日本地球惑星科学連合2019年大会

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[E] 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-IT21] 核-マントルの相互作用と共進化

2019年5月27日(月) 13:45 〜 15:15 A10 (東京ベイ幕張ホール)

コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)、座長:五味 斎飯塚 毅

14:45 〜 15:00

[SIT21-17] Some technological developments in high temperature generation using KMA and precise melting/phase relations of minerals and rocks under deep mantle conditions

*入舩 徹男1,2周 佑黙1有本 岳史1桑原 秀治1野村 龍一3西 真之1山口 桃子1丹下 慶範4栗林 貴弘5劉 兆東6 (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、3.京都大学白眉センター/大学院人間・環境学研究科、4.高輝度光科学研究センター利用研究促進部門、5.東北大学理学研究科、6.吉林大超硬材料研究所)

キーワード:下部マントル、マルチアンビル装置、融解関係、相関係、高温高圧実験、技術開発

Technological developments in stable and homogeneous high temperature generation have been made using conventional LaCrO3 or Re heater for Kawai-type multianvil apparatus (KMA) with tungusten carbide (WC) and sintered diamond (SD) anvils. For WC-KMA, stable temeperature generation to ~3000 K has been achieved under the pressures up to ~27 GPa mainly for quench experiments. Temperatures of ~2000-2300 K have been produced stably for 20-180 minutes at pressures to ~65 GPa for in situ X-ray measurements using SD-KMA, in addition to the ex situ experiments.

Some experimental studies for precise determination of subsolidus and melting phase relations have successfully been made for some simple mineral systems, such as MgSiO3-Al2O3, MgSiO3-FeSiO3, MgSiO3-CaSiO3, CaSiO3-SiO2, Al2O3-SiO2, KAlSi3O8-NaAlSi3O8, Al2SiO5, Ca3Al2Si3O12, etc. at temperatures near and above the typical geotherm at pressures corresponding to those of the mantle transition region to the middle part of the lower mantle. These studies have provided firm experimental databases for the mineralogy of the deep mantle, and also led to findings of some new high-pressure phases stable only under the very high-temperture conditions. Melting and associated partioning of some key trace elements in more complex chemical compositions have also been conducted under the pressures of the uppermost lower manlte to constrain the differentiation and evolution of the deep mantle.