[U-13] Advanced understanding of Quaternary and Anthropocene hydroclimate changes in East Asia:

[U13-P10] Reconstruction of ventilation ages of the Indian Ocean sector of the Southern Ocean using ¹⁴C and U-Th ages of deep-sea isidid octocorals

★Invited Papers

*小坂 由紀子¹、沈川 洲²、佐藤 暢³、南 雅代¹、徳田 悠希⁴、池原 実⁵ (1.名古屋大学 宇宙地球環境研究所、2.國立臺灣大學 地質科學系、3.専修大学 経営学部、4.公立鳥取環境大学 環境学部、5.高知大学 海洋コア総合研究センター)

キーワード：深海サンゴ、竹サンゴ、U-Th年代、放射性炭素年代、南大洋、コンラッドライズ

Carbonaceous skeletons of the deep-sea corals are generally dated by uranium-series systematics. By combining the absolute ages obtained with radiocarbon, the past ocean ventilation rate has been estimated. This approach is particularly effective in the Southern Ocean, where carbonate compensation depths are shallow and carbonate rocks are not likely to remain. Previous studies performed on the Southern Ocean have mainly focused on corals from the Drake Passage and off Tasmania. In this study, we focused on deep-sea isidid octocorals (Bamboo coral) collected from the Conrad Rise, Indian sector of the Southern Ocean, and report the results of ¹⁴C and U-Th ages in the presentation. The skeleton of deep-sea isidid octocorals is formed of very dense calcite material, which makes it difficult to dissolve even after the death of the coral polyp that cover it.

A characteristic of deep-sea isidid octocorals is that new skeletons may form to encapsulate the old coral skeleton. We performed both of uranium-series and radiocarbon measurements on two samples of old coral inclusions. The U-Th dating provided insight into the age distribution of coral skeletons collected by dredge from Conrad Rise. Periods of relatively high coral production frequency may indicate that the environment was conducive to coral growth.