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
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA.
Science. 2005 Feb 25;307(5713):1214-20. doi: 10.1126/science.1101812.
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.
火星在其最初的十亿年里最为活跃。地核、地幔和地壳在太阳系形成后的大约5000万年里形成。对流的流体地核中的磁发电机使地壳磁化,全球磁场保护更厚重的早期大气层免受太阳风剥离。塔尔西斯地区成为火山活动、变形以及水和二氧化碳释放的焦点,释放量可能足以引发气候变暖事件。地表和近地表水促成了区域广泛的侵蚀、沉积物搬运和化学蚀变。深部热液循环加速了地壳冷却,保留了地壳厚度的变化,并改变了地壳磁化模式。