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Gravitational force (universal)
g
G
G = 6.674 × 10-11 N * m2/kg2
gravity vector field
m0 = mass of test particle
Kepler’s Laws
All planets move in ellipses, with the sun at a foci.
dA/dt = constant (r = radius between Sun and planet)
T2 = (4π2/GM)r3 (T2 is proportional to r3)
Potential energy between two bodies
Energy (circular & elliptical orbits)
Escape speed