Tidal synchronization of close-in satellites and exoplanets. III: Tidal dissipation revisited and application to Enceladus
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Publication:2203847
DOI10.1007/s10569-018-9872-2zbMath1445.70007arXiv1707.09229OpenAlexW3099567759WikidataQ128812161 ScholiaQ128812161MaRDI QIDQ2203847
Hugo A. Folonier, Sylvio Ferraz-Mello, Eduardo Andrade-Ines
Publication date: 2 October 2020
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1707.09229
Related Items (4)
Creep tide theory: equations for differentiated bodies with aligned layers ⋮ A direct numerical verification of tidal locking mechanism using the discrete element method ⋮ Rotation and figure evolution in the creep tide theory: a new approach and application to Mercury ⋮ Ellipsoidal equilibrium figure and Cassini states of rotating planets and satellites deformed by a tidal potential in the spatial case
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- Stability in the full two-body problem
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