X-ray diffraction as a function of temperature for Fo92-Fa8: implications for the hermean surface.

Details X-ray diffraction as a function of temperature for Fo92-Fa8: implications for the hermean surface. X-ray diffraction as a function of temperature for Fo92-Fa8: implications for the hermean surface.

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1435f&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1435

Physics

Scientific paper

It is well known that the surface of Mercury shows temperature variations extremely large at specific locations [1]. Such a range can cause strong crystal structure changes and, as a consequence, the detected spectral signature could be significantly affected. Here we investigated the low-high temperature behaviour of one of the olivine, which has been recently considered as a possible constituent of the Mercury surface [2]. Aim of the work is to determine which expansion the olivine undergoes within a temperature range typical of the Mercury surface in order to verify which could be the effect of thermal expansion on a spectra.

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