Isotope analysis of crystalline impact melt rocks from Apollo 16 stations 11 and 13, North Ray Crater

Details Isotope analysis of crystalline impact melt rocks from Apollo 16 stations 11 and 13, North Ray Crater Isotope analysis of crystalline impact melt rocks from Apollo 16 stations 11 and 13, North Ray Crater

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985lpsc...15..431r&link_type=abstract

(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 15th, Houston,

Mathematics

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4

Apollo 16 Flight, Impact Melts, Isotopes, Lunar Craters, Lunar Rocks, Electron Microscopy, Kreep, Mass Spectroscopy, Mineralogy, Neodymium Isotopes, Rubidium Isotopes, Samarium Isotopes, Strontium Isotopes, Moon, Samples, Lunar, Isotopes, Analysis, Crystalline, Impacts, Melts, Apollo 16, Station 11, Station 13, North Ray, Craters, Dating Methods, Isotopic Ratios, Ages, Rubidium, Strontium, Samarium, Imbrium Mare, Neodymium, Isochrons, 67747, 67559, Kreep, Models, Calculations, Melting, Crust, Evolution, His

Scientific paper

The North Ray Crater Target Rock Consortium was formed to study a large number of rake samples collected at Apollo 16 stations 11 and 13 with comparative chemical, mineralogical, and chronological techniques in order to provide a larger data base for the discussion of lunar highland evolution in the vicinity of the Apollo 16 landing region. The present investigation is concerned with Rb-Sr and Sm-Nd isotopic analyses of a number of whole-rock samples of feldspathic microporhyritic (FM) impact melt, a sample type especially abundant among the North Ray crater (station 11) sample collection. Aspects of sample mineralogy and analytical procedures are discussed, taking into account FM impact melt rocks 6715 and 63538, intergranular impact melt rock 67775, subophitic impact melt rock 67747, subophitic impact melt rock 67559, and studies based on the utilization of electron microscopy and mass spectroscopy.

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