Raman spectroscopic peculiarities of Icelandic poorly crystalline minerals and their implications for Mars exploration

• Published in: Scientific Reports
• Main Authors: Muñoz-Iglesias, Victoria, Sánchez-García, Laura, Carrizo, Daniel, Molina, Antonio, Fernández-Sampedro, Maite, Prieto-Ballesteros, Olga
• Format: Text
• Language: English
• Published: Nature Publishing Group UK 2022
• Subjects: Article; Iceland
• Online Access: http://www.ncbi.nlm.nih.gov/pmc/articles/PMC8979959/; http://www.ncbi.nlm.nih.gov/pubmed/35379897; https://doi.org/10.1038/s41598-022-09684-x

In this work, we have analyzed natural samples collected at three hydrothermal areas of Iceland by Raman spectroscopy. The studied high-latitude regions are considered environmentally and mineralogically appropriate Martian analogues since they are rich in weathered basalts that have been altered by hydrothermalism to mineral phases such as silica, clay minerals, sulfates, oxides, and sulfur. The main objective of this work was to assess the relation of the spectroscopic signatures of alteration to hydrothermal processes and biomediation, considering previous studies focused on the detection of lipid biomarkers in the same samples. The recorded Raman spectra, taken with optical parameters similar to the ExoMars 2022 Raman spectrometer, showed structural modifications in all secondary minerals in the form of peak shifts (in the case of sulfur and clay minerals), changes in the relative ratio intensity (in anatase) and/or shape broadening (in sulfates and hematite). These results reveal the suitability of Raman spectroscopy to examine areas rich in water-altered minerals, where a mixture of crystalline and amorphous phases can co-exist. The detection of silica is singularly interesting since, on the one hand, it can imply the past existence of hydrothermal hot springs rich in nutrient and redox gradients and, on the other hand, provides excellent matrix for biosignature preservation. The data can be helpful as an astrobiological database for the forthcoming missions to Mars, where potential upwelling groundwater systems could have altered the mineral phases in a similar way to that observed in this work.