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Fig. 7

image

Evolution of the temperature (left column) and density (right column) assuming accretion of Ceres in the inter-planet disk (top row) and in the Kuiper belt (bottom row) and subsequent migration starting at 10 Myr after CAIs and 600 Myr after CAIs, respectively, within 1 Myr into the outer asteroid belt. The accretion time is tac = 7 Myr (top row) and tac = 100 Myr (bottom row).

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