欧罗巴上的二次石坑以及对石坑表面的影响
Edward B Bierhaus1, Clark R Chapman, William J Merline
1Lockheed Martin, Space Exploration Systems, MS S8110, PO Box 179, Denver, Colorado 80201, USA. edward.b.bierhaus@lmco.com
Nature
|October 21, 2005
概括
像欧罗巴这样的冰月上的小石坑大多是次要撞击,而不是主要撞击. 这一发现表明,整个太阳系的大多数小石坑也是次要的,挑战了关于行星表面日期的先前假设.
科学领域:
- 行星科学 行星科学
- 撞击坑研究 撞击坑研究
- 太阳系探索 太阳系探索
背景情况:
- 传统上,行星研究假设撞击坑群主要反映了直接的小行星和彗星撞击.
- 固体表面物体上的地质单位的年龄估计依赖于这种主要冲击假设.
- 形成坑的记录对于理解行星进化和表面年龄至关重要.
研究的目的:
- 为了分析木星的卫星欧罗巴上的火山口人口.
- 重新评估小石坑主要是由初级撞击造成的假设.
- 调查欧罗巴小坑 (直径小于1公里) 的起源.
主要方法:
- 分析欧罗巴的稀疏坑群.
- 对石坑大小分布的统计检查.
- 观察到的石坑数据与撞击模型的比较.
主要成果:
- 二次石坑 (由较大的撞击物质抛出而形成) 占欧洲大约95%的小石坑 (直径小于1公里).
- 这表明,大型初级撞击产生的次要石坑比以前估计的要多得多.
- 这项研究表明,最近在木星系统中,小彗星 (<100米) 的稀缺性很大.
结论:
- 对于欧洲来说,小石坑主要是直接撞击造成的假设是不正确的.
- 月球,火星和其他天体上的小火山口人口很可能是由次要撞击所主导的.
- 修订石坑模型对于准确的年龄测定和了解行星表面过程是必要的.
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