Klaver Martijn, Carey Steven, Nomikou Paraskevi, Smet Ingrid, Godelitsas Athanasios, Vroon Pieter
Department of Geology and Geochemistry Vrije Universiteit Amsterdam Amsterdam Netherlands; Now at Bristol Isotope Group, School of Earth Sciences University of Bristol Bristol UK.
Graduate School of Oceanography University of Rhode Island Kingston Rhode Island USA.
Geochem Geophys Geosyst. 2016 Aug;17(8):3254-3273. doi: 10.1002/2016GC006398. Epub 2016 Aug 16.
This study reports the first detailed geochemical characterization of Kolumbo submarine volcano in order to investigate the role of source heterogeneity in controlling geochemical variability within the Santorini volcanic field in the central Aegean arc. Kolumbo, situated 15 km to the northeast of Santorini, last erupted in 1650 AD and is thus closely associated with the Santorini volcanic system in space and time. Samples taken by remotely-operated vehicle that were analyzed for major element, trace element and Sr-Nd-Hf-Pb isotope composition include the 1650 AD and underlying K2 rhyolitic, enclave-bearing pumices that are nearly identical in composition (73 wt.% SiO, 4.2 wt.% KO). Lava bodies exposed in the crater and enclaves are basalts to andesites (52-60 wt.% SiO). Biotite and amphibole are common phenocryst phases, in contrast with the typically anhydrous mineral assemblages of Santorini. The strong geochemical signature of amphibole fractionation and the assimilation of lower crustal basement in the petrogenesis of the Kolumbo magmas indicates that Kolumbo and Santorini underwent different crustal differentiation histories and that their crustal magmatic systems are unrelated. Moreover, the Kolumbo samples are derived from a distinct, more enriched mantle source that is characterized by high Nb/Yb (>3) and low Pb/Pb (<18.82) that has not been recognized in the Santorini volcanic products. The strong dissimilarity in both petrogenesis and inferred mantle sources between Kolumbo and Santorini suggests that pronounced source variations can be manifested in arc magmas that are closely associated in space and time within a single volcanic field.
本研究报告了科伦波海底火山的首次详细地球化学特征,以调查源区不均一性在控制爱琴海中弧圣托里尼火山区地球化学变化方面的作用。科伦波位于圣托里尼东北15公里处,最后一次喷发于公元1650年,因此在时空上与圣托里尼火山系统密切相关。通过遥控潜水器采集的样本,分析了其主量元素、微量元素以及Sr-Nd-Hf-Pb同位素组成,这些样本包括公元1650年喷发的火山灰以及其下伏的含包体流纹质浮岩,它们的成分几乎相同(SiO₂含量为73 wt.%,K₂O含量为4.2 wt.%)。火山口暴露的熔岩体和包体为玄武岩到安山岩(SiO₂含量为52 - 60 wt.%)。黑云母和角闪石是常见的斑晶相,这与圣托里尼典型的无水矿物组合形成对比。科伦波岩浆成因过程中角闪石分异和下地壳基底同化的强烈地球化学特征表明,科伦波和圣托里尼经历了不同的地壳分异历史,它们的地壳岩浆系统没有关联。此外,科伦波样本源自一个独特的、更富集的地幔源区,其特征是高Nb/Yb(>3)和低²⁰⁶Pb/²⁰⁴Pb(<18.82),这在圣托里尼火山产物中未被识别。科伦波和圣托里尼在岩浆成因和推断的地幔源区方面的强烈差异表明,明显的源区变化可以在一个单一火山区内时空上紧密相关的弧岩浆中表现出来。