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Kristina Hippe Tiemen Gordijn Vincenzo Picotti Irka Hajdas John D. Jansen Marcus Christl Christof Vockenhuber Colin Maden Naki Akçar Susan Ivy-Ochs 《地球表面变化过程与地形》2019,44(3):766-780
Determining sediment transfer times is key to understanding source-to-sink dynamics and the transmission of environmental signals through the fluvial system. Previous work on the Bolivian Altiplano applied the in situ cosmogenic 14C-10Be-chronometer to river sands and proposed sediment storage times of ~10–20 kyr in four catchments southeast of Lake Titicaca. However, the fidelity of those results hinges upon isotopic steady-state within sediment supplied from the source area. With the aim of independently quantifying sediment storage times and testing the 14C-10Be steady-state assumption, we dated sediment storage units within one of the previously investigated catchments using radiocarbon dating, cosmogenic 10Be-26Al isochron burial dating, and 10Be-26Al depth-profile dating. Palaeosurfaces appear to preserve remnants of a former fluvial system, which has undergone drainage reversal, reduction in catchment area, and local isostatic uplift since ~2.8 Ma. From alluvium mantling the palaeosurfaces we gained a deposition age of ~580 ka, while lower down fluvial terraces yielded ≤34 ka, and floodplains ~3–1 ka. Owing to restricted channel connectivity with the terraces and palaeosurfaces, the main source of channel sediment is via reworking of the late Holocene floodplain. Yet modelling a set of feasible scenarios reveals that floodplain storage and burial depth are incompatible with the 14C-10Be disequilibrium measured in the channel. Instead we propose that the 14C-10Be offset results from: (i) non-uniform erosion whereby deep gullies supply hillslope-derived debris; and/or (ii) holocene landscape transience associated with climate or human impact. The reliability of the 14C-10Be chronometer vitally depends upon careful evaluation of sources of isotopic disequilibrium in a wide range of depositional and erosional landforms in the landscape. © 2018 John Wiley & Sons, Ltd. 相似文献
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The I-Xe chronometer is based upon decay of now-extinct 129I where the ratio of accumulated daughter 129Xe to stable 127I reflects the iodine isotopic ratio at closure of the host mineral. Since none of the parent remains, I-Xe is by nature a relative chronometer but, when referenced by a standard mineral of known age, the I-Xe system becomes an absolute chronometer reflecting true closure times. Most iodine hosts are secondary minerals so the I-Xe system is unique in providing details of post-formational chronometry not readily available with other chronometers. The short half-life of 129I gives it exceptional precision. However, the secondary nature of iodine host minerals, combined with the inherent precision of I-Xe, were responsible for a large database of “whole-rock” I-Xe ages that were not easily interpreted. As this problem evolved historically, doubts were cast upon the viability of the I-Xe system as a chronometer which persisted until it was tested against other chronometers in single-mineral systems. Properly calibrated, absolute I-Xe ages reflect the true closure time of the host minerals, and sequences of closure times in different hosts provide cooling rates for the parent object. 相似文献
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利用LA-ICP-MS在16μm和10μm激光束斑条件下测定独居石U-Th-Pb年龄 总被引：1，自引：1，他引：0
独居石是一种常用的地质年代计,但其内部结构复杂,常具有不同成分分区,只有足够小的激光束斑才能获得地质意义明确的U-Th-Pb年龄。本文在优化ICP-MS参数、匹配两路载气流量(Ar和He)的基础上,设计了两组激光剥蚀条件实验,获得适用于小束斑独居石U-Th-Pb定年的激光剥蚀参数(16μm,3 J/cm~2,5 Hz)和(10μm,3 J/cm2,4 Hz)。在此条件下分别测定标准样品44069和未知样品15SLS-01,获得标准样品44069的~(208)Pb/~(232)Th和~(206)Pb/~(238)U值的单点测试精度小于3%,其U-Th-Pb年龄结果与前人测得SHRIMP U-Pb年龄和TIMS U-Pb年龄一致;未知样品15SLS-01的208Pb/232Th值的单点测试精度小于3%,~(206)Pb/~(238)U值的单点测试精度介于3%~8%,多点测试~(206)Pb-~(238)U和~(208)Pb-~(232)Th的加权平均年龄在误差范围内一致,其中208Pb-232Th年龄更具代表性。本研究表明在16μm和10μm激光束斑下,利用LA-ICP-MS能够实现独居石U-Th-Pb年龄的测定,极大地提高了独居石此种微区定年方法的空间分辨率。 相似文献
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Laser ablation inductively coupled plasma mass spectrometry analyses of U–Pb isotopes and trace elements in zircon and titanite were carried out on epoxy mounts and thin sections for ultrahigh‐pressure (UHP) eclogite in association with paragneiss in the Dabie orogen. The results provide a direct link between metamorphic ages and temperatures during continental subduction‐zone metamorphism. Zircon U–Pb dating gives two groups of concordant ages at 242 ± 2 to 239 ± 5 Ma and 226 ± 2 to 224 ± 6 Ma, respectively. The Triassic zircon U–Pb ages are characterized by flat heavy rare earth element (HREE) patterns typical of metamorphic growth. Ti‐in‐zircon thermometry for the two generations of metamorphic zircon yields temperatures of 697 ± 27 to 721 ± 8 °C and 742 ± 19 to 778 ± 34 °C, respectively. We interpret that the first episode of zircon growth took place during subduction prior to the onset of UHP metamorphism, whereas the second episode in the stage of exhumation from UHP to HP eclogite facies regime. Thus, the continental subduction‐zone metamorphism of sedimentary protolith is temporally associated with two episodes of fluid activity, respectively, predating and postdating the UHP metamorphic phase. The significantly high Ti‐in‐zircon temperatures for the younger zircon at lower pressures indicate the initial ‘hot’ exhumation after the peak UHP metamorphism. There are two types of titanite. One exhibits light rare earth element (LREE) enrichment, steep MREE–HREE patterns and no Eu anomalies, and yields Zr‐in‐titanite temperatures of 551 to 605 °C at 0.5 GPa, and the other shows LREE depletion and flat MREE–HREE patterns, and gives Zr‐in‐titanite temperatures of 782–788 °C at 2.0 GPa. The former is amenable for U–Pb dating, yielding a discordia lower intercept age of 252 ± 3 Ma. Thus, the first type of titanite is interpreted to have grown in the absence of garnet and plagioclase and thus in the early stage of subduction. In contrast, the second one occurs as rims surrounding rutile cores and thus grew in the presence of garnet during the ‘hot’ exhumation. Therefore, there is multistage growth of zircon and titanite during the continental subduction‐zone metamorphism. The combined studies of chronometry and thermobarometry provide tight constraints on the P–T–t path of eclogites during the continental collision. It appears that the mid‐T/UHP eclogite facies zone would not only form by subduction of the continental crust in a P–T path slightly below the wet granite solidus, but also experience decompression heating during the initial exhumation. 相似文献
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C. M. Hohenberg R. H. Brazzle O. V. Pravdivtseva A. P. Meshik 《Journal of Earth System Science》1998,107(4):413-423
129Xe, from the decay of the now-extinct 16.7 Ma129I, accumulates in iodine-bearing sites and since most iodine host phases are secondary, the I-Xe system is typically a chronometer for post-formational processes. The validity of the I-Xe chronometer is confirmed by comparison with Pb-Pb ages on phosphate and feldspar separates from twelve meteorites. Phosphate separates are found to be concordant with Pb-Pb for all six samples in which useful I-Xe data were obtained. Feldspar is a better iodine host than apatite in H chondrites, typically providing good I-Xe isochrons. These too are concordant with the Pb-Pb ages of the corresponding phosphates for five out of six feldspar separates. The exception is Allegan whose feldspar yields one of the oldest I-Xe ages observed, similar to those for CI and CM magnetites. We attribute this to a more primary mineralization, predating the secondary phosphate from which the comparison Pb-Pb age was obtained. Absolute I-Xe ages, found using the reported Pb-Pb age of Acapulco phosphate provide an absolute I-Xe age of 4.566 ± 0.002 Ga for both Shallowater and Bjurböle irradiation standards. This allows relative I-Xe ages to be interpreted in the context of absolute ages. 相似文献
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短周期放射性核素的初始丰度和分布情况,已成为陨石学和天体化学的重要研究领域之一。已有研究证实地外天体中53 Cr的放射性母体为53 Mn。53 Mn的半衰期为3.7±0.4Ma,可对太阳系形成之后的20Ma内发生的事件进行精确定年。本文系统总结了已报道的碳质球粒陨石、普通球粒陨石、顽辉石球粒陨石和分异陨石中的53 Mn-53 Cr同位素体系数据,依据55 Mn/52 Cr值和53 Cr异常探讨了太阳系形成时53 Mn和53 Cr的初始分布情况、太阳系初始的53 Mn/55 Mn值,讨论了陨石中普遍存在的54 Cr/52 Cr值异常和碳质球粒陨石全岩的54 Cr和53 Cr异常值之间的正相关关系对53 Mn-53 Cr体系定年影响。 相似文献
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