Difference between revisions of "Wrottesley"

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Lat: 23.9°S, Long: 56.8°E, Diam: 57 km, Depth: 4.23 km, [/R%C3%BCkl%2059 Rükl: 59]<br />
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Lat: 23.9°S, Long: 56.8°E, Diam: 57 km, Depth: 4.23 km, [[R%C3%BCkl%2059|Rükl: 59]]<br />
 
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[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Wrottesley LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Wrottesley%7C0 Lunar Orbiter Images]<br /> '''Wrottesley''' was photographed by Apollo 15's orbital Mapping/Metric ''Fairchild'' camera. This crater near '''Petavius''' is visible on Apollo 15's south looking oblique photographs. One such ''Fairchild'' frame is [http://www.lpi.usra.edu/resources/apollo/frame/?AS15-M-2527 AS15-M-2527], in which '''Wrottesley''' was captured near the central part of the depicted curved horizon.<br />  Research Danny Caes<br /> <br />  
 
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Wrottesley LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Wrottesley%7C0 Lunar Orbiter Images]<br /> '''Wrottesley''' was photographed by Apollo 15's orbital Mapping/Metric ''Fairchild'' camera. This crater near '''Petavius''' is visible on Apollo 15's south looking oblique photographs. One such ''Fairchild'' frame is [http://www.lpi.usra.edu/resources/apollo/frame/?AS15-M-2527 AS15-M-2527], in which '''Wrottesley''' was captured near the central part of the depicted curved horizon.<br />  Research Danny Caes<br /> <br />  
 
==Maps==
 
==Maps==
''([/LAC%20zone LAC zone] 98A3)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac98/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I794/ Geologic map]<br /> <br />  
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''([[LAC%20zone|LAC zone]] 98A3)'' [http://www.lpi.usra.edu/resources/mapcatalog/LAC/lac98/ LAC map] [http://www.lpi.usra.edu/resources/mapcatalog/usgs/I794/ Geologic map]<br /> <br />  
 
==Description==
 
==Description==
 
<br />  
 
<br />  
 
==Description: Elger==
 
==Description: Elger==
''([/IAU%20Directions IAU Directions])'' WROTTESLEY.--A formation, about 25 miles in diameter, closely associated with the W. wall of [/Petavius Petavius], the shape of which it has clearly modified. Its border on the W., of the linear type, rises nearly 9,000 feet above a light interior, where there is a small bright central mountain and some mounds. There is a prominent valley running along the inner slope of the E. wall.<br /> <br />  
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''([[IAU%20Directions|IAU Directions]])'' WROTTESLEY.--A formation, about 25 miles in diameter, closely associated with the W. wall of [[Petavius|Petavius]], the shape of which it has clearly modified. Its border on the W., of the linear type, rises nearly 9,000 feet above a light interior, where there is a small bright central mountain and some mounds. There is a prominent valley running along the inner slope of the E. wall.<br /> <br />  
 
==Description: Wikipedia==
 
==Description: Wikipedia==
 
[http://en.wikipedia.org/wiki/Wrottesley_(crater) Wrottesley]<br /> <br />  
 
[http://en.wikipedia.org/wiki/Wrottesley_(crater) Wrottesley]<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]]
 
** Westfall, 2000: 4.23 km
 
** Westfall, 2000: 4.23 km
 
** Viscardy, 1985: 2.3 km
 
** Viscardy, 1985: 2.3 km
 
** Cherrington, 1969: 3.44 km
 
** Cherrington, 1969: 3.44 km
 
* Central Peak Height
 
* Central Peak Height
** [/Sekiguchi%2C%201972 Sekiguchi, 1972]: 1.4 km <span class="membersnap">- [http://www.wikispaces.com/user/view/fatastronomer [[Image:fatastronomer-lg.jpg|16px|fatastronomer]]] [http://www.wikispaces.com/user/view/fatastronomer fatastronomer]</span>
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** [[Sekiguchi%2C%201972|Sekiguchi, 1972]]: 1.4 km <span class="membersnap">- [http://www.wikispaces.com/user/view/fatastronomer [[Image:fatastronomer-lg.jpg|16px|fatastronomer]]] [http://www.wikispaces.com/user/view/fatastronomer fatastronomer]</span>
 
<br />  
 
<br />  
 
==Nomenclature==
 
==Nomenclature==
  
 
* Named for [http://en.wikipedia.org/wiki/John_Wrottesley,_2nd_Baron_Wrottesley John (Baron) Wrottesley] (1798-1867), a British astronomer.
 
* Named for [http://en.wikipedia.org/wiki/John_Wrottesley,_2nd_Baron_Wrottesley John (Baron) Wrottesley] (1798-1867), a British astronomer.
* The name was proposed by British amateur [/Birt W. R. Birt] in [http://adsabs.harvard.edu/abs/1863AReg....1..169B 1863], in commemoration of the interest the Baron had shown in astronomy.
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* The name was proposed by British amateur [[Birt|W. R. Birt]] in [http://adsabs.harvard.edu/abs/1863AReg....1..169B 1863], in commemoration of the interest the Baron had shown in astronomy.
 
<br />  
 
<br />  
 
==LPOD Articles==
 
==LPOD Articles==

Revision as of 15:23, 15 April 2018

Wrottesley

Lat: 23.9°S, Long: 56.8°E, Diam: 57 km, Depth: 4.23 km, Rükl: 59

Table of Contents

[#Wrottesley Wrottesley]
[#Wrottesley-Images Images]
[#Wrottesley-Maps Maps]
[#Wrottesley-Description Description]
[#Wrottesley-Description: Elger Description: Elger]
[#Wrottesley-Description: Wikipedia Description: Wikipedia]
[#Wrottesley-Additional Information Additional Information]
[#Wrottesley-Nomenclature Nomenclature]
[#Wrottesley-LPOD Articles LPOD Articles]
[#Wrottesley-Bibliography Bibliography]
external image normal_Petavius_19_10_2005.jpg
George Tasroudis (Wrottesley is crater in front of Petavius)

Images

LPOD Photo Gallery Lunar Orbiter Images
Wrottesley was photographed by Apollo 15's orbital Mapping/Metric Fairchild camera. This crater near Petavius is visible on Apollo 15's south looking oblique photographs. One such Fairchild frame is AS15-M-2527, in which Wrottesley was captured near the central part of the depicted curved horizon.
Research Danny Caes

Maps

(LAC zone 98A3) LAC map Geologic map

Description


Description: Elger

(IAU Directions) WROTTESLEY.--A formation, about 25 miles in diameter, closely associated with the W. wall of Petavius, the shape of which it has clearly modified. Its border on the W., of the linear type, rises nearly 9,000 feet above a light interior, where there is a small bright central mountain and some mounds. There is a prominent valley running along the inner slope of the E. wall.

Description: Wikipedia

Wrottesley

Additional Information


Nomenclature

  • Named for John (Baron) Wrottesley (1798-1867), a British astronomer.
  • The name was proposed by British amateur W. R. Birt in 1863, in commemoration of the interest the Baron had shown in astronomy.


LPOD Articles

Trenchent observations of a Trench Uninspiring, but an Active History Limb Gift

Bibliography

A Portfolio of Lunar Drawings (Harold Hill), page 216 (the Biot region).


This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - afx2u2