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土卫二:首次观测到原始汤可能仲裁生命起源之争。

Enceladus: First Observed Primordial Soup Could Arbitrate Origin-of-Life Debate.

机构信息

Department of Molecular Genetics, the Weizmann Institute of Science, Rehovot, Israel.

Helmholtz Zentrum Muenchen, Research Unit Analytical BioGeoChemistry, Neuherberg, Germany.

出版信息

Astrobiology. 2019 Oct;19(10):1263-1278. doi: 10.1089/ast.2019.2029. Epub 2019 Jul 22.

Abstract

A recent breakthrough publication has reported complex organic molecules in the plumes emanating from the subglacial water ocean of Saturn's moon Enceladus (Postberg 2018, 558:564-568). Based on detailed chemical scrutiny, the authors invoke primordial or endogenously synthesized carbon-rich monomers (<200 u) and polymers (up to 8000 u). This appears to represent the first reported extraterrestrial organics-rich water body, a conceivable milieu for early steps in life's origin ("prebiotic soup"). One may ask which origin-of-life scenario appears more consistent with the reported molecular configurations on Enceladus. The observed monomeric organics are carbon-rich unsaturated molecules, vastly different from present-day metabolites, amino acids, and nucleotide bases, but quite chemically akin to simple lipids. The organic polymers are proposed to resemble terrestrial insoluble kerogens and humic substances, as well as refractory organic macromolecules found in carbonaceous chondritic meteorites. The authors posit that such polymers, upon long-term hydrous interactions, might break down to micelle-forming amphiphiles. In support of this, published detailed analyses of the Murchison chondrite are dominated by an immense diversity of likely amphiphilic monomers. Our specific quantitative model for compositionally reproducing lipid micelles is amphiphile-based and benefits from a pronounced organic diversity. It thus contrasts with other origin models, which require the presence of very specific building blocks and are expected to be hindered by excess of irrelevant compounds. Thus, the Enceladus finds support the possibility of a pre-RNA Lipid World scenario for life's origin.

摘要

最近的一项突破性研究成果报告称,在土星卫星土卫二的冰下海洋羽流中发现了复杂的有机分子(Postberg 2018,558:564-568)。基于详细的化学分析,作者提出了原始的或内源性合成的富碳单体(<200 u)和聚合物(高达 8000 u)。这似乎代表了第一个报道的富含外星有机物的水体,这是生命起源的早期步骤(“原始汤”)的一个可以想象的环境。人们可能会问,哪种生命起源情景与土卫二上报告的分子结构更为一致。观察到的单体有机物是富碳的不饱和分子,与当今的代谢物、氨基酸和核苷酸碱基大不相同,但与简单的脂质在化学上非常相似。这些有机聚合物被提议类似于陆地不溶性干酪根和腐殖质,以及在碳质球粒陨石中发现的难溶性有机大分子。作者假设,这些聚合物在长期的水合作用下,可能会分解成形成胶束的两亲性物质。这一点得到了支持,发表的默奇森陨石的详细分析主要由大量可能的两亲性单体组成。我们用于复制脂质胶束组成的特定定量模型基于两亲性物质,并且得益于显著的有机多样性。因此,这与其他起源模型形成对比,其他模型需要存在非常特定的构建块,并且预计会受到无关化合物的过多阻碍。因此,土卫二的发现支持了生命起源的 RNA 前脂质世界情景的可能性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/36c0/6785169/417b187f4725/fig-1.jpg

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