Extent and Role of Cratonic Lithosphere in the Variscan Orogeny

Thick and relatively cold cratonic lithosphere of Laurussia and Gondwana shaped the Variscan orogen as those continents collided diachronously to form Pangaea. Herein, we summarize and integrate geological and geophysical results that show how cratonic lithosphere of those composite continents created the Variscan geologic foundation of Europe and northwestern Africa. Our analysis focuses on the lithospheric architecture of Baltica, Avalonia, and Gondwana-derived terranes to distinguish preserved cratonic domains from reworked zones. Zircon provenance analysis further constrains terrane origins and accretion history. The European Variscan belt is distinguished by the large proportion of Gondwana-derived terranes compared with its orogenic core. Its tectonic system reflects inherited rift architecture and the influence of rigid lithospheric promontories, setting it apart from other collisional belts.

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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.