Volume: 04, Issue: 15 03/22/2006 
This infrared image from NASA's Spitzer Space Telescope shows Messier 82, or the "Cigar galaxy," smothered in smoky dust particles (red) blown out into space by the galaxy's hot stars (blue). Image credit: NASA/JPL-Caltech/University of Arizona.
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The visible-light picture of the Cigar galaxy shows only a bar of light against a dark patch of space. Image credit: NASA/JPL-Caltech/University of Arizona/NOAO.
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The Spitzer Space Telescope whizzes in front of a brilliant, infrared view of the Milky Way galaxy's plane in this artistic depiction. Image credit: NASA/JPL.
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Other Articles in This Issue:
Scientists Use Satellites to Help Detect Deep-Ocean Whirlpools
Mars Rovers Get New Manager During Challenging Period
Venus Bright in the Morning Sky
Discuss the GOES-N Mission with NOAA Scientist Thomas Wrublewski
 

NASA’s Spitzer Reveals Stellar Smoke

A new infrared image from NASA’s Spitzer Space Telescope shows a burning hot galaxy whose fiery stars appear to be blowing out giant billows of smoky dust.

The galaxy, called Messier 82, or the “Cigar galaxy,” was previously known to host a hotbed of young, massive stars. The new Spitzer image reveals, for the first time, the “smoke” surrounding those stellar fires.

“We’ve never seen anything like this,” said Dr. Charles Engelbracht of the University of Arizona, Tucson. “This unusual galaxy has ejected an enormous amount of dust to cover itself with a cloud brighter than any we’ve seen around other galaxies.”

The false-color view, online at http://www.spitzer.caltech.edu/Media, shows Messier 82, an irregular-shaped galaxy positioned on its side, as a diffuse bar of blue light. Fanning out from its top and bottom like the wings of a butterfly are huge red clouds of dust believed to contain a compound similar to car exhaust.

The smelly material, called polycyclic aromatic hydrocarbon, can be found on Earth in tailpipes, barbecue pits, and other places where combustion reactions have occurred. In galaxies, the material is created by stars, whose winds and radiation blow the material out into space. “Usually you see smoke before a fire, but we knew about the fire in this galaxy before Spitzer’s infrared eyes saw the smoke,” said Dr. David Leisawitz, Spitzer program scientist at NASA Headquarters in Washington D.C.

These hazy clouds are some of the biggest ever seen around a galaxy. They stretch out 20,000 light-years away from the galactic plane in both directions, far beyond where stars are found.

Previous observations of Messier 82 revealed two cone-shaped clouds of very hot gas projecting outward below and above the center of the galaxy. Spitzer’s sensitive infrared vision allowed astronomers to see the galaxy’s dust.

“Spitzer showed us a dust halo all around this galaxy,” said Engelbracht. “We still don’t understand why the dust is all over the place and not cone-shaped.”

Cone-shaped clouds of dust around this galaxy would have indicated that its central, massive stars had sprayed the dust into space. Instead, Engelbracht and his team believe stars throughout the galaxy are sending off these “smoke signals.”

Messier 82 is located about 12 million light-years away in the Ursa Major constellation. It is undergoing a renaissance of star birth in its middle age, with the most intense bursts of star formation taking place at its core. The galaxy’s interaction with its neighbor, a larger galaxy called Messier 81, is the cause of all the stellar ruckus. Our own Milky Way galaxy is a less hectic place, with dust confined to the galactic plane.

The findings will appear in an upcoming issue of the Astrophysical Journal. Other authors who contributed significantly to this work are Praveen Kundurthy and Dr. Karl Gordon, both of the University of Arizona. The image was taken as part of the Spitzer Infrared Nearby Galaxy Survey, which is led by Dr. Robert Kennicutt, also of the University of Arizona.

For more information, please visit the following websites:
http://www.spitzer.caltech.edu/spitzer/
http://www.jpl.nasa.gov/news/news.cfm?release=2006-037.

    
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