日本地球惑星科学連合2019年大会

講演情報

[J] 口頭発表

セッション記号 H (地球人間圏科学) » H-RE 応用地質学・資源エネルギー利用

[H-RE16] 資源地質学

2019年5月29日(水) 10:45 〜 12:15 106 (1F)

コンビーナ:大竹 翼(北海道大学大学院工学研究院 環境循環システム部門)、荒岡 大輔(産業技術総合研究所地圏資源環境研究部門)、高橋 亮平(秋田大学大学院国際資源学研究科)、野崎 達生(海洋研究開発機構海底資源研究開発センター)、座長:大竹 翼(北海道大学大学院工学研究院)、荒岡 大輔

10:45 〜 11:15

[HRE16-01] クロムの濃集における水の役割

★招待講演

*荒井 章司1 (1.金沢大学理工研究域自然システム学系)

キーワード:クロム、クロミタイト、水

The role of water in the formation of chromitites, which have been designated as a typical orthomagmatic ores, has been long controversial. Johan et al. (1983, 2017), for example, concluded that chromites are precipitated from water-rich fluids at relatively low temperatures (< 1000 ºC) to form podiform chromitites in the mantle. Those arguments are mainly based on two observations; (1) podiform chromitites and surrounding peridotites have been preferentially hydrated, which may mean the initial water enrichment, and (2) chromite grains contain fluid and hydrous mineral inclusions of apparently primary origin. I criticize the related interpretations based on those observations. The selective hydration in and around chromitite pods is due to the Mg-rich character of olivines, which has been obtained during a subsolidus cooling stage (Arai, 1978), and does not definitely show the involvement of water-rich fluid in chromitite formation. The origin of the chromite-hosted hydrous mineral inclusions has not been left unclear. Many authors a priori interpreted the inclusions as being representative of the trapped melts or fluids that precipitated the host chromites. This is, however, highly questionable. The inclusions are most probably formed during a stage of peridotite-melt reaction within a complicated igneous stage of podiform chromitite generation in the mantle. Hydrothermal fluids can transport Cr and precipitate chromite, but may not form most of the podifrom chromitites.