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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>2026-06-11T16:48:45+02:00</updated>
    <author>
        <name>Copernicus Publications</name>
    </author>
        <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>2026-06-11T16:48:45+02:00</published>
            <updated>2026-06-11T16:48:45+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>2026-05-22T16:48:45+02:00</published>
            <updated>2026-05-22T16:48:45+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>2026-05-20T16:48:45+02:00</published>
            <updated>2026-05-20T16:48:45+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>2026-05-11T16:48:45+02:00</published>
            <updated>2026-05-11T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-249-2026</id>
            <title type="html">The Tibet leucogranite as a potential high-purity-quartz raw material: first discovery and case study from the Dinggye area
            </title>
            <link href="https://doi.org/10.5194/ejm-38-249-2026"/>
            <summary type="html">
                &lt;b&gt;The Tibet leucogranite as a potential high-purity-quartz raw material: first discovery and case study from the Dinggye area&lt;/b&gt;&lt;br&gt;
                Liting Sun, Xiaoyong Yang, Mei Xia, Yue Qiu, Zhenhui Hou, Xiaohu Fu, and Zetai Chen&lt;br&gt;
                    Eur. J. Mineral., 38, 249&#8211;262, https://doi.org/10.5194/ejm-38-249-2026, 2026&lt;br&gt;
                This study evaluates leucogranites from the Ama Drime Massif, Dinggye, Tibet, as a potential raw material for high-purity quartz. Petrographic, geochemical, and purification analyses of two representative samples show that the rocks are mainly composed of quartz, albite, and K-feldspar. After purification, the quartz reached SiO&amp;#8322; contents of 99.996 % and 99.995 %, indicating promising potential as a supplementary high-purity-quartz resource.
            </summary>
            <content type="html">
                &lt;b&gt;The Tibet leucogranite as a potential high-purity-quartz raw material: first discovery and case study from the Dinggye area&lt;/b&gt;&lt;br&gt;
                Liting Sun, Xiaoyong Yang, Mei Xia, Yue Qiu, Zhenhui Hou, Xiaohu Fu, and Zetai Chen&lt;br&gt;
                    Eur. J. Mineral., 38, 249&#8211;262, https://doi.org/10.5194/ejm-38-249-2026, 2026&lt;br&gt;
                <p>This study evaluates Tibet leucogranites as a potential raw material for high-purity quartz. We systematically investigate the petrography, geochemistry, and purification potential of leucogranites from the Ama Drime Massif of the Dinggye area. Our results demonstrate that these leucogranites hold considerable potential to produce high-purity quartz with SiO<span class="inline-formula"><sub>2</sub></span&gt; contents above 99.995&amp;#8201;%, highlighting their value as a new and extensive source of high-purity quartz in Tibet. Various analytical techniques, including optical microscopy, X-ray fluorescence imaging, X-ray fluorescence spectrometry, ICP-MS, and LA-ICP-MS, together with purification experiments, were applied to representative samples (XZ-BG and XZ-WJ). The results indicate that the leucogranites are composed predominantly of quartz, albite, and K-feldspar, with minor biotite, muscovite, garnet, and amphibole. These rocks display typical S-type granite characteristics and were likely derived from source regions comprising granitic gneiss and metamorphic shale. Quartz-hosted inclusions are dominated by relatively large primary inclusions and secondary fluid inclusions, which are comparatively easy to remove during purification. As a result, the purified samples yielded SiO<span class="inline-formula"><sub>2</sub></span&gt; contents of 99.996&amp;#8201;% and 99.995&amp;#8201;%, respectively. This work represents the first integrated mineralogical, geochemical, and purification assessment of Tibet leucogranites as a source of high-purity quartz and proposes temperature as a key ore-controlling factor. The widespread exposure of leucogranite in the region offers a significant opportunity to develop high-end quartz resources in China, ensuring a stable and strategic supply of high-purity-quartz raw materials.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-30T16:48:45+02:00</published>
            <updated>2026-04-30T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-237-2026</id>
            <title type="html">Erzwiesite, Ag<sub>8</sub>Pb<sub>12</sub>Bi<sub>16</sub>S<sub>40</sub>, the natural orthorhombic <i>N</i>&#8201;=&#8201;&#8201;8 member of the lillianite homologous series
            </title>
            <link href="https://doi.org/10.5194/ejm-38-237-2026"/>
            <summary type="html">
                &lt;b&gt;Erzwiesite, Ag8Pb12Bi16S40, the natural orthorhombic N =  8 member of the lillianite homologous series&lt;/b&gt;&lt;br&gt;
                Dan Topa, Emil Makovicky, Hubert Putz, Werner Hermann Paar, and Georg Zagler&lt;br&gt;
                    Eur. J. Mineral., 38, 237&#8211;247, https://doi.org/10.5194/ejm-38-237-2026, 2026&lt;br&gt;
                <p class="western"><span lang="en-GB">Erzwiesite</span><span lang="en-GB">, ideally Ag</span><sub><span lang="en-GB">8</span></sub><span lang="en-GB">Pb</span><sub><span lang="en-GB">12</span></sub><span lang="en-GB">Bi</span><sub><span lang="en-GB">16</span></sub><span lang="en-GB">S</span><sub><span lang="en-GB">40</span></sub><span lang="en-GB">, </span><span lang="en-GB"><em>Z</em></span><span lang="en-GB"&gt; = 1, is a new sulfosalt mineral discovered in the Erzwies mining area, Gastein Valley, Salzburg Province, Austria. </span><span lang="en-GB">The empirical formula is (Ag,Cu)</span><sub><span lang="en-GB">8.23</span></sub><span lang="en-GB">(Pb,Cd)</span><sub><span lang="en-GB">11.33</span></sub><span lang="en-GB">(Bi,Sb)</span><sub><span lang="en-GB">16.31 </span></sub><span lang="en-GB">(S,Te,Se)</span><sub><span lang="en-GB">40.03</span></sub><span lang="en-GB"&gt; (based on 76 apfu).</span&gt; <span lang="en-GB">Erzwiesite crystallises in space group </span><span lang="en-GB"><em>Cmcm</em></span><span lang="en-GB"&gt; (</span><span lang="en-GB"><em>a</em></span><span lang="en-GB"&gt; = </span><span lang="en-GB">4.085(5), </span><span lang="en-GB"><em>b</em></span><span lang="en-GB"&gt; = 13.462(15), </span><span lang="en-GB"><em>c </em></span><span lang="en-GB">= 33.92(4) &amp;#197;, and </span><span lang="en-GB"><em>V</em></span><span lang="en-GB"&gt; = </span><span lang="en-GB">1866(4) </span><span lang="en-GB">&amp;#197;&amp;#179;)</span><span lang="en-GB">. Erzwiesite is the first natural (8:8) homologue of the lillianite homologous series and is named after its type locality.</span>
            </summary>
            <content type="html">
                &lt;b&gt;Erzwiesite, Ag8Pb12Bi16S40, the natural orthorhombic N =  8 member of the lillianite homologous series&lt;/b&gt;&lt;br&gt;
                Dan Topa, Emil Makovicky, Hubert Putz, Werner Hermann Paar, and Georg Zagler&lt;br&gt;
                    Eur. J. Mineral., 38, 237&#8211;247, https://doi.org/10.5194/ejm-38-237-2026, 2026&lt;br&gt;
                <p>Erzwiesite, ideally Ag<span class="inline-formula"><sub>8</sub></span>Pb<span class="inline-formula"><sub>12</sub></span>Bi<span class="inline-formula"><sub>16</sub></span>S<span class="inline-formula"><sub>40</sub></span>, <span class="inline-formula"><i>Z</i>=</span>&amp;#8201;1, is a new sulfosalt mineral discovered in the Erzwies mining area, Gastein Valley, Salzburg Province, Austria. The mineral occurs as small black, irregular needle-like crystals mixed with galena and heyrovsk&amp;#253;ite in a quartz matrix. In reflected light, erzwiesite is greyish white. Under crossed polars it is distinctly anisotropic, and the rotation tints change from pale brown to pale bluish grey to dark brown. Reflectance measurements in air yield the following <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M12" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>R</mi><mi mathvariant="normal">min</mi></msub><mo>/</mo><msub><mi>R</mi><mi mathvariant="normal">max</mi></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="52pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="18034984ef853bd0183ba070b0f1655b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-237-2026-ie00001.svg" width="52pt" height="14pt" src="ejm-38-237-2026-ie00001.png"/></svg:svg></span></span&gt; values based on the standard wavelengths (Commission on Ore Mineralogy, COM): <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M13" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">44.5</mn><mo>/</mo><mn mathvariant="normal">47.6</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="51pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="b44fd1aa357cf9d6a7548d175c7bd1c0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-237-2026-ie00002.svg" width="51pt" height="14pt" src="ejm-38-237-2026-ie00002.png"/></svg:svg></span></span&gt; (470&amp;#8201;nm), <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M14" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">41.9</mn><mo>/</mo><mn mathvariant="normal">45.0</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="51pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="8b56049a2ec35444d087ac3c566ab4c1"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-237-2026-ie00003.svg" width="51pt" height="14pt" src="ejm-38-237-2026-ie00003.png"/></svg:svg></span></span&gt; (546&amp;#8201;nm), <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M15" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">41.5</mn><mo>/</mo><mn mathvariant="normal">44.5</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="51pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="620e48f99bb3ab4fb8e527265c8ef66b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-237-2026-ie00004.svg" width="51pt" height="14pt" src="ejm-38-237-2026-ie00004.png"/></svg:svg></span></span&gt; (589&amp;#8201;nm), and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M16" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">40.4</mn><mo>/</mo><mn mathvariant="normal">43.6</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="51pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="a312062448cd5d1b14fe3478e8fadd72"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-237-2026-ie00005.svg" width="51pt" height="14pt" src="ejm-38-237-2026-ie00005.png"/></svg:svg></span></span&gt; (650&amp;#8201;nm). The Mohs' hardness is 3&amp;#8211;3.5 (VHN<span class="inline-formula"><sub>50</sub></span&gt; ranges from 195 to 224, mean 210&amp;#8201;kg&amp;#8201;mm<span class="inline-formula"><sup>&amp;#8722;2</sup></span>). Averaged electron-microprobe analyses (<span class="inline-formula"><i>n</i>=</span>&amp;#8201;6) gave (in wt&amp;#8201;%) Ag 11.10(27), Cu 0.04(3), Pb 29.50(77), Cd 0.17(1), Bi 42.90(63), Te 0.21(14), Se 0.08(5), and S 16.08(11), with a total of 100.10(63). The empirical formula is Ag<span class="inline-formula"><sub>8.18</sub></span>Cu<span class="inline-formula"><sub>0.05</sub></span>Pb<span class="inline-formula"><sub>11.31</sub></span>Cd<span class="inline-formula"><sub>0.12</sub></span>Bi<span class="inline-formula"><sub>16.30</sub></span>Sb<span class="inline-formula"><sub>0.01</sub></span>S<span class="inline-formula"><sub>39.81</sub></span>Te<span class="inline-formula"><sub>0.13</sub></span>Se<span class="inline-formula"><sub>0.06</sub></span&gt; (based on 76&amp;#8201;apfu). The calculated density is 7.075&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span&gt; using the empirical formula. Erzwiesite crystallises in space group <i>Cmcm</i&gt; (<span class="inline-formula"><i>a</i>=</span>&amp;#8201;4.085(5), <span class="inline-formula"><i>b</i>=</span>&amp;#8201;13.462(15), <span class="inline-formula"><i>c</i>=</span>&amp;#8201;33.92(4) &amp;#197;, and <span class="inline-formula"><i>V</i>=</span>&amp;#8201;1866(4) &amp;#197;<span class="inline-formula"><sup>3</sup></span>). The crystal structure was determined from single-crystal X-ray diffraction data (<span class="inline-formula"><i>R</i><sub>1</sub>=</span>&amp;#8201;5.24&amp;#8201;% for 308 data with <span class="inline-formula"><i>F</i><sub><i>o</i></sub></span>&amp;#8201;<span class="inline-formula"><i>></i></span>&amp;#8201;4<span class="inline-formula"><i>&amp;#963;</i>(<i>F</i><sub><i>o</i></sub>)</span&gt; and 51 variable parameters). The structural formula is Ag<span class="inline-formula"><sub>8.64</sub></span>Pb<span class="inline-formula"><sub>11.04</sub></span>Bi<span class="inline-formula"><sub>16.32</sub></span>S<span class="inline-formula"><sub>40</sub></span>. The seven strongest lines in the X-ray powder diagram are [<span class="inline-formula"><i>d</i></span&gt; in &amp;#197; (intensity) <i>hkl</i>] 3.588 (64) 028, 3.387 (98) 115, 3.349 (37) 041, 3.288 (85) 029, 2.919 (100)133, 2.846 (99)134, and 2.039(43) 157. Erzwiesite is the first natural (8&amp;#8201;:&amp;#8201;8) homologue of the lillianite homologous series and is named after its type locality.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-29T16:48:45+02:00</published>
            <updated>2026-04-29T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-231-2026</id>
            <title type="html">IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) &#8211; Newsletter 90
            </title>
            <link href="https://doi.org/10.5194/ejm-38-231-2026"/>
            <summary type="html">
                &lt;b&gt;IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) – Newsletter 90&lt;/b&gt;&lt;br&gt;
                Ferdinando Bosi, Frédéric Hatert, Marco Pasero, and Stuart J. Mills&lt;br&gt;
                    Eur. J. Mineral., 38, 231&#8211;235, https://doi.org/10.5194/ejm-38-231-2026, 2026&lt;br&gt;
                There is no short summary.
            </summary>
            <content type="html">
                &lt;b&gt;IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) – Newsletter 90&lt;/b&gt;&lt;br&gt;
                Ferdinando Bosi, Frédéric Hatert, Marco Pasero, and Stuart J. Mills&lt;br&gt;
                    Eur. J. Mineral., 38, 231&#8211;235, https://doi.org/10.5194/ejm-38-231-2026, 2026&lt;br&gt;
                
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-28T16:48:45+02:00</published>
            <updated>2026-04-28T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-209-2026</id>
            <title type="html">Plumbogottlobite, PbMg(VO<sub>4</sub>)(OH), the Pb analogue of gottlobite and the Mg analogue of descloizite
            </title>
            <link href="https://doi.org/10.5194/ejm-38-209-2026"/>
            <summary type="html">
                &lt;b&gt;Plumbogottlobite, PbMg(VO4)(OH), the Pb analogue of gottlobite and the Mg analogue of descloizite&lt;/b&gt;&lt;br&gt;
                Anthony R. Kampf, Joy Désor, and Chi Ma&lt;br&gt;
                    Eur. J. Mineral., 38, 209&#8211;216, https://doi.org/10.5194/ejm-38-209-2026, 2026&lt;br&gt;
                This paper describes the new mineral plumbogottlobite from the Gl&amp;#252;cksstern mine, Gottlob Hill, Friedrichroda, Gotha District, Thuringia, Germany. It occurs as thick, square, orange-brown, tabular crystals up to about 0.2 mm in diameter. The mineral is the lead (Pb) analogue of the mineral gottlobite, which occurs at the same locality and is identical in appearance. Plumbogottlobite is a late-stage, low-temperature hydrothermal mineral occurring on baryte and hausmannite.
            </summary>
            <content type="html">
                &lt;b&gt;Plumbogottlobite, PbMg(VO4)(OH), the Pb analogue of gottlobite and the Mg analogue of descloizite&lt;/b&gt;&lt;br&gt;
                Anthony R. Kampf, Joy Désor, and Chi Ma&lt;br&gt;
                    Eur. J. Mineral., 38, 209&#8211;216, https://doi.org/10.5194/ejm-38-209-2026, 2026&lt;br&gt;
                <p>Plumbogottlobite (IMA 2025-075), PbMg(VO<span class="inline-formula"><sub>4</sub></span>)(OH), is a new mineral from the Gl&amp;#252;cksstern mine, Gottlob Hill, Friedrichroda, Gotha District, Thuringia, Germany; it is a late-stage, low-temperature hydrothermal mineral occurring on baryte and hausmannite. Plumbogottlobite forms orange-brown tablets up to about 0.2&amp;#8201;mm in diameter. The mineral has a light-orange-brown streak, adamantine lustre, a Mohs hardness of <span class="inline-formula">&amp;#8764;</span>&amp;#8201;4 to 4.5, brittle tenacity, irregular to conchoidal fracture, no cleavage, and a calculated density of 5.359&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Optically, plumbogottlobite crystals are biaxial (&amp;#8211;), with <span class="inline-formula">2<i>V</i>=84(1)</span>&amp;#176;. The empirical formula from electron probe microanalyses based on 5 O <i>apfu</i&gt; is (Pb<span class="inline-formula"><sub>0.89</sub>&amp;#9633;<sub>0.11</sub></span>)<span class="inline-formula"><sub>&amp;#931;1.00</sub></span>(Mg<span class="inline-formula"><sub>0.77</sub></span>Cu<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">0.19</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="18pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="b43d57e98c805d286dbc81b0f22e243f"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-209-2026-ie00001.svg" width="18pt" height="17pt" src="ejm-38-209-2026-ie00001.png"/></svg:svg></span></span>Mn<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M10" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">0.09</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="18pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="d9c7677215f733d3985e216817cb81d0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-209-2026-ie00002.svg" width="18pt" height="17pt" src="ejm-38-209-2026-ie00002.png"/></svg:svg></span></span>)<span class="inline-formula"><sub>&amp;#931;1.05</sub></span>(VO<span class="inline-formula"><sub>4</sub></span>)(OH) (<span class="inline-formula">+</span>0.12 H for charge balance). Plumbogottlobite is orthorhombic with space group <i>Pnma</i&gt; and single-crystal unit-cell parameters <span class="inline-formula"><i>a</i>=7.6104(7)</span>, <span class="inline-formula"><i>b</i>=6.1091(6)</span>, <span class="inline-formula"><i>c</i>=9.3968(8)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=436.88(7)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=4</span>. The crystal structure is refined to <span class="inline-formula"><i>R</i><sub>1</sub>=0.0302</span&gt; for 429 reflections with <span class="inline-formula"><i>I</i><i>></i>2<i>&amp;#963;</i><sub><i>I</i></sub></span>. The mineral is the Pb analogue of gottlobite and the Mg analogue of descloizite.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-23T16:48:45+02:00</published>
            <updated>2026-04-23T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-217-2026</id>
            <title type="html">Lopatkaite, a new mineral from Taylor Pit, Madoc, Ontario, Canada
            </title>
            <link href="https://doi.org/10.5194/ejm-38-217-2026"/>
            <summary type="html">
                &lt;b&gt;Lopatkaite, a new mineral from Taylor Pit, Madoc, Ontario, Canada&lt;/b&gt;&lt;br&gt;
                Dan Topa, Emil Makovicky, Hubert Putz, and Georg Zagler&lt;br&gt;
                    Eur. J. Mineral., 38, 217&#8211;229, https://doi.org/10.5194/ejm-38-217-2026, 2026&lt;br&gt;
                Lopatkaite, ideally Pb<sub>10</sub>As<sub>2</sub>Sb<sub>6</sub>S<sub>22</sub&gt; (<em>Z</em&gt; = 4), is a new arsenic-bearing sulfosalt species found in the Madoc deposit, Taylor Pit, Ontario, Canada. Associated minerals in the holotype specimen are boulangerite, veenite, and sterryite, all embedded in a calcite matrix. The ideal formula may be derived from the ideal boulangerite formula, Pb<sub>10</sub>Sb<sub>8</sub>S<sub>22</sub&gt; (<em>Z</em&gt; = 4), by a substitution of 2Sb with 2As. Lopatkaite is a homeotype of boulangerite and a new member of the rod-based family of sulfosalts.&amp;#160;
            </summary>
            <content type="html">
                &lt;b&gt;Lopatkaite, a new mineral from Taylor Pit, Madoc, Ontario, Canada&lt;/b&gt;&lt;br&gt;
                Dan Topa, Emil Makovicky, Hubert Putz, and Georg Zagler&lt;br&gt;
                    Eur. J. Mineral., 38, 217&#8211;229, https://doi.org/10.5194/ejm-38-217-2026, 2026&lt;br&gt;
                <p>Lopatkaite, ideally Pb<span class="inline-formula"><sub>10</sub></span>As<span class="inline-formula"><sub>2</sub></span>Sb<span class="inline-formula"><sub>6</sub></span>S<span class="inline-formula"><sub>22</sub></span&gt; (<span class="inline-formula"><i>Z</i>=4</span>), is a new arsenic-bearing sulfosalt found in the Madoc deposit, Taylor Pit, Ontario, Canada. Associated minerals in the holotype specimen are boulangerite, veenite, and sterryite, all embedded in a calcite matrix. Lopatkaite is greyish black and opaque, with metallic lustre and dark-grey streak. It is brittle without any discernible cleavage and parting and has a Mohs hardness of 3&amp;#8211;3.5. In reflected light lopatkaite is greyish white, with distinct bireflectance and pleochroism from white to grey, especially in oil. Under crossed polarisers, anisotropism is distinct, with rotation tints in shades of grey. Reflectance measurements in air yield the following <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>R</mi><mi mathvariant="normal">min</mi></msub><mo>/</mo><msub><mi>R</mi><mi mathvariant="normal">max</mi></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="52pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="15e3b8f2f995d6104716709ea5b09006"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00001.svg" width="52pt" height="14pt" src="ejm-38-217-2026-ie00001.png"/></svg:svg></span></span&gt; values based on the standard wavelengths (Commission on Ore Mineralogy, COM): 37.0&amp;#8201;%&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" 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="36bd7baae116a5efc17e692d563c2b51"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00002.svg" width="8pt" height="14pt" src="ejm-38-217-2026-ie00002.png"/></svg:svg></span></span>&amp;#8201;39.3&amp;#8201;% (470&amp;#8201;nm), 34.1&amp;#8201;%&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" 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="fb147fccdcf98a9911cf3d26a8f6dc33"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00003.svg" width="8pt" height="14pt" src="ejm-38-217-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;36.9&amp;#8201;% (546&amp;#8201;nm), 33.1&amp;#8201;%&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" 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="880d1b22cfae9b4167ff115d05c6894c"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00004.svg" width="8pt" height="14pt" src="ejm-38-217-2026-ie00004.png"/></svg:svg></span></span>&amp;#8201;36.2&amp;#8201;% (589&amp;#8201;nm), and 31.3&amp;#8201;%&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M10" 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="3af55808dad7e355d8e0b0b2a0272ce7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00005.svg" width="8pt" height="14pt" src="ejm-38-217-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;34.1&amp;#8201;% at (650&amp;#8201;nm). The average result of four electron probe microanalyses for the structurally investigated grain is as follows (in wt&amp;#8201;%): Pb 57.81(4), As 3.53(8), Sb 20.03(6), S 19.08(6), and total 100.46(22), corresponding to Pb<span class="inline-formula"><sub>10.28(3)</sub></span>As<span class="inline-formula"><sub>1.74(4)</sub></span>Sb<span class="inline-formula"><sub>6.06(3)</sub></span>S<span class="inline-formula"><sub>21.92(3)</sub></span&gt; (based on 18<i>Me</i>&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;22S&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;40&amp;#160;atoms per asymmetric unit). The density calculated using the empirical formula is 6.168&amp;#8201;Mg&amp;#8201;m<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Single-crystal X-ray diffraction data show lopatkaite to be monoclinic, 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="M19" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mn mathvariant="normal">1</mn></msub><mo>/</mo><mi>c</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="bf8b16adaa522e3dbc51b1fcf7601416"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-217-2026-ie00006.svg" width="20pt" height="14pt" src="ejm-38-217-2026-ie00006.png"/></svg:svg></span></span&gt; (no.&amp;#160;14), with <span class="inline-formula"><i>a</i>=8.0806(6)</span>, <span class="inline-formula"><i>b</i>=23.3597(18)</span>, <span class="inline-formula"><i>c</i>=21.4880(16)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#946;</i>=100.7090(10)</span>&amp;#176;, <span class="inline-formula"><i>V</i>=3985.4(5)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=4</span>. The seven strongest lines in the (calculated) powder diffraction pattern are as follows (<span class="inline-formula"><i>d</i></span&gt; in &amp;#197; (intensity) (<span class="inline-formula"><i>h</i><i>k</i><i>l</i></span>)): 3.728(39) 211, 3.712(100) 035, 3.653(35) 062, 2.804(41) <span class="inline-formula">&amp;#8722;261</span>, 2.780(43) 260, 2.779(38) <span class="inline-formula">&amp;#8722;262</span>, and 2.020(47) <span class="inline-formula">&amp;#8722;402</span>. The ideal formula is in accordance with the results of the crystal structure analysis, Pb<span class="inline-formula"><sub>10.336</sub></span>As<span class="inline-formula"><sub>1.567</sub></span>Sb<span class="inline-formula"><sub>6.088</sub></span>S<span class="inline-formula"><sub>22&amp;#8201;</sub></span>, and may be derived from the ideal boulangerite formula, Pb<span class="inline-formula"><sub>10</sub></span>Sb<span class="inline-formula"><sub>8</sub></span>S<span class="inline-formula"><sub>22</sub></span&gt; (<span class="inline-formula"><i>Z</i>=4</span>), by means of substitution of two Sb atoms with two As atoms. Lopatkaite is an isotype of boulangerite, differing by dominant As occupancy at two crystallographically independent mixed (Sb, As) sites. This dominant-site substitution defines lopatkaite as the arsenic-dominant isotype of boulangerite and justifies its recognition as a distinct mineral species. Lopatkaite is also a new member of the rod-based family of sulfosalts.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-23T16:48:45+02:00</published>
            <updated>2026-04-23T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-197-2026</id>
            <title type="html">Selective uptake of rare earth elements and other cations in sector-zoned natural calcite as analogues for trivalent actinide behavior 
            </title>
            <link href="https://doi.org/10.5194/ejm-38-197-2026"/>
            <summary type="html">
                &lt;b&gt;Selective uptake of rare earth elements and other cations in sector-zoned natural calcite as analogues for trivalent actinide behavior &lt;/b&gt;&lt;br&gt;
                Ferdinand Baumeister, Martin Kutzschbach, Martina Klinkenberg, Felix Brandt, and Thomas Neumann&lt;br&gt;
                    Eur. J. Mineral., 38, 197&#8211;208, https://doi.org/10.5194/ejm-38-197-2026, 2026&lt;br&gt;
                This study shows that calcite can trap elements similar to radioactive substances very effectively under natural conditions. By studying a sample formed under nuclear-waste-repository-like conditions, it was found that certain crystal parts hold over 200 times more of these elements. This happens through multiple processes, helping to safely store harmful substances even in low-salt environments, which is important for nuclear waste safety.
            </summary>
            <content type="html">
                &lt;b&gt;Selective uptake of rare earth elements and other cations in sector-zoned natural calcite as analogues for trivalent actinide behavior &lt;/b&gt;&lt;br&gt;
                Ferdinand Baumeister, Martin Kutzschbach, Martina Klinkenberg, Felix Brandt, and Thomas Neumann&lt;br&gt;
                    Eur. J. Mineral., 38, 197&#8211;208, https://doi.org/10.5194/ejm-38-197-2026, 2026&lt;br&gt;
                <p>Calcite has been shown to incorporate trivalent actinides into its crystal lattice, highlighting its potential to contribute to radionuclide retention processes in the environment. Earlier studies on calcite's elemental uptake were conducted under controlled laboratory conditions, which do not fully capture the complexities of natural environments. To gain a deeper understanding of calcite's uptake capacity under natural conditions, a sample from the Wenzel ore mine, Germany, was analyzed, originating from a calcite vein that formed under conditions relevant to deep geological-waste repositories. The chemical analogy between rare earth elements (REEs) and trivalent actinides helps to evaluate the retention potential and incorporation mechanisms of trivalent radionuclides. A micro-X-ray fluorescence (<span class="inline-formula">&amp;#181;</span>XRF) element map revealed that the investigated calcite consists of an euhedral crystal core exhibiting sector zoning, characterized by trace element heterogeneity across coevally grown crystal faces. High-resolution laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) further refined and quantified the elemental distribution, revealing preferential incorporation of specific elements, particularly REEs, within one sector of the calcite. Remarkably, this sector showed REE concentrations over 200 times higher than those in the depleted sector, indicating a significant potential for the retention of trivalent actinides. Furthermore, the data indicate that charge equilibration of incorporated trivalent cations occurs via two processes: coupled substitution with monovalent cations and vacancies in the crystal structure. Overall, these results demonstrate that sector-zoned calcite formed under repository-relevant conditions can maintain high retention potential for trivalent actinides, even in environments depleted in monovalent cations.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-20T16:48:45+02:00</published>
            <updated>2026-04-20T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-179-2026</id>
            <title type="html">Hydrous partial melting in gabbros drilled at the Southwest Indian Ridge (ODP Hole 735B): evidence from microstructures at grain boundaries
            </title>
            <link href="https://doi.org/10.5194/ejm-38-179-2026"/>
            <summary type="html">
                &lt;b&gt;Hydrous partial melting in gabbros drilled at the Southwest Indian Ridge (ODP Hole 735B): evidence from microstructures at grain boundaries&lt;/b&gt;&lt;br&gt;
                Jürgen Koepke&lt;br&gt;
                    Eur. J. Mineral., 38, 179&#8211;195, https://doi.org/10.5194/ejm-38-179-2026, 2026&lt;br&gt;
                Gabbroic rocks from the Southwest Indian Ridge have been investigated. The results show that hydrous partial melting triggered by hydrothermal fluids percolating on grain boundaries above the wet gabbro solidus is a common process at slow-spreading mid-ocean ridges. The main indication of this process is plagioclase strongly enriched in anorthite content at grain boundaries, which can only be identified via backscattered electron imaging and related electron microprobe profiles.
            </summary>
            <content type="html">
                &lt;b&gt;Hydrous partial melting in gabbros drilled at the Southwest Indian Ridge (ODP Hole 735B): evidence from microstructures at grain boundaries&lt;/b&gt;&lt;br&gt;
                Jürgen Koepke&lt;br&gt;
                    Eur. J. Mineral., 38, 179&#8211;195, https://doi.org/10.5194/ejm-38-179-2026, 2026&lt;br&gt;
                <p>The Atlantis Bank at the Southwest Indian Ridge (SWIR) is probably the most thoroughly investigated oceanic core complex from a typical slow-spreading ridge. Here, ODP (Ocean Drilling Program) conducted two drilling expeditions at Drill Site 735B. The gabbro massif is characterized by the presence of hundreds of felsic veins, which are rocks consisting of evolved, silica-rich material showing the composition of typical &amp;#8220;oceanic plagiogranites&amp;#8221;. Two models have been suggested for their generation: (1) the extreme differentiation of a MORB magma, resulting in a highly differentiated melt, and (2) the hydrous remelting of gabbroic rocks in the deep oceanic crust.</p&gt;        <p>Detailed petrographical and microanalytical investigations of gabbroic rocks from ODP drill core 735B reveal that many of these gabbros exhibit microstructures characteristic of hydrous partial melting of gabbro. Key features that led to this conclusion are zones of anorthite-enriched plagioclase on grain boundaries, which form parageneses with interstitial brown amphibole and orthopyroxene. These are interpreted as the residual phase assemblage left after hydrous partial melting. These events are triggered by water-rich fluids migrating along grain boundaries within the cooling gabbro complex at temperatures above the wet gabbro solidus. This conclusion is supported by two further observations: (1) trace element concentrations in the An-enriched plagioclase (Ti, Mg, and K) are strongly impoverished, in line with experiments simulating the hydrous partial melting of gabbro. (2) The bulk TiO<span class="inline-formula"><sub>2</sub></span&gt; content of the felsic veins shows characteristically low concentrations, consistently with an origin through the melting of TiO<span class="inline-formula"><sub>2</sub></span>-impoverished cumulate gabbro. This contrasts with melt compositions derived through fractional crystallization of MORB, where TiO<span class="inline-formula"><sub>2</sub></span&gt; concentrations are significantly higher. Our results show that hydrous partial melting of gabbro played a role in the formation of the felsic melts, alongside fractional crystallization, which is the standard model for felsic vein formation evidenced by several papers.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-09T16:48:45+02:00</published>
            <updated>2026-04-09T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-169-2026</id>
            <title type="html">Friisite, Pb<sub>8</sub>Al<sub>3</sub>Si<sub>8</sub>O<sub>27</sub>Cl<sub>3</sub>, a new mineral with a polysomatic relation to jagoite, from L&#229;ngban, Sweden
            </title>
            <link href="https://doi.org/10.5194/ejm-38-169-2026"/>
            <summary type="html">
                &lt;b&gt;Friisite, Pb8Al3Si8O27Cl3, a new mineral with a polysomatic relation to jagoite, from Långban, Sweden&lt;/b&gt;&lt;br&gt;
                Dan Holtstam, Fernando Cámara, and Andreas Karlsson&lt;br&gt;
                    Eur. J. Mineral., 38, 169&#8211;177, https://doi.org/10.5194/ejm-38-169-2026, 2026&lt;br&gt;
                Friisite is a newly identified mineral, with the chemical formula Pb<sub>8</sub>Al<sub>3</sub>Si<sub>8</sub>O<sub>27</sub>Cl<sub>3,</sub&gt; from the L&amp;#229;ngban mine in Sweden, found as tiny, white, flaky grains within a skarn matrix alongside jagoite and other silicates. It has a sub-adamantine luster, perfect basal cleavage, a hardness of 4&amp;#8211;5, and a high density of 5.54 g cm<sup>&amp;#8722;</sup>&amp;#179;. Structurally it is a hexagonal phyllosilicate, closely related to jagoite in a polysomatic series. The mineral is named in honor of Danish mineralogist Henrik Friis.
            </summary>
            <content type="html">
                &lt;b&gt;Friisite, Pb8Al3Si8O27Cl3, a new mineral with a polysomatic relation to jagoite, from Långban, Sweden&lt;/b&gt;&lt;br&gt;
                Dan Holtstam, Fernando Cámara, and Andreas Karlsson&lt;br&gt;
                    Eur. J. Mineral., 38, 169&#8211;177, https://doi.org/10.5194/ejm-38-169-2026, 2026&lt;br&gt;
                <p>Friisite, ideally Pb<span class="inline-formula"><sub>8</sub></span>Al<span class="inline-formula"><sub>3</sub></span>Si<span class="inline-formula"><sub>8</sub></span>O<span class="inline-formula"><sub>27</sub></span>Cl<span class="inline-formula"><sub>3</sub></span>, is a new mineral discovered in a museum sample from the L&amp;#229;ngban mine in V&amp;#228;rmland, Sweden. It occurs as subhedral, flaky grains up to 150&amp;#8201;<span class="inline-formula">&amp;#181;</span>m in size, forming aggregates within a medium-grained skarn matrix and contiguous to jagoite. Both are associated with melanotekite, aegirine&amp;#8211;augite, albite, baryte, fluorapophyllite-K, margarosanite, alamosite, native lead, a serpentine group mineral, and a wickenburgite-like mineral. Friisite is white to colorless with a white streak and sub-adamantine luster. The mineral is transparent and does not fluoresce under UV light. It is brittle, with an uneven fracture and perfect cleavage on {001}. Mohs hardness is 4&amp;#8211;5 (by analogy with jagoite). The calculated density is 5.54(1)&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Optically, friisite is non-pleochroic and uniaxial (&amp;#8211;). Point analyses by means of an electron microprobe using wavelength-dispersive spectroscopy resulted in an empirical formula (based on 30 O<span class="inline-formula">+</span>Cl): <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M19" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>(</mo><msub><mi mathvariant="normal">Pb</mi><mn mathvariant="normal">7.89</mn></msub><msub><mi mathvariant="normal">Na</mi><mn mathvariant="normal">0.11</mn></msub><msub><mi mathvariant="normal">Ca</mi><mn mathvariant="normal">0.08</mn></msub><msub><mo>)</mo><mrow><mo>&amp;#8721;</mo><mo>=</mo><mn mathvariant="normal">8.08</mn></mrow></msub><mspace linebreak="nobreak" width="0.125em"/><mo>(</mo><msub><mi mathvariant="normal">Al</mi><mn mathvariant="normal">2.19</mn></msub><msub><mi mathvariant="normal">Si</mi><mn mathvariant="normal">0.31</mn></msub><msubsup><mi mathvariant="normal">Fe</mi><mn mathvariant="normal">0.20</mn><mrow><mn mathvariant="normal">3</mn><mo>+</mo></mrow></msubsup><msub><mi mathvariant="normal">Zn</mi><mn mathvariant="normal">0.13</mn></msub><msubsup><mi mathvariant="normal">Mn</mi><mn mathvariant="normal">0.11</mn><mrow><mn mathvariant="normal">2</mn><mo>+</mo></mrow></msubsup><msub><mo>)</mo><mrow><mo>&amp;#8721;</mo><mo>=</mo><mn mathvariant="normal">2.94</mn></mrow></msub><msub><mi mathvariant="normal">Si</mi><mn mathvariant="normal">8</mn></msub><msub><mi mathvariant="normal">O</mi><mn mathvariant="normal">27.02</mn></msub><msub><mi mathvariant="normal">Cl</mi><mn mathvariant="normal">2.98</mn></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="374pt" height="18pt" class="svg-formula" dspmath="mathimg" md5hash="d9cd2be6747c49dcee69e8e55aec0143"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-169-2026-ie00001.svg" width="374pt" height="18pt" src="ejm-38-169-2026-ie00001.png"/></svg:svg></span></span>. Friisite is hexagonal, <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M20" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>P</mi><mover accent="true"><mn mathvariant="normal">6</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mn mathvariant="normal">2</mn><mi>c</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="29pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="6cdd735e9e2bbaa23f97ab62cf1f52be"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-169-2026-ie00002.svg" width="29pt" height="13pt" src="ejm-38-169-2026-ie00002.png"/></svg:svg></span></span&gt; (#190), with unit-cell parameters <span class="inline-formula"><i>a</i>=8.5955(1)</span&gt; &amp;#197;, <span class="inline-formula"><i>c</i>=23.4092(2)</span&gt; &amp;#197;, and <span class="inline-formula"><i>V</i>=1497.82(4)</span&gt; &amp;#197;<span class="inline-formula"><sup>3</sup></span&gt; for <span class="inline-formula"><i>Z</i>=2</span>. The eight strongest powder X-ray diffraction lines are [<span class="inline-formula"><i>d</i></span>, &amp;#197; (<span class="inline-formula"><i>I</i><sub>rel</sub></span>) (<i>hkl</i>)]: 5.848 (31) (004), 5.375 (20) (103), 4.040 (96) (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M28" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">11</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mn mathvariant="normal">2</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="9121a63a8326ebbe79e66578e4e65fa8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-169-2026-ie00003.svg" width="20pt" height="13pt" src="ejm-38-169-2026-ie00003.png"/></svg:svg></span></span>, 112), 3.680 (40) (201), 3.463 (100) (114), 2.886 (21) (116), 2.795 (20) (<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M29" display="inline" overflow="scroll" dspmath="mathml"><mrow><mover accent="true"><mn mathvariant="normal">21</mn><mo mathvariant="normal">&amp;#8254;</mo></mover><mn mathvariant="normal">1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="1ab97831b7898d5e502319ba6ad8fa4e"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-169-2026-ie00004.svg" width="20pt" height="13pt" src="ejm-38-169-2026-ie00004.png"/></svg:svg></span></span>), and 2.4828 (35) (300). Friiste is a phyllosilicate and forms a polysomatic series with jagoite characterized by a layer sequence of SiO<span class="inline-formula"><sub>4</sub></span&gt; tetrahedra (T) and metal octahedra (O) between double layers (*) corresponding to *TOT*, whereas jagoite is described as *TOTOT*. Friisite forms from transformation of melanotekite or barysilite in the presence of albite and a Cl-enriched fluid at relatively high <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M31" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>a</mi><mrow class="chem"><msub><mi mathvariant="normal">SiO</mi><mn mathvariant="normal">2</mn></msub></mrow></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="25pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="9cc7b1c5e15f32f2c5e05f24088230b8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-169-2026-ie00005.svg" width="25pt" height="12pt" src="ejm-38-169-2026-ie00005.png"/></svg:svg></span></span>. The mineral (IMA2024-047) is named in honor of Danish mineralogist Henrik Friis (b. 1977), professor at the Natural History Museum, University of Oslo, Norway.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-02T16:48:45+02:00</published>
            <updated>2026-04-02T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-153-2026</id>
            <title type="html">When mineralogy meets the organic chemistry: delchiaroite, Cu<sub>3</sub>I(CH<sub>3</sub>S)<sub>2</sub>, the first copper iodide&#8211;methanethiolate from the Carrara marble quarries, Apuan Alps, Tuscany, Italy
            </title>
            <link href="https://doi.org/10.5194/ejm-38-153-2026"/>
            <summary type="html">
                &lt;b&gt;When mineralogy meets the organic chemistry: delchiaroite, Cu3I(CH3S)2, the first copper iodide–methanethiolate from the Carrara marble quarries, Apuan Alps, Tuscany, Italy&lt;/b&gt;&lt;br&gt;
                Cristian Biagioni, Jiří Sejkora, Yves Moëlo, Antonino Criscuolo, and Zdeněk Dolníček&lt;br&gt;
                    Eur. J. Mineral., 38, 153&#8211;167, https://doi.org/10.5194/ejm-38-153-2026, 2026&lt;br&gt;
                Delchiaroite is the first iodide&amp;#8211;methanethiolate mineral and represents an interesting example where organic chemistry meets mineralogy.
            </summary>
            <content type="html">
                &lt;b&gt;When mineralogy meets the organic chemistry: delchiaroite, Cu3I(CH3S)2, the first copper iodide–methanethiolate from the Carrara marble quarries, Apuan Alps, Tuscany, Italy&lt;/b&gt;&lt;br&gt;
                Cristian Biagioni, Jiří Sejkora, Yves Moëlo, Antonino Criscuolo, and Zdeněk Dolníček&lt;br&gt;
                    Eur. J. Mineral., 38, 153&#8211;167, https://doi.org/10.5194/ejm-38-153-2026, 2026&lt;br&gt;
                <p>The new mineral delchiaroite, Cu<span class="inline-formula"><sub>3</sub></span>I(CH<span class="inline-formula"><sub>3</sub></span>S)<span class="inline-formula"><sub>2</sub></span>, has been discovered in La Piana quarry, Colonnata marble basin, Carrara, Apuan Alps, Tuscany, Italy. It occurs as light-yellow acicular crystals, elongated on [010], up to 0.1&amp;#8201;mm in length and is brittle, with a light-yellow streak and a greasy luster. In reflected light, delchiaroite is light gray with abundant internal yellow reflections; anisotropism is moderate, with gray tints. Reflectance values for the four COM wavelengths are (<span class="inline-formula"><i>&amp;#955;</i></span&gt; (nm) <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>R</mi><mi mathvariant="normal">min</mi></msub><mo>/</mo><msub><mi>R</mi><mi mathvariant="normal">max</mi></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="52pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="f7fe313f554c372821c302cffdb9fd99"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-153-2026-ie00001.svg" width="52pt" height="14pt" src="ejm-38-153-2026-ie00001.png"/></svg:svg></span></span&gt; (%)) 470: 20.6/22.2; 546: 20.9/23.4; 589: 20.7/23.3; and 650: 20.1/22.4. Electron microprobe analysis resulted in the following (average of 12 spot analyses &amp;#8211; in wt&amp;#8201;%): Cu 47.27, I 31.09, S 14.90, C<span class="inline-formula"><sub>calc</sub></span&gt; 5.58, H<span class="inline-formula"><sub>calc</sub></span&gt; 1.40, and total 100.24. The empirical formula of delchiaroite, calculated on the basis of Cu&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;I&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;S&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;6 atoms per formula unit, is Cu<span class="inline-formula"><sub>3.07</sub></span>I<span class="inline-formula"><sub>1.01</sub></span>(CH<span class="inline-formula"><sub>3</sub></span>S)<span class="inline-formula"><sub>1.92</sub></span>, in accordance with the end-member formula Cu<span class="inline-formula"><sub>3</sub></span>I(CH<span class="inline-formula"><sub>3</sub></span>S)<span class="inline-formula"><sub>2</sub></span>. Delchiaroite is orthorhombic, space group <i>Pmmn</i>, with <span class="inline-formula"><i>a</i>=16.924(10)</span>, <span class="inline-formula"><i>b</i>=4.099(2)</span>, <span class="inline-formula"><i>c</i>=5.572(3)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=386.5(4)</span>&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span>, and <span class="inline-formula"><i>Z</i>=2</span>. The crystal structure was refined to <span class="inline-formula"><i>R</i><sub>1</sub>=0.0962</span&gt; for 360 unique reflections, with <span class="inline-formula"><i>F</i><sub><i>o</i></sub><i>></i>4<i>&amp;#963;</i><i>F</i></span&gt; and 27 refined parameters. It can be described as being formed by electroneutral [Cu<span class="inline-formula"><sub>3</sub></span>I(CH<span class="inline-formula"><sub>3</sub></span>S)<span class="inline-formula"><sub>2</sub></span>]<span class="inline-formula"><sup>0</sup></span&gt; {100} layers stacked along <span class="inline-formula"><strong><em>a</em></strong></span>. The origin of delchiaroite is related to the supergene alteration of enargite in vugs of Liassic marbles. Chemically, this mineral belongs to the pseudo-binary system CuI&amp;#8211;Cu(CH<span class="inline-formula"><sub>3</sub></span>S) at a <span class="inline-formula">1:2</span&gt; ratio. It constitutes the first example of natural iodide&amp;#8211;methanethiolate, illustrating the interaction between inorganic and organic chemistry. Its name honors the mineral collector Lorenzo Del Chiaro (b. 1951) for his contribution to the knowledge of the mineralogy of the vugs of the Marble Formation belonging to the Alpi Apuane metamorphic complex.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-04-01T16:48:45+02:00</published>
            <updated>2026-04-01T16:48:45+02:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-135-2026</id>
            <title type="html">Mackinawite transformation into greigite at room temperature under anoxic and acidic conditions: a corrosion pathway?
            </title>
            <link href="https://doi.org/10.5194/ejm-38-135-2026"/>
            <summary type="html">
                &lt;b&gt;Mackinawite transformation into greigite at room temperature under anoxic and acidic conditions: a corrosion pathway?&lt;/b&gt;&lt;br&gt;
                Pierre Le Pape, Benoît Baptiste, Guillaume Radtke, Delphine Cabaret, Julie Aufort, Jessica Brest, Camille Baya, Erik Elkaim, Georges Ona-Nguema, Farid Juillot, and Guillaume Morin&lt;br&gt;
                    Eur. J. Mineral., 38, 135&#8211;152, https://doi.org/10.5194/ejm-38-135-2026, 2026&lt;br&gt;
                Iron sulfides are ubiquitous minerals of sedimentary environments. Several research works consider it to be that they preserve evidence of their original deposition environment, allowing us to derive paleo-environmental information. However, linking environmental factors to final mineralogy requires gaining mechanistic-level information about their formation pathways. Here, we propose a mackinawite to greigite "corrosion" pathway, with H+ acting as an oxidant.
            </summary>
            <content type="html">
                &lt;b&gt;Mackinawite transformation into greigite at room temperature under anoxic and acidic conditions: a corrosion pathway?&lt;/b&gt;&lt;br&gt;
                Pierre Le Pape, Benoît Baptiste, Guillaume Radtke, Delphine Cabaret, Julie Aufort, Jessica Brest, Camille Baya, Erik Elkaim, Georges Ona-Nguema, Farid Juillot, and Guillaume Morin&lt;br&gt;
                    Eur. J. Mineral., 38, 135&#8211;152, https://doi.org/10.5194/ejm-38-135-2026, 2026&lt;br&gt;
                <p>In surface soils and sediments, iron monosulfide (FeS) species, including nanocrystalline mackinawite, tend to quickly form in the presence of iron and sulfide in anoxic conditions. As such, FeS species are the main precursors for the formation of other iron sulfides such as Fe<span class="inline-formula"><sub>3</sub></span>S<span class="inline-formula"><sub>4</sub></span&gt; greigite and FeS<span class="inline-formula"><sub>2</sub></span&gt; pyrite, which are ubiquitous in surface sedimentary environments. It is known that, under prolonged aging under reducing conditions in a sulfidic aqueous medium, FeS species can evolve into crystalline mackinawite. However, the possible influence of pH on the evolution of mackinawite under such anoxic low-temperature conditions relevant to sedimentary (sub)surface environments has not been investigated yet. In this study, we used Rietveld refinement and pair distribution function analysis (PDF) of synchrotron-based X-ray powder diffraction (XRD) patterns to derive the mean coherent domain (MCD) size of mackinawite after aging under various pH conditions and X-ray absorption near-edge structure (XANES) spectroscopy at the S and Fe <span class="inline-formula"><i>K</i></span>-edges to study the structural and electronic properties. Moreover, in order to strengthen our interpretations, we confirmed the shape and relative energy of pre-edge features in the S <span class="inline-formula"><i>K</i></span>-edge XANES spectra of mackinawite (FeS) and pyrite (FeS<span class="inline-formula"><sub>2</sub></span>) model compounds via first-principle calculations. Our results show that, after FeS has precipitated from aqueous Fe(II) and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow class="chem"><msub><mi mathvariant="normal">H</mi><mn mathvariant="normal">2</mn></msub><mi mathvariant="normal">S</mi><mo>/</mo><msup><mi mathvariant="normal">HS</mi><mo>-</mo></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="50pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="4c2e61bebf3aa9ce1218ba765298f1ba"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00001.svg" width="50pt" height="14pt" src="ejm-38-135-2026-ie00001.png"/></svg:svg></span></span&gt; in a saline medium at pH&amp;#160;7.1, aqueous aging at the same pH over 47&amp;#8201;d results in the formation of nanocrystalline mackinawite (MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mrow><mi>a</mi><mi>b</mi></mrow></msub><mo>=</mo><mn mathvariant="normal">11.5</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="73pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="2118cfa36d0a1e9457e8bd91777ce44c"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00002.svg" width="73pt" height="12pt" src="ejm-38-135-2026-ie00002.png"/></svg:svg></span></span>&amp;#8201;nm; MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M9" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mi>c</mi></msub><mo>=</mo><mn mathvariant="normal">7.1</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="62pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="ac2221155b0d94eb38546465fb7c0007"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00003.svg" width="62pt" height="12pt" src="ejm-38-135-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;nm). When Na<span class="inline-formula"><sub>2</sub></span>S is added into the solution to reach pH&amp;#160;9.7 after FeS has precipitated at pH&amp;#160;7.1, no other Fe sulfide is observed during the aging phase, and mackinawite particles are of smaller size (MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M11" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mrow><mi>a</mi><mi>b</mi></mrow></msub><mo>=</mo><mn mathvariant="normal">7.9</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="67pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="fa999fd907eb689fcbdb8c12680b6237"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00004.svg" width="67pt" height="12pt" src="ejm-38-135-2026-ie00004.png"/></svg:svg></span></span>&amp;#8201;nm; MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M12" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mi>c</mi></msub><mo>=</mo><mn mathvariant="normal">4.6</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.1</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="62pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="31f119bd6c4630f13e88f111abe3dff8"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00005.svg" width="62pt" height="12pt" src="ejm-38-135-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;nm). In this sample, an additional weak and broad peak appears at <span class="inline-formula"><i>d</i>=10.5</span>&amp;#8201;&amp;#197; that could be interpreted as being due to either lattice expansion at the particle boundaries or a double-cell super-structure. When H<span class="inline-formula"><sup>+</sup></span&gt; is added as HCl to reach pH&amp;#160;5.1 before the aging phase, the size of mackinawite particles increases (MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M15" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mrow><mi>a</mi><mi>b</mi></mrow></msub><mo>=</mo><mn mathvariant="normal">13.0</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.2</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="73pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="8aadd77d956dbcf7a2e1acff85e27c33"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00006.svg" width="73pt" height="12pt" src="ejm-38-135-2026-ie00006.png"/></svg:svg></span></span>&amp;#8201;nm; MCD<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M16" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mi>c</mi></msub><mo>=</mo><mn mathvariant="normal">8.1</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.2</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="62pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="9e74d8dc994f8d90fbcdf8b67208ec4c"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-135-2026-ie00007.svg" width="62pt" height="12pt" src="ejm-38-135-2026-ie00007.png"/></svg:svg></span></span>&amp;#8201;nm), and a fraction transforms into greigite (Fe<span class="inline-formula"><sub>3</sub></span>S<span class="inline-formula"><sub>4</sub></span>). This reaction is accompanied by a pH increase to 6.4, likely because of H<span class="inline-formula"><sup>+</sup></span&gt; consumption, which suggests that Fe(II) in FeS would serve as an electron donor and that H<span class="inline-formula"><sup>+</sup></span&gt; would serve as an electron acceptor. The calculated electronic structure of mackinawite shows partly filled Fe-3<span class="inline-formula"><i>d</i></span&gt; states, which supports the fact that acidic aging conditions are favorable for Fe(II) to act as an electron donor. We propose and further discuss the fact that the formation of greigite from nanocrystalline mackinawite could result in H<span class="inline-formula"><sub>2</sub></span&gt; production as, for instance, observed for anoxic corrosion of zero-valent Fe at higher temperatures. Greigite has been designated in the literature either as an intermediate towards pyrite formation or as a mineralogical endmember in another reaction route. Our observations raise the question of the existence of such a reaction producing Fe<span class="inline-formula"><sub>3</sub></span>S<span class="inline-formula"><sub>4</sub></span&gt; and H<span class="inline-formula"><sub>2</sub></span&gt; in reducing sedimentary (micro)environments across geological times. In addition, the metallic character of mackinawite suggests that Fe(II) oxidation to Fe(III) by H<span class="inline-formula"><sup>+</sup></span&gt; in this mineral species could proceed without the need for another oxidizing agent. Although the possible formation of pyrite from greigite<span id="page136"/&gt; would require further studies on extended aging time and/or under more acid-sulfidic conditions, our findings could have implications for the understanding of the initial steps of the H<span class="inline-formula"><sub>2</sub></span>S pathway to pyrite.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-23T16:48:45+01:00</published>
            <updated>2026-03-23T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-123-2026</id>
            <title type="html">High-spatial-resolution oxygen isotopic analysis to distinguish natural from synthetic corundum
            </title>
            <link href="https://doi.org/10.5194/ejm-38-123-2026"/>
            <summary type="html">
                &lt;b&gt;High-spatial-resolution oxygen isotopic analysis to distinguish natural from synthetic corundum&lt;/b&gt;&lt;br&gt;
                Elena S. Sorokina, Axel K. Schmitt, Tobias Häger, and Jens Hopp&lt;br&gt;
                    Eur. J. Mineral., 38, 123&#8211;134, https://doi.org/10.5194/ejm-38-123-2026, 2026&lt;br&gt;
                Natural ruby and sapphire are of the rarest gemstones. To further enable their identification from synthetic analogues, this study explores secondary ionization mass spectrometry (SIMS) oxygen isotope analysis. SIMS &amp;#948;<sup>18</sup>O analysis of hydrothermal corundum yielded values between -7.84 &amp;#177; 0.13 &amp;#8240; and -14.54 &amp;#177; 0.13 &amp;#8240; (Vienna Standard Mean Ocean Water), which are atypical for natural corundum. SIMS &amp;#948;<sup>18</sup>O analysis of corundum thus has strong potential to distinguish synthetic and natural corundum.
            </summary>
            <content type="html">
                &lt;b&gt;High-spatial-resolution oxygen isotopic analysis to distinguish natural from synthetic corundum&lt;/b&gt;&lt;br&gt;
                Elena S. Sorokina, Axel K. Schmitt, Tobias Häger, and Jens Hopp&lt;br&gt;
                    Eur. J. Mineral., 38, 123&#8211;134, https://doi.org/10.5194/ejm-38-123-2026, 2026&lt;br&gt;
                <p>Gem-quality corundum varieties of ruby and sapphire are one of the most valuable and desired gemstones. Due to their rarity, new methods of synthesis and treatment were developed over the last decades, complicating the reliable identification between natural, treated, and synthetic specimens. Among the geochemical methods used for identification, trace element analysis using laser ablation inductively coupled plasma mass-spectrometry (LA-ICP-MS) is widely applied. However, solely relying on LA-ICP-MS trace element analysis for differentiation between natural and synthetic corundum origins, especially when grown by the hydrothermal method, can potentially lead to misidentifications. To further enable geochemical tracing of corundum, this study explores secondary ion mass spectrometry (SIMS) oxygen isotope analysis. High-spatial-resolution SIMS <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup>O</span&gt; analysis of hydrothermally synthesized corundum yielded values between <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">7.84</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.13</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="64pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="958a673c4f67de3905a28d5657be75e9"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00001.svg" width="64pt" height="10pt" src="ejm-38-123-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">14.54</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.13</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="ab6daf35aed639651ff8404470462157"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00002.svg" width="70pt" height="10pt" src="ejm-38-123-2026-ie00002.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; (relative to Vienna standard mean ocean water, VSMOW; 1 standard error) that are atypical for natural corundum. For flame fusion corundum, SIMS <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup>O</span&gt; analyses are in the range of <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">6.73</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.13</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="64pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="3834a1a04449a8fbaaff813f6fb73117"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00003.svg" width="64pt" height="10pt" src="ejm-38-123-2026-ie00003.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M6" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">17.46</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.13</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="65f1b16bd88375a589c97f86801cbe11"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00004.svg" width="70pt" height="10pt" src="ejm-38-123-2026-ie00004.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; for sapphires of blue, yellow, and orange colour and <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>+</mo><mn mathvariant="normal">28.51</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.11</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="9eb7d60b60105cd82df5a14bcc475656"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00005.svg" width="70pt" height="10pt" src="ejm-38-123-2026-ie00005.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M8" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>+</mo><mn mathvariant="normal">30.47</mn><mo>&amp;#177;</mo><mn mathvariant="normal">0.10</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="70pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="48389be6ae63b4c7f41343cc22b57feb"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-123-2026-ie00006.svg" width="70pt" height="10pt" src="ejm-38-123-2026-ie00006.png"/></svg:svg></span></span>&amp;#8201;&amp;#8240; for ruby, which, in both cases, are again atypical for natural corundum. SIMS <span class="inline-formula"><i>&amp;#948;</i><sup>18</sup>O</span&gt; analysis of corundum thus has strong potential to distinguish synthetic and natural corundum.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-18T16:48:45+01:00</published>
            <updated>2026-03-18T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-117-2026</id>
            <title type="html">IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) &#8211; Newsletter 89
            </title>
            <link href="https://doi.org/10.5194/ejm-38-117-2026"/>
            <content type="html">
                &lt;b&gt;IMA Commission on New Minerals, Nomenclature and Classification (CNMNC) – Newsletter 89&lt;/b&gt;&lt;br&gt;
                Ferdinando Bosi, Frédéric Hatert, Marco Pasero, and Stuart J. Mills&lt;br&gt;
                    Eur. J. Mineral., 38, 117&#8211;122, https://doi.org/10.5194/ejm-38-117-2026, 2026&lt;br&gt;
                
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-11T16:48:45+01:00</published>
            <updated>2026-03-11T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-103-2026</id>
            <title type="html">Hydrogen diffusion in hydrous minerals from Raman and NanoSIMS mapping &#8211; implications for isotopic characterization of fluid&#8211;rock interactions
            </title>
            <link href="https://doi.org/10.5194/ejm-38-103-2026"/>
            <summary type="html">
                &lt;b&gt;Hydrogen diffusion in hydrous minerals from Raman and NanoSIMS mapping – implications for isotopic characterization of fluid–rock interactions&lt;/b&gt;&lt;br&gt;
                Bruno Reynard, Jannick Ingrin, Anne-Céline Ganzhorn, Julie Jonfal, Hélène Pilorgé, Clémentine Fellah, Nadège Hilairet, and Laurent Remusat&lt;br&gt;
                    Eur. J. Mineral., 38, 103&#8211;116, https://doi.org/10.5194/ejm-38-103-2026, 2026&lt;br&gt;
                Interactions between minerals and water are fundamental to many geological processes on Earth, in meteorites, and on other planetary bodies, for instance, in the development of plate tectonics. In this study, we experimentally determine how quickly hydrogen isotopes are exchanged between minerals and fluids. We then explore how exchange rates can inform us about past interactions between rocks and water on the Earth and in meteorites using hydrogen isotope measurements in natural minerals.
            </summary>
            <content type="html">
                &lt;b&gt;Hydrogen diffusion in hydrous minerals from Raman and NanoSIMS mapping – implications for isotopic characterization of fluid–rock interactions&lt;/b&gt;&lt;br&gt;
                Bruno Reynard, Jannick Ingrin, Anne-Céline Ganzhorn, Julie Jonfal, Hélène Pilorgé, Clémentine Fellah, Nadège Hilairet, and Laurent Remusat&lt;br&gt;
                    Eur. J. Mineral., 38, 103&#8211;116, https://doi.org/10.5194/ejm-38-103-2026, 2026&lt;br&gt;
                <p>Hydrogen diffusion in major hydrous minerals determines the closure temperatures of isotopic exchange used to track fluid&amp;#8211;rock interactions. Deuterium&amp;#8211;hydrogen (D&amp;#8211;H) exchange was experimentally investigated between minerals and deuterated gas (D<span class="inline-formula"><sub>2</sub></span>) in an ambient-pressure furnace over the temperature range of 400&amp;#8211;650&amp;#8201;&amp;#176;C (tremolite, vesuvianite) and between minerals and D<span class="inline-formula"><sub>2</sub></span>O at high pressure (1.5&amp;#8211;3&amp;#8201;GPa) and temperature (315&amp;#8211;500&amp;#8201;&amp;#176;C) in a belt press (glaucophane, epidote). D&amp;#8201;<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M3" 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="e653eaf840568ee76bb20ba3bf368ae0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-103-2026-ie00001.svg" width="8pt" height="14pt" src="ejm-38-103-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;(D&amp;#8201;<span class="inline-formula">+</span>&amp;#8201;H) ratios in exchanged mineral grains were mapped using Raman spectroscopy calibrated by comparison with NanoSIMS analyses. Diffusion coefficients constrained by isotopic profiles were fitted to the Arrhenius equation <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M5" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi>D</mi><mrow><mi mathvariant="normal">D</mi><mspace linebreak="nobreak" width="0.125em"/><mo>/</mo><mspace width="0.125em" linebreak="nobreak"/><mi mathvariant="normal">H</mi></mrow></msub><mo>=</mo><msub><mi>D</mi><mn mathvariant="normal">0</mn></msub><msup><mi>e</mi><mrow><mo>(</mo><mo>-</mo><msub><mi mathvariant="normal">H</mi><mi mathvariant="normal">a</mi></msub><mo>/</mo><mi>R</mi><mi>T</mi><mo>)</mo></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="97pt" height="19pt" class="svg-formula" dspmath="mathimg" md5hash="3fe83e2149b022b24913ea994b1d1e58"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-103-2026-ie00002.svg" width="97pt" height="19pt" src="ejm-38-103-2026-ie00002.png"/></svg:svg></span></span>, where H<span class="inline-formula"><sub>a</sub></span&gt; is the activation enthalpy, and <span class="inline-formula"><i>D</i><sub>0</sub></span&gt; is the diffusion coefficient at infinite temperature <span class="inline-formula"><i>T</i></span>. The validity of intracrystalline diffusion laws from the literature is discussed with respect to the mechanical properties of hydrous minerals. Diffusion in tremolite is affected by intense cleavage, which reduces the effective grain size relative. High pressure appears to suppress cleavage opening in glaucophane. Results suggest that plasticity counteracts grain size reductions along cleavage planes in phyllosilicates. For vesuvianite, which lacks cleavage planes, intracrystalline diffusion is a valid assumption. In epidote, diffusivities are scattered over several orders of magnitude. Closure temperatures for hydrogen isotope diffusion were calculated and indicate that vesuvianite and phyllosilicates can record fluid&amp;#8211;rock interactions under regional metamorphic conditions. Amphiboles may retain information about relatively short-lived eruptive events. Spatially resolved measurements of hydrogen isotopic compositions in those minerals may reveal low-temperature (100&amp;#8201;<span class="inline-formula"><i><</i></span>&amp;#8201;<span class="inline-formula"><i>T</i>&amp;#8201;<i><</i></span>&amp;#8201;400&amp;#8201;&amp;#176;C) fluid&amp;#8211;rock interactions associated with slip along major faults and metamorphic terrane exhumation.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-03-05T16:48:45+01:00</published>
            <updated>2026-03-05T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-53-2026</id>
            <title type="html">Deciphering crystal growth in a sector-zoned interpenetration twin of loparite from Mt Khibiny (Kola Peninsula, Russia) through atomic-scale characterisation of growth sectors and twin boundaries
            </title>
            <link href="https://doi.org/10.5194/ejm-38-53-2026"/>
            <summary type="html">
                &lt;b&gt;Deciphering crystal growth in a sector-zoned interpenetration twin of loparite from Mt Khibiny (Kola Peninsula, Russia) through atomic-scale characterisation of growth sectors and twin boundaries&lt;/b&gt;&lt;br&gt;
                Nina Daneu, José Alberto Padrón-Navarta, Martin Šala, Kristina Mervič, Gerlinde Habler, Goran Dražič, Petruša Borštnar, Aleksander Rečnik, and Rainer Abart&lt;br&gt;
                    Eur. J. Mineral., 38, 53&#8211;73, https://doi.org/10.5194/ejm-38-53-2026, 2026&lt;br&gt;
                Loparite is a chemically complex perovskite oxide; the crystals often show zoning and develop as spinel-type interpenetration twins. Atomic-scale analyses of a sector-zoned twin from Mt Khibiny have revealed that cubic and octahedral sectors exhibit distinct elemental ordering, driven by differences in composition and slow cooling. The configuration of twin boundary contacts indicates twinning by nucleation, followed by independent growth of the domains in twin orientation from the melt.&amp;#160;
            </summary>
            <content type="html">
                &lt;b&gt;Deciphering crystal growth in a sector-zoned interpenetration twin of loparite from Mt Khibiny (Kola Peninsula, Russia) through atomic-scale characterisation of growth sectors and twin boundaries&lt;/b&gt;&lt;br&gt;
                Nina Daneu, José Alberto Padrón-Navarta, Martin Šala, Kristina Mervič, Gerlinde Habler, Goran Dražič, Petruša Borštnar, Aleksander Rečnik, and Rainer Abart&lt;br&gt;
                    Eur. J. Mineral., 38, 53&#8211;73, https://doi.org/10.5194/ejm-38-53-2026, 2026&lt;br&gt;
                <p>Loparite is a natural perovskite (ABO<span class="inline-formula"><sub>3</sub></span>) with a complex composition, essentially a solid solution between loparite(-Ce) (Na<span class="inline-formula"><sub>0.5</sub></span>Ce<span class="inline-formula"><sub>0.5</sub></span>TiO<span class="inline-formula"><sub>3</sub></span>), lueshite (NaNbO<span class="inline-formula"><sub>3</sub></span>), and perovskite (CaTiO<span class="inline-formula"><sub>3</sub></span>), with small amounts of many other elements. The majority of reported loparite crystals are spinel-type interpenetration twins with compositional zoning. Associated with the high variability of compositions, different crystal structures of loparite were described, and the origin of twinning has not been addressed so far.</p&gt;        <p>In this work, we studied a loparite twin composed of two symmetrically intergrown cuboctahedra. Microprobe analyses revealed that the cubic and octahedral growth sectors have slightly different compositions. According to atomic-scale analyses, the cubic sectors with a lower Na<span class="inline-formula">:</span>LREE ratio have a disordered orthorhombic structure, while the octahedral sectors with a higher Na<span class="inline-formula">:</span>LREE ratio show partial ordering of Na and light rare-earth elements along A-type lattice planes in the [001] direction. The degree of ordering was evaluated by quantitative high-angle annular dark-field scanning transmission electron microscopy (HAADF-STEM). Atomic-scale analyses of (111) and <span class="inline-formula"><i>{</i></span>112<span class="inline-formula"><i>}</i></span&gt; twin boundary (TB) contacts have shown that all TBs contain a 1&amp;#8211;2&amp;#8201;nm thin layer of an Si-rich amorphous phase.</p&gt;        <p>Our observations suggest that the loparite twin was established in the nucleation stage of crystallisation, followed by independent crystallisation of both twin domains from the melt. The initial crystal form was cubic; octahedral sectors evolved when the crystal size was still in the nanometre range, as a result of slow crystal growth. Differences in structural ordering between adjacent growth sectors developed during slow cooling due to the compositional variations. Our results imply that compositionally zoned crystals might show different structural ordering within single domains, which should be considered when interpreting bulk diffraction data of compositionally zoned perovskites.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-24T16:48:45+01:00</published>
            <updated>2026-02-24T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-75-2026</id>
            <title type="html">Crystal structure, chemical composition, and twinning of g&#246;tzenite and w&#246;hlerite from the <span style="" class="text">Fohberg</span> phonolite, Kaiserstuhl
            </title>
            <link href="https://doi.org/10.5194/ejm-38-75-2026"/>
            <summary type="html">
                &lt;b&gt;Crystal structure, chemical composition, and twinning of götzenite and wöhlerite from the Fohberg phonolite, Kaiserstuhl&lt;/b&gt;&lt;br&gt;
                Reinhard X. Fischer, Johannes Birkenstock, Georg Biskup, Lennart A. Fischer, Andreas Klügel, Shaghayegh Nezamabadi, and Simon Spürgin&lt;br&gt;
                    Eur. J. Mineral., 38, 75&#8211;101, https://doi.org/10.5194/ejm-38-75-2026, 2026&lt;br&gt;
                G&amp;#246;tzenite and w&amp;#246;hlerite were found as part of a fissure assemblage in the Fohberg phonolite (Kaiserstuhl, SW Germany) in close contact to each other. G&amp;#246;tzenite shows rotation twinning on [001], and w&amp;#246;hlerite shows reflection twinning on (100). G&amp;#246;tzenite represents a special case, where the twin domains are arranged in a certain way with the main axis <em>n</em><sub>x</sub&gt; of the optical indicatrix being parallel to the twin axis <strong>c</strong&gt; in both domains.
            </summary>
            <content type="html">
                &lt;b&gt;Crystal structure, chemical composition, and twinning of götzenite and wöhlerite from the Fohberg phonolite, Kaiserstuhl&lt;/b&gt;&lt;br&gt;
                Reinhard X. Fischer, Johannes Birkenstock, Georg Biskup, Lennart A. Fischer, Andreas Klügel, Shaghayegh Nezamabadi, and Simon Spürgin&lt;br&gt;
                    Eur. J. Mineral., 38, 75&#8211;101, https://doi.org/10.5194/ejm-38-75-2026, 2026&lt;br&gt;
                <p>G&amp;#246;tzenite and w&amp;#246;hlerite were found as part of a fissure assemblage in the Fohberg phonolite (Kaiserstuhl, SW Germany), in close association with natrolite and clinopyroxene (aegirine&amp;#8211;augite). Crystal grains were separated and investigated by single-crystal X-ray diffraction (SXRD), electron probe microanalysis (EPMA), and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS), showing the presence of two intimately intergrown phases, g&amp;#246;tzenite and w&amp;#246;hlerite. SXRD analyses showed that both minerals are twinned. G&amp;#246;tzenite (Na<span class="inline-formula"><sub>1.50</sub></span>Ca<span class="inline-formula"><sub>5.18</sub></span>Sr<span class="inline-formula"><sub>0.13</sub></span>Fe<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">0.03</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="18pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="31f53867b2d70e8e34fbd464badd021b"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-75-2026-ie00001.svg" width="18pt" height="17pt" src="ejm-38-75-2026-ie00001.png"/></svg:svg></span></span>Mn<span class="inline-formula"><sub>0.01</sub></span>Zr<span class="inline-formula"><sub>0.06</sub></span>La<span class="inline-formula"><sub>0.08</sub></span>Ce<span class="inline-formula"><sub>0.11</sub></span>Nd<span class="inline-formula"><sub>0.02</sub></span>Ti<span class="inline-formula"><sub>0.81</sub></span>Nb<span class="inline-formula"><sub>0.19</sub></span>(Si<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>7</sub></span>)<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>1.2</sub></span>F<span class="inline-formula"><sub>2.8</sub></span>) shows rotation twinning on [001] according to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M17" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mi mathvariant="bold-italic">a</mi><mo>-</mo><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">2</mn><mi mathvariant="bold-italic">c</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="53pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="2467cbe125168775b270e161f644cfaa"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-75-2026-ie00002.svg" width="53pt" height="14pt" src="ejm-38-75-2026-ie00002.png"/></svg:svg></span></span>, <span class="inline-formula">&amp;#8722;<strong><em>b</em></strong></span>, <span class="inline-formula"><strong><em>c</em></strong></span>, with contributions of 40&amp;#8201;% and 60&amp;#8201;% from the two twin domains, respectively. Applying the twin law to the diffraction analysis, the crystal structure was refined to <span class="inline-formula"><i>R</i></span>1 (<span class="inline-formula"><i>F</i></span>o&amp;#8201;<span class="inline-formula"><i>></i>4<i>&amp;#963;</i></span>&amp;#8201;(<span class="inline-formula"><i>F</i></span>o))&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;3.0&amp;#8201;%, with <span class="inline-formula"><i>a</i>=9.6191</span>(3)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>b</i>=5.7342</span>(2)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=7.3386</span>(2)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#945;</i>=89.986</span>(1)&amp;#176;, <span class="inline-formula"><i>&amp;#946;</i>=101.040</span>(1)&amp;#176;, <span class="inline-formula"><i>&amp;#947;</i>=100.485</span>(1)&amp;#176;, and <span class="inline-formula"><i>V</i>=390.40</span>(3)&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span&gt; in space group <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M33" display="inline" overflow="scroll" dspmath="mathml"><mrow><mi>P</mi><mspace width="0.125em" linebreak="nobreak"/><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="18pt" height="13pt" class="svg-formula" dspmath="mathimg" md5hash="f2bed5a7db1eec8dbb21a1fefad2ab29"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-75-2026-ie00003.svg" width="18pt" height="13pt" src="ejm-38-75-2026-ie00003.png"/></svg:svg></span></span>. W&amp;#246;hlerite (Na<span class="inline-formula"><sub>1.63</sub></span>Ca<span class="inline-formula"><sub>4.37</sub></span>Sr<span class="inline-formula"><sub>0.04</sub></span>Zr<span class="inline-formula"><sub>0.63</sub></span>Fe<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M38" display="inline" overflow="scroll" dspmath="mathml"><mrow><msubsup><mi/><mn mathvariant="normal">0.23</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="18pt" height="17pt" class="svg-formula" dspmath="mathimg" md5hash="5831138daf0e0d8c013d7a195bf20d00"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-75-2026-ie00004.svg" width="18pt" height="17pt" src="ejm-38-75-2026-ie00004.png"/></svg:svg></span></span>Mn<span class="inline-formula"><sub>0.09</sub></span>Ce<span class="inline-formula"><sub>0.01</sub></span>Ta<span class="inline-formula"><sub>0.01</sub></span>Nb<span class="inline-formula"><sub>0.79</sub></span>Ti<span class="inline-formula"><sub>0.20</sub></span>(Si<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>7</sub></span>)<span class="inline-formula"><sub>2</sub></span>O<span class="inline-formula"><sub>2.6</sub></span>F<span class="inline-formula"><sub>1.4</sub></span>) shows reflection twinning on (100) according to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M49" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mi mathvariant="bold-italic">a</mi><mo>-</mo><mi mathvariant="bold-italic">c</mi></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="35pt" height="8pt" class="svg-formula" dspmath="mathimg" md5hash="4abe2468c4b819ad16d7784298be1136"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-75-2026-ie00005.svg" width="35pt" height="8pt" src="ejm-38-75-2026-ie00005.png"/></svg:svg></span></span>, <span class="inline-formula"><strong><em>b</em></strong></span>, <span class="inline-formula"><strong><em>c</em></strong></span>, with contributions of 31&amp;#8201;% and 69% from the two twin domains, respectively, and with lattice parameters of <span class="inline-formula"><i>a</i>=10.842</span>(1)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>b</i>=10.249</span>(1)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>c</i>=7.2673</span>(8)&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#946;</i>=109.343</span>(4)&amp;#176;, and <span class="inline-formula"><i>V</i>=761.9</span>(2)&amp;#8201;&amp;#197;<span class="inline-formula"><sup>3</sup></span&gt; in the monoclinic space group <span class="inline-formula"><i>P</i></span>2<span class="inline-formula"><sub>1</sub></span>, refined to <span class="inline-formula"><i>R</i></span>1&amp;#8201;<span class="inline-formula">=</span>&amp;#8201;1.3&amp;#8201;%. Refractive indices of g&amp;#246;tzenite were measured using the immersion method yielding <span class="inline-formula"><i>n</i><sub><i>x</i></sub>=1.662</span>(2), <span class="inline-formula"><i>n</i><sub><i>y</i></sub>=1.663</span>(2), <span class="inline-formula"><i>n</i><sub><i>z</i></sub>=1.670</span>(2), and 2<span class="inline-formula"><i>V</i>=61</span>(2)&amp;#176;. Optical measurements on the twinned crystal were possible because of the coincidence of the two indicatrices related to each other by rotation about <span class="inline-formula"><i>n</i><sub><i>x</i></sub></span&gt; being parallel to [001], simulating a unique extinction behavior. W&amp;#246;hlerite could not be optically examined because of the polysynthetic twinning not showing this effect.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-02-24T16:48:45+01:00</published>
            <updated>2026-02-24T16:48:45+01:00</updated>
        </entry>
        <entry>
            <id>https://doi.org/10.5194/ejm-38-39-2026</id>
            <title type="html">Zhenruite, (MoO<sub>3</sub>)<sub>2</sub>&#8201;&#8901;&#8201;H<sub>2</sub>O, and tianhuixinite, (MoO<sub>3</sub>)<sub>3</sub>&#8201;&#8901;&#8201;H<sub>2</sub>O, two new minerals in the MoO<sub>3</sub>&#8211;MoO<sub>3</sub>&#8201;&#8901;&#8201;2H<sub>2</sub>O system
            </title>
            <link href="https://doi.org/10.5194/ejm-38-39-2026"/>
            <summary type="html">
                &lt;b&gt;Zhenruite, (MoO3)2 ⋅ H2O, and tianhuixinite, (MoO3)3 ⋅ H2O, two new minerals in the MoO3–MoO3 ⋅ 2H2O system&lt;/b&gt;&lt;br&gt;
                Xiangping Gu, Hexiong Yang, Ronald B. Gibbs, and Guanghua Liu&lt;br&gt;
                    Eur. J. Mineral., 38, 39&#8211;52, https://doi.org/10.5194/ejm-38-39-2026, 2026&lt;br&gt;
                Two new minerals, zhenruite, ideally (MoO<sub>3</sub>)<sub>2</sub>&amp;#183;H<sub>2</sub>O, and tianhuixinite, ideally (MoO<sub>3</sub>)<sub>3</sub>&amp;#183;H<sub>2</sub>O, are described. Zhenruite&amp;#160;is monoclinic with space group <em>P</em>2<sub>1</sub>/<em>m</em&gt; and unit-cell parameters <em>a</em&gt; = 9.6790(6), <em>b</em&gt; = 3.70653(19), <em>c</em&gt; = 7.1029(4) &amp;#197;, <em>&amp;#946;</em&gt; = 102.391(5)&amp;#176;, <em>V</em&gt; = 248.89(2) &amp;#197;<sup>3</sup>, and <em>Z</em&gt; =2. Tianhuixinite is hexagonal with space group <em>P</em>6<sub>3</sub>/<em>m</em&gt; and unit-cell parameters <em>a</em&gt; = 10.5963(12), <em>c</em&gt; = 3.7216(4) &amp;#197;, <em>V</em&gt; = 361.88(9) &amp;#197;<sup>3</sup>, and <em>Z</em&gt; =2.&amp;#160;
            </summary>
            <content type="html">
                &lt;b&gt;Zhenruite, (MoO3)2 ⋅ H2O, and tianhuixinite, (MoO3)3 ⋅ H2O, two new minerals in the MoO3–MoO3 ⋅ 2H2O system&lt;/b&gt;&lt;br&gt;
                Xiangping Gu, Hexiong Yang, Ronald B. Gibbs, and Guanghua Liu&lt;br&gt;
                    Eur. J. Mineral., 38, 39&#8211;52, https://doi.org/10.5194/ejm-38-39-2026, 2026&lt;br&gt;
                <p>Two new minerals, zhenruite, ideally (MoO<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>2</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O, and tianhuixinite, ideally (MoO<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>3</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O, were discovered, respectively, from the Freedom #2 mine in the central part of the Marysvale volcanic field, Utah, USA, and an unnamed short adit on the Summit group of claims near Cookes Peak, Luna County, New Mexico, USA. Zhenruite occurs as acicular or prismatic crystals (up to <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M19" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">0.06</mn><mo>&amp;#215;</mo><mn mathvariant="normal">0.01</mn><mo>&amp;#215;</mo><mn mathvariant="normal">0.01</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="89pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="c4c3ec84254bad8b9cff1299a428526a"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-39-2026-ie00001.svg" width="89pt" height="10pt" src="ejm-38-39-2026-ie00001.png"/></svg:svg></span></span>&amp;#8201;mm). Associated minerals include alunogen, anhydrite, coquimbite, fluorite, liangjunite, quartz, and raydemarkite. Zhenruite is colorless in transmitted light and transparent with a white streak and vitreous luster. It is brittle with a Mohs hardness of 1 <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M20" display="inline" overflow="scroll" dspmath="mathml"><mrow><mn mathvariant="normal">1</mn><mo>/</mo><mn mathvariant="normal">2</mn></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="20pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="2b1bbe9055f5be658c64af2614c32c50"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-39-2026-ie00002.svg" width="20pt" height="14pt" src="ejm-38-39-2026-ie00002.png"/></svg:svg></span></span>&amp;#8211;2; cleavage is perfect on <span class="inline-formula"><i>{</i></span>001<span class="inline-formula"><i>}</i></span>. The calculated density is 4.081&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. Tianhuixinite occurs as nanometric crystal aggregates, 10&amp;#8211;70&amp;#8201;<span class="inline-formula">&amp;#181;m</span&gt; in size, intergrown with virgilluethite. Associated minerals include barite, fluorite, ilsemannite, jordisite, powellite, pyrite, quartz, raydemarkite, sidwillite, and virgilluethite. Tianhuixinite is dark blue-green and translucent in transmitted light. It has a white streak and vitreous luster. Tianhuixinite is brittle with a Mohs hardness of <span class="inline-formula">&amp;#8764;2</span>; no cleavage was observed. The calculated density is 4.131&amp;#8201;g&amp;#8201;cm<span class="inline-formula"><sup>&amp;#8722;3</sup></span>. At room temperature, neither zhenruite nor tianhuixinite is soluble in water or hydrochloric acid. Electron microprobe analyses yielded an empirical formula (Mo<span class="inline-formula"><sub>1.00</sub></span>O<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>2</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O for zhenruite and (Mo<span class="inline-formula"><sub>1.00</sub></span>O<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>3</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O for tianhuixinite, calculated on the basis of 7 and 10 O apfu, respectively.</p&gt;        <p>Zhenruite and tianhuixinite are the natural counterparts of synthetic (MoO<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>2</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O and hexagonal (MoO<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>3</sub>&amp;#8901;</span>H<span class="inline-formula"><sub>2</sub></span>O, respectively. Zhenruite is monoclinic with 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="M42" 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="968f1f07f74c3749e34a2a7cba74ed2f"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-39-2026-ie00003.svg" width="23pt" height="14pt" src="ejm-38-39-2026-ie00003.png"/></svg:svg></span></span&gt; and unit-cell parameters <span class="inline-formula"><i>a</i>=9.6790(6)</span>, <span class="inline-formula"><i>b</i>=3.70653(19)</span>, <span class="inline-formula"><i>c</i>=7.1029(4)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>&amp;#946;</i>=102.391(5)</span>&amp;#176;, <span class="inline-formula"><i>V</i>=248.89(2)</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 is characterized by two kinds of topologically identical octahedral double chains extending along [010], one consisting of edge-sharing Mo1O<span class="inline-formula"><sub>6</sub></span&gt; octahedra only and the other Mo2O<span class="inline-formula"><sub>5</sub></span>(H<span class="inline-formula"><sub>2</sub></span>O) octahedra only. These two kinds of chains are linked together alternately through sharing corners to form layers parallel to (001), which are interconnected by hydrogen bands along [001]. Tianhuixinite is hexagonal with space group <span class="inline-formula"><i>P</i></span>6<span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M54" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi/><mn mathvariant="normal">3</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="762894c18a3005912d76a1e26c9b92a9"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ejm-38-39-2026-ie00004.svg" width="23pt" height="14pt" src="ejm-38-39-2026-ie00004.png"/></svg:svg></span></span&gt; and unit-cell parameters <span class="inline-formula"><i>a</i>=10.5963(12)</span>, <span class="inline-formula"><i>c</i>=3.7216(4)</span>&amp;#8201;&amp;#197;, <span class="inline-formula"><i>V</i>=361.88(9)</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 is composed of double chains of edge-sharing MoO<span class="inline-formula"><sub>6</sub></span&gt; octahedra extending along [001], which are corner-connected with one another to form hexagonal channels with H<span class="inline-formula"><sub>2</sub></span>O residing at the center. The double chains of edge-sharing MoO<span class="inline-formula"><sub>6</sub></span&gt; octahedra in zhenruite and tianhuixinite are topologically identical to those in molybdite and raydemarkite, and zhenruite can be regarded as a combination of molybdite and raydemarkite both structurally and chemically. The discovery of tianhuixinite implies the likelihood of finding the ammonia analogue, (MoO<span class="inline-formula"><sub>3</sub></span>)<span class="inline-formula"><sub>3</sub>&amp;#8901;</span>NH<span class="inline-formula"><sub>3</sub></span>, in nature.</p>
            </content>
            <author>
                <name>Copernicus Electronic Production Support Office</name>
            </author>
            <published>2026-01-15T16:48:45+01:00</published>
            <updated>2026-01-15T16:48:45+01:00</updated>
        </entry>
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