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Modeling of Gas Hydrate Formation in Marine Sediments<br />
Klaus Wallmann<br />
IFM-GEOMAR, Wischhofstrasse 1-3, 24148 Kiel, Germany<br />
ABSTRACT: A transport-reaction model is presented and applied to simulate the<br />
formation of <strong>gas</strong> <strong>hydrate</strong>s in marine sediments. The modeling confirms that<br />
microbial methane production within the <strong>hydrate</strong> stability zone is usually too slow<br />
to produce significant amounts of <strong>hydrate</strong>. Economically valuable methane <strong>hydrate</strong><br />
deposits with high concentrations of <strong>hydrate</strong> are, however, formed by upward<br />
methane migration.<br />
Keywords: marine <strong>gas</strong> <strong>hydrate</strong>s, methane, fluid flow, numerical modeling, pore<br />
water, sediments<br />
INTRODUCTION<br />
Gas <strong>hydrate</strong>s are widespread in marine sediments accumulating at the slope and rise of<br />
continental margins. They occur as finely disseminated solids but also as massive layers often<br />
associated with sandy sediment horizons. Only the massive layers are of economic<br />
importance since they could be exploited at reasonable costs (Makogon et al., 2005). The<br />
accumulation of <strong>hydrate</strong>s in discrete and massive layers clearly shows that methane is<br />
transported to these layers either as free <strong>gas</strong> or in dissolved form via fluid flow. Methane may<br />
either be formed within the <strong>hydrate</strong> stability zone (HSZ) by microbial decay of organic matter<br />
at low temperatures or may be produced in deeper sedimentary strata at elevated temperatures.<br />
Recent modeling studies clearly showed that microbial methane production within the HSZ<br />
proceeds very slowly so that the resulting methane concentrations are too small to produce<br />
massive <strong>hydrate</strong> deposits (Wallmann et al., 2006). Strong chloride enrichments in pore fluids<br />
from Hydrate Ridge (Haeckel et al., 2004; Torres et al., 2004) and independent constraints on<br />
fluid flow rates at Blake Ridge (Wallmann et al., 2006) clearly show that massive <strong>hydrate</strong><br />
layers found at these sites have been formed by the ascent of <strong>gas</strong> bubbles originated from<br />
deeper sediment layers located below the HSZ. In this paper we present the modeling<br />
approach used for the simulation of <strong>hydrate</strong> formation in marine sediments and additional<br />
modeling results confirming that methane ascent is the most important pathway for the<br />
formation of economically important <strong>hydrate</strong> deposits.<br />
MODELING APPROACH<br />
A numerical transport-reaction model was developed and applied to simulate the degradation<br />
of particulate organic carbon (POC), the microbial methane production and the precipitation<br />
of methane <strong>hydrate</strong>s in anoxic marine sediments. The model calculates the concentration -<br />
depth profiles of 2 solid species (particulate organic carbon, <strong>gas</strong> <strong>hydrate</strong>) and 3 dissolved<br />
species (sulfate, methane, dissolved inorganic carbon). Major processes considered in the<br />
model are POC degradation via sulfate reduction, methanogenesis and the anaerobic oxidation<br />
of methane (AOM).<br />
New Energy Resources in the <strong>CCOP</strong> Region - Gas Hydrates and Coalbed Methane 11