Thermal emission measurements (5-25 microns) of Hawaiian palagonitic soils with implications for Mars

Physics

Scientific paper

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Emissivity, Glass, Igneous Rocks, Infrared Spectra, Iron Oxides, Mineralogy, Spectral Signatures, Thermal Emission, Emission Spectra, Mars Surface, Planetary Geology, Soils, Weathering

Scientific paper

Careful laboratory studies have shown that the coloring agent in Mars analog Hawaiian palagonitic soils is nanophase iron oxide. We have measured the emissivity of two Mauna Kea palagonitic soils whose transmission spectra exhibit different spectral features and of a thermally-altered volcanic tephra sample that exhibits a wide range of crystallinity and degree of alteration (from black cinders to fully hematitic). Both of these samples may represent analogs for formation mechanisms involving the production of highly-altered secondary weathering products on Mars. The emission spectra of all samples were measured at the TES spectroscopy laboratory at Arizona State University. The data were converted to emissivity using blackbody measurements combined with measurements of each sample at different temperatures.

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