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The resonance perturbation of planetary ring by distant satellite is considered. The gravity interaction between rings particles is taken into account. The gravitation interaction between particles in rings can change shape of non-circular rings, so it is differ from keplerian ellipse. The shift between simple mean motion resonances and parametric resonance zones is detected. This shift depends on ring properties.

生成讲解博客的中文版本

生成AI智能校验的中文版本