It’s Not Just a Phase: Over 50 Years of Lunar Sample Science

Landed robots, rovers, and orbital spacecraft provide regional-scale information about the nature of the Moon’s surface, but such data require ground truth information made accessible through lunar samples. Such samples include a range of material including hand-specimen-sized rocks, pieces of rocks chipped from boulders by astronauts wielding geologic hammers, to soil—scooped, trenched, and drilled from the upper few meters of the Moon’s surface by robots as well as humans. This chapter provides an overview of recent discoveries made using the lunar sample collection, highlights outstanding questions about the Moon’s origin and evolution, and discusses how these knowledge gaps will be addressed by future sample return missions.

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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.