GD
Geodynamics

edited by Tobias Rolf

Finding stillness in chaos: The emergence of stable cratons in a hectic young Earth

Finding stillness in chaos: The emergence of stable cratons in a hectic young Earth

Today we know the Earth as a tectonically busy planet, shaped by mantle convection and plate tectonics. But this is nothing compared to the earlier phases of planetary evolution. This week, Fabio Capitanio (ARC Future Fellow and Associate Professor at the School of Earth, Atmosphere and Environment at Monash University, Australia) takes us on a …[Read More]

On the way back to Mercury

On the way back to Mercury

It is the smallest planet of the Solar System, the closest to the Sun and the quickest at orbiting around it, the one with the least inclined and most elongated orbit, the only one where a day lasts two-thirds of a full year, the one with the highest bulk density. Mercury is a planet of …[Read More]

InSights into Mars’ interior

InSights into Mars’ interior

This week Ana-Catalina Plesa, Junior Research Group Leader at the German Aerospace Centre (DLR) in Berlin/Germany takes us on a journey to Mars. Enjoy the read about how spacecraft observations and numerical models provide InSight into the deep enigmas of the “red planet”. Over the course of its evolution, Mars has accumulated heat in its …[Read More]