Hubble image archive
Shock Wave in Kepler's Supernova Remnant
Detailed knots and filamentary ribbons of glowing gas are apparent in this Hubble Space Telescope image of Kepler's supernova remnant. This image was taken with Hubble's Advanced Camera for Surveys (ACS) in August 2003. Filters onboard Hubble isolate visible light emitted by hydr...
- Date
- Jan 1, 2004
- Mission
- Hubble Space Telescope
- Archive ID
- hubblesite-images-2004-29-1592-image
Detailed knots and filamentary ribbons of glowing gas are apparent in this Hubble Space Telescope image of Kepler's supernova remnant. This image was taken with Hubble's Advanced Camera for Surveys (ACS) in August 2003. Filters onboard Hubble isolate visible light emitted by hydrogen, nitrogen, and oxygen in the remnant and also let through starlight from foreground and background stars.
These images reveal where the supernova shock wave is slamming into dense regions of nearby gas. The bright glowing knots are dense clumps that form behind the outward moving shock wave. 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.
Credits
NASA, ESA, and The Hubble Heritage Team (STScI/AURA);Acknowledgment: R. Sankrit and W. Blair (Johns Hopkins University)
Image Details
| About The Object | |
|---|---|
| Object Name | Kepler's Supernova Remnant, SN 1604, V 843 Ophiuchi, G004.5+06.8 |
| Object Description | Supernova Remnant |
| R.A. Position | 17h 30m 40.79s |
| Dec. Position | -21° 29' 11.0" |
| Constellation | Ophiuchus |
| Distance | 13,000 light-years (4,000 parsecs) |
| About The Data | |
| Data Description | This image was created from Hubble observations from proposal : R. Sankrit and W. Blair (Johns Hopkins Univ.), L. Rudnick (U. Minnesota), T. DeLaney (U. Minnesota and Harvard-Smithsonian/Center for Astrophysics), I. Harrus (Goddard Space Flight Center). |
| Instrument | HST>ACS/WFC and HST>WFPC2 |
| Exposure Dates | August 28-29, 2003 and May 26, 2004v, Exposure Time: 23,509 seconds (6.5 hours) |
| Filters | F502N ([O III]), F550M (V), F658N (Halpha+[N II]), F660N ([N II]), and F673N ([S II]) |
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Image and source material are credited to the official mission archive linked below.
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