日本地球惑星科学連合2015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-CG58] 岩石・鉱物・資源

2015年5月25日(月) 14:15 〜 16:00 203 (2F)

コンビーナ:*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)、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)、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)

15:30 〜 15:45

[SCG58-09] 東赤石超マフィック岩体のクロミタイトの特徴:超高圧クロミタイトの起源についての暗示

*三浦 真1荒井 章司1水上 知行1山本 伸次2ブラディミール シュメレフ3 (1.金沢大学大学院 自然科学研究科、2.東京大学大学院 総合文化研究科、3.ウラル ロシア科学アカデミー 地質・地球化学研究科)

キーワード:ポディフォーム・クロミタイト, 東赤石超マフィック岩体, スピネル, 離溶ラメラ, 超高圧クロミタイト

Ultrahigh-pressure (=UHP) chromitites, which contain UHP minerals such as diamond and coesite, have been observed from ophiolites in Tibet and the Polar Urals. However, their nature, i.e. origin, frequency of appearance and P-T path, are still controversial because of insufficiency of detailed petrographic studies. Systematic observation and classification of various chromitites and enclosing peridotites from some localities are required.
Chromitites in the Higashi-akaishi ultramafic complex in the Cretaceous Sanbagawa metamorphic belt, Japan, is one of keys to interpret the origin of UHP chromitite. The Higashi-akaishi ultramafic complex is characterized by the presence of garnet in some peridotites and pyroxenites, and interpreted as a high-P metamorphic (up to 3.8 GPa) complex originally formed at a lower-P subduction zone mantle. The chromitites in the Higashi-akaishi ultramafic complex had also experienced the high-P metamorphism. They will provide us with information on the behavior of low-P chromitite upon compression via subduction.
Spinels in the Higashi-akaishi chromitite contain various inclusions, i.e. numerous needle- and blade-like diopside lamellae, and are free of primary inclusions of hydrous minerals, such as pargasite and Na phlogopite. Solid-phase secondary inclusions are mostly composed of chlorite and serpentine. Chromian spinels in the Higashi-akaishi chromitite show high Cr#s (0.8 to 0.85) and low Ti contents (< 0.1 wt%), suggesting an arc-related feature. Spinels in the Higashi-akaishi chromitite and surrounding peridotite were sometimes fractured by deformation.
The Higashi-akaishi chromitite is similar in features of inclusions in spinel and spinel chemistry to the UHP chromitites from Tibet and the Polar Urals. This similarity suggests that some of the characteristics of the UHP chromitite can be formed by compression of low-P chromitite, e.g., recycling via a subduction zone. In addition, such diopside lamellae in spinel of the Higashi-akaishi chromitite are typically found from some low-P chromitites from the Oman ophiolite and the Iwanai-dake ultramafic complex, Japan. Their occurrence suggests that the UHP Ca-ferrite (or Ca-titanite) type spinel precursor is not a prerequisite for exsolution of silicate lamellae.