Skip to main content

IR Spectroscopy of Acid Insoluble Residues of Carbonaceous Chondrites

  • Conference paper

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 149))

Abstract

Léger and Puget (1984) have suggested polycyclic aromatic hydrocarbons (PAHs) as being responsible for the unidentified infrared emission bands (UIRs). The idea that PAHs are a component of the interstellar medium originated with Donn (1968). Because of this interest, insoluble carbon of carbonaceous chondrites obtained for the purpose of 13C NMR spectroscopy (Cronin et al., 1987) appears to be due to its aromatic content an attractive material to investigate with infrared spectroscopy. This insoluble carbon is a residue of HF and HC1 dissolution of the meteorite. Sample prepared from the Orgueil (C1), Murchison (CM2), and Allende (CV3) carbonaceous chondrites were examined with FTIR spectroscopy in bulk form in KBr pellets, as films evaporated under vacuum onto KBr disks, and as the residues of those evaporations in KBr pellets. The 13C cross polarization, magic angle spinning sample nuclear magnetic resonance (CP-MASS NMR) data indicates two major peaks centered at 29 and 133 ppm relative to tetramethylsilane (Cronin et al., 1987). The strength of the 133 ppm peak due to 13C in aromatic structures, relative to the 29 ppm 13C peak from aliphatic constituents, increases in the sequence of Allende, Murchison, and Orgueil (Figure 1). The 13C aromatic peak of the Orgueil residue is of particular interest in that its lack of structure normally suggestive of carboxyl or methoxy groups, and narrowness indicative of a homogeneity of the aromatic species consistent with large PAH structures, is what would be expected of interstellar PAHs (Wdowiak 1986, Tielens et al., 1987). The 11.3 µm UIR band mandates a family of PAHs that have single hydrogens per peripheral ring as a major interstellar PAH constituent. Molecules such as coronene (Léger and Puget 1984) and hexabenzocoronene (Hendel et al., 1986) are precluded from being maior interstellar PAH species because they have two and three hydrogens per peripheral ring, and hence no 11,3 µm feature exists.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Allamandola, L.J., Sandford, S.A., Wopenka,B.: 1987, Science, 237, 56.

    Article  ADS  Google Scholar 

  • Bregman, J., Allamandola, L.J., Simpson, J., Tielens,A., Witteborn, F.: 1984, in NASA/ASP Symposium, “AirborneAstronomy”, NASA/Ames Research Center (NASA CP-2353).

    Google Scholar 

  • Cohen, M., Tielens, A.G.G.M., Allamandola, L.J.: 1985,Ap.J., 299, L93.

    Article  ADS  Google Scholar 

  • Cronin, J.R., Pizzarello, S., Frye, J.S.: 1987,Geochim. Cosmochim. Acta, 51, 299.

    Article  ADS  Google Scholar 

  • Donn, B.: 1968, Ap., 152, L129.

    Article  ADS  Google Scholar 

  • Hendel, W.,Zhan, Z.H., Schmidt, W.: 1986, Tetrahedron, 42, 1127.

    Article  Google Scholar 

  • Léger, A. Puget,J.L.: 1984, Astron. Astrophys., 137, L5.

    ADS  Google Scholar 

  • Tielens, A.G.G.M., Allamandola, L.J., Barker, J.R.,Cohen, M.: 1987, in “Polycyclic Aromatic Hydrocarbons andAstrophysics”, A. Léger, L.d’Hendecourt, and N. Boccara ed. (D. Reidel, Dordrecht).

    Google Scholar 

  • Wdowiak, T.J.: 1986, Bull. Am. Astron. Soc., 18, 1030.

    Google Scholar 

  • Wopenka, B.: 1987, in Lunar and Planetary Science XVIIF, (Lunar and Planetary Institute,Houston), 1102.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1988 Kluwer Academic Publishers

About this paper

Cite this paper

Wdowiak, T.J., Flickinger, G.C., Cronin, J.R. (1988). IR Spectroscopy of Acid Insoluble Residues of Carbonaceous Chondrites. In: Bussoletti, E., Fusco, C., Longo, G. (eds) Experiments on Cosmic Dust Analogues. Astrophysics and Space Science Library, vol 149. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3033-9_13

Download citation

  • DOI: https://doi.org/10.1007/978-94-009-3033-9_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7863-4

  • Online ISBN: 978-94-009-3033-9

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics