Water near its Supercritical Point and at Alkaline pH for the Production of Ferric Oxides and Silicates in Anoxic Conditions. A New Hypothesis for the Synthesis of Minerals Observed in Banded Iron Formations and for the Related Geobiotropic Chemistry inside Fluid Inclusions.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2018-09-01 Epub Date: 2018-08-08 DOI:10.1007/s11084-018-9560-y
Marie-Paule Bassez
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Abstract

An alternative hypothesis for the origin of the banded iron formations and the synthesis of prebiotic molecules is presented here. I show the importance of considering water near its supercritical point and at alkaline pH. It is based on the chemical equation for the anoxic oxidation of ferrous iron into ferric iron at high-subcritical conditions of water and high pH, that I extract from E-pH diagrams drawn for corrosion purposes (Geophysical Research Abstracts Vol 15, EGU2013-22 Bassez 2013, Orig Life Evol Biosph 45(1):5-13, Bassez 2015, Procedia Earth Planet Sci 17, 492-495, Bassez 2017a, Orig Life Evol Biosph 47:453-480, Bassez 2017b). The sudden change in solubility of silica, SiO2, at the critical point of water is also considered. It is shown that under these temperatures and pressures, ferric oxides and ferric silicates can form in anoxic terrains. No FeII oxidation by UV light, neither by oxygen is needed to explain the minerals of the Banded Iron Formations. The intervention of any kind of microorganisms, either sulfate-reducing, or FeII-oxidizing or O2-producing, is not required. The chemical equation for the anoxic oxidation of ferrous iron is applied to the hydrolyses of fayalite, Fe2SiO4 and ferrosilite, FeSiO3. It is shown that the BIF minerals of the Hamersley Group, Western Australia, and the Transvaal Supergroup, South Africa, are those of fayalite and ferrosilite hydrolyses and carbonations. The dissolution of crustal fayalite and ferrosilite during water-rock interaction needs to occur at T&P just below the critical point of water and in a rising water which is undersaturated in SiO2. Minerals of BIFs which can then be ejected at the surface from venting arcs are ferric oxide hydroxides, hematite, FeIII-greenalite, siderite. The greenalite dehydrated product minnesotaite forms when rising water becomes supersaturated in SiO2, as also riebeckite and stilpnomelane. Long lengths of siderite without ferric oxides neither ferric silicates can occur since the exothermic siderite formation is not so much dependent in T&P. It is also shown that the H2 which is released during hydrolysis/oxidation of fayalite/ferrosilite can lead to components of life, such as macromolecules of amino acids which are synthesized from mixtures of (CO, N2, H2O) in Sabatier-Senderens/Fischer-Tropsch & Haber-Bosch reactions or microwave or gamma-ray excitation reactions. I propose that such geobiotropic synthesis may occur inside fluid inclusions of BIFs, in the silica chert, hematite, FeIII-greenalite or siderite. Therefore, the combination of high-subcritical conditions of water, high solubility of SiO2 at these T&P values, formation of CO also at these T&P, high pH and anoxic water, leads to the formation of ferric minerals and prebiotic molecules in the process of geobiotropy.

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在缺氧条件下生成氧化铁和硅酸盐的接近超临界点和碱性 pH 值的水。带状铁地层中观察到的矿物合成及流体包裹体内部相关地质生物化学的新假说。
本文提出了关于带状铁地层起源和前生物分子合成的另一种假设。我说明了考虑接近超临界点和碱性 pH 值的水的重要性。它基于亚铁在水的高次临界状态和高pH值条件下缺氧氧化为铁的化学方程式,我从为腐蚀目的绘制的E-pH图中提取了这一方程式(《地球物理研究文摘》第15卷,EGU2013-22 Bassez 2013, Orig Life Evol Biosph 45(1):5-13, Bassez 2015, Procedia Earth Planet Sci 17, 492-495, Bassez 2017a, Orig Life Evol Biosph 47:453-480, Bassez 2017b)。研究还考虑了二氧化硅(SiO2)在水临界点溶解度的突然变化。研究表明,在这些温度和压力下,缺氧地层中会形成铁氧化物和铁硅酸盐。要解释铁带地层的矿物,既不需要紫外线氧化 FeII,也不需要氧气氧化 FeII。任何类型的微生物,无论是硫酸盐还原微生物、铁Ⅱ氧化微生物还是产氧微生物,都不需要介入。亚铁缺氧氧化的化学方程式适用于费雅石(Fe2SiO4)和铁硅石(FeSiO3)的水解。结果表明,西澳大利亚哈默斯利群和南非特兰士瓦超群的 BIF 矿物是辉绿岩和铁硅质岩水解和碳化的产物。在水与岩石相互作用过程中,地壳中的辉绿岩和铁硅质岩的溶解需要在温度和压力刚好低于水的临界点,以及在二氧化硅饱和度不足的上升水中进行。从喷气弧喷出地表的BIF矿物有氧化铁氢氧化物、赤铁矿、FeⅢ-绿帘石、菱铁矿。绿帘石的脱水产物明尼苏达石在上升的水变成过饱和的二氧化硅时形成,菱铁矿和菱锰矿也是如此。由于菱铁矿的形成放热与 T&P 的关系不大,因此可能会出现既不含铁质氧化物也不含铁质硅酸盐的长菱铁矿。研究还表明,辉绿岩/铁硅酸盐在水解/氧化过程中释放出的 H2 可以产生生命成分,如氨基酸大分子,这些氨基酸是在萨巴蒂埃-桑德伦斯/费舍尔-特罗普什和哈伯-博什反应或微波或伽马射线激发反应中由(CO、N2、H2O)混合物合成的。我提出,这种地质生物合成可能发生在 BIF 的流体包裹体、硅钙钛矿、赤铁矿、FeIII-绿帘石或菱铁矿中。因此,水的高次临界状态、二氧化硅在这些T&P值下的高溶解度、CO在这些T&P值下的形成、高pH值和缺氧水等因素结合在一起,导致在地质生物合成过程中形成铁矿物和前生物分子。
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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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