Primary tin (Sn) deposits are commonly associated with highly fractionated, reduced granites derived from melting of evolved crustal rocks. While extreme fractionation is necessary to generate Sn-granites from low-Sn siliciclastic sediments (~5–10 ppm Sn), melting of Sn-enriched source rocks can yield Sn-rich magmas with minimal fractionation. We present an example of Sn-rich mica schists from the Bockau area, Western Erzgebirge that underwent metamorphic Sn enrichment prior to post-orogenic Sn-granite intrusion[2]. Strata-bound Sn mineralization in the schists average 50–200 µg/g, with local concentrations up to 1 wt%. Microfabric analysis shows that Sn mobilization was linked to progressive deformation. Tin occurs in prograde minerals—biotite and garnet—as structurally bound Sn and as cassiterite (SnO₂) inclusions. A second phase of Sn mobilization is represented as secondary cassiterite inclusions during the retrogression of biotite to chlorite. Comparative whole-rock geochemical analysis of the protoliths[1], Sn-rich non-retrogressed, and retrogressed schists reveal continuous Si addition throughout metamorphism and significant Fe and Sn enrichment during prograde metamorphism, accompanied by depletion of K, Rb, Ba and a relative decrease in the immobile elements, Al, Ti and Zr. Additionally, Li, B concentrations increased during the prograde and retrograde stages, respectively.
[1] Romer, R.L., and Hahne, K., 2010. Life of the Rheic Ocean: Scrolling through the shale record. Gondwana Research, 17(2-3), pp. 236–253
[2] Romer, R.L., Kroner, U., Schmidt, C., and Legler, C., 2022. Mobilization of tin during continental subduction-accretion processes. Geology, 50(12), pp. 1361–1365.