Confronting Episodic vs. Continuous Heat Sources in Long-Lived Hot Orogens: Insights From Petrochronological Studies in the Nova Venecia Complex, Araçuaí Orogen (SE Brazil)

IF 3.4 2区 地球科学 Q1 GEOLOGY
Lucas R. Schiavetti, Vinicius T. Meira, Sean Mulcahy, Jeffrey D. Vervoort, Peter L. Baker, George L. Luvizotto, Ricardo I. F. Trindade
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Abstract

Orogenic belts that sustain elevated temperatures at intermediate crustal depths for tens of millions of years are known as hot orogens. The evolution of these hot orogens is largely influenced by thermal maturation, primarily driven by the distribution of heat-producing elements (HPEs), such as K, Th and U in the overthickened crust. This process involves widespread anatexis, granulite facies metamorphism, extensive transfer of fluids and magma and large-scale crustal flow. Although most of the thermal evolution of hot orogens is controlled by HPEs, episodic heat transfer may also contribute to their geodynamic development. The Araçuaí orogen, located in southeastern Brazil, represents a Neoproterozoic hot orogen that exposes in its internal domain deeper levels of an overthickened crust, resembling the Tibetan plateau. Its evolution involves more than 120 million years of magmatism and metamorphism, including ultra-high-temperature metamorphism. Different geodynamic models have been suggested to explain the thermal evolution of this orogen, ranging from episodic heat sources within subduction-collisional orogeny to continuous long-lived heat sources in collisional or intracontinental settings. In this paper, we integrate detailed thermodynamic modelling, Lu–Hf and Sm–Nd garnet dating, and U–Pb and REE zircon data from an outcrop that includes granulite facies metasedimentary rocks (Nova Venecia complex) and an intrusive gabbroic stock (São Gabriel pluton). This key outcrop allows us to investigate the history of high-grade regional metamorphism within the internal domain of the Araçuaí orogen, as well as the thermal impact of the late-stage high-temperature magmatism on the later evolution of this hot orogen. Our data indicate that the studied rocks reached near-peak conditions (6.5–10 kbar and ~800°C) at 535–530 Ma and followed a near-isothermal decompression path to 5–6 kbar at ~530–520 Ma. Only local effects of contact metamorphism (~5 kbar and 900°C–1000°C) were observed along the contact between the gabbroic stock and its host rock. Based on this newly integrated dataset and the compilation of existing information, we argue that the Araçuaí orogen evolved from a single, continuous, long-lived heat source controlled by radiogenic decay from HPEs, rather than episodic advective heating from subduction/collision-related processes.

Abstract Image

面对长寿命热造山带的间歇热源与连续热源:来自巴西东南部Araçuaí造山带Nova veneecia杂岩年代学研究的见解
在中间地壳深处维持高温数千万年的造山带被称为热造山带。这些热造山带的演化在很大程度上受热成熟的影响,热成熟主要是由过热地壳中K、Th和U等产热元素的分布所驱动的。这一过程包括广泛的深熔作用、麻粒岩相变质作用、流体和岩浆的广泛转移以及大规模的地壳流动。虽然热造山带的热演化主要受hpe控制,但间歇性的热传递也可能对热造山带的地球动力学发展起作用。它的演化经历了超过1.2亿年的岩浆作用和变质作用,包括超高温变质作用。人们提出了不同的地球动力学模型来解释该造山带的热演化,从俯冲碰撞造山带中的偶发热源到碰撞或陆内环境中的连续长寿命热源。在本文中,我们整合了详细的热力学模拟、Lu-Hf和Sm-Nd石榴石定年、U-Pb和REE锆石数据,这些数据来自一个露头,包括麻粒岩相变质沉积岩(Nova Venecia杂岩)和侵入辉长岩(s o Gabriel岩体)。这一关键的露头使我们能够研究Araçuaí造山带内部域的高级别区域变质史,以及晚期高温岩浆活动对该热造山带后期演化的热影响。研究结果表明,岩石在535 ~530 Ma时达到近峰值状态(6.5 ~ 10 kbar和~800℃),在~530 ~ 520 Ma时达到近等温减压至5 ~ 6 kbar。接触变质作用(~ 5kbar, 900°C ~ 1000°C)仅在辉长岩与寄主岩石接触处发生。基于这一新整合的数据集和现有信息的汇编,我们认为Araçuaí造山带是从一个单一的、连续的、长寿命的热源演化而来的,该热源受HPEs放射性成因衰变的控制,而不是由俯冲/碰撞相关过程产生的偶发性平流加热。
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来源期刊
CiteScore
6.60
自引率
11.80%
发文量
57
审稿时长
6-12 weeks
期刊介绍: The journal, which is published nine times a year, encompasses the entire range of metamorphic studies, from the scale of the individual crystal to that of lithospheric plates, including regional studies of metamorphic terranes, modelling of metamorphic processes, microstructural and deformation studies in relation to metamorphism, geochronology and geochemistry in metamorphic systems, the experimental study of metamorphic reactions, properties of metamorphic minerals and rocks and the economic aspects of metamorphic terranes.
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