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太古代和诺亚撞击形成甲醛的实验研究。

Experimental Investigation of the Formation of Formaldehyde by Hadean and Noachian Impacts.

机构信息

Department of Earth Science, Tohoku University, Sendai, Japan.

National Institute for Materials Science, Tsukuba, Japan.

出版信息

Astrobiology. 2021 Apr;21(4):413-420. doi: 10.1089/ast.2020.2320.

DOI:10.1089/ast.2020.2320
PMID:33784199
Abstract

Formaldehyde (FA) is an important precursor in the abiotic synthesis of major biomolecules including amino acids, sugars, and nucleobases. Thus, spontaneous formation of prebiotic FA must have been crucial for the chemical origin of life. The frequent impacts of meteorites and asteroids on Hadean Earth have been considered one of the abiotic synthetic processes of organic compounds. However, the impact-induced formation of FA from CO as the major atmospheric constituent has not been confirmed yet. This study investigated the formation of FA in impact-induced reactions among meteoritic minerals, bicarbonate, gaseous nitrogen, and water to simulate the abiotic process experimentally. Products were analyzed with ultra-high-performance liquid chromatography/tandem mass spectrometry and powder X-ray diffraction techniques. The results show the formation of FA and oxidation of metallic iron to siderite in the impact shock experiments. This indicates that this important prebiotic molecule was also synthesized by impacts of iron-bearing meteorites/asteroids on the Hadean oceans. The impact events might have generated spatially and temporally FA-enriched localized environments. Moreover, the impact-induced synthesis of FA may have also occurred on Noachian Mars given the presence of liquid water and a CO-N-rich atmosphere on the planet.

摘要

甲醛(FA)是包括氨基酸、糖和核碱基在内的主要生物分子的非生物合成中的重要前体。因此,前生物 FA 的自发形成对于生命的化学起源一定是至关重要的。流星体和小行星对 Hadean 地球的频繁撞击被认为是有机化合物的一种非生物合成过程。然而,从主要大气成分 CO 形成 FA 的撞击诱导尚未得到证实。本研究通过模拟实验,调查了陨石矿物、碳酸氢盐、气态氮和水之间的撞击反应中 FA 的形成。使用超高效液相色谱/串联质谱和粉末 X 射线衍射技术分析产物。结果表明,在冲击实验中形成了 FA 和金属铁向菱铁矿的氧化。这表明,这种重要的前生物分子也是由含铁的流星体/小行星对 Hadean 海洋的撞击合成的。撞击事件可能在局部空间和时间上产生 FA 富集的环境。此外,由于火星上存在液态水和富含 CO-N 的大气,撞击诱导的 FA 合成也可能发生在 Noachian 火星上。

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