The dynamics and evolution of Venus' mantle are of first-order relevance for the origin and
modification of the tectonic and volcanic structures we observe on Venus today. Solid-state …

In this work we discuss various selected mission concepts addressing Venus evolution
through time. More specifically, we address investigations and payload instrument concepts …

Deep understanding of planetary habitability requires identifying key factors that govern the
surface environment over time. Venus is the ultimate control case for understanding how …

Venus is the planet in the Solar System most similar to Earth in terms of size and (probably)
bulk composition. Until the mid-20th century, scientists thought that Venus was a verdant …

Understanding the physical characteristics of Venus, including its atmosphere, interior, and
its evolutionary pathway with respect to Earth, remains a vital component for terrestrial …

Bodily tides provide key information on the interior structure, evolution, and origin of the
planetary bodies. Our Solar system harbors a very diverse population of planetary bodies …

The study of planets and small bodies within our Solar System is fundamental for
understanding the formation and evolution of the Earth and other planets. Compositional …

The long‐wavelength gravity and topography of Venus are dominated by mantle convective
flows, and are hence sensitive to the planet's viscosity structure and mantle density …

The success of the Transiting Exoplanet Survey Satellite mission has led to the discovery of
an abundance of Venus Zone terrestrial planets that orbit relatively bright host stars …

The NASA Discovery-class mission VERITAS, selected in June 2021, will be launched
toward Venus after 2027. In addition to the science instrumentation that will build global …