{"title":"磷在碳酸盐熔体中的溶解度:通过其溶解度产物模拟磷灰石结晶","authors":"Gino Sartori , Max W. Schmidt","doi":"10.1016/j.gca.2023.04.034","DOIUrl":null,"url":null,"abstract":"<div><p>We model apatite-saturation in carbonatite melts based on a compilation of experimental data ranging from 650 to 1430 °C and 1 to 60 kbar. The data show a very strong correlation of inverse temperature with the apatite solubility product, a relation expressed by the equation.</p><p><span><math><mrow><mi>ln</mi><mo>(</mo><msup><mrow><mfenced><mrow><mi>C</mi><mi>a</mi><mi>O</mi></mrow></mfenced></mrow><mn>5</mn></msup><mo>·</mo><msup><mrow><mfenced><mrow><mi>P</mi><msub><mi>O</mi><mrow><mn>2.5</mn></mrow></msub></mrow></mfenced></mrow><mn>3</mn></msup><mo>)</mo><mo>=</mo><mo>-</mo><mn>27450</mn><mo>/</mo><mi>T</mi><mo>+</mo><mn>5.79</mn></mrow></math></span></p><p>(T in Kelvin). Within the available dataset, F and Cl do not play a discernable role. Application of the solubility product to natural Ca-carbonatites indicates that a few rocks with >8 wt% P<sub>2</sub>O<sub>5</sub> have cumulative apatite while most Ca-carbonatites (with typically <5 wt% P<sub>2</sub>O<sub>5</sub>) are apatite undersaturated at their liquidus temperatures, defined by calcite crystallization. To address true carbonatite liquids, we model calcite fractionation and melt evolution for natural rock compositions with 5, 10 and 20 mol% H<sub>2</sub>O and/or (Na,K)<sub>2</sub>CO<sub>3</sub> added, 5% representing the lower bound for any carbonatite formation model. Both H<sub>2</sub>O or (Na,K)<sub>2</sub>CO<sub>3</sub> cause very similar liquidus depressions of ∼10 °C/mol%. The model result is that saturation of apatite occurs in most natural carbonatite melts only after >45, 30–55, and 10–30 mol% calcite-fractionation for 5, 10, and 20 mol% fluxing components added, respectively. We further estimate the melt fractions necessary to dissolve all apatite in carbonatite melts generated from carbonated MORB and pelites, opening the discussion on an unlikely restitic nature of subducted apatites. In both the crystallization and forward melting cases, apatite crystallization or dissolution is mostly governed by temperature, surprisingly, carbonatite melt evolution through calcite-fractionation has a minor influence on the solubility product.</p></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"352 ","pages":"Pages 122-132"},"PeriodicalIF":4.5000,"publicationDate":"2023-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Phosphorous-solubility in carbonatite melts: Apatite crystallization modeled via its solubility product\",\"authors\":\"Gino Sartori , Max W. Schmidt\",\"doi\":\"10.1016/j.gca.2023.04.034\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We model apatite-saturation in carbonatite melts based on a compilation of experimental data ranging from 650 to 1430 °C and 1 to 60 kbar. The data show a very strong correlation of inverse temperature with the apatite solubility product, a relation expressed by the equation.</p><p><span><math><mrow><mi>ln</mi><mo>(</mo><msup><mrow><mfenced><mrow><mi>C</mi><mi>a</mi><mi>O</mi></mrow></mfenced></mrow><mn>5</mn></msup><mo>·</mo><msup><mrow><mfenced><mrow><mi>P</mi><msub><mi>O</mi><mrow><mn>2.5</mn></mrow></msub></mrow></mfenced></mrow><mn>3</mn></msup><mo>)</mo><mo>=</mo><mo>-</mo><mn>27450</mn><mo>/</mo><mi>T</mi><mo>+</mo><mn>5.79</mn></mrow></math></span></p><p>(T in Kelvin). Within the available dataset, F and Cl do not play a discernable role. Application of the solubility product to natural Ca-carbonatites indicates that a few rocks with >8 wt% P<sub>2</sub>O<sub>5</sub> have cumulative apatite while most Ca-carbonatites (with typically <5 wt% P<sub>2</sub>O<sub>5</sub>) are apatite undersaturated at their liquidus temperatures, defined by calcite crystallization. To address true carbonatite liquids, we model calcite fractionation and melt evolution for natural rock compositions with 5, 10 and 20 mol% H<sub>2</sub>O and/or (Na,K)<sub>2</sub>CO<sub>3</sub> added, 5% representing the lower bound for any carbonatite formation model. Both H<sub>2</sub>O or (Na,K)<sub>2</sub>CO<sub>3</sub> cause very similar liquidus depressions of ∼10 °C/mol%. The model result is that saturation of apatite occurs in most natural carbonatite melts only after >45, 30–55, and 10–30 mol% calcite-fractionation for 5, 10, and 20 mol% fluxing components added, respectively. We further estimate the melt fractions necessary to dissolve all apatite in carbonatite melts generated from carbonated MORB and pelites, opening the discussion on an unlikely restitic nature of subducted apatites. In both the crystallization and forward melting cases, apatite crystallization or dissolution is mostly governed by temperature, surprisingly, carbonatite melt evolution through calcite-fractionation has a minor influence on the solubility product.</p></div>\",\"PeriodicalId\":327,\"journal\":{\"name\":\"Geochimica et Cosmochimica Acta\",\"volume\":\"352 \",\"pages\":\"Pages 122-132\"},\"PeriodicalIF\":4.5000,\"publicationDate\":\"2023-07-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geochimica et Cosmochimica Acta\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0016703723002193\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochimica et Cosmochimica Acta","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0016703723002193","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}
Phosphorous-solubility in carbonatite melts: Apatite crystallization modeled via its solubility product
We model apatite-saturation in carbonatite melts based on a compilation of experimental data ranging from 650 to 1430 °C and 1 to 60 kbar. The data show a very strong correlation of inverse temperature with the apatite solubility product, a relation expressed by the equation.
(T in Kelvin). Within the available dataset, F and Cl do not play a discernable role. Application of the solubility product to natural Ca-carbonatites indicates that a few rocks with >8 wt% P2O5 have cumulative apatite while most Ca-carbonatites (with typically <5 wt% P2O5) are apatite undersaturated at their liquidus temperatures, defined by calcite crystallization. To address true carbonatite liquids, we model calcite fractionation and melt evolution for natural rock compositions with 5, 10 and 20 mol% H2O and/or (Na,K)2CO3 added, 5% representing the lower bound for any carbonatite formation model. Both H2O or (Na,K)2CO3 cause very similar liquidus depressions of ∼10 °C/mol%. The model result is that saturation of apatite occurs in most natural carbonatite melts only after >45, 30–55, and 10–30 mol% calcite-fractionation for 5, 10, and 20 mol% fluxing components added, respectively. We further estimate the melt fractions necessary to dissolve all apatite in carbonatite melts generated from carbonated MORB and pelites, opening the discussion on an unlikely restitic nature of subducted apatites. In both the crystallization and forward melting cases, apatite crystallization or dissolution is mostly governed by temperature, surprisingly, carbonatite melt evolution through calcite-fractionation has a minor influence on the solubility product.
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.