Difference between revisions of "April 9, 2004"

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=Copernicus on the Limb=
 
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      <td width="50%"><h2 align="left">Copernicus on the Limb</h2></td>
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  <td width="50%"><h2 align="right">April  9, 2004</h2></td>
 
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<IMG SRC="images/LPOD-2004-04-09.jpeg" NAME="main_image" width="574" height="423" border="0"></div>
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[[File:LPOD-2004-04-09.jpeg|LPOD-2004-04-09.jpeg]]</div>
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      <td><div align="center" span class="main_sm">Image Credit:  <a class="one" HREF="mailto:fmallmann@free.fr">Frederic Mallmann</A> and Apollo 17</div></td>
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<td><div align="center"><p>Image Credit:  [mailto:fmallmann@free.fr Frederic Mallmann]</p></div></td>
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<p class="story" align="center"><b>Copernicus on the Limb </b></p>
  <p class="story" align="center"><b>Copernicus on the Limb </b></p>
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<p class="story" align="left">        Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact
 
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crater formation is so immense, craters of similar size and freshness look pretty much alike. For example,
  <p class="story" align="left">        Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact
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consider these two behemoths. The bottom crater is Copernicus, 93 km wide and famous for its great location for
        crater formation is so immense, craters of similar size and freshness look pretty much alike. For example,
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viewing from Earth. The top image is Housen, 167 km wide and hardly seen at all because its right on the
        consider these two behemoths. The bottom crater is Copernicus, 93 km wide and famous for its great location for
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southwest limb beyond Bailly. Despite the difference in diameters the craters look very similar - both have
        viewing from Earth. The top image is Housen, 167 km wide and hardly seen at all because its right on the
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scarped walls with terraces that step down to the flat floor, which littered with central mountains. Fresh
        southwest limb beyond Bailly. Despite the difference in diameters the craters look very similar - both have
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impact craters from 40 km in diameter to about 200 km look pretty similar. At larger sizes there is a transition
        scarped walls with terraces that step down to the flat floor, which littered with central mountains. Fresh
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to peak ring craters and then multi-ring basins.  </p>
        impact craters from 40 km in diameter to about 200 km look pretty similar. At larger sizes there is a transition
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<blockquote>
        to peak ring craters and then multi-ring basins.  </p>
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<p align="right" class="story">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</p>
  <blockquote>
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</blockquote>  <p><b>Technical Details:</b><br>
    <p align="right" class="story">&#8212; [mailto:chuck@observingthesky.org Chuck Wood]</p>
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This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope
  </blockquote>  <p><b>Technical Details:</b><br>
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at Ludiver Observatory in northern France on 19 Oct. 2003. The telescope worked at f/16 and infrared
 
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filter was used. A ToUcam was used with 1/25 s exposures and the best 400 of 2700 images were used.
                      This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope
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Full details here:[http://fmallmann.free.fr/dethaus.html http://fmallmann.free.fr/dethaus.html] </p>
                    at Ludiver Observatory in northern France on 19 Oct. 2003. The telescope worked at f/16 and infrared
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<p>The Copernicus shot (bottom) was made with more
                    filter was used. A ToUcam was used with 1/25 s exposures and the best 400 of 2700 images were used.
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expensive equipment: Apollo 17. </p>
                    Full details here:[http://fmallmann.free.fr/dethaus.html http://fmallmann.free.fr/dethaus.html] </p>
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<p class="story"><b>Related Links:</b><br>  
  <p>The Copernicus shot (bottom) was made with more
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[http://fmallmann.free.fr/ Mallmann Web Page]<br>
                    expensive equipment: Apollo 17. </p>
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[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_193_h2.jpg Lunar Orbiter IV View]</p>
  <p class"story"><b>Related Links:</b><br>  
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<p><b>Yesterday's LPOD:</b> [[April 8, 2004|Sneaky Schneckenberg]] </p>
[http://fmallmann.free.fr/ Mallmann Web Page]<br>
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<p><b>Tomorrow's LPOD:</b> [[April 10, 2004|Another Farside View]] </p>
[http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_193_h2.jpg Lunar Orbiter IV View]</p>
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</td>
 
 
  <p class"story"> <b>Tomorrow's LPOD:</b> Another Farside View</p>
 
 
 
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<p align="center" class="main_titles"><b>Author & Editor:</b><br>
  <p align="center" class="main_titles"><b>Author & Editor:</b><br>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
      [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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<!-- Cleanup of credits -->
      <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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<!-- Cleanup of credits -->
      <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
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<!-- Cleanup of credits -->
      <p align="center" class="main_titles"><b>A service of:</b><br>
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<!-- Cleanup of credits -->
      <a class="one" href="http://www.observingthesky.org/">ObservingTheSky.Org</a></p>
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<!-- Cleanup of credits -->
      <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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<!-- Cleanup of credits -->
      <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>
  <p>&nbsp;</p>
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Latest revision as of 19:15, 7 February 2015

Copernicus on the Limb

LPOD-2004-04-09.jpeg

Image Credit: Frederic Mallmann

Copernicus on the Limb

Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact crater formation is so immense, craters of similar size and freshness look pretty much alike. For example, consider these two behemoths. The bottom crater is Copernicus, 93 km wide and famous for its great location for viewing from Earth. The top image is Housen, 167 km wide and hardly seen at all because its right on the southwest limb beyond Bailly. Despite the difference in diameters the craters look very similar - both have scarped walls with terraces that step down to the flat floor, which littered with central mountains. Fresh impact craters from 40 km in diameter to about 200 km look pretty similar. At larger sizes there is a transition to peak ring craters and then multi-ring basins.

Chuck Wood

Technical Details:

This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope at Ludiver Observatory in northern France on 19 Oct. 2003. The telescope worked at f/16 and infrared filter was used. A ToUcam was used with 1/25 s exposures and the best 400 of 2700 images were used.

Full details here:http://fmallmann.free.fr/dethaus.html

The Copernicus shot (bottom) was made with more expensive equipment: Apollo 17.

Related Links:
Mallmann Web Page
Lunar Orbiter IV View

Yesterday's LPOD: Sneaky Schneckenberg

Tomorrow's LPOD: Another Farside View


Author & Editor:
Charles A. Wood

 


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