{"id":872,"date":"2017-04-26T21:48:25","date_gmt":"2017-04-26T21:48:25","guid":{"rendered":"https:\/\/courses.lumenlearning.com\/geophysical\/?post_type=chapter&#038;p=872"},"modified":"2017-04-27T21:05:49","modified_gmt":"2017-04-27T21:05:49","slug":"causes-of-long-term-climate-change","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/chapter\/causes-of-long-term-climate-change\/","title":{"raw":"Causes of Long-term Climate Change","rendered":"Causes of Long-term Climate Change"},"content":{"raw":"Many processes can cause climate to change. These include changes in the amount of energy the Sun produces over years; the positions of the continents over millions of years; in the tilt of Earth's axis; orbit over thousands of years; that are sudden and dramatic because of random catastrophic events, such as a large asteroid impact; in greenhouse gases in the atmosphere, caused naturally or by human activities.\r\n<h2>Plate Tectonics<\/h2>\r\nPlate tectonic movements can alter climate. Over millions of years as seas open and close, ocean currents may distribute heat differently. For example, when all the continents are joined into one supercontinent (such as Pangaea), nearly all locations experience a continental climate. When the continents separate, heat is more evenly distributed.Plate tectonic movements may help start an ice age. When continents are located near the poles, ice can accumulate, which may increase albedo and lower global temperature. Low enough temperatures may start a global ice age.\r\n\r\n<img class=\"aligncenter size-large wp-image-938\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27205536\/2008_age_of_oceans_plates-1024x616.jpg\" alt=\"Colors indicate age of oceanic lithosphere, lines represent tectonic plates, world map. The lithosphere is youngest near the tectonic plate boundaries.\" width=\"1024\" height=\"616\" \/>\r\n\r\nPlate motions trigger volcanic eruptions, which release dust and CO<sub>2<\/sub> into the atmosphere. Ordinary eruptions, even large ones, have only a short-term effect on weather. Massive eruptions of the fluid lavas that create lava plateaus release much more gas and dust, and can change climate for many years. This type of eruption is exceedingly rare; none has occurred since humans have lived on Earth.\r\n<h2>Milankovitch Cycles<\/h2>\r\nThe most extreme climate of recent Earth history was the Pleistocene. Scientists attribute a series of ice ages to variation in the Earth's position relative to the Sun, known as <strong>Milankovitch cycles<\/strong>. The Earth goes through regular variations in its position relative to the Sun:\r\n\r\n<img class=\"aligncenter size-large wp-image-937\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27203544\/rotations-1024x276.jpg\" alt=\"A four part image. Part A shows an orbit with eccentricity zero. Part B shows an orbit with an eccentricity of 0.5\u2014its shape is ovular. Part C shows the precession of Earth's rotational axis due to the tidal force raised on Earth by the gravity of the Moon and Sun. Part D shows the range of the tilt of Earth's axis of rotation (obliquity). Present tilt is 23.4 degrees.\" width=\"1024\" height=\"276\" \/>\r\n\r\nThe shape of the Earth's orbit changes slightly as it goes around the Sun. The orbit varies from more circular to more elliptical in a cycle lasting between 90,000 and 100,000 years. When the orbit is more elliptical, there is a greater difference in solar radiation between winter and summer.\r\n\r\nThe planet wobbles on its axis of rotation. At one extreme of this 27,000 year cycle, the Northern Hemisphere points toward the Sun when the Earth is closest to the Sun. Summers are much warmer and winters are much colder than now. At the opposite extreme, the Northern Hemisphere points toward the Sun when it is farthest from the Sun. This results in chilly summers and warmer winters.The planet\u2019s tilt on its axis varies between 22.1 degrees and 24.5 degrees. Seasons are caused by the tilt of Earth's axis of rotation, which is at a 23.5o angle now. When the tilt angle is smaller, summers and winters differ less in temperature. This cycle lasts 41,000 years.\r\n\r\nWhen these three variations are charted out, a climate pattern of about 100,000 years emerges. Ice ages correspond closely with Milankovitch cycles. Since glaciers can form only over land, ice ages only occur when landmasses cover the polar regions. Therefore, Milankovitch cycles are also connected to plate tectonics.\r\n<h2>Sun Variation<\/h2>\r\n<img class=\"alignright wp-image-939\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27205631\/Activity_Continues_On_the_Sun-e1493326823354.jpg\" alt=\"The sun's surface is variable. There are three black sun spots on the surface.\" width=\"400\" height=\"223\" \/>The amount of energy the Sun radiates is variable. <strong>Sunspots<\/strong> are magnetic storms on the Sun\u2019s surface that increase and decrease over an eleven-year cycle. When the number of sunspots is high, solar radiation is also relatively high. But the entire variation in solar radiation is tiny relative to the total amount of solar radiation that there is and there is no known eleven-year cycle in climate variability.\r\n\r\nThe Little Ice Age corresponded to a time when there were no sunspots on the Sun.\r\n<h2>Changes in Atmospheric Greenhouse Gas Levels<\/h2>\r\n<img class=\"alignright wp-image-940\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27210153\/mauna-loa-co2-1955-2005.jpg\" alt=\"Carbon dioxide has been steadily rising since 1995, with yearly cycling. \" width=\"400\" height=\"300\" \/>Since greenhouse gases trap the heat that radiates off the planet\u2019s surfaces what would happen to global temperatures if atmospheric greenhouse gas levels decreased? What if greenhouse gases increased? A decrease in greenhouse gas levels decreases global temperature and an increase raises air temperature.\r\n\r\nGreenhouse gas levels have varied throughout Earth history. For example, CO<sub>2<\/sub> has been present at concentrations less than 200 parts per million (ppm) and more than 5,000 ppm. But for at least 650,000 years, CO<sub>2<\/sub> has never risen above 300 ppm, during either glacial or interglacial periods. Natural processes add (volcanic eruptions and the decay or burning of organic matter) and remove absorption by plants, animal tissue, and the ocean) CO<sub>2<\/sub> from the atmosphere. When plants are turned into fossil fuels the CO<sub>2<\/sub> in their tissue is stored with them. So CO<sub>2<\/sub> is removed from the atmosphere. What does this do to Earth\u2019s average temperature?\r\n\r\nFossil fuel use has skyrocketed in the past few decades more people want more cars and industrial products. This has released CO<sub>2<\/sub> into the atmosphere.\r\n\r\nBurning tropical rainforests, to clear land for agriculture, a practice called <strong>slash-and-burn agriculture<\/strong>, also increases atmospheric CO<sub>2<\/sub>. By cutting down trees, they can no longer remove CO<sub>2<\/sub> from the atmosphere. Burning the trees releases all the CO<sub>2<\/sub> stored in the trees into the atmosphere.\r\n\r\nThere is now nearly 40\u00a0percent more CO<sub>2<\/sub> in the atmosphere than there was 200 years ago, before the Industrial Revolution. About 65 percent of that increase has occurred since the first CO<sub>2<\/sub> measurements were made on Mauna Loa Volcano, Hawaii, in 1958. CO<sub>2<\/sub> is the most important greenhouse gas that human activities affect because it is so abundant. But other greenhouse gases are increasing as well. A few are:\r\n<ul>\r\n \t<li>Methane: released from raising livestock, rice production, and the incomplete burning of rainforest plants.<\/li>\r\n \t<li>Chlorofluorocarbons (CFCs): human-made chemicals that were invented and used widely in the twentieth\u00a0century.<\/li>\r\n \t<li>Tropospheric ozone: from vehicle exhaust, it has more than doubled since 1976.<\/li>\r\n<\/ul>","rendered":"<p>Many processes can cause climate to change. These include changes in the amount of energy the Sun produces over years; the positions of the continents over millions of years; in the tilt of Earth&#8217;s axis; orbit over thousands of years; that are sudden and dramatic because of random catastrophic events, such as a large asteroid impact; in greenhouse gases in the atmosphere, caused naturally or by human activities.<\/p>\n<h2>Plate Tectonics<\/h2>\n<p>Plate tectonic movements can alter climate. Over millions of years as seas open and close, ocean currents may distribute heat differently. For example, when all the continents are joined into one supercontinent (such as Pangaea), nearly all locations experience a continental climate. When the continents separate, heat is more evenly distributed.Plate tectonic movements may help start an ice age. When continents are located near the poles, ice can accumulate, which may increase albedo and lower global temperature. Low enough temperatures may start a global ice age.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter size-large wp-image-938\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27205536\/2008_age_of_oceans_plates-1024x616.jpg\" alt=\"Colors indicate age of oceanic lithosphere, lines represent tectonic plates, world map. The lithosphere is youngest near the tectonic plate boundaries.\" width=\"1024\" height=\"616\" \/><\/p>\n<p>Plate motions trigger volcanic eruptions, which release dust and CO<sub>2<\/sub> into the atmosphere. Ordinary eruptions, even large ones, have only a short-term effect on weather. Massive eruptions of the fluid lavas that create lava plateaus release much more gas and dust, and can change climate for many years. This type of eruption is exceedingly rare; none has occurred since humans have lived on Earth.<\/p>\n<h2>Milankovitch Cycles<\/h2>\n<p>The most extreme climate of recent Earth history was the Pleistocene. Scientists attribute a series of ice ages to variation in the Earth&#8217;s position relative to the Sun, known as <strong>Milankovitch cycles<\/strong>. The Earth goes through regular variations in its position relative to the Sun:<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter size-large wp-image-937\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27203544\/rotations-1024x276.jpg\" alt=\"A four part image. Part A shows an orbit with eccentricity zero. Part B shows an orbit with an eccentricity of 0.5\u2014its shape is ovular. Part C shows the precession of Earth's rotational axis due to the tidal force raised on Earth by the gravity of the Moon and Sun. Part D shows the range of the tilt of Earth's axis of rotation (obliquity). Present tilt is 23.4 degrees.\" width=\"1024\" height=\"276\" \/><\/p>\n<p>The shape of the Earth&#8217;s orbit changes slightly as it goes around the Sun. The orbit varies from more circular to more elliptical in a cycle lasting between 90,000 and 100,000 years. When the orbit is more elliptical, there is a greater difference in solar radiation between winter and summer.<\/p>\n<p>The planet wobbles on its axis of rotation. At one extreme of this 27,000 year cycle, the Northern Hemisphere points toward the Sun when the Earth is closest to the Sun. Summers are much warmer and winters are much colder than now. At the opposite extreme, the Northern Hemisphere points toward the Sun when it is farthest from the Sun. This results in chilly summers and warmer winters.The planet\u2019s tilt on its axis varies between 22.1 degrees and 24.5 degrees. Seasons are caused by the tilt of Earth&#8217;s axis of rotation, which is at a 23.5o angle now. When the tilt angle is smaller, summers and winters differ less in temperature. This cycle lasts 41,000 years.<\/p>\n<p>When these three variations are charted out, a climate pattern of about 100,000 years emerges. Ice ages correspond closely with Milankovitch cycles. Since glaciers can form only over land, ice ages only occur when landmasses cover the polar regions. Therefore, Milankovitch cycles are also connected to plate tectonics.<\/p>\n<h2>Sun Variation<\/h2>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignright wp-image-939\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27205631\/Activity_Continues_On_the_Sun-e1493326823354.jpg\" alt=\"The sun's surface is variable. There are three black sun spots on the surface.\" width=\"400\" height=\"223\" \/>The amount of energy the Sun radiates is variable. <strong>Sunspots<\/strong> are magnetic storms on the Sun\u2019s surface that increase and decrease over an eleven-year cycle. When the number of sunspots is high, solar radiation is also relatively high. But the entire variation in solar radiation is tiny relative to the total amount of solar radiation that there is and there is no known eleven-year cycle in climate variability.<\/p>\n<p>The Little Ice Age corresponded to a time when there were no sunspots on the Sun.<\/p>\n<h2>Changes in Atmospheric Greenhouse Gas Levels<\/h2>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignright wp-image-940\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/250\/2017\/04\/27210153\/mauna-loa-co2-1955-2005.jpg\" alt=\"Carbon dioxide has been steadily rising since 1995, with yearly cycling.\" width=\"400\" height=\"300\" \/>Since greenhouse gases trap the heat that radiates off the planet\u2019s surfaces what would happen to global temperatures if atmospheric greenhouse gas levels decreased? What if greenhouse gases increased? A decrease in greenhouse gas levels decreases global temperature and an increase raises air temperature.<\/p>\n<p>Greenhouse gas levels have varied throughout Earth history. For example, CO<sub>2<\/sub> has been present at concentrations less than 200 parts per million (ppm) and more than 5,000 ppm. But for at least 650,000 years, CO<sub>2<\/sub> has never risen above 300 ppm, during either glacial or interglacial periods. Natural processes add (volcanic eruptions and the decay or burning of organic matter) and remove absorption by plants, animal tissue, and the ocean) CO<sub>2<\/sub> from the atmosphere. When plants are turned into fossil fuels the CO<sub>2<\/sub> in their tissue is stored with them. So CO<sub>2<\/sub> is removed from the atmosphere. What does this do to Earth\u2019s average temperature?<\/p>\n<p>Fossil fuel use has skyrocketed in the past few decades more people want more cars and industrial products. This has released CO<sub>2<\/sub> into the atmosphere.<\/p>\n<p>Burning tropical rainforests, to clear land for agriculture, a practice called <strong>slash-and-burn agriculture<\/strong>, also increases atmospheric CO<sub>2<\/sub>. By cutting down trees, they can no longer remove CO<sub>2<\/sub> from the atmosphere. Burning the trees releases all the CO<sub>2<\/sub> stored in the trees into the atmosphere.<\/p>\n<p>There is now nearly 40\u00a0percent more CO<sub>2<\/sub> in the atmosphere than there was 200 years ago, before the Industrial Revolution. About 65 percent of that increase has occurred since the first CO<sub>2<\/sub> measurements were made on Mauna Loa Volcano, Hawaii, in 1958. CO<sub>2<\/sub> is the most important greenhouse gas that human activities affect because it is so abundant. But other greenhouse gases are increasing as well. A few are:<\/p>\n<ul>\n<li>Methane: released from raising livestock, rice production, and the incomplete burning of rainforest plants.<\/li>\n<li>Chlorofluorocarbons (CFCs): human-made chemicals that were invented and used widely in the twentieth\u00a0century.<\/li>\n<li>Tropospheric ozone: from vehicle exhaust, it has more than doubled since 1976.<\/li>\n<\/ul>\n\n\t\t\t <section class=\"citations-section\" role=\"contentinfo\">\n\t\t\t <h3>Candela Citations<\/h3>\n\t\t\t\t\t <div>\n\t\t\t\t\t\t <div id=\"citation-list-872\">\n\t\t\t\t\t\t\t <div class=\"licensing\"><div class=\"license-attribution-dropdown-subheading\">CC licensed content, Shared previously<\/div><ul class=\"citation-list\"><li>Dynamic Earth: Introduction to Physical Geography. <strong>Authored by<\/strong>: R. Adam Dastrup. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"http:\/\/www.opengeography.org\/physical-geography.html\">http:\/\/www.opengeography.org\/physical-geography.html<\/a>. <strong>Project<\/strong>: Open Geography Education. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/licenses\/by-sa\/4.0\/\">CC BY-SA: Attribution-ShareAlike<\/a><\/em><\/li><\/ul><div class=\"license-attribution-dropdown-subheading\">Public domain content<\/div><ul class=\"citation-list\"><li>2008 age of oceans plates. <strong>Provided by<\/strong>: NOAA. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:2008_age_of_oceans_plates.jpg\">https:\/\/commons.wikimedia.org\/wiki\/File:2008_age_of_oceans_plates.jpg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Eccentricity zero. <strong>Provided by<\/strong>: NASA, Mysid. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_zero.svg\">https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_zero.svg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Eccentricity half. <strong>Provided by<\/strong>: NASA, Mysid. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_half.svg\">https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_half.svg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Earth precession. <strong>Provided by<\/strong>: NASA, Mysid. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Earth_precession.svg\">https:\/\/commons.wikimedia.org\/wiki\/File:Earth_precession.svg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Earth obliquity range. <strong>Provided by<\/strong>: NASA, Mysid. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/commons.wikimedia.org\/wiki\/File:Earth_obliquity_range.svg\">https:\/\/commons.wikimedia.org\/wiki\/File:Earth_obliquity_range.svg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Activity Continues On the Sun. <strong>Provided by<\/strong>: NASA. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/en.wikipedia.org\/wiki\/File:Activity_Continues_On_the_Sun.jpg\">https:\/\/en.wikipedia.org\/wiki\/File:Activity_Continues_On_the_Sun.jpg<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><li>Mauna Loa Data Today: Atmospheric Gases. <strong>Provided by<\/strong>: NOAA. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"http:\/\/www.noaanews.noaa.gov\/stories2006\/s2654.htm\">http:\/\/www.noaanews.noaa.gov\/stories2006\/s2654.htm<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/about\/pdm\">Public Domain: No Known Copyright<\/a><\/em><\/li><\/ul><\/div>\n\t\t\t\t\t\t <\/div>\n\t\t\t\t\t <\/div>\n\t\t\t <\/section>","protected":false},"author":17,"menu_order":12,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Dynamic Earth: Introduction to Physical Geography\",\"author\":\"R. Adam Dastrup\",\"organization\":\"\",\"url\":\"http:\/\/www.opengeography.org\/physical-geography.html\",\"project\":\"Open Geography Education\",\"license\":\"cc-by-sa\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"2008 age of oceans plates\",\"author\":\"\",\"organization\":\"NOAA\",\"url\":\"https:\/\/commons.wikimedia.org\/wiki\/File:2008_age_of_oceans_plates.jpg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Eccentricity zero\",\"author\":\"\",\"organization\":\"NASA, Mysid\",\"url\":\"https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_zero.svg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Eccentricity half\",\"author\":\"\",\"organization\":\"NASA, Mysid\",\"url\":\"https:\/\/commons.wikimedia.org\/wiki\/File:Eccentricity_half.svg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Earth precession\",\"author\":\"\",\"organization\":\"NASA, Mysid\",\"url\":\"https:\/\/commons.wikimedia.org\/wiki\/File:Earth_precession.svg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Earth obliquity range\",\"author\":\"\",\"organization\":\"NASA, Mysid\",\"url\":\"https:\/\/commons.wikimedia.org\/wiki\/File:Earth_obliquity_range.svg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Activity Continues On the Sun\",\"author\":\"\",\"organization\":\"NASA\",\"url\":\"https:\/\/en.wikipedia.org\/wiki\/File:Activity_Continues_On_the_Sun.jpg\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"},{\"type\":\"pd\",\"description\":\"Mauna Loa Data Today: Atmospheric Gases\",\"author\":\"\",\"organization\":\"NOAA\",\"url\":\"http:\/\/www.noaanews.noaa.gov\/stories2006\/s2654.htm\",\"project\":\"\",\"license\":\"pd\",\"license_terms\":\"\"}]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-872","chapter","type-chapter","status-publish","hentry"],"part":596,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapters\/872","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/wp\/v2\/users\/17"}],"version-history":[{"count":3,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapters\/872\/revisions"}],"predecessor-version":[{"id":941,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapters\/872\/revisions\/941"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/parts\/596"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapters\/872\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/wp\/v2\/media?parent=872"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/pressbooks\/v2\/chapter-type?post=872"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/wp\/v2\/contributor?post=872"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geophysical\/wp-json\/wp\/v2\/license?post=872"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}