Difference between revisions of "January 5, 2012"
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| − | <em>image by [mailto:HP-Unigraph@gmx.de | + | <em>image by [mailto:HP-Unigraph@gmx.de Harald Paleske], Langendorf, Germany</em><br /> |
<em>Note: While working on a future Sky & Telescope Exploring the Moon column I came across this excellent LPOD from [http://lpod.wikispaces.com/August+16%2C+2008 Aug 16, 2008]</em> <br /> | <em>Note: While working on a future Sky & Telescope Exploring the Moon column I came across this excellent LPOD from [http://lpod.wikispaces.com/August+16%2C+2008 Aug 16, 2008]</em> <br /> | ||
<em>that is well worth revisting. In the comments in the 2008 LPOD Danny Caes pointed out that the crater behind Drygalski on the left is</em> <br /> | <em>that is well worth revisting. In the comments in the 2008 LPOD Danny Caes pointed out that the crater behind Drygalski on the left is</em> <br /> | ||
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Beyond [http://lpod.wikispaces.com/August+4%2C+2008 Bailly], almost (85° W longitude) on the mean limb, is a large crater that is infrequently seen. With a diameter of 149 (or 163 km <br /> | Beyond [http://lpod.wikispaces.com/August+4%2C+2008 Bailly], almost (85° W longitude) on the mean limb, is a large crater that is infrequently seen. With a diameter of 149 (or 163 km <br /> | ||
according to IAU and Rükl, respectively), [http://the-moon.wikispaces.com/Drygalski Drygalski] is ~50% larger than Copernicus. The only nearside craters with a relatively fresh <br /> | according to IAU and Rükl, respectively), [http://the-moon.wikispaces.com/Drygalski Drygalski] is ~50% larger than Copernicus. The only nearside craters with a relatively fresh <br /> | ||
| − | classical Copernican look that are bigger are nearby [http://www.lpod.org/archive/archive/2004/04/LPOD-2004-04-09.htm | + | classical Copernican look that are bigger are nearby [http://www.lpod.org/archive/archive/2004/04/LPOD-2004-04-09.htm Hausen] (167 km) and distant [http://www.lpod.org/?m=20060307 Humboldt] (207 km) and [http://www.lpod.org/archive/archive/2004/01/LPOD-2004-01-07.htm Petavius] (177 km). Why <br /> |
are these big craters near the limb? Harald's large scale image of Drygalski shows the smooth floor, and hints at the rougher floor behind <br /> | are these big craters near the limb? Harald's large scale image of Drygalski shows the smooth floor, and hints at the rougher floor behind <br /> | ||
the central peak. A terrace is visible on the left wall but the right wall seems more disorganized, probably because of the larger number <br /> | the central peak. A terrace is visible on the left wall but the right wall seems more disorganized, probably because of the larger number <br /> | ||
of craters that cut that side, visible both here and in the Lunar Orbiter IV [http://the-moon.wikispaces.com/Drygalski view].<br /> | of craters that cut that side, visible both here and in the Lunar Orbiter IV [http://the-moon.wikispaces.com/Drygalski view].<br /> | ||
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| − | <em>[mailto:tychocrater@yahoo.com | + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> |
<br /> | <br /> | ||
<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><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+72 72] & VI<br /> | Rükl plates [http://the-moon.wikispaces.com/R%C3%BCkl+72 72] & VI<br /> | ||
| − | Harald's excellent Solar (with Moon coming) [http://www.unigraph.de/ | + | Harald's excellent Solar (with Moon coming) [http://www.unigraph.de/ website]<br /> |
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<hr /> | <hr /> | ||
Revision as of 17:43, 11 January 2015
Limb Magic
image by Harald Paleske, Langendorf, Germany
Note: While working on a future Sky & Telescope Exploring the Moon column I came across this excellent LPOD from Aug 16, 2008
that is well worth revisting. In the comments in the 2008 LPOD Danny Caes pointed out that the crater behind Drygalski on the left is
Ashbrook at 112°W longitude. I've not seen a better image.
Beyond Bailly, almost (85° W longitude) on the mean limb, is a large crater that is infrequently seen. With a diameter of 149 (or 163 km
according to IAU and Rükl, respectively), Drygalski is ~50% larger than Copernicus. The only nearside craters with a relatively fresh
classical Copernican look that are bigger are nearby Hausen (167 km) and distant Humboldt (207 km) and Petavius (177 km). Why
are these big craters near the limb? Harald's large scale image of Drygalski shows the smooth floor, and hints at the rougher floor behind
the central peak. A terrace is visible on the left wall but the right wall seems more disorganized, probably because of the larger number
of craters that cut that side, visible both here and in the Lunar Orbiter IV view.
Chuck Wood
Technical Details
2008-07-26, 4:42 UT. 408mm Newton f 8, 5 m, DMK 1/30sec. exposure, red filter, stack of 300 frames, 3 picture mosaic; seeing good (7/10)
Related Links
Rükl plates 72 & VI
Harald's excellent Solar (with Moon coming) website
