Difference between revisions of "October 11, 2004"

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    <tr><td><div align="center" class="main_sm">Image Credit: Gerardo Sbarufatti</p>
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<p align="center"><b>Fertility Central</b></p>
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<p align="center"><b>Fertility Central</b></p>
<p align="left">Can you imagine an image of the central part of Mare Fecunditatis where [http://www.lpod.org/archive/2004/05/LPOD-2004-05-20.htm Messier] is not the most fascinating feature? Here is one! (But, yes, this fantastic image does show the rarely imaged N-S butterfly wing pattern of ejecta at Messier). Starting at the western edge (left side) the well-known Lubbock fault scarp casts a shahow (see mouseover). Both the scarp and the pits on the mare ridge to the east (dhc?) are dark near full Moon and are pyroclastic units. The rille Messier I and its continuing line of collapse pits (the rille continues as a lava tube) are nicely displayed. But what seems to be new - I can't find it on any previous images, NASA or amateur - are the delicate rilles just east and north of Secchi K. Notice that one rille/line of pits runs NW-SE, but the others are more N-S. This image is also full of beautiful ghost craters, consistent with estimates that the mare here is mostly less than 500 m thick. In a ghost crater near the southeast corner is a classic hemispheric dome with a summit pit; other hills nearby seem to be steeper and not obviously domes. A broad, swell-like, possible dome is visible in the southwest corner. This one image, covering an area poorly shown in spacecraft imagery, has revealed new features and demonstrated that every place on the Moon deserves high resolution, low sun imaging!</p>
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<p align="left">Can you imagine an image of the central part of Mare Fecunditatis where [http://www.lpod.org/archive/2004/05/LPOD-2004-05-20.htm Messier] is not the most fascinating feature? Here is one! (But, yes, this fantastic image does show the rarely imaged N-S butterfly wing pattern of ejecta at Messier). Starting at the western edge (left side) the well-known Lubbock fault scarp casts a shahow (see mouseover). Both the scarp and the pits on the mare ridge to the east (dhc?) are dark near full Moon and are pyroclastic units. The rille Messier I and its continuing line of collapse pits (the rille continues as a lava tube) are nicely displayed. But what seems to be new - I can't find it on any previous images, NASA or amateur - are the delicate rilles just east and north of Secchi K. Notice that one rille/line of pits runs NW-SE, but the others are more N-S. This image is also full of beautiful ghost craters, consistent with estimates that the mare here is mostly less than 500 m thick. In a ghost crater near the southeast corner is a classic hemispheric dome with a summit pit; other hills nearby seem to be steeper and not obviously domes. A broad, swell-like, possible dome is visible in the southwest corner. This one image, covering an area poorly shown in spacecraft imagery, has revealed new features and demonstrated that every place on the Moon deserves high resolution, low sun imaging!</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>
 
Oct 2, 2004, 00:07 UT. Celestron 8 + 2X barlow + 5,500 um IR cutout filter + Phillips Vesta Pro, 200 sec AVI at 10 fps, 400 best frames used. This remarkable image was taken by Gerardo Sbarufatti but I have not been able to contact him. Gerardo, I hope you will be pleased that your excellent image has been used on LPOD! Note that I have aggressively used the Photoshop "unsharp mask" filter to enhance subtle topo in the mouseover image. </p>
 
Oct 2, 2004, 00:07 UT. Celestron 8 + 2X barlow + 5,500 um IR cutout filter + Phillips Vesta Pro, 200 sec AVI at 10 fps, 400 best frames used. This remarkable image was taken by Gerardo Sbarufatti but I have not been able to contact him. Gerardo, I hope you will be pleased that your excellent image has been used on LPOD! Note that I have aggressively used the Photoshop "unsharp mask" filter to enhance subtle topo in the mouseover image. </p>
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<br>Rukl <i>Atlas of the Moon</i> Sheet 48
 
<br>Rukl <i>Atlas of the Moon</i> Sheet 48
 
<p align="left"><b>Tomorrow's LPOD: </b> Polar Dryness?</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Polar Dryness?</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>
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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>
+
[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>
 
 
 
 
 
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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 18:26, 4 January 2015

Fertility Central

<nobr>Fertility Central</nobr>

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Image Credit: Gerardo Sbarufatti


Fertility Central

Can you imagine an image of the central part of Mare Fecunditatis where Messier is not the most fascinating feature? Here is one! (But, yes, this fantastic image does show the rarely imaged N-S butterfly wing pattern of ejecta at Messier). Starting at the western edge (left side) the well-known Lubbock fault scarp casts a shahow (see mouseover). Both the scarp and the pits on the mare ridge to the east (dhc?) are dark near full Moon and are pyroclastic units. The rille Messier I and its continuing line of collapse pits (the rille continues as a lava tube) are nicely displayed. But what seems to be new - I can't find it on any previous images, NASA or amateur - are the delicate rilles just east and north of Secchi K. Notice that one rille/line of pits runs NW-SE, but the others are more N-S. This image is also full of beautiful ghost craters, consistent with estimates that the mare here is mostly less than 500 m thick. In a ghost crater near the southeast corner is a classic hemispheric dome with a summit pit; other hills nearby seem to be steeper and not obviously domes. A broad, swell-like, possible dome is visible in the southwest corner. This one image, covering an area poorly shown in spacecraft imagery, has revealed new features and demonstrated that every place on the Moon deserves high resolution, low sun imaging!

Chuck Wood

Technical Details:
Oct 2, 2004, 00:07 UT. Celestron 8 + 2X barlow + 5,500 um IR cutout filter + Phillips Vesta Pro, 200 sec AVI at 10 fps, 400 best frames used. This remarkable image was taken by Gerardo Sbarufatti but I have not been able to contact him. Gerardo, I hope you will be pleased that your excellent image has been used on LPOD! Note that I have aggressively used the Photoshop "unsharp mask" filter to enhance subtle topo in the mouseover image.

Related Links:
Lunar Orbiter IV Image (Poor)
Rukl Atlas of the Moon Sheet 48

Tomorrow's LPOD: Polar Dryness?



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.