Gas Hydrates In The Ocean

Stefan G. Llewellyn Smith
Devin Conroy       


Gas hydrates are crystalline compounds, made up of water molecule cages held together by hydrogen bonding. The cavities that form are large enough to incorporate a guest gas that stabilizes the structure under low temperature and high pressure. The most abundant type of gas hydrates on earth are natural gas hydrates, which contain mostly methane and a few hydrocarbons such as ethane, propane and iso-butane. These crystals are generally found in the deep ocean and permafrost regions attached to the sediment that makes up the sea  floor where the temperatures are cold and pressures high. Their location is also constrained by a source of gas which comes from either deposits within the earth (thermogenic) or from the decomposition of organic matter (biogenic).   
 
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A Representative diagram for in-situ gas hydrates is shown above for deep ocean regions. The hydrate stability zone (HSZ) is an area determined from the phase diagram, where the temperature and pressure conditions are ideal for formation. The lower edge of the HSZ occurs, in general ,some distance below the ocean  floor since the temperature increases due to the geothermal gradient. This point is believed to coincide with the 3-phase point (gas, hydrate, water) with hydrate above and dissociated gas and water below. The upper end of the HSZ occurs higher in elevation because the pressure is decreasing. In the case of permafrost regions the hydrates can be stable at this low pressure since the temperatures can be quite cold. In most cases the top of the hydrate layer doesn't coincide with the sea  floor but exists some distance below the sediment.

In recent years experts have come to believe that there are massive quantities of methane gas stored in the form of hydrates at the bottom of the ocean. This information has mainly been inferred from bottom simulating reflectors (BSR) that were dragged along the ocean floor and verified by core samples. Since an estimated 1 m3 sample of pure hydrate would yield approximately 180 m^3 of methane gas, many people have come to believe that there is more energy stored in all the hydrates (an estimated 10^19 g of carbon) than all the fossil fuel reserves on earth. With all this methane many people have proposed ways of mining it for use as the next energy source when fossil fuels become too expensive. Some people on the other hand are afraid of global warmer if the gas were to ever reach the surface since methane gas is 23 times more effective than carbon dioxide as a green house gas on a per-mole basis.

The methane hydrates contained at the bottom of the ocean have the potential to dissolve into the water if the dissolved gas concentration is low enough or pass through the 3-phase equilibrium point if the temperature, pressure and salt concentrations are right. The gas that has left its cage will percolate through the sediment, generally along fractures, and rise to the ocean surface. Since the ocean is essentially a giant capacitor for dissolved methane gas the bubbles will only reach the atmosphere if the time scale for dissolution is much longer than the gas residence time in the water. The dissolved gas may also enter the atmosphere on a much longer time scale only if the rate of transport is faster than the rate of bacterial oxidation.


Specific Goals

The specific goals of the project are:



Pictures

During a week long workshop with chemistry and Biology high school teachers we made propane hydrates as a part of a laboratory activity. The hydrate was made by filling a small stainless steel cell with ground ice, pressurizing with propane and leaving the apparatus in an ice bath over night.

Propane hydrate just taken from the ice bath.



Propane hydrates on fire.



Links

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Contacts

Devin Conroy

Department of Mechanical and Aerospace Engineering
University of California, San Diego
9500 Gilman Drive
La Jolla CA 92093-0411
USA
E-mail: dconroy@_ucsd.edu



This work is supported by NSF grant CHE-0404743