Milky Way's center unveils supernova 'dust factory'

March 19, 2015, Cornell University
The dust (yellow contours) that formed from the supernova survives in a cooler, less harsh region of the ejecta as can be seen from its spatial displacement from the x-ray emission from highly excited iron (purple). The red dashed ellipse delineates the forward shock of the supernova and the inset shows a twice zoomed-in image of the dust (orange) and x-ray (cyan) emission within the white box. Credit: Ryan Lau et al. with observations from SOFIA/FORCAST and Chandra/ACIS-I

Sifting through the center of the Milky Way galaxy, astronomers have made the first direct observations - using an infrared telescope aboard a modified Boeing 747 - of cosmic building-block dust resulting from an ancient supernova.

"Dust itself is very important because it's the stuff that forms stars and planets, like the sun and Earth, respectively, so to know where it comes from is an important question," said lead author Ryan Lau, Cornell postdoctoral associate for astronomy, in research published March 19 in Science Express. "Our work strongly reinforces the theory that supernovae are producing the dust seen in galaxies of the early universe," he said.

Lau explains that one of astronomy's big questions is why galaxies - forming as recently as 1 billion years after the Big Bang - contain so much dust. The leading theory is that supernovae - stars that explode at the end of their lives - contain large amounts of metal-enriched material that, in turn, harbors key ingredients of dust, like silicon, iron and carbon.

The astronomers examined Sagittarius A East, a 10,000-year-old supernova remnant near the center of our galaxy. Lau said that when a supernova explodes, the materials in its center expand and form dust. This has been observed in several young - such as the famed SN1987A and Cassiopeia A. In the turbulent supernova environment, scientists expect the churning dust to be destroyed. "That is theoretically," Lau said. "There have been no direct observations of any surviving the environment of the supernova remnant ... until now, and that's why our observations of an 'old' are so important," he said.

Imaging observations with SOFIA/FORCAST of the 10,000 yr-old Sagittarius A East Supernova Remnant at the Galactic center have revealed the presence of warm dust (white contours) that formed in the initial supernova explosion and survived the hot interior of the remnant, as traced by X-rays (blue). The radio emission (red) delineates the expanding forward shock of the supernova, which is interacting with surrounding molecular clouds that are traced by cold dust emission (green). Credit: Ryan Lau et al. with observations from SOFIA/FORCAST, Herschel/PACS, Chandra/ACIS-I, and the VLA

The astronomers captured the observations via FORCAST (the Faint Object Infrared Camera Telescope) aboard SOFIA (the Stratospheric Observatory for Infrared Astronomy), a modified Boeing 747 and a joint project of NASA, the German Aerospace Center and the Universities Space Research Association. It is the world's largest airborne astronomical observatory. Currently, no space-based telescope can observe at far-infrared wavelengths, and ground-based telescopes are unable to observe light at these wavelengths due to the Earth's atmosphere.

Joining Lau on this research, "Old Supernova Dust Factory Revealed at the Galactic Center," are co-authors Terry Herter, Cornell professor of astronomy and principal scientific investigator on FORCAST; Mark Morris, University of California, Los Angeles; Zhiyuan Li, Nanjing University, China; and Joe Adams, NASA Ames Research Center.

Explore further: SOFIA airborne observatory begins 2015 science campaign

More information: Old supernova dust factory revealed at the Galactic center, … 1126/science.aaa2208

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not rated yet Mar 22, 2015
one can see much better and clear data on Milky-way central region through
Giant Magnetised Outflow from milky Way center.
Milky Way- ESA Planck
The microwave sky as seen by ESA's Planck satellite. Light from the main disk of the Milky Way is seen across the center band, while radiation left over from the Big
Bang is visible on the outskirts of the image. courtesy:ESA/ LFI & HFI Consortia

1 / 5 (1) Mar 29, 2015
Lau explains that one of astronomy's big questions is why galaxies - forming as recently as 1 billion years after the Big Bang - contain so much dust.

Patch. Quick, we need another patch to sustain the fantasy. Whew. Supernovas are it!
1 / 5 (2) Mar 30, 2015
Our work strongly reinforces the theory that supernovae are producing the dust seen in galaxies of the early universe
Nice try but IMO the dust in quasars is formed with materialization of dark matter directly in a process, which resembles the tiny big bang at the local scale.

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