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Fig. 27

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Initial and final size distribution of the asteroid main belt (blue) and the synthetic Datura family (cyan) from the 500 kyr lasting simulation of the Boulder code. Intrinsic collisonal probabilities and impact velocities as described in the text. The observed Datura family population from Table A.1 shown by the black curve. No evolution is seen in both populations over the tested timescale and for the sizes displayed.

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