We have spectrophotometrically observed twenty M-class asteroids in the 1.2-to 3.5-µm region, sixteen of them for the first time. When we combined these with earlier surveys by Rivkin et al. (1995) and Jones et al. (1990) for a total of 27 asteroids, we find that over 35% of them have absorption fea
✦ LIBER ✦
The nature of c-class asteroids from 3-μm spectrophotometry
✍ Scribed by Michael A. Feierberg; Larry A. Lebofsky; David J. Tholen
- Publisher
- Elsevier Science
- Year
- 1985
- Tongue
- English
- Weight
- 669 KB
- Volume
- 63
- Category
- Article
- ISSN
- 0019-1035
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