Kathy
May 9, 1998 | Volume 153 | Number 19 - Science News
Gamma-Ray Burst Makes Quite a Bang
by R. Cowen
For one brief moment, long ago in a far-away galaxy, a
titanic explosion
poured a torrent of gamma rays into space. Some 12 billion
years later --
Dec. 14, 1997 -- this flash of radiation reached Earth.
Astronomers are calling this gamma-ray burst "the most
powerful explosion
since the Big Bang." While that may be hyperbole, researchers
have
calculated that this cosmic flash packed 100 times more
energy than a
supernova explosion. Until now, researchers had considered
supernovas the
most energetic phenomenon known.
For the second or two that it lasted, "this burst was
as luminous as all
the rest of the entire universe," says S. George Djorgovski
of the
California Institute of Technology in Pasadena, a member
of the team
reporting the finding in the May 7 Nature. The group
calculated the energy
from the brightness of the burst and its afterglow, as
well as the distance
of the host galaxy from Earth -- 12 billion light-years.
Gamma rays from the burst were detected by the Dutch-Italian
BeppoSAX
satellite and NASA's Compton Gamma Ray Observatory. Then
came a crucial
step in finding the host galaxy. BeppoSAX also recorded
an X-ray afterglow,
part of the smoldering fireball that lingers after gamma
rays have
vanished.
A few hours later, using the afterglow as a guide, Jules
P. Halpern of
Columbia University and his colleagues detected a visible-light
afterglow,
they report in the May 7 Nature. Two weeks later, Djorgovski's
team used
the Keck II Telescope on Hawaii's Mauna Kea to find the
host galaxy.
This marks the second time that astronomers have measured
the distance to a
galaxy that hosted a gamma-ray burst (SN: 5/17/97, p.
305).
These observations settle the long-standing debate over
whether most
gamma-ray bursts originate within our galaxy or far beyond
it, some
astronomers say. However, several of the findings call
into question a
popular theory in which bursts are generated when two
dense stars, known as
neutron stars, collide and merge.
Dale A. Frail of the National Radio Astronomy Observatory
in Socorro, N.M.,
notes that to generate the energy associated with the
Dec. 14 burst,
virtually the entire mass of the neutron stars had to
have been converted
into gamma rays -- an unlikely situation.
Frail told Science News that data from another burst,
detected March 29,
may prove equally damning for the theory. For the first
time, researchers
glimpsed an afterglow at radio wavelengths before finding
one in visible
light.
That sequence suggests that the burst originated from
a place containing
lots of dust, which blocks visible light but is transparent
to radio waves.
Stellar nurseries are rich in dust, and previous studies
have hinted that
several other bursts originated in star-forming locales.
Neutron stars
"cannot merge within star-forming regions," asserts Bohdan
Paczyn´ski of
Princeton University. He explains that during the 100
million years or so
that it would take for neutron stars to form and merge,
they would have
migrated from their birthplace.
Paczyn´ski favors another model -- described in
the Feb. 10 Astrophysical
Journal Letters -- in which a massive, short-lived star
undergoes a
"hypernova" explosion, hurling a shock wave into space
at nearly the speed
of light.
>From Science News, Vol. 153, No. 19, May 9, 1998, p.
292.
Copyright Ó 1998 by Science Service.
References:
Halpern, J.P., et al. Optical afterglow of the g -ray
burst of 14 December
1997. Nature 393(May 7):41.
Kulkarni, S.R., S.G. Djorgovski, et al. 1998. Identification
of a host
galaxy at redshift z = 3.42 for the g -ray burst of 14
December 1997.
Nature 393(May 7):35.
Paczynski, B. 1998. Are gamma-ray bursts in star-forming
regions?
Astrophysical Journal Letters 494(February 10):L45.
Further Readings:
Cowen, R. 1997. Gamma-ray burst mystery continues. Science
News 151(May
17):305.
Sources:
S. George Djorgovski
California Institute of Technology
Palomar Observatory 105-24
Pasadena, CA 91125
Dale A. Frail
National Radio Astronomy Observatory
P.O. Box 1003 Lopezville Road
Socorro, NM 87801
Bohdan Paczynski
Princeton University
Princeton University Observatory
Princeton, NJ 08544-1001