日本地球惑星科学連合2016年大会

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セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS17] 古気候・古海洋変動

2016年5月23日(月) 15:30 〜 17:00 A04 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*入野 智久(北海道大学 大学院地球環境科学研究院)、池原 実(高知大学海洋コア総合研究センター)、岡 顕(東京大学大気海洋研究所)、岡崎 裕典(九州大学大学院理学研究院地球惑星科学部門)、北場 育子(立命館大学古気候学研究センター)、北村 晃寿(静岡大学理学部地球科学教室)、佐野 雅規(総合地球環境学研究所)、多田 隆治(東京大学大学院理学系研究科地球惑星科学専攻)、中川 毅(立命館大学)、林田 明(同志社大学理工学部環境システム学科)、座長:多田 隆治(東京大学大学院理学系研究科地球惑星科学専攻)

16:30 〜 16:45

[MIS17-11] 海洋酸素同位体層序とよい対応を示す大阪湾の中期更新世の海水準変動

*吉住 正斗1廣瀬 孝太郎1,2兵頭 政幸1,2佐藤 裕司3 (1.神戸大学大学院 理学研究科 惑星学専攻、2.神戸大学 内海域環境教育研究センター、3.兵庫県立大学 自然・環境科学研究所)

キーワード:海水準変動、中期更新世、大阪層群、珪藻、海洋酸素同位体ステージ 15、海洋酸素同位体ステージ 13

The Osaka Group consists of Plio-Pleistocene sediments continuously deposited in the Osaka Basin. It mainly consists of freshwater deposits in the lower part, and alternating marine and freshwater layers in the upper part. Each marine layer has been designated as Ma-1, Ma0, Ma0.5, Ma1, etc, and correlated with interglacial highstands. However, marine layers Ma6, Ma7, and Ma8 possibly correlated with Marine Isotope Stages (MISs) 15 and 13, have not been studied well and correlations with MISs are obscure because of low amplitude precession-related signals for marine isotope data. Recent studies revealed many marine clay layers defined based on lithology are partly lacustrine. In this study, we examine sea-level changes with diatom and sulfur analysis of Ma6, Ma7, and Ma8 in the Osaka Bay 1700-m core (GS-K1 core) to construct more detailed and precise correlations with eustatic sea-level changes. The aquatic environment and diatom assemblages in Osaka Bay are strongly affected by eustatic sea-level changes through the Kitan Strait, and also by a huge amount of freshwater from the Yodo River. Diatom taxa were grouped into five ecological categories according to salinity tolerance: marine, marine-brackish, brackish, brackish-freshwater, and freshwater. We adopt 3 per mil of sulfur contents to empirical criterion which defines a marine/freshwater boundary. Parts of Ma6 defined in the previous study are lacustrine. The thickness of marine interval is 27.6 m, which is 0.8 m shorter than before. In the lower part of new Ma6, we found a single sea-level highstand correlated with MIS 15.5. The upper part has a zone of no diatoms. However, this zone is marine because it has high sulfur content over 3 per mil. In Ma7, marine interval is newly defined to be 13.9 m thick, which is 5.4 m shorter than the previous one. In the center of new Ma7, we found a single sea-level highstand correlated with MIS 15.1. Between the new Ma6 and Ma7, we found a lacustrine layer of 3.2 m thick that can be correlated with MIS 15.2. We also investigated Ma8, and found Ma8 splits into two marine intervals, probably caused by desalination due to eustatic sea-level fall correlated with MIS 13.2. A tentative astronomical age model shows an average accumulation rate for MIS 15 is 0.86 m/ka, which is much higher than an average for the middle Pleistocene (0.52 m/ka). The high accumulation rate may reflect that tectonic activities including uplifting in mountain areas and subsidence in the basin became high during MIS 15 (621-576 ka) in the Kinki District.