Pub Date : 2024-10-01DOI: 10.1016/j.lithos.2024.107826
Ben-Xun Su , Shi-Ying Wang , Jing Wang , Hong-Rui Fan
Mantle-derived carbonatites are an important type of igneous carbonate rock found in diverse tectonic settings. They are commonly associated with alkaline rocks and can contain various mineralization. In contrast, crustal-derived carbonatites form from the direct melting of limestones or marbles at depths within the Earth's crust. These crustal-derived carbonatites are exclusively found in orogenic belts, alongside metamorphic silicate rocks and marbles, and generally do not develop mineralization. Both types of carbonatites exhibit distinct differences in their sources, as well as their elemental and isotopic geochemistry. They can be classified as ortho‑carbonatite (mantle-derived) and para‑carbonatite (crustal-derived). The radiogenic SrNd isotope compositions of both types of carbonatites, along with additional stable CO isotopes and radiogenic Hf isotopes in para‑carbonatites, show correlations with geological time. These temporal variations could provide valuable insights into the Earth's evolutionary history.
源自地幔的碳酸盐岩是一种重要的火成碳酸盐岩,存在于不同的构造环境中。它们通常与碱性岩石伴生,并可能含有各种矿化物。相比之下,地壳源碳酸盐岩是由地壳深处的石灰岩或大理岩直接熔化形成的。这些源于地壳的碳酸岩只出现在造山带,与变质硅酸盐岩和大理岩相伴,一般不会形成矿化物。这两种类型的碳酸盐岩在来源以及元素和同位素地球化学方面都有明显差异。它们可分为正碳酸盐岩(源于地幔)和副碳酸盐岩(源于地壳)。这两类碳酸盐岩的放射性 SrNd 同位素组成,以及副碳酸盐岩中额外的稳定 CO 同位素和放射性 Hf 同位素,都显示出与地质年代的相关性。这些时间上的变化可以为了解地球的演化历史提供有价值的信息。
{"title":"Crustal-derived versus mantle-derived carbonatites","authors":"Ben-Xun Su , Shi-Ying Wang , Jing Wang , Hong-Rui Fan","doi":"10.1016/j.lithos.2024.107826","DOIUrl":"10.1016/j.lithos.2024.107826","url":null,"abstract":"<div><div>Mantle-derived carbonatites are an important type of igneous carbonate rock found in diverse tectonic settings. They are commonly associated with alkaline rocks and can contain various mineralization. In contrast, crustal-derived carbonatites form from the direct melting of limestones or marbles at depths within the Earth's crust. These crustal-derived carbonatites are exclusively found in orogenic belts, alongside metamorphic silicate rocks and marbles, and generally do not develop mineralization. Both types of carbonatites exhibit distinct differences in their sources, as well as their elemental and isotopic geochemistry. They can be classified as ortho‑carbonatite (mantle-derived) and para‑carbonatite (crustal-derived). The radiogenic Sr<img>Nd isotope compositions of both types of carbonatites, along with additional stable C<img>O isotopes and radiogenic Hf isotopes in para‑carbonatites, show correlations with geological time. These temporal variations could provide valuable insights into the Earth's evolutionary history.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107826"},"PeriodicalIF":2.9,"publicationDate":"2024-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142428469","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-10-01DOI: 10.1016/j.lithos.2024.107824
Freya R. George , Daniel R. Viete , George L. Guice , Kayleigh M. Harvey , Stephanie Walker , Ethan F. Baxter
Metapelitic assemblages are often considered highly reactive during prograde metamorphism, such that they effectively record a history of tectono-metamorphic processes. Across eastern North America, metamorphosed rift-to-drift stratigraphy has been central to disentangling the terminal history of Appalachian convergence. We report results from a single metapelitic outcrop in the Loch Raven Schist of Maryland's Baltimore Terrane, where regional metamorphism is historically interpreted to have derived only from the Ordovician Taconic orogeny. An aluminum-rich litho-horizon alludes to two phases of metamorphism: an early, low/medium-pressure (P) sillimanite-stabilizing phase largely overprinted by a subsequent medium/high-P kyanite-stabilizing event, terminating at c. 391–383 Ma. This provides evidence of substantial crustal disturbances in the central Appalachians during Avalonian collision of comparable timing to equivalent events in the north. In a subordinate and aluminum-poor litho-horizon, large (2–3.5 cm) garnet provides geochronological evidence only for a protracted phase of metamorphism at 440–424 Ma. We interpret this age as recording the early, low/medium-P phase of metamorphism that either: (a) extends the duration of the Taconic event; or (b) provides new evidence for metamorphism associated with Silurian tectonism and/or extension in the Central Appalachians. However, this assemblage appears to have been metamorphically unresponsive during Devonian overprinting, despite peak metamorphic conditions of ∼670 °C and ∼8 kbar. We suggest that a potential combination of the paucity of fluid, limited strain accumulation, and coarse refractive assemblages stabilized a kinetically sluggish and metastable composition.
变质岩集合体通常被认为在顺层变质过程中具有高度反应性,因此它们有效地记录了构造变质过程的历史。在整个北美东部,变质的裂谷-漂移地层对于厘清阿巴拉契亚汇聚的末期历史至关重要。我们报告了马里兰州巴尔的摩地层中 Loch Raven 片岩的一个变质露头的研究结果,根据历史解释,该地区的变质作用仅来自奥陶纪的塔科尼克造山运动。富铝岩性地层暗示了变质作用的两个阶段:早期的低/中压(P)矽线石稳定阶段在很大程度上被随后的中/高-P奇安岩稳定事件所覆盖,大约在 391-383 Ma 时结束。这提供了阿瓦隆碰撞期间阿巴拉契亚山脉中部地壳剧烈扰动的证据,其时间与北部的同等事件相当。在一个从属的贫铝岩层中,大块(2-3.5 厘米)石榴石仅为 440-424 Ma 的漫长变质阶段提供了地质年代证据。我们将这一年龄解释为记录了变质作用的早期、低/中P阶段,该阶段要么:(a)延长了塔科尼克事件的持续时间;要么(b)为与志留纪构造作用和/或阿巴拉契亚山脉中部延伸有关的变质作用提供了新的证据。然而,尽管峰值变质条件为 ∼670 °C和 ∼8 kbar,但在泥盆纪叠印期间,该组合似乎对变质没有反应。我们认为,流体稀少、有限的应变积累以及粗折射组合的潜在组合稳定了动力学上缓慢和易变的成分。
{"title":"Polymetamorphism and metastability in Paleozoic schists of the central Appalachian Baltimore Terrane, USA","authors":"Freya R. George , Daniel R. Viete , George L. Guice , Kayleigh M. Harvey , Stephanie Walker , Ethan F. Baxter","doi":"10.1016/j.lithos.2024.107824","DOIUrl":"10.1016/j.lithos.2024.107824","url":null,"abstract":"<div><div>Metapelitic assemblages are often considered highly reactive during prograde metamorphism, such that they effectively record a history of tectono-metamorphic processes. Across eastern North America, metamorphosed rift-to-drift stratigraphy has been central to disentangling the terminal history of Appalachian convergence. We report results from a single metapelitic outcrop in the Loch Raven Schist of Maryland's Baltimore Terrane, where regional metamorphism is historically interpreted to have derived only from the Ordovician Taconic orogeny. An aluminum-rich litho-horizon alludes to two phases of metamorphism: an early, low/medium-pressure (<em>P</em>) sillimanite-stabilizing phase largely overprinted by a subsequent medium/high-<em>P</em> kyanite-stabilizing event, terminating at c. 391–383 Ma. This provides evidence of substantial crustal disturbances in the central Appalachians during Avalonian collision of comparable timing to equivalent events in the north. In a subordinate and aluminum-poor litho-horizon, large (2–3.5 cm) garnet provides geochronological evidence only for a protracted phase of metamorphism at 440–424 Ma. We interpret this age as recording the early, low/medium-<em>P</em> phase of metamorphism that either: (a) extends the duration of the Taconic event; or (b) provides new evidence for metamorphism associated with Silurian tectonism and/or extension in the Central Appalachians. However, this assemblage appears to have been metamorphically unresponsive during Devonian overprinting, despite peak metamorphic conditions of ∼670 °C and ∼8 kbar. We suggest that a potential combination of the paucity of fluid, limited strain accumulation, and coarse refractive assemblages stabilized a kinetically sluggish and metastable composition.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107824"},"PeriodicalIF":2.9,"publicationDate":"2024-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142427783","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-29DOI: 10.1016/j.lithos.2024.107818
Douglas R. MacLeod, David R.M. Pattison
Synorogenic exhumation is important for understanding the evolution of mountain belts but is often difficult to discern because traditional thermochronology methods mostly date the final stages of exhumation. Intrusions emplaced during orogenesis provide an alternate method to elucidate these exhumation patterns since they preserve the timing and depth of their emplacement. We apply this concept the southern Omineca belt of the Canadian Cordillera by combining new and existing zircon UPb and mica Ar/Ar ages from 43 intrusions as well as new and existing estimates of emplacement depth from 23 contact aureoles. Seventeen new zircon UPb laser ablation inductively coupled plasma mass spectrometry results are presented in the paper, spanning the existing range of previous ages for four episodes of Phanerozoic magmatism in this region: Middle Jurassic (174–154 Ma), mid-Cretaceous (118–95 Ma), Late Cretaceous (78–76 Ma), and Paleocene (66–60 Ma). This new work has resolved two new distinct periods of Cretaceous magmatism at ∼100 and ∼ 76 Ma compared to what was previously considered to be a single mid-Cretaceous event (Bayonne magmatic suite). Furthermore, the Fry Creek batholith, previously considered to be emblematic of the Bayonne suite, the adjacent Shoreline stock, the ∼60 Ma Nelson stock located 40 km to the southwest, and the 55–62 Ma Ladybird magmatic suite form part of a newly identified phase of 66–55 Ma Paleocene magmatism in the region. Compiled intrusion ages were then combined with estimates of emplacement depth determined from metamorphic mineral assemblages in contact aureoles developed in pelitic host rocks. Jurassic intrusions typically have higher pressure staurolite + andalusite-bearing contact aureoles (3.3–4.0 kbar) corresponding to depths of 12.5–15 km, whereas Cretaceous and Paleocene intrusions mainly have lower pressure andalusite + cordierite-bearing contact aureoles (2.3–2.9 kbar) corresponding to depths of 8.5–11 km. These data indicate regional exhumation of 2–6 km occurred between the Middle Jurassic (180–160 Ma) and mid-Cretaceous to Paleocene (120–60 Ma) periods of Cordilleran orogenesis. In contrast, pluton emplacement depths changed by <2 km, suggesting minimal exhumation occurred in the southern Canadian Cordillera between the mid-Cretaceous and Paleocene. This extended lull in exhumation may be related to the partitioning of compressional deformation east into the foreland along a basal decollement beneath the study area during this time.
同步成因的掘起对了解山带的演化非常重要,但由于传统的热时学方法大多对掘起的最后阶段进行测年,因此往往难以辨别。造山过程中喷出的侵入体保留了喷出的时间和深度,因此为阐明这些喷出模式提供了另一种方法。我们将这一概念应用于加拿大科迪勒拉山系南奥明卡带,将43个侵入体中新的和已有的锆石UPb和云母Ar/Ar年龄,以及23个接触金星中新的和已有的喷出深度估算结合起来。文中介绍了 17 项新的锆石 UPb 激光烧蚀电感耦合等离子体质谱分析结果,这些结果跨越了该地区新生代岩浆活动四个阶段的现有年龄范围:中侏罗世(174-154 Ma)、中白垩世(118-95 Ma)、晚白垩世(78-76 Ma)和古新世(66-60 Ma)。与之前认为的白垩纪中期的单一岩浆活动(巴约讷岩浆套)相比,这项新研究发现了白垩纪岩浆活动的两个新的不同时期,分别为 100 ∼ 100 Ma 和 76 Ma。此外,先前被认为是巴约讷岩浆岩组代表的弗莱溪浴成岩、邻近的海岸线岩浆、位于西南 40 公里处的∼60 Ma 纳尔逊岩浆以及 55-62 Ma 瓢虫岩浆岩组构成了该地区新发现的 66-55 Ma 古新世岩浆活动阶段的一部分。然后,将编译的侵入体年龄与根据辉绿岩母岩中发育的接触金星的变质矿物组合确定的置入深度估算值相结合。侏罗纪的侵入体通常具有较高压力的白云石+含安山岩的接触孔(3.3-4.0千巴),深度为12.5-15千米,而白垩纪和古新世的侵入体主要具有较低压力的安山岩+含堇青石的接触孔(2.3-2.9千巴),深度为8.5-11千米。这些数据表明,在科迪勒拉造山运动的中侏罗世(180-160Ma)和中白垩世至古新世(120-60Ma)期间,发生了2-6千米的区域隆升。与此相反,岩浆喷发深度变化了2千米,这表明在中白垩世到古新世之间,加拿大科迪勒拉山系南部发生的掘起活动微乎其微。这种长时间的隆升可能与这一时期压缩变形沿研究区下方的基底解理向东进入前陆有关。
{"title":"Age and emplacement depth of intrusions in the southeastern Canadian Cordillera: Implications for Jurassic to Paleocene exhumation","authors":"Douglas R. MacLeod, David R.M. Pattison","doi":"10.1016/j.lithos.2024.107818","DOIUrl":"10.1016/j.lithos.2024.107818","url":null,"abstract":"<div><div>Synorogenic exhumation is important for understanding the evolution of mountain belts but is often difficult to discern because traditional thermochronology methods mostly date the final stages of exhumation. Intrusions emplaced during orogenesis provide an alternate method to elucidate these exhumation patterns since they preserve the timing and depth of their emplacement. We apply this concept the southern Omineca belt of the Canadian Cordillera by combining new and existing zircon U<img>Pb and mica Ar/Ar ages from 43 intrusions as well as new and existing estimates of emplacement depth from 23 contact aureoles. Seventeen new zircon U<img>Pb laser ablation inductively coupled plasma mass spectrometry results are presented in the paper, spanning the existing range of previous ages for four episodes of Phanerozoic magmatism in this region: Middle Jurassic (174–154 Ma), mid-Cretaceous (118–95 Ma), Late Cretaceous (78–76 Ma), and Paleocene (66–60 Ma). This new work has resolved two new distinct periods of Cretaceous magmatism at ∼100 and ∼ 76 Ma compared to what was previously considered to be a single mid-Cretaceous event (Bayonne magmatic suite). Furthermore, the Fry Creek batholith, previously considered to be emblematic of the Bayonne suite, the adjacent Shoreline stock, the ∼60 Ma Nelson stock located 40 km to the southwest, and the 55–62 Ma Ladybird magmatic suite form part of a newly identified phase of 66–55 Ma Paleocene magmatism in the region. Compiled intrusion ages were then combined with estimates of emplacement depth determined from metamorphic mineral assemblages in contact aureoles developed in pelitic host rocks. Jurassic intrusions typically have higher pressure staurolite + andalusite-bearing contact aureoles (3.3–4.0 kbar) corresponding to depths of 12.5–15 km, whereas Cretaceous and Paleocene intrusions mainly have lower pressure andalusite + cordierite-bearing contact aureoles (2.3–2.9 kbar) corresponding to depths of 8.5–11 km. These data indicate regional exhumation of 2–6 km occurred between the Middle Jurassic (180–160 Ma) and mid-Cretaceous to Paleocene (120–60 Ma) periods of Cordilleran orogenesis. In contrast, pluton emplacement depths changed by <2 km, suggesting minimal exhumation occurred in the southern Canadian Cordillera between the mid-Cretaceous and Paleocene. This extended lull in exhumation may be related to the partitioning of compressional deformation east into the foreland along a basal decollement beneath the study area during this time.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107818"},"PeriodicalIF":2.9,"publicationDate":"2024-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142536321","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-28DOI: 10.1016/j.lithos.2024.107820
Miguel Roquet , Erwin Schettino , Marc Campeny , José María González-Jiménez , Michel Grégoire , Rubén Piña , Mathieu Leisen , Joaquín A. Proenza , Oscar Laurent , Llorenç Planagumà , Xavier Llovet
Spinel lherzolite xenoliths from the Sant Corneli volcano (Catalan Volcanic Zone, NE Spain) carry the geochemical imprint of melt/rock reaction events that have affected the subcontinental lithospheric mantle (SCLM) beneath the northeastern Iberian margin. Trace element signatures of clinopyroxene indicate that this volume of the SCLM initially experienced low degrees (F = 8 %) of partial melting, followed by extensive refertilization by alkaline silicate melts undergoing chromatographic fractionation while percolating through the mantle peridotites. Furthermore, the presence of interstitial sulphide-bearing silicate glass, as well as secondary coronitic rims around mantle minerals, records the melt/rock reaction product associated with the infiltration of the host alkaline basalts while erupting to the surface. Abundant irregular/blocky sulphides located within the interstitial glass patches are comprised of myrmekitic intergrowths of pentlandite ± bornite ± chalcopyrite, suggesting their derivation from immiscible droplets of Fe-Ni-Cu sulphide melt transported by the host alkaline basalts. The variable chondrite-normalized platinum-group element (PGE) systematics and chalcogenes (Se, Te, As, Bi and Sb) abundances of these sulphides track two distinct transport mechanisms for their parental sulphide melts: 1) by unmixing of Ni-Cu-rich sulphide liquid in alkaline basalts attaining sulphide-saturation while interacting with the peridotite xenoliths, and 2) by mechanical transport of immiscible droplets of Ni-Cu-rich sulphide liquid originally extracted by residual monosulphide solid solution undergoing incongruent melting in their mantle source. In addition, many sulphides have PGE abundances that cannot be explained solely by solid-melt chemical partition coefficients but that were likely influenced by the mechanical entrapment, or early-magmatic segregation, of pre-existing PGE-rich nanoparticles or nanomelts. The geochemical signal of these mineral nanoparticles may significantly influence sulphides PGE distribution, sometimes resulting in pronounced positive anomalies in IrRh, Au, or RuRh, along with negative anomalies in Pt.
{"title":"PGE-Ni-Cu sulphide segregation by interaction of basaltic melt and peridotite xenoliths of the Catalan Volcanic Zone (Spain)","authors":"Miguel Roquet , Erwin Schettino , Marc Campeny , José María González-Jiménez , Michel Grégoire , Rubén Piña , Mathieu Leisen , Joaquín A. Proenza , Oscar Laurent , Llorenç Planagumà , Xavier Llovet","doi":"10.1016/j.lithos.2024.107820","DOIUrl":"10.1016/j.lithos.2024.107820","url":null,"abstract":"<div><div>Spinel lherzolite xenoliths from the Sant Corneli volcano (Catalan Volcanic Zone, NE Spain) carry the geochemical imprint of melt/rock reaction events that have affected the subcontinental lithospheric mantle (SCLM) beneath the northeastern Iberian margin. Trace element signatures of clinopyroxene indicate that this volume of the SCLM initially experienced low degrees (<em>F</em> = 8 %) of partial melting, followed by extensive refertilization by alkaline silicate melts undergoing chromatographic fractionation while percolating through the mantle peridotites. Furthermore, the presence of interstitial sulphide-bearing silicate glass, as well as secondary coronitic rims around mantle minerals, records the melt/rock reaction product associated with the infiltration of the host alkaline basalts while erupting to the surface. Abundant irregular/blocky sulphides located within the interstitial glass patches are comprised of myrmekitic intergrowths of pentlandite ± bornite ± chalcopyrite, suggesting their derivation from immiscible droplets of Fe-Ni-Cu sulphide melt transported by the host alkaline basalts. The variable chondrite-normalized platinum-group element (PGE) systematics and chalcogenes (Se, Te, As, Bi and Sb) abundances of these sulphides track two distinct transport mechanisms for their parental sulphide melts: 1) by unmixing of Ni-Cu-rich sulphide liquid in alkaline basalts attaining sulphide-saturation while interacting with the peridotite xenoliths, and 2) by mechanical transport of immiscible droplets of Ni-Cu-rich sulphide liquid originally extracted by residual monosulphide solid solution undergoing incongruent melting in their mantle source. In addition, many sulphides have PGE abundances that cannot be explained solely by solid-melt chemical partition coefficients but that were likely influenced by the mechanical entrapment, or early-magmatic segregation, of pre-existing PGE-rich nanoparticles or nanomelts. The geochemical signal of these mineral nanoparticles may significantly influence sulphides PGE distribution, sometimes resulting in pronounced positive anomalies in Ir<img>Rh, Au, or Ru<img>Rh, along with negative anomalies in Pt.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107820"},"PeriodicalIF":2.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142427794","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-28DOI: 10.1016/j.lithos.2024.107822
Daniel da Rosa Madruga , Marcus Vinicius Dorneles Remus , Guilherme Sonntag Hoerlle , Ariela Oliveira Mazoz , Cristiano de Carvalho Lana , Norberto Dani
Titanite is a valuable tool for studying polymetamorphism and understanding the evolution of orogenic belts as it potentially records different stages of metamorphic evolution. The combination of geochronology and Zr-in-titanite geothermometry has been widely used in petrochronology studies. However, there is ongoing debate regarding the significance of ages and temperatures obtained from titanite. Here, we conducted the first integrated titanite, zircon, and apatite UPb study, along with Zr-in-titanite geothermometry, on calc-silicate rocks from a polymetamorphic complex of the central Dom Feliciano Belt (Western Gondwana). Our aim was to investigate the impact of various metamorphic events on titanite grains. We carried out a geochronological, geochemical, and petrographic analysis of a calc-silicate sequence of the Passo Feio Complex, which was intruded by the Caçapava do Sul Granitic Complex (CSGC). The metamorphic complex experienced regional, contact, and hydrothermal metamorphism during the Neoproterozoic, but the ages and conditions of these metamorphic events remain widely debated. UPb analyses on over one hundred titanite grains from a K-feldspar-diopside schist revealed three distinct titanite populations. The older group, dated at 639 ± 3/7 Ma (2s; n = 19), was associated with the regional metamorphism event (M1), likely initiated by the primary collision of the Dom Feliciano Belt. The intermediate group exhibited an age of 596 ± 1/6 Ma (2s; n = 91). Given the presence of high-K magmatism and a carbonatite intrusion in the study area, producing zircon UPb ages around 600 Ma, this group was associated with contact metamorphism (M2), belike influenced by these intrusive igneous activities. The youngest titanite population showed an age of 566 ± 3/6 Ma (2s; n = 6), which closely aligns, within analytical error, with the age of 561 ± 1/6 Ma (2s; n = 46) obtained from UPb dating on apatite sourced from a diopside-phlogopite schist. The younger ages observed in both titanite and apatite are attributed to alterations resulting from interactions with hydrothermal fluids (M3) during the cooling phase of the CSGC. Chemical analyses conducted with an electron microprobe assessed the Zr concentrations in fifty titanite grains, examining both bright and dark zones observed in back-scattered electron images. The lowest temperature recorded among the 50 grains was 629 °C, which corresponds to dark BSE zones. In the light zones, the minimum temperature was 639 °C. While temperatures estimated using the Zr content in titanite may not correspond precisely with UPb ages, combining titanite ages with those from other accessory minerals like zircon and apatite, along with microstructural analysis, can provide a more comprehensive understanding of orogenic belt evolution.
榍石是研究多变质作用和了解造山带演化的重要工具,因为它可能记录变质演化的不同阶段。在岩石年代学研究中,地球年代学与钛铁矿中锆元素地热测定法的结合得到了广泛应用。然而,关于从榍石中获得的年龄和温度的意义一直存在争议。在这里,我们首次对来自Dom Feliciano带(西冈瓦纳)中部多变质复合体的钙硅酸盐岩进行了榍石、锆石和磷灰石UPb综合研究以及钛铁矿中Zr地温测定法。我们的目的是研究各种变质事件对榍石晶粒的影响。我们对被南卡萨帕瓦花岗岩群(CSGC)侵入的 Passo Feio 复合体的钙硅酸盐序列进行了地质年代、地球化学和岩石学分析。该变质复合体在新近纪经历了区域变质、接触变质和热液变质,但这些变质事件的年龄和条件仍存在广泛争议。对来自K-长石-透辉石片岩的一百多颗榍石晶粒进行的UPb分析表明,榍石有三个不同的族群。年代较早的一组为 639 ± 3/7 Ma (2s; n = 19),与区域变质事件(M1)有关,可能是由 Dom Feliciano 带的初级碰撞引发的。中间组的年龄为 596 ± 1/6 Ma(2s;n = 91)。鉴于研究区域存在高K岩浆活动和碳酸盐岩侵入,产生了约600 Ma的锆石UPb年龄,该组与接触变质作用(M2)有关,可能受到这些侵入火成岩活动的影响。最年轻的榍石群显示的年龄为 566 ± 3/6 Ma (2s; n = 6),在分析误差范围内,与来自透辉石片岩的磷灰石的 UPb 年龄 561 ± 1/6 Ma (2s; n = 46) 非常接近。在榍石和磷灰石中观察到的较年轻的年龄归因于在CSGC冷却阶段与热液(M3)相互作用所产生的变化。利用电子显微镜进行的化学分析评估了 50 个榍石晶粒中的锆浓度,检查了在背散射电子图像中观察到的亮区和暗区。在这 50 个晶粒中,记录到的最低温度为 629 °C,与 BSE 暗区相对应。在亮区,最低温度为 639 ℃。虽然利用榍石中的锆含量估算的温度可能与 UPb 年龄不完全一致,但将榍石年龄与锆石和磷灰石等其他附属矿物的年龄结合起来,再加上微结构分析,可以更全面地了解造山带的演化。
{"title":"Unraveling the polymetamorphism of calc-silicate rocks from 639 to 561 Ma in the Western Gondwana (Passo Feio Complex, Dom Feliciano Belt, South Brazil) based on U-Pb dating in titanite, apatite and zircon","authors":"Daniel da Rosa Madruga , Marcus Vinicius Dorneles Remus , Guilherme Sonntag Hoerlle , Ariela Oliveira Mazoz , Cristiano de Carvalho Lana , Norberto Dani","doi":"10.1016/j.lithos.2024.107822","DOIUrl":"10.1016/j.lithos.2024.107822","url":null,"abstract":"<div><div>Titanite is a valuable tool for studying polymetamorphism and understanding the evolution of orogenic belts as it potentially records different stages of metamorphic evolution. The combination of geochronology and Zr-in-titanite geothermometry has been widely used in petrochronology studies. However, there is ongoing debate regarding the significance of ages and temperatures obtained from titanite. Here, we conducted the first integrated titanite, zircon, and apatite U<img>Pb study, along with Zr-in-titanite geothermometry, on calc-silicate rocks from a polymetamorphic complex of the central Dom Feliciano Belt (Western Gondwana). Our aim was to investigate the impact of various metamorphic events on titanite grains. We carried out a geochronological, geochemical, and petrographic analysis of a calc-silicate sequence of the Passo Feio Complex, which was intruded by the Caçapava do Sul Granitic Complex (CSGC). The metamorphic complex experienced regional, contact, and hydrothermal metamorphism during the Neoproterozoic, but the ages and conditions of these metamorphic events remain widely debated. U<img>Pb analyses on over one hundred titanite grains from a K-feldspar-diopside schist revealed three distinct titanite populations. The older group, dated at 639 ± 3/7 Ma (2s; <em>n</em> = 19), was associated with the regional metamorphism event (M<sub>1</sub>), likely initiated by the primary collision of the Dom Feliciano Belt. The intermediate group exhibited an age of 596 ± 1/6 Ma (2s; <em>n</em> = 91). Given the presence of high-K magmatism and a carbonatite intrusion in the study area, producing zircon U<img>Pb ages around 600 Ma, this group was associated with contact metamorphism (M<sub>2</sub>), belike influenced by these intrusive igneous activities. The youngest titanite population showed an age of 566 ± 3/6 Ma (2s; <em>n</em> = 6), which closely aligns, within analytical error, with the age of 561 ± 1/6 Ma (2s; <em>n</em> = 46) obtained from U<img>Pb dating on apatite sourced from a diopside-phlogopite schist. The younger ages observed in both titanite and apatite are attributed to alterations resulting from interactions with hydrothermal fluids (M<sub>3</sub>) during the cooling phase of the CSGC. Chemical analyses conducted with an electron microprobe assessed the Zr concentrations in fifty titanite grains, examining both bright and dark zones observed in back-scattered electron images. The lowest temperature recorded among the 50 grains was 629 °C, which corresponds to dark BSE zones. In the light zones, the minimum temperature was 639 °C. While temperatures estimated using the Zr content in titanite may not correspond precisely with U<img>Pb ages, combining titanite ages with those from other accessory minerals like zircon and apatite, along with microstructural analysis, can provide a more comprehensive understanding of orogenic belt evolution.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107822"},"PeriodicalIF":2.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142428474","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-28DOI: 10.1016/j.lithos.2024.107823
Guangyou Zhu , Zhiyong Chen , Weiyan Chen , Lei Yan , Kun Zhao , Huichuan Liu
<div><div>The Ediacaran igneous rocks and sedimentary sequences play a key role for our understanding the transition from dispersing of the Rodinian continents to the assemblage of the Gondwana. On the other hand, some continental massifs at the marginal area of the Rodinia and Gondwana could preserve solid evidences for deciphering the geodynamic background from the break-up of Rodinia to the assemblage of Gondwana. In this contribution, we report field observations, petrography, ages and systematic geochemistry of the diverse Ediacaran igneous activities in the northern margin of the Tarim Block, which was favored as a marginal continental massif in the Rodinia configuration by most geologists. The Ediacaran igneous rocks along the northern margin of Tarim include the Baicheng and Yangxia granites, Tiemenguan syenite, Kurle mafic dykes and the basalt layers in the Zamoketi Formation (northeastern Tarim) and the Sugetbrak Formation (northwestern Tarim). Precise zircon U<img>Pb dating revealed that these distinct rocks were broadly coeval with crystallization/eruption ages of 630–600 Ma. Bulk-rock elemental and Sr<img>Nd isotope compositions as well as zircon Lu<img>Hf isotope compositions demonstrate that the Baicheng and Yangxia granites were derived from Neoarchean mafic lower crust and underwent intensive fractionation before their emplacements. The Tiemenguan syenites have potassic andesitic compositions, in combination with their pronounced enriched Nd<img>Hf isotopes and extremely high Zr saturation temperatures (∼900 °C), we argue that their possible shoshonitic primary magmas were derived from previously metasomatized subcontinental lithospheric mantle source (amphibole-bearing) and then, coupling with assimilation and fractional crystallization (AFC) effects in magma chamber and/or en route to the emplacement space. This can account for their intriguing geochemical features. The ca. 615 Ma Zamoketi and Sugetbrak basalts and the slightly younger porphyrite dykes (ca. 580 Ma) cutting the Zamoketi basalt layer, show typical OIB-like geochemical signatures, they were most likely derived from a depleted asthenospheric mantle source with variable fractionation of olivine and pyroxene and negligible crustal contamination before eruption. On the whole, the geochemistry of the diverse Ediacaran igneous rocks unambiguously demonstrates that they were genetically related to an extensional environment. In combination with the significant passive continental features of the Ediacaran-Cambrian sedimentary sequences, we consider that these Ediacaran igneous rocks were the latest phase of igneous activity related to the dispersing of the Tarim at the margin of the Rodinia supercontinent.</div><div>The dispersing of the Rodinian supra-continent was diachronic with the assemblage of the Gondwana. Late Tonian to Ediacaran dispersing of the Tarim from northern margin of Australia induced the opening of the Proto-Tethys Ocean. Then the initiation of the sou
{"title":"Diverse magmatism along the northern margin of Tarim during the Ediacaran: Transition from Rodinian dispersing to Gondwana assemblage","authors":"Guangyou Zhu , Zhiyong Chen , Weiyan Chen , Lei Yan , Kun Zhao , Huichuan Liu","doi":"10.1016/j.lithos.2024.107823","DOIUrl":"10.1016/j.lithos.2024.107823","url":null,"abstract":"<div><div>The Ediacaran igneous rocks and sedimentary sequences play a key role for our understanding the transition from dispersing of the Rodinian continents to the assemblage of the Gondwana. On the other hand, some continental massifs at the marginal area of the Rodinia and Gondwana could preserve solid evidences for deciphering the geodynamic background from the break-up of Rodinia to the assemblage of Gondwana. In this contribution, we report field observations, petrography, ages and systematic geochemistry of the diverse Ediacaran igneous activities in the northern margin of the Tarim Block, which was favored as a marginal continental massif in the Rodinia configuration by most geologists. The Ediacaran igneous rocks along the northern margin of Tarim include the Baicheng and Yangxia granites, Tiemenguan syenite, Kurle mafic dykes and the basalt layers in the Zamoketi Formation (northeastern Tarim) and the Sugetbrak Formation (northwestern Tarim). Precise zircon U<img>Pb dating revealed that these distinct rocks were broadly coeval with crystallization/eruption ages of 630–600 Ma. Bulk-rock elemental and Sr<img>Nd isotope compositions as well as zircon Lu<img>Hf isotope compositions demonstrate that the Baicheng and Yangxia granites were derived from Neoarchean mafic lower crust and underwent intensive fractionation before their emplacements. The Tiemenguan syenites have potassic andesitic compositions, in combination with their pronounced enriched Nd<img>Hf isotopes and extremely high Zr saturation temperatures (∼900 °C), we argue that their possible shoshonitic primary magmas were derived from previously metasomatized subcontinental lithospheric mantle source (amphibole-bearing) and then, coupling with assimilation and fractional crystallization (AFC) effects in magma chamber and/or en route to the emplacement space. This can account for their intriguing geochemical features. The ca. 615 Ma Zamoketi and Sugetbrak basalts and the slightly younger porphyrite dykes (ca. 580 Ma) cutting the Zamoketi basalt layer, show typical OIB-like geochemical signatures, they were most likely derived from a depleted asthenospheric mantle source with variable fractionation of olivine and pyroxene and negligible crustal contamination before eruption. On the whole, the geochemistry of the diverse Ediacaran igneous rocks unambiguously demonstrates that they were genetically related to an extensional environment. In combination with the significant passive continental features of the Ediacaran-Cambrian sedimentary sequences, we consider that these Ediacaran igneous rocks were the latest phase of igneous activity related to the dispersing of the Tarim at the margin of the Rodinia supercontinent.</div><div>The dispersing of the Rodinian supra-continent was diachronic with the assemblage of the Gondwana. Late Tonian to Ediacaran dispersing of the Tarim from northern margin of Australia induced the opening of the Proto-Tethys Ocean. Then the initiation of the sou","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107823"},"PeriodicalIF":2.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142446564","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-28DOI: 10.1016/j.lithos.2024.107819
Igor González-Pérez , José M. González-Jiménez , Sarah A.S. Dare , Erwin Schettino , Rubén Piña , Claudio Marchesi , Lola Yesares , Fernando Gervilla
The ultramafic massifs of the Serranía de Ronda in southern Spain are the Earth's largest exposures of subcontinental lithospheric mantle (SCLM) peridotites (∼450 km2). These ultramafic massifs experienced asthenosphere melt percolation during their crustal emplacement. Mixing of these mafic melts with anatectic melts and fluids led to the formation of a world's unique Ni-arsenide-rich chromitite ores (hereafter CrNi ores) associated with orthopyroxenite and/or cordieritite (i.e., > 90 % volume of cordierite) hosted within the peridotites. This study uses laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) to investigate the Li in rock-forming minerals of peridotite and CrNi ores to evaluate the role of Li as crustal tracer. Clinopyroxene crystallized from asthenospheric melts exhibits high Li contents (up to 8.5 ppm), exceeding the average values of the upper mantle (∼ 0.7 ppm), whereas orthopyroxene, olivine, and Cr-spinel from peridotite are mostly Li-depleted. In contrast, all rock-forming minerals of CrNi ores have abnormally high Li contents, displaying an overall Li enrichment trend toward the external parts of ultramafic massifs, on the way to the crustal rocks. This trend is evident in Cr-spinel from the CrNi ores, which display 6.9–7.9 ppm Li in the deepest portions of the massif (Arroyo de la Cala CrNi ore) up to 1.4–8.5 ppm in the shallowest part (La Gallega CrNi ore), as well as in orthopyroxenes that have 31.3–44.7 ppm Li in Arroyo de la Cala, and 45.1–51.4 ppm Li in La Gallega. Cordierite is present only in the CrNi ores situated in the external part of the ultramafic massifs, exhibiting 113.15–160.82 ppm Li in the Barranco de las Acedías CrNi ore and 36.5–60.5 ppm Li in La Gallega CrNi ore. Similarly to Li, LREE, fluid-mobile elements (K, Rb, Ba), and Sr in orthopyroxenes from the CrNi ores display enrichment from the inner to the outer parts of the ultramafic massif. These geochemical variations suggest that Li enrichment in CrNi ores and host peridotites was a twofold process: (1) asthenospheric melt percolation slightly increased Li abundances in the SCLM peridotites by modal and cryptic metasomatism involving clinopyroxene; (2) additional infiltration of Li-bearing crustally-derived fluids during the intracrustal emplacement of the mantle section boosted the Li contents of minerals in the CrNi ores. Our results highlight that Li may effectively track the interaction of the SCLM with crustal components.
西班牙南部隆达山脉的超基性岩块是地球上最大的次大陆岩石圈地幔(SCLM)橄榄岩出露区(450 平方公里)。这些超基性岩块在地壳形成过程中经历了星体层熔融渗流。这些黑云母熔体与安山岩熔体和流体混合,形成了世界上独一无二的富含镍砷化物的铬铁矿(以下简称铬镍矿),这些铬镍矿与正长辉石和/或堇青石(即堇青石体积占 90%)伴生在橄榄岩中。本研究采用激光烧蚀电感耦合等离子体质谱法(LA-ICP-MS)研究橄榄岩和铬镍矿石成岩矿物中的锂,以评估锂作为地壳示踪剂的作用。从星体层熔体中结晶出来的霞石显示出较高的锂含量(高达百万分之 8.5),超过了上地幔的平均值(百万分之 0.7),而从橄榄岩中结晶出来的正辉石、橄榄石和铬尖晶石则大多不含锂。与此相反,铬镍矿石的所有成岩矿物都具有异常高的锂含量,在通向地壳岩石的过程中,超基性岩块外部呈现出整体锂富集趋势。这种趋势在铬镍矿石中的铬榍石中很明显,在岩块最深的部分(Arroyo de la Cala 铬镍矿石)显示出百万分之 6.9-7.9 的锂含量,而在最浅的部分(La Gallega 铬镍矿石)则显示出百万分之 1.4-8.5 的锂含量,在 Arroyo de la Cala 和 La Gallega 的正长石中也分别显示出百万分之 31.3-44.7 和 45.1-51.4 的锂含量。堇青石只出现在位于超基性岩丘外部的铬镍矿石中,在 Barranco de las Acedías 铬镍矿石中显示出 113.15-160.82 ppm Li,在 La Gallega 铬镍矿石中显示出 36.5-60.5 ppm Li。与锂元素类似,铬镍矿石中正辉石的 LREE、流体流动元素(K、Rb、Ba)和锶元素也从超基性岩丘的内部向外部富集。这些地球化学变化表明,Li在铬镍矿石和宿主橄榄岩中的富集是一个双重过程:(1)星体层熔体渗流通过涉及挛辉石的模态和隐伏变质作用,使SCLM橄榄岩中的Li丰度略有增加;(2)在地幔段的地壳内成岩过程中,含Li的地壳衍生流体的额外渗入提高了铬镍矿石中矿物的Li含量。我们的研究结果突出表明,锂可能有效地追踪了SCLM与地壳成分的相互作用。
{"title":"Li enrichment in peridotites and chromitites tracks mantle-crust interaction","authors":"Igor González-Pérez , José M. González-Jiménez , Sarah A.S. Dare , Erwin Schettino , Rubén Piña , Claudio Marchesi , Lola Yesares , Fernando Gervilla","doi":"10.1016/j.lithos.2024.107819","DOIUrl":"10.1016/j.lithos.2024.107819","url":null,"abstract":"<div><div>The ultramafic massifs of the Serranía de Ronda in southern Spain are the Earth's largest exposures of subcontinental lithospheric mantle (SCLM) peridotites (∼450 km<sup>2</sup>). These ultramafic massifs experienced asthenosphere melt percolation during their crustal emplacement. Mixing of these mafic melts with anatectic melts and fluids led to the formation of a world's unique Ni-arsenide-rich chromitite ores (hereafter Cr<img>Ni ores) associated with orthopyroxenite and/or cordieritite (i.e., > 90 % volume of cordierite) hosted within the peridotites. This study uses laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) to investigate the Li in rock-forming minerals of peridotite and Cr<img>Ni ores to evaluate the role of Li as crustal tracer. Clinopyroxene crystallized from asthenospheric melts exhibits high Li contents (up to 8.5 ppm), exceeding the average values of the upper mantle (∼ 0.7 ppm), whereas orthopyroxene, olivine, and Cr-spinel from peridotite are mostly Li-depleted. In contrast, all rock-forming minerals of Cr<img>Ni ores have abnormally high Li contents, displaying an overall Li enrichment trend toward the external parts of ultramafic massifs, on the way to the crustal rocks. This trend is evident in Cr-spinel from the Cr<img>Ni ores, which display 6.9–7.9 ppm Li in the deepest portions of the massif (Arroyo de la Cala Cr<img>Ni ore) up to 1.4–8.5 ppm in the shallowest part (La Gallega Cr<img>Ni ore), as well as in orthopyroxenes that have 31.3–44.7 ppm Li in Arroyo de la Cala, and 45.1–51.4 ppm Li in La Gallega. Cordierite is present only in the Cr<img>Ni ores situated in the external part of the ultramafic massifs, exhibiting 113.15–160.82 ppm Li in the Barranco de las Acedías Cr<img>Ni ore and 36.5–60.5 ppm Li in La Gallega Cr<img>Ni ore. Similarly to Li, LREE, fluid-mobile elements (K, Rb, Ba), and Sr in orthopyroxenes from the Cr<img>Ni ores display enrichment from the inner to the outer parts of the ultramafic massif. These geochemical variations suggest that Li enrichment in Cr<img>Ni ores and host peridotites was a twofold process: (1) asthenospheric melt percolation slightly increased Li abundances in the SCLM peridotites by modal and cryptic metasomatism involving clinopyroxene; (2) additional infiltration of Li-bearing crustally-derived fluids during the intracrustal emplacement of the mantle section boosted the Li contents of minerals in the Cr<img>Ni ores. Our results highlight that Li may effectively track the interaction of the SCLM with crustal components.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107819"},"PeriodicalIF":2.9,"publicationDate":"2024-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142428309","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-24DOI: 10.1016/j.lithos.2024.107808
Simiao Wang , Yu Dong , Junhui Bi , Yan Jing , Wenchun Ge , Hao Yang , Jielu Yu , Zheng Ji
This paper presents zircon U-Pb ages, whole-rock major and trace element data, and Sr-Nd-Hf isotopic compositions for the greenschists from the Heilongjiang Complex in NE China. Based on the geochronological and geochemical characteristics, the greenschists from the Heilongjiang Complex can be categorized into three series: Early Permian tholeiitic series (275 ± 1 Ma and 273 ± 1 Ma), Middle Permian alkaline series (261 ± 1 Ma), and Early Jurassic alkaline series (179 ± 1 Ma). The Early Permian tholeiitic greenschist samples are characterized by remarkable negative Nb and Ta anomalies, and they exhibit relatively low whole-rock (87Sr/86Sr)i values (0.703896–0.704252), along with positive εNd(t) values (+7.66 to +8.65) and positive εHf(t) values (+0.92 to +11.51), implying that their protoliths originated from the partial melting of a depleted mantle wedge that has been metasomatized by subducted slab fluids. The Middle Permian alkaline greenschist samples have high Nb (17.3–19.0 ppm), TiO2 (1.40–1.64 wt%), and P2O5 (0.60–0.68 wt%) concentrations, and they are enriched in large ion lithophile elements and light rare earth elements, and depleted in high field strength elements and heavy rare earth elements, with high whole-rock (87Sr/86Sr)i values (0.709434–0.709949), negative εNd(t) values (−4.73 to −4.72) and varied εHf(t) values (−10.11 to +4.86), which compositionally align with those of Nb-enriched basalts. Based on the geochronological and geochemical characteristics, we propose that the protolith generation of Middle Permian alkaline greenschists was associated with the partial melting of a mantle wedge that had been metasomatized by subduction slab-derived melts. The Early Jurassic alkaline greenschist samples display OIB affinities, characterized by whole-rock (87Sr/86Sr)i values ranging from 0.705161 to 0.705926, εNd(t) values between +6.16 and +6.19, and εHf(t) values from +3.44 to +9.32, indicating the formation of the protolith for the Early Jurassic alkaline greenschist was related to the upwelling of the asthenosphere resulting from slab break-off. By integrating regional geological data, we can trace the subduction evolution of the Mudanjiang Ocean back to the Early Permian, and the slab break-off during the Early Jurassic likely corresponded to the early stage of the closure of the Mudanjiang Ocean.
本文介绍了中国东北黑龙江群绿泥石的锆石U-Pb年龄、全岩主要元素和微量元素数据以及Sr-Nd-Hf同位素组成。根据地质年代和地球化学特征,黑龙江岩群的绿泥石可分为三个系列:早二叠世托勒密系列(275±1 Ma 和 273±1 Ma)、中二叠世碱性系列(261±1 Ma)和早侏罗世碱性系列(179±1 Ma)。早二叠世托勒密绿泥石样本具有显著的负 Nb 和 Ta 异常,全岩 (87Sr/86Sr)i 值相对较低 (0.703896-0.704252),εNd(t) 值为正 (+7. 66 至 +8.65),εNd(t) 值为负 (+8. 66 至 +8.65)。66至+8.65)和正εHf(t)值(+0.92至+11.51),这意味着它们的原岩起源于被俯冲板块流体变质的贫化地幔楔的部分熔融。中二叠统碱性绿泥石样品具有较高的 Nb(17.3-19.0 ppm)、TiO2(1.40-1.64 wt%)和 P2O5(0.60-0.68 wt%)浓度,富含大离子亲岩元素和轻稀土元素,贫乏高场强元素和重稀土元素,具有较高的全岩(87Sr/86Sr)i 值(0.709434-0.709949)、负εNd(t)值(-4.73至-4.72)和变化的εHf(t)值(-10.11至+4.86),在成分上与富铌玄武岩一致。根据这些地质年代和地球化学特征,我们认为中二叠统碱性绿泥石的原岩生成与地幔楔的部分熔融有关,而地幔楔是由俯冲板源熔体变质而成的。早侏罗世碱性绿泥石样品具有OIB亲缘特征,其全岩(87Sr/86Sr)i值介于0.705161至0.705926之间,εNd(t)值介于+6.16至+6.19之间,εHf(t)值介于+3.44至+9.32之间,表明早侏罗世碱性绿泥石原岩的形成与板块断裂导致的星体层上涌有关。通过整合区域地质资料,我们可以将牡丹江洋的俯冲演化追溯到早二叠世,而早侏罗世的板块断裂很可能对应于牡丹江洋闭合的早期阶段。
{"title":"Late Paleozoic–Early Mesozoic subduction history of Mudanjiang Ocean: New insights from greenschist in the Heilongjiang Complex, NE China","authors":"Simiao Wang , Yu Dong , Junhui Bi , Yan Jing , Wenchun Ge , Hao Yang , Jielu Yu , Zheng Ji","doi":"10.1016/j.lithos.2024.107808","DOIUrl":"10.1016/j.lithos.2024.107808","url":null,"abstract":"<div><div>This paper presents zircon U-Pb ages, whole-rock major and trace element data, and Sr-Nd-Hf isotopic compositions for the greenschists from the Heilongjiang Complex in NE China. Based on the geochronological and geochemical characteristics, the greenschists from the Heilongjiang Complex can be categorized into three series: Early Permian tholeiitic series (275 ± 1 Ma and 273 ± 1 Ma), Middle Permian alkaline series (261 ± 1 Ma), and Early Jurassic alkaline series (179 ± 1 Ma). The Early Permian tholeiitic greenschist samples are characterized by remarkable negative Nb and Ta anomalies, and they exhibit relatively low whole-rock (<sup>87</sup>Sr/<sup>86</sup>Sr)<sub>i</sub> values (0.703896–0.704252), along with positive ε<sub>Nd</sub>(t) values (+7.66 to +8.65) and positive ε<sub>Hf</sub>(t) values (+0.92 to +11.51), implying that their protoliths originated from the partial melting of a depleted mantle wedge that has been metasomatized by subducted slab fluids. The Middle Permian alkaline greenschist samples have high Nb (17.3–19.0 ppm), TiO<sub>2</sub> (1.40–1.64 wt%), and P<sub>2</sub>O<sub>5</sub> (0.60–0.68 wt%) concentrations, and they are enriched in large ion lithophile elements and light rare earth elements, and depleted in high field strength elements and heavy rare earth elements, with high whole-rock (<sup>87</sup>Sr/<sup>86</sup>Sr)<sub>i</sub> values (0.709434–0.709949), negative ε<sub>Nd</sub>(t) values (−4.73 to −4.72) and varied ε<sub>Hf</sub>(t) values (−10.11 to +4.86), which compositionally align with those of Nb-enriched basalts. Based on the geochronological and geochemical characteristics, we propose that the protolith generation of Middle Permian alkaline greenschists was associated with the partial melting of a mantle wedge that had been metasomatized by subduction slab-derived melts. The Early Jurassic alkaline greenschist samples display OIB affinities, characterized by whole-rock (<sup>87</sup>Sr/<sup>86</sup>Sr)<sub>i</sub> values ranging from 0.705161 to 0.705926, ε<sub>Nd</sub>(t) values between +6.16 and +6.19, and ε<sub>Hf</sub>(t) values from +3.44 to +9.32, indicating the formation of the protolith for the Early Jurassic alkaline greenschist was related to the upwelling of the asthenosphere resulting from slab break-off. By integrating regional geological data, we can trace the subduction evolution of the Mudanjiang Ocean back to the Early Permian, and the slab break-off during the Early Jurassic likely corresponded to the early stage of the closure of the Mudanjiang Ocean.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107808"},"PeriodicalIF":2.9,"publicationDate":"2024-09-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142428470","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"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 : 2024-09-21DOI: 10.1016/j.lithos.2024.107817
Bastien Audran , Philippe Boulvais , Yannick Branquet , Pierre Gautier , Marc Ulrich , Guillaume Raymond , Georges Beaudoin , Daniel Layton-Matthews , Evelyne Leduc , Maëlys Bévan , Rémi Coltat
Serpentinization is a ubiquitous hydrothermal alteration of ultramafic rocks. In the Ronda Massif (Andalusia, Spain), which represents the largest body of subcontinental peridotite exposed at the Earth surface, most studies focused on high-temperature deformation and petrology of mantle rocks. Serpentinization remains poorly constrained. Petro-structural and O and H isotope investigations allow us to identify three successive stages of serpentinization. The first stage of serpentinization is characterized by a widespread lizardite mesh-texture. The extent of serpentinization indicates a regional gradient, with a low proportion of serpentine (around 15 %) in the core of the Sierra Bermeja Massif. The second stage corresponds to highly localized serpentinization, characterized by the presence of lizardite, bastite and high content of magnetite. The third stage was intimately associated with brittle deformation, consisting of fibrous veins and a coating network within cataclastic shear zones. Structural analysis of shear veins of the third serpentinization stage enables identification of a regional syn-serpentinization extensional deformation that corresponded to a multi-directional horizontal stretching and a vertical shortening direction (i.e., flattening). All stages of serpentinization display comparable isotopic compositions, with the mean of δ18O values at ∼ +5.0 ‰ and δD at ∼ −80.5 ‰, suggesting that the two last stages occurred under conditions of fluid-rock interactions that preserved the compositions acquired during stage 1. The fluid source for this stage 1 was likely deeply seated, with a possible contribution of meteoric-derived fluids. Stage 3 serpentinization occurred at 170 ± 50 °C based on magnetite-serpentine isotopic equilibrium. We propose a model of continuous serpentinization that occurred during the rapid exhumation of the Ronda Massif during the Early Miocene period. The syn-serpentinization extensional brittle deformation we document may be compatible either with orogenic thickening (i.e., syn-thrusting) or with early post-thickening collapse.
蛇纹岩化是超基性岩普遍存在的热液蚀变现象。龙达丘陵(西班牙安达卢西亚)是暴露在地表的最大的亚大陆橄榄岩体,在这里,大多数研究都集中在高温变形和地幔岩石岩石学方面。对蛇纹岩化的研究仍然很少。岩石结构以及 O 和 H 同位素研究使我们能够确定蛇绿岩化的三个连续阶段。蛇纹石化的第一阶段以广泛的蜥蜴石网状纹理为特征。蛇纹石化的程度呈现区域梯度,在贝梅哈山脉地块的核心区域,蛇纹石的比例较低(约 15%)。第二阶段是高度局部的蛇纹石化,其特征是存在蜥蜴石、韧皮石和高含量的磁铁矿。第三阶段与脆性变形密切相关,由纤维状矿脉和弹塑性剪切带内的涂层网络组成。通过对蛇纹石化第三阶段剪切脉的结构分析,可以确定区域性的同步蛇纹石化延伸变形,该变形与多方向的水平拉伸和垂直缩短方向(即扁平化)相对应。蛇绿岩化的所有阶段都显示出相当的同位素组成,δ18O 的平均值为∼ +5.0‰,δD 为∼ -80.5‰,这表明最后两个阶段是在流体与岩石相互作用的条件下发生的,保留了第一阶段获得的组成。第一阶段的流体来源可能是深层流体,也可能是陨石流体。根据磁铁矿-蛇绿岩同位素平衡,第三阶段蛇绿岩化发生在 170 ± 50 °C。我们提出了一个在早中新世时期龙达丘块快速掘起过程中发生的连续蛇绿岩化模型。我们所记录的同步蛇绿岩化延伸脆性变形可能与造山增厚(即同步推移)或增厚后早期崩塌相一致。
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Pub Date : 2024-09-21DOI: 10.1016/j.lithos.2024.107812
Russell Bailie , Musa Mhlanga , Jürgen Reinhardt , Deon van Niekerk
The Sea Point contact in Cape Town, South Africa showcases the interaction between the Malmesbury Group metasedimentary rocks and the intrusive S-type Peninsula Granite of the Cape Granite Suite. The Malmesbury Group, comprising weakly metamorphosed mudstones and siltstones, has been intruded by various granitic injections of varying composition and mineralogical make-up. These granitic injections, displaying diffuse contacts with the country rock and termed “hybrid” granites, indicate varying degrees of assimilation of the country rocks. The injections occurred parallel to the country rock's fabric and anisotropies, particularly along the well-developed S1 foliation. The granites exhibit compositional variations and contain K-feldspar megacrysts in a variable grain-sized groundmass. Some of these megacrysts are found within the Malmesbury Group, with or without quartzofeldspathic material envelopes. Most researchers agree that large K-feldspar megacrysts in granites develop through near-solidus growth, resulting from prolonged exposure to renewed magma input. However, the origin of K-feldspar and other phenocrysts in the adjacent country rocks is debated, with proposed mechanisms including entrapment due to magma through-flow and in situ growth due to K-metasomatism from granitic magma-derived fluids. This study compares the textures and chemistry of K-feldspar megacrysts in various granite types at the Sea Point contact with those in the Malmesbury Group country rock to determine the origin of the latter. The megacrysts in all lithologies show notable textural and compositional similarities, exhibiting poorly defined compositional zoning and consistent variations in K2O, Na2O, and BaO, along with rare earth element concentrations. These attributes suggest that the megacrysts formed through renewed magma injection and prolonged growth involving multiple magma pulses. The study proposes that filter pressing, where melt fractions separate from a crystal mush during crystallisation, occurred during active deformation so that filter pressing was strain-induced. During magma intrusion in a syn- to post-tectonic compressive regime, the melt and associated crystals moved into openings, with the melt fraction more easily mobilised and driven out compared to the crystal fraction during transpression. This left K-feldspar megacrysts embedded or mantled by the country rock. These isolated crystals, with or without associated crystallised magmatic material, mark former magma flow pathways through the country rock, contributing to understanding magma emplacement mechanisms and the formation of the continental crust.
南非开普敦的海角接触点展示了马尔梅斯伯里组变质岩与开普花岗岩组的侵入S型半岛花岗岩之间的相互作用。马尔梅斯伯里组由弱变质泥岩和粉砂岩组成,曾被不同成分和矿物组成的各种花岗岩喷入岩侵入。这些花岗岩喷入岩与乡土岩呈弥散接触,被称为 "混合 "花岗岩,表明乡土岩在不同程度上被同化。注入岩与乡村岩的构造和各向异性平行,特别是沿着发达的 S1 叶理。花岗岩呈现出成分变化,在颗粒大小不一的基质中含有钾长石巨晶。其中一些巨晶存在于马姆斯伯里组中,或有或无石英长石包裹体。大多数研究人员一致认为,花岗岩中的大型钾长石巨晶是通过近固结生长形成的,是由于长期暴露于更新的岩浆输入中造成的。然而,对于邻近乡土岩中的钾长石和其他表晶的起源却存在争议,提出的机制包括岩浆贯流导致的夹带以及花岗岩岩浆衍生流体的钾金属气相作用导致的原地生长。本研究比较了海角接触点各种类型花岗岩中的钾长石巨晶与马姆斯伯里组乡村岩中的钾长石巨晶的质地和化学性质,以确定后者的起源。所有岩性中的巨晶在质地和成分上都有明显的相似性,表现出不明确的成分分区,K2O、Na2O 和 BaO 以及稀土元素浓度都有一致的变化。这些特征表明,巨晶是通过岩浆注入和多次岩浆脉冲的长期生长形成的。研究认为,滤压(即在结晶过程中熔体碎片从晶泥中分离出来)发生在活动变形过程中,因此滤压是由应变引起的。在同步构造到后构造压缩机制的岩浆侵入过程中,熔体和相关晶体移动到开口处,与转压过程中的晶体部分相比,熔体部分更容易被移动和驱赶出来。这使得钾长石巨晶嵌入或覆盖在乡土岩中。这些孤立的晶体,无论是否伴有结晶的岩浆物质,都标志着岩浆流经乡村岩石的昔日路径,有助于了解岩浆置换机制和大陆地壳的形成。
{"title":"Magma through-flow and embedding of magmatic crystals in metasedimentary country rocks adjacent to the Peninsula Granite, Cape Granite Suite (South Africa)","authors":"Russell Bailie , Musa Mhlanga , Jürgen Reinhardt , Deon van Niekerk","doi":"10.1016/j.lithos.2024.107812","DOIUrl":"10.1016/j.lithos.2024.107812","url":null,"abstract":"<div><div>The Sea Point contact in Cape Town, South Africa showcases the interaction between the Malmesbury Group metasedimentary rocks and the intrusive S-type Peninsula Granite of the Cape Granite Suite. The Malmesbury Group, comprising weakly metamorphosed mudstones and siltstones, has been intruded by various granitic injections of varying composition and mineralogical make-up. These granitic injections, displaying diffuse contacts with the country rock and termed “hybrid” granites, indicate varying degrees of assimilation of the country rocks. The injections occurred parallel to the country rock's fabric and anisotropies, particularly along the well-developed S<sub>1</sub> foliation. The granites exhibit compositional variations and contain K-feldspar megacrysts in a variable grain-sized groundmass. Some of these megacrysts are found within the Malmesbury Group, with or without quartzofeldspathic material envelopes. Most researchers agree that large K-feldspar megacrysts in granites develop through near-solidus growth, resulting from prolonged exposure to renewed magma input. However, the origin of K-feldspar and other phenocrysts in the adjacent country rocks is debated, with proposed mechanisms including entrapment due to magma through-flow and in situ growth due to K-metasomatism from granitic magma-derived fluids. This study compares the textures and chemistry of K-feldspar megacrysts in various granite types at the Sea Point contact with those in the Malmesbury Group country rock to determine the origin of the latter. The megacrysts in all lithologies show notable textural and compositional similarities, exhibiting poorly defined compositional zoning and consistent variations in K<sub>2</sub>O, Na<sub>2</sub>O, and BaO, along with rare earth element concentrations. These attributes suggest that the megacrysts formed through renewed magma injection and prolonged growth involving multiple magma pulses. The study proposes that filter pressing, where melt fractions separate from a crystal mush during crystallisation, occurred during active deformation so that filter pressing was strain-induced. During magma intrusion in a <em>syn</em>- to post-tectonic compressive regime, the melt and associated crystals moved into openings, with the melt fraction more easily mobilised and driven out compared to the crystal fraction during transpression. This left K-feldspar megacrysts embedded or mantled by the country rock. These isolated crystals, with or without associated crystallised magmatic material, mark former magma flow pathways through the country rock, contributing to understanding magma emplacement mechanisms and the formation of the continental crust.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"488 ","pages":"Article 107812"},"PeriodicalIF":2.9,"publicationDate":"2024-09-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142428471","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}