Rotation and figure evolution in the creep tide theory: a new approach and application to Mercury

DOI10.1007/S10569-019-9935-ZzbMath1451.70043arXiv1910.12990OpenAlexW3101031141WikidataQ126747130 ScholiaQ126747130MaRDI QIDQ2005667

Gabriel O. Gomes, Hugo A. Folonier, Sylvio Ferraz-Mello

Publication date: 8 October 2020

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1910.12990

zbMATH Keywords

Mercuryflatteningsspin-orbitplanetary tide

Mathematics Subject Classification ID

Orbital mechanics (70M20) Parametric resonances for nonlinear problems in mechanics (70K28)

Cites Work

• Unnamed Item
• Unnamed Item
• Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
• The flattenings of the layers of rotating planets and satellites deformed by a tidal potential
• Large scale chaos and marginal stability in the solar system
• Tidal synchronization of close-in satellites and exoplanets. III: Tidal dissipation revisited and application to Enceladus

This page was built for publication: Rotation and figure evolution in the creep tide theory: a new approach and application to Mercury