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        <title>EJM - recent articles</title>


    <link rel="self" href="https://ejm.copernicus.org/articles/"/>
    <id>https://ejm.copernicus.org/articles/</id>
    <updated>2026-09-06T22:15:55+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-545-2026</id>
            <title type="html">The impact of exsolution textures in Fe&#8211;Ti oxide minerals on crushing strategies and vanadium and titanium pre-concentration
            </title>
            <link href="https://doi.org/10.5194/ejm-38-545-2026"/>
            <summary type="html">
                &lt;b&gt;The impact of exsolution textures in Fe–Ti oxide minerals on crushing strategies and vanadium and titanium pre-concentration&lt;/b&gt;&lt;br&gt;
                Thomas Daniel van Gerve, Philippe Muchez, Ted Nuorivaara, and Olivier Namur&lt;br&gt;
                    Eur. J. Mineral., 38, 545&#8211;556, https://doi.org/10.5194/ejm-38-545-2026, 2026&lt;br&gt;
                Vanadium ores from the Bushveld Complex contain distinct microscopic mineral textures that strongly influence how efficiently vanadium can be extracted. Our study shows that some textures tightly intergrow minerals and hinder separation, while others form coarser structures that improve processing by magnetic and flotation methods. Identifying these textures is essential for optimizing vanadium ore processing and resource use.
            </summary>
            <content type="html">
                &lt;b&gt;The impact of exsolution textures in Fe–Ti oxide minerals on crushing strategies and vanadium and titanium pre-concentration&lt;/b&gt;&lt;br&gt;
                Thomas Daniel van Gerve, Philippe Muchez, Ted Nuorivaara, and Olivier Namur&lt;br&gt;
                    Eur. J. Mineral., 38, 545&#8211;556, https://doi.org/10.5194/ejm-38-545-2026, 2026&lt;br&gt;
                <p>Vanadiferous titanomagnetite (VTM) ores in mafic layered intrusions host the world's largest vanadium resources, with the Bushveld Complex representing the principal global deposit. This study examines the mineral textures and element redistributions in magnetite&amp;#8211;ilmenite assemblages from Bushveld Upper Zone magnetites. Two main magnetite exsolution microstructures are identified: cloth textures dominated by ulv&amp;#246;spinel lamellae and sandwich or trellis textures characterized by ilmenite lamellae formed through ulv&amp;#246;spinel oxidation. In situ elemental analyses demonstrate that vanadium is concentrated in magnetite relative to ilmenite and that oxidation-driven exsolution enhances V enrichment in residual magnetite while concentrating Ti into ilmenite. The textural type strongly controls liberation potential: cloth textures exhibit pervasive fine intergrowths that hinder beneficiation, whereas sandwich and trellis textures show coarser separable lamellae. These microstructural variations have direct implications for magnetic, gravity, and flotation processing efficiency. The results highlight the necessity of textural characterization to optimize V&amp;#8211;Ti ore beneficiation strategies.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-21T22:15:55+02:00</published>
            <updated>2026-08-21T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-531-2026</id>
            <title type="html">Belmonteite, CaMn<sub>2</sub>(AsO<sub>4</sub>)<sub>2</sub>(H<sub>2</sub>O)<sub>5</sub>&#8201;&#8901;&#8201;2H<sub>2</sub>O, a new arsenate mineral from the Mn ore deposits of the Graveglia Valley, eastern Liguria, Italy
            </title>
            <link href="https://doi.org/10.5194/ejm-38-531-2026"/>
            <summary type="html">
                &lt;b&gt;Belmonteite, CaMn2(AsO4)2(H2O)5 ⋅ 2H2O, a new arsenate mineral from the Mn ore deposits of the Graveglia Valley, eastern Liguria, Italy&lt;/b&gt;&lt;br&gt;
                Cristian Biagioni, Jiří Sejkora, and Zdeněk Dolníček&lt;br&gt;
                    Eur. J. Mineral., 38, 531&#8211;543, https://doi.org/10.5194/ejm-38-531-2026, 2026&lt;br&gt;
                Belmonteite, CaMn<sub>2</sub>(AsO<sub>4</sub>)<sub>2</sub>(H<sub>2</sub>O)<sub>5</sub>&amp;#183;2H<sub>2</sub>O, is a new mineral discovered in the Mn ore deposits of eastern Liguria (Italy). Its crystal structure shows {010} layers of six-fold-coordinated Mn atoms decorated on both sides by (AsO<sub>4</sub>) groups and Ca atoms and connected through H bonds. The genesis of this mineral is related to the circulation of As-rich oxidizing fluids within the Mn ore deposits. The name honors Donato Belmonte for his contribution to the knowledge of the mineralogy of Liguria.
            </summary>
            <content type="html">
                &lt;b&gt;Belmonteite, CaMn2(AsO4)2(H2O)5 ⋅ 2H2O, a new arsenate mineral from the Mn ore deposits of the Graveglia Valley, eastern Liguria, Italy&lt;/b&gt;&lt;br&gt;
                Cristian Biagioni, Jiří Sejkora, and Zdeněk Dolníček&lt;br&gt;
                    Eur. J. Mineral., 38, 531&#8211;543, https://doi.org/10.5194/ejm-38-531-2026, 2026&lt;br&gt;
                <p>Belmonteite (IMA 2024-040), ideally CaMn<span class="inline-formula"><sub>2</sub></span>(AsO<span class="inline-formula"><sub>4</sub></span>)<span class="inline-formula"><sub>2</sub></span>(H<span class="inline-formula"><sub>2</sub></span>O)<span class="inline-formula"><sub>5</sub>&amp;#8901;</span>2H<span class="inline-formula"><sub>2</sub></span>O, is a new arsenate mineral discovered in the Gambatesa mine, Graveglia Valley, Ne, Genoa Province, Liguria, Italy. It occurs as aggregates up to 0.5&amp;#8201;mm in length, formed by thin tabular crystals, white in color, with a silky luster and white streak. A perfect {010} cleavage was observed. Associated minerals are tennantite-(Cu), calcite, and a still unidentified (Ca,Cu)-arsenate secondary phase. Calculated density is 2.677&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. The empirical chemical formula of belmonteite is (Ca<span class="inline-formula"><sub>0.86</sub></span>Mn<span class="inline-formula"><sub>0.11</sub></span>K<span class="inline-formula"><sub>0.01</sub></span>)<span class="inline-formula"><sub>&amp;#931;0.98</sub></span>(Mn<span class="inline-formula"><sub>1.90</sub></span>Cu<span class="inline-formula"><sub>0.08</sub></span>Al<span class="inline-formula"><sub>0.02</sub></span>)<span class="inline-formula"><sub>&amp;#931;2.00</sub></span>As<span class="inline-formula"><sub>2.01</sub></span>O<span class="inline-formula"><sub>8</sub>&amp;#8901;</span>7H<span class="inline-formula"><sub>2</sub></span>O. Unit-cell parameters are <span class="inline-formula"><i>a</i>=8.8418(9)</span>, <span class="inline-formula"><i>b</i>=23.031(2)</span>, <span class="inline-formula"><i>c</i>=13.5270(14)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=2754.6(5)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, space group <i>Cmce</i>, <span class="inline-formula"><i>Z</i>=8</span>. The crystal structure of belmonteite was refined to <span class="inline-formula"><i>R</i><sub>1</sub>=0.0385</span&gt; for 1195 unique reflections with <span class="inline-formula"><i>F</i>>4<i>&amp;#963;</i>(<i>F</i>)</span&gt; and 129 refined parameters. It can be described as being formed by {010} layers of six-fold-coordinated Mn atoms decorated on both sides by (AsO<span class="inline-formula"><sub>4</sub></span>) groups and Ca atoms. These heteropolyhedral layers are connected along <span class="inline-formula"><i>b</i></span&gt; through H bonds. Belmonteite displays {010} layers topologically similar to those occurring in switzerite. The genesis of belmonteite is probably related to the circulation of As-rich oxidizing fluids within the Mn ore deposit exploited at the Gambatesa mine during its late-stage evolution. The name honors Donato Belmonte (born&amp;#160;1978) for his earlier contribution to the knowledge of the mineralogy of Liguria.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-19T22:15:55+02:00</published>
            <updated>2026-08-19T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-519-2026</id>
            <title type="html">Fengruiite, [Ag<sub>6</sub>Sb<sub>2</sub>S<sub>7</sub>][Ag<sub>9</sub>CuS<sub>2</sub>Te<sub>2</sub>], a new Ag&#8211;Sb&#8211;Te sulfosalt mineral from the Haopinggou Ag&#8211;Pb&#8211;Zn&#8211;Au deposit, eastern Qinling, China
            </title>
            <link href="https://doi.org/10.5194/ejm-38-519-2026"/>
            <summary type="html">
                &lt;b&gt;Fengruiite, [Ag6Sb2S7][Ag9CuS2Te2], a new Ag–Sb–Te sulfosalt mineral from the Haopinggou Ag–Pb–Zn–Au deposit, eastern Qinling, China&lt;/b&gt;&lt;br&gt;
                Yongfei Tian, Guowu Li, Ningyue Sun, Min Liu, Jingwen Mao, Yunpeng Dong, Peng Liu, Wei Jian, Wei Yao, Xiuquan Wang, and Huishou Ye&lt;br&gt;
                    Eur. J. Mineral., 38, 519&#8211;530, https://doi.org/10.5194/ejm-38-519-2026, 2026&lt;br&gt;
                We studied a newly discovered silver-rich mineral from an ore deposit in central China to understand how silver is stored in nature. Using microscopy, chemical, and crystal-structure tests, we found that this mineral is a new species with a unique tellurium-rich structure. Our results show that tellurium helped trap and concentrate silver in hot mineral-forming fluids, offering new clues to how silver-rich deposits form.
            </summary>
            <content type="html">
                &lt;b&gt;Fengruiite, [Ag6Sb2S7][Ag9CuS2Te2], a new Ag–Sb–Te sulfosalt mineral from the Haopinggou Ag–Pb–Zn–Au deposit, eastern Qinling, China&lt;/b&gt;&lt;br&gt;
                Yongfei Tian, Guowu Li, Ningyue Sun, Min Liu, Jingwen Mao, Yunpeng Dong, Peng Liu, Wei Jian, Wei Yao, Xiuquan Wang, and Huishou Ye&lt;br&gt;
                    Eur. J. Mineral., 38, 519&#8211;530, https://doi.org/10.5194/ejm-38-519-2026, 2026&lt;br&gt;
                <p>Fengruiite, ideally [Ag<span class="inline-formula"><sub>6</sub></span>Sb<span class="inline-formula"><sub>2</sub></span>S<span class="inline-formula"><sub>7</sub></span>][Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>Te<span class="inline-formula"><sub>2</sub></span>], is a new mineral species of the pearceite&amp;#8211;polybasite group discovered in the Haopinggou Ag&amp;#8211;Pb&amp;#8211;Zn&amp;#8211;Au deposit, eastern Qinling, China, and approved by the IMA Commission on New Minerals, Nomenclature and Classification as IMA 2024-045. The mineral occurs as irregular grains (<span class="inline-formula"><</span>&amp;#8201;20&amp;#8201;<span class="inline-formula">&amp;#215;</span>&amp;#8201;80&amp;#8201;<span class="inline-formula">&amp;#181;</span>m) intergrown with galena, cervelleite, and chalcopyrite in intermediate-sulfidation epithermal veins. Fengruiite is opaque, gray with a metallic luster, and brittle and has an estimated Mohs hardness of 3&amp;#8211;4. EPMA analyses yield Ag (65.9&amp;#8201;wt&amp;#8201;%&amp;#8211;68.6&amp;#8201;wt&amp;#8201;%), S (12.6&amp;#8201;wt&amp;#8201;%&amp;#8211;13.1&amp;#8201;wt&amp;#8201;%), Sb (9.1&amp;#8201;wt&amp;#8201;%&amp;#8211;10.1&amp;#8201;wt&amp;#8201;%), Te (6.3&amp;#8201;wt&amp;#8201;%&amp;#8211;7.6&amp;#8201;wt&amp;#8201;%), and Cu (3.3&amp;#8201;wt&amp;#8201;%&amp;#8211;3.8&amp;#8201;wt&amp;#8201;%), corresponding to the empirical formula [(Ag<span class="inline-formula"><sub>5.87</sub></span>Cu<span class="inline-formula"><sub>0.29</sub></span>)<span class="inline-formula"><sub>&amp;#931;6.16</sub></span>(Sb<span class="inline-formula"><sub>1.89</sub></span>As<span class="inline-formula"><sub>0.03</sub></span>)<span class="inline-formula"><sub>&amp;#931;1.92<i>S</i>7</sub></span>] [Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>(Te<span class="inline-formula"><sub>1.28</sub></span>S<span class="inline-formula"><sub>0.63</sub></span>)S<span class="inline-formula"><sub>1.91</sub></span>]. Fengruiite is trigonal, space group <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M27" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>P</mi><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mi>m</mi><mn mathvariant="normal">1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="32pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="1bbc046b02fc4937363ceadaa1512235"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-519-2026-ie00001.svg" width="32pt" height="13pt" src="ejm-38-519-2026-ie00001.png"/></svg:svg></span></span&gt; (#164), with <span class="inline-formula"><i>a</i>=7.6087</span>(9)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=11.970</span>(2)&amp;#8201;&amp;#197;, and <span class="inline-formula"><i>V</i>=600.13</span>(17)&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span&gt; (<span class="inline-formula"><i>Z</i>=1</span>). Its structure consists of alternating negatively charged [Ag<span class="inline-formula"><sub>6</sub></span>Sb<span class="inline-formula"><sub>2</sub></span>S<span class="inline-formula"><sub>7</sub></span>] (<span class="inline-formula"><i>A</i></span>) and positively charged [Ag<span class="inline-formula"><sub>9</sub></span>CuS<span class="inline-formula"><sub>2</sub></span>Te<span class="inline-formula"><sub>2</sub></span>] (<span class="inline-formula"><i>B</i></span>) layers, characteristic of the polybasite-Tac polytype. The combination of a Te-dominant <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M41" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><mi mathvariant="normal">Te</mi><mn mathvariant="normal">1</mn><mo>/</mo><mi mathvariant="normal">S</mi><mn mathvariant="normal">1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="39pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="c6fb1d2e9865b77b41ba71cdcd9a84a8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-519-2026-ie00002.svg" width="39pt" height="14pt" src="ejm-38-519-2026-ie00002.png"/></svg:svg></span></span&gt; site in the <span class="inline-formula"><i>B</i></span>-layer module and S-dominant anion sites throughout the <span class="inline-formula"><i>A</i></span>-layer module distinguishes fengruiite from Te-rich polybasite-Tac and benleonardite. As the first structurally characterized Te-rich member of the pearceite&amp;#8211;polybasite group reported from the East Qinling metallogenic belt, fengruiite expands the known structural and chemical diversity of Ag sulfosalts and documents Te incorporation into an Ag-rich sulfosalt structure in an epithermal system.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-13T22:15:55+02:00</published>
            <updated>2026-08-13T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-497-2026</id>
            <title type="html">A novel experimental approach to investigate element transport and isotope fractionation of Li and B in pegmatitic systems during fluid&#8211;melt interaction
            </title>
            <link href="https://doi.org/10.5194/ejm-38-497-2026"/>
            <summary type="html">
                &lt;b&gt;A novel experimental approach to investigate element transport and isotope fractionation of Li and B in pegmatitic systems during fluid–melt interaction&lt;/b&gt;&lt;br&gt;
                Christian Ronny Singer, Harald Behrens, Ingo Horn, Martin Oeser, Stefan Weyer, and François Holtz&lt;br&gt;
                    Eur. J. Mineral., 38, 497&#8211;518, https://doi.org/10.5194/ejm-38-497-2026, 2026&lt;br&gt;
                We developed a novel experimental setup to investigate the transport of Li and B between two melt reservoirs that were connected only via a fluid phase. This was used to simulate fluid exsolution occurring during late-stage pegmatite formation. We found that both Li and B were transported via the fluid, but the observed transport rates were low. It was shown experimentally that the Li isotopes fractionate between melt and fluid with the fluid being preferentially enriched in the heavier <sup>7</sup>Li.
            </summary>
            <content type="html">
                &lt;b&gt;A novel experimental approach to investigate element transport and isotope fractionation of Li and B in pegmatitic systems during fluid–melt interaction&lt;/b&gt;&lt;br&gt;
                Christian Ronny Singer, Harald Behrens, Ingo Horn, Martin Oeser, Stefan Weyer, and François Holtz&lt;br&gt;
                    Eur. J. Mineral., 38, 497&#8211;518, https://doi.org/10.5194/ejm-38-497-2026, 2026&lt;br&gt;
                <p>A novel experimental setup was developed to simulate the transport processes of Li and B and their isotopes via a fluid phase in a flux-rich pegmatitic system (1.7&amp;#8201;% Li<span class="inline-formula"><sub>2</sub></span>O, 2.5&amp;#8201;% B<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span>). The transport capacity of the fluid was estimated by the determination of Li and B in two melt reservoirs, an Li- and B-rich source melt, and an initially Li- and B-free sink melt. These melts were physically separated by a coarse-grained (250&amp;#8211;180&amp;#8201;<span class="inline-formula">&amp;#181;</span>m fraction) porous filling material containing the fluid phase that acted as the transport medium. The effectivity of Li and B transport was investigated at 100&amp;#8201;MPa by changing various parameters in the experimental setup. The impact of the chemical composition of the filling material was tested using either quartz or zircon. Different fluid compositions containing either NaCl or CsCl were investigated with a constant Cl concentration of 0.17&amp;#8201;mol&amp;#8201;kg<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; in the fluid. Two different temperature distribution scenarios were investigated: (1) isothermal conditions of 850&amp;#8201;&amp;#176;C along the sample and (2) a temperature gradient from the source to the sink melt varying from ca. 830 to 770&amp;#8201;&amp;#176;C. The duration of the experiments was varied between 1 and 96&amp;#8201;h.</p&gt;        <p>The results of the experiments indicate that the effectivity of Li and B transport between the two melts via a fluid phase is influenced by a complex interplay of experimental duration, temperature distribution, and reactive surface area (between melt and fluid). The amount of Li and B in the sink melt generally correlates positively with experimental duration, which can be explained by a gradual mobilization of these elements from the source melt. For experiments with a temperature gradient between source and sink, higher Li and B concentrations in the sink melt were observed compared to experiments conducted under isothermal conditions. The sink melt was enriched in the heavier <span class="inline-formula"><sup>7</sup></span>Li, which can be best explained by equilibrium isotope fractionation between silicate melt and fluid. These findings demonstrate experimentally, for the first time, the preferential partitioning of <span class="inline-formula"><sup>7</sup></span>Li into a fluid phase compared to silicate melt. For B, possible isotope effects are smaller than our analytical uncertainty (<span class="inline-formula">&amp;#177;</span>4.7&amp;#8201;&amp;#8240;), which is likely related to the high experimental temperature and similar bonding environments of B in melts and fluids. There is no evidence for kinetic isotope fractionation during transport of Li and B in the fluid which, expectedly, would result in an enrichment of light isotopes in the sink. Our experimental results indicate that equilibrium for Li isotopes can be established rapidly between a melt and a fluid phase. This may be important for the interpretation of isotope data in pegmatite minerals and the role of a fluid phase during their formation by disequilibrium crystallization caused by strong undercooling.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-08-06T22:15:55+02:00</published>
            <updated>2026-08-06T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-491-2026</id>
            <title type="html">IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) &#8211; Newsletter 92
            </title>
            <link href="https://doi.org/10.5194/ejm-38-491-2026"/>
            <content type="html">
                &lt;b&gt;IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) – Newsletter 92&lt;/b&gt;&lt;br&gt;
                Ferdinando Bosi, Frédéric Hatert, Marco Pasero, and Stuart J. Mills&lt;br&gt;
                    Eur. J. Mineral., 38, 491&#8211;495, https://doi.org/10.5194/ejm-38-491-2026, 2026&lt;br&gt;
                
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-31T22:15:55+02:00</published>
            <updated>2026-07-31T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-477-2026</id>
            <title type="html">Preservation of water concentration in mantle xenoliths: a case study from All&#232;gre and Ray Pic volcanoes (French Massif Central)
            </title>
            <link href="https://doi.org/10.5194/ejm-38-477-2026"/>
            <summary type="html">
                &lt;b&gt;Preservation of water concentration in mantle xenoliths: a case study from Allègre and Ray Pic volcanoes (French Massif Central)&lt;/b&gt;&lt;br&gt;
                Konstantinos Thomaidis, Jannick Ingrin, Etienne Deloule, Lydéric France, and Huan Chen&lt;br&gt;
                    Eur. J. Mineral., 38, 477&#8211;489, https://doi.org/10.5194/ejm-38-477-2026, 2026&lt;br&gt;
                Water in the form of hydrous-point-defect pyroxenes from mantle xenoliths is used to trace the water content in the lithospheric mantle. However, little is known about the mechanism that allows xenoliths to preserve deep hydrogen signatures. In particular, it is unknown how much of the water content of xenoliths is modified during the emplacement of lava and cooling at the surface and by the eruption mode (effusive versus explosive). In this work, we attempted to address these matters.
            </summary>
            <content type="html">
                &lt;b&gt;Preservation of water concentration in mantle xenoliths: a case study from Allègre and Ray Pic volcanoes (French Massif Central)&lt;/b&gt;&lt;br&gt;
                Konstantinos Thomaidis, Jannick Ingrin, Etienne Deloule, Lydéric France, and Huan Chen&lt;br&gt;
                    Eur. J. Mineral., 38, 477&#8211;489, https://doi.org/10.5194/ejm-38-477-2026, 2026&lt;br&gt;
                <p>Water in the form of hydrous point defects in the crystal structure of pyroxenes from mantle xenoliths is frequently used to trace the water content in the lithospheric mantle. However, little is known about the mechanism that allows xenoliths to preserve deep hydrogen signatures and if we can avoid a complete or partial reset by reaction with the host magma during transport. In particular, it is unknown how much of the water content of xenoliths is modified during the emplacement of lava and cooling at the surface and by the eruption mode (effusive versus explosive). In this work, we attempted to address to these matters.</p&gt;        <p>We analysed the water content of peridotite xenoliths from two localities in the French Massif Central, All&amp;#232;gre and Ray Pic, using Fourier transform infrared (FTIR) spectroscopy. We performed point analyses and profile measurements in olivine (ol), clinopyroxene (cpx), and orthopyroxene (opx) crystals derived from 17 xenoliths. The two localities have different types of outcrops. In All&amp;#232;gre, the xenoliths are present in a frozen lava lake with a vertical structure, while in Ray Pic, xenoliths are hosted both in pyroclastic deposits and in a lava flow running over more than 20&amp;#8201;km along a riverbed. Both studies on xenoliths in different parts of the lava flow show that the solidification and cooling of the basalt at the surface do not significantly affect the water content of pyroxenes in the xenoliths. The xenoliths do not show the presence of diffusion profiles, and the water content is independent of the location of the xenoliths within the lava bodies. However, the comparison of the water content of xenoliths from the pyroclastic deposit and within the lava flow at Ray Pic shows that the water concentrations are strongly impacted by the degree of degassing of the magma before the eruption. The concentrations of xenoliths in the degassed lava flow are much lower, by a factor of <span class="inline-formula"><i>></i></span>&amp;#8201;10 in ol and <span class="inline-formula">&amp;#8805;</span>&amp;#8201;2 in cpx and opx, compared to xenoliths from the pyroclastic deposits. Therefore, water content measured in pyroxenes can only represent minimal values, even for xenoliths hosted in rapidly cooled volcanic products (e.g. explosive eruptions). The amount of water in mantle xenoliths does not reflect the original amount of water in the lithospheric mantle. On the contrary, this study indicates that xenoliths picked up within the same lava flow, even at a few metres' distance, can exhibit pyroxenes with different spectral signatures. This suggests that the spectral signatures have been acquired before the emplacement of the lava flow and were not affected by the late degassing that occurred just before the eruption of the lava flow.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-27T22:15:55+02:00</published>
            <updated>2026-07-27T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-461-2026</id>
            <title type="html">Thermally activated multistep alteration of Fe<sup>2+</sup>-bearing fluorophlogopite revealed by in situ Raman spectroscopy
            </title>
            <link href="https://doi.org/10.5194/ejm-38-461-2026"/>
            <summary type="html">
                &lt;b&gt;Thermally activated multistep alteration of Fe2+-bearing fluorophlogopite revealed by in situ Raman spectroscopy&lt;/b&gt;&lt;br&gt;
                Christian Reinberg, Stylianos Aspiotis, Thomas Malcherek, Stefan T. M. Peters, and Boriana Mihailova&lt;br&gt;
                    Eur. J. Mineral., 38, 461&#8211;475, https://doi.org/10.5194/ejm-38-461-2026, 2026&lt;br&gt;
                By applying in situ high-temperature Raman spectroscopy to (OH)<sup>-</sup>- and Fe<sup>2+</sup>-bearing fluorophlogopite we show that a phonon-driven structural instability near 600 K triggers the mobilization of interlayer K<sup>+</sup&gt; cations, which can act as charge carriers. Above 1100 K all H<sup>+</sup&gt; cations delocalize and can also contribute to transport processes. Above 1300 K oxidation of Fe takes place, along with limited dehydrogenation and dehydroxylation, facilitating partial K<sup>+</sup&gt; leakage and structural decomposition.
            </summary>
            <content type="html">
                &lt;b&gt;Thermally activated multistep alteration of Fe2+-bearing fluorophlogopite revealed by in situ Raman spectroscopy&lt;/b&gt;&lt;br&gt;
                Christian Reinberg, Stylianos Aspiotis, Thomas Malcherek, Stefan T. M. Peters, and Boriana Mihailova&lt;br&gt;
                    Eur. J. Mineral., 38, 461&#8211;475, https://doi.org/10.5194/ejm-38-461-2026, 2026&lt;br&gt;
                <p>Elucidating the temperature-induced structural and crystallochemical transformations in phlogopite mineral species with a partial substitution of Fe<span class="inline-formula"><sup>2+</sup></span&gt; for Mg at the M(1,2) sites and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msup><mi mathvariant="normal">OH</mi><mo>-</mo></msup><mo>/</mo><msup><mi mathvariant="normal">F</mi><mo>-</mo></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="44pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="bbf2a948f9530a8ff19e0fda7b67cf41"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-461-2026-ie00001.svg" width="44pt" height="14pt" src="ejm-38-461-2026-ie00001.png"/></svg:svg></span></span&gt; occupancy disorder at the X site can help in better understanding the transport phenomena in the lithosphere and mantle metasomatism. Here we present the results from in situ temperature-dependent Raman spectroscopy on fluorophlogopite with Fe<span class="inline-formula"><sup>2+</sup></span&gt; content of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;0.15 atoms per formula unit (apfu) and hydroxyl-group content of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;0.40&amp;#8201;apfu. A few heating&amp;#8211;cooling runs were conducted in air up to different temperatures, with the highest temperature achieved being 1450&amp;#8201;K. The chemical composition and crystal structure before and after cooling down from 1450&amp;#8201;K to room temperature were probed by wavelength-dispersive electron microprobe analysis (WD-EMPA) and single-crystal X-ray diffraction (XRD), respectively. The anomalies in the temperature dependencies of phonons reveal a sequence of heating-induced changes in phlogopite: (1) near 550&amp;#8211;650&amp;#8201;K structural instability related to interlayer interactions occurs, which activates the mobility of interlayer K<span class="inline-formula"><sup>+</sup></span&gt; cations. This process is reversible up to <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1100&amp;#8201;K, and, hence, diffusion of K<span class="inline-formula"><sup>+</sup></span&gt; can potentially contribute to phlogopite electrical conductivity between <span class="inline-formula">&amp;#8764;</span>&amp;#8201;650&amp;#8211;1100&amp;#8201;K. (2) At <span class="inline-formula">&amp;#8764;</span>&amp;#8201;1150&amp;#8201;K all H<span class="inline-formula"><sup>+</sup></span&gt; cations delocalize, including those from OH groups linked to MgMgMg chemical configurations, and therefore can also act as charge carriers. (3) Between 1300 and 1450&amp;#8201;K irreversible Fe<span class="inline-formula"><sup>2+</sup></span>&amp;#8201;<span class="inline-formula">&amp;#8594;</span>&amp;#8201;Fe<span class="inline-formula"><sup>3+</sup></span&gt; oxidation develops, confirmed by a permanent resonance Raman-scattering signal after cooling down to room temperature, along with a subtle decrease in the unit-cell volume. Simultaneously, partial dehydrogenation and dehydroxylation take place as only 65&amp;#8201;% of the hydroxyl groups recover at room temperature. The Raman-scattering data also suggest a minor loss of K<span class="inline-formula"><sup>+</sup></span&gt; (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;0.02&amp;#8201;apfu) from the mica structure, whereas WD-EMPA indicates no change in the content of F<span class="inline-formula"><sup>&amp;#8722;</sup></span&gt; within uncertainties. A partial thermal decomposition of fluorophlogopite occurs above 1300&amp;#8201;K, leading to the formation of a minor amount of nano-sized forsterite (<span class="inline-formula">&amp;#8764;</span>&amp;#8201;1&amp;#8201;% in volume), which nucleates mainly on the sample surface parallel to the cleavage plane.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-22T22:15:55+02:00</published>
            <updated>2026-07-22T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-449-2026</id>
            <title type="html">Xianhuaite-(Ce), K<sub>2</sub>CeNb<sub>5</sub>O<sub>15</sub>, a new niobium mineral from the Bayan Obo deposit, China
            </title>
            <link href="https://doi.org/10.5194/ejm-38-449-2026"/>
            <summary type="html">
                &lt;b&gt;Xianhuaite-(Ce), K2CeNb5O15, a new niobium mineral from the Bayan Obo deposit, China&lt;/b&gt;&lt;br&gt;
                Bo Yang, Yuan Xue, Li Yang, Ningyue Sun, Guowu Li, Junfang Yu, Guoying Yan, Jianyong Liu, Yonggang Zhao, Wenxiang Meng, Zhenyu Chen, Lei Chen, Ze Liu, Zhao Yan, Xinyu Hou, Xin Ao, and Jinlong Wang&lt;br&gt;
                    Eur. J. Mineral., 38, 449&#8211;459, https://doi.org/10.5194/ejm-38-449-2026, 2026&lt;br&gt;
                Researchers studying the Bayan Obo deposit in northern China discovered an unknown mineral named xianhuaite-(Ce). The mineral contains the elements potassium, cerium, and niobium. Using microscopes, chemical analyses, and X-ray measurements, the researchers determined its structure and properties. The study shows that this mineral records the formation of rare earth and niobium ores in geological processes, improving our understanding of how these important resources formed.
            </summary>
            <content type="html">
                &lt;b&gt;Xianhuaite-(Ce), K2CeNb5O15, a new niobium mineral from the Bayan Obo deposit, China&lt;/b&gt;&lt;br&gt;
                Bo Yang, Yuan Xue, Li Yang, Ningyue Sun, Guowu Li, Junfang Yu, Guoying Yan, Jianyong Liu, Yonggang Zhao, Wenxiang Meng, Zhenyu Chen, Lei Chen, Ze Liu, Zhao Yan, Xinyu Hou, Xin Ao, and Jinlong Wang&lt;br&gt;
                    Eur. J. Mineral., 38, 449&#8211;459, https://doi.org/10.5194/ejm-38-449-2026, 2026&lt;br&gt;
                <p>Xianhuaite-(Ce), K<span class="inline-formula"><sub>2</sub></span>CeNb<span class="inline-formula"><sub>5</sub></span>O<span class="inline-formula"><sub>15</sub></span>, is a new mineral species discovered in the Bayan Obo deposit, Inner Mongolia, China. The mineral is named in honor of Professor  Xianhua Li in recognition of his outstanding contributions to research on the Bayan Obo deposit. It occurs as brownish-red to pale yellow-brown tetragonal prisms or irregular granules and exhibits a Mohs hardness of 5&amp;#8211;6, an adamantine luster, and a calculated density of 5.23&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Electron microprobe analysis yields the empirical formula <span class="inline-formula"><sup><i>A</i>1</sup></span>(K<span class="inline-formula"><sub>1.30</sub></span>Ba<span class="inline-formula"><sub>0.69</sub></span>Sr<span class="inline-formula"><sub>0.02</sub></span>)<span class="inline-formula"><sub>&amp;#931;2.01</sub></span><span class="inline-formula"><sup><i>A</i>2</sup></span>(Ce<span class="inline-formula"><sub>0.39</sub></span>La<span class="inline-formula"><sub>0.31</sub></span>Nd<span class="inline-formula"><sub>0.04</sub></span>Pr<span class="inline-formula"><sub>0.02</sub></span>Ca<span class="inline-formula"><sub>0.15</sub></span>Na<span class="inline-formula"><sub>0.09</sub></span>)<span class="inline-formula"><sub>&amp;#931;1.00</sub></span><span class="inline-formula"><sup><i>B</i></sup></span>(Nb<span class="inline-formula"><sub>4.75</sub></span>Fe<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M26" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">0.13</mn><mrow><mn mathvariant="normal">3</mn><mo>+</mo></mrow></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="18pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="528342f61f50e33361fe8570cb52c79f"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-449-2026-ie00001.svg" width="18pt" height="17pt" src="ejm-38-449-2026-ie00001.png"/></svg:svg></span></span>Ti<span class="inline-formula"><sub>0.09</sub></span>Mg<span class="inline-formula"><sub>0.04</sub></span>)<span class="inline-formula"><sub>&amp;#931;5.01</sub></span>O<span class="inline-formula"><sub>15</sub></span>. Xianhuaite-(Ce) crystallizes in the tetragonal system, space group <span class="inline-formula"><i>P</i></span>4<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M32" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="5ea72e5fcd9e8768af40707a0416eed7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-449-2026-ie00002.svg" width="8pt" height="14pt" src="ejm-38-449-2026-ie00002.png"/></svg:svg></span></span><i>mbm</i>, with unit-cell parameters <span class="inline-formula"><i>a</i>=12.5355(4)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=3.9213(2)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=616.19(5)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=2</span>. Its crystal structure adopts a tetragonal tungsten bronze (TTB)-type framework, characterized by corner-sharing NbO<span class="inline-formula"><sub>6</sub></span&gt; octahedra forming channels hosting K, Ba, and rare earth element (REE) cations. Xianhuaite-(Ce) is associated with minerals typical of skarnization assemblages (e.g. dolomite, forsterite, phlogopite, and chlorite), as well as other Nb phases, including fersmite, columbite-(Fe), fergusonite-(Ce), and aeschynite. As the first naturally occurring mineral with a TTB-type structure, xianhuaite-(Ce) expands the known structural diversity of Nb minerals and provides new mineralogical constraints on Nb mineralization at Bayan Obo.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-21T22:15:55+02:00</published>
            <updated>2026-07-21T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-431-2026</id>
            <title type="html">Fluorine-induced melting in the Ihalainen calcite-wollastonite marble deposit, Lappeenranta, Finland
            </title>
            <link href="https://doi.org/10.5194/ejm-38-431-2026"/>
            <summary type="html">
                &lt;b&gt;Fluorine-induced melting in the Ihalainen calcite-wollastonite marble deposit, Lappeenranta, Finland&lt;/b&gt;&lt;br&gt;
                Robert F. Martin, Dirk Schumann, Markku J. Lehtinen, and Sebastian Fuchs&lt;br&gt;
                    Eur. J. Mineral., 38, 431&#8211;448, https://doi.org/10.5194/ejm-38-431-2026, 2026&lt;br&gt;
                The Ihalainen deposit in Finland produces wollastonite, a silicate of calcium. It formed 1.86 x 10<sup>9</sup&gt; years ago; 240 x 10<sup>6&amp;#160;</sup>years later, the area was invaded by a fluorine-rich granitic magma, which interacted with the marble host. The silicate magma lost silica and alkalis; the marble melted. A fluorine-rich vapor phase mobilized niobium, tantalum, and tin to form unknown minerals. The fluid was initially CO<sub>2</sub>-dominant and then became aqueous and formed a complex assemblage of alteration minerals.
            </summary>
            <content type="html">
                &lt;b&gt;Fluorine-induced melting in the Ihalainen calcite-wollastonite marble deposit, Lappeenranta, Finland&lt;/b&gt;&lt;br&gt;
                Robert F. Martin, Dirk Schumann, Markku J. Lehtinen, and Sebastian Fuchs&lt;br&gt;
                    Eur. J. Mineral., 38, 431&#8211;448, https://doi.org/10.5194/ejm-38-431-2026, 2026&lt;br&gt;
                <p>Located adjacent to Lappeenranta in southeastern Finland, the Ihalainen marble deposit has operated continuously since 1910. Regional metamorphism of the calcitic and dolomitic marble of the Ihalainen Formation led to wollastonite formation, well dated at 1.86&amp;#8201;Ga. At about 1.6&amp;#8201;Ga, the area experienced intrusion by the Wiborg batholith of anorogenic granite with a rapakivi texture. Dikes of granite, composite basic&amp;#8211;felsic dikes, and dikelets with an aplitic texture intruded into the wollastonite deposit, now part of a roof pendant, and caused localized fluxed melting of the ore. The gaseous transfer of CaF<span class="inline-formula"><sub>2</sub></span&gt; into the heated ore caused a very strange melt to form. It congealed quickly to forsterite, diopside, and graphically intergrown wollastonite&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;fluorite. Closer to the contact, an injection of geochemically evolved granitic melt induced anatexis of the marble. We investigated an emulsion of the two melts, one desilicated and now syenitic, the other a carbonate melt that contained dissolved silicates. The syenitic melt eventually crystallized to a sanidine solid-solution that underwent spinodal decomposition into two strained feldspars in the presence of a carbothermal fluid. A later influx of an aqueous fluid caused recrystallization of the feldspars but left intact the striking textural evidence of a once-coherent intergrowth. It also led to a bewildering array of calcic secondary minerals like pectolite, grosssular, holtstamite, and lawsomite. Three undescribed minerals in the affected rocks contain the high-field-strength elements Sn, Nb, and Ta.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-20T22:15:55+02:00</published>
            <updated>2026-07-20T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-419-2026</id>
            <title type="html">Mckelveyite group minerals &#8211; Part 5: Bainbridgeite-(NdCe), Na<sub>2</sub>Ba<sub>2</sub>NdCe(CO<sub>3</sub>)<sub>6</sub><span class="Radical">&#9679;</span>3H<sub>2</sub>O, a new neodymium and cerium-dominant species from Mont Saint-Hilaire, Canada
            </title>
            <link href="https://doi.org/10.5194/ejm-38-419-2026"/>
            <summary type="html">
                &lt;b&gt;Mckelveyite group minerals – Part 5: Bainbridgeite-(NdCe), Na2Ba2NdCe(CO3)6●3H2O, a new neodymium and cerium-dominant species from Mont Saint-Hilaire, Canada&lt;/b&gt;&lt;br&gt;
                Inna Lykova, Ralph Rowe, Glenn Poirier, Henrik Friis, Kelsie Ojaste, and Stephanie Barnes&lt;br&gt;
                    Eur. J. Mineral., 38, 419&#8211;429, https://doi.org/10.5194/ejm-38-419-2026, 2026&lt;br&gt;
                The paper describes bainbridgeite-(NdCe), Na<sub>2</sub>Ba<sub>2</sub>NdCe(CO<sub>3</sub>)<sub>6</sub>&amp;#8729;3H<sub>2</sub>O, from the famous Mont Saint-Hilaire complex, Quebec, Canada, the first known mineral with Ce and Nd atoms preferentially concentrated at two different sites of the structure
            </summary>
            <content type="html">
                &lt;b&gt;Mckelveyite group minerals – Part 5: Bainbridgeite-(NdCe), Na2Ba2NdCe(CO3)6●3H2O, a new neodymium and cerium-dominant species from Mont Saint-Hilaire, Canada&lt;/b&gt;&lt;br&gt;
                Inna Lykova, Ralph Rowe, Glenn Poirier, Henrik Friis, Kelsie Ojaste, and Stephanie Barnes&lt;br&gt;
                    Eur. J. Mineral., 38, 419&#8211;429, https://doi.org/10.5194/ejm-38-419-2026, 2026&lt;br&gt;
                <p>The new mckelveyite group mineral bainbridgeite-(NdCe), ideally Na<span class="inline-formula"><sub>2</sub></span>Ba<span class="inline-formula"><sub>2</sub></span>NdCe(CO<span class="inline-formula"><sub>3</sub>)<sub>6</sub></span>&amp;#9899;3H<span class="inline-formula"><sub>2</sub></span>O, was found at Mont Saint-Hilaire, Quebec, Canada. It occurs in two distinct environments: (1)&amp;#160;in a &amp;#8220;carbonate pegmatite&amp;#8221; as pale-yellow or orange barrel-shaped short prismatic crystals up to 2&amp;#8201;mm in size, where bainbridgeite-(NdCe) forms thin rims while the core is composed of bainbridgeite-(YCe), and (2)&amp;#160;in a hornfels rock as white or pale-grey tabular saucer-shaped crystals up to 0.5&amp;#8201;mm in size. It has a white streak, a vitreous lustre, and no cleavage. <span class="inline-formula"><i>D</i><sub>calc</sub></span&gt; is 3.49&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Bainbridgeite-(NdCe) is optically biaxial (<span class="inline-formula">+</span>), <span class="inline-formula"><i>&amp;#945;</i>=1.577(3)</span>, <span class="inline-formula"><i>&amp;#946;</i>=1.592(3)</span>, <span class="inline-formula"><i>&amp;#947;</i>=1.657(3)</span>, 2V (meas.)&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;40(3)&amp;#176;, and 2V (calc.)&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;52&amp;#176; (589&amp;#8201;nm). The IR spectrum is reported. The composition (wt.&amp;#8201;%, average of seven analyses) is Na<span class="inline-formula"><sub>2</sub></span>O 6.85, CaO 1.16, SrO 4.83, BaO 24.02, Y<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 1.84, La<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 6.07, Ce<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 8.82, Pr<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.76, Nd<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 6.24, Sm<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 3.34, Eu<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.46, Gd<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 2.74, Tb<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.21, Dy<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.53, ThO<span class="inline-formula"><sub>2</sub></span&gt; 0.24, CO<span class="inline-formula"><sub>2</sub></span&gt; 27.33, H<span class="inline-formula"><sub>2</sub></span>O 5.73, total 101.17. The empirical formula of the holotype from the &amp;#8220;carbonate pegmatite&amp;#8221; calculated on the basis of six cations is as follows: Na<span class="inline-formula"><sub>2.09</sub></span>Ca<span class="inline-formula"><sub>0.19</sub></span>Sr<span class="inline-formula"><sub>0.44</sub></span>Ba<span class="inline-formula"><sub>1.48</sub></span>Y<span class="inline-formula"><sub>0.15</sub></span>La<span class="inline-formula"><sub>0.35</sub></span>Ce<span class="inline-formula"><sub>0.51</sub></span>Pr<span class="inline-formula"><sub>0.04</sub></span>Nd<span class="inline-formula"><sub>0.35</sub></span>Sm<span class="inline-formula"><sub>0.18</sub></span>Eu<span class="inline-formula"><sub>0.03</sub></span>Gd<span class="inline-formula"><sub>0.14</sub></span>Tb<span class="inline-formula"><sub>0.01</sub></span>Dy<span class="inline-formula"><sub>0.03</sub></span>Th<span class="inline-formula"><sub>0.01</sub></span>(CO<span class="inline-formula"><sub>3</sub>)<sub>5.86</sub></span>(H<span class="inline-formula"><sub>2</sub></span>O)<span class="inline-formula"><sub>3.00</sub></span>. The mineral is triclinic, <span class="inline-formula"><i>P</i></span>1, <span class="inline-formula"><i>a</i>=9.0525(3)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>b</i>=9.1178(2)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=6.85180(19)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#945;</i>=102.575(3)</span>&amp;#176;, <span class="inline-formula"><i>&amp;#946;</i>=116.272(4)</span>&amp;#176;, <span class="inline-formula"><i>&amp;#947;</i>=59.788(4)</span>&amp;#176; and <span class="inline-formula"><i>V</i>=438.23(3)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=1</span>. The strongest reflections of the powder X-ray diffraction pattern [<span class="inline-formula"><i>d</i></span>, &amp;#197;(<span class="inline-formula"><i>I</i>)</span>(hkl)] are as follows: 6.17(50)(001, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M71" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="0cf1ac798004ce4c76220474f3acd5b0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00001.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00001.png"/></svg:svg></span></span>1, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M72" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="3d1aa4d7f73dd3d473d95803b1a12f5f"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00002.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00002.png"/></svg:svg></span></span>01), 4.407(100)(1<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M73" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="7c4360ab9d1e5298cf096d69758d039d"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00003.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00003.png"/></svg:svg></span></span>0, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M74" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="cce5d3ab2371bbc5752167e6acd1c117"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00004.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00004.png"/></svg:svg></span></span>1, 120), 4.077(30)(<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M75" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="279c9b3dba908204d9a32f2f42f2d13b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00005.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00005.png"/></svg:svg></span></span>1, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M76" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="29f766efd99b812d301d568e572a86c7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00006.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00006.png"/></svg:svg></span></span>11, 210), 3.241(32)(1<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M77" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="e3e9d0168f62bf5dbd4a9ac717c5b2eb"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00007.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00007.png"/></svg:svg></span></span>1, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M78" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="70165d2499111b4a6023ad935a87aa1d"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00008.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00008.png"/></svg:svg></span></span>2, 121), 2.870(88)(<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M79" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="f262588d20b021ec17262fd44f240a95"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00009.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00009.png"/></svg:svg></span></span>2, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M80" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">1</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="64f65e5d8a29ffb43b947a1719a515a9"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00010.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00010.png"/></svg:svg></span></span>12, 211), 2.621(39)(<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M81" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="954bcba428fc04affaafd25d5a53c5ee"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00011.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00011.png"/></svg:svg></span></span>01, 030, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M82" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="45b7facc27b55b42bbb99ec9c1afd6b2"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00012.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00012.png"/></svg:svg></span></span>1), 2.253(22)(<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M83" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="ea55ccfa03ced21dd86d878d6235b0a4"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00013.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00013.png"/></svg:svg></span></span>21, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M84" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">4</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="e3a0e297f1fe37a7f66fe5f6612d47bf"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00014.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00014.png"/></svg:svg></span></span>1, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M85" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">4</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">2</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="31e1e10153e26098a2de89f5ba0a9357"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00015.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00015.png"/></svg:svg></span></span>1), and 1.9978(25)(0<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M86" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="e3e0b0619af51b5db5da06ab5e41a3e3"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00016.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00016.png"/></svg:svg></span></span>2, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M87" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="14pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="87b79424395c73080c5209738d242184"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00017.svg" width="14pt" height="13pt" src="ejm-38-419-2026-ie00017.png"/></svg:svg></span></span>3, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M88" display="inline" overflow="scroll" dspmath="mathml"><mover accent="true"><mn mathvariant="normal">3</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="01b58ad75cba429c311c0c73ca774b9b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-419-2026-ie00018.svg" width="8pt" height="13pt" src="ejm-38-419-2026-ie00018.png"/></svg:svg></span></span>03, 301, 032, 331). The crystal structure, solved and refined from single-crystal X-ray diffraction data (<span class="inline-formula"><i>R</i><sub>1</sub>=0.036</span>), is of the weloganite type. Bainbridgeite-(NdCe) is the first known mineral with Ce and Nd atoms preferentially concentrated at two different sites of the structure.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-16T22:15:55+02:00</published>
            <updated>2026-07-16T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-397-2026</id>
            <title type="html">Hydrothermal quartz genesis revealed by the combination of SEM charge contrast maps, FTIR mapping, and LA-ICP-MS trace element geochemistry
            </title>
            <link href="https://doi.org/10.5194/ejm-38-397-2026"/>
            <summary type="html">
                &lt;b&gt;Hydrothermal quartz genesis revealed by the combination of SEM charge contrast maps, FTIR mapping, and LA-ICP-MS trace element geochemistry&lt;/b&gt;&lt;br&gt;
                Marko Bermanec, Nils B. Gies, Thomas Pettke, and Jörg Hermann&lt;br&gt;
                    Eur. J. Mineral., 38, 397&#8211;417, https://doi.org/10.5194/ejm-38-397-2026, 2026&lt;br&gt;
                We investigate how trace elements are incorporated into quartz formed in magmatic&amp;#8211;hydrothermal ore deposits, key environments for critical metal enrichment. By tracking Li, B, Al, Ti, and OH defects across crystal growth zones we reveal distinct trace element zonation patterns linked to temperature and pressure evolution during crystallization. We demonstrate that combined trace element data and mapping of quartz can be a powerful tool for understanding ore deposit genesis and prospecting ores.
            </summary>
            <content type="html">
                &lt;b&gt;Hydrothermal quartz genesis revealed by the combination of SEM charge contrast maps, FTIR mapping, and LA-ICP-MS trace element geochemistry&lt;/b&gt;&lt;br&gt;
                Marko Bermanec, Nils B. Gies, Thomas Pettke, and Jörg Hermann&lt;br&gt;
                    Eur. J. Mineral., 38, 397&#8211;417, https://doi.org/10.5194/ejm-38-397-2026, 2026&lt;br&gt;
                <p>Magmatic&amp;#8211;hydrothermal ore deposits, such as pegmatites, are an increasingly important source of metals and critical elements for the development of green-energy resources. The geochemical processes at the magmatic&amp;#8211;hydrothermal transition influence the degree of element enrichment in these ores. Quartz is a mineral that grows throughout the complete crystallization sequence of granitic pegmatites. Tracking the systematics of trace element incorporation into the quartz crystal structure throughout the magmatic&amp;#8211;hydrothermal pegmatite evolution may offer unprecedented insights into pegmatite genesis.</p&gt;        <p>Quartz crystals from the Rosina pegmatite, Elba, Italy, and from the Misox pegmatite, Ticino, Switzerland, were mapped using scanning electron microscopy (SEM) charge contrast imaging and Fourier transform infrared (FTIR) spectroscopy to determine the distribution of OH coupled to Li, B, and Al. Trace element laser ablation inductively coupled plasma mass spectroscopy (LA-ICP-MS) spot measurements were done on the same quartz crystals, navigated by the spatial distribution of zonation observed via FTIR maps. In Rosina quartz, total Li, B, Al, and Ti mass fractions are higher in the cores of the zoned crystals when compared to the rims, whereas in Misox quartz, the total Li, B, and Al increase from core to rim. In both Rosina and Misox quartz, OH coupled to Li, B, and Al closely follows the zonation of the total trace element contents. Lithium, B, and Al coupled to OH represent 5&amp;#8201;%&amp;#8211;30&amp;#8201;% of the coupled substitutions in quartz. Thus, OH-related point defects provide another tool for provenance and ore body prospecting studies. In Rosina quartz, the LiOH defect is dominant in the FTIR spectra, which is rare for quartz and only characteristic for evolved pegmatitic quartz crystals.</p&gt;        <p>Temperature estimates of quartz formation were constrained by Ti-in-quartz geothermometry, linking the observed geochemical processes to the pressure&amp;#8211;temperature conditions at which they took place. Rosina quartz formed at pressures of 2.3&amp;#8201;kbar and temperatures between 590 (core) and 330 (rim)&amp;#8201;&amp;#176;C, while Misox quartz formed at pressures of 5&amp;#8211;6&amp;#8201;kbar and temperatures between 520 (core) and 300 (rim)&amp;#8201;&amp;#176;C (calculated at TiO<span class="inline-formula"><sub>2</sub></span&gt; activity of 0.5). Relative temperatures consistently decrease from core to rim, and absolute temperatures are uncertain due to the difficulty of constraining the activity of Ti during quartz crystallization. The trace element evolution during quartz crystallization was spatially resolved and tracked through the complete quartz crystal growth period of the pegmatites. Trace elements in quartz crystals from Rosina record a prominent change in incorporation at the core&amp;#8211;rim transition, while the interpretation of quartz trace element patterns in Misox quartz is further complicated by twinning patterns. These results show that a combination of quartz FTIR and LA-ICP-MS analyses successfully constrains the changes in the geochemical environment during ore body formation. In particular, Li enrichment in combination with H<span class="inline-formula"><sub>2</sub></span>O contents in quartz might be useful in the study of detrital quartz when prospecting for Li-rich pegmatites or other economically significant magmatic&amp;#8211;hydrothermal ore deposits.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-13T22:15:55+02:00</published>
            <updated>2026-07-13T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-383-2026</id>
            <title type="html">Boron coordination in haplogranite glasses
            </title>
            <link href="https://doi.org/10.5194/ejm-38-383-2026"/>
            <summary type="html">
                &lt;b&gt;Boron coordination in haplogranite glasses&lt;/b&gt;&lt;br&gt;
                Jakob Rauscher, Michael Fechtelkord, Sandro Jahn, Julie A.-S. Michaud, Draupadi Mothan, Melanie J. Sieber, Robert B. Trumbull, Franziska D. H. Wilke, Max Wilke, and Bernd Wunder&lt;br&gt;
                    Eur. J. Mineral., 38, 383&#8211;396, https://doi.org/10.5194/ejm-38-383-2026, 2026&lt;br&gt;
                Boron and its isotopes, <sup>11</sup>B and <sup>10</sup>B, can track magmatic&amp;#8211;hydrothermal processes, but this requires knowing how the isotopes fractionate between melt and fluid, which depends on B coordination. This is known for aqueous fluids but not for silicate melts. We determined B coordination by nuclear magnetic resonance in granitic glass with variable water content and alkali&amp;#8211;alumina ratios. The results provide a way to estimate B coordination and melt&amp;#8211;fluid fractionation for variable melt compositions.
            </summary>
            <content type="html">
                &lt;b&gt;Boron coordination in haplogranite glasses&lt;/b&gt;&lt;br&gt;
                Jakob Rauscher, Michael Fechtelkord, Sandro Jahn, Julie A.-S. Michaud, Draupadi Mothan, Melanie J. Sieber, Robert B. Trumbull, Franziska D. H. Wilke, Max Wilke, and Bernd Wunder&lt;br&gt;
                    Eur. J. Mineral., 38, 383&#8211;396, https://doi.org/10.5194/ejm-38-383-2026, 2026&lt;br&gt;
                <p>The coordination of boron in silicate melts has been extensively studied in synthetic industrial glasses but rarely in natural volcanic glasses or their synthetic analogues. Because coordination is a controlling factor in the boron isotope exchange between melts and coexisting phases, it is important to close this knowledge gap. We synthesized a set of boron-rich (2&amp;#8201;wt&amp;#8201;% and 5&amp;#8201;wt&amp;#8201;% B<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span>) haplogranite glasses with water content from 0&amp;#8201;wt&amp;#8201;% to 7&amp;#8201;wt&amp;#8201;% and a variable alumina&amp;#8211;alkali ratio, expressed by the aluminum saturation index (ASI), the molar ratio of Al<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span>&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="93e47eb16cb371fe6916d3191efc4f1d"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-383-2026-ie00001.svg" width="8pt" height="14pt" src="ejm-38-383-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;(CaO&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;Na<span class="inline-formula"><sub>2</sub></span>O&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;K<span class="inline-formula"><sub>2</sub></span>O). Boron coordination was determined by <span class="inline-formula"><sup>11</sup></span>B MAS-NMR analyses and is expressed as <span class="inline-formula"><i>R</i></span>(IVB), the ratio of tetrahedral (BO<span class="inline-formula"><sub>4</sub></span>) to tetrahedral and trigonal (BO<span class="inline-formula"><sub>3</sub></span>) groups.</p&gt;        <p>There is a first-order dependency of boron coordination on the ASI ratio within the studied range of 0.8 to 1.7. All glasses with ASI&amp;#8201;<span class="inline-formula"><i>></i></span>&amp;#8201;1.1 showed nearly exclusive trigonal boron regardless of water and boron concentration. The maximum value of <span class="inline-formula"><i>R</i></span>(IVB) was 7&amp;#8201;%. Glasses with lower ASI values showed a steady increase in <span class="inline-formula"><i>R</i></span>(IVB) up to 90&amp;#8201;% in a sample with ASI&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;0.8. High water contents may favor formation of BO<span class="inline-formula"><sub>4</sub></span&gt; groups as suggested by other glass studies, but there are masking effects related to the quench rates that make this trend inconclusive.</p&gt;        <p>Our results concur with the few existing NMR studies of natural glasses that boron is dominantly in trigonal coordination in peraluminous melts. The trigonal coordination of boron as B(OH)<span class="inline-formula"><sub>3</sub></span&gt; in neutral to acidic aqueous fluids means that there should be little if any fractionation of boron isotopes between a granitic melt and exsolved fluid if the granite is peraluminous. For granites with ASI&amp;#8201;<span class="inline-formula"><i><</i>1.1</span>, the ratio <span class="inline-formula"><i>R</i></span>(IVB) and thus the B-isotope fractionation are expected to strongly increase. We present a predictive model based on ab initio fractionation factors that links <span class="inline-formula">&amp;#916;<sup>11</sup></span>B<span class="inline-formula"><sub>melt&amp;#8211;fluid</sub></span&gt; with ASI in the melt, which suggests a fractionation of <span class="inline-formula">&amp;#8722;</span>4&amp;#8201;&amp;#8240; to <span class="inline-formula">&amp;#8722;</span>7&amp;#8201;&amp;#8240; at 730 and 530&amp;#8201;&amp;#176;C, respectively, for a granite with ASI&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;0.8.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-09T22:15:55+02:00</published>
            <updated>2026-07-09T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-373-2026</id>
            <title type="html">Yttrotungstite-(Nd), a new mineral species from the Nyakabingo tungsten mine, Kigali, Rwanda
            </title>
            <link href="https://doi.org/10.5194/ejm-38-373-2026"/>
            <summary type="html">
                &lt;b&gt;Yttrotungstite-(Nd), a new mineral species from the Nyakabingo tungsten mine, Kigali, Rwanda&lt;/b&gt;&lt;br&gt;
                Frédéric Hatert, Simon Philippo, Pietro Vignola, and Maël Guennou&lt;br&gt;
                    Eur. J. Mineral., 38, 373&#8211;382, https://doi.org/10.5194/ejm-38-373-2026, 2026&lt;br&gt;
                Yttrotungstite-(Nd) is a new mineral species discovered in the Nyakabingo tungsten mine, Kigali, Rwanda. The mineral occurs in the oxidized zones of the deposit, where it forms tiny yellow-orange tabular crystals that reach a length of maximum of 100 &amp;#181;m, and frequently form radiated groups. The dominant form is {010}, and a twinning has been observed parallel to (001). Electron microprobe analyses and structural data, confirming that the species belongs to the yttrotungstite group.
            </summary>
            <content type="html">
                &lt;b&gt;Yttrotungstite-(Nd), a new mineral species from the Nyakabingo tungsten mine, Kigali, Rwanda&lt;/b&gt;&lt;br&gt;
                Frédéric Hatert, Simon Philippo, Pietro Vignola, and Maël Guennou&lt;br&gt;
                    Eur. J. Mineral., 38, 373&#8211;382, https://doi.org/10.5194/ejm-38-373-2026, 2026&lt;br&gt;
                <p>Yttrotungstite-(Nd), NdW<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>7</sub></span>(OH)(H<span class="inline-formula"><sub>2</sub></span>O), is a new mineral species discovered in the Nyakabingo tungsten mine, Kigali, Rwanda. The mineral occurs in the oxidized zones of the deposit, where it forms tiny yellow-orange tabular crystals associated with anthoinite and hydrokenoelsmoreite. The crystals are transparent, reach a length of a maximum of 100&amp;#8201;<span class="inline-formula">&amp;#181;</span>m, and frequently form radiated groups. The dominant form is {010}, and a twinning has been observed parallel to (001). The streak of yttrotungstite-(Nd) is white, the lustre is vitreous, and the mineral is non-fluorescent. The Mohs hardness is 1; the tenacity is brittle; and observed cleavage planes are (010) perfect and (100) and (001) excellent. The calculated density is 6.25&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>, and refraction indices are <span class="inline-formula"><i>&amp;#945;</i>=</span>&amp;#8201;1.90(2) and <span class="inline-formula"><i>&amp;#947;</i>=</span>&amp;#8201;2.10(2). The mineral is optically biaxial, its optical plane is parallel to (010), and the optical orientation is <span class="inline-formula"><i>X</i></span>&amp;#8201;<span class="inline-formula">&amp;#8743;</span>&amp;#8201;<span class="inline-formula"><i>c</i></span>&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;6&amp;#176; and <span class="inline-formula"><i>Z</i></span>&amp;#8201;<span class="inline-formula">&amp;#8743;</span>&amp;#8201;<span class="inline-formula"><i>a</i></span>&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;9&amp;#176;. Pleochroism is from light yellow (<span class="inline-formula"><i>X</i></span>) to yellow (<span class="inline-formula"><i>Z</i></span>). The empirical formula of yttrotungstite-(Nd), calculated on the basis of 15 positive charges assuming 1 (OH) group and 1 H<span class="inline-formula"><sub>2</sub></span>O molecule per formula unit, corresponds to the following: (Nd<span class="inline-formula"><sub>0.36</sub></span>Sm<span class="inline-formula"><sub>0.13</sub></span>Ce<span class="inline-formula"><sub>0.12</sub></span>Pr<span class="inline-formula"><sub>0.08</sub></span>La<span class="inline-formula"><sub>0.06</sub></span>Gd<span class="inline-formula"><sub>0.06</sub></span>Y<span class="inline-formula"><sub>0.05</sub></span>Dy<span class="inline-formula"><sub>0.03</sub></span>Yb<span class="inline-formula"><sub>0.02</sub></span>Ca<span class="inline-formula"><sub>0.01</sub></span>)<span class="inline-formula"><sub>&amp;#931;0.92</sub></span>(W<span class="inline-formula"><sub>2.02</sub></span>P<span class="inline-formula"><sub>0.02</sub></span>)<span class="inline-formula"><sub>&amp;#931;2.04</sub></span>O<span class="inline-formula"><sub>7</sub></span>(OH)(H<span class="inline-formula"><sub>2</sub></span>O). The crystal structure was refined in space group <span class="inline-formula"><i>P</i></span>2<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M36" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mn mathvariant="normal">1</mn></msub><mo>/</mo><mi>m</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="23pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="d019fe20974810df04b4a93db0b94079"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-373-2026-ie00001.svg" width="23pt" height="14pt" src="ejm-38-373-2026-ie00001.png"/></svg:svg></span></span&gt; to the final R1 value of 0.0362, and the measured unit-cell parameters are <span class="inline-formula"><i>a</i>=</span>&amp;#8201;5.8534(3), <span class="inline-formula"><i>b</i>=</span>&amp;#8201;8.6881(3), <span class="inline-formula"><i>c</i>=</span>&amp;#8201;7.0488(4)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#946;</i>=</span>&amp;#8201;105.336(5)&amp;#176;, and <span class="inline-formula"><i>V</i>=</span>&amp;#8201;345.70(3)&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>. The structure of yttrotungstite-(Nd) is characterized by edge-sharing WO<span class="inline-formula"><sub>6</sub></span&gt; octahedra, forming kinked chains parallel to the <span class="inline-formula"><i>b</i></span&gt; axis. The NdO<span class="inline-formula"><sub>8</sub></span&gt; complex polyhedra connect three chains together by sharing edges or corners with adjacent WO<span class="inline-formula"><sub>6</sub></span&gt; octahedra. A view perpendicular to the <span class="inline-formula"><i>b</i></span&gt; axis shows that the NdO<span class="inline-formula"><sub>8</sub></span&gt; and WO<span class="inline-formula"><sub>6</sub></span&gt; polyhedra occur in two different types of planes, stacked parallel to the [<span class="inline-formula">&amp;#8722;</span>101] direction. Neodymium occurs in a very large eight-coordinated site, which can be described as two tetragonal pyramids sharing one common basal edge and sharing the opposite basal edge with a square. Calculated bond-valence sums are discussed in detail, as well as the Raman spectral results. The species and its name were approved by the Commission on New Minerals, Nomenclature and Classification of the International Mineralogical Association under number IMA 2023-064; its abbreviation is &amp;#8220;Ytgs-Nd&amp;#8221;.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-07-07T22:15:55+02:00</published>
            <updated>2026-07-07T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-353-2026</id>
            <title type="html">Dehydration reactions in guano-derived minerals: the taranakite-to-francoanellite transformation
            </title>
            <link href="https://doi.org/10.5194/ejm-38-353-2026"/>
            <summary type="html">
                &lt;b&gt;Dehydration reactions in guano-derived minerals: the taranakite-to-francoanellite transformation&lt;/b&gt;&lt;br&gt;
                Yuri Galliano, Nicola Campomenosi, Fabio Bellatreccia, Donato Belmonte, Jo De Waele, and Cristina Carbone&lt;br&gt;
                    Eur. J. Mineral., 38, 353&#8211;372, https://doi.org/10.5194/ejm-38-353-2026, 2026&lt;br&gt;
                Deposits of bat guano in cave environments host diverse assemblages of secondary minerals, which can go through partial dehydration processes in response to varying environmental conditions. In this article, we investigate the thermodynamics and kinetics which lead guano-derived taranakite to lose part of its structural water and transform into francoanellite. Our results allow us to present evidence-based hypotheses to explain the occurrence of the latter in natural environments.
            </summary>
            <content type="html">
                &lt;b&gt;Dehydration reactions in guano-derived minerals: the taranakite-to-francoanellite transformation&lt;/b&gt;&lt;br&gt;
                Yuri Galliano, Nicola Campomenosi, Fabio Bellatreccia, Donato Belmonte, Jo De Waele, and Cristina Carbone&lt;br&gt;
                    Eur. J. Mineral., 38, 353&#8211;372, https://doi.org/10.5194/ejm-38-353-2026, 2026&lt;br&gt;
                <p>Bat guano deposits in caves host diverse assemblages of authigenic phosphates and sulfates. Previous field observations have proposed that some of them (e.g. brushite, gypsum, taranakite) can be subject to dehydration reactions as a response to varying environmental conditions. To evaluate the thermodynamic and kinetic constrains that regulate the dehydration reaction leading guano-derived taranakite (K<span class="inline-formula"><sub>3</sub></span>Al<span class="inline-formula"><sub>5</sub></span>(PO<span class="inline-formula"><sub>3</sub></span>OH)<span class="inline-formula"><sub>6</sub></span>(PO<span class="inline-formula"><sub>4</sub></span>)<span class="inline-formula"><sub>2</sub></span>&amp;#8201;<span class="inline-formula">&amp;#8901;</span>&amp;#8201;18H<span class="inline-formula"><sub>2</sub></span>O) to transform into francoanellite (K<span class="inline-formula"><sub>3</sub></span>Al<span class="inline-formula"><sub>5</sub></span>(PO<span class="inline-formula"><sub>3</sub></span>OH)<span class="inline-formula"><sub>6</sub></span>(PO<span class="inline-formula"><sub>4</sub></span>)<span class="inline-formula"><sub>2</sub></span>&amp;#8201;<span class="inline-formula">&amp;#8901;</span>&amp;#8201;12H<span class="inline-formula"><sub>2</sub></span>O), we conducted a multi-analytical in situ investigation consisting of temperature-resolved X-ray powder diffraction, Fourier transform infrared, and micro-Raman spectroscopy on a sample of taranakite. Thermodynamic calculations were also performed by means of the polyhedral approach to predict the phase transformation temperature at equilibrium, estimated to be 369.12&amp;#8201;K (95.97&amp;#8201;&amp;#176;C). Laboratory experiments conducted under increasing temperature conditions confirmed that the breaking of weak hydrogen bonds between interlayer water molecules and the aluminophosphate layers of taranakite is responsible for the onset of the dehydration reaction. Monitoring the evolution of the phosphate-stretching Raman peaks over time under isothermal conditions enabled us to estimate the activation energy of the process to be 7.6&amp;#8201;<span class="inline-formula">&amp;#177;</span>&amp;#8201;0.7&amp;#8201;kJ&amp;#8201;mol<span class="inline-formula"><sup>&amp;#8722;1</sup></span&gt; by means of the &amp;#8220;time to a given fraction&amp;#8221; method. The release of heat concomitant to the oxidation of organic matter in guano-admixed cave sediments is proposed as a viable trigger for the transformation, given the low kinetic barrier associated with it.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-22T22:15:55+02:00</published>
            <updated>2026-06-22T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-347-2026</id>
            <title type="html">IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) &#8211; Newsletter 91
            </title>
            <link href="https://doi.org/10.5194/ejm-38-347-2026"/>
            <content type="html">
                &lt;b&gt;IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) – Newsletter 91&lt;/b&gt;&lt;br&gt;
                Ferdinando Bosi, Frédéric Hatert, Marco Pasero, and Stuart J. Mills&lt;br&gt;
                    Eur. J. Mineral., 38, 347&#8211;352, https://doi.org/10.5194/ejm-38-347-2026, 2026&lt;br&gt;
                
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-19T22:15:55+02:00</published>
            <updated>2026-06-19T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-337-2026</id>
            <title type="html">Piilonenite-(Nd), NaNd(CO<sub>3</sub>)<sub>2</sub>&#8201;&#8901;&#8201;3H<sub>2</sub>O, a new neodymium-dominant carbonate mineral from Mont Saint-Hilaire, Quebec, Canada
            </title>
            <link href="https://doi.org/10.5194/ejm-38-337-2026"/>
            <summary type="html">
                &lt;b&gt;Piilonenite-(Nd), NaNd(CO3)2 ⋅ 3H2O, a new neodymium-dominant carbonate mineral from Mont Saint-Hilaire, Quebec, Canada&lt;/b&gt;&lt;br&gt;
                Inna Lykova, Ralph Rowe, Simon J. Teat, Glenn Poirier, and Stephanie Barnes&lt;br&gt;
                    Eur. J. Mineral., 38, 337&#8211;345, https://doi.org/10.5194/ejm-38-337-2026, 2026&lt;br&gt;
                The paper is on the new mineral species piilonenite-(Nd), a new Nd-dominate carbonate with no closely related minerals or synthetic compounds from Mont Saint-Hillarie, Canada.
            </summary>
            <content type="html">
                &lt;b&gt;Piilonenite-(Nd), NaNd(CO3)2 ⋅ 3H2O, a new neodymium-dominant carbonate mineral from Mont Saint-Hilaire, Quebec, Canada&lt;/b&gt;&lt;br&gt;
                Inna Lykova, Ralph Rowe, Simon J. Teat, Glenn Poirier, and Stephanie Barnes&lt;br&gt;
                    Eur. J. Mineral., 38, 337&#8211;345, https://doi.org/10.5194/ejm-38-337-2026, 2026&lt;br&gt;
                <p>The new mineral piilonenite-(Nd), ideally NaNd(CO<span class="inline-formula"><sub>3</sub>)<sub>2</sub>&amp;#8901;</span>3H<span class="inline-formula"><sub>2</sub></span>O, was found at Mont Saint-Hilaire, Quebec, Canada, in apophyses of the Poudrette pegmatite. It occurs as thin, bladed crystals up to 600&amp;#8201;<span class="inline-formula">&amp;#181;m</span&gt; in size. Piilonenite-(Nd) is colourless or white. The streak is white; the lustre is vitreous. Cleavage is perfect on {010}. <span class="inline-formula"><i>D</i><sub>calc</sub></span&gt; is 3.21&amp;#8201;<span class="inline-formula">g&amp;#8201;cm<sup>&amp;#8722;3</sup></span>. Piilonenite-(Nd) is optically biaxial (<span class="inline-formula">+</span>), <span class="inline-formula"><i>&amp;#945;</i>=1.546(3)</span>, <span class="inline-formula"><i>&amp;#946;</i>=1.616(3)</span>, <span class="inline-formula"><i>&amp;#947;</i>=1.638(3)</span>, 2&amp;#8201;V (meas.)&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;56(3)&amp;#176;, and 2&amp;#8201;V (calc.)&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;56&amp;#176; (589&amp;#8201;nm). The composition (wt.&amp;#8201;%, average of seven analyses) is Na<span class="inline-formula"><sub>2</sub></span>O 9.29, Y<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 1.71, La<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.93, Ce<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 8.32, Pr<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 2.75, Nd<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 23.90, Sm<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 6.85, Eu<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.27, Gd<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 3.64, Tb<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.12, Dy<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.90, Ho<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.13, Er<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.12, Tm<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span&gt; 0.07, CO<span class="inline-formula"><sub>2</sub></span&gt; 26.32, H<span class="inline-formula"><sub>2</sub></span>O 16.16, total 101.48. The empirical formula of the holotype calculated on the basis of two cations is as follows: Na<span class="inline-formula"><sub>1.00</sub></span>(Nd<span class="inline-formula"><sub>0.48</sub></span>Ce<span class="inline-formula"><sub>0.17</sub></span>Sm<span class="inline-formula"><sub>0.13</sub></span>Gd<span class="inline-formula"><sub>0.07</sub></span>Pr<span class="inline-formula"><sub>0.06</sub></span>Y<span class="inline-formula"><sub>0.05</sub></span>La<span class="inline-formula"><sub>0.02</sub></span>Dy<span class="inline-formula"><sub>0.02</sub>)<sub>&amp;#8721;1.00</sub></span>(CO<span class="inline-formula"><sub>3</sub>)<sub>2</sub></span>(H<span class="inline-formula"><sub>2</sub></span>O)<span class="inline-formula"><sub>3</sub></span>. The IR spectrum shows IR bands of O&amp;#8211;H-stretching and H&amp;#8211;O&amp;#8211;H bending vibrations of H<span class="inline-formula"><sub>2</sub></span>O molecules and C&amp;#8211;O-stretching vibrations of CO<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M56" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">3</mn><mrow><mn mathvariant="normal">2</mn><mo>-</mo></mrow></msubsup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="13pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="75356ac7c53216886a905fbbf1906906"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-337-2026-ie00001.svg" width="13pt" height="17pt" src="ejm-38-337-2026-ie00001.png"/></svg:svg></span></span>-group molecules. The mineral is orthorhombic, <span class="inline-formula"><i>P</i></span>2<span class="inline-formula"><sub>1</sub></span>2<span class="inline-formula"><sub>1</sub></span>2<span class="inline-formula"><sub>1</sub></span>, <span class="inline-formula"><i>a</i>=6.7914(11)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>b</i>=17.135(3)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=6.4360(10)</span>&amp;#8201;&amp;#197;, and <span class="inline-formula"><i>V</i>=749.0(2)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span&gt; and <span class="inline-formula"><i>Z</i>=4</span>. The strongest reflections of the powder X-ray diffraction pattern [<span class="inline-formula"><i>d</i></span>,&amp;#197;(<span class="inline-formula"><i>I</i>)</span>(hkl)] are as follows: 8.59(100)(020), 4.690(14)(101), 4.291(30)(040), 3.417(10)(200), and 3.175(17)(012, 220, 141). The crystal structure, solved and refined from synchrotron data (<span class="inline-formula"><i>R</i><sub>1</sub>=0.092</span>), is unique. There are two alternating layers: (1)&amp;#160;vertex-sharing Nd-centred polyhedra and &amp;#8220;flat-lying&amp;#8221; carbonate (CO<span class="inline-formula"><sub>3</sub>)<sup>2&amp;#8722;</sup></span&gt; groups and (2)&amp;#160;chains of vertex-sharing Na-centred polyhedra parallel to (100) and &amp;#8220;standing-on-edge&amp;#8221; carbonate (CO<span class="inline-formula"><sub>3</sub>)<sup>2&amp;#8722;</sup></span&gt; groups.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-19T22:15:55+02:00</published>
            <updated>2026-06-19T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-325-2026</id>
            <title type="html">Argentotennantite-(Fe), Ag<sub>6</sub>(Cu<sub>4</sub>Fe<sub>2</sub>)As<sub>4</sub>S<sub>13</sub>, a new member of the tetrahedrite group from the San Genaro mine, Peru: occurrence and crystal structure
            </title>
            <link href="https://doi.org/10.5194/ejm-38-325-2026"/>
            <summary type="html">
                &lt;b&gt;Argentotennantite-(Fe), Ag6(Cu4Fe2)As4S13, a new member of the tetrahedrite group from the San Genaro mine, Peru: occurrence and crystal structure&lt;/b&gt;&lt;br&gt;
                Jiří Sejkora, Dalibor Velebil, Cristian Biagioni, Zdeněk Dolníček, and Jaroslav Hyršl&lt;br&gt;
                    Eur. J. Mineral., 38, 325&#8211;336, https://doi.org/10.5194/ejm-38-325-2026, 2026&lt;br&gt;
                Argentotennantite-(Fe), ideally Ag<sub>6</sub>(Cu<sub>4</sub>Fe<sub>2</sub>)As<sub>4</sub>S<sub>13</sub>, is a new member of the tetrahedrite group found in the San Genaro mine, Castrovirreyna Province, Huancavelica, Peru. It occurs as anhedral grains up to 100 &amp;#956;m in size, or, more commonly, it forms micrometer-sized rims around crystals of argentotetrahedrite-(Zn) or replaces the latter around cavities and fissures, along with Ag-rich tennantite-(Fe). It is cubic, <em>I</em>3<em>m</em>, with <em>a</em&gt; = 10.4365(5) &amp;#197;, <em>V</em&gt; = 1136.75(17) &amp;#197;<sup>3</sup>.
            </summary>
            <content type="html">
                &lt;b&gt;Argentotennantite-(Fe), Ag6(Cu4Fe2)As4S13, a new member of the tetrahedrite group from the San Genaro mine, Peru: occurrence and crystal structure&lt;/b&gt;&lt;br&gt;
                Jiří Sejkora, Dalibor Velebil, Cristian Biagioni, Zdeněk Dolníček, and Jaroslav Hyršl&lt;br&gt;
                    Eur. J. Mineral., 38, 325&#8211;336, https://doi.org/10.5194/ejm-38-325-2026, 2026&lt;br&gt;
                <p>Argentotennantite-(Fe), Ag<span class="inline-formula"><sub>6</sub></span>(Cu<span class="inline-formula"><sub>4</sub></span>Fe<span class="inline-formula"><sub>2</sub></span>)As<span class="inline-formula"><sub>4</sub></span>S<span class="inline-formula"><sub>13</sub></span>, has been approved as a new mineral species (IMA 2023-126) by the Commission on New Minerals, Nomenclature and Classification of the International Mineralogical Association (CNMNC-IMA) using a sample of quartz gangue with argentotetrahedrite-(Zn), pyrargyrite, baryte, and siderite from the San Genaro mine, Castrovirreyna Province, Huancavelica, Peru. Argentotennantite-(Fe) occurs as anhedral grains up to 100&amp;#8201;<span class="inline-formula">&amp;#181;m</span&gt; in size. More commonly, it forms micrometer-sized rims around crystals of argentotetrahedrite-(Zn) or replaces the latter around cavities and fissures, along with Ag-rich tennantite-(Fe). Argentotennantite-(Fe) is opaque and dark gray in color, with a metallic luster and black streak. In reflected light, it is isotropic and pale gray, with a brownish shade. The reflectance values for wavelengths recommended by the Commission on Ore Mineralogy of the IMA, measured in air, are as follows [<span class="inline-formula"><i>&amp;#955;</i></span&gt; (nm, <span class="inline-formula"><i>R</i></span&gt; (%)]: 470, 29.9; 546, 30.1; 589, 29.8; and 650, 28.9. The chemical formula of the grain used for the crystal structure study, recalculated on the basis of <span class="inline-formula">&amp;#931;</span><i>Me</i>&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;16 atoms per formula unit, is (Ag<span class="inline-formula"><sub>3.36</sub></span>Cu<span class="inline-formula"><sub>2.70</sub>)<sub>&amp;#931;6.06</sub></span>(Cu<span class="inline-formula"><sub>4.05</sub></span>Fe<span class="inline-formula"><sub>1.88</sub></span>Zn<span class="inline-formula"><sub>0.07</sub>)<sub>&amp;#931;6.00</sub></span>(As<span class="inline-formula"><sub>2.29</sub></span>Sb<span class="inline-formula"><sub>1.66</sub>)<sub>&amp;#931;3.95</sub></span>S<span class="inline-formula"><sub>12.82</sub></span>. Argentotennantite-(Fe) is cubic, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M24" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>I</mi><mover accent="true"><mn mathvariant="normal">4</mn><mo mathvariant="normal">&amp;#8254;</mo></mover></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="12pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="783fcf64256a241cdc07014ed8f6a5c3"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-325-2026-ie00001.svg" width="12pt" height="13pt" src="ejm-38-325-2026-ie00001.png"/></svg:svg></span></span>3<span class="inline-formula"><i>m</i></span>, with <span class="inline-formula"><i>a</i>=10.4365(5)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=1136.75(17)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=2</span>. Its crystal structure has been refined by single-crystal X-ray diffraction data to a final <span class="inline-formula"><i>R</i><sub>1</sub>=0.0384</span&gt; on the basis of 246 unique reflections with <span class="inline-formula"><i>F</i>>4<i>&amp;#963;</i><sub><i>F</i></sub></span&gt; and 20 refined parameters. Argentotennantite-(Fe) is isotypic with other members of the tetrahedrite group. Structural relationships between argentotennantite-(Fe) and selected members of the tetrahedrite-group minerals are discussed, and previous findings relating to this species are briefly reviewed.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-06-11T22:15:55+02:00</published>
            <updated>2026-06-11T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-305-2026</id>
            <title type="html">Formation of black opal in the pegmatites from Volyn (Ukraine) &#8211; an example for interaction of silica with organic matter
            </title>
            <link href="https://doi.org/10.5194/ejm-38-305-2026"/>
            <summary type="html">
                &lt;b&gt;Formation of black opal in the pegmatites from Volyn (Ukraine) – an example for interaction of silica with organic matter&lt;/b&gt;&lt;br&gt;
                Gerhard Franz, Vladimir Khomenko, Vsevolod Chornousenko, Armin Zeh, Ferry Schiperski, Simon Gouzy, Ulrich Gernert, and Jörg Nissen&lt;br&gt;
                    Eur. J. Mineral., 38, 305&#8211;324, https://doi.org/10.5194/ejm-38-305-2026, 2026&lt;br&gt;
                Black opal, a rare&amp;#160;amorphous SiO<sub>2 </sub>variety, results from the interaction of silica with organic matter and therefore hints at traces of life, including the early Earth and Mars. The Volyn occurrence is one of the few examples of black opal worldwide and is the unique case of a pegmatitic occurrence in a granite; its age is at least 200 Ma. The structure consists of micrometer-large sphere-like arrangements of nano-sized grains and shows shape relicts of fossils, known from Volyn as "kerite".
            </summary>
            <content type="html">
                &lt;b&gt;Formation of black opal in the pegmatites from Volyn (Ukraine) – an example for interaction of silica with organic matter&lt;/b&gt;&lt;br&gt;
                Gerhard Franz, Vladimir Khomenko, Vsevolod Chornousenko, Armin Zeh, Ferry Schiperski, Simon Gouzy, Ulrich Gernert, and Jörg Nissen&lt;br&gt;
                    Eur. J. Mineral., 38, 305&#8211;324, https://doi.org/10.5194/ejm-38-305-2026, 2026&lt;br&gt;
                <p>Black opal, a variety of opal pigmented by organic matter, from Volyn, western Ukrainian Shield, was investigated by means of scanning electron microscopy (SEM), electron microprobe analyses (EMPAs), <span class="inline-formula"><i>&amp;#956;</i></span>-X-ray fluorescence (<span class="inline-formula"><i>&amp;#956;</i></span>XRF) element mapping, X-ray diffraction (XRD), and Fourier transformed infrared (FTIR) spectroscopy, and was dated by U-Pb by laser ablation (LA-ICP-SF-MS). Opal occurs as several centimeter large blocks and as cement in a breccia within pegmatites, which intruded into granites of the ca. 1.7&amp;#8211;1.8&amp;#8201;Ga old Korosten pluton. Opal samples were collected underground in miarolitic cavities of the pegmatites, which also host kerite, fossilized organic material (called Volyn biota). Inclusions in opal are typical pegmatitic minerals such as alkali-feldspar, Li-mica, and quartz. Buddingtonite and ammonium-bearing muscovite, as well as shape relicts of the fossils in opal, indicate interactions of organic material with the pegmatite.</p&gt;        <p>The XRD data indicate opal-CT with a complex pattern of the <span class="inline-formula">&amp;#8764;</span>&amp;#8201;4&amp;#8201;&amp;#197; peak. Its microstructure, as seen in SEM and back-scattered electron maps, consists of nanograins 15&amp;#8211;35&amp;#8201;nm in size, arranged in sphere-like structures, in some samples <span class="inline-formula">&amp;#8764;</span>&amp;#8201;5&amp;#8201;<span class="inline-formula">&amp;#181;</span>m-large and monodisperse, in others polydisperse with diameters of between 1 and 10&amp;#8201;<span class="inline-formula">&amp;#181;</span>m, and as lepispheres. Organic matter plus water makes up <span class="inline-formula">&amp;#8764;</span>&amp;#8201;10&amp;#8201;wt&amp;#8201;%&amp;#8211;15&amp;#8201;wt&amp;#8201;%. The organic matter is situated within the core, in concentric zones in the sphere-like structures and in the matrix around them. Infrared (IR) spectra confirm the presence of silanol SiOH and CH<span class="inline-formula"><sub><i>n</i></sub></span>. At the contact with pegmatitic material, a pyrite-enriched zone was observed and interpreted as resulting from the infiltration of a late Fe- and Mn-bearing fluid along grain boundaries.</p&gt;        <p>Results of U-Pb dating yield a minimum age for opal formation of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;200&amp;#8201;Ma, and provide evidence for fluid overprint during the Jurassic (170&amp;#8211;155&amp;#8201;Ma) and Quaternary. These ages are much older than reported so far in opal from deposits worldwide. Furthermore, the here-reported occurrence of opal in pegmatitic rocks is unique, as all other opal deposits are either sedimentary or volcanic hosted.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-22T22:15:55+02:00</published>
            <updated>2026-05-22T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-281-2026</id>
            <title type="html">Mineralogy of sulfide mineralization from the world-class Li&#8211;Sn&#8211;W C&#237;novec greisen-type deposit, Bohemian Massif, Czech Republic
            </title>
            <link href="https://doi.org/10.5194/ejm-38-281-2026"/>
            <summary type="html">
                &lt;b&gt;Mineralogy of sulfide mineralization from the world-class Li–Sn–W Cínovec greisen-type deposit, Bohemian Massif, Czech Republic&lt;/b&gt;&lt;br&gt;
                Ondřej Krátký, Jan Cempírek, Sebastián Hreus, Luboš Vrtiška, Jiří Sejkora, Zdeněk Dolníček, Jakub Výravský, Radek Škoda, Karel Breiter, and Vojtěch Šešulka&lt;br&gt;
                    Eur. J. Mineral., 38, 281&#8211;304, https://doi.org/10.5194/ejm-38-281-2026, 2026&lt;br&gt;
                Mineralogical, paragenetic, and geochemical data on sulfidic mineralization from the C&amp;#237;novec greisen-type deposit show that distribution of sulfides is irregular and not strictly bound to prevalent Li&amp;#8211;Sn&amp;#8211;W mineralization. Progressive development of metal contents in the reduced sulfide-bearing hydrothermal fluid proceeds from Zn&amp;#8211;Cu&amp;#8211;Sn to Pb&amp;#8211;Bi&amp;#8211;Ag and As&amp;#8211;Sb. Late-stage sulfate- and fluorine-bearing fluids partly altered earlier mineralization but did not deposit significant ore content.
            </summary>
            <content type="html">
                &lt;b&gt;Mineralogy of sulfide mineralization from the world-class Li–Sn–W Cínovec greisen-type deposit, Bohemian Massif, Czech Republic&lt;/b&gt;&lt;br&gt;
                Ondřej Krátký, Jan Cempírek, Sebastián Hreus, Luboš Vrtiška, Jiří Sejkora, Zdeněk Dolníček, Jakub Výravský, Radek Škoda, Karel Breiter, and Vojtěch Šešulka&lt;br&gt;
                    Eur. J. Mineral., 38, 281&#8211;304, https://doi.org/10.5194/ejm-38-281-2026, 2026&lt;br&gt;
                <p>Mineralogical, paragenetic, and geochemical data on sulfidic mineralization from the C&amp;#237;novec Li&amp;#8211;Sn&amp;#8211;W greisen-type deposit (Bohemian Massif, Czech Republic) were used to refine the evolution of mineralization at this world-class deposit and to clarify the relationship between base-metal sulfides and the Li&amp;#8211;Sn&amp;#8211;W mineralization. Sulfides occur in three main settings: (i)&amp;#160;quartz&amp;#8211;zinnwaldite veins, (ii)&amp;#160;massive greisens and greisenized granites, and (iii)&amp;#160;late baryte&amp;#8211;fluorite veins that locally overprint earlier types. Electron microprobe analyses and detailed BSE imaging reveal multiple mineralization stages and a surprisingly large suite of sulfide minerals. They were divided into several mineralization stages, including the greisen stage (molybdenite, arsenopyrite, safflorite), early sulfide stage (stannite&amp;#8211;k&amp;#235;sterite, stannoidite, sphalerite), intermediate sulfide stage (galena), and late sulfide stage (pyrite, marcasite, chalcopyrite, tennantite&amp;#8211;tetrahedrite, enargite, lautite, Cu&amp;#8211;Ag&amp;#8211;Bi&amp;#8211;Pb sulfosalts, native Bi, Cu sulfides, pearceite, cupropearceite, stromeyerite). A minor amount of sulfides was remobilized during later the fluorite&amp;#8211;baryte stage. Distribution of sulfide mineralization at the deposit is irregular; sulfides are not strictly bound to prevalent Li&amp;#8211;Sn&amp;#8211;W mineralization. The dominant sphalerite-bearing assemblages (Zn&amp;#8211;Pb&amp;#8211;Cu) display average grades of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;100&amp;#8211;200&amp;#8201;ppm Zn (however, Zn is partly contained in zinnwaldite), 20&amp;#8211;50&amp;#8201;ppm Pb, and <span class="inline-formula"><i><</i></span>&amp;#8201;50&amp;#8201;ppm Cu in disseminated mineralization, with locally elevated In contents (<span class="inline-formula">&amp;#8804;</span>&amp;#8201;0.53&amp;#8201;wt&amp;#8201;%) in sphalerite. Progressive evolution of metal contents in the reduced sulfide-bearing hydrothermal fluid proceeds from Zn&amp;#8211;Cu&amp;#8211;Sn to Pb&amp;#8211;Bi&amp;#8211;Ag and  As&amp;#8211;Sb. Late-stage sulfate- and fluorine-bearing fluids partly altered earlier mineralization but did not deposit significant ore content.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-20T22:15:55+02:00</published>
            <updated>2026-05-20T22:15:55+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-263-2026</id>
            <title type="html">Retrograde crystallization of clay minerals in metamorphic rocks linked to fluid circulation related to fault activity
            </title>
            <link href="https://doi.org/10.5194/ejm-38-263-2026"/>
            <summary type="html">
                &lt;b&gt;Retrograde crystallization of clay minerals in metamorphic rocks linked to fluid circulation related to fault activity&lt;/b&gt;&lt;br&gt;
                Isabel Abad, Matías Reolid, Juan Jiménez-Millán, and Fernando Nieto&lt;br&gt;
                    Eur. J. Mineral., 38, 263&#8211;280, https://doi.org/10.5194/ejm-38-263-2026, 2026&lt;br&gt;
                Metamorphic rocks affected by a fault have undergone chemical, mineralogical, and textural changes. The most significant is the enrichment in clay minerals (chlorite, kaolinite, and smectite). Geothermometry of the new chlorites made it possible to determine the temperatures of the processes (predominantly &lt; 225&amp;#176;C), promoted by the fault dynamics (mainly fluid-related alterations). The retrograde alteration also affected the fluid-accessible zones of the original rocks, with growth of the same clay minerals.
            </summary>
            <content type="html">
                &lt;b&gt;Retrograde crystallization of clay minerals in metamorphic rocks linked to fluid circulation related to fault activity&lt;/b&gt;&lt;br&gt;
                Isabel Abad, Matías Reolid, Juan Jiménez-Millán, and Fernando Nieto&lt;br&gt;
                    Eur. J. Mineral., 38, 263&#8211;280, https://doi.org/10.5194/ejm-38-263-2026, 2026&lt;br&gt;
                <p>The study of two outcrops of schists in the Padul Fault area has allowed us to corroborate the enrichment in clay minerals in the fault zone. In the case of the dark schist outcrop, the fault rocks show a reduction in  mineral diversity  with aluminosilicates, characteristics of the regional metamorphism losing and showing an enrichment in quartz and kaolin-group minerals. In the calc-schists, there is a clear presence of chlorite in the fault rocks, which is practically absent in the fresh rocks, as well as R1 illite/smectite and smectite. The geochemical characterization also showed differences between fresh and fault rocks, more evident in the dark schists than in the calc-schists, with an increase in SiO<span class="inline-formula"><sub>2</sub></span&gt; but a significant decrease in Al<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span>, Fe<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>3</sub></span>, and MgO in the fault rocks with respect to the protolith. The presence of authigenic chlorite in the fault rocks from the calc-schists allowed for the application of semi-empirical thermometric methods for the fault rocks giving predominant temperatures <span class="inline-formula"><i><</i></span>&amp;#8201;225&amp;#8201;&amp;#176;C. All these data are consistent with the circulation of low-temperature fluids along the fault zone that interact with the rocks, promoting clay mineral formation. Such was also the findings in a previous study focused on the predominant rocks of the Padul Fault area, which are dolostones, affected by the dynamics of this fault. Interestingly, the circulation of fluids promoted by the existence of the Padul Fault has not been restricted to the fault rocks, given that some of these clay minerals (kaolinite and smectite) are also present in the fluid-accessible zones of the metamorphic protolith. These data highlight the importance of faults in the retrograde mineralization processes of metamorphic rocks.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-05-11T22:15:55+02:00</published>
            <updated>2026-05-11T22:15:55+02:00</updated>
        </entry>
</feed>