Numerical model of C outgassing shows CC planetesimals deplete >50% carbon while NCs deplete <50% for typical sizes and formation times, favoring NC bodies as the main C source for terrestrial planets.
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Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.
citing papers explorer
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Modeling carbon outgassing from chondritic planetesimals
Numerical model of C outgassing shows CC planetesimals deplete >50% carbon while NCs deplete <50% for typical sizes and formation times, favoring NC bodies as the main C source for terrestrial planets.
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Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.