Fractionation of radiogenic Pb isotopes in meteorites and their components induced by acid leaching

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yuri Amelin, Qing-Zhu Yin, Piers Koefoed, Renaud Merle, Yuki Hibiya, Magdalena H. Huyskens, Tsuyoshi Iizuka, Julia A. Cartwright
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Abstract

In this study we test the possibility that radiogenic 207Pb/206Pb ratios (207Pb*/206Pb*) in meteorites can be fractionated during partial dissolution, and explore the consequences of this fractionation for Pb-isotope chronology of meteorites. We report the results of experiments tailored to detect Pb-isotope fractionation, induced by partial dissolution through acid leaching, in plutonic angrite Northwest Africa (NWA) 4801 and ungrouped achondrites NWA 10132 and Erg Chech (EC) 002. We also re-examine previously published U-Pb data for other achondrites and for Ca-Al-rich refractory inclusions (CAIs), to seek evidence of such fractionation. We observe that, in primitive achondrite NWA 10132, differences in 207Pb*/206Pb* ratios, corresponding to the age bias of ca. 1–2 Ma, exist between the 0.5 M hydrofluoric acid leachates of pyroxene or crushed rock, and the residues after such leaching. In angrite NWA 4801, similar acid treatment of pyroxene separates did not cause a resolvable age bias. In EC 002, three steps of partial dissolution in 0.2 M – 5 M HF caused irregular 207Pb*/206Pb* fractionation between leaching steps, and generally higher 207Pb*/206Pb* ratios in the residues than in HF leachates. These age biases were observed in leaching pairs with highly radiogenic Pb, and cannot be explained by mixing between radiogenic Pb, primordial Pb, and Pb introduced by terrestrial contamination. Instead, the observed isotope fractionation is attributed to the combined effects of the size difference between α-recoil tracks in the decay chains of 238U and 235U, and exsolution of primary pigeonite, leading to the formation of a lamellar structure consisting of augite and low-Ca pyroxene by either slow-cooling or subsequent metamorphic reactions. Where extensive acid leaching intended for removal of non-radiogenic Pb causes fractionation of radiogenic Pb isotopes, its detrimental effect can be reversed by performing a numeric recombination of partial leachate and residue data. Currently, it is unclear how common leaching-induced isotopic fractionation is in Pb-isotopic chronology to meteoritic materials. Acid leaching is an essential step for removal of non-radiogenic Pb in the precise Pb-isotopic dating of meteorites, which currently does not have viable alternatives. However, it is important to be aware of its possible side effects, and to continue search for new non-radiogenic Pb removal techniques that do not cause radiogenic 207Pb* and 206Pb* fractionation.
酸浸出诱导陨石及其成分中放射性铅同位素的分馏
在这项研究中,我们测试了陨石中放射性 207Pb/206Pb 比率(207Pb*/206Pb*)在部分溶解过程中分馏的可能性,并探讨了这种分馏对陨石铅同位素年代学的影响。我们报告了在西北非岩浆岩(NWA)4801 和未成组的隐陨石 NWA 10132 和 Erg Chech(EC)002 中,为探测通过酸浸出部分溶解引起的铅同位素分馏而定制的实验结果。我们还重新研究了以前公布的其他隐晶岩和富钙铝难熔包裹体(CAIs)的 U-Pb 数据,以寻找这种分馏的证据。我们观察到,在原始闪长岩 NWA 10132 中,辉石或碎屑岩的 0.5 M 氢氟酸浸出液与浸出后的残留物之间存在 207Pb*/206Pb* 比率差异,对应于约 1-2 Ma 的年龄偏差。在 NWA 4801 辉绿岩中,对辉石分离物进行类似的酸处理并没有造成可解决的年龄偏差。在 EC 002 中,在 0.2 M - 5 M HF 中分三步进行部分溶解,导致浸出步骤之间出现不规则的 207Pb*/206Pb* 分馏,残留物中的 207Pb*/206Pb* 比率普遍高于 HF 浸出液中的 207Pb*/206Pb* 比率。这些年龄偏差是在高放射性铅的浸出对中观察到的,不能用放射性铅、原始铅和陆地污染引入的铅之间的混合来解释。相反,观察到的同位素分馏现象是由于 238U 和 235U 衰变链中 α 反弹轨迹之间的尺寸差异,以及原生鸽血石的外溶,通过缓慢冷却或随后的变质反应形成了由奥氏体和低钙辉石组成的片状结构的综合影响造成的。如果为去除非放射性铅而进行的大量酸浸出会导致放射性铅同位素的分馏,则可通过对部分浸出液和残留物数据进行数值重组来扭转其不利影响。目前,还不清楚沥滤引起的同位素分馏在陨石材料的铅同位素年代学中的普遍程度。在对陨石进行精确的铅同位素年代测定时,酸浸出是去除非放射源铅的重要步骤,目前还没有可行的替代方法。然而,重要的是要注意其可能产生的副作用,并继续寻找不会导致 207Pb* 和 206Pb* 辐射分馏的新的非辐射性铅去除技术。
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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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