Difference between revisions of "April 17, 2005"

From LPOD
Jump to: navigation, search
Line 12: Line 12:
 
</table>
 
</table>
 
<table width="80%"  border="0" align="center" cellpadding="8">
 
<table width="80%"  border="0" align="center" cellpadding="8">
<tr><td><div align="center" class="main_sm">Image Credit: [mailto:mwirths@superaje.com Mike Wirths]</p>
+
<tr><td><div align="center" class="main_sm"><p>Image Credit: [mailto:mwirths@superaje.com Mike Wirths]</p>
 
</div></td>
 
</div></td>
 
</tr>   
 
</tr>   
Line 22: Line 22:
 
</p>
 
</p>
 
<blockquote>
 
<blockquote>
<p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
+
<p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</p></blockquote>
 
<p align="left"><b>Technical Details:</b><br>
 
<p align="left"><b>Technical Details:</b><br>
 
March 20, 2005. 18" Starmaster + 5X's powermate + a Baader 685nm IR passband filter.</p>
 
March 20, 2005. 18" Starmaster + 5X's powermate + a Baader 685nm IR passband filter.</p>
Line 28: Line 28:
 
[[iv_132_h1.jpg|Lunar Orbiter IV View ]]
 
[[iv_132_h1.jpg|Lunar Orbiter IV View ]]
 
<br>Rukl Plate 53
 
<br>Rukl Plate 53
 +
</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Unknown right now!</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Unknown right now!</p>
 
</tr>
 
</tr>

Revision as of 20:18, 17 January 2015

Collapsing Mountain?

LPOD-2005-04-17.jpeg

Image Credit: Mike Wirths


Collapsing Mountain?

Stephen Keene’s image of the Hippalus Arcs is one of my all-time favorite lunar photos. The focus of attention of both Stephen’s previous LPOD image and today’s excellent one by Mike Wirths is the set of curved graben that mark where the lunar surface fractured when the weight of the Humorum lavas caused that basin center to subside. But on Mike’s image I immediately noticed something that I hadn’t seen before. The isolated peak left of center has a lobe of material to the left. It appears that the graben cuts this lobe because a faint trace of the graben edge is visible through the deposit. A more interesting interpretation is that the lobe flowed down from the mountain as a giant landslide. Landslides are rare on the Moon, but common elsewhere, especially on Mars and Jupiter’s moon Io. Landslides occur most readily where there is a weak layer that breaks apart and collapses gravitationally under stress. Probably most lunar scientists would say that the lobe is simply a residual piece of old lunar terrain surrounded by mare. It probably is, but may not be. This is a good target for hyper-resolution imaging!

Chuck Wood

Technical Details:
March 20, 2005. 18" Starmaster + 5X's powermate + a Baader 685nm IR passband filter.

Related Links:
Lunar Orbiter IV View
Rukl Plate 53

Tomorrow's LPOD: Unknown right now!



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Translator:
Pablo Lonnie Pacheco Railey (Es)
Christian Legrand (Fr)

Contact Webmaster

A service of:
ObservingTheSky.Org

Visit these other PODs:
Astronomy | Mars | Earth

 


COMMENTS?

Register, and click on the Discussion tab at the top of the page.