JpGU-AGU Joint Meeting 2020

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] 水惑星学

コンビーナ:関根 康人(東京工業大学地球生命研究所)、玄田 英典(東京工業大学 地球生命研究所)、福士 圭介(金沢大学環日本海域環境研究センター)、臼井 寛裕(東京工業大学地球生命研究所)

[MIS07-P04] 海底熱水環境における非生物学的硝酸還元反応と初期地球窒素循環

*西澤 学1齋藤 拓也1眞壁 明子1渋谷 岳造1高井 研1 (1.海洋研究開発機構)

キーワード:窒素、初期地球

Nitrogen is an essential element for life as a major component of biomolecules and a substance for energy metabolism. Currently, nitrogen cycle in surface environments is mainly driven by biological processes including nitrogen fixation, nitrification and denitrification. In contrast, little is known about nitrogen cycle in the pre-biotic Earth and its relation to chemical evolution. This study focuses on nitrate chemistry during water-rock interaction in deep-sea hydrothermal environments to understand the fate of atmospherically-derived nitrate in the Hadean ocean. In this study, artificial seawater with nitrate was reacted with synthetic komatiite at i) 250oC and 500 bar or ii) 350oC and 500 bar, using a closed system hydrothermal reactor reaction cell. To unravel the pathway and kinetics of nitrate reduction, time course measurements of chemical and nitrogen isotopic composition of fluid samples were conducted during the ongoing experiments. Our experiments show multi-step reduction of nitrate to ammonium and dinitrogen and temperature-dependence on the molar ratio of final products (NH4+/N2). The experimental results imply that the Hadean deep-sea hydrothermal vents may have been favorable for chemical evolution in that both electron acceptor for energy metabolism (nitrate) and reduced nitrogen for organic synthesis (ammonium) were continuously supplied to the hydrothermal fluid-seawater mixing zone.