Difference between revisions of "April 22, 2010"

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=Colorful Pits=
 
=Colorful Pits=
 
 
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<em>south up image by [mailto:mauricejscollins@hotmail.com Maurice Collins], Palmerston North, New Zealand</em><br />
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<em>south up image by [mailto:mauricejscollins@hotmail.com" rel="nofollow Maurice Collins], Palmerston North, New Zealand</em><br />
 
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A few days [http://lpod.armoredpenguin.com/wiki/April+18%2C+2010 ago] when I saw Maurice's draping of the old (but only one that exists) USGS geologic map of the Moon over a digital terrain map created with Jim Mosher's LTVT using the LRO laser altimetry data, I realized how helpful combining data sets can be in understanding our satellite. But I noticed that away from the terminator the DTM accurately showed no shadows and hence it was hard to compare geology with topography. I asked Maurice if it would be possible to use LTVT to depict the DTM with a constant Sun angle across the Moon. Jim [http://ltvt.wikispaces.com/Special+Version+-+Constant+Illumination modified] LTVT for Maurice to do that and, presto, we have the lunar nearside geology superposed on a topo map with 2° illumination everywhere. The highlands are very reminiscent of the old [http://atschool.eduweb.co.uk/bookman/library/THEMOON/INDEX.HTM Nasmyth] plaster [http://atschool.eduweb.co.uk/bookman/library/THEMOON/PLATE20.JPG models] that exaggerated the relief of craters. But this is the actual, but impossible, way the Moon would look if everywhere could instantaneously be illuminated with a low Sun. The yellow and green colors indicate the post-mare craters, and clearly they are not evenly distributed across the nearside; the only large ones in the upper-right quadrant are Tycho and Bullialdus. The map also shows two long ridges defined by shadows - they cross just above and to the left of Eudoxus. Are they real or eye-fooling imaginary lines?<br />
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A few days [/April+18%2C+2010 ago] when I saw Maurice's draping of the old (but only one that exists) USGS geologic map of the Moon over a digital terrain map created with Jim Mosher's LTVT using the LRO laser altimetry data, I realized how helpful combining data sets can be in understanding our satellite. But I noticed that away from the terminator the DTM accurately showed no shadows and hence it was hard to compare geology with topography. I asked Maurice if it would be possible to use LTVT to depict the DTM with a constant Sun angle across the Moon. Jim [http://ltvt.wikispaces.com/Special+Version+-+Constant+Illumination modified] LTVT for Maurice to do that and, presto, we have the lunar nearside geology superposed on a topo map with 2° illumination everywhere. The highlands are very reminiscent of the old [http://atschool.eduweb.co.uk/bookman/library/THEMOON/INDEX.HTM" rel="nofollow Nasmyth] plaster [http://atschool.eduweb.co.uk/bookman/library/THEMOON/PLATE20.JPG" rel="nofollow models] that exaggerated the relief of craters. But this is the actual, but impossible, way the Moon would look if everywhere could instantaneously be illuminated with a low Sun. The yellow and green colors indicate the post-mare craters, and clearly they are not evenly distributed across the nearside; the only large ones in the upper-right quadrant are Tycho and Bullialdus. The map also shows two long ridges defined by shadows - they cross just above and to the left of Eudoxus. Are they real or eye-fooling imaginary lines?<br />
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
 
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
Maurice's [http://moonscience.yolasite.com/ website]<br />
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Maurice's [http://moonscience.yolasite.com/" rel="nofollow website]<br />
 
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<div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 LPOD!]<br />
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<div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591" rel="nofollow LPOD!]<br />
 
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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 19:22, 4 January 2015

Colorful Pits

LPOD-Apr-22-10.jpg
south up image by " rel="nofollow Maurice Collins, Palmerston North, New Zealand

A few days [/April+18%2C+2010 ago] when I saw Maurice's draping of the old (but only one that exists) USGS geologic map of the Moon over a digital terrain map created with Jim Mosher's LTVT using the LRO laser altimetry data, I realized how helpful combining data sets can be in understanding our satellite. But I noticed that away from the terminator the DTM accurately showed no shadows and hence it was hard to compare geology with topography. I asked Maurice if it would be possible to use LTVT to depict the DTM with a constant Sun angle across the Moon. Jim modified LTVT for Maurice to do that and, presto, we have the lunar nearside geology superposed on a topo map with 2° illumination everywhere. The highlands are very reminiscent of the old " rel="nofollow Nasmyth plaster " rel="nofollow models that exaggerated the relief of craters. But this is the actual, but impossible, way the Moon would look if everywhere could instantaneously be illuminated with a low Sun. The yellow and green colors indicate the post-mare craters, and clearly they are not evenly distributed across the nearside; the only large ones in the upper-right quadrant are Tycho and Bullialdus. The map also shows two long ridges defined by shadows - they cross just above and to the left of Eudoxus. Are they real or eye-fooling imaginary lines?

" rel="nofollow Chuck Wood

Related Links
Maurice's " rel="nofollow website


You can support LPOD when you buy any book from Amazon thru " rel="nofollow LPOD!

COMMENTS?

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