Immiscible iron- and silica-rich liquids in the Upper Zone of the Bushveld Complex

dc.contributor.authorFischer, Lennart A.
dc.contributor.authorWang, Meng
dc.contributor.authorCharlier, Bernard
dc.contributor.authorNamur, Olivier
dc.contributor.authorRoberts, R.J. (James)
dc.contributor.authorVeksler, Ilya V.
dc.contributor.authorCawthorn, Grant
dc.contributor.authorHoltz, François
dc.date.accessioned2016-08-08T05:34:15Z
dc.date.issued2016-06
dc.description.abstractThe Bushveld Complex (South Africa) is the largest layered intrusion on Earth and plays a considerable role in our understanding of magmatic differentiation and ore-forming processes. In this study, we present new geochemical data for apatite-hosted multiphase inclusions in gabbroic cumulates from the Bushveld Upper Zone. Inclusions re-homogenized at high temperature (1060-1100°C) display a range of compositions in each rock sample, from iron rich (35 wt.% FeOtot; 28 wt.% SiO2) to silica-rich (5 wt.% FeOtot; 65 wt.% SiO2). This trend is best explained by an immiscible process and trapping of contrasted melts in apatite crystals during progressive cooling along the binodal of a two-liquid field. The coexistence of both Si rich and Fe-rich immiscible melts in single apatite grains is used to discuss the ability of immiscible melts to segregate from each other, and the implications for mineral and bulk cumulate compositions. We argue that complete separation of immiscible liquids did not occur, resulting in crystallization of similar phases from both melts but in different proportions. However, partial segregation in a crystal mush and the production of contrasting phase proportions from the Fe-rich melt and the Si-rich melt can be responsible for the cyclic evolution from melanocratic (Fe-Ti-P-rich) to leucocratic (plagioclase-rich) gabbros which is commonly observed in the Upper Zone of the Bushveld Complex where it occurs at a vertical scale of 50 to 200 m.en_ZA
dc.description.departmentGeologyen_ZA
dc.description.embargo2017-06-30
dc.description.librarianhb2016en_ZA
dc.description.sponsorshipThis project was supported by a DAAD-Doktorandenstipendium for L.A. Fischer. B. Charlier and O. Namur acknowledge support from the Alexander von Humboldt Foundation. I.V. Veksler has been supported by DFG grant VE 619/2-1.en_ZA
dc.description.urihttp://www.elsevier.com/locate/epslen_ZA
dc.identifier.citationFischer, LA, Wang, M, Charlier, B, Namur, O, Roberts, RJ, Veksler, IV, Cawthorn, RG & Holtz, F 2016, 'Immiscible iron- and silica-rich liquids in the Upper Zone of the Bushveld Complex', Earth and Planetary Science Letters, vol. 443, pp. 108-116.en_ZA
dc.identifier.issn0012-821X
dc.identifier.other10.1016/j.epsl.2016.03.016
dc.identifier.urihttp://hdl.handle.net/2263/56236
dc.language.isoenen_ZA
dc.publisherElsevieren_ZA
dc.rights© 2016 Elsevier B.V. All rights reserved. Notice : this is the author’s version of a work that was accepted for publication in Earth and Planetary Science Letters. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to This article since it was submitted for publication. A definitive version was subsequently published in Earth and Planetary Science Letters, vol. 433, pp. 108-116, 2016. doi : 10.1016/j.epsl.2016.03.016.en_ZA
dc.subjectLayered intrusionen_ZA
dc.subjectMelt inclusionen_ZA
dc.subjectApatiteen_ZA
dc.subjectGabbroen_ZA
dc.subjectImmiscibilityen_ZA
dc.subjectBushvelden_ZA
dc.titleImmiscible iron- and silica-rich liquids in the Upper Zone of the Bushveld Complexen_ZA
dc.typePostprint Articleen_ZA

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