Results from the Mars global surveyor thermal emission spectrometer

  • Philip Christensen
  • , D. L. Anderson
  • , S. C. Chase
  • , R. T. Clancy
  • , R. N. Clark
  • , B. J. Conrath
  • , H. H. Kieffer
  • , R. O. Kuzmin
  • , M. C. Malin
  • , J. C. Pearl
  • , T. L. Roush
  • , M. D. Smith

Research output: Contribution to journalArticlepeer-review

Abstract

The Thermal Emission Spectrometer spectra of low albedo surface materials suggests that a four to one mixture of pyroxene to plagioclase, together with about a 35 percent dust component provides the best fit to the spectrum. Qualitative upper limits can be placed on the concentration of carbonates (<10 percent), olivine (<10 percent), clay minerals (<20 percent), and quartz (<5 percent) in the limited regions observed. Limb observations in the northern hemisphere reveal low-lying dust hazes and detached water-ice clouds at altitudes up to 55 kilometers. At an aerocentric longitude of 224°a major dust storm developed in the Noachis Terra region. The south polar cap retreat was similar to that observed by Viking.

Original languageEnglish (US)
Pages (from-to)1692-1696
Number of pages5
JournalScience
Volume279
Issue number5357
DOIs
StatePublished - Mar 13 1998

ASJC Scopus subject areas

  • General

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