Department of Earth Science, Graduate School of Science, Tohoku University, 6-3 Aramakiaza-Aobu, Aoba-ku, Sendai 980 8578, Japan.
Nat Commun. 2013;4:2649. doi: 10.1038/ncomms3649.
The majority of water has vanished from modern meteorites, yet there remain signatures of water on ancient asteroids. How and when water disappeared from the asteroids is important, because the final fluid-concentrated chemical species played critical roles in the early evolution of organics and in the final minerals in meteorites. Here we show evidence of vestigial traces of water based on a nanometre-scale palaeomagnetic method, applying electron holography to the framboids in the Tagish Lake meteorite. The framboids are colloidal crystals composed of three-dimensionally ordered magnetite nanoparticles and therefore are only able to form against the repulsive force induced by the surface charge of the magnetite as a water droplet parches in microgravity. We demonstrate that the magnetites have a flux closure vortex structure, a unique magnetic configuration in nature that permits the formation of colloidal crystals just before exhaustion of water from a local system within a hydrous asteroid.
大部分水已经从现代陨石中消失,但在古老的小行星上仍然有水的痕迹。水从小行星中消失的方式和时间很重要,因为最终的流体浓缩化学物质在有机物的早期演化和陨石中的最终矿物质中发挥了关键作用。在这里,我们通过纳米级古地磁方法,应用电子全息术研究塔吉什湖陨石中的莓球,证明了水的残余痕迹。莓球是由三维有序的磁铁矿纳米颗粒组成的胶体晶体,因此只能在微重力下,当水滴蒸发时,由磁铁矿表面电荷产生的斥力诱导下形成。我们证明了磁铁矿具有磁通闭合涡旋结构,这是一种在自然界中独特的磁性结构,允许胶体晶体在含水小行星内的局部系统中的水耗尽之前形成。