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      <title>The Sun by Olivia King</title>
      <link>https://padlet.com/olivia_king4/mirm8917kbjt</link>
      <description>Module 16.3</description>
      <language>en-us</language>
      <pubDate>2018-01-10 19:05:02 UTC</pubDate>
      <lastBuildDate>2025-12-07 02:22:26 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title></title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220341446</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:310,&quot;url&quot;:&quot;http://nineplanets.org/images/thesun.jpg&quot;,&quot;width&quot;:325}" data-trix-content-type="image"><img src="http://nineplanets.org/images/thesun.jpg" width="325" height="310"><figcaption class="attachment__caption"></figcaption></figure></div>]]></description>
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         <pubDate>2018-01-10 19:07:30 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220341446</guid>
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      <item>
         <title></title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220341992</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:516,&quot;url&quot;:&quot;https://www.nasa.gov/images/content/171925main_heliolayers_label_516.jpg&quot;,&quot;width&quot;:516}" data-trix-content-type="image"><img src="https://www.nasa.gov/images/content/171925main_heliolayers_label_516.jpg" width="516" height="516"><figcaption class="attachment__caption"></figcaption></figure></div>]]></description>
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         <pubDate>2018-01-10 19:08:35 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220341992</guid>
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      <item>
         <title>The Core</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220344075</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:634,&quot;url&quot;:&quot;https://cdn.thinglink.me/api/image/708382021197496320/1240/10/scaletowidth&quot;,&quot;width&quot;:634}" data-trix-content-type="image"><img src="https://cdn.thinglink.me/api/image/708382021197496320/1240/10/scaletowidth" width="634" height="634"><figcaption class="attachment__caption"></figcaption></figure>The core of the Sun has a temperature of more than 15 million degrees Kelvin. It also has the density of plasma.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:12:39 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220344075</guid>
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         <title>Radiative Layer</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220345448</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:240,&quot;url&quot;:&quot;https://solarscience.msfc.nasa.gov/images/cutaway_sm.jpg&quot;,&quot;width&quot;:240}" data-trix-content-type="image"><img src="https://solarscience.msfc.nasa.gov/images/cutaway_sm.jpg" width="240" height="240"><figcaption class="attachment__caption"></figcaption></figure>The radiative layer is between the core and the convective layer. It is 70% of the sun's radius. At the top of this layer, the energy begins to move in a different direction.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:15:11 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220345448</guid>
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         <title>Convective Layer</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220347714</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:185,&quot;url&quot;:&quot;https://www.cac.cornell.edu/slantz/SPUR/SPUR95/Jason/suncutT.gif&quot;,&quot;width&quot;:238}" data-trix-content-type="image"><img src="https://www.cac.cornell.edu/slantz/SPUR/SPUR95/Jason/suncutT.gif" width="238" height="185"><figcaption class="attachment__caption"></figcaption></figure>The Convective layer is the outermost layer of the interior of the Sun. It is about 2 million degrees Celsius in temperature. The fluid inside this layer begins to "boil".</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:19:25 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220347714</guid>
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         <title>Photosphere</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220349863</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:249,&quot;url&quot;:&quot;http://cronodon.com/sitebuilder/images/Photosphere-249x249.jpg&quot;,&quot;width&quot;:249}" data-trix-content-type="image"><img src="http://cronodon.com/sitebuilder/images/Photosphere-249x249.jpg" width="249" height="249"><figcaption class="attachment__caption"></figcaption></figure>This layer is the lowest layer in the sun's atmosphere and is about 300 miles thick. It is also the layer where the sun's energy is released as light.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:23:49 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220349863</guid>
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         <title>Chromosphere</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220351225</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:350,&quot;url&quot;:&quot;https://scied.ucar.edu/sites/default/files/styles/short_content_small_image/public/images/small_image_for_image_content/chromosphere_eclipse_11aug1999_360x360.jpg?itok=utT7-TG0&quot;,&quot;width&quot;:350}" data-trix-content-type="image"><img src="https://scied.ucar.edu/sites/default/files/styles/short_content_small_image/public/images/small_image_for_image_content/chromosphere_eclipse_11aug1999_360x360.jpg?itok=utT7-TG0" width="350" height="350"><figcaption class="attachment__caption"></figcaption></figure>The chromosphere is the layer that makes the sun have a reddish ring around and can only be seen during a total solar eclipse. It makes the heat from the inside of the sun reach the outer layer of the sun's atmosphere.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:26:45 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220351225</guid>
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         <title>Corona</title>
         <author>olivia_king4</author>
         <link>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220353021</link>
         <description><![CDATA[<div><figure class="attachment attachment--preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:375,&quot;url&quot;:&quot;https://spaceplace.nasa.gov/sun-corona/en/corona1.en.jpg&quot;,&quot;width&quot;:500}" data-trix-content-type="image"><img src="https://spaceplace.nasa.gov/sun-corona/en/corona1.en.jpg" width="500" height="375"><figcaption class="attachment__caption"></figcaption></figure>This is the final layer in the sun's atmosphere. It can only be seen during a solar eclipse. It is about 2 million degrees Celsius in temperature, approximately 300 times hotter than the photosphere.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-01-10 19:30:14 UTC</pubDate>
         <guid>https://padlet.com/olivia_king4/mirm8917kbjt/wish/220353021</guid>
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