A Swift Look at the Biggest Explosions in the Universe
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at the Biggest Explosions in the Universe
to rapidly locate gamma-ray burst sources
By then the mystery had led NASA, in 1978, to select the the Burst and Transient Source Experiment (BATSE) as one of four instruments aboard the Compton Gamma Ray Observatory (launched in 1991). BATSE was envisioned as a fire alarm that would notify the other instruments on the observatory to help scientists settle this nagging little mystery.
Right: Artist's concept of the Swift satellite observing a burst. Credit: NASA/Goddard.
In this role, BATSE wins as "best supporting actor" by showing that bursts are perhaps the most violent explosions we can observe in the universe. This has swept up the astrophysics community. More than 3,200 professional papers have been written about bursts, says Dr. Kevin Hurley of the University of California at Berkeley, and papers are being published at the rate of 1.3 per day, faster than bursts are recorded.
As with any star that has made good, the next step is his or her own starring role. That comes in 2003 with the planned launch of Swift. Breaking with NASA tradition, the name isn't an acronym. It describes how quickly the spacecraft is designed to swing around and put an array of telescopes on target and capture bursts before they fade.
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The primary mission is quite simple, said Dr. Neil Gehrels, the principal investigator at NASA's Goddard Space Flight Center. He described Swift in the last session (Instrumentation) of the 5th Huntsville Gamma Ray Burst Symposium held in Huntsville, Ala., last week.
This animation illustrates why bursts are so hard to localize; they come and go like lightning bolts. By the time you're aware that something had happened, it's too late to turn and look at the flash; you can only listen to the echo. (The burster is superimposed on a galactic gamma-ray image.)
To catch a gamma-ray burst in the act, you need to have
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Swift's three instruments will help answer those questions.
First, BAT will detect the onset of a gamma-ray burst. Unlike BATSE, which has eight modules that view the entire sky (other than what the Earth blocks), BAT will view a smaller fraction of the sky. It will comprise a special kind of pinhole camera called a coded aperture mask placed in front of a large solid-state detector. This will let BAT calculate a burst's location to within a few arc-minutes (a fraction of the Moon's apparent diameter and much finer than BATSE can do).
Left: The XRT and UVOT will be coaligned on the Swift spacecraft, while BAT covers a much larger field of view. The entire spacecraft will turn when BAT detects a burst. Credit: NASA/Goddard.
The UVOT, derived from the optical telescope that Europe's X-ray Multi-Mirror Mission satellite (XMM) will carry, has a 30 cm (12 in.) primary mirror, equivalent to a 4-meter (13.2 ft) telescope on the ground, Gehrels said. It will have a 17 arc-minute field of view (slightly more than half the apparent diameter of the Moon) and sensitivity from 170 nm (ultraviolet) down to 650 nm (deep red).
Using the two telescopes, scientists should be able to locate bursts to within 0.3 arc-seconds, and to tell whether the burst has an optical transient that should be the target of follow-up observations by larger observatories in orbit or on Earth.
While waiting for bursts to go off, Swift will map the sky at high x-ray energies. This hasn't been done since the first High Energy Astronomy Observatory (HEAO-1), which orbited during 1977-79. BAT will be 50 times more sensitive that HEAO-1's Hard X-Ray/Low Energy Gamma Ray Experiment, so it will provide more detailed maps that will help observers find new targets for the Chandra X-ray Observatory and XMM.
And, of course, BATSE, the instrument that has taught us so much about bursts.
Right: The relative fields of view of Swift's two telescopes are overlaid on a segment of the Hubble deep-field image. Swift will provide locations refined enough for Hubble and other high-power telescopes to study bursts in detail. Credit: NASA/Goddard.
And beyond that? After a lead role, most stars look for a blockbuster role. In this case, it will be the Next Generation Gamma-Ray Burst Observatory.
"We want NASA to begin to form a group within this next year to study the mission requirements" for what would come after Swift, said Dr. Gerald Fishman, principal investigator for BATSE at NASA's Marshall Space Flight Center.
"Swift serves as a pathfinder" for the next-generation instrument, Fishman said. "We won't firm up plans until it makes its observations" since those could change the requirements. The design is so distant for now that the next-generation telescope might comprise several spacecraft operating together, and almost certainly will operate interactively with advanced missions like the Gamma-Ray Large Space telescope (GLAST) planned for launch in 2005.
The next-generation instrument would also be used in concert with major observatories on Earth and in orbit.
"This mission is seen primarily as a NASA facility," Fishman continued, "designed by the entire NASA community and used by the science community. Although NASA would play a lead role, it is expected to have international support."
Fishman said scientists are also looking at a new operational model that would involve the National Science Foundation as a full partner rather than having the observatory operated and funded primarily by and for NASA. NSF operates many of the United States' ground-based observatories.
"Since the science is something of interest to both agencies" - ground-based observatories often seek optical counterparts for bursts - "it should be funded by both agencies," Fishman said.
Left: Engineers at MIT prepare HETE-II for launch. Credit: MIT
Right: A Clemson University student examines the primary mirror for Super-LOTIS. Credit: Clemson University.
Chasing those locations will be Super LOTIS, built from an old 60 cm (24-in) reflector telescope provided by the Lick Observatory. Super LOTIS - the Livermore Optical Transient Imaging System built by Lawrence Livermore National Laboratory - has been in tests since "first light" on Feb. 25, 1999.
In addition to looking at night for optical afterglows of gamma-ray bursts, it is programmed to record burst triggers that happen during the day and then try to locate their afterglows at night. Super LOTIS is scheduled to be relocated from Lawrence Livermore to the Kitt Peak National Observatory near Tucson, Arizona where observing conditions are better.1999 GRB Symposium series
Oct 29: A Swift Look at the Biggest Explosions in the Universe Spurred by the thousands of gamma-ray bursts recorded over the last three decades, NASA is planning missions dedicated to discovering the causes of what had been an oddity and now has become a primary mystery.
Oct 25: Postmortems in the Sky To say they are ghoulish may be going too far, but like ghouls those studying Gamma Ray Bursts gleefully seek the moldering remains, and never see the living victim. But they are very much interested in both the victim and the cause.
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.
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