日本地球惑星科学連合2022年大会

講演情報

[J] ポスター発表

セッション記号 H (地球人間圏科学) » H-QR 第四紀学

[H-QR05] 地球惑星科学へのルミネッセンス・ESR年代測定の応用

2022年6月2日(木) 11:00 〜 13:00 オンラインポスターZoom会場 (14) (Ch.14)

コンビーナ:豊田 新(岡山理科大学理学部応用物理学科)、コンビーナ:田村 亨(産業技術総合研究所地質情報研究部門)、下岡 順直(立正大学地球環境科学部環境システム学科)、座長:豊田 新(岡山理科大学古生物学・年代学研究センター)、田村 亨(産業技術総合研究所地質情報研究部門)

11:00 〜 13:00

[HQR05-P03] Testing fine-grained quartz and feldspar luminescence dating on a deep marine sediment core from the Sea of Japan: upper age limit and dust source fingerprinting

*杉崎 彩子1、Buylaert Jan-Pieter2、Murray Andrew3 多田 隆治4 (1.産業技術総合研究所 地質情報研究部門、2.Department of Physics, Technical University of Denmark、3.Nordic Laboratory for Luminescence Dating, Department of Earth Sciences, Aarhus University、4.千葉工業大学 地球学研究センター)

キーワード:光ルミネッセンス年代測定、日本海

Quaternary hemi-pelagic sediments in the Japan Sea record millennial and orbital scale changes in the East Asian Monsoon as alternating dark and light layers. Two holes were cored to explore the development and evolution of monsoonal patterns and their relationship to past changes in the Japan Sea. A tuned age model was constructed using tephro-stratigraphy, magneto-stratigraphy and the sediment GRA profile tuned to the δ18O profiles of LR04 (Lisiecki and Raymo, 2005, Tada et al., 2018).
We have used OSL dating of fine-grained detrital quartz (of aeolian origin) to provide high-resolution numerical age models for the late Quaternary in the cores from holes U1424C and U1425C.Comparison with the quartz OSL ages and the tuned age model indicates that the older quartz ages (>130 ka) should be considered minimum estimates.
Here we test the potential of a post-IR IRSL signal from polymineral fine-grains to date these cores beyond MIS5e. As modern analogue samples, we measured the sea floor sediments taken from the top ~5cm of short multiple cores. Post-IR IR230 apparent equivalent doses from these samples are high, ~30 Gy, suggesting that the pIRIR230 signal may not have been fully reset at deposition. Down the long cores equivalent doses increase with depth, up to ~1000 Gy. However, the pIRIR230 ages also appear to underestimate from ~150 ka onwards, with field saturation reached at ~300-400 ka (800-1000 Gy). From our results, it appears that pIRIR230 dating does not allow us to date significantly beyond the quartz OSL age limit.
Furthermore, we also test the potential of the use of quartz OSL sensitivity (as measured by the natural test dose, Tx) as an indicator for dust source changes with time. This sensitivity correlates with the quartz ESR signature from the same material. Interestingly, the Tx of U1424C and U1425C shows the inverse variation from MIS 6 to 5b, then conformable variation from MIS 4 to 1. These indicators may allow us to distinguish between predominantly Taklimakan Desert, Loess Plateau area and Siberia–Northeast China area dust sources (Nagashima et al., 2007).