This is the list of exoplanets that were detected by the radial velocity method. Note that this category does not include planets that were detected by transit first. Radial velocity measurements constrain mass and determine if it is a planet or not. Although planets detected by radial velocity and later by transit are included.

Properties (mass and semimajor axis) of planets discovered using the radial velocity method, compared (light gray) with planets discovered using other methods.