List of exoplanets detected by radial velocity

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The following is a list of 456 extrasolar planets that were only detected by radial velocity method –– 31 confirmed and 323 candidates, sorted by orbital periods. Since none of these planets are transiting or directly observed, they do not have measured radii and generally their masses are only minimum. The true masses can be determined when astrometry calculates the inclination of the orbit.

There are 160 members of the multi-planet systems –– 21 confirmed and 139 candidates.

List of confirmed extrasolar planets[]

The most massive confirmed exoplanet is Iota Draconis b, which masses 9.40 M_J (i.e. 9.4 times the mass of Jupiter); the least massive confirmed planet is Gliese 581 e, which masses 0.007906 M_J or 2.51 M