X-ray electronic study of iron and of surface characteristics of the lunar regolith from Mare Crisium

Details X-ray electronic study of iron and of surface characteristics of the lunar regolith from Mare Crisium X-ray electronic study of iron and of surface characteristics of the lunar regolith from Mare Crisium

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977geokh.....1516n&link_type=abstract

Geokhimiia, Oct. 1977, p. 1516-1523. In Russian.

Computer Science

Core Sampling, Iron, Lunar Maria, Lunar Soil, X Ray Analysis, Electron Spectroscopy, Lunar Surface, Lunik Lunar Probes, Selenology, Silicon, Titanium

Scientific paper

X-ray electronic studies show that the upper layer of the Luna-24 regolith, in comparison with the lower layer, has a larger amount of unoxidized metallic iron, a larger surface-to-volume concentration of silicon, and a smaller surface-to-volume concentration of calcium. The relation of external cosmic factors to this distribution is considered. A high degree of homogeneity of the regolith surface film is indicated, and unoxidized silicon and titanium are detected in the upper layer of Luna-24 regolith (and of Luna-16 regolith also).

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