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dc.contributor.authorBoocock, Toby J.
dc.contributor.authorStüeken, Eva E.
dc.contributor.authorBybee, Grant M.
dc.contributor.authorKönig, Ramona
dc.contributor.authorBoyce, Adrian J.
dc.contributor.authorPrytulak, Julie
dc.contributor.authorBuisman, Iris
dc.contributor.authorMikhail, Sami
dc.date.accessioned2023-08-01T15:30:01Z
dc.date.available2023-08-01T15:30:01Z
dc.date.issued2023-09-01
dc.identifier290652821
dc.identifierce81837f-2063-47d0-8670-a2ca0c9511ea
dc.identifier85166219725
dc.identifier.citationBoocock , T J , Stüeken , E E , Bybee , G M , König , R , Boyce , A J , Prytulak , J , Buisman , I & Mikhail , S 2023 , ' Equilibrium partitioning and isotopic fractionation of nitrogen between biotite, plagioclase, and K-feldspar during magmatic differentiation ' , Geochimica et Cosmochimica Acta , vol. 356 , pp. 116-128 . https://doi.org/10.1016/j.gca.2023.07.010en
dc.identifier.issn0016-7037
dc.identifier.otherRIS: urn:BD8CBAEE8605ED486A957F8C2FA6C296
dc.identifier.otherORCID: /0000-0001-5276-0229/work/139156745
dc.identifier.otherORCID: /0000-0001-6861-2490/work/139156953
dc.identifier.urihttps://hdl.handle.net/10023/28073
dc.descriptionFunding: UK Natural Environment Research Council (NE/R012253/1, NE/V010824/1, NE/P012167/1).en
dc.description.abstractA significant portion of the continental crust is composed of plutonic igneous rocks. However, little is known about the geochemical behaviour of N between the different minerals during magmatic differentiation. To provide new constraints for the behaviour of N during crust formation, we have characterised the geochemistry of nitrogen (N) in the compositionally zoned calc-alkaline pluton at Loch Doon, SW Scotland. We present N concentration and N isotope values for whole-rock data alongside biotite, plagioclase and K-feldspar mineral separates and assess the degree to which these data preserve equilibrium partitioning during magmatic differentiation. We show that whole rock likely inherited its N contents and δ15N signatures from the initial source composition and that this signature is homogenous at a pluton scale. Whilst the whole-rock data are best explained as crust-derived N in the source, the degree of homogenisation across a pluton scale is inconsistent with empirical N diffusivities, ruling out syn-emplacement crustal assimilation as the source of N. Instead, our data suggest a crustal signature inherited from depth associated with the Iapetus subduction zone. At a mineral scale, we find that N preferentially partitions into the feldspars over mica in this system in the order K-feldspar > plagioclase ≈ biotite > quartz, with average mineral-mineral distribution coefficients of DNplagioclase-biotite = 1.3 ± 0.6 and DNKspar-biotite = 2.8 ± 0.6. Partitioning is accompanied by a large and near constant equilibrium isotope fractionation factor between biotite and both feldspars (averages are Δ15NPlag-Biotite = +7.8 ± 1.2 ‰ and Δ15NKspar-Biotite = +7.9 ± 1.0 ‰), whereas Δ15NKspar-Plagioclase closely approximates 0 ‰, where both minerals show δ15N overlapping with the bulk rock δ15N values. These results show that mica crystallisation generates in a large negative Δ15N resulting a 15N-depleted reservoir within plutonic rocks. Moreover, our dataset suggests that feldspars might be a more significant host of N in the igneous portion of Earth’s continental and oceanic crust than previous thought.
dc.format.extent13
dc.format.extent5173296
dc.language.isoeng
dc.relation.ispartofGeochimica et Cosmochimica Actaen
dc.subjectMagmatic differentiationen
dc.subjectElemental partitioningen
dc.subjectStable isotope fractionationen
dc.subjectNitrogen geochemistryen
dc.subjectQE Geologyen
dc.subjectDASen
dc.subjectMCCen
dc.subject.lccQEen
dc.titleEquilibrium partitioning and isotopic fractionation of nitrogen between biotite, plagioclase, and K-feldspar during magmatic differentiationen
dc.typeJournal articleen
dc.contributor.sponsorNERCen
dc.contributor.sponsorNERCen
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/10.1016/j.gca.2023.07.010
dc.description.statusPeer revieweden
dc.identifier.grantnumberNE/V010824/1en
dc.identifier.grantnumberNE/P012167/1en


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