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Thermal model for impact breccia lithification: Manicouagan and the moon

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dc.contributor.author Simonds, Charles H.
dc.contributor.author Warner, Jeffrey L.
dc.contributor.author Phinney, William C.
dc.contributor.author McGee, Patricia E.
dc.coverage.spatial Canada
dc.date.accessioned 2020-07-09T20:40:40Z
dc.date.available 2020-07-09T20:40:40Z
dc.date.issued 1976
dc.identifier.citation Proc. Lunar Sci. Conf. 7th (1976), p. 2509-2528. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1623
dc.description.abstract This paper extends the thermal model of Simonds to the full spectrum of impact-produced rocks ranging from fragmental breccias to impact melts. This is done by relating the basic textural features of impact-lithified rocks to variations in the mixture, of superheated impact-fused material originating near the point of impact and much cooler fragmented debris originating farther from the point of impact. en
dc.format.extent Pages 2509-2528
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LSI contribution ; no. 250
dc.subject Meteorite craters--Québec (Province) en
dc.subject Meteorite craters--Québec (Province) en_
dc.title Thermal model for impact breccia lithification: Manicouagan and the moon en
dc.type Book chapter en


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