Difference between revisions of "April 17, 2005"

From LPOD
Jump to: navigation, search
Line 8: Line 8:
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<table width="85%"  border="0" align="center" cellpadding="6" cellspacing="2">
 
<tr><td colspan="2" valign="top"><div align="center">
 
<tr><td colspan="2" valign="top"><div align="center">
<img src="archive/2005/04/images/LPOD-2005-04-17.jpeg" border="0">
+
[[File:LPOD-2005-04-17.jpeg|LPOD-2005-04-17.jpeg]]
 
</div></td>
 
</div></td>
 
</tr>
 
</tr>
Line 20: Line 20:
 
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td>
 
<p align="center"><b>Collapsing Mountain?</b></p>
 
<p align="center"><b>Collapsing Mountain?</b></p>
<p align="left">Stephen Keene’s  [http://www.lpod.org/archive/2004/01/LPOD-2004-01-26.htm 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 [http://berlinadmin.dlr.de/Missions/express/first/05.08.2004_eng.shtml Mars] and Jupiter’s moon [http://solarsystem.nasa.gov/scitech/display.cfm?ST_ID=487 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!
+
<p align="left">Stephen Keene’s  [[January_26,_2004|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 [http://berlinadmin.dlr.de/Missions/express/first/05.08.2004_eng.shtml Mars] and Jupiter’s moon [http://solarsystem.nasa.gov/scitech/display.cfm?ST_ID=487 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!
 
</p>
 
</p>
 
<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
 
<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
Line 42: Line 42:
 
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
 
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
 
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
 
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
+
[mailto:pablolonnie@yahoo.com.mx Pablo Lonnie Pacheco Railey]  (Es)<br>
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
+
[mailto:chlegrand@free.fr Christian Legrand] (Fr)</p>
 
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
 
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
 
<p align="center" class="main_titles"><b>A service of:</b><br>
 
<p align="center" class="main_titles"><b>A service of:</b><br>
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
+
[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
 
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
 
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
+
[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
 
</td></tr>
 
</td></tr>
 
</table>  
 
</table>  

Revision as of 14:31, 17 January 2015

Collapsing Mountain?

<nobr>Collapsing Mountain?</nobr>

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.