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Evidence for ancient mare volcanismThe results of the present study suggest that dark-haloed impact craters are indicative of excavated mafic materials, originally emplaced as volcanic units, but subsequently buried by impact ejecta deposits from large craters and basins. Consequently, mapped light plains units should be viewed as soil units that may not reflect the origin of the underlying rock. Some observations which support these conclusions are examined.
Document ID
19800039556
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Schultz, P. H.
(Lunar and Planetary Institute Houston, Tex., United States)
Spudis, P. D.
(Arizona State University Tempe, Ariz., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 19, 1979
End Date: March 23, 1979
Accession Number
80A23726
Funding Number(s)
CONTRACT_GRANT: NSR-09-501-001
Distribution Limits
Public
Copyright
Other

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