Teixeira Livia, Carlut Julie, Rego Eric Siciliano, Trindade Ricardo I F, Philippot Pascal
Departamento de Geofísica, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, São Paulo, Brazil.
Université Paris Cité, Institut de Physique du Globe de Paris, CNRS UMR-7154, Paris, France.
Geobiology. 2024 Nov-Dec;22(6):e70008. doi: 10.1111/gbi.70008.
Banded iron formations (BIFs) are chemical sedimentary rocks commonly utilized for exploring the chemistry and redox state of the Precambrian ocean. Despite their significance, many aspects regarding the crystallization pathways of iron oxides in BIFs remain loosely constrained. In this study, we combine magnetic properties characterization with high-resolution optical and electron imaging of finely laminated BIFs from the 2.7 Ga Carajás Formation, Brazil, to investigate their nature and potential for preserving ancient environmental conditions. Our findings reveal that magnetite, in the form of large 0.1-0.5 mm crystals, is the main iron oxide, with an overall averaged saturation magnetization (M) of 25 Am/kg (corresponding to ~27 wt% of magnetite) over the studied 230 m of the sequence. Nevertheless, the non-negligible contribution of minerals with higher coercivity suggests variable proportions of hematite along the core. Additionally, we observe non-uniform behavior in magnetite grains, with distinct populations identified through low-temperature measurements of the Verwey transition. Petrographic observations indicate that the original sediment was an Fe-Si mud consisting of a ferrihydrite-silica mixture formed in the water column. This assemblage was rapidly transformed into nano-scale hematite embedded in silica as indicated by a honeycomb structure composed of Si-spherules distributed in a microscale hematite matrix. Textural relationships show that the nucleation of magnetite started during or soon after the formation of hematite, as indicated by the preservation of the Si-spherules within magnetite cores. Further magnetite overgrowth stages are characterized by inclusion-free rims, associated with continuous Si supply during the evolving diagenetic or early metamorphic stages. These findings, combined with existing literature, suggest that ferrihydrite precipitated alongside Si and organic material, later crystallizing as hematite on the seafloor. Anaerobic respiration by Fe(III)-reducing microorganisms likely contributed to early magnetite formation in a fluid-saturated, unconsolidated sediment. Subsequent low-grade metamorphism and Si mobilization led to palisade quartz precipitation and a second stage of magnetite growth likely formed at the expense of matrix hematite through thermochemical Fe(III) reduction. Low-temperature magnetic analyses revealed that the two generations of magnetite core and rim are associated with specific stoichiometry.
条带状铁建造(BIFs)是化学沉积岩,常用于探索前寒武纪海洋的化学性质和氧化还原状态。尽管它们很重要,但关于BIFs中氧化铁结晶途径的许多方面仍受到的限制较少。在本研究中,我们将磁性特征与来自巴西27亿年卡拉雅斯组精细层状BIFs的高分辨率光学和电子成像相结合,以研究它们的性质以及保存古代环境条件的潜力。我们的研究结果表明,以0.1 - 0.5毫米大晶体形式存在的磁铁矿是主要的氧化铁,在所研究的230米序列中,总体平均饱和磁化强度(M)为25 Am/kg(相当于磁铁矿的约27 wt%)。然而,具有较高矫顽力的矿物的不可忽略的贡献表明沿岩心赤铁矿的比例可变。此外,我们观察到磁铁矿颗粒的行为不均匀,通过对韦尔维转变的低温测量确定了不同的群体。岩相学观察表明,原始沉积物是一种铁硅泥,由在水柱中形成的水铁矿 - 二氧化硅混合物组成。如由分布在微米级赤铁矿基质中的硅球组成的蜂窝状结构所示,这种组合迅速转变为嵌入二氧化硅中的纳米级赤铁矿。纹理关系表明磁铁矿的成核始于赤铁矿形成期间或之后不久,如磁铁矿核心内硅球的保存所示。进一步的磁铁矿生长阶段的特征是无包裹体的边缘,这与成岩或早期变质阶段演化过程中硅的持续供应有关。这些发现与现有文献相结合,表明水铁矿与硅和有机物质一起沉淀下来,随后在海底结晶为赤铁矿。铁(III)还原微生物的厌氧呼吸可能促成了流体饱和、未固结沉积物中早期磁铁矿的形成。随后的低级变质作用和硅的迁移导致了栅栏状石英的沉淀,磁铁矿生长的第二阶段可能是通过热化学铁(III)还原以基质赤铁矿为代价形成的。低温磁性分析表明,两代磁铁矿的核心和边缘与特定的化学计量有关。