EGU2020-6395
https://doi.org/10.5194/egusphere-egu2020-6395
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Ultramafic rocks at the Isua supracrustal belt and East Pilbara Terrane are crustal cumulates, not slices of early mantle

Jiawei Zuo1, Alex Webb1, Jason Harvey2, Peter Haproff3, Thomas Mueller2, Gary Byerly4, Arthur Hickman5, and Qin Wang6
Jiawei Zuo et al.
  • 1Department of Earth Sciences and Laboratory for Space Research, University of Hong Kong, Pokfulam Road, Hong Kong, 999077, China.
  • 2School of Earth and Environment, University of Leeds, Maths/Earth and Environment Building, Leeds LS2 9JT, United Kingdom.
  • 3Department of Earth and Ocean Sciences, University of North Carolina Wilmington, 601 S. College Rd., Wilmington, North Carolina 28403, USA.
  • 4Department of Geology and Geophysics, Louisiana State University, Baton Rouge LA 70803, USA.
  • 5Geological Survey of Western Australia, 100 Plain St., East Perth, Western Australia 6004, Australia.
  • 6State Key Laboratory for Mineral Deposits Research, Department of Earth Sciences, Nanjing University, Xianlin Avenue 163, Nanjing 210046, China.

The initiation of plate tectonics remains enigmatic, with the proposed onset timing ranging from Hadean to Proterozoic. Recently, many mineralogical, petrological and geochemical studies suggest onset of plate tectonics at ~3 Ga. For example, the geology of East Pilbara Terrane (~3.55 to 2.70 Ga; Australia) is widely interpreted as representing Paleoarchean non-plate tectonics, followed by plate tectonics after a ~3.2 Ga transition. In contrast, Isua supracrustal belt (3.85 to 3.55 Ga; Greenland) has been dominantly interpreted via plate tectonics. There, two ultramafic lenses have been interpreted as depleted mantle slices, emplaced via thrusting in an Eoarchean subduction zone, implying early plate tectonics. We present new petrological and geochemical data of ultramafic samples from the Isua lenses and from the East Pilbara Terrane to explore their origins. Pilbara samples appear to preserve cumulate textures; protolith textures of Isua samples are altered beyond recognition. Samples with low chemical alteration show similar whole-rock chemistry, including up to 5.0 wt.% Al2O3 and up to 0.25 wt.% TiO2 that both covary negatively with MgO (37.1 to 47.5 wt.%); these variations suggest cogenetic relationships with local lavas. Flat trace-element fractionation trends parallel those of local lavas in the primitive-mantle normalized spider diagram. Spinel crystals from Pilbara samples yield ~20-60 Mg#, relatively constant Cr# at ~70, and 0.61-4.81 wt.% TiO2. Our data are consistent with crustal cumulate emplacement. In contrast with depleted mantle rocks, our samples have higher whole-rock Al2O3 and TiO2, flat (vs. upward) trace-element fractionation trends from less to more compatible elements, and spinel crystals with higher TiO2 and relatively constant (vs. varied) Cr#. Therefore, Isua and Pilbara ultramafic rocks may have similar, non-plate tectonic origins, and the Isua record allows a ~3 Ga onset of plate tectonics.

How to cite: Zuo, J., Webb, A., Harvey, J., Haproff, P., Mueller, T., Byerly, G., Hickman, A., and Wang, Q.: Ultramafic rocks at the Isua supracrustal belt and East Pilbara Terrane are crustal cumulates, not slices of early mantle, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-6395, https://doi.org/10.5194/egusphere-egu2020-6395, 2020

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