紫外线和高氯酸钙对Mars压力和温度下氟化锶衬底上沉积的尿嘧啶的影响。

IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Astrobiology Pub Date : 2023-09-01 Epub Date: 2023-08-18 DOI:10.1089/ast.2022.0137
N Chaouche-Mechidal, F Stalport, E Caupos, E Mebold, C Azémard, C Szopa, P Coll, H Cottin
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引用次数: 0

摘要

目前和未来的太空任务都在火星上积极搜索有机物,因为它是探测潜在生物特征的关键。考虑到目前火星表面恶劣的环境条件,许多有机化合物可能无法长期保存,因为它们暴露在高能辐射下,如紫外线,而紫外线在190以上时不会被过滤 纳米的火星大气。此外,风化层中存在的强氧化性物质,如高氯酸盐,可能会增强具有天体生物学意义的有机化合物的光降解。由于目前的太空仪器分析在上表面层收集的样本,因此有必要研究火星表面有机物的稳定性。先前的实验研究表明,尿嘧啶是一种与天体生物学相关的分子,在火星表面的温度和压力条件下,当暴露于紫外线辐射时,它会迅速光解,实验量子光分解效率(φexp)为0.30 ± 0.26分子·光n-1。此外,尿嘧啶的光解导致形成更稳定的光产物,这些光产物被鉴定为尿嘧啶二聚体。本工作旨在表征火星上检测到的高氯酸钙对尿嘧啶降解的额外影响。结果表明,高氯酸钙的存在增强了尿嘧啶与φexp的光分解 = 12.3 ± 8.3分子·光n-1。尽管在这些实验中形成的一些光产物与纯尿嘧啶形成的光产物是常见的,但傅里叶变换红外光谱(FTIR)检测以前看不见的化学功能,如炔烃C ≡ C或腈C ≡ N已经表明,在辐照样品中存在高氯酸钙的情况下会形成额外的化学物质。这意味着高氯酸钙对尿嘧啶光解的影响不仅是动力学的,而且与所形成的光产物的性质有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Effects of UV and Calcium Perchlorates on Uracil Deposited on Strontium Fluoride Substrates at Mars Pressure and Temperature.

Organic matter is actively searched on Mars with current and future space missions as it is a key to detecting potential biosignatures. Given the current harsh environmental conditions at the surface of Mars, many organic compounds might not be preserved over a long period as they are exposed to energetic radiation such as ultraviolet light, which is not filtered above 190 nm by the martian atmosphere. Moreover, the presence of strong oxidizing species in the regolith, such as perchlorate salts, might enhance the photodegradation of organic compounds of astrobiological interest. Because current space instruments analyze samples collected in the upper surface layer, it is necessary to investigate the stability of organic matter at the surface of Mars. Previous experimental studies have shown that uracil, a molecule relevant to astrobiology, is quickly photolyzed when exposed to UV radiation under the temperature and pressure conditions of the martian surface with an experimental quantum efficiency of photodecomposition (φexp) of 0.30 ± 0.26 molecule·photon-1. Moreover, the photolysis of uracil leads to the formation of more stable photoproducts that were identified as uracil dimers. The present work aims to characterize the additional effect of calcium perchlorate detected on Mars on the degradation of uracil. Results show that the presence of calcium perchlorate enhances the photodecomposition of uracil with φexp = 12.3 ± 8.3 molecule·photon-1. Although some of the photoproducts formed during these experiments are common to those formed from pure uracil only, the Fourier transformation infrared (FTIR) detection of previously unseen chemical functions such as alkyne C ≡ C or nitrile C ≡ N has shown that additional chemical species are formed in the presence of calcium perchlorate in the irradiated sample. This implies that the effect of calcium perchlorate on the photolysis of uracil is not only kinetic but also related to the nature of the photoproducts formed.

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来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
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