Thematic Articles

Himalayan Leucogranites: Field Relationships and Tectonics

Himalayan peraluminous leucogranites were derived from in-situ melting of sillimanite + K-feldspar-bearing pelite-migmatite, and were transported via layer-parallel sill complexes and cross-cutting dykes to feed giant sills up to 5 km thick. Partially melted Himalayan middle crust was extruded southwards between two large-scale, north-dipping, synchronous ductile shear zones: the Main Central Thrust (MCT) below and the low-angle normal fault South Tibetan Detachment (STD) above. U-Th/Pb monazite dating constrains granite melting to ~25–18.5 Ma in Manaslu and ~24–13 Ma in Everest-Makalu. The Manaslu sheeted sill complex was emplaced by progressive underplating with the oldest intrusions structurally above younger intrusions. Heat was dominantly derived by internal radioactive heating from crustal thickening with little or no contribution from shear heating along the MCT or from the mantle.

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Himalayan Leucogranites: Petrogenesis and Significance

Himalayan leucogranites crop out intermittently over 2000 km along the crest of the world’s youngest and largest mountain range. They are derived from partial melting of continental crust during a classic continental collisional orogeny. Studies of these leucogranites have significantly advanced knowledge of crustal anatexis, felsic magmatic differentiation, and the tectonic evolution of the Himalayan-Tibetan orogen. This Elements thematic issue provides an overview of the petrogenesis and significance of the Himalayan leucogranites including field relations, source rocks, petrology, geochemistry, tectonics, and links to orogenesis and economic resources. It not only summarizes the state-of-the-art research on Himalayan leucogranites but also demonstrates how a multidisciplinary approach can help constrain the origins and evolution of granites, their associated mineralizations, and related geodynamic development.

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Luminescence Applications in Ore Geology, Mining, and Industry

Luminescence applications in ore geology, mining, and beneficiation include remote prospecting, ground-based exploration, and radio metric sorting. Remote prospecting for ores with a drone or helicopter- borne luminescent sensing using laser excitation and time-delayed detection is becoming commonplace. Modern ground-based exploration increasingly utilises outlining of luminescing “fugitive calcite” veinlet halos, whose characteristics can rapidly and inexpensively give information on the overall size of a mineralised system and the principal structural controls on ore fluid migration pathways. Diamonds and scheelite have been found and recovered through X-ray luminescent radiometric sorting, while laser-induced luminescence has great potential, especially for sorting diamonds lacking X-ray luminescence, fluorite, spodumene, and rare earth element (REE)–bearing minerals. The luminescence concept is expanded here to include laser-induced breakdown spectroscopy; its fusion with X-ray techniques provides simultaneous information on both the mineralogical and chemical composition of a rock.

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Analysing the Luminescence of Gems

Luminescence imaging and spectroscopy have become essential in gem testing, as most gem minerals and materials exhibit specific luminescence when properly excited. With a range of techniques introduced in gem testing laboratories in the past quarter century, such as luminescence imaging and photoluminescence (PL) emission and excitation spectroscopies, there are many applications to gem materials for establishing their identity, separating natural from synthetic gems, and detecting potential treatments. Further, these techniques often give clues towards the identity of emitting defects. Luminescence-based testing has recently gained attention even outside the gemmological laboratory as many simple luminescence-based instruments are offered to the gem and jewellery trade to separate natural from synthetic diamonds or from their imitations.

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Luminescence Applications in Petrology

Luminescence is a powerful tool to infer physical and chemical conditions during mineral growth. It is very subtly linked to temperature of formation, composition and structural state, and related changes during rock evolution that often cause striking contrasts in the light emitted. This information can show magma sources and the hydrothermal evolution of igneous rocks, sources and diagenesis in sedimentary systems, and the pressure–temperature evolution during metamorphism. However, luminescence is most powerful when it goes beyond imaging, coupling with spectroscopies and microgeochemical techniques. We present examples of luminescence spectroscopies in igneous, sedimentary, and metamorphic rocks to show how these methods elucidate geological processes. Luminescence imaging is an exciting scientific frontier in which novel methods provide ever deeper insights into petrogenesis.

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Luminescence Images: What is it That You See?

Luminescence imaging and hyperspectral luminescence mapping are powerful analytical tools with widespread applications in geosciences and materials science. The luminescence of minerals is mainly a defect phenomenon caused by lattice defects and/or impurity elements. This in turn allows one to study trace-element composition and the structural state of a sample by means of its emission. One of the most spectacular and widely used applications of luminescence images is to visualise internal textures in minerals that are not revealed by other analytical techniques. Herein we present a selection of examples for the extraordinary sensitivity of luminescence imaging. We also show that precise information on samples is obtained if luminescence imaging is combined with spectroscopic analysis of the emission and/ or complementary analytical techniques.

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Activators in Minerals and the Role of Electronic Defects

Luminescence in minerals is created by ions, groups of ions, or electronic defects that can absorb energy and emit it as visible light. These units are commonly referred to as “centers” or “activators.” They can be impurities in the mineral or intrinsic constituents. In some cases, separate ions (so-called “sensitizers”) act to aid the luminescence process by preferentially absorbing energy and sending it to the emitting unit. In other cases, ions or electronic defects can slow the emission process by trapping excited electrons. Ions preventing emission from other luminescence centers are called “quenchers.” Some impurities can potentially create almost any luminescent color, while others are known for particular colored emission. Luminescence may exhibit strong zonation in crystals due to selective uptake of the activating ions.

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Luminescence: The “Cold Glow” of Minerals

Luminescence is the eye-catching phenomenon of light emission by a mineral after some input of energy (the excitation). Although commonly used in Earth sciences only to produce images, much more can be extracted from this phenomenon. Luminescence is extremely sensitive to low levels of emitters (activators), which helps to reveal the geochemistry or the creation of defects. We give an overview of the great variety of techniques (cathodoluminescence, photoluminescence, and more), discuss vocabulary issues (such as excitation versus stimulation, or the different types of persistent luminescence phenomena), and propose wording we feel best reflects today’s knowledge. We explain the basics of luminescence spectroscopy with emission, excitation, and time-resolved spectra to obtain useful data for Earth scientists.

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The Geological History of Water: From Earth’s Accretion to the Modern Deep Water Cycle

The abundance of water on Earth and its distribution between surficial and deep reservoirs are the outcome of 4.6 billion years of geological history involving various mechanisms of water in and outgassing. Here, we use the metaphor of a pipeline connecting Earth’s deep and surface water reservoirs. The net flux through this pipeline has changed over time due to contrasting Hadean, Archean, and modern geodynamic regimes. Most water was dissolved in the primordial magma ocean, entrapped in the solidifying mantle, and massively released by volcanism during the Hadean and Archaean. As Earth cooled, plate tectonics enabled water ingassing into the mantle, which appears to exceed outgassing under the modern tectonic regime, implying that Earth’s surface has been drying out and will continue to do so.

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Probing Deep Hydrogen Using Electrical Conductivity

Electrical conductivity is perhaps the physical property of rocks that is most sensitive to the presence of hydrogen. Hydrogen enhances conductivity via proton conduction in minerals or by stabilizing highly conductive phases, such as hydrous silicate melts or aqueous fluids. Hydrogen might also be stored in the metallic core. Electrical conductivity measurements in the laboratory can be used to interpret magnetotelluric maps of the mantle in terms of hydrogen content and distribution. In active tectonic settings like subduction zones, anomalously high conductivities have revealed the distribution and migration pathways of H-bearing melts and fluids, illuminating the transport of hydrogen in our planet’s interior.

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