铁石证据证明了原行星的早期形成和灾难性破坏
Jijin Yang1, Joseph I Goldstein, Edward R D Scott
1Department of Mechanical and Industrial Engineering, University of Massachusetts, Amherst, Massachusetts 01003, USA. jiyang@ecs.umass.edu
Nature
|April 20, 2007
概括
铁石的冷却速度揭示了早期的原行星比以前认为的要大. 这些发现挑战了行星积聚的传统模型,并表明更大的撞击事件形成了第一个行星.
科学领域:
- 行星科学 行星科学
- 宇宙化学 宇宙化学
- 天体物理学 天体物理学
背景情况:
- 行星是通过较小的天体的碰撞成长而形成的,包括原行星.
- 铁石提供了关于早期行星积聚的见解,因为它们的起源很古老.
- 传统模型表明,根据石冷却速度,差异化的物体直径为5-200公里.
研究的目的:
- 为了研究IVA组铁石的冷却速度.
- 重新评估早期分化物体的大小和性质.
- 为了测试行星积聚的传统模型.
主要方法:
- 使用改进模型分析IVA组铁石的冷却速度.
- 从独立的冷却速率指标中纳入新的数据.
- 测量石中的大量含量.
主要成果:
- 对于IVA铁石的冷却速度在100到6000K Myr (-1) 之间,随着散装Ni的减少而增加.
- 在小物体中采用同热冷却的传统模型不再可行.
- 结果表明,IVA石冷却在一个直径为300公里的金属体内,缺乏绝缘地幔.
结论:
- 大约10^3公里的原行星在最初的1.5亿年内形成.
- 这些大型原行星可能是通过"撞击逃跑"碰撞形成的.
- 这些早期的大型天体的碎片可能作为小行星存活下来.
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