magdalen-richard documents

Sect. 3.8: Motion in Time, Kepler Problem We’ve seen: Orbital eqtn for r -2 force law is fairly straightforward. Not so, if want r(t) & θ(t). Earlier:
Documents Sect. 3.8: Motion in Time, Kepler Problem We’ve seen: Orbital eqtn for r -2 force law is fairly straightforward. Not so, if want r(t) & θ(t). Earlier: