For a satellite of mass in an elliptical orbit

PHYSICS · Subjective · AP · Physics 1: Algebra-based · Energy and Momentum of Rotating Systems · Energy and Momentum of Rotating Systems

Problem

For a satellite of mass mm in an elliptical orbit, its distance from the central body is rpr_p at perigee and rar_a at apogee. Derive an expression for the ratio of its kinetic energy at perigee, KpK_p, to its kinetic energy at apogee, KaK_a, in terms of rpr_p and rar_a.

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