进化的小行星地的早期形成
James M D Day1, Richard D Ash, Yang Liu
1Department of Geology, University of Maryland, College Park, Maryland 20742, USA. jamesday@umd.edu
Nature
|January 9, 2009
概括
新发现的石揭示了以前未知的类型的进化地形成在小行星上. 这些富含地的岩石提供了早期太阳系过程和多样化的行星材料的证据.
科学领域:
- 行星科学 行星科学
- 宇宙化学 宇宙化学
- 地质地质地质地质地质地
背景情况:
- 行星地形成机制尚未完全理解.
- 地球的石地是通过板块构造形成的;月球的富含地的地是由岩海洋过程形成的.
- 一些小行星显示了地形成和分化的证据,但没有观察到进化的状地.
研究的目的:
- 为了调查新发现的石GRA 06128和GRA 06129.的起源和组成.
- 了解太阳系早期小行星上地形成的过程.
主要方法:
- 使用放射测量方法测定石的年代.
- 元素和同位素组成分析.
- 石化和变形分析.
主要成果:
- 石GRA 06128和GRA 06129是富含地的石,其中石有大量的成分.
- 它们的年龄为4.52 ± 0.06 Gyr,表明它们在太阳系历史的早期形成.
- 构成和同位素数据表明,由挥发性丰富的氧化小行星的部分融化形成.
结论:
- GRA 06128和06129代表了小行星上新风格的进化地形成.
- 这些发现表明它们的母小行星的差异化不完全.
- 这一发现突显了太阳系早期材料中以前未知的多样性.
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