Abstract
Abstract Hill's equation which describes approximately motions of interacting two bodies orbiting around the Sun is summarized, together with its properties. Hill's equation can be separated into equations of the relative and center of mass motions, and the center of ...
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APA
Nakazawa, K., & Ida, S. (1988). Chapter 15. Hill’s Approximation in the Three-Body Problem. Progress of Theoretical Physics Supplement, 96, 167–174. https://doi.org/10.1143/ptps.96.167
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