火星上的岩演化和多样性的证据来自红外观测
P R Christensen1, H Y McSween, J L Bandfield
1Department of Geological Sciences, Arizona State University Tempe, Arizona 85287, USA. phil.christensen@asu.edu
Nature
|July 12, 2005
概括
火星的岩石呈现出令人惊的多样性,从玄武岩到花岩. 这表明复杂的火山演化和岩过程类似于地球,挑战以前关于火星地的假设.
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 伊格尼岩石学 伊格尼岩石学
背景情况:
- 火星地主要被认为是玄武岩.
- 以前的组成测绘缺乏足够的分辨率来揭示微小的岩石多样性.
研究的目的:
- 为了研究火星岩性材料的组成多样性.
- 了解火星的火山和岩演变.
主要方法:
- 用100米尺度的火星奥德赛热发射成像系统 (THEMIS) 的数据绘制火星的组成地图.
- 对岩石组成的分析,包括玄武岩,大岩和花岩.
主要成果:
- 鉴定了多种不同的火性材料,从低基岩到高石和石英含量的花岩.
- 有证据表明,分数结晶导致了像大石这样的进化岩.
- 在各种深度发现的橄基岩,表明在整个火星地形成中广泛存在.
- 发现了花状岩石的发现表明了极端的岩分化.
结论:
- 火星地表现出与地球相似的组成范围,从皮克里特基岩到花岩.
- 火星火山的进化比以前认为的要复杂,涉及到显著的岩差异化.
- 在火星上,超玛基岩可能比目前估计的更为常见.
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