EGU26-758, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-758
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 04 May, 17:00–17:10 (CEST)
 
Room -2.41/42
Highlighting Natural H2 Generation Potential of the Eastern Mediterranean Ophiolites by Implementing 232Th-238U-40K Concentration Measurements and Thermal Modeling
Ayberk Uyanik
Ayberk Uyanik
  • Product Owner Geoscience - Cegal AS (ayberkuyanik1@gmail.com)

Ophiolitic succession of the Eastern Mediterranean region includes one of the most famous natural H2 leakage spot, globally known as “Chimera Gas Seepage”, noted since ancient times. Geochemical analysis on the seepage revealed that the origin of the gas is abiotic and along CH4, %10-12 of H2 is associated with the seepage due to the serpentinisation process which is widely accepted as one of the main mechanisms for the natural H2 generation.

Radiolysis, considered as another natural H2 generation process, is defined as the decomposition of H2O by decay of 232Th-238U-40K causing an increase in radioactivity levels. Therefore, increasing radioactivity levels can be detected to identify potential natural H2 generating zones by calculating the radiogenic heat generation. This study aims to test this hypothesis by implementing the usually neglected or overlooked 232Th-238U-40K concentration measurements, also known as SGR logs. A-1 well drilled in the onshore portion of the Antalya Bay, SW Turkey, includes 232Th-238U-40K concentration measurements covering an allochthonous ophiolitic section. Penetration into the ophiolites by a well, proximity of well location to the Cirali gas seepage (60 km NE of the seepage) and 2D seismic sections acquired in the region make the study area a perfect spot to test the applicability of integrated methods for natural H2 exploration.

The most significant finding along the ophiolitic section of the A-1 well is the presence of a peak in radiogenic heat generation that might indicate a potential natural H2 generation zone. On the other hand, thermal models derived from the interval velocities of 2D seismic survey nearby indicate that vast majority of generated H2 by serpentinisation process must have migrated from the deepest sections of the ophiolites as temperatures are generally quite low in the area. Apart from that, thermal models also demonstrate the presence of temperature anomalies exhibiting themselves as rapid lateral increases in temperatures that can be associated with the fluids in the sedimentary succession.

As a conclusion, this study provides a unique workflow to reveal potential natural H2 generating zones that can be applied all along the wells if 232Th-238U-40K concentration measurements cover zone of interest not only in the Eastern Mediterranean but for any region. In terms of play fairway, 2 play types have been identified. Naturally generated H2 can accumulate both in the serpentinites as it is already proven by Chimera gas seepage, or it can migrate into Plio-Miocene aged reservoirs in the area. In terms of expulsion mechanism, heavy deformation and compressional tectonic phase controlled by ongoing convergence of African and Anatolian plates create faults and fracture zones that might allow migration of natural H2 from the deeper sections into the shallower structures. However, detailed geomechanical analysis should be performed to understand and prevent potential seal breach risks. The methodologies provided by this study might unlock the path to a potential natural H2 discovery that can turn the Eastern Mediterranean region into a unique natural H2 exploration theatre.

How to cite: Uyanik, A.: Highlighting Natural H2 Generation Potential of the Eastern Mediterranean Ophiolites by Implementing 232Th-238U-40K Concentration Measurements and Thermal Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-758, https://doi.org/10.5194/egusphere-egu26-758, 2026.