Hubble Space Telescope: Kepler's Supernova Remnant (visible-light data)
As the shock ploughs into material lost from the progenitor star after the initial supernova explosion, instabilities left in its wake cause the swept-up gas to fragment into clumps. The Hubble data also show thin filaments of gas. These filaments reveal where the shock wave is encountering lower-density, more uniform interstellar material.
About the Image
About the Object
| Name: | Kepler's SN |
|---|---|
| Type: | Milky Way : Nebula : Type : Supernova Remnant |
| Distance: | 13000 light years |
| Constellation: | Ophiuchus |
| Category: | Nebulae |
Classic Wallpapers
Coordinates
| Position (RA): | 17 30 41.05 |
|---|---|
| Position (Dec): | -21° 29' 30.39" |
| Field of view: | 4.86 x 4.86 arcminutes |
| Orientation: | North is 0.0° right of vertical |
Colours & filters
| Band | Telescope |
|---|---|
| Optical |
Hubble Space Telescope
ACS |
| Optical |
Hubble Space Telescope
WFPC2 |

