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Volcano
Volcano
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Augustine Volcano (Alaska) during its eruptive phase on January 24, 2006

A volcano is commonly defined as a vent or fissure in the crust of a planetary-mass object, such as Earth, that allows hot lava, volcanic ash, and gases to escape from a magma chamber below the surface.[1]

On Earth, volcanoes are most often found where tectonic plates are diverging or converging, and because most of Earth's plate boundaries are underwater, most volcanoes are found underwater. For example, a mid-ocean ridge, such as the Mid-Atlantic Ridge, has volcanoes caused by divergent tectonic plates whereas the Pacific Ring of Fire has volcanoes caused by convergent tectonic plates. Volcanoes resulting from divergent tectonic activity are usually non-explosive whereas those resulting from convergent tectonic activity cause violent eruptions.[2][3] Volcanoes can also form where there is stretching and thinning of the crust's plates, such as in the East African Rift, the Wells Gray-Clearwater volcanic field, and the Rio Grande rift in North America. Volcanism away from plate boundaries most likely arises from upwelling diapirs from the core–mantle boundary called mantle plumes, 3,000 kilometres (1,900 mi) deep within Earth. This results in hotspot volcanism or intraplate volcanism, in which the plume may cause thinning of the crust and result in a volcanic island chain due to the continuous movement of the tectonic plate, of which the Hawaiian hotspot is an example.[4] Volcanoes are usually not created at transform tectonic boundaries where two tectonic plates slide past one another.

Volcanoes, based on their frequency of eruption or volcanism, are referred to as either active or extinct.[5] Active volcanoes have a history of volcanism and are likely to erupt again while extinct ones are not capable of eruption at all as they have no magma source. "Dormant" volcanoes have not erupted in a long time – generally accepted as since the start of the Holocene, about 12000 years ago – but may erupt again.[5] These categories aren't entirely uniform; they may overlap for certain examples.[2][6][7]

Large eruptions can affect atmospheric temperature as ash and droplets of sulfuric acid obscure the Sun and cool Earth's troposphere. Historically, large volcanic eruptions have been followed by volcanic winters which have caused catastrophic famines.[8]

Other planets besides Earth have volcanoes. For example, volcanoes are very numerous on Venus.[9] Mars has significant volcanoes.[10] In 2009, a paper was published suggesting a new definition for the word 'volcano' that includes processes such as cryovolcanism. It suggested that a volcano be defined as 'an opening on a planet or moon's surface from which magma, as defined for that body, and/or magmatic gas is erupted.'[11]

This article mainly covers volcanoes on Earth. See § Volcanoes on other celestial bodies and cryovolcano for more information.

Etymology and terminology

[edit]

The word volcano (UK: /vɒlˈkeɪnəʊ/; and US /vɔlˈkeɪnoʊ/) originates from the early 17th century, derived from the Italian vulcano, a volcanic island in the Aeolian Islands of Italy whose name in turn comes from Latin volcānus or vulcānus referring to Vulcan, the god of fire in Roman mythology.[12][13] The set of processes and phenomena involved in volcanic activity is called volcanism [Early 19th century: from volcano + -ism]. The study of volcanism and volcanoes is called volcanology [mid 19th century: from volcano + -logy], sometimes spelled vulcanology.[12]

Plate tectonics

[edit]

According to the theory of plate tectonics, Earth's lithosphere, its rigid outer shell, is broken into sixteen larger and several smaller plates. These move continuously at a slow pace, due to convection in the underlying ductile mantle, and most volcanic activity on Earth takes place along plate boundaries, where plates are converging (and lithosphere is being destroyed) or are diverging (and new lithosphere is being created).[14]

During the development of geological theory, certain concepts that allowed the grouping of volcanoes in time, place, structure and composition have developed that ultimately have had to be explained in the theory of plate tectonics. For example, some volcanoes are polygenetic with more than one period of activity during their history; other volcanoes that become extinct after erupting exactly once are monogenetic (meaning "one life") and such volcanoes are often grouped together in a geographical region.[15]

Divergent plate boundaries

[edit]
Map showing the divergent plate boundaries (oceanic spreading ridges) and recent sub-aerial volcanoes (mostly at convergent boundaries)

At the mid-ocean ridges, two tectonic plates diverge from one another as hot mantle rock creeps upwards beneath the thinned oceanic crust. The decrease of pressure in the rising mantle rock leads to adiabatic expansion and the partial melting of the rock, causing volcanism and creating new oceanic crust. Most divergent plate boundaries are at the bottom of the oceans, and so most volcanic activity on Earth is submarine, forming new seafloor. Black smokers (also known as deep sea vents) are evidence of this kind of volcanic activity. Where the mid-oceanic ridge is above sea level, volcanic islands are formed, such as Iceland.[16][3]

Convergent plate boundaries

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Subduction zones are places where two plates, usually an oceanic plate and a continental plate, collide. The oceanic plate subducts (dives beneath the continental plate), forming a deep ocean trench just offshore. In a process called flux melting, water released from the subducting plate lowers the melting temperature of the overlying mantle wedge, thus creating magma. This magma tends to be extremely viscous because of its high silica content, so it often does not reach the surface but cools and solidifies at depth. When it does reach the surface, however, a volcano is formed. Thus subduction zones are bordered by chains of volcanoes called volcanic arcs. Typical examples are the volcanoes in the Pacific Ring of Fire, such as the Cascade Volcanoes or the Japanese Archipelago, or the eastern islands of Indonesia.[17][2]

Hotspots

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Hotspots are volcanic areas thought to be formed by mantle plumes, which are hypothesized to be columns of hot material rising from the core-mantle boundary. As with mid-ocean ridges, the rising mantle rock experiences decompression melting which generates large volumes of magma. Because tectonic plates move across mantle plumes, each volcano becomes inactive as it drifts off the plume, and new volcanoes are created where the plate advances over the plume. The Hawaiian Islands are thought to have been formed in such a manner, as has the Snake River Plain, with the Yellowstone Caldera being part of the North American plate currently above the Yellowstone hotspot.[18][4] However, the mantle plume hypothesis has been questioned.[19]

Continental rifting

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Sustained upwelling of hot mantle rock can develop under the interior of a continent and lead to rifting. Early stages of rifting are characterized by flood basalts and may progress to the point where a tectonic plate is completely split.[20][21] A divergent plate boundary then develops between the two halves of the split plate. However, rifting often fails to completely split the continental lithosphere (such as in an aulacogen), and failed rifts are characterized by volcanoes that erupt unusual alkali lava or carbonatites. Examples include the volcanoes of the East African Rift.[22]

Volcanic features

[edit]
Video of lava agitating and bubbling in the volcanic eruption of Litli-Hrútur (Fagradalsfjall), Iceland, 2023

A volcano needs a reservoir of molten magma (e.g. a magma chamber), a conduit to allow magma to rise through the crust, and a vent to allow the magma to escape above the surface as lava. The erupted volcanic material (lava and tephra) that is deposited around the vent is known as a volcanic edifice, typically a volcanic cone or mountain.[2][23]

The most common perception of a volcano is of a conical mountain, spewing lava and poisonous gases from a crater at its summit; however, this describes just one of the many types of volcano. The features of volcanoes are varied. The structure and behaviour of volcanoes depend on several factors. Some volcanoes have rugged peaks formed by lava domes rather than a summit crater while others have landscape features such as massive plateaus. Vents that issue volcanic material (including lava and ash) and gases (mainly steam and magmatic gases) can develop anywhere on the landform and may give rise to smaller cones such as Puʻu ʻŌʻō on a flank of Kīlauea in Hawaii. Volcanic craters are not always at the top of a mountain or hill and may be filled with lakes such as with Lake Taupō in New Zealand. Some volcanoes can be low-relief landform features, with the potential to be hard to recognize as such and be obscured by geological processes.[2][24][25]

Other types of volcano include mud volcanoes, which are structures often not associated with known magmatic activity; and cryovolcanoes (or ice volcanoes), particularly on some moons of Jupiter, Saturn, and Neptune. Active mud volcanoes tend to involve temperatures much lower than those of igneous volcanoes except when the mud volcano is actually a vent of an igneous volcano.

Fissure vents

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Lakagigar fissure vent in Iceland, the source of the major world climate alteration of 1783–84, has a chain of volcanic cones along its length.

Volcanic fissure vents are generally found at diverging plate boundaries, they are flat, linear fractures through which basaltic lava emerges. These kinds of volcanoes are non-explosive and the basaltic lava tends to have a low viscosity and solidifies slowly leading to a gentle sloping basaltic lava plateau. They often relate or constitute shield volcanoes[2][26]

Shield volcanoes

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Skjaldbreiður, a shield volcano whose name means "broad shield"

Shield volcanoes, so named for their broad, shield-like profiles, are formed by the eruption of low-viscosity basaltic or andesitic lava that can flow a great distance from a vent. They generally do not explode catastrophically but are characterized by relatively gentle effusive eruptions.[2] Since low-viscosity magma is typically low in silica, shield volcanoes are more common in oceanic than continental settings. The Hawaiian volcanic chain is a series of shield cones, and they are common in Iceland, as well.[26] Olympus Mons, an extinct martian shield volcano is the largest known volcano in the Solar System.[27]

Lava domes

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East dome, a lava dome located on the lower east flank of St. Helens, part of the Sugar Bowl Eruptive Period (1800 YA).

Lava domes, also called dome volcanoes, have steep convex sides built by slow eruptions of highly viscous lava, for example, rhyolite.[2] They are sometimes formed within the crater of a previous volcanic eruption, as in the case of Mount St. Helens, but can also form independently, as in the case of Lassen Peak. Like stratovolcanoes, they can produce violent, explosive eruptions, but the lava generally does not flow far from the originating vent.

Cryptodomes

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Cryptodomes are formed when viscous lava is forced upward causing the surface to bulge. The 1980 eruption of Mount St. Helens was an example; lava beneath the surface of the mountain created an upward bulge, which later collapsed down the north side of the mountain.

Cinder cones

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Izalco volcano, the youngest volcano in El Salvador. Izalco erupted almost continuously from 1770 (when it formed) to 1958, earning it the nickname of "Lighthouse of the Pacific".

Cinder cones result from eruptions of mostly small pieces of scoria and pyroclastics (both resemble cinders, hence the name of this volcano type) that build up around the vent. These can be relatively short-lived eruptions that produce a cone-shaped hill perhaps 30 to 400 metres (100 to 1,300 ft) high. Most cinder cones erupt only once and some may be found in monogenetic volcanic fields that may include other features that form when magma comes into contact with water such as maar explosion craters and tuff rings.[28] Cinder cones may form as flank vents on larger volcanoes, or occur on their own. Parícutin in Mexico and Sunset Crater in Arizona are examples of cinder cones. In New Mexico, Caja del Rio is a volcanic field of over 60 cinder cones.

Based on satellite images, it has been suggested that cinder cones might occur on other terrestrial bodies in the Solar system too; on the surface of Mars and the Moon.[29][30][31][32]

Stratovolcanoes (composite volcanoes)

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Cross-section through a stratovolcano (vertical scale is exaggerated):
  1. Large magma chamber
  2. Bedrock
  3. Conduit (pipe)
  4. Base
  5. Sill
  6. Dike
  7. Layers of ash emitted by the volcano
  8. Flank
  9. Layers of lava emitted by the volcano
  10. Throat
  11. Parasitic cone
  12. Lava flow
  13. Vent
  14. Crater
  15. Ash cloud

Stratovolcanoes are tall conical mountains composed of lava flows and tephra in alternate layers, the strata that gives rise to the name. They are also known as composite volcanoes because they are created from multiple structures during different kinds of eruptions; the main conduit bringing magma to the surface branches into multiple secondary conduits and occasional laccoliths or sills, the branching conduits may form parasitic cones on the flanks of the main cone.[2] Classic examples include Mount Fuji in Japan, Mayon Volcano in the Philippines, and Mount Vesuvius and Stromboli in Italy.

Mt. Vesuvius, a stratovolcano, Gulf of Naples.

Ash produced by the explosive eruption of stratovolcanoes has historically posed the greatest volcanic hazard to civilizations. The lavas of stratovolcanoes are higher in silica, and therefore much more viscous, than lavas from shield volcanoes. High-silica lavas also tend to contain more dissolved gas. The combination is deadly, promoting explosive eruptions that produce great quantities of ash, as well as pyroclastic surges like the one that destroyed the city of Saint-Pierre in Martinique in 1902. They are also steeper than shield volcanoes, with slopes of 30–35° compared to slopes of generally 5–10°, and their loose tephra are material for dangerous lahars.[33] Large pieces of tephra are called volcanic bombs. Big bombs can measure more than 1.2 metres (4 ft) across and weigh several tons.[34]

Supervolcanoes

[edit]
Lake Taupō, a volcanogenic lake in the caldera of Taupō supervolcano, New Zealand.

A supervolcano is defined as a volcano that has experienced one or more eruptions that produced over 1,000 cubic kilometres (240 cu mi) of volcanic deposits in a single explosive event.[35] Such eruptions occur when a very large magma chamber full of gas-rich, silicic magma is emptied in a catastrophic caldera-forming eruption. Ash flow tuffs emplaced by such eruptions are the only volcanic product with volumes rivalling those of flood basalts.[36]

Supervolcano eruptions, while the most dangerous type, are very rare; four are known from the last million years, and about 60 historical VEI 8 eruptions have been identified in the geologic record over millions of years. A supervolcano can produce devastation on a continental scale, and severely cool global temperatures for many years after the eruption due to the huge volumes of sulfur and ash released into the atmosphere.

Because of the enormous area they cover, and subsequent concealment under vegetation and glacial deposits, supervolcanoes can be difficult to identify in the geologic record without careful geological mapping.[37] Known examples include Yellowstone Caldera in Yellowstone National Park and Valles Caldera in New Mexico (both western United States); Lake Taupō in New Zealand; Lake Toba in Sumatra, Indonesia; and Ngorongoro Crater in Tanzania.

Caldera volcanoes

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Crater lake, a volcanic lake in Oregon.

Volcanoes that, though large, are not large enough to be called supervolcanoes, may also form calderas (collapsed crater) in the same way. There may be active or dormant cones inside of the caldera or even a lake, such lakes are called Volcanogenic lakes, or simply, volcanic lakes.[38][2]

Submarine volcanoes

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Satellite images of the January 15, 2022, eruption of Hunga Tonga-Hunga Haʻapai

Submarine volcanoes are common features of the ocean floor. Volcanic activity during the Holocene Epoch has been documented at only 119 submarine volcanoes, but there may be more than one million geologically young submarine volcanoes on the ocean floor.[39][40] In shallow water, active volcanoes disclose their presence by blasting steam and rocky debris high above the ocean's surface. In the deep ocean basins, the tremendous weight of the water prevents the explosive release of steam and gases; however, submarine eruptions can be detected by hydrophones and by the discoloration of water because of volcanic gases. Pillow lava is a common eruptive product of submarine volcanoes and is characterized by thick sequences of discontinuous pillow-shaped masses which form underwater. Even large submarine eruptions may not disturb the ocean surface, due to the rapid cooling effect and increased buoyancy in water (as compared to air), which often causes volcanic vents to form steep pillars on the ocean floor. Hydrothermal vents are common near these volcanoes, and some support peculiar ecosystems based on chemotrophs feeding on dissolved minerals. Over time, the formations created by submarine volcanoes may become so large that they break the ocean surface as new islands or floating pumice rafts.

In May and June 2018, a multitude of seismic signals were detected by earthquake monitoring agencies all over the world. They took the form of unusual humming sounds, and some of the signals detected in November of that year had a duration of up to 20 minutes. An oceanographic research campaign in May 2019 showed that the previously mysterious humming noises were caused by the formation of a submarine volcano off the coast of Mayotte.[41]

Subglacial volcanoes

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Subglacial volcanoes develop underneath ice caps. They are made up of lava plateaus capping extensive pillow lavas and palagonite. These volcanoes are also called table mountains, tuyas,[42] or (in Iceland) mobergs.[43] Very good examples of this type of volcano can be seen in Iceland and in British Columbia. The origin of the term comes from Tuya Butte, which is one of the several tuyas in the area of the Tuya River and Tuya Range in northern British Columbia. Tuya Butte was the first such landform analysed and so its name has entered the geological literature for this kind of volcanic formation.[44] The Tuya Mountains Provincial Park was recently established to protect this unusual landscape, which lies north of Tuya Lake and south of the Jennings River near the boundary with the Yukon Territory.

Hydrothermal features

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Hydrothermal features, for example geysers, fumaroles, mud pools, mud volcanoes, hot springs and acidic hot springs involve water as well as geothermal or magmatic activity. Such features are common around volcanoes and are often indicative of volcanism.[2][45]

Mud volcanoes

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Mud volcano at Gobustan

Mud volcanoes or mud domes are conical structures created by eruption of liquids and gases, particularly mud (slurries), water and gases, although several activities may contribute. The largest mud volcanoes are 10 kilometres (6.2 mi) in diameter and reach 700 metres (2,300 ft) high.[46][47] Mud volcanoes can be seen off the shore of Indonesia, on the island of Baratang, in Balochistan and in central Asia.

Fumarole

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Fumaroles are vents on the surface from which hot steam and volcanic gases erupt due to the presence of superheated groundwater, these may indicate volcanic activity. Fumaroles erupting sulfurous gases are also often called solfataras.[48][2]

Geysers

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Castle geyser eruption, Yellowstone National Park.

Geysers are springs which will occasionally erupt and discharge hot water and steam. Geysers may indicate ongoing magmatism, water underground is heated by hot rocks and steam pressure builds up before being released along with a jet of hot water. Almost half of all active geysers are present in Yellowstone National Park, US.[2][49]

Erupted material

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Timelapse of San Miguel (volcano) degassing in 2022. El Salvador is home to 20 Holocene volcanoes, 3 of which have erupted in last 100yrs[50]
Pāhoehoe lava flow on Hawaii. The picture shows overflows of a main lava channel.
Litli-Hrútur (Fagradalsfjall) eruption 2023. View from an aeroplane
The Stromboli stratovolcano off the coast of Sicily has erupted continuously for thousands of years, giving rise to its nickname "Lighthouse of the Mediterranean".

The material that is expelled in a volcanic eruption can be classified into three types:

  1. Volcanic gases, a mixture made mostly of steam, carbon dioxide, and a sulfur compound (either sulfur dioxide, SO2, or hydrogen sulfide, H2S, depending on the temperature)
  2. Lava, the name of magma when it emerges and flows over the surface
  3. Tephra, particles of solid material of all shapes and sizes ejected and thrown through the air[51][52]

Volcanic gases

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The concentrations of different volcanic gases can vary considerably from one volcano to the next. Water vapour is typically the most abundant volcanic gas, followed by carbon dioxide[53] and sulfur dioxide. Other principal volcanic gases include hydrogen sulfide, hydrogen chloride, and hydrogen fluoride. A large number of minor and trace gases are also found in volcanic emissions, for example hydrogen, carbon monoxide, halocarbons, organic compounds, and volatile metal chlorides.

Lava flows

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Mount Rinjani eruption in 1994, in Lombok, Indonesia

The form and style of an eruption of a volcano is largely determined by the composition of the lava it erupts. The viscosity (how fluid the lava is) and the amount of dissolved gas are the most important characteristics of magma, and both are largely determined by the amount of silica in the magma. Magma rich in silica is much more viscous than silica-poor magma, and silica-rich magma also tends to contain more dissolved gases.

Lava can be broadly classified into four different compositions:[54]

  • If the erupted magma contains a high percentage (>63%) of silica, the lava is described as felsic. Felsic lavas (dacites or rhyolites) are highly viscous and are erupted as domes or short, stubby flows.[55] Lassen Peak in California is an example of a volcano formed from felsic lava and is actually a large lava dome.[56]
Because felsic magmas are so viscous, they tend to trap volatiles (gases) that are present, which leads to explosive volcanism. Pyroclastic flows (ignimbrites) are highly hazardous products of such volcanoes since they hug the volcano's slopes and travel far from their vents during large eruptions. Temperatures as high as 850 °C (1,560 °F)[57] are known to occur in pyroclastic flows, which will incinerate everything flammable in their path, and thick layers of hot pyroclastic flow deposits can be laid down, often many meters thick.[58] Alaska's Valley of Ten Thousand Smokes, formed by the eruption of Novarupta near Katmai in 1912, is an example of a thick pyroclastic flow or ignimbrite deposit.[59] Volcanic ash that is light enough to erupt high into the Earth's atmosphere as an eruption column may travel hundreds of kilometres before it falls back to ground as a fallout tuff. Volcanic gases may remain in the stratosphere for years.[60]
Felsic magmas are formed within the crust, usually through the melting of crust rock from the heat of underlying mafic magmas. The lighter felsic magma floats on the mafic magma without significant mixing.[61] Less commonly, felsic magmas are produced by extreme fractional crystallization of more mafic magmas.[62] This is a process in which mafic minerals crystallize out of the slowly cooling magma, which enriches the remaining liquid in silica.
  • If the erupted magma contains 52–63% silica, the lava is of intermediate composition or andesitic. Intermediate magmas are characteristic of stratovolcanoes.[63] They are most commonly formed at convergent boundaries between tectonic plates, by several processes. One process is the hydration melting of mantle peridotite followed by fractional crystallization. Water from a subducting slab rises into the overlying mantle, lowering its melting point, particularly for the more silica-rich minerals. Fractional crystallization further enriches the magma in silica. It has also been suggested that intermediate magmas are produced by the melting of sediments carried downwards by the subducted slab.[64] Another process is magma mixing between felsic rhyolitic and mafic basaltic magmas in an intermediate reservoir before emplacement or lava flow.[65]
  • If the erupted magma contains <52% and >45% silica, the lava is called mafic (because it contains higher percentages of magnesium (Mg) and iron (Fe)) or basaltic. These lavas are usually hotter and much less viscous than felsic lavas. Mafic magmas are formed by partial melting of the dry mantle, with limited fractional crystallization and assimilation of crustal material.[66]
Mafic lavas occur in a wide range of settings. These include mid-ocean ridges; Shield volcanoes (such the Hawaiian Islands, including Mauna Loa and Kilauea), on both oceanic and continental crust; and as continental flood basalts.
  • Some erupted magmas contain ≤45% silica and produce ultramafic lava. Ultramafic flows, also known as komatiites, are very rare; indeed, very few have been erupted at Earth's surface since the Proterozoic, when the planet's heat flow was higher. They are (or were) the hottest lavas, and were probably more fluid than common mafic lavas, with a viscosity less than a tenth that of hot basalt magma.[67]

Mafic lava flows show two varieties of surface texture: ʻAʻa (pronounced [ˈʔaʔa]) and pāhoehoe ([paːˈho.eˈho.e]), both Hawaiian words. ʻAʻa is characterized by a rough, clinkery surface and is the typical texture of cooler basalt lava flows. Pāhoehoe is characterized by its smooth and often ropey or wrinkly surface and is generally formed from more fluid lava flows. Pāhoehoe flows are sometimes observed to transition to ʻaʻa flows as they move away from the vent, but never the reverse.[68]

More silicic lava flows take the form of block lava, where the flow is covered with angular, vesicle-poor blocks. Rhyolitic flows typically consist largely of obsidian.[69]

Tephra

[edit]
Light-microscope image of tuff as seen in thin section (long dimension is several mm): the curved shapes of altered glass shards (ash fragments) are well preserved, although the glass is partly altered. The shapes were formed around bubbles of expanding, water-rich gas.

Tephra is made when magma inside the volcano is blown apart by the rapid expansion of hot volcanic gases. Magma commonly explodes as the gas dissolved in it comes out of solution as the pressure decreases when it flows to the surface. These violent explosions produce particles of material that can then fly from the volcano. Solid particles smaller than 2 mm in diameter (sand-sized or smaller) are called volcanic ash.[51][52]

Tephra and other volcaniclastics (shattered volcanic material) make up more of the volume of many volcanoes than do lava flows. Volcaniclastics may have contributed as much as a third of all sedimentation in the geologic record. The production of large volumes of tephra is characteristic of explosive volcanism.[70]

Dissection

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Through natural processes, mainly erosion, so much of the solidified erupted material that makes up the mantle of a volcano may be stripped away that its inner anatomy becomes apparent. Using the metaphor of biological anatomy, such a process is called "dissection".[71] When the volcano is extinct, a plug forms on its vent, over time due to erosion, the volcanic cone slowly erodes away leaving the resistant lava plug intact.[2] Cinder Hill, a feature of Mount Bird on Ross Island, Antarctica, is a prominent example of a dissected volcano. Volcanoes that were, on a geological timescale, recently active, such as for example Mount Kaimon in southern Kyūshū, Japan, tend to be undissected. Devils Tower in Wyoming is a famous example of exposed volcanic plug.

Volcanic eruptions

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As of December 2022, the Smithsonian Institution's Global Volcanism Program database of volcanic eruptions in the Holocene Epoch (the last 11,700 years) lists 9,901 confirmed eruptions from 859 volcanoes. The database also lists 1,113 uncertain eruptions and 168 discredited eruptions for the same time interval.[72][73]

Schematic of volcano injection of aerosols and gases

Eruption styles are broadly divided into magmatic, phreatomagmatic (hydrovolcanic), and phreatic eruptions.[74] The intensity of explosive volcanism is expressed using the volcanic explosivity index (VEI), which ranges from 0 for Hawaiian-type eruptions to 8 for supervolcanic eruptions:[75][76]

  • Magmatic eruptions are driven primarily by gas release due to decompression.[74] Low-viscosity magma with little dissolved gas produces relatively gentle effusive eruptions. High-viscosity magma with a high content of dissolved gas produces violent explosive eruptions. The range of observed eruption styles is expressed from historical examples.
  • Hawaiian eruptions are typical of volcanoes that erupt mafic lava with a relatively low gas content. These are almost entirely effusive, producing local lava fountains and highly fluid lava flows but relatively little tephra. They are named after the Hawaiian volcanoes. The eruption column from these eruptions does not exceed 2 kilometres (1.2 mi) in height.
  • Strombolian eruptions are characterized by moderate viscosities and dissolved gas levels. They are characterized by frequent but short-lived eruptions that can produce eruptive columns hundreds of meters high, which can also be seen in a gas slug. Their primary product is scoria. They are named after Stromboli.
  • Vulcanian eruptions are characterized by yet higher viscosities and partial crystallization of magma, which is often intermediate in composition. Eruptions take the form of short-lived explosions for several hours, which destroy a central dome and eject large lava blocks and bombs. This is followed by an effusive phase that rebuilds the central dome. Vulcanian eruptions are named after Vulcano. Eruption columns from these eruptions do not exceed 20 kilometres (12 mi) in height.
  • Peléan eruptions are more violent still, being characterized by dome growth and collapse that produces various kinds of pyroclastic flows. They are named after Mount Pelée.
  • Plinian eruptions are characterized by sustained huge eruption columns whose collapse produces catastrophic pyroclastic flows. They are named after Pliny the Younger, who chronicled the Plinian eruption of Mount Vesuvius in 79 AD.
  • Ultra-Plinian eruptions are the largest of all volcanic eruptions are more intense, have a higher eruption rate than Plinian ones, form higher eruption columns and may form large calderas. These eruptions produce rhyolitic lava, tephra, pumice and thick pyroclastic flows that cover vast areas and may produce widespread ash-fall deposits. Examples are Mt. Mazama and Yellowstone.
  • Phreatomagmatic eruptions (hydrovolcanic) are characterized by interaction of rising magma with groundwater. They are driven by the resulting rapid buildup of pressure in the superheated groundwater.
  • Phreatic eruptions are characterized by superheating of groundwater that comes in contact with hot rock or magma. They are distinguished from phreatomagmatic eruptions because the erupted material is all country rock; no magma is erupted.

Volcanic activity

[edit]
Fresco with Mount Vesuvius behind Bacchus and Agathodaemon, as seen in Pompeii's House of the Centenary

Volcanoes vary greatly in their level of activity, with individual volcanic systems having an eruption recurrence ranging from several times a year to once in tens of thousands of years.[77] Volcanoes are informally described as erupting, active, dormant, or extinct, but the definitions of these terms are not entirely uniform among volcanologists. The level of activity of most volcanoes falls upon a graduated spectrum, with much overlap between categories, and does not always fit neatly into only one of these three separate categories.[6]

Erupting

[edit]

The USGS defines a volcano as "erupting" whenever the ejection of magma from any point on the volcano is visible, including visible magma still contained within the walls of the summit crater.

Active

[edit]

While there is no international consensus among volcanologists on how to define an active volcano, the USGS defines a volcano as active whenever subterranean indicators, such as earthquake swarms, ground inflation, or unusually high levels of carbon dioxide or sulfur dioxide are present.[78][79]

Dormant and reactivated

[edit]
Narcondam Island, India, is classified as a dormant volcano by the Geological Survey of India.

The USGS defines a dormant volcano as any volcano that is not showing any signs of unrest such as earthquake swarms, ground swelling, or excessive noxious gas emissions, but which shows signs that it could yet become active again.[79] Many dormant volcanoes have not erupted for thousands of years, but have still shown signs that they may be likely to erupt again in the future.[80][81]

In an article justifying the re-classification of Alaska's Mount Edgecumbe volcano from "dormant" to "active", volcanologists at the Alaska Volcano Observatory pointed out that the term "dormant" in reference to volcanoes has been deprecated over the past few decades and that "[t]he term "dormant volcano" is so little used and undefined in modern volcanology that the Encyclopedia of Volcanoes (2000) does not contain it in the glossaries or index",[82] however the USGS still widely employs the term.

Previously a volcano was often considered to be extinct if there were no written records of its activity. Such a generalization is inconsistent with observation and deeper study, as has occurred recently with the unexpected eruption of the Chaitén volcano in 2008.[83] Modern volcanic activity monitoring techniques, and improvements in the modelling of the factors that produce eruptions, have helped the understanding of why volcanoes may remain dormant for a long time, and then become unexpectedly active again. The potential for eruptions, and their style, depend mainly upon the state of the magma storage system under the volcano, the eruption trigger mechanism and its timescale.[84]: 95  For example, the Yellowstone volcano has a repose/recharge period of around 700,000 years, and Toba of around 380,000 years.[85] Vesuvius was described by Roman writers as having been covered with gardens and vineyards before its unexpected eruption of 79 CE, which destroyed the towns of Herculaneum and Pompeii.

Accordingly, it can sometimes be difficult to distinguish between an extinct volcano and a dormant (inactive) one. Long volcano dormancy is known to decrease awareness.[84]: 96  Pinatubo was an inconspicuous volcano, unknown to most people in the surrounding areas, and initially not seismically monitored before its unanticipated and catastrophic eruption of 1991. Two other examples of volcanoes that were once thought to be extinct, before springing back into eruptive activity were the long-dormant Soufrière Hills volcano on the island of Montserrat, thought to be extinct until activity resumed in 1995 (turning its capital Plymouth into a ghost town) and Fourpeaked Mountain in Alaska, which, before its September 2006 eruption, had not erupted since before 8000 BCE.

Extinct

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Capulin Volcano National Monument in New Mexico, US

Extinct volcanoes are those that scientists consider unlikely to erupt again because the volcano no longer has a magma supply. Examples of extinct volcanoes are many volcanoes on the Hawaiian–Emperor seamount chain in the Pacific Ocean (although some volcanoes at the eastern end of the chain are active), Hohentwiel in Germany, Shiprock in New Mexico, U.S., Capulin in New Mexico, U.S., Zuidwal volcano in the Netherlands, and many volcanoes in Italy such as Monte Vulture. Edinburgh Castle in Scotland is located atop an extinct volcano, which forms Castle Rock. Whether a volcano is truly extinct is often difficult to determine. Since "supervolcano" calderas can have eruptive lifespans sometimes measured in millions of years, a caldera that has not produced an eruption in tens of thousands of years may be considered dormant instead of extinct. An individual volcano in a monogenetic volcanic field can be extinct, but that does not mean a completely new volcano might not erupt close by with little or no warning, as its field may have an active magma supply.

Volcanic-alert level

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The three common popular classifications of volcanoes can be subjective and some volcanoes thought to have been extinct have erupted again. To help prevent people from falsely believing they are not at risk when living on or near a volcano, countries have adopted new classifications to describe the various levels and stages of volcanic activity.[86] Some alert systems use different numbers or colours to designate the different stages. Other systems use colours and words. Some systems use a combination of both.

Decade volcanoes

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Koryaksky volcano towering over Petropavlovsk-Kamchatsky on Kamchatka Peninsula, Far Eastern Russia

The Decade Volcanoes are 16 volcanoes identified by the International Association of Volcanology and Chemistry of the Earth's Interior (IAVCEI) as being worthy of particular study in light of their history of large, destructive eruptions and proximity to populated areas. They are named Decade Volcanoes because the project was initiated as part of the United Nations-sponsored International Decade for Natural Disaster Reduction (the 1990s). The 16 current Decade Volcanoes are:

The Deep Earth Carbon Degassing Project, an initiative of the Deep Carbon Observatory, monitors nine volcanoes, two of which are Decade volcanoes. The focus of the Deep Earth Carbon Degassing Project is to use Multi-Component Gas Analyzer System instruments to measure CO2/SO2 ratios in real-time and in high-resolution to allow detection of the pre-eruptive degassing of rising magmas, improving prediction of volcanic activity.[87]

Volcanoes and humans

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Solar radiation graph 1958–2008, showing how the radiation is reduced after major volcanic eruptions
Sulfur dioxide concentration over the Sierra Negra Volcano, Galapagos Islands, during an eruption in October 2005

Volcanic eruptions pose a significant threat to human civilization. However, volcanic activity has also provided humans with important resources.

Hazards

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There are many different types of volcanic eruptions and associated activity: phreatic eruptions (steam-generated eruptions), explosive eruptions of high-silica lava (e.g., rhyolite), effusive eruptions of low-silica lava (e.g., basalt), sector collapses, pyroclastic flows, lahars (debris flows) and volcanic gas emissions. These can pose a hazard to humans. Earthquakes, hot springs, fumaroles, mud pots and geysers often accompany volcanic activity.

Volcanic gases can reach the stratosphere, where they form sulfuric acid aerosols that can reflect solar radiation and lower surface temperatures significantly.[88] Sulfur dioxide from the eruption of Huaynaputina may have caused the Russian famine of 1601–1603.[89] Chemical reactions of sulfate aerosols in the stratosphere can also damage the ozone layer, and acids such as hydrogen chloride (HCl) and hydrogen fluoride (HF) can fall to the ground as acid rain. Excessive fluoride salts from eruptions have poisoned livestock in Iceland on multiple occasions.[90]: 39–58  Explosive volcanic eruptions release the greenhouse gas carbon dioxide and thus provide a deep source of carbon for biogeochemical cycles.[91]

Ash thrown into the air by eruptions can present a hazard to aircraft, especially jet aircraft where the particles can be melted by the high operating temperature; the melted particles then adhere to the turbine blades and alter their shape, disrupting the operation of the turbine. This can cause major disruptions to air travel.

Comparison of major United States prehistoric eruptions (VEI 7 and 8) with major historical volcanic eruptions in the 19th and 20th century (VEI 5, 6 and 7). From left to right: Yellowstone 2.1 Ma, Yellowstone 1.3 Ma, Long Valley 6.26 Ma, Yellowstone 0.64 Ma . 19th century eruptions: Tambora 1815, Krakatoa 1883. 20th century eruptions: Novarupta 1912, St. Helens 1980, Pinatubo 1991.

A volcanic winter is thought to have taken place around 70,000 years ago after the supereruption of Lake Toba on Sumatra island in Indonesia.[92] This may have created a population bottleneck that affected the genetic inheritance of all humans today.[93] Volcanic eruptions may have contributed to major extinction events, such as the End-Ordovician, Permian-Triassic, and Late Devonian mass extinctions.[94]

The 1815 eruption of Mount Tambora created global climate anomalies that became known as the "Year Without a Summer" because of the effect on North American and European weather.[95] The freezing winter of 1740–41, which led to widespread famine in northern Europe, may also owe its origins to a volcanic eruption.[96]

Benefits

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Although volcanic eruptions pose considerable hazards to humans, past volcanic activity has created important economic resources. Tuff formed from volcanic ash is a relatively soft rock, and it has been used for construction since ancient times.[97][98] The Romans often used tuff, which is abundant in Italy, for construction.[99] The Rapa Nui people used tuff to make most of the moai statues in Easter Island.[100]

Volcanic ash and weathered basalt produce some of the most fertile soil in the world, rich in nutrients such as iron, magnesium, potassium, calcium, and phosphorus.[101] Volcanic activity is responsible for emplacing valuable mineral resources, such as metal ores.[101] It is accompanied by high rates of heat flow from Earth's interior. These can be tapped as geothermal power.[101]

Tourism associated with volcanoes is also a worldwide industry.[102]

Safety considerations

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Many volcanoes near human settlements are heavily monitored with the aim of providing adequate advance warnings of imminent eruptions to nearby populations. Also, a better modern-day understanding of volcanology has led to some better informed governmental and public responses to unanticipated volcanic activities. While the science of volcanology may not yet be capable of predicting the exact times and dates of eruptions far into the future, on suitably monitored volcanoes the monitoring of ongoing volcanic indicators is often capable of predicting imminent eruptions with advance warnings minimally of hours, and usually of days prior to any eruptions.[103] The diversity of volcanoes and their complexities mean that eruption forecasts for the foreseeable future will be based on probability, and the application of risk management. Even then, some eruptions will have no useful warning. An example of this occurred in March 2017, when a tourist group was witnessing a presumed to be predictable Mount Etna eruption and the flowing lava came in contact with a snow accumulation causing a situational phreatic explosion causing injury to ten persons.[102] Other types of significant eruptions are known to give useful warnings of only hours at the most by seismic monitoring.[83] The recent demonstration of a magma chamber with repose times of tens of thousands of years, with potential for rapid recharge so potentially decreasing warning times, under the youngest volcano in central Europe,[84] does not tell us if more careful monitoring will be useful.

Scientists are known to perceive risk, with its social elements, differently from local populations and those that undertake social risk assessments on their behalf, so that both disruptive false alarms and retrospective blame, when disasters occur, will continue to happen.[104]: 1–3 

Thus in many cases, while volcanic eruptions may still cause major property destruction, the periodic large-scale loss of human life that was once associated with many volcanic eruptions, has recently been significantly reduced in areas where volcanoes are adequately monitored. This life-saving ability is derived via such volcanic-activity monitoring programs, through the greater abilities of local officials to facilitate timely evacuations based upon the greater modern-day knowledge of volcanism that is now available, and upon improved communications technologies such as cell phones. Such operations tend to provide enough time for humans to escape at least with their lives before a pending eruption. One example of such a recent successful volcanic evacuation was the Mount Pinatubo evacuation of 1991. This evacuation is believed to have saved 20,000 lives.[105] In the case of Mount Etna, a 2021 review found 77 deaths due to eruptions since 1536 but none since 1987.[102]

Citizens who may be concerned about their own exposure to risk from nearby volcanic activity should familiarize themselves with the types of, and quality of, volcano monitoring and public notification procedures being employed by governmental authorities in their areas.[106]

Volcanoes on other celestial bodies

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The Tvashtar volcano erupts a plume 330 km (205 mi) above the surface of Jupiter's moon Io.

Earth's Moon has no large volcanoes and no current volcanic activity, although recent evidence suggests it may still possess a partially molten core.[107] However, the Moon does have many volcanic features such as maria[108] (the darker patches seen on the Moon), rilles[109] and domes.[110]

The planet Venus has a surface that is 90% basalt, indicating that volcanism played a major role in shaping its surface. The planet may have had a major global resurfacing event about 500 million years ago,[111] from what scientists can tell from the density of impact craters on the surface. Lava flows are widespread and forms of volcanism not present on Earth occur as well. Changes in the planet's atmosphere and observations of lightning have been attributed to ongoing volcanic eruptions, although there is no confirmation of whether or not Venus is still volcanically active. However, radar sounding by the Magellan probe revealed evidence for comparatively recent volcanic activity at Venus's highest volcano Maat Mons, in the form of ash flows near the summit and on the northern flank.[112] However, the interpretation of the flows as ash flows has been questioned.[113]

Olympus Mons (Latin, "Mount Olympus"), located on the planet Mars, is the tallest known mountain in the Solar System.

There are several extinct volcanoes on Mars, four of which are vast shield volcanoes far bigger than any on Earth. They include Arsia Mons, Ascraeus Mons, Hecates Tholus, Olympus Mons, and Pavonis Mons. These volcanoes have been extinct for many millions of years,[114] but the European Mars Express spacecraft has found evidence that volcanic activity may have occurred on Mars in the recent past as well.[114]

Jupiter's moon Io is the most volcanically active object in the Solar System because of tidal interaction with Jupiter. It is covered with volcanoes that erupt sulfur, sulfur dioxide and silicate rock, and as a result, Io is constantly being resurfaced. Its lavas are the hottest known anywhere in the Solar System, with temperatures exceeding 1,800 K (1,500 °C). In February 2001, the largest recorded volcanic eruptions in the Solar System occurred on Io.[115] Europa, the smallest of Jupiter's Galilean moons, also appears to have an active volcanic system, except that its volcanic activity is entirely in the form of water, which freezes into ice on the frigid surface. This process is known as cryovolcanism, and is apparently most common on the moons of the outer planets of the Solar System.[116]

In 1989, the Voyager 2 spacecraft observed cryovolcanoes (ice volcanoes) on Triton, a moon of Neptune, and in 2005 the Cassini–Huygens probe photographed fountains of frozen particles erupting from Enceladus, a moon of Saturn.[117][118] The ejecta may be composed of water, liquid nitrogen, ammonia, dust, or methane compounds. Cassini–Huygens also found evidence of a methane-spewing cryovolcano on the Saturnian moon Titan, which is believed to be a significant source of the methane found in its atmosphere.[119] It is theorized that cryovolcanism may also be present on the Kuiper Belt Object Quaoar.

A 2010 study of the exoplanet COROT-7b, which was detected by transit in 2009, suggested that tidal heating from the host star very close to the planet and neighbouring planets could generate intense volcanic activity similar to that found on Io.[120]

History of volcano understanding

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Volcanoes are not distributed evenly over the Earth's surface but active ones with significant impact were encountered early in human history, evidenced by footprints of hominina found in East African volcanic ash dated at 3.66 million years old.[121]: 104  The association of volcanoes with fire and disaster is found in many oral traditions and had religious and thus social significance before the first written record of concepts related to volcanoes. Examples are: (1) the stories in the Athabascan subcultures about humans living inside mountains and a woman who uses fire to escape from a mountain,[122]: 135  (2) Pele's migration through the Hawarian island chain, ability to destroy forests and manifestations of the god's temper,[123] and (3) the association in Javanese folklore of a king resident in Mount Merapi volcano and a queen resident at a beach 50 km (31 mi) away on what is now known to be an earthquake fault that interacts with that volcano.[124]

Many ancient accounts ascribe volcanic eruptions to supernatural causes, such as the actions of gods or demigods. The earliest known such example is a neolithic goddess at Çatalhöyük.[125]: 203  The Ancient Greek god Hephaistos and the concepts of the underworld are aligned to volcanoes in that Greek culture.[102]

However, others proposed more natural (but still incorrect) causes of volcanic activity. In the fifth century BC, Anaxagoras proposed eruptions were caused by a great wind.[126] By 65 CE, Seneca the Younger proposed combustion as the cause,[126] an idea also adopted by the Jesuit Athanasius Kircher (1602–1680), who witnessed eruptions of Mount Etna and Stromboli, then visited the crater of Vesuvius and published his view of an Earth in Mundus Subterraneus with a central fire connected to numerous others depicting volcanoes as a type of safety valve.[127] Edward Jorden, in his work on mineral waters, challenged this view; in 1632 he proposed sulfur "fermentation" as a heat source within Earth,[126] Astronomer Johannes Kepler (1571–1630) believed volcanoes were ducts for Earth's tears.[128][better source needed] In 1650, René Descartes proposed the core of Earth was incandescent and, by 1785, the works of Decartes and others were synthesized into geology by James Hutton in his writings about igneous intrusions of magma.[126] Lazzaro Spallanzani had demonstrated by 1794 that steam explosions could cause explosive eruptions and many geologists held this as the universal cause of explosive eruptions up to the 1886 eruption of Mount Tarawera which allowed in one event differentiation of the concurrent phreatomagmatic and hydrothermal eruptions from dry explosive eruption, of, as it turned out, a basalt dyke.[129]: 16–18 [130]: 4  Alfred Lacroix built upon his other knowledge with his studies on the 1902 eruption of Mount Pelée,[126] and by 1928 Arthur Holmes work had brought together the concepts of radioactive generation of heat, Earth's mantle structure, partial decompression melting of magma, and magma convection.[126] This eventually led to the acceptance of plate tectonics.[131]

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A volcano is a vent or fissure in the Earth's crust through which molten rock, known as magma, rises from beneath the surface and erupts as lava, along with gases, ash, and other pyroclastic materials. These eruptions gradually build the volcano's structure, forming cone-shaped mountains or broad plateaus through the accumulation of solidified lava, , and debris over time. Volcanoes represent dynamic geological features that release internal heat and pressure from the planet's mantle, often resulting in both constructive land-building and destructive events. Volcanoes primarily form at the boundaries of tectonic plates, where the Earth's lithospheric plates interact—either diverging, converging, or sliding past one another—allowing magma to ascend from the mantle due to reduced pressure or melting induced by subduction and rifting. This process is most evident along the Pacific Ring of Fire, a horseshoe-shaped zone encircling the Pacific Ocean where about 75% of the world's active volcanoes are concentrated, driven by subduction of oceanic plates beneath continental ones. Globally, there are approximately 1,350 potentially active volcanoes on land, excluding submarine ones along mid-ocean ridges, with around 500 having erupted in historical times. Eruptions occur when buoyant magma forces its way through crustal weaknesses, with the style depending on magma viscosity: low-viscosity basaltic magma produces effusive flows, while high-viscosity andesitic or rhyolitic magma leads to explosive events. Volcanoes are classified into four principal types based on their shape, eruptive style, and composition: shield volcanoes, broad and gently sloping structures formed by fluid basaltic lava flows, such as in ; composite volcanoes (or stratovolcanoes), steep-sided cones built by alternating layers of lava and pyroclastics, exemplified by ; cinder cones, small, steep piles of loose from gas-rich eruptions, like Paricutin in ; and lava domes, bulbous mounds of viscous lava that grow slowly, as seen at in . These types reflect variations in chemistry and eruption dynamics, with shield volcanoes dominating hotspots and ridges, while composite volcanoes prevail at zones. Volcanic activity poses significant hazards, including lava flows that incinerate landscapes, pyroclastic flows that race down slopes at high speeds carrying superheated gas and debris, ash falls that disrupt and , and lahars—volcanic mudflows—that can bury communities far from the vent. Gases like and released during eruptions can harm , acidify rain, and even influence global through aerosol-induced cooling. Conversely, volcanoes confer benefits: their weathered products create nutrient-rich soils supporting dense populations in regions like and the Mediterranean; they provide sources for electricity and heating; and they yield valuable minerals such as and . Monitoring by organizations like the USGS Volcano Hazards Program helps mitigate risks through early warnings, underscoring volcanoes' role in shaping Earth's , ecosystems, and human societies.

Etymology and Terminology

Etymology

The word "volcano" derives from the Latin Vulcanus (also spelled Volcanus), the name of the Roman god of , , and the , whose mythical workshop was believed to lie beneath volcanic islands due to their emissions of smoke and heat. This association is particularly linked to the island of in the Aeolian archipelago off the coast of , , where ancient Romans observed fumaroles and interpreted them as signs of Vulcan's subterranean activity; the island's name, in turn, influenced the Italian term vulcano, which spread to other European languages. Although the modern term "volcano" emerged centuries later, ancient texts provide early historical accounts of volcanic phenomena that shaped later linguistic and scientific usage. , a Roman author and magistrate, offered the first detailed eyewitness description of a major eruption in two letters to the historian , recounting the catastrophic event at in 79 CE, where a massive column of and rose from the mountain, blanketing nearby cities like Pompeii and in debris. These letters, written around 107 CE, vividly depict the eruption's progression—from an initial pine-tree-shaped plume to darkened skies and seismic tremors—without using the word "volcano," but they established a foundational narrative for understanding such events in . The term gained traction in modern languages during the amid growing European and observation of active volcanoes, entering English around 1613 through travel accounts that borrowed from Italian sources to describe Mediterranean eruptions. By the , as Enlightenment-era formalized , "volcano" was integrated into scientific nomenclature; for instance, British diplomat and naturalist William Hamilton employed it extensively in his 1776 publication Campi Phlegraei, documenting eruptions of Vesuvius and other Italian volcanoes with detailed observations and illustrations that advanced vulcanology. This adoption marked the shift from mythological connotations to empirical study, influencing standardized terminology in texts across .

Key Terms

A volcano is defined as an opening, or vent, in through which molten rock, ash, and gases are ejected from the planet's interior. More precisely, it encompasses a structure containing one or more vents supplied by originating from deep within the . Central to volcanic activity are the terms and lava, which refer to the same substance in different states: denotes molten rock beneath the surface, while lava describes the molten rock after it emerges onto the surface. A vent is the specific opening at the surface through which , lava, or volcanic gases are released. Related features include the , a bowl-shaped depression formed above the vent by explosive ejection of material, typically smaller than 1 kilometer in , and the , a much larger basin-like depression, often exceeding 1 kilometer and up to 50 kilometers across, resulting from the collapse of the volcano's structure after major eruptions. Volcanic processes are classified as endogenic or exogenic: endogenic processes, driven by internal heat from Earth's core such as and , include magma generation and eruption, while exogenic processes, powered by external , involve surface , , and that modify volcanic landforms over time. When or lava cools and solidifies, it forms igneous rocks, a category encompassing both intrusive rocks (crystallized underground) and extrusive rocks (formed at the surface), such as from basaltic lava flows. A common misconception is that volcanoes are always cone-shaped mountains; in reality, their forms vary widely, from broad shields to irregular fissures, and shape alone does not define a volcano, as some are simply vents without significant buildup. The term "volcano" itself derives from the Italian "vulcano," referencing the island of and the Roman Vulcan, but its modern usage emphasizes the geological rupture rather than mythological origins.

Geological Formation

Plate Tectonics Basics

The theory of plate tectonics posits that Earth's outermost layer, the lithosphere, is fragmented into a dozen or more large and small rigid plates that float on the semi-fluid asthenosphere beneath. These plates, which include both continental and oceanic crust, move relative to one another at rates of a few centimeters per year, driven primarily by thermal convection currents in the mantle. Mantle convection arises from heat generated by radioactive decay in Earth's core and residual heat from planetary formation, causing hotter, less dense material to rise and cooler, denser material to sink, creating slow-moving currents that drag the overlying plates. This plate motion plays a crucial role in volcanism by facilitating processes that generate . At convergent boundaries, occurs when one plate is forced beneath another, partially the descending slab and producing that rises to form volcanic arcs. At divergent boundaries, plates spread apart, allowing mantle material to upwell and partially melt due to decompression, creating new crust and mid-ocean ridge . Mantle plumes, buoyant upwellings of hot material from deep within the mantle, can also pierce plates and generate independently of plate boundaries, leading to intraplate . Key evidence supporting includes , first proposed by Harry Hess in 1960, which demonstrates symmetric magnetic stripes on ocean floors recording reversals in as new crust forms at ridges. distributions further corroborate the theory, with most occurring in narrow belts along plate boundaries, such as the circum-Pacific , where stresses from plate interactions accumulate and release. Modern GPS measurements provide direct observations of plate motion; for instance, the Pacific Plate moves northwestward at approximately 10 cm per year relative to the North American Plate.

Boundary Types

Volcanic activity at plate boundaries is driven by the interactions between tectonic plates, where facilitates generation through decompression or of subducted material. At divergent boundaries, plates move apart, allowing mantle material to partially melt and produce that erupts primarily as , forming new oceanic or . These settings include mid-ocean ridges, such as the , where frequent, effusive basaltic eruptions build submarine mountain chains over lengths exceeding 60,000 kilometers globally. In continental settings, divergent boundaries manifest as valleys, like the , where basaltic volcanism accompanies crustal thinning and extension, often leading to fissure eruptions and shield volcanoes. Convergent boundaries occur where one plate subducts beneath another, typically an oceanic plate descending into , which releases water-rich fluids that lower the of the overlying mantle wedge, generating that rises to form volcanic . These are chains of stratovolcanoes parallel to the , characterized by more explosive, andesitic to rhyolitic eruptions due to viscous magmas. A prominent example is the Andean Volcanic Arc, resulting from the of the Nazca Plate beneath the South American Plate at rates of about 6-10 cm per year, producing over 200 active volcanoes along the western edge of . Transform boundaries, where plates slide horizontally past each other along strike-slip faults, generally exhibit limited because the shearing motion does not promote significant mantle or . Instead, these zones are dominated by earthquakes, with rare unless the offsets a , as seen in where the Mid-Atlantic Ridge's spreading interacts with transform segments to sustain basaltic activity.

Hotspots and Rifts

Hotspots represent exceptions to plate boundary volcanism, occurring within tectonic plates due to mantle plumes—buoyant upwellings of abnormally hot mantle material rising from deep within the , often originating near the core-mantle boundary. This model, proposed by W. J. Morgan in 1971, explains persistent sites of excessive that generate volcanic activity independent of plate edges. Plumes create elevated temperatures of 100–300°C above surrounding mantle, promoting decompression as hot material ascends. As plates drift over these relatively fixed plumes, they produce linear chains of volcanoes with age progression reflecting plate motion. The Hawaiian-Emperor chain exemplifies this, spanning over 6,000 km across the Pacific Ocean with volcanoes aging progressively from the active Big Island of Hawaii northwestward at a rate of about 10 cm per year. Initial plume heads can trigger massive eruptions upon reaching the base, forming vast provinces like the , followed by sustained tail-driven hotspot tracks. Continental rifting drives through lithospheric extension and thinning, potentially evolving into new ocean basins as plates diverge. The System illustrates this ongoing process, where intrusion weakens the crust and facilitates breakup, influenced by underlying plumes like the Afar plume. In the Afar Depression, northern terminus of the , continental rifting transitions to akin to the and , with attenuated crust underlain by hot, low-velocity mantle. Active manifests in fissure eruptions and shield volcanoes, such as Erta Ale with its persistent , signaling advanced rifting stages. Magma compositions vary distinctly: hotspots favor tholeiitic basalts and flood basalts from high-degree melting of plume material, as seen in with SiO₂ contents of 36–52 wt%. In contrast, rifts produce alkaline lavas like basanites and phonolites due to lower-degree in the field under extensional conditions. The features such alkaline series, with high Na₂O + K₂O contents reflecting intraplate and rift dynamics.

Volcanic Landforms

Vent Types

Volcanic vents represent the initial openings in through which , gases, and pyroclastic materials are expelled during eruptions, broadly categorized into vents and central vents based on their and eruption style. vents form linear cracks, often spanning kilometers, while central vents are more localized conduits typically situated within craters or summits. These vent types serve as fundamental outlets that influence the scale and nature of volcanic activity, with their formation tied to tectonic stresses and dynamics. Fissure vents are elongated fractures in the crust through which low-viscosity basaltic erupts effusively, commonly associated with provinces where vast lava fields accumulate. These vents arise from the propagation of subsurface dikes, allowing to emerge along a linear zone rather than a single point, often producing curtain-like fire fountains initially that evolve into localized flows as the segments seal. A prominent example is the in , where a 27-km-long system of vents erupted from 1783 to 1784, releasing approximately 14 km³ of and contributing to widespread environmental impacts. Such vents are prevalent at divergent plate boundaries, where crustal extension facilitates fracture development. In contrast, central vents consist of single or clustered conduits that channel upward to a focused or location, facilitating the construction of conical landforms through repeated eruptions. These vents typically connect to underlying chambers via a pipe-like pathway, enabling both effusive and explosive activity depending on composition and gas content. For instance, many composite volcanoes feature a primary central vent at the , through which layered deposits of lava and accumulate over time. The dynamics of vent formation and activity involve magma ascent driven by , as less dense molten rock rises through the crust, eventually breaching the surface via fractures or conduits due to accumulated in storage chambers. Pressure release occurs as magma approaches the surface, promoting and volatile exsolution that can intensify eruptions, particularly in systems where rapid decompression along the fracture length sustains prolonged effusive flows. In central vents, this process concentrates energy, often leading to more explosive outcomes if volatiles are trapped until shallow depths.

Primary Volcano Shapes

Volcanoes exhibit distinct morphological shapes primarily determined by the of their erupted , the explosivity of eruptions, and the accumulation of materials over time. The four principal types—shield volcanoes, stratovolcanoes, cinder cones, and lava domes—represent the most common terrestrial forms, while supervolcanoes denote exceptional systems capable of cataclysmic events. These shapes arise from variations in composition, with basaltic magmas producing gentler forms and more silicic magmas leading to steeper or more explosive builds. Shield volcanoes form broad, gently sloping edifices characterized by low-angle profiles, often resembling a warrior's shield when viewed in profile. They develop through the repeated effusion of highly fluid basaltic lava, which flows great distances before cooling, allowing for wide lateral expansion rather than tall vertical growth. Slopes typically range from 2 to 10 degrees, and these volcanoes can reach immense sizes; for instance, in stands about 13,677 feet above and is considered the world's largest active volcano by volume. This morphology is common in intraplate hotspot settings, where ascends with minimal resistance. Stratovolcanoes, also known as composite volcanoes, build steep-sided, often symmetrical cones through alternating layers of viscous lava flows, pyroclastic deposits, and . The intermediate to magma composition promotes partial solidification and explosive eruptions, resulting in slopes of 30 to 40 degrees and heights up to 8,000 feet or more above their base. These layered structures make stratovolcanoes prone to sector collapses and lahars; in exemplifies this form, with its classic conical silhouette formed over millennia of such activity. Cinder cones are the simplest and smallest volcanic landforms, consisting of steep piles of loose pyroclastic fragments ejected from a single vent during mildly explosive eruptions of gas-rich basaltic to andesitic . These fragments, including and cinders, accumulate around the vent to form a bowl-shaped , with cones rarely exceeding 1,000 feet in height and slopes near 30 to 40 degrees. in , which emerged dramatically in a cornfield in 1943 and grew to 424 meters (1,391 feet) before ceasing activity in 1952, illustrates rapid cinder cone formation from Strombolian-style eruptions. Lava domes emerge as bulbous, steep-sided mounds when highly viscous, silica-rich rhyolitic or dacitic lava extrudes slowly from a vent and piles up without flowing far. The dome's surface often appears craggy due to fracturing from , and it may grow to hundreds of feet high and wide; for example, the Novarupta Dome in measures about 400 meters (1,300 feet) across and 70 meters (230 feet) tall. These features frequently form on the flanks of larger volcanoes or within calderas, posing hazards from collapse and associated pyroclastic flows. Supervolcanoes represent an extreme category, defined by their capacity for supereruptions rated at magnitude 8 on the (VEI), ejecting over 1,000 cubic kilometers of material and forming vast calderas through collapse. Unlike typical cone-shaped volcanoes, these systems lack prominent edifices and instead manifest as large depressions, with Yellowstone serving as a prime example due to its history of three such events, the most recent about 640,000 years ago. The immense scale of these eruptions can alter global climate and ecosystems for years.

Specialized Forms

Submarine volcanoes, also known as underwater or seafloor volcanoes, represent the majority of global volcanic activity, accounting for approximately 80% of Earth's eruptions. These features form primarily along mid-ocean ridges, volcanic arcs, and intraplate hotspots, where rises through the and interacts with . Unlike volcanoes, submarine eruptions produce distinctive landforms due to the quenching effect of water; for instance, basaltic lava cools rapidly upon extrusion, forming pillow lavas—elongated, sack-like structures with glassy exteriors and vesicular interiors that accumulate in flows or mounds. A prominent example is (formerly Lōʻihi), an active submarine off the southeastern coast of the Big Island of Hawaiʻi, which exhibits extensive pillow lava fields and rift zones built over the past 100,000 years, with fresh pillows observed during dives and seismic swarms indicating ongoing activity as of 2024. Hydrothermal vents often emerge from these submarine edifices, where circulates through fractured rock heated by , emerging as superheated, mineral-rich plumes that support unique chemosynthetic ecosystems, though the vents themselves are secondary to the volcanic structure. Subglacial volcanoes occur beneath thick ice sheets or glaciers, leading to specialized eruptive dynamics driven by magma-ice interactions. In these environments, molten lava contacts , causing rapid and the generation of substantial volumes, which can accumulate in subglacial lakes before sudden drainage. This results in jökulhlaups, catastrophic glacier outburst floods that release pressurized , , and volcanic debris, often with peak discharges exceeding 10,000 cubic meters per second and capable of traveling tens of kilometers. A key example is volcano in Iceland's , where subglacial eruptions, such as the 1996 event, have triggered major jökulhlaups by overlying up to several cubic kilometers in volume, producing (glass-rich fragmental deposits) from explosive interactions and altering river courses with loads up to 10^8 tons per event. These eruptions highlight the hazards of subglacial settings, including rapid flood propagation and atmospheric ash dispersal when barriers breach. Cryptodomes form when viscous magma intrudes shallowly into a volcano's edifice without breaching the surface, creating a subsurface bulge that deforms the overlying rock and can destabilize the structure. This intrusion typically involves silicic to intermediate magmas that stall due to high viscosity and degassing, leading to visible surface swelling, faulting, and increased seismicity as pressure builds. The most notable historical example is the 1980 eruption of Mount St. Helens in Washington, USA, where a growing andesitic cryptodome caused a northern flank bulge that reached about 140 meters of horizontal displacement and 30 meters of vertical uplift over two months, ultimately triggering a sector collapse that initiated the lateral blast, releasing over 2 cubic kilometers of material. Such features underscore the role of cryptodomes in transitioning from effusive to explosive activity, often preceding major hazards like debris avalanches.

Associated Hydrothermal Structures

Hydrothermal structures represent non-eruptive surface manifestations of volcanic heat, where groundwater interacts with magmatic sources to produce steam, gases, and fluids without direct magma extrusion. These features form in volcanic regions when heat from underlying magma chambers or cooling intrusions warms subsurface water, leading to phase changes and pressure buildup that drive emissions through fractures and vents. They are prevalent in areas like Yellowstone National Park and the Campi Flegrei caldera, serving as indicators of ongoing subsurface volcanic activity. Fumaroles are vents or fissures in volcanic terrains that emit hot gases, primarily steam mixed with volcanic volatiles such as , , and . These emissions occur as from heated aquifers flashes to upon reaching the surface, often accompanied by a characteristic sulfurous odor and temperatures exceeding 100°C. Fumaroles are fed by conduits that extend through the , allowing gases from magmatic sources to escape without significant water discharge. A prominent example is the Solfatara crater in the Phlegrean Fields of , where persistent fumarolic activity has been monitored since the 1980s, with gas compositions reflecting interactions between magmatic fluids and . Geysers are specialized hot springs that erupt periodically, ejecting columns of boiling water and due to the buildup of pressure in subsurface reservoirs. The mechanism involves percolating into hot , where it superheats and partially vaporizes; when pressure exceeds the strength of overlying rock plugs, rapid steam flashing propels the water upward in bursts. This process is powered by heat from nearby bodies, with eruption intervals varying from minutes to days based on recharge rates and conduit geometry. in exemplifies this, erupting approximately every 90 minutes with water heights up to 55 meters, driven by a complex plumbing system where expansion triggers the discharge. Mud volcanoes, distinct from igneous volcanoes, form through the mobilization and eruption of fine-grained sediments mixed with water and gases from overpressured subsurface layers, rather than molten silicate magma. These structures arise in tectonically active sedimentary basins where hydrocarbons or other fluids generate pore pressures that liquefy clays and silts, forcing slurries to the surface through vents or cones; the resulting features can reach heights of several meters and emit methane-rich gases. Unlike true volcanic edifices sourced from mantle-derived melts, mud volcanoes involve diagenetic and tectonic processes in accretionary prisms or basins, often without direct magmatic involvement. The mud volcano province, hosting over 400 such features in the South Caspian Basin, illustrates this, with eruptions of mud breccias and flames from ignited hydrocarbons providing insights into regional fluid migration.

Erupted Materials

Volcanic Gases

Volcanic gases are volatile compounds dissolved in that are released during volcanic activity, primarily through at vents, fumaroles, and during eruptions. These gases play a crucial role as precursors to other eruptive materials by influencing buoyancy and pressure buildup. The composition varies by type and eruption style, but common emissions include , , , and , alongside trace amounts of other species. Water vapor constitutes the dominant component, typically comprising 70 to 90 percent of emissions by volume, derived from hydration in the source. follows as a significant gas, often 5 to 15 percent, while and each contribute around 1 to 5 percent and 0.1 to 1 percent, respectively, depending on the volcano's geochemical setting. Trace gases include such as and , as well as minor amounts of , , and volatile metals like mercury and , which are emitted in gaseous or form. Sulfur dioxide emissions react with atmospheric water and oxygen to form sulfuric acid aerosols, leading to acid rain that can corrode infrastructure, damage vegetation, and contaminate water supplies by leaching metals like lead from roofing and plumbing. These same aerosols scatter sunlight, causing short-term ; for instance, the released massive SO₂ volumes, forming a stratospheric veil that lowered temperatures by up to 3°C and triggered the "" in 1816, with crop failures and famine. , though a , contributes minimally to long-term warming compared to anthropogenic sources, while water vapor has negligible direct climatic impact due to its short atmospheric . The exsolution of these gases from rising can drive explosive eruptions by rapidly expanding bubble volumes. Measurement techniques include remote , such as (UV) spectrometry for SO₂ flux via plume transects from ground vehicles or aircraft, and (FTIR) for multi-gas including CO₂, HCl, and HF. Direct plume sampling involves collecting gases in evacuated flasks or bubblers at fumaroles for of ratios and isotopes, providing insights into dynamics.

Lava Flows

Lava flows consist of molten rock, or that has reached the Earth's surface, exhibiting behavior that allows it to advance across landscapes as a continuous rather than fragmented . These flows vary significantly in morphology and mobility based on their , primarily the silica content, which dictates —the resistance to flow. Basaltic lavas, with low silica content (around 45-52%), are highly and produce extensive, relatively thin flows, whereas more silica-rich lavas, such as andesitic or rhyolitic (over 60% silica), are viscous and form shorter, thicker accumulations. Among basaltic flows, two primary surface types dominate: pāhoehoe and 'a'ā. Pāhoehoe features a smooth, ropy, or billowy texture formed by the folding of the flow's skin as it advances slowly over gentle slopes, preserving gas bubbles and within a less sheared structure. In contrast, 'a'ā develops a rough, jagged, blocky surface due to increased shear and disruption, often resulting from faster movement or slight cooling that breaks the crust into spiny fragments, with the underlying material remaining more crystalline and gas-poor. These morphologies can transition within a single flow field, influenced by terrain and eruption rate. The mechanics of lava flow advancement depend on , , and , with basaltic lavas typically progressing at rates of less than 1 km per hour on flat ground, though exceptional cases on steep inclines can reach up to 10 km per hour, equating to tens of kilometers per day under optimal conditions. As flows advance, they cool primarily through conduction and , losing heat to the air and substrate at rates that solidify the outer layer within hours to days, forming a crust that insulates the molten interior. Upon complete solidification, basaltic flows often develop —hexagonal fractures perpendicular to the cooling surface—due to contraction, with column thickness reflecting cooling pace: thicker columns (up to 1-2 meters) from slower cooling in thick flows and thinner ones from rapid surface chilling. flows, quenched by water, solidify into rounded forms, where successive lobes form as the exterior rapidly solidifies while the interior remains . A notable example of viscous, silica-rich flows occurred during the 1980-1986 eruptions at , where dacitic lavas (63-68% silica) extruded slowly to form a growing rather than extensive flows, advancing at mere centimeters per day due to high and frequent collapses, ultimately reaching heights over 300 meters within the crater.

Pyroclastic Materials

Pyroclastic materials, also known as , consist of fragmented rock and ejected into the atmosphere during explosive volcanic eruptions, resulting from the rapid expansion of magmatic gases that shatter the material into airborne particles. These fragments vary widely in size and shape, forming the primary solid products of such events, distinct from fluid lava flows. Tephra is classified primarily by particle size based on the intermediate axis dimension. comprises particles smaller than 2 mm, often consisting of fine , , and lithic fragments that can remain suspended in the atmosphere for extended periods. Lapilli range from 2 to 64 mm, typically pea- to walnut-sized and resembling volcanic cinders, which may accrete into larger forms in moist conditions. Particles larger than 64 mm are termed bombs if derived from molten , exhibiting aerodynamic shapes due to in-flight rotation, or blocks if they are solid, angular fragments of pre-existing rock. Pyroclastic deposits form through various transport mechanisms, including fallout, flows, and surges. Tephra fallout occurs when particles settle directly from eruption plumes, creating layered deposits that are coarser near the vent and finer with distance, such as from Strombolian eruptions or from Plinian events. Pyroclastic flows, historically called nuées ardentes, are dense, ground-hugging avalanches of hot , , blocks, and gas traveling at speeds of tens of meters per second (hundreds of kilometers per hour) and temperatures exceeding 800°C. Pyroclastic surges are more dilute, low-density currents of and gas that expand laterally and can overrun , depositing thin, widespread layers with . A notable example is the 1980 eruption of , where a lateral blast generated a that devastated over 600 square kilometers, followed by pumice-rich flows and widespread ash fallout that blanketed areas up to hundreds of kilometers away. The exsolution of volcanic gases from rising triggered the fragmentation that produced these materials. The scale of pyroclastic production is quantified by the (VEI), a from 0 to 8 that assesses eruption intensity based on volume (from less than 10,000 cubic meters for VEI 0 to over 1,000 cubic kilometers for VEI 8), plume height, and duration. The event registered as VEI 5, illustrating a "very large" eruption capable of generating substantial pyroclastic volumes.

Eruptions and Activity

Eruption Mechanisms

Volcanic eruptions are fundamentally driven by the movement of from depth to the surface, where differences in magma properties determine whether the eruption is effusive or explosive. Effusive eruptions occur when low-, gas-poor basaltic magma flows out gently, forming lava flows without significant fragmentation, as seen in Hawaiian-style activity. In contrast, explosive eruptions result from high-, gas-rich silicic magmas that trap volatiles until rapid decompression causes fragmentation into pyroclastic materials like . The key factors influencing this are magma viscosity, which resists gas escape in rhyolitic compositions, and dissolved gas content, typically higher in more evolved magmas, leading to violent expansion upon ascent. Specific eruption styles illustrate these mechanisms. Strombolian eruptions involve mild explosions from moderately viscous basaltic with moderate gas content, producing rhythmic bursts of pyroclasts ejected to heights of hundreds of meters, as observed at volcano. These differ from Plinian eruptions, the most intense explosive style, where highly viscous, gas-saturated silicic generates towering eruption columns exceeding 30 kilometers, driven by efficient magma fragmentation and sustained gas thrust, exemplified by the 79 CE Vesuvius event. In both cases, the outcome links directly to erupted materials: effusive styles yield coherent lava, while explosive ones produce abundant ash and , influencing atmospheric and depositional impacts. Eruptions are triggered by processes that destabilize the magma system. Magma mixing, where hotter mafic magma intrudes cooler silicic reservoirs, induces , superheating, and rapid vesiculation, prompting explosive release, as documented in the 2006 Augustine Volcano eruption. Decompression occurs as magma ascends, reducing pressure and causing exsolved gases to expand violently, with rates up to 0.45 MPa/s during intense events at . External water interaction, such as heated by intruding magma, drives or phreatomagmatic explosions through steam generation, without fresh magma involvement in purely phreatic cases. Precursors to eruptions provide critical warnings through observable changes. , including volcano-tectonic earthquakes from magma-induced rock fracturing, often intensifies as moves upward, as monitored at U.S. volcanoes. Ground deformation, detected via GPS and satellite , signals inflation or dyke propagation, with rates accelerating before events like the 2004-2006 activity. Spikes in emissions, such as increased SO₂ or CO₂ from fumaroles, indicate from rising , serving as an early indicator of unrest.

Activity Stages

Volcanoes are classified into stages of activity based on their eruptive history and potential for future eruptions, providing a framework for understanding their current state and associated risks. These stages—erupting, active, dormant, and extinct—reflect the volcano's interaction with underlying sources and geological processes, though definitions can vary slightly among volcanologists due to the irregular nature of volcanic behavior. An erupting volcano is actively emitting lava, ash, or gases from its vents, often in episodes that can last days to decades. For instance, in underwent a prolonged eruption from 1983 to 2018, characterized by steady lava flows that reshaped the landscape and added over 500 square miles of new land. As of 2025, continues to erupt intermittently, with lava fountains reaching heights of up to 1,246 feet in June, demonstrating ongoing magmatic activity within the crater. Active volcanoes have erupted within the epoch, generally within the last 10,000 years, indicating a persistent source and high potential for future activity, even if not currently erupting. This category encompasses about 1,500 volcanoes worldwide, with examples including in the United States, which erupted catastrophically in after centuries of quiet. Such volcanoes may exhibit precursors like seismic swarms or gas emissions, signaling possible reactivation. Dormant volcanoes show no recent eruptions but maintain geothermal activity, such as hot springs or fumaroles, suggesting an intact magma pathway that could lead to future events. These differ from extinct volcanoes, which lack any magma connection due to crustal changes and are often represented by deeply eroded ancient cones. Mount Thielsen in exemplifies an extinct volcano, with its jagged peak formed by erosion of a long-dormant that last erupted over 250,000 years ago. Volcanoes can transition between stages through reactivation, as seen with in the , which erupted explosively in after 43 years of , producing ash plumes and pyroclastic flows that affected nearby communities. This event highlights how dormant systems can abruptly shift to erupting states when ascends, underscoring the importance of recognizing potential in geothermally active features.

Monitoring and Classification

Volcanic monitoring employs a suite of geophysical and geochemical instruments to detect precursors of unrest, such as magma movement and pressure changes beneath the surface. Seismometers are deployed in networks around volcanoes to record seismic tremors and earthquakes, which often signal the fracturing of rock by ascending or migration. Tiltmeters and strainmeters measure subtle ground surface tilting and deformation, indicating or as magma chambers fill or empty. These ground-based tools provide continuous, essential for early detection of activity changes. Satellite-based (InSAR) complements terrestrial methods by mapping large-scale ground deformation over remote or inaccessible areas, revealing uplift or subsidence patterns associated with volcanic processes. Gas sensors, including spectrometers and multi-gas analyzers, monitor emissions of , , and other volatiles from fumaroles, soil, or plumes, as increases in gas flux can precede eruptions by indicating from rising . Techniques range from direct sampling with evacuated flasks to via aircraft or satellites, allowing assessment of gas composition and emission rates even during hazardous conditions. Classification and alert systems standardize the communication of volcanic threats based on monitoring data. The U.S. Geological Survey (USGS) employs a four-level alert system paired with aviation color codes: Normal/Green for background activity, Advisory/ for elevated unrest, Watch/Orange for eruption likely within weeks, and Warning/Red for imminent or ongoing major eruption with hazards. This framework informs public safety responses and aviation restrictions by integrating seismic, deformation, and gas observations. Globally, networks like WOVOdat, maintained by the World Organization of Volcano Observatories, compile standardized unrest data from observatories worldwide to enhance eruption and research. The initiative, launched by the International Association of Volcanology and Chemistry of the Earth's Interior (IAVCEI) in the 1990s, designates 16 high-risk volcanoes for intensified monitoring and study due to their eruptive history, proximity to populations, and potential for catastrophic impacts. Examples include in , which threatens densely populated areas around , prompting advanced seismic and gas networks. This program fosters international collaboration, , and development of strategies for these priority sites.

Human Impacts

Geological Hazards

Volcanic geological hazards encompass a range of direct physical threats posed by eruptive processes, including rapid mass movements, inundation by molten material, and atmospheric disruptions that can lead to widespread environmental impacts. These hazards arise primarily from the interaction of volcanic materials with the surrounding and atmosphere, often resulting in immediate destruction and, in some cases, prolonged secondary effects. Among the most lethal are lahars, tsunamis triggered by events, pyroclastic density currents, and lava flows, each capable of devastating human settlements and ecosystems with little warning. Lahars, or volcanic mudflows, form when heavy rainfall or glacial melting mixes with loose and debris, creating fast-moving slurries of water, sediment, and rock that can travel tens of kilometers downstream at speeds exceeding 50 km/h. These flows are particularly hazardous in river valleys near volcanoes, as they bury communities under meters of abrasive material, destroying infrastructure and agriculture. A tragic example occurred during the 1985 eruption of in , where lahars triggered by the melting of summit ice caps surged through the town of , killing over 23,000 people in a matter of hours. Tsunamis generated by volcanic activity typically result from collapses, explosive underwater eruptions, or large flank landslides that displace massive volumes of water. These waves can propagate across oceans or seas, inundating coastlines with heights up to 30 meters or more, leading to catastrophic flooding and loss of life far from the eruption site. The in exemplifies this hazard, as the partial collapse of the volcano's flanks into the generated that razed 165 coastal villages on and , claiming over 36,000 lives, with more than 34,000 deaths directly attributed to the waves. Lava flows and pyroclastic density currents represent intense, ground-hugging threats from effusive and eruptions, respectively. Lava inundation occurs when molten rock advances slowly but relentlessly, engulfing and incinerating everything in its path due to temperatures reaching 1,200°C, though flows rarely cause direct fatalities owing to their predictability and lower speeds. In contrast, pyroclastic density currents—searing avalanches of hot gas, ash, and rock fragments—propel downslope at hundreds of km/h, incinerating, abrading, and burying landscapes in seconds, and have accounted for nearly one-third of historical volcanic fatalities. On longer timescales, massive eruptions can inject vast quantities of and aerosols into the , blocking and inducing a "" that cools global temperatures and disrupts . This climatic perturbation can persist for years, leading to crop failures and widespread ; the extreme event of 536 CE, likely triggered by a major eruption, caused summer temperatures in to drop by about 2.5°C below average, exacerbating food shortages and contributing to in affected regions.

Societal Benefits

Volcanoes contribute significantly to human society through the formation of nutrient-rich soils derived from the of . When volcanic eruptions deposit ash layers, these materials, rich in minerals such as , , and magnesium, undergo rapid chemical due to their high content and porosity, leading to the development of Andosols—highly fertile soils characterized by excellent water retention, low , and high content. This process enhances and availability, supporting intensive agriculture in volcanic regions. In , , terraced Andosols formed from weathered ash have enabled extensive paddy rice cultivation, sustaining dense populations and contributing to the island's role as a major agricultural hub. Similarly, in , from eruptions around and other centers has created productive soils in the region near , where farming thrives despite challenging climates elsewhere in , supporting crops like vineyards and orchards that form the backbone of local economies. Beyond agriculture, volcanic activity provides a renewable source of , harnessing heat from chambers and hot springs for electricity generation and heating. In , located on the with frequent volcanic activity, plants utilize steam and hot water from volcanic sources to produce approximately 30% of the nation's electricity as of 2025, while also supplying nearly 90% of residential heating needs. This sustainable energy system reduces reliance on fossil fuels and has positioned as a global leader in , with geothermal resources enabling efficient, low-emission power production that supports industrial applications like aluminum . Volcanic processes also yield valuable mineral resources through hydrothermal systems, where hot fluids circulating in the concentrate metals into economically viable deposits. Porphyry copper deposits, a of global production, form when magmatic-hydrothermal fluids emanating from volcanic intrusions dissolve and transport metals, precipitating them in stockwork veins within altered host rocks. These deposits, often associated with zone , account for about 60% of the world's supply and significant portions of and , with examples like the in exemplifying the scale of extraction enabled by ancient volcanic activity.

Risk Management

Risk management for volcanic activity involves a range of strategies aimed at minimizing threats to human life, property, and economies through proactive planning and response measures. Evacuation planning and zoning are critical components, particularly in regions with frequent eruptions like , where lava flow hazard zones are delineated based on historical eruption patterns and geological features. These zones, ranging from Zone 1 (highest risk, covering summits and rift zones of volcanoes like and ) to Zone 9 (lowest risk, areas inactive for over 10,000 years), guide land-use restrictions and emergency evacuations to prevent inundation by lava flows. For instance, 's zoning system, established by the U.S. Geological Survey (USGS) in the 1970s and updated in the , informs building codes and informs residents of potential risks, with Zone 2 areas facing up to a 15-100% probability of coverage in 100 years. solutions, such as lava flow diversion barriers, complement zoning; in , earthen barriers and dikes have been constructed to protect key , as seen in 1986 when structures delayed flows near during an eruption. Early warning systems play a pivotal role by integrating real-time monitoring data to forecast eruptions and trigger timely evacuations. The USGS National Volcano (NVEWS), authorized in 2019, prioritizes monitoring for 57 high-threat U.S. volcanoes based on hazard potential and population exposure, using seismic, gas, and deformation sensors to provide alerts through a five-level threat ranking from very low to very high. This system builds on established monitoring techniques to disseminate information via partnerships with emergency managers, enabling communities to activate evacuation protocols before hazards escalate. Public education enhances these efforts, with programs at sites like promoting awareness through events such as Volcano Awareness Month, where rangers and USGS scientists conduct seminars, hikes, and exhibits on eruption preparedness and safe viewing practices. These initiatives, including downloadable resources and school outreach, foster community resilience by teaching recognition of warning signs and response actions. Insurance mechanisms and economic recovery planning address post-eruption financial burdens, ensuring long-term societal stability. Parametric insurance, which triggers payouts based on predefined event parameters like eruption intensity, has been explored for volcanic risks to provide rapid liquidity for recovery, as outlined in World Bank assessments for small island nations prone to eruptions. The 2010 Eyjafjallajökull eruption in Iceland exemplifies global economic vulnerabilities, canceling 104,000 flights and disrupting aviation across Europe, resulting in approximately $1.6 billion in lost tourism revenue over eight days. In response, affected regions bolstered resilience through coordinated recovery plans; for Hawaii's 2018 Kīlauea eruption, which destroyed over 700 homes and displaced thousands, a multi-year economic recovery strategy emphasized rebuilding infrastructure, supporting displaced businesses, and diversifying tourism to mitigate ongoing losses estimated at hundreds of millions of dollars, with recovery costs exceeding $800 million. Such frameworks, often involving federal aid and private insurance, prioritize swift resource allocation to restore economic activity while incorporating lessons from past events.

Extraterrestrial Volcanism

Solar System Examples

Volcanic activity on Mars is exemplified by the region, a vast topographic bulge spanning approximately 3,000 miles (5,000 kilometers) across and rising up to 4 miles (6 kilometers) above the planetary average, formed by extensive volcanic construction over billions of years. This region hosts some of the largest shield volcanoes in the solar system, including , which stands about 22 kilometers (14 miles) high above the surrounding plain and covers a base diameter exceeding 600 kilometers (370 miles), making it the tallest known volcano in the solar system. Observed landforms include broad, gently sloping shields built from low-viscosity basaltic lavas, with featuring a massive complex up to 80 kilometers wide and surrounded by aureole deposits of collapsed slopes. Jupiter's moon Io exhibits the most intense volcanic activity in the solar system, driven by from gravitational interactions with and neighboring moons Europa and Ganymede, which flex the moon's interior and generate internal heat exceeding 20 times that of per unit area. This results in over 400 active volcanoes, producing sulfur-rich lavas and explosive plumes that reach heights of up to 500 kilometers, resurfacing the moon's surface in as little as a century. A prominent example is , the largest known in the solar system, spanning about 200 kilometers across with a shield-shaped that periodically erupts, emitting output detectable from and contributing to Io's colorful, sulfur-frosted landscape of paterae (caldera-like depressions) and extensive flow fields. On , volcanic landforms are revealed through radar imaging due to the planet's thick atmosphere, with serving as a key example of a massive rising about 8 kilometers (5 miles) above the surrounding plains and featuring broad lava flows extending hundreds of kilometers. NASA's Magellan mission radar data from the early detected changes in a summit vent of , including enlargement and altered shape over an eight-month period, providing direct evidence of an eruptive event and implying recent resurfacing activity within the geologically recent past of a few hundred thousand years. Subsequent analysis in 2024 identified two more volcanoes with evidence of eruptions in the early , further confirming Venus's active volcanism. The volcano's edifice, similar in scale to Earth's Hawaiian shields but with steeper slopes, highlights Venus's global volcanic resurfacing, where such features contribute to the planet's youthful terrain dominated by plains and coronae.

Comparative Geology

Extraterrestrial volcanism differs markedly from Earth's due to variations in , tectonic regimes, and surface conditions, which influence the scale, style, and persistence of volcanic features. On Mars and the , lower —approximately 0.38g and 0.17g of 's, respectively—permits the accumulation of taller volcanic edifices than those possible on Earth, where stronger gravitational forces limit height through isostatic adjustment and erosion. For instance, Mars' reaches a height of about 22 km above the surrounding plain, far exceeding Earth's tallest volcano, , at roughly 10 km from its base, because Martian can rise higher before collapsing under its own weight, and the absence of erosive processes like rainfall preserves these structures. Similarly, the 's basaltic domes, such as those in the Marius Hills, exhibit steeper slopes and greater relief relative to their volume compared to terrestrial analogs, as low reduces slumping during emplacement. The lack of active plate tectonics on Venus and Mars further promotes hotspot-dominated volcanism, contrasting with Earth's mobile plate regime that disperses volcanic activity along spreading centers and zones. Mars' ancient volcanism, now largely quiescent, was concentrated in fixed hotspots like the region, where stationary mantle plumes built massive shield volcanoes over billions of years without crustal recycling or plate migration to shift the vents. Venus operates under a stagnant lid tectonic mode, where the rigid inhibits widespread , leading to episodic resurfacing via widespread hotspot plumes that form coronae and large volcanic rises, such as Beta Regio, rather than linear island chains like Earth's Hawaiian hotspot track. This hotspot dominance on both bodies results in prolonged activity at single sites, enabling the development of immense volcanic provinces that cover up to 50% of Mars' surface and dominate Venus' global topography. In comparison, Earth's hotspots, such as those underlying Yellowstone, produce similar plume-driven features but are interrupted by plate motion. Cryovolcanism represents a distinct extraterrestrial process absent on , involving the eruption of volatile ices and fluids rather than magmas, driven by in icy satellites. On Saturn's moon , cryovolcanic plumes eject a of , ice particles, and trace volatiles including and from subsurface reservoirs, forming up to 250 km high at the ; these plumes originate from a global beneath the ice shell, where lowers the freezing point and facilitates fluid mobilization. Unlike 's -based eruptions, this process relies on pressure buildup from dissolved gases and cryomagma ascent through fractures, highlighting how lower temperatures and compositions in outer solar system bodies yield explosive, plume-dominated activity. Volcanic outgassing on extraterrestrial bodies plays a crucial role in atmosphere formation and potential , providing volatiles essential for retaining heat and enabling liquid . On and early Mars, degassing from mantle plumes released CO2, , and compounds that built thick atmospheres, with Mars' contributing to a denser early atmosphere capable of supporting transient liquid and prebiotic chemistry before much was lost to space. For icy moons like , cryovolcanic supplies organic molecules and energy sources to the surface, potentially sustaining subsurface habitats by recycling nutrients between the and ice shell, thus enhancing prospects for microbial life in isolated environments. These processes underscore how , modulated by planetary conditions, can create habitable niches beyond Earth's plate-driven cycle.

Historical Perspectives

Early Observations

In ancient Greek mythology, volcanoes were often linked to the god , the deity of fire, metalworking, and craftsmanship, whose subterranean forge was believed to cause eruptions through his laborious activities deep beneath the earth. This association portrayed volcanic activity as a manifestation of divine craftsmanship rather than random natural force, with Hephaestus's workshop imagined under sites like Mount Etna in . The Romans adapted this concept, equating Hephaestus with Vulcan, whose forge was similarly placed beneath Etna, as recorded in ancient texts describing the mountain's frequent eruptions as the god's fiery outbursts. A pivotal early observation came from the Roman author Pliny the Younger, who provided the first detailed eyewitness account of a major volcanic eruption in his letters to the historian Tacitus describing the 79 CE destruction of Pompeii and Herculaneum by Mount Vesuvius. Pliny depicted the event as a towering pine-shaped plume of ash and pumice rising from the volcano, followed by earthquakes, darkness, and pyroclastic flows that buried the cities, emphasizing the terror and scale without attributing it to mythology. His narrative, based on personal observations from across the Bay of Naples, marked a shift toward empirical description amid the era's prevailing supernatural interpretations. During the medieval period, volcanic eruptions were predominantly viewed through a Christian lens as acts of divine punishment or portents of apocalypse, with chroniclers interpreting lava flows and ash clouds as signs of God's wrath against human sinfulness. This perception framed volcanoes as gateways to hell, evoking biblical imagery of fire and brimstone, and prompted communal responses like processions and penance to avert further calamity. For instance, the 1783–1784 Laki eruption in Iceland produced a persistent "dry fog" of sulfurous haze that spread across Europe, causing crop failures, livestock deaths, and widespread famine; contemporary accounts described it as a supernatural mist signaling divine displeasure, exacerbating mortality rates without scientific explanation. By the mid-18th century, perceptions began evolving toward more systematic observation, exemplified by British diplomat Sir William Hamilton's explorations of starting in the 1760s. Upon arriving in as envoy in 1764, Hamilton documented eruptions including the 1760-1761 event through sketches by his artist Pietro Fabris and his own ascents during active phases starting in 1766, documenting lava flows, crater changes, and seismic activity through sketches and letters to the Royal Society. His work, culminating in the illustrated Campi Phlegraei (1776–1779), shifted focus from divine origins to natural processes, treating Vesuvius as a dynamic geological feature worthy of empirical study.

Modern Scientific Advances

In the 19th century, foundational advances in volcanology emphasized empirical observation and gradualist principles. Charles Lyell's Principles of Geology (1830–1833) promoted uniformitarianism, arguing that volcanic features formed through ongoing processes like lava flows and erosion, rather than sudden catastrophes, thereby establishing a framework for interpreting ancient volcanic rocks as products of modern mechanisms. This approach influenced subsequent studies by integrating volcanoes into broader geological histories, such as the uplift and subsidence of landforms. Concurrently, Alexander von Humboldt's fieldwork on Mount Vesuvius involved systematic measurements of fumarole temperatures, gas emissions, and seismic activity during his 1823 visit, providing early quantitative data on volcanic heat dynamics and inspiring interdisciplinary connections between geology, meteorology, and ecology. These efforts shifted volcanology from descriptive accounts toward process-oriented science. A pivotal moment came in 1912 with the eruption in , the largest of the 20th century, which ejected over 15 cubic kilometers of and caused the collapse of Katmai volcano's summit to form a 3-kilometer-wide —the first such feature explicitly recognized as resulting from evacuation during explosive activity. This event, documented through post-eruption surveys, highlighted the role of rhyolitic magmas in plinian eruptions and advanced understanding of caldera-forming processes. The mid-20th century saw transformative theoretical and technological progress. The paradigm, solidified in the 1960s through evidence from and distributions, explained volcanic arcs as products of zones where oceanic plates recycle into , generating melts that rise to form island chains like the Aleutians. This unified global volcanism under dynamics, resolving prior puzzles about hotspot chains like . Complementing this, —developed from the 1970s onward—enabled three-dimensional imaging of subsurface velocities to delineate chambers, such as the low-velocity zones beneath Yellowstone indicating partial melts at depths of 5–15 kilometers. Into the , and computational tools have enhanced real-time monitoring and prediction. Unmanned aerial vehicles (drones) equipped with multispectral cameras and gas sensors now access craters and plumes safely, capturing high-resolution thermal data during eruptions like those at , reducing risks to scientists while providing continuous datasets for hazard assessment. , particularly algorithms trained on seismic and geodetic , has improved eruption forecasting by detecting subtle precursors like velocity changes, achieving up to 80% accuracy in classifying unrest phases across diverse volcanoes. The 2021 eruption on , lasting 85 days and displacing 7,000 residents, yielded critical insights into , revealing how fissure propagation and lateral magma migration interact with pre-existing faults to sustain prolonged effusive activity. Satellite missions using (InSAR), such as those from the European Space Agency's , support global tracking by measuring centimeter-scale surface deformations over wide areas, aiding detection of precursory inflation at remote volcanoes. Recent developments as of 2025 include studies of the 2022 Hunga –Hunga Ha'apai eruption, which provided new insights into submarine formation and the injection of into the , influencing global climate models. Advances in have further refined forecasting, with models achieving over 90% accuracy in some cases for short-term predictions using multi-parameter data integration.

References

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