日本地球惑星科学連合2024年大会

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セッション記号 B (地球生命科学) » B-CG 地球生命科学複合領域・一般

[B-CG06] 地球史解読:冥王代から現代まで

2024年5月29日(水) 09:00 〜 10:30 コンベンションホール (CH-A) (幕張メッセ国際会議場)

コンビーナ:小宮 剛(東京大学大学院総合文化研究科広域科学専攻)、加藤 泰浩(東京大学)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源センター)、中村 謙太郎(東京大学大学院工学系研究科システム創成学専攻)、座長:渡辺 泰士(気象研究所/東京大学)、小宮 剛(東京大学大学院総合文化研究科広域科学専攻)


09:15 〜 09:30

[BCG06-02] Hydrogen isotope compositions in early earth mantle from apatite inclusions in detrital early Archean zircons from the Jack Hills metaconglomerate, W. Australis

*山本 伸次1伊藤 正一2、大野 剛4小宮 剛3坂田 周平5青木 翔吾6 (1.横浜国立大学大学院環境情報研究院、2.京都大学大学院理学研究科 、3.東京大学大学院総合文化研究科、4.学習院大学理学部、5.東京大学地震研究所、6.秋田大学大学院国際資源学研究)

キーワード:水の起源、水素同位体比、アパタイト、砕屑性ジルコン

The origin of Earth’s water remains debated. The hydrogen isotope distribution in earth mantle could be attributed for the origin of Earth’s water. Several scenarios have been proposed, such as delivery from carbonaceous/enstatite chondrites and comets, and capture of solar nebula (e.g. Piani et al., 2020; Young et al., 2023). The present deep earth mantle has been predicted to be D-poor signature (Hallis et al., 2015). Hydrogen isotope compositions are the key to understanding the origin of Earth's water. But their values have not yet been determined, since the lack of terrestrial samples for hydrogen isotope analyses prior to 4 billion years ago limits the means to decipher the origin of Earth’s water. In order to constrain the hydrogen isotope distribution in the early Earth, we have measured hydrogen isotopic compositions (δD; deuterium/hydrogen (D/H) ratio) of minute apatite inclusions in detrital zircons from the Jack hills metaconglomerate, which yields zircon grains with U-Pb ages ranging 3.0 to 4.4 Ga (Wild et al., 2001). Secondary ion mass spectrometry (SIMS) was applied for hydrogen isotope analyses, and laser ablation microprobe-inductively coupled plasma mass spectrometer (LA-ICPMS) was for trace element analysis and U-Pb age analysis, respectively. We evaluated the micro-cracks in zircon to exclude the negative possibility of secondary hydrogen interaction of apatite inclusions using polarized microscopy and cathodoluminescence (CL) images. The hydrogen isotopic compositions for all apatite inclusions (n = 16) were determined with δDSMOW falling within the range from -52 to -354 ‰. The δD values of apatite inclusions with visible cracks or healed cracks observed with CL were likely to be D-rich, on the other hands, those of apatite inclusions with no visible cracks were D-poor, ranged from -130 to a maximum of -354 ‰. This indicates that the hydrogen isotope ratio of apatite is shifted toward D-rich hydrogen isotopic compositions due to the presence of cracks on host zircons, probably from interaction with terrestrial fluid. As a surprising result, the apatite inclusions in the two zircons showed D-poor values beyond the analytical error, the δD = -222 ± 2‰ and -354 ± 23‰, respectively. The Sc/Yb versus Nb/Yb distribution patterns from detrital zircons were used to distinguish those crystals having magma types of arc, mid-ocean ridge and ocean island origins (Grimes, 2015). On diagrams of Sc/Yb versus Nb/Yb, most zircon analyzed were plotted on arc type, but these two grains plotted on mantle type (mid-ocean ridge or ocean island). Therefore, these two apatite inclusions considered to represent hydrogen isotope compositions of the mantle showed δD = -222±2‰ with 3.9 Ga and -354 ± 23‰ with 3.6 Ga. These results indicate that the hydrogen isotopic compositions of mantle in the early Archean were D-poor. Similar depleted (D-poor) hydrogen isotope composition is reported from melt inclusions of 3.3 Ga komatiites (Sobolev et al., 2019) but our data resulted in tracking back as far as 3.9 Ga. We conclude that pristine apatite inclusions in detrital zircons could retain evidence of ancient δD value, and may provide new constraints on the origin of Earth’s water.


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Piani, L. et al. Earth’s water may have been inherited from material similar to enstatite chondrite meteorites. Science 1110–1113 (2020) doi:10.1126/science.aba1948.
Sobolev, A. V. et al. Deep hydrous mantle reservoir provides evidence for crustal recycling before 3.3 billion years ago. Nature 571, 555–559 (2019).
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