From: University of St Andrews
Posted: Tuesday, November 20, 2007
New research led by a University of St Andrews astronomer has found evidence for what might be the raw material for the beginning of shrunken versions of our solar system - miniature worlds in the making.
In their study Dr Alexander Scholz, SUPA Advanced Fellow at the University of St Andrews, and Professor Ray Jayawardhana, from the University of Toronto, challenge the assumption that other planetary systems in the Universe would necessarily look like our own solar system.
The astronomers have found that the birthplaces of planets exist not only around young stars but also around planemos (short for planetary mass objects) that are not much larger or heavier than Jupiter. This may imply the existence of miniature solar systems with a central object having only about 1% of the mass of the Sun.
Since their discovery in 2000, the nature and origin of the enigmatic planemos has been a hot topic - are they tiny stars or giant planets, kicked out from a young planetary system? The new study now suggests that the former scenario is much more likely.
In a paper to be published in the Astrophysical Journal (Letters) Dr Scholz and Professor Jayawardhana used the Spitzer Space Telescope to observe 18 planemos in a star cluster in Orion that is about 3 million years old. At that age many young stars are still surrounded by disks of dust and gas which may evolve into planetary systems. The dust in these disks 'glows' in the infrared wavelength range and can therefore be seen with infrared cameras.
The new observations show that about one third of the planemos are also surrounded by dusty disks, thus these relatively small objects seem to have a star-like infancy.
Evidence for a star-like formation of planemos has been presented previously by other teams but the new observations constitute the first systematic survey and push our knowledge of planemos into new territory.
"The results demonstrate that long-lived dusty disks, the nurseries of planets, are commonly found even around extremely low-mass objects. This could indicate that planetary systems may form even when the central 'star' is not a star, but a planemo. Imagine a solar system where planets encircle an object which itself is not much larger than a planet," explains Dr Scholz.
Although the new findings have not settled the origins of planemos Dr Scholz and Professor Jayawardhana believe the results bring us one step closer.
"How puny an object could nature produce in the same way that it made our Sun? That's the big question motivating our research. The answer will tell us a lot about the star formation process as well as about the true diversity of planetary systems out there," said Professor Jayawardhana.
Note to Editors:
SUPA (Scottish Universities Physics Alliance) is a research collaboration between St Andrews, Edinburgh, Heriot Watt, Paisley, Strathclyde and Glasgow Universities).
This project has been supported by SUPA and an NSERC (National Science and Engineering Research Council of Canada) grant to Professor Jayawardhana. The research project was based on observations using the Spitzer Space Telescope, a NASA mission managed by the Jet Propulsion Laboratory, with support from the Californian Institute of Technology.
The paper, accepted by the Astrophysical Journal (Letters) is available at http://arxiv.org/abs/0711.2510
Dr Scholz is available for interview and further information by contacting: 01334 461666 or firstname.lastname@example.org
An image and caption illustrating the research is also available - please contact the University of St Andrews Press Office on 01334 462529
Issued by the University of St Andrews - reference: Planemos/201107
PIO Source:Allison Irvine
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