Difference between revisions of "Ramsden"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =Ramsden= {| class="wiki_table" | Lat: 32.9°S, Long: 31.8°W, Diam: 25.1 km, Depth: 1.9 km, [/R%C3%BCkl%2063 R...")
 
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Lat: 32.9°S, Long: 31.8°W, Diam: 25.1 km, Depth: 1.9 km, [/R%C3%BCkl%2063 Rükl: 63]<br />
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Lat: 32.9°S, Long: 31.8°W, Diam: 25.1 km, Depth: 1.9 km, [[R%C3%BCkl%2063|Rükl: 63]]<br />
 
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<div id="toc">
 
<div id="toc">
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[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Ramsden LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Ramsden%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Ramsden Apollo Images]<br /> <br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Ramsden LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Ramsden%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Ramsden Apollo Images]<br /> <br />  
 
==Maps==
 
==Maps==
''([/LAC%20zone LAC zone] 111A2)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac111/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I824/ Geologic map]<br /> <br />  
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''([[LAC%20zone|LAC zone]] 111A2)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac111/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I824/ Geologic map]<br /> <br />  
 
==Description==
 
==Description==
 
<br />  
 
<br />  
 
==Description: Elger==
 
==Description: Elger==
''([/IAU%20Directions IAU Directions])'' RAMSDEN.--This ring-plain, 12 miles in diameter, derives its importance from the remarkable rill-system with which it is so closely associated. Its border, about 1,800 feet on the E. above the outside surface, is slightly terraced within on the W., where there is an unrecorded bright crater on the slope. The two principal clefts on the S. originate among the hills W. of [/Capuanus Capuanus]. The more westerly begins at a crater on the N. edge of these objects, and runs N. to the W. side of Ramsden; the other originates at a larger crater, and proceeds in a N. direction up to a bright little mountain S.E. of Ramsden; when, swerving to the N.W., it ends at the E. wall of this formation. This mountain is a centre or node from which three other more delicate branches radiate. On the N., three of the shortest clefts pertaining to the system are easily traceable from neighbouring mountains up to the N. wall, which they apparently partially cut through. The W. pair have a common origin, but open out as they approach the border of Ramsden.<br /> <br />  
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''([[IAU%20Directions|IAU Directions]])'' RAMSDEN.--This ring-plain, 12 miles in diameter, derives its importance from the remarkable rill-system with which it is so closely associated. Its border, about 1,800 feet on the E. above the outside surface, is slightly terraced within on the W., where there is an unrecorded bright crater on the slope. The two principal clefts on the S. originate among the hills W. of [[Capuanus|Capuanus]]. The more westerly begins at a crater on the N. edge of these objects, and runs N. to the W. side of Ramsden; the other originates at a larger crater, and proceeds in a N. direction up to a bright little mountain S.E. of Ramsden; when, swerving to the N.W., it ends at the E. wall of this formation. This mountain is a centre or node from which three other more delicate branches radiate. On the N., three of the shortest clefts pertaining to the system are easily traceable from neighbouring mountains up to the N. wall, which they apparently partially cut through. The W. pair have a common origin, but open out as they approach the border of Ramsden.<br /> <br />  
 
==Description: Wikipedia==
 
==Description: Wikipedia==
 
[http://en.wikipedia.org/wiki/Ramsden_(crater) Ramsden]<br /> <br />  
 
[http://en.wikipedia.org/wiki/Ramsden_(crater) Ramsden]<br /> <br />  
 
==Additional Information==
 
==Additional Information==
* Depth data from [/Kurt%20Fisher%20crater%20depths Kurt Fisher database]
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* Depth data from [[Kurt%20Fisher%20crater%20depths|Kurt Fisher database]]
 
** Pike, 1976: 1.9 km
 
** Pike, 1976: 1.9 km
 
** Arthur, 1974: 1.99 km
 
** Arthur, 1974: 1.99 km
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==Bibliography==
 
==Bibliography==
  
* Harold Hill. ''[/A%20Portfolio%20of%20Lunar%20Drawings A Portfolio of Lunar Drawings]'', pages 154, 155 (the western portion of [/Palus%20Epidemiarum Palus Epidemiarum]).
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* Harold Hill. ''[[A%20Portfolio%20of%20Lunar%20Drawings|A Portfolio of Lunar Drawings]]'', pages 154, 155 (the western portion of [[Palus%20Epidemiarum|Palus Epidemiarum]]).
 
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Revision as of 16:09, 15 April 2018

Ramsden

Lat: 32.9°S, Long: 31.8°W, Diam: 25.1 km, Depth: 1.9 km, Rükl: 63

Table of Contents

[#Ramsden Ramsden]
[#Ramsden-Ramsden - LRO Ramsden - LRO]
[#Ramsden-Images Images]
[#Ramsden-Maps Maps]
[#Ramsden-Description Description]
[#Ramsden-Description: Elger Description: Elger]
[#Ramsden-Description: Wikipedia Description: Wikipedia]
[#Ramsden-Additional Information Additional Information]
[#Ramsden-Nomenclature Nomenclature]
[#Ramsden-LPOD Articles LPOD Articles]
[#Ramsden-Bibliography Bibliography]
external image Ramsden-IV136-h3.jpg
LO IV-136-h3

ramsVOD mala.jpg

Ramsden - LRO

Images

LPOD Photo Gallery Lunar Orbiter Images Apollo Images

Maps

(LAC zone 111A2) LAC map Geologic map

Description


Description: Elger

(IAU Directions) RAMSDEN.--This ring-plain, 12 miles in diameter, derives its importance from the remarkable rill-system with which it is so closely associated. Its border, about 1,800 feet on the E. above the outside surface, is slightly terraced within on the W., where there is an unrecorded bright crater on the slope. The two principal clefts on the S. originate among the hills W. of Capuanus. The more westerly begins at a crater on the N. edge of these objects, and runs N. to the W. side of Ramsden; the other originates at a larger crater, and proceeds in a N. direction up to a bright little mountain S.E. of Ramsden; when, swerving to the N.W., it ends at the E. wall of this formation. This mountain is a centre or node from which three other more delicate branches radiate. On the N., three of the shortest clefts pertaining to the system are easily traceable from neighbouring mountains up to the N. wall, which they apparently partially cut through. The W. pair have a common origin, but open out as they approach the border of Ramsden.

Description: Wikipedia

Ramsden

Additional Information

  • Depth data from Kurt Fisher database
    • Pike, 1976: 1.9 km
    • Arthur, 1974: 1.99 km
    • Westfall, 2000: 1.9 km
    • Viscardy, 1985: 2 km
    • Cherrington, 1969: 1.79 km
  • The system of three rilles just north of Ramsden (which are almost typographically "N"-shaped), is an interesting target for telescope operators at public observatories! - DannyCaes DannyCaes Aug 4, 2009
  • Certain digital lunar atlases show totally wrong coordinates for Ramsden (or just "no" coordinates)(0° 00' N / 0° 00' E). The same phenomenon is noticeable at craterlet Priscilla. - DannyCaes DannyCaes Feb 15, 2010


Nomenclature

  • Named for Jesse Ramsden (October 6, 1735 - November 5, 1800), an English astronomical and scientific instrument maker. Ramsden's speciality was divided circles, which began to supersede the quadrants in observatories towards the end of the 18th century. Ramsden is also responsible for the achromatic eyepiece named after him.


LPOD Articles

How He Does It (the Ramsden/ Marth sector, by Leo Aerts).

Bibliography



This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx3u2