School of Life Sciences, Arizona State University, Tempe, Arizona, USA
Center for Fundamental and Applied Microbiomics, Biodesign Institute, Arizona State University, Tempe, Arizona, USA.
mBio. 2019 May 21;10(3):e00561-19. doi: 10.1128/mBio.00561-19.
The biosynthesis of the unique cyanobacterial (oxyphotobacterial) indole-phenolic UVA sunscreen, scytonemin, is coded for in a conserved operon that contains both core metabolic genes and accessory, aromatic amino acid biosynthesis genes dedicated to supplying scytonemin's precursors. Comparative genomics shows conservation of this operon in many, but not all, cyanobacterial lineages. Phylogenetic analyses of the operon's aromatic amino acid genes indicate that five of them were recruited into the operon after duplication events of their respective housekeeping cyanobacterial cognates. We combined the fossil record of cyanobacteria and relaxed molecular clock models to obtain multiple estimates of these duplication events, setting a minimum age for the evolutionary advent of scytonemin at 2.1 ± 0.3 billion years. The same analyses were used to estimate the advent of cyanobacteria as a group (and thus the appearance of oxygenic photosynthesis), at 3.6 ± 0.2 billion years before present. interpretation of 16S rRNA-based Bayesian analyses was consistent with these estimates. Because of physiological constraints on the use of UVA sunscreens in general, and the biochemical constraints of scytonemin in particular, scytonemin's age must postdate the time when Earth's atmosphere turned oxic, known as the Great Oxidation Event (GOE). Indeed, our biological estimate is in agreement with independent geochemical estimates for the GOE. The difference between the estimated ages of oxygenic photosynthesis and the GOE indicates the long span (on the order of a billion years) of the era of "oxygen oases," when oxygen was available locally but not globally. The advent of cyanobacteria, with their invention of oxygenic photosynthesis, and the Great Oxidation Event are arguably among the most important events in the evolutionary history of life on Earth. Oxygen is a significant toxicant to all life, but its accumulation in the atmosphere also enabled the successful development and proliferation of many aerobic organisms, especially metazoans. The currently favored dating of the Great Oxidation Event is based on the geochemical rock record. Similarly, the advent of cyanobacteria is also often drawn from the same estimates because in older rocks paleontological evidence is scarce or has been discredited. Efforts to obtain molecular evolutionary alternatives have offered widely divergent estimates. Our analyses provide a novel means to circumvent these limitations and allow us to estimate the large time gap between the two events.
蓝细菌(oxyphotobacterial)独特的吲哚-酚类 UVA 防晒剂——石莼素的生物合成由一个保守的操纵子编码,该操纵子包含核心代谢基因和辅助的芳香族氨基酸生物合成基因,专门为石莼素的前体提供物质。比较基因组学表明,该操纵子在许多蓝细菌谱系中得到了保守,但并非所有谱系都如此。对该操纵子的芳香族氨基酸基因的系统发育分析表明,其中 5 个基因是在各自的管家蓝细菌同源物的复制事件后被招募到操纵子中的。我们结合蓝细菌的化石记录和放松的分子钟模型,获得了这些复制事件的多个估计值,从而将石莼素进化出现的最小年龄设定为 21 亿±3 亿年前。同样的分析被用于估计蓝细菌作为一个群体的出现(因此也是有氧光合作用的出现),其时间在距今 36 亿±2 亿年前。16S rRNA 基于贝叶斯分析的解释与这些估计值一致。由于一般来说 UVA 防晒霜的使用受到生理限制,以及石莼素的生化限制,因此石莼素的年龄必须晚于地球大气变为氧化性的时间,即大氧化事件(GOE)。事实上,我们的生物估计与 GOE 的独立地球化学估计值一致。有氧光合作用和 GOE 的估计年龄之间的差异表明,在“氧气绿洲”时代,氧气在局部存在但在全球不存在,这种情况持续了很长一段时间(大约十亿年)。蓝细菌的出现及其有氧光合作用的发明,以及大氧化事件,可以说是地球生命进化史上最重要的事件之一。氧气对所有生命都是一种重要的有毒物质,但它在大气中的积累也使许多需氧生物,特别是后生动物,得以成功发展和繁殖。目前大氧化事件的流行日期是基于地球化学岩石记录。同样,蓝细菌的出现也常常来自于同样的估计,因为在更古老的岩石中,古生物学证据稀缺或已被否定。获得分子进化替代物的努力提供了广泛不同的估计值。我们的分析提供了一种新颖的方法来规避这些限制,并使我们能够估计这两个事件之间的巨大时间差距。