NASA's Swift detects possible birth of black hole
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On Jan. 17, the NASA-led Swift satellite mission detected and imaged its first gamma-ray burst, one of the most powerful explosions to occur in the universe. The burst was in the midst of exploding as Swift, designed to autonomously repoint itself, turned and focused in less than 200 seconds on the event. The satellite was fast enough to capture an image with its X-Ray Telescope (XRT), while gamma rays were still being detected with the Burst Alert Telescope (BAT). "This is the first time an X-ray telescope has imaged a gamma-ray burst whi
On Jan. 17, the NASA-led Swift satellite mission detected and imaged its first gamma-ray burst, one of the most powerful explosions to occur in the universe.
The burst was in the midst of exploding as Swift, designed to autonomously repoint
itself, turned and focused in less than 200 seconds on the event. The satellite was
fast enough to capture an image with its X-Ray Telescope (XRT), while gamma rays were
still being detected with the Burst Alert Telescope (BAT).
"This is the first time an X-ray telescope has imaged a gamma-ray burst while it
was bursting," said Dr. Neil Gehrels, Swift's principal investigator at NASA's
Goddard Space Flight Center, Greenbelt, MD. "Most bursts are gone in about ten
seconds, and few last upwards of a minute. Previous X-ray images have captured
the burst afterglow, not the burst itself."
"This is the one that didn't get away," said Prof. John Nousek, Swift's mission
operations director at Penn State University, in State College, PA. "And this is
what Swift was built to do: to detect these fleeting gamma-ray bursts and focus
its telescopes on them autonomously within about a minute. The most exciting
thing is this mission is just revving up."
Swift has three main instruments. The BAT detects bursts and initiates the
autonomous slewing to bring the XRT and the Ultraviolet/Optical Telescope (UVOT)
within focus of the burst. In December, the BAT started detecting bursts,
including a remarkable triple detection on Dec. 19. Today's announcement
marks the first BAT detection autonomously followed by XRT detection,
demonstrating the satellite is swiftly slewing as planned. The UVOT is still
being tested, and it was not collecting data when the burst was detected. Scientists
expect Swift to be fully operational by Feb. 1.
"We are frantically analyzing the XRT data to understand the X-ray emission seen
during the initial explosion and the very early afterglow," said Dr. David
Burrows, the XRT lead at Penn State. "This is a whole new ballgame. No one has
ever imaged X-rays during the transition of a gamma-ray burst from the brilliant
flash to the fading embers."
The origin of gamma-ray bursts remains a mystery. At least some appear to
originate in massive star explosions. Others might be the result of merging black
holes or neutron stars. Any of these scenarios likely will result in the
formation of a new black hole.
The Swift satellite's two-year mission will be to:
Determine the origin of gamma-ray bursts.
Classify gamma-ray bursts and search for new types.
Determine how the explosion develops.
Use gamma-ray bursts to study the early universe.
Perform the first sensitive hard X-ray survey of the sky.
Swift, still in its checkout phase, is an international collaboration launched on
Nov. 20, 2004. It is a NASA mission in partnership with the Italian Space Agency and the Particle Physics and Astronomy Research Council, United Kingdom.
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Read the source: Wikinews ↗Source published 21 Jan 2005, 05:30 am IST