Pub Date : 2024-10-03DOI: 10.1016/j.gca.2024.09.035
Y.Y. He, S. Bernard, M. Lecasble, J.-C. Viennet, I. Criouet, D. Boulesteix, N. Khodorova, L. Delbes, M. Guillaumet, F. Baudin, B. Laurent, A. Buch, L. Remusat
Carbonaceous chondrites contain amino acids, with variable abundances and isotope compositions between and within carbonaceous chondrites. The parent body processes, and the presence of clay minerals may explain those differences. Here, we experimentally investigate the evolution of 6 amino acids (glycine, β-alanine, α-alanine, 2-aminoisobutyric acid, γ-aminobutyric acid, and isovaline) exposed to hydrothermal conditions in the presence or absence of silicates. We determined the chemical nature and isotopic composition of the organic compounds of the soluble and solid fractions of the residues using X-ray diffraction, spectroscopy, and mass-spectrometry methods. Glycine and α-alanine exhibit a rather high stability, which is consistent with the measured abundances of α-alanine and glycine in chondrites having experienced various degrees of aqueous alteration. In the meantime, the evolution of β-alanine under hydrothermal conditions leads to the formation of a new compound, which likely results from the decarboxylation and deamination of β-alanine followed by recombination. More than 95 % of γ-ABA was transformed into 2-pyrrolidione though self-cyclization during the aqueous alteration. The solid residues of the experiments conducted in the presence of clay minerals contain organic material, with abundances varying depending on the amino acid used for the experiments (TOC isovaline > 2-aminoisobutyric acid > γ-aminobutyric acid > glycine > α-alanine > β-alanine). Clay minerals thus preferentially trap branched amino acids over chained amino acids, likely within their interlayer spaces as suggested by XRD data. The δ13C values of amino acids have not changed significantly during the experiments, even with the presence of silicates. Thus, the δ13C values of amino acids reported in CR and CM chondrites likely relate to synthetic conditions or the origin of their precursors (i.e. inherited from the pre-accretion processes).
碳质软岩含有氨基酸,在碳质软岩之间和碳质软岩内部,氨基酸的丰度和同位素组成各不相同。母体过程和粘土矿物的存在可能是造成这些差异的原因。在这里,我们通过实验研究了6种氨基酸(甘氨酸、β-丙氨酸、α-丙氨酸、2-氨基异丁酸、γ-氨基丁酸和异戊酸)在存在或不存在硅酸盐的热液条件下的演变过程。我们使用 X 射线衍射、光谱和质谱方法测定了残留物可溶部分和固体部分有机化合物的化学性质和同位素组成。甘氨酸和α-丙氨酸表现出相当高的稳定性,这与在经历过不同程度水蚀变的软玉中测量到的α-丙氨酸和甘氨酸的丰度是一致的。与此同时,β-丙氨酸在热液条件下的演化导致了一种新化合物的形成,这种新化合物很可能是由β-丙氨酸脱羧和脱氨基后重组而成的。在水变化过程中,95% 以上的 γ-ABA 通过自我环化转化为 2-吡咯烷酮。在有粘土矿物存在的情况下进行的实验的固体残留物含有有机物质,其丰度随实验所用氨基酸的不同而变化(TOC 异戊酸;2-氨基异丁酸;γ-氨基丁酸;甘氨酸;α-丙氨酸)。因此,粘土矿物更倾向于捕获支链氨基酸,而不是链状氨基酸,这很可能与 XRD 数据所表明的那样,是在它们的层间空隙中。在实验过程中,即使存在硅酸盐,氨基酸的 δ13C 值也没有发生显著变化。因此,报告的 CR 和 CM 软骨中氨基酸的 δ13C 值很可能与合成条件或其前体的来源有关(即继承自生成前的过程)。
{"title":"The evolution of amino acids under asteroidal aqueous alteration","authors":"Y.Y. He, S. Bernard, M. Lecasble, J.-C. Viennet, I. Criouet, D. Boulesteix, N. Khodorova, L. Delbes, M. Guillaumet, F. Baudin, B. Laurent, A. Buch, L. Remusat","doi":"10.1016/j.gca.2024.09.035","DOIUrl":"https://doi.org/10.1016/j.gca.2024.09.035","url":null,"abstract":"Carbonaceous chondrites contain amino acids, with variable abundances and isotope compositions between and within carbonaceous chondrites. The parent body processes, and the presence of clay minerals may explain those differences. Here, we experimentally investigate the evolution of 6 amino acids (glycine, β-alanine, α-alanine, 2-aminoisobutyric acid, γ-aminobutyric acid, and isovaline) exposed to hydrothermal conditions in the presence or absence of silicates. We determined the chemical nature and isotopic composition of the organic compounds of the soluble and solid fractions of the residues using X-ray diffraction, spectroscopy, and mass-spectrometry methods. Glycine and α-alanine exhibit a rather high stability, which is consistent with the measured abundances of α-alanine and glycine in chondrites having experienced various degrees of aqueous alteration. In the meantime, the evolution of β-alanine under hydrothermal conditions leads to the formation of a new compound, which likely results from the decarboxylation and deamination of β-alanine followed by recombination. More than 95 % of γ-ABA was transformed into 2-pyrrolidione though self-cyclization during the aqueous alteration. The solid residues of the experiments conducted in the presence of clay minerals contain organic material, with abundances varying depending on the amino acid used for the experiments (TOC isovaline > 2-aminoisobutyric acid > γ-aminobutyric acid > glycine > α-alanine > β-alanine). Clay minerals thus preferentially trap branched amino acids over chained amino acids, likely within their interlayer spaces as suggested by XRD data. The δ<ce:sup loc=\"post\">13</ce:sup>C values of amino acids have not changed significantly during the experiments, even with the presence of silicates. Thus, the δ<ce:sup loc=\"post\">13</ce:sup>C values of amino acids reported in CR and CM chondrites likely relate to synthetic conditions or the origin of their precursors (i.e. inherited from the pre-accretion processes).","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"197 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2024-10-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142673657","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-10-02DOI: 10.1016/j.gca.2024.09.034
Yixuan Yang, Qingze Chen, Jing Liu, Jieqi Xing, Yiping Yang, Runliang Zhu, Hongping He, Michael F. Hochella Jr.
The formation of nanominerals and mineral nanoparticles (NMMNs) has drawn broad attention due to their high reactivity and omnipresence in the environment. While the heterogeneous formation of NMMNs on surfaces of various minerals has been extensively studied, there is limited understanding of how mineral heteroaggregates influence this process. In this study, we investigated how heteroaggregates of iron (hydr)oxides and clay minerals affect the heterogeneous oxidation of aqueous Mn(II) and crystallization of manganese (hydr)oxides (MnOx). Our results revealed that iron (hydr)oxides (ferrihydrite) and clay minerals (kaolinite or montmorillonite) in heteroaggregates exerted coupled effects on these processes, dictating the distribution of Mn and the morphology of MnOx. Specifically, ferrihydrite catalyzed gradual oxidative removal of Mn(II) and triggered MnOx nucleation; in contrast, kaolinite/montmorillonite rapidly adsorbed Mn(II) but hardly catalyzed its oxidation. These reactions collectively resulted in fast adsorption and gradual oxidation of Mn(II) on the heteroaggregates. Further, MnOx nanoparticles formed on ferrihydrite surfaces migrated to kaolinite/montmorillonite surfaces, leading to interactions between MnOx and various component minerals within the heteroaggregates. This significantly altered the subsequent growth pathways and the eventual morphology of MnOx. Consequently, while MnOx nanoparticles in the ferrihydrite-only system aggregated freely and formed well-extended nanowires, those in the ferrihydrite-kaolinite system predominantly became short nanorods due to the immobilization by kaolinite surfaces; in the ferrihydrite-montmorillonite system, considerable MnOx nanoparticles attached to montmorillonite surfaces due to strong electrostatic attraction, and subsequently grew into blocky particles via particle attachment. These findings illustrate that surface reactivities of heteroaggregated ferrihydrite and kaolinite/montmorillonite are coupled when they interact with aqueous Mn(II) or MnOx. Our work exemplifies, for the first time, the cooperation between surfaces of various minerals during the heterogeneous formation of NMMNs. Findings from this study also enhance our understanding of MnOx formation on surfaces with diverse atomic structures, and contribute to the knowledge of Mn cycling in the environment.
{"title":"Coupled effects of iron (hydr)oxides and clay minerals on the heterogeneous oxidation of aqueous Mn(II) and crystallization of manganese (hydr)oxides","authors":"Yixuan Yang, Qingze Chen, Jing Liu, Jieqi Xing, Yiping Yang, Runliang Zhu, Hongping He, Michael F. Hochella Jr.","doi":"10.1016/j.gca.2024.09.034","DOIUrl":"https://doi.org/10.1016/j.gca.2024.09.034","url":null,"abstract":"The formation of nanominerals and mineral nanoparticles (NMMNs) has drawn broad attention due to their high reactivity and omnipresence in the environment. While the heterogeneous formation of NMMNs on surfaces of various minerals has been extensively studied, there is limited understanding of how mineral heteroaggregates influence this process. In this study, we investigated how heteroaggregates of iron (hydr)oxides and clay minerals affect the heterogeneous oxidation of aqueous Mn(II) and crystallization of manganese (hydr)oxides (MnO<ce:inf loc=\"post\">x</ce:inf>). Our results revealed that iron (hydr)oxides (ferrihydrite) and clay minerals (kaolinite or montmorillonite) in heteroaggregates exerted coupled effects on these processes, dictating the distribution of Mn and the morphology of MnO<ce:inf loc=\"post\">x</ce:inf>. Specifically, ferrihydrite catalyzed gradual oxidative removal of Mn(II) and triggered MnO<ce:inf loc=\"post\">x</ce:inf> nucleation; in contrast, kaolinite/montmorillonite rapidly adsorbed Mn(II) but hardly catalyzed its oxidation. These reactions collectively resulted in fast adsorption and gradual oxidation of Mn(II) on the heteroaggregates. Further, MnO<ce:inf loc=\"post\">x</ce:inf> nanoparticles formed on ferrihydrite surfaces migrated to kaolinite/montmorillonite surfaces, leading to interactions between MnO<ce:inf loc=\"post\">x</ce:inf> and various component minerals within the heteroaggregates. This significantly altered the subsequent growth pathways and the eventual morphology of MnO<ce:inf loc=\"post\">x</ce:inf>. Consequently, while MnO<ce:inf loc=\"post\">x</ce:inf> nanoparticles in the ferrihydrite-only system aggregated freely and formed well-extended nanowires, those in the ferrihydrite-kaolinite system predominantly became short nanorods due to the immobilization by kaolinite surfaces; in the ferrihydrite-montmorillonite system, considerable MnO<ce:inf loc=\"post\">x</ce:inf> nanoparticles attached to montmorillonite surfaces due to strong electrostatic attraction, and subsequently grew into blocky particles via particle attachment. These findings illustrate that surface reactivities of heteroaggregated ferrihydrite and kaolinite/montmorillonite are coupled when they interact with aqueous Mn(II) or MnO<ce:inf loc=\"post\">x</ce:inf>. Our work exemplifies, for the first time, the cooperation between surfaces of various minerals during the heterogeneous formation of NMMNs. Findings from this study also enhance our understanding of MnO<ce:inf loc=\"post\">x</ce:inf> formation on surfaces with diverse atomic structures, and contribute to the knowledge of Mn cycling in the environment.","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"46 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2024-10-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142673693","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-10-02DOI: 10.1016/j.gca.2024.09.024
L. Nicole Arellano , Emily J. Beverly , Ny Riavo G. Voarintsoa , Christopher B. Skinner , Andrew J. Schauer , Eric J. Steig
We present one year of δD, δ18O, d-excess, and Δʹ17O data from monthly precipitation at a Caribbean coastal site in Panama and from tap waters across the country to constrain geographic, climate, and moisture source controls on isotopic variability and better understand the sources and mechanisms of precipitation in Central America, a region facing significant modifications to the annual rainfall cycle due to climate change. Monthly precipitation δD ranged from –52.2 to +14.3 ‰, δ18O from –7.6 to +0.4 ‰, d-excess from +7.1 to +11.6 ‰, and Δ′17O from +11 to +29 per meg. Rainy season precipitation samples were found to have lower δD, δ18O, and d-excess due to Rayleigh distillation during the condensation and rainout of Pacific moisture over the central cordilleras, which results in decoupling between d-excess and Δ′17O. Outlier Δ′17O values during peak dry and rainy months may reflect seasonal changes in water vapor sourcing, from Caribbean to Pacific and/or locally recycled moisture, or may be a result of organic contamination. Tap water δD ranged from –82.3 to –14.3 ‰, δ18O from –11.6 to –2.4 ‰, d-excess from +4.3 to +12.2 ‰ and Δ′17O from –2 to +84 per meg. Tap water δD and δ18O values increase eastward due to lower orographic effects and Pacific and locally recycled moisture contributions to rainfall and greater secondary evaporation. Tap water d-excess and Δ′17O values are also de-coupled but lack clear spatial trends and controls. The results of this study indicate the promise of adding Δ′17O to the isotopic toolkit in tropical mountainous regions with complicated water cycling dynamics and provide a baseline for future triple oxygen isotope investigations.
{"title":"Triple oxygen isotope variability of precipitation in a tropical mountainous region","authors":"L. Nicole Arellano , Emily J. Beverly , Ny Riavo G. Voarintsoa , Christopher B. Skinner , Andrew J. Schauer , Eric J. Steig","doi":"10.1016/j.gca.2024.09.024","DOIUrl":"10.1016/j.gca.2024.09.024","url":null,"abstract":"<div><div>We present one year of δD, δ<sup>18</sup>O, d-excess, and Δʹ<sup>17</sup>O data from monthly precipitation at a Caribbean coastal site in Panama and from tap waters across the country to constrain geographic, climate, and moisture source controls on isotopic variability and better understand the sources and mechanisms of precipitation in Central America, a region facing significant modifications to the annual rainfall cycle due to climate change. Monthly precipitation δD ranged from –52.2 to +14.3 ‰, δ<sup>18</sup>O from –7.6 to +0.4 ‰, d-excess from +7.1 to +11.6 ‰, and Δ′<sup>17</sup>O from +11 to +29 per meg. Rainy season precipitation samples were found to have lower δD, δ<sup>18</sup>O, and d-excess due to Rayleigh distillation during the condensation and rainout of Pacific moisture over the central cordilleras, which results in decoupling between d-excess and Δ′<sup>17</sup>O. Outlier Δ′<sup>17</sup>O values during peak dry and rainy months may reflect seasonal changes in water vapor sourcing, from Caribbean to Pacific and/or locally recycled moisture, or may be a result of organic contamination. Tap water δD ranged from –82.3 to –14.3 ‰, δ<sup>18</sup>O from –11.6 to –2.4 ‰, d-excess from +4.3 to +12.2 ‰ and Δ′<sup>17</sup>O from –2 to +84 per meg. Tap water δD and δ<sup>18</sup>O values increase eastward due to lower orographic effects and Pacific and locally recycled moisture contributions to rainfall and greater secondary evaporation. Tap water d-excess and Δ′<sup>17</sup>O values are also de-coupled but lack clear spatial trends and controls. The results of this study indicate the promise of adding Δ′<sup>17</sup>O to the isotopic toolkit in tropical mountainous regions with complicated water cycling dynamics and provide a baseline for future triple oxygen isotope investigations.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"385 ","pages":"Pages 1-15"},"PeriodicalIF":4.5,"publicationDate":"2024-10-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142421784","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-29DOI: 10.1016/j.gca.2024.09.032
Jeemin H. Rhim , Sebastian Kopf , Jamie McFarlin , Ashley E. Maloney , Harpreet Batther , Carolynn M. Harris , Alice Zhou , Xiahong Feng , Yuki Weber , Shelley Hoeft-McCann , Ann Pearson , William D. Leavitt
<div><div>The stable hydrogen isotope composition of archaeal lipids is emerging as a potential paleoenvironmental proxy, adding to the well-established application of plant leaf wax-derived <em>n</em>-alkanes in paleohydrological reconstruction. A handful of studies reported relatively invariant and depleted hydrogen isotope compositions for archaeal lipids despite the range of different organisms and growth conditions explored. However, how modes of metabolism and physiological state (growth phase) affect the hydrogen isotope signatures of archaeal lipids remains poorly understood, limiting our ability to interpret archaeal lipid biomarker records from the environment. Here we conducted water isotope label experiments with a metabolically flexible and well-studied model archaeon <em>Archaeoglobus fulgidus</em> and quantified the hydrogen isotope fractionation between lipids and water in response to different carbon substrates and electron donor–acceptor pairs at different growth phases. The <sup>2</sup>H/<sup>1</sup>H fractionation between lipids and water (ε<sub>L/W</sub>) was overall negative. Both carbon metabolism and growth phase affected the magnitude of isotope fractionation in <em>A. fulgidus</em>; however, the changes in ε<sub>L/W</sub> values were relatively subtle where they ranged from –283 to –229 ‰ across all tested conditions, overlapping with the ranges observed for other archaea in previous studies. Isotope flux-balance model results suggest that ≥ 80 % and ≥ 50 % of lipid-bound H in <em>A. fulgidus</em> cultures directly reflect water isotope compositions (i.e., not via organic substrate or H<sub>2</sub>) during autotrophy and heterotrophy, respectively. The model results also suggest two main mechanisms of consistent <sup>2</sup>H depletion observed in <em>A. fulgidus</em> tetraethers as well as other archaeal lipids reported in previous studies: 1) isotopic re-equilibration via upstream isomerization reactions involving C<sub>5</sub> units and 2) downstream double bond reduction catalyzed by a flavoenzyme geranylgeranyl reductase. These results are consistent with previous isotope flux-balance model results for a different archaeon. Finally, we synthesized available data to compare ε<sub>L/W</sub> patterns across all three domains of life: Eukarya, Archaea and Bacteria. Because they vary fundamentally in lipid biosynthesis pathways, we present comparative discussions in pairs, focusing on the shared biochemical mechanisms among isoprenoid lipids and potential signals of metabolic adaptations across prokaryotic lipids. Emerging patterns between diverse archaeal and eukaryotic isoprenoid lipids are consistent with the two proposed mechanisms for <sup>2</sup>H depletion identified (isomerization and final saturation). The patterns between archaeal isoprenoids and bacterial fatty acids suggest that the general state of energy limitation may also contribute to large, negative values of ε<sub>L/W</sub> observed in prokaryotic lipi
{"title":"Metabolic imprints in the hydrogen isotopes of Archaeoglobus fulgidus tetraether lipids","authors":"Jeemin H. Rhim , Sebastian Kopf , Jamie McFarlin , Ashley E. Maloney , Harpreet Batther , Carolynn M. Harris , Alice Zhou , Xiahong Feng , Yuki Weber , Shelley Hoeft-McCann , Ann Pearson , William D. Leavitt","doi":"10.1016/j.gca.2024.09.032","DOIUrl":"10.1016/j.gca.2024.09.032","url":null,"abstract":"<div><div>The stable hydrogen isotope composition of archaeal lipids is emerging as a potential paleoenvironmental proxy, adding to the well-established application of plant leaf wax-derived <em>n</em>-alkanes in paleohydrological reconstruction. A handful of studies reported relatively invariant and depleted hydrogen isotope compositions for archaeal lipids despite the range of different organisms and growth conditions explored. However, how modes of metabolism and physiological state (growth phase) affect the hydrogen isotope signatures of archaeal lipids remains poorly understood, limiting our ability to interpret archaeal lipid biomarker records from the environment. Here we conducted water isotope label experiments with a metabolically flexible and well-studied model archaeon <em>Archaeoglobus fulgidus</em> and quantified the hydrogen isotope fractionation between lipids and water in response to different carbon substrates and electron donor–acceptor pairs at different growth phases. The <sup>2</sup>H/<sup>1</sup>H fractionation between lipids and water (ε<sub>L/W</sub>) was overall negative. Both carbon metabolism and growth phase affected the magnitude of isotope fractionation in <em>A. fulgidus</em>; however, the changes in ε<sub>L/W</sub> values were relatively subtle where they ranged from –283 to –229 ‰ across all tested conditions, overlapping with the ranges observed for other archaea in previous studies. Isotope flux-balance model results suggest that ≥ 80 % and ≥ 50 % of lipid-bound H in <em>A. fulgidus</em> cultures directly reflect water isotope compositions (i.e., not via organic substrate or H<sub>2</sub>) during autotrophy and heterotrophy, respectively. The model results also suggest two main mechanisms of consistent <sup>2</sup>H depletion observed in <em>A. fulgidus</em> tetraethers as well as other archaeal lipids reported in previous studies: 1) isotopic re-equilibration via upstream isomerization reactions involving C<sub>5</sub> units and 2) downstream double bond reduction catalyzed by a flavoenzyme geranylgeranyl reductase. These results are consistent with previous isotope flux-balance model results for a different archaeon. Finally, we synthesized available data to compare ε<sub>L/W</sub> patterns across all three domains of life: Eukarya, Archaea and Bacteria. Because they vary fundamentally in lipid biosynthesis pathways, we present comparative discussions in pairs, focusing on the shared biochemical mechanisms among isoprenoid lipids and potential signals of metabolic adaptations across prokaryotic lipids. Emerging patterns between diverse archaeal and eukaryotic isoprenoid lipids are consistent with the two proposed mechanisms for <sup>2</sup>H depletion identified (isomerization and final saturation). The patterns between archaeal isoprenoids and bacterial fatty acids suggest that the general state of energy limitation may also contribute to large, negative values of ε<sub>L/W</sub> observed in prokaryotic lipi","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"386 ","pages":"Pages 196-212"},"PeriodicalIF":4.5,"publicationDate":"2024-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142662968","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-27DOI: 10.1016/j.gca.2024.09.028
Ziyi Zhou , Guangyi Sun , Weiqing Zhou , Jianwei Zhou , Xinbin Feng , Y. Zou Finfrock , Peng Liu
Sorption of antimony (Sb) onto birnessite significantly influences the fate of Sb in oceanic and terrestrial environments and fractionates Sb isotopes. Nevertheless, little is known about Sb isotopic fractionation during its adsorption on birnessite. Here, we show the value of Δ123Sbadsorbed-aqueous increases from −0.398 to −0.332 ‰ in 1 h and then decreases and stabilizes at −0.384 ‰ in 72 h. The enrichment of the light Sb isotope is predominantly due to the distortion of the octahedral symmetry. X-ray absorption spectroscopy results indicate Sb first forms a double-corner-sharing complex on birnessite and then transforms to a double-edge-sharing complex during adsorption. The optimized bond distances for double-corner-sharing (3.37 Å) and double-edge-sharing (2.90 Å) complexes calculated using density functional theory (DFT) fits well with the structure (3.41 and 3.00 Å) revealed by X-ray absorption spectroscopy, respectively. The fractionation derived from reduced partition function ratios calculated using DFT aligns well with the experimental results. Therefore, the variation in Sb isotopic fractionation during adsorption is attributed to the evolving structure of Sb complexes on birnessite. Our results demonstrate the isotopic fractionation of Sb during adsorption on birnessite and provide a molecular-scale understanding of Sb behavior, contributing to the correct reconstruction of the Sb isotope composition of ancient seawater using ferromanganese crusts and nodules, and efforts to trace Sb migration in epigenetic mining environments.
锑(Sb)在白腊石上的吸附作用极大地影响了锑在海洋和陆地环境中的归宿,并使锑的同位素发生分馏。然而,人们对锑在桦锑酸盐吸附过程中的同位素分馏知之甚少。在这里,我们展示了吸附在水体中的Δ123Sb的值在1小时内从-0.398 ‰增加到-0.332 ‰,然后在72小时内降低并稳定在-0.384 ‰。X 射线吸收光谱结果表明,锑首先在比尔奈斯特上形成双角共享复合物,然后在吸附过程中转变为双边共享复合物。用密度泛函理论(DFT)计算出的双角共享复合物(3.37 Å)和双边共享复合物(2.90 Å)的优化键距分别与 X 射线吸收光谱显示的结构(3.41 Å 和 3.00 Å)非常吻合。使用 DFT 计算的还原分配函数比得出的分馏结果与实验结果非常吻合。因此,吸附过程中锑同位素分馏的变化归因于硼锰铁矿上锑络合物结构的演变。我们的研究结果证明了锑在桦锰矿上吸附过程中的同位素分馏,并提供了对锑行为的分子尺度理解,有助于利用铁锰结壳和结核正确重建古海水的锑同位素组成,并努力追踪锑在表生采矿环境中的迁移。
{"title":"Antimony stable isotope fractionation during adsorption onto birnessite: A molecular perspective from X-ray absorption spectroscopy and density functional theory","authors":"Ziyi Zhou , Guangyi Sun , Weiqing Zhou , Jianwei Zhou , Xinbin Feng , Y. Zou Finfrock , Peng Liu","doi":"10.1016/j.gca.2024.09.028","DOIUrl":"10.1016/j.gca.2024.09.028","url":null,"abstract":"<div><div>Sorption of antimony (Sb) onto birnessite significantly influences the fate of Sb in oceanic and terrestrial environments and fractionates Sb isotopes. Nevertheless, little is known about Sb isotopic fractionation during its adsorption on birnessite. Here, we show the value of Δ<sup>123</sup>Sb<sub>adsorbed-aqueous</sub> increases from −0.398 to −0.332 ‰ in 1 h and then decreases and stabilizes at −0.384 ‰ in 72 h. The enrichment of the light Sb isotope is predominantly due to the distortion of the octahedral symmetry. X-ray absorption spectroscopy results indicate Sb first forms a double-corner-sharing complex on birnessite and then transforms to a double-edge-sharing complex during adsorption. The optimized bond distances for double-corner-sharing (3.37 Å) and double-edge-sharing (2.90 Å) complexes calculated using density functional theory (DFT) fits well with the structure (3.41 and 3.00 Å) revealed by X-ray absorption spectroscopy, respectively. The fractionation derived from reduced partition function ratios calculated using DFT aligns well with the experimental results. Therefore, the variation in Sb isotopic fractionation during adsorption is attributed to the evolving structure of Sb complexes on birnessite. Our results demonstrate the isotopic fractionation of Sb during adsorption on birnessite and provide a molecular-scale understanding of Sb behavior, contributing to the correct reconstruction of the Sb isotope composition of ancient seawater using ferromanganese crusts and nodules, and efforts to trace Sb migration in epigenetic mining environments.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"386 ","pages":"Pages 173-184"},"PeriodicalIF":4.5,"publicationDate":"2024-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142662977","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-27DOI: 10.1016/j.gca.2024.09.029
Yingchun Zhang, Xiandong Liu, Xiancai Lu, Rucheng Wang
Deep-sea mud shows tremendous resource potential for rare earth elements (REEs) and its formation is closely associated with sea-floor hydrothermal activities. Iron (oxyhydr)oxides link the sources and sinks of REEs in sea-floor hydrothermal systems. However, the complexation mechanisms of REEs on iron (oxyhydr)oxides have not been well understood yet. In this study, by using the first principles molecular dynamics technique, we first calculated the pKa’s of surface groups on goethite (1 1 0) surface at elevated temperatures relevant to sea-floor hydrothermal systems and then evaluated the complexation structures and free energies of REEs on goethite (1 1 0) and (0 1 0) surfaces using the method of constraint by taking Sc3+, Y3+, and La3+ as model REE cations. The results show that REE complexation occurs in mildly acidic to neutral conditions. The most thermodynamically stable complexes of REEs are bidentate complexes on two neighboring FeOH sites on goethite (1 1 0) surface and tridentate complexes on two neighboring FeOH sites plus one Fe2OH site on goethite (0 1 0) surface. Sc3+ complexes match the goethite lattice and can be incorporated into the lattice. The stabilities of REE complexes increase with the distance from hydrothermal vents. Complexation of Y3+ is less favored on goethite compared to other REEs whereas Sc3+ prefers complexation on goethite (0 1 0) surface and La3+ exhibits similar stabilities on both (0 1 0) and (1 1 0) surfaces. The derived atomic level complexation mechanisms would be helpful for the interpretation of experimental data and the prediction of REEs’ behavior in the sea-floor. The findings presented here provide valuable insights into REEs fractionation and enrichment in deep-sea muds.
{"title":"Surface complexation of rare earth elements on goethite in sea-floor hydrothermal environment: Insight from first principles simulations","authors":"Yingchun Zhang, Xiandong Liu, Xiancai Lu, Rucheng Wang","doi":"10.1016/j.gca.2024.09.029","DOIUrl":"10.1016/j.gca.2024.09.029","url":null,"abstract":"<div><div>Deep-sea mud shows tremendous resource potential for rare earth elements (REEs) and its formation is closely associated with sea-floor hydrothermal activities. Iron (oxyhydr)oxides link the sources and sinks of REEs in sea-floor hydrothermal systems. However, the complexation mechanisms of REEs on iron (oxyhydr)oxides have not been well understood yet. In this study, by using the first principles molecular dynamics technique, we first calculated the pK<sub>a</sub>’s of surface groups on goethite (1<!--> <!-->1<!--> <!-->0) surface at elevated temperatures relevant to sea-floor hydrothermal systems and then evaluated the complexation structures and free energies of REEs on goethite (1<!--> <!-->1<!--> <!-->0) and (0<!--> <!-->1<!--> <!-->0) surfaces using the method of constraint by taking Sc<sup>3+</sup>, Y<sup>3+</sup>, and La<sup>3+</sup> as model REE cations. The results show that REE complexation occurs in mildly acidic to neutral conditions. The most thermodynamically stable complexes of REEs are bidentate complexes on two neighboring <img>FeOH sites on goethite (1<!--> <!-->1<!--> <!-->0) surface and tridentate complexes on two neighboring <img>FeOH sites plus one <img>Fe<sub>2</sub>OH site on goethite (0<!--> <!-->1<!--> <!-->0) surface. Sc<sup>3+</sup> complexes match the goethite lattice and can be incorporated into the lattice. The stabilities of REE complexes increase with the distance from hydrothermal vents. Complexation of Y<sup>3+</sup> is less favored on goethite compared to other REEs whereas Sc<sup>3+</sup> prefers complexation on goethite (0<!--> <!-->1<!--> <!-->0) surface and La<sup>3+</sup> exhibits similar stabilities on both (0<!--> <!-->1<!--> <!-->0) and (1<!--> <!-->1<!--> <!-->0) surfaces. The derived atomic level complexation mechanisms would be helpful for the interpretation of experimental data and the prediction of REEs’ behavior in the sea-floor. The findings presented here provide valuable insights into REEs fractionation and enrichment in deep-sea muds.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"386 ","pages":"Pages 185-195"},"PeriodicalIF":4.5,"publicationDate":"2024-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142662979","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-27DOI: 10.1016/j.gca.2024.09.031
Zheng Qin , Jingao Liu , Huan Cui , Kurt O. Konhauser , He Huang , Dongtao Xu , Yuan Gao , Huaichun Wu , Chengshan Wang
Organic carbon burial in ancient lacustrine settings is a crucial source of petroleum resources. Unlike the marine environment, the dynamics of organic carbon burial in the terrestrial realm are more complex due to the interplay of global and regional climate-tectonic factors. There appears to be a potential linkage between seawater incursion events (SWIEs) and the generation of lacustrine source rocks. However, reliable proxies to reconstruct the frequency and extent of SWIEs are currently lacking. Here, we explore the potential of rhenium-platinum group elements (Re-PGE) system as a novel proxy for determining SWIEs in the Nenjiang Formation of the lacustrine Songliao Basin in China that is noted for its high-quality source rock. By comparing marine and non-marine intervals, we validate the utility of Re-PGE fractionation patterns and osmium (Os) isotope compositions. Moreover, the Re/Ir ratios demonstrate two main episodes of quantitative seawater-lake water exchange. The comparison of variable indicators shows that the Re-PGE system is more sensitive to the changes in water sources, thus providing detailed information of frequency and exchange amount. The inverse variation between seawater contribution and total organic carbon content further implies that the massive sulfate influx from SWIEs facilitated bacterial sulfate reduction in the sediment pile, which had the effect of recycling nutrients (e.g., phosphorous) back into the water column. The SWIEs-triggered eutrophication induced a positive feedback loop between productivity and hypoxia, creating ideal conditions for the preservation of organic carbon. Our data reveals the detailed mechanism of SWIEs-triggered organic carbon burial and emphasizes the significant role of SWIEs in generating economically important hydrocarbon reservoirs.
{"title":"Rhenium-platinum group elements reveal seawater incursion induced massive lacustrine organic carbon burial","authors":"Zheng Qin , Jingao Liu , Huan Cui , Kurt O. Konhauser , He Huang , Dongtao Xu , Yuan Gao , Huaichun Wu , Chengshan Wang","doi":"10.1016/j.gca.2024.09.031","DOIUrl":"10.1016/j.gca.2024.09.031","url":null,"abstract":"<div><div>Organic carbon burial in ancient lacustrine settings is a crucial source of petroleum resources. Unlike the marine environment, the dynamics of organic carbon burial in the terrestrial realm are more complex due to the interplay of global and regional climate-tectonic factors. There appears to be a potential linkage between seawater incursion events (SWIEs) and the generation of lacustrine source rocks. However, reliable proxies to reconstruct the frequency and extent of SWIEs are currently lacking. Here, we explore the potential of rhenium-platinum group elements (Re-PGE) system as a novel proxy for determining SWIEs in the Nenjiang Formation of the lacustrine Songliao Basin in China that is noted for its high-quality source rock. By comparing marine and non-marine intervals, we validate the utility of Re-PGE fractionation patterns and osmium (Os) isotope compositions. Moreover, the Re/Ir ratios demonstrate two main episodes of quantitative seawater-lake water exchange. The comparison of variable indicators shows that the Re-PGE system is more sensitive to the changes in water sources, thus providing detailed information of frequency and exchange amount. The inverse variation between seawater contribution and total organic carbon content further implies that the massive sulfate influx from SWIEs facilitated bacterial sulfate reduction in the sediment pile, which had the effect of recycling nutrients (e.g., phosphorous) back into the water column. The SWIEs-triggered eutrophication induced a positive feedback loop between productivity and hypoxia, creating ideal conditions for the preservation of organic carbon. Our data reveals the detailed mechanism of SWIEs-triggered organic carbon burial and emphasizes the significant role of SWIEs in generating economically important hydrocarbon reservoirs.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"384 ","pages":"Pages 168-177"},"PeriodicalIF":4.5,"publicationDate":"2024-09-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142426520","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-26DOI: 10.1016/j.gca.2024.09.026
Taryn Linzmeyer , James M.D. Day , Raquel Alonso-Perez , Theo Phahla , Anton Wolmarans , Andrew Rogers
<div><div>The ∼ 1.15-billion-year-old (Ga) Premier kimberlite pipe (Cullinan diamond mine), South Africa, is composed of several distinct kimberlite facies (Grey, Brown, Pale Piebald, Dark Piebald, Black Coherent [Type 3C], Blue/Brown Transitional, and Fawn). We report bulk rock Re-Os isotope data for Premier kimberlite facies, as well as for a suite of entrained peridotite and mafic xenoliths. These data are complemented by bulk rock highly siderophile element (HSE: Re, Pd, Pt, Ru, Ir, Os), major- and trace-element abundances. Measured <sup>187</sup>Os/<sup>188</sup>Os for the kimberlite facies range from 0.1223 to 0.1672 (γOs<sub>i</sub> of −2.5 to + 17.4), peridotite xenoliths range from 0.1096 to 0.1244 (γOs<sub>i</sub> of −13.3 to −1.1), and pyroxenite xenoliths range from 0.1796 to 0.938 (γOs<sub>i</sub> of + 27 to + 419). A single measured amphibolite xenolith has the most radiogenic measured <sup>187</sup>Os/<sup>188</sup>Os of 2.86 (γOs<sub>i</sub> of + 43). Harzburgite xenoliths yield time of rhenium depletion model ages (T<sub>RD</sub>) of ∼ 1.5 to 2.8 Ga, consistent with average T<sub>RD</sub> ages for Premier peridotites (2.4 ± 0.4 Ga). With these and published data, we considered the relationships between kimberlite and mantle xenoliths, compare estimates of relative peridotite incorporation to sampled diamond grade, and explore recratonization versus refertilization arguments with regards to T<sub>RD</sub> model ages. Kimberlite melt infiltration into Premier peridotite xenoliths is evident from melt veins accounting for ∼ 2 and ∼ 14 modal % of samples, and has led to incompatible element enrichment, including elevated Re. In turn, kimberlites show geochemical evidence for addition of peridotite xenolith fragments, with Type 3C having > 30 % more peridotite contribution than the Brown volcaniclastic facies. Kimberlites and peridotites plot on a <sup>187</sup>Re/<sup>188</sup>Os versus <sup>187</sup>Os/<sup>188</sup>Os mixing line (R<sup>2</sup> = 0.92), with kimberlites having older apparent ages than the true age of crystallization. This mixing line provides estimates of lithospheric incorporation into the kimberlites, where the units with higher peridotite incorporation do not correlate with diamond grade. This is likely due to lithological and post-emplacement alteration heterogeneity within the kimberlite units, perhaps also reflecting the eclogitic paragenesis of many Premier diamonds. The peridotites provide evidence for the nature of the lithosphere beneath Premier prior to ∼ 1.15 Ga. Metasomatism of the peridotites is possibly linked to the Bushveld Igneous Event at ∼ 2 Ga, as well as to other magmatic events that affected the Kaapvaal craton from the Archean to the Mesoproterozoic. Premier peridotites do not suggest that the cratonic lithosphere beneath the region was completely replaced. Samples with Proterozoic T<sub>RD</sub> eruption model ages may represent Archean lithosphere that experienced alteration by metasoma
{"title":"A 187Re-187Os and highly siderophile element study of diamondiferous kimberlite melt-mantle interactions and the inferred age of continental lithosphere","authors":"Taryn Linzmeyer , James M.D. Day , Raquel Alonso-Perez , Theo Phahla , Anton Wolmarans , Andrew Rogers","doi":"10.1016/j.gca.2024.09.026","DOIUrl":"10.1016/j.gca.2024.09.026","url":null,"abstract":"<div><div>The ∼ 1.15-billion-year-old (Ga) Premier kimberlite pipe (Cullinan diamond mine), South Africa, is composed of several distinct kimberlite facies (Grey, Brown, Pale Piebald, Dark Piebald, Black Coherent [Type 3C], Blue/Brown Transitional, and Fawn). We report bulk rock Re-Os isotope data for Premier kimberlite facies, as well as for a suite of entrained peridotite and mafic xenoliths. These data are complemented by bulk rock highly siderophile element (HSE: Re, Pd, Pt, Ru, Ir, Os), major- and trace-element abundances. Measured <sup>187</sup>Os/<sup>188</sup>Os for the kimberlite facies range from 0.1223 to 0.1672 (γOs<sub>i</sub> of −2.5 to + 17.4), peridotite xenoliths range from 0.1096 to 0.1244 (γOs<sub>i</sub> of −13.3 to −1.1), and pyroxenite xenoliths range from 0.1796 to 0.938 (γOs<sub>i</sub> of + 27 to + 419). A single measured amphibolite xenolith has the most radiogenic measured <sup>187</sup>Os/<sup>188</sup>Os of 2.86 (γOs<sub>i</sub> of + 43). Harzburgite xenoliths yield time of rhenium depletion model ages (T<sub>RD</sub>) of ∼ 1.5 to 2.8 Ga, consistent with average T<sub>RD</sub> ages for Premier peridotites (2.4 ± 0.4 Ga). With these and published data, we considered the relationships between kimberlite and mantle xenoliths, compare estimates of relative peridotite incorporation to sampled diamond grade, and explore recratonization versus refertilization arguments with regards to T<sub>RD</sub> model ages. Kimberlite melt infiltration into Premier peridotite xenoliths is evident from melt veins accounting for ∼ 2 and ∼ 14 modal % of samples, and has led to incompatible element enrichment, including elevated Re. In turn, kimberlites show geochemical evidence for addition of peridotite xenolith fragments, with Type 3C having > 30 % more peridotite contribution than the Brown volcaniclastic facies. Kimberlites and peridotites plot on a <sup>187</sup>Re/<sup>188</sup>Os versus <sup>187</sup>Os/<sup>188</sup>Os mixing line (R<sup>2</sup> = 0.92), with kimberlites having older apparent ages than the true age of crystallization. This mixing line provides estimates of lithospheric incorporation into the kimberlites, where the units with higher peridotite incorporation do not correlate with diamond grade. This is likely due to lithological and post-emplacement alteration heterogeneity within the kimberlite units, perhaps also reflecting the eclogitic paragenesis of many Premier diamonds. The peridotites provide evidence for the nature of the lithosphere beneath Premier prior to ∼ 1.15 Ga. Metasomatism of the peridotites is possibly linked to the Bushveld Igneous Event at ∼ 2 Ga, as well as to other magmatic events that affected the Kaapvaal craton from the Archean to the Mesoproterozoic. Premier peridotites do not suggest that the cratonic lithosphere beneath the region was completely replaced. Samples with Proterozoic T<sub>RD</sub> eruption model ages may represent Archean lithosphere that experienced alteration by metasoma","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"386 ","pages":"Pages 157-172"},"PeriodicalIF":4.5,"publicationDate":"2024-09-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142662976","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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 : 2024-09-21DOI: 10.1016/j.gca.2024.09.023
George D. Cody , Conel M. O’D. Alexander , Dionysis I. Foustoukos , Yoko Kebukawa , Ying Wang
Rotationally resonant Deuterium Nuclear Magnetic Resonance spectroscopy (D MAS NMR) was applied to IOM isolated from a CR1 chondrite Grosvenor Mountains (GRO) 95577 and a CM2 chondrite (Murchison). It is shown that in IOM D strongly prefers the aliphatic hydrogen reservoir over the aromatic hydrogen reservoir. For GRO 95577, that has a bulk δD of 3303 ‰ (Alexander et al., 2010), the average δD value of the aromatic reservoir is 1740 ± 128 ‰ and the aliphatic reservoir is 4477 ± 105 ‰, i.e., D/H enrichments of 1.27 and 0.64, respectively, relative to the bulk. For Murchison IOM, that has a bulk δD of 811 ‰ (Alexander et al., 2010), the average δD of the aromatic reservoir is 512 ± 88 ‰ and the aliphatic reservoir is 1033 ± 64 ‰ i.e., D/H enrichments of 1.12 and 0.82, respectively, relative to the bulk. D-H exchange between D-enriched water and a type III kerogen reveals nearly equivalent D up take by both aromatics and aliphatics. Laboratory synthesis of IOM-like material in the presence of D2O reveals a high degree of deuteration with a strong preferential deuteration of the aliphatic hydrogen reservoir indicating that the δD of the water during IOM synthesis is the primary determinant of syn-IOM’s δD. The IOM in GRO 95577 and Murchison (FA and H/C × 100) lie on the molecular evolution line as defined by the IOM of the Tagish Lake clasts and Murchison IOM has experienced more molecular evolution relative to that exhibited by GRO 95577 IOM. A forward prediction derived from the D/H ratios for the aliphatic and aromatic hydrogen reservoirs in Murchison and GRO 95577, relative to their bulk D/H ratios, derived from D MAS NMR, is applied to explain the origin of the Tagish Lake trend of δD vs molecular evolution (H/C × 100). The results of this forward prediction suggest that the Tagish Lake isotopic trend results from a combination of molecular evolution (loss of predominantly aliphatic H and D) and partial D-H exchange with D depleted chondritic water during a short-term hydrothermal alteration event. Such events may be faithfully identified in chondritic organic solids and be a common occurrence, but not necessarily revealed in the mineralogy of type 1 and 2 carbonaceous chondrites.
旋转共振氘核磁共振波谱(D MAS NMR)被应用于从 CR1 雪岩 Grosvenor Mountains (GRO) 95577 和 CM2 雪岩 Murchison 分离出来的 IOM。结果表明,在 IOM 中,D 强烈偏好脂肪族氢库而不是芳香族氢库。对于体积δD 为 3303 ‰ 的 GRO 95577(Alexander 等人,2010 年),芳香族储氢层的平均δD 值为 1740 ± 128 ‰,脂肪族储氢层为 4477 ± 105 ‰,即相对于体积,D/H 富集度分别为 1.27 和 0.64。对于体积δD 为 811 ‰ 的 Murchison IOM(Alexander 等人,2010 年),芳香族储层的平均δD 为 512 ± 88 ‰,脂肪族储层的平均δD 为 1033 ± 64 ‰,即相对于体积,D/H 富集度分别为 1.12 和 0.82。富集 D 的水与 III 型角质之间的 D-H 交换显示,芳香族和脂肪族对 D 的吸收几乎相等。在 D2O 存在下实验室合成的 IOM 类物质显示出高度的氘化,脂肪族氢库具有强烈的优先氘化,这表明在 IOM 合成过程中水的δD 是决定合成 IOM 的δD 的主要因素。GRO 95577和默奇森的IOM(FA和H/C ×100)位于塔吉什湖碎屑岩IOM所确定的分子演化线上,与GRO 95577 IOM相比,默奇森IOM经历了更多的分子演化。根据 D MAS NMR 得出的 Murchison 和 GRO 95577 脂肪族和芳香族储氢器的 D/H 比值(相对于它们的体积 D/H 比值)进行前瞻性预测,以解释塔吉什湖 δD 与分子演化(H/C ×100)趋势的起源。这一前瞻性预测的结果表明,塔吉什湖的同位素趋势是分子演化(主要是脂肪族 H 和 D 的损失)和在短期热液蚀变事件中与 D 贫化的软玉水进行部分 D-H 交换的综合结果。这类事件可以在软玉有机固体中被忠实地识别出来,并且是一种常见现象,但不一定会在1型和2型碳质软玉的矿物学中被揭示出来。
{"title":"On the origin and evolution of deuterium enrichment in type 1 and 2 chondritic organic solids","authors":"George D. Cody , Conel M. O’D. Alexander , Dionysis I. Foustoukos , Yoko Kebukawa , Ying Wang","doi":"10.1016/j.gca.2024.09.023","DOIUrl":"10.1016/j.gca.2024.09.023","url":null,"abstract":"<div><div>Rotationally resonant Deuterium Nuclear Magnetic Resonance spectroscopy (D MAS NMR) was applied to IOM isolated from a CR1 chondrite Grosvenor Mountains (GRO) 95577 and a CM2 chondrite (Murchison). It is shown that in IOM D strongly prefers the aliphatic hydrogen reservoir over the aromatic hydrogen reservoir. For GRO 95577, that has a bulk δD of 3303 ‰ (Alexander et al., 2010), the average δD value of the aromatic reservoir is 1740 ± 128 ‰ and the aliphatic reservoir is 4477 ± 105 ‰, i.e., D/H enrichments of 1.27 and 0.64, respectively, relative to the bulk. For Murchison IOM, that has a bulk δD of 811 ‰ (Alexander et al., 2010), the average δD of the aromatic reservoir is 512 ± 88 ‰ and the aliphatic reservoir is 1033 ± 64 ‰ i.e., D/H enrichments of 1.12 and 0.82, respectively, relative to the bulk. D-H exchange between D-enriched water and a type III kerogen reveals nearly equivalent D up take by both aromatics and aliphatics. Laboratory synthesis of IOM-like material in the presence of D<sub>2</sub>O reveals a high degree of deuteration with a strong preferential deuteration of the aliphatic hydrogen reservoir indicating that the δD of the water during IOM synthesis is the primary determinant of syn-IOM’s δD. The IOM in GRO 95577 and Murchison (FA and H/C × 100) lie on the molecular evolution line as defined by the IOM of the Tagish Lake clasts and Murchison IOM has experienced more molecular evolution relative to that exhibited by GRO 95577 IOM. A forward prediction derived from the D/H ratios for the aliphatic and aromatic hydrogen reservoirs in Murchison and GRO 95577, relative to their bulk D/H ratios, derived from D MAS NMR, is applied to explain the origin of the Tagish Lake trend of δD vs molecular evolution (H/C × 100). The results of this forward prediction suggest that the Tagish Lake isotopic trend results from a combination of molecular evolution (loss of predominantly aliphatic H and D) and partial D-H exchange with D depleted chondritic water during a short-term hydrothermal alteration event. Such events may be faithfully identified in chondritic organic solids and be a common occurrence, but not necessarily revealed in the mineralogy of type 1 and 2 carbonaceous chondrites.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"386 ","pages":"Pages 139-156"},"PeriodicalIF":4.5,"publicationDate":"2024-09-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142662970","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Marine dissolved organic matter (DOM) is one of the largest reservoirs of organic carbon and nitrogen in the world. Yet, despite its global importance, most DOM remains molecularly uncharacterized. Solid-state nuclear magnetic resonance (NMR) spectroscopy of isolated DOM fractions represents one of the most powerful techniques to understand overall structural composition. However, it is well known that standard cross polarization magic angle spinning (CP/MAS) NMR, the technique used for almost all past solid-state NMR studies of DOM, is at best “semi-quantitative,” and underestimates fully substituted NMR active nuclei. Additionally, almost all past solid-state NMR work analyzed high molecular weight (HMW) material isolated by ultrafiltration, which is now understood to represent mostly 14C-young, “semi-labile” compounds. In contrast, there is far less information regarding the composition of older, low molecular weight (LMW) DOM, which represents the vast majority of the ocean’s accumulated refractory DOM pool.
Here, we applied 13C and 15N solid-state multiCP/MAS NMR, improved NMR methods optimized to more quantitatively resolve fully substituted NMR nuclei, to both HMW and LMW DOM isolated from the surface and deep North Pacific Subtropical Gyre. These methods confirm past work indicating most nitrogen containing HMW DOM as amide compounds, but also demonstrate a modest heterocyclic N component not previously identified. In contrast, we found that LMW DON is almost entirely aromatic heterocyclic N, consistent with the hypothesis that heterocyclic N structures may be largely responsible for the accumulation of the ocean’s refractory DON pool. Surprisingly, however, we find DOC aromatic functionalities still represent only a very minor portion of either the HMW or the LMW refractory carbon pools, in marked contrast to refractory DON composition. Together, these more quantitative solid-state NMR techniques likely represent the most accurate picture of DON and DOC functional and compound-class makeup to date, and so have broad implications for our understanding of marine DOM structure and cycling. Specifically, our new data suggests that while chemical composition likely acts as a key control on DOM lability, the most refractory components of DOC and DON have very different compositions, sources, and cycling, supporting the idea that DOC and DON cycling in the ocean may be largely decoupled.
海洋溶解有机物(DOM)是世界上最大的有机碳和氮库之一。然而,尽管海洋溶解有机物在全球具有重要意义,但大多数海洋溶解有机物仍未得到分子表征。对分离的 DOM 部分进行固态核磁共振(NMR)光谱分析是了解整体结构组成的最强大技术之一。然而,众所周知,标准交叉偏振魔角旋光(CP/MAS)核磁共振(过去几乎所有 DOM 固体核磁共振研究都采用这种技术)充其量只是 "半定量",而且低估了完全取代的核磁共振活性核。此外,过去几乎所有的固态 NMR 研究都是分析通过超滤分离出来的高分子量(HMW)物质,而现在的理解是,这种物质主要代表 14C 年轻的 "半易变 "化合物。在这里,我们将 13C 和 15N 固态多CP/MAS NMR(经过优化的改进 NMR 方法)应用于从北太平洋亚热带环流表层和深层分离出来的 HMW 和 LMW DOM。这些方法证实了过去的工作,表明大多数含氮的 HMW DOM 都是酰胺化合物,但也证明了以前未发现的少量杂环 N 成分。相比之下,我们发现低分子量 DON 几乎完全是芳香杂环氮,这与杂环氮结构可能在很大程度上导致海洋难溶性 DON 池积累的假设一致。然而,令人惊讶的是,我们发现 DOC 芳香族官能团在高分子量或低分子量难溶碳库中仍然只占很小的一部分,这与难溶 DON 的组成形成了明显的对比。总之,这些更定量的固态核磁共振技术很可能代表了迄今为止最准确的 DON 和 DOC 功能及化合物类别构成图谱,因此对我们了解海洋 DOM 结构和循环具有广泛的意义。具体来说,我们的新数据表明,虽然化学成分可能是 DOM 易变性的关键控制因素,但 DOC 和 DON 中最难分解的成分在组成、来源和循环方面存在很大差异,这支持了一种观点,即海洋中 DOC 和 DON 的循环可能在很大程度上是脱钩的。
{"title":"Improved solid-state 13C and 15N NMR reveals fundamental compositional divide between refractory dissolved organic carbon and nitrogen in the sea","authors":"H.L. Ianiri , H.E. Mason , T.A.B. Broek , M.D. McCarthy","doi":"10.1016/j.gca.2024.09.022","DOIUrl":"10.1016/j.gca.2024.09.022","url":null,"abstract":"<div><div>Marine dissolved organic matter (DOM) is one of the largest reservoirs of organic carbon and nitrogen in the world. Yet, despite its global importance, most DOM remains molecularly uncharacterized. Solid-state nuclear magnetic resonance (NMR) spectroscopy of isolated DOM fractions represents one of the most powerful techniques to understand overall structural composition. However, it is well known that standard cross polarization magic angle spinning (CP/MAS) NMR, the technique used for almost all past solid-state NMR studies of DOM, is at best “semi-quantitative,” and underestimates fully substituted NMR active nuclei. Additionally, almost all past solid-state NMR work analyzed high molecular weight (HMW) material isolated by ultrafiltration, which is now understood to represent mostly <sup>14</sup>C-young, “semi-labile” compounds. In contrast, there is far less information regarding the composition of older, low molecular weight (LMW) DOM, which represents the vast majority of the ocean’s accumulated refractory DOM pool.</div><div>Here, we applied <sup>13</sup>C and <sup>15</sup>N solid-state multiCP/MAS NMR, improved NMR methods optimized to more quantitatively resolve fully substituted NMR nuclei, to both HMW and LMW DOM isolated from the surface and deep North Pacific Subtropical Gyre. These methods confirm past work indicating most nitrogen containing HMW DOM as amide compounds, but also demonstrate a modest heterocyclic N component not previously identified. In contrast, we found that LMW DON is almost entirely aromatic heterocyclic N, consistent with the hypothesis that heterocyclic N structures may be largely responsible for the accumulation of the ocean’s refractory DON pool. Surprisingly, however, we find DOC aromatic functionalities still represent only a very minor portion of either the HMW or the LMW refractory carbon pools, in marked contrast to refractory DON composition. Together, these more quantitative solid-state NMR techniques likely represent the most accurate picture of DON and DOC functional and compound-class makeup to date, and so have broad implications for our understanding of marine DOM structure and cycling. Specifically, our new data suggests that while chemical composition likely acts as a key control on DOM lability, the most refractory components of DOC and DON have very different compositions, sources, and cycling, supporting the idea that DOC and DON cycling in the ocean may be largely decoupled.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"384 ","pages":"Pages 155-167"},"PeriodicalIF":4.5,"publicationDate":"2024-09-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142319754","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}