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G54.1+0.3 (Supernova Remnant)


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G54.1+0.3
Supernova Remnant (超新星残骸)
SNR


星座 (Constellation)

いて座 (Sgr) (Sagittarius)


距離 (Distance)
16,000光年 (16,000 light-years)

G54.1+0.3 is a supernova remnant located 16,000 light years from the Earth in the constellation Sagittarius.

G54.1+0.3 (Supernova Remnant) : Picture

G54.1+0.3 (Supernova Remnant)
G54.1+0.3 (Supernova Remnant)
(C) NASA
A new image from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the dusty remains of a collapsed star. The dust is flying past and engulfing a nearby family of stars. Scientists think the stars in the image are part of a stellar cluster in which the a supernova exploded. The material ejected in the explosion is now blowing past these stars at high velocities.

The composite image of G54.1+0.3 shows X-rays from Chandra in blue, and data from Spitzer in green (shorter wavelength infrared) and red-yellow (longer wavelength infrared). The white source near the center of the image is a dense, rapidly rotating neutron star, or "pulsar," left behind after a core-collapse supernova explosion. The pulsar generates a wind of high-energy particles -- seen in the Chandra data -- that expands into the surrounding environment, illuminating the material ejected in the supernova explosion.

The infrared shell that surrounds the pulsar wind is made up of gas and dust that condensed out of debris from the supernova. As the cold dust expands into the surroundings, it is heated and lit up by the stars in the cluster so that it is observable in the infrared. The dust closest to the stars is the hottest and is seen to glow in yellow in the image. Some of the dust is also being heated by the expanding pulsar wind as it overtakes the material in the shell.

The unique environment into which this supernova exploded makes it possible for astronomers to observe the condensed dust from the supernova that is usually too cold to emit in the infrared. Without the presence of the stellar cluster, it would not be possible to observe this dust until it becomes energized and heated by a shock wave from the supernova. However, the very action of such shock heating would destroy many of the smaller dust particles. In G54.1+0.3, astronomers are observing pristine dust before any such destruction.

X-ray Image of G54.1+0.3
X-ray Image of G54.1+0.3
(C) NASA

G54.1+0.3 G54.1+0.3
G54.1+0.3
(C) NASA
G54.1+0.3
(C) NASA
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G54.1+0.3 (Supernova Remnant) : Movie

G54.1+0.3 in 60 Seconds
Data from the Chandra X-ray Observatory and the Spitzer Space Telescope were combined to create this image of the dusty remains of a collapsed star.
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