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Cited by 210

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Results from the Mars Global Surveyor Thermal Emission Spectrometer

Christensen, P. R., Anderson, D. L., Chase, S. C., Clancy, R. T., Clark, R. N., Conrath, B. J., Kieffer, H. H., Kuzmin, R. O., Malin, M. C., Pearl, J. C., Roush, T. L., Smith, M. D.·1998·Science

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.

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Metadata

Authors
Christensen, P. R., Anderson, D. L., Chase, S. C., Clancy, R. T., Clark, R. N., Conrath, B. J., Kieffer, H. H., Kuzmin, R. O., Malin, M. C., Pearl, J. C., Roush, T. L., & Smith, M. D.
Venue
Science
Published
1998-03-13
Volume
279
Issue
5357
Pages
1692-1698
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2156944376
Cited by
210
References
0
FWCI
23.62
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Results from the Mars Global Surveyor Thermal Emission Spectrometer. https://app.cochat.ai/papers/10.1126/science.279.5357.1692
The paper
Christensen, P. R., Anderson, D. L., Chase, S. C., Clancy, R. T., Clark, R. N., Conrath, B. J., Kieffer, H. H., Kuzmin, R. O., Malin, M. C., Pearl, J. C., Roush, T. L., & Smith, M. D. (1998). Results from the Mars Global Surveyor Thermal Emission Spectrometer. Science. https://doi.org/10.1126/science.279.5357.1692

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