Difference between revisions of "January 7, 2004"

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=Petavius: Rilles & Volcanic Spots=
 
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          <td><h2 align="left">Petavius: Rilles &amp; Volcanic Spots</h2></td>
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[[File:LPOD-2004-01-07.jpeg|LPOD-2004-01-07.jpeg]]
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<span class="main_sm"><b>Image Credit:</b>  
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[mailto:kcpaulhk@yahoo.com.hk KC Pau]</p>
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<span class="main_sm"><b>Image Credit:</b>  
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<A class="one" HREF="mailto:kcpaulhk@yahoo.com.hk">KC Pau</A></p>
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<b>Petavius: Rilles &amp; Volcanic Spots</b></p>
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  <p class="story" align="center">
 
    <b>Petavius: Rilles &amp; Volcanic Spots</b></p>
 
 
 
 
<p class="story">One of the most skillful lunar imagers is Hong Kong amateur KC Pau. His picture of Petavius (Sept 11, 2003, 10" newtonian
 
<p class="story">One of the most skillful lunar imagers is Hong Kong amateur KC Pau. His picture of Petavius (Sept 11, 2003, 10" newtonian
 
and Phillips Toucam) reveals details that I have never seen on any Earth-based photo, nor on the best Lunar Orbiter image!  
 
and Phillips Toucam) reveals details that I have never seen on any Earth-based photo, nor on the best Lunar Orbiter image!  
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the red of pyroclastics.</p>
 
the red of pyroclastics.</p>
 
<p><b>Related Links:</b>
 
<p><b>Related Links:</b>
    <br>
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    More [http://observingthesky.org/index.php?p=174 KC Pau]</p>
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More [http://observingthesky.org/index.php?p=174 KC Pau]</p>
  <p><b>Tomorrow's LPOD:</b> The Right Stuff in Lunar Science</p>
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<p><b>Tomorrow's LPOD:</b> The Right Stuff in Lunar Science</p>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>
      <p></p>
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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>
      <p align="center" class="main_titles"><b>Author &amp; 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>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></p>
      <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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<p align="center" class="main_titles"><b>A service of:</b><br>
          [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
      <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>Visit these other PODs:</b> <br>
      <p align="center" class="main_titles"><b>A service of:</b><br>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
          <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?===  
 
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Revision as of 17:08, 4 January 2015

Petavius: Rilles & Volcanic Spots

LPOD-2004-01-07.jpeg
Image Credit:

KC Pau

Petavius: Rilles & Volcanic Spots

One of the most skillful lunar imagers is Hong Kong amateur KC Pau. His picture of Petavius (Sept 11, 2003, 10" newtonian and Phillips Toucam) reveals details that I have never seen on any Earth-based photo, nor on the best Lunar Orbiter image! The 177 km wide Petavius is an older, degraded version of nearby Langrenus. The most fascinating feature of Petavius, apparently unique on the Moon, is the sharply defined rill that slices the crater floor, from the central peak to the southwest wall. Other rilles radiate away from the peaks, and two rille segments - shown to be continuous on a Lunar Orbiter image - cross the northeastern portion of the floor. Darkish, smooth spots are associated with the northern rilles, and a smooth spot at the southern end of the floor is now revealed for the first time to be associated with a shallow, pitted dome. Are the smooth patches volcanic pyroclastic (ash) deposits or mare lava flows? High Sun views show that the patches are as dark as mare lavas, but multi-spectral Clementine images show neither the blue of fresh mare material, nor the red of pyroclastics.

Related Links:
More KC Pau

Tomorrow's LPOD: The Right Stuff in Lunar Science


Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Webmaster

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.