Purico complex

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The Purico complex is a Pleistocene volcanic complex in Chile close to Bolivia, formed by an ignimbrite, several lava domes and stratovolcanoes and one maar. It is in the Chilean segment of the Central Volcanic Zone, one of the four volcanic belts which make up the Andean Volcanic Belt. The Central Volcanic Zone spans Peru, Bolivia, Chile and Argentina and includes 44 active volcanoes as well as the Altiplano–Puna volcanic complex, a system of large calderas and ignimbrites of which Purico is a member. Licancabur to the north, La Pacana southeast and Guayaques to the east are separate volcanic systems.

The Purico complex consists of a shield shaped volcanic structure consisting of the Purico ignimbrite and a number of secondary volcanoes that are emplaced on this volcanic shield. During the ice ages, the shield was in part covered by glaciers which have left moraines. Purico is the source of the Purico ignimbrite, which has a volume of about Script error: No such module "convert".. After the emplacement of the Purico ignimbrite, a number of lava domes and stratovolcanoes developed on the ignimbrite shield. The maar of Alitar is still fumarolically active. In historical times, sulfur was mined on Purico. Today, the Llano de Chajnantor Observatory lies on the ignimbrite shield.

Geography and structure

The Purico complex lies in Chile close to the border between Bolivia and Chile,Template:Sfn east of the town of San Pedro de AtacamaTemplate:Sfn and northeast of Toconao.Template:Sfn The volcanic complex can be seen from San Pedro de Atacama.Template:Sfn A road runs along the northern and eastern margin of the Purico complex,Template:Sfn and a gas pipeline crosses the complex as well.Template:Sfn The existence of the Purico complex was established on the basis of Landsat images.Template:Sfn

Regional

Licancabur volcano was constructed on ignimbrites from Purico[1] just north of the complex.Template:Sfn Guayaques lies east of Purico,Template:Sfn the La Pacana caldera is located southeast of the complex, and La Pacana's Filo Delgado ignimbrite has buried part of the Purico ignimbrite.Template:Sfn The known volcanoes Lascár and El Tatio are found at larger distances from Purico.Template:Sfn

Purico is part of the Central Volcanic Zone (CVZ), a belt of volcanoes that runs along the western margin of South America between 14° and 28° southern latitude.Template:Sfn This Script error: No such module "convert". long beltTemplate:Sfn is one of four separate volcanic belts that make up the Andean Volcanic Belt. They are separated from each other by gaps where no recent volcanism occurs. The CVZ segment includes 44 active systems, 18 minor volcanic centres and over 6 large ignimbrite or caldera systems. One of these volcanoes, Ojos del Salado, is the highest volcano in the world. The largest historical eruption in the CVZ occurred in 1600 at Huaynaputina in Peru[2] while Lascár is its most active member, with a major eruption in 1993.Template:Sfn

Local

File:A view across the plains of Chajnantor with the ALMA construction site at the centre.jpg
A view across the Purico complex
File:Chajnantor2004.jpg
The Purico shield seen from Cerro Toco

Purico is a circular shield with a diameter of Script error: No such module "convert"., whose slopes descend away from a centre at an elevation of Script error: No such module "convert"..Template:Sfn This shield forms a plateau, which is known as the ChajnantorTemplate:Efn Plateau,Template:Sfn and which contains further flat areas such as Llano de Chajnantor, Pampa El Vallecito and Pampa La Bola.[3] There is no evidence that a caldera exists there, unlike in many other volcanoes of this type.Template:Sfn To the west, close to the margin of the Salar de Atacama, the shield drops down to a bajadaTemplate:Efn.Template:Sfn A north-south trending system of fractures and conspicuous normal faults cuts across the western margin of the Purico complex.[4]

On top of this shield, a complex of lava domes and lavas reaches elevations of over Script error: No such module "convert". above sea level;Template:Sfn the vent of the ignimbrite may be buried beneath this complex.Template:Sfn This complex forms approximately a Script error: No such module "convert". wide semicircle open to the southwest around the centre of the shield,Template:Sfn which may reflect the existence of a ring fault on which the individual centres were emplaced.[5]

Clockwise starting from the west this semicircle includes Script error: No such module "convert". high Cerro Negro (Script error: No such module "Coordinates".), Cerro Purico, "dacite dome D" and Script error: No such module "convert". high El Cerillo which is also known as Cerro Chajnantor (Script error: No such module "Coordinates".), Script error: No such module "convert". high Cerro El Chascon (Script error: No such module "Coordinates".), the Script error: No such module "convert". high Cerro Aspero (Script error: No such module "Coordinates". and the Script error: No such module "convert". high Cerro Putas (Script error: No such module "Coordinates".) to the south. All these domes (with the exception of the pancake-like "dacite dome D") have conical shapes, and Aspero, El Cerillo and El Chascon appear to be post-glacial in age.[6]Template:Sfn

The Chascon dome is constructed by lava flows and has a well preserved summit crater,[5] while Cerro Purico is a stratovolcano and also known as Cerro Toco (Script error: No such module "Coordinates".).[6] Additional more subdued structures in the principal complex are Script error: No such module "convert". high Cerro Agua Amarga (Script error: No such module "Coordinates".) just southwest of El Chascon and the Cordon Honor with Cerro Purico Sur in the "opening" of the semicircle.Template:Sfn[6] Lahars and debris flows from the volcanoes have covered parts of the ignimbrite shield with gravels.Template:Sfn A meltwater-fed spring on Cerro Toco is known as Aguada Pajaritos, and a small lake Laguna de Agua Amarga is found south of Chascon.Template:Sfn Presently, the Purico complex forms the drainage divide between the Salar de Atacama and the Salar de Pujsa.[7] The Script error: No such module "convert". high Macon stratovolcano (Script error: No such module "Coordinates".), Alitar maar (Script error: No such module "Coordinates".) and Script error: No such module "convert". high Alitar volcano (Script error: No such module "Coordinates".) lie to the south of the main complex.[5][6]Template:Sfn Alitar maar is located is Script error: No such module "convert". wide and Script error: No such module "convert". deep.Template:Sfn

File:Purico complex seen from nnw from toco to laguna verde chile ii region.jpg

Geology

West of South America, the Nazca Plate subducts beneath the South America PlateTemplate:Sfn at rates of Script error: No such module "convert".. This subduction process along with that of the Antarctic Plate beneath the South American Plate farther south is responsible for volcanism in the Andean Volcanic Belt.[2]

Volcanic activity in the region of the Central Volcanic Zone has been ongoing for 200 million years, but with temporal and local variations; 25 million years ago for example it was centered farther east and later moved west.Template:Sfn About 23 million years ago, large scale ignimbritic activity commenced in the region with the emplacement of the Oxaya Formation, followed by the Altos de Pica Formation 17-15 million years ago. However, effusive activity of andesitic composition dominated volcanism until the late Miocene.Template:Sfn

Regional

Purico appears to be part of a group of large, caldera-forming volcanic centres that erupted dacitic ignimbrites, a group that is known as the Altiplano-Puna volcanic complex. This group includes the Cerro Guacha, Cerro Panizos, Coranzulí, La Pacana, Pastos Grandes and Vilama centres that cluster around the tripoint between Argentina, Bolivia and Chile.Template:Sfn The arid climate of this region means that most volcanic systems are well preserved with little erosion.Template:Sfn

This complex is underpinned by a magma body at depths of Script error: No such module "convert"., where arc magmas interact with the crust to form the secondary magmas later erupted by the volcanoes of the Altiplano-Puna volcanic complex.Template:Sfn This magma body has been imaged with seismic tomography as a sill-like body and has been named the "Altiplano-Puna magma body".Template:Sfn

Ignimbritic activity in such systems is episodic, being interrupted by periods with lower volume "steady state" volcanism.Template:Sfn The eruption of the Purico ignimbrite is the youngest large ignimbrite eruption in the Altiplano-Puna volcanic complex;Template:Sfn the Altiplano-Puna volcanic complex presently is in such a "steady state" stage,Template:Sfn but the presence of active geothermal system indicates that magmatic activity is still ongoing.Template:Sfn

Local

Outcrops in the region range in age from Paleozoic to Holocene.Template:Sfn The Purico complex formed on top of older ignimbrites such as the Puripicar ignimbrite in the north, the AtanaTemplate:Sfn and the La Pacana ignimbrites farther south.Template:Sfn The neighbouring La Pacana caldera between 4.5 and 4.1 million years ago erupted some of these ignimbrites including the Atana ignimbrite.Template:Sfn Occasionally Purico is considered part of the La Pacana system.Template:Sfn[8]

Composition

The Purico complex has erupted various different magmas, ranging from the dacitic Purico ignimbriteTemplate:Sfn over rhyolitic pumices contained in the ignimbriteTemplate:Sfn to the andesitic-dacitic post-ignimbrite volcanics.Template:Sfn Dacite is the dominant component and forms a crystal-rich potassium-rich suite.Template:Sfn Varying amounts of phenocrysts occur in the Purico complex rocks; the minerals they are formed of include augite, biotite, clinopyroxene, hornblende, hypersthene, iron oxides, oligoclase, orthopyroxene, plagioclase, quartz and titanium oxides.Template:Sfn

Additionally, mafic xenoliths are found in the Purico ignimbrite; such xenoliths are a common finding in volcanic arc rocks.Template:Sfn They are even more common in Chascon rocks, where they might reflect the occurrence of mafic magma in the feeder system prior to the formation of Chascon.Template:Sfn

Some physical properties of the Purico magmas have been inferred from the chemistry and petrology of the erupted rocks. The dacites had temperatures of about Script error: No such module "convert". while the andesites and rhyolites reached higher temperatures, up to Script error: No such module "convert".. Water contents ranged from 3.2 to 4.8% by weight, while carbon dioxide concentrations were low throughout.Template:Sfn

Climate and vegetation

The climate at Purico is cold, with annual mean temperatures of Script error: No such module "convert".;Template:Sfn during summer it hovers around Script error: No such module "convert". and during winter it can decrease to Script error: No such module "convert"..Template:Sfn Because of the high altitude, the air is thinTemplate:Sfn and ultraviolet radiation is high.[9] Llano del Chajnantor features the world's highest insolation,Template:Sfn which under particular meteorological conditions can approach that at Venus.Template:Sfn There is little precipitation in the area (about Script error: No such module "convert". on the upper parts of the shield, decreasing to less than Script error: No such module "convert". close to the Salar de AtacamaTemplate:Sfn), which mainly happens during the summer monthsTemplate:Sfn as a consequence of the South American monsoon.Template:Sfn Snow also falls during winterTemplate:Sfn but winter snow mainly evaporates while summer snow melts.Template:Sfn This dry climate is due to the combined effects of the subtropical ridge, the Humboldt Current in the Pacific Ocean and the rain shadow exercised by the Andes, but it was in the past interrupted by wet periods.Template:Sfn

The dry climate and high elevation mean that vegetation is scarce in the region,Template:Sfn with cacti such as Echinopsis atacamensis and grasses occurring at lower elevations.Template:Sfn The little vegetation that is present displays an altitudinal zonation with a lower "Prepuna" with shrubs and succulents, a middle "Puna" with grasses and shrubs and a "high Andean steppe" with bunch grass. Template:Sfn A report in 1993 stated that red-brown cacti and brown grass grew around the foot of Purico.Template:Sfn Conversely, the soils on the Purico complex contain a diverse population of microbesTemplate:Sfn which have to tolerate extreme environmental conditions.Template:Sfn Among these are the bacteria Amycolatopsis vastitatis,[10] Lentzea chajnantorensis,[11] Micromonospora acroterricola, Micromonospora arida, Micromonospora inaquosa,Template:Sfn Modestobacter altitudinis,[12] Modestobacter excelsi,[13] Nocardiopsis deserti[14] and Streptomyces aridus which were first isolated at the Purico complex.[15] Some of these yield pharmacologically interesting compounds.Template:Sfn

File:Penitentes Chajnantor.jpg
Penitentes on Purico

Increased moisture availability during the ice ages caused the development of glaciers on Purico;Template:Sfn at times, an ice cap with outlet glaciersTemplate:Sfn covered an area of Script error: No such module "convert".Template:Sfn-Script error: No such module "convert". at Script error: No such module "convert". elevation on Purico.[16] Apparently three different stages of glaciation occurred, the third between 30,000–25,000 years ago, the second between 50,000–60,000 years ago and the first over 100,000 years ago.Template:Sfn Moraines associated with Lake Tauca appear to be either small or nonexistent.Template:Sfn These glaciations have left moraines on Purico which extend for many kilometres at altitudes of Script error: No such module "convert"., sometimes descending as far down as Script error: No such module "convert".. The moraines reach heights of Script error: No such module "convert". on the eastern side of Purico and Script error: No such module "convert". on its western side. These moraines are covered with boulders and accompanied by striated surfaces and erratics.Template:Sfn Penitentes still occur on Purico to this day.[17]

Eruptive history

The Purico complex is the source of the major Purico ignimbrite,Template:Sfn which was emplaced at the time of the Jaramillo geomagnetic reversal.[18] It was originally called Cajon ignimbrite and attributed to an area northwest of Purico known as Chaxas. Also, the Toconao ignimbrite was originally attributed to the Purico complex,Template:Sfn but now the La Pacana caldera is considered to be its source.Template:Sfn

The Purico ignimbrite itself covers a surface area of Script error: No such module "convert". over the whole complex, and its volume has been estimated to be Script error: No such module "convert". with an additional Script error: No such module "convert". contributed by tephra fall deposits.Template:Sfn The ignimbrite is Script error: No such module "convert". thick and becomes thinner westward,Template:Sfn with more distal sectors reaching thicknesses of Script error: No such module "convert"..[19] Potassium-argon dating has yielded ages between 1,380,000 ± 70,000 and 870,000 ± 520,000 years ago for the Purico ignimbrite.Template:Sfn The Script error: No such module "convert". large[19] "dacitic dome D" has an age of 980,000 ± 50,000 and may thus have formed at the same time as the ignimbrites.Template:Sfn The emplacement of the Purico ignimbrite was part of a pulse of activity in the Altiplano-Puna volcanic complex 1 million years ago.[20]

The Purico ignimbrite contains three flow units, the two Lower Purico Ignimbrites and the Upper Purico Ignimbrite.Template:Sfn Their thicknesses differ; the Upper ignimbrite is Script error: No such module "convert". thick while the two lower ones together reach an average thickness of Script error: No such module "convert".,Template:Sfn with a maximum of Script error: No such module "convert"..Template:Sfn The lowermost Lower Purico Ignimbrite is one single flow. The upper Lower Purico Ignimbrite is more heterogeneous, starting with a base surge, a pumice layer and then another flow unit,Template:Sfn which is volumetrically the largest part. The Lower Purico Ignimbrite covers a surface of Script error: No such module "convert". primarily on the western side of the Purico complex.Template:Sfn Finally, the Upper Purico Ignimbrite is a moderately to densely welded flow that occurs particularly close to the summit of the Purico complex,Template:Sfn where it forms six flow units that contain fiamme textures.Template:Sfn Characteristic for the Purico ignimbrite is the so-called "banded" pumice, which consist of alternating darker mafic and brighter components, in the upper 33% of the ignimbrite.Template:Sfn The extrusion of the Purico ignimbrite was accompanied by the eruption of large amounts of tephra, some of which fell as far as the Coastal Cordillera west of Purico.[21]

After emplacement, the ignimbrites were modified by fluvial erosion, which formed curvilinear channels in the ignimbrites.Template:Sfn In contrast to other ignimbrites in the region, there is little evidence of eolian erosion of the Purico ignimbrite. Eolian erosion takes much longer than fluvial erosion and it is possible that the Purico ignimbrite is too young to have been modified by wind action.Template:Sfn Some surfaces of the ignimbrite have been affected by glaciation, giving them a smooth surface.Template:Sfn

This structure of the ignimbrite has been explained by magma chamber processes. Prior to the Purico ignimbrite eruption, a dacitic magma chamber already existed beneath the volcano. Probably after an injection of andesitic magma, dacitic contents of the magma chamber escaped upwards and formed the lowermost Lower Purico Ignimbrite. This injection of mafic magma rapidly increased the temperature and gas content of the dacite, causing the eruption to become a violent Plinian eruption with the development of an eruption column. This phase then drew onto denser dacitic magma, causing the column to collapse and the Upper Purico Ignimbrite and the "dacite dome D" to form.Template:Sfn

Post-ignimbrite activity

File:Cerro Toco lies at the northern end of the purico complex chile ii region.jpg
Cerro Toco

Volcanic activity after the eruption of the ignimbrite has been subdivided into the older andesitic Purico group and the younger Chascon group. The first includes Cerro Negro, Cerro Purico, Putas and Cerro Toco which assume the structure of polygenetic volcanoes, while the latter is taken to include Aspero, El Cerillo/Chajnantor and El Chascon which are lava dome-lava flow structures.[22] The Chascon group of domes is also the only one which contains mafic xenoliths.Template:Sfn

The Cerro Purico and Macon volcanoes formed a short time after, and possibly even before, the ignimbrites. They are thus old volcanic centres and deeply eroded, displaying moraine deposits from glaciation and rocks which have been subject to hydrothermal alteration from fumarolic activity.Template:Sfn Such hydrothermal alteration processes,Template:Sfn together with desublimation of fumarolic sulfur, are also the origin of the sulfur deposits at Purico.[23]

Aspero, Cerro El Chascon, Cerros El Negro and Putas are younger and show no evidence of glaciation. El Chascon especially may be only tens of thousands of years old, seeing as it displays both a summit crater and pristine lava flow structures.Template:Sfn Aspero was once considered to be of Holocene ageTemplate:Sfn in light of it and Chascon overlying moraines;[8] later, dates of 180,000 ± 20,000 years ago were obtained on Aspero and Chascon.Template:Sfn Apart from these, there are no radiometric dates for post-ignimbrite volcanic structures at Purico.Template:Sfn The Alitar volcano is considered to be of Plio-Pleistocene age.Template:Sfn The eruptive episode that formed these centres is thus more recent than the Purico ignimbrite and may have been triggered by mafic magma being injected into the Purico system. It is also much smaller, with volumes ranging Script error: No such module "convert"..Template:Sfn

This change in the pattern of eruptive activity from large ignimbrites to smaller domes reflects a change in the nature of the magma supply, from large volume flow that heavily interacted with the crust and gave rise to the ignimbrites to smaller volume flows in a colder and thus brittler crust and did not accumulate or interact with it in a significant way.Template:Sfn Thus the later eruption products appear to be more primitive and less affected by crustal contamination.Template:Sfn

Holocene and fumarolic activity

Macon stratovolcano is considered to be of Holocene age, and Alitar maar displays active fumaroles[5] and hot springs.[24] There are no know historical eruptions of AlitarTemplate:Sfn and there is no indication of seismic activity in the Purico area.Template:Sfn Renewed activity at Alitar would likely be in the form of phreatic eruptions of only local significance.[23]

The fumaroles of Alitar are concentrated in the northern and eastern parts of Alitar, while the hot springs occur in the Quepiaco creek area about Script error: No such module "convert". southwest of AlitarTemplate:Sfn and consist of six separate small vents. Template:Sfn The temperatures of the Alitar vents range between Script error: No such module "convert".. Fumarolic gases are mostly water vapour, with lesser amounts of carbon dioxide,Template:Sfn and sulfur deposition takes place.[23] They appear to originate from both magmatic and precipitation water, with a large contribution from atmospheric airTemplate:Sfn and an important role for a hydrothermal system.Template:Sfn

Other

File:The future ALMA array on Chajnantor.jpg
A CGI of the ALMA telescope site

Purico has been quarried for building materials, and many buildings in San Pedro de Atacama were built from rocks quarried there.Template:Sfn since 1984Template:Dated maintenance category (articles)Script error: No such module "Check for unknown parameters"., Alitar was under investigation as a potential source of geothermal power.[25] Two sulfur deposits occur at Purico,[26] the first southeast of Cerro Toco[27] and the second at Alitar. The Purico deposit in 1968 was estimated to feature 4 million tons of caliche with a grade of 50%, while the Alitar deposit in that year amounted to 1.5 million tons of caliche with a grade of 60%.[26] In the 1950s[23] and as recently as 1993, sulfur was mined on Purico and transported by truck to San Pedro de Atacama where it was processed.Template:Sfn In 1993, production of sulfur amounted to Script error: No such module "convert"..Template:Sfn

The Purico complex is the site of a number of astronomical observatories,Template:Sfn including but not limited to the Llano de Chajnantor Observatory[28] and the Atacama Large Millimeter Array,Template:Sfn and an atmospheric observatory that is among the highest in the world.Template:Sfn In 1998, the Cerro Chascón Science Preserve was established on Purico, which among other things disallows mining in the area of the preserve.[29] This Science Preserve covers most of the Purico complex.[28]

See also

Notes

Template:Notelist

References

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Sources

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Further reading

External links

Template:Andean volcanoes

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