相关实验视频
Updated: Jul 9, 2026

09:31
Surface Properties of Synthesized Nanoporous Carbon and Silica Matrices
Published on: March 27, 2019
观测证据表明,火星表面有一个活跃的固体二氧化碳储备
M C Malin1, M A Caplinger, S D Davis
1Malin Space Science Systems, Post Office Box 910148, SanDiego, CA 92191-0148, USA.
概括
火星 火星 火星 火星 火星
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 气候科学 气候科学
背景情况:
- 火星的南极残余盖表现出动态的表面特征.
- 以前的模型没有完全考虑观察到的侵蚀率.
研究的目的:
- 用高分辨率图像分析火星南极残留帽的变化.
- 为了确定驱动观察到的表面侵蚀的主要机制.
主要方法:
- 获取和比较1999年和2001年的高分辨率火星表面图像.
- 对坡的退缩和特征配置变化的定量分析.
主要成果:
- 观察到坑洞,山脊和山丘的显著变化.
- 悬崖每火星一年退缩1-3米.
- 侵蚀速度与二氧化碳冰的升温相一致,而不是水冰.
结论:
- 观测证实火星上存在大量固体二氧化碳的表面储备.
- 火星的气候不处于平衡状态,这表明正在进行的全球气候变化.
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