Question

the radial velocity method preferentially detects large planets that are close to the central star and provides the of the planet. size rotation rate age minimum mass

Explanation:

The radial - velocity method detects exoplanets by measuring the wobble of a star caused by the gravitational pull of an orbiting planet. It can provide information about the minimum mass of the planet based on the star's motion. It doesn't directly measure size, rotation rate, or age.

Answer:

minimum mass