4.8 Review

New perspectives on ancient Mars

期刊

SCIENCE
卷 307, 期 5713, 页码 1214-1220

出版社

AMER ASSOC ADVANCEMENT SCIENCE
DOI: 10.1126/science.1101812

关键词

-

向作者/读者索取更多资源

Mars was most active during its first billion years. The core, mantle, and crust formed within similar to50 million years of solar system formation. A magnetic dynamo in a convecting fluid core magnetized the crust, and the global field shielded a more massive early atmosphere against solar wind stripping. The Tharsis province became a focus for volcanism, deformation, and outgassing of water and carbon dioxide in quantities possibly sufficient to induce episodes of climate warming. Surficial and near-surface water contributed to regionally extensive erosion, sediment transport, and chemical alteration. Deep hydrothermal circulation accelerated crustal cooling, preserved variations in crustal thickness, and modified patterns of crustal magnetization.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.8
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据