Integrated simulations reveal that exoplanet envelope mass fractions are degenerate with instellation and metallicity, enabling more reliable Bayesian inferences of planetary structure and climate from mass-radius data.
R., Seager S., Elkins-Tanton L., 2008, Astrophys
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Beyond the mass-radius plane: Integrated radiative-convective and interior structure simulations of the exoplanet continuum
Integrated simulations reveal that exoplanet envelope mass fractions are degenerate with instellation and metallicity, enabling more reliable Bayesian inferences of planetary structure and climate from mass-radius data.