | 2,62 MJ |
| COROT-9b | CoRoT-9 | 2010 | — | 0,84 MJ |
| NN Ser c | NN Serpentis | 2010 | — | 7,33 MJ |
| NN Serpentis d | NN Serpentis | 2010 | — | 2,30 MJ |
| PSR B1802-07 b | PSR J1802-07 | 2009 | — | 10,00 MJ |
| PSR J1518+0204C b | PSR J1518+0204C | 2009 | — | 37,23 MJ |
| HD 175541 b | HD 175541 | 2007 | espectroscopia Dopple | 0,61 MJ |
| HD 137510 b | HD 137510 | 2004 | espectroscopia Dopple | 27,30 MJ |
| HD 136118 b | HD 136118 | 2002 | espectroscopia Dopple | 16,50 MJ |
| HD 168746 b | Alasia | 2002 | espectroscopia Dopple | 0,23 MJ |
| HD 168443 b | HD 168443 | 1998 | espectroscopia Dopple | 7,66 MJ |