Radiogenic 182W and 142Nd anomalies in a 2.7 Ga old basaltic lava flow indicate long-term preservation of early mantle heterogeneities

IF 5.2 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Geochimica et Cosmochimica Acta Pub Date : 2026-06-15 Epub Date: 2026-03-31 DOI:10.1016/j.gca.2026.03.044
Jan L. Hellmann , Igor S. Puchtel , Vinciane Debaille , Janne Blichert-Toft , Richard J. Walker
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引用次数: 0

Abstract

Understanding the origin and preservation of early mantle heterogeneities is essential for reconstructing Earth’s accretion and early differentiation history. This can be investigated using the short-lived 146Sm–142Nd and 182Hf–182W isotope systems, which provide insights into large-scale differentiation processes through 142Nd and 182W anomalies in Earth’s oldest rocks. In this study, we present 182W data for Theo’s Flow, a thick, differentiated, mafic–ultramafic flow of tholeiitic affinity, as well as 147Sm–143Nd, 176Lu–176Hf, and 187Re–187Os isotope data and trace element concentrations, including highly siderophile elements, for Theo’s Flow and closely spatially and temporally associated Pyke Hill komatiites, both from the ∼2.7 Ga old Kidd-Munro Assemblage of the Abitibi greenstone belt, Ontario, Canada. Theo’s Flow samples are characterized by an average µ182W value of +6.7±2.7, which, together with the previously reported positive µ142Nd anomaly of +6.8±2.5, indicate long-term survival of mantle domains resulting from magmatic differentiation early in Earth’s history. If it is assumed that the bulk silicate Earth evolved with a suprachondritic Sm/Nd ratio, anomalies for both elements can be explained by a single silicate differentiation event at ∼4.54 Ga. Alternatively, if the bulk silicate Earth evolved with a chondritic Sm/Nd ratio, a model fractionation age of ∼4.45 Ga is obtained. In this case, due to extinction of 182Hf by that time, the 182W anomaly would have to have been generated by another process, such as derivation from a mantle source characterized by a deficit in late accreted materials. Regardless of the timing of the early silicate differentiation, the preservation of both 182W and 142Nd anomalies in the 2.7 Ga old rocks highlights the survival of early-formed mantle domains for nearly 1.8 Gyr after Earth’s formation. Comparison of isotopic and chemical data for Theo’s Flow with those for the Pyke Hill and Boston Creek komatiites, which were argued to have all been derived from melting in a single mantle plume, provides evidence for the survival of early mantle heterogeneities on a plume scale.
2.7 Ga古玄武岩熔岩流放射性成因182W和142Nd异常表明早期地幔非均质长期保存
了解早期地幔非均质性的起源和保存是重建地球增生和早期分异史的必要条件。这可以使用寿命较短的146sm - 142和182Hf-182W同位素系统进行研究,该系统通过地球最古老岩石的142和182W异常,提供了对大规模分化过程的见解。在这项研究中,我们获得了来自加拿大安大略省阿比提比绿岩带 ~ 2.7 Ga old Kidd-Munro组合的Theo’s Flow的182W数据,以及Theo’s Flow和Pyke Hill komatiites的147Sm-143Nd、176Lu-176Hf和187Re-187Os的同位素数据和微量元素浓度,其中包括高度亲铁元素,这些元素均与时空密切相关。Theo’s Flow是一个厚的、分异的、具有拉斑岩亲和性的基性-超基性流。Theo’s Flow样品的平均µ182W值为 + 6.7 ± 2.7,加上之前报道的 + 6.8 ± 2.5的正µ142Nd异常,表明地球历史早期岩浆分化导致的地幔域长期存在。如果假定块状硅酸盐地球以超球粒质Sm/Nd比演化,则这两种元素的异常可以用 ~ 4.54 Ga的单一硅酸盐分化事件来解释。另外,如果块状硅酸盐地球以球粒状Sm/Nd比演化,则模型分馏年龄为 ~ 4.45 Ga。在这种情况下,由于182Hf在那个时候已经消失,182W的异常可能是由另一个过程产生的,比如源自一个以晚期吸积物质亏损为特征的地幔源。无论早期硅酸盐分异发生的时间如何,2.7 Ga古岩石中182W和142Nd异常的保存表明,早形成的地幔域在地球形成后近1.8 Gyr存在。西奥流的同位素和化学数据与派克山和波士顿溪科马提岩的同位素和化学数据进行比较,为早期地幔非均质在地幔柱尺度上的存在提供了证据。派克山和波士顿溪科马提岩被认为都是来自于单一地幔柱的融化
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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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