Small impact craters in the lunar regolith - Their morphologies, relative ages, and rates of formation

Details Small impact craters in the lunar regolith - Their morphologies, relative ages, and rates of formation Small impact craters in the lunar regolith - Their morphologies, relative ages, and rates of formation

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980m%26p....23..231m&link_type=abstract

Moon and the Planets, vol. 23, Oct. 1980, p. 231-252.

Statistics

19

Impact Damage, Lunar Composition, Lunar Craters, Lunar Evolution, Lunar Surface, Regolith, Frequency Distribution, Meteoritic Damage, Morphology, Size Determination, Steady State

Scientific paper

The size frequency distributions, relative ages, and absolute age determination of lunar impact craters ranging in diameter from 1 to 100 m are discussed in relation to present-day and past impact rates. The size frequency distributions of craters produced by impacts on the lunar surface and of craters remaining after degradation with time and later impacts are examined, together with the steady state frequency curves for various crater morphologies. Relations between the relative ages of craters, their morphologies and their diameters are discussed, and the calibration of this kind of relationship with absolute crater ages by the location of individual craters with known absolute ages, diameters and frequency distribution statistics is considered. Estimates of present and past cratering rates based on crater size-frequency distributions are presented which suggest that the rate of impacting objects producing small lunar craters could have been constant over the last 100 million years.

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