Magma ocean equilibration depletes atmospheric nitrogen and shifts C/O ratios in sub-Neptune atmospheres, making C/O, SiH4, and H2O potential tracers of formation location.
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Chemical mass transfer in magmatic processes IV. A revised and internally consistent thermodynamic model for the interpolation and extrapolation of liquid-solid equilibria in magmatic systems at elevated temperatures and pressures
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The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
Magma ocean equilibration depletes atmospheric nitrogen and shifts C/O ratios in sub-Neptune atmospheres, making C/O, SiH4, and H2O potential tracers of formation location.