Dynamics of the Galilean Satellites

Auteurs-es

Sylvio Ferraz-Mello
Universidade de São Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas
https://orcid.org/0000-0002-9603-2415

Mots-clés :

Mathematical and Dynamical Astronomy

Synopsis

Theoretical exposition of the motion of the 4 great satellites of Jupiter following the classical theory of Laplace and its developments. The perturbations due to the planetary-like nature of the system are calculated with emphasis in the secular and forced variations in the eccentricity of the satellites orbits. The actions due to the Sun and to the oblateness of Jupiter are also discussed.

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janvier 29, 2024
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