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Highly siderophile element geochemistry of mantle pyroxenites

Fachliche Zuordnung Mineralogie, Petrologie und Geochemie
Förderung Förderung von 2010 bis 2014
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 159831613
 
Erstellungsjahr 2014

Zusammenfassung der Projektergebnisse

The purpose of this study was to evaluate the contribution of mantle pyroxenites to the HSE inventory of the mantle, to constrain the processes of distribution of the HSE during magma-peridotite interaction and to evaluate the impact pyroxenites might have as lithologies in the source regions of plume derived melts. Websterites from the Lanzo and Lherz ultramafic bodies display relatively unfractionated HSE patterns similar to fertile lherzolites. Neither simple sulfid/silicate nor mss/sulfide melt partitioning seem to be able to explain the observed HSE abundances in Lanzo and Lherz pyroxenites. Therefore lowered, more empirical sulfide/silicate HSE partition coefficients under disequilibrium conditions were assumed for the facilitated sulfide/silicate partitioning model. Modelling silicate melt/sulfide melt HSE partitioning in websterites implies a reaction of 20-40% melt (derived by 10% melting of peridotite) with a fertile peridotitic wall rock. In contrast, clinopyroxenites show MORB like HSE compositions with an enrichment of Pt, Pd, Au, Re over Os, Ir, Ru, Rh. Modelling silicate melt/ sulfide melt HSE partitioning resulted in a reaction of 60- 90% partial melt with peridotite. Hence, compared to the websterites, the HSE composition of clinopyroxenites suggests less interaction and contamination of their parent melts with wall rock peridotite. The concentrations of Pd, Au and Re in pyroxenites from Lanzo and Lherz are only rarely higher than in the primitive mantle and peridotites. Thus the significance of mantle pyroxenites for the HSE budget of the mantle may be that they provide localized reservoirs of enhanced Re and radiogenic Os, and therefore complement mantle domains comprised of depleted peridotites. Out of 39 samples only two have the required Pt/Re of 88-100 to make them viable sources for the radiogenic 186-Os-187-Os end member observed in plume related picrites and komatiites. Because of their low volumetric abundance in the mantle (<10%) and the small numbers of pyroxenites displaying the required Pt and Re abundances it appears unlikely that pyroxenites are the cause of the suprachondritic 186-Os-187-Os in plume-related picrites and komatiites. Most sulfides from pyroxenites from Lanzo and Lherz show variable depletions of Pt and Au (at Lanzo also Pd) relative to other HSE, likely reflecting sub- solidus formation of secondary sulfides, Te-Bi phases, alloys and native Au. Some sulfides in pyroxenites have similar HSE ratios as sulfides in peridotites whereas others display a more MORB like HSE signature. Varying Pd/Ir, Re/Os and Ru/Ir in sulfides on the thin section scale reflect entrainment of sulfide melt from peridotite mixed with sulfides from reacted melt. The range of HSE in sulfides indicates multistage melt infiltration and disequilibrium between different populations of sulfides in pyroxenites.

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