activity
20242026
most citedExo-Geoscience Perspectives Beyond Habitability

4 citations · 11 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026★ 1 cited

Evolution and Observable Properties of Rocky Planet Atmospheres

Marie-Luise Steinmeyer, Lena Noack, Philipp Baumeister +9

The atmospheric composition of rocky exoplanets offers an important tool for constraining the properties of the interior of this type of planet, beyond what is possible from measur…

astro-ph.EP2026

Coupled atmospHere Interior modeL Intercomparison (CHILI). I. Evolutionary Modelling -- Primordial Magma Oceans of Earth and Venus

Harrison Nicholls, Joshua Krissansen-Totton, Tim Lichtenberg +22

Earth and Venus represent two evolutionary outcomes arising from initially molten 'magma ocean' periods, followed by lifetimes of chemical and geophysical divergence. Their physics…

astro-ph.EP2026★ 4 cited

Exo-Geoscience Perspectives Beyond Habitability

Tilman Spohn, Akli Roberge, M. J. Way +5

This article reviews the emerging field of exo-geoscience, focusing on the geological and geophysical processes thought to influence the evolution and (eu)habitability of rocky exo…

astro-ph.EP2025★ 1 cited

Fundamentals of interior modelling and challenges in the interpretation of observed rocky exoplanets

Philipp Baumeister, Francesca Miozzi, Claire Marie Guimond +7

Most our knowledge about rocky exoplanets is based on their measure of mass and radius. These two parameters are routinely measured and are used to categorise different populations…

astro-ph.EP2025

Coupled atmospHere Interior modeL Intercomparison (CHILI) Protocol Version 1.0: A CUISINES Intercomparison Project of Magma Ocean Models

Tim Lichtenberg, Laura Schaefer, Joshua Krissansen-Totton +23

Spectroscopic characterization of rocky exoplanets with the James Webb Space Telescope has brought the origin and evolution of their atmospheres into the focus of exoplanet science…

astro-ph.EP2025★ 4 cited

The influence of interior structure and thermal state on impact melt generation upon large impacts onto terrestrial planets

Lukas Manske, Thomas Ruedas, Ana-Catalina Plesa +4

We investigate the melt production of planetary impacts as a function of planet size (=0.1-1.5), impactor size (=1-1000 km), and core size ratio ($R_\mathrm{…

astro-ph.EP2024★ 1 cited

Chapter 10031. Surfaces and Interiors

Lena Noack, Caroline Dorn, Philipp Baumeister

In the last 15 years, since the discovery of the first low-mass planets beyond the solar system, there has been tremendous progress in understanding the diversity of (super-)Earth…