Solid Earth Carbon Degassing and Sequestration Since 1 Billion Years Ago

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geochemistry Geophysics Geosystems Pub Date : 2024-10-30 DOI:10.1029/2024GC011713
R. Dietmar Müller, Adriana Dutkiewicz, Sabin Zahirovic, Andrew S. Merdith, Christopher R. Scotese, Benjamin J. W. Mills, Lauren Ilano, Ben Mather
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Abstract

Solid Earth CO2 outgassing, driven by plate tectonic processes, is a key driver of carbon cycle models. However, the magnitudes and variations in outgassing are poorly constrained in deep-time. We assess plate tectonic carbon emissions and sequestration by coupling a plate tectonic model with reconstructions of oceanic plate carbon reservoirs and a thermodynamic model to quantify outfluxes from slabs and continental arcs over 1 billion years. In the early Neoproterozoic, our model predicts a peak in crustal production and net outgassing from 840 to 780 Ma that corresponds to a contemporaneous pulse in large igneous province eruptions. The Sturtian and Marinoan glaciations (717–635 Ma) correspond to a low in mid-ocean ridge outgassing, while the following Ediacaran global warming coincides with a rise in net atmospheric carbon influx, driven by an increase in plate boundary and rift length. The Cambrian, Silurian/Devonian and Triassic Jurassic hothouse climates are synchronous with a reduction in carbon sequestration flux into oceanic plates, increasing net outgassing. In contrast, the Early Cretaceous hothouse climate is accompanied by a pronounced increase in mid-ocean ridge outgassing. Both the Early Ordovician cooling and the late Paleozoic ice ages coincide with a significant decrease in net atmospheric outgassing, driven by an increase in carbon sequestration. The late Cenozoic glaciation is associated with a long-term decrease in mid-ocean ridge and rift degassing, and a pronounced increase in carbon flux into pelagic carbonate sediments. Our tectono-thermodynamic carbon cycle model provides a new foundation for future long-term climate and geochemical cycling models.

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10 亿年前以来固体地球的碳脱气和螯合作用
由板块构造过程驱动的固体地球二氧化碳排气是碳循环模型的主要驱动力。然而,在深部时间,排气量的大小和变化却没有得到很好的约束。我们通过将板块构造模型与大洋板块碳库重建和热力学模型相结合,对板块构造碳排放和螯合进行了评估,以量化 10 亿年来从板块和大陆弧流出的碳量。在新近纪早期,我们的模型预测了840至780Ma的地壳生产和净排气高峰,这与同时代的大型火成岩群喷发脉冲相吻合。斯图尔纪和马里诺纪冰川(717-635 Ma)与洋中脊脱气量的低谷相对应,而随后的埃迪卡拉纪全球变暖与板块边界和裂谷长度增加导致的大气碳净流入量上升相吻合。寒武纪、志留纪/德文纪和三叠纪侏罗纪的暖房气候与海洋板块碳封存通量的减少同步,增加了净排气量。相比之下,早白垩世温室气候伴随着洋中脊排气的明显增加。早奥陶世的降温和晚古生代的冰期都与碳封存增加导致的大气净排气量显著减少相吻合。新生代晚期的冰川与大洋中脊和裂谷脱气的长期减少以及进入浮游碳酸盐沉积物的碳通量明显增加有关。我们的构造-热力学碳循环模型为未来的长期气候和地球化学循环模型提供了新的基础。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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