An investigation of a superfine fraction of the lunar regolith

Details An investigation of a superfine fraction of the lunar regolith An investigation of a superfine fraction of the lunar regolith

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983geokh.....1481r&link_type=abstract

Geokhimiia (ISSN 0016-7525), Oct. 1983, p. 1481-1484. In Russian.

Physics

Condensed Matter

Fractions, Lunar Soil, Particle Size Distribution, Regolith, Fines, Impact Damage, Metal Oxides, Mineralogy

Scientific paper

A fraction of less than 10 microns can form through the breakup (from impacts) of lunar rocks; it can also result from material produced through breakup in another area which is transported over the lunar surface. Another possibility is condensed matter formed from the melting (from impact), evaporation, and condensation of lunar matter. Methods that have been developed for separating fine fractions are described, and results are presented from an analysis of the morphology and chemical composition of individual particles.

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