Difference between revisions of "Cavendish"
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| − | [http://www.lpod.org/coppermine/albums/userpics/Cavendish_LO-IV-156H_LTVT.JPG [[Image: | + | [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 /> | ||
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==Description: Elger== | ==Description: Elger== | ||
| − | ''([[IAU% | + | ''([[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% | + | 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 | ||
Latest revision as of 01:44, 16 April 2018
Contents
Cavendish
|
Lat: 24.5°S, Long: 53.7°W, Diam: 56 km, Depth: 2.55 km, Rükl: 51 |
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
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
