日本地球惑星科学連合2015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-IS30] 遠洋域の進化

2015年5月26日(火) 09:00 〜 10:45 304 (3F)

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(海洋研究開発機構地球内部ダイナミクス領域)、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:植田 勇人(新潟大学理学部地質科学科)、高橋 聡(東京大学理学系研究科地球惑星科学専攻)

10:30 〜 10:45

[MIS30-07] スロバキアKardolinaセクションにおける上部三畳系石灰岩の堆積環境と炭素・酸素安定同位体比変動

*白水 秀子1Josef Michalik2日下 宗一郎3山下 美沙4山下 勝行4尾上 哲治1 (1.熊本大学大学院自然科学研究科、2.スロバキア科学アカデミー、3.総合地球環境学研究所、4.岡山大学大学院自然科学研究科)

キーワード:炭素・酸素安定同位体比, 石灰岩, 三畳紀/ジュラ紀境界, レーティアン, 炭素同位体比異常, 海水準変動

Triassic / Jurassic (T/J) boundary of approximately 201.3 million years ago is known as a stratigraphic boundary recorded one of the big five Phanerozoic mass extinctions. Catastrophic processes such as widespread eruption of the Central Atlantic Magmatic Province (CAMP) flood basalts and extraterrestrial impacts have been proposed to account for the mass extinction event. This paper reports the results of carbon and oxygen isotopes analysis from the uppermost Triassic limestone in the Kardolina section, Slovakia. The Kardolina section is crops out on a steep western slope of the Mt Palenica in the Belianske Tatry Mts as the most continuous section from the uppermost Triassic (Rhaetian) Fatra Formation. The Fatra Formation is shallow marine carbonate sequence and is overlain with a sharp contact by marine shale of the lowermost Jurassic (Hettangian) Kopieniec Formation. The Rhaetian age of the Fatra Formation was determined by foraminifera fossils. Several excursions of carbon and oxygen isotopes exist in the Fatra Formation. The large negative carbon isotope excursions (CIE) were found in at least four stratigraphic levels. Although the Fatra Formation is composed of packstone and grainstone, the CIE occurred during the deposition of non-fossiliferous lime-mudstone or ostracod lime-mudstone. The largest negative CIE occurs just before the T/J boundary. The cause of this negative CIE at the vicinity of T/J boundary remains uncertain. However it is assumed that the Kardolina section was exposed on the ground by sea-level fall, and subjected to diagenesis of terrestrial water. The large CIE may possibly be associated with sea-level change of the Kardolina section.