Difference between revisions of "May 9, 2013"
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=Positive About Negative= | =Positive About Negative= | ||
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| − | <em>left image by [mailto:digital.astronomy@gmail.com Pete Lawrence] & right image by [http://lpod.wikispaces.com/October+16%2C+2007 Bob Pilz]</em><br /> | + | <em>left image by [mailto:digital.astronomy@gmail.com" rel="nofollow Pete Lawrence] & right image by [http://lpod.wikispaces.com/October+16%2C+2007 Bob Pilz]</em><br /> |
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| − | Mostly we observe features near the terminator because the shadows dramatically exaggerate topographic roughness. Bob's image at right from a 2007 [http://lpod.wikispaces.com/October+16%2C+2007 LPOD] is a wonderful example. But high Sun imaging, as Pete illustrates at left, provides additional information. Pete's image is a negative view, with bright areas being dark and vice-versa. I like this pair because the more commonly observed right view only hints at what becomes obvious when the high Sun is higher: Stöffler is broadly covered by rays from Tycho. If you can remember that rays appear dark in the negative image you will see two to three streamers across the middle of the crater floor, and a large splash of rays near the top. On Bob's low Sun image the top splash is an area of numerous impact craters, probably mostly Tycho secondaries. Look closely at the rays and notice pits long them; the 100 m resolution of the LRO [http://target.lroc.asu.edu/da/qmap.html?mv=eqc&mcx=172031.54192&mcy=-1243996.15457&mz=7 QuickMap] shows many more smaller craters along the rayed areas. Whenever I look at a modest to high illumination image, especially of maria, I often strongly enhance the contrast to detect faint rays. It is surprising that most places on the Moon seem to be veneered with rays, whose source craters are often indeterminant. This means that at diameters below about 1 km, secondary pits are nearly everywhere.<br /> | + | Mostly we observe features near the terminator because the shadows dramatically exaggerate topographic roughness. Bob's image at right from a 2007 [http://lpod.wikispaces.com/October+16%2C+2007 LPOD] is a wonderful example. But high Sun imaging, as Pete illustrates at left, provides additional information. Pete's image is a negative view, with bright areas being dark and vice-versa. I like this pair because the more commonly observed right view only hints at what becomes obvious when the high Sun is higher: Stöffler is broadly covered by rays from Tycho. If you can remember that rays appear dark in the negative image you will see two to three streamers across the middle of the crater floor, and a large splash of rays near the top. On Bob's low Sun image the top splash is an area of numerous impact craters, probably mostly Tycho secondaries. Look closely at the rays and notice pits long them; the 100 m resolution of the LRO [http://target.lroc.asu.edu/da/qmap.html?mv=eqc&mcx=172031.54192&mcy=-1243996.15457&mz=7" rel="nofollow QuickMap] shows many more smaller craters along the rayed areas. Whenever I look at a modest to high illumination image, especially of maria, I often strongly enhance the contrast to detect faint rays. It is surprising that most places on the Moon seem to be veneered with rays, whose source craters are often indeterminant. This means that at diameters below about 1 km, secondary pits are nearly everywhere.<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>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
| − | Lawrence image: April 20, 2013, 21:20. C-14 + PGR Flea-3 at the prime focus; small piece of a 213 hand-stitched panes - full zoomable scene [http://zoom.it/CkFj#full here].<br /> | + | Lawrence image: April 20, 2013, 21:20. C-14 + PGR Flea-3 at the prime focus; small piece of a 213 hand-stitched panes - full zoomable scene [http://zoom.it/CkFj#full" rel="nofollow here].<br /> |
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
Revision as of 22:45, 4 January 2015
Positive About Negative
left image by " rel="nofollow Pete Lawrence & right image by Bob Pilz
Mostly we observe features near the terminator because the shadows dramatically exaggerate topographic roughness. Bob's image at right from a 2007 LPOD is a wonderful example. But high Sun imaging, as Pete illustrates at left, provides additional information. Pete's image is a negative view, with bright areas being dark and vice-versa. I like this pair because the more commonly observed right view only hints at what becomes obvious when the high Sun is higher: Stöffler is broadly covered by rays from Tycho. If you can remember that rays appear dark in the negative image you will see two to three streamers across the middle of the crater floor, and a large splash of rays near the top. On Bob's low Sun image the top splash is an area of numerous impact craters, probably mostly Tycho secondaries. Look closely at the rays and notice pits long them; the 100 m resolution of the LRO " rel="nofollow QuickMap shows many more smaller craters along the rayed areas. Whenever I look at a modest to high illumination image, especially of maria, I often strongly enhance the contrast to detect faint rays. It is surprising that most places on the Moon seem to be veneered with rays, whose source craters are often indeterminant. This means that at diameters below about 1 km, secondary pits are nearly everywhere.
" rel="nofollow Chuck Wood
Technical Details
Lawrence image: April 20, 2013, 21:20. C-14 + PGR Flea-3 at the prime focus; small piece of a 213 hand-stitched panes - full zoomable scene " rel="nofollow here.
Related Links
Rükl plate 65
21st Century Atlas chart 14.
