Department of Earth and Planetary Sciences, University of California, Davis, Davis, California, USA.
Microbiology Graduate Group, University of California, Davis, Davis, California, USA.
Appl Environ Microbiol. 2024 Jun 18;90(6):e0009324. doi: 10.1128/aem.00093-24. Epub 2024 May 31.
The oxygenation of Earth's atmosphere represents the quintessential transformation of a planetary surface by microbial processes. In turn, atmospheric oxygenation transformed metabolic evolution; molecular clock models indicate the diversification and ecological expansion of respiratory metabolisms in the several hundred million years following atmospheric oxygenation. Across this same interval, the geological record preserves C enrichment in some carbonate rocks, called the Lomagundi-Jatuli excursion (LJE). By combining data from geologic and genomic records, a self-consistent metabolic evolution model emerges for the LJE. First, fermentation and methanogenesis were major processes remineralizing organic carbon before atmospheric oxygenation. Once an ozone layer formed, shallow water and exposed environments were shielded from UVB/C radiation, allowing the expansion of cyanobacterial primary productivity. High primary productivity and methanogenesis led to preferential removal of C into organic carbon and CH. Extreme and variable C enrichments in carbonates were caused by C-depleted CH loss to the atmosphere. Through time, aerobic respiration diversified and became ecologically widespread, as did other new metabolisms. Respiration displaced fermentation and methanogenesis as the dominant organic matter remineralization processes. As CH loss slowed, dissolved inorganic carbon in shallow environments was no longer highly C enriched. Thus, the loss of extreme C enrichments in carbonates marks the establishment of a new microbial mat ecosystem structure, one dominated by respiratory processes distributed along steep redox gradients. These gradients allowed the exchange of metabolic by-products among metabolically diverse organisms, providing novel metabolic opportunities. Thus, the microbially induced oxygenation of Earth's atmosphere led to the transformation of microbial ecosystems, an archetypal example of planetary microbiology.IMPORTANCEThe oxygenation of Earth's atmosphere represents the most extensive known chemical transformation of a planetary surface by microbial processes. In turn, atmospheric oxygenation transformed metabolic evolution by providing oxidants independent of the sites of photosynthesis. Thus, the evolutionary changes during this interval and their effects on planetary-scale biogeochemical cycles are fundamental to our understanding of the interdependencies among genomes, organisms, ecosystems, elemental cycles, and Earth's surface chemistry through time.
地球大气的氧化作用代表了微生物过程对行星表面最广泛的已知化学转化。反过来,大气氧化作用通过提供与光合作用场所无关的氧化剂来改变代谢进化。因此,在这段时间内发生的进化变化及其对行星尺度生物地球化学循环的影响,对于我们理解基因组、生物体、生态系统、元素循环和地球表面化学随时间的相互依存关系至关重要。