日本地球惑星科学連合2024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-IS07] アストロバイオロジー

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:藤島 皓介(東京工業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 〜 18:45

[MIS07-P08] Modeling the Light Environment in the Archean Oceans

*新井 千紘1、松尾 太郎1伊藤(三輪) 久美子1藤井 悠里2武田 真之介2菅野 里美1 (1.名古屋大学、2.京都大学)

Approximately 2.5 billion years ago into the Archean Era, the Earth was critically transitioning from a reducing to an oxidizing environment with the advent of oxygenic photosynthetic organisms (i.e., cyanobacteria). This global-scale oxidation of the Earth is believed to have promoted the development of the ozone layer and the prosperity of aerobic respiration, leading to the development of diverse ecosystems. On the other hand, the gradual oxidation of the surface environment before the Great Oxidation Event (GOE) might have significantly altered the light environment under water due to the deposition of Fe(III) hydroxide caused by the oxidation of dissolved ferrous iron, Fe(II), at that time. This research involved simulating underwater light transmission in the Archean oceans, considering the attenuation of light due to Fe(III) hydroxide present in the oceans. Our results provide insights into the habitability of the Earth's surface in the Archean era and contribute to the framework for understanding the co-evolution of photosynthetic organisms and their light environments. Our poster presents an overview of the transmission spectrum underwater in the Archean era and discusses its potential impact on the evolution of life.