M Aghazadeh
Abstract
The Sar Cheshmeh mine, a world-class porphyry copper deposit, is located in the Kerman metallogenic zone. The rock outcrops in the deposit are Eocene basalt, basaltic andesite and andesite, Oligocene granular and porphyry granodioritic intrusions and Miocene Sar Cheshmeh granodioritic porphyry stock, ...
Read More
The Sar Cheshmeh mine, a world-class porphyry copper deposit, is located in the Kerman metallogenic zone. The rock outcrops in the deposit are Eocene basalt, basaltic andesite and andesite, Oligocene granular and porphyry granodioritic intrusions and Miocene Sar Cheshmeh granodioritic porphyry stock, granitic late fine-grained porphyry and andesitic to dacitic hornblende, plagioclase, and biotite porphyry dykes. In the spider diagrams, studied rocks show LILE enrichment and HFSE depletion pattern similar to volcanic arc rocks. Eocene volcanic rocks and Oligocene granular and porphyry granodioritic intrusions represent typical magmas characteristics of volcanic arcs whereas Miocene intrusions and dykes have adakitic nature. The (La/Yb)N ratio in the volcanic rocks and Oligocene intrusions varies between 1-5 and 7-11 respectively, while Miocene intrusions and dykes show highest amount of this ratio(20-40). Low aboundancy of HREE in the Miocene intrusions and dykes implies that garnet have been in the source, which has been formed due to increasing crustal thickness during Oligocene and Miocene. According to U-Pb dating, the Sar Cheshmeh porphyry stock and granitic late fine grained have been emplaced in 12.97 ± 0.23 Ma and 12.37 ± 0.1 Ma respectively, while hornblende porphyry dykes has been intruded in 12.16 ± 0.8 Ma. According to trace element characteristics in zircon crystals, Miocene intrusions and dykes originated from same source. Middle Miocene intrusions and dykes have been generated in a post collisional tectonic setting from various degree partial melting of amphibolitic mafic lower crust with variable garnet.
M Aghazadeh; Z Badrzadeh; A Castro
Abstract
The studied Roudbar and Abhar plutons are located in the western Alborz zone and Taroum subzone. These intrusive bodies show metaluminous and shoshonitic nature and they cut the Eocene volcanic and sedimentary rocks. In the studied plutons, monzonite and quartz monzonite terms are dominant. According ...
Read More
The studied Roudbar and Abhar plutons are located in the western Alborz zone and Taroum subzone. These intrusive bodies show metaluminous and shoshonitic nature and they cut the Eocene volcanic and sedimentary rocks. In the studied plutons, monzonite and quartz monzonite terms are dominant. According to geochemistry, these plutons were crystallized from non-primary magma, and have been experienced fractional crystallization. In the primary mantle normalized spider diagrams and chondrite normalized REE diagrams, studied samples show clear enrichment in the LREE and LILE and depletion in the HFSE. The primary magma originated from 1-5% partial melting of phlogopite bearing lithospheric mantle with spinel lherzolite composition that metasomatized by subduction agents. According to U-Pb SHRIMP dating, these plutons were intruded during 37.8 to 38.9 Ma in the late Eocene and in a post-collision tectonic setting.
M Aghazadeh; Z Badrzadeh
Abstract
In the northwestern Iran mica-and amphibole-rich lamprophyres crop out mainly as dyke and they cut Pre-Pliocene strata. They exposed in the Arasbaran, EslamyPeninsula, and Mishu range. According to the mineralogy and mineral chemistry, amphibole-rich lamprophyres have kaersutite type amphiboles and diopside ...
Read More
In the northwestern Iran mica-and amphibole-rich lamprophyres crop out mainly as dyke and they cut Pre-Pliocene strata. They exposed in the Arasbaran, EslamyPeninsula, and Mishu range. According to the mineralogy and mineral chemistry, amphibole-rich lamprophyres have kaersutite type amphiboles and diopside phenocrysts in the matrix of same mafic minerals, feldspars, and altered glass. These lamprophyres in some thin sections have olivine and phlogopite. Mica-rich lamprophyres include phlogopite and diopside phenocrysts in the matrix of same mafic minerals, abundant glass and secondary minerals. According to the mineralogy, mineral chemistry, and geochemistry, amphibole-rich lamprophyres are alkaline and show camptonite-sannaite composition but mica-rich lamrophyres are calc-alkaline and represent minette composition. Alkaline lamprophyres represent characteristics of OIB type magma while calc-alkaline lamprophyres show characteristics of magmas originated in the subduction dominant tectonic setting. Sorkheh amphibole-bearing lamprophyres show both alkaline and calc-alkaline type lamprophyres. Regarding to geochemical features both calc-alkaline and alkaline lamprophyres originated from heterogeneous mantle with different proportions of spinel, garnet and hydrous minerals (e.g. phlogopite and amphibole). Calc-alkaline lamprophyres originated from a mantle enriched in phlogopite and alkaline lamprophyres originated from lithospheric mantle that metasomatised by deep mantle and enriched in amphibole. Both mentioned mantles associated in the petrogenesis of the Sorkheh amphibole- bearing lamprophyres. The lamprophyres were emplaced in the post collisional tectonic setting.