Part of JME-05 — Gravitation

Shell Theorem

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Newton's Shell Theorem (two parts):

  1. A uniform spherical shell attracts a particle outside it as if the entire mass were concentrated at the centre.
  2. A uniform spherical shell exerts zero net gravitational force on a particle inside it.

Consequences:

  • For a solid sphere, only the mass enclosed within radius r (the sphere of radius r) contributes to the gravitational field at distance r from the centre.
  • g inside Earth (at depth d): gdg_d = g*RdR\frac{R-d}{R} (only inner sphere matters)
  • g outside Earth: g = GMr\frac{GM}{r}^2 (entire mass acts from centre)

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