Widespread clay authigenesis and highly congruent silicate weathering in the Marinoan aftermath

•First paired δ7Li data of different components were reported for the cap carbonates.•Marine clay authigenesis is intense during the late neoproterozoic.•δ7Li data indicate highly congruent weathering in the Marinoan aftermath. The termination of the Cryogenian period marks a transition from an extr...

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Veröffentlicht in:Earth and planetary science letters 2023-12, Vol.623, p.118423, Article 118423
Hauptverfasser: Yin, Yi-Sheng, Wei, Guang-Yi, Pogge von Strandmann, Philip A.E., Lechte, Maxwell A., Hohl, Simon V., Lin, Yi-Bo, Li, Da, Chen, Tianyu, Yang, Tao, Zhang, Feifei, Isson, Terry T., Zhang, He, Cai, Yuanfeng, Ling, Hong-Fei
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Sprache:eng
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Zusammenfassung:•First paired δ7Li data of different components were reported for the cap carbonates.•Marine clay authigenesis is intense during the late neoproterozoic.•δ7Li data indicate highly congruent weathering in the Marinoan aftermath. The termination of the Cryogenian period marks a transition from an extreme ice- to a greenhouse climate, likely initiated by increased atmospheric CO2, however uncertainties persist on continental weathering regarding this climate transition. Here we present paired lithium isotope data from carbonate (δ7Licarb) and carbonate-hosted silicate (δ7Lisili) components of the Marinoan cap carbonates to constrain C and Si cycles in the deglacial period. We find that the silicate component of cap carbonates is dominated by marine authigenic clays with minor contributions from terrestrially detrital materials and oxides. Built from δ7Lisili data, large variations of seawater δ7Li suggest a heterogeneous marine Li reservoir due to a stratified ocean in the deglacial period. Overall, widespread clay authigenesis and low seawater δ7Li values indicate active carbon-silicon cycling and congruent silicate weathering due to warm climate and exposure of fresh rock surface in the Marinoan aftermath, which promotes the deposition of cap carbonates and stabilization of Earth's surface environment.
ISSN:0012-821X
1385-013X
DOI:10.1016/j.epsl.2023.118423