Ocean salinity and planetary obliquity synergize via ice-albedo feedback to produce distinct climate states and enhanced habitability on cold exo-Earths in ROCKE-3D simulations.
J., Aleinov, I., Amundsen, D
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3D GCM simulations favor a thick (>=10 bar), CO2-rich (>1% mixing ratio) atmosphere for 55 Cancri e that matches JWST spectra while ruling out thin or CO/CO2-poor cases.
Early Venus experienced large seasonal and latitudinal insolation redistribution but only modest orbit-averaged flux changes, making atmospheric opacity the dominant control on surface temperature rather than orbital forcing.
citing papers explorer
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Synergistic Effects of Ocean Salinity and Planetary Obliquity Enhance Habitability of Cold Exo-Earths
Ocean salinity and planetary obliquity synergize via ice-albedo feedback to produce distinct climate states and enhanced habitability on cold exo-Earths in ROCKE-3D simulations.
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Reinterpreting the JWST Observations of 55 Cancri e with a Non-Grey General Circulation Model
3D GCM simulations favor a thick (>=10 bar), CO2-rich (>1% mixing ratio) atmosphere for 55 Cancri e that matches JWST spectra while ruling out thin or CO/CO2-poor cases.
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Seasonal Insolation Variability on Early Venus: Implications for Energy Budget
Early Venus experienced large seasonal and latitudinal insolation redistribution but only modest orbit-averaged flux changes, making atmospheric opacity the dominant control on surface temperature rather than orbital forcing.