Cathodoluminescence microscopy and spectroscopy of plagioclases from lunarsoil

Cathodoluminescence (CL) microscopy and spectroscopy of single plagioclase grains from lunar soil show that plagioclases from Luna 20 (highland) have more or less homogeneous CL with both blue or green colors, whereas plagioc lase grains sampled by Luna 24 (mare) luminesce dominantly green with parti ally distinct oscillatory zoning. The three main emission bands in the blue (similar to 450 nm), green (similar to 560 nm), and red-IR (similar to 690 nm), mimic the most common emission bands in terrestrial feldspars. Mn2+ i s the most important activator element in lunar plagioclases. Variations in the amount of structurally incorporated Mn2+ cause variations in the inten sity of the green emission band at 560 nm, in some cases resulting in zonin g of the CL intensity within single crystals. Calculations by a combination of quantitative spectral analysis of CL emission and PIXE measurements yie ld Mn concentrations of 7-47 ppm. The intense intrinsic emission band at 45 0 nm (probably an Al-O--Al center), which was especially prominent in Luna 20 plagioclases, causes their blue CL color. The occurrence of a CL emissio n band at similar to 690 nm in plagioclases from Luna 24 samples confirms t hat Fe3+-activated CL is common in these grains. The results indicate that at least some of the Fe in Luna 24 plagioclases is Fe3+, whereas all Luna 2 0 plagioclases have Fe3+-near the CL detection Limit of about 0.1 ppm.