Onset of slab mantle melting in Earth’s lower mantle: Evidence from ferropericlase in superdeep diamonds

Ferropericlase ([Mg<sub>x</sub>,Fe<sub>1-x</sub>]O), the most common inclusion in sublithospheric diamonds, has a poorly understood crystallization history and depth of origin. Nineteen microscopic ferropericlase grains with different Mg#s were released from Juína and Kankan diamonds with mantle-like carbon, for Mg and Fe isotopic analysis. Two groups of ferropericlase inclusions can be distinguished with respect to diamond growth: high-Mg# inclusions with mantle-like Mg and Fe (δ<sup>26</sup>Mg = -0.23 ± 0.22‰; δ<sup>56</sup>Fe = 0.00 ± 0.14‰) inferred to be preexisting and lower Mg# inclusions with non-mantle-like heavy Fe (δ<sup>56</sup>Fe up to +0.3‰) and light Mg (δ<sup>26</sup>Mg down to -1.4‰) inferred to be coeval. We propose that coeval ferropericlase inclusions formed by melting of hydrated and carbonated peridotitic slab components subducted to lower mantle depths. Continuous reaction of these melts with surrounding reduced, dry slab harzburgite can produce the large range in Mg# and Ni contents of our ferropericlase suite-a heretofore unexplained feature of global ferropericlase data.

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Journal
Science Advances
Published
2025-10-15
DOI
https://doi.org/10.1126/sciadv.adt9106
Primary Topic
High-pressure geophysics and materials
Type
article
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article

Onset of slab mantle melting in Earth’s lower mantle: Evidence from ferropericlase in superdeep diamonds

Steven B. Shirey, D. Graham Pearson, Michael J. Walter, Fabrizio Nestola et al.
Science Advances
High-pressure geophysics and materials
article

Onset of slab mantle melting in Earth’s lower mantle: Evidence from ferropericlase in superdeep diamonds

Steven B. Shirey, D. Graham Pearson, Michael J. Walter, Fabrizio Nestola, A. Steele, Steven D. Jacobsen, Peng Ni, Thomas Stachel, Davide Novella, Janina Czas, Evan M. Smith, Nico Kueter, B. Harte, Anat Shahar, Jeffrey W. Harris, L. R. Gardner
article en

Abstract

Ferropericlase ([Mg<sub>x</sub>,Fe<sub>1-x</sub>]O), the most common inclusion in sublithospheric diamonds, has a poorly understood crystallization history and depth of origin. Nineteen microscopic ferropericlase grains with different Mg#s were released from Juína and Kankan diamonds with mantle-like carbon, for Mg and Fe isotopic analysis. Two groups of ferropericlase inclusions can be distinguished with respect to diamond growth: high-Mg# inclusions with mantle-like Mg and Fe (δ<sup>26</sup>Mg = -0.23 ± 0.22‰; δ<sup>56</sup>Fe = 0.00 ± 0.14‰) inferred to be preexisting and lower Mg# inclusions with non-mantle-like heavy Fe (δ<sup>56</sup>Fe up to +0.3‰) and light Mg (δ<sup>26</sup>Mg down to -1.4‰) inferred to be coeval. We propose that coeval ferropericlase inclusions formed by melting of hydrated and carbonated peridotitic slab components subducted to lower mantle depths. Continuous reaction of these melts with surrounding reduced, dry slab harzburgite can produce the large range in Mg# and Ni contents of our ferropericlase suite-a heretofore unexplained feature of global ferropericlase data.

Science AdvancesVol. 11(42)
Northwestern University (US), Planetary Science Institute (US), University of Padua (IT), University of Alberta (CA), University of California, Los Angeles (US), Carnegie Institution for Science (US), Gemological Institute of America (US), ETH Zurich (CH), University of Glasgow (GB), University of Edinburgh (GB)
Openalex Percentile: Top 70%
High-pressure geophysics and materials
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