Petrographic Diversity in Apollo 12 Regolith Lithic Fragments

S. M. Seddio, R. L. Korotev, B. L. Jolliff, and R. A. Zeigler
Department of Earth and Planetary Sciences and
McDonnell Center for the Space Sciences
Advisor: R. L. Korotev


Abstract
The Apollo 12 regolith is composed of a variety of mare and nonmare lithologies. Most are mare basalts, regolith breccias, and impact melt breccias. Rarer lithologies include brecciated anorthosites, granites, and alkali anorthosites. As part of a survey of 2-4-mm lithic fragments from the Apollo 12 regolith [1,2], we identified several unusual fragments. One such fragment is 12032,366-19, a unique 21-mg granite which contains plagioclase that has the lowest An-value of which we are aware for any lunar sample. 12032,366-19 is the result of extreme lunar melt fractionation. This work demonstrates the diversity of lithologies found in the Apollo 12 regolith.
Stephen Seddio is from Hamlin, NY, and is a graduate student in the Department of Earth and Planetary Science at Washington University in St. Louis. Stephen specializes in Lunar Petrology and Geochemistry.
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