Prolonged Multi-Phase Magmatism Due To Plume-Lithosphere Interaction as Applied to the High Arctic Large Igneous Province

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geochemistry Geophysics Geosystems Pub Date : 2024-06-20 DOI:10.1029/2023GC011380
Björn H. Heyn, Grace E. Shephard, Clinton P. Conrad
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Abstract

The widespread High Arctic Large Igneous Province (HALIP) exhibits prolonged melting over more than 50 Myr, an observation that is difficult to reconcile with the classic view that large igneous provinces (LIPs) originate from melting in plume heads. Hence, the suggested plume-related origin and classification of HALIP as a LIP have been questioned. Here, we use numerical models that include melting and melt migration to investigate a rising plume interacting with lithosphere of variable thickness, that is, a basin-to-craton setting applicable to the Arctic. Models reveal that melt migration introduces significant spatial and temporal variations in melt volumes and pulses of melt production, including protracted melting for at least about 30–40 Myr, because of the dynamic feedback between migrating melt and local lithosphere thinning. For HALIP, plume material deflected from underneath the Greenland craton can re-activate melting zones below the previously plume-influenced Sverdrup Basin after a melt-free period of about 10–15 Myr, even though the plume is already ∼500 km away. Hence, actively melting zones do not necessarily represent the location of the deeper plume stem at a given time, especially for secondary pulses. Additional processes such as (minor) plume flux variations or local lithospheric extension may alter the timing and volume of HALIP pulses, but are to first order not required to reproduce the long-lived and multi-pulse magmatism of HALIP. Since melting zones are always plume-fed, we would expect HALIP magmatism to exhibit plume-related trace element signatures throughout time, potentially shifting from mostly tholeiitic toward more alkalic compositions.

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应用于北极高纬度大火成岩带的岩浆柱-岩石圈相互作用导致的长时间多相岩浆活动
广泛分布的北极高纬度大型火成岩带(HALIP)表现出超过50 Myr的长时间熔融,这一观察结果很难与大型火成岩带(LIPs)起源于羽流头部熔融的传统观点相一致。因此,与羽流有关的起源以及将HALIP归类为LIP的观点受到了质疑。在这里,我们利用包括熔融和熔融迁移的数值模型,研究了上升的羽流与厚度可变的岩石圈相互作用的情况,即适用于北极地区的海盆-地壳背景。模型显示,由于熔体迁移和局部岩石圈变薄之间的动态反馈,熔体迁移会带来熔体量和熔体生成脉冲的显著时空变化,包括至少约 30-40 Myr 的长期熔化。就 HALIP 而言,从格陵兰陨石坑下方偏转过来的羽流物质,在大约 10-15 Myr 的无熔化期之后,可以重新激活先前受羽流影响的斯维尔德鲁普盆地下方的熔化区,尽管羽流已经在 500 km 之外。因此,活跃的熔化带并不一定代表特定时间内更深羽流干的位置,尤其是对次级脉冲而言。额外的过程,如(轻微的)羽流通量变化或局部岩石圈的延伸,可能会改变HALIP脉冲的时间和数量,但对于再现HALIP的长寿命和多脉冲岩浆活动来说,一阶是不需要的。由于熔融带总是由羽流哺育的,我们预计 HALIP 岩浆活动在整个时间段内都会表现出与羽流相关的痕量元素特征,有可能从主要是透辉石成分转向更多的碱性成分。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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