Abstract:A series of empirical expressions for predicting gas hydrate stability, its volume fraction out of pore space and gas hydrate mass-density were established in different systems in consideration of gas composition (CH 4 , C 2 H 6 , H 2 S) and salinity (NaCl, seawater), and pore size at temperature between 273.15 and 300 K, based on our gas hydrate thermodynamic model (Sultan et al., 2004b, c). Six of the developed expressions for predicting gas hydrate stability were validated against the available published ex… Show more
“…B) Change in the volume of the GHSZ and in the mass of carbon due to ocean warming. Notation: P 0 seabed pressure; T 0 , seabed temperature; TG, thermal gradient; K th, thermal conductivity; calculated using six different methane hydrate phase boundaries Quinby-Hunt, 1994, 1997;Distribution Coefficient Method or K vsi -Method, Sloan and Koh, 2008;Moridis et al, 2008;Tischenko et al, 2005;Lu and Sultan, 2008) and assuming 3.5 wt% salinity and steady state conditions. B) Holocene sedimentation rate calculated using the water depth vs sediment accumulation relationship from Burwicz et al (2011).…”
Section: Discussionmentioning
confidence: 99%
“…with six different methane hydrate phase boundaries: (1) and (2) Dickens and Quinby-Hunt (1994;, (3) Distribution Coefficient Method or K vsi -Method (Sloan and Koh, 2008), (4) Moridis et al (2008), (5) Tischenko et al (2005) and (6) Lu and Sultan (2008). Water depth was converted to hydrostatic pressure assuming a constant water density of 1046 kg m 3 (Giustiniani et al, 2013).…”
Highlights⹠The amount of carbon stored in hydrate below the Arctic Ocean remains uncertain⹠A function for the fluid flow that gives observed hydrate saturations is proposed⹠Arctic marine gas hydrates likely form by upwards-advection of carbon-rich fluids⹠Equivalent fluid flows of 0.02-0.04 cm yr -1 result in hydrate saturations of 5-10%The quantification of the carbon stored in gas hydrate (GH) bearing marine sediments still remains a challenge. Despite recent efforts to develop approaches to better estimate the GH inventory globally, these estimates are still highly unconstrained due to insufficient field data and poor understanding of the mechanisms fuelling the GH stability zone (GHSZ). Here we use geophysically-derived GH saturations to constraint estimates of model-derived Arctic marine GH inventory at present. We also estimate the potential carbon released from GH dissociation under a seabed warming of 2°C over 100 yr. We estimate an inventory ranging between 0.28-541 Gt of C, which upper bound results in average GH saturations of 0.25%. Our upper bound is mainly controlled by our imposed upwards carbon-rich fluid flow of 0.01 cm yr -1 and it is five times greater than the most recent estimate that only considers in-situ degradation of particulate organic carbon (POC). To obtain the seismically-inferred GH saturations of 5-10% offshore west of Svalbard and in the Beaufort Sea, an upwards advection of carbon-rich fluids equivalent to 0.02 to 0.04 cm yr -1 is required. This mechanism may be the most important source of carbon reaching the GHSZ in Arctic marine sediments. A 2°C seabed temperature increase over 100 yr may reduce the GH inventory by about 88.44% (0.7 Gt C) if POC is the only source, and by about 5.4% (29.7 Gt C) if the main source of carbon is the upwards advection of carbon-rich fluids.
“…B) Change in the volume of the GHSZ and in the mass of carbon due to ocean warming. Notation: P 0 seabed pressure; T 0 , seabed temperature; TG, thermal gradient; K th, thermal conductivity; calculated using six different methane hydrate phase boundaries Quinby-Hunt, 1994, 1997;Distribution Coefficient Method or K vsi -Method, Sloan and Koh, 2008;Moridis et al, 2008;Tischenko et al, 2005;Lu and Sultan, 2008) and assuming 3.5 wt% salinity and steady state conditions. B) Holocene sedimentation rate calculated using the water depth vs sediment accumulation relationship from Burwicz et al (2011).…”
Section: Discussionmentioning
confidence: 99%
“…with six different methane hydrate phase boundaries: (1) and (2) Dickens and Quinby-Hunt (1994;, (3) Distribution Coefficient Method or K vsi -Method (Sloan and Koh, 2008), (4) Moridis et al (2008), (5) Tischenko et al (2005) and (6) Lu and Sultan (2008). Water depth was converted to hydrostatic pressure assuming a constant water density of 1046 kg m 3 (Giustiniani et al, 2013).…”
Highlights⹠The amount of carbon stored in hydrate below the Arctic Ocean remains uncertain⹠A function for the fluid flow that gives observed hydrate saturations is proposed⹠Arctic marine gas hydrates likely form by upwards-advection of carbon-rich fluids⹠Equivalent fluid flows of 0.02-0.04 cm yr -1 result in hydrate saturations of 5-10%The quantification of the carbon stored in gas hydrate (GH) bearing marine sediments still remains a challenge. Despite recent efforts to develop approaches to better estimate the GH inventory globally, these estimates are still highly unconstrained due to insufficient field data and poor understanding of the mechanisms fuelling the GH stability zone (GHSZ). Here we use geophysically-derived GH saturations to constraint estimates of model-derived Arctic marine GH inventory at present. We also estimate the potential carbon released from GH dissociation under a seabed warming of 2°C over 100 yr. We estimate an inventory ranging between 0.28-541 Gt of C, which upper bound results in average GH saturations of 0.25%. Our upper bound is mainly controlled by our imposed upwards carbon-rich fluid flow of 0.01 cm yr -1 and it is five times greater than the most recent estimate that only considers in-situ degradation of particulate organic carbon (POC). To obtain the seismically-inferred GH saturations of 5-10% offshore west of Svalbard and in the Beaufort Sea, an upwards advection of carbon-rich fluids equivalent to 0.02 to 0.04 cm yr -1 is required. This mechanism may be the most important source of carbon reaching the GHSZ in Arctic marine sediments. A 2°C seabed temperature increase over 100 yr may reduce the GH inventory by about 88.44% (0.7 Gt C) if POC is the only source, and by about 5.4% (29.7 Gt C) if the main source of carbon is the upwards advection of carbon-rich fluids.
“…Global estimates of gas hydrate concentrations rely on the prediction of the extent of the GHSZ at specific geological settings [e.g., Klauda and Sandler , ]. The GHSZ extent can be predicted using thermodynamic models [e.g., Bale et al ., ; Dickens and QuinbyâHunt , ; Lu and Sultan , ; Sloan and Koh , ] together with constraints from direct sampling and indirect evidence from both geophysical and geochemical data. Several numerical models have been proposed that emphasize controls on hydrate stability by specific parameters [ Bale et al ., , and references therein; Peszynska et al ., ].…”
The Vestnesa Ridge comprises a >100Â km long sediment drift located between the western continental slope of Svalbard and the Arctic midâocean ridges. It hosts a deep water (>1000Â m) gas hydrate and associated seafloor seepage system. Nearâseafloor headspace gas compositions and its methane carbon isotopic signature along the ridge indicate a predominance of thermogenic gas sources feeding the system. Prediction of the base of the gas hydrate stability zone for theoretical pressure and temperature conditions and measured gas compositions results in an unusual underestimation of the observed bottomâsimulating reflector (BSR) depth. The BSR is up to 60Â m deeper than predicted for pure methane and measured gas compositions with >99% methane. Models for measured gas compositions with >4% higherâorder hydrocarbons result in a better BSR approximation. However, the BSR remains >20Â m deeper than predicted in a region without active seepage. A BSR deeper than predicted is primarily explained by unaccounted spatial variations in the geothermal gradient and by larger amounts of thermogenic gas at the base of the gas hydrate stability zone. Hydrates containing higherâorder hydrocarbons form at greater depths and higher temperatures and contribute with larger amounts of carbons than pure methane hydrates. In thermogenic provinces, this may imply a significant upward revision (up to 50% in the case of Vestnesa Ridge) of the amount of carbon in gas hydrates.
“…Considering that the theory model of formation condition of gas hydrate is complex in calculation, based on the above theory model, the empirical models for different systems consisting of gas composition, pure water/pore water and pore size were established and applied [32] : where units of P and T are respectively kPa and K; parameters a, b, c, d, and e are determined by the certain gas composition (requiring R 2 > 0.98). Comparing the empirical model and experimental data, the difference between them is generally below 5% [32] . It indicates that the empirical model is applicable.…”
Geological factors affecting gas hydrate formation and distribution are different horizontally and vertically in the northern slope of the South China Sea such as the Shenhu area. Whether variation of gas sources is an important resultant factor is worth exploring. In this paper, 14 cases of gas source are summarized on the base of existing data and a semiâquantitative analysis is conducted by modeling to study their effects on gas hydrate formation in the northern South China Sea. Modeling results show that various gas sources will enhance temperature conditions for gas hydrate formation by 0.49°C to 5.44°C, mostly by more than 2°C, with respect to known gas hydrate in the Shenhu area. This indicates that various gas sources greatly change gas hydrate formation conditions, suggesting that they are probably important factors to affect gas hydrate formation and distribution in the northern South China Sea.
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