Random bombardment by comets, asteroids and associated fragments form and alter the lunar surface and other rocky surfaces.
The accumulation of impact craters over time is of fundamental use in evaluating the relative ages of geologic units, researchers said.
Crater counts and radiometric ages from returned samples help derive age estimates for unsampled units on the Moon and other Solar System objects.
Researchers at the Arizona State University and Cornell University in the US analysed 'before and after' image pairs taken by NASA's Lunar Reconnaissance Orbiter Camera (LROC).
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They quantified the contemporary rate of crater production on the Moon, to unveil previously unknown details of impact-induced jetting, and to identify a secondary impact process that is rapidly churning the regolith - the layer of unconsolidated solid material covering the lunar bedrock.
"We identified broad reflectance zones associated with the new craters that we interpret as evidence of a surface-bound jetting process," researchers said.
"We also observe a secondary cratering process that we estimate churns the top two centimetres of regolith on a timescale of 81,000 years - more than a hundred times faster than previous models estimated from meteoritic impacts (ten million years)," they said.
The study was published in the journal Nature.
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