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We highlight the existence of a topological horseshoe arising from a a–priori stable model of the binary asteroid dynamics. The inspection is numerical and uses correctly aligned windows, as described in a recent paper by A. Gierzkiewicz and P. Zgliczy'nski, combined with a recent analysis of an associated secular problem.

生成讲解博客的中文版本

生成AI智能校验的中文版本