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Preliminary results from the Viking X-ray fluorescence experiment - The first sample from Chryse Planitia, MarsIron, calcium, aluminum, silicon, and sulfur are major elements in the first surface sample of Mars that has been analyzed by the Viking X-ray fluorescence spectrometer. Titanium is present in minor quantities. This is consistent with the sample's being a mixture of fine silicate and oxide mineral grains, with a significant proportion of sulfates, possibly hydrated. Ferric oxide is regarded as the red pigmenting agent on the Martian surface, but if it coats silicate grains, the coatings must be very thin or discontinuous. A high abundance of Fe, relatively low abundances of Al, Rb, Sr, and Zr, and a high Ca/K ratio are distinctive features of the spectra. Preliminary determinations indicate the following abundances (as percentages by weight): Fe, 14 plus or minus 2; Ti, less than 1; S, 2 to 5; the Ca/K ratio by weight is greater than 5.
Document ID
19760087409
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Toulmin, P., III
(Geological Survey Reston, VA, United States)
Rose, H. J., Jr.
(U.S. Geological Survey Reston, Va., United States)
Clark, B. C.
(Martin Marietta Planetary Sciences Laboratory Denver, Colo., United States)
Baird, A. K.
(Pomona College Claremont, Calif., United States)
Keil, K.
(New Mexico, University Albuquerque, N. Mex., United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1976
Publication Information
Publication: Science
Volume: 194
Subject Category
Lunar And Planetary Exploration
Accession Number
76A45442
Funding Number(s)
CONTRACT_GRANT: NAS1-9000
CONTRACT_GRANT: NAS1-11858
CONTRACT_GRANT: NASA ORDER L-9717
CONTRACT_GRANT: NAS1-11855
Distribution Limits
Public
Copyright
Other

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