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Fig. 12
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Effect of the condensation model on the transit radius of an exoplanet, shown as the relative difference in radius as a function of Teq. Calculated for an exoplanet of 5 mE, made up of 22 wt.% Fe, 38 wt.% MgSiO3 |Mantle and 40 wt.% volatiles, and for three different volatile layer compositions, i.e., 
, 
and 
.
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