Assessment of Mars Exploration Rover landing site predictions

Comprehensive analyses of remote sensing data during the three-year effort to select the Mars Exploration Rover landing sites at Gusev crater and at Meridiani Planum correctly predicted the atmospheric density profile during entry and descent and the safe and trafficable surfaces explored by the two rovers. The Gusev crater site was correctly predicted to be a low-relief surface that was less rocky than the Viking landing sites but comparably dusty. A dark, low-albedo, flat plain composed of basaltic sand and haematite with very few rocks was expected and found at Meridiani Planum. These results argue that future efforts to select safe landing sites based on existing and acquired remote sensing data will be successful. In contrast, geological interpretations of the sites based on remote sensing data were less certain and less successful, which emphasizes the inherent ambiguities in understanding surface geology from remotely sensed data and the uncertainty in predicting exactly what materials will be available for study at a landing site.

[1]  A. F. C. Haldemann,et al.  Analysis of MOLA data for the Mars Exploration Rover landing sites , 2003 .

[2]  Philip R. Christensen,et al.  The spatial distribution of rocks on mars , 1986 .

[3]  N. Bridges,et al.  Selection of the Mars Exploration Rover landing sites , 2003 .

[4]  Joy A. Crisp,et al.  Soil‐like deposits observed by Sojourner, the Pathfinder rover , 1999 .

[5]  R. Fergason,et al.  Thermal inertia using THEMIS infrared data , 2003 .

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

[7]  A. F. C. Haldemann,et al.  Rock size-frequency distributions on Mars and implications for Mars Exploration Rover landing safety and operations : Mars exploration rover mission and landing sites , 2003 .

[8]  T. Estlin,et al.  Autonomous onboard traverse science system , 2004, 2004 IEEE Aerospace Conference Proceedings (IEEE Cat. No.04TH8720).

[9]  Terry Z. Martin,et al.  Thermal and albedo mapping of Mars during the Viking primary mission , 1977 .

[10]  S. Ruff,et al.  Formation of the hematite-bearing unit in Meridiani Planum: Evidence for deposition in standing water , 2004 .

[11]  Mark I. Richardson,et al.  Analysis of atmospheric mesoscale models for entry, descent, and landing , 2003 .

[12]  P. Christensen,et al.  Thermal conductivity measurements of particulate materials 2. Results , 1997 .

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

[14]  J. Schofield,et al.  Results of the Mars Pathfinder atmospheric structure investigation , 1999 .

[15]  S. Ruff,et al.  Bright and dark regions on Mars: Particle size and mineralogical characteristics based on thermal emission spectrometer data , 2002 .

[16]  M. Mellon,et al.  High-Resolution Thermal Inertia Mapping from the Mars Global Surveyor Thermal Emission Spectrometer , 2000 .

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

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

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

[20]  David E. Smith,et al.  Mars Orbiter Laser Altimeter: Experiment summary after the first year of global mapping of Mars , 2001 .

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

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

[23]  Jeffrey R. Johnson,et al.  In Situ Evidence for an Ancient Aqueous Environment at Meridiani Planum, Mars , 2004, Science.

[24]  T. Farr,et al.  The roughness of natural terrain: A planetary and remote sensing perspective , 2001 .

[25]  D. Ming,et al.  Pancam Multispectral Imaging Results from the Spirit Rover at Gusev Crater , 2004, Science.

[26]  H. J. Moore,et al.  Selection of the Mars Pathfinder landing site , 1997 .

[27]  P H Smith,et al.  Evidence from Opportunity's Microscopic Imager for Water on Meridiani Planum , 2004, Science.

[28]  Michael D. Smith Interannual variability in TES atmospheric observations of Mars during 1999–2003 , 2004 .

[29]  N. O. Snider,et al.  Mantled and exhumed terrains in Terra Meridiani, Mars , 2002 .

[30]  R E Arvidson,et al.  Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover , 2004, Science.

[31]  D. Ming,et al.  Pancam Multispectral Imaging Results from the Opportunity Rover at Meridiani Planum , 2004, Science.

[32]  Raymond E. Arvidson,et al.  Mars Exploration Rover mission , 2003 .

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

[34]  T. Hagfors,et al.  Backscattering from an undulating surface with applications to radar returns from the Moon , 1964 .

[35]  R. Kirk,et al.  High-resolution topomapping of candidate MER landing sites with Mars Orbiter Camera narrow-angle images , 2003 .

[36]  K Davis,et al.  Localization and Physical Property Experiments Conducted by Opportunity at Meridiani Planum , 2004, Science.