Thermal expansivity of geikielite and ilmenite utilizing in-situ synchrotron X-ray diffraction at high temperature

IF 1.3 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Acta Geochimica Pub Date : 2023-08-19 DOI:10.1007/s11631-023-00632-8
Jiamei Song, Dawei Fan, Shijie Huang, Shanrong Zhang, Mengzeng Wu, Wei Chen, Wenge Zhou
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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.

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利用原位同步辐射X射线衍射研究Gekielite和钛铁矿的高温热膨胀性
采用原位角色散同步加速器X射线衍射方法,在高达700K的高温和环境压力下,研究了gekielite(MgTiO3)和钛铁矿(FeTiO3)的晶胞参数和体积。在实验温度范围内未检测到相变。使用(Berman,1988年《汽油杂志》29:445–522。10.1093/岩石学/29.2.445)方程来拟合温度-体积数据,MgTiO3和FeTiO3在环境条件下的体积热膨胀系数(αV0)如下:2.55(6) × 10–5 K−1和2.82(10) × 10–5 K−1。我们推断,Fe2+(VI)的有效离子半径(0.78Å)比Mg2+(VI)(0.72Å)大,使得FeTiO3比MgTiO3具有更大的体积热膨胀率。同时,环境条件下的精细轴向热膨胀系数为αa0 = 0.74(3) × 10–5 K−1和αc0 = 1.08(5) × MgTiO3的a轴和c轴分别为10–5 K−1,αa0 = 0.95(5) × 10–5 K−1和αc0 = 0.92(12) × FeTiO3的a轴和c轴分别为10–5 K−1。MgTiO3的轴向热膨胀率是各向异性的,但FeTiO3的热膨胀率几乎是各向同性的。我们推断,MgTiO3和FeTiO3之间轴向热膨胀率不同的主要原因是MgTiO3中Mg-O键的热膨胀模式与FeTiO3中Fe–O键的热扩张模式不同。
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来源期刊
Acta Geochimica
Acta Geochimica GEOCHEMISTRY & GEOPHYSICS-
CiteScore
2.80
自引率
6.20%
发文量
1134
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.
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