NASA’’s satellites probe fireworks from a flaring gamma-ray starFebruary 11th, 2009 - 4:48 pm ICT by ANI
Washington, Feb 11 (ANI): Astronomers are using NASA’’s Swift satellite and Fermi Gamma-ray Space Telescope to probe frequent blasts from a flaring gamma-ray star 30,000 light-years away.
The high-energy fireworks arise from a rare type of neutron star known as a soft-gamma-ray repeater. Such objects unpredictably send out a series of X-ray and gamma-ray flares.
“At times, this remarkable object has erupted with more than a hundred flares in as little as 20 minutes,” said Loredana Vetere, who is coordinating the Swift observations at Pennsylvania State University.
“The most intense flares emitted more total energy than the sun does in 20 years,” Vetere added.
The object, which has long been known as an X-ray source, lies in the southern constellation Norma. During the past two years, astronomers have identified pulsing radio and X-ray signals from it.
The object began a series of modest eruptions on October 3, 2008, then settled down. It roared back to life on January 22nd with an intense episode.
Because of the recent outbursts, astronomers will classify the object as a soft-gamma-ray repeater, which is only the sixth known till date.
While neutron stars typically possess intense magnetic fields, a subgroup displays fields 1,000 times stronger. These so-called magnetars have the strongest magnetic fields of any known object in the universe.
SGR J1550-5418, which rotates once every 2.07 seconds, holds the record for the fastest-spinning magnetar.
Astronomers think magnetars power their flares by tapping into the tremendous energy of their magnetic fields.
“The ability of Fermi’’s gamma-ray burst monitor to resolve the fine structure within these events will help us better understand how magnetars unleash their energy,” said Chryssa Kouveliotou, an astrophysicist at NASA’’s Marshall Space Flight Center in Huntsville, Alabama.
Using data from Swift’’s X-ray telescope, Jules Halpern at Columbia University captured the first “light echoes” ever seen from a soft-gamma-ray repeater.
Images acquired when the latest flaring episode began show what appear to be expanding halos around the source.
Multiple rings form as X-rays interact with dust clouds at different distances, with closer clouds producing larger rings.
Both the rings and their apparent expansion are an illusion caused by the finite speed of light and the longer path the scattered light must travel.
“X-rays from the brightest bursts scatter off of dust clouds between us and the star. As a result, we don”t really know the distance to this object as well as we would like,” Halpern said.
“These images will help us make a more precise measurement and also determine the distance to the dust clouds,” he added. (ANI)
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