Difference between revisions of "April 17, 2005"

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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<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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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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[mailto:pablolonnie@yahoo.com.mx Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:chlegrand@free.fr Christian Legrand] (Fr)</p>
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<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
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<p align="center" class="main_titles"><b>A service of:</b><br>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</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>
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Latest revision as of 14:14, 15 March 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

Yesterday's LPOD: Ridgeback Crater

Tomorrow's LPOD: The Lunar Crater Wood



Author & Editor:
Charles A. Wood

 


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