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      <title>The Sun  by Gissel Amaya</title>
      <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1</link>
      <description></description>
      <language>en-us</language>
      <pubDate>2017-05-12 21:57:21 UTC</pubDate>
      <lastBuildDate>2025-04-24 09:06:30 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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      <item>
         <title>The layers of the sun </title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171585429</link>
         <description><![CDATA[]]></description>
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         <pubDate>2017-05-12 21:59:58 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171585429</guid>
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         <title>The core </title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171585483</link>
         <description><![CDATA[<div>The Sun's core is the central region. It has  very high temperature, it also gives the sun energy </div>]]></description>
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         <pubDate>2017-05-12 22:01:05 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171585483</guid>
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      <item>
         <title>Radiative Zone</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171586010</link>
         <description><![CDATA[<div>is the section of the solar interior between the innermost core and the outer convective zone. </div>]]></description>
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         <pubDate>2017-05-12 22:11:33 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171586010</guid>
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         <title>cites </title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171586087</link>
         <description><![CDATA[<div><a href="https://solarscience.msfc.nasa.gov/interior.shtml">https://solarscience.msfc.nasa.gov/interior.shtml</a><br><a href="www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html">www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html</a><br><a href="https://www.cora.nwra.com/~werne/eos/text/convection_zone.html">https://www.cora.nwra.com/~werne/eos/text/convection_zone.html</a><br><a href="https://www.google.com/search?q=sunspots+sun&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;sqi=2&amp;ved=0ahUKEwiN0YaP2OvTAhVL4SYKHVjmC8kQ_AUIBigB&amp;biw=1280&amp;bih=645#imgrc=tCDZWoQkDZblyM:">https://www.google.com/search?q=sunspots+sun&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;sqi=2&amp;ved=0ahUKEwiN0YaP2OvTAhVL4SYKHVjmC8kQ_AUIBigB&amp;biw=1280&amp;bih=645#imgrc=tCDZWoQkDZblyM:</a></div>]]></description>
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         <pubDate>2017-05-12 22:12:48 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171586087</guid>
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      <item>
         <title>Convective Zone</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590329</link>
         <description><![CDATA[<div>it's the interior of the sun, is where light (photons) is created.</div>]]></description>
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         <pubDate>2017-05-13 00:48:18 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590329</guid>
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      <item>
         <title>Photosphere</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590505</link>
         <description><![CDATA[<div>The temperature drops dramatically near the surface of the photosphere Zone. It is visable fpr us in earth. </div>]]></description>
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         <pubDate>2017-05-13 00:54:51 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590505</guid>
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      <item>
         <title>Chromospere</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590668</link>
         <description><![CDATA[<div>it is 2,000-3,00 km thick. glows a reddish color. </div>]]></description>
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         <pubDate>2017-05-13 00:59:50 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590668</guid>
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      <item>
         <title>Corona</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590901</link>
         <description><![CDATA[<div>The temperature is millions of degrees. It's pressure and density are lower than earth.</div>]]></description>
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         <pubDate>2017-05-13 01:08:16 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590901</guid>
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      <item>
         <title>sunspots </title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590977</link>
         <description><![CDATA[<div>They are created when the sun magnetic field gets twisted inside the sun. </div>]]></description>
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         <pubDate>2017-05-13 01:11:30 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171590977</guid>
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      <item>
         <title>prominence.</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591115</link>
         <description><![CDATA[<div>They are arcs of gas, also known has plasma, that erupts from the suns surface. </div>]]></description>
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         <pubDate>2017-05-13 01:16:27 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591115</guid>
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      <item>
         <title>flare</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591332</link>
         <description><![CDATA[<div>Flares are sudden rapid and variation in brightness. They are form when magnetic energy is suddenly released. </div>]]></description>
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         <pubDate>2017-05-13 01:25:33 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591332</guid>
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      <item>
         <title> aurora</title>
         <author>gisselamaya5</author>
         <link>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591481</link>
         <description><![CDATA[<div>Is the sign that something electric  is happening in space. Charged energy particles flow out of the sun towards the earth by the solar wind, This reacts with earth's magnetic field which changes most of the energy and it creates a huge whole in the solar wind.</div>]]></description>
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         <pubDate>2017-05-13 01:31:39 UTC</pubDate>
         <guid>https://padlet.com/gisselamaya5/kf2j4tz32ek1/wish/171591481</guid>
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