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Updated: Aug 3, 2026

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Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
Published on: June 9, 2016
The Opportunity Rover's Athena science investigation at Meridiani Planum, Mars
S W Squyres1, R E Arvidson, J F Bell
1Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA. squyres@astro.cornell.edu
Summary
Mars Exploration Rover Opportunity found evidence of past liquid water at its Meridiani Planum landing site. Sedimentary rocks rich in sulfates suggest episodic water inundation and evaporation, supporting a watery ancient Mars.
Area of Science:
- Planetary Science
- Geology
- Astrobiology
Background:
- The Mars Exploration Rover Opportunity surveyed Eagle crater and Meridiani Planum.
- Surface soils are basaltic sands with hematite-rich spherules and wind ripples.
- Exposed sedimentary rocks lie beneath the soil layer.
Purpose of the Study:
- Investigate the geological composition and depositional environment of Meridiani Planum.
- Determine the role of water in the formation of Martian sedimentary rocks.
- Characterize the nature of hematite spherules.
Main Methods:
- In-situ analysis by the Opportunity rover.
- Geological mapping and observation of rock strata.
- Analysis of soil and rock composition, including sulfur and sulfate content.
Main Results:
- Sedimentary rocks are finely laminated, sulfur-rich, and contain abundant sulfate salts.
- Evidence of small-scale cross-lamination suggests deposition in flowing liquid water.
- Hematite-rich spherules, interpreted as diagenetic concretions, are embedded in and eroding from the rocks.
Conclusions:
- Meridiani Planum's rocks are a mix of chemical and siliciclastic sediments.
- Episodic shallow surface water, followed by evaporation and desiccation, formed these rocks.
- The presence of concretions further supports post-depositional diagenesis involving liquid water.
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