The Role of LA–ICP–MS in Palaeoclimate Research

Past environmental parameters such as temperature, pH and CO2 can be reconstructed from chemical ‘proxies’ (elemental and isotopic compositions) stored in various ‘archives’ such as corals, foraminifera and bivalves. Versatile, rapid, simple and comparatively inexpensive microanalysis via laser ablation inductively coupled plasma mass spectrometry (LA–ICP–MS) provides precise and accurate proxy data and chronologies at micrometer resolution. Moreover, LA–ICP–MS can extract data at a high-temporal resolution from continuously growing samples and even works on partially altered samples. The latter enhances our understanding of ‘deep-time’ palaeoclimate events. Using case studies of various carbonate-hosted archives (coralline algae, giant clams) to illustrate multi-proxy mapping (temperature, pH) and chronology, we showcase current methodological practice and achievements. We conclude with an outlook on likely future LA–ICP–MS developments relevant to palaeoclimatology.

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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.