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NASA NTRS · 19750061316

Heavy element affinities in Apollo 17 samples

Abstract

Pb-204, Bi, Tl, and Zn in samples from the Apollo 17 site exhibit relationships not found in samples from other sites. Pb-204, Tl, and Zn in residues remaining after dilute acid leaching are correlated with one another. Orange soil 74220, which is enriched in Pb-204, Tl, and Zn, is included in these relationships. In addition, the submicron metallic phase generally associated with agglutinate formation is correlated with all three of these elements; this relationship has already been reported for Pb-204 in other samples. Thus, orange soil and agglutinates appear to be involved in concentrating heavy volatile metals. A process other than mixing is required to account for this. As a consequence of the isolation of the landing site by the surrounding massifs, local supply and recycling of volatile trace elements in soils may account for some of the interelement relations.

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BibTeXRIS

Allen, R. O., Jr., Jovanovic, S., Reed, G. W., Jr.. 1975-09-01. Heavy element affinities in Apollo 17 samples. https://ntrs.nasa.gov/citations/19750061316

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