a methane molecule in a "water cage" is a methane hydrate
What are Methane hydrates and why are they important?
Gas hydrates are ice-like crystalline structures that form in deep-sea
sediments when a low-density gas, like methane (CH4), ethane (C2H6),
or carbon dioxide (CO2), combines but does not chemically bond
with water and freezes into a solid under low temperature and moderate
pressure conditions.
Various names include methane clathrate, hydromethane, methane ice, fire
ice, natural gas hydrate, or gas hydrate.
While, for reasons unknown, often sidelined in climate remediation
strategy discussion, their relatively rapid release into an already
warming atmosphere need to be taken into account. Consequences to ocean
life, continental life, humankind, ocean acidification and adding
greenhouse gas to the atmosphere. There are plans, in some circles, to
exploit methane hydrates as a fossil fuel resource with the risk of
accelrated release of Methane CH4
methane "ice" in permafrost
On Earth, gas hydrates occur naturally in some marine sediments and within
and beneath permafrost. They are likely found on other planets.
The Importance of Methane Hydrate:
Huge Carbon Sink - maybe twice the carbon contained in all reserves
of coal, oil, and conventional natural gas combined,
Potentially huge fossil fuel source but it comes with risk...
Huge Environmental Risk - Their decomposition could release large
amounts of the greenhouse gas methane, that will negatively impact
Earth’s climate.
Potential Explosive Release - The sudden release of pressurized
methane gas could cause huge submarine landslides, which in turn
could trigger tsunamis.
Biological risks - Gas hydrates in the ocean associated with
unusual and possibly unique biological communities that use
hydrocarbons or hydrogen sulfide for carbon and energy, via a
process known as chemosynthesis. We do not know the extent or
significance of these process or what role they play in nature.
On current trends as the Oceans and the Arctic permafrost warm large
quantities of methane (CH4) will be liberated into the
atmosphere contributing to accelerated warming. The Earth's contemporary
period of climate change will reach a tipping point, whether this process
will be gradual or catastrophic is subject to debate.
Methane in a "water cage" and the types of "ice" structures it can
form
How do Methane Hydrates form?
Methane hydrate is an ice-like substance formed when CH4 and
water combine at low temperature (up to about 25ºC) and moderate pressure
(greater than 3-5 MPa, which corresponds to combined water and sediment
depths of 300 to 500 m). Globally, an estimated 99% of gas hydrates occurs
in the sediments of marine continental margins. Methane hydrate
concentrates methane CH4 by about 164 times on a volumetric
basis compared to gas at standard pressure and temperature.
In the oceans - methane hydrates occur mainly near the
continental margins at water depths between 350 and 5000 metres. Here
methane gas is primarily formed by microorganisms that live in the
sediment layers and slowly convert organic substances to methane. Methane
can be released by a drop in pressure and/or a rise in temperature.
These organic materials are the remains of plankton that lived in the
ocean long ago, then sank to the ocean floor, and were finally
incorporated into the sediments.
The sea floor is thus an ideal location for methane hydrate formation:
because...
the bottom waters of the oceans and the deep seabed are almost
uniformly cold, with temperatures from 0 to 4 degrees Celsius.
Below a water depth of about 350 metres, the pressure is sufficient
to stabilize the hydrates.
Once the sediment/ hydrate layer gets to be about 1km thick, due to
internal sediment temperatures and proximity to the Earth’s interior
, temperatures rise above about 25ºC, and methane hydrate deposition
throughout the sediment stops. But as the released small methane bubbles
rise in the sediment, they are cooled and transformed back into more
concentrated methane hydrate along the cooler upper sediment / ocean water
boundary.
Almost no methane hydrate is found in really deep water. While the
temperature and pressure are OK, the water is nutrient poor and produces
insufficient organic matter for methane production/ concentration.
In the Arctic - permafrost, is mostly a relic of the last ice age.
While the top layer of permafrost may melt in summer most of it remains
frozen and the top layer re-freezes each year. Called the "active layer"
it thaws during the summer, allowing plants to grow in a variety of
ecosystems—such as grasslands, forests, and wetlands. In some parts of the
Arctic, the landscape features a polygon-like pattern, formed when the
frozen ground contracts evenly is all directions, forming cracks
during the cold winter months. These cracks fill with meltwater in spring,
which then freezes, creating ice wedges and giving the surface its
distinct, appearance. Permafrost is predominantly found in the Northern
Hemisphere, particularly in the Arctic region, where it covers about a
quarter of the land’s surface. In places like Siberia, it can reach depths
of up to 1500 meters. As atmospheric temperatures rise, the "active layer"
is getting thicker in summer and facilitating the release of methane
gas CH4 from the ancient frozen permafrost methane
hydrates.
global locations of methane hydrate
Commercial extraction of methane hydrates in the deep ocean would
involve putting a dual-tube drill string (pipe) into a large concentrated
methane hydrate deposit and
either applying heat or reducing pressure. The methane would sublimate
into gas and come to the surface under its own pressure.
There are problems to this however, once the gas begins to rise, the
pressure will reduce at the deposit end of the drill string, releasing
more gas.
So more surface area of the deposit is exposed increasing the rate of
sublimation...
A self-sustaining accelerating process could start resulting in
explosive release of methane.
If the drill string remained intact the gas could explosively
release to the atmosphere.
If the drill string was ruptured much of the gas would be
re-absorbed in the ocean water creating a "pocket" of acidified water
, killing marine life.
How long would it this "pocket" would take to dissipate in the still
waters of the deep ocean?
When drilling through loose sediment into "ice" - how do you secure
the wellhead to an ocean floor, to prevent leakage or collapse, when
it consists of loose sediment and "ice"?
A natural example: the explosive limnic eruptions of carbon dioxide on
Lake Kivu on the border of Rwanda and the Democratic Republic of the Congo
(and how they are now under control).
Affect on climate of a release of methane
The release of increased methane into the atmosphere , whether slowly or
catastrophically is bad news for us all.
If just 0.1% (1.8 Gt C) of this CH4 were instantaneously
released to the atmosphere, CH4 concentrations would, it
has been estimated would increase from about 1774ppb (2005 value) to
around 2900 ppb (source IPCC 2007).
Methane CH4 is about 20 times more potent than CO2
as a green house gas..
Methane CH4 concentrations have already risen by about
150% since pre-industrial times, compared to only about 40% for carbon
dioxide CO2
It oxidizes carbon dioxide CO2 after about a decade in
the atmosphere.
In recent models, the longer-lived CO2 oxidation product
, not the CH4 itself, is credited with causing most of the
excess atmospheric warming but that could change that would follow
large-scale dissociation of methane hydrates.
Rising atmospheric CH4 concentrations lead to more rapid
depletion of the hydroxyl radicals needed for oxidation, this would
mean longer CH4 residence times, and thus increased CH4-induced
warming
Present-day CH4 emissions are dominated by wetlands,
ruminants, fossil fuel production, and rice cultivation sources that
fluctuate with season, human behavior, and other factors.This makes
detection of hydrate derived methane from melting release or
commercial extraction difficult to separate from the background
variations
Methane Hydrates and Past Warming Events
The geologic record is punctuated by warming events, measurements of the
methane content in ice cores, may provide clues about future interactions
between methane hydrates and contemporary climate change.
Climatic changes in the past could resulted from destabilization of
methane hydrates and thus to the release of methane.
For example:
The Paleocene-Eocene Thermal Maximum (PETM) at ~54.95 Ma where a
large, negative carbon isotopic excursion (CIE) recorded in both
marine and terrestrial sediments has been interpreted as reflecting
widespread release of isotopically-light (microbial) carbon from
dissociating marine methane hydrates
Repeated warming of intermediate ocean waters during the Late
Quaternary (since 400 ka) triggered periodic hydrate dissociation
events
Northern hemisphere wetlands, which may experience increased
production of isotopically-light CH4 in response to local
warming, appear to be the key culprit in enhancing atmospheric CH4
concentrations during several Pleistocene (~2.6 Ma to 10 ka) and
Holocene (since 10 ka) warming events.
Fate of Contemporary Methane Hydrates During Warming Climate
The susceptibility of gas hydrates to warming climate depends on:
the duration of the warming event,
their depth beneath the seafloor or tundra surface, and
the amount of warming required to heat sediments to the point of
dissociating gas hydrates.warming events
Even over 100 yr, only gas hydrates close to the seafloor and initially
within a few degrees of the thermodynamic stability boundary might
experience dissociation in response to reasonable rates of warming.
Less than 5% of the gas hydrate inventory may meet these criteria.
Global Warming and Gas Hydrate Type Locales
Methane hydrates occur in five geographic locales that must be
individually evaluated to determine their susceptibility to warming
climate (see Figure below).
The 5 methane hydrate locales described below:
GHSZ below refers to the gas hydrate stability zone in the diagram
Locale 1. Thick (> 300 m) continuous permafrost onshore (<1%).
Deep gas hydrates beneath capping, permafrost-bearing sediments are stable
over warm periods that endure more than 100 yr , even under scenarios of
doubling atmospheric CO2
Only gas hydrates to a depth of about 225 m depth for pure CH4 hydrate
within permafrost, might be vulnerable to dissociation due to atmospheric
warming over 100 yr.
Locale 2. Subsea permafrost on the circum-Arctic shelves (<0.25%?).
Sediments on shallow marine continental shelves that fringe the Arctic
Ocean are often underlain by permafrost and associated gas hydrates that
formed in Pleistocene time, when these regions were sub-aerial and exposed
to much colder annual temperatures.
Since the Late Pleistocene, marine inundation of these former coastal
plains has led to large (up to 17ºC) temperature increases, partial
thawing of sub-sea permafrost and inferred dissociation of gas hydrates.
Locale 3. Deepwater marine hydrates at the feather edge of Gas Hydrate
Stability Zone GHSZ (~3.5%).
The deepwater marine hydrate system thins to vanishing at shallow water
depths (usually about 500 m) on the upper continental slopes. Because the
entire GHSZ lies near the seafloor, upper continental slopes are the most
susceptible places on Earth for wholesale gas hydrate dissociation driven
by warming of impinging intermediate ocean waters. A maximum 3.5% of the
global gas hydrate inventory might occur in these vulnerable settings.
Locale 4. Deepwater gas hydrates (~95.5%). These gas hydrates,
which constitute most of the global inventory, generally have low
susceptibility to warming climate over time scales shorter than a
millennium. The gas hydrates closest to the edge of thermodynamic
stability lie deep within the sedimentary section and close to the base of
the GHSZ. Sustained bottom water temperature increases lasting many 100 yr
would be required to initiate warming, no less dissociation. Even if CH4
is released from gas hydrate and is able to migrate toward the seafloor,
some CH4 may be trapped in newly formed gas hydrate and much
will be consumed on the sediment/ocean boundary.
Locale 5. Seafloor gas hydrate mounds (trace).
At some marine seeps, massive, relatively pure gas hydrate occurs in
seafloor mounds (e.g., Gulf of Mexico) and in shallow subsea floor layers
or conduits. These mounds are shown schematically as deepwater phenomena
in the above Figure, but in fact often occur at upper continental slope
depths. While seafloor gas hydrate mounds and shallow sub-sea floor gas
hydrates constitute only a trace component of the global gas hydrate
inventory, they can dissociate rapidly due to expulsion of warm fluids
from the seafloor, warming of overlying waters , or possibly pressure
perturbations .
Natural catastrophic, widespread dissociation of methane gas
hydrates will not be triggered by continued climate warming at
contemporary rates (of about 0.2ºC per decade) over timescales of a
few hundred years.
Most methane hydrates occur at low saturations and in sediments at
such great depths below the seafloor or onshore permafrost that they
will barely be affected by warming over 100 yr.
Even when CH4 is liberated from gas hydrates, oxidative
and physical processes may greatly reduce the amount that reaches the
atmosphere as CH4.
The CO2 produced by oxidation of CH4 released
from dissociating gas hydrates will likely have a greater impact on
ocean acidification and greenhouse gas levels.
Contemporary and future gas hydrate degradation will occur primarily
on the circum-Arctic Ocean continental shelves
and at the feather edge of the GHSZ on upper continental slopes
(Locale 3), where the zone's full thickness can dissociate rapidly due
to modest warming of intermediate waters.
What happens when methane hydrate melts?
Not all the methane that is released from unstable methane hydrates
ends up in the atmosphere. The greatest portion is likely to be broken
down during its rise through the sediments and in the water column.
This decomposition is mediated by two biological processes: anaerobic
oxidation of methane by bacteria and archaea within the sea floor;
aerobic oxidation of methane by bacteria in the water column.
During anaerobic oxidation of methane in the sediment the microbes
use sulphate (SO42–), for the methane
decomposition. At the end of this process calcium carbonate (CaCO3)
precipitates, which can remain stored in the sea floor .
During aerobic oxidation in the water column, bacteria break down
methane with the help of oxygen (O2). This process has two
negative effects
carbon dioxide is produced and contributes to ocean acidification
and
aerobic oxidation of methane consumes oxygen. create or expand
fish / marine life threatening low oxygen zones
Rough estimates suggest that anaerobic and aerobic oxidation of
methane together currently convert around 90 per cent of the methane
produced in the sea floor before it can reach the atmosphere. The more
slowly methane migrates through the sea floor or through the water
column, the more effective the microbes are in converting it. A
prerequisite for this kind of degradation is that the methane
molecules are dissolved in water. Methane can only be degraded by the
bacteria in this form.
The disappearance of methane hydrates could have fatal consequences. Gas
hydrates act like a cement that fills the pores between the fine sediment
particles and stabilizes the sea floor. If the methane hydrates decompose,
the stability of the sea floor is reduced due to the missing cement and
the possible generation of excess pore pressure. In the worst case, large
parts of continental margins fail. The resulting submarine landslides
might cause severe tsunamis. The question is - do we really need to
exploit this resource or would it be more prudent to leave it alone?
image: Ruppel, C. et al. Degradation of subsea permafrost and associated
gas hydrates offshore of Alaska in response to climate change. Sound Waves
128, 1-3 (2010). http://soundwaves.usgs.gov/2010/11