Thematic Articles

The Great Oxidation Event and Mineral Diversification

Before the Great Oxidation Event (GOE), at ~2.4 Ga, the mineralogical record of the near-surface continental environment indicates a low partial pressure of oxygen during weathering, which restricted many elements to a low oxidation state and limited the number of possible minerals formed from these elements. Calculations show that local pulses in the production of O2 by photosynthesis could mobilize some metals (e.g. Mo and Re, but not U), but this O2 would be completely consumed. After the GOE, many elements could occur in one or more oxidized forms in minerals in the near-surface environment. This development resulted in an explosive growth in the diversification of minerals.

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Mineral Environments on the Earliest Earth

The oldest vestiges of crust and marine environments occur only in a few remote areas on Earth today. These rocks are Hadean–Eoarchean in age (~4.5 to 3.6 billion years old) and represent the only available archive of the mineral environments in which life originated. A mineral inventory of the oldest rocks would thus help to constrain the likeliest minerals involved in the origin of life. Such a survey is important from the perspective of mineral evolution, as the emergence of life and subsequent global changes caused by organisms were responsible for more than half the 4400 known minerals on the modern Earth.

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Mineralogical Evolution of Meteorites

The approximately 250 mineral species found in meteorites record the earliest stages of the birth of our solar system. Refractory minerals that formed during the violent deaths of other stars and during condensation of our own solar nebula mixed with a wide range of silicates, sulfi des, and metals to form the most primitive chondritic meteorites. Subsequent aqueous alteration, thermal metamorphism, and shock metamorphism further diversified the minerals found in meteorites. Asteroidal melting at first increased and then dramatically decreased mineralogical diversity, before a new phase of igneous differentiation that presaged the processes that would occur in terrestrial planets.

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The Evolution of Elements and Isotopes

The basic building blocks of all minerals are the approximately 290 stable or long-lived isotopes of 84 elements. Yet, when the universe began and nuclear reactions ceased after about 15 minutes, the only elements present were hydrogen, helium, and traces of lithium. After the groundbreaking work by Cameron and Burbidge and coworkers in the 1950s, it is now understood that all the other elements are made in stars in an ongoing cycle of nucleosynthesis. Stars form, create new elements via nuclear reactions, and finally disperse the new elements into space via winds and explosions, forming the seeds for new stars.

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Mineral Evolution: Mineralogy in the Fourth Dimension

Mineral evolution, which frames mineralogy in a historical context, is based on the premise that the geosphere and biosphere have coevolved through a sequence of deterministic and stochastic events. Three eras of mineral evolution—planetary accretion, crust and mantle reworking, and biologically mediated mineralogy—each saw dramatic changes in the diversity and distribution of Earth’s near-surface minerals. An important implication of this model is that different terrestrial planets and moons achieve different stages of mineral evolution, depending on the geological, petrological, and biological evolution of the body.

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Pathological Biomineralization of Kidney Stones

Kidney stones are aggregates of microcrystals, most commonly containing calcium oxalate monohydrate (COM) as the primary constituent. The formation of these aggregates in the renal tubules of the kidney and their attachment to epithelial cells lining the renal tubules are thought to involve adhesion events between COM crystal surfaces and urinary species that bind to these surfaces. The pathological behavior of COM is in stark contrast to calcium oxalate dihydrate (COD), a different mineral phase commonly found in voided urine but much less frequently in stones, and whose presence is thought to protect against stone formation. This observation suggests that the structure and composition of calcium oxalate crystal surfaces and the fundamental interactions of these surfaces with urinary species are crucial to unraveling the complex pathology of this debilitating disease.

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Toxic Potential of Mineral Dusts

In this outline of the most prominent factors involved in particle toxicology, we highlight the differences in the toxic potential among airborne particles and describe what is known about the most notorious toxic agents, such as silica and asbestos. The various biological paths and, consequently, the different outcomes in the health risks associated with inhaled, micron-sized particle and fibers, as well as inhaled nanoparticles, are explained on the basis of form, size, and surface reactivity. The most relevant surface properties addressed here are the potential for free radical generation, the adsorption of endogenous molecules, and the degree of hydrophilicity or hydrophobicity of the various materials.

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Interactions between Proteins and Soil Mineral Surfaces: Environmental and Health Consequences

Proteins have long been recognized as important compounds in the biogeochemical cycles of terrestrial ecosystems. They can, for example, provide a source of nitrogen for plants and soil microorganisms following proteolysis and ammonification. Extracellular enzymes liberated in soil are essential catalysts in the mobilization of carbon, nitrogen, phosphorus and sulphur from macromolecular organic matter. Proteins are also implicated in new environmental topics, such as soil carbon storage, horizontal transmission of spongiform encephalopathies and potential negative effects of insecticidal toxins released from transgenic plants.

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Bioactive Glass Scaffolds for Bone Regeneration

There is a need for new materials that can stimulate the body’s own regenerative mechanisms and heal tissues. Porous templates (scaffolds) are thought to be required for three-dimensional tissue growth. This article discusses bone regeneration and the specifications of an ideal scaffold and the materials that may be suitable. Bioactive glasses have high potential as scaffold materials as they stimulate bone cells to produce new bone, they are degradable in the body and they bond to bone. The two types of bioactive glasses, their mechanisms for bioactivity and their potential for scaffold production are reviewed. Examples of their current clinical use are highlighted.

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Mineralization of Bones and Teeth

Bones and teeth consist of an inorganic calcium phosphate mineral approximated by hydroxylapatite and matrix proteins. The physical and chemical properties of these “bioapatite” crystals are different from those of geologic hydroxylapatite because of the way they are formed, and these unique properties are required for fulfilling the biological functions of bones and teeth. Recent biochemical studies provide insight into the factors controlling the formation and growth of bioapatite crystals and how alteration in the mineralization process can lead to diseases such as osteoporosis. New spectroscopic and microscopic techniques are enabling scientists to characterize changes in crystal properties in these diseases, providing potentially fruitful areas of collaboration among geochemists, mineralogists, and biological researchers and offering hope for the development of novel therapies.

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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.