Fig. 2 | Nature Communications

Fig. 2

From: The impact origin and evolution of Chryse Planitia on Mars revealed by buried craters

Fig. 2

Depth-to-diameter ratio distribution in different units within the Chryse Planitia. a Bouguer gravity anomaly map20 of the Chryse and Acidalia Planitia showing the location of the anomaly units and adjacent units in Mars Simple Cylindrical Projection. b, c The depth-diameter scatter plot (upper) and probability density distribution of depth/diameter ratio (lower). b the Chryse anomaly unit and Small anomaly unit; c The Adjacent units 1 and 2. Shaded regions indicate the distribution of the depth-to-diameter ratio of pristine craters

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