日本地球惑星科学連合2015年大会

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セッション記号 B (地球生命科学) » B-AO 宇宙生物学・生命起源

[B-AO01] Astrobiology: Origins, Evolution, Distribution of Life

2015年5月28日(木) 16:15 〜 18:00 105 (1F)

コンビーナ:*小林 憲正(横浜国立大学大学院工学研究院)、山岸 明彦(東京薬科大学生命科学部)、大石 雅寿(国立天文台天文データセンター)、田近 英一(東京大学大学院新領域創成科学研究科複雑理工学専攻)、掛川 武(東北大学大学院理学研究科地学専攻)、井田 茂(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:掛川 武(東北大学大学院理学研究科地学専攻)、井田 茂(東京工業大学大学院理工学研究科地球惑星科学専攻)

17:30 〜 17:45

[BAO01-16] 約32億年前の縞状鉄鉱層中の希土類元素と酸素同位体組成から制約される海洋環境

*山口 耕生1矢作 智隆1清川 昌一2 (1.東邦大学、NASA Astrobiology Institute、2.九州大学)

キーワード:太古代, 縞状鉄鉱層, 希土類元素, 酸素同位体, 南アフリカ

A popular mechanism for BIF (Banded Iron Formation) deposition is that Fe-oxides were precipitated in deep-water setting by oxidation of dissolved Fe2+ supplied from submarine hydrothermal activity, by dissolved oxygen supplied from oxygenic photosynthesis in the surface ocean. When Fe-oxides precipitated, rare earth elements (REEs) were adsorbed on their surface. REE compositions of seawater have been recognized to reflect redox state of seawater and the extent of input from hydrothermal activity. In this study, we aimed to estimate Mesoarchean seawater chemistry and temperature based on REE signatures of 3.2 Ga old BIFs. These are directly related to pO2 and pCO2 in the Mesoarchean atmosphere.
Samples were collected from outcrops of the Mapepe Fm at the bottom of the Fig Tree Group and Msauli Member in the Onverwacht Group, both belonging to the Swaziland Supergroup. Powdered rock samples were analyzed for their major element, REE, and oxygen isotope compositions. Samples with <0.5 wt.% Al2O3 are considered to be pure chemical precipitates and thus used for further discussion.
Chondrite-normalized REE patterns of the Mapepe samples show positive Eu anomaly, elevated Y/Ho ratios, and LREE>HREE. Furthermore, there exist positive correlations among the extent of positive Eu anomaly, ∑Fe2O3 contents, and Y/Ho ratios. The maximum Y/Ho ratios are surprisingly comparable to those of the modern ocean. These characteristics suggest a coherent story for BIF deposition; Fe2+ emanated from submarine hydrothermal activity was oxidized to Fe3+, which, with enhanced particle reactivity, absorbed dissolved REEs and Y in the 3.2 Ga ocean, producing elevated near-modern Y/Ho ratios. The Msauli samples are mostly enriched in Al2O3 and have clastics-dominated REE patterns, suggesting deposition at shallower, more proximal setting.
We also estimate temperature of seawater 3.2 Ga ago from which the BIF precipitated to be around 60-70℃, based on their oxygen isotope compositions of silicate- and Fe-oxide phases and their binary mixing model. Although crustal heat flux at that time was most likely higher than today, the pCO2 in the Mesoarchean atmosphere should have been high enough to warm up the seawater under faint young Sun. The pO2 in the Mesoarchean atmosphere should have been high enough to oxidize dissolved Fe2+ supplied from submarine hydrothermal activity.