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Ecologically or Biologically Significant Areas (EBSAs)

  published: 17 Mar 2023

Atlantis-Meteor Seamount Complex

General Information
The Atlantis-Meteor Seamount Complex comprises 10 seamounts. These seamounts are hotspots of marine life and areas of enhanced productivity, especially when compared with surrounding abyssal areas. This seamount complex has a total area of 134,079 km2, with depths ranging from 265m (top of Atlantis seamount) to 4,800m (base of Great Meteor seamount). A total of 437 species are present in this area (with 16 per cent of mega- and macrofauna and up to 91 per cent of meiofauna endemic to the seamount group), 3.9 per cent of which are protected under international or regional law.

The Atlantis-Meteor Seamount Complex comprises 10 seamounts: Atlantis, Cruiser, Hyeres, Irving, Pico Sul, Plato, Tyro, Meteor Bank, the latter including Great Meteor, Closs and Small Meteor.

Benthic biological communities on seamounts are highly vulnerable to human activities. Many benthic species are long-lived, slow-growing and vulnerable  to human impacts. Seamounts are defined as isolated topographic features of the seabed that have a limited lateral extent and rise more than 1000m from abyssal depths (Menard, 1964). Large seamounts usually originate as volcanoes and are primarily associated with intraplate hotspots and mid-ocean ridges (Staudigel et al., 2010). Generally, seamount topography is responsible for these structures qualifying as high complexity sites. Due to their isolated location, these structures can be an obstacle to the free circulation of the oceans. This gives rise to different kinds of phenomena and disturbances, including an increase in the speed of sea currents, upwellings, turbulence, Taylor cones, eddies and even jets in the zones where the seamounts interact with ocean currents (Richardson et al., 2000; Kunze & Smith, 2004; White et al., 2007; Pakhorukov, 2008).

Seamounts are hotspots of marine life (e.g., Rogers, 1994; Gubbay, 2003; Morato & Pauly, 2004; Pitcher et al., 2007, 2010; Mendonça et al., 2012) and in general are areas of enhanced productivity in comparison with nearby abyssal areas. In most cases, around the seamounts there is an extensive anticyclonic eddy associated with the lifting of nutrients from the rich deep water, giving rise to high concentrations of nitrates and chlorophyll in shallow waters (Coelho & Santos, 2003), which encourages the development of a wealth of flora and fauna on the structures, leading to exposed hard substrates and improved food conditions for epibenthic suspension feeders (e.g., Cartes et al., 2007 a), b); Genin & Dower 2007), such as cold-water corals or deep-water sponges (e.g., Samadi et al., 2007; Sánchez et al., 2008), tunas (e.g., Yasui 1986; Morato et al., 2010, Ressurreição & Giacomello, 2013), marine mammals (e.g., Cañadas et al., 2002; Correia et al., 2015), and other organisms that apparently feed on prey aggregations (e.g., Boehler & Sasaki, 1988; Porteiro & Sutton, 2007; Tabachnick & Menchenina, 2007). Seamounts are biologically distinctive habitats of the open ocean exhibiting unique features (Rogers, 1994; Probert, 1999; Morato & Clark, 2007). These structures can host very distinctive biological communities that are different from the communities on nearby abyssal plains dominated by soft sediment, and these particular places may attract pelagic fish, including larger, commercially valuable species and other marine top predators such as loggerhead sea turtles (Caretta caretta) and marine mammals (e.g., Holland & Grubbs, 2007, Kaschner, 2007, Santos et al., 2007).

The Atlantis-Meteor Seamount Complex is part of the Macaronesian region. The area is situated about 1500 km northwest of the African continent and contains 10 banks, which usually have flat summit plateaus, together with a few lesser seamounts. The whole feature is a large volcanic complex in the central North Atlantic Ocean, situated some 700 km south of the Azores (Verhoef, 1984). It is the southernmost of a chain of large seamounts extending south from the Azores Plateau (Figure 1).

The Meteor bank is one of the best explored seamounts in the world, and since an expedition in 1998, detailed information on the meiofauna inhabiting its plateau has been made available. The Great Meteor resembles an isolated “island” in respect to the colonization by meiofauna. More data is included in the descriptions of some seamounts, such as Atlantis, Hyeres, Irving and Plato, than others (see Table 1), due to a greater sampling effort. Most of the older research was focused on geology.

Table 1 – Summary of the  EBSA criteria met by each structure of the Atlantis-Meteor Seamount Complex (Crit 1 (Uniqueness or rarity), 2 (Special importance for life-history stages of species, 3 (Importance for threatened, endangered or declining species and/or habitats), 4 (Vulnerability, fragility, sensitivity, or slow recovery), 5 (Biological productivity), 6 (Biological diversity) and 7 (Naturalness). Nº sps – total number of species in each structure. Nº refs - total number of references in each structure. n.i. – No information available.

In terms of geology the structures of the area have different compositions, locations and ages.

The shallower parts of the Atlantis-Meteor Seamount Complex are elevated structures and, with the exception of the Atlantis seamount, are oriented roughly parallel to the ridge, implying a lithospheric control for these volcanic constructions (Gente et al., 2003). The seamount with the highest proportion of studies recorded in the Atlantic was the Great Meteor seamount (Kvile et al., 2014).

The Meteor bank, situated south of the Azores, is one of the largest banks in the North-East Atlantic, with a wide plateau of 1500 km2 developed between 400 m and its summit at 275 m water depth. Great Meteor has a volcanic core and is capped by 150-600 m of post-Middle Miocene carbonate and pyroclastic rocks and covered by highly reworked, residual bioclastic sands. During the late Miocene to Pliocene it was levelled by wave truncation (Mironov & Krylova, 2006). Since the Pliocene, the summit plateau subsided, probably isostatically, to its present water depth of 275 m, interrupted by eustatic sea-level fluctuations during the Plistocene. The Great Meteor is also capped by a sedimentary section around 400 m in thickness (Hinz, 1969). In these areas the sediments mainly comprise carbonated biogenic remains, with very low sedimentation rates. For the last 450,000 years, the pelagic sedimentation rate of deep-sea sediments has been calculated to average 0.25–0.6 cm per thousand years (Kuijpers et al., 1984; Brandes, 2011). As a tablemount, the bank is covered by reef sediments and the debris thereof on the slopes. Seismic reflection and refraction profiles indicate that the Great Meteor seamount mainly consists of volcanic rock superimposed by a cap of sediments, probably consisting of biogenic limestones and calcareous sands (Hinz, 1969; von Rad, 1974).

Between the geographical coordinates 30°45'N and 32°50'N and around 28°W lies a complex of seamounts comprising the Cruiser, Irving and Hyeres. Southward of the Cruiser plateau, the Irving seamount is one of three major volcanic peaks: the Hyeres seamount in the southwest (crestal depth 300 m), the large, flat-topped guyot Irving seamount in the north-central area (265 m) and the Cruiser seamount in the northeast (735 m). These seamount crests are mostly unsedimented (Tucholke and Smoot, 1990).

The Cruiser seamount is located to the furthest North-East, with a maximum height of 590 m below sea level. The seamount rises to 735 m, and its length is about 70 km. Cruiser seamount contains no flat surface (Verhoef, 1984).

Irving seamount is situated at about 32°N/28°W. It rises to 250 m below sea level and is a tablemount. The general direction of Irving seamount is NW-SE, but due to its oval shape it is difficult to assign a distinct orientation to this seamount. The length of the structure is about 100 km.

Between Irving and Hyeres seamounts, there are several structures that are not as shallow as the other seamounts. The alignment of these structures is the same as for the other seamounts inside the complex. Hyeres seamount is the most southwestern structure (Verhoef, 1984).

The Hyeres seamount has a recorded minimum depth of 330 m at 31°20'N/28°50'W. The seismic profiles over Hyeres seamount show no flat surface. Coming from the northwest, Hyeres rises abruptly from the ocean floor. It then seems to divide in two branches in the south-east. Hyeres seamount has a length of about 100 km (Verhoef, 1984).

Inside the complex formed by Cruiser, Irving and Hyeres seamounts, several sedimentary basins are to be found (e.g., between Cruiser and Irving seamounts). On several profiles, a sedimentary cover on the seamounts has been recorded (e.g., the profiles over the northwestern part of Irving seamount) (Verhoef, 1984).

Plato seamount is aligned in a general E-W direction. It consists of an echelon structure with a WNW-ESE direction. The overall length of Plato seamount is about 110 km, and the recorded minimum depth is 580 m. Plato seamount forms the connection with another complex structure, the Atlantis seamount group (Verhoef, 1984).

The Atlantis seamount complex consists of several elevations, separated by deep saddles and with a common base at about 2400m. Some summits and slopes have composite relief with hills and peaks measuring 100 to 200 m. Therefore, the horizontal dimensions of these two seamounts on the contour charts are only schematic Studies conducted by Heezen et al. (1969) concluded that Atlantis seamount was an island within the past 12,000 years.

Tyro seamount is situated at 34°40'N/27°30'W with a minimum depth of 1370 m and roughly defined SE direction (Verhoef, 1984).

Seamounts are locations for a broad range of current-topography interactions and biophysical coupling, with implications for both phyto and zooplankton. Seamounts appear to support relatively large planktonic and higher consumer biomass when compared to surrounding ocean waters, particularly in oligotrophic oceans. It has been a widely held view that in situ enhancement of primary production fuels this phenomenon, but this has recently been challenged (Genin & Dower 2007).

Productivity in oceanic settings depends on light and nutrient availability, while overall production is the result of productivity and accumulation of the phytoplankton. At a seamount, either a seamount-generated, vertical nutrient flux must be shallow enough to reach the euphotic zone and the ensuing productivity retained over the seamount long enough to allow transfer to higher trophic levels, or the seamount must rely on allochthonous inputs of organic material to provide a trophic subsidy to resident populations (Clark et al., 2010).

In terms of biology, these structures have not been extensively studied. A total of 437 species have been identified throughout the area (see feature description). Although seamounts are ecologically important and abundant features in the world’s oceans (Hillier & Watts, 2007), biological research on some seamounts has been limited (see Table 1) (Consalvey et al., 2010).

The most detailed investigations on biodiversity, composition and distribution of the seamount benthic macrofauna and meiofauna have been carried out in the North Atlantic, particularly at the Great Meteor seamount (Emschermann, 1971; Grasshoff, 1977; Bartsch, 1973, 2003, 2004, 2008; Hartmann-Schröder, 1979; George & Schminke, 2002; George 2004; Gad 2004, 2009; Gad & Schminke, 2004; Piepenburg & Müller, 2004; Mironov & Krylova, 2006).


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Description of the location
North-East Atlantic Ocean and Adjacent Areas

The area is situated roughly 700 km south of the Azores and about 1500 km northwest of Africa. It has a total area of 134,079 km2, with depths ranging from 265m (top of Atlantis seamount) to 4800m (bottom of Great Meteor seamount). The area is bounded by the parallels 35º30’0,000’’N and 29º12’0,000’’N, and meridians -27º0’0,000’’W and -31º30’0,000’’W.

The polygon is defined by 19 points (see Table 2). The datum used is World Geodetic System 1984 (WGS84).

Table 2 – Geographic coordinates in two different formats: Decimal degrees and Degrees, Minutes and Seconds, corresponding to the vertices of the polygon that defines the Atlantis-Meteor Seamount Complex
Vertices  Latitude                 Longitude                 Latitude                  Longitude
1        31,00000000°        -29,00000000°        31° 0' 0,000" N        -29° 0' 0,000" W
2        31,60000000°        -29,30000000°        31° 36' 0,000" N        -29° 18' 0,000" W
3        32,00000000°        -28,60000000°        32° 0' 0,000" N        -28° 36' 0,000" W
4        32,90000000°        -28,60000000°        32° 54' 0,000" N        -28° 36' 0,000" W
5        33,00000000°        -30,50000000°        33° 0' 0,000" N        -30° 30' 0,000" W
6        34,00000000°        -31,40000000°        34° 0' 0,000" N        -31° 24' 0,000" W
7        35,00000000°        -31,50000000°        35° 0' 0,000" N        -31° 30' 0,000" W
8        35,00000000°        -30,30000000°        35° 0' 0,000" N        -30° 18' 0,000" W
9        34,00000000°        -29,50000000°        34° 0' 0,000" N        -29° 30' 0,000" W
10        34,00000000°        -28,70000000°        34° 0' 0,000" N        -28° 42' 0,000" W
11        35,50000000°        -28,50000000°        35° 30' 0,000" N        -28° 30' 0,000" W
12        35,40000000°        -27,00000000°        35° 24' 0,000" N        -27° 0' 0,000" W
13        33,30000000°        -27,60000000°        33° 18' 0,000" N        -27° 36' 0,000" W
14        32,20000000°        -27,00000000°        32° 12' 0,000" N        -27° 0' 0,000" W
15        30,70000000°        -28,20000000°        30° 42' 0,000" N        -28° 12' 0,000" W
16        29,30000000°        -28,00000000°        29° 18' 0,000" N        -28° 0' 0,000" W
17        29,20000000°        -29,30000000°        29° 12' 0,000" N        -29° 18' 0,000" W

The Atlantis-Meteor Seamount Complex includes 10 seamount structures.

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Area Details

Knowledge of the Atlantis-Meteor Seamount Complex is based on the analysis of 146 scientific articles containing relevant information about the described area. Several of the seamounts are well known, with a great number of geological and biological studies. The total number of 437 species reported was estimated from scattered taxonomical literature, and the species number is probably underestimated. Knowledge of each structure is uneven.

Around of 4 per cent of the 437 species identified in all seamounts on Atlantis-Meteor Seamount Complex are legally protected or assessed as threatened by CITES, IUCN Red List, European Union Habitats and Birds Directives, Food and Agriculture Organization (VMEs), Bern Convention and OSPAR Convention. For example, OSPAR identified as endangered or declining the deep-water sharks Centroscymus coeleopsis and Centrophorus squamosus. Other examples of species with legal protection (CITES Appendix II) are the corals, Antipathella subpinnata, Leiopathes spp., Parantipathes hirondelle, Aulocyathus atlanticus, Caryophyllia abyssorum, Deltocyathus eccentricus, Deltocyathus moseleyi, Dendrophyllia cornigera, Desmophyllum dianthus, Flabellum alabastrum, Flabellum chuni and Lophelia pertusa among others. For example, the species of sea urchin Centrostephanus longispinus is protected by the EU Habitats Directive, and Ranella olearia is protected by Annex II of the Bern Convention.

The species studied in the described area belong to several phyla, classes or orders (Figure 3). The Meteor Seamount includes various species of scleractinians and gorgonians. In some seamounts the gorgonian and sponge species were reported to form dense gorgonian coral habitat-forming aggregations of Callogorgia verticillata and Elisella flagellum, which may represent important feeding and sheltering grounds for seamount fishes and potential shark nurseries (WWF, 2001; Etnoyer & Warrenchuk, 2007; OSPAR, 2011). Cold-water, deep, habitat-forming corals can shelter higher megafauna in association with the corals than other habitats without coral communities (Roberts et al, 2006; Mortensen et al, 2008, Rogers et al, 2008). Seamounts also harbour large aggregations of demersal or benthopelagic fish (Koslow, 1997; Morato & Pauly, 2004; Pitcher et al., 2007; Morato et al., 2009, 2010).

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Most of the study cruises that have visited the described area focus on Great Meteor bank, with sampling of the demersal vertebrate fauna (fish). Most studies are qualitative and often focus on specific taxonomic groups, such as copepods or gastropods (George & Schminke, 2002; Gofas, 2007; Pitcher et al., 2010).

The unique ecosystems of seamounts are highly vulnerable and sensitive to external actions. Most of the fauna found on seamounts are long-lived, slow-growing organisms with low fecundity and natural mortality (Brewin et al., 2007). Fisheries for horse mackerel (Trachurus trachurus, Carangidae), mackerel (Scomber sp., Scombridae), scabbardfish (family Trichiuridae) and orange roughy (Hoplostethus atlanticus) have been operating on the seamounts of the area (Uiblein et al., 1999).

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Morato, T., Kvile, K., Taranto, G., Tempera, F., Narayanaswamy, B., Hebbeln, D., Menezes, G., Wienberg, C., Santos, R. & Pitcher, T. (2013) Seamount physiography and biology in The North-East Atlantic and Mediterranean Sea. Biogeosciences 10(5): 3039–3054. 

Morato, T., Varkey, D., Damaso, C., Machete, M., Santos, M. & Pitcher, T. (2008) Evidence of a seamount effect on aggregating visitors. Marine Ecology Progress Series 357: 23-32.

Mortensen, P., Buhl-Mortensen, L., Gebruk, A. & Krylovab, E. (2008) Occurrence of deep-water corals on the MidAtlantic Ridge based on MAR-ECO data. Deep-Sea Research II 55:142–152

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Pitcher, T., Clark, M., Morato, T. & Watson, R. (2010) Seamount fisheries: Do they have a future?. Oceanography 23: 134–144.

Pitcher, T., Morato, T., Hart, P., Clark, M., Haggan, N. & Santos, R. (2007) Seamounts: Ecology, Fisheries, and Conservation, Blackwell Fisheries and Aquatic Resources Series, Vol. 12, Blackwell Publishing, Oxford, 527 pp.

Porteiro, F. & Sutton, T. (2007) Midwater fish assemblages and seamounts. In: Pitcher, T.J., T. Morato, P.J.B. Hart, M.R. Clark, N. Haggan and R.S. Santos (Eds) Seamounts: Ecology, Fisheries & Conservation. Fish and Aquatic Resources Series 12, Blackwell Publishing, Oxford, United Kingdom. pp. 101–16.

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EN
Status of submission
Areas described as meeting EBSA criteria that were considered by the Conference of the Parties
  • 15/25
Assessment of the area against CBD EBSA criteria
C1: Uniqueness or rarity High

The fish Protogrammus sousai (Callionymidae) is endemic to Great Meteor Seamount (Uiblein et al., 1999), as is the antipatharian (Leiopathes montana) (Molodstova, 2011). The Atlantis Seamount has strong effects on the composition of the mesopelagic fish community (Pusch et al., 2004).

The fish fauna are ecologically distinct, with some evidence of morphologic adaption of certain fish populations (e.g., Phycis phycis) to the special food-poor conditions at the seamount (Uiblein et al., 1999).

Meiofaunal groups of copepods and nematodes exhibit pronounced endemism, e.g., 54 of 56 observed species of the copepod Harpacticoida are new to science (George and Schminke, 2002).

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C2: Special importance for life-history stages of species High

Atlantis and Great Meteor Banks are vital stopping points for certain migratory species of whales and cetaceans, including sperm whales (e.g., Physeter microcephalus), fin whales (e.g., Balaenoptera acutorostrata), striped (e.g., Stenella coeruleoalba) and bottlenose dolphins (e.g., Tursiops truncatus).

The seamounts support many species of seabirds that use these places to feed; tracking data reveal the occurrence of at least 11 species using the area during breeding and/or the non- breeding seasons e.g., Calonectris borealis,Puffinus lherminieri baroli – an OSPAR listed species – and the threatened Rissa tridactyla, Pterodroma deserta and Pterodroma madeira (BirdLife International  2019).

There is a blue shark nursery in the Central North Atlantic, roughly delimited by the Azoresarchipelago in the North and the Atlantis-Meteor Seamount Complex in the South (Vandeperre et al., 2014)

The aggregation of commercially important fish species in this area use this ecosystem for spawning and as nursery grounds (e.g., Aphanopus carbo, Beryx splendens, Zenopsis conchifer) (Uiblein et al., 1999).

There is evidence for mid-latitude foraging in central North Atlantic waters for fin and blue whales migrating to the northern feeding sites. More importantly, these species can suspend their seasonal migration and remain foraging in middle latitude areas for extended periods of time and much later into the summer than generally assumed (Silva et al., 2013).

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C3: Importance for threatened, endangered or declining species and/or habitats High

Around 4 per cent of the species identified in Atlantis-Meteor Seamount Complex  are legally protected or assessed as threatened by  CITES (e.g., Antipathes furcata, Leiopathes spp., Parantipathes hirondelle, Desmophyllum dianthus, etc), European Union Habitats (e.g., Centrostephanus longispinus), Bern Convention (e.g., Ranella olearium) or OSPAR Convention (e.g., Centroscymnus coelolepis) (see “feature description of the area”).

Tracks of the loggerhead turtle (Caretta caretta), which is protected by CITES, indicate their use of seamount as habitat (Pitcher et al., 2010).

Atlantis seamount and Meteor Bank are vital stopping points for certain migratory species of whales and cetaceans, including sperm whales (e.g., Physeter microcephalus), fin whales (e.g., Balaenoptera acutorostrata), striped (e.g., Stenella coeruleoalba) and bottlenose dolphins (e.g., Tursiops truncates, Romagosa et al., 2009).

Some globally threatened seabird species are also known to occur in the area, such as Rissa tridactyla (VU), Pterodroma deserta (VU) and Pterodroma madeira (EN), along with the OSPAR listed Puffinus lherminieri baroli (BirdLife International 2019).

Blue shark (Prionace glauca) is on the IUCN Red List as a threatened species. As the seamount complex is confirmed as a nursery, it is of paramount importance to the species (Stevens, 2009).

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C4: Vulnerability, fragility, sensitivity, or slow recovery High

These seamounts host unique marine ecosystems, supporting fragile habitats and vulnerable species like habitat-forming sponges and cold-water corals (e.g., Madrepora oculata). Some of these species exhibit extremely slow recovery, such as the black corals (Leiopathes spp.); the age of some specimens in this part of the Atlantic was approximated to be >2000 yrs (Carreiro-Silva et al., 2012).

In the Atlantis-Meteor Seamount Complex, at least 35 species of cold-water corals have been reported (e.g., Antipathella subpinnata; Parantipathes hirondelle, Leiopathes montana, Caryophyllia smithii; Dendrophyllia cornigera, Flabellum macandrewi). All these corals are particularly fragile and recover very slowly (Molodtsova, 2006; Rogers et al., 2007; Molodtsova, 2011).

Presence of species with some legal protection with characteristic features particularly attending to biological factors, such as longevity, low fecundity, and slow growth rates (e.g., sharks and rays) (e.g., Clark, 2001; Morato et al. 2008). Twenty-two species of sharks and rays (e.g., Dalatias licha (shark), Raja clavata (ray)) are reported in this area (see Figure 5).

Long-lived and slow-growing orange roughy (Hoplostethus atlanticus), one of the longest-lived fish species known, with an estimated life span of more than 130 years, is reported in deep waters, over steep continental slopes, ocean ridges and seamounts south of Azores, including Atlantis-Meteor Seamount Complex (Allain & Lorance, 2000).

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C5: Biological productivity Medium

Productivity of the area in general is characterized as low; however, physical oceanography of seamounts leads to enhanced productivity in seamount areas. A circulation system, in the form of an anticyclonic vortex reported atop the Atlantis-Meteor Seamount Complex, has the potential to accumulate mesopelagic zooplankton, micronekton, and even fish species with weak swimming capabilities (Boehlert & Mundy, 1993; Dong et al., 2007).

Studies with plankton prove that the Atlantis-Meteor Seamount Complex (Mouriño et al., 2001; Beckmann & Mohn, 2002; Fock et al., 2002; Martin & Nellen, 2004; Morato et al., 2013) has a relatively high biological productivity.

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C6: Biological diversity High

These structures, like other seamounts, have been conceptualized as habitat “islands” in the deep-sea. The Atlantis-Meteor Seamount Complex structures have high species diversity, with 437 different species registered, some of which are new to science (e.g., George, K. & Schminke, 2002; George, 2004)

The structures also host large aggregations of demersal or benthopelagic fish (see, e.g., Uiblein et al.,1999; Mironov & Krylova, 2006)

In the Atlantis, Hyeres and Irving seamounts, as well as the Meteor banks there is evidence of a great diversity, with records of midwater fish as major predators of zooplankton, such as the highly abundant and very common species, snipefish (Macroramphosus scolopax), seabass (Anthias anthias), boarfishes (Capros aper and Antigonia capros), flatfish (Arnoglossus rueppelli) and aulopid (Aulopus filamentosus). Also, there is presence of corals (e.g., Antipathella subpinnata, Parantipathes hirondelle, Leiopathes spp.), hydroids (e.g., Acryptolaria conferta), echinoderms (e.g., Centrostephanus longispinus), molluscs (e.g., Dermomurex gofasi) and sponges (e.g., Craniella longipilis). These kinds of species often form extensive reef-like structures, which themselves provide a diverse habitat for other animals, for example Cephalopoda (e.g., Ornitoteuthis antillarum, Tremoctopus violaceus) and Elasmobranchii (Heptranchias perlo).

Atlantis seamount and those of the Meteor bank are vital stopping points for certain migratory species of whales and cetaceans, including sperm whales (e.g., Physeter microcephalus), fin whales (e.g., Balaenoptera acutorostrata), striped (e.g., Stenella coeruleoalba) and bottlenose dolphins (e.g., Tursiops truncatus). The seamounts of Meteor Bank receive many species of seabirds that use these places to feed (e.g., Calonectris diomedea, Oceanodroma castro, Puffinus myasthenia). Loggerhead turtle (Caretta caretta) tracks indicate use of seamount as habitat (Pitcher et al., 2010).

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C7: Naturalness Medium

This is an FAO Fishing Area (No. 27 / No. 34). The fisheries for horse mackerel (Trachurus trachurus, Carangidae), mackerel (Scomber sp., Scombridae), scabbardfish (family Trichiuridae) and orange roughy (Hoplostethus atlanticus) have been operating in the seamounts (Uiblein et al., 1999).

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