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在一项长期的米勒型实验中,添加磷酸钙和硫酸镁的“海水”产生了糖类、核酸碱基、核苷、脂质、氨基酸和寡肽。

"Sea Water" Supplemented with Calcium Phosphate and Magnesium Sulfate in a Long-Term Miller-Type Experiment Yields Sugars, Nucleic Acids Bases, Nucleosides, Lipids, Amino Acids, and Oligopeptides.

作者信息

Root-Bernstein Robert, Baker Andrew G, Rhinesmith Tyler, Turke Miah, Huber Jack, Brown Adam W

机构信息

Department of Physiology, Michigan State University, East Lansing, MI 48824, USA.

Department of Chemical Engineering and Biotechnology, University of Cambridge, Cambridge CB3 0AS, UK.

出版信息

Life (Basel). 2023 Jan 18;13(2):265. doi: 10.3390/life13020265.

Abstract

The standard approach to exploring prebiotic chemistry is to use a small number of highly purified reactants and to attempt to optimize the conditions required to produce a particular end product. However, purified reactants do not exist in nature. We have previously proposed that what drives prebiotic evolution are complex chemical ecologies. Therefore, we have begun to explore what happens if one substitutes "sea water", with its complex mix of minerals and salts, for distilled water in the classic Miller experiment. We have also adapted the apparatus to permit it to be regassed at regular intervals so as to maintain a relatively constant supply of methane, hydrogen, and ammonia. The "sea water" used in the experiments was created from Mediterranean Sea salt with the addition of calcium phosphate and magnesium sulfate. Tests included several types of mass spectrometry, an ATP-monitoring device capable of measuring femtomoles of ATP, and a high-sensitivity cAMP enzyme-linked immunoadsorption assay. As expected, amino acids appeared within a few days of the start of the experiment and accumulated thereafter. Sugars, including glucose and ribose, followed as did long-chain fatty acids (up to C). At three-to-five weeks after starting the experiment, ATP was repeatedly detected. Thus, we have shown that it is possible to produce a "one-pot synthesis" of most of the key chemical prerequisites for living systems within weeks by mimicking more closely the complexity of real-world chemical ecologies.

摘要

探索益生元化学的标准方法是使用少量高度纯化的反应物,并尝试优化生产特定终产物所需的条件。然而,纯化的反应物在自然界中并不存在。我们之前曾提出,驱动益生元进化的是复杂的化学生态。因此,我们开始探索,如果在经典的米勒实验中,用含有复杂矿物质和盐分的“海水”替代蒸馏水会发生什么。我们还对实验装置进行了改进,使其能够定期重新注入气体,以维持甲烷、氢气和氨气的相对稳定供应。实验中使用的“海水”是由地中海海水添加磷酸钙和硫酸镁制成的。测试包括几种类型的质谱分析、一种能够测量飞摩尔ATP的ATP监测装置,以及一种高灵敏度的环磷酸腺苷酶联免疫吸附测定法。正如预期的那样,氨基酸在实验开始后的几天内就出现了,并在之后不断积累。包括葡萄糖和核糖在内的糖类以及长链脂肪酸(最长到C)也相继出现。在实验开始后的三到五周,多次检测到了ATP。因此,我们已经表明,通过更紧密地模拟现实世界化学生态的复杂性,有可能在数周内实现对生命系统大多数关键化学先决条件的“一锅合成”。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3e5b/9959757/ee29c8ceb165/life-13-00265-g0A1.jpg

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