Giuseppe D. Saldi , Thierry Decrausaz , Vasileios Mavromatis , Pascale Bénézeth
{"title":"阿曼橄榄岩的碳酸化过程:温度依赖性反应和反应流体的Mg同位素组成","authors":"Giuseppe D. Saldi , Thierry Decrausaz , Vasileios Mavromatis , Pascale Bénézeth","doi":"10.1016/j.gca.2025.01.029","DOIUrl":null,"url":null,"abstract":"<div><div>The study of natural analogues of CO<sub>2</sub> mineral sequestration combined with the experimental quantification of carbonation reactions constitutes a fundamental approach to understand the spatial and structural distribution of carbonated bodies and the time scales by which large amounts of CO<sub>2</sub><span> can be stored in solid form into geologic formations. To better quantify the carbonation rates of ultramafic rocks and study the evolution of dissolved Mg isotope composition during their interaction with CO</span><sub>2</sub><span><span>-rich fluids, a series of batch carbonation experiments using a partially serpentinized harzburgite from the Semail </span>ophiolite (Oman) was conducted at 90–180 °C and at constant CO</span><sub>2</sub> partial pressures (∼ 15–20 bar). The yield of the carbonation reaction increased from ∼ 0 at 90 °C to a maximum of 31 mol % at 150 °C, decreasing to 12 mol % at 180 °C over a period of one month. Magnesites containing 3–9 wt% of Fe and silica polymorphs (SiO<sub>2(am)</sub> and chalcedony) were the main reaction products, with a fraction of secondary Mg-silicates that increased with increasing temperature, significantly reducing the carbonation extent at 180 °C. The aqueous fluid became progressively enriched in heavy isotopes with the progress of the carbonation reaction. The apparent Mg isotope fractionations between the rock and bulk fluid (Δ<sup>26</sup>Mg = δ<sup>26</sup>Mg<sub>solid</sub> − δ<sup>26</sup>Mg<sub>fluid</sub>) varied from −1.6 ‰ at 120 °C to −0.9 ‰ at 180 °C, consistent with the preferential uptake of <sup>24</sup><span>Mg by carbonate minerals and the decrease of isotope fractionation with increasing temperature. The average magnesite isotope compositions (−1.6 ‰ ≤ δ</span><sup>26</sup>Mg ≤ -0.3 ‰) derived from mass-balance calculations were found to be within the range of δ<sup>26</sup>Mg values reported for Oman listvenites, suggesting that the carbonation processes in this geological unit took place within the temperature range considered in this study (∼120–180 °C).</div><div>Comparison of experimental results with observations of a well-studied natural analogue provides new indications on the optimum conditions for the development of CO<sub>2</sub><span> sequestration methods in peridotites, or </span><em>ex situ</em><span> carbonation techniques using ultramafic minerals. The observed evolution of the Mg isotopic composition of the fluid also suggests that the use of Mg-isotopes could be an effective tool to monitor the spatial and temporal progress of carbonation reactions during field-scale CO</span><sub>2</sub> storage operations in ultramafic rocks.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"406 ","pages":"Pages 101-118"},"PeriodicalIF":5.0000,"publicationDate":"2025-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Carbonation processes in Oman peridotite: temperature-dependent reactions and Mg isotope composition of reacting fluids\",\"authors\":\"Giuseppe D. Saldi , Thierry Decrausaz , Vasileios Mavromatis , Pascale Bénézeth\",\"doi\":\"10.1016/j.gca.2025.01.029\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The study of natural analogues of CO<sub>2</sub> mineral sequestration combined with the experimental quantification of carbonation reactions constitutes a fundamental approach to understand the spatial and structural distribution of carbonated bodies and the time scales by which large amounts of CO<sub>2</sub><span> can be stored in solid form into geologic formations. To better quantify the carbonation rates of ultramafic rocks and study the evolution of dissolved Mg isotope composition during their interaction with CO</span><sub>2</sub><span><span>-rich fluids, a series of batch carbonation experiments using a partially serpentinized harzburgite from the Semail </span>ophiolite (Oman) was conducted at 90–180 °C and at constant CO</span><sub>2</sub> partial pressures (∼ 15–20 bar). The yield of the carbonation reaction increased from ∼ 0 at 90 °C to a maximum of 31 mol % at 150 °C, decreasing to 12 mol % at 180 °C over a period of one month. Magnesites containing 3–9 wt% of Fe and silica polymorphs (SiO<sub>2(am)</sub> and chalcedony) were the main reaction products, with a fraction of secondary Mg-silicates that increased with increasing temperature, significantly reducing the carbonation extent at 180 °C. The aqueous fluid became progressively enriched in heavy isotopes with the progress of the carbonation reaction. The apparent Mg isotope fractionations between the rock and bulk fluid (Δ<sup>26</sup>Mg = δ<sup>26</sup>Mg<sub>solid</sub> − δ<sup>26</sup>Mg<sub>fluid</sub>) varied from −1.6 ‰ at 120 °C to −0.9 ‰ at 180 °C, consistent with the preferential uptake of <sup>24</sup><span>Mg by carbonate minerals and the decrease of isotope fractionation with increasing temperature. The average magnesite isotope compositions (−1.6 ‰ ≤ δ</span><sup>26</sup>Mg ≤ -0.3 ‰) derived from mass-balance calculations were found to be within the range of δ<sup>26</sup>Mg values reported for Oman listvenites, suggesting that the carbonation processes in this geological unit took place within the temperature range considered in this study (∼120–180 °C).</div><div>Comparison of experimental results with observations of a well-studied natural analogue provides new indications on the optimum conditions for the development of CO<sub>2</sub><span> sequestration methods in peridotites, or </span><em>ex situ</em><span> carbonation techniques using ultramafic minerals. The observed evolution of the Mg isotopic composition of the fluid also suggests that the use of Mg-isotopes could be an effective tool to monitor the spatial and temporal progress of carbonation reactions during field-scale CO</span><sub>2</sub> storage operations in ultramafic rocks.</div></div>\",\"PeriodicalId\":327,\"journal\":{\"name\":\"Geochimica et Cosmochimica Acta\",\"volume\":\"406 \",\"pages\":\"Pages 101-118\"},\"PeriodicalIF\":5.0000,\"publicationDate\":\"2025-10-01\",\"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/S0016703725000407\",\"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/S0016703725000407","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}
Carbonation processes in Oman peridotite: temperature-dependent reactions and Mg isotope composition of reacting fluids
The study of natural analogues of CO2 mineral sequestration combined with the experimental quantification of carbonation reactions constitutes a fundamental approach to understand the spatial and structural distribution of carbonated bodies and the time scales by which large amounts of CO2 can be stored in solid form into geologic formations. To better quantify the carbonation rates of ultramafic rocks and study the evolution of dissolved Mg isotope composition during their interaction with CO2-rich fluids, a series of batch carbonation experiments using a partially serpentinized harzburgite from the Semail ophiolite (Oman) was conducted at 90–180 °C and at constant CO2 partial pressures (∼ 15–20 bar). The yield of the carbonation reaction increased from ∼ 0 at 90 °C to a maximum of 31 mol % at 150 °C, decreasing to 12 mol % at 180 °C over a period of one month. Magnesites containing 3–9 wt% of Fe and silica polymorphs (SiO2(am) and chalcedony) were the main reaction products, with a fraction of secondary Mg-silicates that increased with increasing temperature, significantly reducing the carbonation extent at 180 °C. The aqueous fluid became progressively enriched in heavy isotopes with the progress of the carbonation reaction. The apparent Mg isotope fractionations between the rock and bulk fluid (Δ26Mg = δ26Mgsolid − δ26Mgfluid) varied from −1.6 ‰ at 120 °C to −0.9 ‰ at 180 °C, consistent with the preferential uptake of 24Mg by carbonate minerals and the decrease of isotope fractionation with increasing temperature. The average magnesite isotope compositions (−1.6 ‰ ≤ δ26Mg ≤ -0.3 ‰) derived from mass-balance calculations were found to be within the range of δ26Mg values reported for Oman listvenites, suggesting that the carbonation processes in this geological unit took place within the temperature range considered in this study (∼120–180 °C).
Comparison of experimental results with observations of a well-studied natural analogue provides new indications on the optimum conditions for the development of CO2 sequestration methods in peridotites, or ex situ carbonation techniques using ultramafic minerals. The observed evolution of the Mg isotopic composition of the fluid also suggests that the use of Mg-isotopes could be an effective tool to monitor the spatial and temporal progress of carbonation reactions during field-scale CO2 storage operations in ultramafic rocks.
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.