Galaxy Exposes Its Dusty Inner Workings in Innovative Spitzer Picture

NASA's Spitzer Space Telescope has captured an action-packed image of the nearby Small Magellanic Cloud, a tiny galaxy that looks like a wispy cloud when seen from Earth.

From Spitzer's perch up in space, the galaxy's clouds of dust and stars come into clear vision. The telescope's infrared vision reveals choppy heaps of recycled stardust -- dust that is being soaked up by new star systems and blown out by old ones.

To some people, the new view might look like a sea creature, or even a Rorschach inkblot test. But to astronomers, it offers a exclusive opportunity to study the whole life cycle of stars close-up. The image is available online at http://www.nasa.gov/AAS and http://www.jpl.nasa.gov/aas .

"It's quite the treasure trove," said Karl Gordon, the principal researcher of the newest Spitzer observations at the Space Telescope Science Institute in Baltimore, Md. "Because this galaxy is so close and comparatively large, we can study all the different stages and facets of how stars form in one environment."

The Small Magellanic Cloud, and its bigger sister galaxy, the Large Magellanic Cloud, are named after the seafaring explorer Ferdinand Magellan, who documented them while circling the globe nearly 500 years ago. From Earth's southern hemisphere, they can emerge as wispy clouds. The Small Magellanic Cloud is the farther of the pair, at 200,000 light-years away.


Recent research has exposed that the galaxies may not, as previously suspected, orbit around the Milky Way. Instead, they are thought to be simply sailing by, destined to go their own way. Astronomers say the two galaxies, which are both less evolved than a galaxy like ours, were triggered to generate bursts of new stars by gravitational interactions with the Milky Way and with each other. In fact, the Large Magellanic Cloud may ultimately consume its smaller companion.

Gordon and his team are concerned in the Small Magellanic Cloud not only because it is so close and compact, but also because it is very similar to young galaxies thought to populate the universe billions of years ago. The Small Magellanic Cloud has only one-fifth the amount of heavier elements, such as carbon, enclosed in the Milky Way, which means that its stars haven't been around long enough to pump large amounts of these elements back into their environment. Such elements were essential for life to form in our solar system.

Studies of the Small Magellanic Cloud therefore offer a glance into the different types of environments in which stars form.

The new Spitzer observations were accessible today at the 215th meeting of the American Astronomical Society in Washington. They expose the galaxy's youngest stars embedded in thick dust, in addition to the older stars, which spit the dust out. Taken together with visible-light explanation, these Spitzer data help provide a census of the whole stellar population.

"With Spitzer, we are indicative how to best calculate the numbers of new stars that are forming right now," said Gordon. "Observations in the infrared give us a outlook into the birthplace of stars, unveiling the dust-enshrouded locations where stars have just formed."

Infrared light is color-coded in the new image, so that blue shows older stars, green shows organic dust and red highlights dust-enshrouded star configuration. Light determined in blue has a wavelength of 3.6 microns; green is 8.0 microns; and red is 24 microns. This picture was taken before Spitzer ran out of its liquid coolant in May 2009 and began its "warm" mission.

Other collaborators comprise: M. Meixner, M, Sewilo and B. Shiao of the Space Telescope Science Institute; M. Meade, B. Babler, S. Bracker of the University of Wisconsin at Madison; C. Engelbracht, M. Block, K. Misselt of the University of Arizona, Tucson; R. Indebetouw of the University of Virginia, Charlottesville; and J. Hora and T. Robitaille of the Harvard Smithsonian Center for Astrophysics, Cambridge, Mass.

The image includes Spitzer explanation taken formerly by a team led by Alberto Bolatto of the University of Maryland, College Park.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope assignment for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA.

For more information about Spitzer, visit http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

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