HR: 09:00h
AN: V41B-05    [PDF]
TI: Kawai-type apparatus equipped with sintered diamond and its application to melting of mantle materials
AU: * Ito, E
EM: eiito@misasa.okayama-u.ac.jp
AU: Kubo, A
EM: akubo@misasa.okayama-u.ac.jp
AU: Katsura, T
EM: tkatsura@misasa.okayama-u.ac.jp
AU: Walter, M J
EM: mjwalter@lbl.gov
AB: Kawai-type (the 6-8 type) of multi-anvil apparatus has been widely used in the mineral physics because of its versatile abilities such as large volume and pressure environment of high hydrostacity. However, it has been realized for last two decades that the maximum attainable pressure is limited to ca. 27 GPa when using tungsten carbide (WC) as anvil material. We have tried to extend capability of Kawai-type apparatus by adopting sintered diamond (SD) cubes of 14 mm edge length with 1.5 or 2.0 mm truncations together with an octahedral magnesia pressure medium. Recently generated pressures of 54 GPa and 40 GPa were confirmed for 1.5 and 2.0 mm truncations, respectively, at room temperature based on the MgO pressure scale. Following above technical innovation, we have carried out melting experiments on peridotite and CI model mantle material up to 35 GPa to examine the hypothesis for crystal fractionation in deep magma ocean in early stage of the Earth's history. Powdered starting material was put directly into a small cylindrical Re heater, which was set in the octahedron with a LaCrO3 sleeve. The sample was heated to ca. $2500\deg$C for 2-3 min at the prescribed load. The quenched products were made to polished sections, which were examined by electron microscopy and then analyzed by the electron probe micro analyzer. In peridotite, ferropericlase (Fp) is the liquidus phase up to about 30 GPa. Both Fp and Mg-perovskite (Mg-Pv), however, coexist on the liquidus at 31 GPa, indicating multiple saturation of these phases. At higher than 32 GPa the front of Fp grains moves back from the liquidus to the slightly lower temperature region and Mg-Pv becomes the liquidus phase. Ca-perovskite (Ca-Pv) crystallizes at a fairly lower temperature than Fp and Mg-Pv at pressures up to ca. 29 GPa. However the crystallization temperatures of Fp and Ca-Pv become closer with increasing pressure, and the former might be only a few degrees higher than the latter at 33 GPa. In CI mantle, on other hand, liquidus phase changes from majorite (Mj) to Fp in pressures of 23-25 GPa. At higher than 28 GPa, Mj and Fp completely disappear in the super solidus region, and the liquidus phase is Mg-Pv followed down temperature by Ca-Pv. Differentiation by crystal fractionation of Mg-Pv, Fp, and Ca-Pv in a deep magma ocean has been examined for a CI chondritic and two peridotitic bulk silicate Earth models, using chemical compositions of theses phases coexisted with melt in peridotite charge at 33 GPa. Mass balance indicates that subtraction of about 40 percent Mg-perovskite and 2 percent Ca-perovskite from a CI chondritic bulk silicate Earth yields a residual melt close to a model fertile upper mantle composition. A crystal layer composed of Mg- and Ca-perovskites would pile up to a depth about 1400 km, and may be characterized as an enriched and possibly heat-producing reservoir by the high capability of Ca-perovskite to accommodate large cations such as La and alkaline elements. For peridotitic bulk silicate Earth models, fractionation would be quite limited, up to 10 percent of Mg-perovskite in addition to trace amount of Ca-Pv.
DE: 3630 Experimental mineralogy and petrology
DE: 3924 High-pressure behavior
DE: 3994 Instruments and techniques
SC: Volcanology, Geochemistry, Petrology [V]
MN: 2003 Fall Meeting