IOWA STATE (US)—The Spitzer Space Telescope is now taking aim at the outer reaches of the Milky Way.
The data is allowing Massimo Marengo, an assistant professor of physics and astronomy at Iowa State University, to study big, cool-temperature stars and the dusty disks that forms around these and other stars as their planetary systems evolve.
He is a coauthor of a new paper—published this month in the Astrophysical Journal Letters—that describes how tight double-star systems could be efficient “destroyers of worlds” because planet collisions may be common within the systems.
Charles Kerton, an associate professor of physics and astronomy Iowa State, also is relying on Spitzer data to study star-forming regions of the Milky Way galaxy. He is coauthor of a new paper that uses Spitzer images to identify regions within the inner Milky Way that are forming intermediate-mass stars. The paper was published in the August issue of the Astronomical Journal.
NASA’s Spitzer Space Telescope launched Aug. 25, 2003, into an orbit of the sun. Its 33.5-inch diameter telescope and three scientific instruments are designed to detect infrared or heat radiation. To do that, the telescope assembly had to be cooled to within a few degrees of absolute zero (or -459 degrees Fahrenheit).
The telescope ran out of liquid helium coolant last summer but is still able to collect data with its two shortest-wavelength detectors.
One of the telescope’s initial tasks was to survey the Milky Way’s dusty, star-filled center. The telescope, as part of an astronomy survey called GLIMPSE360, is now pointed toward outer regions of the galaxy and is beginning to send images of those remote areas.
The survey is led by Barbara Whitney, a senior scientist at the University of Wisconsin-Madison and a senior research scientist at the Space Science Institute in Boulder, Colo.
Iowa State’s Kerton and Marengo say the space telescope is an important part of their work.
“It lets me see objects that are obscured,” says Kerton, who helped plan the GLIMPSE360 survey. “It allows me to detect young, newly formed stars that wouldn’t be seen any other way. And it shows them at a resolution that helps us understand what we’re seeing.”
Where old surveys showed a single blob, Kerton says, the Spitzer images show a cluster of stars.
Marengo was part of the instrument group that built and calibrated Spitzer’s hardware.
“Spitzer is really, really sensitive,” Marengo says. “The first time it was turned on—before it was even calibrated—a 10-second exposure provided the equivalent depth of an exposure that used to take 10 hours with the 10-meter Keck telescope, the largest on Earth.”
That, he says, is a big advantage when astronomers are trying to observe very cool, faint stars. And for his work, there are no ground telescopes that can match Spitzer’s capabilities.
And now that the Spitzer Space Telescope is pointed away from the better-known inner galaxy, Kerton and Marengo say it will help astronomers understand unexplored parts of our galaxy through the end of the GLIMPSE360 survey early next year.
“Spitzer is getting farther and farther away,” Marengo adds. “And it’s revealing more year by year.”
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