Difference between revisions of "March 24, 2005"

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=Floods and Buckshot=
 
=Floods and Buckshot=
 
 
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<td width="50%"><h2><nobr>Floods and Buckshot</nobr></h2></td>
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<img src="archive/2005/03/images/LPOD-2005-03-24.jpeg" border="0">
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    <tr><td><div align="center" class="main_sm">Image Credit: <a class="one" href="starman2@charter.net">Wes Higgins</a></p>
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<tr><td><div align="center" class="main_sm">Image Credit: [starman2@charter.net Wes Higgins]</p>
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<p align="center"><b>Floods and Buckshot</b></p>
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<p align="center"><b>Floods and Buckshot</b></p>
<p align="left">Stadius is one of the Moon’s most famous odd formations. Long ago it was said to be a ring of pits, almost certainly of volcanic origin. But even a casual glance reveals that is an inaccurate description and an unjustified interpretation. The craters near Stadius do not form a ring, but do commonly touch and make many short lines. This remarkable image also shows another key characteristic of these pits that was not visible on pre-spacecraft photos. Many of the craters, especially those in lines, are sources of short ridges, sometimes two ridges that make a vee. Like arrowheads, this “herringbone” pattern points back to the source – Copernicus. Nearly all of the craters on this image are secondaries formed by clots of boulders and small mountains ejected by the formation of Copernicus. The lines of craters result from near simultaneous impacts, and interference of the ejecta from the secondaries creates the Vs. Underneath this ballistic buckshot is Stadius – remnant of a 69 km wide impact crater that has been buried to its rim crests by mare lavas. Stadius is another example of a crater undeserving of a name.</p>
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<p align="left">Stadius is one of the Moon’s most famous odd formations. Long ago it was said to be a ring of pits, almost certainly of volcanic origin. But even a casual glance reveals that is an inaccurate description and an unjustified interpretation. The craters near Stadius do not form a ring, but do commonly touch and make many short lines. This remarkable image also shows another key characteristic of these pits that was not visible on pre-spacecraft photos. Many of the craters, especially those in lines, are sources of short ridges, sometimes two ridges that make a vee. Like arrowheads, this “herringbone” pattern points back to the source – Copernicus. Nearly all of the craters on this image are secondaries formed by clots of boulders and small mountains ejected by the formation of Copernicus. The lines of craters result from near simultaneous impacts, and interference of the ejecta from the secondaries creates the Vs. Underneath this ballistic buckshot is Stadius – remnant of a 69 km wide impact crater that has been buried to its rim crests by mare lavas. Stadius is another example of a crater undeserving of a name.</p>
<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
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<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
 
<p align="left"><p><b>Technical Details:</b><br>
 
<p align="left"><p><b>Technical Details:</b><br>
 
18" Starmaster Newtonian Reflector + DMK-21F04 Firewire Camera, 30FPS
 
18" Starmaster Newtonian Reflector + DMK-21F04 Firewire Camera, 30FPS
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Rukl Plate 32
 
Rukl Plate 32
 
<p align="left"><b>Tomorrow's LPOD: </b> Can You Names These Craters?</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Can You Names These Craters?</p>
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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:chuck@observingthesky.org Charles A. Wood]</p>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
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[mailto:chlegrand@free.fr" class="one 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/" class="one 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>
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[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>
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<p>&nbsp;</p>
 
<p>&nbsp;</p>
 
 
 
 
 
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----
 
===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.

Revision as of 18:30, 4 January 2015

Floods and Buckshot

<nobr>Floods and Buckshot</nobr>

<img src="archive/2005/03/images/LPOD-2005-03-24.jpeg" border="0">

Image Credit: [starman2@charter.net Wes Higgins]


Floods and Buckshot

Stadius is one of the Moon’s most famous odd formations. Long ago it was said to be a ring of pits, almost certainly of volcanic origin. But even a casual glance reveals that is an inaccurate description and an unjustified interpretation. The craters near Stadius do not form a ring, but do commonly touch and make many short lines. This remarkable image also shows another key characteristic of these pits that was not visible on pre-spacecraft photos. Many of the craters, especially those in lines, are sources of short ridges, sometimes two ridges that make a vee. Like arrowheads, this “herringbone” pattern points back to the source – Copernicus. Nearly all of the craters on this image are secondaries formed by clots of boulders and small mountains ejected by the formation of Copernicus. The lines of craters result from near simultaneous impacts, and interference of the ejecta from the secondaries creates the Vs. Underneath this ballistic buckshot is Stadius – remnant of a 69 km wide impact crater that has been buried to its rim crests by mare lavas. Stadius is another example of a crater undeserving of a name.

Chuck Wood

Technical Details:
18" Starmaster Newtonian Reflector + DMK-21F04 Firewire Camera, 30FPS

Related Links:
Rukl Plate 32

Tomorrow's LPOD: Can You Names These Craters?



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Translator:
" class="one Pablo Lonnie Pacheco Railey (Es)
" class="one Christian Legrand (Fr)

Contact Webmaster

A service of:
" class="one ObservingTheSky.Org

Visit these other PODs:
" class="one Astronomy | " class="one Mars | " class="one Earth

 


COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.