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

Abstract 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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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2024-08-01
DOI
https://doi.org/10.1029/2024je008483
Citations
5
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
2.67

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article

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

Uta Rodehorst, Maximilian P. Reitze, I. Weber, Stephan Klemme et al.
5 citations
Journal of Geophysical Research Planets
Geological and Geochemical Analysis
2.67
article

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

Uta Rodehorst, Maximilian P. Reitze, I. Weber, Stephan Klemme, Christian J. Renggli, A. Morlok, H. Hiesinger, Jasper Berndt
article en
5 citations

Abstract

Abstract 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.

Journal of Geophysical Research PlanetsVol. 129(8)
University of Münster (DE), Max Planck Institute for Solar System Research (DE), Helmholtz-Institute Münster (DE)
Deutsche Forschungsgemeinschaft, Deutsches Zentrum für Luft- und Raumfahrt
Openalex Percentile: Top 11%
Geological and Geochemical Analysis
2.67
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Crystallographic and Mid‐Infrared Spectroscopic Properties of the CaS‐MgS Solid Solution — Uta Rodehorst, Maximilian P. Reitze, et al. · Journal of Geophysical Research Planets (2024) | TGRS Research Map | TGRS