Primordial neon and the deep mantle origin of kimberlites

The genesis of kimberlites is unclear despite the economic and scientific interest surrounding these diamond-bearing magmas. One critical question is whether they tap ancient, deep mantle domains or the shallow convecting mantle with partial melting triggered by plumes or plate tectonics. To address this question, we report the He-Ne-Ar isotopic compositions of magmatic fluids trapped in olivine from kimberlites worldwide. The kimberlites which have been least affected by addition of deeply subducted or metasomatic components have Ne isotopes less nucleogenic than the upper mantle, hence requiring a deep-mantle origin. This is corroborated by previous evidence of small negative W isotope anomalies and kimberlite location along age-progressive hot-spot tracks. The lack of strong primordial He isotope signatures indicates overprinting by lithospheric and crustal components, which suggests that Ne isotopes are more robust tracers of deep-mantle contributions in intraplate continental magmas. The most geochemically depleted kimberlites may preserve deep remnants of early-Earth heterogeneities.

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Publication Details

Journal
Nature Communications
Published
2025-04-05
DOI
https://doi.org/10.1038/s41467-025-58625-5
Citations
4
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
7.47

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article

Primordial neon and the deep mantle origin of kimberlites

Bradley J. Peters, D. Graham Pearson, Mark D. Kurz, Quentin Charbonnier et al.
4 citations
Nature Communications
Geological and Geochemical Analysis
7.47
article

Primordial neon and the deep mantle origin of kimberlites

Bradley J. Peters, D. Graham Pearson, Mark D. Kurz, Quentin Charbonnier, Finlay M. Stuart, Janne M. Koornneef, Andrea Giuliani, Peter H. Barry, Senan Oesch, Joshua Curtice, Kristoffer Szilas
article en
4 citations

Abstract

The genesis of kimberlites is unclear despite the economic and scientific interest surrounding these diamond-bearing magmas. One critical question is whether they tap ancient, deep mantle domains or the shallow convecting mantle with partial melting triggered by plumes or plate tectonics. To address this question, we report the He-Ne-Ar isotopic compositions of magmatic fluids trapped in olivine from kimberlites worldwide. The kimberlites which have been least affected by addition of deeply subducted or metasomatic components have Ne isotopes less nucleogenic than the upper mantle, hence requiring a deep-mantle origin. This is corroborated by previous evidence of small negative W isotope anomalies and kimberlite location along age-progressive hot-spot tracks. The lack of strong primordial He isotope signatures indicates overprinting by lithospheric and crustal components, which suggests that Ne isotopes are more robust tracers of deep-mantle contributions in intraplate continental magmas. The most geochemically depleted kimberlites may preserve deep remnants of early-Earth heterogeneities.

Nature CommunicationsVol. 16(1)
University of Copenhagen (DK), Planetary Science Institute (US), University of Alberta (CA), Carnegie Institution for Science (US), ETH Zurich (CH), Scottish Universities Environmental Research Centre (GB), Woods Hole Oceanographic Institution (US), Vrije Universiteit Amsterdam (NL)
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Life below water
Openalex Percentile: Top 3%
Geological and Geochemical Analysis
7.47
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