{"id":96,"date":"2017-01-23T16:35:20","date_gmt":"2017-01-23T16:35:20","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/chapter\/3-3-determining-the-structure-of-earth\/"},"modified":"2021-10-25T21:06:14","modified_gmt":"2021-10-25T21:06:14","slug":"3-3-determining-the-structure-of-earth","status":"publish","type":"chapter","link":"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/chapter\/3-3-determining-the-structure-of-earth\/","title":{"raw":"3.3 Determining the Structure of Earth","rendered":"3.3 Determining the Structure of Earth"},"content":{"raw":"<div>\r\n<div>\r\n\r\nThe previous section described the properties and composition of Earth's interior, which begs the question: how can we know what conditions are like deep in the Earth? It's easy to sample the [pb_glossary id=\"670\"]crust[\/pb_glossary] through drilling, and [pb_glossary id=\"930\"]mantle [\/pb_glossary] material often comes to the surface as magma, but the farthest we have been able to drill into the crust so far is only about 12 km; this for a planet with a radius of 6370 km! So to understand the composition and structure of the Earth's deep interior, we need to use indirect methods such as seismology.\r\n\r\n<strong>[pb_glossary id=\"1130\"]Seismology [\/pb_glossary]<\/strong> is the study of vibrations within the Earth. These vibrations are caused by various events, including earthquakes, extraterrestrial impacts, explosions, storm waves hitting the shore, and tidal effects. Of course, seismic techniques have been most widely applied to the detection and study of earthquakes, but there are many other applications, and arguably seismic waves provide the most important information that we have concerning Earth\u2019s interior. Before going any deeper into Earth, however, we need to take a look at the properties of seismic waves. The types of waves that are useful for understanding Earth\u2019s interior are called <strong>[pb_glossary id=\"596\"]body waves[\/pb_glossary]<\/strong>, meaning that, unlike the surface waves on the ocean, they are transmitted through Earth materials.\r\n\r\nImagine hitting a large block of strong rock (e.g., [pb_glossary id=\"786\"]granite[\/pb_glossary]) with a heavy sledgehammer. At the point where the hammer strikes it, a small part of the rock will be compressed by a fraction of a millimeter. That compression will transfer to the neighboring part of the rock, and so on through to the far side of the rock, from where it will bounce back to the top \u2014 all in a fraction of a second. This is known as a compression wave, and it can be illustrated by holding a loose spring (like a Slinky) that is attached to something (or someone) at the other end. If you give it a sharp push so the coils are compressed, the compression propagates (travels) along the length of the spring and back (Fig. 3.3.1). You can think of a compression wave as a \u201cpush\u201d wave \u2014 it\u2019s called a <strong>[pb_glossary id=\"1060\"]P-wave[\/pb_glossary]<\/strong> (although the \u201cP\u201d stands for \u201cprimary\u201d because P-waves are the first to arrive at seismic stations). In a P-wave the motion of the particles is parallel to the direction of wave propagation.\r\n\r\nWhen we hit a rock with a hammer, we also create a different type of body wave, one that is characterized by back-and-forth vibrations (as opposed to compressions). This is known as a shear wave (<strong>[pb_glossary id=\"1202\"]S-wave[\/pb_glossary]<\/strong>, where the \u201cS\u201d stands for \u201csecondary\u201d), and an analogy would be what happens when you flick a length of rope with an up-and-down motion. As shown in Figure 3.3.1, a wave will form in the rope, which will travel to the end of the rope and back. In this case, the motion of the particles is perpendicular to the direction the wave travels.\r\n\r\n[caption id=\"attachment_90\" align=\"aligncenter\" width=\"700\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2017\/01\/figure3.3.1.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-90\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-1024x683.png\" alt=\"A compression wave can be illustrated by a spring (like a Slinky) that is given a sharp push at one end. A shear wave can be illustrated by a rope that is given a quick flick\" width=\"700\" height=\"467\" \/><\/a> <strong>Figure 3.3.1<\/strong> Representations of a compression wave (P-wave, top) and a shear wave (S-wave, bottom) (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\nCompression waves and shear waves travel very quickly through geological materials. As shown in Figure 3.2.2, typical P-wave velocities are between 0.5 km\/s and 2.5 km\/s in unconsolidated sediments, and between 3.0 km\/s and 6.5 km\/s in solid crustal rocks. Of the common rocks of the crust, velocities are greatest in [pb_glossary id=\"570\"]basalt [\/pb_glossary] and [pb_glossary id=\"786\"]granite[\/pb_glossary]. S-waves are slower than P-waves, with velocities between 0.1 km\/s and 0.8 km\/s in soft [pb_glossary id=\"1126\"]sediments[\/pb_glossary], and between 1.5 km\/s and 3.8 km\/s in solid rocks.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_91\" align=\"aligncenter\" width=\"400\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.2.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-91\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2.png\" alt=\"Typical velocities of P waves (red) and S waves (blue) in sediments and in solid crustal rocks.\" width=\"400\" height=\"342\" \/><\/a> <strong>Figure 3.2.2<\/strong> Typical velocities of P waves (red) and S waves (blue) in sediments and in solid crustal rocks (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\n[pb_glossary id=\"930\"]Mantle [\/pb_glossary] rock is generally denser and stronger than [pb_glossary id=\"670\"]crustal [\/pb_glossary] rock and both P- and S-waves travel faster through the mantle than they do through the crust. Moreover, seismic-wave velocities are related to how tightly compressed a rock is, and the level of compression increases dramatically with depth. Finally, seismic waves are affected by the [pb_glossary id=\"1022\"]phase [\/pb_glossary] state of rock. They are slowed if there is any degree of melting in the rock. If the material is completely liquid, P-waves are slowed dramatically and S-waves are stopped altogether.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_92\" align=\"aligncenter\" width=\"800\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.3.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-92\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-1024x576.png\" alt=\"Wave velocities through the different layers of the Earth (left). Enhanced view of wave velocities in the crust and upper mantle (right)\" width=\"800\" height=\"450\" \/><\/a> <strong>Figure 3.3.3<\/strong> Wave velocities through the different layers of the Earth (left). Enhanced view of wave velocities in the crust and upper mantle (right) (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\nAccurate seismometers have been used for earthquake studies since the late 1800s, and systematic use of seismic data to understand Earth\u2019s interior started in the early 1900s. The rate of change of seismic waves with depth in the Earth (Fig. 3.3.3) has been determined over the past several decades by analyzing seismic signals from large earthquakes at seismic stations around the world. Small differences in arrival time of signals at different locations have been interpreted to show that:\r\n<ul>\r\n \t<li>Velocities are greater in mantle rock than in the crust.<\/li>\r\n \t<li>Velocities generally increase with pressure, and therefore with depth.<\/li>\r\n \t<li>Velocities slow in the area between 100 km and 250 km depth (called the \u201clow-velocity zone\u201d; equivalent to the [pb_glossary id=\"552\"]asthenosphere[\/pb_glossary]).<\/li>\r\n \t<li>Velocities increase dramatically at 660 km depth (because of a mineralogical transition).<\/li>\r\n \t<li>Velocities slow in the region just above the core-mantle boundary (the D\u201d layer or \u201cultra-low-velocity zone\u201d).<\/li>\r\n \t<li>S-waves do not pass through the outer part of the [pb_glossary id=\"660\"]core[\/pb_glossary].<\/li>\r\n \t<li>P-wave velocities increase dramatically at the boundary between the liquid [pb_glossary id=\"998\"]outer core[\/pb_glossary] and the solid [pb_glossary id=\"860\"]inner core[\/pb_glossary].<a href=\"http:\/\/opentextbc.ca\/geology\/wp-content\/uploads\/sites\/110\/2015\/07\/image018.png\">\r\n<\/a><\/li>\r\n<\/ul>\r\nOne of the first discoveries about Earth\u2019s interior made through seismology was in the early 1900s when Croatian seismologist Andrija Mohorovi\u010di\u0107 (pronounced <em>Moho-ro-vi-chich<\/em>) realized that at certain distances from an earthquake, two separate sets of seismic waves arrived at a seismic station within a few seconds of each other. He reasoned that the waves that went down into the mantle, traveled through the mantle, and then were bent upward back into the crust, reached the seismic station first because although they had farther to go, they traveled faster through mantle rock (as shown in Figure 3.3.4). The boundary between the crust and the mantle is known as the <strong>[pb_glossary id=\"954\"]Mohorovi\u010di\u0107 discontinuity[\/pb_glossary]<\/strong> (or <strong>Moho<\/strong>). Its depth is between 60 km and 80 km beneath major mountain ranges, around 30 km to 50 km beneath most of the continental crust, and between 5 km and 10 km beneath the oceanic crust.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_93\" align=\"aligncenter\" width=\"490\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.4.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-93 size-full\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4.png\" alt=\"Depiction of seismic waves emanating from an earthquake (red star). Some waves travel through the crust to the seismic station (at about 6 km\/s), while others go down into the mantle (where they travel at around 8 km\/s) and are bent upward toward the surface, reaching the station before the ones that traveled only through the crust.\" width=\"490\" height=\"118\" \/><\/a> <strong>Figure 3.3.4<\/strong> Depiction of seismic waves emanating from an earthquake (red star). Some waves travel through the crust to the seismic station (at about 6 km\/s), while others go down into the mantle (where they travel at around 8 km\/s) and are bent upward toward the surface, reaching the station before the ones that traveled only through the crust (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\nOur current understanding of the patterns of seismic wave transmission through Earth is summarized in Figure 3.3.5. Because of the gradual increase in [pb_glossary id=\"676\"]density [\/pb_glossary] with depth, all waves are refracted toward the lower density, slower velocity material as they travel through homogenous parts of Earth, and thus tend to curve outward toward the surface. Waves are also refracted at boundaries within Earth, such as at the [pb_glossary id=\"954\"]Moho[\/pb_glossary], at the core-mantle boundary (CMB), and at the outer-core\/inner-core boundary. [pb_glossary id=\"1202\"]S-waves[\/pb_glossary] do not travel through liquids \u2014 they are stopped at the CMB \u2014 and there is an S-wave shadow on the side of Earth opposite a seismic source. The angular distance from the seismic source to the shadow zone is 103\u00b0 on either side, so the total angular distance of the shadow zone is 154\u00b0. We can use this information to infer the depth to the CMB. [pb_glossary id=\"1060\"]P-waves[\/pb_glossary] do travel through liquids, so they can make it through the liquid part of the core. Because of the refraction that takes place at the CMB, waves that travel through the core are bent away from the surface, and this creates a P-wave shadow zone on either side, from 103\u00b0 to 150\u00b0. This information can be used to discover the differences between the inner and outer parts of the core.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_94\" align=\"aligncenter\" width=\"800\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.5.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-94\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-1024x480.png\" alt=\"Patterns of seismic waves moving through Earth's interior. Since S waves do not pass through the liquid outer core, a shadow zone is created on the opposite side from the original disturbance. S-wave patterns are illustrated on the right, and P-wave patterns are illustrated on the left.\" width=\"800\" height=\"375\" \/><\/a> <strong>Figure 3.3.5<\/strong> Patterns of seismic waves moving through Earth's interior. Since S waves do not pass through the liquid outer core, a shadow zone is created on the opposite side from the original disturbance (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\nUsing data from many seismometers and hundreds of earthquakes, it is possible to create a two- or three-dimensional image of the seismic properties of part of the [pb_glossary id=\"930\"]mantle[\/pb_glossary]. This technique is known as seismic tomography, and an example of the result is shown in Figure 3.3.6.\r\n\r\n&nbsp;\r\n\r\n[caption id=\"attachment_95\" align=\"aligncenter\" width=\"500\"]<a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.6.jpg\" target=\"_blank\" rel=\"noopener noreferrer\"><img class=\"wp-image-95\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6.jpg\" alt=\"Seismic tomography image showing the Pacific Plate (blue) subducting beneath Tonga\" width=\"500\" height=\"316\" \/><\/a> <strong>Figure 3.3.6<\/strong> Seismic tomography image showing the Pacific Plate (blue) subducting beneath Tonga (Steven Earle, \"Physical Geology\").[\/caption]\r\n\r\nThe Pacific Plate [pb_glossary id=\"1184\"]subducts [\/pb_glossary] beneath Tonga and appears in Figure 3.3.6 as a 100 km thick slab of cold (blue-colored) [pb_glossary id=\"990\"]oceanic crust[\/pb_glossary] that has pushed down into the surrounding hot mantle. The cold rock is more rigid than the surrounding hot mantle rock, so it is characterized by slightly faster seismic velocities. There is volcanism in the Lau spreading center and also in the Fiji area, and the warm rock in these areas has slower seismic velocities (yellow and red colors).\r\n\r\nSeismic waves provide us with the structure of the inner Earth, but what about it's other properties? In terms of composition, there are several lines of evidence pointing to a [pb_glossary id=\"660\"]core [\/pb_glossary] composed mostly of iron and nickel. Wave properties suggest the core is composed of an element with an atomic number around 25 (iron has an atomic number of 26). Aside from iron, all of the other elements with an atomic number close to 25 are too rare to make up the core. If the Earth was formed through the [pb_glossary id=\"530\"]accretion [\/pb_glossary] of smaller bodies such as [pb_glossary id=\"942\"]meteorites[\/pb_glossary], we would expect the composition of Earth to be similar to the composition of meteorites. Meteorites are mostly iron and nickel, but in higher proportions than the Earth's crust. This suggests that most of this heavy iron and nickel from the meteorites must have sunk to the Earth's center as the planet was forming. However, the core is not dense enough to be pure iron and nickel; it it about 10% below the predicted [pb_glossary id=\"676\"]density [\/pb_glossary] if that was the case. This is why scientists believe the core is composed of about 10% sulfur, oxygen, and hydrogen. Finally, if the Earth's magnetic field comes from the fluid outer core, the outer core must contain iron. In terms of the temperatures, we can calculate the melting points of these materials over the range of pressures that they would experience in the inner Earth, and then infer the temperatures that would allow these elements to exist in their solid or liquid forms.\r\n\r\n<hr \/>\r\n\r\n*\"Physical Geology\" by Steven Earle used under a CC-BY 4.0 international license. Download this book for free at http:\/\/open.bccampus.ca\r\n\r\n<\/div>\r\n<\/div>","rendered":"<div>\n<div>\n<p>The previous section described the properties and composition of Earth&#8217;s interior, which begs the question: how can we know what conditions are like deep in the Earth? It&#8217;s easy to sample the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_670\">crust<\/a> through drilling, and <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_930\">mantle <\/a> material often comes to the surface as magma, but the farthest we have been able to drill into the crust so far is only about 12 km; this for a planet with a radius of 6370 km! So to understand the composition and structure of the Earth&#8217;s deep interior, we need to use indirect methods such as seismology.<\/p>\n<p><strong><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1130\">Seismology <\/a><\/strong> is the study of vibrations within the Earth. These vibrations are caused by various events, including earthquakes, extraterrestrial impacts, explosions, storm waves hitting the shore, and tidal effects. Of course, seismic techniques have been most widely applied to the detection and study of earthquakes, but there are many other applications, and arguably seismic waves provide the most important information that we have concerning Earth\u2019s interior. Before going any deeper into Earth, however, we need to take a look at the properties of seismic waves. The types of waves that are useful for understanding Earth\u2019s interior are called <strong><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_596\">body waves<\/a><\/strong>, meaning that, unlike the surface waves on the ocean, they are transmitted through Earth materials.<\/p>\n<p>Imagine hitting a large block of strong rock (e.g., <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_786\">granite<\/a>) with a heavy sledgehammer. At the point where the hammer strikes it, a small part of the rock will be compressed by a fraction of a millimeter. That compression will transfer to the neighboring part of the rock, and so on through to the far side of the rock, from where it will bounce back to the top \u2014 all in a fraction of a second. This is known as a compression wave, and it can be illustrated by holding a loose spring (like a Slinky) that is attached to something (or someone) at the other end. If you give it a sharp push so the coils are compressed, the compression propagates (travels) along the length of the spring and back (Fig. 3.3.1). You can think of a compression wave as a \u201cpush\u201d wave \u2014 it\u2019s called a <strong><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1060\">P-wave<\/a><\/strong> (although the \u201cP\u201d stands for \u201cprimary\u201d because P-waves are the first to arrive at seismic stations). In a P-wave the motion of the particles is parallel to the direction of wave propagation.<\/p>\n<p>When we hit a rock with a hammer, we also create a different type of body wave, one that is characterized by back-and-forth vibrations (as opposed to compressions). This is known as a shear wave (<strong><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1202\">S-wave<\/a><\/strong>, where the \u201cS\u201d stands for \u201csecondary\u201d), and an analogy would be what happens when you flick a length of rope with an up-and-down motion. As shown in Figure 3.3.1, a wave will form in the rope, which will travel to the end of the rope and back. In this case, the motion of the particles is perpendicular to the direction the wave travels.<\/p>\n<figure id=\"attachment_90\" aria-describedby=\"caption-attachment-90\" style=\"width: 700px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2017\/01\/figure3.3.1.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-90\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-1024x683.png\" alt=\"A compression wave can be illustrated by a spring (like a Slinky) that is given a sharp push at one end. A shear wave can be illustrated by a rope that is given a quick flick\" width=\"700\" height=\"467\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-1024x683.png 1024w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-300x200.png 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-768x512.png 768w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-1536x1024.png 1536w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-65x43.png 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-225x150.png 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1-350x233.png 350w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2017\/01\/figure3.3.1.png 1564w\" sizes=\"auto, (max-width: 700px) 100vw, 700px\" \/><\/a><figcaption id=\"caption-attachment-90\" class=\"wp-caption-text\"><strong>Figure 3.3.1<\/strong> Representations of a compression wave (P-wave, top) and a shear wave (S-wave, bottom) (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p>Compression waves and shear waves travel very quickly through geological materials. As shown in Figure 3.2.2, typical P-wave velocities are between 0.5 km\/s and 2.5 km\/s in unconsolidated sediments, and between 3.0 km\/s and 6.5 km\/s in solid crustal rocks. Of the common rocks of the crust, velocities are greatest in <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_570\">basalt <\/a> and <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_786\">granite<\/a>. S-waves are slower than P-waves, with velocities between 0.1 km\/s and 0.8 km\/s in soft <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1126\">sediments<\/a>, and between 1.5 km\/s and 3.8 km\/s in solid rocks.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_91\" aria-describedby=\"caption-attachment-91\" style=\"width: 400px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.2.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-91\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2.png\" alt=\"Typical velocities of P waves (red) and S waves (blue) in sediments and in solid crustal rocks.\" width=\"400\" height=\"342\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2.png 572w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2-300x256.png 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2-65x56.png 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2-225x192.png 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.2-350x299.png 350w\" sizes=\"auto, (max-width: 400px) 100vw, 400px\" \/><\/a><figcaption id=\"caption-attachment-91\" class=\"wp-caption-text\"><strong>Figure 3.2.2<\/strong> Typical velocities of P waves (red) and S waves (blue) in sediments and in solid crustal rocks (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_930\">Mantle <\/a> rock is generally denser and stronger than <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_670\">crustal <\/a> rock and both P- and S-waves travel faster through the mantle than they do through the crust. Moreover, seismic-wave velocities are related to how tightly compressed a rock is, and the level of compression increases dramatically with depth. Finally, seismic waves are affected by the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1022\">phase <\/a> state of rock. They are slowed if there is any degree of melting in the rock. If the material is completely liquid, P-waves are slowed dramatically and S-waves are stopped altogether.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_92\" aria-describedby=\"caption-attachment-92\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.3.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-92\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-1024x576.png\" alt=\"Wave velocities through the different layers of the Earth (left). Enhanced view of wave velocities in the crust and upper mantle (right)\" width=\"800\" height=\"450\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-1024x576.png 1024w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-300x169.png 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-768x432.png 768w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-1536x864.png 1536w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-2048x1152.png 2048w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-65x37.png 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-225x127.png 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.3-350x197.png 350w\" sizes=\"auto, (max-width: 800px) 100vw, 800px\" \/><\/a><figcaption id=\"caption-attachment-92\" class=\"wp-caption-text\"><strong>Figure 3.3.3<\/strong> Wave velocities through the different layers of the Earth (left). Enhanced view of wave velocities in the crust and upper mantle (right) (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p>Accurate seismometers have been used for earthquake studies since the late 1800s, and systematic use of seismic data to understand Earth\u2019s interior started in the early 1900s. The rate of change of seismic waves with depth in the Earth (Fig. 3.3.3) has been determined over the past several decades by analyzing seismic signals from large earthquakes at seismic stations around the world. Small differences in arrival time of signals at different locations have been interpreted to show that:<\/p>\n<ul>\n<li>Velocities are greater in mantle rock than in the crust.<\/li>\n<li>Velocities generally increase with pressure, and therefore with depth.<\/li>\n<li>Velocities slow in the area between 100 km and 250 km depth (called the \u201clow-velocity zone\u201d; equivalent to the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_552\">asthenosphere<\/a>).<\/li>\n<li>Velocities increase dramatically at 660 km depth (because of a mineralogical transition).<\/li>\n<li>Velocities slow in the region just above the core-mantle boundary (the D\u201d layer or \u201cultra-low-velocity zone\u201d).<\/li>\n<li>S-waves do not pass through the outer part of the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_660\">core<\/a>.<\/li>\n<li>P-wave velocities increase dramatically at the boundary between the liquid <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_998\">outer core<\/a> and the solid <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_860\">inner core<\/a>.<a href=\"http:\/\/opentextbc.ca\/geology\/wp-content\/uploads\/sites\/110\/2015\/07\/image018.png\"><br \/>\n<\/a><\/li>\n<\/ul>\n<p>One of the first discoveries about Earth\u2019s interior made through seismology was in the early 1900s when Croatian seismologist Andrija Mohorovi\u010di\u0107 (pronounced <em>Moho-ro-vi-chich<\/em>) realized that at certain distances from an earthquake, two separate sets of seismic waves arrived at a seismic station within a few seconds of each other. He reasoned that the waves that went down into the mantle, traveled through the mantle, and then were bent upward back into the crust, reached the seismic station first because although they had farther to go, they traveled faster through mantle rock (as shown in Figure 3.3.4). The boundary between the crust and the mantle is known as the <strong><a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_954\">Mohorovi\u010di\u0107 discontinuity<\/a><\/strong> (or <strong>Moho<\/strong>). Its depth is between 60 km and 80 km beneath major mountain ranges, around 30 km to 50 km beneath most of the continental crust, and between 5 km and 10 km beneath the oceanic crust.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_93\" aria-describedby=\"caption-attachment-93\" style=\"width: 490px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.4.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-93 size-full\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4.png\" alt=\"Depiction of seismic waves emanating from an earthquake (red star). Some waves travel through the crust to the seismic station (at about 6 km\/s), while others go down into the mantle (where they travel at around 8 km\/s) and are bent upward toward the surface, reaching the station before the ones that traveled only through the crust.\" width=\"490\" height=\"118\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4.png 490w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4-300x72.png 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4-65x16.png 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4-225x54.png 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.4-350x84.png 350w\" sizes=\"auto, (max-width: 490px) 100vw, 490px\" \/><\/a><figcaption id=\"caption-attachment-93\" class=\"wp-caption-text\"><strong>Figure 3.3.4<\/strong> Depiction of seismic waves emanating from an earthquake (red star). Some waves travel through the crust to the seismic station (at about 6 km\/s), while others go down into the mantle (where they travel at around 8 km\/s) and are bent upward toward the surface, reaching the station before the ones that traveled only through the crust (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p>Our current understanding of the patterns of seismic wave transmission through Earth is summarized in Figure 3.3.5. Because of the gradual increase in <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_676\">density <\/a> with depth, all waves are refracted toward the lower density, slower velocity material as they travel through homogenous parts of Earth, and thus tend to curve outward toward the surface. Waves are also refracted at boundaries within Earth, such as at the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_954\">Moho<\/a>, at the core-mantle boundary (CMB), and at the outer-core\/inner-core boundary. <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1202\">S-waves<\/a> do not travel through liquids \u2014 they are stopped at the CMB \u2014 and there is an S-wave shadow on the side of Earth opposite a seismic source. The angular distance from the seismic source to the shadow zone is 103\u00b0 on either side, so the total angular distance of the shadow zone is 154\u00b0. We can use this information to infer the depth to the CMB. <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1060\">P-waves<\/a> do travel through liquids, so they can make it through the liquid part of the core. Because of the refraction that takes place at the CMB, waves that travel through the core are bent away from the surface, and this creates a P-wave shadow zone on either side, from 103\u00b0 to 150\u00b0. This information can be used to discover the differences between the inner and outer parts of the core.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_94\" aria-describedby=\"caption-attachment-94\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.5.png\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-94\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-1024x480.png\" alt=\"Patterns of seismic waves moving through Earth's interior. Since S waves do not pass through the liquid outer core, a shadow zone is created on the opposite side from the original disturbance. S-wave patterns are illustrated on the right, and P-wave patterns are illustrated on the left.\" width=\"800\" height=\"375\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-1024x480.png 1024w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-300x141.png 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-768x360.png 768w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-65x30.png 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-225x105.png 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5-350x164.png 350w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.5.png 1314w\" sizes=\"auto, (max-width: 800px) 100vw, 800px\" \/><\/a><figcaption id=\"caption-attachment-94\" class=\"wp-caption-text\"><strong>Figure 3.3.5<\/strong> Patterns of seismic waves moving through Earth&#8217;s interior. Since S waves do not pass through the liquid outer core, a shadow zone is created on the opposite side from the original disturbance (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p>Using data from many seismometers and hundreds of earthquakes, it is possible to create a two- or three-dimensional image of the seismic properties of part of the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_930\">mantle<\/a>. This technique is known as seismic tomography, and an example of the result is shown in Figure 3.3.6.<\/p>\n<p>&nbsp;<\/p>\n<figure id=\"attachment_95\" aria-describedby=\"caption-attachment-95\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/rwu.pressbooks.pub\/app\/uploads\/sites\/7\/2019\/05\/figure3.3.6.jpg\" target=\"_blank\" rel=\"noopener noreferrer\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-95\" src=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6.jpg\" alt=\"Seismic tomography image showing the Pacific Plate (blue) subducting beneath Tonga\" width=\"500\" height=\"316\" srcset=\"https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6.jpg 794w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6-300x190.jpg 300w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6-768x486.jpg 768w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6-65x41.jpg 65w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6-225x142.jpg 225w, https:\/\/pressbooks.ccconline.org\/introduction-to-oceanography\/wp-content\/uploads\/sites\/16\/2021\/10\/figure3.3.6-350x221.jpg 350w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-95\" class=\"wp-caption-text\"><strong>Figure 3.3.6<\/strong> Seismic tomography image showing the Pacific Plate (blue) subducting beneath Tonga (Steven Earle, &#8220;Physical Geology&#8221;).<\/figcaption><\/figure>\n<p>The Pacific Plate <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_1184\">subducts <\/a> beneath Tonga and appears in Figure 3.3.6 as a 100 km thick slab of cold (blue-colored) <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_990\">oceanic crust<\/a> that has pushed down into the surrounding hot mantle. The cold rock is more rigid than the surrounding hot mantle rock, so it is characterized by slightly faster seismic velocities. There is volcanism in the Lau spreading center and also in the Fiji area, and the warm rock in these areas has slower seismic velocities (yellow and red colors).<\/p>\n<p>Seismic waves provide us with the structure of the inner Earth, but what about it&#8217;s other properties? In terms of composition, there are several lines of evidence pointing to a <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_660\">core <\/a> composed mostly of iron and nickel. Wave properties suggest the core is composed of an element with an atomic number around 25 (iron has an atomic number of 26). Aside from iron, all of the other elements with an atomic number close to 25 are too rare to make up the core. If the Earth was formed through the <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_530\">accretion <\/a> of smaller bodies such as <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_942\">meteorites<\/a>, we would expect the composition of Earth to be similar to the composition of meteorites. Meteorites are mostly iron and nickel, but in higher proportions than the Earth&#8217;s crust. This suggests that most of this heavy iron and nickel from the meteorites must have sunk to the Earth&#8217;s center as the planet was forming. However, the core is not dense enough to be pure iron and nickel; it it about 10% below the predicted <a class=\"glossary-term\" aria-haspopup=\"dialog\" aria-describedby=\"definition\" href=\"#term_96_676\">density <\/a> if that was the case. This is why scientists believe the core is composed of about 10% sulfur, oxygen, and hydrogen. Finally, if the Earth&#8217;s magnetic field comes from the fluid outer core, the outer core must contain iron. In terms of the temperatures, we can calculate the melting points of these materials over the range of pressures that they would experience in the inner Earth, and then infer the temperatures that would allow these elements to exist in their solid or liquid forms.<\/p>\n<hr \/>\n<p>*&#8221;Physical Geology&#8221; by Steven Earle used under a CC-BY 4.0 international license. Download this book for free at http:\/\/open.bccampus.ca<\/p>\n<\/div>\n<\/div>\n<div class=\"glossary\"><span class=\"screen-reader-text\" id=\"definition\">definition<\/span><template id=\"term_96_670\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_670\"><div tabindex=\"-1\"><p>the uppermost layer of the Earth, ranging in thickness from about 5 km (in the oceans) to over 50 km (on the continents) (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_930\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_930\"><div tabindex=\"-1\"><p>the middle layer of the Earth, dominated by iron and magnesium rich silicate minerals and extending for about 2900 km from the base of the crust to the top of the core (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1130\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1130\"><div tabindex=\"-1\"><p>the study of vibrations within the Earth (3.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_596\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_596\"><div tabindex=\"-1\"><p>a seismic wave that travels through rock (e.g., a P-wave or an S-wave) (3.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_786\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_786\"><div tabindex=\"-1\"><p>an igneous (formed from cooling magma) rock that comprises much of the continental crust (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1060\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1060\"><div tabindex=\"-1\"><p>a seismic body wave that is characterized by deformation of the rock in the same direction that the wave is propagating (compressional vibration) (3.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1202\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1202\"><div tabindex=\"-1\"><p>a seismic body wave that is characterized by deformation of the rock perpendicular to the direction that the wave is propagating (3.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_570\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_570\"><div tabindex=\"-1\"><p>a volcanic rock that makes up much of the oceanic crust (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1126\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1126\"><div tabindex=\"-1\"><p>unconsolidated particles of mineral or rock that settle to the seafloor (12.1)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1022\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1022\"><div tabindex=\"-1\"><p>the change of state between a solid, liquid, or gas (8.1)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_552\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_552\"><div tabindex=\"-1\"><p>the part of the mantle, from about 100 to 200 km below surface, within which the mantle material is close to its melting point, and therefore relatively weak (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_660\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_660\"><div tabindex=\"-1\"><p>the metallic interior part of the Earth, extending from a depth of 2900 km to the center (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_998\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_998\"><div tabindex=\"-1\"><p>the layer of the inner Earth extending 2300 km from the top of the inner core to the bottom of the mantle, composed of fluid metal alloys (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_860\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_860\"><div tabindex=\"-1\"><p>the solid metal mass at the center of the Earth, extending 1200 km from the center (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_954\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_954\"><div tabindex=\"-1\"><p>the boundary between the crust and the mantle (3.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_676\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_676\"><div tabindex=\"-1\"><p>mass per unit volume of a substance (e.g., g\/cubic cm) (6.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_1184\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_1184\"><div tabindex=\"-1\"><p>when part of a plate is forced beneath another plate along a subduction zone (4.3)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_990\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_990\"><div tabindex=\"-1\"><p>the Earth\u2019s crust underlying the oceans (as opposed to continental crust) (3.2)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_530\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_530\"><div tabindex=\"-1\"><p>the process by which solid celestial bodies are added to existing bodies during collisions (3.1)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><template id=\"term_96_942\"><div class=\"glossary__definition\" role=\"dialog\" data-id=\"term_96_942\"><div tabindex=\"-1\"><p>a fragment of either stony or metallic debris in space (12.5)<\/p>\n<\/div><button><span aria-hidden=\"true\">&times;<\/span><span class=\"screen-reader-text\">Close definition<\/span><\/button><\/div><\/template><\/div>","protected":false},"author":33,"menu_order":13,"template":"","meta":{"pb_show_title":"on","pb_short_title":"","pb_subtitle":"Modified from 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