Gravity of a planet
g : G(M/r^2)
Orbital speed or velocity
(V of orbit)^2 : GM/r
Kepler’s First Law
Planets orbit the Sun along an elliptical path where the Sun is at one of the two foci of the ellipse
Kepler’s Second Law
Area 1 = Area 2
Kepler’s Third Law
(Orbital period)^2 proportional to (orbital radius)^3
Newton’s law of universal gravitation
Fg : G(m1m2)/r^2