Sn and W mineralisation in the Iberian Peninsula

• Sn-W mineralisation in Iberia is preferentially linked to S 1 and S 2 granitic suites. • Metal enrichment of magmas likely due to source inheritance plus magmatic processes. • Structural controls are pivotal for water-rich ore-related granitic magma emplacement. • Sn and W mineralisation is decoupled during magmatic and hydrothermal processes. This paper provides a comprehensive review and a refined classification of Sn-W mineralisation in the Iberian Peninsula, based on an extensive review of the available literature. The study synthesises and clarifies previously published information to improve the understanding of the mineralisation processes and their tectonic and magmatic controls. The Sn and W mineralisation in the Iberian Peninsula exhibit a strong correlation with specific granitic suites primarily formed during the late to post-Variscan orogeny. Structural controls, particularly syn- to late-D 3 strike-slip and/or extensional structures developed during the tectonic regime of the late Variscan, appear to be pivotal to facilitate the emplacement of this water-rich granitic magmas, that otherwise would have stalled at deeper environments, and the development of extensive hydrothermal systems. Two main mineralisation styles are identified: Sn-(Nb-Ta-Li) mineralisation under lithostatic pressure conditions, characterised by disseminated cassiterite in some pegmatites and altered granitic cupolas; and Sn-(Nb-Ta-Li) and W-(Sn) deposits formed at shallower levels within the brittle regime. The Sn-(Nb-Ta-Li) mineralisation is primarily associated with S-type granitic intrusions, while the W-(Sn) mineralisation also tends to be linked to these granitic suites, although several W-rich but Sn-poor deposits appear related to I-type granitoids. The metal enrichment in these magmas is likely due to a combination of inheritance from the source of the protoliths and magmatic evolution processes. The observed decoupling between Sn-rich and W-poor deposits versus W-(Sn)-rich deposits suggests contrasting behaviours of W and Sn during magmatic transport, the magmatic-hydrothermal transition, and the subsequent hydrothermal transport and deposition. Both types of deposits likely represent different settings and/or stages within a single magmatic-hydrothermal system.

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Publication Details

Journal
Ore Geology Reviews
Published
2025-03-06
DOI
https://doi.org/10.1016/j.oregeorev.2025.106542
Citations
4
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
7.47
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article

Sn and W mineralisation in the Iberian Peninsula

José M. Castelo Branco, Fernando Tornos, Emma Losantos, Iñigo Borrajo et al.
4 citations
Ore Geology Reviews
Geological and Geochemical Analysis
7.47
article

Sn and W mineralisation in the Iberian Peninsula

José M. Castelo Branco, Fernando Tornos, Emma Losantos, Iñigo Borrajo, Lluís Boixet, Iván Losada
article en
4 citations

Abstract

• Sn-W mineralisation in Iberia is preferentially linked to S 1 and S 2 granitic suites. • Metal enrichment of magmas likely due to source inheritance plus magmatic processes. • Structural controls are pivotal for water-rich ore-related granitic magma emplacement. • Sn and W mineralisation is decoupled during magmatic and hydrothermal processes. This paper provides a comprehensive review and a refined classification of Sn-W mineralisation in the Iberian Peninsula, based on an extensive review of the available literature. The study synthesises and clarifies previously published information to improve the understanding of the mineralisation processes and their tectonic and magmatic controls. The Sn and W mineralisation in the Iberian Peninsula exhibit a strong correlation with specific granitic suites primarily formed during the late to post-Variscan orogeny. Structural controls, particularly syn- to late-D 3 strike-slip and/or extensional structures developed during the tectonic regime of the late Variscan, appear to be pivotal to facilitate the emplacement of this water-rich granitic magmas, that otherwise would have stalled at deeper environments, and the development of extensive hydrothermal systems. Two main mineralisation styles are identified: Sn-(Nb-Ta-Li) mineralisation under lithostatic pressure conditions, characterised by disseminated cassiterite in some pegmatites and altered granitic cupolas; and Sn-(Nb-Ta-Li) and W-(Sn) deposits formed at shallower levels within the brittle regime. The Sn-(Nb-Ta-Li) mineralisation is primarily associated with S-type granitic intrusions, while the W-(Sn) mineralisation also tends to be linked to these granitic suites, although several W-rich but Sn-poor deposits appear related to I-type granitoids. The metal enrichment in these magmas is likely due to a combination of inheritance from the source of the protoliths and magmatic evolution processes. The observed decoupling between Sn-rich and W-poor deposits versus W-(Sn)-rich deposits suggests contrasting behaviours of W and Sn during magmatic transport, the magmatic-hydrothermal transition, and the subsequent hydrothermal transport and deposition. Both types of deposits likely represent different settings and/or stages within a single magmatic-hydrothermal system.

Ore Geology ReviewsVol. 179
Universidad de Salamanca (ES), Centro de Genética Clínica (PT), Instituto de Geociencias (ES), Universidade de Vigo (ES)
Climate action
Openalex Percentile: Top 3%
Geological and Geochemical Analysis
7.47
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