Difference between revisions of "Kirchhoff"
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| − | + | [http://www.lpod.org/coppermine/albums/userpics/Kirchhoff-LOIV-074-H1.jpg [[Image:Kirchhoff-LOIV-074-H1.jpg|external image Kirchhoff-LOIV-074-H1.jpg]]]''[http://lpod.org/coppermine/displayimage.php?pos=-241 LOIV-074-H1]''<br /> <br /> | |
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==Images== | ==Images== | ||
[http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Kirchhoff LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Kirchhoff%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Kirchhoff Apollo Images]<br /> <br /> | [http://www.lpod.org/coppermine/thumbnails.php?album=search&type=full&search=Kirchhoff LPOD Photo Gallery] [http://www.lpi.usra.edu/resources/lunar_orbiter/bin/srch_nam.shtml?Kirchhoff%7C0 Lunar Orbiter Images] [http://www.lpi.usra.edu/resources/apollo/search/feature/?feature=Kirchhoff Apollo Images]<br /> <br /> | ||
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[http://en.wikipedia.org/wiki/Kirchhoff_(crater) Kirchhoff]<br /> <br /> | [http://en.wikipedia.org/wiki/Kirchhoff_(crater) Kirchhoff]<br /> <br /> | ||
==Additional Information== | ==Additional Information== | ||
| − | Depth data from [[Kurt%20Fisher% | + | Depth data from [[Kurt%20Fisher%20Crater%20Depths|Kurt Fisher database]]<br /> |
* Arthur, 1974: 2.59 km | * Arthur, 1974: 2.59 km | ||
* Westfall, 2000: 2.59 km | * Westfall, 2000: 2.59 km | ||
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Latest revision as of 01:55, 16 April 2018
Contents
Kirchhoff
|
Lat: 30.3°N, Long: 38.8°E, Diam: 24 km, Depth: 2.59 km, Rükl: 15 |
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images
Maps
(LAC zone 43A2) LAC map Geologic map
Description
Description: Wikipedia
Additional Information
Depth data from Kurt Fisher database
- Arthur, 1974: 2.59 km
- Westfall, 2000: 2.59 km
- Viscardy, 1985: 2.59 km
Nomenclature
Gustav Kirchhoff (March 12, 1824 - October 17, 1887) was a German physicist who, with Robert Bunsen, established the theory of spectrum analysis (a technique for chemical analysis by analyzing the light emitted by a heated material), which Kirchhoff applied to determine the composition of the Sun. He found that when light passes through a gas, the gas absorbs those wavelengths that it would emit if heated, which explained the numerous dark lines (Fraunhofer lines) in the Sun's spectrum.
LPOD Articles
Bibliography
