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ROCK AND SOIL PHYSICAL PROPERTIES AT THE MER GUSEV CRATER AND MERIDIANI PLANUM LANDING SITESFollowing the successful landings of both Mars Exploration Rover (MER) vehicles at Gusev Crater and Meridiani Planum, respectively, their Athena suite of instruments is being used to study the geologic history of these two very different landing sites on Mars that had been selected on the basis of showing different types of evidence for aqueous processes in the planet s past. Utilizing the on-board instruments as well as the rovers mobility system, a wide range of physical properties investigations is carried out as well - the subject of this abstract - that provide additional information on the geology and processes at the sites. Results of the mission in general as well as of the physical properties studies thus far greatly exceed expectations in that observations and measurements by both vehicles show a rich variety in materials and processes: the Gusev site in the vicinity of the lander is remarkably flat and generally devoid of large rocks along traverses up to the time of this writing (approx.Sol 50) and suggestive of a deflated surface with generally only thin veneers of bright dust while exhibiting evidence of a widespread occurrence of a crust from cemented fines that has been observed to fail in the form of blocky clods when disturbed by vehicle rolling action; numerous small and shallow depressions - presumably created by impacts - are observed at the site which are infilled with bright, fine-grained material that likewise appears indurated and which was studied by a trenching experiment; small ripple bedforms are scattered across the site and were characterized in terms of particle size distributions. At the Meridiani site, studies so far - up to approx.Sol 33 - have focussed on soils and the rock outcrop encountered within the approx.20 m diameter crater that the spacecraft came to rest in: from a physical properties point of view, a mantle of dark, well-sorted, apparently basaltic sand with small to moderate cohesion has been of interest - and has been studied by a trenching experiment - as well as a fine-grained unit underlying the mantle at least locally within the crater. Rock grindings were accomplished successfully at both sites at the time of this writing, suggesting different strengths of the two targets (the basaltic rock nicknamed Adirondack at Gusev and the Meridiani rock outcrop) in addition to enabling compositional measurements below the original rock surfaces.
Document ID
20060009019
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Ming, Douglas W.
(NASA Johnson Space Center Houston, TX, United States)
Richter, L.
(Deutsche Forschungsanstalt fuer Luft- und Raumfahrt Germany)
Arvidson, R.
(Washington Univ. United States)
Bell, J.
(Cornell Univ. NY, United States)
Cabrol, N.
(NASA Ames Research Center Moffett Field, CA, United States)
Gorevan, S.
(Honeybee Robotics Ltd. New York, NY, United States)
Greeley, R.
(Arizona State Univ. Tempe, AZ, United States)
Herkenhoff, K.
(Geological Survey Flagstaff, AZ, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2006
Subject Category
Geophysics
Meeting Information
Meeting: 35th COSPAR Scientific Assembly
Location: Paris
Country: France
Start Date: July 18, 2004
End Date: July 24, 2004
Funding Number(s)
OTHER: 390-30-AA
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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