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实验确定的合成 MgSO<sub>4</sub>·4H<sub>2</sub>O(斯太克石)和 MgSO<sub>4</sub>·3H<sub>2</sub>O 的标准热力学性质:修订后的硫酸镁水合物内部一致热力学数据集。

Experimentally determined standard thermodynamic properties of synthetic MgSO(4)·4H(2)O (Starkeyite) and MgSO(4)·3H(2)O: a revised internally consistent thermodynamic data set for magnesium sulfate hydrates.

机构信息

Institute of Geosciences, Mineralogy, Friedrich-Schiller University, D-07745 Jena, Germany.

出版信息

Astrobiology. 2012 Nov;12(11):1042-54. doi: 10.1089/ast.2012.0823. Epub 2012 Oct 24.

Abstract

The enthalpies of formation of synthetic MgSO(4)·4H(2)O (starkeyite) and MgSO(4)·3H(2)O were obtained by solution calorimetry at T=298.15 K. The resulting enthalpies of formation from the elements are [Formula: see text] (starkeyite)=-2498.7±1.1 kJ·mol(-1) and [Formula: see text] (MgSO(4)·3H(2)O)=-2210.3±1.3 kJ·mol(-1). The standard entropy of starkeyite was derived from low-temperature heat capacity measurements acquired with a physical property measurement system (PPMS) in the temperature range 5 K<T<300 K: [Formula: see text] (starkeyite)=254.48±2.0 J·K(-1)·mol(-1). Additionally, differential scanning calorimetry (DSC) measurements with a Perkin Elmer Diamond DSC in the temperature range 270 K<T<300 K were performed to check the reproducibility of the PPMS measurements around ambient temperature. The experimental C(p) data of starkeyite between 229 and 303 K were fitted with a Maier-Kelley polynomial, yielding C(p)(T)=107.925+0.5532·T-1048894·T(-2). The hydration state of all Mg sulfate hydrates changes in response to local temperature and humidity conditions. Based on recently reported equilibrium relative humidities and the new standard properties described above, the internally consistent thermodynamic database for the MgSO(4)·nH(2)O system was refined by a mathematical programming (MAP) analysis. As can be seen from the resulting phase diagrams, starkeyite is metastable in the entire T-%RH range. Due to kinetic limitations of kieserite formation, metastable occurrence of starkeyite might be possible under martian conditions.

摘要

采用溶液量热法在 T=298.15 K 下测定了合成 MgSO(4)·4H(2)O(斯太利石)和 MgSO(4)·3H(2)O 的生成焓。元素生成焓的结果为 [Formula: see text](斯太利石)=-2498.7±1.1 kJ·mol(-1) 和 [Formula: see text](MgSO(4)·3H(2)O)=-2210.3±1.3 kJ·mol(-1)。斯太利石的标准熵是通过物理性质测量系统(PPMS)在 5 K<T<300 K 的温度范围内获得的低温热容测量值推导出来的:[Formula: see text](斯太利石)=254.48±2.0 J·K(-1)·mol(-1)。此外,在 270 K<T<300 K 的温度范围内,使用 Perkin Elmer Diamond DSC 进行了差示扫描量热法(DSC)测量,以检查周围温度下 PPMS 测量值的可重复性。在 229 和 303 K 之间的斯太利石实验 C(p)数据拟合了 Maier-Kelley 多项式,得到 C(p)(T)=107.925+0.5532·T-1048894·T(-2)。所有 Mg 硫酸盐水合物的水合状态都会根据当地温度和湿度条件而变化。基于最近报道的平衡相对湿度和上述新的标准性质,通过数学规划(MAP)分析对 MgSO(4)·nH(2)O 系统的内部一致热力学数据库进行了细化。从得出的相图可以看出,斯太利石在整个 T-%RH 范围内都是亚稳的。由于无水硫酸镁形成的动力学限制,在火星条件下可能会出现亚稳态的斯太利石。

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