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1
Carbon isotope equilibration during sulphate-‐limited anaerobic oxidation of
methane
Marcos Y. Yoshinaga1*†, Thomas Holler2†, Tobias Goldhammer1, Gunter Wegener1,2,3*, John W.
Pohlman4, Benjamin Brunner2, Marcel M. M. Kuypers2, Kai-‐Uwe Hinrichs1, Marcus Elvert1
1. MARUM Center for Marine Environmental Sciences and Department of Geosciences, University of Bremen, D-‐28359
Bremen, Germany; 2. Max Planck Institute for Marine Microbiology, D-‐28359 Bremen, Germany; 3. Alfred Wegener
Institute for Marine Ecology and Technology, HGF-‐MPG Research Group for Deep Sea Ecology and Technology, D-‐27515
Bremerhaven, Germany; 4. U.S. Geological Survey, Woods Hole Coastal and Marine Science Center, Woods Hole,
Massachusetts 02543, USA.
* Email: [email protected]; gwegener@mpi-‐bremen.de; † these authors contributed equally to this work.
Supplementary Information Table of Contents
1. Culture Experiments
2. Detailed method description and evaluation of background methanogenesis
3. Compilation of global flux data
4. Isotope mass balance model
5. Supplementary References
Carbon isotope equilibration during sulphate-limited anaerobic oxidation of methane
SUPPLEMENTARY INFORMATIONDOI: 10.1038/NGEO2069
NATURE GEOSCIENCE | www.nature.com/naturegeoscience 1
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1. Culture experiments
Sediment-‐free anaerobic oxidation of methane (AOM) enrichment cultures were retrieved by
continuous incubation of methane seep sediments obtained from Hydrate Ridge (offshore Oregon,
USA) and Amon Mud Volcano (Mediterranean Sea) with methane and sulphate as the only energy
sources (see ref. S1). Background methane production was evaluated in these AOM cultures
incubated with sulphate-‐free medium and both N2:CO2 and N2:CO2:H2 headspace. Resulting methane
production rates were compared with sulphide production values (equal to methane oxidation) at
AOM conditions (Eq. 1, Supplementary Fig. S1). Biotic (methane-‐free) and abiotic (incubation
medium without AOM culture) control incubations were performed (Supplementary Fig. S2) to verify
the carbon isotope effects examined in sulphate-‐limited AOM experiments (Fig. 2 and
Supplementary Fig. S3).
2. Detailed method description and evaluation of background methanogenesis
To determine background methane production in relation to AOM, cultures were washed 4
times with sulphate-‐free medium with pH set to 7.2 (via addition of NaOH). Aliquots of 10 mL that
contained similar cell density were transferred into 20 mL Hungate culture vials. Background
methanogenesis was evaluated by filling the headspace with 2 atm of N2:CO2 (90:10; all gases Air
Liquide; Düsseldorf, Germany). We also attempted to stimulate methanogenesis by adding a
hydrogen-‐enriched headspace of 2 atm N2:CO2:H2 (45:15:40). All samples were continuously shaken.
Every 3 to 4 days, 1 mL headspace gas was sampled with a gas tight glass syringe (gas volume was
replaced by N2:CO2) and methane concentrations were determined by gas chromatography coupled
to a flame ionization detector (GC-‐FID, Focus GC, Thermo). The detection limit for methane
concentration using this setup was 1 ppm. To ensure that the culture was metabolically capable of
AOM and to compare rates of methane production to methane oxidation, we performed parallel
incubations under AOM conditions (10 mM sulphate, 2 mM methane). Sulphide production, as proxy
for AOM activity, was determined spectrophotometrically via copper sulphide formationS2.
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3
Supplementary Figure S1| Evaluation of background methanogenesis in sulphate-‐free incubations of AOM cultures from Hydrate Ridge (HR) and Amon Mud Volcano (AMV). Panels a and c, development of methane (CH4) concentrations without additional energy substrates (triangles) and with the addition of 0.8 mM H2 headspace (squares) during 27 days. Panels b and d, sulphide (HS–) production (dots) in parallel incubations at AOM conditions (10 mM sulphate; 2 mM CH4) over 29 days. Methane production (MP) and AOM rates were calculated from the gradient of monitored methane and sulphide concentrations. Dilution effects from sampling were considered. Shaded areas represent the magnitude of methane production in comparison with AOM.
To determine the carbon isotope effects of AOM at sulphate limitation, cell material was
transferred to artificial seawater medium with reduced sulphate concentration (1 mM) compared to
seawater (28 mM). Incubation medium pH was set to 7.2 via addition of NaOH. Cell suspensions were
transferred into 256 mL culture vials, sealed with butyl rubber stoppers and the headspace was
flushed with methane (purity 5.5, Air Liquide, Düsseldorf, Germany). Subsequently, vials were filled
completely with saturated methane medium to reach a starting concentration of 2 mM methane.
Samples were continuously shaken during the incubations. For geochemical measurements, 5 mL of
the medium were sampled via syringe (every 2−3 days) and the medium was concurrently replaced
with sulphate-‐, methane-‐ and carbonate-‐free medium to avoid gas loss into the headspace. The
dilution effect by medium replacement was taken into account in all calculations and displayed data.
All AOM-‐performing experiments were conducted in duplicates (Fig. 2 and Supplementary Fig. S3).
For methane and DIC measurements, sampled medium was transferred into two gas tight 2.2
mL exetainer® vials (Labco, Lampeter, United Kingdom) filled with zinc chloride solution (50 µL, 50%),
HR
time (d)
AOM = 0.11 mmol L–1 d–1
AOM = 0.30 mmol L–1 d–1
10 15 20 25 3050time (d)
0.000.010.02 MP = 0.0005 mmol L–1 d–1
MP = 0.00008 mmol L–1 d–1
MP = 0.0008 mmol L–1 d–1
MP = 0.00006 mmol L–1 d–1
CH4 (m
M)
10 15 20 25 3050
time (d)10 15 20 25 3050
0.03
time (d)
0.000.010.02
CH4 (m
M)
10 15 20 25 3050
0.03
2.04.06.08.010.0
H S– (m
M)
H S– (m
M)
0.0
2.04.06.08.010.0
0.0
a b
c dAMV
range of CH4 concentrations
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4
and 1 mL of medium was replaced by helium. From this set of samples, methane concentrations
were determined using gas chromatography coupled to a flame ionization detector (GC 14; Shimadzu,
Kyoto, Japan) equipped with a Supel-‐Q Plot column, 30 m × 0.53 mm (Supelco, St. Louis, MO, USA).
The detection limit for methane concentration using this setup was 25 ppm. The elevated initial
methane concentrations might have been underestimated (e.g. Fig. 2a, d) due gas phase loss and/or
high room temperatures above 20 °C during preparation of headspace-‐free incubations. Methane
carbon composition was determined by coupled gas chromatography (G 1530A; Agilent Santa Clara,
CA, USA) to combustion (CuO-‐Ni-‐Pt catalyst; 940 °C) isotope ratio mass spectrometry (Thermo
Finnigan, Bremen, Germany), respectively. Analytical error for carbon (< 0.1‰) was checked against
an external methane standard of known isotopic composition. To determine DIC isotopic
composition of the incubation medium, medium was transferred into butyl rubber sealed glass vials,
gas phase was exchanged with helium and samples were acidified with phosphoric acid. The isotopic
composition of the released CO2 was measured via gas-‐bench coupled to isotope ratio mass
spectrometry (MAT 252, Finnigan, Bremen, Germany) and values were measured against external
standards (Solnhofener Plattenkalk), which was calibrated against NBS19 (IAEA, Vienna, Austria).
To determine the sulphate concentrations of the medium, sulphide was removed (via
precipitation with zinc chloride) and sulphate was measured from 50 times diluted medium using ion
chromatography (761 Compact IC, Ω Metrohm, Filderstadt, Germany). Sulphide concentrations were
determined from ZnCl2 fixed medium by colorimetric determination using the methylene blue
formation reactionS3 in a small assayS4.
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5
Supplementary Figure S2| Biotic (methane-‐free) and abiotic (without AOM culture) controls for the sulphate-‐limited AOM experiments during 27 days. From left to right: Panels a and c, development of sulphate (SO4
2–) and sulphide (HS–) concentrations. Methane (CH4) concentrations remained below 5 µM throughout incubation. Panels b and d, development of δ13C values of dissolved inorganic carbon (DIC) in methane-‐free biotic controls for AOM cultures from Hydrate Ridge (HR) and Amon Mud Volcano (AMV). Panel e, development of CH4, SO4
2– and HS– concentrations in the abiotic control incubation. Error bars represent analytical imprecision of 10% for CH4 concentrations. Panel f, development of δ13C values of DIC and CH4 in the abiotic control.
a b
c d
(mM
)
0.0
0.5
1.0
1.5
2.0
2.5
-60
-58
-56
-24
-22
-20Abiotic control
(mM
)
0.0
0.5
1.0
1.5
2.0
-60
-58
-56
-24
-22
-20
(mM
)
0.0
0.5
1.0
1.5
2.0
-60
-58
-56
-24
-22
-20
e f
time (d)10 15 20 25 3050
time (d)10 15 20 25 3050
time (d)10 15 20 25 3050
time (d)10 15 20 25 3050
time (d)10 15 20 25 3050
time (d)10 15 20 25 3050
AMV, Biotic control
HR, Biotic control
AMV, Biotic control
HR, Biotic control
Abiotic control
!13C
(‰)
!13C
(‰)
!13C
(‰)
DIC
CH4
SO42–
HS–DIC
CH4
DICSO42–
HS–
SO42–
HS–
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6
Supplementary Figure S3 | Experimental data (symbols) and model output (lines) for replicate AOM culture incubations Hydrate Ridge 2 (left column) and Amon Mud Volcano 2 (right column). From top to bottom: Panels a and d, development of measured concentrations of methane (CH4, circles), hydrogen sulphide (HS
–, closed triangles), sulphate (SO4
2–, open triangles), along with a first-‐order model approach (lines); DIC concentrations were derived from the modelled AOM reaction; methane concentrations are plotted with 10% error bars due to analytical imprecision. Panels b and e, development of δ13C values (in ‰) for measured DIC (black dots) and CH4 (red dots), along with modelled values by mass balancing (lines). Panels c and f, ratio of back flux (ƒ–) relative to AOM net reaction (ƒnet) as the main variable to achieve best fit for measured δ13CCH4 and calculated Gibbs free energies for AOM (kJ mol−1).
3. Compilation of global sulphate flux data
Location, diffusive flux values, stable carbon isotopic composition of methane and DIC and
references are given in Supplementary Table S1. Sedimentary diffusive fluxes (Jsed) of dissolved
sulphate and methane into the sulphate-‐methane transition zone (SMTZ) were calculated using a
modification of Fick’s first law of diffusionS5 (Eq. S1):
Equation S1
time (d)
(mM
)
Hydrate Ridge 2
time (d)10 15 20 25 30
0
0.5
1.0
1.5
2.0
5.0
6.0a
50
CH4
HS–
SO42–
DIC DIC
CH4
HS–
SO42–
Amon Mud Volcano 2
0
0.5
1.0
1.5
2.0
5.0
6.0
(mM
)
d
10 15 20 25 3050
time (d)
!40
!20
0
0
50
100
10 15 20 25 30
c
50
!Gr
ƒ – / ƒ
net (%
)
!40
!20
0
0
50
100!G
rf
time (d)10 15 20 25 3050
ƒ – / ƒ
net (%
)
b!20!22!24!26"13
C DIC
time (d)10 15 20 25 3050
!28!62!60!58!56
"13C CH
4
!64
e!20!22!24!26"13
C DIC
time (d)10 15 20 25 3050
!28!62!60!58!56
"13C C
H 4
!64
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7
with Φ the sediment porosity and Dsed the sedimentary diffusion coefficient. The concentration
gradient ∂c/∂x is based on a linear regression of concentration data versus sediment depth directly
above the SMTZ. Dsed is calculated by correcting the seawater diffusion coefficient (Dsw) using
Boudreau’s lawS5 (Eq. S2):
Equation S2
We used a sulphate Dsw value of 5.72*10–6 cm2 s–1 (ref. S6) and estimated Φ to 0.66 when no porosity
value was available. Figure S4 provides additional examples for the prevalence of carbon isotope
equilibration during AOM in sediments from different oceanic provinces.
Supplementary Table S1. Data compilation of sulphate and methane fluxes (J in µmol cm–2 yr–1) into the SMTZ from various oceanic sediments. δ13C values (in ‰ VPDB) of methane and DIC within the SMTZ are reported and the ∆δ13CCH4 values are calculated as the offset in δ13C values of methane in the methanogenic zone (MGZ) and at the SMTZ (For details see main text and Fig. 1). na = not available and Refs. = references.
Site/Core information J SO4
2-‐ J
CH4 δ13C SMTZ
δ13C MGZ CH4
∆δ13CCH4 SMTZ Depth Refs.
Cascadia Margin DIC CH4 (cmbsf) Bullseye Vent 2002 (C-‐1) 3.7 -‐2.7 -‐46 -‐112 -‐80 32 478 S7*
Bullseye Vent 2002 (C-‐2) 4.5 -‐2.9 -‐46 -‐111 -‐73 38 330 S7
Bullseye Vent 2002 (C-‐3) 28.7 -‐15.4 -‐48 -‐73 -‐69 4 35 S7
Bullseye Vent 2002 (C-‐4) 4.8 -‐3.6 -‐45 -‐103 -‐75 29 386 S7
Bullseye Vent2002 (C-‐6) 7.9 -‐4.3 -‐47 -‐109 -‐74 35 250 S7
Bullseye Vent 2002 (C-‐7) 2.9 -‐3.0 -‐43 -‐106 -‐75 31 586 S7
Bullseye Vent 2008 (C-‐12) 22.9 -‐16.4 -‐42 -‐72 -‐62 9 170 S8
Bullseye Vent 2008 (C-‐5) 4.8 -‐3.0 -‐42 -‐101 -‐87 14 420 S8
Bullseye Vent 2008 (C-‐6) 2.9 -‐2.6 -‐40 -‐104 -‐76 28 520 S8
Amnesiac Vent (C-‐19) 13.0 -‐8.9 -‐51 -‐94 -‐78 16 230 S8
Barkley Canion (C-‐23) 18.1 -‐12.8 -‐21 -‐56 -‐43 13 110 S8
IODP 311 (U1329) 1.0 -‐0.5 -‐25 -‐105 -‐64 41 935 S9,S10
IODP 311 (U1327) 1.7 -‐1.2 -‐30 -‐99 -‐63 36 590 S10,S11
IODP 311 (U1325) 6.1 -‐1.5 -‐21 -‐102 -‐71 31 290 S10,S11
IODP 311 (U1326) 6.3 -‐2.2 -‐37 -‐94 -‐72 22 215 S10,S11
Porangahau Ridge, NZ
PC17 21.7 -‐18.9 -‐39 -‐98 -‐79 19 180 S12
PC7 11.5 -‐8.2 -‐21 -‐91 -‐79 12 210 S12
PC4 7.4 -‐5.5 -‐39 -‐108 -‐79 29 440 S12
Peru and Chile margins
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Chilean Margin (C-‐10) 9.8 -‐7.1 -‐28 -‐101 -‐79 22 190 S13
Chilean Margin (C-‐11) 18.6 -‐15.5 -‐49 -‐87 -‐66 22 80 S13
Chilean Margin (C-‐17) 16.8 -‐14.0 -‐53 -‐90 -‐61 28 200 S13
Chilean Margin (C-‐2) 8.8 -‐7.3 -‐23 -‐90 -‐79 11 200 S13
Chilean Margin (C-‐3) 8.5 -‐4.9 -‐21 -‐90 -‐82 8 250 S13
ODP Leg 201 (1227A) 0.5 -‐0.2 -‐25 -‐84 -‐55 28 2,000 S14,S15
ODP Leg 201 (1229A) 0.2 0.0 -‐11 -‐89 -‐50 39 3,500 S14,S15
Gulf of Mexico
KC03-‐05 9.7 -‐9.7 -‐62 -‐107 -‐85 22 450 S16
KC03-‐07 10.5 -‐11.4 -‐56 -‐93 -‐78 15 450 S16
KC03-‐19 5.9 -‐6.2 -‐58 -‐104 -‐72 32 350 S16
MD02-‐2751 13.4 -‐9.2 -‐63 -‐90 -‐73 16 300 S17
GeoB10610 3.7 -‐7.0 -‐25 -‐73 -‐50 22 600 S18
Black Sea
E Black Sea (P824GC) 11.3 -‐4.6 -‐35 -‐97 -‐83 15 160 S19
NW Black Sea (core 214) 6.6 -‐3.2 na -‐96 -‐77 19 160 S20
Mud Volcanoes
(Bonjardim GeoB9051) 28.8 -‐30.6 na -‐64 -‐52 12 60 S21
(CAMV MSM1-‐205) 44.7 -‐8.4 -‐12 -‐53 -‐47 6 140 S21
GC38 NW 51.7 -‐11.3 na -‐60 -‐52 8 75 S22
GC46 S 34.8 -‐16.3 na -‐66 -‐58 8 90 S22
Blake Ridge
Kr-‐140-‐1 TC-‐3 35.4 -‐4.9 na -‐73 -‐68 5 53 S23
ODP Leg 164 (995) 0.9 -‐0.1 -‐36 -‐101 -‐74 27 2,190 S24,S25
ODP Leg 164 (997) 0.8 na -‐31 -‐102 -‐67 35 2,130 S24,S25
Shallow water Skagerrak, Denmark (Site 821GC) 36.1 -‐12.0 na -‐82 -‐76 6 70 S26 Eckernförde Bay (1993 Core) 39.9 -‐10.7 -‐2 -‐71 -‐63 8 30 S27 * Methane δ13C values are firstly reported in this study.
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Supplementary Figure S4 | Sulphate flux as a proxy for sulphate availability at SMTZs, and its relationship with the prevalence of carbon isotope equilibration during AOM in sediments from different oceanic provinces. a, Scheme from exemplary sites under distinct regimes of sulphate fluxes into the SMTZ (Cascadia margin Bullseye Vent 2002 C-‐1 and C-‐3, respectively left and right panels). Within the limits of SMTZs, sulphate availability in the AOM zone (grey area) is dependent on the steepness of sulphate profiles (i.e. concentration gradients) from which diffusive fluxes are derived/calculated. In low flux, deep SMTZs, methane overlaps low concentrations of sulphate. Conversely, high flux, shallow SMTZs higher methane concentrations overlap relatively higher sulphate concentrations. b, Bullseye vent 2002 (C-‐6)S7. c, Core 19 from Keathley Canyon, Gulf of MexicoS16. d, Core 10 from the mid-‐Chilean marginS13. Depth profiles of sulphate and methane concentrations are shown in the left panels, with values for sulphate fluxes into the SMTZ (J SO4
2− in µmol cm−2 yr−1). Stable carbon isotope profiles of methane and DIC are shown in the right panels with corresponding Δδ13CCH4 (for details see Main Text and Supplementary Table S1).
4. Isotope mass balance model for the anaerobic oxidation of methane (AOM)
The simplified isotope mass-‐balance model describes the incremental development of δ13C
of dissolved inorganic carbon (DIC) and methane (CH4) for discrete time steps during the incubation
experiment. The model consists of two parts: an approximation of the experimental concentration
time series of CH4, SO42–, DIC and sulphide (HS–) together with a thermodynamic analysis of AOM,
and the actual isotope mass balance based on this concentration time series. The calculations are
stepwise, so that δ13C values for a given time increment t are calculated from the preceding time
0 5 10 2015 0 3 6 129 15Methane (mM)
100
200
300
400
500
600
700
0
Dep
th (c
m)
50
100
150
200
250
300
350
0
Dep
th (c
m)
c
J SO42- = 5.9 J SO4
2- = 9.8
!"C = 32‰
[CH4]
0 4 8 12
[SO42-]
0 10 20 30
Sedi
men
t dep
th
[CH4]
Methane (mM)0 4 8 12
[SO42-]
Sulphate (mM)0 10 20 30
Low !ux (deep SMTZ) High !ux (shallow SMTZ)
Methane (mM)
Sulphate (mM)
0 2 4 86 10Methane (mM)
3020100Sulphate (mM)
0-120 -90 -60 -30"13C (‰)
CH4
DIC
100
200
300
400
500
600
700
0
Dep
th (c
m)
b
d
J SO42- = 7.9
Methane (mM)
Sulphate (mM) "13C (‰)
a
SMTZ
SMTZSMTZ
3020100 0-120 -90 -60 -30Sulphate (mM) "13C (‰)
3020100 0-120 -90 -60 -30
CH4 !"C = 22‰ CH4
!"C = 35‰ CH4
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10
increment t-‐1. The model was implemented in a spreadsheet that can be handled with an
appropriate computer program (LibO Calc®, MS Excel® or similar). This material is available upon
request with the corresponding authors.
Concentration time series and thermodynamics
To approximate the experimental concentration time series and to create an incremental
temporal domain for the isotope calculations, we used a first-‐order reaction model for CH4, SO42–,
bicarbonate (HCO3–; here equal to DIC) and HS–. The k value of the fit was adjusted to the
experimental SO42– data (Eq. S3), as we considered the SO4
2– data the most reliable.
Equation S3
with c(SO42–) the sulphate concentration (mM), k the first-‐order rate constant (s–1), and Δt the time
increment (s).
According to the AOM net reaction equation where substrates and products are equimolar (Eq. S4)
Equation S4
we obtain CH4, HCO3– and HS– concentration changes Δc for each time increment from the SO4
2– time
series (Eq. S5):
Equation S5
The Gibbs free energy for the net AOM reaction (Eq. S4) was calculated for each time step according
to Eq. S6
Equation S6
with the standard energy of reaction
Equation S7
and the activity of substrates and products (Eq. S8) in seawater (example CH4)
Equation S8
with R = 0.00831441 kJ mol−1 K−1, T = 285.15 K (HR) and 293.15 (AMV), respectively, and γ and ΔG0f
values listed in Supplementary Table S2.
[ ] [ ][ ] [ ]−
−−
⋅⋅
⋅⋅+Δ=Δ 244
30,, ln
SOCHHSHCORTGG AOMrAOMr
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11
Supplementary Table S2. Activity coefficients γ and Gibbs energy of formation ΔG0
f for AOM reactants and products. Data from refs. S28 and S29. Species γ ΔG0
f kJ mol−1 CH4 (aq) 1 –34.39 SO4
2– 0.11 –744.6 HCO3
– 0.55 –586.8 HS– 0.55 12.05 H2O 1 –237.2
Isotope mass balance
The realisation of the isotope mass balance is technically a simplifying term of combined gain
and loss in the two relevant carbon pools, CH4 and HCO3–. The C transfers depend on the relative
proportion of the AOM reaction components, which we define as ƒ+ the forward and ƒ– the catalytic
backward flux (Supplementary Fig. S5). Here, ƒ– is the main variable to achieve the best fit of the
experimental data.
Supplementary Figure S5 | Carbon back flux in AOM illustrated by reaction vectors ƒ+ (forward flux), ƒ– (backward flux) and ƒnet (sum or net reaction) modified from ref. S30. Arrows lengths indicate rates and for convenience are not drawn with exact proportionality.
The observable net reaction ƒnet is the balance of forward and backward flux (Eq. S9) and by definition
set to 100 %.
!"#$ = ! !! ! ! Equation S9
The proportion r of backward and forward reaction is (Eq. S10)
! = " !" !
Equation S10
With the above derivations, we set up the δ13C mass balance for HCO3– (here abbreviated as DIC) and
CH4 (Eq. S11, S12)
CH4 HCO3–
ƒ–
ƒ+
ƒnet
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12
!!"!"#! #$
!%"#! #$
=!!"!"#! #$"!
!%"#! #$"!
"$%"#! #$"!
"%"#! #$
%! !!" &
!!"!"#! #$"!
"!+ " ! ! !!"!!"# #$"!
"!"( )#$
%&
Equation S11
and
( )[ ]−−
+−−
−−
−⋅−−−
⋅−−
⋅=⋅
εδεδ
δδ
1,13
1,13
,1,
1,113
,13
11)( tDICttt
tDICttt
CrCr
cc
cCcC
CH4CH4CH4
CH4CH4CH4 ,,
Equation S12
with δ13C the stable carbon isotope value (‰PDB), c the concentration (mM), and ε the isotope
enrichment of forward (ε+) and backward flux (ε–). By convention, ε is calculated from experimental
isotope fractionation factors to
! = !" !"#""$$$%&' Equation S13
We adopted empirical isotope fractionations (α+) in Hydrate Ridge and Amon Mud Volcano cultures
(ref. S1; Supplementary Table S3) for the forward flux. The α– values that we employ in the mass
balance are intrinsic to the isotope effect of the AOM back flux and represent the sum of the isotope
fractionation of the forward flux and the pure physicochemical isotope effects of the CO2-‐HCO3– and
CO2-‐CH4 isotopic equilibria (refs. S31,32). For the calculation of the isotope signature at each time
point t, we solved Eq. S11 and S12 for δ13CDIC,t and δ13CCH4,t, respectively. Finally, the best fit was
achieved by adjusting ƒ– until δ13CCH4 data in the model and the experiment were congruent with a
deviation of ±0.1‰. We emphasize that the step-‐ or kink-‐like nature of the f– adjustment solely
results from the linear approximation of f–, and does not represent an analytical derivation from the
δ13C time series.
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13
Supplementary Table S3. Parameterisation for isotope mass balance calculations. Starting conditions for concentration time series, isotope values and isotope fractionation factors employed in the isotope mass balance calculations. Values are given for the Hydrate Ridge (HR1, HR2) and Amon Mud Volcano (AMV1, AMV2) experiments. Parameter unit HR1 HR2 AMV1 AMV2 Reference
α+ 1.012 1.012 1.019 1.019 S1 α– 1.094 1.094 1.099 1.099 S31,S32 T °C 12 12 20 20 measured δ13CCH4 ‰ PDB –58.12 –58.02 –57.96 –58.07 measured δ13CDIC ‰ PDB –20.95 –20.53 –21.51 –21.23 measured c(SO4
2–) mM 1.03 1.02 1.02 1.02 measured c(CH4) mM 2 2 2 2 estimated c(HS–) mM 0.15 0.19 0.20 0.22 measured c(HCO3
–) mM 5 5 5 5 estimated kAOM s–1 1.15*10–6 1.15*10–6 1.25*10–6 1.25*10–6 estimated
Sensitivity analysis
We tested the sensitivity of our mass balance model against variations in the initialized CH4
concentrations and the carbon isotopic composition of DIC. First, we constructed a confidence belt
for the underlying CH4 concentration time series by calculating the AOM first order reaction with
minimum and maximum concentrations using all measured values plus their analytical error of 10%
(HR1: 1.5-‐2.2 mM CH4, AMV1: 1.6-‐2.4 mM CH4; Supporting Fig. S6a, c). Subsequently, the back flux
proportion f–/fnet was fitted considering four scenarios: I) minimum CH4 concentration, II) maximum
CH4 concentration, III) CH4 as measured at time zero, and IV) 2mM CH4 as used in the applied model
(Main Text Fig. 2a, d). All four scenarios started with identical f– values and continued with diverging
values during the later stages of the experiments (Supplementary Fig. S6b, d). While the first-‐order
CH4 consumption rate remained similar, the variable residual CH4 concentrations obtained from each
scenario produced different results towards the end of the experiments. In scenarios with CH4
concentrations below the model value of 2 mM, generally lower back flux adjustments were required,
whereas the opposite was necessary for concentrations above 2 mM. Similar results have been
obtained for the replicate experiments HR2 and AMV2. We emphasize that the marked shift from
initial f– values (HR1: 0.23, AMV1: 0.45) to their terminal range (HR1: 0.49–0.71, AMV1: 0.66–0.96) is
the most critical finding, rather than the range of the terminal values. This and the fact that
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14
increasing f– values coincide with sulphate depletion below 0.5 mM strongly support that the
observed carbon isotope time series can only be explained by increasing carbon back flux during
sulphate-‐limited AOM.
Supplementary Figure S6 | Model sensitivity towards initialized methane concentrations in experiments HR1 (a, b) and AMV1 (c, d). Panels a and c: Confidence belt for CH4 concentration time series according to the first-‐order AOM reaction employed in the mass balance model for four scenarios (grey area defined by lower and upper limit of all measured values, red line: cCH4,0=2mM; dashed line: cCH4,0 as measured). Circles represent measured CH4 concentrations with a standard analytical error (± 10 %). Panels b and d: Corresponding best fit model results showing the percentage of back flux (f–) vs. net flux (fnet). The best fit model achieved identical values for f– at the beginning of each experiment, and diverging values in the later course of the experiments. The grey area represents the CH4 confidence belt examined in the above four scenarios.
Second, we tested our isotope mass balance model against changes in δ13CDIC that were
observed in the biotic controls (Fig. S2b, d). Applying an initial variability of ± 2 ‰ in the measured
δ13CDIC on the isotope mass balance, we found that such variability triggers a maximum deviation in
δ13CCH4 of ± 0.7 ‰ at the end of the experiments HR1 and AMV1. This effect could be buffered by an
CH4 (m
M)
Hydrate Ridge 1 Amon Mud Volcano 1
a
time (d)
ƒ– /
ƒ net (%
)
00 5 10 15 20 25 30
00 5 10 15 20 25 30
0
0.5
1
1.5
2
2.5
3
0 5 10 15 20 25 30
0
25
50
75
100
0 5 10 15 20 25 30
0.5
1
1.5
2
2.5
3
25
50
75
100
time (d) time (d)
time (d)
ƒ – / ƒ
net (%
)
c
b d
CH4 (m
M)
© 2014 Macmillan Publishers Limited. All rights reserved.
15
average increase or decrease in f– values of 1%, which is small in comparison to the overall change
from initial to terminal f– values (Supplementary Figure S6b, d). There is no experimental evidence
that these changes may result from the formation of solid carbonates and C-‐uptake into AOM
biomass was presumably low during the 30 days of incubationS33. Hence, we consider the impact of
δ13CDIC changes as of minor importance to our conclusion that increased carbon back flux explains the
observed carbon isotope reversal in δ13CCH4 values during the experiments.
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