40Ar(40Ar＊＋40ArE)、39Ar释气特征与过剩氩的甄别及年代学意义

对具有不同地质历史背景的3类⁴⁰Ar/³⁹Ar法样品中的⁴⁰Ar和³⁹Ar释出特征进行对比,研究结果表明,⁴⁰Ar/³⁹Ar法样品中的⁴⁰Ar、³⁹Ar释气曲线主要表现为以下3种形式:完全重合型、过剩氩型和不规则型。当⁴⁰Ar与³⁹Ar释气曲线呈完全重合型时,⁴⁰Ar/³⁹Ar法全熔年龄代表了岩体的形成年龄;当⁴⁰Ar、³⁹Ar释气曲线是过剩氩型时,⁴⁰Ar/³⁹Ar法全熔年龄则大于岩体的形成年龄;当⁴⁰Ar与³⁹Ar释气曲线呈不规则型时,表明样品中的放射成固氩(⁴⁰Ar^*)发生了丢失,其全熔年龄一般较岩体的形成年龄小。对于⁴⁰Ar、³⁹Ar释气曲线呈过剩氩型的样品,⁴⁰Ar/³⁹Ar法年龄谱通常呈马鞍形,且马鞍形年龄谱的底部年龄一般都具有地质意义,代表了岩体的形成年龄。对于⁴⁰Ar、³⁹Ar释气曲线呈不规则型的样品,对其年龄谱的解释应持谨慎态度。     

K-Ar、40Ar/39定年中尼尔值和初始氩比值

K-Ar、⁴⁰Ar/³⁹Ar定年中, 用以计算囚禁⁴⁰Ar绝对量的⁴⁰Ar/³⁶Ar, 称为初始氩比值.现代大气中的初始氩比值叫尼尔值, 为295.5.K-Ar、⁴⁰Ar/³⁹Ar定年的表观年龄都是在假设初始氩比值与现代大气中的尼尔值一致的基础上得到的.事实证明, 地球样品的初始氩比值不总是尼尔值, 因此这种假定不可靠, 尤其在对年轻样品进行K-Ar、⁴⁰Ar/³⁹Ar定年时, 会带来错误的表观年龄结果.对于K-Ar、⁴⁰Ar/³⁹Ar精细年代学, 特别对于年轻样品和低钾含量样品, 只有初始氩比值才对定年研究有意义, 而初始氩比值只能通过⁴⁰Ar/³⁹Ar等时线法求得.所以严格地讲, 只有等时线年龄才是可靠的.结合实验流程, 本文分析了⁴⁰Ar/³⁹Ar定年中为什么大多数等时线获取的初始氩比值接近尼尔值, 一是因为常规⁴⁰Ar/³⁹Ar坪年龄的计算方法, 二是因为吸附氩的干扰.初始氩比值的一致性, 被用来证明样品同位素同源和封闭特性, 对年龄数据的精度及可靠性有非常大的影响, 尤其是年轻样品.因此, 在⁴⁰Ar/³⁹Ar定年中要选取氩同位素初始比值一致的同源样品, 并在实验流程中尽量克服样品吸附气体.本文对传统⁴⁰Ar/³⁹Ar方法中坪年龄、年龄坪的意义提出了质疑, 对提高⁴⁰Ar/³⁹Ar定年的精度具有重要意义, 并使之能够应用到极年轻的火山岩定年中.     

金属成矿40Ar/39Ar年代学的进展与问题——以黄铁矿、闪锌矿为例

长期以来, 由于金属成矿的多期性及易受后期蚀变的干扰, 成矿时代的确定成为难题, 进而成为成矿机理、矿床勘探等研究的制约因素。本文以黄铁矿和闪锌矿这两种典型的矿石矿物为例, 回顾了利用⁴⁰ Ar/³⁹ Ar法直接确定成矿时代的研究现状, 探讨了其中的问题、可能的解决方法及以后的发展前景, 为进一步开展矿石矿物的⁴⁰ Ar/³⁹ Ar年代学提供参考。同时对采自辽宁丹东青城子矿中的黄铁矿和闪锌矿样品做了包裹体镜下观察和电子探针的元素分析, 以期更好地理解矿石矿物⁴⁰ Ar/³⁹ Ar法直接定年的潜力。     

多宝山斑岩铜矿区水热蚀变矿物的激光显微探针40Ar/39Ar定年

在利用脉冲显微激光探针⁴⁰Ar/³⁹Ar定年技术测定标准样品的J值和年龄适用范围的基础上,研究了黑龙江省嫩江县北部多宝山斑岩铜矿区水热成因矿物的年代学。结果表明,高钾含量的水热蚀变矿物适合于激光探针的表面微区测定,并且可以克服水热蚀变矿物中的³⁹Ar “反冲”丢失对年龄结果的影响。矿区的岩浆-水热事件主要有两期,分别为253-220Ma和184-162Ma,前者代表了成矿时代,后者反映出由成矿期后岩浆活动所引起的水热叠加事件。     

高压-超高压变质岩外来40Ar成因探讨

高压—超高压变质带是地球上重要的地质单元,特殊的形成环境使该类变质岩的矿物中常因含有外来⁴⁰Ar而⁴⁰Ar／³⁹Ar年龄偏老,制约了⁴⁰Ar／³⁹Ar年代学在此类岩石中的应用。本文探讨了氩在不同相中的溶解度与分配系数的差异,并着重论述了扩散参数与压力的关系及压力对岩体封闭性的影响,系统总结了高压-超高压变质矿物中外来⁴⁰Ar的形成机制。此外,随Fe/Mg、Si/Al、K等组分不同,氩在矿物中保存能力的某种规律性变化、离子孔隙度研究等也从理论上为研究氩的扩散和封闭行为提供了新的视角。在高压—超高压变质过程中多种因素共同作用,氩在这类矿物中的扩散更为复杂。对外来⁴⁰Ar形成机制的探讨对揭示高压—超高压变质结晶环境、岩体开放与否、不同矿物对氩保存能力等有重要的指示意义。     

南岭中段主要锡矿床He、Ar同位素组成及其意义

对南岭中段主要锡矿床的黄铁矿等进行了流体包裹体的He、Ar同位素研究。结果表明,成矿流体的⁴⁰Ar/³⁶Ar≈288～371,³He/⁴He≈0.09～28.58Ra ,不同地区流体包裹体He、Ar浓度变化较大,而在同一地区⁴⁰Ar/³⁶Ar、³He/⁴He值比较一致;⁴⁰Ar/³⁶Ar值介于大气饱和水(包括大气降水和海水)的同位素组成（⁴⁰Ar/³⁶Ar≈295.5）和夏威夷热点（⁴⁰Ar/³⁶Ar=350～360）之间,³He/⁴He值大大高于大陆地壳特征值（³He/⁴He≈0.03Ra）,介于地壳特征值与原始地幔特征值（³He/⁴He≈8.57Ra）和夏威夷热点特征值（³He/⁴He≈27.14Ra）之间,表明成矿流体与地幔柱的活动有关,为地幔、地壳和大气水的混合产物,以地幔流体为主。这一结果为南岭地区锡多金属矿床为壳幔相互作用的产物及区域地幔柱的存在提供了新证据。     

土壤气中He、Ar组分在金家地区油气化探中应用研究

对济阳凹陷南缘与鲁西隆起接合部开展了土壤气He、Ar组分及Ar同位素测定,结果表明He的丰度从5.1-6μL/L(S.T.P),δHe值从-4%-16%,平均2.59%;⁴⁰Ar/³⁶Ar比值从255-325,δ(⁴⁰Ar/³⁶Ar)值从+11%-11%,He异常主要分布在研究区北部,而Ar等值图分布比较复杂。He、Ar、烃三组分之间的组合关系表明有3个远景区,最有意义的是中深层远景区。此外,根据地质分析及Ar同位素特征表明中深层异常远景区不仅是与已知的第三系油田有关,而且还与深部C-P煤系地层有关,故属煤成气异常。     

延边海沟金矿床石英流体包裹体激光探针40Ar/39Ar测年与成矿背景

海沟金矿为一大型贫硫化物石英脉型金矿床,长期以来其形成时代一直存在争议,致使矿床成因研究受到较大影响,成矿预测等方面研究进展缓慢。采用石英流体包裹体的⁴⁰Ar/³⁹Ar激光探针定年法对该金矿床进行了精细的年代学测定,获得主成矿阶段石英流体包裹体的⁴⁰Ar/³⁹Ar正、反等时线年龄分别为（170±20） Ma和（172±16） Ma,MSWD分别为0.31和0.35,⁴⁰Ar/³⁶Ar比值分别为298±4和299±4;进一步剔除接近大气的成分点和过剩氩高的成分点,计算获得等时线年龄为（170±38） Ma（⁴⁰Ar/³⁶Ar Int.=299±10）和（165±52） Ma（⁴⁰Ar/³⁶Ar Int.=303±23）。结合已有同位素年代学研究成果,进一步明确了海沟金矿床主成矿期发生在早侏罗世晚期,成矿作用与中生代库拉板块向亚洲板块俯冲、特别是由此引发的华北板块东缘与兴蒙造山带东段的强烈拼贴并诱发的岩石圈加厚、减薄作用密切相关。     

柴北缘锡铁山地体花岗质片麻岩退变质作用和40Ar/39Ar年代学研究及其地质意义

本文对柴达木盆地北缘锡铁山地区含榴辉岩透镜体花岗质片麻岩进行了系统的矿物学、相平衡模拟以及黑云母和石英⁴⁰Ar/³⁹Ar年代学研究,旨在查明花岗质片麻岩在加里东超高压变质之后,折返过程中发生角闪岩-绿片岩相退变质作用的变质条件和变质年代。矿物学和相平衡模拟显示,发育变形石英细脉的黑云母花岗质片麻岩高角闪岩相变质矿物组合(M1)为黑云母+钾长石+斜长石+石英+金红石+矽线石+钛铁矿,对应变质条件为T>620℃,P>0.16GPa;低角闪岩相-绿片岩相变质矿物组合(M2)为黑云母+白云母+斜长石+微斜长石+石英+榍石±绿泥石,变质条件为T=390～420℃和P=0.10～0.19 GPa。花岗质片麻岩中黑云母激光阶段加热⁴⁰Ar/³⁹Ar定年获得了一个上升的阶梯状表观年龄图谱,在中高温阶段则形成了一个平坦的表观年龄坪,坪年龄为353.9±1.8 Ma,对应的等时线年龄为356.7±5.6 Ma。变形石英脉样品真空击碎提取流体包裹体⁴⁰Ar/³⁹Ar...     

中生代火山岩锆石Pb/U法与激光40Ar/39Ar法定年结果对比

通过对龙江组和光华组锆石Pb/U和激光⁴⁰Ar/³⁹Ar两种方法同位素定年结果的对比研究,发现二者对于中生代火山岩的定年结果极为相近.后者相对快捷、方便、经济.认为激光⁴⁰Ar/³⁹Ar定年,适用于1：5万和1：25万区域地质调查及相关的综合研究项目工作.     

一种新的 K-Ar定年方法：峰值比较法

K-Ar法定年技术经历了体积法和稀释法等不断趋于成熟，但对于年轻火山岩进行定年时，由于同位素质量分馏的影响，上述方法都具有不可克服的缺陷。随着质谱仪稳定度和精度的提高，直接建立氩同位素含量与峰强度之间的定量关系，从而不再使用稀释剂（ 38 Ar）成为可能，这就是 K-Ar定年的新方法：峰值比较法（或无稀释剂法）。该方法可以消除质量分馏作用带来的误差，对年轻火山岩定年具有重要意义。近代火山物质都含有初始氩，且有不同程度的质量分馏，其同位素比值落在质量分馏线上，这表明质量分馏作用影响 K-Ar定年的准确性，尤其是非常年轻的样品。通过精确测定样品的 38 Ar／ 36 Ar比值，可以准确扣除样品中的初始 40 Ar，从而得到放射成因 40 Ar含量。这种测量方法可以用于较老岩石、矿物样品的年龄测定，其结果与 K-Ar稀释法以及 40 Ar－ 39 Ar法相一致；更重要的是可以用于年轻样品的年龄测定，可以测 2～5ka的岩矿样品，对富钾矿物的测量误差小于 1ka；对老于 0．1Ma的样品，相对误差不大于 1．5％。介绍了峰值比较法的基本原理和测试过程，同时还讨论它的使用条件和定年范围。     

Strain partitioning and preservation of Ar/Ar ages during Variscan exhumation of a subducted crust (Malpica–Tui complex, NW Spain)

The Malpica–Tui complex (NW Iberian Massif) consists of a Lower Continental Unit of variably deformed and recrystallized granitoids, metasediments and sparse metabasites, overridden by an upper unit with rocks of oceanic affinities. Metamorphic minerals dated by the ⁴⁰Ar/³⁹Ar method record a coherent temporal history of progressive deformation during Variscan metamorphism and exhumation. The earliest stages of deformation (D1) under high-pressure conditions are recorded in phengitic white micas from eclogite-facies rocks at 365–370 Ma. Following this eclogite-facies peak-metamorphism, the continental slab became attached to the overriding plate at deep-crustal levels at ca. 340–350 Ma (D2). Exhumation was accompanied by pervasive deformation (D3) within the continental slab at ca. 330 Ma and major deformation (D4) in the underlying para-autochthon at 315–325 Ma. Final tectonothermal evolution included late folding, localized shearing and granitic intrusions at 280–310 Ma.

Dating of high-pressure rocks by the ⁴⁰Ar/³⁹Ar method yields ages that are synchronous with published Rb–Sr and Sm–Nd ages obtained for both the Malpica–Tui complex and its correlative, the Champtoceaux complex in the French Armorican Massif. The results indicate that phengitic white mica retains its radiogenic argon despite been subjected to relatively high temperatures (500–600 °C) for a period of 20–30 My corresponding to the time-span from the static, eclogite-facies M1 peak-metamorphism through D1-M2 eclogite-facies deformation to amphibolite-facies D2-M3. Our study provides additional evidence that under certain geological conditions (i.e., strain partitioning, fluid deficiency) argon isotope mobility is limited at high temperatures, and that ⁴⁰Ar/³⁹Ar geochronology can be a reliable method for dating high pressure metamorphism.     

Ar/Ar dating of Apollo 12 regolith: Implications for the age of Copernicus and the source of nonmare materials

Twenty-one 2–4 mm rock samples from the Apollo 12 regolith were analyzed by the ⁴⁰Ar/³⁹Ar geochronological technique in order to further constrain the age and source of nonmare materials at the Apollo 12 site. Among the samples analyzed are: 2 felsites, 11 KREEP breccias, 4 mare-basalt-bearing KREEP breccias, 2 alkali anorthosites, 1 olivine-bearing impact-melt breccia, and 1 high-Th mare basalt. Most samples show some degree of degassing at 700–800 Ma, with minimum formation ages that range from 1.0 to 3.1 Ga. We estimate that this degassing event occurred at 782 ± 21 Ma and may have been caused by the Copernicus impact event, either by providing degassed material or by causing heating at the Apollo 12 site. ⁴⁰Ar/³⁹Ar dating of two alkali anorthosite clasts yielded ages of 3.256 ± 0.022 Ga and 3.107 ± 0.058 Ga. We interpret these ages as the crystallization age of the rock and they represent the youngest age so far determined for a lunar anorthosite. The origin of these alkali anorthosite fragments is probably related to differentiation of shallow intrusives. Later impacts could have dispersed this material by lateral mixing or vertical mixing.     

Ar/Ar dating of central European K–Mn oxides — a chronological framework of supergene alteration processes during the Neogene

K-bearing Mn oxides may potentially constitute useful objects for isotopic dating of ore-forming events. A comprehensive ⁴⁰Ar/³⁹Ar study performed on supergene K–Mn oxides sampled from different sub-alpine mountain terrains in Germany and France has been undertaken. The objective of these investigations was to provide new insight into how and when these secondary Mn accumulations may have formed. Developed in supergene environments at the expense of Mn²⁺/Mn³⁺-bearing precursor minerals, the Mn⁴⁺ oxides occur either as pseudomorphic ores or as cavity-fillings and linings.

The isotopic ages range from 25 to 1 Ma, indicating intense chemical weathering, especially during the Miocene and Pliocene. It is yet too early to decide whether the age range represents a more or less continuous process or distinct weathering episodes. Formation of supergene Mn oxides may result from combined climatic and tectonic factors: local uplift, exhumation, and associated fracturing of rocks provided fresh mineral surfaces for percolating meteoric fluids that induced subsequent weathering under warm–temperate to subtropical conditions.     

Post-collisional Variscan lamprophyres (Black Forest, Germany): Ar/Ar phlogopite dating, Nd, Pb, Sr isotope, and trace element characteristics

Subsequent to high-pressure and temperature metamorphism of the axial zone of the Variscan foldbelt in central Europe at ca. 340 to 330 Ma, formation of lamprophyre dikes during transtensional tectonics may be viewed as the beginning of the post-collisional stage of the orogeny. We report the results of ⁴⁰Ar/³⁹Ar mica dating, major and trace element data, and isotope compositions for lamprophyre and rhyodacite samples from the southern Black Forest. The chemical compositions of these rocks shed light on the upper mantle and crust at the end of the Variscan orogeny. ⁴⁰Ar/³⁹Ar plateau ages for four phlogopite–biotite separates from lamprophyres indicate emplacement at 332 to 314 Ma. This event coincides with melting of the crust as indicated by ⁴⁰Ar/³⁹Ar biotite plateau ages of ca. 332 Ma for rhyodacite dikes which are probably related to coeval undeformed granites. Incompatible trace element patterns of the lamprophyre samples reveal the characteristics of evolved continental crust and are interpreted as evidence for melting of sediment in a subduction-modified mantle. Nd, Sr, and Pb isotope compositions indicate an enriched mantle source with _Nd-values of −1.5 to −6.8 which is similar to Variscan crust. Significant contamination of the lamprophyric melts by Variscan crust can be ruled out as mantle-derived phlogopite phenocrysts have similar _Nd-values as in the whole-rock samples. We propose that the isotope compositions and incompatible trace element characteristics of the lamprophyres were predominantly inherited from melted sediment. The isotope compositions of Variscan lamprophyres from western Europe suggest that enriched upper mantle was only partly delaminated when ascending hot mantle triggered melting of the lower crust, as has been invoked for the origin of post-collisional granites. The isotope compositions of Tertiary basalts and mantle xenoliths indicate a depleted upper mantle under western Europe, implying that the enriched Variscan material was efficiently removed and mixed into the convecting mantle.