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Association Internationale pour l'Étude des Argiles 国际粘土研究协会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.207
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引用次数: 0
Earth’s Earliest Crust 地球最早的地壳
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.168
J. O’Neil, H. Rizo, Jesse Reimink, Marion Garçon, Richard W. Carlson
The scarcity of rocks preserved from the first billion years (Gy) of Earth’s history hinders our ability to study the nature of the earliest crust. Rare >4.0-Gy-old zircons confirm that felsic crust was present within 500 million years of Earth’s formation. Given that most of that ancient crust has been destroyed, geochemical and isotopic tracers applied to rocks from the oldest sections of continents can be used to provide insights into the nature of the predecessor crust. Evidence from Earth’s oldest rocks and minerals suggests multiple early mantle depletion episodes, possibly linked to the formation of an initial, dominantly mafic, crust. This early crust was the precursor to evolved rocks that now constitute considerable portions of Earth’s oldest surviving crust.
地球历史上最初十亿年(Gy)保存下来的岩石很少,这阻碍了我们研究最早地壳性质的能力。罕见的大于 4.0-Gy 的锆石证实,在地球形成的 5 亿年内曾出现过长石地壳。鉴于古代地壳的大部分已被破坏,对来自大陆最古老地段的岩石使用地球化学和同位素示踪剂,可以帮助我们深入了解前生地壳的性质。来自地球最古老岩石和矿物的证据表明,早期地幔发生过多次耗竭,这可能与最初的、以岩浆岩为主的地壳的形成有关。这种早期地壳是进化岩石的前身,而进化岩石现在构成了地球现存最古老地壳的相当大一部分。
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引用次数: 3
Scientific Laws and Myths, Ockham’s Razor, and Multiple Working Hypotheses 科学定律与神话、奥卡姆剃刀和多重工作假设
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.150
S. McLennan
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引用次数: 0
Embracing Craton Complexity at Depth 深入了解克拉通的复杂性
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.187
Catherine M. Cooper, Meghan S. Miller
Variations within individual cratons, as well as across different cratons, are readily apparent at the Earth’s surface, providing indirect insight into the processes governing the formation and evolution of the underlying regions. However, our views at depth are more limited. As such, there is a risk of interpreting the cratonic lithosphere as a monolith. Recent modeling and advances in seismological imaging have enhanced our perspective of vertical variations within the cratonic lithosphere, which has helped build a general conceptual model. While lateral variations also are increasingly identified, their significance still presents unanswered questions. In this review, we summarize the current state of knowledge of cratonic lithospheric structure and demonstrate the importance of lateral heterogeneity in craton evolution and stability.
在地球表面,各个陨石坑内部以及不同陨石坑之间的变化一目了然,这让我们可以间接地了解底层区域的形成和演变过程。然而,我们在深处的视野却比较有限。因此,我们有可能将板块岩石圈理解为一个整体。最近的建模和地震成像技术的进步增强了我们对板块岩石圈内部垂直变化的认识,有助于建立一个总体概念模型。虽然横向变化也被越来越多地识别出来,但其意义仍是一个未解之谜。在这篇综述中,我们总结了对板块岩石圈结构的认识现状,并论证了横向异质性在板块演化和稳定性中的重要性。
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引用次数: 2
Early—and Future—Planetary Environments 早期和未来行星环境
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.147
Janne Blichert-Toft
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引用次数: 0
European Mineralogical Union 欧洲矿物学联盟
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.211
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引用次数: 0
Archean Cratons: Time Capsules of the Early Earth 阿基坦地壳:早期地球的时间胶囊
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.162
Carol D. Frost, Paul A. Mueller
Studies of Archean cratons, and the rocks and minerals they contain, help us understand the processes that occurred on the early Earth, our place in the Solar System, and how the planet we live on today came to be. The articles in this issue examine different aspects of early Earth evolution from multiple perspectives relying on both theory and observation. We hope they will encourage you to investigate further this most fascinating time in Earth history. Here we introduce the basic characteristics of cratons, the challenges of inferring Earth evolution from the sparse Archean rock record, the concept of cratonic clans, the development of supercratons, and, by the end of the Archean, continents, supercontinents, and plate tectonics.
对阿尔川陨石坑及其所含岩石和矿物的研究有助于我们了解早期地球的演化过程、我们在太阳系中的位置以及我们今天生活的地球是如何形成的。本期的文章从理论和观察两个方面,从多个角度探讨了早期地球演化的不同方面。我们希望这些文章能鼓励你进一步研究地球历史上这段最迷人的时期。在这里,我们将介绍陨石坑的基本特征、从稀少的阿新世岩石记录中推断地球演化所面临的挑战、陨石坑群的概念、超陨石坑的发展,以及到阿新世末期的大陆、超大陆和板块构造。
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引用次数: 1
At the Dawn of Continents: Archean Tonalite-Trondhjemite-Granodiorite Suites 大陆的曙光始新世黑云母-透辉石-花岗闪长岩套石
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.174
Oscar Laurent, M. Guitreau, E. Bruand, J. Moyen
Archean rocks of the tonalite-trondhjemite-granodiorite (TTG) suite are dominant constituents of Earth’s earliest preserved silicic crust, while conversely rare in Phanerozoic continental crust. Their formation represents the first critical step towards the construction and preservation of continents. Formation of most TTG magmas involved partial melting of hydrous, probably silicified, mafic rocks at various depths (20–50 km, possibly up to 100 km). Many possible tectonic scenarios fit the petrological and geochemical constraints on TTG formation, whether compatible with a global plate tectonic-like regime or not. Refining such scenarios is a major challenge that requires systematically integrating the constraints on TTG formation—relying especially on accessory minerals as key petrogenetic tools—with the geological context on a regional scale.
奥新纪岩石中的tonalite-trondhjemite-granodiorite(TTG)套件是地球上最早保存下来的硅质地壳的主要成分,而在新生代大陆地壳中却很少见。它们的形成代表了建造和保存大陆的关键第一步。大多数TTG岩浆的形成涉及含水岩(可能是硅化岩体)在不同深度(20-50千米,最深可能达100千米)的部分熔融。许多可能的构造方案都与 TTG 形成的岩石学和地球化学制约因素相吻合,无论是否与全球板块构造体系相一致。完善这些方案是一项重大挑战,需要将 TTG 形成的制约因素(尤其是作为关键岩石成因工具的附属矿物)与区域范围的地质背景系统地结合起来。
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引用次数: 4
The Quest for Extraterrestrial Cratons 探索地外环形山
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.152
Vicki L. Hansen
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引用次数: 0
Archean Geodynamics Underneath Weak, Flat, and Flooded Continents 软弱、平坦和洪水泛滥大陆下的全新纪地球动力学
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-01 DOI: 10.2138/gselements.20.3.180
Patrice F. Rey, N. Coltice, Nicolas Flament
Although a significant volume of crust was extracted from the mantle early in Earth’s history, the contribution of felsic rocks to the sedimentary record was minimal until ~3.0 Ga. On a hotter Earth, this conundrum dissipates if we consider that the felsic crust was buried under thick basaltic covers, continents were flooded by a near-global ocean, and the crust was too weak to sustain high mountains, making it largely unavailable to erosion. Gravitational forces destabilized basaltic covers within these weak, flat, and flooded continents, driving intra-crustal tectonics and forcing episodic subduction at the edges of continents. Through secular cooling, this dual-mode geodynamics progressively transitioned to plate tectonics.
虽然在地球历史的早期有大量地壳从地幔中被提取出来,但在约3.0 Ga之前,长岩对沉积记录的贡献微乎其微。在一个更热的地球上,如果我们考虑到长岩地壳被掩埋在厚厚的玄武岩覆盖之下,大陆被近乎全球的海洋淹没,地壳过于薄弱,无法支撑高山,使其在很大程度上无法被侵蚀,那么这个难题就会迎刃而解。重力破坏了这些薄弱、平坦和被洪水淹没的大陆内部玄武岩覆盖层的稳定性,推动了地壳内部构造,并迫使大陆边缘发生偶发性俯冲。通过世俗冷却,这种双模式地球动力学逐渐过渡到板块构造。
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引用次数: 2
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