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-CG 固体地球科学複合領域・一般

[S-CG61_2AM1] 岩石・鉱物・資源

2014年5月2日(金) 09:00 〜 10:45 311 (3F)

コンビーナ:*角替 敏昭(筑波大学生命環境系)、藤永 公一郎(東京大学大学院工学系研究科システム創成学専攻)、三宅 亮(京都大学大学院理学研究科地球惑星科学専攻地質学鉱物学教室)、土谷 信高(岩手大学教育学部地学教室)、座長:角替 敏昭(筑波大学生命環境系)、土谷 信高(岩手大学教育学部地学教室)

10:00 〜 10:15

[SCG61-05] ロシア極東,ウスチベラヤ.オフィオライトの2つのタイプのウェブステライト;その起源と意義

*町 澄秋1石渡 明2森下 知晃1早坂 康隆3荒井 章司1田村 明弘1 (1.金沢大学理工研究域自然システム学系、2.東北大学,東北アジア研究センター、3.広島大学大学院理学研究科)

キーワード:ウスチベラヤ・オフィオライト, ウェブステライト, 大陸下マントル

The Ust'-Belaya ophiolite is located in the Koryak Mountains, Far East Russia. We report two types of websterite in the mantle section of the ophiolite. The lithology of the mantle peridotites from the ophiolite is variable from very fertile lherzolite to moderately depleted harzburgite. The mineral chemistry of the very fertile lherzolite shows similar signature to those of the subcontinental peridotite. The two types of websterite (type1 and type2) occur in them as dikes/veins. Type1 is composed of brownish colored cpx, opx and Al-spinel. On the other hand, type2 is composed of green colored cpx, opx and Cr-spinel.Type2 websterite is similar to those reported from many other ophiolites. Websterites, which are characterized by extremely aluminous spinel similar to the type1 websterite, are never found in ophiolitic peridotites but are described in passive margin peridotites (e.g. Zabargad Island in Red Sea and Iberia Abyssal plain peridotites). These websterites are generally interpreted as high-pressure cumulates and the host peridotites are considered as fragments of subcontinental mantle.The mantle section of the Ust'-Belaya ophiolite represents, at least partly, fragments of subcontinental mantle. The two types of websterite might be related to two different magmatisms in two different tectonic settings; type1 is formed former subcontinental to oceanic environment and then type2 is formed later oceanic to arc environment.