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Fig. 12.

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Simulated Dimorphos-like asteroid, with low crater density. We add several layers of craters on the surface, e.g., simple crater types 1 and 2, and fresh craters. The total saturation is nearly 20% and the slope of power law is B = 3. The depth-to-diameter, , ratio of simple craters is in the range [0.15, 0.25].
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