Chandra observatory finds evidence of stellar cannibalism
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Chandra observatory finds evidence of stellar cannibalism

Last Updated: Wednesday, September 15, 2010, 15:30     A- A A+
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Chandra observatory finds evidence of stellar cannibalism Washington: NASA's Chandra X-ray Observatory has found a "cannibal" star which is believed to have eaten up a companion star or planet, a discovery that provides new insight into how stars and the planets around them may interact as they age.

The star identified as BP Piscium (BP Psc) appears to be a more evolved version of the Sun but surrounded by a dusty and gaseous disk.

Located about 1,000 light years from Earth, the star is found with a pair of jets several light years long blasting out of the system in opposite direction.

While the disk and jets are characteristics of a very young star, astronomers believe BP Psc is an old star in its so-called red giant phase.

These are in fact remnants of a recent and catastrophic interaction whereby a nearby star or giant planet was consumed by the star, the scientists said in a paper appeared in 'The Astrophysical Journal Letters'.

According to them, when stars like the Sun begin to run out of nuclear fuel, they expand and shed their outer layers.

For example, the Sun is expected to swell so that it nearly reaches or possibly engulfs Earth, as it becomes a red giant star.

Joel Kastner of the Rochester Institute of Technology, who led the Chandra study, said: "It appears that BP Psc represents a star-eat-star Universe or maybe a tar-eat-planet one. Either way, it just shows it's not always friendly out there."

The Chandra X-ray Observatory is a satellite launched by NASA in 1999. It was named after Indian-American physicist Subrahmanyan Chandrasekhar, who is known for determining the maximum mass for white dwarfs.

Several pieces of information have led astronomers to rethink how old BP Psc might be. The star is not located near any star-forming cloud, and its atmosphere contains only a small amount of lithium. And its surface gravity also appears to be too weak for a young star and instead matches up with one of an old red giant.

"It seems that BP Psc has been energised by its meal," said co-author Rodolfo Montez Jr, also from the Rochester Institute of Technology.

The star's surface is obscured throughout the visible and near-infrared bands, so the Chandra observation represents the first detection at any wavelength of BP Psc itself.

"BP Psc shows us that stars like our Sun may live quietly for billions of years," said co-author David Rodriguez from UCLA, "but when they go, they just might take a star or planet or two with them."

A new paper using observations with the Spitzer Space Telescope has reported possible evidence for a giant planet in the disk surrounding BP Psc. This might be a newly formed planet or one that was part of the original planetary system.

"Exactly how stars might engulf other stars or planets is a hot topic in astrophysics today," said Kastner.

"We have many important details that we still need to work out, so objects like BP Psc are really exciting to find."

PTI

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First Published: Wednesday, September 15, 2010, 15:30

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