may account for their fresh appearance. This mechanism of groove formation requires an interior which coherently trans-Asteroids respond to impact stresses differently from either mits elastic stress. While this precludes a classic ''rubble laboratory specimens or large planets. Gravity is typically
β¦ LIBER β¦
Cratering on Ida
β Scribed by Clark R. Chapman; Eileen V. Ryan; William J. Merline; Gerhard Neukum; Roland Wagner; Peter C. Thomas; Joseph Veverka; Robert J. Sullivan
- Book ID
- 102567379
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 317 KB
- Volume
- 120
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
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