TY - JOUR
T1 - Thermoelastic behaviour of silicate perovskites
T2 - Insights from new high-temperature ultrasonic data for ScAlO3
AU - Jackson, Ian
AU - Kung, Jennifer
N1 - Funding Information:
We thank Lara Weston for her careful conduct and thorough analysis of the data from the high-temperature ultrasonic experiments, Harri Kokkonen for SEM characterisation of the ScAlO 3 specimen and measurement of its density, Craig Saint for maintenance of the internally heated pressure vessel and lapping of the specimen, and Lars Stixrude for guidance in the use of the Stixrude and Lithgow-Bertelloni (2005) model. This research was supported by funding from the Australian Research Council (LX0348106) and partially by a NSF grant (INT 02-33849) to R.C. Liebermann for a collaborative research program with the Australian National University.
PY - 2008/4
Y1 - 2008/4
N2 - (Mg,Fe,Al)(Si,Al)O3 perovskite, stable only at pressures >20 GPa, is the dominant mineral of the Earth's lower mantle and thus controls its physical properties including seismic wave speeds. However, the development of a thorough understanding of the thermoelastic behaviour of this silicate perovskite is compromised by its marginal metastability on recovery at ambient conditions. Study of the close structural analogue ScAlO3, stable at much lower pressure, has the potential to provide insight into the behaviour of its silicate cousin. Here, previous exploratory ultrasonic measurements of the compressional and shear wave speeds on a fine-grained polycrystalline specimen have been extended to 1000 K under 300 MPa confining pressure within an internally heated gas-medium high-pressure apparatus. The wave speeds and derived bulk and shear moduli vary approximately linearly with temperature with derivatives (∂KS/∂T)P = -21.3(3) MPa K-1 and (∂G/∂T)P = -19.0(1) MPa K-1, respectively. The new data, along with previous measurements of thermal expansion and the pressure dependence of the elastic moduli, have been assimilated into the comprehensive internally consistent finite-strain model of thermoelastic behaviour proposed by [Stixrude, L., Lithgow-Bertelloni, C., 2005. Thermodynamics of mantle minerals-I. Physical properties. Geophys. J. Int. 162, 610-632]. Comparison of the newly constrained model for ScAlO3 with emerging data for MgSiO3 perovskite provides guidance in the analysis of the chemical composition and temperature of the Earth's lower mantle.
AB - (Mg,Fe,Al)(Si,Al)O3 perovskite, stable only at pressures >20 GPa, is the dominant mineral of the Earth's lower mantle and thus controls its physical properties including seismic wave speeds. However, the development of a thorough understanding of the thermoelastic behaviour of this silicate perovskite is compromised by its marginal metastability on recovery at ambient conditions. Study of the close structural analogue ScAlO3, stable at much lower pressure, has the potential to provide insight into the behaviour of its silicate cousin. Here, previous exploratory ultrasonic measurements of the compressional and shear wave speeds on a fine-grained polycrystalline specimen have been extended to 1000 K under 300 MPa confining pressure within an internally heated gas-medium high-pressure apparatus. The wave speeds and derived bulk and shear moduli vary approximately linearly with temperature with derivatives (∂KS/∂T)P = -21.3(3) MPa K-1 and (∂G/∂T)P = -19.0(1) MPa K-1, respectively. The new data, along with previous measurements of thermal expansion and the pressure dependence of the elastic moduli, have been assimilated into the comprehensive internally consistent finite-strain model of thermoelastic behaviour proposed by [Stixrude, L., Lithgow-Bertelloni, C., 2005. Thermodynamics of mantle minerals-I. Physical properties. Geophys. J. Int. 162, 610-632]. Comparison of the newly constrained model for ScAlO3 with emerging data for MgSiO3 perovskite provides guidance in the analysis of the chemical composition and temperature of the Earth's lower mantle.
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U2 - 10.1016/j.pepi.2008.04.005
DO - 10.1016/j.pepi.2008.04.005
M3 - Article
AN - SCOPUS:44349150911
SN - 0031-9201
VL - 167
SP - 195
EP - 204
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
IS - 3-4
ER -