Thematic Articles

The SiO2 Gemstone Family

Quartz is the most popular and widely used gemstone of the SiO2 family with its phenomenal varieties and spectacular colors, e.g., near-colorless (rock crystal), purple (amethyst), yellow (citrine), smoky (smoky quartz), and pink. The colors of these varieties are mostly caused by trace contents of foreign ions, which in turn are activated by treatment with high-energy radiation and/or temperature treatment (so-called color centers). Cryptocrystalline SiO2 varieties such as agate, chrysoprase, or jasper mostly represent mixtures of SiO2 minerals and other phases, while the play of colors in amorphous precious opal is caused by light diffraction and interference. Despite their different origins and properties, all these SiO2 varieties have played a dominant role as gemstones and cut stone since antiquity.

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Microcrystalline and Amorphous Silica: Materials that Shaped Humanity

The use of microcrystalline silica has been documented among early hominins, with significant diversification over the last ~3 million years, from early toolmaking to applications in personal adornment and symbolic contexts. From the Oldowan onwards, both microcrystalline quartz and amorphous silica are consistently observed in the archaeological record, and they shaped aspects of human technological and behavioral evolution. This article offers insights into how mechanical, environmental, and cultural factors guided the selection of silica materials and their transformation to purposeful objects—from Pliocene hominins through to the Middle Ages. The crystal chemistry that imbues microcrystalline quartz varieties with their unique properties is reviewed, and the formation pathways for biogenic and abiogenic microcrystalline and amorphous silica are considered.

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Quartz-derived Solutions for Renewable Energy Production, Semiconductors, and Beyond

Humankind’s use of silica raw materials began at least 1.85 million years ago with production of flint tools and spans to today’s more than 1000 industrial applications, all relying on its chemistry and specific physical properties. Among the key achievements are the discovery of the piezoelectric effect of quartz for timekeeping, the critical importance of silicon-based semiconductor technologies for the digitalization of our society, and the production of renewable energy through photovoltaics. One of the greatest challenges regarding raw material supply and security lies in identifying new quartz deposits of sufficient purity, size, and properties to meet increasing demands. Although quartz is mined from a variety of deposits, economically viable sources remain difficult to locate for reasons that we explain.

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Quartz—Hour-Glass for Surface Processes

Quartz is a key archive of Earth surface processes, recording erosion, burial, transport, and landscape evolution across a wide range of timescales. Recent advances in quartz-based analytical techniques have expanded the potential for integrative geochemical and geochronological approaches. Fourier-transform infrared spectroscopy (FTIR) enables detailed characterization of quartz provenance and geological history, while terrestrial cosmogenic nuclides (TCNs) constrain surface exposure, burial histories, and denudation rates. Optically stimulated luminescence (OSL) provides robust age control for fine-grained sediment transport and deposition, and ongoing developments in electron spin resonance (ESR) extend chronological constraints into previously inaccessible time ranges. Understanding the principles and limitations of each method is essential for their effective individual and combined applications in reconstructing Earth surface processes.

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The Narrative of Quartz and Silica in the Earth and Other Planetary Bodies

Quartz and other silica minerals are amongst the most important constituents of the Earth’s crust, both as rock-forming mineral components and as tools for understanding Earth processes. Quartz and other forms of silica are essential parts of both the geological and biochemical cycles with the potential to help us understand the processes of our planet across disciplines. This article is a narrative of quartz, starting with its crystallization from fractionated, silica-rich magmas, transport, and deposition of silica by hydro- thermal fluids, as well as physical, chemical, and biogenic processes resulting in silica weathering, transport, accumulation, and the formation of sedimentary silica deposits. Extraterrestrial quartz and silica occurrences are also discussed.

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Quartz and SiO2—Simple Yet Exciting

Despite their simple chemical composition, silica (silicon dioxide, SiO2) minerals comprise a complex system with diverse polymorphs of distinct crystal structures and different stabilities and properties. Quartz is arguably the most important mineral throughout human history, from early survival tools to critical materials for modern advanced technology. In addition, quartz and other silica polymorphs and varieties are excellent archivers and important tools for deciphering geological, environmental, and planetary processes and histories.

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Paleomagnetic Recording at the Grain Scale

Natural rocks harbor diverse assemblages of magnetic mineral grains that record information about past dynamo activity and plate motions, among other processes. For much of its history, however, the field of paleomagnetism has counted on a thorough theoretical understanding of only very fine (≤100 nm) grains magnetized during heating. Here we review experimental and computational advances to move beyond this limitation. Magnetic field microscopy allows us to physically identify mineral grains carrying specific paleomagnetic signals, while nanotomography coupled with micromagnetic simulations offers, for the first time, a quantitative picture of how most naturally occurring magnetic grains behave across geologic time. Together, these techniques open the door to retrieving records from less-than-ideal rocks with complex geological histories.

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Plugged-in Planet: Accessing the Interior of the Earth and Other Terrestrial Bodies via Electrical Properties

Among the different methods used to probe the interior of planets and moons in the Solar System, the ones providing access to the electrical properties of rocks are particularly powerful. From field induction measurements to laboratory impedance spectroscopy experiments, several techniques explore the electrical response of geomaterials at different scales of observation, from planetary to atomic. Detailed snapshots of the Earth’s crust and mantle are obtained from the combination of magnetotelluric surveys with laboratory measurements. In space, induction observations complemented by electrical laboratory experiments have been key to defining the layered structure and thermal state of several terrestrial bodies. Future electrical investigations will continue to reveal the present structure of planetary deep interiors, which is necessary to decipher their evolution.

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Carrying the Planet on their Backs: How Minerals Respond to Stress

Far from being passive building blocks, minerals govern how Earth evolves and deforms, from seismic wave propagation to rock deformation and plate motion. This article explores how pressure builds within Earth and how minerals’ elastic response to compression and seismic waves reveals its internal structure. At higher stresses, beyond their elastic limit, deformation in minerals becomes permanent through crystal plasticity created by crystal defects and strongly enhanced by temperature. Over geological time scales, aggregates of crystals behave effectively as highly viscous fluids, enabling mantle convection and plate dynamics. Understanding Earth’s large-scale behavior therefore requires linking rock rheology to the mechanics of minerals down to crystal defects. By integrating observations, experiments, and models, we uncover the hidden rules connecting atomic interactions to planetary dynamics.

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The Heat is On: Thermal Transport and Melting

Heat is a fundamental driver of planetary evolution, shaping its interior, surface, and atmosphere. On Earth, the flow of heat powers dynamic systems that are essential to life. Thermochemical variations across the core–mantle boundary play an important role in regulating heat flow, which influences the dynamics of both the mantle and the core, including generation of the geodynamo. In this article, we focus on thermal transport and melting, including highlights of new technological developments in laboratory optics and synchrotron facilities. Here, we offer a perspective that highlights the spatial and temporal characteristics of these processes, where new developments expand our understanding of Earth’s thermochemical evolution, and hold promise for applications to other planetary bodies.

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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.