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Newborn Stars Discovered in Dark Cosmic Cloud

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07 July 2010


Though astronomers first discovered the dark cloud in the Sagittarius constellation more than 30 years ago, it took the keenness of the Spitzer telescope's instruments to spot the hidden stellar nursery within.  Spitzer's infrared vision has shown that M17 SWex is among the closest to Earth and also among the Milky Way's busiest star-making factories, with 488 newly forming stars. More than 200 will become blue-white class B stars, larger and hotter than our Sun. "Most of the stars we've detected are relatively bright," said Povich. "So we predict the actual number of stars forming in M17 SWex is over 10,000, since the fainter stars cannot be detected with the current observations."

Click on image for high-resolution file, or click here for high-resolution image without labels.

Dark, Mysterious Cloud: A dark, wispy cloud of dust (extending from the center, right) seems to billow out from a bright explosion in this false-color image in infrared light from the Spitzer Space Telescope. These views have revealed that the mystery cloud, called M17 SWex, is forming stars at a furious rate but has not yet spawned the most massive stars -- O stars. To the left, on the trailing end of the dark cloud, such mammoth O stars create a dramatic contrast of brilliant light near the image's center.

Credit: NASA/JPL-Caltech/M. Povich (Penn State)

Conspicuously absent from M17 SWex are the bluest, hottest, and biggest of new stars -- the class O stars. Though relatively rare in the cosmos, O stars are what light up neighboring regions within the colossal M17 nebula.

One possible answer to this riddle is that developing O stars — wild, windy, and spewing radiation -- rapidly destroy their dusty envelopes, which Spitzer otherwise would sniff out. But a more likely explanation is that such gigantic stars form later, perhaps needing an extra "nudge" into existence. A shock wave from a burst of star births in the region could set off a chain of massive star formation — a cosmic "domino effect." In support of this idea, Povich and his colleagues point to a giant "bubble" blown by blue O stars aged some two to five million years in the far left of the Spitzer image. Part of this great smoke ring appears to shape the left, curving border of the M17 nebula, whose interior is lit up by a star cluster about one-million years old. Farther to the right, the shrouded, budding stars in the dark M17 SWex cloud have not yet celebrated their one millionth birthdays — truly infants in the stellar sense.

The architecture of our galaxy likely plays a role in this chronology. In its orbit around the Milky Way's center, the M17 region is now passing though the Sagittarius spiral arm, one of the giant bands of stars and gas pinwheeling out from our galaxy's hub. The greater concentration of gas and dust in the arm is mashing material together in the M17 region, triggering a round of massive star formation that moves through this cloud, causing a chain reaction.

"The time-sequence of star formation proceeds in the same direction that a spiral arm crosses the M17 cloud complex," Povich says. "The M17 region brings to mind images of other spiral galaxies where the leading edges of the arms appear blue, with young O stars, but the trailing edges are still dark, with obscuring dust like in M17 SWex." The time required, for the M17 region to pass through the edge of the Sagittarius spiral arm is about a million years.


"We hope that astronomers will use M17 SWex as a new laboratory for studying the mystery of how massive star formation really happens," says Povich. "Most very young clouds being studied don't have as much going on as this one does."

In addition to Povich, another member of the research team is Barbara Whitney of the Space Science Institute of Boulder, Colorado.

[ Katrina Voss ]


Matthew Povich: povich@astro.psu.edu, 814-863-4690

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Q & A with Dr. Povich

Q: "Why is it that star formation is not ubiquitous and everywhere, considering that there are billions and billions of suns?"

--Frank F.


A: Two key facts to remember about stars like the Sun:

  1. They move around quite a bit in our Milky Way Galaxy.
  2. They live for several billion years.

Our Milky Way Galaxy is a vast, disk-shaped structure containing 100 billion stars, the Sun among them. The Milky Way is but one of billions of distinct galaxies that astronomers have observed. The vast spaces in between galaxies are very empty, lacking many stars at all.

The process of star formation is widespread in the Milky Way, but stars can only be born in locations where vast clouds of interstellar gas and dust are able to form and then collapse under the influence of gravity. These clouds tend to form in the beautiful spiral arms that you often see in images of other galaxies (the spiral arms are difficult to see in the Milky Way because we are observing our Galaxy from the inside). In locations where there are no gas clouds, there can be no star formation. But there can still be stars, because the gas clouds themselves dissipate in about 10 million years, but the stars they give birth to live for billions of years (a thousand times longer than the clouds live) and migrate to other parts of the Milky Way.

We can observe many other galaxies where ALL of the gas clouds have dissipated, so there is no star formation in them anymore. But these galaxies, called elliptical galaxies, can contain up to a trillion old stars!