{"title":"Thermal expansivity of geikielite and ilmenite utilizing in-situ synchrotron X-ray diffraction at high temperature","authors":"Jiamei Song, Dawei Fan, Shijie Huang, Shanrong Zhang, Mengzeng Wu, Wei Chen, Wenge Zhou","doi":"10.1007/s11631-023-00632-8","DOIUrl":null,"url":null,"abstract":"<div><p>The unit-cell parameters and volumes of geikielite (MgTiO<sub>3</sub>) and ilmenite (FeTiO<sub>3</sub>) were investigated at high temperatures up to 700 K and ambient pressure, using in-situ angle-dispersive synchrotron X-ray diffraction. No phase transition was detected over the experimental temperature range. Using (Berman in J Petrol 29:445–522, 1988. 10.1093/petrology/29.2.445) equations to fit the temperature-volume data, the volumetric thermal expansion coefficients at ambient conditions (<i>α</i><sub><i>V</i>0</sub>) of MgTiO<sub>3</sub> and FeTiO<sub>3</sub> were obtained as follows: 2.55 (6) × 10<sup>–5</sup> K<sup>−1</sup> and 2.82 (10) × 10<sup>–5</sup> K<sup>−1</sup>, respectively. We infer that the larger effective ionic radius of Fe<sup>2+</sup>(VI) (0.78 Å) than that of Mg<sup>2+</sup>(VI) (0.72 Å) renders FeTiO<sub>3</sub> has a larger volumetric thermal expansivity than MgTiO<sub>3</sub>. Simultaneously, the refined axial thermal expansion coefficients under ambient conditions are <i>α</i><sub><i>a</i>0</sub> = 0.74 (3) × 10<sup>–5</sup> K<sup>−1</sup> and <i>α</i><sub><i>c</i>0</sub> = 1.08 (5) × 10<sup>–5</sup> K<sup>−1</sup> for the <i>a</i>-axis and <i>c</i>-axis of MgTiO<sub>3</sub>, respectively, and <i>α</i><sub><i>a</i>0</sub> = 0.95 (5) × 10<sup>–5</sup> K<sup>−1</sup> and <i>α</i><sub><i>c</i>0</sub> = 0.92 (12) × 10<sup>–5</sup> K<sup>−1</sup> for the <i>a</i>-axis and <i>c</i>-axis of FeTiO<sub>3</sub>, respectively. The axial thermal expansivity of MgTiO<sub>3</sub> is anisotropic, but that of FeTiO<sub>3</sub> is nearly isotropic. We infer that the main reason for the different axial thermal expansivity between MgTiO<sub>3</sub> and FeTiO<sub>3</sub> is that the thermal expansion mode of the Mg-O bond in MgTiO<sub>3</sub> is different from that of the Fe–O bonds in FeTiO<sub>3</sub>.</p></div>","PeriodicalId":7151,"journal":{"name":"Acta Geochimica","volume":"42 6","pages":"988 - 997"},"PeriodicalIF":1.4000,"publicationDate":"2023-08-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Geochimica","FirstCategoryId":"1089","ListUrlMain":"https://link.springer.com/article/10.1007/s11631-023-00632-8","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The unit-cell parameters and volumes of geikielite (MgTiO3) and ilmenite (FeTiO3) were investigated at high temperatures up to 700 K and ambient pressure, using in-situ angle-dispersive synchrotron X-ray diffraction. No phase transition was detected over the experimental temperature range. Using (Berman in J Petrol 29:445–522, 1988. 10.1093/petrology/29.2.445) equations to fit the temperature-volume data, the volumetric thermal expansion coefficients at ambient conditions (αV0) of MgTiO3 and FeTiO3 were obtained as follows: 2.55 (6) × 10–5 K−1 and 2.82 (10) × 10–5 K−1, respectively. We infer that the larger effective ionic radius of Fe2+(VI) (0.78 Å) than that of Mg2+(VI) (0.72 Å) renders FeTiO3 has a larger volumetric thermal expansivity than MgTiO3. Simultaneously, the refined axial thermal expansion coefficients under ambient conditions are αa0 = 0.74 (3) × 10–5 K−1 and αc0 = 1.08 (5) × 10–5 K−1 for the a-axis and c-axis of MgTiO3, respectively, and αa0 = 0.95 (5) × 10–5 K−1 and αc0 = 0.92 (12) × 10–5 K−1 for the a-axis and c-axis of FeTiO3, respectively. The axial thermal expansivity of MgTiO3 is anisotropic, but that of FeTiO3 is nearly isotropic. We infer that the main reason for the different axial thermal expansivity between MgTiO3 and FeTiO3 is that the thermal expansion mode of the Mg-O bond in MgTiO3 is different from that of the Fe–O bonds in FeTiO3.
期刊介绍:
Acta Geochimica serves as the international forum for essential research on geochemistry, the science that uses the tools and principles of chemistry to explain the mechanisms behind major geological systems such as the Earth‘s crust, its oceans and the entire Solar System, as well as a number of processes including mantle convection, the formation of planets and the origins of granite and basalt. The journal focuses on, but is not limited to the following aspects:
• Cosmochemistry
• Mantle Geochemistry
• Ore-deposit Geochemistry
• Organic Geochemistry
• Environmental Geochemistry
• Computational Geochemistry
• Isotope Geochemistry
• NanoGeochemistry
All research articles published in this journal have undergone rigorous peer review. In addition to original research articles, Acta Geochimica publishes reviews and short communications, aiming to rapidly disseminate the research results of timely interest, and comprehensive reviews of emerging topics in all the areas of geochemistry.