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Tidal forces arise from gravity gradient: near side attracted more than far side, stretching objects. Governs Moon stability and planetary rings.

ステップバイステップガイド

  1. 1Input primary mass, satellite mass, separation distance
  2. 2Calculate tidal force gradient
  3. 3Compare to self-gravity

解いた例

入力
Earth-Moon system
結果
Tidal force sufficient to cause 1m ocean tides
Moon receding ~3.8 cm/year

避けるべきよくある間違い

  • Confusing tidal force with mass effect
  • Neglecting density in Roche limit

よくある質問

When does tidal force destroy objects?

When exceeds self-gravity: Roche limit. Depends on density, composition.

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