Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/17167
Appears in Collections:Biological and Environmental Sciences Journal Articles
Peer Review Status: Refereed
Title: Visible and near-infrared multispectral analysis of geochemically measured rock fragments at the Opportunity landing site in Meridiani Planum
Authors: Weitz, Catherine
Farrand, William H
Johnson, Jeffrey R
Fleischer, Iris
Schröder, Christian
Yingst, R Aileen
Jolliff, Bradley L
Gellert, Ralf
Bell, III James F
Herkenhoff, Kenneth E
Klingelhoefer, Goestar
Cohen, Barbara A
Calvin, Wendy M
Rutherford, Malcolm
Ashley, James W
Contact Email: christian.schroeder@stir.ac.uk
Keywords: Mars
Meridiani Planum
MER
Issue Date: Jul-2010
Publisher: American Geophysical Union
Citation: Weitz C, Farrand WH, Johnson JR, Fleischer I, Schröder C, Yingst RA, Jolliff BL, Gellert R, Bell III JF, Herkenhoff KE, Klingelhoefer G, Cohen BA, Calvin WM, Rutherford M & Ashley JW (2010) Visible and near-infrared multispectral analysis of geochemically measured rock fragments at the Opportunity landing site in Meridiani Planum, Journal of Geophysical Research: Planets, 115 (E7), Art. No.: E00F10.
Abstract: We have used visible and near‐infrared Panoramic Camera (Pancam) spectral data acquired by the Opportunity rover to analyze 15 rock fragments at the Meridiani Planum landing site. These spectral results were then compared to geochemistry measurements made by the in situ instruments Mössbauer (MB) and Alpha Particle X‐ray Spectrometer (APXS) to determine the feasibility of mineralogic characterization from Pancam data. Our results suggest that dust and alteration rinds coat many rock fragments, which limits our ability to adequately measure the mineralogy of some rocks from Pancam spectra relative to the different field of view and penetration depths of MB and APXS. Viewing and lighting geometry, along with sampling size, also complicate the spectral characterization of the rocks. Rock fragments with the same geochemistry of sulfate‐rich outcrops have similar spectra, although the sulfate‐rich composition cannot be ascertained based upon Pancam spectra alone. FeNi meteorites have spectral characteristics, particularly ferric oxide coatings, that generally differentiate them from other rocks at the landing site. Stony meteorites and impact fragments with unknown compositions have a diverse range of spectral properties and are not well constrained nor diagnostic in Pancam data. Bounce Rock, with its unique basalt composition, is easily differentiated in the Pancam data from all other rock types at Meridiani Planum. Our Pancam analyses of small pebbles adjacent to these 15 rock fragments suggests that other rock types may exist at the landing site but have not yet been geochemically measured.
Type: Journal Article
URI: http://hdl.handle.net/1893/17167
DOI Link: http://dx.doi.org/10.1029/2010JE003660
Rights: Copyright 2010 by the American Geophysical Union. AGU allows authors to deposit their journal articles if the version is the final published citable version of record, the AGU copyright statement is clearly visible on the posting, and the posting is made 6 months after official publication by the AGU.
Affiliation: Planetary Science Institute
Space Science Institute
U.S. Geological Survey
Johannes Gutenberg University of Mainz
Biological and Environmental Sciences
Planetary Science Institute
Washington University In Saint Louis
University of Guelph
Cornell University
U.S. Geological Survey
Johannes Gutenberg University of Mainz
National Aeronautics and Space Administration (NASA)
University of Nevada, Reno
Brown University
Arizona State University



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