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Characterization of the morphometry of impact craters hosting polar deposits in Mercury's north polar region

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Academic year: 2021

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Figure 3. Illustration of the method used to determine crater depth. (a) Plan view of the crater in Figure 2 with a near-center-crossing MLA profile overlaid
Figure 6. Locations of the 537 craters characterized in this study in a polar stereographic projection about Mercury’s north pole.
Table 1. Power Law Fits of Depth Versus Diameter for Four Populations of Craters With D Between 11 and 50 km
Table 2. Two Samples Compared in the Wilcoxon Rank-Sum Test
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