Lithium isotope evidence for a plumeworld ocean in the aftermath of the Marinoan snowball Earth

dc.contributor.authorGan, Tianen
dc.contributor.authorTian, Mengen
dc.contributor.authorWang, Xi-Kaien
dc.contributor.authorWang, Shijieen
dc.contributor.authorLiu, Xiao-Mingen
dc.contributor.authorJiang, Ganqingen
dc.contributor.authorGill, Benjamin C.en
dc.contributor.authorNolan, Morrisonen
dc.contributor.authorKaufman, Alan J.en
dc.contributor.authorLuo, Taiyien
dc.contributor.authorXiao, Shuhaien
dc.date.accessioned2024-11-12T20:24:24Zen
dc.date.available2024-11-12T20:24:24Zen
dc.date.issued2024-11-05en
dc.description.abstractThe snowball Earth hypothesis predicts that continental chemical weathering diminished substantially during, but rebounded strongly after, the Marinoan ice age some 635 Mya. Defrosting the planet would result in a plume of fresh glacial meltwater with a different chemical composition from underlying hypersaline seawater, generating both vertical and lateral salinity gradients. Here, we test the plumeworld hypothesis using lithium isotope compositions in the Ediacaran Doushantuo cap dolostone that accumulated in the aftermath of the Marinoan snowball Earth along a proximal–distal (nearshore–offshore) transect in South China. Our data show an overall decreasing δ⁷Li trend with distance from the shoreline, consistent with the variable mixing of a meltwater plume with high δ⁷Li (due to incongruent silicate weathering on the continent) and hypersaline seawater with low δ⁷Li (due to synglacial distillation). The evolution of low δ⁷Li of synglacial seawater, as opposed to the modern oceans with high δ⁷Li, was likely driven by weak continental chemical weathering coupled with strong reverse weathering on the seafloor underneath silica-rich oceans. The spatial pattern of δ⁷Li is also consistent with the development and then collapse of the meltwater plume that occurred at the time scale of cap dolostone accumulation. Therefore, the δ7Li data are consistent with the plumeworld hypothesis, considerably reduced chemical weathering on the continent during the Marinoan snowball Earth, and enhanced reverse weathering on the seafloor of Precambrian oceans.en
dc.description.sponsorshipThis research was supported by the NSF (EAR-2021207 to S.X. and EAR-2020593 to A.J.K.), the Patricia Caldwell Faculty Fellowship at Virginia Tech, the University of North Carolina at Chapel Hill, and the National Natural Science Foundation of China (U1812402). T.G. acknowledges financial support from China Scholarship Council and China Postdoctoral Council (PC2022055). M.T. acknowledges a CSH Fellowship of Universität Bern.en
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.doihttps://doi.org/10.1073/pnas.2407419121en
dc.identifier.issue46en
dc.identifier.urihttps://hdl.handle.net/10919/121607en
dc.identifier.volume121en
dc.language.isoenen
dc.publisherNational Academies of Scienceen
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivatives 4.0 Internationalen
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/en
dc.subjectcryogenian perioden
dc.subjectplumeworld modelen
dc.subjectlithium isotopesen
dc.subjectcontinental weatheringen
dc.subjectreverse weatheringen
dc.titleLithium isotope evidence for a plumeworld ocean in the aftermath of the Marinoan snowball Earthen
dc.title.serialProceedings of the National Academies of Scienceen
dc.typeArticle - Refereeden
dc.type.dcmitypeTexten

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