Stellar extremophiles
November 8, 2011 By Dr. Tony Phillips
This composite (radio+UV) image shows long octopus-like arms of star formation stretching far away from the main disk of spiral galaxy M83. Credit: NASA/JPL-Caltech/VLA/MPIA
Back in the 1970s, biologists were amazed to discover a form of life they never expected. Tiny microorganisms with ancient DNA were living in the hot springs of Yellowstone National Park. Instead of dissolving in the boiling waters, the microbes were thriving, ringing the springs with vibrant color.
Scientists coined the term extremophile, which means "extreme-loving", to describe the creatures--and the hunt was on for more. Soon, extremophiles were found living in deep Antarctic ice, the cores of nuclear reactors, and other unexpected places. Biology hasn't been the same since.
Could astronomy be on the verge of a similar transformation?
Researchers using a NASA space telescope named GALEX have discovered a new kind of extremophile: extreme-loving stars.
"Were finding stars in extreme galactic environments where star formation isn't supposed to happen," explains GALEX project scientist Susan Neff of the Goddard Space Flight Center. This is a very surprising development."
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This composite (radio+UV) image shows long octopus-like arms of star formation stretching far away from the main disk of spiral galaxy M83.
GALEX, which stands for Galaxy Evolution Explorer, is an ultraviolet space telescope with a special ability: It is super-sensitive to the kind of UV rays emitted by the youngest stars. This means the observatory can detect stars being born at very great distances from Earth, more than halfway across the Universe. The observatory was launched in 2003 on a mission to study how galaxies change and evolve as new stars coalesce inside them.GALEX accomplished that missionand more.
"In some GALEX images, we see stars forming outside of galaxiesin places where we thought the gas density would be too low for star birth to occur," says GALEX team member Don Neil of Caltech.
Stars are born when interstellar clouds of gas collapse and contract under the pull of their own gravity. If a cloud gets dense and hot enough as it collapses, nuclear fusion will kick in andvoila!--a star is born.
The spiral arms of the Milky Way are a "goldilocks zone" for this process. "Here in the Milky Way we have plenty of gas. Its a cozy place for stars to form," says Neil.
But when GALEX looks at other more distant spiral galaxies, it sees stars forming far outside the gassy spiral disk.
"I was dumbfounded," he says. "These stars are truly 'living on the edge. '"
Spirals arent the only galaxies with stellar extremophiles. The observatory has also found stars being born
--in elliptical and irregular galaxies thought to be gas-poor (e.g., 1, 2)
--in the gaseous debris of colliding galaxies (1, 2)
--in vast "comet-like" tails that trail behind some fast-moving galaxies (1, 2)
--in cold primordial gas clouds, which are small and barely massive enough to hang together
So much for the Goldilocks Zone. According to GALEX, stellar extremophiles populate just about every nook and cranny of the cosmos where a wisp of gas can get together to make a new sun.
This could be telling us something profound about the star-forming process, says Neff. There could be ways to make stars in extreme environments that we havent even thought of yet.
Will extremophiles transform astronomy as they did biology? Its too soon to say, insist the researchers. But GALEX has definitely given them something to think about.
Provided by Science@NASA
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Nov 08, 2011
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A recent paper has been published outlining some of the peculiar features of this galaxy: http://arxiv.org/...50v1.pdf
Nov 08, 2011
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The star formation and galaxy formation process must be hightly inefficient and must leave considerable amounts of matter uncollected. Further galaxy mergers in simulations spew billions of stars into extra-galactic space.
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"The star formation and galaxy formation process must be hightly inefficient and must leave considerable amounts of matter uncollected. Further galaxy mergers in simulations spew billions of stars into extra-galactic space."
The resulting multitudes of stars and gaseous nebulae would show up in the Lyman-alpha forests of the most distant quasars. As this is not observed, it is concluded that the universe is not densely filled with gas and stars between galaxies and galaxy clusters.
This hot intergalactic gas, heated by energetic radiation from the embedded populations of stars would also emit copiously (and isotropically) in the xray portion of the spectrum, and this again is not observed.
Nov 08, 2011
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However, I think this case is probably more related to the plethora of minor satellite galaxies found around the milky way, and the relative lack of detection of these satellites around other major galaxies.
I think our understanding will evolve as our instruments and observations do - I bet this is just a piece of the puzzle understanding the local interactions of a galaxy.
Nov 08, 2011
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Your overlooking the mulitudinous effects of myriads of stars that would present themselves in even the narrowest spectrographic slit, assuming stars are distributed isotropically in intergalactic space. The effect would be quite noticeable in the very noisy S/N ratio.
Nov 08, 2011
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This is supported by the article, as the new instrument finds stars where they were not expected - meaning they were either attributed to be directly in the galaxy or not enough signal to detect at all, probably some variation of both:
Once again, I was just making a statement regarding the limits of our observations, but not the magnitude of the margin of error.
I would assume that it is small enough not to overturn any major conclusions, but just pointing out that there are probably many interesting but small details we have yet to see.
Nov 08, 2011
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A recent paper also uses HST observations to examine starbirth in the inner and outer regions of M 83: http://arxiv.org/...37v1.pdf
M 83 presents a unique, nearby specimen of a massive, isolated galaxy undergoing intense starbirth in its' inner regions, and an abundant supply of raw materiel and a stellar bar to help fuel the vigorous activity that we see.
Nov 08, 2011
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Anything forms wherever it can. Elements, chemical compounds, life, societies, cities, planets, stars, galaxies. That's elementary. The question is: where can it form?
Nov 09, 2011
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I know you actually meant - where CAN'T it form...:-)
I just happen to feel that if ANYthing self-assembles/evolves (utilizing the rudimentary elements in it's environment) into a (more complex than it's elements) "thing", it is alive.
Just my "theory"...
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