Paleomagnetic constraints on the primary iron minerals of the late Paleoproterozoic Xuanlong-type ironstone in the North China Craton

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yuhang Cai , Shuan-Hong Zhang , Junling Pei , Yabo Tong , Zaizheng Zhou , Lifu Hou
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Abstract

The Xuanlong-type ironstone is a late Paleoproterozoic (∼1.64 Ga) hematite-dominated granular iron formation (GIF) in the North China Craton (NCC). However, recent geochemical studies indicated this GIF was precipitated in a weakly oxygenated environment. The conflicts between the mineral composition of the Xuanlong-type ironstone and its geochemical interpretations can be attributed to the potential occurrence of secondary hematite. Here we used paleomagnetic, rock magnetic measurements and petrographic analysis to determine the mineralization age of the hematite. Our objectives were to determine the primary iron mineralogy and to further explore the paleoenvironmental information preserved in the Xuanlong-type ironstone. Rock magnetic measurements and petrographic analysis identified Al-substituted hematite and siderite as the magnetic minerals. The high-temperature characteristic remanent magnetizations, which passed a C-classification reversal test and a fold test, yielded a paleomagnetic pole position at 51°N, 197°E. This pole position is in close proximity to the coeval paleomagnetic pole reconstructed from the ∼1.64 Ga Cuizhuang Formation in the southern NCC. Therefore, the high-temperature component of the natural remanent magnetization is interpreted as primary remanent magnetization acquired through crystal growth of Al-substituted hematite during early diagenesis. The degree of Al-substitution in hematite seems to be influenced by the alternating dense and porous laminae within the hematitic ooids of Xuanlong-type ironstones. It is hypothesized that these laminae are a result of periodic sea level fluctuations, considering that the ironstones were likely formed in a shallow water setting.
对华北克拉通晚古生代玄龙型铁岩原生铁矿物的古地磁约束
玄龙型铁岩是华北克拉通(NCC)晚古生代(∼1.64 Ga)以赤铁矿为主的粒状铁岩层(GIF)。然而,最近的地球化学研究表明,该GIF是在弱含氧环境中沉淀的。玄龙型铁岩的矿物组成与其地球化学解释之间的矛盾可归因于可能存在的次生赤铁矿。在这里,我们利用古地磁、岩石磁性测量和岩石学分析来确定赤铁矿的成矿年代。我们的目标是确定原生铁矿物学,并进一步探索玄龙型铁岩中保存的古环境信息。岩石磁性测量和岩相分析确定了铝代赤铁矿和菱铁矿为磁性矿物。高温特征剩磁通过了 C 级反转测试和褶皱测试,得出了位于北纬 51°、东经 197°的古地磁极位置。该磁极位置与南昌南部∼1.64Ga崔庄地层重建的共生古磁极位置相近。因此,天然剩磁中的高温成分被解释为在早期成岩过程中通过铝代赤铁矿晶体生长获得的原生剩磁。赤铁矿中的铝置换程度似乎受到玄龙型铁矿赤铁矿卵岩中致密和多孔层状交替的影响。考虑到这些铁石很可能是在浅水环境中形成的,因此推测这些层理是周期性海平面波动的结果。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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