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      <title>The Sun by </title>
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      <description>Ariana Benbenek: Module 16 Assignment 3</description>
      <language>en-us</language>
      <pubDate>2017-08-05 01:28:38 UTC</pubDate>
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         <title>The Sun: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156682</link>
         <description><![CDATA[<div>The Sun is an incredible yellow star that all the planets in our solar system revolve around. <br><a href="https://goo.gl/images/ky7tkD">https://goo.gl/images/ky7tkD</a> </div>]]></description>
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         <pubDate>2017-08-05 01:30:05 UTC</pubDate>
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         <title>Layers: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156725</link>
         <description><![CDATA[<div>The Sun has many distinct layers that are vital to the life of the giant star. <br><a href="https://goo.gl/images/7fWZkO">https://goo.gl/images/7fWZkO</a> </div>]]></description>
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         <pubDate>2017-08-05 01:32:31 UTC</pubDate>
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         <title>Core: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156757</link>
         <description><![CDATA[<div>This is the innermost portion of the Sun, where energy is created by nuclear reactions, like fission and fusion of mostly hydrogen and helium. <br><a href="https://goo.gl/images/M38kAj">https://goo.gl/images/M38kAj</a><br><a href="https://soho.nascom.nasa.gov/classroom/glossary.html#CORE">https://soho.nascom.nasa.gov/classroom/glossary.html#CORE</a> </div>]]></description>
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         <pubDate>2017-08-05 01:34:31 UTC</pubDate>
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         <title>Radiative Zone: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156847</link>
         <description><![CDATA[<div>This layer of the Sun if found in between the core and the convectivezone. This layer is where energy travels outward by radiation. <br><a href="https://soho.nascom.nasa.gov/classroom/glossary.html#CORE">https://soho.nascom.nasa.gov/classroom/glossary.html#CORE</a><br><a href="https://goo.gl/images/wS1Fgx">https://goo.gl/images/wS1Fgx</a> </div>]]></description>
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         <pubDate>2017-08-05 01:39:05 UTC</pubDate>
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         <title>Convective Zone: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156933</link>
         <description><![CDATA[<div><br></div><div>This is the layer of the Sun in which convection currents are the main mechanism by which energy is transported outward. This extends outward from the photosphere and into the solar radius by around 70%. <br><a href="https://goo.gl/images/KwmcKC">https://goo.gl/images/KwmcKC</a> </div>]]></description>
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         <pubDate>2017-08-05 01:41:39 UTC</pubDate>
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         <title>Photosphere: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180156971</link>
         <description><![CDATA[<div>This is the visible surface of the Sun. The human eye can see this layer because of the light emitted by gases and other phenomena, and we can also see sunspots. <br><a href="https://goo.gl/images/E1AyQV">https://goo.gl/images/E1AyQV</a> </div>]]></description>
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         <pubDate>2017-08-05 01:44:20 UTC</pubDate>
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         <title>Chromosphere: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180157609</link>
         <description><![CDATA[<div>This is the layer of the Sun that is located above the photosphere and below the Corona. The chromosphere is hotter than the photosphere but not as hot as the corona. <br><a href="https://goo.gl/images/58Q7oY">https://goo.gl/images/58Q7oY</a> </div>]]></description>
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         <pubDate>2017-08-05 01:47:10 UTC</pubDate>
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         <title>Corona: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158235</link>
         <description><![CDATA[<div><br>This is the outermost layer of the Sun. The corona consists of gas with a temperature greater than one million kelvin. It is visible to the naked eye during a solar eclipse. <br><a href="https://goo.gl/images/z33TYL">https://goo.gl/images/z33TYL</a> </div>]]></description>
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         <pubDate>2017-08-05 01:49:26 UTC</pubDate>
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         <title>Sunspots: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158427</link>
         <description><![CDATA[<div>Sunspots are temporary disturbed areas in the photosphere that appears dark because it is cooler than the surrounding areas. <br><a href="https://goo.gl/images/TZel5K">https://goo.gl/images/TZel5K</a> </div>]]></description>
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         <pubDate>2017-08-05 01:51:29 UTC</pubDate>
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         <title>Prominence: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158594</link>
         <description><![CDATA[<div>A bright structure in the corona consisting of cool plasma supported by magnetic fields. Prominences seen on the disk are also known as filaments. <br><a href="https://goo.gl/images/M95kRv">https://goo.gl/images/M95kRv</a> </div>]]></description>
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         <pubDate>2017-08-05 01:59:13 UTC</pubDate>
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         <title>Solar Flare: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158675</link>
         <description><![CDATA[<div>Rapid release of energy from a region on the Sun in the form of electromagnetic radiation,  energetic particles, and mass motions. <br><a href="https://goo.gl/images/J4UiYh">https://goo.gl/images/J4UiYh</a></div>]]></description>
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         <pubDate>2017-08-05 02:01:10 UTC</pubDate>
         <guid>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158675</guid>
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      <item>
         <title>Aurora Borealis: </title>
         <author>ariana_2992</author>
         <link>https://padlet.com/ariana_2992/98i3q512acdn/wish/180158709</link>
         <description><![CDATA[<div>A display of colored light given off by collisions between charged particles trapped in the Sun's magnetic fields and atoms of atmospheric gases near the planet's magnetic poles. <br><a href="https://goo.gl/images/KJWWtZ">https://goo.gl/images/KJWWtZ</a> </div>]]></description>
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         <pubDate>2017-08-05 02:02:49 UTC</pubDate>
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