CaS-MgS 固溶体的晶体学和中红外光谱特性

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Maximilian P. Reitze, Christian Renggli, Andreas Morlok, Iris Weber, Uta Rodehorst, Jasper Berndt, Stephan Klemme, Harald Hiesinger
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引用次数: 0

摘要

我们合成了硫化物 CaS(老汉岩)和 MgS(宁宁岩)之间的固溶体。电子微探针和 X 射线衍射显示合成后的样品均匀纯净。计算得出的晶格参数与早期文献数据相吻合。样品的中红外光谱分析显示,生成的硫化物很脆弱,交替速度非常快。不过,我们还是能够提供所有样品的清晰反射光谱。未改变样品的光谱没有显示峰值或波段,但在 7.0 至 12.5 μm 的分析光谱范围内有一个相当稳定的光谱。改变后的光谱包含硫酸盐和碳酸盐的特征,可能还有其他化合物。收集到的数据有助于了解所研究的硫化物的形成条件,因为它表明 CaS-MgS 系统中的溶胶存在于 1000°C 至 1200°C 之间。此外,红外数据将有助于改进对小行星或水星等可能被含硫化物物质覆盖的行星天体的中红外遥感。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Crystallographic and Mid-Infrared Spectroscopic Properties of the CaS-MgS Solid Solution

Crystallographic and Mid-Infrared Spectroscopic Properties of the CaS-MgS Solid Solution

We synthesized the solid solution between the sulfides CaS (oldhamite) and MgS (niningerite). Electron microprobe and X-ray diffraction showed homogeneous and pure samples after the synthesis. The calculated lattice parameters fit to earlier literature data. Mid-infrared spectroscopy of the samples reveal that the produced sulfides were fragile and tend to alternate very fast. However, we were able to provide clean reflectance spectra of all samples. The spectra of un-altered samples show no peaks or bands but a rather constant spectrum within the analyzed spectral range between 7.0 and 12.5 μm. The altered spectra contain signatures of sulfates and carbonates and probably further compounds. The gathered data help to understand the formation conditions of the studies sulfides as it shows that the solvus exists in the CaS-MgS system between 1000°C and 1200°C. In addition, the infrared data will help to improve remote sensing in the mid-infrared of planetary objects that might be covered with sulfide containing material like asteroids or Mercury.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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