Micrometeoroid abrasion of lunar rocks: A Monte Carlo simulation

dc.contributor.author	Hörz, Friedrich, 1940-
dc.contributor.author	Schneider, Eberhard
dc.contributor.author	Hill, Richard E.
dc.coverage.spatial	Moon
dc.date.accessioned	2020-07-07T18:53:03Z
dc.date.available	2020-07-07T18:53:03Z
dc.date.issued	1974
dc.identifier.citation	Proceedings of the Fifth Lunar Conference (Supplement 5, Geochimica et Cosmochimica Acta) Vol. 3 pp. 2397-2412 (1974)	en
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1615
dc.description.abstract	A Monte Carlo computer model was developed to simulate impact histories and erosion by single particle abrasion of lunar rock surfaces. Microcrater frequencies derived from lunar rocks were used to calculate magnitude and probability of each cratering event.	en
dc.format.extent	Pages 2397-2412
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartofseries	LSI contribution ; no. 193
dc.subject	Lunar petrology	en
dc.subject	Lunar surface samples	en
dc.title	Micrometeoroid abrasion of lunar rocks: A Monte Carlo simulation	en
dc.type	Book chapter	en

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