The effects of deformation inertia (kinetic energy) in the orbital and spin evolution of close-in bodies

DOI10.1007/s10569-018-9847-3zbMath1447.70021OpenAlexW2883274947WikidataQ110098650 ScholiaQ110098650MaRDI QIDQ1785895

C. Ragazzo, Alexandre C. M. Correia, Lucas S. Ruiz

Publication date: 2 October 2018

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

Full work available at URL: http://hdl.handle.net/10773/25063

zbMATH Keywords

dissipative forcesplanetary systemstidesdeformation inertia

Mathematics Subject Classification ID

Orbital mechanics (70M20) General questions in geophysics (86A04)

Related Items (3)

Librations of a body composed of a deformable mantle and a fluid core ⋮ The theory of figures of Clairaut with focus on the gravitational modulus: inequalities and an improvement in the Darwin-Radau equation ⋮ Tidal synchronization of close-in satellites and exoplanets. III: Tidal dissipation revisited and application to Enceladus

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• Analysis of resonances in the spin-orbit problem in celestial mechanics. I: The synchronous resonance
• Viscoelastic tides: models for use in Celestial Mechanics
• The evolution of the lunar orbit revisited. I
• Averaging methods in nonlinear dynamical systems

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