Lara Yannick J, McCann Andréa, Malherbe Cédric, François Camille, Demoulin Catherine F, Sforna Marie Catherine, Eppe Gauthier, De Pauw Edwin, Wilmotte Annick, Jacques Philippe, Javaux Emmanuelle J
Early Life Traces & Evolution-Astrobiology, UR Astrobiology, University of Liège, Liège, Belgium.
MolSys Research Unit, Mass Spectrometry Laboratory, University of Liège, Liège, Belgium.
Astrobiology. 2022 Jun;22(6):735-754. doi: 10.1089/ast.2021.0061. Epub 2022 Mar 25.
Ultraviolet (UV)-screening compounds represent a substantial asset for the survival of cyanobacteria in extreme environments exposed to high doses of UV radiations on modern and early Earth. Among these molecules, the halochromic pigment gloeocapsin remains poorly characterized and studied. In this study, we identified a gloeocapsin-producing cultivable cyanobacteria: the strain ULC007. We succeeded to extract, to partially purify, and to compare the dark blue pigment from both the ULC007 culture and an environmental dominated sample. FT-IR and Raman spectra of and ULC007 pigment extracts strongly suggested a common backbone structure. The high-pressure liquid chromatography-UV-MS/MS analysis of the ULC007 pigment extract allowed to narrow down the molecular formula of gloeocapsin to potentially five candidates within three classes of halochromic molecules: anthraquinone derivatives, coumarin derivatives, and flavonoids. With the discovery of gloeocapsin in , the production of this pigment is now established for three lineages of cyanobacteria (including , and ) that belong to three distinct orders (Chroococcales, Pleurocapsales, Synechoccocales), inhabiting very diverse environments. This suggests that gloeocapsin production was a trait of their common ancestor or was acquired by lateral gene transfer. This work represents an important step toward the elucidation of the structure of this enigmatic pigment and its biosynthesis, and it potentially provides a new biosignature for ancient cyanobacteria. It also gives a glimpse on the evolution of UV protection strategies, which are relevant for early phototrophic life on Earth and possibly beyond.
紫外线(UV)筛选化合物是蓝细菌在现代地球和早期地球暴露于高剂量紫外线辐射的极端环境中生存的重要资产。在这些分子中,卤变色色素球帽菌素的特征和研究仍然很少。在本研究中,我们鉴定出一种可培养的产球帽菌素蓝细菌:ULC007菌株。我们成功地从ULC007培养物和一个以环境为主的样本中提取、部分纯化并比较了深蓝色色素。ULC007色素提取物的傅里叶变换红外光谱(FT-IR)和拉曼光谱强烈表明其具有共同的主链结构。对ULC007色素提取物的高压液相色谱-紫外-串联质谱(HPLC-UV-MS/MS)分析将球帽菌素的分子式缩小到卤变色分子三类中的五个潜在候选物:蒽醌衍生物、香豆素衍生物和黄酮类化合物。随着在[具体内容缺失]中发现球帽菌素,现在已确定属于三个不同目(色球藻目、多球藻目、聚球藻目)的三个蓝细菌谱系(包括[具体内容缺失]、[具体内容缺失]和[具体内容缺失])产生这种色素,它们栖息在非常不同的环境中。这表明产生球帽菌素是它们共同祖先的一个特征,或者是通过横向基因转移获得的。这项工作是阐明这种神秘色素的结构及其生物合成的重要一步,并且它可能为古代蓝细菌提供一种新的生物标志。它还让我们初步了解了紫外线保护策略的演变,这与地球上早期的光合生物以及可能其他地方的光合生物相关。