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      <title>Astronomy TEK 11A by Brieanna Carr</title>
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      <pubDate>2023-10-16 15:14:15 UTC</pubDate>
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         <pubDate>2023-10-16 15:17:39 UTC</pubDate>
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         <description><![CDATA[<div><br>Fusion: Hydrogen into helium.<br>Equilibrium: Gravitational pressure = outward radiation.<br>Timeline: Main sequence stars only change when the fuel runs out and they begin their dying stages.&nbsp;</div>]]></description>
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         <pubDate>2023-10-16 15:18:45 UTC</pubDate>
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         <title>Sun</title>
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         <pubDate>2023-10-16 15:21:06 UTC</pubDate>
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         <title>Tau Ceti</title>
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         <pubDate>2023-10-16 15:21:41 UTC</pubDate>
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         <title>Alpha Centauri A</title>
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         <pubDate>2023-10-16 15:22:24 UTC</pubDate>
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         <description><![CDATA[<div>92% Hydrogen<br>7% Helium<br>1% Heavier Elements</div>]]></description>
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         <pubDate>2023-10-16 15:25:35 UTC</pubDate>
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         <pubDate>2023-10-16 15:26:04 UTC</pubDate>
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         <title></title>
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         <pubDate>2023-10-16 20:06:47 UTC</pubDate>
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         <title>Respond with what you learned from the lesson here. </title>
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         <pubDate>2023-10-17 17:30:47 UTC</pubDate>
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         <title>Additional Notes</title>
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         <pubDate>2023-10-17 17:31:22 UTC</pubDate>
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         <title>If the main sequence is a stage for stars, then does that mean all stars go through it?</title>
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         <pubDate>2023-10-17 17:31:49 UTC</pubDate>
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         <title>Additionally, what stages will a star go through before and after the main sequence?</title>
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         <pubDate>2023-10-17 17:32:07 UTC</pubDate>
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