证据表明水星上有一个没有玄武岩的表面,以及对内部热量的影响
R Jeanloz1, D L Mitchell, A L Sprague
1Department of Geology and Geophysics, University of California, Berkeley 94720, USA.
概括
水星 水星 水星 水星 水星
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 遥感 遥感 遥感 遥感
背景情况:
- 人们对水星表面的组成知之甚少.
- 以前的研究表明与月球有相似之处.
- 较高的白度表明了独特的表面材料.
研究的目的:
- 为了确定水星的表面组成.
- 将水星的组成与月球和地球进行比较.
- 为了了解水星的热进化和内部热保持.
主要方法:
- 微波观测的分析.
- 中红外观测的分析.
- 与月球和地球地幔组成的比较.
主要成果:
- 水星的表面含有较低的FeO + TiO2和与月球高原相比较的地含量.
- 水星的表面成分没有玄武岩.
- 表面构成与高可见的白度保持一致.
结论:
- 水星的地高度分化,没有玄武岩.
- 这支持了水星热进化的模型.
- 水星很可能保留一个热的内部由于低效的对流和低火山热量损失.
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