Fig. 13.

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Simulated Dimorphos-like asteroid, with high crater density. As in Fig. 12, we add several layers of craters (simple craters 1 and 2, fresh craters). The total saturation is nearly 30% and the slope of the power-law is B = 4. The depth-to-diameter ratio, , of simple crater is in [0.12, 0.19]. In fresh craters, we set the degradation vector as: α = (Δk = −0.15, Δγ = −0.1, Δa = −0.25).
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