Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

Milky way churning out new stars at a furious pace

28.05.2004


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 NASA’s 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 NASA’s 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 we’re 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.

"We’re 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 star’s 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 NASA’s Great Observatory Program. NASA’s 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.

Churchwell’s 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.

"We’re making a complete survey of the inner two-thirds of our galaxy," Churchwell explains. "We can’t 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, it’s almost picture perfect. The images are beautiful. It’s a real success story for NASA," he says.


Terry Devitt, (608) 262-8282, trdevitt@wisc.edu

CONTACT: Ed Churchwell, (608) 262-4909, churchwell@astro.wisc.edu; Barbara Whitney, (608) 263-0807, bwhitney@wisc.edu

Terry Devitt | EurekAlert!
Further information:
http://www.wisc.edu/

More articles from Physics and Astronomy:

nachricht Liquid crystals in nanopores produce a surprisingly large negative pressure
25.04.2019 | The Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences

nachricht New robust device may scale up quantum tech, researchers say
25.04.2019 | Purdue University

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Full speed ahead for SmartEEs at Automotive Interiors Expo 2019

Flexible, organic and printed electronics conquer everyday life. The forecasts for growth promise increasing markets and opportunities for the industry. In Europe, top institutions and companies are engaged in research and further development of these technologies for tomorrow's markets and applications. However, access by SMEs is difficult. The European project SmartEEs - Smart Emerging Electronics Servicing works on the establishment of a European innovation network, which supports both the access to competences as well as the support of the enterprises with the assumption of innovations and the progress up to the commercialization.

It surrounds us and almost unconsciously accompanies us through everyday life - printed electronics. It starts with smart labels or RFID tags in clothing, we...

Im Focus: Energy-saving new LED phosphor

The human eye is particularly sensitive to green, but less sensitive to blue and red. Chemists led by Hubert Huppertz at the University of Innsbruck have now developed a new red phosphor whose light is well perceived by the eye. This increases the light yield of white LEDs by around one sixth, which can significantly improve the energy efficiency of lighting systems.

Light emitting diodes or LEDs are only able to produce light of a certain colour. However, white light can be created using different colour mixing processes.

Im Focus: Quantum gas turns supersolid

Researchers led by Francesca Ferlaino from the University of Innsbruck and the Austrian Academy of Sciences report in Physical Review X on the observation of supersolid behavior in dipolar quantum gases of erbium and dysprosium. In the dysprosium gas these properties are unprecedentedly long-lived. This sets the stage for future investigations into the nature of this exotic phase of matter.

Supersolidity is a paradoxical state where the matter is both crystallized and superfluid. Predicted 50 years ago, such a counter-intuitive phase, featuring...

Im Focus: Explosion on Jupiter-sized star 10 times more powerful than ever seen on our sun

A stellar flare 10 times more powerful than anything seen on our sun has burst from an ultracool star almost the same size as Jupiter

  • Coolest and smallest star to produce a superflare found
  • Star is a tenth of the radius of our Sun
  • Researchers led by University of Warwick could only see...

Im Focus: Quantum simulation more stable than expected

A localization phenomenon boosts the accuracy of solving quantum many-body problems with quantum computers which are otherwise challenging for conventional computers. This brings such digital quantum simulation within reach on quantum devices available today.

Quantum computers promise to solve certain computational problems exponentially faster than any classical machine. “A particularly promising application is the...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

VideoLinks
Industry & Economy
Event News

Revered mathematicians and computer scientists converge with 200 young researchers in Heidelberg!

17.04.2019 | Event News

First dust conference in the Central Asian part of the earth’s dust belt

15.04.2019 | Event News

Fraunhofer FHR at the IEEE Radar Conference 2019 in Boston, USA

09.04.2019 | Event News

 
Latest News

High-efficiency thermoelectric materials: New insights into tin selenide

25.04.2019 | Materials Sciences

Salish seafloor mapping identifies earthquake and tsunami risks

25.04.2019 | Earth Sciences

Using DNA templates to harness the sun's energy

25.04.2019 | Life Sciences

VideoLinks
Science & Research
Overview of more VideoLinks >>>