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| Titel |
Black Sea mud volcanoes and their relation to the search for methane gas
hydrates and environmental security |
| VerfasserIn |
Evgeny Shnyukov, Valentina Yanko-Hombach, Irena Motnenko |
| Konferenz |
EGU General Assembly 2016
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| Medientyp |
Artikel
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| Sprache |
en
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 18 (2016) |
| Datensatznummer |
250123844
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| Publikation (Nr.) |
 EGU/EGU2016-3163.pdf |
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| Zusammenfassung |
| As of today, the number of known offshore mud volcanoes in the Black Sea is 68. The areas
possessing the greatest abundance include the northern part of the Black Sea (Sorokin trough,
Tuapsinskaya trough, Shatskiy arch) and the Kerch downfold (the area south of the Kerch
peninsula). An intensive study of mud volcanoes has been performed in the course of
on-shore and off-shore expeditions carried out by Ukrainian scientists since 1990. They
brought to light new geological, geophysical, and geochemical data on the properties of
mud volcanoes by (1) high resolution hydro-acoustic, seismic-acoustic, and gravity
methods, (2) geothermal observations of the thermal regime of the water and uppermost
sediments, (3) gravity core sampling of bottom deposits, (4) dredges and buckets, and (5)
study of these samples by lithological, geochemical, paleontological, and biological
methods.
Methane gas hydrates have been recovered in about 28 localities largely associated with
mud volcanoes below 600-700 m water depth, which suggests their close genetic
relationships. Age of the sediments hosting methane gas hydrates as well as their
lithological properties (e.g., grain-size) vary significantly. Relatively coarse-grained
sediments make better hydrate reservoirs than fine-grained sediments. The area
of the Black Sea suitable for gas hydrate formation is estimated at 288,100 km2,
representing about 68% of the total Black Sea, or almost 91% of the deep-water basin; the
volume of gas hydrates has been set at 4.8 km3 corresponding to 0.1-11012 m3 of free
methane.
A peculiar morphological structure of the sea bottom—conical hills (anticlinals) with low
geostatic pressure and subsidence in their central part—provide a target in the search for
underwater mud volcanoes. Our data show that such structures are formed by mud
breccia and rock debris that are brought to the surface by methane flows, which
escape along tectonic ruptures from the deep part of the lithosphere located beneath
a Mesozoic sediment cover. The amount of escaped methane is enormous. For
example, the mud volcano “Yuzhmorgeologiya” ejects about 17.8 billion m3 of breccia
during one eruption, which requires trillions of cubic meters of gas. As a result of
huge movements of sediment mass from the depths to the surface, areas of low
geostatic pressure and subsidence are formed that are framed by ring or half-ring
grabens, or compensation synclines. These ring structures serve as vents for gas
emissions that catch sediments on their way and form gas-soaked ice (gas hydrates) if
the volcanoes are located below 600-700 m water depth where thermodynamic
conditions allow gas hydrates to crystallize. In fact, mud volcanoes are the sea
floor’s expression of endogenic processes, serving as “cheap windows” into the deep
geosphere. Our presentation will show that they can be used as high-efficiency, low
cost indicators in the investigation of gas hydrates, including those suitable for
industrial exploration, and that their eruptions play a harmful role in the environment. |
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