Computer Science
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mers.work...12c&link_type=abstract
First Landing Site Workshop for the 2003 Mars Exploration Rovers, p. 12
Computer Science
Landing Sites, Spectrometers, Thermal Emission, Roving Vehicles, Hematite, Mars Surface, Near Infrared Radiation, Crystallinity, Mineral Deposits, Mars Global Surveyor
Scientific paper
The Thermal Emission Spectrometer (TES) instrument on the Mars Global Surveyor (MGS) mission has identified an accumulation of crystalline hematite (alpha-Fe2O3) that covers an area with very sharp boundaries approximately 350 by 750 km in size centered near 2 S latitude between 0 and 8 W longitude (Sinus Meridiani). The depth and shape of the hematite fundamental bands in the TES spectra show that the hematite is relatively coarse grained (greater than 5-10 micrometers). The spectrally-derived areal abundance of hematite varies with particle size from approximately 10% for particles greater than 30 micrometers in diameter to 40-60% for unpacked 10 micrometer powders. The hematite in Sinus Meridiani is thus distinct from the fine-grained (diameter less than 5-10 micrometers), red, crystalline hematite considered, on the basis of visible and near-IR data, to be a minor spectral component in Martian bright regions. A global map of the hematite abundance has been constructed using TES data from the MGS mapping mission.
Bandfield Joshua
Christensen Philip R.
Hamilton Victoria
Lane Melissa
Malin Michael
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