Raman study of the role of pressure and temperature on potential Martian mineralogy

Details Raman study of the role of pressure and temperature on potential Martian mineralogy Raman study of the role of pressure and temperature on potential Martian mineralogy

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..978m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.978

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Water is potentially the key to understanding the geological and biological evolution of Mars. Here, we analyses the structure of selected hydrated minerals such as phyllosilicates, hydrated sulphates, carbonates and mafic minerals with Raman spectroscopy in a Mars atmospheric simulation chamber (MASC) between +40 and -40°C and a dominantly CO2 atmosphere between 0.1-30 mbar. Temperature is shown to have a significant influence on Raman spectra emphasizing that quantitative analysis of mineralogy under ambient P-T conditions is needed prior to the use of the Raman techniques on planetary bodies.

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