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      <title>P6B3 Life Cycle of the Sun by Ms. Chang</title>
      <link>https://padlet.com/misschang1/hish6gj5ldnw82z8</link>
      <description>From its birth to its death. </description>
      <language>en-us</language>
      <pubDate>2021-01-21 20:00:47 UTC</pubDate>
      <lastBuildDate>2026-03-16 00:56:58 UTC</lastBuildDate>
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         <title>Nebula</title>
         <author>s1004043787</author>
         <link>https://padlet.com/misschang1/hish6gj5ldnw82z8/wish/1115683011</link>
         <description><![CDATA[<div>They are huge they are size to 1 AU to 10 AU and they are really bright there SNRS 1-6 and its extremely hot 25,000-100,000 degrees. an interesting fact A dark nebula is so dense that objects behind are obscured. This type of nebula extinguishes light with interstellar dust grains. </div>]]></description>
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         <pubDate>2021-01-22 19:52:44 UTC</pubDate>
         <guid>https://padlet.com/misschang1/hish6gj5ldnw82z8/wish/1115683011</guid>
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         <title>RED GIANT</title>
         <author>s1004019246</author>
         <link>https://padlet.com/misschang1/hish6gj5ldnw82z8/wish/1115714459</link>
         <description><![CDATA[<div>This giant fire looking ball is a huge dying star. The helium in the core will run out and fusion stops. The star keeps shrinking until a new helium shell reaches the core. Accorning to scientist in about 5bill. years the sun will begin the helium- burning procces. This star is 100 mil. to 1bill. kilometers in diameter, 62 mill. to 621 mil. miles. It is 100-1000 times the size of the sun. The luminosity of this star is about 3thousand times of the sun.It is 4000 to 5800 degrees fahrenheit.  Extremely bright and hot!! <br>*IN A FEW BILLION YEARS OUR SUN WILL TURN INTO A RED GIANT, IT WILL EXPAND AND SWEEP THE INNER PLANETS, MAYBE EVEN EARTH TOO!</div>]]></description>
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         <pubDate>2021-01-22 20:02:27 UTC</pubDate>
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         <title></title>
         <author>s1000284485</author>
         <link>https://padlet.com/misschang1/hish6gj5ldnw82z8/wish/1124455014</link>
         <description><![CDATA[]]></description>
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         <pubDate>2021-01-25 22:46:46 UTC</pubDate>
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         <title>White Dwarf</title>
         <author>s1004020202</author>
         <link>https://padlet.com/misschang1/hish6gj5ldnw82z8/wish/1124455381</link>
         <description><![CDATA[<div>A white dwarf is very dens its mass is comparable to that of the Sun, while its volume is comparable to that of Earth. <br>A white dwarf is what stars like the Sun become after they have exhausted their nuclear fuel.<br>The first white dwarf discovered was in the triple star system of 40 Eridani.A typical white dwarf has a carbon and oxygen mass similar to the Sun, but is much smaller in size . It is much hotter, but because of its small size its luminosity is low , White dwarf stars can be observed directly through telescopes, though they are extremely faint.white dwarf with temperatures over 180,000 degrees Fahernhite 100,000 degrees Celsius.<br> White dwarf can go supernova. Their gravity is 350,000x Earth's. The Sun will one day become a white dwarf. Many will become black dwarfs.</div><div><br></div><div><br></div><div><br></div><div><br></div><div><br></div>]]></description>
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         <pubDate>2021-01-25 22:47:00 UTC</pubDate>
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