| Texto completo | |
| Autor(es): |
Ferraz-Mello, Sylvio
;
Beauge, Cristian
;
Folonier, Hugo A.
;
Gomes, Gabriel O.
Número total de Autores: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | European Physical Journal-Special Topics; v. 229, n. 8, p. 22-pg., 2020-05-01. |
| Resumo | |
Paper on the creep tide theory and its applications to satellites and planets with emphasis on a new set of differential equations allowing easier numerical studies. The creep tide theory is a new paradigm that does not fix a priori the tidal deformation of the body, but considers the deformation as a low-Reynolds-number flow. The evolution under tidal forces is ruled by an approximate solution of the Navier-Stokes equation depending on the body's viscosity with no ad hoc assumptions on its shape and orientation. It reproduces closely the results of Darwinian theories in the case of gaseous planets and stars, but the results are completely different in the case of stiff satellites and planets. It explains the tidal dissipations of Enceladus and Mimas. The extension of the theory to nonhomogeneous icy satellites with a subsurface ocean allows the amplitude of the forced oscillations around synchronization (librations) to be better determined. (AU) | |
| Processo FAPESP: | 17/25224-0 - Aplicação da teoria das marés planetárias a exoplanetas e satélites planetários |
| Beneficiário: | Gabriel de Oliveira Gomes |
| Modalidade de apoio: | Bolsas no Brasil - Doutorado Direto |
| Processo FAPESP: | 16/20189-9 - Evolução dinâmica devida à maré em exoplanetas e satélites diferenciados |
| Beneficiário: | Hugo Alberto Folonier |
| Modalidade de apoio: | Bolsas no Brasil - Pós-Doutorado |
| Processo FAPESP: | 16/13750-6 - O Brasil no espaço: Astrofísica e Engenharia |
| Beneficiário: | Eduardo Janot Pacheco |
| Modalidade de apoio: | Auxílio à Pesquisa - Projetos Especiais |