The effect of low temperature on the Raman spectra of calcium-rich sulfates on Mars

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Abstract

Raman spectra (532 nm diode laser) of gypsum, syngenite and görgeyite powders were studied from 273 to 83 K every -10 K. Although it was found that not all the Raman peaks are temperature-sensitive, the effect of temperature on the Raman signal of some bands was modelled. It was observed that the main bands of the three sulfates shift toward higher wavenumbers as temperature decreases. The strengthening of the bonds causes an increase in energy and, consequently, higher wavenumbers. However, -OH bands shift depending on the crystal structure they acquire as the temperature decreases, so not all -OH bands behave in the same way. Finally, the gypsum -OH bands change to more ordered crystalline structures with decreasing temperature, so their bandwidths become narrower and sharper.

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Huidobro, J., Aramendia, J., Arana, G., Hausrath, E. M., & Madariaga, J. M. (2023). The effect of low temperature on the Raman spectra of calcium-rich sulfates on Mars. Annals of Glaciology, 64(91), 57–62. https://doi.org/10.1017/aog.2023.29

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