日本地球惑星科学連合2015年大会

講演情報

インターナショナルセッション(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-IT05] Hard-Rock Drilling: Oceanic Lithosphere to Island Arc Formation and Beyond

2015年5月26日(火) 16:15 〜 18:00 303 (3F)

コンビーナ:*田村 芳彦(海洋研究開発機構 海洋掘削科学研究開発センター)、Yildirim Dilek(マイアミ大学)、森下 知晃(金沢大学理工研究域自然システム学系)、佐野 貴司(国立科学博物館地学研究部)、阿部 なつ江(独立行政法人海洋研究開発機構海洋掘削科学研究開発センター)、海野 進(金沢大学理工研究域自然システム学系)、高澤 栄一(新潟大学理学部地質科学科)、小野 重明(独立行政法人海洋研究開発機構)、道林 克禎(静岡大学理学研究科地球科学専攻)、座長:森下 知晃(金沢大学理工研究域自然システム学系)、海野 進(金沢大学理工研究域自然システム学系)

17:24 〜 17:27

[SIT05-P04] 南部マリアナ海溝最西端のかんらん岩はパレスベラリフト起源?

ポスター講演3分口頭発表枠

*大家 翔馬1道林 克禎1小原 泰彦2石井 輝秋3水野 那希1萬年 一剛4 (1.静岡大学・理・地球科学、2.海上保安庁海洋情報部、3.深田地質研究所、4.神奈川県立温泉地学研究所)

The Izu-Bonin-Marina (IBM) arc is a typical intra-oceanic arc system. The forearc is non-accretionary convergent margin, where Mafic crustal rocks occurred along the inner trench slope with mantle peridotites. Mariana arc system is the southern part of the IBM arc system and forms arcuately. The trench axis of the southern Mariana trench runs across Mariana volcanic arc and backarc basin (Mariana trough) and is connected to Parece Vela Basin at the westernmost area. There have been no geological studies on the westernmost Marianas trench since Hawkins and Batiza(1977). Recently, investigations for the junction area between Mariana trench and Parece Vela Basin have been conducted using the submersible Shinkai6500 (Dive 6K1397 and 6K1398) as a part of YK14-13 cruise by the R/V Yokosuka in 2014. Shinkai6500 recovered plagioclase-bearing lherzolites and harzbergites from the tectonic ridge along the inner trench slope of the westernmost Mariana Trench. The samples show coarse grained textures (>1mm), heterogeneous intermediate textures, and fine grained textures (<0.6mm). The peridotites with the coarse grained texture were sampled from the shallowest part (3705-4042m) in the dive area, whereas the peridotites with the fine grained textures were sampled from the deepest part (5996m). Olivine fabrics vary associate with texture. : (010)[100]pattern for the coarse grained textures, {0kl}[100]pattern for the fine grained textures, and various indistinct patterns for the heterogeneous textures. The variations of both olivine textures and crystallographic fabrics with depth suggest variations of deformation processes with depth. Olivine-Spinel compositions are in a range of the Olivine-Spinel Mantle Array, indicating that the peridotites are depleted residues after partial melting of the upper mantle. Spinel compositions is bimodal between moderately high Cr# spinels (up to 0.54 in 6K1398R16) and relatively low Cr# spinels (as low as 0.30 in 6K1397R18). The increase of Cr# appears to be correlated with Ti contents (0.03-0.49), indicating that melt-rock interaction under shallow lithospheric mantle conditions. Furthermore, chemical compositions of Spinel Mg# and Cr# are almost identical to those of Parece Vela Basin peridotites, suggesting that Parece Vela Basin Mantle may be exposed on the inner trench slope in the westernmost Mariana trench.