Meessen J, Sánchez F J, Sadowsky A, de la Torre R, Ott S, de Vera J-P
Institut für Botanik, Heinrich-Heine-Universität (HHU), Universitätsstr.1, 40225, Düsseldorf, Germany,
Orig Life Evol Biosph. 2013 Dec;43(6):501-26. doi: 10.1007/s11084-013-9348-z. Epub 2013 Dec 22.
Lichens, which are symbioses of a fungus and one or two photoautotrophs, frequently tolerate extreme environmental conditions. This makes them valuable model systems in astrobiological research to fathom the limits and limitations of eukaryotic symbioses. Various studies demonstrated the high resistance of selected extremotolerant lichens towards extreme, non-terrestrial abiotic factors including space exposure, hypervelocity impact simulations as well as space and Martian parameter simulations. This study focusses on the diverse set of secondary lichen compounds (SLCs) that act as photo- and UVR-protective substances. Five lichen species used in present-day astrobiological research were compared: Buellia frigida, Circinaria gyrosa, Rhizocarpon geographicum, Xanthoria elegans, and Pleopsidium chlorophanum. Detailed investigation of secondary substances including photosynthetic pigments was performed for whole lichen thalli but also for axenically cultivated mycobionts and photobionts by methods of UV/VIS-spectrophotometry and two types of high performance liquid chromatography (HPLC). Additionally, a set of chemical tests is presented to confirm the formation of melanic compounds in lichen and mycobiont samples. All investigated lichens reveal various sets of SLCs, except C. gyrosa where only melanin was putatively identified. Such studies will help to assess the contribution of SLCs on lichen extremotolerance, to understand the adaptation of lichens to prevalent abiotic stressors of the respective habitat, and to form a basis for interpreting recent and future astrobiological experiments. As most of the identified SLCs demonstrated a high capacity in absorbing UVR, they may also explain the high resistance of lichens towards non-terrestrial UVR.
地衣是一种真菌与一两种光合自养生物的共生体,常常能耐受极端环境条件。这使其成为天体生物学研究中极具价值的模型系统,有助于深入了解真核生物共生关系的极限。多项研究表明,某些极端耐受地衣对包括太空暴露、超高速撞击模拟以及太空和火星参数模拟在内的极端非地球非生物因素具有高度抗性。本研究聚焦于多种作为光保护和紫外线辐射(UVR)保护物质的地衣次生化合物(SLCs)。对当前天体生物学研究中使用的五种地衣物种进行了比较:冷疣衣、环裂黄衣、地图黄卷衣、优美黄藓和绿褶石蕊。通过紫外/可见分光光度法和两种高效液相色谱(HPLC)方法,不仅对整个地衣叶状体,还对无菌培养的菌共生体和光共生体进行了包括光合色素在内的次生物质的详细研究。此外,还进行了一系列化学测试,以确认地衣和菌共生体样本中黑色素化合物的形成。除环裂黄衣仅推测鉴定出黑色素外,所有研究的地衣都显示出各种不同的SLCs。此类研究将有助于评估SLCs在地衣极端耐受性中的作用,理解地衣对各自栖息地普遍存在的非生物应激源的适应性,并为解释近期和未来的天体生物学实验奠定基础。由于大多数已鉴定的SLCs在吸收UVR方面表现出很高的能力,它们也可能解释了地衣对非地球UVR的高度抗性。