在变形的海岸线的地形中,有古代火星海洋的证据
J Taylor Perron1, Jerry X Mitrovica, Michael Manga
1Department of Earth & Planetary Science, University of California, Berkeley, California 94720, USA. perron@eps.harvard.edu
Nature
|June 15, 2007
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
背景情况:
- 火星的北方平原可能是古代海洋的所在地.
- 被解释为古海岸线的表面特征支持了这一假设.
- 长波长的地形趋势挑战了海洋理论.
研究的目的:
- 为了调查沿着火星古海岸线的长波长地形的原因.
- 为了使地形数据与古代火星海洋假设相协调.
- 评估真正的极地流浪在塑造火星地形中的作用.
主要方法:
- 分析沿着火星海岸线推测的地形形状.
- 由真极流浪引起的行星变形的建模.
- 推断的极点路径与地质时间线的比较.
主要成果:
- 长波长地形与真正的极地漫游的变形相一致.
- 真正的极地流浪者解释了观察到的地形趋势.
- 推断的极点路径表明,一个真正的极地流浪事件是在塔西斯火山上升之后发生的.
结论:
- 真正的极地流浪者为火星海岸线的地形提供了可行的解释.
- 古代火星海洋假说得到了极地漫游的解释的支持.
- 这一发现为火星的地质和气候历史提供了新的见解.
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