日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT03_29AM2] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 11:00 〜 12:45 418 (4F)

コンビーナ:*田中 聡(海洋研究開発機構 地球内部ダイナミクス領域)、芳野 極(岡山大学地球物質科学研究センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、ヘルンランド ジョン(東京工業大学 地球生命研究所)、座長:亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、竹内 希(東京大学地震研究所)

11:30 〜 11:45

[SIT03-10] 1600~2200℃における660 km地震波不連続面付近のパイロライトの相転移と鉱物化学

*石井 貴之1糀谷 浩1赤荻 正樹1 (1.学習院大学理学部)

キーワード:ポストスピネル転移, 660 km地震波不連続面, マントルプリューム, パイロライト, ポストガーネット転移

It is widely accepted that pyrolite is a model rock which represents the chemical composition of the Earth's upper mantle. Because the post-spinel transition in pyrolite occurs at about 23 GPa along mantle geotherm (e.g. Litasov et al. 2005), it has been accepted that the transition is responsible for the seismic 660-km discontinuity. Slow velocity anomalies by global seismic tomography which may indicate mantle upwelling have been found in the transition zone and the lower mantle, and these regions are higher in temperature than average mantle. To elucidate the origin and dynamics of the mantle plume, informations on phase relations in pyrolite are essential. However, few investigations on phase relations in pyrolite have been made at hot-plume temperatures (1800-2200C) (Hirose, 2002; Nishiyama and Yagi, 2003). In this study, we demonstrated detailed phase equilibrium experiments in pyrolite composition at hot plume conditions.The starting material was prepared as the oxide mixture in pyrolite composition after McDonugh and Sun (1995) excluding minor components (MnO, K2O and P2O5). Quench experiments were made at about 20-28 GPa and 1600-2200C for 2-10 hours using a Kawai-type 6-8 multianvil high-pressure apparatus at Gakushuin University. The starting material was packed with pressure calibrants (MgSiO3 and pyrope) in a Re multi-sample capsule. A LaCrO3 heater and a W5%Re-W26%Re thermocouple were inserted in a Cr2O3-doped MgO pressure medium. Phases of recovered samples were identified with microfocus-Xray diffractometer and SEM-EDS.The mineral assemblages of MgSiO3-rich perovskite (Mpv) + magnesiowustite (Mw) + garnet (Gt) + CaSiO3-perovskite (Cpv) and Mpv + Mw + Cpv at 1600-2200C are stable at pressure range of 22-24 GPa and above 24 GPa, respectively. The mineral assemblage of ringwoodite (Rw) + Gt + Cpv at 1600C changes to that of Rw + Mw + Gt + Cpv at 1800-2000C, and Rw disappears perfectly above 2200C. From mass balance calculation of analyzed compositions of the phases, we found that Gt content increases with increasing temperature before and after formation of Mpv. We also calculated the densities in pyrolite at each temperature. The density of average pyrolite mantle (1600C) is higher than pyrolite plume (1800-2200C) across 660-km discontinuity due to increase in Gt content with increasing temperature. Therefore, we conclude that hot-plume ascending nearby 660-km discontinuity has positive buoyancy by the phase transitions.