LawHubble's LawThe recessional velocity of a galaxy is directly proportional to its proper distance from the observer: v=H0Dv = H_0 Dv=H0D.
LawKepler's Second LawA line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.
LawKepler's Third LawThe square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit: T2∝a3T^2 \propto a^3T2∝a3.