This work reviews the long-term evolution of the atmosphere of Venus, and modulation of its
composition by interior/exterior cycling. The formation and evolution of Venus's atmosphere …

In preparation for the ESA/JAXA BepiColombo mission to Mercury, thematic working groups
had been established for coordinating the activities within the BepiColombo Science …

The volcanic landforms, eruptive sites and longevity of activity on Mercury and the Moon
contrast substantially with those of Earth, Venus and Mars. Here, I synthesize global maps of …

Over the first billion years of Mercury's history, mantle melting and surface volcanism
produced a secondary magmatic crust varying spatially in composition and mineralogy. By …

The early bombardment history of Mars may have drastically shaped its crustal evolution.
Impact-induced melting of crustal and mantle materials leads to the formation of local and …

We computed interior structure models of Mercury and analyzed their viscoelastic tidal
response. The models are consistent with MErcury Surface, Space Environment …

Mercury's low obliquity and 3: 2 spin‐orbit resonance create a surface temperature
distribution with large latitudinal and longitudinal variations. These propagate via thermal …

Mantle convection, the buoyancy-driven creeping flow of silicate rocks in the interior of
terrestrial planets like Earth, Mars, Mercury, and Venus plays a fundamental role in the long …

This paper reviews habitability conditions for a terrestrial planet from the point of view of
geosciences. It addresses how interactions between the interior of a planet or a moon and …

Patches of small smooth plains cover a substantial portion of the Mercurian surface, but their
origin and relation to the global evolution are not completely understood. Here, we update …