日本地球惑星科学連合2025年大会

講演情報

[J] 口頭発表

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

2025年5月28日(水) 09:00 〜 10:30 301A (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)、白石 史人(広島大学 大学院先進理工系科学研究科 地球惑星システム学プログラム)、澤木 佑介(東京大学大学院総合文化研究科)、柏原 輝彦(国立研究開発法人海洋研究開発機構)、座長:白石 史人(広島大学 大学院先進理工系科学研究科 地球惑星システム学プログラム)、小宮 剛(東京大学大学院総合文化研究科広域科学専攻)

09:45 〜 10:00

[BCG06-04] Thermodynamic simulations of Algoma-type banded iron formation deposition: implications for Archean seawater and hydrothermal fluid chemistry

*石原 湧樹1小宮 剛2 (1.東京大学大学院理学系研究科地球惑星科学専攻、2.東京大学総合文化研究科)


キーワード:縞状鉄鉱層、太古代海水、アルカリ熱水、PHREEQC

Deciphering the ancient oceanic environment is crucial for understanding the coevolutionary history of life and Earth's surface conditions. Banded iron formations (BIFs), typical chemical sedimentary rocks from the Archean era, provide unique records of the hydrosphere during that period. It is classified into two types: Superior-type and Algoma-type. The latter is ubiquitously found in Archean greenstone belts in association with metabasalt and is believed to have formed under the influence of hydrothermal activity.
Traditionally, Fe-hydroxide has been considered the primary precipitate, with hydrothermal fluids thought to be acidic and Fe-rich, which is analogous to modern black smoker-type hydrothermal fluid. However, recent studies have provided alternative models. Archean high CO2 fluid is thermodynamically consistent with highly alkaline hydrothermal fluid (Shibuya et al., 2010) and petrographic observations suggest that Fe-silicate was the primary precipitate in both Superior-type and Algoma-type banded iron formations. (e.g. Ghosh, 2020; Nutman et al., 2017; Rasmussen et al., 2021). Furthermore, our recent investigations of Algoma-type BIFs from the Nuvvuagittuq supracrustal belt (>3.8 Ga) in Canada, which preserve distinct Fe-silicate and Fe-oxide bands, suggest that both silicate and hydroxide phases played major roles in Fe deposition.
Geochemical analyses indicate that Fe-silicate and silica precipitated in the absence of hydrothermal influence, forming non-hydrothermal ferruginous chert. Under weak hydrothermal conditions, enhanced Fe-silicate precipitation led to the formation of silicate-rich BIF, while stronger hydrothermal activity facilitated Fe-hydroxide precipitation, resulting in oxide-rich BIF.
The processes governing mineral precipitation are dependent on the chemical compositions of seawater and hydrothermal fluids. To elucidate these chemical properties, particularly the pH, of Archean seawater and hydrothermal fluids responsible for the formation of Algoma-type BIFs, we conducted thermodynamic simulations using the PHREEQC program. The study focused on three key components: (1) ferruginous and sulfate-free Archean seawater which is saturated in regard to Fe-silicate and silica, (2) high-temperature hydrothermal fluid resulting from interactions between seawater and basaltic materials, and (3) mineral precipitation processes triggered by the mixing of these fluids. Our results indicate that Fe-silicate and Fe-hydroxide precipitation occurs under weak and strong hydrothermal influence, respectively, only under conditions where (1) seawater is acidic and (2) hydrothermal fluid is alkaline. These findings suggest that Archean seawater was acidic and Fe-rich, with the deposition of Algoma-type BIFs occurring as a result of its mixing with alkaline hydrothermal fluids.