Japan Geoscience Union Meeting 2018

Presentation information

[EE] Evening Poster

B (Biogeosciences) » B-AO Astrobiology & the Origin of Life

[B-AO01] Astrobiology

Tue. May 22, 2018 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)

convener:Hikaru Yabuta(Hiroshima University, Department of Earth and Planetary Systems Science), Seiji Sugita(Department of Earth and Planetary Science, Graduate School of Science Sciece, The University of Tokyo), Misato Fukagawa(名古屋大学, 共同), Fujishima Kosuke(Tokyo Institute of Technology, Earth-Life Science Institute)

[BAO01-P01] Formaldehyde formation in asteroid impacts: a new origin of prebiotic sugar precursor

*Saeka Masuda1, Takamichi Kobayashi2, Takeshi Kakegawa1, Yoshihiro Furukawa1 (1.Tohoku University, 2.National Institute for Materials Science)

Keywords:early Earth, asteroid impact, formaldehyde, sugar, abiotic organic synthesis

Ribose, the sole sugar in RNA, is a product of the Formose reaction in which formaldehyde condenses under alkaline conditions. Thus, the accumulation of formaldehyde on the prebiotic Earth is a key step for the formation of biological sugars including ribose. Impacts by extraterrestrial objects were far more frequent on the early Earth than present day. Oceanic impacts of iron-bearing asteroids have been investigated as a generating process of organics, such as amino acids and nucleobases on the prebiotic Earth. However, it remains unclear whether formaldehyde forms in such oceanic impact events. In this study, we investigated the formation of formaldehyde as well as the formation of sugars in an experiment simulating impact-induced reactions by asteroids. A series of shock-recovery experiments was conducted using a single-stage propellant gun. Starting materials containing analogues mineral mixture of meteorite, NaH13CO3, water, and gaseous N2 were enclosed in a stainless-steel capsule. Water was replaced with ammonia water or aqueous solution of Ca(OH)2 in some experimental conditions. A 13C-enriched carbon source (i.e., NaH13CO3) was chosen for the starting material to distinguish between products and contaminants. A flyer collided to the capsule at a velocity of approximately 0.9 km/s to generate a shock wave. After cleaning all the surface of the recovered capsule, the sample was extracted from the capsule with ultrapure water. Aldehyde analysis and sugar analysis was performed by ultra-performance liquid chromatography tandem mass spectrometry (UHPLC-MS/MS) and gas chromatography mass spectrometry (GC/MS), respectively. Analogue mineral mixtures of meteorites were also collected after the impact and analyzed by X-ray powder diffraction. As a result of analyzing the mineral mixtures, the formation of siderite was confirmed. As a result of UHPLC-MS/MS and GC/MS, formation of 13C-formaldehyde was confirmed in all experimental conditions, although sugars were below the detection limit. The yield of formaldehyde was greater in experiments using ammonia whereas the yield was not much different in the experiment with Ca(OH)2. Metallic iron in the analogue meteorite minerals were oxidized to Fe2+ and formed siderite. Bicarbonate was expected to have been abundant in the prebiotic ocean. Further, CO2 was a major component of the atmosphere on the prebiotic Earth. Therefore, the formation of formaldehyde from bicarbonate in the present study suggest that the impacts of asteroids to the early ocean is a new substantial source of formaldehyde on the prebiotic Earth.