Srijita Ray , Gregory M. Yaxley , Laura A. Miller , Andrew J. Berry
{"title":"Monazite saturation in carbonatite melts at crustal and upper mantle conditions","authors":"Srijita Ray , Gregory M. Yaxley , Laura A. Miller , Andrew J. Berry","doi":"10.1016/j.gca.2025.01.039","DOIUrl":null,"url":null,"abstract":"<div><div>Monazite (XPO<sub>4</sub> where X = light rare earth element) is one of the most important ore minerals for rare earth elements (REE) mined from carbonatites. This study explores the influence of pressure, temperature and melt composition on the solubility of monazite in carbonate melt using piston cylinder experiments. We aim to understand how such a highly soluble phosphate mineral may sometimes crystallise from carbonatite magma and form economic deposits of REE. Our findings reveal that the solubility of monazite in a sodic-dolomitic carbonate melt is high over the entire pressure (1.0–2.0 GPa), temperature (1000-1450˚C), and compositional space (Na<sub>2</sub>O-CaO-MgO-SiO<sub>2</sub>-F) of our study. It increases from ∼ 26 to ∼ 61 wt% CePO<sub>4</sub> equivalent over the temperature range of 1000–1450 °C at 2 GPa. However, the solubility product constant (lnK<sub>sp</sub>) decreases by approximately ∼ 23 % and 21 % equivalent with increasing melt SiO<sub>2</sub> (from 0 to ∼ 18 wt% melt SiO<sub>2</sub>) at 1275 °C and fluoride (from 0 to ∼ 5 wt% melt F<sup>-</sup>) concentrations at 1100 °C respectively. Variations in melt Ca# (atomic Ca/(Mg + Ca) = 0.2–1.0) and pressure (1.0–2.0 GPa) have negligible impacts on monazite solubility. We use the experimental data to formulate an empirical model relating the solubility product constant (K<sub>sp</sub>) of monazite in carbonate melt to temperature and melt compositional parameters:</div><div><span><math><msub><mi>lnK</mi><mi>sp</mi></msub><mo>=</mo><mi>ln</mi><mfenced><mrow><mfenced><msub><mrow><msub><mrow><mi>R</mi><mi>E</mi><mi>E</mi></mrow><mn>2</mn></msub><msub><mi>O</mi><mn>3</mn></msub></mrow><mrow><mi>m</mi><mi>e</mi><mi>l</mi><mi>t</mi></mrow></msub></mfenced><mo>.</mo><mfenced><msub><mrow><msub><mi>P</mi><mn>2</mn></msub><msub><mi>O</mi><mn>5</mn></msub></mrow><mrow><mi>m</mi><mi>e</mi><mi>l</mi><mi>t</mi></mrow></msub></mfenced></mrow></mfenced><mo>=</mo><mn>1.31</mn><mfenced><mn>0.50</mn></mfenced><mo>-</mo><mfrac><mrow><mn>8679</mn><mfenced><mn>733</mn></mfenced></mrow><mi>T</mi></mfrac><mo>-</mo><mn>3.35</mn><mrow><mo>(</mo><mn>0.34</mn><mo>)</mo></mrow><mo>×</mo><mfenced><msub><mi>SiO</mi><mn>2</mn></msub></mfenced><mo>-</mo><mn>1.68</mn><mrow><mo>(</mo><mn>0.34</mn><mo>)</mo></mrow><mo>×</mo><mfenced><mi>F</mi></mfenced></math></span></div><div>where [] represents the mole fractions of oxides in the melt of the rare earth elements, phosphorus and silicon, and fluoride, T is in Kelvin, and the parentheses indicate standard errors. <span><math><msub><mrow><msub><mrow><mi>R</mi><mi>E</mi><mi>E</mi></mrow><mn>2</mn></msub><msub><mi>O</mi><mn>3</mn></msub></mrow><mrow><mi>m</mi><mi>e</mi><mi>l</mi><mi>t</mi></mrow></msub></math></span> represents the summation of the melt REE concentrations for those REE which are compatible in the experimentally synthesized monazite (La-Sm and Gd). These experimental results suggest that the formation of monazite requires relatively high concentrations of P<sub>2</sub>O<sub>5</sub> and Ce<sub>2</sub>O<sub>3</sub> under crustal pressure and temperature conditions, making it challenging to crystallise directly from carbonatite melts. However, monazite may instead form through reactions involving evolved carbonatite melts, potentially interacting with siliceous wall rocks or replacing pre-existing phosphates like apatite, as has been observed in natural carbonatites.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"393 ","pages":"Pages 1-17"},"PeriodicalIF":4.5000,"publicationDate":"2025-02-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochimica et Cosmochimica Acta","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0016703725000614","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Monazite (XPO4 where X = light rare earth element) is one of the most important ore minerals for rare earth elements (REE) mined from carbonatites. This study explores the influence of pressure, temperature and melt composition on the solubility of monazite in carbonate melt using piston cylinder experiments. We aim to understand how such a highly soluble phosphate mineral may sometimes crystallise from carbonatite magma and form economic deposits of REE. Our findings reveal that the solubility of monazite in a sodic-dolomitic carbonate melt is high over the entire pressure (1.0–2.0 GPa), temperature (1000-1450˚C), and compositional space (Na2O-CaO-MgO-SiO2-F) of our study. It increases from ∼ 26 to ∼ 61 wt% CePO4 equivalent over the temperature range of 1000–1450 °C at 2 GPa. However, the solubility product constant (lnKsp) decreases by approximately ∼ 23 % and 21 % equivalent with increasing melt SiO2 (from 0 to ∼ 18 wt% melt SiO2) at 1275 °C and fluoride (from 0 to ∼ 5 wt% melt F-) concentrations at 1100 °C respectively. Variations in melt Ca# (atomic Ca/(Mg + Ca) = 0.2–1.0) and pressure (1.0–2.0 GPa) have negligible impacts on monazite solubility. We use the experimental data to formulate an empirical model relating the solubility product constant (Ksp) of monazite in carbonate melt to temperature and melt compositional parameters:
where [] represents the mole fractions of oxides in the melt of the rare earth elements, phosphorus and silicon, and fluoride, T is in Kelvin, and the parentheses indicate standard errors. represents the summation of the melt REE concentrations for those REE which are compatible in the experimentally synthesized monazite (La-Sm and Gd). These experimental results suggest that the formation of monazite requires relatively high concentrations of P2O5 and Ce2O3 under crustal pressure and temperature conditions, making it challenging to crystallise directly from carbonatite melts. However, monazite may instead form through reactions involving evolved carbonatite melts, potentially interacting with siliceous wall rocks or replacing pre-existing phosphates like apatite, as has been observed in natural carbonatites.
期刊介绍:
Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes:
1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids
2). Igneous and metamorphic petrology
3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth
4). Organic geochemistry
5). Isotope geochemistry
6). Meteoritics and meteorite impacts
7). Lunar science; and
8). Planetary geochemistry.