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      <title>mooooo by Tayla Brown</title>
      <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3</link>
      <description>this is gay</description>
      <language>en-us</language>
      <pubDate>2021-10-19 03:15:52 UTC</pubDate>
      <lastBuildDate>2021-10-19 03:59:00 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
      <image>
         <url></url>
      </image>
      <item>
         <title>Stellar Nebula</title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1825999882</link>
         <description><![CDATA[<div>a nebula is a giant cloud of dust and gas </div>]]></description>
         <enclosure url="https://www.universetoday.com/wp-content/uploads/2013/02/NGC5189.jpg" />
         <pubDate>2021-10-19 03:28:13 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1825999882</guid>
      </item>
      <item>
         <title>average or low mass star  </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826020038</link>
         <description><![CDATA[<div>contains less fuel and lower temp </div>]]></description>
         <enclosure url="http://uk.unawe.org/static/archives/images/medium/low-mass_star.jpg" />
         <pubDate>2021-10-19 03:37:48 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826020038</guid>
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      <item>
         <title>high mass star </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826023686</link>
         <description><![CDATA[<div>contains more fuel and hotter temp</div>]]></description>
         <enclosure url="http://svs.gsfc.nasa.gov/vis/a010000/a011000/a011095/SDO_SDO_20120831_335.00007.jpg" />
         <pubDate>2021-10-19 03:39:29 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826023686</guid>
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      <item>
         <title>red giant </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826029211</link>
         <description><![CDATA[<div>Nuclear fusion occurs to form helium. This continues in the core as long as there is hydrogen left to fuel it.</div><div><br><br><br><br></div>]]></description>
         <enclosure url="https://www.schoolsobservatory.org/sites/default/files/astro/redgiant.jpg" />
         <pubDate>2021-10-19 03:42:08 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826029211</guid>
      </item>
      <item>
         <title>planetary nebula </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826031938</link>
         <description><![CDATA[<div>When fuel starts running out, the core will begin to shrink and get hotter, causing the excess energy will radiate outwards, pushing the outer layers away from the core. This stage is known as the red giant</div>]]></description>
         <enclosure url="http://cdn.sci-news.com/images/enlarge7/image_8695e-NGC-2899.jpg" />
         <pubDate>2021-10-19 03:43:32 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826031938</guid>
      </item>
      <item>
         <title>white dwarf</title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826034054</link>
         <description><![CDATA[<div>Once all the hydrogen is gone, nuclear fusion will take a different approach, fusing helium together to form heavier elements. This causes the star to shrink and become hotter, turning bluer.</div>]]></description>
         <enclosure url="http://www.extrasolar.de/images/1/9/1/0/3/19103d5d4a722d187ba6afdaa6933ca2311252a4-white-dwarf.jpeg" />
         <pubDate>2021-10-19 03:44:38 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826034054</guid>
      </item>
      <item>
         <title>red super giant </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826042357</link>
         <description><![CDATA[<div>Nuclear fusion occurs, turning Hydrogen into helium and heavier elements. As nuclear fusion progresses, the radiation is pushed outwards, forming a red supergiant.</div><div><br><br><br><br></div>]]></description>
         <enclosure url="https://d.ibtimes.co.uk/en/full/1633311/antares-red-supergiant.jpg?w=736" />
         <pubDate>2021-10-19 03:49:15 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826042357</guid>
      </item>
      <item>
         <title>supernova </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826047073</link>
         <description><![CDATA[<div>When fuel runs out, the iron core is stable and does not release any more energy. Gravity pulls the outer layers inward, causing it to bounce off the core and trigger an explosion known as a supernova. Elements heavier than iron can be created during this explosion</div><div><br><br><br><br></div>]]></description>
         <enclosure url="https://www.tunisiesoir.com/wp-content/uploads/2020/07/Thermonuclear-blast-sends-supernova-survivor-star-hurtling-across-the-Milky.jpg" />
         <pubDate>2021-10-19 03:51:43 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826047073</guid>
      </item>
      <item>
         <title>black hole </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826056478</link>
         <description><![CDATA[<div>The remnants of a supernova is known as a neutron star. A neutron star is a compressed giant ball of neutrons that was leftover from the explosion.</div>]]></description>
         <enclosure url="https://fossbytes.com/wp-content/uploads/2015/07/02160748/Black-hole.jpg" />
         <pubDate>2021-10-19 03:57:27 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826056478</guid>
      </item>
      <item>
         <title>neutron star </title>
         <author>taylabrown1</author>
         <link>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826058838</link>
         <description><![CDATA[<div>A very massive star that undergoes supernova may result in a black hole occurring. Black holes are objects so dense that not even light can escape their gravity. They are formed due to the pressure of gravity causing the core of the star to be densely packed within 0 volume.</div>]]></description>
         <enclosure url="https://farm4.staticflickr.com/3694/14277320623_66c55777e8_b.jpg" />
         <pubDate>2021-10-19 03:58:52 UTC</pubDate>
         <guid>https://padlet.com/taylabrown1/9gtdva45ifiugcs3/wish/1826058838</guid>
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