The Institute for Geoscience Research, WA-Organic and Isotope Geochemistry Centre (WA-OIGC), School of Earth and Planetary Sciences, Curtin University, Bentley, Western Australia, Australia.
UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK.
Geobiology. 2024 Jan-Feb;22(1):e12583. doi: 10.1111/gbi.12583.
In 2016, IODP-ICDP Expedition 364 recovered an 829-meter-long core within the peak ring of the Chicxulub impact crater (Yucatán, Mexico), allowing us to investigate the post-impact recovery of the heat-sterilized deep continental microbial biosphere at the impact site. We recently reported increased cell biomass in the impact suevite, which was deposited within the first few hours of the Cenozoic, and that the overall microbial communities differed significantly between the suevite and the other main core lithologies (i.e., the granitic basement and the overlying Early Eocene marine sediments; Cockell et al., 2021). However, only seven rock intervals were previously analyzed from the geologically heterogenic and impact-deformed 587-m-long granitic core section below the suevite interval. Here, we used 16S rRNA gene profiling to study the microbial community composition in 45 intervals including (a) 31 impact-shocked granites, (b) 7 non-granitic rocks (i.e., consisting of suevite and impact melt rocks intercalated into the granites during crater formation and strongly serpentinized pre-impact sub-volcanic, ultramafic basanite/dolerite), and (c) 7 cross-cut mineral veins of anhydride and silica. Most recovered microbial taxa resemble those found in hydrothermal systems. Spearman correlation analysis confirmed that the borehole temperature, which gradually increased from 47 to 69°C with core depth, significantly shaped a subset of the vertically stratified modern microbial community composition in the granitic basement rocks. However, bacterial communities differed significantly between the impoverished shattered granites and nutrient-enriched non-granite rocks, even though both lithologies were at similar depths and temperatures. Furthermore, Spearman analysis revealed a strong correlation between the microbial communities and bioavailable chemical compounds and suggests the presence of chemolithoautotrophs, which most likely still play an active role in metal and sulfur cycling. These results indicate that post-impact microbial niche separation has also occurred in the granitic basement lithologies, as previously shown for the newly formed lithologies. Moreover, our data suggest that the impact-induced geochemical boundaries continue to shape the modern-day deep biosphere in the granitic basement underlying the Chicxulub crater.
2016 年,IODP-ICDP 考察队在奇克苏鲁布陨石坑(墨西哥尤卡坦半岛)的峰环内采集了一段 829 米长的岩芯,使我们能够研究撞击点深大陆微生物生物圈在热灭菌后的恢复情况。我们最近报告称,在新生代的最初几个小时内沉积的撞击角砾岩中,细胞生物量增加了,而且微生物群落与角砾岩和其他主要岩芯岩石类型(即花岗岩基底和上覆的早始新世海相沉积物;Cockell 等人,2021)之间存在显著差异。然而,在撞击角砾岩间隔以下的 587 米长的花岗岩核心部分,此前只对地质异质和撞击变形的 7 个岩石间隔进行了分析。在这里,我们使用 16S rRNA 基因谱分析研究了 45 个间隔的微生物群落组成,包括(a)31 个冲击花岗岩,(b)7 个非花岗岩岩石(即由撞击角砾岩和撞击熔融岩石组成,在陨石坑形成过程中插入花岗岩中,并强烈蛇纹石化了前撞击次火山、超镁铁质玄武岩/辉绿岩),和(c)7 个无水和硅的交叉矿物脉。大多数回收的微生物类群与在热液系统中发现的微生物类群相似。Spearman 相关分析证实,随着岩芯深度的增加,钻孔温度从 47°C 逐渐升高到 69°C,显著影响了花岗岩基底岩石中垂直分层的现代微生物群落组成的一部分。然而,即使在相似的深度和温度下,贫化的破碎花岗岩和富含营养的非花岗岩岩石之间的细菌群落也有显著差异。此外,Spearman 分析显示微生物群落与可利用的化学化合物之间存在很强的相关性,并表明存在化能自养生物,它们很可能仍在金属和硫循环中发挥积极作用。这些结果表明,撞击后微生物生态位的分离也发生在花岗岩基底岩石中,就像新形成的岩石类型一样。此外,我们的数据表明,撞击引起的地球化学边界继续塑造奇克苏鲁布陨石坑下的花岗岩基底深部生物圈。