Abstract
We have determined major (Si, Zr, Hf), minor (Al, Y, Fe, P), and trace element (Ca, Sc, Ti, Ba, REE, Th, U) concentrations and Raman spectra of a zoned, 200 μm zircon grain in lunar sample 14161,7069, a quartz monzodiorite breccia collected at the Apollo 14 site. Analyses were obtained on a thin section in situ with an ion microprobe, an electron microprobe, and a laser Raman microprobe. The zircon grain is optically zoned in birefringence, a reflction of variable (incomplete) metamictization resulting from zonation in U and Th concentrations. Variations in the concentrations of U and Th correlate strongly with those ofother high-field-strength trace elements and with changes in Raman spectral parameters. Concentrations ofU and Th range from 21 to 55 ppm and 6 to 31 ppm, respectively, and correlate with lower Raman peak intensities, wider Raman peaks, and shifted Si-O peak positions. Concentrations of heavy rare earth elements range over a factor of three to four and correlate with intensities offluorescence peaks. Correlated variations in trace element concentrations reflect the original magmatic differentiation of the parental melt∼4 b.y. ago. Degradation of the zircon structure, as reflected by the observed Raman spectral parameters,has occurred in this sample over arange of a-decay event dose from ∼5.2 × 1014 to 1.4 × 1015 decay eventsper milligram of zircon, as calculated from the U and Th concentrations. This dose is well below the ∼1016 events per milligram cumulative dose that causes complete metamictization and indicates that laser Raman microprobe spectroscopy is an analytical technique that is very sensitive to the radiation-induced damage in zircon.