Résumé
We highlight the existence of a topological horseshoe arising from an 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. Zgliczyński, combined with a recent analysis of an associated secular problem.
langue originale | Anglais |
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Numéro d'article | 105414 |
journal | Communication in Nonlinear Science and Numerical Simulation |
Volume | 91 |
Date de mise en ligne précoce | 20 juin 2020 |
Etat de la publication | Publié - déc. 2020 |