Canham, Kate R;
              
      
            
                Holwell, David A;
              
      
            
                Du Preez, Lara;
              
      
            
                Nex, Paul AM;
              
      
            
                Wilson, Allan H;
              
      
            
                McFall, Katie;
              
      
            
                Thompson, Erin S;
              
      
            
            
          
      
            
            
            ... Lloyd, Andy; + view all
            
          
      
        
        
        
    
  
(2025)
  Enigmatic High-Tenor Rh-, Ru-, Ir-, and Os-Rich Base Metal Sulfide Mineralization Within the Northern Limb of the Bushveld Complex: A Product of Fractionation of a Sulfide Liquid?
Economic Geology
, 120
       (4)
    
     pp. 997-1023.
    
         10.5382/econgeo.5159.
  
  
       
    
  
| Preview | Text Canhametal_2025-deepPlatreefBMZone.pdf - Accepted Version Download (8MB) | Preview | 
Abstract
The Base Metal zone at Sandsloot in the Northern limb of the Bushveld Complex, South Africa, is a highly unusual and high-grade Os-Ir-Ru-Rh, Fe-Ni sulfide-rich horizon hosted within the deep Platreef, below the main platinum group element (PGE) horizon. The Base Metal zone ranges from 5 to 100 meters in thickness and is located up to 150 meters beneath the PGE reef. Base metal sulfide mineralization occurs as disseminated/blebby to semimassive/massive sulfides, with a typical assemblage of ~60/25/15 pyrrhotite/pentlandite/chalcopyrite modal %. The Base Metal zone is characterized by high (Os + Ir + Ru + Rh)/(Pt + Pd) ratios that reflect monosulfide solid solution, primitive mantle-normalized PGE profiles. The PGM assemblage is dominated by laurite (RuS2) (62% by area) and iridium-group platinum group element (IPGE) + Pt arsenosulfides (21% by area). The PGE tenors of the sulfides vary between different textural styles, either reflecting R-factor variations or dilution of tenors by addition of crustal S. Disseminated/blebby sulfides have the highest tenors (up to 153 ppm Pd, 249 ppm Rh, 818 ppm Ru), whereas semimassive/massive sulfides have lower tenors (up to 2.8 ppm Pd, 1.8 ppm Pt, 11 ppm Rh, 17 ppm Ru, 2.2 ppm Os, 3.5 ppm Ir). The PGE geochemistry, IPGE-dominant platinum group metal (PGM) assemblage, abundance of Fe sulfides, and high Ni/Cu ratios are consistent with the Base Metal zone representing the monsulfide solid solution portion of a sulfide liquid formed by fractional crystallization. Furthermore, the Cu + Pt + Pd + Au-poor nature of the Base Metal zone suggests that these metals were removed from the Base Metal zone, and some Cu-rich veins and sections are present around the margins of Ni-Fe sulfide to support this. Increasing Pd/Ir and decreasing Rh/Cu ratios downhole indicate the sulfide liquid fractionated downward. Therefore, a residual Cu-rich liquid, with associated Pt + Pd + Au, likely separated from monosulfide solid solution and was mobilized downward and away from the Base Metal zone. Significantly, the mobilization of a Cu-rich liquid leaves the possibility that an undiscovered Cu + Pt + Pd + Au orebody may exist at depth.
| Type: | Article | 
|---|---|
| Title: | Enigmatic High-Tenor Rh-, Ru-, Ir-, and Os-Rich Base Metal Sulfide Mineralization Within the Northern Limb of the Bushveld Complex: A Product of Fractionation of a Sulfide Liquid? | 
| Open access status: | An open access version is available from UCL Discovery | 
| DOI: | 10.5382/econgeo.5159 | 
| Publisher version: | https://doi.org/10.5382/econgeo.5159 | 
| Language: | English | 
| Additional information: | For the purposes of open access, the author has applied a creative commons attribution (CC BY) licence to any Author Accepted Manuscript version arising from this submission. | 
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Earth Sciences | 
| URI: | https://discovery.ucl.ac.uk/id/eprint/10212498 | 
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