Journal of GEOsciences Table of Contents for the Journal of GEOsciences. List of articles from the latest print issue.http://www.jgeosci.orgen-US Journal of GEOscienceshttp://www.jgeosci.org/jgeosci_cover.jpghttp://www.jgeosci.org <![CDATA[ Editorial ]]> Janoušek V; Vol. 57, issue 1, page: 1
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http://www.jgeosci.org/rss.php?ID=jgeosci.114 Editorial http://www.jgeosci.org/rss.php?ID=jgeosci.114
<![CDATA[ Multiple monazite growth in the Åreskutan migmatite: evidence for a polymetamorphic Late Ordovician to Late Silurian evolution in the Seve Nappe Complex of west-central Jämtland, Sweden ]]> Majka J, Be’eri-Shlevin Y, Gee DG, Ladenberger A, Claesson S, Konečný P, Klonowska I; Vol. 57, issue 1, pages 3 - 23
Monazite from granulite-facies rocks of the Åreskutan Nappe in the Scandinavian Caledonides (Seve Nappe Complex, Sweden) was dated using in-situ U-Th-total Pb chemical geochronology (CHIME). Multi-spot analyses of a non-sheared migmatite neosome yielded an age of 439 ± 3 Ma, whereas a sheared migmatite gave 433 ± 3 Ma (2σ). Although the obtained dates are rather similar, a continuous array of single dates from c. 400 Ma to c. 500 Ma suggests possibly a more complex monazite age pattern in the studied rocks. The grouping and recalculation of the obtained results in respect to Y-Th-U systematics and microtextural context allowed distinguishing several different populations of monazite grains/growth zones.
In the migmatite neosome, low-Th and low-Y domains dated at 455 ± 11 Ma are considered to have grown under high-grade sub-solidus conditions, most likely during a progressive burial metamorphic event. The monazites with higher Th and lower Y yielded an age of 439 ± 4 Ma marking the subsequent partial melting event caused by decompression. The youngest (423 ± 13 Ma) Y-enriched monazite reveals features of fluid-assisted growth and is interpreted to date the emplacement of the Åreskutan onto the Lower Seve Nappe.
In the sheared migmatite, the high-Th and low-U (high Th/U) monazite with variable Y contents yielded an age of 438 ± 4 Ma, which is interpreted to date the partial melting event. Relatively U-rich rims on some of the monazite grains again reveal features of fluid-assisted growth, and thus their age of 424 ± 6 Ma is interpreted as timing the nappes emplacement. These results call, however, for further more precise, isotopic (preferably ion microprobe) dating of monazite in the studied rocks. ]]>
http://www.jgeosci.org/rss.php?ID=jgeosci.112 Original Paper http://www.jgeosci.org/rss.php?ID=jgeosci.112
<![CDATA[ Oxide minerals in the granitic cupola of the Jálama Batholith, Salamanca, Spain. Part I: accessory Sn, Nb, Ta and Ti minerals in leucogranites, aplites and pegmatites ]]> Llorens T, Moro MC; Vol. 57, issue 1, pages 25 - 43
Sn-Nb-Ta-Ti oxides occur as accessory minerals in the granitic facies of the External Unit in the Jálama Batholith (Salamanca, Spain) and in the related LCT pegmatite dikes of the rare-element class. Moreover, abundant cassiterite and columbite-group minerals crystallized in the Cruz del Rayo peribatholithic pegmatite dikes, cutting the pre-Ordovician low-grade metasedimentary rocks of the surrounding Schist-Graywacke Complex.
Cassiterite, rutile, ilmenite and tantalite-(Fe) occur disseminated in the border facies of the External Unit, especially throughout the tourmaline-bearing leucogranite and the apical aplites. Additionally, cassiterite, rutile and Ta-rich rutile developed locally in the intragranitic pegmatite dikes.
Two types of peribatholithic pegmatites can be distinguished at Cruz del Rayo: (i) granite-like pegmatites, with columbite-(Fe) I and II and cassiterite, in which the influence of metasomatic fluids led to formation of the late albite unit and crystallization of tantalite-(Fe), and (ii), greisen-like bodies, which contain high amounts of columbite-(Fe), columbite-(Mn), tantalite-(Mn) I and II as well as cassiterite.
The primary oxide assemblage in both types of the peribatholithic pegmatite dikes would have crystallized as a result of magmatic differentiation of the residual melts coming from the Jálama granitic cupola. However, crystallization of the secondary assemblage, richer in Fe and Ta, is interpreted mainly as a consequence of interaction with external fluids coming from the metamorphic host rocks, more or less mixed with meteoric fluids, although partial dissolution and re-precipitation could also have played an important role, as well. ]]>
http://www.jgeosci.org/rss.php?ID=jgeosci.113 Original Paper http://www.jgeosci.org/rss.php?ID=jgeosci.113
<![CDATA[ Effect of natural irradiation in fluorites: possible implications for nuclear waste management? ]]> Vlček V, Skála R, Goliáš V, Drahokoupil J, Čížek J, Strnad L, Ederová J; Vol. 57, issue 1, pages 45 - 52
Samples of naturally irradiated fluorite have been analyzed by means of X-ray powder diffraction analysis (XRPD), differential scanning calorimetry (DSC) and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS). The diffraction patterns of all irradiated samples show peak broadening caused by micro-strain, which was evaluated by Williamson-Hall method, and an increase in the unit cell parameter. The DSC analysis showed an exothermic peak at 273 °C corresponding to enthalpy change about 16 kJ.mol-1. This value is an order of magnitude higher than calculated change due to unit cell volume increase that is only 2 kJ.mol-1. The LA-ICP-MS did not show any significant substitutions, which might account for observed unit-cell parameter increase. The results have shown that high radiation doses lead to formation of defect clusters. ]]>
http://www.jgeosci.org/rss.php?ID=jgeosci.110 Original Paper http://www.jgeosci.org/rss.php?ID=jgeosci.110
<![CDATA[ Raman spectra of minerals containing interconnected As(Sb)O3 pyramids: trippkeite and schafarzikite ]]> Kharbish S; Vol. 57, issue 1, pages 53 - 62
Oriented single-crystals of trippkeite (CuAs2O4) and an isostructural mineral schafarzikite (FeSb2O4) were investigated by polarized Raman spectroscopy. The internal vibrations, i.e. the stretching and bending modes, of trippkeite occur between 250 and 850 cm-1, and those of schafarzikite between 200 and 750 cm-1. The higher mass and the longer bond distances of the SbO3 groups readily explain the lower wavenumbers of the latter. Comparing the spectra of minerals containing XO3 pyramids with those of the minerals from the present study, approximate similarities in the spectral features are evident. A clear distinction between Raman spectra of separated and interconnected (As,Sb)O3 groups is not observed. ]]>
http://www.jgeosci.org/rss.php?ID=jgeosci.111 Original Paper http://www.jgeosci.org/rss.php?ID=jgeosci.111