Charge-coupled device imaging spectroscopy of Mars. II - Results and implications for Martian ferric mineralogy

Details Charge-coupled device imaging spectroscopy of Mars. II - Results and implications for Martian ferric mineralogy Charge-coupled device imaging spectroscopy of Mars. II - Results and implications for Martian ferric mineralogy

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar..100..575b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 100, no. 2, p. 575-597.

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41

Ferric Ions, Image Analysis, Infrared Spectroscopy, Mars (Planet), Planetary Geology, Charge Coupled Devices, Visible Spectrum

Scientific paper

Materials similar to nanophase ferric oxides are presently seen to dominate the spectral behavior of the Martian surface in the visible-to-near-IR, in view of imaging spectroscopic observations of Mars. Attention is accordingly given to models for the formation of hematite and other ferric minerals in both current terrestrial environments and in the current and past, possibly wetter Martian climate. It is noted that imaging spectroscopy is an ideal tool for high spatial resolution spacecraft and telescopic studies of the Martian surface.

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