Tidal evolution for any rheological model using a vectorial approach expressed in Hansen coefficients

DOI10.1007/s10569-022-10079-3OpenAlexW4229441703MaRDI QIDQ2159137

Ema F. S. Valente, Alexandre C. M. Correia

Publication date: 26 July 2022

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

Full work available at URL: https://doi.org/10.1007/s10569-022-10079-3

zbMATH Keywords

planetary systemextended body dynamicsstellar systemdissipative forcetidecelestial body rotation

Mathematics Subject Classification ID

Celestial mechanics (70F15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

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• Complete spin and orbital evolution of close-in bodies using a Maxwell viscoelastic rheology
• Secular and tidal evolution of circumbinary systems
• Tidal evolution of hierarchical and inclined systems
• Tidal torques: a critical review of some techniques
• Tidal evolution of close binary asteroid systems
• Wave propagation in a fractional viscoelastic Andrade medium: diffusive approximation and numerical modeling
• Tidal evolution of the Keplerian elements
• The computation of tables of Hansen coefficients
• A note on Hansen's coefficients in satellite theory
• The evolution of the lunar orbit revisited. I
• Solar System Dynamics
• Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations

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