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      <title>Big Bang Project by Ian Wilson</title>
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      <pubDate>2022-09-09 14:16:08 UTC</pubDate>
      <lastBuildDate>2022-09-13 14:03:05 UTC</lastBuildDate>
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         <title>What the Big Bang Theory is</title>
         <author>ianwilson10</author>
         <link>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2289768104</link>
         <description><![CDATA[<div>It is how most astronomers believe the universe began, that the universe began at a single point and then expanded until it was as large as it is now, it´s still expanding! </div>]]></description>
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         <pubDate>2022-09-09 14:28:23 UTC</pubDate>
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         <title>George Leaître</title>
         <author>ianwilson10</author>
         <link>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2289779360</link>
         <description><![CDATA[<div>George Leaître thought of the idea of the Big Bang which he first shared&nbsp;in a paper in 1931.</div>]]></description>
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         <pubDate>2022-09-09 14:35:19 UTC</pubDate>
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         <title></title>
         <author>ianwilson10</author>
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         <pubDate>2022-09-09 14:36:06 UTC</pubDate>
         <guid>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2289780828</guid>
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         <title>Red Shifts</title>
         <author>ianwilson10</author>
         <link>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2292423202</link>
         <description><![CDATA[<div>It's a doppler effect but with color, the faster a star is moving away the more its electromagnetic radiation waves (light) will be on the warm side of the light spectrum.</div>]]></description>
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         <pubDate>2022-09-12 14:07:17 UTC</pubDate>
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         <title>Cosmic Background Radiation (CMB)</title>
         <author>ianwilson10</author>
         <link>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2292463373</link>
         <description><![CDATA[<div>CMB is the recording of the photons at the moment of their escape from the "fog" (Extremely hot plasma). First detected by two scientist, Arno Penzias and Robert Wilson in 1965.</div>]]></description>
         <enclosure url="https://astronomy.swin.edu.au/cosmos/C/Cosmic+microwave+background" />
         <pubDate>2022-09-12 14:25:37 UTC</pubDate>
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         <title>Arno Penzias</title>
         <author>ianwilson10</author>
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         <pubDate>2022-09-12 14:26:18 UTC</pubDate>
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         <title>Robert Wilson</title>
         <author>ianwilson10</author>
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         <pubDate>2022-09-12 14:27:48 UTC</pubDate>
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         <title>H (Hydrogen) to He (Helium)</title>
         <author>ianwilson10</author>
         <link>https://padlet.com/ianwilson10/fzp3wuxxiz0iwaz0/wish/2294353289</link>
         <description><![CDATA[<div>According to <em>Hydrogen-Helium Abundance</em> "Schramm's figures for relative abundances indicate that helium is about 25% by mass and hydrogen about 73% with all other elements constituting less than 2%."</div>]]></description>
         <enclosure url="http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/hydhel.html#:~:text=Hydrogen%20and%20helium%20account%20for,or%20%22big%20bang%22%20model.&amp;text=Schramm%27s%20figures%20for%20relative%20abundances,elements%20constituting%20less%20than%202%25" />
         <pubDate>2022-09-13 13:58:53 UTC</pubDate>
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         <title></title>
         <author>ianwilson10</author>
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         <pubDate>2022-09-13 14:00:19 UTC</pubDate>
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         <title></title>
         <author>ianwilson10</author>
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         <pubDate>2022-09-13 14:02:25 UTC</pubDate>
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