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Arctic Ocean Methane is being Released from Clathrates by Warming Arctic Ocean off Siberia. Jorma Archival Posts
Rising Arctic Ocean temperatures cause gas hydrate
destabilization and ocean acidification
A. Biastoch, 1 T. Treude, 1 L. H. Rüpke, 1 U. Riebesell, 1 C. Roth, 1 E. B. Burwicz, 1
W. Park,1 M. Latif, 1 C. W. Böning, 1 G. Madec, 2 and K. Wallmann 1
Received 21 February 2011; accepted 8 March 2011; published 16 April 2011.
https://oceanrep.geomar.de/id/eprint/13116/1/2011_Biastoch_etal_GRL_2011GL047222.pdf
[ 1 ] Vast amounts of methane hydrates are potentially
stored in sediments along the continental margins, owing
their stability to low temperature – high pressure
conditions. Global warming could destabilize these
hydrates and cause a release of methane (CH 4 ) into the
water column and possibly the atmosphere. Since the Arctic
has and will be warmed considerably, Arctic bottom water
temperatures and their future evolution projected by a
climate model were analyzed. The resulting warming is
spatially inhomogeneous, with the strongest impact on
shallow regions affected by Atlantic inflow. Within the
next 100 years, the warming affects 25% of shallow and
mid‐depth regions containing methane hydrates. Release of
methane from melting hydrates in these areas could
enhance ocean acidification and oxygen depletion in the
water column. The impact of methane release on global
warming, however, would not be significant within the
considered time span. Citation: Biastoch, A., et al. (2011),
Rising Arctic Ocean temperatures cause gas hydrate destabiliza-
tion and ocean acidification, Geophys. Res. Lett., 38, L08602,
doi:10.1029/2011GL047222.
1. Introduction
[ 2] Formed under low temperature – high pressure con-
ditions [Tishchenko et al., 2005] vast amounts of methane
hydrates are considered to be locked up in sediments of
continental margins [Buffett and Archer, 2004; Klauda and
Sandler, 2005]. In the Arctic Ocean (AO), hydrates are
deposited at shallow water depths close to shelf edges,
stabilized by year‐round cold temperatures [Hester and
Brewer, 2009]. Because the Arctic has warmed consider-
ably during the recent decades and because climate models
predict accelerated warming if global greenhouse gas
emissions continue to rise [Intergovernmental Panel on
Climate Change (IPCC), 2007], a destabilization of shallow
Arctic hydrate deposits has been debated [Reagan and
Moridis, 2007; Kerr, 2010]. Methane (CH 4 ), a gas with a
global warming potential ∼25 times higher than CO2 [IPCC,
2007], could be released from the melting hydrates and enter
the water column and atmosphere [Krey et al., 2009]. Recent
field studies indicate an increase in methane fluxes from
submarine Arctic permafrost and the seafloor [Westbrook et
al., 2009; Shakhova et al., 2010]. Our multi‐disciplinary
analysis provides a closer look into regional developments
of submarine Arctic gas hydrate deposits under future global
warming scenarios and reveals where and over which time
scales gas hydrates could be destabilized and affect oceanic
pH, oxygen, and atmospheric methane.
2. Temperature Evolution in the Mid‐depth
Arctic Ocean
[ 3 ] For an evaluation of the general distribution and the
natural variability we investigated the spatio‐temporal vari-
ability of Arctic bottom water in a hindcast experiment with the
ocean/sea‐ice model NEMO (v2.3) [Madec, 2006], carried out
by the DRAKKAR collaboration [The DRAKKAR Group,
2007]. The global simulation was performed at 1/2° reso-
lution (ORCA05) and 46 levels in the vertical, whereby
partial bottom cells allowed realistic topographic slopes.
The experiment, that demonstrated its fidelity in simulating
the salient features of the Atlantic circulation variability
[Biastoch et al., 2008], was forced by inter‐annually varying
atmospheric boundary conditions of the past decades [Large
and Yeager, 2004]. To exclude a potential model drift in the
water masses a second experiment under repeated‐year
forcing was subtracted from the hindcast. The bottom water
temperatures to first order reflect water depth (Figure 1a),
featuring colder values around 0°C below 1000 m and
warmer values on the shelves. However, a clear impact of
the ocean circulation is seen as a band of temperatures
around 1°C surrounding the AO at ∼400 m, an expression of
the Atlantic inflow below the Arctic halocline [Polyakov et
al., 2004]. Colder temperatures appear on the Russian and
Canadian shelves due to the exposure of the surface waters
to continental cold air outbreaks during winter.
[ 4 ] The Atlantic inflow from the European Nordic Seas
(ENS) into the AO exhibits pronounced variability on
decadal time scales [Biastoch et al., 2008], following tem-
perature and transport changes in the branch of the North
Atlantic Current flowing through the ENS [Holliday et al.,
2008]. The flow of Atlantic water towards the AO south
of Svalbard (Figure 2a) shows a remarkable consistency
with observations, both in mean temperature (3.70 ± 0.60°C
vs. 3.96 ± 0.69°C [Holliday et al., 2008]) and variability,
with minima in the late 1970s, mid 1980s and late 1990s.
Changes towards warmer temperatures were reported for the
past few decades [Holliday et al., 2008], which are sup-
ported by the simulated long‐term trend (0.014°C yr−1 ).
Although the long‐term trend (<0.005°C yr−1 ) of the bottom
water is weaker (Figure 2b), a decadal variability by the
Atlantic inflow is also present: changes over a single pentad
repeatedly reach 0.75°C (red lines). The inflow signal extends
to the shelf areas off Russia as part of the cyclonic circu-
1 Leibniz-Institut fu ̈r Meereswissenschaften an der Universita ̈ t Kiel
(IFM-GEOMAR), Kiel, Germany.
2 Laboratoire d’Oce ́ anographie et du Climat: Expe ́ rimentation et
Approches Nume ́ rique, Paris, France.
Copyright 2011 by the American Geophysical Union.
0094‐8276/11/2011GL047222
GEOPHYSICAL RESEARCH LETTERS, VOL. 38, L08602, doi:10.1029/2011GL047222, 2011
L08602 1 of 5
lation around the AO [Dmitrenko et al., 2008]. Although the
Arctic Intermediate Water also varies on a decadal time scale
[Polyakov et al., 2004], bottom water temperatures along the
Russian slope remain almost unaffected (Figure 2c). Only
the shallow and potentially methane‐rich [Shakhova et al.,
2010] shelf regions in the Laptev Sea show significant
annual variations.
[ 5] The future evolution of bottom water temperatures was
analyzed in an ensemble of greenhouse warming integrations
with a coupled climate model (KCM) [Park et al., 2009].
This configuration utilizes the same numerical framework,
but at lower resolution (ORCA2, 2° horizontally, 31 levels)
and the atmospheric model ECHAM5 [Roeckner et al.,
2003] as an active atmosphere. In addition to a 430 year
control experiment with present day greenhouse gas con-
centrations (CO 2 = 348 ppm), an ensemble of eight 100‐year
long global warming simulations, each starting from dif-
ferent states of the control run, were performed with 1%
increase in the CO 2 equivalent concentration [Park et al.,
2009]. The linear trend of the ensemble average was com-
bined with the ORCA05 distribution. The temperature
changes (Figure 1b) show a highly inhomogeneous distri-
bution, with increases of 1–2°C along the continental slopes
and even higher values on the shelves due to the direct
influence from the atmosphere. Individual ensemble mem-
bers resembles strong inter‐annual to decadal variability in
the Nordic Seas (Figure S1 in Text S1 of the auxiliary material)
due to different states of the Atlantic Ocean circulation, but
all feature a consistent long‐term trend of 2.5°C per cen-
tury.1 Anomalies take some decades to protrude into the
Laptev Sea, depending on the state of the Arctic circulation
[Polyakov et al., 2004]; consistent trends are starting typi-
cally after 50 years.
3. Impact on Methane Hydrate Stability and
Ocean Acidification
[ 6 ] Methane hydrate stability in marine sediments is
mainly a function of temperature and pressure [Tishchenko
et al., 2005]. A thermodynamic analysis (Figure 3b) of
selected Arctic regions illustrates that in the ENS the
methane hydrate will experience a phase shift from hydrate
to free gas in mid‐depth levels at around 500 m within the
next 100 years. Natural decadal variability can easily add
another 0.75°C (Figure 2) to the long‐term increase. Along
the Russian slope only shallower depths (∼300 m) undergo a
phase shift.
[ 7 ] For the overall impact of future bottom water warming
on the stability of methane hydrates potentially stored in the
Arctic seafloor we explored the thickness of the gas hydrate
Figure 1. Map of the (a) time‐mean (1985–2004) bottom water temperatures in the ocean hindcast simulation and (b) ensem-
ble‐mean trend in (in °C per 100 years) in the climate model simulation under CO 2 increase. The contour line depicts the 400 m
isobath. The Laptev shelf area used for Figure 2c is marked by black stippling. Acronyms mark the Arctic Ocean (AO),
European Nordic Seas (ENS) and the Laptev Sea (LS).
1 Auxiliary materials are available in the HTML. doi:10.1029/
2011GL047222.
BIASTOCH ET AL.: ARCTIC OCEAN GAS HYDRATES L08602L08602
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stability zone (GHSZ) below the seafloor. The GHSZ is
defined as that part of a sediment column where hydrostatic
fluid pressures are higher than the temperature and salinity
dependent dissociation pressure of gas hydrates. The dis-
sociation pressure was calculated according to Tishchenko
et al. [2005] using the fields from the ocean model and
steady‐state temperatures computed from global heat flow
values in combination with an average sediment conduc-
tivity of 1.5 W m−1 K−1 for present (Figure S2) and future
climates (Figure 3a). To roughly estimate the amount of hydrate
within the GHSZ we used simple constant mean hydrate
pore filling estimates of 2.4% (60–70°N) to 6.1% (north of
70°N) based on ODP data and numerical modeling [Klauda
and Sandler, 2005]. Inhibition of hydrate formation by
sulfate reduction is approximated by including a 5 m thick
hydrate free zone below the seafloor. Assuming a mean
porosity of 0.5 and standard values for density and methane
content of hydrate, we estimated a total inventory of 900 Gt
carbon (C) north of 60°N for the present climate. This value
is not too far off the estimated 500 Gt C based on studies
offshore Alaska [Kvenvolden, 1988] representing a fraction
of the still largely unknown global hydrate inventory of
500–64,000 Gt C [Hester and Brewer, 2009]. Under the global
warming scenario most affected regions are distributed around
the AO and the ENS. Areas exhibiting decreases ≥20 m in
the GHSZ thickness sum up to a total size of ∼850,000 km2
resulting in a total methane release of ∼100 Gt C. However,
these estimates are too high for the considered 100‐year time
window and need to be adjusted for the sluggish diffusion of
heat into marine sediments. Using a constant thermal diffu-
sivity of 4 × 107 m s−2 and neglecting the latent heat of hydrate
melting, we find that only 12% of the worst‐case hydrate
volume is reduced after 100 years for sulfate reduction zone
thicknesses 5 m (Figure 3c). Note that sensitivity runs with
0 and 10 m sulfate reduction zone thicknesses show reductions
of 14 and 10%, respectively.
[ 8 ] What could happen to the released methane? It is
conceivable from environmental hydrate studies that,
depending on the release rate, at least ∼50% of the methane
that dissolves into the sediment porewater, could be retained
inside the seafloor by microbial anaerobic oxidation of
methane (AOM) [Knittel and Boetius, 2009; Treude et al.,
2003]. AOM represents a long‐term sink for methane‐
derived carbon, converting methane into bicarbonate and
eventually precipitating it as authigenic carbonates [Peckmann
et al., 2001]. However, methane rising through sediments as
free gas could bypass the benthic methane filter [Knittel
and Boetius, 2009] and, depending on water depth
[McGinnis et al., 2006], immediately reach the atmosphere.
Methane that on the other hand dissolves into the water
column could be utilized by microbial aerobic oxidation of
methane [Valentine et al., 2001]. Different to its counterpart
AOM in sediments, aerobic oxidation of methane converts
methane with oxygen into CO2 – a molecule that can impact
oceanic pH.
[ 9 ] For the following scenario we assume that 50% of the
methane from the transient GHSZ thickness change is
released into the water column and consumed by aerobic
methanotrophs. A Lagrangian analysis of the oceanic cur-
rents (auxiliary material) shows that (within a given year)
the bulk of the water affected by methane is kept within 100 m
above the bottom and along the mid‐depth topographic
slope. Changes in seawater carbonate chemistry were cal-
culated by adding the microbial produced CO2 to the back-
ground dissolved inorganic carbon (auxiliary material).
Some areas of the AO revealed pH values to drop by up to
0.25 units (Figure 4) within the next 100 years. Additionally,
the aerobic consumption of methane could locally decrease
bottom water oxygen concentrations by up to 25% (auxiliary
material, data not shown). Regional methane‐induced sea-
water acidification from the seafloor would occur in addition
to an ocean‐wide acidification caused by the uptake of
anthropogenic CO 2 from the atmosphere [IPCC, 2007]. The
combined effect of the two processes would accelerate ocean
acidification in parts of the AO, including deeper waters
which otherwise would be exposed to ocean acidification
with a considerable time delay. Research on that topic so far
has been conducted under the premises of a projected pH
decrease due to the anthropogenic CO 2‐uptake of about
0.3 units until the end of this century. Methane‐induced acidi-
fication could nearly double this decrease in parts of the AO.
[ 10] If, in a rather unrealistic scenario, all of the liberated
methane would reach the atmosphere, global warming could
be amplified [Bartdorff et al., 2008]. Under transient con-
ditions we estimated an additional average methane flux of
only 162 Mt CH4 yr−1 from melting Arctic hydrates over the
next 100 years (auxiliary material) – a value lower than the
current anthropogenic input of (600 Mt yr−1 ) [Bartdorff et
al., 2008]. Sensitivity experiments with the climate model
confirm the negligible feedback of the climate system under
Figure 2. Variability of temperatures in the hindcast simu-
lation, shown by monthly and inter‐annually filtered tem-
peratures of (a) the Atlantic inflow (50–200 m depth) off
Svalbard and bottom water temperatures (b) along the east-
ern continental slope in the ENS off Svalbard and Norway
(water depth 416–793 m) and (c) along the Russian conti-
nental slope, (black, 416–793 m, 90–180°E) and on the shelf
(blue, 0–100 m) in the Laptev Sea. The red lines mark trends
in particular 5‐year periods.
BIASTOCH ET AL.: ARCTIC OCEAN GAS HYDRATES L08602L08602
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this limited additional amount of methane (Figure S3). On a
longer time scale, however, the transient heat conduction
leads to a faster methane release; the methane released from
the steady‐state GHSZ calculation causes an upper limit of
0.8°C increase in surface air temperature on top of global
warming.
4. Conclusions
[ 11] The present study is to our knowledge the first
combining ocean hindcasts and future climate projections
with GHSZ calculations and potential consequences. It
should be noted that the overall model still has its limitation
with respect to the resolution of the bottom water tem-
peratures, the actual distribution of sub‐seafloor methane
hydrates and the individual response of the microbial com-
munity in the sediment and water column. Nevertheless, the
study clearly shows that hydrate destabilization can occur in
the Arctic in response to global warming, and that the
potential methane release is substantial, but limited in the
next 100 years. An important finding is that warming and
variability of the Atlantic inflow will play a major role in the
fate of Arctic gas hydrates. Recent observations [Westbrook
et al., 2009; Reagan and Moridis, 2009] agree well with
sensitive areas identified here. Our maps could represent a
useful tool in identifying areas around the Arctic Ocean
where increases in methane release are likely to occur now
or in the near future.
[ 12 ] Acknowledgments. This research was part of the Custer of
Excellence “The Future Ocean” funded by the German Research Founda-
tion (DFG). The integrations of the experiments have been performed at
the Computing Centre at Kiel University.
[ 13] The Editor thanks one anonymous reviewers for their assistance in
evaluating this paper.
Figure 4. Changes in pH due to the release of 50% of the
methane from hydrates within the first 100 years and distrib-
uted over the first 100 m above the bottom.
Figure 3. (a) Changes in thickness of the GHSZ caused by temperature increase of the ensemble mean of the global warm-
ing, (b) phase diagram of methane hydrate as a function of pressure and temperature (constant salinity of S = 35 p.s.u.).
Open symbols mark the bottom water temperatures along the ENS (cycles) and Russian (squares) slopes in the present cli-
mate run, closed symbols the greenhouse warming experiments. Vertical bars indicate the vertical resolution of the ocean
model. (c) Volumetric GHSZ thickness changes north of 60°N as a function of time. A value of 100% corresponds to the
worst case scenario. The shaded range marks estimates for 0 and 10 m sulfate reduction zone thickness.
BIASTOCH ET AL.: ARCTIC OCEAN GAS HYDRATES L08602L08602
4 of 5
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A. Biastoch, C. W. Böning, E. B. Burwicz, M. Latif, W. Park, U. Riebesell,
C. Roth, L. H. Rüpke, T. Treude, and K. Wallmann, Leibniz‐Institut für
Meereswissenschaften an der Universität Kiel (IFM‐GEOMAR),
Düsternbrooker Weg 20, D‐24105 Kiel, Germany. (abiastoch@ifm‐
geomar.de)
G. Madec, Laboratoire d’Océanographie et du Climat: Expérimentation
et Approches Numérique, 4, place Jussieu, F‐7525 Paris CEDEX 05,
France.
BIASTOCH ET AL.: ARCTIC OCEAN GAS HYDRATES L08602L08602
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