show that the escape velocity of a body from the surface of a planet of radius R and mean density p is R√8/3Gπp.
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Kinetic Energy = 1/2 m v^2
Potential Energy = - G M m / R
1/2 m v^2 - G M m / R = 0 total energy at infinity = zero
v^2 = 2 G M / R
M = 4/3 pi p R^3
v^2 = 8/3 G p pi R^2
v = R (8/3 G p pi)^1/2
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