Depth/diameter relations of fresh lunar craters: Revision from spacecraft data
Richard J. Pike
Abstract
Richard J. Pike
Abstract
The first systematic data from Apollo photogrammetry provide a high standard of accuracy for the depth/diameter (Ri/Dr) relation of fresh lunar craters. Apollo Ri/Dr results resemble results obtained by measuring shadows on Lunar Orbiter imagery. The Ri/Dr 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, Ri is ∼0.2 Dr), but larger craters are not much deeper. There is no marked Ri/Dr difference between fresh upland and postmare craters. The new Ri/Dr relation for small lunar craters resembles those of experimental and impact craters on Earth.
OpenAlex reports 260 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The first systematic data from Apollo photogrammetry provide a high standard of accuracy for the depth/diameter (Ri/Dr) relation of fresh lunar craters. Apollo Ri/Dr results resemble results obtained by measuring shadows on Lunar Orbiter imagery. The Ri/Dr 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, Ri is ∼0.2 Dr), but larger craters are not much deeper. There is no marked Ri/Dr difference between fresh upland and postmare craters. The new Ri/Dr relation for small lunar craters resembles those of experimental and impact craters on Earth.
Key concepts: Impact crater, Lunar craters, Geology, Orbiter, Far side of the Moon, Astrobiology, Apollo, Geology of the Moon