吉布斯岛和布鲁斯滩的高难熔成岩形成及其在环南极大陆演化中的作用

N. Akizawa, A. Yamaguchi, K. Tani, A. Ishikawa, Ryo Fujita, S. Choi
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引用次数: 1

摘要

大陆边缘具有深远的意义,因为它记录了造山岩浆的增生和随后的大陆裂谷作用。由于含水流体输入导致的高度地幔熔融预计会同时刺激大陆生长,并比更肥沃的地幔降低地幔的固有密度,这反过来又将大陆岩石圈与对流地幔隔离开来。吉布斯岛(南设得兰群岛)和德雷克海峡布鲁斯滩的地幔橄榄岩为我们了解环南极地区的构造历史提供了线索。为了阐明南极大陆生长过程,我们收集了来自吉布斯岛和布鲁斯滩的8个泥质岩的地球化学数据,包括Re-Os同位素和高亲铁元素组成。由反长花岗岩+水辉石或蜥蜴石(燃烧损失= LOI范围为3 ~ 34 wt.%)所证明的黑钨矿受蛇纹石化影响严重,但含有原生自面状至亚面状铬铁矿,有或没有球形包裹体。铬铁矿很少形成透镜状的聚集体。在吉布斯岛发现的一种含新鲜橄榄石颗粒的灰岩,充填在铬铁矿的裂缝中,LOI值较低(3 wt.%),表明它是由前体蛇纹石化的灰岩形成的。其中,吉布斯岛灰岩的Mg/Si = 1.4 ~ 1.6, Al/Si = 0.004 ~ 0.01,布鲁斯滩灰岩的Mg/Si = 0.66, Al/Si = 0.008,灰岩的主要元素组成高度贫化,与弧前橄榄岩组成域重叠。Re/ Ir-LOI空间的正相关证实了后期蛇纹石化过程中Re的输入。溶质的187Os/188Os比值在0.11907 ~ 0.14493之间。吉布斯岛的显生宙再枯竭(熔体枯竭)年龄约为535 ~ 129ma,除中元古代再枯竭年龄约为1.2 Ga外。由于存在与蛇纹石化有关的Re扰动,这些年龄提供了熔体耗尽事件的最小时间估计。推断早古生代熔体枯竭发生在南极半岛形成的早期,是对冈瓦纳边缘板块收敛的响应,而中元古代再枯竭年龄反映了对流地幔非均质性,与附近的任何地壳形成事件无关。铬铁矿的岩石学特征和高贫质粒的性质归因于俯冲带背景下的熔融-橄榄岩反应。一种可行的解释是,地幔经历了两个阶段的熔融,最后阶段发生在俯冲带背景下的冈瓦纳大陆边缘。由此产生的高度难熔的岩石圈地幔后来在冈瓦纳破裂期间移位和分散。其广泛存在可能是由于沿大陆边缘的多阶段熔体耗损所致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Highly refractory dunite formation at Gibbs Island and Bruce Bank, and its role in the evolution of the circum-Antarctic continent
The continental margin is of profound importance as it records continental growth by accretion of orogenic magmas and following continental rifting. A high degree of mantle melting due to hydrous fluid input is expected to simultaneously stimulate continental growth and lower the intrinsic density of the mantle than more fertile mantle, which in turn isolates the continental lithosphere from the convective mantle. The mantle peridotites from Gibbs Island (South Shetland Islands) and Bruce Bank in the Drake Passage provide us an insight into the tectonic history in the circum-Antarctic region. To elucidate the continental growth of Antarctica, we present geochemical data of eight dunites from Gibbs Island and one dunite from Bruce Bank, including Re–Os isotope and highly siderophile element compositions. The dunites are severely affected by serpentinization as evidenced by antigorite + brucite or lizardite (loss on ignition = LOI ranging from 3 to 34 wt.%) but contain primary euhedral to subhedral chromites with or without spherical inclusions. The chromites rarely form lens-shaped aggregates. A dunite from Gibbs Island contains fresh olivine grains filling a fracture in the chromite with low LOI (3 wt.%), indicating a deserpentinization origin from a precursor serpentinized dunite. The dunites show highly depleted bulk-rock major element compositions (Mg/Si = 1.4–1.6 and Al/Si = 0.004–0.01 for Gibbs Island dunites, Mg/Si = 0.66 and Al/Si = 0.008 for Bruce Bank dunite), overlapping a compositional field defined by forearc peridotites. The positive correlation in Re/Ir–LOI space corroborates Re input during the later serpentinization process. The 187Os/188Os ratios of the dunites range from 0.11907 to 0.14493. Phanerozoic Re-depletion (melt depletion) ages of ca. 535–129 Ma are recorded in the Gibbs Island dunites, except for one with a Mesoproterozoic Re-depletion age of ca. 1.2 Ga. Since there exists serpentinization-related perturbation of Re, the ages provide minimum time estimates for melt depletion events. The early Paleozoic melt depletion is inferred to have occurred at a very early stage of Antarctic Peninsula formation in response to plate convergence along the margin of Gondwana, whereas the Mesoproterozoic Re-depletion age reflects convecting mantle heterogeneity unrelated to any nearby crust-forming events. The petrographic characteristics of the chromites and highly depleted nature of the dunites are attributed to melt–peridotite reaction in a subduction zone setting. A feasible interpretation for the dunite formation is that the mantle had experienced two stages of melting with the final stage occurring along the Gondwana continental margin in the subduction zone setting. Resultant highly refractory lithospheric mantle was later displaced and dispersed during the Gondwana breakup. Widespread existence of the dunite may be attributed to multi-stage melt depletion along the continental margin.
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