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在土星A环中的一个小月球带
Miodrag Sremcević1, Jürgen Schmidt, Heikki Salo
1Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, 392 UCB, Boulder, Colorado 80309-0392, USA. miodrag.sremcevic@lasp.colorado.edu
Nature
|October 26, 2007
概括
土星的环包含隐藏的小月亮,可能是破碎的月亮的残余. 这些小月亮支持行星环是由灾难性碰撞形成的,而不是逐渐积聚的理论.
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:
- 行星环的起源是行星科学中一个关键的未解决的问题.
- 土星A环中的螺旋形状特征表明存在小月球.
- 大型月球小行星的存在有利于灾难性的环形形成而不是共同遗传起源.
研究的目的:
- 探测和描述土星A环中的新的螺旋特征.
- 推断嵌入的月球小行星的大小,数量和分布.
- 为了研究这些小月亮对环形形成理论的影响.
主要方法:
- 对图像序列的分析,涵盖了土星的完整A环.
- 螺旋形状特征的识别和表征. 螺旋形状的特征.
- 模拟月球小行星的特性及其对环粒子的动态影响.
主要成果:
- 检测到八个新的螺旋特征,表明半径在30米至70米之间的月球小行星.
- 这些小月亮集中在一个狭窄的3000公里宽的圆环中.
- 由于石撞击,月球的寿命很短.
结论:
- 检测到的小月亮很可能是更大,破碎的环状月亮的残余.
- 这些小月球为戒指提供了新材料,支持灾难性的戒指创造.
- 这些发现支持了通过碰撞级联形成环的理论.
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