Research ArticleIsotopic mapping reveals the location of crustal fragments along a long-lived convergent plate boundary
Introduction
Convergent plate boundaries are complicated zones where slices of the Earth's crust of different age and composition (‘terranes’) are often juxtaposed. Unravelling the history of these zones is key to understanding what the Earth looked like in the past. New Guinea is recognised as one of the world's youngest arc–continent collisional orogens (Ali and Hall, 1995; Baldwin et al., 2012; Davies, 2012; Hall, 2002; Hill and Hall, 2003; Holm et al., 2016), but has acted as a plate boundary to the northern margin of the Australian Plate since the Triassic (Hill and Hall, 2003; Jost et al., 2018). If we can understand the tectonic evolution of New Guinea in its current setting, then we can use this knowledge to better understand other much older plate boundary systems.
The island of New Guinea marks the meeting point of the Australian, Philippine Sea, and Caroline tectonic plates (Bird, 2003; Hall and Spakman, 2003; Milsom et al., 1992; Tregoning and Gorbatov, 2004). The interaction of these plates during the Cenozoic saw the production of subduction-related volcanism, the collision and accretion of island arc volcanoes, as well as extensive strike-slip faulting. All of this tectonic activity has resulted in the island's current geological configuration, that is a complicated region of juxtaposed sections of oceanic and continental crust. The complicated tectonic history, together with large areas of difficult to access terrain (e.g., mountains, dense tropical rainforest, vegetated wetlands) has meant it has been difficult to identify the location of ancient plate boundaries.
Australian continental crust was initially proposed to extend no further north than the New Guinea Fold and Thrust belt in eastern New Guinea (Abers and McCaffrey, 1988). Recent studies from eastern New Guinea, however, show that underthrust Australian continental crust may continue north beneath the New Guinea Mobile Belt and be in contact with oceanic or island arc crust of the Marum Ophiolite and Adelbert–Finisterre–Huon Block along the Ramu–Markham Fault (Crowhurst et al., 1996). Isotopic studies from central New Guinea indicate that ancient Archaean or Proterozoic Australian continental crust extends north beneath the Central Range to at least the 4th parallel South (based on the location of crustally contaminated Pliocene–Pleistocene igneous rocks) (Housh and McMahon, 2000).
In addition, limited geophysical data exist in this region of the world. This means it is difficult to map the variation of crustal thicknesses across New Guinea. Those data that do exist (e.g., seismic tomography) have typically been applied to only eastern New Guinea (Abers, 1991; Abers and McCaffrey, 1988; Abers and Roecker, 1991) or used to image subducted slabs deeper in the mantle (Hall and Spakman, 2003), while other work has focussed on looking at upper crustal structures that may control the location of ore deposits (White et al., 2014) – however, all of this work has relied on predominately coarse resolution data. It therefore presents a significant challenge as to how one could map the crustal structure of New Guinea.
Recent Nd isotopic studies of the Australian continent have been used to isotopically map different geological domains, from Archaean–Proterozoic cratons to Palaeozoic arc and orogenic terranes (Champion, 2013; Champion and Huston, 2016; Mole et al., 2015). Such work has also been applied in the Himalaya (Ahmad et al., 2000; Richards et al., 2005), the western United States (Bennett and DePaolo, 1987), the Central Asian Orogenic Belt (Wang et al., 2009; Wang et al., 2015), and Antarctica (Borg and DePaolo, 1994), providing insight into the age and isotopic signature of juxtaposed terranes and the underlying crust. Here we take a similar approach using 87Sr/86Sr and 143Nd/144Nd whole-rock isotopic data from a series of Devonian–Carboniferous and Permian–Triassic basement rock granitoids, metamorphosed Mesozoic passive margin sedimentary rocks, Oligocene oceanic island arcs, and Miocene–Pleistocene magmatic rocks from NW New Guinea. Using these isotopic data, we define isotopic signatures for and map different crustal domains across the region. We then compared our data with existing isotopic data available from other parts of New Guinea to map the northern-most extent of Australian continental crust and other crustal fragments.
Section snippets
The crustal domains and tectonics of New Guinea
The island of New Guinea was largely formed by a long history of continental growth along an Andean-type subduction system during the Palaeozoic and Mesozoic, and the accumulation of multiple terranes along its northern margin throughout the Cenozoic (Fig. 1a). The number of terranes and their crustal affinities vary depending on individual studies. For instance, one article indicates that New Guinea consists of up to thirty-two separate terranes (Pigram and Davies, 1987). However, more recent
Whole-rock SrNd isotopic analysis
Twenty-two samples were analysed for their whole-rock SrNd isotopic compositions and LREE concentrations. For both Sr and Nd analyses, 0.1 g of bulk rock powder was dissolved using HF–HNO3 in Teflon beakers for 24 h at 180 °C, they were then evaporated and converted to nitrate by digestion in HNO3 before undergoing total dissolution in 10% HNO3. Twenty-five percent of the resulting solution was then removed for analysis of the light rare earth elements (LREEs). Strontium isotopes were
Whole-rock SrNd isotopic analysis
Twenty-one samples of volcanic, plutonic, metamorphic, and sedimentary rocks from the Bird's Head where analysed for whole-rock 87Sr/86Sr isotopic data, twenty of these samples were also analysed for whole-rock 147Sm/144Nd and 143Nd/144Nd data (Supplementary Data File 1). The remaining sample (MW15–024) did not contain enough Nd for 147Sm/144Nd and 143Nd/144Nd analyses. The results were sub-divided into six groups based on their isotopic values and their geographic location. These groups are
The isotopic signature and tectonic evolution of NW New Guinea
Determining the SrNd isotopic composition of the rocks of NW New Guinea and what they indicate for their source has implications for understanding the nature of the crust beneath NW New Guinea and determining the northern-most extent of Australian continental crust. It also provides a distinct isotopic signature for each of the terranes studied, allowing for the correlation of isotopic signatures and allochthonous terranes across New Guinea. This can in turn be coupled with tectonic
Conclusions
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SrNd isotopic data from rocks in the Bird's Head can be correlated with the isotopic compositions of coeval and cogenetic rocks across New Guinea and indicate the shared tectonic history of eastern and western New Guinea since at least the Triassic.
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Binary isotope mixing models combined with field and petrographic studies show that the middle Miocene Moon Volcanics erupted through thinned continental crust and have been contaminated by up to ~25% partial melt of the underlying Tamrau Formation
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgements
We thank the consortium of oil companies that funded this research as part of the Southeast Asia Research Group (ENI, Murphy Oil, Repsol, Shell, Engie, Statoil, and Inpex) at Royal Holloway University of London (RHUL) with additional support from the Faculty of Science, Medicine and Health at the University of Wollongong. Thanks go to Matthew Thirlwall for advice in collecting the isotopic data at RHUL and Jason Harvey (University of Leeds) for collecting the Nd isotopic data. Finally, we thank
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2022, TectonophysicsCitation Excerpt :These areas consist of altered basic to island arc volcanics and oceanic basalts of Paleogene age and exposed ultramafic rocks, and the island arc volcanics are overlain by middle-late Miocene sediments (Pieters et al., 1983; Dow and Sukamto, 1984). The plate boundary between the Australian Plate and New Guinea is located in the south and west of Cenderawasih Bay, which represents the boundary between continental and oceanic crust (Jost et al., 2018; Webb et al., 2020). Generally, the upper plate of New Guinea in the NW and Cenderawasih Bay belonged to the same oceanic crust before the late Miocene (Dow and Sukamto, 1984).