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The National Methane Hydrates R&D Program
DOE/NETL Methane Hydrate Projects

Gulf of Mexico Gas Hydrates Sea-floor Observatory Project Last Reviewed 9/20/2012

DE-FE26-06NT42877, DE-FC26-02NT41628, and DE-FC26-00NT40920

Goal
The goal of this project is to conduct activities leading to the development, implementation and operation of a remote, multi-sensor seafloor observatory focused on behavior of the marine hydrocarbon system within the gas hydrate stability zone of the deepwater Gulf of Mexico and analysis of data resultant from that observatory over time. Attaining this goal will lead to an enhanced understanding of the role the hydrocarbon system plays in the environment surrounding the site. Investigations include physical, chemical, and microbiological studies. Models developed from these studies are designed to provide a better understanding of gas hydrates and associated free gas as (1) a geo-hazard to conventional deep oil and gas activities; (2) a source of hydrocarbon gases venting to the water column and, eventually, the atmosphere, with global climate implications; and (3) a future potential source of energy.

Photo - Extending from the wall of the southwest crater complex on the mound at MC 118, is the largest (~6x2x1.5m) outcrop of marine gas hydrate ever documented in the Gulf of Mexico.
Extending from the wall of the southwest crater complex on the mound at MC 118, is the largest (~6x2x1.5 m) outcrop of marine gas hydrate ever documented in the Gulf of Mexico.

Performers - active

  • University of Mississippi Center for Marine Resources and Environmental Technology (CMRET) – overall project management, spatial models of gas hydrate occurrences, development and construction of sea-floor probe sensor deployment and test execution system,.
  • University of South Carolina – processing and interpretation of the TGS-NOPEC industry seismic data and integration with existing Surface-Source/Deep Receiver (SSDR) high resolution seismic data to develop overall baseline geologic characterization at the MC118 SFO(Sea-Floor Observatory).
  • University of Texas, Bureau of Economic Geology, Exploration Geophysics Laboratory – characterization of sea-floor geology using converted shear-waves from 4-component sea-floor sensor data
  • Florida State University – geochemical investigations at MC118, pore fluid time series, and gas hydrate stability analyses
  • Mississippi State University – utilization of microbial techniques to extract carbon from stored hydrocarbon gases
  • University of California, Santa Barbara – scoping study to determine validity of Spatio-Temporal Measurement of Seep Emissions by Multibeam Sonar at MC118
  • University of Georgia, Athens – development of Automated Biological/Chemical Monitoring System (ABCMS) to be used for offshore oceanic carbon dynamic studies
  • Science Applications International Cooperation (SAIC) – modification of current version of SAIC hydrate simulator to model carbonate/hydrate mound at MC 118
  • Specialty Devices, Inc. – design, build and fit to gravity corer weight with attached USBL a “sound-speed probe”

Background
The Gulf of Mexico-Hydrate Research Consortium (GOM-HRC), formed to coordinate efforts of hydrates researchers and to promote effective, efficient communication among them, is in its eleventh year of developing a sea-floor station to monitor hydrates in situ. Consortium management includes facilitating research activities, sensor testing, and deployments; cooperation among participants; and reporting via planning regular consortium meetings and research cruises as well as interacting with sponsoring agencies. Established at and administered by the University of Mississippi’s Center for Marine Resources and Environmental Technology (CMRET), the consortium has, as its primary objective, the design and emplacement of a remote monitoring station on the sea floor in the northern Gulf of Mexico. The Monitoring Station/Sea-Floor Observatory (MS/SFO) is a multi-sensor station that will eventually provide more-or-less continuous monitoring of the near-seabed hydrocarbon system within the hydrate stability zone (HSZ) of the northern Gulf of Mexico.

Photo of Observatory components deployed at the foot of the wall of hydrate: Peepers, hydrate collector, mini-osmosampler (left to right)
Observatory components deployed at the foot of the wall of hydrate: Peepers, hydrate collector, mini-osmosampler (left to right)

The site of the observatory, Mississippi Canyon 118 (MC 118), is about 100 miles south of Pascagoula, MS, and was chosen by consensus of the consortium and its funding agencies based on favorable hydrate conditions at the site. The site is dominated by a fault-derived canyon in the northwest and a carbonate mound approximately 1km in diameter to the south. The mound is composed of three crater complexes, as seen in the multibeam image below.

Multibeam image of Mississippi Canyon Block 118
Multibeam image of Mississippi Canyon Block 118

The centerpiece of the SFO will be a series of vertical and horizontal arrays of sensors. One vertical geophysical component is complete and has been tested successfully. It is moored to the sea floor, extends 200 meters into the water column, includes hydrophones to record water-borne acoustic energy (and measure sound speed in the lower water column), thermistors to measure water temperature, tilt meters to sense currents, and compasses to indicate their directions. Another vertical array will consist of hydrophones and 3-component accelerometers to be installed in a borehole. Horizontal water-bottom hydrophone arrays will be laid on the soft sediments of the sea-floor by means of a sea-floor sled designed to lay cable. This sled will also be used as a seismic source of compressional and shear waves. Novel processing techniques for vertical and horizontal array data continue to be developed by consortium participants.

Gas hydrate sea-floor observatory - Mississippi Canyon Block 118

Gas hydrate Sea-Floor Observatory - Mississippi Canyon Block 118

Impacts
The SFO is expected to have a profound impact on our understanding of how natural gas hydrate deposits in the GOM undergo change over time and the repercussions of such changes. Quantification of the volume of natural gas released into the water column from hydrate deposits located on or near the sea-floor as seasonal current and temperature changes occur is one very important finding. Data gathered at the SFO will enhance ongoing efforts to model how hydrates form and dissociate, and will play an important role in the development of methodologies for carrying out commercial natural gas recovery and improving our ability to model climate change. In addition, these observed changes are expected to enhance our understanding of how hydrates affect seafloor stability, a factor critical in the placement and operation of subsea equipment, pipelines, and platforms.

Accomplishments

2012 Accomplishments:

  • Heat flow data were collected from 15 targeted sites in the vicinity of the MC118 observatory.
  • Researchers used the THROBS model to approximate the base of the hydrate stability zone at MC118 using geochemical data from seafloor arrays and heat flow data.
  • Completed logging and lithostratigraphic analyses of jumbo piston cores collected in January 2011.

2011 Accomplishments:

  • Researchers using ocean bottom seismometers supplied by Woods Hole (USGS) successfully collected 4-C seismic data at the SFO. The data were processed by Woods Hole and sent to the University of Texas BEG for interpretation.
  • During the first six months of 2011, researchers collected and partially analyzed Jumbo piston cores which contained various forms of hydrates. This success validated the capability to integrate multiple datasets to predict hydrate in the shallow subsurface with greater accuracy than any known single method could provide. A preliminary hydrate 3-gas model is approaching completion.
  • During a January 2011 cruise, Consortium researchers collected five giant pistons cores from selected sites in the vicinity of the MC118 observatory. A section of one of the cores was selected as a good candidate for further examination based on readings from an infrared camera. This section was found to contain hydrates in the form of massive chunks, blades, nodules, and disseminated grains. The selected core was taken from an area which appeared as an anomaly on a previous resistivity survey and is the first confirmation of subsurface gas hydrate at the site. The finding supports prior geophysical interpretations that suggest that gas delivery to the seafloor, and the distribution of subsurface gas hydrate, are primarily controlled by faults. The cores were transported to a Naval Research Laboratory facility for storage and future analysis.
  • The baseline subsurface characterization of the observatory site was completed. An improved image of the subsurface structure beneath the carbonate-hydrate mound at MC 118 is emerging as a result of high- resolution seismic data, geochemical analyses, and data collected from AUV surveys.
  • New constraints on hydrate formation have been established; multibeam technology has been used effectively to measure both volume and frequency of bubble plumes at vents; and a preliminary hydrate 3-gas reservoir simulation model has been completed.

2010 Accomplishments:

  • All horizontal line arrays tested out during pressure testing in Southwestern Research Institute’s large high-pressure testing facility and are ready for deployment at MC118.
  • Test array deployment operations were carried out on an April cruise to MC118 and to Pensacola Bay (suitable sea state).
  • The Data Recovery System—including the integrated data power unit, pop-up buoy, and battery system—for the observatory was deployed successfully at MC118 in April, following adjustments and updates to the communications system.
  • The array pod was successfully deployed 12m from the IDP on a June cruise.
  • Chemical surveying (via mass spec and water samples) conducted in the wake of the Deepwater Horizon spill approximately 10 miles from the observatory showed increased levels of methane at two depths where detectable levels had not been seen in the past. The evidence that chemical changes are occurring in the water column at MC118 is compelling.
  • The GOM Hydrate Research Consortium Meeting was held in Oxford, Mississippi, October 26–27, 2010. Consortium members gave presentations outlining the status of their research projects and discussed the direction of research efforts going forward.
  • The baseline subsurface characterization of the observatory site was completed.

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