Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.
ExoMol line lists - XV
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Derives irreducible transformation matrices for all operations of G36 and G36(EM) for ethane and implements generator-based symmetry adaptation in TROVE for variational nuclear-motion calculations.
citing papers explorer
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Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.