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Nearby red dwarves could reveal planet secrets

An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation

Date:
September 15, 2015
Source:
Australian National University
Summary:
An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation. Astronomers have found large discs of dust around two of the stars, tell-tale signs of planets in the process of forming.
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Artist's impression of a dusty disc around a red dwarf star.
Credit: NASA/JPL-Caltech/T. Pyle (SSC)

An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation.

Astronomers from The Australian National University (ANU) and UNSW Canberra found large discs of dust around two of the stars, tell-tale signs of planets in the process of forming.

"We think the Earth and all the other planets formed from discs like these so it is fascinating to see a potential new solar system evolving," said the lead researcher Dr Simon Murphy, from the ANU Research School of Astronomy and Astrophysics.

"However, other stars of this age usually don't have discs any more. The red dwarf discs seem to live longer than those of hotter stars like the Sun. We don't understand why," said Dr Murphy.

The discovery of objects like these two challenges current theories about planet formation, said co-author Professor Warrick Lawson from UNSW Canberra. "It suggests the planet forming process can endure a lot longer than previously thought," he said

The red dwarves may also host planets that have already formed from the dusty discs, Dr Murphy said.

"I think a lot of telescopes will be turned toward them in the next few years to look for planets."

The giveaway that the red dwarves had discs around them was an unusual glow in the infrared spectrum of the stars. Although the discs were not observed directly, Dr Murphy said such close red dwarves offered a good chance of catching a rare direct glimpse of a disc, or even a planet, by employing specialised telescopes.

"Because they are fainter than other stars and there is not as much glare, young red dwarves are ideal places to directly pick out recently formed planets," he said.

Our ability to detect these dim stars has improved dramatically in recent decades, revealing a wealth of information, said Professor Lawson. "Less than 20 years ago, the notion that the nearest part of the Galaxy would be littered with young stars was a completely novel one," he said.

"Most of these objects lie in the southern sky and thus are best accessed by telescopes in the southern hemisphere, including those operated by the ANU and Australia more broadly."


Story Source:

Materials provided by Australian National University. Note: Content may be edited for style and length.


Journal Reference:

  1. Simon J. Murphy, Warrick A. Lawson and Joao Bento. New members of the TW Hydrae Association and two accreting M-dwarfs in Scorpius–Centaurus. Monthly Notices of the Royal Astronomical Journal, 2015 DOI: 10.1093/mnras/stv1745

Cite This Page:

Australian National University. "Nearby red dwarves could reveal planet secrets: An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation." ScienceDaily. ScienceDaily, 15 September 2015. <www.sciencedaily.com/releases/2015/09/150915211331.htm>.
Australian National University. (2015, September 15). Nearby red dwarves could reveal planet secrets: An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation. ScienceDaily. Retrieved May 26, 2017 from www.sciencedaily.com/releases/2015/09/150915211331.htm
Australian National University. "Nearby red dwarves could reveal planet secrets: An accidental find of a collection of young red dwarf stars close to our solar system could give us a rare glimpse of slow-motion planet formation." ScienceDaily. www.sciencedaily.com/releases/2015/09/150915211331.htm (accessed May 26, 2017).

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