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Lunar highlands breccias generated by major impactsLunar missions are reported which have returned a variety of different types of breccias. These rocks differ greatly in their mechanisms of formation, source materials, and histories after formation; but all are related in that all were generated by impact processes. The impact processes involved in the formation of several major types of breccias are discussed. Some types that may have originated in large impacts are identified. Such breccias are extremely important. The impacts that formed them penetrated deeply into, and perhaps through the lunar crust and brought up materials that had previously experienced little or no impact modification. Detailed studies of such breccias can permit partial reconstruction of their preimpact source terranes and yield information on the nature of the early lunar crust (and possibly the upper mantle as well).
Document ID
19750006609
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
James, O. B.
(Geological Survey Reston, VA, United States)
Date Acquired
September 3, 2013
Publication Date
January 1, 1974
Publication Information
Publisher: NASA
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
REPT-212
NASA-CR-141172
Report Number: REPT-212
Report Number: NASA-CR-141172
Meeting Information
Meeting: Sov.-Am. Conf. on the Cosmochem. of the Moon and Planets
Location: Moscow
Country: Soviet Union
Start Date: June 4, 1974
End Date: June 8, 1974
Accession Number
75N14681
Funding Number(s)
CONTRACT_GRANT: NASA ORDER T-2357-A
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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