The Re-Os Revolution: Mighty Messages From Two of Earth’s Rarest Elements

The exceptional power and versatility of the Re-Os radioactive decay system for Earth science stems from the distinctive geochemical behavior of its constituent elements. Here, we first explain how the positions of Re and Os in the periodic table are responsible for their highly siderophile, chalcophile, and organophile properties. We then discuss how these properties dictate the distribution of Re and Os within and at the surface of the Earth and other planetary bodies. Lastly, we describe how the analytical challenges posed by the unusual geochemistry of these elements were overcome with major technological advances, leading to a dramatic decrease in the amount of sample material required for Re-Os isotopic analysis, thereby sparking an explosion of new applications.

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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.