Geology ReportsSearch

Geology topics

William F. Waite

Publications and source records attributed to William F. Waite.

60 records · Page 4Linked to original sources

Thermal properties of methane gas hydrates

Gas hydrates are crystalline solids in which molecules of a “guest” species occupy and stabilize cages formed by water molecules. Similar to ice in appearance (fig. 1), gas hydrates are stable at high pressures and temperatures above freezing (0°C). Methane is the most common naturally occurring hydrate guest species. Methane hydrates, also called simply “gas hydrates,” are extremely concentrated stores of methane and are found in shallow permafrost and continental margin sediments worldwide. Brought to sea-level conditions, methane hydrate breaks down and releases up to 160 times its own volume in methane gas. The methane stored in gas hydrates is of interest and concern to policy makers as a potential alternative energy resource and as a potent greenhouse gas that could be released from sediments to the atmosphere and ocean during global warming. In continental margin settings, methane release from gas hydrates also is a potential geohazard and could cause submarine landslides that endanger offshore infrastructure. Gas hydrate stability is sensitive to temperature changes. To understand methane release from gas hydrate, the U.S. Geological Survey (USGS) conducted a laboratory investigation of pure methane hydrate thermal properties at conditions relevant to accumulations of naturally occurring methane hydrate. Prior to this work, thermal properties for gas hydrates generally were measured on analog systems such as ice and non-methane hydrates or at temperatures below freezing; these conditions limit direct comparisons to methane hydrates in marine and permafrost sediment. Three thermal properties, defined succinctly by Briaud and Chaouch (1997), are estimated from the experiments described here: - Thermal conductivity , λ: if λ is high, heat travels easily through the material. - Thermal diffusivity , κ: if κ is high, it takes little time for the temperature to rise in the material. - Specific heat , c p : if c p is high, it takes a great deal of heat to raise the temperature of the material.

Fact Sheet

Physical properties of pressurized sediment from hydrate ridge

As part of an ongoing laboratory study, preliminary acoustic, triaxial strength, and electrical resistivity results are presented from a test performed on a clayey silt sediment sample recovered from Site 1249 at the summit of southern Hydrate Ridge during Ocean Drilling Program Leg 204. The test specimen was stored and transported in two different methane-charged pressure vessels until it was tested using the Gas Hydrate and Sediment Test Laboratory Instrument (GHASTLI). Although gas hydrate may have existed in the core section immediately after recovery, little (if any) hydrate was present in the specimen during testing. We therefore present background physical property results for sediment that may have hosted gas hydrate in situ. Because we consolidated the test specimen in increments beyond its in situ stress state, we are able to present properties representative of similar but deeper subbottom sediment. The increased consolidation stress also helped to mitigate some, but not all, types of disturbance caused by the recovery process. P-wave velocities from 1.54 to 1.74 km/s varied linearly with consolidation stress, σ′c, up to 970 kPa (equivalent to ~160 meters below seafloor). Electrical resistivity was periodically measured by a Wenner array and varied between 1.0 and 2.8 Ωm. These values reflect both the pore water salinity and soft, fine-grained texture of the sediment. Shear behavior is consistent with the induced normally consolidated behavior of clayey silt.

Report

Strength and acoustic properties of Ottawa sand containing laboratory-formed methane gas hydrate

Although gas hydrate occurs in a wide variety of sediment types and is present and even pervasive at some locations on continental margins, little is known about how it forms naturally. Physical properties of the resultant gas hydrate-sediment mixtures, data needed for input into models that predict location and quantity of in situ hydrate are also lacking. Not only do properties of the host materials influence the type and quantity of hydrate formed and whether a particular deposit may be an economic resource or a geohazard, the properties of the natural sediment are also subsequently changed by the formation of gas hydrate in the pore space. The magnitude of the change is primarily related to the amount and the weighted inter-particle distribution of the hydrate deposits in relation to the actual sediment grains. Our goal is to understand the interaction between natural sediments and gas hydrate formation in order to quantify physical properties that are useful to predictive models.

Book chapter

Introduction to physical properties and elasticity models

Estimating the in situ methane hydrate volume from seismic surveys requires knowledge of the rock physics relations between wave speeds and elastic moduli in hydrate/sediment mixtures. The elastic moduli of hydrate/sediment mixtures depend on the elastic properties of the individual sedimentary particles and the manner in which they are arranged. In this chapter, we present some rock physics data currently available from literature. The unreferenced values in Table I were not measured directly, but were derived from other values in Tables I and II using standard relationships between elastic properties for homogeneous, isotropic material. These derivations allow us to extend the list of physical property estimates, but at the expense of introducing uncertainties due to combining property values measured under different physical conditions. This is most apparent in the case of structure II (sII) hydrate for which very few physical properties have been measured under identical conditions.

Book chapter