Elsevier

Icarus

Volume 156, Issue 2, April 2002, Pages 434-441
Icarus

Regular Article
Search for the 3.4-μm C–H Spectral Bands on Low-Albedo Asteroids

https://doi.org/10.1006/icar.2001.6810Get rights and content

Abstract

A report of the detection of the C–H hydrocarbon band complex at 3.4 μm in an asteroid spectrum, by D. P. Cruikshank and R. H. Brown (1987, Science238, 183–184) is not confirmed by recent data of higher quality. Spectra of the same asteroid and six other low-albedo asteroids do not show this feature, which if present would indicate the presence of hydrocarbons and might link these asteroids with certain classes of carbonaceous meteorites.

References (36)

  • S.A. Sandford

    Infrared transmission spectra from 2.5 to 25 μm of various meteorite classes

    Icarus

    (1984)
  • F. Vilas

    A cheaper, faster, better way to detect water of hydration on Solar System bodies

    Icarus

    (1994)
  • F. Vilas et al.

    Ferric iron in primitive asteroids: A 0.43-μm absorption feature

    Icarus

    (1993)
  • Allamandola, L. J., M. P. Bernstein, and S. A. Sandford1997. Photochemical evolution of interstellar/precometry organic...
  • W.M. Calvin et al.

    Spectral characteristics of iron-bearing phyllosilicates: Comparison to Orgueil (CI1), Murchison and Murray (CM2)

    Meteorit. Planet. Sci.

    (1997)
  • Cronin, J. R., S. Pizzarello, and D. P. Cruikshank1988. Organic matter in carbonaceous chondrites, planetary...
  • D.P. Cruikshank et al.

    Organic matter on Asteroid 130 Elektra

    Science

    (1987)
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    Guest observers at the United Kingdom Infrared Telescope.

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