Fig. A.2
Comparisons of mass-radius relationships for water-rich planets (with water in condensed phase) of Zeng et al. (2016) (solid blue lines) with mass-radius relationships calculated in the present work (dashed blue lines), and assuming a layer of condensed water is added on top of mass-radius relationships for pure silicate (MgSiO3) planets of Zeng et al. (2016).
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