Mineralogical, geochemical, fluid inclusion and isotope study of Hohentauern/Sunk sparry magnesite deposit (Eastern Alps/Austria): implications for a metasomatic genetic model
The magnesite deposit of Hohentauern/Sunk, hosted in Viseán carbonate rocks, is one of the best-exposed examples of “Veitsch type” sparry magnesite deposits, which are located in the Veitsch nappe of the Austroalpine Greywacke zone (Eastern Alps/Austria). The sparry magnesite is stratiform and strat...
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Veröffentlicht in: | Mineralogy and petrology 2015-10, Vol.109 (5), p.555-575 |
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Sprache: | eng |
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Zusammenfassung: | The magnesite deposit of Hohentauern/Sunk, hosted in Viseán carbonate rocks, is one of the best-exposed examples of “Veitsch type” sparry magnesite deposits, which are located in the Veitsch nappe of the Austroalpine Greywacke zone (Eastern Alps/Austria). The sparry magnesite is stratiform and stratabound within the Viseán Steilbachgraben Formation and displays distinct metasomatic features and textures. The sparry magnesite of the Hohentauern/Sunk deposit is characterized by pinolites, rosettes and banded (zebra) textures. Due to microinclusions of dolomite and redolomitzation, the CaO/MgO of magnesite is elevated. Concentrations of selected major and trace elements (Fe-Mn, Sr-Ba, Cr-Ni) in sparry magnesite indicate formation in a marine/evaporitic environment and by Mg
2+
-metasomatism. The REE patterns of magnesite are characterized by low LREE/HREE, depletion of LREE and a negative Ce anomaly. The δ
18
O (9.59 to 12.32 ‰ SMOW) and δ
13
C (−2.23 to −0.02 ‰ PDB) values of magnesite overlap with those published for magnesite formed by metasomatic replacement of dolomite. Fluid inclusions in the sparry magnesite indicate a high salinity (22.4 mass% NaCl equivalent) of the Mg-rich fluid; it is of marine/evaporitic origin. All geological, petrographical and geochemical features support a diagenetic dolomitization of the carbonate host rocks followed by magnesite formation via metasomatic replacement and redolomitization. Sm-Nd geochronology indicates a Late Carboniferous to Early Permian age for magnesite formation triggered by intraformational circulation of fluids derived from buried Carboniferous evaporites. |
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ISSN: | 0930-0708 1438-1168 |
DOI: | 10.1007/s00710-015-0386-2 |