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"orbicular texture"
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Tourmaline-rich features in the Heemskirk and Pieman Heads granites from western Tasmania, Australia; characteristics, origins, and implications for tin mineralization
2017
Distinctive magmatic-hydrothermal, tourmaline-rich features have developed in the Heemskirk and Pieman Heads granites from western Tasmania, Australia. They are categorized as tourmaline-rich patches, orbicules, cavities, and veins, based on their distinctive morphologies, sizes, mineral assemblages, and contact relationships with host granites. These textural features occur in discrete layers in the roof zone of granitic sills within the Heemskirk and Pieman Heads granites. Tourmaline patches commonly occur below a tourmaline orbicule-rich granitic sill. Tourmaline-filled cavities have typically developed above the tourmaline-quartz orbicules in the upper layer of the white phase of the Heemskirk Granite. Tourmaline-quartz veins penetrate all exposed levels of the granites, locally cutting tourmaline orbicules and cavities.The tourmalines are mostly schorl (Fe-rich) and foitite, with an average end-member component of schorl45 dravite6 tsilaisite1 uvite0 Fe-uvite3 foitite31 Mg-foitite4 olenite10 Element substitutions of the tourmalines are controlled by FeMg-1, YAlX∎(R2+Na)-1, and minor YAlO(R2+OH)-1 (where R2+ = Fe2+ + Mg2+ + Mn2+) exchange vectors. Several trace elements in tourmaline have consistent chemical evolutions grouped from tourmaline patches, through orbicules and cavities, to veins. There is a progressive decrease of most transition and large ion lithophile elements, and a gradual increase of most high-field strength elements. These compositional variations in the different tourmaline-rich features probably relate to element partitioning occurring in these phases due to volatile exsolution and fluxing of aqueous boron-rich fluids that separated from the granitic melts during the emplacement of S-type magmas into the shallow crust (4 to 5.5 km).Tourmalines from the Heemskirk Granite are enriched in Fe, Na, Li, Be, Sn, Ta, Nb, Zr, Hf, Th, and rare earth elements relative to the tourmalines from the Pieman Heads Granite, but depleted in Mg, Mn, Sc, V, Co, Ni, Pb, Sr, and most transition elements. These results imply that bulk compositions of the host granites exert a major control on the chemical variations of tourmalines. The trace element compositions of tourmalines from the Sn-mineralized Heemskirk Granite are different from those of the barren Pieman Heads Granite. Trace element ratios (e.g., Zn/Nb, Co/Nb, Sr/Ta, and Co/La) and Sn concentrations in tourmaline can distinguish the productive Heemskirk Granite from the barren Pieman Heads Granite.
Journal Article
Field and petrographical insight into the formation of orbicular granitoids from the Bonney Pluton, southern Victoria Land, Antarctica
2014
The diversity of orbicule types exposed within granitoids of the Bonney Pluton in southern Victoria Land attests to the dynamic and complex interplay of magmatic processes that were responsible for their formation. Orbicules formed in small pockets of H2O-rich silicate melt that was extracted from the crystallizing and fractionating Bonney Pluton magma and concentrated along the pluton margins. These pockets of melt experienced a superheating event that destroyed almost all pre-existing nuclei and a subsequent delay in crystallization, which led to undercooling conditions that promoted rapid dendritic crystal growth. Superheating was induced by the injection of hot mafic magmas, evidenced by elevated plagioclase XAn, and Mg-Al-Ti-contents in hornblende that point to a higher temperature and a more mafic composition in the melt that the orbicule shells crystallized from. Variation in the type and structure of orbicules (hornblende-rich versus plagioclase-rich shells) were likely due to repeated changes in the composition, H2O-content, temperature and PH2O at the crystallizing orbicule boundary layer in response to pulses in the movement of magma, competition between crystallizing phases, episodic vesiculation, degassing and/or second boiling which dictated the composition, texture and size of individual orbicule shells. Brittle fragmentation of orbicules occurred in response to vesiculation and fragmented orbicules are often found as cores within intact orbicules, indicating that multiple phases of orbicule formation were common. The alignment and compaction of orbicules in \"pods\" indicates movement of orbicules within the melt-rich pockets occurred, prior to resumption of near-equilibrium crystallization in the host granite.
Journal Article
Petrology and geochemistry of the orbicular granitoid of Sierra de Velasco (NW Argentina) and implications for the origin of orbicular rocks
by
TOSELLI, ALEJANDRO J.
,
ROSSI, JUANA N.
,
GROSSE, PABLO
in
Argentina
,
Carboniferous
,
chemical composition
2010
The Velasco orbicular granitoid is a small (65 × 15 m), irregularly-shaped body that crops out within the Huaco granite, central Sierra de Velasco, NW Argentina. It consists of ellipsoid-shaped orbicules of 3 to 15 cm length immersed in an aplitic to pegmatitic matrix. The orbicules are formed by a core made up of a K-feldspar megacryst, partially to totally replaced by plagioclase, an inner shell of radial and equant plagioclase crystals, a layer of tangentially oriented biotite laths, and an outer shell of plumose plagioclase crystals, containing diffuse rings of tangentially oriented biotite. The orbicular granitoid formed in situ in a pocket of evolved and volatile-rich melt segregated from the surrounding partially crystallized Huaco granite, possibly via a filter pressing mechanism. The segregated melt entrained relatively few K-feldspar megacrysts into the pocket, leaving behind a concentration of megacrysts around the pocket. High water concentration caused effective superheating of the melt and destruction of nuclei, with only the large megacrysts surviving as solids. Sudden water-pressure loss and exsolution of the volatile phase, perhaps related to a volcanic eruption or fracturing of the surrounding granite, caused rapid undercooling of the melt. The orbicules grew in the undercooled melt by heterogeneous nucleation on the megacrysts, which acted as nucleation seeds, and crystallization of reversely zoned radial plagioclase and sporadic crystallization of tangential biotite rings according to fluctuations in its saturation. Orbicular growth gave way to crystallization of the equiaxial inter-orbicular matrix in two stages, when sufficient polymerization of the melt was attained. The time scale of formation of the orbicular granitoid was fast, possibly a matter of a few weeks or months.
Journal Article
Crystallization of orbicular rocks exemplified by the Slättemossa occurrence, southeastern Sweden
2006
The orbicular rock at Slättemossa, southeastern Sweden, has a quartz monzodioritic composition. The cores of the orbicules crystallized directly from the orbicule-forming magma; cores made up of xenoliths have not been observed. Outside the core follow first an inner mafic, a felsic and then an outer mafic shell. The orbicules occur in a matrix, which is similar to the core. They grew simultaneously and show an almost perfect parallelism in evolution. After initial ‘normal’ crystall-ization of the magma, superheating probably triggered by a sudden addition of volatiles destroyed earlier formed nuclei and also affected the already crystallized part of the rock. Cooling caused heterogeneous nucleation and rapid crystallization, which formed the inner mafic shell. This is enriched in mafic minerals, especially biotite, compared to the core. At the same time the grain size becomes significantly smaller. Depletion in mafic components, possibly intensified by a sudden change in physical conditions, destabilized biotite and amphibole crystallization, causing oversaturation in plagioclase components, forming a felsic shell having a sharp boundary with the mafic shell. Plagioclase is extremely altered. Mafic minerals were then stabilized, probably due to depletion of plagioclase components, and an outer mafic shell formed. With the return to homogeneous nucleation, matrix formation concluded the crystallization. Orbicules might have moved in the magma causing some squeezing of magma surrounding the orbicules, but major movements involved the settling of the whole package of orbicules and matrix in the surrounding non-orbicular magma.
Journal Article
ORBICULAR GABBRO AS AN INDICATOR OF MAGMA MIXING FROM STRANDJA MASSIF, NORTHWEST TURKEY: MINERAL CHEMISTRY AND CONFOCAL RAMAN SPECTROMETRY METHODS
2018
Strandja Massifs' units form the basement metamorphic units of north western edge parts of Turkey and intruded by the Late Cretaceous felsic and mafic intrusive rocks. The felsic and mafic rocks have a contact metasomatic effects at the border of sedimentary rocks resulting in the formation hornfels, metasandstone and calcsilicaticfels in the composition. Demirköy is one of the youngest intrusive body which crops out at NE of the massif and mainly composed of granite, granodiorite, diorite and gabbro in composition. The intrusive body of the Demirköy has a fresh out crop and mainly has fine to coarse crystalline texture and they have angular to elliptical shaped mafic microgranular enclaves (MME). The MEE are ranging in size from 1cm up to 30 cm in the composition of diorite and quartz diorite. The mafic intrusive rocks of Demirköy body are in the composition of diorite at the contact with felsic intrusive and change to gabbro in composition at inner part of the body. The gabbroic rocks with the carbonate metamorphic rocks have orbicular textures. These scarce sections with special texture reveals specials conditions. Each orbicular rounded and elliptical shape with different size changing from 1 cm up to 30 cm in size. All orbicular consist of several concentric circles showing magmatic textures in hand specimen and under the microscope. The circle of orbicular is mainly composed of olivine, pyroxene, amphibole, plagioclases and Fe-Ti oxide minerals. The Orbicular rings of gabbroic rocks occupy repeating coarse grain minerals and fine grain crystals. Core of orbicular cycle have subophitic texture and composed of coarse grain crystals. Surrounded rings have subophitic texture with fine texture and rich in olivine with comparison to the core part of the circle. The Mineral chemistry studies with electron prob microanalysis (EPMA) reveal that the pyroxene are ranging in composition from augite to diopside, plagioclase are ranging in composition from bytownite to labrodorite and the olivine are generally in the composition of forsterite with high amount of Mg contents. The mineralogical, petrographical and geochemical features indicate that the orbicular body form a part of mafic magmatic enclaves within the mafic intrusive rocks and they are the products of the late injection of a basic magma in to the whole body of the main basic magma chamber and cause to acting with parent magma body resulting the crystallization of repeated circler body during the circular convection in the form of orbicular texture within the main intrusive body.
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