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The first systematic data from Apollo photogrammetry provide a high standard of accuracy for the depth/diameter (R i /D r ) relation of fresh lunar craters. Apollo R i /D r results resemble results obtained by measuring shadows on Lunar Orbiter imagery. The R i /D r distribution inflects at a crater diameter of 10 km ‐ 15 km. Lunar craters less than 15 km across are at least 50% deeper than older, telescopic data indicated (now, R i is ∼0.2 D r ), but larger craters are not much deeper. There is no marked R i /D r difference between fresh upland and postmare craters. The new R i /D r relation for small lunar craters resembles those of experimental and impact craters on Earth.
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Richard J. Pike
California Institute of Technology
Geophysical Research Letters
United States Geological Survey
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Richard J. Pike (Fri,) studied this question.
synapsesocial.com/papers/6a01f3ad8d267ec217d8cad5 — DOI: https://doi.org/10.1029/gl001i007p00291