Difference between revisions of "August 12, 2011"
| Line 1: | Line 1: | ||
__NOTOC__ | __NOTOC__ | ||
=The Basin Near Schiller= | =The Basin Near Schiller= | ||
| − | |||
<!-- ws:start:WikiTextHeadingRule:0:<h1> --> | <!-- ws:start:WikiTextHeadingRule:0:<h1> --> | ||
<!-- ws:start:WikiTextLocalImageRule:14:<img src="/file/view/LPOD-aug12-11.jpg/245538299/LPOD-aug12-11.jpg" alt="" title="" /> -->[[File:LPOD-aug12-11.jpg|LPOD-aug12-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:14 --><br /> | <!-- ws:start:WikiTextLocalImageRule:14:<img src="/file/view/LPOD-aug12-11.jpg/245538299/LPOD-aug12-11.jpg" alt="" title="" /> -->[[File:LPOD-aug12-11.jpg|LPOD-aug12-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:14 --><br /> | ||
| − | <em>image by [mailto:patricio@geo.ucm.es Patricio Dominguez Alonso], Madrid, Spain</em><br /> | + | <em>image by [mailto:patricio@geo.ucm.es" rel="nofollow Patricio Dominguez Alonso], Madrid, Spain</em><br /> |
<br /> | <br /> | ||
<table class="wiki_table"> | <table class="wiki_table"> | ||
| Line 10: | Line 9: | ||
<td><!-- ws:start:WikiTextLocalImageRule:15:<img src="/file/view/LPOD-aug12b-11.jpg/245538347/LPOD-aug12b-11.jpg" alt="" title="" /> -->[[File:LPOD-aug12b-11.jpg|LPOD-aug12b-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:15 --><br /> | <td><!-- ws:start:WikiTextLocalImageRule:15:<img src="/file/view/LPOD-aug12b-11.jpg/245538347/LPOD-aug12b-11.jpg" alt="" title="" /> -->[[File:LPOD-aug12b-11.jpg|LPOD-aug12b-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:15 --><br /> | ||
</td> | </td> | ||
| − | <td>Paul Kuiper, astronomer Gerard Kuiper's photographer son, was the first person to notice this degraded impact basin near Schiller in 1959. Later, Bill Hartmann and Gerard Kuiper included this double ring, 350 km wide basin near Schiller - what they called it - in their epocal [http://www.lpl.arizona.edu/SIC/journal/pdfs/012_Hartmann_CommLPL_1962.pdf paper] on lunar impact basins. In 1971 Bill and I also described it in our basin [http://www.psi.edu/epo/multiring_impact_basins/multiring_impact_basins_files/Hartmann_Wood_1971.pdf paper] and pointed out the mare ridges that suggested it might have an inner third ring. There haven't been many additional studies about this Zucchius-Schiller basin. Perhaps new data from multiple sensors on LRO will reveal more about this often overlooked feature.<br /> | + | <td>Paul Kuiper, astronomer Gerard Kuiper's photographer son, was the first person to notice this degraded impact basin near Schiller in 1959. Later, Bill Hartmann and Gerard Kuiper included this double ring, 350 km wide basin near Schiller - what they called it - in their epocal [http://www.lpl.arizona.edu/SIC/journal/pdfs/012_Hartmann_CommLPL_1962.pdf" rel="nofollow paper] on lunar impact basins. In 1971 Bill and I also described it in our basin [http://www.psi.edu/epo/multiring_impact_basins/multiring_impact_basins_files/Hartmann_Wood_1971.pdf" rel="nofollow paper] and pointed out the mare ridges that suggested it might have an inner third ring. There haven't been many additional studies about this Zucchius-Schiller basin. Perhaps new data from multiple sensors on LRO will reveal more about this often overlooked feature.<br /> |
<br /> | <br /> | ||
| − | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br /> |
</td> | </td> | ||
</tr> | </tr> | ||
</table> | </table> | ||
| − | Note: [http://en.wikipedia.org/wiki/William_R._Corliss Bill Corliss] of the Sourcebook Project, who unearthed many unusual anomalies in science, has recently died. <br /> | + | Note: [http://en.wikipedia.org/wiki/William_R._Corliss" rel="nofollow Bill Corliss] of the Sourcebook Project, who unearthed many unusual anomalies in science, has recently died. <br /> |
<br /> | <br /> | ||
<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
Revision as of 21:20, 4 January 2015
The Basin Near Schiller
image by " rel="nofollow Patricio Dominguez Alonso, Madrid, Spain
 |
Paul Kuiper, astronomer Gerard Kuiper's photographer son, was the first person to notice this degraded impact basin near Schiller in 1959. Later, Bill Hartmann and Gerard Kuiper included this double ring, 350 km wide basin near Schiller - what they called it - in their epocal " rel="nofollow paper on lunar impact basins. In 1971 Bill and I also described it in our basin " rel="nofollow paper and pointed out the mare ridges that suggested it might have an inner third ring. There haven't been many additional studies about this Zucchius-Schiller basin. Perhaps new data from multiple sensors on LRO will reveal more about this often overlooked feature. |
Note: " rel="nofollow Bill Corliss of the Sourcebook Project, who unearthed many unusual anomalies in science, has recently died.
Technical Details
August 10 2011 22:22UT. Celestron C11 CGE DMK21AU618.AS Infrared
Related Links
Rükl plate 71
