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Fig. 4

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Interior structure (left) and interior melting degree (right) of our Earth analogue shown with time from 0 to 5 Myr represented by the angle. The distance from the centre is normalized by the instantaneous planetary radius. Heating due to decay of 26Al initially leads to melting of the primitive MetSilWat material to form clay beneath a layer of ice. Further heating leads to full interior differentiation within 0.3 Myr. As the radiogenic energy runs out, the continued accretion leads to the emergence of a thick clay mantle overlaid by a massive surface ocean after 3 Myr. The accretion energy finally becomes high enough, after approximately 3.4 Myr, for a run-away greenhouse effect in the ocean-atmosphere system to heat the surface to above the melting temperature of silicates; this leads to a wholesale differentiation of the planet into a silicate mantle and a metal core. The contour lines show the 10, 100 and 1000 bar pressure levels in the outgassed atmosphere.

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