B41OA
Oil and Gas Processing
Section A – Flow Assurance
Heriot-Watt University
Edinburgh EH14 4AS, United Kingdom
Produced by Heriot-Watt University, 2018
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1.1 Introduction
Gas hydrates are crystalline compounds formed as a result of physical
combination of water and suitable size molecules at appropriate conditions of
pressure and temperature.
Neighbouring water molecules in the liquid phase are connected together in an
approximately tetrahedral network through hydrogen bonding. Under the right
conditions this network can be formed into cage-like structures, which are
unstable.
Suitably sized molecules, referred to as “guests”, can be trapped in these
cages – thus, stabilising the whole structure and leading to the formation of
solid gas hydrates. The formation of gas hydrates is not limited to gas
molecules; it is known that some molecules that are liquid under ambient
conditions (e.g., benzene, tetrahydrofuran), can also be trapped in the cavities
made by water molecules, resulting in the formation of gas hydrates.
Gas (or liquid) molecules in the gas hydrate structure are called guest
molecules. Gas hydrates are similar to ice, but unlike ice they can form at
temperatures well above ice point. Because they contain around 85% water, in
some respects they behave very much like ice, but they do have some more
unusual properties (Sloan and Koh, 2008).
When they contain combustible molecules like methane they can be burned
directly, as shown in figure 1.
Figure 1: Direct Combustion of Methane Hydrate
(http://blogs.discovermagazine.com/d-brief/2013/03/12/japan-
becomes-first-to-extract-gas-from-frozen-methane/#.V3uD4PkrKM8)
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Another interesting property of gas hydrates is the fact that unlike inorganic
hydrates (e.g., CuSO
4
.5H
2
O) the ratio between water and gas is not constant
(i.e., the hydration number is variable); it depends amongst other things on
temperature, pressure and guest species. In fact this point was the reason
behind much confusion and debate in the past. This point will be discussed in
more detail later.
Gas hydrates were discovered in 1810 by Sir Humphrey Davy, though some
scientists believed that its discovery goes back to 1770s. Initially it was a
scientific curiosity on how a combination of water and gas formed a solid
compound at temperatures higher than 0
o
C.
For the next century or so, several scientists worked on gas hydrates finding
new compounds that can form gas hydrates. Some other scientists
concentrated their research on finding the hydration number of various gas
hydrates.
In 1934, Hammerschmidt found that gas hydrates, and not ice, were
responsible for gas pipeline blockage, see figure 2:
Figure 2: A Hydrate Plug
(http://www.itp-interpipe.com/products/subsea-production-
flowlines/heat-traced-flowlines.php)
This discovery caused considerable amount of funds to be directed towards
gas hydrate research and, over the following 60 years, this funded research
into the thermodynamics of hydrates – leading eventually to methods that
predict the conditions required for their formation.
The main objectives were to find the crystal structures, to define the phase
boundary for gas hydrates of different gases and their mixtures and to develop
methods for the prediction and the prevention of hydrate formation.
In the 1960s natural gas hydrates were discovered in permafrost regions and
marine sediments (Makogon, 1965). Subsequently, various estimates on the
amount of gas hydrates present in these deposits led to the consensus that
they are considerably higher than the total conventional fossil fuels (Makogon,
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1988 and Klauda and Sandler, 2005). Some scientists think that gas from gas
hydrates will play a major role in the energy supply of the world and some put
a contribution of up to 15% within a decade.
Today gas hydrates provide various challenges and opportunities in science
and engineering. They are a potential hazard in deepwater drilling and provide
an opportunity for processing, storage and transportation of oil and gas.
It is also believed that they had important buffering effect on glacial periods
and that they could be responsible for massive submarine landslides and
destructive tidal waves. They also provide an interesting opportunity for the
sequestration of CO
2
.
The necessary conditions for gas hydrate formation are as follows:
•
The presence of water or ice.
•
The presence of suitably sized non-polar or slightly polar gas (or liquid)
molecule.
•
And suitable conditions of pressure and temperature.
High pressure and low temperature promote gas hydrate formation. Very small
molecules like helium cannot form gas hydrates, as they can escape through
the faces of the cage structure. Also, very large molecules won’t form gas
hydrates as they won’t fit in the cage. Various cages and structures involved in
gas hydrate formation will be discussed later.
There is no need for the presence of a gas phase for the formation of gas
hydrates, i.e., gas hydrates can form from liquid hydrocarbon systems. It is
believed that gas hydrates, which form in a liquid hydrocarbon phase system,
are more transportable.
In addition, there is no need for the presence of a water-rich phase (i.e., free
water). Water in the form of mist – resulting from condensation – can provide
the necessary hydrogen bonding for gas hydrate formation.
Another important point is that gas hydrates do not need particularly low
temperature or particularly high pressure conditions for their formation. The
exact condition for gas hydrate formation depends on system composition
(including exact composition of the hydrate forming mixture), the composition
of water phase (e.g., presence of salts and/or other inhibitors), and kinetic
factors.
The combination of these factors can lead to gas hydrates being formed at
surprisingly high temperature and low pressure conditions.
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The extent of gas hydrate formation and the resulting problems depend on the
following factors:
•
The amount of water and hydrate forming compounds: as one of them
can act as limiting reactant.
•
The composition of the fluid and water: as the hydrate free zone is a
function of fluid composition and water activity.
•
The system temperature and pressure conditions: the further the
system is into the hydrate stable zone the more hydrate will form.
•
The amount of kinetic and/or thermodynamic inhibitors: thermodynamic
inhibitors shift the hydrate phase boundary to higher pressures or lower
temperatures. Kinetic inhibitors, in general, increase the induction time
for gas hydrate formation (see later discussion).
•
The presence of natural inhibitors: some fluids have natural inhibitors
reducing the severity of gas hydrate problems.
•
Issues involving heat and mass transfer: a supply of gas molecules (or
water molecules) is necessary for the growth of gas hydrate crystals.
Also gas hydrate formation is an exothermic process and heat is
released during hydrate formation. Any hindrance to mass and/or heat
transfer will reduce the extent of hydrate formation.
•
Some other important factors include the presence of growth modifiers,
local restriction, fluid type, pipe wall characteristics, etc.
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