Like the radial velocity method, it can be used to determine the orbital eccentricity and the minimum mass of the planet and it is easier to detect massive planets close to their stars as these factors increase star's motion.
With this method, it is easier to detect massive planets close to their stars as these factors increase the star's motion. Like the radial velocity method, it can be used to determine the orbital eccentricity and the minimum mass of the planet.
Like the radial velocity method, it can be used to determine the orbital eccentricity and the minimum mass of the planet. With this method, it is easier to detect massive planets close to their stars as these factors increase the star's motion.
Like the radial velocity method, it can be used to determine the orbital eccentricity and the minimum mass of the planet. With this method, it is easier to detect massive planets close to their stars as these factors increase the star's motion.