Numerical approach to synthesizing realistic asteroid surfaces from morphological parameters

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Fig. A.1.

Simulated Eros-like asteroid, with low crater density. Just as in Figs. 14 and 14, we added several layers of craters (the surface partitioned into nearly 1500 patches). The total saturation is nearly 11% and the slope of power law B = 3. For both simple and fresh craters, .

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