Astronomers find best gravitational wave prospect
15:32 01 June 2005
NewScientist.com news service
Two burned-out stars are spiralling towards each other so fast they may ripple the fabric of space-time more than any other source near Earth, suggest new observations. A future space mission may detect the ripples - or gravitational waves - within 10 years.
Massive, accelerating objects such as black holes and the dense corpses of stars are thought to release gravitational waves as they orbit each other. This allows them to fall inwards until they eventually collide and merge - unleashing even more powerful gravitational radiation.
Though widely theorised, no such waves have yet been detected. But new observations with the Chandra X-ray Observatory may have identified the most likely candidate for a future detection. The space telescope has confirmed previous observations suggesting two white dwarfs - the burned-out embers of stars like our Sun - are whipping around each other every 321.5 seconds.
Tod Strohmayer, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Maryland, US, used Chandra to reveal that the pair's X-ray emission varies on that timescale - and is gradually quickening. Strohmayer thinks the emission comes from matter dropping from one star onto the other, and says the stars may be edging closer to each other by about 3 centimetres per hour.
Stellar cadavers
The pair, called RX J0806.3+1527, appear to be separated by just 80,000 kilometres - five times closer than the distance between the Earth and Moon. That makes them the closest of about 10 known white dwarf binaries.
"It's either the most compact binary known or one of the most unusual systems we've ever seen," says Strohmayer. "Either way it's got a great story to tell." The pair lies just 1600 light years from Earth........cont'd
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