Silicate and iron phosphate melt immiscibility promotes REE enrichment

被引:0
|
作者
Yan, S. C. [1 ,2 ,3 ]
Wan, B. [1 ]
Anenburg, M. [3 ]
Mavrogenes, J. A. [3 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, State Key Lab Lithospher & Environm Coevolut, Beijing 100029, Peoples R China
[2] Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing 100049, Peoples R China
[3] Australian Natl Univ, Res Sch Earth Sci, Canberra, 2600, Australia
基金
澳大利亚研究理事会;
关键词
OXIDE-APATITE DEPOSITS; KIRUNA-TYPE; ORE; GEOCHEMISTRY; BEARING;
D O I
10.7185/geochemlet.2436
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
A surging rare earth element (REE) demand calls for finding new REE resources. Iron oxide-apatite (IOA) deposits have substantial REE potential, but their REE enrichment mechanisms remain uncertain, hindering REE exploration. The dominant process of IOA deposit formation is also hotly debated. Here, we use novel layered piston-cylinder experiments to address these questions. Seventeen magmatic FeP-Si immiscibility experiments, across 800-1150 degrees C, and at 0.4 and 0.8 GPa, reproduced many natural textural (e.g., dendritic magnetite) and geochemical D-Ti=Fe(LFeP) -(LSi)< 1) features of IOA deposits. Magmatic-hydrothermal fluid bubbles and iron oxide-bubble pairs formed as well. The results strongly support FeP-Si immiscibility as a controlling factor in IOA deposits, although not mutually exclusive with other models. Light REE partition into FeP liquids, preferentially to heavy REE, explaining the light REE enrichment of IOA deposits. Some DLREEFeP-LSi REE values reach above 100, much higher than previously reported. Hence, any FeP rich rock that experienced magmatic Fe-Si immiscibility (e.g., IOA, nelsonites) is expected to be light REE enriched and should be considered as a REE exploration target.
引用
收藏
页码:14 / 20
页数:7
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