Other
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agusm.u43a..01s&link_type=abstract
American Geophysical Union, Spring Meeting 2004, abstract #U43A-01
Other
5464 Remote Sensing, 5470 Surface Materials And Properties, 6225 Mars
Scientific paper
The Mars Exploration Rover Spirit landed in Gusev Crater on January 4 (UTC), 2004. It was followed 21 days later by the rover Opportunity, which landed on Meridiani Planum. The landing site at Gusev crater lies on a flat, rock-strewn plain. The rock at Gusev that has been studied best to date has been named Adirondack. In its surface texture, Adirondack appears to be dense, fine-grained and sand-blasted. Three sets of measurements have been made on Adirondack with the full set of payload instruments: one of the natural rock surface, one of the same location after being brushed by the RAT, and one of the same location after removal of 2-3 mm of rock by the RAT. The concentration of presumably dust-borne elements like sulfur and chlorine diminished significantly with brushing, and diminished dramatically with grinding. All of the observations of Adirondack are consistent with it being an essentially unweathered olivine and magnetite-bearing, low-silica basalt. The only soil at Gusev that has been investigated in detail so far is one dominated by fairly coarse (100-300 micron) grains that have the appearance and behavior of well-cemented agglomerates. APXS spectra of this soil are similar to those of soils found at the Viking and Pathfinder sites. Mössbauer spectra show two ferrous doublets and a ferric doublet, with the stronger ferrous doublet assigned to olivine. Mini-TES spectra have been acquired for soils surrounding the the Spirit landing site, and show spectra nearly identical to globally averaged soil viewed by the TES instrument on Mars Global Surveyor. This includes identification of a small amount (a few percent) of carbonate. The landing site at Meridiani Planum lies inside an impact crater that is roughly 20 meters in diameter. The lander came to rest on soil that fills most of the crater. An outcrop of layered bedrock is exposed on the crater wall. The landing site was selected partly because coarse gray hematite was expected to be present on the basis of orbital data. Mini-TES data have confirmed the presence of this hematite in the soil. The soil within the crater has several components. Microscopic images of undisturbed surface soil show that one component is fine (~100 micron) sand. Mössbauer spectra of the sand show two ferrous doublets (one of them due to olivine), a ferric doublet, and a weak magnetic sextet. APXS and Mini-TES data on this sand are consistent with a composition dominated by basalt. Another component of the soil consists of coarse (several mm) granules. These range in shape from subangular to rounded to remarkably spherical. In some locations, granules have been pressed down into the soil by the impact of the landers airbags. At those locations the concentration of hematite as determined by Mini-TES is sharply reduced, suggesting that at least some of the granules are hematite-bearing. The bedrock outcrop is finely laminated, with typical layer thicknesses of only a few mm. The texture of the outcrop as viewed in miroscopic images suggests that it is fine-grained, with well-expressed structure that is revealed by varying degrees of mechanical abrasion of layers of varying induration. Initial APXS results on this fine-grained matrix indicate sulfur concentrations significantly higher than any observed elsewhere on Mars. Embedded within the outcrop and weathering out of it are highly spherical granules with diameters of several mm. The visible to near-IR spectral properties of these embedded spherical granules, as determined by Pancam, are distinctly different from those of the matrix in which they are embedded.
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