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Meteoritic and non-meteoritic trace elements in Luna 16 samples
Authors:JC Laul  R GanapathyJohn W Morgan  Edward Anders
Institution:Department of Chemistry and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637,USA
Abstract:Two Luna 16 soils have been analyzed for Ag, Au, Bi, Br, Cd, Co, Cs, Cu, Ga, Ge, In, Ur, Ni, Rb, Re, Sb, Se, Te, Tl, and Zn. A meteoritic component similar to that in Apollo 11 and 12 soils seems to be present, corresponding to ∼1.5 to 2% Cl chondrites or equivalent. It probably consists largely of micrometeorites. Three elements show strong enrichments compared to Apollo 11 and 12 soils: Cd (5× to 200×), Ag (5× to 10×), and Bi (3×). Presumably these elements were brought in by Cd-Ag-Bi rich material, similar to that in Unit VI of Apollo core 12028.
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