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Volumn 301, Issue 5636, 2003, Pages 1084-1087

Spectroscopic identification of carbonate minerals in the martian dust

Author keywords

[No Author keywords available]

Indexed keywords

CARBON DIOXIDE; INFRARED SPECTROSCOPY; MARTIAN SURFACE ANALYSIS; METEORITES;

EID: 0041930658     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1088054     Document Type: Article
Times cited : (313)

References (33)
  • 12
    • 0041824209 scopus 로고    scopus 로고
    • note
    • The reactivity of the soils was inconsistent with any large (> 1 to 2%) abundance of Mg or Ca carbonate in the presence of smectite clays. There is no conclusive evidence for smectite clays in the martian soil and dust.
  • 17
    • 0042325121 scopus 로고    scopus 로고
    • note
    • Materials and methods are available as supporting material on Science Online.
  • 18
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    • S. W. Ruff, Eos 83, 1059 (2002).
    • (2002) Eos , vol.83 , pp. 1059
    • Ruff, S.W.1
  • 23
    • 0042826198 scopus 로고    scopus 로고
    • note
    • Several investigations have tentatively identified carbonate absorptions in the atmospheric dust based on telescopic data sets (31, 32). The number of spectra collected is limited and the large footprints include a wide range of surface temperatures, making the data difficult to interpret. These absorptions are inconsistent with Mariner 6/7 IRS, Mariner 9 IRIS, and MGS TES data, which all produce consistent spectral features and are considered well calibrated.
  • 26
    • 0000695207 scopus 로고
    • R. Kahn, Icarus 62, 175 (1985).
    • (1985) Icarus , vol.62 , pp. 175
    • Kahn, R.1
  • 27
    • 0002003378 scopus 로고
    • H. H. Kieffer, B. M. Jakosky, C. W. Snyder, M. S. Matthews, Eds. (Univ. of Arizona Press, Tucson)
    • F. P. Fanale et 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.
    • (1992) Mars , pp. 1135-1179
    • Fanale, F.P.1
  • 33
    • 0042325120 scopus 로고    scopus 로고
    • note
    • We thank M. Kraft, M. Smith, J. Pearl, P. Niles, L. Leshin, V. Hamilton, A. Baldridge, and S. Ruff for discussions that significantly improved the manuscript. K. Bender, K. Homan, K. Murray, N. Gorelick, S. Anwar, and H. Moncrief provided operations and software support necessary for the TES investigation. R. Clark and an anonymous reviewer provided helpful discussion and comments that improved the clarity of the data presented here.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.