Problem

The hollow Moon. Newton proved that a sphere of uniform density attracts an external body as if all its mass were concentrated at the centre; he then extended the result to spherical shells of uniform density. Using these two results (and without resorting to integrals), show that a hollow sphere of outer radius RR, inner radius rr and total mass MM distributed uniformly in the shell attracts a body on its outer surface with exactly the same force as a solid sphere of equal mass MM and radius RR. Surprisingly the result does not depend on the inner radius rr: even a very thin “shell” of mass MM has the same effect.

Topics: Gravitazione Concepts: Legge di gravitazione universale · Forza peso Skills: Impostazione simbolica · Analisi di casi limite e fantafisica