Difference between revisions of "May 12, 2004"

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=A Basin Near Schiller=
 
=A Basin Near Schiller=
 
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          <td><h2 align="left"><span class="class">A Basin Near Schiller</span></h2></td>
 
          <td><h2 align="right">May 12, 2004</h2></td>
 
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[[File:LPOD-2004-05-12.jpeg|LPOD-2004-05-12.jpeg]]]
 
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<p class="main_sm">Image Credit: [http://www.lpi.usra.edu/research/cla/info/h21/ Consolidated Lunar Atlas Sheet H21]</p>
            <p class="main_sm">Image Credit: <a class="one" href="http://www.lpi.usra.edu/research/cla/info/h21/">Consolidated Lunar Atlas Sheet H21</a></p>
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<td><p class="Story" align="center"><b><span class="class">A Basin Near Schiller</span></b></p>
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<p class="story" align="left">How many times have you observed the weirdly elongated crater Schiller, or looked past Phocylides to find Wargentin, or beyond Zucchius to see Bailly? Did you ever notice the relatively smooth-surface between these other craters? Did you notice the horse-shoe shaped mountainous rim that arcs around from Schiller C to Segner, past Weigel B to Schiller S? Don't know where those craters are? Mouse over the image to find them. Did you notice the worn down scarp that stretches from Phocylides to Zucchius to Rost and finally Schiller? If you didn't notice those rim segments before don't feel bad - no one else did until the early 1960s when Bill Hartmann and Gerard Kuiper included this Basin near Schiller in their list of multi-ring impact basins. The mouseover image shows the two main rings of this basin and a dashed circle outlines a possible inner ring that seems to be a slight depression surrounded by an indistinct ridge. Thus, the Basin Near Schiller (or the Schiller-Zucchius Basin as the USGS renamed it) is a three ring basin with diameters of 335, 175 and 85 km. If you look at this area under full Moon conditions you will see that the smooth material isn't dark like a mare. But the smoothness and the mare-like ridges suggest that it is mare lavas veneered by light-hued ejecta. Multi-ring basins were the largest craters formed on the Moon - and some of the earliest. And now you know that they may be lurking undetected anywhere. </p>
          <td><p class="Story" align="center"><b><span class="class">A Basin Near Schiller</span></b></p>
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<p class="story"><b>Related Links:</b><br>
              <p class="story" align="left">How many times have you observed the weirdly elongated crater Schiller, or looked past Phocylides to find Wargentin, or beyond Zucchius to see Bailly? Did you ever notice the relatively smooth-surface between these other craters? Did you notice the horse-shoe shaped mountainous rim that arcs around from Schiller C to Segner, past Weigel B to Schiller S? Don't know where those craters are? Mouse over the image to find them. Did you notice the worn down scarp that stretches from Phocylides to Zucchius to Rost and finally Schiller? If you didn't notice those rim segments before don't feel bad - no one else did until the early 1960s when Bill Hartmann and Gerard Kuiper included this Basin near Schiller in their list of multi-ring impact basins. The mouseover image shows the two main rings of this basin and a dashed circle outlines a possible inner ring that seems to be a slight depression surrounded by an indistinct ridge. Thus, the Basin Near Schiller (or the Schiller-Zucchius Basin as the USGS renamed it) is a three ring basin with diameters of 335, 175 and 85 km. If you look at this area under full Moon conditions you will see that the smooth material isn't dark like a mare. But the smoothness and the mare-like ridges suggest that it is mare lavas veneered by light-hued ejecta. Multi-ring basins were the largest craters formed on the Moon - and some of the earliest. And now you know that they may be lurking undetected anywhere. </p>
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[http://www.lpi.usra.edu/research/lunar_orbiter/bin/info.shtml?436 Lunar Orbiter IV View  ]</p>
              <p class"story"><b>Related Links:</b><br>
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<p class="story"><b>Tomorrow's LPOD:</b> A New/Old Catalog of Lunar Craters</p>
              [http://www.lpi.usra.edu/research/lunar_orbiter/bin/info.shtml?436 Lunar Orbiter IV View  ]</p>
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</tr>
              <p class"story"><b>Tomorrow's LPOD:</b> A New/Old Catalog of Lunar Craters</p>
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</table>       
              <p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p></td>
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<hr>
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<p align="center" class="main_titles"><b>Author & Editor:</b><br>
      </table>       
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
      <hr width="640">
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
      <p align="center" class="main_titles"><b>Author & Editor:</b><br>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
          [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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<p align="center" class="main_titles"><b>A service of:</b><br>
      <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
          [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
      <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
      <p align="center" class="main_titles"><b>A service of:</b><br>
 
          <a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a></p>
 
      <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
 
          <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>
 
 
 
 
<p>&nbsp;</p>
 
<p>&nbsp;</p>
 
 
 
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===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
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Revision as of 18:20, 4 January 2015

A Basin Near Schiller

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A Basin Near Schiller

How many times have you observed the weirdly elongated crater Schiller, or looked past Phocylides to find Wargentin, or beyond Zucchius to see Bailly? Did you ever notice the relatively smooth-surface between these other craters? Did you notice the horse-shoe shaped mountainous rim that arcs around from Schiller C to Segner, past Weigel B to Schiller S? Don't know where those craters are? Mouse over the image to find them. Did you notice the worn down scarp that stretches from Phocylides to Zucchius to Rost and finally Schiller? If you didn't notice those rim segments before don't feel bad - no one else did until the early 1960s when Bill Hartmann and Gerard Kuiper included this Basin near Schiller in their list of multi-ring impact basins. The mouseover image shows the two main rings of this basin and a dashed circle outlines a possible inner ring that seems to be a slight depression surrounded by an indistinct ridge. Thus, the Basin Near Schiller (or the Schiller-Zucchius Basin as the USGS renamed it) is a three ring basin with diameters of 335, 175 and 85 km. If you look at this area under full Moon conditions you will see that the smooth material isn't dark like a mare. But the smoothness and the mare-like ridges suggest that it is mare lavas veneered by light-hued ejecta. Multi-ring basins were the largest craters formed on the Moon - and some of the earliest. And now you know that they may be lurking undetected anywhere.

Related Links:
Lunar Orbiter IV View

Tomorrow's LPOD: A New/Old Catalog of Lunar Craters


Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

A service of:
ObservingTheSky.Org

Visit these other PODs:
Astronomy | Mars | Earth

 


COMMENTS?

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