JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-CG07] [EE] 地球惑星科学 生命圏フロンティアセッション

2017年5月22日(月) 10:45 〜 12:15 201B (国際会議場 2F)

コンビーナ:高野 淑識(海洋研究開発機構)、鈴木 庸平(東京大学大学院理学系研究科)、福士 圭介(金沢大学環日本海域環境研究センター)、柳川 勝紀(九州大学大学院比較社会文化研究院)、座長:福士 圭介(金沢大学環日本海域環境研究センター)、座長:柳川 勝紀(九州大学大学院比較社会文化研究院)、座長:高野 淑識(JAMSTEC)

10:45 〜 11:00

[BCG07-07] Experimental study of hypervelocity impact of meteoritic material into liquid water in an open system for better understanding of the fate of extraterrestrial organics in the Hadean ocean

★招待講演

*西澤 学1松井 洋平1渋谷 岳造1須田 好1高井 研1矢野 創2 (1.海洋研究開発機構、2.宇宙航空研究開発機構)

キーワード:hypervelocity impact, hedean ocean, meteorite

Unravelling the origin(s) of prebiotic organic materials that constituted protocells on the early earth is important to constrain the conditions for the emergence of life and the chemical diversity of life in the universe. One proposes that biologically relevant organic materials were mostly produced through atmospheric chemistry and mineral-water interactions from simple compounds (N2, CO2, CO, CH4) available in the early earth, whereas the other proposes that a significant amount of extraterrestrial organic materials, that were produced in the early solar system, protoplanetary disk, and molecular clouds, were delivered to the early earth and served as key components of protocells. If the latter hypothesis is correct, most of the extraterrestrial organic materials in meteorite should have been survived from thermal decomposition during hypervelocity impact into the Hadean ocean (>3 km/s), because geological evidences suggest that the ocean was already present but the continent was almost absent in the Hadean earth. However, the fate of extraterrestrial organic materials during oceanic impact is poorly understood due to the lack of experimental knowledge about the physicochemical processes associated with the hypervelocity impact of meteorite into liquid water. For better understanding of the physicochemical processes associated with the hypervelocity impact of meteorite into liquid water and the fate of impactor, we have newly establish a methodology of experimental impact in an open system that can simulate the Pressure-Temperature path of oceanic impact most faithfully. In this meeting, we report experimental results that polycarbonate and stainless steel projectiles impacted into liquid water at a velocity of 4-6 km/sec.