![From CO2- to H2O-dominated Atmospheres And Back — How Mixed Outgassing Changes The Volatile Distribution In Magma Oceans Around M Dwarf Stars [TRAPPIST-1]](https://flyingtomars.com/wp-content/uploads/2025/05/from-co2-to-h2o-dominated-atmospheres-and-back-how-mixed-outgassing-changes-the-volatile-distribution-in-magma-oceans-around-m-dwarf-stars-trappist-1.png)
This schematic depicts the set-up of the volatile exchange during initialization (t=0) and run time. For initialization, a surface temperature of 4000 K and a completely molten magma ocean is
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