<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Jay M. Thompson</dc:contributor>
  <dc:contributor>Cameron Mark Mercer</dc:contributor>
  <dc:contributor>Ganesh Bhat</dc:contributor>
  <dc:contributor>Heather A. Lowers</dc:contributor>
  <dc:contributor>Adam Boehlke</dc:contributor>
  <dc:creator>Philip L. Verplanck</dc:creator>
  <dc:date>2025</dc:date>
  <dc:description>Carbonatite-hosted rare earth element (REE) deposits are the primary source of the world’s light REEs. The Mount Weld REE deposit in Western Australia is hosted in a lateritic sequence that reflects supergene enrichment of the underlying carbonatite. Water-rock interaction is a key to the formation of this world-class deposit. REE enrichment in the laterite is controlled by the breakdown of primary minerals, the release and transport of REEs, and the formation of secondary minerals. Secondary REE-bearing phosphate minerals are the primary REE-host phases in the laterite ore with monazite as the dominant phase; other REE-bearing phases include rhabdophane, cerianite, churchite, florencite, and crandallite subgroup minerals. Profiles through the laterite show that in the REE-rich zone, apatite and primary calcite and dolomite have broken down such that the loss of Ca and Mg, as well as Si and K, leads to a relative increase in the REEs. Sequestering of REEs in secondary mineral phases formed by groundwater further enhances the REE concentration.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:language>en</dc:language>
  <dc:publisher>UNICApress</dc:publisher>
  <dc:title>Formation of the Mount Weld rare earth element deposit, Western Australia: A carbonatite-derived laterite</dc:title>
  <dc:type>text</dc:type>
</oai_dc:dc>