Aqueous processes at Gusev crater inferred from physical properties of rocks and soils along the Spirit traverse

[1] Gusev crater was selected as the landing site for Spirit on the basis of morphological evidence of long-lasting water activity, including possibly fluvial and lacustrine episodes. From the Columbia Memorial Station to the Columbia Hills, Spirit's traverse provides a journey back in time, from relatively recent volcanic plains showing little evidence for aqueous processes up to the older hills, where rock and soil composition are drastically different. For the first 156 sols, the only evidence of water action was weathering rinds, vein fillings, and soil crust cementation by salts. The trenches of Sols 112–145 marked the first significant findings of increased concentrations of sulfur and magnesium varying in parallel, suggesting that they be paired as magnesium-sulfate. Spirit's arrival at West Spur coincided with a shift in rock and soil composition with observations hinting at substantial amounts of water in Gusev's past. We used the Microscopic Imager data up to Sol 431 to analyze rock and soil properties and infer plausible types and magnitude of aqueous processes through time. We show the role played early by topography and structure. The morphology, texture, and deep alteration shown by the rocks in West Spur and the Columbia Hills Formation (CHF) suggest conditions that are not met in present-day Mars and required a wetter environment, which could have included transport of sulfur, chlorine, and bromine in water, vapor in volcanic gases, hydrothermal circulation, or saturation in a briny fluid containing the same elements. Changing conditions that might have affected flow circulation are suggested by different textural and morphological characteristics between the rocks in the CHF and those of the plains, with higher porosity proxy, higher void ratio, and higher water storage potential in the CHF. Soils were used to assess aqueous processes and water pathways in the top layers of modern soils. We conclude that infiltration might have become more difficult with time.

[1]  W. Boynton,et al.  Maps of Subsurface Hydrogen from the High Energy Neutron Detector, Mars Odyssey , 2002, Science.

[2]  D. Rubin A Simple Autocorrelation Algorithm for Determining Grain Size from Digital Images of Sediment , 2004 .

[3]  S. Brantley,et al.  Chemical weathering rates of silicate minerals , 1995 .

[4]  William H. Farrand,et al.  The Spirit Rover9s Athena Science Investigation at Gusev Crater, Mars , 2004 .

[5]  K. Di,et al.  Spirit rover localization and topographic mapping at the landing site of Gusev crater, Mars , 2006 .

[6]  L. Pel,et al.  Simulating the growth of tafoni , 2004 .

[7]  Steven W. Squyres,et al.  Ancient aqueous sedimentation on Mars , 1988 .

[8]  Raymond E. Arvidson,et al.  Rock Abrasion Tool: Mars Exploration Rover mission , 2003 .

[9]  D. H. Scott,et al.  Martian paleolakes and waterways: Exobiological implications , 2005, Origins of life and evolution of the biosphere.

[10]  N. Cabrol,et al.  On the possibility of liquid water on present‐day Mars , 2001 .

[11]  R Sullivan,et al.  The Spirit Rover's Athena science investigation at Gusev Crater, Mars. , 2004, Science.

[12]  G. Landis,et al.  Transient Liquid Water as a Mechanism for Induration of Soil Crusts on Mars , 2004 .

[13]  R. Greeley,et al.  Fluid lava flows in Gusev crater, Mars , 2005 .

[14]  C. Wentworth A Scale of Grade and Class Terms for Clastic Sediments , 1922, The Journal of Geology.

[15]  D. Ming,et al.  Mössbauer mineralogy of rock, soil, and dust at Gusev crater, Mars: Spirit's journey through weakly altered olivine basalt on the plains and pervasively altered basalt in the Columbia Hills , 2006 .

[16]  J F Bell,et al.  Surficial Deposits at Gusev Crater Along Spirit Rover Traverses , 2004, Science.

[17]  W. Rawls,et al.  Estimating generalized soil-water characteristics from texture , 1986 .

[18]  Rebecca Castano,et al.  Geology of the Gusev cratered plains from the Spirit rover transverse , 2006 .

[19]  A. McEwen,et al.  Morphology and Composition of the Surface of Mars: Mars Odyssey THEMIS Results , 2003, Science.

[20]  N. Cabrol,et al.  A morphological view on potential niches for exobiology on Mars. , 1995, Planetary and space science.

[21]  G. Brakenridge The origin of fluvial valleys and early geologic history, Aeolis Quadrangle, Mars , 1990 .

[22]  D. Leverington,et al.  A Large Paleolake Basin at the Head of Ma'adim Vallis, Mars , 2002, Science.

[23]  J. Muller,et al.  Interferometric synthetic aperture radar atmospheric correction: GPS topography‐dependent turbulence model , 2006 .

[24]  Nathalie A. Cabrol,et al.  Limnologic Analysis of Gusev Crater Paleolake, Mars , 1997 .

[25]  J. Farmer,et al.  Radiocarbon Ages of Lacustrine Deposits in Volcanic Sequences of the Lomas Coloradas Area, Socorro Island, Mexico , 1993, Radiocarbon.

[26]  D. Ming,et al.  Subsurface weathering of rocks and soils at Gusev crater , 2005 .

[27]  Michael D. Smith The annual cycle of water vapor on Mars as observed by the Thermal Emission Spectrometer , 2002 .

[28]  A. Goudie,et al.  Chemical sediments and geomorphology: Precipitates and residua in the near-surface environment. , 1983 .

[29]  John F. McCauley,et al.  Mariner 9 evidence for wind erosion in the equatorial and mid‐latitude regions of Mars , 1973 .

[30]  D. Ming,et al.  Water alteration of rocks and soils on Mars at the Spirit rover site in Gusev crater , 2005, Nature.

[31]  P H Smith,et al.  Textures of the soils and rocks at Gusev Crater from Spirit's Microscopic Imager. , 2004, Science.

[32]  William H. Farrand,et al.  Evidence of phyllosilicates in Wooly Patch, an altered rock encountered at West Spur, Columbia Hills, by the Spirit rover in Gusev crater, Mars , 2006 .

[33]  Robert C. Anderson,et al.  The (in)accuracy of novice rover operators' perception of obstacle height from monoscopic images , 2005, IEEE Transactions on Systems, Man, and Cybernetics - Part A: Systems and Humans.

[34]  R. Greeley,et al.  Geologic map of the MTM-15182 and MTM-15187 quadrangles, Gusev Crater-Ma'adim Vallis region, Mars , 2000 .

[35]  K. Herkenhoff,et al.  Sulfate deposition in subsurface regolith in Gusev crater, Mars , 2006 .

[36]  S. Brantley,et al.  Rates of weathering rind formation on Costa Rican basalt , 2004 .

[37]  William H. Farrand,et al.  Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills , 2006 .

[38]  Nathalie A. Cabrol,et al.  Gusev crater: Wind‐related features and processes observed by the Mars Exploration Rover Spirit , 2006 .

[39]  William H. Farrand,et al.  Rocks of the Columbia Hills , 2006 .

[40]  J. Starkey,et al.  Edge detection in petrographic images , 1993 .

[41]  R J Sullivan,et al.  Wind-Related Processes Detected by the Spirit Rover at Gusev Crater, Mars , 2004, Science.

[42]  D. Ming,et al.  Localization and Physical Properties Experiments Conducted by Spirit at Gusev Crater , 2004, Science.

[43]  Nathalie A. Cabrol,et al.  Ma'adim Vallis Evolution: Geometry and Models of Discharge Rate , 1998 .

[44]  William H. Farrand,et al.  Geochemical and mineralogical indicators for aqueous processes in the Columbia Hills of Gusev crater, Mars , 2006 .

[45]  Kenneth L. Tanaka,et al.  Exploring Gusev Crater with spirit: Review of science objectives and testable hypotheses , 2003 .

[46]  D. Ming,et al.  Mineralogy at Gusev Crater from the Mössbauer Spectrometer on the Spirit Rover , 2004, Science.

[47]  M. Carr,et al.  Martian channels and valleys: Their characteristics, distribution, and age , 1981 .

[48]  Nathalie A. Cabrol,et al.  Overview of the Microscopic Imager Investigation during Spirit's first 450 sols in Gusev crater , 2006 .