Model Uncertainties Here, we discuss the impacts of hydrate concentration, heat flow and climate model uncertainties to our results. Hydrate saturation in the pore space is one of the least certain parameters in our models. For our default model we used a hydrate saturation of the pore space of 5%, which lies between the 6-13%, estimated for the same area from P and S wave velocities in water depths of ~1285-1500 m [Chabert et al., 2011; Westbrook et al., 2008] and less than 5%, estimated in water depths of 480-866 m [Chabert et al., 2011]. Thatcher et al. [2013] showed that for our intrinsic permeability value of 10-13 m2, the time for methane to reach the seabed is independent of the hydrate saturation for values between 5-30% (their Figure 6b). Figure S2a supports the results of Thatcher et al. [2013], but shows that for a hydrate concentration of 2.5% there is a delay of ~50 yr, due to the limited amount of methane from dissociated hydrate to reach the irreducible gas saturation. The maximum rate of seabed methane outflow and the time period over which it is emitted increases with increasing hydrate saturation. With the 20% model there is still significant methane in the system by 2300 yr (Figure S2a). For hydrate saturations of the pore space within 2.5-20%, the maximum rate of seabed methane outflow is between 29-120 mol yr-1 m-2. Importantly, because the period of gas emission increases with increasing hydrate concentration, the magnitude of total gas emission from the area increases, because gas emission is active simultaneously from a greater range of depths and, therefore, from a larger area. In our modeling approach, we decided to impose a constant heat flow instead of a constant geothermal gradient, because the gradient changes with the phase (hydrate, water or gas) occupying the pore space. For a given thermal conductivity, our heat flows were estimated by an iterative process of varying them until our present-day seabed distribution of gas and hydrate (for a 100% methane hydrate) matched current seismic data that image BSR depth in water depths of more than 580 m and the depth of the upper limit of gas-related reflectors in shallower waters. We were more confident about the range of possible thermal conductivities in our study area than about heat flow values, based on the type of sediments, published measurements (Table S2) and recent measurements on the top few meters of sediment in the plume area [1.8-2.1 W m-1K-1, T. Feseker, personal communication], and hence we iterated over the heat flow. If the real thermal conductivity of the sediment is over/underestimated, the heat flow will be over/underestimated by the same relative amount, and so, the temperature profile with depth will remain the same as that which gives a present-day seabed distribution of gas and hydrate consistent with the seismic observations. In our models, uncertainties in heat flow arising from uncertainties in thermal conductivity (within a range of ±30%) do not significantly affect the time for methane to reach the seabed (Figure S2b). However, they do influence the maximum rate of methane outflow, ranging from 46-74 mol yr-1 m-2, and the time for methane from dissociation at the base of the GHSZ to contribute to the methane outflow from dissociation in the upper part, which produces the second significant increase in methane outflow (Figure S2b). The model (or structural) uncertainty was captured by using two different climate models, HadGEM2 and CCSM4, and the scenario-related uncertainty was examined by using the two most extreme scenarios, RCPs 8.5 and 2.6, which represent high and low greenhouse emissions, respectively, to cover the full range of possible future scenarios. The temperatures predicted by these global climate models were offset to make the temperature at 2005 yr the same as the mean temperature for the period 1975-2005 given by CTD measurements in our study area (supporting information Temperature Series Construction). By this means, the bias in the temperatures given by the global climate models was normalised to our study location. The parametric uncertainty of climate models, which is an active area of research in its own right, is beyond the scope of this work. A detailed discussion on climate model uncertainty is given by Hawkins and Sutton, [2009]. Figure S2: Rate of flow of methane from the seabed at 420 m water depth (mwd), using HadGEM2 climate model and climate-forcing scenario RCP 8.5. (a) Results for hydrate saturations (HS) of 2.5, 5,10, and 20% of pore space. All other parameters are identical to those for the default model (supporting information, Table S3). (b) Results for thermal conductivity (TC) of 0.98 W m-1K-1 and (HF) heat flow of 54 mW m-2, TC of 1.4 W m-1K-1 and HF of 54 mW m-2, and TC of 1.82 W m-1K-1 and HF of 100 mW m-2. All other parameters are identical to those for the default model. Table S2: Thermal gradient (TH), thermal conductivity (TC) and heat flow (HF) values west of Svalbard. Water Depth [m] >2200 >900 850 840 820 813 800 700 688 600-350 560 ~400 ~250 Thermal Gradient [°C km-1] 115 85-122 70 113 73 119 108 97 53-61 44 Thermal Conductivity [W m-1K-1] 1.2 1.0-1.2 1.2 1.16 1.09 1.16 1.4 1.4 1.6 1.4 1.14 Heat Flow [mW m-2] 102.5 85-122 102.5 131 80 138 88 85 102.5 77 110 Reference Observations Vanneste et al., [2005] Crane et al., [1991] Vanneste et al., [2005] Crane et al., [1991] Eldholm et al., [1999] Crane et al., [1991] This study This study Crane et al., [1991] This study Crane et al., [1991] Sarkar et al., [2012] Rajan et al., [2012] BSR-derived TG TG, TC, and HF data in the top ~5 m BSR-derived TG TG, TC, and HF data in the top ~5 m TG and TC data in the top ~5 m TG, TC, and HF data in the top ~5 m TC and HF constrained by data TC and HF constrained by data TG, TC, and HF data in the top ~5 m TC and HF constrained by data TG, TC, and HF data in the top ~5 m Inferred TG from BSR at other water depths Inferred TG from BSR at other water depths References Chabert, A., T. 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