Petrographic and ferromagnetic resonance studies of the Apollo 15 deep drill coreDetailed petrographic grain size, and ferromagnetic resonance studies were performed on a representative suite of samples from the Apollo 15 deep drill core. Petrographic analyses of the 90-150 micron size fraction show a subtle upward increase in the ratio of mare to highland components. The agglutinate content at the FMR intensity normalized to FeO show that the soils in the core are generally immature to submature. The most striking feature shown by the maturity indices is a systematic decrease in maturity from the lunar surface to a depth of about 40 cm. Although other mechanisms are possible, the downward decrease in maturity can be attributed to in situ reworking over a time span of 400 m.y. at a 50% probability.
Document ID
19770051806
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Heiken, G. H. (California, University Los Alamos, N. Mex., United States)
Morris, R. V. (Los Alamos Scientific Lab. NM, United States)
Mckay, D. S. (Los Alamos Scientific Lab. NM, United States)
Fruland, R. M. (NASA Johnson Space Center Houston, Tex., United States)