From the 1 of 7 linked papers with an AI index.
7 papers
Evolution and Observable Properties of Rocky Planet Atmospheres
Marie-Luise Steinmeyer, Lena Noack, Philipp Baumeister +9
This review summarizes current knowledge of rocky exoplanet atmospheres, covering their formation, escape processes, long‑term interaction with the surface and interior, and the ro…
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…
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…
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…
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…
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{…