We present near-infrared spectrometer (NIS) observations (0.8 to 2.4 ยตm) of the S-type asteroid 433 Eros obtained by the NEAR Shoemaker spacecraft and report results of our Hapke photometric model analysis of data obtained at phase angles ranging from 1.2 โข to 111.0 โข and at spatial resolutions of 1
Near-Infrared Spectroscopy of Dark Asteroids
โ Scribed by M.A. Barucci; M. Lazzarin; T. Owen; C. Barbieri; M. Fulchignoni
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 224 KB
- Volume
- 110
- Category
- Article
- ISSN
- 0019-1035
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โฆ Synopsis
Near-infrared (J, H and K bands) spectra of nine dark asteroids (chosen among a sample of supposed primitive objects between C and D classes) have been obtained at the Mauna Kea Observatory (Hawaii) with the 2.2-m telescope using KSPEC as spectrograph. The aim of this work was to search for evidence of the presence of organic materials in these objects as found in other planetary bodies as 5145 Pholus, and in some cometary nuclei. A careful analysis of the data has revealed flat or slightly redder spectra than the solar one for all observed asteroids. No evidence of distinct absorption features was found.
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