Fig. 5
Parameters related to the thermal evolution of three-layer planets with core and mantle radii of 1500 and 3000 km, respectively. All three models have different graphite lid thicknesses (1, 50, and 500 km) and consequently different planetary radii. In plots e and f, the 5 Gyr lines for the 50 and 500 km cases overlap; the 1 km case is not shown.
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