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AKKAYA SÖLESTİN YATAĞININ JEOLOJİSİ, MİNERALOJİK-PETROGRAFİK ÖZELLİKLERİ VE İZOTOP (Sr, S, O, H) JEOKİMYASI (ULAŞ, SİVAS-TÜRKİYE)
2019
Journal:  
Kahramanmaraş Sütçü İmam Üniversitesi Mühendislik Bilimleri Dergisi
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Abstract:

Celestine-bearing evaporite mineralization is widespread in Tertiary evaporitic Sivas Basin. Akkaya Celestine deposit is oldest and the biggest open pit mine in the Sivas area. Akkaya Celestine deposit is Eocene in age and characterized by having massif ore. Based on δD (-88 ‰ ile -117 ‰) and δ18 O (O 16.2 ‰ ile 18.1 ‰) data of evaporite minerals, it can be said that sedimentary water is responsible in the formation of Akkaya Celestine deposit. δ34 S data of evaporites from Akkaya Celestine mine is indicate that origin of S is marine evaporite. High δ34 S values (22.9 ‰ ile 30.6 ‰) of celestine indicate that the dissolved sulphur in basinal brines had undergone partial reduction to sulphide.  δ18 O, 87Sr/86Sr (0,707646-0707724-gypsum; 0,707202-0,707391-celestine) with δ34 S suggesting that this evaporite deposit is dominated by a marine signature. All celestine samples have lower 87Sr/86Sr ratios suggest that interstratal brines may have mixed with other circulating fluids (meteoric hydrothermal) that had interacted with the volcanic materials and had undergone Sr isotope exchange. 

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Kahramanmaraş Sütçü İmam Üniversitesi Mühendislik Bilimleri Dergisi

Field :   Mühendislik; Fen Bilimleri ve Matematik

Journal Type :   Uluslararası

Metrics
Article : 200
Cite : 62
2023 Impact : 0.136
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Basic Field of Science and Mathematics
Q2
63/135

Basic Field of Engineering
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44/114

Kahramanmaraş Sütçü İmam Üniversitesi Mühendislik Bilimleri Dergisi