新生代从不稳定性停滞地壳逐渐过渡到现代板块构造体系

IF 2.6 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Journal of the Geological Society Pub Date : 2024-05-23 DOI:10.1144/jgs2024-023
Jean H. Bédard
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Basal anatexis of ASOL ∼40-50 km thick (or melting within down-drips) could generate tonalite-trondhjemite melts (TTGs) and create proto-continental nuclei, while garnet pyroxenite restites delaminate into the mantle. With further reworking, low-K tonalitic rocks would remelt to produce granodiorite and granite, completing the transfer of radioactive elements out of the lower crust. Mantle overturns would generate large-scale lateral currents in the upper mantle that would push against Archaean-aged sub-continental lithospheric mantle keels, causing continental drift and orogenesis despite the absence of plate-boundary forces like slab pull. The validity of this is corroborated by the observed displacement of Lakshmi Planum (>1000 Km) on Venus, a planet with no arcs or ridges. Recent models suggest the Abitibi Greenstone Belt formed as an oceanic tract behind a detached ribbon continent during partial breakup of the Southern Superior craton; and represents a possible sample of Archaean oceanic lithosphere. The Abitibi has ∼50 km of apparent stratigraphy composed of 2-10 My mafic-felsic bimodal volcanic cycles that follow assimilation-fractionation trends indicating contamination of mantle-derived basalts with TTG-like anatectites derived from older basalts. ASOL of this type would be difficult to subduct because of its weakness and buoyancy, but would be fertile and could generate large amounts of second-stage melts. There are no sheeted dykes, precluding a seafloor-spreading model, while the absence of basal cumulates or attached mantle means this type of ASOL should not be called an ophiolite. Archaean/Proterozoic unconformities are followed by deposition of Fe-formations, clastic and volcanic rocks that are only rarely affected by sagduction. The increase in siliciclastic input and decreasing sagduction reflect near-global late Archean emergence from the water of stiffening granitic continents due to secular cooling and intra-continental differentiation. Albeit associated with continent-derived siliciclastic debris, many Paleo-Proterozoic volcanic (and plutonic) rocks resemble Archaean ones geochemically. The similarity of magmatic rocks and hot orogenic styles in the Archaean and Paleo-Proterozoic could imply the overall geodynamic regime was similar in both. The Siderian-Rhyacian\n Quiet Period\n could therefore represent a Stagnant Lid phase that followed the 2.5 Ga Archaean overturn. When the next mantle overturn ruptured the lid at ∼2.2-2.0 Ga (and again at ∼1.9-1.8 Ga), continents would have been set into motion, forming arcs and ridges. Once initiated, arc and ridge segments would have needed to multiply and propagate to create a world-girdling system. Meso-Proterozoic rocks preserve clear evidence of plate mobility, subduction, and orogenesis; but inexplicably, ophiolites, the geological record of seafloor-spreading, are extremely rare prior to 1 Ga. Earth at 2.0 Ga was probably still largely covered by ASOL, possibly similar to the Abitibi, but how and where it was all destroyed and replaced by modern oceanic lithosphere are mysteries. Given the volume of ASOL involved, recognizable by-products of this global-scale reworking process should exist. Voluminous anorthosite-mangerite-charnockite-granite/gabbro suite rocks (AMCG) are mostly of Proterozoic age, requiring either an ephemeral source, or a unique process. Trace element inversion models applied to massif anorthosites imply they crystallized from high-La/Yb melts that do not resemble tholeiitic basalts, invalidating the notion that they are floatation cumulates from basaltic underplates. Model anorthosite-forming melts can, however, be explained by high-pressure melting of an ASOL-like basalt source with garnet-bearing residues. I posit that massif anorthosites record destruction at Proterozoic convergent margins of an ephemeral source: ASOL. When the last ASOL was crushed between converging continents or consumed by an overprinting arc (∼0.8-1 Ga), AMCG rocks ceased to form, and Earth became a modern Plate Tectonic planet.\n","PeriodicalId":17320,"journal":{"name":"Journal of the Geological Society","volume":null,"pages":null},"PeriodicalIF":2.6000,"publicationDate":"2024-05-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A gradual Proterozoic transition from an Unstable Stagnant Lid to the modern Plate Tectonic system\",\"authors\":\"Jean H. 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Basal anatexis of ASOL ∼40-50 km thick (or melting within down-drips) could generate tonalite-trondhjemite melts (TTGs) and create proto-continental nuclei, while garnet pyroxenite restites delaminate into the mantle. With further reworking, low-K tonalitic rocks would remelt to produce granodiorite and granite, completing the transfer of radioactive elements out of the lower crust. Mantle overturns would generate large-scale lateral currents in the upper mantle that would push against Archaean-aged sub-continental lithospheric mantle keels, causing continental drift and orogenesis despite the absence of plate-boundary forces like slab pull. The validity of this is corroborated by the observed displacement of Lakshmi Planum (>1000 Km) on Venus, a planet with no arcs or ridges. Recent models suggest the Abitibi Greenstone Belt formed as an oceanic tract behind a detached ribbon continent during partial breakup of the Southern Superior craton; and represents a possible sample of Archaean oceanic lithosphere. The Abitibi has ∼50 km of apparent stratigraphy composed of 2-10 My mafic-felsic bimodal volcanic cycles that follow assimilation-fractionation trends indicating contamination of mantle-derived basalts with TTG-like anatectites derived from older basalts. ASOL of this type would be difficult to subduct because of its weakness and buoyancy, but would be fertile and could generate large amounts of second-stage melts. There are no sheeted dykes, precluding a seafloor-spreading model, while the absence of basal cumulates or attached mantle means this type of ASOL should not be called an ophiolite. Archaean/Proterozoic unconformities are followed by deposition of Fe-formations, clastic and volcanic rocks that are only rarely affected by sagduction. The increase in siliciclastic input and decreasing sagduction reflect near-global late Archean emergence from the water of stiffening granitic continents due to secular cooling and intra-continental differentiation. Albeit associated with continent-derived siliciclastic debris, many Paleo-Proterozoic volcanic (and plutonic) rocks resemble Archaean ones geochemically. The similarity of magmatic rocks and hot orogenic styles in the Archaean and Paleo-Proterozoic could imply the overall geodynamic regime was similar in both. The Siderian-Rhyacian\\n Quiet Period\\n could therefore represent a Stagnant Lid phase that followed the 2.5 Ga Archaean overturn. When the next mantle overturn ruptured the lid at ∼2.2-2.0 Ga (and again at ∼1.9-1.8 Ga), continents would have been set into motion, forming arcs and ridges. Once initiated, arc and ridge segments would have needed to multiply and propagate to create a world-girdling system. 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引用次数: 0

摘要

地球上的板块构造始于何时,之前发生了什么?已发表的热机械地幔演化模型暗示,成分和大小与地球和金星相似的行星的早期历史应该以持续3000万至1亿年的周期性地幔翻转为特征,其间相隔1亿至300亿年的稳定盖层阶段。我认为将其描述为 "不稳定的停滞盖 "最为恰当,因为这个术语捕捉到了这类世界的 "杰基尔和海德 "双重性,即在地幔翻转之间的 "停滞盖 "阶段和翻转期间的 "移动盖 "阶段交替出现。地幔翻转上涌区将重塑并重新浮出大片先前存在的哈代地壳和以玄武岩为主的阿尔川式海洋岩石圈(ASOL)。厚度为40-50千米的ASOL的基底厌氧(或下滴熔融)可能会产生黑云母-透辉石熔体(TTGs),并形成原大陆核,同时石榴石辉石复原体脱层进入地幔。随着进一步的再加工,低K tonalitic岩石将重熔生成花岗闪长岩和花岗岩,完成放射性元素从下地壳的转移。地幔翻转会在上地幔中产生大规模的侧向流,推动太古宙时期的次大陆岩石圈地幔龙骨,导致大陆漂移和造山运动,尽管没有板块拉力等板块边界力。在没有弧或脊的金星上观测到的拉克希米平面位移(>1000 千米)证实了这一观点的正确性。最近的模型表明,阿比提比绿岩带是在南苏必利尔陨石坑部分解体过程中,在一个分离的带状大陆后面形成的大洋带;它可能是太古宙大洋岩石圈的一个样本。阿比提比地区有长达 50 公里的表观地层,由 2-10 My 的黑云母-长石双峰火山岩循环组成,这些火山岩循环遵循同化-分馏趋势,表明地幔衍生玄武岩受到了来自较古老玄武岩的 TTG 类闪长岩的污染。这种类型的 ASOL 由于其软弱性和浮力而难以俯冲,但却很肥沃,可以产生大量的第二阶段熔体。由于没有片状岩堤,因此不存在海底扩张模式,而没有基底堆积物或附着地幔意味着这种类型的ASOL不应该被称为蛇绿岩。古生代/新生代的非地层沉积之后是铁成岩、碎屑岩和火山岩的沉积,这些岩石很少受到陷落作用的影响。硅质岩输入的增加和矢状侵蚀的减少,反映了近全球范围内的晚阿新世由于持续冷却和大陆内部分异而从变硬的花岗岩大陆水中出现。尽管与来自大陆的硅质碎屑有关,但许多古近原生代火山岩(和柱状火山岩)在地球化学上与太古宙的火山岩(和柱状火山岩)相似。太古代和古近原生代岩浆岩和热造山运动方式的相似性可能意味着两者的整体地球动力机制相似。因此,Siderian-Rhyacian安静期可能代表了2.5Ga太古宙地幔翻转之后的停滞期。当下一次地幔翻转在 2.2-2.0 Ga(1.9-1.8 Ga)时使盖层破裂时,大陆将开始运动,形成弧和脊。弧和脊一旦开始运动,就需要成倍增加和传播,以形成一个环绕世界的系统。中新生代岩石保留了板块移动、俯冲和造山运动的明显证据;但令人费解的是,蛇绿岩--海底扩张的地质记录--在 1 Ga 之前极为罕见。地球在 2.0 Ga 时可能仍主要被 ASOL 所覆盖,可能类似于阿比提比,但它是如何以及在哪里被全部摧毁并被现代海洋岩石圈所取代却是个谜。考虑到所涉及的ASOL的体积,这一全球规模的再加工过程应该存在可识别的副产品。大量的正长岩-芒硝-黝帘石-花岗岩/辉长岩(AMCG)大多是新生代岩石,需要一个短暂的来源或一个独特的过程。应用于块状正长岩的微量元素反演模型表明,它们是由与透辉玄武岩不相似的高la/Yb熔体结晶而成的,这就否定了它们是玄武岩底板浮积物的说法。然而,形成正长岩的熔体模型可以通过高压熔化带有含石榴石残留物的类似 ASOL 的玄武岩源来解释。我假定,地块正长岩记录了新近纪汇聚边缘对一种短暂来源的破坏:ASOL。当最后一个ASOL被挤压在会聚的大陆之间或被叠加弧吞噬(∼0.8-1 Ga)时,AMCG岩石就不再形成,地球就成为了一个现代板块构造行星。
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A gradual Proterozoic transition from an Unstable Stagnant Lid to the modern Plate Tectonic system
When did Plate Tectonics begin on Earth, and what preceded it? Published thermo-mechanical mantle evolution models imply that the early history of planets with a composition and size similar to Earth and Venus should be characterized by periodic mantle overturns of 30-100 million years duration, separated by stable lid phases of 100-300 My. I argue this is best described as an Unstable Stagnant Lid, because this term captures the Jekyll-and-Hyde duality of such worlds, which alternate between a Stagnant Lid ss phase between mantle overturns, and a Mobile Lid phase during overturns. Mantle overturn upwelling zones would rework and resurface large tracts of pre-existing Hadean crust and basalt-dominated Archean-Style Oceanic Lithosphere (ASOL). Basal anatexis of ASOL ∼40-50 km thick (or melting within down-drips) could generate tonalite-trondhjemite melts (TTGs) and create proto-continental nuclei, while garnet pyroxenite restites delaminate into the mantle. With further reworking, low-K tonalitic rocks would remelt to produce granodiorite and granite, completing the transfer of radioactive elements out of the lower crust. Mantle overturns would generate large-scale lateral currents in the upper mantle that would push against Archaean-aged sub-continental lithospheric mantle keels, causing continental drift and orogenesis despite the absence of plate-boundary forces like slab pull. The validity of this is corroborated by the observed displacement of Lakshmi Planum (>1000 Km) on Venus, a planet with no arcs or ridges. Recent models suggest the Abitibi Greenstone Belt formed as an oceanic tract behind a detached ribbon continent during partial breakup of the Southern Superior craton; and represents a possible sample of Archaean oceanic lithosphere. The Abitibi has ∼50 km of apparent stratigraphy composed of 2-10 My mafic-felsic bimodal volcanic cycles that follow assimilation-fractionation trends indicating contamination of mantle-derived basalts with TTG-like anatectites derived from older basalts. ASOL of this type would be difficult to subduct because of its weakness and buoyancy, but would be fertile and could generate large amounts of second-stage melts. There are no sheeted dykes, precluding a seafloor-spreading model, while the absence of basal cumulates or attached mantle means this type of ASOL should not be called an ophiolite. Archaean/Proterozoic unconformities are followed by deposition of Fe-formations, clastic and volcanic rocks that are only rarely affected by sagduction. The increase in siliciclastic input and decreasing sagduction reflect near-global late Archean emergence from the water of stiffening granitic continents due to secular cooling and intra-continental differentiation. Albeit associated with continent-derived siliciclastic debris, many Paleo-Proterozoic volcanic (and plutonic) rocks resemble Archaean ones geochemically. The similarity of magmatic rocks and hot orogenic styles in the Archaean and Paleo-Proterozoic could imply the overall geodynamic regime was similar in both. The Siderian-Rhyacian Quiet Period could therefore represent a Stagnant Lid phase that followed the 2.5 Ga Archaean overturn. When the next mantle overturn ruptured the lid at ∼2.2-2.0 Ga (and again at ∼1.9-1.8 Ga), continents would have been set into motion, forming arcs and ridges. Once initiated, arc and ridge segments would have needed to multiply and propagate to create a world-girdling system. Meso-Proterozoic rocks preserve clear evidence of plate mobility, subduction, and orogenesis; but inexplicably, ophiolites, the geological record of seafloor-spreading, are extremely rare prior to 1 Ga. Earth at 2.0 Ga was probably still largely covered by ASOL, possibly similar to the Abitibi, but how and where it was all destroyed and replaced by modern oceanic lithosphere are mysteries. Given the volume of ASOL involved, recognizable by-products of this global-scale reworking process should exist. Voluminous anorthosite-mangerite-charnockite-granite/gabbro suite rocks (AMCG) are mostly of Proterozoic age, requiring either an ephemeral source, or a unique process. Trace element inversion models applied to massif anorthosites imply they crystallized from high-La/Yb melts that do not resemble tholeiitic basalts, invalidating the notion that they are floatation cumulates from basaltic underplates. Model anorthosite-forming melts can, however, be explained by high-pressure melting of an ASOL-like basalt source with garnet-bearing residues. I posit that massif anorthosites record destruction at Proterozoic convergent margins of an ephemeral source: ASOL. When the last ASOL was crushed between converging continents or consumed by an overprinting arc (∼0.8-1 Ga), AMCG rocks ceased to form, and Earth became a modern Plate Tectonic planet.
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来源期刊
Journal of the Geological Society
Journal of the Geological Society 地学-地球科学综合
CiteScore
6.00
自引率
3.70%
发文量
68
审稿时长
6-12 weeks
期刊介绍: Journal of the Geological Society (JGS) is owned and published by the Geological Society of London. JGS publishes topical, high-quality recent research across the full range of Earth Sciences. Papers are interdisciplinary in nature and emphasize the development of an understanding of fundamental geological processes. Broad interest articles that refer to regional studies, but which extend beyond their geographical context are also welcomed. Each year JGS presents the ‘JGS Early Career Award'' for papers published in the journal, which rewards the writing of well-written, exciting papers from early career geologists. The journal publishes research and invited review articles, discussion papers and thematic sets.
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