Determining the Composition of Martian Dust and Soils Using MGS TES: Midinfrared Emission Spectra of Variable-Composition Palagonites

Details Determining the Composition of Martian Dust and Soils Using MGS TES: Midinfrared Emission Spectra of Variable-Composition Palagonites Determining the Composition of Martian Dust and Soils Using MGS TES: Midinfrared Emission Spectra of Variable-Composition Palagonites

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2123h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2123

Computer Science

1

Scientific paper

To identify palagonitic components on the martian surface it is
important to have spectra representative of the variability in
palagonite chemistry. Our objective is to create a set of midinfrared
spectra of palagonitic soils that exhibit such a range.

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