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Holocene 'turn-on' and evolution of the Southern Great Barrier Reef: Revisiting reef cores from the Capricorn Bunker Group

机译:全新世的“开启”与南部大堡礁的演变:重新探访摩ri座邦克集团的礁石核心

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Extensive drilling of the Great Barrier Reef (GBR) in the 70s and 80s illuminated the main factors controlling reef growth during the Holocene. However, questions remain about: (1) the precise nature and timing of reef "turnon" or initiation, (2) whether consistent spatio-temporal patterns occur in the bio-sedimentologic response of the reef to Holocene sea-level rise then stability, and (3) how these factors are expressed in the context of the different evolutionary states (juvenile-mature-senile reefs). Combining 21 new C14-AMS and 146 existing recalibrated radiocarbon and U/Th ages, we investigated the detailed spatial and temporal variations in sedimentary facies and coralgal assemblages in fifteen cores across four reefs (Wreck, Fairfax, One Tree and Fitzroy) from the Southern GBR. Our newly defined facies and assemblages record distinct chronostratigraphic patterns in the cores, displaying both lateral zonation across the different reefs and shallowing upwards sequences, characterised by a transition from deep (Porites/faviids) to shallow (Acropora/Isopora) coral types. The revised reef accretion curves show a significant lag period, ranging from 0.7-2 ka, between flooding of the antecedent Pleistocene substrate and Holocene reef turn-on. This lag period and dominance of more environmentally tolerant early colonizers (e.g., domal Porites and faviids), suggests initial conditions that were unfavourable for coral growth. We contend that higher input of fine siliciclastic material from regional terrigenous sources, exposure to hydrodynamic forces and colonisation in deeper waters are the main factors influencing initially reduced growth and development. All four reefs record a time lag and we argue that the size and shape of the antecedent platform is most important in determining the duration between flooding and recolonisation of the Holocene reef. Finally, our study of Capricorn Bunker Group Holocene reefs suggests that the size and shape of the antecedent substrate has a greater impact on reef evolution and final evolutionary state (mature vs. senile), than substrate depth alone. (C) 2015 Elsevier B.V. All rights reserved.
机译:在70年代和80年代对大堡礁(GBR)进行了广泛的钻探,揭示了全新世期间控制珊瑚礁生长的主要因素。但是,仍然存在以下问题:(1)礁石“开启”或发动的确切性质和时机;(2)礁石对全新世海平面上升然后稳定的生物沉积学反应是否发生一致的时空格局, (3)这些因素在不同的进化状态(幼稚-成熟-老年礁)中如何表达。结合21种新的C14-AMS和146种经过重新校准的放射性碳和U / Th年龄,我们研究了南部四个珊瑚礁(沉船,费尔法克斯,一棵树和菲茨罗伊)的15个岩心中沉积相和珊瑚组合的详细时空变化。 GBR。我们新定义的相和组合在岩心中记录了不同的年代地层模式,既显示了不同礁石的横向带状分布,又显示了浅层向上的序列,其特征是从深部(Porites / Faviids)向浅部(Acropora / Isopora)珊瑚过渡。修改后的礁石吸积曲线显示,在前世更新世基质的泛滥和全新世礁石开启之间有一个显着的滞后周期,范围为0.7-2 ka。这种滞后时期和对环境更加耐受的早期定居者的统治地位(例如,多孔的多孔质和小孔藻),表明不利于珊瑚生长的初始条件。我们认为,来自区域陆源的精细硅质碎屑岩材料的投入较高,受到流体动力的作用以及在深水域的定殖是影响最初减少的生长和发育的主要因素。所有四个珊瑚礁均记录有时间滞后,我们认为,前平台的大小和形状对于确定全新世珊瑚礁的泛滥和重新定殖之间的持续时间最为重要。最后,我们对摩ri座邦克群全新世珊瑚礁的研究表明,前体基质的大小和形状对珊瑚礁的演化和最终进化状态(成熟与衰老)的影响要大于基质本身的深度。 (C)2015 Elsevier B.V.保留所有权利。

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