Published September 1, 2014 | Version v1
Journal article

In situ calibration using univariate analyses based on the onboard ChemCam targets: first prediction of Martian rock and soil compositions

  • 1. GeoRessources lab, Université de Lorraine, Nancy (France)
  • 2. Los Alamos National Laboratory, Los Alamos, NM (United States)
  • 3. University of NM, Albuquerque (United States)
  • 4. IRAP, Toulouse (France)
  • 5. Museum National d'Histoire Naturelle, Paris (France)
  • 6. Planetary Science Institute, Tucson, AZ (United States)
  • 7. Delaware State University (United States)

Description

Curiosity rover landed on August 6th, 2012 in Gale Crater, Mars and it possesses unique analytical capabilities to investigate the chemistry and mineralogy of the Martian soil. In particular, the LIBS technique is being used for the first time on another planet with the ChemCam instrument, and more than 75,000 spectra have been returned in the first year on Mars. Curiosity carries body-mounted calibration targets specially designed for the ChemCam instrument, some of which are homgeneous glasses and others that are fine-grained glass-ceramics. We present direct calibrations, using these onboard standards to infer elements and element ratios by ratioing relative peak areas. As the laser spot size is around 300 μm, the LIBS technique provides measurements of the silicate glass compositions representing homogeneous material and measurements of the ceramic targets that are comparable to fine-grained rock or soil. The laser energy and the auto-focus are controlled for all sequences used for calibration. The univariate calibration curves present relatively to very good correlation coefficients with low RSDs for major and ratio calibrations. Trace element calibration curves (Li, Sr, and Mn), down to several ppm, can be used as a rapid tool to draw attention to remarkable rocks and soils along the traverse. First comparisons to alpha-particle X-ray spectroscopy (APXS) data, on selected targets, show good agreement for most elements and for Mg# and Al/Si estimates. SiO2 estimates using univariate cannot be yet used. Na2O and K2O estimates are relevant for high alkali contents, but probably under estimated due to the CCCT initial compositions. Very good results for CaO and Al2O3 estimates and satisfactory results for FeO are obtained. - Highlights: • In situ LIBS univariate calibrations are done using the Curiosity onboard standards. • Major and minor element contents can be rapidly obtained. • Trace element contents can be used as a rapid tool along the Martian traverse. • First comparisons to APXS data show good to very good agreement

Availability note (English)

Available from http://dx.doi.org/10.1016/j.sab.2014.03.014

Additional details

Identifiers

DOI
10.1016/j.sab.2014.03.014;
PII
S0584-8547(14)00090-1;

Publishing Information

Journal Title
Spectrochimica Acta. Part B, Atomic Spectroscopy
Journal Volume
99
Journal Page Range
p. 34-51
ISSN
0584-8547
CODEN
SAASBH

Optional Information

Copyright
Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.