Internal water storage capacity of terrestrial planets and the effect of hydration on the M-R relation

no code implementations • 11 Dec 2020 • Oliver Shah, Yann Alibert, Ravit Helled, Klaus Mezger

Here we consider three types of planets: dry interiors, hydrated interiors and dry interiors + surface ocean where the ocean mass fraction corresponds to the mass fraction of $\rm H_2 O$ equivalent in the hydrated case.

Earth and Planetary Astrophysics