<?xml version="1.0"?>
<rss version="2.0">
   <channel>
      <title>Fusion model project  by Jeshuel Segui</title>
      <link>https://padlet.com/273344/brzhdmpl6ij3</link>
      <description>Made with eyes on the prize</description>
      <language>en-us</language>
      <pubDate>2018-09-12 14:01:39 UTC</pubDate>
      <lastBuildDate>2026-03-21 11:23:43 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
      <image>
         <url></url>
      </image>
      <item>
         <title>The sun </title>
         <author>273344</author>
         <link>https://padlet.com/273344/brzhdmpl6ij3/wish/280355621</link>
         <description><![CDATA[<div>The sun is about 10,000 degrees Fahrenheit and rises as you go towards the center of it. Temperatures at the center of the sun can rise up to about 27,000 degrees Fahrenheit.</div>]]></description>
         <enclosure url="https://fthmb.tqn.com/kXHMATRAH5GsKVR7P7r8W3q0UFs=/1733x1733/filters:fill(auto,1)/140892340-56a12e8e3df78cf772683333.jpg" />
         <pubDate>2018-09-12 14:05:32 UTC</pubDate>
         <guid>https://padlet.com/273344/brzhdmpl6ij3/wish/280355621</guid>
      </item>
      <item>
         <title>Inputs of fusion </title>
         <author>273344</author>
         <link>https://padlet.com/273344/brzhdmpl6ij3/wish/280362528</link>
         <description><![CDATA[<div>Two protons fuse together&nbsp;<br><br>Four hydrogen nuclei also come together&nbsp;<br><br>Fusion requires temperatures up to 179,999,540 degrees Fahrenheit.&nbsp;<br><br>A lot of energy is involved in this process<br><br><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2018-09-12 14:17:27 UTC</pubDate>
         <guid>https://padlet.com/273344/brzhdmpl6ij3/wish/280362528</guid>
      </item>
      <item>
         <title>Outputs of fusion </title>
         <author>273344</author>
         <link>https://padlet.com/273344/brzhdmpl6ij3/wish/280370947</link>
         <description><![CDATA[<div>The two protons fuse to make two deuterons<br><br>Four hydrogen nuclei come together in order to make a helium nucleus <br><br>This reaction also causes the sun to produce gamma rays. </div>]]></description>
         <enclosure url="http://i.dailymail.co.uk/i/pix/2014/03/23/article-2587072-1C80D5FC00000578-227_634x535.jpg" />
         <pubDate>2018-09-12 14:30:34 UTC</pubDate>
         <guid>https://padlet.com/273344/brzhdmpl6ij3/wish/280370947</guid>
      </item>
      <item>
         <title>How hydrogen and helium change in a star. </title>
         <author>273344</author>
         <link>https://padlet.com/273344/brzhdmpl6ij3/wish/280377406</link>
         <description><![CDATA[<div>As time goes by in the life cycle of a star the star begins to run out of hydrogen and turns the hydrogen it has into helium.<br><br>When the sun then runs out of helium, the helium ash in the core will build up and become unstable and collapse under its own weight, then the core heats up, gets denser and causes the sun to grow in size, turning into the red giant faze of its life </div>]]></description>
         <enclosure url="http://www.pausetowonder.org/wp-content/uploads/2013/08/RedGiant.jpeg" />
         <pubDate>2018-09-12 14:40:24 UTC</pubDate>
         <guid>https://padlet.com/273344/brzhdmpl6ij3/wish/280377406</guid>
      </item>
      <item>
         <title>Explanation </title>
         <author>273344</author>
         <link>https://padlet.com/273344/brzhdmpl6ij3/wish/280392055</link>
         <description><![CDATA[<div>High temperatures cause particles to move rapidly due to the high temperatures, causing them to collide and fuse together which also causes the particles to lose mass and release energy which will cause fusion</div>]]></description>
         <enclosure url="http://www.physicsoftheuniverse.com/images/glossary_fusion.jpg" />
         <pubDate>2018-09-12 15:02:41 UTC</pubDate>
         <guid>https://padlet.com/273344/brzhdmpl6ij3/wish/280392055</guid>
      </item>
   </channel>
</rss>
