Lee A. Groat
Department of Geological Sciences
University of British Columbia, Cancouver, BC, Canada V6T 1Z4
Frank C. Hawthorne
Department of Geological Sciences
University of Manitoba, Winnipeg, Manitoba, Canada R3T 2N2
George R. Rossman
Division of Geological and Planetary Sciences
California Institute of Technology
Pasadena, CA 91125, U.S.A.
T. Scott Ercit
Canadian Museum of Nature
Minerals Sciences Section, Ottawa, Ontario, Canada K1P 6P4
Abstract
Many important substitutions in vesuvianite involve variable H, and
those that do not still perturb the local environment of the OH-
anions. Consequently, infrared spectroscopy of the OH fundamental and
overtone regions is an important probe of local order. We have examined
a series of vesuvianite crystals carefully characterized (by
electron-microprobe analysis, wet-chemical analysis and
crystal-structure refinement) by polarized single-crystal infrared
spectroscopy. The crystals span the complete range of chemical
variation reported in vesuvianite, and the spectra show tremendous
variability. There are 13 recognizable bands (A-M) that can be divided
into three types: (1) eight bands due to absorptions at the OH site;
these result from different local cation and anion configurations at
nearest-neighbor and next-nearest-neighbor sites; (2) four bands due to
absorption at O(10); these result from different local cation and anion
configurations at nearest-neighbor and next-nearest-neighbor sites, and
(3) a low-energy electronic absorption band. Boron is incorporated into
the vesuvianite structure primarily via the substitution B + Mg = 2H +
Al. In boron-rich vesuvianite, the four bands J-M are not present,
indicating that H has been completely replaced by B in the vicinity of
the O(10) site. Although lacking the fine detail of the
principal-stretching region , the overtone spectra are equally
characteristic of this B=H substitution. The spectra in the principal
OH-stretching region extend over a very wide spectral range (3700-3000
cm-1) and show two features that are of general importance
in the quantitative interpretation of such spectra: (1) the band width
increases significantly with decreasing band-frequency (from ~20 cm-1 at 3670 cm-1 to ~120 cm-1 at 3060 cm-1),
and (2) the band intensity is (nonlinearly) correlated with band
frequency (in addition to H content). These two features are of
significance in quantitatively fitting spectra by numerical techniques,
and in relating band intensities to compositional features.