Triassic lamprophyre dyke in the Palaeozoic basement of NE Sardinia, Italy: Petrogenesis and geodynamic significance

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Gabriele Cruciani , Dario Fancello , Mattia Ferrari , Alessandro Bragagni , Simone Tommasini , Marcello Franceschelli
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Abstract

A Triassic, Si-undersaturated, alkaline lamprophyre from NE Sardinia is studied to decipher its magma source, genesis, and P-T conditions of crystallization and emplacement. It is also compared with similar and coeval rocks occurring throughout Europe to depict a geodynamic scenario associated with the opening of the Pangea. The lamprophyre, crosscutting the Palaeozoic basement, shows a porphyritic texture with centimeter-sized amphibole macrocrystals and biotite, ulvöspinel and apatite phenocrystals. The lamprophyre also contains feldspar clusters, carbonate-rich inclusions, and xenolith nodules. The incompatible trace element patterns show weak positive anomalies for Ba, Nb, K and P and negative ones for Th and Ta, whereas the chondrite-normalized Rare Earth Elements (REE) pattern reflects a constant fractionation from light REEs to heavy REEs without Eu anomaly. The core of the amphibole reflects the deepest crystallization conditions, whereas rims and groundmass amphiboles indicate slightly higher temperature and lower pressure. The bulk Sr and Nd radiogenic isotope composition falls between the E-DMM and BSE mantle components at 220 Ma, ruling out a significant contribution of the local lithospheric mantle, which was metasomatized during the Hercynian orogeny. The comparison with other European lamprophyres along with a palaeogeographic reconstruction suggests that the Sardinia lamprophyre lies along the eastern branch of the fault system responsible for to the opening of the Alpine Tethys. The trace element and radiogenic isotope signature of the Sardinian and the other European lamprophyres is consistent with a progressive transition from the post-collisional orogenic magmatism to anorogenic rift-related alkaline magmatism occurring during Early Mesozoic break-up of Pangea and opening of the Tethys Ocean.
意大利东北撒丁岛古生代基底三叠纪煌斑岩脉:岩石成因及其地球动力学意义
研究了东北撒丁岛三叠系硅欠饱和碱性煌斑岩的岩浆来源、成因、结晶和侵位的P-T条件。它还与整个欧洲发生的类似和同时期的岩石进行了比较,以描绘与泛大陆开放有关的地球动力学情景。煌斑岩横切古生代基底,具有厘米级角闪孔大晶和黑云母、ulvöspinel和磷灰石斑晶的斑状结构。煌斑岩还含有长石簇、富含碳酸盐的包裹体和捕虏岩结核。不相容的微量元素模式表现为Ba、Nb、K和P的弱正异常,而Th和Ta的负异常,而球粒陨石归一化的稀土元素(REE)模式则反映出轻稀土向重稀土的恒定分异,无Eu异常。角闪洞的核心反映了最深的结晶条件,而边缘和地块角闪洞则反映了稍高的温度和稍低的压力。整体Sr和Nd放射性成因同位素组成介于220 Ma的E-DMM和BSE地幔组分之间,排除了海西期造山期交代的局部岩石圈地幔的重要贡献。与欧洲其他煌斑岩的比较以及古地理重建表明,撒丁岛煌斑岩位于阿尔卑斯特提斯断裂系统的东部分支。撒丁岛和其他欧洲煌斑岩的微量元素和放射性同位素特征与早中生代盘古大陆分裂和特提斯洋打开期间发生的碰撞后造山岩浆作用向与造山裂谷有关的碱性岩浆作用的渐进过渡相一致。
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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