Some stars capture rogue planets
Scientists found that if the number of rogue planets equals the number of stars in a young cluster, then 3 to 6 percent of the stars will grab a planet over time.
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Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts —
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April 18, 2012 In this artist's conception, a captured world drifts at the outer edge of a distant star system, so far from its sun-like host that the star's disk is barely resolvable at upper right. New research shows that one in 20 stars within our galaxy might have captured a free-floating planet. Credit: Christine Pulliam (CfA)
"Stars trade planets just like baseball teams trade players," said Hagai Perets from the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts.
To reach their conclusion, Perets and Thijs Kouwenhoven from Peking University in China simulated young star clusters containing free-floating planets. They found that if the number of rogue planets equaled the number of stars, then 3 to 6 percent of the stars would grab a planet over time. The more massive a star, the more likely it is to snag a planet drifting by.
They studied young star clusters because capture is more likely when stars and free-floating planets are crowded together in a small space. Over time, the clusters disperse due to close interactions between their stars, so any planet-star encounters have to happen early in the cluster's history.
Rogue planets are a natural consequence of star formation. Newborn star systems often contain multiple planets. If two planets interact, one can be ejected and become an interstellar traveler. If it later encounters a different star moving in the same direction at the same speed, it can hitch a ride.
A captured planet tends to end up hundreds or thousands of times farther from its star than Earth is from the Sun. It's also likely to have an orbit that's tilted relative to any native planets, and may even revolve around its star backward.
Astronomers haven't detected any clear-cut cases of captured planets yet. Imposters can be difficult to rule out. Gravitational interactions within a planetary system can throw a planet into a wide, tilted orbit that mimics the signature of a captured world.
Finding a planet in a distant orbit around a low-mass star would be a good sign of capture because the star's disk wouldn't have had enough material to form the planet so far out.
The best evidence to date in support of planetary capture comes from the European Southern Observatory, which announced in 2006 the discovery of two planets (weighing 14 and 7 times Jupiter) orbiting each other without a star.
"The rogue double-planet system is the closest thing we have to a 'smoking gun' right now," said Perets. "To get more proof, we'll have to build up statistics by studying a lot of planetary systems."
Could our solar system harbor an alien world far beyond Pluto? Astronomers have looked but haven't found anything yet.
"There's no evidence that the Sun captured a planet," said Perets. "We can rule out large planets. But there's a non-zero chance that a small world might lurk on the fringes of our solar system."
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