彗星在奥尔特云形成期间的快速碰撞进化
1Space Studies Department, Southwest Research Institute, Boulder, Colorado 80302, USA. astern@swri.edu
Nature
|February 24, 2001
概括
物理碰撞,不仅仅是重力,显著影响彗星喷射到奥特云. 这些碰撞可能会限制到达外太阳系的彗星数量.
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:
- 据信奥尔特云是由巨行星抛出的冰体形成的.
- 以前的模型仅使用引力影响来模拟奥特云的形成.
研究的目的:
- 为了调查物理碰撞在彗星喷射到奥特云中的作用.
- 重新评估现有的欧特云形成模型.
主要方法:
- 包含引力效应和物理碰撞的动态模拟.
- 在原太阳星云中对彗星碰撞进化的分析.
主要成果:
- 物理碰撞在彗星喷射中发挥着至关重要的,以前未被探索的作用.
- 彗星的侵蚀寿命比密集的星云区域的动态喷射时间缩短.
- 碰撞可能会阻止彗星广泛逃逸,直到磁盘质量减少.
结论:
- 碰撞过程是奥特云形成的一个基本因素.
- 奥尔特云中的彗星总质量可能被高估了.
- 未来的模型必须包括碰撞效应,以准确进行太阳系进化研究.
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