JpGU-AGU Joint Meeting 2017

講演情報

[EE] 口頭発表

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-IT22] [EE] 核-マントルの相互作用と共進化

2017年5月20日(土) 09:00 〜 10:30 A05 (東京ベイ幕張ホール)

コンビーナ:土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)、寺崎 英紀(大阪大学大学院理学研究科)、Satish-Kumar Madhusoodhan(Department of Geology, Faculty of Science, Niigata University)、入舩 徹男(愛媛大学地球深部ダイナミクス研究センター)、Hernlund John(Earth-Life Science Institute, Tokyo Institute of Technology)、大谷 栄治(東北大学大学院理学研究科地学専攻)、座長:Satish-Kumar Madhusoodhan(新潟大学)

10:00 〜 10:15

[SIT22-05] Experimental investigation of high-pressure phase transitions in AlOOH and FeOOH

*西 真之1,2桑山 靖弘3土屋 旬1,2土屋 卓久1,2 (1.愛媛大学地球深部ダイナミクス研究センター、2.東京工業大学地球生命研究所、3.東京大学)

キーワード:含水鉱物、高圧

Hydrogen is transported into deep Earth’s mantle regions as a form of hydrous minerals via subduction of oceanic plates. Recently discovered CaCl2-type hydroxides such as (Mg,Si)OOH phase H, delta-AlOOH, and their solid solutions were reported to have large P–T stability fields that encompass conditions representative of the lower mantle, implying the possibility that surface water may be transported as far as the core–mantle boundary. However, although Epsilon-FeOOH has CaCl2-type structure as well, the solid solution of FeOOH component in CaCl2-type structure has not been studied. Since FeOOH was recently reported to decompose under the lower-mantle conditions to form FeO2 releasing H2, FeOOH could be a key component that strongly affect the stability of CaCl2-type hydroxide. Here, we report the results of in-situ X-ray diffraction and theoretical studies on AlOOH and FeOOH using a laser-heated diamond anvil cell technique at up to ~200 GPa. In contrast to the previous work suggesting the dehydration of FeOOH in the middle of the lower mantle, we report the formation of a pyrite-type FeOOH that is significantly denser than the surrounding mantle and stable to conditions representative of its base. Furthermore, delta-AlOOH and CaCl2-type (Al,Fe)OOH also transform to a pyrite-type structure at higher pressures. Based on these experimental and theoretical results, the stability of hydrous phase in the lower mantle and deep interiors of icy planets will be discussed.