JpGU-AGU Joint Meeting 2017

講演情報

[JJ] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS22] [JJ] 地球掘削科学

2017年5月25日(木) 10:45 〜 12:15 国際会議室 (国際会議場 2F)

コンビーナ:山田 泰広(海洋研究開発機構 海洋掘削科学研究開発センター)、道林 克禎(静岡大学理学部地球科学科)、池原 実(高知大学海洋コア総合研究センター)、菅沼 悠介(国立極地研究所)、座長:道林 克禎(静岡大学理学部地球科学科)、座長:高澤 栄一(新潟大学)

11:45 〜 12:00

[MIS22-17] 前弧マントルのファブリック〜マリアナ収束域蛇紋岩海山かんらん岩の構造岩石学〜

*道林 克禎1Fryer Patty2前川 寛和3石井 輝秋4 (1.静岡大学理学部地球科学科、2.University of Hawaii、3.大阪府立大学、4.静岡大学防災総合センター)

キーワード:前弧マントル、マリアナ、カンラン石ファブリック

Large serpentinite mud volcanoes form on the overriding plate of the Mariana subduction zone. Fluids from the descending plate serpentinize the forearc mantle and enable serpentine muds to rise along faults to the seafloor, so that the seamounts are direct windows into subduction processes at depths far too deep to be accessed by any known technology (Fryer, 2012 Ann. Rev. Marine. Sci.). In this study, we focused on serpentinized peridotites obtained from nine serpentinite mud volcanoes in the Mariana convergent region.
The peridotite samples consist mainly of harzburgites with a few dunite samples. We analyzed olivine crystallographic fabrics as well as chemical compositions of olivine and spinel grains. Three types of olivine crystal fabrics were obtained: [010]-fiber type (AG-type), [100](010) type (A-type) and [100]{0kl} type (D-type). The chemical compositions show that Cr# (Cr3+/Al3++Cr3+) of spinel is 0.4 to 0.8 and Mg# (Mg2+/Mg2++Fe2+) of olivine is 89 to 92, which are in the range of Olivine-Spinel Mantle Array (OSMA) of Arai (1994 Chem. Geol.). The equilibrium temperatures induced by olivine and spinel compositions are 700 °C for D-type peridotites and 800 to 850 °C for AG-type peridotites.
We argue that AG-type peridotites may be derived from the older lithospheric mantle before the formation of the Mariana arc system, whereas D-type peridotites could be related to the supra-subduction tectonics during the relative plate motion between Philippine Sea Plate and Pacific Plate.