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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

The current orbit of Methone (S/2004 S 1)

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Autor(es):
Callegari Jr, Nelson ; Rodriguez, Adrian [1] ; Ceccatto, Demetrio Tadeu [2]
Número total de Autores: 3
Afiliação do(s) autor(es):
[1] Univ Fed Rio de Janeiro, Observ Valongo, Ladeira Pedro Antonio 43, BR-20080090 Rio de Janeiro - Brazil
[2] Phys Program IGCE Unesp, Rio Claro - Brazil
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY; v. 133, n. 11-12 DEC 2021.
Citações Web of Science: 0
Resumo

The Cassini spacecraft discovered many close-in small satellites in Saturnian system, and several of them exhibit exotic orbital states due to interactions with Mimas and the oblateness of the planet. This work is devoted to Methone, which is currently involved in a 15:14 mean-motion resonance with Mimas. We give an in-deep study on the current orbit of Methone by analyzing and identifying the short, resonant and long-term gravitational perturbations on its orbit. In addition, we perform numerical integrations of full equations of motion of ensembles of close-in small bodies orbiting the non-central field of Saturn. Spectral analyses of the orbits and interpretation of them in dynamical maps allow us to describe the orbit and the dynamics of Methone in view of resonant and long-term dynamics. We show that the current geometric orbit of Methone is aligned with Mimas' due to a forced resonant component in eccentricity, leading to simultaneous oscillations of several critical angles of the expanded disturbing function. Thus, we explain the simultaneous oscillations of four critical arguments associated to the resonance. The mapping of the Mimas-Methone resonance shows that the domains of the 15:14 Mimas-Methone resonance are dominated by regular motions associated to the Corotation resonance located at eccentricities lower than 0.015 and osculating semi-major axis in the interval 194,660-194,730 km. Methone is currently located deeply within this site. (AU)

Processo FAPESP: 20/06807-7 - Dinâmica ressonante de pequenos satélites e partículas no sistema interior de Saturno
Beneficiário:Nelson Callegari Júnior
Modalidade de apoio: Auxílio à Pesquisa - Regular
Processo FAPESP: 19/15162-2 - EPSC-DPS Joint Meeting 2019
Beneficiário:Nelson Callegari Júnior
Modalidade de apoio: Auxílio à Pesquisa - Reunião - Exterior