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Autor(es):
Ragazzo, Clodoaldo ; dos Santos, Lucas Ruiz
Número total de Autores: 2
Tipo de documento: Artigo Científico
Fonte: SAO PAULO JOURNAL OF MATHEMATICAL SCIENCES; v. N/A, p. 37-pg., 2024-04-08.
Resumo

In this study, we formulate a set of differential equations for a binary system to describe the secular-tidal evolution of orbital elements, rotational dynamics, and deformation (flattening), under the assumption that one body remains spherical while the other is slightly aspherical throughout the analysis. By applying singular perturbation theory, we analyze the dynamics of both the original and secular equations. Our findings indicate that the secular equations serve as a robust approximation for the entire system, often representing a slow-fast dynamical system. Additionally, we explore the geometric aspects of spin-orbit resonance capture, interpreting it as a manifestation of relaxation oscillations within singularly perturbed systems. (AU)

Processo FAPESP: 16/25053-8 - Dinâmica e geometria em baixas dimensões
Beneficiário:André Salles de Carvalho
Modalidade de apoio: Auxílio à Pesquisa - Temático