217 citations · 678 across the 10 of their papers we have counts for
10 papers
Interior Dynamics and Thermal Evolution of Mars -- a Geodynamic Perspective
Ana-Catalina Plesa, Mark Wieczorek, Martin Knapmeyer +3
Over the past decades, global geodynamical models have been used to investigate the thermal evolution of terrestrial planets. With the increase of computational power and improveme…
Mercury's crustal thickness correlates with lateral variations in mantle melt production
Mikael Beuthe, Bernard Charlier, Olivier Namur +2
Mercury's crust has a complex structure resulting from a billion years of volcanism. The surface variations in chemical composition have been identified from orbit by the spacecraf…
LaRa after RISE: Expected improvement in the Mars rotation and interior models
Marie-Julie Péters, Sébastien Le Maistre, Marie Yseboodt +4
Two years after InSight's arrival at Mars, the ExoMars 2020 mission will land on the opposite side of the red planet. Similarly to InSight, which carries the RISE (Rotation and Int…
The radioscience LaRa instrument onboard ExoMars 2020 to investigate the rotation and interior of Mars
Veronique Dehant, Sebastien Le Maistre, Rose-Marie Baland +20
LaRa (Lander Radioscience) is an experiment on the ExoMars 2020 mission that uses the Doppler shift on the radio link due to the motion of the ExoMars platform tied to the surface…
A new ab initio equation of state of hcp-Fe and its implication on the interior structure and mass-radius relations of rocky super-Earths
Kaustubh Hakim, Attilio Rivolidini, Tim Van Hoolst +4
More than a third of all exoplanets can be classified as super-Earths based on radius (1-2 ) and mass (< 10 ). Here we model mass-radius relations bas…
Obliquity of Mercury: influence of the precession of the pericenter and of tides
Rose-Marie Baland, Marie Yseboodt, Attilio Rivoldini +1
Mercury is expected to deviate from the classical Cassini state since this state is defined for a uniformly precessing rigid planet. We develop an extended Cassini state model that…