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, Science 238, 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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 434-441 |
| Number of pages | 8 |
| Journal | Icarus |
| Volume | 156 |
| Issue number | 2 |
| DOIs | |
| State | Published - 2002 |
Keywords
- Asteroid composition
- Asteroid surfaces
- Infrared observations
- Organic chemistry
- Spectroscopy
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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