地球上的益生元有机物和氧气的起源。水、甲烷、氨和硫化氢催化前光合作用和羰基硫化物催化二氧化碳还原的一个案例。

R. Larsson, A. Malek
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摘要

据估计,地球大约有45亿年的历史,现在人们认为,到43亿年前,地球可能已经发展出适合生命存在的物理化学条件,当时地球的大气主要由水(H2O)蒸汽、氮(N2)和二氧化碳(CO2)组成,甲烷(CH4)、一氧化碳(CO)、氨(NH3)、氢(H2)、硫化氢(H2S)和其他硫化合物,如羰基硫化氢(COS),地球的大气层是还原性的,没有游离氧。已知最古老的化石记录显示,生命大约在37亿年前出现。也有人认为,只有在病毒进行缺氧光合作用,然后植物进行氧气光合作用产生大规模的生物化学分子和分子氧(O2)之后,生命才得以大规模繁殖和进化。但这需要一段时间的原始生命形式的进化,比如复制细胞,这需要大量的碳基益生元化学物质,由辩证的机会和必然性介导,就像后来的生物进化一样。这需要在大约10亿年的时间里,在有限的、动态的、物理化学适宜的局部环境中,以足够的数量和浓度生产出特定的益生元成分。但是,只有上面提到的几种原始化合物,最丰富的是水和二氧化碳,已经存在于地球上,可能是形成第一个再生细胞所必需的大量和各种生命前化学物质的来源。根据我们其中一人(RL)提出的SET (Selective Energy Transfer Theory)理论,我们第一次有理由推测,羰基硫化物(COS)催化H2O和其他较少的分子(如CH4、NH3和H2S)还原CO2是形成益生元化学成分和地球上第一个再生细胞的化学进化的决定性先决条件。
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Origin of Prebiotic Organics and Oxygen on Earth. A case for the Pre-Photosynthetic and Carbonyl Sulfide Catalyzed Reduction of Carbon Dioxide by Water, Methane, Ammonia and Hydrogen sulfide.
It is estimated that the earth is about 4.5 billion years old and it is now believed that by 4.3 billion years ago, earth may have developed physico-chemical conditions suitable to support life, when its atmosphere consisted largely of water (H2O) vapor, nitrogen (N2), and carbon dioxide (CO2) with much smaller amounts of methane (CH4), carbon monoxide (CO), ammonia (NH3), hydrogen (H2), hydrogen sulfide (H2S) and other sulfur compounds like carbonyl sulfide (COS), and the earth had a reducing atmosphere without any free oxygen. The oldest known fossil records show that life came into being about 3.7 billion years ago. It is also believed that life proliferated and evolved in largest scale only after first aoxygenic photosynthesis by viruses and then oxygenic photosynthesis by plants produced large scale biochemocules and molecular oxygen (O2). But this necessitated a period of the evolution of primitive life forms like reprocing cells, which required enormous carbon-based prebiotic chemicals mediated by dialectical chance and necessity as is the case with later biological evolution. This had to involve the production within about a billion years, of specific prebiotic ingradients in enough quantities, in sufficient concentration in a limited, dynamic and physicochemically suitable localized evironment. But only the few primitive chemical compounds mentioned above, most abundent being H2O and CO2 , laready existing on earth, potentially could be source of enormous amount and variety of prebiotic chemicals necessary for the formation the  first reproducing cell. Based on the SET (Selective Energy Transfer Theory) developed by one of us (RL), we have reason to speculate for the first time that the carbonyl sulphide (COS) catalyzed reduction of CO2 by H2O and by other less abundant molecules like CH4, NH3 and H2S was the decisive prerequisite for the formation of  prebiotic chemical ingredients and for the chemical evolution of the first reproducing cell on Earth.
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