首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Determining accurate temperature-time paths from U-Pb thermochronology: An example from the Kaapvaal craton, southern Africa
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Determining accurate temperature-time paths from U-Pb thermochronology: An example from the Kaapvaal craton, southern Africa

机译:从U-Pb热年代学确定准确的温度-时间路径:以非洲南部Kaapvaal克拉通为例

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摘要

Thermochronology has revolutionized our understanding of the establishment and evolution of lithospheric thermal structure. However, many potential benefits provided by the application of diffusion theory to thermochronology have yet to be fully exploited. This study uses apatite (T-c = 450-550 degrees C) and titanite (T-c = 550-650 degrees C) U-Pb ID-TIMS thermochronology at the single- to sub-grain scale to separate the variable effects of volume diffusion of Ph from metamorphic (over)growth above and below the T, of a mineral. Data are presented from two ca. 3227 Ma tonalite samples from north and south of the Barberton Greenstone Belt (BGB), southern Africa. Two distinct populations of apatite from a sample north of the BGB record fast cooling followed by metamorphic growth similar to 10 Myr later. Both apatite and titanite dates from south of the BGB show a strong correlation with the grain size and record 100 Myr of post-emplacement cooling. Complex core-rim zoning observed in cathodoluminescence images of apatite is interpreted to reflect metamorphic overgrowth above the T-c. The age and topology of grain size versus date curves from titanite and apatite are used in combination with a finite-difference numerical model to show that slow, non-linear, cooling and not thermal resetting is responsible for the observed distribution. The thermal histories from either side of the BGB are very different and provide unique insight into the BGB's tectonic evolution: a similar to 70 Myr period of apparent stability after ca. 3.2 Ga terrane assembly was followed by fast exhumation south of the BGB that led to lower-crustal melting and intrusion of granitic batholiths ca. 3.14-3.10 Ga. (c) 2006 Elsevier Inc. All rights reserved.
机译:热年代学彻底改变了我们对岩石圈热结构建立和演化的理解。然而,将扩散理论应用于热年代学所提供的许多潜在好处尚未得到充分开发。这项研究使用磷灰石(Tc = 450-550摄氏度)和钛铁矿(Tc = 550-650摄氏度)U-Pb ID-TIMS热年代学在单晶粒度至亚晶粒度范围内分离Ph的体积扩散的可变影响来自矿物T之上和之下的变质(过度)生长。数据来自两个ca。来自南非南部巴伯顿绿岩带(BGB)北部和南部的3227 Ma斜纹岩样本。来自BGB北部样本的两个不同的磷灰石种群记录了快速冷却,随后发生了类似于10 Myr的变质生长。 BGB南部的磷灰石和钛矿日期均与晶粒大小密切相关,并记录了放置后冷却的100 Myr。在磷灰石的阴极发光图像中观察到的复杂的核-边缘区带被解释为反映了T-c上方的变质过度生长。钛铁矿和磷灰石的晶粒尺寸与日期曲线的年龄和拓扑结构与有限差分数值模型结合使用,显示出缓慢,非线性,冷却而不是热复位是观察到的分布的原因。 BGB两侧的热史是非常不同的,它们为BGB的构造演化提供了独特的见解:类似于大约20 Myr后的70 Myr明显稳定期。 3.2 Ga地形组装后,BGB以南快速发掘,导致地壳下部熔融和花岗岩基底岩侵入。 3.14-3.10 Ga。(c)2006 Elsevier Inc.保留所有权利。

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