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      <title>the 3 main tapes of galaxy&#39;s  by milagros gonzalez</title>
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      <description>Made with a quick smile</description>
      <language>en-us</language>
      <pubDate>2021-04-15 20:17:55 UTC</pubDate>
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         <title>spiral galaxy</title>
         <author>s1786003</author>
         <link>https://padlet.com/s1812520/i2h2kshjh2k8y2uq/wish/1423021467</link>
         <description><![CDATA[<div>Astronomers believe that <strong>galaxies</strong> have <strong>spiral</strong> arms because <strong>galaxies</strong> rotate – or spin around a central axis – and because of something called “density waves.” ... A <strong>spiral galaxy's</strong> rotation, or spin, bends the waves into <strong>spirals</strong>. Stars pass through the wave as they orbit the <strong>galaxy</strong> center.<strong><mark> milagros gonzalez</mark></strong></div>]]></description>
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         <pubDate>2021-04-15 20:23:00 UTC</pubDate>
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         <title>Elliptical galaxy </title>
         <author>s1754467</author>
         <link>https://padlet.com/s1812520/i2h2kshjh2k8y2uq/wish/1423024958</link>
         <description><![CDATA[<div>An <strong>elliptical galaxy</strong> is a type of <strong>galaxy</strong> with an approximately ellipsoidal shape and a smooth, nearly featureless image. They are one of the three main classes of <strong>galaxy</strong> described by Edwin Hubble in his Hubble sequence and 1936 work The Realm of the Nebulae, along with spiral and lenticular <strong>galaxies</strong>. <br><strong><mark>Dalilah Jimenez&nbsp;</mark></strong></div>]]></description>
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         <pubDate>2021-04-15 20:24:09 UTC</pubDate>
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         <title>Irregular Galaxy</title>
         <author>s1786003</author>
         <link>https://padlet.com/s1812520/i2h2kshjh2k8y2uq/wish/1423034853</link>
         <description><![CDATA[<div>An <strong>irregular galaxy</strong> is a <strong>galaxy</strong> that does not have a distinct regular shape, unlike a spiral or an elliptical <strong>galaxy</strong>.&nbsp; Example:&nbsp; Irregular galaxies are the Small and <strong>Large Magellanic clouds</strong>. These are companion galaxies to our own <strong>Milky Way</strong>, and can be easily seen at dark sites in the Southern Hemisphere. <strong><mark>BY JOHAN</mark></strong></div>]]></description>
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         <pubDate>2021-04-15 20:27:21 UTC</pubDate>
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         <title>Spiral Description</title>
         <author>s1772004</author>
         <link>https://padlet.com/s1812520/i2h2kshjh2k8y2uq/wish/1423057000</link>
         <description><![CDATA[<div>Spiral galaxies form a class of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae and, as such, form part of the Hubble sequence. Most spiral galaxies consist of a flat, rotating disk containing stars, gas and dust, and a central concentration of stars known as the bulge.<mark>Daquarius King</mark>&nbsp;</div>]]></description>
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         <pubDate>2021-04-15 20:35:02 UTC</pubDate>
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         <title>Lenticular Galaxy </title>
         <author>s1798113</author>
         <link>https://padlet.com/s1812520/i2h2kshjh2k8y2uq/wish/1423064578</link>
         <description><![CDATA[<div>A lenticular galaxy is a type of galaxy intermediate between an elliptical and a spiral galaxy in galaxy morphological classification schemes. It contains a large-scale disc but does not have large-scale spiral arms. By<mark> Victor Lopez</mark></div>]]></description>
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         <pubDate>2021-04-15 20:37:47 UTC</pubDate>
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