Difference between revisions of "Rupes Toscanelli"
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| − | + | [http://www.lpod.org/coppermine/albums/userpics/Rupes-Toscanelli_LO-IV-151H_LTVT.JPG [[Image:normal_Rupes-Toscanelli_LO-IV-151H_LTVT.JPG|external image normal_Rupes-Toscanelli_LO-IV-151H_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-2819 LO-IV-151H]'' This [[Lunar%20Orbiter|Lunar Orbiter]] view extends from the 8-km circular crater [[V%C3%A4is%C3%A4l%C3%A4|Väisälä]] in the lower left to 22-km [[Krieger|Krieger]] in the upper right. To the right of [[V%C3%A4is%C3%A4l%C3%A4|Väisälä]] is 7-km '''[[Aristarchus|Aristarchus]] B'''. '''Rupes Toscanelli''' is the ridge extending north from '''[[Aristarchus|Aristarchus]] B''' through 7-km [[Toscanelli|Toscanelli]] and a little beyond it. Much of the view is filled with rilles, most of which are probably regarded as part of the [[Rimae%20Aristarchus|Rimae Aristarchus]] system. The sunlit arc in the lower right corner is part of the northwest rim of 46-km [[Prinz|Prinz]]. The bright sharp-edged half-circles scattered over the frame are defects in the film development.<br /> <br /> | |
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==Images== | ==Images== | ||
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Rupes%20Toscanelli LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Rupes%20Toscanelli%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Rupes%20Toscanelli Apollo Images]<br /> <br /> | [http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Rupes%20Toscanelli LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Rupes%20Toscanelli%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Rupes%20Toscanelli Apollo Images]<br /> <br /> | ||
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''([[LAC%20zone|LAC zone]] 39A4)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac39/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I465/ Geologic map] [http://www.lpi.usra.edu/resources/mapcatalog/LM/lm39/ LM map] [http://www.lpi.usra.edu/resources/mapcatalog/LTO/lto39a4_1/ LTO map]<br /> <br /> | ''([[LAC%20zone|LAC zone]] 39A4)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac39/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I465/ Geologic map] [http://www.lpi.usra.edu/resources/mapcatalog/LM/lm39/ LM map] [http://www.lpi.usra.edu/resources/mapcatalog/LTO/lto39a4_1/ LTO map]<br /> <br /> | ||
==Description== | ==Description== | ||
| − | The small number of named lunar faults are places where the lunar crust has moved vertically, creating a scarp. Rupes Toscanelli does not appear to be a fault like the others. It has a rounded surface rather than a scarp and appears to be a mare ridge with a slightly steep edge. Its curvature is more like a ridge than a vertical fault too. In any case it is too insignificant a feature to warrant a name, especially one that is a wrong classification. <span class="membersnap">- | + | The small number of named lunar faults are places where the lunar crust has moved vertically, creating a scarp. Rupes Toscanelli does not appear to be a fault like the others. It has a rounded surface rather than a scarp and appears to be a mare ridge with a slightly steep edge. Its curvature is more like a ridge than a vertical fault too. In any case it is too insignificant a feature to warrant a name, especially one that is a wrong classification. <span class="membersnap">- tychocrater <small>Nov 24, 2007</small></span><br /> <br /> |
==Description: Wikipedia== | ==Description: Wikipedia== | ||
[http://en.wikipedia.org/wiki/Toscanelli_%28crater%29 Rupes Toscanelli]<br /> <br /> | [http://en.wikipedia.org/wiki/Toscanelli_%28crater%29 Rupes Toscanelli]<br /> <br /> | ||
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Revision as of 17:47, 15 April 2018
Contents
Rupes Toscanelli
|
Lat: 27.4°N, Long: 47.5°W, Length: 70 km, Height: km, Rükl: 18 |
LO-IV-151H This Lunar Orbiter view extends from the 8-km circular crater Väisälä in the lower left to 22-km Krieger in the upper right. To the right of Väisälä is 7-km Aristarchus B. Rupes Toscanelli is the ridge extending north from Aristarchus B through 7-km Toscanelli and a little beyond it. Much of the view is filled with rilles, most of which are probably regarded as part of the Rimae Aristarchus system. The sunlit arc in the lower right corner is part of the northwest rim of 46-km Prinz. The bright sharp-edged half-circles scattered over the frame are defects in the film development.
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images
Maps
(LAC zone 39A4) LAC map Geologic map LM map LTO map
Description
The small number of named lunar faults are places where the lunar crust has moved vertically, creating a scarp. Rupes Toscanelli does not appear to be a fault like the others. It has a rounded surface rather than a scarp and appears to be a mare ridge with a slightly steep edge. Its curvature is more like a ridge than a vertical fault too. In any case it is too insignificant a feature to warrant a name, especially one that is a wrong classification. - tychocrater Nov 24, 2007
Description: Wikipedia
Additional Information
Nomenclature
Named from nearby crater. (Toscanelli)
LPOD Articles
Bibliography
