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We report the closed-form expression for Hill’s surfaces in the circular restricted three-body problem. The solution , derived in the primary-centric spherical coordinate system, is deduced from a cubic equation delivering at most two roots on each side of a separatrix. The famous patterns (tadpole, horseshoe and peanut shapes, Roche lobes and Hill’s quasi-spheres) are exactly produced.

生成讲解博客的中文版本

生成AI智能校验的中文版本