Granites and the Nature of the Variscan Crust

The orogenic crust of the European Variscan belt is granite-rich and only locally has a mafic lower layer. The core of the belt originated by massive melting of fertile quartzo–feldspathic sources (felsic meta-sedimentary or meta-igneous) derived from an Ediacaran–Ordovician accretionary system. An unusually felsic lower crust formed either by relamination of previously subducted continental crust or by melting of crustal rocks to produce a granitic upper crust and a laminated, restitic lower crust. This is in strong contrast to conventional models, developed mainly for magmatic arcs, that find or infer mafic lower crustal compositions. Thus, global estimates on the nature and evolution of the continental crust should consider the heterogeneity of the deep crust produced in various types of orogenies.

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December 2025 --The Variscan Orogeny in Europe – Understanding Supercontinent Formation

The Variscan orogen formed between 380 and 300 million years ago through several accretionary and collisional cycles, culminating with the construction of the Pangea supercontinent. This process occurred via sequential opening and closure of oceanic basins, synchronous detachment of Gondwana derived continental ribbons, and their outboard amalgamation onto the Laurussia margin. The Variscan orogen is rather unique compared with other orogenic belts on Earth: its overthickened and dominantly magmatic crust in the central belt, surprisingly minor mantle involvement in the magmatic and geodynamic processes, coherent and pulsed magmatism along the collision suture, and its complex accretionary history. Because its final product, Pangea, is the youngest and best-understood supercontinent on Earth, the Variscan orogeny offers clues for understanding the mechanisms of supercontinent formation.