NASA's NuSTAR is complementing previous observations of the Cassiopeia A supernova remnant (red and green) by providing the first maps of radioactive material forged in the fiery explosion (blue).
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Adding a New 'Color' to Palate of Cassiopeia A Images

Elements making up the shredded remains of a massive star that exploded in a supernova are highlighted in this three-panel view. Red and green show iron, and both silicon and magnesium, respectively, as seen by NASA's Chandra X-ray Observatory. Blue shows radioactive titanium-44, mapped by NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, for the first time.

The radioactive titanium map amounts to new evidence in the case of why Cassiopeia A, and other massive stars, explode. The radioactive material glows in X-rays all the time, while the iron and other elements only glow in X-rays after they are heated by shock waves sent out from the explosion. For this reason, the radioactive titanium provides a more direct look at the heart of the explosion, and tells researchers what happened right when the star blasted apart.

The supernova explosion was not driven by jets, a realization to come out of the NuSTAR data. The green Chandra map shows that jets left imprints in material at the outer portions of the supernova remnant; if the blast had been directly spurred by these jets, then researchers would have expected the radioactive material seen by NuSTAR to have the same jet pattern. As the blue map does not match the green one, the jet-driven models of supernovas are ruled out.

NuSTAR is a Small Explorer mission led by the California Institute of Technology in Pasadena and managed by NASA's Jet Propulsion Laboratory, also in Pasadena, for NASA's Science Mission Directorate in Washington. The spacecraft was built by Orbital Sciences Corporation, Dulles, Va. Its instrument was built by a consortium including Caltech; JPL; the University of California, Berkeley; Columbia University, N.Y.; NASA's Goddard Space Flight Center, Greenbelt, Md.; the Danish Technical University in Denmark; Lawrence Livermore National Laboratory, Livermore, Calif.; ATK Aerospace Systems, Goleta, Calif., and with support from the Italian Space Agency (ASI) Science Data Center, Rome, Italy.

NuSTAR's mission operations center is at UC Berkeley, with ASI providing its equatorial ground station located at Malindi, Kenya. The mission's outreach program is based at Sonoma State University, Rohnert Park, Calif. NASA's Explorer Program is managed by Goddard. JPL is managed by Caltech for NASA.

For more information, visit http://www.nasa.gov/nustar and http://www.nustar.caltech.edu/.

Image details

ID#:
PIA17839

Date added:
2014-02-19

Mission:
Chandra X-ray Observatory, NuSTAR

Instruments:
Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array

Size:
3072 x 1024 pixels (width x height)

Rating:



Views:
723

Full-Res TIFF:
PIA17839.tif (9.44 MB)

Full-Res JPG:
PIA17839.jpg (0.16 MB)

Image credit:
NASA/JPL-Caltech/CXC/SAO