Zammuto Vincenzo, Rizzo Maria G, De Plano Laura M, Franco Domenico, Guglielmino Salvatore, Caccamo Maria T, Magazù Salvatore, Fujimori Akira, Giudice Angelina Lo, Guglielmin Mauro, McAlpin Kevin Roderick, Moeller Ralf, Gugliandolo Concetta
Department of Chemical, Biological, Pharmaceutical and Environmental Sciences, Research Centre for Extreme Environments and Extremophiles, University of Messina, V.le F. Stagno d'Alcontres 31, 98166 Messina, Italy.
Department of Mathematics, Computer Sciences, Physics and Earth Sciences, University of Messina, V.le F. Stagno d'Alcontres 31, 98166 Messina, Italy.
Life (Basel). 2020 Oct 30;10(11):264. doi: 10.3390/life10110264.
Extremophiles are optimal models in experimentally addressing questions about the effects of cosmic radiation on biological systems. The resistance to high charge energy (HZE) particles, and helium (He) ions and iron (Fe) ions (LET at 2.2 and 200 keV/µm, respectively, until 1000 Gy), of spores from two thermophiles, SBP3 and T14, and two psychrotolerants, sp. A34 and A43, was investigated. Spores survived He irradiation better, whereas they were more sensitive to Fe irradiation (until 500 Gy), with spores from thermophiles being more resistant to irradiations than psychrotolerants. The survived spores showed different germination kinetics, depending on the type/dose of irradiation and the germinant used. After exposure to He 1000 Gy, D-glucose increased the lag time of thermophilic spores and induced germination of psychrotolerants, whereas L-alanine and L-valine increased the germination efficiency, except alanine for A43. FTIR spectra showed important modifications to the structural components of spores after Fe irradiation at 250 Gy, which could explain the block in spore germination, whereas minor changes were observed after He radiation that could be related to the increased permeability of the inner membranes and alterations of receptor complex structures. Our results give new insights on HZE resistance of extremophiles that are useful in different contexts, including astrobiology.
极端微生物是通过实验解决宇宙辐射对生物系统影响问题的理想模型。研究了两种嗜热菌SBP3和T14以及两种耐冷菌A34和A43的孢子对高电荷能量(HZE)粒子、氦(He)离子和铁(Fe)离子(LET分别为2.2和200 keV/µm,直至1000 Gy)的抗性。孢子对He辐射的耐受性更好,而对Fe辐射(直至500 Gy)更敏感,嗜热菌的孢子比耐冷菌对辐射更具抗性。存活的孢子表现出不同的萌发动力学,这取决于辐射的类型/剂量和所用的萌发剂。暴露于1000 Gy的He后,D-葡萄糖增加了嗜热孢子的延迟时间并诱导了耐冷菌的萌发,而L-丙氨酸和L-缬氨酸提高了萌发效率,但A43的丙氨酸除外。傅里叶变换红外光谱(FTIR)显示,250 Gy的Fe辐射后孢子的结构成分发生了重要变化,这可以解释孢子萌发的受阻,而He辐射后观察到的微小变化可能与内膜通透性增加和受体复合物结构改变有关。我们的结果为极端微生物的HZE抗性提供了新的见解,这在包括天体生物学在内的不同背景下都很有用。