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-TT 計測技術・研究手法

[M-TT28] 地球化学の最前線:未来の地球化学を展望して

2016年5月22日(日) 09:00 〜 10:30 A04 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)、角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也(東京工業大学大学院理工学研究科地球惑星科学専攻)、平田 岳史(京都大学大学院理学研究科地球惑星科学専攻)、角皆 潤(名古屋大学大学院環境学研究科)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源研究開発センター)、下田 玄(産業技術総合研究所地質調査総合センター)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、横山 祐典(東京大学 大気海洋研究所 高解像度環境解析研究センター)、座長:角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)

09:45 〜 10:00

[MTT28-04] 高精度・高速U-Th-Pb年代測定法の開発:Jack Hillsジルコン年代学への応用

*大林 秀行1坂田 周平2山本 伸次3磯崎 行雄2服部 健太郎1平田 岳史1 (1.京都大学、2.東京大学、3.横浜国立大学)

キーワード:冥王代、ジャックヒルズ、LA-ICP-MS、多重検出器型ICP-MS、ジルコン、鉱物包有物

Most of the global events, such as formation of magma ocean, core-mantle segregation, crust formation, and/or chemical evolution of atmosphere, could be completed within the first 0.5 Byr of the Earth History, so called Hadean Eon. Despite the great importance of the Hadean Eon, no petrographic record can be found for this stage, and only geochemical information can be derived from small minerals such as zircons or other accessory minerals within zircons (e.g., apatite, muscovite, or biotite). For geochemical studies for Hadean Eon, many pioneering studies have been made based on the isotope geochemistry on zircons collected from Jack Hills and Mt. Narryer, Western Australia. It is widely recognized that zircons collected from these area have been thought one of the most principal clues for Hadean studies. Moreover, further detailed studies have been carried out from small inclusions in zircon crystals. Zircons from Jack Hills contain various mineral inclusions such as muscovite, quartz, biotite, apatite and so on, and about two-thirds of them are muscovite and quartz, probably due to secondary replacement of primary apatite (Hopkins et al., 2008, Rasmussen et al., 2011). Recently, biogenic carbon, as graphite inclusion, was recovered from 4.1 Ga zircon, but an abundance of carbon-bearing Jack Hills zircons of only about 1-in-10,000 (Bell et al., 2015). In addition, the percentage of Hadean zircons to detrital zircons in Jack Hills was as small as 7% (Holden et al., 2009). For these reasons, large number of age data for zircon grains must be defined to derive reliable and objective information concerning the Hadean history of the Earth. To overcome this, we have developed new analytical technique to define precise age data from combination of U-Pb (Pb-Pb) dating method with high sample throughput.
We have developed rapid and precise dating technique for zircons using laser ablation ICP-mass spectrometer (LA-ICP-MS), equipped with two Daly ion collectors (Nu Plasma IID, Wrexham, UK). Laser ablation instrument used in this study was ESI NWR193 laser ablation system (New Wave Research, Oregon, USA). Combination of multiple collector-ICPMS system and ArF Excimer laser ablation system enables us to measure Pb-Pb age for the sample within 10 second/spot, and uncertainties in the resulting Pb-Pb age data can be minimized by the multiple-collector system setup. Based on the age determination system using LA-MC-ICPMS technique, we just started to measure Pb-Pb age data from 180 grains of zircons within an hour . In this presentation, difference in the resulting age histogram for the zircons collected from Jack Hills will be discussed, and detailed observation for various inclusions in the Hadean zircons will be demonstrated in this talk.