Campeche Knolls Campeche Salt Dome Province | |
---|---|
Oceanic basin | |
Coordinates: 20°22′00″N93°47′00″W / 20.366667°N 93.783333°W | |
Location | |
Part of | Campeche Bank |
Offshore water bodies | |
Area | |
• Total | 22,653.6 square nautical miles (30,000.0 sq mi; 77,700 km2) [2] |
Dimensions | |
• Length | 260.7 nautical miles (300.0 mi; 482.8 km) [2] |
• Width | 86.9 nautical miles (100.0 mi; 160.9 km) [2] |
• Depth | 672.5 fathoms (4,035 ft; 1,229.9 m) ~ 1,725 fathoms (10,350 ft; 3,155 m) [3] |
The Campeche Knolls are diapirs rising from a salt deposit in the southern Gulf of Mexico, separated from the Mississippi-Texas-Louisiana salt province by the Sigsbee Abyssal Plain. [4] Located southeast of the Sigsbee Knolls, the Campeche Knolls are bounded by Campeche Bank to the East, the Bay of Campeche to the South, and the salt-free abyssal plain called the Veracruz Tongue to the West. Salt deposition is inferred to have occurred in the Late Jurassic, during the rifting stage of the gulf, equivalent to the Louann Salt of the Texas-Louisiana slope. [5] Multibeam echosounder images collected during R/V Sonne cruise SO174 show the northern Campeche Knolls as distinct, elongated hills that average 3 by 6 mi (4.8 by 9.7 km) in size, with reliefs of 1,475 to 2,625 ft (450 to 800 m) and slopes of 10 to 20 percent. [4]
The Campeche Knolls are covered with a thick column of sediments above the salt unit, with sediment thickness reaching 3–6 mi (4.8–9.7 km) depending upon water depth and distance from the southern coast. The thick sediments provided prolific petroleum source rocks with the most productive one being of latest Jurassic and Cretaceous age. [5] Hydrocarbon generation makes Campeche Knolls a highly ranked and prolific petroleum region, with studies showing that salt activity supports leakage of gas and oil. [5]
The potential for gas hydrate accumulations in the Campeche Knolls was demonstrated as early as 1970, with the retrieval of gassy cores from Site 88 drilled during Leg 10 of the Deep Sea Drilling Program (DSDP). DSDP Site 88 was drilled to demonstrate that the topographic high seen on profiler records was a salt diapir. During the course of drilling, a significant increase in the gas content of recovered cores to a depth of 108 mbsf (354 fbsf) occurred. [6] Of the five cores recovered, four had high levels of H2S and other natural gases. When these cores were brought on board the ship, irregular degassing characteristics were observed, with the cores emitting very large quantities of gas, estimated to be ten times the volume of the core, that required special measures (i.e. drilling of vent holes in the core liner) to prevent complete disruption of core sediments. [7] Degassing the cores also took an abnormally long time of over two hours. [7] These perplexing results have since led the shipboard researchers to believe that gas hydrates were present in the core and would explain the high volumes of gas locked in the small quantity of water filling the sediment pore spaces and the long degassing time. [7]
During the R/V Sonne SO174 research cruise in 2004, remote sensing results guided researchers to the discovery of oil, gas, and asphalt seepage on the top of one knoll in the northern tip of the Campeche Knolls province. [5] This knoll was named Chapapote, the Aztec word for “tar,” and is located at 21° 54’ N by 93° 26’ W in approximately 1.8 mi (3, 000 m) water depth. Extensive surface deposits of solidified asphalt are present at Chapapote, with one subcircular-shaped flow measuring at least 49 ft (15 m) across. [4] A diverse biological community is also present on the Chapapote, with a range of organisms, including tubeworms, bacterial mats, and chemosynthetic mussels all calling the area home. [4] A sample grab conducted on the cruise recovered sediment with thin layers of gas hydrate. Molecular and isotopic compositions of the gas hydrate indicated that the gas was moderately mature and thermogenic in nature. [4]
In 2006, the METEOR Cruise No. 67 (MC67/2b) returned to Chapapote. Hydrates were recovered at one gravity coring station, with Core 10618-1 containing a large piece of pure, white gas hydrate embedded in asphalt. The recovery of this core was accompanied by a strong rising of gas bubbles to the sea surface. It is assumed that hydrate formed internally after deposition of the asphalt. [8] Of the three samples collected from upper first meter of the core, two were composed of Structure I hydrate. The third was a mixture of both Structure I and Structure II. [9] Hydrocarbons from the Chapapote are dominantly thermogenic in origin as evidenced by the stable carbon isotopes of hydrate forming hydrocarbons. [4]
The Chapapote asphalt volcano is located in the Campeche Knolls.It was there that the deepest known recovery of surficial gas hydrate occurred at a water depth of 1.8 mi (3,000 m). The gas hydrate was embedded in an asphalt matrix. Analyses of the hydrate showed both Structure-I and Structure-II gas hydrate present in the recovered sample. [8] The only known recovery of gas hydrate in the southern Gulf of Mexico also occurred in the Campeche Knolls. [10]
Methane clathrate (CH4·5.75H2O) or (8CH4·46H2O), also called methane hydrate, hydromethane, methane ice, fire ice, natural gas hydrate, or gas hydrate, is a solid clathrate compound (more specifically, a clathrate hydrate) in which a large amount of methane is trapped within a crystal structure of water, forming a solid similar to ice. Originally thought to occur only in the outer regions of the Solar System, where temperatures are low and water ice is common, significant deposits of methane clathrate have been found under sediments on the ocean floors of the Earth. Methane hydrate is formed when hydrogen-bonded water and methane gas come into contact at high pressures and low temperatures in oceans.
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The Deep Sea Drilling Project (DSDP) was an ocean drilling project operated from 1968 to 1983. The program was a success, as evidenced by the data and publications that have resulted from it. The data are now hosted by Texas A&M University, although the program was coordinated by the Scripps Institution of Oceanography at the University of California, San Diego. DSDP provided crucial data to support the seafloor spreading hypothesis and helped to prove the theory of plate tectonics. DSDP was the first of three international scientific ocean drilling programs that have operated over more than 40 years. It was followed by the Ocean Drilling Program (ODP) in 1985, the Integrated Ocean Drilling Program in 2004 and the present International Ocean Discovery Program in 2013.
The Integrated Ocean Drilling Program (IODP) was an international marine research program, running from 2003 to 2013. The program used heavy drilling equipment mounted aboard ships to monitor and sample sub-seafloor environments. With this research, the IODP documented environmental change, Earth processes and effects, the biosphere, solid earth cycles, and geodynamics.
A diapir is a type of igneous intrusion in which a more mobile and ductily deformable material is forced into brittle overlying rocks. Depending on the tectonic environment, diapirs can range from idealized mushroom-shaped Rayleigh–Taylor-instability-type structures in regions with low tectonic stress such as in the Gulf of Mexico to narrow dikes of material that move along tectonically induced fractures in surrounding rock.
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Salt tectonics, or halokinesis, or halotectonics, is concerned with the geometries and processes associated with the presence of significant thicknesses of evaporites containing rock salt within a stratigraphic sequence of rocks. This is due both to the low density of salt, which does not increase with burial, and its low strength.
The Orca Basin is a mid-slope, silled, mini-basin in the northern Gulf of Mexico some 300 km southwest of the Mississippi River mouth on the Louisiana continental slope. It is unique amongst the mini-basins in this area, in containing a large brine pool of anoxic salt brine. The pool is approximately 123 km2 (47 sq mi) in area and up to 220 m (720 ft) deep under 2,400 m (7,900 ft) depth of Gulf water and is derived from dissolution of underlying Jurassic age Louann Salt. With a volume of 13.3 km3 (3.2 cu mi) the pool results from the dissolution of about 3.62 billion tonnes of the Louann Salt bed into seawater. The basin owes its shape to ongoing salt tectonics and is surrounded by salt diapirs.
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Bruce Peter Luyendyk is an American geophysicist and oceanographer, currently professor emeritus of marine geophysics at the University of California, Santa Barbara. His work spans marine geology of the major ocean basins, the tectonics of southern California, marine hydrocarbon seeps, and the tectonics and paleoclimate of Antarctica. His research includes tectonic rotations of the California Transverse Ranges, participation in the discovery of deep-sea hydrothermal vents, quantitative studies of marine hydrocarbon seeps, and geologic exploration of the Ford Ranges in Marie Byrd Land, Antarctica.
NOASS Okeanos Explorer Gulf of Mexico 2017 Expedition was the first of three expeditions on the NOAAS Okeanos Explorer intended to increase the understanding of the deep-sea environment in the Gulf of Mexico. Gulf of Mexico 2017 was a 23-day telepresence-enabled expedition focused on acquiring data on priority exploration areas identified by ocean management and scientific communities. The goal of the expedition was to use remotely operated vehicle (ROV) dives and seafloor mapping operations to increase the understanding of the deep-sea ecosystems in these areas to support management decisions. Many of the areas had no sonar data, these areas were top priority for high-resolution bathymetry collection. The expedition established a baseline of information in the region to catalyze further exploration, research, and management activities. The expedition lasted from 29 November 2017 to 21 December 2017.
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