Unexpected Thiocyanate Adsorption onto Ferrihydrite Under Prebiotic Chemistry Conditions.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Dimas A M Zaia, Paulo C G de Carvalho, Rafael B Samulewski, Rodrigo de Carvalho Pereira, Cássia Thaïs B V Zaia
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引用次数: 10

Abstract

The most crucial role played by minerals was in the preconcentration of biomolecules or precursors of biomolecules in prebiotic seas. If this step had not occurred, molecular evolution would not have occurred. Thiocyanate is an important molecule in the formation of biomolecules as well as a catalyst for prebiotic reactions. The adsorption of thiocyanate onto ferrihydrite was carried out under pH and ion composition conditions in seawater that resembled those of prebiotic Earth. The seawater used in this work had high Mg2+, Ca2+ and SO42- concentrations. The most important result of this work was that ferrihydrite adsorbed thiocyanateata pH value (7.2 ± 0.2) that usually does not adsorb thiocyanate. The high adsorptivity of Mg2+, Ca2+ and SO42-onto ferrihydrite showed that seawater ions can act as carriers of thiocyanate to the ferrihydrite surface, creating a huge outer-sphere complex. Kinetic adsorption and isotherm experiments showed the best fit for the pseudo-second-order model and an activation energy of 23.8 kJ mol-1forthe Langmuir-Freundlich model, respectively. Thermodynamic data showed positive ΔG values, which apparently contradict the adsorption isotherm data and kinetic data that was obtained. The adsorption of thiocyanate onto ferrihydrite could be explained by coupling with the exergonic SO42- adsorption onto ferrihydrite. The FTIR spectra showed no difference between the C≡N stretching peaks of adsorbed thiocyanate and free thiocyanate, corroborating the formation of an outer-sphere complex. All the results demonstrated the importance of the artificial seawater composition for the adsorption of thiocyanate and for understanding prebiotic chemistry.

在益生元化学条件下硫氰酸盐在水合铁上的意外吸附。
矿物质在生物元海洋中最重要的作用是对生物分子或生物分子前体的富集。如果这一步没有发生,分子进化就不会发生。硫氰酸盐是生物分子形成的重要分子,也是益生元反应的催化剂。硫氰酸盐在类似于益生元地球的海水pH和离子组成条件下吸附在水合铁上。本研究使用的海水具有较高的Mg2+、Ca2+和SO42-浓度。本研究最重要的结果是在pH值为(7.2±0.2)时,水合铁吸附了通常不吸附硫氰酸盐的硫氰酸盐。Mg2+、Ca2+和so42在水合铁表面的高吸附性表明,海水离子可以作为硫氰酸盐的载体到达水合铁表面,形成一个巨大的外球配合物。动力学吸附和等温实验结果表明,Langmuir-Freundlich模型最适合拟二阶模型,活化能为23.8 kJ mol-1。热力学数据为正ΔG值,这明显与吸附等温线数据和动力学数据相矛盾。硫氰酸盐在水合铁上的吸附可以解释为与水合铁上的逸出性SO42-吸附耦合作用。FTIR光谱显示吸附的硫氰酸盐和游离的硫氰酸盐的C≡N拉伸峰没有差异,证实了外球配合物的形成。这些结果表明了人工海水成分对硫氰酸盐吸附和理解益生元化学的重要性。
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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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