The Roche limit is the distance from a planet within which a moon or satellite held together only by its own gravity would be torn apart by tidal forces — it's why planets like Saturn have rings instead of a moon in that zone..
The Roche limit is the distance from a planet within which a moon or satellite held together only by its own gravity would be torn apart by tidal forces — it's why planets like Saturn have rings instead of a moon in that zone.
A planet with radius 7×10⁷ m and density 1300 kg/m³, and a satellite with density 3000 kg/m³. Roche Limit = 7×10⁷ × ∛(2×1300/3000) ≈ 6.53×10⁷ m — inside this distance, tidal forces would break the satellite apart.
The minimum distance a body can orbit another before tidal forces overcome its own gravity and tear it apart.
It depends on the radius and density of both bodies, using tidal force balance formulas.
Material within the limit gets torn apart before it can coalesce into a moon, forming rings instead.