Geochemical Aspects of Melts: Volatiles and Redox Behavior

Dissolved volatiles can have tremendous effects on the physical and chemical properties of silicate melts. The most abundant volatile in terrestrial magmas is H2O. A few weight percent of added H2O can reduce melting temperatures of rocks by several hundred degrees and enhance the fluidity of magmas by orders of magnitude. Carbon dioxide and sulfur, although less abundant in natural magmas than H2O, often control the initial stage of magma degassing. The strong effect of volatiles on melt properties is related to the chemical bonding of the volatiles in the melt, which depends in particular on melt composition, temperature and oxygen fugacity. The oxygen fugacity, although very low at magmatic conditions, nevertheless has a large influence on the magma, determining the abundance and composition of minerals, fluid–melt partitioning and the physical properties of the melt.

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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.