最近形成的土星小卫星是由于主要环的粘性扩散而形成的
Sébastien Charnoz1, Julien Salmon, Aurélien Crida
1Laboratoire AIM, Université Paris Diderot/CEA/CNRS, 91191 Gif sur Yvette, France. charnoz@cea.fr
Nature
|June 11, 2010
概括
土星的小卫星比预期的要年轻,很可能是由土星的环组成的. 模拟显示粘性环扩散超出罗氏极限创造了这些卫星,并塑造了主要环和F环.
科学领域:
- 行星科学 行星科学
- 天体物理学 天体物理学
- 太阳系的形成太阳系的形成
背景情况:
- 巨行星的常规卫星大约在4.5 Gyr前形成.
- 土星拥有动态年轻的卫星 (<10^7年),密度低 (~600公斤/m−3) 和环状的光谱特征.
- 以前的模型无法完全解释这些小卫星的形成,因为计算的局限性.
研究的目的:
- 为了模拟土星小卫星的形成过程.
- 为了研究土星环边缘的小月球的积累.
- 了解环形动力学与卫星形成之间的关系.
主要方法:
- 使用混合模拟方法.
- 模拟了土星环的粘性扩散超出罗氏极限.
- 研究了环内部的引力不稳定性和积累过程.
主要成果:
- 模拟成功复制了小月球的质量分布和轨道结构.
- 证明了超出罗氏极限的粘性环扩散是小月球形成的可行机制.
- 显示卫星形成与粘性环的演变相结合.
结论:
- 土星的小卫星最近 (<107年前) 从土星的环中分离出来.
- 土星主要环的封闭和F环的存在是这种结合粘性进化和卫星形成过程的结果.
- 土星的环可能代表了太阳系最近的一个活跃积聚的地点,类似于一个小型的原行星盘.
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