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The XRD Amorphous Component in John Klein Drill Fines at Yellowknife Bay, Gale Crater, MarsDrill fines of mudstone (targets John Klein and Cumberland) from the Sheepbed unit at Yel-lowknife Bay were analyzed by MSL payload elements including the Chemistry and Mineralogy (CheMin), APXS (Alpha Particle X-Ray Spectrometer), and Sample Analysis at Mars (SAM) instruments. CheMin XRD results show a variety of crystalline phases including feldspar, pyroxene, olivine, oxides, oxyhydroxides, sulfates, sulfides, a tri-octahedral smectite, and XRD amorphous material. The drill fines are distinctly different from corresponding analyses of the global soil (target Rocknest) in that the mudstone samples contained detectable phyllosilicate. Here we focus on John Klein and combine CheMin and APXS data to calculate the chemical composition and concentration of the amorphous component. The chemical composition of the amorphous plus smectite component for John Klein was calculated by subtracting the abundance-weighted chemical composition of the individual XRD crystalline components from the bulk composition of John Kline as measured by APXS. The chemical composition of individual crystalline components was determined either by stoichiometry (e.g., hematite and magnetite) or from their unit cell parameters (e.g., feldspar, olivine, and pyroxene). The chemical composition of the amorphous + smectite component (approx 71 wt.% of bulk sample) and bulk chemical composition are similar. In order to calculate the chemical composition of the amorphous component, a chemical composition for the tri-octahedral smectite must be assumed. We selected two tri-octahedral smectites with very different MgO/(FeO + Fe2O3) ratios (34 and 1.3 for SapCa1 and Griffithite, respectively). Relative to bulk sample, the concentration of amorphous and smectite components are 40 and 29 wt.% for SapCa1 and 33 and 36 wt.% for Griffithite. The amount of smectite was calculated by requiring the MgO concentration to be approx 0 wt.% in the amorphous component. Griffithite is the preferred smectite because the position of its 021 diffraction peak is similar to that reported for John Klein. In both cases, the amorphous component has low SiO2 and MgO and high FeO + Fe2O3, P2O5, and SO3 concentrations relative to bulk sample. The chemical composition of the bulk drill fines and XRD crystalline, smectite, and amorphous components implies alteration of an initially basaltic material under near neutral conditions (not acid sulfate), with the sulfate incorporated later as veins of CaSO4 injected into the mudstone.
Document ID
20140004213
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Morris, Richard V.
(NASA Johnson Space Center Houston, TX, United States)
Ming,, Douglas W.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Blake, David
(NASA Ames Research Center Moffett Field, CA, United States)
Vaniman, David
(Planetary Science Inst. Tucson, AZ, United States)
Bish, David L
(Indiana Univ. Bloomington, IN, United States)
Chipera, Steve
(Chesapeake Energy Corp. Oklahoma City, OK, United States)
Downs, Robert
(Arizona Univ. Tucson, AZ, United States)
Morrison, Shaunna
(Arizona Univ. Tucson, AZ, United States)
Gellert, Ralf
(Guelph Univ. Ontario, Canada)
Campbell, Iain
(Guelph Univ. Ontario, Canada)
Treiman, Alan H.
(Lunar and Planetary Inst. Houston, TX, United States)
Achilles, Cherie
(Oak Ridge Associated Universities, Inc. Houston, TX, United States)
Bristow, Thomas
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Crisp, Joy A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
McAdam, Amy
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Archer, Paul Douglas
(NASA Johnson Space Center Houston, TX, United States)
Sutter, Brad
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Rampe, Elizabeth B.
(Oak Ridge Associated Universities, Inc. Houston, TX, United States)
Date Acquired
April 30, 2014
Publication Date
December 9, 2013
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-30041
Meeting Information
Meeting: 2013 American Geophysical Union (AGU) Annual Fall Meeitng
Location: San Francisco, CA
Country: United States
Start Date: December 9, 2013
End Date: December 13, 2013
Sponsors: American Geophysical Union
Distribution Limits
Public
Copyright
Public Use Permitted.
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