Pub Date : 2023-10-21DOI: 10.1016/j.chemer.2023.126038
Dino Leopardi , Axel Gerdes , Richard Albert , Jens Gutzmer , Bernd Lehmann , Mathias Burisch
The Sadisdorf Sn-Li-(W-Cu) prospect in the eastern Erzgebirge (Germany) comprises two distinct styles of magmatic-hydrothermal mineralization, namely greisen-type mineralization at the Kupfergrube site, and stockwork-type mineralization at both the Kupfergrube and the Zinnklüfte sites. Previously, these two sites were regarded as expressions of two temporally distinct mineralization events. In this study, this temporal relation was tested by LA-ICP-MS U-Pb data obtained for 16 cassiterite samples, including samples from both sites and styles of mineralization. All 16 samples define a narrow range of ages between 315.1 ± 1.7 / 3.3 Ma and 311.0 ± 3.1 / 4.0 Ma. All ages overlap within uncertainty, suggesting that mineralization across the Sadisdorf prospect is likely related to the same magmatic-hydrothermal event.
On the regional scale, the cassiterite ages suggest that Sn-Li mineralization is associated with late-stage felsic magmatism directly following the collapse (∼314–313 Ma) of the Altenberg-Teplice Caldera. The cassiterite ages also overlap with garnet U-Pb LA-ICP-MS ages of Sn-rich skarn occurrences in the western Erzgebirge (e.g., Breitenbrunn, Antonsthal and Hämmerlein). This observation provides direct evidence that greisen and skarn-hosted Sn mineralization are related to the same period of magmatism. The data indicate that the majority of Sn-mineralization in the Erzgebirge formed after 318 Ma (likely between 318 and 310 Ma), challenging previous models which invoked an older suite of granites (326–318 Ma) as causative source intrusions.
{"title":"LA-ICP-MS U-Pb cassiterite age data of the Sadisdorf deposit link Sn-Li-(W-Cu) mineralization in the eastern Erzgebirge to the collapse of the Altenberg-Teplice Caldera","authors":"Dino Leopardi , Axel Gerdes , Richard Albert , Jens Gutzmer , Bernd Lehmann , Mathias Burisch","doi":"10.1016/j.chemer.2023.126038","DOIUrl":"10.1016/j.chemer.2023.126038","url":null,"abstract":"<div><p>The Sadisdorf Sn-Li-(W-Cu) prospect in the eastern Erzgebirge (Germany) comprises two distinct styles of magmatic-hydrothermal mineralization, namely greisen-type mineralization at the Kupfergrube site, and stockwork-type mineralization at both the Kupfergrube and the Zinnklüfte sites. Previously, these two sites were regarded as expressions of two temporally distinct mineralization events. In this study, this temporal relation was tested by LA-ICP-MS U-Pb data obtained for 16 cassiterite samples, including samples from both sites and styles of mineralization. All 16 samples define a narrow range of ages between 315.1 ± 1.7 / 3.3 Ma and 311.0 ± 3.1 / 4.0 Ma. All ages overlap within uncertainty, suggesting that mineralization across the Sadisdorf prospect is likely related to the same magmatic-hydrothermal event.</p><p>On the regional scale, the cassiterite ages suggest that Sn-Li mineralization is associated with late-stage felsic magmatism directly following the collapse (∼314–313 Ma) of the Altenberg-Teplice Caldera. The cassiterite ages also overlap with garnet U-Pb LA-ICP-MS ages of Sn-rich skarn occurrences in the western Erzgebirge (e.g., Breitenbrunn, Antonsthal and Hämmerlein). This observation provides direct evidence that greisen and skarn-hosted Sn mineralization are related to the same period of magmatism. The data indicate that the majority of Sn-mineralization in the Erzgebirge formed after 318 Ma (likely between 318 and 310 Ma), challenging previous models which invoked an older suite of granites (326–318 Ma) as causative source intrusions.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"84 1","pages":"Article 126038"},"PeriodicalIF":0.0,"publicationDate":"2023-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0009281923000892/pdfft?md5=34b93b3603eae9a8a691455a249a5f33&pid=1-s2.0-S0009281923000892-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"136009258","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
The Inlice high sulfidation epithermal gold deposit with 262,300 oz of gold ore is located in the Erenlerdağ-Alacadağ Volcanic Complex (EAVC) at the northern part of central Taurides. The volcanic succession of the study area is stratigraphically represented by andesite, block and ash flow, basaltic andesite lava flow and andesite lava flow. The deposit consists of seven neighboring mineralized veins termed Ana East, Ana West, West, Discovery, Güllü, Merkez and North Zone and is associated with an andesite (ca 8–9 Ma). Hydrothermal alteration from the innermost to the outermost parts of the deposit includes silicification, advanced argillic, intermediate argillic and propylitic. At the surface, quartz veins related to silicification are exposed as linear topographic relief trending mainly northwest-southeast and secondarily northeast-southwest and east-west. Deep drill core samples, including magnetite, quartz, biotite and anhydrite, imply the presence of potassic alteration in depth (50 to 970 m) possibly related to a porphyry Cu system. Ore assemblages are described as hypogene and supergene. The hypogene ore mainly includes pyrite (Py-I and Py-II) and enargite, and to a lesser extent chalcopyrite, sphalerite and marcasite. The supergene ore incorporates hematite and goethite, and minor covellite, chalcocite, malachite and native copper. Hypogene gold precipitation is associated with the mineral association of Py-II, chalcopyrite and enargite, while enargite mineral is a major host for gold (up to 600 ppm). Supergene oxidation resulted in the development of a secondary enrichment zone for gold (up to 14 g/t) extending to a depth of about 45 m.
Microthermometric measurements show that the silicification associated with the mineralization was formed at homogenization temperatures ranging between 147 and 360 °C and salinities up to 6.5 wt% NaCl. This suggests that the fluid mixing and/or fluid dilution processes were important factors controlling the precipitation of gold. δ34S isotope compositions are between −0.9 and − 9 ‰, and further indicate a significant involvement of magmatic components into the hydrothermal fluids. Thus, it is concluded that at Inlice the hydrothermal fluids responsible for the alteration and mineralization processes were derived by relatively dilute fluids formed by the mixing of magmatic fluids with meteoric waters.
{"title":"Mineralogy, fluid inclusion and stable isotope characteristics of the Inlice (Konya, Turkey) high sulfidation epithermal gold deposit: Implications for hydrothermal evolution and ore genesis","authors":"Mustafa Haydar Terzi , Erkan Yılmazer , İlkay Kuşcu , Tolga Oyman , Sercan Bozan","doi":"10.1016/j.chemer.2023.126040","DOIUrl":"10.1016/j.chemer.2023.126040","url":null,"abstract":"<div><p>The Inlice high sulfidation epithermal gold deposit with 262,300 oz of gold ore is located in the Erenlerdağ-Alacadağ Volcanic Complex (EAVC) at the northern part of central Taurides. The volcanic succession of the study area is stratigraphically represented by andesite, block and ash flow, basaltic andesite lava flow and andesite lava flow. The deposit consists of seven neighboring mineralized veins termed Ana East, Ana West, West, Discovery, Güllü, Merkez and North Zone and is associated with an andesite (<em>ca</em> 8–9 Ma). Hydrothermal alteration from the innermost to the outermost parts of the deposit includes silicification, advanced argillic, intermediate argillic and propylitic. At the surface, quartz veins related to silicification are exposed as linear topographic relief trending mainly northwest-southeast and secondarily northeast-southwest and east-west. Deep drill core samples, including magnetite, quartz, biotite and anhydrite, imply the presence of potassic alteration in depth (50 to 970 m) possibly related to a porphyry Cu system. Ore assemblages are described as hypogene and supergene. The hypogene ore mainly includes pyrite (Py-I and Py-II) and enargite, and to a lesser extent chalcopyrite, sphalerite and marcasite. The supergene ore incorporates hematite and goethite, and minor covellite, chalcocite, malachite and native copper. Hypogene gold precipitation is associated with the mineral association of Py-II, chalcopyrite and enargite, while enargite mineral is a major host for gold (up to 600 ppm). Supergene oxidation resulted in the development of a secondary enrichment zone for gold (up to 14 g/t) extending to a depth of about 45 m.</p><p>Microthermometric measurements show that the silicification associated with the mineralization was formed at homogenization temperatures ranging between 147 and 360 °C and salinities up to 6.5 wt% NaCl. This suggests that the fluid mixing and/or fluid dilution processes were important factors controlling the precipitation of gold. δ<sup>34</sup>S isotope compositions are between −0.9 and − 9 ‰, and further indicate a significant involvement of magmatic components into the hydrothermal fluids. Thus, it is concluded that at Inlice the hydrothermal fluids responsible for the alteration and mineralization processes were derived by relatively dilute fluids formed by the mixing of magmatic fluids with meteoric waters.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"84 1","pages":"Article 126040"},"PeriodicalIF":0.0,"publicationDate":"2023-10-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0009281923000910/pdfft?md5=a47886f3b78fd7efcf5dc1f2f11968a6&pid=1-s2.0-S0009281923000910-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135852349","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-10-06DOI: 10.1016/j.chemer.2023.126037
Giancarlo Della Ventura , Federico Galdenzi , Augusto Marcelli , Giannantonio Cibin , Roberta Oberti , Frank C. Hawthorne , Simone Bernardini , Boriana Mihailova
In this paper, we address two key features of the behaviour of Fe-rich amphibole at high temperatures: (1) the Fe2+ → Fe3+ + e− exchange within the crystal bulk, and (2) the consequent rise in electrical conductivity. Cycling heating-cooling experiments were done in situ up to 542 °C (815 K) at beamline B11 of the Diamond Synchrotron Laboratory (UK). X-ray absorption spectra at the Fe K-edge and electrical resistivity were measured simultaneously on a single crystal of riebeckite with a composition very close to the ideal formula A□BNa2C(Fe2+3Fe3+2)TSi8O22W(OH)2. The Fe3+/Fetot ratio was monitored via analysis of the pre-edge feature in the XANES spectra. Our data show slight oscillations of the oxidation state of Fe with temperature cycling up to around 400 °C (673 K), followed by a substantial gradual increase in Fe2+ → Fe3+ oxidation that starts at ~450 °C (~723 K) and is completed at ~525 °C (~798 K). The conductivity (σ) measured along the crystallographic c-axis oscillates strongly with cycling temperature allowing us to conclude that it is intrinsically related to the electron hopping induced by thermal treatment. The activation-energy derived from the σ(T) trend is Ea = 74.4 ± 0.6 kJ/mol (0.77 ± 0.01 eV), in agreement with small-polaron conduction. This study provides direct and robust support of the conduction mechanisms in Fe-amphibole previously inferred from indirect methods. Given that riebeckite is a significant component in the glaucophanitic amphiboles common in blueschists associated with subducted oceanic crust, our data provide a link between atomic-scale processes and Earth-scale anomalous conductivity observed via geophysical measurements.
在本文中,我们讨论了富铁闪石在高温下行为的两个关键特征:(1) 晶体体内部的 Fe2+ → Fe3+ + e- 交换,以及 (2) 随之而来的电导率上升。循环加热-冷却实验是在英国钻石同步加速器实验室(Diamond Synchrotron Laboratory)的 B11 光束线现场进行的,温度最高达 542 ℃(815 K)。同时测量了铁 K 边的 X 射线吸收光谱和里斑岩单晶体的电阻率,其成分非常接近理想公式 A□BNa2C(Fe2+3Fe3+2)TSi8O22W(OH)2。通过分析 XANES 光谱中的前沿特征,对 Fe3+/Fetot 比率进行了监测。我们的数据显示,铁的氧化态随着温度循环在 400 °C (673 K) 左右出现轻微振荡,随后 Fe2+ → Fe3+ 氧化态逐渐大幅增加,从 ~450 °C (~723 K) 开始,到 ~525 °C (~798 K) 结束。沿晶体学 c 轴测量到的电导率(σ)随循环温度的变化而强烈摆动,因此我们得出结论,电导率与热处理引起的电子跳跃有内在联系。从 σ(T) 趋势得出的活化能为 Ea = 74.4 ± 0.6 kJ/mol (0.77 ± 0.01 eV),与小极子传导一致。这项研究为之前通过间接方法推断的铁闪石传导机制提供了直接而有力的支持。鉴于菱锰矿是与俯冲大洋地壳相关的蓝晶岩中常见的釉闪闪石闪石的重要组成部分,我们的数据提供了原子尺度过程与地球物理测量观测到的地球尺度异常传导性之间的联系。
{"title":"In situ simultaneous Fe K-edge XAS spectroscopy and resistivity measurements of riebeckite: Implications for anomalous electrical conductivity in subduction zones","authors":"Giancarlo Della Ventura , Federico Galdenzi , Augusto Marcelli , Giannantonio Cibin , Roberta Oberti , Frank C. Hawthorne , Simone Bernardini , Boriana Mihailova","doi":"10.1016/j.chemer.2023.126037","DOIUrl":"10.1016/j.chemer.2023.126037","url":null,"abstract":"<div><p>In this paper, we address two key features of the behaviour of Fe-rich amphibole at high temperatures: (1) the Fe<sup>2+</sup> → Fe<sup>3+</sup> + <em>e</em><sup>−</sup> exchange within the crystal bulk, and (2) the consequent rise in electrical conductivity. Cycling heating-cooling experiments were done <em>in situ</em> up to 542 °C (815 K) at beamline B11 of the Diamond Synchrotron Laboratory (UK). X-ray absorption spectra at the Fe K-edge and electrical resistivity were measured simultaneously on a single crystal of riebeckite with a composition very close to the ideal formula <sup>A</sup>□<sup>B</sup>Na<sub>2</sub><sup>C</sup>(Fe<sup>2+</sup><sub>3</sub>Fe<sup>3+</sup><sub>2</sub>)<sup>T</sup>Si<sub>8</sub>O<sub>22</sub><sup>W</sup>(OH)<sub>2</sub>. The Fe<sup>3+</sup>/Fe<sub>tot</sub> ratio was monitored <em>via</em> analysis of the pre-edge feature in the XANES spectra. Our data show slight oscillations of the oxidation state of Fe with temperature cycling up to around 400 °C (673 K), followed by a substantial gradual increase in Fe<sup>2+</sup> → Fe<sup>3+</sup> oxidation that starts at ~450 °C (~723 K) and is completed at ~525 °C (~798 K). The conductivity (σ) measured along the crystallographic c-axis oscillates strongly with cycling temperature allowing us to conclude that it is intrinsically related to the electron hopping induced by thermal treatment. The activation-energy derived from the σ(T) trend is <em>E</em><sub><em>a</em></sub> = 74.4 ± 0.6 kJ/mol (0.77 ± 0.01 eV), in agreement with small-polaron conduction. This study provides direct and robust support of the conduction mechanisms in Fe-amphibole previously inferred from indirect methods. Given that riebeckite is a significant component in the glaucophanitic amphiboles common in blueschists associated with subducted oceanic crust, our data provide a link between atomic-scale processes and Earth-scale anomalous conductivity observed <em>via</em> geophysical measurements.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"84 1","pages":"Article 126037"},"PeriodicalIF":0.0,"publicationDate":"2023-10-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0009281923000880/pdfft?md5=84f74da75e215f9ac495d6f660a089e8&pid=1-s2.0-S0009281923000880-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135567398","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-10-05DOI: 10.1016/j.chemer.2023.126036
Mehrdad Daviran, Reza Ghezelbash, Abbas Maghsoudi
Identifying the geochemical signatures of valuable mineral deposits using regional geochemical data from stream sediments is a challenging task due to the intricate characteristics of geological formations. Our team is currently investigating the potential of unsupervised clustering analysis (CA) and hybridization with the grey wolf optimizer (GWO) in developing multi-element geochemical models using stream sediment data. To cluster the geochemical data and uncover any unusual patterns, we opted to use the K-means (KM) algorithm due to its straightforward implementation, fast computation speed, and capacity to handle the large datasets. Despite its benefits, the KM method also has notable limitations, such as the random selection of cluster centroids. This can result in higher systematic uncertainty in unsupervised geochemical modeling and longer computation times. To mitigate this concern, we have introduced a new hybrid approach, grey wolf optimizer with K-means so-called the GWOKM algorithm to enhance the delineation of multi-elemental patterns in stream sediment geochemical data. This method incorporates the grey wolf optimization algorithm with KM to optimize the identification of both anomalies and backgrounds using factor analysis and sample catchment basin modeling techniques. This approach was utilized to detect anomalous multi-elemental geochemical patterns indicative of porphyry and skarn copper deposits in the Baft area, Kerman belt, Iran. Upon comparison of the geochemical models derived from KM and GWOKM clustering methods, the latter outperformed the former, as evidenced by its higher prediction rate. The outcomes affirm the efficacy of unsupervised KM clustering analysis (CA) as a means of breaking down geochemical anomaly-background populations. Moreover, the integration of clustering methods with optimization algorithms has proven to be successful for enhancing the credibility of mineralized areas, which could be advantageous in future exploration phases. Based on the results, the GWOKM approach generates more reliable and efficient geochemical anomaly targets.
由于地质构造的复杂性,利用溪流沉积物的区域地球化学数据识别有价值矿藏的地球化学特征是一项具有挑战性的任务。我们的团队目前正在研究无监督聚类分析(CA)以及与灰狼优化器(GWO)混合使用的潜力,以便利用溪流沉积物数据开发多元素地球化学模型。为了对地球化学数据进行聚类并发现任何不寻常的模式,我们选择使用 K-均值(KM)算法,因为该算法实施简单、计算速度快,而且能够处理大型数据集。尽管 KM 算法有很多优点,但它也有明显的局限性,比如聚类中心点的随机选择。这可能导致无监督地球化学建模的系统不确定性更高,计算时间更长。为了缓解这一问题,我们引入了一种新的混合方法,即所谓的 GWOKM 算法(Grey Wolf optimizer with K-means),以加强溪流沉积物地球化学数据中多元素模式的划分。该方法将灰狼优化算法与 KM 结合在一起,利用因子分析和样本集水盆地建模技术优化异常和背景的识别。伊朗克尔曼带 Baft 地区的斑岩和矽卡岩铜矿床异常多元素地球化学模式就是利用这种方法进行探测的。在对 KM 和 GWOKM 聚类方法得出的地球化学模型进行比较后发现,后者的预测率高于前者。这些结果肯定了无监督 KM 聚类分析(CA)作为分解地球化学异常-背景群体的一种手段的功效。此外,聚类方法与优化算法的整合被证明可以成功提高矿化区域的可信度,这在未来的勘探阶段可能会很有优势。根据研究结果,GWOKM 方法可以生成更可靠、更有效的地球化学异常目标。
{"title":"GWOKM: A novel hybrid optimization algorithm for geochemical anomaly detection based on Grey wolf optimizer and K-means clustering","authors":"Mehrdad Daviran, Reza Ghezelbash, Abbas Maghsoudi","doi":"10.1016/j.chemer.2023.126036","DOIUrl":"10.1016/j.chemer.2023.126036","url":null,"abstract":"<div><p>Identifying the geochemical signatures of valuable mineral deposits using regional geochemical data from stream sediments is a challenging task due to the intricate characteristics of geological formations. Our team is currently investigating the potential of unsupervised clustering analysis (CA) and hybridization with the grey wolf optimizer (GWO) in developing multi-element geochemical models using stream sediment data. To cluster the geochemical data and uncover any unusual patterns, we opted to use the K-means (KM) algorithm due to its straightforward implementation, fast computation speed, and capacity to handle the large datasets. Despite its benefits, the KM method also has notable limitations, such as the random selection of cluster centroids. This can result in higher systematic uncertainty in unsupervised geochemical modeling and longer computation times. To mitigate this concern, we have introduced a new hybrid approach, grey wolf optimizer with K-means so-called the GWOKM algorithm to enhance the delineation of multi-elemental patterns in stream sediment geochemical data. This method incorporates the grey wolf optimization algorithm with KM to optimize the identification of both anomalies and backgrounds using factor analysis and sample catchment basin modeling techniques. This approach was utilized to detect anomalous multi-elemental geochemical patterns indicative of porphyry and skarn copper deposits in the Baft area, Kerman belt, Iran. Upon comparison of the geochemical models derived from KM and GWOKM clustering methods, the latter outperformed the former, as evidenced by its higher prediction rate. The outcomes affirm the efficacy of unsupervised KM clustering analysis (CA) as a means of breaking down geochemical anomaly-background populations. Moreover, the integration of clustering methods with optimization algorithms has proven to be successful for enhancing the credibility of mineralized areas, which could be advantageous in future exploration phases. Based on the results, the GWOKM approach generates more reliable and efficient geochemical anomaly targets.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"84 1","pages":"Article 126036"},"PeriodicalIF":0.0,"publicationDate":"2023-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0009281923000879/pdfft?md5=c740500510a17aa2654475e19cd6607f&pid=1-s2.0-S0009281923000879-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"134937295","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Climate-driven shifts in soil temperature and soil moisture are crucial factors that control the ecosystem-atmosphere greenhouse gas (GHG) balance. In the present study, the relationship between CO2, CH4 fluxes and soil moisture content and temperature sensitivity was examined in three dominating types of urban ecosystems: grassland, city park and arable land. The analysis was based on the field measurements at biweekly intervals over a year using a static closed chamber method in Wroclaw urban area, Poland. The observed patterns of land-atmosphere CO2 and CH4 exchange varied across land cover types and were strongly influenced by seasonal variations in temperature and soil water content. Emission of CO2 from grassland and the city park was two times higher than from the arable land. The calculated CH4 oxidation rate was one and half times higher (p < 0.05) under grassland and the city park as compared to arable land.
The estimated Q10 values ranged between 1.68 and 1.79 for CO2 and from 1.26 to 1.49 for CH4, depending on the ecosystem type. The temperature sensitivity of soil respiration decreased when the temperature was above 24.5 °C across the moisture gradient from 20 to 25 % m/v. Results suggest that despite the urban areas with agricultural land use revealed the lowest CO2 fluxes compared to grassland and city park, the former showed the lowest seasonal mean CH4 oxidation. This indicates that with ongoing warming, the higher Q10 of CO2 production vs. CH4 oxidation will further shift the carbon balance towards the source and this shift will be especially critical for arable lands in urban areas.
{"title":"Temperature and soil moisture control CO2 flux and CH4 oxidation in urban ecosystems","authors":"Yaroslav Bezyk , Maxim Dorodnikov , Maciej Górka , Izabela Sówka , Tymoteusz Sawiński","doi":"10.1016/j.chemer.2023.125989","DOIUrl":"10.1016/j.chemer.2023.125989","url":null,"abstract":"<div><p><span>Climate-driven shifts in soil temperature and soil moisture are crucial factors that control the ecosystem-atmosphere greenhouse gas (GHG) balance. In the present study, the relationship between CO</span><sub>2</sub>, CH<sub>4</sub><span><span> fluxes and soil moisture content and temperature sensitivity was examined in three dominating types of urban ecosystems: grassland, city park and </span>arable land. The analysis was based on the field measurements at biweekly intervals over a year using a static closed chamber method in Wroclaw urban area, Poland. The observed patterns of land-atmosphere CO</span><sub>2</sub> and CH<sub>4</sub><span> exchange varied across land cover types and were strongly influenced by seasonal variations in temperature and soil water content. Emission of CO</span><sub>2</sub> from grassland and the city park was two times higher than from the arable land. The calculated CH<sub>4</sub> oxidation rate was one and half times higher (p < 0.05) under grassland and the city park as compared to arable land.</p><p>The estimated Q<sub>10</sub> values ranged between 1.68 and 1.79 for CO<sub>2</sub> and from 1.26 to 1.49 for CH<sub>4</sub><span>, depending on the ecosystem type. The temperature sensitivity of soil respiration decreased when the temperature was above 24.5 °C across the moisture gradient from 20 to 25 % m/v. Results suggest that despite the urban areas with agricultural land use revealed the lowest CO</span><sub>2</sub> fluxes compared to grassland and city park, the former showed the lowest seasonal mean CH<sub>4</sub> oxidation. This indicates that with ongoing warming, the higher Q<sub>10</sub> of CO<sub>2</sub> production vs. CH<sub>4</sub><span> oxidation will further shift the carbon balance towards the source and this shift will be especially critical for arable lands in urban areas.</span></p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 125989"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"74003943","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-09-01DOI: 10.1016/j.chemer.2023.125979
Cátia Milene Ehlert von Ahn , Michael Ernst Böttcher , Christoph Malik , Julia Westphal , Benjamin Rach , Carla K.M. Nantke , Anna-Kathrina Jenner , Rhodelyn Saban , Vera Winde , Iris Schmiedinger
The flow path of a river draining a lowland into the southern Baltic Sea, the Warnow River, was investigated to evaluate its freshwater composition and potential to be a source of dissolved substances for regional coastal waters. A spatial study was conducted in April 2019 to follow the variations from the source to the estuary. A temporal study of the composition, for five years (2017–2021), was carried out at a site just before the river reaches the estuary. Surface water was sampled to analyse major and trace elements, stable (H, C, O, S), and short-lived (Ra) isotopes. The results show that the composition of the Warnow River along the flow path is controlled by a complex interplay between in-situ processes, exchange with the atmosphere, diffuse groundwater, and surface water inlets. On a temporal scale, pH, nutrient, and redox-sensitive trace element concentrations are strongly impacted by pelagic primary production in spring. During summer and autumn, influences occurred due to benthic microbial activity, associated diffusive release from soils/sediments, and surface water inlets. Throughout the investigation period, the Warnow River was a source of isotopically light CO2 to the atmosphere and DIC to the estuarine waters. The delivered DIC concentrations seemed to vary with season due to changes in biological pelagic and benthic activities. DOC was derived from a mixture of dominated C3 organic sources and potentially from fertilizers. From concentration-discharge relationships, examples of dilution, mobilization, and chemostasis trends were found. Discharge-controlled seasonal trends were superimposed by system internal processes and the hydrological consequences of the river management. Our analysis thus provides new insights into the controls on the variations of water and solutes in a managed river at the land-sea interface as part of the regional hydrological cycle of a lowland catchment-coastal water system.
{"title":"Spatial and temporal variations in the isotope hydrobiogeochemistry of a managed river draining towards the southern Baltic Sea","authors":"Cátia Milene Ehlert von Ahn , Michael Ernst Böttcher , Christoph Malik , Julia Westphal , Benjamin Rach , Carla K.M. Nantke , Anna-Kathrina Jenner , Rhodelyn Saban , Vera Winde , Iris Schmiedinger","doi":"10.1016/j.chemer.2023.125979","DOIUrl":"10.1016/j.chemer.2023.125979","url":null,"abstract":"<div><p><span>The flow path of a river draining a lowland<span> into the southern Baltic Sea<span>, the Warnow River, was investigated to evaluate its freshwater composition and potential to be a source of dissolved substances for regional coastal waters. A spatial study was conducted in April 2019 to follow the variations from the source to the estuary<span>. A temporal study of the composition, for five years (2017–2021), was carried out at a site just before the river reaches the estuary. Surface water was sampled to analyse major and trace elements, stable (H, C, O, S), and short-lived (Ra) isotopes. The results show that the composition of the Warnow River along the flow path is controlled by a complex interplay between in-situ processes, exchange with the atmosphere, diffuse groundwater, and surface water inlets. On a temporal scale, pH, nutrient, and redox-sensitive trace element concentrations are strongly impacted by pelagic primary production in spring. During summer and autumn, influences occurred due to benthic microbial activity, associated diffusive release from soils/sediments, and surface water inlets. Throughout the investigation period, the Warnow River was a source of isotopically light CO</span></span></span></span><sub>2</sub><span><span> to the atmosphere and DIC to the estuarine waters. The delivered DIC concentrations seemed to vary with season due to changes in biological pelagic and benthic activities. </span>DOC was derived from a mixture of dominated C</span><sub>3</sub><span> organic sources and potentially from fertilizers. From concentration-discharge relationships, examples of dilution, mobilization, and chemostasis trends were found. Discharge-controlled seasonal trends were superimposed by system internal processes and the hydrological consequences of the river management. Our analysis thus provides new insights into the controls on the variations of water and solutes in a managed river at the land-sea interface as part of the regional hydrological cycle of a lowland catchment-coastal water system.</span></p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 125979"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"81954349","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-09-01DOI: 10.1016/j.chemer.2023.125975
Marta Trałka , Marek Błachowicz , Marta Jakubiak
This article presents results of chemical and isotopic studies of shallow groundwater and surface waters in order to determine the degree of their contamination near to artificial irrigation fields. The study applied the methodology of detailed sampling around the river in order to capture the direction of pollutant flow and to determine the state of the environment. Samples were taken on both sides of the river, from its bottom and directly from the river. Thanks to bottom pressure measurements, it was possible to determine in what section the river drains or infiltrates groundwater, which, combined with chemical and isotope analyses, made it possible to determine the aims of this study. As it turns out, the nature of the river in the study area is mainly neutral and in lesser extent draining, which does not translate into the degree of groundwater pollution at every point. Due to the sampling methodology used, it was also possible to determine the depth of redox processes and the origin of sulfur in water, which comes mainly from precipitation and other anthropogenic sources. Chemical tests indicate an average quality of shallow groundwater, anthropogenically transformed to varying degrees depending on the location of measurement point. These preliminary results support the applicability of this sampling methodology to other studies and indicate the need to perform more detailed chemical analysis.
{"title":"Role of rivers in restricting pollution movement, as evidenced by chemical and isotopic research on the Widawa River in Wrocław (SW Poland)","authors":"Marta Trałka , Marek Błachowicz , Marta Jakubiak","doi":"10.1016/j.chemer.2023.125975","DOIUrl":"10.1016/j.chemer.2023.125975","url":null,"abstract":"<div><p>This article presents results of chemical and isotopic studies of shallow groundwater and surface waters in order to determine the degree of their contamination near to artificial irrigation fields. The study applied the methodology of detailed sampling around the river in order to capture the direction of pollutant flow<span> and to determine the state of the environment. Samples were taken on both sides of the river, from its bottom and directly from the river. Thanks to bottom pressure measurements, it was possible to determine in what section the river drains or infiltrates groundwater, which, combined with chemical and isotope analyses, made it possible to determine the aims of this study. As it turns out, the nature of the river in the study area is mainly neutral and in lesser extent draining, which does not translate into the degree of groundwater pollution at every point. Due to the sampling methodology used, it was also possible to determine the depth of redox processes and the origin of sulfur in water, which comes mainly from precipitation and other anthropogenic sources. Chemical tests indicate an average quality of shallow groundwater, anthropogenically transformed to varying degrees depending on the location of measurement point. These preliminary results support the applicability of this sampling methodology to other studies and indicate the need to perform more detailed chemical analysis.</span></p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 125975"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"78756780","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-09-01DOI: 10.1016/j.chemer.2023.125987
Mustafa A. Elsagheer , Mokhles K. Azer , Ayman E. Maurice , Ahmed E.S. Khalil , Maysa M.N. Taha
Alkaline volcanics (felsites) and A-type granites are spatially and temporally associated in the Wadi Atalla area, Central Eastern Desert, Egypt. These rocks represent final Neoproterozoic magmatic activity in the Northern Nubian Shield. Wadi Atalla felsites form NW-trending elongate mass consisting of silicic volcanics, which is intruded by A-type granites of Um Had and Um Effein plutons. Field relations indicate that both felsites and A-type granites were emplaced in a series of magmatic pulses. Felsites include tuffaceous, porphyritic and hypabyssal varieties, while A-type granites comprise syenogranite and alkali feldspar granite. Geochemically, they are highly silicic rocks and display a narrow range of SiO2. They have high-K alkaline nature with metaluminous to peraluminous character and were erupted in a post-collisional tectonic setting. Mineral chemistry of biotite supports the alkaline and A-type characters of the studied rocks. Atalla felsites and associated A-type granites show light REE enrichment relative to heavy REE [(La/Lu)n = 2.67–5.72] with pronounced negative Eu anomalies (Eu/Eu* = 0.15–0.52). Compositional similarities between Atalla felsites and A-type granites in the studied area suggest that the intrusive and extrusive events are broadly related. The systematic variation of major- and trace-element contents of the felsites and A-type granites indicates derivation from similar sources through partial melting of juvenile crustal rocks, followed by extensive fractional crystallization. The main fractionated phases are feldspars, with minor role of fractionation of amphibole, biotite, apatite and FeTi oxides. Multiple saturation calculations indicate water-saturated storage and final equilibration conditions for the felsites ranging from 788 °C at 90 MPa to 740 °C at 255 MPa. The parental magmas of the felsites and A-type granites were linked to lithospheric delamination and upwelling of asthenospheric mantle material. This process led to generation of mantle melts that supplied heat to melt the juvenile crust of the Arabian-Nubian Shield (ANS), along with crustal uplift recorded by intersecting strike-slip faults and shear zones. Atalla felsites represent a distinctive post-collisional alkaline volcanic phase in the Nubian Shield that has been emplaced in an extensional tectonic regime, during a phase of fracturing and crustal uplift, which followed the end of the Pan-African orogeny. This volcanic phase is younger than the Dokhan volcanics in the Eastern Desert and older than the typical Katherina volcanics in southern Sinai.
在埃及东部沙漠中部的瓦迪阿塔拉地区,碱性火山岩(长岩)和 A 型花岗岩在空间和时间上相互关联。这些岩石代表了北努比亚地盾最后的新近纪岩浆活动。瓦迪阿塔拉长英岩由硅质火山岩组成,形成西北走向的细长岩块,被乌姆哈德和乌姆埃菲因岩体的 A 型花岗岩侵入。实地关系表明,长英岩和 A 型花岗岩都是在一系列岩浆脉冲中形成的。长英岩包括凝灰岩、斑岩和超基性岩,而 A 型花岗岩则包括正长花岗岩和碱长石花岗岩。从地球化学角度看,它们是高硅质岩石,二氧化硅含量范围较窄。它们具有高K碱性,含金属铝至过铝,在碰撞后的构造环境中喷发。生物岩的矿物化学成分支持所研究岩石的碱性和A型特征。阿塔拉长英岩和相关的A型花岗岩显示出相对于重REE的轻REE富集[(La/Lu)n = 2.67-5.72]和明显的负Eu异常(Eu/Eu* = 0.15-0.52)。所研究地区的阿塔拉长英岩和A型花岗岩在成分上的相似性表明,侵入和挤出事件大致相关。长英岩和 A 型花岗岩的主要元素和痕量元素含量的系统性变化表明,它们是通过部分熔化幼年地壳岩石,然后进行广泛的分馏结晶而从相似的来源衍生出来的。主要的分馏相是长石,闪长石、斜长石、磷灰石和铁钛氧化物的分馏作用较小。多重饱和度计算表明,长石的水饱和储存和最终平衡条件从90兆帕斯卡时的788摄氏度到255兆帕斯卡时的740摄氏度不等。长英岩和A型花岗岩的母岩与岩石圈脱层和星体层地幔物质上涌有关。这一过程产生了地幔熔体,为熔化阿拉伯-努比亚地盾(ANS)的幼年地壳提供了热量,同时通过交错的走向滑动断层和剪切带记录了地壳隆升。阿塔拉长英岩代表了努比亚地盾中一个独特的碰撞后碱性火山岩阶段,它是在泛非造山运动结束后的断裂和地壳抬升阶段,在伸展构造体系中形成的。这一火山阶段比东部沙漠的多汗火山岩年轻,比西奈半岛南部典型的凯瑟琳娜火山岩古老。
{"title":"Geochemistry and origin of felsites and associated A-type granites at Wadi Atalla area, Central Eastern Desert, Egypt: Implication for genesis of Neoproterozoic post-collisional highly silicic melts","authors":"Mustafa A. Elsagheer , Mokhles K. Azer , Ayman E. Maurice , Ahmed E.S. Khalil , Maysa M.N. Taha","doi":"10.1016/j.chemer.2023.125987","DOIUrl":"10.1016/j.chemer.2023.125987","url":null,"abstract":"<div><p><span>Alkaline volcanics (felsites) and A-type granites are spatially and temporally associated in the Wadi Atalla area, Central Eastern Desert, Egypt. These rocks represent final Neoproterozoic magmatic activity in the Northern Nubian Shield. Wadi Atalla felsites<span> form NW-trending elongate mass consisting of silicic volcanics, which is intruded by A-type granites of Um Had and Um Effein plutons. Field relations indicate that both felsites and A-type granites were emplaced in a series of magmatic pulses. Felsites include tuffaceous, porphyritic and hypabyssal varieties, while A-type granites comprise syenogranite and alkali feldspar granite. Geochemically, they are highly silicic rocks and display a narrow range of SiO</span></span><sub>2</sub><span><span><span>. They have high-K alkaline nature with metaluminous to peraluminous character and were erupted in a post-collisional tectonic setting. </span>Mineral chemistry of </span>biotite<span> supports the alkaline and A-type characters of the studied rocks. Atalla felsites and associated A-type granites show light REE enrichment relative to heavy REE [(La/Lu)</span></span><sub><em>n</em></sub><span> = 2.67–5.72] with pronounced negative Eu anomalies (Eu/Eu* = 0.15–0.52). Compositional similarities between Atalla felsites and A-type granites in the studied area suggest that the intrusive and extrusive events are broadly related. The systematic variation of major- and trace-element contents of the felsites and A-type granites indicates derivation from similar sources through partial melting of juvenile crustal rocks, followed by extensive fractional crystallization<span><span>. The main fractionated phases are feldspars, with minor role of fractionation of amphibole, biotite, </span>apatite and Fe</span></span><img><span>Ti oxides. Multiple saturation calculations indicate water-saturated storage and final equilibration conditions for the felsites ranging from 788 °C at 90 MPa to 740 °C at 255 MPa. The parental magmas<span> of the felsites and A-type granites were linked to lithospheric delamination and upwelling of asthenospheric mantle material. This process led to generation of mantle melts that supplied heat to melt the juvenile crust of the Arabian-Nubian Shield (ANS), along with crustal uplift recorded by intersecting strike-slip faults and shear zones. Atalla felsites represent a distinctive post-collisional alkaline volcanic phase in the Nubian Shield that has been emplaced in an extensional tectonic regime, during a phase of fracturing and crustal uplift, which followed the end of the Pan-African orogeny. This volcanic phase is younger than the Dokhan volcanics in the Eastern Desert and older than the typical Katherina volcanics in southern Sinai.</span></span></p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 125987"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"80523310","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-09-01DOI: 10.1016/j.chemer.2023.126004
Aryavart Anand , Klaus Mezger
Age constraints on early solar system processes and events can be derived from meteorites and their components using different radioisotope systems. Due to the short time interval from the first formation of solids in the solar nebula to the accretion and differentiation of planetesimals and some planets, a high temporal resolution of the chronometers is essential and can be obtained in most cases only with short-lived isotope systems, particularly the decay schemes 26Al-26Mg, 182Hf-182W and 53Mn-53Cr. These chronometers provide highly resolved time constrains for the formation of the first solids (Ca-Al-rich inclusions or CAIs), chondrules, planetary cores, for the accretion and differentiation of planetesimals and hydrous/thermal alteration. Formation of Ca-Al-rich inclusions was restricted to the inner solar system and to a short time interval of ≪1 Ma, and marks the “beginning of the solar system”. It was immediately followed by planetesimal formation. The oldest planetesimals accreted within a few 105 a after the formation of CAIs. The accretion of early formed planetesimals and their subsequent differentiation into a metallic core and a silicate mantle was a continuous process that occurred at different times in different locations of the solar nebula and extended over a time interval of at least ~4 Ma. During this time interval the accretion process may have changed from planetesimal formation via streaming instability to pebble accretion. The earliest formed bodies that still needed to settle into stable orbits could have created bow shocks in the adjacent regions still composed of dust and gas which resulted in the formation of silicate chondrules in a narrow time interval from 1.8 to 3 Ma. The chondrule forming interval was immediately followed by the accretion of the chondrite parent bodies, which did not differentiate due to their late accretion when most of the heat producing 26Al had already decayed. Thus, the chondrite parent bodies are a second generation of planetesimals, but chemically they are the most primitive material preserved from the early solar system. Aqueous alteration of volatile rich planetesimals peaked at ca. 3.5 Ma and coincided with metamorphism recorded in ordinary chondrite parent bodies. The compilation of ages from different meteorites and their components demonstrates that similar accretion and differentiation processes do not follow an identical time line from dust to planetesimal formation and they do not correlate with the location in the disk. The accretion of matter into planetesimals was a local phenomenon with stochastic spatial distribution. The spatial distribution of accretion processes operating in the early solar system appears to be similar to those in some directly observable nascent exo-planetary systems.
利用不同的放射性同位素系统,可以从陨石及其成分中得出太阳系早期过程和事件的年龄限制。由于从太阳星云中固体的首次形成到类地行星和某些行星的吸积和分化的时间间隔很短,计时仪的高时间分辨率至关重要,而且在大多数情况下只能利用短寿命同位素系统,特别是 26Al-26Mg、182Hf-182W 和 53Mn-53Cr 等衰变方案来获得。这些计时器为第一批固体(富钙铝包裹体或 CAIs)、软玉、行星核心的形成,为行星的吸积和分化以及水化/热蚀提供了高分辨率的时间约束。富Ca-Al包裹体的形成仅限于内太阳系和≪1Ma≫的短时间间隔,标志着 "太阳系的开始"。紧随其后的是行星的形成。最古老的类星体是在 CAIs 形成后的几 105 a 内吸积形成的。早期形成的类星体的吸积及其随后分化成金属内核和硅酸盐地幔是一个连续的过程,在太阳星云的不同位置的不同时间发生,时间间隔至少为~4 Ma。在这个时间间隔内,吸积过程可能已经从通过流不稳定性形成行星转变为鹅卵石吸积。最早形成的天体仍然需要稳定地进入稳定轨道,它们可能在邻近区域产生了弓形冲击,这些区域仍然由尘埃和气体组成,从而在 1.8 到 3 Ma 的狭窄时间间隔内形成了硅酸盐软玉。在硅酸盐软玉形成的时间间隔之后,紧接着是软玉母体的吸积,由于吸积较晚,大部分产生热量的26Al已经衰变,因此软玉母体没有分化。因此,软玉母体是第二代行星,但从化学角度来看,它们是早期太阳系保留下来的最原始的物质。富含挥发性物质的类星体的水蚀作用在大约 3.5 Ma 时达到顶峰,与太阳系早期的 "陨落 "时间相吻合。3.5 Ma,与普通软玉母体中记录的变质作用相吻合。不同陨石及其成分的年龄汇编表明,类似的吸积和分化过程并不遵循从尘埃到行星形成的完全相同的时间线,它们与在星盘中的位置也不相关。物质吸积成小行星是一种随机空间分布的局部现象。在早期太阳系中运行的吸积过程的空间分布似乎与一些可直接观测到的新生外行星系统中的吸积过程相似。
{"title":"Early solar system chronology from short-lived chronometers","authors":"Aryavart Anand , Klaus Mezger","doi":"10.1016/j.chemer.2023.126004","DOIUrl":"10.1016/j.chemer.2023.126004","url":null,"abstract":"<div><p>Age constraints on early solar system processes and events can be derived from meteorites and their components using different radioisotope systems. Due to the short time interval from the first formation of solids in the solar nebula to the accretion and differentiation of planetesimals and some planets, a high temporal resolution of the chronometers is essential and can be obtained in most cases only with short-lived isotope systems, particularly the decay schemes <sup>26</sup>Al-<sup>26</sup>Mg, <sup>182</sup>Hf-<sup>182</sup>W and <sup>53</sup>Mn-<sup>53</sup>Cr. These chronometers provide highly resolved time constrains for the formation of the first solids (Ca-Al-rich inclusions or CAIs), chondrules, planetary cores, for the accretion and differentiation of planetesimals and hydrous/thermal alteration. Formation of Ca-Al-rich inclusions was restricted to the inner solar system and to a short time interval of ≪1 Ma, and marks the “beginning of the solar system”. It was immediately followed by planetesimal formation. The oldest planetesimals accreted within a few 10<sup>5</sup> a after the formation of CAIs. The accretion of early formed planetesimals and their subsequent differentiation into a metallic core and a silicate mantle was a continuous process that occurred at different times in different locations of the solar nebula and extended over a time interval of at least ~4 Ma. During this time interval the accretion process may have changed from planetesimal formation via streaming instability to pebble accretion. The earliest formed bodies that still needed to settle into stable orbits could have created bow shocks in the adjacent regions still composed of dust and gas which resulted in the formation of silicate chondrules in a narrow time interval from 1.8 to 3 Ma. The chondrule forming interval was immediately followed by the accretion of the chondrite parent bodies, which did not differentiate due to their late accretion when most of the heat producing <sup>26</sup>Al had already decayed. Thus, the chondrite parent bodies are a second generation of planetesimals, but chemically they are the most primitive material preserved from the early solar system. Aqueous alteration of volatile rich planetesimals peaked at ca. 3.5 Ma and coincided with metamorphism recorded in ordinary chondrite parent bodies. The compilation of ages from different meteorites and their components demonstrates that similar accretion and differentiation processes do not follow an identical time line from dust to planetesimal formation and they do not correlate with the location in the disk. The accretion of matter into planetesimals was a local phenomenon with stochastic spatial distribution. The spatial distribution of accretion processes operating in the early solar system appears to be similar to those in some directly observable nascent exo-planetary systems.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 126004"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0009281923000557/pdfft?md5=e3c832bb9ea90c5a20ff1d3d296903f4&pid=1-s2.0-S0009281923000557-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"83303757","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-09-01DOI: 10.1016/j.chemer.2023.125976
Fang Yang , Zaiwen Yang , Huaidong Zhou , Lu Sun , Aimin Zhang , Yang Li , Lingfei Qu , Liang Tang
Discharge of acid mine drainage (AMD) along with heavy metals mobilization is a critical environmental concern. An urgent need is to manage or treat AMD in the minefield effectively. To this end, based on a hydrogeological investigation, the d-T (deuterium excess parameter-Tritium content) technique was adopted to trace the recharge, runoff, and discharge of AMD in the abandoned Dashu pyrite mine in China. The results reveal that AMD in the minefield originates from local precipitation and shallow groundwater and exhibits apparent seasonal runoff variations. The AMD is associated with shallow groundwater from the top of the Quaternary platform on the axis of the Dashu anticline, and protons could originate from the pyrite oxidation. Therefore, an engineering practice to purify the AMD is combined with (1) water diversion to stop AMD formation and blockage of the AMD outlets. (2) Acceleration of Fe(II) oxidation through aeration promotes the precipitation of Fe-oxide and hydroxide. (3) Neutralization of AMD using Karst water from the Maokou Formation (P2m). This study provides a new research idea and tracing method for improving hydrogeological surveys and effectively handling environmental problems related to AMD of abandoned mines.
{"title":"Isotope provenance of AMD and treatment options for large, abandoned mines: A case study of the abandoned Dashu pyrite mine, Southwest China","authors":"Fang Yang , Zaiwen Yang , Huaidong Zhou , Lu Sun , Aimin Zhang , Yang Li , Lingfei Qu , Liang Tang","doi":"10.1016/j.chemer.2023.125976","DOIUrl":"10.1016/j.chemer.2023.125976","url":null,"abstract":"<div><p><span>Discharge of acid mine drainage<span> (AMD) along with heavy metals mobilization is a critical environmental concern. An urgent need is to manage or treat AMD in the minefield effectively. To this end, based on a hydrogeological investigation, the </span></span><strong>d</strong><span>-T (deuterium excess parameter-Tritium content) technique was adopted to trace the recharge, runoff, and discharge of AMD in the abandoned Dashu pyrite mine in China. The results reveal that AMD in the minefield originates from local precipitation and shallow groundwater and exhibits apparent seasonal runoff variations. The AMD is associated with shallow groundwater from the top of the Quaternary platform on the axis of the Dashu anticline, and protons could originate from the pyrite oxidation. Therefore, an engineering practice to purify the AMD is combined with (1) water diversion to stop AMD formation and blockage of the AMD outlets. (2) Acceleration of Fe(II) oxidation through aeration promotes the precipitation of Fe-oxide and hydroxide. (3) Neutralization of AMD using Karst water from the Maokou Formation (P</span><sub>2</sub><em>m</em>). This study provides a new research idea and tracing method for improving hydrogeological surveys and effectively handling environmental problems related to AMD of abandoned mines.</p></div>","PeriodicalId":55973,"journal":{"name":"Chemie Der Erde-Geochemistry","volume":"83 3","pages":"Article 125976"},"PeriodicalIF":0.0,"publicationDate":"2023-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72892282","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}