- UID
- 1236277
- 在线时间
- 小时
- 注册时间
- 2016-9-18
- 最后登录
- 1970-1-1
- 主题
- 帖子
- 性别
- 保密
|
6#
楼主 |
发表于 2018-5-16 16:56:12
|
只看该作者
When asteroids collide, some collisions cause an asteroid to spin faster; others slow it down. If asteroids are all monoliths-single rocks-undergoing random collisions, a graph of their rotation rates should show a bell-shaped distribution with statistical “tails” of very fast and very slow rotators. If asteroids are rubble piles, however, the tail representing the very fast rotators would be missing, because any loose aggregate spinning faster than once every few hours (depending on the asteroid’s bulk density) would fly apart. Researchers have discovered that all but five observed asteroids obey a strict limit on rate of rotation. The exceptions are all smaller than 200 meters in diameter, with an abrupt cutoff for asteroids larger than that.
The evident conclusion-that asteroids larger than 200 meters across are multicomponent structures or rubble piles-agrees with recent computer modeling of collisions, which also finds a transition at that diameter. A collision can blast a large asteroid to bits, but after the collision those bits will usually move slower than their mutual escape velocity. Over several hours, gravity will reassemble all but the fastest pieces into a rubble pile. Because collisions among asteroids are relatively frequent, most large bodies have already suffered this fate. Conversely, most small asteroids should be monolithic, because impact fragments easily escape their feeble gravity.
这一句话的理解要结合上下文,尤其第一句话末尾的rate of rotation。
前面说:行星碰撞之后,有的变快,有的变慢。但是如果是大块的行星随机碰撞之后,它们的旋转速率会呈现一个bell-shaped distribution,即"_n_"这个形状。也就是说,很慢的,和很快的,都很少,中间地带很多。但是如果是碎石群(前文中应该有谈到,行星分成整体单块儿monoliths-single的和小碎石集成的rubble piles),就不会存在速度非常快的,因为那样就被甩出去了,分崩离析了。然后重点来了:研究者发现了五个行星是遵循一个严格限制的旋转速率的(也就是说这些行星碰撞之后速率不呈现bell-shaped distrubition,而是较为固定的转速),而这些行星都是直径小于200米的,而且相较于那些大于这个直径的行星而言,这个分水岭很明显,也就是但凡大于200米的行星,就都又呈现bell shaped distribution了。
|
|