Subducted ophicarbonates as source for B-bearing diamond formation

This study presents in-situ B isotope compositions (δ 11 B) of antigorite from well-characterized ophicarbonates that underwent prograde to high-pressure (high- P ) metamorphic evolution during the Alpine orogeny (300–500 °C and 0.6–2.3 GPa). The δ 11 B values in antigorite are highly variable, ranging from ca. -8 to +7 ‰. Coupled with in-situ 87 Sr/ 86 Sr ratios of carbonates (ranging from 0.7065 to 0.7085), this B isotope variability may reflect either inherited oceanic imprints or re-equilibration with metamorphic fluids during subduction processes. These interpretations are further corroborated by in-situ REE and incompatible trace element data on antigorite. The devolatilization and densification of slab lithologies during subduction drive the recycling of slab and wedge materials into the Earth's mantle, contributing to its chemical heterogeneity. Remarkably, the δ 11 B signatures of antigorite reported here overlap with the variability observed in B-bearing diamonds formed at transition zone/lower mantle depths, as well as in carbonatites and ocean island basalts (OIBs), suggesting a geochemical connection. Together with literature data, this study proposes that deeply subducted ophicarbonates may transform into carbonate-bearing secondary peridotites with geochemical features compatible with B-bearing diamonds. Deeply subducted ophicarbonates, with enriched trace element and isotopic signatures, may also act as reservoirs influencing mantle dynamics and the geochemical diversity of OIB and carbonatite mantle sources. These findings provide new constraints into the recycling of B and volatiles at convergent margins, extending to depths compatible with the lower mantle region. • In-situ δ 11 B data for antigorite in high-P ophicarbonates from the W. Alps. • In-situ Sr isotope support δ 11 B records of both oceanic and subduction processes. • Subduction of ophicarbonates impacts deep B C cycles. • Deeply subducted ophicarbonates may represent a source for B-bearing diamonds. • Deeply subducted ophicarbonates may represent a source for OIBs and carbonatites.

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Publication Details

Journal
Chemical Geology
Published
2025-02-18
DOI
https://doi.org/10.1016/j.chemgeo.2025.122693
Citations
2
Primary Topic
High-pressure geophysics and materials
Type
article
Field-Weighted Citation Impact
3.73

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article

Subducted ophicarbonates as source for B-bearing diamond formation

Enrico Cannaò
2 citations
Chemical Geology
High-pressure geophysics and materials
3.73
article

Subducted ophicarbonates as source for B-bearing diamond formation

Enrico Cannaò
article en
2 citations

Abstract

This study presents in-situ B isotope compositions (δ 11 B) of antigorite from well-characterized ophicarbonates that underwent prograde to high-pressure (high- P ) metamorphic evolution during the Alpine orogeny (300–500 °C and 0.6–2.3 GPa). The δ 11 B values in antigorite are highly variable, ranging from ca. -8 to +7 ‰. Coupled with in-situ 87 Sr/ 86 Sr ratios of carbonates (ranging from 0.7065 to 0.7085), this B isotope variability may reflect either inherited oceanic imprints or re-equilibration with metamorphic fluids during subduction processes. These interpretations are further corroborated by in-situ REE and incompatible trace element data on antigorite. The devolatilization and densification of slab lithologies during subduction drive the recycling of slab and wedge materials into the Earth's mantle, contributing to its chemical heterogeneity. Remarkably, the δ 11 B signatures of antigorite reported here overlap with the variability observed in B-bearing diamonds formed at transition zone/lower mantle depths, as well as in carbonatites and ocean island basalts (OIBs), suggesting a geochemical connection. Together with literature data, this study proposes that deeply subducted ophicarbonates may transform into carbonate-bearing secondary peridotites with geochemical features compatible with B-bearing diamonds. Deeply subducted ophicarbonates, with enriched trace element and isotopic signatures, may also act as reservoirs influencing mantle dynamics and the geochemical diversity of OIB and carbonatite mantle sources. These findings provide new constraints into the recycling of B and volatiles at convergent margins, extending to depths compatible with the lower mantle region. • In-situ δ 11 B data for antigorite in high-P ophicarbonates from the W. Alps. • In-situ Sr isotope support δ 11 B records of both oceanic and subduction processes. • Subduction of ophicarbonates impacts deep B C cycles. • Deeply subducted ophicarbonates may represent a source for B-bearing diamonds. • Deeply subducted ophicarbonates may represent a source for OIBs and carbonatites.

Chemical GeologyVol. 680
University of Milan (IT)
Dipartimenti di Eccellenza
Openalex Percentile: Top 10%
High-pressure geophysics and materials
3.73
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