海洋趋磁细菌布莱克氏磁弧菌产生的磁铁矿中铁同位素分馏

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Vincent Busigny , François P. Mathon , Matthieu Amor , François Guyot , Nicolas Menguy , Christopher T. Lefevre
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引用次数: 0

摘要

趋磁细菌(MTB)具有在细胞内沉淀纳米级磁铁矿的能力。它们的出现可能可以追溯到太古宙早期(例如3 Ga),但迄今尚未提供如此悠久历史的证据。岩石记录中的MTB鉴定依赖于磁化石,残余的磁铁矿晶体可能及时存活于岩石变形和低变质作用中。提出了若干标准,如大小、形状和磁性,以区分磁化石与其他磁铁矿来源。最近对淡水菌株Magnetospirillum magneticum AMB-1的实验工作表明,铁同位素组成是一个有希望的附加标准,但需要提供不同MTB菌株及其磁铁矿的同位素表征,以评估铁同位素特征的稳健性,以用于古生物应用。在本研究中,我们研究了海洋菌株黑氏磁弧菌MV-1在不同条件下,考察了铁浓度(50、100和150 μM)和氧化还原态(铁(II)-抗坏血酸盐或铁(III)-柠檬酸盐)对细菌生物矿化的影响,并确定了相关的铁同位素分异。我们的研究结果证实,相对于之前在AMB-1中观察到的细菌生长培养基,轻铁同位素更倾向于掺入磁铁矿。通过Rayleigh精馏模拟生长介质和磁铁矿同位素组成的演化,得到铁同位素分馏(Δ56Fegrowth medium-magnetite = Δ56Fegrowth medium- δ56Femagnetite)范围为0.2 ~ 0.9‰,平均值为0.55(±0.35)‰。该同位素分馏与铁浓度或氧化还原状态无明显关系。重要的是,生物磁铁矿的轻铁同位素富集与非生物沉淀形成的磁铁矿的同位素特征形成对比,后者富集重同位素。这表明铁同位素可以作为地球或地外样品中磁化石识别的生物特征。最后,与先前在AMB-1上获得的结果相反,MV-1磁铁矿中没有检测到57Fe(相对于54Fe, 56Fe和58Fe)的特异性富集,我们可以通过两菌株之间铁收支的差异来解释这一点。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Iron isotope fractionation in magnetite produced by the marine magnetotactic bacterium Magnetovibrio blakemorei
Magnetotactic bacteria (MTB) possess the ability to precipitate intracellular nanosized magnetite. Their emergence may date back to the early Archean (e.g. 3 Ga) but evidence of such a long history has yet to be provided. MTB identification in the rock record relies on magnetofossils, the residual magnetite crystals that may survive in time to rock deformation and low-grade metamorphism. Several criteria such as size, shape and magnetic properties have been proposed to distinguish magnetofossils from other magnetite sources. Recent experimental work on the freshwater strain Magnetospirillum magneticum AMB-1 revealed that Fe isotope composition represents a promising additional criterion, but isotopic characterization of distinct MTB strains and of their magnetite needs to be provided to evaluate the robustness of iron isotope signatures for paleontological applications. In the present work, we investigate the marine strain Magnetovibrio blakemorei MV-1 under various conditions selected to examine the influence of Fe concentration (50, 100 and 150 μM) and redox state (Fe(II)-ascorbate or Fe(III)-citrate) on bacterial biomineralization and determine associated Fe isotope fractionations. Our results confirm the preferential incorporation of light iron isotopes into magnetite relative to the bacterial growth medium previously observed in AMB-1. Modeling the evolution of the growth medium and magnetite isotope compositions by Rayleigh distillation process yields iron isotope fractionations (i.e. Δ56Fegrowth medium-magnetite = δ56Fegrowth medium − δ56Femagnetite) ranging between 0.2 and 0.9 ‰ with a mean value of 0.55 (±0.35) ‰. This isotope fractionation shows no clear relation with iron concentration or redox state. Importantly, the enrichment in light iron isotope of biological magnetite contrasts with the isotopic characteristics of magnetite formed by abiotic precipitation, the latter being enriched in heavy isotopes. This suggests that Fe isotopes could be used as a biosignature for magnetofossils identification in terrestrial or extraterrestrial samples. Finally, in contrast with previous results obtained on AMB-1, no specific enrichment of 57Fe (relative to 54Fe, 56Fe and 58Fe) could be detected in MV-1 magnetite, which we interpret by differences in iron budgets between the two strains.
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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