Pub Date : 2023-12-27DOI: 10.1007/s00531-023-02372-9
Abstract
Within the Tethyan belt, the NW-Iranian block is bound by two sutures, the Sevan-Akera suture in the north, and the Zagros suture in the south, where the pre-Cambrian geology is poorly constrained. Lower-Middle Cambrian sandstone in NW Iran is represented by quartz and feldspar dominated sub-arkose and sub-litharenite with well-developed cross bedding structures. They are interlayered with shale and limestone and overlain unconformably by Middle Cambrian dolomite. Here we describe and present U–Pb ages of the detrital zircon and rutile together with in-situ ε-Hf data from Lower to Middle Cambrian sandstones. Some zircons are characterized by oscillatory zoning and Th/U ratios of 0.3 to 2.0, pointing to an igneous provenance. Ages of the detrital zircons range from 481 to 2762 Ma, whereby the majority of zircons have ages between 524 and 1000 Ma (Neoproterozoic), and small peaks at 1800–2000 and 2400–2600 Ma. Late Paleoproterozoic to Mesoproterozoic zircons (1100–1750 Ma) are absent in the detrital record which is a distinctive feature of Gondwana-related detrital zircons. Detrital rutile has elevated Cr contents and variable Zr content (88 to 1087 ppm), suggesting derivation mainly from amphibolite-facies meta-basic rocks. U–Pb rutile ages range from 561 to 1253 Ma. Initial ε-Hf values of the Neo-Proterozoic zircons range from -10 to 20, suggesting an association of highly depleted mantle and crustal magmas. Thus, the Lower-Middle Cambrian sandstones in Iranian Azerbaijan were supplied from a Neoproterozoic igneous and metamorphic provenance. Sandstone whole-rock major and trace elements are in accordance with a detrital material provenance from continental granitoids and Precambrian recycled sediments. These results support the hypothesis that Iranian Azerbaijan Cambrian detritus was supplied from repetitive recycling of the crystalline basement and related sedimentary cover of the Saharides and the Arabian-Nubian Shield and deposited in a passive-margin setting in northern Gondwana land. Our results show a close geological tie between Iranian Azerbaijan, Sanandaj-Sirjan, Zagros, Alborz, and other Gondwana-Land-derived units in terms of Early Paleozoic detritus sources. Northwest Iranian Block was probably a passive continental margin in Late Ediacaran-Cambrian after the so-called Cadomian orogeny.
Graphical Abstract
摘要 在泰提安带中,西北伊朗地块被两条缝合线所束缚,即北部的塞万-阿克拉缝合线和南部的扎格罗斯缝合线。伊朗西北部的下-中寒武统砂岩以石英和长石为主的亚云英岩和亚闪长岩为代表,具有发达的交叉层理结构。它们与页岩和石灰岩互层,与中寒武统白云岩互不叠压。在此,我们描述并展示了下寒武统至中寒武统砂岩中的锆石和金红石的U-Pb年龄以及原位ε-Hf数据。一些锆石具有振荡区带和 0.3 至 2.0 的 Th/U 比值,表明其来源于火成岩。锆石碎片的年龄在 481 至 2762 Ma 之间,其中大部分锆石的年龄在 524 至 1000 Ma 之间(新元古代),在 1800 至 2000 Ma 和 2400 至 2600 Ma 之间有小高峰。晚古生代到中新生代的锆石(1100-1750 Ma)没有出现在碎屑记录中,这是冈瓦纳相关碎屑锆石的一个显著特点。碎屑金红石的铬含量较高,锆含量(88-1087 ppm)不等,表明主要来自闪长岩期元基性岩。金红石的U-Pb年龄在561至1253Ma之间。新近新生代锆石的初始ε-Hf值介于-10到20之间,表明与高度贫化的地幔和地壳岩浆有关。因此,伊朗阿塞拜疆的下-中寒武统砂岩是由新近新生代火成岩和变质岩提供的。砂岩的全岩主要元素和微量元素与来自大陆花岗岩和前寒武纪循环沉积物的碎屑物质来源一致。这些结果支持这样的假设,即伊朗阿塞拜疆寒武纪的碎屑是由撒哈拉沙漠和阿拉伯-努比亚地盾的结晶基底和相关沉积覆盖层的重复循环提供的,并沉积在冈瓦纳陆地北部的被动边缘环境中。我们的研究结果表明,就早古生代碎屑源而言,伊朗阿塞拜疆、萨南达杰-锡尔让、扎格罗斯、阿尔伯兹和其他冈瓦纳-陆地衍生单元之间有着密切的地质联系。伊朗西北地块很可能是晚埃迪卡拉-寒武纪所谓卡多米造山运动之后的被动大陆边缘。 图表摘要
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Pub Date : 2023-12-22DOI: 10.1007/s00531-023-02371-w
Hadi Karimi, G. Topuz, Lothar Ratschbacher, Chuanbo Shen, Jianhua Li
{"title":"Geochemistry and geochronology of the Neyshabur meta-volcanic rocks, Binalood mountains, NE Iran: witnesses of Paleo-Tethys rifting and closure","authors":"Hadi Karimi, G. Topuz, Lothar Ratschbacher, Chuanbo Shen, Jianhua Li","doi":"10.1007/s00531-023-02371-w","DOIUrl":"https://doi.org/10.1007/s00531-023-02371-w","url":null,"abstract":"","PeriodicalId":13845,"journal":{"name":"International Journal of Earth Sciences","volume":"24 3","pages":""},"PeriodicalIF":2.3,"publicationDate":"2023-12-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138947771","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-12-14DOI: 10.1007/s00531-023-02369-4
Abstract
During the Late Permian Wuchiapingian–Changhsingian (W–C) transition, significant biotic and environmental changes occurred. These changes had the potential to greatly influence the type, accumulation, and preservation of organic matter within sediments during this period. The Wujiaping Formation, which acts as the contemporaneous heterotopic facie of the Longtan Formation, is regionally found in the Susong–Dongzhi stratigraphic subregion in the Lower Yangtze Platform (LYP). However, the variations in organic matter input and preservation during the Late Permian W–C transition in this specific area have not been comprehensively understood. Consequently, this study involved the collection of Upper Permian Wujiaping and Dalong shale samples in the LYP. Total organic carbon (TOC) content, vitrinite reflectance (Ro), maceral compositions, carbon isotope composition of kerogen, as well as the major and trace elements in the shale samples were all measured in this study. The results of Ro analysis indicate that the maturity levels of shale derived from the Dalong and Wujiaping Formations exhibit maturity levels exceeding 2%, which indicates an over-mature stage. The maceral compositions and carbon isotope analysis of kerogen reveal that the predominant source of organic matter within the Dalong shale is attributed to algal organism. Conversely, the organic matter in the Wujiaping shale primarily comes from higher plants. The major and trace element distributions provide insights into the depositional conditions of the Upper Permian shale, and significant variations in organic matter input and preservation are evident during the Late Permian W–C transition. The findings indicate that the Wujiaping Formation was characterized by a low paleo-productivity, high terrestrial influx intensity, low paleo-salinity, and a pronounced restricted setting under oxic conditions. However, the Dalong Formation is deposited under an anoxic environment, characterized by high paleo-productivity and paleo-salinity, limited terrestrial influx intensity, and increasing upwelling. In addition, the water mass restriction weakened within the Dalong Formation, attributable to a gradual rise in sea level. The shift of organic matter input and preservation was instigated by the persistent regional rise in the sea level during the Late Permian period. In summary, the great input and favorable preservation conditions of organic matter observed in the Dalong shale indicates a promising potential for shale gas exploration.
{"title":"Input and preservation of organic matter in the Upper Permian shale from the Lower Yangtze Platform, South China: evidence from organic and inorganic geochemistry","authors":"","doi":"10.1007/s00531-023-02369-4","DOIUrl":"https://doi.org/10.1007/s00531-023-02369-4","url":null,"abstract":"<h3>Abstract</h3> <p>During the Late Permian Wuchiapingian–Changhsingian (W–C) transition, significant biotic and environmental changes occurred. These changes had the potential to greatly influence the type, accumulation, and preservation of organic matter within sediments during this period. The Wujiaping Formation, which acts as the contemporaneous heterotopic facie of the Longtan Formation, is regionally found in the Susong–Dongzhi stratigraphic subregion in the Lower Yangtze Platform (LYP). However, the variations in organic matter input and preservation during the Late Permian W–C transition in this specific area have not been comprehensively understood. Consequently, this study involved the collection of Upper Permian Wujiaping and Dalong shale samples in the LYP. Total organic carbon (TOC) content, vitrinite reflectance (<em>R</em><sub><em>o</em></sub>), maceral compositions, carbon isotope composition of kerogen, as well as the major and trace elements in the shale samples were all measured in this study. The results of <em>R</em><sub><em>o</em></sub> analysis indicate that the maturity levels of shale derived from the Dalong and Wujiaping Formations exhibit maturity levels exceeding 2%, which indicates an over-mature stage. The maceral compositions and carbon isotope analysis of kerogen reveal that the predominant source of organic matter within the Dalong shale is attributed to algal organism. Conversely, the organic matter in the Wujiaping shale primarily comes from higher plants. The major and trace element distributions provide insights into the depositional conditions of the Upper Permian shale, and significant variations in organic matter input and preservation are evident during the Late Permian W–C transition. The findings indicate that the Wujiaping Formation was characterized by a low paleo-productivity, high terrestrial influx intensity, low paleo-salinity, and a pronounced restricted setting under oxic conditions. However, the Dalong Formation is deposited under an anoxic environment, characterized by high paleo-productivity and paleo-salinity, limited terrestrial influx intensity, and increasing upwelling. In addition, the water mass restriction weakened within the Dalong Formation, attributable to a gradual rise in sea level. The shift of organic matter input and preservation was instigated by the persistent regional rise in the sea level during the Late Permian period. In summary, the great input and favorable preservation conditions of organic matter observed in the Dalong shale indicates a promising potential for shale gas exploration.</p> <span> <h3>Graphical abstract</h3> <p> <span> <span> <img alt=\"\" src=\"https://static-content.springer.com/image/MediaObjects/531_2023_2369_Figa_HTML.png\"/> </span> </span></p> </span>","PeriodicalId":13845,"journal":{"name":"International Journal of Earth Sciences","volume":"182 1","pages":""},"PeriodicalIF":2.3,"publicationDate":"2023-12-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138684231","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-12-05DOI: 10.1007/s00531-023-02365-8
A. Käßner, M. Tichomirowa, R. Tandler, J. Ziebell
In the Late Permian Zechstein Sea of Central Europe, up to 2000 m of evaporitic rocks were deposited in at least four consecutive cycles. The age of these evaporitic rocks could not yet be precisely determined, because they are virtually fossil-free and do not contain radiometrically datable volcanic layers. A chemostratigraphic age of the succession can be determined by comparing 87Sr/86Sr ratios of marine gypsum and anhydrite to the worldwide marine strontium evolution curve. Unfortunately, published 87Sr/86Sr data of the Zechstein succession are characterized by frequent outliers towards higher ratios, making an age assignment challenging. The scatter in 87Sr/86Sr ratios might be induced by different processes like the contribution of meteoric water to the brine, in-situ Rb decay, or post-depositional hydrothermal or diagenetic overprint. Here, we present a dataset of 26 new gypsum and anhydrite 87Sr/86Sr ratios from drill cores situated at “Alter Stolberg” in the northernmost Thuringian Basin. Evaporites of the Werra-, Staßfurt-, and Leine cycles were sampled. The close proximity of the drillings allows a very accurate assignment of the stratigraphic position of each sample, so that trends and outliers in 87Sr/86Sr ratios can easily be recognized. While the entire Werra Formation obviously revealed non-marine 87Sr/86Sr ratios, the lowermost 87Sr/86Sr ratios in the Staßfurt and Leine Formations can be assumed to represent marine ratios and allow estimating a chemostratigraphic age of 257‒254 Ma. The combination of the 87Sr/86Sr data with the mineral composition of the samples suggests a contribution of meteoric water, probably river water, to the Zechstein Sea as the main reason for the observed increase in 87Sr/86Sr ratios. Additional in-situ Rb decay, related to the riverine input of clay minerals, cannot be excluded. Modelling the amounts of sea water and meteoric water in the brine indicates that 83‒99% of meteoric water would be necessary to explain the highest 87Sr/86Sr ratios observed in the Werra Formation.