Remnants of a Shattered Star Discovered in Milky Way
This composite image of supernova remnant G306.3-0.9 merges Chandra X-ray observations (blue), infrared data acquired by the Spitzer Space Telescope (red and cyan) and radio observations (purple) from the Australia Telescope Compact Array. The image is 20 arcminutes across, which corresponds to 150 light-years at the remnant's estimated distance. Credit: X-ray: NASA/CXC/Univ. of Michigan/M. Reynolds et al; Infrared: NASA/JPL-Caltech; Radio: CSIRO/ATNF/ATCA
Remnants of an exploded star have been discovered in our Milky Way galaxy by a team of scientists including astronomers at Penn State University. The "supernova remnant" was discovered during an extensive X-ray survey of our galaxy's central regions with NASA's Swift satellite, for which science and flight operations are controlled by Penn State from the Mission Operations Center on the University Park campus. A paper describing the team's findings will be published in an upcoming edition of The Astrophysical Journal.
Designated G306.3–0.9 after the coordinates of its sky position, the new object ranks among the youngest-known supernova remnants in the Milky Way. Astronomers estimate that a supernova explosion occurs once or twice a century in the Milky Way. The expanding blast wave and hot stellar debris slowly dissipate over hundreds of thousands of years, eventually mixing with and becoming indistinguishable from interstellar gas. Like fresh evidence at a crime scene, young supernova remnants give astronomers the best opportunity for understanding the nature of the original star and the details of its demise.
This wider view places G306.3-0.9 in context with star-formation regions in the southern-hemisphere constellation Centaurus. Chandra X-ray observations (blue), Spitzer infrared data (red, cyan), and radio observations (purple) from the Australia Telescope Compact Array are merged in this composite. This image is one degree across, which corresponds to 450 light-years at the remnant's estimated distance. Credit: X-ray: NASA/CXC/Univ. of Michigan/M. Reynolds et al; Infrared: NASA/JPL-Caltech; Radio: CSIRO/ATNF/ATCA
"The Swift survey leverages infrared imaging previously compiled by NASA's Spitzer Space Telescope and extends it into X-ray and higher energies," said team member Michael Siegel, a Penn State research associate at the Mission Operations Center for Swift at Penn State. "The infrared and X-ray surveys complement each other because light at these energies penetrates dust clouds in the galactic plane, while the ultraviolet is largely extinguished."
Supernova remnants emit energy across the electromagnetic spectrum, from radio to gamma rays, and important clues can be found in each energy band. X-ray observations figure prominently in revealing the motion of the expanding debris, its chemical content, and its interaction with the interstellar environment, but supernova remnants fade out in X-ray light after 10,000 years. Indeed, only half of those known in the Milky Way galaxy have been detected in X-rays at all.
"We don't yet have enough information to determine what type of supernova this was and therefore what type of star exploded, but we've planned a further Chandra observation to improve the picture,” said coauthor Jamie Kennea, also a researcher at the Mission Operations Center for Swift at Penn State. "We see no compelling evidence that the explosion formed a neutron star, and this is something we hope can be determined one way or the other by future work."
On Feb. 22, 2011, Swift imaged a survey field near the southern border of the constellation Centaurus. Although nothing unusual appeared in the ultraviolet exposure, the X-ray image revealed an extended, semi-circular source reminiscent of a supernova remnant. A search of archival data revealed counterparts in Spitzer infrared imagery and in radio data from the Molonglo Observatory Synthesis Telescope in Australia.
To further investigate the object, the team followed up with an 83-minute exposure using NASA's Chandra X-ray Observatory and additional radio observations from the Australia Telescope Compact Array (ATCA), located near the town of Narrabri in New South Wales.
This image from Swift's X-ray Telescope was taken on 22 February 2011 as part of the Galactic Plane Survey. The dots in the image indicate where X-rays struck the detector. Despite this short 8.5-minute exposure, the extended circular patch of G306.3-0.9 stands out. The image is 25.5 arcminutes across. Credit: NASA/Swift/Stefan Immler
"The fantastic sensitivity of ATCA has enabled us to image what, at radio wavelengths, turns out to be the dimmest remnant we have ever seen in our galaxy," said team member Cleo Loi, an undergraduate student at the University of Sydney who led the analysis of the radio observations.
Using an estimated distance of 26,000 light-years for G306.3–0.9, the scientists determined that the explosion's shock wave is racing through space at about 1.5 million mph (2.4 million km/h). The Chandra observations reveal the presence of iron, neon, silicon and sulfur at temperatures exceeding 50 million degrees F (28 million C), a reminder not only of the energies involved but of the role supernovae play in seeding the galaxy with heavy elements produced in the hearts of massive stars.
"Astronomers previously have cataloged more than 300 supernova remnants in the galaxy," said lead scientist Mark Reynolds, a postdoctoral researcher at the University of Michigan in Ann Arbor. "Our analysis indicates that G306.3–0.9 is likely less than 2,500 years old, making it one of the 20 youngest remnants identified." Reynolds leads the Swift Galactic Plane Survey, a project to image a two-degree-wide strip along the Milky Way's central plane at X-ray and ultraviolet energies at the same time. The ultraviolet portion of the survey will capture the first comprehensive view of the galaxy's midplane at these wavelengths. Imaging began in 2011 and is expected to complete this summer.
CONTACTS
- Jamie A. Kennea: jak51@psu.edu, 814-865-0234
- Michael Siegel: mhs18@psu.edu, 814-865-7748
- Barbara Kennedy (PIO): 814-863-4682, science@psu.edu