Constructing the Pressure–Temperature Path of Ultrahigh-Pressure Rocks

Coesite and diamond in metamorphic rocks point to their very deep burial, but these minerals do not allow a precise derivation of metamorphic pressure–temperature (P–T) conditions at ultrahigh pressure (UHP). Thermodynamic calculations of mineral equilibria can accomplish this task when it is possible to assign mineral compositions to a former UHP equilibrium state. Pressure–temperature pseudosections are superior, because they often permit the construction of P–T paths to and from UHP conditions only on the basis of chemically zoned minerals such as garnet and phengite. The examples of a metapelite from Oman and an eclogite from the Erzgebirge, Germany, illustrate this method, but also demonstrate its limits. The derived paths are the basis for further geodynamic modeling and insight into tectonic processes.

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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.