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dc.contributor.authorChowdhury, Wriju
dc.contributor.authorTrail, Dustin
dc.contributor.authorMiller, Martha
dc.contributor.authorSavage, Paul
dc.date.accessioned2023-03-06T12:30:10Z
dc.date.available2023-03-06T12:30:10Z
dc.date.issued2023-02-28
dc.identifier283628207
dc.identifier45619f45-8352-4a49-986b-d0e5396bf337
dc.identifier85149105657
dc.identifier.citationChowdhury , W , Trail , D , Miller , M & Savage , P 2023 , ' Eoarchean and Hadean melts reveal arc-like trace element and isotopic signatures ' , Nature Communications , vol. 14 , 1140 . https://doi.org/10.1038/s41467-023-36538-5en
dc.identifier.issn2041-1723
dc.identifier.otherJisc: 929250
dc.identifier.otherpublisher-id: s41467-023-36538-5
dc.identifier.othermanuscript: 36538
dc.identifier.otherORCID: /0000-0001-8464-0264/work/130659970
dc.identifier.urihttps://hdl.handle.net/10023/27107
dc.descriptionFunding: This work was supported by NSF EAR-1650033 (DT), NSF EAR-1751903 (DT) and NASA PC3 grant 80NSSC19M0069 (DT).en
dc.description.abstractConstraining the lithological diversity and tectonics of the earliest Earth is critical to understanding our planet’s evolution. Here we use detrital Jack Hills zircon (3.7 − 4.2 Ga) analyses coupled with new experimental partitioning data to model the silica content, Si+O isotopic composition, and trace element contents of their parent melts. Comparing our derived Jack Hills zircons’ parent melt Si+O isotopic compositions (−1.92 ≤ δ30SiNBS28 ≤ 0.53 ‰; 5.23 ≤ δ18OVSMOW ≤ 9.00 ‰) to younger crustal lithologies, we conclude that the chemistry of the parent melts was influenced by the assimilation of terrigenous sediments, serpentinites, cherts, and silicified basalts, followed by igneous differentiation, leading to the formation of intermediate to felsic melts in the early Earth. Trace element measurements also show that the formational regime had an arc-like chemistry, implying the presence of mobile-lid tectonics in the Hadean. Finally, we propose that these continental-crust forming processes operated uniformly from 4.2 to at least 3.7 Ga.
dc.format.extent10
dc.format.extent1200333
dc.language.isoeng
dc.relation.ispartofNature Communicationsen
dc.subjectQE Geologyen
dc.subjectDASen
dc.subjectMCCen
dc.subject.lccQEen
dc.titleEoarchean and Hadean melts reveal arc-like trace element and isotopic signaturesen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1038/s41467-023-36538-5
dc.description.statusPeer revieweden


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