Difference between revisions of "May 9, 2004"

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=The Crater Formerly Known As Prinz=
 
=The Crater Formerly Known As Prinz=
  
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          <td><h2 align="left"><span class="class">The Crater Formerly Known As Prinz</span></h2></td>
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          <td><h2 align="right">May 9, 2004</h2></td>
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          <td><div align="center"><IMG SRC="images/LPOD-2004-05-09.jpeg" NAME="main_image" border="0"></div></td>
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            <p class="main_sm">Image Credit: [mailto:kcpaulhk@yahoo.com.hk K.C. Pau]</p>
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          <td><p class="Story" align="center"><b><span class="class">The Crater Formerly Known As Prinz</span></b></p>
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              <p class="story" align="left">Well, it actually still is known as Prinz. I can't say much about the crater itself - its a 47 km wide crater with a completely mare-flooded interior. The north rim of the crater rises a kilometer above the mare surface, but most of the southern rim is gone. Where did it go? The fact that the rim height smoothly decreases from north to south suggests that the crater either formed on a slope or, more likely, the terrain to the south subsided after Prinz formed. But I don't know why the south would subside, so perhaps the north has been uplifted. According to the topo contours in the Times Atlas of the Moon the high spot of this area is just north of Prinz, which is the source area for sinuous rilles beautifully captured in K.C. Pau's image. Rilles flow downslope, providing further evidence that the area immediately north of Prinz is high. I speculate that the magma that rose near the surface to feed the rilles also domed up the north side of Prinz. Piling speculation on speculation, the uplift also brought up portions of the rim of the Imbrium basin, which are the peaks visible on the upper right side of the image - the Harbinger Mountains! Maybe the Prinz uplift is a smaller and less structured version of the nearby Aristarchus Plateau uplift.</p>
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              <p class="story" align="left"><b>Technical Details</b>:<br>
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              May 1, 2004. 10&quot; f/6 Newtonian + 5X Barlow + Phillips Toucam Pro; 114 stacked frames.</p>
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              <p class"story"><b>Related Links:</b><br>
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              [http://nssdc.gsfc.nasa.gov/imgcat/html/object_page/a15_m_2606.html Apollo 15 View]</p>
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              <p class"story"><b>Tomorrow's LPOD:</b> Galileo's Colorful Moon</p>
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              <p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p></td>
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      <p align="center" class="main_titles"><b>Author & Editor:</b><br>
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          [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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      <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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          [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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      <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
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      <p align="center" class="main_titles"><b>A service of:</b><br>
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          <a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a></p>
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      <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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          <a class="one" href="http://antwrp.gsfc.nasa.gov/apod/astropix.html">Astronomy</a> | <a class="one" href="http://www.msss.com/">Mars</a> | <a class="one" href="http://epod.usra.edu/">Earth</a></p>
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<p>&nbsp;</p>
  
  

Revision as of 15:38, 4 January 2015

The Crater Formerly Known As Prinz

The Crater Formerly Known As Prinz

May 9, 2004

<IMG SRC="images/LPOD-2004-05-09.jpeg" NAME="main_image" border="0">

Image Credit: K.C. Pau

The Crater Formerly Known As Prinz

Well, it actually still is known as Prinz. I can't say much about the crater itself - its a 47 km wide crater with a completely mare-flooded interior. The north rim of the crater rises a kilometer above the mare surface, but most of the southern rim is gone. Where did it go? The fact that the rim height smoothly decreases from north to south suggests that the crater either formed on a slope or, more likely, the terrain to the south subsided after Prinz formed. But I don't know why the south would subside, so perhaps the north has been uplifted. According to the topo contours in the Times Atlas of the Moon the high spot of this area is just north of Prinz, which is the source area for sinuous rilles beautifully captured in K.C. Pau's image. Rilles flow downslope, providing further evidence that the area immediately north of Prinz is high. I speculate that the magma that rose near the surface to feed the rilles also domed up the north side of Prinz. Piling speculation on speculation, the uplift also brought up portions of the rim of the Imbrium basin, which are the peaks visible on the upper right side of the image - the Harbinger Mountains! Maybe the Prinz uplift is a smaller and less structured version of the nearby Aristarchus Plateau uplift.

Technical Details:
May 1, 2004. 10" f/6 Newtonian + 5X Barlow + Phillips Toucam Pro; 114 stacked frames.

Related Links:
Apollo 15 View

Tomorrow's LPOD: Galileo's Colorful Moon

<img src="../../../MainPage/spacer.gif" width="640" height="1">


Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Webmaster

A service of:
<a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a>

Visit these other PODs:
<a class="one" href="http://antwrp.gsfc.nasa.gov/apod/astropix.html">Astronomy</a> | <a class="one" href="http://www.msss.com/">Mars</a> | <a class="one" href="http://epod.usra.edu/">Earth</a>

 



COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.