Evolution of diamond resorption in a silicic aqueous fluid at 1–3 GPa: Application to kimberlite emplacement and mantle metasomatism

Abstract

Natural diamonds grow and partially dissolve during mantle metasomatism and undergo further resorption during the ascent to the Earth's surface in kimberlite magmas. This study uses atomic force microscopy (AFM) for quantitative characterization of diamond resorption morphology in order to provide robust constraints of the composition of kimberlitic and mantle metasomatic fluids. We performed experiments in a piston–cylinder apparatus at pressures (P) of 1–3GPa and temperatures (T) of 1150–1400°C to examine the impact of P, T, and silica content of an aqueous fluid on diamond dissolution. Petrographic observation and microthermometry of synthetic fluid inclusions trapped in olivine at the run conditions provide constraints on the composition and density of the fluid reacting with the diamond. Our results confirm an inverse relationship between P and T on diamond dissolution kinetics. A P increase of 1GPa suppresses diamond oxidation rates by the same value as a T decrease by ~50°C, while the transformation rate of diamond crystal morphology from octahedron to tetrahexahedron increases with both P and T. All dissolved diamonds develop glossy surfaces, ditrigonal {111} faces, sheaf striations, and negative trigons, while circular pits only occur in aqueous fluids with low silica content (≤4.2mol/kg) at 1GPa. We identify five distinct morphological groups of trigons: two types of point-bottomed (p/b) (trumpet- and V-shaped) and three types of flat-bottomed (f/b) (trumpet-shaped, trapezoid-shaped and rounded). AFM measurements of trigons from two successive runs showed three stages of their evolution. Etch pits nucleate at defects as trumpet p/b trigons with the vertical dissolution rate (Vd) faster than the dissolution rates at the surface free of defects; they further develop by growth of the bottoms in (111) plane to create trumpet-shaped f/b trigons accompanied by decrease in Vd; and finally form trapezoid-shaped f/b trigon with constant wall angles. The diameter of f/b trigons developed in the aqueous fluids depends on the diamond weight loss and dissolution kinetics, and does not correlate with their depth. Integration of our AFM data with the theoretical model for trigon formation suggests that the change from point- to flat-bottomed trigons depends on the defect sizes and dissolution conditions. Application of our results to the diamonds from Ekati diamond Mine, Canada, suggests that variations in diamond rounding in different pipes implies variable depth of fluid exsolution; presence of circular pits on diamonds indicates predominantly aqueous fluid during the latest stages of kimberlite emplacement; and comparison to the mantle-derived morphologies on Ekati diamonds implies the importance of CO2-rich fluids and/or carbonate melts during mantle metasomatism. The constrained effect of P on diamond dissolution kinetics indicates that appreciable diamond weight loss can only happen at P<1GPa and therefore the conditions at the latest stages of kimberlite emplacement are very important for assessments of diamond preservation in a kimberlite pipe.