在大型撞击坑中形成峰环
Joanna V Morgan1, Sean P S Gulick2, Timothy Bralower3
1Department of Earth Science and Engineering, Imperial College London, SW7 2AZ, UK. j.morgan@imperial.ac.uk.
概括
大规模撞击会通过抬起深层岩石而形成行星峰环. 奇克苏鲁布峰环由破碎的地下岩石形成, 揭示了撞击机制和地变化.
科学领域:
- 行星地质学
- 撞击坑的形成
- 地质学
背景情况:
- 大规模撞击会通过混合地物质使行星重新浮现.
- 撞击坑中的中心峰会随着大小的增加而转变为峰环.
- 由于直接采样有限,峰环的形成和起源深度仍然存在争议.
研究的目的:
- 调查奇克苏鲁布峰环的形成机制和起源.
- 了解大冲击在行星地进化中的作用.
主要方法:
- 通过Expedition 364钻探获得的Chixulub峰环岩石样本的分析.
- 对岩石破裂,冲击效应和石质学的检查.
- 测量诸如密度和地震速度之类的物理性质.
主要成果:
- 奇克苏鲁布峰环岩是升起的,破碎的,震惊的,的地下材料.
- 这些岩石被堤和剪切区域截断.
- 峰环岩石的密度和地震速度异常低.
结论:
- 大规模撞击会在行星地内产生大量的垂直物质流.
- 撞击过程,就像在奇克苏鲁布,增加地的多孔性.
- 这项研究提供了峰环形成机制及其对行星地的影响的直接证据.
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