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巨陨石撞击对古太古代地表环境和生命的影响。

Effect of a giant meteorite impact on Paleoarchean surface environments and life.

机构信息

Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138.

Department of Earth and Planetary Sciences, Stanford University, Stanford, CA 94305.

出版信息

Proc Natl Acad Sci U S A. 2024 Oct 29;121(44):e2408721121. doi: 10.1073/pnas.2408721121. Epub 2024 Oct 21.

Abstract

Large meteorite impacts must have strongly affected the habitability of the early Earth. Rocks of the Archean Eon record at least 16 major impact events, involving bolides larger than 10 km in diameter. These impacts probably had severe, albeit temporary, consequences for surface environments. However, their effect on early life is not well understood. Here, we analyze the sedimentology, petrography, and carbon isotope geochemistry of sedimentary rocks across the S2 impact event (37 to 58 km carbonaceous chondrite) forming part of the 3.26 Ga Fig Tree Group, South Africa, to evaluate its environmental effects and biological consequences. The impact initiated 1) a giant tsunami that mixed Fe-rich deep waters into the Fe-poor shallow waters and washed debris into coastal areas, 2) heating that caused partial evaporation of surface ocean waters and likely a short-term increase in weathering and erosion on land, and 3) injection of P from vaporization of the S2 bolide. Strata immediately above the S2 impact event contain abundant siderites, which are associated with organic matter and exhibit light and variable δC values. This is consistent with microbial iron cycling in the wake of the impact event. Thus, the S2 impact likely had regional, if not global, positive and negative effects on life. The tsunami, atmospheric heating, and darkness would likely have decimated phototrophic microbes in the shallow water column. However, the biosphere likely recovered rapidly, and, in the medium term, the increase in nutrients and iron likely facilitated microbial blooms, especially of iron-cycling microbes.

摘要

大型陨石撞击肯定强烈影响了早期地球的可居住性。太古宙时代的岩石记录了至少 16 次主要的撞击事件,涉及直径大于 10 公里的陨石。这些撞击可能对地表环境造成了严重的、尽管是暂时的、影响。然而,它们对早期生命的影响还没有得到很好的理解。在这里,我们分析了南非 3.26 亿年前 Fig Tree 组中 S2 撞击事件(37 至 58 公里碳质球粒陨石)形成的沉积岩的沉积学、岩石学和碳同位素地球化学,以评估其环境影响和生物后果。撞击引发了 1)一场巨大的海啸,将富含铁的深海与贫铁的浅海混合,并将碎片冲入沿海地区,2)加热导致表层海洋水部分蒸发,陆地风化和侵蚀可能短期增加,3)S2 陨石蒸发导致磷的注入。S2 撞击事件之上的地层中含有丰富的菱铁矿,这些菱铁矿与有机物有关,并表现出较轻和可变的δC 值。这与撞击事件后微生物铁循环一致。因此,S2 撞击事件可能对生命产生了区域性的,甚至全球性的积极和消极影响。海啸、大气加热和黑暗可能会摧毁浅海水柱中的光合微生物。然而,生物圈可能会迅速恢复,从中期来看,营养物质和铁的增加可能会促进微生物的爆发,尤其是铁循环微生物。

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