Determining the Composition of Martian Dust and Soils Using MGS TES: Midinfrared Emission Spectra of Variable-Composition Palagonites
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.
Lunar and Planetary Science Conference
- Pub Date:
- March 2001