Abiotic Hydrogen and Methane: Fuels for Life

Geologically produced (abiotic) molecular hydrogen and methane could be widely utilized by microbial communities in surface and subsurface environments. These microbial communities can, therefore, have a potentially significant impact on the net emissions of H2 and CH4 to Earth’s ocean and atmosphere. Abiotic H2 and CH4 could enable microbial communities to exist in rock-hosted environments and hydrothermal systems with little or no input from photosynthetic carbon fixation, making these communities potential analogs for the earliest metabolisms on Earth (or other planetary bodies). The possible dependence of rock-hosted ecosystems on H2 and CH4 should factor into current and future plans for engineering the subsurface for storage of these compounds as energy fuels.

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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.