Direct age constraints on the magnetism of Jack Hills zircon

Author:

Taylor Richard J. M.1ORCID,Reddy Steven M.23ORCID,Saxey David W.23ORCID,Rickard William D. A.23ORCID,Tang Fengzai1ORCID,Borlina Cauê S.4ORCID,Fu Roger R.5ORCID,Weiss Benjamin P.4ORCID,Bagot Paul6ORCID,Williams Helen M.1ORCID,Harrison Richard J.1ORCID

Affiliation:

1. Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK.

2. School of Earth and Planetary Sciences, Curtin University, Bentley, WA 6102, Australia.

3. Geoscience Atom Probe Facility, John de Laeter Centre, Curtin University, Bentley, WA 6102, Australia.

4. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.

5. Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA.

6. Department of Materials, University of Oxford, Parks Road, Oxford OX1 3PH, UK.

Abstract

A potential record of Earth’s magnetic field going back 4.2 billion years (Ga) ago is carried by magnetite inclusions in zircon grains from the Jack Hills. This magnetite may be secondary in nature, however, meaning that the magnetic record is much younger than the zircon crystallization age. Here, we use atom probe tomography to show that Pb-bearing nanoclusters in magnetite-bearing Jack Hills zircons formed during two discrete events at 3.4 and <2 Ga. The older population of clusters contains no detectable Fe, whereas roughly half of the younger population of clusters is Fe bearing. This result shows that the Fe required to form secondary magnetite entered the zircon sometime after 3.4 Ga and that remobilization of Pb and Fe during an annealing event occurred more than 1 Ga after deposition of the Jack Hills sediment at 3 Ga. The ability to date Fe mobility linked to secondary magnetite formation provides new possibilities to improve our knowledge of the Archean geodynamo.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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