撞击逃跑的行星碰撞
Erik Asphaug1, Craig B Agnor, Quentin Williams
1Earth Sciences Department, Institute for Geophysics and Planetary Physics, 1156 High St, University of California, Santa Cruz, California 95064, USA.
Nature
|January 13, 2006
概括
在陆地行星形成过程中,巨大的撞击可能会导致行星的形成.
科学领域:
- 行星科学 行星科学
- 天体物理学 天体物理学
- 地质地质地质地质地质地
背景情况:
- 地球行星的形成被认为是以巨大的撞击结束的.
- 数百颗行星胚胎碰撞,形成了行星,月球和小行星.
研究的目的:
- 为了研究行星碰撞的结果,而不仅仅是简单的合并.
- 了解新型碰撞动态对行星形成的影响.
主要方法:
- 星球胚胎碰撞的模拟.
- 对碰撞结果的分析,包括变形和碎片化.
主要成果:
- 碰撞的行星并不总是合并;较小的行星可以逃脱.
- 碰撞的结果包括变形,旋转,压缩和碎片化.
- 撞逃碰撞会产生各种各样的残留物.
结论:
- 撞逃碰撞是行星形成的一个重要因素.
- 这些碰撞残留物与小行星形成和石起源有关.
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