demon planet Archives

Partial pressures of most abundant species in the vapor calculated using the Equilibrium method (left plot, same as Fig B.3 from Charnoz et al. (2023)) and the Sum method (right plot, methodology of Zilinskas et al. (2023); Piette et al. (2023)), for different monoatomic hydrogen pressure P0 H when the atmosphere is at equilibrium with the magma ocean at T = 3000 K and hydrogen is not in equilibrium with the magma ocean. -- astro-ph.EP

Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Exoplanets, -moons, -comets, Habitable Zones, Imaging & Spectroscopy, Lava / magma ocean / Volcanic Worlds, Status Report

Hydrogenated Atmospheres Of Lava Planets: Atmospheric Structure And Emission Spectra

by Keith CowingJanuary 29, 2024May 11, 2024

Hot rocky super-Earths are thought to be sufficiently irradiated by their host star to melt their surface and thus allow for long-lasting magma oceans.

demon planet

Hydrogenated Atmospheres Of Lava Planets: Atmospheric Structure And Emission Spectra

Curiosity Mars Rover Discovers A Field Of Honeycomb Textures

Viking Science

Constraining The Lives And Times Of Exoplanets Through Evolutionary Bayesian Retrievals

Project Hephaistos — III. Characterizing Anomalous Infrared Sources Identified As Dyson-sphere Candidates

SCoRE: The Surface Composition Of Rocky Exoplanets