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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Localization and physical property experiments conducted by Opportunity at Meridiani Planum
R E Arvidson1, R C Anderson, P Bartlett
1Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA. arvidson@wunder.wustl.edu
The Mars Exploration Rover Opportunity precisely mapped its landing site and rover tracks. Surface dust accumulation on solar panels suggests strong winds continually clean Meridiani Planum.
Area of Science:
- Planetary Science
- Geology
- Mars Exploration
Background:
- The Mars Exploration Rover Opportunity's landing site requires precise localization for scientific analysis.
- Understanding the Martian surface morphology and geological processes is crucial for interpreting mission data.
Purpose of the Study:
- To determine the absolute accuracy of the Opportunity landing site location.
- To establish precise rover traverse locations and analyze Martian surface topography.
- To investigate the geological characteristics and erosional processes of Meridiani Planum.
Main Methods:
- Radio tracking data analysis for absolute landing site accuracy.
- Engineering telemetry and overlapping images for rover traverse localization.
- Rover-generated topographic profiles and orbital observation analysis.
- Grinding experiments to assess rock mechanical strength.
Main Results:
- Opportunity's landing site was localized to better than 10-meter absolute accuracy.
- Rover locations during traverses were determined with centimeter-level accuracy.
- Meridiani Planum exhibits very smooth topography at meter- to centimeter-length scales.
- Solar cell performance degradation due to dust deposition was observed.
- Evidence suggests high-velocity winds continuously remove dust, indicated by the lack of dust-covered surfaces.
- Evaporitic rocks possess low mechanical strength, and abundant coarse-grained particles suggest differential erosion.
Conclusions:
- Precise localization of the Opportunity rover and its landing site was achieved.
- The Martian plains at Meridiani Planum are geologically smooth with evidence of ongoing aeolian processes.
- Differential erosion, driven by wind and rock properties, shapes the Meridiani Planum landscape.
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