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Cited by 379

The DOI matches its Crossref record; 25 of the 25 references it cites were found in a registry or an index.

Spectroscopic Identification of Carbonate Minerals in the Martian Dust

Bandfield, Joshua L., Glotch, Timothy D., Christensen, Philip R.·2003·Science

Abstract

Thermal infrared spectra of the martian surface indicate the presence of small concentrations (∼2 to 5 weight %) of carbonates, specifically dominated by magnesite (MgCO 3 ). The carbonates are widely distributed in the martian dust, and there is no indication of a concentrated source. The presence of small concentrations of carbonate minerals in the surface dust and in martian meteorites can sequester several bars of atmospheric carbon dioxide and may have been an important sink for a thicker carbon dioxide atmosphere in the martian past.

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Research works printed but not linked: 5

  1. J. W. Salisburyet al. Infrared (2.1–25 μm) Spectra of Minerals (Johns Hopkins Univ. Press Baltimore 1991).
  2. S. W. Ruff, Eos83, 1059 (2002).
  3. 10.1029/95JE00226 · doi:10.1029/95je00226
  4. 10.1029/GL017i007p00985 · doi:10.1029/gl017i007p00985
  5. F. P. Fanaleet al., in Mars, H. H. Kieffer, B. M. Jakosky, C. W. Snyder, M. S. Matthews, Eds. (Univ. of Arizona Press, Tucson, 1992), pp. 1135–1179.

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Metadata

Authors
Bandfield, J. L., Glotch, T. D., & Christensen, P. R.
Venue
Science
Published
2003-08-22
Volume
301
Issue
5636
Pages
1084-1087
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2150107499
Cited by
379
References
25
FWCI
15.27
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Spectroscopic Identification of Carbonate Minerals in the Martian Dust. https://app.cochat.ai/papers/10.1126/science.1088054
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Bandfield, J. L., Glotch, T. D., & Christensen, P. R. (2003). Spectroscopic Identification of Carbonate Minerals in the Martian Dust. Science. https://doi.org/10.1126/science.1088054

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