首页|安徽巢湖地区早白垩世煌斑岩的形成年代、岩石成因及其地质意义

安徽巢湖地区早白垩世煌斑岩的形成年代、岩石成因及其地质意义

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煌斑岩是一种典型的富含挥发分的超基性—中性岩,作为深部幔源岩石,能很好地反映地幔源区的地球化学属性,为探究地球的深部构造和岩浆过程提供了有利窗口.本文以巢湖地区东南部的闪斜煌斑岩为研究对象,在野外地质调查及岩相学研究的基础上,进行了磷灰石年代学、Sr-Nd同位素和全岩主量元素和微量元素分析,通过数据定量模拟,剖析了岩浆过程和地幔源区特征,探讨了其形成构造背景.结果表明,巢湖闪斜煌斑岩(22CH09、22CH14 和 22CH17)磷灰石 LA-ICP-MS 206Pb/238U 加权平均年龄分别为 119±18 Ma、116.4±7.5 Ma 和 114±13 Ma,均形成于早白垩世.巢湖闪斜煌斑岩SiO2含量为39.80%~43.52%,Mg#值为63~70,K2O的含量为1.60%~2.46%,为碱性煌斑岩,且相对富集大离子亲石元素(LILEs,如Ba、K、Cs),亏损高场强元素(HFSEs,如Nb、Ta、Zr、Hf),类似于弧相关的岩浆岩.巢湖闪斜煌斑岩具有低的(Hf/Sm)N和(Ta/La)N比值(分别为0.60~0.67和0.27~0.38),指示其源区经历了俯冲板片流体的交代作用;其高的Zn/Fe(0.001 2~0.001 5)及Fe/Mn值(65.54~84.49)表明其源区主要为辉石岩.数值定量模拟表明,巢湖闪斜煌斑岩可能源于石榴辉石岩小比例部分熔融(<4%),原生岩浆经历了约3%的橄榄石分离结晶作用.煌斑岩磷灰石原位87Sr/86Sr(t)值为0.706 9~0.707 8,eNd(t)值为-9.5~-6.8,与长江中下游带同期基性岩的Sr-Nd同位素组成相似,表明二者起源于同位素组成相似的富集岩石圈地幔.巢湖地区中生代岩石圈地幔与长江中下游带具有较高的亲缘性,长江中下游带与郯庐断裂带南段岩石圈地幔的分界可能介于巢湖闪斜煌斑岩与肥东杂岩之间.结合区域岩浆活动特点,本文认为巢湖闪斜煌斑岩为古太平洋俯冲板片后撤的产物,形成于弧后伸展构造背景.
Geochronology,petrogenesis and geological implication of Early Cretaceous lamprophyre in Chaohu area,Anhui Province
Lamprophyre is a typical ultrabasic-intermediate and rich in volatile matter.As a deep mantle source rock,lamprophyre can well reflect the geochemical properties of the mantle source,and provide a favorable window for exploring the deep tectonic and magmatic processes of the earth.This paper takes Chaohu spessartites as the research object,and carries out apatite geochronology,Sr-Nd isotopes and whole-rock major and trace elements analysis based on field geological surveys and petrographical studies.Through quantitative data simulation,this study analyzes the magmatic processes and characteristics of the mantle source,and explores the tectonic setting of the Chaohu spessartites formation.The results indicate that the apatite LA-ICP-MS 206Pb/238U weighted mean ages of Chaohu spessartites(22CH09,22CH14 and 22CH17)are 119±18 Ma,116.4±7.5 Ma and 114±13 Ma,respectively,all formed during the Early Cretaceous period.The Chaohu spessartites have low SiO2(39.80%~43.52%),high Mg# values(63~70)and K2O content(1.60%~2.46%),belong to alkaline lamprophyre.The Chaohu spessartites are enriched in large ion lithophile elements(LILEs,e.g.Ba,K,Cs)and depleted in high field strength elements(HFSEs,e.g.Nb,Ta,Zr,Hf),similar to arc-related magmatic rocks.Their low(Hf/Sm)N(0.60~0.67)and(Ta/La)N(0.27~0.38)ratios indicate that their mantle source has undergone metasomatism of subduction slab fluids.The high Zn/Fe(0.001 2~0.001 5)and Fe/Mn(65.54~84.49)suggest that the mantle source of the Chaohu spessartites is mainly composed of pyroxenite.Numerical quantitative calculations indicate that the Chaohu spessartites were generated from small-scale partial melting of garnet pyroxenite(<4%),and followed by 3%olivine fractional crystallization.The in-situ 87Sr/86Sr(t)values of spessartites apatite range from 0.706 9 to 0.707 8 and εNd(t)values from-9.5 to-6.8,which are similar to the Sr-Nd isotopic compositions of the same period basic rocks in the lower Yangtze River belt,indicating that they originated from the enriched lithosphere mantle with similar isotopic compositions.The Mesozoic lithosphere mantle in the Chaohu area has high affinity with the Lower Yangtze River belt,and the lithosphere mantle boundary between the Lower Yangtze River belt and the southern segment of the Tan-Lu fault zone may be between the Chaohu spessartites and Feidong complex.Based on the characteristics of regional magmatic activity,the Chaohu spessartites are considered to be the product of the retreat of the paleo-Pacific subduction slab and formed in the back-arc extensional tectonic setting.

Chaohu spessartiteSouth segment of Tan-Lu fault zoneEarly CretaceousPyroxenite mantle sourcePetrogenesis

陈泽雨、牛漫兰、刘航、朱光、王磊、衡哲

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合肥工业大学资源与环境工程学院 合肥 230009

巢湖闪斜煌斑岩 郯庐断裂带南段 早白垩世 辉石岩地幔源区 岩石成因

国家自然科学基金项目国家自然科学基金项目中央高校基本科研业务费专项

4227224141772228JZ2022HGQA0209

2024

地质科学
中国科学院地质与地球物理研究所

地质科学

CSTPCD北大核心
影响因子:0.79
ISSN:0563-5020
年,卷(期):2024.59(5)
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