The petrology and chemistry of basaltic fragments from the Apollo 11 soil - IA study of basaltic fragments from the Apollo 11 bulk sample using instrumental neutron activation analysis, the petrographic microscope, and the electron microprobe is presented. The fragments include Group A, B2, and B3 basalts, of which two of the Group A samples are vitrophyres with bulk compositions similar to the crystalline high-K rocks which crystallized under different physical conditions and represent a second high-K cooling unit. The B2 samples relate to each other through ilmenite fractionation, and the B3 samples relate through olivine fractionation; it is concluded that the B2 samples have an anomalously high La/K ratio and may have generated in the same source region as the Group D basalts.
Document ID
19800039389
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Beaty, D. W. (California Inst. of Tech. Pasadena, CA, United States)
Hill, S. M. R. (California Inst. of Tech. Pasadena, CA, United States)
Albee, A. L. (California Institute of Technology Pasadena, Calif., United States)
Ma, M.-S. (California Inst. of Tech. Pasadena, CA, United States)
Schmitt, R. A. (Oregon State University Corvallis, Ore., United States)