Illuminated Worlds: How Spectroscopy Lights the Way in Earth and Planetary Sciences

The study of minerals under light, spanning the ultraviolet, visible, infrared (UV-Vis-IR) spectrum, has played an important role in advancing our understanding of terrestrial and extraterrestrial materials. Here, we review light-based spectroscopic techniques across spatial scales in mineralogy and planetary science. Polarized light microscopy helps characterize optical properties, while vibrational and UV-Vis spectroscopies provide insights into mineral structures and compositions. In mineral physics, spectroscopy probes bonding environments, electronic structure, phase transitions, and elastic properties at high pressures and temperatures. In planetary science, UV-Vis-IR techniques from spacecraft and telescopes reveal planetary mineralogy. These methods support the search for habitable environments, planetary evolution studies, and resource identification. Furthermore, technological advances in portability, imaging, and data analysis have improved the precision and scope of mineralogical 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.