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Summary of Results from the Mars Phoenix Lander's Thermal Evolved Gas AnalyzerThe Mars Phoenix Scout Mission with its diverse instrument suite successfully examined several soils on the Northern plains of Mars. The Thermal and Evolved Gas Analyzer (TEGA) was employed to detect evolved volatiles and organic and inorganic materials by coupling a differential scanning calorimeter (DSC) with a magnetic-sector mass spectrometer (MS) that can detect masses in the 2 to 140 dalton range [1]. Five Martian soils were individually heated to 1000 C in the DSC ovens where evolved gases from mineral decompostion products were examined with the MS. TEGA s DSC has the capability to detect endothermic and exothermic reactions during heating that are characteristic of minerals present in the Martian soil.
Document ID
20090022803
Acquisition Source
Johnson Space Center
Document Type
Preprint (Draft being sent to journal)
Authors
Sutter, B.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Ming, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Boynton, W. V.
(Arizona Univ. Tucson, AZ, United States)
Niles, P. B.
(NASA Johnson Space Center Houston, TX, United States)
Hoffman, J.
(Texas Univ. at Dallas Richardson, TX, United States)
Lauer, H. V.
(Barrios Technology, Inc. Houston, TX, United States)
Golden, D. C.
(Hamilton Sundstrand Corp. Houston, TX, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2009
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-18424
Report Number: JSC-CN-18424
Meeting Information
Meeting: The New Martian Chemistry Workshop
Location: Medford, MA
Country: United States
Start Date: July 26, 2009
End Date: July 28, 2009
Sponsors: Universities Space Research Association, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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