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Fig. 8
Mantle depletion and viscosity for different planet bulk compositions after 4.5 Gyr. All shown planets have a mass of 2 M⊕. The left and right panels represent smallest and largest core sizes, respectively, that are in agreement with planet bulk abundances (Fe∕Sibulk and Mg ∕Sibulk). The reference case is shown (Table 3).
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