日本地球惑星科学連合2014年大会

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ポスター発表

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-IT41_28PO1] 海洋プレートの一生:誕生から解体,そして復活

2014年4月28日(月) 18:15 〜 19:30 3階ポスター会場 (3F)

コンビーナ:*森下 知晃(金沢大学理工研究域自然システム学系)、山崎 俊嗣(東京大学大気海洋研究所)、島 伸和(神戸大学大学院理学研究科地球惑星科学専攻)、安間 了(筑波大学生命環境系)、熊谷 英憲(独立行政法人海洋研究開発機構)、中村 大輔(岡山大学)

18:15 〜 19:30

[SIT41-P01] 中央インド洋海嶺南部Kairei熱水場周辺のマフィック岩と超マフィック岩

西村 拓真1針金 由美子2、*道林 克禎3森下 知晃4佐藤 暢5 (1.静岡大学理学部地球科学科、2.産業技術総合研究所地質情報研究部門、3.静岡大学理学研究科地球科学専攻、4.金沢大学理工研究域自然システム学系、5.専修大学経営学部)

キーワード:mafic rock, ultramafic rock, Central Indian Ridge, Kairei Hydrothermal Field

The central Indian Ridge (CIR) is situated at the north of the Rodrigues Triple Junction (RTJ) and is a slow- to intermediate-spreading mid-ocean ridge with a spreading rate increasing from 30 mm/year in full rate near the Equator to 49 mm/year in full rate at the RTJ. In the southern CIR near RTJ, the Kairei Hydrothermal Field (KHF) was discovered in August 2000 as the first directly observed hydrothermal vent site in the Indian Ocean. Recently, KH-10-06 cruise aboard R/V Hakuho-maru was organized for understanding the hydrothermal system and geological feature around KHF. In this study, we present the petrography of mafic and ultramafic rocks dredged from the vicinity of the KHF during KH-10-06 cruise. A total of 76 samples have been studied from 9 sites, including 24 ultramafic rocks and 38 mafic rocks and 14 other rocks. Most of them are remarkably altered and hydrated. We classified them into sub-groups based on their textures and mineral assemblies. The ultramafic rocks were classified into 5 sub-groups: 1 peridotite, 2 pyroxenites, 3 serpentinized peridotites, 9 olivine-bearing serpentinites and 9 serpentinites. The mafic rocks were classified into 8 sub-groups: 21 Fe-Ti oxide gabbros, 4 gabbros including 2 mylonites, 3 olivine gabbros, 7 gabbroic rocks with various textures and 8 amphibole-rich gabbros. The other rocks consist of 5 aragonites and 9 hydrothermally altered rocks.