MELTYQ couples magma-atmosphere equilibrium models with spectral retrievals to constrain sub-Neptune magma oxidation states and volatile inventories from transmission spectra.
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2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes
MELTYQ couples magma-atmosphere equilibrium models with spectral retrievals to constrain sub-Neptune magma oxidation states and volatile inventories from transmission spectra.
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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.