Thematic Articles

The Osmium Isotope Perspective on the Dynamics of the Post-Archean Mantle

The 187Re–187Os system offers a unique perspective among the isotopic approaches used to understand planetary evolution because of the chalcophile and siderophile affinities of the parent and daughter elements and their contrasting behaviors during partial melting. Considered the geochronometer of choice to study the Earth’s mantle, from the scale of individual minerals to large-scale outcrops, this system has revealed the survival of Archean and Proterozoic mantle in younger tectonic settings, and has demonstrated local to regional coupling, and sometimes decoupling, between the crust and mantle. Osmium isotopes are also key tracers of melt–peridotite and mantle–crust interactions and recycling processes in subduction zones, and have furthered our understanding of the origin of multi-scale geochemical and isotopic heterogeneities.

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Osmium and Tungsten Isotopes Reveal Earth’s Youthful Exuberance

The siderophile elements, which include Re, Pt, Os, and W, directly constrain the accretionary history of Earth. The largely chondritic 186,187Os/188Os ratios of Earth’s mantle, coupled with excesses in siderophile element abundances, provide nearly incontrovertible evidence that some meteoritic addition continued after core formation was complete. Osmium and W isotope systematics of plume-derived mafic-ultramafic rocks reveal the complex chemical evolution of their deep mantle sources. In the upper mantle, Re-Os dating of whole-rock xenoliths and sulfide inclusions in diamonds hosted by kimberlites indicate both ancient melt depletion and subsequent modification of the mantle lithosphere beneath the earliest continents, with Re-Os ages of eclogitic diamonds possibly recording the transition to a sustained plate tectonic regime on Earth.

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Oil and Water – Intimate Conversations

Re-Os geochronology is a powerful tool for unravelling the complexity of petroleum systems. Because of their organophile nature, Re and Os are enriched in sedimentary organic matter and the hydrocarbons it produces upon heating. Rhenium and Os isotopes are used to date hydrocarbon generation, to fingerprint oils, to distinguish different pulses of oil generation, and to determine interactions between oil, host rock, and formation water. Here we summarize knowledge on the content, distribution, and isotopic composition of Re and Os in petroleum and associated waters, highlight the main technical advances for Re-Os analyses, review experimental studies on water–oil interaction, and discuss the diverse Re-Os applications to petroleum systems.

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Reel-to-Reel Re-Os Records: Earth System Transactions Preserved in Sediments

A unique feature of the Re-Os isotope system is its ability to provide precise and accurate depositional ages from organic-rich sedimentary rocks. Applications include geologic timescale calibration, stratigraphic correlation, and dating key events such as biological innovations, mass extinctions, carbon cycle perturbations, Snowball Earth glaciations, and atmospheric oxygenation. Multiple sediment types reveal temporal variations in the osmium isotope composition of seawater, driven by changes in osmium inputs from continental weathering, seafloor hydrothermal systems, and extraterrestrial material. These variations provide valuable information on climate–tectonic interactions, glacial–interglacial cycles, large igneous province magmatism, bolide impacts, and crustal evolution. Continental processes can be inferred from lake sediment records. These diverse applications highlight the central role of the Re-Os isotope pair in understanding Earth’s evolution.

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Sulfides and Their Little Darling, Molybdenite

Rhenium-osmium geochronology of sulfides and its Os tracer accompaniment have taken their place among geochronometers, although the journey was not without doubters and disparagers. This review highlights several historical hurdles overcome in dating sulfides. The opening act was the debut of molybdenite, which provided an accessible radiometric clock and early insight into the accuracy of the 187Re decay constant. Once controversies surrounding newly minted and game-changing Re-Os molybdenite ages died down, the door flung wide open to begin dating other sulfides, most notably, arsenopyrite and pyrite. Applications sprinted from the ore geology community to constraining the timing of important events, from Earth’s oxygenation to the amalgamation of tectonic terranes. The power of Re-Os sulfide dating in crustal environments was unleashed.

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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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Greenalite: A Template Fit for Life?

Clays have long been implicated in the story of life’s origin. This idea gained support when experiments suggested that tiny crystals of acid-preactivated montmorillonite catalyze the growth of prebiotic polymers. From a geological viewpoint, there are good reasons to consider another clay—greenalite (Fe₃Si₂O₅(OH)₄). Model predictions and observations from ancient sedimentary rocks indicate that nanoparticulate greenalite was a major phase produced during hydrothermal venting in ancient oceans and lakes. Greenalite is an iron-rich, redox-active mineral whose modulated crystal structure provides surfaces with repetitive, parallel grooves of the right size and orientation to align and potentially facilitate the assembly of long, linear biopolymers, thereby addressing a significant challenge for prebiotic chemistry—the synthesis of polymers with genetic and catalytic functions essential for life.

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The Precambrian Greenalite Factory

Over the last decade, high-resolution petrographic examinations of the sedimentary record revealed that greenalite was deposited across several continental margins and throughout many Archean successions. What physical and chemical processes could be responsible for this distribution? Combined sedimentological observations and geochemical results identify and strongly constrain greenalite’s origins in Precambrian sediments, specifically for iron formation deposits. Although greenalite often formed as a pore water or bottom water precipitate, the Precambrian greenalite factory may have resided at the interface between subseafloor hydrothermal vent fluids and anoxic seawater. Once formed, however, greenalite’s stratigraphic distribution was ultimately controlled by its susceptibility to oxidation, a property first recognised by geologists over 120 years ago.

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Greenalite: Cryptic Mineral of Ancient Ferruginous Oceans

The origin of greenalite in iron-rich Precambrian sedimentary rocks, and its significance in tracking Earth’s oxygenation, is the subject of vigorous debate. While known as a common mineral of the ~1.88 Ga granular iron formations (GIFs) of the Lake Superior district, North America, greenalite was poorly documented in ferruginous cherts and banded IFs (BIFs) deposited prior to the Great Oxidation Event (GOE) at ~2.4 Ga. The advent of nanoscale electron microscopy revealed greenalite nanoparticles “hidden in plain sight,” previously overlooked in well-preserved, pre-GOE BIFs and ferruginous cherts due to their minute size. Here, we document the occurrence of primary greenalite in ancient anoxic and ferruginous sediments and its decline from the rock record as Earth’s surface and oceans became oxygenated.

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Serpentine Solid Solutions and Hydrogen Production on Early Earth and Mars

The unusual structural properties of the Fe-Mg serpentine minerals permit significant chemical variability, but the mechanisms and extent of elemental substitution have only recently come to light. New results show that greenalite forms solid solutions with the Fe(III) end-member hisingerite, cronstedtite, and Mg-serpentines, with the composition depending on formation conditions. Leveraging this new mineralogical context enables quantitative estimation of H₂ production on Earth and Mars. Together, these advances indicate that greenalite solid solutions in ancient rocks produced and released H₂ and thus contributed to planetary habitability. Examination of Martian rocks and analogous Earth materials shows greenalite-hisingerite minerals were responsible for H₂ fluxes to the ancient Martian atmosphere and could be important contributors to planetary habitability throughout the Solar System.

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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.