The importance of carbon to the formation and composition of silicates during mantle metasomatism

Michele Rinaldi*, Sami Mikhail, Dimitri A. Sverjensky, Joanna Kalita

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)
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Abstract

Mineral and fluid inclusions in mantle diamonds provide otherwise inaccessible information concerning the nature of mantle metasomatism and the role of fluids in the mass transfer of material through the Earth’s interior. We explore the role of the carbon concentrations during fluid-rock metasomatism in generating the ranges of garnet and clinopyroxene compositions observed in diamonds from the sub-continental lithospheric mantle. We use the Deep Earth Water model to predict the results of metasomatism between silicic, carbonatitic and peridotitic fluids with common mantle rocks (peridotites, eclogites and pyroxenites) at 5 GPa, 1000 °C, across a range of redox conditions (logfO2 = -2 to -4 ΔFMQ), and a wide range of initial carbon concentrations in the metasomatic fluids. Our results show that the predicted compositions of metasomatic garnets and clinopyroxenes are controlled by the initial geochemistry of the fluids and the rocks, with subsequent mineral-specific geochemical evolution following definable reaction pathways. Model carbon-rich, metasomatic fluids that can form diamond (initial C- content > 5.00 molality) result in Mg-rich garnets and clinopyroxenes typical of peridotitic, eclogitic, and websteritic inclusions in diamonds. However, model carbon-poor, metasomatic fluids that do not form diamond can result in Mg-poor, Ca-rich garnets and clinopyroxenes. Such garnets and clinopyroxenes can nevertheless occur as inclusions in diamonds. In our models, the abundance of carbon in the fluids controls the behaviour of the bivalent ions through the formation of aqueous Mg-Ca-Fe-C complexes which directly govern the composition of garnets and clinopyroxenes precipitated during the metasomatic processes. As the C-rich initial fluids can form the higher Mg-eclogitic, peridotitic, and websteritic inclusions in diamonds, these inclusions can be syngenetic (metasomatic) or possibly protogenetic. However, in our models, the relatively Mg-poor, Ca- and Fe-rich eclogitic garnet and clinopyroxene inclusions found in mantle diamonds formed from C-poor fluids that do not form diamonds. These inclusions most likely reflect a metasomatic event prior to being incorporated into their host diamonds, or they could represent protolith-based protogenetic geochemistry. Therefore, the paragenetic groups used to classify diamonds should not be considered a genetic classification, as the role of the fluid geochemistry appears to be more important than the one played by host rock geochemistry.
Original languageEnglish
Pages (from-to)105-115
Number of pages11
JournalGeochimica et Cosmochimica Acta
Volume356
Early online date24 Jul 2023
DOIs
Publication statusPublished - 1 Sept 2023

Keywords

  • Diamond inclusions
  • Fluid-rock metasomatism
  • Thermodynamic modelling

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