Perspective: The Future Exploration of Io

Io is one of the best natural laboratories in the Solar System to study the intertwined processes of tidal heating, extreme volcanism, and atmospheric–magnetosphere–surface interactions. While substantial advances can be made with forthcoming ground- and space-based observatories, many outstanding questions can only be addressed with in situ measurements at Io. Several spacecraft will explore the Jupiter system in the next decade, but their capabilities to investigate Io are limited. A dedicated Io mission is neces- sary to capitalize on Io’s scientific potential. Previous Io mission concepts have spanned the gamut, including small spacecraft, multiple-flyby missions, orbiters, and landers. New technologies, including advanced solar power and radiation hardening, make Io exploration more tractable, and the potential for contemporaneous measurements from multiple spacecraft in the Jupiter system make a modern Io mission all the more compelling.

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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.