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High-temperature Raman spectroscopy of lawsonite: constraints on bonding changes and dehydration lawsonite的高温拉曼光谱:键合变化和脱水的约束
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-10-11 DOI: 10.1007/s00269-026-01370-y
Connor A. Perkins, Quentin Williams

The Raman spectrum of lawsonite is characterized in situ at high temperatures through its dehydration temperature under vacuum. The structural reorganization associated with dehydration appears to initiate in the Si and Al-dominated layer of the structure, and proceeds between 525–550 and 725 °C. The loss of water from the structure appears complex, with the first structural reorganization associated with dehydration occurring at 550 °C, coexistence of lawsonite and the initial dehydration products up to 700 °C, and rapid disappearance of lawsonite between 675 and 725 °C. The dehydration is likely preceded by increased disorder of the hydroxyls within the structure. Indications of enhanced disorder of hydrogen ions at high temperatures include a dramatic decrease in intensity of an O–H librational vibration, large peak broadening of the principal hydroxyl stretch, and the disappearance of a shoulder on the strongest hydroxyl stretching vibration. The thermal anharmonicity of a range of Raman active modes is determined, and a revision to mode assignments is suggested based on the thermal shifts. Under low pressure conditions and our laboratory timescale, the observed product of lawsonite dehydration is the metastable pseudo-hexagonal polymorph of CaAl2Si2O8, dmisteinbergite. Production of dmisteinbergite through intermediate temperature lawsonite dehydration represents a previously unrecognized pathway for its formation, which previously has been limited to low-temperature hydrothermal environments, pyrometamorphic environments, materials rapidly quenching from melts (including in pseudotachylites), and as a retrograde phase from high grade metamorphic environments. The formation of metastable dmisteinbergite from lawsonite is likely facilitated by a topotactic relation between its layered structure and that of lawsonite.

通过对lawsonite在真空条件下的脱水温度,对其高温原位拉曼光谱进行了表征。与脱水相关的结构重组似乎始于结构的Si和al主导层,并在525-550和725°C之间进行。结构中水分的损失看起来很复杂,在550°C时,与脱水相关的第一次结构重组发生,在700°C时,lawsonite和初始脱水产物共存,在675至725°C之间,lawsonite迅速消失。脱水可能是由结构中羟基的紊乱增加引起的。氢离子在高温下无序性增强的迹象包括O-H振动强度急剧下降,主羟基拉伸峰大幅拓宽,最强羟基拉伸振动处肩部消失。确定了一系列拉曼主动模的热非调和性,并根据热位移对模式分配提出了修正建议。在低压条件下和实验室时间尺度下,观察到褐铁矿脱水产物为CaAl2Si2O8,二辉铝辉石的亚稳伪六方多晶。通过中温lawsonite脱水生产二辉石矿代表了一种以前未被认识到的形成途径,该途径以前仅限于低温热液环境,热变质环境,熔体快速淬火(包括伪石质)的材料,以及来自高品位变质环境的逆行相。铁榴辉石的层状结构与铁榴辉石的层状结构之间的地形关系可能促进了亚稳铁榴辉石的形成。
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引用次数: 0
Enrichment factor (EF) of REEs in soil fractions of different grain sizes: Malatya–Kuluncak, Başören Village 不同粒度土壤组分中稀土元素的富集因子(EF): Malatya-Kuluncak, Başören
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-10-02 DOI: 10.1007/s00269-026-01362-y
Güllü Kirat, Özlem Erdem

This study investigated the enrichment factor (EF) and geochemical relationships of rare earth elements (REEs) in different grain size fractions of soils collected from Başören village, Kuluncak district, Malatya province, Türkiye. A total of 22 surface soil samples were collected and separated into five grain size fractions (< 75, 75–150, 150–180, 180–250, and > 250 μm), yielding 110 samples. Concentrations of La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Yb, Lu, and Y were determined by ICP-MS. EF values ​​were calculated using Al as the reference element, and Pearson correlation was applied to evaluate the relationships between REEs. Strong positive correlations were observed among most REEs (r = 0.999–1.000, p < 0.01), whereas weaker correlations were shown between Eu and Gd elements and La, Ce, Pr, Nd, Sm, Tb, Dy, Ho, Yb, Lu, and Y elements. Moderately positive relationships were determined between Al and REEs, with coefficients of determination (R2) ranging from approximately 0.33 to 0.54, indicating that REE distributions are primarily controlled by aluminosilicate minerals and fine-grained fractions. EF values ​​varied between sampling areas and grain size fractions. While negligible to moderate enrichment was observed in most samples, significant to very high enrichment was observed in some samples, particularly for Gd, Tb, Dy, Ho, and Yb. Samples T16 and T20 showed the highest enrichment levels, with Gd reaching very high enrichment classes (EF = 20–40). The results show that the spatial distribution and enrichment patterns of rare earth elements are largely influenced by lithogenic sources and grain size-dependent mineralogical characteristics.

本文研究了基耶省马拉提亚省库伦卡克区Başören村不同粒度土壤中稀土元素的富集因子(EF)和地球化学关系。共收集了22个表层土壤样品,并将其分为5个粒径组(<; 75、75 - 150、150-180、180-250和>; 250 μm),得到110个样品。采用ICP-MS法测定La、Ce、Pr、Nd、Sm、Eu、Gd、Tb、Dy、Ho、Yb、Lu、Y的浓度。以Al为参考元素计算EF值,并应用Pearson相关性评价稀土元素之间的关系。大多数稀土元素与稀土元素呈显著正相关(r = 0.999 ~ 1.000, p < 0.01),而Eu和Gd元素与La、Ce、Pr、Nd、Sm、Tb、Dy、Ho、Yb、Lu和Y元素呈弱相关。Al与REE呈中等正相关,决定系数(R2)在0.33 ~ 0.54之间,表明稀土元素的分布主要受铝硅酸盐矿物和细粒组分的控制。EF值在不同的采样区域和不同的粒度分数之间存在差异。虽然在大多数样品中观察到可忽略到中等富集,但在一些样品中观察到显著到非常高的富集,特别是Gd, Tb, Dy, Ho和Yb。样品T16和T20的富集程度最高,Gd达到非常高的富集等级(EF = 20-40)。结果表明,稀土元素的空间分布和富集模式在很大程度上受成岩源和粒度相关矿物学特征的影响。
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引用次数: 0
Structural features and spectroscopy study of H-bearing arctite, BaCa7Na5(PO4)6F3, from the Khibiny alkaline massif, Kola Peninsula 科拉半岛希比尼碱性地块含h射影岩BaCa7Na5(PO4)6F3的结构特征及光谱研究
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-09-08 DOI: 10.1007/s00269-026-01367-7
G. S. Ilyin, E. A. Pankrushina, D. V. Deyneko, N. V. Chukanov, D. A. Mandrygina, S. A. Vozchikova, S. M. Aksenov

The crystal structure, infrared, Raman, excitation- and emission-mode photoluminescence spectra as well as thermal behavior of hydrogen- and REE-bearing natural arctite have been studied. The trigonal unit cell parameters are: a = 7.0773(1), c = 41.2197(6) Å, V = 1788.01(4) Å3; sp. gr. R(:stackrel{-}{3})m. The crystal structure was solved and refined to the final R = 2.02% based on 848 I > 3σ(I). Taking into account the IR spectroscopy data, the charge-balanced empirical formula calculated for 6 phosphorus atoms is (Z = 3): (H+,H3O+)0.88(Ca6.62Na4.40Ba1.00Ce0.07La0.03)Σ12.12(PO4)5.82(HPO4)0.18F2.85(OH)0.15. The crystal structure of arctite is characterized by the presence of anion-centered [F3M12] trimers (M = Na, Ca) composed of face-shared anion-centered FM6 octahedra. The simultaneous presence of basic (Ca2+···OH–) and acid (HPO42–, H3O+, H+) species is a specific feature of the studied H-bearing sample. Similar synthetic materials may be of practical interest as luminophores. Luminescent properties of the studied sample are related to the admixed Ce3+ and Sm3+ ions.

研究了含氢和稀土天然摩擦石的晶体结构、红外光谱、拉曼光谱、激发模式和发射模式光致发光光谱以及热行为。三角单元胞参数为:a = 7.0773(1), c = 41.2197(6) Å, V = 1788.01(4) Å3;sp. gr. R (:stackrel{-}{3}) m.对晶体结构进行求解和细化,最终得到R = 2.02% based on 848 I > 3σ(I). Taking into account the IR spectroscopy data, the charge-balanced empirical formula calculated for 6 phosphorus atoms is (Z = 3): (H+,H3O+)0.88(Ca6.62Na4.40Ba1.00Ce0.07La0.03)Σ12.12(PO4)5.82(HPO4)0.18F2.85(OH)0.15. The crystal structure of arctite is characterized by the presence of anion-centered [F3M12] trimers (M = Na, Ca) composed of face-shared anion-centered FM6 octahedra. The simultaneous presence of basic (Ca2+···OH–) and acid (HPO42–, H3O+, H+) species is a specific feature of the studied H-bearing sample. Similar synthetic materials may be of practical interest as luminophores. Luminescent properties of the studied sample are related to the admixed Ce3+ and Sm3+ ions.
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引用次数: 0
Capture of lanthanum atoms by the (111) twin boundary in fluorite: a DFT study 萤石中镧原子的(111)孪晶界俘获:DFT研究
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-08-28 DOI: 10.1007/s00269-026-01366-8
Ekaterina Y. Kotelevskaya, Boris B. Shkurskii, Elena A. Volkova, Vasilii O. Krivchuk, Daniil O. Poletaev, Artem R. Oganov

Ab initio calculations were performed to estimate the energy preference of Ca2+ substitution by La3+ with compensating incorporation of an additional F− ion at the (111) twin boundary of fluorite (CaF2). Model structures of polytypes and polysomes, which are periodic stacking faults within the cubic fluorite matrix, were constructed and optimized using density functional theory (DFT). Our results indicate that the twin boundary has a strong tendency to trap lanthanum cations. These findings suggest that the twin boundaries in CaF2 may act as active sites for the accumulation of rare-earth elements, providing potential routes for modifying the functional properties of the materials. Conversely, addition of lanthanoids may promote growth twinning of fluorite.

通过从头计算来估计La3+取代Ca2+的能量偏好,并在萤石(CaF2)的(111)孪晶界处补偿加入额外的F -离子。利用密度泛函理论(DFT)构建并优化了立方萤石基体中周期性层错的多型和多体模型结构。我们的结果表明,孪晶界有很强的捕获镧离子的倾向。这些发现表明,CaF2中的孪晶界可能是稀土元素积累的活性位点,为修饰材料的功能特性提供了潜在的途径。相反,类镧元素的加入可促进萤石的生长孪晶。
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引用次数: 0
High-temperature behavior of FeTiO3 and MgTiO3: in-situ synchrotron X-ray diffraction study FeTiO3和MgTiO3的高温行为:原位同步x射线衍射研究
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-08-10 DOI: 10.1007/s00269-026-01365-9
Kai Wang, Jingui Xu, Shijie Huang, Shanrong Zhang, Qifa Zhong, Wei Zhao, Dawei Fan

The high-temperature volumetric and axial thermal expansion behaviors of ilmenite (FeTiO3) and geikielite (MgTiO3) were examined up to 773 K using in situ synchrotron X-ray diffraction. No phase transitions were observed within the experimental temperature range. The temperature–volume data were fitted using the Berman (1988)’s equation, yielding V0 = 316.50(3) Å3 and αV0 = 3.73(4) × 10–5 K−1 for FeTiO3, and V0 = 308.20(1) Å3 and αV0 = 2.95(9) × 10–5 K−1 for MgTiO3. In addition, axial thermal expansion analysis showed that FeTiO3 has a0 = 5.0865(1) Å, αa0 = 1.41(1) × 10–5 K−1, c0 = 14.0858(4) Å, and αc0 = 0.92(2) × 10–5 K−1, while MgTiO3 has a0 = 5.0585(1) Å, αa0 = 0.85(3) × 10–5 K−1, c0 = 13.9084(4) Å, and αc0 = 1.23(3) × 10–5 K−1. The results demonstrate that FeTiO3 exhibits more stable volumetric expansion with increasing temperature than MgTiO3. However, FeTiO3 and MgTiO3 display opposite trends in axial expansion: the a-axis expands more than the c-axis in FeTiO3 (αa0/αc0 = 1.53), whereas in MgTiO3, the c-axis expands more (αa0/αc0 = 0.69). These differences mainly reflect the distinct nature of the A-site cations: the 3d electrons of Fe2+ affect the rigidity and thermal response of Fe–O and Ti–O bonds, while Fe-related magnetic exchange interactions and associated magnetoelastic coupling may further constrain Fe–O bond expansion and reduce the thermal expansion of FeTiO3.

{"title":"High-temperature behavior of FeTiO3 and MgTiO3: in-situ synchrotron X-ray diffraction study","authors":"Kai Wang,&nbsp;Jingui Xu,&nbsp;Shijie Huang,&nbsp;Shanrong Zhang,&nbsp;Qifa Zhong,&nbsp;Wei Zhao,&nbsp;Dawei Fan","doi":"10.1007/s00269-026-01365-9","DOIUrl":"10.1007/s00269-026-01365-9","url":null,"abstract":"<div><p>The high-temperature volumetric and axial thermal expansion behaviors of ilmenite (FeTiO<sub>3</sub>) and geikielite (MgTiO<sub>3</sub>) were examined up to 773 K using in situ synchrotron X-ray diffraction. No phase transitions were observed within the experimental temperature range. The temperature–volume data were fitted using the Berman (1988)’s equation, yielding <i>V</i><sub>0</sub> = 316.50(3) Å<sup>3</sup> and <i>α</i><sub><i>V</i>0</sub> = 3.73(4) × 10<sup>–5</sup> K<sup>−1</sup> for FeTiO<sub>3</sub>, and <i>V</i><sub>0</sub> = 308.20(1) Å<sup>3</sup> and <i>α</i><sub><i>V</i>0</sub> = 2.95(9) × 10<sup>–5</sup> K<sup>−1</sup> for MgTiO<sub>3</sub>. In addition, axial thermal expansion analysis showed that FeTiO<sub>3</sub> has <i>a</i><sub>0</sub> = 5.0865(1) Å, <i>α</i><sub><i>a</i>0</sub> = 1.41(1) × 10<sup>–5</sup> K<sup>−1</sup>, <i>c</i><sub>0</sub> = 14.0858(4) Å, and <i>α</i><sub><i>c</i>0</sub> = 0.92(2) × 10<sup>–5</sup> K<sup>−1</sup>, while MgTiO<sub>3</sub> has <i>a</i><sub>0</sub> = 5.0585(1) Å, <i>α</i><sub><i>a</i>0</sub> = 0.85(3) × 10<sup>–5</sup> K<sup>−1</sup>, <i>c</i><sub>0</sub> = 13.9084(4) Å, and <i>α</i><sub><i>c</i>0</sub> = 1.23(3) × 10<sup>–5</sup> K<sup>−1</sup>. The results demonstrate that FeTiO<sub>3</sub> exhibits more stable volumetric expansion with increasing temperature than MgTiO<sub>3.</sub> However, FeTiO<sub>3</sub> and MgTiO<sub>3</sub> display opposite trends in axial expansion: the <i>a</i>-axis expands more than the <i>c</i>-axis in FeTiO<sub>3</sub> (<i>α</i><sub><i>a</i>0</sub>/<i>α</i><sub><i>c</i>0</sub> = 1.53), whereas in MgTiO<sub>3</sub>, the <i>c</i>-axis expands more (<i>α</i><sub><i>a</i>0</sub>/<i>α</i><sub><i>c</i>0</sub> = 0.69). These differences mainly reflect the distinct nature of the A-site cations: the 3d electrons of Fe<sup>2+</sup> affect the rigidity and thermal response of Fe–O and Ti–O bonds, while Fe-related magnetic exchange interactions and associated magnetoelastic coupling may further constrain Fe–O bond expansion and reduce the thermal expansion of FeTiO<sub>3</sub>.</p></div>","PeriodicalId":20132,"journal":{"name":"Physics and Chemistry of Minerals","volume":"53 3","pages":""},"PeriodicalIF":1.5,"publicationDate":"2026-08-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148751940","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Study of strontium hexaferrite prepared by solid state reaction using celestite and hematite 天青石与赤铁矿固相反应制备六铁酸锶的研究
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-08-10 DOI: 10.1007/s00269-026-01364-w
J. B. Neto, C. H. N. Cordeiro, M. M. de Góis, J. Xavier, J. M. Soares

Strontium hexaferrite (SrM) powders were prepared by solid-state reaction using celestite and magnetite/hematite. Energy dispersive X-ray fluorescence spectrometry, X-ray diffractometry (XRD), scanning electron microscopy (SEM), and vibrating sample magnetometry were used for analyses. The precursor ores were purified by hand-sorting and magnetic separation. Magnetic separation yielded 75% magnetite and 25% hematite in iron ore. Strontium reached a single phase of (rm SrSO_4) via hand-sorting. XRD confirmed single-phase (rm SrFe_{12}O_{19}) sample with hexagonal symmetry (space group (rm P6_{3}/mmc)). EDS analyse confirmed that the percentage of elements is in agreement with the expected stoichiometry for the hexaferrite phase. Initial SrM sample exhibited magnetization at maximum field of (rm 56~emu/g) and coercive field of (rm 632~Oe). Although remanence and coercivity were lower than expected for the initial SrM sample, due to wide particle size distribution observed in SEM images, by optimizing synthesis parameters, particularly annealing at (950^circ )C, the coercivity increased by nearly eightfold, reaching 4.96 kOe. The sample annealed at 950 (^circ )C also exhibited a maximum energy product of (rm (BH)_{max}approx 3.20~MGOe) and an estimated magnetocrystalline anisotropy constant of (rm K_1sim 3.6times 10^6~erg/cm^3). Microstructural evidence confirmed the predominance of particles in the monodomain regime, which justifies the increase in the coercive field. The results demonstrate that microstructural control is decisive for tuning the magnetic response of SrM, enabling the large-scale viability of this synthesis route for the production of high-coercivity hexaferrites, using a direct mixture of minerals instead of conventional industrial reagents.

{"title":"Study of strontium hexaferrite prepared by solid state reaction using celestite and hematite","authors":"J. B. Neto,&nbsp;C. H. N. Cordeiro,&nbsp;M. M. de Góis,&nbsp;J. Xavier,&nbsp;J. M. Soares","doi":"10.1007/s00269-026-01364-w","DOIUrl":"10.1007/s00269-026-01364-w","url":null,"abstract":"<div><p>Strontium hexaferrite (SrM) powders were prepared by solid-state reaction using celestite and magnetite/hematite. Energy dispersive X-ray fluorescence spectrometry, X-ray diffractometry (XRD), scanning electron microscopy (SEM), and vibrating sample magnetometry were used for analyses. The precursor ores were purified by hand-sorting and magnetic separation. Magnetic separation yielded 75% magnetite and 25% hematite in iron ore. Strontium reached a single phase of <span>(rm SrSO_4)</span> via hand-sorting. XRD confirmed single-phase <span>(rm SrFe_{12}O_{19})</span> sample with hexagonal symmetry (space group <span>(rm P6_{3}/mmc)</span>). EDS analyse confirmed that the percentage of elements is in agreement with the expected stoichiometry for the hexaferrite phase. Initial SrM sample exhibited magnetization at maximum field of <span>(rm 56~emu/g)</span> and coercive field of <span>(rm 632~Oe)</span>. Although remanence and coercivity were lower than expected for the initial SrM sample, due to wide particle size distribution observed in SEM images, by optimizing synthesis parameters, particularly annealing at <span>(950^circ )</span>C, the coercivity increased by nearly eightfold, reaching 4.96 kOe. The sample annealed at 950 <span>(^circ )</span>C also exhibited a maximum energy product of <span>(rm (BH)_{max}approx 3.20~MGOe)</span> and an estimated magnetocrystalline anisotropy constant of <span>(rm K_1sim 3.6times 10^6~erg/cm^3)</span>. Microstructural evidence confirmed the predominance of particles in the monodomain regime, which justifies the increase in the coercive field. The results demonstrate that microstructural control is decisive for tuning the magnetic response of SrM, enabling the large-scale viability of this synthesis route for the production of high-coercivity hexaferrites, using a direct mixture of minerals instead of conventional industrial reagents.</p></div>","PeriodicalId":20132,"journal":{"name":"Physics and Chemistry of Minerals","volume":"53 3","pages":""},"PeriodicalIF":1.5,"publicationDate":"2026-08-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00269-026-01364-w.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"148751941","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Simulating forsterite surfaces: localised chemistry and surface development under high temperatures 模拟forsterite表面:局部化学和高温下的表面发展
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-07-24 DOI: 10.1007/s00269-026-01359-7
Joshua M. R. Muir, Yi Wang, Feiwu Zhang

Grain boundaries are an important part of many polycrystalline mineral aggregates, possessing unique geometries and chemistries but they are often poorly understood due to the many complexities of studying such large geometrically diverse regions. In this work we shall examine the surfaces of the mineral forsterite in order to understand their controlling behaviour and mechanisms. We shall use a combination of density functional theory and both machine learning and classically trained forcefields. We find that for purposes of partitioning and surface energies most grain boundaries are similar to their constituent planar surfaces. Our main finding is that the relative energies of forsterite surfaces are highly sensitive to T and P and that their planar distributions are not static in real environments. Increasing T at low P can lead to growth of (010) surfaces while increasing T and P together can lead to the growth of (111) surfaces. In mantle conditions we predict a strong favourability of (111) surfaces that increases with depth but with large, sometimes non-monotonic shifts in the favourability of other surfaces. We also demonstrate that changing the surface distribution can lead to changes in crystal properties. The high temperature stabilisation of (010) is driven by a novel collective motion of Mg atoms along [100] channels which will also lead to a large, non-linear, anisotropic increase in grain boundary diffusion as (010) surfaces grow with temperature. We show that partitioning of water to forsterite surfaces is highly surface specific and driven by local chemistry enabling the possibility of hidden reservoirs in the Earth produced by changing surface plane distributions.

晶界是许多多晶矿物聚集体的重要组成部分,具有独特的几何和化学性质,但由于研究如此大的几何多样性区域的许多复杂性,它们往往知之甚少。在这项工作中,我们将检查矿物的表面,以了解其控制行为和机制。我们将使用密度泛函理论与机器学习和经典训练力场的结合。我们发现,在分配和表面能方面,大多数晶界与其组成的平面相似。我们的主要发现是,forsterite表面的相对能量对T和P高度敏感,并且它们的平面分布在实际环境中不是静态的。在低P时增加T可导致(010)表面的生长,同时增加T和P可导致(111)表面的生长。在地幔条件下,我们预测(111)表面的有利度随着深度的增加而增加,但其他表面的有利度会发生大的、有时是非单调的变化。我们还证明了改变表面分布可以导致晶体性质的变化。(010)的高温稳定是由Mg原子沿着[100]通道的新集体运动驱动的,这也将导致(010)表面随着温度的增长而晶界扩散的大量非线性各向异性增加。研究表明,水在复辉石表面的分配具有高度的表面特异性,并受当地化学物质的驱动,从而使地球上通过改变表面分布产生隐藏储层的可能性成为可能。
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引用次数: 0
Laser thermal decomposition of Fe3O4 to metallic iron under vacuum: experimental and thermodynamic investigation 真空条件下Fe3O4激光热分解成金属铁的实验与热力学研究
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-07-23 DOI: 10.1007/s00269-026-01356-w
Xiaohu Zhang, Guangshi Li, Wenyu Xie, Changyuan Li, Zhongya Pang, Xingli Zou, Qian Xu, Xionggang Lu

In-situ manufacturing and resource utilization on the lunar surface present a core challenge for establishing a sustainable lunar base, where the self-sufficiency of metal materials is particularly critical. Therefore, this study presented a novel method for extracting metallic iron from Fe3O4 via laser vacuum (1.0 × 10− 3 Pa) high-temperature (1930 K to 2360 K) decomposition, which could serve as a reference for in-situ metal extraction on the Moon. First, the feasibility of this approach was verified through thermodynamic calculations. Subsequently, the effects of laser power and irradiation time on the vacuum smelting process of Fe3O4 were systematically investigated. The results indicated that the content of metallic iron in the product reached its maximum value (31.71%) at a laser power of 800 W and an irradiation time of 4 min. Furthermore, the distribution, morphology, and particle size of metallic iron in the product were investigated by scanning electron microscopy and X-ray computed tomography. The metallic iron was primarily enriched in the lower region of the product, presenting as aggregates of irregular fine particles. The particle size distribution was predominantly in the range of 10 to 100 μm (98%), with minor amounts in the 100 to 200 μm (1%) and 200 to 500 μm (1%) ranges.

月球表面的原位制造和资源利用是建立可持续月球基地的核心挑战,其中金属材料的自给自足尤为关键。因此,本研究提出了一种通过激光真空(1.0 × 10−3 Pa)高温(1930 K ~ 2360 K)分解从Fe3O4中提取金属铁的新方法,可为月球上的原位金属提取提供参考。首先,通过热力学计算验证了该方法的可行性。随后,系统地研究了激光功率和辐照时间对Fe3O4真空熔炼过程的影响。结果表明,当激光功率为800 W,照射时间为4 min时,产物中金属铁的含量达到最大值(31.71%)。此外,通过扫描电子显微镜和x射线计算机断层扫描研究了产品中金属铁的分布、形态和粒度。金属铁主要富集在产品的下部区域,表现为不规则细颗粒的聚集体。粒径分布以10 ~ 100 μm(98%)为主,100 ~ 200 μm(1%)和200 ~ 500 μm(1%)为少量;
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引用次数: 0
On the color of a large dark-purple crystal of zircon from Afghanistan 来自阿富汗的一大块深紫色锆石晶体的颜色
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-07-16 DOI: 10.1007/s00269-026-01352-0
Michail Taran, Volodymyr Khomenko, Ievgen Naumenko, Jörg Nissen, Martin Kutzschbach

Optical absorption spectroscopic investigation of a zircon from Afghanistan, unique in both size and color, show evidence that it represents a new type of purple color in this mineral. By microprobe and laser ablation-inductively coupled plasm (LA-ICP-MS) mass spectrometry analyses, the material is nearly pure ZrSiO4. The contents of Nb, P, F, Na and Mn are under the detection limits in all point analyses. The mean values of K, Ca, Ti, Sm, Gd, Pb and Ho contents are below 0.001 apfu. The dark-purple, nearly black color of the zircon is thermally unstable. At annealing from 400 to 900 °C it gradually vanishes due to decrease of intensities of the high-energy absorption edge, the broad absorption bands with maxima at ~ 17,970 and 23,900 cm− 1 (E⊥c) and ~ 18,620, 23,680 and 26,240 cm− 1 (E||c). Intensities of the weak narrow lines of absorption, which are very likely caused by electronic spin-forbidden ff-transitions of uranium and REE ions, remain unchanged. The origin of the zircon is unclear. By 206Pb/238U radiometric age ~ 1909 million years, it is Proterozoic.

对一颗来自阿富汗的锆石的光学吸收光谱研究表明,它的大小和颜色都很独特,表明它代表了这种矿物中一种新的紫色。通过微探针和激光烧蚀-电感耦合质谱(LA-ICP-MS)分析,材料接近纯ZrSiO4。各点分析中Nb、P、F、Na、Mn的含量均在检出限以内。K、Ca、Ti、Sm、Gd、Pb、Ho含量平均值均低于0.001 apfu。深紫色,近乎黑色的锆石是热不稳定的。在400°C至900°C退火时,由于高能吸收边强度的降低,它逐渐消失,宽吸收带的最大值在~ 17,970和23,900 cm−1 (E⊥C)和~ 18,620,23,680和26,240 cm−1 (E⊥C)。弱窄吸收谱线的强度保持不变,这很可能是由铀和稀土离子的电子自旋禁止跃迁引起的。锆石的来源尚不清楚。206Pb/238U辐射年龄~ 1909亿年,属于元古代。
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引用次数: 0
Investigating stability in shock compressed europium- and cerium-doped cryptomelane K-OMS-2 through post-shock spectroscopy and microscopy 通过冲击后光谱和显微镜研究冲击压缩铕和铈掺杂隐黑烷K-OMS-2的稳定性
IF 1.5 4区 地球科学 Q4 MATERIALS SCIENCE, MULTIDISCIPLINARY Pub Date : 2026-07-16 DOI: 10.1007/s00269-026-01361-z
Morgan Gray, Jack Gugino, Mithun Bhowmick, Catherine Almquist, Dhanalakshmi Sellan, Mark P. S. Krekeler

Cryptomelane (K-OMS-2) (K(Mn4+, Mn2+)8O16) is a manganese-oxide mineral that is abundant in soils and rock coatings globally and is gaining importance in materials science and industrial mineralogy. The crystal structure is composed of 2 × 2 octahedra that creates a tunnel space for K+. Low-weight percent (wt%) europium (Eu)-doped, high-wt% Eu-doped, low-wt% cerium (Ce)-doped, and high-wt% Ce-doped cryptomelane were synthesized for dynamic shock compression experiments using laser-driven flyer plates. Powder X-ray diffraction (XRD), high resolution inductively coupled plasma mass spectroscopy (HR-ICP-MS), transmission electron microscopy (TEM), and Raman spectroscopy (RS) were utilized to characterize the materials pre-shock. TEM and RS analysis of post-shocked material found that high-wt% Eu- and high-wt% Ce-cryptomelane were the most resistant to shock, showing the least amount of peak changes in RS and few amorphous regions in TEM. RS and TEM indicate disorder and defects are present in both high-wt% versions, such as changes in Mn–O bond length, wavy lattice fringes, and amorphous regions near the crystal surface. This study concludes that doped cryptomelane is more resistant to shock compression than unmodified cryptomelane. This study supports the previously proposed thixotropic rebound model as the proposed mechanism for cryptomelane’s shock resistance. During the shock wave, the nanoporosity of the material allows for the material to compress as the shock wave passes through the crystals before relaxing into a similar position as the original state. The addition of higher bond strength metals appears to enhance this overall effect. The results provide context for new material applications and future molecular dynamic modeling.

隐黑烷(K- om -2) (K(Mn4+, Mn2+)8O16)是一种富含锰的氧化矿物,在全球土壤和岩石涂层中广泛存在,在材料科学和工业矿物学中具有重要意义。晶体结构由2 × 2的八面体组成,为K+创造了一个隧道空间。在激光驱动飞片上合成了低重量% (wt%)掺铕、高重量%掺铕、低重量%掺铈和高重量%掺Ce的暗色烯,用于动态激波压缩实验。利用粉末x射线衍射(XRD)、高分辨率电感耦合等离子体质谱(HR-ICP-MS)、透射电子显微镜(TEM)和拉曼光谱(RS)对材料的预冲击进行了表征。对受冲击后材料的TEM和RS分析发现,高wt% Eu-和高wt% ce -隐黑烷的抗冲击能力最强,其RS峰变化最小,TEM中无定形区较少。红外光谱和透射电镜显示,在两个wt%高的版本中都存在无序和缺陷,如Mn-O键长度的变化,波浪形晶格条纹和晶体表面附近的非晶态区域。本研究的结论是,掺杂的隐黑素比未修饰的隐黑素更能抵抗冲击压缩。本研究支持先前提出的触变回弹模型作为隐黑素抗冲击的机制。在冲击波期间,材料的纳米多孔性允许材料在冲击波穿过晶体时压缩,然后放松到与原始状态相似的位置。添加更高结合强度的金属似乎增强了这种整体效果。结果为新材料的应用和未来的分子动力学建模提供了背景。
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Physics and Chemistry of Minerals
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