Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton

Abstract We present the first oxygen fugacity (fO2) profile through the cratonic lithospheric mantle under the Panda kimberlite (Ekati Diamond Mine) in the Lac de Gras kimberlite field, central Slave Craton, northern Canada. Combining this data with new and existing data from garnet peridotite xenol...

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Main Authors: G. M. Yaxley, A. J. Berry, A. Rosenthal, A. B. Woodland, D. Paterson
Format: Article
Language:English
Published: Nature Publishing Group 2017-02-01
Series:Scientific Reports
Online Access:https://doi.org/10.1038/s41598-017-00049-3
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spelling doaj-90da4f90624142189a71c5e3203c944c2020-12-08T02:43:32ZengNature Publishing GroupScientific Reports2045-23222017-02-017111010.1038/s41598-017-00049-3Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave CratonG. M. Yaxley0A. J. Berry1A. Rosenthal2A. B. Woodland3D. Paterson4Research School of Earth Sciences, The Australian National UniversityResearch School of Earth Sciences, The Australian National UniversityBayerisches Geoinstitut, Universität BayreuthInstitut für Geowissenschaften, Goethe UniversitätAustralian SynchrotronAbstract We present the first oxygen fugacity (fO2) profile through the cratonic lithospheric mantle under the Panda kimberlite (Ekati Diamond Mine) in the Lac de Gras kimberlite field, central Slave Craton, northern Canada. Combining this data with new and existing data from garnet peridotite xenoliths from an almost coeval kimberlite (A154-N) at the nearby Diavik Diamond Mine demonstrates that the oxygen fugacity of the Slave cratonic mantle varies by several orders of magnitude as a function of depth and over short lateral distances. The lower part of the diamond-bearing Slave lithosphere (>120–130 km deep) has been oxidized by up to 4 log units in fO2, and this is clearly linked to metasomatic enrichment. Such coupled enrichment and oxidation was likely caused by infiltrating carbonate-bearing, hydrous, silicate melts in the presence of diamond, a process proposed to be critical for “pre-conditioning” deep lithospheric mantle and rendering it suitable for later generation of kimberlites and other SiO2-undersaturated magmas.https://doi.org/10.1038/s41598-017-00049-3
collection DOAJ
language English
format Article
sources DOAJ
author G. M. Yaxley
A. J. Berry
A. Rosenthal
A. B. Woodland
D. Paterson
spellingShingle G. M. Yaxley
A. J. Berry
A. Rosenthal
A. B. Woodland
D. Paterson
Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
Scientific Reports
author_facet G. M. Yaxley
A. J. Berry
A. Rosenthal
A. B. Woodland
D. Paterson
author_sort G. M. Yaxley
title Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
title_short Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
title_full Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
title_fullStr Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
title_full_unstemmed Redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central Slave Craton
title_sort redox preconditioning deep cratonic lithosphere for kimberlite genesis – evidence from the central slave craton
publisher Nature Publishing Group
series Scientific Reports
issn 2045-2322
publishDate 2017-02-01
description Abstract We present the first oxygen fugacity (fO2) profile through the cratonic lithospheric mantle under the Panda kimberlite (Ekati Diamond Mine) in the Lac de Gras kimberlite field, central Slave Craton, northern Canada. Combining this data with new and existing data from garnet peridotite xenoliths from an almost coeval kimberlite (A154-N) at the nearby Diavik Diamond Mine demonstrates that the oxygen fugacity of the Slave cratonic mantle varies by several orders of magnitude as a function of depth and over short lateral distances. The lower part of the diamond-bearing Slave lithosphere (>120–130 km deep) has been oxidized by up to 4 log units in fO2, and this is clearly linked to metasomatic enrichment. Such coupled enrichment and oxidation was likely caused by infiltrating carbonate-bearing, hydrous, silicate melts in the presence of diamond, a process proposed to be critical for “pre-conditioning” deep lithospheric mantle and rendering it suitable for later generation of kimberlites and other SiO2-undersaturated magmas.
url https://doi.org/10.1038/s41598-017-00049-3
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