Migration and focusing of porphyry deposit-forming fluids through aplitic mush of the Saginaw Hill cupola, Arizona, United States

IF 2 3区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY Frontiers in Earth Science Pub Date : 2024-07-01 DOI:10.3389/feart.2024.1426111
Lawrence C. Carter, Ben J. Williamson
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Abstract

Porphyry-type Cu ± Au ± Mo deposits form in the upper (ca. 2–5 km deep) parts of large, long-lived magmatic-hydrothermal systems in which mineralising fluids are thought to be derived from mid-to shallow-crustal magma chambers. Increasingly, however, magmatic systems are viewed as consisting of mush with minor and transient lenses of magma, with mush being a variably packed framework of crystals with interstitial melt and magmatic volatile phase (MVP). In this context, questions remain as to the source (mainly depth) and mechanisms of transport and focussing of the vast volumes of fluids required for shallow level porphyry-type mineralisation. Even more problematic is a paucity of first-order textural evidence for the presence of mush in magmatic-hydrothermal systems, including those which host porphyry-type deposits. To address this, we have studied the aplitic porphyry cupola of the Saginaw Hill magmatic system, Tuscon, Arizona, United States, where magmatic-hydrothermal features are exceptionally well exposed, including a massive silica cap, quartz unidirectional solidification textures (USTs), stockworks of multiple generations of variably mineralised quartz veins and mineralised miarolitic cavities. From field-to micro-scale textural and geochemical studies, particularly observations of vermiform quartz between earlier generations of magmatic quartz and feldspar, we evidence the development of fluid pathways through mush at the magmatic-hydrothermal transition. These are shown to connect and provide fluids and ore constituents to the mineralised miarolitic cavities and early quartz vein stockworks. We suggest that this process should be considered in all new genetic, exploration and numerical models for porphyry and similar types of magmatic-hydrothermal ore-deposits.
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斑岩矿床形成流体通过美国亚利桑那州萨吉诺山冲天炉的plitic泥浆的迁移和聚焦
斑岩型铜±金±钼矿床形成于大型长寿岩浆-热液系统的上部(约 2-5 千米深),其中成矿流体被认为来自中浅层岩浆室。然而,越来越多的人认为岩浆系统是由岩浆泥和少量瞬时岩浆透镜体组成的,岩浆泥是由晶体和间隙熔体及岩浆挥发相(MVP)组成的不同排列的框架。在这种情况下,浅层斑岩型矿化所需的大量流体的来源(主要是深度)、输送和集中机制仍然存在问题。更成问题的是,岩浆-热液系统(包括斑岩型矿床所在的岩浆-热液系统)中存在泥浆的一阶纹理证据非常缺乏。为了解决这个问题,我们对美国亚利桑那州图斯康的萨吉诺山岩浆系统的斑岩冲天炉进行了研究,在这里岩浆-热液特征暴露得特别明显,包括块状二氧化硅帽、石英单向凝固纹理(UST)、多代可变矿化石英脉的网状结构以及矿化米鲕状空洞。从野外到微观尺度的纹理和地球化学研究,特别是对岩浆石英和长石的前几代之间的蛭石状石英的观察,我们证明了在岩浆-热液转变过程中,流体路径通过蘑菇的发展。研究表明,这些流体通道将流体和矿石成分连接并提供给矿化的混合岩洞和早期的石英脉矿床。我们建议,在斑岩矿床和类似岩浆-热液矿床类型的所有新的遗传、勘探和数值模型中,都应考虑这一过程。
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来源期刊
Frontiers in Earth Science
Frontiers in Earth Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
3.50
自引率
10.30%
发文量
2076
审稿时长
12 weeks
期刊介绍: Frontiers in Earth Science is an open-access journal that aims to bring together and publish on a single platform the best research dedicated to our planet. This platform hosts the rapidly growing and continuously expanding domains in Earth Science, involving the lithosphere (including the geosciences spectrum), the hydrosphere (including marine geosciences and hydrology, complementing the existing Frontiers journal on Marine Science) and the atmosphere (including meteorology and climatology). As such, Frontiers in Earth Science focuses on the countless processes operating within and among the major spheres constituting our planet. In turn, the understanding of these processes provides the theoretical background to better use the available resources and to face the major environmental challenges (including earthquakes, tsunamis, eruptions, floods, landslides, climate changes, extreme meteorological events): this is where interdependent processes meet, requiring a holistic view to better live on and with our planet. The journal welcomes outstanding contributions in any domain of Earth Science. The open-access model developed by Frontiers offers a fast, efficient, timely and dynamic alternative to traditional publication formats. The journal has 20 specialty sections at the first tier, each acting as an independent journal with a full editorial board. The traditional peer-review process is adapted to guarantee fairness and efficiency using a thorough paperless process, with real-time author-reviewer-editor interactions, collaborative reviewer mandates to maximize quality, and reviewer disclosure after article acceptance. While maintaining a rigorous peer-review, this system allows for a process whereby accepted articles are published online on average 90 days after submission. General Commentary articles as well as Book Reviews in Frontiers in Earth Science are only accepted upon invitation.
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