Rosa Caroline Antunes, Bergantini Alexandre, Herczku Péter, Mifsud Duncan V, Lakatos Gergő, Kovács Sándor T S, Sulik Béla, Juhász Zoltán, Ioppolo Sergio, Quitián-Lara Heidy M, Mason Nigel J, Lage Claudia
Carlos Chagas Filho Institute of Biophysics, Federal University of Rio de Janeiro, Rio de Janeiro 21941-170, Brazil.
Celso Suckow da Fonseca Federal Centre for Technological Education, Rio de Janeiro 20271-110, Brazil.
Life (Basel). 2023 Nov 14;13(11):2208. doi: 10.3390/life13112208.
The purine nucleobases adenine and guanine are complex organic molecules that are essential for life. Despite their ubiquitous presence on Earth, purines have yet to be detected in observations of astronomical environments. This work therefore proposes to study the infrared spectra of purines linked to terrestrial biochemical processes under conditions analogous to those found in the interstellar medium. The infrared spectra of adenine and guanine, both in neat form and embedded within an ice made of HO:NH:CH:CO:CHOH (10:1:1:1:1), were analysed with the aim of determining which bands attributable to adenine and/or guanine can be observed in the infrared spectrum of an astrophysical ice analogue rich in other volatile species known to be abundant in dense molecular clouds. The spectrum of adenine and guanine mixed together was also analysed. This study has identified three purine nucleobase infrared absorption bands that do not overlap with bands attributable to the volatiles that are ubiquitous in the dense interstellar medium. Therefore, these three bands, which are located at 1255, 940, and 878 cm, are proposed as an infrared spectral signature for adenine, guanine, or a mixture of these molecules in astrophysical ices. All three bands have integrated molar absorptivity values () greater than 4 km mol, meaning that they should be readily observable in astronomical targets. Therefore, if these three bands were to be observed together in the same target, then it is possible to propose the presence of a purine molecule (i.e., adenine or guanine) there.
嘌呤核碱基腺嘌呤和鸟嘌呤是对生命至关重要的复杂有机分子。尽管它们在地球上无处不在,但在天文环境的观测中尚未检测到嘌呤。因此,这项工作提议在类似于星际介质中发现的条件下,研究与地球生化过程相关的嘌呤的红外光谱。分析了腺嘌呤和鸟嘌呤的红外光谱,包括纯态以及嵌入由HO:NH:CH:CO:CHOH(10:1:1:1:1)制成的冰中的情况,目的是确定在富含其他已知在致密分子云中大量存在的挥发性物质的天体物理冰类似物的红外光谱中,哪些可归因于腺嘌呤和/或鸟嘌呤的谱带能够被观测到。还分析了腺嘌呤和鸟嘌呤混合在一起的光谱。这项研究确定了三个嘌呤核碱基红外吸收带,它们与致密星际介质中普遍存在的挥发性物质的谱带不重叠。因此,这三个位于1255、940和878 cm处的谱带,被提议作为天体物理冰中腺嘌呤、鸟嘌呤或这些分子混合物的红外光谱特征。所有这三个谱带的积分摩尔吸光率值()都大于4 km mol,这意味着它们应该很容易在天文目标中被观测到。因此,如果在同一目标中同时观测到这三个谱带,那么就有可能推断那里存在嘌呤分子(即腺嘌呤或鸟嘌呤)。