Difference between revisions of "August 12, 2011"

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=The Basin Near Schiller=
 
=The Basin Near Schiller=
  
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<em>image by [mailto:patricio@geo.ucm.es Patricio Dominguez Alonso], Madrid, Spain</em><br />
 
<em>image by [mailto:patricio@geo.ucm.es Patricio Dominguez Alonso], Madrid, Spain</em><br />
 
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        <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 />
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<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 />
 
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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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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 Bill Corliss] of the Sourcebook Project, who unearthed many unusual anomalies in science, has recently died. <br />
 
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===COMMENTS?===
 
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Revision as of 00:17, 3 January 2015

The Basin Near Schiller

LPOD-aug12-11.jpg
image by Patricio Dominguez Alonso, Madrid, Spain

LPOD-aug12b-11.jpg
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 paper on lunar impact basins. In 1971 Bill and I also described it in our basin 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.


Chuck Wood

Note: 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