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A GLOBAL OUTLOOK ON METHANE GAS HYDRATES

9

Methane gas hydrates form naturally where adequate supplies

of methane and water can combine in a location with both

high pressure and relatively low temperature. The methane

itself is created by the decomposition of organic carbon, which

generally migrates upward through water-laden sediment. In

the right conditions, this triggers the formation of gas hydrates.

Gas hydrates can form naturally in the Gas Hydrate Stability

Zone (GHSZ), the depths at which pressure and temperature

are suitable for gas hydrates. Exactly where the GHSZ is

found and how far it extends depend on local conditions.

In the Arctic, where cold air temperatures create thick zones

of permanently frozen soils (permafrost), the top of the GHSZ

typically lies about 300 to 400 metres below the land surface,

often in the midst of the permafrost. In regions of relatively

thick permafrost, the GHSZ often extends 500 metres or

more below the base of the permafrost.

In oceans or deep inland lakes, where high pressures are

generated by 300 to 500 metres or more of overlying water,

the top of the GHSZ occurs within the water column, and the

base is some distance below the sea floor.

HOW ARE GAS HYDRATES FORMED?

Depth (metres)

Depth (metres)

Temperature ºC

gnittes tsorfamreP

gnittes eniraM

Temperature ºC

Stability conditions for gas hydrates

0

0

200

400

600

800

1000

1200

1400

1600

200

400

600

800

1000

1200

1400

1600

20

0

01

3

0

-30

-20

-10

0

10

20

30

Base of permafrost

Stability zone

Stability zone

Ground surface

Ice freezing temperature

Sea surface

Sea floor

Summary Graphic 2:

Phase diagrams illustrating where methane hydrate is stable in marine (A) and permafrost settings (B). Hydrate

can exist at depths where the temperature (blue curve) is less than the maximum stability temperature for gas hydrate (given by the

hydrate stability curve in orange). Pressure and temperature both increase with depth in the Earth, and though hydrates can exist at warmer

temperatures when the pressure is high (orange curve), the temperature in the Earth (blue curve) gets too hot for hydrate to be stable,

limiting hydrate stability to the upper ~1km or less of sediment.

A

B