Heat flow in impact melts: Apollo 17 Station 6 Boulder and some applications to other breccias and xenolith laden melts

dc.contributor.author	Onorato, P. I. K.
dc.contributor.author	Uhlmann, D. R.
dc.contributor.author	Simonds, Charles H.
dc.coverage.spatial	Moon
dc.date.accessioned	2020-07-10T20:14:32Z
dc.date.available	2020-07-10T20:14:32Z
dc.date.issued	1976
dc.identifier.citation	Proc. Lunar Sci. Conf. 7th (1976), p. 2449-2467.	en
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1628
dc.description.abstract	Results of calculations for the cooling of an impact melt sheet are reported for the sheet sampled by the Apollo 17 Station 6 Boulder. The calculations were based on a two-stage cooling model involving a short initial phase of thermal equilibration between small clasts and the surrounding melt, and a second phase of heat loss from the melt sheet to the surroundings.	en
dc.format.extent	Pages 2449-2467
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartofseries	LSI contribution ; no. 255
dc.subject	Lunar surface samples	en
dc.subject	Breccia	en
dc.title	Heat flow in impact melts: Apollo 17 Station 6 Boulder and some applications to other breccias and xenolith laden melts	en
dc.type	Book chapter	en

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