International audienceAs the obliquity of Mars is strongly chaotic, it is not possible to give a solution for its evolution over more than a few million years. Using the most recent data for the rotational state of Mars, and a new numerical integration of the Solar System, we provide here a precise solution for the evolution of Mars' spin over 10 to 20 Myr. Over 250 Myr, we present a statistical study of its possible evolution, when considering the uncertainties in the present rotational state. Over much longer time span, reaching 5 Gyr, chaotic diffusion prevails, and we have performed an extensive statistical analysis of the orbital and rotational evolution of Mars, relying on Laskar's secular solution of the Solar System, based on more t...
The long-term variations in the orbit of the Earth govern the insolation on its surface and hence it...
Abstract The knowledge of Martian geology has increased enormously in the last 40 yr. Several missio...
International audienceFan-shaped deposits up to ∼166,000 km in area are found on the northwest flank...
International audienceAs the obliquity of Mars is strongly chaotic, it is not possible to give a sol...
As the obliquity of Mars is strongly chaotic, it is not possible to give a solution for its evolutio...
International audienceAs the obliquity of Mars is strongly chaotic, it is not possible to give a pre...
International audienceThe discovery of the chaotic behavior of the planetary orbits in the Solar Sys...
The correlation of Earth's orbital parameters with climatic variations has been used to generate ast...
The purpose of this thesis is to study the evolution of the obliquity and speed of rotation of terre...
Large-scale variations in the obliquity of the planet Mars are produced by a coupling between the mo...
Many dynamical aspects of the solar system can be explained by the outer planets experiencing a peri...
International audienceMany dynamical aspects of the solar system can be explained by the outer plane...
Solar variability influences the climate of a planet by radiatively forcing changes over a certain t...
The possible polar wandering of the planet Mars is investigated by modeling some of the many surfac...
The long-term variations in the orbit of the Earth govern the insolation on its surface and hence it...
Abstract The knowledge of Martian geology has increased enormously in the last 40 yr. Several missio...
International audienceFan-shaped deposits up to ∼166,000 km in area are found on the northwest flank...
International audienceAs the obliquity of Mars is strongly chaotic, it is not possible to give a sol...
As the obliquity of Mars is strongly chaotic, it is not possible to give a solution for its evolutio...
International audienceAs the obliquity of Mars is strongly chaotic, it is not possible to give a pre...
International audienceThe discovery of the chaotic behavior of the planetary orbits in the Solar Sys...
The correlation of Earth's orbital parameters with climatic variations has been used to generate ast...
The purpose of this thesis is to study the evolution of the obliquity and speed of rotation of terre...
Large-scale variations in the obliquity of the planet Mars are produced by a coupling between the mo...
Many dynamical aspects of the solar system can be explained by the outer planets experiencing a peri...
International audienceMany dynamical aspects of the solar system can be explained by the outer plane...
Solar variability influences the climate of a planet by radiatively forcing changes over a certain t...
The possible polar wandering of the planet Mars is investigated by modeling some of the many surfac...
The long-term variations in the orbit of the Earth govern the insolation on its surface and hence it...
Abstract The knowledge of Martian geology has increased enormously in the last 40 yr. Several missio...
International audienceFan-shaped deposits up to ∼166,000 km in area are found on the northwest flank...