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Chemical Composition, Mineralogy, and Physical Properties of the Moon’s Mantle: A Review
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-01-27 DOI: 10.1134/S0016702924700733
O. L. Kuskov, E. V. Kronrod, V. A. Kronrod
<p>The problem of the internal structure of the Moon plays a special role in understanding its geochemistry and geophysics. The principal sources of information about the chemical composition and physical state of the deep interior are seismic experiments of the Apollo expeditions, gravity data from the GRAIL mission, and geochemical and isotopic studies of lunar samples. Despite the high degree of similarity of terrestrial and lunar matter in the isotopic composition of several elements, the problem of the similarity and/or difference in the major-component composition of the silicate shells of the Earth and its satellite remains unresolved. This review paper summarizes and critically analyzes information on the composition and structure of the Moon, examines the main contradictions between geochemical and geophysical classes models for the mantle structure, both within each class and between the classes, related to the estimation of the abundance of Fe, Mg, Si, Al, and Ca oxides, and analyzes bulk silicate Moon (BSM) models. The paper describes the principles of the approach to modeling the internal structure of a planetary body, based on the joint inversion of an integrated set of selenophysical, seismic, and geochemical parameters combined with calculations of phase equilibria and physical properties. Two new classes of the chemical composition of the Moon enriched in silica (∼50% SiO<sub>2</sub>) and ferrous iron (11–13% FeO, Mg# 79–81) relative to the bulk composition of the silicate component of the Earth (BSE) are discussed: (i) models E with terrestrial concentrations of CaO and Al<sub>2</sub>O<sub>3</sub> (Earth-like models) and (ii) models M with higher contents of refractory oxides (Moon-like models), which determine the features of the mineralogical and seismic structure of the lunar interior. A probabilistic distribution of geochemical (oxide concentrations) and geophysical (<i>P</i>-, <i>S</i>-wave velocities and density) parameters in the four-layer lunar mantle within the range of permissible selenotherms was obtained. Systematic differences are revealed between contents of major oxides in the silicate shells of the Earth and the Moon. Calculations were carried out for the mineral composition, <i>P</i>-, <i>S</i>-wave velocities, and density of the E/M models, and two classes of conceptual geochemical models: LPUM (Lunar Primitive Upper Mantle) and TWM (Taylor Whole Moon) with Earth’s silica content (∼45 wt % SiO<sub>2</sub>) and different FeO and Al<sub>2</sub>O<sub>3</sub> contents. Arguments are presented in support of the SiO<sub>2</sub>- and FeO-enriched (olivine pyroxenite) lunar mantle, which has no genetic similarity with Earth’s pyrolitic mantle, as a geochemical consequence of the inversion of geophysical parameters and determined by cosmochemical conditions and the mechanism that formed the Moon. The dominant mineral of the lunar upper mantle is high-magnesium orthopyroxene with a low calcium content (rather than olivi
{"title":"Chemical Composition, Mineralogy, and Physical Properties of the Moon’s Mantle: A Review","authors":"O. L. Kuskov,&nbsp;E. V. Kronrod,&nbsp;V. A. Kronrod","doi":"10.1134/S0016702924700733","DOIUrl":"10.1134/S0016702924700733","url":null,"abstract":"&lt;p&gt;The problem of the internal structure of the Moon plays a special role in understanding its geochemistry and geophysics. The principal sources of information about the chemical composition and physical state of the deep interior are seismic experiments of the Apollo expeditions, gravity data from the GRAIL mission, and geochemical and isotopic studies of lunar samples. Despite the high degree of similarity of terrestrial and lunar matter in the isotopic composition of several elements, the problem of the similarity and/or difference in the major-component composition of the silicate shells of the Earth and its satellite remains unresolved. This review paper summarizes and critically analyzes information on the composition and structure of the Moon, examines the main contradictions between geochemical and geophysical classes models for the mantle structure, both within each class and between the classes, related to the estimation of the abundance of Fe, Mg, Si, Al, and Ca oxides, and analyzes bulk silicate Moon (BSM) models. The paper describes the principles of the approach to modeling the internal structure of a planetary body, based on the joint inversion of an integrated set of selenophysical, seismic, and geochemical parameters combined with calculations of phase equilibria and physical properties. Two new classes of the chemical composition of the Moon enriched in silica (∼50% SiO&lt;sub&gt;2&lt;/sub&gt;) and ferrous iron (11–13% FeO, Mg# 79–81) relative to the bulk composition of the silicate component of the Earth (BSE) are discussed: (i) models E with terrestrial concentrations of CaO and Al&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;3&lt;/sub&gt; (Earth-like models) and (ii) models M with higher contents of refractory oxides (Moon-like models), which determine the features of the mineralogical and seismic structure of the lunar interior. A probabilistic distribution of geochemical (oxide concentrations) and geophysical (&lt;i&gt;P&lt;/i&gt;-, &lt;i&gt;S&lt;/i&gt;-wave velocities and density) parameters in the four-layer lunar mantle within the range of permissible selenotherms was obtained. Systematic differences are revealed between contents of major oxides in the silicate shells of the Earth and the Moon. Calculations were carried out for the mineral composition, &lt;i&gt;P&lt;/i&gt;-, &lt;i&gt;S&lt;/i&gt;-wave velocities, and density of the E/M models, and two classes of conceptual geochemical models: LPUM (Lunar Primitive Upper Mantle) and TWM (Taylor Whole Moon) with Earth’s silica content (∼45 wt % SiO&lt;sub&gt;2&lt;/sub&gt;) and different FeO and Al&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;3&lt;/sub&gt; contents. Arguments are presented in support of the SiO&lt;sub&gt;2&lt;/sub&gt;- and FeO-enriched (olivine pyroxenite) lunar mantle, which has no genetic similarity with Earth’s pyrolitic mantle, as a geochemical consequence of the inversion of geophysical parameters and determined by cosmochemical conditions and the mechanism that formed the Moon. The dominant mineral of the lunar upper mantle is high-magnesium orthopyroxene with a low calcium content (rather than olivi","PeriodicalId":12781,"journal":{"name":"Geochemistry International","volume":"62 12","pages":"1227 - 1290"},"PeriodicalIF":0.7,"publicationDate":"2025-01-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S0016702924700733.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143109415","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Shaka Ridge (South Atlantic)—a Remnant of Continental Crust?
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-01-27 DOI: 10.1134/S0016702924700757
N. M. Sushchevskaya, G. L. Leitchenkov, B. V. Belyatsky, D. A. Agapitova

As a result of a study of igneous rocks of the basalt - andesite series, dredged on the Shaka Ridge in the South Atlantic, it was found that they differ from the basalts of mid-ocean ridges and ocean islands, and have an age of 183.8 ± 2.2 Ma, comparable to the time of manifestation of the Karoo-Maud mantle plume in central Gondwana. Geochemical and Sr–Nd–Pb isotopic features of the studied igneous rocks show their similarity with the Jurassic mafic complexes of the Ferrar province in Antarctica and the Falkland Islands, formed during the intrusion of the Karoo-Maud plume and under the influence of paleo-Pacific subduction. However the supply of ice rafted debris into the study area due to ice transportation is considered unlikely. Based on the all data obtained, it was concluded that the Shaka Ridge is a continental block that was moved during the opening of the South Atlantic in the Early Cretaceous-Early Miocene from the continental margin of Africa along an extended transform fault into the present Bouvet triple junction area.

{"title":"Shaka Ridge (South Atlantic)—a Remnant of Continental Crust?","authors":"N. M. Sushchevskaya,&nbsp;G. L. Leitchenkov,&nbsp;B. V. Belyatsky,&nbsp;D. A. Agapitova","doi":"10.1134/S0016702924700757","DOIUrl":"10.1134/S0016702924700757","url":null,"abstract":"<p>As a result of a study of igneous rocks of the basalt - andesite series, dredged on the Shaka Ridge in the South Atlantic, it was found that they differ from the basalts of mid-ocean ridges and ocean islands, and have an age of 183.8 ± 2.2 Ma, comparable to the time of manifestation of the Karoo-Maud mantle plume in central Gondwana. Geochemical and Sr–Nd–Pb isotopic features of the studied igneous rocks show their similarity with the Jurassic mafic complexes of the Ferrar province in Antarctica and the Falkland Islands, formed during the intrusion of the Karoo-Maud plume and under the influence of paleo-Pacific subduction. However the supply of ice rafted debris into the study area due to ice transportation is considered unlikely. Based on the all data obtained, it was concluded that the Shaka Ridge is a continental block that was moved during the opening of the South Atlantic in the Early Cretaceous-Early Miocene from the continental margin of Africa along an extended transform fault into the present Bouvet triple junction area.</p>","PeriodicalId":12781,"journal":{"name":"Geochemistry International","volume":"62 12","pages":"1332 - 1351"},"PeriodicalIF":0.7,"publicationDate":"2025-01-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S0016702924700757.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143109280","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Kinetics of Individual C1–C5 Hydrocarbons Formation of Domanik Shale in Hydrothermal Experiments
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-01-27 DOI: 10.1134/S0016702924700769
D. A. Bushnev, N. S. Burdelnaya, A. A. Ilchenko, Ya. D. Sennikova, D. V. Kuzmin

Twelve hydrothermal autoclave experiments were conducted with Domanik oil shale from the Ukhta region (Chut River) at temperatures of 250–375°C and run duration of 24 h (6 experiments), 72 h (5 experiments), and 48 h (1 experiment). The composition of hydrocarbon gases C1–C5 was studied for each experiment and quantitative data on their yields were obtained. Based on these data, the distributions of generation potential of individual gaseous hydrocarbons by activation energy were established under hydrothermal experimental conditions. The character of the kinetic spectra of individual alkanes C2–C5 is virtually identical; their main narrow maximum corresponds to Ea 55 kcal/mol with an Arrhenius factor of 1 × 1014 s–1. The distribution of the methane generation potential by activation energies is distinguished by the fact that a significant part of its generation potential falls within the region of activation energies of 60–70 kcal/mol and by the uncertainty of the distribution character in this region.

{"title":"Kinetics of Individual C1–C5 Hydrocarbons Formation of Domanik Shale in Hydrothermal Experiments","authors":"D. A. Bushnev,&nbsp;N. S. Burdelnaya,&nbsp;A. A. Ilchenko,&nbsp;Ya. D. Sennikova,&nbsp;D. V. Kuzmin","doi":"10.1134/S0016702924700769","DOIUrl":"10.1134/S0016702924700769","url":null,"abstract":"<p>Twelve hydrothermal autoclave experiments were conducted with Domanik oil shale from the Ukhta region (Chut River) at temperatures of 250–375°C and run duration of 24 h (6 experiments), 72 h (5 experiments), and 48 h (1 experiment). The composition of hydrocarbon gases C<sub>1</sub>–C<sub>5</sub> was studied for each experiment and quantitative data on their yields were obtained. Based on these data, the distributions of generation potential of individual gaseous hydrocarbons by activation energy were established under hydrothermal experimental conditions. The character of the kinetic spectra of individual alkanes C<sub>2</sub>–C<sub>5</sub> is virtually identical; their main narrow maximum corresponds to <i>E</i><sub>a</sub> 55 kcal/mol with an Arrhenius factor of 1 × 10<sup>14</sup> s<sup>–1</sup>. The distribution of the methane generation potential by activation energies is distinguished by the fact that a significant part of its generation potential falls within the region of activation energies of 60–70 kcal/mol and by the uncertainty of the distribution character in this region.</p>","PeriodicalId":12781,"journal":{"name":"Geochemistry International","volume":"62 12","pages":"1352 - 1357"},"PeriodicalIF":0.7,"publicationDate":"2025-01-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143109289","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
The Formation of K-Cymrite in Subduction Zones and Its Potential for Transport of Potassium, Water, and Nitrogen into the Mantle
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-01-27 DOI: 10.1134/S0016702924700745
A. G. Sokol, A. V. Korsakov, A. N. Kruk

The conditions of the formation of K-cymrite in volatile-rich pelite and partially devolatilized mica quartz–muscovite–chlorite schist were experimentally investigated at pressures of 5.5, 6.3, and 7.8 GPa and temperatures ranging from 900 to 1090°C corresponding to hot subduction geotherm. Experimental samples at these P–T conditions formed assemblage of solid phases (Grt + Coe + Phe + Cpx + Ky, with accessory Po + Ru + Zrn ± Mnz) and water-enriched supercritical fluid–melt. Analysis of the obtained data indicates that the stability of phengite and its potential replacement by K-cymrite depends on the P–T conditions and the amount of volatiles in the metasediment. In samples of volatile-rich pelite and mica schist at 5.5 GPa and 900°C, as well as at 6.3 GPa and 1000°C, phengite remains stable in equilibrium with 3–13 wt % of the fluid–melt. With increasing pressure up to 7.8 GPa and temperature up to 1090°C, the fraction of supercritical fluid–melt in pelite reaches 20 wt %, while phengite disappears. Only 5 wt % supercritical fluid–melt are formed in the schist at 7.8 GPa and 1070°C, while most part of phengite is preserved. For the first time, phase assemblage with phengite and K-cymrite (±kokchetavite) was obtained in the pelite and schist samples at 7.8 GPa and 1070°C. The assemblage was identified using Raman mapping. At stepwise devolatilization (with removal of fluid–melt portion forming in equilibrium with volatile-bearing minerals that are stable at P–T conditions of experiments), phengite has been preserved up to 7.8 GPa and 1090°C, but K-cymrite is not formed in the absence of fluid–melt. It was concluded that the most effective transport of volatiles (first of all, water) in the metasediment to depths over 240 km may occur during its partial and early (before the formation of supercritical fluid–melt) devolatilization. In this case, almost all phengite may reach depths of 240 km during metasediment subduction and then transform into water-bearing K-cymrite, or, in the presence of nitrogen in the metasediment, into nitrogen-bearing K-cymrite, thus facilitating the further transport of LILE (large-ion lithophile elements), water, and nitrogen. However, the formation of a significant portion of supercritical fluid–melt leads to the complete dissolution of phengite with increasing P–T conditions, making further transport of LILE, water, and nitrogen impossible. During deep multi-stage devolatilization, phengite remains stable up to depths of 240 km; however, during further subduction, it likely transforms into an anhydrous K-hollandite (KAlSi3O8).

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引用次数: 0
Exsolution in the Au–Au3Cu Region and Correction of the Au–Ag–Cu Phase Diagram Au-Au3Cu区域的溶出及Au-Ag-Cu相图的修正
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S0016702924700642
S. A. Onishchenko, K. G. Parkhacheva, Yu. V. Glukhov, S. K. Kuznetsov, N. Yu. Nikulova, E. M. Tropnikov

The phase composition of native gold was examined in an insufficiently studied part of the Au–Ag–Cu system in the range between pure gold and Au3Cu. In this region, a miscibility gap has been established for the Au–Ag–Cu solid solution, which is decomposed into Au–Ag–Cu and Au3Cu phases. These results in combinations with previously obtained and literature data made it possible to construct a complete phase diagram of the Au–Ag–Cu system in the gold-rich region for low (about 100°C) temperature. The diagram demonstrates the field of a homogeneous Au–Ag–Cu solid solution, and two-phase fields (Au3Cu and Au–Ag–Cu solid solution) and (AuCu and Au–Ag–Cu solid solution), which are separated by a three-phase field (Au3Cu, AuCu, and Au–Ag–Cu solid solution).

在纯金和Au3Cu之间的Au-Ag-Cu体系中,研究了原生金的相组成。在该区域,Au-Ag-Cu固溶体形成了一个混相间隙,分解为Au-Ag-Cu和Au3Cu相。这些结果与先前获得的数据和文献数据相结合,使得在低(约100°C)温度下构建富金区Au-Ag-Cu体系的完整相图成为可能。该图展示了均匀的Au-Ag-Cu固溶体场,以及由三相场(Au3Cu、AuCu和Au-Ag-Cu固溶体)分隔的两相场(Au3Cu和Au-Ag-Cu固溶体)和(AuCu和Au-Ag-Cu固溶体)。
{"title":"Exsolution in the Au–Au3Cu Region and Correction of the Au–Ag–Cu Phase Diagram","authors":"S. A. Onishchenko,&nbsp;K. G. Parkhacheva,&nbsp;Yu. V. Glukhov,&nbsp;S. K. Kuznetsov,&nbsp;N. Yu. Nikulova,&nbsp;E. M. Tropnikov","doi":"10.1134/S0016702924700642","DOIUrl":"10.1134/S0016702924700642","url":null,"abstract":"<p>The phase composition of native gold was examined in an insufficiently studied part of the Au–Ag–Cu system in the range between pure gold and Au<sub>3</sub>Cu. In this region, a miscibility gap has been established for the Au–Ag–Cu solid solution, which is decomposed into Au–Ag–Cu and Au<sub>3</sub>Cu phases. These results in combinations with previously obtained and literature data made it possible to construct a complete phase diagram of the Au–Ag–Cu system in the gold-rich region for low (about 100°C) temperature. The diagram demonstrates the field of a homogeneous Au–Ag–Cu solid solution, and two-phase fields (Au<sub>3</sub>Cu and Au–Ag–Cu solid solution) and (AuCu and Au–Ag–Cu solid solution), which are separated by a three-phase field (Au<sub>3</sub>Cu, AuCu, and Au–Ag–Cu solid solution).</p>","PeriodicalId":12781,"journal":{"name":"Geochemistry International","volume":"62 11","pages":"1174 - 1183"},"PeriodicalIF":0.7,"publicationDate":"2024-12-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S0016702924700642.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142890441","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Biomarker Hydrocarbons in Autochthonous and Migrated Bitumens in the Precambrian of Ust’-Mayskaya-366 Well, Siberian Platform 西伯利亚台地Ust -Mayskaya-366井前寒武纪原生和迁移沥青中的生物标志烃
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S001670292470068X
I. D. Timoshina
<p>The distribution of biomarker hydrocarbons in samples from Ust’-Mayskaya-366 well in the Aldan–Maya depression, Siberian platform, was studied in detail using modern techniques to elucidate biogeochemical features of Precambrian source organic matter (OM) and naphthides generated by it. To correlate OM and assess the effect of migration on biomarker parameters, allochthonous and mixed bitumens (AllB and MB, respectively), as well as open-pore bitumens (OPB) extracted from the uncrushed rocks of the Neryuen, Ignikan, Kandyk, Ust-Kirbin (Riphean), and Sardana (Vendian) formations were studied in comparison with the autochthonous bitumen (AutB) of the source-rock horizon of the Neryuen Formation. Saturated cyclanes and aromatic-fraction compounds from this well were analyzed for the first time. The Neryuen mudstones are enriched in organic matter (TOC > 1%), accumulated in clays [the steranes have βα/(αα + ββ) = 0.5], survived diagenesis in reducing environments without excess H<sub>2</sub>S (the homohopanes have C<sub>35</sub>/C<sub>34</sub> = 0.4), and were thermally transformed at MC<sub>2</sub>–<span>({text{MC}}_{3}^{1})</span> (<i>T</i><sub>max</sub> = 452–465°C). The maximum in tricyclanes C<sub>19–31</sub> in almost all of the studied samples falls onto C<sub>23</sub>, as in the Neryuen AutB. Even homologues of 3,7-dimethylalkanes found in the Neryuen AutB and Ust-Kirbin MB, as well as those detected in trace amounts in the Neryuen and Ignikan MBs and in the OPBs of the Sardana Formation, were apparently disseminated during migration. All bitumens were found out to contain 12- and 13-monomethylalkanes, which are most abundant in the Kandyk OPBs. These compounds can likely be accumulated during migration. The migrated bitumens differ from the AutB in containing a higher proportion of steranes C<sub>29</sub> (up to C<sub>29</sub>/<i>n</i>C<sub>27</sub> > 2) and a higher <i>n</i>C<sub>27</sub>/<i>n</i>C<sub>17</sub> ratio (up to >1). Relationships with the bitumen coefficient was found for Pr/Ph, <i>n</i>C<sub>27</sub>/<i>n</i>C<sub>17</sub>, Σ<i>n</i>C<sub>i</sub>/Σ<i>izo</i>C<sub>i</sub> in acyclic hydrocarbons, C<sub>29</sub>/C<sub>27</sub> in steranes, C<sub>35</sub>/C<sub>34</sub> in homohopanes, hopane/tricyclane ratios; these parameters are likely susceptible to effects of migration. The most probable source of the Riphean bitumens was mainly the carbonaceous rocks of the Neryuen horizon, and the variations in characteristics were caused by catagenesis and migration processes of accumulation or dissemination of low-molecular-weight mobile compounds. The OPBs of the Sardana Formation differ from the Riphean ones. The upper two bitumens are immature parautochthonous, and the others are probably a mixture of Riphean and Vendian bitumens, which were influenced by solutions from the Sardana base-metal stratiform deposits (which is located at approximately 35 km southeast occurs of the area) and the Perevalnoye deposit (at about 20
利用现代技术详细研究了西伯利亚地台阿尔丹-玛雅坳陷Ust ' -Mayskaya-366井样品中生物标志烃的分布,阐明了前寒武纪烃源岩有机质及其生成的石脑油的生物地球化学特征。为了关联有机质并评估运移对生物标志物参数的影响,研究了从Neryuen组、Ignikan组、Kandyk组、Ust-Kirbin组(Riphean组)和Sardana组(Vendian组)的未破碎岩中提取的外来沥青和混合沥青(AllB和MB),以及开孔沥青(OPB),并与Neryuen组烃源岩层的原生沥青(AutB)进行了比较。首次对该井的饱和环烷和芳烃组分进行了分析。纳尔源泥岩富含有机质(TOC &gt;1%), accumulated in clays [the steranes have βα/(αα + ββ) = 0.5], survived diagenesis in reducing environments without excess H2S (the homohopanes have C35/C34 = 0.4), and were thermally transformed at MC2–({text{MC}}_{3}^{1}) (Tmax = 452–465°C). The maximum in tricyclanes C19–31 in almost all of the studied samples falls onto C23, as in the Neryuen AutB. Even homologues of 3,7-dimethylalkanes found in the Neryuen AutB and Ust-Kirbin MB, as well as those detected in trace amounts in the Neryuen and Ignikan MBs and in the OPBs of the Sardana Formation, were apparently disseminated during migration. All bitumens were found out to contain 12- and 13-monomethylalkanes, which are most abundant in the Kandyk OPBs. These compounds can likely be accumulated during migration. The migrated bitumens differ from the AutB in containing a higher proportion of steranes C29 (up to C29/nC27 > 2) and a higher nC27/nC17 ratio (up to >1). Relationships with the bitumen coefficient was found for Pr/Ph, nC27/nC17, ΣnCi/ΣizoCi in acyclic hydrocarbons, C29/C27 in steranes, C35/C34 in homohopanes, hopane/tricyclane ratios; these parameters are likely susceptible to effects of migration. The most probable source of the Riphean bitumens was mainly the carbonaceous rocks of the Neryuen horizon, and the variations in characteristics were caused by catagenesis and migration processes of accumulation or dissemination of low-molecular-weight mobile compounds. The OPBs of the Sardana Formation differ from the Riphean ones. The upper two bitumens are immature parautochthonous, and the others are probably a mixture of Riphean and Vendian bitumens, which were influenced by solutions from the Sardana base-metal stratiform deposits (which is located at approximately 35 km southeast occurs of the area) and the Perevalnoye deposit (at about 20 km), whose mineralization is of Vendian age.
{"title":"Biomarker Hydrocarbons in Autochthonous and Migrated Bitumens in the Precambrian of Ust’-Mayskaya-366 Well, Siberian Platform","authors":"I. D. Timoshina","doi":"10.1134/S001670292470068X","DOIUrl":"10.1134/S001670292470068X","url":null,"abstract":"&lt;p&gt;The distribution of biomarker hydrocarbons in samples from Ust’-Mayskaya-366 well in the Aldan–Maya depression, Siberian platform, was studied in detail using modern techniques to elucidate biogeochemical features of Precambrian source organic matter (OM) and naphthides generated by it. To correlate OM and assess the effect of migration on biomarker parameters, allochthonous and mixed bitumens (AllB and MB, respectively), as well as open-pore bitumens (OPB) extracted from the uncrushed rocks of the Neryuen, Ignikan, Kandyk, Ust-Kirbin (Riphean), and Sardana (Vendian) formations were studied in comparison with the autochthonous bitumen (AutB) of the source-rock horizon of the Neryuen Formation. Saturated cyclanes and aromatic-fraction compounds from this well were analyzed for the first time. The Neryuen mudstones are enriched in organic matter (TOC &gt; 1%), accumulated in clays [the steranes have βα/(αα + ββ) = 0.5], survived diagenesis in reducing environments without excess H&lt;sub&gt;2&lt;/sub&gt;S (the homohopanes have C&lt;sub&gt;35&lt;/sub&gt;/C&lt;sub&gt;34&lt;/sub&gt; = 0.4), and were thermally transformed at MC&lt;sub&gt;2&lt;/sub&gt;–&lt;span&gt;({text{MC}}_{3}^{1})&lt;/span&gt; (&lt;i&gt;T&lt;/i&gt;&lt;sub&gt;max&lt;/sub&gt; = 452–465°C). The maximum in tricyclanes C&lt;sub&gt;19–31&lt;/sub&gt; in almost all of the studied samples falls onto C&lt;sub&gt;23&lt;/sub&gt;, as in the Neryuen AutB. Even homologues of 3,7-dimethylalkanes found in the Neryuen AutB and Ust-Kirbin MB, as well as those detected in trace amounts in the Neryuen and Ignikan MBs and in the OPBs of the Sardana Formation, were apparently disseminated during migration. All bitumens were found out to contain 12- and 13-monomethylalkanes, which are most abundant in the Kandyk OPBs. These compounds can likely be accumulated during migration. The migrated bitumens differ from the AutB in containing a higher proportion of steranes C&lt;sub&gt;29&lt;/sub&gt; (up to C&lt;sub&gt;29&lt;/sub&gt;/&lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;27&lt;/sub&gt; &gt; 2) and a higher &lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;27&lt;/sub&gt;/&lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;17&lt;/sub&gt; ratio (up to &gt;1). Relationships with the bitumen coefficient was found for Pr/Ph, &lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;27&lt;/sub&gt;/&lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;17&lt;/sub&gt;, Σ&lt;i&gt;n&lt;/i&gt;C&lt;sub&gt;i&lt;/sub&gt;/Σ&lt;i&gt;izo&lt;/i&gt;C&lt;sub&gt;i&lt;/sub&gt; in acyclic hydrocarbons, C&lt;sub&gt;29&lt;/sub&gt;/C&lt;sub&gt;27&lt;/sub&gt; in steranes, C&lt;sub&gt;35&lt;/sub&gt;/C&lt;sub&gt;34&lt;/sub&gt; in homohopanes, hopane/tricyclane ratios; these parameters are likely susceptible to effects of migration. The most probable source of the Riphean bitumens was mainly the carbonaceous rocks of the Neryuen horizon, and the variations in characteristics were caused by catagenesis and migration processes of accumulation or dissemination of low-molecular-weight mobile compounds. The OPBs of the Sardana Formation differ from the Riphean ones. The upper two bitumens are immature parautochthonous, and the others are probably a mixture of Riphean and Vendian bitumens, which were influenced by solutions from the Sardana base-metal stratiform deposits (which is located at approximately 35 km southeast occurs of the area) and the Perevalnoye deposit (at about 20 ","PeriodicalId":12781,"journal":{"name":"Geochemistry International","volume":"62 11","pages":"1184 - 1199"},"PeriodicalIF":0.7,"publicationDate":"2024-12-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142890437","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Ore Apatite-Bearing Mineralization of the Velimyaki Gabbroid Massif in the Raahe–Ladoga Zone of the Northern Ladoga Region: Identification of Formation Conditions and Estimation of Apatite Age 北拉多加区拉赫-拉多加带维里米亚基辉长岩块含矿磷灰石成矿作用:形成条件鉴定及磷灰石年龄估算
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S0016702924700654
Sh. K. Baltybaev, R. L. Anisimov, I. M. Vasilyeva, N. G. Rizvanova, O. L. Galankina, V. M. Savatenkov

The Early Proterozoic gabbros of the Velimyaki intrusion of the Northern Ladoga region contain titanomagnetite ore, which has been mined as early as the end of the 19th century. Titanomagnetite horizons are enriched in phosphorus in form of apatite reaching 10 vol %. Isotopic Pb–Pb dating indicates that apatite was likely redeposited during superimposed metamorphism that was significantly separated in time from the magmatic stage of gabbros and clinopyroxene–titanomagnetite ores. Mineralogical, petrological, and isotope-geochemical criteria for the superimposed nature of the mineral formation with apatite recrystallization are the relationship of this mineral with the formation of other metamorphic minerals (hornblende, biotite, sodic plagioclase), the isotopic age of apatite (1790 ± 5 Ma), and the lower temperature (620–710°C) of its formation compared to the crystallization temperatures (900–1260°C) of magmatic minerals. The Pb–Pb age of apatite coincides with the age of metamorphic minerals from other rocks of Late Svecofennian region, as well as with the Rb–Sr ages of biotite and amphibole from host supracrustal rocks. Based on the data obtained, it was concluded that recrystallization of apatite and resetting of the U–Pb system occurred during the Late Svecofennian regional metamorphism.

北拉多加地区维里米亚基侵入岩早元古代辉长岩含钛磁铁矿,早在19世纪末就已被开采。钛磁铁矿层位以磷灰石形式富磷,磷含量达10 vol %。同位素Pb-Pb定年表明,磷灰石可能是在辉长岩和斜辉石-钛磁铁矿岩浆期明显分离的叠加变质作用中再沉积的。磷灰石与其他变质矿物(角闪石、黑云母、钠斜长石)形成的关系、磷灰石的同位素年龄(1790±5 Ma)、磷灰石形成的温度(620 ~ 710℃)低于岩浆矿物的结晶温度(900 ~ 1260℃),是磷灰石形成与磷灰石再结晶叠加的矿物学、岩石学和同位素地球化学标准。磷灰石的Pb-Pb年龄与晚西芬系其他岩石中的变质矿物年龄一致,与寄主壳上岩石中的黑云母和角闪洞的Rb-Sr年龄一致。根据所获得的资料,认为在晚斯韦芬尼期区域变质作用中发生了磷灰石的再结晶和U-Pb体系的重置。
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引用次数: 0
Speciation of Chemical Elements in the Waters of the Herberz Historical Mine, Karelia, Russia: Thermodynamic Calculations and Fractionation 俄罗斯卡累利阿赫贝兹历史矿水中化学元素的形态:热力学计算和分馏
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S0016702924700678
E. S. Sidkina, A. S. Toropov, A. A. Konyshev

The speciation of chemical elements in the waters and its dependence on the dissolved organic matter were studied by a complex of methods, involving thermodynamic calculations and experimental fractionation. The waters were studied at the abandoned and flooded Herberz Mine in the Pitkäranta district, Karelia, Russia. The regional natural waters are typically highly humified. In combination with the unique metallogeny of the rocks, this makes the mine suitable for solving the formulated problems. The eastern shaft of the Herberz Mine was sampled to a depth of 20 m to trance the changes induced by changes in the redox conditions. One of the geochemical characteristics of the waters is their relatively high concentrations of trace elements and a low salinity (TDS, total dissolved solids). All water samples from the Herberz Mine contain elevated concentrations of Zn, Fe, Mn, Cu, Ni, As, and W. Experimental fractionation and thermodynamic simulations of the speciation of chemical elements led us to identify metals whose accumulation most strongly depends on organic matter (OM). Both methods have demonstrated that U, Th, Cu, Ni, and Y show a high chemical affinity to OM. Metals (Cd and Fe) weakly bonded to the functional groups of natural OM, with the predominance of electrostatic bonding and a higher proportion of carboxyl bonds, are most susceptible to transformations with changes in geochemical conditions.

通过热力学计算和实验分馏等多种方法研究了水体中化学元素的形态及其对溶解有机物的依赖关系。在俄罗斯卡累利阿Pitkäranta地区的废弃和淹水的Herberz矿山,研究了水。该地区的天然水体通常是高度腐殖化的。结合该矿岩石独特的成矿作用,使该矿适合于解决所制定的问题。对Herberz矿东竖井取样至20 m深度,观察氧化还原条件变化引起的变化。水体的地球化学特征之一是其相对较高的微量元素浓度和较低的盐度(TDS,总溶解固体)。Herberz矿的所有水样都含有高浓度的Zn、Fe、Mn、Cu、Ni、As和w。化学元素形态的实验分馏和热力学模拟使我们确定了其积累最强烈依赖于有机物(OM)的金属。两种方法都证明了U、Th、Cu、Ni和Y对OM具有很高的化学亲和力。与天然OM官能团成键较弱的金属(Cd和Fe),以静电键为主,羧基键比例较高,最容易随着地球化学条件的变化而发生转化。
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引用次数: 0
Gold in Precambrian Rocks of the Yenisei Ridge, East Siberia, and Geological and Geochemical Prerequisites for the Formation of Gold Mineralization in the Central Metallogenic Belt of the Region 东西伯利亚叶尼塞岭前寒武纪岩石中的金及其中央成矿带金矿形成的地质地球化学条件
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S0016702924700666
A. D. Nozhkin, I. I. Likhanov

As a large gold-bearing province, the Yenisei Ridge does not show elevated background gold concentrations. All types of its sedimentary, metamorphic, and igneous rocks, except only the carbonaceous black shales, contain concentrations of the noble metal at the level of its Clarke values. All local gold deposits are constrained within the regional Central Metallogenic Belt, in which geological–geochemical conditions occurred that were favorable for the deposition of gold and gold–uranium ore mineralization: most of the deposits are constrained within a trough structure, the area was affected by several pulses of plume magmatism, which introduced, redistributed, and concentrated gold and uranium, and the developing ore-concentrating and ore-controlling systems formed economic deposits and associated zones of hydrothermal metamorphism with geochemical aureoles of Pb, Zn, Ag, Au, Bi, and As.

叶尼塞岭作为一个大的含金省,并没有显示出背景金浓度的升高。除了碳质黑色页岩外,所有类型的沉积岩、变质岩和火成岩都含有达到克拉克值水平的贵金属。本区金矿均局限于区域中央成矿带内,区内具有有利于金沉积和金铀矿化的地质地球化学条件;区内大部分矿床受槽状构造约束,受数次羽流岩浆活动脉冲的影响,对金、铀进行了引入、再分布和富集,发育的成矿控矿系统形成了具有Pb、Zn、Ag、Au、Bi、As等地球化学光环的经济矿床和热液变质伴生带。
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引用次数: 0
Trace Element Composition of Zircons from Rapakivi Granites of the Gubanov Intrusion, the Wiborg Massif, as a Reflection of the Fluid Saturation of the Melt Wiborg地块Gubanov岩体Rapakivi花岗岩中锆石微量元素组成及其对熔体流体饱和度的反映
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-12-26 DOI: 10.1134/S0016702924700630
I. V. Rogova, V. S. Stativko, D. A. Petrov, S. G. Skublov

SEM-EDS and SIMS in situ methods were used to study the trace element composition of zircon from rapakivi granites of the Wiborg massif: wiborgites of the second phase, trachytoid granites of the third phase, as well as aplitic granites from their contact zone. All three rock varieties are available for study in the building stone quarry of the Vozrozhdenie deposit (Karelian Isthmus), where the granites of the Gubanov intrusion are mined. Zircon composition from all rock types shows traces of active fluid impact. This impact is manifested both at the level of zircon internal structure (dark zones and areas on BSE-image) and in the contents of trace and rare-earth elements, which significantly increase in the altered zones that differ in the BSE color. The total REE content in the studied zircon reaches 9400 ppm. Zircon from granites of the third phase show an opposite slope of LREE and HREE distribution pattern, i.e., “bird wings” profile (SmN/LaN < 1). In the discrimination diagrams, the majority of the analyzed spots falls into the field of hydrothermal zircon. It is possible to assume that a source of fluid that affected zircon in all types of granites was fluid-saturated melts that produced trachytoid granites of the third phase.

采用SEM-EDS和SIMS原位法研究了Wiborg地块的rapakivi花岗岩、第二阶段的wiborgites、第三阶段的trachytoid花岗岩及其接触带的apictic花岗岩中锆石的微量元素组成。在Vozrozhdenie矿床(卡累利阿地峡)的建筑采石场,所有三种岩石品种都可用于研究,那里开采了Gubanov侵入岩体的花岗岩。所有岩石类型的锆石成分都显示了活跃流体冲击的痕迹。这种影响既表现在锆石内部结构水平(暗区和BSE图像上的区域),也表现在微量元素和稀土元素的含量上,在BSE颜色不同的蚀变带中,微量元素和稀土元素的含量显著增加。锆石中稀土元素总含量达9400 ppm。第三期花岗岩锆石呈现重、重稀土元素反斜分布模式,即“鸟翼”型剖面(SmN/LaN <;1)在判别图中,分析的斑点大部分属于热液锆石场。可以假设,影响所有类型花岗岩中锆石的流体来源是流体饱和熔体,这些熔体产生了第三相的粗粒状花岗岩。
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Geochemistry International
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