This two-panel graphic compares an artist's illustration (left) of a simplified picture of the inner layers of a star just before it exploded to form the Cassiopeia A supernova remnant with a Chandra image (right) of what we see today. The different elements are represented by different colors: iron (blue), sulfur and silicon (green), and magnesium, neon and oxygen (red). The Chandra image uses the same color scheme to show the distribution of iron, sulfur and magnesium in the supernova remnant. A comparison of the illustration and the Chandra element map shows clearly that most of the iron, which according to theoretical models of the pre-supernova was originally on the inside of the star, is now located near the outer edges of the remnant.
A massive supernova explosion that destroyed a faraway star apparently turned the left over stellar corpse inside out as well, scientists say.
Using NASA's Chandra X-ray Observatory spacecraft, a team of researchers mapped the distribution of elements in the supernova remnant Cassiopeia A (Cas A for short) in unprecedented detail. They found that Cas A — which is located about 11,000 light-years from Earth and exploded 300 years ago from our perspective — is wearing its guts on the outside.
Before it went supernova, the star Cas A likely had an iron-rich core that was surrounded by layers of sulfur and silicon, which were in turn overlaid by magnesium, neon and oxygen, researchers said.
Chandra's observations showed that, after the explosion, most of that iron has now migrated to Cas A's outer edges. Neither Chandra nor NASA's Spitzer Space Telescope, which is optimized to see in infrared wavelengths, has detected any iron near the supernova remnant's center, where the element was originally formed.
Further, much of the silicon, sulfur and magnesium are now found on the outside of the still-expanding debris shell. Neon distribution hasn't changed much, and not much can be said about the oxygen because its X-ray emissions are strongly absorbed along the line of sight to Cas A.
Overall, this distribution of elements suggests that an instability in the supernova explosion process somehow turned the star inside out, researchers said. These latest Chandra observations, which are based on more than 11 days of observing time, are the most detailed study ever made of X-ray-emitting debris in Cas A, or in any other supernova remnant, they added.
The researchers estimate that the total amount of X-ray emitting debris has a mass just over three times that of our sun. Researchers found clumps of almost pure iron, indicating that this material must have been produced by nuclear reactions near the center of the pre-supernova Cas A.
The study's findings are detailed in the February edition of the The Astrophysical Journal.
The Chandra X-ray Observatory launched aboard the space shuttle Columbia in 1999 and has been observing the heavens ever since. It's one of NASA's "Great Observatories," a class of space telescopes that also includes Spitzer and the iconic Hubble Space Telescope.