Difference between revisions of "May 12, 2012"
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=Copernicus Almost From Lunar Orbit= | =Copernicus Almost From Lunar Orbit= | ||
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<em>image by [mailto:mwirths@starband.ne Michael Wirths], Baja California, Mexico</em><br /> | <em>image by [mailto:mwirths@starband.ne Michael Wirths], Baja California, Mexico</em><br /> | ||
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| − | The Lunar Reconnaissance Orbiter camera team has been issuing a series of high resolution [http://www.lroc.asu.edu/news/index.php?/archives/535-Impact-Melt-Fingers.html images] that document | + | The Lunar Reconnaissance Orbiter camera team has been issuing a series of high resolution [http://www.lroc.asu.edu/news/index.php?/archives/535-Impact-Melt-Fingers.html images] that document |
| − | the varieties of impact melt morphologies. That is very important but Mike with his Baja spaceship is demonstrating | + | the varieties of impact melt morphologies. That is very important but Mike with his Baja spaceship is demonstrating |
| − | that you don't need an orbiter to acquire magnificent images of melt deposits. Most impressive are the tongues | + | that you don't need an orbiter to acquire magnificent images of melt deposits. Most impressive are the tongues |
| − | of melt outside the arc of Copernicus' rim from Fauth (twin craters at bottom) to the mountain at the 9 o'clock | + | of melt outside the arc of Copernicus' rim from Fauth (twin craters at bottom) to the mountain at the 9 o'clock |
| − | position. Just south of the mountain is a superb tongue of melt that built up levees on its flanks as it flowed. Once | + | position. Just south of the mountain is a superb tongue of melt that built up levees on its flanks as it flowed. Once |
| − | this classic example of a melt flow is recognized it is easier to see others on the arc toward Fauth. Melt ponds are | + | this classic example of a melt flow is recognized it is easier to see others on the arc toward Fauth. Melt ponds are |
| − | also visible at various places inside the rim on terrace tops. And the smooth northwest quadrant of Copernicus' floor | + | also visible at various places inside the rim on terrace tops. And the smooth northwest quadrant of Copernicus' floor |
| − | is veneered by impact melt. Along the southern edge of the image secondary craters and their characteristic | + | is veneered by impact melt. Along the southern edge of the image secondary craters and their characteristic herringbone pattern of wrap around ejecta are beautifully seen, while the ridge and furrow continuous ejecta is well seen |
| − | + | along the top of the image. If we had been able to take images like this in the 1950s scientists might have decided | |
| − | along the top of the image. If we had been able to take images like this in the 1950s scientists might have decided | + | that they didn't need to go to the Moon. |
| − | that they didn't need to go to the Moon. | ||
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | Rükl plate [ | + | Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_31 31]<br /> |
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| + | <p><b>Yesterday's LPOD:</b> [[May 11, 2012|High Waves or Low Faults On the Sea of Rainbows]] </p> | ||
| + | <p><b>Tomorrow's LPOD:</b> [[May 13, 2012|Luminous Shades of Gray]] </p> | ||
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Latest revision as of 17:52, 13 October 2018
Copernicus Almost From Lunar Orbit
image by Michael Wirths, Baja California, Mexico
The Lunar Reconnaissance Orbiter camera team has been issuing a series of high resolution images that document
the varieties of impact melt morphologies. That is very important but Mike with his Baja spaceship is demonstrating
that you don't need an orbiter to acquire magnificent images of melt deposits. Most impressive are the tongues
of melt outside the arc of Copernicus' rim from Fauth (twin craters at bottom) to the mountain at the 9 o'clock
position. Just south of the mountain is a superb tongue of melt that built up levees on its flanks as it flowed. Once
this classic example of a melt flow is recognized it is easier to see others on the arc toward Fauth. Melt ponds are
also visible at various places inside the rim on terrace tops. And the smooth northwest quadrant of Copernicus' floor
is veneered by impact melt. Along the southern edge of the image secondary craters and their characteristic herringbone pattern of wrap around ejecta are beautifully seen, while the ridge and furrow continuous ejecta is well seen
along the top of the image. If we had been able to take images like this in the 1950s scientists might have decided
that they didn't need to go to the Moon.
Chuck Wood
Technical Details
2012/04/30 at 20:47 PST; taken with 18" Starmaster dob (Zambuto optics) a Lumenera Infinity 2-2 camera, 2.5X Televue Powermate barlow and R/IR filter.
Processed with AviStack and PS CS.
Related Links
Rükl plate 31
Yesterday's LPOD: High Waves or Low Faults On the Sea of Rainbows
Tomorrow's LPOD: Luminous Shades of Gray
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