Spitzer Exposes Our Galaxy's Deepest Secrets

panoramic, infrared image of a plethora of stellar activity in the Milky Way's galactic plane A panoramic, infrared image from Spitzer of the Milky Way's galactic plane. The red clouds indicate the presence of large organic molecules (mixed with the dust), which have been illuminated by nearby star formation. The patches of black are dense obscuring dust clouds impenetrable by even Spitzer's super-sensitive infrared eyes. Bright arcs of white throughout the image are massive stellar incubators.
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December 13, 2005

Astronomers have at last found inner light! But they didn't find it through the typical Earthly methods of meditation, exercise and therapy. Instead, the light was discovered inside our Milky Way galaxy after hours of deep self-reflection with NASA's Spitzer Space Telescope.

The astronomers, who are members of the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire team, used Spitzer's heat-seeking infrared eyes to gaze at the dust-drenched plane of our galaxy. When they did this, the galaxy's obscuring clouds of gas and dust became transparent, revealing approximately 100 new star clusters, each containing tens to hundreds of stars.

According to lead investigator Emily Mercer, a graduate student at Boston University, Mass., the new clusters will tell astronomers a great deal about the structure of the Milky Way and star formation within the galaxy.

"These little guys were quite hard to find," said Mercer. "The discovery required sophisticated computer sifting of Glimpse data and careful inspection of the Spitzer images."

In the past, our galaxy wasn't so quick to give up its stellar secrets. Because we sit inside its flat, spiral disk, most of the galaxy appears as a thick, blurry band of light that streaks across the sky. Many of the stars in this galactic plane cannot be detected with visible-light or ultraviolet telescopes. That's because the cool clouds of dust and gas that hover around the galaxy's center and make up galactic spiral arms block their starlight from our view.

Two-thirds of the new star clusters were discovered through a computer method developed by Mercer and her advisor, Dr. Dan Clemens, also of Boston University. They used an algorithm, or mathematical procedure, to automatically sift through the Glimpse data for clusters. The rest were found using the traditional method of visually scrutinizing images for star clusters.

Mercer also found that there are nearly twice as many star clusters in the southern portion of the galactic plane, visible from Earth's southern hemisphere, as in the northern galactic plane. She suspects that this observation may help astronomers map the location of the Milky Way's spiral arms.

"Emily has done a great job," says Clemens. "Her computer method for finding clusters has proved to be the most successful automated effort to date."

Both Clemens and Mercer are members of the multi-institutional Glimpse team led by Dr. Edward Churchwell of the University of Wisconsin, Madison. The group was selected to survey the galactic plane with Spitzer's infrared array camera in November 2000 as part of Spitzer's Legacy program. So far, more than 30 million stars in the inner Milky Way have already been catalogued by Glimpse, and the team expects to identify more than 50 million stars by the end of the project.

"By making the galactic plane transparent, Spitzer opens a new door for astronomers to study the Milky Way," says Churchwell. "Some of the most interesting science likely to come out of this project will be serendipitous discoveries, which will open up entirely new avenues of inquiry."


Written by Linda Vu, Spitzer Science Center
Media contact: Whitney Clavin, JPL
(818) 354-4673



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