Difference between revisions of "Volta"
(Created page with "<div id="content_view" class="wiki" style="display: block"> =Volta= {| class="wiki_table" | Lat: 53.9°N, Long: 84.4°W, Diam: 123 km, Depth: 3.0 km, [/R%C3%BCkl%201 Rükl...") |
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| − | Lat: 53.9°N, Long: 84.4°W, Diam: 123 km, Depth: 3.0 km, [ | + | Lat: 53.9°N, Long: 84.4°W, Diam: 123 km, Depth: 3.0 km, [[R%C3%BCkl%201|Rükl: 1]], [[Stratigraphy|pre-Nectarian]]<br /> |
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<div id="toc"> | <div id="toc"> | ||
| − | + | [http://www.lpod.org/coppermine/albums/userpics/Volta-Repsold_LO-IV-188M_LTVT.JPG [[Image:Normal_Volta-Repsold_LO-IV-188M_LTVT.JPG|external image normal_Volta-Repsold_LO-IV-188M_LTVT.JPG]]]<br /> ''[http://lpod.org/coppermine/displayimage.php?pos=-2814 LO-IV-188M]'' The IAU-approved feature names in this medium resolution [[Lunar%20Orbiter|Lunar Orbiter]] view include: '''Volta''', [[Repsold|Repsold]], [[Regnault|Regnault]], [[Stokes|Stokes]], [[Langley|Langley]], [[Galvani|Galvani]], and [[Rimae%20Repsold|Rimae Repsold]].<br /> [[Image:Volta-LRObigShadows.jpg|Volta-LRObigShadows.jpg]]<br /> [[Image:Volta-LRO.jpg|Volta-LRO.jpg]]<br /> LRO images. Regnault, cutting Volta's western rim, has a Pac-Man shadow.<br /> <br /> | |
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==Images== | ==Images== | ||
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Volta LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Volta%7C0 Lunar Orbiter Images]<br /> <br /> | [http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Volta LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Volta%7C0 Lunar Orbiter Images]<br /> <br /> | ||
==Maps== | ==Maps== | ||
| − | ''([ | + | ''([[LAC%20zone|LAC zone]] 21C2)'' [http://planetarynames.wr.usgs.gov/images/Lunar/lac_21.pdf USGS Digital Atlas PDF]<br /> <br /> |
==Description== | ==Description== | ||
Large, smooth-floored crater crossed by numerous rilles. The fact that the entire floor is domed up 275 m implies that rilles may be expansion cracks generated by doming. Amazingly, the floor of Regnault is part of the broad domed area of Volta - both craters are domed.<br /> Why do many of the craters west of Oceanus Procellarum have rilled-floors? This is probably the largest area of rilles on the Moon.<br /> <br /> | Large, smooth-floored crater crossed by numerous rilles. The fact that the entire floor is domed up 275 m implies that rilles may be expansion cracks generated by doming. Amazingly, the floor of Regnault is part of the broad domed area of Volta - both craters are domed.<br /> Why do many of the craters west of Oceanus Procellarum have rilled-floors? This is probably the largest area of rilles on the Moon.<br /> <br /> | ||
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[http://en.wikipedia.org/wiki/Volta_(crater) Volta]<br /> <br /> | [http://en.wikipedia.org/wiki/Volta_(crater) Volta]<br /> <br /> | ||
==Additional Information== | ==Additional Information== | ||
| − | Depth data from [ | + | Depth data from [[Kurt%20Fisher%20Crater%20Depths|Kurt Fisher database]]<br /> |
* Westfall, 2000: 3.58 km | * Westfall, 2000: 3.58 km | ||
<br /> From LRO altimetry, depth varies from 2.7 to about 3,2 km, and central peak height 590 m. (CAW)<br /> Entire floor domed up about 275 m (CAW)<br /> <br /> | <br /> From LRO altimetry, depth varies from 2.7 to about 3,2 km, and central peak height 590 m. (CAW)<br /> Entire floor domed up about 275 m (CAW)<br /> <br /> | ||
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* Count Allessandro Guiseppe Antonio Anastasio Volta; Italian physicist (1745-1827). | * Count Allessandro Guiseppe Antonio Anastasio Volta; Italian physicist (1745-1827). | ||
| − | * Name originally proposed by [ | + | * Name originally proposed by [[Schmidt|Schmidt]] but not in ''[[Named%20Lunar%20Formations|Named Lunar Formations]]''; shifted to a different crater in ''[[Rectified%20Lunar%20Atlas|Rectified Lunar Atlas]]'' (1963) and approved by IAU in 1964 ([[Whitaker|Whitaker]], 1999, pp. 224 and 235). |
* '''''Rimae Volta''''' (an unofficial name from D.Caes for the system of rilles on the floor of '''Volta'''). | * '''''Rimae Volta''''' (an unofficial name from D.Caes for the system of rilles on the floor of '''Volta'''). | ||
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Latest revision as of 03:21, 16 April 2018
Contents
Volta
|
Lat: 53.9°N, Long: 84.4°W, Diam: 123 km, Depth: 3.0 km, Rükl: 1, pre-Nectarian |
LO-IV-188M The IAU-approved feature names in this medium resolution Lunar Orbiter view include: Volta, Repsold, Regnault, Stokes, Langley, Galvani, and Rimae Repsold.
LRO images. Regnault, cutting Volta's western rim, has a Pac-Man shadow.
Images
LPOD Photo Gallery Lunar Orbiter Images
Maps
(LAC zone 21C2) USGS Digital Atlas PDF
Description
Large, smooth-floored crater crossed by numerous rilles. The fact that the entire floor is domed up 275 m implies that rilles may be expansion cracks generated by doming. Amazingly, the floor of Regnault is part of the broad domed area of Volta - both craters are domed.
Why do many of the craters west of Oceanus Procellarum have rilled-floors? This is probably the largest area of rilles on the Moon.
Description: Wikipedia
Additional Information
Depth data from Kurt Fisher database
- Westfall, 2000: 3.58 km
From LRO altimetry, depth varies from 2.7 to about 3,2 km, and central peak height 590 m. (CAW)
Entire floor domed up about 275 m (CAW)
Nomenclature
- Count Allessandro Guiseppe Antonio Anastasio Volta; Italian physicist (1745-1827).
- Name originally proposed by Schmidt but not in Named Lunar Formations; shifted to a different crater in Rectified Lunar Atlas (1963) and approved by IAU in 1964 (Whitaker, 1999, pp. 224 and 235).
- Rimae Volta (an unofficial name from D.Caes for the system of rilles on the floor of Volta).
LPOD Articles
Bibliography
