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      <title>Catalogue by Nasla Reyes</title>
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      <language>en-us</language>
      <pubDate>2024-09-17 19:55:05 UTC</pubDate>
      <lastBuildDate>2024-09-18 15:01:44 UTC</lastBuildDate>
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         <title>Nebulae</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124279100</link>
         <description><![CDATA[<p>A nebula is a giant cloud of dust and gas that floats between stars. The word "nebula" comes from the Latin word for "mist, vapor, fog, smoke, exhalation".</p>]]></description>
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         <pubDate>2024-09-17 19:56:53 UTC</pubDate>
         <guid>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124279100</guid>
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         <title>Planetary nebulae</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124280320</link>
         <description><![CDATA[<p>A planetary nebula is a cloud of gas and dust that forms when a star dies</p>]]></description>
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         <pubDate>2024-09-17 19:58:04 UTC</pubDate>
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         <title>Supernova remnants
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124283835</link>
         <description><![CDATA[<p> A supernova remnant is the structure left behind after a star explodes.</p>]]></description>
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         <pubDate>2024-09-17 20:01:13 UTC</pubDate>
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         <title>Diffuse nebulae</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124298017</link>
         <description><![CDATA[<p><strong>The birthplace of stars</strong>. Diffuse nebula are the clouds of material formed from the explosions of population three, population two stars, and the left over hydrogen and helium from the Big Bang</p>]]></description>
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         <pubDate>2024-09-17 20:13:47 UTC</pubDate>
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         <title>HR Diagram
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124298857</link>
         <description><![CDATA[<p>The Hertzsprung-Russell (H-R) diagram is a graph that plots stars' luminosity against their temperature. It's a tool astronomers use to classify stars and understand their evolution.&nbsp;</p><p><br></p>]]></description>
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         <pubDate>2024-09-17 20:14:38 UTC</pubDate>
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         <title>Main sequence star
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124299850</link>
         <description><![CDATA[<p>A main sequence star is a star that is currently in the most stable phase of its life, fusing hydrogen into helium in its core to produce energy.&nbsp;</p><p><br></p>]]></description>
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         <pubDate>2024-09-17 20:15:24 UTC</pubDate>
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         <title>White dwarf
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124303873</link>
         <description><![CDATA[<p>A white dwarf is what stars like the Sun become after they have exhausted their nuclear fuel. Near the end of its nuclear burning stage, this type of star expels most of its outer material, creating a planetary nebula. Only the hot core of the star remains.</p>]]></description>
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         <pubDate>2024-09-17 20:17:39 UTC</pubDate>
         <guid>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3124303873</guid>
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         <title>Super giants
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125786810</link>
         <description><![CDATA[<p><strong>A star classed as a supergiant may have a diameter several hundred times that of the Sun and a luminosity nearly 1,000,000 times as great</strong>.</p>]]></description>
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         <pubDate>2024-09-18 14:54:57 UTC</pubDate>
         <guid>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125786810</guid>
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         <title>Giants
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125790455</link>
         <description><![CDATA[<p>Giant stars are stars that are much larger and more luminous than other stars with similar colors</p>]]></description>
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         <pubDate>2024-09-18 14:56:38 UTC</pubDate>
         <guid>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125790455</guid>
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         <title>Nova</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125792408</link>
         <description><![CDATA[<p>A nova is a sudden, short-lived explosion that occurs on the surface of a star, causing it to temporarily increase in brightness by hundreds to millions of times. The word "nova" comes from the Latin word for "new star".&nbsp;</p><p><br></p>]]></description>
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         <pubDate>2024-09-18 14:57:41 UTC</pubDate>
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         <title>Supernova
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125797734</link>
         <description><![CDATA[<p>A supernova is a massive explosion that occurs when a star dies.</p>]]></description>
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         <pubDate>2024-09-18 15:00:35 UTC</pubDate>
         <guid>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125797734</guid>
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         <title>Black hole
</title>
         <author>nreyes414</author>
         <link>https://padlet.com/nreyes414/bee5166f0ujk9psk/wish/3125799199</link>
         <description><![CDATA[<p>A black hole is a region in space where gravity is so strong that nothing, including light, can escape.</p>]]></description>
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         <pubDate>2024-09-18 15:01:24 UTC</pubDate>
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