A new Monte Carlo model of lunar megaregolith development.

Physics

Scientific paper

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Moon:Evolution, Moon:Impact Craters

Scientific paper

A new Monte Carlo model is used to examine the development of the lunar megaregolith through impact cratering processes. This improved model predicts greater minimum megaregolith thickness than did the earlier models. If the 25 km seismic horizon on the moon is attributable to the bottom of the crater-excavated material, then the highlands appear to have suffered a bombardment of two to five times the number of craters presently preserved on the surface.

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