This is thelist of 20extrasolar planets that weredetected by timing –– 8 bypulsar timing and 12 byvariable star timing, sorted by orbital periods. It works by detecting the changes in radio emissions from pulsars caused by the gravity of orbiting planets. Same thing works for variable stars, not by radio but light.
The most massive planet detected by timing isHW Virginis b, which masses 19.2 MJ; the least massive planet isPSR B1257+12 b, which masses 0.00007 MJ or 0.022 M🜨. The longest period of any planets detected by timing isPSR B1620-26 b, which is 36525 days or 100 years; the shortest period isSDSS J1228+1040 b, which is 0.0857 days.
There are 9 members ofmulti-planet systems, including three orbiting aroundPSR B1257+12.
| Planet | Mass (MJ) | Radius (RJ) | Period (d) | Semi-major axis (AU) | Eccentricity | Inclination (°) | Year of discovery |
|---|---|---|---|---|---|---|---|
| XTE J1807-294 b | 14.5 | 0.0278292 | 0.0020575 | 2005 | |||
| PSR J0636+5129 b | 8 | 0.067 | 0.18455 | 2016 | |||
| SDSS J1228+1040 b | 0.0009 | 0.0857 | 0.0034 | 2019 | |||
| PSR J1719-1438 b | ~ 1 | ~ 0.4 | 0.090706293 | 0.004 | < 0.06 | 2011 | |
| PSR J2241-5236 b | 12 | 0.1456722395 | 0.005989 | 0 | 2011 | ||
| PSR J2322-2650 b | 0.7949 | 0.322963997 | 0.0102 | 2017 | |||
| Draugr | 0.00007 | 25.262 | 0.19 | 0 | ~50 | 1994 | |
| Kepler-451d | 1.76 | 43 | 0.2 | 0 | 2022 | ||
| Poltergeist | 0.013 | 66.5419 | 0.36 | 0.0186 | 53 | 1992 | |
| Phobetor | 0.012 | 98.2114 | 0.46 | 0.0252 | 47 | 1992 | |
| Kepler-47d | 0.05984 | 0.6281 | 187.35 | 0.6992 | 0.024 | 90 | 2013 |
| TIC 172900988 b | 2.84 | 0.9874 | 188.763 | 0.867 | 0.089 | 2021 | |
| Kepler-451b | 1.86 | 406 | 0.9 | 0.33 | 2015 | ||
| PSR B0943+10 b | 2.8 | 730 | 1.8 | 2014 | |||
| V391 Pegasi b | 3.2 | 1170 | 1.7 | 0 | 2007 | ||
| DW Lyncis b | 5.58 | 1450 | 1.148 | 2013 | |||
| PSR B0943+10 c | 2.6 | 1460 | 2.9 | 2014 | |||
| Kepler-451c | 1.61 | 1800 | 2.1 | 0.29 | 2022 | ||
| UZ Fornacis c | 7.7 | 1900 | 2.8 | 0.05 | 2011 | ||
| HU Aquarii b | 5.4 | 2359 | 3.45 | 0.075 | 2009 | ||
| NN Serpentis d | 2.28 | 2830 | 3.39 | 0.2 | 2009 | ||
| NY Virginis b | 2.3 | 2900 | 3.39 | 2011 | |||
| OGLE-GD-ECL-11388 b | 12.5 | 3250 | 3.642 | 2016 | |||
| NSVS 14256825 d | 13.24 | 3317.7 | 3.12 | 0.12 | 2017 | ||
| FL Lyrae b | 9 | 4400 | 6.835 | 2015 | |||
| V470 Camelopardalis b | 11.8 | 4847 | 4.71 | 2020 | |||
| RR Caeli b | 4.2 | 5479 | 5.3 | 0 | 2012 | ||
| HU Aquarii c | 5.9 | 5646 | 6.18 | 0.29 | 2011 | ||
| NN Serpentis c | 6.91 | 5660 | 5.38 | 0 | 2010 | ||
| KIC 10544976 b | 13.4 | 6136 | 6.56 | 0.29 | 2019 | ||
| OY Carinae b | 8.48 | 6394 | 6.18 | 2014 | |||
| HW Virginis b | 39 | 1 | 9750 | 4.69 | 0.41 | 2008 | |
| NY Virginis c | 4.49 | 9861.75 | 7.54 | 2011 | |||
| PSR B0329+54 b | 0.0062 | 10139.34 | 10.26 | 0.236 | 2017 | ||
| DP Leonis b | 6.05 | 10230 | 8.19 | 0.39 | 2009 | ||
| SW Sextantis b | 14 | 13357 | 2019 | ||||
| HW Virginis c | 40 | 2 | 17000 | 12.8 | 0.47 | 2008 | |
| PSR B1620-26 b | 2.5 | ~36525 | ~23 | 1993 |