火星近期气候变化的证据来自识别了年轻的近地表面地面冰层
J F Mustard1, C D Cooper, M K Rifkin
1Department of Geological Sciences, Brown University, Providence, Rhode Island 02912, USA. john_mustard@brown.edu
Nature
|July 27, 2001
概括
在火星中度地区发现了地下水冰,这表明有大量的冷水库. 这种在土壤孔隙中发现的地面冰,在过去的气候时期形成后,目前正在减少.
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 天体生物学 天体生物学
背景情况:
- 火星地和土壤中的地下冰构成了大量的水库.
- 接近地表的地面冰被预测为40度度的稳定极点,观察到的地形特征支持这一点.
- 中度土壤是潜在的水冰储存库,其容量受到轨道气候周期的影响.
研究的目的:
- 为了调查火星中度的近地表面地面冰的存在和范围.
- 为了量化这种潜在的水冰库的体积.
- 了解时间动态和中度地面冰的起源.
主要方法:
- 收集了观测证据,以确定近地表的水冰.
- 对被冰所占的土壤水库厚度和度分布的分析.
- 根据火星气候历史推断水库形成和退化时间表.
主要成果:
- 直接的观测证据证实,在土壤毛孔空间内,近地表水冰的中度水库存在.
- 这块被冰覆盖的土壤储存库跨越30至60度度带,厚度为1-10米.
- 估计的水库容量是 (1.5-6.0) x 10^4 km3,相当于10-40厘米的全球水层.
结论:
- 发现的中度地下冰库是火星上重要的水资源.
- 这座水库很可能是在不到10万年前的高轨道倾斜期形成的.
- 当前的气候条件正在导致地下水冰的体积减少.
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