Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain.
Department of Physics and Mathematics and Department of Automatics, University of Alcalá, Madrid, Spain.
Astrobiology. 2023 May;23(5):563-604. doi: 10.1089/ast.2022.0083. Epub 2023 Mar 7.
Lipid molecules are organic compounds, insoluble in water, and based on carbon-carbon chains that form an integral part of biological cell membranes. As such, lipids are ubiquitous in life on Earth, which is why they are considered useful biomarkers for life detection in terrestrial environments. These molecules display effective membrane-forming properties even under geochemically hostile conditions that challenge most of microbial life, which grants lipids a universal biomarker character suitable for life detection beyond Earth, where a putative biological membrane would also be required. What discriminates lipids from nucleic acids or proteins is their capacity to retain diagnostic information about their biological source in their recalcitrant hydrocarbon skeletons for thousands of millions of years, which is indispensable in the field of astrobiology given the time span that the geological ages of planetary bodies encompass. This work gathers studies that have employed lipid biomarker approaches for paleoenvironmental surveys and life detection purposes in terrestrial environments with extreme conditions: hydrothermal, hyperarid, hypersaline, and highly acidic, among others; all of which are analogous to current or past conditions on Mars. Although some of the compounds discussed in this review may be abiotically synthesized, we focus on those with a biological origin, namely lipid biomarkers. Therefore, along with appropriate complementary techniques such as bulk and compound-specific stable carbon isotope analysis, this work recapitulates and reevaluates the potential of lipid biomarkers as an additional, powerful tool to interrogate whether there is life on Mars, or if there ever was.
脂质分子是有机化合物,不溶于水,基于碳-碳链,是生物细胞膜的重要组成部分。因此,脂质在地球上的生命中无处不在,这就是为什么它们被认为是在地球环境中探测生命的有用生物标志物。这些分子即使在具有地球化学挑战性的条件下也具有有效的膜形成特性,这些条件挑战了大多数微生物的生命,这使得脂质具有普遍的生物标志物特征,适合在地球以外的地方探测生命,在那里也需要假设的生物膜。脂质与核酸或蛋白质的区别在于,它们能够在其顽固的碳氢骨架中保留有关其生物来源的诊断信息,这在天体生物学领域是必不可少的,因为行星体的地质时代涵盖了很长的时间跨度。这项工作汇集了在具有极端条件的地球环境中(如热液、超干旱、高盐和高酸性等),使用脂质生物标志物方法进行古环境调查和生命探测的研究;所有这些条件都与火星当前或过去的条件类似。虽然本综述中讨论的一些化合物可能是无生命合成的,但我们专注于那些具有生物起源的化合物,即脂质生物标志物。因此,除了批量和化合物特异性稳定碳同位素分析等适当的补充技术外,这项工作还总结和重新评估了脂质生物标志物作为一种额外的、强大的工具,用于探究火星上是否存在生命,或者是否曾经存在过生命。