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用高能紫外光子辐照纯H2O冰中的嘧啶。

Irradiation of pyrimidine in pure H2O ice with high-energy ultraviolet photons.

作者信息

Nuevo Michel, Chen Yu-Jung, Hu Wei-Jie, Qiu Jun-Ming, Wu Shang-Ruei, Fung Hok-Sum, Chu Ching-Chi, Yih Tai-Sone, Ip Wing-Huen, Wu C-Y Robert

机构信息

1 NASA Ames Research Center , Space Science Division, Moffett Field, California, USA.

出版信息

Astrobiology. 2014 Feb;14(2):119-31. doi: 10.1089/ast.2013.1093. Epub 2014 Feb 10.

Abstract

The detection of nucleobases, the informational subunits of DNA and RNA, in several meteorites suggests that these compounds of biological interest were formed via astrophysical, abiotic processes. This hypothesis is in agreement with recent laboratory studies of irradiation of pyrimidine in H2O-rich ices with vacuum UV photons emitted by an H2-discharge lamp in the 6.9-11.3 eV (110-180 nm) range at low temperature, shown to lead to the abiotic formation of several compounds including the nucleobases uracil, cytosine, and thymine. In this work, we irradiated H2O:pyrimidine ice mixtures under astrophysically relevant conditions (14 K, ≤10(-9) torr) with high-energy UV photons provided by a synchrotron source in three different ranges: the 0(th) order light (4.1-49.6 eV, 25-300 nm), the He i line (21.2 eV, 58.4 nm), and the He ii line (40.8 eV, 30.4 nm). The photodestruction of pyrimidine was monitored with IR spectroscopy, and the samples recovered at room temperature were analyzed with liquid and gas chromatographies. Uracil and its precursor 4(3H)-pyrimidone were found in all samples, with absolute and relative abundances varying significantly from one sample to another. These results support a scenario in which compounds of biological interest can be formed and survive in environments subjected to high-energy UV radiation fields.

摘要

在几块陨石中检测到核碱基(DNA和RNA的信息亚基),这表明这些具有生物学意义的化合物是通过天体物理的非生物过程形成的。这一假设与最近的实验室研究结果一致,该研究用H₂放电灯在低温下发射的6.9 - 11.3 eV(110 - 180 nm)范围内的真空紫外光子辐照富含H₂O的冰中的嘧啶,结果显示会非生物形成包括尿嘧啶、胞嘧啶和胸腺嘧啶在内的几种化合物。在这项工作中,我们在天体物理相关条件(14 K,≤10⁻⁹托)下,用同步加速器源提供的高能紫外光子在三个不同波段辐照H₂O:嘧啶冰混合物:零级光(4.1 - 49.6 eV,25 - 300 nm)、氦Ⅰ线(21.2 eV,58.4 nm)和氦Ⅱ线(40.8 eV,30.4 nm)。用红外光谱监测嘧啶的光解,对在室温下回收的样品进行液相和气相色谱分析。在所有样品中都发现了尿嘧啶及其前体4(3H)-嘧啶酮,其绝对丰度和相对丰度在不同样品间有显著差异。这些结果支持了一种情况,即具有生物学意义的化合物可以在受到高能紫外辐射场作用的环境中形成并存活。

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