{"id":128247,"date":"2017-08-14T09:15:03","date_gmt":"2017-08-14T13:15:03","guid":{"rendered":"https:\/\/today.uconn.edu\/?p=128247"},"modified":"2017-08-22T11:42:21","modified_gmt":"2017-08-22T15:42:21","slug":"total-eclipse-heart-america","status":"publish","type":"post","link":"https:\/\/today.uconn.edu\/2017\/08\/total-eclipse-heart-america\/","title":{"rendered":"A Total Eclipse of the Heart (of America)"},"content":{"rendered":"<p>A spectacular and likely unforgettable show will take place in the sky Aug. 21.<\/p>\n<p>\u201cHave you ever seen a total solar eclipse?\u201d asks Cynthia Peterson, professor emerita of physics. \u201cIt\u2019s a really, really exciting event!\u201d<\/p>\n<p>The reason\u00a0she and so many others are excited for this event has a lot to do with its rarity. The last time a total solar eclipse was visible from the mainland United States was 38 years ago, in February 1979.<\/p>\n<p>Very specific conditions have to be met to create an eclipse that can be viewed from Earth. The Earth and the moon must align perfectly with the sun as they speed through space, an amazing coincidence. To fully understand how this happens, Peterson says, it\u2019s helpful to know some basic astronomy.<\/p>\n<p><strong>Conditions for a Total Solar Eclipse<\/strong><\/p>\n<figure id=\"attachment_128392\" aria-describedby=\"caption-attachment-128392\" style=\"width: 550px\" class=\"wp-caption alignright\"><a href=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined.jpg\"><img decoding=\"async\" class=\"wp-image-128392 img-responsive lazyload\" data-src=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined-1024x768.jpg\" alt=\"A total solar eclipse is only visible from Earth when the moon is new and at a node, meaning the sun and Earth are aligned with the moon in the middle. If the moon is above or below node, no shadow will be cast on Earth and no eclipse will be seen from Earth. (Yesenia Carrero\/UConn Image)\" width=\"550\" height=\"413\" data-srcset=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined-1024x768.jpg 1024w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined-300x225.jpg 300w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined-768x576.jpg 768w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined-560x420.jpg 560w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/eclipse-image-refined.jpg 2000w\" data-sizes=\"(max-width: 550px) 100vw, 550px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 550px; --smush-placeholder-aspect-ratio: 550\/413;\" \/><\/a><figcaption id=\"caption-attachment-128392\" class=\"wp-caption-text\">A total solar eclipse is only visible from Earth when the moon is new and at a node, meaning the sun and Earth are aligned with the moon in the middle. If the moon is above or below node, no shadow will be cast on Earth and no eclipse will be seen from Earth. (Yesenia Carrero\/UConn Image)<\/figcaption><\/figure>\n<p>The Earth moves in space around the sun, completing a full orbit once every 365.25 days, she explains. As the Earth and other members of our solar system travel around the sun, they continue\u00a0in essentially the same plane, on a path called the <a href=\"https:\/\/astrobob.areavoices.com\/2011\/11\/12\/meet-the-ecliptic-one-of-astronomys-scariest-concepts\/\">ecliptic<\/a>. Some celestial bodies, such as our moon, deviate from the ecliptic slightly.<\/p>\n<p>The orbit of the moon is inclined on the ecliptic plane at an inclination of 5 degrees. As the moon deviates 5 degrees above or below the ecliptic plane, it will cross the plane at points called nodes.<\/p>\n<p>&#8220;That is the first essential piece of the eclipse puzzle,&#8221; says Peterson. \u201cThe moon must be at a node for an eclipse to occur. Otherwise, the moon will not align and no eclipse will be seen from Earth.&#8221;<\/p>\n<p>The moon\u2019s position in the lunar cycle is another vital eclipse component. As the Earth travels in its orbit, the moon tags along, keeping its gaze locked on Earth, always facing from the same side as it completes its own orbit around Earth once every 29.5 days. Over the course of a month, the moon\u2019s appearance changes, from crescent to full to crescent again and finally to what appears to be its absence, when it\u2019s called a new moon. A new moon is the other requirement for a solar eclipse.<\/p>\n<p>\u201cThe basic rule for a solar eclipse is to have a new moon at a node,\u201d Peterson points out.<\/p>\n<figure id=\"attachment_128400\" aria-describedby=\"caption-attachment-128400\" style=\"width: 2000px\" class=\"wp-caption alignleft\"><a href=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal.jpg\"><img decoding=\"async\" class=\"wp-image-128400 size-full img-responsive lazyload\" data-src=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal.jpg\" alt=\"The lunar cycle. When the moon appears completely dark or absent it is called a new moon, like the moon at the far left. A new moon is an essential element in a solar eclipse. (Yesenia Carrero\/UConn Image)\" width=\"2000\" height=\"637\" data-srcset=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal.jpg 2000w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal-300x96.jpg 300w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal-768x245.jpg 768w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal-1024x326.jpg 1024w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/moonphases2_linearphases_horizontal-630x201.jpg 630w\" data-sizes=\"(max-width: 2000px) 100vw, 2000px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 2000px; --smush-placeholder-aspect-ratio: 2000\/637;\" \/><\/a><figcaption id=\"caption-attachment-128400\" class=\"wp-caption-text\">The lunar cycle. When the moon appears completely dark or absent it is called a new moon, like the moon at the far left. A new moon is an essential element in a solar eclipse. (Yesenia Carrero\/UConn Image)<\/figcaption><\/figure>\n<p>But during an eclipse, how can our moon, which is relatively small, appear almost as big as the sun, which is pretty gigantic?<\/p>\n<p>Peterson explains, \u201cThe sun is 400 times bigger than the moon and the sun is also 400 times farther away from the moon, so the moon appears to fit exactly during an eclipse, when they are both the same angular size.\u201d<\/p>\n<p>Holding up her fist,\u00a0she demonstrates: \u201cFind a large object ahead of you and pretend it is the sun and your fist is the moon. If you hold up your fist and look with one eye, you can\u2019t see the object\/sun.\u201d<\/p>\n<p>These are the conditions for a total solar eclipse like the one coming up. &#8220;Solar eclipses happen when the new moon obstructs the sun and the moon\u2019s shadow falls on the earth, creating a total solar eclipse.&#8221; Peterson moves her fist slightly away from herself until the edges of the object can be seen around it. \u201cOr, when the moon covers the Sun\u2019s center and creates a \u2018ring of fire\u2019 around the moon, it&#8217;s what\u2019s called an annular eclipse.\u201d<\/p>\n<p>It\u2019s those bits of the sun peeking out from behind the moon\u00a0<span style=\"margin: 0px; font-family: 'Calibri',sans-serif; font-size: 11pt;\"><span style=\"color: #000000;\">\u2013<\/span><\/span>\u00a0in both partial and total eclipses <span style=\"margin: 0px; font-family: 'Calibri',sans-serif; font-size: 11pt;\"><span style=\"color: #000000;\">\u2013<\/span><\/span> that everyone needs to be careful of. It&#8217;s extremely important to view the eclipse safely, Peterson stresses. \u201cThe problem with the eclipse is that every time it happens, some people are blinded [from looking at it unprotected]. The shadow goes whipping by at 1,000 miles per hour, and you never want to stare at the sun, even a sliver of it.\u201d<\/p>\n<p>So be prepared, and ensure you wear proper solar eclipse eye protection. Regular sunglasses will not help. Solar eclipse glasses can be used, welder\u2019s goggles, or telescopes with proper lenses. Be sure the eye protection you choose is certified by the <a href=\"https:\/\/www.iso.org\/home.html\">International Organization for Standardization<\/a> (ISO). Other popular viewing methods are DIY viewing boxes like <a href=\"https:\/\/www.livescience.com\/59721-solar-eclipse-viewer-photo-tutorial.html\">these.<\/a><\/p>\n<p>Peterson, like many others who wish to get the full eclipse experience, will be traveling to an area directly in the path of the eclipse&#8217;s shadow. These\u00a0areas are called <a href=\"http:\/\/www.eclipsewise.com\/solar\/SEgmap\/2001-2100\/SE2017Aug21Tgmap.html\">totality<\/a>. The Aug. 21 eclipse will\u00a0cover an expansive area of totality that will include 14 states and 14 major U.S. cities, stretching from Lincoln Beach, Oregon to Charleston, South Carolina.\u00a0For a map of the path of totality, go to the <a href=\"https:\/\/eclipse2017.nasa.gov\/eclipse-who-what-where-when-and-how\">NASA website<\/a>. Connecticut is unfortunately hours of travel from the nearest totality.\u00a0Peterson will\u00a0go as far as Nebraska\u00a0for the\u00a0experience.<\/p>\n<p>\u201cYou\u2019ll only see a partial eclipse here in Connecticut,&#8221; she says.\u00a0&#8220;It will get a little darker, like a cloud covering part of the sun, and then brighten up again.\u201d<\/p>\n<figure id=\"attachment_128454\" aria-describedby=\"caption-attachment-128454\" style=\"width: 550px\" class=\"wp-caption alignright\"><a href=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse.jpg\"><img decoding=\"async\" class=\"wp-image-128454 img-responsive lazyload\" data-src=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-1024x683.jpg\" alt=\"The diamond ring is one of the special effects that may be viewed during a total solar eclipse, as seen here in Queensland, Australia, on Nov. 14, 2012. (Getty Images)\" width=\"550\" height=\"367\" data-srcset=\"https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-1024x683.jpg 1024w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-300x200.jpg 300w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-768x512.jpg 768w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-630x420.jpg 630w, https:\/\/today.uconn.edu\/wp-content\/uploads\/2017\/08\/GettyImages-476869937-diamondringsolareclipse-150x100.jpg 150w\" data-sizes=\"(max-width: 550px) 100vw, 550px\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 550px; --smush-placeholder-aspect-ratio: 550\/367;\" \/><\/a><figcaption id=\"caption-attachment-128454\" class=\"wp-caption-text\">The diamond ring is one of the special effects that may be viewed during a total solar eclipse, as seen here in Queensland, Australia, on Nov. 14, 2012. (Getty Images)<\/figcaption><\/figure>\n<p>She encourages those who can to try to travel to a viewing point for the total eclipse, where they may see &#8220;amazing phenomena&#8221; like the diamond ring, shadowbands, crescent-shaped solar images under trees (instead of the usual \u2018coins\u2019 which are pinhole images of the sun), and extremely sharp shadows in the final minute before totality, due to the very narrow sun at that time. &#8220;These phenomena can <em>only<\/em> be seen in totality,&#8221; she says.<\/p>\n<p>The next chance to see a total solar eclipse will be in 2024, when its shadow will be cast closer to Connecticut. It will start in the U.S. in Texas, then make its way north, through northern Vermont and New Hampshire.<\/p>\n<p>\u201cThat\u2019s less than seven years from now,&#8221; Peterson points out, &#8220;but that\u2019s the end of eclipses crossing the U.S. until the 2050s.\u201d<\/p>\n<p>For those on campus next week, you aren&#8217;t out of luck. For this eclipse there will be a <a href=\"http:\/\/physics.uconn.edu\/2017\/08\/04\/the-solar-eclipse-viewing-party\/\">viewing party<\/a> on Horsebarn Hill behind the Dairy Bar, from 1 to 4 p.m., hosted by the Department of Physics. \u201cWe\u2019ll have solar telescopes, a pinhole camera activity, and will do some short mini-lectures on astronomy at UConn and about how eclipses work,\u201d says assistant professor of physics Jonathan Trump, one of the faculty members who will lead the viewing party.<\/p>\n<p>Peterson, longtime astronomer and scientist,\u00a0says witnessing an eclipse &#8211; especially a total eclipse &#8211; \u00a0can be extremely emotional. She suggests reading <a href=\"https:\/\/www.theatlantic.com\/science\/archive\/2017\/08\/annie-dillards-total-eclipse\/536148\/\">Annie Dillard\u2019s essay<\/a> about solar eclipses, where the author compares the contrast between viewing a partial eclipse\u00a0and viewing a total eclipse to\u00a0the difference between flying in an airplane versus falling out of the airplane. &#8220;Those are very different experiences.&#8221;<\/p>\n<p>But\u00a0wherever you are on the afternoon of Aug. 21,\u00a0Peterson says, stop and enjoy the show: \u201cGood luck and clear skies!\u201d<\/p>\n<p><em>The eclipse will be live-streamed by <a href=\"https:\/\/eclipse2017.nasa.gov\/eclipse-live-stream\">NASA<\/a>, and can also be viewed on PBS&#8217; <a href=\"http:\/\/www.pbs.org\/wgbh\/nova\/space\/eclipse-over-america.html\">NOVA<\/a> at 9 p.m. on Aug. 21.<\/em><\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>On Aug. 21, a solar eclipse will be visible throughout North America for the first time in 38 years. UConn astronomer Cynthia Peterson explains what to expect.<\/p>\n","protected":false},"author":118,"featured_media":128394,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"_crdt_document":"","wds_primary_category":0,"wds_primary_series":0,"wds_primary_attribution":0,"footnotes":""},"categories":[2226,2225,2234],"tags":[],"magazine-issues":[],"coauthors":[2093],"class_list":["post-128247","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-clas","category-uconn-storrs","category-university-life"],"pp_statuses_selecting_workflow":false,"pp_workflow_action":"current","pp_status_selection":"publish","acf":[],"publishpress_future_action":{"enabled":false,"date":"2026-04-23 15:35:10","action":"change-status","newStatus":"draft","terms":[],"taxonomy":"category","extraData":[]},"publishpress_future_workflow_manual_trigger":{"enabledWorkflows":[]},"_links":{"self":[{"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/posts\/128247","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/users\/118"}],"replies":[{"embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/comments?post=128247"}],"version-history":[{"count":15,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/posts\/128247\/revisions"}],"predecessor-version":[{"id":128463,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/posts\/128247\/revisions\/128463"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/media\/128394"}],"wp:attachment":[{"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/media?parent=128247"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/categories?post=128247"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/tags?post=128247"},{"taxonomy":"magazine-issue","embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/magazine-issues?post=128247"},{"taxonomy":"author","embeddable":true,"href":"https:\/\/today.uconn.edu\/wp-rest\/wp\/v2\/coauthors?post=128247"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}