Difference between revisions of "February 17, 2012"
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=Copernicus On the Limb= | =Copernicus On the Limb= | ||
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| − | <em>images by [mailto:fmallmann@free.fr Frederic Mallmann], France and Apollo 17</em><br /> | + | <em>images by [mailto:fmallmann@free.fr" rel="nofollow Frederic Mallmann], France and Apollo 17</em><br /> |
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Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact crater formation is<br /> | Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact crater formation is<br /> | ||
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multi-ring basins.<br /> | multi-ring basins.<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 /> |
| − | This is a classic LPOD from [http://www.lpod.org/archive/archive/2004/04/LPOD-2004-04-09.htm April 9, 2004] - were you reading LPOD then?<br /> | + | This is a classic LPOD from [http://www.lpod.org/archive/archive/2004/04/LPOD-2004-04-09.htm" rel="nofollow April 9, 2004] - were you reading LPOD then?<br /> |
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<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope at Ludiver Observatory<br /> | This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope at Ludiver Observatory<br /> | ||
in northern France on 19 Oct. 2003. The telescope worked at f/16 and an infrared filter was used. A ToUcam was used with 1/25 sec<br /> | in northern France on 19 Oct. 2003. The telescope worked at f/16 and an infrared filter was used. A ToUcam was used with 1/25 sec<br /> | ||
| − | exposures and the best 400 of 2700 images were used. Full details [http://fmallmann.free.fr/dethaus.html here].<br /> | + | exposures and the best 400 of 2700 images were used. Full details [http://fmallmann.free.fr/dethaus.html" rel="nofollow here].<br /> |
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The Copernicus shot (bottom) was made with more expensive equipment: Apollo 17.<br /> | The Copernicus shot (bottom) was made with more expensive equipment: Apollo 17.<br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
Rükl plates [http://the-moon.wikispaces.com/R%C3%BCkl+31 31] & [http://the-moon.wikispaces.com/R%C3%BCkl+71 71]<br /> | Rükl plates [http://the-moon.wikispaces.com/R%C3%BCkl+31 31] & [http://the-moon.wikispaces.com/R%C3%BCkl+71 71]<br /> | ||
| − | Mallmann Web [http://fmallmann.free.fr/dethaus.html Page]<br /> | + | Mallmann Web [http://fmallmann.free.fr/dethaus.html" rel="nofollow Page]<br /> |
| − | Lunar Orbiter IV [http://www.lpi.usra.edu/resources/lunar_orbiter/images/img/iv_193_h2.jpg View]<br /> | + | Lunar Orbiter IV [http://www.lpi.usra.edu/resources/lunar_orbiter/images/img/iv_193_h2.jpg" rel="nofollow View]<br /> |
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Revision as of 21:27, 4 January 2015
Copernicus On the Limb
images by " rel="nofollow Frederic Mallmann, France and Apollo 17
Ya seen one crater, ya seen em all. Sometimes that's the way it feels. Because the energy involved in impact crater formation is
so immense, craters of similar size and freshness look pretty much alike. For example, consider these two behemoths. The bottom
crater is Copernicus, 93 km wide and famous for its great location for viewing from Earth. The top image is Hausen, 167 km wide
and hardly seen at all because it's right on the southwest limb beyond Bailly. Despite the difference in diameters the craters look very
similar - both have scarped walls with terraces that step down to the flat floor, which is littered with central mountains. Fresh impact
craters from 40 km in diameter to about 200 km look pretty similar. At larger sizes there is a transition to peak ring craters and then
multi-ring basins.
" rel="nofollow Chuck Wood
This is a classic LPOD from " rel="nofollow April 9, 2004 - were you reading LPOD then?
Technical Details
This magnificent image of Hausen (top) was taken by Frederic Mallmann using the 24" Cassegrain telescope at Ludiver Observatory
in northern France on 19 Oct. 2003. The telescope worked at f/16 and an infrared filter was used. A ToUcam was used with 1/25 sec
exposures and the best 400 of 2700 images were used. Full details " rel="nofollow here.
The Copernicus shot (bottom) was made with more expensive equipment: Apollo 17.
Related Links
Rükl plates 31 & 71
Mallmann Web " rel="nofollow Page
Lunar Orbiter IV " rel="nofollow View
