首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Synchronization of the astronomical time scales in the Early Toarcian: A link between anoxia, carbon-cycle perturbation, mass extinction and volcanism
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Synchronization of the astronomical time scales in the Early Toarcian: A link between anoxia, carbon-cycle perturbation, mass extinction and volcanism

机译:The Seakarcian中天文时间尺度的同步:缺氧,碳循环扰动,大规模灭绝和火山之间的联系

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The Late Pliensbachian-Early Toarcian is a pivotal time in the Mesozoic era, marked by pronounced carbon-isotope excursions, biotic crises and major climatic and oceanographic changes. Here we present new high-resolution carbon-isotope and magnetic-susceptibility measurements from an expanded hemipelagic Late Pliensbachian-Early Toarcian section from the Middle Atlas Basin (Morocco). Our new astronomical calibration allows the construction of an orbital time scale based on the 100-kyr eccentricity cycle. The Early Toarcian Polymorphum Zone contains 10 to 10.5 repetitions of the 100-kyr eccentricity both in the carbon-isotope and the magnetic-susceptibility data, leading to an average duration of 1.00 +/- 0.08 myr. We also show that the Late Pliensbachian-Early Toarcian global carbon-cycle perturbation has an average duration of 0.24 +/- 0.02 myr. These durations are comparable to previous astrochronological time scales provided for this time interval in the most complete sections of the Tethyan area, and longer than what has been provided in condensed sections. Anchoring this framework on published radiometric ages and astrochronological time scales, we estimate that the carbon-cycle perturbation of the Late Pliensbachian-Early Toarcian corresponds with the early phase of the Karoo and Chonke Aike large igneous provinces. Likewise, our new age constraints confirm that the Toarcian oceanic anoxic event is synchronous to the main phase of the Ferrar volcanic activity. Thus, these successive and short phases of the volcanic activity may have been at the origin of the successive phases of the mass extinctions observed in marine biotas in the Pliensbachian and Toarcian times. (C) 2018 Elsevier B.V. All rights reserved.
机译:晚普班班女子 - 早期的Toarcian是中生代时代的枢轴时间,由明显的碳 - 同位素短途旅行,生物危机和主要气候和海洋变化而标志着。在这里,我们提出了新的高分辨率碳 - 同位素和来自中间地图集盆地(摩洛哥)的扩展血管骨薄妇女早期Toarcian部分的磁化率测量。我们的新天文校准允许基于100-Kyr偏心循环的轨道时间尺度构建。早期托尔阶区多形同时包含在碳同位素和磁磁化率数据100-KYR偏心10〜10.5重复,导致1.00 +/- 0.08 MYR的平均持续时间。我们还表明,晚普班班女子 - 早期Toarcian全球碳周期扰动的平均持续时间为0.24 +/- 0.02 myr。这些持续时间与在Tethyan地区最完整的部分中为此时间间隔提供的先前的十星影传学时间尺度,并且比在冷凝部分中提供的时间更长。将此框架锚定在发布的辐射尺年和天中作用的时间尺度上,我们估计,普利森巴班女性早期的Toarcian的碳循环扰动与卡罗和Chonke的早期阶段相对应。同样,我们的新时代约束证实,Toarcian海洋缺氧事件与法拉尔火山活动的主阶段同步。因此,这些火山活性的这些连续和短阶段可能已经处于普利森尼亚班卓人和Toarcian时期在海洋生物群中观察到的群众灭绝的连续阶段的起源。 (c)2018年elestvier b.v.保留所有权利。

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