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      <title>Big Chungus Star Padlet  by Aidan Butler</title>
      <link>https://padlet.com/444311/46kj5u1qwjet</link>
      <description>Our lord and savior Chungus </description>
      <language>en-us</language>
      <pubDate>2019-01-10 19:58:45 UTC</pubDate>
      <lastBuildDate>2019-01-18 19:56:45 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title>What is a Star?</title>
         <author>444311</author>
         <link>https://padlet.com/444311/46kj5u1qwjet/wish/319850158</link>
         <description><![CDATA[<div>Our Sun is a star,  it's a yellow dwarf.  Our Sun was created through composition and has many layers, the core, the radiation zone and convection zone are just several of them. Our star right now looks like a bright yellow ball, but later in its life it will change. </div>]]></description>
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         <pubDate>2019-01-11 19:51:19 UTC</pubDate>
         <guid>https://padlet.com/444311/46kj5u1qwjet/wish/319850158</guid>
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         <title>Stage 1: Nebulea </title>
         <author>444311</author>
         <link>https://padlet.com/444311/46kj5u1qwjet/wish/321076457</link>
         <description><![CDATA[<div>Nebulea is a large cloud  of gas and dust spread out in an immense volume. The contracting gas and dust from a nebula become so dense and hot that nuclear fission starts, and a star is born. </div>]]></description>
         <enclosure url="http://www.smashinglists.com/wp-content/uploads/2010/05/helix-nebula.jpg" />
         <pubDate>2019-01-16 03:37:17 UTC</pubDate>
         <guid>https://padlet.com/444311/46kj5u1qwjet/wish/321076457</guid>
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         <title>Main Sequence </title>
         <author>444311</author>
         <link>https://padlet.com/444311/46kj5u1qwjet/wish/321533345</link>
         <description><![CDATA[<div>This is the stage our Sun is in right now. In which our Sun creates an enormous amount of energy in its core through a process called nuclear fusion In this process, hydrogen atoms fuse together to form helium. This energy is slowly pushed out into space after going through the layers of the Sun. </div>]]></description>
         <enclosure url="http://hosting.astro.cornell.edu/academics/courses/astro201/images/hydrogen_burn.gif" />
         <pubDate>2019-01-17 03:37:54 UTC</pubDate>
         <guid>https://padlet.com/444311/46kj5u1qwjet/wish/321533345</guid>
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      <item>
         <title>Protostar</title>
         <author>444311</author>
         <link>https://padlet.com/444311/46kj5u1qwjet/wish/321997592</link>
         <description><![CDATA[<div>A protostar is a loose mass of cold dust and gasses. Energy is transported from the core of the protostar to the photoshpere and  through the convection.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-01-18 04:50:38 UTC</pubDate>
         <guid>https://padlet.com/444311/46kj5u1qwjet/wish/321997592</guid>
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