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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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Licensed archive reporting by Wikinews contributors. Text: Public domain (https://en.wikinews.org/wiki/Wikinews:Copyright). Original source date retained. 411 has not independently verified this archive report.

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Source published 21 Jan 2005, 05:30 am IST

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