大火成岩省硅酸盐风化作用下的新元古代雪球地球

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Charlotte Minsky, Robin Wordsworth, Francis A. Macdonald, Andrew H. Knoll
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引用次数: 0

摘要

雪球地球事件是对生命进化至关重要的罕见全球冰川,其成因尚不清楚。最近对斯图亚特雪球和富兰克林大火成岩省(LIP)的地质年代学研究表明,富兰克林火成岩省通过硅酸盐风化作用导致的CO 2下降导致了斯图亚特火山的形成。通过对LIP风化的气候响应进行模拟,表明在低温背景气候、大面积快速化学风化和侵蚀以及硅酸盐风化反馈强度敏感性较弱的条件下,这种启动机制是可行的。我们的模型表明,类似的显生宙LIP可能由于炎热的背景气候和较低的地形或植被造成的较低的侵蚀率而未能触发雪球,而高CO 2抑制了地球历史早期LIP的扰动。因此,我们认为,富兰克林风化形成的雪球是合理的,并且与显生宙和中元古代缺乏雪球是一致的,考虑到激发未来地质观测的特定条件。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Neoproterozoic Snowball Earth Initiation From Silicate Weathering of a Large Igneous Province

The causes of Snowball Earth events, rare global glaciations important for the evolution of life, are unknown. Recent geochronology of the Sturtian Snowball and Franklin Large Igneous Province (LIP) suggest that the Franklin caused the Sturtian via CO 2 ${\text{CO}}_{2}$ drawdown by silicate weathering. By modeling the climate response to LIP weathering, we show that this initiation mechanism is feasible given a cold background climate, rapid chemical weathering and erosion over a large area, and a weak sensitivity of the silicate weathering feedback strength. Our model indicates that similar Phanerozoic LIPs may have failed to trigger Snowballs due to hot background climates and lower erosion rates caused by lower topography or vegetation, while high CO 2 ${\text{CO}}_{2}$ suppressed LIP perturbations earlier in Earth history. We therefore argue that Snowball initiation by weathering of the Franklin is plausible and consistent with the lack of Snowballs in the Phanerozoic and mid-Proterozoic, given specific conditions that motivate future geologic observations.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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