Difference between revisions of "October 6, 2004"

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    <tr><td><div align="center" class="main_sm">Image Credit: [mailto:bruno.daversin@lahague.com Bruno Daversin]</p>
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<p align="center"><b>Cleomedes Unveiled</b></p>
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<p align="center"><b>Cleomedes Unveiled</b></p>
<p align="left">[http://www.lpod.org/LPOD-2004-09-27.htm Spaceship  Daversin] has just returned from another Moon mission with the best images in existence of Cleomedes crater. This view shows many features unknown to lunar science. Congratulations, Bruno! This is the clearest view ever of the two known rilles that meet east of the 550 m high off-center peak, Alpha. On a highly stretched version of the image (mouseover) it is clear that there are additional fainter rilles and spurs- I have given them Roman numerals starting with the previously designated Roman numeral I. Number III conceivable is a continuation of number I, but it seems more convoluted in plan, whereas I is more linear. Number III appears to extend north out of the image. Rille number IV is a nearly linear one, that I estimate to be about one km wide. The really remarkable thing about this image is the number of previously unknown dark halo craters it reveals. Three occur along or near rille III and at least five others are on the floor, mostly on the east side of the floor. The largest dark halo crater, between craters J and B (diameter 10.7 km) is about 1.7 km in diameter and its halo is 4 km wide. Because of their association with rilles these are likely to be explosive volcanic craters (like those in [http://www.lpod.org/archive/2004/05/LPOD-2004-05-21.htm Alphonsus])  rather than impact craters that have excavated underlying dark material (e.g. Copernicus H). Interestingly, Cleomedes is the 19th largest pyroclastic deposit on the Moon, having an area of 1089 km2. This is determined from Clementine images which reveal the dark halos but not the details seen here. I suspect the two V-shaped hills seen in the southwest corner of the floor are volcanic cones that were also sources of a pyroclastic deposit.
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<p align="left">[http://www.lpod.org/LPOD-2004-09-27.htm Spaceship  Daversin] has just returned from another Moon mission with the best images in existence of Cleomedes crater. This view shows many features unknown to lunar science. Congratulations, Bruno! This is the clearest view ever of the two known rilles that meet east of the 550 m high off-center peak, Alpha. On a highly stretched version of the image (mouseover) it is clear that there are additional fainter rilles and spurs- I have given them Roman numerals starting with the previously designated Roman numeral I. Number III conceivable is a continuation of number I, but it seems more convoluted in plan, whereas I is more linear. Number III appears to extend north out of the image. Rille number IV is a nearly linear one, that I estimate to be about one km wide. The really remarkable thing about this image is the number of previously unknown dark halo craters it reveals. Three occur along or near rille III and at least five others are on the floor, mostly on the east side of the floor. The largest dark halo crater, between craters J and B (diameter 10.7 km) is about 1.7 km in diameter and its halo is 4 km wide. Because of their association with rilles these are likely to be explosive volcanic craters (like those in [http://www.lpod.org/archive/2004/05/LPOD-2004-05-21.htm Alphonsus])  rather than impact craters that have excavated underlying dark material (e.g. Copernicus H). Interestingly, Cleomedes is the 19th largest pyroclastic deposit on the Moon, having an area of 1089 km2. This is determined from Clementine images which reveal the dark halos but not the details seen here. I suspect the two V-shaped hills seen in the southwest corner of the floor are volcanic cones that were also sources of a pyroclastic deposit.
 
</p>
 
</p>
<blockquote><p align="right">&#8212; [mailto:chuck@observingthesky.org 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>
 
Sept 1, 2004, 1-01h29; Ludiver Observatory 600 mm (24") Schmidt-Cassegrain & B&W webcam.</p>
 
Sept 1, 2004, 1-01h29; Ludiver Observatory 600 mm (24") Schmidt-Cassegrain & B&W webcam.</p>
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<br>[http://www.ludiver.com/ Ludiver Observatory]
 
<br>[http://www.ludiver.com/ Ludiver Observatory]
 
<p align="left"><b>Tomorrow's LPOD: </b> Diamondback Rille</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Diamondback Rille</p>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
[mailto:chuck@observingthesky.org 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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<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>
+
[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>
 
 
 
 
 
----
 
----
 
===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 18:25, 4 January 2015

Cleomedes Unveiled

<nobr>Cleomedes Unveiled</nobr>

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Image Credit: Bruno Daversin


Cleomedes Unveiled

Spaceship Daversin has just returned from another Moon mission with the best images in existence of Cleomedes crater. This view shows many features unknown to lunar science. Congratulations, Bruno! This is the clearest view ever of the two known rilles that meet east of the 550 m high off-center peak, Alpha. On a highly stretched version of the image (mouseover) it is clear that there are additional fainter rilles and spurs- I have given them Roman numerals starting with the previously designated Roman numeral I. Number III conceivable is a continuation of number I, but it seems more convoluted in plan, whereas I is more linear. Number III appears to extend north out of the image. Rille number IV is a nearly linear one, that I estimate to be about one km wide. The really remarkable thing about this image is the number of previously unknown dark halo craters it reveals. Three occur along or near rille III and at least five others are on the floor, mostly on the east side of the floor. The largest dark halo crater, between craters J and B (diameter 10.7 km) is about 1.7 km in diameter and its halo is 4 km wide. Because of their association with rilles these are likely to be explosive volcanic craters (like those in Alphonsus) rather than impact craters that have excavated underlying dark material (e.g. Copernicus H). Interestingly, Cleomedes is the 19th largest pyroclastic deposit on the Moon, having an area of 1089 km2. This is determined from Clementine images which reveal the dark halos but not the details seen here. I suspect the two V-shaped hills seen in the southwest corner of the floor are volcanic cones that were also sources of a pyroclastic deposit.

Chuck Wood

Technical Details:
Sept 1, 2004, 1-01h29; Ludiver Observatory 600 mm (24") Schmidt-Cassegrain & B&W webcam.

Related Links:
Lunar Orbiter IV View
Ludiver Observatory

Tomorrow's LPOD: Diamondback Rille



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.