Dodging pitfalls in the hunt for the cause of gamma-ray bursts
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Dodging pitfalls in the hunt for the cause of gamma-ray
Oct 21, 1999: Three decades after the discovery of gamma-ray bursts, their causes remain elusive and still offer potential pitfalls for investigators.
"We really need to be careful ... and make sure that we're interpreting the meager data carefully," said Dr. Gerald Fishman of NASA's Marshall Space Flight Center. Speaking at the Fifth biennial Huntsville Gamma Ray Burst Symposium, Fishman reviewed a number of the questions that astrophysicists still have to resolve in what has moved from an oddity to a hot topic.
Right: The Vela 5b satellite, launched in 1965, was one of a series of satellites that recorded the some of the earliest extra-galactic gamma-ray bursts ever seen.
With the launch in April 1991 of the Compton Gamma Ray Observatory, scientists hoped to identify the burst sources. Instead, Fishman's Burst and Transient Source Experiment (BATSE), one of the observatory's four instruments, soon showed that the bursts were evenly scattered across the heavens. Combined with the fact that there were fewer weak bursts than anticipated, the discovery implied bursts originated from near the edge of the observable universe.
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(A gentle reminder of that earned a laugh when Fishman put up a plot of the 2512 bursts BATSE has recorded. "For historical reasons we plot this in galactic coordinates," he said, since even he expected them to have galactic origins. "Perhaps we should change it to celestial coordinates.")
Yet even with more than 2,500 bursts recorded by BATSE, and more than a dozen apparent burst sources captured by optical and other telescopes, mystery still shrouds the cause and caution must be used in interpreting the data.
For example, Fishman said, astrophysicists sometimes refer to statistically significant spectral lines appearing in the data.
Above: Because scientists originally believed gamma-ray bursts came from within our galaxy, location maps for GRBs have always been plotted in galactic coordinates. However, scientists have since discovered GRBs are distributed isotropically, that is, uniformly throughout the sky, indicating a cosmological origin.
"We have yet to see a gamma-ray feature that shows up consistently among detectors," Fishman said. "That says to us that we don't understand the systematic errors in our own system."
Left: One of the 8 BATSE detector modules. This is a "structural test model," built to determine whether the design is rigorous enough for space flight.
A candidate for the cause of gamma-ray bursts is exceptionally violent supernovae or hypernovae. They would have similar energies, and both could involve energy beamed like water from a fire hose. "We see tantalizing results, but none are definitive," Fishman cautioned.
Another reported finding is that short-duration gamma-ray bursts are anisotropic, meaning they are more numerous in one area. (A good example of anisotropy is our night sky: most stars are seen in the Milky Way, our view across our galaxy.) Not so, Fishman said. Short bursts are isotropic - evenly scattered across the sky.
Right: A sample light curve showing a typical profile for a gamma-ray burst..
"It's trying to tell us something," Fishman said. "We're just not smart enough to understand it yet."
Some of the uncertainty comes from how BATSE modules detect and measure bursts, admitted Dr. Charles Meegan, also of NASA/Marshall. These "self-inflicted biases" can make the work more challenging. For example, "slow risers" can be missed if the burst rises slowly enough that the BATSE electronics think it's a variation in the background noise.
Or the apparent peak flux can vary. Whether a burst produces 100 counts in 100 milliseconds or 1 second, the electronics will trigger since they are keyed to 100 counts in 1,024 milliseconds (1.024 sec). Meegan said that the BATSE team is working to measure the biases.
Nevertheless, BATSE and other instruments such as the Dutch-Italian Beppo-SAX and Japanese ASCA satellites have produced a wealth of information allowing scientists to try peeling back some of the layers of mystery surrounding gamma-ray bursts. These include:
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- Dr. Jon Hakkila of Minnesota State University has used pattern
recognition programs from an artificial intelligence project
to analyze three classes of gamma-ray bursts and determined that
there are really two classes. Class 1 bursts are long, have high
fluence or total counts, and intermediate hardness in the spectra.
Class 2 bursts are short and have low fluence and hard spectra.
What appeared to be Class 3 bursts are really Class 1 bursts
that mimic Class 3 due to measurement errors or a newly identified
bias in BATSE.
- The "Holy Grail" of gamma-ray bursts may be in
sight, according to Dr. Jay Norris of NASA's Goddard Space Flight
Center. He said that it appears that time variations in a burst
come directly from the central engine itself. Previously it was
thought that the variations were caused by the expanding blast
wave of material slamming into clumps of materials in space.
Already scientists know that longer bursts have lower peaks.
If the burst were from the central engine - whatever it might
be - then measuring the distance to a burst would become easier.
It would be akin to measuring the scale of the universe by the
apparent brightness of variable Cepheid stars. Their brightness
and periods are closely linked, so measuring the period and brightness
of one allows a quick computation of the distance. A similar
method could be applied to gamma-ray bursts - once enough bursts
have been connected with visible sources and host galaxies to
establish a good unit of measurement.
- 220,000 electron volts is a magic number that characterizes the energy of gamma-ray bursts, but no one yet knows why, said Dr. Rob Preece of the University of Alabama in Huntsville. "It's a mystery," Preece said. "It falls out around 200 keV. But why it should be that particular value, and why you don't very often have bursts that are 10 times that or one-tenth is a mystery." 220 keV is the intersection of two lines drawn in a power law. It's basically two straight-line graphs, except the axes are logarithmic (the same distance on the line means a tenfold increase in value; this compresses immense events to a manageable graph)
"Power laws are eagerly sought in astrophysics because they tend to say something is happening in a particular way," Preece explained. Most bursts observed by BATSE plot as two power-law lines, one rising, and one falling. The great majority intersects around 220 keV. A speaker will offer possible meanings for that number later in the week.
|1999 GRB Symposium series|
Oct 21: Dodging pitfalls in the hunt for the cause of gamma-ray bursts Scientists discuss how to avoid making mistakes while searching for the solution to a big astrophysical mystery - What causes gamma-ray bursts?
Oct 20: Outbursts Result in Controversy Scientists have different ideas to explain the behavior of Soft Gamma Repeaters (SGRs).
Oct 18: After three decades of study, gamma-ray bursts still mystify Science@NASA caught up with Dr. Gerald Fishman for an interview about bursts and the symposium.
Oct 11: Gamma-ray bursts to take center stage at international meeting More than 200 astronomers will gather to talk about gamma-ray bursts, one of the most mysterious and increasingly watched-for phenomena in the universe.
1997 GRB Symposium Series - News from the 4th GRB Symposium in 1997.
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