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NASA'S
HETE SPOTS RARE GAMMA-RAY BURST AFTERGLOW A
rare optical afterglow of a gamma-ray burst, the most powerful type of explosion
in the universe, was recently discovered by NASA's High Energy Transient Explorer
(HETE), the first satellite dedicated to spotting these frequent yet random explosions
that last only for a few seconds. The
burst occurred in the constellation Lacerta, and was relatively close, only about
5 billion light-years from Earth. Gamma-ray bursts (GRBs) can be more than 10
billion light-years distant. "With this first confirmed observation of a
gamma-ray burst and its afterglow, we've really turned the corner," said
Dr. George Ricker of the Massachusetts Institute of Technology (MIT), Cambridge,
principal investigator for HETE. "As HETE locates more of these bursts, we
will begin to understand what causes them."
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| Animation
of HETE2 observing the GRBs | | |
The
opportunity to see the afterglow in optical light provides crucial information
about what is triggering these mysterious bursts, which scientists speculate to
be the explosion of massive stars, the merging of neutron stars and black holes,
or possibly both. The
burst occurred Sept. 21, but because the enigmatic bursts disappear so quickly,
scientists can best study the events by their afterglow. HETE detects these bursts
as gamma rays or high-energy X-rays, and then instantly relays the coordinates
to a network of ground-based and orbiting telescopes for follow-up searches for
such afterglows. While
GRBs often produce corresponding outpourings of X-rays, astronomers rarely detect
visible light associated with the bursts, perhaps because they originate in regions
of dense gas and dust that obscure any visible light that may be produced by the
explosion. Additional
observations of this event, made with the Italian BeppoSAX satellite and the Ulysses
space probe, were coordinated by HETE team member Dr. Kevin Hurley at the University
of California, Berkeley. The combination of the localization by this Interplanetary
Network with the original HETE coordinates provided the refined information needed
by ground-based observers to point their optical telescopes. Armed
with the satellite-derived localization, the team led by Dr. Shri Kulkarni of
the California Institute of Technology (Caltech), Pasadena, spotted the afterglow
in optical light, with a Large Format Camera on the Palomar 200-inch telescope
on Sept. 22. In follow-up observations on Oct. 17, the Caltech group measured
the "redshift," the distance, of the afterglow object using the Double
Spectrograph on the Palomar 200-inch telescope. In addition, on Oct. 17 they also
pinpointed a twinkling radio counterpart using the Very Large Array in Socorro,
N.M. "We believe that this object is very likely the afterglow of GRB 010921,
detected and localized by HETE," said Kulkarni. The
event was also captured 22 hours after the HETE trigger by a robotic telescope
in Tucson, Ariz., operated by Dr. Hye-Sook Park of the Lawrence Livermore National
Laboratory, Livermore, Calif., and her colleagues. HETE
was launched into near-Earth orbit Oct. 9, 2000, to detect gamma-ray bursts, which
signal the extragalactic release of as much power as a billion trillion Suns.
No one is sure though what causes them or exactly where they originate. Like beacons
from the early universe, these bursts are thought to originate billions of light-years
away. "Gamma-ray
bursts are the most energetic events since the Big Bang, yet one occurs about
once a day somewhere in the sky," Ricker said. "The unique power of
HETE is that it not only detects a large sample of these bursts, but it also relays
the accurate location of each burst in real time to ground-based optical and radio
observatories." HETE
was built by MIT and is under NASA's Explorer Program, which is managed by NASA's
Goddard Space Flight Center, Greenbelt, Md. HETE is a collaboration among NASA,
MIT, Los Alamos National Laboratory, N.M.; France's Centre National d'Etudes Spatiales,
Centre d'Etude Spatiale des Rayonnements, and Ecole Nationale Superieure de l'Aeronautique
et de l'Espace; and Japan's Institute of Physical and Chemical Research (RIKEN).
The science team includes members from the University of California (Berkeley
and Santa Cruz) and the University of Chicago, as well as from Brazil, India and
Italy. HETE, the first satellite dedicated to the study of gamma-ray bursts, is
on an extended mission until 2004.
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