Asteroids with very slow rotation rates, up to 100 times slower than the mean for ordinary asteroids, are clearly a statistically distinct population from the rest. The cause of such slow rotation has remained a mystery since the discovery of the population about 20 years ago. The expected distribut
On the shape of rapidly rotating asteroids
✍ Scribed by P. Farinella; P. Paolicchi; V. Zappalà
- Publisher
- Elsevier Science
- Year
- 1981
- Tongue
- English
- Weight
- 166 KB
- Volume
- 1
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
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