Difference between revisions of "March 10, 2010"

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<em>north to the left image of Apollo 15 area constructed by [mailto:howard.fink@nyu.edu" rel="nofollow Howard Fink], New York</em><br />
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<em>north to the left image of Apollo 15 area constructed by [mailto:howard.fink@nyu.edu Howard Fink], New York</em><br />
 
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The problem with the Moon is that the illumination always comes from a limited range of azimuths, so the shadows best emphasize features that are perpendicular to those directions. But with a three dimensional model of a lunar scene you can rotate it to have illumination from any direction. Here, the Sun is to the south, casting a shadow from the [http://the-moon.wikispaces.com/Mons+Hadley+Delta Hadley Delta] peak over the big bend in the Hadley Rille. Such rotations can be [http://lpod.wikispaces.com/December+10%2C+2009 performed] within a computer using digital terrain models (DTM), and Howard has [http://finkh.wordpress.com/" rel="nofollow demonstrated] how those same lines of zeros and ones can be transformed into a physical depiction of the lunar surface. He used a USGS digitized [http://webgis.wr.usgs.gov/pigwad/down/moon_dl.htm" rel="nofollow version] of the old topographic map of the Apollo 15 area, which he read into <em>Mathematica</em>, converted into a 3D model with <em>Maya</em>, and printed with a rapid-prototyper or 3-D printer. Howard was very kind and gave me one of these 5&quot; x 7&quot; models which he mounted in a cherry frame. With the new Kaguya and LRO DTMs it will be possible for many people to make their own models of any part of the Moon, using a 3-D printer at a local university or service center. I am especially pleased to see this because in my [http://lpod.wikispaces.com/Science+for+Everyone review] of technology and education I suggested that 3-D printers would soon be able to bring models of planetary landforms into our hands. I am so happy to have one!<br />
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The problem with the Moon is that the illumination always comes from a limited range of azimuths, so the shadows best emphasize features that are perpendicular to those directions. But with a three dimensional model of a lunar scene you can rotate it to have illumination from any direction. Here, the Sun is to the south, casting a shadow from the [http://the-moon.wikispaces.com/Mons+Hadley+Delta Hadley Delta] peak over the big bend in the Hadley Rille. Such rotations can be [http://lpod.wikispaces.com/December+10%2C+2009 performed] within a computer using digital terrain models (DTM), and Howard has [http://finkh.wordpress.com/ demonstrated] how those same lines of zeros and ones can be transformed into a physical depiction of the lunar surface. He used a USGS digitized [http://webgis.wr.usgs.gov/pigwad/down/moon_dl.htm version] of the old topographic map of the Apollo 15 area, which he read into <em>Mathematica</em>, converted into a 3D model with <em>Maya</em>, and printed with a rapid-prototyper or 3-D printer. Howard was very kind and gave me one of these 5&quot; x 7&quot; models which he mounted in a cherry frame. With the new Kaguya and LRO DTMs it will be possible for many people to make their own models of any part of the Moon, using a 3-D printer at a local university or service center. I am especially pleased to see this because in my [http://lpod.wikispaces.com/Science+for+Everyone review] of technology and education I suggested that 3-D printers would soon be able to bring models of planetary landforms into our hands. I am so happy to have one!<br />
 
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><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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<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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Revision as of 17:16, 11 January 2015

Handheld Moon

LPOD-Mar10-10.jpg
north to the left image of Apollo 15 area constructed by Howard Fink, New York

The problem with the Moon is that the illumination always comes from a limited range of azimuths, so the shadows best emphasize features that are perpendicular to those directions. But with a three dimensional model of a lunar scene you can rotate it to have illumination from any direction. Here, the Sun is to the south, casting a shadow from the Hadley Delta peak over the big bend in the Hadley Rille. Such rotations can be performed within a computer using digital terrain models (DTM), and Howard has demonstrated how those same lines of zeros and ones can be transformed into a physical depiction of the lunar surface. He used a USGS digitized version of the old topographic map of the Apollo 15 area, which he read into Mathematica, converted into a 3D model with Maya, and printed with a rapid-prototyper or 3-D printer. Howard was very kind and gave me one of these 5" x 7" models which he mounted in a cherry frame. With the new Kaguya and LRO DTMs it will be possible for many people to make their own models of any part of the Moon, using a 3-D printer at a local university or service center. I am especially pleased to see this because in my review of technology and education I suggested that 3-D printers would soon be able to bring models of planetary landforms into our hands. I am so happy to have one!

Chuck Wood

Related Links
Rükl plate 22


You can support LPOD when you buy any book from Amazon thru LPOD!

COMMENTS?

Register, and click on the Discussion tab at the top of the page.