Time-space evolution of an Archean craton: a Hf-isotope window into continent formation

D. R. Mole*, C. L. Kirkland, M. L. Fiorentini, S. J. Barnes, K. F. Cassidy, C. Isaac, E. A. Belousova, M. Hartnady, N. Thebaud

*Corresponding author for this work

Research output: Contribution to journalReview articlepeer-review

72 Citations (Scopus)
290 Downloads (Pure)


The Yilgarn Craton of Western Australia represents one of the largest pieces of Precambrian crust on Earth, and a key repository of information on the Meso-Neoarchean period. Understanding the crustal, tectonic, thermal, and chemical evolution of the craton is critical in placing these events into an accurate geological context, as well as developing holistic tectonic models for the Archean Earth. Here, we present a large U-Pb (420 collated samples) and Hf isotopic (2163 analyses) dataset on zircon, and apply it to constrain the evolution of the craton. These data provide strong evidence for a Hadean-Eoarchean origin for the Yilgarn Craton from mafic crust at ca. 4000 Ma, in a proto-craton consisting of the Narryer and north-central Southern Cross Domain. This ancient cratonic nucleus was subsequently rifted, expanded and reworked by successive crustal growth events at ca. 3700 Ma, ca. 3300 Ma, 3000–2900 Ma, 2825–2800 Ma, and ca. 2730–2620 Ma. The <3050 Ma crustal growth events correlate broadly with known komatiite events, and patterns of craton evolution, revealed by Hf isotope time-slice mapping, image the periodic break-up of the Yilgarn proto-continent and the formation of rift-zones between the older crustal blocks. Crustal growth and new magmatic pulses were focused into these zones and at craton margins, resulting in continent growth via internal (rift-enabled) expansion, and peripheral (crustal extraction at craton margins) magmatism. Consequently, we interpret these major geodynamic processes to be analogous to plume-lid tectonics, where the majority of tonalite-trondhjemite-granodiorite (TTG) felsic crust, and later granitic crust, was formed by reworking of hydrated mafic rocks and TTGs, respectively, via a combination of infra-crustal and/or drip-tectonic settings. We argue that subduction-like processes formed a minor tectonic component, re-docking the Narryer Terrane to the craton at ca. 2740 Ma. Overall, these processes led to an intra-cratonic architecture of younger, juvenile terranes located internal and external to older, long-lived, reworked crustal blocks. This framework provided pathways that localized later magmas and fluids, driving the exceptional mineral endowment of the Yilgarn Craton.

Original languageEnglish
Article number102831
Pages (from-to)1-46
Number of pages46
JournalEarth-Science Reviews
Publication statusPublished - Sept 2019

Bibliographical note

Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.


  • Continental crust
  • Crustal evolution
  • Geochronology
  • Plume tectonics
  • Subduction
  • Yilgarn


Dive into the research topics of 'Time-space evolution of an Archean craton: a Hf-isotope window into continent formation'. Together they form a unique fingerprint.

Cite this