Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA.
Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.
Science. 2015 Jul 31;349(6247):521-4. doi: 10.1126/science.aaa9114.
Knowing when the geodynamo started is important for understanding the evolution of the core, the atmosphere, and life on Earth. We report full-vector paleointensity measurements of Archean to Hadean zircons bearing magnetic inclusions from the Jack Hills conglomerate (Western Australia) to reconstruct the early geodynamo history. Data from zircons between 3.3 billion and 4.2 billion years old record magnetic fields varying between 1.0 and 0.12 times recent equatorial field strengths. A Hadean geomagnetic field requires a core-mantle heat flow exceeding the adiabatic value and is suggestive of plate tectonics and/or advective magmatic heat transport. The existence of a terrestrial magnetic field before the Late Heavy Bombardment is supported by terrestrial nitrogen isotopic evidence and implies that early atmospheric evolution on both Earth and Mars was regulated by dynamo behavior.
了解地磁场何时开始对于理解地球核心、大气和生命的演化非常重要。我们报告了来自西澳大利亚杰克山砾岩(Jack Hills conglomerate)的具有磁性包裹体的太古宙到冥古宙锆石的全矢量古地磁强度测量结果,以重建早期地磁场历史。年龄在 33 亿至 42 亿年之间的锆石数据记录了磁场强度在 1.0 至 0.12 倍现代赤道场强之间的变化。需要有一个核心-地幔热流超过绝热值的冥古宙地磁场,这表明存在板块构造和/或对流岩浆热输运。地球氮同位素证据支持在晚期重轰炸之前存在地球磁场,这意味着地球和火星早期的大气演化都受到地磁场行为的调节。