Showing posts with label Methane Seeps. Show all posts
Showing posts with label Methane Seeps. Show all posts

Wednesday, 20 October 2021

Investigating the drivers of methane release from cold seeps on the Southern Hydrate Ridge off the coast of Oregon.

Cold seeps release methane along most coastal margins, either as gas dissolved in water or as bubbles which rise through the water column. Bubbles of methane released from cold seeps have been observed rising hundreds of meters through the water column in the Guaymas Basin in the Gulf of California, on the continental rise off the coast of the Carolinas, along the Cascadia Margin off the coast of British Colombia and the northwestern US, in the Okinawa Trough in the East China Sea, in the Black Sea, and in the Gulf of Mexico, as well as at an experimental station in Monterey Bay. When emitted at depths of less than a hundred metres, methane bubbles typically reach the surface and release their gas into the atmosphere, while bubbles released at greater depths the methane in them is lost into the water column as they rise. However, in areas where stable gas hydrates exist at deeper depths, then the bubbles may have a hydrate coating, which slows dissolution of their gas content, allowing bubbles from greater depths to reach the surface. 

This gas is thought to be of minor significance compared to other sources of carbon entering the atmosphere, but the amount gas produced, and how this varies both geographically and over time, has been the subject of very little investigation. The amount of gas released at different sites is known to vary considerably, which is thought to be related to factors such as the subsurface structure and the source of the methane. External factors are also thought to affect the amount of methane being released, such as variations in hydrostatic pressure caused by the action of tides, swell, or storms, changes in sea temperature linked to seasons or longer term changes, seismic tremors, and even to isostatic rebound.

Hydrate Ridge forms part of the Cascadia Subduction Zone, an anticlinal ridge on the accretionary wedge with a north-south orientation. This ridge has two distinct areas of cold seeps, known as the Northern and Southern Hydrate Ridges, both of which have extremely large methane hydrate deposits close to the sediment surface, which lead to persistent gas emissions in the form of bubble plumes, as well as extensive chemosynthetic ecosystems and authigenic carbonates. Seismic profiling of the Southern Hydrate Ridge has found a reflective surface, thought to be the base of the gas hydrate zone, at 125 m beneath the sediment surface. This hydrate zone overlies a structure called Seismic Horizon A, along which methane-rich fluids appear to migrate from the underlying accretionary wedge. Bubble plumes are extremely visible here, and have not been shown to fluctuate with tidal cycles, as is the case on the Northern Hydrate Ridge. Instead, the rate of bubbling appears to follow a cycle unrelated to the tides. It has been suggested that this might be caused by the formation of gas hydrate seals close to the surface, which remain in place until the amount of gas accumulated in the sediment beneath them overcomes their resistance, then reform when gas emissions tail off sufficiently, a cycle which can take several years to complete. More recent surveys have established that while bubbling is not constant on the Southern Hydrate Ridge, it does appear to occur consitently at the same sites on the ridge, and can vary on an hourly timescale. This unexpected behaviour has led to a need for a more organised long-term monitoring of this system in order to understand it.

The systematic monitoring of activity has been carried out at several cold seeps, including a study on Clayoquot Slope, off the coast of Canada on the northern Cascadia Subduction Zone which lasted over a year, although the equipment used in that study was only able detect gas emissions when bottom currents were flowing in certain directions, hampering understanding of the system.

In a paper published in the journal Geochemistry, Geophysics, Geosystems on 21 September 2021, Yann Marcon of the Center for Marine Environmental Sciences and Department of Geosciences at the University of Bremen, Deborah Kelley of the School of Oceanography at the University of Washington, Blair Thornton of the Centre for In Situ and Remote Intelligent Sensing at the University of Southampton, and the Institute of Industrial Science at the University of Tokyo, and Gerhard Bohrmann, also of the Center for Marine Environmental Sciences and Department of Geosciences at the University of Bremen, present the results of a project that carried out systematic monitoring of the Southern Hydrate Ridge between July and November 2018.

Marcon et al. monitored gas emissions on the Southern Hydrate Ridge with the Southern Hydrate Ridge Rotating Sonar, which consists of a multibeam echosounder mounted on a rotator, with a rotating range of 360°. In addition they used a single-beam scanning-sonar connected to the Ocean Observatories Initiative's Regional Cabled Array to provide a finer detail monitoring gas releases at Einstein’s Grotto, one of the methane vents on the Southern Hydrate Ridge, and photo cameras also connected to the Regional Cabled Array to provide visual ground-truthing information about the dynamics and strength of bubble release, at Einstein’s Grotto and the Summit-A vent area. 

 
Top left: Location of Southern Hydrate Ridge. Top right: Map of the primary infrastructure of the Ocean Observatories Initiative's Regional Cabled Array observatory. Bottom: Overview map of the Southern Hydrate Ridge summit with the location of the Southern Hydrate Ridge Regional Cabled Array fibre optic cables, junction boxes and monitoring instruments. Shaded areas show the location of the main known vents. Marcon et al. (2021).

The bathymetry (depth of water) of the area was established in 2008 by the Autonomous Underwater Vehicle Sentry, operating from the Research Vessel Thomas G. Thompson, during preparation for the laying of the Ocean Observatories Initiative's Regional Cabled Array. A 3D photomosaic of the area was developed from imagery gathered by the University of Tokyo's Autonomous Underwater Vehicle AE2000f during the Schmidt Ocean Institute's FK180731 #Adaptive Robotics expedition.

A conductivity, temperature, and pressure (CTP) probe equipped with a dissolved oxygen optode sensor was used to monitor the conductivity, temperature, pressure, and dissolved oxygen concentration of the bottom water at one minute intervals. High-frequency tidal seafloor pressure was recorded with a tsunami pressure sensor. Current velocities were monitored with an upward-looking acoustic Doppler current profiler. Seismic data was collected by three ocean-bottom seismometers connected to the Regional Cabled Array. Wave height data was obtained from the National Data Buoy Center of the National Oceanographic and Atmospheric Administration.

Seafloor pressure at the Southern Hydrate Ridge was found to vary considerably with the tide, and was sensitive to the neep/spring tide cycle, with pressure varying by 1.4 dbar during neap tides and up to 3.8 dbar during spring tides. The seafloor temperature varied between 3.8°C and 4.5°C over the course of the study (June-November 2018) and between 3.7°C and 4.7°C over the longer period June 2018-June 2020, showing no long-term warming or cooling trend. Seafloor salinity varied between 34.26 to 34.37 psu over the period June-November 2018, while dissolved oxygen varied between 0.24 and 0.30 ml/L.

The Southern Hydrate Ridge Rotating Sonar carried out scans every two hours during the four month period of the experiment (with some gaps due to technical problems), producing a total of 888 readings. Of these, 886 (99.8%) detected gas bubbles, suggesting that bubbling was more-or-less constant. However, the amount of bubbling varied continuously, with peaks and troughs on a twice daily basis. These peaks and troughs appear to become larger at the spring tides and weaker at the neap tides, although the short duration of the experiment combined with the gaps in the data make it difficult to be completely confident about this.

Bubbling appears to be possible at any recorded pressure on the Southern Hydrate Ridge, although it was more pronounced when the pressure was low or falling. Two thirds of all peaks in activity occurred at times when the pressure was below average. The majority (65-70%) of the remaining third of peaks happened when the tide was decreasing, or changing (18-20%), with only a small proportion (15%) occurring while the tide was rising. However, there were some anomalies with this, most notably a large bubble release in July 2018m which occurred during a rising tide when the water pressure was above average.

 
Temporal variations of the Southern Hydrate Ridge Rotating Sonar backscatter magnitude and bottom pressure between 6 and 22 July 2018 (top plots) and between 19 October and 8 November 2018 (bottom plots). The backscatter magnitude non-linearly reflects the strength of the gas bubble emissions. The bottom pressure plot shows the local mixed tidal regime with diurnal and semi-diurnal constituents, as well as the fortnightly neap/spring tidal cycles. Bubble release is commonly stronger during ebb tide, and possibly also during spring tidal phases. However, some ebullition events do not correlate with the tide and may be triggered by local accumulation of pressurized free gas in the subsurface; the prominent peak observed on 18 July 2018 corresponded to the reactivation of the Summit-A vent after a very short venting interruption of about 4 hours; it did not affect the other vents at the Southern Hydrate Ridge summit and happened during flood tide within a neap tidal phase, hinting at shallow, local changes in the sediments. Marcon et al. (2021).

Eight different centres of bubbling were identified on the Southern Hydrate Ridge, with an average of four active at any given time. Five main clusters of activity were identified; each of these being 10-30 m across, and capable of producing more than one stream of bubbles at a time. These were named Smokey Tavern, Einstein's Grotto, Summit-A, Summit-B, and Summit-C. Bubbling at all of these sites was frequent, but not continuous, with sites remaining dormant for days at a time and all sites being active at the same time being a rare occurrence. As well as these main sites of activity around the summit of the Southern Hydrate Ridge, Marcon et al. detected at least six smaller venting sites, further away from the summit and much less active, which they named Smokey Tavern West, Summit-D, Far NE, Far S, Summit South, and Summit SW. Unlike the main sites, these sites were only sporadically active, and would often remain dormant for months between bouts of venting.

 
(a) Location of flare base points recorded with the Southern Hydrate Ridge Rotating Sonar between 8 July and 8 November 2018; the base points are grouped into clusters marking the location of the different Southern Hydrate Ridge vent sites. (b) Location of the main and periphery vents overlain on the photomosaic; the main vent sites are all located on areas covered with microbial mats. (c) Close-up view of the Southern Hydrate Ridge Rotating Sonar location and the Summit-A vent, with the 3D photomosaic in the background; a depression on the seafloor from Ocean Drilling Program drill site 1949 (ODP Leg 204) can be seen in the top-left corner as well as in the bathymetric data. (d) Close-up view of the 3D photomosaic at the Smokey Tavern vent showing the distribution of the microbial mats and the domed, collapsed and hummocky areas. Marcon et al. (2021).

The seafloor around the main vents is highly uneven, and covered by white microbial mats. These areas have numerous up-domed mounds, which extend laterally by as much as 35 m, with hummocky, jagged-edged depressions eaten into them, which are probably caused by the more-or-less constant venting of gas from these areas. The venting of gas does appear to be strongly tied to these areas, with venting restricted to them at all sites except Smokey Tavern, where it occurs across the entire microbial mat-covered dome structure. In the peripheral venting area this kink appears to be broken, with dark sediments and white areas of microbial matting visible, but venting not connected to these.

The sites closest to directly underneath the Southern Hydrate Ridge Rotating Sonar (Summit A and Summit B) appeared to be the most active, with sites moving away from this area being progressively less active. This might indicate that the sonar was better act detecting gas emissions directly beneath it and less good at detecting them further away. Alternatively, it might be a reflection the fact that the sonar was placed directly over the highest point of the Southern Hydrate Ridge, so that the most active points were those in the shallowest water, with sites becoming progressively less active as the water grows deeper.

None of the vents was active all the time, although venting over the wider Southern Hydrate Ridge area was continuous. During the period 6-22 July 2018, The Summit A vent was active 75% of the time, Einstein's Grotto was active 69% of the time, Smokey Tavern was active 65% of the time, Summit B and Summit C were active 54% of the time, Summit D 22% of the time, Far NE 9%, Far S 2%, and Smokey Tavern West was active 1% of the time, while Summit South and Summit SW were completely inactive. During the period 19 October-8 November 2018, the Smokey Tavern vent was active 44% of the time, Summit B 30% of the time, Summit C 70%, Summit D 23%, and Smokey Tavern West was active 6% of the time. A sudden decrease in activity at one site was usually accompanied by an equally sudden increase at another. For example, a pause in venting at Summit A on 10 July 2018 was marked by a sudden increase at Summit C. On 12 July activity at Summit C fell off again, and activity resumed at Summit A and Summit B. During the period 19 October-8 November 2018, Summit B was only active when Summit C was inactive, and vice versa. These synchronous changes in activity were frequent enough that they are unlikely to be coincident. Their timing also appears to be linked to the daily tide cycles. 

Southern Hydrate Ridge Rotating Sonar magnitude data from 19 October to 8 November 2018 for individual plume clusters. Einstein's Grotto and Summit-A are not shown because of the restricted 245° scanning sector of the Southern Hydrate Ridge Rotating Sonar after 10 October 2018. Far NE, Far S, Summit South, and Summit SW are not shown because they were inactive over this period. The vertical axis is logarithmic to facilitate visualisation of low magnitude variations. Absolute magnitude values cannot be compared between the clusters due to a distance bias and are not shown. Marcon et al. (2021).

A closer examination three vents at Einstein's Grotto over a 24 hour period found that, while they were all bubbling continuously throughout the day, the amount of outflow from them varied considerably over the day, with the bubbles undergoing sudden peaks in activity, followed by slower tailing off, several times per day. Furthermore, these peaks in activity always occured when the tide was high or waning.

Cameras directed at the Summit A and Einstein's Grotto vents were able to confirm that the events detected by sonar were in fact bubble releases. The one directed at Einstein's Grotto further revealed that the depression from which the bubbles were escaping was growing slightly wider with each bubble-release event, probably due to the loss of gas hydrates within the sediment, and that during major bubble releases this was accompanied by slumping of the walls of the depression and the collapse of overhanging sections. In some cases, hydrates were exposed by sediment loss, and then rapidly lost. Currents on the seafloor also appeared to contribute to the rate of erosion, by slowly breaking up blocks of sediment. The video films also revealed that events recorded as coming from a single vent could in fact come from different locations within the vent at different times, and that sometimes the location of bubble releases shifted in response to sediment movements. On occasions bubbles were seen emerging from as many as four different locations within a vent.

It was only possible to measure the velocity of bubble streams when they were visible to a camera and immediately adjacent to a measuring scale, but those that could be measured rose at speeds of between 18 and 34 cm per second, with an average speed of 25 cm per second.

The camera directed at the Einstein's Grotto vent detected a significant gas blowout between 0.46 and 1.16 am on 23 July 2018, with a sudden release of a significant volume of gas, along with ejected sediment, which led to a change in the seafloor topography. The event happened about midway through a rising tide, with gas release being week, but active, both before and after the event. 

 
A pressure outburst was documented by the CAMDSB103 camera on 23 July 2018. The camera images show sediment resuspension shortly (0–30 min) after the outburst. Images taken after visibility improved show significant seabed changes including the presence of a large well-lithified sediment block into the collapsed area subsequent to the blow out. Scanning-sonar scans recorded before and after the event show that the seabed morphology at the location of the outburst changed over an area of at least 3 m². The hummocky area east of the sonar is part of the Einstein's Grotto vent. The range of the sonar scans is 20 m. The laser pointers on the camera images are 10 cm apart. In the difference plot, blue and red colours show negative and positive differences respectively. Marcon et al. (2021).

Turbulence in the upper part of the water column was relatively high throughout the study, with currents having an average velocity of 50 cm per second. The depth of this layer varied with season and time of day, between about 300 and about 400 m. Below this the water was much calmer, with velocities below 15 m per second, although here too there were daily and seasonal variations. Currents on the seafloor generally run from the northwest. Upwelling was also a significant component of bottom currents, with upwelling currents of up to 5 cm per second rising for about 300 m (i.e. to a depth of 470 m), where they generally became undetectable, although some reached as high as 400-350 m below the surface, by which time they had lost much of their initial velocity. These upwelling flows were intermittent, generally appearing when the prevailing northwest current was either weak or reversed, and appeared to be linked to episodes of bubbling, although this could be an indicator that the northwest current was deflecting bubbles away from the sonar beam.

Contrary to expectations, no connection was found between bubble outbursts and seismic events. A number of such events were measured during the study period, none of which were linked to conspicuous changes in bubble activity.

Wave height was found to be strongly seasonal in the study area, with the monthly average wave height between October and April exceeding 3 m and individual waves reaching close to 10 m, whereas between May and September the monthly average remained below 2 m, and the highest recorded waves little over 3 m. No correlation was found between wave height and bubble activity.

Macron et al.'s study shows that the Southern Hydrate Ridge has a number of vents (where 'vent' is defined as 'a distinct area of the seafloor where gas ebullition recurs') and that each vent has a number of bubble outlets, with vents capable of producing bubbles from several bubble outlets at once, often at different rates of activity.

Five main vents, and six peripheral vents were detected, a significant increase on the number found by previous, ship-based surveys, although it is possible that others exist and were missed by the study. Macron et al. note that bubble events have been recorded at two other sites on the Southern Hydrate Ridge (named Central and Pinnacle), that were outside the scope of their survey.

The discovery that there are multiple bubble-producing sites within each vent, which may be active at different times and at different rates at the same time, is new. This potentially presents additional challenges for ship-based surveys, as snapshots of bubbling from different locations might not be recognised as the same vent, particularly if the origin of bubbles is further complicated by varying currents.

The main vents all appear to be up-domed and hummocky areas covered by microbial mats. Such areas have previously been linked to the presence of gas hydrates at shallow depths within the sediment, something which was confirmed by Macron et al.'s study. The hummocky topography seen at these locations appears to be directly linked to bubble-venting, which causes changes the seafloor morphology quite rapidly at vent sites.

The loss of gas hydrate deposits is likely to be largely due to direct disolution of gas into non-methane saturated water, without the formation of bubbles. The vent zone of the Southern Hydrate Ridge lies within the gas hydrate stability zone (approximately between 500 and 900 m below sea level), so the excess loss of gas hydrates through bubble formation is unlikely in shallow sediments here. The depressions and hummocky surfaces observed at the site could as easily be formed by hydrate dissolution as by bubble formation, particularly at a site being regularly scoured by currents of non-methane saturated water. Based upon this, Macron et al. suggest that the bubbles observed venting on the Southern Hydrate Ridge are not being formed by the disassociation of gas hydrates, but rather are bubbles of trapped within the sedimenr that are released into the water.

Previous studies of the Southern Hydrate Ridge have captured only snapshots of bubbling activity there, suggesting that bubbling was either 'off' or 'on' at different times. This is consistent with the idea that methane was being delivered to the system from a reservoir more deeply buried gas at Horizon A, which was escaping intermittently through a system of cracks in the overlying rock. Macron et al.'s study contradicts this model, showing that bubbling is more-or-less constant on the Southern Hydrate Ridge, although different parts of the system are active at different times, and that this activity is strongly linked to bottom pressure, and thereby to the tides. However, Macron et al. cannot rule out the possibility that the vents are connected in some way, or that there may be some form of interaction between them.

Tidal modulation of methane vent systems on accretionary wedges has previously been suggested, but until now there has not been sufficient evidence to support this. Notably, video evidence from the Northern Hydrate Ridge appeared to show a correlation, but was not sufficient on its own to prove the link. Therefore the long-term sonar study carried out by Macron et al. at the Southern Hydrate Ridge clearly establishes a relationship between tides and bubbling for the first time. A relationship has also been suggested between tides and bubbling at cold seep sites, which appears to have been supported by observations off the coast of Canada.

Macron et al. suggest that this link is related to the effect that pressure has upon pore spaces within sediments, which are pushed shut at higher pressures (i.e. when the tide is high) and pulled open at lower pressures, allowing gas bubbles trapped within the sediment (where the water is methane-saturated) to escape. At spring tides, the pressure loading on the seafloor would be higher than at neep tides, causing the dilation of pore-spaces deeper into the sediments, which would in turn result in more bubbles being released, something line with Macron et al.'s observations. 

However, this does not appear to be the only factor at play; Macron et al.'s theory can explain why vents tail of activity after outbursts, when they might be expected to have reduced numbers of bubbles within their sediments, but not what causes the reactivation of individual vents after periods of inactivity. Furthermore, a number of significant bubble outbursts were recorded at times which appeared to show no connection to tidal cycles. Another problem with this hypothesis is the absence of any connection with seismic activity. Earthquakes would be expected to cause changes in pore spaces, which should have resulted in bubble releases, but despite several Earthquakes being recorded during the study period, none of them was linked to any change in bubble-activity.

One possibility previously suggested is that gas hydrates accumulating in pore spaces trap a layer of gas below the surface sediments, in Horizon A, which is released when the gas pressure builds up to a point where it overcomes the resilience of the hydrates. This would explain how vents become dormant and then reactivate after a period of inactivity, but the time scale predicted for this model does not fit Macron et al.'s data. Under this model the vents should be inactive for years at a time, whereas the observed quiet periods lasted from a few hours to a few months. Macron et al. suggest that possibly the basic premise of this hypothesis is correct, but that the gas is being trapped much closer to the surface by a less substantial hydrate lid, enabling smaller, more frequent bubble-outbursts from beneath a lid more easily overcome.

This would allow bubble release to be controlled at a local level, will small pockets of trapped gas building up within sediments in the gas hydrate solubility zone, beneath shallow blockages in the sediment pore-system. Overcoming these shallow blockages would require much less pressure to build up, with the increased pressure from tidal forces often being sufficient to trigger outbursts. 

The perpheral sites, where venting occurs but is far less frequent, may be receiving lower levels of gas from the underlying feeder sediments, or may be acting as pressure-release valves for a larger gas system beneath the gas hydrate solubility zone, venting less frequently as is predicted by the deep-reserve, large hydrate-lid model. 

The strong bottom currents observed at the Southern Hydrate Ridge also ought to play a role in the gas hydrate dissolution cycle, since these currents constantly bring in new water unsaturated in methane, leading to more rapid hydrate dissolution. 

Macron et al. note that strong upwelling currents are often observed at the Southern Hydrate Ridge, and that these tend to coincide with outbursts of bubble activity. They suggest that the upwelling currents may in fact be driven by the gas bubbles dragging water along with them as they rise. Curiously, however, the upwelling component of the system appears to be more strongly tied to the tidal system than the bubble activity is, with upwellings tending to stop during rising tides, while bubble activity frequently continues. Both upwelling currents and bubbles appear to reach depths slightly above the gas hydrate stability zone, which is consistent with the two phenomena being linked and the bubbles being protected by a hydrate-skin. The height to which both bubbles and upwelling currents rise varies seasonally, which is likely to be linked to seasonal water stratification.

Methane bubbling from the Southern Hydrate Ridge is a more-or-less constant phenomenon, although the location of the bubbling does vary over time. A number of vents are present, with the controls on bubbling at each of these apparently being independent. The continuous venting of bubbles appears is linked to the slow erosion of sedimentary structures on the seafloor, with occasional more substantial outbursts provoking more substantial overturn. The timing of bubble venting appears to be linked to tidal cycles, and is probably driven by hydrostatic pressure, although some bubble releases appear to be random and unconnected to tidal cycles.

Bubbling is more prevalent at low and falling tides, when pressure is low or falling, and this is more notable around spring tides, when pressure changes are more marked. At these times pore spaces in the sediment are more open, which could conceivably be related to outbursts of bubbling. However, bubbling also occurs at other times, which may indicate that pressure within the sediment is also a significant influencing factor. 

The main vents on the Southern Hydrate Ridge were active for between 50 and 75% of the time, although the level of activity at 'active' vents varied considerably in intensity, and could come from multiple locations within the vents. This makes it hard to estimate the amount of methane being released by the Southern Hydrate Ridge, and Macron et al. were unable to estimate this, despite having undertaken the most detailed study of the system to date. Based upon their findings they do not feel it would be reasonable to extrapolate data from a single vent across the whole system, instead any attempt to estimate the amount of methane being released would require long-term monitoring of the entire system. 

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Sunday, 19 April 2020

Understanding the methane-derived authigenic carbonates of the Croker Carbonate Slabs, and the benthic communities that live on them.

Methane-derived authigenic carbonate is a rocky biogenic substrate, formed just beneath the seabed. This substrate precipitates as a by-product of anaerobic methane oxidation by microbes, during the flow of methane from an underlying geological source. Methane-derived authigenic carbonate structures and their associated microbiota provide a range of important ecosystem functions, and occur globally from the intertidal to the deep ocean, at many thousands of ‘cold seeps’. When exposed at the seabed, the carbonate concretions are colonized by fauna that favour hard substrate, resulting in ‘oases of life’ in comparison with the surrounding, generally featureless, soft sediments. Where gas release is active, assemblages of seep-specialist macrofauna may occur, especially in waters beyond the continental shelf, and chemoautotrophic primary production by Bacteria and Archaea can influence the entire food web. Microbial assemblages also perform an important role in climate regulation. Precipitated carbonates serve as major carbon sinks, with anaerobic oxidation by microbes estimated to convert between 10 and 80% of mobilised methane to benthic biomass and carbonate. Significant active microbial biomass can be harboured within precipitated carbonates, capable of ongoing methane oxidation, even after exposure at the seabed. In light of the unique environmental services provided by methane-derived authigenic carbonate habitats, the need to further understand, assess, and mitigate anthropogenic disturbance to these systems is recognized, particularly in areas where petroleum exploration, mining, and demersal trawling are prevalent, or are likely to become so in the future. Global protection and management of methane-derived authigenic carbonate habitats is, however, currently limited in comparison with other biogenic habitats, such as Coral reefs.

In a paper published in the journal Aquatic Conservation on 21 February 2020, Tamsyn Noble-James of the Joint Nature Conservation Committee, and the Centre for Environment, Fisheries and Aquaculture Science, Alan Judd of the Alan Judd Partnership, Markus Diesing, also of the Centre for Environment, Fisheries and Aquaculture Science, and of the Norges Geologiske Undersøkelse, David Clare, again of the Centre for Environment, Fisheries and Aquaculture Science, Andrew Eggett, also of the Joint Nature Conservation Committee, Briony Silburn, once again of the Centre for Environment, Fisheries and Aquaculture Science, and Graeme Duncan, again of the Joint Nature Conservation Committee, present the first UK effort to develop a multidisciplinary approach to monitoring shallow methane-derived authigenic carbonate feature attributes, using the Croker Carbonate Slabs Special Area of Conservation as a case study.

The Croker Carbonate Slabs Special Area of Conservation is located in the UK sector of the Irish Sea, and covers an area of approximately 116 km², with a water depth ranging from 65 to 109 m below Chart Datum (the water level that depths displayed on a nautical chart, derived from the lowest astronomical tide). This area is influenced by high natural water turbulence, with strong tidal currents and with sediments subject to frequent resuspension and redistribution. The influence of these hydrodynamic forces is evidenced by the presence of a deep-water channel to the east of the marine protected area, and sedimentary bedforms such as sand waves. Mobile demersal, static demersal, and pelagic fishing activities are known to have taken place within the marine protected area, and three telecommunications cables intersect it; however, evidence of anthropogenic pressures within its boundary is generally limited, and at the time of the study the marine protected area was considered to be in ‘Favourable Conservation Status’.

The location of the Croker Carbonate Slabs Special Area of Conservation, within the UK Exclusive Economic Zone. Noble-James et al. (2020).

A multidisciplinary survey was conducted between 24 October and 6 November 2015, onboard the RV Cefas Endeavour. The broad aim of the survey was to investigate key methane-derived authigenic carbonate feature attributes, with the following objectives: (i) investigate the extent and distribution and characterize the physical structure of the methane-derived authigenic carbonate across the marine protected area; (ii) investigate whether methane release is ongoing, estimate the age of the surficial methane-derived authigenic carbonate, and explore the possibility of its continued precipitation; (iii) investigate whether chemoautotrophic taxa occur on the methane-derived authigenic carbonate or in the surrounding sediments; (iv) describe the epifaunal assemblages associated with ‘high relief’ and ‘low-relief’ forms of methane-derived authigenic carbonate; and (v) test the efficacy of combined multidisciplinary survey methods to optimise methane-derived authigenic carbonate monitoring strategies.

An EK60 single-beam echosounder and an EM2040 multibeam echosounder were deployed continuously and simultaneously throughout the acoustic survey operations. The single-beam echosounder data were used to identify potential gas seepage plumes, whereas the multibeam echosounder provided data on the depth, morphology, and backscatter strength of the seabed. Sub-bottom data were acquired using a deep-towed boomer, operated alternately at 135 and 240 J, to investigate the sub-seabed geology and to examine potential fluid transport pathways. Side scan sonar data were acquired using an EdgeTech 4800MP 300/600 kHz dual frequency digital system to identify areas of suspected gas seepage in the water column.

Video and still-image data were collected at 128 locations using a SeaSpyder ‘Telemetry’ drop camera system. Sediment samples were acquired at 56 stations using a 0.1 m² mini-Hamon grab. The sediment samples were sieved over a 1 mm mesh and processed for benthic macrofauna. Additional grab samples were acquired at three locations where suspected gas bubbles were observed leaking from the seabed in acoustic data, using a 0.1 m² Day grab. These samples were subsampled for benthic meiofauna and sieved over a 38 μm mesh. Full macrofauna samples were processed and identified according to National Marine Biological Association Quality Control scheme protocols, and meiofaunal samples were processed and identified.  All three faunal datasets were checked for chemoautotrophic taxa.

Suspected methane-derived authigenic carbonate concretions from 30 grab samples were retained for further analysis, following carbonate testing in the field using 10% hydrochloric acid. These samples underwent petrological, mineralogical, and isotope analysis. Eight samples were selected for strontium isotope (Strontium⁸⁷/Strontium⁸⁶) analysis and nine samples were selected for Uranium–Thorium age dating. X-ray diffraction optical microscopy and backscatter scanning electron microscopy were undertaken, primarily to ascertain the mineralogical composition of carbonate cements. Carbon  and Oxygen stable isotope analyses provided indications for the origin of Carbon in the cements and for seawater temperature at the time of carbonate precipitation, respectively. Strontium isotope analysis of aragonite extracted from five methane-derived authigenic carbonatesamples was conducted to establish the source of pore water fluids, and on three samples of recent calcareous encrusting biota to provide a reference value for the Strontium⁸⁷/Strontium⁸⁶ of the Irish Sea seawater signature. Uranium–Thorium age dating analysis was carried out on a subset of nine methane-derived authigenic carbonate samples previously analysed by petrographic and stable isotope methods.

A pump-driven molecular electronic transducer methane detector system was attached to the camera frame and operated continuously during 125 of the 128 deployments. Data were recorded at 5 second intervals and average methane concentrations were calculated per minute deployed. Water sampling was conducted at six locations, using a 10 L Niskin bottle (a plastic cylinder with stoppers at each end in order to seal the bottle, used to take water samples at a desired depth without the danger of mixing with water from other depths), to provide chemical validation of the methane values detected by the molecular electronic transducer sensor. Four samples were collected within the marine protected area at locations where the molecular electronic transducer sensor, single-beam echosounder, multibeam echosounder, or video data suggested that gas seepage was occurring. In addition, two control locations were sampled outside the marine protected area: one over the deepwater channel east of the marine protected area, and one to the south of the marine protected area. Three water samples were acquired at each location: one just above the seabed, one in mid-water, and one just below the sea surface. They were subsequently analysed by gas chromatography. 

Statistical analyses were undertaken on the still-image dataset, which excluded images of insufficient quality based on clarity, visibility of fauna, and confidence in methane-derived authigenic carbonate identification. Each image was assigned to a habitat class based on the European Nature Information System classification. The topographic character of the methane-derived authigenic carbonate varied on a continuum from small exposed patches to large outcropping cliffs. To further explore the variation in epifaunal assemblages associated with areas of the methane-derived authigenic carbonate that were more elevated from the seabed, the methane-derived authigenic carbonate images were assigned to one of two, broad, ‘highrelief’ and ‘low-relief’ methane-derived authigenic carbonate classes. High-relief methane-derived authigenic carbonate were defined as outcropping from the surrounding sediment and showing distinct elevation, whereas low-relief methane-derived authigenic carbonate formed low-lying slabs and isolated chunks that did not stand substantially above the surrounding seabed. The epifaunal abundance data were transformed according to the semi-quantitative Superabundant-Abundant-Common-Frequent-Occasional-Rare scale, were assigned numerical values; (6) Superabundant; (5) Abundant; (4) Common; (3) Frequent; (2) Occasional; and (1) Rare,  and analysed in PRIMER 6. The use of Superabundant-Abundant-Common-Frequent-Occasional-Rare data enabled the inclusion of the entire epifaunal community, which was recorded using different units (percentage cover for colonial and count data for solitary taxa), and reduced noise in the data caused by field-of-view variance. Mixed sediment and coarse sediment stillimage datasets were extremely large and were randomly subsampled to match the number of low-relief methane-derived authigenic carbonate class images (205 images), whereas all other classes contained fewer images. Analysis of similarity was conducted to test the null hypothesis of there being no difference in epifaunal assemblage structure between the habitat classes, and similarity percentage measures were generated for each class to identify which taxa contributed to similarity within and dissimilarity between classes.

Several epifaunal taxa were major contributors to similarity within the high-relief methane-derived authigenic carbonate class and were also observed in association with low-relief methane-derived authigenic carbonate, albeit at lower abundances. Where the occurrence frequency of these was deemed sufficient at least 20% of images in the high- and low-relief methane-derived authigenic carbonate classes), univariate analyses were conducted to evaluate whether the differences in abundance corresponded to a preference of taxa for high-relief methane-derived authigenic carbonate, or simply reflected the more fragmented nature and reduced continuous coverage of low-relief methane-derived authigenic carbonate. Abundance was compared between: (i) high-relief and low-relief forms; and (ii) different methane-derived authigenic carbonate percentage cover classes. The null hypothesis predicted no difference in abundance of each selected taxon between the high- and low-relief methane-derived authigenic carbonate forms. The test was repeated for three different data subsets to determine whether differences in abundance reflected a genuine preference for high- or low-relief methane-derived authigenic carbonate, or whether they were related to variance in methane-derived authigenic carbonate cover. The three datasets comprised: (A) all images including methane-derived authigenic carbonate; (B) images in which methane-derived authigenic carbonate covered at least 30% of the seabed; and (C) images in which methane-derived authigenic carbonate covered at least 70% of the seabed.

The methane-derived authigenic carbonate was mapped in several stages. First, the area of interest was spatially constrained to an area north and west of the channel and south of a sandwave field. Second, the methane-derived authigenic carbonate was mapped by extracting class descriptions from methane-derived authigenic carbonate observations (still images). Various features were trialled, and the following uncorrelated features were used: area (size of image objects), mean bathymetric roughness, mean backscatter, mean bathymetry, standard deviation of backscatter, and standard deviation of the bathymetric position index with a kernel size of 3 × 3. Third, a rule-based approach was subsequently used to map sand waves, i.e. areas where the methane-derived authigenic carbonate was not present or was buried beneath a substantial volume of sediment. All objects classified as sand waves or left unclassified were then assigned to the class ‘sediment’. Finally, the results were simplified by reclassifying ‘sediment’ objects fully or largely surrounded by methane-derived authigenic carbonate, and below a size of approximately 100 m², as methane-derived authigenic carbonate.

The extensive acoustic surveys provided a comprehensive physical description of the Croker Carbonate Slabs Special Area of Conservation, which was found to comprise an inclined plateau bordered to the south and east by deeper water. This plateau is covered by mobile surficial sandy sediments, in places forming sand waves. These are underlain by postglacial sediments that lie on coal-bearing Carboniferous rocks, believed to be a source of methane. The imagery data generally showed an extremely heterogeneous seabed. High- and low-relief forms of the methane-derived authigenic carbonate were visually identified across the majority of the marine protected area, whereas the remainder of the seabed comprised a range of sediment habitats (sand, mixed sediments, and coarse sediment) according to the European Nature Information System habitat classification. 

There was an increase in the predicted extent of the methane-derived authigenic carbonate within the marine protected area, from approximately 10 km² detected by a 2008 survey, to 20 km² determined by the new model. This new interpretation largely confirmed the extent of the ‘hard substrate’ identified in a 2012/2013 study in areas where the two datasets overlapped; however, differences were observed in the south-east of the site, where the 2012/2013 study indicated a more widespread occurrence of the methane-derived authigenic carbonate that was not confirmed by ground-truthing results. Still images and grab samples provided evidence that surficial sediment was present in areas interpreted acoustically as methane-derived authigenic carbonate, and which the software interpretation delineated the extent of the methane-derived authigenic carbonate ‘at or just below the sea bed’. It was not possible to distinguish between high- and low-relief methane-derived authigenic carbonate in the model interpretation, as none of the predictor features yielded a suitable separation of the two classes (i.e. the image locations for high- and low-relief methane-derived authigenic carbonate did not consistently correspond to distinct ‘objects’ identified from the multibeam echosounder data). 

The extent of the high- and low-relief methane-derived authigenic carbonate classes across the marine protected area could therefore not be predicted, only observed at discrete locations from imagery data. The imagery data indicated that low-relief methane-derived authigenic carbonate was present across the majority of the marine protected area, being most densely concentrated in the central and north-eastern areas, whereas the high-relief methane-derived authigenic carbonate was more prevalent in the south, and a discontinuous methane-derived authigenic carbonate ‘cliff’ line bounded the channel at the north-east edge of the marine protected area, with the cliff being visible from both multibeam echosounder and imagery data. The physical character of this cliff was comparable with a smaller cliff feature to the south of the site centre which was confirmed to be present in 2015. The north-eastern cliff line was also identified from multibeam echosounder in the south-east of the site, although no surficial methane-derived authigenic carbonate was observed here from the imagery. 

Combined multidisciplinary evidence for (a) high-confidence and potential methane-derived authigenic carbonate  extent and (b) active methane release within the Croker Carbonate Slabs Special Area of Conservation. Noble-James et al. (2020).

Sub-bottom profiler data revealed evidence of acoustic turbidity across the marine protected area: this is interpreted as gas within the seabed sediments. The lateral increase in the amplitude of some individual reflections (‘gas brightening’) also suggested an increased concentration of gas within sediments. ‘Gas chimneys’ were apparent in the form of vertical columns of acoustic turbidity. Boomer profiles were crossreferenced with acoustic, visual, and physical evidence, which validated the interpretation of shallow gas.

Low-relief methane-derived authigenic carbonate within the Croker Carbonate Slabs Special Area of Conservation. Noble-James et al. (2020).

Apparent gas bubble plumes were identified from single-beam echosounder (21 locations) and side scan sonar water column data (five locations), and bubbles were directly observed leaking from the seabed in video imagery at two locations.

Images of gas bubbles within the Croker Carbonate Slabs Special Area of Conservation. Noble-James et al. (2020).

Black, potentially sulphidic, sediment patches were recorded adjacent to methane-derived authigenic carbonate concretions at four locations, and at one location white mats thought to comprise thiotrophic (sulphur oxidising) Bacteria (e.g. Beggiatoa spp.) were recorded at their edges.

Twenty-nine of the 30 suspected methane-derived authigenic carbonate samples acquired in grab samples were determined to be carbonate cemented, and contained high-magnesium calcite, aragonite, or a combination of both cements. Carbon¹³ values generally ranged from −34 to −54‰ (parts per thousand) when compared with the Pee Dee Belemnite, a global standard; this is consistent with an authigenic origin in which carbonate precipitation is a consequence of anaerobic methane oxidation. Strontium⁸⁷/Strontium⁸⁶ analysis suggested the aragonite and calcareous encrusting biota were precipitated in sea water that was similar to present-day sea water (strontium isotopes vary a great deal with local geology and hydrology, and are useful for determining the origin of biominerals). 

Uranium-Thorium dating conducted on aragonite extracted from two samples indicated that methane-derived authigenic carbonate formation occurred during the period from approximately 17 000 to 4000 years before present (Uranium-thorium dating works because uranium decays to thorium at a known rate, so that the ratio  of the two elements in minerals that naturally incorporate uranium but not thorium can be used to establish a date for the minerals). It is likely that gas release has been ongoing for a considerable period of time (for tens of thousands of years, at least), and that methane-derived authigenic carbonate formation is likely to have occurred continuously since sea water returned to the site as the sea level rose following the last glaciation, approximately 17 000 years ago.

Multivariate analysis of still-image data showed that epifaunal assemblages associated with the high-relief form of the methane-derived authigenic carbonate were not significantly different from those of the low-relief form, and the statistics indicated a high level of similarity. Assemblages associated with both forms of the methane-derived authigenic carbonate were highly significantly different to all other habitat classes except for coarse sediment, in comparison with high-relief methane-derived authigenic carbonate; however, it should be noted that although statistically significant, the differences between some group pairs were small (e.g. low-relief methane-derived authigenic carbonate versus mixed sediment, and low-relief methane-derived authigenic carbonate versus coarse sediment). 

High-relief methane-derived authigenic carbonate with attached sessile epifauna. Noble-James et al. (2020).

High-relief and low-relief methane-derived authigenic carbonate faunas were both dominated by the clump-forming and solitary Hydrozoa, which occurred in 75 and 76% of high- and low-relief methane-derived authigenic carbonate images, respectively, contributing 30.9 and 42.9% to within-class similarity. A small group of taxa, including clump-forming and solitary Hydrozoa, Polychaetes, turf Hydrozoa, and Serpulids, were consistently dominant within all habitat classes, including sediment. Beyond these dominant taxa, differences in epifaunal assemblage composition between the two methane-derived authigenic carbonate forms and the remaining habitat classes appeared mainly attributable to a small number of taxa. Five taxa (identified to species or genus level) were substantially more abundant in association with the high-relief and/or low-relief methane-derived authigenic carbonate classes in comparison with other habitat classes. These were the soft coral Alcyonium digitatum, the Bryozoan genus Cellaria, the Hydroid genera Nemertesia (including Nemertesia ramosa and Nemertesia antennina) and Tubularia (including Tubularia indivisa), and the Polychaete family Sabellidae (including Sabella pavonina). In combination, these taxa contributed 32.8% to the within-group similarity of high-relief methane-derived authigenic carbonate and 13.0% to the within-group similarity of low-relief methane-derived authigenic carbonate. These five taxa were consistently amongst the top contributors to dissimilarity between the two methane-derived authigenic carbonate classes and other habitat classes (except for Alcyonium digitatum and Tubularia on low-relief methane-derived authigenic carbonate, and mixed and coarse sediments). The frequency of occurrence in still images for the five taxa was higher for both forms of the methane-derived authigenic carbonate than for other habitat classes, particularly for high-relief methane-derived authigenic carbonate.

The occurrence frequency of Alcyonium digitatum, Cellaria, and Sabellidae in still images was deemed sufficient to compare abundances between high- and low-relief forms of methane-derived authigenic carbonate (i.e. they occurred in over 20% of images for each methane-derived authigenic carbonate class). The abundance of Alcyonium digitatum was significantly higher in association with high-relief methane-derived authigenic carbonate than with low-relief methane-derived authigenic carbonate for all three data subsets, however, there was no significant difference in the abundance of Sabellidae between the two methane-derived authigenic carbonate forms in the data. The abundance of Cellaria was significantly higher on high-relief compared with low-relief methane-derived authigenic carbonate for dataset (A) (1–100% methane-derived authigenic carbonate cover), but this difference was not apparent when the test was repeated for subsets (B) (over 30% methane-derived authigenic carbonate cover) and (C) (over 70% methane-derived authigenic carbonate cover). These results indicate that only Alcyonium digitatum was consistently more abundant on high-relief than low-relief methane-derived authigenic carbonate, regardless of the percentage cover of methane-derived authigenic carbonate in the images.

The Soft Coral Alcyonium digitatum. Biopix/iNaturalist.

No conclusive evidence of chemoautotrophic fauna associated with gas seepage was found in the epifaunal, macrofaunal, and meiofaunal taxa identified. Two Desmodorid Nematode genera were recorded within the marine protected area: Leptonemella and Catanema. These taxa exhibit relationships with thiotrophic ectosymbiotic Gammaproteobacteria. Although the presence of sulphidic materials may enhance the sediment conditions for these taxa, they cannot be categorically linked to gas seepage, as bubbles were not directly observed at the sample locations (i.e. only observed from acoustic data).

Petrological, mineralogical, and isotope analysis of suspected methane-derived authigenic carbonate samples confirmed that the mineral assemblage and Carbon isotope values are characteristic of methane-derived authigenic carbonate. The sample characteristics are comparable with those described previously from more limited surveys of the Croker Carbonate Slabs and methane-derived authigenic carbonate occurrences elsewhere, including the UK sector of the North Sea, and the Kattegat, where ‘Submarine structures made by leaking gases’ were first described in 1992.

Methane-derived authigenic carbonate sample with faunal excavations. Noble-James et al. (2020).

Noble-James et al.'s interpretation of the 2015 acoustic and groundtruthing data increased the extent of the methane-derived authigenic carbonate mapped with high confidence within the marine protected area (either exposed at or subcropping close to the seabed), from approximately 10 km² to approximately 20 km². This makes the Croker Carbonate Slabs the largest known shallow methane-derived authigenic carbonate feature within the Natura 2000 marine protected area network, mapped using ‘good’ quality data. The analysis did not confirm the presence of methane-derived authigenic carbonate in the south-east of the site, an area where the possible presence of methane-derived authigenic carbonate was inferred previously based on the presence of ‘hard substrate’ detected from acoustic backscatter data. The large methane-derived authigenic carbonate cliff feature observed from imagery in the north-east of the site was thought to continue southwards to this area below the seabed surface, however. It is possible that the hard substrate interpreted in the previous study may be methane-derived authigenic carbonate buried under a substantial veneer of mobile sediment and/or clay (which was observed as exposed here between sand waves). To reflect the uncertainty around the character of the highly reflective substrates observed from backscatter, additional areas totalling approximately 37 km² were classified as ‘potential methane-derived authigenic carbonate’ within the marine protected area.

The still and video imagery, supported by side scan sonar and multibeam echosounder data, provide clear evidence of a mobile sediment veneer across a significant portion of the marine protected area, forming sand waves in places. These bedforms are likely to impede the detection of methane-derived authigenic carbonate in the affected areas, with the methane-derived authigenic carbonate being uncovered and reburied on various temporal and spatial scales. The exposed extent of the methane-derived authigenic carbonate is thus in a continual state of flux. Exposed methane-derived authigenic carbonate may be colonised by fauna but are also subject to erosion. It has previously been postulated that there may be an evolution from intact sheets of carbonate to sand- and gravel-sized fragments, as a result of erosion from strong currents and mobile sediments and the activity of boring organisms. methane-derived authigenic carbonate is a relatively hard substance, akin to limestone, however, and the persistence of the cliff feature observed in 2004 and 2008, and the high- and low-relief features that were delineated from 2008 data, indicate that this process is slow (in human terms).

The wide range of multidisciplinary data sources used in the study (molecular electronic transducer sensor, water samples, sub-bottom profiler, single-beam echosounder, side scan sonar, and imagery) provide strong evidence with which to conclude that methane seepage is ongoing across much of the site. Most methane concentrations detected by the molecular electronic transducer sensor were supersaturated when compared with the overlying atmosphere. The supersaturated sea surface waters indicate that the site is exporting methane to the atmosphere. It has been suggested that most of the methane rising from sub-seabed sources is used by anaerobic oxidation (the ‘benthic methane filter’) close to the seabed. The methane-derived authigenic carbonate and hydrogen sulphide are by-products of anaerobic methane oxidation beneath the seabed, so it can be concluded that methane-derived authigenic carbonate formation is likely to continue within the Croker Carbonate Slabs Special Area of Conservation. The Uranium-Thorium isotope dating of aragonite crystals in the methane-derived authigenic carbonate samples suggests that it has been forming since the Last Glacial Maximum. Evidence of ongoing gas seepage across the marine protected area supports the theory that methane-derived authigenic carbonate is present beneath the seabed within, and possibly beyond, the areas of ‘potential methane-derived authigenic carbonate’. The rate at which methane-derived authigenic carbonate is expected to be precipitated is unknown, although the Uranium-Thorium dating analysis suggests that the formation of the Croker Carbonate Slabs has taken place over an extended period of time, which is consistent with findings from the North Sea and the Barents Sea. As methane-derived authigenic carbonate is still thought to be forming at the Croker Carbonate Slabs, there may be potential for the generation, regeneration, and improvement of feature condition in terms of methane-derived authigenic carbonate extent and structure, which could counteract the natural erosion of the exposed methane-derived authigenic carbonate. Regeneration is, however, highly unlikely to mitigate any damage caused to the methane-derived authigenic carbonate by non-natural disturbances within the marine protected area (and presumably elsewhere), such as abrasion or physical damage by demersal towed or static fishing gear.

Methane concentrations (nmol/L) from water samples acquired at surface, mid-water and bottom-water. Noble-James et al. (2020).

Six of the seven habitat classes, including high- and low-relief methane-derived authigenic carbonate, were dominated by one or more of the same four high-level (and predominantly attached sessile) taxa, suggesting a hard substrate beneath a sediment veneer or stable lithic material not subject to transport by tidal currents. This apparent lack of distinction between the methane-derived authigenic carbonate forms and the surrounding sediment habitats is likely to reflect the adaptability of the taxa, with many of the same taxa that have colonised the methane-derived authigenic carbonate also attaching to the larger fractions of coarse sediment. The seabed was extremely heterogeneous, meaning that many images contained small areas of secondary substrate in addition to the primary classified substrate (e.g. a small number of pebbles in an image otherwise dominated by sand). As suggested by the results of the analysis, it is also likely that areas of non-visible methane-derived authigenic carbonate buried by a thin sediment veneer (and colonized by typical sessile taxa) have been classified as sediment habitats. Additionally, it should be noted that some areas of methane-derived authigenic carbonate may have been obscured by extensive low-lying aggregations of Sabellaria spinulosa (and therefore images classified as such), although the presence of methane-derived authigenic carbonate could not be verified because of the encrusting nature of this tubiculous Polychaete. 

A reef formed by the tubiculous Polychaete, Sabellaria spinulosa, in the  the Dutch Brown Bank area of the North Sea. Oceana.

Although five taxa were found to be associated with both highand low-relief methane-derived authigenic carbonate (being seldom recorded in the other habitat classes), four of them; Alcyonium digitatum, Cellaria, Nemertesia, and Tubularia, occurred in a notably higher number of high-relief methane-derived authigenic carbonate images. For Alcyonium digitatum, this relationship was not related to disparities in percentage cover between low- and high-relief methane-derived authigenic carbonate. The high-relief form of methane-derived authigenic carbonate clearly provides enhanced conditions for this species (and possibly others that could not be detected from imagery data), potentially through the greater elevation above the seabed and the increased structural complexity. An elevated position above the seabed is likely to afford protection to sessile organisms from intense smothering or scouring by mobile sediments. This seems unlikely to be the sole driver of the increased abundance, however, as Alcyonium digitatum does not appear to be particularly sensitive to these pressures. Tidal currents may become accelerated and water velocity increased with obstruction from high-relief methane-derived authigenic carbonate, potentially resulting in a greater volume of plankton and organic material available to suspension-feeding taxa. Particle uptake by Alcyonium digitatum is limited by low-velocity water flow (in addition to very high velocities at the opposite end of the spectrum). The increased structural complexity of high-relief  methane-derived authigenic carbonate could also provide greater potential for the retention of, and colonisation by, planktonic invertebrate stages.

The presence of biological excavations on the methane-derived authigenic carbonate samples and in imagery data indicates that boring fauna are likely to be a functionally significant component of the fauna within the marine protected area. Such fauna increase the habitat complexity and therefore niche availability to other epifauna, whilst also contributing to the erosion and eventual breakdown of the carbonate. The boring Sponge Cliona celata was recorded on methane-derived authigenic carbonate, although only from a small number of images. It is likely that boring fauna have been underrepresented in Noble-James et al.'s study, as a result of the dense cover of attached fleshy, branching, and foliose Hydroids, Bryozoans, and Soft Corals, and the generally low taxonomic resolution achievable from the imagery data. The characterising and monitoring of such taxa would involve acquiring replicate samples of intact methane-derived authigenic carbonate, a method that is unlikely to be justified in the context of a long-term monitoring programme, given the slow formation rate of the feature.

White patches of suspected thiotrophic Bacteria were observed close to some methane-derived authigenic carbonate concretions; these Bacterial mats are recognized as ubiquitous where there is active anaerobic oxidation of methane. Despite the extensive visual and physical sampling regime, and the analysis of several meiofaunal samples from areas of suspected gas seepage no other chemoautotrophic organisms thought to be directly associated with methane release were recorded. A previous study found no seep specialist macrofauna at the Codling Fault Zone, approximately 30 km south-west of the Croker Carbonate Slabs. The authors of that study noted that seep assemblages in shallow water (0–200 m) are less likely to contain seep-specialised taxa than at deep water sites, as strong competition from fauna that use photosynthetic carbon is expected at shallow depths. In the Kattegat there were found to be ‘major differences’ in the abundance and biomass of Nematode populations close to seeps (5–20 cm) and at control sites 30 m away, which may support this assertion. Another study did, however, record the seep-specialist Bivalve, Thyasira sarsi, and Nematodes of the genus Astomonema at the Scanner Pockmark in the North Sea (roughly 150 m below Chart Datum), indicating that chemoautotrophic infauna could also exist within the marine protected area (beyond the observed Leptonemella and Catanema), but may not have been detected. Another study recorded high densities of Astomonema southwardarum in the Scanner pockmarks, but not at the Braemar pockmarks.

The results of the multidisciplinary survey have highlighted various implications for monitoring shallow water methane-derived authigenic carbonate habitats and faunal assemblages under the feature attribute framework, which can be used to assess condition and to inform management measures.

Geological, mineralogical, and petrographical analyses provided conclusive evidence that previously suspected areas of methane-derived authigenic carbonate did in fact comprise this habitat. These specialist analyses are, however, resource and cost intensive. It is expected that an initial application of these methods will be sufficient to provide evidence on the ‘Natural gas seepage and methane-derived authigenic carbonate formation’ and ‘Climate regulation’ feature attributes, after which a simplified scope can be used to monitor whether gas seepage continues (and probable continued precipitation can be inferred). The use of the molecular electronic transducer sensor (with validating water samples) was extremely cost-effective in comparison with the acoustic methods used to detect gas seepage (sub-bottom profiler, side scan sonar, and single-beam echosounder), as it was deployed on the camera frame (with camera transects taking 23 minutes on average, across the 128 deployments), and readings were instantly available.

The mineralogical and petrographical analyses supported the postulation that methane-derived authigenic accretion is likely to continue at present, indicating that the habitat and its microbial consortia could perform an ongoing role in climate regulation. Methane-derived authigenic carbonates, including sediment-hosted nodules and well-lithified carbonate rocks and pavements at the seabed, host substantial active microbial biomass capable of methane oxidation under both oxic and anoxic conditions. Further sampling and analysis of intact carbonates (at and below the seabed) in areas of active methane release could improve our understanding of endolithic microbial assemblages, and their role (if any) in climate regulation. The value of this (and other) detailed ‘one-off’ study (or studies) would need to be carefully evaluated in the context of the available resources and the competing time-series evidence requirements of the other feature attributes.

At a number of ground-truthing locations methane-derived authigenic carbonate was predicted from the acoustic backscatter interpretation but were not visually observed at the seabed. Multibeam echosounder pulses penetrate the seabed to some extent, depending on the acoustic frequency and the sediment type. Here, it appears that exposed methane-derived authigenic carbonate and methane-derived authigenic carbonate covered by a thin veneer of sediment have essentially the same acoustic signature. Furthermore, the analysis might be confounded by spatial heterogeneity at short length scales on the same order or less than the positioning accuracy of the drop camera system. Therefore, it should not be assumed that perceived methane-derived authigenic carbonate signatures consistently indicate exposed methane-derived authigenic carbonate. Equally, in shallow habitats dynamic regimes can result in the fluctuating resuspension and deposition of sediments and the presence of mobile bedforms, such as sand waves. An apparent reduction of methane-derived authigenic carbonate extent from imagery data alone will therefore not necessarily indicate a loss of habitat and should not automatically be interpreted as such. The acquisition of photo-mosaic data by remotely operated vehicle or autonomous underwater vehicle would allow direct comparison of changes in the extent of methane-derived authigenic carbonate exposed at the seabed, improving our understanding of natural fluctuations in seabed composition over time. Subsurface cores (e.g. using a vibrocore) would confirm the depth and likelihood of exposure of any methane-derived authigenic carbonate underlying the sediment veneers.

Where methane-derived authigenic carbonate is exposed above the seabed, the physical structure is likely to change over time, through erosion by sediment scour and bioturbation. The challenge will lie in determining whether changes have occurred as a result of these natural processes or through human impacts. Given that the cliff structure observed in 2005 and 2008 was physically comparable in 2015, Noble-James et al. postulate that the physical structure should not change dramatically between monitoring events without physical damage having taken place; however, we cannot state this with certainty unless further studies on erosional processes and the rate of methane-derived authigenic carbonate formation are undertaken. The results of the methane-derived authigenic carbonate dating analysis suggest that methane-derived authigenic carbonate formation is extremely slow (in human terms) and that the methane-derived authigenic carbonate has been assessed as highly sensitive to physical loss, physical change, removal of substratum, and abrasion/disturbance of the surface of the substratum. Fishing equipment, such as bottom trawling nets, has been known to tear pieces off the carbonate structures. Methane-derived authigenic carbonate surveys could therefore acquire targeted lines of multibeam echosounder data across high-relief methane-derived authigenic carbonate and cliff features in areas where these pressures are known to occur (e.g. mobile or static demersal fishing grounds, or cable routes) and areas of no impact. Comparing georeferenced bathymetric profiles of these features over time would provide a cost-effective means of monitoring the physical structure in the areas most likely to exhibit detectable change. As the hydrodynamic and sedimentary regimes are thought to exert strong influences on the distribution and character of methane-derived authigenic carbonate and associated communities, an improved understanding of these processes, the natural erosive forces exerted on the methane-derived authigenic carbonate across the entire marine protected area, and the extent to which it is uncovered and reburied, could be achieved through hydrodynamic modelling, sediment capture, seabed coring, and/or the investigation of sediment veneer depth using high-frequency sub-bottom profilers (e.g. a parametric echosounder). It should also be noted that the joint effects of ocean acidification and the production of hydrogen sulphide by anaerobic oxidation of methane could create conditions accelerating the erosion of methane-derived authigenic carbonate, and therefore pH measurements at the seabed would be a valuable addition to future monitoring surveys.

Key and influential species and characteristic communities supported by the methane-derived authigenic carbonates and surrounding methane-rich sediments (and in turn, associated primary and secondary production) are important components of habitat condition assessments. Given the active methane seepage observed within the marine protected area, chemoautotrophic community structure was initially considered for future monitoring; however, Noble-James et al.'s study supports the findings of a number of previous publications indicating that chemoautotrophic assemblages, if present, are highly spatially constrained at shallow water methane seeps through competitive pressure from background fauna. It therefore appears that ‘blind’ infaunal sampling (i.e. using samplers that cannot be guided to specific targets) is of limited value for detecting chemoautotrophic communities in shallow areas, where substrate heterogeneity creates a large number of microhabitats, and when steep geochemical gradients are present. Chemoautotrophic communities, if present, are likely to be more effectively sampled using a remote operated vehicle. This would, however, require direct sampling over visually identified seeping gas bubbles (which were only encountered twice during the survey of Croker Carbonate Slabs) or dark patches of sulphidic sediment. This approach is likely to prove costly and is likely to yield relatively few data with which to evaluate any changes in chemoautotrophic community structure.

The results of Noble-James et al.'s study suggest that future biological monitoring at this marine protected area should focus on epifaunal ‘Characteristic communities’; however, the inherent limitations of epifaunal identification from imagery data have been highlighted at this marine protected area, as a result of both the turbidity of the water column and the problematic nature of remotely identifying taxa that do not have distinctive characteristics to aid the identification from images (including many of the dominant fauna at this marine protected area, e.g. Hydroids, Bryozoans, and Polychaetes). Given that future epifaunal monitoring will be centred on non-destructive imagery data, a morphotaxonomic approach to imagery analysis could be used, as these rely on morphological descriptors rather than the recognition of potentially cryptic taxonomic identification features to record epifauna from imagery. If adopted as the first step in a nested classification approach, morphotaxonomic classification could have advantages in improving the consistency and reliability of epifaunal identification where achievable taxonomic resolution is low. Such an approach would require testing before implementation, as well as the inclusion of a second step using traditional taxonomic identification, where species identification is possible. A fully quantitative approach to monitoring the ‘Characteristic communities’ is also required for robust and accurate assessments of change over time. Although the semiquantitative Superabundant-Abundant-Common-Frequent-Occasional-Rare scale was effective for characterizing both the sessile and motile fauna associated with methane-derived authigenic carbonates, the habitat provision function of methane-derived authigenic carbonates may be best assessed using the percentage coverage of epifauna (with post-hoc standardization of the image field of view). Given the highly variable and discontinuous nature of methane-derived authigenic carbonates exposure in some areas, epifaunal percentage cover should be recorded as the percentage of the methane-derived authigenic carbonates substrate when assessing the role of methane-derived authigenic carbonates in habitat provision, as opposed to the percentage within the image.

The five epifaunal taxa found to associate with the methane-derived authigenic carbonate exhibit similar life-history traits (i.e. they are attached sessile suspension feeders), which are common among hard substrate-inhabiting invertebrates, suggesting that they could be considered characteristic of the methane-derived authigenic carbonates at this marine protected area, when in Favourable Conservation Status. All five taxa were noted in association with methane-derived authigenic carbonate following the 2008 survey, with Alcyonium digitatum, Nemertesia, and Tubularia also recorded at the nearby Codling Fault Zone marine protected area in Republic of Ireland waters. Alcyonium digitatum is widely distributed across the North-East Atlantic, being recorded on hard substrates from Norway to Portugal, and has been noted in association with methane-derived authigenic carbonates elsewhere in Europe. This species is of particular interest as a ‘characteristic’ species for future monitoring (at Croker Carbonate Slabs and elsewhere) because of its large body size, conspicuous shape, and colour range, which can be identified from sediment-obscured images and video footage where the camera is suspended high above the seabed. Although monitoring these easily identifiable and methane-derived authigenic carbonate-associated taxa would contribute to an assessment of whether the ‘status quo’ has been maintained (i.e. the methane-derived authigenic carbonate is in Favourable Conservation Status), these taxa are not thought to be highly sensitive to physical abrasion by fishing gear (to which some areas of the marine protected area have been exposed). Hard substrates such as methane-derived authigenic carbonate are likely to be rapidly colonised by opportunistic Hydroids, Bryozoans, and Ascidians following such a disturbance; three of the five ‘characteristic’ methane-derived authigenic carbonate-associated taxa were Hydroids and Bryozoans, whereas the ‘characteristic’ Soft Coral Alcyonium digitatum is also not thought to be highly sensitive to physical abrasion. The percentage cover of slow-growing sensitive taxa, such as Sponges and Anthozoans (both of which were observed on high- and low-relief methane-derived authigenic carbonate), may therefore be more effective as an indicator of physical damage to methane-derived authigenic carbonate, although the validity of this metric would require further investigation. 

The results of the epifaunal analyses indicated that treating the low and high-relief methane-derived authigenic carbonate forms as separate sampling strata in future monitoring designs may provide greater insights into ‘characteristic’ assemblage composition between different forms, which could potentially be more or less vulnerable to anthropogenic impacts (e.g. demersal trawling). If consistently observed through time, the occurrence ratio of observed taxa between the two methane-derived authigenic carbonate forms could contribute to an understanding of habitat condition. The inability of the model to differentiate the two methane-derived authigenic carbonate forms is most likely a result of fine-scale heterogeneity that could not be resolved using ship-mounted multibeam echosounder data. Mapping the different morphological forms of the methane-derived authigenic carbonate would require higher resolution acoustic data such as that achieved when using an multibeam echosounder or synthetic aperture sonar mounted on an autonomous underwater vehicle. An autonomous underwater vehicle-mounted synthetic aperture sonar could deliver acoustic data with a resolution of a few centimetres, but this is a cost- and time-intensive survey method. Stratification between known areas of high and low methane-derived authigenic carbonate (verified as such by an initial collection of imagery data), is likely to prove sufficient to investigate communities associated with each form in the early stages of a monitoring time series. If a more targeted approach to monitoring specific areas was developed over time, detailed synthetic aperture sonar monitoring could form part of a resource-balanced monitoring programme.

In summary, the multidisciplinary techniques used in Noble-James et al.'s study enabled a comprehensive study of the methane-derived authigenic carbonate feature attributes; however, they do not offer the most cost-effective use of resources for monitoring beyond an initial characterization. For subsequent monitoring events, at the Croker Carbonate Slabs Special Area of Conservation and elsewhere, a simplified combination of methods could provide sufficient evidence for the assessment of whether the methane-derived authigenic carbonate is in Favourable Conservation Status, and whether human impacts have affected the integrity of the methane-derived authigenic carbonate in discrete areas. This simplified sampling scope could primarily consist of towed camera transects A molecular electronic transducer sensor attached to the camera (and validated by water samples) would allow for the assessment of natural gas seepage and methane-derived authigenic carbonate accretion, whereas targeted multibeam echosounder lines could provide further evidence for changes in the physical structure of the methane-derived authigenic carbonate.

Although this approach would deliver sufficient evidence for a condition assessment, a more holistic understanding of the ecosystem, involving research and development studies, would provide valuable context for these assessments and would improve the ability of scientists to make robust and defensible recommendations on future management. Such studies could include subsurface methane-derived authigenic carbonate investigations using acoustic and coring techniques, detailed characterizations of infaunal and endolithic chemoautotrophic assemblages, the improvement of habitat models using photo-mosaics and high-resolution acoustic data, and modelling of the hydrodynamic and sedimentary regimes.

Noble-James et al.'s study has demonstrated that the Croker Carbonate Slabs form an extensive, stable, and complex lithic substrate in an area of the Irish Sea that would otherwise be dominated by sandy sediments; it is one of the largest known examples of shallow methane-derived authigenic carbonate in European waters. This substrate supports dense aggregations of epifauna (being a rich source of secondary production), increases habitat complexity and niche availability, and presumably contributes to larval dispersal by taxa that attach to hard surfaces and are typically rare in the offshore region of the Irish Sea. The observed active methane seepage, and the presence of Bacterial mats, suggests that chemosynthetic primary production is ongoing, and the habitat is still thought to be precipitating subsurface, with chemoautotrophic assemblages performing important climate regulation functions.

Noble-James et al. have demonstrated multidisciplinary approaches to characterising and monitoring these functionally important habitats. They have developed recommendations to maximize the cost effectiveness of future monitoring, whilst optimizing the scientific robustness of data to inform effective decision making on methane-derived authigenic carbonate conservation and management. As mentioned previously, the conservation status of shallow methane-derived authigenic carbonates within the European marine protected area network is largely unknown.

See also...

https://sciencythoughts.blogspot.com/2019/03/lophelia-pertusa-cold-water-coral.htmlhttps://sciencythoughts.blogspot.com/2018/05/meganodontia-haunuiensis-elliptiolucina.html
https://sciencythoughts.blogspot.com/2018/05/rosaliella-svalbardensis-new-species-of.htmlhttps://sciencythoughts.blogspot.com/2018/03/microbial-biodiversity-around-garga-hot.html
https://sciencythoughts.blogspot.com/2017/08/a-hydrocarbon-seep-from-late-triassic.htmlhttps://sciencythoughts.blogspot.com/2016/08/analysing-distribution-of-pleistocene.html
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