日本地球惑星科学連合2019年大会

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[J] 口頭発表

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-CG56] 海洋底地球科学

2019年5月26日(日) 10:45 〜 12:15 A05 (東京ベイ幕張ホール)

コンビーナ:沖野 郷子(東京大学大気海洋研究所)、座長:浅見 慶志朗田中 えりか

11:45 〜 12:00

[SCG56-11] オントンジャワ海台周辺海盆のテクトニクス

*中西 正男1清水 祥伽2末次 大輔3佐野 貴司4 (1.千葉大学大学院理学研究院 地球科学研究部門、2.千葉大大学院融合理工学府 地球生命圏科学専攻、3.国立研究開発法人 海洋研究開発機構 地球深部ダイナミクス研究分野、4.国立科学博物館 地学研究部)

キーワード:オントンジャワ海台、海台、太平洋プレート

We present the tectonics of the abyssal basins that abut the Ontong Java Plateau using the resent geophysical investigations.

Ontong Java Plateau (OJP) is the largest of the major oceanic plateaus in the Pacific Ocean basin. OJP rises about 2 km above the surrounding deep ocean floor and has an area within the 4.5 km contour of about 1.8 x 106 km2. A depth to the Moho discontinuity is more than 30 km (Gladczenko, 1994; Miura et al., 2004). The evidences from drilling samples indicate that most of the OJP formed rapidly about 122 Ma at mid-southern latitude in the Pacific Basin (Mahoney et al., 1993; Tejada et al., 1996, 2002). The widely accepted hypothesis of the formation of OJP is an emergence of a plume head (e.g., Coffin and Eldholm, 1993; Neal et al., 1997). The competing hypotheses are the mantle upwelling as the result of bolide impact (Ingle and Coffin, 2004) and the entrainment of dense fertile mantle by rapid seafloor spreading (Korenaga, 2005). Taylor (2006) proposed that the Ontong Java Plateau formed as a single large volcanic province together with the Manihiki and Hikurangi plateaus ca. 120 Ma, called Ontong Java Nui (Chandler et al., 2012). The OJP formation has been a major enduring problem of marine geology over the past more than 40 years. For settlement of the argument about the OJP formation, the tectonic setting of the abyssal basins around the OJP must be revealed.

Abyssal basins are contiguous withthe OJP: the Lyra Basin to the west, the East Mariana and Pigafetta basins to the north, the Nauru Basin to the northeast, and the Stewart and Ellice basins to the southeast. Tectonic histories of the Nauru, East Mariana, and Pigafetta basins, were revealed using the Mesozoic magnetic anomaly lineations (Nakanishi et al., 1992). Those of Lyra and Stewart basins are, however, still unknown because of lack of magnetic anomaly lineations.In at least three of these basins, the Nauru, East Mariana, and Pigafetta, Lower Cretaceous flood basalts overlie older oceanic crust (Abrams et al., 1993; Shipley et al., 1993; Nakanishi and Winterer, 1998).

To expose the tectonics of the abyssal basins around OJP, we conducted geophysical investigation in Nauru, Ellice, Stewart, and Lyra basins by R/Vs Mirai, Kairei, and Hakuho-maru. Our geomagnetic measurement western margin of Nauru Basin exposes the extension of magnetic anomaly lineations identified in Nauru Basin by Nakanishi et al. (1992). Our geophysical investigation in the Stewart Basin show the northeast-southwest rifting in the formation of the basin.