Difference between revisions of "February 15, 2004"

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=Volcanic Rump=
 
=Volcanic Rump=
 
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      <td width="50%"><h2 align="left">Volcanic Rump</h2></td>
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  <td width="50%"><h2 align="right">February 15, 2004</h2></td>
 
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<IMG SRC="images/LPOD-2004-02-15.jpeg" NAME="main_image" width="412" height="400" border="0"></div>
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[[File:LPOD-2004-02-15.jpeg|LPOD-2004-02-15.jpeg]]</div>
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      <td><div align="center" span class="main_sm">Image Credit:  Apollo 15 (AS15-97-13252)</div></td>
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<td><div align="center" span class="main_sm">Image Credit:  Apollo 15 (AS15-97-13252)</div></td>
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<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
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<p class="story" align="center"><b>Volcanic Rump </b></p>
  <p class="story" align="center"><b>Volcanic Rump </b></p>
+
<p class="story" align="left">We think of the Apollo missions as being near equatorial - and the landing sites were - but the sinusoidal orbit  
 
+
of the Command Modules took them as much as 25 degrees from the equator. And by pointing a handheld Hasselblad  
  <p class="story" align="left">We think of the Apollo missions as being near equatorial - and the landing sites were - but the sinusoidal orbit  
+
toward the horizon, the lone astronaut in the CM could image as far as 40 degrees north, as in this near-profile  
        of the Command Modules took them as much as 25 degrees from the equator. And by pointing a handheld Hasselblad  
+
view of Rumker. This ~60 km wide and few hundred meters high mound can be considered as the largest lunar dome.  
        toward the horizon, the lone astronaut in the CM could image as far as 40 degrees north, as in this near-profile  
+
It is a complex structure with a broad, low-angle rise that hosts 6 to 10 smaller, mostly steeper sided domes.  
        view of Rumker. This ~60 km wide and few hundred meters high mound can be considered as the largest lunar dome.  
+
Lunar Orbiter pictures show that at least two of these small domes have summit pit craters. Rumker has an  
        It is a complex structure with a broad, low-angle rise that hosts 6 to 10 smaller, mostly steeper sided domes.  
+
off-center flat interior, so that the overall structure appears like a broad ring. It is a bizarre feature that  
        Lunar Orbiter pictures show that at least two of these small domes have summit pit craters. Rumker has an  
+
clearly has volcanic features, but its also possible that some of its elevation results from uplift. Two other  
        off-center flat interior, so that the overall structure appears like a broad ring. It is a bizarre feature that  
+
things to note: The wrinkle ridges at the lower right also show a two component structure. They commonly have a  
        clearly has volcanic features, but its also possible that some of its elevation results from uplift. Two other  
+
relatively sharp crestal ridge that rides on a broader, gentler base. Second, did you notice the line of  
        things to note: The wrinkle ridges at the lower right also show a two component structure. They commonly have a  
+
clustered small craters running diagonally across the bottom left? They are secondary impact craters, but the  
        relatively sharp crestal ridge that rides on a broader, gentler base. Second, did you notice the line of  
+
source crater isn't obvious.  </p>
        clustered small craters running diagonally across the bottom left? They are secondary impact craters, but the  
+
<p class="story"><b>Related Links:</b><br>
        source crater isn't obvious.  </p>
 
 
 
  <p class"story"><b>Related Links:</b><br>
 
 
 
 
[http://44.1911encyclopedia.org/R/RU/RUMKER_CARL_LUDWIG_CHRISTIAN.htm Rumker - father and son]<br>
 
[http://44.1911encyclopedia.org/R/RU/RUMKER_CARL_LUDWIG_CHRISTIAN.htm Rumker - father and son]<br>
 
[http://utenti.lycos.it/gibbidomine/rumker.htm Mons Rumker Geology]
 
[http://utenti.lycos.it/gibbidomine/rumker.htm Mons Rumker Geology]
 
</p>
 
</p>
 
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<p class="story"> <b>Tomorrow's LPOD:</b> The Image that Launched LPOD!</p>
  <p class"story"> <b>Tomorrow's LPOD:</b> The Image that Launched LPOD!</p>
+
</td></tr>
 
 
  <p><img src="../../../MainPage/spacer.gif" width="640" height="1"></p>
 
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<p align="center" class="main_titles"><b>Author & Editor:</b><br>
  <table width="100%"  border="0" cellspacing="2" cellpadding="4">
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
    <tr>
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
      <td><hr width="640"></td>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
      </tr>
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<p align="center" class="main_titles"><b>A service of:</b><br>
    <tr>
+
[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
      <td>
+
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
  <p align="center" class="main_titles"><b>Author & Editor:</b><br>
+
[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p></td>
      [mailto:chuck@observingthesky.org Charles A. Wood]</p>
+
</tr>
      <p align="center" class="main_titles"><b>Technical Consultant:</b><br>
 
      [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
 
      <p align="center" class="main_titles"><b>[mailto:webmaster@entropysponge.com Contact Webmaster]</b></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></td>
 
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<p>&nbsp;</p>
 
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Revision as of 18:16, 4 January 2015

Volcanic Rump

LPOD-2004-02-15.jpeg
Image Credit: Apollo 15 (AS15-97-13252)

Volcanic Rump

We think of the Apollo missions as being near equatorial - and the landing sites were - but the sinusoidal orbit of the Command Modules took them as much as 25 degrees from the equator. And by pointing a handheld Hasselblad toward the horizon, the lone astronaut in the CM could image as far as 40 degrees north, as in this near-profile view of Rumker. This ~60 km wide and few hundred meters high mound can be considered as the largest lunar dome. It is a complex structure with a broad, low-angle rise that hosts 6 to 10 smaller, mostly steeper sided domes. Lunar Orbiter pictures show that at least two of these small domes have summit pit craters. Rumker has an off-center flat interior, so that the overall structure appears like a broad ring. It is a bizarre feature that clearly has volcanic features, but its also possible that some of its elevation results from uplift. Two other things to note: The wrinkle ridges at the lower right also show a two component structure. They commonly have a relatively sharp crestal ridge that rides on a broader, gentler base. Second, did you notice the line of clustered small craters running diagonally across the bottom left? They are secondary impact craters, but the source crater isn't obvious.

Related Links:
Rumker - father and son
Mons Rumker Geology

Tomorrow's LPOD: The Image that Launched LPOD!


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.