Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica

  • Giustiniani M
  • Tinivella U
  • Sauli C
  • et al.
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Abstract

The theoretical gas hydrates stability zone (GHSZ) in the Ross Sea area was evaluated by mean of a steady state simple approach by using bathymetric data, sea bottom temperature, a variable geothermal gradient and assuming that the natural gas is methane. The results from our study suggest that bathymetry and distribution of the GHSZ are correlated; in fact, the GHSZ reaches a maximum (ca. 400 m) in the basins, where the water temperature is the lowest, and decreases in the banks with thickness ranging between 7 and

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Giustiniani, M., Tinivella, U., Sauli, C., & Della Vedova, B. (2017). Distribution of the gas hydrate stability zone in the Ross Sea, Antarctica. Andean Geology, 45(1), 78. https://doi.org/10.5027/andgeov45n1-2989

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