We report rotationally resolved spectra of six S-type asteroids obtained at ESO in the wavelength range 4900-9200 Γ . The sample was chosen to span most of the sub-classes defined by M. Gaffey et al. (1993, Icarus 106, 573-602). Three other asteroids of different taxonomic class were also analyzed in
Rotationally Resolved Spectra of Asteroid 16 Psyche
β Scribed by Richard P. Binzel; Schelte J. Bus; Shui Xu; Jessica Sunshine; Thomas H. Burbine; A.William Neely; Robert W. Brown
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 148 KB
- Volume
- 117
- Category
- Article
- ISSN
- 0019-1035
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