Ian R. MacDonald

Gas hydrate that breaches the sea floor on the continental slope of the Gulf of Mexico

We report observations that concern formation and dissociation of gas hydrate near the sea floor at depths of ∼540 m in the northern Gulf of Mexico. In August 1992, three lobes of gas hydrate were partly exposed beneath a thin layer of sediment. By May 1993, the most prominent lobe had evidently broken free and floated away, leaving a patch of disturbed sediment and exposed hydrate. The underside of the gas hydrate was about 0.2 °C warmer than ambient sea water and had trapped a large volume of oil and free gas. An in situ monitoring device, deployed on a nearby bed of mussels, recorded sustained releases of gas during a 44 day monitoring period. Gas venting coincided with a temporary rise in water temperature of 1 °C, which is consistent with thermally induced dissociation of hydrate composed mainly of methane and water. We conclude that the effects of accumulating buoyant force and fluctuating water temperature cause shallow gas hydrate alternately to check and release gas venting.

Global Patterns and Predictions of Seafloor Biomass Using Random Forests

A comprehensive seafloor biomass and abundance database has been constructed from 24 oceanographic institutions worldwide within the Census of Marine Life (CoML) field projects. The machine-learning algorithm, Random Forests, was employed to model and predict seafloor standing stocks from surface primary production, water-column integrated and export particulate organic matter (POM), seafloor relief, and bottom water properties. The predictive models explain 63% to 88% of stock variance among the major size groups. Individual and composite maps of predicted global seafloor biomass and abundance are generated for bacteria, meiofauna, macrofauna, and megafauna (invertebrates and fishes). Patterns of benthic standing stocks were positive functions of surface primary production and delivery of the particulate organic carbon (POC) flux to the seafloor. At a regional scale, the census maps illustrate that integrated biomass is highest at the poles, on continental margins associated with coastal upwelling and with broad zones associated with equatorial divergence. Lowest values are consistently encountered on the central abyssal plains of major ocean basins The shift of biomass dominance groups with depth is shown to be affected by the decrease in average body size rather than abundance, presumably due to decrease in quantity and quality of food supply. This biomass census and associated maps are vital components of mechanistic deep-sea food web models and global carbon cycling, and as such provide fundamental information that can be incorporated into evidence-based management.

Gulf of Mexico hydrocarbon seep communities

Sediment and water samples were collected by submersible in September 1986 at 16 locations on the carbonate cap overlying a conical diapir, which was formed by the upward migration of oil and gas through a subsurface fault on the continental slope off Louisiana, USA (27°47′N; 91°30.4′W). The biological community at the site was photographed quantitatively with still and video cameras. Rigorous spatial sampling indices were maintained so that variation in chemical parameters and in the abundance of photographed organisms could be estimated within the bounds of the study site. Concentrations of extractable organic material (EOM) ranged from 0.24 to 119.26‰ in the sediment samples, while methane concentrations in the water samples were from 0.037 to 66.474 μM. The visible biological community was predominantly composed of the chemosynthetic tube worms (Vestimentifera) Lamellibrachia sp. and Escarpia sp., and an undescribed, methane-oxidizing mussel (Mytilidae: Bathymodiolus-like), as well as diverse non-chemosynthetic organisms. The ranked abundance of tube worms was significantly correlated (p<0.05) with the concentration of EOM in the sediment samples, while the abundance of mussels was significantly correlated (p<0.05) with the concentration of methane in the water samples. Tube worms and mussels both occurred in dense clusters; however, the clusters of mussels had a more restricted distribution within the study site than did clusters of tube worms. Both organisms were most abundant in the vicinity of the subsurface fault.

Natural oil slicks in the Gulf of Mexico visible from space

Natural oil seepage in the Gulf of Mexico causes persistent surface slicks that are visible from space in predictable locations. A photograph of the sun glint pattern offshore from Louisiana taken from the space shuttle Atlantis on May 5, 1989, shows at least 124 slicks in an area of about 15,000 km2; a thematic mapper (TM) image collected by the Landsat orbiter on July 31, 1991, shows at least 66 slicks in a cloud-free area of 8200 km2 that overlaps the area of the photograph. Samples and descriptions made from a surface ship, from aircraft, and from a submarine confirmed the presence of crude oil in floating slicks. The imagery data show surface slicks near eight locations where chemosynthetic communities dependent upon seeping hydrocarbons are known to occur on the seafloor. Additionally, a large surface slick above the location of an active mud volcano was evident in the TM image. In one location the combined set of observations confirmed the presence of a flourishing chemosynthetic community, active seafloor oil and gas seepage, crude oil on the sea surface, and slick features that were visible in both images. We derived an analytical expression for the formation of floating slicks based on a parameterization of seafloor flow rate, downstream movement on the surface, half-life of floating oil, and threshold thickness for detection. Applying this equation to the lengths of observed slicks suggested that the slicks in the Atlantis photograph and in the TM image represent seepage rates of 2.2–30 m3 1000 km−2 d−1 and 1.4–18 m3 1000 km−2 d−1, respectively. Generalizing to an annual rate suggests that total natural seepage in this region is of the order of at least 20,000 m3 yr−1 (120,000 barrels yr−1).

Gas hydrate and chemosynthetic biota in mounded bathymetry at mid-slope hydrocarbon seeps: Northern Gulf of Mexico

Abstract We present nested surveys of four hydrocarbon seeps that contain abundant, shallow deposits of gas hydrate. The two sites mapped in greatest detail were at ∼550 m depths, the others at ∼1050 and ∼1900 m, respectively. Formation and dissociation of shallow deposits generated variability in seafloor geology and ecology that appeared to decrease at greater depths. The deposits typically formed mounds in a size range from a few meters to hundreds of meters in diameter and centimeters to tens of meters in height. These high-flux regions are also colonized by chemosynthetic species. At the two shallower seeps, data comprised laser line-scan mosaics, analog side-scan sonar mosaics, dense bathymetric grids, quantitative video records, 2–12 kHz chirp sub-bottom profiles and surface reflectance, 3D seismic data. Additional ground-truth data were obtained from piston cores and numerous animal and sediment collections. Datasets were assembled as GIS layers and geographically co-registered. In the shallower sites, gas hydrate deposits and extensive chemosynthetic communities were concentrated adjacent to lithified fault scarps where surface reflectance data from 3D seismic records showed the lowest amplitudes. Sub-bottom profiles revealed complex and abrupt transitions from regions in which surface strata appear as distinct, closely spaced layers to areas in which the strata were blanked by continuous, moderate-intensity returns. Within the blanked zone and adjacent to the normally stratified strata, the seafloor had a distinctively undulating profile caused by irregular hydrate deposits. Hydrate occurred as layers, which were ∼10 cm to >1 m thick, and generally buried under tens of centimeters of sediment, but occasionally exposed as outcrops on slopes. Sediments over hydrate deposits were covered with bacterial mats. Larger mounds were colonized by continuous aggregations of vestimentiferans tube worms. Outcropping hydrate deposits were colonized by the polychaete Hesiocaeca methanicola and by the seep mussel Bathymodiolus childressi. Streams of oil and gas escape from vents in the seafloor or from patches of exposed gas hydrate. The tube worms were most abundant in regions that reflected less seismic energy than the surrounding seafloor. At the deeper sites, preliminary survey results found similar topography, and biological colonies that included bacterial mats and mussels, but no active gas venting and very few colonies of tube worms. Negative surface reflectance amplitudes were also absent on these mounds. This suggests that development of chemosynthetic communities changes substantially with increasing depth.

Dynamics of the gas flux from shallow gas hydrate deposits: interaction between oily hydrate bubbles and the oceanic environment

Decomposition of methane hydrates on the continental margins is a potentially significant source of atmospheric methane, but the input depends upon the poorly understood fate of the hydrocarbon bubbles rising from the sea floor. During a field trip to the Gulf of Mexico, three different seepages were imaged and analyzed. Three different imaging techniques were tried (side, front, and back illumination), of which back illumination produced the best results. The images were analyzed and the size-dependent bubble distribution, mass flux, and rise speeds determined. The total observed gas flux was 62.3×10−3 mol s−1, primarily methane, of which a single vent produced seven times the next largest vent. Of this major vent, 50% of the bubble mass was contained in the largest bubbles, r>5500 μm. The vertical velocities demonstrated that these bubbles were heavily contaminated with oil, which was also corroborated by bubble shape and oscillation observations.

Evidence of structure H hydrate, Gulf of Mexico continental slope

Abstract A research submarine was used to sample an amber-colored gas hydrate exposed on the sea-floor at 540 m water depth in the Gulf of Mexico continental slope, offshore Louisiana. The hydrate composition is novel for a natural occurrence because i -C 5 comprises 41.1% of the total C 1 –C 5 hydrocarbon distribution. The relative abundance of i -C 5 is consistent with an hexagonal (H) lattice structure that is capable of enclosing larger hydrocarbon molecules than either structure I or II hydrates. Structure H hydrate, which has not been identified previously in nature, coexists with structure II hydrate on the Gulf slope.

Microbial diversity in sediments associated with surface-breaching gas hydrate mounds in the Gulf of Mexico

Abstract A molecular phylogenetic approach was used to characterize the composition of microbial communities from two gas hydrate sedimentary systems in the Gulf of Mexico. Nucleic acids, extracted from sediments directly overlying surface-breaching gas hydrate mounds collected from a research submersible (water depth 550-575 m), were amplified with nine different 16S rDNA gene primer sets. The polymerase chain reaction primers targeted microorganisms at the domain-specific (Bacteria and Archaea) and group-specific (sulfate-reducing bacteria (SRB) and putative anaerobic methane-oxidizing (ANME) archaea) level. Amplicons were obtained with five of the nine primer sets including two of the six SRB Groups (SRB Group 5 and Group 6) and used to generate five different clone libraries. Analysis of 126 clones from the Archaea library revealed that the sediments associated with naturally occurring gas hydrate harbored a low diversity. Sequence analysis indicated the majority of archaeal clones were most closely related to Methanosarcinales, Methanomicrobiales and distinct phylogenetic lineages within the ANME groups. The most frequently recovered phylotypes in the ANME library were related to either ANME-2 or Methanomicrobiales. In contrast to the two archaeal libraries, bacterial diversity was higher with the majority of the 126 bacterial clones most closely related to uncultured clones dominated by the delta- and epsilon-Proteobacteria. Interestingly, while 82% of the clones in the SRB Group 5 library were affiliated with delta-Proteobacteria, the vast majority (83%) of clones in the SRB Group 6 library was affiliated with the Firmicutes. This is the first phylogenetic-based description of microbial communities extant in methane-rich hydrate-associated sediments from a hydrocarbon seep region in the Gulf of Mexico.

Bacterial methane oxidation in sea-floor gas hydrate: Significance to life in extreme environments

Samples of thermogenic hydrocarbon gases, from vents and gas hydrate mounds within a sea-floor chemosynthetic community on the Gulf of Mexico continental slope at about 540 m depth, were collected by research submersible. The study area is characterized by low water temperature (mean = 7 C), high pressure (about 5,400 kPa), and abundant structure II gas hydrate. Bacterial oxidation of hydrate-bound methane (CH{sub 4}) is indicated by three isotopic properties of gas hydrate samples. Relative to the vent gas from which the gas hydrate formed, (1) methane-bound methane is enriched in {sup 13}C by as much as 3.8% PDB (Peedee belemnite), (2) hydrate-bound methane is enriched in deuterium (D) by as much as 37% SMOW (standard mean ocean water), and (3) hydrate-bound carbon dioxide (CO{sub 2}) is depleted in {sup 13}C by as much as 22.4% PDB. Hydrate-associated authigenic carbonate rock is also depleted in {sup 13}C. Bacterial oxidation of methane is a driving force in chemosynthetic communities, and in the concomitant precipitation of authigenic carbonate rock that modifies sea-floor geology. Bacterial oxidation of hydrate-bound methane expands the potential boundaries of life in extreme environments.

Organic geochemistry of sediments from chemosynthetic communities, Gulf of Mexico slope

We used a research submersible to obtain 33 sediment samples from chemosynthetic communities at 541–650 m water depths in the Green Canyon (GC) area of the Gulf of Mexico slope. Sediment samples from beneath an isolated mat of H2S-oxidizing bacteria at GC 234 contain oil (mean = 5650 ppm) and C1–C5 hydrocarbons (mean = 12,979 ppm) that are altered by bacterial oxidation. Control cores away from the mat contain lower concentrations of oil (mean = 2966 ppm) and C1–C5 hydrocarbons (mean = 83.6 ppm). Bacterial oxidation of hydrocarbons depletes O2 in sediments and triggers bacterial sulfate reduction to produce the H2S required by the mats. Sediment samples from GC 185 (Bush Hill) contain high concentrations of oil (mean = 24,775 ppm) and C1–C5 hydrocarbons (mean = 11,037 ppm) that are altered by bacterial oxidation. Tube worm communities requiring H2S occur at GC 185 where the sea floor has been greatly modified since the Pleistocene by accumulation of oil, thermogenic gas hydrates, and authigenic carbonate rock. Venting to the water column is suppressed by this sea-floor modification, enhancing bacterial activity in sediments. Sediments from an area with vesicomyid clams (GC 272) contain lower concentrations of oil altered by bacterial oxidation (mean = 1716 ppm) but C1–C5 concentrations are high (mean = 28,766 ppm). In contrast to other sampling areas, a sediment associated with the methanotrophic Seep Mytilid I (GC 233) is characterized by low concentration of oil (82 ppm) but biogenic methane (C1) is present (8829 ppm).