Distribution of iron in lunar olivines from data of Moessbauer spectroscopy

Details Distribution of iron in lunar olivines from data of Moessbauer spectroscopy Distribution of iron in lunar olivines from data of Moessbauer spectroscopy

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989geokh.....1164k&link_type=abstract

Geokhimiia (ISSN 0016-7525), Aug. 1989, p. 1164-1169. In Russian.

Computer Science

Iron Compounds, Lunar Maria, Mossbauer Effect, Olivine, Geochemistry, Histograms, Lunar Geology

Scientific paper

Phase distributions of Fe in lunar olivines were determined using the method of Zemcik and Raclavsky (1976), which made it possible to obtain Moessbauer spectra of individual 0.2-0.3-mm particles in lunar-regolith samples. It was found that the distribution of iron in lunar olivines cannot be characterized statistically. Olivines obtained from both the lunar-maria and highland regions were found to be characterized by similar T-P(O2) conditions of formation.

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