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泰坦硫醇中的核酸碱基和泰坦液态中的可能遗传系统。

Nucleic acid bases in Titan tholins and possible genetic systems in the Titan liquidosphere.

机构信息

High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki, 305-0801, Japan.

Yokohama National University, 79-1 Tokiwadai, Hodogaya-ku, Yokohama, 240-8501, Japan.

出版信息

Life Sci Space Res (Amst). 2019 Feb;20:20-29. doi: 10.1016/j.lssr.2018.11.002. Epub 2018 Nov 26.

Abstract

Titan is the largest moon of Saturn and possesses a dense atmosphere composed of nitrogen and methane. Various types of organic compounds (hydrocarbons, nitriles, etc.) have been found on Titan, which were generated by reactions taking place in its atmosphere. These reactions are considered to provide crucial evidence for chemical reactions which may have occurred in the atmosphere of primitive Earth. Cassini discovered several lakes of liquid methane and ethane on Titan's surface; in addition, the presence of ammonia water in its sub-surface was implied. In order to simulate the chemical reactions in Titan's atmosphere, gas mixtures of nitrogen and methane have been exposed to plasma discharges to synthesize complex organic matters. In this study, we focused on the formation of nucleic acid bases and related compounds recovered from synthesized Titan tholins. The five nucleic acid bases that terrestrial life uses (adenine, cytosine, thymine, guanine, and uracil) have already been reported to be present in synthesized Titan tholins. Purines and pyrimidines, including the five aforementioned nucleic acid bases, were extracted from synthesized Titan tholins and analyzed by HPLC and LC/MS. As a result, the pyrimidine bases of isocytosine and 2, 4-diaminopyrimidine were detected together with the terrestrial nucleic acid bases of adenine, uracil, and cytosine. The results obtained in conjunction with those from previous studies show that some nucleic acid bases and related pyrimidine bases are found in synthesized Titan tholins, suggesting that chemical evolutions toward xenogenetic systems could occur in Titan's environment.

摘要

泰坦是土星最大的卫星,拥有由氮气和甲烷组成的稠密大气层。在泰坦上已经发现了各种类型的有机化合物(碳氢化合物、腈等),这些化合物是在其大气层中发生的反应产生的。这些反应被认为为原始地球上可能发生的化学反应提供了重要证据。卡西尼号在泰坦表面发现了几个液态甲烷和乙烷湖泊;此外,还暗示其地下存在氨水溶液。为了模拟泰坦大气层中的化学反应,已经将氮气和甲烷的气体混合物暴露于等离子体放电中以合成复杂的有机物。在这项研究中,我们专注于从合成的泰坦肖林中回收的核酸碱基和相关化合物的形成。地球上生命使用的五种核酸碱基(腺嘌呤、胞嘧啶、胸腺嘧啶、鸟嘌呤和尿嘧啶)已经被报道存在于合成的泰坦肖林中。从合成的泰坦肖林中提取嘌呤和嘧啶,包括上述五种核酸碱基,并通过 HPLC 和 LC/MS 进行分析。结果,检测到了异胞嘧啶和 2,4-二氨基嘧啶的嘧啶碱基,以及腺嘌呤、尿嘧啶和胞嘧啶这三种地球上的核酸碱基。与以前的研究结果相结合的结果表明,一些核酸碱基和相关嘧啶碱基存在于合成的泰坦肖林中,这表明在泰坦的环境中可能发生向异种系统的化学进化。

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