Effects of maturation on the reflectance of the lunar regolith: Apollo 16 - A case study

Details Effects of maturation on the reflectance of the lunar regolith: Apollo 16 - A case study Effects of maturation on the reflectance of the lunar regolith: Apollo 16 - A case study

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975moon...13..293a&link_type=abstract

(Lunar Science Institute, Symposium on Origin and Evolution of the Lunar Regolith, Houston, Tex., Nov. 13-15, 1974.) The Moon, v

Physics

8

Apollo 16 Flight, Lunar Landing Sites, Lunar Rocks, Lunar Soil, Spectral Reflectance, Agglutination, Breccia, Fragments, Minerals

Scientific paper

Soils at the Apollo 16 site become progressively darker as the percentage of glassy agglutinates increases. Magnetic separates of the agglutinate fraction of a soil are always darker than the bulk soil and are darker than the nonagglutinate fraction consisting of rock and mineral fragments. Darkening of a soil with maturity is due mainly to the increasing proportion of agglutinates. Coating of rock and mineral fragments with thin deposits of glass aids darkening in a minor way, but most of these particles eventually are destroyed by melting as the soils mature.

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