Abstract

Abstract Most rare earth element deposits form from magmatic fluids, but there have also been discoveries of heavy rare earth element (HREE)–enriched hydrothermal xenotime deposits within sedimentary basins. As xenotime is notoriously insoluble, the question arises as to whether these lesser-known deposits form at typical basin temperatures or by influx of much hotter magmatic-hydrothermal fluids. The Browns Range District in northern Western Australia hosts deposits of xenotime that are enriched in HREEs and also uranium. The ore bodies consist of fault-controlled hydrothermal quartz-xenotime breccias that crosscut Archean basement rocks and overlying Paleoproterozoic sandstones. Analyses of fluid inclusions show that the xenotime precipitated at remarkably low temperatures, between 100 and 120 °C, in response to decompression boiling. The inclusions contain high excess concentrations of yttrium (10−3 mol/kg), REEs (1–7 × 10−5 mol/kg), and uranium (4 × 10−5 mol/kg) in equilibrium with xenotime at these low temperatures, showing that availability of phosphate limited the amount of xenotime precipitated. The analyses further identify SO42– and Cl– as the ligands that facilitated the elevated REE and uranium solubilities. These findings establish that significant REE transport and deposition is feasible at basin temperatures, and hence they raise the potential of unconformity settings for REE exploration. Moreover, the aqueous metal contents support a genetic link between this type of ore fluid and world-class Proterozoic unconformity-related uranium deposits elsewhere.

Highlights

  • The vast majority of rare earth element (REE) deposits are known to form at high temperatures in association with carbonatitic and peralkaline magmatism (e.g., Migdisov et al, 2016)

  • We address this question by analyzing fluid inclusions in the late Paleoproterozoic Wolverine heavy REE (HREE) deposit in the Browns Range of northern Western Australia

  • Petrography and Paragenesis Xenotime in our samples is present as fine-grained crystals disseminated within the host rock and as coarser-grained, euhedral pyramidal crystals grown into open space, either sitting directly on vein walls or as overgrowths completely mantling the faces of euhedral quartz crystals (Figs. 2B–2D; Fig. DR1 in Data Repository)

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Summary

Introduction

The vast majority of rare earth element (REE) deposits are known to form at high temperatures in association with carbonatitic and peralkaline magmatism (e.g., Migdisov et al, 2016). Lesser-known hydrothermal deposits of heavy REE (HREE)–enriched xenotime (YPO4) occur within sedimentary basins (e.g., Rabiei et al, 2017). Given the low aqueous solubility of xenotime, it has been unclear if REEs are transported in large quantities at basinal temperatures or if hightemperature magmatic-hydrothermal fluids are required to explain the deposits. We address this question by analyzing fluid inclusions in the late Paleoproterozoic Wolverine HREE deposit in the Browns Range of northern Western Australia. It shows how the ore-bearing fluids may be related to those that form world-class unconformity-related uranium deposits

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