Abstract The Interior exploration using Seismic Investigations, Geodesy, and Heat Transport
(InSight) Mission will focus on Mars' interior structure and evolution. The basic structure of …

A planet's crust bears witness to the history of planetary formation and evolution, but for
Mars, no absolute measurement of crustal thickness has been available. Here, we …

Lacking plate tectonics and crustal recycling, the long-term evolution of the crust-mantle
system of Mars is driven by mantle convection, partial melting, and silicate differentiation …

The ChemCam instrument, which provides insight into martian soil chemistry at the
submillimeter scale, identified two principal soil types along the Curiosity rover traverse: a …

We report maps of the concentrations of H, Si, Cl, K, Fe, and Th as determined by the
Gamma Ray Spectrometer (GRS) on board the 2001 Mars Odyssey Mission for±∼ 45° …

We used imaging, laser altimeter and thermal infrared data to map a 0.5 by 0.5° area
containing the landing site of the Zhurong rover of the Tianwen‐1 mission. We analyzed the …

The present‐day thermal state, interior structure, composition, and rheology of Mars can be
constrained by comparing the results of thermal history calculations with geophysical …

Until recently, Mars was considered a basalt-covered world, but this vision is evolving thanks
to new orbital, in situ and meteorite observations, in particular of rocks of the ancient …

The ChemCam instrument onboard the Curiosity rover provides for the first time an
opportunity to study martian soils at a sub-millimeter resolution. In this work, we analyzed 24 …

Transport of fine-grained dust is one of the most widespread sedimentary processes
occurring on Mars today. In the present climate, eolian abrasion and deflation of rocks are …