Research School of Earth Sciences, Australian National University, Canberra, ACT 2601, Australia;
National High Magnetic Field Laboratory, Florida State University, Tallahassee, FL 32310-4005.
Proc Natl Acad Sci U S A. 2018 Jul 24;115(30):E6978-E6986. doi: 10.1073/pnas.1803866115. Epub 2018 Jul 9.
The average cell size of marine phytoplankton is critical for the flow of energy and nutrients from the base of the food web to higher trophic levels. Thus, the evolutionary succession of primary producers through Earth's history is important for our understanding of the radiation of modern protists ∼800 million years ago and the emergence of eumetazoan animals ∼200 million years later. Currently, it is difficult to establish connections between primary production and the proliferation of large and complex organisms because the mid-Proterozoic (∼1,800-800 million years ago) rock record is nearly devoid of recognizable phytoplankton fossils. We report the discovery of intact porphyrins, the molecular fossils of chlorophylls, from 1,100-million-year-old marine black shales of the Taoudeni Basin (Mauritania), 600 million years older than previous findings. The porphyrin nitrogen isotopes (δN = 5.6-10.2‰) are heavier than in younger sedimentary sequences, and the isotopic offset between sedimentary bulk nitrogen and porphyrins (ε = -5.1 to -0.5‰) points to cyanobacteria as dominant primary producers. Based on fossil carotenoids, anoxygenic green (Chlorobiacea) and purple sulfur bacteria (Chromatiaceae) also contributed to photosynthate. The low ε values, in combination with a lack of diagnostic eukaryotic steranes in the time interval of 1,600-1,000 million years ago, demonstrate that algae played an insignificant role in mid-Proterozoic oceans. The paucity of algae and the small cell size of bacterial phytoplankton may have curtailed the flow of energy to higher trophic levels, potentially contributing to a diminished evolutionary pace toward complex eukaryotic ecosystems and large and active organisms.
海洋浮游植物的平均细胞大小对于能量和营养物质从食物网底层向更高营养级的流动至关重要。因此,地球历史上初级生产者的进化演替对于我们理解大约 8 亿年前现代原生生物的辐射以及大约 2 亿年后后生动物的出现非常重要。目前,由于中元古代(约 18 亿至 8 亿年前)的岩石记录几乎没有可识别的浮游植物化石,因此很难将初级生产与大型和复杂生物的增殖联系起来。我们报告了从 11 亿年前的塔乌登尼盆地(毛里塔尼亚)海洋黑色页岩中发现完整的卟啉,卟啉是叶绿素的分子化石,比以前的发现早 6 亿年。卟啉氮同位素(δN = 5.6-10.2‰)比年轻的沉积序列更重,而沉积总氮与卟啉之间的同位素偏移(ε = -5.1 至-0.5‰)表明蓝细菌是主要的初级生产者。基于化石类胡萝卜素,厌氧绿菌(Chlorobiacea)和紫色硫细菌(Chromatiaceae)也为光合作用产物做出了贡献。低 ε 值,再加上在 16 亿至 10 亿年前的时间间隔内缺乏诊断性真核甾烷,表明藻类在中元古代海洋中作用不大。藻类的缺乏和细菌浮游植物的小细胞大小可能限制了能量流向更高的营养级,这可能导致向复杂的真核生态系统和大型活跃生物的进化速度减缓。