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Geochemical Endmembers Preserved in Gale Crater: A Tale of Two Mudstones and Their Compositional Differences According to ChemcamGale crater contains two fine-grained mudstone sedimentary units: The Sheepbed mudstone member, and the Murray formation mud-stones. These mudstones formed as part of an ancient fluviolacustrine system. The NASA Curiosity rover has analysed these mudstone units using the Chemistry and Camera (ChemCam), Alpha Particle X-ray Spectrometer (APXS) and Chemistry and Mineralogy (CheMin) onboard instrument suites. Subsequent mineralogical analyses have uncovered a wide geochemical and mineralogical diversity across and within these two mudstone formations. This study aims to determine the principal cause (alteration or source region) of this geochemical variation through a statistical analysis of the ChemCam dataset up to sol 1482, including the lower to middle Murray formation.
Document ID
20180004267
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Bedford, C. C.
(Open Univ. Milton Keynes, United Kingdom)
Schwenzer, S. P.
(Open Univ. Milton Keynes, United Kingdom)
Bridges, J. C.
(Leicester Univ. United Kingdom)
Wiens, R. C.
(Los Alamos National Lab. NM, United States)
Rampe, E. B.
(NASA Johnson Space Center Houston, TX, United States)
Frydenvang, J.
(Copenhagen Univ. Denmark)
Gasda, P. J.
(Los Alamos National Lab. NM, United States)
Date Acquired
August 8, 2018
Publication Date
March 22, 2018
Subject Category
Geophysics
Report/Patent Number
JSC-E-DAA-TN53578
Report Number: JSC-E-DAA-TN53578
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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