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-IS13] 遠洋域の進化

2016年5月23日(月) 09:00 〜 10:30 203 (2F)

コンビーナ:*松岡 篤(新潟大学理学部地質科学科)、栗原 敏之(新潟大学大学院自然科学研究科)、加藤 泰浩(東京大学大学院工学系研究科システム創成学専攻)、尾上 哲治(熊本大学大学院自然科学研究科)、木元 克典(独立行政法人海洋研究開発機構)、野崎 達生(海洋研究開発機構海底資源研究開発センター)、植田 勇人(新潟大学理学部地質科学科)、小林 健太(新潟大学理学部地質科学科)、長谷川 卓(金沢大学自然システム学系)、座長:松岡 篤(新潟大学理学部地質科学科)、栗原 敏之

10:15 〜 10:30

[MIS13-06] 下部三畳系深海チャートギャップの成因

*武藤 俊1高橋 聡1山北 聡2池田 昌之3尾上 哲治4 (1.東京大学大学院理学系研究科地球惑星科学専攻、2.宮崎大学教育文化学部地学教質、3.静岡大学理学研究科地球科学専攻、4.熊本大学自然科学研究科)

キーワード:下部三畳系、深海チャートギャップ、コノドント、砕屑物埋没速度、生物源シリカ埋没速度

Carboniferous to Jurassic pelagic deep-sea sediments that accumulated in the pelagic Panthalassa Ocean are mostly composed of bedded chert lithofacies (Matsuda and Isozaki, 1991). Among them, the Lower Triassic interval is characterised by siliceous claystone dominant lithofacies instead of bedded chert lithofacies (the deep-sea chert gap) (Ishiga and Yamakita, 1993; Isozaki, 1997). The age of the deep-sea chert gap (ca. 252–247 Ma) corresponds to the time interval of ecosystem recovery from the end-Permian mass extinction, the largest mass extinction event in the Phanerozoic (Chen and Benton, 2012). Therefore, the deep-sea chert gap may reflect anomalous environmental conditions during the Early Triassic that possibly delayed the re-establishment of complex ecosystems after the mass extinction. The deep-sea chert gap may either be a result of an increase in burial flux of fine clastic material, or a decline in burial flux of biogenic silica in the Early Triassic pelagic Panthalassa. However, previous studies have not calculated burial fluxes of fine clastic material and biogenic silica based on well-dated sedimentary sequences. In order to identify the mechanism that led to the formation of the deep-sea chert gap, we estimated the burial fluxes of clastic material and biogenic silica in deep-sea sedimentary sequences, which were newly described in this study.
Detailed geological mapping and reconstruction of lithostratigraphy was carried out at Ogama in the Kuzuu area, Tochigi Prefecture, and in the Tsukumi area, Oita Prefecture, and consequently, several continuous sections were identified. Based on conodont biostratigraphy, the studied sections are correlated to the triangularis-collinsoni Zone, the homeri Zone, the timorensis Zone and the bulgarica Zone of Koike (1981), which corresponds to the Spathian (upper Olenekian; uppermost Lower Triassic) to middle Anisian (lower Middle Triassic). Using the conodont biostratigraphic framework, absolute ages of volcanic tuff beds in South China were projected onto the reconstructed lithostratigraphic columns of the deep-sea sections. Consequently, the lower limit of the linear sedimentation rate (LSR) was obtained for the Spathian and lowermost Anisian siliceous claystone dominant lithofacies.
In addition, major element concentrations were measured for rock samples obtained from the studied sections by X-ray fluorescence (XRF) analysis. The SiO2 and Al2O3 concentrations were were combined with measured rock density data and the lithostratigraphic data of the studied sections to calculate the burial fluxes of clastic material and biogenic silica for the stratigraphic intervals for which LSR was estimated. For the lowermost Anisian in Ogama, the minimum burial fluxes of clastic material and biogenic silica are 1030 g/cm2·m.y. and 1040 g/cm2·m.y., respectively. For the Spathian in the Tsukumi area, the minimum burial fluxes of clastic material and biogenic silica are 960 g/cm2·m.y. and 1130 g/cm2·m.y., respectively. The estimated minimum burial flux of clastic material for the deep-sea chert gap greatly exceeds the burial flux calculated for the Anisian bedded chert lithofacies in the Tsukumi area (80 g/cm2·m.y.), calculated based on LSR by Soda et al. (2015). The estimated minimum burial flux of biogenic silica for the deep-sea chert gap is also higher than that of Anisian bedded chert in the Tsukumi area (390 g/cm2·m.y.), calculated based on LSR by Soda et al. (2015). These results indicate that, during the deposition of sediments in the deep-sea chert gap, burial fluxes of clastic material and biogenic silica were both elevated, but the increase is greater in the former. Hence, the deep-sea chert gap is a result of anomalously high flux of clastic material to the pelagic realm, which diluted biogenic silica in deep-sea sediments.