Paper No. 10
Presentation Time: 1:30 PM-5:30 PM
HIGH-PRESSURE RAMAN SPECTROSCOPIC STUDY OF PREHNITE, CA2AL(ALSI3O10)(OH)2
DETRIE, Theresa, ROSS, Nancy, ZHAO, Jing and ANGEL, Ross, Dept. of Geosciences, Virginia Tech, 4044 Derring Hall, Blacksburg, VA 24061, taddet@vt.edu
The mineral prehnite, Ca
2Al(AlSi
3O
10)(OH)
2 , is an important secondary mineral in mafic igneous rocks and is paired with pumpellyite as a metamorphic grade indicator between the zeolite and greenschist facies. Prehnite is a layer silicate, having alternating sheets of AlO
6 octahedra and double sheets of AlO
4/SiO
4 tetrahedra. The calcium occupies cages created by the sheets and the H atoms are bonded to the apical oxygen atoms of the AlO
6 octahedra. The average structure of prehnite, determined by Papike and Zoltai (1967), was found to be P
ncm. This structure has been confirmed in a single crystal X-ray diffraction study, using a sample of prehnite from Sterzing, Tyrol. Different space group symmetries, including P
2cm, P
2/n, and the average structure, P
ncm, arise from differences in Al/Si ordering on the tetrahedral sites. Raman experiments are underway on a suite of prehnite samples from a range of localities to determine differences that might arise from different Al/Si ordering schemes.
In addition, we report results from the first high-pressure Raman spectroscopic study of prehnite. A single crystal of prehnite from Bealetan Quarry, Fauquior County, Virginia was loaded in a diamond anvil cell along with a ruby sphere for pressure calibration. A 4:1 mixture of methanol:ethanol was used as the pressure-transmitting medium. Raman spectra were collected at ~1 GPa increments between 1 bar and 10 GPa. Fourteen peaks between 200 and 1200 cm-1 were tracked as a function of pressure and all show a slight increase in frequency as pressure increases. No discontinuities in peak positions were observed. Three peaks between 3200 and 3600 cm-1 assigned to O-H stretching modes were also tracked as a function of pressure. Between 1 bar to 8 GPa, the Raman frequencies of the O-H stretching modes increase with increasing pressure, but above 8 GPa, the O-H stretching modes display a decrease in frequency. Further work is underway to confirm and explore this intriguing result.