Dec 21, 1999
Prospecting inside a Supernova
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Right: The red, green, and blue regions in this Chandra X-ray image of the supernova remnant Cassiopeia A show where the intensity of low, medium, and high energy X-rays, respectively, is greatest. The red material on the left outer edge is enriched in iron, whereas the bright greenish white region on the lower left is enriched in silicon and sulfur. In the blue region on the right edge, low and medium energy X-rays have been filtered out by a cloud of dust and gas in the remnant.
The findings are slated for publication in the Astrophysical Journal Letters on Jan. 10, 2000. Authors of the paper "Nucleosynthesis and Mixing in Cassiopeia A" are Hughes, Rutgers graduate student Cara Rakowski, Dr. David Burrows of Pennsylvania State University, University Park, Penn., and Dr. Patrick Slane of the Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
According to Hughes, one of the most profound accomplishments of twentieth century astronomy is the realization that nearly all of the elements other than hydrogen and helium were created in the interiors of stars. "During their lives, stars are factories that take the simplest element, hydrogen, and convert it into heavier ones," he said. "After consuming all the hydrogen in their cores, stars begin to evolve rapidly, until they finally run out of fuel and begin to collapse. In stars 10 times or so more massive than our sun, the central parts of the collapsing star may form a neutron star or a black hole, while the rest of the star is blown apart in a tremendous supernova explosion." Supernovae are rare, occurring only once every 50 years or so in a galaxy like our own.
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Equal in significance to the image clarity is the potential the Chandra data held for measuring the composition of the various knots and filaments of stellar material visible in Cas A. Not only could the astronomers determine the composition of many knots in the remnant from the Chandra data, they were also able to infer where in the exploding star the knots had originated.
For example, the most compact and brightest knots were composed mostly of silicon and sulfur, with little or no iron. This pointed to an origin deep in the star's interior where the temperatures had reached three billion degrees during the collapse and resulting supernova. Elsewhere, they found fainter features that contained significant amounts of iron as well as some silicon and sulfur. This material was produced even deeper in the star, where the temperatures during the explosion had reached higher values of four to five billion degrees.
When Hughes and his collaborators compared where the compact silicon-rich knots and fainter iron-rich features were located in Cas A, they discovered that the iron-rich features from deepest in the star were near the outer edge of the remnant. This meant that they had been flung the furthest by the explosion that created Cas A. Even now this material appears to be streaming away from the site of the explosion with greater speed than the rest of the remnant.
By studying the Cas A Chandra data further, astronomers hope to identify which of the several processes proposed by theoretical studies is likely to be the correct mechanism for explaining supernova explosions, both in terms of the dynamics and elements they produce.
"In addition to understanding how iron and the other elements are produced in stars, we also want to learn how it gets out of stars and into the interstellar medium. This is why the study of supernovae and supernova remnants is so important," said Hughes. "Once released from stars, newly-created elements can then participate in the formation of new stars and planets in a great cycle that has gone on numerous times already. It is remarkable to realize that our planet Earth and indeed even humanity itself is part of this vast cosmic cycle."
The Chandra observation was taken with the Advanced CCD Imaging Spectrometer (ACIS) Aug. 19, 1999. ACIS was built by Pennsylvania State University, and the Massachusetts Institute of Technology, Cambridge, Mass.
To follow Chandra's progress, visit the Chandra sites at: http://chandra.harvard.edu/ and http://chandra.nasa.gov/
NASA's Marshall Space Flight Center manages the Chandra program. TRW, Inc., Redondo Beach, CA, is the prime contractor for the spacecraft. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, MA.
- New Chandra Images Released - X-ray pictures from NASA's Chandra X-ray Observatory reveal previously unobserved features in the remnants of three different supernova explosions. Sept. 23
- Chandra peers into the Large Magellanic Cloud -- The X-ray Observatory's High Resolution Camera catches extraordinary pictures of a distant supernova remnant. September 13, 1999
- NASA Unveils First Light Images from Chandra -- The newest Great Observatory is making an immediate impact with spectacular new views of the Cassiopeia A supernova remnant and a distant quasar. August 26, 1999
- Studying the Titanium Star -- When the Chandra X-ray Observatory took its "first light" image, it wasn't looking at just another star shining in the darkness. It was watching a foundry distribute its wares to the rest of the galaxy. August 26, 1999
- Why Launch Chandra at Night? -- Chandra's beautiful early morning launch will place it into an orbit unlike that of NASA's other Great Observatories, July 23, 1999
- Xraytelescope.com, science news from the Chandra X-Ray Observatory
- Chandra X-ray Observatory Center home page, with links to education, news, and technical pages.
- Chandra news from Marshall Space Flight Center
- Chandra Project Science is managed at NASA/Marshall, has links to individual instruments and the prime contractor.
- X-ray astrophysics branch at NASA/Marshall conducts a broad range of research and technology work, as well as supporting the Chandra X-ray Observatory.
Additional images of the Crab Nebula are available from NASA's Astronomy Picture of the Day web site:
- High Energy Crab Nebula | Pulsar Powered Crab | M1: Filaments of the Crab Nebula | Exploding Crab Nebula
- And from the Students for the Exploration and Development of Space web nebula page.
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