Delaunay (månkrater)
| Månkrater | ||
|---|---|---|
| Delaunay | ||
 | ||
| Egenskaper | ||
| Latitud Longitud | ||
| Medeldiameter | 44.63 km | |
| Djup | 1.9 km | |
| Kolongitud | 358° vid soluppgång | |
| Eponym | Charles-Eugène Delaunay | |
| Kartposition | ||
| Månen - Selenografi - ( ) | ||
Delaunay är en nedslagskrater på månen. Delaunay har fått sitt namn efter den franske astronomen och matematikern Charles-Eugène Delaunay.
Kratern har en diameter på ungefär 44 km.
Satellitkratrar
| Delaunay | Latitud | Longitud | Diameter |
|---|---|---|---|
| A | 21.9° S | 2.0° Ö | 6 km |
Se även
Källor
- ”Delaunay on Moon” (på engelska). International Astronomical Union. 18 oktober 2010. https://planetarynames.wr.usgs.gov/Feature/1468. Läst 21 januari 2024.
Media som används på denna webbplats
FullMoon2010.jpg
(c) Gregory H. Revera, CC BY-SA 3.0
Full Moon photograph taken 10-22-2010 from Madison, Alabama, USA. Photographed with a Celestron 9.25 Schmidt-Cassegrain telescope. Acquired with a Canon EOS Rebel T1i (EOS 500D), 20 images stacked to reduce noise. 200 ISO 1/640 sec.
(c) Gregory H. Revera, CC BY-SA 3.0
Full Moon photograph taken 10-22-2010 from Madison, Alabama, USA. Photographed with a Celestron 9.25 Schmidt-Cassegrain telescope. Acquired with a Canon EOS Rebel T1i (EOS 500D), 20 images stacked to reduce noise. 200 ISO 1/640 sec.
Red Dot.svg
Red dot, based on the image on en:.
Red dot, based on the image on en:.
Moonmap from clementine data.png
cylindrical map projection of the Moon. The Moon's whole surface was mapped by the Clementine spacecraft in 1994, here North is at the top. The dark floor of crater Plato is at the middle top above Mare Imbrium, while the bright floor and rays of crater Tycho is near the middle bottom below Mare Imbrium. Mare Procellarum is at the near left, and Mare Tranquillitatis is just right of centre and Mare Crisium is at the near right. The far left and far right show the contrast of the mostly cratered farside with small isolated mare.
cylindrical map projection of the Moon. The Moon's whole surface was mapped by the Clementine spacecraft in 1994, here North is at the top. The dark floor of crater Plato is at the middle top above Mare Imbrium, while the bright floor and rays of crater Tycho is near the middle bottom below Mare Imbrium. Mare Procellarum is at the near left, and Mare Tranquillitatis is just right of centre and Mare Crisium is at the near right. The far left and far right show the contrast of the mostly cratered farside with small isolated mare.