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      <title>Stars by Adrian Lampos</title>
      <link>https://padlet.com/adrianl16/Bookmarks</link>
      <description></description>
      <language>en-us</language>
      <pubDate>2022-06-13 02:29:45 UTC</pubDate>
      <lastBuildDate>2023-06-14 05:32:15 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title>RIGEL RAAUUGGHHH</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623037221</link>
         <description><![CDATA[<div>Rigel is a silly little star from the Orion constellation. It's a blue supergiant star and is one of the brightest star in the night sky.</div>]]></description>
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         <pubDate>2023-06-14 05:04:53 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623037221</guid>
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      <item>
         <title>BETELGEUSE!!!!!!</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623039426</link>
         <description><![CDATA[<div>I HAVE LIEK AN ESSAY ABOUT IT JSUT WAIT</div>]]></description>
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         <pubDate>2023-06-14 05:07:00 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623039426</guid>
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      <item>
         <title>Jesse</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623042815</link>
         <description><![CDATA[<div>Antares is the brightest star in the constellation of Scorpius. It has the Bayer designation α Scorpii, which is Latinised to Alpha Scorpii. Often referred to as "the heart of the scorpion"</div>]]></description>
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         <pubDate>2023-06-14 05:10:18 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623042815</guid>
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      <item>
         <title>B-type main-sequence star </title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623042903</link>
         <description><![CDATA[<div>A <strong>B-type main-sequence star</strong> (B V) is a <a href="https://en.wikipedia.org/wiki/Main_sequence">main-sequence</a> (<a href="https://en.wikipedia.org/wiki/Hydrogen">hydrogen</a>-burning) <a href="https://en.wikipedia.org/wiki/Star">star</a> of <a href="https://en.wikipedia.org/wiki/Stellar_classification#Type_B">spectral type B</a> and luminosity class V. These stars have from 2 to 16 times the <a href="https://en.wikipedia.org/wiki/Solar_mass">mass</a> of the <a href="https://en.wikipedia.org/wiki/Sun">Sun</a> and <a href="https://en.wikipedia.org/wiki/Effective_temperature">surface temperatures</a> between 10,000 and 30,000 <a href="https://en.wikipedia.org/wiki/Kelvin">K</a>.<a href="https://en.wikipedia.org/wiki/B-type_main-sequence_star#cite_note-1"><sup>[1]</sup></a> B-type stars are extremely luminous and blue.-EJ</div>]]></description>
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         <pubDate>2023-06-14 05:10:23 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623042903</guid>
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      <item>
         <title>KIM DOKJA.</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623043673</link>
         <description><![CDATA[<div>i choose this one becuase someone bought it and named it after my favorite novel character,i have no other detials about it-RJ<br><br></div>]]></description>
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         <pubDate>2023-06-14 05:11:11 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623043673</guid>
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      <item>
         <title>White Dwarf </title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623044906</link>
         <description><![CDATA[<div>A <strong>white dwarf</strong> is a <a href="https://en.wikipedia.org/wiki/Compact_star">stellar core remnant</a> composed mostly of <a href="https://en.wikipedia.org/wiki/Electron-degenerate_matter">electron-degenerate matter</a>. A white dwarf is very <a href="https://en.wikipedia.org/wiki/Density">dense</a>: its mass is comparable to the <a href="https://en.wikipedia.org/wiki/Sun">Sun</a>'s, while its volume is comparable to the <a href="https://en.wikipedia.org/wiki/Earth">Earth</a>'s. A white dwarf's low <a href="https://en.wikipedia.org/wiki/Luminosity">luminosity</a> comes from the <a href="https://en.wikipedia.org/wiki/Thermal_radiation">emission</a> of residual <a href="https://en.wikipedia.org/wiki/Heat">thermal energy</a>; no fusion takes place in a white dwarf.<br><br>White dwarfs are thought to be the final <a href="https://en.wikipedia.org/wiki/Stellar_evolution">evolutionary state</a> of stars whose <a href="https://en.wikipedia.org/wiki/Mass">mass</a> is not high enough to become a <a href="https://en.wikipedia.org/wiki/Neutron_star">neutron star</a> or <a href="https://en.wikipedia.org/wiki/Black_hole">black hole</a>. This includes over 97% of the stars in the <a href="https://en.wikipedia.org/wiki/Milky_Way">Milky Way</a>.<a href="https://en.wikipedia.org/wiki/White_dwarf#cite_note-cosmochronology-4"><sup>[4]</sup></a><sup>: §1 </sup>&nbsp;After the <a href="https://en.wikipedia.org/wiki/Hydrogen">hydrogen</a>-<a href="https://en.wikipedia.org/wiki/Stellar_nucleosynthesis">fusing</a> period of a <a href="https://en.wikipedia.org/wiki/Main_sequence">main-sequence star</a> of low or medium mass ends, such a star will expand to a <a href="https://en.wikipedia.org/wiki/Red_giant">red giant</a> during which it fuses <a href="https://en.wikipedia.org/wiki/Helium">helium</a> to <a href="https://en.wikipedia.org/wiki/Carbon">carbon</a> and <a href="https://en.wikipedia.org/wiki/Oxygen">oxygen</a> in its core by the <a href="https://en.wikipedia.org/wiki/Triple-alpha_process">triple-alpha process</a>. If a red giant has insufficient mass to generate the core temperatures required to fuse carbon (around 1 <a href="https://en.wikipedia.org/wiki/Billion">billion</a> K), an inert mass of carbon and oxygen will build up at its center.</div>]]></description>
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         <pubDate>2023-06-14 05:12:33 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623044906</guid>
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      <item>
         <title>Polaris</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623051226</link>
         <description><![CDATA[<div><strong>Polaris</strong> is a star in the northern circumpolar<a href="https://en.wikipedia.org/wiki/Circumpolar_constellation"> </a>constellation of Ursa Minor. and is commonly called the <strong>North Star</strong> or <strong>Pole Star</strong>. -Nathan</div>]]></description>
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         <pubDate>2023-06-14 05:19:10 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623051226</guid>
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      <item>
         <title>Proxima Centauri</title>
         <author></author>
         <link>https://padlet.com/adrianl16/Bookmarks/wish/2623062134</link>
         <description><![CDATA[<div><br>Proxima Centauri is a small, low mass star located around 4.25 light years away from the Sun.<br>It is a red dwarf star that is part of a trinary star system (with Alpha Centauri A and B). The star has around 12.5% mass and about 14% diameter of the Sun. Unfortunately, the exoplanets that orbit these stars are not habitable because of the dangerous UV radiation from the stars. Proxima Centauri is also part of the Centaurus constellation. Although it looks bright from the view of telescopes, Proxima Centauri is not visible to the naked eye.<br><br><br></div>]]></description>
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         <pubDate>2023-06-14 05:31:13 UTC</pubDate>
         <guid>https://padlet.com/adrianl16/Bookmarks/wish/2623062134</guid>
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