In this work we describe some aspects of the dynamics of the mean-motion resonances. Emphasis to the case of resonances between regular satellites of the giant planets will be given, even so some aspects of the physics of the resonances in extra-solar planetary systems are also briefly treated. The role of the resonances in satellites systems is discussed through examples, showing how certain resonances, and its relations with the tidal dissipation effects, can be the key of the explanation of some phenomena still not explained in the Solar System. Amongst some examples we highlight the problem of the resurfacing of Enceladus, the existence of active volcanoes in Io, and the possible existence of the subsurface ocean in Europe. This work ha...
Uranus and its complex and unexpected system of moons are still today a mystery of the solar system....
International audienceThe motion of a satellite can experience secular resonances between the preces...
A concise, novel description is presented of near-circular satellite motion at arbitrary inclination...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Abstract: Effects due to resonances in the orbital motion of artificial satellites disturbed by the ...
We study the evolution of two planets around a star, in mean-motion resonance and undergoing tidal e...
The Laplace resonance is a configuration that involves the commensurability between the mean motions...
The first three Galilean satellites of Jupiter, Io, Europa, and Ganymede, move in a dynamical config...
Effects due to resonances in the orbital motion of artificial satellites disturbed by the terrestria...
Satellite systems around giant planets are immersed in a region of complex resonant configurations. ...
The motion of a satellite can experience secular resonances between the precession frequencies of it...
In some planetary systems, the orbital periods of two of its members present a commensurability, usu...
We give a description of orbital and spin-orbit resonances in the solar system, providing several ex...
International audienceIn some planetary systems, the orbital periods of two of its members present a...
An ever-growing observational aggregate of extrasolar planets has revealed that systems of planets t...
Uranus and its complex and unexpected system of moons are still today a mystery of the solar system....
International audienceThe motion of a satellite can experience secular resonances between the preces...
A concise, novel description is presented of near-circular satellite motion at arbitrary inclination...
Several examples of satellite dynamics are presented where significant progress has been made in und...
Abstract: Effects due to resonances in the orbital motion of artificial satellites disturbed by the ...
We study the evolution of two planets around a star, in mean-motion resonance and undergoing tidal e...
The Laplace resonance is a configuration that involves the commensurability between the mean motions...
The first three Galilean satellites of Jupiter, Io, Europa, and Ganymede, move in a dynamical config...
Effects due to resonances in the orbital motion of artificial satellites disturbed by the terrestria...
Satellite systems around giant planets are immersed in a region of complex resonant configurations. ...
The motion of a satellite can experience secular resonances between the precession frequencies of it...
In some planetary systems, the orbital periods of two of its members present a commensurability, usu...
We give a description of orbital and spin-orbit resonances in the solar system, providing several ex...
International audienceIn some planetary systems, the orbital periods of two of its members present a...
An ever-growing observational aggregate of extrasolar planets has revealed that systems of planets t...
Uranus and its complex and unexpected system of moons are still today a mystery of the solar system....
International audienceThe motion of a satellite can experience secular resonances between the preces...
A concise, novel description is presented of near-circular satellite motion at arbitrary inclination...