The current state of Venus is the result of the cumulative effects of many processes from the planet’s formation, and its magma ocean phase up to present-day. Venus’s interior thermal evolution, volcanic, tectonic and outgassing history, as well as interaction with the atmosphere have left clues to piece back together what made Earth and Venus evolve differently. Therefore, due to its position at the inner edge of the Solar System habitable zone (HZ), Venus evolution through time provides insights on surface habitability of rocky exoplanets.
ISSI Forum sparks breakthrough guidance for remote sensing collaborations to monitor climate tipping points
Volume 85 in the Space Sciences Series of ISSI
During the recent decades, space missions (e.g., CHAMP, GOCE, GRACE and Swarm) have been developed by space agencies in Europe and the USA to measure the Earth’s gravity and magnetic fields and their spatio-temporal variations. These successful missions have already provided a wealth of groundbreaking results about the permanent and time-variable gravity and magnetic fields of the Earth.
