火星表面附近的的分布:证据表明地下冰沉积
W V Boynton1, W C Feldman, S W Squyres
1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. wboynton@lpl.arizona.edu
概括
火星奥德赛的火星奥德赛
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 地质地质地质地质地质地
背景情况:
- 火星拥有极地冰盖,但地下冰的范围和组成仍然是活跃研究的领域.
- 了解的分布是评估火星过去的可居住性和水资源潜力的关键.
研究的目的:
- 用轨道数据识别和描述火星上富含的地下区域.
- 调查这些沉积物的组成和物理状态.
主要方法:
- 利用了火星奥德赛轨道器上的马射线光谱仪的数据.
- 分析了与度相关的分布和柱密度,并预测了冰的稳定性区域.
主要成果:
- 确定了两个明显的极地区域,其中有显著的地下丰富.
- 观察到对面的贫层厚度在极点的方向下降.
- 富含的层与预测为水冰稳定的区域有很强的相关性.
结论:
- 地下很可能以水冰的形式存在,约占丰富层重量的35%.
- 这些发现支持火星极度上存在大量地下冰沉积物的存在.
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