Milky way churning out new stars at a furious pace
Some of the first data from a new orbiting infrared telescope are revealing that the Milky Way - and by analogy galaxies in general - is making new stars at a much more prolific pace than astronomers imagined.
Caption: The nebula RCW49, shown in infrared light in this image from the Spitzer Space Telescope, is a nursery for newborn stars. Using NASAs Spitzer Space Telescope, astronomers have found in RCW49 more than 300 newborn or protostars, all with circumstellar disks of dust and gas. The discovery reveals that galaxies make new stars at a much more prolific rate than previously imagined. The stelar disks of dust and gas not only feed material onto the growing new stars, but can be the raw material for new planetary systems.
Photo by: NASA/JPL-Caltech/University of Wisconsin-Madison
The findings from NASAs Spitzer Space Telescope were announced today (May 27) at a NASA headquarters press briefing by Edward Churchwell, a University of Wisconsin-Madison astronomer and the leader of a team conducting the most detailed survey to date of our galaxy in infrared light.
Focusing the telescope on a compact cluster of stars at the heart of a distant nebula known as RCW49, Churchwell and his colleagues discovered more than 300 newly forming stars. Each of the stars, known to astronomers as protostars, has a swirling disk of circumstellar dust and creates ideal conditions for the formation of new solar systems.
"In this one small area, we have a stellar nursery like no one has ever seen before," says Churchwell, an expert on star formation. "The sheer number of objects is astounding, and may force us to rewrite our ideas of star formation and how much of it is going on in the Milky Way.
"I am dead sure there are many regions like this throughout the galaxy. It is not unique."
For years, astronomers have probed objects like the nebula RCW49, a thick, obscuring cocoon of dust and gas, with radio telescopes. Listening in, they have learned that these hidden pockets of space are the places where most of the new stars that populate a galaxy are born.
With the Spitzer Space Telescope, astronomers can now look deep inside these regions to directly observe star formation: "We can peel away the dust layers to see what is going on and were seeing things in incredible detail. This telescope is almost perfectly tuned to study star formation and it will provide us with a huge database of protostars. And this is what makes galaxies tick, these areas of massive star formation," Churchwell says.
Indeed, his team has been able to catalog not only a large number of protostars from this one small region of space, but also the spectrum of newborn stars various stages of early development.
"Were finding stars at different points in their evolutionary history," Churchwell explains. "We hope to be able to fill out the entire early evolutionary sequence of a stars development."
Of special interest to astronomers is the potential for protostars to form planetary systems. The stars are formed from large disks of cool dust and gas, known as accretion disks. The nascent stars grow as material spirals inward from the disk to the star.
The same disks, astronomers think, provide the raw material for planets. "Protostars, we believe, develop planetary systems from these accretion disks," Churchwell notes.
The Spitzer Space Telescope is the last of NASAs Great Observatory Program. NASAs Jet Propulsion Laboratory in Pasadena, Calif., manages the telescope project.
The Great Observatory program, which also includes the Hubble Space Telescope, the Compton Gamma Ray Observatory and the Chandra X-ray Observatory, is designed to sample the cosmos across a wide portion of the electromagnetic spectrum.
The Spitzer Space Telescope was launched into an Earth-trailing heliocentric orbit in August of 2003.
Churchwells team, which uses the Infrared Array Camera, one of three scientific instruments aboard the telescope, is charged with creating an infrared mosaic of a swath of the inner Milky Way composed of 300,000 image frames of 1.2 second exposures each.
"Were making a complete survey of the inner two-thirds of our galaxy," Churchwell explains. "We cant survey the very center of the galaxy because it is too bright and would swamp our detectors."
When completed, the survey will provide a wealth of data from regions of space previously obscured by foreground clouds of dust and gas. There will be many more surprises, Churchwell says.
The data are being analyzed by a team of about 20 scientists in Madison and around the country who make up the GLIMPSE or Galactic Legacy Infrared Mid-Plain Survey Extraordinaire. The final data products will be archived and released to the astronomy community by the Spitzer Space Science Center in Pasadena, Calif.
Churchwell says the orbiting observatory is performing superbly. "From the perspective of the Infrared Array Camera, its almost picture perfect. The images are beautiful. Its a real success story for NASA," he says.
Terry Devitt, (608) 262-8282, firstname.lastname@example.org
CONTACT: Ed Churchwell, (608) 262-4909, email@example.com; Barbara Whitney, (608) 263-0807, firstname.lastname@example.org
Terry Devitt | EurekAlert!