Other
Scientific paper
Oct 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...60...56h&link_type=abstract
Icarus (ISSN 0019-1035), vol. 60, Oct. 1984, p. 56-74.
Other
56
Astrometry, Planetary Craters, Solar System, Density Distribution, Diameters, Equilibrium, Impact Damage, Lunar Maria, Lunar Surface, Planets, Craters, Equilibrium, Saturation, Solar System, Density, Surface, Hypotheses, Cratering, Theoretical Studies, Moon, Maria, Saturn, Satellites, Models, Plains, Formation, Lava, Flooding
Scientific paper
The similarity in crater densities on the most heavily cratered surfaces throughout the solar system is statistically examined and discussed in terms of a 'saturation equilibrium' being achieved by cratering processes. This hypothesis accounts for (1) the similarity in maximum relative crater density, below certain theoretically predicted values, on all heavily cratered surfaces; (2) a levelling off at this same relative density among 100-m scale craters in populations on lunar maria and other sparsely cratered lunar surfaces; and (3) the approximate uniformity of maximum relative densities on Saturn satellites. The lunar frontside upland crater population, sometimes described as a well-preserved production function useful for interpreting other planetary surfaces, is found not to be a production function. It was modified by intercrater plains at least partly formed by early upland basaltic lava flooding.
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