Metasomatic ijolite, glimmerite, silicocarbonatite, and antiskarn formation: carbonatite and silicate phase equilibria in the system Na<sub>2</sub>O–CaO–K<sub>2</sub>O–FeO–MgO–Al<sub>2</sub>O<sub>3</sub>–SiO<sub>2</sub>–H<sub>2</sub>O–O<sub>2</sub>–CO<sub>2</sub>

dc.contributor.authorAnenburg, Michaelen
dc.contributor.authorWalters, Jesse B.
dc.date.accessioned2024-06-03T22:28:29Z
dc.date.available2024-06-03T22:28:29Z
dc.date.issued2024
dc.description.abstractSilicocarbonatites are carbonatite rocks containing > 20% silicate minerals. Their formation is not well understood due to low silica solubility in carbonatite melts and negligible amounts of silicate minerals on carbonatite melt cotectics at upper crustal conditions. We explore whether silicocarbonatites can be thought of as antiskarns: rocks formed by leaching of SiO2 from siliceous wall rocks by carbonatite melts, and its deposition as solid silicate minerals by reaction with chemical components already present in the carbonatite melt. Solid state thermodynamic modelling at 1-5 kbar and 500-800 degrees C predicts that calcite-dolomite-magnetite assemblages will transform to dolomite-free silicocarbonatites with an increase in silica contents. In sodic systems, the formation of aegirine and alkali amphiboles suppresses silica activity despite elevated silica contents. Therefore, dolomite remains stable, but Fe3+ is consumed, firstly from magnetite breakdown, and secondly by coupled Fe oxidation and reduction of CO2 to CO, CH4, and graphite, particularly at higher pressures. Despite a net increase in Fe3+/Fe2+, the system evolves to increasingly lower oxygen fugacity. In aluminous systems, nepheline indicates high temperatures whereas alkali feldspars form at lower temperatures. Modelling of potassic systems demonstrates stability of mostly phlogopite-rich biotites, leading to Fe2+ increase in all other carbonate and silicate phases. We find that perthites are expected in high pressures whereas two feldspars are more likely in lower pressures. Aspects of the clinopyroxene natural compositional trend (diopside to hedenbergite to aegirine) of carbonatite systems can be explained by silica contamination. Ferrous clinopyroxenes typically require low alumina and are predicted in potassic or low temperature sodic systems, primarily at mid to high pressures. Silica contamination permits the formation of silicocarbonatite-like assemblages in a way that is not limited by SiO2 solubility in carbonatite melts. Glimmerites and clinopyroxene-rich rocks (such as the ijolite series) that often occur around carbonatite rocks at the contact with silica-oversaturated wall rocks can be explained as the extreme end of silica contamination of carbonatite melts. Therefore, these clinopyroxenites and glimmerites can form solely via metasomatic processes without the presence of a silicate melt.
dc.description.sponsorshipOpen access funding provided by University of Bern. This work was funded by Australian Research Council, LP190100635, Michael Anenburg.
dc.description.statusPeer-revieweden
dc.format.extent25en
dc.identifier.issn0010-7999en
dc.identifier.otherWOS:001198656200001en
dc.identifier.otherORCID:/0000-0001-9880-3087/work/168235250en
dc.identifier.scopus85193918233en
dc.identifier.urihttps://hdl.handle.net/1885/733713050
dc.language.isoenen_AU
dc.rightsPublisher Copyright: © The Author(s) 2024.
dc.sourceContributions to Mineralogy and Petrology
dc.subjectAillikite
dc.subjectAlkaline complexes
dc.subjectAntiskarn
dc.subjectCarbonatite
dc.subjectCarbonatite metasomatism
dc.subjectGlimmerite
dc.subjectPhlogopitite
dc.subjectPyroxenite
dc.titleMetasomatic ijolite, glimmerite, silicocarbonatite, and antiskarn formation: carbonatite and silicate phase equilibria in the system Na<sub>2</sub>O–CaO–K<sub>2</sub>O–FeO–MgO–Al<sub>2</sub>O<sub>3</sub>–SiO<sub>2</sub>–H<sub>2</sub>O–O<sub>2</sub>–CO<sub>2</sub>
dc.typeJournal article
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage25en
local.bibliographicCitation.startpage1
local.contributor.affiliationAnenburg, Michael; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationWalters, Jesse B.; Goethe University Frankfurten
local.identifier.citationvolume179en
local.identifier.doi10.1007/s00410-024-02109-0
local.identifier.pure2981ef7a-d2f7-422d-81bc-a0a689f12588
local.identifier.urlhttps://www.scopus.com/pages/publications/85193918233en
local.type.statusPublisheden

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