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      <title>Tectonic processes of Pluto by Michael Porteous</title>
      <link>https://padlet.com/mickester12/ucl9dw2jpq1o</link>
      <description>evidence for plate activity</description>
      <language>en-us</language>
      <pubDate>2019-04-04 20:37:07 UTC</pubDate>
      <lastBuildDate>2026-01-15 16:12:07 UTC</lastBuildDate>
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         <title>Tectonics</title>
         <author>mickester12</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348725617</link>
         <description><![CDATA[<div>Currently there is some evidence that the only tectonic activity on Pluto is extensional tectonics, driven by surface expansion caused by partial freezing of an ocean below the surface. However, there is some evidence of ancient plate tectonics, as valleys, mountain ranges (3500m high), and faults have formed. ( <em>JEFFREY M. MOORE, WILLIAM B. MCKINNON)  </em></div>]]></description>
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         <pubDate>2019-04-04 20:46:34 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348725617</guid>
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         <title></title>
         <author>davse382</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348726405</link>
         <description><![CDATA[]]></description>
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         <pubDate>2019-04-04 20:49:55 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348726405</guid>
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         <title>Sub-surface ocean</title>
         <author>mickester12</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348727700</link>
         <description><![CDATA[<div>it is one theory that the Ocean beneath Pluto's surface was formed during the collision event that formed both Pluto and its primary moon Charon. the collision caused a super-heated radioactive core to form, and melted most of the water-ice. since there is little evidence of recent compression tectonics, it can be assumed that the ocean has yet to freeze completely. ( <a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Hammond%2C+N+P"><em>Noah P. Hammond</em></a><em>, </em><a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Barr%2C+A+C"><em>Amy C. Barr</em></a><em>, </em><a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Parmentier%2C+E+M"><em>Edgar M. Parmentier</em></a><em>)</em> </div>]]></description>
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         <pubDate>2019-04-04 20:55:51 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348727700</guid>
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         <title>Charon - Moon</title>
         <author>davse382</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348727709</link>
         <description><![CDATA[<div>*Young surface<br>*Geologically active - landslides, mountains<br>*Evidence of plate tectonics<br>*Driven by freezing ice core that expanded and cracked the crust<br><br></div>]]></description>
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         <pubDate>2019-04-04 20:55:54 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348727709</guid>
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         <title>References</title>
         <author>mickester12</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348729970</link>
         <description><![CDATA[<div><br></div><ul><li>The geology of Pluto and Charon through the eyes of New Horizons, <strong>BY JEFFREY M. MOORE, WILLIAM B. MCKINNON</strong> </li><li><h1>Recent Tectonic Activity on Pluto Driven by Phase Changes in the Ice Shell, <a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Hammond%2C+N+P">Noah P. Hammond</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Barr%2C+A+C">Amy C. Barr</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&amp;query=Parmentier%2C+E+M">Edgar M. Parmentier</a> </h1></li><li>O'Rourke, J. (2014) <a href="http://www.planetary.org/blogs/guest-blogs/2014/0526-will-we-find-signs-of-tectonics-on-pluto.html">http://www.planetary.org/blogs/guest-blogs/2014/0526-will-we-find-signs-of-tectonics-on-pluto.html</a></li><li><a href="https://solarsystem.nasa.gov/planets/dwarf-planets/pluto/overview/">https://solarsystem.nasa.gov/planets/dwarf-planets/pluto/overview/</a></li></ul>]]></description>
         <enclosure url="" />
         <pubDate>2019-04-04 21:05:16 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348729970</guid>
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         <title>Simplified model of Pluto&#39;s interior</title>
         <author>davse382</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348730431</link>
         <description><![CDATA[<div> A) Solid, icy crust, a liquid ocean, and a rocky core. B) Solid, icy crust directly above a rocky core. C) Uniform-density interior comprised of a homogenous ice/rock mixture.  (Planetary.org, 2014)</div>]]></description>
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         <pubDate>2019-04-04 21:07:24 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348730431</guid>
      </item>
      <item>
         <title>Pluto Interior and Exterior</title>
         <author>davse382</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348731628</link>
         <description><![CDATA[<div>*Has a surface temperature of roughly -225C<br>*Atmosphere is composed of methane and nitrogen<br>*Diameter is 2370km across<br>*Interior composed of 70% rock and 30% water/ice</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-04-04 21:12:58 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348731628</guid>
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      <item>
         <title></title>
         <author>mickester12</author>
         <link>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348737048</link>
         <description><![CDATA[
Made with magic
Avatar of Michael Porteous
Michael Porteous
 + 1
●
]]></description>
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         <pubDate>2019-04-04 21:39:56 UTC</pubDate>
         <guid>https://padlet.com/mickester12/ucl9dw2jpq1o/wish/348737048</guid>
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