摘要 : Most asteroids with a diameter larger than similar to 300 m are rubble piles, i.e., consisting of more than one solid object. All asteroids are rotating but almost all asteroids larger than similar to 300 m rotate with a period lo... 展开
作者 | Persson~ B. N. J. Biele~ J. |
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作者单位 | |
期刊名称 | 《Tribology letters》 |
总页数 | 19 |
语种/中图分类号 | 英语 / TH117 |
关键词 | adhesion Capillary bridges Van der Waals interaction Asteroids Break-up Granular CONTACT MECHANICS RUBBER-FRICTION ROUGH SURFACES ADHESION MODEL REGOLITH FORCES PARTICLES STRENGTH ENERGY |
馆藏号 | N2008EPST0010681 |