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gas hydrate - CCOP

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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

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