2022 Annual Meeting
(413h) Evaluating CO2 Hydrate Stability in Oceanic Sediments for CO2 Sequestration
Authors
Oceanic CO2 sequestration using gas hydrates is a potential storage approach that is receiving increased interest and research for areas without conventional geologic storage. Gas hydrates are crystalline compounds that are formed when small CO2 molecules are trapped within water molecules at high pressure and low-temperature conditions. One unit of gas hydrate can store up to 184 units of gas at STP. Converting CO2 captured from industry emissions into liquid CO2 and injecting it into the deep ocean sediments to be stored as gas hydrates offers an additional option to existing storage methods. However, the key concern to alleviate is the stability of the CO2 hydrates underneath the deep oceanic sediments or sea bed.
In this work, stability of the CO2 hydrates in oceanic sediments has been evaluated on a lab-scale for an extended period [14-30 days] using a high-pressure reactor system mimicking the thermodynamic conditions [10 MPa, 4 oC] found at the oceanic depth of 1 Km. The high-pressure reactor was equipped with two cameras mounted at the top and front of it. First, the CO2 hydrates were formed across the sediments [Silica sand] using CO2 gas, and then these hydrates were submerged in the water column for the period of 14-30 days. The experimental results indicate that the CO2 hydrates hold an adequate level of stability and a good amount of hydrates were visible across the sediments throughout the stability test. Intentional heating and depressurization of the system after the stability test also indicated that the hydrates inside the sediments tend to be more stable than the hydrates at the surface of the sand bed.