HR: 0800h
AN: MR11A-0887    [Abstracts]
TI: High-pressure, high-temperature Raman spectroscopic study of ilmenite-type MgSiO$_{3}$, MgGeO$_{3}$ and MgTiO$_{3}$
AU: * Okada, T
EM: okataku@ess.sci.osaka-u.ac.jp
AF: Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka, 560-0043 Japan
AU: Narita, T
EM: narita@ess.sci.osaka-u.ac.jp
AF: Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka, 560-0043 Japan
AU: Yamanaka, T
EM: yamanaka@hpc.cmc.osaka-u.ac.jp
AF: Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka, 560-0043 Japan
AU: Nagai, T
EM: nagai@ep.sci.hokudai.ac.jp
AF: Division of Earth and Planetary Sciences, Graduate School of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo, Hokkaido, 060-0810 Japan
AB: Ilmenite-type MgSiO$_{3}$ is a high-pressure polymorph of enstatite, and characterized by a relatively narrow stability field in the 20-24 GPa and 1370-2270 K range. Since MgSiO$_{3}$-ilmenite is stable at thermodynamically low temperature, it is considered to be a candidate component in 600-700 km of subducting slabs. It is important for earth science to understand its crystal structure on the basis of lattice vibrations at high pressure and temperature. High-pressure and high-temperature Raman spectra of ilmenite-type MgSiO$_{3}$ have already been collected up to 7 GPa and 1030 K, respectively (Reynard and Rubie, 1996). In this study, we conducted a high-pressure, high-temperature Raman spectroscopic study of ilmenite-type MgSiO$_{3}$, MgGeO$_{3}$ and MgTiO$_{3}$. From the viewpoint of elasticity and bonding energy, we investigate the behavior of ilmenite at high-pressure and high-temperature and compare structures of ilmenites that have different compositions. Raman spectroscopy was a NRS2100 triple microspectrometer equipped with Ar ion laser (operating at 514.5 nm and 70-80 mW). High-temperature experiments were performed using a Pt-electric resistant heater. Temperature was monitored with chromel-almel thermocouples. For the high-pressure experiments, a diamond-anvil cell (DAC) was used. H$_{2}$O was preferred to an alcohol mixture as the pressure media because it has no strong Raman bands in the measured region. Pressures were determined from the shift of the ruby fluorescence R$_{1}$ line, excited by the Ar ion laser. Raman spectra of each sample were collected up to 770 K at ambient pressure and 30 GPa at room temperature, respectively. For ilmenite, 10 bands were expected from symmetry analysis (five A$_{g}$ and five E$_{g}$). At ambient conditions, we could observe seven (for MgSiO$_{3}$), eight (for MgGeO$_{3}$) and nine (for MgTiO$_{3}$) Raman bands, respectively. With increasing temperature, each band shifted to lower wavenumber. The temperature dependence of the force constant, k, was the order of MgGeO$_{3}$, MgSiO$_{3}$ and MgTiO$_{3}$. The tendency induces the relative expansion rate for each XO$_{6}$ (X=Si,Ge,Ti) octahedron. This is consistent with the fact that MgTiO$_{3}$ ilmenite is the only stable phase up to 770 K at ambient pressure in this study. With increasing pressure at room temperature, each Raman band shifted to higher wavenumber. We also discuss the pressure dependence of the force constant, k.
DE: 3630 Experimental mineralogy and petrology
DE: 3924 High-pressure behavior
DE: 3934 Optical, infrared, and Raman spectroscopy
SC: Mineral and Rock Physics [MR]
MN: 2004 AGU Fall Meeting