首页 | 本学科首页   官方微博 | 高级检索  
     检索      


New perspectives on ancient Mars
Authors:Solomon Sean C  Aharonson Oded  Aurnou Jonathan M  Banerdt W Bruce  Carr Michael H  Dombard Andrew J  Frey Herbert V  Golombek Matthew P  Hauck Steven A  Head James W  Jakosky Bruce M  Johnson Catherine L  McGovern Patrick J  Neumann Gregory A  Phillips Roger J  Smith David E  Zuber Maria T
Institution:Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA. scs@dtm.ciw.edu
Abstract:Mars was most active during its first billion years. The core, mantle, and crust formed within approximately 50 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.
Keywords:
本文献已被 PubMed 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号