5 citations · 12 across the 8 of their papers we have counts for
8 papers
Non-equilibrium condensation of the first Solar System solids
Sebastien Charnoz, Jérome Aleon, Marc Chaussidon +3
Primitive meteorites (chondrites) consist of an out-of-equilibrium assemblage of minerals formed during the assembling of our Solar Nebula. The conditions under which their precurs…
The dynamical surface of Phobos: a morphodynamic atlas
Isabel Herreros, Sébastien Charnoz
Phobos evolves in a highly dynamical environment where surface-material motion is controlled by the combined effects of self-gravity, time-dependent Martian tides, and inertial for…
Tracking low-velocity ejecta from the DART impact on Dimorphos
Isabel Herreros, Sébastien Charnoz
The DART impact on Dimorphos produced a large population of low-velocity ejecta (v < vesc), likely containing most of the excavated mass, whose early fate remains poorly constraine…
Understanding the formation of Saturn's regular moons in the context of giant planet moons formation scenarios
Michel Blanc, Aurélien Crida, Yuhito Shibaike +7
This article explores the different formation scenarios of the Kronian moons system in the context of a highly dissipative Saturn, with the objective of identifying the most likely…
An impact-free mechanism to deliver water to terrestrial planets and exoplanets
Quentin Kral, Paul Huet, Camille Bergez-Casalou +3
To date, the most widespread scenario is that the Earth originated without water and was brought to the planet mainly due to impacts by wet asteroids coming from further out in spa…
Hydrodynamical simulations of proto-Moon degassing
Gustavo Madeira, Leandro Esteves, Sebastien Charnoz +2
Similarities in the non-mass dependent isotopic composition of refractory elements with the bulk silicate Earth suggest that both the Earth and the Moon formed from the same materi…
Hydrogenated atmospheres of lava planets: atmospheric structure and emission spectra
Aurélien Falco, Pascal Tremblin, Sébastien Charnoz +2
Hot rocky super-Earths are thought to be sufficiently irradiated by their host star to melt their surface and thus allow for long-lasting magma oceans. Some processes have been pro…
The role of interior dynamics and differentiation on the surface and atmosphere of lava planets
Charles-Édouard Boukaré, Daphné Lemasquerier, Nicolas Cowan +5
Lava planets are rocky exoplanets that orbit so close to their host star that their day-side is hot enough to melt silicate rock. Their short orbital periods ensure that lava plane…