Roche limit d = R·(2ρ_M/ρ_m)^{1/3} (rigid-body)

Layer 1 — Physicsin the planetary-physics subtree

Roche 1849 — a rigid-body self-gravitating satellite of density ρ_m orbiting a central body of density ρ_M and radius R is tidally disrupted if it approaches within d_rigid = R·(2ρ_M/ρ_m)^{1/3}. Derivation: at the satellite surface…

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