共查询到19条相似文献,搜索用时 46 毫秒
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连续激光探针质谱^40Ar/^39Ar法测定单颗粒矿物年龄 总被引:14,自引:0,他引:14
Nd:YAG激光器与高精密MM1200质谱计-电子倍增器连网,应用连续激光质谱对单颗粒矿物、光片样品进行微区40Ar/39Ar测年、坪年龄和等时线年龄研究。在光片上测定南极乔治王岛(King George Island Antarctica)北海岸玄武岩等时线年龄(52.38±1.05Ma)和贵州绿豆岩年龄(239.16±14.13Ma),两者与实际地质背景吻合。对两个中生代和太古宙单颗粒黑云母进行连续激光质谱阶段升温(40)Ar/(39)Ar坪年龄谱测定,获得与常规法相一致的坪年龄谱。 相似文献
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对采自河北省迁西县太平寨HBT1麻粒岩中的辉石、角门石、斜长石进行了40Ar-39Ar年龄测定,并对上述三种矿物做了40K-40Ar同位素封闭温度计算,进而根据封闭温度与年龄的关系,研究了该区麻粒岩体的冷却抬升历史。分别得到辉石坪年龄为2.16Ga,封闭温度为620℃;角闪石坪年龄为1.97Ga,封闭温度为517℃;斜长石坪年龄为1.66Ga,封闭温度为265℃。从2.5Ga(麻粒岩相变质年龄)到2.16Ga,岩体抬升速率为14.1m/Ma,冷却速率为0.39℃/Ma;从2.16Ga到1.97Ga岩体抬升速率为18.5m/Ma,冷却速率为0.55℃/Ma,从1.97Ga至1.66Ga岩体抬升速率为29.1m/Ma,冷却速率为0.81℃/Ma。Ar-Ar法给出的这些同位素证据,反映了冀东太古代麻粒岩体变质作用晚期多阶段冷却抬升的漫长历史。 相似文献
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激光质谱测定南极乔治王岛北海岸A635玄武岩微区~(40)Ar-~(39)Ar的等时年龄 总被引:1,自引:0,他引:1
采用连续激光直接对岩石光片样品微区熔样,以高灵敏度、高精确度的质谱计测试,对南极乔治王岛玄武岩样品进行(40)Ar-(39)Ar法定年,取得了成功。样品置反应堆中心E-5孔道,以1.8×10(18)n/cm2的快中子总通量照射,时间为50h,放射性冷却后进行测定。样品的加热源为自行设计的Nd:YAG固体激光器,以He-Ne准激光器导光。测定中对4个250μm直径的微区分别在1500℃高温熔融,经Zr-Al泵纯化的气体用MM1200质谱计测量氩同位素各峰值。经计算得到该样品的等时年龄为52.4±1.1Ma,远远低于江个点的视年龄值,而((40)Ar/(36)Ar)>>295.5。这不仅证明该样品含有过剩氩,同时也证明了由K-Ar稀释法得到的偏高年龄值亦是样品中存在过剩氩造成的。激光微区等时年龄的获得进一步厘定了南极乔治王岛北海岸火山岩时代为第三纪,同时证明了我们建立的激光质谱微区、微粒熔样和测定技术是可行的和成功的。 相似文献
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武当地块基性岩墙群^40Ar—^39Ar定年及其地质意义 总被引:12,自引:1,他引:11
通过对南秦岭武当地块内变形变质基性岩墙群中的角闪石、黑云母矿物的40Ar-39Ar定年,获得角闪石三组年龄,分别为高温坪年龄694.4±21Ma,中温坪年龄384.4±3Ma(相应等时线年龄为383.3±10Ma)和低温视年龄240~180Ma。黑云母单一坪年龄为235.3±2Ma(相应等时年龄为236.7±6Ma)。结合本区基性岩墙已获得的Sm-Nd全岩等时年龄(782±164Ma)分析,782±164Ma~694.4±21Ma代表岩墙侵位、冷却过程的时间,提供了武当地块裂解的构造事件年龄;384.4±3Ma和约240Ma则代表岩墙群侵位后两期重要构造-热事件的改造年龄。上述为武当地块的构造作用过程和南秦岭构造带的形成、演化提供了重要证据。 相似文献
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浙江省陈蔡群的^40Ar—^39Ar年龄与变质年代 总被引:2,自引:0,他引:2
本文对陈蔡群变质岩进行了40Ar-39Ar年龄测定。其中在诸暨陈蔡测得的415.1Ma的坪年龄代表了主变质晚期的冷却年代。采自义乌尚阳的样品受燕山期火山活动影响有明显的氩丢失,与主变质有关的年龄亦明显降低,仅315.3Ma。在龙泉东书获得的年龄谱和当地广泛发育的混合岩化作用有关,276.9Ma的坪年龄为这次热事件的冷却年代。根据对现有年代资料的讨论,可以认为不同衰变体系记录了陈蔡群主变质事件的演化。Rb-Sr体系在变质早中期实现均匀化,年龄值为552.4~660.6Ma。锆石、磷灰石在变质高峰期形成的铅丢失年龄为508,4~578Ma。上述资料表明陈蔡群主变质年代属加里东期。 相似文献
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本文给出的滹沱群下亚群青石村组玄武岩Rb-Sr、Sm-Nd全岩等时线年龄为2045.8±17和2369±30Ma(Z),角门石40Ar-39Ar坪年龄和最高视年龄为1364±19和1932±19Ma(1);中亚群河边村组玄武岩Rb-Sr全岩等时线年龄图的投点呈完全离散状,Sm-Nd全岩等时线年龄为2322±31Ma(2),角门石40Ar-39Ar坪年龄和最高视年龄为1360和1742±17Ma(1)。根据上述Rb-Sr、Sm-Nd数据与已知青石村组、河边村组单颗粒锆石U-Pb法确定的成岩年龄2450±10和2400±20Ma(2)的明显差别,40Ar-39Ar均揭示为较典型受扰动的年龄谱和较发育的透人性构造、晚期岩脉等地质证据,认为Rb-Sr、Sm-Nd是重设的同位素体系。 相似文献
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激光显微探针40Ar/39Ar 定年方法研究 总被引:12,自引:0,他引:12
实验结果表明,在激光探针40Ar/36Ar年龄和常规40Ar/39Ar年龄之间有较好的吻合性,多次测定BSP-1角闪石国际标样年龄值大部分在2020-20900Ma之间,多次测定周口店花岗岩中ZBH-25国内标样年龄值大部分在130-135.9Ma。分析区域可小到30μm以下(激光束本身可被聚集到10μm以下)。研究表明,激光显微探针技术在下述工作中将是一个极有前途的工具①测定不易大量获取的样品年龄;②研究遭受多期地质历史事件作用因而有复杂Ar状态的岩石年代;③研究在岩石样品中填充在不同结构位置上的矿物年 相似文献
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Marvin A. Lanphere 《Quaternary Research》2000,53(3):294
K–Ar and 40Ar/39Ar ages have been measured on nine mafic volcanic rocks younger than 1 myr from the Snake River Plain (Idaho), Mount Adams (Washington), and Crater Lake (Oregon). The K–Ar ages were calculated from Ar measurements made by isotope dilution and K2O measurements by flame photometry. The 40Ar/39Ar ages are incremental-heating experiments using a low-blank resistance-heated furnace. The results indicate that high-quality ages can be measured on young, mafic volcanic rocks using either the K–Ar or the 40Ar/39Ar technique. The precision of an 40Ar/39Ar plateau age generally is better than the precision of a K–Ar age because the plateau age is calculated by pooling the ages of several gas increments. The precision of a plateau age generally is better than the precision of an isotope correlation (isochron) age for the same sample. For one sample the intercept of the isochron yielded an 40Ar/36Ar value significantly different from the atmospheric value of 295.5. Recalculation of increment ages using the isochron intercept for the composition of nonradiogenic Ar in the sample resulted in much better agreement of ages for this sample. The results of this study also indicate that, given suitable material and modern equipment, precise K–Ar and 40Ar/39Ar ages can be measured on volcanic rocks as young as the latest Pleistocene, and perhaps even the Holocene. 相似文献
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Leah E. Morgan Madicken Munk Brett Davidheiser‐Kroll Nicholas H. Warner Sanjeev Gupta Rachel Slaybaugh Patrick Harkness Darren F. Mark 《Geostandards and Geoanalytical Research》2017,41(3):381-396
The chronology of the Solar System, particularly the timing of formation of extra‐terrestrial bodies and their features, is an outstanding problem in planetary science. Although various chronological methods for in situ geochronology have been proposed (e.g., Rb‐Sr, K‐Ar), and even applied (K‐Ar), the reliability, accuracy, and applicability of the 40Ar/39Ar method makes it by far the most desirable chronometer for dating extra‐terrestrial bodies. The method however relies on the neutron irradiation of samples, and thus a neutron source. Herein, we discuss the challenges and feasibility of deploying a passive neutron source to planetary surfaces for the in situ application of the 40Ar/39Ar chronometer. Requirements in generating and shielding neutrons, as well as analysing samples are described, along with an exploration of limitations such as mass, power and cost. Two potential solutions for the in situ extra‐terrestrial deployment of the 40Ar/39Ar method are presented. Although this represents a challenging task, developing the technology to apply the 40Ar/39Ar method on planetary surfaces would represent a major advance towards constraining the timescale of solar system formation and evolution. 相似文献
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赣东北地区重要火成岩的40Ar/39Ar年龄 总被引:11,自引:0,他引:11
在赣东北蛇绿混杂岩带发现含晚古生代放射虫硅夺,测定了该带内的和带外几个关键地点的火山岩和辉长岩的^40Ar/^30Ar同位素地南年龄,获得了以下结果:火山岩的坪年龄为434.9-486.7Ma,辉长岩的坪年龄为232.5-266.3Ma,因此可以肯定赣东北地区有早生代晚期的火山活动,证实了上述火成冉不是中、新元古代的产物,它们中的一部分与晚古生代硅质岩都是蛇绿岩套的成员,属该区晚古生代洋壳的组成部 相似文献
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桐柏——大别山主要构造热事件及40Ar/39Ar地质定年研究 总被引:13,自引:0,他引:13
桐柏——大别山是一条复合造山带。在其演化过程中曾经历了扬子旋回(1000Ma-761Ma)和加里东旋回(470Ma-401Ma)两个板块构造旋回的俯冲-碰撞造山作用,之后又经历了早、中华力西(357Ma-314Ma)的平移走滑和晚华力西(286Ma-261Ma)、印支期(224Ma-185Ma)、燕山期(130Ma-111Ma)逆掩或逆冲推覆的陆-陆叠覆造山作用。印支期的高压超高压变质岩系是在陆-陆叠覆造山作用下形成的。燕山期的造山不仅具显著的深层次构造岩浆作用特点,而且还伴随快速的隆升作用。 相似文献
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Leah E. Morgan Brett Davidheiser-Kroll Klaudia F. Kuiper Darren F. Mark Noah M. McLean Jan R. Wijbrans 《Geostandards and Geoanalytical Research》2023,47(1):91-104
The accuracy and traceability of geochronometers are of vital importance to questions asked by many Earth scientists. The widely applied 40Ar/39Ar geochronometer relies on the co-irradiation of samples with neutron fluence monitors (reference materials) of known ages; the ages and uncertainties of these monitors are critical to our ability to apply this chronometer. Previously, first principles, astronomical and optimisation calibrations have been made. The first principles method for determining the age of monitor minerals is the K-Ar method, which involves measurement of their 40K and 40Ar* abundances. The AQuA (Absolute Quantities of Argon) pipette system, which emits calibrated quantities of 40Ar* via the ideal gas law, was used to calibrate the sensitivity of the system across a range of source pressures and estimate 40Ar* abundances in neutron fluence monitors. These 40Ar abundances were combined with existing 40K abundance data for these monitors. Ages for HD-B1 and MD2 (GA1550) biotite fluence monitors were calculated and combined with intercalibration data for HD-B1 and Fish Canyon sanidine (FCs) to determine ages for FCs. Current results do not have the targeted accuracy when compared with previous calibrations; however, we show how the extensive methodology development presented here can be used towards making reliable future measurements. 相似文献