We present results from a paleomagnetic study of the previously undated Erayinia dykes intruding the south-western Yilgarn Craton. The U-Pb TIMs baddeleyite age of these dykes is now 2401±1Ma, which is about 10m.y. younger than the 2418-2410Ma Widgiemooltha dyke swarm. The paleomagnetic study isolated a stable primary remanence with steep downward direction, and the paleomagnetic pole (22.7°S, 150.5°E, A95=11.4°) is similar, but not identical to that of the previously studied Widgiemooltha dykes. We interpret this difference as the result of the movement of the Yilgarn Craton toward the pole at ~1°/m.y. angular speed, which is comparable with tectonic plates' velocities during the Phanerozoic. Paleomagnetic polarities of Widgiemooltha and Erayinia dykes suggest that at least one geomagnetic reversal occurred between these two magmatic events. The estimated amplitude of geomagnetic secular variations at c. 2400Ma is slightly higher than predicted by the existing models for the last 5m.y. at the c. 64° latitude. The paleomagnetic data and patterns of c. 2.6-2.1Ga mafic dyke swarms permit the recently suggested reconstruction of the Paleoproterozoic supercontinent.

Additional Metadata
Keywords Mafic dykes, Paleomagnetism, Paleoproterozoic, Supercontinent, U-Pb TIMs age, Yilgarn Craton
Persistent URL dx.doi.org/10.1016/j.precamres.2014.05.023
Journal Precambrian Research
Citation
Pisarevsky, S.A. (Sergei A.), De Waele, B. (Bert), Jones, S. (Sarah), Söderlund, U. (Ulf), & Ernst, R.E. (2015). Paleomagnetism and U-Pb age of the 2.4Ga Erayinia mafic dykes in the south-western Yilgarn, Western Australia: Paleogeographic and geodynamic implications. Precambrian Research, 259, 222–231. doi:10.1016/j.precamres.2014.05.023