WE PROPOSE TO MODEL THE POST-ACCRETION COOLING OF WATER-RICH EXOPLANETS (WITH AT LEAST 1% WATER BY MASS) TO ASSESS THE CONDITIONS UNDER WHICH THE PLANETS WILL COOL SUFFICIENTLY TO CONDENSE LIQUID WATER OCEANS.
$263,879FY2020National Aeronautics and Space AdministrationNASA
University Of Chicago, Chicago IL