{"title":"辉长岩及其组成矿物中238U/235U同位素变化","authors":"Magdalena H. Huyskens , Yuri Amelin , Qing-Zhu Yin , Tsuyoshi Iizuka","doi":"10.1016/j.gca.2025.04.030","DOIUrl":null,"url":null,"abstract":"<div><div>Ages of angrites, a diverse and rapidly growing group of differentiated meteorites, are important for understanding the history of their parent body, which is proposed to be an archetypal first-generation planetesimal. Angrites also commonly serve as a time reference in the early Solar System chronology. Pb-isotopic ages of angrites can be determined with high precision, and the isotopic composition of uranium thus becomes a major contributor to the age accuracy and its total uncertainty budget. Two main groups of angrites, the rapidly cooled (volcanic and/or impact-generated) and plutonic angrites, were previously found to contain uranium with different <sup>238</sup>U/<sup>235</sup>U ratios. The variations in isotopic compositions between mineral carriers of uranium within individual angrites, which are directly relevant to calculation of accurate Pb-isotopic ages, have not been studied yet. In this study, we determined the <sup>238</sup>U/<sup>235</sup>U for whole rocks, leachate and residue of whole rocks and mineral separates for two rapidly cooled angrites D’Orbigny and Sahara 99555 and three plutonic angrites NWA 4801, NWA 4590 and Angra dos Reis. For the rapidly cooled angrites, all mineral separates as well as the whole rocks show consistent <sup>238</sup>U/<sup>235</sup>U. Whole rock <sup>238</sup>U/<sup>235</sup>U ratios for the plutonic angrites are distinctly lower than the ratios in the rapidly cooled angrites. In Angra dos Reis and NWA 4590, merrillite has higher <sup>238</sup>U/<sup>235</sup>U than pyroxene, and both minerals have higher <sup>238</sup>U/<sup>235</sup>U ratios than the respective whole rock, suggesting the presence of an unidentified mineral host of uranium with lower <sup>238</sup>U/<sup>235</sup>U. These differences in U isotope composition could be possibly attributed to a combination of mass dependent and mass-independent isotope fractionation driven by the differences of oxidation state, and coordination in the crystals. We recalculated the existing Pb-isotopic dates when possible with the measured <sup>238</sup>U/<sup>235</sup>U for the minerals that were used for the Pb-isotopic dating. The differences in U isotopic composition between cogenetic minerals point to the importance of <sup>238</sup>U/<sup>235</sup>U determination in specific minerals that are used for Pb-isotopic dating for plutonic achondrites, rather than U isotopic data for bulk meteorites.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"399 ","pages":"Pages 205-220"},"PeriodicalIF":4.5000,"publicationDate":"2025-05-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"238U/235U isotopic variations in angrites and their constituent minerals\",\"authors\":\"Magdalena H. 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The variations in isotopic compositions between mineral carriers of uranium within individual angrites, which are directly relevant to calculation of accurate Pb-isotopic ages, have not been studied yet. In this study, we determined the <sup>238</sup>U/<sup>235</sup>U for whole rocks, leachate and residue of whole rocks and mineral separates for two rapidly cooled angrites D’Orbigny and Sahara 99555 and three plutonic angrites NWA 4801, NWA 4590 and Angra dos Reis. For the rapidly cooled angrites, all mineral separates as well as the whole rocks show consistent <sup>238</sup>U/<sup>235</sup>U. Whole rock <sup>238</sup>U/<sup>235</sup>U ratios for the plutonic angrites are distinctly lower than the ratios in the rapidly cooled angrites. In Angra dos Reis and NWA 4590, merrillite has higher <sup>238</sup>U/<sup>235</sup>U than pyroxene, and both minerals have higher <sup>238</sup>U/<sup>235</sup>U ratios than the respective whole rock, suggesting the presence of an unidentified mineral host of uranium with lower <sup>238</sup>U/<sup>235</sup>U. These differences in U isotope composition could be possibly attributed to a combination of mass dependent and mass-independent isotope fractionation driven by the differences of oxidation state, and coordination in the crystals. We recalculated the existing Pb-isotopic dates when possible with the measured <sup>238</sup>U/<sup>235</sup>U for the minerals that were used for the Pb-isotopic dating. 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引用次数: 0
摘要
安格氏陨石是一种多样化且快速增长的分化陨石群,其年龄对于理解其母体的历史具有重要意义,该母体被认为是原型的第一代星子。在早期太阳系年表中,安格力岩通常也作为时间参考。长石的pb同位素年龄可以高精度地确定,而铀的同位素组成则成为年龄精度及其总不确定预算的主要贡献者。两类主要的安格尔岩,快速冷却的(火山和/或撞击产生的)和深成安格尔岩,先前被发现含有不同238U/235U比例的铀。单个铀矿石中铀矿物载体之间同位素组成的变化与精确pb同位素年龄的计算直接相关,但尚未得到研究。本文对2个快速冷却的长辉石D 'Orbigny和Sahara 99555以及3个深冲长辉石NWA 4801、NWA 4590和Angra dos Reis进行了全岩、渗滤液、全岩残渣和矿物分离物的238U/235U测定。对于快速冷却的辉长岩,所有矿物分离物以及整个岩石均表现出一致的238U/235U。深成矿辉长岩的全岩238U/235U比值明显低于快速冷却辉长岩。在Angra dos Reis和NWA 4590中,merrillite的238U/235U高于辉石,且两者的238U/235U比值均高于各自的整体岩石,表明存在一种不明铀矿体,其238U/235U较低。这些U同位素组成的差异可能是由于晶体中氧化态和配位的差异所驱动的质量依赖和质量独立同位素分选的结合。在可能的情况下,我们重新计算了现有的铅同位素日期,并测量了用于铅同位素定年的矿物的238U/235U。同生矿物之间铀同位素组成的差异表明,在特定矿物中测定238U/235U的重要性,这些矿物用于深部无球粒陨石的铅同位素测年,而不是用于大块陨石的U同位素数据。
238U/235U isotopic variations in angrites and their constituent minerals
Ages of angrites, a diverse and rapidly growing group of differentiated meteorites, are important for understanding the history of their parent body, which is proposed to be an archetypal first-generation planetesimal. Angrites also commonly serve as a time reference in the early Solar System chronology. Pb-isotopic ages of angrites can be determined with high precision, and the isotopic composition of uranium thus becomes a major contributor to the age accuracy and its total uncertainty budget. Two main groups of angrites, the rapidly cooled (volcanic and/or impact-generated) and plutonic angrites, were previously found to contain uranium with different 238U/235U ratios. The variations in isotopic compositions between mineral carriers of uranium within individual angrites, which are directly relevant to calculation of accurate Pb-isotopic ages, have not been studied yet. In this study, we determined the 238U/235U for whole rocks, leachate and residue of whole rocks and mineral separates for two rapidly cooled angrites D’Orbigny and Sahara 99555 and three plutonic angrites NWA 4801, NWA 4590 and Angra dos Reis. For the rapidly cooled angrites, all mineral separates as well as the whole rocks show consistent 238U/235U. Whole rock 238U/235U ratios for the plutonic angrites are distinctly lower than the ratios in the rapidly cooled angrites. In Angra dos Reis and NWA 4590, merrillite has higher 238U/235U than pyroxene, and both minerals have higher 238U/235U ratios than the respective whole rock, suggesting the presence of an unidentified mineral host of uranium with lower 238U/235U. These differences in U isotope composition could be possibly attributed to a combination of mass dependent and mass-independent isotope fractionation driven by the differences of oxidation state, and coordination in the crystals. We recalculated the existing Pb-isotopic dates when possible with the measured 238U/235U for the minerals that were used for the Pb-isotopic dating. The differences in U isotopic composition between cogenetic minerals point to the importance of 238U/235U determination in specific minerals that are used for Pb-isotopic dating for plutonic achondrites, rather than U isotopic data for bulk meteorites.
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.