Nanoscale variations in 187Os isotopic composition and HSE systematics in a Bultfontein peridotite

• Published in: Earth and planetary science letters 2016-08, Vol.447, p.60-71
• Main Authors: Wainwright, A.N., Luguet, A., Schreiber, A., Fonseca, R.O.C., Nowell, G.M., Lorand, J.-P., Wirth, R., Janney, P.E.
• Format: Article
• Language: English
• Subjects: Age; base metal sulphides; Depletion; Formations; highly siderophile elements; Inclusions; Melting; osmium isotopes; Peridotite; Platinum; Platinum base alloys; Pt–Fe-alloy; Sulfides
• ISSN: 0012-821X; 1385-013X
• DOI: 10.1016/j.epsl.2016.04.034

Understanding the mineralogical controls on radiogenic chronometers is a fundamental aspect of all geochronological tools. As with other common dating tools, it has become increasingly clear that the Re–Os system can be impacted by multiple mineral formation events. The accessory and micrometric nature of the Re–Os-bearing minerals has made assessing this influence complex. This is especially evident in cratonic peridotites, where long residence times and multiple metasomatic events have created a complex melting and re-enrichment history. Here we investigate a harzburgitic peridotite from the Bultfontein kimberlite (South Africa) which contains sub-micron Pt–Fe-alloy inclusions within base metal sulphides (BMS). Through the combination of the focused ion beam lift-out technique and low blank mass spectrometry we were able to remove and analyse the Pt–Fe-alloy inclusions for their Re–Os composition and highly siderophile element (HSE) systematics. Six repeats of the whole-rock yield 187Os/188Os compositions of 0.10893–0.10965, which correspond to Re depletion model ages (TRD) of 2.69–2.79 Ga. The Os, Ir and Pt concentrations are slightly variable across the different digestions, whilst Pd and Re remain constant. The resulting HSE pattern is typical of cratonic peridotites displaying depleted Pt and Pd. The Pt–Fe-alloys have PUM-like 187Os/188Os compositions of 0.1294±24 (2-s.d.) and 0.1342±38, and exhibit a saw-tooth HSE pattern with enriched Re and Pt. In contrast, their BMS hosts have unradiogenic 187Os/188Os of 0.1084±6 and 0.1066±3, with TRD ages of 2.86 and 3.09 Ga, similar to the whole-rock systematics. The metasomatic origin of the BMS is supported by (i) the highly depleted nature of the mantle peridotite and (ii) their Ni-rich sulphide assemblage. Occurrence of Pt–Fe-alloys as inclusions within BMS grains demonstrates the genetic link between the BMS and Pt–Fe-alloys and argues for formation during a single but continuous event of silicate melt percolation. While the high solubility of HSE within sulphide mattes rules out early formation of the alloys from a S-undersaturated silicate melt and subsequent scavenging in a sulphide matte, the alignment of the Pt–Fe-alloy inclusions attests that they are exsolutions formed during the sub-solidus re-equilibration of the high temperature sulphide phases. The significant difference in 187Os/188Os composition between the included Pt–Fe-alloys and their BMS host can only be accounted for by different Re/Os.