Thermal Emission Spectra of Altered Tephras and Constraints on the Composition of Martian Dust

Details Thermal Emission Spectra of Altered Tephras and Constraints on the Composition of Martian Dust Thermal Emission Spectra of Altered Tephras and Constraints on the Composition of Martian Dust

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1936h&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1936

Computer Science

3

Scientific paper

We have acquired IR spectra of unaltered and altered tephras for use in
the interpretation of MGS TES data. We examine correlations between H2O
band strength and composition, and compare tephra spectra to a martian
surface dust spectrum from TES.

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