Temporal and spatial radiogenic heat production rate of granitic plutons from the Eastern Pontides Orogenic Belt, NE Turkey: Constraints for the geothermal resources

IF 1.7 Q3 GEOSCIENCES, MULTIDISCIPLINARY
Mehmet Arslan, İrfan Temizel, Esra Hatipoğlu Temizel
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Abstract

The evaluation of the geothermal potential of the granitic rocks is important in long-term sustainable renewable energy projects due to increasing energy demand. The Eastern Pontides Orogenic Belt in NE Turkey contains a variety of granitic plutons changing in age, size, and composition. In this paper, we discussed the temporal and spatial distribution of radiogenic heat production by using the contents of heat-producing elements (U, Th, K) of the granitic plutons. The average U, Th, and K concentrations for the granitic plutons are 2.97 ± 0.95 ppm, 13.48 ± 3.48 ppm and 2.69 ± 0.47 wt% for Paleozoic plutons, 1.83 ± 0.98 ppm, 8.58 ± 5.10 ppm and 1.77 ± 0.80 wt% for Jurassic plutons, 5.24 ± 1.64 ppm, 26.02 ± 6.43 ppm and 3.17 ± 0.49 wt% for Cretaceous plutons, and 3.82 ± 0.90 ppm, 15.79 ± 4.27 ppm and 2.88 ± 0.40 wt% for Eocene plutons, respectively. Radiogenic heat production rates are 1.43–2.73 µW/m3 for Paleozoic plutons, 0.74–1.70 µW/m3 for Jurassic plutons, 0.66–6.28 µW/m3 for Cretaceous plutons and 1.15–5.22 µW/m3 for Eocene plutons. The studied plutons were classified as low- to moderate heat-producing granitoids. However, some Cretaceous and Eocene granitic plutons with radiogenic heat production values of 5.22–6.28 µW/m3 are considered as high heat-producing granitoids. The thermal indications in the region can be related to radiogenic heat generation and the neotectonic activity of the region. Considering the large volume of the Cretaceous- and Eocene- aged granitic plutons in the Eastern Pontides Orogenic Belt, the moderate to high radiogenic heat production of the granitic plutons in some areas has a significant geothermal impact and can be considered as the potential of enhanced geothermal systems for the future energy demand of the region.

Abstract Image

土耳其东北部庞蒂德斯造山带花岗岩深成岩体的时空辐射产热速率:地热资源的制约因素
由于能源需求的增加,花岗岩地热潜力的评估在长期可持续可再生能源项目中具有重要意义。土耳其东北部的东庞蒂斯造山带包含各种年龄、大小和成分变化的花岗岩深成岩体。本文利用花岗岩深成岩体产热元素(U,Th,K)的含量,讨论了放射性产热的时空分布。花岗岩深成岩体的平均U、Th和K浓度分别为2.97±0.95 ppm、13.48±3.48 ppm和2.69±0.47 wt%,古生代深成岩体为1.83±0.98 ppm、8.58±5.10 ppm和1.77±0.80 wt%,白垩纪深成岩体分别为5.24±1.64 ppm、26.02±6.43 ppm和3.17±0.49 wt%,始新世深成岩体分别为15.79±4.27 ppm和2.88±0.40 wt%。古生代深成岩体的放射产热率为1.43–2.73µW/m3,侏罗纪深成岩体为0.74–1.70µW/m3、白垩纪深成岩体0.66–6.28µW/m3和始新世深成岩体1.15–5.22µW/m3。所研究的深成岩体被归类为低至中等产热花岗岩类。然而,一些白垩纪和始新世花岗质深成岩体的放射成因产热值为5.22–6.28µW/m3,被认为是高产热花岗质岩石。该地区的热迹象可能与该地区的放射成因热和新构造活动有关。考虑到东庞蒂斯造山带白垩纪和始新世年龄的花岗岩深成岩体体积大,一些地区花岗岩深成体的中高放射性热产生具有重大的地热影响,可以认为是该地区未来能源需求的增强型地热系统的潜力。
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来源期刊
Journal of Asian Earth Sciences: X
Journal of Asian Earth Sciences: X Earth and Planetary Sciences-Earth-Surface Processes
CiteScore
3.40
自引率
0.00%
发文量
53
审稿时长
28 weeks
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