日本地球惑星科学連合2025年大会

講演情報

[E] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS08] アストロバイオロジー

2025年5月27日(火) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:藤島 皓介(東京科学大学地球生命研究所)、鈴木 庸平(東京大学大学院理学系研究科)、藤井 友香(国立天文台)、黒澤 耕介(神戸大学 大学院人間発達環境学研究科 人間環境学専攻)

17:15 〜 19:15

[MIS08-P07] The Archean Underwater Light Environment: Implications for Habitability of Earth's Surface and Potential Biosignatures

*新井 千紘1藤井 友香2伊藤(三輪) 久美子1藤井 悠里3菅野 里美1松尾 太郎1,4 (1.名古屋大学、2.国立天文台、3.京都大学、4.大阪大学)


In the Archean era, oxygenic photosynthesis dramatically transformed the water environment from a reducing to an oxidizing state, leading to the formation of large-scale banded iron formations (BIF) as dissolved Fe(II) was oxidized into iron hydroxide. The oxidation of the oceans may have triggered a significant, global-scale change in the underwater light environment, driven by the unique optical properties of the precipitated iron hydroxide. While iron hydroxide absorbed ultraviolet light, which allowed the biosphere to expand to the ocean surface, it might have also absorbed blue light, resulting in a green-light environment.
Understanding the light environment in the Archean oceans will not only provide insights into the habitability of the Earth's surface in the Archean era but also potentially offer a new approach to detecting signs of life on distant planets. In this study, we simulate the underwater light transmission and reflectance of the Archean oceans by combining measured absorption coefficients from iron hydroxide samples with scattering coefficients calculated using Mie theory. We will also discuss how the concentration of iron hydroxide could affect the color of the sea as a potential biosignature.