The Upper Mantle and Transition Zone

The upper mantle is the source of almost all magmas. It contains major transitions in rheological and thermal behaviour that control the character of plate tectonics and the style of mantle dynamics. Essential parameters in any model to describe these phenomena are the mantle’s compositional and thermal structure. Most samples of the mantle come from the lithosphere. Although the composition of the underlying asthenospheric mantle can be estimated, this is made difficult by the fact that this part of the mantle partially melts and differentiates before samples ever reach the surface. The composition and conditions in the mantle at depths significantly below the lithosphere must be interpreted from geophysical observations combined with experimental data on mineral and rock properties. Fortunately, the transition zone, which extends from approximately 410 to 660 km, has a number of characteristic globally observed seismic properties that should ultimately place essential constraints on the compositional and thermal state of the mantle.

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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.