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Impact melt breccias at the Apollo 17 landing siteImpact melt breccias are by far the most common highland rock type collected on the Apollo 17 mission. They tend to be fine grained, with virtually no clast-free impact melt rocks having been identified. All the highland boulders sampled are impact melt breccia, with the possible exception of one South Massif boulder that might have a friable matrix (but nonetheless consists dominantly of impact melt) and a shocked igneous norite boulder from the North Massif. The impact melt breccias were originally described as metaclastic, but their melt origin became apparent as work progressed. Chemical compositions appear to allow natural groupings of the impact melt breccias. Various groupings of the impact melt breccias are discussed.
Document ID
19930009621
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Ryder, Graham
(Lunar and Planetary Inst. Houston, TX, United States)
Date Acquired
September 6, 2013
Publication Date
December 2, 1992
Publication Information
Publication: Workshop on Geology of the Apollo 17 Landing Site
Subject Category
Lunar And Planetary Exploration
Accession Number
93N18810
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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