By Roland Pease

BBC Science



The star is in the equatorial constellation of Ophiuchus

The star flared up suddenly last February, briefly becoming 1,000 times brighter than normal.

RS Ophiuchi is close to destroying itself in a nuclear explosion called a type 1a supernova, scientists report in the journal Nature.

These are among the brightest phenomena in the Universe, radiating five billion times as much light as the Sun.

They are so bright they can be seen far across the cosmos.

They also seem to be remarkably uniform - they always appear to give off the same amount of light, so that their visibility from Earth, dimmed only by their immense distance, has been used to measure the size of the Universe.

The only problem, which is a great embarrassment to astronomers, is that they have never seen a type 1a close up - their measurements are all based on theory.

They are very rare events in our galaxy. It seems certain a type 1a was seen in our galaxy in 1572 by the great Danish astronomer Tycho Brahe, who first coined the term nova, for "new star", not realising he was in fact witnessing the violent end of an unknown star.

Death throes

It has long been believed that type 1a supernovae are the death throes of white dwarf stars. But all modern ones have been so distant that it has not been possible to see what had been there beforehand.

The explosion is so energetic it actually lifts an envelope of material off the surface of the star and throws it off into space

Jeno Sokoloski, Harvard University

Several times in the past century it has flared up, as if in a failed supernova explosion. It is as if a thermonuclear flame has swept across the face of the star without quite catching hold.

The last time it flared up was in 1985, when astronomers' technology was not up to catching all the details.

With space-based telescopes and large arrays of radio dishes, this has all changed. Writing in the journal Nature, a team of astronomers said they managed to detect a plume of gaseous material thrown out by the conflagration.

"The explosion is so energetic it actually lifts an envelope of material off the surface of the star and throws it off into space," lead author Jeno Sokoloski, of Harvard University, US, told the BBC's Science in Action programme.

By tracking the plume, she adds, they could learn more about the star that launched it.

"It started slowing down almost immediately, within just two days, and that tells us the white dwarf must be extremely massive; in fact, almost massive enough to collapse."

Critical mass

Theory says that white dwarfs self destruct when their mass equals 1.4 Suns.

RS Oph is nearing that critical mass. It is slowly gobbling up material from a nearby giant star, gaining a millionth of a solar mass every decade.

At the moment, sitting just below the critical mass, the novae on RS Oph blow themselves out, achieving brief episodes of brilliance.

But soon, RS Oph could pass the tipping point. It is not a certainty; RS Oph could just as easily be eating itself up in these explosions. But if it does reach the critical mass, it will collapse in on itself and blow apart. How soon that might happen is not clear.

"It could be tomorrow, but most likely it'll be 1,000, 10,000, 100,000 years from now," says Jeno Sokoloski.

Whenever it happens, it will be, she says, a spectacular event, outshining the planets, so that its final glory will be visible against the daytime sky.

In the meantime, astronomers will be studying the star closely, to watch its every step towards destruction, and hoping to understand the full details of one of the heavens' great mysteries.