Force of Gravity
F_g = GMm/r^2
Gravitational Acceleration
g = GM/r^2
Gravitational Potential Energy
U = -GMm/r
Escape Velocity
v = sqrt(2GM/r)
Kepler’s Laws
1) Two bodies orbit each other elliptically
2) Equal areas in equal times
3) T^2 = (4(pi^2)/GM’) a^3, where a is the semi major axis, M’ is the sum of the masses
Energy of a circular orbit
-GMm/2a
Vis-Viva Equation
v = sqrt(GM(2/r - 1/a)), r is the distance between the centres of mass, a is the semi major axis