Difference between revisions of "Schrödinger"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =Schrödinger Basin= ''(unofficial name; IAU crater name: '''Schrödinger'''; 312 km diam)''<br /> {| class="wi...")
 
 
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| Lat: 75.0°S, Long: 132.4°E, Main ring diam: 320 km, Depth: 4.8 km, Rükl: ''(farside)''<br />
 
| Lat: 75.0°S, Long: 132.4°E, Main ring diam: 320 km, Depth: 4.8 km, Rükl: ''(farside)''<br />
 
|}
 
|}
[http://www.lpod.org/coppermine/displayimage.php?pid=909&fullsize=1 [[Image:normal_schrodinger-clem1.jpg|external image normal_schrodinger-clem1.jpg]]][http://www.lpod.org/coppermine/displayimage.php?pid=2348&fullsize=1 [[Image:normal_Schrodinger_Basin_LIDAR_LTVT.JPG|external image normal_Schrodinger_Basin_LIDAR_LTVT.JPG]]]<br /> '''Left:''' ''[http://lpod.org/coppermine/displayimage.php?pos=-909 Clementine]''.<br /> '''Right:''' ''[http://lpod.org/coppermine/displayimage.php?pos=-2348 Clementine]'', Clementine LIDAR Altimeter texture from [http://pdsmaps.wr.usgs.gov/PDS/public/explorer/html/lidrlvls.htm PDS Map-a-Planet] remapped to north-up aerial view by [http://www.henriksucla.dk/ LTVT]. The dot is the center position and the white circle the main ring position from Chuck Wood's [http://www.lpod.org/cwm/DataStuff/Lunar%20Basins.htm Impact Basin Database]. Grid spacing = 10 degrees.<br /> <div id="toc">
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[http://www.lpod.org/coppermine/displayimage.php?pid=909&fullsize=1 [[Image:Normal_schrodinger-clem1.jpg|external image normal_schrodinger-clem1.jpg]]][http://www.lpod.org/coppermine/displayimage.php?pid=2348&fullsize=1 [[Image:Normal_Schrodinger_Basin_LIDAR_LTVT.JPG|external image normal_Schrodinger_Basin_LIDAR_LTVT.JPG]]]<br /> '''Left:''' ''[http://lpod.org/coppermine/displayimage.php?pos=-909 Clementine]''.<br /> '''Right:''' ''[http://lpod.org/coppermine/displayimage.php?pos=-2348 Clementine]'', Clementine LIDAR Altimeter texture from [http://pdsmaps.wr.usgs.gov/PDS/public/explorer/html/lidrlvls.htm PDS Map-a-Planet] remapped to north-up aerial view by [http://www.henriksucla.dk/ LTVT]. The dot is the center position and the white circle the main ring position from Chuck Wood's [http://www.lpod.org/cwm/DataStuff/Lunar%20Basins.htm Impact Basin Database]. Grid spacing = 10 degrees.<br /> <div id="toc">
=Table of Contents=
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<div style="margin-left: 1em">[#Schrödinger Basin Schrödinger Basin]</div><div style="margin-left: 2em">[#Schrödinger Basin-Images Images]</div><div style="margin-left: 2em">[#Schrödinger Basin-Maps Maps]</div><div style="margin-left: 2em">[#Schrödinger Basin-Basin Classification Basin Classification]</div><div style="margin-left: 2em">[#Schrödinger Basin-Description Description]</div><div style="margin-left: 3em">[#Schrödinger Basin-Description-Wikipedia Wikipedia]</div><div style="margin-left: 2em">[#Schrödinger Basin-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Schrödinger Basin-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Schrödinger Basin-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Schrödinger Basin-Bibliography Bibliography]</div></div>
 
 
==Images==
 
==Images==
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Schrodinger LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Schrodinger%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Schrodinger Apollo Images] [http://jda.jaxa.jp/jda/p4_e.php?f_id=15970&mode=level&time=N&genre=5&category=5025 Kaguya HDTV]<br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Schrodinger LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Schrodinger%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Schrodinger Apollo Images] [http://jda.jaxa.jp/jda/p4_e.php?f_id=15970&mode=level&time=N&genre=5&category=5025 Kaguya HDTV]<br />  
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* Exterior impact melt deposits to E, max of ~100 km beyond rim. Most extensive ejecta, rays and secondary craters to the NE, with max wall slumping on E side of crater, and topographically lowest rim crest to S ([[Hawke%20and%20Head%2C%201977|Hawke and Head, 1977]]).
 
* Exterior impact melt deposits to E, max of ~100 km beyond rim. Most extensive ejecta, rays and secondary craters to the NE, with max wall slumping on E side of crater, and topographically lowest rim crest to S ([[Hawke%20and%20Head%2C%201977|Hawke and Head, 1977]]).
 
* Mare area of 1,325 km^2 according to measurements by [http://www.lpod.org/cwm/DataStuff/MareAreas.htm Jim Whitford-Stark].
 
* Mare area of 1,325 km^2 according to measurements by [http://www.lpod.org/cwm/DataStuff/MareAreas.htm Jim Whitford-Stark].
* East of '''Schrödinger''' (between '''Schrödinger''' and [[De%20Forest|De Forest]], see [[Clementine%20Atlas|Clementine]]'s photographs of it on LAC 141) is an irregular shaped valley of which the most pronounced (and most shadowed) part is located at 165° to 170° East, 77° South. <span class="membersnap">- [http://www.wikispaces.com/user/view/DannyCaes [[Image:DannyCaes-lg.jpg|16px|DannyCaes]]] [http://www.wikispaces.com/user/view/DannyCaes DannyCaes] <small>May 12, 2009</small></span>
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* East of '''Schrödinger''' (between '''Schrödinger''' and [[De%20Forest|De Forest]], see [[Clementine%20Atlas|Clementine]]'s photographs of it on LAC 141) is an irregular shaped valley of which the most pronounced (and most shadowed) part is located at 165° to 170° East, 77° South. <span class="membersnap">- DannyCaes <small>May 12, 2009</small></span>
* The odd crater '''Schrodinger W''', northwest of '''Schrodinger''' itself, looks a bit like one of the craters of the '''Messier''' pair in '''Mare Fecunditatis'''. A large crater is overlapping a little one, or are both the result of one single oblique impact? <span class="membersnap">- [http://www.wikispaces.com/user/view/DannyCaes [[Image:DannyCaes-lg.jpg|16px|DannyCaes]]] [http://www.wikispaces.com/user/view/DannyCaes DannyCaes] <small>Aug 13, 2014</small></span>
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* The odd crater '''Schrodinger W''', northwest of '''Schrodinger''' itself, looks a bit like one of the craters of the '''Messier''' pair in '''Mare Fecunditatis'''. A large crater is overlapping a little one, or are both the result of one single oblique impact? <span class="membersnap">- DannyCaes <small>Aug 13, 2014</small></span>
 
<br />  
 
<br />  
 
==Nomenclature==
 
==Nomenclature==
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  This page has been edited 1 times. The last modification was made by <span class="membersnap">- [http://www.wikispaces.com/user/view/tychocrater [[Image:tychocrater-lg.jpg|16px|tychocrater]]] [http://www.wikispaces.com/user/view/tychocrater tychocrater]</span> on Jun 13, 2009 3:24 pm - ''afx3u3''</div>
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Latest revision as of 02:16, 16 April 2018

Schrödinger Basin

(unofficial name; IAU crater name: Schrödinger; 312 km diam)

Lat: 75.0°S, Long: 132.4°E, Main ring diam: 320 km, Depth: 4.8 km, Rükl: (farside)
external image normal_schrodinger-clem1.jpgexternal image normal_Schrodinger_Basin_LIDAR_LTVT.JPG
Left: Clementine.
Right: Clementine, Clementine LIDAR Altimeter texture from PDS Map-a-Planet remapped to north-up aerial view by LTVT. The dot is the center position and the white circle the main ring position from Chuck Wood's Impact Basin Database. Grid spacing = 10 degrees.

Images

LPOD Photo Gallery Lunar Orbiter Images Apollo Images Kaguya HDTV


Maps

(LAC zone 140C1) USGS Digital Atlas PDF

Basin Classification

(description of terms and most numeric basin data from Wood, C.A. (2004) Impact Basin Database)
Certainty of Existence
USGS Age
Wilhelms Age Group
Ring Diameters
Mare Thickness
Mascon
Certain
Imbrian
12
150, 320 km



Description


Wikipedia

Schrödinger

Additional Information

  • Exterior impact melt deposits to E, max of ~100 km beyond rim. Most extensive ejecta, rays and secondary craters to the NE, with max wall slumping on E side of crater, and topographically lowest rim crest to S (Hawke and Head, 1977).
  • Mare area of 1,325 km^2 according to measurements by Jim Whitford-Stark.
  • East of Schrödinger (between Schrödinger and De Forest, see Clementine's photographs of it on LAC 141) is an irregular shaped valley of which the most pronounced (and most shadowed) part is located at 165° to 170° East, 77° South. - DannyCaes May 12, 2009
  • The odd crater Schrodinger W, northwest of Schrodinger itself, looks a bit like one of the craters of the Messier pair in Mare Fecunditatis. A large crater is overlapping a little one, or are both the result of one single oblique impact? - DannyCaes Aug 13, 2014


Nomenclature

  • The IAU crater name honors Erwin Rudolf Josef Alexander Schrödinger (August 12, 1887 – January 4, 1961) an Austrian-Irish physicist who achieved fame for his contributions to quantum mechanics, especially the Schrödinger equation, for which he received the Nobel Prize in 1933. In 1935, he proposed the Schrödinger's cat thought experiment.
  • The impact basin is named after the crater.
  • The pronounced valley between Schrödinger and De Forest is unofficially called Vallis Schrödinger-De Forest by D.Caes.
  • Rimae Schrodinger (an unofficial name from D.Caes for the impressive system of rilles on the floor of Schrodinger).


LPOD Articles


Bibliography

  • Kramer, G. Y. et al(2011). Analysis of Schrodinger Basin Using Moon Mineralogy Mapper Spectra – 42nd LPSC Conference (Mar), 2011.
  • Shoemaker, E.M., M.S. Robinson & E.M. Eliason (1994) The South Pole region of the Moon as seen by Clementine. Science 266, 1851-1854.
  • T. Kohout, K. O’Sullivan, A. Losiak, K. G. Thaisen, S. Weider and D. A. Kring (2009) Scientific Opportunities for Human Exploration of the Moon’s Schrödinger Basin LPSC 40th #1572.