小行星和安德西特.
Richard Arculus1, Ian H Campbell, Scott M McLennan
1Research School of Earth Sciences, Australian National University, Canberra, Australian Capital Territory 0200, Australia. Ross.Taylor@anu.edu.au
Nature
|May 30, 2009
概括
这项研究挑战了某些石代表小行星上形成石地的新方法的说法. 分析表明,关于石生成的现有理论仍然有效.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
背景情况:
- 在俯冲区的陆地石产量是众所周知的.
- 最近的一项研究提出了一种新的机制,用于在小行星上产生石地,使用石GRA 06128和GRA 06129.
研究的目的:
- 评估一项关于在小行星上产生石地的新模式的说法.
- 分析石GRA 06128和GRA 06129.的组成数据.
主要方法:
- 分析稀土元素 (REE) 和其他光电爱好者元素数据.
- 流星组成与行星地形成现有模型的比较.
主要成果:
- 构成数据,特别是REEs的构成数据,不支持拟议的石生成的新机制.
- 研究的石的组成与已知的石形成过程一致.
结论:
- 关于在小行星上产生石的新方式的说法没有得到提供的数据的支持.
- 目前产生石行星地的机制仍然有效,不需要修改.
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