Microbe-Worm Symbiosis Stabilizes Methane Hydrates in Deep Marine Environments

• Main Authors: Tianyi Hua (1751884), Maisha T. Ahmad (11741447), Tenzin Choezin (11741450), Ryan L. Hartman (1610311)
• Format: Other Non-Article Part of Journal/Newspaper
• Language: unknown
• Published: 1753
• Subjects: Physiology; Biotechnology; Evolutionary Biology; Ecology; Sociology; Marine Biology; Inorganic Chemistry; Infectious Diseases; Computational Biology; Astronomical and Space Sciences not elsewhere classified; Chemical Sciences not elsewhere classified; ocean temperature rises; feather duster worms; energy balance equations; could otherwise overtake; retreat could avoid; endothermic methanogenic metabolism; natural ecosystem comprised; deep marine environments; stabilizes methane hydrates; retreat deeper; exothermic metabolism; methane hydrates; hydrates via; present work; model suggest; microbial bioreactions; massive release; living organisms; hydrate deposits; greenhouse gas; fragile tolerance; dynamic stability; coupled mass; bioreaction kinetics; Methane hydrate
• Online Access: https://doi.org/10.1021/acs.energyfuels.1c02673.s001

Our planet has a natural ecosystem comprised of living organisms and methane hydrates in deep marine environments. This ecosystem was constructed in the present work to examine the influence that subtle temperature fluctuations could have on the dynamic stability of the hydrate deposits. The coupled mass and energy balance equations that describe the microbial bioreactions, their consumption by feather duster worms, and methane hydrate dissociation confirm that the bioreaction kinetics is dominated by endothermic methanogenic metabolism that stabilizes methane hydrates with a fragile tolerance to 0.001 K temperature increases. The feather duster worms also stabilize the hydrates via their selective consumption of methanotrophs that could otherwise overtake the system by their exothermic metabolism. Critical ocean temperature limits exist, beyond which hydrate dissociations would cause underwater eruptions of methane into the sea. Historical ocean temperature records and gas hydrate inventory estimates combined with our model suggest that hydrate deposits as deep as 560 m below sea level could already be at risk, whereas the methane hydrate stability zone will retreat deeper as the ocean temperature rises. Slowing its retreat could avoid the massive release of greenhouse gas.