Distant galaxies behind NGC 300
An area in the outer regions of NGC 300. Disks of spiral galaxies are usually quite "thin" (some hundred light-years), as compared to their radial extent (tens of thousands of light-years across). In areas where only small amounts of dust are present, it is possible to see much more distant galaxies right through the disk of NGC 300, as demonstrated by this image.
Credit:
ESO
About the Image
| Id: | eso0221g |
| Type: | Observation |
| Release date: | 7 August 2002 |
| Related releases: | eso0221 |
| Size: | 1055 x 797 px |
About the Object
| Name: | NGC 300 |
| Type: | • Local Universe : Galaxy : Type : Spiral • X - Galaxies |
| Distance: | 6 million light years |
Coordinates
| Position (RA): | 0h 54m 53.56s |
| Position (Dec): | -37° 41' 4.10" |
| Field of view: | 4.17 x 3.15 arcminutes |
| Orientation: | North is 0.2° left of vertical |
View in Worldwide Telescope:
Colours & filters
| Band | Telescope |
| Optical B |
MPG/ESO 2.2-metre telescope WFI |
| Optical V |
MPG/ESO 2.2-metre telescope WFI |
| Optical R |
MPG/ESO 2.2-metre telescope WFI |
| Optical H-alpha |
MPG/ESO 2.2-metre telescope WFI |
Images
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