Meteorite Impacts as Triggers to Large Igneous Provinces

Ameteorite impacting on the surface of the Earth produces not only a crater but also, if the impactor is sufficiently large, high melt volumes. Computer simulations suggest that, in addition to shock- induced melting produced by impact, additional decompression melting of the hot target mantle beneath the crater can produce melt volumes comparable to those found in large igneous provinces (LIPs). The coincidence between the expected frequency of such impact events combined with the similarity in magma volumes of LIPs suggests that large meteorite impacts may be capable of triggering LIPs and mantle hotspots from a point source which is subsequently buried. Can the impact model explain any LIP? What are the distinctive macroscopic criteria predicted from an impact model, and how may they be recognised or rejected in the geological record of the Earth?

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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.