3D Convection-resolving Model of Temperate, Tidally Locked Exoplanets
ASTROPHYSICAL JOURNAL 913:2 (2021) ARTN 101
Comment on 'Unintentional unfairness when applying new greenhouse gas emissions metrics at country level'
ENVIRONMENTAL RESEARCH LETTERS 16:6 (2021) ARTN 068001
Vertically resolved magma ocean–protoatmosphere evolution: H2 , H2O, CO2, CH4, CO, O2, and N2 as primary absorbers
Journal of Geophysical Research: Planets American Geophysical Union 126:2 (2021) e2020JE006711
Abstract:The earliest atmospheres of rocky planets originate from extensive volatile release during magma ocean epochs that occur during assembly of the planet. These establish the initial distribution of the major volatile elements between different chemical reservoirs that subsequently evolve via geological cycles. Current theoretical techniques are limited in exploring the anticipated range of compositional and thermal scenarios of early planetary evolution, even though these are of prime importance to aid astronomical inferences on the environmental context and geological history of extrasolar planets. Here, we present a coupled numerical framework that links an evolutionary, vertically‐resolved model of the planetary silicate mantle with a radiative‐convective model of the atmosphere. Using this method we investigate the early evolution of idealized Earth‐sized rocky planets with end‐member, clear‐sky atmospheres dominated by either H2, H2O, CO2, CH4, CO, O2, or N2. We find central metrics of early planetary evolution, such as energy gradient, sequence of mantle solidification, surface pressure, or vertical stratification of the atmosphere, to be intimately controlled by the dominant volatile and outgassing history of the planet. Thermal sequences fall into three general classes with increasing cooling timescale: CO, N2, and O2 with minimal effect, H2O, CO2, and CH4 with intermediate influence, and H2 with several orders of magnitude increase in solidification time and atmosphere vertical stratification. Our numerical experiments exemplify the capabilities of the presented modeling framework and link the interior and atmospheric evolution of rocky exoplanets with multi‐wavelength astronomical observations.
The Phase-curve Signature of Condensible Water-rich Atmospheres on Slowly Rotating Tidally Locked Exoplanets
ASTROPHYSICAL JOURNAL LETTERS 901:2 (2020) ARTN L33
The Equatorial Jet Speed on Tidally Locked Planets. I. Terrestrial Planets
ASTROPHYSICAL JOURNAL 901:1 (2020) ARTN 78