Viedma (volcano)

Last updated
Viedma
Tierra del Fuego location map.svg
Red triangle with thick white border.svg
Viedma
Highest point
Elevation 1,500 m (4,900 ft) [1]
Coordinates 49°22′S73°19′W / 49.367°S 73.317°W / -49.367; -73.317 Coordinates: 49°22′S73°19′W / 49.367°S 73.317°W / -49.367; -73.317 [2]
Geography
Location Argentina/Chile
Parent range Andes
Geology
Mountain type Subglacial volcano
Last eruption November 1988 [1]

Viedma (Spanish pronunciation:  [ˈbjeðma] ) is a subglacial volcano located below the ice of the Southern Patagonian Ice Field, an area disputed between Argentina and Chile. The 1988 eruption deposited ash and pumice on the ice field and produced a mudflow that reached Viedma Lake. [1] The exact position of the edifice is unclear, both owing to the ice cover and because the candidate position, the "Viedma Nunatak", does not clearly appear to be of volcanic nature. Numerous ash layers in the Viedma lake indicate numerous past eruptions. [3]

Contents

Geography and geomorphology

Viedma is located in the southern Patagonian Andes, [4] southwest of Mount FitzRoy. [5] The lake of the same name lies southwest of the volcano. The area is poorly accessible [2] and the volcanic history poorly known. [4]

Viedma is part of the Austral Volcanic Zone. [2] This volcanic zone consists of six volcanoes, from north to south Lautaro, Aguilera, Viedma, Reclus, Monte Burney and Fueguino. [4] These volcanoes form a 700 kilometres (430 mi) long chain of volcanoes, the most southern of which is a volcanic complex of lava domes and lava flows on Cook Island. [6]

Few things are known with certainty about the volcanic edifice of Viedma as it is mostly buried beneath glacial ice. [7] In 1956 Louis Lliboutry proposed that volcanic activity may occur in fissure vents buried beneath glaciers; between eruptions they would be concealed below the ice; [8] Lliboutry considered dark bands on the ice to be tephra deposits, a view supported by a 1958-1959 expedition that found pumice on the Viedma Glacier. [9] Other reports of volcanic phenomena in the region exist, and the existence of a large caldera beneath the Southern Patagonian Ice Field has been suggested as an explanation for volcanism there. [10]

Viedma Nunatak

The Viedma Glacier and the Viedma Nunatak (centre-right) Viedma volcanic complex.jpg
The Viedma Glacier and the Viedma Nunatak (centre-right)

The Viedma Nunatak is commonly interpreted to be the site of the volcano, [11] after observations made in 1944-1945 and 1950 by survey flights including controversial sightings of fumaroles which also led to the nunatak becoming known as the "Volcan Viedma"; [12] [8] but the lack of clear evidence [10] and the difficulty of field sampling has rendered its identification with the Viedma vent contentious. [11]

The nunatak is about 1,500 metres (4,900 ft) high above sea level. Most of the mountain is buried beneath the Viedma Glacier of the Southern Patagonian Ice Field and only parts of it crop out. [2] The outcropping nunatak is elongated in north-south direction. [13] A number of structures interpreted as craters and concave depressions are found especially on the southern part of the volcano, some of which are lined up in north-south direction. The northern sector of the volcano was apparently more heavily affected by glacial erosion; conversely, several craters in the southern sector appear to be young. [14] The nunatak shows clear evidence of glacial action, including glacial striations and coverage by glacial drifts; the Viedma glacier may once have crossed the nunatak in its central part. [15] Rock samples taken from the nunatak are Jurassic metamorphic rocks, including gneiss and schists, [11] and no evidence of magmatic rocks was found in a 1958-1959 expedition. [9]

Different observations have yielded different sizes and numbers of supposed craters; González-Ferrán et al. 1995 reported several craters and calderas with sizes ranging 1.5–4 kilometres (0.93–2.49 mi), while Kobayashi et al. 2010 observed fewer craters and none of them larger than 1.5 kilometres (0.93 mi). [14] These craters were later interpreted as being actually glacial cirques containing tarn lakes. [15]

Geology

Map of the volcanic zones arcs in the Andes, and subducted structures affecting volcanism MAGMAARC1.jpg
Map of the volcanic zones arcs in the Andes, and subducted structures affecting volcanism

Off the southernmost west coast of South America, the Antarctic Plate subducts beneath the South American Plate at a rate of 3 centimetres per year (1.2 in/year). [16] This subduction process is responsible for volcanism in the Austral Volcanic Zone. [17] The Austral Volcanic Zone is one of four volcanic zones in the Andes, the other three are the Northern Volcanic Zone, the Central Volcanic Zone and the Southern Volcanic Zone, all of which are separated from the Austral Volcanic Zone and each other by gaps where no volcanic activity occurs. Unlike the Austral Volcanic Zone, volcanism in these other zones is controlled by the subduction of the Nazca Plate beneath the South American Plate. [18]

The Austral Volcanic Zone was identified as such in 1976, but some volcanoes were identified and localized later. Owing to their similar composition the three northerly volcanoes Lautaro, Viedma and Aguilera are grouped as the "northern Austral Volcanic Zone". Volcanism in the Austral Volcanic Zone is not well known before the Holocene; it is likely that a lull of volcanism occurred before the Pliocene while the Chile Triple Junction was being subducted in the region. Magmas from the Austral Volcanic Zone are adakitic owing to the melting of the subducting slab and the interaction of these melts with the crust and mantle. [18]

The basement consists of metamorphic rocks of Paleozoic age. Outcrops of the basement are found around the volcano and could even occur on the edifice that crops out from the glaciers. [19] The regional basement is formed by these Paleozoic and younger metamorphic and sedimentary rocks as well. [18]

Composition

Viedma like other volcanoes of the Austral Volcanic Zone has erupted andesite and dacite. Phenocrysts include amphibole, biotite, hypersthene and plagioclase; orthoclase, plagioclase and pyroxene also occur as xenoliths. The rocks form a calcalkaline suite, [20] but there is also an adakitic signature. [2] The xenoliths may reflect a crustal contamination of the magma erupted at Viedma. [20]

Eruption history

Tephra attributed to Viedma has been found in the Laguna Potrok Aike, [21] including three tephra layers 26,991 - 29,416, 40,656 - 48,219 and 41,555 - 57,669 years before present which may originate either on Viedma or on Lautaro. [22]

Viedma has erupted during the Holocene; [7] a tephra found in Lago Cardiel and dated 3,345 - 3,010 years before present may have originated at Viedma, although Aguilera and Lautaro are also candidate source volcanoes. [23]

Historical

Many observations referring to volcanic activity on the Southern Patagonian Ice Field exist, including reports of ashfalls, layers of tephra on glaciers and columns of smoke rising from the ice. [8]

A subglacial eruption occurred in 1988, depositing ash and pumice on the Viedma Glacier. These materials later gave rise to a lahar. [2] The eruption had melted part of the ice and formed a network of valleys; it was assumed that it had taken place at some point between September and November of that year. [24]

Hazards

There are no major population centres close to any volcano in the Austral Volcanic Zone, and the volcanoes are largely unmonitored. Among the know eruptions are large Holocene explosive eruptions, while historical eruptions took place in 1908 at Reclus and 1910 at Monte Burney. [6] Future eruptions of volcanoes in the Austral Volcanic Zone may lead to ash fall at large distances from the volcano, including interruptions in air traffic and direct ash damage. [25]

See also

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References

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  2. 1 2 3 4 5 6 Kobayashi et al. 2010, p. 434.
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  7. 1 2 Perucca, Alvarado & Saez 2016, p. 553.
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  14. 1 2 Kobayashi et al. 2010, p. 435.
  15. 1 2 Blampied et al. 2012, p. 381.
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  19. Kobayashi et al. 2010, p. 438.
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Sources