1 00:00:06,876 --> 00:00:12,132 In February of 1942, Mexican farmer Dionisio Pulido 2 00:00:12,132 --> 00:00:15,962 thought he heard thunder coming from his cornfield. 3 00:00:15,962 --> 00:00:19,740 However, the sound wasn’t coming from the sky. 4 00:00:19,740 --> 00:00:25,440 The source was a large, smoking crack emitting gas and ejecting rocks. 5 00:00:25,440 --> 00:00:29,560 This fissure would come to be known as the volcano Paricutin, 6 00:00:29,560 --> 00:00:36,706 and over the next 9 years, its lava and ash would cover over 200 square km. 7 00:00:36,706 --> 00:00:39,056 But where did this new volcano come from, 8 00:00:39,056 --> 00:00:43,160 and what triggered its unpredictable eruption? 9 00:00:43,160 --> 00:00:46,690 The story of any volcano begins with magma. 10 00:00:46,690 --> 00:00:50,820 Often, this molten rock forms in areas where ocean water 11 00:00:50,820 --> 00:00:56,094 is able to slip into the Earth’s mantle and lower the layer’s melting point. 12 00:00:56,094 --> 00:01:00,114 The resulting magma typically remains under the Earth’s surface 13 00:01:00,114 --> 00:01:04,226 thanks to the delicate balance of three geological factors. 14 00:01:04,226 --> 00:01:06,859 The first is lithostatic pressure. 15 00:01:06,859 --> 00:01:11,780 This is the weight of the Earth’s crust pushing down on the magma below. 16 00:01:11,780 --> 00:01:16,570 Magma pushes back with the second factor, magmastatic pressure. 17 00:01:16,570 --> 00:01:20,500 The battle between these forces strains the third factor: 18 00:01:20,500 --> 00:01:23,696 the rock strength of the Earth’s crust. 19 00:01:23,696 --> 00:01:26,846 Usually, the rock is strong enough and heavy enough 20 00:01:26,846 --> 00:01:28,916 to keep the magma in place. 21 00:01:28,916 --> 00:01:34,701 But when this equilibrium is thrown off, the consequences can be explosive. 22 00:01:34,701 --> 00:01:37,421 One of the most common causes of an eruption 23 00:01:37,421 --> 00:01:40,320 is an increase in magmastatic pressure. 24 00:01:40,320 --> 00:01:43,590 Magma contains various elements and compounds, 25 00:01:43,590 --> 00:01:46,740 many of which are dissolved in the molten rock. 26 00:01:46,740 --> 00:01:53,067 At high enough concentrations, compounds like water or sulfur no longer dissolve, 27 00:01:53,067 --> 00:01:56,887 and instead form high-pressure gas bubbles. 28 00:01:56,887 --> 00:01:59,122 When these bubbles reach the surface, 29 00:01:59,122 --> 00:02:02,320 they can burst with the force of a gunshot. 30 00:02:02,320 --> 00:02:05,950 And when millions of bubbles explode simultaneously, 31 00:02:05,950 --> 00:02:10,200 the energy can send plumes of ash into the stratosphere. 32 00:02:10,200 --> 00:02:15,495 But before they pop, they act like bubbles of C02 in a shaken soda. 33 00:02:15,495 --> 00:02:18,355 Their presence lowers the magma’s density, 34 00:02:18,355 --> 00:02:23,098 and increases the buoyant force pushing upward through the crust. 35 00:02:23,098 --> 00:02:28,191 Many geologists believe this process was behind the Paricutin eruption 36 00:02:28,191 --> 00:02:30,011 in Mexico. 37 00:02:30,011 --> 00:02:33,518 There are two known natural causes for these buoyant bubbles. 38 00:02:33,518 --> 00:02:36,688 Sometimes, new magma from deeper underground 39 00:02:36,688 --> 00:02:40,658 brings additional gassy compounds into the mix. 40 00:02:40,658 --> 00:02:44,806 But bubbles can also form when magma begins to cool. 41 00:02:44,806 --> 00:02:50,149 In its molten state, magma is a mixture of dissolved gases and melted minerals. 42 00:02:50,149 --> 00:02:55,621 As the molten rock hardens, some of those minerals solidify into crystals. 43 00:02:55,621 --> 00:02:59,621 This process doesn’t incorporate many of the dissolved gasses, 44 00:02:59,621 --> 00:03:02,912 resulting in a higher concentration of the compounds 45 00:03:02,912 --> 00:03:06,362 that form explosive bubbles. 46 00:03:06,362 --> 00:03:10,332 Not all eruptions are due to rising magmastatic pressure— 47 00:03:10,332 --> 00:03:15,062 sometimes the weight of the rock above can become dangerously low. 48 00:03:15,062 --> 00:03:20,231 Landslides can remove massive quantities of rock from atop a magma chamber, 49 00:03:20,231 --> 00:03:25,201 dropping the lithostatic pressure and instantly triggering an eruption. 50 00:03:25,201 --> 00:03:27,921 This process is known as “unloading” 51 00:03:27,921 --> 00:03:30,822 and it’s been responsible for numerous eruptions, 52 00:03:30,822 --> 00:03:35,544 including the sudden explosion of Mount St. Helens in 1980. 53 00:03:35,544 --> 00:03:39,114 But unloading can also happen over longer periods of time 54 00:03:39,114 --> 00:03:41,762 due to erosion or melting glaciers. 55 00:03:41,762 --> 00:03:45,232 In fact, many geologists are worried that glacial melt 56 00:03:45,232 --> 00:03:49,722 caused by climate change could increase volcanic activity. 57 00:03:49,722 --> 00:03:54,295 Finally, eruptions can occur when the rock layer is no longer strong enough 58 00:03:54,295 --> 00:03:56,735 to hold back the magma below. 59 00:03:56,735 --> 00:03:59,942 Acidic gases and heat escaping from magma 60 00:03:59,942 --> 00:04:04,568 can corrode rock through a process called hydrothermal alteration, 61 00:04:04,568 --> 00:04:08,448 gradually turning hard stone into soft clay. 62 00:04:08,448 --> 00:04:12,088 The rock layer could also be weakened by tectonic activity. 63 00:04:12,088 --> 00:04:16,777 Earthquakes can create fissures allowing magma to escape to the surface, 64 00:04:16,777 --> 00:04:19,789 and the Earth’s crust can be stretched thin 65 00:04:19,789 --> 00:04:23,267 as continental plates shift away from each other. 66 00:04:23,267 --> 00:04:26,217 Unfortunately, knowing what causes eruptions 67 00:04:26,217 --> 00:04:28,617 doesn’t make them easy to predict. 68 00:04:28,617 --> 00:04:31,837 While scientists can roughly determine the strength and weight 69 00:04:31,837 --> 00:04:33,227 of the Earth’s crust, 70 00:04:33,227 --> 00:04:37,007 the depth and heat of magma chambers makes measuring changes 71 00:04:37,007 --> 00:04:40,387 in magmastatic pressure very difficult. 72 00:04:40,387 --> 00:04:44,297 But volcanologists are constantly exploring new technology 73 00:04:44,297 --> 00:04:46,844 to conquer this rocky terrain. 74 00:04:46,844 --> 00:04:49,749 Advances in thermal imaging have allowed scientists 75 00:04:49,749 --> 00:04:52,409 to detect subterranean hotspots. 76 00:04:52,409 --> 00:04:55,839 Spectrometers can analyze gases escaping magma. 77 00:04:55,839 --> 00:05:02,103 And lasers can precisely track the impact of rising magma on a volcano’s shape. 78 00:05:02,103 --> 00:05:06,595 Hopefully, these tools will help us better understand these volatile vents 79 00:05:06,595 --> 00:05:08,801 and their explosive eruptions.