Difference between revisions of "June 11, 2011"

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<em>image by [[mailto:|Wes Higgins]], Tecumseh, Oklahoma</em><br />
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<em>image by Wes Higgins, Tecumseh, Oklahoma</em><br />
 
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I am on travel and was not planning to write a new LPOD and then this evening I saw Wes’ new image and couldn’t help myself. Gosh, this is good! Comparison with the commonly used Lunar &amp; Planetary Institution’s digitized Lunar Orbiter image of nearly the same area demonstrates that Wes’ image shows craters not visible of that orbital view and the rilles and other features are more sharply displayed - and there are no lines from the Orbiter’s photo-reconstruction process! Both Alphonsus and Arzachel are floor-fractured craters, and Alphonsus is the easiest place on the Moon to see volcanic dark halo craters. The Imbrium Basin impact created a number of radial crater chains that are well seen east of Alphonsus, as well as the three gougely like short chains just north of Arzachel. This is a glorious image - look at each square centimeter and try to understand its history!<br />
 
I am on travel and was not planning to write a new LPOD and then this evening I saw Wes’ new image and couldn’t help myself. Gosh, this is good! Comparison with the commonly used Lunar &amp; Planetary Institution’s digitized Lunar Orbiter image of nearly the same area demonstrates that Wes’ image shows craters not visible of that orbital view and the rilles and other features are more sharply displayed - and there are no lines from the Orbiter’s photo-reconstruction process! Both Alphonsus and Arzachel are floor-fractured craters, and Alphonsus is the easiest place on the Moon to see volcanic dark halo craters. The Imbrium Basin impact created a number of radial crater chains that are well seen east of Alphonsus, as well as the three gougely like short chains just north of Arzachel. This is a glorious image - look at each square centimeter and try to understand its history!<br />
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
<strong>Note</strong> This is a classic LPOD from [http://www.lpod.org/?m=20060916 Sept 16, 2006] - and it reminds us that fantastic images were being taken at least 5 years ago.<br />
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<strong>Note</strong> This is a classic LPOD from [[September_16,_2006|Sept 16, 2006]] - and it reminds us that fantastic images were being taken at least 5 years ago.<br />
 
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<strong>Technical Details</strong><br />
 
<strong>Technical Details</strong><br />
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+44 44]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_44 44]<br />
 
Wes’ [http://higginsandsons.com/astro/ website]<br />
 
Wes’ [http://higginsandsons.com/astro/ website]<br />
 
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<p><b>Yesterday's LPOD:</b> [[June 10, 2011|A Small Sea of Lava]] </p>
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<p><b>Tomorrow's LPOD:</b> [[June 12, 2011|Ridges And Subtle Bulges]] </p>
 
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===COMMENTS?===
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 

Latest revision as of 18:49, 13 October 2018

Just Another Glorious Image

LPOD-Jun11-11.jpg
image by Wes Higgins, Tecumseh, Oklahoma

I am on travel and was not planning to write a new LPOD and then this evening I saw Wes’ new image and couldn’t help myself. Gosh, this is good! Comparison with the commonly used Lunar & Planetary Institution’s digitized Lunar Orbiter image of nearly the same area demonstrates that Wes’ image shows craters not visible of that orbital view and the rilles and other features are more sharply displayed - and there are no lines from the Orbiter’s photo-reconstruction process! Both Alphonsus and Arzachel are floor-fractured craters, and Alphonsus is the easiest place on the Moon to see volcanic dark halo craters. The Imbrium Basin impact created a number of radial crater chains that are well seen east of Alphonsus, as well as the three gougely like short chains just north of Arzachel. This is a glorious image - look at each square centimeter and try to understand its history!

Chuck Wood
Note This is a classic LPOD from Sept 16, 2006 - and it reminds us that fantastic images were being taken at least 5 years ago.

Technical Details
September 14, 2006, 18″ Reflector, 4x Powermate, Infinity 2-1M camera, MAP processing.

Related Links
Rükl plate 44
Wes’ website

Yesterday's LPOD: A Small Sea of Lava

Tomorrow's LPOD: Ridges And Subtle Bulges



COMMENTS?

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