{"id":479,"date":"2017-09-19T20:56:33","date_gmt":"2017-09-20T00:56:33","guid":{"rendered":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/chapter\/11-2-materials-produced-by-volcanic-eruptions\/"},"modified":"2021-07-30T22:14:00","modified_gmt":"2021-07-31T02:14:00","slug":"11-2-materials-produced-by-volcanic-eruptions","status":"publish","type":"chapter","link":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/chapter\/11-2-materials-produced-by-volcanic-eruptions\/","title":{"raw":"11.2 Materials Produced by Volcanic Eruptions","rendered":"11.2 Materials Produced by Volcanic Eruptions"},"content":{"raw":"Volcanic eruptions produce three types of materials: gas, lava, and fragmented debris called <strong>tephra<\/strong>.\r\n<h1>Volcanic Gas<\/h1>\r\nMagma contains gas. Most of the gas emitted by volcanoes is water, but gas also contains carbon dioxide (CO<sub>2<\/sub>), sulphur dioxide (SO<sub>2<\/sub>), and hydrogen sulphide (H<sub>2<\/sub>S), in order of decreasing abundance.\r\n\r\n.At high pressures, the gases are dissolved in the magma, but if the pressure decreases, the gas comes out of solution, forming bubbles, similar to what happens when you open a bottle of pop. Pop is bottled under pressure, forcing carbon dioxide gas to dissolve into the fluid. As long as the bottle is closed and the pressure remains high, you'll see few to no bubbles in the pop. But if you open the bottle, air rushes out, decreasing the pressure on the pop. The pop will begin to fizz as carbon dioxide gas comes out of solution and forms bubbles.\r\n\r\nVolcanoes release gases when erupt, and through openings called <strong>fumaroles <\/strong>(Figure 11.7). They can also release gas into soil and groundwater.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_464\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS.jpeg\" rel=\"attachment wp-att-709\"><img class=\"wp-image-464\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS.jpeg\" alt=\"A fumarole at Pu\u02bbu \u02bb\u014c\u02bb\u014d Crater. Hawaii. The yellow crust along the margin of the fumarole is made of sulphur crystals. The crystals form when sulphur vapour cools as it is released from the fumarole. Source: U. S. Geological Survey (2016) Public Domain\" width=\"500\" height=\"333\" \/><\/a> <strong>Figure 11.7<\/strong> A fumarole at Pu\u02bbu \u02bb\u014c\u02bb\u014d Crater, Hawaii. The yellow crust along the margin of the fumarole is made of sulphur crystals. The crystals form when sulphur vapour cools as it is released from the fumarole. Source: U. S. Geological Survey (2016), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/23998018863\/in\/album-72157637377510893\/\" target=\"_blank\" rel=\"noopener noreferrer\">View source<\/a><em>.<br \/><\/em>[\/caption]\r\n<h1>Lava<\/h1>\r\nThe ease with which lava flows, and the structures it forms depend on how much silica and gas are in the lava. The more silica, the more <strong>polymerization\u00a0<\/strong>(formation of long molecules) happens, stiffening the lava. The stiffness of lava is described in terms of <strong>viscosity:<\/strong> lava that flows easily has low viscosity, and lava that is sticky and stiff has high viscosity.\r\n\r\nIn general, higher-silica (felsic) lava contains more gas than low-silica lava. When the gas forms into bubbles, viscosity increases further. Consider the pop analogy again: If you shook the bottle vigorously, then opened it, the pop would gush out in a thick, frothy flow. In contrast, if you took care to not shake the bottle before opening it, you could pour out a thin stream of fluid. The presence of gas not only makes high-silica lava more viscous, but can affect mafic lavas in that way as well.\r\n\r\n&nbsp;\r\n<div class=\"textbox shaded\">\r\n\r\n<strong>Concept Check: Viscosity<\/strong>\r\n\r\n[h5p id=\"229\"\r\n\r\n<\/div>\r\n<h2>Chemical Composition Affects the Thickness and Shape of Lava Flows<\/h2>\r\n<div class=\"textbox shaded\">\r\n\r\n<strong>A Quick Review Before You Continue<\/strong>\r\n\r\n[h5p id=\"230\"]\r\n\r\n<\/div>\r\n&nbsp;\r\n\r\nThe thickness and shape of a lava flow depends on its viscosity. The greater the viscosity, the thicker the flow, and the shorter the distance it can go before solidifying. Highly viscous lava might not flow very far at all, and simply accumulate as a bulge, called a <strong>lava dome<\/strong>, in a volcano\u2019s crater. Figure 11.8 shows a dome formed from rhyolitic lava in the crater of Mt. St. Helens.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_465\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn.jpeg\"><img class=\"wp-image-465\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn.jpeg\" alt=\"Lava dome in the crater of Mt. St. Helens. Source: Terry Feuerborn (2011) CC BY-NC 2.0\" width=\"500\" height=\"333\" \/><\/a> <strong>Figure 11.8<\/strong> Lava dome in the crater of Mt. St. Helens. Source: Terry Feuerborn (2011), CC BY-NC 2.0. <a href=\"https:\/\/www.flickr.com\/photos\/travfotos\/14643432171\/in\/photolist-oiZqdt-hKZ4Yp-hKZ3yv-S8G7AU-hK2PAg-s4VRi6-hK2hgL-hK2gvs-hK1JWa-h2qtV1-kcCjCq-hK2PXZ-deq7h5-hK2gTS-VcfkHk-hKYPwj-kcBxyB-ngDSpY-shn8mY-9KHbrh-hK2i3A-gpocGG-qwiGJE-kcBEbp-kcB8Mk-fKAQpK-d5L9ds-kcCjdh-f51Dmj-fjb2oH-kcDgyC-kcDjGw-dSQmnW-kcDhqC-swDkKA-hKZ8r6-kcAaRa-fmaVQG-kcDgR1-hKZ7fi-hKZ6DZ-kcB79k-kcBxTp-kcB6A6-rC7qJK-kcDeiq-fkwsS9-kcBBWK-kcDez7-oVujqC\" rel=\"noopener noreferrer\">View source.<\/a>[\/caption]\r\n\r\nLess viscous andesitic lava can travel further, as with the thick flow in Figure 11.9 (right). The left of Figure 11.9 shows thin streams of freely-flowing, low-silica, low-viscosity basaltic lava.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_466\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison.png\" rel=\"attachment wp-att-712\"><img class=\"wp-image-466\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison.png\" alt=\"Lava flows. Left: A geologist collects a sample from a basaltic lava flow in Hawaii. Right: an andesitic lava flow from Kanaga Volcano in the Aleutian Islands. Source: Left- U. S. Geological Survey (2014) Public Domain; Right- Michelle Combs, U. S. Geological Survey (2015) Public Domain\" width=\"650\" height=\"244\" \/><\/a> <strong>Figure 11.9<\/strong> Lava flows. Left: A geologist collects a sample from a basaltic lava flow in Hawaii. Right: an andesitic lava flow from Kanaga Volcano in the Aleutian Islands. Source: Left- U. S. Geological Survey (2014), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/14493307891\/in\/album-72157637377510893\/\" rel=\"noopener noreferrer\">View source.<\/a>; Right- Michelle Combs, U. S. Geological Survey (2015), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/22432739869\/in\/album-72157637377510893\/\" rel=\"noopener noreferrer\">View source.<\/a>[\/caption]\r\n\r\nLow-viscosity basaltic lava flows may travel extended distances if they move through conduits called <strong>lava tubes<\/strong>. These are tunnels within older solidified lava flows. Figure 11.10 (top) shows a view into a lava tube through a hole in the overlying rock, called a\u00a0<strong>skylight<\/strong>. Figure 11.10 (bottom) shows the interior of a lava tube, with a person for scale. Lava tubes form naturally and readily because flowing mafic lava preferentially cools near its margins, forming solid <strong>lava lev\u00e9es<\/strong> that eventually close over the top of the flow. Lava within tubes can flow for 10s of km because the tubes insulate the lava from the atmosphere and slow the rate at which the lava cools. The Hawai'ian volcanoes are riddled with thousands of old, drained lava tubes, some as long as 50 km.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_467\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes.png\"><img class=\"wp-image-467\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes.png\" alt=\"Lava tubes. Top: An opening in the roof of a lava tube (called a skylight) permitting a view of lava flowing through the tube (Pu\u02bbu \u02bb\u014c\u02bb\u014d crater, K\u012blauea). The opening is approximately 6 m across. Bottom: Inside a lava tube that channelled lava away from Mt. St. Helens in an eruption 1,895 years ago. Sources: Top: U. S. Geological Survey (2016) Public Domain. Bottom: Thomas Shahan (2013) CC BY-NC 2.0\" width=\"500\" height=\"534\" \/><\/a> <strong>Figure 11.10<\/strong> Lava tubes. Top: An opening in the roof of a lava tube (called a skylight) permitting a view of lava flowing through the tube (Pu\u02bbu \u02bb\u014c\u02bb\u014d crater, K\u012blauea). The opening is approximately 6 m across. Bottom: Inside a lava tube that channelled lava away from Mt. St. Helens in an eruption 1,895 years ago. Sources: Top: U. S. Geological Survey (2016), Public Domain. <a href=\"https:\/\/flic.kr\/p\/JuvsfJ\" rel=\"noopener\">View source.<\/a> Bottom: Thomas Shahan (2013), CC BY-NC 2.0. <a href=\"https:\/\/flic.kr\/p\/s3RDMf\" rel=\"noopener\">View source.<\/a><em><br \/><\/em>[\/caption]\r\n<h2>Lava Structures<\/h2>\r\n<h3>Pahoehoe<\/h3>\r\nLava flowing on the surface can take on different shapes as it cools. Basaltic lava with an unfragmented surface (e.g., Figure 11.9, right), is called <strong>pahoehoe<\/strong>. (pronounced pa-hoy-hoy). Pahoehoe can be smooth and billowy. It can also develop a wrinkled texture, called <strong>ropy lava<\/strong> (Figure 11.11). Ropy lava forms when the outermost layer of the lava cools and develops a skin (visible as a dark layer in Figure 11.11, left), but the skin is still hot and thin enough to be flexible. The skin is stiffer than the lava beneath it, and is dragged by flowing lava and folded up into wrinkles. Figure 11.11 (right) is a close-up view after a cut has been made to show the internal structure of a wrinkled lava flow. Notice the many holes, or <strong>vesicles<\/strong>, within the lava, formed when the lava solidified around gas bubbles.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_468\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava.png\"><img class=\"wp-image-468\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava.png\" alt=\"Ropy lava (pahoehoe) from Hawaii. Left: Ropy texture forming as a thin surface layer of lava cools and is wrinkled by the motion of lava flowing beneath it (near). Right: Cross-section view of ropy lava. Sources: Left: Z. T. Jackson (2005) CC BY NC-ND 2.0; Right: Fiddledydee (2011) CC BY-NC 2.0. \" width=\"650\" height=\"259\" \/><\/a> <strong>Figure 11.11<\/strong> Ropy lava from Hawaii. Left: Ropy texture forming as a thin surface layer of lava cools and is wrinkled by the motion of lava flowing beneath it. Right: Cross-section view of ropy lava. Sources: Left: Z. T. Jackson (2005), CC BY NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/5WpxCf\" rel=\"noopener noreferrer\">View source.<\/a>; Right: Fiddledydee (2011), CC BY-NC 2.0. <a href=\"https:\/\/flic.kr\/p\/9RqSoY\" rel=\"noopener noreferrer\">View source.<\/a>.[\/caption]\r\n<h3>A'a and Blocky Lava<\/h3>\r\nWhen the outer layer of the lava flow can't accommodate the motion of lava beneath by deforming smoothly, the outer layer will break into fragments as lava moves beneath it. This could happen if the lava flow develops a thicker, more brittle outer layer, or if it moves faster. The result is a sharp and splintery rubble-like lava flow called <strong>a\u2019a <\/strong>(pronounced like \"lava\" but without the l and v). Figure 11.12 (left) shows a close-up view of the advancing front of an a\u2019a lava flow (the flow is moving toward the viewer). Figure 11.12 (right) shows an a\u2019a lava flow viewed from the side. Compare the texture of the a\u2019a flow with the texture of the lighter-grey pahoehoe lava in the foreground of the picture.\r\n\r\n[caption id=\"attachment_469\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa.png\"><img class=\"wp-image-469\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa.png\" alt=\"Aa lava flows. Left: Close-up view of aa forming during an eruption of Pacaya Volcano in Guatemala. Field of view approximately 1 m across. Right: Rubbly reddish-brown aa lava flow viewed from Chain of Craters Road, Hawai\u2019i Volcanoes National Park. Pahoehoe is visible in the foreground. Sources: Photo of Hawaiian aa and pahoehoe: Roy Luck (2009) CC BY 2.0; Pacaya aa: Greg Willis (2008) CC BY-SA 2.0\" width=\"650\" height=\"331\" \/><\/a> <strong>Figure 11.12<\/strong> Aa lava flows. Left: Close-up view of a'a forming during an eruption of Pacaya Volcano in Guatemala. Field of view approximately 1 m across. Right: Rubbly reddish-brown a'a lava flow viewed from Chain of Craters Road, Hawai\u2019i Volcanoes National Park. Pahoehoe is visible in lighter grey in the foreground. Sources: Photo of Hawaiian aa and pahoehoe: Roy Luck (2009), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/6JqWTV\" rel=\"noopener noreferrer\">View source.<\/a> Pacaya a'a: Greg Willis (2008), CC BY-SA 2.0 (labels added). <a href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Pacaya_Volcano_-_Guatemala_(4251539562).jpg\" rel=\"noopener noreferrer\">View source.<\/a>.[\/caption]\r\n\r\nHigher viscosity andesitic lava flows also develop a fragmented surface, called <strong>blocky lava<\/strong>. This is visible in the toe of the andesitic lava flow from Figure 11.9 (right). The difference between a\u2019a and the andesitic blocky lava is that the blocky lava has fragments with smoother surfaces and fewer vesicles.\r\n<h3>Lava Pillows<\/h3>\r\nWhen lava flows into water, the outside of the lava cools quickly, making a tube (Figure 11.13 (top left)). Blobs of lava develop at the end of the tube (Figure 11.13 (top right)), forming <strong>pillows<\/strong>. The bottom left of Figure 10.13 shows pillows covering the sea floor, and the bottom right shows the distinctive rounded shape of pillows in outcrop. Because pillows always form underwater, finding them in the rock record gives us information that the environment was underwater.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_470\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas.png\"><img class=\"wp-image-470\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas.png\" alt=\"Pillow lavas. Top left: A tube of lava extruding underwater. Hot lava can be seen through cracks in the wall of the tube. The image is approximately 1 m across. (Pacific Ocean, near Fiji). Top right: The rounded end of a lava tube with cracks showing the lava within. (Pacific Ocean, near Fiji). Bottom left: sea floor covered with pillow lavas near the Gal\u00e1pagos Islands. Bottom right: A boulder made of 2.7 billion year old pillow lavas, derived from the Ely Greenstone in north-eastern Minnesota. Sources: Top left: NSF and NOAA (2010) CC BY 2.0; Top right: NSF and NOAA (2010) CC BY 2.0; Bottom left: NOAA Okeanos Explorer Program, Gal\u00e1pagos Rift Expedition 2011 (2011) CC BY 2.0; Bottom right: James St. John (2015) CC BY 2.0.\" width=\"650\" height=\"515\" \/><\/a> <strong>Figure 11.13<\/strong> Pillow lavas. Top left: A tube of lava extruding underwater. Hot lava can be seen through cracks in the wall of the tube. The image is approximately 1 m across. (Pacific Ocean, near Fiji). Top right: The rounded end of a tube with cracks showing the lava within. (Pacific Ocean, near Fiji). Bottom left: sea floor near the Gal\u00e1pagos Islands covered with pillow lavas. Bottom right: A boulder made of 2.7 billion year old pillows derived from the Ely Greenstone in north-eastern Minnesota. Sources: Top left- NSF and NOAA (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/93orFj\" rel=\"noopener noreferrer\">View source.<\/a>; Top right- NSF and NOAA (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/93kj7x\" rel=\"noopener noreferrer\">View source.<\/a>; Bottom left- NOAA Okeanos Explorer Program, Gal\u00e1pagos Rift Expedition 2011 (2011), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/fUzHjD\" rel=\"noopener noreferrer\">View source.<\/a>; Bottom right- James St. John (2015), CC BY 2.0. <a href=\"https:\/\/www.flickr.com\/photos\/jsjgeology\/20831596894\/in\/photolist-xJPnZG-yGzEkB-xRj8DT-yKZWEE-ypdQSG-xRb6LS-yMdGzQ-ypfznY-yFRoTn-xRhtFG-xJPfvd-ypjTgg-yMdDNC-yDwbyJ-yDw3Wu-yNcwpZ-yNcLeT-yKTeKf-yvzLio-yESdbm-xRocM4-HCZyD2-xRiTPD-yNczMR-JEP1z9-yKZQo1-yvzxY3-yvN9BX-yMhBwA-93kj66-K5b5va-qMVzsN-yETq1w-rJP8eL-yGzXie-qdJd4B-MiF3Yi-MWnmFN-LQw7ks-L5GHUt-M8iUGh-yKZE5A-yvFJbK-ypeH93-ypefhf-fQtYNA-dXbbnp-dX9Gux-8jk155-7Xd75s\" rel=\"noopener noreferrer\">View source.<\/a>.[\/caption]\r\n<h3>Columnar Joints<\/h3>\r\nWhen lava flows cool and solidify, they shrink. Long vertical cracks, or <strong>joints<\/strong>, form within the brittle rock to allow for the shrinkage. Viewed from above, the joints form polygons with 5, 6, or 7- sides, and angles of approximately 120\u00ba between sides (Figure 11.14).\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_471\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway.jpg\"><img class=\"wp-image-471\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-1024x576.jpg\" alt=\"Columnar joints viewed from above. Source: Meg Stewart (2012) CC BY-SA 2.0\" width=\"500\" height=\"281\" \/><\/a> <strong>Figure 11.14<\/strong> Columnar joints viewed from above, Giant's Causeway, Northern Ireland. Source: Meg Stewart (2012), CC BY-SA 2.0. <a href=\"https:\/\/flic.kr\/p\/bBV4xF\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n\r\nFigure 11.15 shows a side view of columnar joints in a basaltic lava flow in Iceland.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_472\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss.jpg\"><img class=\"wp-image-472\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-1024x682.jpg\" alt=\"\" width=\"500\" height=\"333\" \/><\/a> <strong>Figure 11.15<\/strong> Columnar joints in a basaltic lava flow, Svartifoss (Black Fall) Vatnaj\u00f6kull National Park, Iceland. Source: Ron Kroetz (2015), CC BY-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/v5Butv\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n\r\n<div class=\"textbox shaded\">\r\n\r\n<strong><a id=\"231\"><\/a>Practice with Structures Made by Lava<\/strong>\r\n\r\n[h5p id=\"231\"]\r\n\r\n<\/div>\r\n<h1>Pyroclastic Materials<\/h1>\r\nThe pop bottle analogy illustrates another key point about gas bubbles in fluid, which is that the bubbles can propel fluid. In the same way that shaking a pop bottle to make more bubbles will cause pop to gush out when the bottle is opened, gas bubbles can violently propel lava and other materials from a volcano, creating an explosive eruption.\r\n\r\nCollectively, loose material thrown from a volcano is referred to as <strong>tephra<\/strong>. Individual fragments are referred to in general terms as <strong>pyroclasts<\/strong>, so sometimes tephra is also referred to as<strong> pyroclastic debris<\/strong>. Pyroclasts are classified according to size.\r\n<h2>Volcanic Ash<\/h2>\r\nParticles less than 2 mm in diameter are called <strong>volcanic ash<\/strong>. Volcanic ash consists of small mineral grains and glass. Figure 11.16 shows volcanic ash on three scales: in the upper left is ash from the 2010 eruption of\u00a0Eyjafjallaj\u00f6kull in Iceland. The image was taken with a scanning electron microscope at approximately 1000 times magnification. In the upper right is ash from the 1980 eruption of Mt. St. Helens, collected in Yakima, Washington, about 137 km northeast of Mt. St. Helens. Individual particles are under 1 mm in size. Figure 11.16 (bottom) shows a village near Mt. Merapi in Indonesia dusted in ash after an eruption 2010.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_473\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/openpress.usask.ca\/app\/uploads\/sites\/29\/2017\/08\/Volcanic_ash.png\"><img class=\"wp-image-473\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash.png\" alt=\"\" width=\"650\" height=\"726\" \/><\/a> <strong>Figure 11.16<\/strong> Volcanic ash. Upper left: Ash from 2010 eruption of Eyjafjallaj\u00f6kull in Iceland, magnified approximately 1000x. Upper right- Ash from the 1980 eruption of Mt. St. Helens, collected at Yakima, Washington. Bottom: Indonesian village after the eruption of Mt. Merapi in 2010. Sources: Upper left: Birgit Hartinger, AEC (2010), CC BY-NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/86G3Nz\" rel=\"noopener\">View source.<\/a> Upper right: James St. John (2014), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oUPZxZ\" rel=\"noopener\">View source.<\/a> Bottom: AusAID\/Jeong Park (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/hfkWdo\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n<h2>Lapilli<\/h2>\r\nFragments with dimensions between 2 mm and 64 mm are classified as <strong>lapilli<\/strong>. Figure 11.17 (upper left) shows lapilli at the ancient city of Pompeii, which was buried when Mt. Vesuvius erupted in 79 C.E. Figure 11.17 (lower left) is a form of lapilli called <strong>Pele's tears<\/strong>, named after the Hawai'ian diety Pele. Pele's tears form when droplets of lava cool quickly as they are flung through the air. Rapidly moving through the air may draw the Pele's tears out into long threads called <strong>Pele's hair<\/strong> (Figure 11.17, right). The dark masses in Figure 11.17 (right) within the Pele's hair are Pele's tears.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_474\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli.png\" target=\"_blank\" rel=\"noopener\"><img class=\"wp-image-474\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli.png\" alt=\"\" width=\"650\" height=\"499\" \/><\/a> <strong>Figure 11.17<\/strong> Lapilli are pyroclasts ranging between 2 mm and 64 mm in size. Upper left: lapilli from the site of the ancient city of Pompeii. Lower left: Pele's tears, a type of lapilli that forms when droplets of lava fly through the air. Right: Pele's hair, which form when Pele's tears are drawn out into thin threads as they fly. Sources: Upper left: Pauline (2009), CC BY-NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/6JyZWU\" rel=\"noopener\">View source.<\/a>; Lower left: James St. John (2014), CC BY 2.0 (scale added) <a href=\"https:\/\/flic.kr\/p\/oBgw9G\" rel=\"noopener\">View source.<\/a>; Right: James St. John (2009), CC BY 2.0 (scale added) <a href=\"https:\/\/flic.kr\/p\/oRJoBA\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n<h2>Blocks and Bombs<\/h2>\r\nFragments larger than 64 mm are classified as blocks or bombs, depending on their origin. <strong>Blocks<\/strong> are solid fragments of the volcano that form when an explosive eruption shatters the pre-existing rocks. Figure 11.18 shows one of many blocks from an explosive eruption at the\u00a0Halema\u2018uma\u2018u crater at K\u012blauea Volcano in May of 1924. The block has a mass of approximately 7 tonnes and landed 1 km from the crater.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_475\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block.jpg\"><img class=\"wp-image-475\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block.jpg\" alt=\"Volcanic block weighing approximately 7 tonnes thrown 1 km from the Halema\u2018uma\u2018u crater at K\u012blauea Volcano on May 18, 1924. Source: U. S. Geological Survey (1924) Public Domain\" width=\"500\" height=\"362\" \/><\/a> <strong>Figure 11.18<\/strong> Volcanic block weighing approximately 7 tonnes thrown 1 km from the Halema\u2018uma\u2018u crater at K\u012blauea Volcano on May 18, 1924. Source: U. S. Geological Survey (1924), Public Domain. <a href=\"https:\/\/volcanoes.usgs.gov\/vsc\/images\/image_mngr\/5000-5099\/img5019_900w_652h.jpg\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n\r\n<strong>Bombs<\/strong> form when lava is thrown from the volcano and cools as it travels through the air. Traveling through the air may cause the lava to take on a streamlined shape, as with the example in Figure 11.19.\r\n\r\n[caption id=\"attachment_476\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John.png\"><img class=\"wp-image-476\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John.png\" alt=\"Volcanic bomb with a streamlined shape. Source: James St. John (2016) CC BY 2.0\" width=\"500\" height=\"258\" \/><\/a> <strong>Figure 11.19<\/strong> Volcanic bomb with a streamlined shape. Source: James St. John (2016), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/PdzxtC\" rel=\"noopener\">View source.<\/a>[\/caption]\r\n<h2>Effects of Gas on Lapilli and Bombs<\/h2>\r\nThe presence of gas in erupting lava can cause lapilli and bombs to take on distinctive forms as the lava freezes around the gas bubbles, giving the rocks a <strong>vesicular<\/strong> (hole-filled) texture. <strong>Pumice<\/strong> (Figure 11.20) forms from gas-filled felsic lava. Figure 11.20 (right), shows a magnified view of the sample on the left. The dark patches in the photograph are mineral crystals that formed in the magma chamber before the lava erupted. Pumice floats on water because some of the holes are completely enclosed, and air-filled.\r\n\r\n[caption id=\"attachment_477\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp.png\"><img class=\"wp-image-477\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp.png\" alt=\"Lapilli-sided pumice fragment collected from the shores of Lake Atitl\u00e1n in Guatemala by H. Herrmann. The lake is a flooded caldera, and is surrounded by active volcanoes. Right: magnified view showing vesicular structure and amphibole crystals (dark patches). Source: Karla Panchuk (2017) CC BY 4.0\" width=\"650\" height=\"289\" \/><\/a> <strong>Figure 11.20<\/strong> Lapilli-sized pumice collected from the shores of Lake Atitl\u00e1n in Guatemala by H. Herrmann. The lake is a flooded caldera, and is surrounded by active volcanoes. Right: Magnified view showing vesicular structure and amphibole crystals (dark patches). Source: Karla Panchuk (2017), CC BY 4.0.[\/caption]\r\n\r\nThe mafic counterpart to pumice is <strong>scoria <\/strong>(Figure 11.21, left). Mafic lava can also form <strong>reticulite<\/strong> (Figure 11.21, right), a rare and fragile rock in which the walls surrounding the bubbles have all burst, leaving behind a delicate network of glass.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_478\" align=\"aligncenter\" width=\"650\"]<a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular.png\"><img class=\"wp-image-478\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular.png\" alt=\"Mafic lapilli with vesicular textures. Left: Scoria from Mount Fuji, Japan. Scoria is the denser mafic counterpart to pumice. Right: Reticulite from K\u012blauea Volcano. Reticulite is a delicate network of volcanic glass that forms when the walls separating gas bubbles pop. Sources: Left- James St. John (2014) CC BY 2.0 (scale added); Right- James St. John (2014) CC BY 4.0 (scale added) \" width=\"650\" height=\"263\" \/><\/a> <strong>Figure 11.21<\/strong> Mafic lapilli with vesicular textures. Left: Scoria from Mount Fuji, Japan. Scoria is the denser mafic counterpart to pumice. Right: Reticulite from K\u012blauea Volcano. Reticulite is a delicate network of volcanic glass that forms when the walls separating gas bubbles pop. Sources: Left- James St. John (2014), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oCcn1y\" rel=\"noopener\">View source.<\/a> Right- James St. John (2014), CC BY 4.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oBgu7W\" rel=\"noopener\">View source.<\/a>.[\/caption]\r\n\r\n<div class=\"textbox shaded\">\r\n\r\n<strong><a id=\"232\"><\/a>Practice with Types of Pyroclastic Material<\/strong>\r\n\r\n[h5p id=\"232\"]\r\n\r\n<\/div>\r\n<h4>References<\/h4>\r\n<a id=\"USGS-2013\"><\/a>U. S. Geological Survey (2013) <em>Mt. St. Helens National Volcanic Monument<\/em>. Retrieved on 11 June 2017. <em><a href=\"https:\/\/volcanoes.usgs.gov\/volcanoes\/st_helens\/st_helens_geo_hist_106.html\" target=\"_blank\" rel=\"noopener noreferrer\">Visit website<\/a><\/em>\r\n\r\n&nbsp;","rendered":"<p>Volcanic eruptions produce three types of materials: gas, lava, and fragmented debris called <strong>tephra<\/strong>.<\/p>\n<h1>Volcanic Gas<\/h1>\n<p>Magma contains gas. Most of the gas emitted by volcanoes is water, but gas also contains carbon dioxide (CO<sub>2<\/sub>), sulphur dioxide (SO<sub>2<\/sub>), and hydrogen sulphide (H<sub>2<\/sub>S), in order of decreasing abundance.<\/p>\n<p>.At high pressures, the gases are dissolved in the magma, but if the pressure decreases, the gas comes out of solution, forming bubbles, similar to what happens when you open a bottle of pop. Pop is bottled under pressure, forcing carbon dioxide gas to dissolve into the fluid. As long as the bottle is closed and the pressure remains high, you&#8217;ll see few to no bubbles in the pop. But if you open the bottle, air rushes out, decreasing the pressure on the pop. The pop will begin to fizz as carbon dioxide gas comes out of solution and forms bubbles.<\/p>\n<p>Volcanoes release gases when erupt, and through openings called <strong>fumaroles <\/strong>(Figure 11.7). They can also release gas into soil and groundwater.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_464\" aria-describedby=\"caption-attachment-464\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS.jpeg\" rel=\"attachment wp-att-709\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-464\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS.jpeg\" alt=\"A fumarole at Pu\u02bbu \u02bb\u014c\u02bb\u014d Crater. Hawaii. The yellow crust along the margin of the fumarole is made of sulphur crystals. The crystals form when sulphur vapour cools as it is released from the fumarole. Source: U. S. Geological Survey (2016) Public Domain\" width=\"500\" height=\"333\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS.jpeg 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS-300x200.jpeg 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS-65x43.jpeg 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS-225x150.jpeg 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2017\/09\/fumarole_USGS-350x233.jpeg 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-464\" class=\"wp-caption-text\"><strong>Figure 11.7<\/strong> A fumarole at Pu\u02bbu \u02bb\u014c\u02bb\u014d Crater, Hawaii. The yellow crust along the margin of the fumarole is made of sulphur crystals. The crystals form when sulphur vapour cools as it is released from the fumarole. Source: U. S. Geological Survey (2016), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/23998018863\/in\/album-72157637377510893\/\" target=\"_blank\" rel=\"noopener noreferrer\">View source<\/a><em>.<br \/><\/em><\/figcaption><\/figure>\n<h1>Lava<\/h1>\n<p>The ease with which lava flows, and the structures it forms depend on how much silica and gas are in the lava. The more silica, the more <strong>polymerization\u00a0<\/strong>(formation of long molecules) happens, stiffening the lava. The stiffness of lava is described in terms of <strong>viscosity:<\/strong> lava that flows easily has low viscosity, and lava that is sticky and stiff has high viscosity.<\/p>\n<p>In general, higher-silica (felsic) lava contains more gas than low-silica lava. When the gas forms into bubbles, viscosity increases further. Consider the pop analogy again: If you shook the bottle vigorously, then opened it, the pop would gush out in a thick, frothy flow. In contrast, if you took care to not shake the bottle before opening it, you could pour out a thin stream of fluid. The presence of gas not only makes high-silica lava more viscous, but can affect mafic lavas in that way as well.<\/p>\n<p>&nbsp;<\/p>\n<div class=\"textbox shaded\">\n<p><strong>Concept Check: Viscosity<\/strong><\/p>\n<div id=\"h5p-230\">\n<div class=\"h5p-iframe-wrapper\"><iframe id=\"h5p-iframe-230\" class=\"h5p-iframe\" data-content-id=\"230\" style=\"height:1px\" src=\"about:blank\" frameBorder=\"0\" scrolling=\"no\" title=\"Review of igneous rock compositions\"><\/iframe><\/div>\n<\/div>\n<\/div>\n<p>&nbsp;<\/p>\n<p>The thickness and shape of a lava flow depends on its viscosity. The greater the viscosity, the thicker the flow, and the shorter the distance it can go before solidifying. Highly viscous lava might not flow very far at all, and simply accumulate as a bulge, called a <strong>lava dome<\/strong>, in a volcano\u2019s crater. Figure 11.8 shows a dome formed from rhyolitic lava in the crater of Mt. St. Helens.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_465\" aria-describedby=\"caption-attachment-465\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn.jpeg\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-465\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn.jpeg\" alt=\"Lava dome in the crater of Mt. St. Helens. Source: Terry Feuerborn (2011) CC BY-NC 2.0\" width=\"500\" height=\"333\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn.jpeg 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn-300x200.jpeg 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn-65x43.jpeg 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn-225x150.jpeg 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/StHelens_lava_dome_feuerborn-350x233.jpeg 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-465\" class=\"wp-caption-text\"><strong>Figure 11.8<\/strong> Lava dome in the crater of Mt. St. Helens. Source: Terry Feuerborn (2011), CC BY-NC 2.0. <a href=\"https:\/\/www.flickr.com\/photos\/travfotos\/14643432171\/in\/photolist-oiZqdt-hKZ4Yp-hKZ3yv-S8G7AU-hK2PAg-s4VRi6-hK2hgL-hK2gvs-hK1JWa-h2qtV1-kcCjCq-hK2PXZ-deq7h5-hK2gTS-VcfkHk-hKYPwj-kcBxyB-ngDSpY-shn8mY-9KHbrh-hK2i3A-gpocGG-qwiGJE-kcBEbp-kcB8Mk-fKAQpK-d5L9ds-kcCjdh-f51Dmj-fjb2oH-kcDgyC-kcDjGw-dSQmnW-kcDhqC-swDkKA-hKZ8r6-kcAaRa-fmaVQG-kcDgR1-hKZ7fi-hKZ6DZ-kcB79k-kcBxTp-kcB6A6-rC7qJK-kcDeiq-fkwsS9-kcBBWK-kcDez7-oVujqC\" rel=\"noopener noreferrer\">View source.<\/a><\/figcaption><\/figure>\n<p>Less viscous andesitic lava can travel further, as with the thick flow in Figure 11.9 (right). The left of Figure 11.9 shows thin streams of freely-flowing, low-silica, low-viscosity basaltic lava.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_466\" aria-describedby=\"caption-attachment-466\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison.png\" rel=\"attachment wp-att-712\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-466\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison.png\" alt=\"Lava flows. Left: A geologist collects a sample from a basaltic lava flow in Hawaii. Right: an andesitic lava flow from Kanaga Volcano in the Aleutian Islands. Source: Left- U. S. Geological Survey (2014) Public Domain; Right- Michelle Combs, U. S. Geological Survey (2015) Public Domain\" width=\"650\" height=\"244\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison-300x113.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison-65x24.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison-225x84.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Lava_comparison-350x131.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-466\" class=\"wp-caption-text\"><strong>Figure 11.9<\/strong> Lava flows. Left: A geologist collects a sample from a basaltic lava flow in Hawaii. Right: an andesitic lava flow from Kanaga Volcano in the Aleutian Islands. Source: Left- U. S. Geological Survey (2014), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/14493307891\/in\/album-72157637377510893\/\" rel=\"noopener noreferrer\">View source.<\/a>; Right- Michelle Combs, U. S. Geological Survey (2015), Public Domain. <a href=\"https:\/\/www.flickr.com\/photos\/usgeologicalsurvey\/22432739869\/in\/album-72157637377510893\/\" rel=\"noopener noreferrer\">View source.<\/a><\/figcaption><\/figure>\n<p>Low-viscosity basaltic lava flows may travel extended distances if they move through conduits called <strong>lava tubes<\/strong>. These are tunnels within older solidified lava flows. Figure 11.10 (top) shows a view into a lava tube through a hole in the overlying rock, called a\u00a0<strong>skylight<\/strong>. Figure 11.10 (bottom) shows the interior of a lava tube, with a person for scale. Lava tubes form naturally and readily because flowing mafic lava preferentially cools near its margins, forming solid <strong>lava lev\u00e9es<\/strong> that eventually close over the top of the flow. Lava within tubes can flow for 10s of km because the tubes insulate the lava from the atmosphere and slow the rate at which the lava cools. The Hawai&#8217;ian volcanoes are riddled with thousands of old, drained lava tubes, some as long as 50 km.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_467\" aria-describedby=\"caption-attachment-467\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-467\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes.png\" alt=\"Lava tubes. Top: An opening in the roof of a lava tube (called a skylight) permitting a view of lava flowing through the tube (Pu\u02bbu \u02bb\u014c\u02bb\u014d crater, K\u012blauea). The opening is approximately 6 m across. Bottom: Inside a lava tube that channelled lava away from Mt. St. Helens in an eruption 1,895 years ago. Sources: Top: U. S. Geological Survey (2016) Public Domain. Bottom: Thomas Shahan (2013) CC BY-NC 2.0\" width=\"500\" height=\"534\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes-281x300.png 281w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes-65x69.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes-225x240.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lava-tubes-350x374.png 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-467\" class=\"wp-caption-text\"><strong>Figure 11.10<\/strong> Lava tubes. Top: An opening in the roof of a lava tube (called a skylight) permitting a view of lava flowing through the tube (Pu\u02bbu \u02bb\u014c\u02bb\u014d crater, K\u012blauea). The opening is approximately 6 m across. Bottom: Inside a lava tube that channelled lava away from Mt. St. Helens in an eruption 1,895 years ago. Sources: Top: U. S. Geological Survey (2016), Public Domain. <a href=\"https:\/\/flic.kr\/p\/JuvsfJ\" rel=\"noopener\">View source.<\/a> Bottom: Thomas Shahan (2013), CC BY-NC 2.0. <a href=\"https:\/\/flic.kr\/p\/s3RDMf\" rel=\"noopener\">View source.<\/a><em><br \/><\/em><\/figcaption><\/figure>\n<h2>Lava Structures<\/h2>\n<h3>Pahoehoe<\/h3>\n<p>Lava flowing on the surface can take on different shapes as it cools. Basaltic lava with an unfragmented surface (e.g., Figure 11.9, right), is called <strong>pahoehoe<\/strong>. (pronounced pa-hoy-hoy). Pahoehoe can be smooth and billowy. It can also develop a wrinkled texture, called <strong>ropy lava<\/strong> (Figure 11.11). Ropy lava forms when the outermost layer of the lava cools and develops a skin (visible as a dark layer in Figure 11.11, left), but the skin is still hot and thin enough to be flexible. The skin is stiffer than the lava beneath it, and is dragged by flowing lava and folded up into wrinkles. Figure 11.11 (right) is a close-up view after a cut has been made to show the internal structure of a wrinkled lava flow. Notice the many holes, or <strong>vesicles<\/strong>, within the lava, formed when the lava solidified around gas bubbles.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_468\" aria-describedby=\"caption-attachment-468\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-468\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava.png\" alt=\"Ropy lava (pahoehoe) from Hawaii. Left: Ropy texture forming as a thin surface layer of lava cools and is wrinkled by the motion of lava flowing beneath it (near). Right: Cross-section view of ropy lava. Sources: Left: Z. T. Jackson (2005) CC BY NC-ND 2.0; Right: Fiddledydee (2011) CC BY-NC 2.0.\" width=\"650\" height=\"259\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava-300x120.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava-65x26.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava-225x90.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/ropy_lava-350x140.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-468\" class=\"wp-caption-text\"><strong>Figure 11.11<\/strong> Ropy lava from Hawaii. Left: Ropy texture forming as a thin surface layer of lava cools and is wrinkled by the motion of lava flowing beneath it. Right: Cross-section view of ropy lava. Sources: Left: Z. T. Jackson (2005), CC BY NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/5WpxCf\" rel=\"noopener noreferrer\">View source.<\/a>; Right: Fiddledydee (2011), CC BY-NC 2.0. <a href=\"https:\/\/flic.kr\/p\/9RqSoY\" rel=\"noopener noreferrer\">View source.<\/a>.<\/figcaption><\/figure>\n<h3>A&#8217;a and Blocky Lava<\/h3>\n<p>When the outer layer of the lava flow can&#8217;t accommodate the motion of lava beneath by deforming smoothly, the outer layer will break into fragments as lava moves beneath it. This could happen if the lava flow develops a thicker, more brittle outer layer, or if it moves faster. The result is a sharp and splintery rubble-like lava flow called <strong>a\u2019a <\/strong>(pronounced like &#8220;lava&#8221; but without the l and v). Figure 11.12 (left) shows a close-up view of the advancing front of an a\u2019a lava flow (the flow is moving toward the viewer). Figure 11.12 (right) shows an a\u2019a lava flow viewed from the side. Compare the texture of the a\u2019a flow with the texture of the lighter-grey pahoehoe lava in the foreground of the picture.<\/p>\n<figure id=\"attachment_469\" aria-describedby=\"caption-attachment-469\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-469\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa.png\" alt=\"Aa lava flows. Left: Close-up view of aa forming during an eruption of Pacaya Volcano in Guatemala. Field of view approximately 1 m across. Right: Rubbly reddish-brown aa lava flow viewed from Chain of Craters Road, Hawai\u2019i Volcanoes National Park. Pahoehoe is visible in the foreground. Sources: Photo of Hawaiian aa and pahoehoe: Roy Luck (2009) CC BY 2.0; Pacaya aa: Greg Willis (2008) CC BY-SA 2.0\" width=\"650\" height=\"331\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa-300x153.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa-65x33.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa-225x115.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/aa-350x178.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-469\" class=\"wp-caption-text\"><strong>Figure 11.12<\/strong> Aa lava flows. Left: Close-up view of a&#8217;a forming during an eruption of Pacaya Volcano in Guatemala. Field of view approximately 1 m across. Right: Rubbly reddish-brown a&#8217;a lava flow viewed from Chain of Craters Road, Hawai\u2019i Volcanoes National Park. Pahoehoe is visible in lighter grey in the foreground. Sources: Photo of Hawaiian aa and pahoehoe: Roy Luck (2009), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/6JqWTV\" rel=\"noopener noreferrer\">View source.<\/a> Pacaya a&#8217;a: Greg Willis (2008), CC BY-SA 2.0 (labels added). <a href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Pacaya_Volcano_-_Guatemala_(4251539562).jpg\" rel=\"noopener noreferrer\">View source.<\/a>.<\/figcaption><\/figure>\n<p>Higher viscosity andesitic lava flows also develop a fragmented surface, called <strong>blocky lava<\/strong>. This is visible in the toe of the andesitic lava flow from Figure 11.9 (right). The difference between a\u2019a and the andesitic blocky lava is that the blocky lava has fragments with smoother surfaces and fewer vesicles.<\/p>\n<h3>Lava Pillows<\/h3>\n<p>When lava flows into water, the outside of the lava cools quickly, making a tube (Figure 11.13 (top left)). Blobs of lava develop at the end of the tube (Figure 11.13 (top right)), forming <strong>pillows<\/strong>. The bottom left of Figure 10.13 shows pillows covering the sea floor, and the bottom right shows the distinctive rounded shape of pillows in outcrop. Because pillows always form underwater, finding them in the rock record gives us information that the environment was underwater.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_470\" aria-describedby=\"caption-attachment-470\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-470\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas.png\" alt=\"Pillow lavas. Top left: A tube of lava extruding underwater. Hot lava can be seen through cracks in the wall of the tube. The image is approximately 1 m across. (Pacific Ocean, near Fiji). Top right: The rounded end of a lava tube with cracks showing the lava within. (Pacific Ocean, near Fiji). Bottom left: sea floor covered with pillow lavas near the Gal\u00e1pagos Islands. Bottom right: A boulder made of 2.7 billion year old pillow lavas, derived from the Ely Greenstone in north-eastern Minnesota. Sources: Top left: NSF and NOAA (2010) CC BY 2.0; Top right: NSF and NOAA (2010) CC BY 2.0; Bottom left: NOAA Okeanos Explorer Program, Gal\u00e1pagos Rift Expedition 2011 (2011) CC BY 2.0; Bottom right: James St. John (2015) CC BY 2.0.\" width=\"650\" height=\"515\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas-300x238.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas-65x51.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas-225x178.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Pillow_lavas-350x277.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-470\" class=\"wp-caption-text\"><strong>Figure 11.13<\/strong> Pillow lavas. Top left: A tube of lava extruding underwater. Hot lava can be seen through cracks in the wall of the tube. The image is approximately 1 m across. (Pacific Ocean, near Fiji). Top right: The rounded end of a tube with cracks showing the lava within. (Pacific Ocean, near Fiji). Bottom left: sea floor near the Gal\u00e1pagos Islands covered with pillow lavas. Bottom right: A boulder made of 2.7 billion year old pillows derived from the Ely Greenstone in north-eastern Minnesota. Sources: Top left- NSF and NOAA (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/93orFj\" rel=\"noopener noreferrer\">View source.<\/a>; Top right- NSF and NOAA (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/93kj7x\" rel=\"noopener noreferrer\">View source.<\/a>; Bottom left- NOAA Okeanos Explorer Program, Gal\u00e1pagos Rift Expedition 2011 (2011), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/fUzHjD\" rel=\"noopener noreferrer\">View source.<\/a>; Bottom right- James St. John (2015), CC BY 2.0. <a href=\"https:\/\/www.flickr.com\/photos\/jsjgeology\/20831596894\/in\/photolist-xJPnZG-yGzEkB-xRj8DT-yKZWEE-ypdQSG-xRb6LS-yMdGzQ-ypfznY-yFRoTn-xRhtFG-xJPfvd-ypjTgg-yMdDNC-yDwbyJ-yDw3Wu-yNcwpZ-yNcLeT-yKTeKf-yvzLio-yESdbm-xRocM4-HCZyD2-xRiTPD-yNczMR-JEP1z9-yKZQo1-yvzxY3-yvN9BX-yMhBwA-93kj66-K5b5va-qMVzsN-yETq1w-rJP8eL-yGzXie-qdJd4B-MiF3Yi-MWnmFN-LQw7ks-L5GHUt-M8iUGh-yKZE5A-yvFJbK-ypeH93-ypefhf-fQtYNA-dXbbnp-dX9Gux-8jk155-7Xd75s\" rel=\"noopener noreferrer\">View source.<\/a>.<\/figcaption><\/figure>\n<h3>Columnar Joints<\/h3>\n<p>When lava flows cool and solidify, they shrink. Long vertical cracks, or <strong>joints<\/strong>, form within the brittle rock to allow for the shrinkage. Viewed from above, the joints form polygons with 5, 6, or 7- sides, and angles of approximately 120\u00ba between sides (Figure 11.14).<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_471\" aria-describedby=\"caption-attachment-471\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-471\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-1024x576.jpg\" alt=\"Columnar joints viewed from above. Source: Meg Stewart (2012) CC BY-SA 2.0\" width=\"500\" height=\"281\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-1024x576.jpg 1024w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-300x169.jpg 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-768x432.jpg 768w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-1536x864.jpg 1536w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-65x37.jpg 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-225x127.jpg 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway-350x197.jpg 350w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Stewart_causeway.jpg 1920w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-471\" class=\"wp-caption-text\"><strong>Figure 11.14<\/strong> Columnar joints viewed from above, Giant&#8217;s Causeway, Northern Ireland. Source: Meg Stewart (2012), CC BY-SA 2.0. <a href=\"https:\/\/flic.kr\/p\/bBV4xF\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<p>Figure 11.15 shows a side view of columnar joints in a basaltic lava flow in Iceland.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_472\" aria-describedby=\"caption-attachment-472\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-472\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-1024x682.jpg\" alt=\"\" width=\"500\" height=\"333\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-1024x682.jpg 1024w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-300x200.jpg 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-768x512.jpg 768w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-1536x1024.jpg 1536w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-65x43.jpg 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-225x150.jpg 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss-350x233.jpg 350w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kroetz_Svartifoss.jpg 2000w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-472\" class=\"wp-caption-text\"><strong>Figure 11.15<\/strong> Columnar joints in a basaltic lava flow, Svartifoss (Black Fall) Vatnaj\u00f6kull National Park, Iceland. Source: Ron Kroetz (2015), CC BY-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/v5Butv\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<div class=\"textbox shaded\">\n<p><strong><a id=\"231\"><\/a>Practice with Structures Made by Lava<\/strong><\/p>\n<div id=\"h5p-231\">\n<div class=\"h5p-iframe-wrapper\"><iframe id=\"h5p-iframe-231\" class=\"h5p-iframe\" data-content-id=\"231\" style=\"height:1px\" src=\"about:blank\" frameBorder=\"0\" scrolling=\"no\" title=\"Types of lava structures\"><\/iframe><\/div>\n<\/div>\n<\/div>\n<h1>Pyroclastic Materials<\/h1>\n<p>The pop bottle analogy illustrates another key point about gas bubbles in fluid, which is that the bubbles can propel fluid. In the same way that shaking a pop bottle to make more bubbles will cause pop to gush out when the bottle is opened, gas bubbles can violently propel lava and other materials from a volcano, creating an explosive eruption.<\/p>\n<p>Collectively, loose material thrown from a volcano is referred to as <strong>tephra<\/strong>. Individual fragments are referred to in general terms as <strong>pyroclasts<\/strong>, so sometimes tephra is also referred to as<strong> pyroclastic debris<\/strong>. Pyroclasts are classified according to size.<\/p>\n<h2>Volcanic Ash<\/h2>\n<p>Particles less than 2 mm in diameter are called <strong>volcanic ash<\/strong>. Volcanic ash consists of small mineral grains and glass. Figure 11.16 shows volcanic ash on three scales: in the upper left is ash from the 2010 eruption of\u00a0Eyjafjallaj\u00f6kull in Iceland. The image was taken with a scanning electron microscope at approximately 1000 times magnification. In the upper right is ash from the 1980 eruption of Mt. St. Helens, collected in Yakima, Washington, about 137 km northeast of Mt. St. Helens. Individual particles are under 1 mm in size. Figure 11.16 (bottom) shows a village near Mt. Merapi in Indonesia dusted in ash after an eruption 2010.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_473\" aria-describedby=\"caption-attachment-473\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/openpress.usask.ca\/app\/uploads\/sites\/29\/2017\/08\/Volcanic_ash.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-473\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash.png\" alt=\"\" width=\"650\" height=\"726\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash-269x300.png 269w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash-65x73.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash-225x251.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Volcanic_ash-350x391.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-473\" class=\"wp-caption-text\"><strong>Figure 11.16<\/strong> Volcanic ash. Upper left: Ash from 2010 eruption of Eyjafjallaj\u00f6kull in Iceland, magnified approximately 1000x. Upper right- Ash from the 1980 eruption of Mt. St. Helens, collected at Yakima, Washington. Bottom: Indonesian village after the eruption of Mt. Merapi in 2010. Sources: Upper left: Birgit Hartinger, AEC (2010), CC BY-NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/86G3Nz\" rel=\"noopener\">View source.<\/a> Upper right: James St. John (2014), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oUPZxZ\" rel=\"noopener\">View source.<\/a> Bottom: AusAID\/Jeong Park (2010), CC BY 2.0. <a href=\"https:\/\/flic.kr\/p\/hfkWdo\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<h2>Lapilli<\/h2>\n<p>Fragments with dimensions between 2 mm and 64 mm are classified as <strong>lapilli<\/strong>. Figure 11.17 (upper left) shows lapilli at the ancient city of Pompeii, which was buried when Mt. Vesuvius erupted in 79 C.E. Figure 11.17 (lower left) is a form of lapilli called <strong>Pele&#8217;s tears<\/strong>, named after the Hawai&#8217;ian diety Pele. Pele&#8217;s tears form when droplets of lava cool quickly as they are flung through the air. Rapidly moving through the air may draw the Pele&#8217;s tears out into long threads called <strong>Pele&#8217;s hair<\/strong> (Figure 11.17, right). The dark masses in Figure 11.17 (right) within the Pele&#8217;s hair are Pele&#8217;s tears.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_474\" aria-describedby=\"caption-attachment-474\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli.png\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-474\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli.png\" alt=\"\" width=\"650\" height=\"499\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli-300x230.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli-65x50.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli-225x173.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/lapilli-350x269.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-474\" class=\"wp-caption-text\"><strong>Figure 11.17<\/strong> Lapilli are pyroclasts ranging between 2 mm and 64 mm in size. Upper left: lapilli from the site of the ancient city of Pompeii. Lower left: Pele&#8217;s tears, a type of lapilli that forms when droplets of lava fly through the air. Right: Pele&#8217;s hair, which form when Pele&#8217;s tears are drawn out into thin threads as they fly. Sources: Upper left: Pauline (2009), CC BY-NC-ND 2.0. <a href=\"https:\/\/flic.kr\/p\/6JyZWU\" rel=\"noopener\">View source.<\/a>; Lower left: James St. John (2014), CC BY 2.0 (scale added) <a href=\"https:\/\/flic.kr\/p\/oBgw9G\" rel=\"noopener\">View source.<\/a>; Right: James St. John (2009), CC BY 2.0 (scale added) <a href=\"https:\/\/flic.kr\/p\/oRJoBA\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<h2>Blocks and Bombs<\/h2>\n<p>Fragments larger than 64 mm are classified as blocks or bombs, depending on their origin. <strong>Blocks<\/strong> are solid fragments of the volcano that form when an explosive eruption shatters the pre-existing rocks. Figure 11.18 shows one of many blocks from an explosive eruption at the\u00a0Halema\u2018uma\u2018u crater at K\u012blauea Volcano in May of 1924. The block has a mass of approximately 7 tonnes and landed 1 km from the crater.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_475\" aria-describedby=\"caption-attachment-475\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-475\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block.jpg\" alt=\"Volcanic block weighing approximately 7 tonnes thrown 1 km from the Halema\u2018uma\u2018u crater at K\u012blauea Volcano on May 18, 1924. Source: U. S. Geological Survey (1924) Public Domain\" width=\"500\" height=\"362\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block.jpg 690w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block-300x217.jpg 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block-65x47.jpg 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block-225x163.jpg 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/Kilauea-Block-350x254.jpg 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-475\" class=\"wp-caption-text\"><strong>Figure 11.18<\/strong> Volcanic block weighing approximately 7 tonnes thrown 1 km from the Halema\u2018uma\u2018u crater at K\u012blauea Volcano on May 18, 1924. Source: U. S. Geological Survey (1924), Public Domain. <a href=\"https:\/\/volcanoes.usgs.gov\/vsc\/images\/image_mngr\/5000-5099\/img5019_900w_652h.jpg\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<p><strong>Bombs<\/strong> form when lava is thrown from the volcano and cools as it travels through the air. Traveling through the air may cause the lava to take on a streamlined shape, as with the example in Figure 11.19.<\/p>\n<figure id=\"attachment_476\" aria-describedby=\"caption-attachment-476\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-476\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John.png\" alt=\"Volcanic bomb with a streamlined shape. Source: James St. John (2016) CC BY 2.0\" width=\"500\" height=\"258\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John-300x155.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John-65x33.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John-225x116.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/bomb_St-John-350x180.png 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-476\" class=\"wp-caption-text\"><strong>Figure 11.19<\/strong> Volcanic bomb with a streamlined shape. Source: James St. John (2016), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/PdzxtC\" rel=\"noopener\">View source.<\/a><\/figcaption><\/figure>\n<h2>Effects of Gas on Lapilli and Bombs<\/h2>\n<p>The presence of gas in erupting lava can cause lapilli and bombs to take on distinctive forms as the lava freezes around the gas bubbles, giving the rocks a <strong>vesicular<\/strong> (hole-filled) texture. <strong>Pumice<\/strong> (Figure 11.20) forms from gas-filled felsic lava. Figure 11.20 (right), shows a magnified view of the sample on the left. The dark patches in the photograph are mineral crystals that formed in the magma chamber before the lava erupted. Pumice floats on water because some of the holes are completely enclosed, and air-filled.<\/p>\n<figure id=\"attachment_477\" aria-describedby=\"caption-attachment-477\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-477\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp.png\" alt=\"Lapilli-sided pumice fragment collected from the shores of Lake Atitl\u00e1n in Guatemala by H. Herrmann. The lake is a flooded caldera, and is surrounded by active volcanoes. Right: magnified view showing vesicular structure and amphibole crystals (dark patches). Source: Karla Panchuk (2017) CC BY 4.0\" width=\"650\" height=\"289\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp-300x133.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp-65x29.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp-225x100.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/pumice_kp-350x156.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-477\" class=\"wp-caption-text\"><strong>Figure 11.20<\/strong> Lapilli-sized pumice collected from the shores of Lake Atitl\u00e1n in Guatemala by H. Herrmann. The lake is a flooded caldera, and is surrounded by active volcanoes. Right: Magnified view showing vesicular structure and amphibole crystals (dark patches). Source: Karla Panchuk (2017), CC BY 4.0.<\/figcaption><\/figure>\n<p>The mafic counterpart to pumice is <strong>scoria <\/strong>(Figure 11.21, left). Mafic lava can also form <strong>reticulite<\/strong> (Figure 11.21, right), a rare and fragile rock in which the walls surrounding the bubbles have all burst, leaving behind a delicate network of glass.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_478\" aria-describedby=\"caption-attachment-478\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular.png\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-478\" src=\"https:\/\/pressbooks.bccampus.ca\/knowinghome\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular.png\" alt=\"Mafic lapilli with vesicular textures. Left: Scoria from Mount Fuji, Japan. Scoria is the denser mafic counterpart to pumice. Right: Reticulite from K\u012blauea Volcano. Reticulite is a delicate network of volcanic glass that forms when the walls separating gas bubbles pop. Sources: Left- James St. John (2014) CC BY 2.0 (scale added); Right- James St. John (2014) CC BY 4.0 (scale added)\" width=\"650\" height=\"263\" srcset=\"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular.png 720w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular-300x121.png 300w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular-65x26.png 65w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular-225x91.png 225w, https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-content\/uploads\/sites\/1304\/2021\/03\/mafic_vesicular-350x141.png 350w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><\/a><figcaption id=\"caption-attachment-478\" class=\"wp-caption-text\"><strong>Figure 11.21<\/strong> Mafic lapilli with vesicular textures. Left: Scoria from Mount Fuji, Japan. Scoria is the denser mafic counterpart to pumice. Right: Reticulite from K\u012blauea Volcano. Reticulite is a delicate network of volcanic glass that forms when the walls separating gas bubbles pop. Sources: Left- James St. John (2014), CC BY 2.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oCcn1y\" rel=\"noopener\">View source.<\/a> Right- James St. John (2014), CC BY 4.0 (scale added). <a href=\"https:\/\/flic.kr\/p\/oBgu7W\" rel=\"noopener\">View source.<\/a>.<\/figcaption><\/figure>\n<div class=\"textbox shaded\">\n<p><strong><a id=\"232\"><\/a>Practice with Types of Pyroclastic Material<\/strong><\/p>\n<div id=\"h5p-232\">\n<div class=\"h5p-iframe-wrapper\"><iframe id=\"h5p-iframe-232\" class=\"h5p-iframe\" data-content-id=\"232\" style=\"height:1px\" src=\"about:blank\" frameBorder=\"0\" scrolling=\"no\" title=\"Types of pyroclastic materials\"><\/iframe><\/div>\n<\/div>\n<\/div>\n<h4>References<\/h4>\n<p><a id=\"USGS-2013\"><\/a>U. S. Geological Survey (2013) <em>Mt. St. Helens National Volcanic Monument<\/em>. Retrieved on 11 June 2017. <em><a href=\"https:\/\/volcanoes.usgs.gov\/volcanoes\/st_helens\/st_helens_geo_hist_106.html\" target=\"_blank\" rel=\"noopener noreferrer\">Visit website<\/a><\/em><\/p>\n<p>&nbsp;<\/p>\n","protected":false},"author":103,"menu_order":2,"template":"","meta":{"pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[47],"contributor":[],"license":[],"class_list":["post-479","chapter","type-chapter","status-publish","hentry","chapter-type-standard"],"part":457,"_links":{"self":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapters\/479","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/wp\/v2\/users\/103"}],"version-history":[{"count":12,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapters\/479\/revisions"}],"predecessor-version":[{"id":2002,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapters\/479\/revisions\/2002"}],"part":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/parts\/457"}],"metadata":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapters\/479\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/wp\/v2\/media?parent=479"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/pressbooks\/v2\/chapter-type?post=479"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/wp\/v2\/contributor?post=479"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/physicalgeologyh5p\/wp-json\/wp\/v2\/license?post=479"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}