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      <title>Astronomy 1 by Johanna Tirone</title>
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      <description>Made with good vibes</description>
      <language>en-us</language>
      <pubDate>2016-12-07 18:46:54 UTC</pubDate>
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         <title>What is a nebula?</title>
         <author>victoria_stuchell</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142392666</link>
         <description><![CDATA[<div>A nebula is a cloud of gas and dust in space.&nbsp;<br>Ex: Orion's Belt<br><br>Picture from:&nbsp;</div><div>"Orion Nebula." <em>Wikipedia</em>. Wikimedia Foundation, n.d. Web. 10 Dec. 2016.</div>]]></description>
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         <pubDate>2016-12-07 19:01:42 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142392666</guid>
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         <title>What is a Bok Globules? </title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142393670</link>
         <description><![CDATA[<div>Bok Globules are isolated and relatively small dark nebulae<br><br>Picture from: "Thackeray's Globules." <em>Thackeray's Globules</em>. N.p., n.d. Web. 12 Dec. 2016.</div>]]></description>
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         <pubDate>2016-12-07 19:03:53 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142393670</guid>
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         <title>What are Herbig-Haro Objects?</title>
         <author>victoria_stuchell</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142394626</link>
         <description><![CDATA[<div>Herbig-Haro Objects are small nebulae associated with star information that varies irregularly in brightness.   <br><br>Picture from: "Herbig-Haro Object HH 47, a Stellar Jet in Vela." <em>Anne's Astronomy News</em>. N.p., 02 Dec. 2012. Web. 12 Dec. 2016.</div>]]></description>
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         <pubDate>2016-12-07 19:06:17 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142394626</guid>
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         <title>What is  a T- Tauri star?</title>
         <author>johanna_tirone</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142395467</link>
         <description><![CDATA[<div>A T- Tauri star is a young star surrounded by gas and dust contracting toward the main sequence.<br><br>Picture from: "What Is a T Tauri Star? | Space Facts – Astronomy, the Solar System &amp; Outer Space | All About Space Magazine." <em>Space Facts Astronomy the Solar System Outer Space All About Space Magazine</em>. N.p., n.d. Web. 10 Dec. 2016.</div>]]></description>
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         <pubDate>2016-12-07 19:08:34 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142395467</guid>
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      <item>
         <title>What is a Bipolar Flow?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142396357</link>
         <description><![CDATA[<div>Bipolar Flow is matter in two opposite directions from a star. <br><br>Picture from: "Bipolar Outflow." <em>Bipolar Outflow</em>. N.p., n.d. Web. 12 Dec. 2016.</div>]]></description>
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         <pubDate>2016-12-07 19:10:34 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142396357</guid>
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         <title>How do astronomers study the gas and dust between the stars, called the interstellar medium?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142397268</link>
         <description><![CDATA[<div>Some effects of interstellar medium are visible such as interstellar reddening.  Also, astronomers use the absorption spectrum.</div>]]></description>
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         <pubDate>2016-12-07 19:12:49 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142397268</guid>
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         <title>How do stars form in the interstellar medium?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142397913</link>
         <description><![CDATA[<div>Not all clouds of interstellar medium become a star. Temperature, turbulent gas currents, and magnetic fields all have a part in creating the star.</div>]]></description>
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         <pubDate>2016-12-07 19:14:33 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142397913</guid>
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         <title>How do stars maintain stability?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142647050</link>
         <description><![CDATA[<div>Stars keep stability by having an equally balanced relationship between gas, temperature, and pressure.</div>]]></description>
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         <pubDate>2016-12-08 18:38:38 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142647050</guid>
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         <title>How do stars make energy?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142647333</link>
         <description><![CDATA[<div>Stars make energy by burning Hydrogen and turning it into Helium. This causes nuclear fusion.</div>]]></description>
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         <pubDate>2016-12-08 18:39:29 UTC</pubDate>
         <guid>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142647333</guid>
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         <title>How do the luminosities and lifetime of stars depend on their mass?</title>
         <author>danielle_stehle</author>
         <link>https://padlet.com/johanna_tirone/bqevwiltrlia/wish/142647453</link>
         <description><![CDATA[<div>More massive stars must also in turn be more luminous (and make more energy) in order to support their weight. This is the mass-luminosity relationship.</div>]]></description>
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         <pubDate>2016-12-08 18:39:52 UTC</pubDate>
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