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Mini solar systems

New research 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.
Provided by the University of St. Andrews, Scotland
Gas giant planets
The new study suggests that miniture solar systems would not necessarily look like our own. This composite of planets in our solar system was taken by various NASA spacecraft. Included in the image are (from top to bottom) Jupiter, Saturn, Uranus, and Neptune.
NASA/JPL
November 21, 2007
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.

Scholz and 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 dusty disks also surround about one third of the planemos, thus these relatively small objects seem to have a star-like infancy.

Other teams have presented evidence for a star-like formation of planemos previously, 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 plane. Imagine a solar system where planets encircle an object which itself is not much larger than a planet," explains Scholz.

Although the new findings have not settled the origins of planemos, Scholz and 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," says Jayawardhana.
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