COLUMBUS , Ohio -- Are you losing sleep at night because you're
afraid that all life on Earth will suddenly be annihilated by a
massive dose of gamma radiation from the cosmos?
Well, now you can rest easy.
Some scientists have wondered whether a deadly astronomical event
called a gamma ray burst could happen in a galaxy like ours, but a
group of astronomers at Ohio State University and their colleagues
have determined that such an event would be nearly
impossible.
Gamma ray bursts (GRBs) are high-energy beams of radiation that
shoot out from the north and south magnetic poles of a particular
kind of star during a supernova explosion, explained Krzysztof
Stanek, associate professor of astronomy at Ohio State. Scientists
suspect that if a GRB were to occur near our solar system, and one
of the beams were to hit Earth, it could cause mass extinctions all
over the planet.
The GRB would have to be less than 3,000 light years away to pose a
danger, Stanek said. One light year is approximately 6 trillion
miles, and our galaxy measures 100,000 light years across. So the
event would not only have to occur in our galaxy, but relatively
close by, as well.
In the new study, which Stanek and his coauthors submitted to the
Astrophysical Journal, they found that GRBs tend to occur in small,
misshapen galaxies that lack heavy chemical elements (astronomers
often refer to all elements other than the very lightest ones --
hydrogen, helium, and lithium -- as metals). Even among metal-poor
galaxies, the events are rare -- astronomers only detect a GRB once
every few years.
But the Milky Way is different from these GRB galaxies on all
counts -- it's a large spiral galaxy with lots of heavy
elements.
The astronomers did a statistical analysis of four GRBs that
happened in nearby galaxies, explained Oleg Gnedin, a postdoctoral
researcher at Ohio State. They compared the mass of the four host
galaxies, the rate at which new stars were forming in them, and
their metal content to other galaxies catalogued in the Sloan
Digital Sky Survey.
Though four may sound like a small sample compared to the number of
galaxies in the universe, these four were the best choice for the
study because astronomers had data on their composition, Stanek
said. All four were small galaxies with high rates of star
formation and low metal content.
Of the four galaxies, the one with the most metals -- the one most
similar to ours -- hosted the weakest GRB. The astronomers
determined that the odds of a GRB occurring in a galaxy like that
one to be approximately 0.15 percent.
And the Milky Way's metal content is twice as high as that galaxy,
so our odds of ever having a GRB would be even lower than 0.15
percent.
"We didn't bother to compute the odds for our galaxy, because 0.15
percent seemed low enough," Stanek said.
He figures that most people weren't losing sleep over the
possibility of an Earth-annihilating GRB. "I wouldn't expect the
stock market to go up as a result of this news, either," he said.
"But there are a lot of people who have wondered whether GRBs could
be blamed for mass extinctions early in Earth's history, and our
work suggests that this is not the case."
Astronomers have studied GRBs for more than 40 years, and only
recently determined where they come from. In fact, Stanek led the
team that tied GRBs to supernovae in 2003.
He and Gnedin explained that when a very massive, rapidly rotating
star explodes in a supernova, its magnetic field directs gamma
radiation to flow only out of the star's north and south magnetic
poles, forming high-intensity jets.
Scientists have measured the energies of these events and assumed
-- rightly so, Stanek said -- that such high-intensity radiation
could destroy life on a planet. That's why some scientists have
proposed that a GRB could have been responsible for a mass
extinction that occurred on Earth 450 million years ago.
Now it seems that gamma ray bursts may not pose as much a danger to
Earth or any other potential life in the universe, either, since
they are unlikely to occur where life would develop.
Planets need metals to form, Stanek said, so a low-metal galaxy
would probably have fewer planets, and fewer chances for
life.
He added that he didn't originally intend to address the question
of mass extinctions. The study grew out of a group discussion
during the Ohio State Department of Astronomy's "morning coffee" --
a daily half-hour where faculty and students review new astronomy
journal articles that have been posted to Internet preprint servers
overnight. In February, Stanek published a paper on a GRB he had
observed, and during coffee someone asked whether he thought it was
just a coincidence that these events seem to happen in small,
metal-poor galaxies.
"My initial reaction was that it's not a coincidence, and everyone
just knows that GRBs happen in metal-poor galaxies. But then people
asked, 'Is it really that well known? Has anybody actually proven
it to be true?' And we realized that nobody had."
As a result, the list of coauthors on the paper includes
astronomers across a broad range of expertise, which Stanek said is
somewhat unusual in these days of specialized research. The
coauthors were among faculty gathered for coffee that day, plus a
few friends they recruited to help them: Stanek and Gnedin; John
Beacom, assistant professor of physics and astronomy; Jennifer
Johnson, assistant professor of astronomy; Juna Kollmeier, a
graduate student; Andrew Gould, Marc Pinsonneault, Richard Pogge,
and David Weinberg, all professors of astronomy at Ohio State; and
Maryam Modjaz, a graduate student at the Harvard-Smithsonian Center
for Astrophysics.