Single-crystal IR- and UV/VIS-spectroscopic measurements
on transition metal bearing pyrope: the incorporation of hydroxide in garnet
Charles A. Geiger, Andreas Stahl
Institut für Geowissenschaften der Christian-Albrechts-Universität
zu Kiel, Olshausenstraße 40, 24098 Kiel, Germany
George R. Rossman
Division of Geological and Planetary Sciences, California Institute of Technology,
Pasadena, CA 91125, U.S.A.
European Journal of Mineralogy 12, 259-271
Abstract
Pyrope single crystals doped with transition-metal ions (Co, Cr, Ni, Ti
and V) were synthesised in a piston-cylinder device at 950 - 1050ºC and 25
kbar. Stoichiometric oxide mixtures were used as starting materials and distilled
water was used as a fluid flux. Crystals up to 2 mm in size were grown. Microprobe
analysis and optical absorption spectroscopy were used to determine on which
positions and in which oxidation states the transition-metal ions are incorporated
in the pyrope structure. Cr3+-ions occupy the octahedral site and
Co2+ and Ni2+ the dodecahedral site. Although extra
metallic Ti was included in the synthesis of Ti-bearing pyropes, only Ti4+
and no measurable Ti3+ could be stabilised on the octahedral
site. The optical absorption spectra of V-bearing pyropes show, in addition
to the spin-allowed dd-transitions 3T1g(F)-
3T2g(F) at 17000 cm-1 and 3T1g(F)-
3T1g(P) at ~20000 cm-1 corresponding to V3+ in the octahedral
site, absorption bands which are thought to be caused by dd-transitions of
V3+ in the tetrahedral site and V4+ in octahedral and
tetrahedral sites. V4+ was not observed in silicate garnets before.
IR spectra in the OH- stretching region between 4000 and 3000 cm-1,
obtained on pyrope single-crystals which only contain divalent and trivalent
transition-metal ions like Ni2+, Co2+, and Cr3+,
are similar to that normally shown by end-member pyrope (Geiger et al., 1991).
At room temperature the spectra show a single band at ˜ 3630 cm-1,
which splits at ~79 K into two bands of smaller FWHM’s at ˜ 3618 cm-1
and 3636 cm-1. These bands are assigned to OH--stretching
modes resulting from the hydrogarnet substitution. The spectra of Ti4+-bearing
pyrope measured at 298 K show four OH--stretching bands at approximately
3686, 3630, 3567 and 3527 cm-1. At ~79 K the band at 3630 cm-1
splits into two narrow bands at 3636 cm-1 and 3614 cm-1.
This suggests that additional OH- substitutional mechanisms occur
in Ti-containing garnets. In the IR spectrum of a V4+-bearing pyrope the same
number of OH--stretching bands is observed, suggesting that higher
charged cations cause additional OH- substitutions and increased
OH- concentrations in garnet. The IR spectra of most natural pyrope-rich
garnets appear to be different from those of the synthetics, which suggests
that they are not characterised by the hydrogarnet substitution. However,
the OH--substitution mechanism and concentrations in garnets from
grospydite or similar parageneses are similar to those of the synthetics,
which may reflect their formation in water-rich environments.