Astronomers have recently created a 3-D map of nearby supernova remnant with the help of the astronomical equivalent of a CAT scan, which revealed that it has a "bubbly interior."
Cassiopeia A, or Cas A for short, is one of the most well studied supernova remnants in our galaxy. But it still holds major surprises. A Harvard-Smithsonian and Dartmouth College astronomer with the help of map found it was composed of a collection of about a half dozen massive cavities or "bubbles."
To make the 3-D map, Milisavljevic and co-author Rob Fesen of Dartmouth College examined Cas A in near-infrared wavelengths of light using the Mayall 4-meter telescope at Kitt Peak National Observatory, southwest of Tucson, AZ. Spectroscopy allowed them to measure expansion velocities of extremely faint material in Cas A's interior, which provided the crucial third dimension.
They found that the large interior cavities appear to be connected to, and nicely explain, the previously observed large rings of debris that make up the bright and easily seen outer shell of Cas A. The two most well-defined cavities are 3 and 6 light-years in diameter, and the entire arrangement has a Swiss cheese-like structure.
The bubble-like cavities were likely created by plumes of radioactive nickel generated during the stellar explosion. Since this nickel will decay to form iron, Milisavljevic and Fesen predict that Cas A's interior bubbles should be enriched with as much as a tenth of a solar mass of iron.
This enriched interior debris hasn't been detected in previous observations, however, so next-generation telescopes might be needed to find the "missing" iron and confirm the origin of the bubbles.