Secondary magnetite in ancient zircon precludes analysis of a Hadean geodynamo
Secondary magnetite in ancient zircon precludes analysis of a Hadean geodynamo
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DOI:
10.1073/pnas.1811074116
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发表时间:
2018-12
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通讯作者:
Fengzai Tang;Richard J. M. Taylor;J. Einsle;C. Borlina;R. Fu;Benjamin P. Weiss;Helen M. Williams;W. Williams;L. Nagy;Paul A. Midgley;E. Lima;Elizabeth A. Bell;T. M. Harrison;Ellen W. Alexander;R. Harrison
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文献类型:
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作者:
Fengzai Tang;Richard J. M. Taylor;J. Einsle;C. Borlina;R. Fu;Benjamin P. Weiss;Helen M. Williams;W. Williams;L. Nagy;Paul A. Midgley;E. Lima;Elizabeth A. Bell;T. M. Harrison;Ellen W. Alexander;R. Harrison
Significance The Earth’s geodynamo is critical in protecting our atmosphere, and thus plays an important role in the habitability of our planet. As such, the Earth’s magnetic field has likely played a crucial role in the emergence of life around 4 billion years ago during the Hadean–Archean Eons. However, we know little about the behavior of the geodynamo during this critical period. Recent efforts have focused on the magnetic signals harbored by Jack Hills zircon crystals, the oldest terrestrial material. Here we show the magnetic carriers in such grains. Our results demonstrate that although ancient zircon grains may contain ideal magnetic recorders, they do not record the magnetic field strength at the time of zircon growth. Zircon crystals from the Jack Hills, Western Australia, are one of the few surviving mineralogical records of Earth’s first 500 million years and have been proposed to contain a paleomagnetic record of the Hadean geodynamo. A prerequisite for the preservation of Hadean magnetization is the presence of primary magnetic inclusions within pristine igneous zircon. To date no images of the magnetic recorders within ancient zircon have been presented. Here we use high-resolution transmission electron microscopy to demonstrate that all observed inclusions are secondary features formed via two distinct mechanisms. Magnetite is produced via a pipe-diffusion mechanism whereby iron diffuses into radiation-damaged zircon along the cores of dislocations and is precipitated inside nanopores and also during low-temperature recrystallization of radiation-damaged zircon in the presence of an aqueous fluid. Although these magnetites can be recognized as secondary using transmission electron microscopy, they otherwise occur in regions that are indistinguishable from pristine igneous zircon and carry remanent magnetization that postdates the crystallization age by at least several hundred million years. Without microscopic evidence ruling out secondary magnetite, the paleomagnetic case for a Hadean–Eoarchean geodynamo cannot yet been made.