NEAR INFRARED SPECTROSCOPY OF WHITE MICA AND IMPLICATIONS FOR METAMORPHISM IN THE BLACK HILLS, SOUTH DAKOTA
Field spectra of 1953 rock samples were acquired in greenschist and lower amphibolite facies metapelitic and metapsammic rocks in the Black Hills. The wavelength of the Al-OH band shifts from 2218 nm in the biotite zone to 2195 nm in the staurolite zone in response to substitutions in the octahedral layer of white mica. The principal substitution is the aluminoceladonite exchange [(Mg,Fe)2+Oct + Si4+Tet = Al3+Oct + Al3+Tet] which drives white mica to more Al-rich composition as metamorphic temperature increases. When mapped out, variation of Al-OH values follow regional metamorphic patterns in the Black Hills, demonstrating the potential to detect and map metamorphic intensity in similar terranes.
In addition to field spectra, 45 polished thin sections were prepared from representative samples for further petrologic analysis through optical microscopy and scanning electron microscopy coupled with energy-dispersive X-ray spectroscopy. Samples cover the geographic distribution of the study area and span the complete range of Al-OH wavelength values. White mica with wavelengths spanning 2217 to 2196 nm showed a linear increase in AlOct from ~1.62 to ~1.92 cations per 11 O and a linear decrease in (Fe+Mg)Oct from ~0.42 to ~0.09 cations per 11 O. Samples with anomalously lower wavelength values than regional trends are strongly correlated with increasing interlayer Na content in the white micas, up to ~0.22 Na/(K+Na). However, the wavelength for these samples remain consistent with white mica AlOct content variation.