| Texto completo | |
| Autor(es): |
de Oliveira, Vitor M.
Número total de Autores: 1
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| Tipo de documento: | Artigo Científico |
| Fonte: | COMMUNICATIONS IN NONLINEAR SCIENCE AND NUMERICAL SIMULATION; v. 150, p. 13-pg., 2025-11-01. |
| Resumo | |
The tidal evolution of a deformable body may lead to a state where its rotational and orbital motion are in resonance. In this work, we numerically investigate and visually illustrate some dynamical properties of the dissipative spin-orbit problem, namely, the co-existence of multiple periodic and quasi-periodic attractors, and the complexity of the corresponding basins of attraction. We apply our methodology first to Hyperion, and later to the Moon and Mercury. Our results provide a visual aid to understand the complicated dynamics of the system, and show that the different dynamical scenarios in this problem can be well characterized by the Gibbs entropy. (AU) | |
| Processo FAPESP: | 22/12785-1 - Dinâmica rotacional de corpos próximos um ao outro sob evolução de maré |
| Beneficiário: | Vitor Martins de Oliveira |
| Modalidade de apoio: | Bolsas no Exterior - Estágio de Pesquisa - Pós-Doutorado |
| Processo FAPESP: | 21/11306-0 - Acoplamento spin-órbita: o efeito da reologia |
| Beneficiário: | Vitor Martins de Oliveira |
| Modalidade de apoio: | Bolsas no Brasil - Pós-Doutorado |