T213 Planetary Exploration through Remote Compositional Analysis: The G.K. Gilbert Award Session
Tuesday, 2 November 2010
1:30 PM - 5:30 PM
Mile High Ballroom Prefunction
DISTRIBUTION OF PERCHLORATE SALTS AT THE MARS PHOENIX LANDING SITE: INITIAL RESULTS FROM SPECTRAL MAPPING
Paper number: T213-14
Program: Technical Sessions
Time: 5:00 PM – 5:15 PM
Authors
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Raymond ArvidsonWashington University IN St. Louis, St. Louis, MO
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Jeffrey G. CatalanoWashington University in St. Louis, St. Louis, MO
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Douglas W. MingNASA Johnson Space Center, Houston, TX
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Michael T. MellonUniversity of Colorado, Boulder, CO
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Richard V. MorrisNASA Johnson Space Center, Houston, TX
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Mark LemmonTexas A&M University, College Station, TX
Abstract
Here, we use spectra from the Surface Stereo Imager (SSI) aboard Phoenix to map the distribution of perchlorate salts at the Phoenix landing site. We find that perchlorate is concentrated into small subsurface patches with distinct spectral signatures. These patches are morphologically similar to salt patches that form from aqueous redistribution on Earth, for example, in the Antarctic Dry Valleys. We propose that thin films of liquid water, arising from minor melting associated with seasonal ices or long-term obliquity cycles, are responsible for dissolving and concentrating perchlorate into these subsurface patches.