Paleomagnetic age of ferruginous weathering beneath the Hamersley Surface, Pilbara, Western Australia, and the Cenozoic apparent polar wander path

ABSTRACT

During the Mesozoic and Paleogene, the Precambrian rocks in the Pilbara, Western Australia, underwent erosion and deep weathering that produced an undulating landform now represented by the duricrusted and partly eroded Hamersley Surface. A reddened, ferruginous weathering zone occurs immediately beneath this duricrusted surface. Oriented block samples of ferruginised strata of the Neoarchean–early Paleoproterozoic Hamersley Group exposed within approximately 15 m below the duricrust were collected at 20 sites in roadcuts along the Great Northern Highway between Munjina and Newman and exposures along the adjoining Karijini Drive. Stepwise thermal demagnetisation of cored specimens revealed a stable, high-temperature (680°C) component carried by hematite, with a mean direction (n = 55 specimens) of declination D = 182.0°, inclination I = 52.9° (α₉₅ = 3.6°), indicating a pole position at latitude λ_p = 77.6°S, longitude ϕ_p = 113.2°E (A₉₅ = 4.3°) and a paleolatitude λ = 33.5 +3.6/–3.3°S. Both normal and reversed polarities are present, indicating that the remanent magnetism was acquired over an interval of at least two polarity chrons (say 10⁵–10⁶ years). Chi-square tests on the determined pole position and three different sets of Cenozoic poles, namely those for dated volcanic rocks in eastern Australia supplemented by poles for Australian Cenozoic weathering horizons, and inferred poles from Pacific Ocean and Indian Ocean hotspot analyses and North American Cenozoic poles rotated to Australian coordinates, yielded a mean age of ca 24 ± 3 Ma, i.e. late Oligocene to early Miocene, interpreted as the time of formation of hematite in the sampled ferruginous zone. The ferruginous weathering occurred under globally warm conditions and was followed during the early to middle Miocene climatic optimum by the deposition of channel iron deposits, which incorporated detrital hematitic material derived from erosion of the ferruginous weathering zone beneath the Hamersley Surface.

KEYWORDS:

• Pilbara Craton
• Hamersley Province
• Hamersley Surface
• lateritic weathering
• paleomagnetism
• apparent polar wander path
• Oligocene
• Miocene
• channel iron deposits

Acknowledgements

Field and laboratory costs were partly defrayed by an Australian Research Council Large Grant (A39943022). Laboratory work was carried out at the CSIRO Palaeomagnetic Laboratory, North Ryde, Sydney. Bob Musgrave and Brad Pillans are thanked for critical comments.

Disclosure statement

No potential conflict of interest was reported by the authors.

Supplementary paper

The spreadsheet used to combine Euler poles and perform rotations and other calculations.