Some compositional aspects of lunar regolith evolution

Details Some compositional aspects of lunar regolith evolution Some compositional aspects of lunar regolith evolution

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977rspta.285..293r&link_type=abstract

(Royal Society, Discussion on the Moon - A New Appraisal from Space Missions and Laboratory Analyses, London, England, June 9-12

Computer Science

18

Lunar Composition, Lunar Rocks, Lunar Soil, Selenology, Basalt, Chemical Composition, Lunar Landing Sites, Lunar Mantle, Lunar Maria, Massifs, Meteorite Collisions, Transport Properties

Scientific paper

An attempt is made to relate compositional characteristics of lunar regolith bulk soil to regolith dynamics, with particular reference to problems concerning lateral movement of soil components in response to meteoroid bombardment, and to the source of apparently exotic material in mare soils. Contradictory lines of evidence regarding the effectiveness of impact-related lateral transportation of regolith components are stressed. Detailed studies of specific landing sites at mare-highland boundaries reveal that lateral transportation is an inefficient process and that most of the soil is of local derivation. However, many mare soils contain substantial amounts of feldspathic, apparently highland-derived components, implying an effective transport mechanism.

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