Vertically resolved magma ocean–protoatmosphere evolution: H2, H2O, CO2, CH4, CO, O2, and N2 as primary absorbers
Tim Lichtenberg - University of OxfordJan 26, 2021
Formation & evolution
Planet interiors
Atmospheric theory
Habitability & Biosignatures
Future missions & Observatories
planet formation
magma ocean
atmospheres
direct imaging
planetary interiors
Summary of the research published as 'Vertically resolved magma ocean–protoatmosphere evolution:
H2, H2O, CO2, CH4, CO, O2, and N2 as primary absorbers', Tim Lichtenberg, Dan J. Bower, Mark Hammond, Ryan Boukrouche, Patrick Sanan, Shang-Min Tsai, Raymond T. Pierrehumbert (2021) Journal of Geophysical Research: Planets; https://arxiv.org/abs/2101.10991; https://doi.org/10.1029/2020JE006711.
Contact: Tim Lichtenberg (tim.lichtenberg@physics.ox.ac.uk) ...