Pre-Imbrian craters and basins: Ages compositions and excavation depths of Apollo 16 breccias

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Abundance, Apollo 16 Flight, Lunar Craters, Lunar Rocks, Radioactive Age Determination, Anorthosite, Argon Isotopes, Chemical Composition, Lithology, Petrography, Trace Elements

Scientific paper

Breccia fragments were analyzed from the 2-4 mm sieve fraction of three Apollo 16 soils collected in the vicinity of North Ray Crater. The Ar39-Ar40 ages, Ar37-Ar38 exposure ages, abundances of major and certain trace elements, and petrographic data relevant to thermal history were obtained for up to 48 individual fragments. Among the samples, 30 gave Ar39-Ar40 release patterns that allowed the assignment of a high- or intermediate-temperature plateau age and the recognition of three age groups. The oldest fragments are all anorthositic metamorphosed breccias of light-matrix type. The younger fragments are noritic anorthosite and anorthositic norite breccias with textures indicative of greater annealing (melted matrix), one totally melted sample being of KREEP-basalt texture. The very young fragments are chiefly of glass or devitrified glass. The results are interpreted as reflecting two magnitudes of cratering.

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