1. The chromitites of the Herbeira massif (Cabo Ortegal Complex, Spain) revisited
- Author
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Universidad Nacional Autónoma de México, Universidad de Barcelona, Agència de Gestió d'Ajuts Universitaris i de Recerca, Luleå University of Technology, Consejo Nacional de Humanidades, Ciencias y Tecnologías (México), Ministerio de Economía y Competitividad (España), García-Tudela, Matías, Proenza, Joaquín A., Farré-de-Pablo, Júlia, Pujol-Solà, Núria, Aiglsperger, Thomas, Castillo-Oliver, Montgarri, Colás, Vanessa, Arenas, Ricardo, Garcia-Casco, Antonio, Universidad Nacional Autónoma de México, Universidad de Barcelona, Agència de Gestió d'Ajuts Universitaris i de Recerca, Luleå University of Technology, Consejo Nacional de Humanidades, Ciencias y Tecnologías (México), Ministerio de Economía y Competitividad (España), García-Tudela, Matías, Proenza, Joaquín A., Farré-de-Pablo, Júlia, Pujol-Solà, Núria, Aiglsperger, Thomas, Castillo-Oliver, Montgarri, Colás, Vanessa, Arenas, Ricardo, and Garcia-Casco, Antonio
- Abstract
The ultramafic rocks of the Herbeira Massif in the Cabo Ortegal Complex (NW Iberia) host chromitite bodies. The textural and compositional study of the host rocks and the chromitites classified them into: (1) Type-I chromitites, forming massive pods of intermediate-Cr chromite (Cr# = 0.60–0.66) within dunites; and (2) Type-II chromitites forming semi-massive horizons of high-Cr chromite (Cr# = 0.75–0.82) interlayered with dunites and pyroxenites. Minor and trace elements (Ga, Ti, Ni, Zn, Co, Mn, V and Sc) contents in the unaltered chromite cores from both types show patterns very similar to fore-arc chromitites, mimicked by the host dunites and pyroxenites. Calculated parental melt compositions suggest that Type-I chromitites crystallized from a melt akin to fore-arc basalt (FAB), while Type-II chromitites originated from a boninite-like parental melt. Both melts are characteristic of a fore-arc setting affected by extension during rollback subduction and have been related to the development of a Cambrian-Ordovician arc. These chromitites are extremely enriched in platinum-group elements (PGE), with bulk-rock PGE contents between 2,460 and 3,600 ppb. Also, the host dunites and pyroxenites exhibit high PGE contents (167 and 324 ppb, respectively), which are higher than those from the primitive mantle and global ophiolitic mantle peridotites. The PGE enrichment is expressed in positively-sloped chondrite-normalized PGE patterns, characterized by an enrichment in Pd-group PGE (PPGE: Rh, Pt and Pd) over the Ir-group PGE (IPGE: Os, Ir and Ru) and abundant platinum-group minerals (PGM) dominated by Rh-Pt-Pd phases (i.e. Rh-Ir-Pt-bearing arsenides and sulfarsenides, Pt-Ir-Pd-base-metal-bearing alloys, and Pt-Pd-bearing sulfides). The PGM assemblage is associated with base-metal sulfides (mostly pentlandite and chalcopyrite) and occurs at the edges of chromite or embedded within the interstitial (serpentinized) silicate groundmass. Their origin has been linked to direct cry
- Published
- 2024