A Stochastic Treatment of Crystal Dissolution Kinetics

Many areas of science and industry require a fundamental understanding of crystal dissolution. Examples are diverse and include chemical weathering, pharmaceutical delivery, and the response of marine carbonates to CO2 increases. Understanding these processes ultimately demands knowledge of reaction dynamics. Techniques allowing high-resolution observations of dissolving crystals have greatly improved our understanding of reaction kinetics at a variety of scales. Atomic force microscopy and vertical scanning interferometry can reveal reaction mechanisms and permit tests of working hypotheses. However, understanding the substantial complexity and heterogeneous distribution of surface reactivity cannot be made by simple observation alone but requires advances in fundamental theory. Model simulations of molecular-scale processes provide the critical link between nanoscale surface observations of crystal dissolution and the phenomenological result at scales of environmental importance.

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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.