日本地球惑星科学連合2014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-CG67_1PM2] 海洋底地球科学

2014年5月1日(木) 16:15 〜 17:00 414 (4F)

コンビーナ:*沖野 郷子(東京大学大気海洋研究所)、田所 敬一(名古屋大学地震火山研究センター)、石塚 治(産業技術総合研究所地質情報研究部門)、土岐 知弘(琉球大学理学部)、高橋 成実(海洋研究開発機構地震津波・防災研究プロジェクト)、座長:一瀬 建日(東京大学地震研究所)、平野 直人(東北大学東北アジア研究センター)、羽生 毅(海洋研究開発機構 地球内部ダイナミクス領域)

16:15 〜 16:30

[SCG67-08] 地磁気三成分異常に基づくパラオ海盆の起源と西フィリピン海盆拡大モデルの改良

佐々木 智弘1、*山崎 俊嗣2石塚 治3 (1.筑波大学大学院生命環境科学研究科、2.東京大学大気海洋研究所、3.産業技術総合研究所地質情報研究部門)

キーワード:Philippine Sea plate, West Philippine Basin, Palau Basin, magnetic anomaly, seafloor spreading

The western part of the Philippine Sea (PHS) plate was occupied by the West Philippine Basin (WPB) in the north and the Palau Basin (PB) in the south. The WPB is generally considered to have opened from about 50 to 30 Ma, but the details are still unclear; in particular the origin and age of the PB was unknown. Studying the history of the WPB is important for understanding better the initiation and evolution of the IBM Arc. Here we discuss the spreading history of the WPB using new data on three-component magnetic anomaly and swath bathymetry acquired in the PB as well as those obtained previously by JAMSTEC fleets in the southern WPB. NS-trending magnetic boundaries and seafloor fabrics occur in the PB, indicating the formation by EW seafloor spreading. With a constraint from a 40Ar/39Ar age of 40.4 Ma obtained from the northernmost part of the PB, we interpret that the observed magnetic anomalies correspond to polarity reversals from C16n1r to C18n/C18r (35.6 to 38/39 Ma). Previous models of WPB spreading incorporated a spreading-rate decrease around 40 Ma from about 4.4 to 1.8 cm/year. Our study in the southern WPB, however, suggests that the decrease is unnecessary for correlating observed three-component anomalies to the GPTS. A typical profile along 130E corresponds to C16r to C21 (36.3 to 45.3 Ma). The cessation age of the spreading in our interpretation, about 35 to 37 Ma, is older than the previous estimation (about 30 to 33 Ma). It was difficult to constrain rotation of the PHS plate from the magnetic anomaly skewness.