How Minerals Grow: From Monomer-By-Monomer to Particle-Mediated Pathways

Once nucleation is established, mineral growth is the process by which crystals increase in size, either through the addition of individual ions (monomers) or the attachment of more complex species that range from oligomers to nanoparticles. The relative contribution of these two mechanisms, which may occur separately or simultaneously, varies with fluid properties such as supersaturation as well as crystallographic characteristics wherein nonclassical mechanisms involving particle attachment are often more prevalent at early stages of crystallization and classical growth by monomers is dominant at later stages. However, there is no general rule for the type of crystal growth dominating in any given scenario as the interaction of aqueous fluid properties, together with kinetic and thermodynamic factors, will determine the pathway for growth. Ultimately the growth pathway(s) of minerals determines properties such as crystal habit and defect density. The environments where mineralization occurs are as diverse as the materials themselves and require state-of-the-art techniques to probe the details of their formation. Here, we review the current understanding of pathways by which mineral growth occurs in geological, biological, and synthetic 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.