{"id":10725,"date":"2023-12-12T10:00:00","date_gmt":"2023-12-12T10:00:00","guid":{"rendered":"https:\/\/modernsciences.org\/staging\/4414\/?p=10725"},"modified":"2023-12-01T06:34:08","modified_gmt":"2023-12-01T06:34:08","slug":"earths-magnetic-field-protects-life-on-earth-from-radiation-but-it-can-move-and-the-magnetic-poles-can-even-flip","status":"publish","type":"post","link":"https:\/\/modernsciences.org\/staging\/4414\/earths-magnetic-field-protects-life-on-earth-from-radiation-but-it-can-move-and-the-magnetic-poles-can-even-flip\/","title":{"rendered":"Earth\u2019s magnetic field protects life on Earth from radiation, but it can move, and the magnetic poles can even\u00a0flip"},"content":{"rendered":"\n  <figure>\n    <img  decoding=\"async\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/559181\/original\/file-20231113-23-84pk4b.jpg?ixlib=rb-1.1.0&#038;rect=0%2C0%2C5167%2C3387&#038;q=45&#038;auto=format&#038;w=754&#038;fit=clip\" >\n      <figcaption>\n        The Earth\u2019s magnetic field deflects particles emitted by the Sun.\n        <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/www.gettyimages.com\/detail\/illustration\/earths-magnetosphere-illustration-royalty-free-illustration\/1316974949?phrase=earth+magnetosphere&#038;adppopup=true\" target=\"_blank\" rel=\"noopener\">Mark Garlick\/Science Photo Library via Getty Images<\/a><\/span>\n      <\/figcaption>\n  <\/figure>\n\n<span><a href=\"https:\/\/theconversation.com\/profiles\/ofer-cohen-1482327\" target=\"_blank\" rel=\"noopener\">Ofer Cohen<\/a>, <em><a href=\"https:\/\/theconversation.com\/institutions\/umass-lowell-1534\" target=\"_blank\" rel=\"noopener\">UMass Lowell<\/a><\/em><\/span>\n\n<p>The Earth\u2019s magnetic field plays a big role in protecting people from hazardous radiation and geomagnetic activity that could affect satellite communication and the operation of power grids. And it moves. <\/p>\n\n<p>Scientists have studied and tracked the motion of the magnetic poles <a href=\"https:\/\/www.ncei.noaa.gov\/products\/wandering-geomagnetic-poles\" target=\"_blank\" rel=\"noopener\">for centuries<\/a>. The historical movement of these poles indicates a <a href=\"https:\/\/theconversation.com\/old-stone-walls-record-the-changing-location-of-magnetic-north-112827\" target=\"_blank\" rel=\"noopener\">change in the global geometry<\/a> of the Earth\u2019s magnetic field. It may even indicate the beginning of a field reversal \u2013 a \u201cflip\u201d between the north and south magnetic poles. <\/p>\n\n<p><a href=\"https:\/\/www.uml.edu\/research\/locsst\/about\/faculty-staff\/cohen-ofer.aspx\" target=\"_blank\" rel=\"noopener\">I\u2019m a physicist<\/a> who studies the interaction between the planets and space. While the north magnetic pole moving a little bit isn\u2019t a big deal, a reversal could have a big impact on Earth\u2019s climate and our modern technology. But these reversals don\u2019t happen instantaneously. Instead, they occur <a href=\"https:\/\/theconversation.com\/does-an-anomaly-in-the-earths-magnetic-field-portend-a-coming-pole-reversal-47528\" target=\"_blank\" rel=\"noopener\">over thousands of years<\/a>. <\/p>\n\n<figure class=\"align-center zoomable\">\n            <a href=\"https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\" target=\"_blank\" rel=\"noopener\"><img  decoding=\"async\"  alt=\"A map showing the north part of Canada, with yellow dots moving southwards.\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-ls-sizes=\"(min-width: 1466px) 754px, (max-width: 599px) 100vw, (min-width: 600px) 600px, 237px\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"  data-pk-srcset=\"https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=600&amp;h=316&amp;fit=crop&amp;dpr=1 600w, https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=600&amp;h=316&amp;fit=crop&amp;dpr=2 1200w, https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=600&amp;h=316&amp;fit=crop&amp;dpr=3 1800w, https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;h=397&amp;fit=crop&amp;dpr=1 754w, https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=754&amp;h=397&amp;fit=crop&amp;dpr=2 1508w, https:\/\/images.theconversation.com\/files\/557124\/original\/file-20231101-17-7nf5ns.png?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=754&amp;h=397&amp;fit=crop&amp;dpr=3 2262w\" ><\/a>\n            <figcaption>\n              <span class=\"caption\">The north magnetic pole\u2019s observed locations from 1831\u20132007 are yellow squares. Modeled pole locations from 1590\u20132025 are circles progressing from blue to yellow.<\/span>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/www.ncei.noaa.gov\/products\/wandering-geomagnetic-poles\" target=\"_blank\" rel=\"noopener\">National Centers for Environmental Information<\/a><\/span>\n            <\/figcaption>\n          <\/figure>\n\n<h2 id=\"magnetic-field-generation\">Magnetic field generation<\/h2>\n\n<p>So how are magnetic fields like the one around Earth generated?<\/p>\n\n<p>Magnetic fields are generated by <a href=\"https:\/\/www.youtube.com\/watch?v=PgM8zWJr8-U\" target=\"_blank\" rel=\"noopener\">moving electric charges<\/a>. A material that enables charges to easily move in it is <a href=\"https:\/\/en.wikipedia.org\/wiki\/Electrical_conductor\" target=\"_blank\" rel=\"noopener\">called a conductor<\/a>. Metal is one example of a conductor \u2013 people use it to transfer electric currents from one place to the other. The electric current itself is simply negative charges called electrons moving through the metal. This current <a href=\"https:\/\/www.youtube.com\/watch?v=XoVW7CRR5JY\" target=\"_blank\" rel=\"noopener\">generates a magnetic field<\/a>.  <\/p>\n\n<p>Layers of conducting material can be found in the <a href=\"https:\/\/www.youtube.com\/watch?v=4WILyDlmln8\" target=\"_blank\" rel=\"noopener\">Earth\u2019s liquid iron core<\/a>. Currents of charges move throughout the core, and the liquid iron is also moving and circulating in the core. These movements generate the magnetic field. <\/p>\n\n<figure>\n            <iframe loading=\"lazy\" width=\"440\" height=\"260\" src=\"https:\/\/www.youtube.com\/embed\/MtLC8evycaE?wmode=transparent&amp;start=0\" frameborder=\"0\" allowfullscreen=\"\"><\/iframe>\n            <figcaption><span class=\"caption\">Earth\u2019s magnetic field is generated by what\u2019s called a \u201cdynamo effect.\u201d<\/span><\/figcaption>\n          <\/figure>\n\n<p>Earth isn\u2019t the only planet with a magnetic field \u2013 gas giant planets like Jupiter have a <a href=\"https:\/\/doi.org\/10.1038\/s41586-018-0468-5\" target=\"_blank\" rel=\"noopener\">conducting metallic hydrogen layer<\/a> that generates their magnetic fields. <\/p>\n\n<p>The <a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6404\/ab8780\/pdf\" target=\"_blank\" rel=\"noopener\">movement of these conducting layers<\/a> inside planets results in two types of fields. Larger motions, such as large-scale rotations with the planet, lead to a symmetric magnetic field with a north and a south pole \u2013 similar to a toy magnet. <\/p>\n\n<p>These conducting layers may have some local irregular motions due to <a href=\"https:\/\/www.youtube.com\/watch?v=bw_WC-EVs_g\" target=\"_blank\" rel=\"noopener\">local turbulence<\/a> or smaller flows that do not follow the large-scale pattern. These irregularities will manifest in some small anomalies in the planet\u2019s magnetic field or places where the field deviates from being a perfect dipole field. <\/p>\n\n<p>These small-scale deviations in the magnetic field can actually <a href=\"https:\/\/www.youtube.com\/watch?v=I3zFeV24or8\" target=\"_blank\" rel=\"noopener\">lead to changes<\/a> in the large-scale field over time and potentially even a complete reversal of the polarity of the dipole field, where the north becomes south and vice versa. The designations of \u201cnorth\u201d and \u201csouth\u201d on the magnetic field refer to their opposite polarities \u2013 they\u2019re not related to geographic north and south. <\/p>\n\n<figure class=\"align-center zoomable\">\n            <a href=\"https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\" target=\"_blank\" rel=\"noopener\"><img  decoding=\"async\"  alt=\"A diagram showing the Earth, with two blocks on the inside, one pointing upward that says S and one pointing downward that says N, labeled South Magnetic pole and North magnetic pole, respectively. A slightly tilted line depicts the Earth&#039;s rotation axis.\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-ls-sizes=\"(min-width: 1466px) 754px, (max-width: 599px) 100vw, (min-width: 600px) 600px, 237px\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"  data-pk-srcset=\"https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=600&amp;h=600&amp;fit=crop&amp;dpr=1 600w, https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=600&amp;h=600&amp;fit=crop&amp;dpr=2 1200w, https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=600&amp;h=600&amp;fit=crop&amp;dpr=3 1800w, https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;h=754&amp;fit=crop&amp;dpr=1 754w, https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=754&amp;h=754&amp;fit=crop&amp;dpr=2 1508w, https:\/\/images.theconversation.com\/files\/559180\/original\/file-20231113-26-sdwidj.jpg?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=754&amp;h=754&amp;fit=crop&amp;dpr=3 2262w\" ><\/a>\n            <figcaption>\n              <span class=\"caption\">Earth\u2019s magnetic field. The north and south magnetic poles mirror the geographic North and South poles.<\/span>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/www.gettyimages.com\/detail\/illustration\/geomagnetic-field-planet-earth-royalty-free-illustration\/470258936?phrase=earth+magnetosphere&amp;adppopup=true\" target=\"_blank\" rel=\"noopener\">PeterHermesFurian\/iStock via Getty Images Plus<\/a><\/span>\n            <\/figcaption>\n          <\/figure>\n\n<h2 id=\"the-earths-magnetosphere-a-protective-bubble\">The Earth\u2019s magnetosphere, a protective bubble<\/h2>\n\n<p>The Earth\u2019s magnetic field creates a magnetic \u201cbubble\u201d called the <a href=\"https:\/\/science.nasa.gov\/heliophysics\/focus-areas\/magnetosphere-ionosphere\" target=\"_blank\" rel=\"noopener\">magnetosphere<\/a> above the uppermost part of the atmosphere, <a href=\"https:\/\/en.wikipedia.org\/wiki\/Ionosphere\" target=\"_blank\" rel=\"noopener\">the ionosphere layer<\/a>.<\/p>\n\n<p>The magnetosphere plays a major role in protecting people. It shields and deflects damaging, high-energy, <a href=\"https:\/\/www.youtube.com\/watch?v=KbZbfJjiil4\" target=\"_blank\" rel=\"noopener\">cosmic-ray radiation<\/a>, which is created in star explosions and moves constantly through the universe. The magnetosphere also interacts with <a href=\"https:\/\/en.wikipedia.org\/wiki\/Solar_wind\" target=\"_blank\" rel=\"noopener\">solar wind<\/a>, which is a flow of magnetized gas sent out from the Sun.<\/p>\n\n<p>The magnetosphere and ionosphere\u2019s interaction with magnetized solar wind creates what scientists call <a href=\"https:\/\/spaceplace.nasa.gov\/spaceweather\/en\/\" target=\"_blank\" rel=\"noopener\">space weather<\/a>. Usually, the solar wind is mild and there\u2019s little to no space weather. <\/p>\n\n<p>However, there are times when the Sun sheds large magnetized clouds of gas called <a href=\"https:\/\/nso.edu\/for-public\/sun-science\/coronal-mass-ejections-cme\/\" target=\"_blank\" rel=\"noopener\">coronal mass ejections<\/a> into space. If these coronal mass ejections make it to Earth, their interaction with the magnetosphere can generate <a href=\"https:\/\/www.swpc.noaa.gov\/phenomena\/geomagnetic-storms\" target=\"_blank\" rel=\"noopener\">geomagnetic storms<\/a>. Geomagnetic storms <a href=\"https:\/\/www.swpc.noaa.gov\/phenomena\/aurora\" target=\"_blank\" rel=\"noopener\">can create auroras<\/a>, which happen when a stream of energized particles hits the atmosphere and lights up. <\/p>\n\n<p>During space weather events, there\u2019s <a href=\"https:\/\/theconversation.com\/solar-storms-can-destroy-satellites-with-ease-a-space-weather-expert-explains-the-science-177510\" target=\"_blank\" rel=\"noopener\">more hazardous radiation<\/a> near the Earth. This radiation can <a href=\"https:\/\/www.youtube.com\/watch?v=MEd2pvyRpfw\" target=\"_blank\" rel=\"noopener\">potentially harm satellites<\/a> and astronauts. Space weather can also damage large conducting systems, such as major pipelines and power grids, by overloading <a href=\"https:\/\/www.swpc.noaa.gov\/impacts\/electric-power-transmission\" target=\"_blank\" rel=\"noopener\">currents in these systems<\/a>. <\/p>\n\n<figure>\n            <iframe loading=\"lazy\" width=\"440\" height=\"260\" src=\"https:\/\/www.youtube.com\/embed\/URN-XyZD2vQ?wmode=transparent&amp;start=0\" frameborder=\"0\" allowfullscreen=\"\"><\/iframe>\n            <figcaption><span class=\"caption\">Earth\u2019s magnetosphere protects life on Earth from ejections from the Sun.<\/span><\/figcaption>\n          <\/figure>\n\n<p>Space weather events can also disrupt satellite communication and <a href=\"https:\/\/www.swpc.noaa.gov\/impacts\/space-weather-and-gps-systems\" target=\"_blank\" rel=\"noopener\">GPS operation<\/a>, which many people rely on. <\/p>\n\n<h2 id=\"field-flips\">Field flips<\/h2>\n\n<p>Scientists map and track the overall <a href=\"https:\/\/www.ncei.noaa.gov\" target=\"_blank\" rel=\"noopener\">shape and orientation<\/a> of the Earth\u2019s magnetic field using local measurements of the field\u2019s orientation and magnitude and, <a href=\"http:\/\/doi.org\/10.1098\/rsta.2000.0569\" target=\"_blank\" rel=\"noopener\">more recently, models<\/a>. <\/p>\n\n<p>The location of the north magnetic pole <a href=\"https:\/\/royalsocietypublishing.org\/doi\/10.1098\/rsta.2000.0569\" target=\"_blank\" rel=\"noopener\">has moved<\/a> by about 600 miles (965 kilometers) since the first measurement was taken in 1831. The migration speed has increased from 10 miles per year to 34 miles per year (16 km to 54 km) in more recent years. This acceleration could indicate the beginning of a field reversal, but scientists really can\u2019t tell with less than 200 years of data.<\/p>\n\n<p>The Earth\u2019s magnetic field reverses on time scales that vary between <a href=\"https:\/\/pubs.usgs.gov\/of\/2003\/of03-187\/of03-187.pdf\" target=\"_blank\" rel=\"noopener\">100,000 to 1,000,000 years<\/a>. Scientists can tell how often the magnetic field reverses by <a href=\"https:\/\/eos.org\/research-spotlights\/steadying-mid-ocean-ridge-spreading-rates\" target=\"_blank\" rel=\"noopener\">looking at volcanic rocks<\/a> in the ocean. <\/p>\n\n<p>These rocks <a href=\"https:\/\/www.youtube.com\/watch?v=4WILyDlmln8\" target=\"_blank\" rel=\"noopener\">capture the orientation and strength<\/a> of the Earth\u2019s magnetic field when they are created, so dating these rocks provides a good picture of how the Earth\u2019s field has <a href=\"https:\/\/eos.org\/research-spotlights\/steadying-mid-ocean-ridge-spreading-rates\" target=\"_blank\" rel=\"noopener\">evolved over time<\/a>.<\/p>\n\n<p>Field reversals happen fast from a geologic standpoint, though slow from a human perspective. A reversal usually takes a few thousand years, but during this time the magnetosphere\u2019s orientation may shift and <a href=\"https:\/\/agupubs.onlinelibrary.wiley.com\/doi\/full\/10.1029\/2010JA016036\" target=\"_blank\" rel=\"noopener\">expose more of the Earth<\/a> to cosmic radiation. These events may <a href=\"https:\/\/doi.org\/10.1126\/science.abb8677\" target=\"_blank\" rel=\"noopener\">change the concentration of ozone<\/a> in the atmosphere. <\/p>\n\n<p>Scientists can\u2019t tell with confidence when the next field reversal will happen, but we can keep mapping and tracking the movement of Earth\u2019s magnetic north.<!-- Below is The Conversation's page counter tag. Please DO NOT REMOVE. --><img  loading=\"lazy\"  decoding=\"async\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  alt=\"The Conversation\"  width=\"1\"  height=\"1\"  style=\"border: none !important; box-shadow: none !important; margin: 0 !important; max-height: 1px !important; max-width: 1px !important; min-height: 1px !important; min-width: 1px !important; opacity: 0 !important; outline: none !important; padding: 0 !important\"  referrerpolicy=\"no-referrer-when-downgrade\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-pk-src=\"https:\/\/counter.theconversation.com\/content\/216231\/count.gif?distributor=republish-lightbox-basic\" ><!-- End of code. If you don't see any code above, please get new code from the Advanced tab after you click the republish button. The page counter does not collect any personal data. More info: https:\/\/theconversation.com\/republishing-guidelines --><\/p>\n\n<p><span><a href=\"https:\/\/theconversation.com\/profiles\/ofer-cohen-1482327\" target=\"_blank\" rel=\"noopener\">Ofer Cohen<\/a>, Associate Professor of Physics and Applied Physics, <em><a href=\"https:\/\/theconversation.com\/institutions\/umass-lowell-1534\" target=\"_blank\" rel=\"noopener\">UMass Lowell<\/a><\/em><\/span><\/p>\n\n<p>This article is republished from <a href=\"https:\/\/theconversation.com\" target=\"_blank\" rel=\"noopener\">The Conversation<\/a> under a Creative Commons license. Read the <a href=\"https:\/\/theconversation.com\/earths-magnetic-field-protects-life-on-earth-from-radiation-but-it-can-move-and-the-magnetic-poles-can-even-flip-216231\" target=\"_blank\" rel=\"noopener\">original article<\/a>.<\/p>\n\n","protected":false},"excerpt":{"rendered":"The Earth\u2019s magnetic field deflects particles emitted by the Sun. Mark Garlick\/Science Photo Library via Getty Images Ofer&hellip;\n","protected":false},"author":678,"featured_media":10703,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"nf_dc_page":"","fifu_image_url":"","fifu_image_alt":"","footnotes":""},"categories":[13],"tags":[828,661,474],"class_list":{"0":"post-10725","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-earth","8":"tag-earth","9":"tag-magnetic-field","10":"tag-the-conversation","11":"cs-entry","12":"cs-video-wrap"},"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/10725","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/users\/678"}],"replies":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/comments?post=10725"}],"version-history":[{"count":1,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/10725\/revisions"}],"predecessor-version":[{"id":10726,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/10725\/revisions\/10726"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/media\/10703"}],"wp:attachment":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/media?parent=10725"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/categories?post=10725"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/tags?post=10725"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}