日本地球惑星科学連合2025年大会

講演情報

[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS23] 非破壊分析による環境復元の展開

2025年5月27日(火) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:天野 敦子(産業技術総合研究所)、田中 えりか(高知大学)

17:15 〜 19:15

[MIS23-P01] Non-destructive analysis of sediment cores collected on the southwestern flank of the Shatsky Rise during Cruise KH-24-1

*田中 えりか1黒田 潤一郎2安川 和孝3朴 進午2亀尾 桂2、戸田 亮二2飯島 耕一4臼井 洋一5桑原 佑典3小笠原 光基3、池津 雄地3、伊地知 遼行3畠山 裕亮3孫 岳2于 凡2呂 玉琪2山川 登2趙 陽2中川 友紀6吉住 勇輝1、磯田 龍之介5卯田 寿里7本多 楓太7伊藤 颯矢7、堀内 禎希8、澤田 律子9、中尾 眞子10 (1.高知大学、2.東京大学大気海洋研究所、3.東京大学工学系研究科、4.海洋研究開発機構、5.金沢大学、6.東京大学理学系研究科、7.千葉大学、8.日本海洋事業、9.マリンワークジャパン、10.MOLMEC)

キーワード:シャツキー海台、海底堆積物、更新世、X線CT、MSCL

Shatsky Rise is a large igneous province (LIP) in the western North Pacific Ocean, which formed between 147 and 124 million years ago. Its summit reaches 1950 m below sea level (mbsl) whereas the depth of the deep-sea basin around Shatsky Rise is 5500–6000 mbsl [1]. Since Shatsky Rise is situated within the North Pacific subtropical gyre and on the course of the westerlies, nutrient supply around the Shatsky Rise has been attributed to surface current (i.e., Kuroshio Extension and Oyashio Current) and intensified westerlies transporting eolian dust [2–5].
Recently, the nutrient supply system around the Kuroshio area and in the oligotrophic gyre southern off the Shatsky Rise has been reevaluated, considering deep-sea turbulence and upwelling involving the interaction of bottom water current and “topographic high” [6, 7]. However, observations have not verified that such a huge topography can function as a physical barrier to supply nutrients to the surface ocean from the deeper layer. Notably, previous ocean drilling on the southwestern flank of the Shatsky Rise confirmed a sedimentary hiatus between the Pliocene and Cretaceous, implying the existence of strong bottom currents in this area [8].
Therefore, Cruise KH-24-1 aimed to reveal the relationships between depositional environments and paleoceanographic changes, including the intensification of the bottom current, on the southwestern flank of the Shatsky Rise. During Cruise KH-24-1, we conducted piston and multiple coring and CTD observations. These sediment samples are considered to cover the last 500 kyrs. In this presentation, we will introduce the preliminary results of Cruise KH-24-1, focusing on the non-destructive analysis (X-ray CT and MSCL) of the sediment cores and discussing the possibility of further research related to CTD observations.

[1] Zhang et al. (2016) Earth Planet. Sci. Lett., 441, 143–156. [2] Chiyonobu et al. (2012) Mar. Micropaleontol., 96–97, 29–37. [3] Seo et al. (2018) Palaeogeogr. Palaeoclimatol. Palaeoecol., 496, 323–331. [4] Amo and Minagawa (2003) Org. Geochem., 34, 1299–1312. [5] Maher et al. (2010) Earth Sci. Rev. 99, 61–97. [6] Ohta et al. (2020) Sci. Rep., 10, 9896. [7] Kobari et al. (2020) Biogeosciences, 17, 2441–2452. [8] Bralower et al. (2002) Proc. ODP., 198