Characterization of Light-toned Sulfate and Hydrated Silica Layers at Juventae Chasma Using CRISM, OMEGA, HiRISE and CTX Images

Details Characterization of Light-toned Sulfate and Hydrated Silica Layers at Juventae Chasma Using CRISM, OMEGA, HiRISE and CTX Images Characterization of Light-toned Sulfate and Hydrated Silica Layers at Juventae Chasma Using CRISM, OMEGA, HiRISE and CTX Images

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2334b&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

4

Scientific paper

The light-toned deposits in inverted channels on the plains exhibit
hydrated Al/Si spectral features and color variations, whereas the
bright blocky mounds within the chasmata are spectrally dominated by
kieserite and contain sedimentary-type layers.

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