Difference between revisions of "Cavendish"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =Cavendish= {| class="wiki_table" | Lat: 24.5°S, Long: 53.7°W, Diam: 56 km, Depth: 2.55 km, [/R%C3%BCkl%2051...")
 
 
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Lat: 24.5°S, Long: 53.7°W, Diam: 56 km, Depth: 2.55 km, [/R%C3%BCkl%2051 Rükl: 51]<br />
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Lat: 24.5°S, Long: 53.7°W, Diam: 56 km, Depth: 2.55 km, [[R%C3%BCkl%2051|Rükl: 51]]<br />
 
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=Table of Contents=
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[http://www.lpod.org/coppermine/albums/userpics/Cavendish_LO-IV-156H_LTVT.JPG [[Image:Normal_Cavendish_LO-IV-156H_LTVT.JPG|external image normal_Cavendish_LO-IV-156H_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-2007 LO-IV-156H]''<br />  Note the inconspicuous rille on the western part of '''Cavendish''''s floor, and also the system of rilles to the southeast of '''Cavendish'''. According to several sources they were called '''Rima Cavendish I''' and '''Rima Cavendish II''' (see section <u>Nomenclature</u> below).<br /> <br />  
<div style="margin-left: 1em">[#Cavendish Cavendish]</div><div style="margin-left: 2em">[#Cavendish-Images Images]</div><div style="margin-left: 2em">[#Cavendish-Maps Maps]</div><div style="margin-left: 2em">[#Cavendish-Description Description]</div><div style="margin-left: 2em">[#Cavendish-Description: Elger Description: Elger]</div><div style="margin-left: 2em">[#Cavendish-Description: Wikipedia Description: Wikipedia]</div><div style="margin-left: 2em">[#Cavendish-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Cavendish-Nomenclature Nomenclature]</div><div style="margin-left: 2em">[#Cavendish-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Cavendish-Bibliography Bibliography]</div></div>[http://www.lpod.org/coppermine/albums/userpics/Cavendish_LO-IV-156H_LTVT.JPG [[Image:normal_Cavendish_LO-IV-156H_LTVT.JPG|external image normal_Cavendish_LO-IV-156H_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-2007 LO-IV-156H]''<br />  Note the inconspicuous rille on the western part of '''Cavendish''''s floor, and also the system of rilles to the southeast of '''Cavendish'''. According to several sources they were called '''Rima Cavendish I''' and '''Rima Cavendish II''' (see section <u>Nomenclature</u> below).<br /> <br />  
 
 
==Images==
 
==Images==
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Cavendish LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Cavendish%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Cavendish Apollo Images]<br /> <br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Cavendish LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Cavendish%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Cavendish Apollo Images]<br /> <br />  
 
==Maps==
 
==Maps==
''([/LAC%20zone LAC zone] 92C2)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac92/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I755/ Geologic map]<br /> <br />  
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''([[LAC%20zone|LAC zone]] 92C2)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac92/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I755/ Geologic map]<br /> <br />  
 
==Description==
 
==Description==
 
<br />  
 
<br />  
 
==Description: Elger==
 
==Description: Elger==
''([/IAU%20Directions IAU Directions])'' CAVENDISH.--A notable ring-plain, 32 miles in diameter, S.W. of [/Mersenius Mersenius], with a prominently terraced border, rising at one point on the S. to a height of 6,000 feet above the interior, on which are a few low ridges. A large bright ring-plain (<u>e</u>), about 12 miles in diameter, breaks the continuity of the S.W. wall, and adjoining this, but beyond the limits of the formation, is another smaller ring with a central hill. There is also a bright crater on the N.E. border. The E. <u>glacis</u> is very broad, and includes two large shallow depressions. An especially fine valley runs up to the N. wall, to the E. side of <u>e</u>.<br /> <br />  
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''([[IAU%20directions|IAU Directions]])'' CAVENDISH.--A notable ring-plain, 32 miles in diameter, S.W. of [[Mersenius|Mersenius]], with a prominently terraced border, rising at one point on the S. to a height of 6,000 feet above the interior, on which are a few low ridges. A large bright ring-plain (<u>e</u>), about 12 miles in diameter, breaks the continuity of the S.W. wall, and adjoining this, but beyond the limits of the formation, is another smaller ring with a central hill. There is also a bright crater on the N.E. border. The E. <u>glacis</u> is very broad, and includes two large shallow depressions. An especially fine valley runs up to the N. wall, to the E. side of <u>e</u>.<br /> <br />  
 
==Description: Wikipedia==
 
==Description: Wikipedia==
 
[http://en.wikipedia.org/wiki/Cavendish_(crater) Cavendish]<br /> <br />  
 
[http://en.wikipedia.org/wiki/Cavendish_(crater) Cavendish]<br /> <br />  
 
==Additional Information==
 
==Additional Information==
  Depth data from [/Kurt%20Fisher%20crater%20depths Kurt Fisher database]<br />  
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  Depth data from [[Kurt%20Fisher%20Crater%20Depths|Kurt Fisher database]]<br />  
 
* Westfall, 2000: 2.55 km
 
* Westfall, 2000: 2.55 km
 
* Viscardy, 1985: 2.35 km
 
* Viscardy, 1985: 2.35 km
 
* Cherrington, 1969: 3.68 km
 
* Cherrington, 1969: 3.68 km
  
* Satellite crater Cavendish E is on the [/ALPO%20list%20of%20banded%20craters ALPO list of banded craters]
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* Satellite crater Cavendish E is on the [[ALPO%20list%20of%20banded%20craters|ALPO list of banded craters]]
 
* Inconspicuous rille on the western part of '''Cavendish''''s floor ('''Rima Cavendish'''?).
 
* Inconspicuous rille on the western part of '''Cavendish''''s floor ('''Rima Cavendish'''?).
 
<br />  
 
<br />  
 
==Nomenclature==
 
==Nomenclature==
  
* [http://en.wikipedia.org/wiki/Henry_Cavendish Henry Cavendish] (October 10, 1731 - February 24, 1810) was a British scientist noted for his discovery of hydrogen or what he called "inflammable air". He described the density of inflammable air, which formed water on combustion, in a 1766 paper "On Factitious Airs". Antoine [/Lavoisier Lavoisier] later reproduced Cavendish's experiment and gave the element its name. Cavendish is also credited with one of the earliest accurate calculations of the density of the earth.
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* [http://en.wikipedia.org/wiki/Henry_Cavendish Henry Cavendish] (October 10, 1731 - February 24, 1810) was a British scientist noted for his discovery of hydrogen or what he called "inflammable air". He described the density of inflammable air, which formed water on combustion, in a 1766 paper "On Factitious Airs". Antoine [[Lavoisier|Lavoisier]] later reproduced Cavendish's experiment and gave the element its name. Cavendish is also credited with one of the earliest accurate calculations of the density of the earth.
* '''Rima Cavendish''' (a name from a daily explorer of the lunar surface for the inconspicuous rille on the western part of the floor of [http://the-moon.wikispaces.com/Cavendish Cavendish]).
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* '''Rima Cavendish''' (a name from a daily explorer of the lunar surface for the inconspicuous rille on the western part of the floor of [http://the-moon.us/wiki/Cavendish Cavendish]).
* '''Rimae Cavendish''' ('''I''' and '''II'''). Chart 78 in the ''Times Atlas of the Moon'' shows '''Rima Cavendish I''' and '''Rima Cavendish II''' between '''Cavendish, de Gasparis,''' and '''de Gasparis B'''. See also [https://www.lpi.usra.edu/resources/mapcatalog/LAC/lac92/150dpi.jpg LAC 92]''',''' and also Chart [http://the-moon.wikispaces.com/SLC-F6 SLC-F6] in the ''System of Lunar Craters''. The LPI's red-labeled scan of Lunar Orbiter IV frame [https://www.lpi.usra.edu/resources/lunar_orbiter/images/aimg/iv_156_h1.jpg LOIV-156-h1] shows them as members of the '''Rimae de Gasparis''' system.
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* '''Rimae Cavendish''' ('''I''' and '''II'''). Chart 78 in the ''Times Atlas of the Moon'' shows '''Rima Cavendish I''' and '''Rima Cavendish II''' between '''Cavendish, de Gasparis,''' and '''de Gasparis B'''. See also [https://www.lpi.usra.edu/resources/mapcatalog/LAC/lac92/150dpi.jpg LAC 92]''',''' and also Chart [http://the-moon.us/wiki/SLC-F6 SLC-F6] in the ''System of Lunar Craters''. The LPI's red-labeled scan of Lunar Orbiter IV frame [https://www.lpi.usra.edu/resources/lunar_orbiter/images/aimg/iv_156_h1.jpg LOIV-156-h1] shows them as members of the '''Rimae de Gasparis''' system.
 
* '''Rimae Cavendish I''' and '''II''' are also mentioned in Tony Dethier's ''Maanmonografieen'', page 237 (V'''.'''V'''.'''S'''.,''' Vereniging Voor Sterrenkunde, 1989).
 
* '''Rimae Cavendish I''' and '''II''' are also mentioned in Tony Dethier's ''Maanmonografieen'', page 237 (V'''.'''V'''.'''S'''.,''' Vereniging Voor Sterrenkunde, 1989).
 
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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 - ''afx3u2''</div>
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Latest revision as of 02:44, 16 April 2018

Cavendish

Lat: 24.5°S, Long: 53.7°W, Diam: 56 km, Depth: 2.55 km, Rükl: 51

external image normal_Cavendish_LO-IV-156H_LTVT.JPG
LO-IV-156H
Note the inconspicuous rille on the western part of Cavendish's floor, and also the system of rilles to the southeast of Cavendish. According to several sources they were called Rima Cavendish I and Rima Cavendish II (see section Nomenclature below).

Images

LPOD Photo Gallery Lunar Orbiter Images Apollo Images

Maps

(LAC zone 92C2) LAC map Geologic map

Description


Description: Elger

(IAU Directions) CAVENDISH.--A notable ring-plain, 32 miles in diameter, S.W. of Mersenius, with a prominently terraced border, rising at one point on the S. to a height of 6,000 feet above the interior, on which are a few low ridges. A large bright ring-plain (e), about 12 miles in diameter, breaks the continuity of the S.W. wall, and adjoining this, but beyond the limits of the formation, is another smaller ring with a central hill. There is also a bright crater on the N.E. border. The E. glacis is very broad, and includes two large shallow depressions. An especially fine valley runs up to the N. wall, to the E. side of e.

Description: Wikipedia

Cavendish

Additional Information

Depth data from Kurt Fisher database
  • Westfall, 2000: 2.55 km
  • Viscardy, 1985: 2.35 km
  • Cherrington, 1969: 3.68 km
  • Satellite crater Cavendish E is on the ALPO list of banded craters
  • Inconspicuous rille on the western part of Cavendish's floor (Rima Cavendish?).


Nomenclature

  • Henry Cavendish (October 10, 1731 - February 24, 1810) was a British scientist noted for his discovery of hydrogen or what he called "inflammable air". He described the density of inflammable air, which formed water on combustion, in a 1766 paper "On Factitious Airs". Antoine Lavoisier later reproduced Cavendish's experiment and gave the element its name. Cavendish is also credited with one of the earliest accurate calculations of the density of the earth.
  • Rima Cavendish (a name from a daily explorer of the lunar surface for the inconspicuous rille on the western part of the floor of Cavendish).
  • Rimae Cavendish (I and II). Chart 78 in the Times Atlas of the Moon shows Rima Cavendish I and Rima Cavendish II between Cavendish, de Gasparis, and de Gasparis B. See also LAC 92, and also Chart SLC-F6 in the System of Lunar Craters. The LPI's red-labeled scan of Lunar Orbiter IV frame LOIV-156-h1 shows them as members of the Rimae de Gasparis system.
  • Rimae Cavendish I and II are also mentioned in Tony Dethier's Maanmonografieen, page 237 (V.V.S., Vereniging Voor Sterrenkunde, 1989).


LPOD Articles


Bibliography