NASA Ames Research Center, Space Science Division, Moffett Field, California 94035, USA.
Astrobiology. 2012 Apr;12(4):295-314. doi: 10.1089/ast.2011.0726.
Although not yet identified in the interstellar medium (ISM), N-heterocycles including nucleobases-the information subunits of DNA and RNA-are present in carbonaceous chondrites, which indicates that molecules of biological interest can be formed in non-terrestrial environments via abiotic pathways. Recent laboratory experiments and ab initio calculations have already shown that the irradiation of pyrimidine in pure H(2)O ices leads to the formation of a suite of oxidized pyrimidine derivatives, including the nucleobase uracil. In the present work, NH(3):pyrimidine and H(2)O:NH(3):pyrimidine ice mixtures with different relative proportions were irradiated with UV photons under astrophysically relevant conditions. Liquid- and gas-chromatography analysis of the resulting organic residues has led to the detection of the nucleobases uracil and cytosine, as well as other species of prebiotic interest such as urea and small amino acids. The presence of these molecules in organic residues formed under abiotic conditions supports scenarios in which extraterrestrial organics that formed in space and were subsequently delivered to telluric planets via comets and meteorites could have contributed to the inventory of molecules that triggered the first biological reactions on their surfaces.
虽然星际介质(ISM)中尚未发现 N-杂环化合物,包括核苷酸碱基——DNA 和 RNA 的信息亚单位,但它们存在于碳质球粒陨石中,这表明生物感兴趣的分子可以通过非生物途径在非地球环境中形成。最近的实验室实验和从头算计算已经表明,在纯 H(2)O 冰中嘧啶的辐照会导致一系列氧化嘧啶衍生物的形成,包括核苷碱基尿嘧啶。在本工作中,在天体物理相关条件下用 UV 光子辐照具有不同相对比例的 NH(3):嘧啶和 H(2)O:NH(3):嘧啶冰混合物。对所得有机残留物的液-和气-相色谱分析导致检测到核苷碱基尿嘧啶和胞嘧啶,以及其他具有前生物兴趣的物质,如尿素和小氨基酸。这些分子在非生物条件下形成的有机残留物中的存在支持了这样的情景,即在太空中形成的外星有机物随后通过彗星和陨石被输送到地球行星,可能对引发其表面上第一批生物反应的分子库存做出了贡献。