{"id":13100,"date":"2021-09-02T08:00:45","date_gmt":"2021-09-01T22:30:45","guid":{"rendered":"https:\/\/education.australiascience.tv\/?p=13100"},"modified":"2021-10-01T15:32:17","modified_gmt":"2021-10-01T06:02:17","slug":"cosmos-magazine-a-short-history-of-light","status":"publish","type":[8014,8018],"link":"https:\/\/education.australiascience.tv\/cosmos-magazine-a-short-history-of-light\/","title":{"rendered":"A short history of light"},"content":{"rendered":"[vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; angled_section=&#8221;no&#8221; text_align=&#8221;left&#8221; background_image_as_pattern=&#8221;without_pattern&#8221;][vc_column width=&#8221;5\/6&#8243;][vc_separator color=&#8221;white&#8221;][vc_column_text]<strong>Rachel Rayner takes us on a tour of the spectrum beyond the visible and explains why dogs help.<\/strong><\/p>\n<p>Explore the frequencies and wavelengths of the electromagnetic spectrum in a fun way in this resource for Year 5 and 9 Physics students as they learn about waves.<\/p>\n<p>Word Count: approx. 1300[\/vc_column_text][vc_column_text]\n<figure id=\"attachment_13101\" class=\"thumbnail wp-caption alignnone\" style=\"width: 1920px\"><img loading=\"lazy\" class=\"wp-image-13101 size-full\" src=\"https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Header_A-short-history-of-light_1920x1080.png\" alt=\"\" width=\"1920\" height=\"1080\" srcset=\"https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Header_A-short-history-of-light_1920x1080.png 1920w, https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Header_A-short-history-of-light_1920x1080-300x169.png 300w, https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Header_A-short-history-of-light_1920x1080-768x432.png 768w, https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Header_A-short-history-of-light_1920x1080-1024x576.png 1024w\" sizes=\"(max-width: 1920px) 100vw, 1920px\" \/><figcaption class=\"caption wp-caption-text\">Credit: Nafi Nurhadi \/ Getty Images<\/figcaption><\/figure>\n[\/vc_column_text][vc_column_text]<strong>You are radiating. You always have been. <\/strong>[\/vc_column_text][vc_column_text]You are radiating at a frequency of 24,000 GHz. Perhaps, by the end of this article, you will be radiating at a higher frequency as you discover the exciting link between quantum physics and dogs.[\/vc_column_text][vc_column_text]Or you may just have an actual fever \u2013 booked your flu shot yet?[\/vc_column_text][vc_column_text]We all radiate light. But not visible light. The universe has a rainbow that is made up of so many more colours of light than the familiar spectrum of ROYGBIV (red, orange, yellow, green, blue, indigo, violet). When we talk about the light of the universe at its most minute level, the quantum level, we\u2019re talking about light as photons. So, what exactly is a photon? Its name comes from the Greek word for light, \u201cph\u014dto\u201d. A photon is generally described as \u201clight as a packet of energy\u201d.[\/vc_column_text][vc_column_text]A photon is not an envelope or bag for the energy to go into. Rather, it is the light itself, with an inherent, specific energy. A photon is a single energy level of light, and of a single size, which cannot be made smaller. Photons exist in the quantum world. This means they have a dual existence as both a wave and a particle. But like a good poker player\u2019s hand, a photon will only reveal its identity as a wave or as a particle when observed by others. Before then, all we can do is consider it as both. Welcome to the concept of quantum duality.[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]\n<h3>Deeper: <a href=\"https:\/\/education.australiascience.tv\/explainer-is-light-a-wave-or-a-particle\/\" target=\"_blank\" rel=\"noopener noreferrer\">Explainer: Is light a wave or a particle?<\/a><\/h3>\n[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]Physicist Erwin Schr\u00f6dinger used the <a href=\"https:\/\/www.youtube.com\/watch?v=IOYyCHGWJq4\" target=\"_blank\" rel=\"noopener noreferrer\">example<\/a> of his cat to explain quantum duality. The abridged version is that a cat in a box could be alive or dead, but you don\u2019t know until you open the box \u2013 in the interim, it exists in both states. Follow? Perhaps an ANZAC Day two-up analogy works better: the coins are both heads and tails while tossed in the air, and will only truly become tails (or heads) when they land.[\/vc_column_text][vc_column_text]This is quantum duality.[\/vc_column_text][vc_column_text]There are numerous ways to measure photons. The more energetic photons usually have their wavelengths measured in Angstroms \u2013 which is the radius of a chlorine, sulphur or phosphorus atom, measured from the centre of the atom to its covalent electron. However, two units of measure that are used more broadly are hertz and metres. Both of these units are used for any wave \u2013 we tune our radios in hertz, for example, so the station 105.7FM is at 105.7 megahertz. (In fact, radio waves are a type of light \u2013 they\u2019re photons, too!)[\/vc_column_text][vc_column_text]\n<blockquote><p><strong><span style=\"color: #39b54a;\">A photon goes to a hotel and the doorman says, \u201cCan I take your bags?\u201d<\/span><\/strong><\/p>\n<p><strong><span style=\"color: #783b99;\">The photon replies, \u201cNo need, I\u2019m travelling light!\u201d<\/span><\/strong><\/p><\/blockquote>\n[\/vc_column_text][vc_column_text]Hertz, as a unit of measure, tells us how many times a wave cycles in a second, which for many of us is hard to imagine. Using metres to distinguish different photons from one another is a more easily understood yardstick.[\/vc_column_text][vc_column_text]Photon wavelengths range from extremely small, at a trillionth of a metre, to huge, at tens of metres. This range encapsulates nearly everything that we experience, like feeling warm, receiving a phone call, microwaving left-overs, and just optically understanding the world. It\u2019s the full spectrum.[\/vc_column_text][vc_column_text]Sections of this spectrum have names familiar to most of us. The full range of photons, listed across the bottom,\u00a0in order from highest energy to lowest energy, goes from gamma rays to X-rays to ultraviolet light to visible light (which is our visible rainbow of ROYGBIV) to infrared light to microwaves to radio waves.[\/vc_column_text][vc_column_text]Despite their huge variations in energy levels, all these wavelengths travel at the same speed \u2013 the speed of light. Which makes a photon the fastest thing in the universe (in a vacuum \u2013 there\u2019s always a caveat). Light travels at 3&#215;10<sup>8<\/sup> m\/s, which is 900,000 times faster than the speed of sound (through air, at sea level; you\u2019ve got to be specific about these things).[\/vc_column_text][vc_column_text]If you were travelling at the speed of light, you would be able to zip around the Earth\u2019s equator in 0.13 seconds; in a Boeing 747, it would take 45 hours (or 162,000 seconds).[\/vc_column_text][vc_column_text]In our classical world of Newtonian physics, where F = ma, more energy generally means more speed. But not here! We\u2019re in the quantum world now, and things are very different.[\/vc_column_text][vc_column_text css=&#8221;.vc_custom_1629092820945{border-top-width: 5px !important;border-right-width: 5px !important;border-bottom-width: 5px !important;border-left-width: 5px !important;padding-top: 15px !important;padding-right: 15px !important;padding-bottom: 15px !important;padding-left: 15px !important;background-color: #783b99 !important;border-left-color: #783b99 !important;border-right-color: #783b99 !important;border-top-color: #783b99 !important;border-bottom-color: #783b99 !important;}&#8221;]<span style=\"color: #ffffff;\"><strong>A quantum leap<\/strong><\/span><br \/>\n<span style=\"color: #ffffff;\">In the everyday world, you know what something is, where it has been and where it is going. Think of a tennis ball on the ground: you know that if you pick it up and let it go, it will fall to the ground and bounce back. In the quantum world, you have only probabilities: the probability that something will be here or there; the probability of whether it is a wave or particle, or whether it exists at all. If you let the tennis ball go, there is a probability that it will hit the ground or fly away; that it isn\u2019t a tennis ball at all but the path of its movement, or that it just isn\u2019t there. And neither are you.<\/span>[\/vc_column_text][vc_column_text]We\u2019ve used cats to help explain things, but did we mention something about letting the dogs out? Here goes &#8230;[\/vc_column_text][vc_column_text]All light (all photons) travels at the same speed, despite different wavelengths and energy levels. If we were to represent each category of photon as a different breed of dog, we can begin to image how different wavelengths can have different energies, but nevertheless travel at the same speed.[\/vc_column_text][vc_column_text]Let\u2019s first take the highest energy photon with the smallest wavelength, gamma rays.[\/vc_column_text][vc_column_text]These are the Chihuahuas of this light-filled world. To get anywhere quickly, their little legs (short wavelengths) are churning away at a great rate in order to keep up with their larger friends. They are going to need so much more energy to travel any distance at all.[\/vc_column_text][vc_column_text]At the other end of the spectrum are the radio wave photons. With their long wavelengths and low energies, these are the Great Danes. With a few lazy, languid strides, they can get anywhere just as quickly as the Chihuahua, while expending much less energy in the process.[\/vc_column_text][vc_column_text css=&#8221;.vc_custom_1629180726321{border-top-width: 5px !important;border-right-width: 5px !important;border-bottom-width: 5px !important;border-left-width: 5px !important;padding-top: 10px !important;padding-right: 10px !important;padding-bottom: 10px !important;padding-left: 10px !important;background-color: #e8e8e8 !important;border-left-color: #e8e8e8 !important;border-right-color: #e8e8e8 !important;border-top-color: #e8e8e8 !important;border-bottom-color: #e8e8e8 !important;border-radius: 5px !important;}&#8221;]<strong><img loading=\"lazy\" class=\"alignnone wp-image-13120 size-full\" src=\"https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Graphic_EM-Spectrum_no-border_640x342.png\" alt=\"\" width=\"640\" height=\"342\" srcset=\"https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Graphic_EM-Spectrum_no-border_640x342.png 640w, https:\/\/education.australiascience.tv\/wp-content\/uploads\/2021\/08\/Graphic_EM-Spectrum_no-border_640x342-300x160.png 300w\" sizes=\"(max-width: 640px) 100vw, 640px\" \/><\/strong><\/p>\n<p><strong>EM wave v EM Wavelength<\/strong><br \/>\nLight is an electromagnetic wave: it is a ripple through both the electric field and the magnetic field simultaneously. These two fields exist perpendicular to each other, so a wave through them is represented as two sine waves at right angles to each other.<br \/>\nThe wavelength is measured from the peak of one wave to the peak of the next, or the trough of one to the trough of the next. This is different to amplitude, which is the height of the wave from trough to peak.[\/vc_column_text][vc_column_text]We\u2019ve extended this analogy to the entire spectrum (below) where each photon gets its own canine representative.[\/vc_column_text][vc_column_text]Despite their different leg lengths, all these dogs are still going to reach the other side of the park at the same time (they all travel at the same speed, after all). Some just require more energy to do so than others \u2013 those smaller dogs will be moving their legs a lot more to keep up with the larger ones.[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]\n<h3>Also: <a href=\"https:\/\/education.australiascience.tv\/explainer-the-electromagnetic-spectrum\/\" target=\"_blank\" rel=\"noopener noreferrer\">Explainer: The Electromagnetic Spectrum<\/a><\/h3>\n[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]It\u2019s important to paws (couldn\u2019t help myself) here, and appreciate that this is not to scale. The Chihuahua photon has 300 billion times more energy than visible light\u2019s border collie. That is a lot of tiny leg movements! But this is an analogy, remember. It may have gone to the dogs. But it\u2019s much cuter than Schr\u00f6dinger\u2019s Cat; this is Photon\u2019s Hounds. And, unlike that poor old cat, they get to live 100% of the time.[\/vc_column_text][vc_column_text]So, what are we humans radiating? Why, we are beautifully radiating infrared photons, which makes us all lovely (and loyal) golden retrievers.[\/vc_column_text][vc_column_text]Infrared photons are what we sense as our body heat. Infrared light is a colour of light that you can actually feel.[\/vc_column_text][vc_column_text]It sounds outrageous, but it\u2019s true.[\/vc_column_text][vc_column_text]How\u2019s your temperature now?[\/vc_column_text][vc_images_carousel images=&#8221;13113,13114,13115,13116,13117,13118,13119&#8243; img_size=&#8221;full&#8221; slides_per_view=&#8221;3&#8243; autoplay=&#8221;yes&#8221; wrap=&#8221;yes&#8221;][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]<strong>This article was written by <a href=\"https:\/\/www.instagram.com\/raynerexplainer\/\" target=\"_blank\" rel=\"noopener noreferrer\">Rachel Rayner<\/a>, science communicator, poet and performer, for <a href=\"https:\/\/cosmosmagazine.com\/\"><em>Cosmos<\/em> Magazine<\/a> Issue 92. <\/strong><\/p>\n<p><em>Cosmos<\/em> magazine is Australia\u2019s only dedicated print science publication. <a href=\"https:\/\/cosmosmagazine.com\/shop\/\" target=\"_blank\" rel=\"noopener noreferrer\">Subscribe here<\/a> to get your quarterly fill of the best Science of Everything, from the chemistry of fireworks to cutting-edge Australian innovation.[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text njt-role=&#8221;not-logged-in&#8221; css=&#8221;.vc_custom_1605576692266{margin-bottom: 0px !important;border-bottom-width: 0px !important;padding-bottom: 0px !important;}&#8221;]\n<p style=\"text-align: center;\">Login or Sign up for <strong>FREE<\/strong> to download the educational resources<\/p>\n[\/vc_column_text][vc_column_text njt-role=&#8221;not-logged-in&#8221;]\n<div id=\"um-admin-form-shortcode\" class=\"postbox \" style=\"text-align: center;\">\n<div class=\"inside\">\n<div class=\"um-admin-metabox\">\n<noscript class=\"ninja-forms-noscript-message\">\n    Notice: JavaScript is required for this content.<\/noscript><style>\n\n        \/* FIELDS STYLES *\/\n    \n        .nf-form-content .nf-field-container 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'' : '' }}} {{{ part.title }}}<\/a>\n\t\t<\/li>\n\t\t<# } ); #>\n\t<\/ul>\n<\/script>\n\n<script id=\"tmpl-nf-mp-progress-bar\" type=\"text\/template\">\n    <div class=\"nf-progress-container\">\n        <div class=\"nf-progress\" style=\"width: {{{ data.percent }}}%;\"><\/div>\n    <\/div>\n<\/script>        <script id=\"nf-tmpl-cell\" type=\"text\/template\">\n            <nf-fields><\/nf-fields>\n        <\/script>\n\n        <script id=\"nf-tmpl-row\" type=\"text\/template\">\n            <nf-cells><\/nf-cells>\n        <\/script>\n\n        \n<\/div>\n<\/div>\n<\/div>\n[\/vc_column_text][vc_row_inner][vc_column_inner width=&#8221;1\/3&#8243;][vc_btn title=&#8221;Download Teachers&#8217; Resource&#8221; color=&#8221;info&#8221; size=&#8221;lg&#8221; njt-role=&#8221;logged-in&#8221; link=&#8221;url:https%3A%2F%2Feducation.australiascience.tv%2Fwp-content%2Fuploads%2F2021%2F08%2FA-short-history-of-light_Teacher-resource.pdf||target:%20_blank|&#8221;][\/vc_column_inner][vc_column_inner width=&#8221;1\/3&#8243;][vc_btn title=&#8221;Download the Article for Students&#8221; color=&#8221;danger&#8221; size=&#8221;lg&#8221; align=&#8221;left&#8221; njt-role=&#8221;logged-in&#8221; link=&#8221;url:https%3A%2F%2Feducation.australiascience.tv%2Fwp-content%2Fuploads%2F2021%2F08%2FA-History-of-Light_Article.pdf||target:%20_blank|&#8221;][\/vc_column_inner][vc_column_inner width=&#8221;1\/3&#8243;][vc_btn title=&#8221;Download Student Activity&#8221; color=&#8221;warning&#8221; size=&#8221;lg&#8221; align=&#8221;left&#8221; njt-role=&#8221;logged-in&#8221; link=&#8221;url:https%3A%2F%2Feducation.australiascience.tv%2Fwp-content%2Fuploads%2F2021%2F08%2FStudent-Activity_A-short-history-of-light.pdf||target:%20_blank|&#8221;][\/vc_column_inner][\/vc_row_inner][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]\n<h3>Years: 5, 9<\/h3>\n[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]\n<h3>Topics:<\/h3>\n<h3><span style=\"color: #2d3791;\">Physical Sciences: Energy<\/span><\/h3>\n<h3>Additional: Careers, Maths, Technology, Engineering.<\/h3>\n[\/vc_column_text][vc_column_text]\n<h3>Concepts (South Australia):<\/h3>\n<h3><span style=\"color: #2d3791;\">Physical Sciences: Energy<\/span><\/h3>\n[\/vc_column_text][vc_separator color=&#8221;#000000&#8243; type=&#8221;normal&#8221;][vc_column_text]\n<h3>More resources:<\/h3>\n<h3><a href=\"https:\/\/education.australiascience.tv\/cosmos-magazine-resources\/\" target=\"_blank\" rel=\"noopener noreferrer\">Cosmos Magazine &#8211; browse resources<\/a><\/h3>\n<h3><a href=\"https:\/\/education.australiascience.tv\/shining-a-light-on-the-hidden-universe\/\" target=\"_blank\" rel=\"noopener noreferrer\">Shining a Light on the Hidden Universe<\/a><\/h3>\n<h3><a href=\"https:\/\/education.australiascience.tv\/cosmos-magazine-refracted-glory\/\" target=\"_blank\" rel=\"noopener noreferrer\">Refracted Glory<\/a><\/h3>\n[\/vc_column_text][\/vc_column][\/vc_row]\n","protected":false},"excerpt":{"rendered":"<p>[vc_row row_type=&#8221;row&#8221; use_row_as_full_screen_section=&#8221;no&#8221; type=&#8221;full_width&#8221; angled_section=&#8221;no&#8221; text_align=&#8221;left&#8221; background_image_as_pattern=&#8221;without_pattern&#8221;][vc_column width=&#8221;5\/6&#8243;][vc_separator color=&#8221;white&#8221;][vc_column_text]Rachel Rayner takes us on a tour of the spectrum beyond the visible and explains why dogs help. Explore the frequencies and wavelengths of the electromagnetic spectrum in a fun way in &hellip; <a href=\"https:\/\/education.australiascience.tv\/cosmos-magazine-a-short-history-of-light\/\">Continued<\/a><\/p>\n","protected":false},"author":2922,"featured_media":13102,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"kt_blocks_editor_width":""},"categories":[4,8],"tags":[218,43,97,65,37,59,959,907,3851,6014,2384,595,328,5958,5025,3786,1985,3405,3406,231,6035,958,2866,119,213,2135,7763,1913,6513,5023,2899,1845,5590,5035,6030,3950,7690,5027,816,825],"year":[8007,8011],"subject":[8026,8027],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v17.7.1 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>A short history of light - Education - RiAus<\/title>\n<meta name=\"description\" content=\"Rachel Rayner takes us on a tour of the light spectrum beyond the visible and explains why dogs help in this resource for Year 5 and 9 Physics students.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/education.australiascience.tv\/cosmos-magazine-a-short-history-of-light\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"A short history of light - 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