Compositional Variability of Martian Olivines Using Mars Global Surveyor Thermal Emission Spectra

Details Compositional Variability of Martian Olivines Using Mars Global Surveyor Thermal Emission Spectra Compositional Variability of Martian Olivines Using Mars Global Surveyor Thermal Emission Spectra

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2049h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2049

Physics

4

Scientific paper

Data from the Mars Global Surveyor Thermal Emission Spectrometer have
spectral features in the 16 to 50 micron wavelength region correlating
to bands in olivines. Using laboratory spectra, outcrops of olivine were
mapped in the TES data, on the basis of their FeO content.

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