澳大利亚悉尼盆地二叠纪末“死区”(252.10±0.06 Ma)铁氧化还原和铁种类的变化:来自x射线吸收光谱的证据

Vivi Vajda , Kajsa G.V. Sigfridsson Clauss , Ashley Krüger , Susan Nehzati
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引用次数: 0

摘要

二叠纪末的大灭绝事件可以追溯到澳大利亚的几个非海洋盆地。悉尼盆地的岩性演替以煤层到泥岩和砂岩的变化为特征,记录了二叠纪植被消失后的主要环境变化。在最上层的二叠纪煤层和泥岩之间有几毫米厚的富含铁的“锈”层,这一层横向延伸穿过盆地,在南极洲的同时期演替中也有记录。该层被1.5 m厚的Frazer Beach段覆盖,其基底10 cm厚的微角砾岩层由99%的高岭石和石英组成,其年代为252.10±0.06 Ma。弗雷泽海滩成员对应于所谓的二叠纪末“死区”,缺乏化石花粉和树叶。这个独特的成员是在二叠纪泥炭形成森林灭绝后直接沉积的。在这里,我们通过x射线吸收光谱发现,在消光区间内,随着铁的还原量的增加,出现了剧烈的氧化还原位移,其次是高度氧化的铁,最类似于铁(III)与有机物的络合。随后,年轻样本中的值通过“死区”正常化,氧化还原水平仅略高于事件发生前。事件层中的有机络合铁与标准的苏万尼河黄腐酸一致,是一种与有机物结合的酸性铁络合物,而消光层上下样品的产谱主要类似于磁铁矿(Fe3O4)矿物相。我们认为,标志灭绝间隔的铁氧化还原波动与大灭绝后有机质积累的显著环境变化有关。消光层中高度还原的铁可能与细菌降解释放的甲烷或笼形物的排放物有关。富铁灭绝层中黄腐酸的存在表明,植物物质、脂质和氢氧化钙(CaOH)的降解过程突然开始,导致了这一“死亡层”的形成。接下来是数百万年的侵蚀环境,新的复杂植被才得以形成。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Changes in Fe-redox and Fe-species across the end-Permian ‘Dead Zone’ in the Sydney Basin, Australia (252.10 ± 0.06 Ma): Evidence from X-ray absorption spectroscopy

The end-Permian mass extinction event is traceable across several non-marine basins in Australia. In the Sydney Basin, the lithological succession is characterized by a change from coal seams to mudstones and sandstones, recording a major environmental change following the disappearance of the Permian vegetation. A few millimeter-thick iron-rich ‘rusty’ layer occurs between the uppermost Permian coal seam and the mudstone, a layer that extends laterally across the basin and which has also been documented from coeval successions in Antarctica. This layer is overlain by the <1.5-m-thick Frazer Beach Member, whose basal 10-cm-thick microbreccia bed comprises 99% kaolinite and quartz, and is dated as 252.10 ± 0.06 Ma. The Frazer Beach Member corresponds to the so-called end-Permian ‘Dead Zone’ lacking fossil pollen and leaves. This distinctive member was deposited directly following the extinction of the Permian peat-forming forests.

Here we identify, through X-ray absorption spectroscopy, a drastic redox shift across the extinction interval with increasing amount of reduced Fe-species followed by highly oxidized Fe-species, most resembling Fe(III) complexed with organic matter. Values subsequently normalise in younger samples through the ‘Dead Zone’, attaining only slightly higher redox-levels than before the event. The organically complexed Fe-species in the event bed is consistent with the standard Suwannee River fulvic acid, an acid Fe-complex with iron bound to organic matter, whereas the samples above and below the extinction layer yield spectra predominantly resembling magnetite (Fe3O4) mineral phase. We consider that the iron redox fluctuation marking the extinction interval is related to significant environmental changes with accumulation of organic matter following the mass extinction. The highly reduced iron in the extinction layer may relate to methane release from bacterial degradation, or emissions from clathrates. The presence of fulvic acid in the distinct iron-rich extinction layer indicates that an abrupt onset of the process of degradation of plant matter, lipids and calcium hydroxide (CaOH) took place, resulting in this ‘Death layer’. This was followed by millions of years of erosive conditions before new, complex vegetation could establish.

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