Precambrian mantle metasomatism preserved by the Nd-Hf isotopic compositions of modern HIMU-type intraplate basalts

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Leonie Sieger , Bradley J. Peters , Andrea Giuliani , Maria Schönbächler
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Abstract

The presence of HIMU (high-238U/204Pb) signatures in ocean island basalts has long been used to argue that ancient oceanic crust has been tectonically recycled into the mantle sources of plume-derived volcanic hotspots such as St. Helena or Mangaia. However, alternative hypotheses regarding the origins of HIMU signatures have also been put forward. This study addresses the origins of HIMU-like Pb isotopic signatures in Isla Isabel, a small (∼1 km2) intraplate volcanic island located off the western coast of México, southeast of the southern tip of Baja California. The Nd-Hf isotopic signatures of Isla Isabel are nearly identical to the classical HIMU-type hotspots St. Helena and Mangaia; however, the physical and geochemical characteristics of Isla Isabel are inconsistent with the derivation of its lavas from deeply recycled oceanic crust. We argue that Isla Isabel lavas were instead produced by mixing of local depleted mantle and continental lithospheric mantle that experienced a prior enrichment event, likely in a ≥ 600 Ma-old paleo-subduction setting. Such preservation of ancient tectonic events is remarkable, since the exposed geological record in continental México preserves only a limited record of geological events older than the Mexican Cordillera (<165 Ma). Isla Isabel, therefore, illustrates that the origins of HIMU-type intraplate lavas are not limited to ancient recycled oceanic crust. Rather, they can also preserve information about the evolution of the upper mantle through large-scale tectonic cycles, even when these events have been otherwise erased from the surficial rock record.
现代himu型板内玄武岩Nd-Hf同位素组成对前寒武纪地幔交代作用的保存
海洋岛屿玄武岩中存在的高238u /204Pb (high-238U/204Pb)特征长期以来一直被用来论证古代海洋地壳已经被构造再循环到圣赫勒拿或曼盖亚等羽状火山热点的地幔源中。然而,关于HIMU信号起源的其他假设也被提出。这项研究解决了伊莎贝尔岛(Isla Isabel)类似himu的Pb同位素特征的起源,伊莎贝尔岛是一个小的(~ 1平方公里)板内火山岛,位于下加利福尼亚州南端东南的msamuxico西海岸外。伊莎贝尔岛的Nd-Hf同位素特征与经典的himu型热点St. Helena和Mangaia几乎相同;然而,伊莎贝尔岛的物理和地球化学特征与它的岩浆来自深海再循环海洋地壳的起源不一致。我们认为伊莎贝尔岛熔岩是由本地衰竭地幔和大陆岩石圈地幔混合形成的,这些岩石圈地幔经历了先前的富集事件,可能是在≥600 ma的古俯冲背景下形成的。这种对古代构造事件的保存是值得注意的,因为暴露在m西科大陆的地质记录只保存了比墨西哥科迪勒拉(165 Ma)更早的地质事件的有限记录。因此,伊莎贝尔岛的发现说明了himu型板内熔岩的起源并不局限于古代海洋地壳的再循环。相反,它们还可以保存上地幔通过大规模构造循环演变的信息,即使这些事件已经从地表岩石记录中抹去。
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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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