Planetary cratering - On the conical shape of lunar fresh craters

Details Planetary cratering - On the conical shape of lunar fresh craters Planetary cratering - On the conical shape of lunar fresh craters

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mmsai..51..285b&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 51, June 1980, p. 285-297.

Mathematics

Logic

Cratering, Impact Damage, Lunar Craters, Morphology, Cones, Depth, Lunar Far Side, Statistical Analysis

Scientific paper

Results are presented for a statistical analysis of the depths, diameters, floor diameters, and wall slopes of 100 lunar craters with diameter of 4 to 100 km. The craters are located in various highland and basin regions on both the nearside and the farside of the moon. It is found that: (1) a cone or truncated cone is the most common shape for the observed lunar craters; (2) conical craters are the more recent craters in each sampled region; and (3) different geologic units on the moon have different responses to impacts.

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