The variable spectrum of kieserite: Grain size and temperature effects

Details The variable spectrum of kieserite: Grain size and temperature effects The variable spectrum of kieserite: Grain size and temperature effects

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1706j&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1706

Computer Science

Scientific paper

Compositional analysis of the Martian and Europan surfaces often relies on remote sensing using such imaging spectrometers as MRO CRISM, Mars Express OMEGA and Galileo NIMS. To enhance their scientific returns, well-characterized laboratory spectra are required. Several variables affect the observed spectra that must be understood if the return data are to be fully interpreted. We have quantified the effects of temperature and grain size on the kieserite (MgSO4•H2O) spectrum. While only temperature seems to affect the band position, both grain size and temperature alter the band depths and band shapes.

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