Al-Marrakushi (månkrater)
| Månkrater | ||
|---|---|---|
| Al-Marrakushi | ||
 | ||
| Egenskaper | ||
| Latitud Longitud | ||
| Medeldiameter | 8.57 km | |
| Djup | Okänt | |
| Kolongitud | 304° vid soluppgång | |
| Eponym | Ibn al-Banna al-Marrakushi | |
| Kartposition | ||
| Månen - Selenografi - ( ) | ||
 Hitta fler artiklar om Astronomi med Astronomiportalen | ||
Al-Marrakushi är en liten isolerad nedslagskrater som ligger i den östra delen av Mare Fecunditatis på månen. Den är en cirkulär, symmetrisk formation med inre kraterväggar som sluttar ned mot mittpunkten. Till nordöst är den framträdande kratern Langrenus. Månhavet (eng. Lunar mare) nära Al-Marrakushi är markerat av material som blev utkastat från dess större grannar när dessa bildades.
Kratern identifierades som Langrenus D tills den gavs ett namn av IAU. Den döptes efter den marockansk-arabiske matematikern, astronomen och islamologen Ibn al-Banna al-Marrakushi (cirka 1256-cirka 1321).
Se även
Källor
- Artikeln är, helt eller delvis, en översättning från engelskspråkiga Wikipedia.
- ”Al-Marrakushi on Moon” (på engelska). International Astronomical Union. 18 oktober 2010. https://planetarynames.wr.usgs.gov/Feature/150. Läst 11 mars 2023.
Media som används på denna webbplats
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.
Red Dot.svg
Red dot, based on the image on en:.
Red dot, based on the image on en:.
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!) 
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.
Al-Marrakushi crater AS08-13-2215.jpg
Oblique view of Al-Marrakushi crater, on the moon, facing south. The clusters of small craters to the left and right are secondary craters from Langrenus crater.
Oblique view of Al-Marrakushi crater, on the moon, facing south. The clusters of small craters to the left and right are secondary craters from Langrenus crater.