Vema Seamount is a seamount in the South Atlantic Ocean. Discovered in 1959 by a ship with the same name, it lies 1,600 kilometres (1,000 mi) from Tristan da Cunha and 1,000 kilometres (620 mi) northwest of Cape Town. The seamount has a flat top at a mean depth of 73 metres (40 fathoms) which was eroded into the seamount at a time when sea levels were lower; the shallowest point lies at 26 metres (14 fathoms) depth. The seamount was formed between 15-11 million years ago, possibly by a hotspot.
The seamount rises high enough that its summit is at shallow depth, allowing sunlight to reach it and thus permitting the growth of kelp and algae. A number of sea animals and fish are encountered on the seamount; active fisheries existed at Vema Seamount and caused the disappearance of some animal species.
History
Vema Seamount was discovered by the research ship RV Vema of the Lamont–Doherty Earth Observatory in 1959.[1][2] Vema was one of the first seamounts to be the subject of scientific study,[4] and the first seamount investigated by scuba divers without special equipment.[5] It lies in international waters[6] and its summit is so shallow that it is a navigation hazard to ships.[7]
The seamount has a conical shape with a flat top; the shallowest point rises to an elevation of 26 metres (14 fathoms) below sea level[1][2] - later determined to be 21.5 metres (71 ft) deep -[11] and is called Collins Point.[12] At least one source gives a minimum depth of 11 metres (36 ft) for the seamount,[13] while recent bathymetric surveys have found a minimum depth of 21.5 metres (71 ft).[14] The flat top is a summit plateau with a width of 8.0 kilometres (5 mi)[2] and as more recently determined 11 by 8.5 kilometres (6.8 mi × 5.3 mi)[14] at a mean depth of 73 metres (40 fathoms)[3] and has been named Emerson Plateau; it has a vaguely triangular shape pointing west, and Collins Point lies close to the western margin of the Emerson Plateau. Other points on the Plateau also rise to depths of less than 55 metres (30 fathoms).[12] The summit plateau mostly consists of hard rock, like the upper slopes,[11] with rocky outcrops separated by sandy plains.[15] The plateau appears to be a wave-cut platform of Pleistocene age, when sea levels were lower,[3] and is swept by strong ocean currents.[16]
The seamount rises from a depth of 4,600 metres (2,500 fathoms), where it occupies a breadth of 56 kilometres (35 mi)[2] and forms an isolated conical feature.[14] The seafloor from which Vema rises is part of the abyssal plain of the Cape Basin.[1] From there, the slopes of Vema first rise steeply and feature subsidiary summits; above 130 metres (70 fathoms) depth the slopes flatten.[3]
Geology
Volcanic rocks such as tuff as well as calcareous aggregates are found on the plateau. Collins Point is composed of phonolite, which contains aegirine, alkali feldspar, augite and nepheline. Olivine-containing basalt has also been found.[3] A minimum age of 11.0 ± 0.3 million years has been obtained from samples taken at Collins Point by potassium-argon dating,[3] with another age estimate being 15 million years.[17] Older ages have been obtained deeper on the seamount; a sample from 3,000 metres (9,800 ft) depth gave an age of 18 million years.[18] Light-coloured rocks on the summit platform may constitute a former carbonate platform.[19]
Vema is an intraplate volcano.[17] It is considered to be the present-day location of a hotspot, the Vema hotspot,[20] although the hotspot itself may have moved farther south[21] or west (by about 200 kilometres (120 mi)) since when it created the Vema Seamount[22] and may not be active anymore.[23] Earlier volcanism[a] caused by the Vema hotspot may have manifested itself in southern Namibia in the form of alkaline volcanics[29] that define a HIMU[b] suite.[24]
Seismic tomography has shown what may be a mantle plume underneath Vema,[30] another theory considers the Vema hotspot is a consequence of the Tristan hotspot shedding a secondary diapir.[31] The hotspot origin of the Vema Seamount is not universally agreed upon.[32]
Water conditions
Water temperatures at Vema range between 18–21 °C (64–70 °F),[33] and decrease with increasing depth.[14] The cold Benguela Current does not reach the seamount,[5] which is instead influenced by the South Atlantic oceanic gyre.[34] The movement and strength of ocean eddies are altered when they interact with Vema Seamount,[35] with Agulhas eddies often splitting apart at the seamount.[36] During the ice ages, sea level drop may have exposed part of the summit platform.[37]
Biology
The seamount features both shallow-water and deep-water life.[38] Its summit is shallow enough that sunlight can reach it, resulting in the growth of various types of algae and seaweeds such as Eckloniakelp.[3] Such kelp covers large parts of the seamount,[39] and a coral framework makes up much of the summit platform.[11]
A number of fish have been encountered at Vema, although most fish species appear to be pelagic species that are not directly bound to the seamount environment.[43] Fishing operations have attracted seabirds to Vema Seamount.[52]Humpback whales have been detected through their sounds,[53] and baleen whales feed at Vema.[54]Euphausiids and copepods are also found in the waters,[3] including at least one copepod that parasitizes fish.[55] Among the fish species encountered at Vema Seamount are:
Fish on the seamount were commercially fished.[3][c] Rock lobsters in particular were heavily exploited;[43] they disappeared from Vema Seamount after overfishing in the 1960s, briefly recovered and then disappeared again by 1981 due to renewed overfishing.[16][9] The collapse of this fishery is one of the first instances of a seamount fishery collapsing,[64] and has been cited as an example of how fisheries outside of exclusive economic zones end up ungoverned and abused.[65] Vema Seamount was closed to fishery in 2007[38] by the South East Atlantic Fisheries Organisation,[66] and man-made debris such as crab traps[67] and ropes can be found there.[68] The ecosystem is classified as "threatened" by the Food and Agriculture Organization.[38]
Notes
^Including the Gibeon kimberlites and carbonatites[24] (79–72 million years old), the 77 ± 2 million years old Gross Brukkaros, the 49 ± 1 million years old Dicker Willem carbonatites[25] (and associated Tsirubnephelinites[26]), the 46 million years old Klinghardt phonolites, the 37 million years old Swartkop phonolite and the 36 million years old Schwarzeberg nephelinite.[25] Other potential correlates are the melilites close to the mouth of the Orange River, which are 37 million years old,[27] or even the Karoo-Ferrarlarge igneous province.[28]
^Duncan, R. A.; Hargraves, R. B.; Brey, G. P. (2009). "Age, palaeomagnetism and chemistry of melilite basalts in the Southern Cape, South Africa". Geological Magazine. 115 (5): 325. doi:10.1017/S001675680003733X. ISSN1469-5081. S2CID129247512.
^Matano, R. P.; Beier, E. J. (1 December 2002). "On the mesoscale dynamics of the Indian/Atlantic interocean exchange". AGU Fall Meeting Abstracts. 22: OS22E–03. Bibcode:2002AGUFMOS22E..03M.
^Giulivi, Claudia F.; Gordon, Arnold L. (August 2006). "Isopycnal displacements within the Cape Basin thermocline as revealed by the Hydrographic Data Archive". Deep Sea Research Part I: Oceanographic Research Papers. 53 (8): 1292. Bibcode:2006DSRI...53.1285G. doi:10.1016/j.dsr.2006.05.011. ISSN0967-0637.
^Salisbury, Richard (11 August 2015). "A new (Gastropoda: Costellariidae) from the Vema Seamount in the South Atlantic Ocean". Proceedings of the Academy of Natural Sciences of Philadelphia. 164 (1): 17. doi:10.1635/053.164.0104. S2CID128660650.
^Thandar, Ahmed S. (May 1988). "A new subgenus of Holothuria with a description of a new species from the south-east Atlantic Ocean". Journal of Zoology. 215 (1): 50. doi:10.1111/j.1469-7998.1988.tb04884.x.
^De Villiers, J. S.; Edwards, K. Z.; Grindley, J. R.; Lawson, W. J.; Winterbottom, J. M.; Siegfried, W. R.; Payne, R. B.; Payne, Robert B.; Payne, Karen; Steyn, P.; Steyn, P.; Steyn, P.; Steyn, P.; Steyn, P.; Tredgold, D.; Steyn, P.; Tredgold, D.; Every, B.; Ferguson, J. W. H.; Brooke, R. K.; Markus, M. B.; Markus, Miles B.; Tree, A. J.; Tree, A. J.; Clancey, P. A.; Jensen, R. A.C.; Jensen, M. K.; Donnelly, B. G.; Donnelly, B. G.; Vernon, C. J.; Vernon, C. J.; Vernon, C. J.; Mcculloch, D.; Siegfried, W. R.; Grindley, J. R. (December 1967). "SHORT NOTES". Ostrich. 38 (4): 281. Bibcode:1967Ostri..38..281D. doi:10.1080/00306525.1967.9634715.
^Anderson, William D.; Murdy, Edward O. (October 2006). "Meganthias carpenteri, new species of fish from the eastern Atlantic Ocean, with a key to eastern Atlantic Anthiinae (Perciformes: Serranidae)". Proceedings of the Biological Society of Washington. 119 (3): 411. doi:10.2988/0006-324X(2006)119[404:MCNSOF]2.0.CO;2. S2CID85822828.
^Andrew, Timothy G.; Buxton, Colin D.; Hecht, Thomas (1 June 1996). "Aspects of the reproductive biology of the concha wrasse, Nelabrichthys ornatus, at Tristan da Cunha". Environmental Biology of Fishes. 46 (2): 139. Bibcode:1996EnvBF..46..139A. doi:10.1007/BF00005215. ISSN0378-1909. S2CID39535647.
Berrisford, C. D. (January 1969). "Biology and Zoogeography of the Vema Seamount: A Report on the First Biological Collection Made on the Summit". Transactions of the Royal Society of South Africa. 38 (4): 387–398. Bibcode:1969TRSSA..38..387B. doi:10.1080/00359196909519099.
Edwards, A.J. (17 February 2007). "New records of fishes from the Bonaparte Seamount and Saint Helena Island, South Atlantic". Journal of Natural History. 27 (2): 493–503. doi:10.1080/00222939300770241.
Mark A. Richards, Richard G. Gordon, Rob D. van der Hilst (2000). The history and dynamics of global plate motions. Washington, DC: American Geophysical Union. ISBN9781118668535.{{cite book}}: CS1 maint: multiple names: authors list (link)