USRA Houston Repository

A comparison of secondary craters on the Moon, Mercury, and Mars

Show simple item record Schultz, Peter H., 1944- Singer, Jill
dc.coverage.spatial Moon
dc.coverage.spatial Mars (Planet)
dc.coverage.spatial Mercury (Planet) 2020-08-05T19:24:06Z 2020-08-05T19:24:06Z 1980
dc.identifier.citation Proc. Lunar Planet. Sci. Conf. I 11th (1980), p. 2243-2259. en
dc.description.abstract Craters on the Moon, Mars, and Mercury display contrasting styles of ejecta facies that presumably reflect different cratering environments (i.e., gravity, atmosphere, target properties). Two fundamental and distinct problems must be addressed when considering ejecta morphology: ballistic history and ejecta emplacement. On the Moon and Mercury, distinct secondary craters clearly record the effects of the ballistic history. en
dc.format.extent Pages 2243-2259
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LPI contribution ; no. 418
dc.subject Meteorite craters en
dc.subject Mars (Planet) en
dc.subject Moon en
dc.subject Mercury (Planet) en
dc.title A comparison of secondary craters on the Moon, Mercury, and Mars en
dc.type Book chapter en

Files in this item

This item appears in the following Collection(s)

  • LPI Contributions
    Documents the scientific research, meetings, and outreach products from the LPI.

Show simple item record

Search HOU Repository


My Account