Celsius (månkrater)
- För andra betydelser, se Celsius (olika betydelser).
| Månkrater | ||
|---|---|---|
| Celsius | ||
_02.jpg) | ||
| Egenskaper | ||
| Latitud Longitud | ||
| Medeldiameter | 36 km | |
| Djup | 1.5 km | |
| Kolongitud | 341° vid soluppgång | |
| Eponym | Anders Celsius | |
| Kartposition | ||
| Månen - Selenografi - ( ) | ||
 Hitta fler artiklar om Astronomi med Astronomiportalen | ||
Celsius är en liten nedslagskrater på månen som är belägen i den bergiga terrängen på den sydöstra delen av den sida av månen som vetter mot Jorden.
Kratern Celsius har oregelbundna kanter och en mindre krater i sin norra del. Nordost om Celsius ligger kratern Zagut, österut kratern Rabi Levi, en liten bit längre söderut kratern Büsching. Det finns inga månhav eller stora bergskedjor i närheten.
Kratern har fått namnet Celsius efter den svenske vetenskapsmannen Anders Celsius.
Satellitkratrar
| Celsius | Latitud | Longitud | Diameter |
|---|---|---|---|
| A | 33.0° S | 20.5° E | 14 km |
| B | 34.6° S | 19.7° E | 6 km |
| D | 34.7° S | 19.1° E | 19 km |
| E | 32.9° S | 20.1° E | 11 km |
| H | 33.8° S | 20.1° E | 6 km |
Se även
- Lista över månens kratrar
- Lista över månens berg
- Lista över månens hav
- 4169 Celsius
Källor
- Rükl, Antonín, Mondatlas, Prag 1990
- ”Celsius on Moon” (på engelska). International Astronomical Union. 18 oktober 2010. https://planetarynames.wr.usgs.gov/Feature/1098. Läst 9 augusti 2018.
Media som används på denna webbplats
Q space.svg
Författare/Upphovsman: Rursus, Licens: CC BY-SA 3.0
Replacement for faulty
(note the ring "around" Saturn!)
Författare/Upphovsman: Rursus, Licens: CC BY-SA 3.0
Replacement for faulty
(note the ring "around" Saturn!)
Celsius (LROC WAC-Lola) 02.jpg
Cráter Celsius (LROC WAC-Lola)
Cráter Celsius (LROC WAC-Lola)
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.
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.