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在火星浅层地下环境中,氨基酸的快速辐射降解:对寻找灭绝生命的启示。

Rapid Radiolytic Degradation of Amino Acids in the Martian Shallow Subsurface: Implications for the Search for Extinct Life.

机构信息

Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.

Department of Physics, Catholic University of America, Washington, District of Columbia, USA.

出版信息

Astrobiology. 2022 Sep;22(9):1099-1115. doi: 10.1089/ast.2021.0166. Epub 2022 Jun 24.

Abstract

Amino acids are fundamental to life as we know them as the monomers of proteins and enzymes. They are also readily synthesized under a variety of plausible prebiotic conditions and are common in carbon-rich meteorites. Thus, they represent a reasonable class of organics to target in the search for prebiotic chemistry or chemical evidence of life on Mars. However, regardless of their origin, amino acids and other organic molecules present in near-surface regolith and rocks on Mars can be degraded by exposure to cosmic rays that can penetrate to a depth of a few meters. We exposed several pure amino acids in dry and hydrated silicate mixtures and in mixtures of silicates with perchlorate salts to gamma radiation at various temperatures and radiation doses representative of the martian near-subsurface. We found that irradiation of amino acids mixed with dry silica powder increased the rate of amino acid radiolysis, with the radiolysis constants of amino acids in silicate mixtures at least a factor of 10 larger compared with the radiolysis constants of amino acids alone. The addition of perchlorate salts to the silicate samples or hydration of silicate samples further accelerated the rate of amino acid destruction during irradiation and increased the radiolysis constants by a factor of ∼1.5. Our results suggest that even low-molecular-weight amino acids could degrade in just ∼20 million years in the top 10 cm of the martian surface regolith and rock, and even faster if the material contains elevated abundances of hydrated silicate minerals or perchlorates. We did not detect evidence of amino acid racemization after gamma radiation exposure of the samples, which indicates that the chirality of some surviving amino acids may still be preserved. Our experimental results suggest serious challenges for the search of ancient amino acids and other potential organic biosignatures in the top 2 m of the martian surface.

摘要

氨基酸是生命的基础,它们是蛋白质和酶的单体。它们也可以在各种合理的前生物条件下轻易合成,并且在富含碳的陨石中很常见。因此,它们是在火星上寻找前生物化学物质或生命化学证据的合理有机物质类别之一。然而,无论它们的来源如何,火星近地表表土和岩石中存在的氨基酸和其他有机分子都可能因暴露于可以穿透到几米深的宇宙射线而降解。我们将几种纯氨基酸暴露在干燥和水合硅酸盐混合物以及硅酸盐与高氯酸盐盐的混合物中,在各种温度和辐射剂量下用伽马射线辐射,这些剂量代表了火星近地表。我们发现,将氨基酸与干燥的二氧化硅粉末混合进行辐照会增加氨基酸辐射分解的速率,与氨基酸在硅酸盐混合物中的辐射分解常数相比,至少大 10 倍。将高氯酸盐盐添加到硅酸盐样品中或水合硅酸盐样品会进一步加速辐照期间氨基酸破坏的速率,并将辐射分解常数提高约 1.5 倍。我们的结果表明,即使是低分子量的氨基酸也可能在火星表面表土和岩石的顶层 10 厘米内仅在 2000 万年左右降解,如果材料中含有高丰度的水合硅酸盐矿物或高氯酸盐,则降解速度会更快。我们没有在伽马射线辐照样品后检测到氨基酸外消旋的证据,这表明一些幸存氨基酸的手性可能仍然保留。我们的实验结果表明,在火星表面顶层 2 米范围内寻找古代氨基酸和其他潜在的有机生物特征面临着严峻的挑战。

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