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Fig. 14.
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Simulated Didymos-A-like asteroid, with low crater density. We added several layers of craters on the surface with different types (i.e., simple crater types 1 & 2, complex, and fresh craters). The slope of power-law is B = 3. The depth-to-diameter ratio, 
, of simple craters and fresh craters is in [0.1, 0.2].
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