NASA's Spitzer Finds Hints of Planet Birth Around Dead Star

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April 5, 2006

Erica Hupp/Grey Hautaluoma
Headquarters, Washington 
(202) 358-1237/0668

Whitney Clavin
Jet Propulsion Laboratory, Pasadena, Calif.
(818) 354-4673 

RELEASE: 06-133

NASA'S SPITZER FINDS HINTS OF PLANET BIRTH AROUND DEAD STAR

NASA's Spitzer Space Telescope has uncovered new evidence that planets 
might rise up out of a dead star's ashes. 

Spitzer surveyed the scene around a pulsar, the remnant of an exploded 
star. The infrared telescope found a surrounding disk made up of 
debris shot out during the star's death throes. The dusty rubble in 
this disk might ultimately stick together to form planets. 

This is the first time scientists have detected planet-building 
materials around a star that died in a fiery blast.

"We're amazed that the planet-formation process seems to be so 
universal," said Deepto Chakrabarty of the Massachusetts Institute of 
Technology in Cambridge, principal investigator of the new research. 
"Pulsars emit a tremendous amount of high energy radiation, yet 
within this harsh environment we have a disk that looks a lot like 
those around young stars where planets are formed," he added. 

The paper on the Spitzer finding appears in the April 6 issue of 
Nature. Other authors of the paper are lead author Zhongxiang Wang 
and co-author David Kaplan, both of the Massachusetts Institute of 
Technology.

The finding also represents the missing piece in a puzzle that arose 
in 1992, when Aleksander Wolszczan of Pennsylvania State University 
found three planets circling a pulsar called PSR B1257+12. Those 
pulsar planets, two the size of Earth, were the first planets of any 
type ever discovered outside our solar system. Astronomers have since 
found indirect evidence the pulsar planets were born out of a dusty 
debris disk, but nobody had directly detected this kind of disk until 
now. 

The pulsar observed by Spitzer, named 4U 0142+61, is 13,000 
light-years away in the Cassiopeia constellation. It was once a 
large, bright star with a mass between 10 and 20 times that of our 
sun. The star probably survived for about 10 million years, until it 
collapsed under its own weight about 100,000 years ago and blasted 
apart in a supernova explosion. 

Some of the debris, or "fallback," from that explosion eventually 
settled into a disk orbiting the shrunken remains of the star, or 
pulsar. Spitzer was able to spot the warm glow of the dusty disk with 
its heat-seeking infrared "eyes." The disk orbits at a distance of 
about 1 million miles and probably contains about 10 Earth-masses of 
material. 

Pulsars are a class of supernova remnants, called neutron stars, which 
are incredibly dense. They have masses about 1.4 times that of the 
sun squeezed into bodies only 10 miles wide. One teaspoon of a 
neutron star would weigh about 2 billion tons. Pulsar 4U 0142+61 is 
an X-ray pulsar, meaning that it spins and pulses with X-ray 
radiation. 

Any planets around the stars that gave rise to pulsars would have been 
incinerated when the stars blew up. The pulsar disk discovered by 
Spitzer might represent the first step in the formation of a new, 
more exotic type of planetary system, similar to the one found by 
Wolszczan in 1992. 

"I find it very exciting to see direct evidence that the debris around 
a pulsar is capable of forming itself into a disk. This might be the 
beginning of a second generation of planets," Wolszczan said. 

Pulsar planets would be bathed in intense radiation and would be quite 
different from those in our solar system. "These planets must be 
among the least hospitable places in the galaxy for the formation of 
life," said Charles Beichman, an astronomer at NASA's Jet Propulsion 
Laboratory and the California Institute of Technology, both in 
Pasadena, Calif. 

The Jet Propulsion Laboratory manages the Spitzer Space Telescope 
mission for NASA's Science Mission Directorate, Washington. Science 
operations are conducted at the Spitzer Science Center at Caltech. 
JPL is a division of Caltech. For more information about Spitzer, 
visit: 

www.spitzer.caltech.edu/spitzer  

	
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