NASA's Swift, Fermi Probe Fireworks From a Flaring Gamma-Ray Star

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Feb. 10, 2009

J.D. Harrington 
Headquarters, Washington 
202-358-5241 
j.d.harrington@xxxxxxxx 

Lynn Cominsky 
Sonoma State University, Rohnert Park, Calif. 
707-664-2655 
lynnc@xxxxxxxxxxxxxxxxxxx 

RELEASE: 09-028

NASA'S SWIFT, FERMI PROBE FIREWORKS FROM A FLARING GAMMA-RAY STAR

WASHINGTON -- Astronomers using NASA's Swift satellite and Fermi 
Gamma-ray Space Telescope are seeing frequent blasts from a stellar 
remnant 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." 

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 Oct. 3, 2008, then settled 
down. It roared back to life Jan. 22 with an intense episode. 

Because of the recent outbursts, astronomers will classify the object 
as a soft-gamma-ray repeater -- only the sixth known. In 2004, a 
giant flare from another soft-gamma-ray repeater was so intense it 
measurably affected Earth's upper atmosphere from 50,000 light-years 
away. 

Scientists think the source is a spinning neutron star, which is the 
superdense, city-sized remains of an exploded star. Although only 
about 12 miles across, a neutron star contains more mass than the 
sun. The object has been cataloged as SGR J1550-5418. 

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, 
Ala. The object has triggered the instrument more than 95 times since 
Jan. 22. 

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," Halpern said. "As a result, we don't really know 
the distance to this object as well as we would like. These images 
will help us make a more precise measurement and also determine the 
distance to the dust clouds." 

NASA's Wind satellite, the joint NASA-Japan Suzaku mission, and the 
European Space Agency's INTEGRAL satellite also have detected flares 
from SGR J1550-5418. 

NASA's Goddard Space Flight Center in Greenbelt, Md., manages the 
Swift satellite. It is being operated in collaboration with partners 
in the U.S., the United Kingdom, Italy, Germany and Japan. NASA's 
Fermi Gamma-ray Space Telescope is an astrophysics and particle 
physics observatory developed in collaboration with the U.S. 
Department of Energy and with important contributions from academic 
institutions and partners in France, Germany, Italy, Japan, Sweden, 
and the U.S. 

To see the related images, visit: 



http://www.nasa.gov/mission_pages/swift/bursts/gammaray_fireworks.html 



For more information about the Swift satellite, visit: 










http://www.nasa.gov/swift 


For more information about the Fermi mission, visit; 



http://www.nasa.gov/fermi 

	
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