Difference between revisions of "Schrödinger-Zeeman Basin"
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| Lat: 81°S, Long: 165°W, Main ring diam: 250 km, Depth: km, Rukl:<br /> | | Lat: 81°S, Long: 165°W, Main ring diam: 250 km, Depth: km, Rukl:<br /> | ||
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| − | [http://www.lpod.org/coppermine/displayimage.php?pid=2347&fullsize=1 [[Image: | + | [http://www.lpod.org/coppermine/displayimage.php?pid=2347&fullsize=1 [[Image:Normal_Schrodinger-Zeeman_Basin_LIDAR_LTVT.JPG|external image normal_Schrodinger-Zeeman_Basin_LIDAR_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-2347 Clementine]''<br /> <br /> |
==Images== | ==Images== | ||
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Schrodinger-Zeeman 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]<br /> <br /> | [http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Schrodinger-Zeeman 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]<br /> <br /> | ||
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[http://www.lpi.usra.edu/meetings/moon99/pdf/8056.pdf Discovery paper]<br /> | [http://www.lpi.usra.edu/meetings/moon99/pdf/8056.pdf Discovery paper]<br /> | ||
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Latest revision as of 02:16, 16 April 2018
Contents
Schrödinger-Zeeman Basin
(unofficial name)| Lat: 81°S, Long: 165°W, Main ring diam: 250 km, Depth: km, Rukl: |
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images
Maps
(LAC zone 144B1)
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 |
| Proposed |
12 |
150, 250 km |
Description
Additional Information
Nomenclature
Basins filled with maria are named for the mare, and basins that were previously recognized as craters still bear the crater name. Basins located between craters have the names of the two opposite craters with a hyphen in between, in this case Schrödinger and Zeeman.
LPOD Articles
