Excerpt from wired.com
In 2007, A Dutch schoolteacher named Hanny var Arkel
discovered a weird green glob of gas in space. Sifting through pictures
of galaxies online, as part of the citizen science project Galaxy Zoo,
she saw a cloud, seemingly glowing, sitting next to a galaxy.
Intrigued, astronomers set out to find more of these objects, dubbed
Hanny’s Voorwerp (“Hanny’s object” in Dutch). Now, again with the help
of citizen scientists, they’ve found 19 more of them, using the Hubble
space telescope to snap the eight haunting pictures in the gallery
above.
Since var Arkel found the first of these objects, hundreds more
volunteers have swarmed to help identify parts of the universe in the
Galaxy Zoo gallery. To find this new set, a couple hundred volunteers
went through nearly 16,000 pictures online (seven people went through all
of them), clicking yes/no/maybe as to whether they saw a weird green
blob. Astronomers followed up on the galaxies they identified using
ground-based telescopes, and confirmed 19 new galaxies surrounded by
green gas.
What causes these wispy tendrils of gas to glow? Lurking at the
center of each of these galaxies is a supermassive black hole, millions
to billions times as massive as the sun, with gravity so strong that
even light can’t escape them. As nearby gas and dust swirls into the
black hole, like water circling a drain, that material heats up,
producing lots of radiation—including powerful ultraviolet. Beaming out
from the galaxy, that ultraviolet radiation strikes nearby clouds of
gas, left over from past collisions between galaxies. And it makes the
clouds glow an eerie green. “A lot of these bizarre forms we’re seeing
in the images arise because these galaxies either interacted with a
companion or show evidence they merged with a smaller galaxy,” says William Keel, an astronomer at the University of Alabama, Tuscaloosa.
The eight in this gallery, captured with Hubble, are especially
weird. That’s because the quasar, the black-hole engine that’s supposed
to be churning out the ultraviolet radiation, is dim—too dim, in fact,
to be illuminating the green gas. Apparently, the once-bright quasar has
faded. But because that UV light takes hundreds of thousands of years
to travel, it can continue to illuminate the gas long after its light
source has died away.
That glowing gas can tell astronomers a lot about the quasar that
brought it to light. “What I’m so excited about is the fact that we can
use them to do archaeology,” says Gabriela Canalizo,
an astronomer at the University of California, Riverside, who wasn’t
part of the new research. Because the streaks of gas are so vast,
stretching up to tens of thousands of light years, the way they glow
reveals the history of the radiation coming from the quasar. As the
quasar fades, so will the gas’s glow, with the regions of gas closer to
the quasar dimming first. By analyzing how the glow dwindles with
distance from the quasar, astronomers can determine how fast the quasar
is fading. “This was something we’ve never been able to do,” Canalizo
says.
Measuring how fast the quasar fades allows astronomers to figure out
exactly what’s causing it to turn off in the first place. “What makes
them dim is running out of material to eat,” Canalizo says. That could
happen if the quasar is generating enough radiation to blow away all the
gas and dust surrounding the black hole—the same gas and dust that
feeds it. Without a steady diet, the quasar is powerless to produce
radiation. Only if more gas happens to make its way toward the black
hole can the quasar turn on again. The glowing gas can provide details
of this process, and if other mechanisms are at play.
With more powerful telescopes, astronomers will likely find many
more. Hanny’s Verwoort, it turns out, may not be that weird after all.
Source Article from http://feedproxy.google.com/~r/AscensionEarth2012/~3/qMKJK2AJTMI/citizen-scientists-find-green-blobs-in.html
Citizen Scientists Find Green Blobs in Hubble Galaxy Shots
No comments:
Post a Comment