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Astrophysics and Space Science

, Volume 37, Issue 1, pp 3–9 | Cite as

Infrared spectra of carbonaceous chondrites and the composition of intertellar grains

  • A. Zaikowski
  • R. F. Knacke
Article

Abstract

Infrared spectra (7–40 μ) of the carbonaceous chondrites, Cold Bokkeveld, Murray, and Orgueil are compared with phyllosilicate minerals and interstellar grain spectra. Similarities in the position and shape of the silicate feature near 9.8 μ suggest that similar silicate minerals are present in primitive meteorites and the interstellar dust.

Keywords

Dust Silicate Infrared Spectrum Silicate Mineral Carbonaceous Chondrite 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1975

Authors and Affiliations

  • A. Zaikowski
    • 1
  • R. F. Knacke
    • 1
  1. 1.Dept. of Earth and Space SciencesState University of New York at Stony BrookStony BrookU.S.A.

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