Difference between revisions of "March 10, 2010"
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=Handheld Moon= | =Handheld Moon= | ||
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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 /> | + | <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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− | 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" 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 [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 /> | + | 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" 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 [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 Chuck Wood]</em><br /> | + | <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 /> | ||
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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 /> | + | <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 19:20, 4 January 2015
Handheld Moon
north to the left image of Apollo 15 area constructed by " rel="nofollow 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 " 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 " rel="nofollow 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!
" rel="nofollow Chuck Wood
Related Links
Rükl plate 22
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.