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'Dead star' erupts for big show

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By Jonathan Amos

BBC News science reporter, in Leicester

 

 

 

The data will be used to improve the current model of nova events

 

 

Enlarge Image

 

Scientists are studying the violent outburst of a dead star as it

tries to fire back into life.

 

The white dwarf star in the Ophiuchus constellation has exhausted its

own nuclear fuel but is now stealing it from a neighbouring giant.

 

Every 20 years or so, it gathers sufficient material to explode with

enough intensity to be seen from Earth with the naked eye.

 

The so-called recurrent nova event has now flared up six times in 108

years.

 

" It's a runaway nuclear bomb, basically, that has gone off on the

surface of the white dwarf star, " said Mike Bode.

 

The Liverpool John Moores University professor has been detailing the

ongoing incident, along with Dr Tim O'Brien of Jodrell Bank

Observatory, to the 2006 UK National Astronomy Meeting.

 

Amateur stargazers in Japan were the first to report the nova on 12

February, and the professional scientific community has responded by

calling up some of the world's leading facilities to take a look.

 

These telescopes include the US space agency's flagship Swift and

Spitzer missions; as well as ground-based observatories such as the

United Kingdom Infrared Telescope on the summit of Mauna Kea in

Hawaii, and the Merlin radio astronomy network in England.

 

" The level of co-operation and the range of telescopes involved has

been extraordinary, " said Professor Bode, the leader of the Swift's

nova campaign.

 

Slow fade

 

The white dwarf star is about 5,000 light-years from Earth and is

probably little bigger than our own planet, having burnt all its

hydrogen and shed its outer layers.

 

It is now extremely dense and its strong gravity can pull gas off a

companion, red giant star. The two objects orbit each other every 455

days.

 

What is very unusual in this arrangement is that the red giant is

losing enormous amounts of gas in a wind that envelops the whole

system (referred to as RS Ophiuchi, or RS Oph).

 

As a result, when the episodic thermonuclear explosions let go, they

do so " inside " the companion's extended atmosphere.

 

" When this thing goes bang, it blows material out into the wind and

sets off shocks that are at more than 100 million degrees, nearly 10

times the core temperature of our Sun, " Professor Bode told the BBC

News website.

 

The event remained visible in the sky to the unaided eye for about a

week or so. Skywatchers would now need binoculars or a small

telescope to see it.

 

However, the nova remains bright at wavelengths outside the visible

spectrum - especially to the world's biggest telescopes.

 

Great opportunity

 

The space-borne Swift observatory was called in just three days after

the outburst began. The Nasa-managed spacecraft carries UK-built

components that detect X-rays.

 

Swift recorded how this high-energy light brightened, faded and then

lit up again.

 

" About a month after the outburst, the X-ray brightness of RS Oph

increased very dramatically, " explained Dr Julian Osborne, a Swift

scientist at the University of Leicester.

 

" This was presumably because the hot white dwarf, which is still

burning nuclear fuel, then became visible through the red giant's

wind.

 

" This new X-ray flux was extremely variable, and we were able to see

pulsations which repeat every 35 seconds or so. Although it is very

early days, and data are still being taken, one possibility for the

variability is that this is due to instability in the nuclear burning

rate on the white dwarf. "

 

From high energies to lower-energy radio wavelengths, the

astronomical community expects the observations to be a boon to its

understanding of nova behaviour. All the data will be used to improve

the current model for this type of event.

 

" This is our best chance yet of understanding what is truly going

on, " said radio astronomer Dr Stewart Eyres, of the University of

Central Lancashire.

 

RS Oph's activity is expected to die down over the next few weeks and

months - before it pulls enough gas off the red giant to explode

again in 10-30 years' time.

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Guest guest

so weird to think wot we can see now in the white dwarf actually happened 5000

yrs ago....

 

 

>heartwerk <jo.heartwork

>Apr 9, 2006 11:49 PM

>

> 'Dead star' erupts for big show

>

>

>By Jonathan Amos

>BBC News science reporter, in Leicester

>

>

>

>The data will be used to improve the current model of nova events

>

>

>Enlarge Image

>

>Scientists are studying the violent outburst of a dead star as it

>tries to fire back into life.

>

>The white dwarf star in the Ophiuchus constellation has exhausted its

>own nuclear fuel but is now stealing it from a neighbouring giant.

>

>Every 20 years or so, it gathers sufficient material to explode with

>enough intensity to be seen from Earth with the naked eye.

>

>The so-called recurrent nova event has now flared up six times in 108

>years.

>

> " It's a runaway nuclear bomb, basically, that has gone off on the

>surface of the white dwarf star, " said Mike Bode.

>

>The Liverpool John Moores University professor has been detailing the

>ongoing incident, along with Dr Tim O'Brien of Jodrell Bank

>Observatory, to the 2006 UK National Astronomy Meeting.

>

>Amateur stargazers in Japan were the first to report the nova on 12

>February, and the professional scientific community has responded by

>calling up some of the world's leading facilities to take a look.

>

>These telescopes include the US space agency's flagship Swift and

>Spitzer missions; as well as ground-based observatories such as the

>United Kingdom Infrared Telescope on the summit of Mauna Kea in

>Hawaii, and the Merlin radio astronomy network in England.

>

> " The level of co-operation and the range of telescopes involved has

>been extraordinary, " said Professor Bode, the leader of the Swift's

>nova campaign.

>

>Slow fade

>

>The white dwarf star is about 5,000 light-years from Earth and is

>probably little bigger than our own planet, having burnt all its

>hydrogen and shed its outer layers.

>

>It is now extremely dense and its strong gravity can pull gas off a

>companion, red giant star. The two objects orbit each other every 455

>days.

>

>What is very unusual in this arrangement is that the red giant is

>losing enormous amounts of gas in a wind that envelops the whole

>system (referred to as RS Ophiuchi, or RS Oph).

>

>As a result, when the episodic thermonuclear explosions let go, they

>do so " inside " the companion's extended atmosphere.

>

> " When this thing goes bang, it blows material out into the wind and

>sets off shocks that are at more than 100 million degrees, nearly 10

>times the core temperature of our Sun, " Professor Bode told the BBC

>News website.

>

>The event remained visible in the sky to the unaided eye for about a

>week or so. Skywatchers would now need binoculars or a small

>telescope to see it.

>

>However, the nova remains bright at wavelengths outside the visible

>spectrum - especially to the world's biggest telescopes.

>

>Great opportunity

>

>The space-borne Swift observatory was called in just three days after

>the outburst began. The Nasa-managed spacecraft carries UK-built

>components that detect X-rays.

>

>Swift recorded how this high-energy light brightened, faded and then

>lit up again.

>

> " About a month after the outburst, the X-ray brightness of RS Oph

>increased very dramatically, " explained Dr Julian Osborne, a Swift

>scientist at the University of Leicester.

>

> " This was presumably because the hot white dwarf, which is still

>burning nuclear fuel, then became visible through the red giant's

>wind.

>

> " This new X-ray flux was extremely variable, and we were able to see

>pulsations which repeat every 35 seconds or so. Although it is very

>early days, and data are still being taken, one possibility for the

>variability is that this is due to instability in the nuclear burning

>rate on the white dwarf. "

>

>From high energies to lower-energy radio wavelengths, the

>astronomical community expects the observations to be a boon to its

>understanding of nova behaviour. All the data will be used to improve

>the current model for this type of event.

>

> " This is our best chance yet of understanding what is truly going

>on, " said radio astronomer Dr Stewart Eyres, of the University of

>Central Lancashire.

>

>RS Oph's activity is expected to die down over the next few weeks and

>months - before it pulls enough gas off the red giant to explode

>again in 10-30 years' time.

>

>

>

>

>

>

>

>

>

>To send an email to -

>

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Guest guest

It is weird - but I find it interesting.

 

Jo

 

-

" fraggle " <EBbrewpunx

 

Monday, April 10, 2006 5:52 PM

Re: 'Dead star' erupts for big show

 

 

> so weird to think wot we can see now in the white dwarf actually happened

5000 yrs ago....

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