Endogenic Cratering Distribution on the Moon

Details Endogenic Cratering Distribution on the Moon Endogenic Cratering Distribution on the Moon

Jan 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.241..186g&link_type=abstract

Nature, Volume 241, Issue 5386, pp. 186-187 (1973).

Physics

1

Scientific paper

WITHIN the cratering distribution for the Hyginus Rille floor, the chain craters represent a distribution which is distinctly different from that resulting by impact of interplanetary debris. It has been postulated1-7 that Hyginus Rille was controlled in its development by tectonic activity along a graben zone, and some investigators1-5,7-10 have suggested that these chain craters are volcanic in origin.

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