How Well Do We Understand the Geological Carbon Cycle?

The foundation of our understanding of the geological carbon cycle, and how this acts as Earth’s “thermostat,” was articulated in a seminal paper in 1981 (Walker et al). They suggested that silicate weathering on the continents acts as a stabilizing feedback on the carbon cycle such that increased atmospheric pCO2 leads to increased weathering rates and hence increased removal of CO from the atmosphere. This “textbook model” is at the core 2 of most models of long-term biogeochemical cycles. We summarize evidence that there are many other processes in the geological carbon cycle that may be equally or more important than those in the Walker model. We argue there is a need to move beyond the textbook model in both teaching and research.

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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.