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Fig. 5
Mantle depletion and viscosity for the reference case and for planets of a) 1 M⊕, b) 2 M⊕, c) 3 M⊕, and d) 4 M⊕ after 4.5 Gyr. The left and right panels represent smallest and largest core sizes, respectively, that are in agreement with planet bulk abundances (Fe∕Sibulk = 1 ×Fe∕Sisun and Mg ∕Sibulk = 1 ×Mg∕Sisun).
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