Abstract
The Mad Gap Yards ultramafic lamprophyre (UML) dykes in the East Kimberley region of northern Western Australia form part of a widespread Neoproterozoic (~ 842–800 Ma) alkaline mafic–ultramafic magmatic province in the north, east and central regions of the Kimberley Craton of Western Australia. The NE-trending Mad Gap Yards dykes lie at the southeastern margin of the Kimberley Basin adjacent to the Greenvale Fault and intrude the Paleoproterozoic Elgee Siltstone. The dykes are classified as alnöite, and contain abundant macrocrystic olivine in a groundmass of phlogopite, perovskite, spinels, diopside, apatite, andradite–hydroandradite, serpentine, calcite, pseudomorphs after melilite and rare gittinsite. Mantle-derived olivine macrocrysts have compositions in the range Mg#91–92, similar to moderately refractory peridotite from other parts of the Kimberley Craton, whereas magmatic olivine phenocrysts have Mg#88–90. Olivine and chromian spinel were the earliest phenocrysts; they record equilibration temperatures of ~ 1030–920℃ under moderately reducing conditions with fO2 values below the fayalite-magnetite-quartz (FMQ) oxygen buffer (Δ FMQ = mostly − 0.8 to − 1.7 log units). Magnetite rims and groundmass grains crystallised at ~ 850–740℃ under more oxidising conditions with Δ FMQ ~ + 0.6 to − 0.75 log units. Perovskite is well preserved in parts of the dykes and indicates crystallisation inside this fO2 range. The perovskite yielded a SHRIMP 206Pb/238U age of 842 ± 8 Ma. The Mad Gap Yards dykes carry rare partially altered spinel-peridotite xenoliths containing olivine (Mg#86.3–90), Cr-diopside, enstatite and Al-Cr spinel, and well as mantle xenocrysts of Cr-Al spinel and Cr-diopside. Bulk rock trace-element geochemistry, Cr-diopside thermobarometry and Sr–Nd-isotopic compositions of perovskite suggest that the UML magma was derived from partial melting of a garnet-bearing asthenospheric mantle source at ~ 200 km depth. Nd depleted-mantle model ages (TDM) for perovskite range from 1106–865 Ma and broadly correlate with regional mantle metasomatism during the Yampi Orogeny (~ 1000–800 Ma). Rare evidence of mantle metasomatism by LILE and HFSE-enriched melts has been found in the form of priderite and loveringite replacing Mg-rich ilmenite in an olivine macrocryst. The timing of emplacement of the Mad Gap Yards UML dykes at ~ 842 Ma correlates with the early stages of the breakup of Rodinia.
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Availability of data and materials
All data generated in this study are presented in the text of the article and the supplementary data appendices. The drill core described here is held at the Geological Survey of Western Australia Perth Core Library in Carlisle, Perth, and is available for viewing and sampling upon request.
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Acknowledgements
Drillcore from the Mad Gap Yards prospect initially was supplied to the Western Australian Museum by John Towie and Diamin Resources. U-Th-Pb analyses were conducted using a SHRIMP II ion microprobe at the Large Geometry Ionprobe Facility of the John de Laeter Center, Curtin University Perth, Australia. Research in the JdLC GeoHistory Facility is enabled by AuScope (auscope.org.au) and the Australian Government via the National Collaborative Research Infrastructure Strategy (NCRIS). Brendan Griffin assisted with early parts of this work. Janet Dunphy and Neal McNaughton were of great assistance with SHRIMP operation and analysis. Robert Rapp (formerly ANU) is thanked for assistance with the EPMA analyses. ALJ acknowledges the support from ARC Discovery Project DP 140103841. This study used instrumentation funded by the Australian Government, Department of Education, Science and Training (DEST) Systemic Infrastructure Grants, ARC Linkage Infrastructure, Equipment and Facilities (LIEF), NCRIS/AuScope, Macquarie University and industry partners. This is contribution 1758 from the ARC Centre of Excellence for Core to Crust Fluid Systems (http://www.ccfs.mq.edu.au) and 1527 in the GEMOC Key Centre (http://www.gemoc.mq.edu.au). Reviews by Dante Canil, Hugh O’Brien and an anonymous reviewer helped to improve an earlier version of this manuscript.
Funding
No specific funding was received for conducting this study. However, ALJ acknowledges the support from ARC Discovery Project DP 140103841. This study used instrumentation funded by the Australian Government, Department of Education, Science and Training (DEST) Systemic Infrastructure Grants, ARC Linkage Infrastructure, Equipment and Facilities (LIEF), NCRIS/AuScope, Macquarie University and industry partners. This study also used instrumentation in the JdLC GeoHistory Facility that is enabled by AuScope (auscope.org.au) and the Australian Government via the National Collaborative Research Infrastructure Strategy (NCRIS).
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PJD undertook logging and sampling of the drill core, petrography, EDS mineral analysis and wrote the main manuscript text. ALJ performed WDS mineral analysis, thermobarometry and oxygen fugacity calculations, drafted sections of the text related to these areas, and contributed to the revision and editing of the paper. CT undertook the SHRIMP U-Th-Pb perovskite geochronology and wrote the associated text. WLG processed perovskite Nd–Sr isotopic data and advised on its interpretation. SEMG performed the LA-MC-ICPMS Nd–Sr isotopic analysis of perovskite. NJE performed the LA-ICPMS trace-element analysis of perovskite and processed the analytical data. WRT provided HMC mineral analysis data, analysed this data and wrote part of the manuscript describing the spinel chemistry. MV assisted with the processing of EDS mineral analysis data. All authors read and approved the final manuscript.
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Downes, P.J., Jaques, A.L., Talavera, C. et al. Perovskite geochronology and petrogenesis of the Neoproterozoic Mad Gap Yards ultramafic lamprophyre dykes, East Kimberley region, Western Australia. Contrib Mineral Petrol 178, 21 (2023). https://doi.org/10.1007/s00410-023-02002-2
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DOI: https://doi.org/10.1007/s00410-023-02002-2