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| Credit: NASA/JPL-Caltech/Y. Kim (Univ. of Arizona/ Univ. of Chicago) |
Ghostly Stellar Echoes
This image from NASA's Spitzer Space Telescope highlights dramatic changes in phenomena referred to as light echoes (colored areas) around the Cassiopeia A supernova remnant (center). Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion. It consists of a dead star, called a neutron star, and a surrounding shell of material that was blasted off as the star died.
A light echo is created when a star explodes or erupts, flashing light into surrounding clumps of dust. As the light zips through the dust clumps, it heats them up, causing them to glow successively in infrared, like a chain of Christmas bulbs lighting up one by one. The result is an optical illusion, in which the dust appears to be flying outward at the speed of light. This apparent motion can be seen here by the shift in colored dust clumps.
The main underlying image is a composite from Spitzer showing Cassiopeia A and surrounding interstellar clouds of dust. It consists of six images taken over a time span of three years, each represented in a different color, as noted by the key at the bottom of the image.
Dust features that have not changed over time appear gray, while those that have changed are colored blue or orange. Bluer colors represent an earlier time and redder ones, a later time. Certain areas of the light echo are displayed in more detail to show the turbulent patterns formed as the light echo illuminates different areas of gas and dust over time.
The supernova remnant is located 11,000 light-years away in the northern constellation Cassiopeia. The light echo is the largest ever seen, stretching more than 300 light-years away from Cassiopeia A. If viewed from Earth, the entire frame would take up the same amount of space as seven full moons.
The earliest Spitzer image shown here was taken in February 2005, and the latest one in January 2008. The image was processed to emphasize the light echo by enhancing the areas that change, which appear in color, and dimming regions that remain constant, seen in gray. Spurious color artifacts, such as diffraction spikes around stars, were removed by hand.
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| About the Object |
Object Name:
Cassiopeia A
Object Type:
Supernova Remnant
Position (J2000):
RA:
23h 23m 24.00s
Dec:
58d 48m 0.00s
Distance:
11,000 light-years
Constellation:
Cassiopeia
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| About the Data |
Image Credit:
NASA/JPL-Caltech/Y. Kim (Univ. of Arizona/ Univ. of Chicago)
Instrument:
MIPS; Calar Alto 2.2m telescope; Steward Observatory 90-inch telescope; SUBARU Telescope's FOCAS instrument
Wavelength:
24 microns
Exposure Date:
Spitzer: 2 October 2006, 23 January 2007, 20 August 2007, 7 January 2008; Calar Alto 2.2m Telescope: October 6, 2007; Steward Observatory 90-inch telescope: 18 September 2006; SUBARU telescope: 9 October 2007
Release Date:
May 29, 2008
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| Observers |
Oliver Krause (Max-Planck-Institute for Astronomy)
Stephan M. Birkmann (Max-Planck-Institute for Astronomy)
Tomonori Usuda ( National Astronomical Observatory of Japan)
Takashi Hattori ( National Astronomical Observatory of Japan)
Miwa Goto (Max-Planck-Institute for Astronomy)
George H. Rieke (University of Arizona)
Karl A. Misselt (University of Arizona)
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Credit: NASA/JPL-Caltech/Y. Kim (Univ. of Arizona/ Univ. of Chicago)
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