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

机译:恩克拉多斯:第一次观察到的原始汤可以仲裁生命起源的辩论

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A recent breakthrough publication has reported complex organic molecules in the plumes emanating from the subglacial water ocean of Saturn's moon Enceladus (Postberg et al.,2018, Nature 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.
机译:最近的突破性出版物报道了土星月亮土卫二的冰下水域海洋中羽流中的复杂有机分子(Postberg等人,2018,自然558:564-568)。基于详细的化学检查,作者引用了原始的或内源合成的富碳单体(<200 u)和聚合物(最大8000 u)。这似乎代表了第一个报道的外星人富含有机物的水体,这是生命起源早期阶段的可能环境(“益生元汤”)。可能有人会问哪种生命起源场景与土卫二上报道的分子构型更一致。观察到的单体有机物是富含碳的不饱和分子,与当今的代谢物,氨基酸和核苷酸碱基有很大的不同,但化学上非常类似于简单的脂质。提出有机聚合物类似于陆地不溶性干酪根和腐殖质,以及碳质球状陨石中发现的难熔有机大分子。作者认为,这种聚合物在长期的水相互作用下,可能分解为形成胶束的两亲物。为此,公开发表的对Murchison球粒陨石的详细分析以可能的两亲单体的多样性为主导。我们用于合成脂质胶束的特定定量模型是基于两亲的,并且受益于明显的有机多样性。因此,它与其他原始模型形成对比,其他原始模型需要存在非常特殊的构建基块,并且预计会因过量的不相关化合物而受到阻碍。因此,土卫二发现存在RNA脂质世界前场景以支持生命起源的可能性。

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