The evolution and escape of the martian atmosphere and the planet's water inventory can
be separated into an early and late evolutionary epoch. The first epoch started from the …

Decades of space exploration reveal that Mars has been reshaped by volcanism throughout
its history. The range of observed volcanic landforms shows that effusive and explosive …

Numerical convection models of the thermochemical evolution of Venus are compared to
present‐day topography and geoid and recent resurfacing history. The models include …

Abstract Models of thermal evolution, crustal production, and CO2 cycling are used to
constrain the prospects for habitability of rocky planets, with Earth-like size and composition …

Volcanic outgassing is one of the main sources of volatiles for the martian atmosphere and
degassing of the martian interior potentially influenced the early martian climate. Using a …

We have reinvestigated the coupled thermal and crustal evolution of Mars taking new
laboratory data concerning the flow behavior of iron-rich olivine into account. The low mantle …

The energy sources involved in the early stages of the formation of terrestrial bodies can
induce partial or even complete melting of the mantle, leading to the emergence of magma …

We apply improved kinetic modeling of electron transport in the martian thermosphere to fit
pitch angle distributions measured by the Mars Global Surveyor (MGS) Magnetometer …

We present new whole-rock major and trace element, Re–Os isotope and mineral chemistry
data for the upper mantle peridotites and mafic rocks in the Rehafiye ophiolite in NE Anatolia …

Because much or all of the Martian mantle is apparently quite reduced, with oxygen
fugacities within 1 order of magnitude of the iron–wüstite (IW) buffer, the stable form of …