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46 亿年前,在早期太阳系中形成了磁铁矿 3D 胶体晶体。

Magnetite 3D colloidal crystals formed in the early solar system 4.6 billion years ago.

机构信息

Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University, 6-3 Aramaki Aza-Aoba, Sendai 980-8578, Japan.

出版信息

J Am Chem Soc. 2011 Jun 15;133(23):8782-5. doi: 10.1021/ja2005708. Epub 2011 May 18.

Abstract

Three-dimensional colloidal crystals made of ferromagnetic particles, such as magnetite (Fe(3)O(4)), cannot be synthesized in principle because of the strong attractive magnetic interaction. However, we discovered colloidal crystals composed of polyhedral magnetite nanocrystallites of uniform size in the range of a few hundred nanometers in the Tagish Lake meteorite. Those colloidal crystals were formed 4.6 billion years ago and thus are much older than natural colloidal crystals on earth, such as opals, which formed about 100 million years ago. We found that the size of each individual magnetite particle determines its morphology, which in turn plays an important role in deciding the packing structure of the colloidal crystals. We also hypothesize that each particle has a flux-closed magnetic domain structure, which reduces the interparticle magnetic force significantly.

摘要

由铁磁粒子(如磁铁矿(Fe3O4))制成的三维胶体晶体原则上无法合成,因为它们之间存在强烈的吸引力。然而,我们在塔吉什湖陨石中发现了由几百纳米范围内的多面体形磁铁矿纳米晶体组成的胶体晶体。这些胶体晶体形成于 46 亿年前,因此比地球上形成于约 1 亿年前的天然胶体晶体(如蛋白石)要古老得多。我们发现,每个磁铁矿颗粒的大小决定了其形态,而形态又在决定胶体晶体的堆积结构方面起着重要作用。我们还假设每个颗粒都具有磁畴结构,这显著降低了颗粒间的磁力。

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