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)

11:45 〜 12:00

[SIT03-11] 高圧力条件下でのδ-AlOOHの弾性的性質: マントル遷移層における高Vs異常への影響

*増野 いづみ1村上 元彦1大谷 栄治1 (1.東北大学大学院理学研究科地学専攻)

キーワード:delta-AlOOH, Brillouin scattering, Raman spectroscopy, subducting slab, high pressure

delta-AlOOH is a high-pressure polymorph of diaspore (alpha-AlOOH) and boehmite (gamma-AlOOH) (Suzuki et al., 2000). Since delta-AlOOH is identified to be stable from 20 to 120 GPa, and temperatures up to 2300 K, this phase is considered to be a possible carrier and reservoir of water in subducting cold slab into the deep mantle (Ohtani et al., 2001; Sano et al., 2004; 2008). In order to investigate the effect of composition on seismic velocities in subducting slab, it is important to measure the elastic properties of delta-AlOOH at high pressure.We have conducted high-pressure acoustic-wave velocity measurements of delta-AlOOH using Brillouin spectroscopy and also explored the chemical bonding of delta-AlOOH by Raman spectroscopy at high pressure in a diamond anvil cell. We obtained sharp peaks from transverse acoustic mode (VS) of delta-AlOOH over the entire pressure range explored up to a pressure of 89 GPa. The peaks from longitudinal acoustic mode (VP) of delta-AlOOH were masked by the diamond shear acoustic modes from 35 GPa. The pressure dependence of the aggregate velocities for the delta-AlOOH at 300 K suggests that the hydrogen-bonding symmetrization with the space group changes from P21nm to Pnnm occurs during compression above 7 GPa. The shear and adiabatic bulk moduli and their pressure derivatives at zero pressure were determined to be K0 = 192.2(8) (GPa), G0 = 158.8(3) (GPa), (dK/dP)0 = 3.63(6), and (dG/dP)0 = 1.35(6) for the pressures above 15 GPa. Raman spectroscopic measurements have shown that the B1 mode frequencies of P21nm disappeared around 6 GPa and Ag mode frequencies of Pnnm appeared above 5.6 GPa, which also indicates the hydrogen-bonding symmetrization around 6 GPa. These results indicate that delta-AlOOH becomes harder by the hydrogen-bonding symmetrization and probably exists as a phase (Pnnm) with the symmetric hydrogen bonding in the mantle transition zone and lower mantle.Shear wave velocities for delta-AlOOH are larger than those of hydrous wadsleyite (by 30 %), hydrous ringwoodite (by 29 %), and majorite (by 29 %). Those of delta-AlOOH are approximately 7 % below those of stishovite. The delta-AlOOH phase thus found to be one of the hardest phases compared to the minerals of mantle transition zone. The existence of delta-AlOOH may contribute to the cause of high VS and VP anomalies. Shear velocities for sediment containing delta-AlOOH phase are larger than those of pyrolite (by 10 %) and MORB (by 5 %). The subducting slabs often stagnate at the transition zone before reaching the lower mantle. Particularly beneath Korean peninsula, there is a high VS anomaly (~2 %) in the lower part of the transition zone (Zhang et al., 2012). The seismic data under the eastern part of northeast China (NEC) also indicates a slight positive anomaly of VS (~1 %), but the VS value observed around 600 km depth under NEC is ~1 % lower than that beneath Korea. We explain the difference in the VS anomalies beneath the NEC and Korea by the amount of sediment containing the delta-AlOOH phase and the stagnating duration. If sediments stagnate at the transition zone before reaching the lower mantle in this region, we can estimate that the higher VS anomaly (~1 %) than NEC would correspond to sediments with 13.4 vol% in stagnant slab. The average oceanic crust subduction rate is estimated to be about 8 cm/yr around Japan. Assuming this estimated rate of subduction, the slab stagnetion has lasted for at least 30 million years.