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 the absence of global plate tectonics, mantle convection and plume–lithosphere
interaction are the main drivers of surface deformation on Venus. Among documented …

Topography on a wet rocky exoplanet could raise land above its sea level. Although land
elevation is the product of many complex processes, the large-scale topographic features on …

The availability of global gravity fields and topography through calculation services like the
International Centre for Global Earth Models, allows easy access to gravity data, greatly …

Based on topography and gravitational field data, model variations in the crust thickness of
Mars and Venus were calculated using the Love numbers method. The method takes into …

Exoplanets orbiting distant stars have revealed to us that no one could have predicted Earth.
Many stars host planets which appear to be made of rock and iron like Earth, but sit at …

Around 80% of the Venusian surface is covered by volcanic plains that contain prominent,
sinuous, and canali-like lava channels called valles that are hundreds to thousands of …

Вопрос о толщине коры Венеры остается дискуссионным. Оценки модельной средней
толщины коры Венеры варьируются в диапазоне 25-70 км. Толщина коры Венеры …

In the absence of global plate tectonics, mantle convection and plume-lithosphere
interaction are the main drivers of surface deformation on Venus. Whether Venus is …

National report of Sweden to the NKG General Assembly 2018 Page 1 DAN NORINa, ANNA
BO JENSENb, MOHAMMAD BAGHERBANDIc, MEHDI ESHAGHd NATIONAL REPORT …