Called an "infrared echo," this dance began when the remnant's dead star erupted, or "turned in its grave," about 50 years ago. A blast of light from Cassiopeia A is seen waltzing through the dusty skies. Here, the animation flips back and forth between two Spitzer images taken one year apart. It then pans out to show a Spitzer view of Cassiopeia A (yellow ball) and surrounding clouds of dust (reddish orange). The animation begins with the false-color picture of the supernova remnant Cassiopeia A. Chandra can also see Cassiopeia A's neutron star (turquoise dot at center of shell).īlue Chandra data were acquired using broadband X-rays (low to high energies) green Chandra data correspond to intermediate energy X-rays yellow Hubble data were taken using a 900 nanometer-wavelength filter, and red Spitzer data are from the telescope's 24-micron detector. These extremely hot gases were created when ejected material from Cassiopeia A smashed into surrounding gas and dust. Chandra probes unimaginably hot gases, up to about 10 million degrees Kelvin (18 million degrees Fahrenheit). While Spitzer reveals warm dust in the outer shell about a few hundred degrees Kelvin (80 degrees Fahrenheit) in temperature, Hubble sees the delicate filamentary structures of hot gases about 10,000 degrees Kelvin (18,000 degrees Fahrenheit). The neutron star can be seen in the Chandra data as a sharp turquoise dot in the center of the shimmering shell.Įach Great Observatory highlights different characteristics of this celestial orb. It consists of a dead star, called a neutron star, and a surrounding shell of material that was blasted off as the star died. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Infrared data from the Spitzer Space Telescope are colored red visible data from the Hubble Space Telescope are yellow and X-ray data from the Chandra X-ray Observatory are green and blue. It is made up of images taken by three of NASA's Great Observatories, using three different wavebands of light. This stunning false-color picture shows off the many sides of the supernova remnant Cassiopeia A.
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