在Ceres的水性改变的规流体内大量的水冰:核光谱的证据
T H Prettyman1, N Yamashita2, M J Toplis3
1Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719-2395, USA. prettyman@psi.edu.
概括
矮行星塞雷斯的表面元素组成显示出显著的水冰含量,表明过去的水性变化和潜在的冰岩分化. 这表明冰在表面下长期存活.
科学领域:
- 星球科学
- 天文地质学
- 天体化学
背景情况:
- 矮行星塞雷斯的表面组成为其地质历史和挥发性内容提供了关键的见解.
- 对于解读水性变化和内部进化过程来说,了解规律石的组成至关重要.
研究的目的:
- 确定Ceres的表面元素组成 (,铁,).
- 为了限制Ceres的规律冰含量和水性变化历史.
- 调查潜在的冰岩分裂和内部演变.
主要方法:
- 分析了美国宇航局"黎明"任务中的核光谱数据.
- 在Ceres表面的元素度的量化.
主要成果:
- 表面材料显示了塞雷斯内部的水性处理的证据.
- 与碳状地石相比,Ceres的碳含量较高,但铁度较低.
- 在中高度的高度表明大量的地下水冰.
结论:
- 塞雷斯的表面构成表明冰岩的碎裂发生了.
- 表面下有大量的水冰,
- 这些发现支持塞雷斯冰的稳定性理论模型.
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