When we first embarked on this project we were
told unequivocally that precision radial
velocity measurements were impossible at the amateur level and required the funding and resources of an institution.
Furthermore, by knowing the mass of a planet from radial
velocity measurements and the radius of a planet based on how much starlight it blocked, it is a simple calculation to determine a planet's density, which can
tell astronomers whether that planet is rocky or gaseous in nature, or whether it has a small core and a thick atmosphere, or whether it has a large core covered in deep oceans.