Supernova Remnant Cassiopeia A - December 2004

Stsci_2006-30a_1024

stsci_2006-30a August 29th, 2006

Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)- ESA/Hubble Collaboration Acknowledgment: R. Fesen (Dartmouth College) and J. Long (ESA/Hubble)

A new image taken with NASA's Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A). It is the youngest known remnant from a supernova explosion in the Milky Way. The new Hubble image shows the complex and intricate structure of the star's shattered fragments. The image is a composite made from 18 separate images taken in December 2004 using Hubble's Advanced Camera for Surveys (ACS), and it shows the Cas A remnant as a broken ring of bright filamentary and clumpy stellar ejecta. These huge swirls of debris glow with the heat generated by the passage of a shockwave from the supernova blast. The various colors of the gaseous shards indicate differences in chemical composition. Bright green filaments are rich in oxygen, red and purple are sulfur, and blue are composed mostly of hydrogen and nitrogen. A supernova such as the one that resulted in Cas A is the explosive demise of a massive star that collapses under the weight of its own gravity. The collapsed star then blows its outer layers into space in an explosion that can briefly outshine its entire parent galaxy. Cas A is relatively young, estimated to be only about 340 years old. Hubble has observed it on several occasions to look for changes in the rapidly expanding filaments. In the latest observing campaign, two sets of images were taken, separated by nine months. Even in that short time, Hubble's razor-sharp images can observe the expansion of the remnant. Comparison of the two image sets shows that a faint stream of debris seen along the upper left side of the remnant is moving with high speed - up to 31 million miles per hour (fast enough to travel from Earth to the Moon in 30 seconds!). Cas A is located ten thousand light-years away from Earth in the constellation of Cassiopeia. Supernova explosions are the main source of elements more complex than oxygen, which are forged in the extreme conditions produced in these events. The analysis of such a nearby, relatively young and fresh example is extremely helpful in understanding the evolution of the universe.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2006/news-2006-30

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

Image Details Image Details

Image Type
Observation
Object Name
Cassipopeia A
Subject - Milky Way
Nebula > Type > Supernova Remnant

Distance Details Distance

Universescale1
10,000 light years
Stsci_2006-30a_128
 

Position Details Position Details

Position (ICRS)
RA = 23h 23m 28.0s
DEC = 58° 50’ 24.2”
Orientation
North is 0.5° CCW
Field of View
8.6 x 6.2 arcminutes
Constellation
Cassiopeia

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (SDSS r) 625.0 nm
Green Hubble (ACS) Optical (SDSS i) 775.0 nm
Red Hubble (ACS) Optical (SDSS z) 850.0 nm
4-Dec
Spectrum_base
Blue
Green
Red
Stsci_2006-30a_1280
×
ID
2006-30a
Subject Category
B.4.1.4  
Subject Name
Cassipopeia A
Credits
NASA, ESA, and the Hubble Heritage (STScI/AURA)- ESA/Hubble Collaboration Acknowledgment: R. Fesen (Dartmouth College) and J. Long (ESA/Hubble)
Release Date
2006-08-29T00:00:00
Lightyears
10,000
Redshift
10,000
Reference Url
https://hubblesite.org/contents/news-releases/2006/news-2006-30
Type
Observation
Image Quality
Good
Distance Notes
About 10,000 light-years 3,100 parsecs away.
Facility
Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS
Color Assignment
Blue, Green, Red
Band
Optical, Optical, Optical
Bandpass
SDSS r, SDSS i, SDSS z
Central Wavelength
625, 775, 850
Start Time
2003-11-13T00:00:00, 2003-11-13T00:00:00, 2003-11-13T00:00:00
Integration Time
Dataset ID
Notes
4
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
350.86684278122, 58.84006388998
Reference Dimension
10252.00, 7379.00
Reference Pixel
4805.91930093136, 5502.62106061432
Scale
-0.00001390356, 0.00001390356
Rotation
0.47483393444
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center FITS X FITS Y EPO X EPO Y 1283.13 1104.36 5262.99 1926.94 1045.14 1163.95 4790.78 2057.27 453.30 2033.59 3650.60 3823.70 1323.76 1858.26 5383.81 3427.81 784.80 517.04 4235.93 776.53 Center Pixel Coordinates: 5126.00 350.85866892995 3689.50 58.81483502504
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p0630a-f-10252x7379.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0630a-f-10252x7379.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2006/30
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
10,000 light years

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