日本地球惑星科学連合2019年大会

講演情報

[J] 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-IS11] 水惑星学

2019年5月28日(火) 15:30 〜 17:00 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:関根 康人(東京工業大学地球生命研究所)、臼井 寛裕(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)、渋谷 岳造(海洋研究開発機構)

[MIS11-P10] 初期地球深海熱水環境における非生物学的硝酸還元反応とその意義

*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:プレバイオ化学、窒素、深海熱水噴出孔

Nitrogen is an essential element for life as a major component of biomolecules and electron donor/acceptor 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 experiments, artificial seawater with nitrate was reacted with synthetic komatiite at 350oC and 500 bar. Our experiments show that a substantial amount of nitrate was reduced to ammonium in an experimental condition. This implies 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.