Fig. 7
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Ice mass left over total initial mass in the different radial bins in the main belt for a large 100 km body as a function of time (brighter colours are for longer times) for the scenario 1. Most of the mass gets depleted from the inner region after the surge in luminosity at ~20 Myr. There is no ice left on the 100 km body after 1 Gyr evolution.
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