Gas–solid reactions on solar system bodies occur in the vicinity of their surfaces and in their
interiors where gases are liberated through magma degassing or thermal devolatilization …

The common manifestation of an explosive volcanic eruption is the emission of a hot mixture
of solid fragments and expanding magmatic gases, referred to as the eruption plume, into …

This study presents an inventory of possible chemical reactions affecting, or having affected,
the Venus surface. Fluid rock reactions are simulated using experiments under conditions …

We report two experiments using 13 mineral and rock samples exposed to a complex
synthetic Venus atmosphere composed of nine gases for durations of 30 and 11 days …

Climate models for Venus rely heavily on theoretical modeling and laboratory
experimentation due to the extreme surface conditions of the planet and limited in situ …

High temperature gas–solid reactions interactions are ubiquitous in and on the Earth and
other planetary bodies (Fig. 1). In these natural systems, gases are elusive. Like a …

Sulfur dioxide (SO2 (g)) is an important gas species in most common volcanic settings on
Earth including subduction zones (Shinohara 2013). The relative abundances of SO2 (g) …

Chemical and phase compositions of the surface of Venus could reflect a history of gas–rock
and fluid–rock interactions, recent and past climate changes, and a loss of water from the …

Rock alteration processes on Venus are still poorly understood due to the limited
geochemical data on surface rocks and uncertainties in atmospheric compositions. We use …

Extreme conditions encountered in some geological contexts (deep serpentinization,
interaction of Venus atmosphere with its basaltic surface, volcanic degassing) activate …