This page can be used in conjunction with any of the investigations, tasks, or activities in this section which ask students to compare and contrast images of an object in different wavelengths. These include the CAS Timeline investigation, and the perfomance tasks "Signals from the Cosmos", "Point of View", "The universe Rated R!", and "Portrait Gallery of the X-Ray Universe".
Cassiopeia A, or Cas A is the remnant of a massive star that exploded around three hundred years ago. These images show Cas A as viewed by four different types of telescopes.
You can view composited images by selecting the combinations you would like to see from the pull down menu on the right and then clicking the "Get Composite" button.
Cas A in the optical range of the spectrum. The optical image of Cas A shows matter with a temperature of about ten thousand degrees. Some of these wisps contain high concentrations of heavy elements and are thought to be dense clumps of ejected stellar material.
Cas A in the infrared range of the spectrum. The infrared image of Cas A shows dust grains that have been swept up and heated to several hundred degrees by the expanding hot gas. It is not known whether the dust grains were ejected by the star millions of years before it exploded or during the explosion.
Cas A in the radio range of the spectrum. Cas A gets its name from radio astronomers, who 'rediscovered' it in 1948 as the strongest radio source in the constellation of Cassiopeia. About 5 years later optical astronomers found the faint wisps, and it was determined that Cas A is the remnant of an explosion that occurred about 300 years ago. The radio emission comes from high-energy electrons moving in large spirals around magnetic field
Cas A Overlays | Cas A Timeline Activity | Cas A Photo Album