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      <title>Venus- Noah Muniz by Noah Muniz</title>
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      <description>The Planet</description>
      <language>en-us</language>
      <pubDate>2019-12-11 16:44:33 UTC</pubDate>
      <lastBuildDate>2019-12-11 18:56:01 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title>Characteristics</title>
         <author>55868</author>
         <link>https://padlet.com/55868/oom372waw75i/wish/422830297</link>
         <description><![CDATA[<div><strong>Second planet from the sun, 108 million km from the Sun, rotates backwards- clockwise unlike all other planets<br>turns backwards on it's axis<br>225 Earth days is a year for Venus, it takes 243 Earth days for one day to pass on Venus<br>Radius is 6.052 km (95% size of Earth)<br>Volume is 86% of Earth<br>Mass is 4.87 x 10^ 24 kg (82% mass of Earth)<br>90% gravity of Earth<br>Surface temperature is 462 C, hot enough to melt lead<br>Often called Earth's twin for being so similar to the planet<br>Much fewer craters then other planets, 300-500 million years ago an event erased all present craters at that time<br>Smooth volcanic plains, many extinct volcanic peaks and impact craters<br>No moons, No rings</strong></div>]]></description>
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         <pubDate>2019-12-11 16:51:10 UTC</pubDate>
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         <title>Structure of Venus</title>
         <author>55868</author>
         <link>https://padlet.com/55868/oom372waw75i/wish/422841461</link>
         <description><![CDATA[<div><strong>Crust- 10 to 50 kilometers thick crush, made up of silicate rock<br>Mantel- thought to be 3,000 km thick, composition is unknown<br>Core- 2,900 km radius, external core made of liquid iron and Nickle, internal core made of solid iron and Nickle<br>Earth and Venus have a similar internal structure but scientist are not certain about this<br>Average density is 5.25g/cm3<br></strong><br></div>]]></description>
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         <pubDate>2019-12-11 17:06:57 UTC</pubDate>
         <guid>https://padlet.com/55868/oom372waw75i/wish/422841461</guid>
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      <item>
         <title>Atmosphere</title>
         <author>55868</author>
         <link>https://padlet.com/55868/oom372waw75i/wish/422849123</link>
         <description><![CDATA[<div><strong>96.5% Carbon Dioxide<br>3.5% of Nitrogen<br>Trace amounts of other gases, sulfur dioxide, water vapor<br>No water on the surface of the planet<br>Atmosphere Pressure is 92 times that of Earth<br>Greenhouse gases boiled away all water that might have once been there<br>Lack of magnetic field<br>Hydrogen blown away by solar flares from the Sun<br>Has no way to cool down<br></strong><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2019-12-11 17:18:36 UTC</pubDate>
         <guid>https://padlet.com/55868/oom372waw75i/wish/422849123</guid>
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      <item>
         <title>How do we study Venus?</title>
         <author>55868</author>
         <link>https://padlet.com/55868/oom372waw75i/wish/422855566</link>
         <description><![CDATA[<div><strong>Goldstone Solar System Radar in California sent radar waves to Venus to study the surface<br>Spacecrafts have landed on Venus, such as Venera 13 which took colored pictured<br>Spacecrafts sent to orbit around the planet using radar to study it<br>Analyzing infrared radiation that comes from the planet is another way we have learned about the planet<br>Some scientist  that worked on Venus are Carl Sagan, Galileo,  and others</strong></div>]]></description>
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         <pubDate>2019-12-11 17:28:19 UTC</pubDate>
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