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Oxygen and bulk element abundances in Luna 20 fines
Authors:Morteza Janghorbani  David E Gillum  William D Ehmann
Institution:Department of Chemistry, University of Kentucky, Lexington, Kentucky 40506, USA
Abstract:Abundances of O, Si, Al and Mn have been determined in Luna 20 fines sample 22001,9 by instrumental neutron activation analysis. The abundances of O, Si and Al are among the highest we have observed in lunar samples and reflect a highlands origin for much of this regolith sample. The Luna 20 abundances reported here most closely resemble those we have determined in four samples of two Apollo 16 fines, rock 14310, and a clast from breccia 15459. The Luna 20 OSi ratio of 1.96 ± 0.05 is similar to that in most other lunar samples, but the AlSi ratio of 0.532 ± 0.024 is exceeded only by our data on the Apollo 16 fines. This AlSi ratio is in agreement with the value of 0.55 ± 0.06 determined by the remote X-ray fluorescence experiment for the highlands between Mare Crisium and Mare Smythii which lie near the Luna 20 site (Adleret al., 1972).
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