Mathematics – Probability
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pggp.rept...97h&link_type=abstract
In NASA. Washington Rept. of the Planetary Geol. Program, 1983 p 97-99 (SEE N84-23431 13-91)
Mathematics
Probability
Cratering, Lunar Craters, Lunar Maria, Planetary Evolution, Solar System, Ejecta, Icy Satellites, Lithosphere, Mars (Planet), Mercury (Planet), Population Theory, Probability Density Functions
Scientific paper
A number of researchers have concluded that saturation equilibrium cratering exists nowhere in the solar system, and therefore that diameter distributions in even the most heavily cratered provinces reveal initial production functions related to impacting bodies. Based on this premise, different populations of impactors are identified in different epochs and regions of the solar system. These hypotheses are clearly crucial to interpreting planetary history and need further independent examination. The production function in the outer solar system may differ from that in the inner solar system, but it is also possible that viscous relaxation of ice craters or immediate flooding of craters that penetrate through an ice lithosphere into watery substrate may explain the greater deficiency of large craters on icy moons. This problem is controversial and needs more study.
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