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Hydroxymethanesulfonate from Volcanic Sulfur Dioxide: A 'Mineral' Reservoir for Formaldehyde and Other Simple Carbohydrates in Prebiotic Chemistry

机译:火山二氧化硫中的羟甲磺酸盐:益生元化学中甲醛和其他简单碳水化合物的“矿物质”储藏室

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While formaldehyde (HCHO) was likely generated in Earth's prebiotic atmosphere by ultraviolet light, electrical discharge, and/or volcano-created lightning, HCHO could not have accumulated in substantial amounts in prebiotic environments, including those needed for prebiotic processes that generate nucleosidic carbohydrates. HCHO at high concentrations in alkaline solutions self-reacts in the Cannizzaro reaction to give methanol and formate, neither having prebiotic value. Here, we explore the possibility that volcanic sulfur dioxide (SO2) might have generated a reservoir for Hadean HCHO by a reversible reaction with HCHO to give hydroxymethanesulfonate (HMS). We show that salts of HMS are stable as solids at 90 degrees C and do not react with themselves in solution, even at high (8 M) concentrations. This makes them effective stores of HCHO, since the reverse reaction slowly delivers HCHO back into an environment where it can participate in prebiotically useful reactions. Specifically, we show that in alkaline borate solutions, HCHO derived from HMS allows formation of borate-stabilized carbohydrates as effectively as free HCHO, without losing material to Cannizzaro products. Further, we show that SO2 can perform similar roles for glycolaldehyde and glyceraldehyde, two intrinsically unstable carbohydrates that are needed by various models as precursors for RNA building blocks. Zircons from the Hadean show that the Hadean mantle likely provided volcanic SO2 at rates at least as great as the rates of atmospheric HCHO generation, making the formation of Hadean HMS essentially unavoidable. Thus, hydroxymethylsulfonate adducts of formaldehyde, glycolaldehyde, and glyceraldehyde, including the less soluble barium, strontium, and calcium salts, are likely candidates for prebiotically useful organic minerals on early Earth.
机译:虽然紫外线,放电和/或火山喷发的闪电可能在地球的益生元大气中生成甲醛(HCHO),但在益生元环境中,包括在产生核苷碳水化合物的益生元过程所需的环境中,HCHO不可能大量积累。碱性溶液中高浓度的HCHO在Cannizzaro反应中自我反应,生成甲醇和甲酸,两者都不具有益生元的价值。在这里,我们探讨了火山二氧化硫(SO2)可能通过与HCHO发生可逆反应生成羟基甲磺酸盐(HMS)而为Hadean HCHO生成储层的可能性。我们显示,HMS的盐在90摄氏度下作为固体稳定,即使在高浓度(> 8 M)下也不会在溶液中与自身反应。这使它们成为有效的HCHO储存剂,因为逆反应会缓慢将HCH​​O送回到可以参与益生元有用反应的环境中。具体而言,我们表明,在碱性硼酸盐溶液中,源自HMS的HCHO可以与游离HCHO一样有效地形成硼酸盐稳定的碳水化合物,而不会丢失Cannizzaro产品的材料。此外,我们表明SO2可以对乙醇醛和甘油醛(两种内在不稳定的碳水化合物)起类似的作用,这两种碳水化合物是各种模型所需的RNA构建基团的前体。哈德族的锆石表明,哈德族地幔提供的火山SO2的速率至少与大气中HCHO的产生速率相同,这使得Hadean HMS的形成基本上是不可避免的。因此,甲醛,乙醇醛和甘油醛的羟甲基磺酸盐加合物,包括难溶的钡,锶和钙盐,很可能是地球早期益生元有用的有机矿物质的候选物。

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